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Irradiance Statistics, Modulation Transfer Function, and Phase Structure Function of an Optical Wave in a Turbulent Medium

Irradiance Statistics, Modulation Transfer Function, and Phase Structure Function of an Optical Wave in a Turbulent Medium
Author: Harold T. Yura
Publisher:
Total Pages: 19
Release: 1969
Genre: Atmospheric turbulence
ISBN:

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An analysis of experimentally observed far-field irradiance statistics, suggesting an approach to calculating the probability distribution for intensity fluctuations of an optical wave in a turbulent medium and expressions for measuring important wave characteristics. Two theoretical treatments of probability distribution are investigated. Because none of the proposed theories can account for irradiance statistics in a consistent manner, it is suggested that a modified geometric optics approach would lead to an improved quantitative understanding of the phenomena. Expressions are derived for measuring wave phase structure function and modulation transfer function. Results are useful in determining the limited resolution obtainable in forming an image through a turbulent medium, as well as in calculating the signal-to-noise ratio of an optical heterodyne detection system. (Author).


The Modulation Transfer Function and Phase Structure Function of an Optical Wave in a Turbulent Medium

The Modulation Transfer Function and Phase Structure Function of an Optical Wave in a Turbulent Medium
Author: R. F. Lutomirski
Publisher:
Total Pages: 11
Release: 1969
Genre: Optical transfer function
ISBN:

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Expressions are derived for the dependence of the modulation transfer function (MTF) and the phase structure function (D sub phi) on the Kolmogorov turbulence parameters. In particular, it is demonstrated that certain measurements of the MTF and D sub phi can be interpreted in terms of an outer scale of turbulence being of the order 10-50 cm, values which typically can be expected under inversion conditions. (Author).


Scientific and Technical Aerospace Reports

Scientific and Technical Aerospace Reports
Author:
Publisher:
Total Pages: 380
Release: 1995
Genre: Aeronautics
ISBN:

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Lists citations with abstracts for aerospace related reports obtained from world wide sources and announces documents that have recently been entered into the NASA Scientific and Technical Information Database.


Modulation Transfer Function in Optical and Electro-optical Systems

Modulation Transfer Function in Optical and Electro-optical Systems
Author: Glenn D. Boreman
Publisher: SPIE Press
Total Pages: 124
Release: 2001
Genre: Science
ISBN: 9780819441430

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This tutorial introduces the theory and applications of MTF, used to specify the image quality achieved by an imaging system. It covers basic linear systems theory and the relationship between impulse response, resolution, MTF, OTF, PTF, and CTF. Practical measurement and testing issues are discussed.


Mean and Variance of the Irradiance for a Phase-compensated Optical Link in Turbulence

Mean and Variance of the Irradiance for a Phase-compensated Optical Link in Turbulence
Author: Ronald Louis Fante
Publisher:
Total Pages: 32
Release: 1975
Genre: Atmospheric turbulence
ISBN:

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In the last several years considerable progress has been made toward the development of adaptive systems which can compensate for the deleterious effect of atmospheric turbulence on air/air and air/ground optical communications links. One promising method is reciprocity tracking in which a beacon located on the receiver is used in real time to adjust the wavefront of the transmitter. A beacon signal is emitted at x and the phase distribution of this signal is sensed in the plane x = 0. The phase of the transmitter field is then continuously adjusted so that it is the negative of the received beacon phase distribution. because of atmospheric reciprocity, this then continuously compensates for the phase fluctuations induced on the transmitted field by the turbulent medium between the transmitter and receiver.


An Investigation of Atmospheric Turbulence by Stellar Observations

An Investigation of Atmospheric Turbulence by Stellar Observations
Author: Jack Lytle Bufton
Publisher:
Total Pages: 188
Release: 1971
Genre: Astrophysics
ISBN:

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This study of the optical effects of atmospheric turbulence concentrates on the stellar observation problem. When an infinite plane wave from an incoherent stellar source is sampled by an earth-based telescope, the resultant stellar image exhibits random fluctuations in intensity, position, and size due to turbulence-induced scattering in the intervening atmosphere. One familiar aspect of this problem is the scintillation of starlight apparent to the naked eye. The central aim is to express optical statistics in terms of refractive-index structure constant which pertains to strength of turbulence along the optical path. Data is presented on stellar and meteorological observations made between fall 1968 and spring 1969 with a 0.152-meter diameter refracting telescope. Data was recorded simultaneously on the three parameters of image intensity, motion, and size. The data is interpreted in terms of the theory and used to estimate strength of turbulence. The central result is a series of profiles for refractive-index structure constant along the vertical path. These are constructed using stellar data to calculate parameters of a model.


Irradiance Statistics of an Optical Wave in a Turbulent Medium

Irradiance Statistics of an Optical Wave in a Turbulent Medium
Author: R. F. Lutomirski
Publisher:
Total Pages: 7
Release: 1969
Genre: Atmospheric turbulence
ISBN:

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The probability distribution for the intensity fluctuations of an optical wave has received considerable attention in the recent literature. Tatarski has claimed the distribution in I in the far field (where geometric optics is not applicable) to be log-normal (i.e., lnI is normal) by applying the central limit theorem to the first order Rytov solution. It has recently been shown that it is necessary to retain the second order Rytov term in order to compute the standard deviation of the intensity fluctuations correct to first order in n1. Hence, Tatarski's derivation of a log-normal distribution function for propagation paths dominated by single scattering cannot be valid. In fact, it can easily be seen that the only first order function (proportional to n1, the index of refraction fluctuations), which gives the correct mean and standard deviation for the intensity, is a linear one. Hence, the correct first order statistics are given only by the first order Born approximation, and application of the central limit theorem then yields a normally distributed intensity distribution. This result should be valid for propagation paths small compared to the single scattering length, Lc, but the experimental evidence supports a log-normal rather than a normal distribution. (Author).