A near-Sun interplanetary shock's upstream foreshock resolves into four wave families, showing a proton-beam-driven scattering field and a weak compressive fast-mode component that changes resonance energies by up to 13%.
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The Wave-Regulated Precursor of a Near-Parallel Interplanetary Shock Observed by Parker Solar Probe
A near-Sun interplanetary shock's upstream foreshock resolves into four wave families, showing a proton-beam-driven scattering field and a weak compressive fast-mode component that changes resonance energies by up to 13%.