摘要
以上层大气中的气辉(极光)为被探测源,利用干涉成像光谱技术和电磁波的多普勒效应对上层大气风场进行测量,分析和计算了大气风场的速度和温度,并就被探测源和探测器之间的相对速度与其连线成任意角时的情形进行了讨论。采用计算机模拟,分析了大气风场的测量效果。
The interference image spectroscopy coupled with the Doppler effect of electrical and magnetic waves are employed to measure the natural airglow and auroral visible emission lines in the upper atmosphere. The velocity and temperature of the upper atmospheric wind field are analyzed and calculated. The relative velocity of the source to the detector with arbitrary angle to their link line is discussed. Computer simulation is employed for analyzing the effects of the measurement of the upper atmospheric wind field.
出处
《光学学报》
EI
CAS
CSCD
北大核心
2000年第2期234-239,共6页
Acta Optica Sinica
基金
国防科技预研基金!资助项目 ( 97J2 0 .7.3.Zk180 3)
关键词
大气风场
干涉成像光谱技术
多普勒效应
atmospheric wind field, interference image spectroscopy, Doppler effect.
