Analysis of recent data from lunar seismic events shows significant deviations of P- and S-wave travel times from those expected if the lunar interior were homogeneous below the crust. The interpretation of these data results in a lunar model consisting of at least four and possibly five distinguishable zones whose probable characteristics are discussed.


    Zugriff

    Zugriff über TIB

    Verfügbarkeit in meiner Bibliothek prüfen


    Exportieren, teilen und zitieren



    Titel :

    Deep lunar interior inferred from recent seismic data


    Beteiligte:
    Nakamura, Y. (Autor:in) / Latham, G. (Autor:in) / Lammlein, D. (Autor:in) / Ewing, M. (Autor:in) / Duennebier, F. (Autor:in) / Dorman, J. (Autor:in)


    Erscheinungsdatum :

    1974-07-01


    Medientyp :

    Sonstige


    Format :

    Keine Angabe


    Sprache :

    Englisch


    Schlagwörter :


    Recent Re-Analyses of the Apollo Lunar Seismic Data: Insight into the Moons Deep Interior

    Weber, Renee / Garcia, Raphael / Lin, Pei-Ying | NTRS | 2017



    New seismic data on the state of the deep lunar interior.

    Nakamura, Y. / Lammlein, D. / Latham, G. et al. | NTRS | 1973


    Lunar Love Numbers and the Deep Lunar Interior

    Williams, J. G. / Boggs, D. H. / Ratcliff, J. T. et al. | NTRS | 2002


    Lunar love numbers and the deep lunar interior

    Dickey, J. O. / Ratcliff, J. T. / Boggs, D. H. et al. | NTRS | 2002