Daily global mapping of Mars ozone column abundances with MARCI UV band imaging
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- 作者：R. Todd Clancya ; clancy@spacescience.org" class="auth_mail" title="E-mail the corresponding author ; Michael J. Wolffa ; Franck Lefè ; vreb ; Bruce A. Cantorc ; Michael C. Malinc ; Michael D. Smithd
- 关键词：Mars ; atmosphere ; Photochemistry ; Ultraviolet observations ; Atmospheres ; chemistry ; Mars
- 刊名：Icarus
- 出版年：2016
- 出版时间：1 March 2016
- 年：2016
- 卷：266
- 期：Complete
- 页码：112-133
- 全文大小：6544 K
文摘
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5 Mars years of MARCI daily global mapping ozone (O3) column retrievals presented.
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MARCI ozone maps display rotation and wave deformation of North Polar (NP) vortex.
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Winter/Spring transport from SP region drives Hellas Basin O3 and CO columns.
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Heterogeneous chemistry on Mars water ice clouds is not apparent in O3 behaviors.