Some dynamical effects of the sunspot magnetic flux ring

Details Some dynamical effects of the sunspot magnetic flux ring Some dynamical effects of the sunspot magnetic flux ring

Mar 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982acasn..23...23z&link_type=abstract

Acta Astronomica Sinica, vol. 23, Mar. 1982, p. 23-28. In Chinese, with abstract in English.

Physics

Fluid Dynamics

1

Convective Flow, Fluid Dynamics, Magnetic Flux, Solar Atmosphere, Sunspots, Magnetic Field Configurations, Ring Structures, Solar Physics

Scientific paper

The cause of the delta-configuration and the A-configuration sunspot groups, and the phenomena of the filaments and material falling down above the sunspot are explained based on dynamical effects. The contraction, deformation and break of the fluid mass take place under the influence of magnetic ring force. The magnetic fluid motion above AR is due to the dynamical effects of the sunspot magnetic flux ring, and the magnetic fluid motion is characterized by two vertical circulations on both sides of the symmetrical plane, which is the zero plane of the longitudinal magnetic field.

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