2001 Spring Meeting Special Sessions

Designators for special sessions belong to the lead section or committee abbreviation (i.e., A01 denotes Atmospheric Sciences, P01 denotes Planetary Sciences, etc.).  Additionally, special sessions are listed under all sections or committees who have agreed to sponsor particular sessions.  These sessions are listed after the committee and section primary listing but with the lead section designation.  Some technical committees have elected to only cosponsor sessions.
 
Union (U) Nonlinear Geophysics (NG)
Atmospheric Sciences (A) Ocean Sciences (OS)
Biogeosciences (B) Planetary Sciences (P)
Study of Earth's Deep Interior (DI) Public Affairs (PA)
Education and Human Resources (ED) Seismology (S)
Geodesy (G) SPA: Space Physics and Aeronomy (SA)
Geomagnetism and Paleomagnetism (GP) SPA: Solar and Heliospheric Physics (SH)
Geochemical Society (GS) SPA: Magnetospheric Physics (SM)
Hydrology (H) Solar Physics Division-AAS (SPD)
Mineralogical Society of America (M) Tectonophysics (T)
Mineral and Rock Physics (MR) Volcanology, Geochemistry and Petrology (V)

Union

U01 New Frontiers in Mathematical Geoscience
This session solicits papers describing contemporary research in any area of geoscience in which either (a) the understanding of a fundamental geoscience problem has been significantly advanced by the application of  mathematical techniques beyond those included in the traditional geoscience curricula, (b) the nature of the geoscience problem stimulates the development of new mathematics research, or (c) pursuit of the geoscience problem reveals a need for the application of new or unconventional mathematical approaches.  In addition to papers from geoscientists, relevant papers from mathematicians and from collaborations between mathematicians and geoscientists will be welcome.  That this session is convened by program officers from the National Science Foundation's Divisions of Earth, Atmospheric, and Oceanic Sciences is a reflection of the enthusiasm within NSF for increased dialogue and collaboration between geoscientists, mathematicians and statisticians as they tackle some of the complex research questions in the geosciences.
Conveners: Steve Meacham, National Science Foundation, GEO Directorate, 4201 Wilson Boulevard, Arlington, VA 22230 USA, Tel: +1-703-292-8580, Fax: +1-703-292-9085, E-mail: smeacham@nsf.gov; and Robin Reichlin, National Science Foundation, GEO Directorate, 4201 Wilson Boulevard, Arlington, VA 22230 USA, Tel: +1-703-292-8580, Fax: +1-703-292-9085, E-mail: rreichli@nsf.gov; and Pam Stephens, National Science Foundation, GEO Directorate, 4201 Wilson Boulevard, Arlington, VA 22230 USA, Tel: +1-703-292-8580, Fax: +1-703-292-9085, E-mail: pstephen@nsf.gov

U02 Exploring Snowball Earth Conditions During Ancient Times: Geologic Evidence, Modeling, and Implications for the Evolution of Life
The "Snowball Earth" hypothesis implies that sea-ice and land glaciers covered most of the Earth from the Equator to the Poles.  These "Snowball Earth" conditions may have occurred several times in Earth's history, but have not returned in the last 500 million years.  A number of questions arise with respect to the "Snowball Earth" hypothesis such as: (1) What is the evidence for global glaciation?; (2) How did life survive these catastrophic events?; (3) What can models tell us about environmental conditions prior, during and after "Snowball Earth" events?  In this session, we seek contributions from various disciplines (atmospheric sciences, biology, geo-chemistry, geology, oceanography) that examine scientific issues related to the "Snowball Earth" hypothesis. Examples include but are not limited to physical processes initiating and terminating low-latitude glaciation, the impact of "Snowball Earth" conditions on biology (extinction and recovery), and processes that may have led the to rapid diversification of life at the end of the Proterozoic.
Conveners: Gregory S. Jenkins, Penn State University, Department of Meteorology, University Park, PA 16802 USA, Tel: +1-814-865-0479, Fax: +1-814-865-3663, E-mail: osei@essc.psu.edu; and Christopher P. McKay, NASA Ames Research Center, Space Science Division 245-3, Moffett Field, CA 94035 USA, Tel: +1-650-604-6864, Fax: +1-650-604-6779, E-mail: cmckay@arc.nasa.gov; and Linda E. Sohl, Columbia University, Lamont-Doherty Earth Observatory, Palisades, NY USA, Tel: +1-845-365-8510, Fax: +1-845-365-8150, E-mail: sohl@ldeo.columbia.edu; and Mark McMenamin, Mount Holyoke College, Department of Earth and the Environment, South Hadley, MA 01075 USA, Tel: +1-413-538-2280, Fax: +1-413-538-2239, E-mail: mmcmenam@mtholyoke.edu

U03 Western Hemisphere Knowledge Partnerships
The grand challenge for science, technology, and society during the next fifty years is to achieve a civilization that is environmentally sustainable, economically prosperous and equitable, and therefore socially and politically stable. Continuing advances in geophysics and the other physical sciences, an explosion of knowledge in the biological and health sciences, and a revolution in the technologies for distributing knowledge are combining to make knowledge, broadly construed, an organizing principle for society in responding to this grand challenge. New types of partnerships need to be forged among all disciplines, among the major sectors of society, and between disciplines and societal sectors. Western Hemisphere Knowledge Partnerships are being created to test the hypothesis that knowledge has the potential to be the wealth-creating asset that AGU's All-Union session in 1997 concluded is the
case. A new era of science policy is unfolding.
Convener: Thomas F. Malone, North Carolina State University, Department of Marine, Earth, and Atmospheric Sciences, Raleigh, NC 27695 USA, Tel: +1-860-236-2426, Fax: +1-860-233-6250, E-mail: tfmalone@aol.com

U04 Integrated Strategies for the Mitigation of the Adverse Consequences of Natural Hazards Worldwide
This session will examine how science and technology are, or could be, used to guide public policy decisions to mitigate natural hazards risks, with particular focus on mitigation strategies for developing countries. These hazards include hurricanes, abnormal rainfall, floods, droughts, earthquakes, space weather, and climate change. Papers might focus on mitigation strategies that have been used or proposed for particular biophysical or socioeconomic situations. Such studies could describe how data or models were used to predict environmental consequences, such as biochemical and trophic changes, on the basis of known empirical relationships, and how those scientific results were presented in a form suitable for use by non-specialists in the government agencies, NGOs and the general public. They could also describe the methods of coupling and integrating geophysical models of natural hazards with socioeconomic models. We invite papers from geoscientists, social scientists, or policy professionals who have worked on either the relevant scientific research or its application to natural hazards policy. AGU members from developing countries are particularly encouraged to submit abstracts addressing the kinds of scientific research and cooperation they see as important in helping them to make progress against destruction by natural hazards.
Conveners: Margaret R. Goud Collins, American Academy of Arts and Sciences, U.S. Committee for IIASA Norton's Woods, 136 Irving St., Cambridge, MA 02138 USA, Tel: +1-617-576-5019, Fax: +1-508-548-6063, E-mail: mcollins@amacad.org; and U. Aswathanarayana, Advisor on Environment & Technology C.P. 1947, Maputo, Mozambique, Tel: +2581-307068, Fax: +2581-308915, E-mail: anarayan@zebra.uem.mz

U05 Structure and Dynamics of the Inner Core
The solidification of the inner core has been proposed to be a likely energy source for the Earth's geodynamo, and its presence stabilizes the Earth's magnetic field. Computational and observational advances in mineral physics, seismology, and geomagnetism have significantly narrowed the bounds on the variables and observables of inner core properties. These include the composition, structural state, elastic anisotropy, and differential rotation rate of the inner core. Seismology has also recently detected a heterogeneous fabric in the inner core, which may be related to its crystalline texture or melt inclusions. This session invites contributions that seek to unify interdisciplinary observations, and interpret the consequences of inner core structure, composition, state, and fabric.
Conveners: Ronald Cohen, California Institute of Technology, Seismological Laboratory, Pasadena CA 91125 USA, Tel: +1-626-395-6958, Fax: +1-626-564-0715, E-mail: cohen@gl.ciw.edu; and Vernon Cormier, University of Connecticut, Department of Geology and Geophysics, Storrs CT 06269-2045, Tel: +1-860-486-1391, Fax: +1-860-486-1383, E-mail: cormier@geol.uconn.edu

U06 First Science Results from the ASTER Instrument, Onboard the Terra Spacecraft
The ASTER instrument onboard the Terra spacecraft is an international effort, the instrument being provided by the Japanese Ministry of Industry and Transport (MITI) and flying on a NASA spacecraft.  It provides the zoom lens for the other instruments aboard Terra, with 3 channels in the VNIR at 15m resolution, including stereo, 6 channels in the SWIR at 30m resolution, and 5 chaneels in the TIR at 90m resolution. Its primary mission is to measure and monitor global change, particularly on land surfaces where the high resolution is required. Some particular targets are volcano, glacial, and land use monitoring. The data are now available to the public, and this will be one of the first opportunities to see early science results.
Conveners: Anne Kahle, Jet Propulsion Laboratory, U.S. ASTER Science Team MS 183-501, 4800 Oak Grove Avenue, Pasadena, CA 91109 USA, Tel: +1-818-354-7265, Fax: +1-818-354-0966, E-mail: ann@aster.pjl.nasa.gov; and Yasushi Yamaguchi, Nagoya University, Japanese Science Team, Nagoya, Japan,  E-mail: yashushi@eps.nagoya-u.ac.jp

U07 Multidisciplinary Approaches to Understanding Coastal Zone Processes
As human populations continue to expand into coastal areas they intensify urban and agricultural pressures at a time of growing uncertainty over the potential effects of sea-level rise and climate change. Sandy, shallow coastal aquifers are particularly sensitive to the contamination that accompanies this increased population growth, and water resources are stressed due to increased withdrawals. However, many questions remain regarding the physical and biogeochemical processes that control water quality and interactions between groundwater and surface water and between freshwater and saltwater in the coastal zone. Changes in land use may also result in increased sediment transport leading to degradation in quantity and quality of coastal marshes and shallow estuarine areas. Coastal marsh degradation is further complicated by sea-level rise, loss of coastal/barrier islands and increasing wave energy, which combined, threaten their future stability due to changes in hydroperiod and inundation. Climate change may also result in changes in the magnitude, frequency and impact of coastal storms which may further alter sedimentation and depositional processes in coastal areas. The interplay of these various factors results in complicated relationships among the biological, chemical, and physical processes involved making it difficult to predict the outcome of management practices. This session will present an overview of these processes and the important questions that remain, in addition to offering a direction for future research in coastal zone processes.
Convener: Larry J. Puckett, U.S. Geological Survey, MS413 National Center, Reston, VA 20192 USA, Tel: +1-703-648-5842, Fax: +1-703-648-6693, E-mail: lpuckett@usgs.gov

U08 Non-equilibrium Phenomena in Geophysics
This session is designed to bring investigators from different disciplines together to discuss recent research on non-equilibrium processes and of dissipative phenomena in geophysics. Dissipative structures and related fractal scaling, which often appear in non-equilibrium systems, are recognized features of a number of geophysical systems as well. We will address these issues by attracting papers on the global and local structures of geophysical fluids, transport properties and scaling of turbulence, and energetics of the non-equilibrium systems. These include dissipative properties of the atmosphere and ocean, as well as mantle convection, the production of available potential energy and its relation to the 2nd law of thermodynamics, long-range structures and correlations in earthquake fault systems, and extreme properties in the complex geophysical and extra-planetary geophysical fields.
    This session is designed with an innovative format.  It will consist exclusively of 20-minute invited talks, punctuated by 20-minute moderated discussion sessions.  Submitted talks will be included in the accompanying poster session.
Conveners: Bill Klein, Los Alamos National Laboratory, Center for Non-Linear Studies MS-B258, Los Alamos, NM 87545 USA, Tel: +1-505-667-9469, Fax: +1-505-665-2659, E-mail: klein@cnls.lanl.gov; and Kristy Tiampo, University of Colorado, CIRES UCB 216, Boulder, CO 80309-0216 USA, Tel: +1-303-492-4779, Fax: +1-303-492-5770, E-mail: kristy@caldera.colorado.edu

U09 Tools and Systems for EOS Data (POSTER ONLY)
NASA's Earth Science Data Information Systems Project is convening a session on the use of tools to search, order, visualize and manipulate data collected from the various Earth Observing System (EOS) Missions including the recent Terra satellite and the future Aqua satellite.  This is a poster-only session intended to inform EOS Science data producers, data users, planners and managers of available data systems and tools for managing EOS data.  Services include those that will help scientists process, archive and access data and information for research, applications, planning and management.  Posters should describe system services, functionality, access requirements and procedures and the intended user community that work principally with EOSDIS data. Posters could address analysis tools, data population tools, specific EOSDIS data sets and metadata types, tools for metadata creation and management, tools for distribution, EOSDIS data formats and distribution techniques.
Conveners:  Ken McDonald, NASA-GSFC, Code 423, Greenbelt, MD 20771 USA, Tel:+1-301-614-5331, E-mail: ken.mcdonald@gsfc.nasa.gov; and Jeanne Behnke, NASA-GSFC, Code 423, Greenbelt, MD 20771 USA, Tel: +1-301-614-5326, E-mail: jeanne.behnke@gsfc.nasa.gov

Atmospheric Sciences

A01 Earth Science Applications of Reflected and Refracted GPS Transmissions (Joint with G, GP, H, SA)
Transmissions of the Global Positioning System constellation are receiving increasing interest from the Earth science community as an important remote sensing tool. Analysing the signals refracted in the atmosphere and ionosphere, and reflected from land and oceans can provide continuous observations of geophysical phenomena on a global scale. High vertical resolution atmospheric and ionospheric measurements have received attention in diverse disciplines including climate and weather, atmospheric science, hydrology, and space-weather modeling. Signals reflected from the ocean have been successfully received from aircraft and space and show promise for measuring ocean altitudes and wind-induced surface roughness. The solid Earth sciences can benefit from analysis of reflections from Earth's surface, and characterization of ionospheric currents that interfere with geomagnetic remote sensing. We invite papers that discuss the technical aspects of remote sensing with GPS, and encourage the presentation of experimental or theoretical studies that suggest new scientific and weather applications for the measurements.
Conveners: Anthony Mannucci, Jet Propulsion Lab, MS 138-308B 4800 Oak Grove Drive, Pasadena, CA 91109 USA, Tel: +1-818-354-1699, Fax: +1-818-393-5115, E-mail: tony.mannucci@jpl.nasa.gov; and John LaBrecque, NASA, USA, E-mail: jlabrecq@mail.hq.nasa.gov

A02 Satellite Observations of Trace Species in the Global Troposphere
Recent measurements of trace species in the troposphere from several satellite-borne instruments have shown the potential of remotely sensed observations to test and extend our knowledge of global tropospheric chemistry. In the coming years, one of the major challenges to the scientific community will be to assess whether these measurements are consistent with our current understanding of tropospheric chemistry. This session will focus on data retrieval methods and subsequent interpretation of tropospheric trace species measurements from existing satellite missions. The session will also address issues involving missions scheduled for the next few years.
Conveners: Paul I. Palmer, Harvard University, Department of Earth and Planetary Sciences, Pierce Hall, 29 Oxford Street, Cambridge, MA 02138 USA, Tel: +1-617-495-1591, Fax: +1-617-495-4551, E-mail: pip@io.harvard.edu; and Prasad S. Kasibhatla, Duke University, Levine Science Research Center, Nicholas School of the Environment, Room A333, Box 90328, Durham, NC 27708 USA, Tel: +1-919-613-8075, E-mail: psk9@duke.edu

A03 Transient Tracers in Geophysical Flows (Joint with B, H, OS)
Measurements of passive chemical species with natural or anthropogenic time-varying sources or sinks, so called "transient tracers", are used to diagnose the transport in many different geophysical systems. For example, these tracers have been used to estimate transit times or "ages" of air and water masses in the stratosphere, oceans, and groundwater reservoirs. This session will bring together scientists from different geophysical disciplines in order to foster collaboration and exchange ideas. Invited speakers will give overviews of the use of transient tracers in each discipline. Oral and poster contributions are invited that examine any aspect of transient tracers in geophysical flows. Particular foci are the relationship between timescales inferred from different transient tracers, and how these times (ages) are related to the underlying transport processes in the flow. Papers addressing these issues are especially encouraged.
Conveners: Darryn Waugh, Johns Hopkins University, Department of Earth and Planetary Sciences, 3400 N. Charles Street, Baltimore, MD 21218 USA, Tel: +1-410-516-8344, Fax: +1-410-516-7933, E-mail: waugh@jhu.edu; and Thomas Haine, Johns Hopkins University, Department of Earth and Planetary Sciences, 3400 N. Charles Street, Baltimore, MD 21218 USA, Tel: +1-410-516-7048, Fax: +1-410-516-7933, E-mail: thomas.haine@jhu.edu

A04 Influence of Clouds on Tropospheric Chemistry
The influence of clouds on tropospheric chemistry has been studied extensively during the past four decades; initially for understanding acid deposition, but more recently to understand cloud processing of aerosols and chemical species.  At this session, summaries of the results from the 5th International Cloud Modeling Workshop - Cloud Chemistry Case, at which aerosol and photochemical box model results were compared for specified cases, will be presented.  We also welcome presentations discussing cloud chemistry from laboratory, field measurement, and modeling (from 0-D to 3-D) studies,  including a discussion of major needs for future advancements in cloud chemistry modeling.
Conveners: Mary Barth, National Center for Atmospheric Research, PO Box 3000, Boulder, CO 80307 USA, Tel: +1-303-497-8186, Fax: +1-303-497-8171, E-mail: barthm@ucar.edu; and Sonia Kreidenweis, Colorado State University, Department of Atmospheric Science, Fort Collins, CO 80523 USA, Tel: +1-970-491-8350, Fax: +1-970-491-8449, E-mail: soniak@aerosol.atmos.colostate.edu

A05 The Tropospheric Ozone Production About the Spring Equinox
The Tropospheric Ozone Production about the Spring Equinox (TOPSE) investigation combined model studies and simulations with a set of chemical and photochemical measurements taken over the critical winter-spring transition in the northern mid-to-high latitude troposphere. The experiment took place from February to May, 2000 in a series of 7 round trip missions aboard the NCAR C-130 aircraft from Colorado to northern latitudes. The overall goal of the experiment was to investigate the chemical and dynamic evolution of tropospheric chemical composition; a particular emphasis was placed on the springtime ozone maximum in the troposphere. As the experiment progressed additional effort was used to investigate dramatic ozone depletion events found over large regions of the Arctic surface layer.  In this session, summaries of results from the TOPSE mission, as well as detailed analyses of the primary photochemical and dynamic processes that control the budgets of radicals and reservoirs in the free troposphere, will be presented. We also invite presentations of comparisons between models predictions and measurements obtained during TOPSE.
Convener: Elliot Atlas, NCAR, Atmospheric Chemistry Division, PO Box 3000, Boulder, CO 80307-3000 USA, Tel: +1-303-497-1425, Fax: +1-303-497-1477, E-mail: atlas@ucar.edu

A06 Middle Atmospheric Odd Nitrogen (Joint with SA)
Odd nitrogen constituents have key roles in one of the dominant chemical cycles governing the global ozone balance.  Since 1978 components of this chemical family have been observed at near-global scales by the LIMS, SAGE (I and II), SME, CLAES, ISAMS, HALOE, POAM (II and III) satellites, as well as at select latitudes by ATMOS and the JPL MkIV balloon payloads.  Recently, significant rate changes pertinent to the chemistry of odd nitrogen have been published, significant hemispheric-scale changes in NO2 have been observed (SAGE II), and observations (LIMS, ISAMS, HALOE and POAM II) indicating the transport of NOY constituents into the stratosphere from the mesosphere have been reported. The proposed special session on middle atmospheric odd nitrogen would seek contributed papers on all aspects of the odd nitrogen budget within the stratosphere and mesosphere, with the primary emphasis on those contributions which will have an impact on the global and high latitude ozone budget.  This will include papers on photochemical rate measurements, analysis and reanalysis of satellite and balloon odd nitrogen constituent data, new contributions on the effect of aerosols on the repartitioning of odd nitrogen constituents, and studies based upon zero-, 2-, and 3-D model simulations as well as trajectory simulations.  Papers comparing observed and calculated odd nitrogen constituents are of particular interest.
Conveners: Linwood B. Callis, NASA Langley Research Center, MS 401 B, Hampton, VA 23681-0001 USA, Tel: +1-757-864-5843, Fax: +1-757-864-6326, E-mail: l.b.callis@larc.nasa.gov; and Ellis E. Remsberg, NASA Langley Research Center, Hampton, VA 23681-0001 USA, Tel: +1-757-864-5823, Fax: +1-757-864-6236, E-mail: e.e.remsberg@larc.nasa.gov

A07 Calibration of Meteorological Satellite Sensors and Validation of Derived Products (Joint with B, H, OS)
Pre- and post-launch calibration and characterization of meteorological satellite sensors are crucial to ensure the accuracy, continuity, and viability of satellite-derived geophysical products. Independent validation of the geophysical products thus derived will in turn establish the usability of the same in Earth system studies such as those envisaged under the World Climate Research Programme (WCRP), the International Geosphere Biosphere Program (IGBP), and the global climate, terrestrial, and ocean observing systems (G3OS).  Accordingly, papers are solicited in the broad areas of (a) pre- and post-launch calibration of meteorological satellite sensors; (b) inter-sensor calibration; (c) rehabilitation of long-term satellite-derived geophysical records (e.g., NOAA/NASA Pathfinder data sets); (d) procedures for product validation; (e) product validation campaigns; and (f) international collaborative and cooperative efforts.
Convener: C.R. Nagaraja Rao, NOAA/NESDIS Office of Research and Applications, E/RA1 World Weather Building, Room 810, 5200 Auth Road, Camp Springs, MD 20746 USA, Tel: +1-301-763-8136 ext. 138, Fax: +1-301-763-8108, E-mail: nrao@nesdis.noaa.gov

A08 Research in Meteorology and Oceanography Utilizing DoD HPC Resources (Joint with OS)
This session will highlight research in the climate weather ocean (CWO) computational technology area (CTA) of the Department of Defense's High Performance Computing (HPC) program. All research in this CTA which utililizes HPC resources is encouraged to contribute. The grand challenge projects within this CTA will be asked to give invited presentations in order to highlight the leading edge research made possible by this program.
Conveners: Jay F. Shriver, Stennis Space Center, Naval Research Laboratory Code 7323, Bldg 1009, Stennis Space Center, MS 39529 USA, Tel: +1-228-688-4625, Fax: +1-228-688-4759, E-mail: shriver@nrlssc.navy.mil; and George W. Heburn, Major Shared Resource Center Programs Commander, Naval Meteorology and Oceanography Command, N5H, 1020 Balch Blvd., Stennis Space Center, MS 39529 USA, Tel: +1-228-688-5396, Fax: +1-228-688-5791, E-mail: heburn@cnmoc.navy.mil

A09 Climate Model Diagnosis: Tools and Techniques
Assessing how well climate models perform and understanding their systematic errors have long been difficult problems in climate modeling. With increasing resolution and longer simulations, new problems and new opportunities have emerged. Software tools should allow remote data access and manipulation of large data sets for sophisticated diagnostics on high frequency three-dimensional data. Papers will be welcome that discuss new methods of accessing and manipulating large data sets, creative techniques that reveal systematic errors in climate models, model intercomparison, and methods that suggest the causes of model errors.
Conveners: Gerald L. Potter, Lawrence Livermore National Laboratory, Program for Climate Model Diagnosis and Intercomparison, PO Box 808, MS L-264, Livermore, CA 94550 USA, Tel: +1-925-422-1822, Fax: +1-925-422-7675, E-mail: gpotter@llnl.gov; and James J. Hack, National Center for Atmospheric Research, PO Box 3000, Boulder, CO 80307-3000 USA, Tel: +1-303-497-1387, Fax: +1-303-497-1324, E-mail: jhack@cgd.ucar.edu

