🌌 Aurora Solar Wind Chamber

Kristian Birkeland's Terrella experiment. Solar wind plasma streams channeled along geomagnetic dipole field lines excite shimmering atmospheric auroral ovals.

SOLAR WIND FLUX: LEFT TO RIGHT // MAGNETOPAUSE BOW SHOCK Oxygen 557.7 nm Emerald Green Emission

Geomagnetic Kp-Index

Kp = 3.0 (Minor)

Solar Wind Velocity

450 km/s

Auroral Oval Latitude

67.5° N/S

Solar Wind Density 5.5 protons/cm³

Interplanetary Magnetic Field (Bz) -4.2 nT (Southward)

Birkeland Lorentz Drift Active

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