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    Foundations of Amateur Radio

    Starting in the wonderful hobby of Amateur or HAM Radio can be daunting and challenging but can be very rewarding. Every week I look at a different aspect of the hobby, how you might fit in and get the very best from the 1000 hobbies that Amateur Radio represents. Note that this podcast started in 2011 as “What use is an F-call?“.

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    Copyright: ℗ & © 2015 - 2020 Onno Benschop

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    Latest Episodes:
    The antenna system Apr 16, 2023
    Show notes

    Foundations of Amateur Radio

    Several years ago I participated in a local contest. Over a 24 hour period I activated my mobile station in about 30 different locations. On my car, my vertical antenna screwed into a boot-lip mount connected to an antenna tuner or ATU, and my radio. I used rope to guy the antenna, threaded through the rear windows and held tight by closing the car boot.

    Setting up consisted of parking the car, triggering the ATU to tune the antenna system and calling CQ. Moving to the next location consisted of driving there and setting up again.

    Although this worked really well, I'm skipping over what I'm interested in exploring today.

    The phrase "triggering the ATU to tune the antenna system" hides a lot of complexity. It was a surprise to me that there were several locations where the ATU just wouldn't tune. Despite my best efforts I was unable to get the system to a point where the radio was happy. In some cases I tuned off frequency and put up with a poor SWR. In others I physically had to move the car and park somewhere else.

    In every case it was completely unknown if a particular location was going to be a problem. I recall for example parking in an empty nondescript car-park and having to drive around to find a location where my set-up would work. Afterwards I considered that the car-park was potentially built on top of an iron ore deposit, an old industrial area, or a pipe-line, all of which were a good possibility.

    The point of this is that an antenna doesn't exist in isolation, it's called a system for a reason. We talk about the theoretical isotropic antenna and add disclaimers about that it cannot physically exist because it's infinitely small. One often overlooked aspect of an isotropic antenna is that it's in free space.

    Free space is defined as space that contains no electromagnetic or gravitational fields and used as a reference. It's a theoretical place. On Earth there is no such thing, there's a planet under your feet, but even in outer space there are both gravitational and electromagnetic fields that impact on an antenna and its performance.

    Staying nearer to home, recently we had a discussion about how close two antennas can be together. A suggested rule of thumb was that they need to be at least one banana or 30 cm away from each other.

    Similarly when we erect a dipole, there's recommendations around needing to have it mounted more than half a wavelength over the ground. Some sources say higher. I'll ask the first obvious question. Is that dipole completely straight? In other words, should the centre be half a wavelength above the ground, or should the ends, and how far should the ends be from their mounts?

    My point is that every antenna exists within the context of its environment and together it's a system. Some environments help the performance of your antenna system and some don't. Depending on frequency, this might not be the same for any location, or antenna design.

    To be clear, an antenna system consists of the antenna, the feed line and the clips that hold it, the tuner, the radio and its power supply, the mount and the space around it, the radials, the tower, the pigeon poop on the wire, all of it.

    Until recently my process to get any antenna to perform in a reasonable manner was to set it up, connect an antenna analyser, scan the appropriate range, tweak the antenna, scan again, rinse and repeat until it arrived at something approaching useful, or until it was good enough.

    If you recall, I recently added some loading coils to a telescopic antenna to attempt to make it resonant on 10m, so I could connect my Weak Signal Propagation Reporter or WSPR beacon to it directly and leave it running independently from my main station.

    I used the antenna analyser method, got it to the point where I had an antenna with a nice dip right at the required frequency and then watched it go completely sideways when I mounted the antenna in the window.

    Having spent several hours getting to that point, I walked away and left it for another day. Today was that day. I again started on the floor of my shack and got nothing but an infinite SWR and no amount of tweaking could fix it. Right until the coax fell out of the SMA connector I was scratching my head.

    After removing the faulty coax lead, I again tweaked the antenna and instead of using my antenna analyser, I fired up my NanoVNA, a tiny handheld open-hardware Vector Network Analyser or VNA. If you're not familiar, it's a standalone palm sized device with an LCD display and battery which will allow you to test most of your RF equipment. This little box came to me via a generous gift from a fellow amateur. It can repeatedly scan a range of frequencies and report in near real-time what's going on. Instead of waiting a minute after each adjustment, I could wait less than a second and immediately see the effect.

    This has been a game changer.

    I could mount the antenna against a metal surface and immediately see what the impact was. I could see the difference between it being mounted horizontally, where it would sag, to it being vertical where it stayed straight. I could see the steepness of the SWR plot, see how the low point moved around, up and down the band, see what the depth or lowest SWR was at any point. I could see my hand approaching the antenna, how nearby metal objects affect the antenna, what made it better and what made it worse.

    The reason that I'm talking about this is because it's the very first time that I was able to actually get a feel for what affects an antenna, in what way and by how much.

    To describe an analogy, it's like watching someone play a theremin and hearing how their hands affect the sound. If you're not familiar, a theremin is an electronic musical instrument controlled without physical contact by the performer, named after its inventor, Leon Theremin who patented it in 1928. From the outside it looks like a metal antenna that you bring your hands near to change the field. The changes are converted into sound.

    The NanoVNA gives you the same level of feedback, but does so visually in a quantitative way, providing you with the insight to adjust your antenna to your liking and taking into account its entire environment.

    Does this mean that I'm telling you to go out and buy one today? Well, that's not up to me, but I am intensely grateful for it arriving at my doorstep.

    I'm Onno VK6FLAB


    How much antenna is enough? Apr 09, 2023
    Show notes

    Foundations of Amateur Radio

    When you start in this hobby one of the most frustrating aspects is that of selecting the right antenna. If you've been around for a while, you'll discover that this continues to be the case, even when you've been licensed longer than I've been alive.

