Khác biệt giữa bản sửa đổi của “Quang sai (quang học)”

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Dòng 122:
If a constant of reproduction, for instance the focal length, be made equal for two colours, then it is not the same for other colours, if two different glasses are employed. For example, the condition for achromatism (4) for two thin lenses in contact is fulfilled in only one part of the spectrum, since dn2/dn1 varies within the spectrum. This fact was first ascertained by J. Fraunhofer, who defined the colours by means of the dark lines in the solar spectrum; and showed that the ratio of the dispersion of two glasses varied about 20% from the red to the violet (the variation for glass and water is about 50%). If, therefore, for two colours, a and b, fa = fb = f, then for a third colour, c, the focal length is different; that is, if c lies between a and b, then fc<f, and vice versa; these algebraic results follow from the fact that towards the red the dispersion of the positive crown glass preponderates, towards the violet that of the negative flint. These chromatic errors of systems, which are achromatic for two colours, are called the ''secondary spectrum,'' and depend upon the aperture and focal length in the same manner as the primary chromatid errors do.
 
In fig. 11, taken from M. von Rohr,s ''Theorie und Geschichte des photographischen Objectivs'', the abscissae are focal lengths, and the ordinates wave-lengths; of the latter the Fraunhofer lines used are-- :
{| {{prettytable}}
 
|-
A' C D Green Hg. F G' Violet Hg. 767.7 656.3 589.3 546.1 486.2 454.1 405.1 mm,
!Điểm !! Bước sóng
 
|-
|A' || 767.7
|-
|C || 656.3
|-
|D || 589.3
|-
|Green Hg. || 546.1
|-
|F || 486.2
|-
|G' || 454.1
|-
|Violet Hg. || 405.1 mm,
|}
[[Image:ABERR6rev.png|left|]]