Modeling solar near-relativistic electron events - Insights into solar injection and interplanetary transport conditions

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Volume 507 / No 2 (November IV 2009)

A&A, 507 2 (2009) 981-993

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Table 2:

Electromagnetic emissions associated with the electron events.
	Solar Flare
	soft X-rays			H $\alpha$					hard X-rays		type III	CME
date	start	rise	X-ray	start	rise	Imp.	position	$\Delta$	start	duration	time	first ob.		PA	speed	width	ref.^b
	(UT)	(min)	class	(UT)	(min)	opt		( $^\circ$ )	(UT)	(min)	(UT)	t(UT)	$r(R_{\odot})$	( $^\circ$ )	(km s^-1)	( $^\circ$ )
(1)	(2)	(3)	(4)	(5)	(6)	(7)	(8)	(9)	(10)	(11)	(12)	(13)	(14)	(15)	(16)	(17)	(18)
1998 May 27	13:10	25	C7.5	13:16	12	SF	N18W60	8	13:23	-	13:15-13:30	13:45	3.87	175	878	268	1,2
				12:40	32	SF	S12W80	12
2000 May 1	10:16	11	M1.1	10:09	7	SN	-	-	10:20	4	10:20-10:25	10:54	5.58	323	1360	54	3,4
2000 Jul. 14	10:03	21	X5.7	10:12	9	3B	N22W07	33	10:19	13	10:20-10:50	10:54	5.21	Halo	1674	360	4
2000 Nov. 08	22:42	46	M7.4	22:44	43	1F	N19W65	11	23:18	-	22:55-23:05	23:06	3.85	271	1738	>170	4
2001 Apr. 15	13:19	31	X14.4	13:36	13	2B	S20W85	37	13:45	7	13:45-14:15	14:06	4.29	245	1199	167	4
2001 Dec. 26	04:32	68	M7.1	04:32	42	1B	N08W54	10	no observations		05:15-05:20	05:30	3.84	281	1446	>212	5
2002 Aug. 24	00:49	23	X3.1	00:55	8	1F	S02W81	19	00:52	6	01:05-01:15	01:27	5.90	Halo	1913	360	5
2002 Oct. 20	14:10	3	C6.6	14:11	4	SF	S13W63	26	14:22	7	14:10-14:15	14:30	3.46	247	1011	20	6
	14:21	7	M1.8	14:22	2	1B	S19W23	14			14:25-14:40						6
2002 Dec. 19	21:34	19	M2.7	21:38	9	SF	N23W21	25	21:34	5	21:40-21:55	22:06	4.20	Halo	1092	360	-
				21:38	5	2N	N15W09	37
2004 Sep. 19	16:46	26	M1.9	16:11	No flare patrol		-	-	16:49	13	16:55-17:30	22:42	30.56	262	-	99	5
2005 Jun. 16	20:01	21	M4.0	20:09	1	SF	N09W87	50	no observations		20:10-20:20	no observations					5

^a Estimated positions for the 2000 May 1 and 2004 Sep. 19 events are N20W54 (Kahler et al. 2001) and N03W58 (Cane et al. 2006), respectively. No H $\alpha$ flares were reported for these events.
^b References: (1) Torsti et al. (2002); (2) Klein et al. (2005); (3) Kahler et al. (2001); (4) Cane et al. (2002); (5) Cane et al. (2006); (6) Pick et al. (2006).

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