Estimate of the D/H Ratio in the Martian Upper Atmosphere from the Low Spectral Resolution Mode of MAVEN/IUVS-Reference-Cited by-同舟云学术

Estimate of the D/H Ratio in the Martian Upper Atmosphere from the Low Spectral Resolution Mode of MAVEN/IUVS

Published:2021-04 Issue:4 Volume:126 Page:
ISSN:2169-9097
Container-title:Journal of Geophysical Research: Planets
language:en
Short-container-title:J Geophys Res Planets

Author:

Chaufray J‐Y.¹^ORCID,Mayyasi M.²^ORCID,Chaffin M.³^ORCID,Deighan J.³^ORCID,Bhattacharyya D.⁴^ORCID,Clarke J.²^ORCID,Jain S.³^ORCID,Schneider N.³^ORCID,Jakosky B.³^ORCID

Affiliation:

1. LATMOS‐IPSL CNRS UVSQ Université Paris‐Saclay Sorbonne Université Guyancourt France

2. Center for Space Physics Boston University Boston MA USA

3. LASP University of Colorado Boulder Boulder CO USA

4. Department of Electrical and Computer Engineering University of Illinois at Urbana‐Champaign USA

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/10.1029/2020JE006814

Reference44 articles.

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2. Isotopic fractionation through water vapor condensation: The Deuteropause, a cold trap for deuterium in the atmosphere of Mars

3. Two-dimensional model for the martian exosphere: Applications to hydrogen and deuterium Lyman α observations

4. Analysis and modeling of remote observations of the martian hydrogen exosphere

5. Mars Global Ionosphere-Thermosphere Model: Solar cycle, seasonal, and diurnal variations of the Mars upper atmosphere

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