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Theoretical physicists working at a blackboard collaboration pod in the Beecroft building.
Credit: Jack Hobhouse

Professor Felix Parra Diaz

Professor of Physics

Research theme

  • Plasma physics

Sub department

  • Rudolf Peierls Centre for Theoretical Physics

Research groups

  • Theoretical astrophysics and plasma physics at RPC
felix.parradiaz@physics.ox.ac.uk
Rudolf Peierls Centre for Theoretical Physics
  • About
  • Publications

Beam focusing and consequences for Doppler backscattering measurements

Journal of Plasma Physics Cambridge University Press (CUP) 91:2 (2025) e60

Authors:

J Ruiz Ruiz, FI Parra, VH Hall-Chen, N Belrhali, C Giroud, JC Hillesheim, NA Lopez, JET contributors
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Measurement of Zero-Frequency Fluctuations Generated by Coupling between Alfvén Modes in the JET Tokamak.

Physical review letters American Physical Society (APS) 134:9 (2025) 95103

Authors:

J Ruiz Ruiz, J Garcia, M Barnes, M Dreval, C Giroud, Vh Hall-Chen, Mr Hardman, Jc Hillesheim, Y Kazakov, S Mazzi, Bs Patel, Fi Parra, Aa Schekochihin, Ž Štancar, JET Contributors and the EUROfusion Tokamak Exploitation Team

Abstract:

We report the first experimental detection of a zero-frequency fluctuation that is pumped by an Alfvén mode in a magnetically confined plasma. Core-localized Alfvén modes of frequency inside the toroidicity-induced gap (and its harmonics) exhibit three-wave coupling interactions with a zero-frequency fluctuation. The observation of the zero-frequency fluctuation is consistent with theoretical and numerical predictions of zonal modes pumped by Alfvén modes, and is correlated with an increase in the deep core ion temperature, temperature gradient, confinement factor H_{89,P}, and a reduction in the main ion heat diffusivity. Despite the energetic particle transport induced by the Alfvén eigenmodes, the generation of a zero-frequency fluctuation that can suppress the turbulence leads to an overall improvement of confinement.
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Piecewise Omnigenous Stellarators.

Physical review letters 133:18 (2024) 185101

Authors:

JL Velasco, I Calvo, FJ Escoto, E Sánchez, H Thienpondt, FI Parra

Abstract:

In omnigenous magnetic fields, charged particles are perfectly confined in the absence of collisions and turbulence. For this reason, the magnetic configuration is optimized to be close to omnigenity in any candidate for a stellarator fusion reactor. However, approaching omnigenity imposes severe constraints on the spatial variation of the magnetic field. In particular, the topology of the contours of constant magnetic field strength on each magnetic surface must be such that there are no particles transitioning between different types of wells. This, in turn, usually leads to complicated plasma shapes and coils. This Letter presents a new family of optimized fields that display tokamak-like collisional energy transport while having transitioning particles. This result radically broadens the space of accessible reactor-relevant configurations.
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Reduction or Enhancement of Stellarator Turbulence by Impurities.

Physical review letters 133:10 (2024) 105101

Authors:

JM García-Regaña, I Calvo, FI Parra, H Thienpondt

Abstract:

A systematic study of the impact of impurities on the turbulent heat fluxes is presented for the stellarator Wendelstein 7-X (W7-X) and, for comparison, the Large Helical Device and ITER. By means of nonlinear multispecies gyrokinetic simulations, it is shown that impurities, depending on the sign of their density gradient, can significantly enhance or reduce turbulent ion heat losses. For the relevant scenario of turbulence reduction, an optimal impurity concentration that minimizes the ion heat diffusivity emerges as a universal feature. This result demonstrates the potential of impurities for controlling turbulence and accessing enhanced confinement regimes in fusion plasmas and, in particular, in W7-X.
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Ion-temperature- and density-gradient-driven instabilities and turbulence in Wendelstein 7-X close to the stability threshold

Journal of Plasma Physics Cambridge University Press (CUP) 90:4 (2024) 905900414

Authors:

L Podavini, A Zocco, JM García-Regaña, M Barnes, FI Parra, A Mishchenko, P Helander
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