Figure 8 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 8.

Selected magnetic field lines that show the Parker spiral in 3D. The field lines are colored by the radial velocity. The equatorial plane shows the sign of B _r in black (− sign) and white (+ sign).

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