968 resultados para Interval of solidification


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Los resultados en depilación láser son variables entre los diferentes equipos y pacientes, alcanzando reducciones de hasta el 25% por sesión en la literatura disponible. En la práctica clínica se utiliza el conteo de pelos como instrumento para modificar parámetros de tratamiento y realizar cambios o combinaciones de los láseres con el fin de alcanzar la máxima reducción posible. Materiales y métodos: En una cohorte histórica se analizaron 298 sesiones (79 pacientes) a los que se determinó variables clínicas registradas de reducción de pelo con tres láseres diferentes, junto a parámetros para cada uno de los equipos, a un intervalo máximo de 90 días entre cada sesión. Resultados: Se evaluaron 79 mujeres para un total de 298 sesiones, con un rango de edad entre los 18 y 67 años, fototipo de piel III-V, intervalo entre sesiones de 14 a 90 días. Los equipos utilizados fueron Soprano XLi® (64.7%), Lightsheer® (18.4%) y Alexandrita (16.9%). Los promedios de reducción fueron en la primera sesión 43.3±32%, segunda sesión 55.8±42.1%, tercera sesión 48.1±16%, cuarta sesión 51.8±26.6%, quinta sesión 61.2±26.7%.(p<0.001). Se encontró una baja incidencia de complicaciones (7.6% de pacientes), siendo significativa la presencia de éstas con Lightsheer® y Alexandrita, a diferencia del Soprano®. Discusión: Éste estudio longitudinal mostró altas reducciones sesión a sesión comparadas con las disponibles en la literatura, independientemente del equipo utilizado. Soprano® presentó un mejor perfil de seguridad que Lightsheer® y Alexandrita.

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Objetivo: Determinar los factores de riesgo de anteparto, intraparto y fetales asociados a asfixia perinatal en los recién nacidos del servicio de neonatología del Hospital Universitario Mayor Méderi de Bogotá, 2010-2011. Materiales y métodos: Estudio de casos y controles pareado por fecha de nacimiento, con una relación 1:5(51:306). Las asociaciones se evaluaron con la prueba de ji-cuadrado de Mantel y Haenszel o Test de Fisher para datos pareados, con OR e intervalo de confianza del 95%, el análisis multivariado con un modelo de regresión logística condicional. Resultados: Los factores de riesgo con asociación significativa fueron: - Ante parto: Antecedentes patológicos maternos (OR=6.00,IC95%:1.55-23.19,p=0.013), primigestación (OR=1.91,IC95%:1.02-3.56,p=0,090), -Intraparto: Abruptio de placenta (OR=25,00,IC95%:2.92-213.99,p=0.001), hemorragia del tercer trimestre (OR=12.50,IC95%:2.43-64.43,p=0.001), Oligohidramnios(OR=6.25,IC95%:1.68-23.28,p=0.001), taquicardia fetal (OR=7.66,IC95%:1.67-35.04,p=0.011), monitoreo fetal intraparto anormal (OR=10.33,IC95%:4.38-24.34,p=0.001), expulsivo prolongado(OR=13.00,IC95%:4.63-36.46,p=0.001), fiebre materna(p<0.001), corioamnionitis(p<0.001), convulsiones maternas(p<0.001), bradicardia fetal (p=<0.001), -Fetales: Género masculino(OR=1.87,IC95%:1.02-3.44,p=0.026), edad gestacional por BALLARD igual ó <36semanas(OR=4.78(IC95%:2.21-10.35,p=0.001), vía del nacimiento instrumentado(OR=18,80,IC95%:3.69-39.55,p=0.001), líquido amniótico hemorrágico o teñido de meconio(OR= 9.00,IC95%:3.01-26.85,p=0.001), circular de cordón(OR=9.00,IC95%:3.59-22.52,p=0.001), peso al nacer igual ó <2500 gramos (OR=8.88,IC95%:3.73-21.15,p=0.001). Los subrayados y el síndrome hipertensivo asociado al embarazo se encontraron significativos en análisis multivariado. Conclusiones: Los factores de riesgo para asfixia perinatal fueron: antecedentes patológicos maternos, primigestación, abruptio de placenta, hemorragia del tercer trimestre, oligohidramnios, monitoreo fetal intraparto anormal, taquicardia y bradicardia fetal, expulsivo prolongado, corioamnionitis, fiebre materna, convulsiones maternas, género masculino, edad gestacional por BALLARD igual ó <36 semanas, vía del nacimiento instrumentado, líquido amniótico hemorrágico o teñido de meconio, circular de cordón, peso al nacer igual ó <2500 gramos.

