Abstract
The laser guide star (hereinafter referred as LGS) is created by a physical process in the Earth atmosphere. Consequently it is located at a finite distance from the observer, which results in the so-called cone effect, or focus anisoplanatism. The volume of the atmosphere from the LGS to the telescope mirror is a cone, whereas it is a cylinder from any astrophysical source because it is located almost at infinity. This difference causes errors in the measurement of the phase disturbances of the incoming wavefronts [1].
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References
Foy, R. and Labeyrie, A. Astron. Astrophys. 152, L29–32 (1985).
Vernin, J. and Muünoz-Tunön, C. Astron. Astrophys. 284, 311–318 (1994).
Talion, M., Foy, R., and Vernin, J. In Laser guide star adaptive optics workshop, Fugate, R. Q., editor, 555–566 (SOR/Phillips Lab., Albuquerque (NM), 1992).
Fried, D. and Belsher, J. J. Opt. Soc. Am. A 11, 277 (1994).
Talion, M. private communication, (1997).
Le Louarn, M. private communication, (1997).
Zollars, B. Lincoln Lab. J. 5, 67 (1992).
Fried, D. J. Opt. Soc. Am. A 12, 939 (1995).
Sasiela, R. J. J. Opt. Soc. Am. A 11, 379–393 (1994).
Talion, M. and Foy, R. Astron. Astrophys. 235, 549–557 (1990).
Beckers, J. M. In Very Large Telescopes and their instrumentation, M.-H., U., editor, number 30 in ESO conferences, 693–703 (ESO, Garching, Germany, 1988).
Johnston, D. C. and Welsh, B. M. J. Opt. Soc. Am. A 11, 394–408 (1994).
Ellerbroek, B. L. J. Opt. Soc. Am. A 11, 783–805 (1994).
Vernin, J. and Azouit, M. J. Optics (Paris) 14, 131–142 (1983).
Bufton, J. L., Minott, P., Fitzmaurice, M., and Titterton, P. J. Opt. Soc. Am. 62, 1068 (1972).
Roddier, F. Progress in Optics XXI, 281–376 (1981).
T. Young, A. J. Opt. Soc. Am. 60, 248–250 (1970).
Talion, M., Foy, R., and Vernin, J. In Progress in telescope and instrumentation technologies, M.-H., U., editor, number 42 in ESO conferences, 517–521 (ESO, Garching, Germany, 1992).
Ragazzoni, R., Marchetti, E., and Rigaut, F. Astron. Astrophys. 342, L3-L56 (1999).
Cannon, R. C. J. Opt. Soc. Am. A (1995).
Jankevics, A. and Wirth, A. SPIE 1543, 438–448 (1991).
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Foy, R. (2000). The Cone Effect. In: Ageorges, N., Dainty, C. (eds) Laser Guide Star Adaptive Optics for Astronomy. NATO ASI Series, vol 551. Springer, Dordrecht. https://doi.org/10.1007/978-94-015-9624-4_6
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DOI: https://doi.org/10.1007/978-94-015-9624-4_6
Publisher Name: Springer, Dordrecht
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