THE SIGNAL-NOISE RATIO CRITERION WHEN DETECTING WEAK GRAVITATIONAL IMPULSES ON A BACKGROUND OF NON-GAUSSIAN INTERFERENCE

摘要

The optimum scheme for processing data at the output of the linear channel of resonant gravitational antennas from the point of view of the signal-noise ratio criterion, when detecting weak quasideterministic gravitational pulses in the presence of corrected non-Gaussian "mechanical" interference, is considered.