Astronomy and Astrophysics – Astronomy
Scientific paper
Mar 1998
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998arep...42..265k&link_type=abstract
Astronomy Reports, Volume 42, Issue 2, March 1998, pp.265-274
Astronomy and Astrophysics
Astronomy
6
Scientific paper
In an integrated approach to studying the dynamics and energetics of solar and stellar active regions, taking into account their complex self-consistent evolution, the magnetic-field structure in an active region is modelled as an ensemble of current-carrying magnetic loops. These loops are mutually connected by induction and interact with each other. Each loop is represented by an equivalent electric circuit with variable parameters that depend on the shape, size, and location of the loop in the ensemble, as well as on the plasma parameters in the magnetic tube. Energetic processes in individual magnetic loops of the ensemble brought about by changes in the geometrical characteristics of a single loop are considered. In particular, the ascent of one of the magnetic loops in the group leads to a flarelike heating of some loops, while certain other loops are cooled
Khodachenko Maxim L.
Zaitsev Valerii V.
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