Moonbounce, EME propagation

- an overview, summary or tutorial about the basics of Moonbounce or EME radio signal propagation as it is used by radio hams or radio amateurs on the amateur radio bands.

There are many ways for radio amateurs to establish long distance communications at frequencies above those affected by the ionosphere. One is to use satellites, another is to use radio propagation modes such as tropospheric ducting, toposcatter or ever meteor scatter, however it is also possible to use the Moon as a reflector for the radio signals in a mode often referred to as Moonbounce or EME (Earth-Moon-Earth). Although there are difficulties to be overcome, it offers the possibility of making contacts with stations at the other side of the globe on frequencies at VHF and above.

Moonbounce basics

The basis of operation of Moonbounce or EME is the use of the Moon as a passive reflector. In view of the very much greater distances and the fact that the Moon's surface is not an ideal reflector the path losses are colossal, but nevertheless it is still a form of communication that is theoretically possible to use, and one that many radio amateurs regularly use.

To quantify the path losses the distances and reflection efficiency of the Moon are required. The Moon is around 385 000 kilometres distant from the Earth. The surface of the Moon is also reflects only about 6% of the radio signal power that reaches it. Added to the path loss for the signal travelling to and from the Moon, the overall path loss is around 251 dB on 144 MHz and 270 dB on 1296 MHz.

The level of loss also varies because the distance between the Moon and Earth is not constant. There is a "perigee" when the Moon is closest to Earth and an "apogee" when the Moon is at it furthest point from the Earth each month. This distance variation results in a difference in path loss of around 2 dB between the apogee and perigee positions. For small stations where making contacts using Moonbounce may be marginal, the choice of time in the month can make a difference.

Concept of Moonbounce EME propagation

Concept of Moonbounce EME propagation

With radio signals being very low, it is found that galactic noise becomes a significant factor. This noise emanates from a variety of sources in the galaxy - planets, stars, etc. emit noise throughout the radio spectrum, and EME systems are very sensitive and will be able to hear this noise. The level of noise is not constant across the sky and this means that some times the sky around the Moon can be very noisy and at other times it can be much quieter. It is found that sky noise is normally worst when the Moon is crossing the galactic plane (i.e. the Moon appears in the Milky Way) and this occurs twice each month. Fortunately software used for EME Moonbounce indicates this and this helps choose the optimum times for any activity.

Equipment considerations for EME Moonbounce

To overcome the losses and enable radio communications to be established using Moonbounce, very high radio transmitter powers, directive antennas and very sensitive receivers are required. With the distance of the Moon and its diameter being 3475 kilometres it subtends an angle of only 0.52 degree to observers on the Earth. In order to illuminate the Moon with little wasted power either side, enormously directive antennas are required. Also these antennas must be completely steerable to be able to track the steadily changing position of the Moon.

Frequencies used for Moonbounce are generally in the VHF or UHF portion of the spectrum. This allows antennas with sufficiently high gains to be used to overcome the path losses. Although frequencies as low as 50 MHz have been used, it is more normal for the 144 MHz, 432 MHz or 1296 MHz amateur radio bands to be employed.


Moonbounce propagation effects

In addition to the path losses themselves the EME, Moonbounce signals are subject to other signal propagation effects:

  • Faraday rotation:   At frequencies of 1296 MHz and above it is not a problem, but on 432 MHz it is believed that rotations up to 360 degrees are common, and below this the signal may rotate through several complete revolutions. This may result in stations only being able to communicate in one direction at times.


  • Libration fading:   This effect occurs on EME Moonbounce signals because the surface of the Moon is not flat and the reflected signal consists of a variety of wave-fronts each with differing phases because the distance travelled by each one is slightly different due to the rough Moon surface. The received reflected signal is therefore a sum of all the wave-fronts. As the Earth and the Moon are moving relative to each other the sum of these wave-fronts is always changing and this results in a signal onto which is superimposed a rapid flutter as well as deep fading (sometimes up to 20 dB) and some peaks. These peaks can often be very helpful to stations with less power or smaller antennas.

    The reflections seen from the Moon

    The reflections seen from the Moon


    After reflection by the Moon, wavefronts have a variety of phases which sum to give the overall signal. As these change with the relative movements of the earth and the Moon this results in libration fading.


  • Doppler shift:   The relative movement of the Earth and the Moon can result in some degree of Doppler shift being add to the signals. This will vary according to the relative movements of the two bodies, and also to the frequency in use. As an example of how Doppler shift affects a Moonbounce / EME signal it is found that at "Moonrise", a 2 Metre signal may be shifted up in frequency by as much as 350 Hz. It is then found that this figure reduces, reaching zero when the Moon is passing the particular longitude in which you are located (due south or due north azimuth heading) After this, the Doppler shift starts to move in a negative direction, reaching an offset of around 350 Hz LF by "Moonset." As signal levels are low using EME Moonbounce, very narrow bandwidths are often used and as a result Doppler shifts can be of importance.


  • Signal polarisation changes:   Another problem that can occur with Moonbounce is that as stations are located at different positions around the globe, a horizontally polarised signal in one area of the globe will be at right angles to a horizontally polarised signal a quarter of the way round the globe. This spatial polarisation problem adds to the difficulties caused by Faraday rotation.

Operating using EME Moonbounce

In view of the specialised requirements for Moonbounce, EME, some of the operating techniques used have been adapted to enable the best level of communication to be achieved. As EME is a weak signal mode, most of the contacts have traditionally used Morse, although some stations with high powers and very high gain antennas are able to use SSB on occasions.

When using Morse speeds are generally kept to speeds between about 12 and 20 words a minute. The reason for this is that if the speeds are too high then copy becomes difficult in the presence of noise whereas if the speeds are too slow then the characters become affected by the libration fading which again makes copy difficult. Additionally the weighting on the individual dots and dashes is often increased slightly to aid copy.

A good first check of a station can be gained by listening for echoes of one's own signal. If these can be heard then there is a good chance of others hearing. However even if the echoes cannot be heard, it is possible that others with higher gain antennas may hear.

Although many stations call CQ, this is only viable for stations using high powers and high gain antennas. For stations where signal strength may be marginal arranged contacts produce a far better possibility of a contact. These arranged contacts use accurately timed transmit and receive periods to enable the participating stations to have the best chance of communicating.

Various sections of the band are used for EME. A high proportion of the Moonbounce operation takes place on 2 metres where random operation is typically between 144.000 to 144.045 MHz and arranged contacts may take place on frequencies up to 144.170 MHz. For arranged contacts it is necessary to be able to accurately set the frequency to enable the other station to have a good chance of hearing.

EME Moonbounce summary

The use of E-M-E propagation or Moonbounce is a challenge to any radio amateur wanting to use this mode of radio propagation, but it can yield some excellent results. Those with the right equipment are able to make contacts with stations in many different areas of the globe when the Moon is in the right position relative to the Earth. In this way it is a particularly interesting form of propagation to use.


More Ham Radio Topics:
What is ham radio     Callsigns     Morse code     Digimodes     QSL cards     Codes & abbreviations     Ham bands overview     Callsigns     Contact formats    
    Return to Ham radio menu . . .