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Showing posts with label Digital Voice Radio Modes. Show all posts
Showing posts with label Digital Voice Radio Modes. Show all posts

Friday, August 28, 2026

Reminder: Annual ID Verification - Radio ID.net

 

ID numbers used for DMR and other amateur radio digital networks are a finite resource. Due to the growing popularity of these modes, along with some users requiring multiple IDs, certain regions are expected to face ID shortages in the near future.

Beginning July 1, 2026, RadioID.net will implement an annual verification process. On the anniversary of each account's creation, RadioID.net will send an email to the account holder requesting confirmation that the assigned ID(s) are still needed and that the account information remains accurate and up to date.

If no confirmation is received, the associated ID(s) will be temporarily deactivated. If RadioID.net is unable to obtain a response after a reasonable period, the ID(s) will be removed from the database and made available for reassignment. This process is intended to preserve the long-term availability of ID numbers and maintain an accurate database for the amateur radio community.

  • Year 1: If unable to contact you, we mark your account as unvalidated, IDs still work.
  • Year 2: If still unable, we mark your account/IDs as Deleted, IDs no longer work.
  • Year 3: If still unable to contact you for validation, Accounts and IDs are deleted.

** We are also using LastHeard data to help trim this list down.

- RadioID.net 

 

Wednesday, August 19, 2026

Update: The ZS1I - 6 Meter Magic Band Project in the Southern Cape Area of South Africa. (Part 2)


Image:  AI  (Click on image for larger view.)

My mind has been filled with many projects that I would like to construct in the next few years.  Only time will tell if this will be possible as many unforeseen things can happen that prevent me from completing projects.  Now one of the projects that I work on from time to time is the 6 Meter Magic Band Project in the Southern Cape Area of South Africa.  Read more HERE about this project.

I have been reading every single day to gain as much knowledge and information as possible on the various projects that I am busy constructing or putting together.  What a great privilege to still have good health and eye sight  that makes reading and learning possible.

Awhile ago I completed the 6 Meter CW Beacon but it is still not on the air.  One reason for this is I will have to relinquish other RF radio systems to ensure that I have optimal "conditions" in and around the shack for 6 Meter operations.   I also need to use current antenna poles to install 6 Meter antennas.  I need to remove the 2 Meter antenna pole to be used for 6 Meters. 

Be as it may my brain runs in "overdrive" when it comes to amateur radio ideas and projects.  I came up with the following question:

Which mode, CW or WSPR is better for a 6 meter magic band project? The ZS1I 6 meter magic band project for amateur radio involves building or using equipment (radios, antennas) to exploit the unique, unpredictable long-distance propagation (Sporadic-E, F2 skip, Aurora) on the 50-54 MHz frequency, offering both short-range VHF and surprise HF-like DX (long-distance) contacts, often using simple DIY antennas like halo loops or Moxons for great results and rewarding challenges. Projects focus on maximizing these propagation modes, especially during peak seasons like summer (Sporadic-E) and solar maximums (F2).

I was interesting to find out what mode will provide the "better"  outcome taking into account the local factors in the Southern Cape and the equipment I will be using to achieve ultimate success with the 6m project.

I decided to call on AI to answer my question: 

"The question of whether a WSPR (Weak Signal Propagation Reporter) beacon or a traditional CW (Morse Code) beacon is "better" for the 6-metre band (50 MHz) depends entirely on how you plan to monitor the band and what equipment you want to use.


Direct Comparison

Feature

WSPR Beacon

CW Beacon

Sensitivity

Superior (Decodes down to -28 to -31 dB SNR)

Inferior (Human ear cuts off around -10 to -15 dB)

Required Equipment

Radio + Computer/Interface or dedicated digital transmitter

Just a standard receiver (and your ears)

Reporting Network

Automated logging to WSPRnet

Dependent on the Reverse Beacon Network or manual logs

Bandwidth

Ultra-narrow (~6 Hz per signal)

Narrow (~100-200 Hz)

Time to Results

2-minute fixed transmission cycles

Instantaneous identification


Why WSPR is Better

  • Extreme Weak-Signal Decoding: WSPR is specifically designed to dig deep below the static. It can decode signals as low as -31 dB SNR. This allows you to spot micro-openings or tropospheric ducting paths on 6 metres that a human ear scanning a CW frequency would completely miss.

