Inverto IDLB-QUDL40-ULTRA-OPP 3310 Merkblatt
Produktcode
3310
TM
Quad High-Gain Low-Noise 40mm LNB
IDLB-QUDL40-ULTRA-OPP
BLACK Ultra
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 isolation and advanced filter design
enables improved handling of interfering spurious and provides the leap in the overall
reception performance compared with standard LNBs. This LNB enables the reception of
signal from one satellite and its distribution to up-to 4 single tuner Set-top boxes (or 2 in
the case of a twin-tuner STB) and is ready for High Definition transmissions. Manufactured
to the highest industry quality standards and designed to meet strict specifications, this
LNB is an ideal solution for the satellite broadcast reception across Europe.
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 isolation and advanced filter design
enables improved handling of interfering spurious and provides the leap in the overall
reception performance compared with standard LNBs. This LNB enables the reception of
signal from one satellite and its distribution to up-to 4 single tuner Set-top boxes (or 2 in
the case of a twin-tuner STB) and is ready for High Definition transmissions. Manufactured
to the highest industry quality standards and designed to meet strict specifications, this
LNB is an ideal solution for the satellite broadcast reception across Europe.
Main Features
•
Superior Phase Noise performance DVB-S2 (HDTV) compliant
•
Excellent isolation – extremely high cross-pol performance
•
Very low spurious levels
•
Superior Noise Figure
•
Higher conversion gain
•
Ultimate reliability
High-Gain
Low-Noise
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