209 resultados para Explosions


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Estudi elaborat a partir d’una estada a l'Institut de Physique Nucléaire d'Orsay (França), entre els mesos de setembre a novembre del 2005, col·laborant amb el Profesor Jérôme Margueron. La motivació d'aquest estudi sorgeix en el marc de les explosions de supernoves del tipus II. A l'interior d'aquestes supernoves s'hi formen protoestels de neutrons composats d'una matèria densa d'hadrons en interacció amb una quantitat ingent de neutrins. El temps d'escapament d'aquests neutrins és important per evaluar llur influència en l'ona de xoc que, a l'exterior del protoestel, intenta escapar del col∙lapse gravitatori i fer esclatar la supernova. En aquest intent de modelitzar l'interior dels protoestels de neutrons, s’ha tractat una matèria hadrònica composada per nucleons (neutrons i protons) i lambdes, deixant per a estudis futurs la influència de la resta d'hiperons ja que la sola presència de les lambdes altera significativament la resposta del medi en front de pertorbacions externes. Com a resultat de l’estudi s’ha obtingut, doncs, el camí lliure mig dels neutrins en la matèria hadrònica.

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La vulnerabilitat dels vells edificis històrics de maçoneria, a causa del dany desproporcionat fora del plànol de càrrega (causat pel vent, explosions, inundacions o moviments sísmics és un dels greus problemes que enfronten avui dia els enginyers estructurals En l'actualitat s'han desenvolupat diverses tècniques innovadores de rehabilitació d'edificis històrics. L'eficàcia de moltes d'elles ha estat provada tant en laboratoris o sota condicions de càrrega real, tals com moviments sísmics. La qualitat i tipus dels materials de maçoneria i el disseny estructural són criteris fonamentals en l'elecció del mètode de reforç. En aques document es presenten les tècniques més utilitzades en la rehabilitació tradicional i les tècniques modernes i innovadores de rehabilitació utilitzant composites avançats

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To start off, this document describes the Catalan model for emergencies response and its reference frame in terms of geography, location population…In addition, describes the main actors involved in emergencies response such as: police, the Fire and Rescue Emergency Service, the Emergency Medical System, Civil Protection, Reception and Management of Emergency Calls, Rural Agents, ADF’s and UME. Civil Protection, Firefighters and Police are includes in the training model developed by the Institute for Public Safety of Catalonia which at the same time does research in both security and safety matters. Research activities are performed by the Area for Research, Knowledge and International Cooperation at the ISPC and an example of these activities are European Research Projects such as COIM-Best (Coordination Improvement by Best Practices) and BESECU (cross-cultural differences of human behaviour in fire disasters and other crisis situations) among others.

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Les actuacions de bombers en operatius d'extinció d'incendis, habitualment es fan per inèrcies històriques. Ara, si diem: “Per a l'extinció d'un incendi de un vehicle heu d'estacionar l’autobomba a una certa distància, pendent amunt i a contravent, refrigerar a distància el vehicle amb con d'atac, i evitar els extrems del vehicle”, segurament més d'un pensarà o expressarà en veu alta “Això deu ser una broma, oi? Si hem estat apagant cotxes cada dia a la nostra manera… quin és el problema?". Bé, doncs n’hi ha uns quants, de problemes. Podem considerar un incendi en un vehicle com una bomba de temps amb un ble que s'encén abans de l'arribada de la dotació de bombers. Les actuacions inicials en aquests incendis han de centrar-se en la desactivació d'aquesta metxa. Els incendis en vehicles presenten una múltiple varietat perills reals. Els canvis en el disseny i la construcció d'automòbils exigeixen un canvi en la manera com els serveis de bombers s’enfronten als incendis de vehicles. Els nous materials i components incorporats a la indústria automobilística s'han traduït en un millor rendiment, una major economia de combustible, una millor resistència al xoc i en una reducció de les emissions de gasos. Malauradament, alguns d'aquests mateixos materials i components fan que l’extinció d’un automòbil modern sigui més difícil i perillosa que en vehicles més vells. En l’actualitat, un incendi d’un vehicle comporta més fums, més toxicitat, més temperatura, elements sotmesos a pressió, risc de projecció d’elements i la possibilitat d’energies alternatives... en definitiva, molts més riscos. Per donar una resposta adequada a aquest augment del risc, organitzativament cal augmentar les mesures preventives de seguretat, i operativament cal una estratègia d’extinció més cautelosa, tàctiques menys agressives i un major nivell de protecció personal.

