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EM.Tempo

570 bytes added, 17:55, 1 August 2015
/* Computing Far-Field Characteristics in FDTD */
<math> \mathbf{H^{ff}(r)} = \frac{1}{\eta_0} \mathbf{ \hat{k} \times E^{ff}(r)} </math>
Far fields are typically computed in the spherical coordinate system as functions of the elevation and azimuth observation angles &theta; and &phi;. Only far-zone electric fields are normally considered. When your physical structure is excited using a lumped source, a waveguide source, a distributed source, a short dipole source, or an array of such sources, the far fields represent the radiation pattern of your source(s) in the far zone. When your physical structure is illuminated by a plane wave source or a Gaussian beam source, the far fields represent the scattered fields. In the case of a plane source, you can compute the radar cross section (RCS) of your target structure. In the FDTD method, the far fields are calculated using a near-field-to-far-field transformation of the field quantities on a given closed surface. EM.Tempo uses rectangular boxes to define these closed surfaces. You can use EM.Tempo's default radiation box or define your own custom box. Normally, the radiation box must enclose the entire FDTD structure. In this case, the calculated radiation pattern corresponds to the entire radiating structure. Alternatively, the radiation box may contain only parts of a structure, which results in partial radiation patterns.
[[Image:Info_icon.png|40px]] Click here to learn more about '''[[Maxwell%27s_Equations#Definition_of_the_Far_Radiation_Zone | Computing the Far Fields & Radiation Characteristics]]'''.
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