What determines which frequency to use?
The ionized part of the Earth’s atmosphere is known as the ionosphere. Ultraviolet light from the sun collides with atoms in this region knocking electrons loose. This creates ions, or atoms with missing electrons. This is what gives the Ionosphere its name and it is the free electrons that cause the reflection and absorption of radio waves.
https://sciencestruck.com/ionosphere-facts
Sun’s UV light collides with atoms knocking electrons loose:
Free electrons cause reflection and absorption of radio waves.
Interesting facts about the Ionosphere:
Think about visualizing water waves, then consider how we know light behaves too – to help understand these behaviours.
Ground Wave Propagation:
The strength of the groundwave is inversely proportional to frequency, being strongest at low frequencies. As frequency is increased, the distance covered by the groundwave decreases.
A ground wave is considered to have 2 components: a surface wave (travels entirely along the earth’s surface) and a space wave.
Sky Wave Propagation:
The Ionosphere reflects the electromagnetic waves, this zigzag pattern will vary depending on the atmosphere.
Reflects off the Ionosphere, e.g. HF Radio.
The Ionosphere reflects the electromagnetic waves, this zigzag pattern will vary depending on the atmosphere.
For HF radios note the reception created by where the wave is meeting the ground. There are areas of no reception for HF radios, yet at greater distances from the source, the reception improves again. This is normal for HF radios.
Space Wave (Line of Sight) Propagation:
E.g. VHF Radio & Mobile Phones.
While the distance between towers is not so relevant, it is more relevant to consider how far from the VHF transmitter we can operate.
D and R calculate the distance between towers for effective communication
To work out the exact distance a VHF signal will travel, you can use the following equation:
So, with an aircraft at 36,000 feet and the ATC radio tower at 100 feet, communication will be possible up to 250 nautical miles away. However, this is the theoretical optimum and will be much less in practice due to transmitter power and receiver inefficiencies.
Ionosphere affects HF Radio:
During the day, energy from the sun causes the D, E and F layers to become heavily ionized, making the layer more active. At night, with less energy from the sun, only the E and F layers are active. As a result, lower frequencies are better quality during the night and higher frequencies are better during the day.
However, what HF gains in distance, it loses in quality. Quite often, the quality of the signal is so poor that it’s impossible for either station to hear each other.
Terrain – VHF Radio:
Just like your mobile phone if there is terrain between you and the transmitting tower, you will not be able to send and receive messages via your VHF radio.
Sunspot activity – HF Radio:
The level of sunspot activity has an enormous effect on the ionosphere and hence on HF radio propagation conditions.
These sunspots are areas where there is intense magnetic activity.
Around the sunspot there is an area called a plage. This is slightly brighter than the surrounding area and it is a large radiator of cosmic rays, ultra-violet light and X-rays. In fact it results in the overall level of radiation coming from the sun to increase. In turn this increased radiation level from around the sunspots causes the ionosphere to become ionised to a greater extent. This means that higher frequencies can be reflected from the ionosphere.
The higher the levels of radiation received from the Sun, the greater the levels of ionisation in the ionosphere and in general this brings better propagation conditions for HF radio communications.
It is found that over a period of approximately eleven years over which the sunspots vary. At the peak of this cycle conditions on the bands at the top of the short wave spectrum are very good. Low power stations can be heard over remarkably long distances. At the bottom of the cycle bands around 30 MHz will not usually support normal propagation via the ionosphere.
Thunderstorms and Atmospheric Static – HF & VHF:
What is thunderstorms and atmospheric static, and what it means for radio:
Atmospheric noise, caused by lightning discharges in thunderstorms, is normally the major contributor to radio noise in the HF band:
Lightning scattering has sometimes been observed on VHF and UHF over distances of about 500 km. The hot lightning channel scatters radio-waves for a fraction of a second. The RF noise burst from the lightning makes the initial part of the open channel unusable and the ionization disappears quickly because of recombination at low altitude and high atmospheric pressure. Although the hot lightning channel is briefly observable with microwave radar, no practical use for this mode has been found in communications.
Static/noise also occurs from other Atmospheric Static sources:
Installation of Static Dischargers or Wicks:
Static dischargers, or wicks, are installed on aircraft to reduce radio receiver interference.
Static dischargers are normally mounted on the trailing edges of the control surfaces, wing tips and the vertical stabilizer. They discharge precipitation static at points a critical distance away from avionics antennas where there is little or no coupling of the static to cause interference or noise.
Interference from electrical equipment – HF & VHF:
Just like your car radio receives interference from electronic devices, so does your Avionics Radio – HF & lower frequencies most affected.
Any other device creating an electromagnetic wave could create interference:
Attenuation is the reduction of signal strength.
This can be caused by: