Non-axisymmetric solar magnetic fields

Details Non-axisymmetric solar magnetic fields Non-axisymmetric solar magnetic fields

Jun 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999mnras.306..300m&link_type=abstract

Monthly Notices of the Royal Astronomical Society, Volume 306, Issue 2, pp. 300-306.

Astronomy and Astrophysics

Astronomy

26

Scientific paper

A simple non-linear, non-axisymmetric mean field dynamo model is applied to a differentially rotating spherical shell. Two approximations are used for the angular velocity, to represent what is now believed to be the solar rotation law. In each case, stable solutions are found which possess a small non-axisymmetric field component. Although the model has a number of obvious shortcomings, it may be relevant to the problem of the solar active longitudes.

Affiliated with

Also associated with

No associations

Rating

Non-axisymmetric solar magnetic fields 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 Non-axisymmetric solar magnetic fields, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Non-axisymmetric solar magnetic fields will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1797183