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Non-Ballistic Vapor-Driven EjectaImpact-induced vaporization is a key component of early-time cratering mechanics. Previous experimental [1,2] and computational [e.g., 3] studies focused on the generation and expansion of vapor clouds in an attempt to better understand vaporization in hypervelocity impacts. Presented here is a new experimental approach to the study of impact-induced vaporization. The three-dimensional particle image velocimetry (3D PIV) system captures interactions between expanding vapor phases and fine particulates. Particles ejected early in the cratering process may be entrained in expanding gas phases generated at impact, altering their otherwise ballistic path of flight. 3D PIV allows identifying the presence of such non-ballistic ejecta from very early times in the cratering process.
Document ID
20040062056
Acquisition Source
Johnson Space Center
Document Type
Conference Paper
Authors
Wrobel, K. E.
(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, 2004
Publication Information
Publication: Lunar and Planetary Science XXXV: Impacts: Observations and Experiments
Subject Category
Geophysics
Funding Number(s)
CONTRACT_GRANT: NAG5-11538
Distribution Limits
Public
Copyright
Public Use Permitted.
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