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首页> 外文期刊>Journal of Geophysical Research, A. Space Physics: JGR >Survey of the frequency dependent latitudinal distribution of the fast magnetosonic wave mode from Van Allen Probes Electric and Magnetic Field Instrument and Integrated Science waveform receiver plasma wave analysis
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Survey of the frequency dependent latitudinal distribution of the fast magnetosonic wave mode from Van Allen Probes Electric and Magnetic Field Instrument and Integrated Science waveform receiver plasma wave analysis

机译:Van Allen Probes电磁场仪器和Integrated Science波形接收器等离子体波分析对快速磁声波模式的频率依赖性纬度分布进行调查

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摘要

We present a statistical survey of the latitudinal structure of the fast magnetosonic wave mode detected by the Van Allen Probes spanning the time interval of 21 September 2012 to 1 August 2014. We show that statistically, the latitudinal occurrence of the wave frequency (f) normalized by the local proton cyclotron frequency (f_(cP)) has a distinct funnel-shaped appearance in latitude about the magnetic equator similar to that found in case studies. By comparing the observed E/B ratios with themodel E/B ratio, using the observed plasma density and background magnetic field magnitude as input to the model E/B ratio, we show that this mode is consistent with the extra-ordinary (whistler) mode at wave normal angles (θ_k) near 90°. Performing polarization analysis on synthetic waveforms composed from a superposition of extra-ordinary mode plane waves with θ_k randomly chosen between 87 and 90°, we show that the uncertainty in the derived wave normal is substantially broadened, with a tail extending down to θ_k of 60°, suggesting that another approach is necessary to estimate the true distribution of θ_k. We find that the histograms of the synthetically derived ellipticities and θ_k are consistent with the observations of ellipticities and θ_k derived using polarization analysis.Wemake estimates of the median equatorial θ_k by comparing observed and model ray tracing frequency-dependent probability occurrence with latitude and give preliminary frequency dependent estimates of the equatorial θ_k distribution around noon and 4 R_E, with themedian of~4 to 7° from 90° at f/f_(cP) = 2 and dropping to ~0.5° from 90° at f/f_(cP)=30. The occurrence of waves in this mode peaks around noon near the equator at all radial distances, and we find that the overall intensity of these waves increases with AE*, similar to findings of other studies.
机译:我们对Van Allen探针在2012年9月21日至2014年8月1日期间的时间间隔内检测到的快速磁声波模式的纬度结构进行了统计调查。从统计上看,波频率(f)的纬度出现已标准化通过局部质子回旋加速器频率(f_(cP))得出的磁赤道在纬度上具有明显的漏斗状外观,与案例研究相似。通过将观察到的E / B比值与模型E / B比值进行比较,使用观察到的血浆密度和背景磁场强度作为模型E / B比值的输入,我们表明该模式与非常规(吹口哨)模式一致在波法向角(θ_k)接近90°时的模式。对由在87和90°之间随机选择的θ_k的非常规模式平面波的叠加所组成的合成波形进行极化分析,我们表明,导出波法线的不确定性大大加宽,尾部向下延伸至θ_k为60 °,表明需要另一种方法来估计θ_k的真实分布。我们发现合成导出的椭圆度和θ_k的直方图与使用偏振分析得出的椭圆率和θ_k的观测值一致。赤道θ_k分布在中午和4 R_E附近的频率相关估计,主旋律从f / f_(cP)处的90°约4至7°,在f / f_(cP)处从90°下降至约0.5° = 30。在所有径向距离上,这种模式的波的出现在中午附近的赤道附近达到峰值,我们发现这些波的总强度随AE *的增加而增加,类似于其他研究的结果。

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