The next meeting of the Amateur Radio Experimenter’s Group will be held on Friday June 17th starting at 7.45pm. It will be held in person at the Fulham Community Centre, Phelps Court, Fulham.
Our guest speaker will be Michael VK5LN who will talk about his experiences bringing back to life one of the iconic home computers of the 1980s,the Commodore C64! Whats more, he will show us how he has built a new C64 from scratch using the resources of the modern day retro-computing movement, which is very much alive in 2022!
The record breaking Commodore 64 computer that dominated the home computer market in the early 1980s is still going strong 40 years later! There is an endless stream of new software and hardware being developed. During its production life there were a number of different PCB revisions and each has been reverse engineered and gerber files produced so you can build your own Commodore 64 with new components. While you still need some original semiconductors in order to home brew a Commodore 64, there are modern replacements to help out.
My original 1983 Commodore 64 is still working (after needing a few repairs after being in storage for 30 years) but there is something magical about building your own retro computer.
The meeting will be held in a hybrid in-person/online format with Michael attending by remote from Port Lincoln while the live audience will be both in the hall as well as online via Zoom for members. (non members please stay tuned as we sort out if we can Youtube Stream the meeting as well).
Following the presentation there will be the usual business meeting and opportunity to catch up with AREG members in person and online. We look forward to seeing you all come along!
AREG is pleased to announce that is now one step closer to returning a digital voice DMR repeater service to the Adelaide metropolitan area.
Members voted to support the project earlier this year, after a call for interest in re-establishing a DMR service was made in July 2021. Since then, a DMR repeater has been donated to the club by Andrew Chapman VK4QF (one of the leading lights behind multiple DMR projects around Australia). We offer our sincere thanks to Andrew for his generosity!
Preparations are now well advanced to install it up at the club’s digital repeater site – VK5RWN atop Anstey Hill, which overlooks the Adelaide Plains. This is the same site used by the current D*STAR repeater. Paul VK5BX has been able to source and build a multi-coupler/diplexer for the club, to enable the DMR and D*STAR repeaters to be combined onto the same antenna system. The repeater will, once activated, operate on 438.900MHz (with a -7MHz offset).
Timing of the final install is now subject to weather and availability of members for the working bee required to complete the installation (which includes some rearrangements to the UHF repeater antennas on site to accommodate the multi-coupling). It is our objective to have the system operating in the next 6-8 weeks, (earlier if everything falls into place).
Why DMR?
AREG has always been supportive of experimentation and providing opportunities for radio amateurs to try new things and to find new ways of communicating. This is what drove AREG to support the original D*STAR repeater system (then co-sponsoed by Icom and WIA now solely maintained by AREG).
In the case of DMR, AREG considered providing a service after the unexpected closure of the original Adelaide DMR repeater – VK5RSF, which saw the end of all DMR repeater access in the Adelaide region. With an existing KernWi-Fi internet served site covering the metropolitan area (VK5RWN), AREG was also well placed to support the Adelaide DMR community, and in particular its own members who were interested in DMR. This was all the motivation needed!
More information on DMR and the VK-DMR network in Australia can be found via the vkdmr.com website. Keep watching the AREG website too for further news about the final commissioning date for VK5RWN on 438.900
How can you get involved?
The best way to support the new service and to get involved is to become a member of AREG! Your membership will help connect you with other amateurs interested in DMR in Adelaide, as well as helping offset the costs of running the service, particularly the internet link and power used to run the system. Details of how to apply for membership are available (here)!
AREG is planning a new event on the SA Amateur Radio calendar.
Saturday September 3rd will see the first running of our (hopefully annual) Amateur Radio & Electronics Sale. It will be held at the DogsSA Training Facility in Kilburn as a car boot sale format. We will be inviting all of the SA Radio Clubs to participate as well as a number of commercial vendors!
More details will follow in coming weeks – but for now you simply need to:
The next monthly AREG fox-hunt is scheduled for this coming Friday night, the 13th of May, with hunters meeting from 6:15pm at the Adelaide Aquatic Centre car park.
This hunt will again see our usual two 2m (145.3 MHz, 144.390 MHz) and as well as our 70cm foxes (439.4 MHz) deployed somewhere within the Adelaide metropolitan area. The hunt kicks off with the transmitters being activated at 6.30pm.
