Influência dos marcadores inflamatórios sobre a evolução do estado nutricional e progressão da calcificação cardiovascular em pacientes portadores de doença renal crônica tratados por hemodiálise

Coordenação de Aperfeiçoamento de Pessoal de Nível Superior (CAPES)

Impacto do acompanhamento com bioimpedância na predição de eventos cardiovasculares em pacientes em diálise crônica

Coordenação de Aperfeiçoamento de Pessoal de Nível Superior (CAPES)

Efeitos do manto de intemperismo sobre anomalias “VLF” dos corpos tabulares inclinados

A utilização dos métodos indutivos de propagação E.M. na exploração mineral em regiões tropicais, apresenta grandes dificuldades devido a presença de uma camada superficial condutiva (manto de intemperismo) comumente encontrada nestas regiões. Na região Amazônica, o manto apresenta-se bastante desenvolvido e condutivo, e em regiões semi-áridas, pode-se formar uma fina crosta superficial de sal. Em conseqüência disto, a interpretação dos dados E.M. obtidos para modelos que não consideram uma cobertura condutiva levam a erros consideráveis. Objetivando-se estudar os efeitos do manto sobre anomalias VLF devidas a corpos tabulares inclinados em contato com o manto (manto ohmico), foi realizada uma série de experimentos através do modelamento analógico, considerando-se diferentes parâmetros de resposta para o manto e o corpo. O manto de intemperismo foi simulado por soluções de cloreto de amônia (NH₄Cl) dispostas horizontalmente e o corpo condutor por chapas de grafite colocadas em posições inclinadas verticalmente. Utilizou-se quatro corpos condutores e três mantos com diferentes espessuras e condutividades, simulando, desta forma, diversas situações geológicas. Os resultados são dados por simples situações dos corpos localizados em um meio não condutor (ar), onde os parâmetros variados são: profundidade do topo, condutividade e mergulho do corpo. Os efeitos da condutividade da cobertura são amplamente ilustrados e avaliados. Para a análise dos resultados, foi plotado um conjunto de curvas considerando-se os valores pico-a-pico das anomalias de "tilt angle" e de elipsidade. Os resultados foram sintetizados em um outro conjunto de curvas reunidas em diagramas de Argand. Estando ou não o manto presente, observou-se, tanto para o tilt angle quanto para a elipsidade, o efeito do aumento da profundidade é o de reduzir a magnitude pico-a-pico e a forma do pico da anomalia, fazendo com que este afaste-se do ponto de "cross-over". Para um condutor de mesma espessura, o aumento da condutividade causa um ligeiro aumento nas anomalias de tilt angle, e uma atenuação nas anomalias de elipsidade. O efeito geral na variação do mergulho do condutor é o de causar uma assimetria nos perfis de tilt angle e de elipsidade. O aumento da condutância do manto de intemperismo causa um acréscimo nas anomalias de elipsidade e uma ligeira diminuição nas anomalias de tilt angle; porém, a partir de um certo valor de condutância do manto (mantos mais condutivos) tanto as anomalias de tilt angle quanto as anomalias de elipsidade começam a atenuar. Há rotação de fase no sentido anti-horário, sendo mais intensa para grandes valores de número de indução do corpo. Na presença do manto, o corpo parece estar a uma profundidade inferior à verdadeira e a ser menos condutivo.

Evaluation of nutritional indicators and body composition in patients with advanced liver disease enrolled for liver transplantation

