JpGU-AGU Joint Meeting 2017

講演情報

[EE] 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-EM16] [EE] Physics of Inner Magnetosphere Coupling

2017年5月24日(水) 13:45 〜 15:15 ポスター会場 (国際展示場 7ホール)

コンビーナ:Danny Summers(Memorial University of Newfoundland)、Jichun Zhang(University of New Hampshire Main Campus)、海老原 祐輔(京都大学生存圏研究所)、桂華 邦裕(東京大学大学院理学系研究科地球惑星科学専攻)、Aleksandr Y Ukhorskiy(Johns Hopkins University Applied Physics Laboratory)、Dae-Young Lee(Chungbuk Natl Univ)、Yiqun Yu(Beihang University)、三好 由純(名古屋大学宇宙地球環境研究所)

[PEM16-P05] Ground calibration experiments of Magnetic field experiment on the ERG satellite

*寺本 万里子1Matsuoka Ayako2Nomura Reiko2 (1.Institute for Space-Earth Environmental Research, Nagoya University、2.Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency)

キーワード:ERG satellite, Magnetic Filed experiment

The Arase (ERG) satellite was launched on 20 December 2016 to study plasma process in the inner magnetosphere. The Magnetic field experiments (MGF), which is one of the scientific experiments onboard the Arase satellite, observes the background magnetic field and its low frequency fluctuations. The MGF has a set of tri-axis ring-core type fluxgate sensors (MGF-S) to observe the magnetic field in the inner magnetosphere. For accurate measurements of the magnetic field vector along the Arase orbits, ground calibration experiments of MGF-S are needed.
We have been performed in order to determine the sensitivity and alignment via ground calibration experiments. From response of MGF-S to known applied magnetic field, we determined the sensitivity of each axis and found that the error of the sensitivity is less than 0.06%. The axis of the sensor is orthogonal to each other within 0.95 degrees. The estimated error of alignment is within 0.07 degrees. We also have examined the temperature dependence of the sensitivity and offset. The sensitivities relative to the room temperature have linearity with the standard error less than 0.0016, while the offset of the sensors have no clear linearity but reproducibility against temperature. From these ground examinations, the determination accuracies of the amplitude and direction of the magnetic field observed by the MGF will satisfy the science requirements for the Arase observations. In this presentation, we will also evaluate and show measurement error of MGF-S along the Arase orbit.