Wisp-Like Energy Spectrum of Precipitating Electrons Observed by DEMETER Satellite

IF 2.9 2区 地球科学 Q2 ASTRONOMY & ASTROPHYSICS
Jingle Hu, Binbin Ni, Yangxizi Liu, Junhu Dong, Jianhang Wang, Haozhi Guo, Jiakun Dai, Zheng Xiang
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Abstract

Very-low-frequency (VLF) signals used for submarine communication can penetrate the ionosphere and leak into the magnetosphere. These signals interact with hundreds of keV electrons in the inner magnetosphere through cyclotron resonance, resulting in pitch angle diffusion of trapped electrons. The energy-L spectrum of quasi-trapped electrons (in the drift loss cone scattered by North West Cape (NWC) transmitted signals in the inner radiation belt is called “wisp,” characterized by narrow spectral peaks of enhanced fluxes. These quasi-trapped electrons drift eastward and can be clearly observed by Low-Earth-Orbit satellites until they precipitate into the South Atlantic Anomaly (SAA) region, where they drift into the bounce loss cone (BLC). The transmitter-induced BLC precipitation with a wisp structure has been considered uncommon. In this study, we report the direct and clear observational evidence of transmitter-induced precipitating wisps which are commonly observed at the edge of the northern hemisphere precipitation regions (the regions conjugated to the SAA). Moreover, we systematically analyze the dependence of these electron fluxes on L-shell, electron energies and geomagnetic activities, using long-term measurements from the DEMETER satellite. The intensities and positions of the precipitating wisps in the energy-L spectrum are highly correlated with the quasi-trapped wisps. The visible wisp structure in the precipitating electrons can only be detected when the quasi-trapped electron fluxes exceed a certain threshold ∼103 cm−2ster−1s−1 MeV−1. The overall variation in precipitating electron fluxes follows the trend observed in trapped electron fluxes. These results provide new insights into the quantitative scattering effects of NWC transmitter signals on energetic electrons.

Abstract Image

DEMETER卫星观测到的缕缕状沉淀电子能谱
用于海底通信的甚低频(VLF)信号可以穿透电离层并泄漏到磁层。这些信号通过回旋共振与内部磁层中的数百个keV电子相互作用,导致被困电子的俯角扩散。内辐射带中被西北开普(NWC)发射信号散射的漂移损失锥中的准捕获电子的能量l谱称为“小束”,其特征是谱峰窄,通量增强。这些准捕获电子向东漂移,低地球轨道卫星可以清楚地观察到,直到它们沉淀到南大西洋异常区(SAA),在那里它们漂移到反弹损失锥(BLC)。具有束状结构的发射机诱导的BLC降水被认为是罕见的。在这项研究中,我们报告了在北半球降水区边缘(与SAA共轭的区域)通常观测到的发射机诱导的降水缕的直接和明确的观测证据。此外,我们利用DEMETER卫星的长期测量数据,系统地分析了这些电子通量与l -壳层、电子能量和地磁活动的关系。在能量l谱中,沉淀束的强度和位置与准捕获束高度相关。只有当准捕获电子通量超过一定阈值~ 103 cm−2ster−1s−1 MeV−1时,才能探测到沉淀电子中可见的束状结构。沉淀电子通量的总体变化遵循捕获电子通量观察到的趋势。这些结果为NWC发射机信号对高能电子的定量散射效应提供了新的见解。
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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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