DocumentCode
3065922
Title
Prediction of great seismic waves by gravitational wave detectors. II. Noise and sensitivity of detectors
Author
Chiba, J. ; Obata, Tsunehiro
Author_Institution
Dept. of Electr. Eng., Tohoku Univ., Sendai, Japan
fYear
1991
fDate
1-3 Oct 1991
Firstpage
285
Lastpage
289
Abstract
The prediction of a large seismic wave can be done according to gravitational field turbulence, which travels at the speed of light. The authors describe the sensitivity and noise of the corresponding gravitational wave detector. When an earthquake has a magnitude of seven, the gravitational deviation induces a detectable strain in the antenna bar. Accordingly, seismic waves can be detected by a gravitational wave antenna before their arrival and therefore be used in the prediction. Assuming a large earthquake with a 100 km epicenter distance from a city, the seismic waves take at least 14 s to arrive at the city. If people in the city had foreknowledge of the earthquake by observing the gravitational field turbulence generated by the seismic waves, they would be warned of the arrival before the seismic waves approached half the distance, and would be able to take emergency actions, at least 7 s before their arrival
Keywords
earthquakes; geophysical techniques; gravitational wave detectors; noise; seismic waves; sensitivity; antenna bar; city; detector noise; detector sensitivity; earthquake; emergency actions; gravitational field turbulence; gravitational wave detectors; seismic wave prediction; strain; Calibration; Capacitive sensors; Detectors; Engine cylinders; Motion detection; Optical propagation; Seismic waves; Solids; Tellurium; Tires;
fLanguage
English
Publisher
ieee
Conference_Titel
Security Technology, 1991. Proceedings. 25th Annual 1991 IEEE International Carnahan Conference on
Conference_Location
Taipei
Print_ISBN
0-7803-0120-X
Type
conf
DOI
10.1109/CCST.1991.202226
Filename
202226
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