It is now apparent that windblown sand plays a major role in the Martian environment. The existence of great sand and dust storms implies the lateral transport of large quantities of material on Mars that provide a convenient mechanism for the filling of craters- an event directly implied both by crater frequency-diameter statistics, and by the appearance of Martian craters. Such fast moving sand particles, saltating close to the Martian surface, can produce by collision and subsequent abrasion significant erosion of the Martian terrain.


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    Titel :

    Sandstorms and eolian erosion on Mars


    Beteiligte:
    Sagan, C. (Autor:in)


    Erscheinungsdatum :

    15.07.1973


    Medientyp :

    Sonstige


    Format :

    Keine Angabe


    Sprache :

    Englisch


    Schlagwörter :


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    Tanaka, K. L. / Leonard, G. J. / Lunar and Planetary Institute| National Aeronautics and Space Administration| Universities Space Research Association | British Library Conference Proceedings | 1994




    Measurement of Equivalent Dielectric Parameters of Sandstorms from the Microwave Attenuation

    Yan, Y. / Huang, J. Y. | British Library Online Contents | 2000