A formation mechanism for the type II radio emission in the solar corona unrelated to shock waves

Details A formation mechanism for the type II radio emission in the solar corona unrelated to shock waves A formation mechanism for the type II radio emission in the solar corona unrelated to shock waves

2011-05-18

arxiv.org/abs/1105.3556v1

Astronomy and Astrophysics

Astrophysics

Solar and Stellar Astrophysics

Scientific paper

Mark 4, COR1/STEREO and LASCO/SOHO data analysis shows that at least a
portion of type II radio bursts observed in the corona occurs in the presence
of a CME, but in the absence of a shock ahead of them. A drift current
instability in the CME frontal structure is discussed as a possible cause of
such bursts.

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