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The Evolution of Oblique Impact Flow Fields Using Maxwell's Z ModelOblique impacts are the norm rather than the exception for impact craters on planetary surfaces. This work focuses on the excavation of experimental oblique impact craters using the NASA Ames Vertical Gun Range (AVGR). Three-dimensional particle image velocimetry (3D PIV) is used to obtain quantitative data on ejection positions, three-dimensional velocities and angles. These data are then used to test the applicability and limitations of Maxwell's Z Model in representing the subsurface evolution of the excavation-stage flow-field center during vertical and oblique impacts.
Document ID
20030080019
Acquisition Source
Johnson Space Center
Document Type
Conference Paper
Authors
Anderson, J. L. B. (Brown Univ. Providence, RI, United States)
Schultz, P. H. (Brown Univ. Providence, RI, United States)
Heineck, J. T. (NASA Ames Research Center Moffett Field, CA, United States)
Date Acquired
August 21, 2013
Publication Date
January 1, 2003
Publication Information
Publication: Results of the Workshop on Impact Cratering: Bridging the Gap Between Modeling and Observations
Subject Category
Lunar And Planetary Science And Exploration
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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IDRelationTitle20030079993Collected WorksResults of the Workshop on Impact Cratering: Bridging the Gap Between Modeling and Observations
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