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Above
image shows 4.3m Discovery Channel Telescope primary mirror in the
OEFF.
Optical Engineering
and Fabrication Facility
The
Optical Systems Development and Fabrication section of The College
of Optical Sciences at The University of Arizona, is a fully
functional optical design and fabrication facility. This department,
headed by Martin Valente, houses a large optics shop, a small optics
shop, opto-mechanical engineering facility, instrument shop, optical
generation equipment, and optical testing equipment.
The small optics shop opticians have vast experience in fabricating
precision optical components from many different types of glasses,
ceramics and metals. Completed in the small optics shop was an all
metal matrix composite 16" R-C telescope and spectrograph launched
on the Space Shuttle on 10/29/98. Other work done in the small
optics shop includes two facetted quartz blocks for the Gravity
Probe B spaceborne experiment. These blocks are roughly 7" in
diameter and 22" long with geometrically constrained facets which
prevent the use of standard polishing equipment. These facets were
hand polished and held to one arcsecond orthogonality requirements
in two planes. Other work includes several F/0.5 EUV Imager mirrors
with eighth wave surfaces and three Angstrom roughness, an all
SXA(Silicon Carbide/Aluminum) Ritchey-Chretien telescope with a 16
inch diameter foam SXA primary and 15 element lens bench, and a 10"
aperture astrographic lens with diffraction limited performance and
zero distortion over a 10 degree field of view.
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The large optics shop facilities include various polishing machines
with turntables up to 170 inches in diameter, a temperature
stabilized environment, a 125 foot vertical optical test tower, and
a 26 foot vertical optical test tower. The large optics shop is
equipped with IR and visible interferometers, and has developed a
high speed CCD based interferometer, which has excellent performance
over long optical path lengths or in non-ideal testing environments.
Examples of work done in the large optics shop include the
technology demonstrator for the James Webb Space Telescope (JWST)
and a convex mold to be used for the technology demonstrator in the
Far Infrared Space Telescope (FIRST) program. The NGST demonstrator
is a 2 meter diameter 2 mm thick shell which will be actively
controlled for figure correction. The FIRST mold is a 2 meter
diameter F/1 convex sphere which will be used for demonstrating
replicating technology for graphite-composite based optics.
Currently underway in the large optics shop is an approximately
three year project to grind and polish the primary mirror for the
Discovery Channel Telescope (DCT) which is to be housed at Lowell
Observatory. The capacity of the turntable was increased, and a
computer controlled polisher was designed for the completion of the
project. The F/1.9 mirror blank is approximately 4.3 meters. If the
completed mirror were expanded to the size of the United States, the
maximum deviation would be a mere one inch.
The opto-mechanical engineering and instrument shop personnel
design and fabricate such devices as optical support structures,
space and ground based telescopes, precision optical test
instruments, and related equipment. They also perform mirror
structural design, structural analysis and opto-mechanical research
on various subjects, including optimization and mounting of lens
systems and mirrors. Among other projects, they have designed large
optical telescopes and telescope subsystems, space-based detectors,
and airborne optical instruments for government and industry.
Martin Valente, OEFF Director
"The partnership
between OEFF and the LOFT research group (Large Optics Fabrication
and Testing) provides OEFF staff with opportunities to contribute to
basic research, and provides technology for OEFF projects. Optical
Sciences students get real experience with optical systems
engineering, fabrication, and testing. Combined with the strong
academic program, such skills make our graduates among the top in
the world." James H. Burge, LOFT PI
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