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E. N. Parker, “Cosmical Magnetic Fields: Their Origin and Their Activity,” Oxford University Press, New York, 1979, pp. 40-90.

has been cited by the following article:

• TITLE: Simulation Outside Magnetic Field of the Sun

  AUTHORS: Jianqing Wu, Zhiliang Yang

  KEYWORDS: Solar Dynamo, Two-Fluid, Viscous Current

  JOURNAL NAME: International Journal of Astronomy and Astrophysics, Vol.1 No.2, July 5, 2011

  ABSTRACT: 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.