  • Set-and-Forget Automation: When you leave a WSPR beacon running, automated listening stations worldwide upload the data directly to WSPRnet. You can pull up a live map on your phone or PC to see exactly where your 6-metre signal is landing without relying on anyone manually copying your Morse code.

  • Ultra-Low Power: Because of its heavy forward error correction (FEC), you can run a 6-metre WSPR beacon on just a few milliwatts to 1 Watt and still get spots thousands of miles away.

Why CW is Better

  • Instant Band Awareness: 6 metres is known as the "Magic Band" because it can open to sporadic-E propagation instantly. WSPR takes exactly 2 minutes per transmission cycle to decode. If you are actively sitting at your desk waiting for a band opening to make contacts (like FT8 or SSB), listening to a cycling CW beacon provides immediate auditory confirmation the second the band pops open.

  • No Computer Required: You don’t need an interface, software (like WSJT-X), or precise GPS time-syncing to use a CW beacon. You just spin the dial to the 50.000–50.100 MHz beacon sub-band and listen.

  • Indicator of Communication Readiness: If you can hear a CW beacon with your ears, the band is open enough to support live, two-way human communications (SSB, CW, or FT8). WSPR signals can be decoded even when the path is too weak to support a normal conversation.


The Verdict

  • Choose WSPR if your goal is long-term propagation research, antenna testing, or seeing if a path exists when the band appears "dead".

  • Choose CW if you are an active operator waiting to jump on the radio the moment 6 metres opens up for live voice or Morse code contacts."

Many modern beacon builders actually combine the two by setting up a transmitter that alternates—sending a 2-minute WSPR cycle followed by a brief CW identification so that both digital systems and human ears can utilize the signal!

There you have it.  I will have to make a decision as to whether I will be going the WSPR or CW "route".   The decision is quite simple.  

AI makes it easy: 

"Operating from KF15BT (located in the beautiful but radio-isolated Southern Cape region of South Africa, near Mossel Bay/George), you are uniquely positioned for long-distance DXing via interesting propagation modes, but you face the classic "lonely ham" problem. Because there is little to no local 50 Mhz activity to keep the band warm, you must rely entirely on automated "triggers" to tell you when a long-distance opening is happening. 

Given your excellent gear (6 Meter Yaesu Radio, Moxon, Delta Loop) and your homebrew Arduino/ESP32 hardware, digital modes (specifically FT8 for contacts and WSPR for monitoring) are absolutely the way forward. 

Here is the exact strategic blueprint for conquering the "Magic Band" completely solo from your grid square.

The Strategy: Digital over CW

    • The FT8 Reality: 95% of global 6m DX hunting is concentrated on 50.313 MHz (FT8). If the band opens from South Africa to Europe, South America, or up into Africa, those stations will be parked on FT8 waiting for signals. 

    • The Problem with CW: If you sit and text CQ on CW, no one will hear you unless their beam is pointed directly at KF15. Most European or DX stations leave their rigs automated on FT8 overnight or during the day to catch rare openings. "

For raw technical performance and automated global tracking, WSPR is vastly superior. However, for real-time human monitoring and instant "radio-in-hand" notification of sporadic-E band openings, CW beacons remain highly essential."

These last three lines is the crux of my question and answer. I will be using WSPR which is vastly superior and will hopefully provide the best outcome for the project. Along the way I will however also make use of CW. Time to get to work!

Monday, August 17, 2026

Is this possibly the end of the road for the ZS1I AllStar RF Link on 145.550 Mhz in Mossel Bay?

Image: AI (Click on the image for larger view.)

Is this possibly the end of the road for the ZS1I AllStar RF Link on 145.550 Mhz?  For the time being the ZS1I AllStar RF Link on 145.550 Mhz in Mossel Bay has been switched off and will not be available until further notice.

The following reasons are being presented as to why this decision has been taken:

1.  The 145.550 Mhz RF Link is solely being used by yours truly in and around the household.  Running at 25 watts output power this is a waste of RF energy and unnecessary stress on equipment.  To those that do not talk but listen (gooi varkoor) unfortunately you will have to find another source to listen.

