Influence of Initial Proton Energy on the Nonlinear Interactions Between Ring Current Protons and He+ Band EMIC Waves

IF 2.6 2区 地球科学 Q2 ASTRONOMY & ASTROPHYSICS
Su Zhou, Yongzhi Cai
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Abstract

The energy of ring current protons is believed to influence the pitch angle scattering due to electromagnetic ion cyclotron (EMIC) waves and is typically analyzed using quasi-linear theory. However, nonlinear behavior becomes significant as the wave amplitude intensifies. In this study, we aim to explore how the nonlinear behavior depends on the initial proton energy under various background plasma density conditions. The frequency of EMIC waves is 0.96ΩHe (where ΩHe is the gyrofrequency of He+ at the equator). It is found that the higher energy protons with nonlinear phase trapping experience more resonances, causing these trapped protons to move away from the loss cone more quickly compared to lower energy protons. However, the proportion of phase-trapped protons significantly decreases as the initial proton energy increases. This declining trend is more pronounced for a background plasma condition in the plasmapause than within the plasmasphere. The number of phase-trapped protons goes to zero as initial proton energy increases to above approximately 60 keV. Additionally, nonlinear phase bunching is more pronounced for lower energy protons (e.g., below 60 keV) compared to higher energy protons. As a result, both nonlinear phase trapping and phase bunching contribute to larger standard deviations in the net changes of equatorial pitch angle (Δαeq), suggesting a larger pitch agnel diffusion coefficient compared to the prediction of quasi-linear theory.

质子初始能量对环流质子与 He+ 带电磁波之间非线性相互作用的影响
环流质子的能量被认为会影响电磁离子回旋(EMIC)波引起的俯仰角散射,通常使用准线性理论进行分析。然而,随着波幅的增强,非线性行为变得非常重要。在本研究中,我们旨在探索在不同背景等离子体密度条件下,非线性行为如何取决于初始质子能量。EMIC 波的频率为 0.96ΩHe(其中 ΩHe 是 He+ 在赤道的陀螺频率)。研究发现,与低能量质子相比,具有非线性相位捕获的高能量质子会经历更多的共振,导致这些被捕获的质子更快地远离损耗锥。然而,随着质子初始能量的增加,相位捕获质子的比例显著下降。这种下降趋势在质子束的背景等离子体条件下比在质子球内更为明显。当初始质子能量增加到大约 60 keV 以上时,相位捕获质子的数量为零。此外,与能量较高的质子相比,能量较低的质子(例如低于 60 千伏安)的非线性相束缚更为明显。因此,非线性相位捕获和相位束化都会导致赤道俯仰角(Δαeq)净变化的标准偏差增大,这表明与准线性理论的预测相比,俯仰角扩散系数更大。
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来源期刊
Journal of Geophysical Research: Space Physics
Journal of Geophysical Research: Space Physics Earth and Planetary Sciences-Geophysics
CiteScore
5.30
自引率
35.70%
发文量
570
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