日本地球惑星科学連合2021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-EM09] Dynamics of Magnetosphere and Ionosphere

2021年6月6日(日) 13:45 〜 15:15 Ch.05 (Zoom会場05)

コンビーナ:藤本 晶子(九州工業大学)、尾崎 光紀(金沢大学理工研究域電子情報学系)、佐藤 由佳(日本工業大学)、中溝 葵(情報通信研究機構 電磁波研究所)、座長:尾花 由紀(大阪電気通信大学工学部基礎理工学科)、横山 佳弘(京都大学大学院理学研究科地球惑星科学専攻)

14:55 〜 15:10

[PEM09-18] Antarctic large area network observation of auroral phenomena using unmanned system: Current status of project as of early 2021

*門倉 昭1、小川 泰信1、田中 良昌1、山岸 久雄1、岡田 雅樹1、片岡 龍峰1、内田 ヘルベルト陽仁4、大塚 雄一2、元場 哲郎3、佐藤 夏雄1、Henri Robert5、Ashwini Sinha6、Jean Rasson7 (1.国立極地研究所、2.名古屋大学、3.ジョンズホプキンス大学、4.総研大、5.International Polar Foundation、6.Indian Institute of Geomagnetism、7.Royal Meteorological Institute of Belgium)

キーワード:オーロラ、ネットワーク観測、南極

Space and upper atmospheric sciences group in the National Institute of Polar Research (NIPR) is now planning to construct an observation network for auroral phenomena along the coast of the Dronning Maud Land in the Antarctica including Japanese Syowa Station, and has developed a Unmanned Auroral Observation system (UAO), which is equipped with a 3-axis fluxgate magnetometer, all-sky auroral imager, GNSS/TEC receiver, and a data communication system using the Inmarsat satellite data link with a low power consumption. The first UAO (UAO-1) had been installed at Amundsen Bay area, which is located about 500 km eastward from Syowa Station, in February, 2017 in the summer operation of the 58th Japanese Antarctic Research Expedition (JARE-58). The second UAO (UAO-2) had been installed at Belgium Princess Elisabeth Antarctica (PEA) Station in January, 2020. Electric power of the UAO-1 is supplied by a hybrid natural energy electric generation system which consists of three sets of 192W wind generators and 8 sets of 62W solar panels, while that of the UAO-2 is supplied from the AC power source of the PEA Station which is generated by a power generation system of the station using nine big wind generators and solar panels. For the UAO, observed magnetometer data (1 sec resolution), GNSS BINEX data (30 sec resolution), daily Keogram and sample image data of the auroral imager, and House Keeping data (temperatures and power voltages) (1 min resolution) are transmitted at every 1 hour via the satellite link system to a server in Japan by FTP, and auroral image data of 1 sec resolution are stored in a memory card of the video encoder in the system. Sample interval and pixel resolution of the transmitted auroral image data are 1 hour (5 minutes) and 640x480 (160x120) for the UAO-1 (UAO-2), respectively. UAO-2 has the other USB memory in the system which can store auroral still image of 1 sec resolution with 640x480 pixel resolution and GNSS BINEX data of 1 sec resolution. PEA Station is maintained during summer season, and becomes an unmanned station during winter season, while the electric power to all the instruments at the station is supplied continuously all through the season. In January, 2020, we had also installed an auroral imager system at Indian Maitri Station, which consists of four sets of all-sky imager using Watec cameras: 1) Panchromatic (color) ; 2) Panchromatic (black&white); 3) filtered at 560nm (FWHM:10nm); 4) filtered at 632nm (FWHM:10nm), respectively. Maitri is a year-round station. The auroral imager system is run autonomously. We ask expedition members at Maitri to send daily summary files via E-mail to us. In our presentation, we will talk about current status of the project as of early 2021.