Atmospheric Sciences also presents joinly with the following Special Sessions:
B02 Integrated Observations for the Biogeosciences (Joint with A, NG, OS)
B07 Isotopes in Biogeochemistry and Global Change (Joint with A, GS, H, OS)
B09 Mercury in the Environment (Joint with A, GS, H, PA)
B13 CO2 Flux Measurements From the Ground Up (Joint with A, GS)
B14 Land-Atmosphere Interactions (Joint with A, H, NG)
B15 Global Remote Sensing and in-situ Land Surface Data for Weather and Climate Models (Joint with A)
OS01 Non-Equilibrium Phenomena in Geophysics (Joint with A, B, H, P, S, T)
OS04 Ice Cores: Paleoclimates, Glaciology, and Environmental Change (Joint with A, H)
SA03 Polar Mesospheric Clouds, Noctilucent Clouds and Polar Mesospheric Summer Echoes (Joint with A)
NG01 Recent Contributions of Nonlinear Science in Atmospheric Research: From Paradigm Shifts to Problem Solving (Joint with A)
 

Biogeosciences

B01 Carbon Saturation in Ecosystems: Controls, Limits, and Implications (Joint with GS)
Estimates of soil C sequestration ‘potentials’ in managed ecosystems are often made with native (i.e. prior to human use) soil C levels as a point of reference, yet native levels can be increased by implementing a variety  of management practices such as fertilization, sowing more productive species, or irrigation.  Native soil C and vegetation C levels reflect one particular climate and vegetation regime (i.e. that without major human intervention) that can be modified (by changes in land use or management) to increase ecosystem C stocks.   Our best understanding of soil C dynamics assumes a direct relationship between C inputs to soil and soil C stocks that is directly affected by climate and unbounded.  However, a number of investigators have observed no response to continued increases in C inputs to the soil.  Are soils in these systems saturated with respect to C?  What factors define C saturation limits in soils?  What types of systems are at or near saturation?  What are the implications for the global C cycle, in general, and C sequestration in particular? Basic ecological theory states that plant production is constrained by the soil nutrient most limited in amount (Liebig’s law of the minimum). What are the implications of the limited ability of soils to store organic matter, which acts as a nutrient reservoir, for vegetative production?  Could vegetation C pools become saturated?  This session will focus on exploring constraints on and limits to C storage in soil and vegetation.  Abstracts are solicited from all relevant fields.
Conveners: Richard T. Conant, Natural Resource Ecology Laboratory, Fort Collins, CO 80523-1499 USA, Tel: +1-970-491-2104, Fax: +1-970-491-1965, E-mail: conant@nrel.colostate.edu; and Johan Six, Natural Resource Ecology Laboratory, Fort Collins, CO 80523-1499 USA, Tel: +1-970-491-5599, Fax: +1-970-491-0279, E-mail: johan@nrel.colostate.edu

B02 Integrated Observations for the Biogeosciences (Joint with A, NG, OS)
The availability of high-quality field measurements and remotely sensed data has enabled scientists to explore complex biogeochemical dynamics at broad spatial and temporal scales. Often the process studies and models that bring together large, diverse data sets generate patterns and synergistic results that are not possible from traditional small scale studies. Both terrestrial and oceanic biogeochemical processes are to be covered as well as the gas exchanges (CO2, methane, DMS, etc.) with the atmosphere. This session will highlight applications in which data for several parameters are combined at broad spatial and temporal scales, recent data set compilations and the integration of the data sets in state-of-the-art models. Both users and producers of data sets are encouraged to participate.
Conveners: Martha Maiden, NASA Headquarters, 300 E. Street, SW Code Y, Washington, DC 20546 USA, Tel: +1-202-358-1078, Fax: +1-202-358-2770, E-mail: mmaiden@hq.nasa.gov; and Richard Olson, Oak Ridge National Lab, PO Box 2008 MS 6407, Oak Ridge, TN 37831-6407 USA, Tel: +1-865-574-7819, Fax: +1-865-574-4665, E-mail: rjo@ornl.gov; and Charles McClain, NASA Goddard Space Flight Center, Building 28 Room W107, Greenbelt, MD 20771 USA, Tel: +1-301-286-5377, Fax: +1-301-286-0268, E-mail: mcclain@calval.gsfc.nasa.gov

B03 Biogeochemistry of Land Use Change  (Joint with GS, H, PA)
Land use changes such as deforestation, grazing management, and agricultural expansion affect a range of biogeochemical processes, including the transport of nitrogen, carbon, and other elements in vegetation, soil, water, and  air.  This session will present results of field studies and modeling approaches designed to better understand the consequences of land use change on biogeochemical processes.  Land use change in a variety of ecosystems, both tropical and temperate, will be covered.
Conveners: Greg Asner, University of Colorado, Geological Sciences, Campus Box 399, Boulder, CO 80309 USA, Tel: +1-303-735-5033, E-mail: asner@terra.colorado.edu; and Alan Townsend, University of Colorado, Campus Box 450, Boulder, CO 80309 USA, Tel: +1-303-492-6865, Fax: +1-303-492-6388, E-mail: alan.townsend@colorado.edu

B04 Land Cover and Land Use Change: Implications for Resource Management (Joint with H, PA)
Collectively, local scale conversion of rural and agricultural land to suburban and urban uses has regional scale impacts on land and water resources.  This session focuses on the derivation and application of land cover and land use data to yield greater understanding of land use change implications for regional resource management.  Papers that detail models for land cover/land use change prediction or present the use of land cover/land use information in hydrological and chemical transport models are of particular interest.  While efforts in other areas are welcome, special emphasis will be placed on studies of the mid-Atlantic and New England regions.
Conveners: S. Goetz, University of Maryland, Department of Geography, College Park, MD 20742 USA, Tel: +1-301-405-1297, Fax: +1-301-314-9299, E-mail: sgoetz@geog.umd.edu; and J. Jones, U.S. Geological Survey, 521 National Center Science and Applications, USA, Tel: +1-703-648-5543, Fax: +1-703-648-4165, E-mail: jwjones@igsrn008.er.usgs.gov

B05 Remote Sensing to Address the Needs of Local Communities  (Joint with G, H, PA)
Remote sensing data from NASA's Earth Observing System (EOS) and other sensors can be used for a variety of commercial and government applications, although the satellite-monitoring tools were conceived to support research on global environmental change. Speakers in this session will share experiences and discuss results and future plans to illustrate the practical utility of remote sensing and GIS data in applications such as: urban planning and smart growth management, precision agriculture, protection of natural resources, hydrologic forecasting and disaster management and emergency response. For example, it is possible to work closely with Federal/State/County/City/Tribal government agencies to develop value-added products, prototype applications, and disseminate data and information to support viable decision-making and better management/allocation of resources.  Abstracts for the use of remote sensing to a range of practical applications are solicited for this session.
Conveners: Robert Plante, Raytheon Systems Corporation, Science Office, Upper Marlboro, MD 20774 USA, Tel: +1-301-925-0890, Fax: +1-301-925-0438, E-mail: rplante@eos.hitc.com; and Mohamed A. Mohamed, Raytheon Systems Corporation, Science Office, Upper Marlboro, MD 20774 USA, Tel: +1-301-925-0452, Fax: +1-301-925-0438, E-mail: mmohamed@eos.hitc.com; and Satya Kalluri, Raytheon Systems Corporation, Science Office, Upper Marlboro, MD 20774 USA, Tel: +1-301-925-0754, Fax: +1-301-925-0438, E-mail: skalluri@eos.hitc.com

B06 Contributions of Biogeosciences to the Millennium Ecosystem Assessment (Joint with PA)
The Millennium Ecosystem Assessment is an international effort to assess the state of the world's ecosystems and their abilities to provide goods and services important for human development. The assessment will involve the contributions of hundreds of scientists over the next several years and will provide information to policy makers on the current and future condition of ecosystems (see http://www.ma-secretariat.org).  This session will explore the contributions from the biogeosciences that make such an assessment possible, including observation and modeling studies on a range of ecosystems at regional and global scales.
Conveners: Anthony Janetos, World Resources Institute, 10 G Street, NE, Washington, DC 20002 USA, Tel: +1-202-729-7600, Fax: +1-202-729-7610, E-mail: ajanetos@wri.org; and Walter Reid, World Resources Institute, 731 N. 79th Street, Seattle, WA 98103 USA, Tel: +1-206-782-7963, Fax: +1-206-782-5682, E-mail: waltreid@attglobal.net

B07 Isotopes in Biogeochemistry and Global Change (Joint with A, GS, H, OS)
Variations in the isotopic composition of molecules due to biotic activity can provide substantial insight into the processes that have influenced these compounds during their lifetimes. These isotopic signals have led to significant advances in understanding the role of the biosphere in biogeochemical cycling and to how these cycles have changed over time. In this session, we encourage submission of isotope-based experimental and modeling-based approaches to understanding natural and anthropogenic changes to biogeochemical processes. We especially encourage submissions from fields such as oceanography, hydrology, atmospheric science, and terrestrial ecology which will facilitate the development of a cross-system understanding of biogeochemical transformations in a global change context.
Conveners: Jim Randerson, California Institute of Technology, MC 170-25 1200 E. California Boulevard, Pasadena, CA 91125 USA, Tel: +1-626-395-6123, Fax: +1-626-568-0935, E-mail: jimr@gps.caltech.edu; and Julianna Fessenden, USA,  E-mail: fessenden@biology.utah.edu

B08 Large Woody Debris and the Geomorphology, Hydrology and Ecology of Fluvial Systems (Moved to H13)

B09 Mercury in the Environment (Joint with A, GS, H, PA)
Atmospheric deposition of anthropogenic mercury is increasingly recognized as a threat to human health. Most U.S. States and many countries now recommend limits on human fish consumption, and fish-eating animals are also at risk. Although deposition in many areas now may be declining, Hg continues to bioaccumulate from years of cumulative inputs. We have much to learn about how mercury moves from the terrestrial to aquatic environment and within the aquatic environment to its uptake as methyl-Hg by biota. We invite papers on all aspects of environmental mercury cycling in air, land, water, and the biota - including, but not limited to, these questions. (1) Are we accurately measuring inputs of atmospheric Hg? How important are dry deposition and revolatilization? (2) How does Hg move from the terrestrial to the aquatic ecosystem? (3) What is the role of land use / land cover in Hg and methyl Hg fluxes? (4) What factors control Hg methylation? How important is the role of inundation and fluctuating water levels? (5) What are the important in-stream and in-lake processes affecting Hg mobility and food chain uptake?
Conveners: Jamie Shanley, U.S. Geological Survey, PO Box 628, Montpelier, VT 05601 USA, Tel: +1-802-828-4466, Fax: +1-802-828-4465, E-mail: jshanley@usgs.gov; and Neil Kamman, VT Department of Environmental Conservation, 103 S. Main Street 10N, Waterbury, VT 05671-0408 USA, Tel: +1-802-241-3795, Fax: +1-802-241-3287, E-mail: neil.kamman@state.vt.us

B10 Sedimentation in Coastal Marshes (Joint with H, OS)
Limited understanding of sedimentation processes in coastal marshes is a key constraint on the management of environmental impacts associated with sea level rise, degrading quality and quantity of aquatic habitats, and downstream impacts of watershed land use.  The problem is exacerbated by complex interactions among the numerous  physical, ecological, and chemical variables that impact sedimentation over a large range of spatial and temporal scales. This session seeks a broad cross-section of recent research on tidal marsh sedimentation from a variety of disciplinary and interdisciplinary perspectives.
Conveners: Greg B. Pasternack, University of California, Department of Land, Air, and Water Resources, Davis, CA 95616-8628 USA, Tel: +1-530-754-9243, Fax: +1-530-752-5262, E-mail: gpast@ucdavis.edu; and Lynn A. Leonard, Department of Earth Sciences, Deloach Hall, 610 S. College Road, Wilmington, NC 28403-3297 USA, Tel: +1-910-962-2338, Fax: +1-910-962-7077, E-mail: lynnl@uncwil.edu

B11 Linkages Between Biogeochemical and Hydrogeologic Processes in Shallow Ground-Water Systems of the Atlantic and Gulf Coastal Plains (Joint with H, PA)
It has been projected that by the year 2010, 75% of the U.S. population will live within 50 miles of our coastlines, leading to increased urban and agricultural pressures there. The Atlantic and Gulf Coastal Plains comprise a hydrogeologic landscape where increasing water demand for consumption and irrigation, nutrients from fertilizer and animal wastes, and contaminants from urbanization present a potential water resources threat due to the sandy, well drained soils, shallow aquifers, and many small hydrologically connected streams. Many of the biogeochemical processes controlling the transport and fate of contaminants in these systems, and their linkage to the hydrologic and geochemical setting are poorly understood. This session will focus on biogeochemical processes in shallow ground-water systems and hydrologically connected streams, and quantitative field studies to assess the role of the hydrologic and geochemical setting in transforming contaminants. Presentations are encouraged that describe hydrogeologic factors controlling biogeochemical processes, the extent to which subtle geochemical signals can be used to characterize important biogeochemical processes, and studies examining the hydrologic and geochemical connection between shallow aquifers and streams.
Conveners: Larry J. Puckett, U.S. Geological Survey, MS 413 National Center, Reston, VA 20192 USA, Tel: +1-703-648-5842, Fax: +1-703-648-6693, E-mail: lpuckett@usgs.gov; and B. Thomas Nolan, U.S. Geological Survey, MS 413 National Center, Reston, VA 20192 USA, Tel: +1-703-648-5666, Fax: +1-703-648-6693, E-mail: btnolan@usgs.gov

B12 Eco-hydrological Dynamics of Water Controlled Ecosystems (Joint with H, NG)
Many aspects of  the action of climate, soil, and vegetation on both the soil moisture dynamics and the soil nutrient cycle are not yet completely understood. In semi-arid climates these mechanisms are important to the dynamical evolution of vegetation ecosystems, which in turn are responsible for some control on climate and soil moisture dynamics. The section could solicit original papers on the analysis and modeling of soil moisture dynamics, vegetation evolution, as well as on the role of soil moisture and vegetation in the nutrient cycling. Theoretical results and data analyses aimed at providing indications of general validity will be important contributions to the section as a guide for the understanding and mathematical modeling of water-controlled ecosystems.
Conveners: Amilcare Porporato, Polytechnic of Turin, Department of Hydraulics, Turin, Italy, Tel: +39 011 564 5617, Fax: +39 011 564 5698, E-mail: porporato@polito.it; and Paolo D'Odorico, Texas A&M University, Department of Civil Engineering Environmental and Water Resources Division, 3136 TAMU, College Station, TX 77843-3136 USA, Tel: +1-979-458-2678, Fax: +1-979-862-1542, E-mail: Paolo@civilmail.tamu.edu

B13 CO2 Flux Measurements From the Ground Up (Joint with A, GS)
The session will address questions such as: Are component fluxes, such as soil, leaf, and/or bole measurements made with chambers consistent with the net fluxes measured with towers or balloons? What can CO2 flux measurements from soils, peats, or plants tell us about the underlying mechanisms controlling ecosystem uptake and release of carbon?   A complete understanding of the carbon balance of terrestrial ecosystems will require a combination of measurements and modeling of both net and component fluxes of CO2.  This session will include presentations on CO2 flux measurements with chambers, towers, and tethered balloons, and CO2 flux modeling studies that integrate component fluxes to an ecosystem carbon balance. The session will include papers from a range of terrestrial ecosystems, arctic to tropical, natural or managed, upland or wetland.
Conveners: Steve Frolking, University of New Hampshire, Institute for the Study of Earth, Oceans, and Space, Durham, NH 03824-2622 USA, Tel: +1-603-862-1792, Fax: +1-603-862-0188, E-mail: steve.frolking@unh.edu; and Patrick Crill, University of New Hampshire, Institute for the Study of Earth, Oceans, and Space, Durham, NH 03824-2622 USA, Tel: +1-603-659-8695, Fax: +1-603-862-3519, E-mail: patrick.crill@unh.edu

B14 Land-Atmosphere Interactions (Joint with A, H, NG)
The purpose of this session is to provide a forum for reporting recent advances in land-atmosphere interactions at the various spatial and temporal scales. Field experiments, remote sensing analyses, and modeling studies are all welcome.  Various types of exchanges between land and the atmosphere, including energy, water, and trace gases, will be considered as well as the impact on climate.
Conveners: Roni Avissar, Rutgers University, Department of Environmental Sciences, New Brunswick, NJ 08901-8551 USA, Tel: +1-732-932-9520, Fax: +1-732-932-3562, E-mail: avissar@gaia.rutgers.edu; and Ruth DeFries, University of Maryland, Department of Geography and Earth Systems, Science Interdisciplinary Center, College Park, MD 20742 USA, Tel: +1-301-405-4884, Fax: +1-301-314-9299, E-mail: rd63@umail.umd.edu

B15 Global Remote Sensing and in-situ Land Surface Data for Weather and Climate Models (Joint with A)
Global remote sensing and in-situ land surface data is crucial to the understanding of the land-atmosphere interaction which is one of the most important elements in the global climate system.  These data include land cover, fractional vegetation cover,  leaf-area index, canopy height, roughness length, albedo, soil texture, vegetation root, soil moisture, skin temperature, snow cover, snow depth, etc. Some of these data can only be obtained from remote sensing, while others need to be obtained through field survey and in-situ observations. The purpose of this special session is to bring together the data and weather/climate modeling community in the areas of atmospheric sciences, hydrology,  ecosystem, and remote sensing. Papers discussing remote sensing and in-situ land surface data for use in regional and global weather and climate models are solicited. Also welcome are papers that address the impact of various land surface data sets (particularly those from recent field programs and remote sensing missions) on weather and  climate modeling.
Conveners: Xubin Zeng, University of Arizona, Department of Atmospheric Sciences, PO Box 210081, Tucson, AZ 85721-0081 USA, Tel: +1-520-621-4782, Fax: +1-520-621-6833, E-mail: xubin@atmo.arizona.edu; and Forrest G. Hall, NASA Goddard Space Flight Center, Office for Global Carbon Studies, Code 923, Building 33, Room 413, Greenbelt, MD 20771 USA, Tel: +1-301-614-6659, Fax: +1-301-614-6695, E-mail: fghall@ltpmail.gsfc.nasa.gov

B16 Application of Modern Plant Observations to the Fossil Record: Implications for Paleoecology and Paleoclimatology
Recent observations of the chemical and ecological properties of plant taxa and plant communities have yielded predictive relationships for the reconstruction of paleoenvironments.  This session seeks to present a survey of recent observational relationships, as well as examples of application to plant fossil records.
Conveners: A. Hope Jahren, Johns Hopkins University, Department of Earth and Planetary Sciences, Baltimore, MD 21218 USA, Tel: +1-410-516-7134, Fax: +1-410-516-7933, E-mail: jahren@jhu.edu; and Ben LePage, University of Pennsylvania, Department of Earth and Environmental Science, Philadelphia, PA 19104-6316 USA, Tel: +1-215-989-5618, Fax: +1-215-898-0964, E-mail: blepage@sas.upenn.edu

Biogeosciences also presents jointly with the following Special Sessions:
A03 Transient Tracers in Geophysical Flows (Joint with B, H, OS)
A07 Calibration of Meteorological Satellite Sensors and Validation of Derived Products (Joint with B, H, OS)
GP06 Banded Iron Formation, its Chemical and Physical Properties and Relation to the Origin of Life (Joint with B, MR, P, V, GS, M)
H03 Subsurface Microbial Ecology of Contaminant Plumes (Joint with B, GS
H06 Natural and Enhanced Aquifer Denitrification (Joint with B)
H08 The Isotope Signature of the Groundwater Recharge (Joint with B, GS)
H09 Groundwater Flux at the Land-Ocean Margin: Physics, Chemistry, and Ecological Implications (Joint with B, GS, OS)
H17 Interrelationships Between Atmospheric Deposition and Landscape Features of Forest Catchments in Regulating Surface Water Biogeochemistry (Joint with B)
H18 Isotope Tracers as Process Monitors in Hydrologic Systems: Can They Be Trusted? (Joint with B, GS)
H19 Human Impacts on Nitrogen Cycling at Regional Scales: Science and Policy (Joint with B)
H22 Assessing Water Quality in Regional Drainage Basins and Aquifer Systems (Joint with B)
H27 Watershed-Atmosphere-Ecosystem Coupling: Prospects, Approaches and Experience (Joint with B)
H29 Smart Growth: Impacts on Urban Hydrology and the Protection of Natural Resources (Joint with B)
OS01 Non-Equilibrium Phenomena in Geophysics (Joint with A, B, H, P, S, T)
 

Geodesy

G01 Detection, Resolution and Interpretation of Non-Secular Variation in Geodetic Coordinates
This session covers the spectrum of non-secular time variation in coordinates from < 1 sec (e.g, seismology) to years (e.g., hydrology), including both the geophysical signals themselves, and the ability of geodesy (by method, network design, instrumentation, analysis techniques) to detect such signals, resolve model parameters, and discriminate competing hypotheses. It should also cover quantification and mitigation of systematic model errors and frame effects that can confound interpretation of real non-secular signals, and prospects for detecting and resolving specific signals by innovative experiment design and inter-technique synergy.
Convener: Geoff Blewitt, Nevada Bureau of Mines & Geology, University of Nevada/Reno, Mail Stop 178, Reno, NV 89557-0088 USA, Tel:+1-775-784-6691 Ext. 171, Fax: +1-775-784-1709, E-mail: gblewitt@unr.edu

Geodesy also presents jointly with the following Special Sessions:
A01 Earth Science Applications of Reflected and Refracted GPS Transmissions (Joint with G, GP, H, SA)
B05 Remote Sensing to Address the Needs of Local Communities  (Joint with G, H, PA)
T01 Recent Tectonics, Kinematics and Dynamics of Southeast Asian Margins (Joint with G, S)
T04 True Polar Wander on Earth, Mars and Beyond (Joint with G, GP, P)
 

Geomagnetism and Paleomagnetism

GP01 Mapping Aquifers, Oceans, and Planetary Bodies with Passive and Active EM Methods (Joint with H, OS, P)
Active electromagnetic methods are one of the primary techniques for remote sensing and mapping of shallow aquifers and waste-plumes. Passive EM techniques have recently been used to identify a potential ocean at Europa, and EM will necessarily figure prominently in future Martian exploration. We solicit papers on techniques, case studies, and potential future applications.
Conveners: Jeff Wynn, U.S. Geological Survey, 12201 Sunrise Valley Drive MS 954, Reston, VA 20192 USA, Tel: +1-703-648-6490, E-mail: jwynn@usgs.gov; and Pascal Tarits, UBO-IUEM, UMR Domaines Oceaniques Place Nicolas Copernic, Plouzane, F-29280 France, Tel: +33 2 98498763, E-mail: tarits@univ-brest.fr

GP02 Paleomagnetic Studies of the Atlantic-Bordering Continents: Rodinia to Pangea to Present (Joint with T)
The continents bordering the current Atlantic Ocean provide insights into geologic and tectonic history covering several billion years and involving the supercontinents of Rodinia and Pangea as well as numerous smaller continental pieces.  Paleomagnetic studies provide the necessary information to reconstruct these paleocontinents and to investigate details of their evolution.  We invite paleomagnetic papers on various aspects of structure, tectonics, and geologic evolution of present Atlantic-bordering continents at any time in their history.
Conveners: Laurie Brown, University of Massachusetts, Department of Geosciences, Amherst, MA 01003 USA, Tel: +1-413-545-0245, Fax: +1-413-545-1200, E-mail: lbrown@geo.umass.edu; and Conall MacNiocall, Oxford University, Department of Earth Sciences, Oxford, OX1 3PR UK, Tel: +44-1865-282135, E-mail: Conall.Macniocaill@earth.ox.ac.uk

GP03 Paleomagnetic Puzzles, Rock Magnetic Riddles (Joint with MRP, M)
Many paleomagnetic and rock magnetic studies produce data that while reproducible remain mysterious. The data cannot be interpreted by the easy rules of thumb by which most practitioners operate, yet they are not 'noise' or the result of carelessness. This poster session is conceived to address the issue of the unpublished enigmatic data that has been collected and sequestered in the filing cabinets of the paleomagnetic and rock magnetic community.
Conveners: Carlo Laj, CEA-CNRS, Avenue de la Terrasse Batiment 12, Gif-sur-Yvette, 91198 France, Tel: +33-1-6982-3538, E-mail: laj@eole.cfr.cnrs-gif.fr; and Lisa Tauxe, Scripps Institute of Oceanography, La Jolla, CA 92093-0220 USA, Tel: +1-858-534-6084, E-mail: ltauxe@ucsd.edu

