Determination of αs from the QCD static energy: An update

We present an update of our determination of the strong coupling αs from the quantum chromodynamics static energy. This updated analysis includes new lattice data, at smaller lattice spacings and reaching shorter distances, the use of better suited perturbative expressions to compare with data in a wider distance range, and a comprehensive and detailed estimate of the error sources that contribute to the uncertainty of the final result. Our updated value for αs at the Z-mass scale, MZ, is αs(MZ)=0.1166+0.0012−0.0008, which supersedes our previous result.

Luminal particles within cellular microtubules.

The regulation of microtubule dynamics is attributed to microtubule-associated proteins that bind to the microtubule outer surface, but little is known about cellular components that may associate with the internal side of microtubules. We used cryoelectron tomography to investigate in a quantitative manner the three dimensional structure of microtubules in intact mammalian cells. We show that the lumen of microtubules in this native state is filled with discrete, globular particles with a diameter of 7 nm and spacings between 8 and 20 nm in neuronal cells. Cross-sectional views of microtubules confirm the presence of luminal material in vitreous sections of brain tissue. Most of the luminal particles had connections to the microtubule wall, as revealed in tomograms. A higher accumulation of particles was seen near the retracting plus ends of microtubules. The luminal particles were abundant in neurons, but were also observed in other cells, such as astrocytes and stem cells.

Theoretical models of planetary system formation II. Post-formation evolution

Aims. We extend the results of planetary formation synthesis by computing the long-term evolution of synthetic systems from the clearing of the gas disk into the dynamical evolution phase. Methods. We use the symplectic integrator SyMBA to numerically integrate the orbits of planets for 100 Myr, using populations from previous studies as initial conditions. Results. We show that within the populations studied, mass and semimajor axis distributions experience only minor changes from post-formation evolution. We also show that, depending upon their initial distribution, planetary eccentricities can statistically increase or decrease as a result of gravitational interactions. We find that planetary masses and orbital spacings provided by planet formation models do not result in eccentricity distributions comparable to observed exoplanet eccentricities, requiring other phenomena, such as stellar fly-bys, to account for observed eccentricities.

Crevassing and Calving of Glacial Ice

Calving of ice is a relatively new area of research in the still young field of glaciology. In the short time that calving has been studied, it has been mainly treated as an afterthought, with the predominant mode of thinking being that it will happen so to concern oneself with why is not important. Many studies dealt with observations of calving front positions over time vs. ice velocity in an attempt to quantify the calving rate as the difference between the two, while others have attempted to deduce some empirical relationship between calving rate and variables such as water depth or temperature. This study instead addresses the question of why, where, and when ice will first become crevassed, which is an obviously necessary condition for a later calving event to occur. Previous work examining the causes of calving used ideas put forth from a variety of fields, including civil engineering, materials science, and results from basic physics and mechanics. These theories are re-examined here and presented as part of a larger whole. Important results from the field of fracture mechanics are utilized frequently, and these results can be used as a predictor of ice behavior and intrinsic properties of ice, as well as properties like back stresses induced by local pinning points and resistive shears along glacial ice boundaries. A theory of fracture for a material experiencing creep is also presented with applications to ice shelves and crevasse penetration. Finally, a speculative theory regarding large scale iceberg formation is presented. It is meant mainly as an impetus to further discussion on the topic, with the hope that a model relating crevasse geometries to flow parameters can result in crevasse spacings that could produce the tabular icebergs which are so newsworthy. The primary focus of this thesis is to move away from the "after the fact" studies that are so common in calving research, and instead devote energy to determining what creates the conditions that drive the calving of ice in the first place.

Efecto de la densidad de plantación sobre el rendimiento de topinambur (Helianthus tuberosus L.) regado con aguas residuales urbanas

Helianthus tuberosus L. produce tubérculos ricos en hidratos de carbono fermentables que pueden ser usados para producir etanol. Para el destino energético el cultivo puede ser regado con aguas residuales urbanas. La densidad poblacional en un cultivo de topinambur afecta los parámetros de crecimiento y rendimiento. Se evaluó el efecto de la densidad de plantación sobre el rendimiento de tubérculos. Se compararon 6 tratamientos de densidad, combinando 2 espaciamientos entre hileras (0,70 y 0,80 m) y 3 espaciamientos entre plantas en la hilera (0,30; 0,40 y 0,50 m), generando stands desde las 25.000 a 47.600 plantas/ha. Se presentaron los mayores rendimientos con distancias entre plantas en la hilera de 0,30 ó 0,40 m; no se presentaron diferencias en respuesta a la distancia entre hileras. Los componentes del rendimiento (rendimiento de tubérculos por planta, número de tubérculos por planta y tamaño medio de los tubérculos) respondieron a cambios en la densidad generados por la distancias entre plantas y fueron indiferentes a la variación de distancia entre hileras. La altura de las plantas, el número de tallos principales, el porcentaje de MS y de SS en los tubérculos no se modificaron ante variaciones de densidad.

