Expand this Topic clickable element to expand a topic
Skip to content
Optica Publishing Group

Cryogenic Optical Testing of a Fused Quartz Mirror

Not Accessible

Your library or personal account may give you access

Abstract

The Space Infrared Telescope Facility (SIRTF) is an orbital, great observatory planned by NASA to enable diffraction-limited astronomical studies in the infrared from 2 μm to 700 μm. The telescope must be cryogenically cooled by Superfluid Helium at 2.5 K to provide the extreme sensitivity required for natural-background-limited observations. Concern about the image quality of the telescope operating at the extremely low temperature led to a cryogenic optics technology program.

© 1991 Optical Society of America

PDF Article
More Like This
Cryogenic Performance of the Space Infrared Telescope Facility Prototype Secondary Mirror Assembly

Mark T. Stier, John C. Doyle, Michael A. Duffy, Kenneth S. Gottschalck, Sarma N. Gullapalli, and Jeffrey W. Neuner
TuB3 Space Optics for Astrophysics and Earth and Planetary Remote Sensing (SO) 1991

Space Infrared Telescope Facility

David Norris, Mary Bothwell, and Joseph Plamondon
TuB1 Space Optics for Astrophysics and Earth and Planetary Remote Sensing (SO) 1991

Null test optics for large astronomical mirrors

J. H. Burge
WN2 OSA Annual Meeting (FIO) 1991

Select as filters


Select Topics Cancel
© Copyright 2024 | Optica Publishing Group. All rights reserved, including rights for text and data mining and training of artificial technologies or similar technologies.