The mean-field kinematic turbulent geodynamo

Details The mean-field kinematic turbulent geodynamo The mean-field kinematic turbulent geodynamo

Jun 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988ge%26ae..28..475r&link_type=abstract

Geomagnetizm i Aeronomiia (ISSN 0016-7940), vol. 28, May-June 1988, p. 475-480. In Russian.

Physics

3

Dynamo Theory, Geomagnetism, Geophysical Fluids, Turbulent Flow, Asymptotic Methods, Geodynamics, Kinematic Equations, Magnetic Dipoles, Magnetic Field Configurations

Scientific paper

A WKB asymptotic method is used to obtain a solution to the kinematic problem concerning the generation of the large-scale geomagnetic field. The turbulent-dynamo generation of the mean field due to differential rotation and helicity is considered. The solution obtained yields a natural explanation for the small inclination of the dipole component of the geomagnetic field and the westward drift of magnetic irregularities (the first nonaxisymmetric field modes).

Affiliated with

Also associated with

No associations

Rating

The mean-field kinematic turbulent geodynamo 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 The mean-field kinematic turbulent geodynamo, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The mean-field kinematic turbulent geodynamo will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1181167