G4 (Severe) Geomagnetic Storm of April 11, 2001
A G4 (severe) geomagnetic storm began April 11, 2001, reached Kp 8+ and lasted 21 hours, with a daily Ap as high as 85; at that Kp the aurora may be seen from about 43 degrees geomagnetic latitude.
The Kp through the storm
Began Apr 11, 15:00 UTC, peaked in the block from Apr 11, 21:00 UTC, ended Apr 12, 12:00 UTC.
The storm
- Peak Kp
- 8+ (8.33)
- NOAA level
- G4 Severe
- Duration
- 21 hours
- Highest daily Ap
- 85
- Highest 3-hour ap
- 236
- Rank since 1932
- 109 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.
Day by day
The daily Ap is the mean of the day’s eight three-hour ap values.
| UT day | Daily Ap | Highest Kp that day |
|---|---|---|
| April 11, 2001 | 85 | 8+ |
| April 12, 2001 | 50 | 7+ |
Flares before it
| Peak (UTC) | Class | Region | Before the storm began |
|---|---|---|---|
| Apr 10, 05:26 UTC | X2.3 | NOAA 9415 | 34 hours |
| Apr 12, 10:28 UTC | X2.0 | NOAA 9415 | during it |
| Apr 9, 15:34 UTC | M7.9 | NOAA 9415 | 47 hours |
| Apr 11, 13:26 UTC | M2.3 | NOAA 9415 | 2 hours |
| Apr 12, 03:04 UTC | M1.3 | NOAA 9415 | during it |
| Apr 11, 00:31 UTC | M1.0 | 14 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, Apr 9The storm after, Apr 13Every storm of 2001The 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.