Statistical relationship between sunspots and major flares

Details Statistical relationship between sunspots and major flares Statistical relationship between sunspots and major flares

Jan 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987ap%26ss.129..203a&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 129, no. 1, Jan. 1987, p. 203-208.

Astronomy and Astrophysics

Astrophysics

2

Solar Flares, Statistical Analysis, Sunspots, Magnetic Flux, Solar Cycles

Scientific paper

In this study, the statistical relationship between sunspots and major flares observed in the descending branch of the 20th and in the ascending branch of the 21st solar cycle is evaluated. It is found that the sunspots which produced these major flares are of the type Dki or Eki with magnetic class D and the largest magnetic field strength between 1600 and 2500 G.

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