Waveforms generated by the 50t explosion of project Brightlight(Ⅰ) were recorded by HILR array.Using array techniques,the author performed identification,f-k analysis,velocity spectrum analysis,etc.of the weak signals.The analysis results show that the signal-to-noise ratio after beamforming was obviously enhanced,and the signal could be clearly shown.The energy from this explosion was mainly concentrated in the 1 ~ 8Hz range from f-k analysis.The velocity spectrum gave clear positions of event phases,which could not be seen in the original weak signals.The maximum energy distribution obtained by the Beaman method is close to the theoretical value in the azimuth-slowness domain. 相似文献
In an earlier paper, values of exospheric density were obtained from the orbit of Echo 2 for the years 1964–1965. The results indicated a semi-annual variation in density by a factor of between 2 and 3, considerably larger than predicted by existing atmospheric models.
These studies have now been extended to the beginning of 1967, using both Echo 2 and Calsphere 1, to show how the density is responding to increasing solar activity. Variations in density during 1964 have been analysed in more detail. The long-term variation associated with the solar cycle and the short-term variations associated with magnetic and solar disturbances agree with the variations expected on the basis of current models. The semi-annual variation is persisting to higher levels of solar activity, and although its amplitude is diminishing the factor of variation was still 1.6 in 1966. 相似文献