    In the past I've discussed at length why that is the case, but to recap, consider a dipole antenna. In essence it's two pieces of wire that are connected to the radio via some form of feed-line.

    Now consider the idea of changing the length of each wire. You could trim each end in the same way, or you could make one end longer than the other. You could fold the ends at an angle, or you could mount the dipole near the ground, or high up in the trees, you could position it vertically, or arrange the wires at an angle towards each other. You could make the wire thicker, or thinner, from different material or arrange the ends so they meet up in a circle, or a square, a triangle or some other shape.

    You get the point, there is endless variation arranging this single antenna and I've not even discussed things like feed-lines, traps, chokes, counterpoise and other RF shenanigans.

    With that in mind, amateurs around the world are attempting to improve their antenna system every time they get on air to make noise.

    Recently I reported that my 10 mW WSPR, or Weak Signal Propagation Reporter beacon was heard 13,455 km away in Sweden by Mats SM3LNM on the 10m band. The signal report was -25 dB, which means that with an experimental cut-off for a successful decode at -34 dB, I have 9 dB to play with, so at least theoretically, I could reduce my power even further, to 1 dBm, or just over 1 mW and still make the distance.

    The antenna I'm using is one built by Walter VK6BCP (SK). It's a 40m vertical antenna, helically wound on a fibreglass blank and clamped to the side of a metal pergola. The antenna is tuned to the 10m band using an SGC SG-237 antenna coupler, essentially a device that can add or remove inductance or capacitance to make my antenna appear resonant on the appropriate frequency. The antenna coupler in turn is attached to about 20 or 30 meters of 75 Ohm, quad shield RG6 which I have left over from my remote internet satellite dish installation days.

    That's all to say that the antenna system for my beacon is sub-optimal and it's likely that my actual power output is lower than the 10 mW that my beacon is reporting.

    So, with all that in mind, what else could I try?

    I have an indoor telescopic antenna stuck to the window and I've been wondering if I can attach my beacon to it directly and leave it running without the need to worry about disconnecting the beacon when I'm wanting to fire up my actual station to make other noises on air.

    A quick scan with the analyser reveals that the lowest frequency out of the box is about 60 MHz. I decided that adding some loading coils might help, so I set about fabricobbling an antenna, yes, you heard me, fabricobbling, fabricating and cobbling together.

    Anyway, using 7mm thick drip irrigation riser poly pipe as a form I wound two coils with 1.25mm copper wire that I had lying around. Depending on which calculator you used, that was either too much or not enough for my needs. I managed 53 windings, shy of the planned 60, but still a good start.

    Using the same irrigation riser, which as luck would have it managed to match the thread for the telescopic antenna elements and feed point, I separated each element by about 100 mm from the feed point, then used the two loading coils to connect the feed point back to each element. An hour later I now have a telescopic antenna, with two loading coils and as luck would have it, I'm much closer.

    The resonant point is now 30 MHz, down from 60 MHz, so I have a little more tinkering ahead of me. I might change the wire and use some eyelets at the ends to make assembly simpler, but the general idea seems to work as intended.

    If it doesn't work, I've come across a design for a 25.5 meter long End Fed Half Wave antenna that will work on anything between 80m and 10m and it appears that my driveway is just long enough to fit, but that will negate the indoor aspect of the antenna.

    All this reminds me of the ugliest dipole I ever saw, in a bush shack, a decade ago, consisting of two wires, haphazardly soldered onto a piece of coax, looped around an insulator, with a piece of wire holding it together, tied between two trees. It was only ever meant to be temporary, but it was there for years. I used it to speak to stations all over the pacific and in the process learnt a lot about the performance of both my radio and the antenna connected to it.

    The point being that experimentation in antenna building is what we're all about, even going backwards from multi-band, high gain antenna farms, back to basics and exploration.

    In case you're wondering, I haven't forgotten about the Hustler 6BTV antennas packed in boxes. They're still very much part of the grand plan, but in light of my recent low power experiments, I'm getting very curious about using antennas that really stretch the propagation friendship. Why? Because I can.

    What antennas have you built that you were ashamed of?

    I'm Onno VK6FLAB


    Lost in space ... Apr 02, 2023
    Show notes

    Foundations of Amateur Radio

    There is a fascination with space that arguably started long before the first time that human spaceflight was proposed by Scottish astronomer William Leitch in 1861. Names like Sputnik, Mercury, Gemini, Apollo and Columbia speak to millions of people and organisations like NASA, SpaceX and Blue Origin, to name a few, continue to feed that obsession.

    In amateur radio we have our own names, things like ARISS, or Amateur Radio on the International Space Station, or its predecessor SAREX, the Shuttle Amateur Radio Experiment.

    Today, stories about people making contact with the International Space Station continue to make news. We have school programs where amateur radio ground stations schedule a call to speak with an astronaut in space and we've been launching our own amateur satellites for a long time. Launched on the 12th of December 1961, OSCAR1, or Orbiting Satellites Carrying Amateur Radio was built by a group of California based amateur radio operators for 63 dollars. It operated for nearly 20 days, transmitting "Hi" in Morse on 144.983 MHz.

    The first amateur radio space voice contact was made on the 1st of December 1983, almost forty years ago.

    It's surprising that in the age of technology such a significant event has been so poorly recorded for posterity.

    If you go searching for the actual audio, you'll discover several versions of this contact including varying transcripts. I've attempted to reconstruct the wording, but I've yet to hear a complete and unedited version. For example, there's an ARRL movie called "Amateur Radio's Newest Frontier" with out of sync audio. There's also an audio file with a transcript from an archived copy of a website by W7APD. The most recent one is on a video called "HAM - Official Documentary 2022", produced by students from the School of Visual and Media Arts program at the University of Montana and broadcast on Montana PBS on November 24th, 2022.

