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The role of aerodynamic drag in dynamics of coronal mass ejections
Bojan Vršnak, Dijana Vrbanec, Jaša Čalogović and Tomislav Žic Proceedings of the International Astronomical Union 4(S257) 271 (2008) https://doi.org/10.1017/S1743921309029391
Cylindrical and Spherical Pistons as Drivers of MHD Shocks
Strength of Coronal Mass Ejection‐driven Shocks near the Sun and Their Importance in Predicting Solar Energetic Particle Events
Chenglong Shen, Yuming Wang, Pinzhong Ye, et al. The Astrophysical Journal 670(1) 849 (2007) https://doi.org/10.1086/521716
CME Propagation Characteristics from Radio Observations
S. Pohjolainen, L. van Driel-Gesztelyi, J. L. Culhane, P. K. Manoharan and H. A. Elliott Solar Physics 244(1-2) 167 (2007) https://doi.org/10.1007/s11207-007-9006-6
Transit times of interplanetary coronal mass ejections and the solar wind speed
Virginia Trimble and Markus Aschwanden Publications of the Astronomical Society of the Pacific 117(830) 311 (2005) https://doi.org/10.1086/429117
A universal characteristic of type II radio bursts
E. Aguilar‐Rodriguez, N. Gopalswamy, R. MacDowall, S. Yashiro and M. L. Kaiser Journal of Geophysical Research: Space Physics 110(A12) (2005) https://doi.org/10.1029/2005JA011171
Kinematics of coronal mass ejections between 2 and 30 solar radii