A Statistical Survey of E-Region Anomalous Electron Heating Using Poker Flat Incoherent Scatter Radar Observations

IF 2.6 2区 地球科学 Q2 ASTRONOMY & ASTROPHYSICS
Yizhe Zhang, Roger H. Varney
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Abstract

This work presents an algorithm for automatic detection of anomalous electron heating (AEH) events in the auroral E-region ionosphere using data from the Poker Flat Incoherent Scatter Radar (PFISR). The algorithm considers both E-region electron temperature and magnetically conjugate electric field measurements. Application of this algorithm to 14 years of PFISR data spanning 2010 through 2023 detected 505 AEH events. Measured electron temperatures increase linearly with plasma drift speeds. Statistical trends of AEH occurrence as a function of space weather indices (AE and F10.7) demonstrate correlations with the solar cycle and geomagnetic activity levels. The magnetic local time occurrence rates show preferences for dusk and dawn with most events in the dusk sector. Observed AEH events tend to appear in regions of relatively low electron density and do not appear inside intense auroral arcs with high electron density. Furthermore, AEH detection requires a higher electric field than predicted by the threshold for a positive growth rate of the Farley-Buneman instability (FBI), according to linear fluid theory. The implications of these findings for kinetic theories of FBI and AEH are discussed.

利用扑克牌平面非相干散射雷达观测数据对 E 区域异常电子加热的统计调查
这项工作提出了一种利用扑克牌平相干散射雷达(PFISR)数据自动检测极光E区电离层异常电子加热(AEH)事件的算法。该算法同时考虑了 E 区电子温度和磁共轭电场测量值。将该算法应用于 2010 年至 2023 年 14 年的 PFISR 数据,共探测到 505 次 AEH 事件。测量到的电子温度与等离子体漂移速度呈线性增长。作为空间天气指数(AE 和 F10.7)函数的 AEH 发生率的统计趋势显示出与太阳周期和地磁活动水平的相关性。磁场局部时间发生率显示出对黄昏和黎明的偏好,大多数事件发生在黄昏区域。观测到的 AEH 事件往往出现在电子密度相对较低的区域,而不会出现在电子密度较高的强烈极光弧内。此外,根据线性流体理论,AEH探测所需的电场比Farley-Buneman不稳定性(FBI)正增长率阈值所预测的要高。讨论了这些发现对FBI和AEH动力学理论的影响。
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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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