Abstract
A high performance infrared spaceborne telescope such as the Space Infra-Red Telescope Facility (SIRTF) will require aspheric optical forms with smooth, low-scatter surface, high performance coatings, and an ultra-lightweight design approach that can perform from room temperature to cryogenic temperature. The design approach must not only be rugged, low risk, and reliable, but also capable of surviving a launch environment and enduring in space for many years. A design approach, which meets performance requirements at cryogenic temperatures employing passive mirrors (without figure control actuators, sensors, electronics, etc.), offers significant advantage in weight, performance, and reliability.
© 1987 Optical Society of America
PDF ArticleMore Like This
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
Ramsey K. Melugin, Gordon C. Augason, Steven D. Howard, and Jeffrey A. Young
TuB2 Space Optics for Astrophysics and Earth and Planetary Remote Sensing (SO) 1991
H. Philip Stahl
OMC1 Optical Fabrication and Testing (OF&T) 2002