Hydrogeochemistry of surface and spring waters in the surroundings of the CO2 injection site at Hontomín–Huermeces (Burgos, Spain)

In this paper the very first geochemical and isotopic data related to surface and spring waters and dissolved gases in the area of Hontomín–Huermeces (Burgos, Spain) are presented and discussed. Hontomín–Huermeces has been selected as a pilot site for the injection of pure (>99%) CO2. Injection and monitoring wells are planned to be drilled close to 6 oil wells completed in the 1980s for which detailed stratigraphical logs are available, indicating the presence of a confined saline aquifer at the depth of about 1500 m into which less than 100,000 tons of iquid CO2 will be injected, possibly starting in 2013. The chemical and features of the spring waters suggest that they are related to a shallow hydrogeological system as the concentration of the Total Dissolved Solids approaches 800 mg/L with a Ca2+(Mg2+)-HCO3− composition, similar to that of the surface waters. This is also supported by the oxygen and hydrogen isotopic ratios that have values lying between those of the Global and the Mediterranean Meteoric Water Lines. Some spring waters close to the oil wells are haracterized by relatively high concentrations of NO3− (up to 123 mg/L), unequivocally suggesting an anthropogenic source that adds to the main water–rock interaction processes. The latter can be referred to Ca-Mg-carbonate and, at a minor extent, Al-silicate dissolution, being the outcropping sedimentary rocks characterized by Palaeozoic to Quaternary rocks. Anomalous concentrations of Cl−, SO42−, As, B and Ba were measured in two springs discharging a few hundred meters from the oil wells and in the Rio Ubierna. These contents are significantly higher than those of the whole set of the studied waters and are possibly indicative of mixing processes, although at very low extent, between deep and shallow aquifers. No evidence of deep-seated gases interacting with the Hontomín–Huermeces waters was recognized in the chemistry of the disolved gases. This is likely due to the fact that they are mainly characterized by an atmospheric source as highlighted by the high contents of N2, O2 and Ar and by N2/Ar ratios that approach that of ASW (Air Saturated Water) and possibly masking any contribution related to a deep source. Nevertheless, significant concentrations (up to 63% by vol.) of isotopically negative CO2 (<−17.7‰ V-PDB) were found in some water samples, likely related to a biogenic source. The geochemical and isotopic data of this work are of particular importance when a monitoring program will be established to verify whether CO2 leakages, induced by the injection of this greenhouse gas, may be affecting the quality of the waters in the shallow hydrological circuits at Hontomín–Huermeces. In this respect, carbonate chemistry, the isotopic carbon of dissolved CO2 and TDIC (Total Dissolved Inorganic Carbon) and selected trace elements can be considered as useful parameters to trace the migration of the injected CO2 into near-surface environments.

