Numerical simulations of the magnetic field distribution in a solar complex of activity

Details Numerical simulations of the magnetic field distribution in a solar complex of activity Numerical simulations of the magnetic field distribution in a solar complex of activity

Jul 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998an....319..245t&link_type=abstract

Astronomische Nachrichten, vol. 319, no. 4, p. 245.

Astronomy and Astrophysics

Astronomy

1

Scientific paper

Powerful solar complexes of activity are supposed to result from the excitation of Rossby vortices within a thin layer beneath the convection zone. Numerical simulations demonstrate that Rossby vortices generate large-scale arc-like magnetic structures. It is shown that the most powerful complex of activity observed in June-July 1982 was likely to be a result of the excitation of a Rossby anticyclone rather than a cyclone.

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