Evaluating growth rates of sprite streamers

IF 1.9 4区 地球科学 Q3 GEOCHEMISTRY & GEOPHYSICS Journal of Atmospheric and Solar-Terrestrial Physics Pub Date : 2025-04-08 DOI:10.1016/j.jastp.2025.106506
George V. Naidis
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Abstract

Downward-propagating positive sprite streamers are modeled. It is shown that, in agreement with recent high-speed video observations, at the initial stage of streamer propagation the streamer velocity increases with time with a nearly constant growth rate, varying almost proportionally to the streamer length. An approximate expression for the growth rate is presented as a function of the altitude, the driving electric field at this altitude and the peak electric field in the streamer head.
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评估精灵幡的增长率
向下传播的正向精灵流被建模。结果表明,与最近的高速视频观测结果一致,在流传播的初始阶段,流速度随时间以几乎恒定的增长率增长,几乎与流长度成正比。给出了生长速率的近似表达式,该表达式是海拔高度、该海拔高度的驱动电场和流线头部的峰值电场的函数。
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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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