Computer Science – Numerical Analysis
Scientific paper
Jan 1975
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975phdt.........2l&link_type=abstract
Ph.D. Thesis. Final Report Massachusetts Inst. of Tech., Cambridge. Dept. of Earth and Planetary Sciences.
Computer Science
Numerical Analysis
Apollo 12 Flight, Electrical Resistivity, Electromagnetic Fields, Explorer 35 Satellite, Lunar Magnetic Fields, Field Strength, Lunar Surface, Magnetometers, Mathematical Models, Numerical Analysis, Solar Wind
Scientific paper
The electrical conductivity structure was studied of a spherically layered moon consistent with the very low frequency magnetic data collected on the lunar surface and by Explorer 35. In order to obtain good agreement with the lunar surface magnetometer observations, the inclusion of a void cavity behind the moon requires a conductivity at shallow depths higher than that of models having the solar wind impinging on all sides. By varying only the source parameters, a conductivity model can be found that yields a good fit to both the tangential response upstream and the radial response downstream. This model also satisfies the dark side tangential response in the frequency range above 0.006 Hz, but the few data points presently available below this range do not seem to agree with the theory.
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