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Background: Sexual risk behaviors associated with poor information on sexuality have contributed to major public health problems in the area of sexual and reproductive health in teenagers and young adults in Colombia. Objective: To measure the perception of changes in sexual and reproductive risk behavior after the use of a teleconsultation service via mobile devices in a sample of young adults. Methods: A before and after observational study was designed, where a mobile application to inquire about sexual and reproductive health was developed. The perception of changes in sexual and reproductive health risk behaviors in a sample of young adults after the use of the application was measured using the validated survey “Family Health International (FHI) – Behavioral Surveillance Survey (BSS) – Survey for Adults between 15 to 40 Years”. Non-probabilistic convenience recruitment was undertaken through the study´s web page. Participants answered the survey online before and after the use of the mobile application for a six month period (intervention). For the inferential analysis, data was divided into three groups (dichotomous data, discrete quantitative data, and ordinal data), to compare the results of the questions between the first and the second survey. For all tests, a confidence interval of 95% was established. For dichotomous data, the Chi-squared test was used. For quantitative data, we used the Student’s t-test, and for ordinal data, the Mann-Whitney-Wilcoxon test. Results: A total of 257 subjects were registered in the study and met the selection criteria. The pre-intervention survey was answered by 232 subjects, and 127 completely answered the post-intervention survey, of which 54.3% did not use the application, leaving an effective population of 58 subjects for analysis. 53% (n=31) were female, and 47% (n=27) were male. The mean age was 21 years, ranging between 18 and 40 years. The differences between the answers on the first and the second survey were not statistically significant. The main risk behaviors identified in the population were homosexual relations, non-use of condoms, sexual relations with non-regular and commercial partners, the use of psychoactive substances, and ignorance about the symptoms of sexually transmitted diseases and HIV transmission. Conclusions: Although there were no differences between the pre- and post-intervention results, the study revealed different risk behaviors among the participating subjects. These findings highlight the importance of promoting educational strategies on this matter and the importance of providing patients with easily accessible tools with reliable health information.

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Objetivo: evaluar la reproducibilidad prueba-reprueba y el nivel de acuerdo entre mediciones de las pruebas 30 seg (30-s) Arm Curl y 30-s Chair Stand en una muestra de adultos mayores de Bucaramanga. Materiales y métodos: se realizó un estudio de evaluación de tecnologías diagnósticas. Ambas pruebas fueron administradas en dos oportunidades por el mismo evaluador a 111 adultos mayores de 59 años (70,4 ± 7,3), con un intervalo de 4 a 8 días. En el análisis se determinó la reproducibilidad prueba-reprueba mediante el coeficiente de correlación intraclase, CCI= 2,1 con sus respectivos intervalos de confianza de 95% (IC 95%). El nivel de acuerdo se estableció mediante el método de Bland y Altman. Resultados: la reproducibilidad prueba-reprueba para el 30-s Arm Curl test fue muy buena, con un CCI= 0,88 y para el 30-s Chair Stand test fue buena,con un CCI= 0,78. Así, el acuerdo fue muy bueno para las dos pruebas de resistencia muscular. Los límites de acuerdo de 95% estuvieron entre -3,8 y 3,2 repeticiones para la prueba 30-s ChairStand y entre -3,1 y 2,8 repeticiones para la prueba 30-s Arm Curl. Conclusión: las pruebas 30-s Arm Curl y 30-s Chair Stand tienen buena reproducibilidad y nivel de acuerdo para evaluar resistencia muscular en adultos mayores funcionalmente independientes.

