作者: R. Tousey , M. J. Koomen
DOI: 10.1007/BF00154291
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摘要: The white-light corona from 3–9 Rs and the XUV (170–500 A) corona, photographed a rocket at 1930 UT on 7 March, 1970, are compared with X-ray flown 1900 by AS & E, H Ly-α obtained during totality Speer et al., Fexiv 5303 A Hawaii, total eclipse photographs in infrared.