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dc.contributor.authorShuvalov, V.
dc.date.accessioned2021-02-12T22:53:47Z
dc.date.available2021-02-12T22:53:47Z
dc.date.issued2009-01-01
dc.identifier.citationShuvalov, V. (2009). Atmospheric erosion induced by oblique impacts. Meteoritics & Planetary Science, 44(8), 1095-1105.
dc.identifier.issn1945-5100
dc.identifier.doi10.1111/j.1945-5100.2009.tb01209.x
dc.identifier.urihttp://hdl.handle.net/10150/656598
dc.description.abstractPrevious investigations of impact-induced atmospheric erosion considered vertical impacts only. Numerical simulations of oblique impacts presented in this paper show that the loss of air strongly depends on trajectory inclination and it increases as the impact angle decreases. The results of numerical simulations over the wide range of impact parameters (projectile sizes from 1 to 30 km, impact velocities from 15 to 70 km/s, escape velocities from 5 to 11.2 km/s, projectile densities from 1 to 3.3 g/cm3, normal atmospheric densities varying by three orders of magnitude) can be approximated by simple analytical formulae.
dc.language.isoen
dc.publisherThe Meteoritical Society
dc.relation.urlhttps://meteoritical.org/
dc.rightsCopyright © The Meteoritical Society
dc.rights.urihttp://rightsstatements.org/vocab/InC/1.0/
dc.subjectimpact modeling
dc.subjectMartian atmosphere
dc.subjectEarth
dc.subjectasteroid impacts
dc.titleAtmospheric erosion induced by oblique impacts
dc.typeArticle
dc.typetext
dc.identifier.journalMeteoritics & Planetary Science
dc.description.collectioninformationThe Meteoritics & Planetary Science archives are made available by the Meteoritical Society and the University of Arizona Libraries. Contact lbry-journals@email.arizona.edu for further information.
dc.eprint.versionFinal published version
dc.description.admin-noteMigrated from OJS platform February 2021
dc.source.volume44
dc.source.issue8
dc.source.beginpage1095
dc.source.endpage1105
refterms.dateFOA2021-02-12T22:53:47Z


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