
Tap a step to hear that moment. The box shows where it is on the waterfall.
Still pictures sent as sound, one line at a time. A picture takes from about half a minute to a few minutes.
Slow-scan TV sounds like a warbling, whistling tone that sweeps up and down in pitch, punctuated by a regular tick about two to seven times a second, and runs from about half a minute to a few minutes.
A steady, sweeping, whistling sound with a regular rhythm, starting with a short musical tone sequence.

12-second example. Slow-scan TV made by Cohera in Robot 36, the format the Space Station uses: the start tones, then the picture line by line.
This slow-scan TV clip is the first 12 seconds of a Robot 36 picture: the header, then the top of a practice picture, line by line.

Tap a step to hear that moment. The box shows where it is on the waterfall.
Make your own: type a message and hear it as Slow-scan TV (SSTV) in the Signal Maker.
Amateur radio operators, and special events such as picture broadcasts from the International Space Station.
Around 14.230 MHz on shortwave. Space station picture events: 437.550 MHz in 2026 (earlier events used 145.800 MHz); dates are announced on ariss.org.
Hear it live
These are free public receivers run by other people; we only link to them. You'll hear the signal only if it's on the air right now and conditions carry it to that receiver, so if it's quiet, try another time. Links last reviewed 2026-09-28.
SSTV sends a picture as an audio tone whose pitch sets the brightness: 1,500 Hz means black and 2,300 Hz means white, and short 1,200 Hz pulses, blacker than black, mark the start of each line. Color modes send each line in pieces; the popular Martin M1 mode sends green, blue and red in turn after a 4.862-millisecond sync pulse and takes about 114 seconds for a 320 by 256 picture. A short digital header at the start (the VIS code) tells the receiver which mode is coming.
Because the whole signal fits in a voice channel, SSTV works with an ordinary SSB or FM receiver, and space station events can be received with a simple handheld radio or scanner that covers the event frequency, fed into free decoding software.
Copthorne Macdonald, then a University of Kentucky student, began developing SSTV in 1957; the first image crossed the Atlantic on December 20, 1959, and the FCC formally authorized SSTV in 1968. Space station events have used the PD120 mode on 145.800 MHz, and ARISS lists 2026 events in Robot 36 on 437.550 MHz.
An SSTV picture opens with a short, recognizable header: two steady tones with a brief break between them, followed by a quick burst that tells the receiver which format is coming. After that the picture itself is sent as a continuous tone whose pitch follows the brightness of the image, from about 1500 Hz for black to 2300 Hz for white.
Between image lines (every line in most formats, every other line in the PD formats) you hear a short, lower sync pulse at 1200 Hz. That repeating pulse gives SSTV its steady "tick... tick..." rhythm, and the pitch in between sounds busier over detailed parts of the picture and smoother over plain sky.
Easily confused with:
On shortwave, the classic meeting place is 14.230 MHz (upper sideband), with 14.233 as an overflow; you will also find SSTV around 7.171, 3.845, 21.340 and 28.680 MHz. Weekends are busiest. Operators often send picture replies, test cards or their station photo.
The International Space Station runs occasional SSTV events through the ARISS program, sending a themed series of pictures for several days. These are announced ahead of time on ariss.org, and all you need to receive them is a simple VHF or UHF receiver and patience for the station's passes overhead.
Copthorne Macdonald developed slow-scan television in the late 1950s as a way to send pictures through a voice-sized radio channel. Early stations used long-persistence radar screens to view each image as it slowly built up. In the 1970s, scan converters replaced those screens, color pictures became practical in the 1980s, and from the 1990s personal computers with sound cards replaced most dedicated hardware.
Today dozens of formats exist. The most common include Martin 1 and Scottie 1 (each just under two minutes for a color picture), Robot 36 (36 seconds) and PD120 (about two minutes), which space station events used through 2025; the 2026 events use Robot 36.
Yes. Amateur SSTV and the space station's picture events are open transmissions meant to be received by anyone. The pictures themselves still belong to whoever made them, so ask before republishing someone else's image.
Each pixel's brightness is sent as a pitch. As the scan moves across a line, the tone slides up and down with the picture, and each line starts with a short sync pulse, which is what gives the sound its regular tick.
Free programs such as MMSSTV (Windows) and QSSTV (Linux), and free phone apps, can turn the audio into a picture. Many will even work from a phone held near a radio's speaker, though a direct audio cable gives cleaner results.
A slant means the decoding program's timing is slightly different from the sender's. Most programs have a slant or clock-correction setting that fixes it.