Physics
Scientific paper
Feb 1996
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996soph..163..319j&link_type=abstract
Solar Physics, Volume 163, Issue 2, pp.319-325
Physics
7
Scientific paper
The evolution of magnetic helicity in a rapidly growing active region is
governed mainly by the advection of magnetic fields into the
photosphere. Dissipation at the photosphere makes only a minor
contribution to helicity evolution. Current helicity dissipation in the
three-dimensional domain around the active region can be ignored.
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