American Practical Navigator: An Epitome of Navigation and Nautical Astronomy |
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Page 7
... Hour angle . Tan . Tangent . .Haversine . Tr . ( or Trans . ) . Transit . .Hourly difference . Var .. Variation . H. P. ( or Hor . par . ) .. Horizontal parallax . Hr - s .. Hour - s . Vert . H. W. High water . W. , Wly .. W. T .. I. C. ...
... Hour angle . Tan . Tangent . .Haversine . Tr . ( or Trans . ) . Transit . .Hourly difference . Var .. Variation . H. P. ( or Hor . par . ) .. Horizontal parallax . Hr - s .. Hour - s . Vert . H. W. High water . W. , Wly .. W. T .. I. C. ...
Page 70
... angles should be plotted , wherever the method can be usefully employed , and the ... hour some hours before it is expected that soundings can be obtained ... angle of deflection from the course caused by a cross set is greater at low ...
... angles should be plotted , wherever the method can be usefully employed , and the ... hour some hours before it is expected that soundings can be obtained ... angle of deflection from the course caused by a cross set is greater at low ...
Page 82
... hour angle , the solution for the initial course will coincide with that for the azimuth ; by interchanging the latitudes of the points of departure and destination the final course will be similarly obtained . Advantage may thus be ...
... hour angle , the solution for the initial course will coincide with that for the azimuth ; by interchanging the latitudes of the points of departure and destination the final course will be similarly obtained . Advantage may thus be ...
Page 88
... Hour Circles , Declination Circles , or Celestial Meridians are great circles of the celestial sphere passing ... Angle of any point is the angle at the pole between the meridian of the observer and the hour circle passing through that ...
... Hour Circles , Declination Circles , or Celestial Meridians are great circles of the celestial sphere passing ... Angle of any point is the angle at the pole between the meridian of the observer and the hour circle passing through that ...
Page 89
... angle NZH , or the arc NH , from the north point , or the angle SZH , or the ... hour circle of the point and that of the First Point of Aries ; it may also ... angles , or planes , or a combination of these , is used to refer it to some ...
... angle NZH , or the arc NH , from the north point , or the angle SZH , or the ... hour circle of the point and that of the First Point of Aries ; it may also ... angles , or planes , or a combination of these , is used to refer it to some ...
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Common terms and phrases
azimuth barometer bearing celestial sphere Center chart Chro chronometer Church circle Coast Corr correction corresponding cosec course dead reckoning declination departure determined deviation Diff Difference of Latitude difference of longitude direction Dist E.
H. W.
L. W. Spg earth east equal equator EXAMPLE Extreme Flagstaff Greenwich Greenwich mean h. m.
h. m. ft Harbor Head horizon hour angle instrument intersection Island Islet light Lighthouse logarithm Long longitude lunitidal interval magnetic MARITIME POSITIONS mean sun measured meridian altitude method miles nat hav Nautical navigator Neap noon object Observatory observed altitude parallax parallel plane Port POSITIONS AND TIDAL prime vertical rhumb line right ascension Rock Sailing sextant ship ship's sidereal sight station Summit Sumner line sun's telescope theodolite TIDAL DATA tides true vertical vessel watch wind zenith distance
Popular passages
Page 257 - Each degree is divided into 60 equal parts called minutes, and each minute into 60 equal parts called seconds.
Page 26 - St.-Cu.) at the center of the group, but the thickness of the layer varies. At times the masses spread themselves out and assume the appearance of small waves or thin slightly curved plates. At the margin they form into finer flakes (resembling Ci.-Cu.) They often spread themselves out in lines in one or two directions.
Page 5 - Lines are generally marked as follows: 2 fathoms from the lead, with 2 strips of leather, 3 fathoms from the lead, with 3 strips of leather, 5 fathoms from the lead, with a white rag, 7 fathoms from the lead, with a red rag, 10 fathoms from the lead, with leather having a hole in it, 13 fathoms from the lead, same as at 3 fathoms...
Page 54 - ... the fixed arm. To plot a position, the two angles observed between the three selected objects are set on the instrument, which is then moved over the chart until the three beveled edges pass respectively and simultaneously through the three objects. The center of the instrument will then mark the ship's position, which may be pricked on the chart or marked with a pencil point through the center hole. The...
Page 142 - Having sailed from Charleston, SC, 25th November, 1837, bound for Greenock, a series of heavy gales from the westward promised a quick passage; after passing the Azores the wind prevailed from the southward, with thick weather; after passing longitude 21° W. no observation was had until near the land, but soundings were had not far, as was supposed, from the bank. The weather was now more boisterous and very thick, and the wind still southerly; arriving about midnight, 17th December, within 40 miles,...
Page 257 - THEOREM. Every section of a sphere, made by a plane, is a circle.
Page 86 - Moon, having a distance of 90° or more, are brought into contact just at the wire of the telescope which is nearest the plane of the sextant, fixing the index, and altering the position of the instrument 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...
Page 97 - 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 95 - Time, which is perfectly equable in its increase, is measured by the motion of this mean sun. The clocks in ordinary use and the chronometers used by navigators are regulated to mean solar time. True, or Apparent Solar Time is measured by the motion of the real sun. The difference between apparent and mean time is called the Equation of Time.