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| subject: | Re: ATM daytime star testing with sun |
From: "Frank Q" To: "CSC" , "Atm" Reply-To: "Frank Q" Hi All Regarding artificial star -> mirror distance, I crunched some numbers and came up with the following for a 8" F/5 mirror: Mirror/"star" distance KE-Difference 2 * FL 5.006 mm 10*FL 0.555 mm 20*FL 0.263 mm 40*FL 0.128 mm 80*FL 0.063 mm 160*FL 0.031 mm Where: * The "star" is the ball-bearing illuminated by the sun. * The 2*FL, 10*FL etc represent a slit(star) to mirror distance of 2 x Focal-Length, 10 x Focal-Length etc * The "KE-Difference" is the difference between where the rays from the outermost and innermost zones are focussed. Note that for a stationary "star" and moving knife edge, the difference is (r^2) / R = 5.006 mm which corresponds to the 2 * FL entry in the above table (2 * FL = Radius of Curvature) as expected. * The above results were obtained using a ray-tracing algorithm So, from the above numbers, it appears that for a **perfectly** corrected parabolic mirror, the KE-Difference is zero if the "star" is at infinity - in other words, a Focault knife edge test will be a null test. But if the "star" is 10 focal lengths away, you will observe the characteristic dough-nut shadows consistent with an 11% corrected mirror and 1.3% corrected at 80 focal lengths. Cheers Frank Q --- BBBS/NT v4.01 Flag-4* Origin: Email Gate (1:379/100) SEEN-BY: 633/267 270 @PATH: 379/100 1 106/1 2000 633/267 |
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