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MPI-AMRVAC 2.0 for Solar and Astrophysical Applications
C. Xia, J. Teunissen, I. El Mellah, E. Chané and R. Keppens The Astrophysical Journal Supplement Series 234(2) 30 (2018) https://doi.org/10.3847/1538-4365/aaa6c8
Numerical study of the propagation characteristics of coronal mass ejections in a structured ambient solar wind
Three-dimensional MHD simulation of the evolution of the April 2000 CME event and its induced shocks using a magnetized plasma blob model
F. Shen, X. S. Feng, S. T. Wu, C. Q. Xiang and W. B. Song Journal of Geophysical Research: Space Physics 116(A4) n/a (2011) https://doi.org/10.1029/2010JA015809
Why should the latitude of the observer be considered when modeling gradual proton events? An insight using the concept of cobpoint
Three-dimensional MHD modeling of the solar wind structures associated with 13 December 2006 coronal mass ejection
R. Kataoka, T. Ebisuzaki, K. Kusano, et al. Journal of Geophysical Research: Space Physics 114(A10) n/a (2009) https://doi.org/10.1029/2009JA014167
Numerical simulations of the solar corona and Coronal Mass Ejections
Stefaan Poedts, Carla Jacobs, Bart van der Holst, Emmanuel Chané and Rony Keppens Earth, Planets and Space 61(5) 599 (2009) https://doi.org/10.1186/BF03352931
On the combination of ACE data with numerical simulations to determine the initial characteristics of a CME
Virginia Trimble, Markus J. Aschwanden and Carl J. Hansen Publications of the Astronomical Society of the Pacific 118(845) 947 (2006) https://doi.org/10.1086/506157
The effect of the solar wind on CME triggering by magnetic foot point shearing