Hot prominence detected in the core of a coronal mass ejection - II. Analysis of the C iii line detected by SOHO/UVCS

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Table 1

Lines identified in UVCS data.

Line	log T_form ^a	λ ₀ ^b	λ _ref ^c	Spectral resolution
	(K)	(Å)	(Å)	(Å)

C iii	4.9	977.02	976.51	0.198
H i Lβ	4.5	1025.72	1025.76	0.198
O vi	5.5	1031.91		0.198
C ii	4.6	1036.34		0.198
C ii	4.6	1037.02		0.198
O vi	5.5	1037.61		0.198
H i Lα	4.5	1215.67	1215.81	0.183

Notes.

^(a)

Formation temperature of the line.

^(b)

Rest wavelength of the transition.

^(c)

Line reference wavelength (see text).

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