On the origin of short large-amplitude magnetic structures upstream of quasi-parallel collisionless shocks
Author:
Publisher
American Geophysical Union (AGU)
Subject
General Earth and Planetary Sciences,Geophysics
Link
http://onlinelibrary.wiley.com/wol1/doi/10.1029/93GL00803/fullpdf
Reference10 articles.
1. Steepening of parallel propagating hydromagnetic waves into magnetic pulsations: A simulation study;Akimoto;J. Geophys. Res.,1991
2. Electromagnetic ion beam instabilities: Hot beams at interplanetary shocks;Gary;Astrophys. J.,1985
3. Upstream hydromagnetic waves and their association with backstreaming ion populations: ISEE 1 and 2 observations;Hoppe;J. Geophys. Res.,1981
4. A study of ULF wave foreshock morphology - II: Spatial variation of ULP waves;Le;Planet. Space. Sci.,1992
5. Steepening of kinetic magnetosonic waves into shocklets: Simulations and consequences for planetary shocks and comets;Omidi;J. Geophys. Res.,1990
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