Wave-Number Spectrum of Drift-Wave Turbulence
Journal Article
·
· Physical Review Letters
- Laboratoire de Physique des Plasmas, Ecole Polytechnique, CNRS, 91128 Palaiseau Cedex (France)
- CEA, IRFM, F-13108 Saint Paul Lez Durance (France)
- Center for Astrophysics and Space Sciences, University of California San Diego, 9500 Gilman Drive, La Jolla, California 92093-0424 (United States)
A simple model for the evolution of turbulence fluctuation spectra, which includes neighboring interactions leading to the usual dual cascade as well as disparate scale interactions corresponding to refraction by large scale structures, is derived. The model recovers the usual Kraichnan-Kolmogorov picture in the case of exclusively local interactions and midrange drive. On the other hand, when disparate scale interactions are dominant, a simple spectrum for the density fluctuations of the form |n{sub k}|{sup 2}propor tok{sup -3}/(1+k{sup 2}){sup 2} is obtained. This simple prediction is then compared to, and found to be in fair agreement with, Tore Supra CO{sub 2} laser scattering data.
- OSTI ID:
- 21347000
- Journal Information:
- Physical Review Letters, Vol. 102, Issue 25; Other Information: DOI: 10.1103/PhysRevLett.102.255002; (c) 2009 The American Physical Society; ISSN 0031-9007
- Country of Publication:
- United States
- Language:
- English
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