Storms of 1989

G3 (Strong) Geomagnetic Storm of June 9, 1989

June 9 to 10, 1989 · 24 hours

A G3 (strong) geomagnetic storm began June 9, 1989, reached Kp 7 and lasted 24 hours, with a daily Ap as high as 78; at that Kp the aurora may be seen from about 50 degrees geomagnetic latitude.

The Kp through the storm

Began Jun 9, 21:00 UTC, peaked in the block from Jun 10, 15:00 UTC, ended Jun 10, 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 (7.00)
NOAA level
G3 Strong
Duration
24 hours
Highest daily Ap
78
Highest 3-hour ap
132
Rank since 1932
446 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
June 9, 1989346+
June 10, 1989787

Flares before it

Peak (UTC)ClassRegionBefore the storm began
Jun 5, 21:36 UTCX1.0NOAA 552195 hours
Jun 9, 22:55 UTCM6.3NOAA 5533during it
Jun 10, 06:20 UTCM5.0NOAA 5533during it
Jun 6, 11:04 UTCM3.182 hours
Jun 7, 01:35 UTCM3.0NOAA 552167 hours
Jun 7, 20:50 UTCM2.4NOAA 552148 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, Jun 8The storm after, Jun 14Every storm of 1989The 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.