pinecone/core-2020-05-10-deduplication huggingface dataset:
Hydrologic controls on basin-scale distribution of benthic invertebrates

Streamflow variability is a major determinant of basin-scale distributions of benthic invertebrates. Here we present a novel procedure based on a probabilistic approach aiming at a spatially explicit quantitative assessment of benthic invertebrate abundance as derived from near-bed flow variability. Although the proposed approach neglects ecological determinants other than hydraulic ones, it is nevertheless relevant in view of its implications on the predictability of basin-scale patterns of organisms. In the present context, aquatic invertebrates are considered, given that they are widely employed as sensitive indicators of fluvial ecosystem health and human-induced perturbations. Moving from the analytical characterization of site-specific probability distribution functions of streamflow and bottom shear stress, we achieve a spatial extension to an entire stream network. Bottom shear stress distributions, coupled with habitat suitability curves derived from field studies, are used to produce maps of invertebrate suitability to shear stress conditions. Therefore, the proposed framework allows one to inspect the possible impacts on river ecology of human-induced perturbations of streamflow variability. We apply this framework to an Austrian river network for which rainfall and streamflow time series, river network hydraulic properties, and local information on invertebrate abundance for a limited number of sites are available. A comparison between observed species density versus modeled suitability to shear stress is also presented. Although the proposed strategy focuses on a single controlling factor and thus represents an ecological minimal model, it allows derivation of important implications for water resource management and fluvial ecosystem protection. Key Points Hydrologic variability is a major control of invertebrate habitat suitability New analytical basin-scale approach for pdfs of ecohydrological key features Austrian river basin used for ecohydrological data-model compariso
Hybrid modeling and receding horizon control of sewer networks

In this work, a control-oriented sewer network model is presented based on a hybrid linear modeling framework. The model equations are described independently for each network element, thus allowing the model to be applied to a broad class of networks. A parameter calibration procedure using data obtained from simulation software that solves the physically based model equations is described and validation results are given for a case study. Using the control model equations, an optimal control problem to minimize flooding and pollution is formulated to be solved by means of mixed-integer linear or quadratic programming. A receding horizon control strategy based on this optimal control problem is applied to the case study using the simulation software as a virtual reality. Results of this closed-loop simulation tests show the effectiveness of the proposed approach in fulfilling the control objectives while complying with physical and operational constraints.Peer ReviewedPostprint (author’s final draft
Combined 147,146Sm-143,142Nd constraints on the longevity and residence time of early terrestrial crust

Primordial silicate differentiation controlled the composition of Earth's oldest crust. Inherited 142Nd anomalies in Archean rocks are vestiges of the mantle-crust differentiation before ca. 4300 Ma. Here we report new whole-rock 147,146Sm-143,142Nd data for the Acasta Gneiss Complex (AGC; Northwest Territories, Canada). Our 147Sm-143Nd data combined with literature data define an age of 3371 ± 141 Ma (2 SD) and yield an initial ε143Nd of −5.6 ± 2.1. These results are at odds with the Acasta zircon U-Pb record, which comprises emplacement ages of 3920–3960 Ma. Ten of our thirteen samples show 142Nd deficits of −9.6 ± 4.8 ppm (2 SD) relative to the modern Earth. The discrepancy between 142Nd anomalies and a mid-Archean 147Sm-143Nd age can be reconciled with Nd isotope reequilibration of the AGC during metamorphic perturbations at ca. 3400 Ma. A model age of ca. 4310 Ma is derived for the early enrichment of the Acasta source. Two compositional end-members can be identified: a felsic component with 142Nd/144Nd identical to the modern Earth and a mafic component with 142Nd/144Nd as low as −14.1 ppm. The ca. 4310 Ma AGC source is ∼200 Myr younger than those estimated for Nuvvuagittuq (northern Québec) and Isua (Itsaq Gneiss Complex, West Greenland). The AGC does not have the same decoupled Nd-Hf isotope systematics as these other two terranes, which have been attributed to the crystallization of an early magma ocean. The Acasta signature rather is ascribed to the formation of Hadean crust that was preserved for several hundred Myr. Its longevity can be linked to 142Nd evolution in the mantle and does not require slow mantle stirring times nor modification of its convective mode.This project was funded by an ETH internal grant to BB. We thank Colin Maden for maintenance of the mass spectrometer. SJM acknowledges support from the NASA Exobiology and Evolutionary Biology Program (Investigating the Hadean Earth) and the NASA Lunar Science Institute (Center for Lunar Origin and Evolution, CLOE). Additional support to SJM came from the Laboratoire de Géologie de Lyon, Université Claude Bernard Lyon 1, and a Distinguished Professorship awarded by the Hungarian Academy of Sciences. JBT received support from the French Agence Nationale de la Recherche (Grant ANR-10-BLAN-0603 M&Ms — Mantle Melting — Measurements, Models, Mechanisms).This is the version of record, which can also be found on the publisher's website at: http://onlinelibrary.wiley.com/doi/10.1002/2014GC005313/abstract © 2014. American Geophysical Union. All Rights Reserved
Correlation of Cycles in Lava Lake Motion and Degassing at Erebus Volcano, Antarctica

