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⚡ Weather

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Space Weather

Quiet
Kp Index
0 3 5 7 9

IMF Bz
Solar Wind
X-Ray A Normal
Aurora Power

Magnetosphere
Magnetopause— Re
Bow Shock — Re
Plasmapause — Re
Dst proxy — nT
Joule heat — GW

Sun → Earth Coupling
Energy input ε — GW
IMF clock θ —°
Merging rate
X-line Vᵣ — km/s
FAC R1+R2 — MA
Substorm idx
Alfvén speed — km/s
Plasma β
L1 lag — min

Ionospheric Layers

Solar decl.
Subsolar pt

Space Weather Impacts
HF Radio
GPS / GNSS
Spacecraft
Power grids
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Solar Forecast & Time Analysis
Kp (24h forecast)
Trend (H-W)
G1+ storm / 24h
G2+ storm / 72h
27-d echo
SC25 phase
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Weather Analysis

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Updated

T° min
T° max
T° mean

P low
P high

Max wind

Isobars
Max ∇P
Geo wind
Centers

Storm Alerts

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Earth Magnetosphere & Space Weather

A real-time 3D simulation of Earth's magnetic shield — from the bow shock where solar wind first strikes, through the compressed magnetosheath, magnetopause boundary, and out to the elongated magnetotail. Aurora, substorm dynamics, and Kp index are driven by live NOAA data.

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Bow Shock & Magnetosheath
The bow shock forms at roughly 13–14 Earth radii (Re) sunward, where supersonic solar wind (~400 km/s) is abruptly decelerated. The Rankine-Hugoniot jump conditions heat and deflect plasma into the magnetosheath — visualized as orange-tinted shocked particles.
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Magnetopause (Shue Model)
The magnetopause boundary is calculated using the Shue et al. (1998) empirical model, parameterized by solar wind dynamic pressure and the IMF Bz component. Southward Bz compresses the dayside boundary; strong storms push it inside geostationary orbit (~6.6 Re).
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Magnetotail & Plasma Sheet
On the nightside, the magnetotail stretches to 80+ Re — far beyond the Moon's orbit. The central plasma sheet (high-density, ~1–5 keV particles) brightens during substorms as stored magnetic energy explosively reconnects and accelerates particles toward the poles.
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Aurora & Substorms
3D auroral curtains expand equatorward as Kp rises (Kp ≥ 5 = G1 storm). Color gradients reflect emission height: green O 557.7 nm at 100–150 km, shifting to purple N₂⁺ + red O 630 nm above 200 km. Substorm onset (McPherron heuristic) triggers a ripple flash across both ovals.
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3D Globe & Ground Effects
The interactive globe shows live earthquake events (USGS feed), geomagnetic storm impact zones, aurora visibility oval, and atmospheric layers. Overlays include field-aligned current regions and ground-level induction risk during severe storms.
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Live Geomagnetic Data
Kp index, Dst, IMF Bz, solar wind speed and density all update every 5 minutes from NOAA/SWPC. Storm levels follow the NOAA G1–G5 scale, from minor (Kp 5) to extreme (Kp 9), with real-time aurora visibility latitude estimates.
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LayersToggle bow shock, aurora, tail, field lines
InfoLive Kp, Bz, storm level readings
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