983 resultados para JPEG-LS


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By contrast to the Target Normal Sheath acceleration (TNSA) mechanism [1], Radiation Pressure Acceleration (RPA) is currently attracting a substantial amount of experimental [2,3] and theoretical [4-6] attention worldwide due to its superior scaling in terms of ion energy and laser-ion conversion efficiency. Employing Vulcan Petawatt lasers of the Rutherford Appleton Laboratory, UK, both the Hole-boring (HB) and the Light-Sail (LS) regimes of the RPA have been extensively explored. When the target thickness is of the order of hole-boring velocity times the laser pulse duration, highly collimated plasma jets of near solid density are ejected from the foil, lasting up to ns after the laser interaction. By changing the linear polarisation of the laser to circular, improved homogeneity in the jet's spatial density profile is achieved which suggests more uniform and sustained radiation pressure drive on target ions. By decreasing the target areal density or increasing irradiance on the target, the LS regime of the RPA is accessed where relatively high flux (~ 1012 particles/MeV/Sr) of ions are accelerated to ~ 10 MeV/nucleon energies in a narrow energy bandwidth. The ion energy scaling obtained from the parametric scans agrees well with theoretical estimation based on RPA mechanism and the narrow bandwidth feature in the ion spectra is studied by 2D particle-in-simulations.

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Trabalho Final de Mestrado para obtenção do grau de Mestre em Engenharia de Electrónica e telecomunicações

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Partial dynamic reconfiguration of FPGAs can be used to implement complex applications using the concept of virtual hardware. In this work we have used partial dynamic reconfiguration to implement a JPEG decoder with reduced area. The image decoding process was adapted to be implemented on the FPGA fabric using this technique. The architecture was tested in a low cost ZYNQ-7020 FPGA that supports dynamic reconfiguration. The results show that the proposed solution needs only 40% of the resources utilized by a static implementation. The performance of the dynamic solution is about 9X slower than the static solution by trading-off internal resources of the FPGA. A throughput of 7 images per second is achievable with the proposed partial dynamic reconfiguration solution.

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Mémoire numérisé par la Division de la gestion de documents et des archives de l'Université de Montréal

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Absolute cross sections for the transitions of the Kr atom into the 4s^1 and 4p^4nl states of the Kr^+ ion were measured in the 4s-electron threshold region by photon-induced fluorescence spectroscopy (PIFS). The cross sections for the transitions of the Kr atom into the 4s^1 and 4p^4nl states were also calculated, as well as the 4p^4nln'l' doubly excited states, in the frame of LS-coupling many-body technique. The cross sections of the doubly-excited atomic states were used to illustrate the pronounced contributions of the latter to the photoionization process, evident from the measurements. The comparison of theory and experiment led to conclusions about the origin of the main features observed in the experiment.

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Estudi i avaluació de les principals propietats del sòl i la dinàmica erosiva relacionades amb l’ús del sòl i l’abandó agrícola en diferents ambients de la península del Cap de Creus. Per dur a terme aquest estudi s’han seleccionat 7 ambients diferents representatius d’una seqüència d’usos fins l’abandó en diferents etapes de successió vegetal. Els ambients són diferenciats entre sòls cultivats (vinya i olivera), sòls forestals (sureda i pineda), pastures (prats) i matollars (Cistus monspeliensis i d’Erica arborea) respectivament cremat reiteradament i no cremat durant 25 anys. En cada ambient s’han instal.lat parcel.les d’erosió que permeten avaluar la producció de sediments i la mobilització de nutrients (carboni i nitrogen) durant els episodis de precipitació que generen escolament superficial

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We present Very Long Baseline Interferometry (VLBI) observations of the high mass X-ray binary LS I +61˚303, carried out with the European VLBI Network (EVN). Over the 11 hour observing run, performed ~10 days after a radio outburst, the radio source showed a constant flux density, which allowed sensitive imaging of the emission distribution. The structure in the map shows a clear extension to the southeast. Comparing our data with previous VLBI observations we interpret the extension as a collimated radio jet as found in several other X-ray binaries. Assuming that the structure is the result of an expansion that started at the onset of the outburst, we derive an apparent expansion velocity of 0:003 c, which, in the context of Doppler boosting, corresponds to an intrinsic velocity of at least 0:4 c for an ejection close to the line of sight. From the apparent velocity in all available epochs we are able to establish variations in the ejection angle which imply a precessing accretion disk. Finally we point out that LS I +61˚303, like SS 433 and Cygnus X-1, shows evidence for an emission region almost orthogonal to the relativistic jet

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Resumen basado en el de la autora en catalán

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Aquest article estudia el documental històric amb la intenció de confrontar alguna de les controvèrsies que han sorgit sobre la idea de la reconstrucció històrica en el camp del cinema i de la televisió. El primer punt plantejat consisteix en l’actualització de la idea proposada per Marc Ferro de que cada pel•lícula és un document de mentalitats, partint de dues idees bàsiques: primer, que el cinema, a més de ser un document, té una història com a producte artístic i segon, que la documentació del passat ha de dur-se a terme sense caure en el que Tzevan Todorov diu els abusos de la memòria. El segon punt té a veure amb el problema de com la història és modificada donada la percepció que tenim de ella des d’un punt particular al present. Finalment, entra en el tema de la ètica amb la intenció de fer front al problema de les limitacions de l’acte de mostrar en un moment històric particular en que aquesta mostra ha estat transformada en una forma de banalització

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Here we discuss two consecutive MERLIN observations of the X-ray binary LS I +61° 303 . The first observation shows a double-sided jet extending up to about 200 AU on both sides of a central source. The jet shows a bent S-shaped structure similar to the one displayed by the well-known precessing jet of SS 433 . The precession suggested in the first MERLIN image becomes evident in the second one, showing a one-sided bent jet significantly rotated with respect to the jet of the day before. We conclude that the derived precession of the relativistic (beta=0.6) jet explains puzzling previous VLBI results. Moreover, the fact that the precession is fast could be the explanation of the never understood short term (days) variability of the associated gamma-ray source 2CG 135+01 / 3EG J0241+6103

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Pràctiques d’hidrogeologia realitzades per Anna Menció i Domingo, dins aquesta assignatura que forma part del mòdul obligatori de Bases científiques del medi natural del segon curs del grau en Ciències Ambientals.