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Design of Stellar Interferometers II
Theo ten Brummelaar (Georgia State University)
Abstract:
This talk a follow on from the more theoretical talk given by W.J. Tango
and is concerned with the practical elements involved in the
construction of
an optical/IR Interferometer. Given the basic requirements for obtaining
and calibrating fringe visibilities and phases, I will attempt to show
how the engineering and system control challenges can be met, with a
emphasis on examples drawn from current working Interferometers. Since
the
scientific and instrumentation drivers are similar it is not
surprising to find that many of these devices look the same in many
ways. There are, of course, differences in many details, as different
design philosophies and scientific agendas are followed. This "cook's
tour" of existing Interferometers will, with luck, illustrate some of
these similarities and differences.
Besides any of the papers specifically concerned with individual
instruments,
I would recommend reading the review article by Tango and Twiss (1988),
as it contains an excellent summary of the basic requirement
specification of an optical Interferometer.
Viewgraphs PDF 2096k Bytes.
Viewgraphs PowerPoint 33480k Bytes.
A note on the use of Summer School material.
Suggested Reading:
- Michelson Stellar Interferometry
W.J. Tango and R.Q. Twiss
Progress in Optics 17, 239 (1980).
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Caltech 1999
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2001 | CfA 2002
Course Notes from the 2002 Michelson Interferometry Summer School
Smithsonian Astrophysical Observatory, Cambridge Massachusetts, June 24-28, 2002
Edited by P.R. Lawson (JPL), MS 301-451 Jet Propulsion Laboratory
Pasadena, California, 91109
Last Updated 9 February 2004
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