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Isobar Altitude Variations in the Upper Mesosphere Observed With IUVS-MAVEN in Response to Martian Dust Storms
- 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.
- Subjects :
- Martian
Dust storm
geography
Summit
geography.geographical_feature_category
010504 meteorology & atmospheric sciences
IUVS
Library science
Mars dayglow
MAVEN
Storm
010502 geochemistry & geophysics
01 natural sciences
Oxygen 297.2 nm
Geophysics
State agency
Political science
General Earth and Planetary Sciences
Upper atmosphere
Science policy
0105 earth and related environmental sciences
Subjects
Details
- Language :
- English
- Database :
- OpenAIRE
- Journal :
- Digital.CSIC. Repositorio Institucional del CSIC, instname
- Accession number :
- edsair.doi.dedup.....bcb249f8c79d6a7f7e26ac9e64a30223