Towards Understanding Solar Convection and Activity - (Invited Review)

Details Towards Understanding Solar Convection and Activity - (Invited Review) Towards Understanding Solar Convection and Activity - (Invited Review)

Mar 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000soph..192....3g&link_type=abstract

Solar Physics, v. 192, Issue 1/2, p. 3-26 (2000).

Physics

7

Scientific paper

The dynamics of the large-scale eddies which advect angular momentum through the convection zone is controlled in a significant way by the boundary conditions, which, if they are not modelled adequately, do not lead to a distribution of angular velocity that is consistent with observation. The transition boundary layer separating the convection zone from the radiative interior is thought to play a critical role in controlling the magnetic field in the convection zone, and is probably not wholly irrelevant to understanding the cycle of solar activity.

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