Volume 374, Number 1, July IV 2001
|316 - 325
|Planets and planetary systems
|15 July 2001
Coronal restructuring and electron acceleration following a filament eruption
DASOP-LPSH, Observatoire de Meudon, 92195 Meudon Cedex, France
Corresponding author: Ch. Marqué, firstname.lastname@example.org
Accepted: 9 May 2001
We present a multi wavelength observation of a filament eruption occurring on September 2nd 1999. The slow pre-event evolution of the filament ends with energy release signaled by a faint radio burst observed with the Nançay Radioheliograph and a faint LDE. The restructuring of a large area around the site of the eruption was monitored both with soho/eit observations as well as with the radio data. A moving noise storm occurred in the vicinity of the initial radio burst in coincidence with a faint coronal brightening observed with the lasco coronagraph; no Coronal Mass Ejection was seen. On a smaller energetic scale, this event presents several manifestations of coronal disturbances observed in many CME associated events. Finally, it makes the link between previous studies on noise storm onsets and coronal restructuring.
Key words: Sun: corona / Sun: filament / Sun: radio radiation / Sun: activity
© ESO, 2001
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.