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DECLINATION (from Lat. declinare, to ...

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Originally appearing in Volume V07, Page 914 of the 1911 Encyclopedia Britannica.
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DECLINATION (from See also:Lat. declinare, to decline) , in See also:magnetism the See also:angle between true See also:north and magnetic north, i.e. the variation between the true See also:meridian and the magnetic meridian. In 1596 at See also:London the angle of declination was 11° E. of N., in 1652 magnetic north was true north, in 1815 the magnetic See also:needle pointed 241° W. of N., in 1891 18° W., in 1896 17° 56' W. and in 1906 17° 45'. The angle is gradually diminishing and the declination will in See also:time again be o°, when it will slowly increase in an easterly direction, the north magnetic See also:pole oscillating slowly around the North Pole. See also:Regular daily changes of declination also occur. Magnetic storms cause irregular See also:variations sometimes of one or two degrees. (See MAGNETISM, TERRESTRIAL.) In See also:astronomy the declination is the angular distance, as seen from the See also:earth, of a heavenly See also:body from the See also:celestial See also:equator, thus corresponding with terrestrial See also:latitude.

End of Article: DECLINATION (from Lat. declinare, to decline)

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