Standing electron plasma wave mechanism of void array formation inside glass by femtosecond laser irradiation

We investigate the mechanism of formation of periodic void arrays inside fused silica and BK7 glass irradiated by a tightly focused femtosecond (fs) laser beam. Our results show that the period of each void array is not uniform along the laser propagation direction, and the average period of the void array decreases with increasing pulse number and pulse energy. We propose a mechanism in which a standing electron plasma wave created by the interference of a fs-laser-driven electron wave and its reflected wave is responsible for the formation of the periodic void arrays.

Training needs of traditional marine fishermen in Kerala

Training needs of 80 fishermen in 25 subject areas revealed a mean training need score of 23.0l; 95% wanted to get trained. The training needs were fairly strong in all subject areas, with the highest demand being for fishery engineering. Training need was also high for areas related to fishery technology. Most of the fishermen preferred to have the training at their own village, and in the months of June or July for an average period of 20.85 days. Education and income were positively related to intensity of training needs whereas age, number of family members, number of employed family members and experience in fishing were negatively correlated with it. These six variables explained 27 of the variance in training need intensity.

电离层行进式扰动的GPS台网监测研究

In this dissertation, we investigated two types of traveling ionospheric disturbances (TIDs)/gravity waves (GWs) triggered separately by auroral energy input during super geomagnetic storms and solar terminator (ST) under quiet geomagnetic conditions (kp<3+) using TEC measurements from the global network of GPS receivers. Research into the generation and propagation of TIDs/GWs during storms greatly enhance our understandings on the evolution processes of energy transportation from the high-latitude’s magnetosphere to the low-latitude ionosphere and the conjugated effect of TIDs propagation between the northern and southern hemispheres. Our results revealed that the conjugacy of propagation direction between the northern and southern hemispheres was subject to the influence of Coriolis force. We also figure out the evolution processes of ionospheric disturbances at the global scale. These are important topics that had not been well addressed previously. In addition, we also obtained thee wave structures of medium scale TIDs excited by the solar terminator (ST) moving over the northern America and physical mechanisms involved. Our observations confirm that the ST is a stable and repetitive source of ionospheric wave disturbances and the evidence of solar terminator generated disturbances has been demonstrated experimentally via the GPS TEC measurement. The main researches and results of this dissertation are as follows. First, the global traveling ionospheric disturbances (TIDs) during the drastic magnetic storms of October 29–31, 2003 were analyzed using the Global Position System (GPS) total electron content (TEC) data observed in the Asian-Australian, European and North American sectors. We collected the most comprehensive set of the TEC data from more than 900 GPS stations on the International GNSS Services (IGS) website and introduce here a strategy that combines polynomial fitting and multi-channel maximum entropy spectral analysis to obtain TID parameters. Moreover, in collaboration with my thesis advisor, I have developed an imaging technique of 2-dimensional map of TIDs structures to obtain spatial and temporal maps of large scale traveling ionospheric disturbances (LSTIDs). The clear structures of TEC perturbations map during the passage of TIDs were displayed. The results of our study are summarized as follows: (1) Large-scale TIDs (LSTIDs) and medium-scale TIDs (MSTIDs) were detected in all three sectors after the sudden commencement (SC) of the magnetic storm, and their features showed longitudinal and latitudinal dependences. The duration of TIDs was longer at higher latitudes than at middle latitudes, with a maximum of about 16 h. The TEC variation amplitude of LSTIDs was larger in the North American sector than in the two other sectors. At the lower latitudes, the ionospheric perturbations were more complicated, and their duration and amplitude were relatively longer and larger. (2) The periods and phase speeds of TIDs were different in these three sectors. In Europe, the TIDs propagated southward; in North America and Asia, the TIDs propagated southwestward; in the near-equator region, the disturbances propagated with the azimuth (the angle of the propagation direction of the LSTIDs measured clockwise from due north with 0°) of 210° showing the influence of Coriolis force; in