HAMTV from the ISS
HAMTV is the name of the Digital Amateur Television (DATV) transmitter on board the Columbus module of the International Space Station (ISS).
It transmits Digital video and audio in MPEG-2 format using the DVB-S protocol in the 13cms band.
The original HamTV unit was installed on the ISS in 2013 and commissioned in April 2014 and was used for a number of ARISS school contacts in 2016 - 2018.
The unit failed in 2019, and was returned to earth for repair. It is expected to be returned to the ISS on the SpaceX SpX-30 flight currently scheduled for March 21st 2024. It is hoped that it will be recommissioned by a visiting astronaut within a few weeks of its arrival.
HAMTV specifications
Ham Video downlink frequencies
- 2395 MHz (main operating frequency)
- 2369 MHz
- 2422 MHz
- 2437 MHz
DVB-S modulation
- Symbol rates: 1.3 Ms/s or 2.0 Ms/s
- FEC : ½
RF output
The HAMTV transmitter produces 10 watts RF, however this is then fed through a series of interconnecting cables and bandpass filter before passing through the ISS Columbus module external wall. Estimated power at the antenna is ~ 2 watts.
HAMTV antenna
The HamTV transmission runs relatively low power on 2395MHz to a simple patch antenna on the ISS.
This patch antenna is located on the earth facing side of the ISS but there are many other items that project below the antenna and may cause reflections. These include the solar panels, thermal radiator panels, sometimes, two or more visiting vehicles and robotic arms. Depending upon your location in respect to the ISS, these projections may result in strong reflected signals as well as the one from the patch antenna itself. They may cause disturbances to the signal level you receive.
The ISS also “flies” slightly nose down to protect the cupola windows from space debris and so the RF performance, particularly when it is rising from the west, is slightly unpredictable.
The transmissions are right hand circular polarised (RHCP)
Video format
- MPEG-2, approx. 2 Msymbols
- NTSC
- SIF resolution: 352×240 or D1:720×480, 29.97fps
- Note that non-square pixels are used, the 4:3 picture has to be stretched to 16:9 for correct visual aspect ratio.
What is HAMTV used for?
The primary use is for ARISS schools contacts, when the astronaut will use a camera to show himself and the inside of the ISS during the VHF radio contact.
It is hoped in the future that test patterns, including JPEG images, will be transmitted when the cameras are not in use. Note this will NOT happen when HAMTV is recommissioned in Spring / summer 2024.
When will HAMTV be "on the air"?
Once commissioned it is unlikely that the HamTV transmitter will be on air 24/7.
During the first flight on the ISS between 2014 and 2018 it was used primarily for ARISS schools contacts but transmitter was left on at other times but no video was transmitted. This did allow ground stations to test their receive equipment and it is hoped a test signal generator will eventually be included, perhaps in 2025.
Once re-commissioned, it will be tested before school contacts are undertaken.
HamTV will be added to the AMSAT status page https://www.amsat.org/status/ - always check there before doing any receive tests.
How to receive HAMTV?
There are a number of challenges to receive HAMTV from the ISS and a typical ground station is made up of the following elements
A typical groundstation system block diagram
Ground station antenna and feed
The HamTV transmission runs relatively low power on 2395MHz to a simple patch antenna on the ISS.
This means an antenna with reasonable gain is required to receive the signal and whilst it is possible to receive the signal on a simple antenna when the ISS is overhead, to enable more than 5 minutes of reception, a higher gain antenna such as a dish with an efficient feed system is required.
It will be difficult to receive HamTV DATV picture when ISS is at a low elevation at your ground station location. Generally, a minimum of 20 degrees elevation is required to begin receiving DATV pictures.
A 1 meter or larger dish is optimum but smaller antennas such as flat plate or patch antennas will work and have the advantage of a wider beamwidth making it easier to track the ISS. They are unlikely to work at low elevations.
Pre-amp and filter
A low noise pre-amp (LNA) with bandpass filter tuned to 2395MHz should be connected directly to the antenna feed point to minimise co-ax losses. The LNA should have noise figure (NF) less than 1db and a gain of approximately 15 dB.
Note that 2395MHz is only 5MHz below the 2.4GHz WiFi Channel 1, so good filtering will be needed to prevent strong, local WiFi signals from getting into the wide band satellite tuner and causing interference or defense.
