During the time period 1961-1972 eleven magnetometers were sent to the moon. The results of lunar magnetometer data analysis are reviewed, with emphasis on the lunar interior. Magnetic fields have been measured on the lunar surface at the Apollo 12, 14, 15, and 16 landing sites. The remanent field values at these sites are given. Satellite and surface measurements show strong evidence that the lunar crust is magnetized over much of the lunar globe. The origin of the lunar remanent field is not yet satisfactorily understood; several source models are presented. Simultaneous data from the Apollo 12 lunar surface magnetometer and the Explorer 35 Ames magnetometer are used to construct a wholemoon hysteresis curve, from which the global lunar permeability is determined. Total iron abundance is calculated for two assumed compositional models of the lunar interior. Other lunar models with a small iron core and with a shallow iron-rich layer are also discussed in light of the measured global permeability.


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    Titel :

    Magnetism and the interior of the moon


    Beteiligte:
    Dyal, P. (Autor:in) / Parkin, C. W. (Autor:in) / Daily, W. D. (Autor:in)

    Erscheinungsdatum :

    01.01.1974


    Medientyp :

    Report


    Format :

    Keine Angabe


    Sprache :

    Englisch


    Schlagwörter :


    The magnetism of the moon

    Dyal, P. / Parkin, C. W. | NTRS | 1971


    Moon and its interior

    MacDonald, G.J.F. | Engineering Index Backfile | 1962


    The interior of the Moon

    Anderson, D. L. | NTRS | 1974


    Damping device for interior of moon pool of drilling ship

    DING YONG / JI YUAN / DUAN FEI et al. | Europäisches Patentamt | 2015

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