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Objetivo: Establecer la relación de las condiciones de trabajo y salud con los desórdenes músculo-esqueléticos (DME) en los trabajadores asistenciales y administrativos de un hospital en Sogamoso, Boyacá, en el 2013. Metodología: Se llevó a cabo un estudio descriptivo con una muestra de 90 trabajadores, correspondiente al 22%, de 405 incluyendo médicos, jefes de enfermería, auxiliar de enfermería, auxiliares administrativos y profesionales administrativos. Se aplicó una encuesta para determinar las condiciones de trabajo y salud y para el análisis de los síntomas de desorden músculo esquelético, junto con la toma de estatura y peso para calcular el índice de masa corporal. En el análisis de las variables cuantitativas se utilizó medidas de tendencia central y dispersión; para las variables cualitativas se calculó frecuencias absolutas y porcentajes. Se realizó pruebas de asociación Chi cuadrado y se estimó las medidas OR crudas y ajustadas por medio de un modelo de regresión binaria logística, con sus respectivos intervalos de confianza. Resultados: La población estuvo conformada por 78 mujeres (86.7%) y 12 hombres (13.3%), con edades entre 24 y 56 años. Los cargos más representativos fueron el Auxiliar Administrativo y el Auxiliar de Enfermería con el 35.6% (32) y 38.9% (35) respectivamente. Los síntomas de DME más frecuentes se ubicaron en la espalda y en mano afectando al 58.9% (53) y 45.6% (41) respectivamente. Según el 93.3% de los participantes, el factor de riesgo biomecánico que tiene alta influencia en los DME es la realización de movimientos repetidos. Se encontró para los Médicos un Odds Ratio (OR) 4.2; de DME, mientras que para los Auxiliares Administrativos tienen un OR 2.9 y presentan mayor posibilidad de padecer DME que un Auxiliar de Enfermería.

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Introducción: La utilidad de la tomografía computarizada como prueba de rutina en la toma de decisiones para las fracturas de radio distal no ha sido bien establecida. Metodología: Estudio de concordancia intra e interobservador en el tratamiento de fracturas de radio distal Fernández V. Se realizaron dos visitas, con intervalo de 2 semanas entre ellas a 15 ortopedistas de trauma quienes evaluaron 22 radiografías de muñeca y sus respectivas tomografías con fracturas de radio distal Fernández V, determinaron para cada caso la mejor opción de tratamiento. Se utilizó el coeficiente Kappa para evaluar la concordancia intra e interobservador para el plan de tratamiento propuesto y se analizaron los resultados según la interpretación de este coeficiente según Landis y Koch. Resultados: La concordancia entre radiografía y tomografía fue moderada kappa 0,47 – 0,51 en las dos evaluaciones respectivamente, manteniéndose el cambio de tratamiento entre 24,9% y 26,7% (p‹0,001). La concordancia observada intraobservador para radiografía y tomografía evaluadas de manera individual fue buena (72,1% y 64,2% respectivamente) evidenciándose cambio en la decisión de tratamiento hasta en el 35,8% de las evaluaciones (p‹0,001); se determinó concordancia observada muy buena en los casos a los que se propuso manejo abierto. No se identificó influencia de la edad en la decisión de tratamiento. Conclusiones: Existe buena concordancia entre radiografía simple y tomografía en fracturas de radio distal Fernández V en cuanto a la decisión de tratamiento, siendo alta la concordancia en los casos en los que se decide manejo abierto.

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Objetivo Determinar la prevalencia de dolor lumbar y su relación con los factores de riesgo biomecánico en el personal de enfermería de una entidad de salud de cuarto nivel en la ciudad de Bogotá, entre el año 2014 y 2015. Esta investigación se realizó teniendo en cuenta que el dolor lumbar tiene un alto impacto en la calidad de vida del personal de enfermería. Materiales y métodos: Es un estudio de corte transversal con exploración analítica. La población objeto de estudio está conformada por 866 trabajadores de enfermería de la cual se tomó una muestra de 265 individuos a los cuales se les aplicó un cuestionario online que indagó acerca de las características individuales, laborales de riesgo biomecánico. En la elaboración del instrumento se seleccionaron ítems de Ergopar y Nórdico. La muestra fue aleatoria, estratificada con distribución proporcional por servicio de atención y jornada laboral. Resultados La prevalencia de dolor lumbar en la población estudiada fue del 61.1% (n=162) con un intervalo de confianza del 95% (55.1-67.2). Los factores de riesgo biomecánico asociados al problema de estudio fueron: posturas que implican girar y/o inclinar la espalda o el tronco (p 0.05), y tiempo de movilización de pacientes (p 0.01). Los factores a nivel laboral que se relacionan con el dolor lumbar son: el tipo de contrato (p 0.002), las exigencias físicas del trabajo (p 0.001) y la imposibilidad para realizar el trabajo por causa del dolor lumbar (p 0.000). La prevalencia por servicios y la jornada laboral no presentaron asociación significativa. Conclusiones La prevalencia de dolor lumbar en personal de enfermería es alta y coincide con los estudios realizados a nivel nacional e internacional. La exposición a los factores de riesgo biomecánico que se relacionan con la presencia de dolor lumbar en el personal de enfermería, afectan su calidad de vida. Además, no existen diferencias significativas de acuerdo con las funciones de los cargos desempeñados.

