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dc.contributor.author | Demin S. | |
dc.contributor.author | Nefedyev Y. | |
dc.contributor.author | Andreev A. | |
dc.contributor.author | Demina N. | |
dc.contributor.author | Timashev S. | |
dc.date.accessioned | 2019-01-22T20:36:24Z | |
dc.date.available | 2019-01-22T20:36:24Z | |
dc.date.issued | 2018 | |
dc.identifier.issn | 0273-1177 | |
dc.identifier.uri | https://dspace.kpfu.ru/xmlui/handle/net/147938 | |
dc.description.abstract | © 2017 COSPAR The analysis of turbulent processes in sunspots and pores which are self-organizing long-lived magnetic structures is a complicated and not yet solved problem. The present work focuses on studying such magneto-hydrodynamic (MHD) formations on the basis of flicker-noise spectroscopy using a new method of multi-parametric analysis. The non-stationarity and cross-correlation effects taking place in solar activity dynamics are considered. The calculated maximum values of non-stationarity factor may become precursors of significant restructuring in solar magnetic activity. The introduced cross-correlation functions enable us to judge synchronization effects between the signals of various solar activity indicators registered simultaneously. | |
dc.relation.ispartofseries | Advances in Space Research | |
dc.subject | Methods: multi-parametric analysis | |
dc.subject | Non-stationarity and cross-correlation effects | |
dc.subject | Solar activity | |
dc.subject | Sun: magnetic fields | |
dc.subject | Sunspots | |
dc.title | Non-stationarity and cross-correlation effects in the MHD solar activity | |
dc.type | Article | |
dc.relation.ispartofseries-issue | 2 | |
dc.relation.ispartofseries-volume | 61 | |
dc.collection | Публикации сотрудников КФУ | |
dc.relation.startpage | 639 | |
dc.source.id | SCOPUS02731177-2018-61-2-SID85025140246 |