The helicity constraint in spherical shell dynamos

Details The helicity constraint in spherical shell dynamos The helicity constraint in spherical shell dynamos

2007-11-22

arxiv.org/abs/0711.3616v1

Astron. Nachr. 328, 1118-1121 (2007)

Astronomy and Astrophysics

Astrophysics

4 pages, 5 fig, proceedings of 5th Potsdam Thinkshop on Meridional flow, differential rotation, solar and stellar activity, to

Scientific paper

10.1002/asna.200710881

The motivation for considering distributed large scale dynamos in the solar context is reviewed in connection with the magnetic helicity constraint. Preliminary accounts of 3-dimensional direct numerical simulations (in spherical shell segments) and simulations of 2-dimensional mean field models (in spherical shells) are presented. Interesting similarities as well as some differences are noted.

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