Computes the far-field components radiated by a pyramidal horn antenna.
This function models the electromagnetic far-field radiated by a rectangular pyramidal horn using physical optics and Fresnel integrals. It calculates the spherical electric and magnetic field components based on geometry and frequency.
- Parameters
-
eta | Intrinsic impedance of the medium [Ohm] |
a | Width of waveguide aperture in x [m] |
b | Height of waveguide aperture in y [m] |
a1 | Aperture width at horn opening [m] |
b1 | Aperture height at horn opening [m] |
rho1 | Distance from waveguide aperture to horn opening in y-z plane [m] |
rho2 | Distance from waveguide aperture to horn opening in x-z plane [m] |
freq | Frequency of operation [Hz] |
E0 | Field amplitude scaling factor [V/m] |
r | Observation distance(s) [m] |
theta | Elevation angle(s) [rad] |
phi | Azimuthal angle(s) [rad] |
- Return values
-
Er | Radial electric field (zero) |
Etheta | Theta-polarized electric field [V/m] |
Ephi | Phi-polarized electric field [V/m] |
Hr | Radial magnetic field (zero) |
Htheta | Theta-polarized magnetic field [A/m] |
Hphi | Phi-polarized magnetic field [A/m] |