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AMICSA 2012 Evaluation of AMS 0.35mm CMOS for Space Applications Universidad de Sevilla / IMSE-CNM 1/36 Evaluation of the AMS 0.35 µm CMOS Technology for Use in Space Applications J. Ramos-Martos (1 , A. Arias-Drake (2 , A. Ragel-Morales (1 , J. Ceballos-Cáceres (1 , J. M. Mora-Gutiérrez (1 , B. Piñero-García (2 , M. Muñoz-Díaz (2 , M. A. Lagos-Florido (1 , S. Sordo-Ibáñez (2 , S. Espejo-Meana (1,2 1) Instituto de Microelectrónica de Sevilla - Centro Nacional de Microelectrónica - Consejo Superior de Investigaciones Científicas (IMSE) Avenida Américo Vespucio, s/n; Sevilla, Spain 2) Departamento de Electrónica y Electromagnetismo – Universidad de Sevilla (US) Avenida Américo Vespucio, s/n; Sevilla, Spain

Evaluation of the AMS 0.35 µm CMOS Technology for Use in Space …microelectronics.esa.int/amicsa/2012/pdf/S5_07_Ramos... · 2012. 9. 5. · Ids vs. Vgs – NMOS/M (0-1Mrad) –

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Page 1: Evaluation of the AMS 0.35 µm CMOS Technology for Use in Space …microelectronics.esa.int/amicsa/2012/pdf/S5_07_Ramos... · 2012. 9. 5. · Ids vs. Vgs – NMOS/M (0-1Mrad) –

AMICSA 2012

Evaluation of AMS 0.35mm CMOS for Space Applications

Universidad de Sevilla / IMSE-CNM 1/36

Evaluation of the AMS 0.35 µm CMOS Technology for Use in Space Applications

J. Ramos-Martos(1, A. Arias-Drake(2, A. Ragel-Morales(1, J. Ceballos-Cáceres(1, J. M. Mora-Gutiérrez(1, B. Piñero-García(2, M. Muñoz-Díaz(2, M. A. Lagos-Florido(1, S. Sordo-Ibáñez(2, S. Espejo-Meana(1,2

1)Instituto de Microelectrónica de Sevilla - Centro Nacional de Microelectrónica - Consejo Superior de Investigaciones

Científicas (IMSE) Avenida Américo Vespucio, s/n; Sevilla, Spain

2)Departamento de Electrónica y Electromagnetismo – Universidad de Sevilla (US)

Avenida Américo Vespucio, s/n; Sevilla, Spain

Page 2: Evaluation of the AMS 0.35 µm CMOS Technology for Use in Space …microelectronics.esa.int/amicsa/2012/pdf/S5_07_Ramos... · 2012. 9. 5. · Ids vs. Vgs – NMOS/M (0-1Mrad) –

AMICSA 2012

Evaluation of AMS 0.35mm CMOS for Space Applications

Universidad de Sevilla / IMSE-CNM 2/36

AMS 0.35 µm CMOS for Space Applications

Introduction The Characterization Plan

Low-Temperature Characterization

Equivalent Width for ELTs

TID Characterization

SEE Characterization

Conclusions and Future Work

Page 3: Evaluation of the AMS 0.35 µm CMOS Technology for Use in Space …microelectronics.esa.int/amicsa/2012/pdf/S5_07_Ramos... · 2012. 9. 5. · Ids vs. Vgs – NMOS/M (0-1Mrad) –

AMICSA 2012

Evaluation of AMS 0.35mm CMOS for Space Applications

Universidad de Sevilla / IMSE-CNM 3/36

Introduction Application of IMSE and US Mixed-Signal Design expertise to space

ASICs • Collaboration with Instituto Nacional de Técnica Aeroespacial (INTA)

started in 2008 • Selection of technology from an European foundry (AMS 0.35µm)

– Mature, reliable, long-life (automotive market) – Reduced prototyping and low-volume production cost – Suitable for moderate performance MS designs

• Start from the ground (technology evaluation and characterization)

Design, then try to see what happens….. or See what happens, then design!