Chert petrology and geochemistry at DSDP Leg 62 Holes

Sixty-five chert, porcellanite, and siliceous-chalk samples from Deep Sea Drilling Project Leg 62 were analyzed by petrography, scanning electron microscopy, analysis by energy-dispersive X-rays, X-ray diffraction, X-ray spectroscopy, and semiquantitative emission spectroscopy. Siliceous rocks occur mainly in chalks, but also in pelagic clay and marlstone at Site 464. Overall, chert probably constitutes less than 5% of the sections and occurs in deposits of Eocene to Barremian ages at sub-bottom depths of 10 to 820 meters. Chert nodules and beds are commonly rimmed by quartz porcellanite; opal-CT-rich rocks are minor in Leg 62 sediments 65 to 108 m.y. old and at sub-bottom depths of 65 to 520 meters. Chert ranges from white to black, shades of gray and brown being most common; yellow-brown and red-brown jaspers occur at Site 464. Seventy-eight percent of the studied cherts contain easily recognizable burrow structures. The youngest chert at Site 463 is a quartz cast of a burrow. Burrow silica maturation is always one step ahead of host-rock silicification. Burrows are commonly loci for initial silicification of the host carbonate. Silicification takes place by volume-f or-volume replacement of carbonate sediment, and more-clay-rich sediment at Site 464. Nannofossils are commonly pseudomorphically replaced by quartz near the edges of chert beds and nodules. Other microfossils, mostly radiolarians and foraminifers, whether in chalk or chert, can be either filled with or replaced by calcite, opal-CT, and (or) quartz. Chemical micro-environments ultimately control the removal, transport, and precipitation of calcite and silica. Two cherts from Site 465 contain sulfate minerals replaced by quartz. Site 465 was never subaerially exposed after sedimentation began, and the formation of the sulfate minerals and their subsequent replacement probably occurred in the marine environment. Several other cherts with odd textures are described in this paper, including (1) a chert breccia cemented by colloform opal-CT and chalcedony, (2) a transition zone between white porcellanite containing opal-CT and quartz and a burrowed brown chert, consisting of radial aggregates of opal-CT with hollow centers, and (3) a chert that consists of silica-replaced calcite pseudospherules interspersed with streaks and circular masses of dense quartz. X-ray-diffraction analyses show that when data from all sites are considered there are poorly defined trends indicating that older cherts have better quartz crystallinity than younger ones, and that opal-CT crystallite size increases and opal-CT cf-spacings decrease with depth of occurrence in the sections. In a general way, depth of burial and the presence of calcite promote the ordering in the opal-CT crystal structure which allows its eventual conversion to quartz. Opal-CT in porcellanites converts to quartz after reaching a minimum d-spacing of 4.07 Å. Quartz/opal-CT ratios and quartz crystallinity vary randomly on a fine scale across four chert beds, but quartz crystallinity increases from the edge to the center of a fifth chert bed; this may indicate maturation of the silica. Twenty-four rocks were analyzed for their major- and minor-element compositions. Many elements in cherts are closely related to major mineral components. The carbonate component is distinguished by high values of CaO, MgO, Mn, Ba, Sr, and (for unknown reasons) Zr. Tuffaceous cherts have high values of K and Al, and commonly Zn, Mo, and Cr. Pure cherts are characterized by high SiO2 and B. High B may be a good indicator of formation of chert in an open marine environment, isolated from volcanic and terrigenous materials.

Implementation of the Heated Pulsed Theory using actively heated fiber optics: measurements of soil volumetric water content and soil volumetric heat capacity

