The plasma filling factor of coronal bright points - II. Combined EIS and TRACE results

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Table 1:

Coronal bright point intensities, densities, widths, filling factors, and subresolution widths for observations on 2007 June 16.
	EIS	TRACE	Intensity	Log	Width	Filling	Corrected	Length
Label	UT	UT	erg cm^-2 s^-1 sr^-1	density (cm^-3)	( $^{\prime \prime }$ )	factor	width ( $^{\prime \prime }$ )	( $^{\prime \prime }$ )
A	11:59	12:44	4.84e+02	9.59	2.0	2.2e-01	0.9	19.4
11	05:25	06:16	8.61e+01	9.67	4.9	1.1e-02	0.5
11	11:59	12:44	1.87e+02	9.77	2.0	3.7e-02	0.4	6.0
13	00:31	01:22	1.26e+02	9.3	3.1	1.4e-01	1.2	13.5
13	02:11	02:59	1.23e+02	9.23	4.8	1.2e-01	1.7
14	00:31	01:22	9.69e+01	9.39	4.0	5.6e-02	0.9	9.3
25	02:11	02:59	9.69e+01	9.46	2.0	8.1e-02	0.6
25	17:14		8.25e+02	10.3	3.4	8.5e-03	0.3	7.5
26	02:11	02:59	1.04e+02	9.4	4.3	5.4e-02	1.0
26	13:38	14:12	3.34e+02	9.76	3.4	4.1e-02	0.7
27	03:47	04:36	4.52e+02	9.56	5.0	9.6e-02	1.5
28	03:47	04:36	1.18e+02	9.45	8.0	2.6e-02	1.3	10.6
31	11:59	12:44	1.08e+02	9.62	2.8	3.2e-02	0.5	2.5
32	11:59	12:44	2.87e+02	9.57	2.7	1.1e-01	0.9	5.9
35	17:14		1.33e+02	9.81	2.0	2.2e-02	0.3	7.2
35	20:29	20:37	2.22e+02	10.04	2.4	1.1e-02	0.2	6.4
36	20:29	20:37	2.62e+02	9.53	3.1	1.0e-01	1.0	8.9

Source LaTeX | All tables | In the text

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