A comparison of magnetosheaths, ICME sheaths, and the heliosheath

Details A comparison of magnetosheaths, ICME sheaths, and the heliosheath A comparison of magnetosheaths, ICME sheaths, and the heliosheath

Aug 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aipc..932..387r&link_type=abstract

TURBULENCE AND NONLINEAR PROCESSES IN ASTROPHYSICAL PLASMAS; 6th Annual International Astrophysics Conference. AIP Conference P

Astronomy and Astrophysics

Astrophysics

2

Magnetosheath, Solar Wind/Magnetosphere Interactions

Scientific paper

Sheaths are regions of compressed, heated, decelerated, and deflected
flow behind a shock. We compare three types of sheath observed in the
heliosphere, planetary magnetosheaths, ICME sheaths, and the
heliosheath. Features common to these sheaths are plasma depletion
layers, mirror mode waves, hot proton components, and asymmetries.

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