留言板

尊敬的读者、作者、审稿人, 关于本刊的投稿、审稿、编辑和出版的任何问题, 您可以本页添加留言。我们将尽快给您答复。谢谢您的支持!

姓名
邮箱
手机号码
标题
留言内容
验证码

COSMIC PLASMA DYNAMO

Yang Zhiliang

Yang Zhiliang. COSMIC PLASMA DYNAMO[J]. 空间科学学报, 2002, 22(4): 289-299. doi: 10.11728/cjss2002.04.289
引用本文: Yang Zhiliang. COSMIC PLASMA DYNAMO[J]. 空间科学学报, 2002, 22(4): 289-299. doi: 10.11728/cjss2002.04.289
COSMIC PLASMA DYNAMO[J]. Journal of Space Science, 2002, 22(4): 289-299. doi: 10.11728/cjss2002.04.289
Citation: COSMIC PLASMA DYNAMO[J]. Journal of Space Science, 2002, 22(4): 289-299. doi: 10.11728/cjss2002.04.289

COSMIC PLASMA DYNAMO

doi: 10.11728/cjss2002.04.289

COSMIC PLASMA DYNAMO

  • 摘要: A new dynamo model based on the polarization of plasma is presented in this paper.From the Maxwell equations in a moving medium, a magnetization vector can be causedwith Rongon current. The steady solar magnetic field is solved from the equations. Onthe assumption that the meridianal flow is ignored, the distribution of magnetic field isput out. In the model, there is no additional parameter considered. The intensity ofmagnetic field inside the sun ranges from 1-6T. The surface magnetic field around thepole is in the order of 1×10-3T, at low latitude the calculated surface magnetic fieldhas the order of 1×10-2 T. The maximum magnetic field is around 30° in latitude.

     

  • 加载中
计量
  • 文章访问数:  1730
  • HTML全文浏览量:  7
  • PDF下载量:  1035
  • 被引次数: 0
出版历程
  • 收稿日期:  1900-01-01
  • 修回日期:  1900-01-01
  • 刊出日期:  2002-11-15

目录

    /

    返回文章
    返回