| 扇形边界附近太阻风粘性的数学描写和物理效应 |
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| 引用本文： | 赵学溥,Thomas E.Holzer.扇形边界附近太阻风粘性的数学描写和物理效应[J].地球物理学报,1987,30(3):219-225. |
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| 作者姓名： | 赵学溥 Thomas E.Holzer |
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| 作者单位： | 1. 北京大学地球物理系;
2. High Altitude Observator, U. S. A |
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| 摘 要： | 本文首先指出经典粘性理论应适用于扇形边界低速风,接着论证了常用太阳风粘性数学表式的不正确性,导出了螺旋磁场中径向球对称强磁化等离子体流动的各种经典粘性表式,并证明了这些公式的合理性;最后讨论了常用太阳风经典粘性表式出错原因,估计了具有正确粘性公式的扇形边界低速太阳风粘性模式应有的结果。
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| 关 键 词： | 扇形边界 太阳风 经典粘性 |
| 收稿时间： | 1986-04-01 |
MATHEMATICAL DESCRIPTIONS AND PHYSICAL EFFECTS OF THE CLASSICAL VISCOSITY IN THE SOLAR WIND NEAR THE SECTOR BOUNDARIES |
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| ZHAO XUE-PU.MATHEMATICAL DESCRIPTIONS AND PHYSICAL EFFECTS OF THE CLASSICAL VISCOSITY IN THE SOLAR WIND NEAR THE SECTOR BOUNDARIES[J].Chinese Journal of Geophysics,1987,30(3):219-225. |
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| Authors: | ZHAO XUE-PU |
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| Institution: | 1. Department of Geophysics, Peking University, Beijing;
2. High Altitude Observatory, U. S. A |
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| Abstract: | The questions existing in both the formulas of the radial viscous force and heating and the formula of the corrected viscous stress by the magnetic field in the, solar wind viscous models are proposed. The various viscous formulas for .the radial and spherical-symmetric plasma flow in the Parker's spiral configuration of the interplanetary magnetic field have been derived. The cause which makes the commonly used expressions incorrect and the possible results of the new solar wind viscous model in the present paper are discussed. |
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| Keywords: | Sector boundary Solar wind Classical viscosity |
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