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首页> 外文期刊>Journal of Geophysical Research, A. Space Physics: JGR >DEMETER observations of bursty MF emissions and their relation to ground-level auroral MF burst
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DEMETER observations of bursty MF emissions and their relation to ground-level auroral MF burst

机译:得墨忒耳的观察丛发性排放和曼氏金融他们与地面极光MF破裂

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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:中频的调查(MF)电场从选择的轨道检测数据电磁排放从地震(得墨忒耳)飞船显示68一种新型丛发性的例子MF排放高纬度地区与发生极光现象。破裂,一个自然的射电辐射观测地面附近的当地的亚暴发作。曼氏金融破裂,丛发性MF海浪观测到得墨忒耳有宽带,冲动的频率结构覆盖1.5 - -3.0 MHz的振幅50 - 100μV / m ~ 0.76%的总体发生率出现较高的活跃时期强烈的相关性和极光嘶嘶声。磁波曼氏金融的当地时间分布观察到得墨忒耳显示出现率峰值有点早于18 MLT附近等价的在地面MF的发生率达到顶峰破裂,但传播效果和差异在取样的纬度的两种技术也许可以解释这种差异。风和SuperMAG数据显示,虽然丛发性MF波浪观测到得墨忒耳与增强的极光活动有关,他们的巧合与亚暴发作不得精确的地面MF破裂。结合发生在曼氏金融破裂观察在马尼托巴省丘吉尔,在曼氏金融的8分钟电场线排放检测到得墨忒耳丘吉尔东南大约1000公里处。这些观察结果可信的可能是相关的用同样的极光事件探测到地面水平磁力计在几个加拿大人天文台。证据表明,丛发性的平衡波曼氏金融观察和得墨忒耳都是相同的现象的地面MF破裂。曼氏金融理论生成的电离层,比如beam-generated朗缪尔波兴奋在一系列高度或强朗缪尔湍流产生的频率在一个狭窄的高度范围内,所需要的要重新审视是否他们预测现场检测MF破裂。

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