Science.gov

Sample records for formations recent results

  1. The formation, destruction and chemical influence of water ice: a review of recent laboratory results

    NASA Astrophysics Data System (ADS)

    Oberg, Karin I.

    2015-08-01

    Water ice is ubiquitous in dense molecular clouds, the stellar nurseries of the Galaxy. Recent theoretical investigations (Cleeves et al. 2014) suggest that much of this pre-stellar ice survives disk formation and thus takes part in forming of planets and planetesimals. Interstellar and circumstellar ice abundances thus affect the compositions of planets. The presence of water ice is also important for the formation of other molecules on grains. Water is the most abundant ice constituent and therefore sets the ice diffusion environment, which regulates for example the organic photochemistry proposed to drive the complex chemical evolution during star formation.The processes that regulate the formation, destruction and chemical influence of water have all been explored in laboratory experiments. One of the most significant advances in recent years is the arrival of laboratory experiments on hydrogen additions to condensed O, O2 and O3 — the proposed main formation pathways of water ice. These experiments have revealed how the interplay between diffusion and reaction barriers together regulate the water formation chemistry as well as the chemistry of closely related carbon-bearing species such as CO2. A very different set of laboratory experiments have in the same time period constrained the efficiency of non-thermal water desorption, especially UV-induced ice photodesorption. Laboratory work on other non-thermal desorption pathways, e.g. chemical desorption, has also advanced, though more experiments are needed to quantify the importance of these desorption pathways relative to photodesorption. There are also an increasing number of experiments aimed at constraining the diffusion environment of water-dominated ices and its effects on the formation of organics when ice mixtures are exposed to UV photons or other kinds of energetic radiation.I will review the many significant laboratory water ice experiments that has been relaized in the past few years and how they

  2. Recent flight test results using an electronic display format on the NASA B-737

    NASA Technical Reports Server (NTRS)

    Morello, S. A.

    1977-01-01

    This paper presents results of a flight evaluation of two electronic display formats for the approach-to-landing under instrument conditions. The evaluation was conducted for a baseline electronic display format and for the same format with runway symbology and track information added; its evaluation was conducted during 3-deg manual straight-in approaches with and without initial localizer offsets. Flight-path tracking performance data and pilot subjective comments were examined with regard to pilot's ability to capture and maintain the localizer and glide slope using both display fomats. The results of the flight tests agree with earlier simulation results and show that the addition of a perspective runway symbol with an extended centerline and relative track information to a baseline electronic display format improved both lateral and vertical flight-path tracking. Pilot comments indicated that the mental workload required to assess the approach situation was reduced as a result of integrating the perspective runway with extended centerline along with relative track information into the vertical situation display. The limited flight-test results also show that the flight-path performance with the integrated situation display format meets Category II Flight-Director performance criteria.

  3. Stability of synchronized dynamics and pattern formation in coupled systems: Review of some recent results

    NASA Astrophysics Data System (ADS)

    Chen, Yonghong; Rangarajan, Govindan; Ding, Mingzhou

    2006-12-01

    In arbitrarily coupled dynamical systems (maps or ordinary differential equations), the stability of synchronized states (including equilibrium point, periodic orbit or chaotic attractor) and the formation of patterns from loss of stability of the synchronized states are two problems of current research interest. These two problems are often treated separately in the literature. Here, we present a unified framework in which we show that the eigenvalues of the coupling matrix determine the stability of the synchronized state, while the eigenvectors correspond to patterns emerging from desynchronization. Based on this simple framework three results are derived: First, general approaches are developed that yield constraints directly on the coupling strengths which ensure the stability of synchronized dynamics. Second, when the synchronized state becomes unstable spatial patterns can be selectively realized by varying the coupling strengths. Distinct temporal evolution of the spatial pattern can be obtained depending on the bifurcating synchronized state. Third, given a desired spatiotemporal pattern, one is able to design coupling schemes which give rise to that pattern as the coupled system evolves. Systems with specific coupling schemes are used as examples to illustrate the general methods.

  4. Recent results from CDF

    SciTech Connect

    R. Harr

    2004-01-26

    The authors report on the recent heavy-quark results from CDF in Run IIa. They focus on a selection of mature analyses that demonstrate the capabilities of the experiment to extract interesting physics from the data. A few of the results presented have already been submitted for publication and papers are being prepared for most of the others.

  5. Recent CDF results

    SciTech Connect

    Gomez, Gervasio; /Cantabria Inst. of Phys.

    2007-11-01

    As of November of 2007, the CDF detector has recorded approximately 2.7 fb{sup -1} of data. This contribution describes some of the most recent and most relevant results from the CDF collaboration in all areas of its wide physics program, as well as some insights into the Tevatron reach for Higgs searches within the next few years.

  6. Recent results from MAMI

    SciTech Connect

    Arends, Hans-Juergen

    2011-10-24

    The Mainz Microtron MAMI is an ideal facility to study the hadron structure with the electromagnetic probe. With the new accelerator stage (HDSM), which went into operation in 2007, high-intensity polarized electron and photon beams with energies up to 1.6 GeV are delivered to the experiments. Polarized targets and recoil polarimeters in combination with dedicated detectors are available for precision experiments in hadron physics. In this article, an overview over selected recent results is given.

  7. Recent BABAR Results

    SciTech Connect

    Eigen, Gerald

    2015-04-29

    We present herein the most recent BABAR results on direct CP asymmetry measurements in B → Xsγ, on partial branching fraction and CP asymmetry measurements in B → Xs+-, on a search for B → π/ηℓ+- decays, on a search for lepton number violation in B+ → X-+ℓ'+ modes and a study of B0 →ωω and B0 → ωφ decays.

  8. Recent Results from Phobos

    NASA Astrophysics Data System (ADS)

    García, Edmundo; Back, B. B.; Baker, M. D.; Ballintijn, M.; Barton, D. S.; Betts, R. R.; Bickley, A. A.; Bindel, R.; Busza, W.; Carroll, A.; Chai, Z.; Decowski, M. P.; García, E.; Gburek, T.; George, N.; Gulbrandsen, K.; Halliwell, C.; Hamblen, J.; Hauer, M.; Henderson, C.; Hofman, D. J.; Hollis, R. S.; Hołyński, R.; Holzman, B.; Iordanova, A.; Johnson, E.; Kane, J. L.; Khan, N.; Kulinich, P.; Kuo, C. M.; Lin, W. T.; Manly, S.; Mignerey, A. C.; Nouicer, R.; Olszewski, A.; Pak, R.; Reed, C.; Roland, C.; Roland, G.; Sagerer, J.; Seals, H.; Sedykh, I.; Smith, C. E.; Stankiewicz, M. A.; Steinberg, P.; Stephans, G. S. F.; Sukhanov, A.; Tonjes, M. B.; Trzupek, A.; Vale, C.; van Nieuwenhuizen, G. J.; Vaurynovich, S. S.; Verdier, R.; Veres, G. I.; Wenger, E.; Wolfs, F. L. H.; Wosiek, B.; Woźniak, K.; Wysłouch, B.

    2007-02-01

    The PHOBOS detector is one of four heavy ion experiments at the Relativistic Heavy Ion Collider at Brookhaven National Laboratory. In this paper we will review some of the results of PHOBOS from the data collected in p+p, d+Au and Au+Au collisions at nucleon-nucleon center-of-mass energies up to 200 GeV. Evidence is found of the formation of a very high energy density and highly interactive system, which can not be described in terms of hadrons, and has a relatively low baryon density. There is evidence that the system formed is thermalized to a certain degree. Scaling with the number of participants and extended longitudinal scaling behavior are also observed in distributions of produced charged particles.

  9. Recent results from ANTARES

    NASA Astrophysics Data System (ADS)

    Trovato, Agata

    2015-08-01

    Operating 40 km off the coast of France since 2007, the ANTARES detector is the largest deep-sea neutrino telescope in the Northern Hemisphere with an instrumented volume of more than 0.01 cubic kilometers. It consists of an array of 885 photomultipliers detecting the Cherenkov light induced by charged leptons produced by neutrino interactions in and around the detector. The primary goal of ANTARES is to search for astrophysical neutrinos in the TeV-PeV range. This comprises generic searches for any diffuse cosmic neutrino flux as well as more specific searches for astrophysical galactic and extragalactic sources. The search program also includes multi-messenger analyses based on time and/or space coincidences with other cosmic probes. The ANTARES observatory is sensitive to a wide-range of other phenomena, from atmospheric neutrino oscillations to dark matter annihilation. In this contribution, recent results from the ANTARES neutrino telescope will be presented.

  10. Observational astrochemistry: recent results.

    PubMed

    Irvine, W M

    1989-01-01

    More than 80 molecular species have now been observed by astronomers in the dense interstellar clouds where stars and planets form or in the envelopes expelled by evolved stars. Elemental constituents of these compounds include all of the "biogenic" elements, hydrogen, carbon, nitrogen, oxygen, sulfur, and (most recently) phosphorus. In addition, silicon is found in several molecules, and a series of metal halides have recently been detected in the outflowing envelope of a nearby carbon star. Additions to the list of known interstellar molecules since the last COSPAR meeting are discussed individually. Recent measurements of the hydrogen isotopic fractionation for the cyclic molecule C3H2 are described; values up to 10,000 times the cosmic deuterium-to-hydrogen ratio are found. Knowledge of the chemical reservoirs for the major volatile elements and a comparison between observed molecular abundances and theoretical models are both discussed. PMID:11537359

  11. Recent results from TRISTAN

    SciTech Connect

    Enomoto, Ryoji

    1997-01-01

    TRISTAN results on {gamma}{gamma} physics from 1994 to 1995 are reviewed in this report. We have systematically investigated jet production, the {gamma}-structure function, and charm pair production in {gamma}{gamma} processes. The results are discussed, and future prospects are presented.

  12. Recent results from MAC

    SciTech Connect

    MAC Collaboration

    1982-05-01

    Some preliminary results from the MAC detector at PEP are presented. These include measurements of the angular distribution of ..gamma gamma.., ..mu mu.. and tau tau final states, a determination of the tau lifetime, a measurement of R, and a presentation of the inclusive muon p/sub perpendicular/ distribution for hadronic events.

  13. Recent result from RENO

    NASA Astrophysics Data System (ADS)

    Seo, Hyunkwan; RENO Collaboration

    2016-05-01

    The Reactor Experiment for Neutrino Oscillation (RENO) started data-taking from August, 2011 and has measured the smallest neutrino mixing angle θ13 by observing the disappearance of reactor antineutrinos. Antineutrinos from the six reactors at Hanbit Nuclear Power Plant in Korea are detected and compared by the two identical detectors located in the near and far distances from the reactor array center. We present new results on precisely measured sin 22θ13 value and |Δm2 ee| based on spectral analysis using the 800 days of data sample, which are taken from August, 2011 to Dec., 2013.

  14. Formation of gas-phase peroxides in a rural atmosphere: An interpretation of the recent SOS/SERON field results

    SciTech Connect

    Lee, J.H.; Tang, I.N.; Weinstein-Lloyd, J.B.

    1993-09-01

    Hydrogen perioxide (H{sub 2}O{sub 2}) and certain organic peroxides such as hydroxymethyl-hydroperoxide (HMHP), are gas-phase oxidants present in the atmosphere at ppbv concentration levels. These oxidants play an important role in atmospheric chemistry. In addition, precipitation containing H{sub 2}O{sub 2} is toxic to trees, and it has also been suggested that organic peroxides formed presumably by ozone reactions with biogenic alkenes are responsible for leaf disorders. Recently, we have developed a nonenzymatic method or aqueous-phase H{sub 2}O{sub 2} measurement, using Fenton reagent and fluorescent hydroxy- benzoic acid. The new method, in conjunction with the well-known method of p-hydroxyphenylacetic acid and horseradish peroxidase for total peroxides, and together with an improved gas scrubber to mitigate sampling line problems, has been successfully deployed in recent SOS/SERON field measurements in rural Georgia. For the first time, continuously measured and speciated gas-phase peroxide data have become available, making it possible to examine some aspects of the ozone chemistry leading to the formation of these oxidants. It is observed that daily H{sub 2}O{sub 2} maximum frequently occurs at a different time than does HMHP, and that H{sub 2}O{sub 2} concentration, but not HMHP, tends to correlate with solar fluxes measured at the same location. These findings seem to indicate that the formation mechanisms for H{sub 2}O{sub 2} and organic peroxides are basically different. It is likely that H{sub 2}O{sub 2} is formed from radical-radical recombination, while HMHP is formed by ozone-alkene reactions. Since the gas-phase ozone-alkene reactions are usually too slow to account for the diurnal concentration variations observed for HMHP, heterogeneous processes involving ozone and alkenes are also a possibility.

  15. Recent results from DORIS II

    SciTech Connect

    Bloom, E.D.

    1985-01-01

    This report contains a brief review of recent results from the ARGUS and Crystal Ball experiments at DORIS II, concentrating on UPSILON(1S) and UPSILON(2S) spectroscopy with a short foray into ..gamma gamma.. physics. 18 refs., 10 figs.

  16. Recent Results from the Tevatron

    SciTech Connect

    Demorden, L.

    1998-06-01

    We review recent results from fixed-target and collider experiments at the Fermilab Tevatron. Among the topics discussed are jet production rates, {alpha}{sub S} measurements, the {anti d}/{anti u} ratio in the proton sea, diffraction, heavy quark physics and leptoquark searches.

  17. Recent QCD results from CDF

    SciTech Connect

    Huston, J. |; CDF Collaboration

    1994-01-01

    CDF has recently concluded a very successful 1992--93 data run in which an integrated luminosity of 21.3 pb {sup {minus}1} was written to tape. The large data sample allows for a greater discovery potential for new phenomena and for better statistical and systematic precision in analysis of conventional physics. This paper summarizes some of the new results from QCD analyses for this run.

  18. Recent DIII-D results

    SciTech Connect

    Petersen, P.I.

    1994-07-01

    This paper summarizes the recent DIII-D experimental results and the development of the relevant hardware systems. The DIII-D program focuses on divertor solutions for next generation tokamaks such as International Thermo-nuclear Experimental Reactor (ITER) and Tokamak Physics Experiment (TPX), and on developing configurations with enhanced confinement and stability properties that will lead to a more compact and economical fusion reactor. The DIII-D program carries out this research in an integrated fashion.

  19. Recent CMS results on diffraction

    NASA Astrophysics Data System (ADS)

    Benoît, Roland

    2015-03-01

    Recent CMS results on diffraction are presented. These include the measurements of the soft diffractive cross sections, of the forward rapidity gap cross section, of the diffractive dijet cross section, the measurement of a large rapidity gap in W and Z boson events and the measurement of the pseudorapidity distribution of charged particles in a single diffractive enhanced sample. This last measurement is the first common result of the CMS and TOTEM collaborations. Some prospects of common CMS-TOTEM data taking are also discussed.

  20. Recent Results in Solar Neutrinos

    NASA Astrophysics Data System (ADS)

    Saldanha, Richard

    2011-10-01

    Solar neutrinos are an invaluable tool for studying neutrino oscillations in matter as well as probing the nuclear reactions that fuel the Sun. In this talk I will give an overview of solar neutrinos and discuss the latest results in the field. I will highlight the recent precision measurement of the ^7Be solar neutrino interaction rate with the Borexino solar neutrino detector and present the status of the analysis of pep and CNO neutrinos. I will also briefly describe future experiments and their potential to detect low energy solar neutrinos.

  1. Some Recent Results with CLAS

    SciTech Connect

    Maurik Holtrop

    2010-10-01

    The CLAS is a multipurpose, large acceptance magnetic spectrometer, instrumented with detector systems sensitive to charged and neutral particles. The experimental program at CLAS is aimed at furthering our understanding of hadronic and nuclear physics, through electron and photon scattering experiments, which cover a large range of topics, including meson and baryon spectroscopy, nucleon structure through elastic and deep inelastic scattering, nuclear transparency, nuclear correlations and nuclear structure. This talk will briefly describe the detector and the collaboration that uses it and will highlight some recent results.

  2. Recent results from SND detector

    NASA Astrophysics Data System (ADS)

    Achasov, M. N.; Barnyakov, A. Yu.; Beloborodov, K. I.; Berdyugin, A. V.; Bogdanchikov, A. G.; Botov, A. A.; Dimova, T. V.; Druzhinin, V. P.; Golubev, V. B.; Kardapoltsev, L. V.; Kharlamov, A. G.; Koop, I. A.; Korol, A. A.; Koshuba, S. V.; Kovrizhin, D. P.; Kupich, A. S.; Martin, K. A.; Obrazovsky, A. E.; Pakhtusova, E. V.; Rogozina, E. V.; Serednyakov, S. I.; Shatunov, Yu. M.; Shtol, D. A.; Silagadze, Z. K.; Surin, I. K.; Usov, Yu. V.; Vasiljev, A. V.

    2016-05-01

    Recent results from the SND detector obtained in experiments at the VEPP-2000 e+e- collider are presented. The reactions e+e- → ηπ+π-, e+e- → K+K-, e+e- → π+π-π0, e+e- → ωπ0, e+e- → ωη have been studied in the energy region 1.05-2.00 GeV. The neutron and proton electromagnetic form factors have been measured in the energy range from the threshold up to 2 GeV. The result of the search of the rare process e+e- → η' is also presented.

  3. Recent Opportunity Microscopic Imager Results

    NASA Astrophysics Data System (ADS)

    Herkenhoff, K. E.; Arvidson, R. E.; Jolliff, B. L.; Yingst, R.; Team, A.

    2013-12-01

    Opportunity. The extremely soft bedrock exposed at a Whitewater Lake outcrop target dubbed 'Azilda' is mostly fine-grained, with dispersed 2-5 mm-diameter spherules and resistant veins. This target was easily abraded by the RAT, exposing a sandstone-like texture, but the sorting of grains is difficult to determine at MI resolution. Darker, erosion-resistant veneers, similar to desert varnishes on Earth, appear to record aqueous alteration that post-dates the formation of the Ca sulfate veins; they likely contain the nontronite that is observed by CRISM in this area. The inferred neutral pH and relatively low temperature of the fluids involved in these phases of alteration would have provided a habitable environment for life if it existed on Mars at that time. Because Opportunity can no longer directly sense phyllosilicate mineralogy with the MiniTES or Mössbauer spectrometers, it is focusing on characterizing the chemistry with the APXS and texture with the MI of potential phyllosilicate host rocks. The Athena MI continues to return useful images of Mars that are being used to study the textures of rocks and soils at Endeavour crater. Exploration by Opportunity continues, with the rover approaching 'Solander Point' and more exposures of phyllosilicates detected from orbit; the latest MI results will be presented at the conference.

  4. Recent results from telescope array

    NASA Astrophysics Data System (ADS)

    Fukushima, Masaki

    2015-08-01

    The Telescope Array (TA) is an experiment to observe Ultra-High Energy Cosmic Rays (UHECRs). TA's recent results, the energy spectrum and anisotropy based on the 6-year surface array data, and the primary composition obtained from the shower maximum (XMAX) are reported. The spectrum demonstrates a clear dip and cutoff. The shape of the spectrum is well described by the energy loss of extra-galactic protons interacting with the cosmic microwave background (CMB). Above the cutoff, a medium-scale (20∘ radius) flux enhancement was observed near the Ursa-Major. A chance probability of creating this hotspot from the isotropic flux is 4.0 σ. The measured ⟨XMAX⟩ is consistent with the primary being proton or light nuclei for energies 1018.2 eV-1019.2 eV.

  5. Overview of recent HERMES results

    NASA Astrophysics Data System (ADS)

    Marukyan, Hrachya

    2016-02-01

    An overview of more recent and important results from the HERMES experiment are presented in this paper. HERMES collected a wealth of data using the 27.6 GeV polarized HERA lepton beam and various polarized and unpolarized gaseous targets. This unique data set opens the door to the measurements of observables sensitive to the multidimensional structure of the nucleon. Among them are semi-inclusive deep-inelastic scattering measurements of azimuthal modulations sensitive to the transverse momentum distributions, such as the leading- twist Sivers and Collins distributions and distributions sensitive to the convolutions of the twist-2 and twist-3 functions. They all provide an information on the three-momentum-dependent quark distributions. Knowledge on the quark distribution as a function of longitudinal momentum and transverse position in impact-parameter space can be accessed, e.g., through exclusive ω—meson leptoproduction, particularly through the measurement of spin density matrix elements and the measurement of azimuthal modulations on transversely polarized proton target. The measurement of Bose-Einstein correlations of hadron pairs in quasi-real leptoproduction are also presented. The transverse polarization of Λ hyperons measured again in quasi-real leptoproduction regime are presented as well. Finally, the new analysis for the search on pentaquark at HERMES are mentioned.

  6. Recent Results on Singularity Strengths

    NASA Astrophysics Data System (ADS)

    Nolan, Brien

    2002-12-01

    In this contribution, we review some recent results on strengths of singularities. In a space-time (M,g), let γ[τ0, 0) → M be an incomplete, inextendible causal geodesic, affinely parametrised by τ, tangent ěc k. Let Jτ1 :=set of Jacobi fields along γ, orthogonal to γ and vanishing at time τ1 ≥ τ0 i.e. ěc ξ ∈ J{τ 1 } iff D2ξa = -Rbcdakbkdξc, gabξakb = 0, and ěc ξ (τ 1 ) = 0. Vτ1(τ) := volume element defined by full set of independent elements of Jτ1 (2-dim for null geodesies, 3-dim for time-like); Vτ1 := ∥Vτ1∥. Definition (Tipler 1977): γ terminates in a gravitationally strong singularity if for all 0 > τ1 ≥ τ0, lim infτ→0- Vτ1(τ) = 0. γ... gravitationally weak ... lim infτ→0- Vτ1(τ) > 0. The interpretation is that at a strong singularity, an extended body, e.g. a gravitational wave detector, is crushed to zero volume by the singularity. Tipler's definition does not take account of the possibility that (i) V → ∞ or (ii) V → finite, non-zero value, but with infinite stretching/crushing in orthogonal directions ('spaghettifying singularity'). Extended definition (Nolan 1999): strong if either V → 0,∞ or if for every τ1, there is an element ěc ξ of Jτ1 satisfying ||ěc ξ || -> 0. Otherwise weak. (Ori 2000): singularity is 'deformationally strong' if either (i) it is Tipler-strong or (ii) for every τ1, there is an element ěc ξ of Jτ1 satisfying ||ěc ξ || -> ∞ . Otherwise, deformationally weak...

  7. Recent results from the Tevatron

    SciTech Connect

    Vellidis, Costas; Bravina, L.; Foka, Y.; Kabana, S.

    2015-01-01

    The Tevatron p$\\bar{p}$ collider was shut down in 2011, after 10 years of high performance operation at a center-of-mass energy √s = 1.96 TeV in Run II. The two experiments, CDF and DZero, continue to analyze the collected data, aiming to extract all possible information regarding studies of the standard model and searches for new physics. A short review of some of the recent measurements at the Tevatron, and of the impact of the Tevatron program to high energy physics, is presented.

  8. Recent QCD results from CDF

    SciTech Connect

    Yun, J.C.

    1990-10-10

    In this paper we report recent QCD analysis with the new data taken from CDF detector. CDF recorded an integrated luminosity of 4.4 nb{sup {minus}1} during the 1988--1989 run at center of mass system (CMS) energy of 1.8 TeV. The major topics of this report are inclusive jet, dijet, trijet and direct photon analysis. These measurements are compared of QCD predictions. For the inclusive jet an dijet analysis, tests of quark compositeness are emphasized. 11 refs., 6 figs.

  9. Recent results from the Tevatron

    NASA Astrophysics Data System (ADS)

    Vellidis, Costas

    2015-05-01

    The Tevatron pp¯ collider was shut down in 2011, after 10 years of high performance operation at a center-of-mass energy √s = 1.96 TeV in Run II. The two experiments, CDF and DZero, continue to analyze the collected data, aiming to extract all possible information regarding studies of the standard model and searches for new physics. A short review of some of the recent measurements at the Tevatron, and of the impact of the Tevatron program to high energy physics, is presented.

  10. Some recent results from ICARUS

    SciTech Connect

    Farnese, Christian

    2015-07-15

    ICARUS T600 is the largest Liquid Argon (LAr) Time Projection Chamber (TPC) ever built. Thanks to the excellent spatial and calorimetric resolutions and the three-dimensional visualization capabilities ICARUS T600 represents a major milestone towards the realization of future LAr detectors for neutrino physics and for the search of rare events. Three new important results from the analysis of the events collected by this detector will be here shortly presented: in particular the new improved results on the electron neutrino search, the results on the determination of the muon momentum using the Multiple Scattering and the new LAr purification methods and improvements of the electron lifetime.

  11. PT quantum mechanics - Recent results

    NASA Astrophysics Data System (ADS)

    Bender, Carl M.

    2012-09-01

    Most quantum physicists believe that a quantum-mechanical Hamiltonian must be Dirac Hermitian (invariant under matrix transposition and complex conjugation) to be sure that the energy eigenvalues are real and that time evolution is unitary. However, the non-Dirac-hermitian Hamiltonian H = p2+ix3 has a real positive discrete spectrum and generates unitary time evolution and defines a fully consistent and physical quantum theory. Evidently, Dirac Hermiticity is too restrictive. While H = p2+ix3 is not Dirac Hermitian, it is PT symmetric (invariant under combined space reflection P and time reversal T). Another PT-symmetric Hamiltonian whose energy levels are real, positive and discrete is H = p2-x4, which contains an upside-down potential. The quantum mechanics defined by a PT-symmetric Hamiltonian is a complex generalization of ordinary quantum mechanics. When quantum mechanics and quantum field theory are extended into the complex domain, new kinds of theories having strange and remarkable properties emerge. In the past two years some of these properties have been verified in laboratory experiments. Here, we first discuss PT-symmetric Hamiltonians at a simple intuitive level and explain why the energy levels of such Hamiltonians may be real, positive, and discrete. Second, we describe a recent experiment in which the PT phase transition was observed. Third, we briefly mention that PT-symmetric theories can be useful at a fundamental level. While the double-scaling limit of an O(N)-symmetric gφ4 quantum field theory appears to be inconsistent because the critical value of g is negative, this limit is in fact not inconsistent because the critical theory is PT symmetric.

  12. Catastrophic disruption experiments: Recent results

    NASA Technical Reports Server (NTRS)

    Martelli, G.; Ryan, E. V.; Nakamura, A. M.; Giblin, I.

