日本地球惑星科学連合2021年大会

講演情報

[E] ポスター発表

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) 17:15 〜 18:30 Ch.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)

17:15 〜 18:30

[PEM09-P31] Application of magneto-impedance sensor to geomagnetic field measurements for constructing Distributed Arrays of Small Instruments (DASI)

野村 太志1、*能勢 正仁1、青山 均2、河野 剛健2、市原 寛3、平原 聖文1 (1.名古屋大学 宇宙地球環境研究所、2.愛知製鋼株式会社、3.名古屋大学大学院 環境学研究科附属地震火山研究センター)

キーワード:磁気インピーダンスセンサー、地磁気観測、小型計測器分散アレイ (DASI)、フラックスゲート磁力計

Magneto-impedance (MI) effect was discovered about 25 years ago and micro-size magnetic sensors that utilizes this effect become commercially available. MI sensors are much less expensive than fluxgate sensors. We are developing a low-cost system to measure the geomagnetic field using the MI sensor, which is named MIM-Pi. MIM-Pi includes a Raspberry Pi, low-cost 24-bit AD converters, and power supply circuits for generating a stable power supply voltage.
For the period of June 17 to June 25, 2020, we conducted experimental observations of geomagnetic field variations with MIM-Pi at Inabu observation site in Japan (26.8°, –152.5° in geomagnetic coordinates). Inabu observation site is operated by Nagoya University. Data obtained with MIM-Pi were compared with those from the fluxgate magnetometer that has been working at the site. Results showed that MIM-Pi recorded Sq variations and geomagnetic pulsations with amplitudes of ~2 nT that were also detected with the fluxgate magnetometer.
In presentation, we will show long term observations by MIM-Pi and discuss the possibility of using this system for construction of Distributed Arrays of Small Instrument (DASI). We will also show the result of an attempt to remove artificial noises by placing multiple observation systems at neighboring observation points and performing independent component analysis.