The evolution of loop structures in flux rings within the solar convection zone

Details The evolution of loop structures in flux rings within the solar convection zone The evolution of loop structures in flux rings within the solar convection zone

Sep 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989soph..123..217c&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 123, no. 2, 1989, p. 217-239.

Physics

101

Convection Currents, Coronal Loops, Dynamo Theory, Magnetic Field Configurations, Solar Magnetic Field, Buoyancy, Coriolis Effect, Equations Of Motion, Magnetic Flux, Sunspots

Scientific paper

The present consideration of whether the action of the solar Coriolis force is subdued when the initial configuration of the flux ring has nonaxisymmetries, in the form of loop structures, notes results to be dramatically dependent on whether the flux ring with the loops lies completely within the convection zone, or whether its lower parts are embedded in the stable layers beneath the convection zone. In the former case, the Coriolis force suppresses the nonaxisymmetric perturbations and the flux ring tends to remain symmetric; in the latter case, the lower parts of the flux ring may remain anchored under the bottom of the convection zone, although the upper parts of the loops still tend to move parallel to the rotation axis and emerge.

Affiliated with

Also associated with

No associations

Rating

The evolution of loop structures in flux rings within the solar convection zone does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with The evolution of loop structures in flux rings within the solar convection zone, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The evolution of loop structures in flux rings within the solar convection zone will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1827236