GP04 Fluctuations of the Earth's Magnetic Field (Direction and Intensity): From Paleosecular Variation to Reversals (Joint with SEDI)
Despite recent growth of the quality and quantity of geomagnetic intensity measurements,  reliable paleointensity results are still scarce and cannot be yet used to document the general characteristics of the Earth's magnetic field. It has been recently shown that paleointensity during and around transitions is a fundamental constraint on recent numerical models that promise to provide unprecedented insight into the operation of the geodynamo. The new high quality experimental data from volcanic and sedimentary records, which describe the behavior of full geomagnetic field vector (directions and intensity), are welcome. Contributions on related theoretical modeling as well as new and improved techniques are also encouraged.
Conveners: Avto Gogichaishvili, Ciudad Universitaria, U.N.A.M. Instituto de Geofisica, Depto de Paleomagnetism y Geofisica Nuclear, Mexico, D.F. 04510 Mexico, Tel: +52 5 622 4230, Fax: +52 5 550 2486, E-mail: avto@tonatiuh.igeofcu.unam.mx; and Peter Riisager, Danish Lithosphere Centre, Oester Voldgade 10, 1350 Copenhagen K, Denmark, Tel: +45 38142638, Fax: +45 33110878, E-mail: pri@dlc.ku.dk

GP05 Earth and Planetary Magnetic Survey Satellites (Joint with P)
Papers are solicited on results from magnetic field satellites operational during the Decade of Geopotential Research (1998-2008) and on all recent planetary (Mars, Moon, Eros) magnetometer-carrying missions.
Conveners: Y. Cohen, Institut de Physique du Globe de Paris, Departement de Geomagnetisme et Paleomagnetisme 4, place Jussieu, Paris, 75252 France, Tel: +33-0144273904, E-mail: cohen@ipgp.jussieu.fr; and N. Grammatica, Danish Space Research Institute, Juliane Maries Vej 30, Copenhagen, DK-2100 Denmark, Tel: +45-3532-5830, E-mail: naphisica@dsri.dk; and M. Purucker, USA, E-mail: purucker@geomag.gsfc.nasa.gov

GP06 Banded Iron Formation, its Chemical and Physical Properties and Relation to the Origin of Life (Joint with B, MR, P, V, GS, M)
Early stages of the development of life on Earth can be associated with the environment which led to the deposition of Banded Iron Formations (BIFs). A comparative planetology approach to the origin of life suggests we look for possible analogs elsewhere in the solar system. We solicit papers on the physical, isotopic, and chemical characteristics of BIFs and their possible analogs.
Conveners: Gunther Kletetschka, GSFC/NASA, Code 691/695, Greenbelt, MD 20771 USA, Tel: +1-301-286-3804, E-mail: gunther@denali.gsfc.nasa.gov; and J. L. Kirschvink, Caltech, Division of Geology and Planetary Sciences 170-25, Pasadena, CA 91125 USA, Tel: 626-395-6136, E-mail: kirschvink@caltech.edu

GP07 Magnetic Investigations of the Antarctic (Joint with T)
This session highlights magnetic programs and investigations of the Antarctic, including the first compilation of the Antarctic magnetic anomaly map by ADMAP (Antarctic Digital Magnetic Anomaly Project). Papers are solicited on the Antarctic core, lithospheric, and external geomagnetic fields, as well as rock physical properties, and gravity and other geophysical studies that contribute to understanding south polar geomagnetism.
Conveners: Ralph Von Frese, Ohio State University, Department of Geological Sciences, 125 S. Oval Mall, Columbus, OH 43210 USA, Tel: +1-614-292-5635, E-mail: vonfrese.1@geology.ohio-state.edu; and Massimo Chiappini, Istituto Nazionale di Geofisica, Via di Vigna Murata 605, Roma, 00143 Italy, E-mail: chiappini@ingrm.it; and Peter Morris, British Antarctic Survey, High Cross Madingley Road, Cambridge, United Kingdom, E-mail: pmor@bas.ac.uk

GP08 Precise Correlation of Strata: Magnetic and Other Methods (Joint with OS, V)
Precise regional and global correlations of strata remain a great challenge. Although magnetic polarity stratigraphy is widely applied, it requires calibration by other methods. Multidisciplinary methods involving radio-isotope dating, faunal assemblages, cyclic (Malankovitch) litho-variations, stable isotope ratios, marker horizons (ashes and tektite layers), unique chemical signatures, and a variety of magnetic methods provide the best results. Among the magnetic methods, recent studies suggest that unique magnetic susceptibility signatures may allow precise global correlations near certain time horizons. This session focuses on magnetic methods for correlation of strata but also invites contributions from other specialities.
Conveners: William D. MacDonald, State University of New York, Department of Geological Sciences, Binghamton, NY 13902 USA, Tel: +1-607-777-2863, Fax: +1-607-777-2288, E-mail: wdmacdon@binghamton.edu

Geomagnetism and Paleomagnetism also presents jointly with the following Special Sessions:
A01 Earth Science Applications of Reflected and Refracted GPS Transmissions (Joint with G, GP, H, SA)
S01 Core Mantle Boundary Region (Joint with GP, GS, MR, NG, SEDI, T)
T03 Computational Earth Laboratories (Joint with GP, M, MR, NG, S)
T04 True Polar Wander on Earth, Mars and Beyond (Joint with G, GP, P)
 

Geochemical Society

GS01 Magmatic Volatile Histories: Stable Isotopic Tracing of Sources and Degassing Processes in Magmatic Systems and Implications for Volcanology and Earth System Science (Joint with T, M)
Stable isotopic tracing of magmatic volatiles (CO2, H2O, and SO2/H2S in particular), from their source to magmatic degassing processes, have provided information of potential use to several disciplines in science. Isotopic fractionation between volatile species in the melt and exsolving vapor phases often allows quantification of volcanic volatile budgets, particularly when the extent of degassing is constrained by studies of glass inclusions and tephra matrix glasses. These results have implications for several fields of research, including volcanology, hazard management, climatology/atmospheric science, and economic geology. This session will bring together contributions from the field, laboratory, and theoretical/numerical modeling to outline a state-of-the-art understanding of what we know and what we have yet to learn regarding sourcing, storage, and degassing of volatiles from magmas in all tectonic settings.
Conveners: Bruce E. Taylor, Geological Survey of Canada, Ottawa, ON K1A 0E8 Canada, Fax: +1-613-943-1286, E-mail: btaylor@nrcan.gc.ca; and Charlie Mandeville, American Museum of Natural History, New York, NY 10024-5192 USA, Fax: +1-212-769-5339, E-mail: cmandy@amnh.org

GS02 Light Stable Isotope Ratio Standards Metrology: Recent Advances and Needs Assessment (Joint with V)
The measurement, calibration and data reduction issues concerning the light stable isotope reference materials (e.g., tritium, sulfur, nitrogen, oxygen and carbon, both inorganic and organic) are of major importance to all that use isotopes as a tool to quantify earth processes.  Over the past several years there have been some exciting metrological advances including a novel and very successful CO2 intercomparison exercise, the nearly fully realized VCDT scale for sulfur isotopes and a reassessment of the half life of tritium.  The value assignments of nearly all of the standards for the above mentioned elements will soon be updated and published.  This session will focus on how best to effectively relate and disseminate measurement results across laboratories, industries, nations, and international networks so that real progress is made at understanding complex chemical systems of importance to the atmospheric and geologic communities and are traceable at the highest level.  Additionally, despite the fact that continuous flow mass spectrometric techniques are proliferating, there exists almost a complete lack of reference materials for these analyses. Contributions are invited that focus on these issues so that; 1.) the atmospheric and geologic communities are informed of current NIST and IAEA recommended practices and 2.) as a forum for presenting new results on appropriate isotopic reference materials for both bulk and compound specific continuous flow techniques.
Convener: Donna B. Klinedinst, National Institute of Standards and Technology, 100 Bureau Drive MS 8372, Gaithersburg, MD 20899-8372 USA, Tel: +1-301-975-3927, Fax: +1-301-926-6689, E-mail: donna.klinedinst@nist.gov

Geochemical Society also presents jointly with the following Special Sessions:
B01 Carbon Saturation in Ecosystems: Controls, Limits, and Implications (Joint with GS)
B03 Biogeochemistry of Land Use Change  (Joint with GS, H, PA)
B07 Isotopes in Biogeochemistry and Global Change (Joint with A, GS, H, OS)
B09 Mercury in the Environment (Joint with A, GS, H, PA)
B13 CO2 Flux Measurements From the Ground Up (Joint with A, GS)
GP06 Banded Iron Formation, its Chemical and Physical Properties and Relation to the Origin of Life (Joint with B, MR, P, V, GS, M)
H03 Subsurface Microbial Ecology of Contaminant Plumes (Joint with B, GS)
H04 Geologic Sequestration of Carbon Dioxide (Joint with GS)
H05 Physicochemical Hydrodynamics of Nonaqueous Phase Liquid in Porous and Fractured Media (Joint with GS, NG)
H08 The Isotope Signature of the Groundwater Recharge (Joint with B, GS)
H09 Groundwater Flux at the Land-Ocean Margin: Physics, Chemistry, and Ecological Implications (Joint with B, GS, OS)
H18 Isotope Tracers as Process Monitors in Hydrologic Systems: Can They Be Trusted? (Joint with B, GS)
H20 Arsenic and Other Toxic Metals in Natural Waters (Joint with GS)
M02 Characterizing Organic and Inorganic Hydrothermal Systems (Joint with V, GS)
OS02 High-Resolution Climate Records From Laminated Sediments (Joint with V, GS)
P02 New Views of the Moon (ORAL) (Joint with V, GS)
S01 Core Mantle Boundary Region (Joint with GP, GS, MR, NG, SEDI, T)
S04 How Rifting Worked in Northeastern North America (Joint with T, V, GS)
S06 The Structure and Early Evolution of Cratons (Joint with T, V, GS)
T02 Dynamics of Gas Hydrate Reservoirs and Similar Shallow Marine Flow Systems (Joint with B, GS, H, OS)
V01 Continental Weathering and Ocean Chemistry (Joint with H, OS, GS)
V05 The Construction of Archean Cratons: Reconciling Radiometric Dates From Crustal and Mantle Rocks (Joint with T, GS)
 

Hydrology

H01  Pore-Scale Characterization of Subsurface Transport and Fate Processes
Pore-scale processes are important because many mixing, mass transfer, and reaction phenomena in the subsurface depend upon factors such as local solute concentrations, pore-space topology, and grain-scale heterogeneity. Pore-scale processes are also important because they affect the models and parameters used at the Darcy or field-scale. The goal of this session is to present results from innovative experimental and modeling techniques that examine pore-scale transport and fate processes, and the effects of these processes at a larger scale. Topics of interest include multi-phase flow, DNAPL dissolution, systems with dynamically changing pore-space topology (e.g., fracture dissolution), colloid-facilitated transport, biodegradation, and dispersive mixing. Systems dealing with both artificial and natural porous media are of interest.
Conveners: Albert Valocchi, Department of Civil and Environmental Engineering, University of Illinois at Urbana-Champaign, 205 North Mathews Ave., MC-250, Urbana, IL 61801 USA, Tel: +1-217-333-3176, Fax: +1-217-333-0687, E-mail: valocchi@uiuc.edu; and Charles Werth, Department of Civil and Environmental Engineering, University of Illinois at Urbana-Champaign, 205 North Mathews Ave, MC-250, Urbana, IL 61801 USA, Tel: +1-217-333-3822, Fax: +1-217-333-6968, E-mail: werth@uiuc.edu; and Thomas Baumann, Department of Hydrogeology, Hydrochemistry and Environmental Analytical Chemistry, Technical University Munich (TUM), Marchioninistrasse 17, D-81377 Munich, Germany, Tel: +49-89-7095-7993, Fax: +49-89-7095-7999, E-mail: thomas.baumann@ch.tum.de

H02 Methods for Identifying Contaminant Source Location, Release History, and Boundary-Initial Conditions
There exists a need for a suite of field measurement and simulation tools that can both reconstruct the spatial/temporal history of contaminant plumes in groundwater and identify the contaminant source location, geometry, and release rate. Reconstruction is complicated by uncertainty in quantifying plume transport processes (dispersion, retardation and transformation) and the ill-posedness of the problem. Methods applied to the problem to date include tools such as: modeling, isotope composition analysis, and chemical fingerprinting. Papers are encouraged that will enhance interaction and synergism among different groups, in particular mathematical modelers, field experimentalists, tracer hydrologists, forensic legal experts, and regulatory agencies.
Conveners: A.C. Bagtzoglou, Columbia University, Department of Civil Engineering and Engineering Mechanics, 500 W. 120th Street, New York, N.Y. 10027 USA, Tel.: +1-212-854-3154, Fax: +1-212-854-6267, E-mail: abagtzog@civil.columbia.edu; and Zbigniew J. Kabala, Duke University, Department of Civil and Environmental Engineering, Durham, NC 27708-0287 USA, Tel.: +1-919-660-5479, Fax: +1-919-660-5219, E-mail: kabala@copernicus.egr.duke.edu

H03 Subsurface Microbial Ecology of Contaminant Plumes (Joint with B, GS)
The activities of subsurface microbial populations are critical to the long-term fate of biodegradable groundwater contaminants. Plumes of degradable contaminants exhibit temporal changes in redox conditions and sharp spatial chemical gradients, particularly at plume boundaries. Aquifers impacted by these changes offer a variety of ecological niches for subsurface microorganisms which are only beginning to be explored. The purpose of this session is to examine how geochemical variations in contaminant plumes control (1) the genesis, propagation, and death of subsurface microbial communities and (2) the associated contaminant degradation. Papers that evaluate the development of microbial populations in the field or laboratory, as well as the aqueous and solid phase chemical changes associated with microbial succession are welcome. Modelling approaches to understanding microbial succession in contaminated subsurface environments are also encouraged. Other microbial ecology issues that may be explored include the distribution of populations between attached and suspended phases, predation by protists, and degradation processes mediated by microbial consortia.
Conveners: Barbara Bekins, U.S. Geological Survey, 345 Middlefield Road, MS 496, Menlo Park, CA 94025 USA, Tel.: +1-650-329-4691, E-mail: babekins@usgs.gov; and Isabelle Cozzarelli, U.S. Geological Survey, 12201 Sunrise Valley Drive, MS 431, Reston, VA 20192 USA, Tel.: +1-703-648-5899, E-mail: icozzare@usgs.gov

H04 Geologic Sequestration of Carbon Dioxide (Joint with GS)
Recently, interest has grown in sequestering CO2 in geologic formations to prevent the accumulation of greenhouse gases in the atmosphere.  Many issues must be addressed to assess the effectiveness and safety of this approach.  Issues include — how much CO2 can be sequestered?  Which formations are good for sequestration?  How can CO2 migration be monitored? How effective are hydrodynamic traps and will geochemical interactions transform CO2 into stable aqueous or mineral phases?  What are the potential environmental impacts of geologic sequestration?  This session invites papers related to these issues in the areas of (1) flow and transport simulation, (2) geophysical, hydrological and geochemical monitoring of CO2 migration in the subsurface, (3) geochemical interactions controlling the long term fate and environmental impacts of sequestered CO2, (4) geomechanical factors affecting the integrity of the reservoir seal and (5) environmental impacts of CO2 sequestration on water resources.
Conveners: Sally M. Benson, Lawrence Berkeley National Laboratory, Earth Sciences Division, 1 Cyclotron Road, MS 90-1116, Berkeley, CA 94720 USA, Tel.: +1-510-486-5875, Fax: +1-510-486-7714, E-mail: smbenson@lbl.gov; and Robert C. Burruss, U.S. Geological Survey, National Center, MS 956, 12201 Sunrise Valley Drive, Reston, VA 20192 USA, Tel.: +1-703-648-6144, Fax: +1-703-648-6419, E-mail: burruss@usgs.gov; and Larry Myer, Lawrence Berkeley National Laboratory, Earth Sciences Division, 1 Cyclotron Road MS 90-1116, Berkeley, CA 94720 USA, Tel.: +1-510-486-6456, Fax: 1+510-486-7714, E-mail: lrmyer@lbl.gov

H05 Physicochemical Hydrodynamics of Nonaqueous Phase Liquid in Porous and Fractured Media (Joint with GS, NG)
Mass exchanges between NAPL, aqueous, gas, and solid phases are important processes with regard to the ultimate fate of NAPLs in the subsurface. However, our ability to quantify rates of interphase mass exchange at the field scale is still insufficient. Multiphase mass exchange processes have been investigated intensely in other disciplines, notably chemical engineering. The intent of this session is to bring together researchers and practitioners from the hydrology, chemical engineering, and others communities. We seek contributions that include results from theoretical, mathematical modeling, and experimental studies of the physico-chemical hydrodynamics of the nonaqueous-phase-liquid/water interface at different scale for enhancing aquifer remediations.
 The following schedule is suggested:
Oral Sessions: 3 oral sessions are desired. Each expected to cover a specific topics such as:
i- Physicochemical hydrodynamic of NAPL-APL interface.
ii- Numerical and Analytical modeling of NAPL in the subsurface.
iii- Cleanup efforts, applications in real field cases.
One-half day poster Session.
Conveners: Said Doss, Lawrence Livermore National Laboratory, L-530, Livermore, CA 94551 USA, Tel.: +1-925-423-4281, E-mail: doss1@llnl.gov; and Souheil Ezzedine, Lawrence Livermore National Laboratory, L-530, Livermore, CA 94551 USA, Tel.: +1-925-422-0565, Fax: +1-925-424-3155, E-mail: ezzedine1@llnl.gov; and Andrew F. B. Tompson, Lawrence Livermore National Laboratory, L-204, Livermore, CA 94551 USA, Tel.: +1-925-422-6348, Fax: +1-925-422-1997, E-mail: afbt@llnl.gov; and John Ziagos, Lawrence Livermore National Laboratory, L-544, Livermore, CA 94551 USA, Tel.: +1-925-422-5479, Fax: +1-925-423-5764, E-mail: ziagos1@llnl.gov

H06 Natural and Enhanced Aquifer Denitrification (Joint with B)
Nitrate is the most common groundwater contaminant (Freeze and Cherry, 1979). As such, understanding denitrification is essential for groundwater quality protection and aquifer remediation. The goal of this session is to present basic and applied research on natural and enhanced aquifer denitrification. Topics may include, but are not limited to: use of stable isotope ratios to monitor denitrification; field experiments to determine denitrification rates and associated geochemical reactions; niches for and characteristics of denitrifying bacteria; analytical and numerical models of denitrification; selection of electron-donor amendments for enhanced denitrification; design of amendment delivery systems; limiting biofouling; and criteria for evaluating and managing denitrification in aquifers.
Conveners: Simon Bottrell, School of Earth Sciences, The University of Leeds, Leeds LS2 9JT, UK, Tel.: +44-113-233-5228, Fax: +44-113-233-5259, E-mail: S.Bottrell@earth.leeds.ac.uk; and Scott F. Korom, Department of Geology & Geological Engineering, PO Box 8358, University of North Dakota, Grand Forks, ND 58202-8358 USA, Tel.: +1-701-777-6156, Fax: +1-701-777-4449, E-mail: scott_korom@mail.und.nodak.edu; and Roy Spalding, University of Nebraska-Lincoln, 103 Natural Resources Hall, Lincoln, NE 68583-0844 USA, Tel.: +1-402-472-8214, Fax: +1-402-472-9599, E-mail: rspalding@unl.edu

H07 Strategies for Water Supply Development / Management in Developing Nations
Provision of water supplies of sufficient quantity and quality remains a critical challenge in the economic development of many regions of the third world. In this session, we seek papers which discuss strategies for the development and/or management of water resources in developing countries. We anticipate that a range of topics will be covered including, but not limited to, efficient use of water for agriculture and industry, technical and social issues related to development of water resources in complex geologic settings (e.g., in fractured crystalline rock or arid environments), evaluation of the economic value of water, concepts in water source protection, and novel strategies for reducing risk from chemical and biological contaminants.
Conveners: Stephen E.Silliman, Department of Civil Engineering, University of Notre Dame, Notre Dame, IN 46556 USA, Tel.: +1-219-631-5846, Fax: +1-219-631-9236, E-mail: silliman@thiem.ce.nd.edu; and Nina D. Rosenberg, Lawrence Livermore National Laboratory, L-206, Livermore, CA 94551 USA, Tel.: +1-510-424-5212, E-mail: nina@s11.es.llnl.gov

H08 The Isotope Signature of the Groundwater Recharge (Joint with B, GS)
The stable isotope composition of groundwater is being widely used to characterize among others, the geographic location of the recharge zones, the seasonality of the recharge process and the contribution of surface waters to the groundwater. Such characterisations are commonly based on very simplified assumptions regarding the change of the isotopic composition of the groundwater relative to that of the precipitation input (termed the Isotope Transfer Function {ITF} of the recharge process), which neglect the eco-hydrological feedbacks. This special session invites papers that address field experience in applying stable isotopes to the description of recharge processes under a variety of settings, attempts to model the ITF and applications that would enable a reliable paleo-climatic interpretation of the isotopic composition of old groundwaters.
Conveners: Klaus-Peter Siler, GSF Institute of Hydrology, Ingolstädter Landstraße 1, D-85764 Neuherberg, Germany, Tel.: +49 (0)89 3187-2585, Fax: +49 (0)89 3187-3361, E-mail: seiler@gsf.de; and Joel Gat, Ben-Gurion University, Center for Water Science and Technology, Sede Boker Campus, 84990, Israel, Tel.: +972-7-659-6714, Fax: +972-7-659-6889, E-mail: jgat@bgumail.bgu.ac.il

H09 Groundwater Flux at the Land-Ocean Margin: Physics, Chemistry, and Ecological Implications (Joint with B, GS, OS)
The ongoing migration of human populations to the world's coastal zones has placed a new emphasis on a range of scientific and social issues related to the interaction between groundwater and surface water and between freshwater and saltwater at the margin between land and ocean.  This session focuses on studies that constrain the amount, location, or degree of spatial and temporal variability of groundwater flux into estuaries, bays, and the coastal ocean through direct measurements (e.g., seepage and flux meters), geophysical surveys, geochemical (e.g., nutrient, radiotracer) analyses, or remote sensing (e.g., thermal infrared surveys).   Studies that link freshwater-saltwater interactions at the land-ocean margin to ecological conditions are also welcome, as are the new generation of modeling studies that emphasize flow and transport processes near the land-ocean margin.
Conveners: C. Ruppel, School of Earth and Atmospheric Sciences, Georgia Tech, Atlanta, GA  30332-0340 USA, Tel.: +1-404 894-0231, Email: cdr@piedmont.eas.gatech.edu; and S. Joye, Department of Marine Sciences, University of Georgia, Athens, GA 30602 USA, Tel.: +1-706 542-5893, Email: mjoye@arches.uga.edu

H10 Subsurface Transport of Domestic and Animal-Farm Wastewater Pollutants from Site to Watershed Scales
Approximately 25% of all homes in the United States use individual soil-based wastewater treatment systems (SBWTS) to dispose of and treat household wastewater.  In addition, large animal feeding operations generate a substantial amount of wastewater pollution.  Potential subsurface pollution from wastewater contaminants (e.g., nitrogen, phosphates, biological pathogens, organic chemicals, etc.) is important at various scales in a watershed, including the point scale at individual homes, and upward to the watershed scale, where wastewater pollutants from up-gradient sources may impact the groundwater (drinking-water) supply.  In addition, wastewater sources of contaminants make a substantial contribution to the allowable total maximum daily loads (TMDLs) in streams and rivers.  Groundwater transport and transformation of wastewater pollutants at the watershed scale are not well understood. Predicting the biophysicochemical processes at the watershed scale requires a thorough understanding of the processes at the site and intermediate scales. This session will include papers that elucidate the processes influencing transport and transformation of wastewater pollutants from the site to watershed scales. Papers that describe the results of laboratory, site or field scale studies, or aim to improve modeling efforts of site- and field-scale processes, are especially encouraged.
Conveners: John E. McCray, Department of Geology and Geological Engineering, Colorado School of Mines, Golden, CO 80401-1887 USA, Tel.: +1-303-384-2181, Fax: +1-303-273-3859; E-mail: jmccray@mines.edu; and Robert L. Siegrist, Environmental Science and Engineering, Colorado School of Mines, Golden, CO 80401-1887 USA

