Diffusive scattering of electrons by electron holes around injection fronts. Issue 3 (15th March 2017)

• Record Type: Journal Article
• Authors: Vasko, I. Y.; Agapitov, O. V.; Mozer, F. S.; Artemyev, A. V.; Krasnoselskikh, V. V.; Bonnell, J. W.
• Is Part Of: Journal of geophysical research. Volume 122:Issue 3(2017)
• Page Start: 3163
• Page End: 3182
• Publication Date: 2017-03-15
• Subjects: electron holes -- solitary waves -- injection -- radiation belt -- electron losses; Magnetospheric physics -- Periodicals; Space environment -- Periodicals; Cosmic physics -- Periodicals; Planets -- Atmospheres -- Periodicals; Heliosphere (Astrophysics) -- Periodicals; Geophysics -- Periodicals; 523.01
• DOI: 10.1002/2016JA023337
• Languages: English
• ISSNs: 2169-9380

Abstract

Abstract: Van Allen Probes have detected nonlinear electrostatic spikes around injection fronts in the outer radiation belt. These spikes include electron holes (EH), double layers, and more complicated solitary waves. We show that EHs can efficiently scatter electrons due to their substantial transverse electric fields. Although the electron scattering driven by EHs is diffusive, it cannot be evaluated via the standard quasi‐linear theory. We derive analytical formulas describing local electron scattering by a single EH and verify them via test particle simulations. We show that the most efficiently scattered are gyroresonant electrons (crossing EH on a time scale comparable to the local electron gyroperiod). We compute bounce‐averaged diffusion coefficients and demonstrate their dependence on the EH spatial distribution (latitudinal extent and spatial filling factor) and individual EH parameters (amplitude of electrostatic potential, velocity, and spatial scales). We show that EHs can drive pitch angle scattering of ≲ 5 keV electrons at rates 10 −2 −10 −4 s −1 and, hence, can contribute to electron losses and conjugated diffuse aurora brightenings. The momentum and pitch angle scattering rates can be comparable, so that EHs can also provide efficient electron heating. The scattering rates driven by EHs at L shells L ∼ 5–8 are comparable to those due to chorus waves and may exceed those due to electron cyclotron harmonics. Key Points: Electrostatic broadband turbulence around injection fronts in the outer radiation is due to electron phase space holes Electron holes drive efficient pitch angle and momentum scattering of gyroresonant electrons (typical energies are below a few keV) Bounce‐averaged diffusion coefficients driven by electron holes for electrons below a few keV are comparable to those due to chorus and electron cyclotron harmonics