Kondratyev, K. Ya. and Nikolsky, G. A. (2006) Further about impact of solar activity on geospheres. Il nuovo cimento C, 29 (6). pp. 695-708. ISSN 1826-9885
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Abstract
Twenty-five years high-mountainous researches on solar-weather effects have given a number of direct proofs of the occurrence of weather meteoelements abnormal responses (in scale hours-days-week) on the passage in the central area of the solar disk by separate large sunspots and powerful groups of spots. The brightest shows were marked by us in October 1981 and in the last decade of October 2003. Certainly, the most grandiose effect was registered in March 1920 at the Calama station of the Smithonian Astrophysical Observatory (ΔS0 ≈ 5%). The analysis of the data set unambiguously has specified the presence of a special kind of radiation in the solar emissions—spirally vortical radiation (SVR), having a forcible pulse and powerful angular moment. In our opinion spirally vortical radiation is generated in the nu cleu s of the Su n with a speed of 104 quantums/s and leaves the photosphere through magnetic structures with a speed ∼ 8–9 · 103 km/s. In the paper we discuss the effects of the direct interaction of spirally vortical radiation with different kinds of terrestrial environments, including the biosphere. It is supposed that SVR in the Universe can play a role of dark energy, as it is radiated by each star and has a pulse.
| Item Type: | Article |
|---|---|
| Uncontrolled Keywords: | Solar physics ; Electric and magnetic fields, solar magnetism ; Helioseismology, pulsations, and shock waves |
| Subjects: | 500 Scienze naturali e Matematica > 530 Fisica |
| Depositing User: | Marina Spanti |
| Date Deposited: | 19 Mar 2020 14:58 |
| Last Modified: | 19 Mar 2020 14:58 |
| URI: | http://eprints.bice.rm.cnr.it/id/eprint/16126 |
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