日本地球惑星科学連合2025年大会

講演情報

[E] 口頭発表

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-EM14] 太陽地球系結合過程の研究基盤形成

2025年5月28日(水) 09:00 〜 10:30 303 (幕張メッセ国際会議場)

コンビーナ:山本 衛(京都大学生存圏研究所)、小川 泰信(国立極地研究所)、野澤 悟徳(名古屋大学宇宙地球環境研究所)、吉川 顕正(九州大学大学院理学研究院地球惑星科学部門)、座長:山本 衛(京都大学生存圏研究所)、岩井 一正(名古屋大学 宇宙地球環境研究所)

09:15 〜 09:30

[PEM14-02] PBASEプログラムによる地上多点観測・衛星観測・モデリングの連携の現状

*塩川 和夫1、PWING Team、PBASE Team (1.名古屋大学宇宙地球環境研究所)

キーワード:PBASEプログラム、PWINGプロジェクト、地上ネットワーク観測、人工衛星観測

A new JSPS Kakenhi program “International joint research of geospace variability by combining multi-point ground and satellite observations and modeling (PBASE program)” has been started since January 2023. This program encourages international collaborative studies of combining ground-based and satellite observations of geospace with modeling through supporting students and early-career scientists. The ground-based network observations are originally based on the PWING project (study of dynamical variation of Particles and Waves in the INner magnetosphere using Ground-based network observations, 2016-2022) which operates all-sky airglow/aurora imagers, 64-Hz sampled induction magnetometers, 40-kHz VLF receivers, and 64-Hz riometers at 8 stations at magnetic latitudes of ~60 degree around the north-pole, in order to cover longitudinal variation of aurora, airglow, and electromagnetic disturbances in the inner magnetosphere. These aurora/airglow imagers are part of the Optical Mesosphere Thermosphere Imagers (OMTIs). These PWING and OMTIs instruments are in automatic operation at various locations from high to equatorial latitudes in Canada, US (Alaska), Russia, Norway, Finland, Iceland, Japan, Thailand, Indonesia, and Australia. In the presentation, we show current configuration of these ground-based network observations and provide updates of the ground-satellite-modeling coordination under the PBASE program.

PWING Team: https://www.isee.nagoya-u.ac.jp/dimr/PWING/en/
PBASE Team: https://www.isee.nagoya-u.ac.jp/dimr/PBASE/en/