NASA NTRS · 19780062868
Mapping of lunar surface remanent magnetic fields by electron scattering
Abstract
The 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.
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Lin, R. P., Mcguire, R. E., Howe, H. C., Anderson, K. A., Mccoy, J. E.. 1975-01-01. Mapping of lunar surface remanent magnetic fields by electron scattering. https://ntrs.nasa.gov/citations/19780062868
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