 | John Holmes Agnew, Walter Hilliard Bidwell - 1862 - 604 Seiten
...distinct absorptionlines which we see in the solar spectrum ; and the hypothesis is further invalidated by the fact that these lines do not appreciably alter when the sun approaches the horizon. Hence the presence of the iron group of dark lines in the solar spectrum appears to prove the presence... | |
 | 1862 - 620 Seiten
...practically certain that these lines have a common cause. ' Hence this coincidence,' says Kirchhoff, ' must be produced by some cause, and a cause can be...unlikely, owing to the high temperature which we must suppose the sun's atmosphere to possess, that such vapours should be present in it. Hence the observations... | |
 | 1862 - 648 Seiten
...earth. But it is not easy to understand how our atmosphere can contain such a quantity of iron vapor as would produce the very distinct absorptionlines...unlikely, owing to the high temperature which we must suppose the sun's atmosphere to possess, that such vapors should be present in it. Hence the observations... | |
 | 1862 - 618 Seiten
...which we see in the solar spectrum ; and this supposition is rendered still less probable by the tact that these lines do not appreciably alter when the...unlikely, owing to the high temperature which we must suppose the sun's atmosphere to posses?, that such vapours should be present in it. Hence the observations... | |
 | 1863 - 376 Seiten
...atmosphere can contain such a quantity of iron vapor as would produce the very distinct absorption lines which we see in the solar spectrum ; and this supposition...unlikely, owing to the high temperature which we must suppose the sun's atmosphere to possess, that such vapors should be present in it. Hence the observations... | |
 | Robert Galloway - 1864 - 808 Seiten
...But it is not easy to understand how our atmosphere can contain such a quantity of metallic vapours as would produce the very distinct absorptionlines...unlikely, owing to the high temperature which we must suppose the sun's atmosphere to possess, that such vapours should be present in it. Hence the observations... | |
 | Forbes Winslow - 1867 - 332 Seiten
...iron vapour as would produce the very distinct absorption lines which are seen in the solar spectrum. This supposition is rendered still less probable by...unlikely, owing to the high temperature which we must suppose the sun's atmosphere to possess, that such vapours should be present in it. Hence the observations... | |
 | Forbes Winslow - 1868 - 236 Seiten
...iron vapor as would produce the very distinct absorption lines which are seen in the solar spectrum. This supposition is rendered still less probable by...all unlikely, owing to the high temperature which we has not sunk below a white heat. Our terrestrial atmosphere, in which now so few elements are found,... | |
 | Henry Enfield Roscoe - 1870 - 514 Seiten
...atmosphere can contain such a quantity of iron vapour as would produce the very distinct absorption lines which we see in the solar spectrum ; and this supposition...unlikely, owing to the high temperature which we must suppose the tun's atmosphere to possess, that such vapours should be present in it. Hence the observations... | |
 | Henry E. Roscoe - 1869 - 372 Seiten
...atmosphere can contain such a quantity of iron vapour as would produce the very distinct absorption lines which we see in the solar spectrum ; and this supposition...unlikely, owing to the high temperature which we must suppose the sun's atmosphere to possess, that such vapours should be present in it. Hence the observations... | |
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... which we see in the solar spectrum ; and this supposition is rendered still less probable by the fact that these lines do not appreciably alter when the sun approaches the horizon. It does not, on the other hand, seem at all unlikely, owing to the... 
