Aurora activity
LiveQuiet
Kp 1.3
How disturbed Earth's magnetic field is right now — higher means aurora reaches further south.
NOAA SWPC · planetary Kp· 2026-11-05T09:00:00.000Z
Aurora forecast · tonight
Kp is 1.3 (quiet). On a clear, dark night the aurora should be overhead near 64°N — roughly northern Alaska, Iceland, and northern Scandinavia — and may be visible low on the northern horizon for a few degrees further south. NOAA's OVATION model puts tonight's peak overhead probability at 21%. Enter your city below for a verdict for your exact latitude.
Explanations by Spaceweathertracker staff · Last reviewed · Editorial standards · About
Search any city, town, or postcode for a verdict calculated against your exact latitude.
Aurora activity
LiveQuiet
Kp 1.3
How disturbed Earth's magnetic field is right now — higher means aurora reaches further south.
NOAA SWPC · planetary Kp· 2026-11-05T09:00:00.000Z
Next 3 hours
LiveQuiet
Forecast Kp 1.7
NOAA's official forecast for the upcoming 3-hour interval.
NOAA SWPC · 3-day Kp forecast
OVATION peak
Live21%
Peak overhead probability
Highest chance anywhere on the modelled oval of aurora directly overhead in the next 30 minutes.
NOAA OVATION · 30-minute model· 2026-11-05T12:10:04.525+00:00
Visibility line
Live63.8°N
Southern edge of the aurora zone
Above this latitude the aurora can appear overhead; just below it, look low to the north.
Derived from verified Kp· 2026-11-05T09:00:00.000Z
NOAA's OVATION 30-minute forecast, drawn on the real map. Brighter bands mark a higher chance of aurora directly overhead.
Latest NOAA planetary Kp is 1.3, observed Nov 5, 2026, 9:00 AM UTC. NOAA OVATION peak overhead aurora probability is 21%.
NOAA OVATION Aurora Oval Model
Interactive map with live data layers
What NOAA expects over the next three days.
Official SWPC forecast in 3-hour intervals. Kp 5 or higher is storm level, when aurora pushes furthest from the poles.
Thu, 5 Nov
Max Kp 4
Fri, 6 Nov
Max Kp 5
Sat, 7 Nov
Max Kp 5
What this means: geomagnetic activity is one factor used to assess aurora potential. Higher Kp can expand auroral visibility toward lower latitudes, but cloud cover, darkness, your location, and solar wind conditions (like Bz) also matter — a high Kp forecast does not guarantee a visible aurora at any given spot.
Continuous all-sky and webcam feeds from high-latitude observing sites.
📡 STATUS: Live camera feed from the observatory operator.
Northumberland AstroEmbleton, Northumberland, England — A north-facing camera on the UK's northeast coast — only catches visible aurora during strong geomagnetic storms, given its lower latitude.
Genuine NASA photographs of the aurora, from orbit and from satellite.
Plain-English answers to the questions people ask most about the northern lights.
🚀 Local Aurora Intent: QUIET geomagnetic activity right now (Kp 1.3). Conditions are currently quiet — check your specific location below for real visibility odds.
💡 What This Means for You (Plain English Mode)
The real, current Kp index of 1.3 puts overall activity in the "Quiet" range. Aurora visibility from any specific place still depends heavily on that location's magnetic latitude — search your city on the dashboard for a real, calculated answer.
• Data source: NOAA SWPC
It depends on three things: the current Kp index, how far north (or south) you are in magnetic latitude, and whether your sky is clear and dark. Search your city above to see tonight's Kp needed for your location, the live aurora oval, and your viewing probability.
Enter your town in the location search on this page. We compare NOAA's live OVATION aurora model and Kp forecast with your latitude, then show whether the northern lights are likely overhead, on your northern horizon, or out of reach tonight.
Activity usually peaks within an hour or two of local magnetic midnight, roughly 10 PM to 2 AM local time. Watch from full darkness (after astronomical twilight) and stay out for at least an hour, because the aurora comes and goes in bursts.
