NASA NTRS · 20010044692
Oblique Impact Ejecta Flow Fields: An Application of Maxwells Z Model
Abstract
Oblique 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.
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Anderson, J. L. B., Schultz, P. H., Heineck, J. T.. 2001-01-01. Oblique Impact Ejecta Flow Fields: An Application of Maxwells Z Model. https://ntrs.nasa.gov/citations/20010044692
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