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After a rockfall event, a usual post event survey includes qualitative volume estimation, trajectory mapping and determination of departing zones. However, quantitative measurements are not usually made. Additional relevant quantitative information could be useful in determining the spatial occurrence of rockfall events and help us in quantifying their size. Seismic measurements could be suitable for detection purposes since they are non invasive methods and are relatively inexpensive. Moreover, seismic techniques could provide important information on rockfall size and location of impacts. On 14 February 2007 the Avalanche Group of the University of Barcelona obtained the seismic data generated by an artificially triggered rockfall event at the Montserrat massif (near Barcelona, Spain) carried out in order to purge a slope. Two 3 component seismic stations were deployed in the area about 200 m from the explosion point that triggered the rockfall. Seismic signals and video images were simultaneously obtained. The initial volume of the rockfall was estimated to be 75 m3 by laser scanner data analysis. After the explosion, dozens of boulders ranging from 10¿4 to 5 m3 in volume impacted on the ground at different locations. The blocks fell down onto a terrace, 120 m below the release zone. The impact generated a small continuous mass movement composed of a mixture of rocks, sand and dust that ran down the slope and impacted on the road 60 m below. Time, time-frequency evolution and particle motion analysis of the seismic records and seismic energy estimation were performed. The results are as follows: 1 ¿ A rockfall event generates seismic signals with specific characteristics in the time domain; 2 ¿ the seismic signals generated by the mass movement show a time-frequency evolution different from that of other seismogenic sources (e.g. earthquakes, explosions or a single rock impact). This feature could be used for detection purposes; 3 ¿ particle motion plot analysis shows that the procedure to locate the rock impact using two stations is feasible; 4 ¿ The feasibility and validity of seismic methods for the detection of rockfall events, their localization and size determination are comfirmed.

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Propane can be responsible for several types of lethal intoxication and explosions. Quantifying it would be very helpful to determine in some cases the cause of death. Some gas chromatography-mass spectrometry (GC-MS) methods of propane measurements do already exist. The main drawback of these GC-MS methods described in the literature is the absence of a specific propane internal standard necessary for accurate quantitative analysis. The main outcome of the following study was to provide an innovative Headspace-GC-MS method (HS-GC-MS) applicable to the routine determination of propane concentration in forensic toxicology laboratories. To date, no stable isotope of propane is commercially available. The development of an in situ generation of standards is thus presented. An internal-labeled standard gas (C3DH7) is generated in situ by the stoichiometric formation of propane by the reaction of deuterated water (D2O) with Grignard reagent propylmagnesium chloride (C3H7MgCl). The method aims to use this internal standard to quantify propane concentrations and, therefore, to obtain precise measurements. Consequently, a complete validation with an accuracy profile according to two different guidelines, the French Society of Pharmaceutical Sciences and Techniques (SFSTP) and the Gesellschaft für toxikologische und Forensische Chemie (GTFCh), is presented.

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Työn tavoitteena oli kehittää Kaukaan sellutehtaalle luotettava vesi-höyrypiirin vuodonvalvontajärjestelmä. Vesi-höyrypiirin vuodonvalvontajärjestelmällä pystytään ehkäisemään soodakattilassa mahdollisen putkivaurion aiheuttama sulavesiräjähdys. Työn teoreettisessa osassa käsitellään soodakattilan turvallisuutta sekätutustutaan kaupallisilla markkinoilla oleviin vuodonvalvontajärjestelmiin. Vuodonvalvontajärjestelmän kehityksessä käytetään hyväksi prosessitietoa noin vuoden ajalta sekä yhden vakavan vesi-höyrypiirin putkirikon aikaisia mittaustietoja.Työssä testataan käytännössä Kaukaan soodakattilaan rakennettu järjestelmä. Työn tuloksena Kaukaan sellutehtaan soodakattilan on rakennettu vuodonvalvontajärjestelmä, joka havaitsee vesi-höyrypiirin putkirikon aiheuttaman vuodon, määrittää sen suuruuden sekä pystyy paikantamaan vuodon sijainnin.

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An accidental burst of a pressure vessel is an uncontrollable and explosion-like batch process. In this study it is called an explosion. The destructive effectof a pressure vessel explosion is relative to the amount of energy released in it. However, in the field of pressure vessel safety, a mutual understanding concerning the definition of explosion energy has not yet been achieved. In this study the definition of isentropic exergy is presented. Isentropic exergy is the greatest possible destructive energy which can be obtained from a pressure vessel explosion when its state changes in an isentropic way from the initial to the final state. Finally, after the change process, the gas has similar pressure and flow velocity as the environment. Isentropic exergy differs from common exergy inthat the process is assumed to be isentropic and the final gas temperature usually differs from the ambient temperature. The explosion process is so fast that there is no time for the significant heat exchange needed for the common exergy.Therefore an explosion is better characterized by isentropic exergy. Isentropicexergy is a characteristic of a pressure vessel and it is simple to calculate. Isentropic exergy can be defined also for any thermodynamic system, such as the shock wave system developing around an exploding pressure vessel. At the beginning of the explosion process the shock wave system has the same isentropic exergyas the pressure vessel. When the system expands to the environment, its isentropic exergy decreases because of the increase of entropy in the shock wave. The shock wave system contains the pressure vessel gas and a growing amount of ambient gas. The destructive effect of the shock wave on the ambient structures decreases when its distance from the starting point increases. This arises firstly from the fact that the shock wave system is distributed to a larger space. Secondly, the increase of entropy in the shock waves reduces the amount of isentropic exergy. Equations concerning the change of isentropic exergy in shock waves are derived. By means of isentropic exergy and the known flow theories, equations illustrating the pressure of the shock wave as a function of distance are derived. Amethod is proposed as an application of the equations. The method is applicablefor all shapes of pressure vessels in general use, such as spheres, cylinders and tubes. The results of this method are compared to measurements made by various researchers and to accident reports on pressure vessel explosions. The test measurements are found to be analogous with the proposed method and the findings in the accident reports are not controversial to it.

