Measurements of Lunar Magnetic Field Interaction with the Solar Wind

Details Measurements of Lunar Magnetic Field Interaction with the Solar Wind Measurements of Lunar Magnetic Field Interaction with the Solar Wind

Apr 1972

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1972natur.236..381d&link_type=abstract

Nature, Volume 236, Issue 5347, pp. 381-385 (1972).

Computer Science

6

Scientific paper

The remanent magnetic field at the lunar surface is compressed as much
as 40% above its initial value by the solar wind, but the total remanent
magnetic pressure is less than the stagnation pressure by a factor of
six, implying that a local shock is not formed.

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