🧊 Superconductor Meissner Effect
Interactive 3D superconductor simulator. Cool a puck below its critical temperature to watch it actively expel a magnetic field (the Meissner effect) and levitate a magnet. Explore London penetration depth, Cooper pairs and Type-I vs Type-II superconductivity.
About the Meissner Effect
This interactive 3D simulator renders, in real WebGL, the defining property of superconductivity: the Meissner effect. A superconductor below its critical temperature Tc does not merely conduct without resistance — it actively expels an applied magnetic field from its interior using persistent surface supercurrents, so the field survives only in a thin layer near the surface, the London penetration depth λ. That expulsion is what pushes a permanent magnet upward and holds it levitating in mid-air, and in real Type-II materials, defects that pin the resulting flux vortices in place give the levitation lateral stability rather than just vertical repulsion.
Cool the puck below Tc and a magnet resting on its surface lifts off and hovers. Warm it back above Tc and the field floods back through the now-normal material, and the magnet settles back down. Switch between Type-I (mercury-like, abrupt and complete expulsion, low Tc) and Type-II (YBCO-like, partial flux penetration above a lower critical field, high Tc) to see how the two classes of superconductor behave differently as you push the magnet's field strength higher.
Frequently Asked Questions
What is the Meissner effect, exactly?
The Meissner effect is the spontaneous expulsion of magnetic field lines from the interior of a material as it transitions into the superconducting state. It is distinct from simple perfect diamagnetism or "flux freezing": a hypothetical perfect conductor would merely trap whatever field was present when it became resistance-free, but a real superconductor actively pushes existing field out too, regardless of the field's history. This was demonstrated experimentally by Walther Meissner and Robert Ochsenfeld in 1933.
How do I use this simulation?
Pick a material — Type-I (mercury) or Type-II (YBCO) — then drag the Temperature slider through the critical temperature Tc and watch the magnet lift off once the puck goes superconducting. The Magnet field strength slider controls how strong the hovering magnet's field is; push it high enough on a Type-II sample and you will see the flux condition switch from full Meissner expulsion to a partial "mixed state" with vortices, and on Type-I it can quench superconductivity outright. Toggle Field Lines and Penetration Depth to see the underlying physics, and drag/scroll to orbit and zoom the 3D scene.
Why does the magnet actually levitate?
The expelled magnetic flux has to go somewhere: the superconductor's surface supercurrents generate a field that mirrors the magnet's own field, repelling it exactly like an "image magnet" pushed up from below. That repulsive force grows as the magnet gets closer to the surface, and it balances gravity at a stable height — the magnet floats. In Type-II superconductors, flux vortices get pinned to defects in the crystal lattice, which locks the magnet's lateral and rotational position too, not just its height, so it can even levitate upside-down or off to the side.
What is the London penetration depth?
The London penetration depth λ is the characteristic distance over which an external magnetic field decays exponentially as it enters a superconductor's surface, following B(x) = B₀·exp(−x/λ). It is not a hard wall — the field is not zero at the very surface, it just falls off fast, typically over tens to a few hundred nanometres depending on the material. λ grows as temperature approaches Tc, formally diverging as λ(T) = λ₀ / √(1 − (T/Tc)⁴) in the London/BCS picture, meaning the superconductor "leaks" more field just below its transition.
What are Cooper pairs and BCS theory?
In 1957, John Bardeen, Leon Cooper and Robert Schrieffer (BCS theory) showed that below Tc, electrons that would normally repel each other can form weakly bound pairs — Cooper pairs — mediated by lattice vibrations (phonons): one electron slightly distorts the ion lattice, and that distortion attracts a second electron. These pairs behave as bosons and condense into a single coherent quantum state that moves through the lattice without scattering, which is the microscopic origin of both zero resistance and the Meissner effect.
What is the difference between Type-I and Type-II superconductors?
Type-I superconductors (mostly pure elemental metals like mercury, lead and tin) show complete Meissner expulsion up to a single critical field Hc, above which superconductivity collapses abruptly and completely. Type-II superconductors (alloys and ceramics like niobium-titanium and YBCO) expel flux completely only below a lower critical field Hc1; between Hc1 and a much higher Hc2 they enter a "mixed state" where magnetic field penetrates in quantized flux vortices while the rest of the material stays superconducting. This mixed state, and the flux pinning it enables, is what makes practical high-field magnets and stable levitation possible.
What are some real critical temperatures?
Mercury, the first superconductor discovered (Heike Kamerlingh Onnes, 1911), has Tc ≈ 4.2 K, requiring liquid helium cooling. Niobium-titanium, used in MRI and particle-accelerator magnets, has Tc ≈ 9–10 K. The high-Tc ceramic superconductor YBa₂Cu₃O₇ (YBCO), discovered in 1987, has Tc ≈ 93 K — above the 77 K boiling point of liquid nitrogen, which made superconductivity vastly cheaper to demonstrate and use.
Is quantum levitation the same as ordinary magnetic repulsion?
Not quite. Two ordinary magnets pushed apart by like poles are inherently unstable sideways — they slip and flip. A superconductor levitating a magnet via the Meissner effect, especially a Type-II superconductor with pinned flux vortices, is locked into place in all directions: push it sideways and the pinned vortices pull it back, tilt it and it self-corrects. This "flux pinning" stability, not just repulsion, is what lets demonstrations levitate a magnet on a curved track or hold it suspended at an angle.
What is an active research frontier in superconductivity?
The search for room-temperature superconductivity is one of condensed-matter physics' biggest open problems. Hydrogen-rich compounds such as lanthanum hydride (LaH₁₀) have shown superconductivity above 250 K, but only under enormous pressures (over a million atmospheres), which limits practical use. Researchers are also exploring iron-based superconductors, twisted bilayer graphene (which becomes superconducting at a "magic angle"), and topological superconductors that could host exotic quasiparticles useful for fault-tolerant quantum computing.
Cool a puck below its critical temperature to watch it actively expel a magnetic field (the Meissner effect) and levitate a magnet.
2D · HTML5 Canvas 2D · 60 FPS target · runs fully client-side, no install