Register file reliability enhancement through adjacent narrow-width exploitation

Due to the increasing vulnerability of CMOS circuits, new generations of microprocessors require an inevitable focus on reliability issues. As the Register File (RF) constitutes a critical element within the processor pipeline, it is mandatory to enhance the RF reliability to develop fault tolerant architectures. This paper proposes Adjacent Register Hardened RF (ARH), a new RF architecture that exploits the adjacent byte-level narrow-width values for hardening registers at runtime. Registers are paired together by some special switches referred to as joiners. Dummy sign bits of each register are used to keep redundant data of its counterpart register. We use 7T/14T SRAM cell [6] to combine redundant bits together to make a single bit cell which is, by far, more resilient against faults. Our simulations show that with 3% to 12% power overhead and 10% to 20% increase in area, in comparison to baseline RF, we can obtain up to 80% reduction in soft error rate (SER). © 2016 IEEE

Conception de systèmes embarqués fiables et auto-réglables : applications sur les systèmes de transport ferroviaire

During the last few decades, a tremendous progress in the performance of semiconductor devices has been accomplished. In this emerging era of high performance applications, machines need not only to be efficient but also need to be dependable at circuit and system levels. Several works have been proposed to increase embedded systems efficiency by reducing the gap between software flexibility and hardware high-performance. Due to their reconfigurable aspect, Field Programmable Gate Arrays (FPGAs) represented a relevant step towards bridging this performance/flexibility gap. Nevertheless, Dynamic Reconfiguration (DR) has been continuously suffering from a bottleneck corresponding to a long reconfiguration time.In this thesis, we propose a novel medium-grained high-speed dynamic reconfiguration technique for DSP48E1-based circuits. The idea is to take advantage of the DSP48E1 slices runtime reprogrammability coupled with a re-routable interconnection block to change the overall circuit functionality in one clock cycle. In addition to the embedded systems efficiency, this thesis deals with the reliability chanllenges in new sub-micron electronic systems. In fact, as new technologies rely on reduced transistor size and lower supply voltages to improve performance, electronic circuits are becoming remarkably sensitive and increasingly susceptible to transient errors. The system-level impact of these errors can be far-reaching and Single Event Transients (SETs) have become a serious threat to embedded systems reliability, especially for especially for safety critical applications such as transportation systems. The reliability enhancement techniques that are based on overestimated soft error rates (SERs) can lead to unnecessary resource overheads as well as high power consumption. Considering error masking phenomena is a fundamental element for an accurate estimation of SERs.This thesis proposes a new cross-layer model of circuits vulnerability based on a combined modeling of Transistor Level (TLM) and System Level Masking (SLM) mechanisms. We then use this model to build a self adaptive fault tolerant architecture that evaluates the circuit’s effective vulnerability at runtime. Accordingly, the reliability enhancement strategy is adapted to protect only vulnerable parts of the system leading to a reliable circuit with optimized overheads. Experimentations performed on a radar-based obstacle detection system for railway transportation show that the proposed approach allows relevant reliability/resource utilization tradeoffs.Un énorme progrès dans les performances des semiconducteurs a été accompli ces dernières années. Avec l’´émergence d’applications complexes, les systèmes embarqués doivent être à la fois performants et fiables. Une multitude de travaux ont été proposés pour améliorer l’efficacité des systèmes embarqués en réduisant le décalage entre la flexibilité des solutions logicielles et la haute performance des solutions matérielles. En vertu de leur nature reconfigurable, les FPGAs (Field Programmable Gate Arrays) représentent un pas considérable pour réduire ce décalage performance/flexibilité. Cependant, la reconfiguration dynamique a toujours souffert d’une limitation liée à la latence de reconfiguration.Dans cette thèse, une nouvelle technique de reconfiguration dynamiqueau niveau ”grain-moyen” pour les circuits à base de blocks DSP48E1 est proposée. L’idée est de profiter de la reprogrammabilité des blocks DSP48E1 couplée avec un circuit d’interconnection reconfigurable afin de changer la fonction implémentée par le circuit en un cycle horloge. D’autre part, comme les nouvelles technologies s’appuient sur la réduction des dimensions des transistors ainsi que les tensions d’alimentation, les circuits électroniques sont devenus de plus en plus susceptibles aux fautes transitoires. L’impact de ces erreurs au niveau système peut être catastrophique et les SETs (Single Event Transients) sont devenus une menace tangible à la fiabilité des systèmes embarqués, en l’occurrence pour les applications critiques comme les systèmes de transport. Les techniques de fiabilité qui se basent sur des taux d’erreurs (SERs) surestimés peuvent conduire à un gaspillage de ressources et par conséquent un cout en consommation de puissance électrique. Il est primordial de prendre en compte le phénomène de masquage d’erreur pour une estimation précise des SERs.Cette thèse propose une nouvelle modélisation inter-couches de la vulnérabilité des circuits qui combine les mécanismes de masquage au niveau transistor (TLM) et le masquage au niveau Système (SLM). Ce modèle est ensuite utilisé afin de construire une architecture adaptative tolérante aux fautes qui évalue la vulnérabilité effective du circuit en runtime. La stratégie d’amélioration de fiabilité est adaptée pour ne protéger que les parties vulnérables du système, ce qui engendre un circuit fiable avec un cout optimisé. Les expérimentations effectuées sur un système de détection d’obstacles à base de radar pour le transport ferroviaire montre que l’approche proposée permet d’´établir un compromis fiabilité/ressources utilisées

