Abstract
A modified shell model for rotating turbulence, applied to statistical properties of the rotating turbulence was described. Randomization was observed to play a significant role in correctly modeling the rotation effect. A randomized linear term, which represented the effect of the coherent structures was introduced to the shell model for magnetohydrodynamic (MHD) turbulence. A weak turbulence approximation was used to obtain scaling properties of the energy spectrum in the shell model. The transition from k-5/3 spectrum for weak rotation to k-2 spectrum for strong rotation was also observed, which was predicted by weak turbulence theory.
Original language | English |
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Article number | 046311 |
Pages (from-to) | 046311-1-046311-6 |
Journal | Physical Review E - Statistical, Nonlinear, and Soft Matter Physics |
Volume | 70 |
Issue number | 4 2 |
DOIs | |
Publication status | Published - 2004 Oct |
Externally published | Yes |
ASJC Scopus subject areas
- Statistical and Nonlinear Physics
- Statistics and Probability
- Condensed Matter Physics