AIA observations of a flare/CME system in conjunction with X-ray and radio data

Details AIA observations of a flare/CME system in conjunction with X-ray and radio data AIA observations of a flare/CME system in conjunction with X-ray and radio data

Dec 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010agufmsh11a1600b&link_type=abstract

American Geophysical Union, Fall Meeting 2010, abstract #SH11A-1600

Astronomy and Astrophysics

Astrophysics

[7513] Solar Physics, Astrophysics, And Astronomy / Coronal Mass Ejections, [7519] Solar Physics, Astrophysics, And Astronomy / Flares, [7534] Solar Physics, Astrophysics, And Astronomy / Radio Emissions, [7554] Solar Physics, Astrophysics, And Astronomy / X-Rays, Gamma Rays, And Neutrinos

Scientific paper

During solar flares and coronal mass ejections, free magnetic energy, previously stored within the magnetic field, is released and used to accelerate particles and heat the surrounding plasma. Using multiwavelength observations from AIA onboard SDO, combined with X-ray observations from RHESSI and radio observations from the Nancay Radioheliograph we investigate sources of particle acceleration and heating within the flare-CME system of an event which occurred on the 14 August 2010. This was the first proton event in more than three years. In addition, radio spectrogram data show Type III radio bursts associated with the impulsive/launch phase of the CME, indicating the location of energetic electrons as they escape into the interplanetary medium. A Type II radio burst is also observed as electrons are accelerated in a CME driven shock as the ejected material propagates away from the Sun.

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