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      <title>This Week's Most Downloaded Articles</title>
      <link>http://www.agu.org/contents/journals/ViewPublishedToday.do</link>
      <description><![CDATA[]]></description>
      <language>en-us</language>
      <copyright>AGU</copyright>
      <docs>http://blogs.law.harvard.edu/tech/rss</docs>
      <webMaster>webmaster@agu.org</webMaster>
      <item>
         <title>Outline of Some Topics in Homogeneous Turbulent Flow</title>
         <link>http://dx.doi.org/10.1029/JZ064i012p02134</link>
         <description><![CDATA[Following general remarks on the homogeneous turbulence problem, and an indication of kinematic and dynamic relations in the isotropic case, outlines are given of the phenomena of spectral transfer and tendencies toward isotropy. A discussion of Reynolds numbers is followed by detailed comparisons of some characteristic lengths. There are, finally, an outline of some theories on spectral turbulent energy transfer and a mention of static pressure fluctuations.]]></description>
         <author>Stanley Corrsin</author>
         <category>Journal of Geophysical Research</category>
         <pubDate>64</pubDate>
      </item>
      <item>
         <title>Resolute Bay CADI ionosonde drifts, PolarDARN HF velocities, and cross polar cap potential</title>
         <link>http://dx.doi.org/10.1029/2011RS004947</link>
         <description><![CDATA[In this study, velocities measured by the Rankin Inlet and Inuvik PolarDARN HF radars over Resolute Bay (RB) are compared with measurements from the RB CADI ionosonde to investigate the consistency of the measurements. Two types of comparisons are performed: 1-D, where each PolarDARN radar line-of-sight velocity is plotted against CADI velocity projected onto appropriate radar beam, and 2-D, where the PolarDARN merged velocity is compared with the full CADI vector. In both cases, velocities were found to statistically agree. For the 1-D comparison, the velocities were comparable in ∼85% of cases. For the 2-D comparison, a minor tendency for larger PolarDARN merge velocities (∼60 m/s) was noticed. The second task performed is a comparison of the SuperDARN cross polar cap potential (CPCP) and the CADI-based CPCP and their dependence on the CADI velocity. Linear dependences were found allowing for inter-conversion between these parameters. For large plasma drifts, the SuperDARN CPCPs were found to be much smaller than the CADI-based CPCPs hinting that the separation between the foci of a large-scale convection pattern is often underestimated in the SuperDARN convection mapping.]]></description>
         <author>D. Mori, A. V. Koustov, P. T. Jayachandran and N. Nishitani</author>
         <category>Radio Science</category>
         <pubDate>47</pubDate>
      </item>
      <item>
         <title>Dissolved zinc in the subarctic North Pacific and Bering Sea: Its distribution, speciation, and importance to primary producers</title>
         <link>http://dx.doi.org/10.1029/2010GB004004</link>
         <description><![CDATA[The eastern subarctic North Pacific, an area of high nutrients and low chlorophyll, has been studied with respect to the potential for iron to control primary production. The geochemistry of zinc, a critical micronutrient for diatoms, is less well characterized. Total zinc concentrations and zinc speciation were measured in near-surface waters on transects across the subarctic North Pacific and across the Bering Sea. Total dissolved zinc concentrations in the near-surface ranged from 0.10 nmol L−1 to 1.15 nmol L−1 with lowest concentrations in the eastern portions of both the North Pacific and Bering Sea. Dissolved zinc speciation was dominated by complexation to strong organic ligands whose concentration ranged from 1.1 to 3.6 nmol L−1 with conditional stability constants (K′ZnL/Zn′) ranging from 109.3 to 1011.0. The importance of zinc to primary producers was evaluated by comparison to phytoplankton pigment concentrations and by performing a shipboard incubation. Zinc concentrations were positively correlated with two pigments that are characteristic of diatoms. At one station in the North Pacific, the addition of 0.75 nmol L−1 zinc resulted in a doubling of chlorophyll after 4 days.]]></description>
         <author>Rachel Wisniewski Jakuba, Mak A. Saito, James W. Moffett and Yan Xu</author>
         <category>Global Biogeochemical Cycles</category>
         <pubDate>26</pubDate>
      </item>
      <item>
         <title>ON ELECTRIC CURRENTS INDUCED BY ROTATING MAGNETS, AND THEIR APPLICATION TO SOME PHENOMENA OF TERRESTRIAL MAGNETISM</title>
         <link>http://dx.doi.org/10.1029/TM001i001p00001</link>
         <description/>
         <author>Arthur Schuster</author>
         <category>Terrestrial Magnetism</category>
         <pubDate>1</pubDate>
      </item>
      <item>
         <title>Monitoring glacier surface seismicity in time and space using Rayleigh waves</title>
         <link>http://dx.doi.org/10.1029/2011JF002259</link>
         <description><![CDATA[Sliding glaciers and brittle ice failure generate seismic body and surface wave energy characteristic to the source mechanism. Here we analyze continuous seismic recordings from an array of nine short-period passive seismometers located on Bench Glacier, Alaska (USA) (61.033°N, 145.687°W). We focus on the arrival-time and amplitude information of the dominant Rayleigh wave phase. Over a 46-hour period we detect thousands of events using a cross-correlation based event identification method. Travel-time inversion of a subset of events (7% of the total) defines an active crevasse, propagating more than 200 meters in three hours. From the Rayleigh wave amplitudes, we estimate the amount of volumetric opening along the crevasse as well as an average bulk attenuation (Q¯ = 42) for the ice in this part of the glacier. With the remaining icequake signals we establish a diurnal periodicity in seismicity, indicating that surface run-off and subglacial water pressure changes likely control the triggering of these surface events. Furthermore, we find that these events are too weak (i.e., too noisy) to locate individually. However, stacking individual events increases the signal-to-noise ratio of the waveforms, implying that these periodic sources are effectively stationary during the recording period.]]></description>
         <author>T. D. Mikesell, K. van Wijk, M. M. Haney, J. H. Bradford, H. P. Marshall and J. T. Harper</author>
         <category>Journal of Geophysical Research</category>
         <pubDate>117</pubDate>
      </item>
      <item>
         <title>DIE VERTEILUNG DES ERDMAGNETISCHEN POTENTIALS IN BEZUG AUF BELIEBIGE DURCHMESSER DER ERDE</title>
         <link>http://dx.doi.org/10.1029/TM001i001p00018</link>
         <description/>
         <author>Ad. Schmidt</author>
         <category>Terrestrial Magnetism</category>
         <pubDate>1</pubDate>
      </item>
      <item>
         <title>A Note on the Muskingum Flood-Routing Method</title>
         <link>http://dx.doi.org/10.1029/JZ064i008p01053</link>
         <description><![CDATA[An exact method of solution of the flood-routing equation, when the storage is a linear function of weighted inflow and outflow, is developed. This operation is shown to be equivalent to routing a multiple of the inflow through reservoir storage and subtracting the excess inflow. Modified coefficients for the Muskingum equation are developed which do not depend on the routing interval being small relative to K.]]></description>
         <author>J. E. Nash</author>
         <category>Journal of Geophysical Research</category>
         <pubDate>64</pubDate>
      </item>
      <item>
         <title>Impact of wildfire on the thermal behavior of northern peatlands: Observations and model simulations</title>
         <link>http://dx.doi.org/10.1029/2011JG001910</link>
         <description><![CDATA[Wildfire represents the single largest disturbance to the ecohydrological function of northern peatlands. Alterations to peatland thermal behavior as a result of wildfire will modify the carbon balance of these important long-term global carbon stores and regulate post-fire ecosystem recovery. We simulate the 3-D thermal behavior of a peatland that has been disturbed by wildfire to identify how changes in peat temperatures emerge from changes to the surface energy balance and peat thermal properties. Peat temperatures are simulated within two adjacent peatlands, one area having burned 4 years previously, the second which has been wildfire-free for 75 years. We demonstrate that there is only a small alteration to the thermal response in Sphagnum fuscum hummocks that are not severely burnt within the wildfire. In contrast, wildfire produces important changes to the energy balance of Sphagnum hollows. A large reduction in the latent heat flux post-fire increases surface temperatures by up to 30°C during daytime summer conditions. However, temperatures through the peat profile are insensitive to these increases in surface temperature. The low surface moisture content of near-surface peat insulates the profile from these higher temperatures and, at depths below 0.015 m, only small differences are identifiable between burned and unburned hollow temperatures. Nevertheless, we argue that these alterations to near-surface temperatures and evaporation rates likely substantially influence the thermal and hydrological conditions post-wildfire, impacting the peatland recovery.]]></description>
         <author>N. Kettridge, D. K. Thompson and J. M. Waddington</author>
         <category>Journal of Geophysical Research</category>
         <pubDate>117</pubDate>
      </item>
      <item>
         <title>Hydromagnetic Theory of Geomagnetic Storms</title>
         <link>http://dx.doi.org/10.1029/JZ064i012p02239</link>
         <description><![CDATA[A hydromagnetic theory is presented which explains the average characteristics of geomagnetic storms. The magnetic storm is caused by a sudden increase in the intensity of the solar wind. Stresses are then set up in the geomagnetic field by the solar plasma impinging upon the geomagnetic field and becoming trapped in it. These stresses, which are propagated to the earth as hydromagnetic waves, account for the observed average magnetic storm variations. The sudden commencement of the magnetic storm is due to a hydromagnetic wave generated by the impact of the solar plasma on the geomagnetic field. The initial phase of the magnetic storm, during which the magnetic field is above average intensity, is due to the increased solar wind pressure. During the initial phase, instability causes small plasma clouds to become imbedded in the magnetic field. They break up and diffuse into the magnetic field to form a belt of trapped particles from the sun (principally protons and electrons). The trapped protons set up stresses, mainly due to centrifugal force, which account for the main phase of the magnetic storm. The recovery from the main phase is attributed to the relief of the stress on the geomagnetic field by the transfer of the energy of the trapped protons to neutral hydrogen by means of ion-atom charge exchange. The correct recovery time for the magnetic storm is predicted from the measured cross section of the ion-atom charge-exchange process and the hydrogen density values around the earth deduced from the scattering of solar Lyman-α radiation.]]></description>
         <author>A. J. Dessler and E. N. Parker</author>
         <category>Journal of Geophysical Research</category>
         <pubDate>64</pubDate>
      </item>
      <item>
         <title>Changes in permeability caused by transient stresses: Field observations, experiments, and mechanisms</title>
         <link>http://dx.doi.org/10.1029/2011RG000382</link>
         <description><![CDATA[Oscillations in stress, such as those created by earthquakes, can increase permeability and fluid mobility in geologic media. In natural systems, strain amplitudes as small as 10−6 can increase discharge in streams and springs, change the water level in wells, and enhance production from petroleum reservoirs. Enhanced permeability typically recovers to prestimulated values over a period of months to years. Mechanisms that can change permeability at such small stresses include unblocking pores, either by breaking up permeability-limiting colloidal deposits or by mobilizing droplets and bubbles trapped in pores by capillary forces. The recovery time over which permeability returns to the prestimulated value is governed by the time to reblock pores, or for geochemical processes to seal pores. Monitoring permeability in geothermal systems where there is abundant seismicity, and the response of flow to local and regional earthquakes, would help test some of the proposed mechanisms and identify controls on permeability and its evolution.]]></description>
         <author>Michael Manga, Igor Beresnev, Emily E. Brodsky, Jean E. Elkhoury, Derek Elsworth, S. E. Ingebritsen, David C. Mays and Chi-Yuen Wang</author>
         <category>Reviews of Geophysics</category>
         <pubDate>50</pubDate>
      </item>
      <item>
         <title>Oceanic anoxic events and plankton evolution: Biotic response to tectonic forcing during the mid-Cretaceous</title>
         <link>http://dx.doi.org/10.1029/2001PA000623</link>
         <description><![CDATA[Mid-Cretaceous (Barremian-Turonian) plankton preserved in deep-sea marl, organic-rich shale, and pelagic carbonate hold an important record of how the marine biosphere responded to short- and long-term changes in the ocean-climate system. Oceanic anoxic events (OAEs) were short-lived episodes of organic carbon burial that are distinguished by their widespread distribution as discrete beds of black shale and/or pronounced carbon isotopic excursions. OAE1a in the early Aptian (∼120.5 Ma) and OAE2 at the Cenomanian/Turonian boundary (∼93.5 Ma) were global in their distribution and associated with heightened marine productivity. OAE1b spans the Aptian/Albian boundary (∼113–109 Ma) and represents a protracted interval of dysoxia with multiple discrete black shales across parts of Tethys (including Mexico), while OAE1d developed across eastern and western Tethys and in other locales during the latest Albian (∼99.5 Ma). Mineralized plankton experienced accelerated rates of speciation and extinction at or near the major Cretaceous OAEs, and strontium isotopic evidence suggests a possible link to times of rapid oceanic plateau formation and/or increased rates of ridge crest volcanism. Elevated levels of trace metals in OAE1a and OAE2 strata suggest that marine productivity may have been facilitated by increased availability of dissolved iron. The association of plankton turnover and carbon isotopic excursions with each of the major OAEs, despite the variable geographic distribution of black shale accumulation, points to widespread changes in the ocean-climate system. Ocean crust production and hydrothermal activity increased in the late Aptian. Faster spreading rates [and/or increased ridge length] drove a long-term (Albian–early Turonian) rise in sea level and CO2-induced global warming. Changes in ocean circulation, water column stratification, and nutrient partitioning lead to a reorganization of plankton community structure and widespread carbonate (chalk) deposition during the Late Cretaceous. We conclude that there were important linkages between submarine volcanism, plankton evolution, and the cycling of carbon through the marine biosphere.]]></description>
         <author>R. Mark Leckie, Timothy J. Bralower and Richard Cashman</author>
         <category>Paleoceanography</category>
         <pubDate>17</pubDate>
      </item>
      <item>
         <title>Rapid switches in subpolar North Atlantic hydrography and climate during the Last Interglacial (MIS 5e)</title>
         <link>http://dx.doi.org/10.1029/2011PA002244</link>
         <description><![CDATA[At the peak of the previous interglacial period, North Atlantic and subpolar climate shared many features in common with projections of our future climate, including warmer-than-present conditions and a diminished Greenland Ice Sheet (GIS). Here we portray changes in North Atlantic hydrography linked with Greenland climate during Marine Isotope Stage (MIS) 5e using (sub)centennially sampled records of planktonic foraminiferal isotopes and assemblage counts and ice-rafted debris counts, as well as modern analog technique and Mg/Ca-based paleothermometry. We use the core MD03-2664 recovered from a high accumulation rate site (∼34 cm/kyr) on the Eirik sediment drift (57°26.34′N, 48°36.35′W). The results indicate that surface waters off southern Greenland were ∼3–5°C warmer than today during early MIS 5e. These anomalously warm sea surface temperatures (SSTs) prevailed until the isotopic peak of MIS 5e when they were interrupted by a cooling event beginning at ∼126 kyr BP. This interglacial cooling event is followed by a gradual warming with SSTs subsequently plateauing just below early MIS 5e values. A planktonic δ18O minimum during the cooling event indicates that marked freshening of the surface waters accompanied the cooling. We suggest that switches in the subpolar gyre hydrography occurred during a warmer climate, involving regional changes in freshwater fluxes/balance and East Greenland Current influence in the study area. The nature of these hydrographic transitions suggests that they are most likely related to large-scale circulation dynamics, potentially amplified by GIS meltwater influences.]]></description>
         <author>Nil Irvalı, Ulysses S. Ninnemann, Eirik V. Galaasen, Yair Rosenthal, Dick Kroon, Delia W. Oppo, Helga F. Kleiven, Kate F. Darling and Catherine Kissel</author>
         <category>Paleoceanography</category>
         <pubDate>27</pubDate>
      </item>
      <item>
         <title>Thermal and albedo mapping of Mars during the Viking primary mission</title>
         <link>http://dx.doi.org/10.1029/JS082i028p04249</link>
         <description><![CDATA[Measurements of Martian emission and reflection reveal wide variations of surface properties and indicate the presence of a larger atmospheric contribution to the observed radiances than was anticipated. Temperatures observed during the Viking primary mission range from 130 to 290 K. Surface thermal inertias from 1.6 to 11×10−3 cal cm−2 s−1/2 K−1 are mapped, and they correlate with surficial geologic units. An equatorial map of bolometric albedo generally correlates with prior narrowband observations. These albedos range from 0.09 to 0.43; some regional brightenings are atmospheric in origin. The photometric behavior implies quasi-Lambertian surface reflectance plus a strongly forward-scattering atmosphere. Brightness temperatures at large emission angles are strongly influenced by atmospheric infrared opacity and by the presence of rocks on the surface. The correlation and grouping of albedo and thermal inertia indicate that there are two major components of Martian surface material, with bright regions having a fine particulate covering. Winter polar temperatures show spatial and temporal variations, suggesting variation of atmospheric composition; a strong atmospheric temperature inversion exists above the south polar cap during winter. Surface CO2 condensation may also occur locally near the equator before dawn. Rising temperatures before dawn in a region near Arsia Mons imply the presence of daily local water ice fogs.]]></description>
         <author>Hugh H. Kieffer, T. Z. Martin, Alan R. Peterfreund, Bruce M. Jakosky, Ellis D. Miner and Frank Don Palluconi</author>
         <category>Journal of Geophysical Research</category>
         <pubDate>82</pubDate>
      </item>
      <item>
         <title>Imaging of lunar surface maturity</title>
         <link>http://dx.doi.org/10.1029/1999JE001110</link>
         <description><![CDATA[The physical evolution of the lunar surface with exposure to the space environment is termed maturation, and maturity is the degree to which a particular lunar soil possesses quantitative characteristics consistent with that exposure. Several quantitative measures or indices of maturity have been proposed and employed, including the abundance of solar wind gas, abundance of various types of agglutinates, various measures of grain size, and Is/FeO. Among the changes attendant with space exposure are striking changes in the optical characteristics of soils. Mature lunar soils are dark red and exhibit reduced spectral contrast relative to immature soils. This paper presents an optical maturity index that quantifies the spectral effects of maturation. We show that this optical maturity index correlates with other maturity indices about as well as the accepted maturity indices correlate among themselves and is only weakly coupled to composition. The modest correlations among maturity indices suggest important controls on individual maturity indices other than age, uncorrelated variations in the rates of accumulation of individual indicators, or variations in depths over which indicators are emplaced. In addition to mixing, these effects conspire to reduce the equivalence of maturity and duration of surface exposure. Optical maturity illustrates some of these effects, showing that ejecta of large and small craters mature at different rates and that the interiors and ejecta of large craters exhibit systematically different optical maturities. The same or analogous effects are likely to influence other maturity indices.]]></description>
         <author>Paul G. Lucey, David T. Blewett, G. Jeffrey Taylor and B. Ray Hawke</author>
