ska aa-low: lpd antenna (skala) & path towards aavs0 at cambridge eloy de lera acedo university...
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![Page 1: SKA AA-low: LPD antenna (SKALA) & path towards AAVS0 at Cambridge Eloy de Lera Acedo University of Cambridge 1 AAVP 2011: Taking the AA programme into](https://reader035.vdocuments.net/reader035/viewer/2022062322/56649d625503460f94a44df9/html5/thumbnails/1.jpg)
SKA AA-low: LPD antenna (SKALA) &
path towards AAVS0 at Cambridge
Eloy de Lera AcedoUniversity of Cambridge
1AAVP 2011:
Taking the AA programme into SKA Pre-Construction12-16 December, 2011 - ASTRON, Dwingeloo
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Overview• Introduction• Current status of SKALA (LPD antenna)• Low Noise Amplifier for SKALA• SKALA tests and AAVS0 (16-element array)• Important numbers• Summary and conclusions
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IntroductionParameter Specification Remarks
Low frequency MHz 70 Lowest frequency expected for the EoR
Nyquist frequency MHz 100 Frequency with element spacing is λ/2, defines max A eff
High frequency MHz 450 Freq where sky noise is low, overlaps with AA-hi and/or dishes
Frequency coverage contiguous There are no gaps between low and high frequency
Bandwidth, max MHz 380 Individual beams can operate over the full frequency range
Polarisations 2 Orthogonal
Station diameter m 180 Determined from SKA2. Uses 250 arrays for expected SKA2 sensitivity
Geometric area m2 ~25,000
No. of element types 1 A single wide-band element type e.g. bow-tie or conical spiral
No. of elements ~10k Each element is low gain, dual polarisation
Scan angle range deg ±45 Will operate at larger scan angles, but sensitivity not defined
Sensitivity @ 100 MHz m2/K 17Single array, sensitivity varies over the band.
Assumes Tsky= 1000K, 70% for appodisation.
Frequency channel kHz 250Assumes 2048 channels splitting the full sample rate, further channelization will be required at correlator
Output data rate Tb/s 16Defines the survey performance of the array.
Can be used flexibly for frequency, bandwidth and number of beams
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Evolution: from BLU to SKALA
BLU
ImpedanceDual polarisationSky coverageCost
Toothed log periodic
ImpedanceDual polarisationSky coverageCost
SKALA
ImpedanceDual polarisationSky coverageCost
w-SKALA
ImpedanceDual polarisationSky coverageCost
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SKALA: SKA Log-periodic Antenna
1.6 m
1.3 m
* GND mesh is 1.5 x 1.5 m.
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Current status of SKALA
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Mass production of SKALA and LNA
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Mass production of SKALA and LNA
• Some numbers:– Cost of antennas for AAVS1 is around 150€/element.– Cost of antenna for AAVS2 is targeted at 75€/element (this is for the 2
polarisations and includes the electronics).– Weight of each arm would be 1.56 kg if made of steel wire.
