7 resultados para large woody debris
em Universidad Politécnica de Madrid
Resumo:
La fauna saproxílica ha cobrado mucha relevancia en los últimos años. Por una parte, debido a los múltiples papeles que juega en la ecología de los bosques y por otra, por encontrarse muchas especies de ese grupo amenazadas como consecuencia de la intensificación de las actividades forestales. Se supone que los bosques de Europa meridional albergan una fauna saproxílica rica y variada. Sin embargo apenas se han realizado estudios que permitan conocer la composición de las biocenosis saproxílicas, así como el estatus y grado de amenaza a que está sometida cada especie. En esta tesis se han muestreado de forma sistemática las comunidades de coleópteros saproxílicos de cuatro montes del norte de la Comunidad de Madrid, muy diferentes a pesar de su cercanía: Dehesa Bonita de Somosierra, Hayedo de Montejo, Dehesa de Madarcos y Pinar de La Maleza. Para llevar a cabo la recogida de muestras se definió una estación de muestreo tipo, compuesta por cuatro trampas aéreas con cebo oloroso, dos trampas de ventana y una trampa de embudos. En los dos primeros montes mencionados se desplegaron seis estaciones de muestreo, por sólo tres en los otros dos. El primer objetivo de esta tesis fue conocer las especies de coleópteros que constituyen la fauna de los cuatro montes estudiados. Los muestreos sistemáticos reportaron la presencia de un total de 357 especies de coleópteros saproxílicos, siendo el Hayedo de Montejo el bosque con la diversidad más alta, 220 especies; le siguen la Dehesa de Madarcos con 116; el pinar de La Maleza con 115; y la Dehesa de Somosierra con 109, si bien la fauna de este ultimo bosque podría ser mucho más variada dado que la interferencia del ganado con algunos dispositivos de captura hizo que se perdiera parte del material allí recolectado. Se han encontrado nueve especies nuevas para la fauna de la Península Ibérica, y otras muchas desconocidas previamente en el centro peninsular. Un total de 50 especies se encuentran incluidas en la Lista Roja Europea de coleópteros saproxílicos. El segundo objetivo fue estimar la riqueza de fauna de coleópteros saproxílicos en cada bosque. Partiendo de los datos de los respectivo muestreos se calcularon diferentes estimadores, paramétricos y no paramétricos, y se elaboraron las curvas de rarefacción para cada bosque y para el conjunto. El bosque con más biodiversidad ha resultado ser el Hayedo de Montejo, que albergaría entre 254 y 332 especies. En el Pinar de la Maleza se encontrarían de 132 a 223; de 128 a 205 en la Dehesa de Somosierra; y entre 134 y 188 en la Dehesa de Madarcos. Para el conjunto del área se estimó la presencia de entre 411 y 512 especies. El tercer objetivo fue evaluar la influencia de algunos factores como la especie arbórea dominante y la cantidad de madera muerta en la riqueza y diversidad de coleópteros saproxílicos. El estudio se realizó en el Hayedo de Montejo, encontrando una alta correlación positiva entre cantidad y calidad de madera muerta, y diversidad y riqueza de especies de coleópteros saproxílicos. El cuarto objetivo fue evaluar la eficacia y complementariedad de los diferentes tipos de dispositivos de captura empleados en los muestreos. El más eficaz resultó ser la trampa de ventana, seguido por la trampa aérea con cebo oloroso, y finalmente la trampa de embudos. La mayor complementariedad se encontró entre trampas de ventana y aéreas con cebo oloroso. No obstante, si se quiere optimizar la exhaustividad del inventario no se debe prescindir de ninguno de los sistemas. En cualquier caso, puede afirmarse que la efectividad de los tres tipos de dispositivos de captura utilizados en los muestreos fue baja, pues para la gran mayoría de especies presentes se capturó un número de ejemplares realmente bajo. El bajo rendimiento de captura implica un bajo impacto sobre las poblaciones de las especies muestreadas, y esto supone una importante ventaja desde el punto de vista de la conservación. Finalmente, se dejan algunas recomendaciones de manejo a aplicar en cada uno de los montes con el fin de preservar o mejorar los hábitats utilizables por la fauna saproxílica que garanticen el mantenimiento y mejora de dichas comunidades. ABSTRACT The saproxylic fauna has become increasingly important in recent years. It has been due, on the one hand, to the multiple roles they play in the forest ecosystems and, on the other, because of the large proportion of endangered saproxylic species as a result of the intensification of forestry. It is generally assumed that southern Europe forests are home to a rich and diverse saproxylic fauna. However, there are hardly any studies leading to reveal the composition of saproxylic biocenosis, or the stage and extent of the threat each species is suffering. For the purpose of this thesis the communities of saproxylic beetles of four mountain forests in northern