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CVAN
Aurora viewing guide

How to see the Northern Lights

What drives whether the aurora reaches your latitude tonight: the Kp index, your geomagnetic latitude (which is different from your geographic latitude), the season, and the simple sky-condition factors that can ruin even a perfect forecast.

Open the live aurora forecast →

What the aurora actually is

The aurora is high-altitude (80–500 km) emission from oxygen and nitrogen atoms in the upper atmosphere, energised when charged particles from the Sun get steered down magnetic field lines into the polar regions. The bright green colour is from atomic oxygen at ~100 km altitude; the red glow above is from oxygen at higher altitudes; pinks and blues come from nitrogen.

Activity is driven by the Sun's wind and especially by coronal mass ejections — and follows the ~11-year solar cycle. We're currently near the maximum of Solar Cycle 25, so 2024–2027 are unusually good years for aurora at mid-latitudes.

The Kp index

The Kp index is a 0-to-9 number summarising global geomagnetic activity, derived every three hours from ground magnetometer readings around the world. NOAA's Space Weather Prediction Center (SWPC) publishes a real-time estimated Kp every 5 minutes and a 3-day forecast every 30 minutes.

Geomagnetic vs geographic latitude

The auroral oval is centred on the geomagnetic pole, which is offset from the geographic pole by about 11°. The geomagnetic north pole is currently in the Canadian Arctic near Ellesmere Island. This means:

CVAN computes your geomagnetic latitude using the IGRF-13 dipole model and compares it directly to the Kp viewing threshold. That's why the verdict can say "viewable" at Kp 4 from one location and "too far from pole" from another at the same geographic latitude.

Kp thresholds by city

Approximate minimum Kp needed for aurora to be visible on the northern horizon from common viewing cities (assuming clear skies and dark site):

Tromsø, Norway
Kp 0 — directly under the auroral oval
Fairbanks, AK
Kp 0–1
Reykjavík, Iceland
Kp 2
Edmonton, AB
Kp 2–3
Stockholm
Kp 3
Edinburgh
Kp 5
Seattle, WA
Kp 5
Minneapolis, MN
Kp 5
Boston, MA
Kp 5–6
London
Kp 6
New York, NY
Kp 6–7
Chicago, IL
Kp 6–7
San Francisco, CA
Kp 7–8
Madrid
Kp 8
Texas, US south coast
Kp 9 (rare)

Other essential factors

It must be night

Aurora doesn't show against a daylight or twilight sky. The sun must be below about −12° altitude (nautical twilight) to start seeing colour; below −18° (astronomical night) is ideal. This is why summer in northern Scandinavia is hopeless for aurora despite massive solar activity — the sun never sets enough.

Clear skies

Cloud cover above ~70% blocks aurora completely. CVAN factors in the Open-Meteo cloud cover forecast and warns when you've got viewing latitude but lose the bet to weather.

Magnetic local time

Aurora is strongest around magnetic midnight — the time when your location is on the night side of the Earth's magnetic axis. For most of North America and Europe this corresponds roughly to 10 PM – 2 AM local time.

Solar activity

High Kp comes from coronal-mass ejections (CMEs) and coronal-hole high-speed streams. SWPC's 3-day Kp forecast — pulled into CVAN's Kp Forecast tab — is the most actionable signal; a CME that arrives in 2 days will already be in the forecast curve.

Using the live forecast

CVAN's Aurora tab presents:


Quick reference

Best season
September–March in N. Hemisphere (long, dark nights)
Best time
10 PM – 2 AM local (magnetic midnight)
Min sun altitude
Below −12° (nautical twilight)
Max cloud cover
Under 70%
Live Kp source
NOAA SWPC, refreshed every 5 minutes
Geomagnetic model
IGRF-13 dipole approximation
Open the live aurora forecast →

Related guides

Guide
Seeing the Milky Way
Season-by-season viewing plan, photography tips, and the role of light pollution.
Guide
The Bortle Scale
What each tier of darkness actually looks like, and what's visible from each.
Reference
Stargazing FAQ
Fifteen short answers to the most common stargazing questions.