PURPOSE: Malnutrition is prevalent in patients with advanced liver disease (LD) related to multifactorial causes. Fluid retention can underestimate the nutritional status based on anthropometric measures. We evaluated nutritional indicators and body composition (BC) in patients with liver cirrhosis and correlated them with LD severity. METHODS: Forty three patients with LD enrolled for liver transplantation were evaluated by Anthropometric measures, subjective evaluation (Global Assessment of Nutritional Status - SGA) and biochemical indicators. Single-frequency electrical bioimpedance (SFE-BIA) was used to evaluate body composition (BC). It measured resistance (R), reactance (Xc) and the phase angle (PA). LD severity was estimated by Child-Pugh and Meld criteria (Model for End-Stage Liver Disease). RESULTS: Child-Pugh index between patients was 7.11±1.70 and Meld was 12.23±4.22. Arm Circumference, Arm Muscle Circumference and Arm Muscle Area, SGA, hemoglobin, hematocrit and albumin showed better correlation with disease severity. Xc and PA showed correlation both with Meld and Child-Pugh score when BC were evaluated. PA was depleted in 55.8% of the patients. CONCLUSIONS: Diagnosis of malnutrition varied according to the method. Global assessment of nutritional status showed better correlation with disease severity than with objective methods. Single-frequency electrical bioimpedance for body composition analysis in cirrhotic patients must be cautiously used; however, primary vectors seems to be valid and promising in clinical practice.

Papel dos receptores Toll-Like 2 e 4 do estado nutricional em pacientes com leishmaniose visceral

Pós-graduação em Doenças Tropicais - FMB

Analysis of 25 mutual eclipses and occultations between the Galilean satellites observed from Brazil in 2009

Conselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq)

Influência do estado nutricional e da composição corporal na evolução clínica dos pacientes com doença inflamatória intestinal

Pós-graduação em Fisiopatologia em Clínica Médica - FMB

Investigação do Ângulo de Fase como preditor da resposta virológica em pacientes portadores de hepatite C

Coordenação de Aperfeiçoamento de Pessoal de Nível Superior (CAPES)

Bioelectrical impedance vector analysis (BIVA) in stable preterm newborns

Objective: To observe the behavior of the plotted vectors on the RXc (R - resistance - and Xc - reactance corrected for body height/length) graph through bioelectrical impedance analysis (BIVA) and phase angle (PA) values in stable premature infants, considering the hypothesis that preterm infants present vector behavior on BIVA suggestive of less total body water and soft tissues, compared to reference data for term infants. Methods: Cross-sectional study, including preterm neonates of both genders, in-patients admitted to an intermediate care unit at a tertiary care hospital. Data on delivery, diet and bioelectrical impedance (800 mA, 50 kHz) were collected. The graphs and vector analysis were performed with the BIVA software. Results: A total of 108 preterm infants were studied, separated according to age (< 7 days and >= 7 days). Most of the premature babies were without the normal range (above the 95% tolerance intervals) existing in literature for term newborn infants and there was a tendency to dispersion of the points in the upper right quadrant, RXc plan. The PA was 4.92 degrees (+/- 2.18) for newborns < 7 days and 4.34 degrees (+/- 2.37) for newborns >= 7 days. Conclusion: Premature infants behave similarly in terms of BIVA and most of them have less absolute body water, presenting less fat free mass and fat mass in absolute values, compared to term newborn infants.

Effect of the Type of Emulsifying Salt on Microstructure and Rheological Properties of "Requeijao Cremoso" Processed Cheese Spreads

The role of different types of emulsifying saltssodium citrate (TSC), sodium hexametaphosphate (SHMP), sodium tripolyphosphate (STPP) and tetrasodium pyrophosphate (TSPP)on microstructure and rheology of requeijao cremoso processed cheese was determined. The cheeses manufactured with TSC, TSPP, and STPP behaved like concentrated solutions, while the cheese manufactured with SHMP exhibited weak gel behavior and the lowest values for the phase angle (G/G). This means that SHMP cheese had the protein network with the largest amount of molecular interactions, which can be explained by its highest degree of fat emulsification. Rotational viscometry indicated that all the spreadable cheeses behaved like pseudoplastic fluids. The cheeses made with SHMP and TSPP presented low values for the flow behavior index, meaning that viscosity was more dependent on shear rate. Regarding the consistency index, TSPP cheese showed the highest value, which could be attributed to the combined effect of its high pH and homogeneous fat particle size distribution.

