Storms of 1990

G3 (Strong) Geomagnetic Storm of November 27, 1990

November 27, 1990 · 6 hours

A G3 (strong) geomagnetic storm began November 27, 1990, reached Kp 7- and lasted 6 hours, with a daily Ap as high as 45; at that Kp the aurora may be seen from about 52 degrees geomagnetic latitude.

The Kp through the storm

Began Nov 27, 15:00 UTC, peaked in the block from Nov 27, 15:00 UTC, ended Nov 27, 21:00 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
6 hours
Highest daily Ap
45
Highest 3-hour ap
111
Rank since 1932
738 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 27, 1990457-

Flares before it

Peak (UTC)ClassRegionBefore the storm began
Nov 26, 23:16 UTCM7.5NOAA 636816 hours
Nov 24, 14:19 UTCM3.1NOAA 637773 hours
Nov 25, 22:24 UTCM1.8NOAA 636841 hours
Nov 25, 18:59 UTCM1.5NOAA 636844 hours
Nov 27, 05:12 UTCM1.510 hours
Nov 26, 16:52 UTCM1.4NOAA 636822 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, Oct 30Every storm of 1990The 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.