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Absolute intensities in the solar X-ray spectrum near minimum activity

✍ Scribed by J. N. Gils; W. Graaff

Publisher
Springer
Year
1967
Tongue
English
Weight
159 KB
Volume
2
Category
Article
ISSN
0038-0938

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πŸ“œ SIMILAR VOLUMES

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Observations of solar X-ray line emission using crystal spectrometers during a large chromospheric flare have provided a list of wavelengths with a precision of 0.003 A\_ in first order of diffraction and correspondingly better in higher orders. In addition to the resonance, intersystem (1 1S0-2 zP1

Analysis of the intensities and profiles
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High resolution profiles of the Mg xn 8.42 A line in the solar X-ray spectrum were recorded from the Intercosmos 7 satellite. The Mg xaI line intensity provides a sensitive indicator of the hot plasma content (T > 3 β€’ 106K) in coronal condensations and X-ray flare volumes. The ratio of the line inte