Surface InGaAs nanostructures for sensing applications

El desarrollo de sensores está ganando cada vez mayor importancia debido a la concienciación ciudadana sobre el medio ambiente haciendo que su desarrollo sea muy elevado en todas las disciplinas, entre las que cabe destacar, la medicina, la biología y la química. A pesar de la existencia de estos dispositivos, este área está aún por mejorar, ya que muchos de los materiales propuestos hasta el momento e incluso los ya comercializados muestran importantes carencias de funcionamiento, eficiencia e integrabilidad entre otros. Para la mejora de estos dispositivos, se han propuesto diversas aproximaciones basadas en nanosistemas. Quizá, uno de las más prometedoras son las nanoestructuras de punto cuántico, y en particular los semiconductores III-V basados en la consolidada tecnología de los arseniuros, las cuáles ofrecen excelentes propiedades para su uso como sensores. Además, estudios recientes demuestran su gran carácter sensitivo al medio ambiente, la posibilidad de funcionalizar la superficie para la fabricación de sensores interdisciplinares y posibilididad de mejorar notablemente su eficiencia. A lo largo de esta tesis, nos centramos en la investigación de SQD de In0.5Ga0.5As sobre substratos de GaAs(001) para el desarrollo de sensores de humedad. La tesis abarca desde el diseño, crecimiento y caracterización de las muestras hasta la el posterior procesado y caracterización de los dispositivos finales. La optimización de los parámetros de crecimiento es fundamental para conseguir una nanoestructura con las propiedades operacionales idóneas para un fin determinado. Como es bien sabido en la literatura, los parámetros de crecimiento (temperatura de crecimiento, relación de flujos del elemento del grupo V y del grupo I II (V/III), velocidad de crecimiento y tratamiento térmico después de la formación de la capa activa) afectan directamente a las propiedades estructurales, y por tanto, operacionales de los puntos cuánticos (QD). En esta tesis, se realiza un estudio de las condiciones de crecimiento para el uso de In0.5Ga0.5As SQDs como sensores. Para los parámetros relacionados con la temperatura de crecimiento de los QDs y la relación de flujos V / I I I se utilizan los estudios previamente realizados por el grupo. Mientras que este estudio se centrará en la importancia de la velocidad de crecimiento y en el tratamiento térmico justo después de la nucleación de los QDs. Para ello, se establece la temperatura de creciemiento de los QDs en 430°C y la relación de flujos V/III en 20. Como resultado, los valores más adecuados que se obtienen para la velocidad de crecimiento y el tratamiento térmico posterior a la formación de los puntos son, respectivamente, 0.07ML/s y la realización de una bajada y subida brusca de la temperatura del substrato de 100°C con respecto a la temperatura de crecimiento de los QDs. El crecimiento a una velocidad lo suficientemente alta que permita la migración de los átomos por la superficie, pero a su vez lo suficientemente baja para que se lleve a cabo la nucleación de los QDs; en combinación con el tratamiento brusco de temperatura que hace que se conserve la forma y composición de los QDs, da lugar a unos SQDs con un alto grado de homogeneidad y alta densidad superficial. Además, la caracterización posterior indica que estas nanoestructuras de gran calidad cristalina presentan unas propiedades ópticas excelentes incluso a temperatura ambiente. Una de las características por la cual los SQD de Ino.5Gao.5As se consideran candidatos prometedores para el desarrollo de sensores es el papel decisivo que juega la superficie por el mero hecho de estar en contacto directo con las partículas del ambiente y, por tanto, por ser capaces de interactuar con sus moléculas. Así pues, con el fin de demostrar la idoneidad de este sistema para dicha finalidad, se evalúa el impacto ambiental en las propiedades ópticas y eléctricas de las muestras. En un primer lugar, se analiza el efecto que tiene el medio en las propiedades ópticas. Para dicha evaluación se compara la variación de las propiedades de emisión de una capa de puntos enterrada y una superficial en distintas condiciones externas. El resultado que se obtiene es muy claro, los puntos enterrados no experimentan un cambio óptico apreciable cuando se varían las condiciones del entorno; mientras que, la emisión de los SQDs se modifica significativamente con las condiciones del medio. Por una parte, la intensidad de emisión de los puntos superficiales desaparece en condiciones de vacío y decrece notablemente en atmósferas secas de gases puros (N2, O2). Por otra parte, la fotoluminiscencia se conserva en ambientes húmedos. Adicionalmente, se observa que la anchura a media altura y la longitud de onda de emisión no se ven afectadas por los cambios en el medio, lo que indica, que las propiedades estructurales de los puntos se conservan al variar la atmósfera. Estos resultados apuntan directamente a los procesos que tienen lugar en la superficie entre estados confinados y superficiales como responsables principales de este comportamiento. Así mismo, se ha llevado a cabo un análisis más detallado de la influencia de la calidad y composición de la atmósfera en las propiedades ópticas de los puntos cuánticos superficiales. Para ello, se utilizan distintas sustancias con diferente polaridad, composición atómica y masa molecular. Como resultado se observa que las moléculas de menor polaridad y más pesadas causan una mayor variación en la intensidad de emisión. Además, se demuestra que el oxígeno juega un papel decisivo en las propiedades ópticas. En presencia de moléculas que contienen oxígeno, la intensidad de fotoluminiscencia disminuye menos que en atmósferas constituidas por especies que no contienen oxígeno. Las emisión que se observa respecto a la señal en aire es del 90% y del 77%, respectivamente, en atmósferas con presencia o ausencia de moléculas de oxígeno. El deterioro de la señal de emisión se atribuye a la presencia de defectos, enlaces insaturados y, en general, estados localizados en la superficie. Estos estados actúan como centros de recombinación no radiativa y, consecuentemente, se produce un empeoramiento de las propiedades ópticas de los SQDs. Por tanto, la eliminación o reducción de la densidad de estos estados superficiales haría posible una mejora de la intensidad de emisión. De estos experimentos de fotoluminiscencia, se deduce que las interacciones entre las moléculas presentes en la atmósfera y la superficie de la muestra modifican la superficie. Esta alteración superficial se traduce en un cambio significativo en las propiedades de emisión. Este comportamiento se atribuye a la posible adsorción de moléculas sobre la superficie pasivando los centros no radiativos, y como consecuencia, mejorando las