    So, what follows is not necessarily complete, but calling from Space Shuttle Columbia it went a little like this:

    "..U.S. west coast and calling CQ. Calling CQ North America. This is W5LFL in Columbia. In another 30 seconds I'll be standing by. Our spacecraft is in a rotation at the moment and we're just now getting the antenna pointed down somewhat more toward the Earth. So I should be able to pick up your signals a little bit better in the next few minutes. So W5LFL in Columbia is calling CQ and standing by. Go ahead."

    "This is W5LFL in Colombia, W5LFL in Columbia, orbiting the Earth at an altitude of 135 Nautical Miles. Passing over the US West Coast and calling CQ. So W5LFL in Columbia is calling CQ and, ah, standing by. Go ahead."

    "W5LFL on STS-9, WA1JXN, WA1 Japan X-Ray Norway, WA1JXN, Frenchtown Montana, WA1JXN standing by."

    "Hello W1JXN, WA1 Juliet X-Ray November, this is W5LFL, I picked up your signals fairly weakly. I think our attitude is not really the best as yet, but you're our first contact from orbit. WA1 Juliet X-Ray November. How do you read? Over."

    On board STS-9, Space Shuttle Columbia, was Dr Owen Garriott, W5LFL, now silent key. On the ground was Lance Collister, then WA1JXN, now W7GJ.

    NASA published an Educational Brief for the Classroom that described Owen's set-up as a battery powered 5 Watt FM transceiver feeding a split-ring on a printed circuit board antenna that will be placed in the upper crew compartment window on the aft flight deck. Others reported that the radio was a Motorola handheld. Logging was done with a tape recorder velcroed to the transceiver.

    Owen describes the antenna as a "well-designed, hand-held antenna, known as a 'cavity antenna', which could be velcroed to the window. It was about 24 inches in diameter and looked somewhat like a large aluminum (sic) cake pan"

    There's an edited version of a similarly titled ARRL video called "Amateur Radio's Newest Frontier - ARRL documentary featuring Owen Garriot, W5LFL, on STS-9" showing the antenna as a copper tube, bent into a circle, mounted inside an open aluminium box that was hinged on the window to face outwards.

    The NASA brief also described a range of frequencies and designated 145.55 MHz as the primary frequency over the United States. It included a whole section about synchronising clocks using WWV in Fort Collins, Colorado, odd and even minute transmission schedules and descriptions on how this should work.

    Operating during time off, when the antenna was facing Earth, and being on air for about four hours during the mission, around 300 contacts were made across the globe.

    Today we continue to experiment in space. The callsign N1SS is heard on-air regularly from the International Space Station, astronauts are often licensed radio amateurs, there's a permanent repeater on the ISS, we launch research spacecraft called nano-satellites or more popularly CubeSats for amateur radio at every opportunity. So far there's over 160 satellites and the adventure continues.

    Speaking of experiments, albeit earthbound, the other day, my WSPR or Weak Signal Propagation Reporter beacon, using 10 milliwatts was heard 13,455 km away in Sweden, that's 1.3 Million kilometres per Watt.

    What have you been up to in Amateur Radio lately?

    I'm Onno VK6FLAB


    The Contester In Me... Mar 26, 2023
    Show notes

    Foundations of Amateur Radio

    So, I have a confession to make. I'm a contester. I'm not ashamed of this. While I'm in a confessing mood, I'll also mention that I've not participated in many contests in the past few years. This is not for the want of desire, but for the lack of motivation to fix things in my shack that are fundamentally broken.

    On the weekend I participated in a local contest. I took part for six hours, got on-air and made noise, made about 30 contacts, had a ball. I wasn't playing to win, though I did use the opportunity to refresh and hone some of my rusty skills.

    The next day I spent much too long converting my log into something that the contest organiser asked for. I also discovered that there was a duplicate entry in my log, not something which I'd expect with only so few contacts, but a reflection on the tool I was using to create my log.

    I started writing down what I learnt from the experience, operating from my own shack, documenting what worked and what didn't.

    I commented on several things relevant to me, but to give you a flavour, my operator position is terrible because I'm logging on my main computer and the radio is side-on when I'm facing the computer. The sun was shining directly into my eyes when facing the computer. Holding a microphone I didn't have hands-free, I still don't have an auto-keyer to save my voice, my foot pedal didn't work and my data interface was on loan to another amateur.

    As I said, these things are specific to me.

    Logging was worse.

    It didn't quite bring me to tears, but as the contest went on, it became a problem. I started to write down what was wrong with the tool I was using with a view to submitting patches to fix it when I realised that it wasn't actually built as a contesting logging tool, so I stopped and instead started writing a new list, one that describes what a good contesting tool looks like. It builds on a decade of using different tools and participating in contests in all manner of different situations, from special portable event activations, through to the annual top-tier contests run from a purpose built contest station and everything in between.

    So, what does the ideal contesting tool look like, for me?

    It needs to be cross platform, as-in, I should be able to use it on whatever computer I have access to, my Linux workstation, a Macintosh Laptop, an Android phone or tablet and while I'm at it, Windows and iOS and I think it should be able to run on a Raspberry Pi. In other words, there shouldn't be a situation where you cannot run the tool because you have some random combination of operating system or CPU that the developer doesn't support.

    It must be open source. By that I mean, the code should be available to the entire community. There are too many stories of great tools dying or being held hostage by individuals or small groups. The tool should continue to exist and be usable regardless of the participation of the original developer. Users should be able to fix things, add functionality, change themes, whatever.

