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Instituto de Geofisica, UNAM National University of Mexico, 04510 Mexico, D.F.
Abstract
The amplification of a strainmeter is frequency dependent. As the wavelength
approaches the length L of the strainmeter, the amplitude vanishes, because the two extremes of the strainmeter are in phase. The sign of the response is inverted at zero crossings such that
= L/n, n = 1, 2,.... Between L <
< 2L, the amplitude of an incoming signal may be reduced by 60% or more. Filtering of the output may worsen the problem. Thus, strainmeters may be poorly suited for certain research purposes, including surface-wave studies and first-motion studies. The output of long-base strainmeters sited on low-velocity materials (such as the 732-m-long strainmeters at Piñon Flat Observatory) may require correction for amplitude distortion.
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