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Mapping of lunar surface remanent magnetic fields by electron scatteringThe electron scattering technique for measurement of lunar surface remanent magnetic fields is described and a map of the remanent field regions derived from the 14-keV electron measurements of the particle experiment aboard the Apollo 16 Subsatellite is presented. The mapping achieves a spatial resolution of about 40 km and a sensitivity of about 0.1 gamma at the lunar surface.
Document ID
19780062868
Acquisition Source
Legacy CDMS
Document Type
Conference Proceedings
Authors
Lin, R. P. (California Univ. Berkeley, CA, United States)
Mcguire, R. E. (California Univ. Berkeley, CA, United States)
Howe, H. C. (California Univ. Berkeley, CA, United States)
Anderson, K. A. (California, University Berkeley, Calif., United States)
Mccoy, J. E. (NASA Johnson Space Center Houston, Tex., United States)
Date Acquired
August 9, 2013
Publication Date
January 1, 1975
Subject Category
Lunar And Planetary Exploration
Meeting Information
Meeting: Lunar Science Conference
Location: Houston, TX
Start Date: March 17, 1975
End Date: March 21, 1975
Accession Number
78A46777
Funding Number(s)
CONTRACT_GRANT: NSG-7127
CONTRACT_GRANT: NGL-05-003-017
Distribution Limits
Public
Copyright
Other

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