Magnetic reconnection as a mechanism to produce multiple thermal proton populations and beams locally in the solar wind Article

Lavraud, B, Kieokaew, R, Fargette, N et al. (2021). Magnetic reconnection as a mechanism to produce multiple thermal proton populations and beams locally in the solar wind . ASTRONOMY & ASTROPHYSICS, 656 10.1051/0004-6361/202141149

Open Access International Collaboration

cited authors

  • Lavraud, B; Kieokaew, R; Fargette, N; Louarn, P; Fedorov, A; Andre, N; Fruit, G; Genot, V; Reville, V; Rouillard, AP; Plotnikov, I; Penou, E; Barthe, A; Prech, L; Owen, CJ; Bruno, R; Allegrini, F; Berthomier, M; Kataria, D; Livi, S; Raines, JM; D'Amicis, R; Eastwood, JP; Froment, C; Laker, R; Maksimovic, M; Marcucci, F; Perri, S; Perrone, D; Phan, TD; Stansby, D; Stawarz, J; Toledo-Redondo, S; Vaivads, A; Verscharen, D; Zouganelis, I; Angelini, V; Evans, V; Horbury, TS; O'Brien, H

sustainable development goals

authors

publication date

  • December 14, 2021

published in

keywords

  • ACCELERATION
  • ALFVEN WAVES
  • Astronomy & Astrophysics
  • DISCONTINUITIES
  • ELECTROMAGNETIC PROTON/PROTON INSTABILITIES
  • EXHAUSTS
  • GENERATION
  • ION-ION INSTABILITIES
  • MAGNETOPAUSE
  • PROBE OBSERVATIONS
  • Physical Sciences
  • SPACE PLASMAS
  • Science & Technology
  • Sun
  • magnetic fields
  • solar wind

Digital Object Identifier (DOI)

publisher

  • EDP SCIENCES S A

volume

  • 656