Figure 9 from A Data-driven, Two-temperature Solar Wind Model with Alfvén Waves

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation

Hi-Resolution Export to PDF PPT Format

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 9.

Slow and fast speed streams in the equatorial plane (left panel) leading to CIRs with the formation of compressed region at the front of the fast stream and rarefaction at the rear as shown by the density plot (right panel).

Other Images in This Article

Copyright and Terms & Conditions