    1994-01-01

    This paper presents a review of the progress in the field of catastrophic disruption experiments over the past 4 years, since the publication of the review paper by Fujiwara et al. (1989). We describe the development of new techniques to produce shattering impacts relevant to the study of the collisional evolution of the asteroids, and summarize the results from numerous experiments which have been performed to date, using a variety of materials for both the impactor and the targets. Some of these, such as ice-on-ice, loose aggregates and pressurized targets, are quite new and have provided novel and exciting results. Some of the gaps existing previously in the data on fragment ejection-angle distributions, as well as translational and rotational velocity fields (including fine fragments) have been filled, and these new results will be surveyed.

  13. Recent diffractive results from HERA

    NASA Astrophysics Data System (ADS)

    Valkárová, Alice

    2016-07-01

    The diffractive dijet cross sections for photoproduction and deep inelastic scattering were studied and compared with theoretical NLO QCD predictions. The results of exclusive dijet production were compared to predictions from models which are based on different assumptions about the nature of diffractive exchange. Isolated prompt photons in diffractive photoproduction produced inclusively or together with a jet were studied for the first time.

  14. Double Chooz and recent results

    NASA Astrophysics Data System (ADS)

    Meregaglia, A.; Double Chooz Collaboration

    2016-07-01

    The reactor bar{{ν}}e^{} disappearance experiment Double Chooz, located in France near the power plant of Chooz, has as main goal the measurement of the θ_{{13}}^{} mixing angle. For the first time, in 2011, the experimental results gave an indication for a non-zero value of such an oscillation parameter. The mixing angle was successively measured using only the far detector finding the best fit value of sin2(2 θ_{{13}}^{}) = 0.090+0.033-0.029 . The near detector started data taking in December 2014 and it will allow to reduce the systematic errors so far dominated by the reactor flux uncertainty. In this paper a review of the experiment is presented focusing on the so-called Gadolinium-III results (DOUBLE CHOOZ COLLABORATION (ABE Y. et al.), JHEP, 10 (2014) 086; 02 (2015) 074). Furthermore additional physics measurements are presented such as the capability of Double Chooz to identify the ortho-positronium state on event by event basis.

  15. Gap analysis: Concepts, methods, and recent results

    USGS Publications Warehouse

    Jennings, M.D.

    2000-01-01

    Rapid progress is being made in the conceptual, technical, and organizational requirements for generating synoptic multi-scale views of the earth's surface and its biological content. Using the spatially comprehensive data that are now available, researchers, land managers, and land-use planners can, for the first time, quantitatively place landscape units - from general categories such as 'Forests' or 'Cold-Deciduous Shrubland Formation' to more categories such as 'Picea glauca-Abies balsamea-Populus spp. Forest Alliance' - in their large-area contexts. The National Gap Analysis Program (GAP) has developed the technical and organizational capabilities necessary for the regular production and analysis of such information. This paper provides a brief overview of concepts and methods as well as some recent results from the GAP projects. Clearly, new frameworks for biogeographic information and organizational cooperation are needed if we are to have any hope of documenting the full range of species occurrences and ecological processes in ways meaningful to their management. The GAP experience provides one model for achieving these new frameworks.

  16. Symposium on Recent Results in Infrared Astrophysics

    NASA Technical Reports Server (NTRS)

    Dyal, P. (Editor)

    1977-01-01

    Abstracts of papers presented at a symposium titled Recent Results in Infrared Astrophysics are set forth. The abstracts emphasize photometric, spectroscopic, polarization, and theoretical results on a broad range of current topics in infrared astrophysics.

  17. Recent observations of the formation of filaments

    NASA Astrophysics Data System (ADS)

    Martin, Sara F.

    1986-12-01

    Two examples of the formation of small filaments in H alpha are described and illustrated. In both cases, the formation is seen to be the spontaneous appearance of strands of absorbing mass that evolve from no previous structure. The initial development of the filaments appears to consist of the accumulation of these absorptive strands along approximately parallel paths in a channel between large-scale, opposite polarity magnetic fields on either side of the filaments. The strands exhibit continuous changes in shape and degree of absorption which can be due to successive condensations resulting in new strands, mass motions within the strands, and outflow of the mass from the strands. For at least several hours before the formation of both filaments, small-scale fragments of opposite polarity, line-of-sight magnetic flux adjacent to or immediately below the filaments, and at the ends of the filaments, were cancelling. This type of magnetic flux disappearance continued during the development of the filaments and is commonly observed in association with established filaments. Cancellation is interpreted as an important evolutionary change in the magnetic field that can lead to configurations suitable for the formation of filaments.

  18. Jefferson Lab physics overview: Recent results

    SciTech Connect

    Meziani, Zein-Eddine

    2007-09-01

    I review highlights of the Jefferson Lab nucleon structure program. I shall emphasize recent results from experiments exploring the spin structure of the nucleon and from dedicated experiments aimed at accessing the generalized parton distributions (GPDs).

  19. Recent QCD results from the Tevatron

    SciTech Connect

    Pickarz, Henryk; CDF and DO collaboration

    1997-02-01

    Recent QCD results from the CDF and D0 detectors at the Tevatron proton-antiproton collider are presented. An outlook for future QCD tests at the Tevatron collider is also breifly discussed. 27 refs., 11 figs.

  20. Recent Results from the MAGIC Telescope

    SciTech Connect

    Bock, Rudolf K.

    2005-02-21

    Some recent results are shown, obtained during the commissioning period of the MAGIC telescope. They demonstrate that the telescope is now approaching a performance level suitable for physics observations.

  1. Highlights of Recent Results with Clas

    SciTech Connect

    Volker Burkert

    2005-04-01

    Recent results on the study of the electromagnetic structure of nucleon resonances, the spin structure of proton and neutrons at small and intermediate photon virtualities, and the search for exotic pentaquark baryons are presented.

  2. Recent work and results on sparrow project

    SciTech Connect

    Harvey, Neal R

    2010-12-23

    This briefing describes recent work undertaken on the Sparrow Project and results of this work. It describes experiments comparing the use of Genie with 2 classes with 3 classes for the problem of ship delineation. It also describes some preliminary work in the area of the optimization of segmentation techniques.

  3. Recent Stirling engine loss-understanding results

    NASA Technical Reports Server (NTRS)

    Tew, Roy C.; Thieme, Lanny G.; Dudenhoefer, James E.

    1990-01-01

    For several years, NASA and other U.S. government agencies have been funding experimental and analytical efforts to improve the understanding of Stirling thermodynamic losses. NASA's objective is to improve Stirling engine design capability to support the development of new engines for space power. An overview of these efforts was last given at the 1988 IECEC. Recent results of this research are reviewed.

  4. Recent results from COMPASS muon scattering measurements

    SciTech Connect

    Capozza, Luigi [Irfu Collaboration: COMPASS Collaboration

    2012-10-23

    A sample of recent results in muon scattering measurements from the COMPASS experiment at CERN will be reviewed. These include high energy processes with longitudinally polarised proton and deuteron targets. High energy polarised measurements provide important constraints for studying the nucleon spin structure and thus permit to test the applicability of the theoretical framework of factorisation theorems and perturbative QCD. Specifically, latest results on longitudinal quark polarisation, quark helicity densities and gluon polarisation will be reviewed.

  5. Random walk through recent CDF QCD results

    SciTech Connect

    C. Mesropian

    2003-04-09

    We present recent results on jet fragmentation, jet evolution in jet and minimum bias events, and underlying event studies. The results presented in this talk address significant questions relevant to QCD and, in particular, to jet studies. One topic discussed is jet fragmentation and the possibility of describing it down to very small momentum scales in terms of pQCD. Another topic is the studies of underlying event energy originating from fragmentation of partons not associated with the hard scattering.

  6. Recent Results in Ring-Diagram Analysis

    NASA Astrophysics Data System (ADS)

    Rabello-Soares, M. C.

    2013-12-01

    The ring-diagram technique was developed by Frank Hill 25 years ago and matured quickly during the late 1990s. It is nowadays one of the most commonly used techniques in local helioseismology. The method consists in the power spectral analysis of solar acoustic oscillations on small regions (2° to 30°) of the solar surface. The power spectrum resembles a set of trumpets nested inside each other and for a given frequency, it looks like a ring, hence the technique's name. It provides information on the horizontal flow field and thermodynamic structure in the layers immediately below the photosphere. With data regularly provided by MDI, GONG, and more recently HMI, many important results have been achieved. In recently years, these results include estimations of the meridional circulation and its evolution with solar cycle; flows associated with active regions, as well as, flow divergence and vorticity, and thermal structure beneath and around active regions. Much progress is expected with data now provided by HMI's high spatial resolution observations and high duty cycle. There are two data processing pipelines (GONG and HMI) providing free access to the data and the results of the ring-diagram analysis. Here we will discuss the most recent results and improvements in the technique, as well as, the many challenges that still remain.

  7. Recent Results from PHOBOS at RHIC

    NASA Astrophysics Data System (ADS)

    Garcia, Edmundo; Back, B. B.; Baker, M. D.; Ballintijn, M.; Barton, D. S.; Betts, R. R.; Bickley, A. A.; Bindel, R.; Busza, W.; Carroll, A.; Chai, Z.; Decowski, M. P.; Garcia, E.; Gburek, T.; George, N.; Gulbrandsen, K.; Halliwell, C.; Hamblen, J.; Hauer, M.; Henderson, C.; Hofman, D. J.; Hollis, R. S.; Hołyński, R.; Holzman, B.; Iordanova, A.; Johnson, E.; Kane, J. L.; Khan, N.; Kulinich, P.; Kuo, C. M.; Lin, W. T.; Manly, S.; Mignerey, A. C.; Nouicer, R.; Olszewski, A.; Pak, R.; Reed, C.; Roland, C.; Roland, G.; Sagerer, J.; Seals, H.; Sedykh, I.; Smith, C. E.; Stankiewicz, M. A.; Steinberg, P.; Stephans, G. S. F.; Sukhanov, A.; Tonjes, M. B.; Trzupek, A.; Vale, C.; van Nieuwenhuizen, G. J.; Vaurynovich, S. S.; Verdier, R.; Veres, G. I.; Wenger, E.; Wolfs, F. L. H.; Wosiek, B.; Woźniak, K.; Wysłouch, B.

    2006-04-01

    The PHOBOS detector is one of four heavy-ion experiments at the Relativistic Heavy Ion Collider (RHIC) at Brookhaven National Laboratory. In this paper we will review some of the results of PHOBOS from the data collected in p+p, d+Au and Au+Au collisions at nucleon-nucleon center-of-mass energies up to 200 GeV. In the most central Au+Au collisions at the highest energy, evidence is found for the formation of a very high energy density and highly interactive system, which can not be described in terms of hadrons, and which has a relatively low baryon density.

  8. Recent results from the Pierre Auger Observatory

    SciTech Connect

    Gascón, Alberto; Collaboration: Pierre Auger Collaboration

    2014-07-23

    The Pierre Auger Observatory has been designed to investigate the origin and nature of Ultra High Energy Cosmic Rays (UHECR) using a hybrid detection technique. In this contribution we present some of the most recent results of the observatory, namely the upper-end of the spectrum of cosmic rays, state-of-the-art analyses on mass composition, the measurements of the proton-air cross-section, and the number of muons at ground.

  9. Recent Results from MINERvA

    SciTech Connect

    Miller, Jonathan

    2014-09-01

    MINERvA (Main INjector ExpeRiment for v-A) is a few-GeV neutrino nucleus scattering experiment at Fermilab using various nuclei as targets. The experiment provides measurements of neutrino and anti-neutrino cross sections off of nuclear targets which are important for neutrino oscillation experiments and the probing of the nuclear medium.Presented are recent results from MINERvA on quasi-elastic, inclusive charged-current neutrino scattering, and pion production processes.

  10. Recent Results of Explorer and NAUTILUS

    NASA Astrophysics Data System (ADS)

    Fafone, V.; Rog Collaboration

    2002-12-01

    The most recent results of the resonant-mass gravitational wave (GW) detectors NAUTILUS and EXPLORER, operated by the ROG collaboration at the INFN Frascati National Laboratories and at CERN respectively, are reported. The passage of cosmic rays has been observed to excite mechanical vibrations in NAUTILUS. The new read-out electronics and the improved sensitivity of EXPLORER-with a bandwidth larger than 40 Hz at the level of 5·10-21 Hz-1/2 - are described.

  11. Recent Results from KTeV

    SciTech Connect

    Leo Bellantoni et al.

    2001-08-02

    Recent results are presented for (1) the charge asymmetry in semielectronic kaon decay; (2) the charge radius of the neutral kaon; (3) the decay K{sub L}{sup 0} {r_arrow} {pi}{sup 0}{pi}{sup 0}e{sup +}e{sup {minus}}; (4) constraints on {rho}{sub CKM} from kaon decays; (5) lepton flavor violation. A few words about future kaon physics work at Fermilab are included.

  12. Recent Higgs results from the ATLAS experiment

    SciTech Connect

    Brendlinger, Kurt; Collaboration: ATLAS Collaboration

    2014-06-24

    This paper presents recent results on the Higgs boson from the ATLAS experiment at the Large Hadron Collider. The Collaboration reports on measurements of the signal strength, couplings, and spin of the Higgs in several decay channels. We find all measurements to be consistent with Standard Model predictions. The Higgs branching fraction to invisible particles is constrained and no evidence of physics beyond the Standard Model is found.

  13. Recent Stirling engine loss - understanding results

    SciTech Connect

    Tew, R.C.; Thieme, L.G.; Dudenhoefer, J.E.

    1994-09-01

    For several years, the National Aeronautics and Space Administration and other US Government agencies have been funding experimental and analytical efforts to improve the understanding of Stirling thermodynamic losses. NASA`s objective is to improve Stirling engine design capability to support the development of new engines for space power. An overview of these efforts was last given at the 1988 IECEC. Recent results of this research are reviewed.

  14. The recent results from KIMS experiment

    NASA Astrophysics Data System (ADS)

    Kim, SeungCheon; Kims Collaboration

    2012-09-01

    In this paper, the recent results from KIMS (Korea invisible mass search) experiment are presented. KIMS has searched for WIMPs (Weakly Interactig Massive Particles) scattering off the nucleus by using the CsI(Tl) scintillator. The detector is an array of 12 CsI(Tl) scintilltors, whose total mass is 103.4 kg. The results reported here used the exposure of 24524.3 kg-days. With pulse shape discrimination (PSD) analysis, we estimated the nuclear recoil (NR) event rate and no meaningful excess of NR events rate were found. From this, we derived the improved cross section limit for WIMP-nucleon interaction.

  15. Recent results from strangeness in transport models

    NASA Astrophysics Data System (ADS)

    Steinheimer, J.; Botvina, A. S.; Bleicher, M.

    2016-01-01

    In these proceedings we discuss recent developments in the microscopic description of strange particle production in nuclear collisions. We put a special emphasis on the production of hypernuclei at the upcoming FAIR and NICA facilities as well as the deep sub threshold, ϕ and Ξ- production yields measured with the HADES experiment. Employing new resonance decay channels we obtain a satisfactory description of ϕ and Ξ- production in deep sub threshold Ar+KCl reactions. Our results implicate that no new medium effects are required to describe the rare strange particle production data from low energy nuclear collisions.

  16. Heavy baryons - Recent and very new results

    SciTech Connect

    Peter S Cooper

    2003-01-15

    Recent results on observations, properties and decay modes of the charmed and beauty baryons will be reviewed. Candidates for several new high mass states which include a cleanly-identified daughter {Lambda}{sub c}{sup +} baryon are seen in data from the SELEX experiment at Fermilab. These states are candidates for doubly-charmed baryons: a {Xi}{sub cc}{sup ++} state and a {Xi}{sub cc}{sup +} state. These candidates are more than 5{sigma} signals in each case at masses of 3520 and 3460 MeV respectively.

  17. Recent Results from NASA's Morphing Project

    NASA Technical Reports Server (NTRS)

    McGowan, Anna-Maria R.; Washburn, Anthony E.; Horta, Lucas G.; Bryant, Robert G.; Cox, David E.; Siochi, Emilie J.; Padula, Sharon L.; Holloway, Nancy M.

    2002-01-01

    The NASA Morphing Project seeks to develop and assess advanced technologies and integrated component concepts to enable efficient, multi-point adaptability in air and space vehicles. In the context of the project, the word "morphing" is defined as "efficient, multi-point adaptability" and may include macro, micro, structural and/or fluidic approaches. The project includes research on smart materials, adaptive structures, micro flow control, biomimetic concepts, optimization and controls. This paper presents an updated overview of the content of the Morphing Project including highlights of recent research results.

  18. Recent results of the LOPES experiment

    NASA Astrophysics Data System (ADS)

    Haungs, A.; Apel, W. D.; Arteaga, J. C.; Asch, T.; Badea, F.; Bähren, L.; Bekk, K.; Bertaina, M.; Biermann, P. L.; Blümer, J.; Bozdog, H.; Brancus, I. M.; Brüggemann, M.; Buchholz, P.; Buitink, S.; Cantoni, E.; Chiavassa, A.; Cossavella, F.; Daumiller, K.; de Souza, V.; di Pierro, F.; Doll, P.; Ender, M.; Engel, R.; Falcke, H.; Finger, M.; Fuhrmann, D.; Gemmeke, H.; Ghia, P. L.; Glasstetter, R.; Grupen, C.; Heck, D.; Hörandel, J. R.; Horneffer, A.; Huege, T.; Isar, P. G.; Kampert, K.-H.; Kang, D.; Kickelbick, D.; Kolotaev, Y.; Krömer, O.; Kuijpers, J.; Lafebre, S.; Link, K.; Łuczak, P.; Ludwig, M.; Mathes, H. J.; Mayer, H. J.; Melissas, M.; Mitrica, B.; Morello, C.; Navarra, G.; Nehls, S.; Nigl, A.; Oehlschläger, J.; Over, S.; Palmieri, N.; Petcu, M.; Pierog, T.; Rautenberg, J.; Rebel, H.; Roth, M.; Saftoiu, A.; Schieler, H.; Schmidt, A.; Schröder, F.; Sima, O.; Singh, K.; Toma, G.; Trinchero, G.; Ulrich, H.; Walkowiak, W.; Weindl, A.; Wochele, J.; Wommer, M.; Zabierowski, J.; Zensus, J. A.; Lopes Collaboration

    2009-12-01

    LOPES measures radio pulses from extensive air showers and aims to calibrate the emitted signal in the primary energy range of 10 16-10 18 eV. LOPES, a digital radio interferometer using high bandwidths and fast data processing, is set up at the location of the KASCADE-Grande extensive air shower experiment in Karlsruhe, Germany and profits from the reconstructed air shower observables of KASCADE-Grande. We report about recent analysis results of the radio signals measured by LOPES.

  19. Gamma Ray Bursts and recent Swift Results .

    NASA Astrophysics Data System (ADS)

    Chincarini, G.

    Due to the large activity we had during these last months with the Swift satellite I started the writing of the presentation I gave at the SAIt Catania meeting only in the middle of September. The Swift satellite, however, never rested. Since then and in addition to the results I showed at the meeting in relation to the early and steep light curves observed with the XRT telescope in the 0.2 - 10 keV band, we had fundamental discoveries among which the detection and localization of short bursts and the detection of the largest redshift ever. It obviously would be improper to discuss here the most recent results but it would also be silly in such a fast evolving topics where the day by day observations show excellent results and the observer is far ahead of the theoretician, to write an article that, from the observational point of view, would be completely obsolete. The best approach here seems to be a brief description of what was presented during the meeting briefly mentioning also some of the most recent results. We remind the reader, however, that a copious literature written, and in preparation, exists so that we urge the reader to refer to the specialized articles. This brief article will touch on the basic characteristics of the Gamma Ray Bursts (GRBs) in the Introduction (section 1) and illustrate the basic characteristics of the Swift mission in section 2. Preliminary science results will be discussed in section 3 and finally we will mention one, among many, of the main goal we plan to achieve in Cosmology via the observations of very distant GRBs.

  20. Recent results on XYZ States at Belle

    NASA Astrophysics Data System (ADS)

    Shen, Chengping

    2016-05-01

    Exotic hadronic states beyond the conventional quark model (called charmoniumlike/bottomoniumlike states or XYZ particles) have been sought and many candidates were proposed including glueballs, hybrids, multi-quark states, hadron molecules, etc. Dramatic progress has been made in the study of such exotic hadrons after the running of the B-factories. In this report, I present the most recent results on the XYZ states at Belle, including (1) X states: the first observation of B0 → X(3872)K+π- and evidence for B+ → X(3872)K0 π+; search for the Xb state; (2) Y states: the updated results for the Y(4360) and Y(4660) and cross section measurement of e+e- → K+ K- J/ψ; (3) Z states: the evidence for the Zc(4050)± → π±ψ(2S); search for the Zcs in e+e- → K+ K- J/ψ.

  1. Recent B Physics Results from the Tevatron

    SciTech Connect

    Behari, Satyajit

    2011-07-01

    We review recent B physics results from the CDF and D0 experiments in p{bar p} collisions at {radical}(s) = 1.96 TeV. Using a data sample of 1.4-6.0 fb{sup -1} collected by the CDF II detector we present searches for New Physics in B{sub s} sector and some competitive results with B-factories in the B/charm sector. In the first category we report the BR in B{sub s} J/{Psi} f{sub 0}(980) decays and the time-integrated mixing probability ({bar {chi}}) of B mesons. In the second category BR and A{sub CP} in doubly Cabibbo-suppressed B{sup {+-}} D{sup 0} h{sup {+-}} decays and time-integrated CP violation in D{sup 0} {yields} h{sup +}h{sup -} are presented.

  2. Overview of the recent results from CLAS

    SciTech Connect

    Marco Mirazita

    2012-03-01

    An overview of the recent results obtained at the Thomas Jefferson Laboratory on the study of the nucleon internal structure is presented, with main focus on the CLAS measurements of the Transverse Momentum Dependent partonic functions. The JLab with its CEBAF accelerator and the three experimentals halls is a Laboratory dedicated to the study of the hadronic physics with electromagnetic probes in a large variety of aspects. The physics program extends from typical nuclear effects like long range correlations in nuclei to the study of the short distance vacuum structure in parity violating experiments. In recent years, a big part of the physics program was devoted to the study of the Transverse Momentum Dependent distribution functions, new functions introduced to describe the internal structure of the nucleon. Studies of TMDs at JLab and in other laboratories have shown sizeable effects due to transverse motion of the quarks inside the nucleon, but also have open questions. These questions need to be addressed in a new generation of experiments, poviding higher precisions experimental data, and with new analysis techniques, necessary to unfold fundamental properties from the measured obsevables.

  3. Some Recent Results from the CHARA Array

    NASA Astrophysics Data System (ADS)

    ten Brummelaar, T. A.; Huber, D.; von Braun, K.; Boyajian, T.; Richardson, N. D.; Schaefer, G.; Tallon-Bosc, I.; Mourard, D.; McAlister, H. A.; Turner, N. H.; Sturmann, L.; Sturmann, J.; Monnier, J. D.; Ireland, M.

    2014-09-01

    The CHARA Array is a six 1-m telescope optical and near infrared interferometer located at the Mount Wilson Observatory in southern California and operated by the Center for High Angular Resolution Astronomy of Georgia State University. The CHARA Array has been in regular scientific operation since 2005 and now has over 55 publications in the refereed literature, including two in Science and one in Nature. The Array now supports seven beam combiners ranging from 0.5 microns up to 2.3 microns and combing from 2 to 4 beams at a time. An upgrade to a full 6-beam combiner is now underway, and fringes with all six telescopes were achieved soon after the meeting. We present some of the more recent results from the CHARA Array.

  4. Beryllium for fusion application - recent results

    NASA Astrophysics Data System (ADS)

    Khomutov, A.; Barabash, V.; Chakin, V.; Chernov, V.; Davydov, D.; Gorokhov, V.; Kawamura, H.; Kolbasov, B.; Kupriyanov, I.; Longhurst, G.; Scaffidi-Argentina, F.; Shestakov, V.

    2002-12-01

    The main issues for the application of beryllium in fusion reactors are analyzed taking into account the latest results since the ICFRM-9 (Colorado, USA, October 1999) and presented at 5th IEA Be Workshop (10-12 October 2001, Moscow Russia). Considerable progress has been made recently in understanding the problems connected with the selection of the beryllium grades for different applications, characterization of the beryllium at relevant operational conditions (irradiation effects, thermal fatigue, etc.), and development of required manufacturing technologies. The key remaining problems related to the application of beryllium as an armour in near-term fusion reactors (e.g. ITER) are discussed. The features of the application of beryllium and beryllides as a neutron multiplier in the breeder blanket for power reactors (e.g. DEMO) in pebble-bed form are described.

  5. Recent X-ray Reverberation Mapping Results

    NASA Astrophysics Data System (ADS)

    Kara, Erin

    2016-04-01

    In recent years, X-ray reverberation has opened a new way to investigate the inner accretion flow around black holes. XMM-Newton and NuSTAR observations of the high-frequency variability have shown that the soft excess, broad iron K line and Compton hump lag behind the continuum emission, suggesting light travel distances of a few gravitational radii. Beyond simply detecting reverberation, we are beginning to use reverberation to map out the geometry of the inner accretion flow, testing the compactness of the X-ray emitting source, the structure of the disc and the origin of the variability. In this talk, I will give an overview of the observational results discovered thus far, and will discuss future prospects for reverberation with upcoming observations and telescopes.

  6. Recent results from the Crystal Ball

    SciTech Connect

    Porter, F.C.

    1981-09-01

    During the past year, the Crystal Ball experiment has continued the investigation of e/sup +/e/sup -/ interactions at SPEAR. In the course of the year, we have slightly more than doubled the available datasets at the J/psi (to 2.2 x 10/sup 6/ produced J/psi) and the psi' (to 1.8 x 10/sup 6/ produced psi') resonances, and have increased the data in the 5.2 to 7.4 GeV center-of-mass (E/sub c.m./) region. The present discussion is limited to recent results obtained with the J/psi and psi' datasets, primarily dealing with transitions among the charmonium bound states.

  7. Some recent results from CLEO II

    SciTech Connect

    Kass, R.

