Dynamical Phenomena in the Martian Atmosphere Through Mars Express Imaging

被引：2
|
作者：
Sanchez-Lavega, A. [1 ]
del Rio-Gaztelurrutia, T. [1 ]
Spiga, A. [2 ]
Hernandez-Bernal, J. [2 ]
Larsen, E. [1 ]
Tirsch, D. [3 ]
Cardesin-Moinelo, A. [4 ,5 ,6 ]
Machado, P. [6 ]
机构：
[1] Univ Pais Vasco UPV EHU, Escuela Ingn Bilbao, Dept Fis Aplicada, Bilbao, Spain
[2] Sorbonne Univ, Ecole Normale Super, Lab Meteorol Dynam LMD IPSL, Ctr Natl Rech Sci,Ecole Polytech, Paris, France
[3] Inst Planetary Res, German Aerosp Ctr DLR, Berlin, Germany
[4] ESA ESAC European Space Astron Ctr, Aurora Technol European Space Agcy, Madrid, Spain
[5] Inst Astrofis Andalucia CSIC, Granada, Spain
[6] Inst Astrophys & Space Sci, Observ Astron Lisboa, Lisbon, Portugal
来源：
SPACE SCIENCE REVIEWS | 2024年 / 220卷 / 01期
关键词：
Mars atmosphere; Mars Express; Atmosphere dynamics; STEREO CAMERA HRSC; DUST STORMS; CLOUDS; WATER; HEMISPHERE;
D O I：
10.1007/s11214-024-01047-4
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
This review describes the dynamic phenomena in the atmosphere of Mars that are visible in images taken in the visual range through cloud formation and dust lifting. We describe the properties of atmospheric features traced by aerosols covering a large range of spatial and temporal scales, including dynamical interpretations and modelling when available. We present the areographic distribution and the daily and seasonal cycles of those atmospheric phenomena. We rely primarily on images taken by cameras on Mars Express.
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页数：25
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