Sunday, July 31, 2011

A, B, C's of Dx Fundamentals of the Art of DXing V

 HF Antennas

Now that you've got a feel for the basic principles of what RF waves are, and how they propagate, let's review a few things about antennas - the part of the station that actually puts the signal into - and pulls it out of - the air! This short discussion of antenna science is to highlight some of the factors that are important to DXers and very briefly review a few of the more commonly used antennas types. Since an understanding of HF propagation and antenna principles are THE most important "tools" that a DXer can have, it follows that one should develop a sense for "continuing education" on these subjects. Not only will it be helpful in improving your ability to work DX, it may also save you some money. How? Well, before mortgaging the house to buy a new DX4000ProIX transceiver so that you can "work more DX", be advised that the most effective investment that you can make is in the antenna that you use, and often this can be done at a fraction of the cost of even a modestly priced transceiver.
So, after P.E.P.S.I., the next three most important things for DXing are (i) the antenna, (ii) the antenna, and (iii) the antenna. Its easy to see why this is so - on receive, if the antenna cannot produce enough signal strength (vs. noise), then the most sophisticated and expensive receiver can do little more than light up and look pretty; while on transmit, a KW amplifier will do little good if all of the radiated power is going straight up to warm the clouds or straight down to warm the worms. Once you reach the point at which you're ready to improve your station, then it's time to learn more - and as much as you can - about the fascinating field of antenna theory, design, and practice. As in almost all of the other subjects having to do with amateur radio, antennas can be as complex as one has time to invest in learning about them, or as simple as taking someone else's advice and hoping that they're right. What follows is a highly over-simplified attempt to distill and summarize some of the common questions and points of interest to DXers. It is meant only as a brief introduction which may help to spur further interest in learning more. There is an abundance of information available on antenna theory, design, and performance in the printed literature as well as on the Web (Note: Probably one of the most extensive online antenna resources for hams can be found at www.cebik.com). Look for it and make use of it! Provided in the References are other sources of expertise, detail, and ideas.

First, what is an Antenna?

Most would say that it's "... that thing in the air, used to send and receive radio signals". That's partly true, in fact that's why it was (and sometimes still is) called an "aerial" from the ancient Greek word for "air" (aerios). But for radio communications, there is more to it than that. The "antenna" is actually one component of the antenna system, of which there are four parts: the commonly envisioned device usually called the "antenna" that is supposed to do the actual radiating and receiving; the antenna transmission line (or "feedline") that is supposed to carry the signal from the transmitter to the "feedpoint" of the radiator; the matching device or "antenna tuning unit" (ATU) that optimizes signal energy transfer from the transceiver output to the transmission line; and finally, the surrounding antenna environment (height-above-ground, nearby structures, ground conductivity, etc), that one hopes will not adversely affect performance. The four components of an antenna system are diagrammed schematically in the figure below. Most of the time, discussion focuses upon the radiating portion ("aerial") and that is usually
what we think of when we speak of an "antenna". However, it would be a mistake to ignore the other components because a poor or improperly matched feedline, or a failure to address detrimental environmental conditions can easily reduce the performance of the best of the radiators. Below, we'll cover some of the key points about the four components, including the types of antenna radiators that are commonly used for DX. Readers are strongly urged to do additional research on all components of the system when considering an antenna.

Measuring Antenna Performance: The Reference Antenna and Free Space models

When comparing different antennas, it would be useful to be able to describe each of them in terms of how well each performs. But how do you describe the capability of one type of antenna as compared to another? Well, we can do so in a manner similar to that we use to compare the size and weight of different objects - we describe them in terms of a defined standard unit of length (meter, cm, foot, inch) and a standard unit of mass (kilogram, gram, pound, ounce). To do this for antennas, we choose one type, along with a defined environment, as a reference standard for performance measurement. The ideal reference antenna would be one that radiates energy equally in all 3 dimensions, called an isotropic radiator. To visualize an approximation of the concept of an isotropic radiator, think of it as similar to a very small light bulb that is emitting light in all directions of the surrounding space. While it is possible to approximate an isotropic radiator, in fact it does not (cannot) exist, but is just a convenient theoretical tool that is used for describing the properties of real antennas.
An alternative reference antenna that is sometimes used is the half-wavelength dipole antenna, illustrated in the figures below.
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In its original configuration (left figure), it was constructed with a feedline consisting of two parallel wires held apart (e.g., from 2-12 inches) by insulated spacers; today, coaxial cable (right figure) is more commonly used for dipole antenna feedlines. What defines a dipole antenna is the balanced symmetry of the radiating elements about the center: both sides of the feed-point are identical. As shown in the left illustration, dipole antennas were originally fed with "twin-lead" and, because of the double-sided symmetry, were often called "doublets", a term which one still occasionally hears. A dipole fed with twin-lead and matched to the transmitter with an "antenna tuning unit" can serve as an inexpensive multi-band antenna (e.g., see "All-band doublet " at www.cebik.com/edu/edu6.html). While the dipole can be a useful reference that is easy to understand, it isn't as convenient as the theoretical isotropic radiator because, as we shall soon see, the dipole has directional (non-isotropic) properties.

Of course, we must also define the standard reference environment. In reality, it is impossible to have an environment at one geographical location that is truly identical to others elsewhere. Fortunately, science and computers come to the rescue! There are theoretical mathematical antenna modeling programs that can provide very good estimates of the way different antennas radiate, and with readily available computers, anyone can experiment with antenna designs and evaluations. Mathematical models, based upon the physics of EM wave production, define two regions of space for antenna analyses: the near-field region within a large number of wavelengths surrounding the antenna, and the far-field region beyond. The near-field is where the radiation pattern is formed as a result of interactions among the antenna variables, including the radiating elements and the environment (notably the ground surface). The far-field is the region sufficiently distant (many wavelengths) from the antenna so that in the portion of space in which we detect the radiation, it appears to be a "flat" or "plane" wave without any noticeable sphericity.
To avoid problems with environmental variables, the most effective way to compare different antenna designs is to imagine them to be placed in outer-space away from everything, and let the software simulate their radiation patterns for analysis. This is referred to as the "free-space environment". With these data, one can then compare apples-to-apples, the premise being that if antenna "A" exhibits characteristics in free-space that are more favorable for the intended application than does antenna "B", although it may not perform as ideally in the real-world, it may still be expected to exhibit a similar performance edge when both A and B would encounter the same environmental variables. How well do these models work? Field tests on Earth-bound antennas have verified the reliability of the theoretical model comparisons in providing very good estimates of the results to be expected in actual applications. Further, today's antenna modeling software can now also do a pretty good job of including estimates of some of the real-world environmental variables (nearby structures, height-above-ground, ground conditions, etc.) in the evaluation of antenna characteristics in situ (i.e., in your backyard!).
The figures below, produced by the EZNEC modeling software by W7EL (www.eznec.com/), show the predicted radiation pattern of an 80m dipole in free-space in the far-field many wavelengths from the antenna. The left figure shows the free-space 3-dimensional pattern and the right figure shows the azimuthal radiation pattern, a horizontal cross-section of the 3-D pattern viewed from above the antenna.
In the 3-D view, we see that the antenna produces a doughnut-shaped toroidal pattern, with no radiation in the direction of the ends. The adjacent azimuthal slice at 0o in the horizontal plane shows that the dipole radiation favors the directions broad-side to the antenna in a "figure-8" pattern. Using antenna modeling software, radiation patterns like these can be generated for other types of antennas, allowing you to compare them without concern for the environmental differences that likely exist between your backyard and that of someone else's next door or around the globe. Of course, as we shall see below, once you decide which is best for you, the actual pattern of the HF antenna that you do install in your back yard will be quite different than it appears in free space! However, as mentioned, you can also incorporate an estimated description of your own Earth-bound environment in order to get a pretty good idea of what your expected on-site results will be. A brief example of how to interpret the pattern graphs can be found in the "Miscellaneous Notes" Appendix under "Antenna Notes".

