Tungsten isotope evidence from similar to 3.8-Gyr metamorphosed sediments for early meteorite bombardment of the Earth

The 'Late Heavy Bombardment' was a phase in the impact history of the Moon that occurred 3.8-4.0 Gyr ago, when the lunar basins with known dates were formed(1,2). But no record of this event has yet been reported from the few surviving rocks of this age on the Earth. Here we report tungsten isotope anomalies, based on the Hf-182-W-182 system (half-life of 9 Myr), in metamorphosed sedimentary rocks from the 3.7-3.8-Gyr-old Isua greenstone belt of West Greenland and closely related rocks from northern Labrador, Canada. As it is difficult to conceive of a mechanism by which tungsten isotope heterogeneities could have been preserved in the Earth's dynamic crust-mantle environment from a time when short-lived Hf-182 was still present, we conclude that the metamorphosed sediments contain a component derived from meteorites.

New W-isotope evidence for rapid terrestrial accretion and very early core formation

The short-lived Hf-182-W-182-isotope system is an ideal clock to trace core formation and accretion processes of planets. Planetary accretion and metal/silicate fractionation chronologies are calculated relative to the chondritic Hf-182-W-182-isotope evolution. Here, we report new high-precision W-isotope data for the carbonaceous chondrite Allende that are much less radiogenic than previously reported and are in good agreement with published internal Hf-W chronometry of enstatite chondrites. If the W-isotope composition of terrestrial rocks, representing the bulk silicate Earth, is homogeneous and 2.24 epsilon(182W) units more radiogenic than that of the bulk Earth, metal/silicate differentiation of the Earth occurred very early. The new W-isotope data constrain the mean time of terrestrial core formation to 34 million years after the start of solar system accretion. Early terrestrial core formation implies rapid terrestrial accretion, thus permitting formation of the Moon by giant impact while Hf-182 was still alive. This could explain why lunar W-isotopes are more radiogenic than the terrestrial value. Copyright (C) 2002 Elsevier Science Ltd.

Estudo comparativo de sistemas em aquecimento

Trabalho Final de Mestrado para obtenção do grau de Mestre em Engenharia Mecânica

Prática de ensino supervisionado no 1.º e 2.º ciclo do ensino básico: de que modo o recurso às tecnologias de comunicação e de informação altera as conceções alternativas acerca dos astros em alunos do 1.ª ciclo do ensino básico

Relatório apresentado à Escola Superior de Educação de Lisboa para obtenção do grau de mestre em Ensino do 1.º e do 2.º Ciclo do Ensino Básico

Estudo e análise das centrais híbridas de energias renováveis

Com o aumento do preço da eletricidade e o fim dos combustíveis fósseis, associados à necessidade de Portugal reduzir a sua dependência energética do exterior, provoca a necessidade urgente de apostar nas energias renováveis. Perante este cenário, e assumindo que o custo da fatura energética, é para as empresas portuguesas um fator cada vez mais determinante para serem competitivas, devido aos aumentos consecutivos da energia nos últimos anos, bem como, a subida do imposto de valor acrescentado (IVA) de 6% para 23%. Outro aspeto importante é a eficiência energética como instrumento para reduzir os consumos de eletricidade. Com estas duas medidas: utilização de energias renováveis e o aumento da eficiência energética, são extremamente importantes para a redução da produção dos gases de efeito estufa (GEE). Consequentemente, as empresas terão de investir na produção da própria energia a partir de fontes renováveis, de modo a proporcionar um desenvolvimento sustentável, associado à redução da fatura energética. Esta dissertação propõe o dimensionamento de um sistema híbrido composto por tecnologia fotovoltaica e eólica, com e sem armazenamento de energia em baterias, adequado para reduzir uma parte dos consumos de uma empresa enquadrada no sector dos plásticos. O dimensionamento deste sistema, foi efetuado com recurso à caracterização dos consumos da empresa através da recolha de dados e leituras no local da instalação. Paralelamente, foi efetuada uma pesquisa em diversos fabricantes, de modo a identificar qual o sistema mais indicado a adotar, considerando painéis fotovoltaicos, turbinas eólicas, inversores e baterias. Com base nos dados recolhidos na empresa e referentes ao potencial eólico e solar para o distrito do Porto, em conjunto com as características técnicas dos equipamentos selecionados, foi delineado o sistema híbrido utilizando para o efeito um software de simulação e otimização de sistemas híbridos, denominado Hybrid Optimization Model for Eletric Renewable (HOMER). São apresentadas várias simulações para as diversas configurações escolhidas e estudos comparativos entre si, com o objetivo de reduzir o consumo de eletricidade da rede. Adicionalmente, foram realizadas duas configurações apenas com tecnologia fotovoltaica, de modo a efetuar uma análise comparativa entre um sistema híbrido e outro apenas com uma fonte renovável. Os resultados apresentados focaram-se no desempenho diário, mensal e anual, bem como, a produção individual de cada tecnologia evidenciada. Por último, procedeu-se ao estudo da viabilidade técnico-económica das configurações.

