Showing posts with label Propagation. Show all posts
Showing posts with label Propagation. Show all posts

Wednesday, April 15, 2026

UPDATED: ZS1I WSPR Beacon now active on 10 Meters from Mossel Bay, Southern Cape, South Africa


(Click on the image for larger view.) 

UPDATE 19 April 2026:  The ZS1I WSPR Beacon frequency was changed back to 40 Meters.  The standard 40-meter WSPR (Weak Signal Propagation Reporter) beacon dial frequency is 7.0386 MHz (USB/dial) or 7.0401 MHz (dial). The actual WSPR signals are transmitted in a 200 Hz window, typically placing the center of the transmissions around 7.0401 MHz, using USB mode.

The current WSPR (Weak Signal Propagation Reporter) beacon is set up to transmit low-power signals to monitor global radio wave propagation paths over extended periods, providing data to visualize which radio bands are open and how they are performing
. It's used by amateur radio operators to study atmospheric conditions, test antennas, identify optimal bands for communication, and contribute to a global database of propagation information without requiring manual operation.

I have decided to change the Band / Frequency of the WSPR Beacon currently in operation from Mossel Bay in the Southern Cape.  It was running on the 40 Meter band from  7 October 2025 @ 10h00 SAST to the 15 April 2026 @ 08h00 SAST.  From the 15 April 2026 09h00 SAST it will be transmitting on the 10 Meter band until further notice.

Particulars of the ZS1I Ultimate 3S Beacon active on 10 Meters:

  • Call: ZS1I
  • Freq. Band: 28.126 000 Mhz
  • Dial Freq. :  28.124.600
  • Band:  10 Meters (28 Mhz)
  • Grid:  KF15BT
  • Power:  250 mW
  • Mode: W-2  (WSPR2)
  • Antenna:  EFHW (49:1 Balun)
  • TX Period:  Every 10 Minutes
  •  Beacon on the air from:  15 April 2026 @ 09h00 SAST
  •  First Spotter:??????  (Who will it be?)

Spotting reports are welcome for 10-meter WSPR beacons, as this band is frequently active and highly dependent on daily propagation changes. WSPR (Weak Signal Propagation Reporter) is frequently used to test HF antenna performance at low power (e.g., 200mW to 5W), with reports uploaded globally.

How to Spot and Report 10m WSPR
  • WSPRnet.org: The primary database for all WSPR spots. Data can be analyzed in real-time.
  • WSPR.rocks: A fast, interactive site for searching WSPR data.
  • WSPR Watch (iOS App): Useful for monitoring where 10m beacons are being heard in real-time.
  • PSK Reporter: An excellent tool to visualize real-time propagation maps and see who is hearing your beacon.
  • 10m Frequency: WSPR 10m activity is usually found around 28.1246 MHz (USB dial frequency).
Key Considerations for 10m WSPR
  • Propagation: Even when the 10m band seems quiet for voice (SSB), WSPR can show open paths, particularly as the sun moves toward solar maximum.
  • Timing: An accurate clock (GPS-synced) is essential, as transmissions start 1 second into an even UTC minute.
  • Reporting Frequency: Even very low power (10mW - 20mW) can yield significant DX on 10m.
Finally:  I am looking forward to receive spotting reports of the ZS1I 10m WSPR Beacon active from Mossel Bay, South Africa. 

 

Wednesday, March 18, 2026

Update: Next Generation Amateur Radio Beacon (s) for the Southern Cape!! (Part 3)


This past two weeks I have been working on two more beacons.  Both beacons are for the 6m Magic Band.  You can read more HERE about the ZS1I 6 Meter Magic Band Project in the Southern Cape Area of South Africa.

Herewith a short update on the progress made with regards to the two 6 Meter Amateur  Radio Beacons: 

1.  Antennas:

The antennas for the 6 Meter CW Beacon and the 6 Meter WSPR Beacon has been built and tested with my SWR Analyzer.  More information available HERE and HERE about the antennas.

The 6m Delta Loop Antenna was installed and is ready for operation.  The 6 m Moxon Antenna is now ready to be installed hopefully in the next few days.  More on this once the Moxon antenna has been installed.

