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Determination of atmospheric structure function by using a single coherent detector.
Applied Optics
|February 4, 2010
Summary
This study presents a novel method for measuring the wave structure function, crucial for atmospheric turbulence research and telescope design. The technique utilizes an existing optical receiver, simplifying the characterization of optical wave distortions.
Area of Science:
- Optics and Photonics
- Atmospheric Science
- Astronomy Instrumentation
Background:
- Atmospheric turbulence significantly impacts optical wave propagation, affecting the performance of telescopes and coherent optical receivers.
- Accurate measurement of the wave structure function is essential for mitigating these turbulence-induced distortions and improving system design.
Purpose of the Study:
- To describe a practical method for measuring the wave structure function using an existing optical receiver.
- To establish a relationship between the receiver's output and the wave structure function under specific conditions.
Main Methods:
- Modifying an existing optical receiver's telescope aperture with a screen containing two small holes.
- Analyzing the amplitude modulation (A.M.) output of the receiver.
Main Results:
- A simple relationship was derived between the receiver's A.M. output and the wave structure function.
- This relationship holds true when the incident optical beam follows Gaussian statistics.
Conclusions:
- The developed method offers a feasible approach to measure the wave structure function with readily available equipment.
- This technique can aid in the effective design and calibration of telescopes for applications sensitive to atmospheric turbulence.


