Storms of 1991

G3 (Strong) Geomagnetic Storm of November 21, 1991

November 21 to 22, 1991 · 33 hours

A G3 (strong) geomagnetic storm began November 21, 1991, reached Kp 7- and lasted 33 hours, with a daily Ap as high as 65; at that Kp the aurora may be seen from about 52 degrees geomagnetic latitude.

The Kp through the storm

Began Nov 21, 06:00 UTC, peaked in the block from Nov 21, 15:00 UTC, ended Nov 22, 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- (6.67)
NOAA level
G3 Strong
Duration
33 hours
Highest daily Ap
65
Highest 3-hour ap
111
Rank since 1932
584 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 52 degrees geomagnetic latitude: 43°N in the central US, 42°N in the eastern US, 46°N in the western US and 52°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

  • Sioux Falls, SD 51.8° geomag.
  • Madison, WI 51.8° geomag.
  • Milwaukee, WI 51.9° geomag.
  • Grand Rapids, MI 51.9° geomag.
  • Buffalo, NY 52.0° geomag.
  • Tri-Cities, WA 52.1° geomag.
  • Rochester, NY 52.3° geomag.
  • Tacoma, WA 52.7° geomag.
  • Seattle, WA 53.0° geomag.
  • Saint Paul, MN 53.5° geomag.

13 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
November 21, 1991657-
November 22, 1991576+

Flares before it

Peak (UTC)ClassRegionBefore the storm began
Nov 20, 01:00 UTCM4.0NOAA 692929 hours
Nov 17, 18:33 UTCM1.9NOAA 692983 hours
Nov 21, 19:03 UTCM1.5NOAA 6919during it
Nov 17, 07:06 UTCM1.1NOAA 692995 hours
Nov 18, 10:55 UTCM1.1NOAA 691967 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, Nov 18The storm after, Nov 23Every storm of 1991The 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.