The VLT interferometer. I - Proposed implementation

Details The VLT interferometer. I - Proposed implementation The VLT interferometer. I - Proposed implementation

Jul 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990spie.1236..108b&link_type=abstract

IN: Advanced technology optical telescopes IV; Proceedings of the Meeting, Tucson, AZ, Feb. 12-16, 1990. Part 1 (A91-23201 08-89

Physics

Optics

5

Imaging Techniques, Very Large Array (Vla), Very Long Base Interferometry, Adaptive Optics, Radio Astronomy, Signal To Noise Ratios, Speckle Interferometry, Systems Engineering, Telescopes

Scientific paper

The Very Large Telescope Interferometer (VLTI) is one of the operating modes of the VLT. In addition to consisting of the four stationary 8-meter-diameter telescopes, it includes a number of movable Auxiliary Telescopes which both complement the (u,v) plane coverage of the large telescopes and provide a powerful interferometric facility by itself (available 100 percent of the time). The current plans for the implementation of the VLTI are described. These plans will be finalized after the choice of the VLT site in 1990.

Affiliated with

Also associated with

No associations

Rating

The VLT interferometer. I - Proposed implementation 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 The VLT interferometer. I - Proposed implementation, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The VLT interferometer. I - Proposed implementation will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1097814