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31.
Observations were carried out at National Astronomy and Ionospheric Center (NAIC) in Puerto Rico with a dual-frequency (46.8MHz/430MHz) Strato-Tropospheric radar associated with ground-based precipitation and electrostatic field measurements. This experimental set-up is devoted to provide wind measurements and detection of clear air turbulence. During a thunderstorm event, VHF-UHF radar receivers detected wide frequency band radiation emitted by lightning flashes. We present in this paper observations of a specific storm for which lightning radiation and ionized lightning channel were fortuitously and simultaneously detected. A bi-level structure of the lightning flash channel is observed and is consistent with observations obtained previously by other authors with VHF lightning mapper. 相似文献
32.
D. Wang N. Takagi T. Watanabe V.A. Rakov M.A. Uman K.J. Rambo M.V. Stapleton 《Atmospheric Research》2005,76(1-4):412
A comparative analysis has been performed of the channel-base current and light waveforms for four rocket-triggered lightning strokes. It has been found that the current and light signals at the bottom of the channel exhibit a linear relationship (direct proportionality) in their rising portions. However, just after the peaks the linearity disappears, and the light signals usually decrease faster than the currents during the next several microseconds. Later, this trend is reversed and in some cases the light signals show another rising trend, even when the currents continue to decrease. The linear light/current relationship for the rising portions of the waveforms appears to be the same for different strokes. The findings support the idea of evaluating the variation of return stroke current along the lightning return stroke channel using light signals, provided that evaluation is limited to the rising portions of those signals and assuming that the light/current relationship observed at the bottom of the channel holds at other heights. 相似文献
33.
Triggered-lightning properties inferred from measured currents and very close electric fields 总被引:1,自引:0,他引:1
V. Kodali V.A. Rakov M.A. Uman K.J. Rambo G.H. Schnetzer J. Schoene J. Jerauld 《Atmospheric Research》2005,76(1-4):355
Triggered-lightning properties, including dart-leader charge density, return-stroke propagation speed, dart-leader electric potential, dart-leader propagation speed, and dart-leader current, inferred from return-stroke current and very close electric field measurements, are presented. Although most of the estimates are based on relatively crude models, they are all generally in good agreement with independent measurements and/or theoretical considerations found in the literature. The results are likely to be applicable to subsequent strokes in natural lightning. 相似文献
34.
用远场辐射场反演云闪放电参数 总被引:2,自引:0,他引:2
用地面电磁场遥感闪电放电参数无论是在实际应用还是理论研究中都具有重要意义。文中基于电流传输线模式 ,提出了一种用单站远场VLF/LF辐射场反演云内放电参数的简便方法。当传输线电流从底部传播到顶部的时间只有几微秒时 ,整个传输线的VLF/LF辐射可以近似成偶极子辐射 ,即远场辐射场与电流的时间变化率和传输线长度的乘积成正比。因此 ,对远场辐射场做时间积分就能获得完整的电流矩波形 (上升沿有所加宽 ) ,而且传输线模式中的重要参数 ,电流从底部传播到顶端经历的时间 ,也可以近似地用辐射场时间积分幅度与辐射场幅度之比来估计。这一方法具有估计云闪双极性大脉冲辐射过程的放电参数的潜力。 相似文献
35.
热带测雨卫星对淮河一次暴雨降水结构与闪电活动的研究 总被引:13,自引:8,他引:13
文中利用热带测雨卫星 (TRMM )搭载的测雨雷达 (PR)、闪电成像仪 (LIS)、GOES卫星红外通道辐射亮温(TBB)对 2 0 0 3年淮河汛期一锋面气旋系统的两个时次的探测结果 ,分析研究了降水结构及闪电活动 ,并与“98.7.2 0”武汉附近地区中尺度强降水的结构和闪电活动进行了比较。GOES的TBB、降水系统中的对流降水与层云降水比例、闪电活动频数随时间的变化均能表征锋面气旋系统的发展。TRMMPR探测结果表明 :冷锋降水狭窄细长 ,且均为强对流降水 (特别在冷锋加强时 ) ;暖锋宽广 ,且为大片层云降水 ,但其中存在面积不等的强对流降水云团 ;与“98.7.2 0”武汉附近地区中尺度强降水垂直结构的比较表明 ,锋面气旋降水的最大降水率出现在近地面 ,而中尺度强降水的最大降水率出现在低空 (3.0~ 3.5km) ,表明两者之间的降水微物理过程存在差别。TRMMLIS探测结果表明 :闪电活动均发生在冷锋的强对流降水云团中 ,暖锋中虽有强对流降水 ,但无闪电活动 ;闪电活动频数高所对应的降水廓线中、上部存在大量的冰相粒子。 相似文献
36.
