56 research outputs found

    A TCAD calibrated approach for on-state modeling of amorphous oxide semiconductor TFTs

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    Amorphous oxide semiconductor materials such as IGZO exhibit electrical characteristics that are not well represented by conventional device models due to the presence of band-tail states (BTS). Common parameters such as threshold voltage and channel mobility that are extracted from measured electrical characteristics can be misrepresentative due to discrepancies between the device operation and the chosen operational model. Compact models that have been developed for model accuracy and circuit simulation efficiency offer limited insight on the underlying device physics involved. The focus of this work is a model for device engineering which maintains a close physical connection to device operation, and captures the 2D influence of both the gate and drain bias conditions on the ionization and deionization of acceptor-like BTS near the conduction band edge. A device model for the on-state operation of accumulation-mode IGZO TFTs was recently presented as an adaptation of a Level 2 SPICE (L2S) model [1]. The model introduced channel charge adjustments which account for the occupancy of BTS as influenced by the gate and drain voltage, and provided an exceptional match to both simulated and measured device characteristics. However the integrity of the model as assessed by the ability to discriminate between the influence of BTS and short-channel effects (SCE) was compromised as the device channel length was decreased. Accumulation-mode devices are susceptible to the onset of SCE at relatively long channel lengths due to the lack of a source-channel junction barrier. While the subthreshold region may show minimal influence of drain induced barrier lowering (DIBL), the on-state may exhibit an effective decrease in the triode region of operation. A new model is presented which incorporates this on-state DIBL along with channel length modulation, and demonstrates improved discrimination between BTS and SCE in the model fit at device channel lengths L ≥ 3 µm. Silvaco® Atlas™ TCAD played a key role in device model development. A long-channel reference device was used to establish the impact of SCE on short devices, which was then modeled by and terms in associated triode and saturation regions of operation. For channel lengths L \u3c 3 µm, a lumped SCE multiplier was used to represent short-channel behavior, followed by the application of BTS parameters for channel charge adjustments. Modeling results derived from both simulated and measured TFT characteristics will be presented. [1] K.D. Hirschman, T. Mudgal, E. Powell and R.G. Manley, ECS Trans. 86, 153 (2018

    Flash lamp annealed polycrystalline silicon as a potential candidate for large panel manufacturing

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    The flat-panel display industry is in pursuit of TFT manufacturing processes which are cost-effective, easily scalable to large glass panels, and meet the performance requirements of advanced display products. While excimer laser anneal (ELA) low-temperature polycrystalline silicon (LTPS) can offer exceptional TFT performance, a lower grade LTPS may still satisfy product requirements at a lower production cost. Flash-Lamp Annealing (FLA) is an emerging candidate for the manufacture of LTPS. Multi-lamp exposure systems with high repetition pulse rates would potentially offer significant advantages in manufacturing throughput and cost over ELA. Techniques to overcome challenges that have hindered device scaling and reduction in variation of device operation are under investigation. The following presents a status update on the development of FLA Polycrystalline Silicon (FLAPS) technology. The FLA equipment used for this work was a NovaCentrix PulseForge 3300 system, capable of uniform exposure of a 7 cm x 12 cm area at intensities as high as 50 kW/cm2 over microseconds pulse duration. PMOS TFTs were fabricated using combinations of FLA, ion implantation and furnace annealing to define the source/drain and channel regions. Predefined polygons of 60 nm thick amorphous silicon vertically sandwiched between layers of SiO2 were crystallized on Corning Lotus NXT display glass using single-pulse FLA exposure. The amorphous silicon melts while absorbing a sufficient fraction of the xenon emission spectrum, and becomes polycrystalline while staying within the thermal constraints of the underlying glass substrate. Boron dopant ions were implantation into the source/drain regions defined by lithographic patterning or a self-aligned gate strategy. Boron activation was realized by combinations of FLA, furnace annealing, and pre-amorphization using an electrically inactive species. FLA conditions following dopant introduction avoided silicon melting which causes significant lateral diffusion. Representative electrical characteristics are shown in figure 1. While the device operation demonstrates a general dependence on the degree of dopant activation, observations on the electrical characteristics indicate a complex relationship between defect states and the specific implant/activation strategy applied. The influence of doping strategy on both device performance and resistance to failure is the primary focus of this work. Additional experiments involving variations in the FLAPS morphology will also be discussed. Please click Additional Files below to see the full abstract