Page 4: Evaluation of the AMS 0.35 µm CMOS Technology for Use in Space …microelectronics.esa.int/amicsa/2012/pdf/S5_07_Ramos... · 2012. 9. 5. · Ids vs. Vgs – NMOS/M (0-1Mrad) –

AMICSA 2012

Evaluation of AMS 0.35mm CMOS for Space Applications

Universidad de Sevilla / IMSE-CNM 4/36

Introduction

The Characterization Plan Low-Temperature Characterization

Equivalent Width for ELTs

TID Characterization

SEE Characterization

Conclusions and Future Work

AMS 0.35 µm CMOS for Space Applications

Page 5: Evaluation of the AMS 0.35 µm CMOS Technology for Use in Space …microelectronics.esa.int/amicsa/2012/pdf/S5_07_Ramos... · 2012. 9. 5. · Ids vs. Vgs – NMOS/M (0-1Mrad) –

AMICSA 2012

Evaluation of AMS 0.35mm CMOS for Space Applications

Universidad de Sevilla / IMSE-CNM 5/36

Objectives

Test Chips

Test Hardware

Test Software

Test Facilities

The Characterization Plan

Page 6: Evaluation of the AMS 0.35 µm CMOS Technology for Use in Space …microelectronics.esa.int/amicsa/2012/pdf/S5_07_Ramos... · 2012. 9. 5. · Ids vs. Vgs – NMOS/M (0-1Mrad) –

AMICSA 2012

Evaluation of AMS 0.35mm CMOS for Space Applications

Universidad de Sevilla / IMSE-CNM 6/36

Objectives

Evaluation • At low-temperature (-110ºC) • Radiation (TID, SEE)

Development • Models of Enclosed-Layout Transistors • RHBD Digital Library

Application • Two instrumentation chips for Mars missions • Future use in internal projects and in collaboration with other

interested groups

Page 7: Evaluation of the AMS 0.35 µm CMOS Technology for Use in Space …microelectronics.esa.int/amicsa/2012/pdf/S5_07_Ramos... · 2012. 9. 5. · Ids vs. Vgs – NMOS/M (0-1Mrad) –

AMICSA 2012

Evaluation of AMS 0.35mm CMOS for Space Applications

Universidad de Sevilla / IMSE-CNM 7/36

Test Chips (1)

•Geometry

•Temperature

•TID

•SEUs & SETs

•Latch-Ups

CHIP#1

CHIP#2

CHIP#3

MOS Transistors Bipolar Transistors Resistances Diodes Ring Oscillator Shift Registers Latch-Up Structures

Library Cells Shift Registers Combinational Logic

Page 8: Evaluation of the AMS 0.35 µm CMOS Technology for Use in Space …microelectronics.esa.int/amicsa/2012/pdf/S5_07_Ramos... · 2012. 9. 5. · Ids vs. Vgs – NMOS/M (0-1Mrad) –

AMICSA 2012

Evaluation of AMS 0.35mm CMOS for Space Applications

Universidad de Sevilla / IMSE-CNM 8/36

Test Chips (2) – CHIPS #1 & #2

CHIP#1 with five multiplexed arrays of 4 x

4 CMOS transistors

Page 9: Evaluation of the AMS 0.35 µm CMOS Technology for Use in Space …microelectronics.esa.int/amicsa/2012/pdf/S5_07_Ramos... · 2012. 9. 5. · Ids vs. Vgs – NMOS/M (0-1Mrad) –

AMICSA 2012

Evaluation of AMS 0.35mm CMOS for Space Applications

Universidad de Sevilla / IMSE-CNM 9/36

Test Chips (3) – Muxed Arrays MUX-D connects to DRAIN the drains of all transistors in its column, other columns have its drain open; MUX-S connects to SOURCE the source of all transistors in its column, other columns have its source to BULK; MUX-G connects to GATE the gates of all transistors in its row, other rows have its gate to BULK (GND (NMOS) or to VDD (PMOS)). SOURCE, GATE and DRAIN are connected externally to the measuring equipment.

