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Reading tonight's activity against the recent baseline…

needed here
Kp 03579
usual range (recent) needed to see it here tonight

Current conditions

Kp index
Solar wind
OVATION chance here
model probability at this cell
Magnetic latitude
centred-dipole estimate
Kp needed here

3-day outlook

About these numbers

The anomaly gauge — how "usual" is defined method
The gauge compares tonight's Kp to a rolling baseline built from the readings we have on hand — roughly the last three days of stored snapshots. The shaded band is the middle half of that recent range (25th–75th percentile); the dot is now. It is deliberately simple, and honest about its limits: this is "usual lately," not "usual for this place and season." Kp is a planetary index — the same number everywhere on Earth at a given moment — so the baseline says nothing location-specific on its own; what makes it local is the "needed here" line, set by your magnetic latitude. A proper per-location seasonal climatology would need years of history and a real model; that's a later milestone (a longer-term data store), not this.
Kp index what it measures
Kp is a 0–9 planetary index of geomagnetic disturbance, issued every three hours by NOAA from a network of magnetometer stations. Higher means the Earth's magnetic field is being shaken harder by the solar wind, which pushes the auroral oval further from the poles. It's a global average, not a local reading — so a high Kp is necessary but not sufficient to see aurora where you are; that depends on how far the oval reaches your latitude (next card).
Magnetic latitude & "Kp needed here" the threshold
Aurora sits over the geomagnetic poles, which don't line up with the geographic ones — so what matters for you is your magnetic latitude, not the one on a map. We estimate it with a centred-dipole approximation (a tilted-bar-magnet model of Earth; pole near 80.6°N, 72.7°W). The "Kp needed here" figure uses the well-known rule of thumb required Kp ≈ (66 − |magnetic latitude|) ÷ 2. It's a rough estimate, not a precise forecast — it ignores the non-dipole wrinkles of the real field and local sky conditions — but it's honest about which places need a big storm (low magnetic latitude) versus a quiet night (under the oval).
OVATION probability the model
OVATION Prime is NOAA's short-term auroral-precipitation model. Every few minutes it estimates, on a 1° global grid, the chance of visible aurora overhead — driven by live solar-wind measurements from the DSCOVR/ACE spacecraft upstream of Earth. The "chance here" number is that model's value at your exact grid cell (we snap your coordinates to the nearest degree). It's a genuine physical model, but a short-range one: it says what the sky is likely doing in the next ~30 minutes, not tonight as a whole, and it can't know your clouds.
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