1989
DOI: 10.1364/ao.28.003918
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Optical spatial tracking using coherent detection in the pupil plane

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Cited by 6 publications
(3 citation statements)
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“…The intermediate frequency (IF) signal, in the absence of nutation, at the balanced detector output can be written as _________________ sjp(t) = tJ2PIFrIhet(tI)z, t,1y) SiiL(WIFt + 9) + n(t), (3) where PIF S the ideal IF signal power when i(1i, t) = 1, WIF = w -wL is the IF frequency, and 9 = 9 -9L represents the random modulation and phase. Noise at the balanced detector output, n(t), is modelled as a narrowband Gaussian random process with two sided power spectral density of .…”
Section: Mathematical Modelmentioning
confidence: 99%
See 1 more Smart Citation
“…The intermediate frequency (IF) signal, in the absence of nutation, at the balanced detector output can be written as _________________ sjp(t) = tJ2PIFrIhet(tI)z, t,1y) SiiL(WIFt + 9) + n(t), (3) where PIF S the ideal IF signal power when i(1i, t) = 1, WIF = w -wL is the IF frequency, and 9 = 9 -9L represents the random modulation and phase. Noise at the balanced detector output, n(t), is modelled as a narrowband Gaussian random process with two sided power spectral density of .…”
Section: Mathematical Modelmentioning
confidence: 99%
“…Spatial tracking systems have been investigated by several authors. [2][3][4][5][6][7][8]. Most of the studies were carried for either tracking point source using a quadrant type detector or extended source tracking using array detector.…”
Section: Introductionmentioning
confidence: 99%
“…Another advantage of an array is that an array of N small telescopes will have volume 14-N the volume of a single large telescope with the same F-number and total aperture size. The array may be constructed with separate telescopes or it may be formed by placing a detector array in the pupil plane of a larger telescope [1]. Previously such an array was constructed using a Bragg cell as a phase shifter for each channel [2].…”
Section: Introductionmentioning
confidence: 99%