Engineering study for a mass memory system for advanced spacecrafts Final report, 1 Dec. 1969 - 1 Jul. 1970

Mass memory system for advanced spacecraf

Development of a new trigger system for spin-filtering studies

Polarized antiprotons allow unique access to a number of fundamental physics observables. One example is the transversity distribution which is the last missing piece to complete the knowledge of the nucleon partonic structure at leading twist in the QCD-based parton model. The transversity is directly measurable via Drell-Yan production in double polarized antiproton-proton collisions. This and a multitude of other findings, which are accessible via ~p ~p scattering experiments, led the Polarized Antiproton eXperiments (PAX) Collaboration to propose such investigations at the High Energy Storage Ring (HESR) of the Facility for Antiproton and Ion Research (FAIR). Futhermore the production of intense polarized antiproton beams is still an unsolved problem, which is the core of the PAX proposal. In this frame, an intense work on the feasibility of this ambitious project is going on at COSY (COoler SYnchrotron of the Institut für KernPhysik –IKP– of the Forschungs Zentrum Jülich) (FZJ) where the work of this thesis has been performed. Presently, the only available method to polarize an antiproton beam is by means of the mechanism of spin-filtering exploiting the spin dependence of the (p p) interaction via the repeated interaction with a polarized hydrogen target. Since the total cross section is different for parallel and antiparallel orientation of the beam particle spins relative to the direction of the target polarization, one spin direction is depleted faster than the other, so that the circulating beam becomes increasingly polarized, while the intensity decreases with time. A spin-filtering experiment with protons has been prepared and finally realized in 2011 at the COSY ring in Jülich. Aims of the spin-filtering experiments at COSY performed by the PAX Collaboration were two. The first was to confirm the present understanding of the spin filtering processes in storage rings, and the second was the commissioning of the experimental setup, which will be used for the experiments with the antiprotons. The major part of my PhD work consisted in the development and commissioning of a new trigger board to be implemented in the Data Acquisition System (DAQ) of the experiment. The motivation for the project was the replacement of the existing old-fashioned trigger system based on NIM logic modules, with a modern system based on FPGA programmable chips. This, also in perspective of the more complex detection system that the Collaboration is planning to realize for the future experimental activity. The trigger board was designed and realized by the electronic workshop of the University of Ferrara and INFN of Ferrara. My first task was to write the control-software of the board. After that I performed a series of development and commissioning tests which successfully demonstrated the full efficiency of the board and gave green light for the implementation of the board in the experimental setup

D2.1 Performance evaluation framework

This deliverable contains a proposal for a performance evaluation framework that aims at ensuring that multiple projects within 5G-PPP wireless strand can quantitatively assess and compare the performance of different 5G RAN design concepts. The report collects the vision of several 5G-PPP projects and is conceived as a living document to be further elaborated along with the 5G-PPP framework workshops planned during 2016.Weber, A.; Agyapong, P.; Rosowski, T.; Zimmerman, G.; Fallgren, M.; Sharma, S.; Kousaridas, A.... (2016). D2.1 Performance evaluation framework. https://doi.org/10.13140/RG.2.2.35447.2192

Proceedings of the Second FAROS Public Workshop, 30th September 2014, Espoo, Finland

