The effect of sun exposure on 25-hydroxyvitamin D concentrations in young healthy subjects living in the city of São Paulo, Brazil

The range of 25-hydroxyvitamin D (25OHD) concentration was determined in a young healthy population based on bone metabolism parameters and environmental and behavioral aspects. We studied 121 healthy young volunteers (49 men, 72 women) living in São Paulo (23º 34' south latitude) belonging to three occupational categories: indoor workers (N = 28), medical school students (N = 44), and resident physicians (N = 49). Fasting morning blood samples were collected once from each volunteer from August 2002 to February 2004, and 25OHD, total calcium, albumin, alkaline phosphatase, phosphorus, creatinine, intact parathyroid hormone, osteocalcin, and type I collagen carboxyterminal telopeptide were measured. Data are reported as means ± SD. Mean subject age was 24.7 ± 2.68 years and mean 25OHD level for the entire group was 78.7 ± 33.1 nM. 25OHD levels were lower (P < 0.05) among resident physicians (67.1 ± 27.0 nM) than among students (81.5 ± 35.8 nM) and workers (94.0 ± 32.6 nM), with the last two categories displaying no difference. Parathyroid hormone was higher (P < 0.05) and osteocalcin was lower (P < 0.05) among resident physicians compared to non-physicians. Solar exposure and frequency of beach outings showed a positive association with 25OHD (P < 0.001), and summer samples presented higher results than winter ones (97.8 ± 33.5 and 62.9 ± 23.5 nM, respectively). To define normal levels, parameters such as occupational activity, seasonality and habits related to solar exposure should be taken into account. Based on these data, we considered concentrations above 74.5 nM to be desired optimal 25OHD levels, which were obtained during the summer for 75% of the non-physicians.

Automated system of seedling image analysis (SVIS) and electrical conductivity to assess sun hemp seed vigor

The development of new procedures for quickly obtaining accurate information on the physiological potential of seed lots is essential for developing quality control programs for the seed industry. In this study, the effectiveness of an automated system of seedling image analysis (Seed Vigor Imaging System - SVIS) in determining the physiological potential of sun hemp seeds and its relationship with electrical conductivity tests, were evaluated. SVIS evaluations were performed three and four days after sowing and data on the vigor index and the length and uniformity of seedling growth were collected. The electrical conductivity test was made on 50 seed replicates placed in containers with 75 mL of deionised water at 25 ºC and readings were taken after 1, 2, 4, 8 and 16 hours of imbibition. Electrical conductivity measurements at 4 or 8 hours and the use of the SVIS on 3-day old seedlings can effectively detect differences in vigor between different sun hemp seed lots.

Reconstruction of the surface of the Sun from stereoscopic images

Mémoire numérisé par la Division de la gestion de documents et des archives de l'Université de Montréal

Nothing New (Ethically) Under the Sun: Policy & Clinical Implications of Nanomedicine

Article

Les effets politiques des spectacles médiatiques d’immigration : une analyse critique des discours de la presse écrite canadienne sur l’arrivée du MV Sun Sea

Ce mémoire de maîtrise porte sur les effets politiques des discours médiatiques sur la gouvernance et la régulation des demandeurs d’asile au Canada. À travers une analyse critique des discours de la presse écrite canadienne au sujet de l’arrivée en août 2010 de 492 requérants du statut de réfugié à bord du bateau MV Sun Sea en Colombie-Britannique, l’auteure identifie les principales interprétations de cet évènement ainsi que leurs relations avec la mise en place subséquente de mesures visant à restreindre les possibilités d’accès non autorisés au Canada, notamment par la création d’une nouvelle catégorisation discriminatoire des demandeurs d’asile. L’analyse révèle l’articulation de ces discours autour de deux thématiques distinctes, mais interreliées. Tandis que les discours sécuritaires associent l’arrivée non autorisée des demandeurs d’asile à une menace à la sécurité de la nation, les discours humanitaires interprètent cet évènement comme une demande d’aide de la part d’un groupe de personnes menacées par leur propre pays. Ce mémoire propose une analyse multidimensionnelle de ces deux cadrages et de leurs effets politiques qui considère leurs dimensions discursives, contextuelles et affectives. L’analyse démontre comment ces deux discours en apparence conflictuels partagent en fait un même sous-texte racial qui fait de ce type de spectacle médiatique un dispositif clé de « gouvernementalité racialisée de l’immigration » (Bilge, 2012, 2013).

Aporte de Oriente a las empresas de Occidente Sun Tzu un clásico de la estrategia.

Quienes no hayan escuchado el nombre Sun Tzu podrían imaginar muchas cosas sobre quién es esa persona. Sun Tzu es un general oriental que escribió su libro El arte de la guerra hace más de 21 siglos. Es un libro que a través de la narración de situaciones propias de un ejército enseña a las empresas a enfrentarse a un mercado complejo mediante la formulación, selección e implementación de la estrategia. Este artículo hace una interpretación de los 13 capítulos, buscando que aquellos que se encuentran al frente de una empresa cuenten con una lectura que les permita encontrar elementos para asegurar la perdurabilidad de su  organización.