the Southern Hemisphere, the LSTIDs propagated conjugatedly northwestward. Both the southwestward and northeastward propagating LSTIDs are found in the equatorial region. These results mean that the Coriolis effect cannot be ignored for the wave propagation of LSTIDs and that the propagation direction is correlated with the polar magnetic activity. (3) The day (day of year: 301) before the SC (sudden commencement) of magnetic storm, we observed a sudden TEC skip disturbances (±10 TECU). It should be a response for the high flux of proton during the solar flare event, but not the magnetic storms. Next, the most comprehensive and dense GPS network’s data from North-America region were used in this paper to analyze the medium scale traveling ionospheric disturbances (MSTIDs) which were generated by the moving solar terminator during the quiet days in 2005. We applied the multi-channel maximum entropy spectral analysis to calculated TID parameters, and found that the occurrence of ST-MSTIDs depends on the seasonal variations. The results of our study are summarized as follows: (1) MSTIDs stimulated by the moving ST (ST-MSTIDs) are detected at mid-latitudes after the passage of the solar terminator with the life time of 2～3 hours and the variation amplitude of 0.2～0.8 TECU. Spectral analysis indicated that the horizontal wavelength, average period, horizontal phase velocity of the MSTIDs are around 300±150 km，150±80 m/s and 25±15 min, respectively. In addition, ST-MSTIDs have wave fronts elongating the moving ST direction and almost parallel to ST. (2) The statistical results demonstrate that the dusk MSTIDs stimulated by ST is more obvious than the dawn MSTIDs in summer. On the contrary, the more-pronounced dawn MSTIDs occurs in winter. (3) Further analysis indicates that the seasonal variations of ST-MSTIDs occurrence frequency are most probably related to the seasonal differences of the variations of EUV flux in the ionosphere region and recombination process during sunrise and sunset period at mid-latitudes. Statistical study of occurrence characteristics of TIDs using the GPS network in North-American and European during solar maximum, In conclusion, statistical studies of the propagation characteristics of TIDs, which excited by the two common origins including geomagnetic storms and moving solar terminator, were involved with global GPS TEC databasein this thesis. We employed the multichannel maximum entropy spectral analysis method to diagnose the characteristics of propagation and evolvement of ionospheric disturbances, also, the characteristics of their regional distribution and climatological variations were revealed by the statistic analysis. The results of these studies can improve our knowledge about the energy transfer in the solar-terrestrial system and the coupling process between upper and lower atmosphere (thermosphere-ionosphere-mesosphere). On the other hand, our results of the investigation on TIDs generated by particular linear origin such as ST are important for developing ionospheric irregularity physics and modeling the transionosphere radio wave propagation. Besides, the GPS TEC representation of the ST-generated ionospheric structure suggests a better possibility for investigating this phenomenon. Subsequently, there are scientific meaning of the result of this dissertation to deeply discuss the energy transfer and coupling in the ionosphere, as well as realistic value to space weather forecast in the ionosphere region.

Safety and efficacy of rivastigmine in adolescents with Down syndrome: long-term follow-up.

Following the completion of a 20-week, open-label study of the safety and efficacy of liquid rivastigmine for adolescents with Down syndrome, 5 of the 10 adolescents in the clinical trial continued long-term rivastigmine therapy and 5 did not. After an average period of 38 months, all 10 subjects returned for a follow-up assessment to determine the safety and efficacy of long-term rivastigmine use. Rivastigmine was well tolerated and overall health appeared to be unaffected by long-term rivastigmine use. Performance change on cognitive and language measures administered at the termination of the open-label clinical trial was compared between the two groups. No between-group difference in median performance change across the long-term period was found, suggesting that the long-term use of rivastigmine does not improve cognitive and language performance. However, two subjects demonstrated remarkable improvement in adaptive function over the long-term period. Both subjects had received long-term rivastigmine therapy. The discussion addresses the challenge of assessing cognitive change in clinical trials using adolescents with Down syndrome as subjects and the use of group versus individual data to evaluate the relevance of medication effects.

