パレオマグネティズム シングルジルコンの結晶によって記録されたハデアからパレオアケアンの地形図
John A Tarduno1, Rory D Cottrell2, William J Davis3
1Department of Earth and Environmental Sciences, University of Rochester, Rochester, NY 14627, USA. Department of Physics and Astronomy, University of Rochester, Rochester, NY 14627, USA. john.tarduno@rochester.edu.
まとめ
初期の地球
科学分野:
- 地理学
- 古磁気学
- 惑星科学
背景:
- 地球の進化にとって ジオダイナモの起源を理解することは 極めて重要です
- 地磁石は地球の磁場を作り 大気を遮断します
研究 の 目的:
- 古力学データを用いて初期の地力学の歴史を再構築する.
- ハーデンの地磁場に必要な条件を調査する
主な方法:
- ハーデアン・アーケイアンジルコンの磁気インクルージョンの全ベクトルパレオインテンシティー測定
- ジャック・ヒルズのジルコンの分析 西オーストラリア
主要な成果:
- 記録された磁場は 33億から 42億年前のものです
- 最近の赤道値の 0.12 倍から 1.0 倍に変化した.
- ハーデアの地磁場がある証拠だ
結論:
- ハーデンの地磁場は 超アディアバティックなコア・マントルの熱流を意味する
- 初期のプレート構造や 磁気熱伝導を示唆している
- 地球と火星の初期の大気進化に影響を与えた 遅い重爆撃前の磁場を 支持している.
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