Want multiple satelites?

Want to receive more then 2 satellites on a standard dish?Have a look at our innovative MultiConnect system and learn what it can do for you...

BLACK Ultra

Twin HGLN 40mm LNB

IDLB-TWNL40-ULTRA-OPP

IDLB-TWNL40-ULTRA-OPP

This LNB is a high performance product featuring the lowest noise figure available to address the need for superior reception under the edges of the satellite footprint skirt. Thanks to its novel front-end architecture and superior components, this LNB provides higher conversion gain yet with lowest noise figure and best phase noise performance. The combination of higher spec components, excellent cross polarization isolation and advanced filter design enables improved handling of interfering spurious. All in all, this LNB provides a leap in the overall reception performance compared with standard LNBs. This LNB enables the reception of signals from one satellite, its distribution to maximum up to two  Set Top Boxes with Single Tuner (or one STB with Twin Tuner) and is ready for High Definition transmissions. Designed to meet strict specifications and manufactured to the highest industry quality standards, this LNB is an ideal solution for the satellite broadcast reception across Europe.  

 

Main Features•  Superior Phase Noise Performance, DVB-S2 (HDTV) compliant

•  Excellent Cross Polarization Isolation

•  Very low Spurious Levels

•  Superior Noise Figure

•  Higher Conversion Gain

•  Ultimate Reliability

Product Specifications
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Low Band Input Frequency Range 10.7 ~ 11.7 GHz
Low Band Output Frequency Range 950 ~ 1950 MHz
Low Band LO Frequency 9.75 GHz
High Band Input Frequency Range 11.7 ~ 12.75 GHz
High Band Output Frequency Range 1100 ~ 2150 MHz
High Band LO Frequency 10.6 GHz
Noise Figure 0.2 dB Typ. (0.7 dB Max.)
LO Initial Accuracy +/- 1.0 MHz Max.
LO Temperature Drift +/- 3.0 MHz Max.
Phase Noise (@ 10 kHz) - 90 dBc / Hz Max.
Conversion Gain 60 dB Min.
Gain Ripple (Over 26MHz Bandwidth) +/- 0.75 dB
Gain Variation (Over Full Band)  +/- 4 dB Max.
Image Rejection 40 dB Min.
1 dB Compression Point (@ Output) 0.0 dBm Min.
Cross Polarization Isolation 22 dB Min.
Control Signal Ca (Vertical Polarization) 11.0 ~ 14.0 V
Control Signal Cb (Horizontal Polarization) 16.0 ~ 20.0 V
Control Signal Cc (Band Switching) 22 +/- 4 kHz
Output VSWR 2.0 : 1 
In-Band Spurious - 60 dBm Max.
Current Consumption 180 mA Max. @ 11 ~ 20 V
Operating Temperature - 30 °C  ~  + 60 °C
Output Impedance 75 Ω
Output Connector F-Type (Female)
Weight 181 g
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Frequently Asked Questions

What is a feedhorn?

The feedhorn is the part of a satellite dish system which gathers the reflected signal from the dish and focuses it towards the LNB.

What is an LNB?

An LNB - Low Noise Block (also called an LNC- Low Noise Converter), is used for communications (broadcast) satellite reception. The LNB is usually affixed either in or on the satellite dish.

What is an LNBF?

An LNBF is an LNB with an integrated feedhorn

What is a Monoblock LNB?
This design consists of two independent LNBs in a single case. The two LNBs can be automatically addressed with any DiSEqC 1.0 or higher receiver. In some cases they can also be addressed with ToneBurst / MiniDiSEqC. However, they are only available for satellites with a fixed 3 degree, 4.3 degree, 6 degree …spacing. In Europe, for example, there are monoblock single, twin and quad LNBs for the Ku band, which have a pre-defined spacing of 6 degrees (for Astra 1 / Hotbird , for example).

Why can I receive only one satellite with my Monoblock?

Monoblock LNBs are designed for a specific dish size, 80cm for example. If your dish is too small (70cm for example) or too wide (90cm for example) it is not possible to receive both satellites together. Please choose the dish size for which the monoblock LNB has been designed.