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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... "
A Treatise on Chemistry - Pàgina 178
per Henry Enfield Roscoe, Carl Schorlemmer - 1907
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Eclectic Magazine, and Monthly Edition of the Living Age, Volum 57

John Holmes Agnew, Walter Hilliard Bidwell - 1862 - 604 pàgines
...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...
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Researches on the solar spectrum, and the spectra of the ..., Volum 2,Part 1

Gustav Robert Kirchhoff - 1862 - 62 pàgines
...These iron vapours might be contained either in the atmosphere of the sun or in that of the earth. But it is not easy to understand how our atmosphere...unlikely, owing to the high temperature which we must 3—2 suppose the sun's atmosphere to possess, that such vapours should be present in it. Hence the...
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Littell's Living Age, Volum 75

1862 - 648 pàgines
...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...suppose the sun's atmosphere to possess, that such vapors should be present in it. Hence the observations of the solar spectrum appear to me to prove...
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The Edinburgh Review, Volum 116

1862 - 618 pàgines
...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...temperature which we must suppose the sun's atmosphere to posses?, that such vapours should be present in it. Hence the observations of the solar spectrum appear...
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Annual of Scientific Discovery: Or, Year-book of Facts in Science and Art

1863 - 376 pàgines
...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...suppose the sun's atmosphere to possess, that such vapors should be present in it. Hence the observations of the solar spectrum appear to me to prove...
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The Second Step in Chemistry, Or the Student's Guide to the Higher Branches ...

Robert Galloway - 1864 - 804 pàgines
...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...suppose the sun's atmosphere to possess, that such vapoun should be present in it. Hence the observations of the aolar spectrum appear to me to prove...
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Light: Its Influence on Life and Health

Forbes Winslow - 1868 - 236 pàgines
...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,...
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Spectrum Analysis: Six Lectures, Delivered in 1868, Before the Society of ...

Henry Enfield Roscoe - 1870 - 514 pàgines
...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...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 of the...
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Spectrum analysis, 6 lects

sir Henry Enfield Roscoe - 1870 - 452 pàgines
...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...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 of the...
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British and Foreign Medico-chirurgical Review: Or, Quarterly ..., Volum 46

1870 - 588 pàgines
...lines which we see in the solar spectrum ; and this supposition is rendered still less probable, since these lines do not appreciably alter when the sun...approaches the horizon. It does not on the other hand seem unlikely, owing to the high temperature which wt must suppose the sun's atmosphere to possess, that...
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