         <category>Journal of Geophysical Research</category>
         <pubDate>105</pubDate>
      </item>
      <item>
         <title>Effects of the Intermediate Principal Stress on the Failure of Limestone, Dolomite, and Glass at Different Temperatures and Strain Rates</title>
         <link>http://dx.doi.org/10.1029/JZ072i002p00611</link>
         <description><![CDATA[ Strength and ductility of ordinarily brittle substances are commonly observed to increase with mean pressure. However, since the pioneering work of von Kármán and of Böker fifty years ago, it has been recognized that the effects differ from compression (σ1 > σ2 = σ3) to extension (σ3 < σ2 = σ1) tests, where subscripts denote maximum, intermediate, and minimum principal (compressive) stresses. This difference has been ascribed to the influence of σ2, but, to our knowledge, it has not previously been quantitatively demonstrated. By subjecting jacketed cylinders to combined triaxial compression or extension and torsion, one can obtain relative values of σ2 that lie between the limits σ2 = σ1 and σ2 = σ3; in torsion alone σ2 lies midway between. The data from different types of test are conveniently compared by plotting octahedral stress τoct against mean pressure Pm             at fracture or yielding. Tests have been done at temperatures of 25 to 500°C, confining pressure to 10 kb, and different strain rates (10−4 to 10−7 per second) on 1- by 2-cm solid cylinders and 1.2- by 2.5-cm hollow cylinders (0.7-mm wall) of homogeneous, statistically Isotropic Solenhofen limestone, Blair dolomite, and glass. At strain rates near 10−4 per second at 25°C, the τoct versus Pm             curves for limestone are essentially linear and reflect brittle behavior at relatively low pressures. In compression, failure occurs by shear fracturing; in extension and torsion, tensile fracture dominates. The shear strength is dependent upon mean pressure but tensile breaking strength is not. At intermediate pressures the curves become concave toward the Pm             axis. This is associated with transitional behavior, faulting in all three types of test. This brittle-ductile transition occurs at 2.7 and 5.4 kb in compression and extension, respectively; in torsion it is near 4.0 kb. This strongly suggests that ductility is a linear function of the relative magnitude of the intermediate principal stress. At high pressures all curves tend to approach the same asymptote, τoct = constant. The results for dolomite and glass are similar. Increasing the temperature or decreasing the strain rate tends to lower the transition confining pressures for all states of stress. ]]></description>
         <author>John Handin, H. C. Heard and J. N. Magouirk</author>
         <category>Journal of Geophysical Research</category>
         <pubDate>72</pubDate>
      </item>
      <item>
         <title>The Low-Latitude Ionosphere Sensor Network: Initial results</title>
         <link>http://dx.doi.org/10.1029/2011RS004978</link>
         <description><![CDATA[The Low-Latitude Ionospheric Sensor Network (LISN) is a distributed observatory designed to nowcast the state and dynamics of the low-latitude ionosphere and to develop forecasts of the electric fields, densities, and equatorial spread F over the South American continent. The LISN observatory consists of three different types of instruments: GPS receivers, fluxgate magnetometers, and vertical incidence pulsed ionospheric radar (VIPIR) ionosondes. This report provides a succinct summary of recent observations obtained using the LISN GPS receivers and complemented with measurements from other instruments and GPS receivers that operate in South America. More specifically, the following are shown here: (1) observations of total electron content (TEC) enhancements that occur near local midnight, (2) maps of TEC perturbations associated with the passage of traveling ionospheric disturbances over South America, and (3) statistics of TEC depletions for 2 years of low solar activity. Near-midnight TEC enhancements consist of sudden increases in TEC that occur after sunset at low latitudes on 30% of the days. These TEC enhancements last for several hours and can have amplitudes between 1 and 50 TEC units. On 11–12 March 2011 the largest TEC enhancement was observed in South America at times when the Jicamarca incoherent scatter radar operated and observed peak densities above 106 el/cc at 300 km altitude. It is suggested that a combination of zonal electric fields and meridional neutral winds are able to redistribute the plasma along the field lines and create regions of enhanced TEC. Maps of TEC perturbations associated with the passage of gravity waves (GWs) over South America have been used to measure the phase velocity and direction of propagation of GWs. The large number of GPS receivers over South America has allowed us to record bubble events for every day during 2008 and 2009. It was found that the number of TEC depletion detections varies with a periodicity of 28 days. It is mentioned how these new observations and the installation of the last four VIPIR ionosondes will lead to new discoveries in the near future.]]></description>
         <author>C. E. Valladares and J. L. Chau</author>
         <category>Radio Science</category>
         <pubDate>47</pubDate>
      </item>
      <item>
         <title>Exceptional melt pond occurrence in the years 2007 and 2011 on the Arctic sea ice revealed from MODIS satellite data</title>
         <link>http://dx.doi.org/10.1029/2011JC007869</link>
         <description><![CDATA[Melt ponds contribute to the ice-albedo feedback as they reduce the surface albedo of sea ice, and hence accelerate the decay of Arctic sea ice. Here, we analyze the melt pond fraction, retrieved from the MODIS sensor for the years 2000–2011 to characterize the spatial and temporal evolution. A significant anomaly of the relative melt pond fraction at the beginning of the melt season in June 2007 is documented. This is followed by above-average values throughout the entire summer. In contrast, the increase of the relative melt pond fraction at the beginning of June 2011 is within average values, but from mid-June, relative melt pond fraction exhibits values up to two standard deviations above the mean values of 30 ± 1.2% which are even higher than in Summer 2007.]]></description>
         <author>Anja Rösel and Lars Kaleschke</author>
         <category>Journal of Geophysical Research</category>
         <pubDate>117</pubDate>
      </item>
      <item>
         <title>Correction to “Interannual variability of snowmelt in the Sierra Nevada and Rocky Mountains, United States: Examples from two alpine watersheds”</title>
         <link>http://dx.doi.org/10.1029/2012WR012168</link>
         <description/>
         <author>Steven M. Jepsen, Noah P. Molotch, Mark W. Williams, Karl E. Rittger and James O. Sickman</author>
         <category>Water Resources Research</category>
         <pubDate>48</pubDate>
      </item>
      <item>
         <title>Book Review: Opening Space Research: Dreams, Technology, and Scientific Discovery</title>
         <link>http://dx.doi.org/10.1029/2012SW000778</link>
         <description><![CDATA[In Opening Space Research: Dreams, Technology, and Scientific Discovery, George Ludwig takes the reader behind the scenes of space exploration in the 1950s. The well-known episodes in this history—such as the stories of Sputnik, Laika the cosmodog, and the founding of NASA—are here placed in the rich context of the scientific and technical goals that motivated Ludwig and his fellow researchers. Ludwig relates the personal experiences of the many engineers, physicists, and university students who made possible humanity’s first ventures into space.]]></description>
         <author>Gregory A. Good</author>
         <category>Space Weather: The International Journal of Research and Applications</category>
         <pubDate>10</pubDate>
      </item>
      <item>
         <title>Data assimilation of thermospheric mass density</title>
         <link>http://dx.doi.org/10.1029/2012SW000773</link>
         <description><![CDATA[Accurate modeling of thermospheric mass density variation is of foremost importance to low Earth orbital prediction. The accuracy of empirical neutral density models based on global indices for solar and geomagnetic activity is inherently limited by the resolution of these indices. Assimilative modeling is appealing, as it provides a means to systematically identify and correct the inconsistencies between model specification and observations. In this paper we present a practical assimilative mass density specification methodology that optimally combines the mass density prediction by the Coupled-Thermosphere-Ionosphere-Plasmasphere-electrodynamics (CTIPe) model with in-situ observations of neutral mass density by research satellites such as Challenging Minisatellite Payload (CHAMP) and Gravity Recovery and Climate Experiment (GRACE). The methodology yields an analysis of the global density according to Bayes's rule under the assumption of Gaussian prior and observation error distribution (namely, by using the Optimal Interpolation or Kalman Filter update formula). To make best use of under-sampled global neutral mass density observations, the background (prior) error covariance is built on the principal component analysis to represent the long-distance correlation effectively, with an adaptive capability by using the maximum-likelihood method. The neutral mass density specification at 400 km can be improved up to 50% beyond what has been attained by the CTIPe by assimilating CHAMP and GRACE density observations.]]></description>
         <author>Tomoko Matsuo, Mariangel Fedrizzi, Timothy J. Fuller-Rowell and Mihail V. Codrescu</author>
         <category>Space Weather: The International Journal of Research and Applications</category>
         <pubDate>10</pubDate>
      </item>
      <item>
         <title>Sediment sorting and transport by flash floods</title>
         <link>http://dx.doi.org/10.1029/2003JF000067</link>
         <description><![CDATA[Flash floods partition the sediment load of arid and semiarid watersheds into components that travel at different rates through the fluvial system and are deposited in characteristic settings. This paper examines sediment sorting and transport by flash floods within a small, sand-dominated alluvial valley in a semiarid environment, upper Los Alamos Canyon, New Mexico. Floods in the study area partition the sediment load into two distinct facies: a coarse-grained facies that travels near the channel bed and a fine-grained facies that travels in suspension. The particle size distributions of channel and floodplain deposits resemble the measured textures of the bed load and suspended load, respectively. Calculations predict that typical flows sort the load into the same two fractions observed in the field. Whereas the transport rate of the coarse fraction depends on flow transport capacity, transport of the fine fraction is controlled by its supply. The long-term discharge of both fractions is estimated by integrating instantaneous transport relationships over the probability distribution of flows. Over several decades the computed fluxes of the two fractions are approximately the same. Most of the load in both fractions is transported during small to moderate events that occur more than once per year. However, the two fractions are distinct because they are supplied by different sources, transported by different mechanisms, and stored in distinct locations in the valley floor. Sediment sorting by flash floods is an important mechanism in constructing floodplains and in determining the residence times of various particle size classes in alluvial valleys.]]></description>
         <author>Daniel V. Malmon, Steven L. Reneau and Thomas Dunne</author>
         <category>Journal of Geophysical Research</category>
         <pubDate>109</pubDate>
      </item>
      <item>
         <title>THE ALTITUDE OF THE AURORA ABOVE THE EARTH'S SURFACE</title>
         <link>http://dx.doi.org/10.1029/TM003i001p00005</link>
         <description/>
         <author>Cleveland Abbe</author>
         <category>Terrestrial Magnetism</category>
         <pubDate>3</pubDate>
      </item>
      <item>
         <title>A detailed paleomagnetic record between 2.1 and 2.75 Ma at IODP Site U1314 in the North Atlantic: Geomagnetic excursions and the Gauss-Matuyama transition</title>
         <link>http://dx.doi.org/10.1029/2012GC004080</link>
         <description><![CDATA[This study investigated the detailed geomagnetic field variation between 2.1 and 2.75 Ma from a sediment core (IODP Site U1314) with high sedimentation rate (≥10 cm/kyr) and good age control. Characteristic remanent magnetization directions were well resolved by stepwise alternating field demagnetization. As a proxy of relative paleointensity, natural remanent magnetization (NRM) normalized by anhysteretic remanent magnetization (ARM) was used after testing that the influence of magnetic interaction in ARM is negligible. As a result, the following features of the geomagnetic field in the studied period have been revealed. During the transition of the Gauss-Matuyama (G-M) reversal and the Réunion Subchron, the paleointensity decreased to the value lower than 20% of the average intensity in the whole studied interval. In addition to these lows, eight paleointensity lows were found associated with large directional changes that satisfy the definition of a geomagnetic excursion. Four of these have ages close to ages reported for geomagnetic excursions in prior studies, whereas the other four excursions have not previously been observed. In our results, we confirm that the G-M transition occurred in marine isotope stage 103 even if we consider the shift in depth due to the lock-in process of magnetic particles. The temporal variation in paleointensity showed asymmetric behavior associated with the G-M transition, with a gradual decrease prior to the transition and a rapid recovery after the transition.]]></description>
         <author>Masao Ohno, Tatsuya Hayashi, Fumiki Komatsu, Fumi Murakami, Meng Zhao, Yohan Guyodo, Gary Acton, Helen F. Evans and Toshiya Kanamatsu</author>
         <category>Geochemistry Geophysics Geosystems</category>
         <pubDate>13</pubDate>
      </item>
      <item>
         <title>Meteorological results from the surface of Mars: Viking 1 and 2</title>
         <link>http://dx.doi.org/10.1029/JS082i028p04559</link>
         <description><![CDATA[We deal here primarily with the surface meteorological data for both Viking landers during the nominal missions (44 sols for lander 1 and 61 sols for lander 2). The diurnal patterns of wind, temperature, and pressure were strongly similar from sol to sol, as was expected in the summer. The chief characteristics of the wind data are that winds were light (a few meters per second), with a complex hodograph at VL-1 dominated by counterclockwise turning of the wind and a simpler hodograph at VL-2 marked by clockwise turning of the wind. This repetitive pattern of wind has begun to break down at VL-2 with advancing season, and several episodes of protracted northeasterly winds have occurred. Some of these are associated with lower than normal temperatures. Examples are given of wind and temperature traces over short periods, illustrating the effects of convection, static stability, and lander interference. We present a theoretical argument based upon the horizontal scale dictated by heating of slopes and upon vertical mixing of momentum to explain the different sense of rotation of the wind vectors at the two sites. Analysis of the semidiurnal pressure oscillation suggests that absorption of solar radiation is an important thermal drive but that convective heat flux from the surface is also significant. The seasonal variation of pressure extending past the end of the nominal missions shows a decrease of pressure to a minimum at Ls ≈ 149° with a rapid rise thereafter. This is clearly due to condensation and sublimation of CO2 on and from the southern polar cap.]]></description>
         <author>S. L. Hess, R. M. Henry, C. B. Leovy, J. A. Ryan and J. E. Tillman</author>
         <category>Journal of Geophysical Research</category>
         <pubDate>82</pubDate>
      </item>
      <item>
         <title>Monitoring seismic velocity change caused by the 2011 Tohoku-oki earthquake using ambient noise records</title>
         <link>http://dx.doi.org/10.1029/2012GL051405</link>
         <description><![CDATA[We estimated the changes in seismic velocity in the southern Tohoku district of Japan during the six-month period centered on the 11 March 2011 Tohoku-oki earthquake, using scattered waves retrieved by autocorrelation of ambient seismic noise. The estimated velocity decrease after the earthquake, and after two large aftershocks in the study area, was as great as 1.5% in the area nearest to the mainshock. The velocity changes displayed gradual healing. The spatial distribution of the velocity change showed a correlation with both the changes in static strain, derived from GPS records, and the peak particle velocity experienced during the three earthquakes, derived from strong-motion records. Therefore, our results show that velocity changes possibly contain information from deep in the crust bearing on coseismic stress release, in addition to shallower effects due to strong ground motion.]]></description>
         <author>Shohei Minato, Takeshi Tsuji, Shiro Ohmi and Toshifumi Matsuoka</author>
         <category>Geophysical Research Letters</category>
         <pubDate>39</pubDate>
      </item>
      <item>
         <title>Modeling the carbon fluxes of the northwest European continental shelf: Validation and budgets</title>
         <link>http://dx.doi.org/10.1029/2011JC007402</link>
         <description><![CDATA[Carbon budgets are simulated for the northwest European continental shelf and adjacent regions of the northeast Atlantic. Both physical and biological processes are evaluated, including exchanges between the water column and the atmosphere and sea bed. We use a multi-year simulation of a coupled 3D hydrodynamics-ecosystem model (POLCOMS-ERSEM) driven by realistic atmospheric data, ocean boundary conditions and freshwater inputs for 1989 to 2004. The northeast Atlantic (20°W to 13°E, 40°N to 65°N), including the European shelf, is found to be a net sink for atmospheric CO2. Biological processes exert a stronger control over pCO2 than temperature, and hence have a stronger effect on the air-sea CO2 exchange. For the European shelf, carbon sources of rivers and the uptake of atmospheric CO2 are balanced by horizontal transport off shelf and there is little carbon burial. There is net transport of carbon onto the shelf in the top 180 m of the water column and off the shelf below that depth, with a net carbon loss of ∼6 ± 1 × 1012 mol C yr−1. Up to 50% of the carbon exported from the shelf is transported below the permanent pycnocline and so is isolated from release into the atmosphere on centennial timescales.]]></description>
         <author>S. L. Wakelin, J. T. Holt, J. C. Blackford, J. I. Allen, M. Butenschön and Y. Artioli</author>
         <category>Journal of Geophysical Research</category>
         <pubDate>117</pubDate>
      </item>
      <item>
         <title>Evaluating the “critical relative humidity” as a measure of subgrid-scale variability of humidity in general circulation model cloud cover parameterizations using satellite data</title>
         <link>http://dx.doi.org/10.1029/2012JD017495</link>
         <description><![CDATA[A simple way to diagnose fractional cloud cover in general circulation models is to relate it to the simulated relative humidity, and allowing for fractional cloud cover above a “critical relative humidity” of less than 100%. In the formulation chosen here, this is equivalent to assuming a uniform “top-hat” distribution of subgrid-scale total water content with a variance related to saturation. Critical relative humidity has frequently been treated as a “tunable” constant, yet it is an observable. Here, this parameter, and its spatial distribution, is examined from Atmospheric Infrared Sounder (AIRS) satellite retrievals, and from a combination of relative humidity from the ECMWF Re-Analyses (ERA-Interim) and cloud fraction obtained from CALIPSO lidar satellite data. These observational data are used to evaluate results from different simulations with the ECHAM general circulation model (GCM). In sensitivity studies, a cloud feedback parameter is analyzed from simulations applying the original parameter choice, and applying parameter choices guided by the satellite data. Model sensitivity studies applying parameters adjusted to match the observations show larger positive cloud-climate feedbacks, increasing by up to 30% compared to the standard simulation.]]></description>
         <author>Johannes Quaas</author>
         <category>Journal of Geophysical Research</category>
         <pubDate>117</pubDate>
      </item>
      <item>
         <title>Field measurement of upper ocean turbulence dissipation associated with wave-turbulence interaction in the South China Sea</title>
         <link>http://dx.doi.org/10.1029/2011JC007806</link>