2.  I have the following radio equipment running every day in the shack.

  • DMR Repeater
  • WSPR Beacon
  • 2m RF Simplex Link
  • 6 cm CW Beacon
  • 70 cm RF Simplex Link (at times when necessary)
  • 2 x WiFi Routers
  • 5.8 Ghz AREDN Node 

I am getting ready for the 6 Meter "Magic Band" Season that will soon commence.  I want to keep RF levels in and around the shack as low as possible.  This will entail switching of other RF radio equipment that does not get used regularly.  

3.  I have indicated before that I want to concentrate more on DMR and 6 Meter Operation. Well the time has arrived for just doing that.  Unfortunately I will have to relinquish other systems to ensure that I have optimal "conditions" in and around the shack for DMR and 6 Meter operations.

4.  I also need to use current antenna poles to install 6 Meter and 70 cm antennas.  I will therefor remove the 2 Meter antenna pole to be used for 6 Meters.

5.  The current EMI / Ground Level Noise is running quite high in the shack due to various outside factors.  I need to lower this noise factor and need to eliminate the source of this noise if possible.  I will use the process of elimination to hopefully solve the high noise level. 

6.  I intend using separate TX and RX equipment for 6 Meters.  Power output will also differ depending on the mode of communication.  I do not want to run any equipment that is not being utilized regularly.  I will run all equipment from solar power, hopefully noise free!

There you have it.   Will the ZS1I AllStar Hub in Mossel Bay still be available and operational for use by radio amateur?  YES, it will work as before, just without the 2m RF Link on 145.550 Mhz.  I will monitor the running systems and might utilize the 145.550 Mhz RF Link again in future when the need arise.


Wednesday, July 22, 2026

Compliments to the DMR-ZA Net Controller and Participating Stations - "ET phoned home last night during the Net!!"


Image:  ET phoning home, thanks to the DMR-ZA Net! 

Some time ago I "complained" in general about the operating procedures of some of our fellow radio amateurs in South Africa.  Articles  HERE, HERE and HERE. I indicated that ET cannot phone home from certain Nets in South Africa where bad operating practices exist.  This of cause all tongue in the cheek but these blatant transgressions and bad incidents is of great concern, not only to me but many others as well.  However one Net and that is the DMR-ZA Net is showing how it should be done.

Last night I listened to the Net and to Brian ZS5BR, the Net Controller. I would like to complement all those who participated in the Net and in particular Brian ZS5BR who "controlled" the Net.  This is how a net should function and on the forefront was the excellent operating procedures of everybody involved in the Net.  I listen to a few nets and also participate in some nets in South Africa but the DMR-ZA Net's outstanding procedures make it a real pleasure to listen and participate in.  Great practice by all those involved.

No I am not going to go into detail but join this Net on a Tuesday evenings at 19h30 SAST and experience the net for yourself.  The DMR-ZA Net has set the standard of how it should be done.  It took me back to the olden day's where it was of the utmost importance and pride to run a net professionally and using good operating procedures and practices.  

A big thank you to all involved in the DMR-ZA Net - "ET was able to phone home last night thanks to the DMR-ZA Net!! 

Wednesday, July 15, 2026

South Africa's own Oscar- DMR 1 Satellite. Will this DMR Satellite ever go to Space?


Image:  AI (Click on image for larger view.) 

I wrote several articles in the past where I refer to innovation in Amateur Radio.  This morning a thought came to mind on why is there currently not a satellite with a DMR Transponder (repeater) up in space?  I was trying to think "out of the box" and look at ways and means to turn my thoughts into reality, if there is such a possibility.

Thinking "out of the box" is absolutely a great way to approach innovation in amateur radio.  Amateur Radio has a rich history of development driven entirely by amateurs experimenting with limited resources and unique constraints. 

However, true innovation in this hobby relies on a balance between unconventional thinking and foundational science. 

Why Out-of-the-Box Thinking Works

  • Resourcefulness: Limited power regulations and frequency bands force you to find clever ways to maximize efficiency.

  • Historical Precedent: Amateurs invented weak-signal digital modes (like FT8) and bounce signals off the moon (EME) because someone asked "what if?"

  • Cross-Pollination: Bringing concepts from computing, machine learning, or material science into radio often yields breakthrough results.

The Innovation Blueprint in Amateur Radio

To make your creative ideas successful, pair your out-of-the-box thinking with these structured approaches:

  • Master the Fundamentals: You must understand Maxwell's equations, wave propagation, and circuit design to break the rules effectively.

  • Identify Real Constraints: True innovation solves a specific problem, such as reducing noise, shrinking antenna size, or bridging communication gaps during disasters.

