Paper
25 November 1985 Pupil And Image Plane Interferometry At Optical Wavelengths: Visibility And Phase Analysis.
Alain Chelli, Jean Marie Mariotti
Author Affiliations +
Abstract
Coherent arrays of telescopes, either ground or space based, are likely to become in the next decade a new class of powerful and wide-spread astronomical instruments. It has often been argued that at optical wavelengths these arrays are only able to measure the modulus of the source's spatial spectrum, and therefore are poorly suited for imaging. In this paper we show that phase reconstruction techniques developed for speckle interferometry can be applied to two telescopes Michelson interferometry. We make the comparison between image plane and pupil plane interferometry and compute a merit factor: for modulus determination, pupil plane is always preferable, while image plane is better for phase retrieval.
© (1985) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Alain Chelli and Jean Marie Mariotti "Pupil And Image Plane Interferometry At Optical Wavelengths: Visibility And Phase Analysis.", Proc. SPIE 0556, Intl Conf on Speckle, (25 November 1985); https://doi.org/10.1117/12.949555
Advertisement
Advertisement
RIGHTS & PERMISSIONS
Get copyright permission  Get copyright permission on Copyright Marketplace
KEYWORDS
Interferometry

Visibility

Signal to noise ratio

Speckle

Telescopes

Space telescopes

Atmospheric optics

RELATED CONTENT

Spatial Interferometry With The European VLT
Proceedings of SPIE (August 20 1986)
OHANA: representative science objectives
Proceedings of SPIE (February 21 2003)
Steps toward hypertelescopes on Earth and in space
Proceedings of SPIE (July 28 2008)
Recent progress on the infrared Michelson array
Proceedings of SPIE (August 01 1990)

Back to Top