Editorial Technical Reference

Low-Noise Block Downconverter (LNB)

This page explains how Low-Noise Block Downconverter (LNB) is classified within Computer, Electronic and Optical Product Manufacturing. Technical values and manufacturer relationships are research references; confirm the current specification and supplier evidence for each order.

Technical Definition & Core Assembly

A device that receives and downconverts satellite signals to a lower frequency for transmission via coaxial cable.

Representative product image. Confirm appearance and specifications with the manufacturer.

Product Specifications

Technical details and manufacturing context for Low-Noise Block Downconverter (LNB)

Definition
A Low-Noise Block Downconverter (LNB) is a critical component in satellite communication systems, typically mounted on satellite dishes. It receives weak microwave signals from satellites, amplifies them with minimal added noise, and converts them to lower frequencies (typically L-band) for transmission through coaxial cables to satellite receivers inside buildings. The LNB is part of the outdoor unit of a satellite reception system and is designed for continuous outdoor operation, with weatherproofing rated IP54 to IP67 per IEC 60529. It operates over a wide temperature range, from -40°C to 60°C, and can be stored from -40°C to 80°C. The device is powered via the coaxial cable with a supply voltage of 11–20 V DC and consumes 150–250 mA. It features an input frequency range covering Ku-band (10.7–12.75 GHz) and C-band (3.4–4.2 GHz) downlinks, and outputs intermediate frequencies in the 950–2150 MHz range. Key performance parameters include a noise figure of 0.1–0.5 dB, conversion gain of 50–60 dB, and input/output VSWR of ≤2.5:1 and ≤2.0:1, respectively. The local oscillator frequency is selectable at 9.75 or 10.6 GHz. The LNB uses an F-type connector for output. Typical materials include an aluminum housing, printed circuit board, semiconductor components such as GaAs FETs/HEMTs, dielectric materials, and copper conductors. The weight ranges from 100–300 g. Always verify model-specific values and standards with the legal manufacturer or supplier.
Working Principle
The LNB receives high-frequency satellite signals (e.g., Ku-band: 10.7-12.75 GHz, C-band: 3.4-4.2 GHz) via the feedhorn. It amplifies these weak signals using a low-noise amplifier (LNA) to minimize signal degradation. Then, a local oscillator (LO) generates a fixed frequency that mixes with the incoming signal in a mixer, producing intermediate frequencies (IF) in the 950-2150 MHz range. These lower-frequency signals are then transmitted through coaxial cable to the indoor receiver.
Common Materials
Aluminum housing, Printed circuit board (PCB), Semiconductor components (GaAs FETs/HEMTs), Dielectric materials, Copper conductors
Technical Parameters
ParameterTypical rangeNotes & selection driver
Input Frequency Range10.7–12.75 GHzCovers Ku-band satellite downlink.
Output Frequency Range950–2150 MHzStandard IF for satellite receivers.
Noise Figure0.1–0.5 dBLower is better for weak signals.
Conversion Gain50–60 dBEnsures sufficient signal level.
Local Oscillator Frequency9.75 or 10.6 GHzSelectable for different bands.
Input VSWR≤2.5:1Max reflection at input.
Output VSWR≤2.0:1Max reflection at output.
Supply Voltage11–20 V DCPowered via coaxial cable.
Current Consumption150–250 mATypical for LNB operation.
Operating Temperature-40–60 °COutdoor installation range.
Storage Temperature-40–80 °CNon-operating survival range.
Ingress ProtectionIP54–IP67Weatherproof for outdoor use.IEC 60529
Connector TypeF-typeStandard for satellite IF.
Weight100–300 gLightweight for mounting.

Ranges are indicative industry figures for RFQ preparation, not a supplier commitment. Confirm every value and standard with the legal manufacturer before ordering.

