Possible influence of Martian surface mineralogy on the detectability of atmospheric trace gases - mid-infrared simulation results-Reference-Cited by-同舟云学术

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Possible influence of Martian surface mineralogy on the detectability of atmospheric trace gases - mid-infrared simulation results

Published:2024-09 Issue: Volume:249 Page:105877
ISSN:0032-0633
Container-title:Planetary and Space Science
language:en
Short-container-title:Planetary and Space Science

Author:

Błęcka Maria I.

Publisher

Elsevier BV

Reference29 articles.

1. Mars surface diversity as revealed by the OMEGA/mars express observations;Bibring;Science,2005

2. Passive detection of biological aerosols in the atmosphere with a fourier transform instrument (FTIR)—the results of the measurements in the laboratory and in the field;Błęcka;Orig. Life Evol. Biosph.,2012

3. Numerical simulation of the visible and near infrared radiance of Mars: effect of atmospheric scattering;Blecka;Adv. Space Res.,2004

4. A study of the influence of the surface emittance and extinction by dust on Martian spectra;Blecka;Adv. Space Res.,1999

5. Absorption and Scattering of Light by Small Particles;Bohren,1983

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