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Distribution of small volcanic cones on the surface of Venus by size and elevation: Implications for differential deposition of volcanic featuresIt appears that volcanic features are not evenly distributed on the surface of Venus. Head et. al. theorizes that the sparcity of volcanic features in the lowlands may be due to an altitude dependent inhibition of volatile exsolution and the resulting products of neutral buoyancy zones sufficient to form magma reservoirs and favoring flood lavas at lower elevation. The astronomy research classes of Evergreen and Sahuaro High Schools surveyed a cross-section of different elevation topography to investigate size and distribution of small volcanic cones by elevation. The results from this survey are presented.
Document ID
19940016258
Document Type
Conference Paper
Authors
Lockwood, J. F. (Sahuaro High School Tucson, AZ, United States)
Ellison, Mike (Sahuaro High School Tucson, AZ, United States)
Johnson, J. (Arizona Univ. Tucson., United States)
Kamatsu, G. (Arizona Univ. Tucson., United States)
Date Acquired
September 6, 2013
Publication Date
January 1, 1993
Publication Information
Publication: Lunar and Planetary Inst., Twenty-Fourth Lunar and Planetary Science Conference. Part 3: N-Z
Subject Category
LUNAR AND PLANETARY EXPLORATION
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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