[Paper Review] On the characteristic form of histograms appearing at the culmination of solar eclipse

S. E. Shnoll, V. A. Panchelyuga|ArXiv.org|Mar 5, 2006

Geophysics and Gravity Measurements12 references3 citations

TL;DR

This paper investigates the emergence of distinct, consistent histogram forms in fluctuation data during solar eclipses, demonstrating that these patterns appear simultaneously worldwide regardless of geographic location or process type. The authors propose that these forms arise from spacetime fluctuations influenced by celestial mechanics, particularly the geocentric alignment of the Sun and Moon, suggesting a cosmophysical origin for non-random variations in physical measurements.

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 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.

Motivation & Objective

• To investigate whether specific histogram forms emerge during solar eclipses across diverse geographical locations.
• To determine if these histogram forms are independent of the physical process being measured or local conditions.
• To explore the hypothesis that these patterns stem from spacetime fluctuations influenced by celestial body positions.
• To compare the histogram forms observed during solar eclipses with those seen during new moons, as previously documented.
• To establish whether the observed effects are due to tidal forces or require novel cosmophysical explanations.

Proposed method

• Data collection from multiple global noise generators in the GCP network during solar eclipse events.
• Analysis of amplitude fluctuation histograms from various physical processes (e.g., radioactive decay, biochemical reactions, electronic noise).
• Synchronization of observations with precise timing of the geocentric solar-lunar conjunction during eclipses.
• Comparison of histogram shapes across different latitudes and longitudes to assess spatial uniformity.
• Use of statistical pattern recognition to identify recurring, characteristic forms in the fluctuation distributions.
• Application of cosmophysical models to interpret the observed histogram forms as reflections of spacetime fluctuations.

Experimental results

Research questions

• RQ1 Do characteristic histogram forms appear simultaneously during solar eclipses across the globe, independent of location or process type?
• RQ2 How do the histogram forms observed during solar eclipses differ from those observed during new moons?
• RQ3 Are the observed histogram patterns attributable to tidal forces or do they require a deeper cosmophysical explanation?
• RQ4 Is the timing of the histogram form's appearance correlated with the precise moment of geocentric solar-lunar alignment?
• RQ5 Can the universal occurrence of these forms be explained by fluctuations in spacetime influenced by celestial body motion?

Key findings

• Specific, reproducible histogram forms consistently appear at the culmination of solar eclipses across diverse geographical locations, from the Arctic to the Antarctic.
• These histogram forms are independent of the nature of the physical process being measured, indicating a universal underlying mechanism.
• The forms appear simultaneously worldwide, suggesting a non-local, cosmophysically driven phenomenon rather than a local or terrestrial effect.
• The histogram patterns observed during solar eclipses are distinct from those seen during new moons, indicating different physical conditions or influences.
• The results challenge conventional explanations based on tidal forces and suggest a deeper connection between spacetime fluctuations and celestial mechanics.