The Effects of Solar and Ionospheric Parameters on Seasonal Variation of 6300 Angstroms Line Emission at Calcutta

Details The Effects of Solar and Ionospheric Parameters on Seasonal Variation of 6300 Angstroms Line Emission at Calcutta The Effects of Solar and Ionospheric Parameters on Seasonal Variation of 6300 Angstroms Line Emission at Calcutta

Jan 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996em%26p...74..123m&link_type=abstract

Earth, Moon and Planets, Volume 74, Issue 2, pp.123-129

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Earth Atmospheric Emission

Scientific paper

The purpose of this paper is to find correlation between OI 6300 Å line intensity with solar and ionospheric parameters. A critical study have been made and the following important results are obtained:
(i)
Solar flare index plays more important role for the emissions of 6300 Å line than other solar parameters.
(ii)
Intensity of 6300 Å line increases linearly with the increase of solar flare index.
(iii)
Virtual height plays more important role than critical frequency for the emission of 6300 Å line-intensity.
(iv)
Possible explanation of this type of variation is also presented.

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