photonic beamforming network for multibeam satellite-on
TRANSCRIPT
Photonic beamforming
network for multibeam
satellite-on-board phased-
array antennas
M. A. Piqueras, F. Cuesta-Soto, P. Villalba, A. Martí, A.
Hakansson, J. Perdigués, G. Caille
ICSO Conference
October 14-17th, 2008 - Toulouse
• Beam Handling/Processing
• Optical Beamforming
• Proposed Architecture
• Implementation
• Test and Results
• Technology Comparison
• Further Developments
• Conclusions
PRESENTATION OUTLINE
BEAM HANDLING/PROCESSING
Broadband Telecom Satellites
BEAM HANDLING/PROCESSING
State-of-the-art
(Europe) French STENTOR
mission
- 48 SSPAs
- 3 beams (Ku-band)
(US) SPACEWAY (Ka-band)
- 3000 SSPAs
- 24 beams (Ku-band)
DirecTV's Spaceway F1 satellite undergoes final
preparations for its launch aboard a Zenit-3SL
vehicle. (Boeing photo)
• Problem to be addressedFUTURE SCENARIOS
Coverage of a wide area by multiple fixed narrow beams
Direct Radiating Array (DRA) scheme
Hundred of antenna elements to be feed
Multibeam capability
„‟Europe + Maghreb‟‟ coverage:
44 spots, =0.8°
Antenna = 256-elements DRA
BEAM HANDLING/PROCESSING
• Problem to be addressedHigh complexity
High mass and volume of the classical RF implementations
Heavy impact in the digital beamforming approach.
High mass of the feeding cables (hundred of antennas)
Crosstalk and EMI issuesIn the vertical plane, regular beams
arrangement is provided. by a 2nd set of 6
16 Butler matrices, for each of the 48
input ports to feed all R.E
2/ 16 vertical
616 matrices
Optional 18 fast switches
for beam-hopping mode 6
beams independently on
each 8-spot row (would be
implemented on the same
board than input-matrices
1/ 6 horizontal
816 matrices
1+2: 6+16
(6 or 816)
matrices are
necessary
16x16=256
ports to R.E.
16 outputs
per matrix
3dB / 90°
couplers
*2D: in 2
dimensions
Analogue ‘classical’ BFN
(1slide per beam)
Spot-beams
= S inputs
Radiating
Array
(N R.E.)
Nth
beam
j1
-
j2
jm
beam
j1
-
j2
jm
N SSPAN Filters
N CombinersS ->1
S dividers1->N
Fixed or controllable phase shifters
1stb
eam
j1
-
j2
jm
2n
d b
ea
m
BEAM HANDLING/PROCESSING
• Solution proposedTo use photonic technology for the Beamforming Network
Size reduction
High integration of several functionalities in a single chip
High precision in the phase shifting (SOI technology)
Mass reduction: using optical fiber for the antenna feeding
Huge electrical bandwidth (typically > 40 GHz).
EMI Free technology
Excellent crosstalk
Scalability with low size/mass
OPTICAL BEAMFORMING
Optical Beam Forming
The ESA is assessing the benefits of using optical beam forming networks on Telecom
and EO satellites for steerable pencil or spotlight beams, or for adjusting broadband
multimedia beams.
Different scenarios:
-Wide bandwidth requirements: True Time Delay (TTD) architectures
-Narrow bandwidth: no need of TTD
Broadband Telecom Satellites
•Ka band (30GHz) multimedia satellites
•Large number of beams (200)
•Small Steering Angles (few degrees)
•LC SLMs used for Amplitude and Phase control
(true time delay not required)
•Integrated photonics implementing beamforming
networks as Butler Matrix (true time delay not
required)
Errico Armandillo (ESA), Space Optoelectronic Day, Cork 7 April 2006
OPTICAL BEAMFORMING
E/O
E/O
E/O
… OBM
Subsystem
O/E TIA
O/E TIA
…O/E TIA
SSPA Antenna Element
SSPA Antenna Element
SSPA Antenna Element
Up-conv
Up-conv
Up-conv
Optical Beamforming
Network
D1
D2
D44Ort
hogonal B
eam
s
Array Antenna
Optical Fiber
Feeding of antennas
PROPOSED ARCHITECTURE
Butler Matrix: Principle of Operation
Orthogonal beams
Passive structure: couplers and phase shifters
Scalable solution (FFT structure)
Very well known solution
PROPOSED ARCHITECTURE
OPTICAL Butler Matrix: Heterodine Generation
fRF
A)
f0 + fRF
B)
DC
Electrical
Spectrum
Optical
Spectrum
f0
E1(t)
E2(t)
C) Optical
Spectrum
f0
E1(t)
f0 + fRF
D) Optical
Spectrum
f0
E2(t)
E1) Optical
Spectrum
f0
E1(t)·ej1
E1) Optical
Spectrum
f0
E1(t)·ej2
S(t)
f0 + fRF
F1) Optical
Spectrum
f0
E2(t) ·ej0
E1(t)·ej1
f0 + fRF
F2) Optical
Spectrum
f0
E2(t) ·ej0
E1(t)·ej2
Out1 = S(t)·ej(1-0)
Out2 = S(t)·ej(2-0)
fRF
A)
f0 + fRF
B)
DC
Electrical
Spectrum
Optical
Spectrum
f0
E1(t)
E2(t)
C) Optical
Spectrum
f0
E1(t)
f0 + fRF
D) Optical
Spectrum
f0
E2(t)
E1) Optical
Spectrum
f0
E1(t)·ej1
E1) Optical
Spectrum
f0
E1(t)·ej2
S(t)
f0 + fRF
F1) Optical
Spectrum
f0
E2(t) ·ej0
E1(t)·ej1
f0 + fRF
F2) Optical
Spectrum
f0
E2(t) ·ej0
E1(t)·ej2
Out1 = S(t)·ej(1-0)
Out2 = S(t)·ej(2-0)
E/O
S(t)Demux
1:2
Optical
Butler
Matrix2x2
+
+
1:2
O/E
O/E
A) B)
C)
D)
E1)
E2)
F1)
F2)
Out1
Out2
OBMS
…
PROPOSED ARCHITECTURE
CMOS compatible tech.
