Abstract
Possibilities of the correction of the general wavefront tilt using a signal from a laser guide star (LGS) are analyzed. The quality of an image of an extraterrestrial object formed by an astronomic optical system through a turbulent atmosphere is analyzed. The efficiency of the adaptive correction of distortions for different LGS schemes is analyzed. Calculations are performed for different models of the vertical dependence of the structural parameter of the refractive index of the turbulent atmosphere.
Similar content being viewed by others
References
V. P. Linnik, “About Principal Possibilities to Overcome the Impact of Atmosphere on Star Image,” Opt. Spek–trosk. 3, 401–402(1957).
R. Fugate, “Laser Beacon Adaptive Optics,” Opt. Photon. News 4 (6), 14–19 (1993).
R. Ragazzoni, “Absolute Tip–tilt Determination With Laser Beacons,” Astron. Astrophys. 305, L13–L16 (1996).
V. I. Tatarskii, Wave Propagation in a Turbulent Atmosphere (Nauka, Moscow, 1961) [in Russian].
V. M. Orlov, I. V. Samokhvalov, G. G. Matvienko, M. L. Belov, and A. N. Kozhemyakov, Elements of Light Scattering Theory and Optical Location (Nauka, Novosibirsk, 1982) [in Russian].
V. I. Tatarskii and A. Ishimaru, Digest of ‘scintillation’ Meeting for Wave Propagation in Random Media (Univ. of Washington, Seattle, USA, 1992).
M. A. Kalistratova and A. I. Kon, “Fluctuations of Arrival Angle of Light Waves From Extended Source in Turbulent Atmosphere,” Izv. Vyssh. Uchebn. Zaved., Ser. Radiofiz. 9, 1100–1107 (1966).
V. P. Lukin, “Tracking of Random Angular Shifts of Optical Beams,” in Proc. of the 5th All—Union Symp. on Propagation of Laser Emission in Atmosphere (Tomsk, 1979), Part 2, Pp. 33–36.
V. I. Klyatskin, Statistical Description of Dynamic Systems With Fluctuating Parameters (Nauka, Moscow, 1975) [in Russian].
V. L. Mironov, V. V. Nosov, and B. N. Chen, “Correlation of the Shifts of Optical Images of Laser Sources in a Turbulent Atmosphere,” Izv. Vyssh. Uchebn. Zaved., Ser. Radiofiz. 25, 1467–1471 (1982).
V. P. Lukin, “Efficiency of the Compensation of Phase Distortions of Optical Waves,” Kvant. Elektron. 7, 923–927 (1978) [Sov. J. Quant. Electron. 7, 522 (1977)].
V. P. Lukin, “Correction of Random Angular Displacements of Optical Beams,” Kvant. Elektron. 10, 1270–1279 (1980) [Sov. J. Quant. Electron. 10, 727 (1980)].
V. P. Lukin and M. I. Charnotskii, “Reciprocity Principle and Adaptive Control of Optical Radiation Parameters,” Kvant. Elektron. 12, 952–958 (1982) [Sov. J. Quant. Electron. 12, 602 (1982)].
V. P. Lukin and O. N. Emaleev, “Correction of Angular Displacements of Optical Beams,” Kvant. Elektron. 12, 2465–2473 (1982) [Sov. J. Quant. Electron. 12, 1470 (1982)].
V. P. Lukin and V. F. Matyukhin, “Adaptive Correction of Images,” Kvant. Elektron. 13, 2465–2473 (1983) [Sov. J. Quant. Electron. 13, 1604 (1983)].
V. P. Lukin, Atmispharin Adaptiva Iptins (Nauka, Novosibirsk, 1986; SPIA Ipt. Ang. Prass, 1996), Eng. Vol. I23.
V. P. Lukin, “Limiting Resolution of Adaptive Telescope With the Use of Artificial Star,” in Proc. of the ICO–16 on Active and Adaptive Optics (1993), pp. 521–524.
V. P. Lukin and B. V. Fortes, “Efficiency of Adaptive Correction of Images in a Telescope Using an Artificial Guide Star,” OSATechn. Digest. 23, 192–194 (1995).
V. P. Lukin, “Laser Beacon and Full Aperture Tilt Measurements,” Adapt. Opt. Techn. Digest Ser. 13, 35-1–35-5 (1996).
V. P. Lukin, “Adaptive Formation of Beams and Images in Turbulent Atmosphere,” Opt. Atmosf. Okeana 8, 301–341 (1995).
V. P. Lukin and B. V. Fortes, “Comparison of Limit Efficiencies for Various Schemes of Laser Reference Star Formation,” Opt. Atmosf. Okeana 10 (1), 34–41 (1997)
R. Ragazzoni, S. Esposito, and E. Marchetti, “Auxiliary Telescopes for the Absolute Tip–tilt Determination of a Laser Guide Star,” Mon. Not. R. Astron. Soc. 276, L76–L78 (1995).
M. S. Belen’kii, “Full Aperture Tilt Measurement Technique With a Laser Guide Star,” Proc. SPIE 2471, 289–296 (1995).
V. P. Lukin, “Mono and Bistatic Schemes and Optimal Algorithm for Tilt Correction in Ground–Based Adaptive Telescopes,” Appl. Opt. 37, 4561–4568 (1998).
A. S. Gurvich, A. I. Kon, V. L. Mironov, and S.S. Khmelevtsov, Laser Emission in Atmosphere (Nauka, Moscow, 1976) [in Russian].
D. F. Buscher, G. Love, and R. Myers, “Laser Beacon Wave–Front Sensing without Focal Anisoplanatism,” Opt. Lett. 27, 149–151 (2002).
D. Bonaccini and V. Lukin, “Laser Guide Star with Collimated Laser Beam for Large Aperture Telescope,” in Proc. of Frontiers in Optics, 2006 (Rochester, USA, 2006), p. 129.
L. Bolbasova, A. Goncharov, and V. Lukin, “Field–Oriented Wavefront Sensor for Laser Guide Stars, ” in Proc. of the 6th Int. Workshop for Industry and Medicine (Gal–way, Ireland, 2007), pp. 174–175.
L. A. Bol’basova and V. P. Lukin, “Laser Guide Star and Models of Atmospheric Turbulence,” Opt. Atmosf. Okeana 20, 1096–1104(2007).
R. R. Parenti and R. J. Sasiela, “Laser–guide–star Systems for Astronomical Applications,” J. Opt. Soc. Am. A11, 288–309(1994).
Author information
Authors and Affiliations
Additional information
Original Russian Text © L.A. Bol’basova, V.P. Lukin, 2010, published in Optica Atmosfery i Okeana.
Rights and permissions
About this article
Cite this article
Bol’basova, L.A., Lukin, V.P. Investigation of the efficiency of the application of laser guide stars. Atmos Ocean Opt 23, 65–72 (2010). https://doi.org/10.1134/S1024856010010136
Received:
Published:
Issue Date:
DOI: https://doi.org/10.1134/S1024856010010136