Wave Damping Observed in Upwardly Propagating Sausage-Mode Oscillations Contained within a Magnetic Pore

We present observational evidence of compressible MHD wave modes propagating from the solar photosphere through to the base of the transition region in a solar magnetic pore. High cadence images were obtained simultaneously across four wavelength bands using the Dunn Solar Telescope. Employing Fourier and wavelet techniques, sausage-mode oscillations displaying significant power were detected in both intensity and area fluctuations. The intensity and area fluctuations exhibit a range of periods from 181 to 412 s, with an average period∼290 s, consistent with the global p-mode spectrum. Intensity and area oscillations present in adjacent band passes were found to be out of phase with one another, displaying phase angles of 6.°12, 5.°82,and 15.°97 between the 4170 Å continuum–G-band,G-band–Na i D1, and Na i D1–Ca ii K heights, respectively, reiterating the presence of upwardly propagating sausage-mode waves. A phase relationship of ∼0° between same-bandpass emission and area perturbations of the pore best categorizes the waves as belonging to the “slow” regime of a dispersion diagram. Theoretical calculations reveal that the waves are surface modes, with initial photospheric energies in excess of 35,000 Wm‑2. The wave energetics indicate a substantial decrease in energy with atmospheric height, confirming that magnetic pores are able to transport waves that exhibit appreciable energy damping, which may release considerable energy into the local chromospheric plasma.

Exposição a radiações ionizantes em cirurgia ortopédica num hospital público de Lisboa.

RESUMO - A monitorização individual dos trabalhadores (dosimetria individual) é obrigatória (Decreto Regulamentar n.o 9/90, de 19 de Abril) para os profissionais de saúde que desempenham funções com risco de exposição à radiação X, quando classificados como categoria A. Apesar disso, a exposição a radiações ionizantes é frequentemente pouco, ou mesmo nada, valorizada pelos profissionais de saúde. O presente estudo, realizado no contexto de intervenções cirúrgicas de ortopedia, teve por objectivos: • avaliar a dose de radiação em diferentes zonas durante as cirurgias ortopédicas; • estimar a dose de exposição a radiações ionizantes dos profissionais de saúde, em função das suas posições, predominantemente adoptadas durante o acto cirúrgico; • sensibilizar os profissionais de saúde para a utilização correcta da dosimetria individual e para a adopção das medidas de protecção radiológica. A avaliação do risco foi efectuada através de: 1) medições preliminares com recurso a um fantoma colocado a 50 cm e a 100 cm do eixo central do feixe de radiação e em direcções de 45°, 90° e 135°; 2) medições durante uma cirurgia ortopédica em «localizações » correspondentes às gónadas, ao cristalino e às mãos dos profissionais de saúde intervenientes na cirurgia (ortopedistas, enfermeiros instrumentistas); 3) medições ao nível do topo da mesa (posição do anestesista) e ao nível do comando do equipamento emissor de raios X (técnico de radiologia); 4) determinação do tempo de utilização dos raios X durante as cirurgias ortopédicas; 5) cálculo da estimativa do número anual de cirurgias ortopédicas realizadas, com base nos registos existentes. Assumindo a não utilização de aventais plúmbeos os valores máximos medidos foram de 2,5 mSv/h (ao nível das gónadas), de 0,6 mSv/h ao nível do cristalino e de 1 mSv/ h ao nível das mãos dos ortopedistas e dos enfermeiros instrumentistas (que se situavam próximo do feixe de raios X, a 50 cm do feixe de radiação). A estimativa de exposição anual (dose equivalente) para os profissionais que operam junto ao feixe de radiação X foi de: • Ortopedistas — 20,63 a 68,75 mSv (gónadas), 4,95 a 16,50 mSv (cristalino) e 8,25 a 27,50 mSv (mãos); • Enfermeiros instrumentistas — 130,63 a 151,25 mSv (gónadas), 31,35 a 36,30 mSv (cristalino) e 52,25 a Os profissionais que ocupam posições mais afastadas do feixe (por exemplo: anestesistas) terão doses de radiação mais reduzidas, embora estas possam ainda ser importantes ao nível das gónadas na zona do topo da mesa (anestesista). Conclui-se que a exposição profissional em blocos operatórios pode implicar, em cirurgia ortopédica, a sujeição a níveis de exposição consideráveis, o que permite classificar estes profissionais de categoria A, justificando a utilização obrigatória (e correcta de acordo com as recomendações) da dosimetria individual e a adopção de medidas de protecção radiológica, tantas vezes negligenciadas.

