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

Dr Louis Richard

Marie Curie Fellow

Research theme

  • Plasma physics

Sub department

  • Rudolf Peierls Centre for Theoretical Physics

Research groups

  • Theoretical astrophysics and plasma physics at RPC
louis.richard@physics.ox.ac.uk
  • About
  • Publications

Statistical Study of Betatron and Fermi Electron Acceleration at Dipolarization Fronts

(2025)

Authors:

Apostolos Kolokotronis, Daniel Bruce Graham, Yuri V Khotyaintsev, Cecilia Norgren, Konrad Steinvall, Louis Richard
More details from the publisher

Ion Temperature Anisotropy Limits from Magnetic Curvature Scattering in Magnetotail Reconnection Jets

ArXiv 2511.18956 (2025)

Authors:

Louis Richard, Anton V Artemyev, Cecilia Norgren, Xin An, Sergey R Kamaletdinov, Yuri V Khotyaintsev
Details from ArXiV

Non-Maxwellianity of ion velocity distributions in the Earth's magnetosheath.

Physical review. E 112:5 (2025) L053201

Authors:

Louis Richard, Sergio Servidio, Ida Svenningsson, Anton V Artemyev, Kristopher G Klein, Emiliya Yordanova, Alexandros Chasapis, Oreste Pezzi, Yuri V Khotyaintsev

Abstract:

We analyze the deviations from local thermodynamic equilibrium (LTE) of the ion velocity distribution function (iVDF) in collisionless plasma turbulence. Using data from the magnetospheric multiscale (MMS) mission, we examine the non-Maxwellianity of 439 685 iVDFs in the Earth's magnetosheath. We find that the iVDFs' anisotropies and the high-order non-bi-Maxwellian features are widespread and can be significant. Our results show that the complexity of the iVDFs is strongly influenced by the ion plasma beta and turbulence intensity, with high-order non-LTE features emerging in the presence of large-amplitude magnetic field fluctuations. Furthermore, our analysis indicates that turbulence-driven magnetic curvature contributes to the isotropization of the iVDFs by scattering the ions, emphasizing the complex interaction between turbulence and the velocity distribution of charged particles in collisionless plasmas.
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Finding Local Parallel Electric Fields in Magnetotail Reconnection Using a Two-Spacecraft Method

(2025)

Authors:

Jack White, Yuri V Khotyaintsev, Cecilia Norgren, Daniel Bruce Graham, Louis Richard
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Electron and Ion Dynamics in Reconnection Diffusion Regions

Space Science Reviews Springer Science and Business Media LLC 221:5 (2025) 73

Authors:

C Norgren, L-J Chen, DB Graham, N Bessho, J Egedal, L Richard, Yu V Khotyaintsev, J Shuster, S Toledo-Redondo, B Lavraud, H Hasegawa, JP Eastwood, M Hesse, Y-H Liu, JC Holmes, M Argall

Abstract:

Abstract Magnetic reconnection is a fundamental plasma process responsible for the sometimes explosive release of magnetic energy in space and laboratory plasmas. Inside the diffusion regions of magnetic reconnection, the plasma becomes demagnetized and decouples from the magnetic field, enabling the change in magnetic topology necessary to power the energy release over larger scales. Since it was launched in 2015, the Magnetospheric MultiScale (MMS) mission has significantly advanced the understanding of the particle dynamics key to magnetic reconnection by providing high-resolution, in-situ measurements able to resolve ion and electron kinetic scales, i.e. a fraction of a gyroradius, that have confirmed theoretical predictions, revealed new phenomena, and refined existing models. These breakthroughs are critical for understanding not only space plasmas but also laboratory and astrophysical plasmas where magnetic reconnection occurs. In this work, we review the ion and electron dynamics occurring within the diffusion regions, in the inflow, along the separatrices, and downstream of the diffusion regions, in different reconnection configurations: symmetric, asymmetric, antiparallel, and guide field reconnection.
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