How to Read the Aurora Forecast
Chasing the lights shouldn't feel like guesswork. Hello Aurora tracks real-time space weather to tell you exactly when to look up.
Here are the three main metrics you need to know:
Aurora Strength
Aurora Strength is a real-time measurement used to predict how active, bright, and visible the Northern Lights are at any given moment. Think of this as the main "go or no-go" signal. It measures real-time changes in Earth’s magnetic field caused by solar activity.
The Aurora Borealis are caused by streams of charged particles from the sun smashing into Earth’s magnetic field. When this happens, it causes the magnetic field to vibrate, bend, and fluctuate. Magnetometers detect these fluctuations and record them in a unit called nanoteslas (nT). The bigger the fluctuation in nanoteslas, the more intense the aurora display will be.
- When it drops sharply (around -150 nT): A "substorm" is happening. The lights are likely actively dancing right now. The lower this number goes, the wilder and brighter the show will be.
- When it spikes up (around +150 nT): The aurora is "charging up." Get your camera ready, because a display is often just minutes away.
- When it hovers near zero (around 5 nT): The skies are temporarily quiet. Time to grab a warm drink and wait.
Why it is Better Than Traditional Forecasts
Many people rely on the Kp-index to hunt the Northern Lights, which is a global average calculated only once every 3 to 6 hours.
Because the aurora can change in a matter of minutes, Aurora Strength is much more accurate for active hunting. It updates in real time, letting you know exactly when to step outside your hotel so you don't miss a sudden, spectacular show.
The Interplanetary Magnetic Field (IMF)
The Interplanetary Magnetic Field (IMF) is the sun’s magnetic field traveling through space. When forecasting the lights, this field is broken down into two main numbers: Bt and Bz.
Here is what those numbers mean for aurora hunting:
IMF Bz (The Direction)
Bz measures the north-south direction of the magnetic field. When Bz points south (showing as a negative number), it connects with Earth’s magnetic field near the poles and creates the conditions needed for an aurora.
- What to look for: Look for a negative Bz number. The further below zero the number goes, the higher your chances of seeing a display.
- Good conditions: A Bz of -10 nT or lower.
- Best conditions: A Bz of -15 nT or even lower (such as -20 nT). Deeply negative numbers produce the strongest, most vibrant auroras.
IMF Bt (The Strength)
Bt measures the total strength of the incoming solar magnetic field. The aurora is much more likely to happen when this field presses strongly against Earth’s magnetic shield.
- What to look for: In contrast to Bz, you want the Bt number to be as high as possible.
- Good conditions: A Bt higher than 10 nT shows decent energy.
- Best conditions: A Bt higher than 20 nT means a large amount of solar energy is arriving, significantly increasing your chances of seeing a spectacular show.
Solar Wind
Just as you feel the wind more strongly when walking outside on a breezy day, the same principle applies to the solar wind.
The faster the solar wind travels toward Earth, the more energy it transfers into the planet’s magnetic field. This increases the likelihood that the aurora will become brighter, more dynamic, and more visible in the night sky.
Monitoring solar wind speed is an important factor for predicting when and where the Northern Lights will put on their most spectacular displays.
Real-Time Metrics Summary