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Lightning-driven electric and magnetic fields measured in the stratosphere: Implications for sprites.

机译:在平流层中测量的闪电驱动的电场和磁场:对子画面的影响。

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A well accepted model for sprite production involves quasi-electrostatic fields (QSF) driven by large positive cloud-to-ground (+CG) strokes that can cause electrical breakdown in the middle atmosphere. A new high voltage, high impedance, double Langmuir probe instrument is designed specifically for measuring these large lightning-driven electric field changes at altitudes above 30 km. This High Voltage (HV) Electric Field Detector measured 200 nearby (75 km) lightning-driven electric field changes, up to 140 V/m in magnitude, during the Brazil Sprite Balloon Campaign 2002--03.; A numerical QSF model is developed and compared to the in situ measurements. It is found that the amplitudes and relaxation times of the electric fields driven by these nearby lightning events generally agree with the numerical QSF model, which suggests that the QSF approach is valid for modeling lightning-driven fields. Using the best fit parameters of this comparison, it is predicted that the electric fields at sprite altitudes (60--90 km) never surpass conventional breakdown in the mesosphere for each of these 200 nearby lightning events.; Lightning-driven ELF to VLF (25 Hz--8 kHz) electric field changes were measured for each of the 2467 cloud-to-ground lightning (CGs) detected by the Brazilian Integrated Lightning Network (BIN) at distances of 75--600 km, and magnetic field changes (300 Hz--8 kHz) above the background noise were measured for about 35% (858) of these CGs. ELF pulses that occur 4--12 ms after the retarded time of the lightning sferic, which have been previously attributed to sprites, were found for 1.4% of 934 CGs examined with a strong bias towards +CGs (4.9% or 9/184) compared to -CGs (0.5% or 4/750). These results disagree with results from the Sprites99 Balloon Campaign [Bering et al., 2004b], in which the lightning-driven electric and magnetic field changes were rare, while the CG delayed ELF pulses were frequent. The Brazil Campaign results thus suggest that mesospheric currents are likely the result of the QSF driven by large charge moment strokes, which are usually +CG strokes, initiating breakdown in the middle atmosphere.
机译:一个广为接受的精灵生成模型涉及准静电场(QSF),它由大的正向云对地(+ CG)笔划驱动,可能导致中间大气中的电击穿。新型高电压,高阻抗双Langmuir探头仪器专门设计用于测量海拔30 km以上的这些大的雷电驱动的电场变化。该高压(HV)电场探测器在2002--03巴西雪碧气球运动期间,测量了200个附近(<75 km)由雷电驱动的电场变化,幅度最高为140 V / m。开发了一个数字QSF模型并将其与现场测量结果进行比较。发现由这些附近的雷电事件驱动的电场的振幅和弛豫时间通常与数值QSF模型一致,这表明QSF方法对于模拟雷电驱动的电场是有效的。使用该比较的最佳拟合参数,可以预测,对于这200个附近的闪电事件中的每一个,在子午线高度(60--90 km)的电场都不会超过中层常规击穿。对巴西综合闪电网络(BIN)在75--600距离处检测到的2467个云对地闪电(CG)中的每一个,测量了闪电驱动的ELF到VLF(25 Hz--8 kHz)电场的变化对于这些CG的约35%(858),测量了高于背景噪音的磁场变化(300 Hz--8 kHz)。在闪电干扰的延迟时间后的4--12毫秒内发生的ELF脉冲被发现是先前归因于子画面的,占被检查的934个CG的1.4%,对+ CG的偏向性强(4.9%或9/184)相较于-CG(0.5%或4/750)。这些结果与Sprites99气球运动[Bering等人,2004b]的结果不同,在该运动中,闪电驱动的电场和磁场变化很少,而CG延迟的ELF脉冲却很频繁。因此,“巴西战役”的结果表明,中层电流很可能是QSF的结果,该QSF是由较大的充电力矩冲程(通常为+ CG冲程)驱动的,从而在中层大气中引起击穿。

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