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首页> 外文期刊>Journal of Geophysical Research, A. Space Physics: JGR >ELF/VLF wave propagation at subauroral latitudes: Conjugate observation between the ground and Van Allen Probes A
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ELF/VLF wave propagation at subauroral latitudes: Conjugate observation between the ground and Van Allen Probes A

机译:极耳下纬度的ELF / VLF波传播:地面与Van Allen探针A的共轭观测

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摘要

We report simultaneous observation of ELF/VLF emissions, showing similar spectral and frequency features, between a VLF receiver at Athabasca (ATH), Canada, (L = 4.3) and Van Allen Probes A (Radiation Belt Storm Probes (RBSP) A). Using a statistical database from 1 November 2012 to 31 October 2013, we compared a total of 347 emissions observed on the ground with observations made by RBSP in the magnetosphere. On 25 February 2013, from 12:46 to 13:39 UT in the dawn sector (04–06 magnetic local time (MLT)), we observed a quasiperiodic (QP) emission centered at 4 kHz, and an accompanying short pulse lasting less than a second at 4.8 kHz in the dawn sector (04–06 MLT). RBSP A wave data showed both emissions as right-hand polarized with their Poynting vector earthward to the Northern Hemisphere. Using cross-correlation analysis, we did, for the first time, time delay analysis of a conjugate ELF/VLF event between ground and space, finding +2 to +4 s (ATH first) for the QP and ?3 s (RBSP A first) for the pulse. Using backward tracing from ATH to the geomagnetic equator and forward tracing from the equator to RBSP A, based on plasmaspheric density observed by the spacecraft, we validate a possible propagation path for the QP emission which is consistent with the observed time delay.
机译:我们报告了加拿大Athabasca(ATH)的VLF接收器(L = 4.3)与Van Allen探头A(辐射带风暴探头(RBSP)A)之间同时观察到的ELF / VLF发射,显示出相似的频谱和频率特征。使用2012年11月1日至2013年10月31日的统计数据库,我们将地面上观测到的总共347种排放与RBSP在磁层的观测值进行了比较。 2013年2月25日,在黎明时区(04–06磁性当地时间(MLT))的UT,从12:46到13:39,我们观察到以4 kHz为中心的准周期(QP)发射,伴随的短脉冲持续时间更短比黎明扇区(04-06 MLT)的4.8 kHz高一秒。 RBSP的波浪数据显示,两种辐射都是右旋极化的,与它们的Poynting矢量向地球偏向北半球。使用互相关分析,我们首次对地面与空间之间的共轭ELF / VLF事件进行了时延分析,发现QP和+3 s(RBSP A)为+2到+4 s(ATH优先)首先)为脉冲。基于航天器观测到的等离子层密度,使用从ATH到地磁赤道的反向跟踪以及从赤道到RBSP A的反向跟踪,我们验证了QP发射的可能传播路径,该路径与观察到的时延一致。

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