Upstream and downstream wave packets associated with low-Mach number interplanetary shocks

Wave packets are frequently observed upstream and/or downstream of shocks in a magnetized plasma. We present a comparison of Wind and Spektr‐R observations of 27 interplanetary low‐Mach number (

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Bibliographic Details
Published in:Geophysical research letters 2014-11, Vol.41 (22), p.8100-8106
Main Authors: Goncharov, O., Šafránková, J., Němeček, Z., Přech, L., Pitňa, A., Zastenker, G. N.
Format: Article
Language:English
Subjects:
Astrophysics
Atmospheric pressure
Density
Downstream
Downstream effects
Geophysics
interplanetary shocks
Kinetics
Mach number
Packets (communication)
Phase shift
plasma waves
Precursors
Ramps
Separation
Shock
Spacecraft
Temperature
Temperature effects
Temperature variations
Upstream
Wave packets
Wavelengths
Wind
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Description
Summary:Wave packets are frequently observed upstream and/or downstream of shocks in a magnetized plasma. We present a comparison of Wind and Spektr‐R observations of 27 interplanetary low‐Mach number (
ISSN:0094-8276
1944-8007
DOI:10.1002/2014GL062149