Abstract
A model of essentially transient ionization of plasma is suggested to explain some features in observed spectra of solar flares, which cannot be understood if stationary conditions are assumed.
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Koshelev, K.N., Kononov, E.Y. A possible explanation of non-steady-state appearances in X-ray spectra of solar flares. Sol Phys 77, 177–181 (1982). https://doi.org/10.1007/BF00156103
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DOI: https://doi.org/10.1007/BF00156103