Radar has the unique capability of looking under the dry and cold surfaces of Mars. The depth of penetration of radio waves depends on a number of surface and subsurface parameters such as surface topography, subsurface geological structure and surface and subsurface electromagnetic properties. Among these parameters, the surface topography is known best largely due to valuable data provided by Mars Global Surveyor's MOLA instrument. However, little information is available on the electromagnetic properties and subsurface characteristics of Mars.


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    Titel :

    Radar Sounding of Mars: A Focus on MARSIS


    Beteiligte:
    Safaeinili, A. (Autor:in) / Biccari, D. (Autor:in) / Bombaci, O. (Autor:in) / Gurnett, D. (Autor:in) / Johnson, W. T. K. (Autor:in) / Jordan, R. L. (Autor:in) / Orosei, R. (Autor:in) / Picardi, G. (Autor:in) / Plaut, J. (Autor:in) / Seu, R. (Autor:in)

    Kongress:

    Conference on the Geophysical Detection of Subsurface Water on Mars ; 2001 ; Houston, TX, United States


    Erscheinungsdatum :

    2001-08-06


    Medientyp :

    Aufsatz (Konferenz)


    Format :

    Keine Angabe


    Sprache :

    Englisch




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