Sun · flares

A Sun that bursts

Flares are sudden releases of magnetic energy above active regions. The flashes in this view recall the classes of the strongest flares in the GOES catalogue (X, M); their positions are illustrative.

Latest catalogued flare

B4.2

2026-10-27 02:20 UTC

Strongest in the catalogue

X28

2003-11-04

X-class flares

558

1975 → 2026

GOES X-ray flare lists (NOAA SWPC/NGDC events, yearly compilations by NASA GSFC) · U.S. Government work, public domain (NOAA/NASA) · 10/27/26

Illustrative rendering: procedural prominence loops and flashes; classes from the GOES catalogue below.

Catalogued flares

94,061

1975 → 2026-10-27

GOES X-ray flare lists (NOAA SWPC/NGDC events, yearly compilations by NASA GSFC) · U.S. Government work, public domain (NOAA/NASA) · 10/27/26 Current · provisional

X-class flares

558

7954 M-class

GOES X-ray flare lists (NOAA SWPC/NGDC events, yearly compilations by NASA GSFC) · U.S. Government work, public domain (NOAA/NASA) · 10/27/26 Current · provisional

Latest catalogued flare

B4.2

2026-10-27 02:20 UTC · AR 14561

GOES X-ray flare lists (NOAA SWPC/NGDC events, yearly compilations by NASA GSFC) · U.S. Government work, public domain (NOAA/NASA) · 10/27/26

Strongest in the catalogue

X28

2003-11-04 18:29 UTC · S19W83

GOES X-ray flare lists (NOAA SWPC/NGDC events, yearly compilations by NASA GSFC) · U.S. Government work, public domain (NOAA/NASA) · 10/27/26

X- and M-class flares per year GOES X-ray flare lists (NOAA SWPC/NGDC events, yearly compilations by NASA GSFC) · U.S. Government work, public domain (NOAA/NASA) · 10/27/26 Current · provisional

Show the data as a table

Number of flares per calendar year in the GOES catalogue (NOAA). The current year is provisional; 2020 is marked “instrument change”: since December 2019 the flux is no longer reduced by the 0.7 factor, which raises classes by about 40%.

C-class flares per year GOES X-ray flare lists (NOAA SWPC/NGDC events, yearly compilations by NASA GSFC) · U.S. Government work, public domain (NOAA/NASA) · 10/27/26 Current · provisional

Show the data as a table

Detection of C-class flares depends on the background level, hence on the cycle phase and the instrument; these counts are less homogeneous than those of M and X classes.

Ten strongest flares (peak flux derived from the class)

#	Class	Start (UTC)	Peak	Peak flux (W/m²)	Position	Active region
1	X28	2003-11-04 18:29	18:50	3E-3	S19W83	10486
2	X20	1989-08-15 23:08	23:17	2E-3	S18W84	5629
3	X20	2001-04-02 19:32	19:51	2E-3	—	—
4	X17	2003-10-28 08:51	10:10	2E-3	—	10486
5	X17	2005-09-07 15:17	15:40	2E-3	S11E77	10808
6	X15	1989-03-06 12:54	13:10	2E-3	N35E69	5395
7	X14	2001-04-15 11:19	11:50	1E-3	S20W85	9415
8	X13	1984-04-24 21:56	22:01	1E-3	S12E43	4474
9	X13	1989-10-19 11:29	11:55	1E-3	S27E10	5747
10	X12	1982-06-06 14:30	14:54	1E-3	S09E25	3763

The peak flux (0.1–0.8 nm, W/m²) is derived from the published class, e.g. X28 = 28 × 10⁻⁴ W/m²; the GOES detectors saturated above X17 before 2003, so the 4 November 2003 flare is an estimate.

Filterable catalogue GOES X-ray flare lists (NOAA SWPC/NGDC events, yearly compilations by NASA GSFC) · U.S. Government work, public domain (NOAA/NASA) · 10/27/26

