A laser guide-star experiment performed at the National Solar Observatory's Vacuum Tower Telescope on Sacramento Peak, New Mexico, on November 20th, 1997. Picture by Fang Shi.
Downloadable versions (see
NOAO Conditions of Use):
Laser-Guide-Star at the Sacramento Peak Vacuum Tower Telescope
The University of Chicago Adaptive Optics System (ChAOS) group
has been developing its sodium laser-guide-star system at the Sac Peak
solar Vacuum Tower Telescope (VTT), since the VTT provides a good
optics laboratory environment combined with a good supply of nighttime
observing time. ChAOS is a high-order laser-guide-star adaptive optics
(AO) system built for the large ground-based astronomical telescopes.
One of the critical techniques in the system is to generate an
artificial star in the upper atmosphere for the AO system's wavefront
sensor. Using a laser with wavelength tuned to the sodium D2 line
shining upon the mesosphere at about 90 kilometers above sea level, a
bright "sodium star" can be generated.
The picture shows the laser-guide-star experiment at the NSO VTT. During
the experiment, the artificial star, as bright as the 9th magnitude
and as small as about the size of a natural star, was generated, and
various factors that affect the quality of the artificial star were
explored. The VTT was used to launch the laser beam to the mesosphere
and observe the return light from the generated artificial star
simultaneously. The photo was taken during the experiment on the night
of 20 November 1997. In the photo, the VTT was lit up by moonlight and
a 4-watt laser beam was launched from the top of the telescope. Some
well-known constellations such as Orion and Taurus are also visible in
the picture.
Fang Shi, Ed Kibblewhite, Jacques Beckers
Minimum credit line: Fang Shi/NSO/NOAO/AURA/NSF
(for details see Conditions of Use)
400 x 558 37 kb color JPEG
1468 x 2047 480 kb color JPEG
1468 x 2047 2.9 Mb 8-bit color TIFF
1468 x 2047 8.8 Mb 24-bit color TIFF
From the NOAO Newsletter for June 1998 (Number 54)
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