A locally optimal algorithm for detecting weak low-frequency geophysical signals by the use of long-baseline laser interferometric gravitational antennas that operate in the free spectral range mode is considered. The likelihood ratio is derived using the estimate-correlation online processing of signals. The main element of the optimal detector in the Gaussian approximation is the realizable Wiener filter. A calculation formula for the signal-to-noise ratio is presented.
95.55.Ym Gravitational radiation detectors; mass spectrometers; and other instrumentation and techniques
Sternberg State Astronomical Institute, Universitetskii pr. 13, Moscow, 119991, Russia
Science News of the Faculty of Physics, Lomonosov Moscow State University
This new information publication, which is intended to convey to the staff, students and graduate students, faculty colleagues and partners of the main achievements of scientists and scientific information on the events in the life of university physicists.