The periodicity of the eta Carinae events

Extensive spectral observations of eta Carinae over the last cycle, and particularly around the 2003.5 low-excitation event, have been obtained. The variability of both narrow and broad lines, when combined with data taken from two earlier cycles, reveal a common and well-defined period. We have combined the cycle lengths derived from the many lines in the optical spectrum with those from broad-band X-rays, optical and near-infrared observations, and obtained a period length of P(pres) = 2022.7 +/- 1.3 d. Spectroscopic data collected during the last 60 yr yield an average period of P(avg) = 2020 +/- 4 d, consistent with the present-day period. The period cannot have changed by more than Delta P/P = 0.0007 since 1948. This confirms the previous claims of a true, stable periodicity, and gives strong support to the binary scenario. We have used the disappearance of the narrow component of He I 6678 to define the epoch of the Cycle 11 minimum, T(0) = JD 245 2819.8. The next event is predicted to occur on 2009 January 11 (+/- 2 d). The dates for the start of the minimum in other spectral features and broad-bands are very close to this date, and have well-determined time-delays from the He I epoch.

Análise da dentina de dentes decíduos submetidos ao capeamento pulpar indireto

O objetivo do estudo foi avaliar as características da dentina cariada remanescente de molares decíduos quanto à coloração, consistência e microdureza, após um período médio de 3 anos e 8 meses da realização do capeamento pulpar indireto. O estudo clínico constou de 27 dentes que apresentavam lesões cariosas ativas com expressão radiográfica em metade interna de dentina. Aleatoriamente, foi realizado o capeamento pulpar indireto e utilizado como material capeador o hidróxido de cálcio (HC) e o cimento de ionômero de vidro resinoso modificado (CIVRM). As crianças foram acompanhadas através de exames clínicos e radiográficos, e ao longo de um período médio de 3 anos e 8 meses, observou-se um índice de sucesso de 89% para o grupo do HC e de 93% para o CIVRM, não havendo diferença estatisticamente significante entre os dois grupos (p=0,62). Os dentes considerados como sucesso no estudo clínico foram agrupados em um único grupo (grupo teste), que constou de 13 dentes que sofreram esfoliação natural ou exodontia por motivos ortodônticos. Além disso, foram selecionados 15 molares decíduos hígidos (grupo controle positivo) e 15, portadores de lesões cariosas ativas em metade interna de dentina (grupo controle negativo). As amostras do grupo teste tiveram suas respectivas restaurações removidas, a profundidade medida e a dentina remanescente avaliada por um operador calibrado, seguindo critérios descritivos, quanto à consistência e a coloração. Nos dentes do grupo controle positivo, foram realizados preparos cavitários oclusais em até 4 mm de profundidade, enquanto que, no grupo controle negativo, o mesmo operador do estudo clínico realizou a remoção parcial de tecido cariado in vitro. A partir daí, todos os dentes foram preparados para análise de microdureza, que foi realizada por um examinador calibrado, que empregou o princípio de cegamento. Na análise da consistência, todos os dentes do grupo teste (n=13) apresentaram-se endurecidos, enquanto que 9, apresentaram coloração amarela-clara (8 do CIVRM e 1 do HC) e 4, castanho-escura (1 do CIVRM e 3 do HC). Para o teste de microdureza no grupo teste, obteve-se uma média KHN de 40,81 (±16,28) MPa, enquanto que nos grupos controles positivo e negativo, foram alcançados valores médios de 62,73 (±11,24) MPa e 19,15 (±6,99) MPa, respectivamente. A análise estatística mediante o teste ANOVA indicou que houve diferença significativa entre os 3 grupos. Foi constatada a remineralização da dentina de dentes decíduos em que foi realizada a técnica do capeamento pulpar indireto após um período médio de 3 anos e 8 meses, através de critérios clínico (consistência) e laboratorial (análise da microdureza).

