Solar activity (SA) oscillations over the past millennia are analyzed and extrapolated based on reconstructed solar-related records. Here, simple recurrent models of SA signal are applied and tested. The consequent results strongly suggest the following: (a) the existence of multi-millennial ( ∼ 9500-year) scale solar patterns linked with planetary gravitational forcing (PGF), and (b) their persistence, over at least the last glacial–interglacial cycle, but possibly since the Miocene (10.5 Myr ago). This empirical modeling of solar recurrent patterns has also provided a consequent multi-millennial-scale experimental forecast, suggesting a solar decreasing trend toward grand (super) minimum conditions for the upcoming period, A...
Using a special technique of data analysis, we have found 34 grand minima of solar activity in a 770...
Some intriguing statistical evidence from readily available data suggests that longer-term (>11-year...
We have examined the long-term trends in the solar variability that can be deduced from some indirec...
The Schwabe frequency band of the Zurich sunspot record since 1749 is found to be made of three majo...
The Schwabe frequency band of the Zurich sunspot record since 1749 is found to be made of three majo...
The Schwabe frequency band of the Zurich sunspot record since 1749 is found to be made of three majo...
Abstract Presented here is a review of present knowledge of the long-term behavior of solar activity...
Observations of solar activity (Wolf sunspot numbers) last only about 250 years, moreover, from spor...
As our civilization depends increasingly on space-borne assets and on a delicate and vulnerable eart...
International audienceAims. The Sun shows strong variability in its magnetic activity, from Grand mi...
Aims. Using a reconstruction of sunspot numbers stretching over multiple millennia, we analyze the s...
The recent decline in the open magnetic flux of the Sun heralds the end of the Grand Solar Maximum (...
ABSTRACT Aims. The Sun shows strong variability in its magnetic activity, from Grand minima to Grand...
Aims.Using a reconstruction of sunspot numbers stretching over multiple millennia, we analyze the st...
The sun is quite variable in time. When the solar activity is numerated by counting sunspots in numb...
Using a special technique of data analysis, we have found 34 grand minima of solar activity in a 770...
Some intriguing statistical evidence from readily available data suggests that longer-term (>11-year...
We have examined the long-term trends in the solar variability that can be deduced from some indirec...
The Schwabe frequency band of the Zurich sunspot record since 1749 is found to be made of three majo...
The Schwabe frequency band of the Zurich sunspot record since 1749 is found to be made of three majo...
The Schwabe frequency band of the Zurich sunspot record since 1749 is found to be made of three majo...
Abstract Presented here is a review of present knowledge of the long-term behavior of solar activity...
Observations of solar activity (Wolf sunspot numbers) last only about 250 years, moreover, from spor...
As our civilization depends increasingly on space-borne assets and on a delicate and vulnerable eart...
International audienceAims. The Sun shows strong variability in its magnetic activity, from Grand mi...
Aims. Using a reconstruction of sunspot numbers stretching over multiple millennia, we analyze the s...
The recent decline in the open magnetic flux of the Sun heralds the end of the Grand Solar Maximum (...
ABSTRACT Aims. The Sun shows strong variability in its magnetic activity, from Grand minima to Grand...
Aims.Using a reconstruction of sunspot numbers stretching over multiple millennia, we analyze the st...
The sun is quite variable in time. When the solar activity is numerated by counting sunspots in numb...
Using a special technique of data analysis, we have found 34 grand minima of solar activity in a 770...
Some intriguing statistical evidence from readily available data suggests that longer-term (>11-year...
We have examined the long-term trends in the solar variability that can be deduced from some indirec...