SEPs and Radio Bursts

Main Table

Data on 86 SEPs of 1986-2008 and Corresponding Radio Bursts Associated with Western Solar Flares

To the paper of I.M. Chertok, V.V. Grechnev, and N.S. Meshalkina,

On the Correlation Between Spectra of Microwave Bursts on the Sun and Proton Flux Spectra Near the Earth,

Astronomicheskii Zhurnal (Astronomy Reports), 2009

No.	Solar Proton Events						Flares			RSTN Radio Bursts			NoRP Radio Bursts			f_m*, GHz	Remarks
No.	Date yyyy/mm/dd	Time, Start-End (hh), UT	J₁₀, pfu	J₁₀₀, pfu	δ=lg(J₁₀/J₁₀₀)	GLE, %	Time, hh:mm, UT	Importance	Coordinates	S₉, sfu	S₁₅, sfu	S₉/S₁₅	S₁₇, sfu	S₃₅, sfu	S₁₇/S₃₅	f_m*, GHz	Remarks
1	1988/10/12	13-18	5.2	0.14	1.57	-	05:02	2N/X2	S20 W66	3000	6000	0.5	5640	5970	0.91	25
2	1988/11/14	02-03	5	0.15	1.52	-	13d, 23:08**	1N/M3	S23 W27	2650	1500	1.77	1215	-	-	9.4
3	1989/03/23	22-23	27	0.18	2.18	-	19:40	3B/X1.5	N18 W28	2350	1050	2.24	-	-	-	5
4	1989/07/25	11-12	24	5	0.73	8	08:40	1B/X2.6	N26 W85	825	1450	0.57	-	-	-	≥15.4
5	1989/08/12	20-22	700	3.5	2.3	-	14:09	2B/X2.6	S16 W38	5630	6850	0.82	-	-	-	≥15.4	1
6	1989/08/16	10-12	650	45	1.16	24	01:19	2N/X>12.5	S15 W85	22500	33000	0.68	-	-	-	≥15.4	8
7	1989/10/19	20-22	1300	180	0.86	92	12:56	3B/X13	S25 E09	37000	48000	0.77	-	-	-	≥15.4	2
8	1989/10/22	21-24	2500	150	1.22	193	18:02	1N/X2.9	S27 W32	30500	23500	1.3	-	-	-	5	1
9	1989/10/24	22-24	2000	100	1.3	162	18:10	2N/X5.7	S29 W57	48500	27000	1.8	-	-	-	8.8
10	1989/11/15	09-10	26	3	0.94	12	06:56	2B/X3.2	N11 W28	3100	4400	0.7	-	-	-	≥15.4
11	1989/11/30	21-23	400	0.7	2.76	-	12:12	2N/X2.6	N25 W52	4400	3700	1.19	-	-	-	8.8	1
12	1990/03/19	15-18	600	0.11	2.48	-	04:44	1N/X1.5	N33 W39	1900	1000	1.9	780	290	2.67	5	1
13	1990/05/21	23-02	300	18	1.22	24	22:15	2B/X5.5	N34 W37	6400	10000	0.64	8580	37800	0.23	35 (47)
14	1990/05/24	23-03	170	12	1.18	52	20:48	1B/X9.3	N36 W76	45000	42000	1.07	-	-	-	8.8
15	1990/05/27	01-03	80	13	0.79	13	20:49	X1.4	N35 W>90	1200	2100	0.57	-	-	-	≥15.4
16	1990/06/12	12-18	70	0.06	3.07	-	05:29	2B/M6.4	N10 W32	340	170	2	150	80	1.88	2.8	3
17	1990/12/23	12-13	3	0.03	2	-	09:45	2B/X1	N12 W70	1400	1900	0.74	-	-	-	12
18	1990/12/24	19-23	1.8	0.05	1.56	-	15:36	1B/X1.8	N10 W80	2100	3500	0.6	-	-	-	≥15.4