    1997-06-01

    The CLEO experiment has been operating for several years now collecting e{sup +}e{sup {minus}} annihilation data at and near the {Upsilon}(4S) resonance (E{sub cm} {approx} 10.6 GeV). The accumulated event sample contains several million B{anti B} and {tau}{sup +}{tau}{sup {minus}} pairs. These data are used to explore rare b, c, and {tau} decays. In this report, several recent CLEO results in the area of B-meson and {tau} decay are presented. The topics covered include: penguin decays of B-mesons, measurement of exclusive b {r_arrow} u semileptonic transitions, {tau} decays with an {eta} in the final state, precision measurement of the Michel parameters in leptonic {tau} decay, and a search for lepton number violation using {tau}`s. 39 refs., 26 figs.

  8. Recent Results from the ANTARES Neutrino Telescope

    NASA Astrophysics Data System (ADS)

    Kouchner, Antoine

    2014-10-01

    The ANTARES detector, located 40 km off the French coast, is the largest deep-sea neutrino telescope in the world. It consists of an array of 885 photomultipliers detecting the Cherenkov light induced by charged leptons produced by neutrino interactions in and around the detector. The primary goal of ANTARES is to search for astrophysical neutrinos in the TeV-PeV range. This comprises generic searches for any diffuse cosmic neutrino flux as well as more specific searches for astrophysical sources such as active galactic nuclei or galactic sources. The search program also includes multi-messenger analyses based on time and/or space coincidences with other cosmic probes. The ANTARES observatory is sensitive to a wide range of other phenomena, from atmospheric neutrino oscillations to dark matter annihilation or potential exotics such as nuclearites and magnetic monopoles. The most recent results are reported.

  9. Recent results from the Crystal Barrel experiment

    SciTech Connect

    Not Available

    1991-10-09

    The Crystal Barrel experiment has been constructed and installed at the Low Energy Antiproton Ring (LEAR) at CERN. It has been fully operational since late 1989. In this talk, recent results of meson spectroscopy in p[bar p]-annihilations are presented. The main emphasis is on all-neutral annihilations, the study of the strange quark content of the proton, and the investigation of the decay mode of il particles. A 2[sup ++] resonance decaying into [pi][degrees][pi][degrees]at a mass of 1515 [plus minus] 10 MeV with a width of 120 [plus minus] 10 MeV has been seen in a 3[pi][degrees] final state.

  10. Recent results from the Crystal Barrel experiment

    SciTech Connect

    The Crystal Barrel Collaboration

    1991-10-09

    The Crystal Barrel experiment has been constructed and installed at the Low Energy Antiproton Ring (LEAR) at CERN. It has been fully operational since late 1989. In this talk, recent results of meson spectroscopy in p{bar p}-annihilations are presented. The main emphasis is on all-neutral annihilations, the study of the strange quark content of the proton, and the investigation of the decay mode of il particles. A 2{sup ++} resonance decaying into {pi}{degrees}{pi}{degrees}at a mass of 1515 {plus_minus} 10 MeV with a width of 120 {plus_minus} 10 MeV has been seen in a 3{pi}{degrees} final state.

  11. Recent charm physics results from CLEO

    SciTech Connect

    Fujino, D.H.; CLEO Collaboration

    1997-07-01

    In this talk I present recent charm physics results from the CLEO experiment. Final state interactions and W-annihilation effects in charmed mesons decays are discussed. These include an isospin analysis of D {yields} K{anti K}, observation of the candidate W- annihilation decay D{sup +}{sub s} {yields} {omega}{pi}{sup +}, and evidence of non-factorizable effects in D{sup +}{sub s} {yields} {eta}{pi}{sup +}, {eta}`{pi}{sup +}, {eta}{rho}{sup +}, and {eta}`{rho}{sup +} decays. Presented next are CLEO`s observations of the spin 3/2 {sup +} excited charmed baryons {Sigma}{sup *++}{sub c} and {Sigma}{sup *0}{sub c}, and the excited charmed-strange baryons {Xi}{sup *+}{sub c} and {Xi}{sup *0}{sub c}. I conclude with future prospects in charm physics with CLEO`s new silicon detector.

  12. Recent Results on Semileptonic Decays at Babar

    SciTech Connect

    Serrano, Justine; /Orsay, LAL

    2011-11-07

    Some recent BABAR results on semileptonic decays are presented. They focus on the determination of the CKM matrix elements |V{sub ub}| and |V{sub cb}| in inclusive and exclusive b {yields} u{ell}v and b {yields} c{ell}v decays, and on form factors measurement in exclusive c {yields} s{ell}v decays. Semileptonic decays play a crucial role in the determination of the unitarity triangle parameters: decays of the b quark give access to the CKM matrix elements |V{sub ub}| and |V{sub cb}|, while charm decays provide a way to validate lattice QCD computations through form factors measurements. Such calculations provide theoretical inputs that are used, especially, in the b sector. A lot of new results have been obtained by the BABAR collaboration during the last years, thanks to the large b{bar b} and c{bar c} production cross-sections and to the large recorded statistics. Some of these measurements are presented here.

  13. Recent trial results of an LWIR polarimeter

    NASA Astrophysics Data System (ADS)

    Connor, Barry; Carrie, Iain

    2009-05-01

    The aim of this paper is to describe the results of various trials involving a high-resolution thermal imager that has been designed to be sensitive to polarised radiation. Polarisation has the potential to discriminate man-made objects and disturbed earth from background clutter. Polarisation combined with conventional thermal imaging within the one camera offers the potential to significantly reduce false alarms in surveillance and detection applications. The camera used during the trials is a technology demonstrator developed by Thales Optronics, UK. The camera operates in the longwave infra red and has a QWIP polarisation-sensitive detector. The results presented in this paper include recent trials in the UK and USA. The aim of the trials was to assess the utility in using a LWIR polarimeter for detection of difficult objects from background clutter. Thermal and polarised images were captured and processed in order to detect anomalies. Several polarisation-based discriminative imaging techniques are applied to trials imagery. The effect of the diurnal cycle on the effectiveness of polarisation for object discrimination will be assessed.

  14. Overview of recent DVCS results from HERMES

    NASA Astrophysics Data System (ADS)

    Yaschenko, Sergey; Hermes Collaboration

    2012-09-01

    Hard exclusive leptoproduction of real photons on nucleons and nuclei, Deeply Virtual Compton Scattering (DVCS), is one of the theoretically cleanest ways to access Generalized Parton Distributions (GPDs). The theoretical framework of GPDs includes parton distribution functions and form factors as limiting cases and as moments of GPDs, respectively, and can provide a multidimensional representation of the structure of hadrons at the partonic level. The HERMES experiment at DESY, Hamburg, collected a wealth of data on DVCS utilizing the HERA polarized electron or positron beams with an energy of 27.6 GeV and longitudinally and transversely polarized or unpolarized gas targets (H, D or heavier nuclei). The azimuthal asymmetries measured in the DVCS process allow access to the imaginary and/or real part of certain combinations of GPDs. For the last two years of HERA running, the HERMES collaboration installed a recoil detector to improve the selection of DVCS events by direct measurement of the recoil protons. An overview of recent HERMES results on DVCS including first results obtained with the recoil detector is presented.

  15. Morphology Composition Isotopes: Recent Results from Observations

    NASA Astrophysics Data System (ADS)

    Schulz, R.

    2008-07-01

    This article presents some recent imaging and spectroscopic observations that led to results which are significant for understanding the properties of comet nuclei. The coma morphology and/or composition were investigated for 12 comets belonging to different dynamical classes. The data analysis showed that the coma morphology of three non-periodic comets is not consistent with the general assumption that dynamically new comets still have a relatively uniform nucleus surface and therefore do not exhibit gas and/or dust jets in their coma. The determination of carbon and nitrogen isotopic ratios revealed the same values for all comets investigated at various heliocentric distances. However, the relative abundance of the rare nitrogen isotope 15N is about twice as high as in the Earth’s atmosphere. Observations of comets at splitting events and during outbursts led to indications for differences between material from the nucleus surface and the interior. The monitoring of the induced outburst of 9P/Temple revealed that under non-steady state conditions the fast disintegration of species is detectable.

  16. Recent ADI iteration analysis and results

    SciTech Connect

    Wachspress, E.L.

    1994-12-31

    Some recent ADI iteration analysis and results are discussed. Discovery that the Lyapunov and Sylvester matrix equations are model ADI problems stimulated much research on ADI iteration with complex spectra. The ADI rational Chebyshev analysis parallels the classical linear Chebyshev theory. Two distinct approaches have been applied to these problems. First, parameters which were optimal for real spectra were shown to be nearly optimal for certain families of complex spectra. In the linear case these were spectra bounded by ellipses in the complex plane. In the ADI rational case these were spectra bounded by {open_quotes}elliptic-function regions{close_quotes}. The logarithms of the latter appear like ellipses, and the logarithms of the optimal ADI parameters for these regions are similar to the optimal parameters for linear Chebyshev approximation over superimposed ellipses. W.B. Jordan`s bilinear transformation of real variables to reduce the two-variable problem to one variable was generalized into the complex plane. This was needed for ADI iterative solution of the Sylvester equation.

  17. Recent Results from the MINOS Experiment

    SciTech Connect

    Diwan,M.V.

    2009-03-10

    MINOS is an accelerator neutrino oscillation experiment at Fermilab. An intense high energy neutrino beam is produced at Fermilab and sent to a near detector on the Fermilab site and also to a 5 kTon far detector 735 km away in the Soudan mine in northern Minnesota. The experiment has now had several years of running with millions of events in the near detector and hundreds of events recorded in the far detector. I will report on the recent results from this experiment which include precise measurement of |{Delta}m{sup 2}{sub 32}|, analysis of neutral current data to limit the component of sterile neutrinos and the search for {nu}{sub {mu}} {yields} {nu}{sub e} conversion. The focus will be on the analysis of data for {nu}{sub {mu}} {yields} {nu}{sub e} conversion. Using data from an exposure of 3.14 x 10{sup 20} protons on target, we have selected electron type events in both the near and the far detector. The near detector is used to measure the background which is extrapolated to the far detector. We have found 35 events in the signal region with a background expectation of 27 {+-} 5(stat) {+-} 2(syst). Using this observation we set a 90% C.L. limit of sin{sup 2} 2{theta}{sub 13} < 0.29 for {delta}{sub cp} = 0 and normal mass hierarchy. Further analysis is under way to reduce backgrounds and improve sensitivity.

  18. Recent star formation in 30 Doradus

    NASA Astrophysics Data System (ADS)

    De Marchi, Guido; Paresce, F.; Panagia, N.; Beccari, G.; Spezzi, L.; Sirianni, M.; Andersen, M.; SOC, WFC3

    2011-01-01

    Using observations obtained with the WFC3 camera on board the Hubble Space Telescope, we have studied the star formation properties of the central regions of 30 Dor, in the Large Magellanic Cloud. The observations clearly reveal the presence of considerable differential extinction across the field. We characterise and quantify this effect using young massive main sequence stars to derive a statistical reddening correction for each object in the field. We then search for pre-main sequence (PMS) stars by looking for objects with a strong (>5 sigma) Halpha excess emission and find about 1200 of them over the entire field. Comparison of their location in the Hertzprung--Russell diagram with theoretical PMS evolutionary tracks for the appropriate metallicity reveals that about one third of these objects have an age of < 3 Myr, compatible with that of the massive stars in the central ionising cluster R136, whereas the rest have ages up to 30 Myr, with a median of 10 Myr. This indicates that star formation has proceeded over an extended period of time, although we cannot discriminate between an extended episode and a series of short and frequent bursts that are not resolved in time. While the younger PMS population preferentially occupies the central regions of the cluster, older PMS objects are more uniformly distributed across the field and are remarkably few at the very centre of the cluster. We attribute this latter effect to photoevaporation of the older circumstellar discs caused by the massive ionising members of R136. This paper is based on Early Release Science observations made by the WFC3 Scientific Oversight Committee. We are grateful to the Director of the Space Telescope Science Institute for awarding Director's Discretionary time for this program.

  19. Recent results from the VLNDEF network

    NASA Astrophysics Data System (ADS)

    Capra, Alessandro; Zanutta, Antonio; Negusini, Monia; Gandolfi, Stefano; Sarti, Pierguido; Vittuari, Luca; Salvini, Francesco; Cianfarra, Paola; Sterzai, Paolo

    2013-04-01

    measurements, geomagnetic field measurements and other geophysical observations. The deformation patterns obtained with GPS observations over the VLNDEF network are coupled with the data acquired during the geological and geomorphological surveys; the set of observations is used to study the neo-tectonics of NVL. We present the most recent geodetic results derived from the VLNDEF GPS data set and a recent cinematic model of the whole area. We present the preliminary geoid model in the northern part of the network.

  20. Recent results from tokamak divertor plasma measurements

    SciTech Connect

    Allen, S.L.

    1996-05-01

    New diagnostics have been developed to address key divertor physics questions, including: target plate heat flux reduction by radiation, basic edge transport issues, and plasma wall interactions (PWI) such as erosion. A system of diagnostics measures the target plate heat flux (imaging IR thermography) and particle flux (probes, pressure and Penning gauges, and visible emission arrays). Recently, T{sub e},n{sub e}, and P{sub e} (electron pressure) have been measured in 2-D with divertor Thomson Scattering. During radiative divertor operation T{sub e} is less than 2 eV, indicating that new atomic processes are important. Langmuir probes measure higher T{sub e} in some cases. In addition, the measured P{sub e} near the separatrix at the target plate is lower than the midplane pressure, implying radial momentum transport. Bolometer arrays, inverted with reconstruction algorithms, provide the 2-D core and divertor radiation profiles. Spectroscopic measurements identify the radiating species and provide information on impurity transport; both absolute chordal measurements and tomographic reconstructions of images are used. Either intrinsic carbon or an inert species (e.g., injected Ne) are usually observed, and absolute particle inventories are obtained. Computer codes are both benchmarked with the experimental data and provide important consistency checks. Several techniques are used to measure fundamental plasma transport and fluctuations, including probes and reflectometry. PWI issues are studied with in-situ coupons and insertable samples (DiMES). Representative divertor results from DIII-D with references to results on other tokamaks will be presented.

  1. Recent results on hadron structure from COMPASS

    NASA Astrophysics Data System (ADS)

    Makke, Nour

    2016-05-01

    A review of the most recent measurements of longitudinal and transverse momentum dependent distributions and fragmentation functions accessed in the inclusive and the semi-inclusive deep inelastic scattering from COMPASS is given.

  2. Recent lattice QCD results on nucleon structure

    SciTech Connect

    Konstantinos Orginos

    2006-07-01

    I review recent developments in lattice calculations of nucleon structure. In particular, I cover the calculations of nucleon matrix elements related to generalized parton distribution functions, structure functions and form factors.

  3. Recent results on baryon production at PETRA

    SciTech Connect

    Wu, S.L.

    1982-01-01

    One of the recent excitements at PETRA is the observation of the copious production of baryons. About a year ago, TASSO observed the inclusive production of protons and antiprotons. More recently JADE confirmed the inclusive antiproton spectrum to about 1 GeV/c and also observed the inclusive anti ..lambda.. spectrum to about 1.4 GeV/c, while TASSO obtained the ..lambda.. and anti-..lambda.. spectrum all the way up 10 GeV/c in momentum.

  4. Report on recent results obtained in TCABR

    NASA Astrophysics Data System (ADS)

    Galvão, R. M. O.; Amador, C. H. S.; Baquero, W. A. H.; Borges, F.; Caldas, I. L.; Cuevas, N. A. M.; Duarte, V. N.; Elfimov, A. G.; Elizondo, J. I.; Fonseca, A. M. M.; Germano, T. M.; Grenfell, G. G.; Guimarães-Filho, Z. O.; Jeronimo, J. L.; Kuznetsov, Yu K.; Manrique, M. A. M.; Nascimento, I. C.; Pires, C. J. A.; Puglia, P. G. P.; Reis, A. P.; Ronchi, G.; Ruchko, L. F.; de Sá, W. P.; Sgalla, R. J. F.; Sanada, E. K.; Severo, J. H. F.; Theodoro, V. C.; Toufen, D. L.

    2015-03-01

    Recent results of experimental work and theoretical modeling carried out in the TCABR tokamak are reported on characterization of MHD instabilities, improved diagnostics of rotation of the plasma column, excitation of Alven global modes, identification of GAMs, and the effect of rotation on their behavior. Detailed measurements of edge electrostatic perturbations and of magnetic island evolution and rotation indicate that the edge turbulence is substantially affected by the islands growth, leading to a strong modulation of the edge particle losses at the same frequency of the MHD activity. Measurements with spatial resolution also show that the growth of the MHD activity is due to nonlinear coupling of magnetic islands with different poloidal mode numbers, which increases the impurity influx. A new system of data acquisition and processing of the TCABR plasma rotation diagnostic was implemented. The system is based upon a single monochromator coupled with six photomultipliers tubes and allows one toroidal and two poloidal simultaneous rotation measurements. The excitation of Global Alfven Waves - GAW has been investigated, using a new type of radio frequency amplifier. The GAW resonances are searched either by a pre-programmed density variation, at fixed generator frequency, or through three RF frequency sweeps from 2 to 4.5 MHz, at stationary density. GAW resonances have been found and their somewhat new characteristics are presented. The investigation of the effect of poloidal and toroidal rotation on the characteristics of the geodesic acoustic mode has been investigated, both theoretically and experimentally. It is found that the assumption of isothermal flux surfaces gives rise to a third branch of this mode. Detailed predictions coupled with experimental measurements are currently being carried out to investigate this question.

  5. Natural Time Analysis of Seismicity: Recent Results

    NASA Astrophysics Data System (ADS)

    Varotsos, P.; Uyeda, S.; Sarlis, N. V.; Skordas, E. S.; Nagao, T.; Kamogawa, M.

    2013-12-01

    Natural time analysis introduced almost a decade ago[1] may uncover novel dynamic features hidden in the time series of complex systems and has been applied[2] to diverse fields. For a time series comprising N events, the natural time for the occurrence of the k-th event of energy Qk is defined by χk=k/N and the analysis is made by studying the evolution of the pair (χk,pk ), where pk=Qk/ΣQn is the normalized energy. In natural time analysis of seismicity, the variance κ1 of natural time χ weighted for pk calculated from seismic catalogues serves as an order parameter [2]. The Japan seismic catalog was analyzed in natural time by employing a sliding natural time window of fixed length comprised of the number of events that would occur in a few months. This is a crucial time scale since it corresponds to the average lead time of the observed Seismic Electric Signals (SES) activities [2]. The following results are obtained: First, the fluctuations of the order parameter of seismicity exhibit [3] a clearly detectable minimum approximately at the time of the initiation of the pronounced SES activity observed [4] almost two months before the onset of the volcanic-seismic swarm activity in 2000 in the Izu Island region, Japan. This is the first time that before the occurrence of major earthquakes, anomalous changes are found to appear almost simultaneously in two different geophysical observables. Second, these two phenomena were shown to be also linked in space[3]. Third, minima of the order parameter fluctuations of seismicity were observed [5] a few months before all shallow earthquakes of magnitude 7.6 or larger that occurred from 1 January 1984 to 11 March 2011 (the day of the M9 Tohoku earthquake) in Japanese area. Among these minima, the minimum before the M9 Tohoku earthquake was the deepest. Additional recent results are forwarded which shed more light on the importance of the aforementioned minima for earthquake prediction purposes. [1] Varotsos, P. A

  6. Recent Electroweak Results from the Tevatron

    SciTech Connect

    Zhu, Junjie; /SUNY, Stony Brook

    2009-07-01

    W and Z bosons are mainly produced via quark-antiquark annihilations at the Fermilab Tevatron collider. Precision measurements with these gauge bosons provide us with high precision tests of the Standard Model (SM) as well as indirect search for possible new physics beyond the SM. I present the recent electroweak measurements related to single W, Z boson and diboson productions from the CDF and D0 experiments at the Fermilab Tevatron collider.

  7. Recent results from Super-Kamiokande

    SciTech Connect

    Himmel, Alexander; Collaboration: Super-Kamiokande Collaboration

    2014-06-24

    The Super-Kamiokande experiment has collected more than 11 live-years of atmospheric neutrino data. Atmospheric neutrinos cover a wide phase space in both energy and distance travelled, the parameters relevant for studying neutrino oscillations. We present here recent measurements of the three-flavor neutrino oscillation parameters using this atmospheric neutrino data, as well as new limits on mixing with a fourth sterile neutrino state.

  8. Some recent results on meson spectroscopy

    SciTech Connect

    Chung, S.U.

    1987-06-01

    A comparative survey of established meson states with the predictions of a q anti q (quarkonium) model by Godfrey and Isgur shows that most meson states are well described, from pion to UPSILON(6S). However, a number of states in the light- quark isoscalar sector are not predicted at all in their model, pointing to a need for glueballs, hybrids and multi-quark states to fully account for recently reported meson states. 48 refs.

  9. Recent results from the super EBIT

    SciTech Connect

    Marrs, R.E.

    1995-09-15

    The Super EBIT device at LLNL can produce and trap any highly charged ion at rest in the laboratory, including bare U{sup 92+} ions. Recently, the ionization cross sections for high-Z hydrogenlike ions have been measured for the first time, and measurements of the L-shell ionization cross sections for uranium ions are in progress. The two-electron contributions to the ground state energies of heliumlike ions have been directly measured using a novel technique, and spectra of 2s-2p transitions in highly ionized thorium and uranium have been used to test QED corrections to the energy levels of few electron high-Z ions. A new capability for the study of rare isotopes has been demonstrated. Ion cooling has been used to reduce the thermal broadening of x-ray emission lines to the point where natural line widths can be observed in some cases.

  10. Recent Experimental Results at General Fusion

    NASA Astrophysics Data System (ADS)

    Howard, Stephen

    2013-10-01

    Experiments relevant to MTF are underway at General Fusion in which self-confined Compact Toroid (CT) plasmas in a spheromak configuration are rapidly compressed. Plasma Injector 1 (PI-1) is a two stage Marshal gun with a conical accelerator, 5 meters long and 1.9 m diameter in formation where a high aspect ratio (4.4) spheromak is formed with λ = 9 m-1. CTs formed with Bp = 0.2 T, Te = 40 eV, and ne = 0.5×1020 m-3 when compressed (2x radial) reached Bp = 0.8 T, Te = 160 eV, ne = 4×1020 m-3 which is consistent with adiabatic compressional heating. A smaller device, the Magnetized Ring Test (MRT) can form a unity-aspect ratio CT of λ = 35 m-1 directly within an implodable cylindrical liner of aluminum. The MRT electrodes form a bow-tie cavity known for its high- β stability. MRT has begun a set of implosive compression tests to observe the behavior of a high density CT as it experiences increasing beta, possible interactions with the liner wall, and changing profiles as the compression proceeds. Progress is being made to understand losses during compression via analysis of magnetic fluctuations, spectroscopy, and comparison to 3D MHD simulation.

  11. Language and counting: Some recent results

    NASA Astrophysics Data System (ADS)

    Bell, Garry

    1990-02-01

    It has long been recognised that the language of mathematics is an important variable in the learning of mathematics, and there has been useful work in isolating and describing the linkage. Steffe and his co-workers at Georgia, for example, (Steffe, von Glasersfeld, Richardson and Cobb, 1983) have suggested that young children may construct verbal countable items to count objects which are hidden from their view. Although there has been a surge of research interest in counting and early childhood mathematics, and in cultural differences in mathematics attainment, there has been little work reported on the linkage between culture as exemplified by language, and initial concepts of numeration. This paper reports on some recent clinical research with kindergarten children of European and Asian background in Australia and America. The research examines the influence that number naming grammar appears to have on young children's understandings of two-digit numbers and place value. It appears that Transparent Standard Number Word Sequences such as Japanese, Chinese and Vietnamese which follow the numerical representation pattern by naming tens and units in order ("two tens three"), may be associated with distinctive place value concepts which may support sophisticated mental algorithms.

  12. Vanadium alloys - overview and recent results

    NASA Astrophysics Data System (ADS)

    Muroga, T.; Nagasaka, T.; Abe, K.; Chernov, V. M.; Matsui, H.; Smith, D. L.; Xu, Z.-Y.; Zinkle, S. J.

    2002-12-01

    This paper reviews recent progress in research on vanadium alloys with emphasis on V-4Cr-4Ti as a reference composition. New high purity V-4Cr-4Ti ingots and products (NIFS-HEATs) were made. The improved purity of the alloys made a practical demonstration of enhanced feasibility of recycling as a method of handling after use in fusion reactors. Significant progress has been made in the understanding of physical metallurgy of V-4Cr-4Ti and effects of O, N and C on the alloy properties such as low and high temperature mechanical properties, welding properties and low temperature irradiation effects, by means of including the comparison of various large heats and model alloys with different impurity levels. The effects of other trace impurities on some of the properties are also discussed. Other current efforts to characterize V-4Cr-4Ti, to improve its properties and to explore advanced vanadium alloys are reviewed. Issues remaining for the future investigations are discussed.

  13. Recent results from the ANTARES neutrino telescope

    NASA Astrophysics Data System (ADS)

    Van Elewyck, Véronique

    2014-04-01

    The ANTARES neutrino telescope is currently the largest operating water Cherenkov detector and the largest neutrino detector in the Northern Hemisphere. Its main scientific target is the detection of high-energy (TeV and beyond) neutrinos from cosmic accelerators, as predicted by hadronic interaction models, and the measurement of the diffuse neutrino flux. Its location allows for surveying a large part of the Galactic Plane, including the Galactic Centre. In addition to the standalone searches for point-like and diffuse high-energy neutrino signals, ANTARES has developed a range of multi-messenger strategies to exploit the close connection between neutrinos and other cosmic messengers such as gamma-rays, charged cosmic rays and gravitational waves. This contribution provides an overview of the recently conducted analyses, including a search for neutrinos from the Fermi bubbles region, searches for optical counterparts with the TAToO program, and searches for neutrinos in correlation with gamma-ray bursts, blazars, and microquasars. Further topics of investigation, covering e.g. the search for neutrinos from dark matter annihilation, searches for exotic particles and the measurement of neutrino oscillations, are also reviewed.

  14. Recent Radiation Test Results for Power MOSFETs

    NASA Technical Reports Server (NTRS)

    Lauenstein, Jean-Marie; Topper, Alyson D.; Casey, Megan C.; Wilcox, Edward P.; Phan, Anthony M.; Kim, Hak S.; LaBel, Kenneth A.

    2013-01-01

    Single-event effect (SEE) and total ionizing dose (TID) test results are presented for various hardened and commercial power metal-oxide-semiconductor field effect transistors (MOSFETs), including vertical planar, trench, superjunction, and lateral process designs.

