地基发射机触发内辐射带电子沉淀:揭开观测和建模结果的神秘面纱

IF 8.3 Q1 GEOSCIENCES, MULTIDISCIPLINARY AGU Advances Pub Date : 2024-11-21 DOI:10.1029/2024AV001354
Zheng Xiang, Xinlin Li, Daniel N. Baker, Yang Mei, Declan O'Brien, Benjamin Hogan, Hong Zhao, David Brennan, Binbin Ni, Theodore Sarris, Michael A. Temerin
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引用次数: 0

摘要

人类活动影响着地球环境,包括地球上空数百至数千公里的空间环境。一个直接证据是,澳大利亚西北角(NWC)发射站发射的 19.8 千赫电磁信号在地球内部辐射带产生了缕状的高能电子沉淀能量分布,许多低地轨道卫星都观测到了这种能量分布。通常情况下,卫星观测到的是一缕能量随 L(约为赤道平面上的径向距离)增大而减小的能量,这是由发射机信号与高能电子的一阶回旋共振产生的。在这里,我们首次报告了最近发射的科罗拉多内辐射带实验(CIRBE)立方体卫星上的相对论电子和质子望远镜集成小实验-2(REPTile-2)观测到的多缕。根据模拟结果,我们证明了高斜度 NWC 发射信号产生的包括 1、-1 和 2 阶在内的谐波回旋共振会产生这些多缕。在太空中同时发生多阶回旋共振的发现,为近地空间的波粒相互作用提供了新的启示。它还对开发人工辐射带补救技术以及了解等离子体波在行星磁层中的传播和散射具有重要意义。
本文章由计算机程序翻译,如有差异,请以英文原文为准。

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Earth-Based Transmitters Trigger Precipitation of Inner Radiation Belt Electrons: Unveiling Observations and Modeling Results

Human activity influence Earth's environment, including the space environment hundreds to thousands of kilometers above the Earth. One direct evidence is that the 19.8 kHz electromagnetic signals launched by the North West Cape (NWC) transmitter station in Australia produce a wisp-like energy distribution of precipitating energetic electrons in Earth's inner radiation belt, observed by many Low Earth Orbiting satellites. Typically, satellites observe a single wisp with energy that decreases with increasing L (approximately the radial distance in the equatorial plane), which is produced by a first-order cyclotron resonance of transmitter signals with energetic electrons. Here we report, for the first time, multiple wisps observed by the Relativistic Electron and Proton Telescope integrated little experiment-2 (REPTile-2) on board the recently launched Colorado Inner Radiation Belt Experiment (CIRBE) CubeSat. Based on simulation results, we demonstrate that harmonic cyclotron resonances including the 1, −1, and 2 orders by highly oblique NWC transmitter signals produce these multiple wisps. The discovery of multiple-order cyclotron resonances simultaneously occurring in space sheds new light on wave-particle interactions in near-Earth space. It also has implications for developing artificial radiation belt remediation techniques and understanding the propagation and scattering of plasma waves in planetary magnetospheres.

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