The near field and far field are regions of the electromagnetic (EM) field around an object, such as a transmitting antenna, or the result of radiation scattering off an object. Non-radiative near-field behaviors dominate close to the antenna or scatterer, while electromagnetic radiation far-field behaviors predominate at greater distances. Far-field E (electric) and B (magnetic) radiation field strengths decrease as the distance from the source increases, resulting in an inverse-square law for the power intensity of electromagnetic radiation in the transmitted signal. By contrast, the near-field's E and B strengths decrease more rapidly with distance: The radiative field decreases by the inverse-distance squared, the reactive field by an inverse-cube law, resulting in a diminished power in the parts of the electric field by an inverse fourth-power and sixth-power, respectively. The rapid drop in power contained in the near-field ensures that effects due to the near-field essentially vanish a few wavelengths away from the radiating part of the antenna, and conversely ensure that at distances a small fraction of a wavelength from the antenna, the near-field effects overwhelm the radiating far-field.
Introduction
The distinction between near-field and radiated field can be illustrated by the Panofsky–Phillips equations, which give the general expression of the electric and magnetic fields produced by an arbitrary distribution of charges and currents. The terms of the Panofsky–Phillips equations can be separated into two categories: The "near field" terms have a 1 / r 2 {\displaystyle 1/r^{2}} dependence, and are significant only in the immediate vicinity of the sources. The "far field" terms have a 1 / r {\displaystyle 1/r} dependence. Due to their slower decrease with distance, they dominate as one moves away from the sources.
… excerpt ends here. Continue reading the full article.