  15. Stitching interferometry: recent results and absolute calibration

    NASA Astrophysics Data System (ADS)

    Bray, Michael

    2004-02-01

    Stitching Interferometry is a method of analysing large optical components using a standard "small" interferometer. This result is obtained by taking multiple overlapping images of the large component, and numerically "stitching" these sub-apertures together. We have already reported the industrial use our Stitching Interferometry systems (Previous SPIE symposia), but experimental results had been lacking because this technique is still new, and users needed to get accustomed to it before producing reliable measurements. We now have more results. We will report user comments and show new, unpublished results. We will discuss sources of error, and show how some of these can be reduced to arbitrarily small values. These will be discussed in some detail. We conclude with a few graphical examples of absolute measurements performed by us.

  16. Recent cusp and cleft results from interball

    NASA Astrophysics Data System (ADS)

    Sandahl, Ingrid

    The Interball project has given important contributions to our understanding of the morphology and the physical processes in the cusp and cleft. Interball Tail and Magion-4 have performed more extensive measurements in the high altitude cusp than any previous spacecraft. Interball has also been a part in the ISTP program and data have been used in many multipoint studies. In this paper recent cusp and cleft studies based entirely or partly on Interball data will be reviewed. Interball data show that processes at high latitudes are very important for plasma entry into the magnetosphere. A case study for southward IMF conditions agrees with a model in which the mantle is populated via entry along open high-latitude field lines. A statistical study of events dominated by IMF B y shows that merging in anti-parallel fields, rather than subsolar point reconnection, populates the mantle. Plasma entry also takes place through the turbulent boundary layer, TBL, a region of strong, Alfvenic ULF turbulence above the cusp and cleft. The TBL is almost always present. It extends tailward from the cusp and is proposed to be related to the magnetospheric sash. For the overall magnetosheath plasma entry into the magnetosphere the magnetotail boundary is probably more important than the cusp. The position of the cusp is controlled by the solar wind in a similar way as the low altitude cusp. The mid-altitude cusp was found to maintain its fine structure over periods of the order of one hour. A suprathermal proton population not previously described has been detected in the mid-altitude cusp.

  17. Recent results from COMPASS on exclusive muoproduction

    NASA Astrophysics Data System (ADS)

    Sandacz, Andrzej

    2016-02-01

    The 160 GeV polarised muon beam available at CERN, with positive or negative charge, makes COMPASS a unique place for GPD studies. The first GPD related COMPASS results come from exclusive vector meson production on transversely polarised protons and deuterons. The data were taken in 2003-2010 with large solid-state polarised targets, although without detection of recoil particles. Results on various transverse target spin dependent azimuthal asymmetries are presented and their relations to GPDs are discussed. The dedicated COMPASS GPD program started in 2012 with commissioning of a new long liquid hydrogen target and new detectors such as the large recoil proton detector and the large-angle electromagnetic calorimeter. It was followed by a short pilot 'DVCS run'. The performance of the setup and first results on DVCS and exclusive π0 channels have been demonstrated. The full data taking for the GPD program approved within COMPASS-II proposal is planned for 2016 and 2017.

  18. Recent results for the Raytheon RELI program

    NASA Astrophysics Data System (ADS)

    Filgas, David; Clatterbuck, Todd; Cashen, Matt; Daniele, Andrew; Hughes, Steve; Mordaunt, David

    2012-06-01

    We describe our approach and latest results for Raytheon's RELI (Robust Electric Laser Initiative) program. Our architecture leverages a slab-based, Master Oscillator / Power Amplifier (MOPA) architecture based on Raytheon's unique planar waveguide amplifier. Technical objectives for this effort are to demonstrate > 25 kW output with excellent beam quality and an electrical to optical efficiency > 30%. The planar waveguide architecture provides compact packaging and is inherently scalable to 100 kW or greater in a single beam line. We report on the latest progress and test results for the program.

  19. Recent results from the HERMES experiment.

    SciTech Connect

    Jackson, H. E.; HERMES Collaboration

    2010-01-01

    Results are presented from the Hermes experiment which uses semi-inclusive deep inelastic lepton scattering to study the flavor structure of the nucleon. Data have been accumulated for pion and kaon double spin asymmetries, single-spin azimuthal asymmetries for meson electroproduction, deep virtual Compton scattering (DVCS), and meson multiplicities. These results provide information on the properties of the strange sea in the proton, constraints on transverse momentum dependent quark parton distributions, and demonstrate the promise of DVCS for isolating the total angular momentum carried by the quarks in the proton.

  20. Recent results from the Hubble Space Telescope

    NASA Astrophysics Data System (ADS)

    Maran, Stephen P.; Kinney, Anne L.

    1993-05-01

    The present survey of observational results from the HST supplements the earlier presentation by Kinney and Maran (1991), and encompasses such noteworthy achievements as the first UV results from the High Speed Photometer and spectroscopic studies of black hole/neutron-star binaries and a flare star. New data are also presented for the intergalactic absorption clouds along various lines-of-sight and imaging observations of planetary nebulae in the Magellanic Clouds. An animated sequence derived from images showing the evolution of a great storm on Saturn is noted to be of especially far-ranging relevance.

  1. Recent results from the Hubble Space Telescope

    NASA Technical Reports Server (NTRS)

    Maran, Stephen P.; Kinney, Anne L.

    1993-01-01

    The present survey of observational results from the HST supplements the earlier presentation by Kinney and Maran (1991), and encompasses such noteworthy achievements as the first UV results from the High Speed Photometer and spectroscopic studies of black hole/neutron-star binaries and a flare star. New data are also presented for the intergalactic absorption clouds along various lines-of-sight and imaging observations of planetary nebulae in the Magellanic Clouds. An animated sequence derived from images showing the evolution of a great storm on Saturn is noted to be of especially far-ranging relevance.

  2. Results from recent NASA tire thermal studies

    NASA Technical Reports Server (NTRS)

    Mccarty, J. L.

    1983-01-01

    The testing technique and some results from an experimental study to determine tire temperature profiles to aid in defining the strength and fatigue limitations of the tire carcass structure are described. This effort is part of a program to explore analytically and through experiment the temperature distribution in an aircraft tire during free roll and braked and yawed rolling conditions.

  3. Recent results from Fermilab E791

    NASA Astrophysics Data System (ADS)

    Nguyen, A.; Aitala, E. M.; Amato, S.; Anjos, J. C.; Appel, J. A.; Aryal, M.; Ashery, D.; Banerjee, S.; Bediaga, I.; Blaylock, G.; Bracker, S. B.; Burchat, P. R.; Burnstein, R. A.; Carter, T.; Carvalho, H. S.; Costa, I.; Cremaldi, L. M.; Darling, C.; Denisenko, K.; Dubbs, T.; Fernandez, A.; Gagnon, P.; Gerson, S.; Gounder, K.; Granite, D.; Halling, M.; Herrera, G.; Hurwitz, G.; James, C.; Kasper, P. A.; Kwan, S.; Langs, D. C.; Leslie, J.; Lichtenstadt, J.; Lundberg, B.; MayTal-Beck, S.; Meadows, B.; de Mello Neto, J. R. T.; Milburn, R. H.; de Miranda, J. M.; Napier, A.; d'Oliveira, A. B.; Peng, K. C.; Perera, L. P.; Purohit, M. V.; Quinn, B.; Radeztsky, S.; Rafatian, A.; Reay, N. W.; Reidy, J. J.; dos Reis, A. C.; Rubin, H. A.; Santha, A. K. S.; Santoro, A. F. S.; Schwartz, A.; Sheaff, M.; O'Shaughnessy, K.; Sidwell, R. A.; Slaughter, A. J.; Smith, J. G.; Sokoloff, M. D.; Stanton, N.; Sugano, K.; Summers, D. J.; Takach, S.; Thorne, K.; Tripathi, A. K.; Watanabe, S.; Weiss, R.; Wiener, J.; Witchey, N.; Wolin, E.; Yi, D.; Zaliznyak, R.; Zhang, C.

    1995-07-01

    Fermilab E791 is a high statistics charm experiment using a 500 GeV/c π- beam incident on a segmented target. We present results based on one third of the 1991-1992 data, with particular emphasis on a search for the flavor changing neutral current decay D+→π+μ+μ-.

  4. An Overview of Recent Results from CLAS

    SciTech Connect

    Kenneth Hicks

    2011-12-01

    The unique capabilities of the CLAS detector to measure exclusive meson electroproduction off protons, with almost complete coverage of the final hadron phase space, has extended our knowledge of excited baryon structure. Consistent results from Np and Npp final states provide convincing evidence for reliable extraction of N* electrocouplings. Theoretical analyses of these results, using self-consistent dynamical calculations using an internal quark core and an external meson-baryon cloud suggest that meson-baryon dressing amplitudes need to be included. The meson-baryon dressing was already shown to be necessary to get agreement between calculations and data on the D resonance transition magnetic moment at low Q{sup 2}. Similarly, a new measurement of the transition magnetic moment for strange baryons also disagrees with quark models, suggesting the need for meson-baryon dressings. In the near future, the CLAS detector will be replaced with CLAS12, providing new high-precision data.

  5. Recent results of the ANTARES neutrino telescope

    SciTech Connect

    Hernández-Rey, Juan José

    2015-07-15

    The latest results from the ANTARES Neutrino Telescope are reported. Limits on a high energy neutrino diffuse flux have been set using for the first time both muon–track and showering events. The results for point sources obtained by ANTARES are also shown. These are the most stringent limits for the southern sky for neutrino energies below 100 TeV. Constraints on the nature of the cluster of neutrino events near the Galactic Centre observed by IceCube are also reported. In particular, ANTARES data excludes a single point–like neutrino source as the origin of this cluster. Looking for neutrinos coming from the Sun or the centre of the Galaxy, very competitive limits are set by the ANTARES data to the flux of neutrinos produced by self-annihilation of weakly interacting massive particles.

  6. Recent Results from KMAX tandem mirror experiment

    NASA Astrophysics Data System (ADS)

    Sun, Xuan; Luo, M.; Zhang, Q.; Lin, M.; Shi, P.

    2015-11-01

    KMAX, Keda Mirror with AXisymmeticity, is a tandem mirror machine with a length of ~ 10 meters and diameters of 1.2 meters in the central cell and 0.3 meters in the mirror throat. As a versatile plasma experimental platform, KMAX is currently conducting experiments on the Alfven wave launching, electrode biasing, radio frequency heating and etc. The latest results will be presented. In the experiment of Alfven wave launching, we observed the shear Alfven waves decay into the forward and backward propagating compressional waves. And in the bias experiment we successfully extracted plasma current up to 0.5kA with biasing voltage of ~ 1kV. During biasing, the plasma density and temperature have siginificantly increasing. Preliminary results on the radio frequency heating will also be presented.

  7. Recent results from CERN-WA98

    SciTech Connect

    Stankus, P.; WA98 Collaboration

    1997-02-01

    The CERN experiment WA98 is a general-survey, open-spectrometer experiment designed to examine 160 A GeV/c Pb+A collisions at the CERN-SPS. The experiment has a broad physics agenda, as suggested by its many different subsystems. A diagram of the experiment as it stood in 1995 is shown in the report. Detectors whose results are presented here are described briefly.

  8. Recent Results from Fermilab E690

    SciTech Connect

    Berisso, M.C.; Christian, D.C.; Felix, J.; Gara, A.; Gottschalk, E.; Gutierrez, G.; Hartouni, E.P.; Knapp, B.C.; Kreisler, M.N.; Lee, S.; Markianos, K.; Moreno, G.; Reyes, M.A.; Sosa, M.; Wang, M.H.L.S.; Wehmann, A.; Wesson, D.

    1998-01-01

    Partial wave analysis results of centrally produced mesons in the reaction pp {yields} P{sub slow}(X)P{sub fast}, with 800 GeV/c protons incident on a liquid hydrogen target are presented. In the reactions considered in this paper the (X) system decays into: a) K{sup 0}{sub s}K{sup {+-}}{pi}{sup {-+}}, b) K{sub s}K{sub s}, and c) {pi}{sup +}{pi}{sup -}.

  9. Recent results from the DREAM project

    NASA Astrophysics Data System (ADS)

    Wigmans, Richard

    2009-04-01

    The aim of the DREAM project is to develop calorimeters that are able to measure the four-vectors of all fundamental constituents of matter, including fragmenting quarks, with a precision of 1% or better. To achieve this, the factors that limit the performance of the present generation of calorimeters are eliminated one by one, in the order at which these factors dominate. In this talk, I give an overview of the results achieved so far, and outline our plans for the future.

  10. Recent results from Daya Bay experiment

    NASA Astrophysics Data System (ADS)

    Naumov, Dmitry V.

    2015-05-01

    This manuscript is a short summary of my talk given at ICNFP2014 Conference. Here we report on new results of sin2 2θ13 and Δm2ee measurements, search for the sterile neutrino within 10-3 eV2 < Δm241 < 0.1 eV2 domain and precise measurement of the reactor absolute antineutrino flux.

  11. Recent Results from the MERIT Experiment

    NASA Astrophysics Data System (ADS)

    Kirk, H. G.

    2010-03-01

    MERIT is a proof-of-principle experiment which demonstrates the key target concepts for the production of muons required for a muon collider or a neutrino factory. The experiment was run at CERN utilizing 14 and 24 GeV proton beams from the PS. The key elements of the experiment include the impact of the proton beam with a free flowing mercury jet within the confines of a 15-T solenoid field. Results from the experiment are reported.

  12. Recent results from the Telescope Array Experiment

    NASA Astrophysics Data System (ADS)

    Abbasi, Rasha; Telescope Array Collaboration

    2016-03-01

    The Telescope Array (TA) is the largest ultrahigh energy cosmic rays detector in the northern hemisphere. TA is a hybrid detector comprised of three air fluorescence stations and a large surface array consisting of 507 scintillator counters. Each of the three fluorescence stations, located at the periphery of the ground array, views 108 degrees in azimuth and up to 30 degrees in elevation. The surface detectors are arranged in a square grid of 1.2 km spacing, covering over 700 square kilometers. TA has collected more than seven years of data. In this talk, we will present some of the main results on the cosmic rays composition and energy spectrum obtained by TA and its low energy extension (TALE). Finally, we will present our results from the search for arrival direction anisotropy, including the observed large excess of events at the highest energies, seen in the region of the northern sky centered on Ursa Major. Based on the current results, the ``hot spot'' in particular, TA is pursuing the expansion of the surface array to four times its current size.

  13. Recent Results of the Telescope Array Experiment

    NASA Astrophysics Data System (ADS)

    Ivanov, Dmitri

    2015-04-01

    The Telescope Array (TA) is the largest cosmic ray experiment in the northern hemisphere and covers 10 PeV to 100 EeV range. TA is a hybrid detector that uses air fluorescence detectors combined with a ground array. TA consists of 507 plastic scintillation counters on a 1.2km square grid, overlooked by 3 fluorescence detector stations, and measures cosmic rays above 1 EeV. TA has collected 6.5 years of data. Results from the TA low energy extension (TALE), which sees cosmic rays down to 10 PeV, will also be shown. This contribution will consist of three parts. First, we will present the cosmic ray energy spectrum measured over 4 decades in energy. Next, we will discuss the latest results of the measurements of cosmic ray mass composition by the TA fluorescence detectors. Finally, we will show the latest results of the TA anisotropy measurements at the highest energies, where we have seen a concentration of events, called the ``hotspot,'' centered in the Ursa Major. For the Telescope Array Collaboration. Done...processed 1261 records...10:46:59 Beginning APS data extraction...10:47:48

  14. Recent Results of the CMS Experiment

    NASA Astrophysics Data System (ADS)

    Dorigo, Tommaso

    2014-04-01

    The CMS experiment obtained a large number of groundbreaking results from the analysis of 7- and 8-TeV proton-proton collisions produced so far by the Large Hadron Collider at CERN. In this brief summary only a sample of those results will be discussed. A new particle with mass mH = 125.3 ± 0.4(stat.) ± 0.5(syst.) GeV and characteristics compatible with those expected for a standard model Higgs boson has been observed in its decays to photon pairs, WW pairs, and ZZ pairs. Searches for the rare decays Bd → µµ and Bs → µµ have allowed to set limits on the branching fractions which are close to standard model predictions, strongly constraining new physics models. The top quark has been studied with great detail, obtaining among other results the world's best measurement of its mass as Mt = 173.49 ± 0.43(stat. + JES ) ± 0.98(syst.) GeV. New physics models have been strongly constrained with the available data.

  15. Recent JET results and future prospects

    SciTech Connect

    Rebut, P.H.

    1990-01-01

    The latest results of JET plasmas in transient and steady states are presented. Substantial improvements in plasma purity and corresponding reductions in plasma dilution have resulted from the use of beryllium as the first wall material facing the hot plasma. As a consequence, plasmas with a fusion triple product (n{sub D}(0){tau}{sub E}T{sub i}(0)) in the range 8--9 {times} 10{sup 20} m{sup {minus}3} skeV have been achieved (within a factor of 8 that required in a fusion reactor), albeit under transient conditions. The general JET performance has also improved, allowing the parameters of a reactor plasma to be individually achieved in JET. In view of their importance for reactors, the JET results are presented with particular emphasis on their significance for the formulation of a plasma model for the Next Step. However, impurity influxes limit the attainment of better parameters and prevent the realization of steady state conditions at high heating powers. To address these problems of impurity control, plasma fueling and helium ash exhaust, a New Phase is planned for JET. An axisymmetric pumped divertor configuration will allow operating conditions close to those of a reactor. The divertor configuration should demonstrate a concept of impurity control and determine the size and geometry needed to fulfill this concept in a reactor. It should identify appropriate materials for plasma facing components and define the operational domain for the Next Step.

  16. Recent results on meson spectroscopy from JETSET

    SciTech Connect

    Evangelista, C.; Palano, A.; Drijard, D.; Ferro-Luzzi, M.; Hamann, N.; Moueellie, B.; Ohlsson, S.; Perreau, J.M.; Price, M.; Eyrich, W.

    1994-09-01

    The JETSET experiment at CERN LEAR studies the process p{bar p} {yields} {phi}{phi} {yields} K{sup +}K{sup {minus}}K{sup +}K{sup {minus}} to search for hadronic resonances. {phi}{phi} are directly formed through the annihilation of an antiproton beam onto an internal-jet target. Preliminary results on the {phi}{phi} cross section in the energy range 2.1-2.4 GeV/c are presented from data taken in 1991. 19 refs., 18 figs.

  17. Recent Physics Results with the COMPASS Experiment

    SciTech Connect

    Paul, Stephan

    2006-02-11

    The COMPASS experiment has obtained first physics results in the field of polarized distribution functions for quarks and gluons using muon scattering off polarized deuterons. The analysis using open charm production and pairs of high pT hadrons is presented. We also have used a transversely polarized target to address transverse information for quarks inside the nucleon. In addition, a pilot run with incoming pions taken late 2004 will give first information on the pion polarizabilities and hadron resonances. The physics prospects from this run as well as from future data taking in this field are also outlined.

  18. Recent results from PHOBOS at RHIC

    NASA Astrophysics Data System (ADS)

    Back, B. B.; Baker, M. D.; Barton, D. S.; Betts, R. R.; Ballintijn, M.; Bickley, A. A.; Bindel, R.; Budzanowski, A.; Busza, W.; Carroll, A.; Decowski, M. P.; García, E.; George, N.; Gulbrandsen, K.; Gushue, S.; Halliwell, C.; Hamblen, J.; Heintzelman, G. A.; Henderson, C.; Hofman, D. J.; Hollis, R. S.; Hołyński, R.; Holzman, B.; Iordanova, A.; Johnson, E.; Kane, J. L.; Katzy, J.; Khan, N.; Kucewicz, W.; Kulinich, P.; Kuo, C. M.; Lin, W. T.; Manly, S.; McLeod, D.; Michałowski, J.; Mignerey, A. C.; Nouicer, R.; Olszewski, A.; Pak, R.; Park, I. C.; Pernegger, H.; Reed, C.; Remsberg, L. P.; Reuter, M.; Roland, C.; Roland, G.; Rosenberg, L.; Sagerer, J.; Sarin, P.; Sawicki, P.; Skulski, W.; Steadman, S. G.; Steinberg, P.; Stephans, G. S. F.; Stodulski, M.; Sukhanov, A.; Tang, J.-L.; Teng, R.; Trzupek, A.; Vale, C.; van Niewwenhuizen, G. J.; Verdier, R.; Wadsworth, B.; Wolfs, F. L. H.; Wosiek, B.; Woźniak, K.; Wuosmaa, A. H.; Wysłouch, B.; Robert PakThe Phobos Collaboration

    2003-06-01

    The PHOBOS experiment at RHIC has recorded measurements for AuAu collisions spanning nucleon-nucleon center-of-mass energies from √ SNN = 19.6 GeV to 200 GeV. Global observables such as elliptic flow and charged particle multiplicity provide important constraints on model predictions that characterize the state of matter produced in these collisions. The nearly 4π acceptance of the PHOBOS experiment provides excellent coverage for complete flow and multiplicity measurements. Results including beam energy and centrality dependencies are presented and compared to elementary systems.

  19. Recent results from experiments at MAMI

    NASA Astrophysics Data System (ADS)

    Müller, U.

    2012-04-01

    The Mainz Microtron MAMI is an ideal tool for studying the structure of strongly interacting systems with an electromagnetic probe. With the new HDSM accelerator stage of MAMI C, a continuous-wave electron beam with an energy of up to 1604 MeV and excellent beam quality is available for precision experiments. In addition, polarisation degrees of freedom can be exploited with polarised beams and either polarised targets or recoil polarimetry. This paper presents selected results of the A1, A2, and A4 collaborations.

  20. Recent results from the OPERA experiment

    SciTech Connect

    Meregaglia, Anselmo

    2009-04-17

    OPERA is a long-baseline neutrino oscillation experiment whose main goal is to detect for the first time neutrino oscillations in an appearance mode. Using an almost pure v{sub {mu}} beam we search for a v{sub {mu}}{r_reversible}v{sub {tau}}, transition detecting in a direct way the {tau} lepton. The detector is located on the high-energy, long-baseline CERN to LNGS beam (CNGS) at a baseline of 730 km. The apparatus consists of a target made of lead/emulsion-films bricks and of electronic detectors which are used to tag the neutrino interaction. Experiment description and results from the short but fruitful 2007 CNGS run are reported in details.

  1. Recent results from the OPERA experiment

    NASA Astrophysics Data System (ADS)

    Meregaglia, Anselmo

    2009-04-01

    OPERA is a long-baseline neutrino oscillation experiment whose main goal is to detect for the first time neutrino oscillations in an appearance mode. Using an almost pure vμ beam we search for a vμ<-->vτ, transition detecting in a direct way the τ lepton. The detector is located on the high-energy, long-baseline CERN to LNGS beam (CNGS) at a baseline of 730 km. The apparatus consists of a target made of lead/emulsion-films bricks and of electronic detectors which are used to tag the neutrino interaction. Experiment description and results from the short but fruitful 2007 CNGS run are reported in details.

  2. Recent Results of the Opera Experiment

    NASA Astrophysics Data System (ADS)

    Pupilli, F.

    2014-06-01

    The OPERA experiment aims at the direct confirmation of the leading oscillation mechanism in the atmospheric sector looking for the appearance of ντ in an almost pure νμ beam (the CERN CNGS beam). In five years of physics run the experiment collected 17.97 × 1019 p.o.t. The detection of τS produced in ντ CC interactions and of their decays is accomplished exploiting the high spatial resolution of nuclear emulsions. Furthermore OPERA has good capabilities in detecting electron neutrino interactions, setting limits on the νμ → νℯ oscillation channel. In this talk the status of the analysis will be presented together with updated results on both oscillation channels.

  3. Numerical simulations of catastrophic disruption: Recent results

    NASA Technical Reports Server (NTRS)

    Benz, W.; Asphaug, E.; Ryan, E. V.

    1994-01-01

    Numerical simulations have been used to study high velocity two-body impacts. In this paper, a two-dimensional Largrangian finite difference hydro-code and a three-dimensional smooth particle hydro-code (SPH) are described and initial results reported. These codes can be, and have been, used to make specific predictions about particular objects in our solar system. But more significantly, they allow us to explore a broad range of collisional events. Certain parameters (size, time) can be studied only over a very restricted range within the laboratory; other parameters (initial spin, low gravity, exotic structure or composition) are difficult to study at all experimentally. The outcomes of numerical simulations lead to a more general and accurate understanding of impacts in their many forms.

  4. Entropy of balance - some recent results

    PubMed Central

    2010-01-01

    Background Entropy when applied to biological signals is expected to reflect the state of the biological system. However the physiological interpretation of the entropy is not always straightforward. When should high entropy be interpreted as a healthy sign, and when as marker of deteriorating health? We address this question for the particular case of human standing balance and the Center of Pressure data. Methods We have measured and analyzed balance data of 136 participants (young, n = 45; elderly, n = 91) comprising in all 1085 trials, and calculated the Sample Entropy (SampEn) for medio-lateral (M/L) and anterior-posterior (A/P) Center of Pressure (COP) together with the Hurst self-similariy (ss) exponent α using Detrended Fluctuation Analysis (DFA). The COP was measured with a force plate in eight 30 seconds trials with eyes closed, eyes open, foam, self-perturbation and nudge conditions. Results 1) There is a significant difference in SampEn for the A/P-direction between the elderly and the younger groups Old > young. 2) For the elderly we have in general A/P > M/L. 3) For the younger group there was no significant A/P-M/L difference with the exception for the nudge trials where we had the reverse situation, A/P < M/L. 4) For the elderly we have, Eyes Closed > Eyes Open. 5) In case of the Hurst ss-exponent we have for the elderly, M/L > A/P. Conclusions These results seem to be require some modifications of the more or less established attention-constraint interpretation of entropy. This holds that higher entropy correlates with a more automatic and a less constrained mode of balance control, and that a higher entropy reflects, in this sense, a more efficient balancing. PMID:20670457

  5. GERDA: Recent results and future plans

    NASA Astrophysics Data System (ADS)

    Lehnert, Björn

    2014-04-01

    The GERmanium Detector Array (GERDA) is an experiment designed to investigate the neutrinoless double beta decay (0 νββ) in 76Ge. An array of high purity germanium detectors isotopically enriched to 87% of 76Ge is operated within 64 m3 of liquid argon (LAr) at the Laboratori Nazionali del Gran Sasso (LNGS). The experiment aims to explore the 0 νββ half-life up to 1.4×1026 yr with a collected exposure of 100 kg yr separated into two physics phases. The data taking of Phase I started in November 2011 and finished in May 2013 with 21.6 kg yr of exposure and a background index (BI) of 2×10-2cts/(kg yr keV) around the Q-value of 2039 keV before pulse shape cuts. Phase II of the experiment is being prepared with additional 30 Broad Energy Germanium (BEGe) detectors and an instrumentation of the LAr, aiming at a BI reduction by a factor of 10 w.r. to Phase I. This paper will present the GERDA setup and the latest results of the experiment including a new measurement of the 2 νββ spectrum of 76Ge and the decomposition of the background spectrum. The 0 νββ analysis, finished in the meanwhile, will be briefly mentioned. Furthermore, the major improvements planned for Phase II will be discussed.

