dorsal/arxiv
View SchemaThe shell model approach to the rotating turbulence
| Authors | M. Reshetnyak, B. Steffen |
|---|---|
| Categories | |
| ArXiv ID | physics/0311001 |
| URL | https://arxiv.org/abs/physics/0311001 |
Abstract
Applications of the shell model of turbulence to the case of rapidly rotating bodies are considered. Starting from the classical GOY model we introduce the Coriolis force and obtain a $\sim k^{-2}$ spectrum for 3D hydrodynamical turbulence for the free decay regime as well for the regime with external forcing. Additional modifications of the GOY model providing a realistic form of the helicity are proposed.
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"date_created": "2026-03-02T18:00:46.599000Z",
"date_modified": "2026-03-02T18:00:46.599000Z",
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"record": {
"abstract": "Applications of the shell model of turbulence to the case of rapidly rotating\nbodies are considered. Starting from the classical GOY model we introduce the\nCoriolis force and obtain a $\\sim k^{-2}$ spectrum for 3D hydrodynamical\nturbulence for the free decay regime as well for the regime with external\nforcing. Additional modifications of the GOY model providing a realistic form\nof the helicity are proposed.",
"arxiv_id": "physics/0311001",
"authors": [
"M. Reshetnyak",
"B. Steffen"
],
"categories": [
"physics.flu-dyn",
"physics.geo-ph"
],
"title": "The shell model approach to the rotating turbulence",
"url": "https://arxiv.org/abs/physics/0311001"
},
"schema_id": "dorsal/arxiv",
"source": {
"execution_id": "f16d0cff-e26e-443e-b63c-25819016b728",
"id": "arXiv Dataset IDs",
"type": "Model",
"variant": "snapshot-2026-03-01",
"version": "0.1.0"
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"user_id": 1000002
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