Counter-streaming solar energetic electrons at 1 AU are reflected from precursor ICME shocks beyond 1 AU, shown by multi-spacecraft timing, anisotropy, and prior ICME positioning.
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Analysis of the September 6, 2011 coronal wave with the SOLERwave multi-sector method reveals over 40% speed variation (750-1500 km/s) between northward and northwestward segments, attributed to differences in magnetosonic speed from an MHD solution.
citing papers explorer
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Solar Energetic Particle Reflection by Precursor ICMEs: Multi-spacecraft Observations of Bi-Directional Electron Beams at 1 AU
Counter-streaming solar energetic electrons at 1 AU are reflected from precursor ICME shocks beyond 1 AU, shown by multi-spacecraft timing, anisotropy, and prior ICME positioning.
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Investigation of the Two-Dimensional Velocity Field of the Large-Scale Coronal Wave from September 6, 2011 using the SOLERwave Tool
Analysis of the September 6, 2011 coronal wave with the SOLERwave multi-sector method reveals over 40% speed variation (750-1500 km/s) between northward and northwestward segments, attributed to differences in magnetosonic speed from an MHD solution.