Guide · Reading forecasts
How much warning do aurora forecasts give?
Answer
Three layers of warning
Aurora forecasting works in layers, each with its own horizon. The longest layer starts at the sun, with coronal mass ejections. SWPC says CMEs typically take several days to arrive, though some of the most intense storms have arrived in as little as 18 hours.
That transit time is what allows a watch. SWPC issues K-index watches when the highest Kp predicted for a day reaches 5, 6, 7, or 8 and above, and reports them on the G-scale. A watch says a storm is possible on a date. It cannot say which hours, or how far south the oval will reach.
The middle layer is warnings: SWPC issues them when a Kp of 4 or more is expected. The shortest layer is the live map and alerts. An alert fires when Kp actually reaches a threshold, and the OVATION map shows the oval for the next 30 to 90 minutes.
Where the 30 to 90 minutes comes from
Spacecraft at the L1 point, 1.6 million km upstream of Earth toward the sun, measure the solar wind before it arrives. OVATION takes those measurements and models the aurora they will cause. The lead is the travel time from L1 to Earth, which depends on how fast the wind is moving.
The arithmetic is simple: divide 1.6 million km by the speed. The table runs it for sample speeds. SWPC's 30 to 90 minute range corresponds to speeds between roughly 300 and 890 km per second. At 400 km per second the trip takes about 67 minutes; at 800 km per second, about 33.
| Solar wind speed | Travel time | Inside 30 to 90 minutes? |
|---|---|---|
| 300 km/s | 89 min | Yes |
| 400 km/s | 67 min | Yes |
| 500 km/s | 53 min | Yes |
| 600 km/s | 44 min | Yes |
| 700 km/s | 38 min | Yes |
| 800 km/s | 33 min | Yes |
| 900 km/s | 30 min | No |
Faster wind gives less warning. That is awkward, because fast wind is part of what drives strong storms, according to SWPC's storm page. The nights with the most dramatic aurora can come with the shortest lead on the map.
When the lead drops to zero
If the L1 data are missing or contaminated, SWPC runs OVATION from the current Kp instead. SWPC says there is then no forecast lead time: the map becomes a nowcast. Glow reads both timestamps in the file and labels a map with less than 20 minutes between observation and forecast as a Kp-based fallback.
Glow also rejects any file more than 2 hours old. Feeds can stall, and an old map looks the same as a fresh quiet one. The status strip at the top of every Glow page shows the feed's age and mode. If it reads fallback, treat the map as a picture of now, not of the next hour.
Using each layer
- Days ahead: watch SWPC's forecasts and watches. Use the best nights tool to see which of those nights are dark and moon-free where you are.
- The afternoon of: check the cloud timeline and dark hours.
- Once dark: open the oval map and your live cell. Refresh every few minutes; the map only sees 30 to 90 minutes ahead.
No layer can promise a sighting. The early layers are forecasts of solar wind that has not yet reached L1. The last layer is a model of aurora from wind already measured. The alerts guide lists the thresholds behind each SWPC product.
Questions
- How far in advance can the aurora be predicted?
- Storm watches can come days ahead, since SWPC says CMEs typically take several days to reach Earth. The OVATION map itself looks only 30 to 90 minutes ahead.
- What is the L1 point?
- A position 1.6 million km upstream of Earth where spacecraft measure the solar wind before it arrives. OVATION uses those measurements as input.
- Why does the aurora forecast sometimes have no lead time?
- When L1 solar wind data are unavailable, SWPC drives OVATION from the current Kp, and SWPC says there is then no forecast lead time.
- How fast can a CME reach Earth?
- SWPC says as short as 18 hours for some of the most intense storms, and typically several days.
- Does faster solar wind mean less warning?
- Yes. The lead is 1.6 million km divided by the wind speed, so doubling the speed halves the warning.
Sources and verification
- NOAA SWPC, Geomagnetic stormshttps://www.swpc.noaa.gov/phenomena/geomagnetic-storms
- NOAA SWPC, Planetary K-indexhttps://www.swpc.noaa.gov/products/planetary-k-index
- NOAA SWPC, Aurora 30-minute forecasthttps://www.spaceweather.gov/products/aurora-30-minute-forecast
Quoted figures last checked against their sources on 2026-09-30; next review 2026-12-31. Computed figures come from SunCalc and the IGRF-14 dipole as described in the methodology. Every quote is listed in the sources ledger.