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- W1674592052 abstract "The stationary models by E.N.Parker for the magnetic field in the solar wind and by K.H.Schatten for the “source surface” in the solar corona are generalized. The configuration of the interplanetary magnetic field, stretched by the expanding corona, depends on the magnitude of the electrical conductivity ó of the solar wind plasma. Knowing the main empirical features of the field configuration, one may estimate the phenomenological value of ó. The estimates show that the electrical conductivity should be approximately 1013 times smaller than that calculated by Spitzer." @default.
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- W1674592052 date "1992-01-01" @default.
- W1674592052 modified "2023-09-23" @default.
- W1674592052 title "MAGNETIC FIELD OF THE SOLAR WIND: A STATIONARY KINEMATIC SOLUTION WITH A FINITE ELECTRIC CONDUCTIVITY" @default.
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- W1674592052 doi "https://doi.org/10.1016/b978-0-08-042049-3.50036-3" @default.
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