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Water vapor, water-ice clouds, and dust in the North Polar RegionThe behavior of water vapor, water-ice and dust in the Martian atmosphere is important for understanding the overall Martian climate system, which is characterized by three main cycles: water, including water-ice, dust, and CO2. Understanding these cycles will lend insight into the behavior of the atmospheric dynamics, the atmosphere's ability to transport dust, water-ice, and vapor to different parts of the planet, and how that ability changes as a function of dust and water-ice loading.
Document ID
20060043675
Acquisition Source
Jet Propulsion Laboratory
Document Type
Conference Paper
External Source(s)
Authors
Tamppari, Leslie K.
Smith, Michael D.
Bass, Deborah S.
Hale, Amy S.
Date Acquired
August 23, 2013
Publication Date
February 27, 2006
Meeting Information
Meeting: Mars Atmospheric Models and Observations
Location: Granada
Country: Spain
Start Date: February 27, 2006
End Date: March 3, 2006
Distribution Limits
Public
Copyright
Other
Keywords
water vapors
water-ice clouds
dust
Mars

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