Impedance, Standing Wave Ratio, and Balance

Remember the 3rd component of the antenna system, the matching device or "antenna tuning unit (atu)"? What exactly does that do for us? Let's review some basic electronics theory. When dealing with alternating currents (such as RF), everything (including air and outer-space) that the currents flow through will have some effect upon the flow. The effects are a result of the fact that, in addition to resistance (R), every material has the intrinsic ability to exhibit capacitive (C) and/or inductive (L) properties to some extent. We are familiar with the effect of resistance (current reduction and heat-loss due to electron collisions with stationary atoms & molecules), but what about that of L and C? Simply stated, both L and C can each reduce AC flow due to electromagnetic force interactions, but they do so in off-setting ways, because each may have a different effect upon the phase of the alternating current and so, for certain combinations of L,C values, their combined effects may be reduced, or even canceled out. This complex effect upon AC flow by the intrinsic L and C properties of circuits is called Reactance (X); however, unlike resistance, reactance does not directly result in energy loss due to heat. The total effect of resistance and reactance is called the impedance (Z), expressed as Z = R + jX, where the "j" signifies that the quantity "X" has not only a magnitude, but also a phase, reminding us that the impedance is a function of the frequency of the current.
All circuits have some impedance, but when an AC flows from one circuit to another, if there is an impedance difference between the circuits, part of the current will "flow forward" into the second circuit while an amount in proportion to the impedance difference will be "reflected back" into the first circuit. The circuits of interest to us at this point are the transmitter output circuit, the transmission line, and the antenna radiator. Impedance mismatches anywhere between the transmitter and the radiator may result in part of the RF power from the transmitter being reflected back by the mismatch. Mismatches may occur between the transmitter and the transmission line and/or between the transmission line and the radiator. The "forward" and "reflected" waves on the transmission line can constructively/destructively interfere with each other by periodically adding and subtracting each cycle, establishing a periodic wave pattern on the line that, if it could be envisioned, would appear to be an undulating wave that seems to "stand in place" in terms of the locations of the crests and troughs. For this reason, it is called a Standing Wave (e.g., www.glenbrook.k12.il.us/gbssci/Phys/mmedia/waves/swf.html). For a given operating frequency, the extent of any impedance mismatch between the antenna and the transmitter can be described in terms of the ratio of the voltage maxima to the voltage minima on the transmission line: the higher the ratio, the worse is the impedance mismatch and the more power is being reflected. This is called the Standing Wave Ratio (SWR). If there is no impedance mismatch between the antenna and the feedline at a given frequency, then all of the power going to the antenna is radiated and there is none reflected to interfere (add/subtract), therefore the voltage remains the same at all points between the transmitter and radiator, providing a SWR of 1:1.
If we measure the wave energy in terms of voltage, we then speak of the "voltage standing wave ratio" or VSWR. Impedance mismatches mean that the VSWR is greater than 1:1, because at the points where the waves interfere constructively, the voltage peaks can be very much higher than normally expected. The table below shows the approximate percentage of forward power that will be reflected, depending upon the impedance mismatch.
VSWR
Power reflected (approx.)
1.0 : 1
0%
1.3 : 1
2%
1.6 : 1
5%
2.0 : 1
10%
3.0 : 1
25%
6.0 : 1
50%
As long as the feedline is of good quality and the total length of the run is relatively short (e.g., up to 30m or 100ft or so), losses at HF will be minimal and the signal will eventually get back to the antenna to be radiated. High SWR becomes a concern in lossy feedlines at high output power levels because of RI2 heat-loss, possible dielectric breakdown (arcing) on feedlines, or undue heating/arcing in the transmitter output circuitry. At HF, good-quality coaxial feedlines are capable of occasionally handling reasonably high SWR at moderate power levels, and most modern transmitters will reduce or "fold back" the output power in proportion to a high impedance mismatch. Nevertheless, it is advisable to always monitor transmission line SWR and correct significant mismatches; which then brings up two practical questions about SWR:
  1. What is an acceptable SWR? Often, we are overly concerned about SWR, fretting when is isn't exactly 1:1. If we can presume that there are minimal losses in the feedline, then it may be helpful to think of a 1:1 ratio as a goal rather than an absolute necessity, since some of the factors that may influence SWR (operating frequency, wind movement of the antenna or of nearby tree limbs, seasonal foliage variations, temperature, air moisture, etc) are constantly changing. Furthermore, even the better "SWR meters" are generally accurate to only +/- 5% of mid-scale readings. Note that in the above table, even assuming that the reflected power is lost (which it usually isn't), it would really not be of a concern below 2:1. Of course, one should always strive to improve the antenna system as much as possible, but for HF operation at amateur power levels, little or no practical difference in communications ability will be noticed between a SWR meter reading of 2:1 and one of 1:1. At high SWR (usually 2:1 or greater), modern transmitters will "fold back" the output power in proportion to the mismatch; however, when necessary, reasonable operation can usually be enjoyed with a reading as high as 2:1 despite the reduction in output power.
  2. What happens to the reflected power when the SWR is not 1:1?
    Again, assuming that there are minimal losses in the transmission line, since it is an AC, upon cycle reversal the reflected component along with the forward component will flow back to the antenna impedance mismatch and part will be radiated while part will be reflected, and so on, until the transmission is ended. This is analogous to the action of sea waves encountering a river inlet (another "circuit" with an "impedance difference"): part of the water flows into the river and a portion is "reflected" back into the sea. Is the reflected water "lost"? No, it is just incorporated into the next wave cycle, flowing back to the river mouth. So it is with AC in loss-less circuits with differing impedances - the reflected energy just returns as part of the next cycle.
Of course, it follows that if there is no impedance mismatch between circuits, then there is no current flow difference in them. Maximum power transfer per cycle between circuits occurs when they have closely matched impedances. Since we are interested in transferring RF power from the transceiver to/from the radiating element of the antenna system, we must be concerned with matching the impedances all along the route. Ideally, this means that we would like the same impedance to exist from the transceiver output terminal to the antenna radiator. Fortunately, transceivers are designed to have a standard output impedance of 50, so all one need do is "match" the rest of the antenna system to this value. For the time being, suffice to say that this can usually be accomplished by using a transmission line and a radiator of similar impedance, or by using some form of "antenna tuning unit (ATU)", that can make the antenna system impedance appear to be the same as that of the transceiver output. A word of caution: since there are ATUs that can match almost anything to a transmitter output, it should be evident that an SWR of 1:1 is not a guarantee of the effectiveness of the antenna, but only the ATU. Indeed, a 50 resistor connected across the transmitter output will provide a nice 1:1 SWR, but not much power will be radiated. So, when monitoring your antenna SWR, you should also be aware of how your antenna is supposed to perform and keep a close eye on any performance changes - if you notice anything, then maintenance may be required! A very good practical discussion of SWR appeared in the November, 2006 issue of QST (p.37): "Understanding SWR by Example"' by Darrin, K5DVW.
While on the subject of matching, there is another issue of importance: the symmetry or "balance" of the current flows in the feedline and antenna. Referring to the dipole illustrations above, can you spot any difference between the "ladder-line" and the "coax" fed dipoles? Consider the symmetry of the ladder-line example: one can split the picture "down the middle" and have two identical halves on either side of the center feedpoint - what one might call a "balanced" symmetry. On the other hand, that cannot be done for the coax-fed antenna - the "balance" ends at the feedpoint, as the coax (center conductor surrounded by an outer shield) is clearly asymmetrical, or "unbalanced" in terms of symmetry. Does it matter? Briefly, the answer is "YES" it can. For the ladder-line dipole, any feedline current on one side of the symmetrical "halves" is equal to, but opposite in direction of that on the other, so any radiation by one side of the feedline is canceled by that of the other. This is what we expect, as we want the radiator to do all of the radiating, especially if it is intended to provide a directed radiation pattern. In the case of the coax dipole, the feedline currents from the transmitter flow in the center conductor and on the inner surface of the shield ("skin effect"), completely contained within the cable and therefore also not radiating, as illustrated in the figure below for one-half of the cycle. So far, so good.
However, difficulties can arise with coax when an unbalanced current flow occurs in the feedline (e.g., by an off-center feedpoint of the radiator, or induced directly from the antenna radiation field) in such a way that the current flow is common to both the inner and outer surfaces of the shield: that is, one on the inner-, and the other on the outer-surface, both flowing in the same direction, as shown in half-cycle illustration below.
While the inner current is intended to be there by design, that isn't the case with the outer "common mode" current, and it is free to radiate from the feedline, possibly altering the radiation pattern of the antenna, or return into the shack to cause problems. To avoid this situation, whenever an unbalanced feedline like coax is used to feed a balanced radiator, it is advisable that something be done at the feedpoint to avoid the common mode current flow. A device that corrects the problem of balanced-to-unbalanced currents is called a "balun"; of which there are two types: the transformer balun or the choke balun. The transformer balun is usually used when there is a need to match (transform) impedances, while the choke balun is used in the case of matched impedances but un-balanced circuits. (Note: Although it may be a less-frequent problem with balanced ("twin-lead") transmission lines, common-mode current flow can occur if the line symmetry is corrupted by running it too closely parallel to one section of the radiator element, or too close to metallic objects.)

Antenna Parameters of Interest to DXers

Now that we have a "yardstick" for comparing antenna types, what exactly do we measure and compare? Any conductor connected to the output of a transmitter will radiate some RF energy, so what we must be concerned with is the efficiency of the radiator for its intended purpose and environment. Basically, there are five attributes of an antenna that are of concern for DXing:
  • angle of radiation - the angle from horizontal (sometimes measured from vertical) at which a major portion of the radiated power leaves the antenna.
  • gain - how much radiated power will be effectively focused in a specific direction compared to a reference antenna.
  • front-to-back ratio - difference in directional gain between the forward and reverse direction; a measure of the attenuation provided at the "back" of a directional antenna.
  • bandwidth - the band of frequencies over which the antenna will perform as well as intended.
  • noise susceptibility - to what extent it may be vulnerable to reception of manmade (environmental) noise or interferences.
The first four attributes apply to antennas on both transmit and receive - a transmitted signal gain in one direction means a received signal gain as well. Although the value of directional antennas with gain is obvious, the idea of a "negative gain" (signal attenuation) described by the front-to-back ratio may initially seem odd to some. However, it provides a well-known edge for DXers: when you're in a pileup, not only is it nice to be able to direct more of your signal energy towards the desired station, but it is also nice to simultaneously reduce the interference caused by the clamor of stations calling from the opposite direction! The last factor, noise susceptibility, is of importance for weak signal reception where antennas that provide high signal-to-noise ratio are desirable. These factors are not necessarily independent of one-another and trade-offs among them are usually required. We'll look briefly into the meaning of each, but readers are advised to consult antenna reference books and web-sources, some of which are listed under References below.
Here is a brief discussion of each:
- Radiation Angle: The need for reliable close-range communication would warrant the use of an antenna that concentrated most of the radiated energy locally, that is, an antenna that produced a spherically symmetrical radiation pattern (figure below) so that most of the RF energy went straight up, to be reflected back down in the immediate region, as in the figure below for an 80m dipole at a height of 10m (33 ft). The first thing to notice is that, unlike the free-space results, the pattern for a dipole near ground level is quite different: no longer do we see the "figure-8" pattern; rather it is essentially omni-directional, with half - or more - of the energy radiating upwards at high angles.

