Constraints on dust aerosols from the Mars Exploration Rovers using MGS overflights and Mini‐TES
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Mark T. Lemmon | Anupam Ghosh | M. J. Wolff | Geoffrey A. Landis | Joshua L. Bandfield | James F. Bell | S. W. Squyres | S. Squyres | G. Landis | J. Bell | M. Lemmon | D. Banfield | R. Clancy | M. Wolff | B. Whitney | A. Ghosh | J. Bandfield | Michael D. Smith | N. Spanovich | P. R. Christensen | Barbara A. Whitney | R. T. Clancy | N. Spanovich | Donald J. Banfield | P. Christensen
[1] K. Stamnes,et al. Radiative Transfer in the Atmosphere and Ocean , 1999 .
[2] R. Wilson,et al. Simulation of the Martian dust cycle with the GFDL Mars GCM , 2004 .
[3] K. Vikram,et al. Time-domain ultrasonic NDE of layered media: Texas A&M University, Aerospace Engineering Department, College Station, TX 77843, USA , 1992 .
[4] Amitabha Ghosh,et al. First Atmospheric Science Results from the Mars Exploration Rovers Mini-TES , 2004, Science.
[5] R. Todd Clancy,et al. Constraints on the size of Martian aerosols from Thermal Emission Spectrometer observations , 2003 .
[6] Donald E. Jennings,et al. Exploration of the Solar System by Infrared Remote Sensing: Retrieval of physical parameters from measurements , 1992 .
[7] J. Hansen,et al. Light scattering in planetary atmospheres , 1974 .
[8] S. T. Elliot,et al. Mars Exploration Rover Athena Panoramic Camera (Pancam) investigation , 2003 .
[9] P. Drossart,et al. Post‐Phobos model for the altitude and size distribution of dust in the low Martian atmosphere , 1995 .
[10] R E Arvidson,et al. Spectral Reflectance and Morphologic Correlations in Eastern Terra Meridiani, Mars , 2005, Science.
[11] Terry Z. Martin,et al. Thermal infrared opacity of the Mars atmosphere , 1986 .
[12] K. Stamnes,et al. Numerically stable algorithm for discrete-ordinate-method radiative transfer in multiple scattering and emitting layered media. , 1988, Applied optics.
[13] J. Bandfield,et al. Spectral data set factor analysis and end-member recovery: Application to analysis of Martian atmospheric particulates , 2000 .
[14] O. Talagrand,et al. Global structure and composition of the martian atmosphere with SPICAM on Mars express , 2005 .
[15] Mark T. Lemmon,et al. Properties of dust in the Martian atmosphere from the Imager on Mars Pathfinder , 1999 .
[16] Miles J. Johnson,et al. In‐flight calibration and performance of the Mars Exploration Rover Panoramic Camera (Pancam) instruments , 2006 .
[17] P. R. Bevington,et al. Data Reduction and Error Analysis for the Physical Sciences, 2nd ed. , 1993 .
[18] S. Squyres,et al. Coordinated Mars Exploration Rover and Mars Express OMEGA Observations over Meridiani Planum , 2004 .
[19] P. R. Bevington,et al. Data Reduction and Error Analysis for the Physical Sciences , 1969 .
[20] R. Todd Clancy,et al. Hubble Space Telescope observations of the Martian aphelion cloud belt prior to the Pathfinder mission: Seasonal and interannual variations , 1999 .
[21] Joshua L. Bandfield,et al. Global mineral distributions on Mars , 2002 .
[22] Carl Sagan,et al. Physical properties of the particles composing the Martian dust storm of 1971–1972 , 1977 .
[23] David P. Hinson,et al. Temperature inversions, thermal tides, and water ice clouds in the Martian tropics , 2003 .
[24] Thomas E. Wolverton,et al. Miniature Thermal Emission Spectrometer for the Mars Exploration Rovers , 2003 .
[25] M. Mellon,et al. Mars Global Surveyor Thermal Emission Spectrometer experiment: Investigation description and surface science results , 2001 .
[26] G. R. Gladstone,et al. A new model for Mars atmospheric dust based upon analysis of ultraviolet through infrared observations from Mariner 9, Viking, and Phobos , 1995 .
[27] Amitabha Ghosh,et al. One Martian year of atmospheric observations using MER Mini‐TES , 2006 .
[28] Jimmy D Bell,et al. Atmospheric Imaging Results from the Mars Exploration Rovers: Spirit and Opportunity , 2004, Science.
[29] R. Todd Clancy,et al. Mars aerosol studies with the MGS TES emission phase function observations: Optical depths, particle sizes, and ice cloud types versus latitude and solar longitude , 2003 .
[30] Barney J. Conrath,et al. Thermal structure of the Martian atmosphere during the dissipation of the dust storm of 1971 , 1975 .
[31] B. Hapke,et al. Mineralogy of Martian atmospheric dust inferred from thermal infrared spectra of aerosols , 2005 .
[32] J. Bandfield,et al. Multiple emission angle surface–atmosphere separations of thermal emission spectrometer data , 2001 .
[33] G. Hunt. On the opacity of Martian dust storms derived by Viking IRTM spectral measurements , 1979 .
[34] M. D. Smith,et al. Mineralogy at Meridiani Planum from the Mini-TES Experiment on the Opportunity Rover , 2004, Science.
[35] R. Todd Clancy,et al. A new look at dust and clouds in the Mars atmosphere: analysis of emission-phase-function sequences from global viking IRTM observations , 1991 .
[36] Duane O. Muhleman,et al. WATER VAPOR SATURATION AT LOW ALTITUDES AROUND MARS APHELION : A KEY TO MARS CLIMATE ? , 1996 .
[37] Michael D. Smith. Interannual variability in TES atmospheric observations of Mars during 1999–2003 , 2004 .
[38] R E Arvidson,et al. Initial Results from the Mini-TES Experiment in Gusev Crater from the Spirit Rover , 2004, Science.
[39] Jimmy D Bell,et al. Absorption and scattering properties of the Martian dust in the solar wavelengths. , 1997, Journal of geophysical research.
[40] F. Palluconi,et al. Infrared Thermal Mapping of the Martian Surface and Atmosphere: First Results , 1976, Science.
[41] Michael D. Smith. The annual cycle of water vapor on Mars as observed by the Thermal Emission Spectrometer , 2002 .