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An Algorithm for the Determination of Coronal Mass Ejection Kinematic Parameters Based on Machine Learning
Rongpei 荣沛 Lin 林, Yi 易 Yang 杨, Fang 芳 Shen 沈, Gilbert Pi and Yucong 雨淙 Li 李 The Astrophysical Journal Supplement Series 271(2) 59 (2024) https://doi.org/10.3847/1538-4365/ad2dea
Impact of the Solar Activity on the Propagation of ICMEs: Simulations of Hydro, Magnetic and Median ICMEs at the Minimum and Maximum of Activity
Barbara Perri, Brigitte Schmieder, Pascal Démoulin, Stefaan Poedts and Florian Regnault The Astrophysical Journal 955(1) 50 (2023) https://doi.org/10.3847/1538-4357/acec6f
Numerical Research on the Effect of the Initial Parameters of CME Flux-rope Model on Simulation Results. III. Different Initial Energy of CMEs
Numerical Simulation on the Propagation and Deflection of Fast Coronal Mass Ejections (CMEs) Interacting with a Corotating Interaction Region in Interplanetary Space
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
Solar signatures and eruption mechanism of the August 14, 2010 coronal mass ejection (CME)
Elke D’Huys, Daniel B. Seaton, Anik De Groof, David Berghmans and Stefaan Poedts Journal of Space Weather and Space Climate 7 A7 (2017) https://doi.org/10.1051/swsc/2017006
Modeling Coronal Mass Ejections with the Multi-Scale Fluid-Kinetic Simulation Suite
Ward Manchester, Emilia K. J. Kilpua, Ying D. Liu, et al. Space Sciences Series of ISSI, The Scientific Foundation of Space Weather 67 165 (2017) https://doi.org/10.1007/978-94-024-1588-9_6
Numerical study of the propagation characteristics of coronal mass ejections in a structured ambient solar wind
Evolution of the 12 July 2012 CME from the Sun to the Earth: Data‐constrained three‐dimensional MHD simulations
Fang Shen, Chenglong Shen, Jie Zhang, Phillip Hess, Yuming Wang, Xueshang Feng, Hongze Cheng and Yi Yang Journal of Geophysical Research: Space Physics 119(9) 7128 (2014) https://doi.org/10.1002/2014JA020365
MHD numerical study of the latitudinal deflection of coronal mass ejection
The relation between coronal holes and coronal mass ejections during the rise, maximum, and declining phases of Solar Cycle 23
A. A. Mohamed, N. Gopalswamy, S. Yashiro, S. Akiyama, P. Mäkelä, H. Xie and H. Jung Journal of Geophysical Research: Space Physics 117(A1) (2012) https://doi.org/10.1029/2011JA016589
Acceleration and deceleration of coronal mass ejections during propagation and interaction
Fang Shen, S. T. Wu, Xueshang Feng and Chin-Chun Wu Journal of Geophysical Research: Space Physics 117(A11) n/a (2012) https://doi.org/10.1029/2012JA017776
INFLUENCE OF SOLAR WIND HEATING FORMULATIONS ON THE PROPERTIES OF SHOCKS IN THE CORONA
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
Quantitative Analysis of CME Deflections in the Corona
Propagation of an Earth-directed coronal mass ejection in three dimensions
Jason P. Byrne, Shane A. Maloney, R.T. James McAteer, Jose M. Refojo and Peter T. Gallagher Nature Communications 1(1) (2010) https://doi.org/10.1038/ncomms1077
On the combination of ACE data with numerical simulations to determine the initial characteristics of a CME