Please use this identifier to cite or link to this item:
|Title:||Analysis of Solar Optical Flares in Relation to Their Peak Intensities|
|Authors:||Gupta, M. K. Das|
Mitra, R. K.
Sarkar, S. K.
|Abstract:||Peak intensities of 5200 optical flares reported during the period January 1968 to December 1971 were examined in relation to their (i) occurrences, (ii) durations, (Hi) ratios' of rise time to duration, and (iv) classifications, both area-wise and intensity-wise. important results obtained are (i) flares as reported by the different observatories fall under two major groups, one group confined within the percentage intensity increase range 40-100% and the other within the range 140-300%, (ii) intensity-wise flare classification in vogue does not show any direct relationship with the present system of quantitative intensity increase evaluation and (iii) majority of the flares are 'impulsive' in nature.|
|ISSN:||0975-105X (Online); 0367-8393 (Print)|
|Appears in Collections:||IJRSP Vol.02(2) [June 1973]|
Items in NOPR are protected by copyright, with all rights reserved, unless otherwise indicated.