On the characteristic form of histograms appearing at the culmination of solar eclipse
S.E. Shnoll, V.A. Panchelyuga

TL;DR
This paper investigates the characteristic forms of histograms of amplitude fluctuations during solar eclipses, revealing that these forms are globally synchronized and influenced by spacetime fluctuations related to celestial movements.
Contribution
It demonstrates that histogram forms during solar eclipses are distinct, globally synchronized, and depend on celestial alignments, suggesting a cosmophysical influence on noise distributions.
Findings
Histogram forms appear during solar eclipses at all locations simultaneously.
These forms differ from those observed during new moons.
The phenomenon is independent of geographical location and process type.
Abstract
As shown in a number of our works, the form of histograms - distributions of amplitude fluctuations - varies regularly in time, with these variations being similar for processes of any nature, from biochemical reactions to noise in the gravitational antenna and all types of the radioactive decay. In particular, we have revealed basic laws, suggesting a cosmo-physical nature of these phenomena, in the time series created by the noise generators of the global GCP net. On the basis of all the results obtained, a conclusion has been made that the histogram form is determined by fluctuations of the spacetime, which depend on the movement of the measured system (laboratory) relative to the heavenly bodies. An important step to understand the nature of these phenomena was the finding that at the moments of the new Moon, a specific histogram form appears practically simultaneously at different…
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Taxonomy
TopicsGeophysics and Gravity Measurements