  • Iterate and Test: Build prototypes, collect data, and use antenna analyzers or software simulation tools to prove your theories.

  • Share with the Community: Amateur radio thrives on open-source collaboration. Presenting your ideas on forums, Git repositories, or at club meetings helps refine them.

Prominent Areas Needing Innovation

If you are looking for modern challenges to apply your creativity, focus on these emerging sectors:

  • AI and Machine Learning: Using neural networks for predictive propagation filtering or automated signal decoding in dense noise.

  • Alternative Materials: Experimenting with meta materials, fractal geometry, or everyday conductive liquids for stealth antenna designs.

  • Digital Signal Processing (DSP): Developing open-source algorithms to extract ultra-weak signals from high-noise urban environments.

  • Green Energy Integration: Creating ultra-efficient, off-grid solar or kinetic power management systems for remote field operations.

Now reading the above my thoughts ran away with me regarding a DMR transponder (repeater / beacon / node / hotspot) payload on a South African satellite.  Can it be done and is it possible to communicate using  DMR via a satellite?  Is there a satellite specifically named "Oscar-DMR 1" in existence or being built in South Africa's space programme or amateur radio history. Currently this type of communications is not possible.

If you are waiting for a homegrown South African satellite or an OSCAR (Orbiting Satellite Carrying Amateur Radio) series spacecraft to launch, here is the factual reality of what has actually happened and what is currently in progress.

The Real South African Satellites

South Africa has already successfully launched multiple satellites. If you are looking for local aerospace achievements "seeing the daylight," they have already made it to space: 

  • SUNSAT (SO-35): Launched in 1999, SUNSAT was South Africa's very first satellite, built by Stellenbosch University. Critically, it carried an amateur radio payload and was officially designated as OSCAR 35 (SO-35) by AMSAT. It saw plenty of daylight before its mission ended. 

  • ZACUBE-1 & ZACUBE-2: Developed by the Cape Peninsula University of Technology (CPUT). ZACUBE-1 (TshepisoSAT) launched in 2013, and ZACUBE-2 launched in 2018. 

  • MDASat-1 Constellation: In January 2022, South Africa successfully launched a three-nanosatellite constellation via a SpaceX Falcon 9 rocket. These operational maritime domain awareness satellites track shipping traffic off the South African coast. 

ZS1I created the fictional "DMR 1" Satellite Name 

The term DMR stands for Digital Mobile Radio, which is a widely popular land-based digital protocol used by radio enthusiasts and businesses across South Africa. 

  • Terrestrial, Not Space: Amateur radio operators in SA heavily utilize the South Africa DMR Repeater Network. This network relies on ground-based repeater towers, not dedicated South African "DMR satellites." 

  • Conflation with Commercial Satellites: You may be thinking of commercial mobile satellite services or push-to-talk satellite radios that interface with DMR-style dispatch systems on the ground. 

Future South African Space Missions

If you are wondering about the next major government-backed leap into orbit, the Department of Science and Innovation has active plans: 

  • National Communication Satellite: The government has been exploring multi-billion-rand plans to acquire or launch a dedicated communications satellite to bridge the digital divide and reduce reliance on international space entities.  However this look like a very "far in the future" project with many logistical and financial issues to first solve.

  • Deep Space Ground Tracking: While not a satellite itself, South Africa broke ground on a massive, state-of-the-art Deep-Space Ground Station in Matjiesfontein (Karoo), built in partnership with NASA to track future lunar missions. 

Sadly you cannot work DMR (Digital Mobile Radio) directly through orbiting amateur radio satellites.  Hopefully by means of innovation in technology my thought on building such is satellite is not far fetched and will not forever just be a thought.  In South Africa building such a satellite will be problematic but that is a topic for another time.

Let's see why this can or cannot currently be implemented.  

You can absolutely build a physical DMR repeater and launch it into orbit on a satellite. However, doing so introduces a severe physics and timing challenge that standard DMR protocols are not designed to handle. 

The core issue is the speed of light and the Doppler effect.

The Timing Problem (TDMA Breakdown)

DMR relies on TDMA (Time Division Multiple Access). It divides a single frequency channel into two distinct time slots (Slot 1 and Slot 2). 

  • The Rule: Each radio must transmit in an incredibly precise window—exactly 30 milliseconds long.

