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A low-noise block converter (LNB, for low-noise block, or sometimes LNC, for low-noise converter) is used in communications satellite (usually broadcast satellite) reception (downlink). The LNB is usually fixed on or in the satellite dish, for the reasons outlined below. An LNB is used in conjunction with a Block upconverter (BUC).

Satellites use comparatively high radio frequencies to transmit their signals.

As microwave satellite signals do not easily pass through walls, roofs, or even glass windows, satellite antennas are required to be outdoors, and the signal needs to be passed indoors via cables. When radio signals are sent through coaxial cables, the higher the frequency, the more losses occur in the cable per unit of length. The signals used for satellite are of such high frequency (in the multiple gigahertz range) that special (costly) cable types or waveguides would be required and any significant length of cable leaves very little signal left on the receiving end.

The job of the LNB is to use the superheterodyne principle to take a wide block (or band) of relatively high frequencies, amplify and convert them to similar signals carried at a much lower frequency (called intermediate frequency or IF). These lower frequencies travel through cables with much less attenuation of the signal, so there is much more signal left on the satellite receiver end of the cable. It is also much easier and cheaper to design electronic circuits to operate at these lower frequencies, rather than the very high frequencies of satellite transmission.

The “low-noise” part means that special electronic engineering techniques are used, that the amplification and mixing takes place before cable attenuation and that the block is free of additional electronics like a power supply or a digital receiver. This all leads to a signal which has less noise (unwanted signals) on the output than would be possible with less stringent engineering. Generally speaking, the higher the frequencies with which an electronic component has to operate, the more critical it is that noise be controlled. If low noise engineering techniques were not used, the sound and picture of satellite TV would be of very low quality, if it could even be received at all without a much larger dish reflector. The low-noise quality of an LNB is expressed as the noise figure or noise temperature.

For the reception of wideband satellite television carriers, typically 27 MHz wide, the accuracy of the frequency of the LNB local oscillator need only be in the order of ±500 kHz, so low cost dielectric oscillators (DRO) may be used. For the reception of narrow bandwidth carriers or ones using advanced modulation techniques, such as 16-QAM, highly stable and low phase noise LNB local oscillators are required. These use an internal crystal oscillator or an external 10 MHz reference from the indoor unit and a phase-locked loop (PLL) oscillator.

Contents 1 LNBFs 2 Universal LNB 3 Standard North America Ku-band LNB 4 North America DBS LNB 5 C-band LNB 6 Dual/Quad/Octo LNBs 7 Monobloc LNBs 8 Cold temperatures 9 See also 10 External links

Direct broadcast satellite (DBS) dishes use an LNBF (“LNB feedhorn”), which integrates the antenna’s feedhorn with the LNB. Small diplexers are often used to distribute the resulting IF signal (usually 950 to 1450 MHz) “piggybacked” in the same cable TV wire that carries lower-frequency terrestrial television from an outdoor antenna. Another diplexer then separates the signals to the receiver of the TV set, and the integrated receiver/decoder (IRD) of the DBS set-top box.

Newer K_a band systems use additional IF blocks from the LNBF, one of which will cause interference to UHF and cable TV frequencies above 250 MHz, precluding the use of diplexers. The other block is higher than the original, up to 2.5 GHz, requiring the LNB to be connected to high-quality all-copper RG-6/U cables. This is in addition to higher electrical power and electrical current requirements for multiple dual-band LNBFs.

For some satellite Internet and free-to-air (FTA) signals, a universal LNB (K_u band) is recommended. Most North American DBS signals use circular polarization, instead of linear polarization, therefore requiring a different LNB type for proper reception. In this case, the polarization must be adjusted between clockwise and counterclockwise, rather than horizontal and vertical.

In the case of DBS, the voltage supplied by the set-top box to the LNB determines the polarisation setting. With multi-TV systems, a dual LNB allows both to be selected at once by a switch, which acts as a distribution amplifier. The amplifier then passes the proper signal to each box according to what voltage each has selected. The newest systems may select polarization and which LNBF to use by sending DiSEqC codes instead. The oldest satellite systems actually powered a rotating antenna on the feedhorn, at a time when there was typically only one LNB or LNA on a very large TVRO dish.

A universal LNB can receive both polarisations and the full range of frequencies in the satellite Ku or C band. Some models can receive both polarisations simultaneously through two different connectors, and others are switchable or fully adjustable in their polarisation.

Here is an example of Universal LNB specifications:

• LO: 9.75 / 10.6 GHz.
• Freq: 10.7–12.75 GHz.
• NF: 0.7 dB (although significantly lower is possible)
• Polarization: Linear

By covering a smaller frequency range a LNB with a better noise figure can be produced. Pay TV operators can also supply a single fixed polarization LNBF to save a small amount of expense.

Here is an example of a Standard Linear LNB:

• Local oscillator: 10.75 GHz
• Frequency: 11.7-12.2 GHz
• Noise Figure: 0.5 dB
• Polarization: Linear
• Today,modern LNB'S give 0.3 - 0.2 and now also 0.1 dB(Noise levels during the transmission of signals)

Here is an example of an LNB used for DBS:

• Local oscillator: 11.25 GHz
• Frequency: 12.2-12.7 GHz
• Noise figure: 0.7 dB
• Polarization: Circular

Here is an example of a North American C-band LNB:

• Local oscillator: 5.15 GHz
• Frequency: 3.4-4.2 GHz
• Noise figure: ranges from 15 to 100 kelvins (uses Kelvin ratings as opposed to dB rating).
• Polarization: Linear

Two or four LNBs are in one unit to enable use of multiple receivers on one dish. In the case of an octo LNB, the unit contains a quad and a multiswitch.

A monobloc LNB (also spelled "monoblock") is a unit consisting of two LNBs and is designed to receive satellites spaced close together, generally 6 degrees. For example in parts of Europe monoblocs designed to receive the Hot Bird (13E) and Astra 1 (19E) satellites are popular because they enable reception of both satellites on a single dish without requiring an expensive and noisy rotator.

It is possible for an LNB to physically freeze due to ice build-up in very low temperatures, obscuring the signal. This is only likely to occur when the LNB is not receiving power from the satellite receiver (i.e. no programmes are being watched). To combat this, many satellite receivers provide an option to keep the LNB powered while the receiver is on standby.

• Block Up Converter BUC
• Orthomode Transducer
• signal-to-noise ratio
• Bias tee

• LNB Installation Diagram.
• LNB mysteries explained.
• Explanation and block diagram of LNB
• Noise Temperature and Noise Figure