5 resultados para Revalorización de lo local

em BORIS: Bern Open Repository and Information System - Berna - Suiça


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Neutral hydrogen atoms that travel into the heliosphere from the local interstellar medium (LISM) experience strong effects due to charge exchange and radiation pressure from resonant absorption and re-emission of Lyα. The radiation pressure roughly compensates for the solar gravity. As a result, interstellar hydrogen atoms move along trajectories that are quite different than those of heavier interstellar species such as helium and oxygen, which experience relatively weak radiation pressure. Charge exchange leads to the loss of primary neutrals from the LISM and the addition of new secondary neutrals from the heliosheath. IBEX observations show clear effects of radiation pressure in a large longitudinal shift in the peak of interstellar hydrogen compared with that of interstellar helium. Here, we compare results from the Lee et al. interstellar neutral model with IBEX-Lo hydrogen observations to describe the distribution of hydrogen near 1 AU and provide new estimates of the solar radiation pressure. We find over the period analyzed from 2009 to 2011 that radiation pressure divided by the gravitational force (μ) has increased slightly from μ = 0.94 ± 0.04 in 2009 to μ = 1.01 ± 0.05 in 2011. We have also derived the speed, temperature, source longitude, and latitude of the neutral H atoms and find that these parameters are roughly consistent with those of interstellar He, particularly when considering the filtration effects that act on H in the outer heliosheath. Thus, our analysis shows that over the period from 2009 to 2011, we observe signatures of neutral H consistent with the primary distribution of atoms from the LISM and a radiation pressure that increases in the early rise of solar activity.

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We report the first in situ measurements of neutral deuterium originating in the local interstellar medium (LISM) in Earth’s orbit. These measurements were performed with the IBEX-Lo camera on NASA’s interstellar boundary explorer (IBEX) satellite. All data from the spring observation periods of 2009 through 2011 have been analysed. In the three years of the IBEX mission time, the observation geometry and orbit allowed for a total observation time of 115.3 days for the LISM. However, the effects of the spinning spacecraft and the stepping through 8 energy channels mean that we are only observing the interstellar wind for a total time of 1.44 days, in which 2 counts for interstellar deuterium were collected. We report here a conservative number, because a possibility of systematic error or additional noise, though eliminated in our analysis to the best of our knowledge, only supports detection at a 1-sigma level. From these observations, we derive a ratio D/H = (5.8 ± 4.4) × 10-4 at 1 AU. After modelling the transport and loss of D and H from the termination shock to Earth’s orbit, we find that our result of D/HLISM = (1.6 ± 1.2) × 10-5 agrees with D/HLIC = (1.6 ± 0.4) × 10-5 for the local interstellar cloud. This weak interstellar signal is extracted from a strong terrestrial background signal consisting of sputter products from the sensor’s conversion surface. As reference, we accurately measure the terrestrial D/H ratio in these sputtered products and then discriminate this terrestrial background source. Because of the diminishing D and H signal at Earth’s orbit during the rising solar activity due to photoionisation losses and increased photon pressure, our result demonstrates that in situ measurements of interstellar deuterium in the inner heliosphere are only possible during solar minimum conditions.

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We report on a comprehensive signal processing procedure for very low signal levels for the measurement of neutral deuterium in the local interstellar medium from a spacecraft in Earth orbit. The deuterium measurements were performed with the IBEX-Lo camera on NASA’s Interstellar Boundary Explorer (IBEX) satellite. Our analysis technique for these data consists of creating a mass relation in three-dimensional time of flight space to accurately determine the position of the predicted D events, to precisely model the tail of the H events in the region where the H tail events are near the expected D events, and then to separate the H tail from the observations to extract the very faint D signal. This interstellar D signal, which is expected to be a few counts per year, is extracted from a strong terrestrial background signal, consisting of sputter products from the sensor’s conversion surface. As reference we accurately measure the terrestrial D/H ratio in these sputtered products and then discriminate this terrestrial background source. During the three years of the mission time when the deuterium signal was visible to IBEX, the observation geometry and orbit allowed for a total observation time of 115.3 days. Because of the spinning of the spacecraft and the stepping through eight energy channels the actual observing time of the interstellar wind was only 1.44 days. With the optimised data analysis we found three counts that could be attributed to interstellar deuterium. These results update our earlier work.