Extraction of spin periods of space debris from optical light curves

The population of space debris increased drastically during the last years. These objects have become a great threat for active satellites. Because the relative velocities between space debris and satellites are high, space debris objects may destroy active satellites through collisions. Furthermore, collisions involving massive objects produce large number of fragments leading to significant growth of the space debris population. The long term evolution of the debris population is essentially driven by so-called catastrophic collisions. An effective remediation measure in order to stabilize the population in Low Earth Orbit (LEO) is therefore the removal of large, massive space debris. To remove these objects, not only precise orbits, but also more detailed information about their attitude states will be required. One important property of an object targeted for removal is its spin period, spin axis orientation and their change over time. Rotating objects will produce periodic brightness variations with frequencies which are related to the spin periods. Such a brightness variation over time is called a light curve. Collecting, but also processing light curves is challenging due to several reasons. Light curves may be undersampled, low frequency components due to phase angle and atmospheric extinction changes may be present, and beat frequencies may occur when the rotation period is close to a multiple of the sampling period. Depending on the method which is used to extract the frequencies, also method-specific properties have to be taken into account. The astronomical Institute of the University of Bern (AIUB) light curve database will be introduced, which contains more than 1,300 light curves acquired over more than seven years. We will discuss properties and reliability of different time series analysis methods tested and currently used by AIUB for the light curve processing. Extracted frequencies and reconstructed phases for some interesting targets, e.g. GLONASS satellites, for which also SLR data were available for the period confirmation, will be presented. Finally we will present the reconstructed phase and its evolution over time of a High-Area-to-Mass-Ratio (HAMR) object, which AIUB observed for several years.

Malnutrition Predicts Clinical Outcome in Patients with Neuroendocrine Neoplasias.

Malnutrition is a common problem in oncologic diseases influencing treatment outcomes, treatment complications, quality of life and survival. The potential role of malnutrition has not yet systematically been studied in neuroendocrine neoplasms (NEN), which due to growing prevalence and additional therapeutic options provide an increasing clinical challenge for diagnosis and management. The aim of this cross-sectional observational study, which included a long-term follow-up, was therefore to define the prevalence of malnutrition in 203 patients with NEN using various methodological approaches and to analyze the short- and long-term outcome of malnourished patients. A detailed subgroup analysis was also performed to define risk factors for poorer outcome. By applying malnutrition screening scores 21-25% of NEN-patients were at risk of or demonstrated manifest malnutrition. This was confirmed by anthropometric measurements, determination of serum surrogate parameters such as albumin and bioelectrical impedance analysis particularly phase angle α. Length of hospital stay (LoS) was significantly longer in malnourished NEN-patients while long-term overall survival was highly significantly reduced. Patients with high-grade (G3) neuroendocrine carcinomas, progressive disease and undergoing chemotherapy were at particular risk for malnutrition associated with a poorer outcome. Multivariate analysis confirmed the important and highly significant role of malnutrition as an independent prognostic factor for NEN besides proliferative capacity (G3-NEC). Malnutrition is therefore an underrecognized problem in NEN-patients, which should systematically be diagnosed by widely available standard methods such Nutritional Risk Screening (NRS) score, serum albumin levels and bioelectrical impedance analysis (BIA) and treated to improve both short- and long-term outcomes.

Spectrophotometric properties of the nucleus of comet 67P/Churyumov-Gerasimenko from the OSIRIS instrument onboard the ROSETTA spacecraft

