Microchip Technology Incorporated · NASDAQ:MCHP

Microchip Technology — Space Forum 2019

32 slides from Microchip Technology's conference presentation, Oct 17, 2019

  1. Slide 1: RTG4 FPGA Update: Qualification, Radiation, Sub-QML

    RTG4™ FPGA Update: Qualification, Radiation, Sub-QML Minh Nguyen Space Forum 2019

  2. Slide 2: Agenda

    Agenda  RTG4™ FPGA Update  Qualification  Radiation  Sub-QML FPGAs Space Forum 2019 2

  3. Slide 3: RTG4 FPGA Update

    RTG4 FPGA Update Space Forum 2019 3

  4. Slide 4: RTG4 Product Overview

    RTG4 Product Overview Resources RT4G150 CG1657 / LG1657 CQ352 Logic Elements (TMR Register + 4-Input C Logic) 151,824 151,824 18x18 Multiply-Accumulate Blocks 462 462 RAM Mbits (1.5 Kbit and 24 Kbit Blocks, with ECC) 5.2 5.2 UPROM Kbits 381 381 DDR2/3 SDRAM Controller (with ECC)hjhkjhkj 2 x 32 0 PCI

  5. Slide 5: Low-Power Grade

    RTG4 Low-Power Grade  Low-power grade (–L) for RTG4 9 standard speed (-STD) available 8 NOW 7 25% quiescent supply current reduction: Static Power (W)  6 Competing RT FPGA from 4.1 A to 3.1 A at 125 °C 5 Competing RT FPGA -L  RT4G150L device setting available 4 (Low Power Grade) RTG4 in Libero So

  6. Slide 6: Qualification Status

    RTG4 Qualification Status  CG/LG 1657 QML Class Q and Class V qualification completed!  SMD 5962-16208  SMD has been approved and is posted on the DLA web site  SMD numbers are also posted on the Microsemi web site  CQ352 QML Class Q and QML Class V in progress  QML-Q qualification is expected

  7. Slide 7: Availability Schedule

    RTG4 Availability Schedule  RT4G150 PROTO FPGAs: Available to lead time now  RT4G150 development kit: Available to lead time now  CG1657 daisy chain packages: Available to lead time now  CG1657 B, E, V-flow flight units, and CQ352 B, E-flow flight units: Available to lead time now  CQ352 EV-flo

  8. Slide 8: Radiation Summary

    RTG4 Radiation Summary Total Ionizing Dose Stays within parametric limits > 125 Krad (Si) Single Event Latch-Up No failure at facility limit of 103 MeV-cm2/mg, 100 °C Configuration Upset No failure at facility limit of 103 MeV-cm2/mg, 100 °C Flip-Flop Single Event Upset 2.6E-12 errors/bit-day, GEO s

  9. Slide 9: Radiation Update

    RTG4 Radiation Update Test Environment Test Schedule Status Fabric, SRAM and PLL SEE Proton Complete Report available on Microsemi Web SERDES SEE Proton UCD in 10/2018 Less link loss than previous HI testing Report in progress SERDES SEE Heavy Ion LBNL in 10/2018 Report in progress In-Beam Programmi

  10. Slide 10: PLL Results

    PLL Results  Heavy Ion Testing, GEO solar min PLL Mode Clock Source Recovery Error rate 1 Loss of Lock (upset/PLL/day) every Single PLL External Self 8.28 E-05 33 years Single PLL External PLL Reset 4.00 E-07 6800 years TMR PLL External PLL Reset 1.88 E-05 145 years  Proton Testing  No upsets det

  11. Slide 11: Power-On Reset

    RTG4 Power-On Reset  Power-on reset (POR) test in heavy ion beam  Average flux = 46 ions/cm2/s  LET = 37 MeV.cm2/mg  10 out of 10 attempts were successful Space Forum 2019 11

  12. Slide 12: In-Beam Programming Radiation Test Campaigns

    RTG4 In-Beam Programming Radiation Test Campaigns  4 test campaigns were performed to test RTG4 in-beam programming 1. Heavy ion test done at LBNL (2016) with average flux ~1x103 ions/cm2/s 2. Neutron test at LANL (August 2018) 3. Heavy ion test at TAMU (September 2018) with average flux ~35 ions/c