propiedades ópticas. Además, los resultados demuestran que las moléculas que contienen oxígeno con mayor polaridad y más ligeras son adsorbidas con mayor facilidad, lo que hace que la intensidad óptica sufra variaciones despreciables con respecto a la emisión en aire. Con el fin de desarrollar sensores, las muestras se procesan y los dispositivos se caracterizan eléctricamente. El procesado consiste en dos contactos cuadrados de una aleación de Ti/Au. Durante el procesado, lo más importante a tener en cuenta es no realizar ningún ataque o limpieza que pueda dañar la superficie y deteriorar las propiedades de las nanostructuras. En este apartado, se realiza un análisis completo de una serie de tres muestras: GaAs (bulk), un pozo cuántico superficial (SQW) de Ino.5Gao.5As y SQDs de Ino.5Gao.5As. Para ello, a cada una de las muestras se le realizan medidas de I-V en distintas condiciones ambientales. En primer lugar, siguiendo los resultados obtenidos ópticamente, se lleva a cabo una comparación de la respuesta eléctrica en vacío y aire. A pesar de que todas las muestras presentan un carácter más resistivo en vacío que en aire, se observa una mayor influencia sobre la muestra de SQD. En vacío, la resistencia de los SQDs decrece un 99% respecto de su valor en aire, mientras que la variación de la muestras de GaAs e Ino.5Gao.5As SQW muestran una reducción, respectivamente, del 31% y del 20%. En segundo lugar, se realiza una evaluación aproximada del posible efecto de la humedad en la resistencia superficial de las muestras mediante la exhalación humana. Como resultado se obtiene, que tras la exhalación, la resistencia disminuye bruscamente y recupera su valor inicial cuando dicho proceso concluye. Este resultado preliminar indica que la humedad es un factor crítico en las propiedades eléctricas de los puntos cuánticos superficiales. Para la determinación del papel de la humedad en la respuesta eléctrica, se somete a las muestras de SQD y SQW a ambientes con humedad relativa (RH, de la siglas del inglés) controlada y se analiza el efecto sobre la conductividad superficial. Tras la variación de la RH desde 0% hasta el 70%, se observa que la muestra SQW no cambia su comportamiento eléctrico al variar la humedad del ambiente. Sin embargo, la respuesta de la muestra SQD define dos regiones bien diferenciadas, una de alta sensibilidad para valores por debajo del 50% de RH, en la que la resistencia disminuye hasta en un orden de magnitud y otra, de baja sensibilidad (>50%), donde el cambio de la resistencia es menor. Este resultado resalta la especial relevancia no sólo de la composición sino también de la morfología de la nanostructura superficial en el carácter sensitivo de la muestra. Por último, se analiza la influencia de la iluminación en la sensibilidad de la muestra. Nuevamente, se somete a las muestras SQD y SQW a una irradiación de luz de distinta energía y potencia a la vez que se varía controladamente la humedad ambiental. Una vez más, se observa que la muestra SQW no presenta ninguna variación apreciable con las alteraciones del entorno. Su resistencia superficial permanece prácticamente inalterable tanto al modificar la potencia de la luz incidente como al variar la energía de la irradiación. Por el contrario, en la muestra de SQD se obtiene una reducción la resistencia superficial de un orden de magnitud al pasar de condiciones de oscuridad a iluminación. Con respecto a la potencia y energía de la luz incidente, se observa que a pesar de que la muestra no experimenta variaciones notables con la potencia de la irradiación, esta sufre cambios significativos con la energía de la luz incidente. Cuando se ilumina con energías por encima de la energía de la banda prohibida (gap) del GaAs (Eg ~1.42 eV ) se produce una reducción de la resistencia de un orden de magnitud en atmósferas húmedas, mientras que en atmósferas secas la conductividad superficial permanece prácticamente constante. Sin embargo, al inicidir con luz de energía menor que Eg, el efecto que se produce en la respuesta eléctrica es despreciable. Esto se atribuye principalmente a la densidad de portadores fotoactivados durante la irradiación. El volumen de portadores excita dos depende de la energía de la luz incidente. De este modo, cuando la luz que incide tiene energía menor que el gap, el volumen de portadores generados es pequeño y no contribuye a la conductividad superficial. Por el contrario, cuando la energía de la luz incidente es alta (Eg), el volumen de portadores activados es elevado y éstos contribuyen significantemente a la conductividad superficial. La combinación de ambos agentes, luz y humedad, favorece el proceso de adsorción de moléculas y, por tanto, contribuye a la reducción de la densidad de estados superficiales, dando lugar a una modificación de la estructura electrónica y consecuentemente favoreciendo o dificultando el transporte de portadores. ABSTRACT Uncapped three-dimensional (3D) nanostructures have been generally grown to assess their structural quality. However, the tremendous growing importance of the impact of the environment on life has become such nanosystems in very promising candidates for the development of sensing devices. Their direct exposure to changes in the local surrounding may influence their physical properties being a perfect sign of the atmosphere quality. The goal of this thesis is the research of Ino.5Gao.5As surface quantum dots (SQDs) on GaAs(001), covering from their growth to device fabrication, for sensing applications. The achievement of this goal relies on the design, growth and sample characterization, along with device fabrication and characterization. The first issue of the thesis is devoted to analyze the main growth parameters affecting the physical properties of the Ino.5Gao.5As SQDs. It is well known that the growing conditions (growth temperature , deposition rate, V/III flux ratio and treatment after active layer growth) directly affect the physical properties of the epilayer. In this part, taking advantage of the previous results in the group regarding Ino.5Gao.5As QD growth temperature and V/III ratio, the effect of the growth rate and the temperature treatment after QDs growth nucleation is evaluated. Setting the QDs growth temperature at 430°C and the V/III flux ratio to ~20, it is found that the most appropriate conditions rely on growing the QDs at 0.07ML/s and just after QD nucleation, rapidly dropping and again raising 100°C the substrate temperature with respect to the temperature of QD growth. The combination of growing at a fast enough growth rate to promote molecule migration but sufficiently slow to allow QD nucleation, together with the sharp variation of the temperature preserving their shape and composition yield to high density, homogeneous Ino.5Gao.5As SQDs. Besides, it is also