H11 Fundamental Physics of Vadose Zone Flow and Transport
Conceptual models for flow and transport in the vadose zone must be founded on a solid understanding of the underlying physical processes.  This session will focus on laboratory, field, and numerical experiments exploring the fundamental physics of unsaturated flow and transport.  Similar investigations considering multi-phase flow are also encouraged.
Conveners: Michael Nicholl, M3GE, University of Idaho, Moscow, ID 83844-3024 USA, Tel.: +1-208-885-9242, Fax: +1-208-885-2855, E-mail: mnicholl@uidaho.edu; and Jerry Fairley, Geological Sciences, University of Idaho, Moscow, ID 83844-3022 USA, Tel.: +1-208-885-9259, Fax: +1-208-885-5724, e-mail: jfairley@uidaho.edu

H12 Computational Fluid Dynamics Applications to Rivers (Joint with NG)
Geomorphological and hydrological applications of computational fluid dynamics.  There is growing interest amongst geomorphologists and other fluvial scientists in several countries in applying vertically-averaged or full 3-D Computational fluid dynamics (CFD) models to flow in rivers, tidal channels, or over floodplains. Many such applications are technically challenging so a session to review both the potential and the problems is seen as timely. Papers which demonstrate novel geomorphologically-oriented applications of CFD are encouraged, along with papers which examine technical issues involved in setting up and testing such models, and papers concerned with how flow modelling can be used to help predict sediment transport.
Conveners: Rob Ferguson, Department of Geography, Sheffield University, Sheffield S10 2TN, UK, Tel.: +44 114 222 7907, E-mail: r.ferguson@shef.ac.uk; and David Furbish, Department of Geological Sciences, Florida State University, Tallahassee, FL 32306-4100 USA, Tel.: +1-850-644-5892, Fax: +1-850-644-4214, E-mail: furbish@gly.fsu.edu

H13 Large Woody Debris and the Geomorphology, Hydrology and Ecology of Fluvial Systems
Research has shown that large woody debris can significantly affect the structure and function of rivers and streams.  In light of increasing awareness regarding the influence of large woody debris, new issues are emerging regarding its management in streams and rivers.  However, research and management of large woody debris both occur in diverse settings.  To address this heterogeneity, this session endeavors to bring together researchers studying large woody debris in a variety of systems that vary based on degree of human impact, scale, gradient, and geographic location.  In particular, abstracts are solicited on the role of large woody debris in the geomorphology, hydrology and ecology of fluvial systems.
Conveners: Melinda D. Newell, Department of Geography, University of Illinois, Urbana, IL 61801 USA, Tel: +1-217-333-1880, Fax: +1-217-244-1785, E-mail: mdnewell@uiuc.edu; and Gordon Grant, USFS Pacific Northwest Forest and Range Research Station, 280 Forestry Sciences Lab, Corvallis, OR 97331 USA, Tel: +1-541-750-7328, Fax: +1-541-737-1200, E-mail: Gordon.Grant@orst.edu

H14 Geomorphology (POSTER ONLY) (Joint with NG)
Diverse approaches are required to understand the processes of erosion, transport, and deposition of sediment and solutes, and to predict their influence on short- and long-term landscape changes.  In this session we solicit poster presentations on geomorphic processes, particularly the influence of wind, water, and ice on the land surface; the behavior of soil, rock, and ice under applied stresses; and the rates of landscape development and the ages of surfaces.  We welcome contributions from field or lab experiments, modeling, field monitoring, application of cosmogenic radionuclides, and development of new techniques.  Please send one copy of your abstract to AGU and one copy directly to both of the conveners.
Conveners: Arjun M. Heimsath, Dartmouth College, Department of Earth Sciences, 6105 Fairchild Hall, Hanover, NH 03755-3571 USA, Tel.: +1-603-646-2374, Fax: +1-603-646-3922, E-mail: Arjun.Heimsath@Dartmouth.edu; and Kelin X. Whipple, Department of Earth, Atmospheric and Planetary Sciences, Massachusetts Institute of Technology, Rm 54-1016, Cambridge, MA 02139 USA, Tel.: +1-617-253-2578, Fax: +1-617-252-1800, E-mail: kxw@mit.edu

H15 Recent Advances in Forested Catchment Intercomparison (POSTER ONLY)
Comparison of results among forested headwater catchment studies is complicated by differences in climate, geomorphology, geology, and spatial scale, yet such comparisons are critical to determine general patterns and hence to elucidate processes controlling streamflow generation and water quality genesis. Posters are solicited that either explicitly compare results among catchments or state general principles that can be tested across catchments. Appropriate topics include hydrologic, biogeochemical and geomorphic processes in headwater catchments, and recent advances in instrumentation, tracer, and modeling techniques.  The poster session will be followed by roundtable discussion of themes emerging from posters.
Conveners: Richard P. Hooper, U.S. Geological Survey, 10 Bearfoot Road, Northborough, MA 01532 USA, Tel: +1 508-490-5065, Fax: +1 508-409-5068, E-mail: rphooper@usgs.gov; and Maki Tsujimura, Institute of Geosciences, University of Tsukuba, Tsukuba, Ibarki 305-8571, Japan, Tel: +81-298-53-2568, Fax: +81-298-51-9764, E-mail: mktsuji@atm.geo.tsukuba.ac.jp

H16 Recent Advances in Forested Catchment Intercomparison (MODERATED DISCUSSION)
As a follow-up to the poster session, a discussion session will be held in lieu of an oral session. Discussants will be used to encourage audience participation and to facilitate interaction among participants. Themes to be discussed include processes controlling streamflow generation and water quality across a range of spatial scales, the feasibility of a "standard" catchment characterization to aid in catchmnet intercomparison, and topics that emerge from the posters. Discussants will be Maki Tsujimura and Yuichi Onda (Univ. of Tsukuba), Nobu Ohte (Univ. of Kyoto), Jeff McDonnell (Oregon State University) and Rick Hooper (USGS).

H17 Interrelationships Between Atmospheric Deposition and Landscape Features of Forest Catchments in Regulating Surface Water Biogeochemistry (Joint with B)
Forest watersheds in the USA and Canada have been studied with particular emphasis on evaluating the effects of atmospheric deposition on surface water quality.  Landscape features including uplands, wetlands and lakes have a major influence on water flow paths and biogeochemical transformations of atmospheric inputs.  Differences in forest vegetation including the stage of maturation and species composition have also been shown to influence biogeochemical processes within forests.  These differences in landscape attributes combined with patterns of atmospheric deposition contribute to strong temporal and spatial variation in surface water chemistry within and among regions. This session will address similarities and differences in surface water chemistry of intensively studied forest watersheds.  Particular focus will be given to studies that have included synoptic, site-intensive, and experimental investigations.  Results from these studies provide a template for a comprehensive evaluation of the interrelationships between hydrology and biogeochemistry in affecting surface water chemistry.
Conveners: Myron J. Mitchell, SUNY-ESF, 1 Forestry Drive, Syracuse, NY 13210-2788 USA, Tel: +1-315-470-6765, Fax: +1-315-470-6996, E-mail: mitchell@mailbox.syr.edu; Charles T. Driscoll, Syracuse University, Syracuse, NY 13244 USA, Tel: +1-315-443-3434, Fax: +1-315-443-1243, E-mail: ctdrisco@mailbox.syr.edu

H18 Isotope Tracers as Process Monitors in Hydrologic Systems: Can They Be Trusted? (Joint with B, GS)
Determining the important biotic and abiotic chemical processes in hydrologic systems is essential to our ability to assess both trends in water quality and the effectiveness of remediation efforts.  Isotope tracers are commonly used as process monitors in hydrologic systems, but can provide ambiguous information. For example, stable isotope variations resulting from abiotic processes may be similar in magnitude to those resulting from biologic activity, and thus the isotope compositions considered alone may not provide a robust "biosignature".  The purpose of this session is to explore the effectiveness of both stable and radiogenic isotope tracers as monitors of both biotic and abiotic processes.  We particularly encourage abstracts that discuss water quality studies in which application of a "multi-tracer" approach has provided an especially rigorous assessment.
Conveners: Thomas Bullen, U.S. Geological Survey, MS 420, 345 Middlefield Rd., Menlo Park, CA 94025USA, Tel: +1-650-329-4577, Fax +1-650-329-4538, E-mail: tdbullen@usgs.gov; and Thomas Johnson, University of Illinois at Urbana-Champaign, Urbana, IL 61801 USA, Tel: +1-217-244-2002, Fax: +1-217-244-4996, E-mail: tmjohnsn@uiuc.edu

H19 Human Impacts on Nitrogen Cycling at Regional Scales: Science and Policy (Joint with B)
Globally, the cycling of nitrogen (N) is changing more rapidly than that of any other element cycle, with significant environmental consequences. We seek presentations focusing on N transport and transformations at the scale of large catchments or regions.  Topics include all components of regional nitrogen budgets: pollution of surface waters and groundwater; atmospheric deposition of nitrogenous compounds and its effects; agricultural N transfers (e.g. production and consumption of food & feed); estimates of N processing (e.g., fixation in forests or crop lands, denitrification & other sinks); water quality standards (e.g., critical loads, nutrient criteria); source identification (e.g., nitrogen-oxygen multi-isotope approaches); assessments (e.g., concentrations and fluxes, consequences of N pollution, risk, and future impacts); and policy developments.
Conveners: Robert W. Howarth, Environmental Defense, 6 North Market Bldg., Faneuil Hall Marketplace, Boston, MA 02109 USA, Tel: +1-607-255-6175, Fax: +1-607-254-4271, E-mail: bhowarth@environmentaldefense.org; and Elizabeth W. Boyer, SUNY-ESF, 1 Forestry Drive, Syracuse, NY 13210 USA, Tel: +1-315-470-4818, Fax: +1-315-470-6956, E-mail: ewboyer@syr.edu; and Alan R. Townsend, Department of EPO-Biology, Campus Box 450, University of Colorado, Boulder, CO 80309 USA, Tel: +1-303-492-6865, Fax: +1-303-492-6388, E-mail: alan.townsend@colorado.edu; and Douglas A. Burns, Watersheds Research Section, U.S. Geological Survey, 425 Jordan Road, Troy, New York 12180-8349 USA, Tel: +1-518-285-5662, Fax: +1-518-285-5601, E-mail: daburns@usgs.gov

H20 Arsenic and Other Toxic Metals in Natural Waters (Joint with GS)
Dissolved trace metals and metalloids in natural waters, particularly those that are known to be toxic and hazardous to human health, are of great concern to regulatory and statutory agencies. For example, the U.S. Environmental Protection Agency has recently proposed lowering the arsenic MCL from 50 ppb to 5 ppb. Many studies link elevated levels of arsenic and other toxic metals to natural processes and/or to anthropogenic activities, though exact sources, transport pathways, and fate often remain insufficiently understood. This is due in part to limitations in our understanding of the geochemical conditions that mobilize contaminant metals, and analytical criteria for delineating natural and anthropogenic origins. This session solicits contributions on all aspects of arsenic and other toxic metal hydrogeochemistry in natural waters.  In particular we encourage contributions that 1) explore modeling and correlations between metals for source identification, transport and fate, and 2) build on the existing geochemical database relevant to contaminant mobilization.
Conveners: Rudolph Hon, Department of Geology and Geophysics, Boston College, Devlin Hall 315, Chestnut Hill, MA 02467 USA, Tel: +1-617-552-3656, Fax: +1-617-552-2462, E-mail: hon@bc.edu; and Carol Stein and Dave McTigue, Gannett Fleming, Inc., Braintree, MA 02184 USA, Tel: +1-603-878-4056, E-mail: mctigue@top.monad.net; and Robert Ford, U.S. Environmental Protection Agency, National Risk Management Research Laboratory, P.O. Box 1198, Ada, OK 74820 USA, Tel: +1-580-436-8872, Fax: +1-580-436-8703, E-mail: Ford.Robert@epamail.epa.gov

H21 Water Quality of Natural Systems (POSTER ONLY)
The quality of natural waters is determined by the complex interactions of biogeochemistry and hydrology.   Poster presentations are invited on all aspects of water quality, ranging from field and laboratory studies to modeling approaches and theoretical work.  Possible topics include behavior of contaminants and naturally occurring solutes, interaction of hydrology and water quality, geochemical reactions and processes, and novel techniques of analysis or investigation.  These studies could be conducted at any spatial or temporal scale, and address issues related to groundwater or surface water.
Conveners: Annett B. Sullivan, Environmental Sciences Division, Oak Ridge National Laboratory, P.O. Box 2008, MS-6036, Oak Ridge, TN 37831 USA, Tel: +1-865-574-6367, Fax: +1-865-576-8543, E-mail: 4as@ornl.gov; and James Bowen, Department of Civil Engineering, University of North Carolina, Charlotte, NC 28223 USA, Tel: +1-704-687-3130, Fax: +1-704-687-6953, E-mail: jdbowen@uncc.edu

H22 Assessing Water Quality in Regional Drainage Basins and Aquifer Systems (Joint with B)
Reliable assessments of water quality in regional drainage basins and aquifer systems are important to water management.  Regional water quality assessments present several challenges, such as separating anthropogenic influences on water quality from the natural variability present in large-scale systems, designing economically feasible sampling strategies to characterize the spatial and temporal variability in water quality, and synthesizing results for use in land and water management to improve water quality. In addition, assessments are often complicated because many water contamination issues span multiple scales of jurisdiction, such as municipalities, counties, States or Provinces.  This session will bring together researchers who have designed regional assessments of water quality or analyzed large databases of chemical, hydrologic, or biological data.  Investigators who have  synthesized regional water-quality data for management purposes are particularly encouraged to participate.
Conveners: Kevin F. Dennehy, U.S. Geological Survey, DFC, Bldg. 53, MS 415, Denver, Colorado 80225 USA; Tel: +1-303-236-4882; Fax: +1-303-236-4912; E-mail: kdennehy@usgs.gov; and Jeffrey D. Stoner, U.S. Geological Survey, DFC, Bldg. 53, MS 415, Denver, Colorado 80225 USA; Tel: +1-303-236-2101, Fax: +1-303-236-4912, E-mail: stoner@usgs.gov; and William D. Gummer, Environment Canada, Suite 200, 4999-98 Ave., Edmonton, Alberta T6B 2X3 Canada, Tel: +1-780-951-8912, E-mail: Bill.Gummer@ec.gc.ca

H23 Science and Water Resource Issues: Challenges and Opportunities
Over the past decade there has been an increasing awareness within the hydrologic sciences community of the need to ensure that its scientific advances are used in the service of society.  This need has been reinforced by the policy community and politicians who increasingly expect greater socio-economic benefits from their investment in science.  Nowhere are the needs and expectations greater for science than they are in the field of water.  Water is a growing issue, nationally and internationally, and, unless a crisis is averted, it will become a major environmental issue for the 21st century.  Over the past five years, the hydrological and meteorological sciences have made great advances in land surface hydrology, and in providing knowledge, techniques and prediction capabilities that are particularly useful in water resource applications.  This session is intended to be a step in improving the dialogue between the water sciences community and the water resource community to determine how water research can more effectively meet the needs of water managers and policy makers.  Papers are invited that deal with the use of scientific information in making decisions to aid in managing water resources or developing policies related to water management.  Papers that demonstrate the successful application of hydrologic sciences to issues of water management in sectors such as navigation, fisheries, agriculture, transportation, energy, recreation, forestry and ecology are invited.  In addition, papers that deal with extremes in water availability (e.g., floods and droughts) are also welcome. Papers that review the areas of water science that need to be strengthened to better address the needs of the public are also invited.
Conveners: Rick Lawford, NOAA Office of Global Programs, 1100 Wayne Ave., Suite 1225, Silver Spring, MD 20910 USA, Tel.: +1-301-427-2089, ext. 40, Fax: +1-301-427-2222, E-mail: lawford@ogp.noaa.gov; and Holly Hartmann, Department of Hydrology and Water Resources, University of Arizona, Tucson, AZ 85721 USA, Tel.: +1-520-621-5082, Fax: +1-520-626-2488, E-mail: hollyh@hwr.arizona.edu

H24 Observations and Modeling of Precipitation (POSTER ONLY)
This special session will cover a broad range of topics related to precipitation measurement and modeling.  The session will consist entirely of poster presentations.  Papers are solicited on the estimation, validation, and error/uncertainty assessment of precipitation measured by ground-based remote sensors such as radar (e.g., NEXRAD WSR-88D), and airborne and satellite sensors (e.g., VIS, IR, SSM/I, TRMM).  Analyses of ground-based sensors relevant for validation (e.g., raingauge, drop spectra devices, microwave links) are welcome as well.  Research on statistical approaches, scaling theories, and mesoscale numerical modeling of precipitation processes are encouraged.  The session will also highlight operational applications involving precipitation estimation.  Presentations related to research programs such as the GEWEX Continental Scale International Project (GCIP), the TOGA Coupled Ocean-Atmosphere Experiment (COARE), the Tropical Rainfall Measuring Mission (TRMM) and related recent field experiments, the Pan American Climate Studies (PACS), and the Mesoscale Alpine Program (MAP) are particularly encouraged.
Convener: Allen Bradley, University of Iowa, Iowa Institute of Hydraulic Research, Iowa City, IA 52242 USA, Tel: +1-319-335-6117, Fax: +1-319-335-5238, E-mail: allen-bradley@uiowa.edu

H25 Reliability and Uncertainty Analyses in Environmental Modeling
In the environmental decision-making process relying on mathematical modeling predictions, it is essential to account for modeling uncertainties. More often than not, these uncertainties - which are a combination of our incomplete understanding of the modeled systems, inadequate measurements of model parameters and input variables - lead us to a point where standard model calibration and validation need to be revisited. In the context of selecting a specific course of actions among alternatives, these uncertainties represent a major hurdle to the operational use of environmental models.  The need to evaluate the uncertainties associated with environmental modeling has been recognized for a while and, thus, several reliability and uncertainty analysis approaches have been developed to assess model predictions. Abstracts are solicited on recent reliability and uncertainty analysis studies applied to environmental modeling.  Special attention will be paid to those studies that focus on: (i) the performance of various reliability and uncertainty analysis approaches, (ii) the development of innovative reliability and uncertainty analysis approaches, and (iii) the implementation of reliability and uncertainty analysis into the environmental decision-making process.  The expected outcome of this session is to bring up to date recent developments in the field of reliability-based assessment of model predictions to improve the environmental decision-making process.
Conveners: Alain Mailhot, Universite du Quebec, INRS-Eau, 2800 rue Einstein, Suite 105, C. P. 7500, Ste-Foy, Quebec, Canada, G1V 4C7, Tel.: +1-418-654-3821, Fax: +1-418-654-2600, E-mail: Alain_Mailhot@inrs-eau.uquebec.ca ; and Alain N. Rousseau, Universite du Quebec, INRS-Eau, 2800 rue Einstein, Suite 105, C. P. 7500, Ste. Foy, Quebec, Canada, G1V 4C7, Tel.: +1-418-654-2621, Fax: +1-418-654-2600, E-mail: Alain_Rousseau@inrs-eau.uquebec.ca

H26 Lumped Versus Distributed Modeling: Issues in Real World Applications (Joint with NG)
Distributed hydrologic models have been in existence for many years.  In spite of this and the abundance of spatial data sets to support distributed modeling, research is only now emerging that compares distributed modeling results to those from simpler lumped models.  Distributed models are clearly beneficial for land use change analysis and the prediction of basin interior processes.  However, the hypothesis that high resolution data sets and distributed approaches will produce more accurate basin outlet simulations than simpler lumped models requires further evaluation.  It is also unclear which basin attributes are responsible for gains realized by distributed modeling: basin shape, channel network definition, variability of precipitation and soils, rainfall-runoff mechanism (Hortonian vs. Saturation Excess) and others may individually or in combination play a role. It is hoped that this session will also be used to present intermediate results from the NWS Distributed Model Intercomparison Project (DMIP).  This project is formulated as the first broad comparison of distributed and lumped modeling approaches.  The results of DMIP will be used to guide NWS research on distributed models for operational river and flash flood forecasting. Papers comparing distributed and lumped approaches are encouraged.  Also welcome are papers identifying basin characteristics or runoff mechanisms that facilitate gains by distributed models.
Conveners: Michael Smith, National Weather Service W/OHD, 1325 East West Highway, Silver Spring, MD 20910-3283 USA, Tel.: +1-301-713-0640 x128, Fax: +1-301-713-0963; E-mail: Michael.Smith@noaa.gov; and Doug Boyle, Division of Hydrologic Sciences, Desert Research Institute, 2215 Raggio Parkway, Reno, NV 89512 USA, Tel.: +1-775-673-7441, Fax: +1-775-673-7363; E-mail: dboyle@dri.edu

H27 Watershed-Atmosphere-Ecosystem Coupling: Prospects, Approaches and Experience (Joint with B)
The dynamics of watershed soil moisture patterns, hydrologic flowpaths and land cover are understood to have an important influence on the exchange of water, carbon and nutrients between the land surface and atmosphere and on the coupling of terrestrial and aquatic ecosystems. These processes are pertinent to a set of significant environmental problems including the occurrence of large floods, drought, non-point source pollution, soil erosion and the stability of ecosystem structure and function.  Each of these occur within the context of human and institutional feedbacks with the natural system, and are seen to require an integrative, multi-disciplinary approach, both to foster scientific understanding of system behavior and to develop a decision-making framework for resource and environmental management.  Difficulties in developing such an approach include significant differences in dominant space and time scales of the components, potential gaps in the understanding of basic processes, and substantial uncertainty in environmental data sets required for analytical and modeling purposes.  Despite these limitations, a number of recent projects have developed a diverse set of methods for integrating data sets and analytical tools to capture the important feedbacks between hydrologic, atmospheric and ecosystem processes, typically geared towards a specific environmental problem. We invite papers that address the interactions of watershed soil moisture patterns and flowpath dynamics with land-atmosphere exchange and the watershed cycling and export of water, carbon and nutrients.  Presentations can include analytical and modeling frameworks, consideration of uncertainty due to gaps in process understanding and required data quality, and the prospects and barriers to developing and operationalizing these frameworks as tools for watershed management.
Conveners: Lawrence Band, University of North Carolina, Chapel Hill, NC, Tel.: +1-919-962-3921; E-mail: lband@email.unc.edu; and Alice Gilliland, NOAA-EPA, Research Triangle Park, NC, Tel.: +1-919-541-0347, Email: gilliland.alice@epa.gov

H28 Watershed Processes and Receiving Water Quality
Urbanization pressures are changing land use patterns in watersheds of surface reservoirs supplying drinking water to many communities. What are the hydrologic and water quality effects of the land use changes? How do land use changes effect trihalomethane formation potential? Pathogen transport to the reservoir? What hydrologic pathways are changed, and to what extent? Can the changes in hydrology be used as a rational design basis for best management practices on the watershed? This session will focus on linkages between terrestrial processes and water quality, with particular emphasis on issues of drinking water quality. Work that investigates the hydrology of urbanizing systems is strongly encouraged. Submissions could include both field-based and model studies. Policy studies relating land uses and water quality should be of particular interest in this session. The session should appeal to hydrologists, water resources engineers, landscape architects and policy makers with an interest in the hydrology of anthropogenically disturbed systems.
Convener: James M. Hassett, Faculty of Environmental Resources and Forest Engineering, 312 Bray Hall, State University of New York College of Environmental Science and Forestry, Syracuse, NY 13210, USA, Tel: +1-315-470-6637, Fax: +1-315-470-6958, E-mail: jhassett@esf.edu

