Abstract
An effect of rotation on a developed turbulent stratified convection was discussed. The difference in the effective drift velocities for the toroidal and poloidal magnetic fields was elaborated. It was found that a poloidal effective drift velocity was diamagnetic or paramagnetic depending on the rate of rotation.
| Original language | English |
|---|---|
| Article number | 026321 |
| Pages (from-to) | 263211-2632119 |
| Number of pages | 2368909 |
| Journal | Physical Review E |
| Volume | 67 |
| Issue number | 2 2 |
| State | Published - 1 Feb 2003 |
ASJC Scopus subject areas
- Statistical and Nonlinear Physics
- Statistics and Probability
- Condensed Matter Physics