Through detecting the Doppler shifts of airglow (aurora) in upper atmosphere, the physical quantity such as velocity, temperature and pressure of upper atmosphere is derived.
通过探测高层大气中气辉（极光）辐射线的多普勒频移，可以反演出高层大气中的速度、温度和压强等物理量。
Through detecting the Doppler shifts of airglow (aurora) in upper atmosphere, the physical quantity such as velocity, temperature and pressure of upper atmosphere is derived.
通过探测高层大气中气辉（极光）辐射线的多普勒频移，可以反演出高层大气中的速度、温度和压强等物理量。
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