Projeto de antenas multibandas integradas para terminais 4G

O presente trabalho apresenta um projeto e análise de uma antena monopolo planar multibanda operante nas frequências de 2000 MHz, 2500 MHz e 3500 MHz para aplicação em dispositivos móveis 3G e 4G. Dentre essas faixas estão contidos os espectros 3G (1895- 2165 MHz), 4G (2500-2690 MHz) e 4G (3400-3600 MHz) utilizadas pelo LTE e WIMAX 3,5. Para o desenvolvimento desse estudo foi tomado como referência uma antena dual-band de Hua- Ming Chen projetada para operar em sistemas ISM 1800 MHz, redes Wireless e Bluetooth 2400 MHz. O projeto proposto neste trabalho é uma modificação na estrutura da antena dual-band adaptada para tripla ressonância simultânea em frequências utilizadas em redes móveis 4G. Para alcançar o objetivo proposto utilizou-se para simulação o software CST® MICROWAVE STUDIO baseado no método Integração Finita no Domínio, as simulações foram feitas no domínio do tempo. Após obtenção satisfatória dos resultados simulados, um protótipo da antena foi confeccionado para medição e teste, os resultados apresentados são coerentes aos obtidos na simulação, o que valida o método proposto.

Avaliação neurocomportamental da exposição crônica ao Mercúrio inorgânico na memória social e memória emocional de ratos wistar machos adultos

O mercúrio inorgânico é facilmente absorvido por ingestão ou via cutânea. Entretanto, uma quantidade relativamente pequena de Hg²⁺ atravessa a barreira hematoencefálica ou as membranas biológicas, sendo em ratos adultos, o transporte axonal retrógrado a única via para a absorção de Hg²⁺ por neurônios, apresentando um forte potencial neurotóxico. Desta forma, o presente estudo objetivou investigar os efeitos da exposição crônica ao cloreto de mercúrio em memória social e emocional de ratos adultos. Para isso utilizou-se ratos Wistar, machos (n=40), com 5 meses de idade, distribuídos em dois grupos, um dos quais foi exposto ao Cloreto de Mercúrio (HgCl₂) via oral, por gavagem intra-gástrica (0,375mg/Kg), durante 45 dias. O outro grupo, denominado grupo controle (n=20) recebeu água destilada por gavagem. Foram utilizados os seguintes testes comportamentais: teste do campo aberto, teste de reconhecimento social para avaliação de memória social; o Teste do Labirinto em T Elevado (LTE) foi usado para avaliar o aprendizado do estado de esquiva e as memórias de curta e longa-duração. Após a finalização dos testes, os animais foram sacrificados para a dosagem do mercúrio total no hipocampo e através de um Espectrofotômetro de Absorção Atômica. Os resultados revelaram que os animais submetidos à exposição ao cloreto de mercúrio não manifestaram déficits em atividade exploratória. Nos dados do Teste de Reconhecimento Social, observamos que não houve alteração em memória social. No teste do LTE, o grupo exposto ao HgCl₂ necessitou de um número maior de exposições para aquisição do critério de esquiva (p<0,05) e apresentaram latência maior no braço aberto do aparato (p<0,05). Após 24 horas, verificou-se que os animais expostos passaram menos tempo no braço fechado em relação ao grupo controle, sugerindo déficits de memória de longa duração. Ao observar apenas o grupo HgCl₂, percebeu-se uma melhora no reteste, indicando preservação na memória de curta duração. Os dados de espectrometria de absorção atômica mostraram uma maior deposição de mercúrio no hipocampo de animais intoxicados, em relação aos animais do grupo controle.

