Proceedings of the Royal Society of London, Volume 20

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Taylor & Francis, 1872
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Page 590 - There is a river in the ocean. In the severest droughts it never fails, and in the mightiest floods it never overflows. Its banks and its bottom are of cold water, while its current is of warm. The Gulf of Mexico is its fountain, and its mouth is in the Arctic Seas. It is the Gulf Stream.
Page xxiii - In 1830 he became one of the eight foreign associates of the French Academy of Sciences.
Page x - Statement of the Question of Parliamentary Reform, with a Reply to the Objections of the Edinburgh Review.
Page 291 - Transactions of the North of England Institute of Mining Engineers, and accomr•nny a short paper by Mr.
Page 159 - April 22, 1663, constituted them a body politic and corporate, by the appellation of the President, Council, and Fellows of the Royal Society of London, for improving Natural Knowledge.
Page 590 - ... the quantity of heat discharged over the Atlantic from the waters of the Gulf Stream in a winter's day, would be sufficient to raise the whole column of atmosphere that rests upon France and the British Islands, from the freezing point to summer heat.
Page 277 - I have had the honour to lay before The Queen the loyal and dutiful Address of the President...
Page 272 - The amount of alcohol eliminated per day does not increase with the continuance of the alcohol diet ; therefore all the alcohol consumed daily must, of necessity, be disposed of daily ; and as it certainly is not eliminated within that time, it must be destroyed in the system. The elimination of alcohol following the...
Page 381 - ... confirm. I was not then able to use a slit sufficiently narrow to show that the nebular line is single and not coincident with the middle of the double line of nitrogen. I am still pursuing the investigation of the parts of this inquiry which remain unsettled. Second line. — This line was found by my former comparisons to be a little less refrangible than a strong line in the spectrum of barium.
Page 384 - H /3 occurs in the space between two groups of strong lines where the lines are faint. On one night of unusual steadiness of the air, when the finer lines in the star's spectrum were seen with more than ordinary distinctness, I was able with the more powerful instruments now at my command to see a narrow defined line in the red apparently coincident with H a, and a similar line at the position of H ft.

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