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    Impact demagnetization of the Martian crust: Primaries versus secondaries

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    Name:
    Artemieva_et_al-2005-Geophysic ...
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    Author
    Artemieva, N.
    Hood, L.
    Ivanov, B. A.
    Affiliation
    Univ Arizona, Lunar & Planetary Lab
    Issue Date
    2005-11
    
    Metadata
    Show full item record
    Publisher
    AMER GEOPHYSICAL UNION
    Citation
    Impact demagnetization of the Martian crust: Primaries versus secondaries 2005, 32 (22):n/a Geophysical Research Letters
    Journal
    Geophysical Research Letters
    Rights
    Copyright 2005 by the American Geophysical Union.
    Collection Information
    This 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.
    Abstract
    Numerical 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.
    Note
    6 month embargo; Version of record online: 30 November 2005
    ISSN
    00948276
    DOI
    10.1029/2005GL024385
    Version
    Final published version
    Sponsors
    This work was supported by a grant from the NASA Mars Data Analysis Program.
    Additional Links
    http://doi.wiley.com/10.1029/2005GL024385
    ae974a485f413a2113503eed53cd6c53
    10.1029/2005GL024385
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