Planning, operations and data handling of planetary science missions

Dissertação para obtenção do Grau de Mestre em Engenharia Física

Study of nuclear reactions relevant for astrophysics by Micro-AMS

Dissertação para obtenção do Grau de Doutor em Física

Sistemas solares e arquitetura: uma relação holística

Dissertação de mestrado integrado em Arquitectura

Seguidor do ponto de máxima potência multi-conversor para sistemas solares fotovoltaicos

Dissertação de mestrado integrado em Engenharia Eletrónica Industrial e de Computadores

Comission 49: Interplanetary plasma and heliosphere. TRIENNIAL REPORT 2006 - 2009

Commission 49 covers research on the solar wind, shocks and particle acceleration, both transient and steady-state, e.g., corotating, structures within the heliosphere, and the termination shock and boundary of the heliosphere. The present triennal report is particularly rich in important results and events. The crossing of the solar wind termination shock by Voyager 2 in 2007 is a highlight and a milestone that will certainly have important consequences for astrophysical processes in general (Section 7). The fiftieth anniversary of the International Geophysical Year (19571958), which is also the fiftieth anniversary of the birth of the Space Age, was marked not only by celebrations and a strong Education and Public Outreach Program, but also by efforts in coordinating present observations and in starting new scientific programs, particularly implying developing countries (Section 8). Studies of solar energetic particles (Section 3) and the related radio bursts (Section 4) benefited from new data from a number of spacecraft. The STEREO mission was launched in October 2006 and has obtained new results on 3-D aspects of the inner heliosphere. Meanwhile, solar cycle 24 is expected to become active soon, following what is already the deepest solar minimum of the space age...

Small and Large Scale Dynamics in the Milky Way

This thesis contains dynamical analysis on four different scales: the Solar system, the Sun itself, the Solar neighbourhood, and the central region of the Milky Way galaxy. All of these topics have been handled through methods of potential theory and statistics. The central topic of the thesis is the orbits of stars in the Milky Way. An introduction into the general structure of the Milky Way is presented, with an emphasis on the evolution of the observed value for the scale-length of the Milky Way disc and the observations of two separate bars in the Milky Way. The basics of potential theory are also presented, as well as a developed potential model for the Milky Way. An implementation of the backwards restricted integration method is shown, rounding off the basic principles used in the dynamical studies of this thesis. The thesis looks at the orbit of the Sun, and its impact on the Oort cloud comets (Paper IV), showing that there is a clear link between these two dynamical systems. The statistical atypicalness of the orbit of the Sun is questioned (Paper I), concluding that there is some statistical typicalness to the orbit of the Sun, although it is not very significant. This does depend slightly on whether one includes a bar, or not, as a bar has a clear effect on the dynamical features seen in the Solar neighbourhood (Paper III). This method can be used to find the possible properties of a bar. Finally, we look at the effect of a bar on a statistical system in the Milky Way, seeing that there are not only interesting effects depending on the mass and size of the bar, but also how bars can capture disc stars (Paper II).

Maalämpöpumpun ja aurinkosähköjärjestelmän yhteiskäyttö pientalon lämpimän käyttöveden tuotannossa

Tässä kandidaatintyössä tutkitaan maalämpöpumpun ja aurinkosähköjärjestelmän yhteis-käyttöä pientalon lämpimän käyttöveden tuotannossa. Tarkoituksena on tuottaa päivittäin tarvittava lämmin käyttövesi maalämpöpumpulla, jonka tarvitsema sähkö tuotetaan aurin-kosähköjärjestelmän avulla keskimäärin kello 12–15. Aurinkosähköjärjestelmän tuotto simuloidaan kuvitteelliselle Lappeenrannassa sijaitsevalle omakotitalolle Homer-ohjelmistolla. Maalämpöpumpun koko pidetään vakiona ja vertai-lussa on 4, 5 ja 6 kW:n kokoiset aurinkosähköjärjestelmät. Yli 5 kW:n aurinkosähköjärjestelmällä saadaan katettua talon peruskuorman lisäksi, myös maalämpöpumpun tarvitsema teho kyseisenä ajanjaksona. 4 kW:n aurinkosähköjärjestel-mällä ja maalämpöpumpulla saadaan tuotettua päivässä riittävästi energiaa neljän henkilön tarvitsemaan käyttöveteen, mutta tällöin maalämpöpumppua täytyy käyttää pidempi ajan-jakso, jos lämmitykseen halutaan käyttää vain tuotettua aurinkosähköä.

