摘要:In the Second Japanese Antarctic Research . Expedition, the measurement of the intensity of 5577A emission was repeated as in the first expedition, on board the "Soya". The general tendency of latitude effect was almost same as in the first expedition. An analysis was made to qualify the intensity of airglow into two parts, the stormy airglow which seems to be the effect of solar activity and the stationary airglow which is generally weak and calm. The former has not much latitude effect and the latter shows latitude effect besides seasonal variation. The stationary airglow is weakest at the geographic equator, and it has secondary minima roughly between 35° and 40° of geographic latitude.