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Subsatellite measurements of the lunar magnetic fieldThe Apollo 15 subsatellite magnetometer data have been used to map the lunar magnetic field over a narrow band of the lunar surface. Within this band the magnetic field is generally stronger and more variable over the farside highlands than the nearside maria. The correspondence between the strong variable lunar field regions and the source regions for limb compressions suggests that limb compressions arise as the result of the deflection of the solar wind just upstream of the terminator by the lunar magnetic field. Using this apparent relationship between field strength and limb compression source regions, it is deduced that the field strength in the northern farside highlands is not as strong as in the southern hemisphere at similar longitudes. Simultaneous measurements of the interplanetary magnetic field obtained by Explorer 35 and the Apollo 15 subsatellite above the dayside hemisphere are essentially identical. Thus, both instruments are measuring the undisturbed interplanetary field.
Document ID
19740040252
Acquisition Source
Legacy CDMS
Document Type
Conference Proceedings
Authors
Russell, C. T.
Coleman, P. J., Jr.
Lichtenstein, B. R.
Schubert, G.
Sharp, L. R.
(California, University Los Angeles, Calif., United States)
Date Acquired
August 7, 2013
Publication Date
January 1, 1973
Subject Category
Space Sciences
Meeting Information
Meeting: Lunar Science Conference
Location: Houston, TX
Start Date: March 5, 1973
End Date: March 8, 1973
Accession Number
74A23002
Funding Number(s)
CONTRACT_GRANT: NAS9-12236
CONTRACT_GRANT: NGR-05-007-351
Distribution Limits
Public
Copyright
Other

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