Magnetic Structures on the Sun

Astronomy and Astrophysics – Astrophysics

Scientific paper

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Electric And Magnetic Fields, Solar Magnetism, Sun Spots, Solar Cycles

Scientific paper

The dynamo processes inside the Sun produce magnetic fields that manifest themselves over a vast range of scales in the solar atmosphere, from the global scales that govern the evolution over the 11-year cycle, to the diffusion and reconnection scales, which are orders of magnitude smaller than the resolution of solar telescopes. Here we present an overview of the structures on the various scales, their observed properties, their physical origins, and their roles for the structure and dynamics of stellar atmospheres.

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