AuroraCast / Methodology

Methodology & sources

Every number on this site is derived from public space-weather and weather data, recomputed hourly. Here's exactly how — and where it comes from — so you can check our work.

Data vintage Forecasts last recomputed 2026-06-13 17:38 UTC · latest observed planetary Kp 2.67.

Where the data comes from

We are not affiliated with NOAA, the University of Alaska, or Open-Meteo; we reproduce and combine their public data and cite it here.

How the score is computed

For each destination and each 3-hour forecast window we combine three factors into a 0–100 score:

  1. Solar activity vs. the local threshold. Each destination has a minimum Kp baked into its profile, derived from its geomagnetic latitude (the latitude that actually governs where the auroral oval sits — not the map latitude). At or above the threshold, the aurora reaches roughly overhead; below it, the credit falls off as the lights drop toward the horizon.
  2. Cloud cover (the dealbreaker). The Kp credit is multiplied by a sky factor from the Open-Meteo cloud forecast over the dark-hours window. Overcast skies crush the score even when activity is high — because you genuinely won't see it. We keep a small floor (15%) because clouds can break; we never claim a sighting is impossible.
  3. Darkness. A night with less than 5 hours of real darkness is treated as out of season (midnight sun / white nights) — no usable window regardless of Kp. We use sun-below-horizon hours from Open-Meteo and err toward the honest "out of season" call near the season edges, where twilight, not true darkness, dominates.

The score maps to a plain band: Low (0+), Fair (25+), Good (50+), Excellent (75+).

How fresh it is

An automated job re-pulls all four feeds every hour, recomputes every destination's score, and rebuilds these pages. We track 35 destinations. If a feed is stale or failing, we omit the affected reading and flag it rather than show a number we can't stand behind.

This is a probabilistic forecast, not a guarantee. Source feeds can be late, revised, or briefly unavailable; solar activity and cloud cover are inherently uncertain. The absence of good odds is not proof the aurora won't appear, and great odds are not proof it will. Full terms.