Coherent Receiver Design for Optical Inter-satellite Links · Semjon Schaefer, Future Photonics...
Transcript of Coherent Receiver Design for Optical Inter-satellite Links · Semjon Schaefer, Future Photonics...
Coherent Receiver Design for Optical Inter-satellite Links
Semjon Schaefer
Future Photonics 17. September 2015
Hamburg
Lehrstuhl für Nachrichten- und Übertragungstechnik Technische Fakultät
Christian-Albrechts-Universität zu Kiel
-2- Chair for Communications
Lehrstuhl für Nachrichten- und Übertragungstechnik
Semjon Schaefer, Future Photonics 2015, 17.09.2015
Motivation
Advantages compared to RF: Main challenges:
Data rates of several Gb/s Lower power consumption Lower weight lower costs Data security
Pointing, Acquisition, Tracking system (PAT) For line-of-sight connection (LOS)
No transmission through atmosphere/clouds
Optical Inter-satellite Link
-3- Chair for Communications
Lehrstuhl für Nachrichten- und Übertragungstechnik
Semjon Schaefer, Future Photonics 2015, 17.09.2015
Content
1. Optical Inter-satellite Links
2. Homodyne Detection with Optical Phase-Locked Loop
3. Intradyne Detection with Digital Signal Processing
4. Conclusions
-4- Chair for Communications
Lehrstuhl für Nachrichten- und Übertragungstechnik
Semjon Schaefer, Future Photonics 2015, 17.09.2015
Optical Intersatellite Link (OISL)
Current RF Scenario: OISL Scenario:
LEO GEO GS: High data rate (LEO GEO) Long time window (GEO GS)
LEO GS: Low data rate Short time window
LEO: Low-Earth Orbit GEO: Geostationary Orbit
-5- Chair for Communications
Lehrstuhl für Nachrichten- und Übertragungstechnik
Semjon Schaefer, Future Photonics 2015, 17.09.2015
Caused by the relative velocity between the satellites
Maximum frequency offset of approx. 7 GHz Coarse compensation by using satellite trajectory data (frequency sweeping) Fine compensation by optical PLL (homodyne) or DSP (intradyne)
Residual Doppler shift, natural frequency drift and phase noise
Doppler Frequency Shift
2
21
1 cos
vc
Tx vc
Rxf fα
−=
−
: Transmitted frequency: Received frequency
: Speed of light in vacuum: Relative velocity
Tx
Rx
ffcv
±
-6- Chair for Communications
Lehrstuhl für Nachrichten- und Übertragungstechnik
Semjon Schaefer, Future Photonics 2015, 17.09.2015
Content
1. Optical Inter-satellite Links
2. Homodyne Detection with Optical Phase-Locked Loop
3. Intradyne Detection with Digital Signal Processing
4. Conclusions
-7- Chair for Communications
Lehrstuhl für Nachrichten- und Übertragungstechnik
Semjon Schaefer, Future Photonics 2015, 17.09.2015
OISL Transmission System with Homodyne Detection
Laser Communication Terminal (LCT) Setup: Typical Setup: Solid-state laser at 1064 nm Tx-power of up to 5 W BPSK transmission of up to 1.8 Gb/s Coherent homodyne detection
Carrier recovery based on OPLL techniques
PM: Phase modulator YDFA: Ytterbium-doped fiber amplifier OPLL: Optical phase-locked loop LO: Local oscillator
-8- Chair for Communications
Lehrstuhl für Nachrichten- und Übertragungstechnik
Semjon Schaefer, Future Photonics 2015, 17.09.2015
Carrier Recovery
Optical phase-locked loop for BPSK transmission based on Costas loop
( )( )
1 2
1 2
( ) ~ cos ( ) ( ) ( )
( ) ~ sin ( ) ( ) ( )I M
Q M
U t t t t
U t t t t
φ φ φ
φ φ φ
− +
− + [ ]( )1 2
( ) ( )· ( )
~ sin 2 ( ) ( )I Qt U t U t
t t
ε
φ φ
=
−
AGC: Automatic gain control TIA: Transimpedance amplifier LO: Local oscillator
{ }( ) 0,M tφ π∈
Demodulated data signal after coherent detection:
BPSK modulation
Phase error
-9- Chair for Communications
Lehrstuhl für Nachrichten- und Übertragungstechnik
Semjon Schaefer, Future Photonics 2015, 17.09.2015
Frequency Acquisition
Example: Residual frequency offset of 5 MHz (after coarse Doppler compensation) Error Signal Frequency Error
( )tε
-10- Chair for Communications
Lehrstuhl für Nachrichten- und Übertragungstechnik
Semjon Schaefer, Future Photonics 2015, 17.09.2015
QPSK Extension for Future Systems
