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 |
|