Insights on Turbulent Flows in the Solar Interior from the Behaviour of Dynamo Generated Magnetic Fields

Abstract

Turbulent flows in the interior of the Sun, both at small and large scales, are believed to feed and sustain the solar hydromagnetic dynamo that generates the solar cycle. The solar cycle itself strikingly manifests in a 11-year periodic variation in the number of sunspots seen on the solar surface. Sunspots are regions of concentrated magnetic fields… (More)

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