         <description><![CDATA[The turbulence dissipation rate within the mixed layer was measured in the open ocean and the coastal water of the South China Sea under moderate winds of 4.7 ∼ 8.9 m s−1 using a free-falling MSS profiler. In the open ocean, the profile of the dissipation rate within the mixed layer exhibited an exponential decay with the depth at most stations, which was satisfactorily consistent with that predicted by the parameterization of wave-turbulence interaction presented by Huang and Qiao (2010) while deviating from that by the law of the wall. In the coastal ocean, however, both the parameterization of wave-turbulence interaction and the law of the wall can give approximate predictions to the measured dissipation rate.]]></description>
         <author>Chuan Jiang Huang, Fangli Qiao, Dejun Dai, Hongyu Ma and Jingsong Guo</author>
         <category>Journal of Geophysical Research</category>
         <pubDate>117</pubDate>
      </item>
      <item>
         <title>Numerical simulations of the ionosphere of Mars during a solar flare</title>
         <link>http://dx.doi.org/10.1029/2011JA017399</link>
         <description><![CDATA[Electron densities in planetary ionospheres increase substantially during solar flares in response to the increased solar irradiance at soft X-ray and extreme ultraviolet wavelengths. Here we modify an existing model of the ionosphere of Mars to incorporate time-dependent solar irradiances and use it to simulate ionospheric conditions during the X14.4 and M7.8 solar flares of 15 and 26 April 2001, respectively. Simulations were validated by comparison to Mars Global Surveyor radio occultation measurements of vertical profiles of ionospheric electron density. Adjustments to the model's representation of the neutral atmosphere were required to adequately reproduce the observations before and during these solar flares. An accurate representation of electron-impact ionization, an important process in the lower ionosphere of Mars, is required in order to adequately simulate the doubling of electron densities that can occur in the lower ionosphere of Mars during a solar flare. We used the W-value representation of electron-impact ionization, in which the number of ion-electron pairs created per photon absorbed equals the ratio of the difference between photon energy and the ionization potential of carbon dioxide to the W-value. A range of possible W-values for Mars have been suggested in the literature, and a value of 28 eV led to the best reproduction of flare-affected observations. Simulated enhancements in the electron density are largest and persist the longest in the M1 region. We predict that the peak electron density in the M1 region can exceed that of the M2 region for short periods during intense solar flares.]]></description>
         <author>Anthony Lollo, Paul Withers, Kathryn Fallows, Zachary Girazian, Majd Matta and P. C. Chamberlin</author>
         <category>Journal of Geophysical Research</category>
         <pubDate>117</pubDate>
      </item>
      <item>
         <title>First simultaneous measurement of vertical air velocity, particle fall velocity, and hydrometeor sphericity in stratiform precipitation: Results from 47 MHz wind-profiling radar and 532 nm polarization lidar observations</title>
         <link>http://dx.doi.org/10.1029/2011RS004823</link>
         <description><![CDATA[Results from simultaneous measurements of vertical air velocity (W), particle fall velocity, and hydrometeor sphericity in stratiform precipitation are reported for the first time. Cases of stratiform precipitation on 8 (case A) and 16 December 2008 (case B) observed at Sumatra, Indonesia (0.2°S, 100.32°E), are described. A 47 MHz wind-profiling radar measured W and reflectivity-weighted particle fall velocity relative to the air (VZ) simultaneously. Upward W above ∼6.0 km altitude in case B (>0.2 m s−1) was greater than in case A (<0.1 m s−1). VZ at 300 m above the 0°C altitude in case B (1.8 m s−1) was greater than in case A (1.3 m s−1). The thickness of melting layer (ML) in case B (900 m) was greater than in case A (300 m). Because the large-sized aggregates contribute to produce greater VZ and thicker ML, it is likely that entangled growth of dendritic crystals under the presence of significant upward W and enhanced aggregation occurrence by the well-developed dendritic crystals produced the large-sized aggregates. Lidar measured an increase of linear depolarization ratio (δ) and lidar dark band in the ML. Volume δ of raindrops was 0.08–0.10 in case B and close to zero in case A. Stronger multiple scattering in case B is likely a cause that produced the greater δ. In case B, a dip of δ was measured at the bottom of ML. The decrease of hydrometeor nonsphericity at the final stage of melting explains the dip.]]></description>
         <author>Tomoaki Mega, Masayuki K. Yamamoto, Makoto Abo, Yasukuni Shibata, Hiroyuki Hashiguchi, Noriyuki Nishi, Toyoshi Shimomai, Yoshiaki Shibagaki, Mamoru Yamamoto, Manabu D. Yamanaka, Shoichiro Fukao and Timbul Manik</author>
         <category>Radio Science</category>
         <pubDate>47</pubDate>
      </item>
      <item>
         <title>Catchment hydrological responses to forest harvest amount and spatial pattern</title>
         <link>http://dx.doi.org/10.1029/2010WR010165</link>
         <description><![CDATA[Forest harvest effects on streamflow generation have been well described experimentally, but a clear understanding of process-level hydrological controls can be difficult to ascertain from data alone. We apply a new model, Visualizing Ecosystems for Land Management Assessments (VELMA), to elucidate how hillslope and catchment-scale processes control stream discharge in a small Pacific Northwest catchment. VELMA is a spatially distributed ecohydrology model that links hydrological and biogeochemical processes within watersheds. The study site is WS10 of the H.J. Andrews LTER, a 10 ha forested catchment clearcut in 1975. Simulated and observed daily streamflow are in good agreement for both the pre- (1969–1974) and postharvest (1975–2008) periods (Nash-Sutcliffe efficiency = 0.807 and 0.819, respectively). One hundred scenarios, where harvest amounts ranged from 2% to 100% were conducted. Results show that (1) for the case of a 100% clearcut, stream discharge initially increased by ∼29% or 345 mm but returned to preclearcut levels within 50 years, and (2) annual streamflow increased at a near linear rate of 3.5 mm year−1 for each percent of catchment harvested, irrespective of location. Thereafter, to assess the impact of harvest location on stream discharge, 20 harvest scenarios were simulated, where harvest amount was fixed at 20% but harvest location varied. Results show that the streamflow response is strongly sensitive to harvest distance from the stream channel. Specifically, a 20% clearcut area near the catchment divide resulted in an average annual streamflow increase of 53 mm, whereas a 20% clearcut near the stream resulted in an average annual streamflow increase of 92 mm.]]></description>
         <author>Alex Abdelnour, Marc Stieglitz, Feifei Pan and Robert McKane</author>
         <category>Water Resources Research</category>
         <pubDate>47</pubDate>
      </item>
      <item>
         <title>A new global database of Mars impact craters ≥1 km: 1. Database creation, properties, and parameters</title>
         <link>http://dx.doi.org/10.1029/2011JE003966</link>
         <description><![CDATA[Impact craters have been used as a standard metric for a plethora of planetary applications for many decades, including age-dating, geologic mapping and stratigraphic relationships, as tracers for surface processes, and as locations for sampling lower crust and upper mantle material. Utilizing craters for these and other investigations is significantly aided by a uniform catalog of craters across the surface of interest. Consequently, catalogs of craters have been developed for decades for the Moon and other planets. We present a new global catalog of Martian craters statistically complete to diameters D ≥ 1 km. It contains 384,343 craters, and for each crater it lists detailed positional, interior morphologic, ejecta morphologic and morphometric data, and modification state information if it could be determined. In this paper, we detail how the database was created, the different fields assigned, and statistical uncertainties and checks. In our companion paper (Robbins and Hynek, 2012), we discuss the first broad science applications and results of this work.]]></description>
         <author>Stuart J. Robbins and Brian M. Hynek</author>
         <category>Journal of Geophysical Research</category>
         <pubDate>117</pubDate>
      </item>
      <item>
         <title>Strike-slip tectonics and Quaternary basin formation along the Vienna Basin fault system inferred from Bouguer gravity derivatives</title>
         <link>http://dx.doi.org/10.1029/2011TC002979</link>
         <description><![CDATA[The Vienna Basin at the transition between the Alpine and Carpathian belt hosts a number of large Pleistocene sub-basins forming along an active continental scale strike-slip fault (Vienna Basin strike-slip fault). We utilize first-order derivatives from industrial Bouguer gravity data to unravel the impacts of Pleistocene kinematics on the Vienna Basin and to compensate for the lack of near-surface fault data. Anomalies have been evaluated by independent geophysical and geological data and were integrated to build up a tectonic model. Factors influencing the wavelength and the amplitude of anomalies were additionally investigated by 2-D models to better interpret field data. Subsidence and related accumulation of Quaternary sediments in the Vienna Basin produce significant gravity signals related to the activity of the strike-slip fault. The constrained fault patterns and structures highlight tight and elongated transtensional pull-apart basins with typically associated features like separated depocenters and Riedel fractured sidewalls in an en-echelon alignment. Further Pleistocene basins are highlighted as tectonic grabens developing along branches of the master fault. The Vienna Basin is additionally affected by minor deformation represented by both subsidence along major Miocene sidewalls and NW-SE faulting resulting in distinct topographic features, which manifests kinematics on a regional scale. The clear density contrasts between Miocene marine and Quaternary terrestrial sediments, as well as the exceptional database, provide a unique framework to demonstrate advantages of incorporating gravity derivatives for near-surface fault analysis.]]></description>
         <author>B. C. Salcher, B. Meurers, J. Smit, K. Decker, M. Hölzel and M. Wagreich</author>
         <category>Tectonics</category>
         <pubDate>31</pubDate>
      </item>
      <item>
         <title>Impact of aerosols on convective clouds and precipitation</title>
         <link>http://dx.doi.org/10.1029/2011RG000369</link>
         <description><![CDATA[Aerosols are a critical factor in the atmospheric hydrological cycle and radiation budget. As a major agent for clouds to form and a significant attenuator of solar radiation, aerosols affect climate in several ways. Current research suggests that aerosol effects on clouds could further extend to precipitation, both through the formation of cloud particles and by exerting persistent radiative forcing on the climate system that disturbs dynamics. However, the various mechanisms behind these effects, in particular, the ones connected to precipitation, are not yet well understood. The atmospheric and climate communities have long been working to gain a better grasp of these critical effects and hence to reduce the significant uncertainties in climate prediction resulting from such a lack of adequate knowledge. Here we review past efforts and summarize our current understanding of the effect of aerosols on convective precipitation processes from theoretical analysis of microphysics, observational evidence, and a range of numerical model simulations. In addition, the discrepancies between results simulated by models, as well as those between simulations and observations, are presented. Specifically, this paper addresses the following topics: (1) fundamental theories of aerosol effects on microphysics and precipitation processes, (2) observational evidence of the effect of aerosols on precipitation processes, (3) signatures of the aerosol impact on precipitation from large-scale analyses, (4) results from cloud-resolving model simulations, and (5) results from large-scale numerical model simulations. Finally, several future research directions for gaining a better understanding of aerosol-cloud-precipitation interactions are suggested.]]></description>
         <author>Wei-Kuo Tao, Jen-Ping Chen, Zhanqing Li, Chien Wang and Chidong Zhang</author>
         <category>Reviews of Geophysics</category>
         <pubDate>50</pubDate>
      </item>
      <item>
         <title>Validation and comparison of two soil-vegetation-atmosphere transfer models for tropical Africa</title>
         <link>http://dx.doi.org/10.1029/2011JG001802</link>
         <description><![CDATA[This study aims to compare and validate two soil-vegetation-atmosphere-transfer (SVAT) schemes: TERRA-ML and the Community Land Model (CLM). Both SVAT schemes are run in standalone mode (decoupled from an atmospheric model) and forced with meteorological in-situ measurements obtained at several tropical African sites. Model performance is quantified by comparing simulated sensible and latent heat fluxes with eddy-covariance measurements. Our analysis indicates that the Community Land Model corresponds more closely to the micrometeorological observations, reflecting the advantages of the higher model complexity and physical realism. Deficiencies in TERRA-ML are addressed and its performance is improved: (1) adjusting input data (root depth) to region-specific values (tropical evergreen forest) resolves dry-season underestimation of evapotranspiration; (2) adjusting the leaf area index and albedo (depending on hard-coded model constants) resolves overestimations of both latent and sensible heat fluxes; and (3) an unrealistic flux partitioning caused by overestimated superficial water contents is reduced by adjusting the hydraulic conductivity parameterization. CLM is by default more versatile in its global application on different vegetation types and climates. On the other hand, with its lower degree of complexity, TERRA-ML is much less computationally demanding, which leads to faster calculation times in a coupled climate simulation.]]></description>
         <author>T. Akkermans, D. Lauwaet, M. Demuzere, G. Vogel, Y. Nouvellon, J. Ardö, B. Caquet, A. De Grandcourt, L. Merbold, W. Kutsch and N. Van Lipzig</author>
         <category>Journal of Geophysical Research</category>
         <pubDate>117</pubDate>
      </item>
      <item>
         <title>World ocean heat content and thermosteric sea level change (0–2000 m), 1955–2010</title>
         <link>http://dx.doi.org/10.1029/2012GL051106</link>
         <description><![CDATA[We provide updated estimates of the change of ocean heat content and the thermosteric component of sea level change of the 0–700 and 0–2000 m layers of the World Ocean for 1955–2010. Our estimates are based on historical data not previously available, additional modern data, and bathythermograph data corrected for instrumental biases. We have also used Argo data corrected by the Argo DAC if available and used uncorrected Argo data if no corrections were available at the time we downloaded the Argo data. The heat content of the World Ocean for the 0–2000 m layer increased by 24.0 ± 1.9 × 1022 J (±2S.E.) corresponding to a rate of 0.39 W m−2 (per unit area of the World Ocean) and a volume mean warming of 0.09°C. This warming corresponds to a rate of 0.27 W m−2 per unit area of earth's surface. The heat content of the World Ocean for the 0–700 m layer increased by 16.7 ± 1.6 × 1022 J corresponding to a rate of 0.27 W m−2 (per unit area of the World Ocean) and a volume mean warming of 0.18°C. The World Ocean accounts for approximately 93% of the warming of the earth system that has occurred since 1955. The 700–2000 m ocean layer accounted for approximately one-third of the warming of the 0–2000 m layer of the World Ocean. The thermosteric component of sea level trend was 0.54 ± .05 mm yr−1 for the 0–2000 m layer and 0.41 ± .04 mm yr−1 for the 0–700 m layer of the World Ocean for 1955–2010.]]></description>
         <author>S. Levitus, J. I. Antonov, T. P. Boyer, O. K. Baranova, H. E. Garcia, R. A. Locarnini, A. V. Mishonov, J. R. Reagan, D. Seidov, E. S. Yarosh and M. M. Zweng</author>
         <category>Geophysical Research Letters</category>
         <pubDate>39</pubDate>
      </item>
      <item>
         <title>Flow and transport effects of compaction bands in sandstone at scales relevant to aquifer and reservoir management</title>
         <link>http://dx.doi.org/10.1029/2005WR004664</link>
         <description><![CDATA[Thin, tabular, low-porosity, low-permeability compaction bands form pervasive, subparallel, anastomosing arrays that extend over square kilometers of exposure in the Aztec Sandstone of southeastern Nevada, an exhumed analog for active aquifers and reservoirs. In order to examine the potential flow and transport effects of these band arrays at scales relevant to production and management, we performed a suite of simulations using an innovative discrete-feature modeling technique to capture the exact pattern of compaction bands mapped over some 150,000 m2 of contiguous outcrop. Significant impacts related to the presence of the bands and their dominant trend are apparent: the average pressure drop required to drive flow between wells exceeds that for band-free sandstone by a factor of three and is 10% to 50% higher across the bands versus along them; reservoir production efficiency varies up to 56% for a typical five-spot well array, depending on its orientation relative to the dominant band trend; and contaminant transport away from a point source within an aquifer tends to channel along the bands, regardless of the regional gradient direction. We conclude that accounting for the flow effects of similar compaction-band arrays would prove essential for optimal management of those sandstone aquifers and reservoirs in which they occur.]]></description>
         <author>K. R. Sternlof, M. Karimi-Fard, D. D. Pollard and L. J. Durlofsky</author>
         <category>Water Resources Research</category>
         <pubDate>42</pubDate>
      </item>
      <item>
         <title>Detection of Rossby wave breaking and its response to shifts of the midlatitude jet with climate change</title>
         <link>http://dx.doi.org/10.1029/2012JD017469</link>
         <description><![CDATA[A Rossby wave breaking identification method is presented which searches for overturning of absolute vorticity contours on pressure surfaces. The results are compared to those from an analysis of isentropic potential vorticity, and it is demonstrated that both yield similar wave breaking distributions. As absolute vorticity is easily obtained from most model output, we present wave breaking frequency distributions from the ERA-Interim data set, thirteen general circulation models (GCMs) and a barotropic model. We demonstrate that a poleward shift of the Southern Hemisphere midlatitude jet is accompanied by a decrease in poleward wave breaking in both the barotropic model and all GCMs across multiple climate forcing scenarios. In addition, it is shown that while anticyclonic wave breaking shifts poleward with the jet, cyclonic wave breaking shifts less than half as much and reaches a poleward limit near 60 degrees S. Comparison of the observed distribution of Southern Hemisphere wave breaking with those from the GCMs suggests that wave breaking on the poleward flank of the jet has already reached its poleward limit and will likely become less frequent if the jet migrates any further poleward with climate change.]]></description>
         <author>Elizabeth A. Barnes and Dennis L. Hartmann</author>
         <category>Journal of Geophysical Research</category>
         <pubDate>117</pubDate>
      </item>
      <item>
         <title>Martian impact craters and emplacement of ejecta by surface flow</title>
         <link>http://dx.doi.org/10.1029/JS082i028p04055</link>
         <description><![CDATA[Several types of Martian impact craters have been recognized. The most common type, the rampart crater, is distinctively different from lunar and Mercurian craters. It is typically surrounded by several layers of ejecta, each having a low ridge or escarpment at its outer edge. Outward flow of ejecta along the ground after ballistic deposition is suggested by flow lines around obstacles, the absence of ejecta on top and on the lee side of obstacles, and the large radial distance to which continuous ejecta is found. The peculiar flow characteristics of the ejecta around these craters are tentatively attributed to entrained gases or to contained water, either liquid or vapor, in the ejecta as a result of impact melting of ground ice. Ejecta of other craters lacks flow features but has a marked radial pattern; ejecta of still other craters has patterns that resemble those around lunar and Mercurian craters. The internal features of Martian craters, in general, resemble their lunar and Mercurian counterparts except that the transition from bowl shaped to flat floored takes place at about 5-km diameter, a smaller size than is true for Mercury or the moon.]]></description>
         <author>M. H. Carr, L. S. Crumpler, J. A. Cutts, R. Greeley, J. E. Guest and H. Masursky</author>
         <category>Journal of Geophysical Research</category>
         <pubDate>82</pubDate>
