Maxwell Equations
Maxwell’s equations describe all (classical) electromagnetic phenomena:
\[\nabla \times E =−\dfrac{\partial B}{\partial t}\] \[\nabla \times H = J + \dfrac{\partial D}{\partial t}\] \[\nabla \cdot D = \rho\] \[\nabla \cdot B = 0\]
The first is Faraday’s law of induction, the second is Ampere’s law
as amended by Maxwell to include the displacement current \(\dfrac{\partial D}{\partial t}\), the third
and fourth are Gauss’ laws for the electric and magnetic fields.
The displacement current term \(\dfrac{\partial D}{\partial t}\) in
Ampere’s law is essential in predicting the existence of propagating
electromagnetic waves. Its role in establishing charge
conservation.
Maxwell equations are in SI units. The quantities E and H are the
electric and magnetic field intensities and are measured in units of
[volt/m] and [ampere/m], respectively.
The quantities D and B are the electric and magnetic flux densities and
are in units of [coulomb/m\(^2\)] and
[Weber/m\(^2\)], or [tesla].D is also
called the electric displacement, and B, the magnetic induction. The
quantities ρ and J are the volume charge density and electric current
density (Charge flux) of any external charges (that is, not including
any induced polarization charges and currents.) They are measured in
units of [coulomb/m\(^3\)] and
[ampere/m\(^2\)].
The right-hand side of the fourth equation is zero because there are no
magnetic mono-pole charges. The charge and current densities \(\rho\),J may be thought of as the sources
of the electro-magnetic fields. For wave propagation problems, these
densities are localized in space; for example, they are restricted to
flow on an antenna. The generated electric and magnetic fields are
radiated away from these sources and can propagate to large distances to
the receiving antennas.
Maxwell’s equations take the simpler form: \[\nabla \times E =− \dfrac{\partial B}{\partial t}\] \[\nabla \times H = \dfrac{\partial D}{\partial t}\] \[\nabla \cdot D = \rho\] \[\nabla \cdot B = 0\]
For example, a time-varying current J on a linear antenna generates a circulating and time-varying magnetic field H, which through Faraday’s law generates a circulating electric field E, which through Ampere’s law generates a magnetic field, and so on. The cross-linked electric and magnetic fields propagate away from the current source.