favor the transport of noncondensable gases outside the polar region. Another aspect of the martian polar night atmosphere that is far from understood is the formation of CO 2 ice clouds and snowfall. Although it is thought that most of the carbonic ice directly condenses on the surface, a fraction...
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| Online Access: | http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.139.5736 http://www.biochem.wisc.edu/faculty/wickens/lab/publications/pdfs/Wickens_Gonzalez_2004_Science.pdf |
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ftciteseerx:oai:CiteSeerX.psu:10.1.1.139.5736 2023-05-15T18:02:12+02:00 The Pennsylvania State University CiteSeerX Archives application/pdf http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.139.5736 http://www.biochem.wisc.edu/faculty/wickens/lab/publications/pdfs/Wickens_Gonzalez_2004_Science.pdf en eng http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.139.5736 http://www.biochem.wisc.edu/faculty/wickens/lab/publications/pdfs/Wickens_Gonzalez_2004_Science.pdf Metadata may be used without restrictions as long as the oai identifier remains attached to it. http://www.biochem.wisc.edu/faculty/wickens/lab/publications/pdfs/Wickens_Gonzalez_2004_Science.pdf text ftciteseerx 2016-01-07T14:50:51Z favor the transport of noncondensable gases outside the polar region. Another aspect of the martian polar night atmosphere that is far from understood is the formation of CO 2 ice clouds and snowfall. Although it is thought that most of the carbonic ice directly condenses on the surface, a fraction should also condense in the atmosphere, strongly influencing the radiative properties of the atmosphere and the martian surface (3). Most of these clouds form in the polar night, and thus evidence of their existence has remained theoretical (4) or indirect (3). It is only with the advent of the Mars Global Surveyor laser altimeter Text polar night Unknown |
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ftciteseerx |
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English |
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favor the transport of noncondensable gases outside the polar region. Another aspect of the martian polar night atmosphere that is far from understood is the formation of CO 2 ice clouds and snowfall. Although it is thought that most of the carbonic ice directly condenses on the surface, a fraction should also condense in the atmosphere, strongly influencing the radiative properties of the atmosphere and the martian surface (3). Most of these clouds form in the polar night, and thus evidence of their existence has remained theoretical (4) or indirect (3). It is only with the advent of the Mars Global Surveyor laser altimeter |
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The Pennsylvania State University CiteSeerX Archives |
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Text |
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http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.139.5736 http://www.biochem.wisc.edu/faculty/wickens/lab/publications/pdfs/Wickens_Gonzalez_2004_Science.pdf |
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http://www.biochem.wisc.edu/faculty/wickens/lab/publications/pdfs/Wickens_Gonzalez_2004_Science.pdf |
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