    Mars Earth Return Vehicle (MERV) Propulsion Options

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    The COMPASS Team was tasked with the design of a Mars Sample Return Vehicle. The current Mars sample return mission is a joint National Aeronautics and Space Administration (NASA) and European Space Agency (ESA) mission, with ESA contributing the launch vehicle for the Mars Sample Return Vehicle. The COMPASS Team ran a series of design trades for this Mars sample return vehicle. Four design options were investigated: Chemical Return /solar electric propulsion (SEP) stage outbound, all-SEP, all chemical and chemical with aerobraking. The all-SEP and Chemical with aerobraking were deemed the best choices for comparison. SEP can eliminate both the Earth flyby and the aerobraking maneuver (both considered high risk by the Mars Sample Return Project) required by the chemical propulsion option but also require long low thrust spiral times. However this is offset somewhat by the chemical/aerobrake missions use of an Earth flyby and aerobraking which also take many months. Cost and risk analyses are used to further differentiate the all-SEP and Chemical/Aerobrake options

    Human Exploration Using Real-Time Robotic Operations (HERRO)- Crew Telerobotic Control Vehicle (CTCV) Design

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    The HERRO concept allows real time investigation of planets and small bodies by sending astronauts to orbit these targets and telerobotically explore them using robotic systems. Several targets have been put forward by past studies including Mars, Venus, and near Earth asteroids. A conceptual design study was funded by the NASA Innovation Fund to explore what the HERRO concept and it's vehicles would look like and what technological challenges need to be met. This design study chose Mars as the target destination. In this way the HERRO studies can define the endpoint design concepts for an all-up telerobotic exploration of the number one target of interest Mars. This endpoint design will serve to help planners define combined precursor telerobotics science missions and technology development flights. A suggested set of these technologies and demonstrator missions is shown in Appendix B. The HERRO concept includes a crewed telerobotics orbit vehicle as well three Truck rovers, each supporting two teleoperated geologist robots Rockhounds (each truck/Rockhounds set is landed using a commercially launched aeroshell landing system.) Options include a sample ascent system teamed with an orbital telerobotic sample rendezvous and return spacecraft (S/C) (yet to be designed). Each truck rover would be landed in a science location with the ability to traverse a 100 km diameter area, carrying the Rockhounds to 100 m diameter science areas for several week science activities. The truck is not only responsible for transporting the Rockhounds to science areas, but also for relaying telecontrol and high-res communications to/from the Rockhound and powering/heating the Rockhound during the non-science times (including night-time). The Rockhounds take the place of human geologists by providing an agile robotic platform with real-time telerobotics control to the Rockhound from the crew telerobotics orbiter. The designs of the Truck rovers and Rockhounds will be described in other publications. This document focuses on the CTCV design

    Venus Landsailer Zephyr

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    Imagine sailing across the hot plains of Venus! A design for a craft to do just this was completed by the COncurrent Multidisciplinary Preliminary Assessment of Space Systems (COMPASS) Team for the NASA Innovative Advanced Concepts (NIAC) project. The robotic craft could explore over 30 kilometers of the surface of Venus, driven by the power of the wind. The Zephyr Venus Landsailer is a science mission concept for exploring the surface of Venus with a mobility and science capability roughly comparable to the Mars Exploration Rovers (MER) mission, but using the winds of the thick atmosphere of Venus for propulsion. It would explore the plains of Venus in the year 2025, near the Venera 10 landing site, where wind velocities in the range of 80 to 120 centimeters per second (cm/s) were measured by earlier Soviet landing missions. These winds are harnessed by a large wing/sail which would also carry the solar cells to generate power. At around 250 kilograms (kg), Zephyr would carry an 8 meter tall airfoil sail (12 square meters area), 25 kg of science equipment (mineralogy, grinder, and weather instruments) and return 2 gigabytes of science over a 30 day mission. Due to the extreme temperatures (450 degrees Centigrade) and pressures (90 bar) on Venus, Zephyr would have only basic control systems (based on high temperature silicon carbide (SiC)electronics) and actuators. Control would come from an orbiter which is in turn controlled from Earth. Due to the time delay from the Earth a robust control system would need to exist on the orbiter to keep Zephyr on course. Data return and control would be made using a 250 megahertz link with the orbiter with a maximum data rate of 2 kilobits per second. At the minimal wind speed required for mobility of 35 cm/s, the vehicle move at a slow but steady 4 cm/s by positioning the airfoil and use of one wheel that is steered for pointing control. Navigation commands from the orbiter will be based upon navigation cameras, simple accelerometers and stability sensors; Zephyr's stability is robust, using a wide wheel base along with controls to "feather" or "luff" the airfoil and apply brakes to stop the vehicle in the case of unexpected conditions. This would be the science gathering configuration. The vehicle itself would need to be made from titanium (Ti) as the structural material, with a corrosion-barrier overcoating due to extreme temperatures on the surface

