MAVEN/IUVS Stellar Occultation Measurements of Mars Atmospheric Structure and Composition-Reference-Cited by-同舟云学术

MAVEN/IUVS Stellar Occultation Measurements of Mars Atmospheric Structure and Composition

Published:2018-06 Issue:6 Volume:123 Page:1449-1483
ISSN:2169-9097
Container-title:Journal of Geophysical Research: Planets
language:en
Short-container-title:J. Geophys. Res. Planets

Author:

Gröller H.¹^ORCID,Montmessin F.²^ORCID,Yelle R. V.¹^ORCID,Lefèvre F.²,Forget F.³,Schneider N. M.⁴^ORCID,Koskinen T. T.¹^ORCID,Deighan J.⁴,Jain S. K.⁴^ORCID

Affiliation:

1. Lunar and Planetary Laboratory University of Arizona Tucson AZ USA

2. Guyancourt LATMOS, Université Versailles Saint‐Quentin/CNRS France

3. Laboratorie de Météorologie Dynamique, Institute Pierre‐Simon Laplace Paris France

4. Laboratory for Atmospheric and Space Physics University of Colorado Boulder Boulder CO USA

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

Link

https://onlinelibrary.wiley.com/doi/pdf/10.1029/2017JE005466

Reference77 articles.

1. The first Mars thermospheric general circulation model: The Martian atmosphere from the ground to 240 km

2. Upper atmosphere of Mars up to 120 km: Mars Global Surveyor accelerometer data analysis with the LMD general circulation model

3. Room temperature photoabsorption cross section measurements of CO2 between 91,000 and 115,000cm−1

4. Detection of Molecular Oxygen in the Martian Atmosphere

5. Detection of Molecular Oxygen on Mars

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