Q FOR SHORT-PERIOD P-WAVES - IS IT FREQUENCY-DEPENDENT - REPLY

被引:1
|
作者
DOUGLAS, A
机构
[1] MOD(PE), Reading, RG7 4RS, Blacknest, Brimpton
关键词
D O I
10.1111/j.1365-246X.1993.tb00907.x
中图分类号
P3 [地球物理学]; P59 [地球化学];
学科分类号
0708 ; 070902 ;
摘要
Using network averaged spectra Murphy (1989) demonstrates that if it is assumed that the source functions of explosions at Pahute Mesa, Nevada Test Site (NTS) are as predicted by the Mueller‐Murphy (M‐M) source model then the average t* at around 1 Hz for P waves radiated from the test site must be about 0.75 s. With this value of t* Murphy (1989) estimates the best fitting M‐M spectrum for each explosion studied, by adjusting A, to & c; A & to being the amplitude and delay time of pP relative to P and c the wave speed for the material in which the explosion was fired. The absolute amplitudes of the theoretical spectra are obtained using a calibration factor estimated from the data. Murphy (1993) extends the analysis to explosions in granite at the Nevada, French Sahara and E. Kazakh test sites. For the French Sahara explosion t* is assumed to be 0.75 s (Murphy's estimate for NTS explosions), and for the E. Kazakh explosion a t* of 0.55 s is used. For the French Sahara and E. Kazakh explosions Murphy (1993) shows that by using the same calibration factor as for the NTS it is possible by varying A & to to fit the estimated average network spectra using the M‐M granite source. Murphy (1993) states that the amplitudes and spectra for the largest NTS explosion in granite (PILE DRIVER) can also be predicted using the M‐M model but these results are not shown. Copyright © 1993, Wiley Blackwell. All rights reserved
引用
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页码:541 / 542
页数:2
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