FAROS is an EC FP7 funded, three year project to develop an approach to incorporate human factors into Risk-Based Design of ships. The project consortium consists of 12 members including industry, academia and research institutes. The second FAROS Public Workshop was held in Dipoli Congress Centre in Otaniemi, Espoo, Finland, on the 30th of September 2014. The workshop included keynotes from industry, papers on risk models for aspects such as collision and grounding, fire and the human element, descriptions of parametric ship models and the overall approach being adopted in the FAROS project

Reconfiguration for Fault Tolerance and Performance Analysis

Architecture reconfiguration, the ability of a system to alter the active interconnection among modules, has a history of different purposes and strategies. Its purposes develop from the relatively simple desire to formalize procedures that all processes have in common to reconfiguration for the improvement of fault-tolerance, to reconfiguration for performance enhancement, either through the simple maximizing of system use or by sophisticated notions of wedding topology to the specific needs of a given process. Strategies range from straightforward redundancy by means of an identical backup system to intricate structures employing multistage interconnection networks. The present discussion surveys the more important contributions to developments in reconfigurable architecture. The strategy here is in a sense to approach the field from an historical perspective, with the goal of developing a more coherent theory of reconfiguration. First, the Turing and von Neumann machines are discussed from the perspective of system reconfiguration, and it is seen that this early important theoretical work contains little that anticipates reconfiguration. Then some early developments in reconfiguration are analyzed, including the work of Estrin and associates on the fixed plus variable restructurable computer system, the attempt to theorize about configurable computers by Miller and Cocke, and the work of Reddi and Feustel on their restructable computer system. The discussion then focuses on the most sustained systems for fault tolerance and performance enhancement that have been proposed. An attempt will be made to define fault tolerance and to investigate some of the strategies used to achieve it. By investigating four different systems, the Tandern computer, the C.vmp system, the Extra Stage Cube, and the Gamma network, the move from dynamic redundancy to reconfiguration is observed. Then reconfiguration for performance enhancement is discussed. A survey of some proposals is attempted, then the discussion focuses on the most sustained systems that have been proposed: PASM, the DC architecture, the Star local network, and the NYU Ultracomputer. The discussion is organized around a comparison of control, scheduling, communication, and network topology. Finally, comparisons are drawn between fault tolerance and performance enhancement, in order to clarify the notion of reconfiguration and to reveal the common ground of fault tolerance and performance enhancement as well as the areas in which they diverge. An attempt is made in the conclusion to derive from this survey and analysis some observations on the nature of reconfiguration, as well as some remarks on necessary further areas of research

CALIFA, the Calar Alto Legacy Integral Field Area survey: IV. Third public data release

