Seasonal Variation of 5577 å Line Emission At Calcutta and its Variation with Different Solar Parameters

Details Seasonal Variation of 5577 å Line Emission At Calcutta and its Variation with Different Solar Parameters Seasonal Variation of 5577 å Line Emission At Calcutta and its Variation with Different Solar Parameters

Feb 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997em%26p...76..135m&link_type=abstract

Earth, Moon, and Planets, v. 76, Issue 3, p. 135-140 (1997).

Computer Science

1

Airglow, Relative Sunspot Numbers, 10.7 Cm Solar Flux

Scientific paper

The paper presents the variation of 5577 Å line intensity with relative sunspot number, and 10.7 cm solar flux. The study has obtained the following important results. [(i)] The 5577 Å line intensity at Calcutta is plotted against relative sunspot number, and the variable component of 10.7 cm solar flux during 1984-1985, which is the secondary peak of the descending phase of the 21st solar cycle. The intensity curves show periodic variation with different solar parameters. [(ii)] The 5577 Å line intensity at Mt. Abu also shows periodic variation with solar parameters during the period 1965-1968 when there was a peak phase of the 20th solar cycle. [(iii)] A possible explanation for such variation is also presented.

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