Thin silicon (Si) layer on top of an Oxide (SiO2) cladding
Si thickness = 200 nm
SiO2 layer = 3000 nm
Waveguide width = 500 nm
Mode profile highly confined
Effective refraction index @ 1550 nm = 2,36
500 nm
SOI TECHNOLOGY
IMPLEMENTATION
10 cm
0.003 cm
18 GHz 8x8 Butler MatrixTechnical Research and Manufacturing, Inc.
Optica Butler Matrix SOI CHIP
SEM PHOTOGRAPH
MICROSCOPE PHOTOGRAPH
TESTS AND RESULTS
L= 0.5 mm
Lensed
fiber
Ridge waveguide
Objective
Linear Taper
Photonic Wire
Photonic Device
(a)
IR camera
Input
polariser
Lens
Power
Meter
Polarised Lens
Laser signal
Aperture
(x,y,z)-axis traslation stages
Lensed Fiber
Sample
Objective
Microscope
Reference Waveguide (3m wide)
MEASUREMENTS AT CHIP LEVEL
TESTS AND RESULTS
Parameter Specification Obtained
Standard deviation of
phase errors < 10/√2 < 5 - 10º
Standard deviation of
amplitude errorsa < 0.5 dB a < 2 dB
Phase performance in line with the specifications
Amplitude performance worse than specifications
Mainly due to the coupling method (introduce extra attenuations)
Amplitude equalization is expected in future devices.
Chip post-proccesing
Due to the
in-chip test method
TESTS AND RESULTS
• Targeted for high complexity beamforming
networks for array antennas (DRA)
BFN optionEstimated
mass
Estimated
volumeDC consump.
EMI
FREE
Upgradeability in
Nº of antenna
elements
„Pure-RF‟ with
Butler Matrixes100% 100% 100% NO Low/medium
„opto-wave‟ 70% <1% 200% YES High
Comments
Cable vs. Fiber
mass shaving
has not been
considered
Greater for
large
antennas
Including added
amplifiers to
compensate
converion losses
Infinite
isolation
Easy for large number
of antenna elements (in
the Opto-uwave)
Example: 44 beams. 256 antenna elements
TECHNOLOGY COMPARISON
• Improvement of the phase/amplitude
performance
• Extend higher number of I/O ports
• Implementation of the whole heterodine
structure (RF performance)
• Whole system packaged (including the
fiber coupling)
FURTHER DEVELOPMENTS
SBE
SBE
SBE
● ● ● ●
● ● ● ●● ● ● ●
SBE
SBE
SBE
SBE
● ● ● ●
SBE: Side-Band Extraction
Input Ports (#1 to #8)
Output Ports (#1 to #16)
•Basic Unit (BU) for the OBFN design
•Based on 8x8 Butler Matrices and a proprietary
2N beam multiplication solution: simpler than
the truncated 16x16 alternative (especially much
fewer line crossing‟s)
•Heterodine distribution included in the basic
unit:
•Result in a 8x16 Butler matrix “RF-to-RF”
•Different Basic Units can be
interconnected with optical fiber
•Do not requires the integration of optical
switches inside the block.
Optimised OPTICAL Butler Matrix (OBM)
FURTHER DEVELOPMENTS
Conclusions
• Successful fabrication of an SOI integrated 8x8
Optical Butler Matrix
• The performance in terms of phase/amplitude
obtained is comparable with the traditional
electrical solution
• Low mass and size
• Remote feeding by optical fibre: weigh reduction
• EMI free technology
• Promising alternative for the implementation of
Beamforming systems.
CONCLUSIONS
Conclusions
THANK YOU FOR YOUR ATTENTION