Wiki » History » Version 19
Version 18 (GOMEZ, Ramon, 12/12/2015 11:49 AM) → Version 19/54 (GOMEZ, Ramon, 12/12/2015 11:54 AM)
Proposal of structure:
Introduction - tell what is the aim of the project
State of art - talk about how L-band reception systems work currently
Project - Present our results, discuss them point by point
-Linearity - what is, show results, compare to the technical specification provided.
-Intermodulation - what is, show results, explain and compare to coax (theoretically)
-Phase/noise - what is, show results, explain and compare to coax (theoretically)
-Application
/////////////////START OF THE DOCUMENT//////////////////////////////////////////////////
h1. 1. Introduction
Earth stations are based on an indoor/outdoor unit architecture. The outdoor unit comprises antennas and the RF frontend (amplifier and up/down converter). The indoor unit includes the receiver, modem and network/application appliances. On typical consumer systems, the outdoor and indoor units are connected by means of a 75-ohm coaxial cable. The cable conveys the intermediate frequency (typically L band) signal between the indoor/outdoor units.
This approach, while being cost effective, is not optimal from a signal quality standpoint and might severely impair the end-to-end link budget. For example, typical attenuation values for a coaxial cable at a frequency of 1 GHz are in the order of 15 dB/100 m.
The objective of this project is to test and evaluate a system that makes possible to convert the L-band RF signal from/to optical and use an optical fibre (up to 10 km) as primary interconnection media. The signal is converted from optical back to RF in the indoor unit. As such, it is directed to DTH (Direct-To-Home) TV systems.
!schema.jpg!
h1. 2. State of the art
h1. 3. Measures
h2. 3.1 Linearity
h2. 3.2 Intermodulation
h2. 3.3 Phase/Noise
h1. 4. Results
h1. 5. Conclusions
h1. 6. Application
This section explains how the Outdoor system has been installed and the results obtained measuring a real TV signal from a Satellite.
h2. 6.1 Preparation
The optical transmitter has been put in an hermetic box.
Its interface consists of :
* The power supply plug to be connected to the mains ;
* The optical fiber harness (2 fibers) : only the red fiber is actually connected to optical transmitter ; the black fiber is not used, it will enable to have a b ;
* The type F coaxial cable to connect the Antenna Low Noise Block, LNB, to optical transmitter.
Optical transmitter is set to :
* To supply 18 V to LNB, which selects Horizontale polarization ;
* To provide 0 kHz tone to LNB, which set its Local Oscillator to 9.75 GHz to transpose lower Ku Band from 10.7 to 11.7 GHz into IF Band.
* This hermetic box has been mounted on Antenna mast. This Antenna is pointing to Astra 1KR/1L/1M/1N colocalized satellites on 19.2° East.
h2. 6.2 Trials
h3. 6.2.1 IF Spectrum with Optical Link
RF output from Optical receiver has been analyzed with Rohde & Schwartz FSV spectrum analyzer :
!rsz_1combine_images.png!
_IF Band, 1 Channel (with Optical Link)_
It is possible to distinguish several channels within the Inter Frequency, IF, band. There is a zoom on left side. The 3 dB channel bandwdith is 22 MHz.
The power is about -32 dBm for the channel centered around 1141 MHz.
!rsz_tv_channel.png!
_TV channel at 1141 MHz_
h3. 6.2.2 Link Quality with Optical link
First, optical link performance enables to have a good TV quality (for example, Eins Plus on 10744H). More deeply, physical link quality has been assessed with the information provided by IPRICOT SCB router.
This data has been compared with data from website like [[www.lingsat.com]] :
<table>
~~~~~~~~~
<table style="width:100%">
<tr>
<td>Jill</td>
<td>Smith</td>
<td>50</td>
</tr>
<tr>
<td>Eve</td>
<td>Jackson</td>
<td>94</td>
</tr>
</table>
~~~~~~~~~
|_.Ku Channel [MHz] |_.IF Channel [MHz] |_.TV |_.www.lingsat.com | _.Spectrum Analyzer | _.IPRICOT |
| 10744H | 994 | NI USRP 2920 | EINS Plus| DVB-S QPSK 22 Msps 5/6 | 22| 7.7 |
| 11244H | 1494 | Schau TV | EINS Plus| DVB-S QPSK 22 Msps 5/6 | 22 | 7.9 |
Introduction - tell what is the aim of the project
State of art - talk about how L-band reception systems work currently
Project - Present our results, discuss them point by point
-Linearity - what is, show results, compare to the technical specification provided.
