A fast tracking Mirror for Adaptive Optics

Details A fast tracking Mirror for Adaptive Optics A fast tracking Mirror for Adaptive Optics

Sep 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996ap%26ss.239..213k&link_type=abstract

Astrophysics and Space Science, Volume 239, Issue 2, pp.213-219

Physics

Optics

1

Adaptive Optics, Mirrors

Scientific paper

A piezo driven tilt mirror was developed and built as one component of an image motion compensation system for a solar telescope. The bandwidth of the mirror with a diameter of 60 mm is about 1 kHz with negligible phase shift between input signal and mirror response up to 900 Hz. The tilt range is 1.6 mrad. Special care was taken to maintain the surface quality of the mirror to better than λ/15 after fixing it to the substrate.

Affiliated with

Also associated with

No associations

Rating

A fast tracking Mirror for Adaptive Optics 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 A fast tracking Mirror for Adaptive Optics, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and A fast tracking Mirror for Adaptive Optics will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1457695