Type II Radio Bursts and Energetic Solar Eruptions

Details Type II Radio Bursts and Energetic Solar Eruptions Type II Radio Bursts and Energetic Solar Eruptions

Dec 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003agufmsh42c0556g&link_type=abstract

American Geophysical Union, Fall Meeting 2003, abstract #SH42C-0556

Physics

7513 Coronal Mass Ejections, 7514 Energetic Particles (2114), 7534 Radio Emissions, 7851 Shock Waves

Scientific paper

Type II radio bursts at decameter-hectometric (DH) and kilometric wavelengths are indicative of CME-driven shocks in the interplanetary medium. Only a subset of these type II bursts continue from the DH to the km regimes. We report on a study of these long-lasting type II bursts using data from the Wind/WAVES experiment in conjunction with white-light coronal mass ejection (CME) data from SOHO. We find the majority of these events (80 percent) are also associated with metric Type II bursts. We also studied the properties of the associated CMEs and found them to be the most energetic when compared to CMEs associated with bursts in any single wavelength regime.

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