Hostname: page-component-7bb8b95d7b-2h6rp Total loading time: 0 Render date: 2024-09-23T06:10:54.031Z Has data issue: false hasContentIssue false
  • English
  • Français

Differential Diffraction in Michelson Stellar Interferometry

Published online by Cambridge University Press:  19 July 2016

M. Hrynevych
M. Hrynevych*
Affiliation:
Chatterton Astronomy Dept University of Sydney, NSW, 2006 Australia

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

Diffraction in Michelson Stellar Interferometery, with particular reference to SUSI, is examined. A justification of the use of Fresnel diffraction is made, both theoretically and experimentally, and a calculation of fringe visibility loss for SUSI is given.

Keywords

DiffractionSUSIFringe visibility
Type
Imaging Theory
Information
Symposium - International Astronomical Union , Volume 158: Very High Angular Resolution Imaging , 1994 , pp. 224 - 226
Copyright
Copyright © Kluwer 1994 

References

Bagnuolo, W.G.: 1988, in Simulations for the CHARA/GSU Interferometer and Binary Star Speckle Photometry, ed(s)., Frieden, B.R., NOAO-ESO Conference on High Resolution Imaging by Interferometry, Springer-Verlag:Munchen, 981–994 Google Scholar
Hrynevych, M.: 1992, Diffraction Effects in Michelson Stellar Interferometry, , Chatterton Astronomy Department, University of Sydney:Sydney Google Scholar
Mekarnia, D. and Gay, J.: 1989, ‘Alteration du Visibilite par Diffraction de Fresnel en Synthese D'Ouverture’, J. Optics 20, 131–140 Google Scholar
Tango, W.J. and Twiss, R.Q.: 1974, ‘Diffraction Effects in Long Path Interferometers’, Appl. Opt. 13, 1814–1819 Google Scholar