Low noise signal converter

from Wikipedia, the free encyclopedia
Mounted LNB

The first electronic component of a satellite receiving system located in the focus of a parabolic antenna or in the signal decoupling of a panel antenna is referred to as the low-noise signal converter (from the English Low Noise Block , LNB for short ; and Low Noise Converter , LNC for short ) .

It converts the satellite frequency from, for example, 10.7-11.75 or 11.8-12.75  GHz to the 950-2150 MHz range  , thereby enabling cable transmission through a coaxial cable and, more recently, also with fiber optics and reception with a satellite receiver . A "digitally suitable" universal LNB does not have to process digital signals, but only has to be able to convert the full frequency range from 10.7 to 12.75 GHz. Initially, DVB signals were only sent in the upper range from 11.7 GHz, but in view of the analog TV switch-off, almost all transponders from 10.7 GHz upwards are now occupied with digital TV signals.

An LNB consists of the combination of a low-noise amplifier ( LNA ) with a block converter (see below). If a feed horn (from the English feed horn for " feed horn ") is attached, it is also referred to as LNBF ( Low Noise Block Feed ) or LNF ( Low Noise Feed ).

Layout and function

After the high-frequency microwaves of a geostationary telecommunications satellite have been bundled by a parabolic mirror or a panel antenna , the LNB fulfills the following additional tasks for satellite reception:

LNB disassembled ( all parts )
Block diagram of a universal LNB
Historic TV-SAT- LNB with HF filter, left and right polarization
  1. The feed horn (also: croissant) used in parabolic antennas consists of a metallic cylinder or cone with dimensions that exactly match the reception frequency range. It serves to match the impedance and, as a waveguide structure, also fulfills a filter function against external radiation. The end facing the parabolic mirror is open and allows the electromagnetic waves to enter, a plastic protective cap prevents dust or water from entering. At the other end are the exciters of the antenna construction, i. H. the transition from waveguide to stripline .
  2. The LNBs have to separate the polarization modes of the incident waves (horizontal, vertical or circular polarization ). While this was achieved in the early days of satellite reception using mechanical rotating devices or polarizers , there have usually been separate signal paths with appropriately arranged antennas since the 1990s . These two receiving antennas, which protrude from the left and from above into the waveguide of the grooved horn antenna , can be clearly seen in the adjacent picture. They direct the received energy over a short distance to the downstream amplifier transistors.
  3. It amplifies the captured signals and reduces the frequency to the intermediate frequency (IF) according to the principle of the heterodyne receiver . This is necessary in order to be able to transmit the received signal with normal coaxial cable to a satellite receiver with little loss . The reaction is accomplished by the received signal with a local oscillator frequency (LOF) multiplicatively mixed is (typically 9.75 GHz at Lowband- and 10.6 GHz at high band reception). With the so-called universal LNB, different satellite frequency bands can be mapped to the same IF range by remote-controlled switching of this frequency and thus switched between the low band (mainly analog programs) and the high band (mainly digital programs).

The LNB is supplied with power via remote feed via the antenna cable. The Marconi standard, which has been established since the late 1980s, enables the level of polarization to be selected via the level of the supply voltage (14 volts vertical, 18 volts horizontal). The switching threshold is 15 V and allows voltage drops on up to 3 diodes in upstream DiSEqC switches and in the supply cable itself. With the universal LNB (10.7–12.75 GHz), a superimposed permanent switching frequency (22 kHz ± 20% ) Alternatively, the later added high band from 11.7 GHz can be selected. In order to be able to serve more than two switching criteria, the digital control bus DiSEqC - later with return channel - was developed jointly by the satellite operator Eutelsat and the Philips company in the early 1990s . With a modulated 22 kHz frequency, this enables the control of up to 256 different components of a satellite receiving system. DiSEqC components can work with a reduced operating voltage of 12 volts in order to reduce power loss.

The entire functional unit is usually integrated in a common weatherproof housing - in the case of panel antennas, in this. In addition to protection against moisture, dust and temperature influences, it must ensure that in the area of ​​the wave entry window, as far as possible, no impurities or water (possibly also as snow or ice) can adhere to the outside. The neck has a diameter of 40 mm (in the commonly received Ku-band), with which the LNB is attached to a clamp (feed holder) of the parabolic antenna. For multi-feed systems there are LNBs with a 23 mm neck diameter.

Problem areas of satellite reception

If you look at the transmission lobe of a satellite , i.e. its coverage zone on the earth's surface ( called footprint ), it becomes understandable that the signal power density on the ground can only be low. Highly bundling antennas ( parabolic mirrors , panel antennas ) are used so that the useful signal stands out from the thermal background noise of the cosmic background radiation in relation to the entire baseband . If they are correctly aligned on the geostationary satellite, they transmit a sufficient amount of useful signal and only little interference into the “feed” of the LNB. At too low signal to noise ratio (SNR, English signal-to-noise ratio given) to which it further by a too small or misaligned antenna, by attenuation of the signal (snow, rain), or by injecting noise sources (reflections ) can occur is no more reception possible.

