Storms of 2003

G4 (Severe) Geomagnetic Storm of May 29, 2003

May 29 to 31, 2003 · 42 hours

A G4 (severe) geomagnetic storm began May 29, 2003, reached Kp 8+ and lasted 42 hours, with a daily Ap as high as 109; at that Kp the aurora may be seen from about 43 degrees geomagnetic latitude.

The Kp through the storm

Began May 29, 12:00 UTC, peaked in the block from May 29, 18:00 UTC, ended May 31, 06:00 UTC.

From 00 UT the day before to the end of the day after. Blocks in the storm are colored by level; the rest are gray.

The storm

Peak Kp
8+ (8.33)
NOAA level
G4 Severe
Duration
42 hours
Highest daily Ap
109
Highest 3-hour ap
236
Rank since 1932
95 of 4,139

How far south the aurora could have been seen

At Kp 8+ NOAA’s scales put the aurora’s reach at about 43 degrees geomagnetic latitude: 35°N in the central US, 34°N in the eastern US, 37°N in the western US and 44°N in northern Europe.

NOAA says a G4 storm’s aurora has been seen as low as Alabama and northern California.

US cities within reach, the southernmost first

  • San Francisco, CA 43.3° geomag.
  • Little Rock, AR 43.3° geomag.
  • Oakland, CA 43.4° geomag.
  • Modesto, CA 43.4° geomag.
  • Huntsville, AL 43.6° geomag.
  • Stockton, CA 43.7° geomag.
  • Oklahoma City, OK 43.7° geomag.
  • New South Memphis, TN 43.8° geomag.
  • Memphis, TN 43.9° geomag.
  • Santa Rosa, CA 44.0° geomag.

106 US cities of 150,000 people or more sit at or poleward of that line. Low on the northern horizon under a dark, clear sky; not a record of sightings.

Tonight’s aurora forecast

Day by day

The daily Ap is the mean of the day’s eight three-hour ap values.

UT dayDaily ApHighest Kp that day
May 29, 20031098+
May 30, 2003597+
May 31, 2003205+

Flares before it

Peak (UTC)ClassRegionBefore the storm began
May 28, 00:27 UTCX3.636 hours
May 27, 23:07 UTCX1.3NOAA 1036537 hours
May 29, 01:05 UTCX1.2NOAA 1036511 hours
May 31, 02:24 UTCM9.3NOAA 10365during it
May 29, 19:37 UTCM2.8NOAA 10368during it
May 26, 05:50 UTCM1.9NOAA 1036578 hours

The strongest M and X class flares GOES recorded from four days before the storm began to its end, the window in which a coronal mass ejection launched with a flare usually arrives. A flare in this list is context, not proof of the cause: many storms come from coronal holes, and many flares launch nothing toward Earth.

More

The storm before, May 27The storm after, Jun 2Every storm of 2003The strongest on recordThis day in weather historyTonight’s aurora forecast

Sources

Kp and ap from GFZ Helmholtz Centre for Geosciences, Geomagnetic Observatory Niemegk, licensed CC BY 4.0: Matzka, J., Stolle, C., Yamazaki, Y., Bronkalla, O. and Morschhauser, A., 2021, The geomagnetic Kp index and derived indices of geomagnetic activity, Space Weather, doi:10.1029/2020SW002641; data doi:10.5880/Kp.0001. Storms, levels and aurora reach worked out by WeatherOverTime from those values and NOAA’s space weather scales. Definitive through August 31, 2026; later values are preliminary. Rebuilt 2026-09-24. Flares from NOAA NCEI’s GOES X-ray flare reports (1975 to 2017) and SWPC’s edited solar event lists, public domain; classes as NOAA recorded them at the time.