Submission_time: 2013/04/18 22:19 EST

Last_Name:Shen
First_Name:Fang
Middle_Name:
Badge_Name:Fang Shen
Email_Address:fshen@spaceweather.ac.cn

Affiliation:Center for Space Science and Applied Research, Chinese Academy of Sciences

Working_Group 1st Choice:WG3

Working_Group 2nd Choice:WG1

Title:Could the collision of CMEs in the heliosphere be super-elastic? Validation through three-dimensional simulations

Abstract:Though coronal mass ejections (CMEs) are magnetized fully ionized gases, a recent observational study of a CME collision event in 2008 November has suggested that their behavior in the heliosphere is like elastic balls, and their collision is probably superelastic [C. Shen et al., 2012, Nature Phys., 8, 923–928]. If this istrue, this finding has an obvious impact on the space weather forecasting because the direction and velocity of CMEs may change. To verify it, we numerically study the event through three-dimensional MHD simulations. The nature of CMEs' collision is examined by comparing two cases. In one case, the two CMEs collide as observed, but in the other, they do not. Results show that the collision leads to extra kinetic energy gain by 3–4% of the initial kinetic energy of the two CMEs. It firmly proves that the collision of CMEs could be superelastic.

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