Comparing Chromatic Aberration Quantitatively?

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Two lens systems for basic astronomy are being compared for chromatic aberration: a telephoto lens and an objective from an old pair of binoculars. An experimental setup is suggested to quantitatively measure chromatic aberrations using colored lasers and standard spectral lines. The discussion highlights the importance of factors such as image distance and f/# in optical testing. A 'star test' is recommended to observe the differences in image location at various wavelengths, distinguishing between transverse and longitudinal chromatic aberration. The measurements are expected to show displacements on the order of microns, providing insight into the performance of both systems.
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Hi, I have 2 similar lens systems used for basic astronomy (as refracting telescopes). The first is a telephoto lens designed for a camera and the second is the main objective of an old pair of binocs paired with an eyepiece in a tube. I am suspecting the former exhibits more chromatic aberration just based on some observations of the moon and bright stars.

I was wondering if there is an experimental setup I could perform, even crudely, on my workbench tabletop that would allow me to compare the chromatic aberrations of both systems quantitatively.
 
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If you have two different colored lasers, you can measure their refraction angles.
 
mishima said:
I was wondering if there is an experimental setup I could perform, even crudely, on my workbench tabletop that would allow me to compare the chromatic aberrations of both systems quantitatively.

As with any optical test, the details matter: image and object distance, field height, f/#... There are two 'flavors' of chromatic aberration- transverse (or lateral) and longitudinal, and these are independent.

Start with the standard spectral lines: 656.3, 587.6, and 486.1 nm. If you don't have access to a 'clean' spectral source, you can probably use a compact fluorescent source. Use of a broadband source (sunlight) will make the measurement more difficult.

The simplest measurement is a 'star test': image a point source and compare the locations of the image at different colors: transverse chromatic will shift the image from side to side, while longitudinal will shift the focal plane along the optical axis. Note that typical chromatic aberrations in a reasonably corrected lens will give displacements on the order of microns. Imaging the 'star' at different field heights and stop sizes will characterize the system.
 
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