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Updated: Jul 11, 2026

06:14
Simulating Imaging of Large Scale Radio Arrays on the Lunar Surface
Published on: July 30, 2020
まとめ
原子ナトリウムは,月面の大気の軌跡をたどり,100km以下で検出されました. 観測により,ナトリウムは月の半径数回まで広がり,主に太陽光子や風によって放出されるもので,微小隕石によって放出されるものではないことが明らかになった.
科学分野:
- 月科学は月科学である.
- 大気科学 大気科学
- 原子物理学 原子物理学とは
背景:
- 原子ナトリウムは,太陽光が波長D(1) とD(2) で効率的に散乱するので,月のエクソスフィアの効果的なトレーサーです.
- 1988年の地上の観測では,高度100km未満で50原子/cm3未満の密度でナトリウムが検出されました.
研究 の 目的:
- 月の大気中のナトリウム原子の分布と源を調査する.
- 月面からナトリウムが解放される過程を理解する.
主な方法:
- 月の円盤を覆い隠すために,冠動脈撮影技術による望遠鏡観測を用いた.
- 月周りのナトリウム原子の空間分布と密度を分析した.
主要な成果:
- 月から数月の半径まで広がる原子ナトリウムの存在が確認された.
- ソーラーゼニット角度によるナトリウム分布を証明した.
- 100km以下では,ナトリウム密度は50原子/cm3未満であることが判明しました.
結論:
- 高地にある月のナトリウムの主要な源は,太陽光子相互作用 (加熱/噴出) と太陽風の影響である可能性が高い.
- マイクロ隕石の爆撃は,より高い高度での月のナトリウムの主な供給源ではありません.
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