  13. Slide 13: 1st Test Campaign: Heavy Ion at LBNL, 2016

    1st Test Campaign: Heavy Ion at LBNL, 2016  Single event effects on reprogramming  Reprogramming in-beam performed to maximum LET 30 MeV-cm2/mg with average flux of 1x103 ions/cm2/s  Programming failures detected  Programming successful after parts were removed from heavy ion beam  Programming

  14. Slide 14: Programming SEFI (LBNL, 2016)

    Programming SEFI (LBNL, 2016) Weibull Fitting LETth W S σsat 0.1 500 1.2 1.2×10-3 Space Forum 2019 Microchip Confidential ©2019 14

  15. Slide 15: 2nd Test Campaign: Neutron at LANSCE (August 2018)

    2nd Test Campaign: Neutron at LANSCE (August 2018)  Los Alamos National Laboratory LANSCE - WNR  Neutron energies 10 MeV – 800 MeV  Programming passed 10 times out of 10 attempts in neutron beam Attempt # 1 2 3 4 5 6 7 8 9 10 Program Pass Pass Pass Pass Pass Pass Pass Pass Pass Pass Verify Pass P

  16. Slide 16: 3rd Test Campaign: Heavy ion at TAMU (Sept 2018)

    3rd Test Campaign: Heavy ion at TAMU (Sept 2018)  Beam parameters at TAMU:  Average flux = 35 ions/cm2/s  LET = 37 MeV-cm2/mg  In beam 2 out of 10 Programming attempts passed; 2 out of 2 Verify failed  If more Verify attempts are tested, it is most likely that Verify will pass Attempt # 1 2 3 4

  17. Slide 17: Comparison Between TAMU & GEO Flux

    Comparison Between TAMU & GEO Flux  Goal: “real” Programming failure rate GEO Solar Min, 100 Mil Al  Beam parameter @ TAMU: • LET = 37 MeV.cm2/mg • Average flux = 35 ions/cm2/s  GEO parameters (CREME96), 100 Mil Al shielding: • LET = 37 MeV.cm2/mg • Flux Solar Min ~ 6.41E-10 ions/cm2/s • Flux Sol

  18. Slide 18: 4th Test Campaign: Proton at UCD (Oct 2018)

    4th Test Campaign: Proton at UCD (Oct 2018)  In beam, 10 out of 10 programming attempts passed; 10 out of 10 verify passed  UC Davis, 64MeV proton beam Attempt # 1 2 3 4 5 6 7 8 9 10 Program Pass Pass Pass Pass Pass Pass Pass Pass Pass Pass Verify Pass Pass Pass Pass Pass Pass Pass Pass Pass Pass

  19. Slide 19: In-Flight Programming Guidance

    RTG4 In-Flight Programming Guidance  Current guidance  Highly unlikely that a destructive event will occur during programming in space  Probability of first-time success for programming in GEO is estimated > 99%, based on 1st test campaign  It is highly likely that in space, no ion will disrupt

  20. Slide 20: Programs Baselining RTG4

    Programs Baselining RTG4 Mission Extension Orion WFIRST SBC AIDA Vehicle MEV-1 (NASA) (NASA) (LANL) (ESA, DLR, NASA) Launched Oct 9th, 2019 SLIM JPSS-2 Reconfigurable ALOS-3 Optical ALOS-4 SAR (JAXA) (NOAA) Processor (JAXA) (JAXA) (Commercial) Space Forum 2019 20

  21. Slide 21: Sub-QML FPGAs

    SUB-QML FPGAS Space Forum 2019 21

  22. Slide 22: RT FPGAs for New Space

    RT FPGAs for New Space  Objective  Create versions of RT FPGAs that can meet aggressive price targets to support New Space constellations that would not use traditional B / E / V flow FPGAs  Requirements  Reduction in cost and price  Faster lead-time / cycle-time  Sub-QML RT FPGAs  Ceramic –