This paper describes the third public data release (DR3) of the Calar Alto Legacy Integral Field Area (CALIFA) survey. Science-grade quality data for 667 galaxies are made public, including the 200 galaxies of the second public data release (DR2). Data were obtained with the integral-field spectrograph PMAS/PPak mounted on the 3.5 m telescope at the Calar Alto Observatory. Three different spectral setups are available: i) a low-resolution V500 setup covering the wavelength range 3745-7500 Å (4240-7140 Å unvignetted) with a spectral resolution of 6.0 Å (FWHM) for 646 galaxies, ii) a medium-resolution V1200 setup covering the wavelength range 3650-4840 Å (3650-4620 Å unvignetted) with a spectral resolution of 2.3 Å (FWHM) for 484 galaxies, and iii) the combination of the cubes from both setups (called COMBO) with a spectral resolution of 6.0 Å and a wavelength range between 3700-7500 Å (3700-7140 Å unvignetted) for 446 galaxies. The Main Sample, selected and observed according to the CALIFA survey strategy covers a redshift range between 0.005 and 0.03, spans the color-magnitude diagram and probes a wide range of stellar masses, ionization conditions, and morphological types. The Extension Sample covers several types of galaxies that are rare in the overall galaxy population and are therefore not numerous or absent in the CALIFA Main Sample. All the cubes in the data release were processed using the latest pipeline, which includes improved versions of the calibration frames and an even further improved image reconstruction quality. In total, the third data release contains 1576 datacubes, including ~1.5 million independent spectra. © 2016 ESO.SFS thanks the CONACYT-125180 and DGAPA-IA100815 projects for providing him support in this study. R.G.B., R.G.D., and E.P. are supported by grants AYA2014-57490-P and JA-FQM-2828. SZ is supported by the EU Marie Curie Integration Grant >SteMaGE> No. PCIG12-GA-2012-326466 (Call Identifier: FP7-PEOPLE-2012 CIG). J. F.-B. from grant AYA2013-48226-C3-1-P from the Spanish Ministry of Economy and Competitiveness (MINECO), as well as from the FP7 Marie Curie Actions of the European Commission, via the Initial Training Network DAGAL under REA grant agreement 289313 B.G-L- acknowledges financial support by the Spanish MINECO under grants AYA2013-41656-P and AYA2015-68217-P Support for L.G. is provided by the Ministry of Economy, Development, and Tourism's Millennium Science Initiative through grant IC12009, awarded to The Millennium Institute of Astrophysics, MAS. L.G. also acknowledges support by CONICYT through FONDECYT grant 3140566, and AYA2013-42227-P from the Spanish Ministerio de Ciencia e Innovacion and TIC 114 and PO08-TIC-3531 from Junta de Andalucia. AG acknowledges support from the FP7/2007-2013 under grant agreement no. 267251 (AstroFIt). RAM was funded by the Spanish programme of International Campus of Excellence Moncloa (CEI). JMA acknowledges support from the European Research Council Starting Grant (SEDmorph; P.I. V. Wild). I.M. and A.d.O. acknowledge the support by the projects AYA2010-15196 from the Spanish Ministerio de Ciencia e Innovacion and TIC 114 and PO08-TIC-3531 from Junta de Andalucia. AMI acknowledges support from Agence Nationale de la Recherche through the STILISM project (ANR-12-BS05-0016-02). M.M. acknowledges financial support from AYA2010-21887-004-02 from the Ministerio de Economia y Competitividad. PSB acknowledges support from the Ramon y Cajal program, grant ATA2010-21322-C03-02 from the Spanish Ministry of Economy and Competitiveness (MINECO). C.J.W. acknowledges support through the Marie Curie Career Integration Grant 303912. V.W. acknowledges support from the European Research Council Starting Grant (SEDMorph P.I. V. Wild) and European Career Re-integration Grant (Phiz-Ev P.I. V. Wild). YA acknowledges financial support from the Ramon y Cajal programme (RyC-2011-09461) and project AYA2013-47742-C4-3-P, both managed by the Ministerio de Economia y Competitividad, as well as the >Study of Emission-Line Galaxies with Integral Field Spectroscopy> (SELGIFS) programme, funded by the EU (FP7-PEOPLE-2013-IRSES-612701) within the Marie-Sklodowska-Curie Actions scheme. ROM acknowledges support from CAPES (Brazil) through a PDJ fellowship from project 88881.030413/2013-01, program CSF-PVE.Peer Reviewe

CALIFA, the Calar Alto Legacy Integral Field Area Survey IV. Third public data release

This paper describes the third public data release (DR3) of the Calar Alto Legacy Integral Field Area (CALIFA) survey. Science-grade quality data for 667 galaxies are made public, including the 200 galaxies of the second public data release (DR2). Data were obtained with the integral field spectrograph PMAS/PPak mounted on the 3.5 m telescope at the Calar Alto Observatory. Three different spectral setups are available: i) a low-resolution V500 setup covering the wavelength range 3745-7500 angstrom (4240-7140 angstrom unvignetted) with a spectral resolution of 6.0 angstrom (FWHM) for 646 galaxies, ii) a medium-resolution V1200 setup covering the wavelength range 3650-4840 angstrom (3650-4620 angstrom unvignetted) with a spectral resolution of 2.3 angstrom (FWHM) for 484 galaxies, and iii) the combination of the cubes from both setups (called COMBO) with a spectral resolution of 6.0 angstrom and a wavelength range between 3700-7500 angstrom (3700-7140 angstrom unvignetted) for 446 galaxies. The Main Sample, selected and observed according to the CALIFA survey strategy covers a redshift range between 0.005 and 0.03, spans the color-magnitude diagram and probes a wide range of stellar masses, ionization conditions, and morphological types. The Extension Sample covers several types of galaxies that are rare in the overall galaxy population and are therefore not numerous or absent in the CALIFA Main Sample. All the cubes in the data release were processed using the latest pipeline, which includes improved versions of the calibration frames and an even further improved image reconstruction quality. In total, the third data release contains 1576 datacubes, including-1.5 million independent spectra