Configurations of dynamo waves in a two-layer medium and the 11-year solar cycle

Details Configurations of dynamo waves in a two-layer medium and the 11-year solar cycle Configurations of dynamo waves in a two-layer medium and the 11-year solar cycle

Mar 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011astl...37..210p&link_type=abstract

Astronomy Letters, Volume 37, Issue 3, pp.210-217

Astronomy and Astrophysics

Astronomy

Sun, Dynamo Waves, Parker Dynamo, Turbulent Diffusivity, Meridional

Scientific paper

The behavior of dynamo waves in a two-layer medium is investigated in terms of the Parker dynamo model. The solar cycle duration is shown to depend on the ratio of turbulent diffusivities in the layers. Meridional circulation has been incorporated into the Parker system. An increase in the intensity of meridional flows is shown to decelerate the propagation of dynamo waves. The minimum of solar magnetic activity can occur not only in the case of intense meridional circulation in both layers but also when a difference in physical characteristics arises between the layers and the meridional flows are moderate.

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