Volume 11 Issue 3
Aug.  1991
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Guo Wei-ping, Wang Jing-fang, Yao Yong-qiao, Liang Bai-xian. THE STRUCTURE OF THE MERIDIAN SOLAR WIND AND ITS EFFECT ON THE PROPAGATION OF CORONALMASS EJECTIONS[J]. Journal of Space Science, 1991, 11(3): 168-175. doi: 10.11728/cjss1991.03.168
Citation: Guo Wei-ping, Wang Jing-fang, Yao Yong-qiao, Liang Bai-xian. THE STRUCTURE OF THE MERIDIAN SOLAR WIND AND ITS EFFECT ON THE PROPAGATION OF CORONALMASS EJECTIONS[J]. Journal of Space Science, 1991, 11(3): 168-175. doi: 10.11728/cjss1991.03.168

THE STRUCTURE OF THE MERIDIAN SOLAR WIND AND ITS EFFECT ON THE PROPAGATION OF CORONALMASS EJECTIONS

doi: 10.11728/cjss1991.03.168
  • Received Date: 1990-07-02
  • Rev Recd Date: 1900-01-01
  • Publish Date: 1991-08-24
  • Acombined scheme is developed to solve the ideal MHDequations. Keeping certain precision, this model has ensured stability and small computing capacity. Atwo-dimensional hemlet-streamer solution of the meridian solar wind near the sun is obtained. Using this solution as initial state, the effect of the hemlet-streamer configuration on the propagation of coronal mass ejections is investigated. It is found that the configuration deflects the ejected mass toward equator. This effect can explain some observational results satisfactorily.

     

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