demonstrated that this high quality SQDs show excellent optical properties even at room temperature (RT). One of the characteristics by which In0.5Ga0.5As/GaAs SQDs are considered promising candidates for sensing applications is the crucial role that surface plays when interacting with the gases constituting the atmosphere. Therefore, in an attempt to develop sensing devices, the influence of the environment on the physical properties of the samples is evaluated. By comparing the resulting photoluminescence (PL) of SQDs with buried QDs (BQDs), it is found that BQDs do not exhibit any significant variation when changing the environmental conditions whereas, the external conditions greatly act on the SQDs optical properties. On one hand, it is evidenced that PL intensity of SQDs sharply quenches under vacuum and clearly decreases under dry-pure gases atmospheres (N2, O2). On the other hand, it is shown that, in water containing atmospheres, the SQDs PL intensity is maintained with respect to that in air. Moreover, it is found that neither the full width at half maximun nor the emission wavelength manifest any noticeable change indicating that the QDs are not structurally altered by the external atmosphere. These results decisively point to the processes taking place at the surface such as coupling between confined and surface states, to be responsible of this extraordinary behavior. A further analysis of the impact of the atmosphere composition on the optical characteristics is conducted. A sample containing one uncapped In0.5Ga0.5As QDs layer is exposed to different environments. Several solvents presenting different polarity, atomic composition and molecular mass, are used to change the atmosphere composition. It is revealed that low polarity and heavy molecules cause a greater variation on the PL intensity. Besides, oxygen is demonstrated to play a decisive role on the PL response. Results indicate that in presence of oxygen-containing molecules, the PL intensity experiments a less reduction than that suffered in presence of nonoxygen-containing molecules, 90% compared to 77% signal respect to the emission in air. In agreement with these results, it is demonstrated that high polarity and lighter molecules containing oxygen are more easily adsorbed, and consequently, PL intensity is less affected. The presence of defects, unsaturated bonds and in general localized states in the surface are proposed to act as nonradiative recombination centers deteriorating the PL emission of the sample. Therefore, suppression or reduction of the density of such states may lead to an increase or, at least, conservation of the PL signal. This research denotes that the interaction between sample surface and molecules in the atmosphere modifies the surface characteristics altering thus the optical properties. This is attributed to the likely adsoption of some molecules onto the surface passivating the nonradiative recombination centers, and consequently, not deteriorating the PL emission. Aiming for sensors development, samples are processed and electrically characterized under different external conditions. Samples are processed with two square (Ti/Au) contacts. During the processing, especial attention must be paid to the surface treatment. Any process that may damage the surface such as plasma etching or annealing must be avoided to preserve the features of the surface nanostructures. A set of three samples: a GaAs (bulk), In0.5Ga0.5As SQDs and In0.5Ga0.5As surface quantum well (SQW) are subjected to a throughout evaluation. I-V characteristics are measured following the results from the optical characterization. Firstly, the three samples are exposed to vacuum and air. Despite the three samples exhibit a more resistive character in vacuum than in air, it is revealed a much more clear influence of the pressure atmosphere in the SQDs sample. The sheet resistance (Rsh) of SQDs decreases a 99% from its response value under vacuum to its value in air, whereas Rsh of GaAs and In0.5Ga0.5As SQW reduces its value a 31% and a 20%, respectively. Secondly, a rough analysis of the effect of the human breath on the electrical response evidences the enormous influence of moisture (human breath is composed by several components but the one that overwhelms all the rest is the high concentration of water vapor) on the I-V characteristics. Following this result, In0.5Ga0.5As SQDs and In0.5Ga0.5As SQW are subjected to different controlled relative humidity (RH) environments (from 0% to 70%) and electrically characterized. It is found that SQW shows a nearly negligible Rsh variation when increasing the RH in the surroundings. However, the response of SQDs to changes in the RH defines two regions. Below 50%, high sensitive zone, Rsh of SQD decreases by more than one order of magnitude, while above 50% the dependence of Rsh on the RH becomes weaker. These results remark the role of the surface and denote the existence of a finite number of surface states. Nevertheless, most significantly, they highlight the importance not only of the material but also of the morphology. Finally, the impact of the illumination is determined by means of irradiating the In0.5Ga0.5As SQDs and In0.5Ga0.5As SQW samples with different energy and power sources. Once again, SQW does not exhibit any correlation between the surface conductivity and the external conditions. Rsh remains nearly unalterable independently of the energy and power of the incident light. Conversely, Rsh of SQD experiences a decay of one order of magnitude from dark-to-photo conditions. This is attributed to the less density of surface states of SQW compared to that of SQDs. Additionally, a different response of Rsh of SQD with the energy of the impinging light is found. Illuminating with high energy light results in a Rsh reduction of one order of mag nitude under humid atmospheres, whereas it remains nearly unchanged under dry environments. On the contrary, light with energy below the bulk energy bandgap (Eg), shows a negligible effect on the electrical properties regardless the local moisture. This is related to the density of photocarriers generated while lighting up. Illuminating with excitation energy below Eg affects a small absorption volume and thus, a low density of photocarriers may be activated leading to an insignificant contribution to the conductivity. Nonetheless, irradiating with energy above the Eg can excite a high density of photocarriers and greatly improve the surface conductivity. These results demonstrate that both illumination and humidity are therefore needed for sensing. The combination of these two agents improves the surface passivation by means of molecule adsorption reducing the density of surface states, thus modifying the electronic structures, and consequently, promoting the carrier motion.

