Near field — where it appears
Named by 4 essays across 4 fields — each of them below, with the objects they name alongside it.
The spiral that says how much light arrives
Huygens' construction says where a wave has got to and refuses to say how bright it is, because an envelope is a locus and a locus has no amplitude. Adding the wavelets with their phases instead of taking their envelope turns the whole subject into one curve, and every near-field pattern there is becomes a chord of it.
The grating that photographs itself
Put a grating in a beam of light and hold a screen behind it. At one particular distance the screen shows the grating again — sharp, at full contrast, right way up, with no lens anywhere in the apparatus. Half way there it shows the grating shifted sideways by half a period. A quarter of the way there, a half-open grating shows nothing at all.
The distance where a field changes its mind
An oscillating source has three fields around it, falling as the inverse cube, the inverse square and the inverse first power of distance. They are all equal at one radius, and that radius is the wavelength over 2π — a number containing nothing about the source at all. Inside it a source mostly stores energy; outside it, mostly loses it, and the two behaviours are different technologies rather than different strengths.
The bill that arrives when the pushing stops
A charge accelerating steadily radiates at the full Larmor rate while the radiation reaction force on it is exactly zero, so for as long as the push holds, nothing about the charge's motion pays a single watt. The energy is lent by the field that travels with the charge, the loan is called the Schott term, and it is repaid the moment the acceleration changes.
Named alongside it
The objects these essays reach for when they reach for this one.
DiffractionInterferencePhaseWavefrontAmplitudeCoherenceDipole radiationElectromagnetic waveEnergy conservationFourier transformFresnel diffractionFresnel zones