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Gopalswamy et al. 2000
Gopalswamy, N., Kaiser, M.L., Thompson, B.J., Burlaga, L.F., Szabo, A., Lara, A., Vourlidas, A., Yashiro, S. and Bougeret, J.-L. (2000). Radio-rich solar eruptive events. Geophysical Research Letters 27: doi: 10.1029/1999GL003665. issn: 0094-8276.

We report on the analysis of a large number of solar eruptive events that produced radio emission in the dekameter-hectometric (DH) radio window (1--14 MHz), newly opened by the Wind/WAVES experiment. The distinguishing characteristics of coronal mass ejections (CMEs) associated with the DH type II radio bursts are larger-than-average width and speed. Flares of all sizes (X-ray importance B to X) occurring at all longitudes were associated with the DH type II bursts and CMEs. We found a global enhancement in EUV over an area much larger than the flaring active region in the beginning many events. A comparison between the 'Shock Associated' events and microwave bursts shows that at least half of the events do not have temporal relation. A majority of the DH type II bursts were associated with IP shocks and kilometric type II bursts. In particular, we found a very close relationship between the kilometric type II bursts and the IP shocks. ¿ 2000 American Geophysical Union

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Abstract

Keywords
Interplanetary Physics, Ejecta, driver gases, and magnetic clouds, Solar Physics, Astrophysics, and Astronomy, Coronal mass ejections, Solar Physics, Astrophysics, and Astronomy, Flares, Solar Physics, Astrophysics, and Astronomy, Radio emissions
Journal
Geophysical Research Letters
http://www.agu.org/journals/gl/
Publisher
American Geophysical Union
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