An antenna like this, with a significant portion of its energy radiated in a near-vertical incidence pattern, is affectionately called a "cloud warmer". Although very effective for local HF communications within couple of hundred miles or so, a cloud warmer, with most of its radiation going up at very high angles rather than out towards the horizon, will have very short skip, so it is definitely NOT a DXer's antenna of choice!
This brings up an important fact about the fourth component of antenna systems: the radiated waves interact with the environment. Many hams expect that dipoles always radiate energy in the free-space doughnut pattern, broadside to the wire, which, if sliced in a plane parallel to the ground, appears in the azimuthal view like a figure-8; that is NOT the case for low antennas because of the significant interaction (absorption and reflection) of the waves with the near-field ground surface. A rule-of-thumb is that unless a dipole is at least a half-wavelength above ground, one may not expect to obtain the bi-directional pattern. Keep this in mind!
OK, fine, but cloud warmers are NOT what we want for DXing! We want an antenna that will radiate a significant portion of its energy at low angles towards the horizon so that the signal will reach out as far as possible, because we learned in the chapter on Propagation that radio waves can "ricochet" from the ionosphere and back to Earth. As mentioned in the discussion of "skip" in the chapter on Propagation, radiation angles of less than 30o are desirable for DX. The figure below is a refresher of that seen in the chapter on propagation. In (A) the skip phenomena is shown, and (B) illustrates the rule that the smaller the angle of radiation, the greater will be the skip distance.
Now, you ask, what exactly is the "radiation angle" (sometimes also called the "take-off angle")? If, as we saw in the Propagation chapter, the radiation leaves the antenna as an ever-increasing spherical blob, how can we speak of a specific angle of radiation ... isn't radiation emitted in just about all directions? While it is true that antenna radiation is not quite like the figures used to illustrate skip, and the "rays" depicted are for convenience only, it is possible to design antennas that radiate a significant portion of the energy in preferential directions, not only azimuthally (i.e., in horizontal directions) but also in the degree of elevation (radiation angle) above the horizontal plane. In the previous figures illustrating the radiation pattern for a dipole in free-space, it is evident that the radiation is more focused in the broad-side direction, even though some is also emitted off at different angles. In fact, one can see a small green dot at the farthest-extended point of the broad-side lobe, used by EZNEC to mark the azimuthal location of maximum signal strength in the horizontal direction. As we'll see later, when we look at a vertical slice of the 3-D pattern, a similar marker will indicate the elevation angle at which the maximum radiation occurs ("radiation angle").
The angle of radiation of an antenna is dependent upon a number of factors: the antenna design; the height above ground; the ground conductivity in the near-field region of the antenna; and the proximity of other objects (especially conductors). Since it is difficult, if not impossible, to do anything about the last two without re-locating, DXers usually concentrate their efforts on the first two - antenna design and height above ground. We'll look at some popular DX antenna designs below; and as for what to do about height above ground, the answer is self-evident - get it as high as you can! A general rule-of-thumb is that for horizontal antennas to have reasonably low radiation angles, the minimum height above ground should be one-half wavelength at the operating frequency.
- Gain & Front-to-Back (F/B) Ratio: The ability to design antennas with a directional radiation pattern means that we need some way of evaluating just how "directional" they are. Directional antennas are described in terms of their gain and front-to-back ratio (F/B). The gain of a directional antenna is dependently coupled to the front-to-back ratio - as one goes up, the other may go down - so that proper design is important in order to optimize the figure of interest. Although one frequently hears only comments about antenna gain, experienced DXers know that the front-to-back ratio is also important, since one of the benefits of using a directional antenna is to be able to attenuate strong signals from areas in the opposite direction of the incoming signal, making it easier to select weak signals in a pileup of strong signals. Remember that since an antenna's effective gain (what you're interested in when you're working DX!) will also be affected by the angle of radiation, we can expect that height-above-ground will be another important factor.
When the strength of a test antenna's directed radiation component is compared to that of a reference antenna, the ratio of the two is defined to be the gain of the test antenna over the reference antenna, expressed in decibels. That is, Gain(dB) = 10 log (Ptest/Pref), where Ptest is the power radiated by the test antenna in a given direction and Pref is the reference antenna power radiated in that direction. Unfortunately, it can sometimes be confusing when trying to understand the gain figures when they are used in the different contexts of the three commonly discussed antenna environments: (1) free-space, (2) perfect ground, and (3) real ground. Let's take a brief look at these:
  1. Antenna design comparisons with mathematical models are typically done in the theoretical free-space environment using an isotropic radiator defined as having unity gain in all directions. The resulting measure for the test antenna is said to be the "gain over the isotropic antenna", or "dBi gain" for short, where the "i" indicates that the comparison was with an isotropic radiator. Alternatively, comparisons may be made with a standard half-wave dipole, in which case the gain is expressed as "dB gain over a dipole", or "dBd gain" for short. There is a difference between the two measures that arises from the fact that, as we saw in the free-space pattern for the dipole, it does favor a broadside direction, so a dipole has an intrinsic gain over an isotropic radiator of about 2.1 dB in the directions broadside to the dipole; more appropriately, we should say that the free-space dipole has a gain of 2.1 dBi. What this means is that free-space dBi and dBd gain figures are related as follows: dBd = dBi - 2.1.
  2. The theoretical modeling can also be done in an environment that resembles actual use, but is still idealized to reduce unknowns. This is the "perfect ground" environment in which the antenna is imagined to be on a perfectly conducting, flat plane surface in the near-field. In this case, the free-space 3-D pattern is cut in half, and the "bottom-half" energy is reflected up into the "top-half", doubling the radiated power forming the pattern. As we might expect, the result is that the gain figures for directional antennas would increase over that of free-space. For example, the gain of a dipole over perfect ground would be 8.4 dBi (6.3 dBd) at an elevation angle of 30o.
  3. Modeling programs such as EZNEC can simulate "real" ground conditions that more nearly approximate the conditions in your backyard. The effect of real ground on the antenna pattern is also to reflect the near-field energy upwards to contribute to the radiated pattern, but to less extent than the perfect ground, as there now will be some loss. In the case of the dipole, gain would be 7.6 dBi (5.5 dBd) at an elevation angle of 30o.
It is easy to feel that this is all more confusing than helpful, but the important thing to remember is that in looking at the specifications of different directional antennas, you should always be certain that comparisons are made using the same units of gain. If the units are of the same measure, then you will have a fair comparison. A final note about antenna "gain": while it may seem that the use of the term implies an amplification of the radiated energy, that isn't the case. What a directional antenna does is the same as what is done with a "spotlight" - rather than allowing the energy to radiate in all directions, it is simply focused into a desired direction; so a more appropriate term is "directional gain". For this reason, directional antennas are referred to as "beam antennas" or just "beams".
One last comment about antenna gain: occasionally one encounters the term Effective Radiated Power (ERP) of an antenna, such as in radiation safety considerations. As the name implies, it is a measure of the effective (as opposed to actual) power radiated in the direction of interest, such as towards the neighbors' houses. ERP is the product of power supplied to an antenna and the antenna gain in a given direction, as compared to a reference antenna. For example, an output of 100w-PEP into a 3-el Yagi with 6 dBd gain (x4 power gain over a dipole) would provide an ERP of 400w PEP in the forward direction of the beam as compared to a dipole.
- Bandwidth: The bandwidth of an antenna describes the frequency range over which it will function as expected. In the simplest case, this is the frequency range over which the impedance match to the transmitter output is within satisfactory limits, usually specified as an SWR of 2:1 or less. However, in the case of the directional antennas discussed below, bandwidth is a critical measure of the frequency range over which the antenna gain and F/B ratio hold up.
- Noise Susceptibility: RF waves, as discussed in that chapter, have electric and magnetic field components that "leap-frog" through space once the wave is radiated from its source and, by convention, the orientation or "polarization" of the wave is described in terms of the orientation of the electric field component. That is the reason we say that horizontal antennas, such as a dipole, will produce "horizontally polarized" radio waves (see illustrations in "RF Waves"), while vertical antennas will produce "vertically polarized" waves. It follows that if the antenna orientation is the same as that of an incoming wave polarization, then it will be somewhat more sensitive to signal induction by the wave. However, wave polarization may be altered by several factors, the most common being reflection at conductive surfaces. Radio waves from distant stations, having undergone ionospheric refraction and ground reflection, may have a variety of polarization angles. Therefore, differences in the polarization of the antennas at each end of a long communications path are not of great significance in regard to communications signals. On the other hand, receive-antenna polarization is of importance when there is a significant amount of locally generated noise (as in suburban and urban areas), since this type of noise happens to be predominantly vertically polarized. This means that a vertical antenna will be more sensitive to locally generated noise. For this reason, vertically oriented antennas, while they can be very effective transmit antennas, have a reputation for being "noisy" receiving antennas.
To help understand the first three parameters above, as well as the data available in the radiation pattern graphs that one frequently sees (some previously, with more below), an illustrated example is explained in "Antenna Notes" in the "Miscellaneous Notes" Appendix. Antenna design, modification, and optimization would be a tedious process if one had to continually resort to field testing for new ideas or changes to see if they performed as expected. Since it is difficult (more to the point: IMPOSSIBLE!) to control the environment around antennas when making comparisons, software modeling and the theoretical construct of the free space environment are very useful. Yet, it can often be confusing to the uninitiated, making it a good marketing tool! Caveat emptor ... .