    Advanced Lithium Ion Venus Explorer (ALIVE)

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    The COncurrent Multidisciplinary Preliminary Assessment of Space Systems (COMPASS) Team partnered with the Applied Research Laboratory to perform a NASA Innovative Advanced Concepts (NIAC) Program study to evaluate chemical based power systems for keeping a Venus lander alive (power and cooling) and functional for a period of days. The mission class targeted was either a Discovery (500M)orNewFrontiers(500M) or New Frontiers (750M to 780M)classmission.HistoricSovietVenuslandershaveonlylastedontheorderof2hoursintheextremeVenusenvironment:temperaturesof460degreesCentigradeandpressuresof93bar.Longerdurationmissionshavebeenstudiedusingplutoniumpoweredsystemstooperateandcoollandersforuptoayear.However,theplutoniumloadisverylarge.ThisNIACstudysoughttostillprovidepowerandcoolingbutwithouttheplutonium.Batteriesarefartooheavybutasystemwhichusestheatmosphere(primarilycarbondioxide)andonon−boardfueltopowerapowergenerationandcoolingsystemwassought.TheresulingdesignwastheAdvancedLong−LifeLanderInvestigatingtheVenusEnvironment(ALIVE)Spacecraft(S/C)whichburnslithium(Li)withtheCO2atmospheretoheataDuplexStirlingtopowerandcoolthelanderfora5−dayduration(untiltheLiisexhausted).WhileitdoesnotlastyearsachemicalpoweredsystemsurvivingdayseliminatesthecostassociatedwithutilizingaflybyrelayS/Candallowsacontinuouslowdataratedirecttoearth(DTE)linkinthisinstancefromtheOvdaRegioofVenus.Thefive−daycollectiontimeprovidedbythechemicalpowersystemsalsoenablessciencepersonnelonearthtointeractandretargetscience−somethingnotpossiblewithanapproximately2−hourspacecraftlifetime.Italsoallowsforcontingencyoperationsdirectedbytheground(reducedrisk).ThesciencepackagewasbasedonthatenvisionedbytheVenusIntrepidTesseraLander(VITaL)DecadalSurveyStudy.TheLiBurnerwithinthelongdurationpowersystemcreatesapproximately14000Wofheat.This1300degreeCentigradeheatusingLiinthebottom"ballast"tankismeltedtoliquidbytheVenustemperature,drawnintoafurnacebyawickandburnedwithatmosphericCO2.TheLicarbonateexhaustisliquidat1300degreesCentigradeandbeingdenserthanLidrainsintothetheLitankandsolidifies.Sincetheexhaustproductisadenseliquidno"chimney"isrequiredwhichconservestheheatforthestirlingpowerconvertor.TheDuplexStirlingprovidesabout300Wofpowerandremovesabout300Wofheatfromtheavionicsandheatthatleaksintothe1−bar−insulatedpayloadpressurevesselkeptat25degreesCentigrade.TheNaKradiatorisruntothetopofthedragflap.TheALIVEvehicleiscarriedtoVenusviaanAtlas411launchvehicle(LV)withaC3of7km2/s2.AnAeroshell,derivedfromtheGenesismission,enablesadirectentryintotheatmosphereofVenus(−10degreesCentigrade,40gmax)and6m/sforlanding(44g)usingadragring.Forsurfacescienceandcommunication,a100WRF(WebExRecordingFormat),X−Band0.6−meterpointableDTE(Direct−to−Earth)antennaprovides2kbps(kilobitspersecond)toDSN(Deep−SpaceNetwork)34−meterantennaclusters.Table1.1summarizesthetop−leveldetailsofeachsubsystemthatwasincorporatedintothedesign.CostestimatesoftheALIVEmissionshowitatapproximately780M) class mission. Historic Soviet Venus landers have only lasted on the order of 2 hours in the extreme Venus environment:temperatures of 460 degrees Centigrade and pressures of 93 bar. Longer duration missions have been studied using plutonium powered systems to operate and cool landers for up to a year. However, the plutonium load is very large. This NIAC study sought to still provide power and cooling but without the plutonium. Batteries are far too heavy but a system which uses the atmosphere (primarily carbon dioxide) and on on-board fuel to power a power generation and cooling system was sought. The resuling design was the Advanced Long-Life Lander Investigating the Venus Environment (ALIVE) Spacecraft (S/C) which burns lithium (Li) with the CO2 atmosphere to heat a Duplex Stirling to power and cool the lander for a 5-day duration (until the Li is exhausted). While it does not last years a chemical powered system surviving days eliminates the cost associated with utilizing a flyby relay S/C and allows a continuous low data rate direct to earth (DTE) link in this instance from the Ovda Regio of Venus. The five-day collection time provided by the chemical power systems also enables science personnel on earth to interact and retarget science - something not possible with an approximately 2-hour spacecraft lifetime. It also allows for contingency operations directed by the ground (reduced risk). The science package was based on that envisioned by the Venus Intrepid Tessera Lander (VITaL) Decadal Survey Study. The Li Burner within the long duration power system creates approximately 14000 W of heat. This 1300 degree Centigrade heat using Li in the bottom "ballast" tank is melted to liquid by the Venus temperature, drawn into a furnace by a wick and burned with atmospheric CO2. The Li carbonate exhaust is liquid at 1300 degrees Centigrade and being denser than Li drains into the the Li tank and solidifies. Since the exhaust product is a dense liquid no "chimney" is required which conserves the heat for the stirling power convertor. The Duplex Stirling provides about 300 W of power and removes about 300 W of heat from the avionics and heat that leaks into the 1-bar-insulated payload pressure vessel kept at 25 degrees Centigrade. The Na K radiator is run to the top of the drag flap.The ALIVE vehicle is carried to Venus via an Atlas 411 launch vehicle (LV) with a C3 of 7 km2/s2. An Aeroshell, derived from the Genesis mission, enables a direct entry into the atmosphere of Venus (-10 degrees Centigrade, 40 g max) and 6 m/s for landing (44 g) using a drag ring. For surface science and communication, a 100 WRF (WebEx Recording Format), X-Band 0.6-meter pointable DTE (Direct-to-Earth) antenna provides 2 kbps (kilobits per second) to DSN (Deep-Space Network) 34-meter antenna clusters.Table 1.1 summarizes the top-level details of each subsystem that was incorporated into the design. Cost estimates of the ALIVE mission show it at approximately 760M which puts it into the New Frontiers class.The ALIVE landed duration is only limited by the amount of Li which can be carried by the lander. Further studies are needed to investigate how additional mass can be carried, perhaps by a larger launcher and larger aeroshell

