NASA Logo

NTRS

NTRS - NASA Technical Reports Server

Back to Results
Oblique Impact Ejecta Flow Fields: An Application of Maxwells Z ModelOblique impact flow fields show an evolution from asymmetric to symmetric ejecta flow. This evolution can be put into the simple analytical description of the evolving flow field origin using the Maxwell Z Model. Additional information is contained in the original extended abstract.
Document ID
20010044692
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 20, 2013
Publication Date
January 1, 2001
Publication Information
Publication: Lunar and Planetary Science XXXII
Subject Category
Lunar And Planetary Science And Exploration
Funding Number(s)
CONTRACT_GRANT: NAG5-3877
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

Related Records

IDRelationTitle20010044353Analytic PrimaryLunar and Planetary Science XXXII
No Preview Available