Title
Design and characterization of a prototype divertor viewing infrared video bolometer for NSTX-U
Date Issued
01 November 2016
Access level
open access
Resource Type
journal article
Author(s)
Van Eden G.G.
Reinke M.L.
Peterson B.J.
Gray T.K.
Jaworski M.A.
Lore J.
Mukai K.
Sano R.
Pandya S.N.
Morgan T.W.
Princeton University
Publisher(s)
American Institute of Physics Inc.
Abstract
The InfraRed Video Bolometer (IRVB) is a powerful tool to measure radiated power in magnetically confined plasmas due to its ability to obtain 2D images of plasma emission using a technique that is compatible with the fusion nuclear environment. A prototype IRVB has been developed and installed on NSTX-U to view the lower divertor. The IRVB is a pinhole camera which images radiation from the plasma onto a 2.5 μm thick, 9 × 7 cm2 Pt foil and monitors the resulting spatio-temporal temperature evolution using an IR camera. The power flux incident on the foil is calculated by solving the 2D+time heat diffusion equation, using the foil's calibrated thermal properties. An optimized, high frame rate IRVB, is quantitatively compared to results from a resistive bolometer on the bench using a modulated 405 nm laser beam with variable power density and square wave modulation from 0.2 Hz to 250 Hz. The design of the NSTX-U system and benchtop characterization are presented where signal-to-noise ratios are assessed using three different IR cameras: FLIR A655sc, FLIR A6751sc, and SBF-161. The sensitivity of the IRVB equipped with the SBF-161 camera is found to be high enough to measure radiation features in the NSTX-U lower divertor as estimated using SOLPS modeling. The optimized IRVB has a frame rate up to 50 Hz, high enough to distinguish radiation during edge-localized-modes (ELMs) from that between ELMs.
Volume
87
Issue
11
Language
English
OCDE Knowledge area
Física de plasmas y fluídos Física nuclear
Scopus EID
2-s2.0-85048157232
Source
Review of Scientific Instruments
ISSN of the container
00346748
Sponsor(s)
This work was carried out with financial support from NWO (the Netherlands) and the Department of Energy (USA) with Contract Nos. DE-AC05-00OR22725 and DE-AC02-09CH11466l. The authors wish to acknowledge Yury Mala-ment, Robert Ellis, and Gustav Smalley (PPPL) for technical assistance and Dennis McCabe from FLIR Systems, Inc. for having camera models on loan. Horizon 2020 Framework Programme - 633053.
Sources of information: Directorio de Producción Científica Scopus