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Explore Earth's magnetosphere as a teaching schematic: dipole field lines tilted ~11 deg, sunward magnetopause compressed to ~6-10 Earth radii by the solar wind, and surface field ~25-65 uT.

Preparing the 3D scene...

Published figures: surface field ~25-65 uT, dipole tilt ~11 deg, sunward magnetopause typically ~6-10 Re under solar-wind pressure (NASA magnetosphere overview).

Drag to orbit and scroll or pinch to zoom. Use Quiet / Compressed presets or the magnetopause slider; toggle solar-wind particles.

Earth Magnetosphere 3D Explorer


Earth's magnetosphere is a teaching schematic here - dipole field lines, a compressed sunward magnetopause, and optional solar-wind particles - not an MHD model.

Surface field intensity is about 25-65 uT. The magnetic dipole tilts about 11 deg from Earth's spin axis. Solar wind compresses the sunward magnetopause to roughly 6-10 Earth radii (Re) - Quiet about 10 Re and Compressed about 6 Re presets match that published range.

Adjust tilt and magnetopause standoff, or hide the solar-wind particle stream. The facts panel lists the same figures.

  • Dipole field-line cage with adjustable about 11 deg tilt
  • Orange magnetopause wire shell at 6-12 Re (teaching standoff)
  • Quiet about 10 Re and Compressed about 6 Re presets
  • Optional solar-wind particles from the Sunward side
  • Surface field about 25-65 uT in the facts table
  • Complements aurora (emission curtains) and solar-wind-heliosphere (AU-scale bubble)
  • Runs fully in the browser with the vendored three.js engine - no account, no upload
Compare four Earth-magnetosphere explorer features: Dipole field, magnetopause, Quiet about 10 Re, Optional solar wind.
Dipole field, magnetopause, Quiet about 10 Re, Optional solar wind at a glance.

Students see why the day side is squashed; teachers demo magnetopause standoff without a blackboard sketch; curious readers connect field tilt to the aurora oval's magnetic frame.

FigureValueSource note
Surface fieldabout 25-65 uTPublished surface intensity range
Dipole tiltabout 11 degMagnetic vs rotation axis
Magnetopause (sunward)about 6-10 ReSolar-wind compression (NASA overview)

Everything renders on your device with WebGL. The 3D engine loads once (about 0.7 MB) and is cached; no scene data is sent to a server.

This is an educational dipole + boundary schematic - not an MHD magnetosphere model, not a live solar-wind or IMF feed, and not a Van Allen belt particle solver.

For a step-by-step walkthrough, read the Earth Magnetosphere 3D Explorer step-by-step guide. When you need session fit and limits, see when to use Earth Magnetosphere 3D Explorer. The Space 3D collection also includes Aurora 3D and Solar Wind Heliosphere 3D.

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Frequently Asked Questions

What does the Earth Magnetosphere 3D Explorer show?

A teaching schematic of Earth's dipole field lines, ~11 deg tilt, sunward magnetopause at ~6-10 Re, and surface field ~25-65 uT with optional solar-wind particles.

How far is the magnetopause on the day side?

Typically about 6-10 Earth radii sunward under solar-wind pressure. Quiet ~10 Re and Compressed ~6 Re presets span that published range.

What is the dipole tilt?

About 11 degrees between Earth's magnetic axis and its rotation axis - the tilt slider defaults near that published value.

How strong is Earth's surface magnetic field?

About 25-65 microtesla across the surface - listed in the facts panel as the published intensity range.

Is this an MHD magnetosphere model?

No. It is an educational dipole and boundary schematic - not an MHD solver or a live space-weather forecast.

How is this different from Aurora 3D?

Aurora 3D teaches emission curtains and Kp oval size. This page teaches the large-scale field and magnetopause boundary that frames those ovals.