Astronomy and Astrophysics – Astrophysics – Solar and Stellar Astrophysics
Scientific paper
2009-12-26
Astrophys.Space Sci.328:295-300,2010
Astronomy and Astrophysics
Astrophysics
Solar and Stellar Astrophysics
Accepted for publication on Astrophysics and Space Science
Scientific paper
10.1007/s10509-009-0244-y
Understanding the reasons of the cyclic variation of the total solar irradiance is one of the most challenging targets of modern astrophysics. These studies prove to be essential also for a more climatologic issue, associated to the global warming. Any attempt to determine the solar components of this phenomenon must include the effects of the magnetic field, whose strength and shape in the solar interior are far from being completely known. Modelling the presence and the effects of a magnetic field requires a 2D approach, since the assumption of radial symmetry is too limiting for this topic. We present the structure of a 2D evolution code that was purposely designed for this scope; rotation, magnetic field and turbulence can be taken into account. Some preliminary results are presented and commented.
Basu Sarbani
Demarque Pierre
Li Lexin
Penza Valentina
Sofia Sabatino
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