Dynamics of interplanetary CMEs and associated type II bursts

Details Dynamics of interplanetary CMEs and associated type II bursts Dynamics of interplanetary CMEs and associated type II bursts

Mar 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009iaus..257..287l&link_type=abstract

Universal Heliophysical Processes, Proceedings of the International Astronomical Union, IAU Symposium, Volume 257, p. 287-290

Astronomy and Astrophysics

Astronomy

1

Sun: Coronal Mass Ejections (Cmes), Sun: Radio Radiation, Shock Waves, Solar-Terrestrial Relations, Solar Wind

Scientific paper

Coronal mass ejections (CMEs) are large scale structures of plasma (~1016 g) and magnetic field expelled from the solar corona to the interplanetary medium. During their travel in the inner heliosphere, these “interplanetary CMEs” (ICMEs), suffer acceleration due to the interaction with the ambient solar wind. Based on hydrodynamic theory, we have developed an analytical model for the ICME transport which reproduce well the observed deceleration of fast ICMEs. In this work we present the results of the model and its application to the CME observed on May 13, 2005 and the associated interplanetary type II burst.

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