Changes In Surface Albedo Induced By Dust Devils And
The My 36 Ls155 Dust Storm At Jezero Crater
A. Vicente-Retortillo1,2, G.M. Martínez3, M. T. Lemmon4, R. Hueso5, R. Sullivan6, C. E. Newman7, E. Sebastián1, D. Toledo8, V. Apéstigue8, I. Arruego8, A. Munguira4, A. Sánchez-Lavega5, L. Mora-Sotomayor1,
T. Bertrand9, L. K. Tamppari10, M. De La Torre Juárez10, J.-A. Rodríguez-Manfredi1, 1centro De Astrobiología (Inta-Csic), Madrid, Spain (Adevicente@Cab.Inta-Csic.Es) , 2university Of Michigan, Ann Arbor, Mi,
Usa, 3lunar And Planetary Institute, Usra, Houston, Tx, Usa, 4space Science Institute, Boulder, Co, Usa,
5
Universidad Del País Vasco (Upv/Ehu), Bilbao, Spain, 6ccaps, Cornell University, Ithaca, Ny, Usa, 7aeolis
Research, Chandler, Az, Usa, 8instituto Nacional De Técnica Aeroespacial (Inta), Madrid, Spain, 9lesia,
Meudon, France, 10jet Propulsion Laboratory/California Institute Of Technology, Pasadena, Ca, Usa.

Introduction:
Since February 2021, The Environmental Conditions At Jezero Crater Have Been Monitorized By
Meda, The Suite Of Meteorological Sensors Onboard
The Mars 2020 Perseverance Rover [1]. Simultaneous
Measurements From The Thermal And Infrared Sensor
(Tirs), The Radiation And Dust Sensor (Rds), The
Pressure Sensor And The Wind Sensor Allow Studying
Dust Lifting At The Martian Surface By Analyzing An
Unprecedented Set Of Magnitudes, Including High
Frequency Measurements (1 – 2 Hz) Of Surface