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)

[PEM18-08] Review of the mid-latitude SuperDARN and the future of the SuperDARN

*西谷 望1 (1.名古屋大学宇宙地球環境研究所)

キーワード:SuperDARN、mid-latitude、low-latitude

The Super Dual Auroral Radar Network (SuperDARN) is a powerful tool for monitoring ionospheric plasma convection and electron density changes. The SuperDARN began its official operation in 1995 For the first few years, the SuperDARN field of view (FOV) was limited to high latitudes. About ten years later, the first purpose-built mid-latitude SuperDARN radars started operation at sites in Virginia and Hokkaido in 2005 and 2006, respectively. Subsequent construction of additional radars at mid-latitudes have greatly expanded the SuperDARN FOV, and made accessible a range of research topics that are distinctive to the subauroral and mid-latitude ionosphere. In this paper we review the accomplishments of the mid-latitude SuperDARN in several scientific and technical areas, as well as the history of the mid-latitude SuperDARN. We also discuss the future directions of the SuperDARN, including the expansion of SuperDARN FOV to even lower latitudes up to the equatorial region.