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Soft X-ray emission lines of Ni XVIII in the solar spectrum

โœ Scribed by F.P. Keenan; M. Mathioudakis; D.J. Pinfield; W.A. Brown; M.E. Bruner


Book ID
110220402
Publisher
Springer
Year
1999
Tongue
English
Weight
58 KB
Volume
185
Category
Article
ISSN
0038-0938

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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