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

C1.5

2026-10-26 04:36 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) · 10/26/26

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

Catalogued flares

94,047

1975 → 2026-10-26

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

Latest catalogued flare

C1.5

2026-10-26 04:36 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) · 10/26/26

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) · 10/26/26

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) · 10/26/26 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) · 10/26/26 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) · 10/26/26

Year

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Start (UTC)	Peak	End	Duration	Class	Peak flux (W/m²)	Position	Active region
1989-02-13 17:11	17:27	18:44	93 min	M1.4	1E-5	N20W13	5355
1989-02-11 10:39	11:23	12:38	119 min	M2.9	3E-5	N22E15	5355
1989-02-10 03:07	03:37	05:03	116 min	X1.8	2E-4	N19E30	5355
1989-02-09 18:17	18:27	18:43	26 min	M1	1E-5	N31E28	5354
1989-02-09 11:56	12:04	13:16	80 min	X3.9	4E-4	N22E39	5355
1989-02-08 18:53	19:23	19:36	43 min	M9.8	1E-4	N30E27	5354
1989-02-08 13:49	14:11	14:21	32 min	M1.4	1E-5	N37E37	5354
1989-02-08 09:59	10:10	10:54	55 min	M1.9	2E-5	N24E56	5355
1989-02-08 08:35	08:48	09:05	30 min	M1.1	1E-5	N36E42	5354
1989-02-07 15:38	15:40	15:57	19 min	M2.1	2E-5	N31E45	5354
1989-02-07 01:09	01:16	01:25	16 min	M1.2	1E-5	—	—
1989-02-06 18:17	18:18	18:48	31 min	M1.4	1E-5	N29E55	5354
1989-02-06 15:42	15:58	16:50	68 min	M2.1	2E-5	—	—
1989-02-06 08:19	08:22	08:34	15 min	M1.2	1E-5	N30E57	5354
1989-02-06 01:13	01:15	01:33	20 min	M1.1	1E-5	N29E64	5354
1989-02-04 08:50	09:17	11:41	171 min	X1.5	2E-4	N29E73	5354
1989-02-03 15:03	15:26	16:57	114 min	M1.1	1E-5	—	—
1989-02-03 13:08	13:16	13:24	16 min	M3	3E-5	S20W72	5336
1989-02-02 16:26	16:27	16:56	30 min	M1	1E-5	S22W19	5334
1989-02-01 09:01	09:34	10:48	107 min	M3.9	4E-5	S21W02	5334
1989-02-01 01:05	01:05	01:10	5 min	M1.4	1E-5	S20E01	5334
1989-01-31 20:01	20:21	20:39	38 min	M1.1	1E-5	S23E06	5334
1989-01-31 16:34	16:41	17:00	26 min	M1.3	1E-5	N15W65	5329
1989-01-31 11:01	11:09	13:13	132 min	M7.5	8E-5	S23E08	5334
1989-01-31 02:06	02:08	02:55	49 min	M1	1E-5	S24E12	5334
1989-01-31 00:18	00:27	00:51	33 min	M1	1E-5	S25E14	5334
1989-01-30 19:40	20:03	20:50	70 min	M2.1	2E-5	N14W53	5329
1989-01-30 02:47	02:52	03:05	18 min	M1.3	1E-5	N17W42	5329
1989-01-29 23:43	00:08	00:37	54 min	M2.9	3E-5	S23E29	5334
1989-01-29 10:40	10:43	11:11	31 min	M1	1E-5	S20W04	5330
1989-01-28 20:38	20:44	21:06	28 min	M1.7	2E-5	S22E49	5334
1989-01-28 11:17	12:04	12:53	96 min	M1.4	1E-5	N15W26	5329
1989-01-27 18:08	18:17	19:46	98 min	X1.1	1E-4	S19E17	5330
1989-01-27 14:16	14:20	14:43	27 min	M1	1E-5	N17W14	5329
1989-01-27 02:27	02:30	02:58	31 min	M1.6	2E-5	S21E32	5330
1989-01-26 22:50	22:51	23:19	29 min	M3.2	3E-5	S22E74	5334
1989-01-26 13:08	13:10	13:40	32 min	M1.2	1E-5	N15W03	5329
1989-01-26 03:19	03:38	04:50	91 min	M2.8	3E-5	N17E03	5329
1989-01-25 13:49	13:55	15:16	87 min	M2.1	2E-5	S20E43	5330
1989-01-24 21:43	22:05	23:12	89 min	M1.2	1E-5	N17E23	5329
1989-01-24 16:30	17:08	17:51	81 min	M1.1	1E-5	N15E26	5329
1989-01-23 20:37	20:48	22:28	111 min	M1.2	1E-5	—	—
1989-01-23 00:48	01:05	01:30	42 min	M1.2	1E-5	N16E46	5329
1989-01-22 23:50	00:03	00:48	58 min	M1.6	2E-5	N16E47	5329
1989-01-22 11:47	12:05	12:25	38 min	M1.5	2E-5	—	—
1989-01-22 08:44	09:02	10:19	95 min	M2.4	2E-5	—	—
1989-01-22 01:55	02:03	02:18	23 min	M1	1E-5	—	—
1989-01-21 05:58	06:09	06:37	39 min	M1.4	1E-5	—	—
1989-01-20 14:10	14:58	16:06	116 min	M8.4	8E-5	—	5312
1989-01-18 17:04	17:15	19:30	146 min	M9.6	1E-4	N26W23	5317

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 26, 2026 · SHA-256 d24560b7385e…
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