Existe una creciente necesidad de hacer el mejor uso del agua para regadío. Una alternativa eficiente consiste en la monitorización del contenido volumétrico de agua (θ), utilizando sensores de humedad. A pesar de existir una gran diversidad de sensores y tecnologías disponibles, actualmente ninguna de ellas permite obtener medidas distribuidas en perfiles verticales de un metro y en escalas laterales de 0.1-1,000 m. En este sentido, es necesario buscar tecnologías alternativas que sirvan de puente entre las medidas puntuales y las escalas intermedias. Esta tesis doctoral se basa en el uso de Fibra Óptica (FO) con sistema de medida de temperatura distribuida (DTS), una tecnología alternativa de reciente creación que ha levantado gran expectación en las últimas dos décadas. Específicamente utilizamos el método de fibra calentada, en inglés Actively Heated Fiber Optic (AHFO), en la cual los cables de Fibra Óptica se utilizan como sondas de calor mediante la aplicación de corriente eléctrica a través de la camisa de acero inoxidable, o de un conductor eléctrico simétricamente posicionado, envuelto, alrededor del haz de fibra óptica. El uso de fibra calentada se basa en la utilización de la teoría de los pulsos de calor, en inglés Heated Pulsed Theory (HPP), por la cual el conductor se aproxima a una fuente de calor lineal e infinitesimal que introduce calor en el suelo. Mediante el análisis del tiempo de ocurrencia y magnitud de la respuesta térmica ante un pulso de calor, es posible estimar algunas propiedades específicas del suelo, tales como el contenido de humedad, calor específico (C) y conductividad térmica. Estos parámetros pueden ser estimados utilizando un sensor de temperatura adyacente a la sonda de calor [método simple, en inglés single heated pulsed probes (SHPP)], ó a una distancia radial r [método doble, en inglés dual heated pulsed probes (DHPP)]. Esta tesis doctoral pretende probar la idoneidad de los sistemas de fibra óptica calentada para la aplicación de la teoría clásica de sondas calentadas. Para ello, se desarrollarán dos sistemas FO-DTS. El primero se sitúa en un campo agrícola de La Nava de Arévalo (Ávila, España), en el cual se aplica la teoría SHPP para estimar θ. El segundo sistema se desarrolla en laboratorio y emplea la teoría DHPP para medir tanto θ como C. La teoría SHPP puede ser implementada con fibra óptica calentada para obtener medidas distribuidas de θ, mediante la utilización de sistemas FO-DTS y el uso de curvas de calibración específicas para cada suelo. Sin embargo, la mayoría de aplicaciones AHFO se han desarrollado exclusivamente en laboratorio utilizando medios porosos homogéneos. En esta tesis se utiliza el programa Hydrus 2D/3D para definir tales curvas de calibración. El modelo propuesto es validado en un segmento de cable enterrado en una instalación de fibra óptica y es capaz de predecir la respuesta térmica del suelo en puntos concretos de la instalación una vez que las propiedades físicas y térmicas de éste son definidas. La exactitud de la metodología para predecir θ frente a medidas puntuales tomadas con sensores de humedad comerciales fue de 0.001 a 0.022 m3 m-3 La implementación de la teoría DHPP con AHFO para medir C y θ suponen una oportunidad sin precedentes para aplicaciones medioambientales. En esta tesis se emplean diferentes combinaciones de cables y fuentes emisoras de calor, que se colocan en paralelo y utilizan un rango variado de espaciamientos, todo ello en el laboratorio. La amplitud de la señal y el tiempo de llegada se han observado como funciones del calor específico del suelo. Medidas de C, utilizando esta metodología y ante un rango variado de contenidos de humedad, sugirieron la idoneidad del método, aunque también se observaron importantes errores en contenidos bajos de humedad de hasta un 22%. La mejora del método requerirá otros modelos más precisos que tengan en cuenta el diámetro del cable, así como la posible influencia térmica del mismo. ABSTRACT There is an increasing need to make the most efficient use of water for irrigation. A good approach to make irrigation as efficient as possible is to monitor soil water content (θ) using soil moisture sensors. Although, there is a broad range of different sensors and technologies, currently, none of them can practically and accurately provide vertical and lateral moisture profiles spanning 0-1 m depth and 0.1-1,000 m lateral scales. In this regard, further research to fulfill the intermediate scale and to bridge single-point measurement with the broaden scales is still needed. This dissertation is based on the use of Fiber Optics with Distributed Temperature Sensing (FO-DTS), a novel approach which has been receiving growing interest in the last two decades. Specifically, we employ the so called Actively Heated Fiber Optic (AHFO) method, in which FO cables are employed as heat probe conductors by applying electricity to the stainless steel armoring jacket or an added conductor symmetrically positioned (wrapped) about the FO cable. AHFO is based on the classic Heated Pulsed Theory (HPP) which usually employs a heat probe conductor that approximates to an infinite line heat source which injects heat into the soil. Observation of the timing and magnitude of the thermal response to the energy input provide enough information to derive certain specific soil thermal characteristics such as the soil heat capacity, soil thermal conductivity or soil water content. These parameters can be estimated by capturing the soil thermal response (using a thermal sensor) adjacent to the heat source (the heating and the thermal sources are mounted together in the so called single heated pulsed probe (SHPP)), or separated at a certain distance, r (dual heated pulsed method (DHPP) This dissertation aims to test the feasibility of heated fiber optics to implement the HPP theory. Specifically, we focus on measuring soil water content (θ) and soil heat capacity (C) by employing two types of FO-DTS systems. The first one is located in an agricultural field in La Nava de Arévalo (Ávila, Spain) and employ the SHPP theory to estimate θ. The second one is developed in the laboratory using the procedures described in the DHPP theory, and focuses on estimating both C and θ. The SHPP theory can be implemented with actively heated fiber optics (AHFO) to obtain distributed measurements of soil water content (θ) by using reported soil thermal responses in Distributed Temperature Sensing (DTS) and with a soil-specific calibration relationship. However, most reported AHFO applications have been calibrated under laboratory homogeneous soil conditions, while inexpensive efficient calibration procedures useful in heterogeneous soils are lacking. In this PhD thesis, we employ the Hydrus 2D/3D code to define these soil-specific calibration curves. The model is then validated at a selected FO transect of the DTS installation. The model was able to predict the soil thermal response at specific locations of the fiber optic cable once the surrounding soil hydraulic and thermal properties were known. Results using electromagnetic moisture sensors at the same specific locations demonstrate the feasibility of the model to detect θ within an accuracy of 0.001 to 0.022 m3 m-3. Implementation of the Dual Heated Pulsed Probe (DPHP) theory for measurement of volumetric heat capacity (C) and water content (θ) with Distributed Temperature Sensing (DTS) heated fiber optic (FO) systems presents an unprecedented opportunity for environmental monitoring. We test the method using different combinations of FO cables and heat sources at a range of spacings in a laboratory setting. The amplitude and phase-shift in the heat signal with distance was found to be a function of the soil volumetric heat capacity (referred, here, to as Cs). Estimations of Cs at a range of θ suggest feasibility via responsiveness to the changes in θ (we observed a linear relationship in all FO combinations), though observed bias with decreasing soil water contents (up to 22%) was also reported. Optimization will require further models to account for the finite radius and thermal influence of the FO cables, employed here as “needle probes”. Also, consideration of the range of soil conditions and cable spacing and jacket configurations, suggested here to be valuable subjects of further study and development.