Higher data rate e.g. by higher order modulation formats Modifications in transmitter structure (e.g. optical IQ-modulator) Modifications in receiver/OPLL structure (e.g. phase discriminator)
OPLL complexity increases with modulation order! Intradyne detection with DSP as alternative
-11- Chair for Communications
Lehrstuhl für Nachrichten- und Übertragungstechnik
Semjon Schaefer, Future Photonics 2015, 17.09.2015
BER Performance: BPSK vs. QPSK
Low receive power due to high free-space loss High receiver sensitivity required
Tx Power 32 dBm Baud Rate 1 Gbaud OPLL Bandwidth 3.5 MHz LO Power 11 dBm PD Bandwidth 4 GHz Linewidth (Tx/LO) 10 kHz
TxP
BdD
LBLOP
eB
Simulation Setup:
-12- Chair for Communications
Lehrstuhl für Nachrichten- und Übertragungstechnik
Semjon Schaefer, Future Photonics 2015, 17.09.2015
Content
1. Optical Inter-satellite Links
2. Homodyne Detection with Optical Phase-Locked Loop
3. Intradyne Detection with Digital Signal Processing
4. Conclusions
-13- Chair for Communications
Lehrstuhl für Nachrichten- und Übertragungstechnik
Semjon Schaefer, Future Photonics 2015, 17.09.2015
Intradyne Detection with DSP
No changes at transmitter compared to OPLL setup Free-running LO for intradyne detection Combination of coarse and fine compensation
ADC: Analog-digital-converter FO: Frequency offset PN: Phase noise LO: Local oscillator
Coarse Fine
-14- Chair for Communications
Lehrstuhl für Nachrichten- und Übertragungstechnik
Semjon Schaefer, Future Photonics 2015, 17.09.2015
Coarse Compensation: Phase Differential Algorithm
1) Complex signal at coherent receiver output 2) Estimate the phase difference 3) Data elimination and phase averaging (BPSK M=2) 4) Final estimated frequency offset
( ) ( ) ( )X t I t jQ t 0ˆ M nj k k kRxX k A e n k
0 01 1*
1 1
ˆ1ˆ
M M
M M
j k k j k k
j k k k k
X k X k Ae e
Ae
1* ˆ1M jM k kX k X k Ae *
1
1 arg 1L M
k
X k X kM
2 s
fT
max1 1
2 2s s
fT M MT
Rx
: Symbol duration :Modulation order
:Data modulation:FO phase signal
A :Amplitude of received signal:Phase noise:Additive noise
S
M
n
TM
n
-15- Chair for Communications
Lehrstuhl für Nachrichten- und Übertragungstechnik
Semjon Schaefer, Future Photonics 2015, 17.09.2015
Coarse Compensation: Phase Differential Algorithm
Setup: • BPSK •
Results (with shot/phase noise): Limited working range as expected Frequency error influenced by SNR and L Remaining error in the lower MHz range
1 1GHzss
fT
= =
2M =
max1 0.25GHz
2 s
fMT
Without noise
-16- Chair for Communications
Lehrstuhl für Nachrichten- und Übertragungstechnik
Semjon Schaefer, Future Photonics 2015, 17.09.2015
Fine Compensation: Phase noise compensation
Based on Viterbi & Viterbi-method Length N of averaging influences compensation accuracy
-17- Chair for Communications
Lehrstuhl für Nachrichten- und Übertragungstechnik
Semjon Schaefer, Future Photonics 2015, 17.09.2015
Fine Compensation: Phase noise compensation
BER simulations depending on the frequency offset, N and SNR
Increasing N Working range decreases Increasing SNR Shot noise influence decreases Compensation of a remaining frequency error of 1 MHz possible Trade-off between DSP speed and compensation accuracy
SNR=18dB N=32
-18- Chair for Communications
Lehrstuhl für Nachrichten- und Übertragungstechnik
Semjon Schaefer, Future Photonics 2015, 17.09.2015
Conclusions
OISL as an attractive alternative to current RF communications Higher data rates, lower power consumption High free-space loss requires high receiver sensitivity
OPLL based carrier recovery for homodyne BPSK detection
OPLL-QPSK scheme for future OISL transmission systems
Hardware complexity increases with modulation order
Intradyne detection with digital frequency offset compensation as alternative
Shift complexity to the digital domain
-19- Chair for Communications
Lehrstuhl für Nachrichten- und Übertragungstechnik
Semjon Schaefer, Future Photonics 2015, 17.09.2015
Acknowledgment
For supporting part of this work!
-20- Chair for Communications
Lehrstuhl für Nachrichten- und Übertragungstechnik
Semjon Schaefer, Future Photonics 2015, 17.09.2015
Thank you!