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Width of Radio-Loud and Radio-Quiet CMEs

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arxiv 0710.4519 v1 pith:DOTJ6MA3 submitted 2007-10-24 astro-ph

G. Michalek , N. Gopalswamy , H. Xie This is my paper · ORCID
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keywords cmesradio-quietradio-loudexpandingobtainedalmostangularbright
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In the present paper we report on the difference in angular sizes between radio-loud and radio-quiet CMEs. For this purpose we compiled these two samples of events using Wind/WAVES and SOHO/LASCO observations obtained during 1996-2005. It is shown that the radio-loud CMEs are almost two times wider than the radio-quiet CMEs (considering expanding parts of CMEs). Furthermore we show that the radio-quiet CMEs have a narrow expanding bright part with a large extended diffusive structure. These results were obtained by measuring the CME widths in three different ways.

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Cited by 1 Pith paper

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  1. The location and propagation of fine structures in type II solar radio bursts

    astro-ph.SR 2026-08 conditional novelty 4.0 of 10

    Fine structures in a CME-less type II solar radio burst originate from multiple, non-uniformly moving radio sources around the flare site.

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