2.  6 Meter CW Beacon:

I have been working on and off on the beacon the last week or two.  I ran into a few software snags one being the fact that no RF power was generated by the SI5351.  Although the Arduino Nano, OLED, LED and Beeper was fully operational I could not get any RF signal from the SI5351.  Fault finding revealed that I had a small solder bridge at CLK0.  I removed the tiny bridge but still no RF signal.  The only other area to look at was the Arduino Sketch (firmware program) installed on the Arduino Nano.  To look at the sketch I had to access it via the Arduino IDE and guess what I ran into port issues to program the Nano.  Well all the issues took some time to fix.  I changed the sketch several times and than ran the beacon.  I managed to get RF output at CLK0 but now the OLED was not working.  This also took some time to sort out.  Eventually "Old Murphy" left the Workbench and Shack and the 6m CW Beacon was fully operational with +- 5 Mw output at CLK0.  Success at last!

3.  6 Meter Low Pass Filter:

As the SI5351 puts out a square wave signal, I needed to construct a 6 m low pass filter to keep the harmonics (if any) at bay.  You will need this filter!  Luckily I had the parts available in my junk box.  So the filter was constructed and tested.  It works as it should and I did not detect any harmonics after testing the unit.

4.  6 Meter Power Amplifier:

The current 5 Mw RF output of the beacon is way to little power and I decided to construct a 6m amplifier designed by the late Doug DeMaw  W1FB.  More on this once I constructed the amplifier.

Well once the amplifier is constructed and working as it should, all the modules will then be built into a cabinet and the beacon will be put on the air.

5. ZS1I 6m WSPR Beacon  (STILL UNDER CONSTRUCTION):

I uploaded the firmware (sketch) into the ESP32 S3 N16R8.  Apart from this no other work has been done to the 6m WSPR Beacon.  More information on this beacon will be provided once I finished the CW Beacon Project.

Finally:  

Please take note that these projects do take some time and that I do not work on them all the time.   A lot has been done this far and I hope to have the 6m CW Beacon on the air by the end of next week.  Updates to follow on the Next Generation Amateur Radio Beacon (s) for the Southern Cape.

Images:   (Click on images for larger view)












Friday, March 13, 2026

Building Low Budget Antennas - DIY Delta Loop Antenna for the 6 Meter Band ( 50 - 54 Mhz)


In this article I will describe how I built my version of the 6m Delta Loop Antenna for use with a 6m Beacon.  But first let's look at some information relating to the Delta Loop Antenna.

    A delta loop antenna is a high-efficiency, full-wavelength, triangular-shaped wire antenna known for low-noise, excellent DX (long-distance) performance, and low-angle radiation. It is typically fed with coaxial cable using a 4:1 balun or a 75 Ohm Quarter-Wave Transformer for impedance matching, configured with one apex up or down, and can be horizontally or vertically polarized depending on feed point placement.
    Key Features and Design Aspects:
     
  • Structure: A full-wave loop (total length in meters = 306 divided by Frequency in Mhz
    ) formed into a triangle.
  • Versatility: It can be configured as apex-up or apex-down, or even laid flat (horizontal) for NVIS (local) communication.
  • Polarization: Feeding the antenna at a corner or the bottom side generally results in vertical polarization, ideal for DX. Feeding it at the center of the base can produce horizontal polarization.
  • Performance: Offers low-noise reception compared to dipoles, making it ideal for urban environments.
  • Impedance: The feed point impedance is roughly 100-200 ohms, often requiring a 4:1 or 2:1 balun or 75 Ohm quarter-wave transformer for a 50-ohm match.
  • Multiband Capability: Can be used on harmonics with a tuner, though it is fundamentally a single-band antenna.
Key Benefits of Delta Loop Antenna:

 A Delta Loop antenna is quieter, providing roughly 2–3 dB more gain than a dipole, and offering excellent, low-angle radiation for DX (long-distance) contacts.   They are versatile for mounting, often requiring only one high support point, and are less sensitive to ground quality than vertical antennas.

  • Lower Noise Floor: Because they are closed loops, they are much quieter and less susceptible to environmental RF noise compared to open-ended antennas like dipoles or verticals.
  • Superior Gain and Performance: Delta loops offer higher gain (roughly 2-3 dB) compared to a standard dipole. They function effectively as stacked, bent dipoles, especially when oriented vertically.
  • Excellent for DX (Low-Angle Radiation): When vertically mounted, they produce a low-angle radiation pattern, which is ideal for long-distance communication.
  • Easy Installation: They generally only require one high support point (such as a tree limb or mast) to hang, making them easier to deploy than horizontal loops or complex beam antennas.
  • Wide Bandwidth: They are typically broad-banded and often allow for operation across a wide SWR range without a tuner.
  • Versatile Polarization: Depending on where they are fed (top, bottom, or side), they can provide either horizontal or vertical polarization.
  • No Radial System Required: Unlike traditional vertical antennas, a delta loop does not require a complex, extensive ground radial system.
  • Multi-band Potential: A single full-wave loop can be used on its fundamental frequency as well as higher harmonics, increasing its versatility.

