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CHAPTER 11<br />

Vertical Arrays<br />

Despite its longevity, the vertical antenna is either praised or cursed by its users,<br />

depending upon their experiences with it. At HF in particular, “DXability” is<br />

often the criterion for judging the antenna’s performance. As amateurs and<br />

others have come to appreciate the importance of a good RF ground system to the vertical’s<br />

performance, in recent years the vertical has come into its own on the 1.8- and<br />

3.5-MHz bands because it provides superior low-angle radiation compared to the low<br />

dipoles that are the only alternative for most users.<br />

But a vertical antenna is omnidirectional in its azimuthal (compass rose) coverage;<br />

that is, it transmits and it “hears” equally well in all directions. Thus, a single vertical<br />

exhibits two weaknesses:<br />

• It puts far more RF energy out in directions that are of no use (at that particular<br />

moment, at least) than it does in the desired direction.<br />

• It does not have any way of eliminating noise coming from all 360 degrees<br />

around the compass when trying to receive a weak signal from a specific<br />

heading.<br />

With respect to the first point, there are only three things the user with a single vertical<br />

can do to improve his/her signal at a specific faraway receiving location:<br />

• Increase the transmitter power to the antenna.<br />

• Improve the antenna efficiency by reducing resistive losses, especially by<br />

making sure an adequate system of radials is installed at the base of the antenna.<br />

• Increase the electrical length of the vertical radiator (up to a maximum of<br />

5 l/8). This causes the low-angle field strength for a given transmitter power<br />

to increase because high-angle radiation is being reduced as the vertical is<br />

lengthened.<br />

With respect to the second point, we note:<br />

• Atmospheric band noise arrives from compass headings where the band is<br />

“open”. That is, if it’s shortly after sunset at the site of the vertical antenna,<br />

atmospheric noise on the MF and lower HF bands is likely coming only from<br />

points east of the antenna, where darkness and ionospheric propagation are<br />

prevalent. To the west, daylight absorption in the lower layers of the ionosphere<br />

substantially reduces the noise levels at the vertical. This is true of the noise<br />

(“QRN” in the long-established radio shorthand known as Q-signals) from<br />

distant thunderstorms.<br />

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