The Effect of Solar Parameters on Seasonal Variation of 5893 Angstrom Line Intensity at Calcutta

Details The Effect of Solar Parameters on Seasonal Variation of 5893 Angstrom Line Intensity at Calcutta The Effect of Solar Parameters on Seasonal Variation of 5893 Angstrom Line Intensity at Calcutta

Oct 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996em%26p...75..177m&link_type=abstract

Earth, Moon, and Planets, Volume 75, Issue 3, pp.177-183

Computer Science

2

Airglow Emissions, Relative Sun-Spot Numbers, Solar Flare Numbers, 10.7 Cm Solar Flux

Scientific paper

The purpose of this paper is to present the correlation of seasonal variation of 5893 Å line intensity with relative sunspot numbers, solar flare numbers and the variable component of 10.7 cm solar flux. A study has been made and the following important results have been obtained.
(i)
The intensity of 5893 Å line at Calcutta shows periodic variation with different solar parameters during descending part of secondary peak of 21st solar cycle (1984 1985).
(ii)
5893 Å line intensity of Mt. Abu also shows periodic variation with solar parameters during the period 1965 1968 when there was a peak phase of 20th solar cycle.
(iii)
A possible explanation for such type of variation is also presented.

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