Figure 4 from A Data-driven, Two-temperature Solar Wind Model with Alfvén Waves

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A Data-driven, Two-temperature Solar Wind Model with Alfvén Waves

Authors: B. van der Holst, W. B. Manchester IV, R. A. Frazin, A. M. Vásquez, G. Tóth, and T. I. Gombosi

VAN DER HOLST et al. 2010 The Astrophysical Journal 725 1373.

Provider: AAS Journals

Caption: Figure 4.

Three-dimensional magnetic field topology showing a few selected field lines of the helmet streamer and coronal hole. The signed radial magnetic field strength at r = 1.05 R _☉ is shown in color contour.

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