Radio Observations of Rapid Acceleration in a Slow Filament Eruption/Fast Coronal Mass Ejection Event

2004 ◽  
Vol 607 (1) ◽  
pp. 530-539 ◽  
Author(s):  
M. R. Kundu ◽  
S. M. White ◽  
V. I. Garaimov ◽  
P. K. Manoharan ◽  
P. Subramanian ◽  
...  
Keyword(s):  
Coronal Mass Ejection ◽  
Radio Observations ◽  
Filament Eruption ◽  
Mass Ejection ◽  
Ejection Event

On the Disk Hα and Radio Observations of the 2003 October 28 Flare and Coronal Mass Ejection Event

2005 ◽  
Vol 631 (1) ◽  
pp. L97-L100 ◽  
Author(s):  
Monique Pick ◽  
Jean-Marie Malherbe ◽  
Alain Kerdraon ◽  
Dalmiro Jorge Filipe Maia
Keyword(s):  
Coronal Mass Ejection ◽  
Radio Observations ◽  
Mass Ejection ◽  
Ejection Event

scholarly journals Giant Meterwave Radio Telescope observations of an M2.8 flare: Insights into the initiation of a flare–coronal mass ejection event

Solar Physics ◽  
2003 ◽  
Vol 218 (1/2) ◽  
pp. 247-259 ◽  
Author(s):  
Prasad Subramanian ◽  
S. Ananthakrishnan ◽  
P. Janardhan ◽  
M.R. Kundu ◽  
S.M. White ◽  
...  
Keyword(s):  
Coronal Mass Ejection ◽  
Radio Telescope ◽  
Mass Ejection ◽  
Ejection Event

Quadrupolar Dimmings During a Partial Halo Coronal Mass Ejection Event

Solar Physics ◽  
2011 ◽  
Vol 270 (2) ◽  
pp. 551-559 ◽  
Author(s):  
J. Yang ◽  
Y. Jiang ◽  
R. Zheng ◽  
J. Hong ◽  
Y. Bi ◽  
...  
Keyword(s):  
Coronal Mass Ejection ◽  
Halo Coronal Mass Ejection ◽  
Mass Ejection ◽  
Ejection Event

scholarly journals Observation of interactions between two erupting filaments

2009 ◽  
Vol 5 (S264) ◽  
pp. 99-101
Author(s):  
Yu Liu ◽  
Jiangtao Su ◽  
Yuandeng Shen ◽  
Liheng Yang
Keyword(s):  
Observational Study ◽  
Coronal Mass Ejection ◽  
Spatial Resolution ◽  
Mass Flow ◽  
Interesting Case ◽  
Filament Eruption ◽  
Initial Stage ◽  
Flux Ropes ◽  
Mass Ejection

AbstractFollowing the first observational study of the interaction between two distinct filaments (Su et al. 2007; hereafter, event 1), we present another interesting case observed by SMART telescope on 2005 June 25 with higher spatial resolution (hereafter, event 2). The two events are compared with each other. In event 1 the two filaments erupted subsequently and obvious mass flow was observed to be transferred from one erupting filament to one stable filament which triggered its eruption. On the contrary, in event 2, the two filaments erupted simultaneously and there was no transfer of material noticed between them during the initial stage. The two filaments merged together along the ejection path, indicating the bodily coalesce between the two interacting flux ropes. Moreover, event 1 was associated with a coronal mass ejection (CME), while event 2 was a failed filament eruption, thus without CME association.

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