Title
In situ wavelength calibration system for the X-ray Imaging Crystal Spectrometer (XICS) on W7-X
Date Issued
01 October 2018
Access level
open access
Resource Type
review
Author(s)
Kring J.
Pablant N.
Langenberg A.
Rice J.
Maurer D.
Traverso P.
Bitter M.
Hill K.
Reinke M.
Princeton University
Publisher(s)
American Institute of Physics Inc.
Abstract
An in situ wavelength calibration system for the X-ray Imaging Crystal Spectrometer (XICS) on W7-X has been developed to provide routine calibration between plasma shots. XICS is able to determine plasma flow profiles by measuring the Doppler shift of x-ray line emission from highly charged impurity species. A novel design is described that uses an x-ray tube with a cadmium anode placed in front of the diffracting spherically bent crystal. This arrangement provides calibration lines over the full detector extent for both the Ar16+ and Ar17+/Fe24+ spectrometer channels. This calibration system can provide a relative wavelength accuracy of 3 × 10−7 Å across the full spatial extent of the detector, which corresponds to 50 m/s in the W7-X system. An absolute wavelength calibration of 1 × 10−5 Å is expected, corresponding to 1 km/s, based on the current known accuracy of the calibration wavelength and the achievable measurement of the absolute positioning of the hardware. This calibration system can be used to independently calibrate XICS systems on both stellarators and tokamaks, without the need for special plasma conditions often used for calibration, such as locked modes on tokamaks. Experimental and simulated results are shown along with expected results, and the complete design of the calibration hardware that is to be installed in the W7-X XICS system.
Volume
89
Issue
10
Language
English
OCDE Knowledge area
Física de plasmas y fluídos
Scopus EID
2-s2.0-85052601263
PubMed ID
Source
Review of Scientific Instruments
ISSN of the container
00346748
Sponsor(s)
Research was supported by the U.S. DOE under Contract No. DE-AC02-09CH11466 with Princeton University. This work has been carried out within the framework of the EUROfusion Consortium and has received funding from the Euratom research and training programme 2014-2018 under Grant Agreement No. 633053. The views and opinions expressed herein do not necessarily reflect those of the European Commission. We thank MIT PSFC for the use of their facilities in testing the calibration schemes.
Sources of information:
Directorio de Producción Científica
Scopus