Cascade Processes in Rapid Rotation
- Авторлар: Reshetnyak M.Y.1,2, Pokhotelov O.A.1
-
Мекемелер:
- Institute of Physics of the Earth, Russian Academy of Sciences
- Institute of Terrestrial Magnetism, Ionosphere, and Radiowave Propagation, Russian Academy of Sciences
- Шығарылым: Том 53, № 5 (2019)
- Беттер: 362-367
- Бөлім: Article
- URL: https://journals.rcsi.science/0038-0946/article/view/171374
- DOI: https://doi.org/10.1134/S0038094619040099
- ID: 171374
Дәйексөз келтіру
Аннотация
The process of the kinetic energy and kinetic helicity transfer over the spectrum in an incompressible, rapidly rotating turbulent medium is considered. An analog of the Fjortoft theorem for 3D turbulence is proposed. It is shown that, similar to 2D turbulence, there are two cascades simultaneously: the inverse cascade of the kinetic energy and the direct cascade of the kinetic helicity, which in the case of 2D turbulence corresponds to the cascade of enstrophy. The result is in agreement with our earlier calculations, some recent numerical simulations, and physical experiments on geostrophic turbulence. The proposed scenario is applicable to explain the processes in the liquid cores of planets and fast-rotating stars.
Негізгі сөздер
Авторлар туралы
M. Reshetnyak
Institute of Physics of the Earth, Russian Academy of Sciences; Institute of Terrestrial Magnetism, Ionosphere, and Radiowave Propagation, Russian Academy of Sciences
Хат алмасуға жауапты Автор.
Email: m.reshetnyak@gmail.com
Ресей, Moscow; Moscow
O. Pokhotelov
Institute of Physics of the Earth, Russian Academy of Sciences
Email: m.reshetnyak@gmail.com
Ресей, Moscow
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