    Effects of eight neuropsychiatric copy number variants on human brain structure

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    Cuidados biomédicos de saúde em Angola e na Companhia de Diamantes de Angola, c. 1910-1970

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    Pretende-se caracterizar a prestação de cuidados biomédicos em Angola durante a atividade da Companhia de Diamantes de Angola. Uma análise comparativa de políticas e práticas de saúde pública de vários atores coloniais, como os serviços de saúde da Companhia, sua congénere do Estado e outras empresas coloniais, revelará diferenças de investimento na saúde, isto é, instalações e pessoal de saúde, e tratamentos. Este escrutínio bem como as condições de vida iluminarão o carácter idiossincrático e central dos serviços de saúde da Companhia em termos de morbimortalidade em Angola, e a centralidade destes para as representações de um império cuidador

    Effects of eight neuropsychiatric copy number variants on human brain structure

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    peer reviewedMany copy number variants (CNVs) confer risk for the same range of neurodevelopmental symptoms and psychiatric conditions including autism and schizophrenia. Yet, to date neuroimaging studies have typically been carried out one mutation at a time, showing that CNVs have large effects on brain anatomy. Here, we aimed to characterize and quantify the distinct brain morphometry effects and latent dimensions across 8 neuropsychiatric CNVs. We analyzed T1-weighted MRI data from clinically and non-clinically ascertained CNV carriers (deletion/duplication) at the 1q21.1 (n = 39/28), 16p11.2 (n = 87/78), 22q11.2 (n = 75/30), and 15q11.2 (n = 72/76) loci as well as 1296 non-carriers (controls). Case-control contrasts of all examined genomic loci demonstrated effects on brain anatomy, with deletions and duplications showing mirror effects at the global and regional levels. Although CNVs mainly showed distinct brain patterns, principal component analysis (PCA) loaded subsets of CNVs on two latent brain dimensions, which explained 32 and 29% of the variance of the 8 Cohen’s d maps. The cingulate gyrus, insula, supplementary motor cortex, and cerebellum were identified by PCA and multi-view pattern learning as top regions contributing to latent dimension shared across subsets of CNVs. The large proportion of distinct CNV effects on brain morphology may explain the small neuroimaging effect sizes reported in polygenic psychiatric conditions. Nevertheless, latent gene brain morphology dimensions will help subgroup the rapidly expanding landscape of neuropsychiatric variants and dissect the heterogeneity of idiopathic conditions. © 2021, The Author(s)
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