e/o and o/e devices, the collaboration with the industry:

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E/O and O/E devices, the collaboration with the industry: Optical connectors: Optical fibre cable: Analogue optical links experiences in the framework of the SKA/BEST activities Federico Perini INAF-IRA (I) Custom product: optimised specs (<1GHz) and mechanical RX housing. TX RX Power Supply, single positive = (12- 15)Volt@75mA Passive optical receiver APC (Angle Polished Connector) has RL>70dB → increases the performance of the RoF link (Dynamic and NF) Motivation: Necessity to bring the signal from the BEST Front End, on the antenna focal lines, to the central processing room. Which solution: Coax or Optical cables? Analogue or Digital links? Cost and Reliability prediction analysis of the whole receiver chain indicated the analogue optical link as the best solution, so: Which kind of fibre? Which kind of optical connectors? What E/O and O/E devices? Monomode loose fibre cable are the best in term of insertion loss and phase stability vs temperature and bending DIN best on moving antennas SC: best for fixed indoor applications with high integration SC could be the best compromise Laser DFB 1310nm MQW SPV4260 Sumitomo RIN = -155dB/Hz = 0,2 mW/mA I th = 8mA PIN Photodiode SPV3313 Sumitomo = 0,9 mA/mW Idark = 1nA fmax = 2GHz Selected devices after market survey Direct optical modulation and detection: simpler, cheaper and high performances up to some GHz. TX-O features: Resistive matching APD circuit through the integrated monitor photodiode Slow power-on circuit RX-O features: Direct detection by PIN photodiode Passive optical receiver (no transimpedance amplifier) First custom prototype under evaluation: prliminary results! Double power Supply =+/- 5.8V Amplified link: transmipedence amplifier in the RX-O IIP3>+32dBm IIP3>+20dBm Ripple, induced by TX-O, detected on the transit of CAS-A with a single BEST-1 RX! Interferometer 1-4 Sideral time (sec) Complex correlatio n fringes, about 1 hour acquisitio n, CAS-A source Quasi perfect match between simulated and measured fringes (no ripple is reconisable) Still to investigate the effect on a beamformer Analisys of the ripple impact on real observations Lab. ripple test with an automatic measurement system

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Analogue optical links experiences in the framework of the SKA/BEST activities. Federico Perini. INAF-IRA (I). Motivation: Necessity to bring the signal from the BEST Front End, on the antenna focal lines, to the central processing room. - PowerPoint PPT Presentation

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Page 1: E/O and O/E devices, the collaboration with the industry:

E/O and O/E devices, the collaboration with the industry:E/O and O/E devices, the collaboration with the industry:

E/O and O/E devices, the IRA link:E/O and O/E devices, the IRA link:

Optical connectors:Optical connectors:Optical fibre cable:Optical fibre cable:

Analogue optical links experiences in the framework of the SKA/BEST activities

Federico Perini

INAF-IRA (I)

Custom product: optimised specs (<1GHz) and mechanical RX housing.

TXRX

Power Supply, single positive = (12-15)Volt@75mA Passive optical receiver

APC (Angle Polished Connector)

has RL>70dB → increases the

performance of the RoF link (Dynamic

and NF)

Motivation:

Necessity to bring the signal from the BEST Front End, on the antenna focal lines, to the central processing room.

Which solution: Coax or Optical cables? Analogue or Digital links?

Cost and Reliability prediction analysis of the whole receiver chain indicated the analogue optical link as the best solution, so:

Which kind of fibre?

Which kind of optical connectors?

What E/O and O/E devices?

Motivation:

Necessity to bring the signal from the BEST Front End, on the antenna focal lines, to the central processing room.

Which solution: Coax or Optical cables? Analogue or Digital links?

Cost and Reliability prediction analysis of the whole receiver chain indicated the analogue optical link as the best solution, so:

Which kind of fibre?

Which kind of optical connectors?

What E/O and O/E devices?

Monomode loose fibre cable are the best in term of insertion

loss and phase stability vs temperature and bending

DIN best on moving antennas

SC: best for fixed indoor applications with high integration

SC could be the best compromise

Laser DFB 1310nm MQWSPV4260 Sumitomo

RIN = -155dB/Hz= 0,2 mW/mA

Ith = 8mA

PIN PhotodiodeSPV3313 Sumitomo

= 0,9 mA/mWIdark = 1nA

fmax = 2GHz

Selected devices after market survey

Direct optical modulation and detection: simpler, cheaper and high performances up to some GHz.

TX-O features:

Resistive matching APD circuit through the integrated monitor photodiode Slow power-on circuit

RX-O features:

Direct detection by PIN photodiode

Passive optical receiver(no transimpedance amplifier)

First custom prototype under evaluation: prliminary results!

Double power Supply =+/- 5.8V

Amplified link: transmipedence amplifier in the RX-O

IIP3>+32dBm

IIP3>+20dBm

Ripple, induced by TX-O,

detected on the transit of CAS-A

with a single BEST-1 RX!

Interferometer 1-4

Sideral time (sec)

Complex correlation

fringes, about 1 hour

acquisition, CAS-A source

Quasi perfect match between simulated and

measured fringes (no ripple is

reconisable)

Still to investigate the

effect on a beamformer

Analisys of the ripple impact on

real observations

Lab. ripple test with an automatic

measurement system