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Proceedings Paper

Near Infrared (1To5 µm) Multichannel Speckle Interferameter
Author(s): M J Selby; K Jason; D Xin; C Sanchez
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Paper Abstract

Speckle interferometry was first introduced by Labeyrie (1970) in the visible as a method of restoring diffraction-limited information from large telescopes despite the presence of a turbulent atmosphere. It has been extensively used in the visible to resolve small sources and measure binary separations (Bonneau and Foy, 1980; McAllister and Hendry, 1982; Beddoes et al, 1976; Morgan et al, 1978).

Paper Details

Date Published: 9 January 1984
PDF: 7 pages
Proc. SPIE 0445, Instrumentation in Astronomy V, (9 January 1984); doi: 10.1117/12.966132
Show Author Affiliations
M J Selby, Imperial College (United Kingdom)
K Jason, Imperial College (United Kingdom)
D Xin, North China Institute of Electro-optics (China)
C Sanchez, Universidad de la Laguna (United Kingdom)


Published in SPIE Proceedings Vol. 0445:
Instrumentation in Astronomy V
Alec Boksenberg; David L. Crawford, Editor(s)

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