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Dynamic evolution of interplanetary shock waves driven by CMEs

Published online by Cambridge University Press:  05 July 2012

P. Corona-Romero  and
J. A. Gonzalez-Esparza
P. Corona-Romero
Affiliation:
Posgrado en Ciencias de la Tierra, Universidad Nacional Autonoma de Mexico, Av. Universidad 2000, Mexico City, Mexico. email: [email protected] Insituto de Geofisica Michoacan, Universidad Nacional Autonoma de Mexico, Tzintzuntzan 310, Morelia, Mexico. email: [email protected]
J. A. Gonzalez-Esparza
Affiliation:
Insituto de Geofisica Michoacan, Universidad Nacional Autonoma de Mexico, Tzintzuntzan 310, Morelia, Mexico. email: [email protected]
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Abstract

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We present a study about the propagation of interplanetary shock waves driven by super magnetosonic coronal mass ejections (CMEs). The discussion focuses on a model which describes the dynamic relationship between the CME and its driven shock and the way to approximate the trajectory of shocks based on those relationships, from near the Sun to 1 AU. We apply the model to the analysis of a case study in which our calculations show quantitative and qualitative agreements with different kinds of data. We discuss the importance of solar wind and CME initial conditions on the shock wave evolution.

Keywords

Sun: coronal mass ejections (CMEs)Shock wavesSun: activityMethods: analytical
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 7 , Symposium S286: Comparative Magnetic Minima: Characterizing quiet times in the Sun and Stars , October 2011 , pp. 159 - 163
Copyright
Copyright © International Astronomical Union 2012

References

Bisi, M. M., Breen, A. R., Jackson, B. V., Fallows, R. A., Walsh, A. P., Mikić, Z., Riley, P., Owen, C. J., Gonzalez-Esparza, A., Aguilar-Rodriguez, E., Morgan, H., Jensen, E. A., Wood, A. G., Owens, M. J., Tokumaru, M., Manoharan, P. K., Chashei, I. V., Giunta, A. S., Linker, J. A., Shishov, V. I., Tyul'Bashev, S. A., Agalya, G., Glubokova, S. K., Hamilton, M. S., Fujiki, K., Hick, P. P., Clover, J. M., & Pintér, B. 2010, Solar Phys., 265, 49CrossRefGoogle Scholar
Bothmer, V. & Schwenn, R. 1998, Ann. Geophysicae, 16, 1CrossRefGoogle Scholar
Cavaliere, A. & Messina, A. 1976, ApJ, 209, 424CrossRefGoogle Scholar
Corona-Romero, P. & Gonzalez-Esparza, J. A. 2011, JGR, 116, A05104CrossRefGoogle Scholar
Farris, M. H. & Russell, C. T. 1994, JGR, 99, 17681CrossRefGoogle Scholar
Gopalswamy, N., Lara, A., Lepping, R. P., Kaiser, M. L., & Berdichevsky, D., St.Cyr, O. C. 2000, GRL, 27, 145CrossRefGoogle Scholar
Landau, D. L. & Lifshitz, M. E. 2005, Fluid Mechanics, Course of Theoretical Physics Vol. 6 (Edit. Elsevier).Google Scholar
Ontiveros, V. & Vourlidas, A. 2009, ApJ, 693, 267CrossRefGoogle Scholar
Pintér, S. & Dryer, M. 1990, Bull. Astron. Inst. Czechosl., 41, 137Google Scholar
Smart, D. F. & Shea, M. A. 1985, JGR, 90, 183CrossRefGoogle Scholar