Features of the Dynamics of a Shock Excited by Fast Coronal Mass Ejections
Author:
Publisher
Pleiades Publishing Ltd
Subject
Space and Planetary Science,Astronomy and Astrophysics,Aerospace Engineering
Link
http://link.springer.com/content/pdf/10.1134/S001095251903002X.pdf
Reference22 articles.
1. Stepanova, T.V. and Kosovichev, A.G., Observation of shock waves associated with coronal mass ejections from SOHO/LASCO, Adv. Space Res., 2000, vol. 25, pp. 1855–1858.
2. Yan, Y., Pick, M., Wang, M., et al., A radio burst and its associated CME on March 17, 2002, Sol. Phys., 2006, vol. 239, pp. 277–292.
3. Gopalswamy, N., Thompson, W.T., Davila, J.M., et al., Relation between type II bursts and CMEs inferred from stereo observations, Sol. Phys., 2009, vol. 259, pp. 227–254.
4. Vourlidas, A., Wu, S.T., Wang, A.H., et al., Direct detection of a CME-associated shock in LASCO white light images, Astrophys. J., 2003, vol. 598, pp. 1392–1402.
5. Ontiveros, V. and Vourlidas, A., Quantitative measurements of coronal mass election-driven shocks from LASCO observations, Astrophys. J., 2009, vol. 693, pp. 267–275.
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