Magnetohydrodynamical winds with Finite Electrical Conductivities
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概要
- 論文の詳細を見る
We discuss a numerical treatment of the resistive. MHD winds which are driven by strongly magnetized, rotating stars. For simplicity, the axis of rotation is assumed to coincide with that of magnetization. It is shown that rotation-driven wind solutions surely exist, to the set of resistive MHD equations even when the stellar magnetic fields remain of closed type.Magnetohydrodynamics(MHD)resistive MHDstellar windscentrifugal force
- 東北大学の論文
- 1991-01-31
著者
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KUDOH Takahiro
Astronomical Data Analysis Center, National Astronomical Observatory
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Kudoh Takahiro
Astronomical Institute Faculty Of Science Tohoku University
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KABURAKI Osamu
Astronomical Institute, Faculty of Science, Tohoku University
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Kaburaki Osamu
Astronomical Institute Faculty Of Science Tohoku University
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