Acceleration of Ring Current Protons Driven by Magnetosonic Waves: Comparisons of Test Particle Simulations with Quasilinear Calculations
نویسندگان
چکیده
Wave–particle interactions play important roles in local acceleration and pitch angle scattering loss of charged particle dynamics astrophysics space physics, energy transfer between plasma waves particles is a key problem physics. Using full relativistic test simulations, we quantitatively evaluate the magnetosonic wave-driven Earth's ring current protons both inside outside plasmapause at L = 4.5. Analysis resonance conditions indicates that broadband can affect by multiple harmonic cyclotron resonances. With representative amplitude ∼200 pT, produce diffusion coefficients, obtained from rates ∼10−4 s−1 for ∼1–3 keV ∼3–30 plasmapause, equatorial angles ∼75°–90°. Compared with quasilinear theory calculations, coefficients exhibit difference due to nonresonant transit time effect plasmapause. Subsequent 2D Fokker–Planck simulations indicate on timescale ∼2 days, effectively enhance phase density ∼10 ∼100 ∼60°–90°, thereby leading evolvement proton distribution Kappa-type 90°-peaked profile. Our results demonstrate an process different populations magnetospheric hence contributes dynamic evolution current.
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ژورنال
عنوان ژورنال: The Astrophysical Journal
سال: 2021
ISSN: ['2041-8213', '2041-8205']
DOI: https://doi.org/10.3847/1538-4357/abd2b3