Carta Circular de la Red de Cooperación en la Gestión Integral de Recursos Hídricos para el Desarrollo Sustentable en América Latina y el Caribe N° 41

El tema del diseño de sistemas apropiados de gestión del agua reviste enorme importancia para América Latina y el Caribe. En este documento, se destaca la asistencia técnica dada a un gran número de países en la formulación y puesta en marcha de leyes, regulaciones y políticas públicas relacionadas con los recursos hídricos. Esto siempre hecho bajo la óptica de que la inserción sustentable del agua en la economía y en la sociedad depende de un adecuado equilibrio entre intereses públicos, ambientales, económicos, sociales y privados.

Impactos y vulnerabilidad al cambio climático de los principales ríos de Mendoza y San Juan a partir de la evolución de los glaciares cordilleranos: la economía del cambio climático en la Argentina

Mendoza y San Juan son las provincias de la región de Cuyo con recursos hídricos de origen netamente cordilleranos. El hidrograma de los ríos cuyanos se está modificado debido principalmente al aumento de la temperatura. De incrementarse la tendencia observada en la temperatura esta alteración podría tener un alto impacto en el manejo y regulación de los caudales. En este documento se muestran los resultados de dos estudios para esta región. El primero evalúa el comportamiento de las tendencias en la variabilidad de las precipitaciones, la temperatura, los caudales y el hidrograma frente a escenarios de cambio climático. Las cuencas más afectadas serían aquellas ubicadas hacia el sur de la región porque son las más bajas, en las cuales la disminución de las superficies alcanzaría porcentajes entre el 75% y 80% para fines de este siglo, con respecto a las superficies actuales. En estas condiciones es previsible una disminución de la superficie de los glaciares, con un fuerte retroceso de los mismos y la pérdida consiguiente de la reserva de agua en ellos almacenada. En la segunda parte del documento se cuantifica el impacto socioeconómico del cambio climático en las cuencas de Mendoza y San Juan. La reducción de los derrames de los ríos (oferta), el aumento de la demanda y los procesos de degradación del agua, determinaría el aumento del valor social marginal del agua. Mediante modelos de simulación se trazó el valor de corte entre oferta y demanda en el tiempo. La posición y trayectoria temporal del valor social marginal del agua, revelará la magnitud de la escasez, y la velocidad con que esta se incrementa. Estos indican el costo social de la escasez y robustez de la sustentabilidad en cada caso. Se realizan distintas corridas bajo escenarios alternativos para cada cuenca, lo que permite identificar políticas óptimas.

Los medios de comunicación social y su incidencia en el desarrollo local en el canton y Provincia de Zamorra Chinchipe - Ecuador

Analisa a diversidade de formas dos sistemas de comunicação em Zamora - no Equador, os relacionamentos da instituição, participação social e mídias sociais a partir da produção e emissão radiofônica, televisão, comunicação impressa (escrita) e a presença das novas tecnologias na comunicação, tentando achar espaços dos quais seja possível desenvolver práticas alternativas e democráticas para contribuir com o desenvolvimento social. Examina as práticas de comunicação radiofônica, sendo um dos meios principais e com maior tradição na área. Estuda o rádio, particularmente local, analisando seus modelos e programações, observando em cada um deles suas características, objetivos e estratégias assumidas desde sua visão comercial ou ideológica, seu nível profissional e inovação técnica, prestando atenção e nomeando valor à posição critica dos ouvintes, para interpretar as tendências atuais e futuras que se apresentam para eles.Finalmente, chegou-se à comunicação no contexto, examinando os usos e formas, como também a influencia positiva ou negativa na formação da identidade, harmonia com o ambiente, valores e conhecimento em perspectiva de melhorar a qualidade da vida da população. A investigação apóia-se no conhecimento cientifico, pois aplica a técnica qualitativa: Diversidade de grupos focais, entrevistas, observação e uso de investigação bibliográfica.O trabalho considera a historia, a dinâmica própria e a estima que tem os Zamoranos da percepção de sua identificação no contexto de códigos, idiomas e bens, postura desde a qual eles estabelecem normas que devem ser usadas para o seu uso, enquanto permitem articular pontos de vista, analise e conceitos, examinar a teoria para entender o papel que melhor desempenham as mídias sociais e sua importância na sociedade.

