This article includes a list ofgeneral references, butit lacks sufficient correspondinginline citations. Please help toimprove this article byintroducing more precise citations.(April 2013) (Learn how and when to remove this message) |

Tropospheric propagation describeselectromagnetic propagation in relation to thetroposphere.The service area from a VHF or UHF radio transmitter extends to just beyond theoptical horizon, at which point signals start to rapidly reduce in strength. Viewers living in such a "deep fringe" reception area will notice that during certain conditions, weak signals normally masked by noise increase in signal strength to allow quality reception. Such conditions are related to the current state of thetroposphere.
Tropospheric propagated signals travel in the part of theatmosphere adjacent to the surface and extending to some 25,000 feet (8 km). Such signals are thus directly affected byweather conditions extending over some hundreds of miles. During very settled, warmanticyclonic weather (i.e., highpressure), usually weak signals from distant transmitters improve in strength. Another symptom during such conditions may beinterference to the local transmitter resulting inco-channel interference, usually horizontal lines or an extrafloating picture with analog broadcasts and break-up with digital broadcasts. A settledhigh-pressure system gives the characteristic conditions for enhanced tropospheric propagation, in particular favouring signals which travel along the prevailingisobar pattern (rather than across it). Such weather conditions can occur at any time, but generally the summer and autumn months are the best periods. In certain favourable locations, enhanced tropospheric propagation may enable reception ofultra high frequency (UHF) TV signals up to 1,000 miles (1,600 km) or more.
The observable characteristics of such high-pressure systems are usually clear, cloudless days with little or no wind. At sunset the upper air cools, as does the surface temperature, but at different rates. This produces a boundary ortemperature gradient, which allows aninversion level to form – a similar effect occurs at sunrise. The inversion is capable of allowingvery high frequency (VHF) and UHF signal propagation well beyond the normalradio horizon distance.
The inversion effectively reducessky waveradiation from a transmitter – normally VHF and UHF signals travel on into space when they reach the horizon, therefractive index of the ionosphere preventing signal return. With temperature inversion, however, the signal is to a large extentrefracted over the horizon rather than continuing along a direct path intoouter space.
Fog also produces good tropospheric results, again due to inversion effects. Fog occurs during high-pressure weather, and if such conditions result in a large belt of fog with clear sky above, there will be heating of the upper fog level and thus an inversion. This situation often arises towards night fall, continues overnight and clears with the sunrise over a period of around 4 – 5 hours.
Tropospheric ducting is a type of radio propagation that tends to happen during periods of stable, anticyclonic weather. In this propagation method, when the signal encounters a rise in temperature in the atmosphere instead of the normal decrease (known as a temperature inversion), the higherrefractive index of the atmosphere there will cause the signal to be bent. Tropospheric ducting affects all frequencies, and signals enhanced this way tend to travel up to 800 miles (1,300 km) (though some people have received "tropo" beyond 1,000 miles / 1,600 km), while with tropospheric-bending, stable signals with good signal strength from 500+ miles (800+ km) away are not uncommon when the refractive index of the atmosphere is fairly high.
Tropospheric ducting of radio and television signals is relatively common during the summer and autumn months, and is the result of change in the refractive index of the atmosphere at the boundary between air masses of differenttemperatures andhumidities. Using ananalogy, it can be said that thedenser air at ground level slows the wave front a little more than does the rare upper air, imparting a downward curve to the wave travel.
Ducting can occur on a very large scale when a large mass of cold air is overrun by warm air. This is termed atemperature inversion, and the boundary between the two air masses may extend for 1,000 miles (1,600 km) or more along a stationaryweather front.
Temperature inversions occur most frequently along coastal areas bordering large bodies of water. This is the result of natural onshore movement of cool, humid air shortly after sunset when the ground air cools more quickly than the upper air layers. The same action may take place in the morning when the rising sun warms the upper layers.
Even though tropospheric ducting has been occasionally observed down to 40 MHz, the signal levels are usually very weak. Higher frequencies above 90 MHz are generally more favourably propagated.
Highmountainous areas and undulating terrain between the transmitter and receiver can form an effective barrier to tropospheric signals. Ideally, a relatively flat land path between the transmitter and receiver is ideal for tropospheric ducting. Sea paths also tend to produce superior results.
In certain parts of the world, notably theMediterranean Sea and thePersian Gulf, tropospheric ducting conditions can become established for many months of the year to the extent that viewers regularly receive quality reception of signals over distances of 1,000 miles (1,600 km). Such conditions are normally optimum during very hot settled summer weather.
Tropospheric ducting over water, particularly betweenCalifornia andHawaii,Brazil andAfrica, Australia andNew Zealand, Australia andIndonesia, Strait of Florida, andBahrain andPakistan, has produced VHF/UHF reception ranging from 1000 to 3,000 miles (1,600 – 4,800 km). AUS listening post was built in Ethiopia to exploit a common ducting of signals from southern Russia.
Tropospheric signals exhibit a slow cycle of fading and will occasionally produce signals sufficiently strong for noise-freestereo, reception ofRadio Data System (RDS) data, and solid locks ofHD Radio streams onFM, noise-free, colorTV pictures, or stable DTV reception, as well stableDAB Radio reception. WithDVB-T it can also enable a wideSFN, so long as the two transmitters are within a guard interval and are almost equidistant from the receiver as well as synchronised. However, if they are not synchronised and are not equidistant they will interfere with each other.
Virtually all long-distance reception ofdigital television occurs by tropospheric ducting (due to most, but not all, TV stations broadcasting in theUHF band).
"DXing is the art and science of listening to distant stations."[1] The ARRL, association for amateur radio maintains the list of North American distance records, which includes tropo results.