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Geomagnetic Conditions

Discover the impact of the solar wind on Earth. Data retrieved in real time from the DSCOVR and ACE satellites orbiting at L1.

Real-Time Solar Wind

SpeedNOAA
-- km/s

Solar wind speed indicates how quickly plasma travels from the Sun to Earth. Normal values range from 300-400 km/s. Above 500 km/s, geomagnetic storms become much more likely, pushing the aurora to lower latitudes.

DensityNOAA
-- p/cm³

Represents the number of plasma particles per cubic centimeter. High density (above 10 p/cm³) acts as 'fuel' for the aurora, making it extremely bright, dynamic and visible to the naked eye.

Bt (Total Field)NOAA
-- nT

Represents the overall strength of the interplanetary magnetic field. Even if Bz is negative, a sufficiently high Bt (e.g. > 10 nT) is needed to trigger a strong geomagnetic storm.

Bz (Magnetic Field)NOAA
-- nT

The most important factor. It indicates the orientation of the interplanetary magnetic field (IMF). It must be negative (southward) to connect with Earth's field and allow solar particles to enter our atmosphere. The more negative, the better.

Kp Forecasts & Activity

Auroral Oval Extent (Ovation Model)Ovation Prime
Aurora Forecast
Visibility Tonight
Tonight Viewline
Visibility Tomorrow Night
Tomorrow Viewline

The red line (Viewline) indicates the southernmost limit where the aurora may be visible on the horizon under optimal weather conditions.

Planetary Kp Index (Last 24h)NOAA API

The Kp index measures disturbances in Earth's magnetic field on a scale from 0 to 9. The chart shows activity recorded over the past few hours. Green values indicate quiet conditions, yellow moderate activity, and red an ongoing storm.

Kp Forecast (3 Days)NOAA Prediction
Caricamento previsioni...

Maximum Kp peaks forecast by NOAA for the next 3 days.

Energy & Space Propagation

Hemispheric Power (HP)Real-Time
-- GW (Gigawatts)
0 GW50 GW100+ GW

Hemispheric Power estimates the total energy deposited by solar particles in the upper atmosphere. It is much more accurate than Kp for real-time conditions. Values below 20 GW indicate low activity. Between 50 and 100 GW, the aurora is spectacular and widespread.

WSA-Enlil Model (CME Propagation)WSA-Enlil Player
Caricamento player...

This NASA/NOAA model simulates the propagation of a coronal mass ejection (CME) from the Sun to Earth. Earth is the yellow (or green) dot. A dense plasma wave (red/white) colliding with Earth indicates the imminent arrival of a strong geomagnetic storm.

Live Webcams

Check current activity in real time through the main Arctic webcams.

Abisko (Sweden)
Abisko (Sweden)
Tromsø (Norway)
Tromsø (Norway)
Rovaniemi (Finland)
Rovaniemi (Finland)
Yellowknife (Canada)
Yellowknife (Canada)

Take monitoring with you

Download the app to set custom sound alerts for Kp, negative Bz and live sightings near you.

Get it on Google PlayDownload on the App Store