Transport of Solar Wind H+ and He++ Ions across Earth's Bow Shock

Authors :: H. E. Kim
Henri Rème
George K. Parks
Yuqiang Ma
S. Y. Fu
P. Canu
M. L. Goldstein
Ying Liu
Zhongwei Yang
Ensang Lee
Iannis Dandouras
J. Hong
N. Lin
Laboratoire de Physique des Plasmas (LPP)
Université Paris-Sud - Paris 11 (UP11)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Observatoire de Paris
Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-École polytechnique (X)-Sorbonne Université (SU)-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS)
Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-École polytechnique (X)-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS)
Source :: The Astrophysical journal letters, The Astrophysical journal letters, Bristol : IOP Publishing, 2016, 825 (2), pp.L27. ⟨10.3847/2041-8205/825/2/L27⟩, The Astrophysical journal letters, 2016, 825 (2), pp.L27. ⟨10.3847/2041-8205/825/2/L27⟩
Publication Year :: 2016
Publisher :: HAL CCSD, 2016.
Abstract: International audience; We have investigated the dependence of mass, energy, and charge of solar wind (SW) transport across Earth?s bow shock. An examination of 111 crossings during quiet SW in both quasi-perpendicular and quasi-parallel shock regions shows that 64 crossings had various degrees of heating and thermalization of SW. We found 22 crossings where the SW speed was

Language :: English
ISSN :: 20418205 and 20418213
Database :: OpenAIRE
Journal :: The Astrophysical journal letters, The Astrophysical journal letters, Bristol : IOP Publishing, 2016, 825 (2), pp.L27. ⟨10.3847/2041-8205/825/2/L27⟩, The Astrophysical journal letters, 2016, 825 (2), pp.L27. ⟨10.3847/2041-8205/825/2/L27⟩
Accession number :: edsair.doi.dedup.....3f6f1cec083c1d07507b0fd27cc285e1
Full Text :: https://doi.org/10.3847/2041-8205/825/2/L27⟩