19	1991/01/31	09-10	3.5	0.01	2.54	-	02:04	2B/X1.3	S17 W35	330	175	1.89	-	-	-	2.7	1
20	1991/02/25	11-13	8	0.025	2.5	-	08:14	2N/X1.2	S15 W82	1600	1500	1.07	1460	580	2.52	9.1
21	1991/06/11	05-07	300	12	1.4	12	02:06	3B/X12	N32 W15	17000	28000	0.61	30000	45000	0.67	35 (30)	1
22	1991/06/15	12-13	800	52	1.19	42	08:15	3B/X12.5	N36 W70	17000	25000	0.68	-	-	-	≥15.4	1
23	1991/10/30	09-11	94	3	1.5	-	06:22	2N/X2	S09 W26	990	630	1.57	460	370	1.24	2.7
24	1992/06/25	22-24	160	7	1.36	7	20:04	1B/X3.9	N09 W69	20000	50000	0.4	-	-	-	≥15.4
25	1992/10/31	02-05	1600	10	2.2	-	30d, 17:50	2N/X1.7	S26 W63	8600	4800	1.79	-	-	-	5	1
26	1992/11/02	06-10	800	70	1.06	6.5	02:54	2B/X9	S23 W90	17000	43000	0.4	37000	41000	0.9	35	4
27	1993/03/04	13-16	15	0.4	1.57	-	12:24	1N/C8.1	S13 W55	50	40	1.25	-	-	-	8.8
28	1993/03/12	22-24	37	1.2	1.49	-	18:02	3B/M7	S03 W48	480	420	1.14	-	-	-	2.7
29	1993/06/07	15-17	4.2	0.05	1.92	-	14:21	2B/M5.4	S10 W30	900	820	1.1	577	311	1.86	5.2	5
30	1994/02/20	03-05	60	0.2	2.48	-	01:34	3B/M4	N09 W02	140	92	1.52	100	100	1	2.7
31	1995/10/20	09-12	45	0.05	2.95	-	05:58	1N/M1.5	S11 W53	600	270	2.22	330	150	2.2	5
32	1997/11/04	10-12	72	2.8	1.41	-	05:57	2B/X2	S14 W33	1000	1600	0.63	2040	920	2.22	17 (18)
33	1997/11/06	17-21	400	50	0.9	19	11:53	2B/X9	S18W63	8400	9800	0.86	-	-	-	≥15.4
34	1998/05/02	13-17	150	7	1.33	7	13:41	3B/X1.1	S15 W15	1700	1300	1.31	-	-	-	8.8
35	1998/05/06	09-10	210	2.7	1.89	4	08:07	1N/X2	S11W65	2000	1500	1.33	-	-	-	8.8
36	1998/08/25	00-03	140	3.8	1.57	4	24d, 22:03	3B/X1	N30 E07	2000	1055	1.9	1190	550	2.16	5	2
37	1998/09/30	16-19	210	2.7	1.89	-	13:31	2N/M2.8	N23 W81	230	105	2.19	-	-	-	2.7
38	1999/06/04	10-11	64	0.1	2.81	-	07:00	2B/M3.9	N17 W69	1950	1300	1.5	1550	520	2.98	8.8
39	2000/04/04	19-20	12	0.04	2.48	-	15:26	2F/C9.7	N16 W66	160	104	1.53	-	-	-	2.7	1
40	2000/06/10	18-20	46	1.6	1.46	-	16:53	3B/M5.2	N22 W38	320	200	1.6	-	-	-	5
41	2000/07/14	13-15	2700	350	0.89	59	10:27	3B/X5.7	N22 W07	8800	6100	1.44	-	-	-	8.8	1
42	2000/07/22	13-14	15	0.28	1.78	-	11:34	2N/M3.7	N14 W56	63	52	1.21	-	-	-	8.8
43	2000/09/12	21-23	200	0.3	2.82	-	12:22	2N/M1	S17 W09	45	46	0.98	-	-	-	5	6
44	2000/11/09	03-06	14000	320	1.64	-	8d, 23:43	1N/M7.8	N10 W75	225	160	1.41	150	140	1.07	2.8
