What Is the Kp Index?

The Kp index is the single most important number for predicting whether you'll see the aurora tonight. Here's what it means and how to use it.

The Basics

The Kp index measures geomagnetic activity on a scale from 0 to 9. Higher numbers mean stronger disturbances in Earth's magnetic field, which means brighter, more widespread aurora. It's updated every 3 hours by NOAA's Space Weather Prediction Center based on data from magnetometer stations around the world.

KpActivity LevelWhat It Means for Aurora
0–1QuietAurora only visible near the Arctic (Fairbanks, northern Scandinavia)
2–3UnsettledGood displays in Fairbanks/Denali; faint in Anchorage
4ActiveVisible across most of Alaska; possible in northern Lower 48
5Minor Storm (G1)Strong displays statewide; visible in northern US states
6–7Moderate–Strong StormVivid aurora across Alaska and into the Lower 48
8–9Severe StormRare. Aurora visible from the southern US. Historic display.

What Kp Do You Need in Alaska?

Each location in Alaska has a different Kp threshold because of its latitude. The further north you are, the less activity you need.

LocationKp for Visible AuroraKp for Strong Display
Fairbanks13
Denali Area23
Talkeetna24
Palmer–Wasilla35
Anchorage35
Kenai Peninsula45
Juneau56

Kp Isn't the Whole Story

The Kp index tells you about geomagnetic activity, but three other factors matter just as much:

Alaska Glow combines all four of these factors into a single score for each location, so you don't have to check multiple sources.

Check tonight's aurora conditions across 7 Alaska locations

View Tonight's Forecast →

Where Does the Kp Forecast Come From?

NOAA's Space Weather Prediction Center monitors the sun for coronal mass ejections (CMEs) and solar wind streams. They issue Kp forecasts up to 3 days out, though accuracy drops significantly beyond 24 hours. Real-time Kp is measured every minute from ground-based magnetometers worldwide.

For aurora watching, the most useful data is the 1-minute real-time Kp combined with solar wind measurements from the DSCOVR satellite positioned between Earth and the Sun. When a burst of solar wind with strong southward Bz is detected at DSCOVR, aurora follows about 30–60 minutes later.