Search for indications of stellar mass ejections using FUV spectra

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Table 4

Solar flare events covered by both the TIMED and SORCE missions.

	30.06.2003	19.10.2003	04.04.2003

SORCE	09:07:12	06:34:59	19:53:28
TIMED	09:07:03	06:34:01	19:52:02
Flare peak	09:03:21	06:23:12	20:16:09
Class	C 2.2	M 1.9	M 1.9
Luminosity range	1.1–1.4 × 10²³	1.9–2.8 × 10²⁴	4.0–8.6 × 10²³
[erg s^-1]
CME	–	06:09:10	19:43:56
CME width [°]	–	38	89
Δt [s]	9	58	86
Index	1	2	3

	02.12.2003	27.10.2003	17.06.2003

SORCE	23:01:41	09:23:37	22:57:04
TIMED	23:02:59	09:22:54	22:58:22
Flare peak	22:58:12	09:25:57	22:50:09
Class	M 1.9	M 5	M 6.8
Luminosity range	1.0–3.0 × 10²⁴	0.3–1.7 × 10²⁵	1.5–2.0 × 10²⁵
[erg s^-1]
CME	–	–	22:39:21
CME width [°]	–	–	360
Δt [s]	78	43	78
Index	4	5	6

	19.01.2005	04.11.2003

SORCE	08:20:32	19:49:00
TIMED	08:23:51	19:45:33
Flare peak	08:19:42	19:42:21
Class	X 1.3	X28
Luminosity range	4.9–6.4 × 10²⁵	>6.8 × 10²⁶
[erg s^-1]
CME	08:11:37	19:35:55
CME width [°]	360	360
Δt [s]	199	207
Index	7	8

Notes. The SORCE and TIMED times are the exposure start times of the used flare spectra. The flare peak times are peak times obtained by GOES, the flare classes are GOES X-ray classes, the CME times are LASCO times for Onset2, and Δt is the time difference between SORCE and TIMED exposure start times. The luminosity range gives the X-ray luminosity of the flare that is covered by both instruments. The index corresponds to the index in Fig. 6 to easily compare Fig. 6 with Table 4.

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