The Dynamic Atmospheric And Aeolian Environment Of
Jezero Crater, Mars
C. E. Newman, Aeolis Research, Chandler, Az, Usa (Claire@Aeolisresearch.Com), R. Hueso, Upv/Ehu, Bilbao, Spain, M. T. Lemmon, Ssi, College Station, Tx, Usa, A. Munguira, Upv/Ehu, Bilbao, Spain, Á. Vicente-Retortillo, Cab, Inta, Madrid, Spain, V. Apestigue, Inta, Madrid, Spain, G. Martínez Martínez, Lpi,
Houston, Tx, Usa, D. Toledo Carrasco, Inta, Madrid, Spain, R. Sullivan, Cornell, Ithaca, Ny, Usa, K.
Herkenhoff, Usgs Astrogeology Science Center, Flagstaff, Az, Usa, M. De La Torre Juárez, Jpl-Caltech,
Pasadena, Ca, Usa, M. I. Richardson, Aeolis Research, Chandler, Az, Usa, A. Stott, Isae-Supaero, Toulouse, France, N. Murdoch, Isae-Supaero, Toulouse, France, A. Sanchez-Lavega, Upv/Ehu, Bilbao,
Spain, M. Wolff, Ssi, College Station, Tx, Usa, I. Arruego Rodriguez, Inta, Madrid, Spain, E. Sebastián,
Cab, Inta, Madrid, Spain, S. Navarro, Cab, Inta, Madrid, Spain, J. Gómez-Elvira, Cab-Inta, Madrid,
Spain, L. Tamppari, Jpl-Caltech, Pasadena, Ca, Usa, D. Viúdez-Moreiras, Cab, Inta, Madrid, Spain, J.
Pla-Garcia, Cab, Inta, Madrid, Spain; Ssi, Boulder, Co, Usa, Mars 2020 Atmospheres Working Group.

Introduction:
Aeolian Processes Are The Main Causes Of Change
To The Martian Surface And Atmosphere In The Modern
Era (1,2). Large Dust Storms Hugely Alter Atmospheric
Temperatures, Densities, And Circulation, Presenting
Hazards To Robotic And Human Missions, But Atmospheric Dust Is Present Year-Round, Affecting Visibility
And Solar Power (3,4). Yet, Despite Their Importance
To Science And Exploration, Processes That Move Sand
And Raise Dust Have Not Been Well Quantified In Situ,