AURORA SIMULATION

Auroral colours are elemental signatures. Oxygen between roughly 100 and 250 km emits the familiar green line at 557.7 nm; thinner oxygen at 200 to 400 km gives the deep red 630.0 nm; nitrogen tints the lower fringe violet-pink near 427.8 nm. The stronger the solar wind, the more energy is fed in, so the auroral oval swells down towards lower latitudes while the Kp index climbs. A substorm dumps the magnetotail’s stored energy all at once, and the curtains flare and dance for some 30 to 60 minutes.

▸ Launching solar wind from the corona…
▸ Guiding particles along field lines to both poles
▸ Atmospheric collisions ~100–300 km
▸ Exciting oxygen (green/red) & nitrogen (violet)
▸ Calibrating auroral oval & Kp…
▸ Ready — Online. ✅
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Simulation room Aurora

Aurora
Online
solar wind · Kp
Kp gauge
🌌 Aurora intensity
Kp ≥ 5 = geomagnetic storm
Scenario—
Solar wind—
Kp index—
Emission altitude—
Dominant colour—
Visible down to—
Notes
Solar wind follows the magnetic field lines toward the two poles, exciting oxygen (green 557.7 nm · red up high) & nitrogen (violet). Geographic North = magnetic South; the northern & southern aurorae are symmetric.
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Adjust the solar wind & try “Strong storm” on the right · toggle field lines · click a concept for details
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Solar wind & Kp over time windKp
About Aurora

Auroral colours are elemental signatures. Oxygen between roughly 100 and 250 km emits the familiar green line at 557.7 nm; thinner oxygen at 200 to 400 km gives the deep red 630.0 nm; nitrogen tints the lower fringe violet-pink near 427.8 nm. The stronger the solar wind, the more energy is fed in, so the auroral oval swells down towards lower latitudes while the Kp index climbs. A substorm dumps the magnetotail’s stored energy all at once, and the curtains flare and dance for some 30 to 60 minutes.

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