Abstract
Generation of magnetic field energy, without mean field generation, is studied. Isotropic mirror-symmetric turbulence of a conducting fluid amplifies the energy of small-scale magnetic perturbations if the magnetic Reynolds number is high, and the dimensionality of space d satisfies 2.103 < d < 8.765. The result does not depend on the model of turbulence, incompressibility, and isotropy being the only requirements.
| Original language | English (US) |
|---|---|
| Pages (from-to) | 4342-4345 |
| Number of pages | 4 |
| Journal | Physical review letters |
| Volume | 77 |
| Issue number | 21 |
| DOIs | |
| State | Published - 1996 |
All Science Journal Classification (ASJC) codes
- General Physics and Astronomy
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