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Start (UTC)	Peak	End	Duration	Class	Peak flux (W/m²)	Position	Active region
1983-05-09 21:02	21:07	22:07	65 min	X2.4	2E-4	S29E39	4171
1983-05-09 12:07	12:16	13:29	82 min	M1	1E-5	S12E46	4172
1983-05-08 00:24	01:17	07:13	409 min	X1.3	1E-4	S31E62	4171
1983-05-07 20:16	20:16	21:05	49 min	X3.1	3E-4	S30E67	4171
1983-05-07 08:36	08:47	08:54	18 min	M1.2	1E-5	—	—
1983-05-07 05:43	05:46	06:11	28 min	M1	1E-5	S28E72	4171
1983-05-01 20:58	21:10	21:36	38 min	M2.9	3E-5	S15W38	4154
1983-05-01 11:16	11:25	11:51	35 min	M1.1	1E-5	S10E50	4165
1983-04-30 06:08	06:22	09:06	178 min	M2.9	3E-5	S19W17	4154
1983-04-28 08:48	08:52	09:18	30 min	M1.2	1E-5	S05E26	4157
1983-04-27 11:50	11:56	12:28	38 min	M1.3	1E-5	S19E15	4154
1983-04-27 00:48	00:55	01:04	16 min	M1.1	1E-5	S20E22	4154
1983-04-17 23:22	23:48	00:28	66 min	M6.7	7E-5	S11E90	4150
1983-03-18 03:40	03:44	03:54	14 min	M1.7	2E-5	S07E38	4116
1983-03-18 00:54	00:56	01:24	30 min	M1.1	1E-5	S08E37	4116
1983-03-17 19:11	19:13	19:16	5 min	M5.2	5E-5	S08E42	4116
1983-03-17 18:30	18:33	18:35	5 min	M2.7	3E-5	—	—
1983-03-17 12:32	12:37	12:53	21 min	M2.2	2E-5	—	—
1983-03-17 08:28	08:31	08:34	6 min	M4.8	5E-5	—	4116
1983-03-17 08:00	08:04	08:40	40 min	M2.2	2E-5	S08E48	4116
1983-03-17 01:24	01:27	01:46	22 min	M1.1	1E-5	S07E52	4116
1983-03-12 13:16	13:24	13:43	27 min	M1.9	2E-5	—	—
1983-03-10 07:34	08:09	08:32	58 min	M1.1	1E-5	S26W58	4104
1983-02-22 18:20	18:36	18:55	35 min	M4.2	4E-5	—	—
1983-02-06 09:14	09:17	09:19	5 min	M2.7	3E-5	—	—
1983-02-05 12:03	12:37	12:58	55 min	M1.2	1E-5	S21W38	4077
1983-02-05 08:28	08:33	09:17	49 min	M1.7	2E-5	S19W35	4077
1983-02-03 04:43	05:19	07:42	179 min	X4.1	4E-4	S19W08	4077
1983-01-27 02:30	02:38	02:57	27 min	M1.2	1E-5	S15E73	4075
1983-01-02 01:02	01:02	01:21	19 min	M1.1	1E-5	S12W78	4033
1982-12-30 00:40	00:47	01:52	72 min	M7.1	7E-5	S13W22	4033
1982-12-29 05:43	05:45	06:17	34 min	X1.9	2E-4	S13W12	4033
1982-12-28 14:51	14:59	15:20	29 min	M4.3	4E-5	—	4032
1982-12-26 13:56	14:13	14:20	24 min	M1.4	1E-5	—	—
1982-12-26 08:09	08:37	09:07	58 min	M1.1	1E-5	S11E14	4033
1982-12-25 06:43	06:50	07:43	60 min	X2.2	2E-4	S14E31	4033
1982-12-22 07:26	07:33	07:57	31 min	X2.4	2E-4	S09W82	4025
1982-12-21 05:43	05:47	05:55	12 min	M1.1	1E-5	—	—
1982-12-21 03:58	04:12	04:37	39 min	M3.3	3E-5	—	4033
1982-12-21 01:09	01:15	01:22	13 min	M2.9	3E-5	—	—
1982-12-20 16:02	16:08	16:18	16 min	M1	1E-5	—	4033
1982-12-20 14:58	15:07	15:35	37 min	M1	1E-5	—	4022
1982-12-20 06:10	06:15	06:28	18 min	M1	1E-5	—	—
1982-12-20 01:16	01:17	01:21	5 min	M1.3	1E-5	N07W79	4022
1982-12-19 23:19	23:25	23:44	25 min	M2	2E-5	N10W76	4022
1982-12-19 21:28	21:32	21:38	10 min	M1.4	1E-5	—	4022
1982-12-19 14:41	15:32	17:34	173 min	M9	9E-5	N10W75	4022
1982-12-19 00:25	00:39	01:20	55 min	M3.3	3E-5	S11W29	4026
1982-12-18 14:04	14:08	14:45	41 min	X1.1	1E-4	S11W22	4026
1982-12-18 08:53	08:58	09:16	23 min	M1	1E-5	N11W53	4022

Method and sources

The catalogue reproduces the NOAA (SWPC/NGDC) GOES event lists compiled yearly by the NASA GSFC Hesperia centre: start, peak and end (UT), class, heliographic position and active region when known. The class encodes the peak flux in the 0.1–0.8 nm band: C = 10⁻⁶ W/m², M = 10⁻⁵, X = 10⁻⁴, times the number (M2.3 = 2.3 × 10⁻⁵ W/m²).

Lines without an X-ray class (optical or sub-threshold events) are not imported. The last two years are re-read on each import; duplicates are rejected by start time and class. Yearly counts are computed from the imported catalogue.

Reading these data

Until December 2019 NOAA applied a 0.7 factor to the XRS-B flux of GOES 8 to 15; since GOES-16 became the primary satellite the raw flux is used. For the same physical flux, a class after 2020 is therefore about 1.4 times higher (Janssens et al., 2025). Counts before and after 2020 are not directly comparable.

SOURCES OF THIS PAGE

GOES X-ray flare lists (NOAA SWPC/NGDC events, yearly compilations by NASA GSFC): NOAA SWPC/NGDC GOES X-ray flare event lists (1975–), yearly compilations by K. Tolbert, NASA GSFC Hesperia. Flare classes as reported by NOAA at the time: until December 2019 the XRS-B flux carried a 0.7 scaling factor (Janssens et al., 2025). · source page ↗
Licence : U.S. Government work, public domain (NOAA/NASA) · retrieved on Oct 27, 2026 · SHA-256 5d2e8b2d3452…
Janssens (2025): Janssens, J., et al. (2025). Solar flare rates and probabilities based on the McIntosh classification: impacts of GOES/XRS rescaling and recalibration. Journal of Space Weather and Space Climate. · doi:10.1051/swsc/2025007
Licence : Published literature; cited

Solar flares GOES X-ray flare catalogue since 1975

A Sun that bursts