SUMMARY
The radiation intensity of a dish antenna is primarily defined by the function K(theta), which depends on the angle theta from the Z axis and the distance R from the antenna, while remaining independent of the rotational angle Theta around the Z axis. This behavior is attributed to the assumption of radial symmetry in many analysis procedures, although practical variations can occur due to antenna geometry and polarization. For large, round parabolic dishes, these variations typically have minimal impact, mainly affecting sidelobes rather than the main beam. Understanding these principles is essential for accurately modeling antenna performance.
PREREQUISITES
- Understanding of spherical coordinates in three-dimensional space
- Familiarity with parabolic mirror principles and their applications
- Basic knowledge of antenna theory and radiation patterns
- Calculus and trigonometry fundamentals
NEXT STEPS
- Study the mathematical derivation of K(theta) for dish antennas
- Explore the impact of antenna feed geometry on radiation patterns
- Learn about the differences between E-plane and H-plane patterns in linearly polarized antennas
- Investigate the effects of asymmetry in offset parabolic antennas on radiation intensity
USEFUL FOR
Electrical engineers, antenna designers, and anyone involved in RF communications or satellite technology will benefit from this discussion.