Quiescent and eruptive filaments in the metric radio range

Details Quiescent and eruptive filaments in the metric radio range Quiescent and eruptive filaments in the metric radio range

Jun 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002sf2a.conf..109m&link_type=abstract

SF2A-2002: Semaine de l'Astrophysique Francaise, meeting held in Paris, France, June 24-29, 2002, Eds.: F. Combes and D. Barret,

Astronomy and Astrophysics

Astrophysics

Scientific paper

We present new observations of filaments during quiescent and eruptive phases, performed with the Nancay Radioheliograph. Brightness depressions are described for the first time and are related to the coronal cavity that surrounds the filament. Eruptive events, with minor energy release signatures, reveal the coronal restructuring on the disk following the filament eruption; it is shown that the motion of the radio depression on the disk and the CME cavity in the field of view of the coronagraph can be fitted by a single function, suggesting that they belong to the same magnetic structure.

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