Electromotive force in strongly compressible magnetohydrodynamic turbulence
Abstract
Fully compressible magnetohydrodynamic (MHD) turbulence is investigated in the framework of the multiple-scale direct-interaction approximation. With the aid of the propagators (correlation and Green's functions), fluctuating fields are solved, and turbulent correlations are estimated in highly compressible turbulence. We focus on the expression of the turbulent electromotive force (EMF). Obliqueness between the mean magnetic field and the mean-density gradient, the mean internal density gradient and the non-equilibrium mean velocity contributes to the EMF in the presence of the density variance, which is ubiquitous in turbulence in strongly variable density flows such as the shock-front region. This density-variance effect is expected to locally enhance the turbulence intensity across the shock front, leading to a fast reconnection.
- Publication:
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Journal of Plasma Physics
- Pub Date:
- October 2018
- DOI:
- 10.1017/S0022377818000727
- Bibcode:
- 2018JPlPh..84e7301Y
- Keywords:
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- astrophysical plasmas;
- plasma nonlinear phenomena;
- space plasma physics