  • The Margin: The standard protocol only accounts for standard terrestrial distances, leaving a guard timing buffer of about 1.25 milliseconds to handle propagation delay. 

When a satellite is orbiting overhead (even a Low Earth Orbit, or LEO satellite at ~500 km), the distance from the ground station to the spacecraft changes continuously and rapidly. Because the radio waves must travel hundreds of kilometers to space and back, the propagation delay exceeds that 1.25 ms guard window.

Consequently, your radio's packet arrives late, shifts out of its slot, and bleeds into the adjacent time slot. This completely breaks the synchronization, causing the repeater's onboard computer to reject the handshake. 

The Frequency Problem (Doppler Shift)

DMR uses 4FSK digital modulation. It relies on precisely mapping four distinct, narrow frequency shifts to represent binary data. 

Because a LEO satellite travels at roughly 27,000 km/h, the frequency shifts dramatically as it approaches and moves away from you. This Doppler shift warps the digital signal. While a human ear can decode an uncorrected analog FM signal through a bit of static, a digital DMR modem will see the warped 4FSK signal as corrupted gibberish and refuse to decode it. 

How to Make a Space-DMR Repeater Work

If an amateur radio group or space agency wanted to make a true DMR satellite work, they would have to implement one of two workarounds:

  1. Modify the Radio Firmware (Software Solution)
    The ground station's DMR radio would need custom firmware capable of predicting the satellite's exact orbit. The radio would then have to continuously alter its timing (transmit early or late to hit the slot perfectly) and automatically adjust its frequency to cancel out the Doppler shift in real-time.
     

  2. Put the Spacecraft in a Geostationary Orbit (Hardware Solution)
    If you put the DMR repeater on a geostationary satellite (35,786 km above Earth), the satellite remains stationary relative to the ground. This eliminates the Doppler shift entirely. While the time delay would be much larger, it would be
    constant, allowing engineers to build custom terrestrial radios with a massive, fixed timing buffer specifically for space.
     

Consolation Prize 

There is currently a "consolation prize" on how you can use your DMR Radio to connect to satellites indirectly.

You can use your DMR radio to connect to satellites indirectly by talking through an MMDVM hotspot (or a local digital repeater) connected to the internet. From there, your signal is routed to space through a commercial geostationary satellite (such as QO-100) using an up/down converter, a dish, and an SDR (Software Defined Radio). 

Unlikely that a dedicated amateur satellite named "Oscar - DMR 1" will be built in South Africa

It is highly unlikely that a dedicated amateur satellite named "Oscar - DMR 1" will be built specifically for standard DMR voice communications in South Africa. While amateur radio organizations like AMSAT constantly develop new spacecraft, standard commercial DMR protocol is fundamentally incompatible with the physics of Low Earth Orbit (LEO) satellites.

The Geostationary Exception, there is hope!! 

The only way a true DMR transponder could work in space is on a Geostationary (GEO) satellite like QO-100. Because GEO satellites remain completely stationary relative to the Earth's surface, there is zero Doppler shift or changing propagation delay. While there is no official "Oscar - DMR 1" payload planned, experimental digital voice links are routinely tested via GEO transponders using specialized ground stations.  More on this in a future article once I put on my "out of the box" and "innovation" hat.

Was this article a waste of time?  NO definitely not.  I now have more questions than answers that I will be looking into.

ED. This article was compiled by ZS1I with the assistance of AI. 

Saturday, July 11, 2026

ZS1I Mossel Bay DMR Repeater Coverage - Radio Mobile Maps


Image:  Mossel Bay Area (Click on image for larger view.) 

The ZS1I DMR Repeater in Heiderand, Mossel Bay has been running from time to  time since June 2023.  It is permanently on the air from the 1 May 2026 after several hardware and software modifications were done for optimum functioning. Several radio amateurs have provided reports and positive comments with regard to the repeater.  It is quite strange that I never plotted the coverage area using Radio Mobile since June 2023.  I have now plotted the expected coverage area of the repeater.  

Before I publish the images it is important to first publish the repeater- , equipment- , feedline- and antenna information. 

