We define the solar cycle as a spatiotemporal rather than a purely temporal entity. This allows us to introduce new methods to determine timing parameters of the activity cycles. We discuss the physical interpretation of our spatiotemporal definition as a pair of activity waves travelling towards the equator and pole respectively, and present results of the corresponding statistical analysis. Three important trends of solar activity which are clearly seen in summary statistics can be used for prediction. We present evidence of a long term cycle of 90 years manifesting as a modulation of both length and symmetry of the Schwabe cycle and identify this with the Gleissberg cycle
Context. The study of solar activity over long time intervals using proxies. Aims. The peri...
Abstract Aims: The 11-year solar cycle (Schwabe cycle) is the dominant pattern of solar magnetic ac...
Aims. The 11-year solar cycle (Schwabe cycle) is the dominant pattern of solar magnetic activity ref...
International audienceWe show in this short note that the method of singular spectrum analysis (SSA)...
The solar equatorial rotation rate, determined from sunspot group data during the period 1879-2004, ...
Aims. The spatio-temporal dynamics of solar activity has been investigated by studying the main osci...
Aims. The revised dataset of sunspot and group numbers (released by WDC-SILSO) and the sunspot numbe...
Contains fulltext : 207560.pdf (publisher's version ) (Open Access)Sunspot number ...
The solar cycle is reviewed. The 11-year cycle of solar activity is characterized by the rise and fa...
Abstract One obvious feature of the solar cycle is its variation from one cycle to another. In this ...
A solar activity cycle of about 2400 years has until now been of uncertain origin. Recent results i...
The Schwabe frequency band of the Zurich sunspot record since 1749 is found to be made of three majo...
The Solar Cycle is reviewed. The 11-year cycle of solar activity is characterized by the rise and fa...
Abstract. The sunspot number series forms the longest directly observed index of solar activity and ...
Aims.The problem of the unusual sunspot cycle in 1784–1799 is considered. Why was the length of the ...
Context. The study of solar activity over long time intervals using proxies. Aims. The peri...
Abstract Aims: The 11-year solar cycle (Schwabe cycle) is the dominant pattern of solar magnetic ac...
Aims. The 11-year solar cycle (Schwabe cycle) is the dominant pattern of solar magnetic activity ref...
International audienceWe show in this short note that the method of singular spectrum analysis (SSA)...
The solar equatorial rotation rate, determined from sunspot group data during the period 1879-2004, ...
Aims. The spatio-temporal dynamics of solar activity has been investigated by studying the main osci...
Aims. The revised dataset of sunspot and group numbers (released by WDC-SILSO) and the sunspot numbe...
Contains fulltext : 207560.pdf (publisher's version ) (Open Access)Sunspot number ...
The solar cycle is reviewed. The 11-year cycle of solar activity is characterized by the rise and fa...
Abstract One obvious feature of the solar cycle is its variation from one cycle to another. In this ...
A solar activity cycle of about 2400 years has until now been of uncertain origin. Recent results i...
The Schwabe frequency band of the Zurich sunspot record since 1749 is found to be made of three majo...
The Solar Cycle is reviewed. The 11-year cycle of solar activity is characterized by the rise and fa...
Abstract. The sunspot number series forms the longest directly observed index of solar activity and ...
Aims.The problem of the unusual sunspot cycle in 1784–1799 is considered. Why was the length of the ...
Context. The study of solar activity over long time intervals using proxies. Aims. The peri...
Abstract Aims: The 11-year solar cycle (Schwabe cycle) is the dominant pattern of solar magnetic ac...
Aims. The 11-year solar cycle (Schwabe cycle) is the dominant pattern of solar magnetic activity ref...