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Cratering flow fields: Implications for the excavation and transient expansion stages of crater formation

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dc.contributor.author Croft, Steven Kent
dc.date.accessioned 2020-08-06T20:17:19Z
dc.date.available 2020-08-06T20:17:19Z
dc.date.issued 1980
dc.identifier.citation Proc. Lunar Planet. Sci. Conf. 11th (1980), p. 2347-2378. en
dc.identifier.uri https://hdl.handle.net/20.500.11753/1670
dc.description.abstract A Maxwell Z-model cratering flow field originating at non-zero depths-of-burst has been used to calculate theoretical depths and volumes of excavation, hinge radii, ejection angles, and transient structural rim uplifts for comparison with experimental and field data from impact and explosion craters. en
dc.format.extent Pages 2347-2378
dc.format.mimetype application/pdf
dc.language.iso en en
dc.publisher Pergamon Press en
dc.relation.ispartofseries LPI contribution ; no. 421
dc.subject Cratering en
dc.title Cratering flow fields: Implications for the excavation and transient expansion stages of crater formation en
dc.type Book chapter en


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