Cuticle Structure in Relation to Chemical Composition: Re-assessing the Prevailing Model

The surface of most aerial plant organs is covered with a cuticle that provides protection against multiple stress factors including dehydration. Interest on the nature of this external layer dates back to the beginning of the 19th century and since then, several studies facilitated a better understanding of cuticular chemical composition and structure. The prevailing undertanding of the cuticle as a lipidic, hydrophobic layer which is independent from the epidermal cell wall underneath stems from the concept developed by Brongniart and von Mohl during the first half of the 19th century. Such early investigations on plant cuticles attempted to link chemical composition and structure with the existing technologies, and have not been directly challenged for decades. Beginning with a historical overview about the development of cuticular studies, this review is aimed at critically assessing the information available on cuticle chemical composition and structure, considering studies performed with cuticles and isolated cuticular chemical components. The concept of the cuticle as a lipid layer independent from the cell wall is subsequently challenged, based on the existing literature, and on new findings pointing toward the cell wall nature of this layer, also providing examples of different leaf cuticle structures. Finally, the need for a re-assessment of the chemical and structural nature of the plant cuticle is highlighted, considering its cell wall nature and variability among organs, species, developmental stages, and biotic and abiotic factors during plant growth.

A peptide that inhibits hydroxyapatite growth is in an extended conformation on the crystal surface

Proteins play an important role in the biological mechanisms controlling hard tissue development, but the details of molecular recognition at inorganic crystal interfaces remain poorly characterized. We have applied a recently developed homonuclear dipolar recoupling solid-state NMR technique, dipolar recoupling with a windowless sequence (DRAWS), to directly probe the conformation of an acidic peptide adsorbed to hydroxyapatite (HAP) crystals. The phosphorylated hexapeptide, DpSpSEEK (N6, where pS denotes phosphorylated serine), was derived from the N terminus of the salivary protein statherin. Constant-composition kinetic characterization demonstrated that, like the native statherin, this peptide inhibits the growth of HAP seed crystals when preadsorbed to the crystal surface. The DRAWS technique was used to measure the internuclear distance between two 13C labels at the carbonyl positions of the adjacent phosphoserine residues. Dipolar dephasing measured at short mixing times yielded a mean separation distance of 3.2 ± 0.1 Å. Data obtained by using longer mixing times suggest a broad distribution of conformations about this average distance. Using a more complex model with discrete α-helical and extended conformations did not yield a better fit to the data and was not consistent with chemical shift analysis. These results suggest that the peptide is predominantly in an extended conformation rather than an α-helical state on the HAP surface. Solid-state NMR approaches can thus be used to determine directly the conformation of biologically relevant peptides on HAP surfaces. A better understanding of peptide and protein conformation on biomineral surfaces may provide design principles useful for the modification of orthopedic and dental implants with coatings and biological growth factors that are designed to enhance biocompatibility with surrounding tissue.

The role of surface loops (residues 204-216 and 627-646) in the motor function of the myosin head.

