The interactive tools below provide a visual bridge between 350-year-old textbook collision mechanics and the non-contact dynamics of Active Magnetic Oscillation (AMO). While analytical equations can obscure the underlying mechanics, observing energy handovers in real time offers intuitive, cognitive clarity for researchers and learners alike.
A visual sandbox to explore macro-level energy exchange, observe bifilar parallel linkages that eliminate tilt shear, and examine progressive 2.5-cycle handovers where standard Simple Harmonic Motion (SHM) fails to apply.
An interactive laboratory to test conservation of momentum and kinetic energy, understand why Newton’s Cradle dampens so quickly in the real world, and see what happens when physical impacts are replaced by magnetic cushions.
Non-contact bifilar dipole carriages demonstrating progressive 2.5-cycle Active Magnetic Oscillation (AMO) energy handover.
While this simulation visualises the 2.5-cycle kinetic energy handover, the underlying physics of Active Magnetic Oscillation (AMO) remains an active frontier of research. Areas currently beyond the scope of this numerical model include:
In physical Active Magnetic Cradle (AMC) systems, each horizontal dipole carriage is suspended using a dual-line bifilar linkage. This geometry ensures the repelling South–South (S–S) magnetic pole faces remain horizontal and parallel throughout the entire stroke, eliminating the vertical magnetic tilt shear that occurs with single-pivot spherical pendulums.
Compressing against a non-contact magnetic repulsion cushion, the system exchanges energy progressively rather than through instantaneous mechanical impact:
Standard linear Simple Harmonic Motion (SHM) equations assume constant linear restoring forces and cannot capture the non-linear potential fields of close-proximity magnetic repulsion.
Simulation Scope & Open Scientific Frontiers
While this browser visualiser models the observable envelope of the 2.5-cycle handover, the complete analytical formulation of Active Magnetic Oscillation (AMO) remains an active research frontier. The mathematical complexities beyond the scope of this web model include:
Higher-Order Multipole Near-Field Repulsion: Standard dipole-dipole approximations (F∝r−4) underpredict the acceleration observed during close-proximity compression. Complete characterisation may require higher-order multipole expansions—including hypothetical quadrupole and octupole near-field contributions, governing the steep repulsive barrier.
Dynamic Potential-to-Kinetic Energy Conversion: Current numerical scripts illustrate kinetic energy (Ek) flow based on velocity vectors. They do not calculate the real-time conversion rates between stored electromagnetic potential energy (Umag) within the compressed magnetic boundary and the resulting kinetic output.
Inseparable Gravitational & Electromagnetic Potentials: In physical AMC motion, gravitational potential energy (Ug=mgh) and non-linear electromagnetic potential energy (Umag) act simultaneously across dynamic spatial coordinates. These coupled forces cannot be separated into independent, linear differential equations.
Non-Linear Decay & Carrier Period Invariance: Unlike classical contact restitution (where energy loss is governed by acoustic and frictional decay constants), magnetic damping involves multi-variable flux interactions. Furthermore, physical prototypes demonstrate an empirical carrier period invariance across variable swing amplitudes that linear damping models fail to predict.
Wavelet Architecture & Modulation Cadence: Real-world magnetometer telemetry exhibits deterministic wavelet packets and frequency-modulation cadences. Replicating these complex wavelets requires advanced spectral modeling tools beyond lightweight front-end browser runtimes.
For the mathematical formulations, time-frequency wavelets, and empirical kinematic datasets governing Active Magnetic Oscillation, explore our open-access research papers on Zenodo or view our Scientific Research Documentation →
Compare classical mechanical sphere impacts with parallel-face Active Magnetic Cradle (AMC) dipole carriages.
While this simulation visualises the 2.5-cycle kinetic energy handover, the underlying physics of Active Magnetic Oscillation (AMO) remains an active frontier of research. Areas currently beyond the scope of this numerical model include:
This interactive telemetry visualiser directly contrasts classical rigid-body collision mechanics with non-contact, field-coupled magnetic oscillations. By transitioning between classical elastic spheres and parallel-face magnetic dipole carriages within the same analytical framework, the tool demonstrates how energy conservation laws manifest differently across physical contact impacts versus continuous magnetic flux cushions.
1. Classical Rigid-Body Regimes (Ideal SHM vs. Contact Decay)
2. The Conservation Paradox Demonstration
3. Real-Time Telemetry Mapping (Inside-the-Mass Readouts)
4. Active Magnetic Cradle (AMC) Coupled Dipole Mode
5. Motion Controls & Variable Cadence Tuning

