Storms of 2005

G4 (Severe) Geomagnetic Storm of January 17, 2005

January 17 to 19, 2005 · 63 hours

A G4 (severe) geomagnetic storm began January 17, 2005, reached Kp 8- and lasted 63 hours, with a daily Ap as high as 84; at that Kp the aurora may be seen from about 47 degrees geomagnetic latitude.

The Kp through the storm

Began Jan 17, 00:00 UTC, peaked in the block from Jan 18, 06:00 UTC, ended Jan 19, 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
8- (7.67)
NOAA level
G4 Severe
Duration
63 hours
Highest daily Ap
84
Highest 3-hour ap
179
Rank since 1932
200 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 47 degrees geomagnetic latitude: 38°N in the central US, 37°N in the eastern US, 41°N in the western US and 47°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

  • Richmond, VA 46.7° geomag.
  • Lexington, KY 47.0° geomag.
  • Lexington-Fayette, KY 47.0° geomag.
  • Louisville, KY 47.2° geomag.
  • Lakewood, CO 47.3° geomag.
  • Denver, CO 47.3° geomag.
  • Aurora, CO 47.3° geomag.
  • St. Louis, MO 47.3° geomag.
  • Overland Park, KS 47.4° geomag.
  • Meads, KY 47.5° geomag.

71 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 17, 2005586+
January 18, 2005848-
January 19, 2005607-

Flares before it

Peak (UTC)ClassRegionBefore the storm began
Jan 17, 09:52 UTCX3.8NOAA 10720during it
Jan 15, 23:02 UTCX2.6NOAA 1072025 hours
Jan 19, 08:22 UTCX1.3NOAA 10720during it
Jan 15, 00:43 UTCX1.2NOAA 1072047 hours
Jan 15, 06:38 UTCM8.6NOAA 1072041 hours
Jan 15, 04:31 UTCM8.4NOAA 1072043 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 14The storm after, Jan 21Every 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 2026-09-25. 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.