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This process is a physical basis for the important phenomenon of “dynamic corona”. The magnitude of the flow of materials was evaluated due to the following considerations: if the corona were in hydrodynamic equilibrium, then the altitudes of homogenous atmosphere for hydrogen and iron would correlate as 56/1. In other words, in such case iron ions must not be observed in the distant corona. But this is not so. In 1955 it was a considerable achievement, but nobody believed in the phenomenon of “dynamic corona”.

Impact of the Large-Scale Solar Magnetic Field on the Solar Corona and Solar Wind