The first proper snowfall in 7 years, so peaceful. Reminded me to upload a track that I’d forgotten about- Ice Palace Ambient – The chilly ice cold extended 45 minute version, check it out below on SoundCloud or whichever streaming service you use, it’ll be there!
During the 2016 MicroGNeXT asteroid anchor project “involvement” (they earned an extra VIP tour at the Houston NASA NBL because of our interactions in their public outreach efforts) I created this abstract art based background video version, also on YouTube. Featuring rendered radar data of the Asteroid Bennu, pre-OsirisREX mission, so based on normalized radar data taken from Earth.
The objects stuck into it are abstract but they really do have a meaning 🤔😸
This began as a journal blog entry just about a newly acquired antenna however I have expanded it to include some backstory about the early days of my youth before I became a fully licensed radio amateur, a little bit of my life from the age 14 and up.
I hope you enjoy the read, please let me know if there are things that you would like to hear about in the future. This story is not embellished, though it does lack some pieces I had originally intended to publish but the things I wanted to include with the permission of a friend unfortunately didn’t materialize in time but will hopefully make it into another journal entry at some point in the near future.
That afternoon, my radio had been particularly noisy with the usual noisy pest- skip from the continent. All the channels were full of it, just a splatter of constant atonal screeching- the all too familiar FM carriers colliding from people too far away to hear one another. The whine and raspy hash of mashed up signals mixed with Italian and Spanish SSB wobble & warble breakthrough- it was useless trying to get out anywhere “local”.
While clunking the channel selector on the radio I settled on some unusually strong signals. I’d heard POCSAG pagers from the local hospital before but these were entirely different and I could tell that some, but not all were coming in on the skip. I really didn’t know what I was listening to but the tones were pleasant and definitely structured in packets. A header, a data burst and a tail, each one a little bit like the loading sounds from a cassette loaded computer game.
It just to happened that I’d actually been flipping through the Maplins catalogue while sat on the bog. Looking back now, it was probably a bit weird but for me at the time, it was how I chose how to blow all of my saved up birthday & pocket money.
I’d seen the kit several times in the mag already but not really bothered to read the item description before, but I’d got a spark from the idea that it might actually be for this type of signal so I looked it up. A packet radio modem kit, 1200 baud speed. Hmmm.
I had a hunch. After a neatly coordinated bus and train trip to and from the Maplins in Coventry, I’d bought home a pile of components and a plastic box.
After successfully constructing and then setting up the modem with the radio and then configuring the terribly old and slow Compaq Deskpro XT PC with the Baycom software, the first packets decoded floored me.
Readable data traveling through the air from France, the Netherlands, Germany, Italy, Spain and probably more- incredible!
This was gonna be huge for me and my mates. Unlimited “online” chatting, connected so no need to use the mic to talk all night- we could chatter & trollolol on about cheese without any distractions or interruptions or sleep- today in the age of smartphones this is seriously taken for granted.
By 1996 ENG01A BBS had served quite a large portion of the Midlands during its four or so years of operation. The radio also served as a digital packet repeater (digipeater) during frequent radio path openings to the continent as well as a “hotspot” for forwarding mail up to Cannock and across to Birmingham. Some of my mates even used my system to hop to distant stations on the continent during “sporadic-E”-layer ionospheric propagation– it was awesometo watch in action!
The BBS in its final form was a machine comprised of a “custom built” 486 DX built from 2nd hand scrap, with a Kantronics KPC-3 Terminal Node Controller (TNC) connected to a “Superstar 3900” CB radio- operating on Channel 24. (27.235MHz). Running inside a shed that would easily spike at over 35°C during the summer months, the gear was punished pretty severely!
Networked to the secondary machine located in my old teenage bedroom via a massive run of RG-213 coaxial Ethernet cable, enabling remote access, saving uncountable trips down to the owl house attached shed during freezing cold or miserably wet British weather.
