2020
DOI: 10.1029/2020gl088434
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Revisit the Analytical Approximation of Transit‐Time Scattering for Fast Magnetosonic Waves

Abstract: Nonresonant interactions between fast magnetosonic waves and magnetospheric particles have obtained more and more attention. Through such nonresonant interactions, magnetosonic waves can lead to the so‐called transit‐time scattering on particles. The previous analytical approximation has been demonstrated capable of capturing the main results of test particle simulations but takes a computation time about 4 order of magnitude faster than the latter. However, the typical ripples in the diffusion coefficient map… Show more

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Cited by 22 publications
(30 citation statements)
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“…To further demonstrate that the observed MS waves can cause flux enhancements of mirroring ring current ions, following the analytical approximation in Bortnik et al (2015) which can capture the main results of test particle simulations but take a computation time about 4 order of magnitude faster than the latter, we calculate the equatorial pitch angle diffusion coefficients for protons (X. Yu et al, 2020). As denoted by two green horizontal lines in Figure 2, within the anisotropic zone the intersected footprint of the RBSP‐A and NOAA 16 corresponds to about L = 5.78.…”
Section: Discussion and Resultsmentioning
confidence: 99%
“…To further demonstrate that the observed MS waves can cause flux enhancements of mirroring ring current ions, following the analytical approximation in Bortnik et al (2015) which can capture the main results of test particle simulations but take a computation time about 4 order of magnitude faster than the latter, we calculate the equatorial pitch angle diffusion coefficients for protons (X. Yu et al, 2020). As denoted by two green horizontal lines in Figure 2, within the anisotropic zone the intersected footprint of the RBSP‐A and NOAA 16 corresponds to about L = 5.78.…”
Section: Discussion and Resultsmentioning
confidence: 99%
“…For each fitting process, the high determine coefficient of R 2 shows the accuracy of our model. In the future, we will study the effect of MS wave in dynamic evolution of the radiation belts and ring current protons based on this model, including transit‐time scattering on particles (Bortnik et al, 2015; Yu et al, 2020).…”
Section: Discussionmentioning
confidence: 99%
“…Additionally, MS waves have a wide MLT coverage and can exist both inside and outside the plasmapause. Some previous works have put forward that MS wave plays a role in accelerating electrons from keVs to MeVs via Landau resonance (Horne et al, 2000, 2007; Ni et al, 2018; Shprits, 2016; Shprits et al, 2013; Yu et al, 2020), as well as in scattering ring current ions (Fu et al, 2016; Yu et al, 2019; Yuan et al, 2020). Therefore, MS waves become an essential part in the inner magnetospheric kinetic process.…”
Section: Introductionmentioning
confidence: 99%
“…According to the quasilinear theory, MS waves are considered to play an important role in the dynamic evolution of the radiation belt electrons (Fu et al, 2019;Horne et al, 2007;Li et al, 2016;Xiao et al, 2015;J. Yu et al, 2019;X. Yu et al, 2020).…”
Section: Introductionmentioning
confidence: 99%