On Dissipation inside Turbulent Convection Zones from Three-dimensional Simulations of Solar Convection

@article{Penev2007OnDI,
  title={On Dissipation inside Turbulent Convection Zones from Three-dimensional Simulations of Solar Convection},
  author={Kaloyan Penev and Dimitar D. Sasselov and Francis J. Robinson and MA PierreDemarqueHarvard--SmithsonianCenterforAstroph and CT DepartmentofAstronomyYaleUniversityNewHaven},
  journal={The Astrophysical Journal},
  year={2007},
  volume={655},
  pages={1166-1171}
}
The development of two-dimensional and three-dimensional simulations of solar convection has lead to a picture of convection quite unlike the usually assumed Kolmogorov spectrum turbulent flow. We investigate the impact of this changed structure on the dissipation properties of the convection zone, parameterized by an effective viscosity coefficient. We use an expansion treatment developed by Goodman & Oh, applied to a numerical model of solar convection, to calculate effective viscosity as a… Expand

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