Volume 395, Number 2, November IV 2002
|Page(s)||677 - 683|
|Section||Planets and planetary systems|
|Published online||14 November 2002|
High-frequency slowly drifting structures in solar flares
Astronomical Institute of the Academy of Sciences of the Czech Republic, 25165 Ondřejov, Czech Republic e-mail: email@example.com, firstname.lastname@example.org
Corresponding author: M. Karlický, email@example.com
Accepted: 27 August 2002
Radio emission of four solar flares with high-frequency slowly drifting structures is presented. Three sub-classes of these structures were recognized. It is shown that the April 15, 2001 X14.4 flare started with the slowly drifting structure associated with a plasmoid ejection observed by TRACE in the 171 Å line. The August 18, 1998 event presents an example of the drifting pulsation structure (DPS) which is well limited in frequency extent at both sides. A further example of the DPS, but followed by clouds of the narrowband dm-spikes, was observed during the November 23, 2001 flare. Finally, in the case of the April 12, 2001 flare, the drifting pulsation-continuum structure was recorded at the same time as the metric type II radio burst, i.e. in different frequency ranges. The slowly drifting structures were analyzed and in two cases their relation to hard X-ray emission was studied. Possible underlying physical processes are discussed assuming the plasmoid ejection model of eruptive solar flares.
Key words: Sun: activity / Sun: flares / Sun: radio radiation
© ESO, 2002
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