首页> 外文学位 >Numerical modeling of lightning initiation and stepped leader propagation.
【24h】

Numerical modeling of lightning initiation and stepped leader propagation.

机译:闪电引发和引导者阶跃传播的数值模型。

获取原文
获取原文并翻译 | 示例

摘要

Initial breakdown pulses (IBPs) observed at the beginning of cloud-to-ground (CG) lightning flashes and stepped leaders that followed IBPs were modeled using multi-sensor electric field change (E-change) measurements. This study uses data collected with a network of ten E-change sensors located at Kennedy Space Center.;Locations (x,y,z,t) of IBPs were found using a time-of-arrival technique called PBFA. Location errors were determined from Monte Carlo simulations and were usually less than 100 m for horizontal coordinates and several hundreds of meters for altitude. Comparison of PBFA source locations to locations from a VHF lightning mapping system shows that PBFA locates most of the `classic' IBPs while the VHF system locates only a few percent of them. As the flash develops during the IB stage, PBFA and the VHF system obtain similar locations when they detect the same IBPs. PBFA also can reliably locate the IBPs of intra-cloud flashes and return stroke (RS) locations.;PBFA locations were used as constraints to model six 'classic' IBPs using three modified transmission line (MTL) models (MTLL--linearly decaying current, MTLE---exponentially decaying current, MTLEI---exponentially increasing current) from the literature and a new model, MTLK, with the current following the Kumaraswami distribution. All four models did a good job of modeling all six IBPs; the MTLE model was most often the best fit. It is important to note that for a given pulse, there is good agreement between the different models on a number of parameters: current risetime, current falltime, two current shape factors, current propagation speed, and the IBP charge moment change. Ranges and mean values of physical quantities found are: current risetime [4.8--25, (13+/-6)] microseconds, current falltime [15--37, (25+/-6)] microseconds, current speed [0.78--1.8, (1.3+/-0.3)]x10 8 m/s (excluding one extreme case of MTLEI), channel length [0.20--1.6, (0.6+/-0.3)] km, charge moment [0.015--0.30, (0.12+/-0.10)] C km, peak current [16--404, (80+/-80)] kA , and absolute average line charge density [0.11--4.7, (0.90+/-0.90)] mC/m. Currents in the MTLL and MTLE models deposit negative charge along their paths and the mean total charges deposited (Qtot) were -0.35 and -0.71 C. MTLEI currents effectively deposited positive charge along their paths with Qtot = 1.3 C. MTLK is more special regarding how it handles the charges. Initially, along the lower current path, negative charge is deposited and positive charge is deposited onto its upper path making the overall charge transfer almost zero, (Qtot = 3.8x10 -5). Because of this the MTLK model apparently obeys conservation of charge (without making that a model constraint).;Two stepped leaders were modeled to match multiple E-change measurements. Time evolution and 2-D locations of stepped leaders were obtained from data collected with a high-speed video camera operated at 50,000 frames/s. The Lu et al. 2011 TDMD (time dependent multidipole) model was used with some modifications. Negative charges were deposited at stepped leader tips based on measured light intensity, and positive charges were deposited at PBFA/LDAR2 locations of IBPs where the stepped leaders probably started. The method has unique advantage of obtaining locations of CG stepped leaders including its branches, unlike previous studies that used simpler paths. Some physical quantities calculated for both stepped leaders: average line charge density = -1.49 and -0.813 mC/m, average current = 0.39 and 0.38 kA, average 2-D stepped leader speed 2.67 and 4.8x105 m/s. These quantities are in excellent agreement with previous studies.
机译:使用多传感器电场变化(E-change)测量对在云对地(CG)闪电开始时观察到的初始击穿脉冲(IBP)和跟随IBP的阶梯状前导进行建模。这项研究使用的数据是由位于肯尼迪航天中心的十个电子变化传感器网络收集的; IBP的位置(x,y,z,t)是使用称为PBFA的到达时间技术找到的。位置误差是根据蒙特卡洛模拟确定的,水平坐标通常小于100 m,海拔高度通常为数百米。将PBFA源位置与VHF闪电测绘系统的位置进行比较,可以发现PBFA可以找到大多数“经典” IBP,而VHF系统只能找到其中的百分之几。随着闪光灯在IB阶段的发展,PBFA和VHF系统在检测到相同的IBP时会获得相似的位置。 PBFA还可以可靠地定位云内闪烁的IBP和回程(RS)位置; PBFA位置被用作约束,使用三个修改的传输线(MTL)模型(MTLL-线性衰减电流)对六个``经典''IBP进行建模,从文献和新模型MTLK得出的MTLE-指数衰减电流,MTLEI-指数增加电流,电流遵循Kumaraswami分布。所有四个模型都很好地为所有六个IBP建模。 MTLE模型通常最适合。重要的是要注意,对于给定的脉冲,不同模型之间在许多参数上具有良好的一致性:电流上升时间,电流下降时间,两个电流形状因子,电流传播速度和IBP充电力矩变化。找到的物理量的范围和平均值是:当前上升时间[4.8--25,(13 +/- 6)]微秒,当前下降时间[15--37,(25 +/- 6)]微秒,当前速度[0.78 --1.8,(1.3 +/- 0.3)] x10 8 m / s(不包括MTLEI的一种极端情况),通道长度[0.20--1.6,(0.6 +/- 0.3)] km,充电力矩[0.015-- 0.30,(0.12 +/- 0.10)] km,峰值电流[16--404,(80 +/- 80)] kA,绝对平均线电荷密度[0.11--4.7,(0.90 +/- 0.90) ] mC / m。 MTLL和MTLE模型中的电流沿其路径沉积负电荷,平均沉积总电荷(Qtot)为-0.35和-0.71C。MTLEI电流沿Qtot = 1.3 C沿其路径有效沉积正电荷。MTLK在以下方面更为特殊它如何处理费用。最初,沿着较低的电流路径,会沉积负电荷,而将正电荷沉积到其较高的路径上,从而使总电荷转移几乎为零(Qtot = 3.8x10 -5)。因此,MTLK模型显然服从于电荷守恒(没有产生模型约束)。对两个阶梯状领导者进行建模以匹配多个E变化测量。从以50,000帧/秒的速度运行的高速摄像机收集的数据获得阶梯状领导者的时间演化和二维位置。卢等。使用2011 TDMD(时间相关的多偶极子)模型进行了一些修改。负电荷会根据测得的光强度沉积在阶梯状前导尖端处,而正电荷会沉积在可能开始阶梯状前导的IBP的PBFA / LDAR2位置。该方法具有获得CG阶梯状领导者及其分支的位置的独特优势,这与以前使用简单路径的研究不同。为这两个阶梯状引线计算的一些物理量:平均线电荷密度= -1.49和-0.813 mC / m,平均电流= 0.39和0.38 kA,平均二维阶梯状引线速度2.67和4.8x105 m / s。这些数量与以前的研究非常吻合。

著录项

  • 作者

    Karunarathne, Sumedhe.;

  • 作者单位

    The University of Mississippi.;

  • 授予单位 The University of Mississippi.;
  • 学科 Atmospheric sciences.;Electromagnetics.;Physics.
  • 学位 Ph.D.
  • 年度 2013
  • 页码 198 p.
  • 总页数 198
  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类
  • 关键词

相似文献

  • 外文文献
  • 中文文献
  • 专利
获取原文

客服邮箱:kefu@zhangqiaokeyan.com

京公网安备:11010802029741号 ICP备案号:京ICP备15016152号-6 六维联合信息科技 (北京) 有限公司©版权所有
  • 客服微信

  • 服务号