66 resultados para radio galaxy,spectral ageing,synchrotron radiation,AGN,radio emission
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Los autores presentan una clasificación más actual de las patologías del pie, basándose en tres aspectos: morfológico, funcional y degenerativo. Esta nueva clasificación entendemos que reemplazaría a las que se han venido utilizando hasta el momento las cuales a menudo no son útiles para los podólogos. Asimismo en este artículo se describe el proceso de aplicación del soporte funcional del primer radio, las características de los materiales utilizados en su confección y varios casos clínicos, de diferente etiología a los cuales se le ha aplicado este tipo de soporte.
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La posición del primer radio tanto desde el plano frontal como desde el plano sagital, es de vital importancia para la consecución de una correcta y adecuada marcha, así como para mantener la estructura anatómica del pie durante la bipedestación estática. La deformidad en flexión plantar del primer radio modifica estos parámetros creando mecanismos compensatorios que pueden afectar a otras unidades funcionales articulares, tanto del mediopié como del retropié, lo que puede dar lugar a un patrón de metatarsalgia de difícil valoración al tener que contemplar y analizar varios diagnósticos y sus respectivos patrones mecánicos: el equino de columna lateral, el retropié varo compensado y el primer radio plantarflexionado flexible. Se presenta un caso clínico para su análisis conjunto.
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Introducción: Las fracturas distales de radio (FDR) presentan diferentes resultadosfuncionales siendo desfavorables entre el 24% y el 31% de los casos. Una de lascomplicaciones más frecuentes es el síndrome del dolor regional complejo tipo I(SDRC-I), cuyo origen es desconocido. Sólo el 20-30% de los pacientes recuperarán sugrado de funcionalidad anterior.Objetivos: Estimar la prevalencia de SDRC-I tras una FDR de acuerdo a cuatro tipos detratamiento.Métodos: estudio de una serie de casos retrospectivos. La población de referencia hansido los 391 trabajadores afiliados a una Mutua en Cataluña y diagnosticados deFDR tras una lesión por accidente laboral durante lo años 2008-2010.Los casos han sido trabajadores accidentados que tras una FDR desarrollaron el SDRCI.Como variable dependiente se ha utilizado el diagnóstico de SDRC-I; como variablesindependientes el tipo de tratamiento, la edad, el sexo, la ocupación y el mecanismo dela lesión.Resultados: el 19,7% de la muestra ha desarrollado SDRC-I, siendo esta prevalenciasuperior en los pacientes intervenidos mediante la técnica de tracción bipolar o conagujas de Kirschner; 29,17% y 30,56% respectivamente, que para aquellos en los quese ha realizado un tratamiento conservador o una intervención quirúrgica con placa en Ty tornillos; 15,92% y 15,79%.Conclusiones El tratamiento conservador y la técnica quirúrgica de fijación con placaen T y tornillos han dado una menor prevalencia de SDRC-I.Los mecanismos de lesión asociados a una mayor fuerza presentan fracturas másinestables y requieren un tratamiento quirúrgico. Los tratamientos conservadores sonlos más usados en edades mayores relacionados con fracturas estables.A nivel clínico se extrae una recomendación profiláctica con Vitamina C para evitar laaparición de SDRC-I sobre los pacientes de edad comprendida entre los 36 y los 55años, con mecanismo lesional de caída o caída desde altura, intervenidos con agujas de Kirschner o tracción bipolar.
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The formation of silicon particles in rf glow discharges has attracted attention due to their effect as a contaminant during film deposition or etching. However, silicon and silicon alloy powders produced by plasma¿enhanced chemical vapor deposition (PECVD) are promising new materials for sintering ceramics, for making nanoscale filters, or for supporting catalytic surfaces. Common characteristics of these powders are their high purity and the easy control of their stoichiometry through the composition of the precursor gas mixture. Plasma parameters also influence their structure. Nanometric powders of silicon¿carbon alloys exhibiting microstructural properties such as large hydrogen content and high surface/volume ratio have been produced in a PECVD reactor using mixtures of silane and methane at low pressure (-1 Torr) and low frequency square¿wave modulated rf power (13.56 MHz). The a¿Si1¿xCx:H powders were obtained from different precursor gas mixtures, from R=0.05 to R=9, where R=[SiH4]/([SiH4]+[CH4]). The structure of the a¿Si1¿xCx:H powder was analyzed by several techniques. The particles appeared agglomerated, with a wide size distribution between 5 and 100 nm. The silane/methane gas mixture determined the vibrational features of these powders in the infrared. Silicon-hydrogen groups were present for every gas composition, whereas carbon¿hydrogen and silicon¿carbon bonds appeared in methane¿rich mixtures (R-0.6). The thermal desorption of hydrogen revealed two main evolutions at about 375 and 660¿°C that were ascribed to hydrogen bonded to silicon and carbon, respectively. The estimated hydrogen atom concentration in the sample was about 50%.
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Desde su nacimiento, la radio ha estado en constante peligro de desaparición. La prescripción y legitimidad asociadas a las ondas pueden resguardar a un servicio público en constante crisis. Las listas de reproducción o playlists son la base de la programación radiofónica musical y la posibilidad de acceder a las obras musicales tal y como “se oyen” es una opción que la radio en Internet ofrece. Este trabajo analiza cómo abordan los programas temáticos musicales de las emisoras de radio de antena convencional y bitcasters de titularidad pública en España la creación y publicación de listas de reproducción en Internet.
