Line-of-sight propagation

For other uses, see Line-of-sight (disambiguation).

Line of sight propagation to an antenna

Line-of-sight propagation is a characteristic of electromagnetic radiation or acoustic wave propagation. Electromagnetic transmission includes light emissions traveling in a straight line. The rays or waves may be diffracted, refracted, reflected, or absorbed by atmosphere and obstructions with material and generally cannot travel over the horizon or behind obstacles.

At low frequency (below approximately 3 MHz), radio signals travel as ground waves, which follow the Earth's curvature due to diffraction with the layers of the atmosphere. This enables AM radio signals in low-noise environments to be received well after the transmitting antenna has dropped below the horizon. Additionally, frequencies between approximately 1 and 30 MHz can be reflected by the F1/F2 Layer, thus giving radio transmissions in this range a potentially global reach (see shortwave radio), again along multiple deflected straight lines. The effects of multiple diffraction or reflection lead to macroscopically "quasi-curved paths".

However, at frequencies above 30 MHz (VHF and higher) and in lower levels of the atmosphere, neither of these effects are significant. Thus, any obstruction between the transmitting antenna (transmitter) and the receiving antenna (receiver) will block the signal, just like the light that the eye may sense. Therefore, since the ability to visually see a transmitting antenna (disregarding the limitations of the eye's resolution) roughly corresponds to the ability to receive a radio signal from it, the propagation characteristic at these frequencies is called "line-of-sight". The farthest possible point of propagation is referred to as the "radio horizon".

In practice, the propagation characteristics of these radio waves vary substantially depending on the exact frequency and the strength of the transmitted signal (a function of both the transmitter and the antenna characteristics). Broadcast FM radio, at comparatively low frequencies of around 100 MHz, are less affected by the presence of buildings and forests.

Impairments to line-of-sight propagation

Objects within the Fresnel zone can disturb line of sight propagation even if they don't block the geometric line between antennas

Low-powered microwave transmitters can be foiled by tree branches, or even heavy rain or snow.

If a direct visual fix cannot be taken, it is important to take into account the curvature of the Earth when calculating line-of-sight from maps. Designs for microwave used to use 4/3 earth radius to compute clearances along the path.

The presence of objects not in the direct visual line of sight can interfere with radio transmission. This is caused by diffraction effects: for the best propagation, a volume known as the first Fresnel zone should be kept free of obstructions.

Reflected radiation from the ground plane also acts to cancel out the direct signal. This effect, combined with the free-space r⁻² propagation loss to a r⁻⁴ propagation loss. This effect can be reduced by raising either or both antennas further from the ground: the reduction in loss achieved is known as height gain.

Mobile telephones

Although the frequencies used by mobile phones (cell phones) are in the line-of-sight range, they still function in cities. This is made possible by a combination of the following effects:

r⁻⁴ propagation over the rooftop landscape
diffraction into the "street canyon" below
multipath reflection along the street
diffraction through windows, and attenuated passage through walls, into the building
reflection, diffraction, and attenuated passage through internal walls, floors and ceilings within the building

The combination of all these effects makes the mobile phone propagation environment highly complex, with multipath effects and extensive Rayleigh fading. For mobile phone services, these problems are tackled using:

rooftop or hilltop positioning of base stations
many base stations (usually called "cell sites"). A phone can typically see at least three, and usually as many as six at any given time.
"sectorized" antennas at the base stations. Instead of one antenna with omnidirectional coverage, the station may use as few as 3 (rural areas with few customers) or as many as 32 separate antennas, each covering a portion of the circular coverage. This allows the base station to use a directional antenna that is pointing at the user, which improves the signal to noise ratio. If the user moves (perhaps by walking or driving) from one antenna sector to another, the base station automatically selects the proper antenna.
rapid handoff between base stations (roaming)
the radio link used by the phones is a digital link with extensive error correction and detection in the digital protocol
sufficient operation of mobile phone in tunnels when supported by split cable antennas
local repeaters inside complex vehicles or buildings

A Faraday cage is composed of a conductor that completely surrounds an area on all sides, top, and bottom. Electromagnetic radiation is blocked where the wavelength is longer than any gaps. This means that windowless metal enclosures will completely block cell signs, such as elevator cabins, and parts of trains, cars, and ships. The same problem can affect signals in buildings with extensive steel reinforcement.

Two stations not in line-of-sight may be able to communicate through an intermediate radio repeater station.

