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X-ray and extreme ultraviolet (1–400 Å) spectroscopy of the sun, from OSO-III

✍ Scribed by W. M. Neupert; W. A. White; W. J. Gates; M. Swartz; R. M. Young

Book ID: 104643602
Publisher: Springer
Year: 1969
Tongue: English
Weight: 513 KB
Volume: 6
Category: Article
ISSN: 0038-0938
DOI: 10.1007/bf00150943

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✦ Synopsis

X-ray spectra of the sun have been obtained during solar flares. New emission lines arc observed in the spectral range from 1.3 A to 3 7X, and 8/~-20 ,~, the most intense of the new emission features being tentatively attributed to optical transitions in high stages of ionization of iron (Fexxv through Fexx). Studies of the variability of these lines during flarcs provide new information of the development of a hot plasma in the initial stages of the flare event.

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