Evolução da tecnologia móvel até 2013

In this paper expounds on the major phases or generations of the evolutionary process of wireless mobile communication, emphasizing their characteristics and changes over time. The main benefit of this process is the rate of data transfer remembering capacity spectral and methods of harnessing and improving its efficiency. The current network today is 4G and the technologies developed over the following requirements of the ITU are: Long Term Evolution Advanced (LTE-Advanced) and WirelessMAN-Advanced as part of the WiMAX IEEE 802.16m also described in this graduate work

Cumulative long-term safety, efficacy and patient-reported outcomes in children with juvenile idiopathic arthritis treated with intravenous abatacept: up to 7 years of treatment

The long-term efficacy and safety of intravenous abatacept in patients (pts) with juvenile idiopathic arthritis (JIA) have been reported previously from the Phase III AWAKEN trial ([1, 2]). Here, we report efficacy, safety and pt-reported outcomes from the open-label, long-term extension (LTE) of AWAKEN, with up to 7 years of follow-up. Pts entered the LTE if they were JIA ACR 30 non-responders (NR) at the end of the 4-month lead-in period (abatacept only), or if they received abatacept or placebo (pbo) in the 6-month double-blind (DB) period. The Child Health Questionnaire was used to evaluate health-related quality of life (HRQoL); physical (PhS) and psychosocial (PsS) summary and pain scores were analyzed. Pain was assessed by parent global assessment using a 100 mm visual analog scale. Efficacy and HRQoL evaluations are reported up to Day 1765 (~ Year 5.5). Safety is presented for the cumulative period (lead-in, DB and LTE), for all pts who received abatacept during the LTE. Of the 153 pts entering the LTE (58 from DB abatacept group, 59 from DB pbo group, 36 NR), 69 completed the trial (29 abatacept, 27 pbo, 13 NR). For pts treated in the LTE, mean (range) exposure to abatacept was 53.6 (5.6–85.6) months. During the LTE, incidence rates of AEs and serious AEs per 100 pt-years were 209.1 and 5.6. Thirty pts (19.6%) had serious AEs; most were unrelated and were musculoskeletal (8.5%) or infectious events (6.5%). No malignancy was reported. There was one death (accidental; unrelated). At Day 169, JIA ACR 50 and 70 response rates were 79.3% and 55.2% in the abatacept group, and 52.5% and 30.5% in the pbo group; 31.0% and 10.2% of pts in the abatacept and pbo groups, respectively, had inactive disease. By Day 1765, JIA ACR 50 and 70 response rates were 93.9% and 78.8% in the abatacept group, and 80.0% and 63.3% in the pbo group; 51.5% and 33.3% had inactive disease. In the NR group, 69.2% and 53.8% of pts achieved JIA ACR 50 and 70 responses at Day 1765, and 30.8% had inactive disease. In pts who entered the LTE, mean baseline PhS scores were below the range for healthy children (abatacept 30.2, pbo 31.0, NR 29.5). At Day 169, 38.3% of pts had reached a PhS score >50 ((1). By the end of the LTE, 43.5% of pts had reached a PhS score >50. At baseline, mean PsS scores for those who entered the LTE were slightly lower than the mean for healthy children (abatacept 43.5, pbo 44.2, NR 47.0). At Day 169, 54.9% of pts had a PsS score >50 (1). By Day 1765, 58.1% of pts had reached a PsS score >50. At baseline, the mean pain score was 42.9. By Day 169, 13.9% of pts were considered pain free (pain score = 0); this was maintained over the LTE (1).

Envolvimento de receptores 5-HT1A no hipocampo ventral na regulação de comportamentos defensivos relacionados com a ansiedade generalizada e com o pânico

Coordenação de Aperfeiçoamento de Pessoal de Nível Superior (CAPES)

Aplicação da tecnologia 4G em projetos de telefonia

This paper presents a study based on bibliographic research on LTE technology, chosen for the fourth generation of mobile phones, and the current status of implementation of 4G network in Brazil. The change in user behavior, which now uses data over the voice services, requires transmission networks to be increasingly robust and fast to enable the viewing of videos and use of other platforms that require internet connection. The retrospective of the development of mobile technologies, from 1G up to 4G that is currently used, shows the long road until it came to appliances and how the phone is used nowadays. Finally, the popularity of smartphones and hence the growing number of people with access to 4G networks, demanded new researchs for the development of future generations technologies in order to achieve the demand for speed enabling significant changes in user experience

