海洋の潮流による磁場の衛星観測
Robert H Tyler1, Stefan Maus, Hermann Lühr
1Ocean Physics Department, Applied Physics Laboratory, University of Washington, 1013 NE 40th Street, Seattle, WA 98103, USA. tyler@apl.washington.edu
まとめ
海流は,衛星によって検出可能な磁場を作り出します. この研究は,海洋の月面半昼間 (M2) 潮からの磁気信号を特定し,海洋の磁場を遠くから明確に観測できることを証明しています.
科学分野:
- 地質物理学 地質物理学とは地質物理学です.
- 海洋学 海洋学 海洋学
- 宇宙科学 スペースサイエンス
背景:
- 地球の海は電気伝導性のある液体である.
- 地球の磁場と相互作用する海流は,二次磁場を生成する.
- 衛星技術により,これらの磁場の遠隔感知が可能になっています.
研究 の 目的:
- 月の半昼間 (M2) 潮の海によって生成される磁場を調査するために.
- 衛星観測で海洋磁場の検出性を実証する.
主な方法:
- 衛星による磁場測定の分析.
- 海洋の潮流によって生成される磁場のモデリング.
主要な成果:
- 月の半日間潮 (M2) の海から発生する磁場が成功裏に特定されました.
- これらの海洋磁気信号は,衛星データから明確に識別できます.
結論:
- 衛星観測は,海潮によって生成される磁場を効果的に検出することができます.
- この能力は,海洋のダイナミクスをリモートで研究するための新しい道を開きます.
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