Liaison will be via the Summertown (VK5RSB) UHF Repeater on 439.900MHz (-5MHz Input with 91.5Hz CTCSS).
As usual, everyone is welcome to join in on the fun, you don’t need to be a member of AREG to participate. We hope you can make it!
Horus 57 was the first ‘large’ Project Horus high-altitude balloon launch in over a year, and was aimed at getting more stations involved in receiving the common telemetry and imagery systems used on our launches, and at the same time try and get some nice imagery of our state from the air!
The launch was originally scheduled for the 1st of May, but weather conditions resulted in the imagery launch being bumped a week, and a small telemetry launch taking its place. The telemetry-only flight was very well received, with 37 unique stations contributing telemetry, building anticipation for the full-scale launch, which was performed on Saturday the 7th of May at 10AM.
The Payloads: Wenet Imagery
The main payload on this launch was a Wenet imagery payload. Wenet is an imagery downlink system first developed by David VK5DGR and Mark VK5QI in 2016, to enable high resolution imagery to be downlinked from a balloon launch. It uses Frequency Shift Keying (FSK) at 115kbit/s to send specially encoded JPEG images which can be reassembled from packets received by many spatially diverse receivers. It’s also completely open source, so anyone can have a go at using it!
This particular Wenet payload was testing a camera lens made by ArduCam, in the hope of obtaining higher quality imagery. Unfortunately this lens de-focused as the temperature of the payload dropped during flight, resulting in many blurred images. We’ll be switching back to the tried-and-tested Raspberry PiCam v2 for future flights of this payload.
The Payloads: Tracking & Flight Management
The flight also included the usual complement of telemetry and flight management payloads. Primary telemetry was provided by a reprogrammed RS41, transmitting the ‘Horus Binary‘ 4FSK mode on 434.200 MHz. This was received by a large number of amateur stations running the ‘Horus-GUI’ demodulation software. Tracking of the payload was available on the SondeHub-Amateur tracker online, allowing global access to the position of the balloon throughout the flight.
The separate flight management payload was a LoRa-based payload operating in the 70cm amateur band. This payload allows remote termination of the flight if necessary (and it was very nearly used on this flight!).
The Payloads: LoRaWAN Beacon
Also on this flight was an experimental LoRaWAN tracking payload built by Liam VK5LJG. The aim was to transmit position beacons into ‘The Things Network‘ (‘TTN’), which has gateways (receiver stations) in many locations across Australia. This payload previously flew on Horus 55.
The payload operated on the 915-928 MHz LIPD band, with a transmit power of ~50mW. The hardware was a RAK Wireless RAK5205 board, running custom firmware for the flight. Position updates were only sent every ~3 minutes to comply with TTN fair-usage guidelines.
Unfortunately this payload stopped being received approximately 30 minutes into the flight, due to a misconfiguration. We’ll try this again on another flight!
Launch!
The launch crews arrived on-site at the Mt Barker High School oval around 9AM on the Saturday morning, and started preparations for launch. The entire preparation process through to launch was documented by AREG club member Iain VK5ZD:
This flight used a Hwoyee 1600g balloon, one of the largest balloon sizes we regularly use. Since the combined payload mass was relatively light (~600g), a relatively small amount of gas was required, resulting in the balloon being quite under-inflated, and prone to wind drag.
Immediately after launch, it was noted that the ascent rate was lower than the expected 5 m/s, a direct result of the increased drag on the under-inflated balloon.
Thanks to all that helped out at the launch site! It was great to see some new faces, and the many hands made the launch much easier.
Starting the Chase
Original Horus 57 Flight-Path Prediction
The original flight path prediction had the flight landing somewhere off the Stott highway, between Swan Reach and Loxton. However, the slower than expected ascent rate after launch meant the live flight-path predictions began to move further to the east.
The chase teams for the day consisted of Mark VK5QI and Will VK5AHV, and Gerard VK5ZQV.
The chase teams immediately headed off towards Swan Reach, and met up with some members of the Riverland Radio Club who had setup a receiving station for the imagery payload near the locality of Maggea. Peter VK5PE, Colin VK5CBM, Andy VK5LA, and Ivan VK5HS with his grandson Reece had decided to head out to setup near the predicted landing area and have a go at receiving imagery. This was their first time receiving the Wenet imagery payload, and so had brought along a lot of equipment to experiment with!
