The Squarial (a portmanteau of the words square and aerial ) was a satellite antenna used for reception of the now defunct British Satellite Broadcasting television service (BSB). The Squarial was a flat plate satellite antenna, built to be unobtrusive and unique. BSB were counting on the form factor of the antenna to clearly differentiate themselves from their competitors at the time. At the time of development, satellite installations usually required a 90 cm dish in order to receive a clear signal from the transmitting satellite. The smaller antenna was BSB's unique selling point and was heavily advertised in order to attract customers to their service.
The Squarial was launched at a high-profile event in Marco Polo House, BSB's headquarters. The media were invited to a demonstration to see how much better MAC pictures could be than PAL. But MAC took a back seat when BSB unveiled the mock up Squarial, to replace the dish aerials usually needed for satellite reception. The Squarial was a surprise to everyone, including the four companies which had signed to manufacture the receivers which would have to work with the new aerial. The Squarial deal, with British company Fortel, had been struck only hours before the London event. BSB was itself surprised at the press reaction.
The media were apparently so excited by the new antenna that they failed to ask whether there was a working prototype, and there wasn't. All that existed at this point was a wood-and-plastic dummy. Believing that someone would be able to make the Squarial work as well as a much larger dish, BSB built a whole advertising campaign on the Squarial. STC in Paignton was the first company to make a British Squarial. These were a little bigger, 38 cm across, to provide adequate reception throughout the UK, and more expensive than a dish.[ citation needed ] Due to production delays and limited availability of the STC squarial and to save face at launch, BSB sourced already available Squarials from Matsushita (now called Panasonic) in Japan who were producing them in quantity for the Japanese market. Industry rumours at the time of launch suggested that BSB were buying the squarials from Matsushita for several hundred pounds each and heavily subsidising the cost to the four manufacturers of DMAC receiver. The Matsushita squarial was of a slightly better quality construction compared to the STC design and was used by Ferguson, Philips and Tatung while ITT-Nokia supplied the STC squarial. However all offered the 30 cm traditional mini dish for a slightly lower price (several dish manufacturers were used including Lenson Heath and Channel Master).
The Squarial became obsolete in 1993, when the Marcopolo satellites, which the Squarial received, stopped broadcasting signals from BSkyB, which had carried the Sky channels over the D-Mac system for a period.
Unlike a normal satellite dish, which uses a parabolic reflector to focus the radio waves on a single feed horn antenna, the Squarial was a phased array antenna, a common design in which multiple small antennas work together to receive the waves. [1] The Squarial consisted of a planar array of either 144 or 256 resonant cavity antennas spaced 0.9 wavelength apart, all embedded in plastic. Each antenna element was a tiny open-ended metal box in which the microwave downlink radio waves excited standing waves, with a wire probe projecting in which received the radio waves and conducted them to an integral low-noise block converter (LNB) amplifier. The feed network combined the radio currents from the separate elements with the correct phase so that radio waves from the desired direction would be in phase and add together, while radio waves from other directions would be out of phase and cancel.
Since the microwaves had to pass through the plastic surface to reach the antennas, special low-loss plastic was used. Three of these plastic sheets were stacked upon each other, padded with polystyrene layers to add rigidity to the unit. All this was engineered into a 38 cm white plastic body with the BSB logo at the bottom. The low-noise block converter mounted in the center, behind the layers, was a standard unit similar to those in other satellite dishes, which converts the frequencies from the satellite down to a lower frequency band around 800 MHz and transmits it through a coaxial cable into the building to the set-top box at the TV. It was manufactured by Matsushita and rated as a 10 GHz standard unit.
The Squarial's small size was possible thanks to the high power of the two Marcopolo DBS satellites, which simulcast the same channels on the same frequencies. The broadcast power was 59 dBW, with a 0.05 degree accuracy. [2]
Manufacturers of the DMAC receivers used with the Squarial included, Ferguson, Phillips, Nokia and Tatung.
The Squarial was a specialized antenna designed specifically for operation on the Marco Polo satellites' frequency range. The LNB could only tune a limited range of frequencies and when utilised in modern circumstances the frequency is subsequently offset by around 100 MHz.
Some owners modified the squarial to operate with the Thor satellite system (formerly BSB's own satellites, Marcopolo) after the decline of BSB. This was due in large part to the highly discounted price of the unit during the final months of BSB's existence. D2-MAC programmes could be picked up from the Scandinavian satellites during the early 1990s and viewed using modified receivers. Once transmissions ceased from these satellites, Squarials could be used to receive broadcasts from the French terrestrial relay satellites at 5.0°W.
BSB's alternative dishes were also successfully used to receive analogue transmissions from the Astra and Hot Bird satellites.
