Atmospheric dispersion compensation for extremely large telescopes

Physics – Optics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

3

Active Or Adoptive Optics, Atmospheric Propagation, Telescopes, Aberration Compensation

Scientific paper

Achieving diffraction limited imaging with future ground-based optical telescopes will require adaptive optics for correction of atmospheric turbulence and also efficient techniques for atmospheric dispersion compensation. We study the benefit of using a linear atmospheric dispersion corrector (ADC) coupled with a deformable mirror on a 42-m Extremely Large Telescope (ELT) operating in the VIRJ spectral bands. The ADC design consists of two identical thin wedges made of F5 glass. The amount of dispersion introduced by the ADC is adjusted by translating one of the wedges along the optical axis so that it always cancels atmospheric dispersion as it varies with telescope elevation. We show that the ADC working in conjunction with a deformable mirror provides diffraction-limited image quality over a 1-arcmin field.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Atmospheric dispersion compensation for extremely large telescopes does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Atmospheric dispersion compensation for extremely large telescopes, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Atmospheric dispersion compensation for extremely large telescopes will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-1156287

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.