On triple objectives with complete color correction

C. S. Hastings
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Abstract

THE prime defect in the large refractors of tbe present day is the secondary spectrum. This, arising from the irrationality in the spectra. produced by the crown and flint glass, hardly noticeable in small apertures, detrimental in telescopes of medium power, is positively obnoxious in the large instl"Uments and will speedily put an end to farther increase in dimensions. On this account thel·e have been many efforts to produce two kinds of glass differing sufficiently in dispersive power, which would still yield mutually rational spectra. As far as I know we are now no nearer success in this direction than when Brewster investigated the subject fifty years ago. Can we secure the same end by increasing the number of glasses in the objective? Theoretically, since a new disposable constant for color change is introduced with each lens in the system, tbe answer is evidently affirmative; but if we limit ourselves by the condition that the construction shall be practicable, i. e., that there shall not be too many lenses and the curvatures shall be moderate, the conclusion is not so read.y. On entering the discussion we will assume three as the limiting number of lenses and n the focal length as the minimum radius of curvature. The formula Tor tbe focal lengtb F of three thin lenses in
在三个物镜上进行完全的色彩校正
目前大型折射望远镜的主要缺陷是二次光谱。这是由于光谱的不合理性。在小口径的望远镜中很难察觉,在中等倍率的望远镜中是有害的,在大口径的望远镜中是令人讨厌的,并且会很快阻止尺寸的进一步增加。由于这个原因,我们已经做了许多努力来生产两种色散功率足够不同的玻璃,这两种玻璃仍然会产生相互合理的光谱。据我所知,与50年前布鲁斯特研究这个问题时相比,我们现在在这个方向上并没有取得更大的成功。我们能否通过增加物镜中的镜片数量来达到同样的目的?从理论上讲,由于系统中的每个透镜都引入了一个新的一次性颜色变化常数,因此答案显然是肯定的;但是,如果我们把自己限制在构造必须可行的条件下,即不能有太多的透镜,曲率必须适中,那么结论就不那么容易理解了。在开始讨论时,我们将假定三个作为透镜的极限数量,并将焦距n作为曲率的最小半径。三个薄透镜的焦距F的公式
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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