Volume 16 Issue 2
Apr.  1996
Turn off MathJax
Article Contents
Lin Hua-an. THREE CLASSES OF PROTON FLARES[J]. Journal of Space Science, 1996, 16(2): 115-121. doi: 10.11728/cjss1996.02.115
Citation: Lin Hua-an. THREE CLASSES OF PROTON FLARES[J]. Journal of Space Science, 1996, 16(2): 115-121. doi: 10.11728/cjss1996.02.115

THREE CLASSES OF PROTON FLARES

doi: 10.11728/cjss1996.02.115
  • Received Date: 1995-01-12
  • Rev Recd Date: 1900-01-01
  • Publish Date: 1996-04-24
  • The nuclear γ-ray line (GRL) and the proton event (PE) observed in interplanetary space are direct evidences that protons and heavy ions are accelerated to energies above several MeV per nucleon for solar proton flares。 Solar Hard X--ray properties obtained by SMM satellite show there are three classes of solar proton flares: GRL, PE and GRL/PE。 The results indicate the different behavours respect to the hard X--ray properties for the three classes of proton flares seem to be relative with the different height distribution of energetic particles acceleration region (or active region) for the GRL, PE and GRL/PE proton flares。

     

  • 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(1768) PDF Downloads(1002) Cited by()
    Proportional views
    Related

    /

    DownLoad:  Full-Size Img  PowerPoint
    Return
    Return