Abstract
AbstractThis 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.
Funder
Ministerio de Ciencia, Innovación y Universidades
Eusko Jaurlaritza
Universidad del País Vasco
Publisher
Springer Science and Business Media LLC
Reference97 articles.
1. Altieri F, Spiga A, Zasova L, Bellucci G, Bibring JP (2012) Gravity waves mapped by the OMEGA/MEX instrument through O2 dayglow at 1.27 μm: data analysis and atmospheric modeling. J Geophys Res, Planets 117(11):E00J08. https://doi.org/10.1029/2012JE004065
2. Arya A.S. et al. (2015) Mars color camera onboard Mars orbiter mission: initial observations and results. In: 46th lunar and planetary science conference LPSC 2123. The Woodlands, TX. Retrieved from https://www.hou.usra.edu/meetings/lpsc2015/pdf/2123.pdf
3. Ball ER, Mitchell DM, Seviour WJM, Thomson SI, Vallis GK (2021) The roles of latent heating and dust in the structure and variability of the northern Martian polar vortex. Planet Sci J 2:203. https://doi.org/10.3847/PSJ/ac1ba2
4. Balme M, Greeley R (2006) Dust devils on Earth and Mars. Rev Geophys 44(3):RG3003. https://doi.org/10.1029/2005RG000188
5. Banfield D, Conrath BJ, Gierasch PJ, Wilson RJ, Smith MD (2004) Traveling waves in the Martian atmosphere from MGS TES nadir data. Icarus 170(2):365–403. https://doi.org/10.1016/j.icarus.2004.03.015
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