THE STRAY LIGHT DBSERVED DURING A PARTIAL ECLIPSE OF THE SUN

Hu Ju; Ni Xiang-bin

doi:10.11728/cjss1989.04.311

Volume 9 Issue 4

Dec. 1989

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Article Navigation > Chinese Journal of Space Science > 1989 > 9(4): 311-316

Hu Ju, Ni Xiang-bin. THE STRAY LIGHT DBSERVED DURING A PARTIAL ECLIPSE OF THE SUN[J]. Chinese Journal of Space Science, 1989, 9(4): 311-316. doi: 10.11728/cjss1989.04.311

Citation:

Hu Ju, Ni Xiang-bin. THE STRAY LIGHT DBSERVED DURING A PARTIAL ECLIPSE OF THE SUN[J]. Chinese Journal of Space Science, 1989, 9(4): 311-316. doi: 10.11728/cjss1989.04.311

Hu Ju, Ni Xiang-bin. THE STRAY LIGHT DBSERVED DURING A PARTIAL ECLIPSE OF THE SUN[J]. Chinese Journal of Space Science, 1989, 9(4): 311-316. doi: 10.11728/cjss1989.04.311

Citation:

Hu Ju, Ni Xiang-bin. THE STRAY LIGHT DBSERVED DURING A PARTIAL ECLIPSE OF THE SUN[J]. Chinese Journal of Space Science, 1989, 9(4): 311-316. doi: 10.11728/cjss1989.04.311

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THE STRAY LIGHT DBSERVED DURING A PARTIAL ECLIPSE OF THE SUN

doi: 10.11728/cjss1989.04.311 cstr: 32142.14.cjss1989.04.311

Hu Ju,
Ni Xiang-bin

1.
Dept. of Astronomy, Nanjing University
2.
Nanjing Artillery Institute

Received Date: 1988-10-27
Rev Recd Date: 1900-01-01
Publish Date: 1989-12-24

Abstract

Abstract

In this paper, an diffusion function which discribes the scattering characteristics of the earth's atmosphere is obtained by fitting a theoretical profile with an aureole intensity profile, observed during a partial eclipse on July 31, 1981. This function may be applied to correction of scattered light in the photometry measurements of sunspots or other active phenomena.