Context. The Rosetta mission of the European Space Agency has been orbiting the comet 67P/Churyumov-Gerasimenko (67P) since August 2014 and is now in its escort phase. A large complement of scientific experiments designed to complete the most detailed study of a comet ever attempted are onboard Rosetta. Aims. We present results for the photometric and spectrophotometric properties of the nucleus of 67P derived from the OSIRIS imaging system, which consists of a Wide Angle Camera (WAC) and a Narrow Angle Camera (NAC). The observations presented here were performed during July and the beginning of August 2014, during the approach phase, when OSIRIS was mapping the surface of the comet with several filters at different phase angles (1.3 degrees-54 degrees). The resolution reached up to 2.1 m/px. Methods. The OSIRIS images were processed with the OSIRIS standard pipeline, then converted into I/F. radiance factors and corrected for the illumination conditions at each pixel using the Lommel-Seeliger disk law. Color cubes of the surface were produced by stacking registered and illumination-corrected images. Furthermore, photometric analysis was performed both on disk-averaged photometry in several filters and on disk-resolved images acquired with the NAC orange filter, centered at 649 ran, using Hapke modeling. Results. The disk-averaged phase function of the nucleus of 67P shows a strong opposition surge with a G parameter value of -0.13 +/- 0.01 in the HG system formalism and an absolute magnitude H-v(1, 1, 0) = 15.74 +/- 0.02 mag. The integrated spectrophotometry in 20 filters covering the 250-1000 nm wavelength range shows a red spectral behavior, without clear absorption bands except for a potential absorption centered at similar to 290 rim that is possibly due to SO2 ice. The nucleus shows strong phase reddening, with disk-averaged spectral slopes increasing from 11%/( 100 nm) to 16%/(100 nm) in the 1.3 degrees-54 degrees phase angle range. The geometric albedo of the comet is 6.5 +/- 0.2% at 649 nm, with local variations of up to similar to 16% in the Hapi region. From the disk-resolved images we computed the spectral slope together with local spectrophotometry and identified three distinct groups of regions (blue, moderately red, and red). The Hapi region is the brightest, the bluest in term of spectral slope, and the most active surface on the comet. Local spectrophotometry shows an enhancement of the flux in the 700-750 nm that is associated with coma emissions.

Size-frequency distribution of boulders ≥7 m on comet 67P/Churyumov-Gerasimenko

Aims. We derive for the first time the size-frequency distribution of boulders on a comet, 67P/Churyumov-Gerasimenko (67P), computed from the images taken by the Rosetta/OSIRIS imaging system. We highlight the possible physical processes that lead to these boulder size distributions. Methods. We used images acquired by the OSIRIS Narrow Angle Camera, NAC, on 5 and 6 August 2014. The scale of these images (2.44−2.03 m/px) is such that boulders ≥7 m can be identified and manually extracted from the datasets with the software ArcGIS. We derived both global and localized size-frequency distributions. The three-pixel sampling detection, coupled with the favorable shadowing of the surface (observation phase angle ranging from 48° to 53°), enables unequivocally detecting boulders scattered all over the illuminated side of 67P. Results. We identify 3546 boulders larger than 7 m on the imaged surface (36.4 km2), with a global number density of nearly 100/km2 and a cumulative size-frequency distribution represented by a power-law with index of −3.6 +0.2/−0.3. The two lobes of 67P appear to have slightly different distributions, with an index of −3.5 +0.2/−0.3 for the main lobe (body) and −4.0 +0.3/−0.2 for the small lobe (head). The steeper distribution of the small lobe might be due to a more pervasive fracturing. The difference of the distribution for the connecting region (neck) is much more significant, with an index value of −2.2 +0.2/−0.2. We propose that the boulder field located in the neck area is the result of blocks falling from the contiguous Hathor cliff. The lower slope of the size-frequency distribution we see today in the neck area might be due to the concurrent processes acting on the smallest boulders, such as i) disintegration or fragmentation and vanishing through sublimation; ii) uplifting by gas drag and consequent redistribution; and iii) burial beneath a debris blanket. We also derived the cumulative size-frequency distribution per km2 of localized areas on 67P. By comparing the cumulative size-frequency distributions of similar geomorphological settings, we derived similar power-law index values. This suggests that despite the selected locations on different and often opposite sides of the comet, similar sublimation or activity processes, pit formation or collapses, as well as thermal stresses or fracturing events occurred on multiple areas of the comet, shaping its surface into the appearance we see today.