How to match the very large telescopes with a high dispersion spectrograph efficiently?

Details How to match the very large telescopes with a high dispersion spectrograph efficiently? How to match the very large telescopes with a high dispersion spectrograph efficiently?

Jun 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992pabei..10..136j&link_type=abstract

Prog. Astron., Vol. 10, No. 2, p. 136 - 142

Physics

Optics

Scientific paper

The author points out the difficulties encountered in matching efficiently a very large telescope with a high dispersion spectrograph. After analysing the advantages and disadvantages of the very large grating, the mosaic grating, the superwidth grating and the image slicer, the author mentions the MMT and its analogy. He calls all these as sub-aperture methods. Then he introduces a new way, the sub-aperture adaptive optics-optical fiber system after the primary, and analyses its advantages and disadvantages.

Affiliated with

Also associated with

No associations

Rating

How to match the very large telescopes with a high dispersion spectrograph efficiently? 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 How to match the very large telescopes with a high dispersion spectrograph efficiently?, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and How to match the very large telescopes with a high dispersion spectrograph efficiently? will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1523013