How to Read the Aurora Forecast

Most aurora disappointment comes from the same mistake: reading a single number, seeing it look promising, driving somewhere dark, and finding nothing. This is the full check, in the order that actually matters.

TL;DR

Aurora needs four things at once: enough geomagnetic activity, the right solar wind setup, a dark sky, and no cloud. Miss any one and the night is a write-off. Kp only covers the first.

1. Kp is not about you

The Kp index is a 0–9 scale of how disturbed Earth’s magnetic field is as a whole. It’s a planetary average, updated every three hours. It genuinely tells you how big the storm is.

What it does not tell you is whether the aurora is above your head, because that depends on where you are relative to the magnetic pole — not the geographic one. The auroral oval is a ring centred on the magnetic pole, and the magnetic pole is currently up near northern Canada, nowhere near true north.

The practical consequence is large. Edinburgh sits at 56.0°N and Moscow at 55.8°N — nearly identical on a map. But in geomagnetic terms Edinburgh is at about 58° and Moscow about 52°. Edinburgh sees aurora several times a year. Moscow, at the same map latitude, needs a far bigger storm.

So the useful question isn’t “what’s the Kp?” It’s “what Kp does my location need?” That’s exactly what our per-location forecasts calculate — the threshold for over 200 places, from Fairbanks to Lille.

As a rough guide, the aurora becomes visible on the poleward horizon at these geomagnetic latitudes:

| Kp | Visible from geomagnetic latitude | |----|-----------------------------------| | 3 | 60.4° and poleward | | 5 (G1) | 56.3° | | 7 (G3) | 52.2° | | 9 (G5) | 48.1° |

Add roughly two more Kp for the aurora to be overhead rather than a glow near the horizon.

2. Bz is the on/off switch

If you check one solar wind value, make it Bz — the north–south direction of the magnetic field carried by the solar wind.

Negative (southward) Bz is what you want. It lets the solar wind’s field connect with Earth’s, which is what actually pours energy into the system. Positive Bz largely closes that door, and the same storm can produce very little.

Bz flips around on timescales of minutes. A steady −10 nT or lower for a sustained period is a strong signal. Brief dips matter less than sustained ones. Watch it live on the solar wind dashboard.

Speed helps too — 500 km/s and up is a good sign — and Bt, the total field strength, tells you how much magnetic field is available to work with. But a fast wind with northward Bz is a common and thoroughly disappointing combination.

3. Kp is a lagging number; the solar wind is a leading one

This trips up a lot of people. Kp is calculated after the fact, from magnetometers, and published in three-hour blocks. The solar wind data comes from satellites parked upstream at the L1 point, about 1.5 million kilometres sunward of Earth.

That gives you roughly 15 to 60 minutes of genuine warning. If Bz swings sharply south right now, the effect reaches Earth well before the Kp number catches up. Watching Bz is watching the future; watching Kp is reading the past.

4. Darkness — the one people forget

You need an actually dark sky, and at high latitudes in summer you may simply not get one. Above the Arctic Circle the sun doesn’t set at all for weeks around midsummer. Tromsø has no aurora season from roughly late May to late July, no matter what the Sun does.

Even outside those extremes, you want astronomical darkness, not just sunset. Aurora activity also tends to peak around magnetic midnight, generally somewhere in the 22:00–02:00 window local time.

A bright full moon won’t cancel a strong display, but it will wash out a faint one.

5. Cloud beats everything

Cloud is the most common reason a promising night produces nothing at all. Kp 7 under solid overcast is worth exactly the same as Kp 0. It is genuinely worth driving an hour to a gap in the cloud — that’s often a bigger improvement than anything the Sun is doing.

Every location page shows tonight’s cloud cover and darkness window alongside the Kp threshold, so you can rule out a night in about five seconds.

Set your expectations correctly

This is the honest part, and it’s where most first-timers get let down.

At your threshold Kp — the point where aurora just clears your horizon — you are looking for a faint grey-green glow low in the northern sky. To the naked eye it can look like a pale cloud that doesn’t drift. It will not look like the photographs.

Those saturated green-and-purple images are long exposures. A camera sensor accumulates light over several seconds; your eye does not. Human colour vision also gives out in low light, which is why a display that photographs vividly green often reads as grey to the eye.

You need to be well inside the oval, not at its edge, before you get the bright overhead curtains that move. That’s a genuinely different experience — and it needs a much higher Kp, or a trip further north.

Knowing this in advance is the difference between a disappointing night and a good one.

The checklist

• Kp is at or above your location’s threshold — not just “high”
• Bz negative and staying there
• Speed 500 km/s+ helps
• Sky is properly dark where you are
• Cloud cover is low
• You’ve got an unobstructed view toward the pole, away from streetlights
• Give your eyes 20 minutes to adapt, and don’t look at your phone