  23. Slide 23: Cost and COTS

    Cost and COTS  Satellite operators seeking lower acquisition cost and faster service entry  Commercial Off The Shelf (COTS) components to reduce cost and lead-time  The cost of COTS – lower component cost, higher cost of ownership General Industry QML COTS Rad Tolerant Unit Cost  Low  High Lead

  24. Slide 24: Sub-QML: Bridging the Gap Between QML and COTS

    Sub-QML: Bridging the Gap Between QML and COTS Qualification QML Class V Rad Characterization Rad Hardened Traceability QML Class Q By Design Lot Homogeneity Rad Hardened By Design Sub-QML Hermetic Rad Hardened By Design Sub-QML Plastic • Flight Heritage / Baselined Rad Hardened • Radiation Support

  25. Slide 25: Sub-QML Components

    Sub-QML Components  Reducing or eliminating QML testing and documents removes a lot of cost  Elimination of solder columns removes cost and reduces lead times  Plastic packaging reduces cost further General Industry QML Sub-QML Sub-QML COTS Rad Tolerant RT Hermetic RT Plastic Unit Cost  Lowest 

  26. Slide 26: Screening Flows

    RTG4 Screening Flows Screening Flow Purpose Package Qualification Burn-In Temp Test Life Test DPA Static -55°C – V NSS, NASA Class1 Hermetic Ceramic QML-V Wafer-Lot Assy Lot Dynamic 125°C Advanced Static -55°C – Generic E Hermetic Ceramic QML-Q Optional Traditional Space Dynamic 125°C Group C Entry

  27. Slide 27: Screening Flows for Traditional Space

    RTG4 Screening Flows for Traditional Space Screening Flow Purpose Package Qualification Burn-In Temp Test Life Test DPA Static -55°C – V NSS, NASA Class1 Hermetic Ceramic QML-V Wafer-Lot Assy Lot Dynamic 125°C Advanced Static -55°C – Generic E Hermetic Ceramic QML-Q Optional Traditional Space Dynami

  28. Slide 28: Screening Flows: Hermetic Ceramic for New Space

    RTG4 Screening Flows: Hermetic Ceramic for New Space Screening Flow Purpose Package Qualification Burn-In Temp Test Life Test DPA Static -55°C – V NSS, NASA Class1 Hermetic Ceramic QML-V Wafer-Lot Assy Lot Dynamic 125°C Advanced Static -55°C – Generic E Hermetic Ceramic QML-Q Optional Traditional Sp

  29. Slide 29: Reduced Flow and Mil Temp Hermetic

    RTG4 Reduced Flow and Mil Temp Hermetic  Reduced Flow  Same test and screening flow as B-flow (no test elimination)  Internal gas analysis screened to 10,000 ppm(v) moisture limit  Minimum order quantity (MOQ) and non-cancelable, non-returnable (NCNR) will apply  No datapack, no assembly lot gr

  30. Slide 30: Screening Flows – Plastic Packages for New Space

    RTG4 Screening Flows – Plastic Packages for New Space Screening Flow Purpose Package Qualification Burn-In Temp Test Life Test DPA Static -55°C – V NSS, NASA Class1 Hermetic Ceramic QML-V Wafer-Lot Assy Lot Dynamic 125°C Advanced Static -55°C – Generic E Traditional Space • Hermetic Plastic Ceramic

  31. Slide 31: Plastic Package

    RTG4 Plastic Package  Military temperature screening flow  Test all parts at hot, cold and room  Guarantee TJ -55°C to 125°C  No MIL-STD-883 screening – no burn-in, temp cycle, centrifuge, fine and gross leak, etc. Silicon Thermal Interface Die Material Decoupling  FCG1657 Package Capacitors 

  32. Slide 32: Conclusion

    Conclusion  RTG4 achieved QML Class V qualification  RTG4 achieved first flight heritage on MEV-1  RTG4 FPGA family continues to grow with low-power version, qualified CQ352 package, and new plastic package  New RTG4 radiation data available on Microsemi website  Sub-QML FPGAs bridging the gap

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