Several studies at Erebus volcano have recorded pulsatory behaviour in many of the observable properties of its active lava lake. A strong correlation between the variations in surface speed of the lake and the composition of gas emitted has previously been noted. While previous studies
have shown that the SO2 flux and the surface elevation exhibit pulsatory behaviour with a similar period to that of the surface speed and gas composition, suggesting they are linked, a lack of overlap between the di erent measurements has prevented direct comparisons from being made. Using high time-resolution measurements of surface elevation, surface speed, gas composition and SO2 flux we demonstrate for the  rst time an unambiguous link between the cyclic behaviour in each of these properties. We also show that the variation in gas composition may be explained by a subtle change in oxygen fugacity. The cycles are found to be in-phase with each other, with a small but consistent lag of 1-3 min between the peaks in surface elevation and surface speed. Explosive events are found to have no observable e ffect on the pulsatory behaviour beyond the ~5 min period required for lake refi ll. The close correspondences between the varying lake  surface motion, gas flux and composition, and modelled oxygen fugacity suggest strong links between magma degassing, redox change and the fluid dynamics of the shallow magmatic system.This is the final version of the article. It was originally published by Wiley on behalf of the American Geophysical Union in Geochemistry, Geophysics, Geosystems here: http://onlinelibrary.wiley.com/doi/10.1002/2014GC005399/abstract. It will be embargoed until 19/1/15
Reactive halogens (BrO and OClO) detected in the plume of Soufrière Hills Volcano during an eruption hiatus

Volcanic plumes are sites of dynamic chemistry involving halogen gases. Here we present new data on the relative abundances of SO2, BrO and OClO gases emitted from Soufrière Hills Volcano [SHV). They were collected during an eruptive hiatus but during sustained degassing at this halogen-rich volcano. By comparison with data from a previous study during an eruptive phase and application of the data and modeling of Villemant et al. (2008), we suggest that, after consideration of errors, either the rate of HBr conversion to BrO is variable, ranging from ∼30% to ∼15%, and/or the relative partitioning of Cl and Br into the gas phase from the melt changes according to eruptive activity. We examine the potential implications of this for fluid-melt partitioning, and compare our results with data from the experimental literature. Our work contributes toward understanding the controls on the BrO/SO2 ratio for volcano monitoring purposes; the changes in plume chemistry with regard to bromine at the onset of lava extrusion may be large and rapid. OClO was detected in the plume at SHV for the first time. This species has only previously been detected in emissions from Mount Etna (using ground-based methods) and from Puyehue Cordon Caulle (using satellite-based methods). No HCHO or NOy species were detected in the spectra.The MVO is thanked for support during fieldwork. This work was also supported by the UK National Centre for Earth Observation (“Dynamic Earth and Geohazards"; http://comet.nerc.ac.uk).This is the final published version. It's also available from Wiley at http://onlinelibrary.wiley.com/doi/10.1002/2014GC005419/abstract
Changing tectonic controls on the long-term carbon cycle from Mesozoic to present

Copyright © 2014. The Authors.Tectonic drivers of degassing and weathering processes are key long-term controls on atmos-
pheric CO2. However, there is considerable debate over the changing relative importance of different car-
bon sources and sinks. Existing geochemical models have tended to rely on indirect methods to derive
tectonic drivers, such as inversion of the seawater 87Sr/86Sr curve to estimate uplift or continental basalt
area. Here we use improving geologic data to update the representation of tectonic drivers in the COPSE
biogeochemical model. The resulting model distinguishes CO2 sinks from terrestrial granite weathering,
total basalt weathering, and seafloor alteration. It also distinguishes CO2 sources from subduction zone met-
amorphism and from igneous intrusions. We reconstruct terrestrial basaltic area from data on the extent of
large igneous provinces and use their volume to estimate their contribution to degassing. We adopt a
recently published reconstruction of subduction-related degassing, and relate seafloor weathering to ocean
crust creation rate. Revised degassing alone tends to produce unrealistically high CO2, but this is counter-
acted by the inclusion of seafloor alteration and global basalt weathering, producing a good overall fit to
Mesozoic-Cenozoic proxy CO2 estimates and a good fit to 87Sr/86Sr data. The model predicts that seafloor
alteration and terrestrial weathering made similar contributions to CO2 removal through the Triassic and
Jurassic, after which terrestrial weathering increased and seafloor weathering declined. We predict that
basalts made a greater contribution to silicate weathering than granites through the Mesozoic, before the
contribution of basalt weathering declined over the Cenozoic due to decreasing global basaltic area.UK Natural Environment Research Council (NE/G018332/2). 
Leverhulme Trust (RPG-2013-106).Royal Society Wolfson Research Merit Awar
FORCulator: a micromagnetic tool for simulating first-order reversal curve diagrams

