このアイテムのアクセス数: 244
このアイテムのファイル:
ファイル | 記述 | サイズ | フォーマット | |
---|---|---|---|---|
s40623-018-0800-1.pdf | 2.24 MB | Adobe PDF | 見る/開く |
タイトル: | The ARASE (ERG) magnetic field investigation |
著者: | Matsuoka, Ayako ![]() ![]() ![]() Teramoto, Mariko Nomura, Reiko Nosé, Masahito Fujimoto, Akiko Tanaka, Yoshimasa Shinohara, Manabu Nagatsuma, Tsutomu Shiokawa, Kazuo Obana, Yuki Miyoshi, Yoshizumi Mita, Makoto Takashima, Takeshi Shinohara, Iku |
著者名の別形: | 能勢, 正仁 |
キーワード: | EMIC wave Geospace Magnetic field Magnetometer Radiation belts Ring current ULF wave |
発行日: | 14-Mar-2018 |
出版者: | Springer Nature |
誌名: | Earth, Planets and Space |
巻: | 70 |
論文番号: | 43 |
抄録: | The fluxgate magnetometer for the Arase (ERG) spacecraft mission was built to investigate particle acceleration processes in the inner magnetosphere. Precise measurements of the field intensity and direction are essential in studying the motion of particles, the properties of waves interacting with the particles, and magnetic field variations induced by electric currents. By observing temporal field variations, we will more deeply understand magnetohydrodynamic and electromagnetic ion-cyclotron waves in the ultra-low-frequency range, which can cause production and loss of relativistic electrons and ring-current particles. The hardware and software designs of the Magnetic Field Experiment (MGF) were optimized to meet the requirements for studying these phenomena. The MGF makes measurements at a sampling rate of 256 vectors/s, and the data are averaged onboard to fit the telemetry budget. The magnetometer switches the dynamic range between ± 8000 and ± 60, 000 nT, depending on the local magnetic field intensity. The experiment is calibrated by preflight tests and through analysis of in-orbit data. MGF data are edited into files with a common data file format, archived on a data server, and made available to the science community. Magnetic field observation by the MGF will significantly improve our knowledge of the growth and decay of radiation belts and ring currents, as well as the dynamics of geospace storms. |
著作権等: | © The Author(s) 2018. This article is distributed under the terms of the Creative Commons Attribution 4.0 International License (http://creativecommons.org/licenses/by/4.0/), which permits unrestricted use, distribution, and reproduction in any medium, provided you give appropriate credit to the original author(s) and the source, provide a link to the Creative Commons license, and indicate if changes were made. |
URI: | http://hdl.handle.net/2433/235014 |
DOI(出版社版): | 10.1186/s40623-018-0800-1 |
出現コレクション: | 学術雑誌掲載論文等 |

このリポジトリに保管されているアイテムはすべて著作権により保護されています。