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Modelling of atmospheric dust emission and surface of Mars applying a radiative transfer simulation in the 2.0 and 2.7 µm CO2 bands

Haus, R. (1998) Modelling of atmospheric dust emission and surface of Mars applying a radiative transfer simulation in the 2.0 and 2.7 µm CO2 bands. XXIII General Assembly of the European Geophysical Society, Nice, France, April 20-24, 1998.

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Abstract

Synthetic infrared radiation spectra of Mars which can be measured by an orbiting Planetary Fourier Spectrometer (PFS) have been calculated in the spectral region from 1 to 50 µm. A radiative transfer simulation technique was applied taking into consideration absorption, emission and mutiple scattering by molecular (CO2, H2O, CO) and particulate (palagonite, carbonate, ice) species. It is shown that the radiation contributions from atmospheric dust emission and surface reflectance can be separated in the region of the CO2 bands at 2.0 and 2.7 µm, respectively. Quantitative results on an aerosol retrieval procedure are discussed.

Document Type:Conference or Workshop Item (Speech)
Additional Information: LIDO-Berichtsjahr=1999,
Title:Modelling of atmospheric dust emission and surface of Mars applying a radiative transfer simulation in the 2.0 and 2.7 µm CO2 bands
Authors:
AuthorsInstitution or Email of Authors
Haus, R.UNSPECIFIED
Date:1998
Status:Published
Keywords:IR spectra, Mars, dust, surface
Event Title:XXIII General Assembly of the European Geophysical Society, Nice, France, April 20-24, 1998
Organizer:European Geophysical Society
HGF - Research field:Aeronautics, Space and Transport (old)
HGF - Program:Space (old)
HGF - Program Themes:W EW - Erforschung des Weltraums
DLR - Research area:Space
DLR - Program:W EW - Erforschung des Weltraums
DLR - Research theme (Project):UNSPECIFIED
Location: Berlin-Adlershof
Institutes and Institutions:Institute of Planetary Research > Institut für Planetenerkundung
Deposited By: Susanne Pieth
Deposited On:16 Sep 2005
Last Modified:14 Jan 2010 15:50

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