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

HIGHLIGHTS

• who: Lavraud B. and colleagues from the Laboratoire d'astrophysique Bordeaux, UnivBordeaux, CNRS, Pessac, France Department of Surface and Plasma Science, Faculty of Mathematics and Physics, Charles University, Prague, Czech Republic have published the article: Magnetic reconnection as a mechanism to produce multiple thermal proton populations and beams locally in the solar wind, in the Journal: (JOURNAL) of 16/07/2020
• what: The authors discuss how this proportion may be underestimated and how it may depend on solar wind type and distance from the Sun. Note that the authors focus here on populations or beams . . .
  

   

  

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