 | Tobias Smollett - 1803 - 614 sider
...Lieut. Maignon, respecting theoretic and practical Explanations of a trigonometric Chart for reducing the apparent Distance of the Moon from the Sun, or a Star, at a true Distance, and for resorving other Questions of Navigation, by M. 1'Eveque.' — This is an... | |
 | Jeremias David Reuss - 1804 - 588 sider
...des parallaxes. Mem. de l'Acad. des Se. de Paris. A. 1764. Mem. p. 489. Nevil MASKPXYNE, \ Cotacise rules for computing the effects of refraction and...varying the apparent distance of the moon from the sub, or a star; abo an eaey rule of approximation for computing the distance of the moon from a star,... | |
 | John Bonnycastle - 1806 - 464 sider
...hour from noon when each altitude was taken, the azimuth at each observation, 8rc. 241 PROBLEM XXII. The apparent distance of the moon from the sun, or a star, and their apparent altitudes, or zenith distances, being given, to find their true distances, as seen... | |
 | Thomas Thomson - 1813 - 514 sider
...on the Tides in the Island of St. Helena. Ibid. p. 586. 8. Concise Rules for computing the Effeots of Refraction and Parallax in varying- the apparent Distance of the Moon from the Sun or a Star; also an Easy Rule of Approximation for computing the Distance of the Moon from a Star, the Longitudes... | |
 | Ralph Griffiths, George Edward Griffiths - 1814 - 574 sider
...discussions of this subject wholly unnecessary. Investigations relative to the Problem for clearing the apparent Distance of the Moon from the Sun or a Star, from the Effects of Parallax and Refraction, and an easy and concise Method pointed out. By the Same.—The... | |
 | 1814 - 574 sider
...discussions of this subject wholly unnecessary. Investigations relative to the Problem for clearing the apparent Distance of the Moon from the Sun or a Star, from the Effects of ^ Parallax and Refraction, and an easy and concise Method pointed out. By the Same.... | |
 | American Academy of Arts and Sciences - 1818 - 474 sider
...equal to i°-Jl°.a. [lf-ft. cos.S(f+e)|. sin. y — 3°. a ft. cos. S(f +C). IV. Method of correcting the apparent distance of the Moon from the Sun, or a Star for the effects of Parallax and Refraction. BY NATHANIEL BOWDITCH, LL. D. A HE method of correcting... | |
 | John Farrar - 1822 - 270 sider
...means of a table of the t There arc many ways of abridging the process for ohtaining the true from the apparent distance of the moon from the sun or a star. The object of the above is merely to illustrate the essential parts of the operation to the theoretical... | |
 | John Farrar - 1822 - 244 sider
...means of a table of the t There are many ways of abridging the process for obtaining the true from the apparent distance of the moon from the sun or a star. The object of the above is merely to illustrate the essential parts of the operation to the theoretical... | |
 | Robert Watt - 1824 - 720 sider
...tbe Sun and Fixed Stars. Ib 636 — Observations on the Tides at the Island of Si. Helen«. Ib. 647. —Concise Rules for Computing the Effects of Refraction...apparent Distance of the Moon from the Sun, or a Star, See. Ib. 152. 1764. — On the Equation of Time, and true Manner of Computing it. Ib. 163. — Astronomical... | |
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Method of correcting the apparent distance of the Moon from the Sun, or a Star, for the effects of Parallax and Refraction. 