  6. Recent COMPASS results on the gluon polarization

    SciTech Connect

    Quintans, Catarina

    2009-03-23

    The spin structure of the nucleon is studied in the COMPASS experiment at CERN/SPS, from the collisions of 160 GeV polarized muon beam with a {sup 6}LiD target. The data collected from 2002 to 2006 provide an accurate measurement of longitudinal double spin cross-section asymmetries. The latest results on the gluon polarization, accessed from two independent analyses of photon-gluon fusion selected events, are presented. The study of the open-charm production allows to extract the gluon polarization (in LO QCD) from the measurement of the asymmetry, the value obtained being {delta}g/g -0.49{+-}0.27(stat){+-}0.11(syst), at an average x{sub g} 0.11{sub -0.05}{sup +0.11} and a scale <{mu}{sup 2}> = 13(GeV/c){sup 2}. An alternative and independent way to study the gluon polarization, by studying the high transverse momentum hadron pairs produced, leads to a value {delta}g/g 0.08{+-}0.10(stat){+-}0.05(syst), at x{sub g}{sup a{nu}} 0.082{sub -0.027}{sup +0.041} and <{mu}{sup 2}> = 3(GeV/c){sup 2}.

  7. Recent results of the SPHINX Collaboration

    SciTech Connect

    Landsberg, L. G.

    1998-05-29

    The results of the first stage of the experiments with the SPHINX facility are presented. In these experiments several diffractive production processes in a 70 GeV proton beam of the IHEP accelerator were studied. The evidence for new baryon states with masses {>=}2 GeV is obtained in the hyperon-kaon effective mass spectra in the coherent reactions p+C{yields}|{sigma}(1385){sup 0}K{sup +}|+C and p+C{yields}|{sigma}{sup 0}K{sup +}|+C. The unusual features of these massive states (small enough decay widths, large branching ratios for decays with strange particles in final states) make them serious candidates for cryptoexotic pentaquark baryons with hidden strangeness. Preliminary data for p+N reactions in nonperipheral region with transverse momenta square >0.3 GeV{sup 2} (the mass spectra M({sigma}{sup 0}K{sup +}), M|p{eta}| and M|p{eta}{sup '}|) are also presented in this talk.

  8. Recent results from the LHCf experiment

    NASA Astrophysics Data System (ADS)

    Tiberio, A.; Adriani, O.; Berti, E.; Bonechi, L.; Bongi, M.; Castellini, G.; D'Alessandro, R.; Del Prete, M.; Haguenauer, M.; Itow, Y.; Kasahara, K.; Kawade, K.; Makino, Y.; Masuda, K.; Matsubayashi, E.; Menjo, H.; Mitsuka, G.; Muraki, Y.; Papini, P.; Perrot, A.-L.; Pfeiffer, D.; Ricciarini, S.; Sako, T.; Sakurai, N.; Shimizu, Y.; Sugiura, Y.; Suzuki, T.; Tamura, T.; Torii, S.; Tricomi, A.; Turner, W. C.; Zhou, Q.

    2015-06-01

    The LHC-forward (LHCf) experiment, situated at the LHC accelerator, has measured neutral particles production in a very forward region (pseudo-rapidity > 8.4) in proton-proton and proton-lead collisions. The main purpose of the LHCf experiment is to test hadronic interaction models used in cosmic rays experiments to imulate cosmic rays induced air-showers in Earth's atmosphere. The experiment is composed of two independent detectors located at 140m from the ATLAS interaction point (IP1) on opposite sides ; each detector is composed of two sampling calorimeters. Latest physics results from p-p and p-Pb collisions (at √s = 7 TeV and 5.02 TeV respectively) will be discussed in this paper ; in particular, the inclusive energy spectra of neutrons in p-p collisions and the transverse momentum spectra of neutral pions for different pseudo-rapidity ranges in p-Pb collisions will be shown.

  9. Recent Results for the ECHo Experiment

    NASA Astrophysics Data System (ADS)

    Hassel, C.; Blaum, K.; Goodacre, T. Day; Dorrer, H.; Düllmann, Ch. E.; Eberhardt, K.; Eliseev, S.; Enss, C.; Filianin, P.; Fäßler, A.; Fleischmann, A.; Gastaldo, L.; Goncharov, M.; Hengstler, D.; Jochum, J.; Johnston, K.; Keller, M.; Kempf, S.; Kieck, T.; Köster, U.; Krantz, M.; Marsh, B.; Mokry, C.; Novikov, Yu. N.; Ranitzsch, P. C. O.; Rothe, S.; Rischka, A.; Runke, J.; Saenz, A.; Schneider, F.; Scholl, S.; Schüssler, R. X.; Simkovic, F.; Stora, T.; Thörle-Pospiech, P.; Türler, A.; Veinhard, M.; Wegner, M.; Wendt, K.; Zuber, K.

    2016-02-01

    The Electron Capture in ^{163} Ho experiment, ECHo, is designed to investigate the electron neutrino mass in the sub-eV range by means of the analysis of the calorimetrically measured spectrum following the electron capture (EC) in ^{163} Ho. Arrays of low-temperature metallic magnetic calorimeters (MMCs), read-out by microwave SQUID multiplexing, will be used in this experiment. With a first MMC prototype having the ^{163} Ho source ion-implanted into the absorber, we performed the first high energy resolution measurement of the EC spectrum, which demonstrated the feasibility of such an experiment. In addition to the technological challenges for the development of MMC arrays, which preserve the single pixel performance in terms of energy resolution and bandwidth, the success of the experiment relies on the availability of large ultra-pure ^{163} Ho samples, on the precise description of the expected spectrum, and on the identification and reduction of background. We present preliminary results obtained with standard MMCs developed for soft X-ray spectroscopy, maXs-20, where the ^{163} Ho ion-implantation was performed using a high-purity ^{163} Ho source produced by advanced chemical and mass separation. With these measurements, we aim at determining an upper limit for the background level due to source contamination and provide a refined description of the calorimetrically measured spectrum. We discuss the plan for a medium scale experiment, ECHo-1k, in which about 1000 Bq of high-purity ^{163} Ho will be ion-implanted into detector arrays. With one year of measuring time, we will be able to achieve a sensitivity on the electron neutrino mass below 20 eV/c^2 (90 % C.L.), improving the present limit by more than one order of magnitude. This experiment will guide the necessary developments to reach the sub-eV sensitivity.

  10. Recent Results for the ECHo Experiment

    NASA Astrophysics Data System (ADS)

    Hassel, C.; Blaum, K.; Goodacre, T. Day; Dorrer, H.; Düllmann, Ch. E.; Eberhardt, K.; Eliseev, S.; Enss, C.; Filianin, P.; Fäßler, A.; Fleischmann, A.; Gastaldo, L.; Goncharov, M.; Hengstler, D.; Jochum, J.; Johnston, K.; Keller, M.; Kempf, S.; Kieck, T.; Köster, U.; Krantz, M.; Marsh, B.; Mokry, C.; Novikov, Yu. N.; Ranitzsch, P. C. O.; Rothe, S.; Rischka, A.; Runke, J.; Saenz, A.; Schneider, F.; Scholl, S.; Schüssler, R. X.; Simkovic, F.; Stora, T.; Thörle-Pospiech, P.; Türler, A.; Veinhard, M.; Wegner, M.; Wendt, K.; Zuber, K.

    2016-08-01

    The Electron Capture in ^{163}Ho experiment, ECHo, is designed to investigate the electron neutrino mass in the sub-eV range by means of the analysis of the calorimetrically measured spectrum following the electron capture (EC) in ^{163}Ho. Arrays of low-temperature metallic magnetic calorimeters (MMCs), read-out by microwave SQUID multiplexing, will be used in this experiment. With a first MMC prototype having the ^{163}Ho source ion-implanted into the absorber, we performed the first high energy resolution measurement of the EC spectrum, which demonstrated the feasibility of such an experiment. In addition to the technological challenges for the development of MMC arrays, which preserve the single pixel performance in terms of energy resolution and bandwidth, the success of the experiment relies on the availability of large ultra-pure ^{163}Ho samples, on the precise description of the expected spectrum, and on the identification and reduction of background. We present preliminary results obtained with standard MMCs developed for soft X-ray spectroscopy, maXs-20, where the ^{163}Ho ion-implantation was performed using a high-purity ^{163}Ho source produced by advanced chemical and mass separation. With these measurements, we aim at determining an upper limit for the background level due to source contamination and provide a refined description of the calorimetrically measured spectrum. We discuss the plan for a medium scale experiment, ECHo-1k, in which about 1000 mathrm {Bq} of high-purity ^{163}Ho will be ion-implanted into detector arrays. With one year of measuring time, we will be able to achieve a sensitivity on the electron neutrino mass below 20 eV/c^2 (90 % C.L.), improving the present limit by more than one order of magnitude. This experiment will guide the necessary developments to reach the sub-eV sensitivity.

  11. Negative ions at Titan and Enceladus: recent results.

    PubMed

    Coates, Andrew J; Wellbrock, Anne; Lewis, Gethyn R; Jones, Geraint H; Young, David T; Crary, Frank J; Waite, J Hunter; Johnson, Robert E; Hille, Thomas W; Sittler, Edward C

    2010-01-01

    The detection of heavy negative ions (up to 13 800 amu) in Titan's ionosphere is one of the tantalizing new results from the Cassini mission. These heavy ions indicate for the first time the existence of heavy hydrocarbon and nitrile molecules in this primitive Earth-like atmosphere. These ions were suggested to be precursors of aerosols in Titan's atmosphere and may precipitate to the surface as tholins. We present the evidence for and the analysis of these heavy negative ions at Titan. In addition we examine the variation of the maximum mass of the Titan negative ions with altitude and latitude for the relevant encounters so far, and we discuss the implications for the negative ion formation process. We present data from a recent set of encounters where the latitude was varied between encounters, with other parameters fixed. Models are beginning to explain the low mass negative ions, but the formation process for the higher mass ions is still not understood. It is possible that the structures may be chains, rings or even fullerenes. Negative ions, mainly water clusters in this case, were seen during Cassini's recent close flybys of Enceladus. We present mass spectra from the Enceladus plume, showing water clusters and additional species. As at Titan, the negative ions indicate chemical complexities which were unknown before the Cassini encounters, and are indicative of a complex balance between neutrals and positively and negatively charged ions. PMID:21302552

  12. The Recent Star Formation History of the M31 Disk

    NASA Astrophysics Data System (ADS)

    Williams, Benjamin F.

    2003-09-01

    The star formation history of the northern and southern M31 disk is measured using samples of BV photometry for 4'×4' regions taken from the KPNO/CTIO Local Group Survey. The distances, mean reddening values, and age distributions of the stars in these regions were measured using the routines of Dolphin. Independent measurements of overlapping fields show that the results are stable for most samples. A slight distance gradient is seen across the major axis of the southern disk, and a mean distance of 24.47+/-0.03 is found by combining the results. Higher mean reddening values are seen to follow the spiral structure. The stellar age distributions are consistent with episodic star formation confined mainly to the gas-rich arm regions. If these episodes were caused by propagating density waves, the waves did not cause significant star formation episodes in the gas-poor interarm regions. A combination of all of the results provides the total star formation rate for 1.4 deg2 of the M31 disk for six epochs. These results suggest that star formation in the disk declined by ~50% from ~250 to ~50 Myr ago. The lowest star formation rate occurred ~25 Myr ago, followed by a ~20% increase to the present. The mean star formation rate for this large portion of M31 over the past 60 Myr is 0.63+/-0.07 Msolar yr-1, suggesting a total mean rate for the disk of ~1 Msolar yr-1.

  13. Recent Formation of Saturnian Moons: Constraints from Their Cratering Records

    NASA Astrophysics Data System (ADS)

    Dones, Henry C. Luke; Charnoz, Sebastien; Robbins, Stuart J.; Bierhaus, Edward B.

    2015-05-01

    Charnoz et al. (2010) proposed that Saturn's small "ring moons" out to Janus and Epimetheus consist of ring material that viscously spread beyond the Roche limit and coagulated into moonlets. The moonlets evolve outward due to the torques they exert at resonances in the rings. More massive moonlets migrate faster; orbits can cross and bodies can merge, resulting in a steep trend of mass vs. distance from the planet. Canup (2010) theorized that Saturn's rings are primordial and originated when a differentiated, Titan-like moon migrated inward when the planet was still surrounded by a gas disk. The satellite's icy shell could have been tidally stripped, and would have given rise to today's rings and the mid-sized moons out to Tethys. Charnoz et al. (2011) investigated the formation of satellites out to Rhea from a spreading massive ring, and Crida and Charnoz (2012) extended this scenario to other planets. Once the mid-sized moons recede far from the rings, tidal interaction with the planet determines the rate at which the satellites migrate. Charnoz et al. (2011) found that Mimas would have formed about 1 billion years more recently than Rhea. The cratering records of these moons (Kirchoff and Schenk 2010; Robbins et al. 2015) provide a test of this scenario. If the mid-sized moons are primordial, most of their craters were created through hypervelocity impacts by ecliptic comets from the Kuiper Belt/Scattered Disk (Zahnle et al. 2003; Dones et al. 2009). In the Charnoz et al. scenario, the oldest craters on the moons would result from low-speed accretionary impacts. We thank the Cassini Data Analysis program for support.ReferencesCanup, R. M. (2010). Nature 468, 943Charnoz, S.; Salmon, J., Crida, A. (2010). Nature 465, 752Charnoz, S., et al. (2011). Icarus 216, 535Crida, A.; Charnoz, S. (2012). Science 338, 1196Dones, L., et al. (2009). In Saturn from Cassini-Huygens, p. 613Kirchoff, M. R.; Schenk, P. (2010). Icarus 206, 485Robbins, S. J.; Bierhaus, E. B.; Dones, L

  14. Recent Results for the Bak-Sneppen Model

    NASA Astrophysics Data System (ADS)

    Boettcher, Stefan; Paczuski, Maya

    2001-03-01

    We discuss our recent result that determines the upper critical dimension of the Bak-Sneppen model to be d_c=4 [see Phys. Rev. Lett. /bf 84, 2267-2270 (2000)], and the theoretical arguments supporting it. Also, we review other aspects of recent interest, such as the aging behavior of the model.

  15. Quasi-elastic reactions: a survey on recent results

    SciTech Connect

    Szilner, S.; Jelavic-Malenica, D.; Soic, N.; Corradi, L.; Stefanini, A. M.; Fioretto, E.; Gadea, A.; Mason, P.; Mengoni, D.; Napoli, D. R.; Recchia, F.; Silvestri, R.; Sahin, E.; Valiente-Dobon, J. J.; Ur, C. A.; Beghini, S.; Farnea, E.; Lenzi, S. M.; Lunardi, S.; Montagnoli, G.

    2010-04-30

    Binary reactions at energies close to the Coulomb barrier received recently a significant boost thanks to the advent of the large solid angle magnetic spectrometer PRISMA coupled to the gamma array CLARA. In the present paper different aspects of the recent results of nuclear structure and reaction dynamics will be presented, focusing more closely on the reaction mechanism.

  16. Searches for new physics at Tevatron: Most recent results

    SciTech Connect

    Popov, A.V.; /Serpukhov, IHEP

    2011-01-01

    The most recent results obtained from searches of particles and phenomena beyond the Standard Model (new physics) in the D0 and CDF experiments at the Tevatron accelerator (FNAL, USA) on the basis of statistics corresponding to the integrated luminosity of up to 4 fb{sup -1} in 2009 are considered. Particular attention is given to the most recent results on searches for a supersymmetric Higgs boson.

  17. A Review of recent results from the Tevatron

    SciTech Connect

    Chiarelli, Giorgo; /INFN, Pisa

    2007-06-01

    The D0 and CDF experiments have been taking data at the Run 2 of the Tevatron Collider since 2001. We present a selection of recent results, most of them obtained with an integrated luminosity of {approx_equal} 1 fb{sup -1}. I will describe the most important facets of the physics programme and detail some results. Recent direct limits on standard model Higgs obtained at the Tevatron, and their their prospects will be also reviewed.

  18. Recent physics results from CDF and D0

    SciTech Connect

    Evelyn Thomson

    2004-02-25

    Recent physics results from CDF and D0 on heavy flavor physics, electroweak precision measurements, top physics, QCD and searches for new physics are discussed. The results are based on approximately 140 pb{sup -1} of data collected at {radical}s = 1.96 TeV between 2002 and 2003.

  19. Recent heavy flavor physics results from fixed target experiments

    SciTech Connect

    Spiegel, L.

    1991-11-01

    Recent results from fixed target experiments in the field of heavy quark flavors, as published or otherwise disseminated in the last year, are reviewed. Emphasis is placed on distilling the main conclusions from these results. 35 refs., 5 figs., 4 tabs.

  20. Recent run II QCD results from D0

    SciTech Connect

    Wobisch, Markus; /Fermilab

    2004-11-01

    We present recent QCD results from the D0 experiment at the Fermilab Tevatron Collider in p{bar p} collisions at {radical}s = 1.96TeV. Results are presented for the inclusive jet and dijet cross sections, a measurement of dijet azimuthal decorrelations, studies of elastic scattering, and a search for diffractively produced Z bosons.

  1. Recent LEP2 results on searches for new phenomena

    SciTech Connect

    Pan Yibin

    1998-05-29

    Recent results of searches for supersymmetric particles, Higgs bosons, and other new phenomena at LEP2 are summarized. These results are based on data and analyses from the four LEP experiments: ALEPH, DELPHI, L3, and OPAL. The data were collected during the summer and fall of 1996 with center-of-mass energies of 161 and 172 GeV.

  2. Recent PHENIX results on hard probes and direct photon production

    NASA Astrophysics Data System (ADS)

    Riabov, V.; PHENIX Collaboration

    2016-02-01

    A hot and dense matter called strongly interacting quark-gluon plasma (sQGP) is created in heavy ion collisions at RHIC energies. Detailed study of the properties of this new state of matter is a driving force of recent research at RHIC. In these proceedings we present most recent PHENIX results for system size and energy dependence of hadron and jet production at high transverse momentum in heavy ion collisions at RHIC. We also report latest results for direct photon production including soft direct photon yields and anisotropic flow.

  3. The Wide-Field Imaging Interferometry Testbed: Recent Results

    NASA Technical Reports Server (NTRS)

    Rinehart, Stephen

    2006-01-01

    We present recent results from the Wide-Field Imaging Interferometry Testbed (WIIT). The data acquired with the WIIT is "double Fourier" data, including both spatial and spectral information within each data cube. We have been working with this data, and starting to develop algorithms, implementations, and techniques for reducing this data. Such algorithms and tools are of great importance for a number of proposed future missions, including the Space Infrared Interferometric Telescope (SPIRIT), the Submillimeter Probe of the Evolution of Cosmic Structure (SPECS), and the Terrestrial Planet Finder Interferometer (TPF-I)/Darwin. Recent results are discussed and future study directions are described.

  4. The Intra-cluster medium: recent results and future prospects

    NASA Astrophysics Data System (ADS)

    Molendi, Silvano

    2010-07-01

    This comunication is divided in two parts: in the first I present some recent observational results obtained by my group; in the second I list what I consider to be the top priorities in terms of X-ray instrumentation for cluster science and compare them with missions currently under development.

  5. Recent results from the Argonne Fragment Mass Analyzer

    SciTech Connect

    Davids, C.N.; Back, B.; Carpenter, M.P.; Henderson, D.J.; Henry, R.G.; Janssens, R.V.F.; Khoo, T.L.; Lauritsen, T.; Liang, Y.; Bindra, K. |; Chung, W. |; Soramel, F. |; Bearden, I.G.; Daly, P.J.; Fornal, B.; Grabowski, Z.W.; Mayer, R.H.; Nisius, D.; Broda, R. |; Bingham, C.R.; Moltz, D.M.; Ramayya, A.V.; Robertson, J.D.; Scarlassara, F.; Spolaore, P.; Toth, K.S.; Walters, W.B.

    1992-12-31

    The Fragment Mass Analyzer (FMA) at the ATLAS accelerator has been operational for about one year. During that period a number of test runs and experiments have been carried out. The test runs have verified that the ion optics of the FMA are essentially as calculated. A brief facility description is followed by recent experimental results.

  6. Recent results from the Argonne Fragment Mass Analyzer

    SciTech Connect

    Davids, C.N.; Back, B.; Carpenter, M.P.; Henderson, D.J.; Henry, R.G.; Janssens, R.V.F.; Khoo, T.L.; Lauritsen, T.; Liang, Y. ); Bindra, K. Vanderbilt Univ., Nashville, TN ); Chung, W. Notre Dame Univ., IN ); Soramel, F. (Argonne National Lab., IL (

    1992-01-01

    The Fragment Mass Analyzer (FMA) at the ATLAS accelerator has been operational for about one year. During that period a number of test runs and experiments have been carried out. The test runs have verified that the ion optics of the FMA are essentially as calculated. A brief facility description is followed by recent experimental results.

  7. Recent Progress and Results of LEPS, LEPS2, and ELPH

    NASA Astrophysics Data System (ADS)

    Muramatsu, Norihito

    2013-08-01

    Hadron photoproduction reactions are complementarily studied at SPring-8/LEPS and ELPH, Tohoku University. Their recent results on hadron structure and interaction are summarized in the present article. On the pentaquark candidate Θ+, a clear peak structure is seen in new exclusive analyses using increased statistics data of the γ d→K+K-X reaction. A new project LEPS2 has started at SPring-8 in conjunction with LEPS and ELPH. Recent progress is discussed including a new photon detector system BGO-EGG, which is under construction at ELPH. LEPS2 beam commissioning will start from the end of FY2012.

  8. Recent results in secondary voltage control of power systems

    SciTech Connect

    Stankovic, A.; Ilic, M. . Lab. for Electromagnetic and Electronic Systems); Maratukulam, D. )

    1991-02-01

    This paper reports recent results on a pilot point based secondary voltage control in power systems. Similarities and differences compared to the optimal power flow methodology are described and theoretical background for secondary voltage controller design is reviewed. Two complementary design problem formulations are reported together with simulations on a 39 bus and a 338 bus power system models. The results validate the feasibility of the pilot point approach and reveal the nature of tradeoffs involved in secondary voltage controller designs.

  9. Recent results on TMDs from the HERMES experiment

    NASA Astrophysics Data System (ADS)

    Korotkov, V. A.

    2016-02-01

    HERMES has taken a wealth of deep-inelastic scattering data using the 27.6 GeV polarized lepton beam at HERA and various pure gas targets, both unpolarized and polarized, which opened the door to several unique results. Among them are the first evidences for the naive-T-odd Sivers and Collins effects. An overview of recent HERMES results on measurement of azimuthal asymmetries in semi-inclusive production of pions, charged kaons and (anti)protons is presented.

  10. Recent Geologic Mapping Results for the Polar Regions of Mars

    NASA Technical Reports Server (NTRS)

    tanaka, K. L.; Kolb, E. J.

    2008-01-01

    The polar regions of Mars include the densest data coverage for the planet because of the polar orbits of MGS, ODY, and MEX. Because the geology of the polar plateaus has been among the most dynamic on the planet in recent geologic time, the data enable the most detailed and complex geologic investigations of any regions on Mars, superseding previous, even recent, mapping efforts [e.g., 1-3]. Geologic mapping at regional and local scales is revealing that the stratigraphy and modificational histories of polar materials by various processes are highly complex at both poles. Here, we describe some of our recent results in polar geologic mapping and how they address the geologic processes involved and implications for polar climate history.

  11. Recent Radio Results on X-ray Binaries and Transients

    NASA Astrophysics Data System (ADS)

    Rupen, M. P.; Dhawan, V.; Mioduszewski, A. J.

    2003-03-01

    We present recent results from observations with the Very Large Array (VLA) and Very Long Baseline Array (VLBA) on a number of recent X-ray transients, and a few old friends. In addition to any new X-ray transients discovered between now and the HEAD meeting, we discuss the radio counterpart to XTE J1720-318; the recent resurgence of XTE J1908+094 and GRS 1758-258; the connection between the radio and X-ray emission in the millisecond X-ray pulsars XTE J0929-314 and SAX J1808.4-3658; and VLBA imaging of the 1999 outburst of the microquasar V4641 Sgr, confirming the rapid expansion seen with the VLA. The National Radio Astronomy Observatory is a facility of the National Science Foundation operated under cooperative agreement by Associated Universities, Inc.

  12. Recent results in high pT physics from CDF

    SciTech Connect

    G. Veramendi

    2004-03-09

    The authors present the most recent high p{sub T} results from the CDF experiment using p{bar p} collisions at {radical}s = 1.96 TeV produced at the Tevatron Collider at Fermilab. They summarize results in electroweak physics, top physics and searches for physics beyond the Standard Model. Many measurements of important signals like W boson, Z boson, and the top quark have been reestablished. Taking advantage of the increase in energy and detector upgrades, these measurements already begin to be competitive with previous results.

  13. ANTARES and Baikal: Recent results from underwater neutrino telescopes

    NASA Astrophysics Data System (ADS)

    Schüssler, Fabian

    2016-07-01

    Two Northern hemisphere neutrino telescopes are currently searching for astrophysical neutrinos in the TeV/PeV range: ANTARES and Baikal. Both observatories utilize various signatures like a high energy excess over the atmospheric neutrino flux, searches for localized neutrino sources of various extensions and multi-messenger analyses based on time and/or space coincidences with other cosmic probes. We here review the status of both experiments and discuss a selection of recent results.

  14. Recent Fermilab results on hadroproduction of heavy flavors

    SciTech Connect

    Garbincius, P.H.

