A Vorticity-Magnetic Field Dynamo Instability

Astronomy and Astrophysics – Astrophysics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

7pages, 0 figs, aas2pp4.sty, ApJL

Scientific paper

10.1086/310959

We generalize the mean field magnetic dynamo to include local evolution of the mean vorticity in addition to the mean magnetic field. The coupled equations exhibit a general mean field dynamo instability that enables the transfer of turbulent energy to the magnetic field and vorticity on larger scales. The growth of the vorticity and magnetic field both require helical turbulence which can be supplied by an underlying global rotation. The dynamo coefficients are derived including the backreaction from the mean magnetic field to lowest order. We find that a mean vorticity field can actually seed exponential growth of mean magnetic field from only a small scale seed magnetic field, without the need for a seed mean magnetic field. The equations decouple when the fluctuating velocity and magnetic field cross-correlations vanish, resulting in the separate mean field magnetic and mean field vorticity dynamo equations.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

A Vorticity-Magnetic Field Dynamo Instability 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 A Vorticity-Magnetic Field Dynamo Instability, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and A Vorticity-Magnetic Field Dynamo Instability will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-383039

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.