Astronomy and Astrophysics – Astronomy
Scientific paper
Jan 1989
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989pazh...15...89d&link_type=abstract
Pis'ma v Astronomicheskii Zhurnal (ISSN 0320-0108), vol. 15, Jan. 1989, p. 89-94. In Russian. In Russian.
Astronomy and Astrophysics
Astronomy
Lunar Core, Lunar Magnetic Fields, Lunar Mantle, Chemical Composition, Inhomogeneity, Temperature Profiles
Scientific paper
It is suggested that observed local (about 100 km) magnetic fields on the moon and the relatively large field at its initial stage of evolution are due to the temperature and compositional inhomogenities of the inner regions of the moon. The importance of this type of inhomogeneity at the core-mantle boundary to the process of terrestrial magnetic field generation is demonstrated.
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