Millefeuille: The layering of the Martian atmosphere observed in forward scattering geometry.

We report on observations of the atmosphere above the limb of Mars in forward scattering geometry (~174° phase angle) using the Colour and Stereo Surface Imaging System (CaSSIS) aboard the European Space Agency's ExoMars Trace Gas Orbiter spacecraft. These unique observations provide high-resolution (18 meters per pixel) measurements of light scattered by aerosols in the atmosphere. The observations are characterized by subkilometer-scale layering, ±20% variations in color of the individual layers, and high radiance (I/F > 1). Strong spatial (latitudinal) variability is also evident, suggesting highly inhomogeneous absorption and atmospheric heating. Models of the radiance, while likely to be degenerate, indicate good agreement with lower-resolution results inferred from other techniques. Mesospheric aerosol layers (strongly blue in CaSSIS color ratios) are also evident. The observed decrease in the CaSSIS RED/BLU color ratio with altitude is indicative of a decrease in particle radius.

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Publication Details

Journal
Open Access CRIS of the University of Bern
Published
2025-09-19
DOI
https://doi.org/10.48620/91484
Primary Topic
Diverse Scientific and Economic Studies
Type
article
Field-Weighted Citation Impact
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article

Millefeuille: The layering of the Martian atmosphere observed in forward scattering geometry.

Open Access CRIS of the University of Bern
Diverse Scientific and Economic Studies
article

Millefeuille: The layering of the Martian atmosphere observed in forward scattering geometry.

article en

Abstract

We report on observations of the atmosphere above the limb of Mars in forward scattering geometry (~174° phase angle) using the Colour and Stereo Surface Imaging System (CaSSIS) aboard the European Space Agency's ExoMars Trace Gas Orbiter spacecraft. These unique observations provide high-resolution (18 meters per pixel) measurements of light scattered by aerosols in the atmosphere. The observations are characterized by subkilometer-scale layering, ±20% variations in color of the individual layers, and high radiance (I/F > 1). Strong spatial (latitudinal) variability is also evident, suggesting highly inhomogeneous absorption and atmospheric heating. Models of the radiance, while likely to be degenerate, indicate good agreement with lower-resolution results inferred from other techniques. Mesospheric aerosol layers (strongly blue in CaSSIS color ratios) are also evident. The observed decrease in the CaSSIS RED/BLU color ratio with altitude is indicative of a decrease in particle radius.

Open Access CRIS of the University of Bern
Planetary Science Institute (US), Center For Remote Sensing (United States) (US), Lunar and Planetary Institute (US)
Openalex Percentile: Top 35%
Diverse Scientific and Economic Studies
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Millefeuille: The layering of the Martian atmosphere observed in forward scattering geometry. · Open Access CRIS of the University of Bern (2025) | TGRS Research Map | TGRS