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01/14/2009 - Laboratory Studies of Water Ice Cloud formation under Martian Conditions

 
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内容由SETI Institute Colloquium Series Videos提供。所有播客内容(包括剧集、图形和播客描述)均由 SETI Institute Colloquium Series Videos 或其播客平台合作伙伴直接上传和提供。如果您认为有人在未经您许可的情况下使用您的受版权保护的作品,您可以按照此处概述的流程进行操作https://zh.player.fm/legal

Dr. Laura T. Iraci, NASA Ames Research Center

Water ice clouds are an important part of the martian hydrological cycle, influencing the water and energy budgets. Microphysical models can be used to study the connections between cloud formation and water distribution throughout the system (for example, as surface frost layers), but only if the intricacies of cloud formation and growth are understood and properly parameterized. To that end, we have performed laboratory studies of water ice nucleation on a variety of surrogate materials and have found that initiation of ice is more difficult than often presumed. We will report these results, along with preliminary growth rate observations.

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Manage episode 121133764 series 103556
内容由SETI Institute Colloquium Series Videos提供。所有播客内容(包括剧集、图形和播客描述)均由 SETI Institute Colloquium Series Videos 或其播客平台合作伙伴直接上传和提供。如果您认为有人在未经您许可的情况下使用您的受版权保护的作品,您可以按照此处概述的流程进行操作https://zh.player.fm/legal

Dr. Laura T. Iraci, NASA Ames Research Center

Water ice clouds are an important part of the martian hydrological cycle, influencing the water and energy budgets. Microphysical models can be used to study the connections between cloud formation and water distribution throughout the system (for example, as surface frost layers), but only if the intricacies of cloud formation and growth are understood and properly parameterized. To that end, we have performed laboratory studies of water ice nucleation on a variety of surrogate materials and have found that initiation of ice is more difficult than often presumed. We will report these results, along with preliminary growth rate observations.

Watch video

  continue reading

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