Finite Exposure Time, Astronomical Speckle Transfer Function
作者:
Richard Barakat,
Peter Nisenson,
期刊:
Optica Acta: International Journal of Optics
(Taylor Available online 1983)
卷期:
Volume 30,
issue 10
页码: 1405-1416
ISSN:0030-3909
年代: 1983
DOI:10.1080/713821066
出版商: Taylor & Francis Group
数据来源: Taylor
摘要:
The effects of finite exposure time (used to record astronomical speckle data) on the speckle transfer function are shown to be highly dependent on the details of the atmospheric turbulence in the optical path as well as on the deterministic wavefront aberrations of the optical system. Both Taylor turbulence, where a frozen layer or layers are convected across the aperture, and Mintzer turbulence, where the turbulence is boiling and stationary, are taken into account. Computations have been made for some typical cases of the time integrated speckle transfer function for various combinations of Taylor and Mintzer turbulence with focused and defocused optical systems.
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