      </item>
      <item>
         <title>Effect of point bar development on the local force balance governing flow in a simple, meandering gravel bed river</title>
         <link>http://dx.doi.org/10.1029/2010JF001838</link>
         <description><![CDATA[The patterns of depth, velocity, and shear stress that direct a river's morphologic evolution are governed by a balance of forces. Analyzing these forces, associated with pressure gradients, boundary friction, channel curvature, and along- and across-stream changes in fluid momentum driven by bed topography, can yield insight regarding the establishment and maintenance of stable channel forms. This study examined how components of the local force balance changed as a meandering channel evolved from a simple, flat-bedded initial condition to a more complex bar-pool morphology. A numerical flow model, constrained by measurements of velocity and water surface elevation, characterized the flow field for four time periods bracketing two floods. For each time increment, runs were performed for discharges up to bankfull, and individual force balance components were computed from model output. Formation and growth of point bars enhanced topographic steering effects, which were of similar magnitude to the pressure gradient and centrifugal forces. Convective accelerations induced by the bar reduced the cross-stream pressure gradient, intensified flow toward the outer bank, and routed sediment around the upstream end of the bar. Adjustments in the flow field thus served to balance streamwise transport along the inner bank onto the bar and cross-stream transport into the pool. Even in the early stages of bar development, topographically driven spatial gradients in velocity played a significant role in the force balance at flows up to bankfull, altering the orientation of the shear stress and sediment transport to drive bar growth.]]></description>
         <author>C. J. Legleiter, L. R. Harrison and T. Dunne</author>
         <category>Journal of Geophysical Research</category>
         <pubDate>116</pubDate>
      </item>
      <item>
         <title>Volcanic eruptions and climate</title>
         <link>http://dx.doi.org/10.1029/1998RG000054</link>
         <description><![CDATA[ Volcanic eruptions are an important natural cause of climate change on many timescales. A new capability to predict the climatic response to a large tropical eruption for the succeeding 2 years will prove valuable to society. In addition, to detect and attribute anthropogenic influences on climate, including effects of greenhouse gases, aerosols, and ozone-depleting chemicals, it is crucial to quantify the natural fluctuations so as to separate them from anthropogenic fluctuations in the climate record. Studying the responses of climate to volcanic eruptions also helps us to better understand important radiative and dynamical processes that respond in the climate system to both natural and anthropogenic forcings. Furthermore, modeling the effects of volcanic eruptions helps us to improve climate models that are needed to study anthropogenic effects. Large volcanic eruptions inject sulfur gases into the stratosphere, which convert to sulfate aerosols with an e-folding residence time of about 1 year. Large ash particles fall out much quicker. The radiative and chemical effects of this aerosol cloud produce responses in the climate system. By scattering some solar radiation back to space, the aerosols cool the surface, but by absorbing both solar and terrestrial radiation, the aerosol layer heats the stratosphere. For a tropical eruption this heating is larger in the tropics than in the high latitudes, producing an enhanced pole-to-equator temperature gradient, especially in winter. In the Northern Hemisphere winter this enhanced gradient produces a stronger polar vortex, and this stronger jet stream produces a characteristic stationary wave pattern of tropospheric circulation, resulting in winter warming of Northern Hemisphere continents. This indirect advective effect on temperature is stronger than the radiative cooling effect that dominates at lower latitudes and in the summer. The volcanic aerosols also serve as surfaces for heterogeneous chemical reactions that destroy stratospheric ozone, which lowers ultraviolet absorption and reduces the radiative heating in the lower stratosphere, but the net effect is still heating. Because this chemical effect depends on the presence of anthropogenic chlorine, it has only become important in recent decades. For a few days after an eruption the amplitude of the diurnal cycle of surface air temperature is reduced under the cloud. On a much longer timescale, volcanic effects played a large role in interdecadal climate change of the Little Ice Age. There is no perfect index of past volcanism, but more ice cores from Greenland and Antarctica will improve the record. There is no evidence that volcanic eruptions produce El Niño events, but the climatic effects of El Niño and volcanic eruptions must be separated to understand the climatic response to each. ]]></description>
         <author>Alan Robock</author>
         <category>Reviews of Geophysics</category>
         <pubDate>38</pubDate>
      </item>
      <item>
         <title>Magnetic and seismic reflection study of Lake Cheko, a possible impact crater for the 1908 Tunguska Event</title>
         <link>http://dx.doi.org/10.1029/2012GC004054</link>
         <description><![CDATA[A major explosion occurred on 30 June 1908 in the Tunguska region of Siberia, causing the destruction of over 2,000 km2 of taiga; pressure and seismic waves detected as far as 1,000 km away; bright luminescence in the night skies of Northern Europe and Central Asia; and other unusual phenomena. This “Tunguska Event” is probably related to the impact with the Earth of a cosmic body that exploded about 5–10 km above ground, releasing in the atmosphere 10–15 Mton of energy. Fragments of the impacting body have never been found, and its nature (comet or asteroid) is still a matter of debate. We report here results from a magnetic and seismic reflection study of a small (∼500 m diameter) lake, Lake Cheko, located about 8 km NW of the inferred explosion epicenter, that was proposed to be an impact crater left by a fragment of the Tunguska Cosmic Body. Seismic reflection and magnetic data revealed a P wave velocity/magnetic anomaly close to the lake center, about 10 m below the lake floor; this anomaly is compatible with the presence of a buried stony object and supports the impact crater origin for Lake Cheko.]]></description>
         <author>L. Gasperini, L. Cocchi, C. Stanghellini, G. Stanghellini, F. Del Bianco, M. Serrazanetti and C. Carmisciano</author>
         <category>Geochemistry Geophysics Geosystems</category>
         <pubDate>13</pubDate>
      </item>
      <item>
         <title>Phenomenology of transionospheric pulse pairs: Further observations</title>
         <link>http://dx.doi.org/10.1029/98RS02031</link>
         <description><![CDATA[We report on further observations of transionospheric pulse pairs (TIPPs), which are the most powerful transient radio signals observed by the Blackbeard broadband digital radio receiver on the ALEXIS satellite. The source of these signals is unknown but appears to be associated with thunderstorm activity. The signals do not resemble those reported for known lightning processes. We have previously reported observations of these events in the frequency band 28-95 MHz. In this paper we report observations of TIPPs in the 117- to 166-MHz band, with the subsatellite point situated over the contiguous United States. The main results are that the measured pulse parameter statistics are nearly the same as reported for the low-frequency events, with the exception that the pulse separation distribution is biased toward smaller values in the high-frequency observations. The radiated power does not drop off appreciably even at 166 MHz, which further constrains the possible size and timescale of the source(s). We also report results of experiments designed to measure the apparent reflectivity of dry, flat ground at frequencies around 100 MHz. We find that the apparent reflectivity can exceed 90%. This result helps to explain how the second pulse in a TIPP can have so much energy relative to the first.]]></description>
         <author>Robert S. Massey, Daniel N. Holden and Xuan-Min Shao</author>
         <category>Radio Science</category>
         <pubDate>33</pubDate>
      </item>
      <item>
         <title>Introducing a disturbance ionosphere index</title>
         <link>http://dx.doi.org/10.1029/2011RS004939</link>
         <description><![CDATA[Although ionospheric perturbations such as traveling ionospheric disturbances have a strong impact on Global Navigation Satellite Systems (GNSS) and other space-based radio systems, the description of individual perturbations is difficult. To overcome this problem, it is suggested to use a disturbance ionosphere index (DIX) that describes the perturbation degree of the ionosphere in a less specific form as a proxy. Although such an index does not describe the exact propagation conditions at the measurement site, the estimated index number indicates the probability of a potential impact on radio systems used in communication, navigation, and remote sensing. The definition of such a DIX must take into account the following major requirements: relevance to practical needs, objective measure of ionospheric conditions, easy and reproducible computation, and availability of a reliable database. Since the total electron content has been shown in many publications to act as an outstanding parameter for quantifying the range error and also the strength of ionospheric perturbations, we propose a DIX that is based on GNSS measurements. To illustrate the use of the index, recent storms monitored in 2011 and the Halloween storm are discussed. The proposed index is a robust and objective measure of the ionospheric state, applicable to radio systems which are impacted by a highly variable perturbed ionosphere.]]></description>
         <author>N. Jakowski, C. Borries and V. Wilken</author>
         <category>Radio Science</category>
         <pubDate>47</pubDate>
      </item>
      <item>
         <title>NATURAL RESIDUAL MAGNETISM OF ERUPTIVE ROCKS</title>
         <link>http://dx.doi.org/10.1029/TE043i003p00299</link>
         <description/>
         <author>J. G. Koenigsberger</author>
         <category>Terrestrial Magnetism and Atmospheric Electricity</category>
         <pubDate>43</pubDate>
      </item>
      <item>
         <title>The Martian ionosphere as observed by the Viking retarding potential analyzers</title>
         <link>http://dx.doi.org/10.1029/JS082i028p04351</link>
         <description><![CDATA[The retarding potential analyzers on the Viking landers obtained the first in situ measurements of ions from another planetary ionosphere. Mars has an F1 ionospheric layer with a peak ion concentration of approximately 105 cm−3 just below 130-km altitude, of which ∼90% are O2+ and 10% CO2+. At higher altitudes, O+ ions were detected with peak concentration near 225 km of less than 103 cm−3. Viking 1 measured ion temperatures of approximately 150°K near the F1 peak increasing to an apparent exospheric temperature of 210°K near 175 km. Above this altitude, departures from thermal equilibrium with the neutral gas occur, and Ti increases rapidly to >1000°K at 250 km. An equatorward horizontal ion velocity of the order of 100–200 m/s was observed near 200 km and near the F1 peak, with a minimum velocity at intermediate heights. Both landers entered the F1 layer at a solar zenith angle near 44°, though the local times of the Viking 1 and 2 entries were 16:13 and 9:49 LT, respectively. On Viking 2, considerably more structure was observed in the height profiles of ionospheric quantities, although they were similar in shape to the Viking 1 profiles.]]></description>
         <author>W. B. Hanson, S. Sanatani and D. R. Zuccaro</author>
         <category>Journal of Geophysical Research</category>
         <pubDate>82</pubDate>
      </item>
      <item>
         <title>A Pliocene-Pleistocene stack of 57 globally distributed benthic δ18O records</title>
         <link>http://dx.doi.org/10.1029/2004PA001071</link>
         <description><![CDATA[We present a 5.3-Myr stack (the “LR04” stack) of benthic δ18O records from 57 globally distributed sites aligned by an automated graphic correlation algorithm. This is the first benthic δ18O stack composed of more than three records to extend beyond 850 ka, and we use its improved signal quality to identify 24 new marine isotope stages in the early Pliocene. We also present a new LR04 age model for the Pliocene-Pleistocene derived from tuning the δ18O stack to a simple ice model based on 21 June insolation at 65°N. Stacked sedimentation rates provide additional age model constraints to prevent overtuning. Despite a conservative tuning strategy, the LR04 benthic stack exhibits significant coherency with insolation in the obliquity band throughout the entire 5.3 Myr and in the precession band for more than half of the record. The LR04 stack contains significantly more variance in benthic δ18O than previously published stacks of the late Pleistocene as the result of higher-resolution records, a better alignment technique, and a greater percentage of records from the Atlantic. Finally, the relative phases of the stack's 41- and 23-kyr components suggest that the precession component of δ18O from 2.7–1.6 Ma is primarily a deep-water temperature signal and that the phase of δ18O precession response changed suddenly at 1.6 Ma.]]></description>
         <author>Lorraine E. Lisiecki and Maureen E. Raymo</author>
         <category>Paleoceanography</category>
         <pubDate>20</pubDate>
      </item>
      <item>
         <title>Crustal structure of Australia from ambient seismic noise tomography</title>
         <link>http://dx.doi.org/10.1029/2011JB008403</link>
         <description><![CDATA[Surface wave tomography for Australian crustal structure has been carried out using group velocity measurements in the period range 1–32 s extracted from stacked correlations of ambient noise between station pairs. Both Rayleigh wave and Love wave group velocity maps are constructed for each period using the vertical and transverse component of the Green's function estimates from the ambient noise. The full suite of portable broadband deployments and permanent stations on the continent have been used with over 250 stations in all and up to 7500 paths. The permanent stations provide a useful link between the various shorter-term portable deployments. At each period the group velocity maps are constructed with a fully nonlinear tomographic inversion exploiting a subspace technique and the Fast Marching Method for wavefront tracking. For Rayleigh waves the continental coverage is good enough to allow the construction of a 3D shear wavespeed model in a two stage approach. Local group dispersion information is collated for a distribution of points across the continent and inverted for a 1D SV wavespeed profile using a Neighbourhood Algorithm method. The resulting set of 1D models are then interpolated to produce the final 3D wavespeed model. The group velocity maps show the strong influence of thick sediments at shorter periods, and distinct fast zones associated with cratonic regions. Below the sediments the 3D shear wavespeed model displays significant heterogeneity with only moderate correlation with surface tectonic features. For example, there is no evident expression of the Tasman Line marking the eastern edge of Precambrian outcrop. The large number of available inter-station paths extracted from the ambient noise analysis provide detailed shear wavespeed information for crustal structure across the Australian continent for the first time, including regions where there was no prior sampling because of difficult logistics.]]></description>
         <author>Erdinc Saygin and B. L. N. Kennett</author>
         <category>Journal of Geophysical Research</category>
         <pubDate>117</pubDate>
      </item>
      <item>
         <title>Factors controlling the mode of rift interaction in brittle-ductile coupled systems: A 3D numerical study</title>
         <link>http://dx.doi.org/10.1029/2012GC004077</link>
         <description><![CDATA[The way individual faults and rift segments link up is a fundamental aspect of lithosphere extension and continental break-up. Little is known however about the factors that control the selection of the different modes of rift interaction observed in nature. Here we use state-of-the-art large deformation 3D numerical models to examine the controls on the style and geometry of rift linkage between rift segments during extension of crustal brittle-ductile coupled systems. We focus on the effect of viscosity of the lower layer, the offset between the rift basins and the amount of strain weakening on the efficiency of rift linkage and rift propagation and the style of extension. The models predict three main modes of rift interaction: 1) oblique to transform linking graben systems for small to moderate rift offset and low lower layer viscosity, 2) propagating but non linking and overlapping primary grabens for larger offset and intermediate lower layer viscosity, and 3) formation of multiple graben systems with inefficient rift propagation for high lower layer viscosity. The transition between the linking (Mode 1) and non-linking mode (Mode 2) is controlled by the trade-off between the rift offset, the strength of brittle-ductile coupling, and the amount of strain weakening. The mode transition from overlapping non-connecting rift segments (Mode 2) to distributed deformation (Mode 3) is mainly controlled by the viscosity of the lower layer and can be understood from minimum energy dissipation analysis arguments.]]></description>
         <author>Vaneeda Allken, Ritske S. Huismans and Cedric Thieulot</author>
         <category>Geochemistry Geophysics Geosystems</category>
         <pubDate>13</pubDate>
      </item>
      <item>
         <title>PRELIMINARY REPORT ON ATMOSPHERIC POTENTIAL-GRADIENT OBSERVATIONS AT CHRISTCHURCH, NEW ZEALAND, 1928–1929</title>
         <link>http://dx.doi.org/10.1029/TE035i003p00133</link>
         <description/>
         <author>H. F. Skey</author>
         <category>Terrestrial Magnetism and Atmospheric Electricity</category>
         <pubDate>35</pubDate>
      </item>
      <item>
         <title>The mechanics of lubricated faults: Insights from 3-D numerical models</title>
         <link>http://dx.doi.org/10.1029/2011JB008929</link>
         <description><![CDATA[The weakening mechanisms occurring during an earthquake failure are of prominent importance in determining the resulting energy release and the seismic waves excitation. In this paper we consider the fully dynamic response of a seismogenic structure where lubrication processes take place. In particular, we numerically model the spontaneous propagation of a 3-D rupture in a fault zone where the frictional resistance is controlled by the properties of a low viscosity slurry, formed by gouge particles and fluids. This model allows for the description of the fault motion in the extreme case of vanishing effective normal stress, by considering a viscous fault response and therefore without the need to invoke, in the framework of Coulomb friction, the generation of the tensile mode of fracture. We explore the effects of the parameters controlling the resulting governing law for such a lubricated fault; the viscosity of the slurry, the roughness of the fault surfaces and the thickness of the slurry film. Our results indicate that lubricated faults produce a nearly complete stress drop (i.e., a very low residual friction coefficient; μ ∼ 0.01), a high fracture energy density (EG ∼ few 10s of MJ/m2) and significant slip velocities (vpeak ∼ few 10s of m/s). The resulting values of the equivalent characteristic slip-weakening distance (d0eq = 0.1–0.8 m, depending on the adopted parameters) are compatible with the seismological inferences. Moreover, in the framework of our model we found that supershear ruptures are highly favored. In the case of enlarging gap height we can have the healing of slip or even the inhibition of the rupture. Quantitative comparisons with different weakening mechanisms previously proposed in the literature, such as the exponential weakening and the frictional melting, are also discussed.]]></description>
         <author>Andrea Bizzarri</author>
         <category>Journal of Geophysical Research</category>
         <pubDate>117</pubDate>
      </item>
      <item>
         <title>Density and porosity of the lunar crust from gravity and topography</title>
         <link>http://dx.doi.org/10.1029/2012JE004062</link>
         <description><![CDATA[Newly obtained gravity and topography data of the Moon, combined with a lithospheric flexure model that considers both surface and subsurface loading, are used to place constraints on the density of the upper crust from a localized spectral admittance analysis. Subsurface loads are found to be relatively unimportant in the highlands, and when subsurface loads are neglected, the best fitting bulk densities for a number of highland regions are found to vary from 2590 to 2870 kg m−3, with a mean value of 2691 kg m−3. Crustal rock densities estimated from geochemical considerations and global iron and titanium abundances imply somewhat greater densities, which we interpret as porosity affecting the gravity-derived bulk density estimates. The average porosity in the upper few kilometers of crust is calculated to be about 7.7%, which is consistent with porosity estimates of impact-fractured meteorites and terrestrial impact craters.]]></description>
