Effects of Global Dust Storms on Water Vapor in the Southern Polar Region of Mars

Author:

Pankine Alexey A.1ORCID,Leung Cecilia2,Tamppari Leslie2ORCID,Martinez German3ORCID,Giuranna Marco4ORCID,Piqueux Sylvain2ORCID,Smith Michael5ORCID,Trokhimovskiy Alexander6ORCID

Affiliation:

1. Space Science Institute Boulder CO USA

2. NASA Jet Propulsion Laboratory California Institute of Technology Pasadena CA USA

3. Lunar and Planetary Institute Houston TX USA

4. Istituto di Astrofisica e PlanetologiaSpaziali (IAPS)—Istituto Nazionale di Astrofisica (INAF) Rome Italy

5. NASA Goddard Space Flight Center Greenbelt MD USA

6. Space Research Institute RAS Moscow Russia

Abstract

AbstractMartian global dust storms (GDS) can significantly affect the water cycle in the lower atmosphere (0−40 km). We compare the evolution of water vapor abundances, dust opacity and surface temperatures in the Southern Polar Region (SPR) during GDS years of MY25, MY28, and MY34 relative to years without GDS. During all GDS years, the vapor abundances decrease in the lower atmosphere in the SPR following the storm. Our results suggest that this decrease could be the result of disruption of the southward transport of vapor by atmospheric circulation. Alternatively, the decrease in vapor abundances could be caused by decreased desorption of vapor from the subsurface.

Funder

National Aeronautics and Space Administration

Publisher

American Geophysical Union (AGU)

Subject

Space and Planetary Science,Earth and Planetary Sciences (miscellaneous),Geochemistry and Petrology,Geophysics

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