Petrovay, K. (2005) The Sun as a laboratory for turbulence theory: the problem of anomalous diffusion. In: British-Romanian-Hungarian N+N+N Workshop for Young Researchers On Plasma- and Astrophysics: from laboratory to outer space Edited by I. Ballai, E. Forgács-Dajka, A. Marcu and K. Petrovay. Publications of the Astronomy Department of the Eötvös University (15). ELTE Sokszorosítóüzeme, Budapest, pp. 53-58.
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Abstract
The solar atmosphere offers a unique possibility to study tuubulent motions under conditions presently unattainable in laboratory experiment or even numerical simulations. This short review will focus on one controversial issue in turbulence theory, on which some light can be shed by solar observations: anomalous turbulent diffusion.
| Item Type: | Book Section |
|---|---|
| Additional Information: | PADEU Volume 15 British-Romanian-Hungarian N+N+N Workshop for Young Researchers On Plasma- and Astrophysics: from laboratory to outer space Edited by I. Ballai, E. Forgács-Dajka, A. Marcu and K. Petrovay |
| Uncontrolled Keywords: | Sun: interior, MHD, Sun: rotation |
| Subjects: | Q Science / természettudomány > QB Astronomy, Astrophysics / csillagászat, asztrofizika |
| Depositing User: | Emese Kató |
| Date Deposited: | 24 Oct 2024 13:01 |
| Last Modified: | 24 Oct 2024 13:01 |
| URI: | https://real.mtak.hu/id/eprint/207885 |
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