MAGNETOSPHERE & AURORA SIMULATION

The needle that points north is actually being pulled by a magnetic SOUTH pole: Earth’s geographic north is where the south end of the giant magnet born in the liquid iron core sits, and that magnetic axis is tilted about 11 degrees from the spin axis. The magnetosphere is therefore no sphere but a teardrop, squashed on the dayside and drawn out into a tail on the nightside. As the solar wind strengthens from 250 to 1,000 km/s it presses the magnetopause inward, and one such storm brought down the Quebec power grid in 1989.

▸ Building the dipole field…
▸ Launching the solar wind & bow shock
▸ Compressing the magnetopause, drawing the magnetotail
▸ Wiring the Van Allen belts & aurora
▸ Calibrating the Kp index…
▸ Ready — Online. ✅
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Simulation room Magnetosphere & Aurora

Magnetosphere
Online
solar wind · Kp
Kp gauge
🧲 Geomagnetic disturbance
Kp ≥ 5 = storm
Mode—
Solar wind—
Kp index—
Aurora—
Magnetopause—
Note
The magnetosphere deflects the solar wind — a shield that keeps the atmosphere & life. Particles entering at the poles → aurora.
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Adjust the solar wind & try “Storm” on the right · toggle the Van Allen belts · click a structure for details
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Solar wind & Kp over time windKp
About Magnetosphere

The needle that points north is actually being pulled by a magnetic SOUTH pole: Earth’s geographic north is where the south end of the giant magnet born in the liquid iron core sits, and that magnetic axis is tilted about 11 degrees from the spin axis. The magnetosphere is therefore no sphere but a teardrop, squashed on the dayside and drawn out into a tail on the nightside. As the solar wind strengthens from 250 to 1,000 km/s it presses the magnetopause inward, and one such storm brought down the Quebec power grid in 1989.

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