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首页> 外文期刊>Journal of Geophysical Research, D. Atmospheres: JGR >Radio frequency radiation beam pattern of lightning return strokes: Inferred from FORTE satellite observations
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Radio frequency radiation beam pattern of lightning return strokes: Inferred from FORTE satellite observations

机译:雷击回程的射频辐射束方向图:从FORTE卫星观测中推断

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The fast propagating return stroke is expected to produce a radiation pattern differing from a dipole pattern, with a “correction” of (1 ? v cos /c)?1 or the so-called F factor. The FORTE satellite measures lightning Very High Frequency (VHF) radiation at different angles from the up space and offers the first opportunity of examining the F factor. In this report, we studied a group of FORTE-detected lightning events that were also observed by the National Lightning Detection Network (NLDN). NLDN provided the discharges' geolocations and helped to identify the discharge types. During the summers of 1998 and 1999, 25,721 coincident events were found. Among these, 2092 were found to be narrow (<100 ns), VHF-intense and highly polarized bursts and were found to be associated with the beginning of return strokes. Through careful statistical analysis regarding the distributions of the event occurrence, we found that the overall ensemble of events can be considered to have an isotropic pattern in the upper half-space. The subset of the narrow bursts displays a beam pattern that agrees with the F factor at a propagating speed of v = 0.75c. The latter is inferred by comparing FORTE observations to a free-space transmission line (TL) model. The analysis shows that the ground does not affect the narrow-burst beam pattern observed from the upper half-space; the source for the narrow burst needs to be a few tens of meters above the surface of the Earth and is apparently associated with the junction point of the attachment process. The physical size of the corresponding discharge is estimated to be less than 20 m. The analysis also suggests that a single upward current is responsible for the observations, rather than a bidirectional current as suggested by others for the attachment process. Similarly, the traveling current source (TCS) model that consists of a simultaneous downward current is found less suitable for the initiation of return strokes.
机译:预期快速传播的返回冲程将产生与偶极子图不同的辐射图,其“校正”为(1?v cos / c)?1或所谓的F因子。 FORTE卫星从高空以不同角度测量闪电甚高频(VHF)辐射,这是第一个研究F因子的机会。在本报告中,我们研究了一组由FORTE检测到的闪电事件,这些事件也被国家闪电检测网络(NLDN)观察到。 NLDN提供了放电的地理位置,并帮助确定了放电类型。在1998年和1999年夏季,发现了25,721起巧合事件。其中,发现2092窄(<100 ns),VHF强烈和高度极化的猝发,并被发现与回程的开始有关。通过对事件发生的分布进行仔细的统计分析,我们发现事件的整体集合可以认为在上半空间具有各向同性模式。窄脉冲串的子集在v = 0.75c的传播速度下显示出与F因子一致的波束方向图。后者是通过将FORTE观测值与自由空间传输线(TL)模型进行比较来推断的。分析表明,地面不会影响从上半空间观察到的窄脉冲光束图;狭窄爆发的源头必须在地球表面上方数十米处,并且显然与附着过程的交汇点有关。相应放电的物理尺寸估计小于20 m。分析还表明,一个向上的电流负责观测,而不是其他人对附着过程建议的双向电流。同样,发现由同时向下的电流组成的行进电流源(TCS)模型不太适合返回行程的启动。

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