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From several small stratigraphic sections, we have reconstituted the Liassic interval of the Girona Province (NE Spain). We have been able to identify paleontologically the Carixian (Jamesoni, Ibex, and perhaps, Davoei zones), the Lower Domerian (Stockesi zone), and the Middle Toarcian (possibily Variabilis zone, as well as Thouarsense and Insigne zones). The Lower Toarcian (Serpentinus zone) is represented by fossil remains no ‘in situ’. The lowest Toarcián (Tenuicos-tatum zone) as well as the Middle and Upper Domerian (Margaritatus and Spinatum zones respectively, are probably represented by stratigraphic gaps

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Large temperature variations on land, in the air, and at the ocean surface, and highly variable flux of ice-rafted debris (IRD) delivered to the North Atlantic Ocean show that rapid climate fluctuations took place during the last glacial period. These quasi-periodic, high-amplitude climate variations followed a sequence of events recognized as a rapid warming, followed by a phase of gradual cooling, and terminating with more rapid cooling and increased flux of IRD to the north Atlantic Ocean. Each cycle lasted ˜1500 years, and was followed by an almost identical sequence. These cycles are referred to as Dansgaard/Oechger cycles (D/O cycles), and approximately every fourth cycle culminated in a more pronounced cooling with a massive discharge of IRD into the north Atlantic Ocean over an interval of ˜500 years. These massive discharges of IRD are known as Heinrich layers. “Heinrich events” are thus characterized as a rapid transfer of IRD from a “source,” the bed of the Laurentide Ice Sheet (LIS), to a “sink,” the North Atlantic.

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Varroa destructor is a parasitic mite of the Eastern honeybee Apis cerana. Fifty years ago, two distinct evolutionary lineages (Korean and Japanese) invaded the Western honeybee Apis mellifera. This haplo-diploid parasite species reproduces mainly through brother sister matings, a system which largely favors the fixation of new mutations. In a worldwide sample of 225 individuals from 21 locations collected on Western honeybees and analyzed at 19 microsatellite loci, a series of de novo mutations was observed. Using historical data concerning the invasion, this original biological system has been exploited to compare three mutation models with allele size constraints for microsatellite markers: stepwise (SMM) and generalized (GSM) mutation models, and a model with mutation rate increasing exponentially with microsatellite length (ESM). Posterior probabilities of the three models have been estimated for each locus individually using reversible jump Markov Chain Monte Carlo. The relative support of each model varies widely among loci, but the GSM is the only model that always receives at least 9% support, whatever the locus. The analysis also provides robust estimates of mutation parameters for each locus and of the divergence time of the two invasive lineages (67,000 generations with a 90% credibility interval of 35,000-174,000). With an average of 10 generations per year, this divergence time fits with the last post-glacial Korea Japan land separation. (c) 2005 Elsevier Inc. All rights reserved.