         <author>Qian Huang and Mark A. Wieczorek</author>
         <category>Journal of Geophysical Research</category>
         <pubDate>117</pubDate>
      </item>
      <item>
         <title>The magnitude of the effect of air pollution on sunshine hours in China</title>
         <link>http://dx.doi.org/10.1029/2011JD016753</link>
         <description><![CDATA[This study investigates the changes in sunshine hours in relation to API (Air Pollution Index) across China. Data were collected from a total of 38 cities over the period of 1960–2009. Sunshine hours in over 84% of the cities significantly (p < 0.05) decline with an average of 16.7% for the 1960s–2000s. This decline is mainly prevalent over Sichuan Basin (22.4%), North China Plain (18.8%), and Yangtze River Delta (18.2%). While the sunshine hour decline is largely in the 20th century (with the strongest drop in the 1980s and the least in the 1990s), it rebounds by 0.3% after 2000. For especially in winter seasons and the North China region, API is negatively related with sunshine hours. For days with API > 80, sunshine hours are on the average 0.7 h d−1 (8.4%) shorter than for days with API ≤ 80 under clear-sky condition for 2001–2005. In cities with average daily API ≤ 80 and >80 for the 2000s, sunshine hour decline for the 1960s–2000s is 0.8 h d−1 (13.4%) and 1.0 h d−1 (15.9%) respectively. Winter seasons with high API (90) exhibit the highest sunshine hour decline (21.5%). The study shows that spatiotemporal changes in sunshine hours in China could largely be explained in terms of API.]]></description>
         <author>Yawen Wang, Yonghui Yang, Na Zhao, Chen Liu and Qinxue Wang</author>
         <category>Journal of Geophysical Research</category>
         <pubDate>117</pubDate>
      </item>
      <item>
         <title>Biological production in the NE Pacific and its influence on air-sea CO2 flux: Evidence from dissolved oxygen isotopes and O2/Ar</title>
         <link>http://dx.doi.org/10.1029/2011JC007450</link>
         <description><![CDATA[We determine rates of gross photosynthetic O2 production (GOP) and net community O2 production (NCP) using the triple oxygen isotope and O2/Ar approach on two spring and two late summer meridional transects of the NE Pacific. Observed GOP and NCP in the subtropical (89 ± 9 and 8.3 ± 1.3 mmol O2 m−2 d−1, respectively) and subarctic (193 ± 16 and 16.3 ± 3.8 mmol O2 m−2 d−1) were in agreement with rates previously determined at time series stations in each region, validating the regional representativeness of these sites. At the transition zone chlorophyll front (TZCF), which migrates seasonally from 32°N in spring to 40°N in summer, GOP and NCP were elevated by 2–4× compared to adjacent areas. Coincident with the TZCF, increases in surface nitrate concentration and extensive changes in phytoplankton community composition were observed. HPLC pigment data indicated substantial increases in a prymnesiophyte (e.g., coccolithophore) biomarker at the TZCF on a spring and summer cruise, and a diatom biomarker on the spring cruise. Increases in remotely sensed surface particulate inorganic carbon concentration were also observed at the TZCF on all four cruises, indicating that coccolithophore production may contribute to increased productivity at the TZCF. Meridional trends in observed air-sea CO2 flux on each cruise resembled those of the biologically induced CO2 flux (NCP), but with an overprinting of the response of air-sea CO2 exchange to summer warming. A simple carbon budget based on regional CO2 flux climatology demonstrates the importance of NCP for net annual air-sea CO2 uptake, although slow air-sea equilibration and seasonal solubility effects obscure this term.]]></description>
         <author>L. W. Juranek, P. D. Quay, R. A. Feely, D. Lockwood, D. M. Karl and M. J. Church</author>
         <category>Journal of Geophysical Research</category>
         <pubDate>117</pubDate>
      </item>
      <item>
         <title>A REPRESENTATION OF THE SUNSPOT-CYCLE</title>
         <link>http://dx.doi.org/10.1029/TE044i002p00175</link>
         <description/>
         <author>C. N. Anderson</author>
         <category>Terrestrial Magnetism and Atmospheric Electricity</category>
         <pubDate>44</pubDate>
      </item>
      <item>
         <title>Airborne validation of cirrus cloud properties derived from CALIPSO lidar measurements: Optical properties</title>
         <link>http://dx.doi.org/10.1029/2011JD017053</link>
         <description><![CDATA[The Cloud-Aerosol Lidar Infrared Pathfinder Satellite Observations (CALIPSO) satellite was successfully launched in April 2006 to study cloud and aerosol layers using range-resolved laser remote sensing. Dedicated flights were conducted from July 26 to August 14, 2006 using the airborne Cloud Physics Lidar (CPL) to validate the CALIPSO lidar (CALIOP) data products. This paper presents results from coincident ice cloud measurements of lidar ratio, extinction coefficient, and optical depth. Flight segment case studies are shown as well as statistics for all coincident measurements during this CALIPSO-CloudSat Validation Experiment (CC-VEX). For the penetrated portion of opaque layers, CALIOP estimates of lidar ratio and extinction are substantially lower than the corresponding CPL values. Significant differences were also found for measurements of horizontally aligned ice, where different instrument viewing geometries precluded meaningful comparisons. After filtering the data set to exclude these discrepancies, overall CALIOP lidar ratio and extinction averages compared favorably to within 1% of overall CPL averages. When restricting the data further to exact coincident in-cloud point-pairs, CALIOP lidar ratios remained close to CPL values, averaging 2.1% below CPL, and the retrieved extinction and optical depth averaged 14.7% above CPL values, a result partially of higher average CALIOP attenuated backscatter but still a respectably close match.]]></description>
         <author>Dennis L. Hlavka, John E. Yorks, Stuart A. Young, Mark A. Vaughan, Ralph E. Kuehn, Matthew J. McGill and Sharon D. Rodier</author>
         <category>Journal of Geophysical Research</category>
         <pubDate>117</pubDate>
      </item>
      <item>
         <title>The formation of Valles Marineris: 2. Stress focusing along the buried dichotomy boundary</title>
         <link>http://dx.doi.org/10.1029/2011JE003954</link>
         <description><![CDATA[Although Valles Marineris is widely regarded as an extensional tectonic feature, the source of stress responsible for its formation remains unknown. This study argues that the tensile stresses that triggered Valles Marineris tectonism are a result of its location south of and subparallel to the buried crustal dichotomy boundary beneath Tharsis. The emplacement of the Tharsis volcanic load straddling the pre-existing topographic step of the crustal dichotomy boundary would have resulted in an abrupt change in the thickness of the load, causing differential subsidence and extension across the boundary. Thin-shell flexural models predict a narrow belt of focused tensile stresses south of the buried dichotomy boundary, coinciding with the location of present-day Valles Marineris. The interaction of these boundary-generated stresses with the competing stress fields associated with Tharsis loading can explain the formation of Noctis Labyrinthus in the west, and the deflection of the Valles Marineris troughs away from the buried boundary toward the east. Finite element models demonstrate that the magnitudes and vertical variations of stress at Valles Marineris are sensitive to the timing of loading and flexure in Tharsis. The incremental loading and flexure expected for a large volcanic rise results in the maximum tensile stress at Valles Marineris occurring at depth, with tensile stresses through the majority of the lithospheric column. Dikes forming within this tensile stress belt would propagate through the full vertical extent of the lithosphere due to the stress release associated with the dilation of the dikes, playing a crucial role in the formation of the Valles Marineris troughs.]]></description>
         <author>Jeffrey C. Andrews-Hanna</author>
         <category>Journal of Geophysical Research</category>
         <pubDate>117</pubDate>
      </item>
      <item>
         <title>Nadir observations of sprites from the International Space Station</title>
         <link>http://dx.doi.org/10.1029/2003JA009972</link>
         <description><![CDATA[The experiment LSO (Lightning and Sprite Observations) is dedicated to the optical study, from the International Space Station, of sprites occurring in the upper atmosphere above thunderstorms. The objectives were to study these phenomena and to validate a new measurement concept for future measurements of sprites from space at the nadir. The first measurements were performed in the frame of the flight of the French Astronaut Claudie Haigneré (mission Andromède) in October 2001. Observations were performed by two microcameras, one in the visible and near-infrared and the other equipped with a moderately wide band filter at 761 nm. This filter includes the most intense N2 1P emission of the sprites and partly the oxygen absorption A band of the atmosphere. The light emissions from sprites occurring in the middle and upper atmosphere are then differentiated from the emissions from lightning, occurring more deeply in the atmosphere and then more absorbed. This paper presents the first observations of sprites from space at the nadir and statistics about the respective intensities of lightning and sprites emissions as observed with this experiment.]]></description>
         <author>E. Blanc, T. Farges, R. Roche, D. Brebion, T. Hua, A. Labarthe and V. Melnikov</author>
         <category>Journal of Geophysical Research</category>
         <pubDate>109</pubDate>
      </item>
      <item>
         <title>A SUMMARY OF THE RESULTS OF THE RECENT MAGNETIC SURVEY OF GREAT BRITAIN AND IRELAND CONDUCTED BY PROFESSORS RÜCKER AND THORPE. PART III: ON THE RELATION BETWEEN THE MAGNETIC AND THE GEOLOGICAL CONSTITUTION OF GREAT BRITAIN AND IRELAND</title>
         <link>http://dx.doi.org/10.1029/TM001i003p00125</link>
         <description/>
         <author>A. W. Rücker</author>
         <category>Terrestrial Magnetism</category>
         <pubDate>1</pubDate>
      </item>
      <item>
         <title>On the probability of occurrence of extreme space weather events</title>
         <link>http://dx.doi.org/10.1029/2011SW000734</link>
         <description><![CDATA[By virtue of their rarity, extreme space weather events, such as the Carrington event of 1859, are difficult to study, their rates of occurrence are difficult to estimate, and prediction of a specific future event is virtually impossible. Additionally, events may be extreme relative to one parameter but normal relative to others. In this study, we analyze several measures of the severity of space weather events (flare intensity, coronal mass ejection speeds, Dst, and >30 MeV proton fluences as inferred from nitrate records) to estimate the probability of occurrence of extreme events. By showing that the frequency of occurrence scales as an inverse power of the severity of the event, and assuming that this relationship holds at higher magnitudes, we are able to estimate the probability that an event larger than some criteria will occur within a certain interval of time in the future. For example, the probability of another Carrington event (based on Dst < −850 nT) occurring within the next decade is ∼12%. We also identify and address several limitations with this approach. In particular, we assume time stationarity, and thus, the effects of long-term space climate change are not considered. While this technique cannot be used to predict specific events, it may ultimately be useful for probabilistic forecasting.]]></description>
         <author>Pete Riley</author>
         <category>Space Weather: The International Journal of Research and Applications</category>
         <pubDate>10</pubDate>
      </item>
      <item>
         <title>Structure of the atmosphere of Mars in summer at mid-latitudes</title>
         <link>http://dx.doi.org/10.1029/JS082i028p04364</link>
         <description><![CDATA[The structure of Mars' atmosphere was measured in situ by instruments on board the two Viking landers from an altitude of 120 km to near the surface. The two entries were separated by 178° in longitude, 25° in latitude, 45 days elapsed time, and 6 hours in Mars local time. Atmosphere structure was very well defined by the measurements and was generally similar at the two sites. Viking 1 and 2 surface pressures and temperatures were 7.62 and 7.81 mbar and 238°K and 226°K, respectively, while pressures at the elevation of the reference ellipsoid were 6.74 and 6.30 mbar. Mean temperature decreased with a lapse rate of about 1.6°K/km, significantly subadiabatic, from above the boundary layer to about 40 km, then was near isothermal but with a large-amplitude wave superimposed, attributed to the diurnal thermal tide. The mean profile appears to be governed by radiative equilibrium. Differences between the two temperature profiles are due to diurnal effects in the boundary layer, a small cooling of the Viking 2 profile up to 40 km due to latitude and season, and effects of time of day, latitude, terrain, and season on the wave structure. The density data merge well with those of the upper-atmosphere mass spectrometer to define a continuous profile to 200 km. The temperature wave continues above 100 km, increasing in amplitude and wavelength.]]></description>
         <author>Alvin Seiff and Donn B. Kirk</author>
         <category>Journal of Geophysical Research</category>
         <pubDate>82</pubDate>
      </item>
      <item>
         <title>Soil O2 controls denitrification rates and N2O yield in a riparian wetland</title>
         <link>http://dx.doi.org/10.1029/2011JG001799</link>
         <description><![CDATA[Wetland soil oxygen (O2) is rarely measured, which limits our understanding of a key regulator of nitrogen loss through denitrification. We asked: (1) How does soil [O2] vary in riparian wetlands? (2) How does this [O2] variation affect denitrification rates and end products? and (3) How does [O2] variation and previous exposure to O2 affect trace gas fluxes? We collected a continuous seven-month record of [O2] dynamics in a “wet” and “dry” riparian zone. In April 2009, soil [O2] ranged from 0 to 13% and consistently increased with increasing distance from the stream. [O2] gradually declined in all sensors until all sensors went anoxic in early September 2009. In mid-fall, a dropping water table increased soil [O2] to 15–20% within a 2–3 day period. We measured denitrification using the Nitrogen-Free Air Recirculation Method (N-FARM), a direct measurement of N2 production against a helium background. Denitrification rates were significantly higher in the wetter areas, which correlated to lower O2 conditions. Denitrification rates in the drier areas correlated with [O2] in the early spring and summer, but significantly decreased in late summer despite decreasing O2 concentrations. Increasing [O2] significantly increased core N2O production, and therefore may be an important control on nitrous oxide yield. Field N2O fluxes, however, were highly variable, ranging from 0 to 800 ug N m−2 hr−1 with no differences between the wet and dry sites. Future research should focus on understanding the biotic and abiotic controls on O2 dynamics, and O2 dynamics should be included in models of soil N cycling and trace gas fluxes.]]></description>
         <author>Amy J. Burgin and Peter M. Groffman</author>
         <category>Journal of Geophysical Research</category>
         <pubDate>117</pubDate>
      </item>
      <item>
         <title>Experimental alluvial fan evolution: Channel dynamics, slope controls, and shoreline growth</title>
         <link>http://dx.doi.org/10.1029/2011JF002261</link>
         <description><![CDATA[River deltas and alluvial fans have channelization and deposition dynamics that are not entirely understood, but which dictate the evolution of landscapes of great social, economic, and ecologic value. Our lack of a process-based understanding of fan dynamics hampers our ability to construct accurate prediction and hazard models, leaving these regions vulnerable. Here we describe the growth of a series of experimental alluvial fans composed of a noncohesive grain mixture bimodal in size and density. We impose conditions that simulate a gravel/sand fan prograding into a static basin with constant water and sediment influx, and the resulting fans display realistic channelization and avulsion dynamics. We find that we can describe the dynamics of our fans in terms of a few processes: (1) an avulsion sequence with a timescale dictated by mass conservation between incoming flux and deposit volume; (2) a tendency for flow to reoccupy former channel paths; and (3) bistable slopes corresponding to separate entrainment and deposition conditions for grains. Several important observations related to these processes are: an avulsion timescale that increases with time and decreases with sediment feed rate; fan lobes that grow in a self-similar, quasi-radial pattern; and channel geometry that is adjusted to the threshold entrainment stress. We propose that the formation of well-defined channels in noncohesive fans is a transient phenomenon resulting from incision following avulsion, and can be directly described with dual transport thresholds. We present a fairly complete, process-based description of the mechanics of avulsion and its resulting timescale on our fans. Because the relevant dynamics depend only on threshold transport conditions and conservation of mass, we show how results may be directly applied to field-scale systems.]]></description>
         <author>Meredith D. Reitz and Douglas J. Jerolmack</author>
         <category>Journal of Geophysical Research</category>
         <pubDate>117</pubDate>
      </item>
      <item>
         <title>Little Ice Age cold interval in West Antarctica: Evidence from borehole temperature at the West Antarctic Ice Sheet (WAIS) Divide</title>
         <link>http://dx.doi.org/10.1029/2012GL051260</link>
         <description><![CDATA[The largest climate anomaly of the last 1000 years in the Northern Hemisphere was the Little Ice Age (LIA) from 1400–1850 C.E., but little is known about the signature of this event in the Southern Hemisphere, especially in Antarctica. We present temperature data from a 300 m borehole at the West Antarctic Ice Sheet (WAIS) Divide. Results show that WAIS Divide was colder than the last 1000-year average from 1300 to 1800 C.E. The temperature in the time period 1400–1800 C.E. was on average 0.52 ± 0.28°C colder than the last 100-year average. This amplitude is about half of that seen at Greenland Summit (GRIP). This result is consistent with the idea that the LIA was a global event, probably caused by a change in solar and volcanic forcing, and was not simply a seesaw-type redistribution of heat between the hemispheres as would be predicted by some ocean-circulation hypotheses. The difference in the magnitude of the LIA between Greenland and West Antarctica suggests that the feedbacks amplifying the radiative forcing may not operate in the same way in both regions.]]></description>
         <author>Anais J. Orsi, Bruce D. Cornuelle and Jeffrey P. Severinghaus</author>
         <category>Geophysical Research Letters</category>
         <pubDate>39</pubDate>
      </item>
      <item>
         <title>Decrease of dissolved oxygen after the mid-1980s in the western North Pacific subtropical gyre along the 137°E repeat section</title>
         <link>http://dx.doi.org/10.1029/2011GB004227</link>
         <description><![CDATA[The Japan Meteorological Agency has acquired dissolved oxygen (DO) concentration data each year since 1967 along the 137°E repeat section in the western North Pacific. In this data set we found significant regional temporal trends of decreasing or increasing DO concentrations on various isopycnal surfaces. DO decreases were particularly significant after the mid-1980s in the subtropical gyre; mean rates of DO change at 20–25°N for 1985–2010 were −0.28 ± 0.08 μmol kg−1 yr−1 on 25.5 σθ in North Pacific Subtropical Mode Water (NPSTMW), −0.36 ± 0.08 μmol kg−1 yr−1 on 26.8 σθ in North Pacific Intermediate Water (NPIW), and −0.23 ± 0.04 μmol kg−1 yr−1 on 27.3 σθ in the O2 minimum Layer (OML). The cause of DO decrease differed among isopycnal surfaces. On density surfaces shallower than 26.0 σθ (less than about 400 m), the deepening of isopycnal surfaces and decline of oxygen solubility due to ocean warming have had the greatest influence. In particular, between 25.2 σθ and 25.8 σθ near the NPSTMW their combined contributions accounted for >50% of the DO decrease. In the NPIW core at roughly 26.8 σθ (∼700 m), the decline in DO was attributable to the DO decrease in the formation region. In the OML between 27.0 σθ and 27.3 σθ (∼1000 m), the DO decrease likely resulted from an increase in westward transport of low O2 water due to strengthening of the subtropical gyre. The result of this study shows the importance of the long-term and high-frequency along the 137°E repeat section.]]></description>