H29 Smart Growth: Impacts on Urban Hydrology and the Protection of Natural Resources (Joint with B)
The spirit of the Smart Growth philosophy is to steer future development with an eye towards optimizing existing resources and halting urban sprawl.  Optimization strategies may vary from preserving open space, to minimizing commute distances, to maximizing the use of existing infrastructure.  Since the specific quantity being optimized may vary, there are many possible outcomes to the application of smart growth concepts in a particular region. Many questions arise: How does smart growth intersect with hydrology?  In planning future development, what hydrologic objectives should be optimized?  From the standpoint of the health of stream and watershed ecosystems, what development patterns are optimal?  How do we measure hydrologic impacts in a way that can be used to genuinely assess the relative merits of several differing future growth patterns or scenarios?  How do we assert that smart growth is, in fact, smart?
 This session welcomes papers offering a broad range of perspectives reflecting the complex and multi-disciplinary nature of this issue.  Policy pieces, theoretical research, papers highlighting new methods or approaches, and case studies are all welcome.
Convener: Glenn Moglen, Department of Civil and Environmental Engineering, Room 1161 - Martin Hall, University of Maryland, College Park, MD 20742 USA, Tel.: +1-301-405-1964, Fax: +1-301-405-2585, E-mail: moglen@eng.umd.edu

H30 Remote Sensing, Land Surface Hydrology and Field Experiments
Recent advances in ground, aircraft and satellite remote sensing techniques have provided hydrologists with new and unique views of land surface hydrological processes.  This session seeks to present recent results of experiments in land surface hydrology that incorporate remote sensing.  Satellite data can be utilized by land surface hydrological models as input and/or validation and/or assimilation.  The hydrological processes include (but are not limited to) soil moisture, surface temperature, evapotranspiration, runoff, and stream flow.  Papers dealing with retrieval algorithms for aircraft and satellites, field experimentation, and small to global scale hydrologic modeling are solicited. Papers can examine comparison of aircraft and satellite retrieved variables with (a) measurements at the ground surface; or (b) output from land models; or (c) measurements from other satellite/aircraft sensors of the same variables.
Conveners: Venkat Lakshmi, Department of Geological Sciences, University of South Carolina, Columbia SC 29208 USA, Tel.: +1-803-777-3552, Fax: +1-803-777-6610, E-mail: vlakshmi@geol.sc.edu; and Thomas J. Jackson, USDA ARS Hydrology Lab, 104 Bldg 007 BARC-West, Beltsville, MD 20705 USA, Tel.: +1-301-504-8511, Fax: +1-301-504-8931, E-mail: tjackson@hydrolab.arsusda.gov

H31 Advances in Land Data Assimilation Systems
Assimilation of remotely sensed land surface observations into regional to global scale numerical models have the potential to significantly advance our ability to assess, understand, and predict surface water, energy, and carbon cycles.  This session seeks to assess the state-of-the-art in data assimilation methods for integrating land surface remote sensing and modeling, with a focus on practical applications and techniques.  Assimilated land surface variables of interest include (but are not limited to) soil moisture, surface temperature, snowpack, streamflow, vegetation dynamics, and carbon storage. Contributions describing the development of practical land surface data assimilation methods, multivariate land surface data assimilation strategies, evaluation of the required accuracy and resolution of remote sensing observations, the effects of scale, process complexity, and uncertainty on data assimilation, and the optimal treatment of model and observation errors are encouraged.
Conveners: Paul Houser, Hydrological Sciences Branch, NASA-GSFC Code 974,Greenbelt, MD 20771 USA, Tel.: +1-301-614-5772, Fax: +1-301-614-5808, E-mail: Paul.Houser@gsfc.nasa.gov; and Jeff Walker, Hydrological Sciences Branch, NASA-GSFC Code 974,Greenbelt, MD 20771 USA, Tel: +1-301-614-5804, Fax: +1-301-614-5808, E-mail: cejpw@land.gsfc.nasa.gov

H32 Is the Global Water Cycle Intensifying?
The cycling of water in its three physical states is at the heart of Global Change processes, strongly controls energy budgets and fluxes, and drives the ocean thermohaline circulation as well as land surface hydrology.  Furthermore, the most significant manifestations of climate change for humans and the environment are changes in the global water cycle, the distribution of precipitation, the intensity and paths of weather systems, flooding events, and droughts. The session seeks contributions that shed light on the existence of long-term trends in the components of the global water cycle, the extent to which large-scale changes in mean climate can be linked to significant changes in the distribution and intensity of weather systems and precipitation, and observed or predicted impacts on the recharge of water reservoirs.
Conveners: Pierre Morel, Goddard Earth Science and Technology Institute (GEST), University of Maryland, Baltimore County, 1000 Hilltop Circle, Baltimore, MD 21250 USA, Tel: +1-410-455-8808, Fax: +1-410+455-8899, E-mail: morel@umbc.edu; and Mike Jasinski, NASA Headquarters, Washington, DC, 20546-0001 USA, Tel: +1-202-358-1847, E-mail: mjasinsk@mail.hq.nasa.gov

Hydrology presents jointly with the following Special Sessions:
A01 Earth Science Applications of Reflected and Refracted GPS Transmissions (Joint with G, GP, H, SA)
A03 Transient Tracers in Geophysical Flows (Joint with B, H, OS)
A07 Calibration of Meteorological Satellite Sensors and Validation of Derived Products (Joint with B, H, OS)
B03 Biogeochemistry of Land Use Change  (Joint with GS, H, PA)
B04 Land Cover and Land Use Change: Implications for Resource Management (Joint with H, PA)
B05 Remote Sensing to Address the Needs of Local Communities  (Joint with G, H, PA)
B07 Isotopes in Biogeochemistry and Global Change (Joint with A, GS, H, OS)
B09 Mercury in the Environment (Joint with A, GS, H, PA)
B10 Sedimentation in Coastal Marshes (Joint with H, OS)
B11 Linkages Between Biogeochemical and Hydrogeologic Processes in Shallow Ground-Water Systems of the Atlantic and Gulf Coastal Plains (Joint with H, PA)
B12 Eco-hydrological Dynamics of Water Controlled Ecosystems (Joint with H, NG)
B14 Land-Atmosphere Interactions (Joint with A, H, NG)
GP01 Mapping Aquifers, Oceans, and Planetary Bodies with Passive and Active EM Methods (Joint with H, OS, P)
OS01 Non-Equilibrium Phenomena in Geophysics (Joint with A, B, H, P, S, T)
OS04 Ice Cores: Paleoclimates, Glaciology, and Environmental Change (Joint with A, H)
T02 Dynamics of Gas Hydrate Reservoirs and Similar Shallow Marine Flow Systems (Joint with B, GS, H, OS)
V01 Continental Weathering and Ocean Chemistry (Joint with H, OS, GS)
NG02 Integrating and Applying Models, Simulations, and Data to the Forecasting of Nonlinear Geophysical Systems (Joint with H, T)
 

Mineralogical Society of America

M01 Equation of State and Elasticity of Earth Materials (Joint with MR, SEDI, T, V)
The physical state of Earth's interior is controlled by the properties of the constituent materials and their chemical interactions. Understanding the physical properties of these constituent materials at the pressure and temperature conditions of the Earth's interior has long been the greatest effort in the mineral physics community. Over the past decade, technical advances in various experimental methods, including X-ray diffraction, vibrational spectroscopy, opto-acoustic techniques, shock wave experiments, and inelastic scattering at different pressure and temperature regimes, as well as the new synchrotron facilities, have brought a revolution in the equation of state and elasticity studies. An alternative to direct measurement is made by computational techniques based on empirical information or the quantum theory of matter, providing valuable insights and complimentary results to experimental data.  This session will focus on the recent results of the physical properties of the Earth materials from both laboratory and theoretical calculations, aiming for a better understanding of the state of the Earth's interior.
Conveners: Jennifer Kung, State University of New York, Department of Geosciences, Stony Brook, NY 11794 USA, E-mail: jkung@notes.cc.sunysb.edu; and Jianzhong Zhang, State University of New York, Mineral Physics Institute, Stony Brook, NY 11794 USA, E-mail: zhang@sbmp04.ess.sunysb.edu

M02 Characterizing Organic and Inorganic Hydrothermal Systems (Joint with V, GS)
The development and application of new experimental procedures, supplemented by rigorous theoretical modeling, have recently provided new insights into several key organic and inorganic hydrothermal systems.  Direct observations of experiments at extreme conditions reveal valuable and unique information for these systems including metastable and non-quenchable phases. While spectroscopic methods enable monitoring phase-equilibria, kinetics and reaction pathways, in-situ X-ray analysis of these products make the characterization of the structure as well as interpretation of the nature of inter-molecular interactions possible.  Increasing numbers of such experimental results are scattered amongst different disciplines such as molecular physics, physical chemistry, organic geochemistry and high-pressure crystallography. The goal of this session is to bring together diverse techniques and results to help better understand observed phenomena. Studies addressing a wide variety of questions in organic and inorganic hydrothermal systems including structure, phase-equilibria, mineral-fluid interactions and reaction kinetic in chemical and biochemical systems are invited to contribute to this special session. In addition to invited presentations, contributed papers are solicited discussing organic reactions, supercritical fluid behavior, catalytic reaction networks at high pressure and temperature, in-situ molecular spectroscopy and crystallography.
Conveners: Anurag Sharma, Carnegie Institution of Washington, Geophysical Laboratory, 5251 Broad Branch Rd., NW, Washington, DC 20015 USA, Tel: +1-202-478-8957, Fax: +1-202-478-8901, E-mail: sharma@gl.ciw.edu; and Przemyslaw Dera, Carnegie Institution of Washington, Geophysical Laboratory 5251 Broad Branch Rd., NW, Washington, DC 20015 USA, Tel: +1-202-478-8989, Fax: +1-202-478-8901, E-mail: pdera@gl.ciw.edu

M03 Spectroscopy of Minerals and Other Planetary Phases (Joint with MR, T)
The addition of spectroscopy to the toolbox of available techniques for studying Earth and planetary materials has given us the ability to constrain physical properties and to do a variety of tasks in new ways.  For example, vibrational spectra collected over a wide pressure and/or temperature range yield important information about thermodynamic properties, phase transitions and/or kinetics that cannot be obtained by other techniques as easily or as accurately.  Constraints on the crystal chemistry and phase identification of mineral and other phases can now be obtained using different microspectroscopy techniques, many of which were developed over the last twenty years.  It has been approximately a decade since we last gathered workers in this field together to share their latest developments in this area.  We would like to invite contributions in all areas of spectroscopy on Earth and planetary materials, particularly emphasizing new developments and uses over the last decade.
Conveners: Anastasia Chopelas, University of Nevada, Department of Physics, 4505 S. Maryland Parkway, Box 454002, Las Vegas, NV 89154-4002 USA, Tel: +1-702-895-1703, Fax: +1-702-895-0804, E-mail: chope-las@physics.unlv.edu; and Monika Koch-Mueller, Carnegie Institution of Washington, Geophysical Laboratory and CHiPR, 5251 Broad Branch Rd., NW, Washington, DC 20015-1305 USA, Tel: +1-202-478-8931, Fax: +1-202-478-8901, E-mail: monika.koch-muller@gl.ciw.edu

Mineralogical Society of America presents jointly the following Special Sessions:
GP03 Paleomagnetic Puzzles, Rock Magnetic Riddles (Joint with MRP, M)
GP06 Banded Iron Formation, its Chemical and Physical Properties and Relation to the Origin of Life (Joint with B, MR, P, V, GS, M)
GS01 Magmatic Volatile Histories: Stable Isotopic Tracing of Sources and Degassing Processes in Magmatic Systems and Implications for Volcanology and Earth System Science (Joint with T, M)
S03 Integrated Models of Earth Structure and Evolution (ONLINE-only Session) (Joint with MR, SEDI, T, M)
T03 Computational Earth Laboratories (Joint with GP, M, MR, NG, S)
 

Ocean Sciences

OS01 Non-Equilibrium Phenomena in Geophysics (Joint with A, B, H, P, S, T)
This session will be designed to attract different disciplines together to discuss recent research on non-equilibrium thermodynamics and a variety of dissipative phenomena in the geophysical fields. These include dissipative properties of the atmosphere and ocean, mantle convection, production of available potential energy and its relation to the second law of thermodynamics, and extreme properties in the complex geophysical and extra-planetary fluids. Dissipative structures and related fractal scaling often appeared in the non-equilibrium systems are also of the main subject of the session. We hope to address these issues by attracting papers on the global and local structures of the geophysical fluids, transport properties and scaling of turbulence, and energetics of the non-equilibrium systems.
Conveners: Kerry A. Emanuel, MIT, Center for Meteorology and Physical Oceanography, Cambridge, MA 02139 USA, Tel: +1-617-253-2462, Fax: +1-617-253-6208, E-mail: emanuel@texmex.mit.edu; and G. W. Paltridge, University of Tasmania, Antarctic Cooperative Research Centre, Hobart, TAS 7001 Australia, Tel: +61 3 62262971, Fax: +61 3 62262973, E-mail: g.paltridge@utas.edu.au

OS02 High-Resolution Climate Records From Laminated Sediments (Joint with V, GS)
Reduced sediment bioturbation due to low oxygen has resulted in the preservation of particularly detailed records of past environmental change linked to climate.  With this special session, the conveners hope to provide a representative update of the many ongoing efforts to recover and interpret such records, both marine and lacustrine, throughout the world.  Submissions describing novel techniques that either reduce the effort required to obtain high-resolution information from laminated sediment or improve the dating of such records are also encouraged.
Conveners: Alexander van Geen, Columbia University, Lamont-Doherty Earth Observatory, Route 9 W, Palisades, NY 10964 USA, Tel: +1-845-365-8644, Fax: +1-845-365-8154, E-mail: avangeen@ldeo.columbia.edu; and Larry C. Peterson, University of Miami, Rosenstiel School of Marine & Atmospheric Science, 4600 Rickenbacker Causeway, Miami, FL 33149 USA, Tel: +1-305-361-4692, Fax: +1-305-361-4632, E-mail: peterson@rsmas.miami.edu

OS03 Middle to Late Miocene Perturbations of the Earth's Ocean and Climate Systems: An Integrated Approach
The Middle and late Miocene is a time of transitions in global climate, including a Mid-Miocene Climate Optimum followed by expansion of the East Antarctic and West Antarctic, and small northern-hemisphere ice sheets, sea-level fluctuations, and cooling of deep and intermediate water masses.  The ocean carbonate system illustrated so-called "crash" intervals when the carbonate sediments were poorly preserved, as well as intervals referred to as "biogenic blooms or bursts”.  Moreover, the modern pattern of deepwater formation became firmly established.  This session will bring together a broad range of earth scientists focusing on (1) the expansion and establishment of ice sheets in Antarctica and in the northern hemisphere, (2) the high resolution benthic and planktic oxygen and carbon isotope records, (3) the sequence stratigraphy framework along carbonate and siliciclastic margins, (4) the carbonate “crash” or “crashes”, (5) the biogenic “blooms and bursts”, (6) the global surface, deep and intermediate ocean circulation, and (7) the continental climate changes associated with some major vegetation modifications.  Through integrated discussion we seek to better understand the timing, amplitudes, causes, and effects of the observed Earth ocean and climate perturbations during the middle and late Miocene.
Conveners: Andre W. Droxler, Rice University, Department of Geology and Geophysics MS 126, PO Box 1892, Houston, TX 77251-1892 USA, Tel: +1-713-348-4885, Fax: +1-713-348-5214, E-mail: andre@rice.edu; and Liselotte Diester-Haass, Universitat des Saarlandes, Zentrum fur Umweltforschung, Saarbrucken, 66041 Germany, Fax: ++6841-171774, E-mail: A.L.Haass@t-online.de; and James Wright, Rutgers University, Department of Geology Wright Chemistry Building, Piscataway, NJ 08854 USA, Tel: +1-732-445-5722, Fax: +1-732-445-3374, E-mail: JDWRIGHT@RCI.RUTGERS.EDU; and John Anderson, Rice University, Department of Geology and Geophysics MS 126, PO Box 1892, Houston, TX 77251-1892 USA, Tel: +1-713-348-4884, Fax: +1-713-348-5214, E-mail: johna@rice.edu

OS04 Ice Cores: Paleoclimates, Glaciology, and Environmental Change (Joint with A, H)
This session builds on previous annual sessions at Spring AGU, which have emphasized ice core projects in Greenland, Antarctica, and low-latitude ice caps.  This years' session will highlight U.S. ITASE spacial survey of West Antactica, from the Siple Dome deep core, and from the Program for Arctic Regional Climate Assessment based on ice cores in Greenland. We also strongly encourage submissions from other ice-core and ice-core related projects.
Conveners: Christopher A. Shuman, University of Maryland, Earth System Science Interdisciplinary Center, Oceans and Ice Branch 2104 Computer and Space Sciences Building, Room A215, Building 33, College Park, MD 20742-2465 USA, Tel: +1-301-405-8291, Fax: +1-301-405-8468; and Eric Steig, University of Pennsylvania, USA, E-mail: steig@geophys.washington.edu; and James White, University of Colorado, USA, E-mail: james.white@colorado.edu; and Paul Mayewski, University of New Hampshire, USA, E-mail: paul.mayewski@maine.edu

OS05 Storm Effects, Sedimentation and Depositional Processes on the Coast and Continental Shelf
Our understanding of past storminess as a calibration for future change is incomplete.  Knowledge of the impact of such storminess on the coastal zone is even more indistinct.  This session will concentrate on new efforts to identify changes taking place in the magnitude, frequency and impact of storms along the Atlantic seaboard of the European Union, Gulf and Atlantic coasts of the U.S. and Canada.  Papers presented will examine changes over the last 2,000 years to present in addition to the hydrodynamic and sedimentary processes associated with high-energy events.  Such a timescale necessitates a strongly interdisciplinary approach, combining techniques from geology, geomorphology, biogeography, history and meteorology as well as employing a range of statistical and computational techniques.  A goal of this research is to determine trends and develop models of storm behavior, and to outline a framework for the management of environmentally sensitive coastal areas in the light of changing storminess incidence, magnitude and impact.
Conveners: Gregory W. Stone, Louisiana State University, Coastal Studies Institute, USA, Tel: +1-225-388-6188, Fax: +1-225-388-2520, E-mail: gagreg@lsu.edu; and Julian Orford, Queens University, Northern Ireland

Ocean Sciences presents jointly the following Special Sessions:
A03 Transient Tracers in Geophysical Flows (Joint with B, H, OS)
A07 Calibration of Meteorological Satellite Sensors and Validation of Derived Products (Joint with B, H, OS)
A08 Research in Meteorology and Oceanography Utilizing DoD HPC Resources (Joint with OS)
B02 Integrated Observations for the Biogeosciences (Joint with A, NG, OS)
B07 Isotopes in Biogeochemistry and Global Change (Joint with A, GS, H, OS)
B10 Sedimentation in Coastal Marshes (Joint with H, OS)
GP01 Mapping Aquifers, Oceans, and Planetary Bodies with Passive and Active EM Methods (Joint with H, OS, P)
GP08 Precise Correlation of Strata: Magnetic and Other Methods (Joint with OS, V)
H09 Groundwater Flux at the Land-Ocean Margin: Physics, Chemistry, and Ecological Implications (Joint with B, GS, OS)
T02 Dynamics of Gas Hydrate Reservoirs and Similar Shallow Marine Flow Systems (Joint with B, GS, H, OS)
V01 Continental Weathering and Ocean Chemistry (Joint with H, OS, GS)
 

Planetary Sciences

P01 Galileo and Cassini at Jupiter: An Historic Two-Spacecraft Experiment
The Galileo and Cassini/Huygens missions will be carrying out an historic two-spacecraft experiment at Jupiter. A relatively high level of intensity will be reached at the end of this year when Cassini/Huygens has its closest approach to Jupiter on December 30th.  While the data from Cassini/Huygens are returned almost immediately, the receipt of the synergistic Galileo data on the Earth will take many weeks because of the slow Galileo communication rate.  Accordingly, looking forward by about six months, we are looking for the presentation of results from this unique experiment.
Conveners: Torrence Johnson, Jet Propulsion Laboratory, 264-570H 4800 Oak Grove Drive, Pasadena, CA 91109 USA, Tel: +1-818-393-7957, Fax: +1-818-354-0966, E-mail: Torrence.V. Johnson@jpl.nasa.gov; and Dennis Matson, JPL, 230-205 4800 Oak Grove Drive, Pasadena, CA 91109 USA, Tel: +1-818-354-2253, Fax: +1-818-393-4495, E-mail: dmatson@jpl.nasa.gov; and Jean-Pierre Lebreton, ESA/ESTEC, Space Science Department Mail Code SCI-SO, Postbus 299, Noordwijk, 2200 AG The Netherlands, Tel: +31 71 565-3600, Fax: +31 71 565-4697, E-mail: jlebreto@estec.esa.nl

P02 New Views of the Moon (ORAL) (Joint with V, GS)
Recent spacecraft missions are refining our view of Earth's nearest neighbor.  The Lunar Prospector and Clementine spacecraft returned data that have revealed fundamental new insights into the record of the early history of the solar system, and are stimulating new Earth-based measurements and lab studies.
Conveners: Brad Joliff, Washington University, St. Louis, MO USA, E-mail: blj@levee.wust1.edu; and Carlie Pieters, Brown University, Providence, RI 02912 USA, Tel: +1-401-863-2416, E-mail: Carlie_Pieters@brown.edu

P03 Mars: New Perspectives on Processes and Evolution
Data from the Mars Global Surveyor Mission has completely changed our perspectives on the nature of atmospheric, surface, and interior processes and how they have interacted to produce the geological record.  In this session, papers are solicited that treat new perspectives on these processes and the evolution of Mars. Implications for future exploration will also be emphasized.
Conveners: James W. Head, Brown University, Department of Geological Sciences, Box 1846, Providence, RI 02912 USA, Tel: +1-401-836-2526, Fax: +1-401-836-3978, E-mail: James_Head_III@Brown.Edu; and James Zimbelman, National Air and Space Museum, Center of Earth and Planetary Studies, Smithsonian Institution, Washington, DC 20560 USA, Tel: +1-202-786-2981, E-mail: jrz@nasml.si.edu

Planetary Sciences presents jointly with the following Special Sessions:
GP01 Mapping Aquifers, Oceans, and Planetary Bodies with Passive and Active EM Methods (Joint with H, OS, P)
GP05 Earth and Planetary Magnetic Survey Satellites (Joint with P)
GP06 Banded Iron Formation, its Chemical and Physical Properties and Relation to the Origin of Life (Joint with B, MR, P, V, GS, M)
OS01 Non-Equilibrium Phenomena in Geophysics (Joint with A, B, H, P, S, T)
SH08 X-Ray Emission in the Solar System (Joint with P, SA, SM)
T04 True Polar Wander on Earth, Mars and Beyond (Joint with G, GP, P)
V02 New Views of Mars Volcanism: Extrusive, Explosive, and Possible Influences of H2O (Joint with P)
 

Seismology

S01 Core Mantle Boundary Region (Joint with GP, GS, MR, NG, SEDI, T)
This session addresses the study of structure, dynamics, and composition of Earth's lower mantle at both fine and large scale, laterally and vertically.  We invite contributions from all disciplines, such as seismology, geodynamics, mineral physics, and geomagnetics, including both observational and theoretical approaches. Topics include: better characterization of the depth and geographic variations in features that scatter seismic energy in the deep mantle, and their interpretation; do ultra-low velocity zones (ULVZs) really exist?  If so, are they associated with extreme (-30%) variations in shear-wave velocity?  What are the thermo-chemical interpretations of these models? What is the style, magnitude and length scale of anisotropy in the deep  mantle? What are the mineral physics and dynamical flow implications of anisotropy at these depths? What is the large-scale structure of the lower mantle and lowermost boundary layer and how does it relate to (or not) the subducting lithosphere and rising plumes? Is the lower mantle chemically distinct from the upper mantle? Or alternatively, where are chemical heterogeneities located in the deep mantle, and what are their scale lengths? Are bulk modulus and shear modulus really anti-correlated at the base of the mantle?  What are the implications of this? Combination of geochemical and geophysical approaches will be the key to the success of this session, thus we encourage contribution from all the deep Earth disciplines. In this first ever "online-only" session, participants will be able to submit their graphics and figure captions to AGU via the World Wide Web (www). A message board will permit interaction with the authors, which everyone can view. This session will allow global participation on this timely topic, and will stay posted after the 2001 Spring Meeting.  Anyone with an AGU membership number will be allowed viewing access of the online session.
Conveners: Ken Creager, University of Washington, Geophysics Box 351650, Seattle, WA 98195-1650 USA, Tel: +1-206-685-2803, Fax: +1-206-543-0489, E-mail: kcc@geophys.washington.edu; and Ed Garnero, Arizona State University, Department of Geological Sciences, Box 871404, Tempe, AZ 85287-1404 USA, Tel: +1-480-965-7653, Fax: +1-480-965-8102, E-mail: garnero@asu.edu; and Shun-ichiro Karato, University of Minnesota, Department of Geology, 108 Pillsbury Hall, Minneapolis, MN 55455 USA, Tel: +1-612-624-7553, Fax: +1-612-625-3819, E-mail: karato@tc.umn.edu

