JpGU-AGU Joint Meeting 2020

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-EM18] 太陽地球系結合過程の研究基盤形成

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)

[PEM18-04] PWINGプロジェクトと超高層大気イメージングシステムによる地上多点観測網の現状

*塩川 和夫1大塚 雄一1 (1.名古屋大学宇宙地球環境研究所)

キーワード:地上多点観測、超高層大気イメージングシステム、PWINGプロジェクト

Additional Coauthor: PWING Team (http://www.isee.nagoya-u.ac.jp/dimr/PWING/en/)

The PWING project (study of dynamical variation of Particles and Waves in the INner magnetosphere using Ground-based network observations, 2016-2020) deploy 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 to cover longitudinal variation of aurora and electromagnetic disturbances in the inner magnetosphere. The Optical Mesosphere Thermosphere Imagers (OMTIs) consist of 21 all-sky cooled-CCD imagers, 5 Fabry-Perot interferometers, 3 airglow temperature photometers, and 3 meridian-scanning photometers to measure two-dimensional airglow images in the mesopause region and in the thermosphere, wind and temperatures in the lower thermosphere, and airglow rotational temperatures in the mesopause region. 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, Nigeria, and Australia. In the presentation, we introduce current status and recent major results obtained by these multi-instrument ground networks around the world. Details of the PWING project and OMTIs can be seen at http://www.isee.nagoya-u.ac.jp/dimr/PWING/PWING_web_e.htm and at http://stdb2.isee.nagoya-u.ac.jp/omti/, respectively.