Since the noise power of the thermal noise depends on the baseband bandwidth, this becomes all the more problematic the larger the frequency range used.

A universal LNB switches between two different frequency ranges in order to cover the entire reception range from 10.7-12.75 GHz, as the frequency bandwidth between the upper and lower limit frequency (2.05 GHz) does not fall into the reception range of the satellite receiver of 950– 2150 MHz fits.

Since every amplifier makes noise and adds this inherent noise to the signal, the SNR in a signal chain can never get better, it can only get worse. An LNB therefore requires a particularly low-noise amplifier in the entire baseband in order to still be able to receive reception even in poor reception conditions. Typical of universal LNBs is since 2004 a self-noise (related terms: noise , noise figure , Eng. Noise figure , noise floor ) of about 0.6 dB (0.6 to 0.7 dB at 21 ° C are considered to be very good) . Lower noise figures of 0.2 and 0.3 dB are not possible in the private sector, since in the first stage of the LNA, according to the manufacturer's data sheets, the amplifier transistor already has a self-noise of approx. 0.3 dB under optimal conditions. This means that the total noise figure can only be higher if several amplifier stages (with low-noise so-called HEMTs ) are connected in series. The reinforcement of the individual levels also plays a decisive role.

When choosing receiver components, weather resistance should also be taken into account. In addition to general air pollution, snow and ice as well as bird droppings (feedhorn receiving side) can also dampen the signal. Occasionally, LNBs are offered with a thin film cover in order to achieve an even lower attenuation value. However, these are very delicate and difficult to clean.

Origin of the name

A low self-noise is an important quality feature of this component, but "Low Noise" as part of the name is quite peculiar and can only be explained by historical development.

In the early days of satellite reception (and for special applications still today), the high-frequency signal from the satellite was only amplified and passed to the receiver without conversion to an intermediate frequency. Low noise was particularly important and the corresponding high-frequency amplifiers, which were very complex at the time, were called LNAs ( low-noise amplifiers ). With this construction, only short, low-attenuation cable connections between antenna and receiver are possible.

To enable satellite reception for private users, the LNC ( low noise converter ) was introduced in the 1980s . In addition to amplification, this is also converted to a lower intermediate frequency (IF), which simplifies the connection to the receiver. Reception frequency range of an LNC was normally 10.95-11.7 GHz; for the TV-SAT and TDF satellites there were LNCs with a reception frequency range of 11.7–12.5 GHz.

  • To receive several polarization planes, either a polarizer connected upstream in an LNC or a polarization switch with its own LNC for each polarization arranged in the waveguide was necessary.
  • For the reception of two different satellite frequency bands, as used for the first time by the German telecommunications satellite DFS-Kopernikus in direct radio reception, LNCs that can receive two frequency bands were necessary. DFS-Kopernikus broadcast in the frequency range of 10.95–11.7 and 12.5–12.75 GHz.

LNBs that can receive both polarization levels have been used in the private sector since the early 1990s. The additional block refers to the fact that an LNB processes several frequency blocks of different polarization and frequency at once;

Universal twin LNBF
  • either they are output in parallel via separate IF signal outputs
  • or the receivers use control signals on an LNB to select a frequency block desired for reception.

LNCs can therefore only be found on old systems and in professional antenna systems and are no longer newly installed in direct reception.

When the components are fully integrated, one sometimes speaks of the LNBF or the LNF . "Feed" means the signal supply.

The various abbreviations are often used synonymously in practice, even by experts.


LNBF with integrated DiSEqC switch and open grooved horn radiator

Only with the advent of the DTH antennas (antennas for direct-to-home reception, where Astra was one of the pioneers) are the feed horns attached directly to the Ku-band LNBs. Previously, the LNBs had a standardized flange that fit onto the counter flange of the feedhorn. This was also necessary because the LNBs did not have a level switch or a low / high band switch in the early years. The level separation was done with so-called orthomodes - for this a separate LNC was necessary for each level - or polarizers. LNBs are often used together in receiving systems with so-called multi - switches .