    1993-08-01

    Recent results from various Fermilab experiments on the hadroproduction of states containing charm, bottom, and top quarks are discussed. These include observation of the spectra, lifetime, and production characteristics of charmonium, open charm states, and bottom particle production with both high energy fixed target and {bar p}-p collider facilities. The status of the search for the top quark by the Fermilab collider experiments is updated.

  15. Recent Results of Top Quark Physics from the Tevatron

    SciTech Connect

    Peters, R. Y.

    2015-07-09

    Twenty years after its discovery in 1995 by the CDF and D0 collaborations at the Tevatron proton-antiproton collider at Fermilab, the top quark still undergoes intensive studies at the Tevatron and the LHC at CERN. In this article, recent top quark physics results from CDF and D0 are reported. In particular, measurements of single top quark and double top quark production, the $t\\bar{t}$ forward-backward asymmetry and the top quark mass are discussed.

  16. Recent Results in Electroweak B Decays from the BABAR Experiment

    SciTech Connect

    Koeneke, Karsten

    2006-07-11

    A review of the most recent BABAR results on electroweak penguin B decays is presented. The focus of this paper is on the measurement of observables in the decays B {yields} X{sub s}{gamma}, B {yields} K{sup (*)}l{sup +}l{sup -} B {yields} K{sub s}{sup 0}{pi}{sup 0}{gamma} (time-dependent analysis) and B {yields} ({rho}/{omega}){gamma}.

  17. Satellite Communications for Aeronautical Applications: Recent research and Development Results

    NASA Technical Reports Server (NTRS)

    Kerczewski, Robert J.

    2001-01-01

    Communications systems have always been a critical element in aviation. Until recently, nearly all communications between the ground and aircraft have been based on analog voice technology. But the future of global aviation requires a more sophisticated "information infrastructure" which not only provides more and better communications, but integrates the key information functions (communications, navigation, and surveillance) into a modern, network-based infrastructure. Satellite communications will play an increasing role in providing information infrastructure solutions for aviation. Developing and adapting satellite communications technologies for aviation use is now receiving increased attention as the urgency to develop information infrastructure solutions grows. The NASA Glenn Research Center is actively involved in research and development activities for aeronautical satellite communications, with a key emphasis on air traffic management communications needs. This paper describes the recent results and status of NASA Glenn's research program.

  18. Recent results in analysis and simulation of beam halo

    SciTech Connect

    Ryne, Robert D.; Wangler, Thomas P.

    1995-09-15

    Understanding and predicting beam halo is a major issue for accelerator driven transmutation technologies. If strict beam loss requirements are not met, the resulting radioactivation can reduce the availability of the accelerator facility and may lead to the necessity for time-consuming remote maintenance. Recently there has been much activity related to the core-halo model of halo evolution [1-5]. In this paper we will discuss the core-halo model in the context of constant focusing channels and periodic focusing channels. We will present numerical results based on this model and we will show comparisons with results from large scale particle simulations run on a massively parallel computer. We will also present results from direct Vlasov simulations.

  19. Recent results in analysis and simulation of beam halo

    SciTech Connect

    Ryne, R.D.; Wangler, T.P.

    1994-09-01

    Understanding and predicting beam halo is a major issue for accelerator driven transmutation technologies. If strict beam loss requirements are not met, the resulting radioactivation can reduce the availability of the accelerator facility and may lead to the necessity for time-consuming remote maintenance. Recently there has been much activity related to the core-halo model of halo evolution. In this paper the authors will discuss the core-halo model in the context of constant focusing channels and periodic focusing channels. They will present numerical results based on this model and they will show comparisons with results from large scale particle simulations run on a massively parallel computer. They will also present results from direct Vlasov simulations.

  20. Recent Star-formation in Post-Starburst Quasars

    NASA Astrophysics Data System (ADS)

    Townsend, Shonda; Ganguly, R.; Strom, A.; Cales, S.; Brotherton, M. S.

    2011-01-01

    Post-Starburst Quasars (PSQ, alternatively Q+As) show simultaneously the spectrum of a massive A-type stellar population and a quasar. The prototype PSQ, UNJ1025-0040, shows a UV excess over the quasar spectrum, indicating more recent star-formation (Brotherton et al 2002). To gauge the frequency and distribution of these younger stellar populations in PSQs, we have collected GALEX (GR45) and 2MASS photometry for 409 objects. The objects are catalog 609 spectroscopically-selected PSQs from Brotherton et al. (2010) that uses similar criteria as Zabludoff et al. (1996) for post-starburst galaxies (PSG, E+A). For comparison, we have compiled two samples: (1) 16,000 quasars that is matched in redshift (0.01-0.7) and Sloan-u magnitude (16.1-21.2), which is blueward of the Balmer edge and provides the least contamination from the massive stellar population; and (2) 500 PSGs from Goto et al. (2007). 389 (55) PSQs show an NUV (FUV) excess over the expected UV flux if the underlying quasar were ``normal.'’ 126 (460) objects show an NUV (FUV) decrement. The observed NUV to u-band flux ratio of the median PSQ rises from 1 at z=0.01 to 2.5 at z=0.4, while the same for the median QSO remains at 1. The observed FUV to u-band flux ratio of the median QSO rises slightly from 0.6 to 0.8 over the redshift range 0.05-0.2, whereas the median PSQ is nearly a factor of three lower. The disparity between the median PSQ and QSO suggests the presence of young stars that add in NUV light, but not FUV light. To quantify the youth and mass of this putative population, we will present preliminary efforts to model PSQs using two simple stellar populations, an underlying quasar, and dust reddening. We acknowledge funding from GALEX through grant NNX10AC63G.

  1. Recent laboratory photochemical studies and their relationship to the photochemical formation of cometary radicals

    NASA Technical Reports Server (NTRS)

    Jackson, William M.

    1991-01-01

    Experimental laboratory techniques used in studying the photochemistry of stable and unstable molecules are discussed. The laboratory evidence for the photochemical formation of C2 from C2H, C3 from C3H2, and NH from NH2 is presented. Other recent results obtained in laboratory studies of H2O, H2S, NH3, and HCN are reported.

  2. News from the proton - recent DIS results from HERA

    SciTech Connect

    Meier, K.

    1997-01-01

    Recent results from the two large general-purpose detectors H1 and ZEUS at HERA (DESY, Hamburg, Germany) are presented. Emphasis is given to the analysis of deep inelastic scattering defined by the observation of the scattered electron or positron in the main calorimeters. Results on purely inclusive cross sections lead to a determination of the charged (quarks) parton distribution F{sub 2}(x, Q{sup 2}). Access to the electrically neutral parton content (gluons) is obtained indirectly by an analysis of the expected scaling violation behavior of F{sub 2} or directly from multijet rates originating from well-defined initial parton configurations. Finally, the recently uncovered subclass of large rapidity gap (LRG) events has been analyzed in terms of F{sub 2}. The result supports the concept of a color neutral object (Pomeron IP) being probed by a hard scattering electron. Evidence for factorization of the Pomeron radiation process as well as for scaling in the inclusive IP structure functions has been found.

  3. Review of Recent Results from the Rhic Beam Energy Scan

    NASA Astrophysics Data System (ADS)

    Kumar, Lokesh

    2013-10-01

    We review recent results from the RHIC beam energy scan (BES) program, aimed to study the Quantum Chromodynamics (QCD) phase diagram. The main goals are to search for the possible phase boundary, softening of equation of state or first order phase transition, and possible critical point. Phase-I of the BES program has recently concluded with data collection for Au+Au collisions at center-of-mass energies (√ {sNN}) of 7.7, 11.5, 19.6, 27 and 39 GeV. Several interesting results are observed for these lower energies where the net-baryon density is high at the mid-rapidity. These results indicate that the matter formed at lower energies (7.7 and 11.5 GeV) is hadron dominated and might not have undergone a phase transition. In addition, a centrality dependence of freeze-out parameters is observed for the first time at lower energies, slope of directed flow for (net)-protons measured versus rapidity shows an interesting behavior at lower energies, and higher moments of net-proton show deviation from Skellam expectations at lower energies. An outlook for the future BES Phase-II program is presented and efforts for the detailed study of QCD phase diagram are discussed.

  4. Recent Results in Semileptonic B Decays with BaBar

    SciTech Connect

    Hamilton, B.K.; /Maryland U.

    2012-04-02

    In this note, recent results of studies of semileptonic B meson decays from BABAR are discussed and preliminary results given. In particular, a recent measurement of {Beta}(B {yields} D{sup (*)}{tau}{nu}) and the ratio {Beta}(B {yields} D{sup (*)}{tau}{nu})/{Beta}(B {yields} D{sup (*)}{ell}{nu}) is presented. For the D* mode, a branching fraction of 1.79 {+-} 0.13(stat) {+-} 0.17(syst) is found, with a ratio of 0.325 {+-} 0.023(stat) {+-} 0.027(syst). For the D mode, the results are 1.04 {+-} 0.12(stat) {+-} 0.14(syst) and 0.456 {+-} 0.053(stat) {+-} 0.056(syst), respectively. In addition, a study of B{sub s} production and semileptonic decays using data collected in a center-of-mass energy region above the {Upsilon}(4S) resonance is discussed. The semileptonic branching fraction {Beta}(B{sub s} {yields} {ell}{nu}X) is measured to be 9.9{sub -2.1}{sup +2.6}(stat){sub -2.0}{sup +1.3}(syst).

  5. Present status and recent results from the APS SASE FEL

    NASA Astrophysics Data System (ADS)

    Lewellen, J. W.; Milton, S. V.; Gluskin, E.; Arnold, N. D.; Benson, C.; Berg, W.; Biedron, S. G.; Borland, M.; Chae, Y.-C.; Dejus, R. J.; Hartog, P. K. Den; Deriy, B.; Erdmann, M.; Eidelman, Y. I.; Hahne, M. W.; Huang, Z.; Kim, K.-J.; Li, Y.; Lumpkin, A. H.; Makarov, O.; Moog, E. R.; Nassiri, A.; Sajaev, V.; Soliday, R.; Tieman, B. J.; Trakhtenberg, E. M.; Vasserman, I. B.; Vinokurov, N. A.; Wiemerslage, G.; Yang, B. X.

    2002-05-01

    The Low-Energy Undulator Test Line (LEUTL) at the Advanced Photon Source, Argonne National Laboratory, is intended to demonstrate the basic operation of a SASE-based free-electron laser. Goals include comparison of experimental results with theoretical predictions and scaling laws, identification of problems relevant to fourth-generation light source construction and operation and the means of addressing them, the development of operational and diagnostic techniques to optimize SASE FEL performance and increase repeatability from run to run, and performance of initial pioneering experiments capable of exploiting the unique properties of the laser. The basic layout and operational philosophy of the LEUTL experiment is presented. A summary of past results, including saturation, is reviewed, and a description of recent results is presented. We conclude with future plans, which include pressing to shorter wavelengths and incorporating user experiments into the LEUTL experimental program.

  6. Recent results in electroweak physics at the Tevatron

    SciTech Connect

    Giulia Manca

    2004-02-13

    The Run II physics program of CDF and D0 has just begun with the first 72 pb{sup -1} of analysis quality data collected at the center-of-mass energy of 1.96 TeV. The Electroweak measurements are among the first and most important benchmarks for the best understanding of the detectors and testing the Standard Model. We present measurements of the W and Z inclusive cross sections and decays asymmetries, recent results in di-boson physics and searches for new physics which make use of distinct electroweak signatures.

  7. Steps Toward Identifying PAHs: A Child's Garden of Recent Results

    NASA Technical Reports Server (NTRS)

    Hudgins, Douglas M.

    2005-01-01

    Based on over two decades of experimental, observational and theoretical studies by scientists around the world. It is now widely accepted that the composite emission of mixtures of vibrationally-excited PAHs and PAH ions can accommodate the general pattern of band positions, intensities, and profiles observed in the discreet IR emission features of carbon-rich interstellar dust, as well as the variations in those characteristics. These variations provide insight into the detailed nature of the emitting PAH population and reflect conditions within the emitting regions giving the population enormous potential as probes of astrophysical environments. Moreover, the ubiquity and abundance of this material has impacts that extend well beyond the IR. In this presentation we will examine recent, combined experimental, theoretical, and observational studies that indicate that nitrogen-substituted PAHs represent an important component of the interstellar dust population, and we will go on to explore some of the ramifications of this result. We will also explore the results of recent experimental studies of the strong, low-lying electronic transitions of ionized PAH ions in the Near-IR (0.7 - 2.5 microns) and explore the role that these transitions might play in pumping the PAH IR emission in regions of low-excitation.

  8. Recent Experimental Results from Cryogenic Implosions on OMEGA

    NASA Astrophysics Data System (ADS)

    Sangster, T. C.; Goncharov, V. N.; Radha, P. B.; Betti, R.; Boehly, T. R.; Glebov, V. Yu.; Hu, S. X.; McCrory, R. L.; McKenty, P. W.; Meyerhofer, D. D.; Seka, W.; Smalyuk, V. A.; Frenje, J. A.; Petrasso, R. D.; Shvarts, D.

    2008-11-01

    The implosion performance of energy-scaled cryogenic D2 and DT targets on the 60-beam OMEGA laser is important for understanding the physics of highly compressed fuel and the validation of ignition designs for the NIF. Recent experiments have demonstrated good performance using a multi-shock drive that has been tuned based on cryogenic cone-in-shell targets. Fuel areal densities are now consistently exceeding 80% of the 1-D prediction, while the yields are between 10% and 20% of 1-D predictions. These results demonstrate the benefit (and necessity) of an independent shock-timing platform. This talk will present the latest implosion performance results and potentially show the first cryogenic-fuel-core radiographs using a short pulse beam from the new OMEGA EP Laser Facility. This work was supported by the U.S. Department of Energy Office of Inertial Confinement Fusion under Cooperative Agreement No. DE-FC52-08NA28302.

  9. Recent results on structural control of an active precision structure

    NASA Technical Reports Server (NTRS)

    Chu, C. C.; Fanson, J. L.; Smith, R. S.

    1991-01-01

    This paper describes recent results in structural control of an active precision truss structure at JPL. The goal is to develop practical control methodology and to apply to active truss structures intended for high precision space-based optics applications. The active structure considered incorporates piezoelectric active members which apply control forces internal to the structure and thereby improve the structure's dimensional stability. Two approaches to structural control system design were investigated. The first approach uses only noncollocated measurements of acceleration at the location of a simulated optical component to achieve structural stabilization. The second approach is essentially the same as the first one except that a viscous damper was used in place of a truss member on the structure to improve the dampings of selected flexible modes. The corresponding experimental closed-loop results are presented in this paper.

  10. Overview of recent results from the HERMES experiment

    NASA Astrophysics Data System (ADS)

    Schnell, G.

    2013-11-01

    HERMES has taken a wealth of deep-inelastic scattering (DIS) data using the 27.6 GeV polarized lepton beam at HERA and various pure gas targets, both unpolarized and polarized, which opened the door to several unique results. Among them are the first evidences for the naive-T-odd Sivers and Collins effects but also the recent first measurements of azimuthal modulations in the unpolarized semi-inclusive DIS cross section for charged kaons and pions and of beam-helicity asymmetries in exclusive leptoproduction of real photons using recoil-proton detection. An overview of HERMES results is given with emphasis on the exploration of the three-dimensional structure of the nucleon.

  11. Recent results in nonlinear strain and modulus imaging

    PubMed Central

    Hall, Timothy J.; Barbone, Paul; Oberai, Assad A.; Jiang, Jingfeng; Dord, Jean Francois; Goenezen, Sevan; Fisher, Ted G.

    2012-01-01

    We report a summary of recent developments and current status of our team’s efforts to image and quantify in vivo nonlinear strain and tissue mechanical properties. Our work is guided by a focus on applications to cancer diagnosis and treatment using clinical ultrasound imaging and quasi-static tissue deformations. We review our recent developments in displacement estimation from ultrasound image sequences. We discuss cross correlation approaches, regularized optimization approaches, guided search methods, multiscale methods, and hybrid methods. Current implementations can return results of high accuracy in both axial and lateral directions at several frames per second. We compare several strain estimators. Again we see a benefit from a regularized optimization approach. We then discuss both direct and iterative methods to reconstruct tissue mechanical property distributions from measured strain and displacement fields. We review the formulation, discretization, and algorithmic considerations that come into play when attempting to infer linear and nonlinear elastic properties from strain and displacement measurements. Finally we illustrate our progress with example applications in breast disease diagnosis and tumor ablation monitoring. Our current status shows that we have demonstrated quantitative determination of nonlinear parameters in phantoms and in vivo, in the context of 2D models and data. We look forward to incorporating 3D data from 2D transducer arrays to noninvasively create calibrated 3D quantitative maps of nonlinear elastic properties of breast tissues in vivo. PMID:22754425

  12. Seismological constraints on deep mantle structure: recent results

    NASA Astrophysics Data System (ADS)

    Ritsema, J. E.

    2002-12-01

    Thanks to the development of global seismic networks, especially in the past two decades when digital broadband ground motion sensors were employed, full waveform analysis has led to the development of three-dimensional models of the structure of Earth's interior. Yet, many of the new models confirm a number of critical conclusions that F. Birch drew in his seminal 1952 JGR paper. For example, he envisioned that the upper mantle transition zone plays a prominent role in mantle circulation and he emphasized the significant effect of pressure on thermodynamic parameters. Indeed, a large number of seismic studies of the transition zone indicate that the descent of slabs of former oceanic lithosphere is, with few exceptions, impeded by the 660--km discontinuity. Furthermore, the observation of predominantly broad seismic velocity structures in the lower mantle (> 1500 km depth) may reflect sluggish convection, due to reduced thermal expansivity. I will review several recent seismological studies of the deep mantle and place them in the context of Birch's paper. In particular, I will discuss surprising new findings in the deep mantle beneath Africa, which is especially well studied with data from recent African deployments. Furthermore, I will show results of the application of a new 3D waveform modeling technique that may prove invaluable in future seismological studies of the deep mantle.

  13. Commissioning results from the recently upgraded RHIC LLRF system

    SciTech Connect

    Smith, K.S.; Harvey, M.; Hayes, T.; Narayan, G.; Severino, F.; Yuan, S.; Zaltsman, A.

    2011-03-28

    During RHIC Run 10, the first phase of the LLRF Upgrade was successfully completed. This involved replacing the aging VME based system with a modern digital system based on the recently developed RHIC LLRF Upgrade Platform, and commissioning the system as part of the normal RHIC start up process. At the start of Run 11, the second phase of the upgrade is underway, involving a significant expansion of both hardware and functionality. This paper will review the commissioning effort and provide examples of improvements in system performance, flexibility and scalability afforded by the new platform. The RHIC LLRF upgrade is based on the recently developed RHIC LLRF Upgrade Platform. The major design goals of the platform are: (1) Design a stand alone, generic, digital, modular control architecture which can be configured to satisfy all of the application demands we currently have, and which will be supportable and upgradeable into the foreseeable future; and (2) It should integrate seamlessly into existing controls infrastructure, be easy to deploy, provide access to all relevant control parameters (eliminate knobs), provide vastly improved diagnostic data capabilities, and permit remote reconfiguration. Although the system is still in its infancy, we think the initial commissioning results from RHIC indicate that these goals have been achieved, and that we've only begun to realize the benefits the platform provides.

  14. An Overview of Recent PISCES Program PMI Results

    NASA Astrophysics Data System (ADS)

    Tynan, George; Doerner, Russell; Abe, Shota; Baldwin, Matthew; Barton, Joseph; Chen, Renkun; Gosselin, Jordan; Hollmann, Eric; Nishijima, Daisuke; Simmonds, Michael; Wang, Yong; Yu, Jonathan

    2015-11-01

    The PISCES Program is focused on fundamental PMI studies of Be and W-based solid plasma facing components under steady-state and transient conditions. We will show results from studies in W, Be and mixed W-Be material systems. Topics of investigation include formation of near-surface nanobubbles from He plasma ion implantation, growth of W-fuzz from these bubbles in steady-state and transient conditions, D retention in Be and W and development of a D-retention model for both H/D isotope exchange and displacement damage experiments. Initial studies of PMI in displacement damaged W are also presented, showing the effect of damage and exposure temperature on D retention, D diffusion, W thermal conductivity. Be-based results include morphology evolution under high plasma flux exposure, Be erosion mechanisms, and retention in Be-based materials. Future plans and connections to fusion energy system requirements will be discussed. This work supported by grant DE-FG02-07ER54912.

  15. Recent results of invariant torus breakup in nontwist maps

    NASA Astrophysics Data System (ADS)

    Wurm, Alexander; Fuchss, Kathrin; Morrison, P. J.

    2006-10-01

    As simple models for degenerate Hamiltonian systems, nontwist maps have been used to describe, e.g., magnetic field lines in toroidal plasma devices with reversed magnetic shear profiles. Of particular interest in these maps are the so-called shearless invariant tori which correspond to transport barries in the physical system. We investigate the breakup of shearless tori in several maps and with several different winding numbers, in order to understand the dependence of the details of the breakup on the winding number and on the symmetries of the map model. Here we report on recent results of this investigation.[1][1] K. Fuchss, A. Wurm, A. Apte, and P.J. Morrison, to appear in Chaos (2006); K. Fuchss, A. Wurm, and P.J. Morrison, preprint/submitted to PRL (2006).

  16. Recent Results in Quantum Chemical Kinetics from High Resolution Spectroscopy

    SciTech Connect

    Quack, Martin

    2007-12-26

    We outline the approach of our group to derive intramolecular kinetic primary processes from high resolution spectroscopy. We then review recent results on intramolecular vibrational redistribution (IVR) and on tunneling processes. Examples are the quantum dynamics of the C-H-chromophore in organic molecules, hydrogen bond dynamics in (HF){sub 2} and stereomutation dynamics in H{sub 2}O{sub 2} and related chiral molecules. We finally discuss the time scales for these and further processes which range from 10 fs to more than seconds in terms of successive symmetry breakings, leading to the question of nuclear spin symmetry and parity violation as well as the question of CPT symmetry.

  17. Automatic Structures — Recent Results and Open Questions

    NASA Astrophysics Data System (ADS)

    Stephan, Frank

    2015-06-01

    Regular languages are languages recognised by finite automata; automatic structures are a generalisation of regular languages where one also uses automatic relations (which are relations recognised by synchronous finite automata) and automatic functions (which are functions whose graph is an automatic relation). Functions and relations first-order definable from other automatic functions and relations are again automatic. Automatic functions coincide with the functions computed by position-faithful one-tape Turing machines in linear time. This survey addresses recent results and open questions on topics related to automatic structures: How difficult is the isomorphism problem for various types of automatic structures? Which groups are automatic? When are automatic groups Abelian or orderable? How can one overcome some of the limitations to represent rings and fields by weakening the automaticity requirements of a structure?

  18. SIM Interferometer Testbed (SCDU) Status and Recent Results

    NASA Technical Reports Server (NTRS)

    Nemati, Bijan; An, Xin; Goullioud, Renaud; Shao, Michael; Shen, Tsae-Pyng; Wehmeier, Udo J.; Weilert, Mark A.; Wang, Xu; Werne, Thomas A.; Wu, Janet P.; Zhai, Chengxing

    2010-01-01

    SIM Lite is a space-borne stellar interferometer capable of searching for Earth-size planets in the habitable zones of nearby stars. This search will require measurement of astrometric angles with sub micro-arcsecond accuracy and optical pathlength differences to 1 picometer by the end of the five-year mission. One of the most significant technical risks in achieving this level of accuracy is from systematic errors that arise from spectral differences between candidate stars and nearby reference stars. The Spectral Calibration Development Unit (SCDU), in operation since 2007, has been used to explore this effect and demonstrate performance meeting SIM goals. In this paper we present the status of this testbed and recent results.

  19. Solar neutrino experiments: recent results and future prospects

    NASA Astrophysics Data System (ADS)

    Chen, M. C.

    2011-09-01

    Recent results from the SNO and Borexino solar neutrino experiments have pushed the observation of solar neutrinos to lower energies. Borexino's measurement of the rate of 7Be solar neutrinos demonstrates that the survival probability for solar neutrinos below 1 MeV is larger than for the 8B solar neutrinos, consistent with our expectation for neutrino propagation affected by matter. On the other hand, by looking at lower energy 8B solar neutrinos, SNO (and also Borexino) do not see the predicted rise in the survival probability and there is even a hint that the survival probability drops to a lower value. Future solar neutrino experiments, in particular the SNO+ experiment, will look at this question by making precision measurements of the survival probability of the pep solar neutrinos (1.44 MeV energy).

  20. Recent Run II Electroweak and QCD Results from D0

    SciTech Connect

    Robert L. Kehoe

    2003-12-17

    The D0 Detector is a hermetic, multipurpose detector residing at one interaction region designated for p{bar p} collisions at 2 TeV at the Fermilab Tevatron. Both the detector and accelerator have undergone major upgrades to increase the luminosity and handle higher interaction rates. This paper presents recent results from Run II data which explore QCD and electroweak physics at the energy frontier. The dijet mass cross section and a search for Z' in dielectron decays are presented, and these are already approaching sensitivities seen in Run I. Additionally, the first measurement of the {sigma}{sub Z} * BR(Z {yields} {mu}{mu}) is given for the new collision energy.

  1. An overview of recent DVCS results at HERMES

    NASA Astrophysics Data System (ADS)

    Yaschenko, S.

    2014-01-01

    The HERMES experiment at DESY, Hamburg, collected unique data on Deeply Virtual Compton Scattering (DVCS) utilizing the HERA polarized electron or positron beams with an energy of 27.6 GeV and longitudinally or transversely polarized or unpolarized gas targets (H, D or heavier nuclei). For the last two years of HERA running, a recoil detector was installed to improve the selection of DVCS events by direct measurement of the recoil protons. Recent HERMES results on DVCS off the hydrogen target and on associated processes ep → epπ0γ and ep → enπ+γ in the Δ-resonance region obtained with the recoil detector are presented.

  2. Trojan Horse Method: recent results in nuclear astrophysics

    NASA Astrophysics Data System (ADS)

    Spitaleri, C.; Lamia, L.; Gimenez Del Santo, M.; Burjan, V.; Carlin, N.; Li, Chengbo; Cherubini, S.; Crucilla, V.; Gulino, M.; Hons, Z.; Kroha, V.; Irgaziev, B.; La Cognata, M.; Mrazek, J.; Mukhamedzhanov, M.; Munhoz, M. G.; Palmerini, S.; Pizzone, R. G.; Puglia, M. R.; Rapisarda, G. G.; Romano, S.; Sergi, L.; Zhou, Shu-Hua; Somorjai, E.; Souza, F. A.; Tabacaru, G.; Szanto de Toledo, A.; Tumino, A.; Wen, Qungang; Wakabayashi, Y.; Yamaguchi, H.

