Oblique Whistler-Mode Waves in the Inhomogeneous Magnetospheric Plasma: Resonant Interactions with Energetic Charged Particles

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Modeling the evolution of chorus waves into plasmaspheric hiss (2011, background): “…are at present not well understood and remain a topic of intense research [e.g., Nunn, 1971; 1974; Nunn et al., 2009; Trakhtengerts et al., 1996, 2004; Shklyar and Matsumoto, 2009; Bespalov et al., 2010; Lampe et al., 2010; Omura et al., 2008, 2009; Schriver et al., 2010; Santolik et al., 2010].”
Statistics of whistler mode waves in the outer radiation belt: Cluster STAFF‐SA measurements (2013, background): “It is worth noting that obtained results of distribution of normal angles can play an important role for models of nonlinear wave-particle interaction [Shklyar and Matsumoto, 2009].”
Particle Dynamics in the Earth's Radiation Belts: Review of Current Research and Open Questions (2020, background): “Multiple theoretical analyses and numerical simulations (see reviews, Shklyar & Matsumoto, 2009; Nunn & Omura, 2015) show that phase trapping of electrons in large‐amplitude oblique whistler mode waves in an inhomogeneous magnetic field can result in rapid acceleration, as well as atmospheric loss,…”
Earth's Van Allen Radiation Belts: From Discovery to the Van Allen Probes Era (2019, background): “LI AND HUDSON 8331 interactions with highly oblique chorus result in trapping of keV electrons and their acceleration up to a few hundred keV (Agapitov et al., 2015; Artemyev, Vasiliev, et al., 2014; Artemyev, Agapitov, et al., 2016; Shklyar & Matsumoto, 2009).”