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Ethnobiology research contributes significantly to initiatives that aim to enhance food sovereignty among indigenous and/or traditional people. In Bolivia, one of the Latin-American countries that shows the highest poverty and undernourishment levels, the purpose of this research-action project was to enhance food sovereignty through the revitalization of the local ecological knowledge and to promote local technological innovation processes in the Andean community of Tallija-Confital. During a first step the endogenous knowledge and strategies related to food security and sovereignty were investigated, based on the principles and tools of the Revitalizing Participatory Research (RPR). In a second step local technical innovation processes were supported through a “knowledge dialogue” between exogenous and endogenous knowledge systems, focusing on the processing of the cañahua (Chenopodium pallidicaule Aellen) gluten. The research results demonstrate that Andean people have developed complex endogenous knowledge and strategies to adapt to socio-environmental changes that show a great potential to contribute to the enhancement of food sovereignty. Nevertheless, in the current globalized context that translates into new challenges for local communities, beyond the revitalization of local ecological knowledge, a dialogue between different knowledge systems can lead to important local technological innovation for the improvement of their well-being. Key words: food sovereignty, knowledge dialogue, endogenous development, technological innovation

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La medicina tradicional no solamente sigue vigente en los Andes bolivianos, sino constituye la opción de primera elección para las familias rurales. Un estudio realizado en dos comunidades de la Subcentral Waka Playa, Municipio Tapacarí, muestra que los campesinos quechua-hablantes de los valles interandinos integran el sistema tradicional con el sistema de salud formal en el marco de sus estrategias familiares, reflejando un diálogo ínter-ontológico entre diferentes concepciones de salud y de enfermedad. A lo largo de una larga interacción con su entorno natural, los pobladores de los Andes han desarrollado concepciones específicas sobre el ser humano, su relación con la naturaleza, la salud y la enfermedad. Este proceso resultó en un sistema de salud complejo, donde intervienen expertos locales como son los curanderos-adivinos y los parteros y que se basa en un amplio uso y conocimiento de la flora y fauna nativas. A parte de estos conocimientos especializados, la medicina tradicional andina se expresa también en las prácticas terapéuticas diarias de la población, transmitidas y re-inventadas de generación en generación en el contexto de la familia y de la comunidad. La introducción del sistema de salud formal en el área de estudio en los años 90, representado por una posta de salud, impactó las comunidades locales principalmente por el acceso a vacunas – y la consecuente erradicación de algunas enfermedades - y a métodos contraceptivos. Sin embargo, la biomedicina es todavía de acceso muy limitado además de, según la población local, no tener la capacidad para curar ciertas enfermedades locales como el “susto,” el “mal viento” o la “colerina”. Como en otras áreas del conocimiento ecológico local, se observa una pérdida general de los conocimientos vinculados a la medicina tradicional andina debido a varios factores socioeconómicos, el más impactante siendo el proceso masivo de migración de las zonas rurales a los centros urbanos y al trópico boliviano. Sin embargo, estos conocimientos todavía se mantienen vigentes y son altamente valorizados por la población local, como un elemento del mantenimiento de sus formas de vida y de relacionamiento con la “Madre Tierra” (Pachamama). Las familias de Waka Playa integran la medicina tradicional y el sistema de salud formal en sus estrategias de vida, en diferentes grados según factores como la migración, la educación, el sexo y la edad. El uso de la flora medicinal local también es diferenciado según la localización de la vivienda principal de las familias y la consecuente concentración geográfica de sus actividades en las diferentes zonas de producción agroecológicas. Por ultimo, el interés personal influye sobre el grado y el tipo de conocimiento de cada familia. La medicina tradicional juega un rol fundamental en el bien-estar de las familias campesinas andinas y por ello constituye un potencial importante para un desarrollo sostenible. En esta perspectiva, la revalorización de los saberes locales y la construcción de puentes de diálogo con el sistema de salud local son sumamente importantes. Este punto de vista tiene perspectivas prometedoras en el contexto político actual boliviano, que apoya la medicina tradicional en el marco del reconocimiento de las identidades indígenas, en miras a un desarrollo endógeno.