Multiscale Structure of Active Region Magnetic Fields

Details Multiscale Structure of Active Region Magnetic Fields Multiscale Structure of Active Region Magnetic Fields

Jun 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006spd....37.0301h&link_type=abstract

American Astronomical Society, SPD meeting #37, #3.01; Bulletin of the American Astronomical Society, Vol. 38, p.222

Astronomy and Astrophysics

Astronomy

Scientific paper

Flows in the photosphere of solar active regions are in a state ofhighly developed turbulence. As magnetic fields are frozen into theplasma in the solar surface, magnetograms can therefore be used toinvestigate the processes responsible for structuring active regions.Here, the multiscale structure of a large sample of active regionmagnetograms from the Michelson Doppler Imager (MDI) onboard theSolar and Heliospheric Observatory (SOHO) are investigated. Initialresults regarding the relationship between multiscale structuring andactive region evolution and flaring activity is discussed.

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