Abstract
The basic concept of locality of turbulent interactions in k→ space is considered. It is suggested that some nonlocal turbulent spectra can be turned into the local ones by virtue of appropriate “hidden parameters.” Based on this idea, a local description is developed for optical turbulence that escaped investigation by standard methods for a while, and a broad set of the Kolmogorov spectra is found explicitly. The developed method is applied then to describe formation of Kolmogorov spectra and evolution of free optical turbulence.
Original language | English (US) |
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Pages (from-to) | 4524-4527 |
Number of pages | 4 |
Journal | Physical review letters |
Volume | 76 |
Issue number | 24 |
DOIs | |
State | Published - 1996 |
Externally published | Yes |
All Science Journal Classification (ASJC) codes
- General Physics and Astronomy