Aplicação da tecnologia 4G em projetos de telefonia

This paper presents a study based on bibliographic research on LTE technology, chosen for the fourth generation of mobile phones, and the current status of implementation of 4G network in Brazil. The change in user behavior, which now uses data over the voice services, requires transmission networks to be increasingly robust and fast to enable the viewing of videos and use of other platforms that require internet connection. The retrospective of the development of mobile technologies, from 1G up to 4G that is currently used, shows the long road until it came to appliances and how the phone is used nowadays. Finally, the popularity of smartphones and hence the growing number of people with access to 4G networks, demanded new researchs for the development of future generations technologies in order to achieve the demand for speed enabling significant changes in user experience

The remarkable solar twin HIP 56948: a prime target in the quest for other Earths

Context. The Sun shows abundance anomalies relative to most solar twins. If the abundance peculiarities are due to the formation of inner rocky planets, that would mean that only a small fraction of solar type stars may host terrestrial planets. Aims. In this work we study HIP 56948, the best solar twin known to date, to determine with an unparalleled precision how similar it is to the Sun in its physical properties, chemical composition and planet architecture. We explore whether the abundances anomalies may be due to pollution from stellar ejecta or to terrestrial planet formation. Methods. We perform a differential abundance analysis (both in LTE and NLTE) using high resolution (R similar to 100 000) high S/N (600-650) Keck HIRES spectra of the Sun (as reflected from the asteroid Ceres) and HIP 56948. We use precise radial velocity data from the McDonald and Keck observatories to search for planets around this star. Results. We achieve a precision of sigma less than or similar to 0.003 dex for several elements. Including errors in stellar parameters the total uncertainty is as low as sigma similar or equal to 0.005 dex (1%), which is unprecedented in elemental abundance studies. The similarities between HIP 56948 and the Sun are astonishing. HIP 56948 is only 17 +/- 7 K hotter than the Sun, and log g, [Fe/H] and microturbulence velocity are only +0.02 +/- 0.02 dex, +0.02 +/- 0.01 dex and +0.01 +/- 0.01 km s(-1) higher than solar, respectively. Our precise stellar parameters and a differential isochrone analysis shows that HIP 56948 has a mass of 1.02 +/- 0.02 M-circle dot and that it is similar to 1 Gyr younger than the Sun, as constrained by isochrones, chromospheric activity, Li and rotation. Both stars show a chemical abundance pattern that differs from most solar twins, but the refractory elements (those with condensation temperature T-cond greater than or similar to 1000 K) are slightly (similar to 0.01 dex) more depleted in the Sun than in HIP 56948. The trend with T-cond in differential abundances (twins -HIP 56948) can be reproduced very well by adding similar to 3 M-circle plus of a mix of Earth and meteoritic material, to the convection zone of HIP 56948. The element-to-element scatter of the Earth/meteoritic mix for the case of hypothetical rocky planets around HIP 56948 is only 0.0047 dex. From our radial velocity monitoring we find no indications of giant planets interior to or within the habitable zone of HIP 56948. Conclusions. We conclude that HIP 56948 is an excellent candidate to host a planetary system like our own, including the possible presence of inner terrestrial planets. Its striking similarity to the Sun and its mature age makes HIP 56948 a prime target in the quest for other Earths and SETI endeavors.

Origin of the heavy elements in HD 140283 Measurement of europium abundance

Context. HD 140283 is a nearby (V = 7.7) subgiant metal-poor star, extensively analysed in the literature. Although many spectra have been obtained for this star, none showed a signal-to-noise (S/N) ratio high enough to enable a very accurate derivation of abundances from weak lines. Aims. The detection of europium proves that the neutron-capture elements in this star originate in the r-process, and not in the s-process, as recently claimed in the literature. Methods. Based on the OSMARCS 1D LTE atmospheric model and with a consistent approach based on the spectrum synthesis code Turbospectrum, we measured the europium lines at 4129 angstrom and 4205 angstrom, taking into account the hyperfine structure of the transitions. The spectrum, obtained with a long exposure time of seven hours at the Canada-France-Hawaii Telescope (CFHT), has a resolving power of 81 000 and a S/N ratio of 800 at 4100 angstrom. Results. We were able to determine the abundance A(Eu) = -2.35 +/- 0.07 dex, compatible with the value predicted for the europium from the r-process. The abundance ratio [Eu/Ba] = +0.58 +/- 0.15 dex agrees with the trend observed in metal-poor stars and is also compatible with a strong r-process contribution to the origin of the neutron-capture elements in HD 140283.

