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- W2034451956 abstract "Abstract A magnetostatic boundary value problem has been solved within the magnetospheric cavity and in the interplanetary space in order to incorporate the interplanetary magnetic field in a quantitative magnetospheric vacuum- B -field model. The boundary condition for the closed model, B ⊥ = 0 at the magnetopause, is replaced by the condition that the normal component of the total field penetrates the boundary continuously. Penetration of the B -field depends on a ‘merging-constant’ C 0 , which is assumed to be independent of position on the magnetopause. C 0 = 0 indicates the closed model and C 0 = 1 describes, the complete interconnection between the magnetospheric and the interplanetary field. The model is valid for the field-line topology on the dayside including the polar cusp region. The position of the polar cusp's equatorial edge depends on the actual value of the merging constant C 0 and the orientation of the interplanetary magnetic field. Plasma-physical effects enter the model implicitly by the fact that a magnetopause shields the solar wind from the magnetospheric cavity. The static model neglects the hydrodynamic behaviour of the field-line merging process." @default.
- W2034451956 created "2016-06-24" @default.
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- W2034451956 date "1978-03-01" @default.
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- W2034451956 title "A static-state field-line reconnection model for the Earth's magnetosphere" @default.
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- W2034451956 doi "https://doi.org/10.1016/0021-9169(78)90052-1" @default.
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