Paper
23 July 2008 A super-corrected atmospheric dispersion corrector
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Abstract
The effects of atmospheric dispersion are well known in astrometry and astronomical spectroscopy. To reduce these effects, glass prisms are used. Two different prisms, coupled together, give better corrections. However glass dispersion curves do not match very well the dispersion of the atmosphere and secondary spectrum of the order of 50-100 milliarcseconds (mas) or more will be present. I propose a method to find solutions with residuals less than few parts of 10 milliarcsecond and I show some results.
© (2008) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Paolo Spanò "A super-corrected atmospheric dispersion corrector", Proc. SPIE 7018, Advanced Optical and Mechanical Technologies in Telescopes and Instrumentation, 70181G (23 July 2008); https://doi.org/10.1117/12.789161
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Cited by 1 scholarly publication.
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KEYWORDS
Glasses

Prisms

Refractive index

Telescopes

Atmospheric modeling

Ray tracing

Zemax

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