Study of nuclear reactions relevant for astrophysics by Micro-AMS

Dissertação para obtenção do Grau de Doutor em Física

Disseny i aplicació del protocol d'instal·lació d'energia fotovoltaica en edificis aïllats de la xarxa elèctrica al PNAP

En el perímetre del parc es troben gran nombre d’edificacions amb mancances de subministrament elèctric per la gran dispersió de la població de la comarca. L’objectiu d’aquest estudi és desenvolupar un protocol per determinar la viabilitat de l’energia fotovoltaica en edificis aïllats i aplicar-la de forma pilot a dos edificis gestionats pels responsables del Parc Natural de l’Alt Pirineu: el Centre de Logística i Manteniment (CLM) i el Refugi del Fornet. Aquests han estat escollits per la seva representativitat com a edificis aïllats de la xarxa elèctrica convencional. S’ha elaborat una metodologia pròpia, el Protocol d’instal·lació d’energia fotovoltaica en edificis aïllats de la xarxa elèctrica. S’ha realitzat una anàlisi de sensibilitats del dimensionat fotovoltaic davant la modificació de diversos paràmetres rellevants. Això ha permès determinar les característiques òptimes de viabilitat per als dos edificis en estudi i el cost de la instal·lació fotovoltaica (17.183€ el CLM i 164.815 € el Refugi del Fornet). Els resultats obtinguts en els dos edificis pilot han mostrat el gran cost relatiu entre l’energia fotovoltaica i l’energia elèctrica produïda a partir de combustibles fòssils.

Plan de gestión de energías renovables en el Monasterio Sakya Tashi Ling del Garraf

En el presente estudio se han analizado las posibilidades de reducción del impacto ambiental que genera el consumo de energía en el Monasterio budista Sakya Tashi Ling del Parque del Garraf, mediante la mejora de la eficiencia energética de los edificios y la producción de la energía consumida a partir de fuentes de energía renovables. Se ha realizado un inventario exhaustivo de los flujos energéticos de entrada del Monasterio: electricidad y combustibles fósiles, y el análisis de estos datos ha permitido observar que la mayor parte del consumo energético del Monasterio tiene como uso final la iluminación. El consumo total de energía se ha cuantificado en 138 kWh/m2/año y la emisiones de CO2 en 177 kg CO2/m2/año. A partir de estos datos se ha estudiado la posibilidad de reducir el consumo y abastecer la demanda energética del Monasterio a través de fuentes de energía renovable como las placas solares fotovoltaicas o las calderas de biomasa. Para alcanzar este objetivo se han propuesto tres escenarios posibles con costes económicos y resultados muy distintos. A diferencia de los escenarios “Edificio Energía Plus” y “Edificio Energía 0”, el tercer escenario propuesto, que trataba de alcanzar el triple objetivo del Plan 20/20/20 (producir a partir de fuentes renovables el 20% de la energía consumida, aumentar en una 20% la eficiencia energética y reducir en un 20% las emisiones de CO2 derivadas del uso de la energía) ha resultado ser muy viable económicamente: la inversión necesaria se amortizaría en tan sólo 5 años.

Estudi d’integració d’energia tèrmica i fotovoltaica a façana

L’objecte d’aquest projecte és realitzar un estudi d’un tipus instal·lacions molt específiques: l’energia solar fotovoltaica i l’energia solar tèrmica, destinada a la producció d’energia elèctrica i la producció d’ACS a un edifici plurifamiliar. Aplicar un cas concret a un edifici plurifamiliar, mitjançant d’integració dels panells fotovoltaics i tèrmics a la façana, i així, poder conformar la instal•lació d’energiasolar tèrmica per la producció d’aigua calenta sanitària i la instal·lació d’energia solar fotovoltaica. Comprovar si es possible complir CTE, mitjançant l’ integració arquitectònica dels panells a façana. Determinar el cost que suposa d’integració arquitectònica d’aquest panells, mitjançant el pressupost de la proposta a portada . Comparar el cost de la proposta, amb una façana tradicional més els panells solars tèrmics que exigeix el codi tècnic. Extreure conclusions al comparar les tipologies de façana a nivell econòmic i de rendibilitat

