The physical conditions in inner corona
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E. A. Gurtovenko; K. V. Alikayeva
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Article
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1971
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Springer
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English
β 442 KB
The spectrum of the solar corona obtained during the eclipse of 7 March, 1970 has been studied. From the analysis of the line halfwidths it is concluded that the emission of coronal lines of various groups arises in different volumes of the corona. The lines 15303 and 14231 are analyzed in detail an