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High-resolution satellite radar observations of erupting volcanoes can yield valuable information on rapidly changing deposits and geomorphology. Using the TerraSAR-X (TSX) radar with a spatial resolution of about 2 m and a repeat interval of 11-days, we show how a variety of techniques were used to record some of the eruptive history of the Soufriere Hills Volcano, Montserrat between July 2008 and February 2010. After a 15-month pause in lava dome growth, a vulcanian explosion occurred on 28 July 2008 whose vent was hidden by dense cloud. We were able to show the civil authorities using TSX change difference images that this explosion had not disrupted the dome sufficient to warrant continued evacuation. Change difference images also proved to be valuable in mapping new pyroclastic flow deposits: the valley-occupying block-and-ash component tending to increase backscatter and the marginal surge deposits reducing it, with the pattern reversing after the event. By comparing east- and west-looking images acquired 12 hours apart, the deposition of some individual pyroclastic flows can be inferred from change differences. Some of the narrow upper sections of valleys draining the volcano received many tens of metres of rockfall and pyroclastic flow deposits over periods of a few weeks. By measuring the changing shadows cast by these valleys in TSX images the changing depth of infill by deposits could be estimated. In addition to using the amplitude data from the radar images we also used their phase information within the InSAR technique to calculate the topography during a period of no surface activity. This enabled areas of transient topography, crucial for directing future flows, to be captured.

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Global efforts to mitigate climate change are guided by projections of future temperatures1. But the eventual equilibrium global mean temperature associated with a given stabilization level of atmospheric greenhouse gas concentrations remains uncertain1, 2, 3, complicating the setting of stabilization targets to avoid potentially dangerous levels of global warming4, 5, 6, 7, 8. Similar problems apply to the carbon cycle: observations currently provide only a weak constraint on the response to future emissions9, 10, 11. Here we use ensemble simulations of simple climate-carbon-cycle models constrained by observations and projections from more comprehensive models to simulate the temperature response to a broad range of carbon dioxide emission pathways. We find that the peak warming caused by a given cumulative carbon dioxide emission is better constrained than the warming response to a stabilization scenario. Furthermore, the relationship between cumulative emissions and peak warming is remarkably insensitive to the emission pathway (timing of emissions or peak emission rate). Hence policy targets based on limiting cumulative emissions of carbon dioxide are likely to be more robust to scientific uncertainty than emission-rate or concentration targets. Total anthropogenic emissions of one trillion tonnes of carbon (3.67 trillion tonnes of CO2), about half of which has already been emitted since industrialization began, results in a most likely peak carbon-dioxide-induced warming of 2 °C above pre-industrial temperatures, with a 5–95% confidence interval of 1.3–3.9 °C.

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Extended cusp-like regions (ECRs) are surveyed, as observed by the Magnetospheric Ion Composition Sensor (MICS) of the Charge and Mass Magnetospheric Ion Composition Experiment (CAMMICE) instrument aboard Polar between 1996 and 1999. The first of these ECR events was observed on 29 May 1996, an event widely discussed in the literature and initially thought to be caused by tail lobe reconnection due to the coinciding prolonged interval of strong northward IMF. ECRs are characterized here by intense fluxes of magnetosheath-like ions in the energy-per-charge range of _1 to 10 keV e_1. We investigate the concurrence of ECRs with intervals of prolonged (lasting longer than 1 and 3 hours) orientations of the IMF vector and high solar wind dynamic pressure (PSW). Also investigated is the opposite concurrence, i.e., of the IMF and high PSW with ECRs. (Note that these surveys are asking distinctly different questions.) The former survey indicates that ECRs have no overall preference for any orientation of the IMF. However, the latter survey reveals that during northward IMF, particularly when accompanied by high PSW, ECRs are more likely. We also test for orbital and seasonal effects revealing that Polar has to be in a particular region to observe ECRs and that they occur more frequently around late spring. These results indicate that ECRs have three distinct causes and so can relate to extended intervals in (1) the cusp on open field lines, (2) the magnetosheath, and (3) the magnetopause indentation at the cusp, with the latter allowing magnetosheath plasma to approach close to the Earth without entering the magnetosphere.

