Bow-Tie Antenna
Understanding Bow-Tie Antennas
The flare angle α (half-angle of each triangle) determines the input impedance: wider flare = lower impedance, broader bandwidth. At α=90° (flat plate), the impedance approaches that of a biconical antenna (~188 Ω for infinite bow-tie). Practical finite bow-ties with α=60° have ~150 Ω impedance. A balun transforms this to 50 Ω.
Adding a ground plane or reflector behind the bow-tie creates a unidirectional pattern with 5-8 dBi gain, useful for GPR and imaging arrays. Resistive loading (Wu-King profile) at the triangle edges absorbs reflections, extending bandwidth beyond 10:1 at the cost of 3-5 dB efficiency loss.
L = triangle length (tip to base)
Upper frequency: limited by feed gap
Input impedance (infinite):
Z ≈ 120·ln(cot(α/4)) Ω
α=90°: Z ≈ 188 Ω
α=60°: Z ≈ 150 Ω
Wideband Antenna Comparison
| Antenna | BW Ratio | Gain (dBi) | Form Factor |
|---|---|---|---|
| Bow-Tie | 3:1-10:1 | 2-5 | Planar (PCB) |
| Vivaldi | 10:1+ | 5-12 | Planar endfire |
| Log-periodic | 10:1+ | 6-10 | 3D structure |
| Spiral | 10:1+ | 2-5 | Planar (circular) |
Frequently Asked Questions
Why wideband?
Triangular flare gives gradual impedance transition. Multiple current modes. Flare angle controls BW: wider = broader. 2D biconical equivalent.
Specs?
BW: 3:1-10:1. Gain: 2-5 dBi (8-12 with reflector). Z: 100-300 Ω. Linear polarized. PCB-fabricable.
Applications?
GPR (range resolution), UWB comms, EMC probes, microwave imaging arrays, SKA radio astronomy aperture arrays.