technology perspective and results with mhemts

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JGBdV wide band low noise receiver Technology Perspective and Technology Perspective and results with mHEMTs results with mHEMTs Jan Geralt Bij de Vaate ASTRON

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Technology Perspective and results with mHEMTs. Jan Geralt Bij de Vaate ASTRON. Specification R Schillizi et. al. Sept. ‘07. T instrument =40K (excluding sky noise), goal 30K BW70MHz – 1.0 GHz (two systems) Survey speed ~1/T 2 Sensitivity~1/T. Costing. - PowerPoint PPT Presentation

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Page 1: Technology Perspective and results with mHEMTs

JGBdVwide band low noise receiver

Technology Perspective and Technology Perspective and results with mHEMTsresults with mHEMTs

Jan Geralt Bij de Vaate

ASTRON

Page 2: Technology Perspective and results with mHEMTs

JGBdVwide band low noise receiver SKADS Workshop 2007

SpecificationSpecificationR Schillizi et. al. Sept. ‘07R Schillizi et. al. Sept. ‘07

• Tinstrument= 40K (excluding sky noise), goal 30K

• BW 70MHz – 1.0 GHz (two systems)

• Survey speed ~1/T2

• Sensitivity ~1/T

Page 3: Technology Perspective and results with mHEMTs

JGBdVwide band low noise receiver SKADS Workshop 2007

CostingCosting

• A 9 million element system with a total system cost of 250M € can spend:– 1,5 € per LNA per Kelvin improvement (Survey)

– Or 8,5 € for 5 Kelvin improvement, again for Surveys

• Given a bare die costs of:– 0,5 € for Silicon technologies (only 500 12 inch wafers)

– 2 € for GaAs technologies (2000 6 inch wafers)

• Low cost technologies cannot compromise on noise!

Page 4: Technology Perspective and results with mHEMTs

JGBdVwide band low noise receiver SKADS Workshop 2007

TechnologyTechnology

• GaAs PsHEMT / mHEMT

• SiGe BJT

• with b0 =100: FMIN~30K

• CMOS

• In principle similar to GaAs

sgmT

MIN rrgf

fF 1

20

22

20

2

0

)1)((2

1f

fn

f

frr

V

I

f

fnF TT

BET

C

TMIN

211 cf

fF

TMIN

Amplifier Noise Figure Trends @1.4 GHz Tamb=290K

0

10

20

30

40

50

60

70

2000 2002 2004 2006 2008 2010 2012

year

No

ise

Tem

per

atu

re

III/V: GaAs or InP

SiGe

CMOS

Page 5: Technology Perspective and results with mHEMTs

JGBdVwide band low noise receiver SKADS Workshop 2007

PsHEMTPsHEMT

• 0.2um technology

• OMMIC differential LNA– 2109

– ASTRON design

Page 6: Technology Perspective and results with mHEMTs

JGBdVwide band low noise receiver SKADS Workshop 2007

InPInP

• Differential LNA

• NGST

Page 7: Technology Perspective and results with mHEMTs

JGBdVwide band low noise receiver SKADS Workshop 2007

mHEMTmHEMT

• 70nm OMMIC technology – 250GHz fT

– Differential design

– Optional on-chip biasing

Page 8: Technology Perspective and results with mHEMTs

JGBdVwide band low noise receiver SKADS Workshop 2007

mHEMTmHEMT

• 70nm OMMIC technology – 250GHz fT

– Differential design

– Optional on-chip biasing

Page 9: Technology Perspective and results with mHEMTs

JGBdVwide band low noise receiver SKADS Workshop 2007

mHEMTmHEMTATNF01_40LNA_05A, Russel GoughATNF01_40LNA_05A, Russel Gough

• 70nm OMMIC technology

• Designed for 30-50 GHz band

• 4-stage low-noise amplifier

• Transistors: 6-fingers, 90um gate width

• Bias: – Vds = 1.0 V

– Id = 13 mA

Page 10: Technology Perspective and results with mHEMTs

JGBdVwide band low noise receiver SKADS Workshop 2007

ATNF01_40LNA_05AATNF01_40LNA_05A

• 10 circuits were delivered – sample of 4 was measured

• 1 circuit was unstable (|S11|>1)

• The performance of remaining 3 circuits was similar

• Measured gain is greater than modelled

• Input and output match is poorer than expected

Page 11: Technology Perspective and results with mHEMTs

JGBdVwide band low noise receiver SKADS Workshop 2007

SiGeSiGe

• IBM technology– 8HP (0.13µm) : sub 0.5dB noise figure possible

• 0.25dB for 9HP??

– (relative) high Rn

– Good power match possible

– Limited cooling boosts current gain β:

Weinreb 2005

Page 12: Technology Perspective and results with mHEMTs

JGBdVwide band low noise receiver SKADS Workshop 2007

Page 13: Technology Perspective and results with mHEMTs

JGBdVwide band low noise receiver SKADS Workshop 2007

• SKA / LOFAR workshop!(or focussed session)

vaate@astron

Page 14: Technology Perspective and results with mHEMTs

JGBdVwide band low noise receiver SKADS Workshop 2007

ConclusionConclusion

• SKA specifications for AA within reach it seems but…– T coupling (<5) (active reflection coefficient)

– T spill-over, ground noise (<5)

– T antenna losses (<5)

• Technology choice will be based on performance

• Good case for III/V, but also CMOS