Figure 11 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 11.

Meridional slice of the IH showing the radial velocity (left panel) and proton temperature (right panel). The lower SC is embedded in these figures to demonstrate that the framework coupling between the SC and IH is smooth.

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