Respuesta fisiológica y agronómica del olivar en seto (cv. Arbequina) a la orientación de filas y al ancho de calle: relación entre la producción y calidad del aceite y la radiación interceptada

En las últimas dos décadas, los productores han plantado olivares en seto para lograr la mecanización de la poda y en especial de la cosecha, reducir los costes de mano de obra y permitir intervenciones de manejo rápidas y oportunas. Los olivares se desarrollaron en ausencia del conocimiento científico, sobre el diseño óptimo de la estructura de la copa, necesario para incrementar la producción y calidad del aceite. En contraste, con los árboles muy espaciados y distribuidos uniformemente de las plantaciones tradicionales, en el olivar en seto hay una marcada variabilidad espacial y temporal de la radiación disponible en función del diseño de la plantación. Así, conocer la respuesta fisiológica y productiva del olivo a la radiación resulta fundamental en el olivar en seto. La orientación de las filas y el ancho de calle son aspectos que se deciden en el diseño de las plantaciones en seto. Ambos aspectos modifican la radiación interceptada por la canopia y, por lo tanto, pueden incidir en la productividad y calidad del aceite. Una vez realizada la plantación no pueden ser modificados, y así las ventajas o desventajas permanecerán fijas durante toda la vida productiva del olivar. A pesar de esto, el impacto de la orientación de las filas y el ancho de calle han recibido poca atención en olivos y en la mayoría de los frutales conducidos en seto. Por todo ello, los objetivos principales de esta tesis fueron, (i) evaluar el efecto de la orientación del seto y del ancho de calle, sobre la productividad y calidad del aceite, (ii) evaluar un modelo que estime la radiación dentro de la canopia. Este modelo permitirá cuantificar las relaciones entre la radiación y los componentes del rendimiento y calidad del aceite de olivares en setos con un amplio rango de estructuras y (iii) conocer la variabilidad en las características de las hojas (morfológicas y fisiológicas) y de los tejidos del fruto (tamaño y composición) en diferentes posiciones de la copa de los setos. Para ello, se dispuso de 3 ensayos de olivar en seto (cv. Arbequina) implantados en 2008 en el municipio de La Puebla de Montalbán, Toledo. La primera cosecha fue en 2010 y a partir del 2012 los setos formaron una copa continua. A partir de ese año, los setos se mantuvieron mediante poda, con similar ancho (~1 m) y altura (~2,5 m), acordes a las dimensiones de la cosechadora vendimiadora. En los años 2012 y 2013 se estudió en profundidad la respuesta de las plantas de estos ensayos. En el ensayo 1, los setos fueron plantados con cuatro orientaciones de filas: N–S, NE–SO, NO–SE y E–O y el mismo ancho de calle (4 m). En los otros dos ensayos, los setos fueron plantados con tres anchos de calle (5,0, 4,0 y 2,5 m), y con filas orientadas N–S (ensayo 2) y E–O (ensayo 3). La respuesta de la orientación de las filas se evaluó a nivel de seto y de estratos del seto (alturas y caras), a través de mediciones del crecimiento de brotes, componentes reproductivos, características y temperatura del fruto, estado hídrico del suelo y de las plantas, fotosíntesis neta de las hojas y contenido de ácidos grasos. Los setos orientados NE–SO (2,7 t/ha) lograron la mayor producción de aceite, que fue significativamente más alta que la de los setos E–O (2,3 t/ha). La producción de aceite de los setos E–O no se diferenció estadísticamente de los setos N–S (2,5 t/ha). Las diferencias productivas entre orientaciones fueron explicadas por el número de frutos en cosecha, a su vez la variación en el número de frutos estuvo asociada al efecto de la orientación de las filas sobre el número de yemas desarrolladas y el porcentaje de inflorescencias fértiles. Las hojas en las caras iluminadas de los setos NE–SO y N–S presentaron mayor tasa fotosintética a la mañana (~10.0 h) que los setos E–O, en el año 2012, pero no en 2013. La orientación de las filas no tuvo un efecto significativo en el contenido de ácidos grasos de los aceites extraídos, esto ocurrió a pesar de variaciones en la temperatura interna de los frutos (3 °C) y de la radiación (40%) entre las distintas caras de los setos. La orientación del seto afectó significativamente al contenido relativo de agua del suelo, donde setos E–O presentaron valores más altos (12%) que setos N–S durante el verano y otoño. Sin embargo, el potencial hídrico de tallo fue similar entre orientaciones. En los ensayos 2 y 3, se evaluó el efecto que produce, a nivel de seto y de estratos (caras y alturas), reducir el ancho de calle de 5,0 a 4,0 y 2,5 m, en un seto orientado N–S y otro E–O, respectivamente. La relación entre altura/ancho de calle libre aumentó 0,6 a 0,8 y 1,6, al reducir 5,0, 4,0 y 2,5 m el ancho de calle, mientras la longitud de seto y el volumen de copa por hectárea incrementó 100% al reducir de 5,0 a 2,5 m, el ancho de calle. En los setos orientados N–S, la producción de aceite por ha acumulada en 4 campañas, incrementó significativamente un 52 %, al reducir de 5,0 a 2,5 m el ancho de calle. Los setos N–S con calle más estrecha (2,5 m) tuvieron un 19% menos frutos que los setos con calle más ancha (5,0 m) y a su vez el 60% de los mismos se localizaron los estratos altos de la canopia de los setos con calles estrecha en comparación al 40% en setos con calle de 5,0 m. En los estratos más bajos de los setos con calles de 2,5m hubo menor crecimiento de los brotes y los frutos tuvieron menor peso seco, contenido