相关实验视频
Updated: Jul 12, 2026

06:14
Simulating Imaging of Large Scale Radio Arrays on the Lunar Surface
Published on: July 30, 2020
概括
来自月球远端的地震剪切波并未被一些阿波罗空间站检测到. 这表明月球内部,在1000-1100公里深处,可能部分化,类似于地球的天气层.
科学领域:
- * 地震学 关于地震的研究
- *行星科学 *行星科学
- * 月球内部结构
背景情况:
- *阿波罗地震网络提供了关于月球内部结构的关键数据.
- * 了解地震波传播揭示了地下物质的特性.
研究的目的:
- * 为了研究月球内部的地震特性.
- * 为了确定月球地幔是否部分化.
主要方法:
- * 对来自地震事件的直接剪切波到达的分析.
- * 来自阿波罗月球地震网络的地震数据比较.
主要成果:
- * 对于月球背面的事件,在某些地震站没有观察到直接的剪切波到来.
- *月球内部在1000-1100公里深处的地震剪切波消散率高于上面的石化层.
结论:
- *月球内部1000-1100公里深处的月球内部可能对地震剪切波的消散能力更强.
- *这个区域可能存在于部分化状态,类似于地球的天气层.
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