A mechanism for heating the solar corona

Physics

Scientific paper

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Magnetic Flux, Magnetohydrodynamic Shear Heating, Plasma Waves, Solar Corona, Chromosphere, Plasma Heating, Solar Atmosphere, Solar Magnetic Field

Scientific paper

The high temperatures measured in the solar corona are explained in
terms of heating which results from the work done on the plasma by
expanding magnetic flux. This theory, which invokes no wave deposition
or ohmic heating processes, is consistent with the strongly magnetized,
highly variable nature of the solar atmosphere.

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