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DEMETER observations of bursty MF emissions and their relation to ground-level auroral MF burst

机译:DEMETER爆发性MF发射的观测及其与地面极光MF爆发的关系

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A survey of medium frequency (MF) electric field data from selected orbits of the Detection of Electro-Magnetic Emissions Transmitted from Earthquakes (DEMETER) spacecraft reveals 68 examples of a new type of bursty MF emissions occurring at high latitudes associated with auroral phenomena. These resemble auroral MF burst, a natural radio emission observed at ground level near local substorm onsets. Similar to MF burst, the bursty MF waves observed by DEMETER have broadband, impulsive frequency structure covering 1.5–3.0 MHz, amplitudes of 50–100 μV/m, an overall occurrence rate of ~0.76% with higher occurrence during active times, and strong correlation with auroral hiss. The magnetic local time distribution of the MF waves observed by DEMETER shows peak occurrence rate near 18 MLT, somewhat earlier than the equivalent peak in the occurrence rate of ground level MF burst, though propagation effects and differences in the latitudes sampled by the two techniques may explain this discrepancy. Analysis of solar wind and SuperMAG data suggests that while the bursty MF waves observed by DEMETER are associated with enhanced auroral activity, their coincidence with substorm onset may not be as exact as that of ground level MF burst. One conjunction occurs in which MF burst is observed at Churchill, Manitoba, within 8 min of MF emissions detected by DEMETER on field lines approximately 1000 km southeast of Churchill. These observations may plausibly be associated with the same auroral event detected by ground level magnetometers at several Canadian observatories. Although it is uncertain, the balance of the evidence suggests that the bursty MF waves observed with DEMETER are the same phenomenon as the ground level MF burst. Hence, theories of MF burst generation in the ionosphere, such as beam-generated Langmuir waves excited over a range of altitudes or strong Langmuir turbulence generating a range of frequencies within a narrow altitude range, need to be revisited to see whether they predict in situ detection of MF burst.
机译:对地震(DEMETER)航天器发射的电磁辐射探测的选定轨道的中频(MF)电场数据的调查揭示了在高纬度发生的与极光现象相关的新型爆裂MF发射的68个例子。这些类似于极光MF爆发,这是在局部亚暴发作附近的地面上观察到的自然无线电发射。与中频脉冲爆发类似,DEMETER观测到的中频脉冲爆发波具有宽带性,脉冲频率结构覆盖1.5–3.0 MHz,振幅为50–100μV/ m,总发生率约为0.76%,在活跃时期发生率更高,并且强度大。与极光嘶嘶声相关。通过DEMETER观测到的MF波的磁局部时间分布显示出峰值发生率在18 MLT附近,比地面水平MF爆发的发生率中的等效峰值稍早一些,尽管这两种技术可能会产生传播效应和纬度差异。解释这种差异。对太阳风和SuperMAG数据的分析表明,尽管由DEMETER观测到的爆发性MF波与增强的极光活动有关,但它们与亚暴爆发的重合可能不如地面MF爆发的精确。一种结合发生时,在DEMETER在丘吉尔东南约1000公里处的野外测线发现的MF排放量的8分钟内,在曼尼托巴省丘吉尔观察到MF爆发。这些观察结果可能与加拿大几座天文台地面磁力计检测到的同一极光事件有关。尽管尚不确定,但证据的平衡表明,用DEMETER观测到的脉冲MF波是与地面MF脉冲相同的现象。因此,需要重新研究电离层中MF爆裂产生的理论,例如在一定高度范围内激发的束产生的朗缪尔波或在狭窄高度范围内产生一定频率范围的强朗缪尔湍流,以查看它们是否就地预测MF突发检测。

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