    2015-07-01

    The accurate knowledge of thermonuclear reaction rates is important in understanding the energy generation, the neutrinos luminosity and the synthesis of elements in stars. The physical conditions under which the majority of astrophysical reactions proceed in stellar environments make it difficult or impossible to measure them under the same conditions in the laboratory. That is why different indirect techniques are being used along with direct measurements. The Trojan Horse Method (THM) is introduced as an independent technique to obtain the bare nucleus astrophysical S(E)-factor. As examples the results of recent the application of THM to the 2H(11B, σ08Be)n and 2H(10B, σ07Be)n reactions are presented.

  3. Solar Irradiance: Recent Results and Future Research Plans

    NASA Astrophysics Data System (ADS)

    Woods, Thomas N.

    2009-05-01

    The solar irradiance, being the radiance integrated over the full disk, is the primary energy input for Earth's environment. Understanding the solar input is key for several terrestrial research topics concerning, to name a few, atmospheric ozone photochemistry, natural forcings on climate change, and improving space weather forecasting. From a solar physics viewpoint, the solar irradiance offers interesting challenges on understanding the sources of the variability of the solar irradiance, which has a strong dependence in wavelength and varies over all time periods from seconds to centuries. Recent solar irradiance results from the TIMED and SORCE satellite missions, such as concerning the current solar cycle minimum, will be presented. In addition, some outstanding questions for solar irradiance research will be addressed within the context of how they can be answered with the new missions, SDO, Glory, and PICARD, that are expected to be launched in late 2009.

  4. Recent forward physics and diffraction results from CMS

    NASA Astrophysics Data System (ADS)

    Veres, Gábor

    2016-07-01

    Recent CMS results on forward physics and diffraction are reviewed. The differential diffractive cross section is measured as a function of ξ = M2X/S in the region dominated by single dissociation (SD) and double dissociation (DD), where MX is the mass of one of the two final-state hadronic systems separated by the largest rapidity gap in the event. The total SD and DD cross sections are extracted. The observation of a hard color-singlet exchange process in events with a large rapidity gap between two leading jets (jet-gap-jet) is reported. The fraction of jet-gap-jet to all dijet events is measured as a function of the second leading jet transverse momentum and the size of the pseudorapidity gap. The measured fractions are compared with predictions as well as Tevatron data.

  5. Recent results on nuclear structure functions for light nuclei

    SciTech Connect

    Kulagin, S. A.; Petti, R.

    2011-09-21

    We discuss the nuclear EMC effect with particular emphasis on recent data for light nuclei including {sup 2}H, {sup 3}He, {sup 4}He, {sup 9}Be, {sup 12}C and {sup 14}N. In order to verify the consistency of available data, we calculate the {chi}{sup 2} deviation between different data sets. We find a good agreement between the results from the NMC, SLAC E139, and HERMES experiments. However, our analysis indicates an overall normalization offset of about 2% in the data from the recent JLab E03-103 experiment with respect to previous data for nuclei heavier than {sup 3}He. We also discuss the extraction of the neutron/proton structure function ratio F{sub 2}{sup n}/F{sub 2}{sup p} from the nuclear ratios {sup 3}He/{sup 2}H and {sup 2}H/{sup 1}H. Our analysis shows that the E03-103 data on {sup 3}He/{sup 2}H require a renormalization of about 3% in order to be consistent with the F{sub 2}{sup n}/F{sub 2}{sup p} ratio obtained from the NMC experiment. After such a renormalization, the {sup 3}He data from the E03-103 data and HERMES experiments are in a good agreement. We also present a detailed comparison between data and model calculations, which include a description of the nuclear binding, Fermi motion and off-shell corrections to the structure functions of bound proton and neutron, as well as the nuclear pion and shadowing corrections.

  6. Recent results of medium wave infrared compressive sensing.

    PubMed

    Mahalanobis, A; Shilling, R; Murphy, R; Muise, R

    2014-12-01

    The application of compressive sensing (CS) for imaging has been extensively investigated and the underlying mathematical principles are well understood. The theory of CS is motivated by the sparse nature of real-world signals and images, and provides a framework in which high-resolution information can be recovered from low-resolution measurements. This, in turn, enables hardware concepts that require much fewer detectors than a conventional sensor. For infrared imagers there is a significant potential impact on the cost and footprint of the sensor. When smaller focal plane arrays (FPAs) to obtain large images are allowed, large formats FPAs are unnecessary. From a hardware standpoint, this benefit is independent of the actual level of compression and effective data rate reduction, which depend on the choice of codes and information recovery algorithm. Toward this end, we used a CS testbed for mid-wave infrared (MWIR) to experimentally show that information at high spatial resolution can be successfully recovered from measurements made with a small FPA. We describe the highly parallel and scalable CS architecture of the testbed, and its implementation using a reflective spatial light modulator and a focal plane array with variable pixel sizes. We also discuss the impact of real-world devices and the effect of sensor calibration that must be addressed in practice. Finally, we present preliminary results of image reconstruction, which demonstrate the testbed operation. These results experimentally confirm that high-resolution spatial information (for tasks such as imaging and target detection) can be successfully recovered from low-resolution measurements. We also discuss the potential system-level benefits of CS for infrared imaging, and some of the challenges that must be addressed in future infrared CS imagers designs. PMID:25607964

  7. Recent experimental results of KSTAR RF heating and current drive

    SciTech Connect

    Wang, S. J. Kim, J.; Jeong, J. H.; Kim, H. J.; Joung, M.; Bae, Y. S.; Kwak, J. G.

    2015-12-10

    The overview of KSTAR activities on ICRH, LHCD and ECH/CD including the last experimental results and future plan aiming for long-pulse high-beta plasma will be presented. Recently we achieved reasonable coupling of ICRF power to H-mode plasma through several efforts to increase system reliability. Power balance will be discussed on this experiment. LHCD is still struggling in the low power regime. Review of antenna spectrum for the higher coupling in H-mode plasma will be tried. ECH/CD provides 41 sec, 0.8 MW of heating power to support high-performance long-pulse discharge. Also, 170 GHz ECH system is integrated with the Plasma Control System (PCS) for the feedback controlling of NTM. Status and plan of ECH/CD will be discussed. Finally, helicon current drive is being prepared for the next stage of KSTAR operation. The hardware preparation and the calculation results of helicon current drive in KSTAR plasma will be discussed.

  8. Recent experimental results of KSTAR RF heating and current drive

    NASA Astrophysics Data System (ADS)

    Wang, S. J.; Kim, J.; Jeong, J. H.; Kim, H. J.; Joung, M.; Bae, Y. S.; Kwak, J. G.

    2015-12-01

    The overview of KSTAR activities on ICRH, LHCD and ECH/CD including the last experimental results and future plan aiming for long-pulse high-beta plasma will be presented. Recently we achieved reasonable coupling of ICRF power to H-mode plasma through several efforts to increase system reliability. Power balance will be discussed on this experiment. LHCD is still struggling in the low power regime. Review of antenna spectrum for the higher coupling in H-mode plasma will be tried. ECH/CD provides 41 sec, 0.8 MW of heating power to support high-performance long-pulse discharge. Also, 170 GHz ECH system is integrated with the Plasma Control System (PCS) for the feedback controlling of NTM. Status and plan of ECH/CD will be discussed. Finally, helicon current drive is being prepared for the next stage of KSTAR operation. The hardware preparation and the calculation results of helicon current drive in KSTAR plasma will be discussed.

  9. Morphology-Composition-Isotopes: Recent Results from Observations

    NASA Astrophysics Data System (ADS)

    Schulz, R.

    This article presents some recent imaging and spectroscopic observations that led to results which are significant for understanding the properties of comet nuclei. The coma morphology and/or composition were investigated for 12 comets belonging to different dynamical classes. The data analysis showed that the coma morphology of three non-periodic comets is not consistent with the general assumption that dynamically new comets still have a relatively uniform nucleus surface and therefore do not exhibit gas and/or dust jets in their coma. The determination of carbon and nitrogen isotopic ratios revealed the same values for all comets investigated at various heliocentric distances. However, the relative abundance of the rare nitrogen isotope 15N is about twice as high as in the Earth's atmosphere. Observations of comets at splitting events and during outbursts led to indications for differences between material from the nucleus surface and the interior. The monitoring of the induced outburst of 9P/Temple revealed that under non-steady state conditions the fast disintegration of species is detectable.

  10. Recent Results of a New Microwave SQUID Multiplexer

    NASA Technical Reports Server (NTRS)

    Hahn, Inseob; Limketkai, B.; Bumble, B.; LeDuc, H. G.

    2007-01-01

    We are developing a proof-of-concept microwave SQUID multiplexer containing four SQUIDs coupled to GHz frequency resonant circuits and fed with a single microwave readout line. The resonators are half-wave coplanar waveguide sections and are similar to the structures used for the microwave kinetic inductance detectors developed in our group. Optimal values for the interdigital gap capacitors were determined to maximize the sensitivity of the transmitted and reflected microwave signal with respect to changes in the dynamic resistance of the SQUID. The dc current-bias line for the SQUID has an in-line inductive high frequency filter to minimize coupling between the bias line and resonator. A high frequency modulation scheme is proposed to eliminate the need for individual flux biasing of the SQUIDs, which extends the dynamic range of the readout. In this scheme a common modulation signal is imposed on each SQUID and the received signal is demodulated at one and two times the modulation frequency to maintain sensitivity at any flux state. We present the recent results of the microwave SQUID multiplexer system operating at a readout frequency range of 10 - 11GHz.

  11. Recent Results and Future Plans from the A4 Experiment

    NASA Astrophysics Data System (ADS)

    Deconinck, Wouter; A4 Collaboration

    2011-04-01

    In the A4 experiment at the MAMI facility in Mainz, Germany, we use the parity-violating asymmetry present in the scattering of longitudinally polarized electrons from unpolarized protons or deuterons to measure the strangeness contribution to the electromagnetic form factors of the nucleon. The A4 experiment uses a PbF2 calorimeter that can be positioned in the forward or backward direction to measure the electrons scattered in a liquid hydrogen or deuterium target. Recent results for the proton at a momentum transfer Q2 = 0 . 23 GeV2 /c2 and the ongoing analysis of the data at Q2 = 0 . 61 GeV2 /c2 will be discussed. Future plans include the measurement of the strangeness form factor at Q2 = 0 . 1 GeV2 /c2 with the current detector to a twice higher precision than the currently available data, and a high precision measurement at an even lower Q2 with an upgraded polarimeter and detector.

  12. The knee and beyond: a review of recent results

    NASA Astrophysics Data System (ADS)

    Chiavassa, Andrea

    2015-08-01

    Primary cosmic rays of energy greater than ∼ 1014eV must be studied by ground based experiments measuring the particles generated in the EAS (Extensive Air Shower) development in atmosphere. These experiments are mainly limited by the systematic uncertainties on an event due to their energy calibration. I will discuss the main sources of these errors: the choice of the hadronic interaction model and of the mass of the primary particle (that cannot be measured on a event by event basis). I will then summarize some of the more recent measurements of the all particle spectrum, and I will show that, keeping into account the differences due to the energy calibration, they all agree on the spectral shape. In addition to the well known change of slope, the so called knee, two faint but significant structures have been measured by different experiments: a concavity around 1016eV and a steepening at ∼ 1017eV. Then I will describe the measurements of the spectra of light and heavy primaries, discussing the claimed spectral features. Using a simple calculation of the elemental spectra (based on the hypothesis that the knee energies follow a Peter's cycle) I will try to discuss if and how these results can be interpreted in a single picture.

  13. Recent results and persisting problems in modeling flow induced coalescence

    SciTech Connect

    Fortelný, I. E-mail: juza@imc.cas.cz; Jza, J. E-mail: juza@imc.cas.cz

    2014-05-15

    The contribution summarizes recent results of description of the flow induced coalescence in immiscible polymer blends and addresses problems that call for which solving. The theory of coalescence based on the switch between equations for matrix drainage between spherical or deformed droplets provides a good agreement with more complicated modeling and available experimental data for probability, P{sub c}, that the collision of droplets will be followed by their fusion. A new equation for description of the matrix drainage between deformed droplets, applicable to the whole range of viscosity ratios, p, of the droplets and matrixes, is proposed. The theory facilitates to consider the effect of the matrix elasticity on coalescence. P{sub c} decreases with the matrix relaxation time but this decrease is not pronounced for relaxation times typical of most commercial polymers. Modeling of the flow induced coalescence in concentrated systems is needed for prediction of the dependence of coalescence rate on volume fraction of droplets. The effect of the droplet anisometry on P{sub c} should be studied for better understanding the coalescence in flow field with high and moderate deformation rates. A reliable description of coalescence in mixing and processing devices requires proper modeling of complex flow fields.

  14. European Fusion Materials Research Program - Recent Results and Future Strategy

    SciTech Connect

    Diegele, E.; Andreani, R.; Laesser, R.; Schaaf, B. van der

    2005-05-15

    The paper reviews the objectives and the status of the current EU long-term materials program. It highlights recent results, discusses some of the key issues and major existing problems to be resolved and presents an outlook on the R and D planned for the next few years. The main objectives of the Materials Development program are the development and qualification of reduced activation structural materials for the Test Blanket Modules (TBMs) in ITER and of low activation structural materials resistant to high fluence neutron irradiation for in-vessel components such as breeding blanket, divertor and first wall in DEMO. The EU strategy assumes: (i) ITER operation starting in 2015 with DEMO relevant Test Blanket Modules to be installed from day one of operation, (ii) IFMIF operation in 2017 and (iii) DEMO final design activities in 2022 to 2025. The EU candidate structural material EUROFER for TBMs has to be fully code qualified for licensing well before 2015. In parallel, research on materials for operation at higher temperatures is conducted following a logical sequence, by supplementing EUROFER with the oxide dispersion strengthened ferritic steels and, thereafter, with fibre-reinforced Silicon Carbide (SiC{sub f}/SiC). Complementary, tungsten alloys are developed as structural material for high temperature applications such as gas-cooled divertors.

  15. Recent high energy gamma-ray results from SAS-2

    NASA Technical Reports Server (NTRS)

    Thompson, D. J.; Fichtel, C. E.; Hartman, R. C.; Kniffen, D. A.; Bignami, G. F.; Ogelman, H. B.; Ozel, M. E.; Tumer, T.; Lamb, R. C.

    1977-01-01

    Recent developments in gamma-ray astronomy due to the results from SAS-2 have focused on two areas. First, the emission from the plane of the Galaxy is the dominant feature in the gamma-ray sky. The galactic latitude and longitude distributions are consistent with the concept that the high-energy radiation originates from cosmic rays interacting with interstellar matter, and the measurements support a galactic origin for cosmic rays. Second, searches of the SAS-2 data for emission from localized sources have shown three strong discrete gamma-ray sources: the Crab nebula and PSR 0531 + 21, the Vela supernova remnant and PSR 0833-45, and a source near galactic coordinates 193 deg longitude, +3 deg latitude, which does not appear to be associated with other known celestial objects. Evidence has also been found for pulsed gamma-ray emission from two other radio pulsars, PSR 1818-04 and PSR 1747-46. A localized source near longitudes 76-80 deg may be associated with the X-ray source Cyg X-3.

  16. Recent results from the T2K experiment

    NASA Astrophysics Data System (ADS)

    Wachala, T.

    2016-07-01

    T2K is a long-baseline experiment which has been designed to measure neutrino oscillations. A high intensity beam of muon neutrinos is produced at the J-PARC accelerator complex and sent towards the near detector station (280meters away from the neutrino source) and the far detector Super-Kamiokande (295km). The change in the measured intensity and composition of the beam is used to provide information on the oscillation parameters. The T2K experiment has discovered electron neutrino appearance with a significance of 7.3 σ , measured the associated θ_{{13}}^{} mixing angle and provided the first hint for the δ_{{CP}}^{} phase. T2K has also delivered the world's best measurement of the θ_{{23}}^{} angle by looking at the disappearance of muon neutrinos. Several useful neutrino cross section measurements have also been performed by the T2K experiment. A summary of the recent oscillation measurements as well as selected cross section results are presented.

  17. Recent Results from KASCADE-Grande and LOPES

    NASA Astrophysics Data System (ADS)

    Kascade-Grande; Lopes Collaboration; Kampert, K.-H.; Apel, W. D.; Arteaga, J. C.; Asch, T.; Badea, F.; Bähren, L.; Bekk, K.; Bertaina, M.; Biermann, P. L.; Blümer, J.; Bozdog, H.; Brancus, I. M.; Brüggemann, M.; Buchholz, P.; Buitink, S.; Cantoni, E.; Chiavassa, A.; Cossavella, F.; Daumiller, K.; de Souza, V.; di Pierro, F.; Doll, P.; Ender, M.; Engel, R.; Engler, J.; Falcke, H.; Finger, M.; Fuhrmann, D.; Gemmeke, H.; Ghia, P. L.; Gils, H. J.; Glasstetter, R.; Grupen, C.; Haungs, A.; Heck, D.; Hörandel, J. R.; Horneffer, A.; Huege, T.; Isar, P. G.; Kang, D.; Kickelbick, D.; Klages, H. O.; Kolotaev, Y.; Krömer, O.; Kuijpers, J.; Lafebre, S.; Link, K.; Łuczak, P.; Ludwig, M.; Mathes, H. J.; Mayer, H. J.; Milke, J.; Melissas, M.; Mitrica, B.; Morello, C.; Navarra, G.; Nehls, S.; Nigl, A.; Oehlschläger, J.; Ostapchenko, S.; Over, S.; Palmieri, N.; Petcu, M.; Pierog, T.; Rautenberg, J.; Rebel, H.; Roth, M.; Saftoiu, A.; Schieler, H.; Schmidt, A.; Schröder, F.; Sima, O.; Singh, K.; Stümpert, M.; Toma, G.; Trinchero, G.; Ulrich, H.; Walkowiak, W.; Weindl, A.; Wochele, J.; Wommer, M.; Zabierowski, J.; Zensus, J. A.; KASCADE-Grande and LOPES Collaboration

    2009-05-01

    KASCADE-Grande is an extensive air-shower experiment located at Forschungszentrum Karlsruhe, Germany. Main parts of the experiment are the Grande array spread over an area of 700×700 m, the original KASCADE array covering 200×200 m with unshielded and shielded detectors, and additional muon tracking devices. This multi-detector system allows to investigate the energy spectrum, composition, and anisotropies of cosmic rays in the energy range up to 1 EeV. LOPES is co-located at the same site to measure radio pulses from extensive air showers in coincidence with KASCADE-Grande. It consists of 30 digital antennas operated in different geometrical configurations. Read out is performed at high bandwidths and rate data processing with the aim to calibrate the emitted signal in the primary energy range of 10-10 eV by making use of reconstructed air-shower observables of KASCADE-Grande. An overview on the performance of both experiments will be given and recent analysis results be reported.

  18. Blazars and gamma-ray cosmology: recent and prospective results

    NASA Astrophysics Data System (ADS)

    Biteau, Jonathan; Williams, David A.

    2016-01-01

    Blazars are dazzling gamma-ray beacons shedding light on some of the darkest mysteries of modern-day astroparticle physics. Some of these mysteries include the light content of the universe, including the UV-IR background, the emission of first stars and of organic molecules; large-scale magnetic fields and their potential primordial origin; spacetime structure, with the potential for Lorentz-invariance violations near the Planck scale; and the search for new interaction channels with photons, e.g. in the form of axion-like particles. These crucial scientific topics can be studied through the signatures of billion-year propagation of GeV-TeV gamma rays that reach Earth from astrophysical sources. We discuss how spectral imprints in data from ground-based and satellite experiments are beginning to answer some of the fundamental questions of gamma-ray cosmology. Recent results, obtained with increased datasets and advanced analysis techniques, are opening the path for future observatories. We examine the areas that remain to be explored, in particular by the proposed Cherenkov Telescope Array, CTA.

  19. The Status and Recent Results of the Telescope Array Experiment

    NASA Astrophysics Data System (ADS)

    Yamazaki, Katsuya

    The Telescope Array (TA) is a cosmic ray observatory of the largest aperture in the northern hemisphere, located in a desert in the western part of Utah, U.S.A., to explore the origin of ultrahigh energy cosmic rays, photons, and neutrinos. The TA employs two types of detectors to observe air showers generated by cosmic rays in the atmosphere: the first is a "surface detector (SD)" of scintillation counters to measure shower particles on the ground, and the second is a "fluorescence detector (FD)" of telescopes installed in three stations to observe fluorescence light, caused by air shower particles, from the atmosphere above the SD array. The TA detectors have been in routine operation since May 2008. We measured the energy spectrum of cosmic rays with energy greater than 1018 eV from our first 4-year data. We found a clear suppression of comic ray intensity above 5 × 1019 eV. This feature is consistent with a theoretical prediction that cosmic rays lose energies due to interaction with cosmic microwave background photons during propagation in the intergalactic space. In this talk, We will present the status of the TA experiment and the recent results, including the energy spectrum, study of the primary mass composition, and searches for anisotropies in the arrival directions. We also briefly describe plans for further extensions.

  20. Editorial: solar radiophysics — recent results on observations and theories

    NASA Astrophysics Data System (ADS)

    Nakariakov, Valery M.; Kashapova, Larisa K.; Yan, Yi-Hua

    2014-07-01

    Solar radiophysics is a rapidly developing branch of solar physics and plasma astrophysics. Solar radiophysics has the goal of analyzing observations of radio emissions from the Sun and understanding basic physical processes operating in quiet and active regions of the solar corona. In the near future, the commissioning of a new generation of solar radio observational facilities, which include the Chinese Spectral Radio Heliograph (CSRH) and the upgrade of the Siberian Solar Radio Telescope (SSRT), and the beginning of solar observations with the Atacama Large Millimeter/submillimeter Array (ALMA), is expected to bring us new breakthrough results of a transformative nature. The Marie-Curie International Research Staff Exchange (MC IRSES) “RadioSun” international network aims to create a solid foundation for the successful exploitation of upcoming solar radio observational facilities, as well as intensive use of the existing observational tools, advanced theoretical modeling of relevant physical processes and observables, and training a new generation of solar radio physicists. The RadioSun network links research teams from China, Czech Republic, Poland, Russia and the UK. This mini-volume presents research papers based on invited reviews and contributed talks at the 1st RadioSun workshop in China. These papers cover a broad range of research topics and include recent observational and theoretical advances in solar radiophysics, MHD seismology of the solar corona, physics of solar flares, generation of radio emission, numerical modeling of MHD and plasma physics processes, charged-particle acceleration and novel instrumentation.

  1. Recent Results from BaBar, Belle, BESIII and CDF

    SciTech Connect

    Olsen, Stephen Lars

    2011-05-23

    A brief report of some recent experimental developments concerning the X, Y and Z charmoniumlike mesons states and other puzzling states from the BaBar, Belle, BESIII and CDF experiments is presented.

  2. Magnetohydrodynamic waves and coronal seismology: an overview of recent results.

    PubMed

    De Moortel, Ineke; Nakariakov, Valery M

    2012-07-13

    Recent observations have revealed that magnetohydrodynamic (MHD) waves and oscillations are ubiquitous in the solar atmosphere, with a wide range of periods. We give a brief review of some aspects of MHD waves and coronal seismology that have recently been the focus of intense debate or are newly emerging. In particular, we focus on four topics: (i) the current controversy surrounding propagating intensity perturbations along coronal loops, (ii) the interpretation of propagating transverse loop oscillations, (iii) the ongoing search for coronal (torsional) Alfvén waves, and (iv) the rapidly developing topic of quasi-periodic pulsations in solar flares. PMID:22665899

  3. Recent development of glacier complex Adygine and resulting risks

    NASA Astrophysics Data System (ADS)

    Falatkova, Kristyna; Sobr, Miroslav; Engel, Zbynek; Jansky, Bohumir

    2015-04-01

    Recent development of glacier complex Adygine and resulting risks Falátková, K., Šobr, M., Engel, Z., Janský, B. Charles University in Prague, Faculty of Science, Prague, Czech republic Glacier complex Adygine (3,400-4,200 m asl) is situated on the northern flank of the Kyrgyz Range, Tien Shan, Kyrgyzstan. The valley downstream is part of National Park Ala Archa, which is popular with tourists, and is heading towards the country's capital - Bishkek. At the study site there is a glacier which is observed since 1960's. The glacier has been monitored by satellite imagery and in last 10 years by on-site geodetic measurement as well. Due to glacier shrinkage several glacial lakes of different genetic types (moraine-dammed, moraine- and rock-dammed, termokarst) have appeared at the site. Nowadays, the lakes are situated on three levels in front of the glacier's terminus and form a cascade, they are also hydrologically connected. The lakes were subjected to detailed bathymetric measurement and some parts of the dams were surveyed by geophysical methods. Especially the newest lakes in proximity of the terminus has been undergoing dynamic changes and may pose a threat in the near future. The risks arising together with changing climatic conditions and retreat of the glacier are associated with mainly three of the lakes. The largest one with area of 3.2 ha is dammed by a rock step overlaid by a moraine. Geophysical research of the dam revealed buried ice and seepage channels in its western part. It is the capacity of these subsurface channels, which are draining the lake throughout the year that represents a weak point in terms of dam stability. The second lake, a termokarst one, is a similar case but drained solely by subsurface channels. Very steep slopes of the lake basin are covered with loose material which could slide down and block the drainage channels. The lake would then fill all the basin (approx. 50,000 m3) very quickly as it is supplied with water from the

  4. Recent Results from the Physics of Colloids in Space

    NASA Technical Reports Server (NTRS)

    Weitz, David A.; Bailey, A.; Christianson, R.; Manley, S.; Prasad, V.; Segre, P.; Gasser, U.; Cipelletti, L.; Schoefield, A.; Pusey, P.

    2002-01-01

    The Physics of Colloids in Space is an experiment which flew in the ISS. Data on several different samples of colloidal particles were obtained. They provided unexpected information about the behavior of the samples in microgravity. The data are currently being analyzed. The most recent findings will be discussed in this talk.

