Different types of coronal mass ejections at minimum and maximum of solar activity and their relation to magnetic field evolution

Solar Physics

Volumn 180, Issue 1-2, 1998, Pages 461-471

  Bravo, S ^a   Blanco Cano, X ^a   Nikiforova, E ^a  

^a UNIVERSIDAD NACIONAL AUTÓNOMA DE MÉXICO   (Mexico)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 0032379161     PISSN: 00380938     EISSN: None     Source Type: Journal    
DOI: 10.1023/a:1005010926470     Document Type: Article

References (5)

1. Bravo, S. Stewart, G. A., and Blanco-Cano, X.: 1998, Solar Phys., in press.
2. Howard, R. A., Sheeley, N. R., Jr., Koomen, M. I., and Michels, D. J.: 1985, J. Geophys. Res. 90, 8137.
3. Howard, R. A., Sheeley, N. R., Jr., Michels, D. J., and Koomen, M. I.: 1986, in R. G. Marsden (ed.), The Sun and the Heliosphere in Three Dimensions, D. Reidel Publ. Co., Dordrecht, Holland, p. 107.
4. Hundhausen, A. J.: 1993, J. Geophys. Res. 98, 13177.
5. Webb, D. F. and Howard, R. A.: 1994, J. Geophys. Res. 99, 4201.