Design and implementation of an image stabilization device at the THEMIS solar telescope

Details Design and implementation of an image stabilization device at the THEMIS solar telescope Design and implementation of an image stabilization device at the THEMIS solar telescope

Oct 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008exa....22...67g&link_type=abstract

Experimental Astronomy, Volume 22, Issue 1-2, pp. 67-85

Astronomy and Astrophysics

Astronomy

1

Sun, Solar Instrumentation, Solar Observation, Atmospheric Turbulence, Image Stabilizer

Scientific paper

An image stabilizer has been inserted into the optical path of the THEMIS solar telescope. THEMIS is a Ritchey Chretien reflector telescope using an altazimuthal mount and closely tied to its spectrograph. The optical and mechanical design, implementation and system tests are described, and emphasis is put on the complexity of situations that this stabilizer must accept, including the scanning of the solar surface while stabilizing. The current closed-loop crossover frequency of the device is 65 Hz at - 3 dB on all typical solar scenes.

Affiliated with

Also associated with

No associations

Rating

Design and implementation of an image stabilization device at the THEMIS solar telescope 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 Design and implementation of an image stabilization device at the THEMIS solar telescope, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Design and implementation of an image stabilization device at the THEMIS solar telescope will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1699968