Uma análise empírica sobre o processo de recuperação econômica pela via judicial adotado pelas sociedades empresárias: a experiência no Tribunal de Justiça do Estado do Rio de Janeiro

Este estudo objetiva analisar os processos de recuperação judicial iniciados, desde a vigência da Lei de Recuperação de Empresas (fevereiro de 2005) até 31/06/2011 nas varas empresarias da comarca da capital do Tribunal de Justiça do Estado do Rio de Janeiro. Além da aferição do tempo médio de cada uma das etapas previstas na Lei de Recuperação de Empresas (deferimento do processamento da recuperação judicial, concessão da recuperação judicial e encerramento do processo após cumprimento de todas as obrigações previstas no plano que se vencerem até dois anos depois da concessão da recuperação judicial), busco também verificar se, de fato, alguma sociedade requerente conseguiu se recuperar. Para tanto, considerarei recuperada a sociedade que, após o encerramento do processo, estiver cumprindo plenamente o seu plano de recuperação, sem que tenha havido qualquer requerimento posterior de falência. Considerando que a Lei de Recuperação de Empresas já está no seu sétimo ano de vigência, bem como o fato de o legislador ter idealizado o processo para que dure no máximo 3 anos, entendo não haver óbices à adoção do conceito supra, tendo em vista que já haver tempo suficiente para o início e encerramento desse tipo de processo. Diante disso, o presente estudo observou que o tempo médio para cumprimento das etapas ultrapassa o limite do razoável, bem como que nenhuma sociedade conseguiu se recuperar até o desfecho da pesquisa, havendo casos, inclusive, de convolação da recuperação judicial em falência.

Em busca de um novo indicador Espectroscópico do período de rotação das Estrelas do tipo solar

The study of sunspots consistently contributed to a better understanding of magnetic phenomena of the Sun, as its activity. It was found with the dynamics of sunspots that the Sun has a rotation period of twenty-seven days around your axis. With the help of Project Sun-As-A-Star that solar spectra obtained for more than thirty years we observed oscillations of both the depth of the spectral line and its equivalent width, and analysis of the return information about the characteristics of solar magnetism. It also aims to find patterns of solar magnetic activity cycle and the average period of rotation of the Sun will indicate the spectral lines that are sensitive to magnetic activity and which are not. Sensitive lines how Ti II 5381.0 Å stands as the best indicator of the solar rotation period and also shows different periods of rotation cycles of minimum and maximum magnetic activity. It is the first time we observe clearly distinct rotation periods in the different cycles. The analysis also shows that Ca II 8542.1 Å and HI 6562.0 Å indicate the cycle of magnetic activity of eleven years. Some spectral lines no indicated connection with solar activity, this result can help us search for programs planets using spectroscopic models. Data analysis was performed using the Lomb-Scargle method that makes the time series analysis for unequally spaced data. Observe different rotation periods in the cycles of magnetic activity accounts for a discussion has been debated for many decades. We verified that spectroscopy can also specify the period of stellar rotation, thus being able to generalize the method to other stars

