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a. m. sight applied approximate astronomical azimuth Bowditch chronometer circle coefficients column compass course compass heading compass needle component computed Corr correction corresponding cosec course and distance curve declination departure determined deviation due difference of latitude difference of longitude dygogram earth and ship earth's East or West easterly equation fore-and-aft formula given Greenwich mean heavenly body heeling error horizontal force hour angle inducing force instant intersection interval latitude and longitude limb line of position magnetic bearing magnetic course mean noon Mercator chart meridian altitude method miles minutes of arc Nautical Almanac navigator North end North point obtained parallel plane polar pole prime vertical quadrantal deviation represented result rhumbs right ascension sailing sextant ship swings ship's head sidereal star starboard sun's tangent tion transit triangle true altitude true course tude versin westerly zero
Page 478 - A cos 6 = cos a cos c + sin a sin c cos B cos c = cos a cos 6 + sin a sin 6 cos C Law of Cosines for Angles cos A = — cos B...
Page 362 - Sun, and other fundamental astronomical data for equi-distant intervals of Greenwich mean time. Part II, Ephemeris for the Meridian of Washington, gives the ephemerides of the fixed stars, sun, moon, and major planets for transit over the meridian of the old Naval Observatory, Washington.
Page 345 - Mean Solar Day is the interval between two successive transits of the mean sun over the same meridian ; it begins when the mean sun is on the meridian.
Page 776 - ZZ' within the frame or phantom G. The phantom G has a hollow stem H to which the strand £ is attached at its upper end, and the stem forms a journal for rotation in azimuth with respect to the supporting base frame /. The frame / is mounted in gimbal rings K'K...
Page 179 - The first step in compensation of the compass is to correct approximately the quadrantal deviation and the heeling error, in the order named. This is necessary because a material factor in the deviation may be caused by the induction in quadrantal spheres set up by the magnet correctors, and it is essential that the semicircular correction, which is the largest and most important one, should be made when the magnetic conditions approximate as nearly as possible to those when the compensation is complete.
Page 177 - ... of suspension may be measured by a scale on the glass cover. There is a small glass window in each end provided with an index line to mark the horizontal plane. Without the small weight, the needle before being magnetized was exactly balanced, so the weight is intended to balance the vertical magnetic force ashore or on board. If a...
Page 344 - A sidereal day has already been defined as the interval of time between two successive transits of the vernal equinox, or the first point of Aries, over the upper branch of the same meridian.
Page 306 - Fig. 1002, let the sextant be held vertically and let a be the index glass after the index arm ad has been turned so that the index glass is parallel to the horizon glass b and the index d coincides with the zero of the limb. A ray of light...
Page 559 - The transmitting clock that sends out the signals is corrected very accurately, shortly before noon, from the mean of three standard clocks that are rated by star sights with a meridian transit instrument. The noon signal is seldom in error to an amount greater than one or two tenths of a second, although a tenth more may be added by the relays in use on long telegraph lines. Electric transmission over a continuous wire is practically instantaneous.