Semiempirical Models of the Impulsive Phase of the Chromospheric Flare

Gan Wei-qun; Fang Cheng

doi:10.11728/cjss1988.01.012

Volume 8 Issue 1

Jan. 1988

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Gan Wei-qun, Fang Cheng. Semiempirical Models of the Impulsive Phase of the Chromospheric Flare[J]. Chinese Journal of Space Science, 1988, 8(1): 12-19. doi: 10.11728/cjss1988.01.012

Citation:

Gan Wei-qun, Fang Cheng. Semiempirical Models of the Impulsive Phase of the Chromospheric Flare[J]. Chinese Journal of Space Science, 1988, 8(1): 12-19. doi: 10.11728/cjss1988.01.012

Gan Wei-qun, Fang Cheng. Semiempirical Models of the Impulsive Phase of the Chromospheric Flare[J]. Chinese Journal of Space Science, 1988, 8(1): 12-19. doi: 10.11728/cjss1988.01.012

Citation:

Gan Wei-qun, Fang Cheng. Semiempirical Models of the Impulsive Phase of the Chromospheric Flare[J]. Chinese Journal of Space Science, 1988, 8(1): 12-19. doi: 10.11728/cjss1988.01.012

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Semiempirical Models of the Impulsive Phase of the Chromospheric Flare

doi: 10.11728/cjss1988.01.012

Dept. of Astronomy, Nanjing University

Received Date: 1987-04-22
Rev Recd Date: 1900-01-01
Publish Date: 1988-01-24

Abstract

Abstract

In this paper,the detailed semiempirical models representing the chromospheric state during the impulsive phase of the 2B flare on Feb.3,1983 are proposed.The physical pictures of total evolutionary pattern of the impulsive phase of the flare are improved either quantitatively or qualitatively in comparison with the former work we did.Based on these semiempirical models,some dynamical properties and energy processes are also discussed.