Radio horizon

The radio horizon is the locus of points at which direct rays from an antenna are tangential to the surface of the Earth. If the Earth was a perfect sphere and there was no atmosphere, the radio horizon would be a circle.

The radio horizon of the transmitting and receiving antennas can be added together to increase the effective communication range. Antenna heights above 1,000,000 feet (189 miles; 305 kilometres) will cover the entire hemisphere and not increase the radio horizon.

Radio wave propagation is affected by atmospheric conditions, ionospheric absorption, and the presence of obstructions, for example mountains or trees. Simple formulas that include the effect of the atmosphere give the range as:

\mathrm {horizon} _{\mathrm {miles} }\approx 1.23\cdot {\sqrt {\mathrm {height} _{\mathrm {feet} }}}.

\mathrm {horizon} _{\mathrm {km} }\approx 3.57\cdot {\sqrt {\mathrm {height} _{\mathrm {metres} }}}

The simple formulas give a best-case approximation of the maximum propagation distance, but are not sufficient to estimate the quality of service at any location.

Earth bulge and atmosphere effect

Earth bulge is a term used in telecommunications. It refers to the circular segment of earth profile that blocks off long distance communications. Since the geometric line of sight passes at varying heights over the Earth, the propagating radio wave encounters slightly different propagation conditions over the path. The usual effect of the declining pressure of the atmosphere with height is to bend radio waves down towards the surface of the Earth, effectively increasing the Earth's radius, and the distance to the radio horizon, by a factor of around 4/3.^[1] This k-factor can change from its average value depending on weather.

Geometric distance to horizon

Assuming a perfect sphere with no terrain irregularity, the distance to the horizon from a high altitude transmitter (i.e., line of sight) can readily be calculated.

Let R be the radius of the Earth and h be the altitude of a telecommunication station. The line of sight distance d of this station is given by the Pythagorean theorem;

d^{2}=(R+h)^{{2}}-R^{2}=2\cdot R\cdot h+h^{2}

Since the altitude of the station is much less than the radius of the Earth,

d\approx {\sqrt {2\cdot R\cdot h}}

If the height is given in metres, and distance in kilometres,^[2]

d\approx 3.57\cdot {\sqrt {h}}

If the height is given in feet, and the distance in miles,

d\approx 1.23\cdot {\sqrt {h}}

The actual service range

The above analysis does not consider the effect of atmosphere on the propagation path of RF signals. In fact, RF signals don’t propagate in straight lines. Because of the refractive effects of atmospheric layers, the propagation paths are somewhat curved. Thus, the maximum service range of the station is not equal to the line of sight (geometric) distance. Usually, a factor k is used in the equation above

d\approx {\sqrt {2\cdot k\cdot R\cdot h}}

k > 1 means geometrically reduced bulge and a longer service range. On the other hand, k < 1 means a shorter service range.

Under normal weather conditions, k is usually chosen^[3] to be 4/3. That means that the maximum service range increases by 15%.

d\approx 4.12\cdot {\sqrt {h}}

for h in metres and d in kilometres; or

d\approx 1.41\cdot {\sqrt {h}}

for h in feet and d in miles.

But in stormy weather, k may decrease to cause fading in transmission. (In extreme cases, k can be less than 1.) That is equivalent to a hypothetical decrease in Earth radius and an increase of Earth bulge.^[4]

Example

In normal weather conditions, the service range of a station at an altitude of 1500 m with respect to receivers at sea level can be found as,

d\approx 4.12\cdot {\sqrt {1500}}=160{\mbox{ km.}}

References

↑ Christopher Haslett, Essentials of radio wave propagation, Cambridge University Press, 2008 052187565X pages 119-120
↑ Mean radius of the Earth is ≈ 6.37×10⁶ metres = 6370 km. See Earth radius
↑ R.Busi: Technical Monograph3108-1967 High Altitude VHF and UHF Broadcasting Stations, European Broadcasting Union Brussels,1967
↑ This analysis is for high altitude to sea level reception. In microwave radio link chains, both stations are at high altitudes.

External links

This article incorporates public domain material from the General Services Administration document "Federal Standard 1037C" (in support of MIL-STD-188).

Electromagnetic spectrum

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Modes of radio propagation

Line-of-sight Ionospheric Meteor burst Sporadic E Tropospheric scatter Earth–Moon–Earth (EME) Interstellar Medium (ISM)

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