日本地球惑星科学連合2023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-EM15] 太陽地球系結合過程の研究基盤形成

2023年5月26日(金) 10:45 〜 12:15 101 (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:吉川 顕正(九州大学大学院理学研究院地球惑星科学部門)、岩井 一正(名古屋大学 宇宙地球環境研究所)

10:45 〜 11:00

[PEM15-07] Mid-latitude SuperDARN – latest achievements, recent progress and future plans

*西谷 望1行松 彰2堀 智昭1 (1.名古屋大学宇宙地球環境研究所、2.国立極地研究所)

キーワード:SuperDARN、mid-latitude、magnetosphere-ionosphere-thermosphere coupling、Hokkaido Pair of (HOP) radars

The Super Dual Auroral Radar Network (SuperDARN) is a powerful tool for monitoring ionospheric plasma convection and electron density changes in the high- and mid-latitude ionosphere. At present, a total of more than 35 SuperDARN radars in both hemispheres cover the geomagnetic latitude range of about 40 to 90 degrees, yielding many scientific results on a wide variety of scientific topics related to the dynamics of the ionosphere, which is affected both by the disturbances from above (magnetosphere), and those from below (thermosphere, atmosphere and even the ground/sea surface perturbations). In particular, mid-latitude SuperDARN radars, including two radars located in Hokkaido and operated by ISEE, Nagoya University, have been demonstrating the capabilities of the mid-latitude SuperDARN in various aspects. This paper will present an overview of the latest achievements, recent progress, and future plans (both short- and long-span) of the mid-latitude SuperDARN network.