Active and Eruptive Prominences and Their Relationship to Coronal Mass Ejections

By H. Gilbert, T. Holzer, J. Burkepile, A. Hundhausen. 2000

208 citations recorded by the source corpus.

View Paper: https://www.semanticscholar.org/paper/c1ec20695f13d19caaa47f189dca5555fdc7d44b

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In Astronomy and Astrophysics

Citations in the corpus

Coronal prominence structure and dynamics: A magnetic flux rope interpretation (2006, background): “That is, if all of the dips were filled, a partially erupting filament might be observed [Tang, 1986; Gilbert et al., 2000; Qiu and Yurchyshyn, 2005], with some portion escaping, some surviving, and perhaps some first accelerating up and than falling back down [Tripathi et al., 2006].”
Prominence Eruptions and Coronal Mass Ejection: A Statistical Study Using Microwave Observations (2003, background): “Gilbert et al. (2000) found that nearly every other (46”
The Physical Processes of CME/ICME Evolution (2017, background): “Gilbert et al. (2000) found 94% of erupting filaments were in association with CMEs and of those, 84% were found to have a portion of the filament escape the corona and contribute to the ejected CME plasma.”
The Partial Expulsion of a Magnetic Flux Rope (2006, background): “…flux rope: for example, partially or non-erupting filaments and the immediate re-formation of long-lived X-ray sigmoids after eruptions (Tang 1986; Gilbert et al. 2000; Pevtsov 2002; Gibson et al. 2002) A three-dimensional flux rope has the potential to break in two during eruption, with one rope…”
The Calm before the Storm: The Link between Quiescent Cavities and Coronal Mass Ejections (2006, background): “It is also likely to be associated with a trend for filaments to be more likely to erupt in a CME if they extend high enough up in the corona (between 1.2 and 1.35 R and thus visible above the occulter in the Mark IV coronameter; Munro et al. 1979; Zirin 1988, p. 267; Gilbert et al. 2000).”