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地球磁层中合声波的频率与传播角分布特征

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合声波的频率和传播角是影响其与电子相互作用的关键参数.2013年1月1日至2015年12月31日期间范艾伦卫星数据的统计分析结果表明,在传播角θ≈35°处,较强的合声波(>7×10-4 mV2·m-2·Hz-1)更倾向于出现在更窄的频率范围(0.3~0.4 fce).随着磁壳数L的增大,θ≈35°处的合声波频谱变窄趋势逐渐明显.从夜侧到晨侧(21:00 MLT-09:00 MLT),较强的合声波能够在0.1~0.8 fce的频率范围内被观测到,但夜侧θ≈35°处的合声波频谱宽度比晨侧更窄.从上午到昏侧(09:00 MLT-21:00 MLT),合声波电场功率谱密度明显降低,且主要以斜传播(θ>60°)的下带合声波为主.随着磁纬度λMLAT的增大,上带合声波迅速减弱.同时,θ≈35°处的下带合声波电场功率谱密度也逐渐下降.本文揭示了不同区域内合声波强度的频率和传播角分布特征,为构建更加精确的合声波-电子相互作用全球模型提供了重要信息.
Statistical Study on Propagation Characteristics of Chorus in the Earth's Magnetosphere
The frequency and normal angle of chorus waves are the key parameters affecting its inter-action with electrons.Statistical analysis of Van Allen satellite data from 1 January 2013 to 31 Decem-ber 2015,indicates that the strong chorus waves(>7×10-4 mV2·m-2·Hz-1)tend to appear in a narrower frequency range(0.3~0.4 fce)at normal angle θ around 35°.As L increases,the trend of narrowing cho-rus wave spectrum at θ≈35° becomes more pronounced.From the night to the dawn(21:00 MLT-09:00 MLT),chorus waves can be observed within a frequency range of 0.1~0.8 fce,but the spectral width of chorus waves at θ≈35° on the nightside is narrower than that on the dawn.From the morning to the dusk(09:00 MLT-21:00 MLT),the electric power spectral density of chorus waves decreases significant-ly,mainly manifesting as lower band chorus waves with oblique propagation(θ>60°).With increasing magnetic latitude(λMLAT),the upper band chorus waves diminish rapidly,and the electric power spec-tral density of the lower band chorus waves at θ≈35° also gradually decreases.This study reveals the distribution characteristics of chorus wave intensity in terms of frequency and the normal angle in differ-ent regions,providing crucial information for constructing a more accurate global model of chorus wave-electron interactions.

Radiation beltsVan Allen ProbesStatistical analysisChorusNormal angle

杨立贤、刘斯、高中磊、周亚雄、高阳、王博闻、金宇玥

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长沙理工大学物理与电子科学学院 长沙 410004

辐射带 范艾伦探测器 统计分析 合声波 传播角

2024

空间科学学报
中国科学院空间科学与应用研究中心 中国空间科学学会

空间科学学报

CSTPCD北大核心
影响因子:0.328
ISSN:0254-6124
年,卷(期):2024.44(6)