SOLAR SYSTEM OSCILLATIONS AND MODELS OF NATURAL PROCESSES

dc.contributor.author	Berry B.L.
dc.date.accessioned	2025-02-08T08:30:14Z
dc.date.available	2025-02-08T08:30:14Z
dc.date.issued	2006
dc.description.abstract	Tidal and momentum interactions of the bodies of the solar system create stable oscillations of the momenta of inertia of the Sun and planets. The laws of momentum conservation are the reasons for synchronous oscillations, which are observed in geodynamic, solar and climatic processes. The stable harmonics of the processes have to be detected from representative sets of helio-geophysical data. The regular parts of natural processes can be modelled by the sum of the stable harmonics. © 2005 Elsevier Ltd. All rights reserved.
dc.identifier	https://www.elibrary.ru/item.asp?id=31336510
dc.identifier.citation	Journal of Geodynamics, 2006, 41, 1-3, 133-139
dc.identifier.doi	10.1016/j.jog.2005.08.027
dc.identifier.issn	0264-3707
dc.identifier.uri	https://repository.geologyscience.ru/handle/123456789/47942
dc.subject	HARMONIC MODELS
dc.subject	SOLAR ACTIVITY
dc.subject	STABLE OSCILLATIONS
dc.subject	TERRESTRIAL PROCESSES
dc.subject	SOLAR SYSTEM
dc.title	SOLAR SYSTEM OSCILLATIONS AND MODELS OF NATURAL PROCESSES
dc.type	Статья

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