Next Project Horus Launch – Horus 63 – 1st December 2024 – Cross-band Repeater – Mt Barker Launch!

AREG’s High-Altitude Ballooning sub-group, Project Horus, is planning their next launch for Sunday the 1st of December, with a planned launch time of 10 AM ACDST. If we have to scrub due to poor weather, the backup launch date will be the 8th of December.

UPDATE 27th Nov: This launch is currently planned to be performed from the Mt Barker High School Oval with the launch team arriving on site from around 9:15 AM. Note that access to the oval is via Stephenson street, and parking near the oval is extremely limited. 

TRACKING LINKS

This flight will feature a new cross-band repeater payload, enabling amateur radio operators around the state to communicate via the balloon! Along with this will be a newly built Wenet Imagery payload, using a PiCam v3 in autofocus mode.

  • FM Crossband Repeater: 145.075 MHz Input (91.5 Hz CTCSS), 438.975 MHz output.
  • Wenet Imagery on 443.5 MHz.
  • Primary Horus Binary telemetry on 434.200 MHz
  • Backup Horus Binary payload, on 434.210 MHz
  • TheThingsNetwork tracking payload, using the AU915 band-plan.

During the flight, all the payloads can be tracked lived on the SondeHub-Amateur tracker here!

FM Cross-band Repeater Payload

This is the first test flight of a new experimental FM cross band voice repeater based around a Yaesu FT-530 handheld transceiver.The balloon repeater should be heard on:

  • INPUT: 145.075MHz with 91.5Hz CTCSS
  • OUTPUT: 438.975MHz  – 0.5W into 1/2-wave omni

Please note that this repeater is experimental, and may have performance issues or even fail completely during the flight!

To transmit to the balloon at the maximum range of 800km (once the balloon reaches 100,000ft ++) you should only need approximately 10-20W and an 2-4dB gain antenna.

Receiving the balloon at 400km range in a handheld environment should be achievable, but to hear the repeater at the maximum range of 800km you should expect to need a 10dB gain Yagi for a 0.4uV capable receiver and 2dB feeder loss

This setup is much the same as the LEO satellites but without the doppler shift.

PLEASE MAKE SURE YOU CAN HEAR IT BEFORE YOU TRANSMIT!

This repeater will be operated as a controlled net, with the net control callsign VK5ARG – please listen out for net control before calling!

We will be offering QSL cards to stations that make a contact with net control during the flight, so get your stations setup and give it a go!

Primary Telemetry – Horus Binary 434.200 MHz – HORUS-V2

Reprogrammed RS41The primary tracking telemetry will be transmitted on 434.200 MHz using the Horus Binary 4FSK data mode. Amateurs in the Adelaide and Central SA region are also 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!

If you try receiving the telemetry from this flight, you’ll need a SSB-capable 70cm receiver (or a SDR), and the Horus-GUI telemetry decoder software. A brief guide on setting this up is available here: https://github.com/projecthorus/horusdemodlib/wiki/1.1-Horus-GUI-Reception-Guide-(Windows-Linux-OSX)

Listeners that already have Horus-GUI installed are encouraged to update to the latest version, which is available at this link.

Note that you will need to use a USB ‘dial’ frequency of 434.199 MHz for the 4FSK signal to be centred in your receiver passband and hence be decodable.

Backup Telemetry – Horus Binary 434.210 MHz – VK5ARG

A backup tracking payload will be transmitting on 434.210 MHz using the Horus Binary 4FSK data mode, and can be received in the same way as the primary tracking payload, with information above. For this payload you will need to use a USB ‘dial’ frequency of 434.209 MHz.

Wenet 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).

This payload will be experimenting with a PiCam v, which we previously flew with only partial success on Horus 59. This time around many software updates have been written, hopefully allowing the PiCam v3’s autofocus to work on a balloon launch. This flight aims to test out these software changes, and gather data to help improve performance on future launches.

Wenet imagery from Horus 62

A guide on how to get set up to receive the Wenet signal is available here: https://github.com/projecthorus/wenet/wiki/Wenet-RX-Instructions-(Linux-using-Docker)

Please note the transmit frequency of 443.5 MHz, which may require listeners to re-configure their Wenet setup. 

Note: Stations that are already ready to receive Wenet are advised to update to the latest testing version for this flight. See here for instructions: https://gist.github.com/darksidelemm/cdc36a90ca96b87d148fdd7d68d5d5fe

During the flight, the live imagery will be available at this link: http://ssdv.habhub.org/

TheThingsNetwork Payload – 915 MHz LIPD Band

This flight will also fly a LoRaWAN payload built by Liam VK5ALG, relaying positions via TheThingsNetwork (TTN), a global Internet-of-Things network with hundreds of receiver gateways across Australia. You can find out more about how TheThingsNetwork works here.

