 | Richard Anthony Proctor - 1875 - 452 pages
...reflected from our atmosphere near the sun's edge would be greatly reduced in in tensity by the dispersion, while the bright lines of the prominences, if such...would remain but little diminished in brilliancy.' It is to be remarked that Huggins himself seemed to consider Lockyer's previous statement unsatisfactory,... | |
 | 1885 - 520 pages
...their spectra would consist of bright lines. With a powerful spectroscope the light reflected from our atmosphere near the sun's edge would be greatly...would remain, but little diminished in brilliancy. In the words which we have italicised in the above quotation the principle on which the spectra of... | |
 | 1900 - 600 pages
...bright lines. With a powerful spectroscope the light reflected from our atmosphere near the sun's limb edge would be greatly reduced in intensity by the...other contrivances, but hitherto without success." At the total eclipse of the sun, August 18, 1868, several observers saw the light of the red flames... | |
 | 1897 - 1044 pages
...bright lines. With a powerful spectroscope the light reflected from our atmosphere near the sun's limb edge would be greatly reduced in intensity by the...other contrivances, but hitherto without success. At the total eclipse of the sun, August 18, 1868, several observers saw the light of the red flames... | |
 | 1897 - 1074 pages
...bright lines. With a powerful spectroscope the light reflected from our atmosphere near the sun's limb edge would be greatly reduced in intensity by the...other contrivances, but hitherto without success. At the total eclipse of the sun, August 18, 1868, several observers saw the light of the red flames... | |
 | Miss Angel - 1875 - 796 pages
...their spectra would consist of bright lines. With a powerful spectroscope the light reflected from our atmosphere near the sun's edge would be greatly reduced in intensity by the dispersion, while the bright lines of the prominences, if such be present, would remain but little diminished in... | |
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With a powerful spectroscope the light reflected from our atmosphere near the sun's limb edge would be greatly reduced in intensity by the dispersion of the prisms, while the bright lines of the prominences, if such be present, would remain but little... 
