Bulletin of the American Physical Society
65th Annual Meeting of the APS Division of Plasma Physics
Monday–Friday, October 30–November 3 2023; Denver, Colorado
Session BO05: MFE: Diagnostics, Heating, and Current Drive
9:30 AM–12:30 PM,
Monday, October 30, 2023
Room: Governor's Square 14
Chair: Mirela Cengher, Massachusetts Institute of Technology
Abstract: BO05.00007 : DIP, a high-power IR dispersion interferometer using OpGaAs crystal for electron density measurement
10:42 AM–10:54 AM
Presenter:
Vincent Carrat
(Bertin technologies)
Authors:
Vincent Carrat
(Bertin technologies)
Guillaume Raffault
(Bertin Technologies)
Cécile Carcy
(Bertin Technologies)
David A Anthoine
(Bertin Technologies)
Antoine Sirinelli
(ITER Organization)
Reaching desired performances requires that sufficient laser power returning to the reception system after travelling to the vacuum vessel, crossing the plasma and going back, a 120 m long travel. So, it’s mandatory to limit laser power loss in the system and generate sufficient power at the beginning.
Mirrors surfaces in the vacuum vessel will suffer from the very harsh environment. Since longer wavelength are less sensitive to surface deteriorations, this throughout loss is mitigated by operating the interferometer in the IR region.
Bertin is currently building an IR dispersion interferometer operating at unprecedented power levels in this spectral region. A commercially available CO2 laser, is producing 30W CW of power at 9.6μm. One report the reliable generation of more than 100 mW CW at 4.8μm by frequency doubling, using a periodically poled GaAs (OpGaAs) crystal. This high pump power regime, will be on the emission side, before lasers are going through the plasma. After the plasma, on the reception side, a second doubling crystal needs to operate with 20 times less power. Bertin used the crystal in a different doubling geometry, in order to optimize 2nd harmonic generation and get a high SNR on the interference signal observed at 4.8μm.
The views and opinions expressed herein do not necessarily reflect those of the ITER Organization.
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