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CORONA (Lat. for " crown ")

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Originally appearing in Volume V07, Page 185 of the 1911 Encyclopedia Britannica.
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CORONA (See also:Lat. for " See also:crown ")  , in See also:astronomy, the exterior envelope of the See also:sun, being beyond the photosphere and See also:chromosphere, invisible in the See also:telescope and unrecognized by the spectroscope, except during a See also:total See also:eclipse (see SUN; ECLIPSE) . See also:Corona Borealis, also known as the Corona septentrionalis, and the See also:Northern See also:Crown or See also:Garland, is a See also:constellation of the Northern hemisphere, mentioned by See also:Eudoxus (4th cent . B.C.) and See also:Aratus (3rd cent . B.C.) . In the catalogues of See also:Ptolemy, Tycho See also:Brahe, and See also:Hevelius, eight stars are mentioned; but See also:recent uranographic surveys have greatly increased this number . The most interesting members are: v Coronae, a binary consisting of a yellow See also:star of the 6th magnitude, and a bluish star of the 7th magnitude ; R Coronae, an irregular variable star ; and T Coronae or Nova Coronae, a temporary or new star, first observed in 1866 . Corona Australis, also known as Corona meridionalis, or the See also:Southern Crown, is a constellation of the Southern hemisphere, mentioned by Eudoxus and Aratus . In Ptolemy's See also:catalogue thirteen stars are described . In See also:physical See also:science, coronae (or " glories ") are the coloured rings frequently seen closely encircling the sun or See also:moon . Formerly classified by the See also:ancient Greeks with halos, rainbows, &c., under the See also:general See also:group of "meteors," they came to receive considerable See also:attention at the hands of See also:Descartes, Christiaan See also:Huygens, and See also:Sir See also:Isaac See also:Newton ; but the correct explanation of coronae was reserved until the beginning of the loth See also:century, when See also:Thomas See also:Young applied the theories of the diffraction and interference of See also:light to this phenomenon . See also:Prior to Young, halos and coronae had not been clearly differentiated ; they were both regarded as caused by the See also:refraction of light by atmospheric moisture and See also:ice, although observation had shown that important distinctions existed between these phenomena . Thus, while halos have certain definite radii, viz .

22° and 46°, the radii of coronae vary very considerably ; also, halos are coloured red on the inside, whereas coronae are coloured red on the outside (see See also:

HALO) . It has now been firmly established, both experimentally and mathematically, that coronae are due to diffraction by the See also:minute particles of moisture and dust suspended in the See also:atmosphere, and the radii of the rings depend on the See also:size of the diffracting particles . (See DIFFRACTION OF LIGHT.) Other meteorological phenomena caused by the diffraction of light include the anthelia, and the See also:chromatic rings seen encircling shadows thrown on a See also:bank of clouds, mist or See also:fog . These appear- ances differ from halos and coronae inasmuch as their centres are at the See also:anti-See also:solar point; they thus resemble the See also:rainbow . The anthelia (from the See also:Greek &vat, opposite, and ')Xtos, the sun) are coloured red on the inside, the outside being generally See also:colour-less owing to the continued overlapping of many spectra . The See also:diameter increases with the size of the globules making up the mist . The chromatic rings seen encircling the " spectre of the See also:Brocken " are similarly explained . The See also:blue colour of the See also:sky (q.v.), supernumerary rainbows, and the gorgeous sunsets observed of ter intense volcanic disturbances, when the atmosphere is charged with large quantities of extremely minute dust particles (e.g . See also:Krakatoa), are also explicable by the diffraction of light . (See DuaT) See E . Mascart, Traite d'optique (1899–1903) ; J . Pernter, Meteorologische Optik (1902–1905) .

In See also:

architecture, the See also:term " corona " is used of that See also:part of a See also:cornice which projects over the See also:bed See also:mould and constitutes the See also:chief See also:protection to the See also:wall from See also:rain; it is always throated, and its See also:soffit rises towards the wall . The term is also given to the See also:apse or semicircular termination of the See also:choir; as at See also:Canterbury in the part called " See also:Becket's crown." The large circular See also:chandelier suspended in churches, of which the finest example is that given by See also:Barbarossa to See also:Aix-la-Chapelle, is often called a corona . The term is also used in See also:botany of the crown-like appendage at the See also:top of See also:compound See also:flowers, the diminutive being coronule .

End of Article: CORONA (Lat. for " crown ")
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