-Intermodulation - what is, show results, explain and compare to coax (theoretically)
-Phase/noise - what is, show results, explain and compare to coax (theoretically)
-Application
/////////////////START OF THE DOCUMENT//////////////////////////////////////////////////
h1. 1. Introduction
Earth stations are based on an indoor/outdoor unit architecture. The outdoor unit comprises antennas and the RF frontend (amplifier and up/down converter). The indoor unit includes the receiver, modem and network/application appliances. On typical consumer systems, the outdoor and indoor units are connected by means of a 75-ohm coaxial cable. The cable conveys the intermediate frequency (typically L band) signal between the indoor/outdoor units.
This approach, while being cost effective, is not optimal from a signal quality standpoint and might severely impair the end-to-end link budget. For example, typical attenuation values for a coaxial cable at a frequency of 1 GHz are in the order of 15 dB/100 m.
The objective of this project is to test and evaluate a system that makes possible to convert the L-band RF signal from/to optical and use an optical fibre (up to 10 km) as primary interconnection media. The signal is converted from optical back to RF in the indoor unit. As such, it is directed to DTH (Direct-To-Home) TV systems.
!schema.jpg!
h1. 2. State of the art
h1. 3. Measures
h2. 3.1 Linearity
h2. 3.2 Intermodulation
h2. 3.3 Phase/Noise
h1. 4. Results
h1. 5. Conclusions
h1. 6. Application
This section explains how the Outdoor system has been installed and the results obtained measuring a real TV signal from a Satellite.
h2. 6.1 Preparation
The optical transmitter has been put in an hermetic box.
Its interface consists of :
* The power supply plug to be connected to the mains ;
* The optical fiber harness (2 fibers) : only the red fiber is actually connected to optical transmitter ; the black fiber is not used, it will enable to have a b ;
* The type F coaxial cable to connect the Antenna Low Noise Block, LNB, to optical transmitter.
Optical transmitter is set to :
* To supply 18 V to LNB, which selects Horizontale polarization ;
* To provide 0 kHz tone to LNB, which set its Local Oscillator to 9.75 GHz to transpose lower Ku Band from 10.7 to 11.7 GHz into IF Band.
* This hermetic box has been mounted on Antenna mast. This Antenna is pointing to Astra 1KR/1L/1M/1N colocalized satellites on 19.2° East.
h2. 6.2 Trials
h3. 6.2.1 IF Spectrum with Optical Link
RF output from Optical receiver has been analyzed with Rohde & Schwartz FSV spectrum analyzer :
!rsz_1combine_images.png!
_IF Band, 1 Channel (with Optical Link)_
It is possible to distinguish several channels within the Inter Frequency, IF, band. There is a zoom on left side. The 3 dB channel bandwdith is 22 MHz.
The power is about -32 dBm for the channel centered around 1141 MHz.
!rsz_tv_channel.png!
_TV channel at 1141 MHz_
h3. 6.2.2 Link Quality with Optical link
First, optical link performance enables to have a good TV quality (for example, Eins Plus on 10744H). More deeply, physical link quality has been assessed with the information provided by IPRICOT SCB router.
This data has been compared with data from website like [[www.lingsat.com]] :
<table>
~~~~~~~~~
<table style="width:100%">
<tr>
<td>Jill</td>
<td>Smith</td>
<td>50</td>
</tr>
<tr>
<td>Eve</td>
<td>Jackson</td>
<td>94</td>
</tr>
</table>
~~~~~~~~~
|_.Ku Channel [MHz] |_.IF Channel [MHz] |_.TV |_.www.lingsat.com | _.Spectrum Analyzer | _.IPRICOT |
| 10744H | 994 | NI USRP 2920 | EINS Plus| DVB-S QPSK 22 Msps 5/6 | 22| 7.7 |
| 11244H | 1494 | Schau TV | EINS Plus| DVB-S QPSK 22 Msps 5/6 | 22 | 7.9 |