Solar rotation in the chromosphere and c
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William Henze; A. K. Dupree
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Article
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1973
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Springer
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English
⚖ 275 KB
Extreme ultraviolet spectroheliograms in Mg x (625 ~) and the Lyman continuum (897/~) obtained from OSO-6 are used to determine the differential rotation rate in the solar chromosphere and corona. The equatorial rotation rate agrees with spectroscopic measurements of the photospheric plasma velocity