The correlation of solar flare production with magnetic energy in active regions

Details The correlation of solar flare production with magnetic energy in active regions The correlation of solar flare production with magnetic energy in active regions

Apr 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985soph...96..293m&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 96, April 1985, p. 293-305. Research supported by Aerospace Corp.

Physics

16

Correlation Coefficients, Magnetic Flux, Solar Flares, Solar Magnetic Field, Faculae, H Alpha Line, Regression Analysis, Sunspots

Scientific paper

An investigation of 531 active regions was made to determine the correlation between energy released by flares and the available energy in magnetic fields of the regions. Regions with magnetic flux greater than 10 to the 21st maxwell during the years 1967-1969, which included sunspot maximum, were selected for the investigation. A linear regression analysis of flare production on magnetic flux showed that the flare energy is correlated with magnetic energy with a coefficient of correlation of 0.78. Magnetic classification and field configuration also significantly affect the production of flares.

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