Simulation Outside Magnetic Field of the Sun
Jianqing Wu, Zhiliang Yang
DOI: 10.4236/ijaa.2011.12013   PDF   HTML     4,196 Downloads   8,900 Views  


We derive the viscous current in the fully ionized two-fluid plasma to generate the solar magnetic field. The global magnetic field of the Sun can be simulated by the viscous current from the differential rotation inside the Sun. The field presents a structure with 6-polar. As the viscous current is very weak, the magnetic field intensity is only about G, which could be considered as the background field of the Sun. The theory is a start for the generation of solar magnetic field. The local strong magnetic field of the Sun is not considered in the paper.

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J. Wu and Z. Yang, "Simulation Outside Magnetic Field of the Sun," International Journal of Astronomy and Astrophysics, Vol. 1 No. 2, 2011, pp. 90-97. doi: 10.4236/ijaa.2011.12013.

Conflicts of Interest

The authors declare no conflicts of interest.


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