By aged 17, having passed the RAE (amateur radio exam qualification), and then diving head first into the internet, it was not long before an online relationship quickly matured to a very real life getting-engaged situation. A sudden and swift decision on my part to save money on the phone bill and weekly plane tickets- I ultimately quit my job and moved to live in the Netherlands, with some hard graft put in at Ericsson R&D, we finally purchased our first home together in 2001.
CB radio had been booming & blooming in the Netherlands with digital packet radio networks for almost a decade. Dutch legislation had effectively enabled the digital adoption by deregulating the Citizens Band entirely. This lead the way for manufacturers to legally advertise and sell packet radio equipment to quite a substantially larger market then just radio hams. A stark contrast compared with the UK.
Later, unlicensed usage and the allowance of data over RF would be ratified and somewhat protected in the CEPT specification with several channels/frequencies specifically set aside for packet/data.
The CB and ham packet stations in the Netherlands eventually began to decline beyond a sustainable network in the mid-2000s. For the CBers, The sunspot cycle had come to an end and so too did the interest in long distance (DX). For the hams, there were fresher new digital-mode pastures to play with now that the internet had most certainly won.
The lockdown due to the COVID-19 pandemic has seen a noticeable increase of activity on amateur radio as people- perhaps likely perturbed by everything going on- have come back to their radios. As a consequence the packet community has been busy helping a number of hams set their packet stations back up again. Yay! 🎉
The idea to put up a new 10 meter band antenna began to gather momentum as personal forecasts for 2021 predicted it likely to be up to another year locked indoors- something we are already quite familiar with due to Ilona’s cancer treatment in 2019. So I purchased a shiny new antenna from the local ham shop and it was delivered the very next day:
The radiator is the short stub on the lower left that couples to the large vertical in the center.
At the top of the antenna is a wire ball for hypothetically reducing corona discharge- high voltage RF (radio frequency) sparking into the air when running very high power. Though I suspect this is yet another window dressing feature of CB antennas- its probably for the looks. I operate almost exclusively within my limits and I have consideration for my densely packed in neighbors so it’ll never be presented with more than 100 watts of power.
The circular basket? Probably extra capacitive coupling for the radiator element, though- jury is still out on this one… Looks cool though 😎 📡
If only we could see RF with our eyes… 👀
Yay! 😁 I’m once again able to work 10 meter band digital modes, so you may hear me on FT8 or WSPR from time to time.
I have checked the packet signals on 11 meters (CB)- there is a bit of “local” FM packet activity from stations about 80-100km away, but it is too weak to decode- unfortunate!
Luckily I am able to log into those packet stations remotely via the internet gateway and can remotely trigger their transmitters, so far I have worked out who I can hear: NL9UTR and NL9SHB – Utrecht and Den Bosch respectively. Bit of a reach to Rijen apparently. 😿
Due to quite high levels of neighborhood interference from power-line networking, solar panels, crappy laptop chargers and ISM band encroachment- its a constant S5 of noise here, even with local phase cancellation mitigation on the packet frequency. However, during good skip conditions, signals from abroad can easily be 20db+ so its a bit of a mixed bag- now on to some testing ⚡️
Early Signal Reports
Above are a couple of maps showing my experiment on the 10 meter amateur band with FT-8, an insanely narrowband slow digital transmission capable of penetrating signal-to-noise ratios previously only touchable by Morse code.
With the use of advanced digital signal processing machine FT-8 can decode signals that are barely perceptible to the human ear.
The maps were created with the use of the reverse beacon network– a bunch of automated listening stations. The RBN is mostly unmanned ham equipment left running while the operator is away, decoding and reporting what they can hear to a central database on the Internet, (pskreporter.info for example).
So the Vector 4000 is basically as good as I remember it being back in the 90s. It is limited in use though, as one cannot tune it to anything other than the designed band.
The resonance drops way off after 1.5MHz bandwidth curve so don’t be expecting this to work as a multi band antenna.
For 10 meters, the Vector 4000 is an exceptional performer, the reception across the shortwave spectrum is also decent but not overwhelmingly as you might expect for a vertical.