de aceite y madurez, que los frutos en los estratos bajos de los setos a 5,0 m. Los componentes del rendimiento y características de los frutos (agua y madurez) fueron similares entre la caras E y O, independientemente del ancho de calle. En los setos orientados E–O, la producción de aceite por ha acumulada en 4 campañas, no respondió significativamente al ancho de calle, debido a una disminución significativa en el número de frutos y producción de aceite por m de seto, al reducir de 5,0 a 2,5 m, el ancho de calle. En los setos orientados E–O, con calles de 5,0 m, los frutos presentaron similar peso seco, contenido de aceite y agua, en las caras S y N, sin embargo, cuando la calle fue reducida a 2,5, los frutos de la cara S fueron más pesado y maduros que en la cara N. Independientemente del ancho de calle y de la orientación del seto, el aceite presentó mayor contenido de ácidos palmitoleico, palmítico, esteárico y linoleico en los frutos del estrato más alto de la canopia disminuyendo hacia la base. En contraste, el contenido de ácido oleico aumentó desde el estrato más alto hacia la base de los setos. Las diferencias en el contenido de ácidos grasos entre la parte alta y baja de los setos, incrementó al reducir el ancho de calle en los setos N–S, pero no en los E-O. En conclusión, en olivares en seto, reducir el ancho de calle permite incrementar la producción de aceite, en setos orientados N–S, pero no en E–O. Un modelo que estima la cantidad y distribución de la radiación en toda la copa del seto, fue utilizado para estimar la radiación interceptada en distintos estratos del seto. El modelo requiere un valor del coeficiente de extinción (k) para estimar la transmisión de radiación a través de la copa, el cual fue obtenido experimentalmente (k=1,2). Utilizando los datos del ensayo 1, un único modelo lineal relacionó el peso seco y el rendimiento graso de setos con la radiación interceptada por los distintos estratos de setos con cuatro orientaciones de filas. La densidad de frutos fue también relacionada con la radiación, pero más débilmente. En los setos orientados N–S, plantados con tres anchos de calles, (ensayo 2) el contenido de ácidos palmitoleico y linoleico del aceite incrementó linealmente con el incremento de la radiación interceptada, mientras el contenido ácido oleico disminuyó linealmente con el incremento de la radiación. El contenido de ácidos grasos del aceite no estuvo relacionado con la radiación interceptada en setos orientados E–O (Ensayo 3). En los setos N–S y E–O, plantados con anchos de calle de 2,5 m, se estudiaron las interacciones entre la radiación y características de las hojas, número de fruto, tamaño y composición de los frutos a nivel de órgano, tejido y células. Independientemente de la orientación del seto, el área y el contenido de clorofila de las hojas incrementaron significativamente en los estratos más bajos de los setos. Mientras, las hojas de los estratos medios del seto presentaron mayor capacidad fotosintética que en los estratos bajos y alto de los setos. Los estratos del seto que interceptaron más radiación produjeron frutos con mayor tamaño y contenido de aceite en el mesocarpo, sin efectos sobre el tamaño y composición del endocarpo. A nivel celular, los frutos expuestos a mayor nivel de radiación desarrollaron en el mesocarpo células de mayor tamaño en comparación a frutos menos expuestos, mientras el número de células no fue afectado. Adicionalmente, el número y tamaño de las células estuvo relacionado con la composición del mesocarpo en términos de aceite, agua y peso seco menos aceite. Esta tesis, contribuye, desde una perspectiva integral del cultivo del olivo, a cuantificar el impacto de la orientación y ancho de calle sobre la producción y calidad del aceite en olivares conducidos en setos. El análisis y discusión de la relación entre la radiación y los componentes del rendimiento y calidad del aceite, puede ayudar a diseñar plantaciones en seto con dimensiones óptimas para la intercepción de la radiación. ABSTRACT In the last two decades, olive hedgerow system has been established by commercial growers to allow continuous mechanized pruning and especially harvest, reduce costs of manual labour and allow more rapid and timely management interventions. The adoption of hedgerow was done in the absence of adequate scientific knowledge of the impact of this orchard structure and associated mechanization on tree response, yield and quality, after centuries in low-density orchards and open-formed trees. The row orientation and width alley are fundamental aspects in the hedgerow design and have been scarcely studied in olive. Both aspects modify the radiation intercepted by the canopy, and consequently the productivity and oil quality, and once defined in orchard planting cannot be changed, so advantages and disadvantages remain fixed for the lifespan of the orchard. The main objectives of this thesis were to (i) evaluate the impact of the row orientation and width alley on productivity and oil quality by the measurements of profile of the determining processes of shoot growth, fruit temperature, yield components and fruit and oil characteristics on opposite sides of olive hedgerows. Additionally, the effect of row orientation on the plant water status was also evaluated; (ii) evaluate a mathematical model for estimating the radiation within the canopy and quantify the relationships between the radiation estimated and yield components and oil quality in olive hedgerows under wide range of structures and; (iii) determine