Comunidad de Madrid have been systematically sampled: Dehesa Bonita de Somosierra, Hayedo de Montejo, Dehesa de Madarcos and Pinar de La Maleza. They are very different from each other in spite of not being too far apart. In order to carry out sample collection, a standard sampling station was defined as follows: four smelly bait aerial traps, two window traps and one funnel trap. Six sampling stations were deployed in each of the first two forests mentioned above; put only three in each of the other two. The first aim of this thesis was to determine the composition of saproxylic beetles fauna inhabiting each of the four forests studied. Systematic sampling reported the presence of a total of 357 species of saproxylic beetles. Hayedo de Montejo, with 220 species, is the forest with the highest diversity, followed by Dehesa de Madarcos, 116; Pinar de La Maleza, 115, and Dehesa de Somosierra, 109. The fauna of the latter forest, however, could be much more varied, since cattle interference with some capture devices caused the loss of part of the material collected there. Nine new species in the fauna of the Iberian Peninsula were found, and many others previously unknown in the center of the Peninsula. A total of 41 of those species are included in the European Red List of saproxylic beetles. The second aim was to estimate the richness of saproxylic (beetle) fauna in each forest. From the data of the respective sampling, different parametric and nonparametric estimators were calculated, and rarefaction curves for each forest, as well as for the four of them together, were drawn. The most biodiverse forest turned out to be Hayedo de Montejo, which houses between 254 and 332 species. In Pinar de La Maleza, between 132 and 223 species were found; between 128 and 205 in Dehesa de Somosierra, and between 134 and 188 in Dehesa de Madarcos. The estimated diversity of species for the whole area ranges from 411 to 512. The third aim was to evaluate the influence of such factors as the dominant tree species and the amount of dead wood in the richness and diversity of saproxylic beetles. The study was conducted at Hayedo de Montejo, finding a high positive correlation between quantity and quality of coarse woody debris and diversity and richness of saproxylic beetle species. The fourth aim was to evaluate the effectiveness and complementarity of the different sampling methods used in this research work. The most effective proved to be the window trap, followed by the smelly bait aerial trap and the funnel trap, in that order. The greater complementarity was found between window and aerial traps. However, in order to optimize the completeness of the inventory, neither of the systems should be discarded. Nevertheless, the effectiveness of the three types of capture devices used in this piece of research was on the whole rather low, since for the vast majority of species, a significant low number of specimens were captured. Poor trapping performance implies a low impact on the populations of the sampled species, and this is an important advantage in terms of conservation. Finally, this thesis gives some recommendations with regard to the management of each of those four forests, leading to preserve and improve the habitats of the saproxylic wildlife and so ensure the maintenance and growth of their communities.
Resumo:
We assessed whether the relative importance of positive and negative interactions in early successional communities varied across a large landslide on Casita Volcano (Nicaragua). We tested several hypotheses concerning the signatures of these processes in the spatial patterns of woody pioneer plants, as well as those of mortality and recruitment events, in several zones of the landslide differing in substrate stability and fertility, over a period of two years (2001 and 2002). We identified all woody individuals with a diameter >1 cm and mapped them in 28 plots measuring 10 × 10-m. On these maps, we performed a spatial point pattern analysis using univariate and bivariate pair-correlation functions; g (r) and g12 (r), and pairwise differences of univariate and bivariate functions. Spatial signatures of positive and negative interactions among woody plants were more prevalent in the most and least stressful zones of the landslide, respectively. Natural and human-induced disturbances such as the occurrence of fire, removal of newly colonizing plants through erosion and clearcutting of pioneer trees were also identified as potentially important pattern-creating processes. These results are in agreement with the stress-gradient hypothesis, which states that the relative importance of facilitation and competition varies inversely across gradients of abiotic stress. Our findings also indicate that the assembly of early successional plant communities in large heterogeneous landslides might be driven by a much larger array of processes than previously thought.