Antennas for DXers

There are as many different antenna designs as there are ways to draw lines on paper, but here are a very few of the more popular ones used by DXers. These are presented in approximate order of increasing over-all (transmit and receive) effectiveness for DXing. The antenna that you use, or select to install, will probably depend upon the usual variables that affect most of our choices: available space, money, antenna support structures, and any neighborhood restrictions. No matter what your circumstances, there is a solution to whatever problems that you happen to face and, while it may not be the "pileup buster" of your dreams (don't we all dream ...?) it should allow you to get into the chase. As an example, years ago from my single-story apartment building, I was able to work more than 100 different DXCC entities with a 50-watt transmitter and a 15m vertical mounted at the roof edge, using the roof flashing as a "ground" (a small school banner on the antenna was my "disguise").
- Random-wire or "Long-wire" antennas: Consisting of as long a piece of wire as can be installed at as great a height as possible, these are by far the simplest of all antennas. As illustrated in the figure below, a typical installation consists
of a length of wire that runs directly from the radio room, out a window to the first support at the eaves of the house, then extending to the farthest possible structural support. Although the best configuration is usually a straight run of the horizontal portion, it is not essential. The wire may run straight up and terminate at the top of a tree, or be laced through trees and supports, up, down, and around, as needed. While length is not critical, a minimum of 20m (66 ft) will generally assure reasonable performance on all bands from 80m - 10m, with increasing effectiveness on the higher bands; however, the longer and higher is the wire, the better will be the performance for DX. Use of small-gauge wire also makes this a good "stealth" antenna when the situation demands it. One can use any conduction material of any length, orientation, or layout that is conveniently available (wire, aluminum foil strip taped to the wall or window, large metal window frames, copper gutters insulated from ground, or anything that your imagination can fathom) being careful that the conductor is reasonably protected from curious and wandering hands, because there is always a danger of severe burns from high RF current!!!
An important thing to note when using a random wire is that, since the radiator part goes directly to the transceiver, the "transmission line" coming down into the radio shack is actually part of the radiator, so take care! Since the impedance of a random wire antenna will be highly variable, depending on length, height, and environment, it will require the use of an impedance matching device (i.e, a robust antenna tuning unit, ATU) to transform the line impedance to 50.
Random wire antennas are typically omni-directional, except that when they are over a wavelength in length and at least a half-wavelength in height at the operating frequency. Then they begin to exhibit some directional lobes. For the higher bands, these conditions are very feasible. If you have access to enough real estate to put up a random wire of 150 feet or more in length and at a reasonable (~10m) height, you will not only have an all-band antenna, but also an excellent chance of working some good DX on the higher frequency bands (14 - 28 MHz), since it may have some good low-angle lobes, as can be seen in the figure below.
Also, if the random wire antenna has an appreciable portion that is of vertical wire run (e.g., one-eighth wavelength or more) in addition to the horizontal portion, it may function as a vertical radiator, providing additional low angle components at lower frequencies (see the inverted-L below).
- Dipole antennas: Next on the scale of "low-cost, ease and simplicity", the dipole antenna described earlier is easy to construct and erect, cheap, and, if sufficiently elevated, very effective - that's a hard combination to beat! Dipoles are usually mounted horizontally between end supports. Since the intrinsic impedance of a dipole elevated to a height of one-half wavelength is close to 50, most hams use a 52 coax feedline since it offers a good impedance match between the antenna and the transceiver. However, the balanced dipole and the unbalanced coax poses a problem of common-mode
current flow. Since there is no need to transform the feedline-to-antenna impedance, the simplest solution is to use a choke balun. Several methods of construction are discussed in the references below, but the simplest consists of coiling turns of the coax feedline just before the feedpoint. Other methods are to use a number of ferrite bead "collars" placed around the coax near the feedpoint, or one of the commercially-produced 1:1 baluns. The following guidelines are based upon data posted by WA2SRQ several years ago and now available on various websites (see: www.bcdxc.org/balun_information.htm#Ed,%20WA2SRQ):
Band
# Turns @ 6" Diameter
160m
Use ferrite beads instead
80m - 30m
8-turns, bunched closely
20m - 10m
4-turns, single layer
For the single-layer winding, PVC pipe or a 1-Liter soft-drink bottle can be used as forms. Once adjusted for proper resonant length, a dipole fed with 52 coax through a balun may be connected directly to the transceiver without the need of an impedance matching device.
In order to provide low-angle lobes for hearing and working DX, the dipole should be at a height of at least one-half-wavelength above ground. The figure below shows the dipole radiation elevation pattern (vertical slice through the 3-D pattern), and it is clear that at a height of 10m (33 ft), a dipole on 20m can be expected to exhibit better low-angle radiation
than its counterpart on 40m at the same height. A half-wave dipole may also be used on odd-multiple harmonic frequencies without serious impedance mismatch. For example, a 40m dipole cut for the lower end of 40m will usually work on 15m, where it becomes a 3/2-wavelength dipole antenna. Dipoles (and verticals) may also be designed for operation on multiple bands through the use of "band traps" (or just "traps"): resonant L-C devices that act as automatic switches, isolating the end-most sections of the antenna above their design frequency band.
An interesting variant form of the dipole is the inverted-V, which is simply a half-wave dipole with the center feedpoint forming the apex of an upside-down V (see figure). This is a great way to mount a dipole if there are no convenient end-supports available. Ideally, the legs at the feed-point apex should form a right-angle, but this isn't critical.
The inverted-V can be easily adjusted and pruned to provide a feedpoint impedance that is close to 50. The advantage of the inverted-V dipole over the flat-top dipole is that it requires less space and only one tall support, while providing nearly the same performance as a horizontal version at the same apex height. In the picture below is the author's 30m/40m inverted-V combination made from 14-gauge stranded/insulated wire from the hardware store (Home Depot).
The 30m antenna hangs below the 40, suspended by 4" spacers made from readily available 3/8-inch polybutylene water supply-line tubing, cut & drilled at each end to allow "threading" of the antenna wire through each. The coax feedline attaches to a commercial 1:1 balun, which also supports the antenna at the apex (a better angle view of the feedpoint may be seen below in the picture of the Quad).
Finally, a great all-band wire antenna is a 1/2 wave 80m dipole or inverted-V with apex at a height of at least 40 feet, fed with ladder-line through an ATU. In the early 1990s, this was used by the author to work DXCC on 12m, 17m, 40m, and 80m (as well as on 30m before the award was offered for that band) all with 100w. An excellent discussion of most aspects of a multiband "doublet" can be found at www.cebik.com/edu/edu6.html. Several variants of the dipole, usually touted as "multiband" antennas, are the G5RV and Windom. Each has its merits, but be aware that an impedance matching tuner is required for effective multiband performance.
Loop antennas: Another simple directional antenna is a one-wavelength vertical loop (figure below).
The actual loop geometry can be a diamond, triangle, or rectangular configuration. When constructed in the square (4 equal sides) geometry, it is usually called a "quad loop". The impedance of a full-wave loop is approximately 100-ohms, so a 2:1 matching transformer is required when using 52 coax. Full-wave loops have an azimuthal radiation pattern that is similar to the "figure-8" of the dipole, but the elevation pattern is different, as seen in the comparison below of a full-wave 15m loop and a 15m dipole, both at a height of one-half wavelength. The loop has slightly more gain at a
lower radiation angle (8.34 dBi at 21o) compared to the dipole (7.38dBi at 28o), but also shows some high-elevation radiation "loss".
- Vertical antennas: The most commonly used vertical antenna is the 1/4-wave vertical. Illustrated on the left is a typical schematic of a /4 ground-mounted vertical with "ground radials".
Used with a radially-dispersed wire radial system to enhance the ground conductivity at the base of the antenna, it will have a reasonably good impedance match to 52 coax. This antenna can be very effective low-angle radiator, as seen in the elevation plot, modeled over average ground, of the radiation pattern on the left below. It shows a low-angle lobe hugging the ground, with a maximum at 26o above the surface.
On the right (above) is an azimuthal view of the vertical's pattern at the elevation of maximum radiation, from which we see that the antenna is omni-directional with essentially unity gain (-0.19 dBi, the difference between the vertical and an isotropic radiator, is close enough to zero to be a negligible difference). Because of its good DX potential (low radiation angle), small "footprint", and easily disguisable profile, the vertical antenna is particularly appealing when residential restrictions are an issue, since it can be readily concealed in flagpoles, trees, alongside chimneys, etc.
A 1/4-wave ground-mounted vertical antenna is conceptually equivalent to a vertically-mounted 1/2-wave dipole antenna with the lower end buried below ground, where the buried portion is considered to be the virtual "mirror-image half" in which the antenna currents flow. The 3-D radiation pattern is similar to the doughnut pattern of the dipole seen previously, but turned on its side and bisected by the ground surface and, were the ground to be a perfect conductor, the lower-lobe would then extend outward flush with the surface for a 0o angle of maximum radiation. If that were so, a metal stake would provide a sufficient ground connection for the currents to flow into the idealized below-ground image; however, ground conductivity is generally not very good. Without the improved conductivity of a radial system, two problems occur: (1) most of the virtual "bottom-half" current is dissipated as heat by the poor conductivity of the ground surface; and (2) the expected "center-fed dipole" impedance of approximately 50 truns out to be considerably less.
