On the characteristic form of histograms appearing at the culmination of solar eclipse

• Main Authors: Shnoll, S E, Panchelyuga, V A
• Language: English
• Published: 2006
• Subjects: Other Fields of Physics; Antarctic; Arctic; Antarc*
• Online Access: http://cds.cern.ch/record/933630

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 geographical points, from Arctic to Antarctic, in middle latitudes of West and East hemispheres. This effect seems to be not due to a change of the tide-generating forces; to explain it, nontrivial hypotheses are needed. The present paper shows the appearance of specific histogram forms at the culminations of the solar eclipses (moments of the geocentric superposition of the Sun and the Moon), with the eclipse forms differing from the new-moon ones. Specific histogram forms appear practically simultaneously all over the Earth and depend nor on the geographical coordinates, nor on the nature of the process studied.