OXYGEN ABUNDANCES IN LOW- AND HIGH-alpha FIELD HALO STARS AND THE DISCOVERY OF TWO FIELD STARS BORN IN GLOBULAR CLUSTERS

Oxygen abundances of 67 dwarf stars in the metallicity range -1.6 < [Fe/H] < -0.4 are derived from a non-LTE analysis of the 777 nm O I triplet lines. These stars have precise atmospheric parameters measured by Nissen and Schuster, who find that they separate into three groups based on their kinematics and alpha-element (Mg, Si, Ca, Ti) abundances: thick disk, high-alpha halo, and low-alpha halo. We find the oxygen abundance trends of thick-disk and high-alpha halo stars very similar. The low-alpha stars show a larger star-to-star scatter in [O/Fe] at a given [Fe/H] and have systematically lower oxygen abundances compared to the other two groups. Thus, we find the behavior of oxygen abundances in these groups of stars similar to that of the a elements. We use previously published oxygen abundance data of disk and very metal-poor halo stars to present an overall view (-2.3 < [Fe/H] < +0.3) of oxygen abundance trends of stars in the solar neighborhood. Two field halo dwarf stars stand out in their O and Na abundances. Both G53-41 and G150-40 have very low oxygen and very high sodium abundances, which are key signatures of the abundance anomalies observed in globular cluster (GC) stars. Therefore, they are likely field halo stars born in GCs. If true, we estimate that at least 3% +/- 2% of the local field metal-poor star population was born in GCs.

DYNAMICAL EVOLUTION OF VISCOUS DISKS AROUND Be STARS. I. PHOTOMETRY

Be stars possess gaseous circumstellar disks that modify in many ways the spectrum of the central B star. Furthermore, they exhibit variability at several timescales and for a large number of observables. Putting the pieces together of this dynamical behavior is not an easy task and requires a detailed understanding of the physical processes that control the temporal evolution of the observables. There is an increasing body of evidence that suggests that Be disks are well described by standard alpha-disk theory. This paper is the first of a series that aims at studying the possibility of inferring several disk and stellar parameters through the follow-up of various observables. Here we study the temporal evolution of the disk density for different dynamical scenarios, including the disk buildup as a result of a long and steady mass injection from the star, the disk dissipation that occurs after mass injection is turned off, as well as scenarios in which active periods are followed by periods of quiescence. For those scenarios, we investigate the temporal evolution of continuum photometric observables using a three-dimensional non-LTE radiative transfer code. We show that light curves for different wavelengths are specific of a mass loss history, inclination angle, and alpha viscosity parameter. The diagnostic potential of those light curves is also discussed.

Origin of the heavy elements in HD 140283: measurement of europium abundance

Context. HD140283 is a nearby (V = 7:7) subgiant metal-poor star, extensively analysed in the literature. Although many spectra have been obtained for this star, none showed a signal-to-noise (S/N) ratio high enough to enable a very accurate derivation of abundances from weak lines. Aims. The detection of europium proves that the neutron-capture elements in this star originate in the r-process, and not in the s-process, as recently claimed in the literature. Methods. Based on the OSMARCS 1D LTE atmospheric model and with a consistent approach based on the spectrum synthesis code Turbospectrum, we measured the europium lines at 4129 Å and 4205 Å, taking into account the hyperfine structure of the transitions. The spectrum, obtained with a long exposure time of seven hours at the Canada-France-Hawaii Telescope (CFHT), has a resolving power of 81 000 and a S/N ratio of 800 at 4100 Å. Results. We were able to determine the abundance A(Eu) =