45	2000/11/24	09-11	8	0.3	1.43	-	05:00	3B/X2	N20 W05	3500	5500	0.64	7760	8540	0.91	35 (32)	7
46	2000/11/24	17-19	77	1.1	1.84	-	15:08	2B/X2.3	N22 W07	7300	14000	0.52	-	-	-	≥15.4	8
47	2001/01/28	21-22	20	0.2	2	-	16:02	1N/M1.5	S04 W59	39	42	0.93	-	-	-	2.7
48	2001/03/29	16-19	18	0.09	2.3	-	10:11	1N/X1.7	N14 W12	9950	5800	1.72	-	-	-	6.9
49	2001/04/03	05-07	380	4.8	1.9	-	2d, 21:48	X17.1	N18 W82	7350	13000	0.57	13050	24580	0.53	35
50	2001/04/09	19-21	4	0.35	1.06	-	15:26	2B/M7.9	S21 W04	5300	5900	0.9	-	-	-	≥15.4
51	2001/04/10	13-16	55	0.3	2.26	-	05:23	3B/X2.3	S23 W09	6400	4300	1.5	4260	2920	1.46	8.8
52	2001/04/12	13-14	16	1	1.2	-	10:20	X2	S22 W40	3800	6200	0.61	-	-	-	≥15.4	8
53	2001/04/15	15-17	600	140	0.63	237	13:49	2B/X14.4	S20 W85	1500	5100	0.29	-	-	-	≥15.4
54	2001/09/15	13-15	10	0.05	2.3	-	11:34	1N/M1.5	S21 W49	230	100	2.3	-	-	-	5
55	2001/10/19	04-06	6	0.14	1.63	-	01:00	2B/X1.6	N16 W18	925	580	1.59	560	290	1.93	8.8	9
56	2001/10/19	19-20	6	0.15	1.6	-	16:24	2B/X1.6	N15 W29	3600	4200	0.86	-	-	-	≥15.4	8
57	2001/11/04	20-21	1100	50	1.34	8	16:17	3B/X1	N06 W18	2800	1600	1.75	-	-	-	6.9
58	2001/11/23	10-12	4000	3.2	3.09	-	22d, 22:57	2N/M9.9	S15 W34	715	305	2.34	-	-	-	2.7	9, 10
59	2001/12/26	07-10	700	47	1.17	13	05:06	1B/M7.1	N08 W54	3800	1800	2.11	2030	740	2.74	6.9
60	2002/02/20	07	13	0.06	2.34	-	06:11	1N/M5.1	N12 W72	770	950	0.81	1270	1530	0.83	35 (27)	7
61	2002/04/17	15-17	15	0.02	2.87	-	08:57	2N/M2.6	S14 W34	2350	930	2.53	-	-	-	5	3
62	2002/04/21	07-10	2000	20	2	-	01:15	1F/X1.5	S14 W84	2800	1400	2	1300	330	3.94	5
63	2002/07/16	20-23	40	0.05	2.9	-	15d, 20:04	3B/X3	N19 W01	15000	20000	0.75	-	-	-	≥15.4
64	2002/08/14	07-09	10	0.08	1.39	-	02:01	1N/M2.3	N09 W54	170	100	1.7	70	50	1.4	8.8
65	2002/08/22	05-06	30	1.5	1.3	-	01:53	2B/M5.7	S07 W52	230	150	1.53	130	110	1.18	5
66	2002/08/24	02-05	220	27	0.91	14	01:00	1F/X3.1	S02 W81	11350	17500	0.65	16000	11200	1.43	≥15.4 (18)
67	2003/05/28	10-15	5	0.1	1.7	-	00:23	2B/X3.6	S07 W17	5250	5500	0.95	5820	3430	1.7	17 (16)
68	2003/05/31	04-06	25	0.7	1.55	-	02:22	2B/M9.3	S07 W65	6950	8400	0.83	7020	2260	3.1	≥15.4 (15)
69	2003/10/26	18-20	320	0.75	2.63	-	17:30	1N/X1.2	N02 W38	4300	3100	1.39	-	-	-	8.8	3
