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東方アフロディテ・テラ,ヴェーヌスの地形学と火山学: 沈下はなく,広がりはなく,
まとめ
金星の東方アフロディテ・テラにおける地質学は,マグマのダイアピールによって駆動され,地殻の水泡を形成する. この垂直の構造構造は,この地域がプレート境界ではないことを意味し,ヴェヌスの地質学の以前の解釈に挑戦しています.
科学分野:
- 惑星科学は惑星科学である.
- 地質学 地質学 地質学
- 地質物理学 地質物理学とは地質物理学です.
背景:
- 金星の東方アフロディーテ・テラは,著しい変形と高い地形を示しています.
- 以前の解釈では,この地域が地形型のプレート境界 (拡張的または収束) を表す可能性があると示唆されていた.
研究 の 目的:
- 東アプロディテ・テラを形作る構造的プロセスを再評価する.
- その地域がプレート境界を表しているか,または他の地質的な力によって支配されているかどうかを判断する.
主な方法:
- 東方アフロディーテ・テラスの地質学的および構造的データの分析.
- 観測された特徴を垂直対水平構造のモデルと比較.
主要な成果:
- 地質学的および構造的分析は,マグマダイアピルによる地殻の水泡形成が支配的なプロセスであることを示しています.
- マグマの上流によって引き起こされる垂直構造は,この地域の水平構造に取って代わります.
結論:
- 東方アフロディーテ・テラは,地上の分岐または収束プレート境界に類するものではありません.
- 垂直構造は,この地域における金星の地殻の変形を形作る上で支配的な役割を果たしています.
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When analyzing a single line-to-ground fault from phase A to ground at a three-phase bus, it is important to consider the fault impedance. This impedance is zero for a bolted fault, equal to the arc impedance for an arcing fault, and represents the total fault impedance for a transmission-line insulator flashover. To derive sequence and phase currents, fault conditions are translated from the phase domain to the sequence domain.
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