Remote sensed data for automatic detection of land-use changes due to human activity in support to landslide studies

Slope instability studies appear to recognize a number of potential superficial slide-producing agents, which may be directly detected and monitored with Earth Observation (EO) data. The main objective of this work is to use conventional EO data and automatic techniques for providing land-use change maps useful in landslide prevention. The idea is to use the detection of changes in areas already involved in landslide events as a precursory sign of variations in the equilibrium status of the slope, independently from other natural triggering events, such as rain and seismic events. Attention is focused on man-induced surface changes, such as deforestation, urban expansion and construction of artificial structures. A historical set of 20 multi-temporal Landsat TM images, covering the period 1987–2000, was analyzed using a supervised change detection technique on a test site affected by slope instability phenomena located in the Abruzzo region in Southern Italy. A change image is obtained by comparing year-specific thematic map pairs. It contains useful information not only on the place where a transition occurred, but also on the specific classes involved in the transitions between two different years. The full set of change images is used to extract class-conditional transition probabilities, to evaluate variations in specific class distribution and the total number of changed pixels in time. Four classes and their transitions were considered in the analysis: (1) arboreous land, (2) agricultural land, (3) barren land, and (4) artificial structures. The quantitative analysis of the class-joint transition probability values of some specific class-transitions that may worsen slope stability showed that in an area prone to landslides the probability of landslide re-activation or first activation is higher where changes have occurred. Although based on a limited number of known events, such a result encourages extensive experimentation of the proposed technique on better documented landslide test sites.     

Analysis of the rock accretions in the lower pecos region of southwest texas

Calcium oxalate (whewellite) was found to be the primary component of crusts on limestone in the dry rock shelters throughout the Lower Pecos region of Texas. This material forms a translucent patina that covers the pictographs in this area. Evidence from analyses using SEM/EDS, FTIR, XRD, Raman spectroscopy, and AMS is presented that suggests the oxalate-rich crusts were produced by metabolic activity of lichen or fungi on or near the surface of the limestone substrate. The paucity of hyphae and microbes in samples studied using SEM may indicate that the organisms responsible for the production of the oxalate are no longer present on the shelter walls. Radiocarbon ages of three oxalate samples range from 2100 to 5570 years B. P., indicating that the crust may be used for obtaining chronological information on the rock art.     

Short-term,linear, and non-linear local effects of the tides on the surface dynamics in a new,high-resolution model of the Mediterranean Sea circulation

Ocean Dynamics - The tides in the Mediterranean Sea are generally weaker than in other regions of the world ocean, but are locally intensified in passages with complex bathymetry, such as the...     

Investigating pesticide transport in the León-Chinandega aquifer, Nicaragua

Nicaragua’s León-Chinandega aquifer has seen extensive contamination by persistent organochlorine pesticides applied over decades of intensive agricultural activity. Models of flow and transport of a 330 km² sub-region of the aquifer were developed to test conceptual models of contaminant transport, to constrain the value of certain key transport parameters, and to investigate contamination-related concerns raised in past studies. To support these models, a variety of hydrogeologic and geochemical data were collected. It was concluded that the organochlorine pesticides seen in groundwater originate in soils, and are transported to the water table through widespread preferential flow, through shortcutting around wells, or through wind-blown particles delivered to poorly protected hand-dug wells. The distribution coefficient (K _d) of these pesticides is estimated to be between 0.1 and 100 ml/g and the concentration of pesticides being delivered to the water table is estimated to be between 10² and 10⁵ ng/L. It was found that the distribution and concentration of pesticides in the aquifer would be affected by an increase in groundwater abstraction within the region.

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Résumé L’aquifère du León-Chinandega au Nicaragua a été soumis à des contaminations étendues par des pesticides organochlorés persistants qui ont été répandus pendant des dizaines d’années d’agriculture intensive. Des modèles d’écoulement et de transport d’une sous-région de 330 km² de l’aquifère ont été construits pour tester des modèles conceptuels du transport de contaminants, pour contraindre la valeur de certains paramètres de transport clefs, et pour étudier les problèmes liés au transport de contaminations qui avaient été rencontrés lors d’études précédentes. Différents types de données hydrogéologiques et géochimiques ont été collectés pour réaliser ces modèles. La conclusion montre que les pesticides organochlorés rencontrés dans les eaux souterraines proviennent des sols et qu’ils sont transportés jusqu’à l’aquifère via de grandes zones d’écoulement préférentiel, via des raccourcis hydrauliques autour des puits, ou encore via des particules emportées par le vent et tombées dans des puits creusés à la main et mal protégés. Le coefficient de distribution (K _d) de ces pesticides est estimé entre 0.1 et 100 ml/g et la concentration de pesticides arrivant dans la nappe est estimée entre 10² et 10⁵ ng/L. L’étude a montré qu’une augmentation des prélèvements d’eau souterraine dans la région aurait un impact sur la distribution et la concentration des pesticides dans l’aquifère.