RADIATE sets all transistors with gate to VDD and all other terminals grounded.

MUX-D

MUX-G

Page 10: Evaluation of the AMS 0.35 µm CMOS Technology for Use in Space …microelectronics.esa.int/amicsa/2012/pdf/S5_07_Ramos... · 2012. 9. 5. · Ids vs. Vgs – NMOS/M (0-1Mrad) –

AMICSA 2012

Evaluation of AMS 0.35mm CMOS for Space Applications

Universidad de Sevilla / IMSE-CNM 10/36

Test Chips (4) – CHIP#3

Dedicated to evaluation of SEU, SET and SEL in standard and RHBD digital cells.

Page 11: Evaluation of the AMS 0.35 µm CMOS Technology for Use in Space …microelectronics.esa.int/amicsa/2012/pdf/S5_07_Ramos... · 2012. 9. 5. · Ids vs. Vgs – NMOS/M (0-1Mrad) –

AMICSA 2012

Evaluation of AMS 0.35mm CMOS for Space Applications

Universidad de Sevilla / IMSE-CNM 11/36

Temperature & TID Characterization

Hardware

Switch Matrix Board

Connects measurement lines and stores the configuration bits for control of DUT.

PC

•Programming of configuration register

•Control of HP 4155A (test configuration, execution & data trace)

•Output-data local storage

•Test Automation

HP 4155A Semiconductor Parametric Analyzer

•Stimuli generation

•Output data sampling

ASIC board

Placed inside climatic chamber for controlled-temperature tests

Page 12: Evaluation of the AMS 0.35 µm CMOS Technology for Use in Space …microelectronics.esa.int/amicsa/2012/pdf/S5_07_Ramos... · 2012. 9. 5. · Ids vs. Vgs – NMOS/M (0-1Mrad) –

AMICSA 2012

Evaluation of AMS 0.35mm CMOS for Space Applications

Universidad de Sevilla / IMSE-CNM 12/36

SEE Characterization Hardware

ASIC board

ADCs to detect and resolve over-current in supply lines due to latch-ups

FPGA monitors SEU, SET & Latch-Up events and resets power lines if neccessary

Monitors up to six different supplies

PC

•Periodically reads SEU, SET & Latch-Up totals from the FPGA

•Output-data local storage

Page 13: Evaluation of the AMS 0.35 µm CMOS Technology for Use in Space …microelectronics.esa.int/amicsa/2012/pdf/S5_07_Ramos... · 2012. 9. 5. · Ids vs. Vgs – NMOS/M (0-1Mrad) –

AMICSA 2012

Evaluation of AMS 0.35mm CMOS for Space Applications

Universidad de Sevilla / IMSE-CNM 13/36

Postprocessing Software

Raw data visualization

Parameter extraction

Graphical data comparison among tests performed in different conditions

Export selected data to text files

MATLAB scripts

Page 14: Evaluation of the AMS 0.35 µm CMOS Technology for Use in Space …microelectronics.esa.int/amicsa/2012/pdf/S5_07_Ramos... · 2012. 9. 5. · Ids vs. Vgs – NMOS/M (0-1Mrad) –

AMICSA 2012

Evaluation of AMS 0.35mm CMOS for Space Applications

Universidad de Sevilla / IMSE-CNM 14/36

Data Post-processing

Raw data is compensated for: • Voltage drop in multiplexer switches • Body-effect due to increase in source voltage • Leakage currents in input pads and multiplexers

CMOS Parameters Extracted: Vth (linear (Vds=Vgs) and saturation (Vds=0.1 V)) Subthreshold leakage current Gain Factor (KP) Body effect Saturation current

