Distribution of light intensity fluctuations behind a telescope lens in the case of reflection in a turbulent atmosphere

Computer Science

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

Atmospheric Turbulence, Fluctuation Theory, Luminous Intensity, Telescopes, Atmospheric Attenuation, Correlation Coefficients, Lenses, Light Beams, Reflected Waves

Scientific paper

Th dispersion and spatial correlation coefficient of the intensity of light reflected in a turbulent atmosphere are analyzed as a function of the observation-plane position with respect to the entrance pupil of the receiving telescope lens. It is shown that the amplification or attenuation of the intensity fluctuations in the lens image plane as compared with the lens plane is localized in a region limited in the longitudinal direction. These effects and the size of the localization plane depend on the receiving-system parameters and the initial coherence of the source field.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Distribution of light intensity fluctuations behind a telescope lens in the case of reflection in a turbulent atmosphere does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Distribution of light intensity fluctuations behind a telescope lens in the case of reflection in a turbulent atmosphere, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Distribution of light intensity fluctuations behind a telescope lens in the case of reflection in a turbulent atmosphere will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-1548723

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.