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First prototype
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Performance
0.1 0.15 0.2 0.25 0.3 0.35 0.4 0.45-20
-18
-16
-14
-12
-10
-8
-6
-4
-2
0
Freq /GHz
S11
/dB
0.08 0.1 0.12 0.14 0.16 0.18 0.2-20
-18
-16
-14
-12
-10
-8
-6
-4
-2
0
Freq /GHz
S11
/dB
SimulationMeasurement
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Low Noise Amplifier for SKALA• Frequency range 70 to 450MHz• Gain > 20dB• Gain flatness, as flat as possible consistent with meeting
other spec. parameters• Noise temperature < 30K at 450MHz• P1dB, high enough to allow astronomical observations to be
made at Lords Bridge• Power consumption < 100mW• Unconditionally stable at both input and output ports• Differential source (antenna), single-ended load • High Level of Common Mode Signal Rejection
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Concept
Diferrential input
Static discharge path
Balun Coaxial output
LNA1
LNA2
DC block
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Dual Matched Low Noise RF FETs Required
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SchematicAVAGO MGA-16516
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Board layout
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Picture
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LNA & antenna performance0 1.0
1.0
-1.0
10.0
1 0 . 0
-10.0
5.0
5 .0
-5.0
2.0
2.0
-2.0
3.0
3 .0
-3.0
4.0
4 .0
-4.0
0.2
0.2
- 0. 2
0.4
0.4
- 0. 4
0.6
0.6
-0.6
0.8
0.8
-0.8
A n te n n a S 1 1 a n d L N A N o ise C ir c le sS w p Ma x
4 5 0 MH z
S w p Min
7 0 MH z
p8
p7
p6
p5
p4
p3
p2p1
4 5 0 M H zr 1 .5 8 1 3 5x - 0 .0 3 2 4 0 5
7 0 M H zr 0 .4 6 2 5 9 1x - 0 .2 3 6 8 5 4
D B (N FC IR (1 ,0 .1 ))L N A _ M G A 1 65 1 6_ a ll_ in _ on e .$ FS W P 1
S (1 ,1 )S K A L A _ C C L _5 _ s im p le _1 p o lL o ad e d_ W ing _ d iff_ m e ta lP o le G o od _ no n M eta l.$FP R J
p 1 : F R E Q = 7 0 M H zN F = 0 .5 3 9 5 3 d B
p 2 : F R E Q = 7 0 M H zN F = 0 .6 3 9 5 3 d B
p 3 : F R E Q = 1 3 0 M H zN F = 0 .4 1 3 5 5 d B
p 4 : F R E Q = 1 3 0 M H zN F = 0 .5 1 3 5 5 d B
p 5 : F R E Q = 3 0 0 M H zN F = 0 .4 1 0 0 5 d B
p 6 : F R E Q = 3 0 0 M H zN F = 0 .5 1 0 0 5 d B
p 7 : F R E Q = 4 5 0 M H zN F = 0 .4 3 0 0 3 d B
p 8 : F R E Q = 4 5 0 M H zN F = 0 .5 3 0 0 3 d B
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70 170 270 370 450Frequency (MHz)
SK A Lo LNA Transducer Gain and Noise Figure in dB
0
10
20
30
40
50
dB
70 MHz44.1 dB
449.3 MHz0.4301 dB
448.3 MHz40.94 dB
70 MHz0.7654 dB
DB(NF())LNA_MGA16516_all_in_one.$FPRJ
DB(GT())LNA_MGA16516_all_in_one.$FPRJ
Operating with Cambridge Log Periodic
LNA+antenna simulated performance (includes a 20dB gain second stage on chip)
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LNA+antenna simulated performance (includes a 20dB gain second stage on chip)
70 170 270 370 450Frequency (MHz)
Noise Figure of SK A Lo LNA operating with Cambridge Log Periodic
0.4
0.5
0.6
0.7
0.8
No
ise
Fig
ure
dB
70 MHz0.7654 dB
103.3 MHz0.4528 dB
255.2 MHz0.4608 dB
449.5 MHz0.4301 dB
DB(NF())LNA_M GA16516_all_in_one.$FPRJ
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Simulated A/T for SKA1 (with log-periodic antenna)
• η (radiation efficiency) = 90%• D (directivity)• Tsky (sky noise temperature) following Tsky = 1.691*(freq[GHz].^-2.751) + 4.875 K• Tamb (ambient temperature) = 295 K• Trec (receiver noise temperature) -> Assuming ideal amplifier with:
• Zopt (optimum noise impedance) = 100 Ω• Rn (noise resistor) = 10 Ω• Fmin (minimum noise figure) = 0.3 dB -> 21 K
- A/T shown is A/T of 1 antenna x N (number of antennas in a 180 m station with elements spaced 1.5 m apart) x 50 stations.
