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Fractal Properties of Active Regions View all abstracts by submitter

Aleksey Golovko   Submitted: 2012-06-08 19:56

The dynamics of active regions have been investigated using multi-fractal analysis methods, based on magnetograms of the full solar disk in the 630.2 nm line obtained with the SOLIS vector spectromagnetograph of Kitt Peak Observatory (USA) during 2006?2007 and January 1, 2009?April 12, 2010. The applied method of multi-fractal segmentation reveals the appearance of new magnetic fluxes on the Sun disk. A comparison of these fluxes with flare activity shows that the flares are generated in areas of interaction of emerging fluxes with existing structures.

Authors: A. A. Golovko and I. I. Salakhutdinova
Projects: None

Publication Status: Astronomy Reports, 'Online First' on SpringerLink
Last Modified: 2012-06-10 17:20
Go to main E-Print page  Impulsive acceleration of coronal mass ejections: II. Relation to SXR flares and filament eruptions  Composition of the Solar Corona, Solar Wind, and Solar Energetic Particles  Edit Entry  Download Preprint  Submitter's Homepage Delete Entry 

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