Skip to main content
U.S. Department of Energy
Office of Scientific and Technical Information

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

Journal Article · · Review of Scientific Instruments
DOI:https://doi.org/10.1063/1.4955487· OSTI ID:1368686
 [1];  [2];  [3];  [2];  [4];  [4];  [2];  [3];  [5];  [6];  [1]
  1. Dutch Institute for Fundamental Energy Research, AJ Eindhoven (The Netherlands)
  2. Oak Ridge National Lab. (ORNL), Oak Ridge, TN (United States)
  3. National Institute for Fusion Science, Toki (Japan)
  4. Princeton Plasma Physics Lab. (PPPL), Princeton, NJ (United States)
  5. National Institutes for Quantum and Radiological Science and Technology, Naka (Japan)
  6. Institute for Plasma Research, Gujarat (India)
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. Here, 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.
Research Organization:
Oak Ridge National Laboratory (ORNL), Oak Ridge, TN (United States); Princeton Plasma Physics Lab. (PPPL), Princeton, NJ (United States)
Sponsoring Organization:
USDOE
Grant/Contract Number:
AC02-09CH11466; AC05-00OR22725
OSTI ID:
1368686
Alternate ID(s):
OSTI ID: 1412066
OSTI ID: 22596633
Journal Information:
Review of Scientific Instruments, Journal Name: Review of Scientific Instruments Journal Issue: 11 Vol. 87; ISSN 0034-6748; ISSN RSINAK
Publisher:
American Institute of Physics (AIP)Copyright Statement
Country of Publication:
United States
Language:
English

References (9)

Bolometric imaging of detached plasmas in LHD journal August 2011
Calibration and sensitivity of the infrared imaging video bolometer journal March 2003
Two dimensional radiated power diagnostics on Alcator C-Mod journal October 2008
Development of imaging bolometers for magnetic fusion reactors (invited) journal October 2008
A reconsideration of the noise equivalent power and the data analysis procedure for the infrared imaging video bolometers journal December 2014
Progress toward commissioning and plasma operation in NSTX-U journal June 2015
Simulation of the Edge Plasma in Tokamaks journal January 2004
Comparison of Au and Pt Foils for an Imaging Bolometer journal January 2010
Foil Calibration for IR Imaging Bolometer by Laser Irradiation journal January 2012

Cited By (2)

Experimental tests of an infrared video bolometer on Alcator C-Mod journal October 2018
Plasma radiation studies in Magnum-PSI using resistive bolometry journal July 2018

Similar Records

Design and characterization of a prototype divertor viewing infrared video bolometer for NSTX-U
Journal Article · Mon Nov 14 23:00:00 EST 2016 · Review of Scientific Instruments · OSTI ID:22596633

Preliminary design of a tangentially viewing imaging bolometer for NSTX-U
Journal Article · Tue Aug 02 20:00:00 EDT 2016 · Review of Scientific Instruments · OSTI ID:1368172