Solar Dynamo Theory

@article{Charbonneau2014SolarDT,
  title={Solar Dynamo Theory},
  author={P. Charbonneau},
  journal={Annual Review of Astronomy and Astrophysics},
  year={2014},
  volume={52},
  pages={251-290}
}
  • P. Charbonneau
  • Published 2014
  • Physics
  • Annual Review of Astronomy and Astrophysics
The Sun's magnetic field is the engine and energy source driving all phenomena collectively defining solar activity, which in turn structures the whole heliosphere and significantly impacts Earth's atmosphere down at least to the stratosphere. The solar magnetic field is believed to originate through the action of a hydromagnetic dynamo process operating in the Sun's interior, where the strongly turbulent environment of the convection zone leads to flow-field interactions taking place on an… Expand
169 Citations
On self-organization of the solar magnetic fields
Dynamo cycles in global convection simulations of solar-like stars
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