K stat'e
"The Abundance of Iron in the Solar Photosphere"
The resulting abubances appear to be independent of exitation potential, but seem to increase slightly with increasing wavelenght. The average value of the derived abudance lg NFe/NH + 12.0 = 6.64, is in very good agreement with other modern determinations.
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Astrometriya
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Astronomicheskie instrumenty
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Astronomicheskoe obrazovanie
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Astrofizika
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Istoriya astronomii
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Kosmonavtika, issledovanie kosmosa
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Lyubitel'skaya astronomiya
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Planety i Solnechnaya sistema
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Solnce