Weather robustness – this Vector 4000 has happily survived some close-to-gale force winds recently, metal fatigue is a factor I may yet have to contend with as the aluminum joints aren’t all that large or convincingly strong. My previous Vector 4000 back in the 90s suffered from a severe clobbering from an Oak tree, breaking it in half, though if not for that, it probably would have lasted many more years.
All of the bolts, joints and connections have been triple wrapped in “Scotch 23” electrical self amalgamating tape which does offer some extra tensile strength as well as waterproofing, so we will have to see!
Bonus quiz round: what “B” was the name of a successful British television game-show popular with the 90s youth?
You will see several mentions of Sporadic-E on this site, so I’ve taken a shot here at explaining the phenomenon in my own words. I hope you enjoy the tangent from the usual posts, but if you are already versed in solar physics feel free to skip along- wait maybe you won’t get that reference unless you read this bit… 🤔
Sporadic E events- a phenomenon frequently observed in the early 90s as the increased frequency of the Sun’s coronal mass ejections created observable disturbances in the Earth’s ionosphere.
The phenomena occurs naturally every 11-year cycle, waxing and waning between the peaks- known as the solar maximum– during these periods, the most sunspots are produced.
Sunspots are a product of the complex interactions between the suns powerful magnetic fields and the fusion reactions occurring deep within the core of the sun. Magnetic fields twist and contort through the plasma as the sun rotates on its axis, eventually some of these powerful magnetic fields can no longer hold on to their couplings and break apart in violent and destructive solar flares, scattering the sun’s plasma deep into space. Sometimes, directly at Earth.
Powerful magnetic interactions during solar flare events also cause magnetic disturbances that travel at the speed of light towards Earth. These are known as geomagnetic storms and can in the most extreme cases cause severe problems for the electrical grids that deliver power to our industry and homes, as well as damage satellites that operate out beyond the protection of our magnetic field.
Approximately three days after a geomagnetic storm, the sub-light-speed particles ejected from the sun arrive at Earth and hit the magnetic field, and if powerful enough can sometimes reach the upper ionosphere. These particles are extremely high-energy, if they were to reach the surface of Earth they would have a devastating and deadly effect on biological organisms.
The magnetic field of Earth is generated by the planet’s liquid core- much like a bicycle dynamo, the magnetic interaction though rotation of the different densities of liquid metal in the core produce strong magnetic fields that protrude out from the north and south poles, enveloping the Earth with a magnetic shield.
As the sun shines, it also emits solar radiation in the form of a constant stream of charged particles- this ambient bombardment is known as the solar wind.
The solar wind speed increases dramatically during sunspot activity, putting greater pressure on Earth’s magnetic envelope. As the magnetic field interacts with the solar wind, particles billow around the envelope towards the poles- the weakest points of the magnetic field- where the charged particles interact with the oxygen and nitrogen gas in the upper atmosphere- this can be observed visually as the Aurora Borealis and Aurora Australis.
Sporadic-E is the name designated for the unpredictable property of the ionosphere when the solar wind travels deep and at high enough energy through the ionosphere that it causes a plasma to occur. This plasma is conductive, and therefore capable of reflecting radio frequency back to the ground.
This is how high frequency (HF) radio waves that would otherwise be absorbed by the ambient ionosphere propagate great distances beyond line of sight. Although the radio waves always travel in a straight line from the source, they can bounce off the sporadic plasma and back towards the ground. In combination with the ocean, this can sometimes happen multiple times before the radio wave is intercepted by a radio receiver. This is colloquially known as radio skip.
For the most part the F1 and F2 layers form from the separation of the radio-absorbing D layer at night when the solar wind reduces pressure on the magnetic field facing away from the sun, as Earth rotates from day to night- this allows shortwave to propagate further which is why distant radio stations can only be heard coming through in the evening hours.
Sporadic-E layers of the ionosphere are responsible for the majority of radio propagation phenomenon at upper-HF frequencies, such frequencies as the common CEPT and UK CB radio specification and the 10, 6 and 4 meter amateur radio band.