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LargeSEP

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yyyy-mm-dd	flare class (x 10^-6 W/m^2)	CME speed	SEP flux (J_p)	EP/start	EP/remark		CME/start/ width	Flare	Coronal Wave:
2010-08-03	u	221	0.0478		NO		11:12/93	Start: 11:40:00
2010-08-14	4.4	1205	0.1583	09:48	Y	check if EP is associated with flare	10:12/HALO	Start: 09:38
2010-08-18	4.5	1471	0.0486	05:02	Y		05:48/255	Start: 04:45:00
2011-01-28	13	606	0.0511	00:00	Y		01:25/288
2011-01-28	C1.5	499	0.0326	11:42:09 UT	An arc rises slowly and then erupts with some of material falls back on the SW disk		10:36/280	Start: 10:05:00
2011-02-15	X2.2(220)	669	0.0382	08:42:10	Filament/surge eruption from an active region hours after an X2 flare, still on the decreasing flank of the GOES lightcurve.		02:24/HALO	Start: 01:44
2011-03-07	M3.737	2125	1.012	19:00	Y		20:00/HALO	Srart: 19:43
2011-03-21	u	1341	0.2427		NO		02:24/HALO
2011-05-11	B.1	735	????	01:43	Filament eruption (and two-ribbon flare), transitioning into a clear "bubble-like" coronal propagating front (EIT wave) as the eruption transitions to a CME.	check SEP association	02:48/Partial Halo	Start: 02:23:00
2011-06-05	u	U (511 km/s)	0.0724	01:59:56 UT	!!!This eruption may account for a slow proton event. There is no trace of this event in GOES X-ray light curves. It's a asymmetric filament eruption, untwisting		05:27 (Cactus)	No

Showing 1 to 10 of 81 entries

EP_SC24

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yyyy	mm	dd	lat	long	Filament Eruption (FE)	Mcouley		AR	Eruption TYPE	max V (km/s)	START (UT)	END	FLARE CALSS	Flare onset	Flare peak	CME onset (UT)	CME velocity (km/s)	m/s^2	Angular Width [deg]	PA
2010	8	14	17	52	FE	N	1	11093	F		09:18	10:18	C4.4	09:38	10:05		1205	-43	360	halo
2010	8	18	18	88	Two EPs in AR 11099; 1st bright EP started northwestward at 04:36 and faint 2nd one started southwestward at 05:02	N	2	11099	P?		04:36		C4.5	04:45	05:48		1471	-20	184	255
2010	9	8	21	87	Huge EP in AR 11105 well visible as FE near STEREO A central meridian	N	3	11105	F				C3.3	23:05	23:33		818	-19.36	147	281
2011	1	28	16	88	Two consecutive FEs in AR 11149; 1st spectculer one (00:00-03:59) followed by M-class flare associated with AR 11149 ( This was the first large eruption in a sequence of several ) and 2nd large one (03:38-06:10) followed by C-class flare associated with AR 11149	Y	4	11149	F		00:00		M1.3	00:44	01:03	Y (01:36)	606	-20	119	288
2011	2	15	-20	10	FE in AR 11158 (00:07-01:28) northward surge-like eruption associated with X2 flare (01:26-02:29)	Y	5	11158	C		00:07		X2	01:44	01:56	N	669	-18	360	halo
2011	3	7	30	48	Massive FE (19:00-20:53), spectacular eruption of a massive filament seem to happen before the M-class flare (19:43-20:01) in AR 11164. An oscillation of loop tops (19:20 - 21:01) and coronal wave (19:31 - 22:59) followed filament eruption. Halo CME (2125 km/s)	Y	6	11164	F		19:00	20:53	M3.7	19:43	20:12	Y(20:12)	2125	-60	360	halo
2011	5	11	17	85	Two FEs, first FE (01:31:57-03:59:5) with bright leading coronal propagating front (EIT wave), and post-eruption cooling loop arcade; second FE (01:43:55-03:55:55) with dark leading coronal propagating front, and two-ribbon flare, transitioning into a CME	Y	7		F		01:43	03:59	B8.1	02:23	02:43	Y (02:48)	745	3.3	225	320
2011	6	7	-21	54	Huge FE (05:36-10:32) associated with M2.5 flare (06:16-06:59); Large amounts of the lifted filament material (much is part of a associated CME), falling down impact brighteninings over half a solar radius away.	Y	8	11226	P		05:36	10:32	M2.5	06:16	06:41	Y (06:49)	1255	0.3	360	Halo
2011	8	4	19	36	Two FEs: first FE (03:30-09:00) associated with M-flare in AR 11261, coronal wave and Halo CME; second large FE (03:50-08:00) take place during M-flare and it is similar to the 2011 June 07 event. Twist – Yes	Y	9	11261	F		03:30	09:00	M9	03:41	03:57	Y (04:12)	1315	-41	360	Halo
2011	9	6	14	7	Filament Eruption; one footpoint is in the flare site	N	10	?solar monitor			?????		X2.1	22:12	22:20		557	1.1	360	halo	Acceleration is uncertain due to either poor height measurement or a small number of height-time measurements

Showing 1 to 10 of 35 entries