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On the spatial and temporal distribution of global thunderstorm cells

机译:全球雷暴单元的时空分布

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Estimates of global thunderstorm activity have been made predominately by direct measurements of lightning discharges around the globe, either by optical measurements from satellites, or using ground-based radio antennas. In this paper we propose a new methodology in which thunderstorm clusters are constructed based on the lightning strokes detected by the World Wide Lightning Location Network (WWLLN) in the very low frequency range. We find that even with low lightning detection efficiency on a global scale, the spatial and temporal distribution of global thunderstorm cells is well reproduced. This is validated by comparing the global diurnal variations of the thunderstorm cells, and the currents produced by these storms, with the well-known Carnegie Curve, which represents the mean diurnal variability of the global atmospheric electric circuit, driven by thunderstorm activity. While the Carnegie Curve agrees well with our diurnal thunderstorm cluster variations, there is little agreement between the Carnegie Curve and the diurnal variation in the number of lightning strokes detected by the WWLLN. When multiplying the number of clusters we detect by the mean thunderstorm conduction current for land and ocean thunderstorms (Mach et al 2011 J. Geophys. Res. 116 D05201) we get a total average current of about 760 A. Our results show that thunderstorms alone explain more than 90% in the variability of the global electric circuit. However, while it has been previously shown that 90% of the global lightning occurs over continental landmasses, we show that around 50% of the thunderstorms are over the oceans, and from 00-09UTC there are more thunderstorm cells globally over the oceans than over the continents. Since the detection efficiency of the WWLLN system has increased over time, we estimate that the lower bound of the mean number of global thunderstorm cells in 2012 was around 1050 per hour, varying from around 840 at 03UTC to 1150 storms at 19UTC.
机译:对全球雷暴活动的估算主要是通过对卫星周围的雷电测量或使用地面无线电天线直接测量全球各地的雷电来进行的。在本文中,我们提出了一种新的方法,其中基于由全球闪电定位网络(WWLLN)在非常低的频率范围内检测到的雷击来构建雷暴簇。我们发现,即使在全球范围内,雷电探测效率较低,也可以很好地再现全球雷暴单元的时空分布。通过将雷暴电池的全球日变化以及这些风暴产生的电流与著名的卡内基曲线进行比较,可以证明这一点,卡内基曲线代表由雷暴活动驱动的全球大气电路的平均日变化。卡内基曲线与我们的日间雷暴群集变化非常吻合,但卡内基曲线与WWLLN探测到的雷击次数的日变化之间几乎没有一致性。将我们检测到的簇数乘以陆地和海洋雷暴的平均雷暴传导电流(Mach等,2011 J. Geophys。Res。116 D05201),我们得到的平均总电流约为760A。我们的结果表明,仅雷暴解释全球电路可变性的90%以上。但是,虽然先前已经证明全球90%的闪电发生在大陆陆地上,但我们显示大约有50%的雷暴发生在海洋上,并且从00-09UTC以来,全球海洋上的雷暴单元数量超过了大洲。由于WWLLN系统的检测效率随着时间的推移而提高,我们估计2012年全球雷暴平均数量的下限约为每小时1050个,范围从03UTC的约840个到19UTC的1150个。

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