Modelling of Ultraviolet and Vissible Emissions in Comets

Comets are the spectacular objects in the night sky since the dawn of mankind. Due to their giant apparitions and enigmatic behavior, followed by coincidental calamities, they were termed as notorious and called as `bad omens'. With a systematic study of these objects modern scienti c community understood that these objects are part of our solar system. Comets are believed to be remnant bodies of at the end of evolution of solar system and possess the material of solar nebula. Hence, these are considered as most pristine objects which can provide the information about the conditions of solar nebula. These are small bodies of our solar system, with a typical size of about a kilometer to a few tens of kilometers orbiting the Sun in highly elliptical orbits. The solid body of a comet is nucleus which is a conglomerated mixture of water ice, dust and some other gases. When the cometary nucleus advances towards the Sun in its orbit the ices sublimates and produces the gaseous envelope around the nucleus which is called coma. The gravity of cometary nucleus is very small and hence can not in uence the motion of gases in the cometary coma. Though the cometary nucleus is a few kilometers in size they can produce a transient, extensive, and expanding atmosphere with size several orders of magnitude larger in space. By ejecting gas and dust into space comets became the most active members of the solar system. The solar radiation and the solar wind in uences the motion of dust and ions and produces dust and ion tails, respectively. Comets have been observed in di erent spectral regions from rocket, ground and space borne optical instruments. The observed emission intensities are used to quantify the chemical abundances of di erent species in the comets. The study of various physical and chemical processes that govern these emissions is essential before estimating chemical abundances in the coma. Cameron band emission of CO molecule has been used to derive CO2 abundance in the comets based on the assumption that photodissociation of CO2 mainly produces these emissions. Similarly, the atomic oxygen visible emissions have been used to probe H2O in the cometary coma. The observed green ([OI] 5577 A) to red-doublet emission ([OI] 6300 and 6364 A) ratio has been used to con rm H2O as the parent species of these emissions. In this thesis a model is developed to understand the photochemistry of these emissions and applied to several comets. The model calculated emission intensities are compared with the observations done by space borne instruments like International Ultraviolet Explorer (IUE) and Hubble Space Telescope (HST) and also by various ground based telescopes.

Achieving Real-Time Mode Estimation through Offline Compilation

As exploration of our solar system and outerspace move into the future, spacecraft are being developed to venture on increasingly challenging missions with bold objectives. The spacecraft tasked with completing these missions are becoming progressively more complex. This increases the potential for mission failure due to hardware malfunctions and unexpected spacecraft behavior. A solution to this problem lies in the development of an advanced fault management system. Fault management enables spacecraft to respond to failures and take repair actions so that it may continue its mission. The two main approaches developed for spacecraft fault management have been rule-based and model-based systems. Rules map sensor information to system behaviors, thus achieving fast response times, and making the actions of the fault management system explicit. These rules are developed by having a human reason through the interactions between spacecraft components. This process is limited by the number of interactions a human can reason about correctly. In the model-based approach, the human provides component models, and the fault management system reasons automatically about system wide interactions and complex fault combinations. This approach improves correctness, and makes explicit the underlying system models, whereas these are implicit in the rule-based approach. We propose a fault detection engine, Compiled Mode Estimation (CME) that unifies the strengths of the rule-based and model-based approaches. CME uses a compiled model to determine spacecraft behavior more accurately. Reasoning related to fault detection is compiled in an off-line process into a set of concurrent, localized diagnostic rules. These are then combined on-line along with sensor information to reconstruct the diagnosis of the system. These rules enable a human to inspect the diagnostic consequences of CME. Additionally, CME is capable of reasoning through component interactions automatically and still provide fast and correct responses. The implementation of this engine has been tested against the NEAR spacecraft advanced rule-based system, resulting in detection of failures beyond that of the rules. This evolution in fault detection will enable future missions to explore the furthest reaches of the solar system without the burden of human intervention to repair failed components.

Learning-Based Approach to Estimation of Morphable Model Parameters

We describe the key role played by partial evaluation in the Supercomputing Toolkit, a parallel computing system for scientific applications that effectively exploits the vast amount of parallelism exposed by partial evaluation. The Supercomputing Toolkit parallel processor and its associated partial evaluation-based compiler have been used extensively by scientists at MIT, and have made possible recent results in astrophysics showing that the motion of the planets in our solar system is chaotically unstable.