Components / BOM
  • Feedhorn
    Collects and focuses satellite signals into the waveguide
    Material: Aluminum or plastic
  • Waveguide
    Transmits microwave signals from feedhorn to PCB
    Material: Aluminum
  • Low-Noise Amplifier (LNA)
    Amplifies weak satellite signals with minimal added noise
    Material: Gallium Arsenide (GaAs) semiconductor
  • Local Oscillator (LO)
    Generates stable frequency for downconversion mixing
    Material: Quartz crystal, semiconductor components
  • Mixer
    Combines incoming signal with LO frequency to produce IF
    Material: Semiconductor diodes or transistors
  • IF Amplifier
    Amplifies the downconverted intermediate frequency signal
    Material: Semiconductor components on PCB

Industry Taxonomies & Aliases

Commonly used trade names and technical identifiers for Low-Noise Block Downconverter (LNB).

Applied To / Applications

This component is essential for the following industrial systems and equipment:

Industrial Ecosystem & Supply Chain Structure

Complementary Systems
Downstream Applications
Specialized Tooling

Application Fit & Sizing Matrix

Operational Limits
pressure: Atmospheric pressure only (sealed unit, not pressure-rated)
other spec: Input Frequency Range: 10.7-12.75 GHz, Output Frequency: 950-2150 MHz, Local Oscillator Frequency: 9.75/10.6 GHz, Noise Figure: 0.3-0.7 dB typical
temperature: -40°C to +70°C (operational), -55°C to +85°C (storage)
Media Compatibility
✓ Satellite RF signals (Ku-band, C-band) ✓ Coaxial cable transmission (75Ω impedance) ✓ Outdoor weather exposure (with proper housing)
Unsuitable: High-vibration industrial environments without vibration damping
Sizing Data Required
  • Satellite frequency band (Ku/C/Ka-band)
  • Required LO frequency and polarization (single/dual/universal)
  • Antenna size and required gain/noise figure

Reliability & Engineering Risk Analysis

Failure Mode & Root Cause
Dielectric breakdown in RF amplifier
Cause: Moisture ingress due to compromised weather seals or condensation from thermal cycling, leading to short circuits and signal loss.
Local oscillator frequency drift
Cause: Thermal stress on oscillator components from prolonged exposure to temperature extremes, causing component aging and frequency instability.
Maintenance Indicators
  • Intermittent or complete loss of signal despite clear line-of-sight and proper alignment
  • Visible corrosion, cracking, or water droplets inside the LNB housing or on the feedhorn
Engineering Tips
  • Apply high-quality dielectric grease to all coaxial connections and ensure weatherproofing boots are intact to prevent moisture ingress.
  • Install a passive thermal shield or sunshade to reduce direct solar heating, minimizing thermal cycling stress on electronic components.

Indicative industry ranges for design and RFQ preparation. Confirm the exact figures and applicable standard with the manufacturer before specifying.

Compliance & Manufacturing Standards

Applicable Standards
CE Marking (Electromagnetic Compatibility Directive 2014/30/EU) ASTM E595-15 (Standard Test Method for Total Mass Loss and Collected Volatile Condensable Materials from Outgassing in a Vacuum Environment)

Quoted from the published standard.

Manufacturing Precision
  • Local Oscillator Frequency Stability: +/- 500 kHz
  • Gain Flatness: +/- 0.5 dB across operating band
Quality Inspection
  • Phase Noise Measurement Test
  • Return Loss/VSWR Test

Manufacturers of Low-Noise Block Downconverter (LNB)

Manufacturer profiles associated with Low-Noise Block Downconverter (LNB).

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Frequently Asked Questions

What is the typical input frequency range of an LNB?

The input frequency range covers Ku-band (10.7–12.75 GHz) and C-band (3.4–4.2 GHz) downlink frequencies, as listed in the directory. Confirm the exact range for your model.

How is the LNB powered?

The LNB is powered via the coaxial cable with a DC supply voltage of 11–20 V and consumes 150–250 mA. The receiver typically provides this voltage.

What is the noise figure and why is it important?

The noise figure is 0.1–0.5 dB. Lower noise figure means less signal degradation, which is critical for weak satellite signals. Verify the value for your specific LNB.

What connector type does the LNB use?

The output connector is F-type, which is standard for satellite IF signals. Ensure your cable and receiver are compatible.

Data Basis

Editorial classification, named public sources where available, and source-reviewed manufacturer records.

Preliminary Technical Classification
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