Observations of conduction driven evaporation in the early rise phase of solar flares

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Table 1:

Eventlist. The attenuator state is 0 for all events at the very beginning, then changes to 1 as the flux increases. The attenuator times give the rough time interval that must be avoided because of attenuator motion.
Date	Analyzed time	GOES class	xy-position [arcsec]	coronal source volume [cm³]	Attenuator	Attenuator times
03-Aug.-2002	18:59-19:02	X1.2	912/-271	$4.9\times 10^{26}$	0/1	19:02:20/19:03:10
13-Nov.-2003	04:55:40-04:57:12	M1.7	-977/23	$4.8\times 10^{26}$	0/1	04:57:20/04:58:20
06-Jan.-2004	06:13-06:16	M5.9	-992/88	$2.8\times 10^{27}$	0/1	06:18/06:19
21-May-2004	23:37:30-23:39	M2.6	-757/-157	$7.5\times 10^{26}$	0/1	23:40:30/23:41:30

Source LaTeX | All tables | In the text

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