newmask1avi













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http://youtube.com/watch?v=e3xWzopFQ4Q



This is the diffraction pattern produced by a new focussing mask for astronomical telescopes. There is software that uses line detecting algorithms to find the optimum focus for a Bahtinov Mask. • This variant produces pairs of intersecting lines that have a much greater relative displacement compared to a Bahtinov mask. This results in greater accuracy. • Optimum focus is reached at the point when the intersection points coincide. See here for how the Bahtinov works http://geoastro.co.uk/bahtinov.htm • This variant is the Carey mask http://geoastro.co.uk/bahtinov3.htm

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