Length and Velocity Scales in Protoplanetary Disk Turbulence
In the theory of protoplanetary disk turbulence, a widely adopted ansatz, or assumption, is that the turnover frequency of the largest turbulent eddy, Ω _L , is the local Keplerian frequency Ω _K . In terms of the standard dimensionless Shakura–Sunyaev α parameter that quantifies turbulent viscosity...
Gorde:
| Egile Nagusiak: | , , , |
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| Formatua: | Artigo |
| Hizkuntza: | Inglês |
| Argitaratua: |
IOP Publishing
2024-01-01
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| Saila: | The Astrophysical Journal |
| Gaiak: | |
| Sarrera elektronikoa: | https://doi.org/10.3847/1538-4357/ad2c89 |
| Etiketak: |
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