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Atmospheric optical communications systems
Proceedings of the IEEE, 1970The increasing sophistication of optical (and infrared) components and techniques, combined with rapidly expanding communication requirements, suggests that optical systems operating partly or entirely within the atmosphere may soon represent desirable solutions to real communications problems.
J.R. Kerr +3 more
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Optical investigations of atmospheric aerosol
Uspekhi Fizicheskih Nauk, 1968CONTENTS 1. Introduction 353 2. Certain Information on the Atmospheric Aerosol 355 3. Theory of Optical Properties of Aerosol 358 4. Optical Methods of Investigating the Atmosphere as Part of the General Problem of Indirect Measurements 362 5. Optical Properties of Aerosol and Microphysics of the Dispersed Phase 365 6.
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Fiber-optic atmospheric turbulence sensor
Optics Letters, 1995A novel dual-air-gap fiber-optic Mach - Zehnder interferometer is proposed for the direct measurement of the atmospheric optical turbulence structure constant C(n)(2). The shot-noise-limited minimum detectable structure constant is estimated to be 4.5 x 10(-20) m(-2/3), which is more than 2 orders of magnitude below a typical value of 10(-17) m(-2/3 ...
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Atmospheric Optical Communication System
IEEE Transactions on Communications, 1977The prototype atmospheric optical communication system has been developed, and various field tests have been carried out in Tokyo and Niigata. The system with a laser diode can transmit a 4-MHz color television signal or 120 telephone channels. This paper gives an outline description of system design based on field test results.
T. Kobayashi, K. Kohiyama, K. Nishino
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Journal of the Optical Society of America, 1941
By means of a telescopic photometer measurements were made in daylight of b, the brightness of a large approximately blackbody at a distance d=3.2 km, and of h, the brightness of the sky just above the blackbody. For visual ranges v from 3.2 to 15 km the measurements agreed with the theoretical relations v=(1/β) log 1/η and β=(1/d) log (1/(1−b/h ...
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By means of a telescopic photometer measurements were made in daylight of b, the brightness of a large approximately blackbody at a distance d=3.2 km, and of h, the brightness of the sky just above the blackbody. For visual ranges v from 3.2 to 15 km the measurements agreed with the theoretical relations v=(1/β) log 1/η and β=(1/d) log (1/(1−b/h ...
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Singular Atmospheric Optics: From Wavefront Dislocations to Synthesis of Vortex Laser Beams
, 2020V. Aksenov, V. Dudorov, V. Kolosov
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