Dint

Sint

BulkGate

Rsw

Rsw

Dext

Sext

ID

IS

ILD

ILD

Page 15: Evaluation of the AMS 0.35 µm CMOS Technology for Use in Space …microelectronics.esa.int/amicsa/2012/pdf/S5_07_Ramos... · 2012. 9. 5. · Ids vs. Vgs – NMOS/M (0-1Mrad) –

AMICSA 2012

Evaluation of AMS 0.35mm CMOS for Space Applications

Universidad de Sevilla / IMSE-CNM 15/36

Test Facilities

Low-Temperature • Instituto de Microelectrónica de Sevilla • Instituto Nacional de Técnica Aeroespacial (INTA)

TID • Laboratorio de Radiofísica – Univ. de Santiago de Compostela

SEE • Centre de Ressources du Cyclotron – Louvain-la-Neuve • Centro Nacional de Aceleradores - Sevilla

Page 16: Evaluation of the AMS 0.35 µm CMOS Technology for Use in Space …microelectronics.esa.int/amicsa/2012/pdf/S5_07_Ramos... · 2012. 9. 5. · Ids vs. Vgs – NMOS/M (0-1Mrad) –

AMICSA 2012

Evaluation of AMS 0.35mm CMOS for Space Applications

Universidad de Sevilla / IMSE-CNM 16/36

AMS 0.35 µm CMOS for Space Applications

Introduction

The Characterization Plan

Low-Temperature Characterization Equivalent Width for ELTs

TID Characterization

SEE Characterization

Conclusions and Future Work

Page 17: Evaluation of the AMS 0.35 µm CMOS Technology for Use in Space …microelectronics.esa.int/amicsa/2012/pdf/S5_07_Ramos... · 2012. 9. 5. · Ids vs. Vgs – NMOS/M (0-1Mrad) –

AMICSA 2012

Evaluation of AMS 0.35mm CMOS for Space Applications

Universidad de Sevilla / IMSE-CNM 17/36

Operation at Low Temperature

Instruments located in the outside of the main spacecraft body (masts, booms) have to stand temperatures below the range characterized by the foundries.

• Alternatives: – Heat the ASIC to keep it within the standard temperature range (complex

assembly and high power consumption) – Characterize the behaviour at lower temperatures, adapt the models if

needed, and take extra margins in the design.

Page 18: Evaluation of the AMS 0.35 µm CMOS Technology for Use in Space …microelectronics.esa.int/amicsa/2012/pdf/S5_07_Ramos... · 2012. 9. 5. · Ids vs. Vgs – NMOS/M (0-1Mrad) –

AMICSA 2012

Evaluation of AMS 0.35mm CMOS for Space Applications

Universidad de Sevilla / IMSE-CNM 18/36

Low Temperature Measurements

IMSE • Down to -55ºC using

Thermonics T-2650BV

INTA • Down to -110ºC using SUN

Systems liquid N2 cooled thermal chamber.

Low-Temperature (-110ºC) setup at INTA

Page 19: Evaluation of the AMS 0.35 µm CMOS Technology for Use in Space …microelectronics.esa.int/amicsa/2012/pdf/S5_07_Ramos... · 2012. 9. 5. · Ids vs. Vgs – NMOS/M (0-1Mrad) –

AMICSA 2012

Evaluation of AMS 0.35mm CMOS for Space Applications

Universidad de Sevilla / IMSE-CNM 19/36

Low Temperature Results

-110 -90 -70 -50 -30 -10 10 30 50 70

Resistances

RPOLY1RPOLY2RPOLY2PHRDIFFNRDIFFP

Temperature [ºC]

Res

ista

nce

[Ohm

]

-110 -90 -70 -50 -30 -10 10 30 50 700,40

0,45

0,50

0,55

0,60

0,65

0,70NMOS - 3.3V

Temperature [ºC]

Vth

[V]

Temperature dependence do not show unexpected behaviour beyond the range guaranteed by the foundry (-40ºC)

Page 20: Evaluation of the AMS 0.35 µm CMOS Technology for Use in Space …microelectronics.esa.int/amicsa/2012/pdf/S5_07_Ramos... · 2012. 9. 5. · Ids vs. Vgs – NMOS/M (0-1Mrad) –

