日本地球惑星科学連合2025年大会

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[E] ポスター発表

セッション記号 P (宇宙惑星科学) » P-EM 太陽地球系科学・宇宙電磁気学・宇宙環境

[P-EM12] Coupling Processes in the Atmosphere-Ionosphere System

2025年5月25日(日) 17:15 〜 19:15 ポスター会場 (幕張メッセ国際展示場 7・8ホール)

コンビーナ:細川 敬祐(電気通信大学大学院情報理工学研究科)、Liu Huixin(九州大学理学研究院地球惑星科学専攻 九州大学宙空環境研究センター)、大塚 雄一(名古屋大学宇宙地球環境研究所)、Chang Loren(Institute of Space Science, National Central University)

17:15 〜 19:15

[PEM12-P03] Investigation on relationships among polar mesospheric cloud, temperature, and water vapor based on simultaneous observations by Himawari-8/AHI and Aura/MLS

*酒井 晶成1津田 卓雄1安藤 芳晃1鈴木 秀彦2中川 広務3西山 尚典4田中 良昌4 (1.電気通信大学、2.明治大学、3.東北大学、4.国立極地研究所)


キーワード:極中間圏雲、温度、水蒸気、ひまわり8号/AHI、オーラ/MLS

Polar mesospheric clouds (PMCs) are water ice clouds that can form in the mesopause region at altitudes of 80 to 85 km during summer, mainly in the polar region. Hence, the condition of supersaturation in water vapor would be vitally important for PMC formation, and it is supposed to be determined mainly by temperature and water vapor in the background atmosphere. Thus, it would be important to understand relationships among PMC, temperature, and water vapor. A previous study based on the latitudinal averaged analysis reported that the ice water content (IWC) in PMCs was generally controlled by temperature. In addition, they suggested that the relationship between the IWC and water vapor volume mixing ratio (VMR) changed seasonally from the cooling phase to the warming phase, implying more complexity in water vapor effects.

In this study, to advance our understanding of temperature and water vapor in PMC formation, we have investigated simultaneous observation events of the temperature, water vapor VMR, and PMC. The PMC data were obtained from limb-viewing PMC observations by Advanced Himawari Imager (AHI) onboard the geostationary satellite, Himawari-8. The field of view (FOV) of Himawari-8/AHI is fixed on the ground because of its geostationary orbit. The temperature and water vapor VMR data were obtained from the Microwave Limb Sounder (MLS) onboard the sun-synchronized polar orbit satellite, Aura. Thus, when the moving Aura/MLS FOV overlaps with the fixed Himawari-8/AHI FOV, we are able to obtain simultaneous observation events. In data analysis, we focused on the northern summer at higher latitudes. The analyzed data covered May to August in 2016-2022, and its latitudes were 80-81ºN. As for the Aura/MLS data, we selected data at 81.5 km.

As a result of the analysis, we obtained 12,953 simultaneous observation events, including 5,809 PMC detection events and 7,144 non-PMC events between 2016 and 2022. The obtained events were classified by grids with intervals of 2.5 K in temperature and 0.5 ppmv in water vapor VMR. Then, we calculated PMC occurrence rates for each grid. The results showed that the PMC occurrence rate was generally increasing with decreasing temperature. In cases of lower temperature (<152.5 K), the relationship between PMC occurrence rate and water vapor VMR was unclear. Then, in cases of higher temperature (>152.5 K), increases in the water vapor mixing ratio from 4.5 to 7.0 ppmv led to 17.9-44.2% increases in PMC occurrence rate. These results suggest that the supersaturation condition for the PMC formation can be satisfied in lower temperatures even with a relatively small amount of water vapor. On the other hand, in higher temperatures, a greater amount of water vapor would be needed to satisfy the supersaturation condition. Thus, our investigation implies an importance in the water vapor for PMC formation in such higher temperature conditions.