ANTENNA HANDBOOK (PART 1).
Edited by Radio Canada International , Montreal, Canada. 1988.
As a shortwave listener you would no doubt prefer to hear every distant broadcast with the clarity and fidelity of your local AM radio. Given the number and variety of obstacles that confront a radio signal on its path between broadoaster and listener, that is unlikely to happen. However, you can take many steps to improve reception. Some steps may be as easy as changing frequencies or listening times, or the location of your receiver. Others are more complicated, such as building an antenna.
Most of this handbook is devoted to antenna use and construction, but it also includes information about basic radio principles. Whether your shortwave receiver is an economical portable or an expensive tabletop, we trust Radio Canada International's Antenna Handbook will increase your knowledge and enjoyment of shortwave broadcasting.
HOW RADIO WAVES TRAVEL
An antenna is a conductor capable of radiating or receiving energy. A transmitter convert electric energy into electromagnetic (radio) waves that are radiated outward by the antenna at the speed of light (approx. 300,000,000 metres per second or 186,000 miles per second). A receiving antenna converts these radio waves into electric energy which is interpreted by the electronic circuits in your receiver and transformed again into voices and music.
Wavelength and Frequency
The terms wavelength and frequency are used interchangeably to denote the presence of radio energy in some part or at some point in the Radio Frequency Spectrum: they are different units of measurement closely related to each other Let's start with wavelength. Although all radio waves travel at the speed of light, they vary in length from fractions of a centimetre to thousands of metres. The wavelength of a shortwave frequency is expressed in metres.
Frequency is the number of cycles (or waves) per second emitted by an antenna (See Figure 1). Cycles per second is abbreviated to Hertz (in honour of Heinrich Rudolf Hertz, the german physicist who discovered electromagnetic waves in 1888). One thousand cycles per second is therefore expressed as one kilohertz (kHz) and one million cycles per second is one megahertz (MHz).
The relationship of the speed of a radio wave, its frequency and its wavelength is expressed mathematically in the following equation:
wavelength = speed
The speed of light is a constant (300,000,000 metres per second). Wavelength and frequency are variables; if we know one, we can determine the other suppose we wish to determine the wavelength of a radio signal whose frequency is 15,325 kHz.
Wavelength = 300,000,000 metres / sec = 19.58 metres
This frequency is located in the 19 metre band. Bands are discussed below.
As frequency increases, wavelength decreases. Shortwave broadcasting is often referred to as high frequency broadcasting.
By international agreement a certain number of distinct "bands" of frequencies within the radio spectrum have been allocated for use by shortwave broadcast stations. These are located roughly between 2,000 and 30,000 kilohertz or 120 and 11 metres (See Table 1).
Types of Radio Waves
Radio waves are emitted from an antenna in all directions, expanding outward similar to water ripples spreading out on the surface of a pond into which a stone has been thrown. While the rippled water metaphor helps us visualize how waves are propagated through space, the actual field pattern of a wave radiated from a vertical antenna more closely resembles a huge doughnut lying on the ground with the antenna in the hole at the centre. (See Figure 2).
Part of the wave moves outward in contact with the ground to form a ground wave. The rest of the wave moves upward and outward to form a sky wave.
Shortwave transmissions are achieved by means of sky waves which broadcasters concentrate and direct at a region high in the earth's atmosphere called the ionosphere.
The ionosphere that encircles the earth 50 to 400 kilometres above the surface differs from the surrounding atmosphere in that it contains a much higher number of charged particles (positive and negative ions).
The ionosphere acts as a conductor, absorbing energy in varying amounts from the radio wave. But, more importantly, it also acts as a radio mirror, gradually refracting the sky wave back to earth. The effectiveness of this ionospheric mirror depends upon the angle at which it is struck by the sky wave, the frequency of the signal, and the ion density.
A sky wave, after it has been refracted by the ionosphere can be reflected by the earth and directed toward
the ionosphere once again. Each complete path - from earth to ionosphere and back to earth is called a "hop".
It's because of this multi-hop ability that shortwave radio signals are able to span continents and oceans with
only moderate power. (See Figure 3). Because the ionosphere is produced mainly by ultraviolet radiation emitted
by the Sun, the amount of ionization varies with changes in solar radiation: it changes hourly, between day and
night, seasonally, geographically, and over an 11-year solar cycle.
If broadcasters were to change frequencies and target areas without consultation and mutual agreement, the result would be chaos. Instead, regular international notification procedures give all broadcasters a fair chance of reaching their chosen audiences at the desired times.
There are a number of generalizations surrounding the propagation of radio waves. For example: higher frequency signals travel best during the day and lower frequency signals travel best during the night. Therefore, if a broadcaster offers you a choice of frequencies during a night transmission, you should tune the lowest frequency first. Like all generalizations, this is correct...most of the time. But shortwave broadcasting is full of exceptions that prove the rule. In fact, you may have to change frequencies during a single transmission to maintain optimum reception. And there will be occasions, such as during high solar activity, when reception will be unavoidably bad.
HOW EXTERNAL ANTENNAS IMPROVE RECEPTION
If you have a tabletop receiver, you have no choice in the matter: you must erect an external antenna and connect it to the receiver via the antenna jack. If you have a small - or medium - sized portable receiver, you have a choice: to operate with the built-in whip antenna, or erect an external antenna. In the latter case, the big question is: will installing an externall antenna improve reception? In most cases, yes, but unfortunately there's no absolute answer.
A shortvtrave radio capable of receiving weak signals over long distances is described as "sensitive". Most transistor portable receivers are designed for optimum sensitivity using the built-in whip antenna. Under normal reception conditions, therefore, the equipment should provide enjoyable listening. Poor reception can often be improved simply by placing the radio near a window or an exterior wall. However, it reception is only sporadically good, or you wish to expand the range of frequencies available to you, or you wish to capture a station that has thus far eluded your receiver, an external antenna is the only solution.
It's often thought that the main reason for erecting an external antenna is to increase signal strength. In fact, signal strength may already be adequate; the real problem is usually local electrical noise of various kinds. The main adventage of an external antenna is that it increases signal strength relative to noise interference by removing the reception point away from the source of electrical noise. The higher the signal-to-noise ratio, the higher the listening pleasure.
The reception of shortwave stations indoors is subjed to interference from a variety of sources: fluorescent light fixtures, light dimmers, TV sets, microwave ovans, home computers, thermostats, electric motors, heating pads, etc. When a receiver and its built-in antenna are close to any of these noise generators, reception is likely to suffer.
lndoor reception can also be hindered by construction materials in the building itself. This is espacially true of aparment buildings which have a lot of metal in their walls, floors and ceilings. This metal acts like a shield, reducing the strength of radio signals reaching the antenna - or even eliminating them completely. The goal, then, is to place the antenna as far away as possible from noise sources and metallic shields.
There are a few simple rules which govern the installation, materials and performance of almost any receiving antenna.
While a lightning arrestor can protect an older receiver equipped with vacuum tubes, it is inadequate for a transistor receiver which can be damaged by even the small amounts of static electricity which accumulate on an external antenna (even when no electrical storm is underway). Transistor receivers require a static arrestor which slowly and continuously discharges accumulated electricity. As a final precaution, always disconnect your antenna during storms or when you plan to be away from home for long periods.
The performance and installation characteristics of antennas may be categorized in several ways. The most important are directivity and impedance.
While hardly robust enough for permanent installation, such kits are fine for experimentation at home or temporary installation while on a business trip or vacation. A horizontal antenna can be arranged on a balcony; a vertical antenna can be suspended from a window and held motionless by a weight at the bottom.
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