7,237 research outputs found

    Petrology and depositional environment of the Foord seam, Pictou Coalfield, Nova Scotia

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    The Pictou Coalfield is one of several coal deposits in the northern Appalachians. This coalfield is of particular interest because: (1) it is restricted to a synsedimentary, pull-apart graben. (2) the coals are in a late Westphalian lacustrine - deltaic sequence with minor fluvial deposits, (3) it also contains numerous organic-rich shales, and (4) in spite of its small size and long history of mining it remains among the most important coal reserves in the region. The Foord seam is the most importantof several seams that have been mined. In contrast with typical (fluvial basin) Appalachian coals, the Pictou coals are characterized by microbanding, comparatively high rank, low sulphur, and relatively high ash content. Macroscopic appearance and relative proportions of maceral groups (vitrinite > inertinite > liptinite) indicate broad petrographic uniformity within the Foord seam, but the proportions of individual macerals vary widely, reflecting environmental and diagenetic changes. Specific maceral ratios confirm evidence from lithotype studies for cylic development of wet forest swamp, fen, and limnic conditions in response to alternate flooding and drying trends during peat accumulation. Although secular coal facies variations within the Foord seam can be correlated laterally, differences in maceral distribution indicate that depositional and diagenetic conditions must have been locally variable. RÉSUMÉ Le bassin houiller de Pictou est Tun des gisements de charbon du nord des Appalaches. Il présente un intérés particulier car: (1) il est confiné à un graben rhomboélrique synséotimentaire, (2) les charbons font paitie d'une série lacustro-deltaique tardi-westphalierme incorporant de faiblcs dépôts fluviatiles, (3) on y rencontre plusieurs shales riches en matiere organique, et (4) en dépit de sa faible dimension et d'une exploitation prolongée, ce bassin demeure Tune des plus importantes réserves de charbon de la région. Le faisceau charbonneux de Foord est le plus important à avoir été exploité Contrairement aux charbons appalachiens typiques des bassins fluviatiles, les charbons de Pictou sont caractérisés par une microlamination, une classe assez haute, une teneur faible en soufre et relativement élevée en cendres. L'allure macroscopique et la proportion relative des différents groupes de maceraux (vitrinite > inertinite > liptinite) indiquent une uniformity pétrographique générale au sein du faisceau de Foord. Cependant la proportion de chaque macéral varie fortement, ce qui reflète des changements dans le milieu et la diagénèse. Les rapports specifiques des macéraux confirment les arguments qu'apportent les études des lithotypes en faveur d'un développement cyclique de conditions de marécages de foret humide, de fens et de conditions limniques en réponse à des tendances alternant entre les inondations et les assèchements durant l’accumulation de la tourbe. Quoiqu'on puisse corréler latéralement les variations seculaires des faciès charbormeux au sein du faisceau de Foord, la distribution différente des macéraux démontre que les conditions diagénéiques et de dépôt devaient varier localement [Traduit par le journal

    The Complexity of Vector Spin Glasses

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    We study the annealed complexity of the m-vector spin glasses in the Sherrington-Kirkpatrick limit. The eigenvalue spectrum of the Hessian matrix of the Thouless-Anderson-Palmer (TAP) free energy is found to consist of a continuous band of positive eigenvalues in addition to an isolated eigenvalue and (m-1) null eigenvalues due to rotational invariance. Rather surprisingly, the band does not extend to zero at any finite temperature. The isolated eigenvalue becomes zero in the thermodynamic limit, as in the Ising case (m=1), indicating that the same supersymmetry breaking recently found in Ising spin glasses occurs in vector spin glasses.Comment: 4 pages, 2 figure

    Solar Irradiance Variability is Caused by the Magnetic Activity on the Solar Surface

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    The variation in the radiative output of the Sun, described in terms of solar irradiance, is important to climatology. A common assumption is that solar irradiance variability is driven by its surface magnetism. Verifying this assumption has, however, been hampered by the fact that models of solar irradiance variability based on solar surface magnetism have to be calibrated to observed variability. Making use of realistic three-dimensional magnetohydrodynamic simulations of the solar atmosphere and state-of-the-art solar magnetograms from the Solar Dynamics Observatory, we present a model of total solar irradiance (TSI) that does not require any such calibration. In doing so, the modeled irradiance variability is entirely independent of the observational record. (The absolute level is calibrated to the TSI record from the Total Irradiance Monitor.) The model replicates 95% of the observed variability between April 2010 and July 2016, leaving little scope for alternative drivers of solar irradiance variability at least over the time scales examined (days to years).Comment: Supplementary Materials; https://journals.aps.org/prl/supplemental/10.1103/PhysRevLett.119.091102/supplementary_material_170801.pd

    First-Order Transition and Critical End-Point in Vortex Liquids in Layered Superconductors

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    We calculate various thermodynamic quantities of vortex liquids in a layered superconductor by using the nonperturbative parquet approximation method, which was previously used to study the effect of thermal fluctuations in two-dimensional vortex systems. We find there is a first-order transition between two vortex liquid phases which differ in the magnitude of their correlation lengths. As the coupling between the layers increases,the first-order transition line ends at a critical point. We discuss the possible relation between this critical end-point and the disappearance of the first-order transition which is observed in experiments on high temperature superconductors at low magnetic fields.Comment: 9 pages, 5 figure

    A Sub-Type of Familial Pancreatic Cancer: Evidence and Implications of Loss-of-Function Polymorphisms in Indoleamine-2,3-Dioxygenase-2.