Riverland Radio Club Portable Receiving Station
There was also many other stations that had gone portable to receive the Wenet imagery. Peter VK5KX was setup near Sanderston with a WiMo X-Quad antenna and tracking rotator system, and Andrew VK5LA setup north of Swan Reach with a 15-element yagi. Andrew VK5CLD was also setup near Mt Barker summit with a homebrew 8-element yagi.
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Burst & Recovery
As the flight progressed, the reported altitude reached the expected 38000 m, and kept on rising! Unfortunately for the chase teams, at this altitude the balloon and payloads were heading east at 150 kph, and the predicted landing location with it, and so they had to get back on the road and continue onwards.
There was a tense period as the predicted landing location moved right across the Murray River, before finally moving further onwards to the east of Loxton. Around this time the flight continued on upwards, passing through 39000 m altitude, then finally 40000 m.
The ascent rate slowed down considerably above 40 km altitude, and there was a short time when the use of the cutdown payload was seriously considered to avoid the payloads ending up across the Victorian border. This ended up not being necessary though, as the balloon burst for a maximum reported altitude (based on the Wenet telemetry) of40246 m! This is most likely the highest altitude ever reached by an amateur balloon launch in Australia!
Wenet Imagery from 40205m altitude!
The payloads then began to plummet back to earth (a peak descent rate of 114 m/s was observed just after burst!) and ended up landing in a newly seeded paddock approximately 15 km to the north-east of Loxton.
Horus 57 Flight Path
After obtaining permission from the landowner, the chase teams were able to carefully drive into the paddocks and recover the payloads.
The Wenet imagery payload was still operating, and captured the recovery and walk back to the car:
Wenet Imagery!
All the way through the flight, the Wenet payload continued to transmit live imagery to many receiving stations around the state. Unfortunately the new ArduCam lens shifted in focus due to the extreme cold temperatures experienced during the flight, resulting in most of the imagery above 3 km altitude being blurred. The lens appeared to recover around the peak of the flight, but then degraded again on descent before recovering after landing:
Wenet Imagery from 40205m altitude!
Wenet Reception Statistics
This flight saw the highest number of Wenet receiver stations ever, with 14 separate receiving stations contributing imagery packets. As a result, we had 100% image reception over the vast majority of the flight! This is a great result, and allows those watching from home to experience our high-altitude balloon launches in near real-time.
The following amount of data was contributed by each station:
VK5LA: 205297 packets (50.12 MB)
VK5KX: 179744 packets (43.88 MB)
VK5QI-1 (Home): 160507 packets (39.19 MB)
VK5CBM: 145899 packets (35.62 MB)
VK5PW: 134465 packets (32.83 MB)
VK3TNU: 134264 packets (32.78 MB)
VK5APR: 157585 packets (38.47 MB)
VK5EME: 146062 packets (35.66 MB)
VK5QI (Mobile): 131933 packets (32.21 MB)
VK5HS: 104472 packets (25.51 MB)
VK5CLD: 47650 packets (11.63 MB)
VK5IS: 21995 packets (5.37 MB)
VK5TRM: 16950 packets (4.14 MB)
VK5FJGM: 5355 packets (1.31 MB)
Horus 57 Wenet Receiver Map
While most of the receiver stations were relatively close to the flight path, we also saw Ian VK5IS receiving from 160km away, and Tim VK3TNU receiving from over 300km distance! Tim was using a 9-element RFI yagi, paired with a RTLSDR and preamplifier, and has set the new record for Wenet reception distance!
The following plots show the percentage of each image that was received by each receiver station:
We also saw a huge number of Horus Binary receiving stations come online for this flight, with stations as far away as Melbourne contributing telemetry. A total of 41 unique callsigns were observed to upload telemetry throughout the flight, which is also a new record for a Project Horus launch!
A huge thanks to everyone that contributed to the flight tracking, and we hope to see you on the map on future launches!
