High‐Frequency Waves Driven by Agyrotropic Electrons Near the Electron Diffusion Region

National Aeronautics and Space Administration's Magnetosphere Multiscale mission reveals that agyrotropic electrons and intense waves are prevalently present in the electron diffusion region. Prompted by two distinct Magnetosphere Multiscale observations, this letter investigates by theoretical means and the properties of agyrotropic electron beam‐plasma instability and explains the origin of different structures in the wave spectra. The difference is owing to the fact that in one instance, a continuous beam mode is excited, while in the other, discrete Bernstein modes are excited, and the excitation of one mode versus the other depends on physical input parameters, which are consistent with observations. Analyses of dispersion relations show that the growing mode becomes discrete when the maximum growth rate is lower than the electron cyclotron frequency. Making use of particle‐in‐cell simulations, we found that the broadening angle Δ in the gyroangle space is also an important factor controlling the growth rate. Ramifications of the present finding are also discussed.
Key Points MMS observed two different types of waves near the electron diffusion region (discrete electron Bernstein waves and continuous beam modes)A unified kinetic theory that can explain both types of wave generation is derivedThe condition that the maximum growth rate of instability equals the electron cyclotron frequency is the threshold of transitions