NIST - National Institute of Standards and Technology

10/23/2026 | Press release | Distributed by Public on 10/24/2026 03:22

Advanced Sensors for Multi-Color Infrared Imaging Bolometers

Published
October 23, 2026

Author(s)

Christopher Yung, Glen Wurden

Abstract

A new form of infrared imaging bolometer (IRIB) suitable for radiometric imaging of high temperature plasmas is presented offering several key advantages: instantaneous power read-out via an IR camera (within thermal timescale constraints), increased robustness and uniformity as compared to a traditional imaging foil, ease of calibration, and pixelated imaging. These advantages are accomplished with the use of silicon microfabrication techniques and vertically aligned carbon nanotubes (VACNTs). An additional feature of this approach is the ability to make a multi-color pixel array, which we call the RGB imaging bolometer sensor. By customizing a pattern of individual neighboring pixels with different radiation absorption characteristics, imaging bolometers for multiple energy bands are possible. Since the thin film architecture for each pixel determines its respective photon stopping power, individual pixels can be designed to absorb varying levels of photon energy depending upon the presence of an optical absorber, thickness, and Z of the thin film metals. As a result, we can image three (or more) different energy bands of plasma radiation, simultaneously, with hundreds, if not thousands of lines of sight.
Citation
Review of Scientific Instruments
Volume
97
Issue
10
Pub Type
Journals

Keywords

fusion, diagnostic, IRVB

Citation

Yung, C. and Wurden, G. (2026), Advanced Sensors for Multi-Color Infrared Imaging Bolometers, Review of Scientific Instruments, [online], https://doi.org/10.1063/5.0349799, https://nps-ext.nist.gov/nps/nps_public_api/api/Publication/file/962459 (Accessed October 24, 2026)
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NIST - National Institute of Standards and Technology published this content on October 23, 2026, and is solely responsible for the information contained herein. Distributed via Public Technologies (PUBT), unedited and unaltered, on October 24, 2026 at 09:22 UTC. If you believe the information included in the content is inaccurate or outdated and requires editing or removal, please contact us at [email protected]