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ANDERS JONAS ANGSTROM (1814-1874)

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Originally appearing in Volume V02, Page 42 of the 1911 Encyclopedia Britannica.
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ANDERS See also:

JONAS See also:ANGSTROM (1814-1874)  , See also:Swedish physicist, was See also:born on the t3th of See also:August 1814 at Logdo, Medelpad, See also:Sweden . He was educated at See also:Upsala University, where in 1839 he became See also:privet docent in physics . In 1842 he went to See also:Stockholm See also:Observatory in See also:order to gain experience in See also:practical astronomical See also:work, and in the following See also:year he became observer at Upsala Observatory . Becoming interested in terrestrial See also:magnetism he made many observa tions of magnetic intensityand See also:declination in various parts of Sweden, and was charged by the Stockholm See also:Academy of Sciences with the task, not completed till shortly before his See also:death, of working out the magnetic data obtained by the Swedish See also:frigate " See also:Eugenie " on her voyage See also:round the See also:world in 1851—1853 . In 1858 he succeeded Adolph See also:Ferdinand Svanberg (18o6—1857) in the See also:chair of physics at Upsala, and there he died on the 21st of See also:June 18i4 . His most important work was concerned with the See also:conduction of See also:heat and with See also:spectroscopy . In his See also:optical researches, Optiska Undersokningar, presented to the Stockholm Academy in 1853, he not only pointed out that the electric spark yields two superposed spectra, one from the See also:metal of the electrode and the other from the See also:gas in which it passes, but deduced from See also:Euler's theory of resonance that an incandescent gas emits luminous rays of the same refrangibility as those which it can absorb . This statement, as See also:Sir E . See also:Sabine remarked when awarding him the See also:Rumford See also:medal of the Royal Society in 1872, contains a fundamental principle of spectrum See also:analysis, and though for a number of years it was overlooked it entitles him to See also:rank as one of the founders of spectroscopy . From 1861 onwards he paid See also:special See also:attention to the See also:solar spectrum . He announced the existence of See also:hydrogen, among other elements, in the See also:sun's See also:atmosphere in 1862, and in 1868 published his See also:great See also:map of the normal solar spectrum which See also:long remained authoritative in questions of See also:wave-length, although his measurements were inexact to the extent of one See also:part in 7000 or 8000 owing to the See also:metre which he used as his See also:standard having been slightly too See also:short . He was the first, in 1867, to examine the spectrum of the See also:aurora borealis, and detected and measured the characteristic See also:bright See also:line in its yellow See also:green region; but he was mistaken in supposing that this same line, which is often called by his name, is also to be seen in the zodiacal See also:light. y His son, KNuT JOHAN See also:ANGSTROM, was born at Upsala on the 12th of See also:January 1857, and studied at the university of that See also:town from 1877 to 1884 .

After spending a short See also:

time in See also:Strassburg he was appointed lecturer in physics at Stockholm University in 1885, but in 1891 returned to Upsala, where in 1896 he became See also:professor of physics . He especially devoted himself to investigations of the See also:radiation of heat from the sun and its absorption by the See also:earth's atmosphere, and to that end devised various delicate methods and See also:instruments, including his electric See also:compensation pyrheliometer, invented in 1893, and apparatus for obtaining a photographic See also:representation of the infra-red spectrum (1895) .

End of Article: ANDERS JONAS ANGSTROM (1814-1874)
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