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.
H., Lazar, M., & Qureshi, M
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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.