Simulating the density and thermal structure of the middle atmosphere (∼80–130 km) of Mars using the MGCM–MTGCM: A comparison with MEX/SPICAM observations

The objective of this work is to advance the understanding of the structure and dynamics of the middle altitude region of the martian atmosphere. While numerous advancements have been made in the level of scientific understanding of Mars’s upper and lower atmospheres over the past several decades, i...

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Veröffentlicht in:	Icarus (New York, N.Y. 1962) N.Y. 1962), 2010-03, Vol.206 (1), p.5-17
Hauptverfasser:	McDunn, T.L., Bougher, S.W., Murphy, J., Smith, M.D., Forget, F., Bertaux, J.-L., Montmessin, F.
Format:	Artikel
Sprache:	eng
Schlagworte:	Aeronomy Astrophysics Atmosphere, Structure Earth and Planetary Astrophysics Mars, Atmosphere Physics Sciences of the Universe
Online-Zugang:	Volltext
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