Fractal Brownian surface and distribution of longitudinal magnetic fields in two solar active regions.

Details Fractal Brownian surface and distribution of longitudinal magnetic fields in two solar active regions. Fractal Brownian surface and distribution of longitudinal magnetic fields in two solar active regions.

Mar 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995soph..157..199w&link_type=abstract

Solar Physics, Vol. 157, No. 1 - 2, p. 199 - 212

Physics

1

Solar Magnetic Fields: Solar Active Regions, Solar Magnetic Fields: Surfaces, Solar Magnetic Fields: Distribution, Solar Magnetic Fields: Magnetograms

Scientific paper

The distribution of photospheric longitudinal magnetic fields in a solar active region can be considered to be a natural surface in a mathematical sense. Just as with landscapes on the Earth, the surface may be a fractal Brownian surface (FBS). A method suggested in the paper can manifest whether the surface is an FBS or not. The method has been applied to the longitudinal magnetic fields in AR 5988 on March 24, 1990 and AR 6233 on August 30, 1990, in which the observational characteristics are quite different. The test results indicate that the distributions of the longitudinal magnetic field in both regions are not in agreement with the FBS model.

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