Projecte d’instal·lacions sostenibles d’una masia rural aïllada

En aquest projecte es vol donar solució a la contaminació que es produeix a les llars ja sigui en forma de gasos d’efecte hivernacle o la contaminació d’aqüífers i rius per les aigües residuals d’aquestes. Els objectius a aconseguir són la disminució del consum d’energia de la llar, reduint així el consum de combustibles fòssils, amb la conseqüent disminució de gasos d’efecte hivernacle i l’estalvi econòmic que això suposa. I per altra banda la depuració de les aigües residuals, tot i que actualment totes les grans poblacions de Catalunya de més de 10.000 habitants ja disposen de EDARS i en pocs anys en tindran totes les de més de 2000 habitants. Però en aquest cas es tracta d’una població molt petita que no disposa de xarxa de clavegueram. En primer lloc s’ha plantejat un sistema de calefacció d’energia geotèrmica que ens permet aprofitar l’energia tèrmica que es va emmagatzemant a la terra degut a l’escalfor del sol i que ens permet extreure d’aquesta fins a ¾ parts de l’energia tèrmica necessària per el sistema de calefacció. En segon lloc es planteja un sistema de producció d’energia elèctrica per panells fotovoltaics que produeixi el consum elèctric anual familiar, tot i que no de forma directe, sinó venent l’energia a la xarxa elèctrica i comprant-la després de la xarxa. Per últim es projecta un sistema de depuració d’aigües per mitjà d’un aiguamoll artificial que permetrà a la casa, que no disposa de xarxa de clavegueram, retornar les aigües residuals en bones mediambientals a l’entorn rural que envolta l’edificació, sense perjudicar la fauna i els rius que l’envolten

Autosuficiència energètica a la casa rural "Les Vinyes Grosses"

L’objectiu del present projecte és aconseguir l’autosuficiència energètica per a la casa rural “Les Vinyes Grosses”. Aquesta casa rural està situada a Sant Agustí de Lluçanès, comarca d’Osona. Es vol aconseguir fer una canvi de les instal·lacions que utilitzen energies no renovables a unes instal·lacions que funcionin amb energies renovables. Es pretén canviar la instal·lació de calefacció i aigua calenta que funciona amb gas-oil per una instal·lació que funcioni amb estella de pi roig que provingui de la mateixa finca. També es vol fer un canvi de la instal·lació elèctrica que funciona amb electricitat de la xarxa per una instal·lació elèctrica que utilitzi energia solar fotovoltàica. Per últim, es pretén que tota l’aigua consumida en la casa rural sigui aigua de la pluja en comptes d’utilitzar l’aigua de la xarxa. El cost total calculat per a realitzar aquests canvis d’instal·lacions és de 58.825 €, amb un temps d’amortització de 15,32 anys.

Investigation of defect formation and electronic transport in microcrystalline silicon deposited by hot-wire CVD

We have investigated doped and undoped layers of microcrystalline silicon prepared by hot-wire chemical vapour deposition optically, electrically and by means of transmission electron microscopy. Besides needle-like crystals grown perpendicular to the substrate's surface, all of the layers contained a noncrystalline phase with a volume fraction between 4% and 25%. A high oxygen content of several per cent in the porous phase was detected by electron energy loss spectrometry. Deep-level transient spectroscopy of the crystals suggests that the concentration of electrically active defects is less than 1% of the undoped background concentration of typically 10^17 cm -3. Frequency-dependent measurements of the conductance and capacitance perpendicular to the substrate surface showed that a hopping process takes place within the noncrystalline phase parallel to the conduction in the crystals. The parasitic contribution to the electrical circuit arising from the porous phase is believed to be an important loss mechanism in the output of a pin-structured photovoltaic solar cell deposited by hot-wire CVD.

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.

Causes and Effects of Chaos

Most of the recent literature on chaos and nonlinear dynamics is written either for popular science magazine readers or for advanced mathematicians. This paper gives a broad introduction to this interesting and rapidly growing field at a level that is between the two. The graphical and analytical tools used in the literature are explained and demonstrated, the rudiments of the current theory are outlined and that theory is discussed in the context of several examples: an electronic circuit, a chemical reaction and a system of satellites in the solar system.

Exploiting the Parallelism Exposed by Partial Evaluation

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.