Distribution of sunspots according to their magnetic fluxes /Research note/

Details Distribution of sunspots according to their magnetic fluxes /Research note/ Distribution of sunspots according to their magnetic fluxes /Research note/

May 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982soph...78...67d&link_type=abstract

Solar Physics, vol. 78, May 1982, p. 67-70.

Physics

5

Frequency Distribution, Magnetic Flux, Solar Magnetic Field, Sunspots, Line Spectra, Maxwell-Boltzmann Density Function, Solar Physics, Solar Spectra

Scientific paper

The occurrence frequency distribution of sunspots at different magnetic flux values is examined, using magnetic field data measured with the Fe I spectral line. The sunspots are grouped in three longitudinal ranges and their occurrence in selected flux ranges simultaneously determined. The number of sunspots decreases as the -1.9 power of the flux of a sunspot, for sunspots with magnetic flux greater than 3 x 10 to the 21st Maxwell. It may be presumed that there exists a proper balance between the area and the respective magnetic field of a sunspot so that the frequency distribution of associated magnetic fluxes follows a definite rule.

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