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Variation in OviiX-ray line-emission from the solar corona

โœ Scribed by H. R. Rugge; A. B. C. Walker

Publisher
Springer
Year
1970
Tongue
English
Weight
352 KB
Volume
15
Category
Article
ISSN
0038-0938

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The profiles of the Fe XlV, 25303, and Fe x, 26374, emission lines of the solar corona have been observed at different positions using a photoelectric scanning Fabry-Perot interferometer. These profiles were obtained during the eclipse of 7th March 1970, in Mexico and at the Pic-du-Midi coronagraph

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