BSB placed the Squarial at the heart of its advertising campaign, using the diamond shape throughout all of its channel logos and on screen presentation. This square/diamond image extended down to BSB's corporate logo and even printed and televisual advertising mediums. This led to the company's slogan (used throughout the company's existence) "It's smart to be square". [3]
The unique appearance was a design first for satellite antennae, its flat plate measured only a few millimetres thick and the LNB unit protruded another 3 cm from the rear. It was built to a very high standard, featuring good quality plastics, weather resistant coatings and stainless steel mounting arm. Compared with the Amstrad-manufactured dishes offered by Sky — made from cheap metal — the Squarial offered a much more attractive, upmarket appearance.
BSB offered two alternatives to the squarial, the cheaper more conventional looking mini-dish format and the rounded-rectangle format dish.
The first revision was in the shape of a vertical ellipse of roughly 30 cm in diameter. The design employed a short LNB arm with a 'spike' design LNB operating at a frequency of 10 GHz. Essentially this design could be considered the forerunner to BSkyB's minidish. The second revision took on the appearance of a perfectly circular dish (around 25 cm in diameter), using a standard LNB at 10 GHz. In essence both function like a normal satellite dish, only scaled down.
Microwave is a form of electromagnetic radiation with wavelengths ranging from about one meter to one millimeter corresponding to frequencies between 300 MHz and 300 GHz respectively. Different sources define different frequency ranges as microwaves; the above broad definition includes UHF, SHF and EHF bands. A more common definition in radio-frequency engineering is the range between 1 and 100 GHz. In all cases, microwaves include the entire SHF band at minimum. Frequencies in the microwave range are often referred to by their IEEE radar band designations: S, C, X, Ku, K, or Ka band, or by similar NATO or EU designations.
A radio telescope is a specialized antenna and radio receiver used to detect radio waves from astronomical radio sources in the sky. Radio telescopes are the main observing instrument used in radio astronomy, which studies the radio frequency portion of the electromagnetic spectrum emitted by astronomical objects, just as optical telescopes are the main observing instrument used in traditional optical astronomy which studies the light wave portion of the spectrum coming from astronomical objects. Unlike optical telescopes, radio telescopes can be used in the daytime as well as at night.
A feed horn is a small horn antenna used to couple a waveguide to e.g. a parabolic dish antenna or offset dish antenna for reception or transmission of microwave. A typical application is the use for satellite television reception with a satellite dish. In that case the feed horn can either be a separate part used together with e.g. a "low-noise block downconverter" (LNB), or more typically today is integrated into a "low-noise block feedhorn" (LNBF).
The Ku band is the portion of the electromagnetic spectrum in the microwave range of frequencies from 12 to 18 gigahertz (GHz). The symbol is short for "K-under", because it is the lower part of the original NATO K band, which was split into three bands because of the presence of the atmospheric water vapor resonance peak at 22.24 GHz, (1.35 cm) which made the center unusable for long range transmission. In radar applications, it ranges from 12 to 18 GHz according to the formal definition of radar frequency band nomenclature in IEEE Standard 521–2002.
Television receive-only (TVRO) is a term used chiefly in North America, South America to refer to the reception of satellite television from FSS-type satellites, generally on C-band analog; free-to-air and unconnected to a commercial DBS provider. TVRO was the main means of consumer satellite reception in the United States and Canada until the mid-1990s with the arrival of direct-broadcast satellite television services such as PrimeStar, USSB, Bell Satellite TV, DirecTV, Dish Network, Sky TV that transmit Ku signals. While these services are at least theoretically based on open standards, the majority of services are encrypted and require proprietary decoder hardware. TVRO systems relied on feeds being transmitted unencrypted and using open standards, which heavily contrasts to DBS systems in the region.
Radio waves are a type of electromagnetic radiation with the longest wavelengths in the electromagnetic spectrum, typically with frequencies of 300 gigahertz (GHz) and below. At 300 GHz, the corresponding wavelength is 1mm, which is shorter than a grain of rice. At 30 Hz the corresponding wavelength is ~10,000 kilometers longer than the radius of the Earth. Like all electromagnetic waves, radio waves in a vacuum travel at the speed of light, and in the Earth's atmosphere at a slightly lower speed. Radio waves are generated by charged particles undergoing acceleration, such as time-varying electric currents. Naturally occurring radio waves are emitted by lightning and astronomical objects, and are part of the blackbody radiation emitted by all warm objects.
Ultra high frequency (UHF) is the ITU designation for radio frequencies in the range between 300 megahertz (MHz) and 3 gigahertz (GHz), also known as the decimetre band as the wavelengths range from one meter to one tenth of a meter. Radio waves with frequencies above the UHF band fall into the super-high frequency (SHF) or microwave frequency range. Lower frequency signals fall into the VHF or lower bands. UHF radio waves propagate mainly by line of sight; they are blocked by hills and large buildings although the transmission through building walls is strong enough for indoor reception. They are used for television broadcasting, cell phones, satellite communication including GPS, personal radio services including Wi-Fi and Bluetooth, walkie-talkies, cordless phones, satellite phones, and numerous other applications.
