Development and field testing of a UHF antenna system for the observation of electrical discharge phenomena in the atmosphere

IF 1.9 4区 地球科学 Q3 GEOCHEMISTRY & GEOPHYSICS
Nobuaki Shimoji , Itsuki Tofuku
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引用次数: 0

Abstract

In Japan, the digital terrestrial television broadcasting band (470–710 MHz) is legally protected, resulting in extremely low levels of artificial electromagnetic noise within this frequency range. Therefore, when an antenna is directed toward targets such as cumulus clouds, high-voltage transmission towers, volcanic plumes, or trees, the received signals are highly likely to be ultra high frequency (UHF) event signals—discharge emissions—from those targets. Because discharge phenomena last only tens of nanoseconds, developing instruments capable of directly recording them is technically difficult. Considering Japan’s radio-wave environment and practical hardware constraints, we developed a UHF antenna system with a 0.4ms sampling interval. A dual-integration system was devised and implemented in the backend, enabling continuous recording with no dead time.
Although a 0.4ms interval is long relative to discharge timescales, it becomes a practical method when the objective is not to resolve individual pulses but to detect the collective occurrence of numerous discharge events. The developed system was installed outdoors, and tests confirmed reception of both discharge signals and television broadcasts. Subsequent observations included cumulus clouds, partial discharges from high-voltage transmission towers, small-scale volcanic eruptions, and tree corona discharges. For each target, characteristics consistent with streamers, corona discharges, or partial discharges were obtained. These results suggest that, although improvements are still possible, the compact UHF antenna system developed in this study has the potential to serve as a new observational method for atmospheric discharge phenomena.
用于观测大气中放电现象的超高频天线系统的研制和现场试验
在日本,数字地面电视广播频段(470-710兆赫)受到法律保护,因此在该频率范围内的人工电磁噪声水平极低。因此,当天线指向诸如积云、高压输电塔、火山烟柱或树木等目标时,接收到的信号极有可能是来自这些目标的超高频(UHF)事件信号——放电发射。由于放电现象仅持续几十纳秒,开发能够直接记录它们的仪器在技术上是困难的。考虑到日本的无线电波环境和实际硬件限制,我们开发了一种采样间隔为0.4ms的UHF天线系统。后端设计并实现双集成系统,实现连续录制,无死区。虽然相对于放电时间尺度而言,0.4ms的时间间隔很长,但当目标不是解析单个脉冲而是检测大量放电事件的集体发生时,它就成为一种实用的方法。开发的系统安装在室外,测试证实了放电信号和电视广播的接收。随后的观测包括积云、高压输电塔的局部放电、小规模火山喷发和树木电晕放电。对于每个目标,获得了与流光、电晕放电或部分放电相一致的特征。这些结果表明,尽管仍有改进的可能,但本研究开发的紧凑型超高频天线系统有可能作为一种新的大气放电现象观测方法。
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来源期刊
Journal of Atmospheric and Solar-Terrestrial Physics
Journal of Atmospheric and Solar-Terrestrial Physics 地学-地球化学与地球物理
CiteScore
4.10
自引率
5.30%
发文量
95
审稿时长
6 months
期刊介绍: The Journal of Atmospheric and Solar-Terrestrial Physics (JASTP) is an international journal concerned with the inter-disciplinary science of the Earth''s atmospheric and space environment, especially the highly varied and highly variable physical phenomena that occur in this natural laboratory and the processes that couple them. The journal covers the physical processes operating in the troposphere, stratosphere, mesosphere, thermosphere, ionosphere, magnetosphere, the Sun, interplanetary medium, and heliosphere. Phenomena occurring in other "spheres", solar influences on climate, and supporting laboratory measurements are also considered. The journal deals especially with the coupling between the different regions. Solar flares, coronal mass ejections, and other energetic events on the Sun create interesting and important perturbations in the near-Earth space environment. The physics of such "space weather" is central to the Journal of Atmospheric and Solar-Terrestrial Physics and the journal welcomes papers that lead in the direction of a predictive understanding of the coupled system. Regarding the upper atmosphere, the subjects of aeronomy, geomagnetism and geoelectricity, auroral phenomena, radio wave propagation, and plasma instabilities, are examples within the broad field of solar-terrestrial physics which emphasise the energy exchange between the solar wind, the magnetospheric and ionospheric plasmas, and the neutral gas. In the lower atmosphere, topics covered range from mesoscale to global scale dynamics, to atmospheric electricity, lightning and its effects, and to anthropogenic changes.
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