Science. 1970 Sep 11;169(3950):1071-5. doi: 10.1126/science.169.3950.1071.
The seismic signal caused by the Apollo 12 lunar module is interpreted in terms of propagation between source and receiver through a layer of powder in which sound velocity increases with depth. This increase, which is due to compaction, extends over several kilometers and leads to a concentration of seismic waves toward the surface. Computer simulations with the use of ray acoustics and on the assumption of a randomly undulating lunar surface approximate well the observed signal. Seismic amplitudes are greatly enhanced in such a medium compared to solid rock, so that the observed signal requires less power to be transmitted than previously estimated.
阿波罗 12 号登月舱产生的地震信号,根据通过一层音速随深度增加的粉末层从震源到接收器的传播来解释。这种由于压实而导致的增加延伸了数公里,导致地震波向表面集中。使用射线声学的计算机模拟,并假设月球表面随机波动,很好地逼近了观测到的信号。与固体岩石相比,在这样的介质中,地震幅度大大增强,因此观测到的信号所需的传输功率比以前估计的要小。