Size-Flux Relation in Solar Active Regions

Details Size-Flux Relation in Solar Active Regions Size-Flux Relation in Solar Active Regions

Apr 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003chjaa...3..175c&link_type=abstract

Chinese Journal of Astronomy & Astrophysics, Vol. 3, p. 175-182

Astronomy and Astrophysics

Astrophysics

1

Sun: Activity, Sun: Magnetic Fields

Scientific paper

We present a study of the relationship between integral area and corresponding total magnetic flux for solar active regions. It is shown that some of these relationships are satisfied to simple power laws. Fractal examination showed that some of these power laws can not be justified inside the simple models of stationary magnetic flux tube aggregation. All magnetic fluxes and corresponding areas were calculated using the data measured with the Solar Magnetic Field Telescope of the Huairou Solar Observing Station in Beijing.

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