Astronomy and Astrophysics – Astronomy
Scientific paper
Aug 1995
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995apj...449..739b&link_type=abstract
Astrophysical Journal v.449, p.739
Astronomy and Astrophysics
Astronomy
60
Magnetohydrodynamics: Mhd, Plasmas, Turbulence
Scientific paper
It is shown that the requirements of self-consistency constrain the functional form of the turbulent dynamo field in an incompressible plasma. These requirements involve the back-reaction of the magnetic field through the Lorentz force in the momentum equation and the conservation laws of magnetohydrodynamic turbulence. The dynamo field is calculated in the weak-field limit when the turbulence is isotropic, as well as in the strong-field limit when the turbulence is anisotropic. For magnetic fields of a nontrivial topology, it is shown that the results of kinematic dynamo theory are strongly modified by the production of hyperresistivity (in the mean-field induction equation) which is left as a remnant after a near-cancellation between the alpha and beta effects. An interpolation formula for alpha quenching, encompassing weak-field and strong-field regimes, is proposed.
Bhattacharjee Anirban
Yuan Yu
No associations
LandOfFree
Self-Consistency Constraints on the Dynamo Mechanism 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 Self-Consistency Constraints on the Dynamo Mechanism, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Self-Consistency Constraints on the Dynamo Mechanism will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1269342