Share Email Print
cover

Proceedings Paper

Sum frequency generation process for a new astronomical instrument
Author(s): R. Baudoin; J. T. Gomes; L. Delage; L. Grossard; T. A. Ten Brummelar; N. J. Scott; J. Sturmann; F. Reynaud
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

We propose an exotic use of sum frequency generation process (SFG) to develop a new kind of high resolution interferometer for astronomical imaging. SFG is well known to be intrinsically a noiseless non linear process of upconversion which permits a wavelength shift. Thereby we propose to shift astronomical MIR and FIR radiation to shorter wavelength where optical fibers and optical components are available and efficient. In order to demonstrate the validity of this method for high resolution imaging, we plan to set up a two-arm upconversion interferometer on the CHARA telescope array (California). Each arm would include an upconversion stage at the focus of telescope. The success of such a project is obviously conditioned by the quality of nonlinear components (waveguided PPLN) in term of efficiency and noise biases. Moreover, coherence study requires the use of identical non linear components which implies manufacturing constraints. To ensure the feasibility of this project, several studies have been conducted. By implementing an upconversion interferometer in laboratory we have recently demonstrated our ability to analyze the coherence properties of a 1550nm signal at visible wavelength. We also have successfully converted astronomical light using one arm of this interferometer at the Hawaï observatory. It showed the capability of our instrument to astronomical observing conditions in photon counting regime. A preliminary mission at CHARA observatory allowed us to check the compatibility of our instrument with the environment onsite and expected photometric levels. From these data we estimate to be able to study the coherence of astronomical target at 1550nm using such an instrument.

Paper Details

Date Published: 20 February 2014
PDF: 9 pages
Proc. SPIE 8964, Nonlinear Frequency Generation and Conversion: Materials, Devices, and Applications XIII, 89641G (20 February 2014); doi: 10.1117/12.2039083
Show Author Affiliations
R. Baudoin, Xlim, CNRS, Univ. de Limoges (France)
Leukos Ester Technopole (France)
J. T. Gomes, Xlim, CNRS, Univ. de Limoges (France)
L. Delage, Xlim, CNRS, Univ. de Limoges (France)
L. Grossard, Xlim, CNRS, Univ. de Limoges (France)
T. A. Ten Brummelar, Mount Wilson Observatory (United States)
N. J. Scott, Mount Wilson Observatory (United States)
J. Sturmann, Mount Wilson Observatory (United States)
F. Reynaud, Xlim, CNRS, Univ. de Limoges (France)


Published in SPIE Proceedings Vol. 8964:
Nonlinear Frequency Generation and Conversion: Materials, Devices, and Applications XIII
Konstantin L. Vodopyanov, Editor(s)

© SPIE. Terms of Use
Back to Top