OH and O2 airglow emissions during the 1998 Leonid outburst and the 2002 Leonid storm

被引：0

作者：

Trigo-Rodriquez, JM ^{[1
]}

López-González, MJ

Ortiz, JL

机构：

[1] Univ Calif Los Angeles, Inst Geophys & Planetary Phys, Astrobiol Ctr, Los Angeles, CA 90095 USA

[2] CSIC, Inst Astrofis Andalucia, E-18080 Granada, Spain

来源：

EARTH MOON AND PLANETS | 2003年 / 93卷 / 03期

关键词：

airglow; Leonids; 1998; and; 2002; lower thermosphere; O-2; OH; meteor;

D O I：

10.1023/B:MOON.0000047525.24190.de

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

In order to enhance our understanding of the possible influence of meteor ablation on the enrichment in OH and O-2 of the lower thermosphere we studied intense Leonid meteor activity by using the SATI ( Spectral Airglow Temperature Imager) interferometer of the Instituto de Astrofisica de Andalucia. We measured the emission rate and rotational temperature of OH and O-2 airglow emission layers during two observation periods of high meteoric activity: the 1998 Leonid outburst and the 2002 Leonid storm. The results show that there is not a clear relation of O2 and OH airglow emission and rotational temperature with meteoric activity.

引用

页码：191 / 201

页数：11

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