S02 Challenges in Regional Seismic Nuclear Test-Ban Treaty Monitoring (Joint with PA)
A significant research effort over the past four decades has resulted in a large body of knowledge for teleseismic monitoring of nuclear testing treaties, such as the Limited Test Ban Treaty (LTBT) and Threshold Test Ban Treaty (TTBT). Because large explosions (>150 kilotons) were the subject of these treaties' teleseismic methods could be used effectively. However, under a Comprehensive Nuclear Test-Ban Treaty (CTBT) monitoring regime, in which all nuclear tests are prohibited, the monitoring challenge is enormously more difficult for a number of reasons. First, regional wave analysis must be invoked because seismic waves from very small tests do not propagate to teleseismic distances. Second, the geographic regions of monitoring interest are not limited to small well-defined test sites (as they were under the LTBT and TTBT), but rather very broad regions such as the Middle East and Asia. Third, there is virtually no experience in regional analysis from actual nuclear tests in these broad regions upon which to formulate an empirical basis for regional discriminants. And, unfortunately, almost all validated teleseismic-monitoring techniques fail when applied to regional data. Consequently, a new body of scientific knowledge regarding regional wave propagation needs to be developed to form the basis for the development of new regional monitoring techniques. This session will begin with a number of invited papers that will provide the background and an overview of the scientific problems inherent is regional monitoring, in addition to important monitoring problems. We invite papers that address specific scientific problems that must be overcome to make progress in regional monitoring and those that address particular regional monitoring problems, e.g., discrimination of large chemical explosions. We are particularly interested in papers that discuss new approaches to interpreting the myriad of phases observed on regional seismograms and innovative empirical methods. Finally, we encourage papers that deal with testing and validation of proposed discriminants for particular geographic regions.
Conveners: James F. Lewkowicz, Weston Geophysical Corporation, 325 West Main Street, Northboro, MA 01532-2117 USA, Tel: +1-508-393-4600, E-mail: JimL@weston-geo.com; and Delaine T. Reiter, Weston Geophysical Corporation, 325 West Main Street, Northboro, MA 01532-2117 USA, Tel: +1-508-393-4600, E-mail: Delaine@weston-geo.com

S03 Integrated Models of Earth Structure and Evolution (ONLINE-only Session) (Joint with MR, SEDI, T, M)
Global Earth modeling has reached a point at which future progress in our understanding of the structure, dynamics and evolution of the Earth requires a truly multidisciplinary approach. Many sub-disciplines within geophysics are becoming sufficiently mature that "reference" data sets and algorithms can be identified that serve to constrain our modeling. Such products would come in a "standardized format" and could conceivably be used by non-specialists. This session will be a first ever AGU "online"-only session, permitting a truly global forum whereby participants not physically attending Spring AGU can electronically contribute their research via the web. This session invites contributions on (1) Reference data sets and algorithms from seismology, geodynamics, geodesy, geomagnetism, etc.; (2) Potential "Reference" models in individual sub-disciplines (such as a successor to PREM, electric conductivity, etc); (3) Models which tie together several sub-disciplines of geophysics (e.g. mineral physics models that constrain seismic modeling); (4) Models which attempt to reconcile geophysical and geochemical data. We also encourage papers that give feedback from one sub-discipline to another (e.g. the effect of current uncertainties in seismic tomography on geodynamical modeling).
Conveners: Gabi Laske, University of California, Scripps Institute of Oceanography, San Diego, CA USA, E-mail: gavi@mahi.ucsd.edu; and Carolina Lithgow-Bertelloni, University of Michigan, 2534 C.C. Little Building 425 E. University Avenue, Ann Arbor, MI 48109-1063 USA, Tel: +1-734-647-9938, Fax: +1-734-763-4690, E-mail: crlb@umich.edu

S04 How Rifting Worked in Northeastern North America (Joint with T, V, GS)
This session addresses the massive basaltic volcanism, lithospheric thinning, and subsidence strongly interacted during the Mesozoic rifting of North America from Pangea. These processes left an imprint that spans a wide range of processes and spatial scales, from local faulting, to sedimentary basin subsidence, to regional patterns of fabric in the upper mantle. This session will combine recent contributions from geophysics, structural geology, geochemistry, and geochronolgy that improve our understanding of the formative processes of the Northeastern North American passive margin.
Conveners: Vadim Levin, Yale University, PO Box 208109, New Haven, CT 06520 USA, E-mail: vadim@geology.yale.edu; and Bill Menke, Columbia University, Lamont-Doherty Earth Observatory, Department of Earth and Environmental Sciences, Route 9W, Palisades, NY 10964 USA, E-mail: menke@ldeo.columbia.edu; and Paul Olsen, Columbia University, Lamont-Doherty Earth Observatory, Department of Earth and Environmental Sciences, Route 9W, Palisades, NY 10964 USA, E-mail: polsen@ldeo.columbia.edu

S05 Progress in Methods of Earthquake Source Estimation
Recent earthquakes such as the great 1998 Antarctic Plate, 1999 Izmit Turkey, 1999 Taiwan and 1999 Hector Mine, CA events have provided an unprecedented amount of new data with which to investigate the source processes of earthquakes. Understanding the source process is essential to unraveling the physics of earthquake nucleation and breakaway rupture, studying tectonics, as well as for the simulation of strong ground motions. Studies of recent events have revealed levels of complexity, such as rupture over multiple fault segments and spatial and temporal slip heterogeneity that haven't been widely observed, however such analyses involve many parameters and model uncertainty is not usually reported.  This session seeks theoretical and observational papers utilizing state-of-the-art earthquake source inverse methodologies to examine the earthquake source process over the entire range of observable phenomena, and to assess the uncertainty in the derived source models. Papers are sought on, but not limited to, the application of inversions for the full moment tensor, source kinematics and rupture dynamics, with emphasis on those which combine seismic and other non-seismic data sets, and which examine the uncertainty in the model parameter estimates.
Conveners: Douglas Dreger, University of California Berkeley, USA, E-mail: dreger@seismo.berkeley.edu; and Michael Antolik, Harvard University, USA, Tel: +1-617-495-9604, E-mail: antolik@seismology.harvard.edu

S06 The Structure and Early Evolution of Cratons (Joint with T, V, GS)
In the last decade, several large-scale, multidisciplinary projects have focused on the problem of understanding the continents. They have involved a variety of techniques including, seismic imaging, geological mapping, geochemistry, geochronology, heat flow, and geodynamical modeling. In this session we review results of these studies and their implications for our current understanding of the structure, composition, and geological evolution of continents. While we welcome contributions regarding all aspects of continental structure and evolution, we aim to focus on the Archean, which gives us glimpses of dynamics and evolution in the earliest era of continental history.
Conveners: Paul Silver, Carnegie Institution of Washington, Washington, DC 20015 USA, Tel: +1-202-686-4370 ext. 4386, Fax: +1-202-364-8726, E-mail: silver@dtm.ciw.edu; and Rob van der Hilst, MIT, Cambridge, MA 02139 USA, Tel: +1-617-253-6977, Fax: +1-617-258-9697, E-mail: hilst@mit.edu

Seismology also presents jointly with the following Special Sessions:
OS01 Non-Equilibrium Phenomena in Geophysics (Joint with A, B, H, P, S, T)
T01 Recent Tectonics, Kinematics and Dynamics of Southeast Asian Margins (Joint with G, S)
T03 Computational Earth Laboratories (Joint with GP, M, MR, NG, S)
 

SPA: Aeronomy

SA01 Short-term Variability in the Thermosphere and Ionosphere: Measurements and Modeling (Joint with SM)
This special session seeks to develop a coherent view of  minute-to-minute to day-to-day variability in the thermosphere and ionosphere. We welcome papers dealing with the sources: fluctuations in the forcing functions at high latitude, ups and downs in solar EUV, tidal variability due to planetary and gravity waves propagating from below, and low-latitude electrodynamics, as well as the ionospheric and thermospheric response they produce. Both experimental results and modeling techniques will be  emphasized in order to achieve a better understanding of short-term changes in the space environment. Understanding variability is not only an interesting science problem, but is also essential for  space weather applications.
Conveners: Mihail V. Codrescu, University of Colorado, CIRES SEC/NOAA, R/E/SE, 325 Broadway, Boulder, CO 80305 USA, Tel: +1-303-497-6763, Fax: +1-303-497-3645, E-mail: Mihail.Codrescu@noaa.gov; and Tim J. Fuller-Rowell, University of Colorado, CIRES/SEC/NOAA R/E/SE, 325 Broadway, Boulder, CO 80305 USA, Tel: +1-303-497-5764, Fax: +1-303-497-3645, E-mail: Tim.Fuller-Rowell@noaa.gov; and David N. Anderson, University of Colorado, CIRES/SEC/NOAA R/E/SE, 325 Broadway, Boulder, CO 80305 USA, Tel: +1-303-497-7754, Fax: +1-303-497-3645, E-mail: David.Anderson@noaa.gov

SA02 Space-Based Auroral Remote Sensing (Joint with SM)
Space-based auroral remote sensing can quantify key elements of the high latitude energy budget including incident energy flux and mean energy as well as their spatial and temporal evolution. Estimates of ionospheric conductivity and composition changes follow from these determinations. This session explores the degree to which current remote sensing techniques can determine high latitude energy inflow and use this information to infer ionospheric and thermospheric parameters. Papers which use space-based imaging or other remote sensing data of the Earth's auroral regions to investigate these topics are appropriate.
Conveners: Glynn Germany, University of Alabama in Huntsville, Center for Space Plasma and Aeronomic Research, S131 Technology Hall, Huntsville, AL 35899 USA, Tel: +1-256-824-5129, Fax: +1-256-890-6575, E-mail: germanyg@cspar.uah.edu; and Doug Strickland, Computational Physics, Inc., 8001 Braddock Road Suite 210, Springfield, VA 22151 USA, Tel: +1-703-764-7501, Fax: +1-703-764-7500, E-mail: dstrick@cpi.com

SA03 Polar Mesospheric Clouds, Noctilucent Clouds and Polar Mesospheric Summer Echoes (Joint with A)
Observations of the number of noctilucent clouds (NLCs) made from ground-based locations in northwest Europe have shown significant changes over the last 30 years. These clouds, also called Polar Mesospheric Clouds (PMCs) when observed from satellites, are believed to respond to even small changes in their environment and may be the most visually obvious manifestation of mesospheric climate change. Such changes could be linked to increases in the “greenhouse” gas CO2.  Despite their importance, little is known about the formation of PMCs or the causes of the apparent related phenomenon, Polar Mesosphere Summer Echoes (PMSEs). This session invites papers describing the theory and observations of NLCs, PMCs, PMSEs and related parameters such as mesospheric and lower thermospheric temperature, H2O, particle composition, NO, and correlated dynamics phenomena.  It is intended to be a forum for exchanges of ideas and a catalyst for expanded research in this emerging field.
Conveners: James M. Russell, III, Hampton University, Center for Atmospheric Sciences, 23 Tyler Street, Hampton, VA 23668 USA, Tel: +1-757-728-6893, Fax: +1-757-727-5090, E-mail: james.russell@hamptonu.edu; and Gary E. Thomas, University of Colorado, Laboratory for Atmospheric and Space Physics, Boulder, CO 80309-0392 USA, Tel: +1-303-492-7022, Fax: +1-303-492-6946, E-mail: gary.thomas@lasp.colorado.edu; and Richard A. Goldberg, NASA Goddard Space Flight Center, Laboratory for Extraterrestrial Physics Code 690, Greenbelt, MD 20771 USA, Tel: +1-301-286-8603, Fax: +1-301-286-1648, E-mail: goldberg@pop600.gsfc.nasa.gov

SA04 Remote Sensing of the Low- and Mid- Latitude Thermosphere and Ionosphere From the Ground and From Space
The low- and mid-latitude thermosphere and ionosphere are dynamic regions exhibiting strong and complex coupling. There is coupling between charged and neutral species, between different altitudes, and between equatorial and nonequatorial latitudes.  Contributions are solicited which address the observation and interpretation of low- or mid-latitude thermospheric and ionospheric phenomena at altitudes above 100 km. Observations and modeling studies on all length scales (global, regional, and local) are of interest. The emphasis will be on determinations of the composition and temperature of the ionosphere and thermosphere and how these variables are affected by dynamics, electric fields, photochemistry, and geomagnetic and solar forcing.
Conveners: K. F. Dymond, Naval Research Laboratory, Code 7623, Washington, DC 20375 USA, Tel: +1-202-767-2816, E-mail: dymond@tip.nrl.navy.mil; and P. A. Bernhardt, Naval Research Laboratory, Code 6794, Washington, DC 20375 USA, Tel: +1-202-767-0196, E-mail: bern@ppdu.nrl.navy.mil

SPA: Aeronomy also presents jointly with the following Special Sessions:
A01 Earth Science Applications of Reflected and Refracted GPS Transmissions (Joint with G, GP, H, SA)
A06 Middle Atmospheric Odd Nitrogen (Joint with SA)
SH07 Sources of Long-Term Trends in Space Weather (Joint with SA, SM, SPD)
SH08 X-Ray Emission in the Solar System (Joint with P, SA, SM)
SM01 Driving Mechanisms for Transient Phenomena in the Dayside Auroral Zone (Joint with SA)
SM02 Ionospheric Mass Loading of Magnetospheric Dynamics (Joint with SA, SH)
SM04 Global Dynamics of the Magnetosphere from Imaging and Remote Sensing as Compared with Theoretical Models (Joint with SA, SH)
SM05 Magnetic Storm Development: Relative Roles of Enhanced Convection, Particle Sources, and Substorms (Joint with SA)
 

SPA: Solar and Heliospheric Physics

SH01 Abundance Variations in the Solar Corona, Solar Wind and Solar Energetic Particles (Joint with SPD)
The sun contains the bulk of solar system material, and spacecraft can directly sample this material with optical observations of the corona and in-situ measurements of solar energetic particles and the solar wind.  Understanding the variability of the elemental, isotopic, and charge-state composition of the corona, solar wind, and solar energetic particles is crucial for determining how these samples originate from the Sun's reservoir of largely unfractionated material, the outer convective zone.  High resolution measurements of the composition of coronal, solar wind and energetic particles are increasingly highlighting their variability.  The papers in this session will not only focus on our increased capabilities to observe and characterize these variations with the instrumentation on spacecraft such as Ulysses, Wind, SOHO, and ACE, but will also present theoretical interpretations and consequences of this variability.
Conveners: Robert F. Wimmer-Schweingruber, University of Bern, Physikalisches Institut Silderstrasse 5, Bern, CH-3012 Switzerland, Tel: +41 31 631 44 20, Fax: +41 31 631 44 05, E-mail: robert.wimmer@phim.unibe.ch; and Joe Mazur, The Aerospace Corporation, M2/259 2350 El Segundo Boulevard, El Segundo, CA 90245-4691 USA, Tel: +1-310-336-2389, Fax: +1-310-563-3165, E-mail: joseph.mazur@aero.org; and Rick Leske, California Institute of Technology, M/C 220-47 Downs Laboratory, Pasadena, CA 91125 USA, Tel: +1-626-395-8400, Fax: +1-626-449-8676, E-mail: ral@citsrl.srl.caltech.edu; and John Raymond, Center for Astrophysics, 60 Garden Street MS 15, Cambridge, MA 02138 USA, Tel: +1-617-495-7416, Fax: +1-617-495-7049, E-mail: jraymond@cfa.harvard.edu

SH02 The Coronal Solar Wind: Observations and Theory (Joint with SPD)
Observations carried out from the Solar and Heliospheric Observatory have revised our view about plasma conditions in the regions where the solar wind is formed and accelerated. For example, data from the Ultraviolet Coronagraph Spectrometer (UVCS) show surprisingly high values for ion temperatures, temperature anisotropies and ion flow speeds near the sun. As a result, theories on solar wind expansion must be revised to accommodate these new data.  To further advance the knowledge of the formation of the solar wind, papers are invited on any aspect of the fast and slow solar wind dynamic, heating and acceleration, and on plasma structures originating within the solar wind source regions, e.g. plumes and jets.
Conveners: Ruth Esser, Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138 USA, Tel: +1-617-496-7566, Fax: +1-617-495-7049, E-mail: resser@cfa.harvard.edu; and Danuta Dobrzycka, Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138 USA, Tel: +1-617-496-7568, Fax: +1-617-495-7049, E-mail: ddobrzycka@cfa.harvard.edu

SH03 Solar Magnetism and its Relation to Coronal Heating and Dynamics (Joint with SPD)
Recent developments of advanced theoretical and numerical methods have enabled a more comprehensive description of the causes and consequences of coronal mass ejections (CMEs).  Different scenarios for CME genesis and propagation can now be described in much more detail, enabling direct comparisons of solar and interplanetary data that have not been possible so far. A large volume of solar data from SOHO, TRACE, and Yohkoh are ideally suited for such tests, particularly if the measurements are put into the context of in situ data, for example from Wind, ACE and Ulysses.  We encourage presentations on solar and in situ data providing important constraints for successful model descriptions, in particular, those involving both solar and heliospheric aspects of the CME phenomenon.  We also encourage contributions on theoretical models providing testable scenarios and quantitative comparisons between theoretical predictions and data.
Conveners: John M. Davis, NASA Marshall Space Flight Center, Code SD50, Huntsville, AL 35812, USA, Tel: +1-256-961-7600, Fax: +1-256-961-7215, E-mail: John.Davis.3@msfc.nasa.gov; and George Doschek, NRL, Code 7670, Washington, DC 20375-5352 USA, Tel: +1-202-767-3527, Fax: +1-202-404-7997, E-mail: doschek@sola.nrl.navy.mil; and Leon Golub, Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge MA 02138 USA, Tel: +1-617-495 7177, Fax: +1-617-496 8495, E-mail: lgolub@cfa.harvard.edu; and Alan Title, Lockheed Martin Advanced Technology Center, 3251 Hanover St., Palo Alto, CA 94304-1121 USA, Tel: +1-650-424-4032, Fax: +1-650-424-3994, E-mail: title@lmsal.com

SH04 Physics of CMEs: Comparison of Theory and Observations (Joint with SPD)
Recent developments of advanced theoretical and numerical methods have enabled a more comprehensive description of the causes and consequences of coronal mass ejections (CMEs).  Different scenarios for CME genesis and propagation can now be described in much more detail, enabling direct comparisons of solar and interplanetary data that have not been possible so far. A large volume of solar data from SOHO, TRACE, and Yohkoh are ideally suited for such tests, particularly if the measurements are put into the context of in situ data, for example from Wind, ACE and Ulysses.  We encourage presentations on solar and in situ data providing important constraints for successful model descriptions, in particular, those involving both, solar and heliospheric aspects of the CME phenomenon.  We also encourage contributions on theoretical models providing testable scenarios and quantitative comparisons between theoretical predictions and data.
Conveners: Thomas H. Zurbuchen, University of Michigan, Space Research Laboratory, Ann Arbor, MI 48109-2143 USA, E-mail: thomasz@umich.edu; and James Chen, Naval Research Laboratory, Code 6790, Washington, DC 20375-5352 USA; and Spiro K. Antiochos, Naval Research Laboratory, Code 7675, Washington, DC 30375-5352 USA; and Joan Burkepile, High Altitude Observatory, Boulder, CO 80307-3000 USA; and Nat Gopalswamy, GSFC, Greenbelt, MD 20771 USA

SH05 Are There Two Classes of Coronal Mass Ejections?  (Joint with SPD)
Coronal mass ejections (CMEs) are spectacular solar phenomena involving the release of large quantities of solar material into interplanetary space. They may play a crucial role in the large-scale evolution of the solar corona and are the principal cause of large geomagnetic storms. Over the years, a number of solar and in situ studies have hinted that two intrinsic classes of CMEs may exist. In particular, it has been found that fast, flare-related events often propagate away from the Sun at constant speed, whereas slower, prominence-related events are observed to accelerate. However, other studies have refuted these claims, arguing that either insufficient evidence exists, or that CMEs are better described by a continuous distribution of properties. We solicit abstracts pertaining to all aspects of this issue, including interplanetary counterparts, and we particularly encourage presentations that combine disparate datasets and/or theoretical predictions. In an effort to foster collaborative projects and disseminate information prior to the session, a Web site has been developed.
Conveners: Pete Riley, Science Applications International Corporation, 10260 Campus Point Drive, San Diego, CA 92121 USA, Tel: +1-858-826-9550, E-mail: uk2@haven.saic.com; and Hilary Cane, University of Tasmania, School of Mathematics and Physics, GPO Box 252-21, Hobart, TAS 7001 Australia, Tel: +61-03-6293-1335, E-mail: hilary.cane@utas.edu.au

SH06 Tracking CMEs From the Sun Into the Heliosphere  (Joint with SPD)
The large amount of data obtained during this solar cycle on the characteristics of both coronal mass ejections (CMEs) and interplanetary ejecta give us an unprecedented opportunity for a major advance in our understanding of the life cycle of CMEs and related solar wind phenomena.  Recent spectroscopic and imaging studies with the SOHO instruments, TRACE, and Yohkoh SXT have provided insights into the solar dynamics and source regions of CMEs as well as their evolution through the corona, including associated shock propagation.  In situ observations at 1 AU, primarily by the ACE and Wind spacecraft, have revealed their magnetic and particle structures, which can be related both to their solar origins and to their coupling to the magnetosphere.  Observations of halo CMEs have been particularly useful for these studies and have been the bases of joint campaigns involving the Sun-to-Earth connections of transient disturbances.  We invite papers related to these subjects, and, in particular, on those studies which compare CMEs and interplanetary ejecta.
Conveners: David F. Webb, Boston College, ISR AFRL/VSBS, 29 Randolph Road, Hanscom AFB, MA 01731-3030 USA, Tel: +1-781-377-3086, Fax: +1-781-377-3160, E-mail: david.webb@hanscom.af.mil; and Stephen Kahler, AFRL/VSBS, 29 Randolph Road, Hanscom AFB, MA 01731-3030 USA, Tel: +1-781-377-9665, Fax: +1-781-377-3160, E-mail: stephen.kahler@hanscom.af.mil; and Len Burlaga, NASA/GSFC, Code 692, Greenbelt, MD 20771 USA, Tel: +1-301-286-5956, Fax: +1-301-286-1683, E-mail: burlaga@lepvax.gsfc.nasa.gov; and Chris St. Cyr, NASA/GSFC/CUA, Code 682, Greenbelt, MD 20771 USA, Tel: +1-301-286-2575, Fax: +1-301-286-1617, E-mail: stcyr@cua.edu

SH07 Sources of Long-Term Trends in Space Weather (Joint with SA, SM, SPD)
An ongoing puzzle in solar-terrestrial coupling is the long-term increase in some geomagnetic indices, notably the "aa" index, over the last century. Recently Lockwood et al. [Nature, 399, 1999] proposed that this trend results from an increase in the solar source magnetic field.  Their explanation is considered consistent with the corresponding increase inferred for solar radiative fluxes by both Lean [GRL, 1999] and Fligge and Solanki [GRL, 2000].  While the interpretation has met with some challenges, attention has been refocused on this timely question that we are now, in theory at least, much better equipped to re-examine because of our improved grasp of the space weather system.  The aim of this special session is to bring together scientists from the solar, interplanetary, magnetospheric and ionospheric communities to discuss results that resolve, or contribute to the resolution of this long-standing enigma.  Questions to be addressed include:  1) What geomagnetic indices show increasing trends, and what is the physics underlying those indices?  2) Is the Sun's magnetic field really changing, and if so what is causing the change and what are its consequences for solar outputs (solar wind, radiative, particles) that affect the Earth?  3) Is there any evidence for long-term changes in the interplanetary medium?  4) Do long-term changes in geomagnetic indices suggest corresponding long-term changes in the magnetosphere or upper atmosphere/ionosphere?  5) If the increasing trend in solar irradiance continues, what can we expect from a space weather perspective?
Conveners: Nick Arge, University of Colorado, CIRES/NOAA/SEC R/E/SE, 325 South Broadway, Boulder, CO 80305 USA, Tel: +1-303-497-7394, Fax: +1-303-497-3645, E-mail: Nick.Arge@noaa.gov; and Janet G. Luhmann, University of California Berkeley, Space Sciences Laboratory, Berkeley, CA 94720 USA, Tel: +1-510-642-2545, Fax: +1-510-643-8302, E-mail: jgluhman@SSL.Berkeley.EDU; and Rodney Viereck, NOAA, Space Environment Center R/E/SE, 325 South Broadway, Boulder, CO 80305 USA, Tel: +1-303-497-7348, Fax: +1-303-497-3645, E-mail: Rodney.Viereck@noaa.gov

