Abstract
The features and the method for solving of two fundamental problems of astrophysics are considered: the anomalously high temperature of the solar corona above the surface of the Sun, which is 200 times higher than the temperature of the surface itself, as well as the anomalously high concentration of the He3 isotope (compared to He4) in this region. It is shown that both of these effects are associated with the implementation of LENR in a low-temperature magnetized plasma in the solar atmosphere due to the self-similar formation of coherent correlated states and the generation of giant particle energy fluctuations in this region.
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