Abstract
Resonant gravitational antennas with slow filtering are considered and characteristics are calculated for a parametric model for the a priori uncertainty in the class of ε-corrupted distributions in the presence of wide-band chaotic pulsed Poisson interference.
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Translated from Izmeritel’naya Tekhnika, No. 5, pp. 5–8, May, 2006.
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Gusev, A.V. Resonance gravitational antennas: Pulse interference. Meas Tech 49, 419–424 (2006). https://doi.org/10.1007/s11018-006-0125-5
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DOI: https://doi.org/10.1007/s11018-006-0125-5