Diagnosing the pedestal magnetic field and magnetohydrodynamics radial structure with pedestal–scrape of layer electron cyclotron emission radiation inversion in H-mode plasma (invited)

Author:

Yu G.1ORCID,Zhu Y.1ORCID,Austin M.2ORCID,Chen Y.1ORCID,Cao J.1,Diallo A.3,Kramer G.3ORCID,Li Z.4ORCID,Li X.1,Liu X.1ORCID,Nazikian R.5ORCID,Zheng Y.1ORCID,Luhmann N. C.1

Affiliation:

1. Department of Electrical and Computer Engineering, University of California, Davis, California 95616, USA

2. Institute for Fusion Studies, University of Texas, Austin, Texas 78712, USA

3. Princeton Plasma Physics Lab, Princeton, New Jersey 08540, USA

4. Oak Ridge Associated Universities, Oak Ridge, Tennessee 37831, USA

5. General Atomic, San Diego, California 92121, USA

Abstract

Forward modeling is used to interpret inversion patterns of the pedestal–Scrape of Layer (SOL) Electron Cyclotron Emission (ECE) in DIII-D H-mode experiments. The modeling not only significantly improves the ECE data interpretation quality but also leads to the potential measurements of (1) the magnetic field strength |B| at the separatrix, (2) the pedestal |B| evolution during an inter-Edge Localized Mode (ELM) period, and (3) the pedestal Magnetohydrodynamics (MHD) radial structure. The ECE shine-through effect leads to three types of pedestal–SOL radiation inversions that are discussed in this paper. The first type of inversion is the non-monotonic T e, rad profile with respect to the major radius. Using the ECE frequency at the minimum T e, rad, the inversion can be applied to measure the magnetic field |B| at the separatrix and calibrate the mapping of the ECE channels with respect to the separatrix. The second type of inversion refers to the opposite phase between the radiation fluctuations δT e, rad at the pedestal and SOL. This δT e, rad phase inversion is sensitive to density and temperature fluctuations at the pedestal foot and, thus, can be used to qualitatively measure the MHD radial structure. The third type of inversion appears when the pedestal and SOL T e, rad evolve in an opposite trend, which can be used to infer the pedestal |B| field change during an inter-ELM period. The bandwidth effect on measuring δT e, rad due to pedestal MHD is also investigated in the radiation modeling.

Funder

DOE Office of Science

Publisher

AIP Publishing

Subject

Instrumentation

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