SH08 X-Ray Emission in the Solar System (Joint with P, SA, SM)
X-ray and extreme ultraviolet (EUV) emission has been observed from many objects throughout the solar system including the Sun, the Moon, the Earth, Jupiter, and comets.  X-ray emission associated with the interaction of the solar wind with interstellar neutrals has also been predicted. The recently launched Chandra X-ray observatory, with its unprecedented high spatial and spectral resolution, has recently provided strong evidence for solar wind charge exchange induced x-ray emission from comets, and further exciting results from both Chandra and FUSE can be expected. X-ray observations of solar system objects is a potentially important diagnostic tool for understanding physical processes operating at these objects, such as particle precipitation at Jupiter or the solar wind interaction with comets.  In this session, a few invited review papers will summarize recent progress and future directions, including relevant laboratory measurements. Contributed papers on all aspects of this interesting topic are welcome.
Conveners: T. E. Cravens, University of Kansas, Department of Physics and Astronomy, Lawrence, KS 66045 USA, Tel: +1-785-864-4739, Fax: +1-785-864-5262, E-mail: cravens@kuplas.phsx.ukans.edu; and V. Kharchenko, Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138 USA, Tel: +1-617-495-7536, Fax: +1-617-496-7668, E-mail: kharchen@cfa.harvard.edu; and C. M. Lisse, NISD, Space Telescope Institute 3700 San Martin Drive, Baltimore, MD 21218 USA, Tel: +1-410-338-4395, Fax: +1-410-338-4796, E-mail: lisse@stsci.edu

SPA: Solar and Heliospheric Physics presents jointly with the following Special Sessions:
SPD01 Nanoflare Statistics, Self-Organized Criticality, and Coronal Heating (Joint with NG, SH)
SM02 Ionospheric Mass Loading of Magnetospheric Dynamics (Joint with SA, SH)
SM03 Progress in Magnetic Reconnection Research in Space and Laboratory Plasmas (Joint with SH)
SM04 Global Dynamics of the Magnetosphere from Imaging and Remote Sensing as Compared with Theoretical Models (Joint with SA, SH)
 

American Astronomical Society, Solar Physics Division (AAS/SPD)

SPD01 Nanoflare Statistics, Self-Organized Criticality, and Coronal Heating (Joint with NG, SH)
A major number of statistical studies on solar (as well as stellar) flares, microflares, and nanoflares has been published recently, focusing on their potential for explaining the heating of the solar corona. Observational statistics have been gathered from recent space missions such as Yohkoh, SoHO, and TRACE in EUV and soft X-rays, spanning a range over 8 orders of magnitude in energy, E=10(24)-10(32) erg, but yielding controversial results on the numerical value of the power-law slope of their frequency distributions. On the theoretical side, since nanoflares have been postulated by Parker in 1988, a continuous string of theoretical models emerged on the physics and statistics of solar nanoflares, also stimulated by the pioneering work of Lu and Hamilton (1993) by applying the principle of self-organized criticality to solar nanoflares. It is therefore timely to dedicate a special session to address observational and data analysis issues of nanoflare statistics, to compare theoretical models with new observations, and to discuss the implications for coronal heating.
Conveners: Markus J. Aschwanden, Lockheed Martin Solar and Astrophysics Laboratory, Dept. L9-41 Bldg. 252, 3251 Hanover Street, Palo Alto, CA 94304 USA, Tel: +1-650-424-4001, Fax: +1-650-424-3994, E-mail: aschwanden@lmsal.com; and Grisha Vekstein, UMIST, Dept. of Physics PO Box 88, Manchester, M60 1QD United Kingdom, Tel: +44 161-200-3913, Fax: +44 161-200-3941, E-mail: G.Vekstein@umist.ac.uk

SPD02 Physical Mechanisms of Solar Luminosity Variation
A consensus is emerging from empirical modelling of total irradiance variation, that most of the variance in the 22-year radiometric record can be explained by the competing effects of dark sunspots and bright faculae and network.  Physical explanations of the effect of these magnetic structures on solar heat flow have been developed, and their thermal blocking seems to explain the observed irradiance variations quite well.  Nevertheless controversy continues on the possible importance of other physical  effects such as stirring of convection by rising magnetic flux, and and by hypothesized global variations in convective efficiency, or solar diameter.  Even if such effects turn out to be small over the solar cycle, they might play an important role over climatically more significant time scales.  The purpose of this session will be to confront the various physical mechanisms with the latest observational constraints derived from solar radiometry and photometry, from helioseismology, and also from stellar photometry.
Conveners: Peter Foukal, CRI, Inc., 80 Ashford Street, Boston, MA 02134 USA, Tel: +1-617-787-5700, Fax: +1-617-787-4488, E-mail: pfoukal@world.std.com; and Hendrick Spruit, Max Planck Institut fur Astrophysik, Karl Schwarzschild Strasse 1, Postfach 1523, Garching, D-85740 Germany, Tel: +49-89-3299-00, Fax: +49-89-3299-3235, E-mail: henk@mpa.garching.mpg.de

SPD03 Helioseismology and Variability of the Solar Interior
The session will focus on the results of continuous monitoring of the solar interior by ground-based networks (GONG, LOWL, BISON, TON and others) and by three helioseismology instruments (MDI, GOLF and VIRGO) on board SOHO spacecraft. The new data have provided a tremendous amount of new information about the internal structure and dynamics of the Sun at various spatial and temporal scales, covering the raising phase of the current solar cycle. These data open a unique opportunity for understanding the physics of the Sun's interior and mechanisms of solar variability. The topics of this session include, but are not limited to, observational, theoretical and computational methods of both global and local-area helioseismology; physics of solar interior and oscillations; results of helioseismic analyses and inversions; global structures, dynamics and circulation and their variations with the solar cycle; physics of solar convection, dynamo, active regions and sunspots; links between the solar interior and coronal activity, and applications of helioseismic diagnostics for understanding solar variability and space weather forecasts.
Conveners: Frank Hill, National Solar Observatory, PO Box 26732, Tucson, AZ 85726-6732 USA, Tel: +1-520-318-8138, Fax: +1-520-318-8278, E-mail: fhill@noao.edu; and Alexander Kosovichev, Stanford University, W.W. Hansen Experimental Physics Laboratory 455 via Palou, Stanford, CA 94305-4085 USA, Tel: +1-650-723-7667, Fax: +1-650-725-2333, E-mail: AKosovichev@solar.stanford.edu; and Philip Scherrer, Stanford University, W.W. Hansen Experimental Physics Laboratory, 455 via Palou, Stanford, CA 94305-4085 USA, Tel: +1-650-723-1504, Fax: +1-650-725-2333, E-mail: PScherrer@solar.stanford.edu

Solar Physics Division-AAS also presents jointly with Special Sessions:
SH01 Abundance Variations in the Solar Corona, Solar Wind and Solar Energetic Particles (Joint with SPD)
SH02 The Coronal Solar Wind: Observations and Theory (Joint with SPD)
SH03 Solar Magnetism and its Relation to Coronal Heating and Dynamics (Joint with SPD)
SH04 Physics of CMEs: Comparison of Theory and Observations (Joint with SPD)
SH05 Are There Two Classes of Coronal Mass Ejections?  (Joint with SPD)
SH06 Tracking CMEs From the Sun Into the Heliosphere  (Joint with SPD)
SH07 Sources of Long-Term Trends in Space Weather (Joint with SA, SM, SPD)
 

SPA: Magnetospheric Physics

SM01 Driving Mechanisms for Transient Phenomena in the Dayside Auroral Zone (Joint with SA)
Traveling convection vortices, flow bursts, transient auroral brightenings and other impulsive events observed in the dayside auroral oval provide evidence for unsteady solar wind-magnetosphere interaction mechanisms like bursty merging, the Kelvin-Helmholtz instability, and pressure-pulse driven magnetopause boundary waves.  Once the ionospheric events have been correctly associated with corresponding phenomena at the dayside magnetopause, it should be possible to use their occurrence patterns to determine the significance of each proposed mechanism.  This session will emphasize efforts to compare theoretical predictions with observed event characteristics and occurrence patterns in the ionosphere.
Conveners: David G. Sibeck, JHU/APL, 11100 Johns Hopkins Rd., Laurel, MD 20723 USA, Tel: +1-240-228-8545, Fax: +1-240-228-6670, E-mail:david.sibeck@jhuapl.edu; and M. Hesse, NASA/GSFC, Code 696, Greenbelt, MD 20771 USA, Tel: +1-301-286-8224, Fax: +1-301-286-1648, E-mail: michael.hesse@gsfc.nasa.gov

SM02 Ionospheric Mass Loading of Magnetospheric Dynamics (Joint with SA, SH)
A GEM campaign has been organized to investigate Magnetosphere-Ionosphere Coupling via mass loading by plasma outflows from the ionosphere. The ultimate objective of this campaign is to foster the development of a predictive heliosphere geosphere interaction model, with ionospheric plasma appearing as a dynamical as well as electrodynamic element of interactions with the magnetosphere. Three challenges were identified as steps toward this end: 1. Mass Exchange Characterization, as a function of solar, heliospheric, and local conditions; 2. Impacts of Ionospheric Plasmas, both from observations and global circulation modeling; and 3. Mass Extraction Process Modeling, capable of incorporating flux tube history effects, that would run inside of global circulation models. Papers are solicited that use observations or theoretical modeling to address any aspect of these overarching objectives.
Conveners: T. E. Moore, NASA Goddard Space Flight Center, Laboratory for Extraterrestrial Physics, Greenbelt, MD 20771 USA, Tel: +1-301-286-5236, Fax: +1-707-988-7835, E-mail: thomas.e.moore@gsfc.nasa.gov; and W. K. (Bill) Peterson, Lockheed Martin Space Sciences Laboratory, C/O University of Colorado LASP, 1234 Innovation Drive, Boulder, CO 80303 USA, Tel: +1-303-492-0686, Fax: +1-303-492-6444, E-mail: pete@willow.colorado.edu

SM03 Progress in Magnetic Reconnection Research in Space and Laboratory Plasmas (Joint with SH)
This special session will bring together experts from different disciplines to discuss the important problem of magnetic reconnection. The crucial question concerns the rate at which a local reconnection can proceed, and lead to rapid conversion of magnetic energy to other forms.  The experts who will present talks for discussion come from the fields of numerical simulation, experimental plasma physics, solar physics and magnetosphere physics. Special attention will be put on two-fluid MHD physics issues. By comparing the results on magnetic reconnection from space and laboratory plasma, it is hoped to obtain new insights on the physics of magnetic reconnection.
Conveners: Masaaki Yamada, Princeton University, Princeton Plasma Physics Laboratory, PO Box 451, Princeton, NJ 08543 USA, Tel: +1-609-243-2566, Fax: +1-609-243-2418, E-mail: myamada@pppl.gov; and David Rust, Johns Hopkins University, Applied Physics Laboratory, 11100 Johns Hopkins Road, Laurel, MD 20723 USA, Tel: +1-240-228-6670, Fax: +1-240-228-5414, E-mail: dave.rust@jhuapl.edu; and James Drake, University of Maryland, Institute of Plasma Physics, College Park, MD 20742 USA, Tel: +1-301-405-1471, Fax: +1-301-405-1678, E-mail: drake@plasma.umd.edu

SM04 Global Dynamics of the Magnetosphere from Imaging and Remote Sensing as Compared with Theoretical Models (Joint with SA, SH)
The magnetosphere is the critical link in the Sun-Earth connection, between the solar wind and the Earth. During the past few years, and especially since the launch of the IMAGE mission, a fundamentally new set of observational tools has become available for magnetospheric research, including various kinds of global imaging and remote sensing. To an unusual degree, these new observations lend themselves to qualitative and quantitative comparisons with global dynamic models of the magnetosphere, and indeed depend upon such models for their interpretation in some cases. Concurrently, magnetospheric modeling has advanced significantly in global comprehensiveness and dynamic realism.  For this session, we seek invited and contributed papers that report relevant efforts designed to exploit the new measurements and global models, by identifying and interpreting familiar features, model predictions, and especially those new aspects of the observations not apparently described by current modeling efforts.
Conveners: D. L. Gallagher, NASA Marshall Space Flight Center, Code SD50 Space Science Department, Huntsville, AL 35812 USA, Tel: +1-256-544-7587, Fax: +1-256-544-5244, E-mail: dennis.gallagher@msfc.nasa.gov; and C. J. Pollock, Southwest Research Institute, Instrumentation and Space Science Division, San Antonio, TX 78208 USA, Tel: +1-210-522-3978, E-mail: cpollock@swri.org; and J. L. Green, NASA Goddard Space Flight Center, Code 630 Space Science Data Operations Office, Greenbelt, MD 20771 USA, Tel: +1-301-286-7354, E-mail: james.green@gsfc.nasa.gov; and T. E. Moore, NASA Goddard Space Flight Center, Laboratory for Extraterrestrial Physics, Greenbelt, MD 20771 USA, Tel: +1-301-286-5236, E-mail: thomas.e.moore@gsfc.nasa.gov

SM05 Magnetic Storm Development: Relative Roles of Enhanced Convection, Particle Sources, and Substorms (Joint with SA)
For many years the standard paradigm for the creation of magnetic storms has been the idea that a substorm expansion phase injects plasma sheet ions that drift westward forming a partial ring current that eventually becomes symmetric due to differential drift. The ions are then lost by charge exchange decay. This paradigm has been challenged by a number of recent observations. The new observations suggest that a substantial part of the symmetric ring current is injected by global convection rather than the substorm expansion. Variations in the particle sources modulate the geoeffectivess for a given convection strength. Also considerable numbers of the ions may come from the ionosphere rather than the tail. A significant fraction of the ions may be lost through the magnetopause rather than charge exchange. In addition, it appears that a substantial part of the ground disturbance present in Dst during a magnetic storm may be produced by currents on the magnetopause, in the tail, in the partial ring current (which includes ions on paths open to the magnetopause), and in the substorm current wedge, in addition to ring current. The controversial issue is whether the old paradigm needs substantial alteration or the recent observations provide an incomplete view of the important storm processes.
This session invites experimental and theoretical contributions related to the problem of ring current formation and particularly to the interplay between convection and substorm injections in that process.
Conveners: Robert L. McPherron; UCLA IGPP, 405 Hilgard Ave., Los Angeles, CA 90095-1567, Tel: +1-310-825-1882, Fax: +1-310-206-8042; E-mail: rmcpherron@igpp.ucla.edu; and Y. Kamide, Nagoya University, Solar Terrestrial Environment Laboratory, Honohara 3-13, Toyokawa, Aichi 442, Japan, Tel: +81-533895183, Fax +81-533890409, E-mail: kamide@stelab.nagoya-u.ac.jp; and Janet U. Kozyra, University of Michigan, Space Physics Research Lab, 2455 Hayward, Ann Arbor, MI 48109- 2143; Tel: +1-734-647-3550, Fax: +1-734-647-3083; E-mail:jukozyra@engin.umich.edu.

SPA: Magnetospheric Physics also presents jointly with the following Special Sessions:
SA01 Short-term Variability in the Thermosphere and Ionosphere: Measurements and Modeling (Joint with SM)
SA02 Space-Based Auroral Remote Sensing (Joint with SM)
SH07 Sources of Long-Term Trends in Space Weather (Joint with SA, SM, SPD)
SH08 X-Ray Emission in the Solar System (Joint with P, SA, SM)
 

Tectonophysics

T01 Recent Tectonics, Kinematics and Dynamics of Southeast Asian Margins (Joint with G, S)
Oblique convergence along subduction margins is responsible for distributed and/or localized deformation in the upper plate, thus offering the opportunity to investigate long-term and short-term coupling at these plate boundaries. In the general framework of the convergence of India, Australia and Pacific plates towards Eurasia, a large amount of kinematic data has been collected at Sundaland margins, including space geodetic measurements (GPS), land geological surveys of the active faults involved in partitioning (Sagaing fault in Myanmar, Sumatra fault in Indonesia, Philippines fault), marine surveys of marginal basins (Andaman basin, South China and Banda basins) seismological studies and tomography of the slabs. Integration of the different types of data is limited by the wide range of time-scale covered by these observations. Strong constraints are now available both for the present-day crustal deformation and the recent tectonic evolution during the past few million years. The proposed session thus aims at gathering these tectonics and kinematics observations, and papers  combining the various geological and geophysical fields involved are greatly encouraged.
Conveners: Nicolas Chamot-Rooke, Ecole normale superieure, Laboratoire de geologie 24, rue Lhomond, Paris, 75231 Cedex 5 France, Tel: +33-1-4432-2257, Fax: +33-1-4432-2000, E-mail: rooke@geologie.ens.fr; and William E. Holt, State University of New York at Stony Brook, Department of Geosciences, Stony Brook, NY 11794-2100 USA, Tel: +1-631-632-8215, Fax: +1-631-632-8240, E-mail: wholt@horizon.ess.sunysb.edu

T02 Dynamics of Gas Hydrate Reservoirs and Similar Shallow Marine Flow Systems (Joint with B, GS, H, OS)
An emerging frontier in the study of gas hydrate reservoirs, submarine slope stability issues, and so-called "shallow water flow" is the quantitative analysis of the shallow sedimentary section as a dynamic hydrogeologic system.  A deeper understanding of these systems requires observations and methods that: (1) quantitatively constrain the fluxes of fluid, gas, and energy and (2) consider the impact of sedimentation rates and permeability variations on enhancing and focusing fluid fluxes, respectively. This session emphasizes geochemical or biological proxies, direct seafloor or borehole geophysical measurements, and theoretical analyses that constrain critical flux rates in marine gas hydrate reservoirs and similar shallow marine hydrogeologic systems. Observational studies that link sedimentary processes to the evolution of shallow flow regimes or the destabilization of submarine slopes are encouraged.  Modeling studies that evaluate the relationships among sedimentation rate, permeability variations, discharge of fluid or gas at the seafloor, formation/dissociation of gas hydrates, the evolution of two- and three-dimensional flow regimes, and/or slope stability are also welcome.
Conveners: C. Ruppel, Georgia Tech, School of Earth and Atmospheric Sciences, Atlanta, GA 30332-0340 USA, Tel: +1-404-894-0231, E-mail: cdr@piedmont.eas.gatech.edu; and P. Flemings, Penn State University, Department of Geosciences 442 Deike Building, University Park, PA 16802 USA, Tel: +1-814-865-2309, E-mail: flemings@geosc.psu.edu

T03 Computational Earth Laboratories (Joint with GP, M, MR, NG, S)
In the last decade geophysics has profited from an unprecedented growth in computer resources, a development that is likely to continue into the future. The impact of this development on our field is already being felt. First principle calculations of Earth materials now reinforce high-pressure experiments. Geodynamo simulations add insight into interpreting palaeomagnetic observations. Seismologists study wave propagation numerically, while geodynamicists turn to seismic, tectonic and geochemical data to test their models. The numerical techniques and challenges shared by computational geophysicists are numerous. However, the true opportunity of growing computer resources is to combine these modeling efforts into a virtual Earth Laboratory, where we integrate geodynamic, seismic and mineralogic hypotheses and test them with laboratory and observational data. In this session, we invite contributions from computational mineralogy, seismic wave propagation modeling and geodynamics. We also strongly encourage contributions from observational seismology, tectonics, mantle geochemistry and high pressure mineral physics aimed at constraining Earth structure and processes.
Conveners: Hans-Peter Bunge, Princeton University, Department of Geological and Geophysical Sciences, Princeton, NJ 08540 USA, Tel: +1-609-258-4128, Fax: +1-609-258-1274, E-mail: bunge@seismo.berkeley.edu; and Rainer Hollerbach, Princeton University, Department of Geological and Geophysical Sciences, Princeton, NJ 08540 USA, Tel: +1-609-258-4128, Fax: +1-609-258-1274, E-mail: rainer@maths.gla.ac.uk; and Guusth Nolet, Princeton University, Department of Geological and Geophysical Sciences, Princeton, NJ 08540 USA, Tel: +1-609-258-4128, Fax: +1-609-258-1274, E-mail: guust@geo.princeton.edu; and Lars Stixrude, University of Michigan, Department of Geological Sciences, Ann Arbor, MI 48109-1063 USA, Tel: +1-734-647-9071, Fax: +1-734-763-4690, E-mail: stixrude@umich.edu

T04 True Polar Wander on Earth, Mars and Beyond (Joint with G, GP, P)
True Polar Wander (TPW), a geographic shift of the inertial axis or a shift of the outer shell of a rotating body, has been proposed for Earth and Mars, and conceivably could have occurred on other planets. This session examines models for the excitation of TPW and its damping. Observations on Earth for TPW — gradual or catastrophic — from magnetic anomalies, paleomagnetic data or hotspots, as well as geological evidence will be examined.  Possible occurrence on Mars and the implications for its surface and polar deposits will also be included, as well as evidence from other bodies. Diverse contributions are invited relevant to the process and observations of TPW on Earth, Mars and beyond.
Conveners: Donna M. Jurdy, Northwestern University, Department of Geological Sciences, Evanston, IL 60208-2150 USA, Tel: +1-847-491-7163, E-mail: donna@earth.nwu.edu; and Maria T. Zuber, MIT, Earth, Atmospheric & Planetary Sciences 54-518, Cambridge, MA 02139 USA, Tel: +1-617-253-6397, E-mail: zuber@mit.edu

Tectonophysics also presents jointly with the following Special Sessions:
GP01 Mapping Aquifers, Oceans, and Planetary Bodies with Passive and Active EM Methods (Joint with H, OS, P)
GP07 Magnetic Investigations of the Antarctic (Joint with T)
GS01 Magmatic Volatile Histories: Stable Isotopic Tracing of Sources and Degassing Processes in Magmatic Systems and Implications for Volcanology and Earth System Science (Joint with T, M)
M01 Equation of State and Elasticity of Earth Materials (Joint with MR, SEDI, T, V)
M03 Spectroscopy of Minerals and Other Planetary Phases (Joint with MR, T)
OS01 Non-Equilibrium Phenomena in Geophysics (Joint with A, B, H, P, S, T)
S01 Core Mantle Boundary Region (Joint with GP, GS, MR, NG, SEDI, T)
S03 Integrated Models of Earth Structure and Evolution (ONLINE-only Session) (Joint with MR, SEDI, T, M)
S04 How Rifting Worked in Northeastern North America (Joint with T, V, GS)
S06 The Structure and Early Evolution of Cratons (Joint with T, V, GS)
V04 Petrological and Geochemical Constraints of the Formation of Archean Cratons (Joint with T, GS)
V05 The Construction of Archean Cratons: Reconciling Radiometric Dates From Crustal and Mantle Rocks (Joint with T, GS)
NG02 Integrating and Applying Models, Simulations, and Data to the Forecasting of Nonlinear Geophysical Systems (Joint with H, T)
 

Volcanology, Geochemistry, and Petrology

V01 Continental Weathering and Ocean Chemistry (Joint with H, OS, GS)
Recent studies link chemical weathering on the continents to changes in global ocean chemistry.  This session will focus on the specific linkages between chemical weathering on the continents as recorded by fluvial, estuarine and sediment geochemical processes and the chemistry of the oceans.  Contributions that focus on spatial and temporal chemical variations in river water and groundwater chemistry, estuarine chemistry, ocean chemistry as well as experimental studies of mineral/rock weathering are solicited.  The goal is a multidisciplinary session that brings together experimental and aqueous geochemistry, sedimentary and isotopic-geochemical aspects of these and related topics.
Conveners: Robyn E. Hannigan, Arkansas State University, Department of Chemistry and Program for Environmental Science, AR 72467 USA, Tel: +1-870-972-3086, Fax: +1-870-972-3089, E-mail: hannigan@navajo.astate.edu; and Asish R. Basu, University of Rochester, Department of Earth and Environmental Sciences, Rochester, NY 14627 USA, Tel: +1-716-275-2413, Fax: +1-716-244-5689, E-mail: abasu@earth.rochester.edu

