RUNAWAY ELECTRONS AS A SOURCE OF RED-SPRITES IN THE MESOSPHERE

被引:102
作者
BELL, TF
PASKO, VP
INAN, US
机构
[1] STAR Laboratory, Stanford University, Stanford, California
关键词
D O I
10.1029/95GL02239
中图分类号
P [天文学、地球科学];
学科分类号
07 ;
摘要
Large quasi-electrostatic (QE) fields above thunderclouds [Pasko et al, 1995] produce an upward traveling beam of similar to 1 MeV runaway electrons which may contribute to the production of optical emissions above thunderclouds referred to as Red Sprites. Results of a one dimensional computer simulation model suggest that the runaway electrons can produce optical emissions similar in intensity and spectra to those observed in Red Sprites, but only for large QE fields produced by positive CG discharges lowering 250 C or more to ground from an altitude of at least 10 km. Differences in predicted optical spectra from that of other mechanisms suggest that the runaway electron mechanism can be readily tested by high resolution spectral measurements of Red Sprites.
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页码:2127 / 2130
页数:4
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