Propagation and Decoupling of ICMEs and interplanetary shocks

Details Propagation and Decoupling of ICMEs and interplanetary shocks Propagation and Decoupling of ICMEs and interplanetary shocks

Dec 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008agufmsh13b1558g&link_type=abstract

American Geophysical Union, Fall Meeting 2008, abstract #SH13B-1558

Physics

2100 Interplanetary Physics, 2101 Coronal Mass Ejections (7513), 2111 Ejecta, Driver Gases, And Magnetic Clouds, 2139 Interplanetary Shocks

Scientific paper

The tracking of a solar storm from the Sun to 1~AU is one of the crucial issues for space weather forecasting. We use white light, remote radio and in-situ measurements to study the propagation of ICME/shock events. We compare these observations with two simple 1-D HD models: analytical and numerical, which focus on the transferring of momentum from the CME to the shock. The aim of the study is to understand how a fast CME/shock decelerates in the interplanetary medium.

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