Storms of 1981

G3 (Strong) Geomagnetic Storm of May 10, 1981

May 10 to 11, 1981 · 18 hours

A G3 (strong) geomagnetic storm began May 10, 1981, reached Kp 7 and lasted 18 hours, with a daily Ap as high as 61; at that Kp the aurora may be seen from about 50 degrees geomagnetic latitude.

The Kp through the storm

Began May 10, 21:00 UTC, peaked in the block from May 10, 21:00 UTC, ended May 11, 15:00 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
7 (7.00)
NOAA level
G3 Strong
Duration
18 hours
Highest daily Ap
61
Highest 3-hour ap
132
Rank since 1932
465 of 4,139

How far south the aurora could have been seen

At Kp 7 NOAA’s scales put the aurora’s reach at about 50 degrees geomagnetic latitude: 42°N in the central US, 41°N in the eastern US, 44°N in the western US and 51°N in northern Europe.

NOAA says a G3 storm’s aurora has been seen as low as Illinois and Oregon.

US cities within reach, the southernmost first

  • Washington Heights, NY 50.0° geomag.
  • The Bronx, NY 50.0° geomag.
  • Fort Wayne, IN 50.1° geomag.
  • Des Moines, IA 50.1° geomag.
  • Yonkers, NY 50.1° geomag.
  • Akron, OH 50.2° geomag.
  • Salem, OR 50.3° geomag.
  • Aurora, IL 50.6° geomag.
  • Cleveland, OH 50.6° geomag.
  • Toledo, OH 50.7° geomag.

32 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 10, 1981327
May 11, 1981617-

Flares before it

Peak (UTC)ClassRegionBefore the storm began
May 10, 12:56 UTCM3.5NOAA 31068 hours
May 11, 05:48 UTCM2.9NOAA 3099during it
May 9, 02:48 UTCM2.6NOAA 307942 hours
May 9, 22:11 UTCM1.9NOAA 309923 hours
May 8, 22:51 UTCM1.7NOAA 309946 hours
May 10, 07:31 UTCM1.3NOAA 307913 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 9The storm after, May 15Every storm of 1981The 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.