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On the stability of the solar chromosphere-corona transition region
Authors:O V Ptitsyna  B V Somov
Institution:1.Sternberg State Institute of Astronomy,Moscow State University,Moscow,Russia
Abstract:We prove the stability of a previously obtained temperature-versus-thickness distribution in the solar chromosphere-corona transition region. The temperature distribution has been obtained on the assumption that the plasma heating by classical heat flux is balanced by the energy loss due to radiation.
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