Inertial oscillations in the solar convection zone. II - A cylindrical model for equatorial regions

1985 ◽  
Vol 296 ◽  
pp. 685 ◽  
Author(s):  
P. A. Gilman ◽  
D. B. Guenther
Keyword(s):  
Convection Zone ◽  
Inertial Oscillations ◽  
Solar Convection Zone ◽  
Cylindrical Model ◽  
Solar Convection ◽  
Zone Ii

Emerging Flux Tubes in the Solar Convection Zone. II. The Influence of Initial Conditions

1998 ◽  
Vol 502 (1) ◽  
pp. 481-492 ◽  
Author(s):  
P. Caligari ◽  
M. Schussler ◽  
F. Moreno‐Insertis
Keyword(s):  
Convection Zone ◽  
Initial Conditions ◽  
Solar Convection Zone ◽  
Flux Tubes ◽  
Solar Convection ◽  
Zone Ii

scholarly journals Can short time delays influence the variability of the solar cycle?

2010 ◽  
Vol 6 (S271) ◽  
pp. 288-296
Author(s):  
Laurène Jouve ◽  
Michael R. E. Proctor ◽  
Geoffroy Lesur
Keyword(s):  
Solar Cycle ◽  
Convection Zone ◽  
Mean Field ◽  
Period Doubling ◽  
Temporal Modulation ◽  
Solar Convection Zone ◽  
Flux Tubes ◽  
Solar Convection ◽  
Short Time ◽  
Period Doubling Bifurcations

AbstractWe present the effects of introducing results of 3D MHD simulations of buoyant magnetic fields in the solar convection zone in 2D mean-field Babcock-Leighton models. In particular, we take into account the time delay introduced by the rise time of the toroidal structures from the base of the convection zone to the solar surface. We find that the delays produce large temporal modulation of the cycle amplitude even when strong and thus rapidly rising flux tubes are considered. The study of a reduced model reveals that aperiodic modulations of the solar cycle appear after a sequence of period doubling bifurcations typical of non-linear systems. We also discuss the memory of such systems and the conclusions which may be drawn concerning the actual solar cycle variability.

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