Observations of the Failed Eruption of a Filament

By H. Ji, Haimin Wang, E. Schmahl, Y. Moon, Yunchun Jiang. 2003

257 citations recorded by the source corpus.

View Paper: https://www.semanticscholar.org/paper/83efc31574dd78367f63f24a61302aa8386f0a5e

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In Astronomy and Astrophysics

Citations in the corpus

WHY IS THE GREAT SOLAR ACTIVE REGION 12192 FLARE-RICH BUT CME-POOR? (2015, background): “We dub all flares without a CME “confined”: they either produce no eruption or eruptions that fail to escape the Sun (e.g., Ji et al. 2003).”
Driving major solar flares and eruptions: A review (2008, background): “At least some of these failed eruptions have no CME counterpart (e.g., Ji et al. 2003).”
Coronal prominence structure and dynamics: A magnetic flux rope interpretation (2006, background): “If only the lower dips were filled, the filament might undergo a ‘‘failed eruption,’’ with some temporary motion upward but no apparent ejection of material [Ji et al., 2003], or it might not show any sign of”
Confined and Ejective Eruptions of Kink-unstable Flux Ropes (2005, background): “SIMULATION OF A CONFINED ERUPTION The eruption of an active region filament (on 2002 May 27), which was accompanied by an M2 flare but did not lead to a CME, was described by Ji et al. (2003).”
Ideal kink instability of a magnetic loop equilibrium (2003, methodology): “Apparently, a global eruption is not reached in ideal-MHD simulations, due to the counteraction by the strong overlying field in the model, as also found by Roussev et al. However, the exponential rise and helical shape of the loop and the saturation correspond excellently to eruptive filaments that”
Homologous Confined Filament Eruptions via Magnetic Breakout (2008, background): “Several well-observed eruptions of filaments orX-ray sigmoids have been analyzed to reveal both two-phase (Sterling & Moore 2004a, 2004b) and three-phase (Ji et al. 2003; Li et al. 2005; Bong et al. 2006) acceleration profiles of the disrupted structures.”
DIRECT EVIDENCE FOR A FAST CORONAL MASS EJECTION DRIVEN BY THE PRIOR FORMATION AND SUBSEQUENT DESTABILIZATION OF A MAGNETIC FLUX ROPE (2012, background): “(Ji et al. 2003; Alexander et al. 2006; Török & Kliem 2005) reported on very clearly kinked prominences which were also failed eruptions.”