the variability in the characteristics of the leaves (morphological and physiological) and fruit tissues (size and composition) in different positions of the hedgerows canopy. Three plots of olive hedgerows (cv. Arbequina) planted in 2008 in La Puebla de Montalbán, Toledo were evaluated during the 2012 and 2013 seasons. The hedgerows were maintained by lateral pruning and topping with the same width (1 m) and height (2.5 m) compatible with the intended harvester. In a plot (experiment 1), the hedgerows were planted with the same width alley (4 m) and four row orientations: N–S, NE–SW, NW–SE and E–W. Other two plots (Experiments 2 and 3) separated by approximately 100 m were planted with N–S and E–O oriented rows and three alley widths in each orientation: 5.0, 4.0 and 2.5 m. In the exp. 1, maximum fruit yield were achieved by NE–SW and NW–SW (15.7 t/ha). Of these, NE–SW achieved the highest oil yield (2.7 t/ha). There were no differences in fruit or oil yield between N–S (2.5 t oil/ha) and E–W (2.3 t oil/ha) orientations. Fruit number was the most important component to explain these differences, by previous influence on number of bud developed and percentage of fertile inflorescences. Fruit maturity and oil quality on both sides of the hedgerows were not affected by row orientation. This occurred despite significant variations in the internal fruit temperature, which was closely related to the irradiance received by the canopy and the time of day. Additionally, row orientation significantly affected the relative water content of the soil, where E–W oriented hedgerows showed consistently higher values than N–S during summer-autumn season. The stem water potential at midday, however, was similar between orientations, revealing possible lower water consumption of E–W than N–S oriented hedgerows. In the exp. 2, regardless of row orientation, reduction of row spacing from 5.0 to 4.0 and 2.5 m increases the ratio of canopy depth to free alley width (Al/An) from 0.6 to 0.8 and 1.6, respectively, and ads 25 and 100 % more hedgerow length per ha. In N–S oriented hedgerows, oil production per ha increased significantly by 14 and 52 % in 4.0 m and 2.5 m relative to 5.0 m row spacing, the effect being proportionally less than the increase in hedgerow length per ha. Hedgerows spaced 2.5 m with Al/An = 1.6 produced relatively fewer fruits per unit length than did wider spacings and were preferentially distributed in upper layers. Fruits located at the bottom of the canopy were smaller, with lower oil content and were less mature. In E–W oriented hedgerows, oil production per ha did not respond significantly to row spacing, despite the doubling of row length from the 5.0 to the 2.5 m row spacing. The explanation was found in fewer fruit per unit length of hedgerow and smaller oil content at 2.5 m than 5.0 m row spacing, averaged over the experimental period. In E–W hedgerows spaced at 5.0 m with Al/An = 0.6, the vertical profiles of fruit characteristics (mass, oil and water contents, and maturity) were similar between opposing sides, but at 4.0 m (Al/An= 0.8) and 2.5 m (Al/An=1.6) spacings, fruits on the S side were heavier and more mature than on N side. The oil extracted from fruits harvested at different heights of N–S and E–W oriented hedgerows showed higher palmitoleic, palmitic, stearic and linoleic contents at the canopy top decreasing toward base. The oleic content was reverse, increased from top to base. In N–S hedgerows, vertical gradients increased by reducing the alley width, but not in the E–W oriented hedgerows. The simulation of internal canopy irradiance was related in a single relationship (R2 = 0.63) to the vertical profiles of fruit weight and oil content of olive hedgerows with wide range of structures. The density of fruits was also associated with the irradiance but more weakly (R2 = 0.27), and revealed a more complex response involving changes in the vegetative structure by canopy management (topping) and the effect of radiation on the previous sequence that defines the number of fruits. The vertical profiles of oil quality traits were closely associated to canopy irradiance, but only when the N–S oriented hedgerows were considered. The contents of palmitoleic and linoleic acid in the oil increased linearly when intercepted irradiance increased from 9 to 19 mol PAR/m2. In contrast, oleic content decreased linearly in this irradiance range. Additionally, we advanced knowledge regarding the interactions among irradiance and leaf, fruit number, size and composition at organ-, tissue- and cellular- levels. The irradiance received at different positions in the canopy strongly affected the leaf area and chlorophyll content, and mesocarp size and composition (water and oil), without effects on endocarp size and composition. At the cellular level, light-exposed fruit developed larger mesocarp cells than shaded fruits, but cell number was not affected. Our results indicate that cell number and size are related to mesocarp composition in term of oil, water, and dry weight menus oil, although the specific manner in which they interact remains to be determined. This research contributes from an integral perspective of olive growing to quantify the impact of row orientation and width alley on productivity and oil quality in hedgerows systems. The analysis and discussion of the relationships between radiation and yield components and oil quality can help understand the impact of design olive hedgerows in general and in a wide range of environmental conditions.

