A numerical study of convection in a condensing CO2 atmosphere under early mars-like conditions

Tatsuya Yamashita, Masatsugu Odaka, Ko Ichiro Sugiyama, Kensuke Nakajima, Masaki Ishiwatari, Seiya Nishizawa, Yoshiyuki O. Takahashi, Yoshi Yuki Hayashi

Research output: Contribution to journalArticle

Abstract

Cloud convection of a CO2 atmosphere where the major constituent condenses is numerically investigated under a setup idealizing a possible warm atmosphere of early Mars, utilizing a two-dimensional cloud-resolving model forced by a fixed cooling profile as a substitute for a radiative process. The authors compare two cases with different critical saturation ratios as condensation criteria and also examine sensitivity to number mixing ratio of condensed particles given externally. When supersaturation is not necessary for condensation, the entire horizontal domain above the condensation level is continuously covered by clouds irrespective of number mixing ratio of condensed particles. Horizontal-mean cloud mass density decreases exponentially with height. The circulations below and above the condensation level are dominated by dry cellular convection and buoyancy waves, respectively. When 1.35 is adopted as the critical saturation ratio, clouds appear exclusively as intense, short-lived, quasi-periodic events. Clouds start just above the condensation level and develop upward, but intense updrafts exist only around the cloud top; they do not extend to the bottom of the condensation layer. The cloud layer is rapidly warmed by latent heat during the cloud events, and then the layer is slowly cooled by the specified thermal forcing, and supersaturation gradually develops leading to the next cloud event. The periodic appearance of cloud events does not occur when number mixing ratio of condensed particles is large.

Original languageEnglish
Pages (from-to)4151-4169
Number of pages19
JournalJournal of the Atmospheric Sciences
Volume73
Issue number10
DOIs
Publication statusPublished - Jan 1 2016

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Mars
convection
atmosphere
condensation
mixing ratio
supersaturation
saturation
updraft
buoyancy
cooling

All Science Journal Classification (ASJC) codes

  • Atmospheric Science

Cite this

Yamashita, T., Odaka, M., Sugiyama, K. I., Nakajima, K., Ishiwatari, M., Nishizawa, S., ... Hayashi, Y. Y. (2016). A numerical study of convection in a condensing CO2 atmosphere under early mars-like conditions. Journal of the Atmospheric Sciences, 73(10), 4151-4169. https://doi.org/10.1175/JAS-D-15-0132.1

A numerical study of convection in a condensing CO2 atmosphere under early mars-like conditions. / Yamashita, Tatsuya; Odaka, Masatsugu; Sugiyama, Ko Ichiro; Nakajima, Kensuke; Ishiwatari, Masaki; Nishizawa, Seiya; Takahashi, Yoshiyuki O.; Hayashi, Yoshi Yuki.

In: Journal of the Atmospheric Sciences, Vol. 73, No. 10, 01.01.2016, p. 4151-4169.

Research output: Contribution to journalArticle

Yamashita, T, Odaka, M, Sugiyama, KI, Nakajima, K, Ishiwatari, M, Nishizawa, S, Takahashi, YO & Hayashi, YY 2016, 'A numerical study of convection in a condensing CO2 atmosphere under early mars-like conditions', Journal of the Atmospheric Sciences, vol. 73, no. 10, pp. 4151-4169. https://doi.org/10.1175/JAS-D-15-0132.1
Yamashita, Tatsuya ; Odaka, Masatsugu ; Sugiyama, Ko Ichiro ; Nakajima, Kensuke ; Ishiwatari, Masaki ; Nishizawa, Seiya ; Takahashi, Yoshiyuki O. ; Hayashi, Yoshi Yuki. / A numerical study of convection in a condensing CO2 atmosphere under early mars-like conditions. In: Journal of the Atmospheric Sciences. 2016 ; Vol. 73, No. 10. pp. 4151-4169.
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