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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

Proton and Helium Ion Acceleration at Magnetotail Plasma Jets

Journal of Geophysical Research: Space Physics American Geophysical Union (AGU) 127:8 (2022) e2022JA030430

Authors:

L Richard, Yu V Khotyaintsev, DB Graham, A Vaivads, R Nikoukar, IJ Cohen, DL Turner, SA Fuselier, CT Russell

Abstract:

AbstractWe investigate two flow bursts in a series of Earthward bursty bulk flows (BBFs) observed by the Magnetospheric Multiscale spacecraft in Earth's magnetotail at (−24, 7, 4) RE in Geocentric Solar Magnetospheric coordinates. At the leading edges of the BBFs, we observe complex magnetic field structures. In particular, we focus on one BBF which contains large�amplitude magnetic field fluctuations on the time scale of the proton gyroperiod, and another with a large scale dipolarization. For both events, the magnetic field structures are associated with flux increases of supra�thermal ions with energies ≳100 keV. We observe that helium ions dominate the ion flux at energies ≳150 keV. We investigate the ion acceleration mechanism and its dependence on the mass and charge state of H+ and He2+ ions. We show that for both events, the ions with gyroradii smaller than the dawn�dusk scale of the structure are accelerated by the ion bulk flow. For ions with larger gyroradii, the acceleration is likely due to a localized spatially limited electric field for the event with a large�scale dipolarization. For the event with fluctuating magnetic field, the acceleration of ions with gyroradii comparable with the scale of the magnetic fluctuations can be explained by resonance acceleration.

Ion Acceleration at Magnetotail Plasma Jets

ArXiv 2203.00708 (2022)

Authors:

L Richard, Yu V Khotyaintsev, DB Graham, A Vaivads, R Nikoukar, IJ Cohen, DL Turner, SA Fuselier, CT Russell

Investigation of the homogeneity of energy conversion processes at dipolarization fronts from MMS measurements

Physics of Plasmas AIP Publishing 29:1 (2022) 012906

Authors:

SW Alqeeq, O Le Contel, P Canu, A Retinò, T Chust, L Mirioni, L Richard, Y Aït-Si-Ahmed, A Alexandrova, A Chuvatin, N Ahmadi, SM Baraka, R Nakamura, FD Wilder, DJ Gershman, PA Lindqvist, Yu V Khotyaintsev, RE Ergun, JL Burch, RB Torbert, CT Russell, W Magnes, RJ Strangeway, KR Bromund, H Wei, F Plaschke, BJ Anderson, BL Giles, SA Fuselier, Y Saito, B Lavraud

Abstract:

We report on six dipolarization fronts (DFs) embedded in fast earthward flows detected by the Magnetospheric Multiscale mission during a substorm event on 23 July 2017. We analyzed Ohm's law for each event and found that ions are mostly decoupled from the magnetic field by Hall fields. However, the electron pressure gradient term is also contributing to the ion decoupling and likely responsible for an electron decoupling at DF. We also analyzed the energy conversion process and found that the energy in the spacecraft frame is transferred from the electromagnetic field to the plasma (J·E>0) ahead or at the DF, whereas it is the opposite (J·E<0) behind the front. This reversal is mainly due to a local reversal of the cross-tail current indicating a substructure of the DF. In the fluid frame, we found that the energy is mostly transferred from the plasma to the electromagnetic field (J·E′<0) and should contribute to the deceleration of the fast flow. However, we show that the energy conversion process is not homogeneous at the electron scales due to electric field fluctuations likely related to lower-hybrid drift waves. Our results suggest that the role of DF in the global energy cycle of the magnetosphere still deserves more investigation. In particular, statistical studies on DF are required to be carried out with caution due to these electron scale substructures.

Observations of Short�Period Ion�Scale Current Sheet Flapping

Journal of Geophysical Research: Space Physics American Geophysical Union (AGU) 126:8 (2021) e2021JA029152

Authors:

L Richard, Yu V Khotyaintsev, DB Graham, MI Sitnov, O Le Contel, P�A Lindqvist

Abstract:

AbstractKink�like flapping motions of current sheets are commonly observed in the magnetotail. Such oscillations have periods of a few minutes down to a few seconds and they propagate toward the flanks of the plasma sheet. Here, we report a short�period ( s) flapping event of a thin current sheet observed by the Magnetospheric Multiscale spacecraft in the dusk�side plasma sheet following a fast Earthward plasma flow. We characterize the flapping structure using the multi�spacecraft spatiotemporal derivative and timing methods, and we find that the wave�like structure is propagating along the average current direction with a phase velocity comparable to the ion velocity. We show that the wavelength of the oscillating current sheet scales with its thickness as expected for a drift�kink mode. The decoupling of the ion bulk motion from the electron bulk motion suggests that the current sheet is thin. We discuss the presence of the lower hybrid waves associated with gradients of density as a broadening process of the thin current sheet.

Observations of Short-Period Ion-Scale Current Sheet Flapping

ArXiv 2101.08604 (2021)

Authors:

L Richard, Yu V Khotyaintsev, DB Graham, MI Sitnov, O Le Contel, P-A Lindqvist

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