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• W2292015100 abstract "The solution to the problem of the motion of the Moon relative to spatial irregularities in the interplanetary magnetic field is found. The lunar electrical conductivity is modeled by a two- layer conductivity profile. For the interaction of the Moon with the corotating sector structure of the interplanetary magnetic field it is found that the magnetic field in the lunar shell is the super- position of an oscillatory uniform field, an oscillatory dipole field and an oscillatory fieM that is toroidal about the axis of the motionat electric field. With various lunar conductivity models and the theory of this paper, lunar surface magnetometer data can be quantitatively interpreted to yield information on the conductivity and consequently the temperature of the lunar core. The electromagnetic interaction of the Moon and the solar wind plasma has been considered by several authors. Sonett and Colburn (1967, 1968) described the steady state electromagnetic interaction of a Moon with electrical conductivity a moving with velocity v relative to a constant magnetic field B in terms of a unipolar generator. For an infinitely conducting plasma, an observer moving with the Moon would measure a magnetic field B and an electric field v x B in the solar wind. The electric field within the homogeneous Moon is everywhere the motional field v x B. Thus currents, whose density is av x B, flow in the lunar interior and produce an induced magnetic field which is toroidal with respect to the direction of the motional electric field. Currents at the Moon-plasma boundary provide for the completion of closed current paths. Hollweg (1968) has applied this steady state solution to a Moon with a two-layer electrical conductivity model, i.e. a core of constant electrical conductivity a c surrounded by a shell of constant electrical conductivity a s. The two-layer con- ductivity model provides a simple method of accounting for the possibility that the lunar electrical conductivity may change by several orders of magnitude between the Moon's surface and its interior (England et al., 1968). The quasi-periodic sector structure of the interplanetary magnetic field necessitates consideration of the time-dependent electromagnetic interaction problem. The relative motion of the Moon with respect to spatial irregularities in the incident interplanetary magnetic field produces time-dependent electric and magnetic field fluctuations in the * Presently visiting the Max-Planck-Institut ffir Physik und Astrophysik, Mfinchen, Germany." @default.
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• W2292015100 date "1969-01-01" @default.
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• W2292015100 title "LUNAR S URFACE M AGNETOMETER D ATA" @default.
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