通过 RAM-SCB 模拟量化 2014 年 2 月 27 日风暴期间电磁波散射的作用

IF 2.6 2区 地球科学 Q2 ASTRONOMY & ASTROPHYSICS Journal of Geophysical Research: Space Physics Pub Date : 2024-07-17 DOI:10.1029/2024JA032606
Xingzhi Lyu, Vania K. Jordanova, Miles Engel, Weichao Tu, Qianli Ma
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引用次数: 0

摘要

电磁离子回旋加速器(EMIC)波散射已被证明是造成辐射带(RB)电子和环流(RC)质子快速损耗的原因。然而,它在这两个共定位种群的同时衰减中所起的作用仍有待量化。在这项工作中,我们采用基于全球物理学的 RAM-SCB 模型,研究了 2014 年 2 月 27 日风暴期间电磁波散射对这两个种群的影响。在整个风暴事件中,MeV RB 电子和 100s keV RC 质子在强烈的 EMIC 波发生后同时发生了衰减。通过实施数据驱动的初始条件和边界条件,我们对这两个种群与 EMIC 波的相互作用进行了模拟,并与范艾伦探测器的观测结果进行了比较。结果表明,通过加入电磁波散射损耗,特别是氦波段电磁波的散射损耗,模型与两个种群的数据非常吻合。此外,我们还研究了两个星群的模拟俯仰角分布(PADs)。在我们的模型中加入 EMIC 波散射,可以预测电子的 PAD 为 90° 峰值,在较低俯仰角时损耗更强,而质子的 PAD 为各向同性,在 40° 以上俯仰角时损耗更强。此外,根据我们的模型预测,在风暴的主要阶段,这两种粒子群都会出现大量降水,主要集中在下午到午夜(12 小时 < MLT < 24 小时),这与电磁波的存在密切相关。
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Quantifying the Role of EMIC Wave Scattering During the 27 February 2014 Storm by RAM-SCB Simulations

Electromagnetic Ion Cyclotron (EMIC) wave scattering has been proved to be responsible for the fast loss of both radiation belt (RB) electrons and ring current (RC) protons. However, its role in the concurrent dropout of these two co-located populations remains to be quantified. In this work, we study the effect of EMIC wave scattering on both populations during the 27 February 2014 storm by employing the global physics-based RAM-SCB model. Throughout this storm event, MeV RB electrons and 100s keV RC protons experienced simultaneous dropout following the occurrence of intense EMIC waves. By implementing data-driven initial and boundary conditions, we perform simulations for both populations through the interplay with EMIC waves and compare them against Van Allen Probes observations. The results indicate that by including EMIC wave scattering loss, especially by the He-band EMIC waves, the model aligns closely with data for both populations. Additionally, we investigate the simulated pitch angle distributions (PADs) for both populations. Including EMIC wave scattering in our model predicts a 90° peaked PAD for electrons with stronger losses at lower pitch angles, while protons exhibit an isotropic PAD with enhanced losses at pitch angles above 40°. Furthermore, our model predicts considerable precipitation of both particle populations, predominantly confined to the afternoon to midnight sector (12 hr < MLT < 24 hr) during the storm's main phase, corresponding closely with the presence of EMIC waves.

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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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