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Isobar Altitude Variations in the Upper Mesosphere Observed With IUVS-MAVEN in Response to Martian Dust Storms

Authors :
Benoît Hubert
Francisco Gonzalez-Galindo
Jean-Claude Gérard
Leonardos Gkouvelis
Nicholas M. Schneider
Fonds de la Recherche Scientifique (Fédération Wallonie-Bruxelles)
Ministerio de Ciencia, Innovación y Universidades (España)
European Commission
Belgian Science Policy Office
European Space Agency
National Science Foundation (US)
University of Colorado
Source :
Digital.CSIC. Repositorio Institucional del CSIC, instname
Publication Year :
2020
Publisher :
American Geophysical Union, 2020.

Abstract

We report limb measurements of the oxygen dayglow emission at 297.2 nm performed during four Martian dust storms. The emission peak provides a good remote sensing tool to probe changes of the altitude of the 39 mPa pressure level for the first time during dust storms. We illustrate the time variation of these changes and compare them with the infrared opacity in the lower atmosphere. We find that the 39 mPa level rises in response to the increase in dust opacity. It reaches a plateau, and additional dust load does not significantly increase its altitude. Numerical simulations with the LMD global circulation model shows a similar response, except for the event observed during MY33 regional storm when the model fails to reproduce the observed variations. Observations collected during the onset of the global dust storm in June 2018 show that the upper atmosphere rapidly responds within two Martian days to the increased amount of tropospheric dust. ©2020. American Geophysical Union. All Rights Reserved.<br />B. Hubert is a research associate of the Belgian Fund for Scientific Research (FNRS). F.G.G. is funded by the Spanish Ministerio de Ciencia, Innovación y Universidades, the Agencia Estatal de Investigacion and EC FEDER funds under project RTI2018‐100920‐J‐I00, and acknowledges financial support from the State Agency for Research of the Spanish MCIU through the “Center of Excellence Severo Ochoa” award to the Instituto de Astrofísica de Andalucía (SEV‐2017‐0709). We acknowledge L. Montabone for providing infrared opacity data before their final publication. This project acknowledges funding by the Belgian Science Policy Office (BELSPO), with the financial and contractual coordination by the ESA Prodex Office. IUVS archive, V13 was used for this study. This work utilized the RMACC Summit supercomputer, which is supported by the National Science Foundation (awards ACI‐341 1532235 and ACI‐1532236), the University of Colorado Boulder, and Colorado State University. The Summit supercomputer is a joint effort of the University of Colorado Boulder and Colorado State University.

Details

Language :
English
Database :
OpenAIRE
Journal :
Digital.CSIC. Repositorio Institucional del CSIC, instname
Accession number :
edsair.doi.dedup.....bcb249f8c79d6a7f7e26ac9e64a30223