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Ionic Composition Structure of Coronal Mass Ejections in Axisymmetric Magnetohydrodynamic Models

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Complete Citation

Lynch, B. J., Reinard, A. A., Mulligan, T., Reeves, Katharine K., Rakowski, C. E., Allred, J. C., Li, Y., Laming, J. M., MacNeice, P. J., and Linker, J. A. 2011. "Ionic Composition Structure of Coronal Mass Ejections in Axisymmetric Magnetohydrodynamic Models." The Astrophysical Journal, 740 112. https://doi.org/10.1088/0004-637X/740/2/112.

Overview

Abstract

We present the ionic charge state composition structure derived from axisymmetric MHD simulations of coronal mass ejections (CMEs), initiated via the flux-cancellation and magnetic breakout mechanisms. The flux-cancellation CME simulation is run on the Magnetohydrodynamics-on-A-Sphere code developed at Predictive Sciences, Inc., and the magnetic breakout CME simulation is run on ARC7 developed

Publication Date

2011

Authors

Reeves, Katharine