火星における太陽風による大気浸食:火星エクスプレス号のASPERA-3からの最初の結果
R Lundin1, S Barabash, H Andersson
1Swedish Institute of Space Physics, Box 812, S-98 128, Kiruna, Sweden. rickard.lundin@irf.se
まとめ
宇宙プラズマとエネルギー原子の分析機 (ASPERA) は,火星のイオン圏の奥深くで太陽風とイオンを検出しました. これは,太陽風と火星の大気間の直接的な相互作用を示唆し,磁気異常によって引き起こされる可能性があります.
科学分野:
- 惑星科学は惑星科学である.
- 宇宙物理学 宇宙物理学
- エアロノミーはエアロノミーです.
背景:
- 火星は薄い大気と弱い地球磁場を持っています.
- 太陽風と惑星の大気間の相互作用は,大気の進化にとって極めて重要です.
研究 の 目的:
- 太陽風のプラズマと,火星のイオン圏へのイオン圏の浸透の範囲を調査する.
- この相互作用が火星の大気に及ぼす影響を理解するために.
主な方法:
- 火星エクスプレス号の宇宙プラズマとエネルギー原子の分析器 (ASPERA) 装置からのデータを活用する.
- 火星表面より低い高度でのプラズマとエネルギーイオン観測を分析する.
主要な成果:
- 太陽風のプラズマと加速されたイオノスフィアのイオンは,火星表面から270kmほど低いところまで観測されました.
- この深い浸透は,火星の上部の大気圏が太陽風の強引に直接曝されていることを示しています.
結論:
- 低高度での浸透とイオンエネルギー化は,太陽風と大気の相互作用が有意であることを示唆しています.
- 潜在的な原因には,太陽風の異常,火星の磁気異常,または要因の組み合わせが含まれます.
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