Effects of physical activity program based on technological progress: exer-games as health promoters

La finalidad de este trabajo es analizar la mejora en la salud y calidad de vida de los niños/as y jóvenes detectados con sedentarismo y/o sobrepeso, mediante la aplicación de un programa de entrenamiento basado en los entornos virtuales motrices. En el estudio participaron un total de 359 niños y niñas de entre 3 y 12 años pertenecientes a cuatro centros escolares, de los que se seleccionaron 20 niños de entre 5 y 12 años, para formar dos grupos de 10 niños/as cada uno. El grupo experimental llevó a cabo el programa de entrenamiento, junto a pautas nutricionales, mientras que el grupo control no tuvo ninguna intervención. Las variables analizadas fueron el IMC y perímetro de la cintura, mediante mediciones antropométricas, el tiempo de uso de pantalla, el tipo de desplazamiento al colegio y el nivel de adherencia a la dieta mediterránea, medidos mediante cuestionario, y la imagen corporal, evaluado a través de las siluetas. Para complementar la investigación, se efectuaron valoraciones nutricionales iniciales y finales al grupo experimental. Se analizaron los estadísticos descriptivos para todas las variables, calculando para las variables cuantitativas la media, mediana y desviación típica; porcentajes y frecuencias para las variables cualitativas. Los resultados obtenidos pueden indicar que un programa de intervención motriz basado en los entornos virtuales motrices contribuye a promover la salud de los escolares con rasgos de sedentarismo y/o sobrepeso.The purpose of this work is to analyse the improvement in the health and quality of life of children and youth detected with sedentary lifestyle and/or overweight, through the application of a training program based on exer-games. A total of 359 boys and girls between the ages of 3 and 12 from four schools participated in the study, from which 20 children between the ages of 5 and 12 were selected, to form two groups of 10 children each. The experimental group carried out the training program, together with nutritional guidelines, while the control group had no intervention. The variables analysed were the BMI and waist circumference, through anthropometric measurements, screen time, the type of commute to school and the level of adherence to the Mediterranean diet, measured by questionnaire, and body image, evaluated at through the silhouettes. To complement the research, initial and final nutritional evaluations were carried out on the experimental group. Descriptive statistics for all variables were analysed, calculating the mean, median and standard deviation for the quantitative variables; percentages and frequencies for qualitative variables. The results obtained may indicate that a motor intervention program based on exer-games contributes to promoting the health of students with sedentary and/or overweight traits

Advances in reconstructing the AMOC using sea surface observations of salinity

The Atlantic meridional overturning circulation (AMOC) is one of the main drivers of climate variability at decadal and longer time scales. As there are no direct multi-decadal observations of this key circulation, the reconstruction of past AMOC variations is essential. This work presents a step forward in reconstructing the AMOC using climate models and time-varying surface nudging of salinity and temperature data, for which independent multi-decadal observed series are available. A number of nudging protocols are explored in a perfect model framework to best reproduce the AMOC variability accommodating to the characteristics of SST and SSS available products. As reference SST products with sufficient space and time coverage are available, we here choose to focus on the limitations associated to SSS products with the goal of providing protocols using independent salinity products. We consider a global gridded dataset and, additionally, a coarser SSS dataset restricted to the Atlantic and with a quite low spatial resolution (order of 10 degrees vs. 2 for the model grid). We show how, using the latter, we can improve the efficiency of the nudging on the AMOC reconstruction by adding a high-resolution annual cycle to the coarse resolution SSS product as well as a spatial downscaling to account for SSS gradient. The final protocol retained for the coarse SSS data is able to reconstruct a 100-year long AMOC period (average of 10.18 Sv and a standard deviation of 1.39 Sv), with a correlation of 0.76 to the target and a RMSE of 0.99 Sv. These values can be respectively compared to 0.85 and 0.75 Sv when using the global salinity surface observations. This work provides a first step towards understanding the limitations and prospects of historical AMOC reconstructions using different sea surface salinity datasets for the surface nudging

Supplement: "Localization and broadband follow-up of the gravitational-wave transient GW150914" (2016, ApJL, 826, L13)

This Supplement provides supporting material for Abbott et al. (2016a). We briefly summarize past electromagnetic (EM) follow-up efforts as well as the organization and policy of the current EM follow-up program. We compare the four probability sky maps produced for the gravitational-wave transient GW150914, and provide additional details of the EM follow-up observations that were performed in the different bands

Localization and Broadband Follow-up of the Gravitational-wave Transient GW150914