We describe a method for simulating first-order reversal curve (FORC) diagrams of interacting single-domain particles. Magnetostatic interactions are calculated in real space, allowing simulations to be performed for particle ensembles with arbitrary geometry. For weakly interacting uniaxial particles, the equilibrium magnetization at each field step is obtained by direct solution of the Stoner-Wohlfarth model, assuming a quasi-static distribution of interaction fields. For all other cases, the equilibrium magnetization is calculated using an approximate iterated solution to the Landau-Lifshitz-Gilbert equation. Multithreading is employed to allow multiple curves to be computed simultaneously, enabling FORC diagrams to be simulated in reasonable time using a standard desktop computer. Statistical averaging and post processing lead to simulated FORC diagrams that are comparable to their experimental counterparts. The method is applied to several geometries of relevance to rock and environmental magnetism, including densely packed random clusters and partially collapsed chains. The method forms the basis of FORCulator, a freely available software tool with graphical user interface that will enable FORC simulations to become a routine part of rock magnetic studies.The
research leading to these results has
received funding from the European
Research Council under the European
Union’s Seventh Framework
Programme (FP/2007–2013)/ERC grant
agreement 320750.This is the final published version of the article. It first appeared at http://onlinelibrary.wiley.com/doi/10.1002/2014GC005582/abstract
Significant groundwater contribution to Antarctic ice streams hydrologic budget

Satellite observations have revealed active hydrologic systems beneath Antarctic ice streams, but sources and sinks of water within these systems are uncertain. Here we use numerical simulations of ice streams to estimate the generation, flux, and budget of water beneath five ice streams on the Siple Coast. We estimate that 47% of the total hydrologic input (0.98 km3 yr−1) to Whillans (WIS), Mercer (MIS), and Kamb (KIS) ice streams comes from the ice sheet interior and that only 8% forms by local basal melting. The remaining 45% comes from a groundwater reservoir, an overlooked source in which depletion significantly exceeds recharge. Of the total input to Bindschadler (BIS) and MacAyeal (MacIS) ice streams (0.56 km3 yr−1), 72% comes from the interior, 19% from groundwater, and 9% from local melting. This contrasting hydrologic setting modulates the ice streams flow and has important implications for the search for life in subglacial lakes.This work was carried out with support from the Isaac Newton Trust, Cecil H. and Ida M. Green Foundation and Natural Environment Research Council (grant NE/E005950/1 and NE/J005800/1).This is the final version of the article. It was originally published in Geophysical Research Letters and is also available from the Wiley website at http://onlinelibrary.wiley.com/doi/10.1002/2014GL059250/abstract. © American Geophysical Union 201
Separation of aerosol fine- and coarse-mode radiative properties: Effect on the mineral dust longwave, direct radiative forcing

An improvement of the estimation of mineral dust longwave, direct radiative forcing is presented. It is based on recent developments that combine Sun photometer and multiwavelength lidar data to retrieve range-resolved coarse- and fine-mode extinction coefficients. The forcings are calculated separately for each mode, and their sum is compared to the classical approach in which only the total extinction is considered. The results of four cases of mineral dust intrusion in Barcelona, Spain, show that when the coarse mode predominates, the longwave forcings calculated with the classical approach are underestimated up to 20% near the surface. In all cases the strong coarse-mode predominance near the surface has also an effect on the forcing in the upper layers.Peer ReviewedPostprint (published version
Sedimentation Rates Test Models of Oceanic Detachment Faulting

This is the accepted manuscript version.The final version is available from Wiley at http://onlinelibrary.wiley.com/doi/10.1002/2014GL061555/full.Long-lived detachment faults play an important role in the construction of new oceanic
crust at slow-spreading mid-oceanic ridges. Although the corrugated surfaces of exposed
low-angle faults demonstrate past slip, it is difficult to determine whether a given fault is
currently active. If inactive, it is unclear when slip ceased. This judgment is crucial for
tectonic reconstructions where detachment faults are present, and for models of plate
spreading. We quantify variation in sediment thickness over two corrugated surfaces
near 16.5°N at the Mid-Atlantic Ridge using near-bottom CHIRP data. We show that the
distribution of sediment and tectonic features at one detachment fault is consistent with
slip occurring today. In contrast, another corrugated surface 20 km to the south shows a
sediment distribution suggesting that slip ceased ~150,000 years ago. Data presented here
provide new evidence for active detachment faulting, and suggest along-axis variations in
fault activity occur over tens of kilometers.This work was supported by the National Science Foundation grant number OCE-1155650
Onshore sandbar migration in the surf zone: new insights into the wave-induced sediment transport mechanisms

