A Note on the Evolution of Magnetic Helicity in Active Regions

Details A Note on the Evolution of Magnetic Helicity in Active Regions A Note on the Evolution of Magnetic Helicity in Active Regions

Feb 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996soph..163..319w&link_type=abstract

Solar Physics, v. 163, p. 319-325.

Physics

22

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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