Measures against noise in sensors for prediction of large seismic waves

The paper outlines the measures against noise in detectors for prediction of large seismic waves. According to Einstein´s general theory of relativity, gravitational field turbulence is propagated by light velocity 3×10⁸ (m/s), but on the other hand, the seismic wave itself is propagated by elastic wave velocity 7×10 ³ (m/s). Accordingly, gravitational field turbulence due to a seismic wave reaches an observer instantaneously, whereas the seismic wave arrives much later. Prediction of a large seismic wave can therefore be achieved by observing the gravitational field turbulence. During the observation, optimum filtering plays an important role