Prevalência do aleitamento materno

OBJETIVO: Avaliar os indicadores de aleitamento materno em consultórios particulares e centros de saúde no município de Lins, SP, e comparar a prevalência de aleitamento materno exclusivo dessa região com a encontrada em outras pesquisas. MÉTODOS: Estudo de corte transversal com amostra aleatória de 255 crianças de quatro a doze meses de idade, estratificada por sexo, condição socioeconômica e escolaridade dos pais. Foram avaliados os indicadores de aleitamento materno em dois grupos de crianças: as acompanhadas em consultórios particulares e as acompanhadas em centros de saúde. Foram utilizados questionários respondidos pelos responsáveis. Os dados desta pesquisa foram comparados aos de outros estudos. RESULTADOS: Apesar de haver diferenças significativas nas condições de renda, estrato social e escolaridade dos pais, não houve diferença significativa nos índices de aleitamento materno entre os dois grupos. No grupo total, a prevalência de aleitamento materno exclusivo aos quatro meses foi de 61,1% e a mediana de aleitamento materno exclusivo foi de 120 dias. Os resultados foram superiores aos dos demais estudos consultados. CONCLUSÃO: Os resultados mostraram diferenças relacionadas às condições socioeconômicas, porém, os índices de aleitamento materno foram semelhantes entre os dois grupos. Os resultados de aleitamento materno exclusivo foram superiores aos das demais pesquisas.

Densidade de plantio na produtividade e nos teores de nutrientes nas folhas e frutos da bananeira cv. Thap Maeo

Conselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq)

Life cycle and host specificity of Amblyomma triste (Acari : Ixodidae) under laboratory conditions

We report biological data of two generations of Amblyomma triste in laboratory and compared the suitability of different host species. Infestations by larval and nymphal stages were performed on guinea pigs (Cavia porcellus), chickens (Gallus gallus), rats (Rattus norvegicus), rabbits (Oryctolagus cuniculus), wild mice (Calomys callosus), dogs (Canis familiaris) and capybaras (Hydrochaeris hydrochaeris). Infestations by adult ticks were performed on dogs, capybaras and rabbits. Tick developmental periods were observed in an incubator at 27degreesC and RH 90%. Guinea pigs were the most suitable hosts for larvae and nymphs, followed by chickens. The remaining host species were less suitable for immature ticks as fewer engorged ticks were recovered from them. Mean larval feeding periods varied from 3.8 to 4.7 d between different host species. Mean larval premolt periods ranged from 8.9 to 10.4 d. Nymphal mean feeding periods varied from 4.2 to 6.2 d for ticks fed on different host species. Premolt period of male nymphs (mean: 15.4 d) was significantly longer than that of female nymphs (14.7 d). Female nymphs were significantly heavier than male nymphs. The overall sex ratio of the adult ticks emerged from nymphs was 0.9:1 (M:F). Capybaras were the most suitable host for the tick adult stage as significantly more engorged females were recovered from them and these females were significantly heavier than those recovered from dogs or rabbits. The life cycle of A. triste in laboratory could be completed in an average period of 155 d. The potential role of guinea pigs, birds and capybaras, as hosts for A. triste in nature, is discussed.

Estudo biológico e morfométrico dos estádios ninfais de Rhodnius neglectus Lent, 1954 (Hemiptera, Reduviidae)

The following parameters of the biological cycle of the Rhodnius neglectus were determined under a temperature of 28°C and relative humidity of the air varying between 52-94%: a) average period of incubation: 13.67 days; b) rate of the eggs eclosion: 86.18%; c) average period of growth of the 1st, 2nd, 3rd, 4th, 5th instar nymphs: 18.91, 15.19, 21.38, 21.34, 30.43 days, respectively; d) percentage of death in the instar nymphs: 13.82, 18.26, 9.95, 8.78, 15.06% respectively; e) percentage of changes per instar nymphs: 86.18, 81.74, 90.05, 91.22, 84.94% respectively. The morphometric study with the stereoscopic microscope and Leica image analyses system, using the Qwin software, of the five instar nymphs showed that in the five instar nymphs a gradual growth of the head, thorax and abdomen occurs. In all the instars the abdomen is the largest segment. In the four first instars the head is larger than the thorax. In the fifth instar the head and the thorax present equivalent sizes.

A qualidade de vida de dependentes de álcool

Coordenação de Aperfeiçoamento de Pessoal de Nível Superior (CAPES)