On the structure of magnetic fields in the solar convection zone

Details On the structure of magnetic fields in the solar convection zone On the structure of magnetic fields in the solar convection zone

Nov 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984esasp.220...67s&link_type=abstract

In ESA The Hydromagnetics of the Sun p 67-76 (SEE N85-25091 14-92)

Physics

17

Convection Currents, Magnetic Field Configurations, Magnetic Flux, Solar Magnetic Field, Boundary Layer Flow, Rotating Generators, Solar Rotation, Stellar Models, Vorticity

Scientific paper

Expulsion of solar magnetic flux and vorticity; fragmentation and
accumulation of fields; and the dominating forces that govern the
evolution of a magnetic structure are discussed. These aspects are
united in a picture of a boundary layer dynamo near the bottom of the
convection zone.

Affiliated with

Also associated with

No associations

Rating

On the structure of magnetic fields in 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 On the structure of magnetic fields in the solar convection zone, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and On the structure of magnetic fields in the solar convection zone will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1753277