Key Disadvantages of a Delta Loop if not installed correctly: 

Delta loop antennas, while efficient, have several disadvantages, including requiring significant height and complex, multi-point support structures.  They are generally limited in multi-band performance and can be very narrow-banded, making them less versatile than other antennas. Additionally, they are highly dependent on ground height for optimal, low-angle performance.

  • Complex Installation: They require more involved installation compared to dipoles, demanding a tall, sturdy support structure.
  • High-Angle Radiation/Limited DX: If not placed high enough (ideally at least a 1/2  wavelength above ground), they can favor high-angle, NVIS (Near Vertical Incidence Sky-wave) propagation rather than the low-angle radiation needed for long-distance (DX) communication.
  • Narrow Bandwidth: They often have high-Q, resulting in a very narrow operating bandwidth, which can limit performance outside of the designed frequency.
  • Limited Multi-band Performance: While they can work on harmonics, their performance, impedance, and radiation patterns can become unpredictable, making them less ideal for multi-band use. 
  • Large Size & Wind Load: They are physically large, increasing wind loading and making them more susceptible to weather damage.
  • Impedance Mismatch on Harmonics: Their feed point impedance can swing wildly on frequencies other than the primary design frequency, requiring a good antenna tuner.

In any project one needs a plan, diagram, guidelines and information.  At least that is my way of constructing any DIY Project.  I research the project thoroughly before I start any work.  I did exactly this before I started on this project.

Now the Internet is your friend but can also be your enemy if you just jump in and start constructing the first plan you find.  I was looking for the dimensions of a DIY 6m Delta Loop Antenna and ran into an abundance of information which included a calculator.  

The dimensions for the antenna was calculated using the free  Calculator program available HERE ). I set my frequency to  50.000 MHz as this antenna needs to resonate in the 6m CW beacon frequency allocation section. The resulting calculations is shown in Image 1 and 2 below. 


Image 1 and 2  (Click for larger view.)

The calculator was fed with the information to the left of the antenna drawings above.  Needless to say my dimensions differ slightly from those provided by the calculator.  This is mainly due to several inputs that changed due to the way I constructed the antenna and also the parts I used.  The calculator however provides good information when building a Delta Loop Antenna.  I decided to use the good old antenna formula to calculate the dimensions of the antenna I constructed.

Image:  Final calculator measurements  (Click on image for larger view.)

Formula for full-wave loop antenna:

Full-Wave in Meters   =  306  /  Frequency in MHz

       6.12 meter            =  306  /  50.000 MHz

       6120 mm              =  306  /  50.000 MHz

Formula for Impedance Matching Transformer:

Quarter-wave matching section length in Meters  =  75* cable's velocity factor / frequency in MHz

       99 cm      =    75 x 0.66  /  50 000 MHz

       990 mm   =   75 x 0.66  /  50 000 MHz

Materials that I used:

6100 millimeter x 2 mm PVC Insulated Copper Wire
2200 millimeter x 25 mm PVC Electrical Conduit Pipe
2200 millimeter x 22 mm Wooden Dowel (Fits into the 25mm  PVC Conduit Pipe to stiffen the pipe.)
2 x 25 mm PVC End Caps
3 x 10 mm Stainless Steel Self Tapping Screws.
1 x SO239 Connector
2 x Electrical Eye Lug (Terminal)
2 x 45mm x 5mm Stainless Steel Bolts + Washer + Lock Nuts
2 x 15mm x 3mm Stainless Steel Bolts and 2 x Lock Nut
2 x Stainless Steel TV - U Clamps
2 x Stainless Steel Pipe - U Clamps
1 x 150 mm x 100 mm x 5mm Aluminum Flat Plate to mount PVC Pipe to the mast for support.
1 x 1.5 m RG59 CU Mil-Spec Coax Cable (75 Ohm)
8  x 300mm x 4.6 Hellermann Cable Ties
6 meter 3 mm Nylon Rope to support the PVC Pipe fitted tot the mast

Odds and Sods:

Hot Glue Sticks
Self Amalgamating Tape
Solder
Solder Paste
Marine Silicone Sealant
Heat Shrink Tubing
 
Tools:
 
Metal Punch
Drill
Various Drill Bits 3mm - 8mm
Hack Saw 
Hot Glue Gun
Soldering Iron
Screw Driver (Small flat)
Alen Keys 
Spanner Set
 
Test Equipment:
 
SWR Meter
Antenna Analyzer (If you have one but not compulsory)
Amateur Radio Transceiver
Coax Patch Leads
Mast (Non conductive)
Coax feed line cable  12 m  RG58CU 50 ohm
Power Supply for Radio 

Building the Antenna:

My final dimensions is listed in the image below:


 

I am not going to go into detail how I constructed my version of the antenna. I will however describe my findings in constructing and testing the antenna.  The images below provide good detail of how I constructed the 6 m Delta Loop Antenna.

