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Design elements and first data from a new Doppler backscattering system on the MAST-U spherical tokamak.
Rhodes, T L; Michael, C A; Shi, P; Scannell, R; Storment, S; Pratt, Q; Lantsov, R; Fitzgerald, I; Hall-Chen, V H; Crocker, N A; Peebles, W A.
Afiliação
  • Rhodes TL; Physics and Astronomy Department, University of California, Los Angeles, California 90098, USA.
  • Michael CA; Physics and Astronomy Department, University of California, Los Angeles, California 90098, USA.
  • Shi P; UKAEA/CCFE, Culham Science Centre, Abingdon, Oxfordshire, OX14 3DB, UK.
  • Scannell R; UKAEA/CCFE, Culham Science Centre, Abingdon, Oxfordshire, OX14 3DB, UK.
  • Storment S; Physics and Astronomy Department, University of California, Los Angeles, California 90098, USA.
  • Pratt Q; Physics and Astronomy Department, University of California, Los Angeles, California 90098, USA.
  • Lantsov R; Physics and Astronomy Department, University of California, Los Angeles, California 90098, USA.
  • Fitzgerald I; UKAEA/CCFE, Culham Science Centre, Abingdon, Oxfordshire, OX14 3DB, UK.
  • Hall-Chen VH; Institute of High Performance Computing, Singapore 138632, Singapore.
  • Crocker NA; Physics and Astronomy Department, University of California, Los Angeles, California 90098, USA.
  • Peebles WA; Physics and Astronomy Department, University of California, Los Angeles, California 90098, USA.
Rev Sci Instrum ; 93(11): 113549, 2022 Nov 01.
Article em En | MEDLINE | ID: mdl-36461471
ABSTRACT
A new Doppler backscattering (DBS) system has been installed and tested on the MAST-U spherical tokamak. It utilizes eight simultaneous fixed frequency probe beams (32.5, 35, 37.5, 40, 42.5, 45, 47.5, and 50 GHz). These frequencies provide a range of radial positions from the edge plasma to the core depending on plasma conditions. The system utilizes a combination of novel features to provide remote control of the probed density wavenumber, the launched polarization (X vs O-mode), and the angle of the launched DBS to match the magnetic field pitch angle. The range of accessible density turbulence wavenumbers (kθ) is reasonably large with normalized wavenumbers kθρs ranging from ≤0.5 to 9 (ion sound gyroradius ρs = 1 cm). This wavenumber range is relevant to a variety of instabilities believed to be important in establishing plasma transport (e.g., ion temperature gradient, trapped electron, electron temperature gradient, micro-tearing, kinetic ballooning modes). The system is specifically designed to address the requirement of density fluctuation wavevector alignment which can significantly reduce the SNR if not accounted for.

Texto completo: 1 Coleções: 01-internacional Base de dados: MEDLINE Idioma: En Revista: Rev Sci Instrum Ano de publicação: 2022 Tipo de documento: Article País de afiliação: Estados Unidos

Texto completo: 1 Coleções: 01-internacional Base de dados: MEDLINE Idioma: En Revista: Rev Sci Instrum Ano de publicação: 2022 Tipo de documento: Article País de afiliação: Estados Unidos
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