Detailed statistics for each receiver are available in the table below:
Callsign
Received Packets
Percentage of Flight Received
First-Received Altitude (m)
Last-Received Altitude (m)
VK3BQ
346
14.0%
28056
22885
VK3DNS
88
3.6%
34109
38312
VK3EEK
45
1.8%
33822
36313
VK3ER
5
0.2%
34374
34470
VK3GP
156
6.3%
32298
5773
VK3IRV
224
9.1%
38516
35917
VK3KZM
153
6.2%
37802
35134
VK3MD
496
20.1%
30032
25910
VK3MTV
1964
79.5%
5740
1233
VK3TNU
1755
71.1%
7858
5469
VK3TOS
123
5.0%
33418
26680
VK5AKH
136
5.5%
1529
35569
VK5AKK
2327
94.2%
366
2674
VK5APR
1879
76.1%
1062
7080
VK5BRL
552
22.4%
39251
103
VK5CBM
910
36.9%
11305
34184
VK5DJ
1668
67.6%
5920
7698
VK5DMC
1165
47.2%
4678
29733
VK5EI
1627
65.9%
6025
22298
VK5FD
2180
88.3%
1074
7979
VK5FJGM
2075
84.0%
951
10397
VK5GA
2037
82.5%
1268
16657
VK5GY
1981
80.2%
2838
8713
VK5HI
2187
88.6%
978
6851
VK5IS
2084
84.4%
1568
5469
VK5KX
2418
97.9%
645
369
VK5LA
2374
96.2%
790
1011
VK5LJG
2178
88.2%
523
8136
VK5LJG-9
1292
52.3%
854
3455
VK5LN
1770
71.7%
4401
14119
VK5MAD
560
22.7%
854
9830
VK5MAS
388
15.7%
16694
40115
VK5NEX
1972
79.9%
3055
7659
VK5NTM
2360
95.6%
1189
655
VK5PE
1633
66.1%
2685
39540
VK5PE-9
1525
61.8%
7485
747
VK5QI-1
1935
78.4%
1529
10201
VK5QI-9
2071
83.9%
344
58
VK5RK
1576
63.8%
9645
6597
VK5RR/VK5FO
1891
76.6%
2536
369
VK5ST-0
2084
84.4%
2587
5348
VK5ST-991
1306
52.9%
3255
38937
VK5TRM
2354
95.3%
1402
103
VK5TRM-12
32
1.3%
36821
37624
VK5ZAI
1722
69.7%
8895
4908
VK5ZSH
678
27.5%
5549
39972
The SondeHub-Amateur Tracker
Horus 56 and 57 made use of the new SondeHub-Amateur tracker website to enable anyone online to follow the flight’s progress. This is an extension to the SondeHubRadiosonde tracker, which allows tracking of meteorological radiosondes, and is developed by club members Michaela VK3FUR and Mark VK5QI, along with many other contributors.
The SondeHub-Amateur tracker in action during Horus 57.
The next large Horus launch will likely be a re-flight of the DVB-S payload flown on Horus 55, with an improved payload antenna. This will likely need to wait until after winter, for clearer skies.
In the meantime, there are some initial plans for:
A re-flight of the LoRaWAN payload, though not to as high an altitude as on this flight.
Experiments with new sensors attached to our primary tracking payload.
Another Wenet flight, to give some more opportunities for listeners to refine their receiver setups.
This flight was a huge success, reading over 40km altitude! Thanks to all that were involved in the launch and received telemetry. A full writeup will be written in the next few days.
The re-attempt of the imagery launch intended for last weekend will now occur this weekendon Saturday the 7th of May, with a planned launch time of 10AM ACDT.
Update Friday 6th May: Launch is GO! With the ~25kph winds forecast for the launch site, we will likely be going with the larger balloon, to avoid having to perform accurate filling.
Weather predictions are still somewhat variable for Saturday, and the final GO / NO-GO decision will be made Friday evening, around 8PM. Check this post on Saturday morning for the final launch decision.
Depending on the weather conditions, we will be launching under either a 600g Hwoyee balloon, with an expected maximum altitude of 28km, or a 1600g Hwoyee balloon, with an expected maximum altitude of 38km(!). This will likely be decided on the morning of the launch based on wind conditions at the launch site. If we go with the larger balloon, the radio footprint of the launch will be approximately 1400km in diameter.
We will be launching from the Mt Barker High School Oval, with the launch team on-site from approximately 9:00AM. Visitors are welcome! Note that there are construction works around the entrance to the oval (off Stephenson Street), but the oval is still accessible.
