Virtual Laboratory for EEEN 566
Study the concave reflector geometry with focal point feed configuration, including f/D ratio effects on illumination.
Visualize and interpret E-plane and H-plane radiation patterns from concave reflector configuration.
Apply the gain formula G = η(πD/λ)² for prime-focus parabolic reflectors.
Calculate half-power beamwidth (HPBW) and analyze focal point illumination effects.
A parabolic antenna consists of a concave parabolic reflector (dish) that curves inward toward the focal point, with a feed antenna located at the focus. The parabolic shape follows the equation y² = 4fx, where f is the focal length measured from the vertex to the focal point.
The f/D ratio (focal length to diameter ratio) is critical for determining the feed horn illumination pattern. Typical values range from 0.3 to 0.5 for prime-focus reflectors, where the feed is positioned at the focal point facing the concave surface.
The gain of a parabolic antenna is given by:
Where η is the aperture efficiency (typically 0.5-0.65), D is the diameter, and λ is the wavelength. In decibels: G(dBi) = 10log₁₀[η(πD/λ)²]
The half-power beamwidth (HPBW) is approximated by:
The concave reflector focuses incoming plane waves to the focal point (receiving) and transforms spherical waves from the feed into plane waves (transmitting). Edge illumination of -10 to -11 dB relative to the center provides optimal trade-off between gain and sidelobe levels.
The concave parabolic reflector focuses parallel incoming rays to the focal point where the feed horn is located.
Simulated 3D directive gain pattern
Max Directivity: 39.9 dBi
Submit a PDF report including screenshots of the concave geometry visualization for at least 3 different f/D ratios. Show ray tracing from the feed to the reflector surface.