The Ratio of OI5577Åto N<SUB>2</SUB><sup>+</sup> 3914Åunder Diffuse Auroral Condition

Tad Hong-sheng

doi:10.11728/cjss1985.01.034

Volume 5 Issue 1

Jan. 1985

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Article Navigation > Chinese Journal of Space Science > 1985 > 5(1): 34-39

Tad Hong-sheng. The Ratio of OI5577Åto N2+ 3914Åunder Diffuse Auroral Condition[J]. Chinese Journal of Space Science, 1985, 5(1): 34-39. doi: 10.11728/cjss1985.01.034

Citation:

Tad Hong-sheng. The Ratio of OI5577Åto N₂⁺ 3914Åunder Diffuse Auroral Condition[J]. Chinese Journal of Space Science, 1985, 5(1): 34-39. doi: 10.11728/cjss1985.01.034

Tad Hong-sheng. The Ratio of OI5577Åto N2+ 3914Åunder Diffuse Auroral Condition[J]. Chinese Journal of Space Science, 1985, 5(1): 34-39. doi: 10.11728/cjss1985.01.034

Citation:

Tad Hong-sheng. The Ratio of OI5577Åto N₂⁺ 3914Åunder Diffuse Auroral Condition[J]. Chinese Journal of Space Science, 1985, 5(1): 34-39. doi: 10.11728/cjss1985.01.034

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The Ratio of OI5577Åto N₂⁺ 3914Åunder Diffuse Auroral Condition

doi: 10.11728/cjss1985.01.034 cstr: 32142.14.cjss1985.01.034

Tad Hong-sheng

Institute of Space Physics, Academia Sinica

Received Date: 1982-09-11
Rev Recd Date: 1984-05-25
Publish Date: 1985-01-24

Abstract

Abstract

Alinear relationship between the ratio of 015577Å to N₂+3914Å and the corresponding altitudes are found in this paper. With this dependence the quenching factor of O(¹S) in lower thermosphere is obtained, this quenching factor is not very large.