Physics – Fluid Dynamics
Scientific paper
May 2004
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004gapfd..98..385f&link_type=abstract
Geophysical and Astrophysical Fluid Dynamics, vol. 98, Issue 5, p.385-406
Physics
Fluid Dynamics
2
Scientific paper
A key non-linear mechanism in a strong-field geodynamo is that a finite amplitude magnetic field drives a flow through the Lorentz force in the momentum equation and this flow feeds back on the field-generation process in the magnetic induction equation, equilibrating the field. We make use of a simpler non-linear α 2-dynamo to investigate this mechanism in a rapidly rotating fluid spherical shell. Neglecting inertia, we use a pseudo-spectral time-stepping procedure to solve the induction equation and the momentum equation with no-slip velocity boundary conditions for a finitely conducting inner core and an insulating mantle. We present calculations for Ekman numbers (E) in the range 2.5× 10-3 to 5.0× 10-5, for α =α 0cos θ sin π (r-ri) (which vanishes on both inner and outer boundaries). Solutions are steady except at lower E and higher values of α 0. Then they are periodic with a reversing field and a characteristic rapid increase then equally rapid decrease in magnetic energy. We have investigated the mechanism for this and shown the influence of Taylor's constraint. We comment on the application of our findings to numerical hydrodynamic dynamos.
Fearn David R.
Rahman Moshiur Md.
No associations
LandOfFree
Evolution of non-linear α 2-dynamos and taylor's constraint 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 Evolution of non-linear α 2-dynamos and taylor's constraint, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Evolution of non-linear α 2-dynamos and taylor's constraint will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1058075