Partially-erupting prominences: a comparison between observations and model-predicted observables

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Table 1:

Comparison between the PEFR model observables described in Sect. 2 and observations.
	Evidence of	Evidence of	Evidence of	Evidence of
	ejected	surviving	internal reconnections	internal reconnections
	filament material	filament material	(not unique to	(unique to
			PEFR model)	PEFR model)
29-Apr.-1998	white-light CME core;	reformed filament	flare ribbons	sigmoid to
	ejected material visible	visible within	straddling surviving	cusp-over-sigmoid (SXR);
	in EIT running difference	two hours	filament	dimmings outside source (EUV)
17-Aug.-1999	white-light CME core	reformed filament	flare ribbons	sigmoid to
		visible within	straddling surviving	cusp-over-sigmoid (SXR);
		two and a half hours	filament	dimmings outside source (EUV)
12-Sep.-2000	white-light CME core	reformed filament	flare ribbons	No SXR
		visible within	straddling surviving	observations available;
		twenty minutes	filament	dimmings outside source (EUV)
11-Jun.-2003	white-light CME core	reformed filament	Simultaneous	No SXR
		visible within	red and blue shift	observations available;
	four hours	in erupting filament (He II)	dimmings outside source
25-Aug.-2003	white-light CME core;	surviving filament	brightening and diverging	No SXR
		material in TRACE;	flows at apparent break	observations available;
		reformed next day in H- $\alpha$	point (EUV and white-light)	dimmings outside source
13-May-2005	white-light CME core	reformed filament	flare ribbons	No SXR: but EUV
		visible within	straddling surviving	pre-eruption sigmoid
		four hours	filament	and sheared loops
				above surviving filament;
				dimmings outside source

Source LaTeX | All tables | In the text

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