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Maximilien Péters de Bonhome

3 papers here

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • first author2
  • middle author1

Across the 3 of 3 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR2
  • physics.plasm-ph1
ORCID 0000-0002-7493-6181

identity via Semantic Scholar / OpenAlex

most citedA Kinetic Model of Solar Wind Acceleration Driven by Ambipolar Electric Potential and Velocity-Space Diffusion

5 citations · 5 across the 3 of their papers we have counts for

collaborators

3 papers

astro-ph.SR2026

Formation of Suprathermal Electron Populations in the Expanding, Turbulent Solar Wind

Maximilien Péters de Bonhome, Fabio Bacchini, Luca Pezzini +1

Nonthermal features are ubiquitously observed in electron velocity distribution functions in the solar wind, yet their origin in the collisionless, turbulent, expanding solar-wind…

physics.plasm-ph2026

Particle-in-Cell Methods for Simulations of Sheared, Expanding, or Escaping Astrophysical Plasma

Fabio Bacchini, Evgeny A. Gorbunov, Maximilien Péters de Bonhome +4

Particle-in-Cell (PIC) methods have achieved widespread recognition as simple and flexible approaches to model collisionless plasma physics in fully kinetic simulations of astrophy…

astro-ph.SR2025★ 5 cited

A Kinetic Model of Solar Wind Acceleration Driven by Ambipolar Electric Potential and Velocity-Space Diffusion

Maximilien Péters de Bonhome, Viviane Pierrard, Fabio Bacchini

Parker Solar Probe (PSP) observations have revealed that most of the solar wind acceleration occurs very close to the Sun. This acceleration is partly due to the global electric po…

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