Figure 10 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 10.

Comparison of the simulated whole month results with ACE at 1 AU. The comparisons are for the radial solar wind velocity (top left), the proton number density (top right), the proton temperature (bottom left), and the magnetic field strength (bottom right). The simulated electron temperature is included in the temperature plot.

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