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Optical observations of a dayside auroral brightening sequence, by means of all-sky TV cameras and meridian scanning photometers, have been combined with EISCAT ion drift observations within the same invariant latitude-MLT sector. The observations were made during a January 1989 campaign by utilizing the high F region ion densities during the maximum phase of the solar cycle. The characteristic intermittent optical events, covering ∼300 km in east-west extent, move eastward (antisunward) along the poleward boundary of the persistent background aurora at velocities of ∼1.5 km s−1 and are associated with ion flows which swing from eastward to westward, with a subsequent return to eastward, during the interval of a few minutes when there is enhanced auroral emission within the radar field of view. The breakup of discrete auroral forms occurs at the reversal (negative potential) that forms between eastward plasma flow, maximizing near the persistent arc poleward boundary, and strong transient westward flow to the south. The reported events, covering a 35 min interval around 1400 MLT, are embedded within a longer period of similar auroral activity between 0830 (1200 MLT) and 1300 UT (1600 MLT). These observations are discussed in relation to recent models of boundary layer plasma dynamics and the associated magnetosphere-ionosphere coupling. The ionospheric events may correspond to large-scale wave like motions of the low-latitude boundary layer (LLBL)/plasma sheet (PS) boundary. On the basis of this interpretation the observed spot size, speed and repetition period (∼10 min) give a wavelength (the distance between spots) of ∼900 km in the present case. The events can also be explained as ionospheric signatures of newly opened flux tubes associated with reconnection bursts at the magnetopause near 1400 MLT. We also discuss these data in relation to random, patchy reconnection (as has recently been invoked to explain the presence of the sheathlike plasma on closed field lines in the LLBL). In view of the lack of IMF data, and the existing uncertainty on the location of the open-closed field line boundary relative to the optical events, an unambiguous discrimination between the different alternatives is not easily obtained.

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We present observations of a transient event in the dayside auroral ionosphere at magnetic noon. F-region plasma convection measurements were made by the EISCAT radar, operating in the beamswinging “Polar” experiment mode, and simultaneous observations of the dayside auroral emissions were made by optical meridian-scanning photometers and all-sky TV cameras at Ny Ålesund, Spitzbergen. The data were recorded on 9 January 1989, and a sequence of bursts of flow, with associated transient aurora, were observed between 08:45 and 11:00 U.T. In this paper we concentrate on an event around 09:05 U.T. because that is very close to local magnetic noon. The optical data show a transient intensification and widening (in latitude) of the cusp/cleft region, as seen in red line auroral emissions. Over an interval of about 10 min, the band of 630 nm aurora widened from about 1.5° of invariant latitude to over 5° and returned to its original width. Embedded within the widening band of 630 nm emissions were two intense, active 557.7 nm arc fragments with rays which persisted for about 2 min each. The flow data before and after the optical transient show eastward flows, with speeds increasing markedly with latitude across the band of 630 nm aurora. Strong, apparently westward, flows appeared inside the band while it was widening, but these rotated round to eastward, through northward, as the band shrunk to its original width. The observed ion temperatures verify that the flow speeds during the transient were, to a large extent, as derived using the beamswinging technique; but they also show that the flow increase initially occurred in the western azimuth only. This spatial gradient in the flow introduces ambiguity in the direction of these initial flows and they could have been north-eastward rather than westward. However, the westward direction derived by the beamswinging is consistent with the motion of the colocated and coincident active 557.7 nm arc fragment, A more stable transient 557.7 nm aurora was found close to the shear between the inferred westward flows and the persisting eastward flows to the North. Throughout the transient, northward flow was observed across the equatorward boundary of the 630 nm aurora. Interpretation of the data is made difficult by lack of IMF data, problems in distinguishing the cusp and cleft aurora and uncertainty over which field lines are open and which are closed. However, at magnetic noon there is a 50% probability that we were observing the cusp, in which case from its southerly location we infer that the IMF was southward and many features are suggestive of time-varying reconnection at a single X-line on the dayside magnetopause. This IMF orientation is also consistent with the polar rain precipitation observed simultaneously by the DMSP-F9 satellite in the southern polar cap. There is also a 25% chance that we were observing the cleft (or the mantle poleward of the cleft). In this case we infer that the IMF was northward and the transient is well explained by reconnection which is not only transient in time but occurs at various sites located randomly on the dayside magnetopause (i.e. patchy in space). Lastly, there is a 25% chance that we were observing the cusp poleward of the cleft, in which case we infer that IMF Bz was near zero and the transient is explained by a mixture of the previous two interpretations.