Kp-Index (Disturbance)
Measures geomagnetic activity on a scale of 0 to 9. Higher values indicate Earth's magnetic field is being shaken by the solar wind.
Current Kp
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Wind Speed
The velocity of particles leaving the Sun. Fast winds (500+ km/s) act like a powerful blower that lights up the aurora.
Wind Speed
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IMF Bz (The Door)
Shows if the magnetic field is pointing South (negative). A negative Bz 'opens the door' for energy to enter our atmosphere.
IMF Bz
-- nT
Direction
Proton Density
The thickness of the solar wind. High density means more particles are hitting the atmosphere, making the aurora brighter.
Density
-- p/cm³
Particle Density
HPI (Power GW)
Real-time estimate of the total energy (Gigawatts) entering the atmosphere. Higher GW = bigger, brighter aurora.
Power (HPI)
-- GW
Total Energy
Radio Flux (F10.7)
Indicates how active the Sun is overall. During 'Solar Maximum', this number is high, meaning more solar storms.