         <author>Yusuke Takatani, Daisuke Sasano, Toshiya Nakano, Takashi Midorikawa and Masao Ishii</author>
         <category>Global Biogeochemical Cycles</category>
         <pubDate>26</pubDate>
      </item>
      <item>
         <title>Kinematic evolution of Andean fold-thrust structures along the boundary between the Eastern Cordillera and Middle Magdalena Valley basin, Colombia</title>
         <link>http://dx.doi.org/10.1029/2011TC003089</link>
         <description><![CDATA[Surface and subsurface data support a kinematic reconstruction of Cenozoic fold-thrust deformation along the Eastern Cordillera-Magdalena Valley transition in Colombia. The La Salina fault (LSF) marks the boundary between west-vergent Eastern Cordillera structures and hinterland deposits of the Middle Magdalena Valley basin. Apatite fission track and (U-Th)/He thermochronological results for the west-directed LSF reveal initial hanging wall exhumation during middle Eocene–early Oligocene (45–30 Ma) shortening, renewed exhumation in the early middle Miocene (18–12 Ma), and accelerated late Miocene-Pliocene (12–3 Ma) exhumation. Vitrinite reflectance data suggest maximum burial of 4–6 km, helping constrain Cenozoic basin architecture. Mapping of the LSF reveals hanging wall Cretaceous–Eocene rocks in a broad anticline-syncline pair with limited faulting and footwall Eocene–Quaternary basin fill in a complex series of tight thrust-related folds. Limited displacement along the westernmost (frontal) thrust suggests that shortening is largely accommodated by east-directed thrusting within a broader triangle zone of a passive-roof duplex (and probable minor strike-slip deformation). In the preferred kinematic restoration, the most recent phase of shortening to transpressional deformation represents out-of-sequence reactivation of the LSF consistent with irregular crosscutting relationships among footwall structures. Earliest exhumation by 45–30 Ma in the Eastern Cordillera fold-thrust belt is correlated with increased sedimentary lithic fragments and high compositional maturity in sandstones of the adjacent Magdalena Valley basin. Exhumation since ∼15 Ma coincided with decreased compositional maturity and elevated accumulation rates for the Real Group. The compositional provenance shifts are attributed to westward advance of fold-thrust deformation into the proximal (eastern) segments of the Magdalena Valley basin.]]></description>
         <author>Javier Sánchez, Brian K. Horton, Eliseo Tesón, Andrés Mora, Richard A. Ketcham and Daniel F. Stockli</author>
         <category>Tectonics</category>
         <pubDate>31</pubDate>
      </item>
      <item>
         <title>River channel slope, flow resistance, and gravel entrainment thresholds</title>
         <link>http://dx.doi.org/10.1029/2011WR010850</link>
         <description><![CDATA[River beds are traditionally assumed to become mobile at a fixed value of nondimensional shear stress, but several flume and field studies have found that the critical value is higher in steep shallow flows. Explanations for this have been proposed in terms of the force balance on individual grains. The trend can also be understood in bulk-flow terms if total flow resistance has “base” and “additional” components, the latter due to protruding immobile grains as well as any bedforms, and the stress corresponding to “additional” resistance is not available for grain movement in threshold conditions. A quantitative model based on these assumptions predicts that critical Shields stress increases with slope, critical stream power is near-invariant with slope, and each has a secondary dependence on bed sorting. The proposed slope dependence is similar to what force-balance models predict and consistent with flume data and most field data. Possible explanations are considered for the inability of this and other models to match the very low critical values of width-averaged stress and power reported for some low-gradient gravel bed rivers.]]></description>
         <author>Robert I. Ferguson</author>
         <category>Water Resources Research</category>
         <pubDate>48</pubDate>
      </item>
      <item>
         <title>Historical land use change and associated carbon emissions in Brazil from 1940 to 1995</title>
         <link>http://dx.doi.org/10.1029/2011GB004133</link>
         <description><![CDATA[The evaluation of impacts of land use change is in general limited by the knowledge of past land use conditions. Most publications on the field present only a vague description of the earlier patterns of land use, which is usually insufficient for more comprehensive studies. Here we present the first spatially explicit reconstruction of historical land use patterns in Brazil, including both croplands and pasturelands, for the period between 1940 and 1995. This reconstruction was obtained by merging satellite imagery with census data, and provides a 5′ × 5′ yearly data set of land use for three different categories (cropland, natural pastureland and planted pastureland) for Brazil. The results show that important land use changes occurred in Brazil. Natural pasture dominated in the 1950s and 1960s, but since the beginning of 1970s it has been gradually replaced by planted pasture, especially in southeast and center west of Brazil. The croplands began its expansion in the 1960s reaching extensive areas in almost all states in 1980. Carbon emissions from historical land use changes were calculated by superimposing a composite biomass map on grids of a weighted average of the fractions of the vegetation types and the replacement land uses. Net emissions from land use changes between 1940 and 1995 totaled 17.2 ± 9.0 Pg-C (90% confidence range), averaging 0.31 ± 0.16 Pg-C yr−1, but reaching up to 0.47 ± 0.25 Pg-C yr−1 during the 1960s and through 1986–1995. Despite international concerns about Amazon deforestation emissions, 72% of Brazil's carbon emissions during the period actually came from deforestation in the Atlantic Forest and Cerrado biomes. Brazil's carbon emissions from land use change are about 11 times larger than its emissions from fossil fuel burning, although only about 18.1% of the native biomass has been lost due to agricultural expansion, which is similar to the global mean (17.7%).]]></description>
         <author>Christiane Cavalcante Leite, Marcos Heil Costa, Britaldo Silveira Soares-Filho and Letícia de Barros Viana Hissa</author>
         <category>Global Biogeochemical Cycles</category>
         <pubDate>26</pubDate>
      </item>
      <item>
         <title>Forcing, feedbacks and climate sensitivity in CMIP5 coupled atmosphere-ocean climate models</title>
         <link>http://dx.doi.org/10.1029/2012GL051607</link>
         <description><![CDATA[We quantify forcing and feedbacks across available CMIP5 coupled atmosphere-ocean general circulation models (AOGCMs) by analysing simulations forced by an abrupt quadrupling of atmospheric carbon dioxide concentration. This is the first application of the linear forcing-feedback regression analysis of Gregory et al. (2004) to an ensemble of AOGCMs. The range of equilibrium climate sensitivity is 2.1–4.7 K. Differences in cloud feedbacks continue to be important contributors to this range. Some models show small deviations from a linear dependence of top-of-atmosphere radiative fluxes on global surface temperature change. We show that this phenomenon largely arises from shortwave cloud radiative effects over the ocean and is consistent with independent estimates of forcing using fixed sea-surface temperature methods. We suggest that future research should focus more on understanding transient climate change, including any time-scale dependence of the forcing and/or feedback, rather than on the equilibrium response to large instantaneous forcing.]]></description>
         <author>Timothy Andrews, Jonathan M. Gregory, Mark J. Webb and Karl E. Taylor</author>
         <category>Geophysical Research Letters</category>
         <pubDate>39</pubDate>
      </item>
      <item>
         <title>13C constraints on ocean carbon cycle models</title>
         <link>http://dx.doi.org/10.1029/2010GB003980</link>
         <description><![CDATA[The sensitivity of oceanic δ13C fields to overturning and gas exchange is investigated in a suite of ocean general circulation models. The deep and oceanic mean δ13C in the models was sensitive to the balance between deep waters forming in the North Atlantic and the Southern Ocean. Increasing the Southern Ocean deep water formation rate to improve deep sea 14C and AOU fields was detrimental to model-data δ13C fidelity. A concurrent increase in North Atlantic Deep water would be needed to match the observed 14C and δ13C, constraining both the rate and schematics of model deep water formation, respectively, and improving sensitivity to future perturbations. Inter-basin trends in δ13C were sensitive to the rate of overturning in the models, with ‘high mixing’ model configurations matching the observations best. Models' anthropogenic δ13C changes, used as a diagnostic of model CO2 uptake, were in agreement with the observations, except at high southern latitudes (<50°S), where the model δ13C changes were greater than observed. There were predictive relationships among models' uptake of anthropogenic CO2 and depth-integrated δ13C changes. Model relationships between model anthropogenic CO2 uptake and the air-sea δ13C disequilibrium, and the sea surface δ13C, depend on preindustrial riverine fluxes of terrestrial organic carbon, and on the wind field used to drive the model circulation, respectively. Among the models tested, the relations among anthropogenic CO2 uptake and δ13C changes in the ocean are biased by the OCMIP practice of driving model momentum with one wind field, and gas exchange rates with another.]]></description>
         <author>Rolf E. Sonnerup and Paul D. Quay</author>
         <category>Global Biogeochemical Cycles</category>
         <pubDate>26</pubDate>
      </item>
      <item>
         <title>OLD MAGNETIC DECLINATIONS</title>
         <link>http://dx.doi.org/10.1029/TM001i001p00039</link>
         <description/>
         <author>W. van Bemmelen</author>
         <category>Terrestrial Magnetism</category>
         <pubDate>1</pubDate>
      </item>
      <item>
         <title>High-resolution mantle tomography of China and surrounding regions</title>
         <link>http://dx.doi.org/10.1029/2005JB004066</link>
         <description><![CDATA[A high-resolution P wave tomographic model of the crust and mantle down to 1100 km depth under China and surrounding regions is determined by using about one million arrival times of P, pP, PP, and PcP waves from 19,361 earthquakes recorded by 1012 seismic stations. The subducting Pacific slab is imaged clearly as a high-velocity zone from the oceanic trenches down to about 600 km depth, and intermediate-depth and deep earthquakes are located within the slab. The Pacific slab becomes stagnant in the mantle transition zone under east China. The western edge of the stagnant slab is roughly coincident with a surface topographic boundary in east China. The active Changbai and Wudalianchi intraplate volcanoes in northeast China are underlain by significant slow anomalies in the upper mantle, above the stagnant Pacific slab. These results suggest that the active intraplate volcanoes in NE China are not hot spots but a kind of back-arc volcano associated with the deep subduction of the Pacific slab and its stagnancy in the transition zone. Under the Mariana arc, however, the Pacific slab penetrates directly down to the lower mantle. The active Tengchong volcano in southwest China is related to the eastward subduction of the Burma microplate. The subducting Indian and Philippine Sea plates are also imaged clearly. The Indian plate has subducted down to 200–300 km depth under the Tibetan Plateau with a horizontal moving distance of about 500 km. High-velocity anomalies are revealed in the upper mantle under the Tarim basin, Ordos, and Sichuan basin, which are three stable blocks in China.]]></description>
         <author>Jinli Huang and Dapeng Zhao</author>
         <category>Journal of Geophysical Research</category>
         <pubDate>111</pubDate>
      </item>
      <item>
         <title>The seismic coupling of subduction zones revisited</title>
         <link>http://dx.doi.org/10.1029/2011JB009003</link>
         <description><![CDATA[The nature of seismic coupling for many of the world's subduction zones has been reevaluated. Geodetic estimates of seismic coupling obtained from GPS measurements of upper plate deformation during the interseismic period are summarized. We compared those with new estimates of seismic coupling obtained from seismological data. The results show that with a few notable exceptions the two methods agree to within about 10%. The seismological estimates have been greatly improved over those made 20–30 years ago because of an abundance of paleoseismological data that greatly extend the temporal record of great subduction earthquakes and by the occurrence, in the intervening years, of an unusual number of great and giant earthquakes that have filled in some of the most critical holes in the seismic record. The data also, again with a few notable exceptions, support the frictional instability theory of seismic coupling, and in particular, the test of that theory made by Scholz and Campos (1995). Overall, the results support their prediction that high coupling occurs for subduction zones subjected to high normal forces with a switch to low coupling occurring fairly abruptly as the normal force decreases below a critical value. There is also considerable variation of coupling within individual subduction zones. Earthquake asperities correlate with areas of high coupling and hence have a semblance of permanence, but the rupture zones and asperity distributions of great earthquakes may differ greatly between seismic cycles because of differences in the phase of seismic flux accumulation.]]></description>
         <author>Christopher H. Scholz and Jaime Campos</author>
         <category>Journal of Geophysical Research</category>
         <pubDate>117</pubDate>
      </item>
      <item>
         <title>Numerical investigation of deformation mechanics in fold-and-thrust belts: Influence of rheology of single and multiple décollements</title>
         <link>http://dx.doi.org/10.1029/2011TC003047</link>
         <description><![CDATA[Thin-skinned fold-and-thrust belts related to convergence tectonics develop by scraping off a rock sequence along a weaker basal décollement often formed by water-saturated shale layers or low-viscosity salt horizons. A two-dimensional finite element model with a viscoelastoplastic rheology is used to investigate the structural evolution of fold-and-thrust belts overlying different types of décollements. In addition, the influence of multiple weak layers in the stratigraphic column is studied. Model shale décollements are frictional, with lower friction angles as the cover sequence. Model salt layers behave linear viscous, due to a lower viscosity as the cover sequence, or with a power law rheology. Single viscous décollement simulations have been compared to an analytical solution concerning faulting versus folding. Results show that fold-and-thrust belts with a single frictional basal décollement generate thrust systems ramping from the décollement to the surface. Spacing between thrust ramps depends on the thickness of the cover sequence. The structural evolution of simulations with an additional low-frictional layer depends on the strength relationship between the basal and the intersequential décollement. Tectonic underplating and antiformal stacking occur if the within-sequence décollement is weaker. In the frontal part of models, deformation is restricted to the upper part and imbrication occurs with a wavelength depending on the depth of the intermediate weak layer. “Salt” décollement with a viscosity of 1018 Pa⋅s leads to isolated box folds (detachment folds). Multiple salt layers (1018 Pa⋅s) result in long-wavelength folding. Our results for both frictional and viscous décollements are in bulk agreement with the Mohr-Coulomb type, critical wedge theory.]]></description>
         <author>Jonas B. Ruh, Boris J. P. Kaus and Jean-Pierre Burg</author>
         <category>Tectonics</category>
         <pubDate>31</pubDate>
      </item>
      <item>
         <title>Particle Coatings Affecting the Wettability of Soils</title>
         <link>http://dx.doi.org/10.1029/JZ064i002p00263</link>
         <description><![CDATA[The fundamental principles underlying the process of wetting show that a reduction in the surface tension of a solid substance to be wetted reduces the wettability. Conversely, a reduction in the surface tension of the applied liquid increases the wettability. The wetting of a soil, which exhibits water-repellency in an air-dry state, can sometimes be achieved by leaving water in contact with this soil. There is some evidence that this wetting is achieved by an interaction of the solid and the liquid phase, leading to a reduction in the surface tension of the liquid. The phenomenon of advancing and receding angle of contact had led to an hypothesis that the angle of contact changes as the soil wets up or dries out. Some evidence is presented which does not support such an assumption, as the angle of contact seems fixed at a moisture content just above air-dry. There is some evidence that under certain conditions an improvement in the base status of the soil may lead to improved wettability. Particle coatings by hydrophobic films are in some cases responsible for the observed water-repellency. There is some evidence that this film is strongly adsorbed. No quantitative relationship could be detected between the characteristics of substances extracted by chloroform from a problem soil and the degree of unwettability of such a soil.]]></description>
         <author>Bessel D. van't Woudt</author>
         <category>Journal of Geophysical Research</category>
         <pubDate>64</pubDate>
      </item>
      <item>
         <title>Paleoceanography of the Atlantic-Mediterranean exchange: Overview and first quantitative assessment of climatic forcing</title>
         <link>http://dx.doi.org/10.1029/2011RG000376</link>
         <description><![CDATA[The Mediterranean Sea provides a major route for heat and freshwater loss from the North Atlantic and thus is an important cause of the high density of Atlantic waters. In addition to the traditional view that loss of fresh water via the Mediterranean enhances the general salinity of the North Atlantic, and the interior of the eastern North Atlantic in particular, it should be noted that Mediterranean water outflowing at Gibraltar is in fact cooler than compensating inflowing water. The consequence is that the Mediterranean is also a region of heat loss from the Atlantic and contributes to its large-scale cooling. Uniquely, this system can be understood physically via the constraints placed on it by a single hydraulic structure: the Gibraltar exchange. Here we review the existing knowledge about the physical structure of the Gibraltar exchange today and the evidential basis for arguments that it has been different in the past. Using a series of quantitative experiments, we then test prevailing concepts regarding the potential causes of these past changes. We find that (1) changes in the vertical position of the plume of Mediterranean water in the Atlantic are controlled by the vertical density structure of the Atlantic; (2) a prominent Early Holocene “contourite gap” within the Gulf of Cadiz is a response to reduced buoyancy loss in the eastern Mediterranean during the time of “sapropel 1” deposition; (3) changes in buoyancy loss from the Mediterranean during MIS3 caused changes in the bottom velocity field in the Gulf of Cadiz, but we note that the likely cause is reduced freshwater loss and not enhanced heat loss; and (4) strong exchange at Gibraltar during Atlantic freshening phases implies that the Gibraltar exchange provides a strong negative feedback to reduced Atlantic meridional overturning. Given the very counterintuitive way in which the Strait of Gibraltar system behaves, we recommend that without quantitative supporting work, qualitative interpretations of how the system has responded to past external forcing are unlikely to be robust.]]></description>
         <author>M. Rogerson, E. J. Rohling, G. R. Bigg and J. Ramirez</author>
         <category>Reviews of Geophysics</category>
         <pubDate>50</pubDate>
      </item>
      <item>
         <title>Spatial and temporal variability of biogenic isoprene emissions from a temperate estuary</title>
         <link>http://dx.doi.org/10.1029/2011GB004210</link>
