Martian Dust Dynamics Constrained by OMEGA/MARS EXPRESS Orbital Data
Abstract
We developed a new method to detect dust storms on Mars based on orbital spectroscopy (OMEGA/MEx). This method is used to characterize dust dynamics, notably the links between dust storms and small-scaled surface phenomena like RSL.
- Publication:
-
52nd Lunar and Planetary Science Conference
- Pub Date:
- March 2021
- Bibcode:
- 2021LPI....52.1471L