    You should be able to customise it because not every contest needs the same information. For example, the John Moyle Memorial Field Day, a contest run every year during March in Australia requires that VHF and UHF contacts record the maidenhead locator, a four or six character message that designates the location of the station. This is used to calculate distance between two stations and award points accordingly. Such a requirement isn't needed in most other contests.

    Some contests are considered friendly contests, like the Remembrance Day contest in August. It's common to exchange your name, details about your station and have a chat. You'd be unpopular if you used that approach for the Oceania DX, the CQ World Wide or the CQ WPX contests. In other words, some fields are expected for some contests, but not for others.

    The tool needs to be able to show if a contact is valid by whatever means the rules for a particular contest decide. It needs to automatically log the time, keep track of previous entries and know about the super check partial list to validate partial callsigns.

    The user needs to be able to use either a keyboard or mouse, or both, to do all the common contesting data entry. No dependency on crazy keyboard shortcuts, no requirement to click the mouse to make an entry, in other words, the tool needs to be able to get out of the way of the contester.

    I think it needs to have a plug-in system to accommodate different rules and it needs to be able to export data in whatever format the contest organiser expects.

    You should be able to use it without needing to be connected to the internet during the contest, it should be easy to update and have the ability to keep a station log for all the contacts ever made.

    It would be great if it could also import existing logs so you can start to consolidate older logs.

    Having spent quite some time looking for such a tool and failing, I've come to the conclusion that there's only one thing for it, I'm going to have to write my own tool and it would be great if you could help by sharing your opinion on the matter.

    At this point I'm looking for suggestions on what you think is needed for a great contesting tool. I realise that for some, pen and paper is sufficient, and I'm not trying to dissuade you from using that, I've used it myself on more than one occasion, rather, I'm asking if you can think of things that it should do out of the box, things that are basic functionality that you would like to see as part of the design.

    You can find the project on my vk6flab GitHub page, comment on Reddit, or you can drop me an email, cq@vk6flab.com.

    Look forward to hearing from you.

    I'm Onno VK6FLAB


    What's with a negative SNR? Mar 19, 2023
    Show notes

    Foundations of Amateur Radio

    We describe the relationship between the power of a wanted signal and unwanted noise as the signal to noise ratio or SNR. It's often expressed in decibels or dB which makes it possible to represent really big and really small numbers side-by-side, rather than using lots of leading and trailing zeros. For example one million is the same as 60 on a dB scale and one millionth, or 0.000001 is -60.

    One of the potentially more perplexing ideas in communication is the notion of a negative signal to noise ratio. Before I dig in how that works and how we can still communicate, I should point out that in general for communication to happen, there needs to be a way to distinguish unwanted noise from a desired signal and how that is achieved is where the magic happens.

    Let's look at a negative SNR, let's say -20 dB. What that means is that the ratio between the wanted signal and the unwanted noise is equivalent to 0.01, said differently, the signal is 100 times weaker than the noise. In other words, all that a negative SNR means is that the ratio between signal and noise is a fraction, as-in, more than zero, but less than one. It's simpler to say the SNR is -30 dB than saying the noise is 1000 times stronger than the signal.

    Numbers like this are not unusual. The Weak Signal Propagation Reporter or WSPR is often described as being able to work with an SNR of -29 dB, which indicates that the signal is about 800 times weaker than the noise.

    To see how this works behind the scenes, let's start with the idea of bandwidth.

    On a typical SSB amateur radio, voice takes up about 3000 Hz. For better readability, most radios filter out the lower and upper audio frequencies. For example, my Yaesu FT857d has a frequency response of 400 Hz to 2600 Hz for SSB, effectively keeping 2200 Hz of usable signal.

    Another way to say this is that the bandwidth of my voice is about 2200 Hz, when I'm using single side band. That bandwidth is how much of the radio spectrum is used to transmit a signal. For comparison, a typical RTTY or radio teletype signal has a bandwidth of about 270 Hz. A typical Morse Code signal is about 100 Hz and a WSPR signal is about 6 Hz.

    Before I continue, I should point out that the standard for measuring in amateur radio is 2500 Hz.

    This is significant because when you're comparing wide and narrow signals to each other you'll end up with some interesting results like negative signal to noise ratios. This happens because you can filter out the unwanted noise before you even start to decode the signal. That means that the signal stays the same, but the average noise reduces in comparison to the 2500 Hz standard.

    This adds up quickly. For a Morse Code signal, it means that turning on your 100 Hz filter, will feel like improving the signal to noise ratio by 14 dB, that's a 25 fold increase in your desired signal.

    Similarly, filtering the WSPR signal before you start decoding will give you roughly a 26 dB improvement before you even start.

    But there's more, since I started off with claiming that WSPR can operate with an SNR of -29 dB. I'll note that -29 dB is only one of the many figures quoted. I have described testing the WSPR decoder on my system and it finally failed at about -34 dB. Even with a 26 dB gain from filtering we're still deep into negative territory, so our signal is still much weaker than the noise.

    There are several phenomena that affect the decoding of a signal.

    To give you a sense, consider using a limited vocabulary, like say the phonetic alphabet, or a Morse character, the higher the chance of figuring out which letter you meant. This is why it's important that everyone uses the same alphabet and why there's a standard for it. To send a message, WSPR uses an alphabet of four characters, that is, four different tones or symbols.

    Another is how long you send a symbol. A Morse dit sent at 6 words per minute or WPM lasts two tenths of a second, but sent at 25 WPM lasts less than 5 hundredth of a second This is why WSPR uses two minutes, actually 110.6 seconds, to send 162 bits of data, lasting just under one and a half seconds each.

    If that's not enough, there's a processing gain. One of the fun things about signal processing is that when you combine two noise signals, they don't reinforce each other, but when you combine two actual signals, they do. Said in another way, signal adds coherently and noise adds incoherently.

