Solar wind interaction with the moon - Enhanced magnetic field fluctuations at low altitudes

Details Solar wind interaction with the moon - Enhanced magnetic field fluctuations at low altitudes Solar wind interaction with the moon - Enhanced magnetic field fluctuations at low altitudes

Jul 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978georl...5..592w&link_type=abstract

Geophysical Research Letters, vol. 5, July 1978, p. 592-594.

Physics

Lunar Magnetic Fields, Magnetic Disturbances, Plasma Turbulence, Solar Wind, Analysis Of Variance, Apollo Flights, Histograms, Interplanetary Magnetic Fields, Moon, Solar Wind, Interactions, Magnetic Fields, Particles, Perturbations, Surface

Scientific paper

Evidence of a magnetically turbulent region above the lunar dayside is
presented. This region apparently exists when the moon is in the solar
wind and is approximately 100 kms thick. Possible explanations for the
presence of a dayside turbulent sheath are investigated and, to within
the accuracy of the data, none can satisfactorily explain its presence.

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