Sistemi OFDM: prestazioni di livello fisico

I primi studi su Orthogonal Frequency Division Multiplexing (OFDM) sono stati fatti fin dal 1960, ma negli ultimi anni la modulazione OFDM è emersa come una tecnica di modulazione chiave commerciale per i sistemi di comunicazione ad alta velocità. La ragione principale di questo crescente interesse è dovuto alla sua capacità di fornire dati ad alta velocità impiegando sistemi con complessità bassa e contrastando l'interferenza intersimbolo (ISI) e quella intercanale (ICI). Per questo motivo la modulazione OFDM è stata adottata da diversi sistemi digitali wireline e wireless standard, come Digital Audio Broadcasting (DAB), Asymmetric Digital Subscriber Line (ADSL), Wireless Local Area Network (IEEE 802.11 a,g,n) oppure per WiMAX e LTE.

Synchronization and Detection Techniques for Navigation and Communication Systems

Synchronization is a key issue in any communication system, but it becomes fundamental in the navigation systems, which are entirely based on the estimation of the time delay of the signals coming from the satellites. Thus, even if synchronization has been a well known topic for many years, the introduction of new modulations and new physical layer techniques in the modern standards makes the traditional synchronization strategies completely ineffective. For this reason, the design of advanced and innovative techniques for synchronization in modern communication systems, like DVB-SH, DVB-T2, DVB-RCS, WiMAX, LTE, and in the modern navigation system, like Galileo, has been the topic of the activity. Recent years have seen the consolidation of two different trends: the introduction of Orthogonal Frequency Division Multiplexing (OFDM) in the communication systems, and of the Binary Offset Carrier (BOC) modulation in the modern Global Navigation Satellite Systems (GNSS). Thus, a particular attention has been given to the investigation of the synchronization algorithms in these areas.

Evoluzione dei Modelli e delle Tecnologie per il Web: DART e HTML5 come caso di studio

Nell’ultimo decenno si è assisitito ad una frenetica evoluzione delle tecnologie di connessione e trasferimento dati, dagli impianti di fibra ottica sempre più diffusi e performanti, alle varie tecnologie mobile UMTS e LTE. Tutto ciò ha permesso a sempre più persone di poter spendere una maggiore fetta del proprio tempo sulla rete sia per svago che per lavoro. Questo ha portato col tempo l’utente interattivo alla ricerca di servizi remoti che prima usufruiva in locale, sia per motivi di portabilità e di interconnessione, sia per una semplice questione di sincronizzazione fra i vari dispositivi posseduti. Il presente progetto di tesi si pone come obiettivo di indagare con occhio ingegneristico all’evoluzione della struttura del web fino ad identificare e analizzare l’attuale necessità di poter avere in rete tutti quei servizi anche completi e strutturalmente complessi che prima si aveva sul proprio desktop; tutto ciò attraverso l’esempio di un nuovo linguaggio di sviluppo per applicazioni web strutturate proposto da Google: DART. In questa analisi non si potrà prescindere dallo studio attento della tecnologia che sin dagli inizi della rete ha fatto da struttura al web ovvero l’Html e il suo ultimo standard Hmtl5. Nella prima parte verrà mostrata, attraverso un breve percorso, la nascita e lo sviluppo del web, sino ai giorni nostri. Si effettuerà quindi una panoramica, rivisitando tutti più importanti passi che hanno portato la rete internet ad essere ciò che oggi utilizziamo, ponendo una particolare attenzione alle attuali esigenze di progettazione della struttura dei servizi web. Nel secondo capitolo viene introdotta la tecnologia a base del web, l’Html; attraverso una breve analisi dell’evoluzione di quest’ultima si arriverà sino all’attuale HTML5 e alle funzionalità offerte nell’ottica della programmazione web strutturata. Nel terzo capitolo si analizzerà in maniera più approfondita la necessità di un web strutturato e le potenzialità del progetto Dart attraverso alcuni esempi esplicativi. Infine si trarranno alcune conclusioni sull’attuale situazione del web, sulla necessità di un web strutturato e sulla possibilità di riuscita del progetto Dart.