Blue-light imagery and photometry of sprites

被引:48
作者
Suszcynsky, DM
Roussel-Dupre, R
Lyons, WA
Armstrong, RA
机构
[1] Univ Calif Los Alamos Natl Lab, Space & Atmospher Sci Grp, Los Alamos, NM 87545 USA
[2] FMA Res, Ft Collins, CO 80524 USA
[3] Mission Res Corp, Nashua, NH 03062 USA
基金
美国国家航空航天局;
关键词
D O I
10.1016/S1364-6826(98)00027-3
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
We have obtained blue (350-475 nm) video images and simultaneous high-time resolution narrow-band blue (415-435 nm) photometry records of four sprite events. The brightest blue images show a sustained tendril geometry and a nearly constant intensity of emission over the entire vertical extent of the sprite (from 35-90 km altitude). Photometer light curves display an exponential decay with a 0.3 ms time constant, a FWHM on the order of 0.1-1.0 ms, and are probably dominated by 427.8 nm (N-2(+) 1N) emission. The data support the observations of Armstrong et al. (1998) and support the contention that significant ionization occurs during sprite generation. (C) 1998 Elsevier Science Ltd. All rights reserved.
引用
收藏
页码:801 / 809
页数:9
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