Solar Interior: Convection Zone

Astronomy and Astrophysics – Astrophysics

Scientific paper

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Sun, Solar Interior

Scientific paper

The Sun, like all main sequence stars of moderate mass, possesses a deep convective envelope just below its surface in which turbulent fluid motions serve to carry outward the energy flux that results from nuclear burning within its core. Observations of the Sun reveal complex flows and magnetic structures that are evidence of highly turbulent convection just below the surface of this rotating s...

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