LVI. Investigations in optics, with special reference to the spectroscope
LVI. Investigations in optics, with special reference to the spectroscope
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DOI:
10.1080/14786447908639715
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发表时间:
1879-12
期刊:
影响因子:
--
通讯作者:
Lord Rayleigh F.R.S.
中科院分区:
文献类型:
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作者:
Lord Rayleigh F.R.S.
478 Lord Rayleigh's Inve~ tlgatioT~ s in Optics. approximating to a plane, which will answer the purpose, coincides with the family of surfaces most likely to beproduced; in the second case the family of ellipsoidal or hyperbolic surfaces capable (with suitable focus) of giving good definition contains only one symmetrical member--the perfect plane. In order to test experimentally the correctness of the theoretical result, it would be necessary to retain the focus suitable to the true surface, and not to allow a readjustment by which its errors may be in greater or less degree compensated. A further difficulty~ not touched by the preceding considerations, still remains to be mentioned. In the ordinary method of testing plane surfaces by measuring the change of focus required when a distant point is viewed through a telescope, first directly, and then after reflection in the surfacej the test is found to be more delicate as the reflection is more oblique. The explanation of the apparent inconsistency will be best understood by a calculation of the focal length of mirrors, founded directly upon the principles of the wave theory. Let ACB (fig. 8) be an arc of a (parabolic) mirror, which reflects parallel rays GA, tt D, KB Fig. 8. to a focus F. AD= y, DF= f, CD= t. In calculating the retardations of the various rays~ we will take as standard the phase at F of a ray coincident with HD~ reflected at D (as by a plane mirror ADB) instead of at