Satellite lines in the solar X-ray spect
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Werner M. Neupert
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Article
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1971
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Springer
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English
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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