Principle of Minimum Energy in Magnetic Reconnection in a Self-Organized Critical Model for Solar Flares

27 Apr 2018 Farhang Nastaran Safari Hossein Wheatland Michael S.

Solar flares are an abrupt release of magnetic energy in the Sun's atmosphere due to reconnection of the coronal magnetic field. This occurs in response to turbulent flows at the photosphere which twist the coronal field... (read more)

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  • SOLAR AND STELLAR ASTROPHYSICS