Share Email Print

Proceedings Paper

Achromatic prism-based phaseshifter for nulling in the visible
Author(s): H. J. P. Vink; Henk Bokhove; Bas R. Ouwerkerk; J. Pieter Kappelhof; Hedser H. van Brug; Bart Snijders; L. L. A. Vosteen
Format Member Price Non-Member Price
PDF $14.40 $18.00
cover GOOD NEWS! Your organization subscribes to the SPIE Digital Library. You may be able to download this paper for free. Check Access

Paper Abstract

Nulling interferometry is a direct method to detect earth-like planets. To determine whether a planet is earth-like spectrometry is performed on a broadband infra-red (l = 4-20 mm) input signal from the planet. The star signal in this region is roughly 106 times stronger than the planet signal. Nulling interferometry should decrease the broadband star signal by about this factor of 106. This can be performed using an achromatic phaseshifter based on dispersive elements. The design of a complete breadboard under an ESA contract including a prism based (eight prisms in total) dispersive achromatic phaseshifter is presented including error budget and implied tolerances on the mechanical components. Measurements with this breadboard resulted in nulling depths of 3.5.105 for polarized laser light and just below 103 for polarized visible broadband light in the wavelength range of 530-750nm.

Paper Details

Date Published: 26 February 2003
PDF: 6 pages
Proc. SPIE 4852, Interferometry in Space, (26 February 2003); doi: 10.1117/12.460741
Show Author Affiliations
H. J. P. Vink, TNO TPD (Netherlands)
Henk Bokhove, TNO TPD (Netherlands)
Bas R. Ouwerkerk, TNO TPD (Netherlands)
J. Pieter Kappelhof, TNO TPD (Netherlands)
Hedser H. van Brug, TNO TPD (Netherlands)
Bart Snijders, TNO TPD (Netherlands)
L. L. A. Vosteen, TNO TPD (Netherlands)

Published in SPIE Proceedings Vol. 4852:
Interferometry in Space
Michael Shao, Editor(s)

© SPIE. Terms of Use
Back to Top