There’s a lot to amateur radio. It’s not essential that radio amateurs understand all the core radio communications concepts – but it helps!
The Fresnel zone is important in radio propagation because any path obstruction that impinges the First Fresnel zone causes obstruction loss. Most paths between amateur radio stations are heavily obstructed (unless both are on hilltops) but it doesn’t do to tolerate avoidable loss. Make sure that your foreground is as clear as you can make it at all azimuths round your station. Often the single variable here is antenna height. Here’s an analysis and explanation.
When one radio amateur sends a signal to another, there’s a chance that the signal will be received above the threshold of reception. If the signal received is indeed above the threshold of reception, an exchange of voice or data messages may be possible. Chance governs communication between amateur stations. Many amateurs embrace this, and chance gives the well-established concept of ‘DX’. Read why chance is so significant to radio amateurs.
The system value is the maximum loss between the transmitter output and the receiver input for a given response in the receiver. The system value is a fixed value for that system technology (comprising modulation and coding). There are differing system values for narrow band FM voice, SSB and each narrow band data mode such as FT8. Here’s how it’s calculated.
A path budget is as it implies – a currency pot in decibels that you as radio amateur can ‘spend’ in communicating with others. It’s not quoted in monetary terms – though some might argue that the bigger your purse, the greater the path budget and resulting DX. But that’s another story. The path budget guides the way you choose to spend your system value, and the benefit you get as a result of choices you make. Here’s how it’s calculated.
There’s huge ambiguity across the radio amateur books, magazines, and sites when it comes to describing how it is that the ionosphere returns radio waves to Earth. The ambiguity is this. Many writers routinely talk of reflection. Others call it scattering. And some refer to the mechanism as refraction. So, which is it? Here’s an argument and conclusion.
Hams routinely identify skywave propagation, and, to a much lesser extent, talk of space wave and ground wave. But how do these modes come about? It’s to do with the launch angle of the antenna in use and the frequency of operation. Generally, ground wave is used for LF and MF propagation, sky wave is used for HF communications and space wave is for VHF, UHF, SHF and above. Here’s a description and summary.
Radio hams frequently jump to conclusions about propagation modes. It’s no surprise. Propagation is complex and a little knowledge can lead to assumptions. This page attempts to give a logic to understanding how far signals can go for a given frequency, time of day and station characteristics. It aims to describe propagation modes, and in so doing, give understanding of propagation range limits. Read about propagation modes.
There’s the direct path assuming free space transmission. Paths between radio amateur stations are typically attenuated hugely by diffraction loss (discussed in another blog), with huge diffraction contribution from the Earth’s bulge protruding into the path. And then there are all the reflected paths from buildings, atmospheric layers, aircraft and frankly everything and anything in the vicinity of, and mid-way between, both stations. The result is fading.
The threshold of reception is.. well, just that. It’s the input to a receiver required to just produce the required communication result. The receiver threshold forms one of the two parameters to calculate the System Value. The other is the power output from the corresponding transmitter. The System Value is the total loss permissible between transmitter output and receiver input. Click for more on receiver threshold.
Radio amateurs are interested in the signal to noise ratio of received signals. To include electrical noise (from the various system components including antenna array, low noise amplifier and feeder) we need to be able to calculate the threshold degradation. This is explained here using a cascade approach to reveal the system noise figure and deduce how the sensitivity changes.