Dipole Antenna Radiation Patterns Article
used with permission and courtesy of John,
WB4YJT - Ventenna.com www.ventenna.com
"A dipole antenna in free space exhibits a feed impedance
of 72 Ohms, and has a doughnutshaped
radiation
pattern. But, as the dipole is brought close to the earth, the radiation
pattern changes, and the feed point impedance also
changes. An awareness of these changes can help ease
the task of setting up a dipole for communications. And, careful selection
of the dipole's position above the ground can make its
impedance exactly match the impedance of the feed line used.
For me, one of the
fun aspects of antennas is that they are still "magical". There is a lot
of art involved in their design, setup and operation,
compared to much of digital electronics, where it is almost literally "plug-and-play". But, at the same time, when you
are trying to make an HF contact, the "magic" can
quickly turn to frustration when things don't work as expected. Perhaps
this discussion will help reduce some of the
frustrations, let you make that rare DX contact, and bring back some of the "magic". I had fun creating this report,
and I hope you have fun using it!" - John,
WB4YJT
Much confusion exists about the
radiation patterns of antennas. In particular, the horizontal dipole is misunderstood by most who use it. It is
generally assumed that a horizontal dipole has a radiation pattern which aims most of its signal toward the
horizon, perpendicular to the line of the antenna. As we will see here, that is only true in one
particular circumstance, and, even then, not quite an accurate picture. Following is a series of dipole radiation pattern plots, produced
by a popular antenna modeling program.
The first plot below shows a dipole at an elevation of two wavelengths
above a standard earth ground
model.
Note the multiple lobes at
varying elevation angles above the horizontal. These lobes represent a
division of the radiated energy, so that
much energy is sent off at angles which may not be helpful to the particular communication in progress.
In addition, the nulls represent angles at which no energy is transmitted. Depending on the height of the
ionosphere, and the location of the
distant target station, the null may exist at the precise angle necessary
to effect the desired contact.
Page 2 of 2
The next
plot shows the dipole at 1.75 times the wavelength above the earth.
There are fewer lobes and
fewer nulls, but they are still present. In addition, two of the upper
lobes have moved up and merged to
produce a single, wide lobe aimed straight up.
Next is the dipole at 1.5
wavelengths elevation.
Page 3 of 3 Again, fewer nulls and lobes, but still not
necessarily concentrating the energy in the desired direction. Next is the dipole at 1.25 wavelengths
high.
The large vertical lobe is
back, and the nulls and lobes are fewer, but still not the expected
pattern. Next is the dipole at 1
wavelength high. By now, we should be
noticing a sequence to the patterns. As we lower the antenna, the lobes
move higher, combine and
disappear.
Page 4 of 4 Next is the dipole at .75 wavelength.
And, the dipole at .5
wavelength over the ground below.
Page 5 of 5 Finally we see a pattern that looks somewhat like
what we expected. But, notice that, rather than the energy being directed at the horizon, the peak of the pattern
is elevated at about a 30 degree angle
(actually 28 degrees). However, the lobe is broad enough so that there is
considerable signal strength from about
ten degrees to about 55 degrees elevation - the 6 dB down points on
the lobe. Remember that 6 dB represents
one "S" unit on the signal level meter of most HF receivers. Thus, for a quite broad range of elevation
angles, and for a correspondingly broad expanse of geographical area covered by the signal reflected off
the ionosphere, there is substantial
signal strength.
As we continue to lower the
dipole, we continue to see the now familiar raising and combining
of the lobes, until, at .25 wavelength
shown below,
the lobes have combined to produce a single broad peak,
aimed straight up. Clearly, this is not going to make for great DX
communications, with most of the energy concentrated above the 30 degree elevation angle. But, notice that
there is still considerable energy
directed even as low as 15 degrees, the 6 db down point.
This is the radiation pattern
which is normally used for NVIS operations. NVIS stands for Near
Vertical Incidence Skywave. Below a
certain critical frequency (which depends on the density of the ionization in the ionosphere), a signal
directed straight upward will be reflected back down into an area near the transmitter. This can allow
communications within a 100-200 mile radius of the transmitter, the area normally skipped over by signals
transmitted from the dipole at lower
radiation angles (generated by higher positions above ground). NVIS
antennas are normally elevated at about
.1 to .25 wavelength above the ground.
The next plot shows the dipole at
.1 wavelength.
Page 6 of 6 At .1 wavelength, we see the single lobe even more
tightly pointed up, with the 6 dB points now at about 25 degrees. This appears to be a very good NVIS antenna.
But, as we will shortly see, there is
another factor involved, the antenna's impedance.
Before we leave the NVIS
discussion, lets go back and look at the .75 wavelength elevation
pattern shown below:
Page 7 of 7 Notice that this pattern has both the low-angle lobes
and a broad vertical lobe. The vertical lobe is about 2 dB below the low-angle lobes, an almost insignificant
difference in signal strength. It
may be that a
dipole at .75 wavelength height over ground is the best of all possible
setups, providing both
DX communications and NVIS communications at the same
time.
Dipole
Impedance
One other factor should
be discussed, the antenna feed point impedance. A dipole's impedance varies according to its
height above the ground. The following chart shows the
variations in impedance as the dipole is
lowered from .5 wavelength above ground to .1 wavelength.
For each
calculation, the
antenna's length was adjusted for best SWR, using 50 Ohms as the reference
impedance. The calculated dipole was
modeled using #12 wire for the elements.
The Best Dipole
Setup
Note that, somewhere between 20% and 15%
wavelength height, in the chart above, the dipole's impedance crosses
50
Ohms. If we specifically calculate for
the 50 Ohm point, we discover that, at a height of 16.7
% wavelength, with a length
of 47.4 % wavelength, we get an antenna setup which exactly matches 50 Ohms. The following chart shows the 16.7 % / 47.4 %
dimensions for various Ham frequencies in the HF bands.
Page 8 of 8 The radiation pattern for a dipole set up according
to the 16.7% / 47.7% chart looks like this:
This is not the ideal
DX antenna, but it does provide good signal strength at reasonably low
angles (6 dB down at 20 degrees
elevation angle). It is essentially the same pattern as the .25
wavelength height dipole, but with the
benefit of being matched to 50 Ohms. In addition, it provides a very broad NVIS signal lobe. This
looks like a good compromise between both modes, and is fairly easy to set up on
frequencies above 10 MHz. At lower frequencies, the height above ground becomes a problem to achieve with
a reasonable support structure.
The HFp Dipole
For the HFp Ventenna
Dipole, the element length is set according to the
element chart in the Dipole instructions. The 16.7% wavelength antenna height for each band is
listed here:
80 Meters (3.6 MHz) 45.7 Ft. high
75 Meters (3.8 MHz) 43.3 Ft.
high 40 Meters (7.2 MHz) 22.8
Ft. high 30 Meters (10.125
MHz) 16.2 Ft. high 20 Meters
CW (14.1 MHz) 11.7 Ft. high 20
Meters SSB (14.3 MHz) 11.4 Ft. high 17 Meters (18.125 MHz) 9.1 Ft. high 15 Meters (21.25 MHz) 7.7 Ft. high
12 Meters (24.5 MHz) 6.7 Ft.
high 10 Meters low (28.5 MHz)
5.8 Ft. high 10 Meters high (29.5
MHz) 5.6 Ft. high
73, John, WB4YJT
(This article courtesy of Ventenna and John, WB4YJT and
slightly modified for presentation here.)