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Based on the microwave observations of the Sun on the RATAN-600 and the Large Pulkovo Radio Telescope with high spatial and frequency resolution a new model of interaction of the photospheric and coronal magnetic fields in active regions was finalized. The model of the magnetosphere of the active region is represented as a space in the solar atmosphere, where the plasma parameters, its structure, magnetic field value, the energy release processes are defined and regulated by the interaction of the coronal plasma with magnetic fields, which are a continuation of photospheric magnetic fields of the active region.
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