Heated fiber optic distributed temperature sensing for measuring soil volumetric heat capacity and water content: A dual probe heat-pulse approach

The first feasibility study of using dual-probe heated fiber optics with distributed temperature sensing to measure soil volumetric heat capacity and soil water content is presented. Although results using different combinations of cables demonstrate feasibility, further work is needed to gain accuracy, including a model to account for the finite dimension and the thermal influence of the probes. Implementation of the dual-probe heat-pulse (DPHP) approach for measurement of volumetric heat capacity (C) and water content (θ) with distributed temperature sensing heated fiber optic (FO) systems presents an unprecedented opportunity for environmental monitoring (e.g., simultaneous measurement at thousands of points). We applied uniform heat pulses along a FO cable and monitored the thermal response at adjacent cables. We tested the DPHP method in the laboratory using multiple FO cables at a range of spacings. The amplitude and phase shift in the heat signal with distance was found to be a function of the soil volumetric heat capacity. Estimations of C at a range of moisture contents (θ = 0.09– 0.34 m3 m−3) suggest the feasibility of measurement via responsiveness to the changes in θ, although we observed error with decreasing soil water contents (up to 26% at θ = 0.09 m3 m−3). Optimization will require further models to account for the finite radius and thermal influence of the FO cables. Although the results indicate that the method shows great promise, further study is needed to quantify the effects of soil type, cable spacing, and jacket configurations on accuracy.

Single-pair fluorescence resonance energy transfer on freely diffusing molecules: Observation of Förster distance dependence and subpopulations

Photon bursts from single diffusing donor-acceptor labeled macromolecules were used to measure intramolecular distances and identify subpopulations of freely diffusing macromolecules in a heterogeneous ensemble. By using DNA as a rigid spacer, a series of constructs with varying intramolecular donor-acceptor spacings were used to measure the mean and distribution width of fluorescence resonance energy transfer (FRET) efficiencies as a function of distance. The mean single-pair FRET efficiencies qualitatively follow the distance dependence predicted by Förster theory. Possible contributions to the widths of the FRET efficiency distributions are discussed, and potential applications in the study of biopolymer conformational dynamics are suggested. The ability to measure intramolecular (and intermolecular) distances for single molecules implies the ability to distinguish and monitor subpopulations of molecules in a mixture with different distances or conformational states. This is demonstrated by monitoring substrate and product subpopulations before and after a restriction endonuclease cleavage reaction. Distance measurements at single-molecule resolution also should facilitate the study of complex reactions such as biopolymer folding. To this end, the denaturation of a DNA hairpin was examined by using single-pair FRET.

Molecular evolution of integrins: Genes encoding integrin β subunits from a coral and a sponge

The integrin family of cell surface receptors is strongly conserved in higher animals, but the evolutionary history of integrins is obscure. We have identified and sequenced cDNAs encoding integrin β subunits from a coral (phylum Cnidaria) and a sponge (Porifera), indicating that these proteins existed in the earliest stages of metazoan evolution. The coral βCn1 and, especially, the sponge βPo1 sequences are the most divergent of the “β1-class” integrins and share a number of features not found in any other vertebrate or invertebrate integrins. Perhaps the greatest difference from other β subunits is found in the third and fourth repeats of the cysteine-rich stalk, where the generally conserved spacings between cysteines are highly variable, but not similar, in βCn1 and βPo1. Alternatively spliced cDNAs, containing a stop codon about midway through the full-length translated sequence, were isolated from the sponge library. These cDNAs appear to define a boundary between functional domains, as they would encode a protein that includes the globular ligand-binding head but would be missing the stalk, transmembrane, and cytoplasmic domains. These and other sequence comparisons with vertebrate integrins are discussed with respect to models of integrin structure and function.

