P - ω Dynamo in Spherical Geometry

Details P - ω Dynamo in Spherical Geometry P - ω Dynamo in Spherical Geometry

Sep 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001ap%26ss.277..531h&link_type=abstract

Astrophysics and Space Science, v. 277, Issue 4, p. 531-543 (2001).

Astronomy and Astrophysics

Astrophysics

Scientific paper

Based on the fundamental P - ω dynamo equation, using spherical polar coordinates, we carry out a study of turbulent plasma wave dynamo effect. For various rotation laws, different analytical solutions are derived. In the cases of no rotation and rigid rotation, the dynamo generates poloidal field only, while with differential rotation, regardless the differential rotation is radial or latitudinal, poloidal and toroidal fields are all generated. We may think that the solutions are the analytical forms of the magnetic field in a turbulent source region of celestial bodies.

Affiliated with

Also associated with

No associations

Rating

P - ω Dynamo in Spherical Geometry 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 P - ω Dynamo in Spherical Geometry, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and P - ω Dynamo in Spherical Geometry will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1484143