Intense Whistler-mode Waves at Foreshock Transients: Characteristics and Regimes of Wave−Particle Resonant Interaction

• Published in: The Astrophysical journal Vol. 944; no. 2; pp. 193 - 202
• Main Authors: Shi, Xiaofei, Liu, Terry, Artemyev, Anton, Angelopoulos, Vassilis, Zhang, Xiao-Jia, Turner, Drew L.
• Format: Journal Article
• Language: English
• Published: Philadelphia The American Astronomical Society 01.02.2023; IOP Publishing
• Subjects: Amplitudes; Anisotropy; Astrophysics; Electromagnetic radiation; Electron acceleration; Electrons; Energetic particles; Heat flux; Magnetic fields; Narrowband; Particle dynamics; Particle interactions; Planetary bow shocks; Resonant interactions; Thermalization (energy absorption); Whistler waves; Whistlers
• ISSN: 0004-637X; 1538-4357
• DOI: 10.3847/1538-4357/acb543

Thermalization and heating of plasma flows at shocks result in unstable charged-particle distributions that generate a wide range of electromagnetic waves. These waves, in turn, can further accelerate and scatter energetic particles. Thus, the properties of the waves and their implication for wave−particle interactions are critically important for modeling energetic particle dynamics in shock environments. Whistler-mode waves, excited by the electron heat flux or a temperature anisotropy, arise naturally near shocks and foreshock transients. As a result, they can often interact with suprathermal electrons. The low background magnetic field typical at the core of such transients and the large wave amplitudes may cause such interactions to enter the nonlinear regime. In this study, we present a statistical characterization of whistler-mode waves at foreshock transients around Earth’s bow shock, as they are observed under a wide range of upstream conditions. We find that a significant portion of them are sufficiently intense and coherent (narrowband) to warrant nonlinear treatment. Copious observations of background magnetic field gradients and intense whistler wave amplitudes suggest that phase trapping, a very effective mechanism for electron acceleration in inhomogeneous plasmas, may be the cause. We discuss the implications of our findings for electron acceleration in planetary and astrophysical shock environments.