To minimize ground-current losses at the base and to have a good impedance match to 50 coax, one must provide a bed of radially symmetric conductive media, or radial ground system. Insulated wires placed above the ground surface should be /4 in length; however, length is not critical if the wires are buried just below the surface. In any case, radials should be symmetrically dispersed about the base and as plentiful as possible. The theoretical base feed-point impedance of a /4 ground-mounted vertical over a good radial system is approximately 25 - 30, providing an acceptable match to 52-ohm coax (SWR <2:1). Note that the feedpoint symmetry of the /4 vertical is unbalanced, so a balun is not required when using a coax feedline. If one wishes to achieve a better impedance match, then an impedance transformer can be used that provides a 2:1 unbalanced-to-unbalanced transform; such a device is called a "unun".
If nearby structures are a problem, one way to avoid them is to raise the /4 vertical above ground and use elevated radials. The main difference in elevated vs. ground-level mounting is that the elevated radials must be /4 resonant lengths, because the antenna is now akin to a half-wave vertical dipole with the lower /4 section bent horizontally. By using 3 or more horizontally symmetrical (i.e., "radial") elements, most of the horizontally polarized radiation is canceled, leaving only the vertically polarized low-angle component. When mounted above ground with elevated radials, a /4 vertical is also known as a "ground-plane" antenna.
Mentioned above was the idea of a 1/2-wave vertical dipole. This is actually an interesting antenna - a true dipole mounted above the ground in a vertical orientation. Since both "halves" of the dipole are available for use, no radials are needed and the low radiation angle is essentially that of the /4 vertical with radials. Although a full-sized 1/4-wavelength antenna is rather long for frequencies below 14 MHz, it is possible to use a "trapped" version that is shorter. This is the basis for some of the commercial multi-band "no-radial" type verticals, and they may offer good a good compromise in difficult situations where there isn't room for radials.
Which brings us to the difficulty of antennas for 80m and 160m. These bands are a problem for most of us, as they usually require more space than we have available, especially for antennas that have low radiation angles, much less gain. Ideally, a dipole for 80m DXing would have to be mounted 40m (130 ft) high in order to have a reasonably directive pattern with a low radiation angle. For 160m, think twice that height! That is NOT to say the lower antennas will not work - the author achieved DXCC on 80m using an 80m inverted-V with an apex at just 12m (40ft). However, to put this in perspective, 40ft is about 0.15 at 80m, so the 80m antenna would be roughly comparable to a 20m antenna at 0.15, which would be a height of 3m (7ft)! That is why the low-bands are a problem for DXers without large land area and tall support structures. We not only want to be able to work stations, we want to be able to work DX! Well, there are solutions. Home-brew, or commercially available, compact vertical radiators for 80/160 can provide good results when used with a good bed of radials. If one has a tower for a beam antenna on the higher bands, it may be possible to "shunt-feed" the tower itself as a vertical radiator with the beam providing a "top-hat" capacitance loading that can improve efficiency (www.qsl.net/w9rb/webdoc9.htm; also see References); of course, a radial ground system is needed for this as well. A simple but very efficient antenna for the 80m & 160m bands is the Inverted-L shown in the figure.
The Inverted-L is a /4 vertical with the top bent over into the horizontal plane. Depending upon the proportions of the vertical and horizontal components, radiation will occur from both. A typical arrangement is a vertical section of 12m - 20m, with the rest (28m - 20m) along the horizontal. For greatest efficiency, the vertical section should be as tall as possible. Since the radiation efficiency is proportional to the square of the vertical length, even a few feet of extra vertical height can make a difference. With a suitable radial ground system, the feedpoint impedance is about 30, so a direct coax feed is possible. If one prefers a better impedance match, then a 2:1 unun can be used. As has been stressed, the overall effectiveness of vertical antennas hinges upon the availability of a good ground system with as many radials as possible. The ever-present question is "How many and how long ...?". Considerable studies, trials, and countless discussions have explored this issue and it continues today. Based upon current wisdom, it is suggested that one use as many as possible, at least /8 long, symmetrically spread about the base feedpoint, on the surface or buried. A minimum of 10-15 is believed to be necessary in order to attain a noticeable efficiency over none, while 30-40 reaches the next level of improvement, and minimal incremental change from that is realized as one approaches the commercial broadcast standard of 120 one-quarter-wavelength wires. Nevertheless, the ultimate rule is: try whatever you can manage!
Another versatile low-band antenna for those with a tower is the " /4 sloper" shown below.
Although the "quarter-wave sloper" appears to be half of an inverted-V, it is actually more of a top-loaded vertical. The pattern is essentially omni-directional, with low-angle radiation from the tower and some high angle radiation from the sloping element. Many articles have been published about using slopers on 80m and 160m, but it seems that users have had mixed results. Tuning of a sloper may be affected by the angle of slope, antenna(s) mounted on the tower, and nearby structures. There appear to be two conclusions about the low-band sloper:
  • When they are adjusted to operate properly, they seem to perform very well.
  • The ability to get them to operate properly may require a considerable amount of effort.
For those interested in 160m antennas, the premier reference book is "Low-Band DXing: Your Guide to Ham Radio DXcitement on 160, 80 & 40m" by ON4UN (www.arrl.org/catalog/7040/). In addition, a wealth of information (and interesting discussions!) about Top Band antennas, equipment, and operating techniques are to be had by subscribing to the Topband list at lists.contesting.com/mailman/listinfo/topband.
Receive-only antennas: DXing on the low bands with vertical antennas brings up another problem: that of local noise. As stated previously, vertical antennas are susceptible to vertically-polarized man-made noise - a big problem in suburban and urban areas. While some are able to erect dipoles (or inverted-Vs) that are high enough to be useful for transmitting and receiving, it isn't easy to find room for a 260 foot-long antenna, and even more difficult to get it high enough to enjoy low-angle radiation. That means verticals are the usual choice for the low bands. So how does one get around the noise problem? A common practice is to use the vertical for Tx, taking advantage of its low radiation angle and "footprint", and use a second "low-noise" antenna for Rx. The subject of 160m Rx antennas is a shelf of books unto itself, so those who may be interested are directed to the references below. Having said this, let me add that on 160m the Inverted-L is a good all-around compromise for anyone with limited space. The reason is that the horizontal portion (which usually turns out to be longer than the vertical part) seems to provide reasonably "lower" noise receiving than would a full-height vertical.
As evidence of this last observation, consider my "late-life" adventure on 160m. Living on a relatively small (18m x 30m) urban lot, I felt lucky to have been able to put up a 20m-high crank-up tower for my 5-band quad. Some years ago, after 40 years as a licensed and active ham, I had never tried 160m because I had been told that it was " ... only for hams with plenty of green-space ...". Well, after some limited but unexpected success in working DX with an low 80m Inverted-V hung from the tower, I decided that it was definitely possible for even a city-slicker to enjoy 160m. I put up an Inverted-L for 160m: 40m of 12AWG stranded/insulated copper wire running approximately 12m vertically up a small oak tree in the rear, and going out horizontally for 28m to a pine tree in the front yard. Initially, I buried 10 radials varying in length (20m - 40m), and eventually squeezed in another 6, weaving around structures and plants in the yard and, with permission, sneaking a few out on the property behind and adjacent to mine. Did it work? Well, after some 5 years, I had over 100 DXCC entities confirmed, while having as much fun as I did when I first began to work DX in the middle 1950s! Of course, it was not easy and required a lot of late night/early morning listening through a LOT of noise, along with developing a new understanding of propagation, receiver sensitivity/selectivity, improving signal-to-noise ratio, and plenty of P.E.P.S.I.!!. But I will tell you that it was, for me, an achievement of immense satisfaction that I never imagined possible! Topband - try it, you'll like it!
For those who prefer multiband antennas, the inverted-L could be used as an all-band antenna with the placement of an ATU at the base. There are also commercially-available multiband verticals. Multi-band wire antennas can be constructed using resonant inductor-capacitor circuits to electrical "cut" the length of a long conductor at a desired operating frequency, thereby "trapping" the currents within that length, hence the popular name: "traps". Just remember that, regardless of any marketing claims to the contrary, low angle radiation from a short vertical antenna is contingent upon an effective ground system.
Directional antennas: Described in terms of their gain and front-to-back ratio (F/B), these are the ultimate antennas for DXing because they offer not only directivity, but also front-to-back rejection that is invaluable in DX pileups. Directional antennas are constructed by combining two or more antenna elements in an array that makes use of the "interference" property of waves in which phase similarities and differences can produce reinforcement or suppression of the mixed wave. We have already encountered and discussed the simplest of the directional antennas - the dipole and the full-wave loop. By proper design and layout of an array of dipole, loop, or vertical elements, one can focus radiation (constructive interference) in one direction while minimizing (destructive interference) it in other directions. Remember that since an antenna's directional gain will also be affected by the angle of radiation, we can expect that height-above-ground can be another important factor. Also, the F/B ratio will decrease (or may even reverse!) as one exceeds the design bandwidth of the antenna (typically 100 - 200 KHz or so).
There are three methods for designing directional antennas, depending upon how the elements are made to radiate:
  • parasitic arrays - power is fed to one element ("active" or "driven element"), and the other ("parasitic") elements absorb and re-radiate at different relative phases depending upon placement.
  • phased arrays - power of is fed to all elements, using a method for varying the relative phase of the signal going to each active element.
  • combination of both - more than one active element, along with one or more parasitic elements.
The most popular rotatable beam design is a parasitic array known as the Yagi-Uda (named after the inventors and more commonly shortened to "Yagi"), consisting of a half-wave dipole driven-element with a parasitic half-wavelength "reflector" element and one or more parasitic half-wavelength "director" elements mounted in parallel on a boom, each spaced approximately 0.15 - 0.25 wavelengths apart, as seen in the left illustration below. The free-space azimuthal radiation pattern of a 20m version is shown on the right. Yagi parasitic elements are tuned to slightly different resonant frequencies than the operating frequency for the driven element: the reflector is about 5% longer, while the director is about 5% shorter.
The 3-element 20m Yagi modeled in the figures below is at a height of one-wavelength (66 ft) above real ground and uses a 8.5m (28ft) boom, providing a theoretical gain of 13.02 dBi.
While this is not an optimized design, it is obvious that it offers some distinct advantages over the antennas previously discussed. For one thing, in the left figure, we see that the radiation angle of the major (lower) lobe is 14o - very nice! In the right figure, the data indicates that the forward gain is 13.02 dBi (11.9 dBd) and, reading from the scaled chart rings, we see that the F/B is about 18 dB (see "Antenna Notes" in the "Miscellaneous Notes Appendix"). By changing the various dimensions, one can maximize the forward gain, or the F/B, or find the optimum balance between the two. This used to be tedious trial-and-error work, but in recent years, software with sophisticated optimization algorithms has become readily available for designing antenna arrays. A fairly extensive listing of various antenna-related software and online materials can be found at www.dxzone.com/catalog/Software/Antenna_analysis/.
Yagis are rugged, relatively compact, and can readily be "stacked" on a tower mast to provide multi-band coverage with a single tower. The picture below shows a 3-el 15/10m Yagi "stacked" above a 5-el 20m "monoband" Yagi (courtesy KB5GL).
Multi-band Yagis, like verticals, can be constructed using either resonant inductor-capacitor "traps" to electrically "cut" long elements at a desired operating frequency, or by essentially mounting multiple Yagis strategically spaced on the same boom, with a common-feed for the driven elements. Looking closely at the upper Yagi in the picture above, you can see the "traps" that "cut" the elements for 10m, and are ignored by the 15m currents so that they use the entire length. In recent years, a new method of providing Yagi (and vertical) multi-band capability was developed and is now marketed as the StepIR, in which the element lengths are dynamically altered remotely in order to change the operating frequency (www.steppir.com/design.htm).
A popular simple beam is the cubical quad which consists of two or more full-wave quad-loops made of wire suspended by "spreader-arms" spaced 0.15 - 0.25 wavelengths apart, and typically mounted on a boom in a "cube" configuration as illustrated schematically in the left-below.
Below are the elevation and azimuthal patterns for a 2-element 20m cubical quad on a 15ft boom at a height of one-wavelength (20m) above ground.
The radiation angle of the maximum lobe is 10o and the calculated gain of the model is 13.0 dBi. As for the Yagi, these figures are affected by element spacing, which typically varies from 0.1 - 0.25. However, for multi-band quads using the same spreader-arms for each band, it is usually necessary to make severe compromises, and the gain and F/B on each band may be far from optimal. Not shown in the simple illustration above are reflector tuning stubs (short wire extensions hanging from the lower side mid-point that can be adjusted to extend/contract the reflector resonant length), or the balun and impedance matching needed for the driven element. For details of quad antenna design and construction, a Google search of "cubical quad" will return more than you can read. For a classic reference, try to get a copy of "All About Cubical Quad Antennas" by W.I. Orr/W6SAI and S.D. Cowan/W2LX.
A 5-band (20/15/17/12/10) cubical quad is shown in the picture below, using a single feedline connected to all 5-director element "loops" through a 2:1 impedance matching transformer - note the choke balun, consisting of coiled coax, attached to the mast and just visible above the top of the tower (courtesy W5FKX). This type of antenna is far from optimal but does work well and is relatively inexpensive and easy to assemble and install; for example, with the help of my XYL, I measured, assembled, installed and tuned one like this in one day. Also, despite the reputation of being easily damaged by bad weather, this one survived Katrina atop the nested (lowered) tower.
A long-standing debate of many years that persists today, despite ample data addressing all of the issues, is the question of whether the Yagi or the Quad is the better antenna for DX. Sorry, it will not be reviewed here. Suffice to say that in making the choice of an antenna, many considerations come into play in addition to performance, such as cost, size, ease of installation, tuning, maintenance, and even prevailing weather conditions. Whatever one decides, it should be based upon a thorough review all currently available data, and with the understanding that environment is part of the antenna system. Make your choice and enjoy the results - you can always change to something else later on if need be. As for the debate about Quads vs. Yagis, that will be left for DXers to argue at the next club meeting.
- Low-frequency directional arrays: If space, neighborhood regulations, and budget allow, then a rotatable beam antenna mounted as high as possible is the unqualified best all-around antenna of choice for DXing. Because of their size, rotatable antennas are mostly found on the higher frequency bands of 20m and above. Of course, some compact beams are available for 30m & 40m, and even a few full-sized rotatable beams are being used on 80m (e.g., 2-el 80m beam on 160ft tower at YT6A: www.kolumbus.fi/oh2bn/partypix.htm). However, when space is not a constraint, using vertical phased-element arrays is a good option for constructing directional antennas for 80m and 160m. Even a simple array of two inverted-Ls can be effective. One should consult the References below for more information.
- Special Circumstances - Hidden Antennas: Increasingly, many hams find themselves in the unfortunate situation where the usual antennas that many of us take for granted are not an option. The most common reasons are (a) confined space living, as in apartment buildings; (b) codified residential restrictions; or (c) someone near-and-dear saying in a very unfriendly voice "You're going to put up what ...???". While ingenuity can come to the rescue with (a), and the ARRL may be of some help with (b), you may well be on your own in the case of (c)! Many hams have overcome restrictive environments by using antennas that are completely hidden from sight, or are at least very unobtrusive. A good example of the latter is an installation of a multi-band beam antenna by one of our local "Top-of-the-Honor Role" DX club members on a 50 foot tower in the midst of a very exclusive, densely populated city neighborhood. Using a low-profile wire-beam antenna (see Hex or Spider beams below) mounted on a telescoping tubular tower extending through his second-level rear deck, hidden at the base by potted plants and obscured by trees from the view of neighbors, he was able to effectively conceal his formidable DX-chasing antenna from all but those who knew to look for it. Unlike the distinctive "tower" look of the usual lattice-braced triangular construction, a tubular tower is not too different than flag poles or the aluminum street-light standards seen in many neighborhoods, and the compact Hex or Spider beam configurations seem to be less noticeable than large Yagis or quads. Of course, adjacent foliage and the discrete placement of decorative plants do help!
A good "stealth" antenna for DXers is commonly known as the "flag-pole" vertical, consisting of a vertical radiator disguised as a flagpole. Variations on this include: an actual flagpole mounted on an insulating base, or a multiband vertical mounted inside of heavy-walled PVC conduit that serves as the flagpole. Another "vertical" option is the use of a light-weight tilt-over installation that can be erected at night and then concealed during the day.
Attic-mounted dipoles, verticals, or even small compact beams, can often work just as well as outdoor antennas, especially in multi-level residences where attic-level antennas may be as high (or higher!) as their outdoor counterparts. Just be very careful not to use excessive power that may cause harmful RF exposure to occupants. Usually, for bands below 10m, output levels of 100w or even more may be within safety limits as long as there is no prolonged exposure at close proximity. My son lives in a covenant-restricted subdivision near Chicago, so he mounted a pair of dipoles for 20m and a 17m in his attic, about 30ft above ground. He does not use an amplifier, and our regular week-end schedule has been working well for over 7-years with this simple arrangement. During visits, I have used his station to make some very nice DX contacts.
Very small verticals like the "window-sill" vertical shown below can be useful in highly compromised situations such as apartments, condominiums, or hotels. Consisting of a short, clamp-mountable vertical radiating element with a base-loading coil and a /4 wire on the floor of the radio room, it can be mounted on a window-sill in the evening hours and then removed before daylight. While the "wire-on-the-floor" is often called a "counterpoise", it is actually just an inefficient (lossy) radiator, as this antenna is conceptually equivalent to a vertical dipole, with the vertical as the upper half and the wire on the floor as the lower half. Although severely shortened antennas are not very efficient radiators, they will at least allow one to have some fun. Also, an antenna like this can be easily packed and carried in luggage, and one performed reasonably well on a cruise-ship for one of our Delta DX Association club members. Efficiency of shortened antennas improve in the higher frequency bands (e.g., above 20m) as their physical length more closely approaches a 1/4-wavelength at the operating frequency.
Other alternatives are aluminum foil-tape dipoles for 10m taped to windows; dipoles taped/tacked to an apartment wall or ceiling; very thin wire (eg, enameled 28 AWG ) run from a window to a tree or other convenient support; all of which can be practically invisible, yet will allow you to enjoy some level of activity despite restrictions.

