Non-uniform ionisation of the upper atmosphere due to the electromagnetic pulse from a horizontal lightning discharge

被引:47
作者
Cho, M
Rycroft, MJ
机构
[1] Kyushu Inst Technol, Dept Elect Engn, Tobata Ku, Kitakyushu, Fukuoka 804, Japan
[2] Int Space Univ, F-67400 Illkirch, France
[3] De Montfort Univ, Fac Comp Sci & Engn, Leicester LE1 9BH, Leics, England
关键词
non-uniform ionisation; upper atmosphere; electromagnetic pulse; horizontal lightning discharge;
D O I
10.1016/S1364-6826(00)00235-2
中图分类号
P3 [地球物理学]; P59 [地球化学];
学科分类号
0708 ; 070902 ;
摘要
The purpose of this paper is to model numerically the ionisation created in the mesosphere above a strong horizontal (cloud-to-cloud) lightning discharge, and thus to understand better the formation of elves and related columniform (spatially structured) sprites. Such ionisation depends upon height, via the ratio of the VLF/LF wave electric field (radiated by the current in the discharge) to the atmospheric neutral density. The simulation shows local maxima on the order of 10 km apart due to the interference between direct waves radiated by the discharge current, waves reflected by the ground and waves reflected by the ionosphere. Parametric studies are carried out varying the frequency, amplitude, height, length and duration of the current. For waves greater than or equal to 30 kHz generated by a current greater than or equal to 50 kA, localised peaks of electron density occur from 75 to 85 km altitude, particularly for discharges longer than 15 km. From such peaks, time-varying "stalactites" on the bottom of the ionosphere, streamers could develop and propagate downwards. These could become columniform sprites in the presence of the quasi-electrostatic field due to the negative charge remaining in the thundercloud after a positive cloud-to-ground discharge. (C) 2001 Elsevier Science Ltd. All rights reserved.
引用
收藏
页码:559 / 580
页数:22
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