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| Paper: |
Understanding the Solar Inner Magnetism and Dynamics |
| Volume: |
454, The 3rd Hinode Science Meeting |
| Page: |
3 |
| Authors: |
Brun, A. S.; Strugarek, A. |
| Abstract: |
The observations of solar magnetic activity by the satellite Hinode confirm the large range of spatial and temporal
scales present on the Sun's surface and the complexity of the flows and fields. How such magnetic field is generated, amplified, maintained and emerge
over the course of the solar cycle is key to determine in order to progress in our understanding of the Sun. It is believed that dynamo action in and at the base of the convective envelope
is the main source of solar magnetism. Further the radiative interior of the Sun may also posses a primordial field whose influences
on the dynamo generated field needs to be studied. We propose in this paper to make a brief review of our effort
to model in 3-D the Sun's inner magnetism and the coupling between its convective and radiative zones and how such magnetism
may emerge at the solar surface. |
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