New American Practical NavigatorU.S. Government Printing Office, 1880 |
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Side
... minutes , d the distance of the land in sea miles , and h the height of the eye of the observer in feet . Tables XVII . , XVIII . , and XIX . , were first calculated by the author of this work , and published in the Appendix to the ...
... minutes , d the distance of the land in sea miles , and h the height of the eye of the observer in feet . Tables XVII . , XVIII . , and XIX . , were first calculated by the author of this work , and published in the Appendix to the ...
Side
... minutes and parts of a minute of time corresponding to every second from 0 to 12 " 59 " . This requires no explanation . Table XXXIV . contains the error of an observed angle arising from a deviation of ' in the parallelism of the ...
... minutes and parts of a minute of time corresponding to every second from 0 to 12 " 59 " . This requires no explanation . Table XXXIV . contains the error of an observed angle arising from a deviation of ' in the parallelism of the ...
Side 1
... minutes , Part IV . corresponding to S and D , will be SX ( D + 16 ) ( D — 16 ) . 256 Table XLV . The arguments at the side being B and 12 - B hours , and the second difference at the top A , the correction of this table will be B. ( 12 ...
... minutes , Part IV . corresponding to S and D , will be SX ( D + 16 ) ( D — 16 ) . 256 Table XLV . The arguments at the side being B and 12 - B hours , and the second difference at the top A , the correction of this table will be B. ( 12 ...
Side 3
... minutes , and seconds , corresponding to any log . sine , cosine , & c . To find the arithmetical complement of any ... minute . 68 76 77 78 78 Page Table of solutions of the various cases of Mercator's.
... minutes , and seconds , corresponding to any log . sine , cosine , & c . To find the arithmetical complement of any ... minute . 68 76 77 78 78 Page Table of solutions of the various cases of Mercator's.
Side 5
... minutes of each other , by one observer .... 18 of two different objects , taken at different times 178 To estimate the effects of small errors in the observations First method of calculating double altitudes 179 180 Second method ...
... minutes of each other , by one observer .... 18 of two different objects , taken at different times 178 To estimate the effects of small errors in the observations First method of calculating double altitudes 179 180 Second method ...
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American Practical Navigator: An Epitome of Navigation : Originally by ... Uten tilgangsbegrensning - 1962 |
Vanlige uttrykk og setninger
angle apparent altitude azimuth bearing calculated Cape centre chord chronometer circle column compass Corr corresponding Cosec courses sailed degrees diameter diff difference of latitude difference of longitude Dist draw east equal equator error EXAMPLE extent will reach feet find the course find the difference given Greenwich Half-sum horizon glass horizontal parallax hour angle hypotenuse instrument latitude and departure Latitude Sailing line of numbers line of sines logarithm lower limb lunitidal interval mean meridian altitude method middle latitude miles moon moon's multiplied Nautical Almanac nearly noon object observed altitude parallel Parallel Sailing perpendicular Plane Sailing points polar distance quadrant radius 90 refraction right ascension screw sea account secant semidiameter sextant ship side sine course star subtracted sun's declination Suppose telescope transit triangle true altitude true distance true longitude variation wires
Populære avsnitt
Side 11 - The angle in a semicircle is a right angle ; the angle in a segment greater than a semicircle is less than a right angle ; and the angle in a segment less than a semicircle is greater than a right angle.
Side 15 - In any plane triangle, as the sum of the sides about the vertical angle is to their difference, so is the tangent of half the sum of the angles at the base to the tangent of half their difference.
Side 15 - In any plane triangle, the sum of any two sides is to their difference as the tangent of half the sum of the opposite angles is to the tangent of half their difference. By Theorem II. we have a : b : : sin. A : sin. B.
Side 6 - A plane rectilineal angle is the inclination of two straight lines to one another, which meet together, but are not in the same straight line.
Side 254 - Emersion (Em.) the instant of its reappearance at coming out of the shadow. They generally happen when the Satellite is apparently at some distance from the body of Jupiter, except near the opposition of Jupiter to the Sun, when the eclipse takes place near to the body of the planet.
Side 7 - In a right triangle, the side opposite the right angle is called the hypotenuse, and the other two sides the legs.
Side 233 - ... distance, to obtain the approximate Greenwich mean time corresponding to the given distance. If the distance between the Moon and a Star increased or decreased uniformly, the Greenwich...
Side 126 - ... to the depth of 80 or 100 fathoms ; then heave the log, and the number of knots run out in half a minute will be the miles the current sets per hour, and the bearing of the log will show the set of it. There is a very remarkable current, called the GULF STREAM, which sets in a north-east direction along the coast of America, from Cape Florida towards the Isle of Sables...
Side 148 - ... placed by the maker equidistant from each other and parallel to the middle one — therefore, when the middle one is adjusted, the others are so too ; he also places the two transverse wires at right angles to the vertical middle wire. These adjustments are always performed by the maker, and but little liable to derangement. When, however, they happen to get out of order, and the observer wishes to correct them, it is done by loosening the screws which hold the eye-end of the telescope in its...
Side 136 - ... to make the objects appear on the other wire ; if the contact still remains perfect, the axis of the telescope is in proper adjustment ; if not, it must be altered by moving the two screws which fasten, to the up-and-down piece, the collar into which the telescope screws. This adjustment is not very liable to be deranged.