A characteristic feature of all myosins is the presence of two sequences which despite considerable variations in length and composition can be aligned with loops 1 (residues 204-216) and 2 (residues 627-646) in the chicken myosin-head heavy chain sequence. Recently, an intriguing hypothesis has been put forth suggesting that diverse performances of myosin motors are achieved through variations in the sequences of loops 1 and 2 [Spudich, J. (1994) Nature (London) 372, 515-518]. Here, we report on the study of the effects of tryptic digestion of these loops on the motor and enzymatic functions of myosin. Tryptic digestions of myosin, which produced heavy meromyosin (HMM) with different percentages of molecules cleaved at both loop 1 and loop 2, resulted in the consistent decrease in the sliding velocity of actin filaments over HMM in the in vitro motility assays, did not affect the Vmax, and increased the Km values for actin-activated ATPase of HMM. Selective cleavage of loop 2 on HMM decreased its affinity for actin but did not change the sliding velocity of actin in the in vitro motility assays. The cleavage of loop 1 and HMM decreased the mean sliding velocity of actin in such assays by almost 50% but did not alter its affinity for HMM. To test for a possible kinetic determinant of the change in motility, 1-N6-ethenoadenosine diphosphate (epsilon-ADP) release from cleaved and uncleaved myosin subfragment 1 (S1) was examined. Tryptic digestion of loop 1 slightly accelerated the release of epsilon-ADP from S1 but did not affect the rate of epsilon-ADP release from acto-S1 complex. Overall, the results of this work support the hypothesis that loop 1 can modulate the motor function of myosin and suggest that such modulation involves a mechanism other than regulation of ADP release from myosin.

Azimuthal asymmetry in the risetime of the surface detector signals of the Pierre Auger Observatory.

The azimuthal asymmetry in the risetime of signals in Auger surface detector stations is a source of information on shower development. The azimuthal asymmetry is due to a combination of the longitudinal evolution of the shower and geometrical effects related to the angles of incidence of the particles into the detectors. The magnitude of the effect depends upon the zenith angle and state of development of the shower and thus provides a novel observable, (sec theta)(max), sensitive to the mass composition of cosmic rays above 3 x 10(18) eV. By comparing measurements with predictions from shower simulations, we find for both of our adopted models of hadronic physics (QGSJETII-04 and EPOS-LHC) an indication that the mean cosmic-ray mass increases slowly with energy, as has been inferred from other studies. However, the mass estimates are dependent on the shower model and on the range of distance from the shower core selected. Thus the method has uncovered further deficiencies in our understanding of shower modeling that must be resolved before the mass composition can be inferred from (sec theta)(max).

Spectral features in isolated neutron stars induced by inhomogeneous surface temperatures

The thermal X-ray spectra of several isolated neutron stars display deviations from a pure blackbody. The accurate physical interpretation of these spectral features bears profound implications for our understanding of the atmospheric composition, magnetic field strength and topology, and equation of state of dense matter. With specific details varying from source to source, common explanations for the features have ranged from atomic transitions in the magnetized atmospheres or condensed surface, to cyclotron lines generated in a hot ionized layer near the surface. Here, we quantitatively evaluate the X-ray spectral distortions induced by inhomogeneous temperature distributions of the neutron star surface. To this aim, we explore several surface temperature distributions, we simulate their corresponding general relativistic X-ray spectra (assuming an isotropic, blackbody emission), and fit the latter with a single blackbody model. We find that, in some cases, the presence of a spurious ‘spectral line’ is required at a high significance level in order to obtain statistically acceptable fits, with central energy and equivalent width similar to the values typically observed. We also perform a fit to a specific object, RX J0806.4−4123, finding several surface temperature distributions able to model the observed spectrum. The explored effect is unlikely to work in all sources with detected lines, but in some cases it can indeed be responsible for the appearance of such lines. Our results enforce the idea that surface temperature anisotropy can be an important factor that should be considered and explored also in combination with more sophisticated emission models like atmospheres.

Procedure for calculating the chloride diffusion coefficient and surface concentration from a profile having a maximum beyond the concrete surface

Chlorides induce local corrosion in the steel reinforcements when reaching the bar surface. The measurement of the rate of ingress of these ions, is made by mathematically fitting the so called “error function equation” into the chloride concentration profile, obtaining so the diffusion coefficient and the chloride concentration at the concrete surface. However, the chloride profiles do not always follow Fick’s law by having the maximum concentration at the concrete surface, but often the profile shows a maximum concentration more in the interior, which indicates a different composition and performance of the most external concrete layer with respect to the internal zones. The paper presents a procedure prepared during the time of the RILEM TC 178-TMC: “Testing and modeling chloride penetration in concrete”, which suggests neglecting the external layer where the chloride concentration increases and using the maximum as an “apparent” surface concentration, called C max and to fit the error function equation into the decreasing concentration profile towards the interior. The prediction of evolution should be made also from the maximum.