We present a novel process-based morphodynamic model, which includes transport processes due to both velocity and acceleration skewness and a new formulation for intrawave motions, that successfully simulates observations of onshore sandbar migration. Results confirm findings of previous studies, in which each process was considered separately and in which sediment transport was computed from the observed water motion. However, our results indicate that accounting for the joint action of both velocity and acceleration skewnesses causes major improvement of the modeled onshore bar migration and is essential to accurately model the evolution of the entire cross-shore bottom profile, when compared with observations. We also demonstrate that the morphodynamics in the shoaling zone are dominated by velocity skewness (bed shear stresses), while sediment transport induced by acceleration skewness (pressure gradients) controls the morphodynamics in the inner surf zone.Postprint (author’s final draft
In situ properties of small and large flux ropes in the solar wind

Two populations of twisted magnetic field tubes, or flux ropes (hereafter, FRs), are detected by in situ measurements in the solar wind. While small FRs are crossed by the observing spacecraft within few hours, with a radius typically less than 0.1 AU, larger FRs, or magnetic clouds (hereafter, MCs), have durations of about half a day. The main aim of this study is to compare the properties of both populations of FRs observed by the Wind spacecraft at 1 AU. To do so, we use standard correlation techniques for the FR parameters, as well as histograms and more refined statistical methods. Although several properties seem at first different for small FRs and MCs, we show that they are actually governed by the same propagation physics. For example, we observe no in situ signatures of expansion for small FRs, contrary to MCs. We demonstrate that this result is in fact expected: small FRs expand similar to MCs, as a consequence of a total pressure balance with the surrounding medium, but the expansion signature is well hidden by velocity fluctuations. Next, we find that the FR radius, velocity, and magnetic field strength are all positively correlated, with correlation factors than can reach a value >0.5. This result indicates a remnant trace of the FR ejection process from the corona. We also find a larger FR radius at the apex than at the legs (up to 3 times larger at the apex), for FR observed at 1 AU. Finally, assuming that the detected FRs have a large-scale configuration in the heliosphere, we derived the mean axis shape from the probability distribution of the axis orientation. We therefore interpret the small FR and MC properties in a common framework of FRs interacting with the solar wind, and we disentangle the physics present behind their common and different features.<br />Fil: Janvier, M.. University of Dundee; Reino UnidoFil: Démoulin, Pascal. Centre National de la Recherche Scientifique. Observatoire de Paris; FranciaFil: Dasso, Sergio Ricardo. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomia y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomia y Física del Espacio; Argentin
Upstream proton cyclotron waves at Venus near solar maximum

Long-term magnetometer data of Venus Express are analyzed for the occurrence of waves at the proton cyclotron frequency in the spacecraft frame in the upstream region of Venus, for conditions of rising solar activity. The data of two Venus years up to the time of highest sunspot number so far (1 Mar 2011 to 31 May 2012) are studied to reveal the properties of the waves and the interplanetary magnetic field (IMF) conditions under which they are observed. In general, waves generated by newborn protons from exospheric hydrogen are observed under quasi- anti)parallel conditions of the IMF and the solar wind velocity, as is expected from theoretical models. The present study near solar maximum finds significantly more waves than a previous study for solar minimum, with an asymmetry in the wave occurrence, i.e., mainly under antiparallel conditions. The plasma data from the Analyzer of Space Plasmas and Energetic Atoms instrument aboard Venus Express enable analysis of the background solar wind conditions. The prevalence of waves for IMF in direction toward the Sun is related to the stronger southward tilt of the heliospheric current sheet for the rising phase of Solar Cycle 24, i.e., the ?bashful ballerina? is  responsible for asymmetric background solar wind conditions. The increase of the number of wave occurrences may be explained by a significant increase in the relative density of planetary protons with respect to the solar wind background. An exceptionally low solar wind proton density is observed during the rising phase of Solar Cycle 24. At the same time, higher EUV increases the ionization in the Venus exosphere, resulting in higher supply of energy from a higher number of newborn protons to the wave. We conclude that in addition to quasi- (anti)parallel conditions of the IMF and the solar wind velocity direction, the higher relative density of Venus exospheric protons with respect to the background solar wind proton density is the key parameter for the higher number of observable proton cyclotron waves near solar maximum.Fil: Delva, M.. Space Research Institute; AustriaFil: Bertucci, Cesar. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; ArgentinaFil: Volwerk, M.. Space Research Institute; AustriaFil: Lundin, R.. Swedish Institute For Space Physics; SueciaFil: Mazelle, C.. Irap UPS-CNRS; FranciaFil: Romanelli, Norberto Julio. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; Argentin