Cyclic flows in the solar convection zone due to the dynamo reaction

Details Cyclic flows in the solar convection zone due to the dynamo reaction Cyclic flows in the solar convection zone due to the dynamo reaction

Nov 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984esasp.220..225t&link_type=abstract

In ESA The Hydromagnetics of the Sun p 225-226 (SEE N85-25091 14-92)

Computer Science

Atmospheric Circulation, Dynamo Theory, Solar Atmosphere, Solar Rotation, Convection, Kinematic Equations, Solar Magnetic Field

Scientific paper

The feedback of the oscillating mean magnetic field of the kinematic alpha omega dynamo on the mean flows in the Sun is investigated. The observational constraints on the magnetic field and on the mean cycle-dependent flows (the time variations of the differential rotation and meridional motion) accord with the dynamo excitation mechanism. The solutions of the mean-field equations of motion give the observed components of the mean flows. The detailed properties of the flows give a possibility to investigate the dynamo mechanism itself.

Affiliated with

Also associated with

No associations

Rating

Cyclic flows in the solar convection zone due to the dynamo reaction 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 Cyclic flows in the solar convection zone due to the dynamo reaction, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Cyclic flows in the solar convection zone due to the dynamo reaction will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1753346