Planeamiento y análisis integral del paisaje de la cuenca hidrográfica del río buenavista provincia de Manabí-Ecuador para la implementación de políticas de incentivos a la restauración de ecosistemas con fines de conservación (programa socio Bosque-Ecuador)

Pós-graduação em Geografia - FCT

A search for anisotropy in the arrival directions of ultra high energy cosmic rays recorded at the Pierre Auger Observatory

Observations of cosmic rays arrival directions made with the Pierre Auger Observatory have previously provided evidence of anisotropy at the 99% CL using the correlation of ultra high energy cosmic rays (UHECRs) with objects drawn from the Veron-Cetty Veron catalog. In this paper we report on the use of three catalog independent methods to search for anisotropy. The 2pt-L, 2pt+ and 3pt methods, each giving a different measure of self-clustering in arrival directions, were tested on mock cosmic ray data sets to study the impacts of sample size and magnetic smearing on their results, accounting for both angular and energy resolutions. If the sources of UHECRs follow the same large scale structure as ordinary galaxies in the local Universe and if UHECRs are deflected no more than a few degrees, a study of mock maps suggests that these three method can efficiently respond to the resulting anisotropy with a P-value = 1.0% or smaller with data sets as few as 100 events. using data taken from January 1, 2004 to July 31, 2010 we examined the 20, 30, ... , 110 highest energy events with a corresponding minimum energy threshold of about 49.3 EeV. The minimum P-values found were 13.5% using the 2pt-L method, 1.0% using the 2pt+ method and 1.1% using the 3pt method for the highest 100 energy events. In view of the multiple (correlated) scans performed on the data set, these catalog-independent methods do not yield strong evidence of anisotropy in the highest energy cosmic rays.

Description of atmospheric conditions at the Pierre Auger Observatory using the Global Data Assimilation System (GDAS)

Atmospheric conditions at the site of a cosmic ray observatory must be known for reconstructing observed extensive air showers. The Global Data Assimilation System (GDAS) is a global atmospheric model predicated on meteorological measurements and numerical weather predictions. GDAS provides altitude-dependent profiles of the main state variables of the atmosphere like temperature, pressure, and humidity. The original data and their application to the air shower reconstruction of the Pierre Auger Observatory are described. By comparisons with radiosonde and weather station measurements obtained on-site in Malargue and averaged monthly models, the utility of the GDAS data is shown. (C) 2012 Elsevier B.V. All rights reserved.

The rapid atmospheric monitoring system of the Pierre Auger Observatory

The Pierre Auger Observatory is a facility built to detect air showers produced by cosmic rays above 10(17) eV. During clear nights with a low illuminated moon fraction, the UV fluorescence light produced by air showers is recorded by optical telescopes at the Observatory. To correct the observations for variations in atmospheric conditions, atmospheric monitoring is performed at regular intervals ranging from several minutes (for cloud identification) to several hours (for aerosol conditions) to several days (for vertical profiles of temperature, pressure, and humidity). In 2009, the monitoring program was upgraded to allow for additional targeted measurements of atmospheric conditions shortly after the detection of air showers of special interest, e. g., showers produced by very high-energy cosmic rays or showers with atypical longitudinal profiles. The former events are of particular importance for the determination of the energy scale of the Observatory, and the latter are characteristic of unusual air shower physics or exotic primary particle types. The purpose of targeted (or "rapid") monitoring is to improve the resolution of the atmospheric measurements for such events. In this paper, we report on the implementation of the rapid monitoring program and its current status. The rapid monitoring data have been analyzed and applied to the reconstruction of air showers of high interest, and indicate that the air fluorescence measurements affected by clouds and aerosols are effectively corrected using measurements from the regular atmospheric monitoring program. We find that the rapid monitoring program has potential for supporting dedicated physics analyses beyond the standard event reconstruction.

