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Updated: Jun 21, 2026

10:35
Bringing the Visible Universe into Focus with Robo-AO
Published on: February 12, 2013
概括
来自阿波罗火箭的低频声波在百慕大被检测到. 这些来自高海拔的信号是由稀释大气中的冲击形成理论解释的.
科学领域:
- 声学 声学 在声学方面
- 航空航天工程 航空航天工程
- 大气物理学 大气物理学
背景情况:
- 低频声音现象可能是由高速大气事件产生的.
- 之前的研究已经探索了火箭发射的声学信号,但高空来源仍然不太了解.
研究的目的:
- 调查阿波罗火箭发射期间记录的低频声音的起源和特征.
- 为了确定这些声信号是否可以通过大气冲击波理论来解释.
主要方法:
- 在阿波罗火箭穿越期间,百慕大三方阵列记录的声学数据的分析.
- 信号特征 (连贯性,速度,到达时间,频率) 与火箭轨道数据的比较.
- 动力理论用于稀释大气中的冲击形成和气体动力学冲击理论的应用.
主要成果:
- 连贯的低频声信号多次被记录下来,与阿波罗火箭在188公里高度发射相吻合.
- 信号表现出高,超音速的轨迹速度和一致的特征 (外观,频率,到达时间) 跨阵列.
- 观察到的表面压力变化与高海拔冲击形成的理论模型一致.
结论:
- 记录的低频声音是绝对归因于高空的阿波罗火箭飞行器.
- 综合动力学理论和气体动力学方法成功地解释了观察到的声学现象和表面压力效应.
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