Resumo:
The increase of orbital debris and the consequent proliferation of smaller objects through fragmentation are driving the need for mitigation strategies. The issue is how to deorbit the satellite with an efficient system that does not impair drastically the propellant budget of the satellite and, consequently, reduces its operating life. We have been investigating, in the framework of a European-Community-funded project, a passive system that makes use of an electrodynamics tether to deorbit a satellite through Lorentz forces. The deorbiting system will be carried by the satellite itself at launch and deployed from the satellite at the end of its life. From that moment onward the system operates passively without requiring any intervention from the satellite itself. The paper summarizes the results of the analysis carried out to show the deorbiting performance of the system starting from different orbital altitudes and inclinations for a reference satellite mass. Results can be easily scaled to other satellite masses. The results have been obtained by using a high-fidelity computer model that uses the latest environmental routines for magnetic field, ionospheric density, atmospheric density and a gravity field model. The tether dynamics is modelled by considering all the main aspects of a real system as the tether flexibility and its temperature-dependent electrical conductivity. Temperature variations are computed by including all the major external and internal input fluxes and the thermal flux emitted from the tether. The results shows that a relatively compact and light system can carry out the complete deorbit of a relatively large satellite in a time ranging from a month to less than a year starting from high LEO with the best performance occurring at low orbital inclinations.
Resumo:
The low earth orbit (LEO) environment contains a large number of artificial debris, of which a significant portion is due to dead satellites and fragments of satellites resulted from explosions and in-orbit collisions. Deorbiting defunct satellites at the end of their life can be achieved by a successful operation of an Electrodynamic Tether (EDT) system. The effectiveness of an EDT greatly depends on the survivability of the tether, which can become debris itself if cut by debris particles; a tether can be completely cut by debris having some minimal diameter. The objective of this paper is to develop an accurate model using power laws for debris-size ranges, in both ORDEM2000 and MASTER2009 debris flux models, to calculate tape tether survivability. The analytical model, which depends on tape dimensions (width, thickness) and orbital parameters (inclinations, altitudes) is then verified with fully numerical results to compare for different orbit inclinations, altitudes and tape width for both ORDEM2000 and MASTER2009 flux data.
Resumo:
Debris avalanches are complex phenomena due to the variety of mechanisms that control the failure stage and the avalanche formation. Regarding these issues, in the literature, either field evidence or qualitative interpretations can be found while few experimental laboratory tests and rare examples of geomechanical modelling are available for technical and/or scientific purposes. As a contribution to the topic, the paper firstly highlights as the problem can be analysed referring to a unique mathematical framework from which different modelling approaches can be derived based on limit equilibrium method (LEM), finite element method (FEM), or smooth particle hydrodynamics (SPH). Potentialities and limitations of these approaches are then tested for a large study area where huge debris avalanches affected shallow deposits of pyroclastic soils (Sarno-Quindici, Southern Italy). The numerical results show that LEM as well as uncoupled and coupled stress–strain FEM analyses are able to individuate the major triggering mechanisms. On the other hand, coupled SPH analyses outline the relevance of erosion phenomena, which can modify the kinematic features of debris avalanches in their source areas, i.e. velocity, propagation patterns and later spreading of the unstable mass. As a whole, the obtained results encourage the application of the introduced approaches to further analyse real cases in order to enhance the current capability to forecast the inception of these dangerous phenomena.
Resumo:
El entorno espacial actual hay un gran numero de micro-meteoritos y basura espacial generada por el hombre, lo cual plantea un riesgo para la seguridad de las operaciones en el espacio. La situación se agrava continuamente a causa de las colisiones de basura espacial en órbita, y los nuevos lanzamientos de satélites. Una parte significativa de esta basura son satélites muertos, y fragmentos de satélites resultantes de explosiones y colisiones de objetos en órbita. La mitigación de este problema se ha convertido en un tema de preocupación prioritario para todas las instituciones que participan en operaciones espaciales. Entre las soluciones existentes, las amarras electrodinámicas (EDT) proporcionan un eficiente dispositivo para el rápido de-orbitado de los satélites en órbita terrestre baja (LEO), al final de su vida útil. El campo de investigación de las amarras electrodinámicas (EDT) ha sido muy fructífero desde los años 70. Gracias a estudios teóricos, y a misiones para la demostración del funcionamiento de las amarras en órbita, esta tecnología se ha desarrollado muy rápidamente en las últimas décadas. Durante este período de investigación, se han identificado y