My build observations and findings:

Pointing Up or Down:  The Delta Loop can be orientated so that it is pointing up or down. The advantage of having the apex at the top is that it may be be more mechanically secure as the antenna hangs from a single point. The advantage of having it pointing down as in the diagram above is that it means the maximum current part of the antenna is slightly higher above ground level.

Mast Material:  The support for the Delta Loop should be a PVC or Glass Fiber pipe or a similar material. A metallic mast running through the center of the Delta Loop will probably de-tune it.

Feed point impedance and coaxial matching section:  The feed point impedance at the design frequency is about 100 ohms, so full wave loops are often fed with an impedance-matching section made from a piece of 75 ohm RG59 coaxial cable, one quarter wavelength long.

Length of an impedance-matching section with 75 ohm cable with a velocity factor of 0.66:  The most important thing with the matching transformer is the length of the shielded part.  It must be 990 mm long.  Here is how I cut the transformer cable (RG59).  Cut a piece with a length of 1050mm and remove 30mm of the PVC-coating from each end.  I then wound the braid together and remove the small piece of isolation from the center.  I tinned the wires and then constructed the "dummy balun" from 40mm PVC pipe and end caps plus a few screws, washers and bolts.   See images below of how I built the matching transformer.

The wire for the loop is simple 2 mm PVC coated wire used in household electrical wiring.  Each end of the antenna is fitted with an electrical eye lug that is screwed to the matching transformer.

The antenna is horizontal polarized with a final SWR of 1.15  :   1 @ 50 Ohm Impedance.  The antenna wire is adhered to the PVC pipe and top apex by means of cable ties.

The antenna is not yet at it's optimal height.  I am waiting for my son to assist me in adding the second mast section to bring the antenna to a height of  at least 9 meters.  This article will be updated with images when I extended the mast length.

The wooden dowel is kept in place by 3 Stainless Steel Self Tapping Screws while the matching transformer is kept in place by 3 cable ties.

The two nylon lines running downwards towards the mast is to keep the 25 mm PVC pipe secure during strong wind storms.  You need not install these but where I live we experience gale force winds from time to time.

If the antenna is mount with a feedpoint-height of 10 m above ground we get a elevation diagram as follows:  (Images courtesy of DK7ZB -  110-Ohm-Delta-Loops for 2 m, 4 m and 6 m)

 



Preliminary Tuning Result:  1.37 : 1 SWR @ 49.9 Ohm Impedance

Final Tuning Result:  1.15  :  1 SWR @ 50 Ohm Impedance

Good enough for me!!

Use of the 6m Delta Loop Antenna:

This antenna will be used for the 6m CW Beacon that are in the final stage of construction.  More on this in a future article.

Finally:  

The 6 m Delta Loop is a pretty easy antenna to construct and most of the material can be obtained at a local hardware store. It's an easy way to get an antenna with a small amount of gain well above ground level.

Images (Click on images for larger view.)



















Sunday, December 14, 2025

Feedback: WSPR Beacon to monitor propagation conditions from the Southern Cape (Part 3)


In Part 1 - HERE and Part 2 - HERE we looked at:

Why would one setup a WSPR Beacon in the Southern Cape?  

Particulars of the ZS1I Ultimate 3S Beacon.

Construction of the Southern Cape Beacon.

First station to spot the ZS1I WSPR Beacon on 40 Meters.

Reception of the ZS5SAM WSPR Beacon on an SDR and Antenna inside the Shack and other spotting stations that received the ZS1I WSPR Beacon on 40 Meters.

In Part 3 I will be looking at two Antarctic Research (WSPR) Stations that spotted the ZS1I 40 M WSPR Beacon recently.  One fixed station and one a maritime mobile station.


Station 1:   DP0GVN Antarctica flag Antarctica

Neumayer Station III
Ekstroem Ice Shelf
Atka Bay, Dronning Maud Land
Antarctica


Station 2:  DP0POL Antarctica flag Antarctica

Research Vessel "Polarstern"
Home Port: Bremerhaven
Germany

Both the above stations spotted the ZS1I WSPR Beacon on 40 Meters on the 14 December 2025.  See image below.


