We present a theoretical analysis of electron pitch-angle scattering by ion-acoustic electrostatic fluctuations present in the Earth's bow shock and, presumably, collisionless shocks in general. We numerically simulate electron interaction with a single wave packet to demonstrate the scattering through phase bunching and phase trapping and quantify electron pitch-angle scattering in dependence on the wave amplitude and wave normal angle to the local magnetic field. The iterative mapping technique is used to model pitch-angle scattering of electrons by a large number of wave packets, which have been reported in the Earth's bow shock. Assuming that successive electron scatterings are not correlated, we revealed that the long-term dynamics of electrons is diffusive. The diffusion coefficient depends on the ratio ₀/W between the wave packet amplitude and electron energy, D∝ ( ₀/W)ν . A quasi-linear scaling ( ν ≈ 2 ) is observed for sufficiently small wave amplitudes, ₀ 10⁻³W , while the diffusion is nonlinear ( 1<ν <2 ) above this threshold. We show that pitch-angle diffusion of 1 keV electrons in the Earth's bow shock can be nonlinear. The corresponding diffusion coefficient scales with the intensity Ew² of the electrostatic fluctuations in a nonlinear fashion, D∝ Ewν with ν <2 , while its expected values in the Earth's bow shock are D~ 0.1x2013100 (Tₑ/W)ν -1/2\, rad²\, s⁻¹ . We speculate that in the Earth's quasi-perpendicular bow shock the stochastic shock drift acceleration mechanism with pitch-angle scattering provided by the electrostatic fluctuations can contribute to the acceleration of thermal electrons up to approximately 1 keV. The potential effects of a finite perpendicular coherence scale of the wave packets on the efficiency of electron scattering are discussed.
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Kamaletdinov et al. (2024) studied this question.
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