日本地球惑星科学連合2019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

2019年5月30日(木) 10:45 〜 12:15 A01 (東京ベイ幕張ホール)

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:野澤 悟徳

11:45 〜 12:00

[PEM15-10] SuperDARN Hokkaido Pair of (HOP) radars and mid-latitude SuperDARN: today and future

*西谷 望1 (1.名古屋大学宇宙地球環境研究所)

キーワード:中緯度SuperDARN

The Super Dural Auroral Radar Network (SuperDARN) is a network of HF radars. At present there are total of 36 SuperDARN radars located in high- to mid-latitude regions of both northern (23) and southern (13) hemispheres. Mid-latitude SuperDARN radars started operation about 15 years ago and have been acquiring scientific data, which could be obtained using the pre-existing high-latitude radars. The SuperDARN Hokkaido Pair of (HOP) radars consisting of Hokkaido East / West radars are located equatorward of 40 degrees geomagnetic latitude (currently located at the lowest geomagnetic latitude) and have been storing important scientific data during quiet to very active periods. In this presentation accomplishments, present status and future directions of the SuperDARN HOP radars and mid-latitude SuperDARN be reviewed.