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* Peak is at 2452 m^2/K
200
200
400600
8001000
12001400
16001800
2000
2200
2400
30o
45o
60o
A/T for polarization 1 [m 2/K] for SKA1 (based on SKALA) @ 170 MHz
sin()*cos()
sin
()*
sin
()
-1 -0.5 0 0.5 1-1
-0.8
-0.6
-0.4
-0.2
0
0.2
0.4
0.6
0.8
1
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* Peak is at 2452 m^2/K
200
2002
00
40060080010001200140016001800
2000
2200
2400
30o
45o
60o
A/T for polarization 2 [m 2/K] for SKA1 (based on SKALA) @ 170 MHz
sin()*cos()
sin
()*
sin
()
-1 -0.5 0 0.5 1-1
-0.8
-0.6
-0.4
-0.2
0
0.2
0.4
0.6
0.8
1
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* Peak is at 3468 m^2/K
5001000
1500
2000
2500
3000
3400
30o
45o
60o
A/T Stokes I [m2/K] for SKA1 (based on SKALA) @ 170 MHz
sin()*cos()
sin
()*
sin
()
-1 -0.5 0 0.5 1-1
-0.8
-0.6
-0.4
-0.2
0
0.2
0.4
0.6
0.8
1
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0.05 0.1 0.15 0.2 0.25 0.3 0.35 0.4 0.450
500
1000
1500
2000
2500
3000
3500
4000
A/T Stokes I [m2/K] for SKA1 (based on SKALA)
Freq /GHz
A/T
/m
2 /K
Zenith
30o
45o
60o
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Effect of Soil/GND – (Soil B – 5% humidity)
Even a bigger pitch may be possible!
0.1 0.15 0.2 0.25 0.3 0.35 0.4 0.450
20
40
60
80
100
120
Freq /GHz
Tg
nd /K
10 cm pitch5 cm pitchNo ground
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X-pol
0.1 0.15 0.2 0.25 0.3 0.35 0.4 0.45-50
-45
-40
-35
-30
-25
-20
-15
-10
-5
0
Freq /GHz
x-p
ol /
dB
Zenith
22.5 o H-plane
22.5 o E-plane
45 o H-plane
45 o E-plane
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SKALA tests and AAVS0• 16 dual-polarised SKALA elements.• Aim:
– Test realistic SKA AA-low front-end technology in an array environment:
• Effect of cables.• Effect of ground mesh/soil.• Effect of mutual coupling on noise and pattern.
– Challenges:• Measure the pattern in an array environment.
Options:– Use of known field source: NF, FF.– Use data from interferometry experiment.
– Cost:• Estimated total cost is 5-10 K€ depending on
tools and equipment needed for the tests.
e/o
e/o
e/o
Analogue
ADC: 1GS/s
Data
Control
Sync.
50- 100m all optical
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Lord’s Bridge Observatory
SKALA-AAVS0
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Upcoming tests:• December 2011:
– Impedance test with “dummy” board.
• January 2011:– Single element pattern measurement in outdoor test range, Perth?– Single element pattern measurement in outdoor test range, UK.– Noise matching with integrated LNA in reverberation chamber, UK.– Impedance tests on AAVS0.
• February-March 2011: (with Roach back-end)– Noise tests on AAVS0: pointing the array to hot and cold patches of the sky.– Pattern tests on AAVS0: (compare with analytical/EM models - UCL)
• Interferometry experiment: full correlation/correlation with high gain antenna• Known source: Near field source (no back-end needed), minicopter?
– More tests... Any suggestion? Plug into other back-ends?
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Important numbers• Noise:
– <30 K @ 450 MHz.
• Sky coverage – A/T:– Meets DRM specifications down to +/- 45o at all frequencies.
• Frequency band:– Potential to go down to 50 MHz (lower arm).
• Foot-print: 1x1 m possible (lower arm).• Cost:
– Targeted to 75 € including LNA and ground mesh.
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Single-Dual band• Low-band: high gain element, OK.• High-band: low gain element? Not so easy... Getting down to 30 K
with a low gain antenna in a 3:1 band is not that easy. You will probably need a high gain element anyway and rather large.
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Summary and conclusions• Antenna+LNA pair meets DRM requirements.• In early 2012 noise and pattern tests for AAVS0.• Mass production prototypes are in their way (75€/element).
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Thank you! Any questions?
SKALA1(Cambridge)
SKALA2(ICRAR)
SKALA3(Cambridge)
SKALA4(ASTRON)
SKALA0miniSKALA
(Cambridge)