High-resolution observations and numerical simulations provide insight into solar atmospheric heating
Nature Astronomy, Published online: 15 April 2024; doi:10.1038/s41550-024-02242-7
What mechanisms power the heating of the solar atmosphere is a long-standing, complex question. Satellite and sounding-rocket observations, coupled with computer simulations, now support the idea that dissipation of electrical currents causes strong heating in the brightest parts of the solar chromosphere and corona.
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