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 fm*, GHz Remarks
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
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 fm 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, fm=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.