The aim of this payload is to test a new antenna, and try and beat our previous range records on the 915 MHz band.

Project Horus Balloon Project: Digital ATV DVB-T Terrestrial Testing – Success!

Today Mark VK5QI took the Balloon ATV transmitter out for a terrestrial test. He carried out line-of-sight testing of the DVB-S payload from BlackTop Hill to the AREG remote site near Tarlee – a distance of 54km!

First test – could he see the signal on the SDR up at the site (RTLSDR, Diamond X-50, no preamp)… yes!

Next, Mark dumped some samples with rtl_sdr, then transferred them back to his laptop. He processed them through leandvb – and got video!!! A bit of fading, but for an omni receiver with no preamp, this is a pretty damn good result!

… and here’s some of the raw video

The MER as reported by leandvb was around 8-11 dB, right on the edge of what is decodable. Still, with such a basic system, a good result!

Based on the path, it is estimated to give us a working range of about 150km from the balloon given a receiving station with 15dBi gain and a good low noise preamplifier.

Stay tuned for more information on how to receive and decode the Digital ATV signal and save the date – we hope to launch the transmitter into the stratosphere on Sunday March 7th. (We also plan on streaming the event on Youtube).


For those who missed it late last year here is a bit more information about the Balloon ATV payload and some minimum signal testing that was carried out.

HNY 2019: January Meeting – HF Remote SDRs & AREG’s Remote Site Project

Firstly, Happy New Year 2019 to everyone. This year promises to be yet another action packed fun filled series of events brought to you by the members of the Amateur Radio Experimenters Group.

Next Meeting – Friday January 18th – 7.45pm

The next meeting of the Amateur Radio Experimenters Group Inc will be held on Friday the 18th of this month. The topic of the evening will start with a short introduction to the world of remote HF SDR receivers and how to access them.

It will then be followed by a workshop event looking at the original AREG project intended to setup and host one of these systems here in Adelaide. The original project was plagued with problems, most notably getting an internet link out to the site some 40km away from VK5RWN. In the end we weren’t successful in getting the microwave link to be stable. The secondary issue of local site noise at the receive site was never even addressed because the internet feed couldn’t be resolved.

Now that 2019 is here, and the opportunity of a new site has presented itself (that solves the internet access issue), the club is looking for members to form a new team to try and complete the project. The second half of the meeting this month will explore what tasks need to be done to make this a reality and we will be looking for volunteers to put their hands up to help

Visitors are always welcome! The club meets at the Fulham Community Centre, Phelps Crt, Fulham from 7.45pm. The presentation starts at 8.00pm and will be followed by coffee and cake before a formal business meeting.

We look forward to seeing you all there!

AREG at Adelaide Maker Faire 2017 – Update!

AREG will again have a stand at the Adelaide Maker Faire on this weekend. The faire runs from 10am to 4pm this Sunday, at the Tonsley Innovation hub in Adelaide’s SE suburbs. The AREG team are planning on showcasing a raft of things that link making and building with Amateur Radio.

AREG is stand number 76!

What will AREG be doing?

 If you have ever wanted to find out more about our Project Horus high altitude balloon program, or radio direction finding, satellite tracking, home built magnetic loop antenna construction and much more then this is an ideal opportunity to come and talk to the club members about some of their regular activities and how they are always “Making Things” within the hobby of Amateur Radio.

One of the new projects on display will be the satellite tracker based on an earlier project by Joe VK3YSP and Julie VK3FOWL from SARCnet in Victoria. As an open source project, AREG members have been adapting it to track balloons based on the received GPS telemetry from our payloads.

 

So why not come on down! We would love to see you there. On site we hope to have a handheld listening on 439.025. We would also love to make QSOs with people on the VK5RSB 6m repeater (53.75MHz / 52.75MHz) which we will be accessing using a magnetic loop antenna from the site.

AREG’s New 160m/80m Contesting Portable Antenna – Progress

Update – July 12th: Mounting of the tuning capacitor and motor drive is complete. Just a few more things and we will be ready for final assembly and tune up!


A group of members inside AREG, inspired by Steve VK5SFA’s success with his transmitting magnetic loop antennas have banded together to construct for the club it’s own 160/80m TMLA, specifically designed to be portable. It is able to be knocked down into components that can be packed into the back of a station wagon.

Significant progress was made today in assembling the antenna as we had hoped to have it ready to try at the IARU HF contest next weekend. We didn’t quite make it unfortunately, running out of daylight before we completed construction. However, we are now planning another session next weekend with the goal being to have the antenna finished and ready to run for the Trans Tasman Low Band Challenge contest the following weekend.

