G4 (Severe) Geomagnetic Storm of September 27, 1978
A G4 (severe) geomagnetic storm began September 27, 1978, reached Kp 8 and lasted 66 hours, with a daily Ap as high as 109; at that Kp the aurora may be seen from about 45 degrees geomagnetic latitude.
The Kp through the storm
Began Sep 27, 00:00 UTC, peaked in the block from Sep 29, 09:00 UTC, ended Sep 29, 18:00 UTC.
The storm
- Peak Kp
- 8 (8.00)
- NOAA level
- G4 Severe
- Duration
- 66 hours
- Highest daily Ap
- 109
- Highest 3-hour ap
- 207
- Rank since 1932
- 137 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.
Day by day
The daily Ap is the mean of the day’s eight three-hour ap values.
| UT day | Daily Ap | Highest Kp that day |
|---|---|---|
| September 27, 1978 | 51 | 6+ |
| September 28, 1978 | 50 | 6+ |
| September 29, 1978 | 109 | 8 |
Flares before it
| Peak (UTC) | Class | Region | Before the storm began |
|---|---|---|---|
| Sep 23, 10:29 UTC | X0.1 | NOAA 1294 | 86 hours |
| Sep 27, 14:48 UTC | M0.7 | NOAA 1304 | during it |
| Sep 24, 17:29 UTC | M0.1 | NOAA 1301 | 55 hours |
| Sep 27, 08:39 UTC | M0.1 | NOAA 1304 | during it |
| Sep 27, 17:27 UTC | M0.1 | NOAA 1304 | during it |
| Sep 29, 10:54 UTC | M0.1 | during it |
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, Sep 26The storm after, Oct 18Every storm of 1978The 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.