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Nulling Interferometry
M.J. Creech-Eakman (Jet Propulsion Laboratory)
Abstract:
An overview of the techniques and current state of "nulling" interferometry are presented.
This will include an explanation for the motivation for nulling, along with a brief
comparison to other techniques. I will present a brief history of how the field developed
and where it stands today. Details of the theory of nulling, including some comparisons of
different types of nullers will be given. I will finish with some results from
laboratory nulls for the Keck Interferometer Nuller and published telescope-based nulls
and the implications of these results.
Viewgraphs PDF 1056k Bytes.
Suggested Reading:
- Principles of Long Baseline Stellar Interferometry, P. R. Lawson, ed.
Chapter 16, "Nulling Interferometry and Planet Detection" by E. Serabyn
(Jet Propulsion Laboratory: 1999).
- Achromatic
Interfero Coronagraphy: I. Theoretical capabilities for ground-based observations,
P. Baudoz, Y. Rabbia, J. Gay
Astron. Astrophys. Supp. Ser. 141, 319 (2000).
-
Achromatic interfero coronagraphy II. Effective performance on the sky (Abstract HTML)
P. Baudoz, Y. Rabbia, J. Gay, R. Burg, L. Petro, P. Bely, B. Fleury, P.-Y. Madec, F. Charbonnier
Astron. Astrophys. Suppl. Ser. 145, 341-350 (2000).
- Fully Symmetric Nulling Beam Combiners
Eugene Serabyn and M. Mark Colavita
Appl. Opt. 40, 1668-1671 (2001).
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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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