Image Details

Choose export citation format:

Evolution of Piled-up Compressions in Modeled Coronal Mass Ejection Sheaths and the Resulting Sheath Structures

  • Authors: Indrajit Das, Merav Opher, Rebekah Evans, Cristiane Loesch, and Tamas Gombosi

Das et al. 2011 The Astrophysical Journal 729 112.

  • Provider: AAS Journals

Caption: Figure 5.

Synthetic white light coronagraphic image at 42 minutes for the TD simulation. The black line locates the CME flux rope on the XZ plane. The black disk shows the blocked portion of the Sun. The WL Ratio at any location is defined as the ratio between its density integrated along the line of sight at that time and background density at the corresponding location when no CME was present.

Other Images in This Article
Copyright and Terms & Conditions