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Kandidaatintyön johdantokappaleessa esitellään vetyperoksidi ja mihin sitä käytetään teollisuudessa. Työssä vertaillaan antrakinoniprosessia ja suoraa prosessia sekä selvitetään nykyisin enemmän vetyperoksidituotantoon käytetyn antrakinoniprosessin ongelmakohdat ja osoitetaan, miksi suora synteesi vetyperoksidin tuotannossa olisi parempi vaihtoehto. Kandidaatintyön käsittelee suurilta osin turvallisuusongelmia, joita esiintyy suoran synteesin yhteydessä. Kirjallisuudesta on etsitty ratkaisuja näihin ongelmiin, kuten membraaniprosessin käyttöä räjähdysvaaran välttämiseksi. Pienemmän reaktorin eli ns. mikroreaktorin käyttö tuo mukanaan monia etuja vetyperoksidin tuotantoon. Tällöin prosessi on turvallisempi ja sitä on helpompi hallita. Mikroreaktorissa voidaan käyttää korkeampia lämpötiloja ja paineita kuin makroreaktorilla ilman, että räjähdysvaara prosessissa kasvaisi. Mikroreaktorin sisällä olevat mikrokanavat luovat turvallisen ympäristön synteesille. Aspen plus – simulointiohjelmalla mallinnettiin ja simulointiin suoran prosessin kriittisiä virtoja mikroreaktorissa. Tarkoituksena oli löytää virrat, joissa kulkee mahdollisesti räjähtävä kaasuseos. Kaasumaiset prosessivirrat ovat kriittisimmät vetyperoksidin suorassa synteesissä, koska ne aiheuttavat todennäköisemmin räjähdyksen kuin nestemäiset prosessivirrat. Kaikkein eniten prosessiturvallisuutta uhkaavat ainevirrat ennen ja jälkeen mikroreaktoria.

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This essay reviews the decision-making process that led to India exploding a nuclear device in May, 1974. An examination of the Analytic, Cybernetic and Cognitive Theories of decision, will enable a greater understanding of the events that led up to the 1974 test. While each theory is seen to be only partially useful, it is only by synthesising the three theories that a comprehensive account of the 1974 test can be given. To achieve this analysis, literature on decision-making in national security issues is reviewed, as well as the domestic and international environment in which involved decisionmakers operated. Finally, the rationale for the test in 1974 is examined. The conclusion revealed is that the explosion of a nuclear device by India in 1974 was primarily related to improving Indian international prestige among Third World countries and uniting a rapidly disintegrating Indian societal consensus. In themselves, individual decision-making theories were found to be of little use, but a combination of the various elements allowed a greater comprehension of the events leading up to the test than might otherwise have been the case.

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La Ciencia Política siempre ha buscado profundizar en el fenómeno del poder y sus causas. Las teorías han cambiado conforme a las circunstancias sociales a lo largo de la historia; no obstante, en la actualidad las dinámicas de comunicación facilitadas por elementos tecnológicos han generado coyunturas sin antecedentes como la ocurrida en Colombia el 4 de febrero de 2008 “Un Millón de voces contra las FARC” La generalización en el uso de Internet y –sobre todo- las redes sociales ha producido un acelerado nivel de activismo debido a la facilidad de cooperación y coordinación que se deriva de estructuras en red. Es sano pensar en una reevaluación de la teoría tradicional del poder vertical y traer al campo teórico nuevos elementos que generen herramientas de análisis sobre comunicación, poder horizontal, activismo y oportunidades políticas. El nacimiento de lo que algunos llaman “sociedad informacional” es lo que permitirá describir el concepto de “noopolitik”. Las que otrora eran movilizaciones políticas costosas y exigentes en recursos de coordinación y tiempo han venido siendo reemplazadas por explosiones de activismo catalizadas por un sentimiento común que han sabido servirse de las ventajas tecnológicas para lograr sus objetivos. Bien habla de ello el caso de estudio de esta investigación al ser la movilización más grande registrada, con más de 12 millones de personas alrededor del mundo y con el uso protagónico de redes sociales. El valor de la información –y por supuesto su difusión-, es ahora uno de los principales asuntos de la Ciencia Política moderna.

