Abstract
A zonal magnetic field is found in a toroidal plasma. The magnetic field has a symmetric bandlike structure, which is uniform in the toroidal and poloidal directions and varies radially with a finite wavelength of mesoscale, which is analogous to zonal flows. A time-dependent bicoherence analysis reveals that the magnetic field should be generated by the background plasma turbulence. The discovery is classified as a new kind of phenomenon of structured magnetic field generation, giving insight into phenomena such as dipole field generation in rotational planets.
Original language | English |
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Article number | 165001 |
Journal | Physical review letters |
Volume | 98 |
Issue number | 16 |
DOIs | |
Publication status | Published - Apr 18 2007 |
All Science Journal Classification (ASJC) codes
- Physics and Astronomy(all)