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Solar Differential Rotation Dynamics by Erik Martinez is a document available to read on EtoBox.
This document summarizes a study on the periodic change in solar differential rotation using MHD dynamo theory. The authors propose that the solar magnetic field induces turbulent flows through an alpha-dynamo effect, which in turn drives periodic changes in the solar rotation profile with a period of 11 years, similar to the solar magnetic activity cycle. They present a theoretical model to explain the observed 11-year oscillation of differential rotation in the solar convection zone and surface based on t
- Author
- Erik Martinez
- Language
- EN