624 research outputs found

    Exploratory studies of contact angle hysteresis, wetting of solidified rare gases and surface properties of mercury Final report

    Get PDF
    Contact angle hysteresis, wetting of solidified rare gases, and surface properties of mercur

    PNNL - Using Matrix and Tensor Factorization for Analyzing Radiation Transport Data

    Get PDF
    The Disruptive Technologies Group in the National Security Directorate of Pacific Northwest National Laboratory teamed up with students at Embry-Riddle Aeronautical University on a research project that aims to develop quantitative methods for characterizing features in radiation transport simulation data and comparing features across different computational approaches. Understanding how radiation particles are transported throughout a system and interact with shielding is extremely computationally expensive. Reduced order models (ROMs) can be used to significantly increase the speed of these calculations. This project focuses on analysis of the simulated radiation transport for Cobalt-60, Cesium-137, and Technetium-99. A ROM may be developed from several formalisms and then analyzing the feature vectors of each. The methods considered here include principal component analysis (PCA), non-negative matrix factorization (NNMF), and CP tensor decomposition (CPT). By comparing the signal from fitted Lorentzian profiles to spectral features, we evaluate whether each ROM is capable of accurately displaying the radiation signal traces in the data

    Police bail without charge: The human rights implications

    Get PDF
    Whilst the power of the police to release a person on bail prior to trial has existed for centuries, the power to release on bail a person suspected of but not charged with a criminal offence has been available to the police only since 1925. The power to attach conditions to pre-charge bail is of very recent origin, having been introduced for the first time in 2003 but rapidly expanded since then. Whilst imposing restrictions on the liberty of a person should, constitutionally, be reserved to the judiciary, the fact that it was originally conceived, in part at least, as a mechanism for enhancing liberty reduced the constitutional tension created by allowing members of the executive such powers. However, the changing role of arrest in the investigation of crime and the granting of extensive powers to the police to impose bail conditions means that the police now have the ability to place controls on people not charged with a criminal offence for extended periods of time. It is argued here that this is in breach of the right to liberty under Article 5 of the European Convention on Human Rights and, in practice, may also breach other Convention rights

    INCREASING ENGAGEMENT IN ONLINE LEARNING

    Get PDF
    Motivated by the need to improve students’ engagement and learning outcomes, in 2018/2019 we implemented two engagement interventions to 1650 students in twelve online courses across Science, Education, Engineering and Accounting at a regional university. Both “click” data and video analytics were used to measure engagement. The first initiative applied findings from behavioural research to ‘nudge’ students toward early engagement with key learning resources and to create ‘teaching presence’ (Garrison, 2007). The second initiative was to help move ‘knowledge’ to ‘know-how’ by nudging videos to offer a sense of real-life expertise, application, motivation and advanced connection. We aimed to improve student learning outcomes and their online engagement by providing explicit guidance about which course resources were critical for students’ success. We were interested in interrogating the data in both learning management systems (Moodle®) and Video analytics (Vimeo®) to answer questions about learner engagement and to explore evidence of impact. The nudges successfully engaged students in the key online resources showing an 18% average increase in access and confirmed via student feedback. The project developed a Nudge Guidelines document that has been presented institutionally and nationally to enable academics to utilise the strategies in their courses

    Probing cosmic dawn with emission lines: predicting infrared and nebular line emission for ALMA and JWST

    Get PDF
    Infrared and nebular lines provide some of our best probes of the physics regulating the properties of the interstellar medium (ISM) at high-redshift. However, interpreting the physical conditions of high-redshift galaxies directly from emission lines remains complicated due to inhomogeneities in temperature, density, metallicity, ionisation parameter, and spectral hardness. We present a new suite of cosmological, radiation-hydrodynamics simulations, each centred on a massive Lyman-break galaxy that resolves such properties in an inhomogeneous ISM. Many of the simulated systems exhibit transient but well defined gaseous disks that appear as velocity gradients in [CII]~158.6μ\mum emission. Spatial and spectral offsets between [CII]~158.6μ\mum and [OIII]~88.33μ\mum are common, but not ubiquitous, as each line probes a different phase of the ISM. These systems fall on the local [CII]-SFR relation, consistent with newer observations that question previously observed [CII]~158.6μ\mum deficits. Our galaxies are consistent with the nebular line properties of observed z23z\sim2-3 galaxies and reproduce offsets on the BPT and mass-excitation diagrams compared to local galaxies due to higher star formation rate (SFR), excitation, and specific-SFR, as well as harder spectra from young, metal-poor binaries. We predict that local calibrations between Hα\alpha and [OII]~3727A˚\AA luminosity and galaxy SFR apply up to z>10z>10, as do the local relations between certain strong line diagnostics (R23 and [OIII]~5007A˚\AA/Hβ\beta) and galaxy metallicity. Our new simulations are well suited to interpret the observations of line emission from current (ALMA and HST) and upcoming facilities (JWST and ngVLA)

    In vitro culture with gemcitabine augments death receptor and NKG2D ligand expression on tumour cells