A gravitational-wave (GW) transient was identified in data recorded by the Advanced Laser Interferometer Gravitational-wave Observatory (LIGO) detectors on 2015 September 14. The event, initially designated G184098 and later given the name GW150914, is described in detail elsewhere. By prior arrangement, preliminary estimates of the time, significance, and sky location of the event were shared with 63 teams of observers covering radio, optical, near-infrared, X-ray, and gamma-ray wavelengths with ground- and space-based facilities. In this Letter we describe the low-latency analysis of the GW data and present the sky localization of the first observed compact binary merger. We summarize the follow-up observations reported by 25 teams via private Gamma-ray Coordinates Network circulars, giving an overview of the participating facilities, the GW sky localization coverage, the timeline, and depth of the observations. As this event turned out to be a binary black hole merger, there is little expectation of a detectable electromagnetic (EM) signature. Nevertheless, this first broadband campaign to search for a counterpart of an Advanced LIGO source represents a milestone and highlights the broad capabilities of the transient astronomy community and the observing strategies that have been developed to pursue neutron star binary merger events. Detailed investigations of the EM data and results of the EM follow-up campaign are being disseminated in papers by the individual teams. </p

Multi-messenger Observations of a Binary Neutron Star Merger

On 2017 August 17 a binary neutron star coalescence candidate (later designated GW170817) with merger time 12:41:04 UTC was observed through gravitational waves by the Advanced LIGO and Advanced Virgo detectors. The Fermi Gamma-ray Burst Monitor independently detected a gamma-ray burst (GRB 170817A) with a time delay of ∼ 1.7 {{s}} with respect to the merger time. From the gravitational-wave signal, the source was initially localized to a sky region of 31 deg2 at a luminosity distance of {40}-8+8 Mpc and with component masses consistent with neutron stars. The component masses were later measured to be in the range 0.86 to 2.26 {M}ȯ . An extensive observing campaign was launched across the electromagnetic spectrum leading to the discovery of a bright optical transient (SSS17a, now with the IAU identification of AT 2017gfo) in NGC 4993 (at ∼ 40 {{Mpc}}) less than 11 hours after the merger by the One-Meter, Two Hemisphere (1M2H) team using the 1 m Swope Telescope. The optical transient was independently detected by multiple teams within an hour. Subsequent observations targeted the object and its environment. Early ultraviolet observations revealed a blue transient that faded within 48 hours. Optical and infrared observations showed a redward evolution over ∼10 days. Following early non-detections, X-ray and radio emission were discovered at the transient’s position ∼ 9 and ∼ 16 days, respectively, after the merger. Both the X-ray and radio emission likely arise from a physical process that is distinct from the one that generates the UV/optical/near-infrared emission. No ultra-high-energy gamma-rays and no neutrino candidates consistent with the source were found in follow-up searches. These observations support the hypothesis that GW170817 was produced by the merger of two neutron stars in NGC 4993 followed by a short gamma-ray burst (GRB 170817A) and a kilonova/macronova powered by the radioactive decay of r-process nuclei synthesized in the ejecta.</p

Análisis del rendimiento del sistema de juego defensivo 5: 1 posicional en balonmano

Los sistemas de juego constituyen la expresión más clara en la estrategia y el juego colectivo en este caso en función defensiva. En este trabajo se analiza un análisis comparativo entre los sistemas de juego defensivos más universales 6:0 y 5:1. Para ello hemos utilizado el programa informático SportCode Gamebreaker. La muestra la constiuyen 5 equipos de diferetes países participantes en el Campeonato del Mundo de Alemania de 2007.No data (2008)UE

Offensive zones in beach volleyball: differences by gender

Gender differences in anthropometric and athletic properties (e.g. strength) as well as the different net heights (2.24 vs. 2.43 m) on the same field size (8x16 m) would be reflected in the game. The literature about differences between male and female playing characteristics in beach volleyball is scarce. Therefore, the aim of this study was to analyse the differences by gender in the use of offensive zones. Study participants were 20 players (10 female and 10 male) who took part in the European Beach Volleyball Championship 2005 and 2006. Video recordings were made of the 659 points in eight matches played. The beach volleyball court was divided into six zones (z1 to z6). The results showed that men and women use different offensive zones and also were different in the percentages of ball out (15.53 and 27.38% respectively). Concretely, men players used more 1, 2, 4 and 5 zones and women 1 and 5 zones. A few differences were observed in the percentage the ball to the net (7.73 and 5.35% respectively). An understanding of the use of offensive zones is relevant to establish specific tactical training patterns for beach volleyball