Proposed standardization of gravitational burst detector signals

The response of detectors of different mass, length, etc. subjected to the same gravitational perturbation is compared with that caused by a hypothetical pulse of J=(Rsub(iojo) dt different of 0. The correction between J and the area below the largest semi-undulation of Rsub(iojo) (t) is calculated as a function of x (frequency of the Fourier spectrum maximum/resonance frequency of the detector) and of the number of undulations. The energy of an event of total duration D becomes J2d