Experimental Verification of Kozyrev's Interaction of Natural Processes: Difference between revisions
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A setup has been devised to measure the effect of Kozyrev's interaction of natural geophysical and solar processes, treated as macroscopic non-locality. The detectors used in the setup have efficiency three orders of magnitude better than ones used before. Exhaustive steps have been taken to control noise-forming factors and protect the detectors against them. As a result, effects of non-social influences of several large-scale processes related with weather changes, geomagnetic variations, ionospheric and solar activity have been reliably detected. A large advanced lag has been found in a number of processes, which might be used in the geophysical forecasts.[[Category:Scientific Paper]] | A setup has been devised to measure the effect of Kozyrev's interaction of natural geophysical and solar processes, treated as macroscopic non-locality. The detectors used in the setup have efficiency three orders of magnitude better than ones used before. Exhaustive steps have been taken to control noise-forming factors and protect the detectors against them. As a result, effects of non-social influences of several large-scale processes related with weather changes, geomagnetic variations, ionospheric and solar activity have been reliably detected. A large advanced lag has been found in a number of processes, which might be used in the geophysical forecasts. | ||
[[Category:Scientific Paper|experimental verification kozyrev 's interaction natural processes]] | |||
Latest revision as of 13:24, 1 January 2017
| Scientific Paper | |
|---|---|
| Title | Experimental Verification of Kozyrev\'s Interaction of Natural Processes |
| Author(s) | S M Korotaev |
| Keywords | {{{keywords}}} |
| Published | 2000 |
| Journal | Galilean Electrodynamics |
| Volume | 11 |
| Number | S2 |
| Pages | 23-28 |
Abstract
A setup has been devised to measure the effect of Kozyrev's interaction of natural geophysical and solar processes, treated as macroscopic non-locality. The detectors used in the setup have efficiency three orders of magnitude better than ones used before. Exhaustive steps have been taken to control noise-forming factors and protect the detectors against them. As a result, effects of non-social influences of several large-scale processes related with weather changes, geomagnetic variations, ionospheric and solar activity have been reliably detected. A large advanced lag has been found in a number of processes, which might be used in the geophysical forecasts.