Correlation between polarities areas and their integral magnetic fluxes in solar active regions

Details Correlation between polarities areas and their integral magnetic fluxes in solar active regions Correlation between polarities areas and their integral magnetic fluxes in solar active regions

Sep 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003esasp.535...79c&link_type=abstract

In: Solar variability as an input to the Earth's environment. International Solar Cycle Studies (ISCS) Symposium, 23 - 28 June 2

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2

Sun: Activity, Sun: Magnetic Fields

Scientific paper

The results of study the correlation between integral areas of polarities and corresponding total magnetic fluxes for solar active regions are presented. It is shown that some of these relationships satisfy to simple power laws. These laws can differ from each other for different active regions or different polarities of the same active region. Fractal examination showed that some of these power laws can not be justified inside the simple models of stationary magnetic flux tubes aggregation. Time independence of these power laws and their high level of trustworthiness allow to regard exponents of these laws as being quasi-invariant parameters effective for quantitative classification of solar active regions.

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