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Poynting vectorIn physics, the Poynting vector can be thought of as representing the energy flux (W/m^{2}) of an electromagnetic field. It is named after its inventor John Henry Poynting. Oliver Heaviside independently codiscovered the Poynting vector. Usually, it is defined as where E is the electric field, H the auxiliary magnetic field, B the magnetic field, μ_{0} the permeability of vacuum, and μ_{r} the dimensionless relative permeability of the surrounding medium. (All bold letters represent vectors.) For example, the Poynting vector within the dielectric insulator of a coaxial cable is nearly parallel to the wire axis (assuming no fields outside the cable)  so electric energy is flowing through the dielectric between the conductors. If the core conductor was replaced by a wire having significant resistance, then the Poynting vector would become tilted toward that wire, indicating that energy flows from the e/m field into the wire, producing resistive Joule heating in the wire. Additional recommended knowledge
InterpretationThe Poynting vector appears in the energyconservation law^{[1]}, or Poynting's theorem, where J is the current density and u is the electromagnetic energy density, where ε_{0} is the permittivity of free space and ε_{r} the relative dielectric constant of the medium. The first term in the righthand side represents the net electromagnetic energy flow into a small volume, while the second term represents negative of the work done by electrical currents that are not necessarily converted into electromagnetic energy. The Poynting vector in electromagnetic wavesIn a propagating sinusoidal electromagnetic plane wave of a fixed frequency, the Poynting vector oscillates, always pointing in the direction of propagation. The timeaveraged magnitude of the Poynting vector is where E_{0} is the maximum amplitude of the electric field and c is the speed of light. This timeaveraged value is also called the irradiance or intensity I. DerivationIn an electromagnetic plane wave, and are always perpendicular to each other and the direction of propagation. Moreover, their amplitudes are related according to and their time and position dependences are where ω is the frequency of the wave and is wave vector. The timedependent and position magnitude of the Poynting vector is then In the last step, we used the equality . Since the time or spaceaverage of is , it follows that Radiation pressureS divided by the square of the speed of light in a vacuum is the density of the linear momentum of the electromagnetic field. The timeaveraged intensity divided by the speed of light in a vacuum is the radiation pressure exerted by an electromagnetic wave on the surface of a target: References
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This article is licensed under the GNU Free Documentation License. It uses material from the Wikipedia article "Poynting_vector". A list of authors is available in Wikipedia. 