Near the Arctic Circle, Kp 1–3 is often enough. Southern Canada and the northern US tier typically need Kp 5 (a G1 storm), and mid-latitude states need Kp 7 or higher. The visibility line on our map shows the southern edge for the current Kp.
The solar wind and coronal mass ejections from the Sun disturb Earth's magnetic field, which drives charged particles into the upper atmosphere. They collide with oxygen (green and red light) and nitrogen (blue and purple light), making the sky glow.
Auroral activity typically peaks around local magnetic midnight, between 10:00 PM and 2:00 AM local time. Optimum viewing requires true astronomical darkness (after twilight ends) with clear skies facing north. Check our live planetary Kp index and auroral oval map to see if activity is currently surging.
The most active viewing window occurs between 10:00 PM and 2:00 AM local time. However, sudden substorms can ignite auroral curtains earlier in the evening or persist into the pre-dawn hours whenever the solar wind magnetic field (Bz) points strongly southward.
Look for an open location with an unobstructed view of the northern horizon, far away from city streetlights. Locations rated Bortle Class 1 to 3 offer the highest contrast. Use our interactive Dark Sky Map (/interactive-maps/dark-sky) to locate dark sky parks and low light pollution viewing spots near you.
Yes, major geomagnetic storms triggered by Coronal Mass Ejections (CMEs) often persist over 24 to 48 hours as Earth passes through the interplanetary plasma cloud. Check the live Kp gauge on this page: if the index remains elevated at Kp 5 or above, active aurora displays may continue for a second consecutive night.
Visibility depends on your geomagnetic latitude and the current Kp index. At Kp 5 (G1 storm), northern US states and southern Canada can see the aurora. At Kp 7 (G3 storm), the aurora line drops into mid-latitude states like Iowa, Illinois, and Pennsylvania. Check our real-time visibility line above to see if your town is within tonight's view line.
New to aurora watching? Watch what causes the northern lights.
Aurora visibility for every US state and major city — 50 states and 212 cities.
Weekly Space Weather Briefing
We track coronal mass ejections and Kp spikes live. Get notified when geomagnetic conditions favor viewing in your region.
The aurora begins with the solar wind — a continuous stream of charged particles flowing outward from the Sun. When this stream, sometimes intensified by a coronal mass ejection, reaches Earth, it collides with and compresses our planet's magnetosphere. Along field lines near the poles, charged particles are funneled down into the upper atmosphere, where they collide with oxygen and nitrogen molecules and transfer energy into them — a process called ionization.
Once ionized, those atmospheric atoms release the absorbed energy as light as they return to their normal state, and the color depends on which atom is involved and at what altitude. Oxygen produces the aurora's familiar green glow at lower altitudes (around 100-150 miles up) and a rarer red glow higher up. Nitrogen typically produces blue and purple hues, often visible along the lower edges of an active display.
Aurora activity isn't constant — it rises and falls with the Sun's roughly 11-year solar cycle. Near solar maximum, sunspots, flares, and coronal mass ejections are all more frequent, driving stronger and more frequent geomagnetic storms and pushing the aurora to lower latitudes than usual. Tracking the current phase of the solar cycle is one real way to gauge how active a given season is likely to be.
The aurora is driven by the Sun's continuous solar wind and occasional coronal mass ejections, which compress Earth's magnetosphere and funnel charged particles into the upper atmosphere, where they collide with oxygen and nitrogen to produce visible light.
The optimal observation window opens during maximum astronomical dark hours, when moon illumination is low and local cloud cover stays under about 20% for a genuinely clear sky.
Baseline tracking can be done with the naked eye. For fainter, low-contrast targets, a steady tripod-mounted pair of wide-field binoculars or a small telescope makes a real difference.
Search your specific city or coordinates above — visibility depends on your exact latitude and local horizon, not just your general region.
Learn how to plan your Northern Lights viewing — best months, best places, photography tips, and how to read the data above.