    To explain that, imagine that you have an unknown signal and you pretended that it said VK6FLAB.

    If you combined the unknown signal with your first guess of VK6FLAB and you were right, the unknown signal would be reinforced by your guess. If it was wrong, it wouldn't. If your vocabulary is small, like say four symbols, you could try each in turn to see what was reinforced and what wasn't.

    There's plenty more, things like adding error correction so you can detect any potentially incorrect words. Think of it as a human understanding Bravo when the person at the other end said Baker.

    If you knew when to expect a signal, it would make it easier to decode, which is why a WSPR signal starts at one second into each even minute and each symbol contains information about when that signal was sent, which is why it's so important to set your computer clock accurately.

    Another is to shuffle the bits in your message in such a way that specific types of noise don't obscure your entire message. For example, if you had two symbols side-by-side that when combined represented the power level of your message, a brief burst of noise could obliterate the power level, but if they were stored in different parts of your message, you'd have a better chance of decoding the power level.

    I've only scratched the surface of this, but behind every seemingly simple WSPR message lies a whole host of signal processing magic that underlies much of the software defined radio world.

    These same techniques and plenty more are used in Wi-Fi communications, in your mobile phone, across fibre-optic links and the high speed serial cable connected to your computer.

    Who said that Amateur Radio stopped at the antenna connected to your radio?

    I'm Onno VK6FLAB


    Acronym not found ... Mar 12, 2023
    Show notes

    Foundations of Amateur Radio

    Our community is full of TLAs, or three letter acronyms. Some of them more useful than others. For example, I can tell you thank you for the QSO, I'm going QRT, QSY to my QTH. Or, thanks for the chat, I'll just shut up and take my bat and ball and go home.

    Acronyms arise every day and it came as no surprise to spot a new one in the wild the other day, SHF. It was in a serious forum, discussing antennas if I recall, so I didn't blink and looked it up. Super High Frequency. Okay, so, where's that?

    I'm familiar with VHF and UHF and as radio amateurs we're often found somewhere on HF, that's Very High Frequency, Ultra High Frequency and High Frequency if you're curious.

    Turns out that the ITU, the International Telecommunications Union has an official list, of course it does. The current ITU "Radio Regulations" is the 2020 edition. It's great bedtime reading. Volume one of four, Chapter one of ten, Article two of three, Section one of three, Provision 2.1 starts off with these words: "The radio spectrum shall be subdivided into nine frequency bands, which shall be designated by progressive whole numbers in accordance with the following table."

    When you look at this table you'll discover it starts with band number four and ends with band number twelve, between them covering 3 kHz to 3000 GHz. In position ten you'll see the designation "SHF", covering 3 to 30 GHz, centrimetric waves.

    A couple of things to note.

    The list starts at band four. There are of course frequencies below 3 kHz. The list ends at twelve, but there are frequencies above 3000 GHz. You'll also note that I'm not saying 3 Terahertz, since the ITU regulations specify that you shall express frequencies up to 3000 GHz using "gigahertz".

    Interestingly the same document has a provision for reporting interference where you can report using Terahertz frequencies, so I'm not sure how the ITU deals with such reports.

    Another thing to note is that this table doesn't actually define what SHF means. It's nowhere in the radio regulations either, I looked. I'm not sure where the words Super High Frequency came from. There is an ITU online database for looking up acronyms and terms. That leads to a document called "Nomenclature of the frequency and wavelength bands used in telecommunications", which also doesn't use "Super High Frequency" anywhere.

    That said, using the ITU band four, where its definition starts, the VLF band, or Very Low Frequency, followed by LF, Low Frequency, MF, Medium Frequency, the familiar HF or High Frequency, VHF, UHF, then SHF and beyond that, EHF, Extremely High Frequency and THF or Tremendously High Frequency, yes, Tremendously High.

    There's a report called the "Technical and operational characteristics and applications of the point-to-point fixed service applications operating in the frequency band 275-450 GHz". It introduces the term "THF which stands for tremendously high frequency" but adds the disclaimer that "this terminology is used only within this Report."

    Seems that there are plenty of documents on the ITU website using that same definition, so I'm guessing that the cat is out of the bag. THF by the way is defined as being for 300 to 3000 GHz frequencies.

    By the way, the ITU TLA finder exposes that THF stands for Topology Hiding Function. Where's a good acronym when you need it?

    Speaking of definitions, I came across the definition of a "taboo channel" which according to the ITU is "A channel which coincides with the frequency of the local oscillator in the single super heterodyne receiver which is tuned to an analogue channel."

    Anyway, we still have a way to go.

    Below band four, less than 3 kHz, we have ULF or Ultra Low Frequency, SLF, Super Low Frequency and ELF, Extremely Low Frequency, which is defined as band one, between 3 and 30 Hz. Below that, some have suggested TLF, or Tremendously Low Frequency which apparently goes between 1 and 3 Hz with a wavelength between 300,000 down to 100,000 km. Others have suggested that this is an internet meme, but so far it seems to me that it has just as much legitimacy as any of the other wordings, since it appears that the ITU explicitly excludes such definitions, even if internal documents introduce terms from time to time.

    It did make me wonder, what comes after Tremendously High Frequencies, Red?

    Turns out, yes, well, infra-red pretty much follows on from Tremendously High Frequencies.

    If you think that's the end of it, think again. The IEEE, the Institute of Electrical and Electronics Engineers has its own definitions, of course it does. Unfortunately they decided that you need to pay for their standard. It was first issued in 1976 "to remove the confusion". There's an xkcd comic called "Standards", number 927 if you're looking. It goes like this:

    Situation: There are 14 competing standards. 14?! Ridiculous! We need to develop one universal standard that covers everyone's use cases. Yeah! Soon: Situation: There are 15 competing standards.