         <description><![CDATA[Isoprene is important for its atmospheric impacts and the ecophysiological benefits it affords to emitting organisms; however, isoprene emissions from marine systems remain vastly understudied compared to terrestrial systems. This study investigates for the first time drivers of isoprene production in a temperate estuary, and the role this production may play in enabling organisms to tolerate the inherently wide range of environmental conditions. Intertidal sediment cores as well as high and low tide water samples were collected from four sites along the Colne Estuary, UK, every six weeks over a year. Isoprene concentrations in the water were significantly higher at low than high tide, and decreased toward the mouth of the estuary; sediment production showed no spatial variability. Diel isoprene concentration increased with light availability and decreased with tidal height; nighttime production was 79% lower than daytime production. Seasonal isoprene production and water concentrations were highest for the warmest months, with production strongly correlated with light (r2 = 0.800) and temperature (r2 = 0.752). Intertidal microphytobenthic communities were found to be the primary source of isoprene, with tidal action acting as a concentrating factor for isoprene entering the water column. Using these data we estimated an annual production rate for this estuary of 681 μmol m−2 y−1. This value falls at the upper end of other marine estimates and highlights the potentially significant role of estuaries as isoprene sources. The control of estuarine isoprene production by environmental processes identified here further suggests that such emissions may be altered by future environmental change.]]></description>
         <author>D. A. Exton, D. J. Suggett, M. Steinke and T. J. McGenity</author>
         <category>Global Biogeochemical Cycles</category>
         <pubDate>26</pubDate>
      </item>
      <item>
         <title>Simulating streamflow and dissolved organic matter export from a forested watershed</title>
         <link>http://dx.doi.org/10.1029/2011WR011423</link>
         <description><![CDATA[Stream water concentrations of dissolved organic matter (DOM) exhibit large temporal variations during precipitation on forested, headwater catchments. We present a modeling framework appropriate for describing streamflow and event-driven export of DOM from small, forested watersheds. Our model links parametrically simple formulations for rainfall-runoff generation and soil water carbon dynamics. The rainfall-runoff formulation is developed by modifying the catchment model of Kirchner (2009) to account for hysteresis in the relationship between stream discharge and catchment water storage. Time series computations of catchment water storage are used by the soil carbon model to approximate the effects of leaching, adsorption, and mineralization on soil water DOM concentrations and the export of DOM from the terrestrial reservoir to the stream. Our findings show that this model is capable of reproducing hourly variations of stream discharge (ranging from 0.01 to 0.38 mm h−1) and stream water DOM concentrations (ranging from 1.8 to 14 mg C L−1) measured in a forested headwater stream in north central Massachusetts. Our analysis highlights the strong linkage between soil carbon dynamics and hydrological processes that govern catchment water storage and flow paths connecting the terrestrial system to the stream.]]></description>
         <author>Na Xu, James E. Saiers, Henry F. Wilson and Peter A. Raymond</author>
         <category>Water Resources Research</category>
         <pubDate>48</pubDate>
      </item>
      <item>
         <title>Electric Fields Preceding Cloud-to-Ground Lightning Flashes</title>
         <link>http://dx.doi.org/10.1029/JC087iC07p04883</link>
         <description><![CDATA[We analyzed in detail the electric field variations preceding the first return strokes of 80 cloud-to-ground lightning flashes in nine different storms observed at the NASA Kennedy Space Center during the summers of 1976 and 1977. The electric field variations are best characterized as having two sections: preliminary variations and stepped leader. The stepped-leader electric-field change begins during a transition period of a few milliseconds duration marked by characteristic bipolar pulses. The durations of stepped leaders lie most frequently in the range 6–20 milliseconds. We infer from our measurements and critical review of the previous literature that there is only one type of stepped leader, not the two types, α and β, often referred to in the literature.]]></description>
         <author>William Beasley, Martin A. Uman and P. L. Rustan</author>
         <category>Journal of Geophysical Research</category>
         <pubDate>87</pubDate>
      </item>
      <item>
         <title>Generation of 100-year geomagnetically induced current scenarios</title>
         <link>http://dx.doi.org/10.1029/2011SW000750</link>
         <description><![CDATA[A series of 100-year extreme geoelectric field and geomagnetically induced current (GIC) scenarios are explored by taking into account the key geophysical factors associated with the geomagnetic induction process. More specifically, we derive explicit geoelectric field temporal profiles as a function of ground conductivity structures and geomagnetic latitudes. We also demonstrate how the extreme geoelectric field scenarios can be mapped into GIC. Generated statistics indicate 20 V/km and 5 V/km 100-year maximum 10-s geoelectric field amplitudes at high-latitude locations with poorly conducting and well-conducting ground structures, respectively. We show that there is an indication that geoelectric field magnitudes may experience a dramatic drop across a boundary at about 40°–60° of geomagnetic latitude. We identify this as a threshold at about 50° of geomagnetic latitude. The sub-threshold geoelectric field magnitudes are about an order of magnitude smaller than those at super-threshold geomagnetic latitudes. Further analyses are required to confirm the existence and location of the possible latitude threshold. The computed extreme GIC scenarios can be used in further engineering analyses that are needed to quantify the geomagnetic storm impact on conductor systems such as high-voltage power transmission systems. To facilitate further work on the topic, the digital data for generated geoelectric field scenarios are made publicly available.]]></description>
         <author>A. Pulkkinen, E. Bernabeu, J. Eichner, C. Beggan and A. W. P. Thomson</author>
         <category>Space Weather: The International Journal of Research and Applications</category>
         <pubDate>10</pubDate>
      </item>
      <item>
         <title>Geodetic observations detecting coseismic displacements and gravity changes caused by the Mw = 9.0 Tohoku-Oki earthquake</title>
         <link>http://dx.doi.org/10.1029/2011JB008849</link>
         <description><![CDATA[This paper reports coseismic displacements and gravity changes caused by the Tohoku-Oki earthquake (Mw 9.0), as observed respectively using GPS in Japan and China and its surrounding area, and as observed by GRACE. To interpret geodetic observation data, we must choose a reasonable model among the slip models presented for the event. For this purpose, we first calculated the displacements using three slip models from USGS, UCSB, and ARIA respectively, with different dislocation theories. Then we compared the results with the displacements observed in Japan and China. Results show that the modeled coseismic displacements calculated using the slip model of Wei et al. (ARIA) and the spherically layered dislocation theory under the PREM model agree well with the observed ones, indicating that the Earth's layer-structural and curvature effects should be considered. Then, we computed the coseismic geoid and gravity changes on the earth surface and at a space-fixed point using the three slip models and the spherically layered dislocation theory. Results show that the maximum coseismic geoid change reaches 2.5 cm and that the coseismic gravity changes are about −1000–600 μgal for a solid Earth. Furthermore, we processed GRACE data to extract coseismic changes with decorrelation and a Gaussian filter of 350 km. The gravity changes observed by GRACE were dominated by a decrease over the back-arc region, with −5 μgal reflecting coseismic crustal dilatation of the landward plate, which agrees well with the theoretically modeled values from the three finite fault models. After the 2004 Sumatra–Andaman and 2010 Central Chile (Maule) earthquakes, this study presents the third case of clear detection of coseismic gravity changes by GRACE.]]></description>
         <author>Xin Zhou, Wenke Sun, Bin Zhao, Guangyu Fu, Jie Dong and Zhaosheng Nie</author>
         <category>Journal of Geophysical Research</category>
         <pubDate>117</pubDate>
      </item>
      <item>
         <title>Effect of spectral-dependent surface albedo on Saharan dust direct radiative forcing</title>
         <link>http://dx.doi.org/10.1029/2012GL051360</link>
         <description><![CDATA[Direct radiative forcing (DRF) due to mineral dust has quite large uncertainty. Surface albedo is one of the most important factors affecting dust radiative forcing and climate. Here we investigate the effect of spectral-dependent surface albedo on dust DRF over the Saharan desert region using MODIS surface albedo data and a size-resolved global aerosol model. In one simulation, surface albedo in 7 wavebands from MODIS-retrieved data is interpolated to the corresponding 4 solar wavebands of the radiation transfer model (case 1). In another simulation, surface albedo for visible wavebands is applied to all 4 solar spectral-bands (case 2), which was previously used by many global model simulations. Our results show that the annual averaged DRF for all sky over the Saharan dust is −2.4 W m−2 and −5.6 W m−2 at TOA, and −9.9 W m−2 and −12.9 W m−2 at surface for cases 1 and 2, respectively. Such a large difference highlights the importance of using accurate spectral-dependent surface albedo, and implies that previous studies employing only visible-band surface albedo might have significantly overestimated the dust cooling effect over the Saharan dust.]]></description>
         <author>Xiaoyan Ma and Fangqun Yu</author>
         <category>Geophysical Research Letters</category>
         <pubDate>39</pubDate>
      </item>
      <item>
         <title>The 15N natural abundance of the N lost from an N-saturated subtropical forest in southern China</title>
         <link>http://dx.doi.org/10.1029/2010JG001615</link>
         <description><![CDATA[The 15N-enrichment of plants and soils is believed to indicate characteristics of the open nitrogen (N) cycle in terrestrial ecosystems because N lost from an ecosystem is presumably 15N-depleted through isotopic fractionation. However, because of a lack of an appropriate analytical methodology to confirm that supposition, the δ15N value for total dissolved nitrogen (TDN, the sum of ammonium, nitrate, and dissolved organic N) in stream water from forests has been measured only rarely. This report describes the δ15N values for TDN, ammonium, and nitrate in precipitation and stream water, together with those for soil-emitted nitrous oxide (N2O; measured once) in an N-saturated subtropical forest in southern China. Concentration-weighted δ15N values of TDN were −0.7‰ in precipitation and +1.2‰ in stream water. The difference in δ15N between soil (+3.9‰) and TDN in the stream water was 2.7‰. In contrast, soil-emitted N2O was strongly 15N-depleted (−14.3‰): 18‰ lower than that of the soil. Our results demonstrate that the discharged N loss is 15N-depleted only slightly compared with soil N, and gaseous N losses can be a strong driver for raising the terrestrial ecosystem δ15N. Our findings suggest that the relation between ecosystem δ15N and the open N cycle can be interpreted better by considering the net discrimination against 15N determined by the balance between gaseous and discharge N losses. Steady state 15N budget calculations proposed by Houlton and Bai (2009) can provide important information about the gaseous N fluxes, which are difficult to measure directly. The steady state calculation for the relationships among gaseous N loss, apparent isotopic fractionation during gaseous N loss, and isotopic signature of N inputs suggests that precise measurements of unmeasured components (e.g., dry deposition, NO and N2 emission) are quite important for better estimation of gaseous N losses from the ecosystem.]]></description>
         <author>Keisuke Koba, Yunting Fang, Jiangming Mo, Wei Zhang, Xiankai Lu, Lei Liu, Tao Zhang, Yu Takebayashi, Sakae Toyoda, Naohiro Yoshida, Keisuke Suzuki, Muneoki Yoh and Keishi Senoo</author>
         <category>Journal of Geophysical Research</category>
         <pubDate>117</pubDate>
      </item>
      <item>
         <title>How well do we know recent climate trends at the tropical tropopause?</title>
         <link>http://dx.doi.org/10.1029/2012JD017444</link>
         <description><![CDATA[The tropical tropopause is a transition layer between the troposphere and stratosphere that influences global climate and atmospheric chemistry. Several studies have reported multidecadal tropical tropopause cooling and have suggested a correlation between observed tropopause temperature and stratospheric water vapor. Our more rigorous examination of the observations shows tropopause trends have greater uncertainty than previously suggested and the cooling may not be statistically significant. We used two approaches to remove time-varying bias effects from cold-point tropopause trends estimated from radiosonde observations. Our results are consistent with expectations from a conceptual model of tropopause changes and could resolve discrepancies between complex climate models and observations.]]></description>
         <author>James S. Wang, Dian J. Seidel and Melissa Free</author>
         <category>Journal of Geophysical Research</category>
         <pubDate>117</pubDate>
      </item>
      <item>
         <title>Tectonic and climatic controls on knickpoint retreat rates and landscape response times</title>
         <link>http://dx.doi.org/10.1029/2011JF002157</link>
         <description><![CDATA[The rate at which transient knickpoints propagate through a landscape fundamentally controls the rate of geomorphic response to tectonic and climatic perturbation. Here we present knickpoint retreat rates upstream of active faults for 19 bedrock catchments in Turkey and 11 bedrock catchments in Italy where we have very good constraints on both the magnitude and timing of the tectonic perturbation and where climate histories are well documented. We show that the knickpoints have average retreat rates of between 0.2 and 2 mm/yr for catchments with drainage areas between 6 and 65 km2 and we test whether differences in rock mass strength and catchment size are sufficient to explain this range in retreat rates. Our analysis suggests that even accounting for these two variables, knickpoint propagation velocities differ markedly, and we show that channels crossing faults with higher throw rates have knickpoints that are retreating faster. The dependence of knickpoint retreat velocity on throw rate is at least as important as catchment drainage area. These results indicate, counterintuitively, that landscapes forced by large amplitude tectonic perturbations will have shorter response times than those perturbed by smaller amplitude changes. The link between the knickpoint propagation velocity and throw rate is largely (but not completely) explained by channel narrowing in areas of high uplift rate. Channel steepening upstream of the active faults may explain all of the residual dependency of knickpoint retreat rate on fault throw rate, but only if the slope exponent, n, in the standard stream power model is greater than 1.3. However, we cannot rule out a role for sediment supply in driving enhanced knickpoint retreat rate in addition to the well-documented channel narrowing effect. Finally, we find that mean knickpoints retreat rates in Turkey are only half of those in Italy, for catchments of equivalent size, crossing faults with similar throw rates. This difference in fluvial response time is accounted for by long-term differences in the ratio of precipitation to infiltration in the two areas over the last 1 My.]]></description>
         <author>Alexander C. Whittaker and Sarah J. Boulton</author>
         <category>Journal of Geophysical Research</category>
         <pubDate>117</pubDate>
      </item>
      <item>
         <title>Morphometric analysis of small-scale lobate scarps on the Moon using data from the Lunar Reconnaissance Orbiter</title>
         <link>http://dx.doi.org/10.1029/2011JE003907</link>
         <description><![CDATA[Prior to Lunar Reconnaissance Orbiter (LRO), the morphology and dimensions of only a limited number of lobate scarps, all located near the equator (within 21°), had been characterized. Topography derived from LRO Camera stereo images and Lunar Orbiter Laser Altimeter (LOLA) ranging is used to measure the relief and analyze the morphology of previously known and newly detected low and high latitude lobate scarps. The asymmetric profiles and maximum slopes on scarp faces (∼5° to 29°) of lunar lobate scarps are similar to those of lobate scarps observed on Mars and Mercury. Scarp lengths range from ∼0.6 to 21.6 km (mean = ∼6.0 km, median = ∼4.4 km, n = 79), and measured relief ranges from ∼5 to 150 m (mean = ∼35 m, median = ∼20 m, n = 26). Assuming a range of 20° to 40° for the fault plane dip, estimated lower limits for the horizontal shortening (S) expressed by the lobate scarp thrust faults range from ∼10 to 410 m. The range in S estimated for the lunar scarps is roughly an order of magnitude lower than estimates of S for lobate scarp thrust faults on Mars and Mercury. The relatively small range of S estimated for the growing number of well-characterized lunar scarps is consistent with a small amount of global contraction.]]></description>
         <author>M. E. Banks, T. R. Watters, M. S. Robinson, L. L. Tornabene, T. Tran, L. Ojha and N. R. Williams</author>
         <category>Journal of Geophysical Research</category>
         <pubDate>117</pubDate>
      </item>
      <item>
         <title>The source of the steep plasma density gradient in middle latitudes during the 11–12 April 2001 storm</title>
         <link>http://dx.doi.org/10.1029/2011JA017349</link>
         <description><![CDATA[A steep plasma density gradient has been observed in the middle-latitude F region during large geomagnetic storms. This phenomenon can be understood as a special form of the middle-latitude ionization trough (hereafter trough), but its causal linkage has not yet been clarified. We investigate the association of the steep density gradient and the trough by comparing their morphologies and occurrence locations using the satellite and ground observation data during the 11–12 April 2001 storm. Steep density gradients are detected in the dusk sector at the equatorward edges of the aurora by the Defense Meteorological Satellite Program (DMSP) F13 spacecraft. The locations of the steep density gradients coincide with the locations of the ionospheric footprints of the plasmapause identified by the Imager for Magnetopause-to-Aurora Global Exploration satellite. These observations demonstrate that the steep density gradient is created at the typical location of the trough. However, the steep density gradient is not produced by the formation of an intense trough during the storm. The temporal evolution of the total electron content maps shows that the steep density gradient observed at dusk by DMSP is associated with the plasma density enhancement in the dayside and its corotation into the dusk sector. The severe plasma density enhancement in middle latitudes, in combination with the trough and presumably the plasma depletion in high latitudes by the neutral composition change, produces the steep density gradient in the subauroral region during the storm.]]></description>
         <author>S. Park, K.-H. Kim, H. Kil, G. Jee, D.-H. Lee and J. Goldstein</author>
         <category>Journal of Geophysical Research</category>
         <pubDate>117</pubDate>
      </item>
      <item>
         <title>Computer simulations on sprite initiation for realistic lightning models with higher-frequency surges</title>
         <link>http://dx.doi.org/10.1029/2008JA013651</link>
         <description><![CDATA[Computer simulations on transient luminous emissions in the mesosphere and lower ionosphere have been performed for realistic lightning modelings with fast-varying current surges (M components) superimposed on the lightning continuing current (CC). The algorithm used here is an electromagnetic (EM) code, which enables us to estimate self-consistently the reduced electric field, electron density, conductivity, and luminosity as a function of space and time by solving the Maxwell equations. It is found that M components in the CC with small amplitudes, but with a fast-varying EM effect, can initiate or enhance the occurrence of sprites. Even for a return stroke (RS) without CC, subsequent high-frequency current variations (like M components) are found to lead to dramatic changes in the sprite occurrence. The physics underlying these changes is studied by means of, e.g., temporal and spatial variations of luminosity, electron density, and conductivity. As the conclusion, the RS is a fundamental agency for spites, but high-frequency variations as EM effects exhibit an additional essential influence on sprite occurrence. These computational results are used to offer some useful ideas concerning the unsolved problems of sprites and halos, including polarity asymmetry, long-delay characteristics, and morphological shapes of sprites.]]></description>
         <author>T. Asano, T. Suzuki, Y. Hiraki, E. Mareev, M. G. Cho and M. Hayakawa</author>
         <category>Journal of Geophysical Research</category>
         <pubDate>114</pubDate>
      </item>
      <item>
         <title>High-precision isotopic characterization of USGS reference materials by TIMS and MC-ICP-MS</title>
         <link>http://dx.doi.org/10.1029/2006GC001283</link>