ZS1I Digital Mobile Radio (DMR) Repeater

DMR Repeater Talkgroup 65522:   This repeater is NOT located on a remote mountain site but is situated in the Shack of ZS1I in Heiderand, Mossel Bay. This allows ZS1I to monitor and control the repeater while it is on the air.  
Mossel Bay DMR Repeater Information:

Mode: DMR
Band:  70cm
TX Frequency:  438.262500 Mhz
RX Frequency:  430.662500 Mhz
Radio Mode:  Duplex
Talk Group (TG): 65522
Colour Code: 1
Time Slot:  1 or 2 
RF Power Output: 15 Watt
Logarithmic power level: 41.76 dBm
Antenna EIRP:  46.96 dBm
Antenna:  Diamond X50
Antenna Gain:  7.2 dBi
Antenna Height:  12 Meters
Coax Cable:  RG213 Mil-Spec (West Germany)

This repeater is linked to the ZS1I AllStar Hub Network (Node 49355) (Analog Repeaters / Simplex Link Radio / Echolink / SVXLink / AllStar / South Cape Reflector) via the ZS1I DMR Bridge and Repeater.  

With your system operating at 440 MHz (70cm UHF band) with an EIRP of 46.96 dBm from an antenna height of 12 metres at sea level in Mossel Bay, your real-world coverage will be highly asymmetrical.

Because UHF signals rely almost entirely on line-of-sight propagation and are easily blocked by solid earth, your coverage splits into two completely different zones: vast open coverage over the ocean, and a sharp cutoff to the north caused by the Outeniqua Mountains.

Here is how your 46.96 dBm EIRP system will perform under these specific local conditions:

Line-of-Sight Horizon Limit

The theoretical radio horizon for an antenna 12 metres above sea level is calculated using the standard RF horizon formula:

===================================================================

RADIO HORIZON CALCULATION

===================================================================

Formula:

d = √(17 × h)

Where:

d = Distance to the radio horizon (in kilometres)

h = Antenna height above the ground/sea level (in metres)

-------------------------------------------------------------------

Your Setup Calculation (12-Metre Antenna Height):

d = √(17 × 12)

d = √(204)

d ≈ 14.28 km

Result:

The theoretical radio horizon for your repeater antenna is 14.28 kilometres.

===================================================================

  • To a Handheld Radio (Ground Level): If communicating with a person holding a radio at ground level (approx. 1.5 metres high), their radio horizon is about 5 km. Adding your horizons together means you will have clean, high-clarity Line-of-Sight coverage up to 19–20 km away over the flat ocean surface or open coastal flats towards Hartenbos and Klein Brak River.

2. Terrain Obstacles: The Outeniqua Mountains

To the north of Mossel Bay, the Outeniqua Mountains rise sharply to heights between 800 and over 1,500 metres (such as the Robinson Pass area).

  • The Shadow Effect: At 440 MHz, radio waves behave much like light beams. When your signal hits the massive sandstone slopes of the Outeniquas, the mountains will cast a massive "radio shadow" directly behind them.

  • The Cutoff: Your signal will cleanly illuminate the southern, seaward-facing slopes of the mountains. However, coverage will completely drop off on the northern side of the ridge. You will not be able to reach deeper inland areas like the Little Karoo (Oudtshoorn region) unless you bounce a signal off a mountain-top repeater.

3. Signal Penetration in Town (Urban Factor)

Because your antenna is mounted at 12 metres, it is likely sitting just above or level with standard two-story residential rooftops in Mossel Bay.

  • Structural Losses: 440 MHz UHF is excellent at bouncing between buildings and penetrating walls.

  • Local Range: You can expect highly reliable, punchy coverage throughout the immediate town, even over the hilly terrain of the Cape St. Blaize peninsula. The 46.96 dBm (approx. 50 W) of effective directional power is more than enough to overcome urban attenuation within a 10 to 15 km radius through town structures.

Summary of Estimated Range

  • Over Ocean / Flat Coastline: 20–35 km (Excellent clarity to marine traffic or coastal stations with elevated antennas).

  • Urban Mossel Bay: 10–15 km (Robust signal piercing through local neighborhood obstacles).

  • To the North (Mountains): Up to the ridge line (Signal stops abruptly at the mountain peaks; no coverage in valleys behind them).

     

Images: Courtesy Radio Mobile (Click on images for larger view.)

 Above image:  Mossel Bay wide coverage area

 
 Above image:  Mossel Bay close-up image 1

Above image:  Mossel Bay close-up image 2

Above image: Repeater coverage Albertinia Town.  Bad coverage!!