Assuming the imagery payload works as intended (fingers crossed!), live imagery using the combined contributions of the ‘Wenet’ receiver stations will be available here: https://ssdv.habhub.org/VK5ARG
The predicted flight path (for 28km burst altitude) is currently as follows:
Primary Telemetry – 434.200 MHz
The primary tracking telemetry will be transmitted on 434.200 MHz using the Horus Binary 4FSK data mode. Amateurs in the Central SA region, and even those as far away as Melbourne are encouraged to get involved with the flight through receiving and uploading flight telemetry from our 70cm band tracking beacons. Every piece of telemetry data is valuable to the flight tracking and recovery teams so if you can help join the distributed receiver network to collect that data you will be making an important contribution to the project!
Note that you will need to use a ‘dial’ frequency of 434.199 MHz for the 4FSK signal to be centred in your receiver passband and hence be decodable.
Tracking Details – Imagery – 443.500 MHz
Imagery on this flight will be transmitted via the Wenet downlink system, which uses 115kbit/s Frequency-Shift-Keying to send HD snapshots. Reception of the Wenet imagery requires a Linux computer, a RTLSDR, and a 70cm antenna with some gain (a 5-element Yagi is usually enough).
Imagery received via the Wenet payload from a previous flight.
Due to adverse predicted weather conditions, the imagery flight planned for Sunday the 1st of May was replaced with a telemetry-only launch. A Vaisala RS41 radiosonde, re-flashed with ‘Horus Binary’ firmware was launched under a 200g Hwoyee balloon, with a planned target altitude of 27km. The aim of the flight was to give receivers in the Central South Australia area an opportunity to get set up to receive the flight telemetry using the ‘Horus-GUI’ software.
Launch team filling the balloon.
This launch was performed from the Mt Barker High School Oval, a common launch site used by the group. The site was a little breezy, which would have made filling a larger balloon a bit difficult, but with the small balloon it was no problem. Thanks to those that came along and helped out!
— Mark Jessop – @vk5qi@cloudisland.nz (@vk5qi) May 1, 2022
In retrospect, the weather would have actually been pretty good for imagery, but this was difficult to tell based on the predictions in the preceding days. We’ll try to launch the imagery payload next weekend (hopefully on Saturday the 7th of May).
Many New Receivers!
As the balloon and payload ascended, it was great to see many receiver stations coming online to contribute telemetry. The new SondeHub-Amateur tracker shows the signal-to-noise ratio that each receivers is seeing, so it was interesting to watch how this varied for the different receiver stations. There were a few bugs encountered on the tracker which should be fixed before the next launch.
Horus 56 being received by 36 stations simultaneously!
Over the course of the flight we ended up seeing telemetry from 37 unique callsigns, including many new stations, and a few we haven’t seen in a while. We also saw stations from as far away as Swan Hill and Horsham in Victoria, and Mount Gambier in the South-East of South Australia!
After the launch, a few of the launch team headed up to a lookout near Mt Pleasant to track the flight (and get some lunch from the Mt Pleasant Bakery!). As this was just a telemetry payload (and we have plenty of those thanks to the Bureau of Meteorology!) there was no attempt to recover it.
The balloon burst just under 25km, a bit short of the expected 27km, and came to land to the east of Bowhill.
Overall flight path of Horus 56
Flight Telemetry Statistics
The following callsigns uploaded telemetry during this flight:
Weather permitting, we’ll have another attempt at the imagery launch next weekend, on either Saturday the 7th, or Sunday the 8th of May (noting Sunday is Mother’s Day – we’ll try and avoid this if possible!). We’ll post more about this as weather predictions become available.
AREG wishes to announce that due to our regular meeting night falling on the Easter Good Friday holiday this year, the committee has agreed to reschedule the April meeting to Friday 22nd . The meeting will be held both in person at the club rooms, (Fulham Community Centre, Phelps Crt, Fulham) and online using Zoom starting from 7.45pm ACST.
This meeting’s presentation is titled: “VHF/UHF Contesting – A Trilogy in 2 parts”
Do you remember a time when operating below 50MHz required CW and specialised license privileges? Are you new to the hobby and unaware that VHF/UHF is used for more than just fox-hunting and repeaters? If so, come and join Matthew VK5ZM and Grant VK5GR as we explore contesting on the higher VHF/UHF bands. Perhaps this year is the year to dust off that shack-in-a-box radio you have stashed in a cupboard and come sit on top of a hill for an hour or two on a Sunday afternoon ? Curious then join us on Friday the 22nd of April.