Storms of 2005

G4 (Severe) Geomagnetic Storm of January 21, 2005

January 21 to 22, 2005 · 15 hours

A G4 (severe) geomagnetic storm began January 21, 2005, reached Kp 8 and lasted 15 hours, with a daily Ap as high as 66; at that Kp the aurora may be seen from about 45 degrees geomagnetic latitude.

The Kp through the storm

Began Jan 21, 15:00 UTC, peaked in the block from Jan 21, 18:00 UTC, ended Jan 22, 06:00 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
8 (8.00)
NOAA level
G4 Severe
Duration
15 hours
Highest daily Ap
66
Highest 3-hour ap
207
Rank since 1932
178 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 45 degrees geomagnetic latitude: 37°N in the central US, 36°N in the eastern US, 39°N in the western US and 45°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

  • Nashville, TN 45.1° geomag.
  • Durham, NC 45.1° geomag.
  • Greensboro, NC 45.2° geomag.
  • Winston-Salem, NC 45.2° geomag.
  • Clarksville, TN 45.4° geomag.
  • Reno, NV 45.4° geomag.
  • Springfield, MO 45.7° geomag.
  • Wichita, KS 45.9° geomag.
  • Chesapeake, VA 46.0° geomag.
  • Norfolk, VA 46.0° geomag.

84 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
January 21, 2005668
January 22, 2005336

Flares before it

Peak (UTC)ClassRegionBefore the storm began
Jan 20, 07:01 UTCX7.1NOAA 1072032 hours
Jan 19, 08:22 UTCX1.3NOAA 1072055 hours
Jan 19, 07:31 UTCM6.7NOAA 1072055 hours
Jan 18, 15:51 UTCM4.6NOAA 1072071 hours
Jan 19, 10:24 UTCM2.7NOAA 1072053 hours
Jan 21, 10:16 UTCM1.7NOAA 107205 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, Jan 17The storm after, Feb 7Every storm of 2005The 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.