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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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)|
|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|
|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|
|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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