The club’s version of Steve’s antenna is using LCF78 coax instead of the wave-guide, with the vacuum capacitor mounted inside a water proof ex-camera case (great for transport and moisture proofing). The frame is made out of laminated bamboo broomsticks and a timber hub arrangement with the frame held together through compression provided by 8 ratchet straps. The aim is for the antenna to be suspended from a tree (or trees) at least 1 loop diameter above the ground (to increase it’s efficiency). It has been designed to accept 400W input power as well to overcome the efficiency issues these antennas can have.

Today’s construction efforts were led by Steve VK5SFA, Grant VK5GR and Scott VK5TST. The project wouldnt have been possible without generous donations from Steve VK5SFA, Peter VK5KX and Trevor VK5YFR.

The next steps are to complete mounting the motor tuning drive, do some structural adjustments to the frame, assemble the coupling loop and then test the antenna. This work will be completed next weekend, so keep an ear out for us during the TTLBC Contest on July 15th on 160 and 80m using our Transmitting Magnetic Loop Antennas!

AREG Develops new DX Pileup Defeating Technology

Introducing the DX Buster(tm)!


SORRY! ALL SOLD OUT on APRIL 1st 2017 – Stay tuned next year for more Amateur Radio products from the mad scientists division of the Amateur Radio Experimenters Group!


After months of rigorous testing, the Amateur Radio Experimenters Group Inc is pleased to announce the beta version of our new DX Buster(tm)! is nearly ready for initial release. What is it you might ask? Well, it is designed to help you to break through pile ups during DX Contests and DXPeditions, ensuring your signal is the one heard clear and true, first time, every-time!

There will be no more disappointment that the DX got away when you are using a DXBuster!(tm), even if you are only a small 100W pistol or 400W VK “high power” station located more than double the distance from that rare DX station compared to the majority (as is often the case when comparing VK to Europe, North America and Japan where they run 1kW or more). Now, with DX Buster!(tm) on your team, you can rest assured your signal will always be clearly heard among the pileups at the DX stations end, guaranteeing you will get that rare one in your log, even with modest power.

How does it work?

DX Buster!(tm) is a DSP device you insert into your microphone audio stream, and then also connect to the Internet. It works by mixing your transmitted audio with an anti-phase, time correlated / corrected version of the signals that the DX station is listening to, based on what is being received via any WebSDR located close to the major source of the DX calling pile-up stations.

Using patented Flux capacitor technology, and augmented by feeds from the Reverse Beacon and PSK Reporter systems tuned to the WSJT JT65 networks as well as space weather predictions from the NOAA and Australian Bureau of Meteorology, the propagation channel between your station and the rare DX is computed. Then, the anti-phase signals matching the majority of the pile up stations within 4kHz of your signal are delay matched to your station and then injected into your audio. The rest follows the laws of physics! When the out of phase signals are combined at the DX stations receiver with the other pile up traffic, that traffic is attenuated, while your own audio laid over the top passes through unaffected. The end result is a minimum 10-30dB improvement in your apparent signal to noise ratio as measured at the DX station.

Don’t quite believe it? Take a look at the following waterfall charts and sample audio streams to be convinced!

How can I get one?

Currently only a prototype of the unit is available, as a number of technical details are still being refined to make it adaptable to as many transceivers as possible. As soon as these are resolved, we will open our books for orders!

Keep watching the AREG website for further details!

 

 

VK5RWN Wireless Link

On October 18th the AREG installed a new 5.8GHz wireless link into the VK5RWN repeater system.

The system is on test for the next couple of weeks, the results have been very promising with the link providing in excess of 30Mbit throughput (full duplex).  Certainly many times faster than the current 512kbit symmetrical ADSL connection.

RWN_Antennas_20141018

Once the wireless link has been finally commissioned and cut over the AREG will be able to close the current ADSL and Telephone internet connection which will significantly reduce the on-going running costs of this site.

I’d like to thank Bob VK5FO, Ray VK5RR, Andy VK5AKH and Mark VK5QI for assisting me with the installation and setup of both ends of the link.

73 Matt, VK5ZM

IRLP Updates

Thanks to the hard work of Ben, VK5BB, our IRLP node is back up and running on VK5RSB 70cm. The usual access conventions apply, and currently no access code is required (though this will change shortly).

To accommodate the (often quite busy!) drive-time nets, the IRLP node is automatically disabled between 7AM to 9AM, and 4PM to 6PM. Enjoy the node, and please make sure you identify before using it, even if just checking the node status!

73s, Mark VK5QI
AREG Secretary