The lunar lithosphere from electromagnetic-sounding data

Details The lunar lithosphere from electromagnetic-sounding data The lunar lithosphere from electromagnetic-sounding data

Sep 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977moon...17....3v&link_type=abstract

The Moon, vol. 17, Sept. 1977, p. 3-9. Translation.

Computer Science

Sound

3

Electrical Resistivity, Lithosphere, Lunar Crust, Solar Wind, Astronomical Models, Diurnal Variations, Frequency Response, Lunar Core, Lunar Magnetic Fields, Magnetic Variations, Solar Activity Effects, Sounding

Scientific paper

Published data are examined and found to be consistent with a model of the lunar lithosphere in which resistivity of several hundred ohm-m to a depth of 700-800 km is assumed. The analysis of the data indicates the probable absence of significant amounts of molten material at these depths. Four sets of published data were studied: frequency dependence of the day-side horizontal magnetic amplification, frequency dependence for the dark-side vertical decrease, the day-side transient amplification, and the dark-side transient decrease. All data are converted to the form of the day-side frequency response.

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