AMICSA 2012

Evaluation of AMS 0.35mm CMOS for Space Applications

Universidad de Sevilla / IMSE-CNM 20/36

AMS 0.35 µm CMOS for Space Applications

Introduction

The Characterization Plan

Low-Temperature Characterization

Equivalent Width for ELTs TID Characterization

SEE Characterization

Conclusions and Future Work

Page 21: Evaluation of the AMS 0.35 µm CMOS Technology for Use in Space …microelectronics.esa.int/amicsa/2012/pdf/S5_07_Ramos... · 2012. 9. 5. · Ids vs. Vgs – NMOS/M (0-1Mrad) –

AMICSA 2012

Evaluation of AMS 0.35mm CMOS for Space Applications

Universidad de Sevilla / IMSE-CNM 21/36

Equivalent Width for ELTs

W3

W2

W

L3 L

2

L

d) Annular

a) Standard c) Double Ringed-Source

b) Ringed-Source

Accounts for extra S-D current by an effective width Weff • For Ringed-Source:

• For Double-Ringed Source:

+⋅

+⋅⋅+=3

3

2

2

432

2LWn

LWLWW c

eff

+

+⋅⋅+=3

3

2

2

65

4LWn

LWLWW c

eff

• Incorporated in transistor models and extraction tools.

Page 22: Evaluation of the AMS 0.35 µm CMOS Technology for Use in Space …microelectronics.esa.int/amicsa/2012/pdf/S5_07_Ramos... · 2012. 9. 5. · Ids vs. Vgs – NMOS/M (0-1Mrad) –

AMICSA 2012

Evaluation of AMS 0.35mm CMOS for Space Applications

Universidad de Sevilla / IMSE-CNM 22/36

AMS 0.35 µm CMOS for Space Applications

Introduction

The Characterization Plan

Low-Temperature Characterization

Equivalent Width for ELTs

TID Characterization SEE Characterization

Conclusions and Future Work

Page 23: Evaluation of the AMS 0.35 µm CMOS Technology for Use in Space …microelectronics.esa.int/amicsa/2012/pdf/S5_07_Ramos... · 2012. 9. 5. · Ids vs. Vgs – NMOS/M (0-1Mrad) –

AMICSA 2012

Evaluation of AMS 0.35mm CMOS for Space Applications

Universidad de Sevilla / IMSE-CNM 23/36

TID Tests Three TID Test Campaigns

• CHIP#1, preliminary test, 1 day, 65 krad(Si) • CHIP#1, 4 samples, 9 days, 350 krad(Si)

– From 0.02 rad/s to 2.5 rad/s, doubling at each step. – Annealing 6 weeks @RT, 84 hours @ 100ºC unbiased, 84 hours @ 100ºC

biased.

• CHIP#2, 4 samples, 6 irradiation steps of 42 hours each, reaching 1Mrad(Si) over 6 weeks, with delayed measurements.

– From 0.5 rad/s to 2 rad/s, increasing by 1.33 at each step. – Annealing 16 days @RT -> 95 hours @ 100ºC unbiased -> 73 hours @

100ºC unbiased.

• Irradiations performed at Laboratorio de Radiofísica (USC, Spain)

Page 24: Evaluation of the AMS 0.35 µm CMOS Technology for Use in Space …microelectronics.esa.int/amicsa/2012/pdf/S5_07_Ramos... · 2012. 9. 5. · Ids vs. Vgs – NMOS/M (0-1Mrad) –

AMICSA 2012

Evaluation of AMS 0.35mm CMOS for Space Applications

Universidad de Sevilla / IMSE-CNM 24/36

Irradiation CHIP#1 – NMOS/M

0 50 100 150 200 250 300 350-50

-40

-30

-20

-10

0

10

20

30

40

50TID - Delta_Vth - NMOS/NMOSM

NMOS-LongNMOSM-LongNMOSM-ShortNMOS-Short

TID [krad(Si)]

Del

ta_V

th [m

V]

Drift inmediately after irradiation negligible for thin-oxide gates. More significant for thick-oxide with short length Leakage important for short transistors. Negligible effect for long transistors with thin-oxide.

