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Source: The Open Library
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1Infrared speckle interferometry with 2-D arrays
By P. M. Harvey
“Infrared speckle interferometry with 2-D arrays” Metadata:
- Title: ➤ Infrared speckle interferometry with 2-D arrays
- Author: P. M. Harvey
- Language: English
- Publisher: ➤ National Aeronautics and Space Administration - National Technical Information Service, distributor
- Publish Date: 1994
- Publish Location: ➤ [Washington, DC - Springfield, Va
“Infrared speckle interferometry with 2-D arrays” Subjects and Themes:
- Subjects: Speckle interferometry - Infrared interferometers - Infrared detectors - Speckle patterns - Noise reduction
Edition Identifiers:
- The Open Library ID: OL15507944M
Access and General Info:
- First Year Published: 1994
- Is Full Text Available: No
- Is The Book Public: No
- Access Status: No_ebook
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Source: Wikipedia
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Speckle imaging
divided into the shift-and-add ("image stacking") method and the speckle interferometry methods. These techniques can dramatically increase the resolution
Electronic speckle pattern interferometry
Electronic speckle pattern interferometry (ESPI), also known as TV holography, is a technique that uses laser light, together with video detection, recording
Interferometry
pattern interferometry in 1970, and since then, speckle has been exploited in a variety of other applications. A photograph is made of the speckle pattern
Speckle (interference)
Speckle, speckle pattern, or speckle noise designates the granular structure observed in coherent light, resulting from random interference. Speckle patterns
Betelgeuse
(1978). "Speckle Interferometry". New Scientist. Vol. 78. pp. 238–40. Bibcode:1978NewSc..78..238W. Roddier, F. (1999). "Ground-based interferometry with adaptive
Aperture masking interferometry
Aperture masking interferometry (or Sparse aperture masking) is a form of speckle interferometry, that allows diffraction limited imaging from ground-based
R136a1
100 times fainter than the cluster and can only be resolved using speckle interferometry. In 1960, a group of astronomers working at the Radcliffe Observatory
532 Herculina
determination of its shape and rotation somewhat difficult. A set of 1982 speckle interferometry observations led to a simple preliminary model of Herculina as a
Holography
001593. Jones, Robert; Wykes, Catherine (1989). Holographic and Speckle Interferometry. Cambridge: Cambridge University Press. ISBN 0-521-34417-4. Beigzadeh
Iota Orionis
Orionis A, B and C. Iota Orionis A has also been resolved using speckle interferometry and is also a massive spectroscopic binary, with components Iota