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Solar electromagnetic radiation powers Earth’s climate system and, consequently, it is often naively assumed that changes in this solar output must be responsible for changes in Earth’s climate. However, the Sun is close to a blackbody radiator and so emits according to its surface temperature and the huge thermal time constant of the outer part of the Sun limits the variability in surface temperature and hence output. As a result, on all timescales of interest, changes in total power output are limited to small changes in effective surface temperature (associated with magnetic fields) and potential, although as yet undetected, solar radius variations. Larger variations are seen in the UV part of the spectrum which is emitted from the lower solar atmosphere (the chromosphere) and which influences Earth’s stratosphere. There is interest in“top-down” mechanisms whereby solar UV irradiance modulates stratospheric temperatures and winds which, in turn, may influence the underlying troposphere where Earth’s climate and weather reside. This contrasts with “bottom-up” effects in which the small total solar irradiance (dominated by the visible and near-IR) variations cause surface temperature changes which drive atmospheric circulations. In addition to these electromagnetic outputs, the Sun modulates energetic particle fluxes incident on the Earth. Solar Energetic Particles (SEP) are emitted by solar flares and from the shock fronts ahead of supersonic (and super-Alfvenic) ejections of material from the solar atmosphere. These SEPs enhance the destruction of polar stratospheric ozone which could be an additional form of top-down climate forcing. Even more energetic are Galactic Cosmic Rays (GCRs). These particles are not generated by the Sun, rather they originate at the shock fronts emanating from violent galactic events such as supernovae explosions; however, the expansion of the solar magnetic field into interplanetary space means that the Sun modulates the number of GCRs reaching Earth. These play a key role in enabling Earth’s global electric (thunderstorm) circuit and it has been proposed that they also modulate the formation of clouds. Both electromagnetic and corpuscular solar effects are known to vary over the solar magnetic cycle which is typically between 10 and 14 yrs in length (with an average close to 11 yrs). The solar magnetic field polarity at any one phase of one of these activity cycles is opposite to that at the same phase of the next cycle and this influences some phenomena, for example GCRs, which therefore show a 22 yr (“Hale”) cycle on average. Other phenomena, such as irradiance modulation, do not depend on the polarity of the magnetic field and so show only the basic 11-yr activity cycle. However, any effects on climate are much more significant for solar drifts over centennial timescales. This chapter discusses and evaluates potential effects on Earth’s climate system of variations in these solar inputs. Because of the great variety of proposed mechanisms, the wide range of timescales studied (from days to millennia) and the many debates (often triggered by the application of inadequate statistical methods), the literature on this subject is vast, complex, divergent and rapidly changing: consequently the number of references cited in this review is very large (yet still only a small fraction of the total).

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Lava dome eruptions are sometimes characterised by large periodic fluctuations in extrusion rate over periods of hours that may be accompanied by Vulcanian explosions and pyroclastic flows. We consider a simple system of nonlinear equations describing a 1D flow of lava extrusion through a deep elastic dyke feeding a shallower cylindrical conduit in order to simulate this short-period cyclicity. Stick-slip conditions depending on a critical shear stress are assumed at the wall boundary of the cylindrical conduit. By analogy with the behaviour of industrial polymers in a plastic extruder, the elastic dyke acts like a barrel and the shallower cylindrical portion of the conduit as a die for the flow of magma acting as a polymer. When we applied the model to the Soufrière Hills Volcano, Montserrat, for which the key parameters have been evaluated from previous studies, cyclic extrusions with periods from 3 to 30 h were readily simulated, matching observations. The model also reproduces the reduced period of cycles observed when a major unloading event occurs due to lava dome collapse.

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Using a time series of TerraSAR-X spaceborne radar images we have measured the pulsatory motion of an andesite lava flow over a 14-month period at Bagana volcano, Papua New Guinea. Between October 2010 and December 2011, lava flowed continuously down the western flank of the volcano forming a 3 km-long blocky lava flow with a channel, levees, overflows and branches. We captured four successive pulses of lava advancing down the channel system, the first such behaviour of an andesite flow to be recorded using radar. Each pulse had a volume of the order of 107 m3 emplaced over many weeks. The average extrusion rate estimated from the radar data was 0.92 ± 0.35 m3 s-1 , and varied between 0.3 and 1.8 m3 s-1, with higher rates occurring earlier in each pulse. This, together with observations of sulphur dioxide emissions, explosions and incandescence suggest a variable supply rate of magma through Bagana’s conduit as the most likely source of the pulsatory behaviour.