日本地球惑星科学連合2025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

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-P25] Localization and Classification of Gravity Wave Events from VIIRS Day/Night Band Satellite Imagery Using Machine Learning Techniques

*穂積 裕太1,2Jia Yue1,2、Mostafa Seraj3、Wang Chenxi3、Wang Jianwu3、Purushotham Sanjay3、Miller Steven4 (1.The Catholic University of America、2.NASA Goddard Space Flight Center/CCMC、3.Department of Information Systems, University of Maryland, Baltimore County、4.Cooperative Institute for Research in the Atmosphere, Colorado State University)

キーワード:Gravity Waves、Airglow imaging、Machine Learning

A machine learning model was developed to detect and classify gravity wave events from Day/Night Band (DNB) images of the Visible Infrared Imaging Radiometer Suite (VIIRS) aboard the Suomi National Polar-orbiting Partnership (Suomi NPP) satellite. Spaceborne airglow imaging provides an excellent opportunity to study gravity waves, especially those with short horizontal wavelengths, from a global perspective. DNB/VIIRS has captured mesospheric airglow images since 2012, providing over twelve years of data for long-term studies. The broadband sensitivity (505–890 nm) of DNB results in significant contamination from lower atmospheric emissions, city lights, orographic features, and cloud reflections. Due to this contamination, automated systematic detection of wave events is challenging, and manual identification is impractical given the large volume of data. Therefore, a novel machine learning technique for identifying wave events is crucial to fully utilize the extensive DNB dataset for long-term research. In this study, we focus on four types of wave events with distinct appearances: concentric gravity waves, frontal waves, ripples, and other gravity wave events. These waves are associated with different physical processes, making it beneficial to distinguish among them. The YOLOv5 machine learning model, short for “You Only Look Once version 5,” was trained using manually labeled gravity wave event images with the four event labels. After training, we applied the model to twelve years of DNB data. In this presentation, we will discuss the model training process, performance evaluations, and the global distribution of the detected wave events.