Energy-dependent polarization angle variability distinguishes reconnection from turbulence as the driver of blazar flares, with Mrk 421 and 1ES 1959+650 data favoring reconnection.
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2 Pith papers cite this work. Polarity classification is still indexing.
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Hybrid simulations demonstrate formation of hammerhead proton distributions via beam-driven right-handed wave instabilities under young solar wind conditions, consistent with quasi-linear theory.
citing papers explorer
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Energy-Dependent Polarization Angle Variability as a Robust Diagnostic for Blazar Flaring Mechanisms
Energy-dependent polarization angle variability distinguishes reconnection from turbulence as the driver of blazar flares, with Mrk 421 and 1ES 1959+650 data favoring reconnection.
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Hybrid simulations of the proton beam instabilities in the young solar wind. The formation of hammerhead-like distributions
Hybrid simulations demonstrate formation of hammerhead proton distributions via beam-driven right-handed wave instabilities under young solar wind conditions, consistent with quasi-linear theory.