Meridional circulation and dynamo waves

Details Meridional circulation and dynamo waves Meridional circulation and dynamo waves

Sep 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008an....329..766p&link_type=abstract

Astronomische Nachrichten, Vol.329, Issue 7, p.766

Astronomy and Astrophysics

Astronomy

6

Magnetic Fields, Magnetohydrodynamics (Mhd), Waves, Meridional Circulation

Scientific paper

The effect of meridional circulation on spherical shell dynamos is considered in the Parker approximation. We demonstrate that the type of the exited solution crucially depend on the intensity of the meridional circulation. If the circulation is equatorward or if it is polarward however do not exceed some critical value, an oscillating solution in form of an equatorward traveling wave is excited. If the polarward meridional circulation becomes too intensive the solution becomes steady growing.

Affiliated with

Also associated with

No associations

Rating

Meridional circulation and dynamo waves 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 Meridional circulation and dynamo waves, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Meridional circulation and dynamo waves will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1292989