White Light and Radio Emission of CME-Shocks: their Evolution in the Interplanetary Medium

Details White Light and Radio Emission of CME-Shocks: their Evolution in the Interplanetary Medium White Light and Radio Emission of CME-Shocks: their Evolution in the Interplanetary Medium

Dec 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010agufmsh23b1845o&link_type=abstract

American Geophysical Union, Fall Meeting 2010, abstract #SH23B-1845

Astronomy and Astrophysics

Astrophysics

[7513] Solar Physics, Astrophysics, And Astronomy / Coronal Mass Ejections, [7534] Solar Physics, Astrophysics, And Astronomy / Radio Emissions

Scientific paper

We analysed fast Coronal Mass Ejections (CMEs) driving shocks close to the solar surface and their evolution in the interplanetary (IP) medium. For each event we derived the CME kinematics and the shock strength from coronograph images, and the shock speeds in the IP medium from their type II radio burst emissions. We studied these events with an analytical model to illuminate their IP evolution.

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