    Get PDF
    Much effort has been made to try to understand the relationship between chemotherapeutic treatment of cancer and the immune system. Whereas much of that focus has been on the direct effect of chemotherapy drugs on immune cells and the release of antigens and danger signals by malignant cells killed by chemotherapy, the effect of chemotherapy on cells surviving treatment has often been overlooked. In the present study, tumour cell lines: A549 (lung), HCT116 (colon) and MCF-7 (breast), were treated with various concentrations of the chemotherapeutic drugs cyclophosphamide, gemcitabine (GEM) and oxaliplatin (OXP) for 24 hours in vitro. In line with other reports, GEM and OXP upregulated expression of the death receptor CD95 (fas) on live cells even at sub-cytotoxic concentrations. Further investigation revealed that the increase in CD95 in response to GEM sensitised the cells to fas ligand treatment, was associated with increased phosphorylation of stress activated protein kinase/c-Jun N-terminal kinase and that other death receptors and activatory immune receptors were co-ordinately upregulated with CD95 in certain cell lines. The upregulation of death receptors and NKG2D ligands together on cells after chemotherapy suggest that although the cells have survived preliminary treatment with chemotherapy they may now be more susceptible to immune cell-mediated challenge. This re-enforces the idea that chemotherapy-immunotherapy combinations may be useful clinically and has implications for the make-up and scheduling of such treatments

    Detection of an intergalactic meteor particle with the 6-m telescope

    Full text link
    On July 28, 2006 the 6-m telescope of the Special Astrophysical Observatory of the Russian Academy of Sciences recorded the spectrum of a faint meteor. We confidently identify the lines of FeI and MgI, OI, NI and molecular-nitrogen N_2 bands. The entry velocity of the meteor body into the Earth's atmosphere estimated from radial velocity is equal to 300 km/s. The body was several tens of a millimeter in size, like chondrules in carbon chondrites. The radiant of the meteor trajectory coincides with the sky position of the apex of the motion of the Solar system toward the centroid of the Local Group of galaxies. Observations of faint sporadic meteors with FAVOR TV CCD camera confirmed the radiant at a higher than 96% confidence level. We conclude that this meteor particle is likely to be of extragalactic origin. The following important questions remain open: (1) How metal-rich dust particles came to be in the extragalactic space? (2) Why are the sizes of extragalactic particles larger by two orders of magnitude (and their masses greater by six orders of magnitude) than common interstellar dust grains in our Galaxy? (3) If extragalactic dust surrounds galaxies in the form of dust (or gas-and-dust) aureoles, can such formations now be observed using other observational techniques (IR observations aboard Spitzer satellite, etc.)? (4) If inhomogeneous extragalactic dust medium with the parameters mentioned above actually exists, does it show up in the form of irregularities on the cosmic microwave background (WMAP etc.)?Comment: 9 pages, 6 EPS figure

    Studies on the Removal of Fluorine from Drinking Waters in the State of Iowa

    Get PDF
    Our knowledge concerning the distribution of fluorine in drinking waters and the effect of such waters on the structure of the teeth has been appreciably expanded by the recent researches of Smith, Lantz, and Smith (1), Churchill (2), McKay (3), Kehr (4), Ostrem, Nelson, Greenwood, and Wilhelm (5), Boissevain (6), Dean (7), Sebrell, Dean, Elvove, and Breaux (8) and Boruff and Abbott (9). Smith, Lantz, and Smith (1), of the University of Arizona, were the first to show that mottled enamel is clue to fluorides in the drinking water; in fact, their analyses of waters from endemic areas show that the fluorine concentration in such waters is high

    Aspirin Inhibits TGFβ2-Induced Epithelial to Mesenchymal Transition of Lens Epithelial Cells:Selective acetylation of K56 and K122 in histone H3

    Get PDF
    Posterior capsule opacification (PCO) is a complication after cataract surgery that can disrupt vision. The epithelial to mesenchymal transition (EMT) of lens epithelial cells (LECs) in response to transforming growth factor β2 (TGFβ2) has been considered an obligatory mechanism for PCO. In this study, we tested the efficacy of aspirin in inhibiting the TGFβ2-mediated EMT of human LECs, LECs in human lens capsular bags, and lensectomized mice. In human LECs, the levels of the EMT markers α-smooth muscle actin (α-SMA) and fibronectin were drastically reduced by treatment with 2 mM aspirin. Aspirin also halted the EMT response of TGFβ2 when introduced after EMT initiation. In human capsular bags, treatment with 2 mM aspirin significantly suppressed posterior capsule wrinkling and the expression α-SMA in capsule-adherent LECs. The inhibition of TGFβ2-mediated EMT in human LECs was not dependent on Smad phosphorylation or MAPK and AKT-mediated signaling. We found that aspirin significantly increased the acetylation of K56 and K122 in histone H3 of human LECs. Chromatin immunoprecipitation assays using acetyl-H3K56 or acetyl-H3K122 antibody revealed that aspirin blocked the TGFβ2-induced acetylation of H3K56 and H3K122 at the promoter regions of ACTA2 and COL1A1. After lensectomy in mice, we observed an increase in the proliferation and α-SMA expression of the capsule-adherent LECs, which was ameliorated by aspirin administration through drinking water. Taken together, our results showed that aspirin inhibits TGFβ2-mediated EMT of LECs, possibly from epigenetic down-regulation of EMT-related genes
    corecore