Quantifying Mirror Distortion ```Name: Enrique C. Status: educator Age: 50s Location: N/A Country: N/A Date: 2/26/2003 ``` Question: How can the distortion of an image viewed in a mirror be stated, or quantified? Replies: Enrique, As you may already know, introductory and advanced physics textbooks contain many mathematical formulas that relate to how and where an image is produced by lenses and mirrors. However, "distortion of an image" is in the eye of the beholder -- it can be described, but not "quantified." For example, is the distortion to which you refer the result of an out-of-focus condition, astigmatism, lack of contrast, barrel distortion, pincushion distortion, spherical or chromatic aberration etc.? That which constitutes distortion in the eye of a person with perfect eyesight might not even be noticed by one with less than perfect vision. Regards, ProfHoff 595 If you mean a flat mirror, then the distortions are just a result of it not being flat. These can be quantified in terms of how many wavelength different are the various paths to the image. After all, if an mirror is to reflect, all "rays" from a object point should make it to the image with the same optical path, and the mirror should not be so wavy that it throws other light into the path. If you want to go further, then a flat mirror is just a special case of a curved mirror. The distortions of a curved mirror are quantified the same as the distortions in a lens. This means that with few changes to the math, applying the same equations, you can understand mirrors as easily as lenses, for optics. Under the heading of 5th order aberrations or corrections, people came up with 5 distortions: spherical aberration (SA), coma, astigmatism, field distortion, curvature of field long ago (before computers). These are called the Siedel aberrations I think. But again this was a way to explain problems with optics in an age before exact computations were easy. So people spent much time on this, and there are chapters in optics books on the subject, with lots of equations. These aberrations produce very recognizable distortions. SA makes the image dot sort of a fuzzy circle, but symmetric. (Its what the Hubble Space Telescope had when first launched, and they needed to correct by going back with astronauts). Coma leads to a "comet" like tail on the image. Astigmatism can be seen sort of if you rotate the lens -- take a pair of glasses from someone who has astigmatism, and rotate them, but continue to look through the lens, and look at a piece of graph paper. You will see the lines of the graph paper wave around. Now try this with a pair of reading glasses from K-mart (no astigmatism correction), you do not see the same. Distortion makes a piece of graph paper look like a barrel instead of a square grid etc, etc. I doubt many people know these equations by heart anymore, but the affects are still useful to simplify things. (It is not much fun to just tell people go run a computer code, it helps to know how things scale, or change if you "tweak" on this or that). The useful thing here is the simple equations guide you. You see that some aberrations cannot be seen if the light is basically going through the center of the lens. In this case, in the day time, your pupils contract, you only use the center of the lens, and you do not see the effect (same with camera on a bright sunny day). But if you need to open up the lens more, then more of the glass is being used, and you pick up the effects. Of course modern cameras have these things pretty well eliminated. I refer you to almost any college level book on optics, but do not bother too much with the math, look for pictures of how the image gets distorted. Steve Ross Click here to return to the Physics Archives

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