superado múltiples problemas técnicos de diversa índole. Gran parte del funcionamiento básico del sistema EDT depende de su capacidad de supervivencia ante los micro-meteoritos y la basura espacial. Una amarra puede ser cortada completamente por una partícula cuando ésta tiene un diámetro mínimo. En caso de corte debido al impacto de partículas, una amarra en sí misma, podría ser un riesgo para otros satélites en funcionamiento. Por desgracia, tras varias demostraciones en órbita, no se ha podido concluir que este problema sea importante para el funcionamiento del sistema. En esta tesis, se presenta un análisis teórico de la capacidad de supervivencia de las amarras en el espacio. Este estudio demuestra las ventajas de las amarras de sección rectangular (cinta), en cuanto a la probabilidad de supervivencia durante la misión, frente a las amarras convencionales (cables de sección circular). Debido a su particular geometría (longitud mucho mayor que la sección transversal), una amarra puede tener un riesgo relativamente alto de ser cortado por un único impacto con una partícula de pequeñas dimensiones. Un cálculo analítico de la tasa de impactos fatales para una amarra cilindrica y de tipo cinta de igual longitud y masa, considerando el flujo de partículas de basura espacial del modelo ORDEM2000 de la NASA, muestra mayor probabilidad de supervivencia para las cintas. Dicho análisis ha sido comparado con un cálculo numérico empleando los modelos de flujo el ORDEM2000 y el MASTER2005 de ESA. Además se muestra que, para igual tiempo en órbita, una cinta tiene una probabilidad de supervivencia un orden y medio de magnitud mayor que una amarra cilindrica con igual masa y longitud. Por otra parte, de-orbitar una cinta desde una cierta altitud, es mucho más rápido, debido a su mayor perímetro que le permite capturar más corriente. Este es un factor adicional que incrementa la probabilidad de supervivencia de la cinta, al estar menos tiempo expuesta a los posibles impactos de basura espacial. Por este motivo, se puede afirmar finalmente y en sentido práctico, que la capacidad de supervivencia de la cinta es bastante alta, en comparación con la de la amarra cilindrica. El segundo objetivo de este trabajo, consiste en la elaboración de un modelo analítico, mejorando la aproximación del flujo de ORDEM2000 y MASTER2009, que permite calcular con precisión, la tasa de impacto fatal al año para una cinta en un rango de altitudes e inclinaciones, en lugar de unas condiciones particulares. Se obtiene el numero de corte por un cierto tiempo en función de la geometría de la cinta y propiedades de la órbita. Para las mismas condiciones, el modelo analítico, se compara con los resultados obtenidos del análisis numérico. Este modelo escalable ha sido esencial para la optimización del diseño de la amarra para las misiones de de-orbitado de los satélites, variando la masa del satélite y la altitud inicial de la órbita. El modelo de supervivencia se ha utilizado para construir una función objetivo con el fin de optimizar el diseño de amarras. La función objectivo es el producto del cociente entre la masa de la amarra y la del satélite y el numero de corte por un cierto tiempo. Combinando el modelo de supervivencia con una ecuación dinámica de la amarra donde aparece la fuerza de Lorentz, se elimina el tiempo y se escribe la función objetivo como función de la geometría de la cinta y las propietades de la órbita. Este modelo de optimización, condujo al desarrollo de un software, que esta en proceso de registro por parte de la UPM. La etapa final de este estudio, consiste en la estimación del número de impactos fatales, en una cinta, utilizando por primera vez una ecuación de límite balístico experimental. Esta ecuación ha sido desarollada para cintas, y permite representar los efectos tanto de la velocidad de impacto como el ángulo de impacto. Los resultados obtenidos demuestran que la cinta es altamente resistente a los impactos de basura espacial, y para una cinta con una sección transversal definida, el número de impactos críticos debidos a partículas no rastreables es significativamente menor. ABSTRACT The current space environment, consisting of man-made debris and tiny meteoroids, poses a risk to safe operations in space, and the situation is continuously deteriorating due to in-orbit debris collisions and to new satellite launches. Among these debris a significant portion is due to dead satellites and fragments of satellites resulted from explosions and in-orbit collisions. Mitigation of space debris has become an issue of first concern for all the institutions involved in space operations. Bare electrodynamic tethers (EDT) can provide an efficient mechanism for rapid de-orbiting of defunct satellites from low Earth orbit (LEO) at end of life. The research on EDT has been a fruitful field since the 70’s. Thanks to both theoretical studies and in orbit demonstration missions, this technology has been developed very fast in the following decades. During this period, several technical issues were identified and overcome. The core functionality of EDT system greatly depends on their survivability to the micrometeoroids and orbital debris, and a tether can become itself a kind of debris for other operating satellites in case of cutoff due to particle impact; however, this very issue is still inconclusive and conflicting after having a number of space demonstrations. A tether can be completely cut by debris having some minimal diameter. This thesis presents a theoretical analysis of the survivability