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38.
液态水含量和冰晶浓度对闪电频数影响的数值模拟研究 总被引:4,自引:1,他引:4
假定在软雹和冰晶碰撞的非感应起电机制为主要的起电机制成立的条件下,数值模拟研究了国际上公认的Fletcher和H—M冰晶产生机制以及云中的液态水含量对雷暴云放电过程(区分了云闪和地闪)的影响。结果表明,随着气压和温度的变化,在两种冰晶产生机制假定下,冰晶浓度分布有很大差异,这直接导致了雷暴云内电活动的差异。液态水含量的增加将使得首次放电时间延迟,同时将引起放电位置的下降和闪电频数的减少。 相似文献
39.
Chandima Gomes Vernon Cooray Mahendra Fernando Raul Montano Upul Sonnadara 《Journal of Atmospheric and Solar》2004,66(18):428
Pulse trains of irregular pulse characteristics and erratic amplitudes are observed in lightning flashes. These are termed “chaotic pulse trains” in this study. The average width of the individual pulses of these pulse trains is in the range of a few microseconds, with the lower limit of individual measurements extending into the sub-microsecond region. The typical pulse separation lies in the range of 2–. The pulse duration shows a consistent distribution with the most probable value at 400–. Chaotic pulse trains occur most often immediately prior to subsequent strokes. However, they occur also a few milliseconds to several tens of milliseconds prior to return strokes and sometimes do not precede return strokes at all. Twenty-six percent of the total subsequent strokes recorded in this study were preceded by chaotic pulse trains. A few of these pulse trains have occurred in a sequence of several tens of millisecond intervals in between return strokes. We have also found them to occur within very intense cloud flashes. These chaotic pulse trains have features that are different from those of other known pulse trains reported in the lightning literature. Hence, they may be caused by a physical process that has not yet been identified. 相似文献
40.
M. B. Baker A. M. Blyth H. J. Christian J. Latham K. L. Miller A. M. Gadian 《Atmospheric Research》1999,51(3-4)
The lightning frequency model developed by Baker et al. [Baker, M.B., Christian, H.J., Latham, J., 1995. A computational study of the relationships linking lightning frequency and other thundercloud parameters, Q. J. R. Meteorol. Soc., 121, 1525–1548] has been refined and extended, in an effort to provide a more realistic framework from which to examine computationally the relationships that might exist between lightning frequency f (which is now being routinely measured from a satellite, using the NASA/MSFC Optical Transient Detector (OTD)) and a variety of cloud physical parameters. Specifically, superior or more comprehensive representations were utilised of: (1) glaciation via the Hallett–Mossop (H–M) process; (2) the updraught structure of the model cloud; (3) the liquid-water-content structure of the model cloud; (4) the role of the reversal temperature Trev in influencing lightning characteristics; (5) the critical breakdown field for lightning initiation; and (6) the electrical characteristics of the ice crystal anvil of the model cloud. Although our extended studies yielded some new insights into the problem, the basic pattern of relationships between f and the other parameters was very close to that reported by Baker et al. (1995). The more elaborate treatment of Trev restricted somewhat the range of conditions under which reverse-polarity lightning could be produced if the cloud glaciated via H–M, but confirmed the earlier conclusion that such lightning would not occur if the glaciation was of the Fletcher type. The computations yielded preliminary support for the hypothesis that satellite measurements of f might be used to determine values of the ice-content of cumulonimbus anvils: a parameter of climatological importance. The successful launch and continuing satisfactory functioning of the OTD [Christian, H.J., Goodman, S., 1992. Global observations of lightning from space, Proc. 9th Int. Conf. on Atmospheric Electricity, St. Petersburg, pp. 316–321; Christian, H.J., Blakesee, R.J., Goodman, S.J., 1992. Lightning imaging sensor (LIS) for the earth observing system. NASA Tech. Memorandum, 4350] make it possible—with a high degree of precision—to measure lightning location, occurrence time and frequency f over extensive areas of the Earth's surface. Measured global distributions of lightning and associated lightning stroke radiance demonstrate that: lightning activity is particularly pronounced over the tropics, much greater over land than over the oceans, and exhibits great seasonal variability; lightning radiance tends to be greater over the oceans, less when lightning activity is high, and greater in the Northern Hemisphere winter than summer. 相似文献