まとめ
パイオニア 11
科学分野:
- 惑星科学は惑星科学である.
- プラズマ物理学 プラズマ物理学
- 磁気圏物理学 磁気圏物理学
背景:
- パイオニア11号は,土星の磁気圏と放射線帯を初めて徹底的に探査した.
- 土星の磁気圏は,地球の磁気圏と木星の磁気圏に匹敵し,放射線の強度は異なる.
- 磁気圏の内側と外側には,異なる放射線特性と粒子エネルギーがある.
研究 の 目的:
- 土星の磁気圏と捕捉された放射線帯の構造と動態を調査する.
- 粒子のピッチ角度分布とその磁気圏プロセスへの影響を分析する.
- 土星の環の吸収特性を特徴付け,新しい天体を特定する.
主な方法:
- パイオニア11号宇宙船によるインシトゥ測定.
- 粒子のピッチ角度分布の分析.
- 粒子の拡散率を使用してリングの横断面積と不透明性の推定.
主要な成果:
- 土星の磁気圏は中程度の大きさで,放射の強度は地球のそれと似ています.
- Fリング,パイオニア部門,そして月1979 S 2が確認されましたが,他の天体の証拠は曖昧です.
- 土星のリングと衛星は,捕獲された放射線を大幅に吸収し,リングの下の放射線を完全に弱める.
- Fリングの横断面積と不透明性が推定されました.
結論:
- パイオニア11号は,土星の磁気圏と放射線環境に関する重要なデータを提供した.
- 土星の環は,磁気圏の放射線景観を形作る上で重要な役割を果たしています.
- 粒子源としての宇宙線アルベド中性子崩壊のさらなる調査が推奨されています.
関連する概念動画
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