Abstract
ATMOSPHERIC turbulence limits the resolution of a ground-based astronomical telescope to much worse than the diffraction limit of the instrument. An adaptive-optics system, in which some part of the optical train of the telescope can be adjusted in real time, can compensate for atmospheric turbulence, but a beacon or guide-star is needed to allow measurement of the atmospheric optical distortion. It has been suggested1 that the measurement could be achieved by means of a synthetic beacon (also called an artificial beacon, and sometimes a laser guide-star) formed by atmospheric backscatter from a ground-based laser. We have performed an experiment to demonstrate atmospheric compensation using a synthetic beacon. With a pulsed dye laser to generate the beacon and a 241-channel adaptive-optics system to perform the phase correction, we obtained almost diffraction-limited resolution of star images in the visible part of the spectrum. Our results indicate that there are no technical barriers to atmospheric compensation using synthetic beacons at ground-based observatories.
This is a preview of subscription content, access via your institution
Access options
Subscribe to this journal
Receive 51 print issues and online access
$199.00 per year
only $3.90 per issue
Buy this article
- Purchase on Springer Link
- Instant access to full article PDF
Prices may be subject to local taxes which are calculated during checkout
Similar content being viewed by others
References
Foy, R. & Labeyrie, A. Astr. Astrophys. 152, L29–31 (1985).
Hardy, J. W., Lefebvre, J. E. & Koliopoulos, C. L. J. opt. Soc. Am. 67, 360–369 (1977).
Everett, P. N. Proc. Int. Conf. Lasers. 1988 (ed. Duarte, F. J.) 404–409 (STS, McLean. Virginia, 1989).
Twichell, J. C. et al. Rev. scient. Instrum. 61, 2744–2746 (1990).
Sasiela, R. J. & Mooney, J. G. Proc. SPIE 551, 170–176 (1985).
Humphreys, R. A., Primmerman, C. A., Bradley, L. C. & Herrmann, J. Opt. Lett. 16 (1991).
Jeys, T. H., Brailove, A. A. & Mooradian, A. Appl. Opt. 28, 2588–2591 (1989).
Author information
Authors and Affiliations
Rights and permissions
About this article
Cite this article
Primmerman, C., Murphy, D., Page, D. et al. Compensation of atmospheric optical distortion using a synthetic beacon. Nature 353, 141–143 (1991). https://doi.org/10.1038/353141a0
Received:
Accepted:
Issue Date:
DOI: https://doi.org/10.1038/353141a0
This article is cited by
-
Astrophotonics: astronomy and modern optics
The Astronomy and Astrophysics Review (2021)
-
Performance analysis of 349-element adaptive optics unit for a coherent free space optical communication system
Scientific Reports (2019)
-
Inversion-free image recovery from strong aberration using a minimally sampled transmission matrix
Scientific Reports (2019)
-
Investigation of return photons from sodium laser beacon excited by a 40-watt facility-class pulsed laser for adaptive optical telescope applications
Scientific Reports (2018)
-
Time-reversed ultrasonically encoded optical focusing into scattering media
Nature Photonics (2011)
Comments
By submitting a comment you agree to abide by our Terms and Community Guidelines. If you find something abusive or that does not comply with our terms or guidelines please flag it as inappropriate.