The latitude belts of solar activity as a consequence of a boundary-layer dynamo

Details The latitude belts of solar activity as a consequence of a boundary-layer dynamo The latitude belts of solar activity as a consequence of a boundary-layer dynamo

Apr 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991natur.350..481b&link_type=abstract

Nature (ISSN 0028-0836), vol. 350, April 11, 1991, p. 481-483.

Physics

23

Boundary Layer Plasmas, Dynamo Theory, Helioseismology, Solar Activity, Convection, Solar Interior, Solar Magnetic Field, Wave Propagation

Scientific paper

Calculative results in agreement with observations are presented form a
model in which solar dynamo action arises in a very thin spherical
boundary layer. This model explains why a latitudinal boundary exists on
the solar surface below which features such as sunspots migrate toward
the equator whereas above it they migrate polewards.

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