DPØGVN is a club station located at the German Antarctic Research Station "Neumayer III" in Dronning Maud Land, Antarctica. Find more on this outpost of global research at https://www.awi.de/en/expedition/stations/neumayer-station-iii.html. 

WSPR Beacon

  • Station Info

The setup consists of a receiver and a transmitter which independently of each other operate in the WSPR segments of the amateur radio HF bands.

  • Receiver

The receiver is located at the "SpuSo" which is the station's air chemistry laboratory. SpuSo's main purpose is to collect continuous, year-round and long-term data records for important gaseous and particulate trace components of the troposphere. This observatory is located about 1.5 km south of the main station where it finds an outstandingly clean air environment.

This is a perfect place for a receiver setup because the RF environment, too, is amazingly  QRM-free with a noise floor well 20, 30 or even more dB below of what we are used to in urban areas.

The receiver is a SDR built around three Red Pitaya (StemLAB 125-14 with 50 dB preamplifier). They permanently observe all eleven WSPR band segments between 160m and 6m and upload the spots to wsprnet.org. A BananaPi and a RaspberryPi single board computer take care of control tasks.

The antenna setup consists of two two triangle-shaped horizontal loop antennas with 1:4 baluns. The lower bands are received by an antenna with a circumference of 171 meters, the upper bands use a shorter loop of 61 meters.

The antennas are mounted on short masts about one to two meters above the ice shelf. This is not "above ground" as the ice shelf is almost invisible to HF. You even can use antennas lying flat on the ice to do HF QSOs! The real ground is about 200 meters below as this is the average thickness of the ice shelf in this area. Every year precipitation adds about one meter of snow and ice. Therefore the antennas have to be reestablished regularly to not risk having them covered by snow.

  • Transmitter

The transmitter is located at the main station and is based on the TX design of the Charly-25 SDR project. Ats it heart is another Red Pitaya StemLAB 125-14 which feeds a rock-solid PA designed to emit up to 20 watts RF. The Red Pitaya runs Pavel Demin’s WSPR transceiver software. A PC Engines APU2 single board computer is in charge of control and monitoring tasks. RF output, SWR and system temperature are constantly monitored.

The antenna is an approx. 20 meter long wire installed on the southern part of the station’s roof. The wire runs in North-South direction and is matched by a 1:9 Unun-type RF transformer. While not being a high-performance antenna it is well suited for the task because it is broad band and believed to be able to stand the stress caused by the extreme Antarctic whether conditions.

The transmitter transmits on all WSPR segments between 160m and 6m on a round-robin schedule. One complete cycle takes 30 minutes. The bands between 40 and 17 meters are served twice per cycle because these offer the best chances for the signal to be heard. So these four bands are visited four times per hour, the other bands twice per hour. The RF output is 5 watts on all bands.

Update June 2020: On 2020-06-04 something in the RF transformer feeding the long wite antenna broke causing the antenna to be unusable. Therefore we are currently transmitting with the 5.5m vertical antenna which was already in use for the project before 2020. This antenna offers a less favorable radiation pattern when compared to the long wire, so expect somewhat degraded reception opportunities. Maintenance work at the antenna can only take place during Anarctic summer so that the repair will not be executed before January 2021.

  • The Project

This setup is a long-term project realized by the Technical University of Munich (TUM) and the Hochschule Bremen City University of Applied Sciences (HSB) in cooperation with the Alfred Wegener Institute Helmholtz-Zentrum für Polar- und Meeresforschung (AWI) and the German Amateur Radio Club (DARC). AWI operates the Neumayer Station III and provides logistics. DARC builds and maintains the receiver and transmitter setup.

The project is meant to run several years to gain long-term data on radio propagation and spectrum pollution in a very specific HF environment as the station is located within the southern auroral oval. The setup will see changes in the future -- we will keep you updated here. As the station is inaccessible from the outside world for about eight months during south polar winter modifications will usually happen during the Antarctic summer season between November and February.

DP0POL is only operated from the vessel when it is en route in international waters, so the call sign always is DP0POL/mm.  You can follow the ship's research activities in our Polarstern Web App. For the ship's current position, please check the SEAICE portal.

I made two adjustment on the ZS1I Beacon and it is now running flawlessly.  Before I had to "reboot" the beacon every second day. Since the setup adjustments I just left the beacon and it operated continually.

In Part 4 we will be looking at changing the band and frequency as what the beacon was intended for.  More on this in Part 4.

Images:  (Click on the images for larger view.)








Closure of this ZS Link Network Blog - 29 April 2026

This will be the final posting on the ZS Link Network Blog. This blog will no longer be updated but will remain available for research an...