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CMEs and Prominences and their Evolution Over the Solar Cycle

Published online by Cambridge University Press:  12 April 2016

David F. Webb
David F. Webb*
Affiliation:
Institute for Scientific Research, Boston College, 140 Commonwealth Ave., Chestnut Hill, MA 02467-3862, USA

Abstract

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Coronal mass ejections (CMEs) are an important aspect of coronal and interplanetary dynamics. They cause large geomagnetic storms and can drive transient interplanetary shocks, which in turn are a key source of energetic particle events. However, our knowledge of the origins and early development of CMEs at the Sun is limited. CMEs are most frequently associated with erupting prominences and long-enduring soft X-ray arcades, but sometimes with no observed surface activity. I review some of the well determined coronal properties of CMEs and what we know about their source regions, with emphasis on the characteristics of the associated prominences and helmet streamers. One of these characteristics is that many CMEs seem to arise from multipolar magnetic structures with multiple or kinked inversion lines. I also discuss the solar-cycle dependencies of these structures, including the role that erupting prominences and CMEs may play in the ejection of magnetic flux and helicity from the Sun.

Type
Global Patterns
Information
International Astronomical Union Colloquium , Volume 167: New Perspectives on Solar Prominences , 1998 , pp. 463 - 474
Copyright
Copyright © Astronomical Society of the Pacific 1998

References

Bothmer, V. and Schwenn, R. 1994, in Mass Supply and Flows in the Solar Corona, (eds.) Fleck, B. et al., Kluwer, Norwell, MA, p. 225 Google Scholar
Bothmer, V. and Rust, D. M. 1997, in Coronal Mass Ejections, (eds.) Crooker, N. et al., GM 99, AGU, Washington, DC, p. 139 Google Scholar
Burlaga, L. et al. 1998, J. Geophys. Res., 103, 277 CrossRefGoogle Scholar
Cliver, E.W., Cyr, O. C.St., Howard, R. A. and Mclntosh, P. S. 1994, Solar Coronal Structures, (eds.) Rusin, V. et al., Veda, Bratislava, p. 83 Google Scholar
Crooker, N.U., Siscoe, G. L., Shodan, S. Webb, D.F., J.T., Gosling, and Smith, E. J. 1993, J. Geophys. Res., 98, 9371 CrossRefGoogle Scholar
Gosling, J.T. 1993, J. Geophys. Res. 98, 18, 937 Google Scholar
Guhathakurta, M., Fisher, R. R. and Altrock, R. C. 1993, ApJ, 414, L145 CrossRefGoogle Scholar
Hansen, R.T., Garcia, C.J., Hansen, S.F., and Yasukawa, E. 1974, PASP, 86, 500 CrossRefGoogle Scholar
Harrison, R.A. 1991, Adv. Space Res., 11 (1), 25 CrossRefGoogle Scholar
Hick, P., Jackson, B. V. and Altrock, R. C. 1996, in Solar Wind Eight, (eds.) Winterhalter, et al., AIP, Woodbury, NY, p. 169 Google Scholar
Howard, R.A. and 18 coauthors 1997, in Coronal Mass Ejections, (eds.) Crooker, N. et al., GM 99, AGU, Washington, DC, p. 17 Google Scholar
Howard, R.A., Sheeley, N. R., Koomen, M.J. and Michels, D.J. 1985, J. Geophys. Res., 90, 8173 CrossRefGoogle Scholar
Hudson, H.S. and Webb, D.F. 1997, in Coronal Mass Ejections, (eds.) Crooker, N. et al., GM 99, AGU, Washington, DC, p. 27 Google Scholar
Hudson, H., Haisch, B., and Strong, K. T. 1995, J. Geophys. Res. 100, 3473 CrossRefGoogle Scholar
Hudson, H.S., Lernen, J. R. and Webb, D.F. 1996, in Magnetic Reconnection in the Solar Atmosphere, (eds.) Bentley, R.D. and Mariska, J.T., ASP Conf. Ser. Vol. III, San Francisco, p. 379 Google Scholar
Hundhausen, A.J. 1993, J. Geophys. Res. 98, 13, 177 Google Scholar
Hundhausen, A.J., 1997, in Cosmic Winds and the Heliosphere, (eds.) Jokipi, J. et al., University of Arizona Press, Tucson, AZ Google Scholar
Hundhausen, A.J. 1998, in The Many Faces of the Sun, (eds.) Strong, K. et al., Springier-Verlag, New York, in pressGoogle Scholar
Hundhausen, A.J., Burkepile, J. T. and Cyr, O.C.St. 1994, J. Geophys. Res., 99, 6543 CrossRefGoogle Scholar
Jackson, B.V. 1996, in Magnetic Storms, (eds.) Tsurutani, B. et al., GM 98, AGU, Washington, DC, p. 59 Google Scholar
Jackson, B.V., Howard, R. A. and Webb, D. F. 1996, Solar Wind Eight, (eds.) Winterhalter, et al., AIP, Woodbury, NY, p. 540 Google Scholar
Jackson, B.V., Webb, D.F., Hick, P.L., and Nelson, J.L. 1994, Catalog of Helios 90° Photometer Events, PL-TR-94-2040, Phillips Laboratory, Hanscom AFB, MACrossRefGoogle Scholar
Klimchuk, J., Acton, L., Harvey, K., Hudson, H., Kluge, K., Sime, D., Strong, K., and Watanabe, T. 1994, in X-ray Solar Physics from Yohkoh, (eds.) Uchida, Y. et al., Universal Academy Press, Tokyo, p. 181 Google Scholar
Low, B.C. and Hundhausen, J. R. 1995, ApJ, 443, 818 CrossRefGoogle Scholar
Martin, S.F. and McAllister, A.H. 1997, in Coronal Mass Ejections, (eds.) Crooker, N. et al., GM 99, AGU, Washington, DC, p. 127 Google Scholar
Marubashi, K. 1997, in Coronal Mass Ejections, (eds.) Crooker, N. et al., GM 99, AGU, Washington, DC, p. 147 Google Scholar
McIntosh, P.S. 1992, in The Solar Cycle, (ed.) Harvey, K., ASP Conf. Ser. Vol. 27, San Francisco, p. 14 Google Scholar
Rust, D.M. 1994, Geophys. Res. Lett. 21, 241 CrossRefGoogle Scholar
Rust, D.M. and Hildner, E. 1976, Solar Phys., 48, 381 CrossRefGoogle Scholar
Rust, D.M. and Kumar, A. 1994, Solar Phys., 155, 69 CrossRefGoogle Scholar
Sheeley, N.R., Howard, R.A., Koomen, M.J. and Michels, D.J. 1983, ApJ, 272, 349 CrossRefGoogle Scholar
Webb, D.F. 1995, Rev. Geophys. Suppl., 577 CrossRefGoogle Scholar
Webb, D.F. 1992, in Eruptive Solar Flares, (eds.) Švestka, Z., Jackson, B. and Machado, M., Springer-Verlag, New York, p. 234 CrossRefGoogle Scholar
Webb, D.F. and Howard, R.A. 1994, J. Geophys. Res. 99, 4201 CrossRefGoogle Scholar
Webb, D.F., Kahler, S.W., McIntosh, P.S. and Klimchuk, J.A. 1997, J. Geophys.Res., 102, 24, 161 Google Scholar
Webb, D.F., Cliver, E.W., Gopalswamy, N., Hudson, H.S. and Cyr, O.C.St. 1998, Geophys. Res. Lett., in pressGoogle Scholar