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Resumen El acuifero León-Chinandega (Nicaragua) presenta una contaminación extensiva por la aplicación de plaguicidas organoclorados en la agricultura intensiva durante décadas. Se han desarrollado modelos de flujo y transporte de una subregión del acuífero de 330 km² para comprobar los modelos conceptuales del transporte de contaminantes, estimar los valores de ciertos parámetros clave de transporte e investigar los temas relacionados con la contaminación en estudios anteriores. Para elaborar estos modelos, se recogió una variedad de datos hidrogeológicos y geoquímicos. Se ha concluido que los plaguicidas organoclorados presentes en el agua subterránea se originan en el suelo y son transportados hacia el nivel freático a través de flujos preferentes generalizados, a través de cortes alrededor de los pozos o a través de partículas transportadas por el viento depositadas en pozos excavados a mano con poca protección. El coeficiente de distribución (K _d) de estos plaguicidas se ha estimado entre 0.1 y 100 ml/g y la concentración de plaguicidas que sale hacia el nivel freático se estima que puede estar entre 10² y 10⁵ ng/L. Se ha concluido que el incremento de la extracción de aguas subterráneas dentro de la región afectaría la distribución y concentración de plaguicidas en el acuífero.

     

The future of Stardust science

Recent observations indicate that >99% of the small bodies in the solar system reside in its outer reaches—in the Kuiper Belt and Oort Cloud. Kuiper Belt bodies are probably the best‐preserved representatives of the icy planetesimals that dominated the bulk of the solid mass in the early solar system. They likely contain preserved materials inherited from the protosolar cloud, held in cryogenic storage since the formation of the solar system. Despite their importance, they are relatively underrepresented in our extraterrestrial sample collections by many orders of magnitude (~10¹³ by mass) as compared with the asteroids, represented by meteorites, which are composed of materials that have generally been strongly altered by thermal and aqueous processes. We have only begun to scratch the surface in understanding Kuiper Belt objects, but it is already clear that the very limited samples of them that we have in our laboratories hold the promise of dramatically expanding our understanding of the formation of the solar system. Stardust returned the first samples from a known small solar system body, the Jupiter‐family comet 81P/Wild 2, and, in a separate collector, the first solid samples from the local interstellar medium. The first decade of Stardust research resulted in more than 142 peer‐reviewed publications, including 15 papers in Science. Analyses of these amazing samples continue to yield unexpected discoveries and to raise new questions about the history of the early solar system. We identify nine high‐priority scientific objectives for future Stardust analyses that address important unsolved problems in planetary science.     

Low resistivity zones at contacts of igneous intrusions emplaced in organic-rich formations and their implications on fluid flow and petroleum systems: A case study in the northern Neuquén Basin,Argentina

Igneous sills and laccoliths emplaced in sedimentary basins may significantly impact petroleum systems, both positively and negatively. Igneous intrusions provide heat to maturate regionally immature organic-rich host rocks, act as fractured reservoirs hosting commercial accumulations of hydrocarbons, and form structures affecting fluid flow and trapping at different scales. Nevertheless, the petrophysical implications of igneous intrusions on their host rock are poorly known. In this study, we analyse 200 wells in the Río Grande Valley oil field, Neuquén basin, Argentina, where the main reservoirs are in fractured igneous sills. This dataset represents a globally unique possibility to characterize the igneous–host rock interaction using both wireline logs and core material. We identify a systematic Contact Low Resistivity Zone (CLRsZ) at both the upper and lower contacts of the sills emplaced in the organic-rich Vaca Muerta and Agrio Formations. We characterize the nature of these CLRsZ and their petrophysical properties by integrating resistivity and gamma ray well logs, petrographic analyses, petrophysical tests and geochemical analyses. The low resistivity signal of the CLRsZ is dominantly carried by massive-sulphide deposits, mainly pyrite, observed both in the host rock and the chilled margin of the sills. Well log images and porosity-permeability analysis on core plugs show that both the sills and their associated CLRsZ can act as carrier for fluid flow and reservoir for hydrocarbons storage. The thickness of the upper and lower CLRsZ correlates linearly with the thickness of the sill, and the volume of both the upper and lower CLRsZ represents ca. 40% with respect to the volume of their associated sill. The thickness of the CLRsZ represents ca. 13% of the thickness of contact aureole induced by the sills. In the CLRsZ, a great proportion of kerogen was transformed to hydrocarbon, so that CLRsZ were restricted to the innermost contact aureole of the sills. Our results show that the CLRsZ can have major implications on fluid flow and should be considered in reservoir models in volcanic basins hosting sills emplaced in organic-rich formations.