1. Forbes, T.G., A Review on the Genesis of Coronal Mass Ejections, J. Geophys. Res., 2000, vol. 105, pp. 23153–23165.
2. Eselevich, V.G. and Eselevich, M.V., Common Characteristic of CMEs and BLOBs: A New View of Their Possible Origin, Solar Phys., 2001, vol. 203, pp. 165–178.
3. Eselevich, V.G. and Eselevich, M.V., An Investigation of the Fine Ray Structure of the Coronal Streamer Belt Using LASCO Data, Solar Phys., 1999, vol. 188, pp. 299–313.
4. Eselevich, M.V. and Eselevich, V.G., Additional Plasma Flows with Steep Fronts in the Rays of Increased Brightness of the Coronal Streamer Belt, Astron. Zh., 2004, vol. 81, no. 8, pp. 757–768.
5. Sheeley Jr. N.R., Wang, Y.-M., Hawley, S.H., et al., Measurements of Flow Speeds in the Corona between 2 and 30 R0, Astroph. J., 1977, vol. 485, pp. 472–478.