Abstract Recent hypervelocity studies have been conducted which simulate the collision of interplanetary dust with rocky planetary satellite surfaces. Preliminary flux-mass distributions of micron and submicron ejecta from these hypervelocity impact studies have been determined. Several models of the flux-mass distribution of primary interplanetary dust are used to determine ratios of satellite surface ejecta and primary meteoroid flux-mass distributions. The results are used in a second model to determine the ejecta spatial mass densities near the surface of the satellite.


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    Titel :

    Mass loading of planetary magnetospheres by rocky satellites—I: Production of rocky ejecta


    Beteiligte:
    Alexander, M. (Autor:in) / Anz, P. (Autor:in) / Lyons, D. (Autor:in) / Tanner, W. (Autor:in) / Chen, Y.-L. (Autor:in) / McDonnell, J.A.M. (Autor:in)

    Erschienen in:

    Erscheinungsdatum :

    1984-01-01


    Format / Umfang :

    4 pages




    Medientyp :

    Aufsatz (Zeitschrift)


    Format :

    Elektronische Ressource


    Sprache :

    Englisch




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