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8 - Transmitting and Receiving Optics

Published online by Cambridge University Press:  24 February 2022

Chiao-Yao She
Affiliation:
Colorado State University
Jonathan S. Friedman
Affiliation:
Universidad Ana G. Mendez
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Summary

In Chapter 8, we give an overview of the optics that control beam transmission and signal reception. We open with a description of the use and benefits of a beam expander to control the output beam divergence. From there, we move to describing receiver optics, starting with the telescope and importance of size, field of view, and using high-quality optics. This includes using an optical fiber to transport the received photons to the downstream filtering and detection optics. Next, we discuss detector characteristics and the trade-offs one must consider when selecting an appropriate photon counting sensor. We follow with a short section on the value of computer modeling the receiver optics. We close the chapter with a concise discussion of atmospheric turbulence and of laser guide stars and adaptive optics for the mitigation of atmospheric turbulence effects on astronomical telescopes.

Type
Chapter
Information
Atmospheric Lidar Fundamentals
Laser Light Scattering from Atoms and Linear Molecules
, pp. 244 - 267
Publisher: Cambridge University Press
Print publication year: 2022

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References

Siegman, A. E. (1997). How to (Maybe) Measure Laser Beam Quality. Tutorial presentation at the Optical Society of America Annual Meeting, Long Beach, CA, October 1997. Accessed at https://en.wikipedia.org/wiki/Beam_parameter_product.Google Scholar
Kogelnik, H. and Li, T. (1966). Laser beams and resonators. Applied Optics, 5(10), 15501567, doi: https://doi.org/10.1364/AO.5.001550.Google Scholar
She, C. Y., Latifi, H., Yu, J. R. et al. (1990). Two-frequency lidar technique for mesospheric Na temperature measurements. Geophys. Res. Lett., 17(7), 929932.Google Scholar
Mahajan, V. N. (1982). Strehl ratio for primary aberrations: some analytical results for circular and annular pupils. J. Opt. Soc. Am., 72(9), 12581266.Google Scholar
Donovan, D. P., Whiteway, J. A., and Carswell, A. I.. (1993). Correction of nonlinear photon-counting effects in lidar systems. Appl. Opt., 32(33), 67426753.Google Scholar
Smith, J. A. and Chu, X.. (2015). High-efficiency receiver architecture for resonance-fluorescence and Doppler lidars. Appl. Opt., 54(11), 31373184. doi: https://doi.org/10.1364/AO.54.003173.Google Scholar
Liu, A. and Guo, Y.. (2016). Photomultiplier tube calibration based on Na lidar observation and its effect on heat flux bias. Appl. Opt., 55(33), 94679475. doi: https://doi.org/10.1364/AO.55.009467.Google Scholar
Boyd, R. (1978). The wavelength dependence of seeing. J. Opt. Soc. Am., 68(7), 877883.Google Scholar
Fried, D. (1966). Optical resolution through a randomly inhomogeneous medium for very long and very short exposures. J. Opt. Soc. Am., 56(10), 13721379.Google Scholar
Hickson, P. (2014). Atmospheric and adaptive optics. Astron. Astrophys. Rev., 22(1), 76. doi: https://doi.org/10.1007/s00159-014-0076-9.Google Scholar
Roddier, F. (1981). The effect of atmospheric turbulence in optical astronomy. Prog. Opt., XIX, 281376. doi: https://doi.org/10.1016/S0079-6638(08)70204-X.Google Scholar
Max, C. (2001). Introduction to adaptive optics and its history. The 197th Annual Meeting of the American Astronomical Society, jointly with the American Association of Physics Teachers, 7–11 January 2001, San Diego, California. Accessed at www.researchgate.net/publication/228761974.Google Scholar
Wright, J. (2015). A brief history of laser adaptive optics. Posted in AstroWright under science, Uncategorized and tagged science on January 17, 2015. Accessed at https://sites.psu.edu/astrowright/2015/01/17.Google Scholar
Babcock, H. (1953). The possibility of compensating astronomical seeing. Publ. Astron. Soc. Pac., 65(386), 229–23.CrossRefGoogle Scholar
Dyson, F. (1975). Photon noise and atmospheric noise in active optical systems. J. Opt. Soc. Am., 65(5), 551558.Google Scholar
Foy, R., and Labeyrie, A. (1985). Feasibility of adaptive telescope with laser probe. Astron. Astrophys., 152(2), L29L31.Google Scholar
Thompson, L., and Gardner, C. (1987). Experiments on laser guide stars at Mauna Kea Observatory for adaptive imaging in astronomy. Nature 328(6127), 229231.Google Scholar
Fugate, R. (1994). Two generations of laser-guide-star adaptive-optics experiments at the Starfire Optical Range. J. Opt. Soc. Am. A, 11(1), 310324.Google Scholar

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