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    BACKGROUND: Variation in an individual\u27s genetic status can impact the development of pancreatic ductal adenocarcinoma; however, the majority of familial pancreatic cancers (FPC) cannot yet be attributed to a specific inherited mutation. We present data suggesting a correlation between loss-of-function single nucleotide polymorphisms (SNPs) in an immune regulator gene, indoleamine-2,3-dioxygenase-2 (IDO2), and an increased risk of FPC. STUDY DESIGN: Germline DNA from patients who underwent resection for pancreatic ductal adenocarcinoma (n = 79) was sequenced for the IDO2 SNPs R248W and Y359Stop. Genotypes resulting in inactivation of IDO2 (Y325X homozygous, R248W homozygous) were labeled as homozygous, and the other genotypes were grouped as wild-type or heterozygous. Genotype distributions of each SNP were analyzed for Hardy-Weinberg deviation. A genotype frequency set from the 1000 Genomes Project (n = 99) was used as a genetic control for genotype distribution comparisons. RESULTS: A significant 2-fold increase in the overall prevalence of the Y359Stop homozygous genotype compared with the expected Hardy-Weinberg equilibrium was noted (p \u3c 0.05). Familial pancreatic cancer was noted in 15 cases (19%) and comparison of the FPC cohort set to the genetic control set showed a 3-fold increase in Y359Stop homozygous rates (p = 0.054). Overall in our cohort, the homozygous genotype group was associated with increased risk of FPC (odds ratio 5.4; 95% CI 1.6 to 17.6; p \u3c 0.01). Sex, age at diagnosis, and history of tobacco use were not found to be significantly associated with FPC. CONCLUSIONS: Our preliminary data suggest a strong association between the IDO2 inactivating Y359Stop SNP and an increased risk of FPC when compared with the control group. Future studies will evaluate the value of IDO2 genotyping as a prognostic, early detection marker for pancreatic ductal adenocarcinoma and a predictive marker for novel immune checkpoint therapies

    Reconstruction of spectral solar irradiance since 1700 from simulated magnetograms

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    We present a reconstruction of the spectral solar irradiance since 1700 using the SATIRE-T2 (Spectral And Total Irradiance REconstructions for the Telescope era version 2) model. This model uses as input magnetograms simulated with a surface flux transport model fed with semi-synthetic records of emerging sunspot groups. We used statistical relationships between the properties of sunspot group emergence, such as the latitude, area, and tilt angle, and the sunspot cycle strength and phase to produce semi-synthetic sunspot group records starting in the year 1700. The semisynthetic records are fed into a surface flux transport model to obtain daily simulated magnetograms that map the distribution of the magnetic flux in active regions (sunspots and faculae) and their decay products on the solar surface. The magnetic flux emerging in ephemeral regions is accounted for separately based on the concept of extended cycles whose length and amplitude are linked to those of the sunspot cycles through the sunspot number. The magnetic flux in each surface component (sunspots, faculae and network, and ephemeral regions) was used to compute the spectral and total solar irradiance between the years 1700 and 2009. This reconstruction is aimed at timescales of months or longer although the model returns daily values. We found that SATIRE-T2, besides reproducing other relevant observations such as the total magnetic flux, reconstructs the total solar irradiance (TSI) on timescales of months or longer in good agreement with the PMOD composite of observations, as well as with the reconstruction starting in 1878 based on the RGO-SOON data. The model predicts an increase in the TSI of 1.2[+0.2, -0.3] Wm-2 between 1700 and the present. The spectral irradiance reconstruction is in good agreement with the UARS/SUSIM measurements as well as the Lyman-alpha composite.Comment: 13 pages, 10 figure

    Millisecond spin-flip times of donor-bound electrons in GaAs

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    We observe millisecond spin-flip relaxation times of donor-bound electrons in high-purity n-GaAs . This is three orders of magnitude larger than previously reported lifetimes in n-GaAs . Spin-flip times are measured as a function of magnetic field and exhibit a strong power-law dependence for fields greater than 4 T . This result is in qualitative agreement with previously reported theory and measurements of electrons in quantum dots.Comment: 4 pages, 4 figure

    T-junction ion trap array for two-dimensional ion shuttling, storage and manipulation

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    We demonstrate a two-dimensional 11-zone ion trap array, where individual laser-cooled atomic ions are stored, separated, shuttled, and swapped. The trap geometry consists of two linear rf ion trap sections that are joined at a 90 degree angle to form a T-shaped structure. We shuttle a single ion around the corners of the T-junction and swap the positions of two crystallized ions using voltage sequences designed to accommodate the nontrivial electrical potential near the junction. Full two-dimensional control of multiple ions demonstrated in this system may be crucial for the realization of scalable ion trap quantum computation and the implementation of quantum networks.Comment: 3 pages, 5 figure

    Bostonia: The Boston University Alumni Magazine. Volume 29

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    Founded in 1900, Bostonia magazine is Boston University's main alumni publication, which covers alumni and student life, as well as university activities, events, and programs
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