Title
A computational tool for simulation and design of tangential multi-energy soft x-ray pin-hole cameras for tokamak plasmas
Date Issued
01 October 2018
Access level
metadata only access
Resource Type
journal article
Author(s)
Yamazaki H.
Groebner R.
Grierson B.
Hill K.
Pablant N.
Stratton B.
Efthimion P.
Ejiri A.
Takase Y.
Ono M.
Princeton University
Publisher(s)
American Institute of Physics Inc.
Abstract
A new tool has been developed to calculate the spectral, spatial, and temporal responses of multi-energy soft x-ray (ME-SXR) pinhole cameras for arbitrary plasma densities (ne,D), temperature (Te), and impurity densities (nZ). ME-SXR imaging provides a unique opportunity for obtaining important plasma properties (e.g., Te, nZ, and Zeff) by measuring both continuum and line emission in multiple energy ranges. This technique employs a pixelated x-ray detector in which the lower energy threshold for photon detection can be adjusted independently. Simulations assuming a tangential geometry and DIII-D-like plasmas (e.g., ne,0 ≈ 8 × 1019 m-3 and Te,0 ≈ 2.8 keV) for various impurity (e.g., C, O, Ar, Ni, and Mo) density profiles have been performed. The computed brightnesses range from few 102 counts pixel-1 ms-1 depending on the cut-off energy thresholds, while the maximum allowable count rate is 104 counts pixel-1 ms-1. The typical spatial resolution in the mid-plane is ≈0.5 cm with a photon-energy resolution of 500 eV at a 500 Hz frame rate.
Volume
89
Issue
10
Language
English
OCDE Knowledge area
Física de plasmas y fluídos Óptica
Scopus EID
2-s2.0-85054829898
PubMed ID
Source
Review of Scientific Instruments
ISSN of the container
00346748
Sponsor(s)
This work was supported by Princeton-UTokyo Educational Partnership on Plasma Physics and Dr. L. F. Delgado-Aparicio’s 2015 Department of Energy Early Career Award. This work was supported by the U.S. Department of Energy under Grant No. DE-FC02-04ER54698. This work was partly supported by JSPS Grant-in-Aid for Scientific Research (S) (No. 21226021), NIFS Collaboration Research Program No. NIFS14KOCR001, and JSPS A3 Foresight Program. We also acknowledge Princeton Plasma Physics Laboratory for their hosting and support for this work.
Sources of information: Directorio de Producción Científica Scopus