Differentiation of the LNBs according to the reception area
Until the end of the 1990s, LNBs designed for what is now called the low-band (10.7–11.7 GHz) were common. Since the advent of digital technology, satellite operators have also been using the so-called high band (11.7–12.75 GHz). LNBs, which can convert both frequency ranges directly into the frequency band used by the receiver, have since been referred to as universal LNB . Such a universal LNB is necessary for systems with which (mostly digital) programs are to be received in high band. The designation digitally suitable for the LNB itself is misleading, because every LNB can convert analog and digital signals from both the low-band and the high-band into the corresponding frequencies. It stems from the fact that the older low band mainly contained analog signals, while the later added high band was primarily used for digital programs. In the course of the displacement of analog channels in favor of digital broadcasting technology, the low-band has now also been switched to digital broadcasts. The term digitally suitable for an LNB only means that it can also convert the frequencies / channels of the high band and has nothing to do with any analog or digital electronics in the LNB. LNBs that can only receive the low band have meanwhile been pushed out of the market by the compatible universal LNBs and are no longer used for new installations or repairs. In the course of switching off the analogue satellite supply in Germany, most of these LNBs have been replaced by the universal LNBs at the customer.
Some manufacturers advertise LNBs as HD or 3D compatible. However, an LNB works independently of the video and transmission standard. Since the frequency band has not changed for DVB-S2 (or 3D and HDTV ), every digital LNB works for it. For the vast majority of HDTV channels (exceptions include Tele 5, WDR and Sky), it doesn't even have to be digital.
Wideband LNBs have also been available since 2015. These LNBs each have an outlet for the horizontal and vertical signal. The entire frequency band (10.7–12.75 GHz) is converted to the output frequency range of 300–2350 MHz with an oscillator frequency of 10.40 GHz. Currently these LNBs are mainly used to supply Unicable 2 multiswitches with several satellites. Satellite receivers, on the other hand, are generally unable to receive or can hardly receive more than the intermediate frequencies 950–2,150 MHz.
Differentiation of the LNBs according to the number and type of outputs
  • Single or single LNB with an output for direct connection of a receiver.
  • Twin or double LNB with two independent outputs for connecting two receivers. The corresponding switching device ( multi-switch ) is usually integrated. But there are also (older) variants of so-called dual LNB for pure lowband reception with two different connections that deliver both horizontal and vertical polarization (for connection to an external multi-switch).
  • Wideband LNB have one outlet each for the horizontal and vertical signal. The entire frequency band (10.7–12.75 GHz) is converted to the output frequency range of 300–2350 MHz with an oscillator frequency of 10.40 GHz. These LNBs are currently mainly used to supply Unicable2 multiswitches with several satellites.
  • Quad or Quattro switch LNB with 4 independent connections for connecting 4 receivers. The multi-switch is integrated.
  • Quattro LNB with 4 different connections (also with note: suitability for feed system). With this variant without a built-in multi-switch, horizontally and vertically polarized signals are brought out separately for low band and high band. A downstream multi-switch can then be used for distribution to almost any number of satellite receivers (up to a few hundred).
    • There is a high risk of confusion between the two types with 4 connections. In the meantime, at least the uniform designation has become established, according to which LNBs for the direct connection of up to four receivers are called Quad or sometimes Quattro with switch , while a Quattro LNB can only be used with a downstream multi-switch. With the Quattro the 4 connections are marked accordingly (polarization level: horizontal / vertical, frequency band high / low).
  • Octo-LNB with integrated multi-switch for the direct connection of up to eight satellite receivers.
  • Unicable- LNB has a single connection, through which several receivers can be connected via a common coaxial cable. A Unicable LNB does not output a complete frequency band, as is usually the case, but only a UB (= User Band ) (UB slot ID and UB frequency)for each receiver that can be connected. The program selection takes place in the LNB for each receiver separately via DiSEqC -controlled commands. The output frequency on the LNB does not change. A Unicable LNB can usually supply a maximum of four satellite receivers (tuners) with signals via a common coaxial cable. These are standardized according to the SCR / CSS CENELEC EN50494 standard. In addition to the pure Unicable LNBs, there are also those with 1 to 3 so-called legacy outputs, to which non-Unicable-capable receivers (tuners) can be connected.
    • Unicable II LNB has been around since 2015. These enable the connection of up to 32 receivers (tuners) via a common coaxial cable. These are standardized according to the SCR / CSS CENELEC EN50494 / EN50607 standard. In 2017, however, there was no commercially available Unicable II LNB with additional legacy outputs.
    • Since 2018 there has also been a Unicable II LNB with a connection option for up to 24 receivers (tuners) via a common coaxial cable and the further option of up to 3 legacy outputs.
Differentiation of the LNBs through additional functions
  • iLNB (interactive LNB): Recently used in satellite systems with a return channel, mainly for sending and receiving internet signals. Depending on the design, it can send to and receive from the satellite in the Ku or Ka band.

Monoblock LNB

Monoblock LNB for two satellite positions

A so-called monoblock LNB (sometimes also called DUO-LNB for two satellite positions) combines several LNBs for two to four different satellite positions in one housing. The satellite positions are specified by the LNB housing and the size of the parabolic antenna. In addition, an is DiSEqC - relay installed. In older duo LNBs, the satellite switching is also controlled via Toneburst . This allows you to switch between the two satellite positions using the DiSEqC signal.

An iLNB for Astra2Connect

Other satellite systems

The designs described above relate to the satellite television systems customary in Germany, all of which work in the Ku band . However, there are many other LNBs for other frequency ranges and applications, e.g. B. Meteosat LNBs, L-band LNBs, S-band LNBs, C-band LNBs.

Web links

Commons : Low Noise Signal Converters (LNBs)  - collection of images, videos and audio files