Simulating Solar Global Magnetism in 3-D
2012 ◽
Vol 10
(H16)
◽
pp. 101-103
Keyword(s):
The Mean
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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.
1976 ◽
Vol 71
◽
pp. 305-321
Keyword(s):
2012 ◽
Vol 428
(1)
◽
pp. 470-475
◽
Keyword(s):
1998 ◽
Vol 185
◽
pp. 463-464
1993 ◽
Vol 157
◽
pp. 49-50
1995 ◽
Vol 12
(2)
◽
pp. 180-185
◽
Keyword(s):
1987 ◽
Vol 178
◽
pp. 521-534
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