Theoretical astrophysics and plasma physics at RPC

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Interpreting Radial Correlation Doppler Reflectometry using Gyrokinetic Simulations

(2022)

Authors:

J Ruiz Ruiz, FI Parra, VH Hall-Chen, N Christen, M Barnes, J Candy, J Garcia, C Giroud, W Guttenfelder, JC Hillesheim, C Holland, NT Howard, Y Ren, AE White, JET contributors.
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A novel approach to radially global gyrokinetic simulation using the flux-tube code $\texttt{stella}$

(2022)

Authors:

DA St-Onge, M Barnes, FI Parra
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Insensitivity of a turbulent laser-plasma dynamo to initial conditions

(2022)

Authors:

AFA Bott, L Chen, P Tzeferacos, CAJ Palmer, AR Bell, R Bingham, A Birkel, DH Froula, J Katz, MW Kunz, C-K Li, H-S Park, R Petrasso, JS Ross, B Reville, D Ryu, FH Séguin, TG White, AA Schekochihin, DQ Lamb, G Gregori
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Input files for "A novel approach to radially global gyrokinetic simulation using the flux-tube code stella": arXiv 2201.01506

University of Oxford (2022)

Authors:

Denis A St-Onge, Michael Barnes, Felix I Parra

Abstract:

A collection of input files, and instructions on how to use them, for the manuscript entitled 'A novel approach to radially global gyrokinetic simulation using the flux-tube code stella'. These input files, which are designed for the gyrokinetic flux-tube code stella, are specifically for the simulations resulting in figures 2-10.
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Supplementary data for "extended electron tails in electrostatic microinstabilities and the nonadiabatic response of passing electrons": arXiv 2108.02822

University of Oxford (2022)

Authors:

Michael Richard Hardman, Felix Parra Diaz, Jason Parisi, Michael Barnes, Ching Lok Chong, Toby Adkins, Michail S Anastopoulos-Tzanis, David Dickinson, Howard Wilson

Abstract:

Supplementary data for the article "Extended electron tails in electrostatic microinstabilities and the nonadiabatic response of passing electrons": arXiv 2108.02822. The dataset includes a readme, GS2 FORTRAN namelist input files necessary to reproduce the simulations presented in the article, as well as scripts (using a mixture of Mathematica, MATLAB, and Python) for the calculation of collisional transport coefficients that appear in the collisional theory of the studied microinstabilities.
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