0 50 100 150 200 250 300 3501E-12

1E-11

1E-10

1E-9

1E-8

1E-7

1E-6

1E-5TID - D_S Leakage - NMOS/NMOSM

NMOSM-ShortNMOS-ShortNMOSM-LongNMOS-Long

TID [krad]IL

DS

[A/u

m]

Page 25: Evaluation of the AMS 0.35 µm CMOS Technology for Use in Space …microelectronics.esa.int/amicsa/2012/pdf/S5_07_Ramos... · 2012. 9. 5. · Ids vs. Vgs – NMOS/M (0-1Mrad) –

AMICSA 2012

Evaluation of AMS 0.35mm CMOS for Space Applications

Universidad de Sevilla / IMSE-CNM 25/36

Annealing CHIP#1 – NMOS/M

0 10 20 30 40 50 60 70-90

-70

-50

-30

-10

10

30

50

70

90Annealing - NMOSM - Delta_Vth

Long (Avg)Short (Avg)Long (Worst)Short (Worst)

Time [Days]

Del

ta_V

th [m

V]

Irradiation: Days 0 to 9 (up to 350 krad(Si)) Annealing: Day 47, 6 wk @ RT; Day 54, 70h @100ºC unbiased, Days 61/ 63/ 64/ 69, after 90/ 112/ 133/ 157 hours @ 100ºC biased

0 10 20 30 40 50 60 701E-12

1E-11

1E-10

1E-9

1E-8

1E-7

1E-6

1E-5Annealing - D_S Leakage - NMOS/NMOSM

NMOSM-ShortNMOS-ShortNMOSM-LongNMOS-Long

Time [days]

ILD

S [A

/um

]

Page 26: Evaluation of the AMS 0.35 µm CMOS Technology for Use in Space …microelectronics.esa.int/amicsa/2012/pdf/S5_07_Ramos... · 2012. 9. 5. · Ids vs. Vgs – NMOS/M (0-1Mrad) –

AMICSA 2012

Evaluation of AMS 0.35mm CMOS for Space Applications

Universidad de Sevilla / IMSE-CNM 26/36

Ids vs. Vgs – NMOS/M (0-1Mrad) – CHIP#2

0 0,2 0,4 0,6 0,8 1 1,2 1,41E-12

1E-11

1E-10

1E-09

1E-08

1E-07

1E-06

1E-05

1E-04

1E-03NMOSM, L=0.5, 0 - 1010 krad

w1/0.5 - 0 kradw1/0.5 - 1010 kradw2/0.5 - 0 kradw2/0.5 - 1010 kradw3/0.5 - 0 kradw3/0.5 - 1010 kradRw2/0.5 - 0 kradRw2/0.5 - 1010 kradRw3/0.5 - 0 kradRw3/0.5 - 1010 krad

Vgs = Vds [V]

Ids

[A]

0 0,2 0,4 0,6 0,8 1 1,2 1,41E-12

1E-11

1E-10

1E-09

1E-08

1E-07

1E-06

1E-05

1E-04

1E-03

1E-02NMOS, L=0.35, 0 - 1010 krad

w1/0.35 - 0 kradw1/0.35 - 1010 kradw2/0.35 - 0 kradw2/0.35 - 1010kradw3/0.35 - 0 kradw3/0.35 - 1010 kradw4/0.35 - 0 kradw4/0.35 - 1010 kradw5/0.35 - 0 kradw5/0.35 - 1010 kradRw4/0.35 - 0 kradRw4/0.35 - 1010 kradRw5/0.35 - 0 kradRw5/0.35 - 1010 krad

Vgs = Vds [V]

Ids

[A]

Irradiation: 6 weekly steps of 42 hours each (up to 350 krad(Si)) Thin-oxide (NMOS): Little effect for standard layout, negligible for ringed layout Thick-oxide (NMOSM): Increase in zero bias leakage for standard transistors. Increased subthreshold swing in all types.