Desiccant capability of organic xerogels: Surface chemistry vs porous texture

Resorcinol-Formaldehyde xerogels are organic polymers that can be easily tailored to have specific properties. These materials are composed of carbon, hydrogen and oxygen, and have a surface that is very rich in oxygen functionalities, and is therefore very hydrophilic. Their most interesting feature is that they may have the same chemical composition but a different porous texture. Consequently, the influence of porous characteristics, such as pore volume, surface area or pore size can be easily assessed. In this work, a commonly used desiccant, silica gel, is compared with organic xerogels to determine their rate and capacity of water adsorption, and to evaluate the role of surface chemistry versus porous texture. It was found that organic xerogels showed a higher rate of moisture adsorption than silica gel. Pore structure also seems to play an important role in water adsorption capacity. The OX-10 sample, whose porosity was mainly composed of micro-mesoporosity displayed a water adsorption capacity two times greater than that of the silica gel, and three times higher than that of the totally macroporous xerogel OX-2100. The presence of feeder pores (mesopores) that facilitate the access to the hydrophilic surface was observed to be the key factor for a good desiccant behaviour. Neither the total pore volume nor the high surface area (i.e. high microporosity) of the desiccant sample, is as important as the mesopore structure.

Improving the photoactivity of bismuth vanadate thin film photoanodes through doping and surface modification strategies

Currently, one of the most attractive and desirable ways to solve the energy challenge is harvesting energy directly from the sunlight through the so-called artificial photosynthesis. Among the ternary oxides based on earth–abundant metals, bismuth vanadate has recently emerged as a promising photoanode. Herein, BiVO4 thin film photoanodes have been successfully synthesized by a modified metal-organic precursor decomposition method, followed by an annealing treatment. In an attempt to improve the photocatalytic properties of this semiconductor material for photoelectrochemical water oxidation, the electrodes have been modified (i) by doping with La and Ce (by modifying the composition of the BiVO4 precursor solution with the desired concentration of the doping element), and (ii) by surface modification with Au nanoparticles potentiostatically electrodeposited. La and Ce doping at concentrations of 1 and 2 at% in the BiVO4 precursor solution, respectively, enhances significantly the photoelectrocatalytic performance of BiVO4 without introducing important changes in either the material structure or the electrode morphology, according to XRD and SEM characterization. In addition, surface modification of the electrodes with Au nanoparticles further enhances the photocurrent as such metallic nanoparticles act as co-catalysts, promoting charge transfer at the semiconductor/solution interface. The combination of these two complementary ways of modifying the electrodes has resulted in a significant increase in the photoresponse, facilitating their potential application in artificial photosynthesis devices.

The Composition of Holocene Aeolianites; Western Eyre Peninsula, Great Australian Bight, South Australia

The Australian southern continental margin is the world’s largest site of cool-water carbonate deposition, and the Great Australian Bight is its largest sector. The Eyre Peninsula is fringed by coastal beaches with aeolianites and marks the eastern edge of the Great Australian Bight. Five shoreline transects of varying lengths spanned a 150km longitudinal distance and at each the intertidal, beach, dune and secondary dune environments were sampled, for a total of 18 samples. Sediments are a mixture of modern, relict, and Cenozoic carbonates, and quartz grains. Carbonate aeolianites on the western Eyre Peninsula are mostly composed of modern carbonate grains: predominantly molluscs (23-33%) and benthic foraminifera (10-26%), locally abundant coralline algae (3-28%), echinoids (2-22%), and bryozoans (2-14%). Cenozoic grain abundance ranges from 1-6% whereas relict grain abundance ranges from 0-17%. A southward increase in bryozoan particles correlates with a nutrient element abundance and decrease in temperature due to a large seasonal coastal upwelling system that drives 2-3 major upwelling events per year, bringing cold, nutrient rich, Sub-Antarctic Surface Water (<12°C) onto the shelf. In southern, mostly wind protected locations, the beach and dune sediment compositions are similar, indicating that wind energy has successfully carried all sediment components of the beach into the adjacent dunes. In northern, exposed locations, the composition is not the same everywhere, and trends indicate that relative wind energy has the ability to impact grain composition through preferential wind transport. Aeolianite composition is therefore a function of both upwelling and the degree of coastal exposure.