    Anyway, the IEEE designates that after UHF comes L or Long wave, followed by S, or Short wave, then comes C, the compromise between Short wave and X or cross or Exotic. Then there's Ku, Kurtz Under, K, Kurtz, and Ka or Kurtz above, Kurtz being the German word for Short. There's the V band and the W band which follows the V band.

    Had enough yet?

    NATO, the EU and the US define these using letters of the alphabet.

    And broadcasters use Band Numbers which link up to nothing in particular.

    I wonder if the measure of a society is just how many different ways can be used to describe the same thing. Perhaps we should have stopped at Hertz or Hz, which was established in 1930 by the International Electrotechnical Commission, as an expression of the number of times that a repeated event occurs per second, in honour of Heinrich Hertz.

    One more three letter acronym, the International Electrotechnical Commission is better known as the IEC.

    I wonder if the ITU is taking suggestions, ginormous, utterly, inordinately, awfully and humongously seem like perfect opportunities for future expansion.

    I'm Onno VK6FLAB.


    Antenna Testing Day ... Mar 05, 2023
    Show notes

    Foundations of Amateur Radio

    Last week I went outside. I know, it was a shock to me too. The purpose of this adventure was to test an antenna that has been sitting in my garage for nearly a year. Together with a friend we researched our options and at the end of the process the Hustler 6BTV was the answer to our question. Before the commercial interest police come out of the woodwork, I'll point out that I'm not providing a review, good or bad, of this antenna, it was the antenna I purchased and went to test.

    Between the two of us we have three of these antennas. I have the idea to use one as a portable station antenna and another as my base station antenna. Glynn VK6PAW intends to use his as a base station antenna.

    To set the scene. The antennas came in quite large boxes, just over six bananas long, or more than 180 cm. When they arrived I opened my boxes and checked their content, then sealed it all up and put the boxes on a shelf. Last week Glynn proposed that we set one up and see what we could learn from the experience.

    You know that I love a good spreadsheet, so planning went into overdrive, well, I put together a list of the things we'd need, starting with the antenna and ending with sunscreen to protect my pasty skin from the fusion experiment in the sky. In between were things like an antenna analyser, spare batteries, tools, imperial, since apparently there are still parts of the world that haven't gone beyond barley measurements. I jest, they authorised the use of the metric system in 1866. My list also included a magnetic bowl to capture loose nuts and washers, you get the idea, anything you might need to test an antenna in the field.

    Our setup was on a rural property where we had lovely shady trees and oodles of space to extend out a 25m radial mat. We tested many different set-ups. I won't go through them all, but to give you an idea of scale, in the time we were there, we recorded forty different antenna frequency scans. The 6BTV antenna is suitable for 80m, 40m, 30m, 20m, 15m and 10m. We tested with and without radials, raised and on the ground and several other installations.

    We learnt several useful things. For starters, sitting on the ground with radials the antenna measurements line up pretty well with the specifications and with a suitable base mount to protect the plastic base the portable station antenna is usable out of the box.

    Any variation on this will result in change, sometimes subtle, sometimes less so. For example, we came up with one installation where the SWR never dropped below 3:1. That's with the antenna on the ground without any radials in case you're wondering.

    Other things we learnt were that manually scanning each band is painful. When we do this again we'll have to come up with a better way of measuring. The aim for my base antenna is to install it on my roof, bolted to a clamp on the side of my metal pergola. This means that we're going to have to do some serious tuning to make this work for us. It might turn out that we'll start with installing the antenna at Glynn's QTH first, but we haven't yet made that decision.

    Other things I learnt are that I had actually put together the base clamp when I checked the boxes a year ago, so that was a bonus. The magnetic bowl saved our hides once when a spring washer fell into the lawn. The hose-clamps that come with the antenna require a spanner, but there are thumb screw variations of those that I'll likely use for my portable setup.

    Other things we need to do is learn exactly how the traps work and how adjusting them affects things. In case you're unfamiliar with the concept of a trap, think of it as a radio signal switch that lets signals below a certain resonant frequency pass and blocks signals above that frequency. In other words, a 10m trap resonates just below 28 MHz. It lets frequencies below 28 MHz pass, but blocks those above it, essentially reducing the length of the antenna to the point where the trap is installed.

    One test we did was to only use the base and the 10m trap. We discovered that this doesn't really work and that the metal above the trap, as-in the rest of the antenna, isn't just for show, even though it's on the blocked side of the 10m trap.

    Given that I intend to use my base antenna as my main WSPR transmission point, I need to adjust things so the antenna works best on WSPR frequencies. I intend to use a tuner for when I want to work outside those frequencies.

    One unexpected lesson was that the awning that Glynn attached to his vehicle was an absolutely essential item. I don't think I'll ever go portable again without one. Life changing would be an understatement. I'm investigating if I can fit one to my vehicle.

    Having had some health issues over the past months I was anxious about going outside and being somewhat active. I paced myself, protected my back, took regular breaks, sat down a lot, drank litres of water and slept like a baby that night. No ill effects, very happy.

    As a bonus, I even transferred our measuring data to a spreadsheet.

    I can't wait to see the results of our next adventure.

    Oh, we did connect a radio. Heard a beacon in Israel, heard a QSO in Italy, listened to WWV on 10 MHz and almost missed the bliss of not having to tune or switch when moving from band to band.

    What have you been up to in the great outdoors?

    I'm Onno VK6FLAB


    Are all spiky antennas the same? Feb 26, 2023
    Show notes

    Foundations of Amateur Radio

    The world is filled with antennas. You'll find them on towers, buildings, cars and on your next door neighbour's roof. They come in an astonishing variety, to the point where you might start thinking that antennas are a fashion accessory that vary with the season and if you start digging through the history books you'll come across designs that dial that variety up to eleven.

