DC component of spacecraft-origin magnetic field noise at the Arase/MGF sensor: (2) Evaluation with Tsyganenko-Sitnov 04 model

Material type: 文書・図像類

Author: 生松, 聡ほか

Publisher: 宇宙航空研究開発機構(JAXA)

Publication date: 2019-03-07

Material Format: Digital

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Note (General)：: The evaluation of the spacecraft-origin magnetic field noise (B_sub(DCnoise)) at the position of the sensor of Magnetic Field Experiments (MGF) onboar...

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Material Type: 文書・図像類
Title: DC component of spacecraft-origin magnetic field noise at the Arase/MGF sensor: (2) Evaluation with Tsyganenko-Sitnov 04 model
Author/Editor: 生松, 聡
山本, 和弘
能勢, 正仁
松岡, 彩子
寺本, 万里子
今城, 峻
Oimatsu, Satoshi
Yamamoto, Kazuhiro
Nose, Masahito
Matsuoka, Ayako
Teramoto, Mariko
Imajo, Shun
Author Heading: 生松, 聡
山本, 和弘
能勢, 正仁
松岡, 彩子
寺本, 万里子
今城, 峻
Oimatsu, Satoshi
Yamamoto, Kazuhiro
Nose, Masahito
Matsuoka, Ayako
Teramoto, Mariko
Imajo, Shun
Publication, Distribution, etc.: 宇宙航空研究開発機構(JAXA)
Publication Date: 2019-03-07
Publication Date (W3CDTF): 2019-03-07
Alternative Title: あらせ衛星/MGF センサにおける人工衛星起因の直流成分磁場ノイズ: (2) Tsyganenko-Sitnov 04 モデルを用いた評価
Periodical title: 宇宙航空研究開発機構研究開発報告 = JAXA Research and Development Report
No. or year of volume/issue: JAXA-RR-18-005E
Volume: JAXA-RR-18-005E
Pages: 29-34
ISSN (Periodical Title): ISSN : 2433-2216
Text Language Code: eng
Subject Heading: Arase
Magnetic field experiments (MGF)
Spacecraft-origin noise
Tsyganenko-Sitnov 04 model
Target Audience: 一般
Note (General): The evaluation of the spacecraft-origin magnetic field noise (B_sub(DCnoise)) at the position of the sensor of Magnetic Field Experiments (MGF) onboard the Arase satellite has been performed. We examined the difference between the observation of the magnetic field with MGF and the Tsyganenko-Sitnov 04 (TS04) model field in DSI coordinates (ΔB sub(DSI)) during the quiet time intervals. ΔB sub(z, DSI) was - 0.7 nT on average, which indicates that the B_sub(DCnoise) in the spin-axis direction is quite small. We conclude that the MGF data are well-calibrated and no large B_sub(DCnoise) is included in the measured magnetic field. Although the difference between the MGF observations and the TS04 model in the X sub(DSI) and Y sub(DSI) directions was a few nT, it may be attributed to the TS04 model field, not an observational error of MGF.
形態: カラー図版あり
Physical characteristics: Original contains color illustrations
資料番号: AA1830033005
レポート番号: JAXA-RR-18-005E
DOI: 10.20637/JAXA-RR-18-005E/0005
Source: https://jaxa.repo.nii.ac.jp/?action=repository_action_common_download&item_id=1797&item_no=1&attribute_id=31&file_no=1
https://jaxa.repo.nii.ac.jp/?action=repository_action_common_download&item_id=1797&item_no=1&attribute_id=31&file_no=1
Access Restrictions: 限定公開
Data Provider (Database): 国立情報学研究所 : 学術機関リポジトリデータベース（IRDB）（機関リポジトリ）
https://irdb.nii.ac.jp
Original Data Provider (Database): 宇宙航空研究開発機構 : 宇宙航空研究開発機構リポジトリ