Mathematical tracts on the lunar and planetary theories, the figure of the earth, precession and nutation, the calculus of variations, and the undulatory theory of optics.

262 UNDULATORY TIEORY OP OPTICS. Case 1. Suppose X much greater than b. (This will generally be the case with sound, as for all audible sounds X varies from a few inches to several feet.) Here - O will be a small arc, and will not differ X much from its sine: putting the arc for the sine, the maximum of vibration becomes cX 2 7rb cos 0 2cb, or -,5 7rrcosO r which is the same for all values of 0. Case 2. Suppose X much smaller than b. (This will generally be the case with light.) For the part nearly opposite to the entering wave, cos 0 is very small, and cX 27rb cos 2cb.sin - 7r cos 0 \X r In other parts it is to be observed that the disturbance is o when 27rb cos 0 - r or =o 2r, or = 2, or = 7r, &c., that is, when X 2X 3X cos O= 6 -, or =5 or = - &c. 2b 2b 2b Hence there is a succession of points in which there is absolute darkness. Of the intermediate parts, the brightest will be found (nearly) by making 27b cos 0 sin = 1 cX then the maximum of vibration is.Consequently -r cos the intensity of light at the brightest part of one of the bright portions is to that of the part nearly opposite to the entering

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Title
Mathematical tracts on the lunar and planetary theories, the figure of the earth, precession and nutation, the calculus of variations, and the undulatory theory of optics.
Author
Airy, George Biddell, Sir, 1801-1892.
Canvas
Page 248
Publication
Cambridge,: J. & J.J. Deighton;
1842.
Subject terms
Celestial mechanics.
Calculus of variations
Geometrical optics.

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"Mathematical tracts on the lunar and planetary theories, the figure of the earth, precession and nutation, the calculus of variations, and the undulatory theory of optics." In the digital collection University of Michigan Historical Math Collection. https://name.umdl.umich.edu/aan8938.0001.001. University of Michigan Library Digital Collections. Accessed April 30, 2025.
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