Linked from

The 90 pages that link to Maxwell's equations, each with the reason it gives.

• Ohm's lawNarrower topic: They provide a broader field-level framework than this component-level law.

• Speed of lightNarrower topic: Their wave solutions revealed a characteristic electromagnetic speed matching measured light speed.

• MagnetohydrodynamicsNarrower topic: They provide the electromagnetic laws that are simplified in fluid-scale models.

• Faraday's law of inductionNarrower topic: Faraday's law is one of the equations in this broader framework.

• Kirchhoff's circuit lawsNarrower topic: They provide the broader field theory behind circuit laws and their limits.

• Magnetic fluxNarrower topic: Magnetic flux appears in the integral forms of these field laws.

• Hendrik LorentzNarrower topic: Lorentz developed his electromagnetic theory by extending Maxwell’s account of fields and light.

• Mie scatteringNarrower topic: Lorenz–Mie theory solves these equations for a sphere illuminated by a wave.

• Heinrich HertzNarrower topic: Their predicted wave solutions supplied the theoretical target for Hertz’s experiments.

• Geometrical opticsNarrower topic: They provide a broader framework from which ray optics can emerge as an approximation.

• Vacuum permittivityNarrower topic: ε₀ appears in the equations governing electric fields and electromagnetic waves.

• Skin effectNarrower topic: Their field relations yield the frequency-dependent current distribution in conductors.

• Biot–Savart lawNarrower topic: The law is consistent with their magnetostatic limit, but is not the general time-dependent field solution.

• Fresnel equationsNarrower topic: They supply the field laws whose interface boundary conditions yield Fresnel relations.

• Ampère's circuital lawNarrower topic: The corrected circuital law is one of the four equations.

• Gauss's lawNarrower topic: Gauss's law is the electric-field divergence equation within this set.

• Nonlinear opticsNarrower topic: They connect material polarization to the propagation of optical fields.

• ElectricityNarrower topic: They unify electricity with magnetism and describe classical electromagnetic phenomena.

• Joseph HenryNarrower topic: They later unified the electromagnetic phenomena that Henry investigated experimentally.

• Kirchhoff's current lawNarrower topic: The field equations provide the broader framework behind charge continuity and circuit laws.

• Lenz's lawNarrower topic: Faraday's induction equation expresses Lenz's law within the broader field theory.

• Poynting vectorNarrower topic: They yield the conservation equation that defines electromagnetic energy flux.

• Displacement currentNarrower topic: Displacement current is essential to the equations’ consistent description of changing fields.

• Gauss's law for magnetismNarrower topic: This law is one of the four equations governing classical electromagnetism.

• Magnetic circuitNarrower topic: They provide the broader field theory from which circuit approximations are drawn.

• Magnetic vector potentialNarrower topic: The potential offers a way to formulate these field equations.

• MagnetotelluricsNarrower topic: They provide the physical foundation for interpreting electromagnetic induction in Earth.

• NaturalnessNarrower topic: Their successful unification helped establish symmetry and simplicity as guides to physical theory.

• Vacuum permeabilityNarrower topic: μ₀ appears in these equations alongside the vacuum permittivity.

• Electromagnetic wave equationNarrower topic: Taking curls of the field equations yields wave equations when sources vanish.

• Magnetic energyNarrower topic: They place magnetic energy within the full dynamics of electromagnetic fields.

• Impedance of free spaceNarrower topic: In vacuum, these equations relate the electric and magnetic amplitudes of a traveling wave.

• Astrophysical electromagnetic fieldsNarrower topic: They provide the general laws governing fields, beyond the conducting-fluid approximation.

• Displacement current densityNarrower topic: They establish the broader field equations in which displacement current density appears.

• Electromagnetic field calculationsNarrower topic: They provide the fundamental laws that field calculations solve.

• First-principles calculations in plasma physicsNarrower topic: They provide the field laws coupled to plasma particle motion.

• Lorenz gauge conditionNarrower topic: Applying the condition turns the potential equations into wave equations.

• Methods in electromagnetismNarrower topic: They provide the governing relations that electromagnetic solution methods must satisfy.