Changes in the Fine Structure of Stochastic Distributions As a Consequence of Space-Time Fluctuations.

By Progress in Physics

Changes in the Fine Structure of Stochastic Distributions As a Consequence of Space-Time Fluctuations. - Progress in Physics
  • Release Date: 2006-04-01
  • Genre: Physics

Description

This is a survey of the fine structure stochastic distributions in measurements obtained by me over 50 years. It is shown: (1) The forms of the histograms obtained at each geographic point (at each given moment of time) are similar with high probability, even if we register phenomena of completely different nature--from biochemical reactions to the noise in a gravitational antenna, or a-decay. (2) The forms of the histograms change with time. The iterations of the same form have the periods of the stellar day (1.436 min), the solar day (1.440 min), the calendar year (365 solar days), and the sidereal year (365 solar days plus 6 hours and 9 min). (3) At the same instants of the local time, at different geographic points, the forms of the histograms are the same, with high probability. (4) The forms of the histograms depend on the locations of the Moon and the Sun with respect to the horizon. (5) All the facts are proof of the dependance of the form of the histograms on the location of the measured objects with respect to stars, the Sun, and the Moon. (6) At the instants of New Moon and the maxima of solar eclipses there are specific forms of the histograms. (7) It is probable that the observed correlations are not connected to flow power changes (the changes of the gravity force)--we did not find the appropriate periods in changes in histogram form. (8) A sharp anisotropy of space was discovered, registered by a-decay detectors armed with collimators. Observations at 54 North (the collimator was pointed at the Pole Star) showed no day-long periods, as was also the case for observations at 82 North, near the Pole. Histograms obtained by observations with an Easterly-directed collimator were determined every 718 minutes (half stellar day) and with observations using a Westerly-directed collimator. (9) Collimators rotating counter-clockwise, in parallel with the celestial equator, gave the probability of changes in histograms as the number of the collimator rotations. (10) Collimators rotating clockwise once a day, show no day-long periods, and similarly, collimators pointed at the Pole Star, and measurements taken near the North Pole. All the above lead us to the conclusion (proposition) that the fine structure of the histograms should be a result of the interference of gravitational waves derived from orbital motions of space masses (the planets and stars). Introduction