V02 New Views of Mars Volcanism: Extrusive, Explosive, and Possible Influences of H2O (Joint with P)
Before the recent Mars missions, volcanic activity on Mars was thought to be primarily "old" (restricted to more than 1.3 b.y. ago) and mafic. Although a range of eruption styles seemed likely, available topographic data poorly constrained the existing models. Today, analyses of Pathfinder and MGS data suggest a range of lava compositions, and provide topographic and image evidence for more extensive volcanism-some of it quite recent (possibly even current). This session is intended to explore our changing views of the thermal and chemical evolution of Mars by examining new evidence for volcanic activity on Mars throughout its geologic history. We will provide a forum for discussing compositional data, proposed eruption styles and mechanisms, and evidence for recent volcanic activity.
Conveners: Susan Sakimoto, NASA/GSFC, UMBC Code 921, Greenbelt, MD 20771 USA, Tel: +1-301-614-6470, Fax: +1-301-614-6522, E-mail: sakimoto@denali.gsfc.nasa.gov; and Tracy Gregg, The University of Buffalo, Department of Geology and Geophysics, 876 Nat. Science and Mathematics Complex, Buffalo, NY 14260-3050 USA, Tel: +1-716-645-6800 ext. 2463, Fax: +1-716-636-4827, E-mail: Tgregg@nsm.buffalo.edu; and Lori Glaze, Proxemy Research, 20528 Farcroft Lane, Laytonsville, MD 20882 USA, Tel: +1-301-313-0026, Fax: +1-301-313-0021, E-mail: lori@proxemy.com

V03 Advances in Subsurface Sampling and Borehole Measurement
During the last several years the technology for acquiring subsurface samples and for characterizing and monitoring subsurface conditions has undergone a number of significant advances.  For example, these new technologies have enabled us to expand the temporal spectrum of observations with real-time, continuous monitoring of borehole conditions in the short term and greatly extended shallow water sediment records over the longer term.  We can now access and recover samples from extreme environments to depths of >6 km and conduct geophysical surveys at substantially higher temperatures than were possible even a decade ago.  These technologies have not only made it possible to greatly expand the breadth of our analysis of regional and planetary processes, they have also increased our awareness of the ability of specialized technologies to provide us with access to environments that were previously inaccessible.  This special session invites submissions on state-of-the-art technologies for borehole sampling, measurement, and monitoring as well as papers by those whose research programs require significant advances of currently available technology in order to monitor or sample challenging subsurface environments.
Conveners: Donald Thomas, University of Hawaii, DOSECC and Department of Geophysics, 2525 Correa Road, Honolulu, HI 96822 USA, Tel: +1-808-956-6482, Fax: +1-808-956-3188, E-mail: dthomas@soest.hawaii.edu; and Allan R. Sattler, Sandia National Laboratories, PO Box 5800, Albuquerque, NM 87185-1033 USA, Tel: +1-505-844-1019; and David Goldberg, Columbia University, Lamont-Doherty Earth Observatory, Route 9W, Palisades, NY 10964-0190 USA, Tel: +1-845-365-8674 ext. 674

V04 Petrological and Geochemical Constraints of the Formation of Archean Cratons (Joint with T, GS)
The Archean cratons of Earth are noteworthy for their occurences of tonalite-trondhjemite-granodiorite and komatiite along with a mantle keel that contains metasomatized, depleted harzburgite, eclogite and diamonds. Contributions from experimental petrology, theoretical petrology, mineralogy, and trace element and isotope geochemistry are invited that focus on the processes of formation and assembly of cratons and whether craton formation requires conditions unique to the Archean Earth.
Conveners: Timothy L. Grove, MIT, Department of Earth Atmospheric and Planetary Sciences, Cambridge, MA 02139-4307 USA, Tel: +1-617-253-2878, Fax: +1-617-253-7102, E-mail: tlgrove@mit.edu; and Steven B. Shirey, Carnegie Institution of Washington, Department of Terrestrial Magnetism, 5241 Broad Branch Road, NW, Washington, DC 20015 USA, Tel: +1-202-478-8473, Fax: +1-202-478-8821, E-mail: shirey@dtm.ciw.edu

V05 The Construction of Archean Cratons: Reconciling Radiometric Dates From Crustal and Mantle Rocks (Joint with T, GS)
Reconciling radiometric dates from crustal and mantle rocks. Our understanding of the growth, stabilization, and reactivation of Archean cratons hinges on radiometric dates from both crustal and mantle xenoliths and exposed rocks.  In particular, the relationships between timing of lithospheric assembly and development of a thick bouyant "tectosphere" are not well known.  We seek papers that address the interpretation and integration of radiometric dates from crustal and mantle rocks, with the specific goal of  constraining the timing and processes of tectosphere/crustal juxtaposition and reactivation.
Conveners: Samuel A. Bowring, MIT, Department of Earth, Atmospheric and Planetary Sciences, Cambridge, MA 02139 USA, Tel: +1-617-253-3775, Fax: +1-617-253-6735, E-mail: sbowring@mit.edu; and Desmond E. Moser, University of Utah, Department of Geology and Geophysics, 135 S, 1460 E, Salt Lake City, UT 84112 USA, Tel: +1-801-585-3782, Fax: +1-801-581-7065, E-mail: demoser@mines.utah.edu

Volcanology also presents jointly with the following Special Sessions:
GP01 Mapping Aquifers, Oceans, and Planetary Bodies with Passive and Active EM Methods (Joint with H, OS, P)
GP08 Precise Correlation of Strata: Magnetic and Other Methods (Joint with OS, V)
GS02 Light Stable Isotope Ratio Standards Metrology: Recent Advances and Needs Assessment (Joint with V)
M01 Equation of State and Elasticity of Earth Materials (Joint with MR, SEDI, T, V)
M02 Characterizing Organic and Inorganic Hydrothermal Systems (Joint with V, GS)
OS02 High-Resolution Climate Records From Laminated Sediments (Joint with V, GS)
P02 New Views of the Moon (ORAL) (Joint with V, GS)
S04 How Rifting Worked in Northeastern North America (Joint with T, V, GS)
S06 The Structure and Early Evolution of Cratons (Joint with T, V, GS)
 

Education and Human Resources

ED01 DLESE and Digital Earth: Bridging Multidimensional Geospatial Data Resources for Educators
The Digital Library for Earth System Education (DLESE) and the interagency Digital Earth (DE) initiative are each charged with making information available to a wide community of users. DLESE aims to enable educators and students to rapidly locate and access high quality interdisciplinary educational resources about the Earth system, to provide training and tools for utilization of Earth data, and to be a community center for Earth System Education. DLESE and Digital Earth goals are complementary in providing a virtual representation of our planet that enables exploration and interaction with the vast amounts of natural and cultural information about Earth. DE plays an important role in making multidimensional temporal/spatial data accessible in a consistent and standardized fashion to the public. Building on that infrastructure, DLESE will make such data meaningful to educators and students by providing context, lesson plans and ancillary information. This session will explore the intersection of the concepts, capabilities and vision of the DLESE and DE communities. The session will consist of invited and contributed presentations of example data sets and interfaces, simulations, animations, visualization and viewing tools, case studies, and educational scenarios, focused especially on multidimensional geospatial data that bridge these two efforts. Interdisciplinary contributions which broaden the communities involved with DLESE and DE are encouraged.
Conveners: Martin Ruzek, Universities Space Research Association, 8426 Polifka Road, Whitelaw, WI 54247 USA, Tel: +1-920-732-4514, Fax: +1-920-732-3316, E-mail: ruzek@usra.edu; and Jeff de la Beaujardiere, NASA/UMBC, USA, E-mail: delabeau@iniki.gsfc.nasa.gov; and Ben Domenico, UCAR, USA, E-mail: ben@unidata.ucar.edu; and Roger Kassebaum, USA, E-mail: rkasseba@esu3.esu3.k12.ne.us; and Betty Sword, JPL, USA, E-mail: bsword@mail1.jpl.nasa.gov

ED02 Geophysical Science Education
Outreach Solicited papers would cover education outreach initiatives in the geophysical sciences: Atmospheric and Ocean Sciences, Solid Earth Sciences, Hydrologic Sciences, and Space Sciences. They would discuss the integration of geophysical sciences and the national science education standards. Examples of projects engaged in these initiatives are NSF's Graduate Teaching Fellows Program in K-12 education, the JASON Project, and a suite of NASA programs directed at K-12 audiences. The purpose of the session would be to examine the impact of successful outreach programs that are making a difference in the lives of students, teachers, and the general public while providing a linkage between K-12 education and ongoing scientific research.
Conveners: Gail Scowcroft, University of Rhode Island, Marine and Environmental Sciences, South Ferry Road, Narragansett, RI 02882 USA, Tel: +1-401-874-6724, Fax: +1-401-874-6486, E-mail: gailscow@gso.uri.edu; and Cheryl Schroeder, University of Rhode Island, Graduate School of Oceanography, South Ferry Road, Narragansett, RI 02882 USA, E-mail: cschroed@gso.uri.edu

ED03 Increasing Diversity in the Geosciences
Understanding the environment in which we live and gathering the information needed to make good decisions in this environment are important tools for everyone. Yet, the geosciences are dominated by representatives of a small fraction of this diverse population. This session seeks to highlight examples of programs that have successfully engaged members of groups under represented in the Earth sciences, as well as ideas for ways that geoscience education can better serve these groups in the future. Contributed presentations describing existing programs, as well as future opportunities are encouraged. Invited speakers will report on activities taking place at NSF, NASA and other agencies and organizations as well as in community-wide programs such as DLESE.
Convener: Cathryn A. Manduca, Carleton College, DLESE Outreach Coordinator PO Box 3000, Boulder, CO 80307 USA, Tel: +1-507-252-8658, Fax: +1-507-252-0472, E-mail: cmanduca@carleton.edu; www.dlese.org; and Tom Windham, UCAR PO Box 3000, Boulder, CO 80307 USA, Tel: +1303-497-8624, E-mail: twindham@ucar.edu

ED04 Linking Undergraduate Geoscience and Education Departments: Earth Science Teacher Preparation for the Real World
This session will highlight the work of the nine institutions that participated in AGU's NSF funded Linkages project to bring together geoscience and education departments to develop preservice teacher training programs that reflect the needs of students. Invited papers from several of the Linkages institutions will outline progress — or lack of progress — in implementing programs based on their Linkages workshop experiences. Contributed papers will be encouraged that reflect the development of similar programs in other institutions. Participating Linkages Institutions: Arizona Western College, University of Arizona, University of Washington, Montana State University, New Mexico State University, Northern Arizona University, San Diego State University, and University of Oklahoma.
Conveners: M. Frank Watt Ireton, SESDA. Science Systems and Applications, Inc. 10210 Greenbelt Road, Suite 400, Lanham, MD 20706 USA, Tel: +1-240-232-0300 Ext.1054, E-mail: Frank_Ireton@sesda.com; and Michael Conway, Arizona Western College, Division of Science and Math Box 929, Yuma, AZ 85366 USA, Tel: +1-520-317-6022, Fax: +1-520-344-7730, E-mail: aw_conway@awc.cc.az.us; and Dean McManus, University of Washington, USA; and John Snow, University of Oklahoma, USA

ED05 Where are the Jobs? Career Choices for Students in the Geosciences
Although 100% of recent PhDs in the geosciences are employed, 45% of them have jobs outside of academia or of their PhD specialty. What kinds of jobs are recent PhDs taking and how are they finding these jobs? What marketable skills can a recent PhD offer prospective employers? In order to address these questions we invite presentations from (1) researchers studying employment trends in the geosciences, (2) recent PhDs who are willing to share stories of their successful job searches, (3) recruiters discussing techniques for finding jobs outside the traditional path, and (4) representatives from industry, governmental agencies, the media, and non-profits describing jobs they have available for students of the geosciences and the types of skills and experience that they deem valuable in the workplace. A reception following the session will allow for informal discussions with speakers.
Conveners: Amanda C. Staudt, Harvard University, Department of Earth and Planetary Sciences, Pierce Hall G3G, 29 Oxford Street, Cambridge, MA 02138 USA, Tel: +1-617-495-8455, Fax: +1-617-495-4551, E-mail: acstaudt@fas.harvard.edu; and Jennifer Giesler, American Geophysical Union, 2000 Florida Avenue, NW, Washington, DC 20009 USA, Tel: +1-202-777-7512, Fax: +1-202-328-0566, E-mail: jgiesler@agu.org

ED06 Showcase on Undergraduate Research
Many academic programs for undergraduates provide little opportunity for students to engage in research activities.  Yet most students who have had these opportunities, when asked about their impact, describe the research as the highlight of their undergraduate program and the activity that best prepared them for their subsequent graduate school and/or work careers. This session will feature examples of successful research programs for undergraduate students.  We will select examples across the range of geophysical disciplines and from a variety of institutional settings. Speakers will present the perceived benefits derived from their programs, potential pitfalls, and suggestions about the ingredients that create successful experiences for undergraduate students.  This morning oral session will be followed by an afternoon poster session that showcases examples of research completed by undergraduate students.  Students must submit their  posters to a regular scientific theme session, as well as to the Showcase on Undergraduate Research poster session.
Conveners: Karen Grove, San Francisco State University, Department of Geosciences, San Francisco, CA 94132 USA, Tel: +1-415-338-2061, E-mail: kgrove@sfsu.edu; and Jill Singer, Buffalo State College, Department of Earth Sciences, Buffalo, NY 14222 USA, Tel: +1-716-878-6731, E-mail: singerjk@buffalostate.edu; and Roberta Johnson, UCAR/NCAR, UCAR Director of Education and Public Outreach, PO Box 3000, Boulder, CO 80307 USA, Tel: +1-303-497-2173, E-mail: rmjohnsn@ucar.edu

ED07 AGU Scientists' Roles and Partnerships in Support of K-12 Education and Public Outreach
Traditionally, the research directorates of funding agencies like NASA and NSF contribute substantively to training the next generation of scientists via fellowships and the support of graduates and postgraduates in their usual scientific roles on research proposals. In recent years, research directorates at NASA and NSF have been expanding their educational scope to address national needs for improving K-12 science education and enhancing general literacy in science, mathematics and technology. There is now a greater emphasis on the integration of research and education at all levels and on the involvement of NASA and NSF-supported scientists in partnership with K-12 education and public outreach (EPO) professionals.  This session is intended to showcase the diversity of roles scientists are playing in support of successful partnerships with the education and public outreach programs of research institutions and NASA missions, teachers, schools of education, school districts, museums, curriculum developers, educational radio and television, educational Web developers, and others.
Conveners: Cherilynn A. Morrow, Space Science Institute, Education and Public Outreach, 3100 Marine St., Suite A353, Boulder, CO 80303-1058 USA, Tel: +1-303-492-7321, Fax: +1-303-492-3789, E-mail: camorrow@spot.colorado.edu and Roberta Johnson, UCAR/NCAR, UCAR Director of Education and Public Outreach, PO Box 3000, Boulder, CO 80307 USA, Tel: +1-303-497-2173, E-mail: rmjohnsn@ucar.edu

Public Affairs

PA01 "Intelligent Design" a Challenge to Teaching Earth and Space Science?
The Earth and its environment in space represent a complex natural system. Proponents of a branch of creationism called "Intelligent Design (ID)" hold the view that an intelligent designer is the only explanation for irreducibly complex natural systems, and that the diversity and complexity of life on Earth could not have come about through natural selection over geologic time. ID supporters further demand that ID should be taught as a viable alternative to the theory of Darwinian evolution, claiming that the debate is between scientists, not whether ID represents a scientific way of explaining natural phenomena.  Speakers in this session will discuss the roots and ramifications of ID and whether ID has any bearing on how Earth and space scientists conduct their research. Because ID proponents endeavor to make their case to the public, the implications for the teaching of Earth and space science in public schools will be a consistent theme throughout the session.
Conveners: Peter Folger, American Geophysical Union, 2000 Florida Avenue, NW, Washington, DC 20009 USA, Tel: +1-202-777-7509, Fax: +1-202-328-0566, E-mail: pfolger@agu.org; and David Applegate, AGI, USA, E-mail: apple@agiweb.org

Public Affairs also presents jointly with the following Special Sessions:
B03 Biogeochemistry of Land Use Change  (Joint with GS, H, PA)
B04 Land Cover and Land Use Change: Implications for Resource Management (Joint with H, PA)
B05 Remote Sensing to Address the Needs of Local Communities  (Joint with G, H, PA)
B06 Contributions of Biogeosciences to the Millennium Ecosystem Assessment (Joint with PA)
B09 Mercury in the Environment (Joint with A, GS, H, PA)
B11 Linkages Between Biogeochemical and Hydrogeologic Processes in Shallow Ground-Water Systems of the Atlantic and Gulf Coastal Plains (Joint with H, PA)
S02 Challenges in Regional Seismic Nuclear Test-Ban Treaty Monitoring (Joint with PA)
 

Mineral and Rock Physics presents jointly with the following Special Sessions:
GP03 Paleomagnetic Puzzles, Rock Magnetic Riddles (Joint with MRP, M)
GP06 Banded Iron Formation, its Chemical and Physical Properties and Relation to the Origin of Life (Joint with B, MR, P, V, GS, M)
M01 Equation of State and Elasticity of Earth Materials (Joint with MR, SEDI, T, V)
M03 Spectroscopy of Minerals and Other Planetary Phases (Joint with MR, T)
S01 Core Mantle Boundary Region (Joint with GP, GS, MR, NG, SEDI, T)
S03 Integrated Models of Earth Structure and Evolution (ONLINE-only Session) (Joint with MR, SEDI, T, M)
T03 Computational Earth Laboratories (Joint with GP, M, MR, NG, S)
 

Nonlinear Geophysics

NG01 Recent Contributions of Nonlinear Science in Atmospheric Research: From Paradigm Shifts to Problem Solving (Joint with A)
Atmospheric processes have always inspired nonlinear scientists: Richardson’s eddy cascades, Lorenz’s attractor and the “butterfly” effect have become staples of nonlinearity; turbulence phenomenology was grounded in observations of atmospheric dispersion; fractal geometry is often invoked with clouds. Despite the frequently strong nonlinear component in atmospheric phenomena, many in AGU’s Atmospheric Sciences (A) Section feel they have not fully benefited from the tremendous progress of nonlinear science. This might be due partially to the nonlinear community’s propensity for abstraction and swift cross-disciplinary moves. This session, jointly sponsored by A and NG (Nonlinear Geophysics Technical Committee), aims to rectify that situation by offering an opportunity (1) for nonlinear experts to showcase the more applied aspects of their atmospherically-related work, and (2) for atmospheric scientists with little or no experience in nonlinear science to describe their least tractable problems. Research issues in “A” that are likely candidates for “NG-induced” breakthroughs typically cover many temporal and/or spatial scales, exhibit intermittent bursts, or may be plagued with quasi-singularities, poorly-explained amplitudes and/or frequencies of occurrence. These problems can stem from studies in weather, climate, chemistry, transport, pollution, etc. Possible applications of “NG” approaches to “A” problems are: sub-pixel variability effects in remote sensing; parameterizations of dynamical or radiative effects of unresolved structures in numerical models (with grid-scales now ranging from meters to hundreds of kilometers); or development of meaningful comparisons between coarsely-modeled atmospheric fields and quasi-point-wise in situ measurements. “NG” concepts we anticipate seeing at work here include chaos, self-organized criticality, cascade models, scale-invariance, (multi)fractals, power-law statistics, and kin, or else (or possibly combined with) new computational tools such as wavelet transforms, singular-spectrum analysis, machine-learning algorithms, and so on. We therefore solicit papers from and for a broad range of NG- and A-practitioners on outstanding or emerging problems addressed with or calling for these advanced techniques. However, because current nonlinear approaches are congruent with the inherent complexity of the atmosphere, we expect to see gains in physical insight as well as practical deliverables.
Conveners: Anthony Davis, Los Alamos National Laboratory, Space and Remote Sensing Sciences Group, PO Box 1663, MS C-323, Los Alamos, NM 87545 USA, Tel: +1-505-665-6577, Fax: +1-505-667-9208, E-mail: adavis@lanl.gov; and Lynn Sparling, NASA Goddard Space Flight Center, Code 916, Greenbelt, MD 20771 USA, Tel: +1-301-614-6009, Fax: +1-301-614-5903, E-mail: sparling@dynarama.gsfc.nasa.gov; and Klaus Pfeilsticker, University of Heidelberg, Institut fur Umweltphysik Im Neuenheimer Feld 36, Heidelberg, D-69120 Germany, Tel: +490-6221-546401, Fax: +490-6221-546405, E-mail: klaus.pfeilsticker@iup.uni-heidelberg.de; and Jun-Ichi Yano, Hamburg University, Meteorologisches Institut Bundesstrasse 55, Hamburg, D-20146 Germany, Tel: +49-040-42838-5071, Fax: +49-040-42838-5066, E-mail: yano@dkrz.de

NG02 Integrating and Applying Models, Simulations, and Data to the Forecasting of Nonlinear Geophysical Systems (Joint with H, T)
Many geophysical processes are nonlinear over wide ranges of time scales, resulting in complex spatial and temporal behaviors.  Examples include the ocean-atmosphere interface, fault networks, mantle convection, and solar activity.  Our understanding of such systems is complicated by the difficulty in acquiring complete and accurate data sets that span many time scales.  Yet many of these geophysical systems have significant economic, societal, and humanitarian impacts on regional and national scales. On the other hand, recent developments resulting in relatively inexpensive access to increasingly powerful computers have greatly improved the ability to analyze the available data, yielding important scientific insights. In addition, these computational advances have encouraged the development of advanced computer models and simulations designed specifically to aid in the understanding of these complex systems and the physical parameters which govern their activity.  These simulations can then be used to model the behavior of the system over time, and perhaps to forecast both the general physics of the system as well as its extreme events.  Applications include the El Nino Southern Oscillation, mantle convection, and biometrics.  The purpose of this session is to encourage papers which detail the integration of these simulations and the available data, and their application together in the modeling and forecasting of the behavior of geophysical systems.
Conveners: Kristy Tiampo, University of Colorado, CIRES CB 216, Boulder, CO 80309-0216 USA, Tel: +1-303-492-4779, E-mail: kristy@fractal.colorado.edu; and Seth Veitzer, University of Colorado, CIRES CB 216, Boulder, CO 80309-0216 USA, Tel: +1-303-492-8124, E-mail: veitzer@terra.colorado.edu

Nonlinear Geophysics also presents jointly with the following Special Sessions:
B02 Integrated Observations for the Biogeosciences (Joint with A, NG, OS)
B12 Eco-hydrological Dynamics of Water Controlled Ecosystems (Joint with H, NG)
B14 Land-Atmosphere Interactions (Joint with A, H, NG)
H05 Physicochemical Hydrodynamics of Nonaqueous Phase Liquid in Porous and Fractured Media (Joint with GS, NG)
H12 Computational Fluid Dynamics Applications to Rivers (Joint with NG)
H14 Geomorphology (POSTER ONLY) (Joint with NG)
H26 Lumped Versus Distributed Modeling: Issues in Real World Applications (Joint with NG)
S01 Core Mantle Boundary Region (Joint with GP, GS, MR, NG, SEDI, T)
SPD01 Nanoflare Statistics, Self-Organized Criticality, and Coronal Heating (Joint with NG, SH)
T03 Computational Earth Laboratories (Joint with GP, M, MR, NG, S)
 

Study of Earth's Deep Interior presents jointly with the following Special Sessions:
GP04 Fluctuations of the Earth's Magnetic Field (Direction and Intensity): From Paleosecular Variation to Reversals (Joint with SEDI)
M01 Equation of State and Elasticity of Earth Materials (Joint with MR, SEDI, T, V)
S01 Core Mantle Boundary Region (Joint with GP, GS, MR, NG, SEDI, T)
S03 Integrated Models of Earth Structure and Evolution (ONLINE-only Session) (Joint with MR, SEDI, T, M)
 

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