Evidence of the interaction of multiple CMEs: what can we learn from simulations?

Details Evidence of the interaction of multiple CMEs: what can we learn from simulations? Evidence of the interaction of multiple CMEs: what can we learn from simulations?

Dec 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006agufmsh51a1461l&link_type=abstract

American Geophysical Union, Fall Meeting 2006, abstract #SH51A-1461

Physics

2111 Ejecta, Driver Gases, And Magnetic Clouds, 2139 Interplanetary Shocks, 7513 Coronal Mass Ejections (2101), 7959 Models

Scientific paper

The interaction of multiple CMEs has been detected by LASCO C2 and C3 and by the Wind/ACE spacecrafts. It is also thought to be associated with large Solar Energetic Particles events and enhanced radio II bursts. New and future missions such as STEREO, Sentinels, and Solar Orbiter should provide additional observations of the interaction of multiple CMEs between the Sun and the Earth. We will present the results of simulations of two and more CMEs interacting in the heliosphere done with the Space Weather Modeling Framework. We will discuss the observational evidence of their interaction (both in situ and from coronographs). The importance of having multiple spacecrafts at different distances and angular positions from the Sun will be emphasized.

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