         <description><![CDATA[The Pacific Centre for Isotopic and Geochemical Research (PCIGR) at the University of British Columbia has undertaken a systematic analysis of the isotopic (Sr, Nd, and Pb) compositions and concentrations of a broad compositional range of U.S. Geological Survey (USGS) reference materials, including basalt (BCR-1, 2; BHVO-1, 2), andesite (AGV-1, 2), rhyolite (RGM-1, 2), syenite (STM-1, 2), granodiorite (GSP-2), and granite (G-2, 3). USGS rock reference materials are geochemically well characterized, but there is neither a systematic methodology nor a database for radiogenic isotopic compositions, even for the widely used BCR-1. This investigation represents the first comprehensive, systematic analysis of the isotopic composition and concentration of USGS reference materials and provides an important database for the isotopic community. In addition, the range of equipment at the PCIGR, including a Nu Instruments Plasma MC-ICP-MS, a Thermo Finnigan Triton TIMS, and a Thermo Finnigan Element2 HR-ICP-MS, permits an assessment and comparison of the precision and accuracy of isotopic analyses determined by both the TIMS and MC-ICP-MS methods (e.g., Nd isotopic compositions). For each of the reference materials, 5 to 10 complete replicate analyses provide coherent isotopic results, all with external precision below 30 ppm (2 SD) for Sr and Nd isotopic compositions (27 and 24 ppm for TIMS and MC-ICP-MS, respectively). Our results also show that the first- and second-generation USGS reference materials have homogeneous Sr and Nd isotopic compositions. Nd isotopic compositions by MC-ICP-MS and TIMS agree to within 15 ppm for all reference materials. Interlaboratory MC-ICP-MS comparisons show excellent agreement for Pb isotopic compositions; however, the reproducibility is not as good as for Sr and Nd. A careful, sequential leaching experiment of three first- and second-generation reference materials (BCR, BHVO, AGV) indicates that the heterogeneity in Pb isotopic compositions, and concentrations, could be directly related to contamination by the steel (mortar/pestle) used to process the materials. Contamination also accounts for the high concentrations of certain other trace elements (e.g., Li, Mo, Cd, Sn, Sb, W) in various USGS reference materials.]]></description>
         <author>Dominique Weis, Bruno Kieffer, Claude Maerschalk, Jane Barling, Jeroen de Jong, Gwen A. Williams, Diane Hanano, Wilma Pretorius, Nadine Mattielli, James S. Scoates, Arnaud Goolaerts, Richard M. Friedman and J. Brian Mahoney</author>
         <category>Geochemistry Geophysics Geosystems</category>
         <pubDate>7</pubDate>
      </item>
      <item>
         <title>EVALUATION AND INTERPRETATION OF THE COLUMNAR RESISTANCE OF THE ATMOSPHERE</title>
         <link>http://dx.doi.org/10.1029/TE049i003p00159</link>
         <description/>
         <author>O. H. Gish</author>
         <category>Terrestrial Magnetism and Atmospheric Electricity</category>
         <pubDate>49</pubDate>
      </item>
      <item>
         <title>AIMANTATION INDUITE PAR LE CHAMP TERRESTRE SUR LES AIMANTS</title>
         <link>http://dx.doi.org/10.1029/TE004i001p00001</link>
         <description/>
         <author>Par M. E. Mascart</author>
         <category>Terrestrial Magnetism and Atmospheric Electricity</category>
         <pubDate>4</pubDate>
      </item>
      <item>
         <title>The geochemical evolution of the continental crust</title>
         <link>http://dx.doi.org/10.1029/95RG00262</link>
         <description><![CDATA[ A survey is given of the dimensions and composition of the present continental crust. The abundances of immobile elements in sedimentary rocks are used to establish upper crustal composition. The present upper crustal composition is attributed largely to intracrustal differentiation resulting in the production of granites senso lato. Underplating of the crust by ponded basaltic magmas is probably a major source of heat for intracrustal differentiation. The contrast between the present upper crustal composition and that of the Archean upper crust is emphasized. The nature of the lower crust is examined in the light of evidence from granulites and xenoliths of lower crustal origin. It appears that the protoliths of most granulite facies exposures are more representative of upper or middle crust and that the lower crust has a much more basic composition than the exposed upper crust. There is growing consensus that the crust grows episodically, and it is concluded that at least 60% of the crust was emplaced by the late Archean (ca. 2.7 eons, or 2.7 Ga). There appears to be a relationship between episodes of continental growth and differentiation and supercontinental cycles, probably dating back at least to the late Archean. However, such cycles do not explain the contrast in crustal compositions between Archean and post-Archean. Mechanisms for deriving the crust from the mantle are considered, including the role of present-day plate tectonics and subduction zones. It is concluded that a somewhat different tectonic regime operated in the Archean and was responsible for the growth of much of the continental crust. Archean tonalites and trond-hjemites may have resulted from slab melting and/or from melting of the Archean mantle wedge but at low pressures and high temperatures analogous to modern boninites. In contrast, most andesites and subduction-related rocks, now the main contributors to crustal growth, are derived ultimately from the mantle wedge above subduction zones. The cause of the contrast between the processes responsible for Archean and post-Archean crustal growth is attributed to faster subduction of younger, hotter oceanic crust in the Archean (ultimately due to higher heat flow) compared with subduction of older, cooler oceanic crust in more recent times. A brief survey of the causes of continental breakup reveals that neither plume nor lithospheric stretching is a totally satisfactory explanation. Speculations are presented about crustal development before 4000 m.y. ago. The terrestrial continental crust appears to be unique compared with crusts on other planets and satellites in the solar system, ultimately a consequence of the abundant free water on the Earth. ]]></description>
         <author>Stuart Ross Taylor and Scott M. McLennan</author>
         <category>Reviews of Geophysics</category>
         <pubDate>33</pubDate>
      </item>
      <item>
         <title>Did geomagnetic activity challenge electric power reliability during solar cycle 23? Evidence from the PJM regional transmission organization in North America</title>
         <link>http://dx.doi.org/10.1029/2011SW000752</link>
         <description><![CDATA[During solar cycle 22, a very intense geomagnetic storm on 13 March 1989 contributed to the collapse of the Hydro-Quebec power system in Canada. This event clearly demonstrated that geomagnetic storms have the potential to lead to blackouts. This paper addresses whether geomagnetic activity challenged power system reliability during solar cycle 23. Operations by PJM Interconnection, LLC (hereafter PJM), a regional transmission organization in North America, are examined over the period 1 April 2002 through 30 April 2004. During this time PJM coordinated the movement of wholesale electricity in all or parts of Delaware, Maryland, New Jersey, Ohio, Pennsylvania, Virginia, West Virginia, and the District of Columbia in the United States. We examine the relationship between a proxy of geomagnetically induced currents (GICs) and a metric of challenged reliability. In this study, GICs are proxied using magnetometer data from a geomagnetic observatory located just outside the PJM control area. The metric of challenged reliability is the incidence of out-of-economic-merit order dispatching due to adverse reactive power conditions. The statistical methods employed make it possible to disentangle the effects of GICs on power system operations from purely terrestrial factors. The results of the analysis indicate that geomagnetic activity can significantly increase the likelihood that the system operator will dispatch generating units based on system stability considerations rather than economic merit.]]></description>
         <author>Kevin F. Forbes and O. C. St. Cyr</author>
         <category>Space Weather: The International Journal of Research and Applications</category>
         <pubDate>10</pubDate>
      </item>
      <item>
         <title>Alpine inversion of the North African margin and delamination of its continental lithosphere</title>
         <link>http://dx.doi.org/10.1029/2011TC002989</link>
         <description><![CDATA[This paper aims at summarizing the current extent and architecture of the former Mesozoic passive margin of North Africa from North Algeria in the west up to the Ionian-Calabrian arc and adjacent Mediterranean Ridge in the east. Despite that most paleogeographic models consider that the Eastern Mediterranean Basin as a whole is still underlain by remnants of the Permo-Triassic or a younger Cretaceous Tethyan-Mesogean ocean, the strong similarities documented here in structural styles and timing of inversion between the Saharan Atlas, Sicilian Channel and the Ionian abyssal plain evidence that this portion of the Eastern Mediterranean Basin still belongs to the distal portion of the North African continental margin. A rim of Tethyan ophiolitic units can be also traced more or less continuously from Turkey and Cyprus in the east, in onshore Crete, in the Pindos in Greece and Mirdita in Albania, as well as in the Western Alps, Corsica and the Southern Apennines in the west, supporting the hypothesis that both the Apulia/Adriatic domain and the Eastern Mediterranean Basin still belong to the former southern continental margin of the Tethys. Because there is no clear evidence of crustal-scale fault offsetting the Moho, but more likely a continuous yet folded Moho extending between the foreland and the hinterland beneath the Mediterranean arcs, we propose here a new model of delamination of the continental lithosphere for the Apennines and the Aegean arcs. In this model, only the mantle lithosphere of Apulia and the Eastern Mediterranean is still locally subducted and recycled in the asthenosphere, most if not all the northern portion of the African crust and coeval Moho being currently decoupled from its former, currently delaminated and subducted mantle lithosphere.]]></description>
         <author>François Roure, Piero Casero and Belkacem Addoum</author>
         <category>Tectonics</category>
         <pubDate>31</pubDate>
      </item>
      <item>
         <title>Effects of sampling and mineral separation on accuracy of detrital zircon studies</title>
         <link>http://dx.doi.org/10.1029/2012GC004106</link>
         <description><![CDATA[We investigated some of the sampling and mineral separation biases that affect the accuracy of detrital zircon provenance studies. The study has been carried on a natural catchment in the Scottish Highlands that represents a simple two-component source system and on samples of synthetic sediment prepared for this study to test the effects of heavy mineral separation on the resulting zircon age spectra. The results suggest that zircon fertility of the source rocks and physical properties of zircon represent the most important factors affecting the distribution of zircon age populations in the stream sediments. The sample preparation and selection of zircons for analysis may result in preferential loss of information from small zircon grains. Together with the preference for larger crystals during handpicking, it can result in several-fold difference compared to the real age distribution in the sediment sample. These factors appear to be more important for the reproducibility of zircon age spectra than is the number of zircon grains analyzed per sample.]]></description>
         <author>Jiří Sláma and Jan Košler</author>
         <category>Geochemistry Geophysics Geosystems</category>
         <pubDate>13</pubDate>
      </item>
      <item>
         <title>Modeling ring current ion and electron dynamics and plasma instabilities during a high-speed stream driven storm</title>
         <link>http://dx.doi.org/10.1029/2011JA017433</link>
         <description><![CDATA[The temporal and spatial development of the ring current is evaluated during the 23–26 October 2002 high-speed stream (HSS) storm, using a kinetic ring current-atmosphere interactions model with self-consistent magnetic field (RAM-SCB). The effects of nondipolar magnetic field configuration are investigated on both ring current ion and electron dynamics. As the self-consistent magnetic field is depressed at large (>4RE) radial distances on the nightside during the storm main phase, the particles' drift velocities increase, the ion and electron fluxes are reduced and the ring current is confined closer to Earth. In contrast to ions, the electron fluxes increase closer to Earth and the fractional electron energy reaches ∼20% near storm peak due to better electron trapping in a nondipolar magnetic field. The ring current contribution to Dst calculated using Biot-Savart integration differs little from the DPS relation except during quiet time. RAM-SCB simulations underestimate ∣SYM-H∣ minimum by ∼25% but reproduce very well the storm recovery phase. Increased anisotropies develop in the ion and electron velocity distributions in a self-consistent magnetic field due to energy dependent drifts, losses, and dispersed injections. There is sufficient free energy to excite whistler mode chorus, electromagnetic ion cyclotron (EMIC), and magnetosonic waves in the equatorial magnetosphere. The linear growth rate of whistler mode chorus intensifies in the postmidnight to noon sector, EMIC waves are predominantly excited in the afternoon to midnight sector, and magnetosonic waves are excited over a broad MLT range both inside and outside the plasmasphere. The wave growth rates in a dipolar magnetic field have significantly smaller magnitude and spatial extent.]]></description>
         <author>V. K. Jordanova, D. T. Welling, S. G. Zaharia, L. Chen and R. M. Thorne</author>
         <category>Journal of Geophysical Research</category>
         <pubDate>117</pubDate>
      </item>
      <item>
         <title>Climatic responses to tropical sea surface temperature changes on a “greenhouse” Earth</title>
         <link>http://dx.doi.org/10.1029/1999PA000455</link>
         <description><![CDATA[ The uncertainty associated with tropical sea surface temperatures (SSTs) during past “greenhouse” climates may have important and unaccounted for effects. We explore early Paleogene climatic sensitivity to changes in tropical-subtropical SSTs with a general circulation model. We demonstrate that tropical SST changes have local and far-field climatic effects, underscoring their importance in understanding greenhouse climates. The responses of winds, upwelling, and surface water balance to tropical SST changes are substantial. Our results indicate that current tropical SST reconstructions may have a significant cool bias despite corrections and that the existence of hot (>30°C) tropical SSTs may be realistic for greenhouse climate intervals, including the Eocene. ]]></description>
         <author>Matthew Huber and L. Cirbus Sloan</author>
         <category>Paleoceanography</category>
         <pubDate>15</pubDate>
      </item>
      <item>
         <title>Controls on in situ oxygen and dissolved inorganic carbon dynamics in peats of a temperate fen</title>
         <link>http://dx.doi.org/10.1029/2011JG001888</link>
         <description><![CDATA[Changes in hydrological conditions are expected and may alter carbon cycling in peatlands. Peat aeration with water table change has not commonly been investigated, and the water table is often assumed to constitute the oxic-anoxic boundary in peat. We analyzed temperature, moisture, oxygen (O2), and carbon dioxide (CO2) concentrations in profiles of a temperate fen during two seasons. A drying-rewetting cycle and flooding were induced and compared to controls. The response of moisture and water table position varied greatly and was related to gradients of peat compaction and ash content. Background drought raised air-filled porosity (AFP) to a maximum of 15%–38% in shallow peat and experimental drought up to 50%. Decline in water table and soil moisture broadly led to O2 penetration and CO2 degassing, and rewetting and flooding led to anoxic conditions and CO2 accumulation in peat pore water. In dense peat with ≥20% ash content the unsaturated zone remained partly low in oxygen, however, and up to 5% AFP and 20 cm above water table O2 concentrations frequently remained below 50 μmol L−1. Moderately intense and short drying did not induce substantial oxygen penetration in the compacted soil profiles. The likelihood of the presence of oxygen in the peat was predicted by logistic regression using water table and ash content or bulk density as predictors (p < 0.0005). The model is potentially useful for predicting the position of the redoxcline in peat deposits and may assist in improving statistical models of trace gas emission from peatlands.]]></description>
         <author>Cristian Estop-Aragonés, Klaus-Holger Knorr and Christian Blodau</author>
         <category>Journal of Geophysical Research</category>
         <pubDate>117</pubDate>
      </item>
      <item>
         <title>Paleocean circulation during the Last Deglaciation: A bipolar seesaw?</title>
         <link>http://dx.doi.org/10.1029/97PA03707</link>
         <description><![CDATA[Hughen et al. [1998] have documented that during the first 200 years of Younger Dryas time the 14C content of atmospheric CO2 increased by ∼50‰ and that during the remainder of this 1200-year-duration cold event it steadily declined. The initial increase in 14C/C was likely the result of a reduction in the Atlantic's conveyor circulation. However, were the subsequent radiocarbon decline due to the rejuvenation of this potent heat pump, then it is difficult to understand why the climate conditions in the northern Atlantic basin remained cold throughout the Younger Dryas. Modeling exercises by Stocker and Wright [1996], Mikolajewicz [1998], and Schiller et al. [1998] show that if the conveyor is terminated, the transfer of radiocarbon into the deep sea shifts to the Southern Ocean, thereby stabilizing the atmospheric 14C/C ratio. Paleoclimatic evidence from the Antarctic continent suggests that this model-based scenario might have been played out in the real world. While the Younger Dryas cooling has been documented in many places around the world, including New Zealand [Denton and Hendy, 1994], Sowers and Bender [1995], using their 18O in O2-based correlation between the ice core 18O in ice records for Antarctica and Greenland, have demonstrated that in Antarctica the Younger Dryas was a time of maximum warming. The point of this paper is that the steep rise in 18O rise in Antarctic ice which commenced close to the onset of the Younger Dryas might have been caused by heat released to the atmosphere in response to an increase in deep-sea ventilation in the Southern Ocean. ]]></description>
         <author>Wallace S. Broecker</author>
         <category>Paleoceanography</category>
         <pubDate>13</pubDate>
      </item>
      <item>
         <title>Contrasting rift and subduction-related plagiogranites in the Jinshajiang ophiolitic mélange, southwest China, and implications for the Paleo-Tethys</title>
         <link>http://dx.doi.org/10.1029/2011TC002937</link>
         <description><![CDATA[The Jinshajiang ophiolitic mélange zone in southwest China represents a remnant of the eastern Paleo-Tethys Ocean. Field, geochronological and geochemical studies have identified two distinct suites of plagiogranites within the mélange, the Dongzhulin trondhjemite and Jiyidu tonalite, which represent rift and subduction settings, respectively, related to opening and closing of the ocean. SHRIMP U-Pb analysis on zircons extracted from the Dongzhulin trondhjemite yields a mean 206Pb/238U age of 347 ± 7 Ma. REE and isotopic characteristics suggest an origin from low pressure partial melting of an amphibolitic protolith. Highly variable Hf isotopic compositions for zircons from this body may indicate a heterogenous source involving both depleted mantle and enriched continental components. This, together with geologic relations, suggests formation near an embryonic spreading center in a continent-ocean transition setting. The Jiyidu tonalite has a U-Pb zircon age of 283 ± 3 Ma, and geochemical data indicates high Sr/Y, (La/Yb)N, Nb/Ta and low Y, and marked heavy REE depletion. These signatures suggest derivation from low degree partial melting of subducted slab at pressure high enough to stabilize garnet and rutile. A slab-melt origin is also supported by in situ Hf and O data for zircon that show isotopic compositions comparable with typical altered oceanic crust. Thus, the crystallization age of the Jiyidu high Sr/Y tonalite provides a constraint for the subduction of the Jinshajiang ocean floor. The rift-related Dongzhulin trondhjemite and subduction-related Jiyidu high-Sr/Y tonalite constrain the timing and setting of opening and closing of this segment of the Paleo-Tethys Ocean.]]></description>
         <author>Jian-Wei Zi, Peter A. Cawood, Wei-Ming Fan, Yue-Jun Wang and Eric Tohver</author>
         <category>Tectonics</category>
         <pubDate>31</pubDate>
      </item>
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