Published October 8, 1992 | Version v1
Report Restricted

Tip-tilt compensation: Resolution limits for ground-based telescopes using laser guide star adaptive optics

Description

The angular resolution of long-exposure images from ground-based telescopes equipped with laser guide star adaptive optics systems is fundamentally limited by the the accuracy with which the tip-tilt aberrations introduced by the atmosphere can be corrected. Assuming that a natural star is used as the tilt reference, the residual error due to tilt anisoplanatism can significantly degrade the long-exposure resolution even if the tilt reference star is separated from the object being imaged by a small angle. Given the observed distribution of stars in the sky, the need to find a tilt reference star quite close to the object restricts the fraction of the sky over which long-exposure images with diffraction limited resolution can be obtained. In this paper, the authors present a comprehensive performance analysis of tip-tilt compensation systems that use a natural star as a tilt reference, taking into account properties of the atmosphere and of the Galactic stellar populations, and optimizing over the system operating parameters to determine the fundamental limits to the long-exposure resolution. Their results show that for a ten meter telescope on Mauna Kea, if the image of the tilt reference star is uncorrected, about half the sky can be imaged in the V band with long-exposure resolution less than 60 milli-arc-seconds (mas), while if the image of the tilt reference star is fully corrected, about half the sky can be imaged in the V band with long-exposure resolution less than 16 mas. Furthermore, V band images long-exposure resolution of less than 16 mas may be obtained with a ten meter telescope on Mauna Kea for unresolved objects brighter than magnitude 22 that are fully corrected by a laser guide star adaptive optics system. This level of resolution represents about 70% of the diffraction limit of a ten meter telescope in the V band and is more than a factor of 45 better than the median seeing in the V band on Mauna Kea

Availability note (English)

MF available from INIS under the Report Number; OSTI as DE93016426; NTIS; INIS; US Govt. Printing Office Dep.

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Additional details

Additional titles

Subtitle (English)
Revision 2

Publishing Information

Imprint Pagination
52 p.
Report number
UCRL-JC--109219-Rev.2

Conference

Title
Laser guide star adaptive optics workshop.
Dates
10-12 Mar 1992.
Place
Albuquerque, NM (United States).

INIS

Country of Publication
United States
Country of Input or Organization
United States
INIS RN
24075588
Subject category
S46: INSTRUMENTATION RELATED TO NUCLEAR SCIENCE AND TECHNOLOGY;
Resource subtype / Literary indicator
Conference
Descriptors DEI
ACCURACY; CHROMATIC ABERRATIONS; CONTROL SYSTEMS; IMAGES; LASERS; NIGHT SKY; OPTICAL SYSTEMS; OPTICS; PERFORMANCE TESTING; SPATIAL RESOLUTION; STARS; TELESCOPES
Descriptors DEC
AMPLIFIERS; EQUIPMENT; RESOLUTION; TESTING

Optional Information

Contract/Grant/Project number
Contract W-7405-ENG-48
Funding organization
USDOE, Washington, DC (United States).
Secondary number(s)
CONF-9203139--5-Rev.2.