Cosmo-physical effects in the time series of the GCP network

S. E. Shnoll; V. A. Panchelyuga

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Cosmo-physical effects in the time series of the GCP network

S. E. Shnoll·V. A. Panchelyuga

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Abstract

In the GCP network, an Internet system of noise generators developed under the direction of Prof. R. Nelson and deployed at various geographical points, synchronous measurements of a priori random noise processes are carried out every second. The time series obtained in these measurements are "quite random" from the viewpoint of traditional methods of statistical analysis. However, as shown in our works, using the method of histogram comparison allows one to discover clear regularities in the noise processes of any nature, from biochemical reactions to radioactive decay or noise in the gravitational antenna. These regularities cannot be revealed by the traditional methods of time series analysis and seem to be determined by fluctuations of the space-time, which result from the movement of the "laboratory" relative to the mass thicknesses (celestial bodies). The application of this method to the analysis of time series of the GCP system showed all the main regularities described earlier: the histogram pattern changes with well-resolved sidereal and solar daily periods; at different geographical points, similar histogram patterns are highly probable to appear at the same local time; histograms with a specific "eclipse" pattern appear synchronously "all over the Earth" at the moments of culmination of a solar eclipse.

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S. E. Shnoll, V. A. Panchelyuga. 2006-05-07. Cosmo-physical effects in the time series of the GCP network. https://arxiv.org/abs/physics/0605064

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