Evolution of the stable carbon isotope composition of atmospheric CO₂ over the last glacial cycle

We present new δ¹³C measurements of atmospheric CO₂ covering the last glacial/interglacial cycle, complementing previous records covering Terminations I and II. Most prominent in the new record is a significant depletion in δ¹³C(atm) of 0.5‰ occurring during marine isotope stage (MIS) 4, followed by an enrichment of the same magnitude at the beginning of MIS 3. Such a significant excursion in the record is otherwise only observed at glacial terminations, suggesting that similar processes were at play, such as changing sea surface temperatures, changes in marine biological export in the Southern Ocean (SO) due to variations in aeolian iron fluxes, changes in the Atlantic meridional overturning circulation, upwelling of deep water in the SO, and long-term trends in terrestrial carbon storage. Based on previous modeling studies, we propose constraints on some of these processes during specific time intervals. The decrease in δ¹³C(atm) at the end of MIS 4 starting approximately 64 kyr B.P. was accompanied by increasing [CO₂]. This period is also marked by a decrease in aeolian iron flux to the SO, followed by an increase in SO upwelling during Heinrich event 6, indicating that it is likely that a large amount of δ¹³C-depleted carbon was transferred to the deep oceans previously, i.e., at the onset of MIS 4. Apart from the upwelling event at the end of MIS 4 (and potentially smaller events during Heinrich events in MIS 3), upwelling of deep water in the SO remained reduced until the last glacial termination, whereupon a second pulse of isotopically light carbon was released into the atmosphere.

Organic geochemistry on surface sediments from the Laptev Sea

Sediment samples from the Laptev Sea, taken during the 1993 RV Polarstern expedition ARK IX/4 and the RV Ivan Kireyev expedition TRANSDRIFT I, were investigated for the amount and composition of their organic carbon fractions. Of major interest was the identification of different processes controlling organic carbon deposition (i.e. terrigenous supply vs. surface water productivity). Long-chain unsaturated alkenones derived from prymnesiophytes, and fatty acids derived from diatoms and dinoflagellates, were analysed by means of gas chromatography and mass spectrometry. First results on the distribution of these biomarkers in surface sediments indicate that the surface water productivity signal is well preserved in the sediment data. This is shown by the distribution of the 16:1(n-7) and 20:5(n-3) fatty acids indicative for diatoms, and the excellent correlation with the chlorophyll a concentrations in the surface water masses and the biogenic-opal content and increased hydrogen indices of the sediments. The high concentration of these unsaturated fatty acids in shallow water sediments shows the recent deposition of the organic material. In deep-sea sediments, on the other hand, the concentrations are low. This decreased content is typical for phytoplankton material which has been degraded by microorganisms or autoxidation. In general, the alkenone concentrations are very low, suggesting low production rates by prymnesiophytes. Only at one station from the lower continental margin influenced by the inflow of Atlantic water masses, were some higher amounts of alkenones determined. Long-chain n-alkanes as well as high C/N ratios and low hydrogen indices indicate the importance of (fluvial) supply of terrigenous organic matter.

(Table 8.4, Page 220-223) Chemical composition of different growth structures of manganese nodules, SONNE cruise SO78

In the nodule field of the Peru Basin, situated south of the zone of high bioproductivity, a relatively high flux of biogenic matter explains a distinct redox boundary at about 10 cm depth separating very soft oxic surface sediments from stiffer suboxic sediments. Maximum abundance (50 kg/m**2) of diagenetic nodules is found near the calcite compensation depth (CCD), currently at 4250 m. There, the accretion rate of nodules is much higher (100 mm/Ma) than on ridges (5 mm/Ma). Highest accretion rates are found at the bottom of large nodules that repeatedly sink to a level immediately above the redox boundary. There, distinct diagenetic growth conditions prevail and layers of dense laminated Mn oxide of very pure todorokite are formed. The layering of nodules is mainly the result of organisms moving nodules within the oxic surface sediment from diagenetic to hydrogenetic environments. The frequency of such movements is much higher than that of climatic changes. Two types of nodule burial occur in the Peru Basin. Large nodules are less easily moved by organisms and become buried. Consequently, buried nodules generally are larger than surface nodules. This type of burial predominates in basins. At ridges where smaller nodules prevail, burial is mainly controlled by statistical selection where some nodules are not moved up by organisms.

Macerals in surface sediments of the Laptev Sea (Arctic Ocean)

Surface sediments from the Laptev Sea and adjacent continental slope were studied for their composition of particulate organic matter (OM) by means of maceral analysis. The composition of macerals in sediments gives information about the environment, terrigenous supply from the hinterland, and marine OM. With reference to their biological sources, we distinguish between terrigenous and marine macerals. We found that the particulate OM in the surface sediments of the Laptev Sea is predominantly of terrigenous origin (mean: 78%). However, distinct variations exist when looking in detail. In the shelf area, sediments may contain up to 99% terrigenous OM. Freshwater algae occur directly north of the river mouths, reflecting the strong fluvial influence. Relatively high amounts of marine OM (20-40%) are restricted to the upper continental slope, the Vilkitsky Strait and west of the New Siberian Islands, explained by increased surface-water productivity due to increased fluvial nutrient supply, open-water conditions, and phytoplankton blooms at the ice-edge.