of tethers in space. The study demonstrates the advantages of tape tethers over conventional round wires particularly on the survivability during the mission. Because of its particular geometry (length very much larger than cross-sectional dimensions), a tether may have a relatively high risk of being severed by the single impact of small debris. As a first approach to the problem, survival probability has been compared for a round and a tape tether of equal mass and length. The rates of fatal impact of orbital debris on round and tape tether, evaluated with an analytical approximation to debris flux modeled by NASA’s ORDEM2000, shows much higher survival probability for tapes. A comparative numerical analysis using debris flux model ORDEM2000 and ESA’s MASTER2005 shows good agreement with the analytical result. It also shows that, for a given time in orbit, a tape has a probability of survival of about one and a half orders of magnitude higher than a round tether of equal mass and length. Because de-orbiting from a given altitude is much faster for the tape due to its larger perimeter, its probability of survival in a practical sense is quite high. As the next step, an analytical model derived in this work allows to calculate accurately the fatal impact rate per year for a tape tether. The model uses power laws for debris-size ranges, in both ORDEM2000 and MASTER2009 debris flux models, to calculate tape tether survivability at different LEO altitudes. The analytical model, which depends on tape dimensions (width, thickness) and orbital parameters (inclinations, altitudes) is then compared with fully numerical results for different orbit inclinations, altitudes and tape width for both ORDEM2000 and MASTER2009 flux data. This scalable model not only estimates the fatal impact count but has proved essential in optimizing tether design for satellite de-orbit missions varying satellite mass and initial orbital altitude and inclination. Within the frame of this dissertation, a simple analysis has been finally presented, showing the scalable property of tape tether, thanks to the survivability model developed, that allows analyze and compare de-orbit performance for a large range of satellite mass and orbit properties. The work explicitly shows the product of tether-to-satellite mass-ratio and fatal impact count as a function of tether geometry and orbital parameters. Combining the tether dynamic equation involving Lorentz drag with space debris impact survivability model, eliminates time from the expression. Hence the product, is independent of tether de-orbit history and just depends on mission constraints and tether length, width and thickness. This optimization model finally led to the development of a friendly software tool named BETsMA, currently in process of registration by UPM. For the final step, an estimation of fatal impact rate on a tape tether has been done, using for the first time an experimental ballistic limit equation that was derived for tapes and accounts for the effects of both the impact velocity and impact angle. It is shown that tape tethers are highly resistant to space debris impacts and considering a tape tether with a defined cross section, the number of critical events due to impact with non-trackable debris is always significantly low.
Resumo:
The study of functional morphological traits enables us to know fundamental aspects of the dynamics of plant communities in local and global habitats. Regenerative morphological traits play an important role in defining plant history and ecological behavior. Seed and fruit characteristics determine to a large extent the patterns for dispersal, germination, establishment and seedling recruitment a given species exhibits on its natural habitat. Despite their prominent role, seed and fruit traits have been poorly studied at the community level of woody plant species in neo-tropical dry forests. In the present study we aimed at i) evaluate the functional role of morphological traits of seeds, fruits and embryo in woody plant species; ii) determine which are the morphological patterns present in seeds collected from the community of woody species that occur in neo-tropical dry forests; and iii) compare woody plant species seed mass values comparatively between neo-tropical dry and tropical forests. To do so, mature seeds were collected from 79 plant species that occur in the Tumbesian forest of Southwest Ecuador. The studied species included the 42 and 37 most representative tree and shrubbery species of the Tumbesian forest respectively. A total of 18 morphological traits (seven quantitative and 11 qualitative) were measured and evaluated in the seeds, fruits and embryos of the selected species, and we compared the seeds mass with other forest types. Our results showed a huge heterogeneity among traits values in the studied species. Seed mass, volume and number were the traits that vary the most at the community level, i.e. seed length ranged from 1.3 to 39 mm, and seed width from 0.6 to 25 mm. Only six embryo types were found among the 79 plant species. In 40 % of the cases, fully developed inverted embryos with large and thick cotyledons to store considerable amount of nutrients were recorded. We concluded that highly variable and functionally complementary morphological traits occur among the studied woody plants of the dry Tumbesian forest. The latter favors a plethora of behavioral mechanisms to coexist among woody species of the dry forest in response to the environmental stress that is typical of arid areas.