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ANDERS See also: Swedish physicist, was See also: born on the t3th of See also: August 1814 at Logdo, Medelpad, 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 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 round the See also: world in 1851—1853
.
In 1858 he succeeded Adolph See also: Ferdinand Svanberg (18o6—1857) in the 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 heat and with 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 Rumford medal of the Royal Society in 1872, contains a fundamental principle of spectrum 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 solar spectrum
.
He announced the existence of hydrogen, among other elements, in the See also: sun's atmosphere in 1862, and in 1868 published his See also: great map of the normal solar spectrum which 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 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 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 Strassburg he was appointed lecturer in physics at Stockholm University in 1885, but in 1891 returned to Upsala, where in 1896 he became 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 compensation pyrheliometer, invented in 1893, and apparatus for obtaining a photographic See also: representation of the infra-red spectrum (1895)
.
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