Comparative study of ring current development using empirical, dipolar, and self-consistent magnetic field simulations

2010 ◽  
Vol 115 (A12) ◽  
pp. n/a-n/a ◽  
Author(s):  
V. K. Jordanova ◽  
S. Zaharia ◽  
D. T. Welling
2012 ◽  
Vol 117 (A9) ◽  
pp. n/a-n/a ◽  
Author(s):  
Margaret W. Chen ◽  
Colby L. Lemon ◽  
Timothy B. Guild ◽  
Michael Schulz ◽  
James L. Roeder ◽  
...  

2004 ◽  
Vol 31 (21) ◽  
pp. n/a-n/a ◽  
Author(s):  
C. Lemon ◽  
R. A. Wolf ◽  
T. W. Hill ◽  
S. Sazykin ◽  
R. W. Spiro ◽  
...  

2012 ◽  
Vol 10 (H16) ◽  
pp. 101-103
Author(s):  
A. S. Brun ◽  
A. Strugarek

AbstractWe briefly present recent progress using the ASH code to model in 3-D the solar convection, dynamo and its coupling to the deep radiative interior. We show how the presence of a self-consistent tachocline influences greatly the organization of the magnetic field and modifies the thermal structure of the convection zone leading to realistic profiles of the mean flows as deduced by helioseismology.


Sign in / Sign up

Export Citation Format

Share Document