A satellite dish is a dish-shaped type of parabolic antenna designed to receive or transmit information by radio waves to or from a communication satellite. The term most commonly means a dish which receives direct-broadcast satellite television from a direct broadcast satellite in geostationary orbit.
A parabolic antenna is an antenna that uses a parabolic reflector, a curved surface with the cross-sectional shape of a parabola, to direct the radio waves. The most common form is shaped like a dish and is popularly called a dish antenna or parabolic dish. The main advantage of a parabolic antenna is that it has high directivity. It functions similarly to a searchlight or flashlight reflector to direct radio waves in a narrow beam, or receive radio waves from one particular direction only. Parabolic antennas have some of the highest gains, meaning that they can produce the narrowest beamwidths, of any antenna type. In order to achieve narrow beamwidths, the parabolic reflector must be much larger than the wavelength of the radio waves used, so parabolic antennas are used in the high frequency part of the radio spectrum, at UHF and microwave (SHF) frequencies, at which the wavelengths are small enough that conveniently-sized reflectors can be used.
British Satellite Broadcasting (BSB) was a television company, based in London, that provided direct broadcast satellite television services to the United Kingdom. It started broadcasting on 25 March 1990. The company was merged with Sky Television plc on 2 November 1990 to form British Sky Broadcasting.
A low-noise block downconverter (LNB) is the receiving device mounted on satellite dishes used for satellite TV reception, which collects the radio waves from the dish and converts them to a signal which is sent through a cable to the receiver inside the building. Also called a low-noise block, low-noise converter (LNC), or even low-noise downconverter (LND), the device is sometimes inaccurately called a low-noise amplifier (LNA).
A diplexer is a passive device that implements frequency-domain multiplexing. Two ports are multiplexed onto a third port. The signals on ports L and H occupy disjoint frequency bands. Consequently, the signals on L and H can coexist on port S without interfering with each other.
A horn antenna or microwave horn is an antenna that consists of a flaring metal waveguide shaped like a horn to direct radio waves in a beam. Horns are widely used as antennas at UHF and microwave frequencies, above 300 MHz. They are used as feed antennas for larger antenna structures such as parabolic antennas, as standard calibration antennas to measure the gain of other antennas, and as directive antennas for such devices as radar guns, automatic door openers, and microwave radiometers. Their advantages are moderate directivity, broad bandwidth, low losses, and simple construction and adjustment.
The RATAN-600 is a radio telescope in Zelenchukskaya, Karachay–Cherkess Republic, Russia. It comprises a 576 m diameter circle of rectangular radio reflectors and a set of secondary reflectors and receivers, based at an altitude of 970 m. Each of the 895 2×7.4 m reflectors can be angled to reflect incoming radio waves towards a central conical secondary mirror, or to one of five parabolic cylinders. Each secondary reflector is combined with an instrumentation cabin containing various receivers and instruments. The overall effect is that of a partially steerable antenna with a maximum resolving power of a nearly 600 m diameter dish, when using the central conical receiver, making it the world's largest-diameter individual radio telescope.
A radio transmitter or receiver is connected to an antenna which emits or receives the radio waves. The antenna feed system or antenna feed is the cable or conductor, and other associated equipment, which connects the transmitter or receiver with the antenna and makes the two devices compatible. In a radio transmitter, the transmitter generates an alternating current of radio frequency, and the feed system feeds the current to the antenna, which converts the power in the current to radio waves. In a radio receiver, the incoming radio waves excite tiny alternating currents in the antenna, and the feed system delivers this current to the receiver, which processes the signal.
Microwave transmission is the transmission of information by electromagnetic waves with wavelengths in the microwave frequency range of 300MHz to 300GHz(1 m - 1 mm wavelength) of the electromagnetic spectrum. Microwave signals are normally limited to the line of sight, so long-distance transmission using these signals requires a series of repeaters forming a microwave relay network. It is possible to use microwave signals in over-the-horizon communications using tropospheric scatter, but such systems are expensive and generally used only in specialist roles.
Low-noise block downconverters (LNBs) are electronic devices coupled to satellite dishes for TV reception or general telecommunication that convert electromagnetic waves into digital signals that can be used to transform information into human or machine interpretable data, e.g., optical images, video, code, communications, etc.
Satellite television is a service that delivers television programming to viewers by relaying it from a communications satellite orbiting the Earth directly to the viewer's location. The signals are received via an outdoor parabolic antenna commonly referred to as a satellite dish and a low-noise block downconverter.
Radio is the technology of signaling and communicating using radio waves. Radio waves are electromagnetic waves of frequency between 3 hertz (Hz) and 3,000 gigahertz (GHz). They are generated by an electronic device called a transmitter connected to an antenna which radiates the waves, and received by another antenna connected to a radio receiver. Radio is widely used in modern technology, in radio communication, radar, radio navigation, remote control, remote sensing, and other applications.
Fibre satellite distribution is a technology that enables satellite TV signals from an antenna to be distributed using an optical fibre cable infrastructure and then converted to electrical signals for use with conventional set-top box receivers.