Design and characterization of a prototype divertor viewing infrared video bolometer for NSTX-U

G. G. Van Eden, M. L. Reinke, B. J. Peterson, T. K. Gray, L. F. Delgado-Aparicio, M. A. Jaworski, J. Lore, K. Mukai, R. Sano, S. N. Pandya, T. W. Morgan

Research output: Contribution to journalArticlepeer-review

4 Scopus citations

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.

Original languageEnglish
Article number11D402
JournalReview of Scientific Instruments
Volume87
Issue number11
DOIs
StatePublished - Nov 2016

Funding

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.

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