Kinematics of coronal mass ejections between 2 and 30 solar radii - What can be learned about forces governing the eruption?
A&A, 423 2 (2004) 717-728
Published online: 2004-08-06
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N. Gopalswamy, S. Yashiro, G. Michalek, G. Stenborg, A. Vourlidas, S. Freeland and R. HowardEarth, Moon, and Planets 104 (1-4) 295 (2009)
https://doi.org/10.1007/s11038-008-9282-7
Radial Evolution of Well-Observed Slow CMEs in the Distance Range 2 – 30 R ⊙
A. Shanmugaraju, Y.-J. Moon, Bojan Vrsnak and Dijana VrbanecSolar Physics 257 (2) 351 (2009)
https://doi.org/10.1007/s11207-009-9379-9
CME Projection Effects Studied with STEREO/COR and SOHO/LASCO
M. Temmer, S. Preiss and A. M. VeronigSolar Physics 256 (1-2) 183 (2009)
https://doi.org/10.1007/s11207-009-9336-7
ROTATION OF WHITE-LIGHT CORONAL MASS EJECTION STRUCTURES AS INFERRED FROM LASCO CORONAGRAPH
Vasyl Yurchyshyn, Valentyna Abramenko and Durgesh TripathiThe Astrophysical Journal 705 (1) 426 (2009)
https://doi.org/10.1088/0004-637X/705/1/426
Modeling and prediction of fast CME/shocks associated with type II bursts
H. Xie, N. Gopalswamy and O. C. St. CyrProceedings of the International Astronomical Union 4 (S257) 489 (2009)
https://doi.org/10.1017/S1743921309029755
Dynamics of interplanetary CMEs and associated type II bursts
Alejandro Lara and Andrea I. BorgazziProceedings of the International Astronomical Union 4 (S257) 287 (2009)
https://doi.org/10.1017/S1743921309029421