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dc.contributor.authorArtemieva, N.
dc.contributor.authorHood, L.
dc.contributor.authorIvanov, B. A.
dc.date.accessioned2017-05-02T23:27:18Z
dc.date.available2017-05-02T23:27:18Z
dc.date.issued2005-11
dc.identifier.citationImpact demagnetization of the Martian crust: Primaries versus secondaries 2005, 32 (22):n/a Geophysical Research Lettersen
dc.identifier.issn00948276
dc.identifier.doi10.1029/2005GL024385
dc.identifier.urihttp://hdl.handle.net/10150/623349
dc.description.abstractNumerical simulations presented here show that demagnetization of crust near the largest Martian basins by secondary impacts can be comparable to that by direct shock waves outside the transient cavity. The relative input from secondary impacts, which demagnetize only the uppermost layers, depends on the magnetic carrier distribution within the crust. Thus, we discuss properties of likely magnetic remanence carriers and their possible spatial distribution within the crust.
dc.description.sponsorshipThis work was supported by a grant from the NASA Mars Data Analysis Program.en
dc.language.isoenen
dc.publisherAMER GEOPHYSICAL UNIONen
dc.relation.urlhttp://doi.wiley.com/10.1029/2005GL024385en
dc.rightsCopyright 2005 by the American Geophysical Union.en
dc.titleImpact demagnetization of the Martian crust: Primaries versus secondariesen
dc.typeArticleen
dc.contributor.departmentUniv Arizona, Lunar & Planetary Laben
dc.identifier.journalGeophysical Research Lettersen
dc.description.note6 month embargo; Version of record online: 30 November 2005en
dc.description.collectioninformationThis item from the UA Faculty Publications collection is made available by the University of Arizona with support from the University of Arizona Libraries. If you have questions, please contact us at repository@u.library.arizona.edu.en
dc.eprint.versionFinal published versionen
dc.contributor.institutionInstitute for Dynamics of Geospheres; Moscow Russia
dc.contributor.institutionLunar and Planetary Laboratory; University of Arizona; Tucson Arizona USA
dc.contributor.institutionInstitute for Dynamics of Geospheres; Moscow Russia
refterms.dateFOA2006-05-31T00:00:00Z
html.description.abstractNumerical simulations presented here show that demagnetization of crust near the largest Martian basins by secondary impacts can be comparable to that by direct shock waves outside the transient cavity. The relative input from secondary impacts, which demagnetize only the uppermost layers, depends on the magnetic carrier distribution within the crust. Thus, we discuss properties of likely magnetic remanence carriers and their possible spatial distribution within the crust.


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