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Night side electromagnetic response of the moon.The inductive response of the moon to interplanetary magnetic field fluctuations has been measured by the Apollo 12 lunar surface magnetometer. The dependence of the night side lunar response on frequency in the band from about 0.001 to 0.01 Hz is reported. It is shown that the night side response of the moon is not that of a sphere in vacuum. Instead, hydromagnetic radiation scattered from the moon is strongly confined to the interior of the cavity formed downstream from the moon in the solar wind.
Document ID
19730051466
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Schubert, G.
(California, University Los Angeles, Calif., United States)
Smith, B. F.
Sonett, C. P.
Colburn, D. S.
(NASA Ames Research Center Moffett Field, Calif., United States)
Schwartz, K.
Date Acquired
August 7, 2013
Publication Date
July 1, 1973
Publication Information
Publication: Journal of Geophysical Research
Volume: 78
Subject Category
Space Sciences
Accession Number
73A36268
Funding Number(s)
CONTRACT_GRANT: NAS2-6876
Distribution Limits
Public
Copyright
Other

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