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Read Full Article (file size: 2383108 bytes) Cited by
JOURNAL OF GEOPHYSICAL RESEARCH,
VOL. 113,
D15S11,
doi:10.1029/2007JD008783,
2008
Validation of the Aura Microwave Limb Sounder temperature and geopotential height measurements
M. J. Schwartz
Jet Propulsion Laboratory, California Institute of Technology, Pasadena, California, USA
A. Lambert
Jet Propulsion Laboratory, California Institute of Technology, Pasadena, California, USA
G. L. Manney
Jet Propulsion Laboratory, California Institute of Technology, Pasadena, California, USA Department of Physics, New Mexico Institute of Mining and Technology, Socorro, New Mexico, USA
W. G. Read
Jet Propulsion Laboratory, California Institute of Technology, Pasadena, California, USA
N. J. Livesey
Jet Propulsion Laboratory, California Institute of Technology, Pasadena, California, USA
L. Froidevaux
Jet Propulsion Laboratory, California Institute of Technology, Pasadena, California, USA
C. O. Ao
Jet Propulsion Laboratory, California Institute of Technology, Pasadena, California, USA
P. F. Bernath
Department of Chemistry, University of Waterloo, Waterloo, Ontario, Canada
C. D. Boone
Department of Chemistry, University of Waterloo, Waterloo, Ontario, Canada
R. E. Cofield
Jet Propulsion Laboratory, California Institute of Technology, Pasadena, California, USA
W. H. Daffer
Jet Propulsion Laboratory, California Institute of Technology, Pasadena, California, USA
B. J. Drouin
Jet Propulsion Laboratory, California Institute of Technology, Pasadena, California, USA
E. J. Fetzer
Jet Propulsion Laboratory, California Institute of Technology, Pasadena, California, USA
R. A. Fuller
Jet Propulsion Laboratory, California Institute of Technology, Pasadena, California, USA
R. F. Jarnot
Jet Propulsion Laboratory, California Institute of Technology, Pasadena, California, USA
J. H. Jiang
Jet Propulsion Laboratory, California Institute of Technology, Pasadena, California, USA
Y. B. Jiang
Jet Propulsion Laboratory, California Institute of Technology, Pasadena, California, USA
B. W. Knosp
Jet Propulsion Laboratory, California Institute of Technology, Pasadena, California, USA
K. Krüger
Leibniz Institute for Marine Sciences, IFM-GEOMAR, Kiel University, Kiel, Germany
J.-L. F. Li
Jet Propulsion Laboratory, California Institute of Technology, Pasadena, California, USA
M. G. Mlynczak
NASA Langley Research Center, Hampton, Virginia, USA
S. Pawson
Global Modeling and Assimilation Office, NASA Goddard Space Flight Center, Greenbelt, Maryland, USA
J. M. Russell III
Hampton University, Hampton, Virginia, USA
M. L. Santee
Jet Propulsion Laboratory, California Institute of Technology, Pasadena, California, USA
W. V. Snyder
Jet Propulsion Laboratory, California Institute of Technology, Pasadena, California, USA
P. C. Stek
Jet Propulsion Laboratory, California Institute of Technology, Pasadena, California, USA
R. P. Thurstans
Jet Propulsion Laboratory, California Institute of Technology, Pasadena, California, USA
A. M. Tompkins
European Centre for Medium-range Weather Forecasts, Reading, UK
P. A. Wagner
Jet Propulsion Laboratory, California Institute of Technology, Pasadena, California, USA
K. A. Walker
Department of Chemistry, University of Waterloo, Waterloo, Ontario, Canada
J. W. Waters
Jet Propulsion Laboratory, California Institute of Technology, Pasadena, California, USA
D. L. Wu
Jet Propulsion Laboratory, California Institute of Technology, Pasadena, California, USA
Abstract
Global satellite observations of temperature and geopotential height (GPH) from the Microwave Limb Sounder (MLS) on the EOS
Aura spacecraft are discussed. The precision, resolution, and accuracy of the data produced by the MLS version 2.2 processing
algorithms are quantified, and recommendations for data screening are made. Temperature precision is 1 K or better from 316
hPa to 3.16 hPa, degrading to ∼3 K at 0.001 hPa. The vertical resolution is 3 km at 31.6 hPa, degrading to 6 km at 316 hPa
and to ∼13 km at 0.001 hPa. Comparisons with analyses (Goddard Earth Observing System version 5.0.1 (GEOS-5), European Centre
for Medium-range Weather Forecasts (ECMWF), Met Office (MetO)) and other observations (CHAllenging Minisatellite Payload (CHAMP),
Atmospheric Infrared Sounder/Advanced Microwave Sounder Unit (AIRS/AMSU), Sounding of the Atmosphere using Broadband Radiometry
(SABER), Halogen Occultation Experiment (HALOE), Atmospheric Chemistry Experiment (ACE), radiosondes) indicate that MLS temperature
has persistent, pressure-dependent biases which are between −2.5 K and +1 K between 316 hPa and 10 hPa. The 100-hPa MLS v2.2
GPH surface has a bias of ∼150 m relative to the GEOS-5 values. These biases are compared to modeled systematic uncertainties.
GPH biases relative to correlative measurements generally increase with height owing to an overall cold bias in MLS temperature
relative to correlative temperature measurements in the upper stratosphere and mesosphere.
Received 11
April
2007;
accepted 27
December
2007;
published 2
May
2008.
Keywords: temperature;
GPH;
MLS.
Index Terms: 0350 Atmospheric Composition and Structure: Pressure, density, and temperature; 0394 Atmospheric Composition and Structure: Instruments and techniques; 3360 Atmospheric Processes: Remote sensing; 3394 Atmospheric Processes: Instruments and techniques; 1694 Global Change: Instruments and techniques.
Read Full Article (file size: 2383108 bytes) Cited by
Citation: Schwartz, M. J., et al.
(2008),
Validation of the Aura Microwave Limb Sounder temperature and geopotential height measurements,
J. Geophys. Res.,
113,
D15S11,
doi:10.1029/2007JD008783.
Copyright 2008 by the American Geophysical Union.
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