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Updated: Apr 20, 2026

Applying X-ray Imaging Crystal Spectroscopy for Use as a High Temperature Plasma Diagnostic
Published on: August 25, 2016
Design and initial operation of a two-color soft x-ray camera system on the Compact Toroidal Hybrid experiment
J L Herfindal1, J D Dawson1, D A Ennis1
1Physics Department, Auburn University, Auburn, Alabama 36849, USA.
A new soft x-ray diagnostic system was developed for the Compact Toroidal Hybrid experiment. This system measures electron temperature profiles and fluctuations, aiding in understanding magnetohydrodynamic activity in stellarators.
Area of Science:
- Plasma Physics
- Fusion Energy Research
Background:
- The Compact Toroidal Hybrid (CTH) experiment is a five-field period current-carrying stellarator.
- Understanding plasma behavior, including electron temperature profiles and magnetohydrodynamic (MHD) activity, is crucial for fusion energy development.
Purpose of the Study:
- To develop and implement a multi-camera soft x-ray diagnostic system for the CTH experiment.
- To measure equilibrium electron temperature profiles and temperature fluctuations caused by MHD activity.
Main Methods:
- Utilized a multi-camera system with three cameras, each equipped with two 20-channel diode arrays.
- Employed two different beryllium filter thicknesses (1.8 μm and 3.0 μm) for dual-color measurements.
- Measured soft x-ray emissions to determine electron temperatures between 50 eV and 200 eV.
Main Results:
- Successfully developed a diagnostic capable of measuring electron temperature profiles and fluctuations.
- Observed temperature perturbations associated with sawtooth oscillations in hybrid discharges.
- Discussed the impact of plasma asymmetry and impurity line radiation on diagnostic design and measurements.
Conclusions:
- The developed soft x-ray diagnostic is effective for characterizing electron temperature in the CTH stellarator.
- The diagnostic provides valuable data for studying MHD activity and plasma dynamics.
- Further analysis of temperature perturbations can enhance understanding of plasma stability in current-carrying stellarators.
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