    Possibly the most visible antenna today is the television antenna and when you start noticing them, the more variation you'll discover.

    Their basic shape consists of a vertical pole, the mast, with a horizontal pole, the boom. Attached to the boom are various different shapes, or elements, that often vary in length according to some pattern.

    The shape is designed to collect as much electromagnetic radiation from a particular direction, or in the case of a transmitter, focus as much energy as possible into one direction. This focus is called gain. The more focus, the more gain.

    One of the oldest designs for this kind of antenna, still in use today, is the Yagi-Uda or Yagi antenna. It was invented in 1923 by Shintaro Uda at the Tohoku Imperial University in Japan and popularised to the English speaking world by his boss Hidetsugu Yagi who claimed to be the sole inventor in his Japanese patent application. He went on to file similar patents in Germany and the United States.

    Gain for a Yagi varies depending on design. Generally more elements means more gain. Sometimes you'll see a Yagi with weird shorter elements along the boom. This is a design to make the antenna work across multiple frequencies. Another way that this can be achieved is by adding traps along an element. They look like a thick stubby tube at some distance along an element. You can have more than one of these to allow for more frequencies. These improvements allow for several Yagi antennas to share elements and boom space, essentially combining several independent antennas into one.

    It can be tricky to discover in which direction a Yagi is pointing, but essentially the boom indicates the direction and the end with the shortest element is the front.

    There's another type of antenna that to the casual observer looks similar. It's called a log periodic dipole array, LPDA or log periodic antenna. It was invented in 1952 by John Dunlavy whilst he was contracted to the United States Air Force. He wasn't credited because it was classified as "Secret", later changed to "Restricted". In 1958 Dwight Isbell built a log periodic antenna as an undergraduate student at the University of Illinois at Urbana-Champaign. He was part of a larger team that included Raymond DuHamel, John Dyson and Robert Carrell. Later Paul Mayes developed a variant that improved performance.

    Before I dig in, I'll also note that this antenna caused all manner of legal issues that are still in force today. The so-called Blonder-Tongue Doctrine states that a patent holder isn't permitted to re-litigate the validity of a patent that has been held invalid previously. It was a result of the University attempting and ultimately failing to protect its patent for the widely copied antenna design. Reading about this is a fascinating discovery in how a single Judge can make a massive impact on law and society.

    The log periodic antenna is designed in a way that to the uninitiated looks very similar to a Yagi antenna. It's based on the idea that you can design an antenna made up from independent dipoles that are spaced in such a way that they form an antenna where each dipole radiates to take advantage of its neighbours. Generally a log periodic antenna looks like a triangle. Often the elements are on two separate booms, alternating side-to-side, or you'll see a zig-zag structure that causes the antenna signal to alternate side-to-side.

    One characteristic of an antenna is called bandwidth. It's a measure of how many frequencies it can operate on within the constraints of the antenna. The wider the bandwidth, the more frequencies you can use with the same antenna.

    A Yagi antenna typically operates within about four percent of the design frequency. If you combine multiple Yagis by adding traps or different length elements, you'll end up with several frequencies, each with a similar range.

    A log periodic antenna on the other hand is designed to be used across a large range of frequencies. In shortwave broadcasting there are log periodic antennas that operate between 6 and 26 MHz. In more common use today you'll find log periodic antennas used for higher frequencies. It's not unusual to find log periodic antennas that operate between 400 and 4000 MHz.

    For even more confusion, you can share the boom of a log periodic antenna with a Yagi antenna as is popular in fringe television reception areas.

    Some other things to note are that for a Yagi most of the elements are passive and only one is generally a driven element, in a log periodic antenna all elements are driven. For a Yagi antenna, more elements means more gain, whereas for a log periodic antenna it means more frequencies.

    I'll also point out that there are experiments where the frequency range for Yagi antennas is being increased to more than twenty percent of the main frequency by varying the design. Much of this is achieved by using computer simulations to test many different virtual antennas until one promising design pops out. This optimisation technique can also be applied to log periodic antennas resulting in very interesting shapes that look nothing like the antennas you see on the roof today.

    I've completely skipped over how these antennas are actually fed, as-in, how is the coax connected to the antenna. That's a whole different topic of conversation worthy of many hours of research and discussion.

    Next time you look at a spiky antenna you should be able to discover if it's a Yagi or log periodic, or both and why.

    I'm Onno VK6FLAB


    Some Amateur Radio ABCs ... Feb 19, 2023
    Show notes

    Foundations of Amateur Radio

    A is for Antenna, the eyes and ears of any amateur station. You'll spend eighty percent of your life attempting to get twenty percent improvement for any antenna you'll ever use.

    B is for Balun, bringing together the balanced and unbalanced parts of your antenna system.

    C is for Coax, the versatile conductor that snakes into your station, one roll at a time.

    D is for Dipole, the standard against which all antennas are measured, simple to make, simple to use and often first in the many antenna experiments you'll embark on in your amateur journey.

    E is for Electron, source of all things RF, the beginning, middle and end of electromagnetism, the reason you are an amateur.

    F is for Frequency, the higher you go, the faster it happens.

    G is for Gain, measured against a baseline, you'll throw increasing amounts of effort at getting more, one decibel at a time.

    H is for Hertz, Heinrich to his mother, the first person to transmit and receive controlled radio waves in November of 1886 proving that James Clerk Maxwell's theory of electromagnetism was correct.

    I is for Ionosphere, the complex and ever changing layers that surround Earth which led radio amateurs to discover HF propagation in 1923.

