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Cited article:

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Assessing the Influence of Input Magnetic Maps on Global Modeling of the Solar Wind and CME‐Driven Shock in the 2013 April 11 Event

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Evolution of Interplanetary Coronal Mass Ejection Complexity: A Numerical Study through a Swarm of Simulated Spacecraft

Camilla Scolini, Reka M. Winslow, Noé Lugaz and Stefaan Poedts
The Astrophysical Journal Letters 916 (2) L15 (2021)
https://doi.org/10.3847/2041-8213/ac0d58

Magnetohydrodynamic Modeling of the Solar Corona and Heliosphere

Xueshang Feng
Atmosphere, Earth, Ocean & Space, Magnetohydrodynamic Modeling of the Solar Corona and Heliosphere 695 (2020)
https://doi.org/10.1007/978-981-13-9081-4_10

Effect of the solar wind density on the evolution of normal and inverse coronal mass ejections

S. Hosteaux, E. Chané and S. Poedts
Astronomy & Astrophysics 632 A89 (2019)
https://doi.org/10.1051/0004-6361/201935894

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

Yufen Zhou and Xueshang Feng
Journal of Geophysical Research: Space Physics (2017)
https://doi.org/10.1002/2016JA023053

Modelling large solar proton events with the shock-and-particle model

Jens Pomoell, Angels Aran, Carla Jacobs, et al.
Journal of Space Weather and Space Climate 5 A12 (2015)
https://doi.org/10.1051/swsc/2015015

PLASMA PHYSICAL PARAMETERS ALONG CME-DRIVEN SHOCKS. II. OBSERVATION–SIMULATION COMPARISON

F. Bacchini, R. Susino, A. Bemporad and G. Lapenta
The Astrophysical Journal 809 (1) 58 (2015)
https://doi.org/10.1088/0004-637X/809/1/58

MHD numerical study of the latitudinal deflection of coronal mass ejection

Y. F. Zhou and X. S. Feng
Journal of Geophysical Research: Space Physics 118 (10) 6007 (2013)
https://doi.org/10.1002/2013JA018976

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)
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Why should the latitude of the observer be considered when modeling gradual proton events? An insight using the concept of cobpoint

R. Rodríguez-Gasén, A. Aran, B. Sanahuja, C. Jacobs and S. Poedts
Advances in Space Research 47 (12) 2140 (2011)
https://doi.org/10.1016/j.asr.2010.03.021

AUTOMATED LASCO CME CATALOG FOR SOLAR CYCLE 23: ARE CMEs SCALE INVARIANT?

E. Robbrecht, D. Berghmans and R. A. M. Van der Linden
The Astrophysical Journal 691 (2) 1222 (2009)
https://doi.org/10.1088/0004-637X/691/2/1222

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

E. Chané, S. Poedts and B. van der Holst
Astronomy & Astrophysics 492 (2) L29 (2008)
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Numerical Investigation of the Homologous Coronal Mass Ejection Events from Active Region 9236

N. Lugaz, W. B. Manchester IV, I. I. Roussev, G. Toth and T. I. Gombosi
The Astrophysical Journal 659 (1) 788 (2007)
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Inverse and normal coronal mass ejections: evolution up to 1 AU

E. Chané, B. Van der Holst, C. Jacobs, S. Poedts and D. Kimpe
Astronomy & Astrophysics 447 (2) 727 (2006)
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Astrophysics in 2005

Virginia Trimble, Markus J. Aschwanden and Carl J. Hansen
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