The density of the upper martian atmosphere measured by Lyman-α absorption with Mars Express SPICAM
Author:
Publisher
Elsevier BV
Subject
Space and Planetary Science,Astronomy and Astrophysics
Reference15 articles.
1. Nightglow in the upper atmosphere of Mars and implications for atmospheric transport;Bertaux;Science,2005
2. SPICAM on Mars Express: Observing modes and overview of the spectrometer data and scientific results;Bertaux;J. Geophys. Res.,2006
3. SPICAV on Venus Express: Three spectrometers to study the global structure and composition of the Venus atmosphere;Bertaux;Planet. Space Sci.,2007
4. Solar cycle variability of Mars dayside exospheric temperatures: Model evaluation of underlying thermal balances;Bougher;Geophys. Res. Lett.,2009
5. Observation of the hydrogen corona with SPICAM on Mars Express;Chaufray;Icarus,2008
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1. A denser and elevated Martian nightside ionosphere during Mars season Ls 180–360°;Icarus;2022-12
2. Neutral Composition and Horizontal Variations of the Martian Upper Atmosphere From MAVEN NGIMS;Journal of Geophysical Research: Planets;2022-06
3. Effect of the 2018 Martian Global Dust Storm on the CO 2 Density in the Lower Nightside Thermosphere Observed From MAVEN/IUVS Lyman‐Alpha Absorption;Geophysical Research Letters;2020-03-25
4. Prediction of blue, red and green aurorae at Mars;Planetary and Space Science;2015-09
5. The electron thermal structure in the dayside Martian ionosphere implied by the MGS radio occultation data;Journal of Geophysical Research: Planets;2015-02
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