A Discussion on the Splited Phenomenon of the Rays or Streamers in Type I Cometary Tail

Li Zhong-yuan

doi:10.11728/cjss1990.02.096

Volume 10 Issue 2

Apr. 1990

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Article Navigation > Chinese Journal of Space Science > 1990 > 10(2): 96-100

Li Zhong-yuan. A Discussion on the Splited Phenomenon of the Rays or Streamers in Type I Cometary Tail[J]. Chinese Journal of Space Science, 1990, 10(2): 96-100. doi: 10.11728/cjss1990.02.096

Citation:

Li Zhong-yuan. A Discussion on the Splited Phenomenon of the Rays or Streamers in Type I Cometary Tail[J]. Chinese Journal of Space Science, 1990, 10(2): 96-100. doi: 10.11728/cjss1990.02.096

Li Zhong-yuan. A Discussion on the Splited Phenomenon of the Rays or Streamers in Type I Cometary Tail[J]. Chinese Journal of Space Science, 1990, 10(2): 96-100. doi: 10.11728/cjss1990.02.096

Citation:

Li Zhong-yuan. A Discussion on the Splited Phenomenon of the Rays or Streamers in Type I Cometary Tail[J]. Chinese Journal of Space Science, 1990, 10(2): 96-100. doi: 10.11728/cjss1990.02.096

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A Discussion on the Splited Phenomenon of the Rays or Streamers in Type I Cometary Tail

doi: 10.11728/cjss1990.02.096

Li Zhong-yuan

Dept. of Earth and Space Science, University of Science and Technology of China, Hefei, Anhui

Received Date: 1989-09-19
Rev Recd Date: 1900-01-01
Publish Date: 1990-04-24

Abstract

Abstract

In this paper, the splited phenomenon of plasma rays or streamers is already discussed. By means of MHD theory, it is pointed out that the splited phenomenon results from the space plasma turbulence. Aqualitative analysis is given in the article, and a quantitative analysis-as well. Thus the splited phenomenon of rays in plasma tail, is explained reasonably.
- The magnetic field of Type I tail,
- Type I cometary tail,