日本地球惑星科学連合2024年大会

講演情報

[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

2024年5月30日(木) 17:15 〜 18:45 ポスター会場 (幕張メッセ国際展示場 6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 〜 18:45

[PEM12-P05] A plan for ground-based observation of noctilucent clouds in Antarctic region.

*遠藤 哲歩1川上 莉奈1増田 歩音1鈴木 秀彦1 (1.明治大学)

キーワード:夜光雲、中間圏、超高層大気、極域、南極

Noctilucent cloud (NLC) images often contain very fine wavy structures ranging from several kilometers to several tens of kilometers. These are thought to reflect small-scale local atmospheric disturbances in the upper atmosphere. Satellite imaging data cannot resolve these fine structures, and thus, ground-based imaging is an effective method to study the relationship between fine structures in NLC and background disturbances in the upper mesosphere. However, previous NLC observations have been conducted mainly in the Northern Hemisphere, as represented by Northern Europe [e.g. Dalin et al.,2020] and the North American continent [e.g. Russell III et al.,2014]. In contrast, there are very few observations in the Southern Hemisphere. The reason for this asymmetry is that most of the best observation latitudes (50 - 60°S) for NLC observation in the Southern Hemisphere are in the ocean, and most of the land area of Antarctica is under the influence of the midnight sun, which makes it difficult to detect NLCs because of a bright background sky condition. Therefore, opportunities for NLC observations in the Southern Hemisphere are quite limited. We have examined the feasibility to overcome this problem by developing an optical imager specialized for noctilucent cloud observations [Nakamura et al.,2021]. Noctilucent clouds are known to have a spectral peak at 400-500 nm in their radiance [Lange et al.,2022]. On the other hand, the background spectrum in twilight sky attenuates in wavelengths shorter than 680nm. Therefore, there is the optimum wavelength band for noctilucent cloud observation with the best signal-to-noise ratio (SNR) in shorter wavelength region. In this study, the most suitable bandpass for NLC observations is proposed based on the ground spectral data of twilight background sky acquired in the polar region.
As a result, we conclude that an imaging observation by using a cooled CMOS camera equipped with the bandpass filter which has the center wavelength at 371 nm and 40nm bandwidth can give effective SNR(SNR>1.80) for NLC even under a bright sky condition corresponding to a local solar zenith angle ~91°.
The new imager can expand the observation period in the high-latitude region. For example, the observation period would increase +15 days to the conventional period of 14 days in Syowa Station (69.00°S, 39.58°E) (See Figure). And we also have estimated the expected observation period at 3 stations (Rothera station, Davis station and Zhongshan station) with the new imager.

References
Dalin, P.et al., Stratospheric observations of noctilucent clouds: a new approach in studying middle- and large-scale mesospheric dynamics, Ann. Geophys., 38, 61–71, https://doi.org/10.5194/angeo-38-61-2020, 2020.
James M. Russell III et al., Analysis of northern midlatitude noctilucent cloud occurrences using satellite data and modeling, JGRA,199,3238-3250,2014.
Nakamura et al.,sgepss, 2021.
Lange, A.et al., On the colour of noctilucent clouds, Ann. Geophys., 40, 407–419, https://doi.org/10.5194/angeo-40-407-2022, 2022.