SEARCH FOR POINT-LIKE SOURCES OF ULTRA-HIGH ENERGY NEUTRINOS AT THE PIERRE AUGER OBSERVATORY AND IMPROVED LIMIT ON THE DIFFUSE FLUX OF TAU NEUTRINOS

The surface detector array of the Pierre Auger Observatory can detect neutrinos with energy E-nu between 10(17) eV and 10(20) eV from point-like sources across the sky south of +55 degrees and north of -65 degrees declinations. A search has been performed for highly inclined extensive air showers produced by the interaction of neutrinos of all flavors in the atmosphere (downward-going neutrinos), and by the decay of tau leptons originating from tau neutrino interactions in Earth's crust (Earth-skimming neutrinos). No candidate neutrinos have been found in data up to 2010 May 31. This corresponds to an equivalent exposure of similar to 3.5 years of a full surface detector array for the Earth-skimming channel and similar to 2 years for the downward-going channel. An improved upper limit on the diffuse flux of tau neutrinos has been derived. Upper limits on the neutrino flux from point-like sources have been derived as a function of the source declination. Assuming a differential neutrino flux k(PS) . E-nu(-2). from a point-like source, 90% confidence level upper limits for k(PS) at the level of approximate to 5x10(-7) and 2.5x10(-6) GeV cm(-2) s(-1) have been obtained over a broad range of declinations from the searches for Earth-skimming and downward-going neutrinos, respectively.

A search for point sources of EeV neutrons

A thorough search of the sky exposed at the Pierre Auger Cosmic Ray Observatory reveals no statistically significant excess of events in any small solid angle that would be indicative of a flux of neutral particles from a discrete source. The search covers from -90 degrees to +15 degrees in declination using four different energy ranges above 1 EeV (10(18) eV). The method used in this search is more sensitive to neutrons than to photons. The upper limit on a neutron flux is derived for a dense grid of directions for each of the four energy ranges. These results constrain scenarios for the production of ultrahigh energy cosmic rays in the Galaxy.

LARGE-SCALE DISTRIBUTION OF ARRIVAL DIRECTIONS OF COSMIC RAYS DETECTED ABOVE 10(18) eV AT THE PIERRE AUGER OBSERVATORY

A thorough search for large-scale anisotropies in the distribution of arrival directions of cosmic rays detected above 10(18) eV at the Pierre Auger Observatory is presented. This search is performed as a function of both declination and right ascension in several energy ranges above 10(18) eV, and reported in terms of dipolar and quadrupolar coefficients. Within the systematic uncertainties, no significant deviation from isotropy is revealed. Assuming that any cosmic-ray anisotropy is dominated by dipole and quadrupole moments in this energy range, upper limits on their amplitudes are derived. These upper limits allow us to test the origin of cosmic rays above 10(18) eV from stationary Galactic sources densely distributed in the Galactic disk and predominantly emitting light particles in all directions.

Measurement of the proton-air cross section at root s=57 TeV with the Pierre Auger Observatory

We report a measurement of the proton-air cross section for particle production at the center-of-mass energy per nucleon of 57 TeV. This is derived from the distribution of the depths of shower maxima observed with the Pierre Auger Observatory: systematic uncertainties are studied in detail. Analyzing the tail of the distribution of the shower maxima, a proton-air cross section of [505 +/- 22(stat)(-36)(+28)(syst)] mb is found.

Alcances y limitaciones actuales de la actividad experimental en escuelas de Enseñanza Media de la provincia Santiago de Cuba: criterios de alumnos y profesores

El propósito de este estudio es explorar el estado actual de desarrollo de las actividades experimentales en la asignatura de Física en escuelas de Enseñanza Media de la provincia de Santiago de Cuba ya que constituye un aspecto medular en la construcción del conocimiento científico. Para la recogida de la información se utilizaron dos instrumentos: una encuesta y una entrevista que fueron aplicadas a 268 alumnos y 18 profesores de cinco escuelas con entornos socioculturales diferentes. Los datos obtenidos de las encuestas de ambos sujetos están referidos a: la existencia o no de infraestructura de laboratorio en las escuelas, las características de sus participaciones en los laboratorios y la frecuencia de realización de los mismos. Complementan esta información sus opiniones expresadas en las respuestas a las entrevistas, donde se destaca el papel que atribuyen a los experimentos en el proceso de enseñanza-aprendizaje. Los resultados indican un incremento en la motivación y en la asimilación de los contenidos por parte de los alumnos que participaron en las demostraciones experimentales en las escuelas con infraestructura de laboratorio. Se manifiestan también limitaciones en el orden material con énfasis en las escuelas más alejadas del centro de la ciudad de Santiago de Cuba y de preparación de los profesores para una eficiente utilización del instrumental que poseen en función de la docencia.