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AMICSA 2012

Evaluation of AMS 0.35mm CMOS for Space Applications

Universidad de Sevilla / IMSE-CNM 27/36

Dependence on Transistor Dimensions

0 1 2 3 4-120

-100

-80

-60

-40

-20

0

20

40Annealing NMOSMB

0.4/0.5 2.1/0.5 4/0.5 R2.12/0.5R4/0.5 0.8/1 2.10/1 4/1R2.12/1 R4/1 2.10/3 4/3R2.12/3 R4/3

Step

dVth

[mV]

∆Vth for thick-oxide NMOS after: 1) 1 Mrad(Si); 2) 16 days @25ºC; 3) 95 hours @ 100ºC; 4) 168 hours @ 100ºC Note clustering on transistor length: 0.5µm (red); 1µm (green); 3µm (blue); and stronger effect for narrow transistors

Page 28: Evaluation of the AMS 0.35 µm CMOS Technology for Use in Space …microelectronics.esa.int/amicsa/2012/pdf/S5_07_Ramos... · 2012. 9. 5. · Ids vs. Vgs – NMOS/M (0-1Mrad) –

AMICSA 2012

Evaluation of AMS 0.35mm CMOS for Space Applications

Universidad de Sevilla / IMSE-CNM 28/36

Comparison of Irradiation Campaigns

Comparison made using transistors of similar dimensions.

Upward shift of ∆Vth for NMOSM and PMOSM transistors in second TID test (up to 1 Mrad). Probably due to longer time between irradiation steps, combined with faster annealing of oxide charges (Not) than interface charges (Nit).

0 200 400 600 800 1000 1200-70

-60

-50

-40

-30

-20

-10

0

10NMOSM

2.1/0.5 1p65-0p5

TID [krad(Si)]

d_V

th [m

V]

0 200 400 600 800 1000 1200-100

0

100

200

300

400

500

600PMOSM

0.4/2 0p4-10

TID [krad(Si)]

d_V

th [m

V]

Page 29: Evaluation of the AMS 0.35 µm CMOS Technology for Use in Space …microelectronics.esa.int/amicsa/2012/pdf/S5_07_Ramos... · 2012. 9. 5. · Ids vs. Vgs – NMOS/M (0-1Mrad) –

AMICSA 2012

Evaluation of AMS 0.35mm CMOS for Space Applications

Universidad de Sevilla / IMSE-CNM 29/36

AMS 0.35 µm CMOS for Space Applications

Introduction

The Characterization Plan

Low-Temperature Characterization

Equivalent Width for ELTs

TID Characterization

SEE Characterization Conclusions and Future Work

Page 30: Evaluation of the AMS 0.35 µm CMOS Technology for Use in Space …microelectronics.esa.int/amicsa/2012/pdf/S5_07_Ramos... · 2012. 9. 5. · Ids vs. Vgs – NMOS/M (0-1Mrad) –

AMICSA 2012

Evaluation of AMS 0.35mm CMOS for Space Applications

Universidad de Sevilla / IMSE-CNM 30/36

SEE Tests

Eight-hours beam time using Heavy-Ion Cocktail #1 of Cyclone-UCL

• Normal incidence, room temperature.

