TY  -  
T1  - Modeling a Coronal Mass Ejection from an Extended Filament Channel. I. Eruption and Early Evolution 
SN  -  /  
UR  - http://hdl.handle.net/10138/331791 
T3  -  
A1  - Lynch, Benjamin J.; Palmerio, Erika; DeVore, C. Richard; Kazachenko, Maria D.; Dahlin, Joel T.; Pomoell, Jens; Kilpua, Emilia K. J. 
A2  -  
PB  -  
Y1  - 2021 
LA  - eng 
AB  - We present observations and modeling of the magnetic field configuration, morphology, and dynamics of a large-scale, high-latitude filament eruption observed by the Solar Dynamics Observatory. We analyze the 2015 July 9-10 filament eruption and the evolution of the resulting coronal mass ejection (CME) through the solar corona. The slow streamer-blowout CME leaves behind an elongated post-eruption arcade above the extended polarity inversion line that is only poorly visible in extreme ultraviole... 
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IS  -  
SP  -  
OP  -  
KW  - MAGNETIC-HELICITY; ENERGY BUILDUP; CURRENT SHEETS; SOLAR; RECONNECTION; DYNAMICS; PROMINENCE; CONDENSATION; ONSET; CMES; 114 Physical sciences 
N1  -   
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ER  -