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Entrevista a Radio Nikosia
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Cognitive radio is a wireless technology aimed at improvingthe efficiency use of the radio-electric spectrum, thus facilitating a reductionin the load on the free frequency bands. Cognitive radio networkscan scan the spectrum and adapt their parameters to operate in the unoccupiedbands. To avoid interfering with licensed users operating on a givenchannel, the networks need to be highly sensitive, which is achieved byusing cooperative sensing methods. Current cooperative sensing methodsare not robust enough against occasional or continuous attacks. This articleoutlines a Group Fusion method that takes into account the behavior ofusers over the short and long term. On fusing the data, the method is basedon giving more weight to user groups that are more unanimous in their decisions.Simulations have been performed in a dynamic environment withinterferences. Results prove that when attackers are present (both reiterativeor sporadic), the proposed Group Fusion method has superior sensingcapability than other methods.
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Cognitive radio networks (CRN) sense spectrum occupancy and manage themselves to operate in unused bands without disturbing licensed users. The detection capability of a radio system can be enhanced if the sensing process is performed jointly by a group of nodes so that the effects of wireless fading and shadowing can be minimized. However, taking a collaborative approach poses new security threats to the system as nodes can report false sensing data to force a wrong decision. Providing security to the sensing process is also complex, as it usually involves introducing limitations to the CRN applications. The most common limitation is the need for a static trusted node that is able to authenticate and merge the reports of all CRN nodes. This paper overcomes this limitation by presenting a protocol that is suitable for fully distributed scenarios, where there is no static trusted node.
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Spectrum is an essential resource for the provision of mobile services. In order to control and delimit its use, governmental agencies set up regulatory policies. Unfortunately, such policies have led to a deficiency of spectrum as only few frequency bands are left unlicensed, and these are used for the majority of new emerging wireless applications. One promising way to alleviate the spectrum shortage problem is adopting a spectrum sharing paradigm in which frequency bands are used opportunistically. Cognitive radio is the key technology to enable this shift of paradigm.Cognitive radio networks are self-organized systems in which devices cooperate to use those spectrum ranges that are not occupied by licensed users. They carry out spectrum sensing in order to detect vacant channels that can be used for communication. Even though spectrum sensing is an active area of research, an important issue remains unsolved: the secure authentication of sensing reports. Not providing security enables the input of false data in the system thus empowering false results. This paper presents a distributed protocol based on wireless physical layer security, symmetric cryptography and one-way functions that allows determining a final sensing decision from multiple sources in a quick and secure way, as well as it preserves users¿ privacy.
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Spectrum scarcity demands thinking new ways tomanage the distribution of radio frequency bands so that its use is more effective. The emerging technology that can enable this paradigm shift is the cognitive radio. Different models fororganizing and managing cognitive radios have emerged, all with specific strategic purposes. In this article we review the allocation spectrum patterns of cognitive radio networks andanalyse which are the common basis of each model.We expose the vulnerabilities and open challenges that still threaten the adoptionand exploitation of cognitive radios for open civil networks.
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Cognitive radio networks sense spectrum occupancyand manage themselves to operate in unused bands without disturbing licensed users. Spectrum sensing is more accurate if jointly performed by several reliable nodes. Even though cooperative sensing is an active area of research, the secureauthentication of local sensing reports remains unsolved, thus empowering false results. This paper presents a distributed protocol based on digital signatures and hash functions, and ananalysis of its security features. The system allows determining a final sensing decision from multiple sources in a quick and secure way.
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The atmospheric Cherenkov gamma-ray telescope MAGIC, designed for a low-energy threshold, has detected very-high-energy gamma rays from a giant flare of the distant Quasi-Stellar Radio Source (in short: radio quasar) 3C 279, at a distance of more than 5 billion light-years (a redshift of 0.536). No quasar has been observed previously in very-high-energy gamma radiation, and this is also the most distant object detected emitting gamma rays above 50 gigaelectron volts. Because high-energy gamma rays may be stopped by interacting with the diffuse background light in the universe, the observations by MAGIC imply a low amount for such light, consistent with that known from galaxy counts.
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LS 5039 is one of the few TeV emitting X-ray binaries detected so far. The powering source of its multiwavelength emission can be accretion in a microquasar scenario or wind interaction in a young nonaccreting pulsar scenario. Aims.To present new high-resolution radio images and compare them with the expected behavior in the different scenarios. Methods.We analyze Very Long Baseline Array (VLBA) radio observations that provide morphological and astrometric information at milliarcsecond scales. Results.We detect a changing morphology between two images obtained five days apart. In both runs there is a core component with a constant flux density, and an elongated emission with a position angle (PA) that changes by 12 $\pm$ $3\degr$ between both runs. The source is nearly symmetric in the first run and asymmetric in the second one. The astrometric results are not conclusive. Conclusions.A simple and shockless microquasar scenario cannot easily explain the observed changes in morphology. An interpretation within the young nonaccreting pulsar scenario requires the inclination of the binary system to be very close to the upper limit imposed by the absence of X-ray eclipses.
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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