Back to Search
Start Over
Tip-tilt compensation - Resolution limits for ground-based telescopes using laser guide star adaptive optics
- Source :
- The Astrophysical Journal. 407:428
- Publication Year :
- 1993
- Publisher :
- American Astronomical Society, 1993.
-
Abstract
- 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 Vmore » 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.« less
- Subjects :
- Physics
business.industry
media_common.quotation_subject
Astrophysics::Instrumentation and Methods for Astrophysics
Astronomy
Astronomy and Astrophysics
Astrophysics::Cosmology and Extragalactic Astrophysics
law.invention
Telescope
Laser guide star
Tilt (optics)
Optics
Space and Planetary Science
law
Sky
Astrophysics::Solar and Stellar Astrophysics
Angular resolution
Astrophysics::Earth and Planetary Astrophysics
Adaptive optics
business
Image resolution
Astrophysics::Galaxy Astrophysics
V band
media_common
Subjects
Details
- ISSN :
- 15384357 and 0004637X
- Volume :
- 407
- Database :
- OpenAIRE
- Journal :
- The Astrophysical Journal
- Accession number :
- edsair.doi...........1c42f46b036d95ffee46c0896366b931
- Full Text :
- https://doi.org/10.1086/172525