Vertical Yagi For 160 Meters

Were you imagining a horizontal yagi at 270 feet in the air? No way. It is actually a vertical yagi, meaning three 160m vertical antennas are in a line and spaced a typical distance apart for a yagi. Only the center vertical is driven and the other two verticals are a director and a reflector. The concept for this antenna came from an article in QST, W2FMI 20-Meter Vertical Beam, June, 1972, p 14, by Dr. Jerry Sevick. This is an autumn 2021 project with a goal of working the final 34 countries needed for 160 meter DXCC. Orientation is toward Europe.

The only vertical that didn’t already exist is the new reflector shown in the foreground. It is 50 feet tall. The tower with the beam on top is doing double duty. The beam is being used as a top hat for 160m. The tower becomes the 160m driven element thanks to Omega matching. Faintly visible in front of the tower is the director, which is a 43 ft. vertical with a top hat, resonated to 160m.

What distinguishes the yagi from a phased array is how it is driven. In a phased array all three verticals would be driven at certain phase angles and magnitudes with phasing cables and a phasing network. A phased array has more gain but is very complicated to implement. This yagi has only one driven element, no phasing cables, and is quite forgiving as to spacing. Yagi elements can be spaced for maximum gain or can be spaced for best front-to-back ratio. These yagi elements are spaced for gain using .2 wavelength. The reflector is resonated 5% lower in frequency than the driven element and the director is 5% higher. Center frequency is 1.840 MHz with a 2:1 bandwidth from 1.8 MHz to 1.885. The yagi will be ready for the winter 160m DX season.

A loading coil is housed in this enclosure at the base of the reflector. The coil is a roller inductor adjusted to resonate at 1744KHz, which is 5% lower than the driven element resonance of 1840 KHz.

At the base of the director (the other element) is an identical loading coil, resonated to a frequency 5% higher, or shorter, than the driven element. The director resonates at 1930KHz, shown below. SWR is irrelevant because it is not being connected to a feedline. It is connected directly to the radial ground screen.


In the pskreporter screen-shot below notice that the strongest reports (look at the “dB” numbers) are in a line to the northeast of the Colorado QTH which is very good news running barefoot at 100 watts.

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