The Relation Between the Sunspots Number and the Solar Radio Emission in the Frequency Range 1000 MHz ≤ f ≤ 9400 MHz

Yang Jian; Lou Guo-fang; Lu Ben-kui

doi:10.11728/cjss1984.02.156

Volume 4 Issue 2

Apr. 1984

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Yang Jian, Lou Guo-fang, Lu Ben-kui. The Relation Between the Sunspots Number and the Solar Radio Emission in the Frequency Range 1000 MHz ≤ f ≤ 9400 MHz[J]. Chinese Journal of Space Science, 1984, 4(2): 156-163. doi: 10.11728/cjss1984.02.156

Citation:

Yang Jian, Lou Guo-fang, Lu Ben-kui. The Relation Between the Sunspots Number and the Solar Radio Emission in the Frequency Range 1000 MHz ≤ f ≤ 9400 MHz[J]. Chinese Journal of Space Science, 1984, 4(2): 156-163. doi: 10.11728/cjss1984.02.156

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The Relation Between the Sunspots Number and the Solar Radio Emission in the Frequency Range 1000 MHz ≤ f ≤ 9400 MHz

doi: 10.11728/cjss1984.02.156 cstr: 32142.14.cjss1984.02.156

Purple Mountain Observatory, Academia Sinica

Received Date: 1983-08-19
Rev Recd Date: 1900-01-01
Publish Date: 1984-04-24

Abstract

Abstract

The analytical relations between the relative sunspot number and the solar radio flux density in the frequency range 1000 MHz≤f≤9400 MHz are given in this paper. These raletions are derived based on the methods of least squares, least percentage squares and compound least squares. The computed results show that the third order equation derived by the method of least percentage squares is the best regression equation. The solar quiet radio component obtained from this equation is consistent with the measurements of radio interferometer.