Physics
Scientist
Sibirskii IZMIRAN, Irkutsk, USSR
Akademiia Nauk SSSR, Sibirskii Institut Zemnogo Magnetizma, Ionosfery i Rasprostraneniia Radiovoln, Irkutsk, USSR
Akademiia Nauk SSSR, Institut Zemnogo Magnetizma, Ionosfery i Rasprostraneniia Radiovoln, Irkutsk, USSR
Sibirskii IZMIRAN, Irkutsk, Russia
AN SSSR, Institut Zemnogo Magnetizma, Ionosfery i Rasprostraneniia Radiovoln, Irkutsk, USSR
Changes of the chromosphere model during 'umbral flashes'
Contribution and response functions for CA II lines in different atmospheric models
Determination of the radiation field in the chromosphere using the method of the observed line profile inversion
Determination of the thermodynamic conditions in the chromosphere above a sunspot by solving an inverse problem. I - Numerical simulation of temperature and electron density distributions
Determination of thermodynamic conditions in the chromosphere above a sunspot by solving an inverse problem. II - Numerical modeling of pressure and density distributions
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