Cross-validated maximum likelihood enhances crystallographic simulated annealing refinement

Recently, the target function for crystallographic refinement has been improved through a maximum likelihood analysis, which makes proper allowance for the effects of data quality, model errors, and incompleteness. The maximum likelihood target reduces the significance of false local minima during the refinement process, but it does not completely eliminate them, necessitating the use of stochastic optimization methods such as simulated annealing for poor initial models. It is shown that the combination of maximum likelihood with cross-validation, which reduces overfitting, and simulated annealing by torsion angle molecular dynamics, which simplifies the conformational search problem, results in a major improvement of the radius of convergence of refinement and the accuracy of the refined structure. Torsion angle molecular dynamics and the maximum likelihood target function interact synergistically, the combination of both methods being significantly more powerful than each method individually. This is demonstrated in realistic test cases at two typical minimum Bragg spacings (dmin = 2.0 and 2.8 Å, respectively), illustrating the broad applicability of the combined method. In an application to the refinement of a new crystal structure, the combined method automatically corrected a mistraced loop in a poor initial model, moving the backbone by 4 Å.

Structure of the ripple phase in lecithin bilayers.

The phases of the x-ray form factors are derived for the ripple (Pbeta') thermodynamic phase in the lecithin bilayer system. By combining these phases with experimental intensity data, the electron density map of the ripple phase of dimyristoyl-phosphatidylcholine is constructed. The phases are derived by fitting the intensity data to two-dimensional electron density models, which are created by convolving an asymmetric triangular ripple profile with a transbilayer electron density profile. The robustness of the model method is indicated by the result that many different models of the transbilayer profile yield essentially the same phases, except for the weaker, purely ripple (0,k) peaks. Even with this residual ambiguity, the ripple profile is well determined, resulting in 19 angstroms for the ripple amplitude and 10 degrees and 26 degrees for the slopes of the major and the minor sides, respectively. Estimates for the bilayer head-head spacings show that the major side of the ripple is consistent with gel-like structure, and the minor side appears to be thinner with lower electron density.

Periodicity of strong nucleosome positioning sites around the chicken adult beta-globin gene may encode regularly spaced chromatin.

Positioned nucleosomes contribute to both the structure and the function of the chromatin fiber and can play a decisive role in controlling gene expression. We have mapped, at high resolution, the translational positions adopted by limiting amounts of core histone octamers reconstituted onto 4.4 kb of DNA comprising the entire chicken adult beta-globin gene, its enhancer, and flanking sequences. The octamer displays extensive variation in its affinity for different positioning sites, the range exhibited being about 2 orders of magnitude greater than that of the initial binding of the octamer. Strong positioning sites are located 5' and 3' of the globin gene and in the second intron but are absent from the coding regions. These sites exhibit a periodicity (approximately 200 bp) similar to the average spacing of nucleosomes on the inactive beta-globin gene in vivo, which could indicate their involvement in packaging the gene into higher-order chromatin structure. Overlapping, alternative octamer positioning sites commonly exhibit spacings of 20 and 40 bp, but not of 10 bp. These short-range periodicities could reflect features of the core particle structure contributing to the pronounced sequence-dependent manner in which the core histone octamer interacts with DNA.

Discontinuity spacing analysis in rock masses using 3D point clouds

The complete characterization of rock masses implies the acquisition of information of both, the materials which compose the rock mass and the discontinuities which divide the outcrop. Recent advances in the use of remote sensing techniques – such as Light Detection and Ranging (LiDAR) – allow the accurate and dense acquisition of 3D information that can be used for the characterization of discontinuities. This work presents a novel methodology which allows the calculation of the normal spacing of persistent and non-persistent discontinuity sets using 3D point cloud datasets considering the three dimensional relationships between clusters. This approach requires that the 3D dataset has been previously classified. This implies that discontinuity sets are previously extracted, every single point is labeled with its corresponding discontinuity set and every exposed planar surface is analytically calculated. Then, for each discontinuity set the method calculates the normal spacing between an exposed plane and its nearest one considering 3D space relationship. This link between planes is obtained calculating for every point its nearest point member of the same discontinuity set, which provides its nearest plane. This allows calculating the normal spacing for every plane. Finally, the normal spacing is calculated as the mean value of all the normal spacings for each discontinuity set. The methodology is validated through three cases of study using synthetic data and 3D laser scanning datasets. The first case illustrates the fundamentals and the performance of the proposed methodology. The second and the third cases of study correspond to two rock slopes for which datasets were acquired using a 3D laser scanner. The second case study has shown that results obtained from the traditional and the proposed approaches are reasonably similar. Nevertheless, a discrepancy between both approaches has been found when the exposed planes members of a discontinuity set were hard to identify and when the planes pairing was difficult to establish during the fieldwork campaign. The third case study also has evidenced that when the number of identified exposed planes is high, the calculated normal spacing using the proposed approach is minor than those using the traditional approach.