The solar dynamo and its phase transitions during the last millennium
We analyze the variation of the solar-dynamo magnetic-field components during the last millennium through a study of their proxy data. We introduce a phase diagram with as abscissa and ordinate the proxies of the values of the toroidal and poloidal magnetic field components. In this diagram the dyna...
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paper:paper_00380938_v250_n1_p1_Duhau2023-06-08T15:02:42Z The solar dynamo and its phase transitions during the last millennium Duhau de Romero, Silvia We analyze the variation of the solar-dynamo magnetic-field components during the last millennium through a study of their proxy data. We introduce a phase diagram with as abscissa and ordinate the proxies of the values of the toroidal and poloidal magnetic field components. In this diagram the dynamo system appears to regularly cross a well-defined point, which we call the Transition Point. Such crossings occurred five times during the past millennium. Each of these crossings preceded a Grand Episode, either a Minimum or a Maximum one. In addition to these two types of quasiperiodic behavior, a third type consisting of weaker quasiregular oscillations (R) around the Transition Point's coordinates is identified. These periods appear to last one or two times the Gleissberg cycle length. Between the various types of episodes there are brief phase transitions. We identify two types of such phase transitions. © 2008 Springer Science+Business Media B.V. Fil:Duhau, S. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales; Argentina. 2008 https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00380938_v250_n1_p1_Duhau http://hdl.handle.net/20.500.12110/paper_00380938_v250_n1_p1_Duhau |
institution |
Universidad de Buenos Aires |
institution_str |
I-28 |
repository_str |
R-134 |
collection |
Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) |
description |
We analyze the variation of the solar-dynamo magnetic-field components during the last millennium through a study of their proxy data. We introduce a phase diagram with as abscissa and ordinate the proxies of the values of the toroidal and poloidal magnetic field components. In this diagram the dynamo system appears to regularly cross a well-defined point, which we call the Transition Point. Such crossings occurred five times during the past millennium. Each of these crossings preceded a Grand Episode, either a Minimum or a Maximum one. In addition to these two types of quasiperiodic behavior, a third type consisting of weaker quasiregular oscillations (R) around the Transition Point's coordinates is identified. These periods appear to last one or two times the Gleissberg cycle length. Between the various types of episodes there are brief phase transitions. We identify two types of such phase transitions. © 2008 Springer Science+Business Media B.V. |
author |
Duhau de Romero, Silvia |
spellingShingle |
Duhau de Romero, Silvia The solar dynamo and its phase transitions during the last millennium |
author_facet |
Duhau de Romero, Silvia |
author_sort |
Duhau de Romero, Silvia |
title |
The solar dynamo and its phase transitions during the last millennium |
title_short |
The solar dynamo and its phase transitions during the last millennium |
title_full |
The solar dynamo and its phase transitions during the last millennium |
title_fullStr |
The solar dynamo and its phase transitions during the last millennium |
title_full_unstemmed |
The solar dynamo and its phase transitions during the last millennium |
title_sort |
solar dynamo and its phase transitions during the last millennium |
publishDate |
2008 |
url |
https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00380938_v250_n1_p1_Duhau http://hdl.handle.net/20.500.12110/paper_00380938_v250_n1_p1_Duhau |
work_keys_str_mv |
AT duhauderomerosilvia thesolardynamoanditsphasetransitionsduringthelastmillennium AT duhauderomerosilvia solardynamoanditsphasetransitionsduringthelastmillennium |
_version_ |
1768544769381761024 |