A Treatise on Trigonometry, Plane and Spherical: With Its Application to Navigation and Surveying, Nautical and Practical Astronomy and Geodesy, with Logarithmic, Trigonometrical, and Nautical Tables ...G.P. Putnam, 1851 - 372 pages |
From inside the book
Results 1-5 of 31
Page 4
... intervals usually but not necessarily equal to the whole breadth of the 10 spaces . The last one of these intervals is divided into ten spaces , and the first division at top is joined to the second at bottom , the second at top to the ...
... intervals usually but not necessarily equal to the whole breadth of the 10 spaces . The last one of these intervals is divided into ten spaces , and the first division at top is joined to the second at bottom , the second at top to the ...
Page 145
... * Degrees are converted into hours by multiplying by 4 and dividing by 60 , which is equivalent to dividing by 15 . be so adjusted , because the interval between the successive 10 DIFFERENT KINDS OF TIME . 145 nation,
... * Degrees are converted into hours by multiplying by 4 and dividing by 60 , which is equivalent to dividing by 15 . be so adjusted , because the interval between the successive 10 DIFFERENT KINDS OF TIME . 145 nation,
Page 146
... interval between the successive returns of the sun to the meridian is continually varying , on account of the unequal motion of the sun in its orbit , and of the obliquity of the ecliptic ; each of these varying intervals is called a ...
... interval between the successive returns of the sun to the meridian is continually varying , on account of the unequal motion of the sun in its orbit , and of the obliquity of the ecliptic ; each of these varying intervals is called a ...
Page 147
... interval of mean solar hours , or minutes , or seconds , the equivalent interval in siderial time . And similarly on pages 586 , 587 , for any given siderial interval will be found the equivalent mean solar interval . EXAMPLE . Required ...
... interval of mean solar hours , or minutes , or seconds , the equivalent interval in siderial time . And similarly on pages 586 , 587 , for any given siderial interval will be found the equivalent mean solar interval . EXAMPLE . Required ...
Page 150
... interval of time between the superior and inferior transit be the same with that between the latter and the next superior transit of the same star again , the instrument is in the meridian . If not , it is on that side of the meridian ...
... interval of time between the superior and inferior transit be the same with that between the latter and the next superior transit of the same star again , the instrument is in the meridian . If not , it is on that side of the meridian ...
Contents
33 | |
34 | |
50 | |
54 | |
66 | |
72 | |
75 | |
80 | |
85 | |
102 | |
103 | |
109 | |
115 | |
122 | |
128 | |
131 | |
136 | |
157 | |
164 | |
171 | |
174 | |
224 | |
237 | |
244 | |
251 | |
252 | |
257 | |
267 | |
273 | |
279 | |
294 | |
303 | |
315 | |
321 | |
329 | |
335 | |
341 | |
349 | |
352 | |
358 | |
365 | |
111 | |
Other editions - View all
Common terms and phrases
altitude azimuth called celestial sphere centre circle colatitude collimation column comp computed correction corresponding cos² cosc cosec cotangent course decimal declination departure determined diagram diff difference of latitude difference of longitude divided equal equation error EXAMPLE expressed feet formula Geom given number hence horizontal hour angle hypothenuse instrument intersection limb logarithm longitude means measured meridian miles multiplied Nautical Almanac number of degrees object observed obtained parallax parallel perpendicular plane sailing plane triangle polar pole proportion quadrant quotient radius right angled triangle right ascension sailing screw secant second member semidiameter ship side opposite siderial sin a sin sin² sine and cosine sine of half solution sphere spherical triangle spherical trigonometry spirit level star subtracting supporting axis tangent telescope transit trigonometrical lines vernier vertical wire zenith distance
Popular passages
Page 204 - ... 6. The latitude of a place is its distance north or south of the equator, measured on the meridian of the place.
Page 136 - The sine of half the sum of two angles of a spherical triangle is to the sine of half their difference as the tangent of half the interjacent side is to the tangent of half the difference of the other two sides.
Page 33 - The logarithm of a number is the exponent of the power to which it is necessary to raise a fixed number, in order to produce the first number.
Page 86 - When a ray of light passes from one medium to another, it is refracted so that the ratio of the sine of the angle of incidence to the sine of the angle of refraction is equal to the ratio of the velocities in the two media.
Page 79 - 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.
Page 66 - FH is the sine of the arc GF, which is the supplement of AF, and OH is its cosine ; hence, the sine of an arc is equal to the. sine of its supplement ; and the cosine of an arc is equal to the cosine of its supplement* Furthermore...
Page 219 - Then, along the horizontal line, and under the given difference of latitude, is inserted the proper correction to be added to the middle latitude to obtain the latitude in which the meridian distance is accurately equal to the departure. Thus, if the middle latitude be 37°, and the difference of latitude 18°, the correction will be found on page 94, and is equal to 0° 40'. EXAMPLES. 1. A ship, in latitude 51° 18...
Page 213 - A2,lay off the distance BC = 23 miles; in the direction parallel to A3, lay off CD = 36 ; in the direction parallel to A4, lay off DE = 12 miles ; and, lastly, in the direction parallel to A5, lay off EF = 41 ; then F will be the place of the ship at the end of the traverse ; consequently, AF will be the distance made good, and the angle FAS the direct course ; applying, therefore, the distance AF to the scale of equal parts, we shall find it reach from 0 to 62| ; and applying the distance Sa to...
Page 284 - ZP. Now, in the triangle PSS', we have given two sides and the included angle to find the third side SS', and one of the remaining angles, say the angle PSS'.
Page 13 - SINE of an arc, or of the angle measured by that arc, is the perpendicular let fall from one extremity of the arc, upon the diameter passing through the other extremity. The COSINE is the distance from the centre to the foot of the sine.