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ANGEO | Articles | Volume 36, issue 6
Ann. Geophys., 36, 1631-1646, 2018
https://doi.org/10.5194/angeo-36-1631-2018
© Author(s) 2018. This work is distributed under
the Creative Commons Attribution 4.0 License.
Ann. Geophys., 36, 1631-1646, 2018
https://doi.org/10.5194/angeo-36-1631-2018
© Author(s) 2018. This work is distributed under
the Creative Commons Attribution 4.0 License.

Regular paper 06 Dec 2018

Regular paper | 06 Dec 2018

Influence of gravity waves on the climatology of high-altitude Martian carbon dioxide ice clouds

Erdal Yiğit et al.
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Cited articles  
Ando, H., Imamura, T., and Tsuda, T.: Vertical wavenumber spectra of gravity waves in the Martian atmosphere obtained from Mars Global Surveyor radio occultation data, J. Atmos. Sci., 69, 2906–2912, https://doi.org/10.1175/JAS-D-11-0339.1, 2012. a
Aoki, S.,  Sato, Y.,  Giuranna, M.,  Wolkenberg, P.,  Sato, T.,  Nakagawa, H., and  Kasaba, Y.: Mesospheric CO2 ice clouds on Mars observed by Planetary Fourier Spectrometer onboard Mars Express, Icarus, 302, 175–190, https://doi.org/10.1016/j.icarus.2017.10.047, 2018. a
Brecht, A., Bougher, S. W., and  Yiğit, E.: Parameterizing gravity waves and understanding their impacts on venus' upper atmosphere, in 52nd ESLAB Symposium, Noordwijk, Netherlands, May, 2018. a
Clancy, R. T. and Sandor, B. J.: CO2 ice clouds in the upper atmosphere of Mars, Geophys. Res. Lett., 25, 489–492, 1998. a, b
Clancy, R. T., Wolff, M. J., Whitney, B. A., Cantor, B. A., and Smith, M. D.: Mars equatorial mesospheric clouds: Global occurrence and physical properties from mars global surveyor thermal emission spectrometer and mars orbiter camera limb observations, J. Geophys. Res., 112, E04004, https://doi.org/10.1029/2006JE002805, 2007. a, b
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Short summary
Carbon dioxide (CO2) clouds have been frequently observed in the Martian middle atmosphere. There are still uncertainties concerning the formation of the clouds. Using an atmospheric model for Mars, including a gravity wave parameterization, we assess the role of gravity waves in cloud formation. Simulations suggest that gravity wave processes constitute a necessary physical mechanism for CO2 cloud formation in the Martian upper atmosphere during all seasons.
Carbon dioxide (CO2) clouds have been frequently observed in the Martian middle atmosphere....
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