On the origin of the quasi-perpendicular ion foreshock: Full-particle simulations
Author:
Affiliation:
1. LPP-Ecole polytechnique-UPMC; Laboratoire de Physique des Plasmas, Ecole polytechnique; Palaiseau France
2. LATMOS-UVSQ-IPSL-CNRS; Guyancourt France
Publisher
American Geophysical Union (AGU)
Subject
Space and Planetary Science,Geophysics
Link
http://onlinelibrary.wiley.com/wol1/doi/10.1002/jgra.50158/fullpdf
Reference73 articles.
1. Quasi-perpendicular shock structure and processes;Bale;Space Sci. Rev.,2005
2. Macrostructure of collisionless bow shocks: 2. ULF waves in the foreshock and magnetosheath;Blanco-Cano;J. Geophys. Res.,2006a
3. ULF waves and their influence on bow shock and magnetosheath structures;Blanco-Cano;Adv. Space Res.,2006b
4. Global hybrid simulations: Foreshock waves and cavitons under radial interplanetary magnetic field geometry;Blanco-Cano;J. Geophys. Res.,2009
5. Reflected and diffuse ions backstreaming from the Earth's bow shock: 2. Origin;Bonifazi;J. Geophys. Res.,1981a
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