Calibration improvements expand filterscope diagnostic use

J. L. Herfindal, E. A. Unterberg, K. M. Davda, E. W. Garren, M. Groth, F. Scotti, A. C. Sontag, D. D. Truong, R. S. Wilcox

Research output: Contribution to journalArticlepeer-review

2 Scopus citations

Abstract

The filterscope diagnostic on DIII-D utilizes photomultiplier tubes to measure visible light emission from the plasma. The system has undergone a substantial upgrade since previous attempts to cross-calibrate the filterscope with other spectroscopic diagnostics were unsuccessful. The optics now utilize a dichroic mirror to initially split the light at nearly 99% transmission or reflectance for light below or above 550 nm. This allows the system to measure Dα emission without degrading visible light emission from the plasma for wavelengths below 550 nm (to measure Dβ, Dγ, W-I, C-III, etc.). Additional optimization of the optical components and calibration techniques reduce the error in the signal up to 10% in some channels compared to previous methods. Cross-calibration measurements with two other high resolution spectroscopic diagnostics now show excellent agreement for the first time. This expands the capabilities of the filterscope system allowing measurement of divertor detachment, emission profiles, edge-localized mode behavior, and plasma-wall interactions. It also enables direct comparisons against calculations from boundary plasma simulations. These were not possible before.

Original languageEnglish
Article number023504
JournalReview of Scientific Instruments
Volume95
Issue number2
DOIs
StatePublished - Feb 1 2024

Funding

Discussions with Adam Mclean are gratefully acknowledged. This material is based upon work supported by the U.S. Department of Energy, Office of Science, Office of Fusion Energy Sciences, using the DIII-D National Fusion Facility, a DOE Office of Science user facility, under Award Nos. DE-FC02-04ER54698, DE-AC05-00OR22725, DE-AC52-07NA27344, and DE-NA0003525. This manuscript has been authored by UT-Battelle, LLC, under Contract No. DE-AC05-00OR22725 with the U.S. Department of Energy (DOE). A. C. Sontag and K. M. Davda were supported through the ORNL DOE Award No. DE-AC05-00OR22725. The publisher, by accepting this article for publication, acknowledges that the U.S. government retains a nonexclusive, paid-up, irrevocable, worldwide license to publish or reproduce the published form of this manuscript, or allow others to do so, for U.S. government purposes. DOE will provide public access to these results of federally sponsored research in accordance with the DOE Public Access Plan ( http://energy.gov/downloads/doe-public-access-plan ). Discussions with Adam Mclean are gratefully acknowledged. This material is based upon work supported by the U.S. Department of Energy, Office of Science, Office of Fusion Energy Sciences, using the DIII-D National Fusion Facility, a DOE Office of Science user facility, under Award Nos. DE-FC02-04ER54698, DE-AC05-00OR22725, DE-AC52-07NA27344, and DE-NA0003525. This manuscript has been authored by UT-Battelle, LLC, under Contract No. DE-AC05-00OR22725 with the U.S. Department of Energy (DOE). A. C. Sontag and K. M. Davda were supported through the ORNL DOE Award No. DE-AC05-00OR22725. The publisher, by accepting this article for publication, acknowledges that the U.S. government retains a nonexclusive, paid-up, irrevocable, worldwide license to publish or reproduce the published form of this manuscript, or allow others to do so, for U.S. government purposes. DOE will provide public access to these results of federally sponsored research in accordance with the DOE Public Access Plan (http://energy.gov/downloads/doe-public-access-plan).

FundersFunder number
DOE Public Access Plan
ORNL DOE
U.S. Government
U.S. Department of Energy
Office of ScienceDE-AC05-00OR22725, DE-NA0003525, DE-FC02-04ER54698, DE-AC52-07NA27344
Fusion Energy Sciences

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