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lumination at a particular point O due to all the components which have their foci in its neighbourhood, we may conveniently regard O as origin. [xi] is then the co-ordinate relatively to O of any focal point O' for which the retardation is R; and the required result is obtained by simply integrating (5) with respect to [xi] from -[oo] to +[oo]. To each value of [xi] corresponds a different value of [lambda], and (in consequence of the dispersing power of the plate) of R. The variation of [lambda] may, however, be neglected in the integration, except in 2[pi]R/[lambda], where a small variation of [lambda] entails a comparatively large alteration of phase. If we write [rho] = 2[pi]R/[lambda] (6), we must regard [rho] as a function of [xi], and we may take with sufficient approximation under any ordinary circumstances [rho] = [rho]' + [=omega][xi] (7), where [rho]' denotes the value of [rho] at O, and [=omega] is a constant, which is positive when the retarding plate is held at the side on which the lue of the spectrum _is seen_. The possibility of dark bands depends upon [=omega] being positive. Only in this case can cos {[rho]' + ([=omega] - 2[pi]h/[lambda]f)[xi]} retain the constant value -1 throughout the integration, and then only when [=omega] = 2[pi]h / [lambda]f (8) and cos [rho]' = -1 (9). The first of these equations is the condition for the formation of dark bands, and the second marks their situation, which is the same as that determined by the imperfect theory. The integration can be effected without much difficulty. For the first term in (5) the evaluation is effected at once by a known formula. In the second term if we observe that cos {[rho]' +([=omega] - 2[pi]h/[lambda]f)[xi]} = cos {[rho]'- g1[xi]} = cos [rho]' cos g1[xi] + sin [rho]' sin g1[xi], we see that the second part vanishes when integrated, and that the remaining integral is of the form _+[oo] / d[xi] w = | sin^2 h1[xi] cos g1[xi] ------, _/-[oo] [xi]^2 where h1 = [pi]h/[lambda]f, g1 = [omega] - 2[pi]h/[lambda]f (10). By differentiation wi
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