Receive co-ax cable
It is recommended to use professional grade satellite co-ax. If you are using a long cable run you must check the received signal level at the receiver - see below.
Receive Line amplifier
Satellite TV receivers need a high level of RF signal - they are designed for use with satellite LNBs which have ~55dB gain. Your masthead pre-amp must be followed by at least one satellite TV line amplifier with greater than 30 dB gain in the shack.
Your masthead LNB MUST have enough gain to overcome your co-ax cable loss. The satellite line amplifier can be placed at masthead if needed to help overcome the feeder loss or in the shack.
You can check if you have enough gain in your receive system by checking the RF signal level on the Ryde, OpenTuner, MiniTiouner or Portsdown DATV receivers - the noise floor should sit between -30 to -70dBm when not receiving any signals.
If you are powering the LNA at masthead up the co-ax, you will need to place the DC inserter AFTER the filter.
Do I need a downconverter?
The HAMTV frequency on 2395MHz is outside the frequency range of a standard consumer set top box or satellite tuner.
Unless you are using the BATC MiniTiouner Mark 2 or PicoTuner USB receiver equipped with the Serit 4434 NIM, which can tune up to 2450MHz, you will need a frequency down converter to place the HAMTV signal between 950 and 2150MHz which is within the range of a standard satellite receiver.
Note: The MiniTiouner Mk1 PCB with a Sharp or Eardertek tuner does NOT cover 2395MHz and will require a downconverter.
The downconverter should be placed between the low noise amplifier and satellite receiver – placing it at the masthead will mean that lower grade feeder can be used to bring the IF signal back to the shack.
Previous suppliers of suitable downconverters, such as Kuhne Electronics, no longer market suitable items and BATC strongly recommends purchasing a new USB tuner hardware kit using the Serit 4334 tuner rather than building or sourcing a down converter - see next section on HamTV receivers.
Digital receivers for HAMTV
The HamTV transmissions can be received using a DVB-S receiver capable of decoding 2 Msymbol / second MPEG2 transmission. This means that a standard consumer Set Top Box (STB) can be used. However, because the signal is only available during the ISS pass it is essential to use a receiver that can be set to both the frequency and symbol rate before the pass.
A receiver, such as a typical consumer STB, that needs to scan the frequency is unlikely to lock to the signal in the time available during the pass. This solution is therefore not recommended.
Receivers designed for DATV
For optimum performance, a receiver designed for receiving narrow band DATV signals should be used. The Amateur TV community has developed a number of receive solutions based around a USB connected tuner hardware.
Hardware
The BATC Minitiouner and PicoTuner are PCBs which host the Serit 4334 satellite tuner and a USB interface. This unit is designed to be built at home, requiring only intermediate skills and does not use surface mount components.
The hardware is connected to either a PC or Raspberry Pi 4 using the USB 2 connection.
As mentioned above, the original BATC MiniTiouner Mk1 PCB launched in 2015 with a Sharp or Eardertek tuner does NOT cover 2395MHz and will require a downconverter. As well as covering the HAMTV frequency without a down converter, the Serit 4334 has much better RF performance than the original Sharp and Eardertek units and has been integrated into the OpenTuner and Portsdown DATV receive systems.
Full details of the USB tuner hardware, including parts list and construction details are available here: MiniTiouner hardware Version 2
Software for use with the USB receiver
When the original HamTV was on the air, due to a problem with the DVB tables in the transmission, the MiniTiouner software by F6DZP running on Windows had to be used.
However, during the last few years many developments have taken and so we now have a choice of software to use with the USB tuner hardware:
- Ryde - Raspberry Pi 4 based set-top box software designed specifically for receiving narrow band DATV signals.
For more details see this page:Ryde Receiver
- Opentuner - PC based software developed by Tom ZR6TG
For more details see this wiki page: OpenTuner
- Portsdown - The BATC designed DATV transceiver system based on a Rpi 4 has a receiver which has been tested and decodes the HAMTV signal
See The_Portsdown_DATV_transceiver_system#Portsdown_DATV_receiver
- MiniTiouner - the MiniTiouner software is still available however the author F6DZP is no longer involved in the amateur radio community so is not providing support or enhancements and you can no longer register on the Viva DATV forum to download the software.