Summary

So what is important to know about antennas and what kind should you put up? There is really no "one fits all" answer. It depends upon many factors, but undoubtedly the most important are cost, available space, and local community regulations. From the brief discussion above, you should be able to begin looking into the best choice for your circumstances, using these very general observations:
  • random wire, dipole, and vertical antennas are usually the cheapest and easiest to erect and can be very effective.
  • for horizontal antennas, height is important; for vertical antennas, ground system is important.
  • variable-direction antennas (Yagi, cubical quad, or vertical arrays) are generally more effective than non-directional or fixed-direction antennas.
  • for a directional array, front-to-back ratio may often be as important as gain.
  • impedance matching is important, but SWR should not be an obsession: below 2:1 is usable; below 1.5:1 is acceptable.
  • low SWR doesn't guarantee that all is working as expected - know your antenna.
The important thing that must be stressed is that virtually any conductor will receive and radiate signals to some extent, so begin with whatever you have and work to improve it. Just because others may have a grand setup and you cannot is no reason for you to give up on DXing. Many DXers, at one time or another - myself included - have been faced with antenna restrictions, but that is just one of life's many challenges. You can still manage to have some fun, even with a "stealth" antenna. Indeed, DXCC has been achieved with amazingly simple stations running QRP and using hidden random wires or attic dipoles. Whatever antenna you put up, use it to develop your DXing skills: tuning, learning about propagation, understanding the characteristics of the various bands, and above all else, practice P.E.P.S.I.! A last word of caution: the question of "what is the best antenna" is probably the most controversial in ham radio and usually the quickest way to start a friendly argument, so be advised! ;-)

 Operating Modes

Is there a "Best" mode for DXing?

