Laser perturbation by directional signals

Michele Zanoni

Laser light perturbation by directional signals

Abstract Similar and coincidental signals at a particular frequency were
recorded simultaneously from two or three optical sensors piloted by a laser
diode at distances up to hundreds of kilometers. Some of the signal’s forms
repeat at approximately the same time over the course of a two to three day
period. This paper presents and discusses the data collected during a long
period of observation (from October 2005 to January 2008). Studying the
symmetry of the time series plot, three particular directions of the incoming
signals were identified: RA 15h 35m ± 10m, RA 17h 22m ± 40m and RA
23h ± 40m. These three directions (if using only the RA coordinate) point
respectively to the Great Attractor zone, to an area close to the center of the
Galaxy and to the area opposite to the Virgo Cluster. In order to explain
the observed phenomena a few hypotheses have been formulated and inter-
preted. It is remarkable that the directions detected in our experiment are
in agreement with the estimates quoted in literature. A new possible mecha-
nism explaining the laser light fluctuations was finally identified and a naive
model based on this mechanism was developed in order to find out not only
the AR coordinates of the sources but also their declinations. The results of
this analysis confirm the quoted directions.

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