Other
Scientific paper
May 2010
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aas...21640624m&link_type=abstract
American Astronomical Society, AAS Meeting #216, #406.24
Other
Scientific paper
Dynamical changes in the solar magnetic field are responsible for coronal mass ejections (CMEs), one of the most violent phenomena observed in the Sun. During a CME, mass is lifted away from the Sun and accelerated into the interplanetary medium, sometimes interacting with the Earth or other planets. Some of these CMEs produce radio emission, including type II bursts, which are generated by a strong upstream interplanetary (IP) shocks. The emission is strongest in regions where the direction of the IP shock is quasi-perpendicular to the interplanetary magnetic field. Due to small-scale shock structure, this occurs at various sites along the shock front. We study the different emissions associated with the CME observed on 2007 December 31 using data from the RHESSI, Proba-2/SWAP, and STEREO A/B spacecraft. We track and probe the CME and associated shock signatures from its origin in the lower corona through the interplanetary medium.
Agueda Neus
Bale Stuart
Krucker Sa"m
Lindsey Charles
Martinez Oliveros Juan Carlos
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