Las Jarretaderas, Nayarit, Mexico: a Social Interstice in Touristic Zona Metropolitana of Sun and Sand

The objective of the present article is to illustrate the social interstice (Las Jarretaderas) existing between the municipalities Bahía de Banderas, Nayarit and Puerto Vallarta, Jalisco. The researched community is an outstanding case-study providing an in-depth analysis of a number of social process mostly related to the chiapaneca migration. The text is divided into two sections. The first one deals with the urbanization process of the metropolitan area of Puerto Vallarta. The second and longer section defines the concept of social interstice and explains how the researched locality falls under under that previously-defined concept according to the processes analyzed.

I wonder why the sun rises : and other questions about time and seasons.

Pertenece a una colección que quiere responder a las preguntas que se hacen los jóvenes lectores sobre el tiempo y las estaciones del año. Podemos conocer las respuestas a temas como la duración del día según la época del año, la influencia de la latitud para que haya cuatro o menos estaciones; la creación del calendario, la forma de medir con exactitud el tiempo, la diferencia horaria en los distintos países del mundo.

I wonder why the sun rises : and other questions about time and seasons.

Pertenece a una colección que quiere responder a las preguntas que se hacen los jóvenes lectores sobre el tiempo y las estaciones del año. Podemos conocer las respuestas a temas como la duración del día según la época del año, la influencia de la latitud para que haya cuatro o menos estaciones; la creación del calendario, la forma de medir con exactitud el tiempo, la diferencia horaria en los distintos países del mundo.

The sun.

Desde tiempos muy antiguos, personas de todo el mundo se han dado cuenta de la importancia del Sol y en torno a él se han creado historias y leyendas, e incluso, se le ha adorado como a un dios. Es una estrella que parece una enorme bola de gas ardiente, muy brillante, que gira en el cielo y está muy alejada de la Tierra. Gracias al sol se suceden los días y las noches y las estaciones en nuestro planeta. Es nuestro amigo pues sus rayos calientes y brillantes hacen posible la existencia de vida, y la acumulación de su calor produce un tipo de energía; pero los humos y gases y algunos productos originan contaminación sobre la tierra, dañan la capa de ozono y la aparición del llamado efecto invernadero.

Predicting magnetospheric dynamics with a coupled sun-to-Earth model: challenges and first results

Results from the first Sun-to-Earth coupled numerical model developed at the Center for Integrated Space Weather Modeling are presented. The model simulates physical processes occurring in space spanning from the corona of the Sun to the Earth's ionosphere, and it represents the first step toward creating a physics-based numerical tool for predicting space weather conditions in the near-Earth environment. Two 6- to 7-d intervals, representing different heliospheric conditions in terms of the three-dimensional configuration of the heliospheric current sheet, are chosen for simulations. These conditions lead to drastically different responses of the simulated magnetosphere-ionosphere system, emphasizing, on the one hand, challenges one encounters in building such forecasting tools, and on the other hand, emphasizing successes that can already be achieved even at this initial stage of Sun-to-Earth modeling.

From the sun to the Earth: The 13 May 2005 coronal mass ejection

We report the results of a multi-instrument, multi-technique, coordinated study of the solar eruptive event of 13 May 2005. We discuss the resultant Earth-directed (halo) coronal mass ejection (CME), and the effects on the terrestrial space environment and upper Earth atmosphere. The interplanetary CME (ICME) impacted the Earth’s magnetosphere and caused the most-intense geomagnetic storm of 2005 with a Disturbed Storm Time (Dst) index reaching −263 nT at its peak. The terrestrial environment responded to the storm on a global scale. We have combined observations and measurements from coronal and interplanetary remote-sensing instruments, interplanetary and near-Earth in-situ measurements, remote-sensing observations and in-situ measurements of the terrestrial magnetosphere and ionosphere, along with coronal and heliospheric modelling. These analyses are used to trace the origin, development, propagation, terrestrial impact, and subsequent consequences of this event to obtain the most comprehensive view of a geo-effective solar eruption to date. This particular event is also part of a NASA-sponsored Living With a Star (LWS) study and an on-going US NSF-sponsored Solar, Heliospheric, and INterplanetary Environment (SHINE) community investigation.

A solar storm observed from the Sun to Venus using the STEREO, Venus Express, and MESSENGER spacecraft

The suite of SECCHI optical imaging instruments on the STEREO-A spacecraft is used to track a solar storm, consisting of several coronal mass ejections (CMEs) and other coronal loops, as it propagates from the Sun into the heliosphere during May 2007. The 3-D propagation path of the largest interplanetary CME (ICME) is determined from the observations made by the SECCHI Heliospheric Imager (HI) on STEREO-A (HI-1/2A). Two parts of the CME are tracked through the SECCHI images, a bright loop and a V-shaped feature located at the rear of the event. We show that these two structures could be the result of line-of-sight integration of the light scattered by electrons located on a single flux rope. In addition to being imaged by HI, the CME is observed simultaneously by the plasma and magnetic field experiments on the Venus Express and MESSENGER spacecraft. The imaged loop and V-shaped structure bound, as expected, the flux rope observed in situ. The SECCHI images reveal that the leading loop-like structure propagated faster than the V-shaped structure, and a decrease in in situ CME speed occurred during the passage of the flux rope.We interpret this as the result of the continuous radial expansion of the flux rope as it progressed outward through the interplanetary medium. An expansion speed in the radial direction of ~30 km s-1 is obtained directly from the SECCHI-HI images and is in agreement with the difference in speed of the two structures observed in situ. This paper shows that the flux rope location can be determined from white light images, which could have important space weather applications.