• Measurements on 2 samples

Ion LET [MeV·cm2/mg]

DUT Energy[MeV]

Range [µm (Si)]

15N3+ 3.3 60 59 20Ne4+ 6.4 78 45 40Ar8+ 15.9 151 40 84Kr17+ 40.4 305 39

124Xe25+ 67.7 420 37

LET [MeV·cm2/mg]

Fluence [1/s·cm2] Standard Ringed Enclosed DICE

6.4 5.6·107 3 0 0 0

15.9 2.8·107 178 1 0 0

40.4 7.5·106 233 127 15 0

67.7 5.5·106 617 179 104 4 SEU Errors

Ion Cocktail #1

Page 31: Evaluation of the AMS 0.35 µm CMOS Technology for Use in Space …microelectronics.esa.int/amicsa/2012/pdf/S5_07_Ramos... · 2012. 9. 5. · Ids vs. Vgs – NMOS/M (0-1Mrad) –

AMICSA 2012

Evaluation of AMS 0.35mm CMOS for Space Applications

Universidad de Sevilla / IMSE-CNM 31/36

SEU & Latchup Results

0 10 20 30 40 50 60 701E-7

1E-6

1E-5

1E-4

1E-3

1E-2

1E-1

1E+0

StandardRingedEnclosedDICEWeibull-StandardWeibull-RingedWeibull-Enclosed

LET [MeV/mg/cm2]

SEU

Prob

abili

ty

0 10 20 30 40 50 60 701E-7

1E-6

1E-5

1E-4

1E-3

1E-2

1E-1

1E+0

LET [MeV/mg/cm2]

Latc

h-up

Pro

babi

lity

SEU Lth [MeV·cm2/mg] / σsat [cm2]

Standard: 5.5 2.8·10-6

Ringed: 16.0 3.3·10-7

Enclosed: 35.0 1 9·10-7

Latch-Up Lth [MeV·cm2/mg] / σsat [cm2]

Standard: 9 1.1·10-5

RHBD: > 67.7 ?

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AMICSA 2012

Evaluation of AMS 0.35mm CMOS for Space Applications

Universidad de Sevilla / IMSE-CNM 32/36

AMS 0.35 mm CMOS for Space Applications

Introduction

The Characterization Plan

Low-Temperature Characterization

Equivalent Width for ELTs

TID Characterization

SEE Characterization

Conclusions and Future Work

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AMICSA 2012

Evaluation of AMS 0.35mm CMOS for Space Applications

Universidad de Sevilla / IMSE-CNM 33/36

Summary of Tests CHIP#1

Temperature: -50, -25, 0, 25, 50, 75 ºC @ IMSE Temperature: -50, -70, -90, -110 ºC @ INTA TID: 1.15, 3.7, 8.9, 19.4, 40, 81, 167, 326, 366 krad(Si) @ USC SEE: N, Ne, Ar, Kr, Xe @ UCL Annealing @ IMSE

CHIP#2 Temperature / -50, 25, 100 ºC @ IMSE TID / 75, 175, 305, 480, 710, 1010 krad(Si) @ USC Annealing @ IMSE

CHIP#3 SEE: @ UCL (scheduled for October 2012)

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AMICSA 2012

Evaluation of AMS 0.35mm CMOS for Space Applications

Universidad de Sevilla / IMSE-CNM 34/36

Conclusions

Temperature Behaviour down to -110ºC in good agreement with the prediction of the standard foundry models.

TID Vth drift low (< 30 mV @ 300 krad(Si)) for thin-oxide transistors. Vth drift moderate (+180mV PMOSM, -30mV NMOSM @ 300 krad(Si)) for thick-oxide transistors Ringed-source layout is effective in reduction of TID induced S-D leakage in NMOS.

SEE SEU Lth [MeV·cm2/mg]: 5.5 (standard); 16 (ringed-source); > 68 (DICE) Latch-Up Lth [MeV·cm2/mg]: 9 (standard); > 68 (RHBD layout)

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AMICSA 2012

Evaluation of AMS 0.35mm CMOS for Space Applications

Universidad de Sevilla / IMSE-CNM 35/36

Future Work

RHBD Digital Library • Perform SEE Tests • Improve cell layout and add more cell types

Analog • Model dependence of Vth with radiation and transistor dimensions • Characterize bipolar devices for displacement damage using

proton source at CNA

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AMICSA 2012

Evaluation of AMS 0.35mm CMOS for Space Applications

Universidad de Sevilla / IMSE-CNM 36/36

Thank you for your attention!