Finding the circle of least confusion for a multi-element optical system

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SUMMARY

The optimal placement of an image sensor in a multi-element optical system is at the circle of least confusion, which is influenced by aberrations that alter the point spread function. Aberrations such as spherical and astigmatic aberrations affect the image formation, moving it away from the Gaussian focus. To accurately determine the circle of least confusion, detailed ray tracing is necessary, particularly using ray heights of 0.866d and 0.707d, which correspond to conventional practices. There is no straightforward formula to replace paraxial ray tracing; however, implementing a ray trace algorithm in Excel or using specialized software can facilitate this process.

PREREQUISITES
  • Understanding of optical aberrations, including spherical and astigmatic aberrations
  • Familiarity with ray tracing techniques in optical systems
  • Knowledge of the concept of the circle of least confusion in optics
  • Basic skills in using Excel for algorithm implementation
NEXT STEPS
  • Research detailed ray tracing methods for optical systems
  • Explore software tools for optical design, such as Zemax or Code V
  • Learn about the impact of different types of aberrations on image quality
  • Study the mathematical principles behind the circle of least confusion
USEFUL FOR

This discussion is beneficial for mechanical engineers transitioning into optics, optical engineers, and anyone involved in designing or analyzing multi-element optical systems.

nevhuan
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Hi,

I'm a mechanical engineer that's new to optics. I'm trying to determine the best location to place an image sensor for an optical system with multiple lenses and mirrors. In doing so, I've come to the understanding that the best position to put the sensor is at the circle of least confusion. However, I have a few questions:

1. Just to confirm, does this mean that the image is no longer formed at the Gaussian focus due to aberrations in the system?

2. From my understanding, the only way to find the circle of confusion is to find the focal point for a ray that enters the entrance pupil of the system at a height of 0.866d or 0.707d etc. I used the information from this website: "[URL ).[/URL] I notice that this only considers spherical aberration. What about astigmatic aberrations etc?

3. Is there a formula I can use in place of paraxial raytracing and aberration calculations?

Many thanks,
N.
 
Last edited by a moderator:
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nevhuan said:
Hi,

I'm a mechanical engineer that's new to optics. I'm trying to determine the best location to place an image sensor for an optical system with multiple lenses and mirrors. In doing so, I've come to the understanding that the best position to put the sensor is at the circle of least confusion. However, I have a few questions:

1. Just to confirm, does this mean that the image is no longer formed at the Gaussian focus due to aberrations in the system?

2. From my understanding, the only way to find the circle of confusion is to find the focal point for a ray that enters the entrance pupil of the system at a height of 0.866d or 0.707d etc. I used the information from this website: "[URL ).[/URL] I notice that this only considers spherical aberration. What about astigmatic aberrations etc?

3. Is there a formula I can use in place of paraxial raytracing and aberration calculations?

Many thanks,
N.

The website is http://www.telescope-optics.net/spherical1.htm"
 
Last edited by a moderator:
nevhuan said:
Hi,

I'm a mechanical engineer that's new to optics. I'm trying to determine the best location to place an image sensor for an optical system with multiple lenses and mirrors. In doing so, I've come to the understanding that the best position to put the sensor is at the circle of least confusion. However, I have a few questions:

1. Just to confirm, does this mean that the image is no longer formed at the Gaussian focus due to aberrations in the system?

Yes- aberrations change the shape and location of the point spread function. Object points do not get mapped to an Airy disk, and the Airy disk is not uniform over the image plane.

nevhuan said:
2. From my understanding, the only way to find the circle of confusion is to find the focal point for a ray that enters the entrance pupil of the system at a height of 0.866d or 0.707d etc. I used the information from this website: "[URL ).[/URL] I notice that this only considers spherical aberration. What about astigmatic aberrations etc?

It has been a while since I've done detailed ray tracing, but AFAIK the answer to the first question is 'not really'. The ray heights 0.866 and 0.707 correspond to the 'midpoint' (0.707) and 75% (0.866) of the entrance pupil diameter, those were chosen for convenience (and now, convention). But, in order to locate the circle of least confusion, a detailed ray trace must be performed.

Other aberrations will change things as well- astigmatic aberrations result in a 'medial' focal plane, similar to the circle of least confusion. Coma is another common aberration in telescope optics: off-axis stars are imaged as elliptical blobs.

nevhuan said:
3. Is there a formula I can use in place of paraxial raytracing and aberration calculations?

Many thanks,
N.

I don't know of a simple formula that gives you the results you want. Ray tracing is fairly simple to perform (although it's also time consuming to perform by hand)- you can implement a ray trace algorithm in Excel, and there may even be semi-free programs available.
 
Last edited by a moderator:

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