Volume 16 Issue 2
Apr.  1996
Turn off MathJax
Article Contents
Zhang GOng-liang. A Sun-ALFVENIC FLOW IN THE STRONG INTERPLANETARY MAGNETIC FIELD STRUCTURE[J]. Journal of Space Science, 1996, 16(2): 92-96. doi: 10.11728/cjss1996.02.092
Citation: Zhang GOng-liang. A Sun-ALFVENIC FLOW IN THE STRONG INTERPLANETARY MAGNETIC FIELD STRUCTURE[J]. Journal of Space Science, 1996, 16(2): 92-96. doi: 10.11728/cjss1996.02.092

A Sun-ALFVENIC FLOW IN THE STRONG INTERPLANETARY MAGNETIC FIELD STRUCTURE

doi: 10.11728/cjss1996.02.092
  • Received Date: 1995-05-05
  • Rev Recd Date: 1900-01-01
  • Publish Date: 1996-04-24
  • On November 23, 1982, an extremely high-speed stream was overtaking a strong magnetic field structure, resulting in an interplanetary combinative structire including high-density front sheath, main part with strong magnetic field and low density, high density rear sheath, and extremely high-speed streams. The MHD characteristics of the combinative structure are analyzed in this paper. A sub-Alfvenic flow is found inside the main part of the strong magnetic field structure, the formation of which is also discussed.

     

  • loading
  • 加载中

Catalog

    通讯作者: 陈斌, bchen63@163.com
    • 1. 

      沈阳化工大学材料科学与工程学院 沈阳 110142

    1. 本站搜索
    2. 百度学术搜索
    3. 万方数据库搜索
    4. CNKI搜索

    Article Metrics

    Article Views(1698) PDF Downloads(1035) Cited by()
    Proportional views
    Related

    /

    DownLoad:  Full-Size Img  PowerPoint
    Return
    Return