 | 1882 - Liczba stron: 426
...distinguishable, though the lines G- and H are well seen in the star's spectrum. Dr. Huggins therefore concludes that the part of the comet's original light...which gives a continuous spectrum is much stronger relatively to the reflected solar light in this comet than was the case in the comet of last year.... | |
 | Sir Norman Lockyer - 1882 - Liczba stron: 722
...and H are well seen in the star's spectrum taken under the same conditions. We may therefore conclude that the part of the comet's original light which gives a continuous spectrum is much stronger relatively to the reflected solar light in this comet, than was the case in the comet of last year,... | |
 | Sir Norman Lockyer - 1882 - Liczba stron: 960
...and H are well seen in the star's spectrum taken under the same conditions. We may therefore conclude that the part of the comet's original light which gives a continuous spectrum is much stronger relatively to the reflected solar light in this comet, than was the case in the comet of last year,... | |
 | Sir Norman Lockyer - 1882 - Liczba stron: 674
...seen in the star's spectrum taken under the same conditions. We may therefore conclude that the pjrt of the comet's original light which gives a continuous spectrum is much stronger relatively to the reflected solar light in this comet, than was the case in the comet of last year,... | |
 | 1883 - Liczba stron: 552
...extending from F to a little beyond If, without any Fraunhofer lint's, from which Dr. Huggins coneludes that the part of the comet's original light which...possibly owing to the sodium detected in the visible spectrum. On May 17, during the total eclipse of the Sun at Sohag, a comet was seen and photographed... | |
 | Royal Astronomical Society - 1883 - Liczba stron: 560
...spectrum extending from F to a little beyond H, without any Frauuhofer lines, from which Dr. Jluggius concludes that the part of the comet's original light...the ultra-violet, presumably due to cyanogen, were &ot present. In the continuous spectrum five places of greater brightness were evident, possibly owing... | |
 | Royal Astronomical Society - 1883 - Liczba stron: 562
...spectrum extending from F toa little beyond H, without any Fraunhofer lines, from which Dr. Huggius concludes that the part of the comet's original light...last year. The groups in the ultra-violet, presumably duo to cyanogen, were, not present. In the continuous spectrum five places of greater brightness were... | |
 | British Association for the Advancement of Science - 1883 - Liczba stron: 932
...II are well swn £ "I star's spectrum taken under the same conditions. We may conclude theref« : 4 the part of the comet's original light which gives a continuous spectrum и '^ stronger relatively to the reflected solar light in this comet than was thf »* * the comet of... | |
 | 1883 - Liczba stron: 966
...and H are well seen in the star's spectrum taken under the same conditions. We may therefore conclude that the part of the comet's original light which gives a continuous spectrum is much stronger relatively to the reflected solar light in this comet, than was the case in the comet of last year,... | |
 | Sir Norman Lockyer - 1882 - Liczba stron: 720
...and H are well seen in the star's spectrum taken under the same conditions. We may therefore conclude that the' part of the comet's original light which gives a continuous spectrum is much stronger relatively to the reflected solar light in this comet, than was the case in the comet of last year,... | |
| |
... continuous spectrum. The slit was rather more open than was the case in photographing the spectrum of the comet of last year ; this would make these lines less distinct, but the lines G and H are well seen in the star's spectrum taken under the same... 