PC software receivers
SDR Angel is PC software that receives DATV signals using SDR hardware such as the ADALM Pluto and Hack RF - at this time we do not have any experience of using SDR Angel to receive HamTV. For more details see https://www.sdrangel.org/
Receiving the Signal
First - always check the HamTV transmitter status before attempting to align your system as it is unlikely that it will be left on 24/7 and it certainly will not be available when EVAs (space walks) and docking of space craft are happening.
It is likely but not confirmed that the status will be published on the ARISS international website and Twitter account – the ISSfanclub website may also have the status updates.
Tracking the ISS
Perhaps the most challenging aspect of receiving HamTV is that, unlike the QO-100 satellite available in the Europe and Africa, the ISS is not geo-stationary and orbits the earth every 96 minutes and is visible at any location for a maximum of 11 minutes.
In order to track the ISS, an azimuth and elevation rotator system is required. The most commonly used system is the Yaesu G5500, which is capable of rotating a 1.2m dish with a 5 degree beam width to track the ISS. When choosing/designing your system remember the ISS does go north of 50 degrees and so any system will need to be capable of flip mode to track it when it goes overhead.
Just like for other spacecraft in low earth orbit, software is available to control the rotator system – there are a number of different programs available. PSTrotator which is a very versatile system with almost unlimited number of interfaces to control rotators is one of them..
Testing your system
As the ISS is not visible every day at a given location and then only for short periods, it is difficult to see if your HAMTV receive system is working.
There are a number of tests you can do to ensure your system is optimised but the most useful is to measure the sun noise received on your system. This will not only measure your system performance but if you leave it running for a few hours with your rotator control system set to track the sun, it will confirm the accuracy of your tracking system.
Measuring sun noise
Portsdown DATV test system
The Portsdown DATV transceiver incorporates a test function that has a continuous noise measurement facility designed to measure sun noise. It is very easy to use. Simply connect the signal from your LNA to the rx port on a Pluto or Lime SDR and run the software - see https://wiki.batc.org.uk/Portsdown_Noise_Meter
SDR continuum mode
Measuring sun noise can be done using SDR software running in continuum mode and running a program such as spectra view on the audio output – a Google search for sun noise measurement will show several techniques.
MiniTiouner Noise power measurement
F6DZP developed a suite of programs to help test a HamTV receive system which included a Noise Power Measurement program (see CQ-TV253 page 27 for more details). This was available as part of the MiniTiouner v0.8 package but appears to have been dropped in later releases. The program can be used to measure the noise power received by a Serit 4334 tuner over a period of time and requires no extra software or equipment to make sun noise measurements – the picture shows the sun noise recording from a RFHams 1.2 m mesh dish used to receive HamTV for the Principia mission in 2016.
Decoding a local signal
Once you have checked your system sun noise and tracking accuracy it is worth testing you’re your system can receive a locally generated 2Ms DVB-S signal on 2395 MHz. You can use the Portsdown Pi4 based system with a Pluto or Lime SDR to generate this signal.
If this is successful you should be set to receive HamTV!
Receiving HamTV
All that remains is to wait until it is confirmed that the HamTV transmitter has been turned on then set your tracking program to follow the ISS and wait for the magic signs on the spectrum display (BandViewer?) or lock indicator that you are receiving the signal!
Once you have successfully received the HamTV transmission, the Dsave button in MiniTioune can be used to record data such as RF level, MER and Vber to show how well and for how long you received the pass.
Further information
BATC have setup a new forum thread to discuss receiving HamTV. Please post any questions, comments and status updates here:
https://forum.batc.org.uk/posting.php?f=2&mode=post&sid=9c1b12a07706567454ebeca685548796 (NOT SURE THIS LINK IS CORRECT!)
Receivers compatible with HamTV:
A lot of information is available on the BATC forum:
https://forum.batc.org.uk/viewtopic.php?t=4389
Colin G4KLB made a video on how he received HamTV
https://www.youtube.com/watch?v=9keVA21DPBc
BATC TS (transport stream) merger system
Once HamTV is active from ISS, BATC will be running the TS merger system. This is a server which combines the UDP outputs from several ground stations and enables continuous video stream from the ISS to be presented to a web page.
It typically gives 25 mins of continuous video over Europe and we will be looking for ground stations to join the network.