Above image: Repeater coverage George Area.  Good coverage!!

Above image: Repeater coverage Mossel Bay and Hartenbos Areas.  Good coverage!!

Above image: Repeater coverage West of Mossel Bay / Gouritz River Areas.  Spotted coverage!!


 Above image:  Repeater Coverage - Still Bay, Heidelberg, Riversdale, Albertinia and Herbertsdale.  Bad coverage!!

Friday, July 10, 2026

The decline in Amateur Radio during winter is neutralized by creating activity!!


Who said there is a decline in Amateur Radio during the winter months?  I said so.  Look HERE.

My OM had a saying that if a door is closed into your face, you must always find another door to open and continue with what you are doing and enjoying.  This means do not give up and you will be able to continue also in amateur radio.  So true and this saying I have been following throughout the years.  It allowed me to bounce back in life sometimes even with better results than before.

Well amateur radio activity is up here in the Mossel Bay area as well as parts of South Africa.   Let's look at some of the activity by means of illustrated images:  


Image above:  Connected nodes to the ZS1I HUB in Mossel Bay  (Click on image for larger view.)

Image Above:  Bubble Chart of stations connected to the HUB yesterday afternoon.  (Click on image for larger view.

1.  ZS1I HUB Network Activity:  I will let the images speak for themself.  The HUB is alive and active on a daily basis with stations frequently heard also via all the cross-links and connected nodes and repeaters.  A few overseas stations were also heard on the ZS1I HUB Network.  I do not take any credit for this as the network consists of many participating entities.  Great to hear all the activity taking place.

 Image: Some "useless" information? (Click on image for larger view.)

Image:  Winter playing a role in the decline? (Click on image for larger view.)

2.  ZS1I  Amateur Radio Projects / Activities Blog:  This blog is was created in April 2026 and is already being visited by many viewers on a daily basis.  Hopefully the blog is not only my place were I keep some back-up information but also a medium where young and old can learn something.  I am not a person chasing records or wanting any attention in amateur radio.  I am to old for that nonsense.  The Blog for me is like a amateur radio "diary".  Many article might also be bored and not of interest to others.  None the less thank you to all the visitors for visiting the ZS1I Blog.   I hope to keep up rolling articles out that might be of interest to the general amateur radio community. 


Image:  Brandmeister Hoseline  (Click in image for larger view.) 

3.  DMR Activity still on the increase World Wide!  - Need I say anything about the increase in the use of DMR World Wide and in South Africa?   This is great news for amateur radio operators and the future of digital radio modes.  With the cross-linking of analogue systems to digital systems nobody is left out in the cold even if you only have a analogue HT radio.  At times the ZS1I HUB Network is linked to various DMR Talk Groups which resulted in an increase in activity.  The audio is good and the linked systems work great.  Yesterday operators were heard from Germany, Australia, UK, USA, Japan on Hoseline which was cross linked to the ZS1I DMR Bridge and DMR Repeater in Mossel Bay.  And no it was all country talk groups and not the World Wide Talk Group (91).  Great conversations and activity on DMR.  I do have a few ideas and changes that I would like to make to even better the current cross linked system.   Stay tuned!!

 
 
Image: 40 m WSPR Map South Africa (Click in image for larger view.) 

Image:  Stations that spotted the ZS1I 40m WSPR Beacon recently,  thanks to all.  (Click on image for larger view.)

4.  40m WSPR Activity:  WSPR is a great amateur radio propagation tool.  I am amazed on how propagation changes on the 40m band from time to time.  At one stage only a few stations received the 40m ZS1I WSPR Beacon.  Then all of a sudden there was a increase in spotted stations.  I must admit that I have lots to learn about WSPR.  Sure this will come with time.  In the mean time many thanks to all who regularly spot the Mossel Bay WSPR Beacon.  More interesting developments to come relating to WSPR Beacons in the future. 

5.  ZA-Net Network Activity:  For the past few days I have connected the HUB to the ZA-Net Network up in Gauteng.  At times there were activity even from abroad.  The audio quality was good and the network is working great.  Herewith more information about the network:

ZA-Net Network Web-Site:  Click HERE

Let's build the Modified "Squeakie" RF Field Strength Meter - Peter Parker VK3YE (Part 3)

I was not satisfied with the functioning and build of the veroboard "Squeakie" Field Strength Meter described in Part 2.  I decide...