From the single mode of keying a spark-gap signal, to more than a dozen different ways of communicating over the radio waves, ham radio has undergone a phenomenal technological evolution over the relatively brief period of its existence. Despite arguments to the contrary (" ... CW always gets through"; "... PSK is the most efficient ..."; " ...SSB is the most robust method ..."; " ... you can't beat the fidelity of AM ..."), there is no single mode that is best for all people, purposes, or operating conditions. Although most DXers enjoy mixing up their use of operating modes, there are some who prefer to operate only on a single mode. Others find this too limiting since, depending upon circumstances, it often happens that one mode is more productive in making a DX contact than others. For example, if a DX station only operates with a single mode, you may not be able to make a contact if that particular mode is not available to you. For that reason, it is useful to be proficient in the use of - and have the ability to operate - as many of the modes that are available. For the purpose of chasing DX, all of the available modes are useful at one time or another and, the fact is, that most of the truly serious DXers use them all. Indeed, many have had great success with all three of the modes for which the DXCC award is now offered (CW, Phone, RTTY/Digital), achieving DXCC Honor Roll awards for all three. But the over-riding consideration is, as with any hobby, you should choose to do that which you enjoy the most. Since it should be the enjoyment that counts, you should use whatever mode or modes that you like.
Let's take look at the currently most popular modes used in DXing. In decreasing order of current users among DXers, the modes are:
SSB - Single Side-Band telephony is today, by far, the most frequently used mode on the bands, and may well be considered the universal mode. Its popularity undoubtedly derives from the fact that its use is intuitive, as voice communication is learned from birth, so telephony is easy to use, requiring no additional effort at learning a new skill - you just talk! Unlike the older telephony modes of AM and FM that require up as much as 6 KHz of bandwidth, SSB uses 3KHz or less. Those who remember the days before SSB can tell you how much of a significant improvement in communications capability it provided over AM phone. The lack of a base carrier and elimination of one of the sidebands meant that more of the output power was usable for signal information output as compared to AM. SSB signals were much more reliable, especially at lower power output, than the former telephony modes. The combination of narrow bandwidth and power efficiency means that under severe conditions, SSB can be intelligible within as narrow a bandwith as 1.2 KHz, and this means everything to a DXer! Also, since SSB output is proportional to modulation (see Equipment chapter), speech compression is an extremely useful DXing aide. Most SSB transceivers have selectable, adjustable speech compressors built in. DXers should take full advantage of this useful signal enhancement technique by following the manufacturers' recommended settings for speech compression. Always solicit over-the-air critiques of your compressed audio signal from others, especially DXers, as it will not necessarily sound "normal" to someone who is interested only in audio quality. As long as you're not distorted, or splattering your signal beyond the normal 2-3 KHz bandwidth, don't be disturbed by comments from non-DXers that " ... you don't sound normal ...". Of course, for casual contacts, you may want to switch off the speech compressor.
CW - After SSB, the next most popular mode on the bands is Continuous Wave (CW) as we hams call it, but more widely known by the encoding schema used: International Morse code. CW is a term that is a throwback to the early days in which this newer method of generating a constant (continuous) RF signal at a single frequency was distinguished from the spark-gap method that was essentially a ragged sequence of rising and decaying broadband RF noise. Interestingly (and unknown to most), CW was actually the first digital mode used by hams, since it a binary (ON/OFF) encoding scheme for information exchange. Compared to SSB, CW uses even less of the spectrum, needing at most a few hundred Hertz. In fact, CW signals are copiable in a filter bandwidth of as little as 50Hz, allowing one enjoy a greatly improved signal-to-noise ratio (Ever since I was able to afford one of the transceivers that employed DSP within the IF chain, I have used a 50 Hz bandwidth for all of my CW DXing - quite a change from the 4 KHz bandwidth of my S-38C!).
With rare exceptions, almost all DX stations will, at some time or another, operate CW. This is good news for DXers, especially those with modest stations, because a good operator can often copy a weaker station on CW than on SSB, especially under adverse interference conditions. DX station operators are usually excellent CW operators and when using split, they are quite capable of picking up even a very weak station that is calling from a clear frequency. That is why most successful DXers operate CW, knowing that there is often a better chance of working a DX station on CW than on SSB, especially when competing with the Big Guns. For this reason, it is definitely worth the effort to learn how to use CW. Since all transceivers today offer CW output along with SSB, all that is needed to operate this mode is a key and a bit of skill (you DID pass the code test, didn't you? ). The fact that DX station operators, like contest operators, generally send at a high rate of speed may scare off some DXers who don't feel that their CW ability is up to the task. Should you feel this way, my advice is not to give up because all you really need to be able to do is reliably copy your callsign, and most can recognize their own callsign even at very high speed. Since a DX contact only requires the exchange of a callsign and signal report, and since all pile-up reports are "599", if you can copy your callsign you can work the DX on CW. Your sending speed is not an issue - send at whatever speed is comfortable for you. Just get in there and do it! Which brings up another option for CW operation: with the appropriate software, one can interface the transceiver to the soundcard of a PC and use the PC keyboard to send CW at any rate of speed desired (see References). Some of the programs will also decode received CW; however, the software generally lacks the ability to copy well under adverse conditions. Note that software packages that provide a transceiver-PC interface for using the soundcard to code/decode digital modes can generally do more than one mode, if not all (CW, RTTY, PSK, etc).
The fact that CW is less popular than SSB among the ham population at-large should not be misinterpreted to mean that competition will be less among DXers. Anyone who believes that has never been in a CW pileup! Be assured that in a pileup for a moderately rare DX station, it will seem as if the whole world is there - and it is worse for the very rare ones!
RTTY - Next on the list of popularity among DXers is Radio TeleType, or RTTY. It is a relatively narrow bandwidth (300 Hz) digital mode that transmits keyboard-typed text encoded in the Baudot code, a 5-bit code devised in the late 1800s and used to develop wireline teletype communications. RTTY offers the advantages of both SSB (intuitive) and CW (narrow bandwidth). At the same time, since its user base is the least among the modes, it does offer a somewhat less competitive field of play for DXing. That alone makes it worthy of prime consideration! The only disadvantage of RTTY is that it usually requires additional equipment. In the old days before computers, large, heavy, pedestal-mounted teletypewriter devices (more akin to machinery than electronics!) were used to generate and receive (print on paper) RTTY signals. With the advent of the early computer chips, teletypewriters were replaced by a relatively small device called a Terminal Node Controller (TNC) for encoding/decoding, a terminal (monitor) for print display, and interface connections between the devices and the radio. In recent years, as computers with sound-processing capability became widely available, software was developed to allow the computer to replace the TNC, interfacing directly to the transceiver. While there may be extra costs and effort needed to implement RTTY, it is certainly not a foreboding obstacle. In fact, many stations today already have a computer. Free RTTY software is available for download from the Internet (see References). Rig-to-PC interfaces that isolate any stray RF from the PC are available commercially from $50 - $300), or can be readily built with low cost parts.
One popular and freely downloadable software program that is widely used is called MMTTY, developed by Mako, JE3HHT and available on his website at mmhamsoft.amateur-radio.ca/. With this program (and many others), one can set up "macros", activated at the click of a button, that will automatically send information. For example, a typical macro may send the following information:
%c DE %m
OK TNX %n UR %r %r
NAME IS DON ... DON
QTH IS RIVER RIDGE, LA ... RIVER RIDGE, LA
BTU %n
%c DE %m KK
This is a macro that I use in MMTTY, where "%c", "%n", and "%r" are the respective values for the called station's callsign, the called operator's name, and the signal report. The variable values are typed into appropriate windows on the screen, as may be seen in the examples below. The figure shows a screen-shot of a RTTY session "printing" of Ed, D2PFN from Luanda, Angola calling "CQ NA". (Ed developed his RTTY interest while operating as P5/4L4FN from Pyongyang, DPRK). Note the error in the first line where "D" was decoded instead of "DE", and in the third line where the callsign was decoded as "D2PKN". These are typical of decode errors due to fading or interference when printing DX signals.
Some seem to believe that RTTY requires high-power for reliable contacts, but this is really not true. RTTY reliability compares well with that of CW. For example, in the above screen-shot, print copy of D2PFN was better than 98%, despite the fact that Ed was operating "barefoot" and using (I believe) a Butternut multiband vertical antenna. Even under extremely poor conditions, RTTY operators can usually complete exchanges of contact information (callsign and RST) with as little as 40-50% error-free printing. An example of this can be seen in the figure below of 3C0M working RTTY on 20m, with plenty of print errors but still enough information content to complete a contact (Clicking on the image requires Shockwave Flash player for video display).
The MMTTY software provides highly automated RTTY operation. Clicking on the callsign in the Rx window automatically causes it to appear in the "call box", ready for making a call using a macro button, and the same can be done for the operator's name if it appears on the screen. If desired, upon completion of the QSO, a button-click will log the contact.
Notice in the RTTY screen-shots that all the letters are capitalized. Baudot code provides encoding for capital letters only. In general, binary coding schema can be used to represent up to 2-nth power characters. In this case, 2 raised to the 5th power is 32, so coding of the 26-character alphabet is possible, and upper-case was chosen (probably because telegraphers traditionally wrote telegrams in caps). Since the null-code (00000) is unused. the remaining 5 binary 5-bit codes are used for control characters (carriage-return, line-feed, space, and two "shift" character controls). By preceding a character code with a "shift" code (as on a standard keyboard), it is then possible to "re-use" the 26 alpha-codes to also encode the numbers 0-9, along with the commonly used symbols that appear on standard keyboards ( period, comma, etc).
There are two ways in which RTTY can be transmitted: either by using Frequency Shift Keying (FSK), or by using Audio Frequency Shift Keying (AFSK). The difference between these two is very simple to understand. FSK mode may be thought of as a form of CW in which the key is not only closed and opened, generating a "tone" at the desired HF, but may also be done at second frequency spaced 170 KHz higher. The first (lower) frequency is the "Mark" tone and the second (higher) frequency is the "space" tone. Because it is essentially a form of CW, it is possible to improve selectivity for RTTY reception by making use of the narrow filters typically available for CW. On the other hand, in AFSK mode, the Mark/Space tones are generated at audio frequencies and then transmitted as a SSB signal (by convention, using LSB). While the Mark/Space separation of the audio tones is the same (170 Hz), the AFSK signal is received in SSB mode where usually only wide filters are available, in which case selectivity is not as good as for FSK. Another important difference between FSK and AFSK is that on the receiver end, the reception tuning bandwidth for FSK is centered on the actual transmit frequency, while in AFSK, the transmit frequency is centered on the LSB signal that is 2.4 KHz below the transmit (zero-beat) frequency. To illustrate, if one reports ("spots") the frequency of an AFSK signal on a DX cluster as 14085.0 MHz, then in order for someone tuning in FSK mode to be able to hear it, they will have to tune their receiver to 14083.6, since the LSB signal tones are 2.4 KHz below the actual transmit zero-beat frequency. In other words, FSK (MHz) = AFSK (MHz) - 2.4 KHz. Which is best? Most serious RTTY DXers prefer FSK because of the selectivity issues; however, with the great improvements in DSP filtering now widely available for any mode of operation, selectivity may be less of an issue. One note about AFSK and FSK: RTTY spots posted on the DXCluster should ALWAYS indicate whether the spotter is using AFSK or FSK in order to allow others to tune to the correct frequency. It is frustrating to look for a DX station spotted at 14085.0 and then have to tune around to finally find them 2.4 KHZ lower at 14082.6 or higher at 14087.4!
One last thing to know about RTTY is that it can happen (and frequently does!) that the Mark/Space tones may be received in reverse. This can be duse to an error on the transmitter end (the tones are transmitted in reverse due to an incorrect connection or menu setting at the transmitter), or on the receiver end (incorrect receiver-TNC or PC sound card connection/setting). This becomes apparent when, despite careful tuning, only garbled print is received. All RTTY software, TNC or PC based, allows selection of "Reverse mode" reception for this purpose, and reversing the tone-decode process at the received end will allow proper printing. If it should happen that you are told that you are transmitting RTTY "in reverse" (or "upside down"), you should immediately look into correcting the problem. For FSK, first check your transmitter options for RTTY and, if available, reverse the Mark/Space polarity. If the option is not available or you're using AFSK, then swap the signal wires connecting your radio to the TNC or PC sound card.
See some of the links below for more information on getting started with this great mode. An especially good website is the one provided by Don, AA5AU, for all that you need to know about RTTY.
PSK31 - More properly, BPSK31, Binary Phase Shift Keying at 31.25 Hz is one of the most efficient HF modes currently available and has grown in popularity to the point where it has greatly surpassed RTTY in prevalence on the bands and may become the digital mode of choice for DXers. More detailed information sources can readily be found on the Internet and some are listed below. Using a variable length binary digital encoding scheme called Varicode, it offers the use of a fully complete character set with both upper- and lower-case. Further, the code is optimized to provide the least amount of code-level changes for the most frequently used characters, thereby minimizing dropped bits without the use of cumbersome error correction methods An alternate form, QPSK , provides error correction, but at the expense of significant reduction (3db) in signal-to-noise ratio, thereby rendering it less useful than PSK31 for DXing. Because of its extremely narrow bandwidth (31 Hz), PSK31 offers excellent signal-to-noise ratio to the extent that many have reported solid printing for signals that were almost imperceptible to the ear. The usual output power level is less than 50 watts (more power can cause obnoxiously severe splattering). A screen image of a PSK31 QSO between Serge, UA0FO and the author, using one of the free PSK software packages, DigiPan ("Digital Panoramic Tuning "by KH6TY, UT2DZ, & UU9IDR; www.digipan.net/download/) is shown in the figure below (Clicking on the image requires Shockwave Flash player for video display).
A few things to note in the figure (showing DigiPan v. 1.6d):
  • In addition to the macro buttons, there are three windows: Rx#1 (top), Rx#2 (below #1), Tx (small, below #2), and Waterfall (bottom).
  • Bothe upper- and lower-case characters are seen; in fact the Varicode encoding schema supports the entire set of ASCII characters & symbols.
  • PSK31 band segments are as wide as a receiver SSB passband (3 KHz wide; shown above is 14.070 - 14.073)
  • A PSK31 signal is a 31Hz-wide set of audio tones generated somewhere within the 3 KHz passband and seen as a bright line "flowing" down the waterfall display.
  • Tx frequency selection is done by placing the mouse curser at some spot in the waterfall display and left-clicking (red diamond w/green flag in figure).
  • On the Rx end, one can look at the waterfall and see all signals currently being received within the passband; placing the cursor on a signal and left-clicking will allow print to begin.
  • While printing a signal in Rx#1, a second signal may be printed simultaneously in Rx#2 by placing the cursor on it and right-clicking the mouse (blue triangle in figure).

Because of its superior qualities (low power, narrow bandwidth, excellent signal-to-noise ratio), many stations all over the world now operate in PSK31 mode, offering many opportunities to "work a new one" with modest equipment and antennas.

Other Modes

Of course, there are a number of other modes that may also be used, such as PSK63, FM, SSTV, and MFSK to name a few. However, these are all less frequently used for DXing due to (1) the lower number of overall users; and (2) the fact that they are somewhat less efficient. 


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