70	2003/10/28	15-17	5200	180	1.46	47	11:04	4B/X>17.2	S16 E08	>70000	>57000	1.23	-	-	-	8.8	2
71	2003/10/29	22-23	2100	102	1.31	35	20:43	2B/X10	S15 W02	13000	18800	0.69	-	-	-	≥15.4
72	2003/11/02	18-21	750	45	1.22	39	17:16	2B/X8.3	S14 W56	18500	36000	0.51	-	-	-	≥15.4
73	2003/11/05	01-02	65	0.67	1.98	-	4d, 19:45	3B/X>17.4	S19 W83	21500	41000	0.52	-	-	-	≥15.4	1
74	2003/11/20	10-11	5.5	0.04	2.14	-	07:26	2B/M9.6	N01 W08	2100	1300	1.62	-	-	-	2.7	3
75	2004/04/11	07-09	7	0.01	2.85	-	04:15	1F/C9.6	S14 W47	430	180	2.39	200	140	1.43	2.7	1
76	2004/07/25	19-21	40	0.04	3	-	15:43	1F/M1.1	N08 W33	82	38	2.16	-	-	-	5
77	2004/09/19	20-22	42	0.2	2.32	-	16:58	M1.9	N03 W58	170	87	1.95	-	-	-	2.7
78	2004/11/07	21-23	400	0.4	3	-	16:27	X2	N09 W17	6600	3600	1.83	-	-	-	5
79	2005/01/16	02-04	32	0.25	2.11	-	15d, 22:48	X2.6	N15 W05	21000	13000	1.61	11760	-	-	8.8	1
80	2005/01/17	14-15	1600	25	1.81	3.5	09:26	X3.8	N15 W25	16500	16500	1	-	-	-	12	1
81	2005/01/20	07-08	1800	680	0.42	5400	06:46	2B/X7.1	N12 W58	62000	>80000	0.77	81600	87500	0.93	35 (28)
82	2005/07/14	00-03	10	0.05	2.3	-	13d, 14:17	M5	N10 W80	4900	4950	0.99	-	-	-	5
83	2005/08/22	04-06	6	0.06	2	-	01:22	1N/M2.6	S08 W50	1300	710	1.83	590	260	2.27	5
84	2005/08/22	22-24	60	0.15	2.6	-	17:06	1N/M5.6	S12 W60	9800	8350	1.17	-	-	-	5	1
85	2006/12/13	06-09	698	90	0.89	92	02:21	4B/X3.4	S06 W24	6700	10000	0.67	12440	13000	0.96	35 (40)
86	2006/12/14	22-24	200	2.2	1.96	-	22:09	2B/X1.5	S06 W46	1600	1300	1.23	-	-	-	8.8

*- Values of f_m computed from light curves recorded by Nobeyama Radio Polarimeters (NoRP) are parenthesized.

*- In records of such a kind, letter “d” means “day” (previous).

1 - Proton fluxes were estimated from a prominent leading bump in GOES time profiles.

2 - GLE is considered despite a small eastern heliolongitude.

3 - SSC effect is possible.

4 - According to NoRP data, S₃₅>S₁₇; thus, f_m=35 GHz.

5 - BERN data at 19 and 35 GHz are taken as S₁₇ and S₃₅ radio fluxes.

6 - Event associated with a filament eruption.

7 - Short-duration microwave burst.

8 - The proton event is discriminated at declining background of a previous enhancement.

9 - Radio emission with an intense decimeter component.

10 - Complex proton event.