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.
Institutions
- Planetary Science Institute (US)
- Center For Remote Sensing (United States) (US)
- Lunar and Planetary Institute (US)
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
- 0.00