相关实验视频
Updated: Aug 3, 2026

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Single-unit In vivo Recordings from the Optic Chiasm of Rat
Published on: April 2, 2010
克莱门廷的双眼雷达实验
S Nozette1, C L Lichtenberg, P Spudis
1U.S. Air Force Phillips Laboratory, Space Experiments Directorate, 711 North Fayette Street, Alexandria, VA 22314, USA.
概括
来自月球南极的雷达回声显示,在永久阴影的地区,极化呈现出独特的增强. 这一发现表明,在这些寒冷的月球区域中存在体积散射器,可能是水冰.
科学领域:
- 月球科学 月球科学
- 星球雷达天文学 行星雷达天文学
- 地质物理学 地质物理学
背景情况:
- 比斯塔基雷达实验提供了对表面性质的洞察.
- 雷达回声的极化可以揭示有关散射机制的信息.
- 月球永久阴影区域 (PSR) 具有重要的科学意义.
研究的目的:
- 为了研究不同月球区域的雷达回声特征.
- 为了分析极化变化与不同的比斯塔特角度的变化.
- 在月球PSR中识别潜在的散射器.
主要方法:
- 在克莱门1号任务期间进行了双静态雷达测量.
- 测量了雷达回声大小和对比比斯塔特角度 (β) 的偏振.
- 从月球南极PSR与其他月球表面的数据进行了比较.
主要成果:
- 观察到在月球南极的β=0周围明显的相同意义上的极化增强.
- 这种增强局限于PSRs.
- 在定期照亮的表面上没有发现类似的增强,包括北极.
结论:
- 南极的极化增强可能源于体积散射.
- 低损耗体积散射器,可能是水冰,是PSR中观察到的现象的可能解释.
- 这表明在永久阴影的月球区域内存在独特的物质特性.
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