ANGSTROM, ANDERS JONAS (1814-1874)

This article appears in Volume V02, Page 42 of the Encyclopedia Britannica.

Encyclopedia Britannica - Main :: ANC-APO

ANGSTROM, ANDERS JONAS (1814-1874) , Swedish physicist, was born on the t3th of August 1814 at Logdo, Medelpad, Sweden. He was educated at Upsala University, where in 1839 he became

privet

PRIVET

docent in physics. In 1842 he went to Stockholm

Observatory

OBSERVATORY

in order to gain experience in

practical

PRACTICAL

astronomical

work

WORK

, and in the following year he became observer at Upsala

Observatory

OBSERVATORY

. Becoming interested in terrestrial magnetism he made many observa tions of magnetic intensityand declination in various parts of Sweden, and was charged by the Stockholm

Academy

ACADEMY, GREEK
ACADEMY, ROYAL

of Sciences with the task, not completed till shortly before his death, of working out the magnetic data obtained by the Swedish frigate " Eugenie " on her voyage round the world in 18511853. In 1858 he succeeded Adolph Ferdinand Svanberg (18o61857) in the chair of physics at Upsala, and there he died on the 21st of June 18i4. His most important

work

WORK

was concerned with the conduction of heat and with spectroscopy. In his optical researches, Optiska Undersokningar, presented to the Stockholm

Academy

ACADEMY, GREEK
ACADEMY, ROYAL

in 1853, he not only pointed out that the electric spark yields two superposed spectra, one from the metal of the electrode and the other from the gas in which it passes, but deduced from 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 Sir E. 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 rank as one of the founders of spectroscopy. From 1861 onwards he paid

special

SPECIAL

attention to the solar spectrum. He announced the existence of hydrogen, among other elements, in the sun's atmosphere in 1862, and in 1868 published his

great

GREAT

map of the normal solar spectrum which long remained authoritative in questions of wave-length, although his measurements were inexact to the extent of one part in 7000 or 8000 owing to the metre which he used as his standard having been slightly too short. He was the first, in 1867, to examine the spectrum of the aurora borealis, and detected and measured the characteristic

bright

BRIGHT, JOHN (1811-188g)
BRIGHT, SIR CHARLES TILSTON

line in its yellow 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 light. y
His son, KNuT JOHAN ANGSTROM, was born at Upsala on the 12th of January 1857, and studied at the university of that town from 1877 to 1884. After spending a short 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 radiation of heat from the sun and its absorption by the earth's atmosphere, and to that end devised various delicate methods and

instruments

INSTRUMENTS

, including his electric compensation pyrheliometer, invented in 1893, and apparatus for obtaining a photographic representation of the infra-red spectrum (1895).

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