Documentdetail
ID kaart

oai:arXiv.org:2411.10110

Onderwerp
Astrophysics - Solar and Stellar A...
Auteur
Koleva, K. Chandra, R. Duchlev, P. Devi, P.
Categorie

wetenschappen: astrofysica

Jaar

2024

vermelding datum

20-11-2024

Trefwoorden
solar observed eruption filament
Metriek

Beschrijving

We present the observations of a quiescent filament eruption and its deflection from the radial direction.

The event occurred in the southern solar hemisphere on 2021 May 9 and was observed by the Atmospheric Imaging Assembly (AIA) on board the Solar Dynamics Observatory (SDO), by the STEREO A Observatory and GONG.

Part of the filament erupted in the west direction, while major part of the filament deviated towards east direction.

LASCO observed a very weak CME towards the west direction where it faded quickly.

Moreover, the eruption was associated with CME observed by STEREO A COR1 and COR2.

Our observations provide the evidence that the filament eruption was highly non-radial in nature.

;Comment: Accepted in the Proceedings of IAUS 388

Koleva, K.,Chandra, R.,Duchlev, P.,Devi, P., 2024, Filament eruption deflection and associated CMEs

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