    J is for JOTA, the Jamboree On The Air where radio amateurs, guides and scouts come together on the third full weekend of October to share global communications.

    K is for Kerchunk, the sound caused by the local repeater that brings a smile to the operator and a grimace to the listener, created by pushing the talk button and not saying anything.

    L is for Logging, the only way you'll ever remember who you spoke to and when and the perfect excuse for bragging to your friends after you managed to collect contacts all over the globe.

    M is for Modulation, adding information to a radio signal by varying the amplitude, frequency, or phase.

    N is for Net, a social excuse for getting on air and making noise with your friends.

    O is for Oscillator, making repeating currents or voltages by non-mechanical means.

    P is for Prefix, the beginning part of an amateur callsign that identifies your country or region of origin.

    Q is for QRP, the best way to make just enough noise to make yourself heard, low power is the way to go!

    R is for Resonance, the point where a circuit responds strongly to a particular frequency and less to others, used every time you tune a radio or an antenna or both.

    S is for Shack, the space you call home, where you live your radio dream. The size of the corner of the kitchen table, the back-seat of your car or a purpose built structure with never enough space, no matter how much you try.

    T is for Transceiver, a single box that contains both a transmitter and receiver that share a common circuit.

    U is for UTC, Coordinated Universal Time, the only time zone that radio amateurs should use for any activity that goes beyond their suburb.

    V is for VFO, the Variable Frequency Oscillator that provides radio amateurs with frequency agility, the means to listen anywhere, any-time.

    W is for Waterfall, which displays radio signals across multiple frequencies at the same time.

    X is for XIT, Transmit Incremental Tuning, changing your transmitter frequency whilst listening on the same frequency, helpful when you're trying to break through a DX pile-up.

    Y is for Yagi, or Yagi-Uda antenna, the most popular directional antenna invented in 1926 by Shintaro Uda at the Tohoku Imperial University in Japan and popularised to the English speaking world by his boss Hidetsugu Yagi.

    Z is for Zulu, the last word in the phonetic alphabet that every amateur should know and use.

    73 is for best regards. Saying goodbye is hard to do, this says so without fanfare and clears your station from the air.

    I'm Onno VK6FLAB


    Do you really know when the best time is to go on air? Feb 12, 2023
    Show notes

    Foundations of Amateur Radio

    Getting on air and making noise is a phrase that you've likely heard me repeat often, actually, this will be the 24th time or so. It's an attempt at encouraging you to actually transmit and use the radio spectrum that is available to you. It's a nicer way of saying: Use it or lose it!

    One of the more frustrating aspects of our hobby is finding other people to interact with. At the beginning of your hobby you have access to all these magic radio frequencies with no idea on how to use them. Often a new amateur will turn on their radio, call CQ a couple of times to see if there's anyone out there, hear nothing and give up.

    As you get more experience you'll discover that radio frequencies change over time and that some work better at certain times of the day. This is reinforced by others who will talk to you about propagation, the solar cycle and how the ionosphere and its various so-called layers will change and what you can achieve throughout the day, the year and the long term cycle.

    Armed with all this knowledge you are likely to get to a point where you make noise on a certain band depending on the time of day.

    For example, experienced amateurs will avoid the 10m band at night because it's a so-called day-time band, in other words, their perception is that you cannot make contact on the 10m band after sunset and for the same reason, it's not suitable for early morning contacts.

    What if we could test that perception and see if it's true or not?

    Turns out that we have a perfect dataset to discover what actually happens. If I look at the 10m band WSPR or Weak Signal Propagation Reporter data for the past year, a year that had me using a beacon pretty much 24 hours a day, you'd expect that you could see just which times worked and which ones didn't. Turns out that regardless of time of day, my beacon was heard across every hour of the day. Of course the numbers aren't uniform across the day. The peak is at noon local time, the trough is at 5 am local time, 10% of reports are at noon, about 1.5% at 5 am. In other words, the worst time of day for my beacon to be reported is 5 am in the morning and it's not zero.

    Interestingly the same isn't true for the signal to noise ratio, a measure of just how weak or strong a signal is in comparison to the local noise at the receiver. If you account for differences in transmitter power, meaning that a stronger transmitter is measured in the same way as a weaker one, the 10m band has the best signal to noise ratio at my location at 9 pm local time and the worst at 4 pm local time.

    Given that I'm only using the 10m band with my beacon I also looked at the local OF78 grid square across all bands. It shows that reports are not directly related to when the average signal to noise is best. It seems to me that people are transmitting when they think it works best, not when it actually works best and I'll mention that the definition of "best" depends on each user.

    Note that I haven't yet sat down to discover if there are automatic transmitter and receiver pairs that have been reporting 24/7 across a year on the same band to determine if there is more to learn about the relationship between how often something is reported and what the signal report was at the time. I can say that it's likely that your favourite band is more popular when others think it's popular, not when the conditions are better.

    Consider for example that there are no local reports on the 12m band at 10am, but there are at 9am and 11am, so, was the band magically unusable the whole year at that time, or did people just not use it? The same is true for 160m. No reports at all before 5pm or after 3am, despite the bands around it having contacts throughout the day.

    I will point out some things I've ignored. For example, what is a useful contact? Is it measured by distance, by quantity, by uniqueness? Is this choice the same for each band? Is it reasonable to compare a whole year, or should it be by some other time period, like month, season or lunar month? What is the signal to noise ratio for a band that's considered closed?

    I'm mentioning this because each of those will directly affect what it looks like when you create a chart and it's likely to change what works best for you.

    So, next time you get on air, try a band that shouldn't work according to your knowledge and see what happens. Perhaps you'll get lucky, make a contact and discover something unexpected.

    I'm Onno VK6FLAB


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