  5. Recent transition crossing results from the Fermilab Main Ring

    SciTech Connect

    Bhat, C.M.; Ng, K.Y.

    1997-03-01

    This paper outlines the known mechanisms for emittance dilution and beam loss during transition crossing. These include scraping, Johnsen`s nonlinear effect, bunch length mismatch, microwave and negative-mass instabilities, and beam loading. A recent experiment on transition crossing performed with 13 proton bunches injected into the Main Ring is discussed.

  6. Corona Mass Ejections: a Summary of Recent Results

    NASA Astrophysics Data System (ADS)

    Gopalswamy, N.

    2010-12-01

    Corona mass ejections (CMEs) have been Recognized as the most energetic phenomenon in the heliosphere, deriving their energy from the stressed magnetic fields on the Sun. This paper highlights some of the recent results obtained on CMEs from the Solar and Heliospheric Observatory (SOHO) and the Solar Terrestrial Relations Observatory (STEREO) missions. The summary of follows the talk. SOHO observations revealed that the CME rate is almost a factor of: Two larger than previously thought and varied with the solar activity cycle in a complex way (eg, high-latitude CMEs occurred in great abundance during the solar years maximum). CMEs were found to interact with other CMEs as well as with other large-scale structures (corona holes), Resulting in deflections and additional particle acceleration. STEREO observations have confirmed the three-dimensional nature of CMEs and shocks the surrounding them. The EUV signatures (flare arcades, Corona dimming, filament Eruption, and EUV waves) associated with CMEs have become vital in the identification of sources from Which solar CMEs erupt. CMEs with speeds exceeding the characteristic speeds of the corona and the interplanetary medium drive shocks, which produce type II radio bursts. The wavelength range of type II bursts depends on the CME kinetic energy: type II bursts with emission components at all wavelengths (metric to kilometric) due to CMEs are of the highest kinetic energy. Some CMEs, as fast as 1600 km / s do not produce type II bursts, while slow CMEs (400 km / s) occasionally produce type II bursts. These observations can be explained as the variation in the ambient flow speed (solar wind) speed and the Alfvén. Not all CME-driven shocks produce type II bursts because they are either subcritical Or do not have the appropriate geometry. The same shocks that produce type II bursts also produce solar energetic particles (SEPS), Whose release near the Sun seems to be delayed with respect to the onset of type II bursts

  7. Coronal Mass Ejections: a Summary of Recent Results

    NASA Technical Reports Server (NTRS)

    Gopalswamy, Nat; Davila, J. M.

    2010-01-01

    Coronal mass ejections (CMEs) have been recognized as the most energetic phenomenon in the heliosphere, deriving their energy from the stressed magnetic fields on the Sun. This paper highlights some of the recent results on CMEs obtained from the Solar and Heliospheric Observatory (SOHO) and the Solar Terrestrial Relations Observatory (STEREO) missions. The summary of the talk follows. SOHO observations revealed that the CME rate is almost a factor of two larger than previously thought and varied with the solar activity cycle in a complex way (e.g., high-latitude CMEs occurred in great abundance during the solar maximum years). CMEs were found to interact with other CMEs as well as with other large-scale structures (coronal holes), resulting in deflections and additional particle acceleration. STEREO observations have confirmed the three-dimensional nature of CMEs and the shocks surrounding them. The EUV signatures (flare arcades, corona) dimming, filament eruption, and EUV waves) associated with CMEs have become vital in the identification of solar sources from which CMEs erupt. CMEs with speeds exceeding the characteristic speeds of the corona and the interplanetary medium drive shocks, which produce type II radio bursts. The wavelength range of type II bursts depends on the CME kinetic energy: type II bursts with emission components at all wavelengths (metric to kilometric) are due to CMEs of the highest kinetic energy. Some CMEs, as fast as 1600 km/s do not produce type II bursts, while slow CMEs (400 km/s) occasionally produce type II bursts. These observations can be explained as the variation in the ambient flow speed (solar wind) and the Alfven speed. Not all CME-driven shocks produce type II bursts because either they are subcritical or do not have the appropriate geometry. The same shocks that produce type II bursts also produce solar energetic particles (SEPs), whose release near the Sun seems to be delayed with respect to the onset of type II bursts

  8. The LIGO Gravitational Wave Observatories:. Recent Results and Future Plans

    NASA Astrophysics Data System (ADS)

    Harry, G. M.; Adhikari, R.; Ballmer, S.; Bayer, K.; Betzwieser, J.; Bochner, B.; Burgess, R.; Cadonati, L.; Chatterji, S.; Corbitt, T.; Csatorday, P.; Fritschel, P.; Goda, K.; Hefetz, Y.; Katsavounidis, E.; Lawrence, R.; Macinnis, M.; Marin, A.; Mason, K.; Mavalvala, N.; Mittleman, R.; Ottaway, D. J.; Pratt, M.; Regimbau, T.; Richman, S.; Rollins, J.; Shoemaker, D. H.; Smith, M.; van Putten, M.; Weiss, R.; Aulbert, C.; Berukoff, S. J.; Cutler, C.; Grunewald, S.; Itoh, Y.; Krishnan, B.; Machenschalk, B.; Mohanty, S.; Mukherjee, S.; Naundorf, H.; Papa, M. A.; Schutz, B. F.; Sintes, A. M.; Williams, P. R.; Colacino, C.; Danzmann, K.; Freise, A.; Grote, H.; Heinzel, G.; Kawabe, K.; Kloevekorn, P.; Lück, H.; Mossavi, K.; Nagano, S.; Rüdiger, A.; Schilling, R.; Smith, J. R.; Weidner, A.; Willke, B.; Winkler, W.; Cusack, B. J.; McClelland, D. E.; Scott, S. M.; Searle, A. C.; Drever, R. W. P.; Tinto, M.; Williams, R.; Buonanno, A.; Chen, Y.; Thorne, K. S.; Vallisneri, M.; Abbott, B.; Anderson, S. B.; Araya, M.; Armandula, H.; Asiri, F.; Barish, B. C.; Barnes, M.; Barton, M. A.; Bhawal, B.; Billingsley, G.; Black, E.; Blackburn, K.; Bogue, L.; Bork, R.; Busby, D.; Cardenas, L.; Chandler, A.; Chapsky, J.; Charlton, P.; Coyne, D.; Creighton, T. D.; D'Ambrosio, E.; Desalvo, R.; Ding, H.; Edlund, J.; Ehrens, P.; Etzel, T.; Evans, M.; Farnham, D.; Fine, M.; Gillespie, A.; Grimmett, D.; Hartunian, A.; Heefner, J.; Hoang, P.; Hrynevych, M.; Ivanov, A.; Jones, L.; Jungwirth, D.; Kells, W.; King, C.; King, P.; Kozak, D.; Lazzarini, A.; Lei, M.; Libbrecht, K.; Lindquist, P.; Liu, S.; Logan, J.; Lyons, T. T.; Mageswaran, M.; Mailand, K.; Majid, W.; Mann, F.; Márka, S.; Maros, E.; Mason, J.; Meshkov, S.; Miyakawa, O.; Miyoki, S.; Mours, B.; Nocera, F.; Ouimette, D.; Pedraza, M.; Rao, S. R.; Redding, D.; Regehr, M. W.; Reilly, K. T.; Reithmaier, K.; Robison, L.; Romie, J.; Rose, D.; Russell, P.; Salzman, I.; Sanders, G. H.; Sannibale, V.; Schmidt, V.; Sears, B.; Seel, S.; Shawhan, P.; Sievers, L.; Smith, M. R.; Spero, R.; Sumner, M. C.; Sylvestre, J.; Takamori, A.; Tariq, H.; Taylor, R.; Tilav, S.; Torrie, C.; Tyler, W.; Vass, S.; Wallace, L.; Ware, B.; Webber, D.; Weinstein, A.; Wen, L.; Whitcomb, S. E.; Willems, P. A.; Wilson, A.; Yamamoto, H.; Zhang, L.; Zweizig, J.; Ganezer, K. S.; Babak, S.; Balasubramanian, R.; Churches, D.; Davies, R.; Sathyaprakash, B.; Taylor, I.; Christensen, N.; Ebeling, C.; Flanagan, É.; Nash, T.; Penn, S.; Dhurandar, S.; Nayak, R.; Sengupta, A. S.; Barker, D.; Barker-Patton, C.; Bland-Weaver, B.; Cook, D.; Gray, C.; Guenther, M.; Hindman, N.; Landry, M.; Lubiński, M.; Matherny, O.; Matone, L.; McCarthy, R.; Mendell, G.; Moreno, G.; Myers, J.; Parameswariah, V.; Raab, F.; Radkins, H.; Ryan, K.; Savage, R.; Schwinberg, P.; Sigg, D.; Vorvick, C.; Worden, J.; Abbott, R.; Carter, K.; Coles, M.; Evans, T.; Frolov, V.; Fyffe, M.; Gretarsson, A. M.; Hammond, M.; Hanson, J.; Kern, J.; Khan, A.; Kovalik, J.; Langdale, J.; Lormand, M.; O'Reilly, B.; Overmier, H.; Parameswariah, C.; Riesen, R.; Rizzi, A.; Roddy, S.; Sibley, A.; Stapfer, G.; Traylor, G.; Watts, K.; Wooley, R.; Yakushin, I.; Zucker, M.; Chickarmane, V.; Daw, E.; Giaime, J. A.; González, G.; Hamilton, W. O.; Johnson, W. W.; Wen, S.; Zotov, N.; McHugh, M.; Whelan, J. T.; Walther, H.; Ageev, A.; Bilenko, I. A.; Braginsky, V. B.; Mitrofanov, V. P.; Tokmakov, K. V.; Vyachanin, S. P.; Camp, J. B.; Kawamura, S.; Belczynski, K.; Grandclément, P.; Kalogera, V.; Kim, C.; Nutzman, P.; Olson, T.; Yoshida, S.; Beausoleil, R.; Bullington, A.; Byer, R. L.; Debra, D.; Fejer, M. M.; Gustafson, E.; Hardham, C.; Hennessy, M.; Hua, W.; Lantz, B.; Robertson, N. A.; Saulson, P. R.; Finn, L. S.; Hepler, N.; Owen, B. J.; Rotthoff, E.; Schlaufman, K.; Shapiro, C. A.; Stuver, A.; Summerscales, T.; Sutton, P. J.; Tibbits, M.; Winjum, B. J.; Anderson, W. G.; Díaz, M.; Johnston, W.; Romano, J. D.; Torres, C.; Ugolini, D.; Aufmuth, P.; Brozek, S.; Fallnich, C.; Goßler, S.; Heng, I. S.; Heurs, M.; Kötter, K.; Leonhardt, V.; Malec, M.; Quetschke, V.; Schrempel, M.; Traeger, S.; Weiland, U.; Welling, H.; Zawischa, I.; Ingley, R.; Messenger, C.; Vecchio, A.; Amin, R.; Castiglione, J.; Coldwell, R.; Delker, T.; Klimenko, S.; Mitselmakher, G.; Mueller, G.; Rakhmanov, M.; Reitze, D. H.; Rong, H.; Sazonov, A.; Shu, Q. Z.; Tanner, D. B.; Whiting, B. F.; Wise, S.; Barr, B.; Bennett, R.; Cagnoli, G.; Cantley, C. A.; Casey, M. M.; Crooks, D. R. M.; Dupuis, R. J.; Elliffe, E. J.; Grant, A.; Heptonstall, A.; Hewitson, M.; Hough, J.; Jennrich, O.; Killbourn, S.; Killow, C. J.; McNamara, P.; Newton, G.; Pitkin, M.; Plissi, M.; Robertson, D. I.; Rowan, S.; Skeldon, K.; Sneddon, P.; Strain, K. A.; Ward, H.; Woan, G.; Chin, D.; Gustafson, R.; Riles, K.; Brau, J. E.; Frey, R.; Ito, M.; Leonor, I.

    2006-02-01

    The LIGO interferometers are operating as gravitational wave observatories, with a noise level near an order of magnitude of the goal and the first scientific data recently taken. This data has been analyzed for four different categories of gravitational wave sources; millisecond bursts, inspiralling binary neutron stars, periodic waves from a known pulsar, and stochastic background. Research and development is also underway for the next generation LIGO detector, Advanced LIGO.

  9. Recent results on hadronic final states from Babar

    NASA Astrophysics Data System (ADS)

    Gary, J. William

    2015-03-01

    Two recent studies from the Babar Collaboration at SLAC are presented on the production of hadrons at low energies. The first is a study of exclusive K+K- production in e+e- annihilation events with initial-state photon radiation. The second is a study of ηc production in two-photon interactions and a three-body Dalitz-plot analysis searching for intermediate scalar meson production in ηc decays.

  10. AFGL ten micron mosaic array spectrometer: Recent results

    NASA Technical Reports Server (NTRS)

    Levan, Paul D.

    1989-01-01

    Recent measurements were made with a novel mosaic array prism spectrometer on long period variable stars of carbon and oxygen-rich atmospheres. These stars have generally large IR excesses and show strong SiC and silicate emission features, respectively. A comparison is provided by published spectra obtained with the IRAS Low Resolution Spectrometer. Emission feature equivalent widths are independent of the absolute photometric level of the spectra and provide information on the relative variation of the feature and continuum fluxes between the epochs of the space and groundbased observations.

  11. Recent nuclear pumped laser results. [gas mixtures and laser plasmas

    NASA Technical Reports Server (NTRS)

    Miley, G. H.; Wells, W. E.; Akerman, M. A.; Anderson, J. H.

    1976-01-01

    Recent direct nuclear pumped laser research has concentrated on experiments with three gas mixtures (Ne-N2, He-Ne-O2, and He-Hg). One mixture has been made to lase and gain has been achieved with the other two. All three of these mixtures are discussed with particular attention paid to He-Hg. Of interest is the 6150-angstroms ion transition in Hg(+). The upper state of this transition is formed directly by charge transfer and by Penning ionization.

  12. Recent Results on Top-Quark Physics at D0

    SciTech Connect

    Bloom, Kenneth

    2015-10-23

    We present the most recent measurements on top-quark physics obtained with Tevatron $p\\bar{p}$ collisions recorded by the D0 experiment at $\\sqrt{s}= 1.96$ TeV. The full Run II data set of 9.7 fb$^{-1}$ is analyzed. Both lepton+jets and dilepton channels of top-quark pair production are used to measure the differential and inclusive cross sections, the forward-backward asymmetries, the top-quark mass, the spin correlations, and the top-quark polarization.

  13. Stellar activity and coronal heating: an overview of recent results.

    PubMed

    Testa, Paola; Saar, Steven H; Drake, Jeremy J

    2015-05-28

    Observations of the coronae of the Sun and of solar-like stars provide complementary information to advance our understanding of stellar magnetic activity, and of the processes leading to the heating of their outer atmospheres. While solar observations allow us to study the corona at high spatial and temporal resolution, the study of stellar coronae allows us to probe stellar activity over a wide range of ages and stellar parameters. Stellar studies therefore provide us with additional tools for understanding coronal heating processes, as well as the long-term evolution of solar X-ray activity. We discuss how recent studies of stellar magnetic fields and coronae contribute to our understanding of the phenomenon of activity and coronal heating in late-type stars. PMID:25897087

  14. Recent Results on T and CP Violation at BABAR

    SciTech Connect

    Perez Perez, Alejandro

    2015-02-06

    CP-violation (CPV) and Time-reversal violation (TRV) are intimately related through the CPT theorem: if one of these discrete symmetries is violated the other one has to be violated in such a way to conserve CPT. Although CPV in the B0B0-bar system has been established by the B-factories, implying indirectly TRV, there is still no direct evidence of TRV. We report on the observation of TRV in the B-meson system performed with a dataset of 468 × 106 BB-bar pairs produced in Υ(4S) decays collected by the BABAR detector at the PEP-II asymmetric-energy e+e- collider at the SLAC National Accelerator Laboratory. We also report on other CPV measurements recently performed on the B-meson system

  15. Stellar activity and coronal heating: an overview of recent results

    PubMed Central

    Testa, Paola; Saar, Steven H.; Drake, Jeremy J.

    2015-01-01

    Observations of the coronae of the Sun and of solar-like stars provide complementary information to advance our understanding of stellar magnetic activity, and of the processes leading to the heating of their outer atmospheres. While solar observations allow us to study the corona at high spatial and temporal resolution, the study of stellar coronae allows us to probe stellar activity over a wide range of ages and stellar parameters. Stellar studies therefore provide us with additional tools for understanding coronal heating processes, as well as the long-term evolution of solar X-ray activity. We discuss how recent studies of stellar magnetic fields and coronae contribute to our understanding of the phenomenon of activity and coronal heating in late-type stars. PMID:25897087

  16. Recent bed rest results and countermeasure development at NASA

    NASA Technical Reports Server (NTRS)

    Hargens, A. R.

    1994-01-01

    Bedrest studies of normal subjects provide opportunities to understand physiologic responses to supine posture and inactivity. Furthermore, head-down tilt has been a valuable procedure to investigate adaptation to microgravity and development of countermeasures to maintain the health and well-being of humans during space-flight. Recent bedrest experiments at NASA have ranged in duration from a few hours to 17 weeks. Acute studies of 6 degrees head-down tilt indicate that elevation of capillary blood pressure from 28 to 34 mm Hg and increased capillary perfusion in tissues of the head cause facial and intracranial edema. Intracranial pressure increases from 2 to 17 mm Hg going from upright posture to 6 degrees head-down tilt. Microvessels of the head have a low capacity to constrict and diminish local perfusion. Elevation of blood and tissue fluid pressures/flow in the head may also explain the higher headward bone density associated with long-term head-down tilt. These mechanistic studies of head-down tilt, along with a better understanding of the relative stresses involved with upright posture and lower body negative pressure, have facilitated development of suitable physiologic countermeasures to maintain astronaut health during microgravity. Presently no exercise hardware is available to provide a blood pressure gradient from head to feet in space. However, recent studies in our laboratory suggest that treadmill exercise using a graded lower-body compression suit and 100 mmHg lower body negative pressure provides equivalent or greater physiologic stress than similar upright exercise on Earth. Therefore, exercise within a lower body negative pressure chamber may provide a cost-effective and simple countermeasure to maintain the cardiovascular and neuro-musculoskeletal systems of astronauts during long-duration flight.

  17. Analysis methodology and recent results of the IGS network combination

    NASA Astrophysics Data System (ADS)

    Ferland, R.; Kouba, J.; Hutchison, D.

    2000-11-01

    A working group of the International GPS Service (IGS) was created to look after Reference Frame (RF) issues and contribute to the densification and improvement of the International Terrestrial Reference Frame (ITRF). One important objective of the Reference Frame Working Group is to generate consistent IGS station coordinates and velocities, Earth Rotation Parameters (ERP) and geocenter estimates along with the appropriate covariance information. These parameters have a direct impact on other IGS products such as the estimation of GPS satellite ephemerides, as well as satellite and station clocks. The information required is available weekly from the Analysis Centers (AC) (cod, emr, esa, gfz, jpl, ngs, sio) and from the Global Network Associate Analysis Centers (GNAAC) (JPL, mit, ncl) using a "Software Independent Exchange Format" (SINEX). The AC are also contributing daily ERPs as part of their weekly submission. The procedure in place simultaneously combines the weekly station coordinates, geocenter and daily ERP estimates. A cumulative solution containing station coordinates and velocity is also updated with each weekly combination. This provides a convenient way to closely monitor the quality of the estimated station coordinates and to have an up to date cumulative solution available at all times. To provide some necessary redundancy, the weekly station coordinates solution is compared against the GNAAC solutions. Each of the 3 GNAAC uses its own software, allowing independent verification of the combination process. The RMS of the coordinate differences in the north, east and up components between the AC/GNAAC and the ITRF97 Reference Frame Stations are 4-10 mm, 5-20 mm and 6-25 mm. The station velocities within continental plates are compared to the NNR-NUVEL1A plate motion model (DeMets et al., 1994). The north, east and up velocity RMS are 2 mm/y, 3 mm/y and 8 mm/y. Note that NNR-NUVEL1A assumes a zero vertical velocity.

  18. Spin Structure of the Nucleon - Status and Recent Results

    SciTech Connect

    Kuhn, Sebastian; Chen, Jian-Ping; Leader, Elliot

    2009-07-01

    After the initial discovery of the so-called "spin crisis in the parton model" in the 1980s, a large set of polarization data in deep inelastic lepton-nucleon scattering was collected at labs like SLAC, DESY and CERN. More recently, new high precision data at large $x$ and in the resonance region have come from experiments at Jefferson Lab. These data, in combination with the earlier ones, allow us to study in detail the polarized parton densities, the $Q^2$ dependence of various moments of spin structure functions, the duality between deep inelastic and resonance data, and the nucleon structure in the valence quark region. Together with complementary data from HERMES, RHIC and COMPASS, we can put new limits on the flavor decomposition and the gluon contribution to the nucleon spin. In this report, we provide an overview of our present knowledge of the nucleon spin structure and give an outlook on future experiments. We focus in particular on the spin structure functions $g_

  19. Overview of Recent DIII-D Experimental Results

    NASA Astrophysics Data System (ADS)

    Fenstermacher, M. E.; DIII-D Team

    2014-10-01

    Recent DIII-D experiments have added to the ITER physics basis and to physics understanding for extrapolation to future devices. Physics mechanisms contributing to resonant magnetic perturbation ELM suppression and QH-mode were identified. The QH-mode operating space was extended to ITER-relevant parameters and predicted Super-H mode performance was observed at high shaping. Upgraded divertor Thomson data was combined with edge modeling to identify the core density limit at divertor detachment. Pedestal studies were done to determine the role of ν*, Zeff and kinetic ballooning mode instabilities in controlling pedestal structure. Injection of massive high-Z gas dissipates magnetic and kinetic energy of runaway electron beams. 3D magnetics data validate several linear MHD codes, including ability to predict neoclassical tearing viscosity torque. Feedback control of applied 3D fields facilitates access to increased βN values above the no-wall limit. The effect of test blanket module (TBM) fields on fast ion losses and momentum transport, and partial correction of TBM fields at high β was achieved. Density gradient driven trapped electron modes and core ne peaking were controlled by electron cyclotron heating suggesting a possible burn control technique. Work supported by the US DOE under DE-FC02-04ER54698 and DE-AC52-07NA27344.

  20. Recent Results From the Opportunity Rover's Exploration of Endeavour Crater, Mars

    NASA Technical Reports Server (NTRS)

    Arvidson, R. E.; Squyres, S. W.; Gellert, R.; Mittlefehldt, D. W.

    2014-01-01

    The Mars Exploration Rover Opportunity is beginning its 11th year of exploration and as of sol 3535 (1/3/14 UTC) has traversed 38,729 m (based on wheel turns) across the plains of Meridiani and the rim of the approx. 22 km wide Noachian Endeavour Crater. Opportunity has investigated ancient sulfate-rich sand-stones (Burns formation) that dominate the plains and formed in ancient playa and dune environments, characterized impact breccias (Shoemaker formation) and their aqueous alteration on Endeavour's Cape York rim segment, and investigated extensive aqueous alteration of rocks on Cape York's Matijevic Hill that stratigraphically underlie Shoemaker formation and predate the Endeavour-forming event. In this abstract results from Opportunity's recent exploration of Endeavour's rim are covered, focusing on comparing what was found on Matijevic Hill with observations acquired on Murray Ridge, where Opportunity will spend its sixth winter at Cook Haven.

  1. Recent Results for the Ferritics Isotopic Tailoring (FIST) Experiment

    SciTech Connect

    Gelles, David S.; Hamilton, Margaret L.; Oliver, Brian M.; Greenwood, Lawrence R.; Ohnuki, Somei; Shiba, K.; Kohno, Y.; Kohyama, Akira; Robertson, J. P.

    2001-10-01

    The results of shear punch testing, microstructural examination, and hydrogen and helium analyses performed on irradiated isotopically tailored alloys are reported for specimens irradiated in the HFIR JP20 experiment.

  2. Tracing recent star formation of red early-type galaxies out to z ∼ 1

    SciTech Connect

    Ko, Jongwan; Lee, Jong Chul; Hwang, Ho Seong; Im, Myungshin; Le Borgne, Damien; Elbaz, David

    2014-08-20

    We study the mid-infrared (IR) excess emission of early-type galaxies (ETGs) on the red sequence at z < 1 using a spectroscopic sample of galaxies in the fields of Great Observatories Origins Deep Survey (GOODS). In the mass-limited sample of 1025 galaxies with M {sub star} > 10{sup 10.5} M {sub ☉} and 0.4 < z < 1.05, we identify 696 Spitzer 24 μm detected (above the 5σ) galaxies and find them to have a wide range of NUV-r and r-[12 μm] colors despite their red optical u – r colors. Even in the sample of very massive ETGs on the red sequence with M {sub star} > 10{sup 11.2} M {sub ☉}, more than 18% show excess emission over the photospheric emission in the mid-IR. The combination with the results of red ETGs in the local universe suggests that the recent star formation is not rare among quiescent, red ETGs at least out to z ∼ 1 if the mid-IR excess emission results from intermediate-age stars or/and from low-level ongoing star formation. Our color-color diagram including near-UV and mid-IR emissions are efficient not only for identifying ETGs with recent star formation, but also for distinguishing quiescent galaxies from dusty star-forming galaxies.

  3. Double-beta decay: Some recent results and developments

    NASA Astrophysics Data System (ADS)

    Avignone, F. T.

    A brief review and status of theoretical issues associated with double-beta decay (ββ-decay) is given. The final results of the measurement of 2ν ββ-decay of 100Mo to the first excited 0 + state in 100Ru are presented prior to publication. Corrections to the earlier PNL/USC/ITEP/YPI measurement of 2ν ββ-decay of 76Ge are also given prior to publication. Finally, a status report and first results of the phase-I of the International Germanium Experiment (IGEX) are presented.

  4. Recent results on. nu. /sub e/ e/sup -/ scattering

    SciTech Connect

    Allen, R.C.; Bharadwaj, V.; Brooks, G.A.; Chen, H.H.; Doe, P.J.; Hausammann, R.; Lee, W.P.; Mahler, H.J.; Potter, M.E.; Rushton, A.M.; and others

    1986-10-15

    The latest results from the neutrino-electron elastic scattering experiment at the LAMPF beam stop are presented. Based on the data sample collected from September 1983 to December 1985, we observed 121 +- 25 events consistent with ..nu../sub x/ e/sup -/ scattering, of which 99 +- 25 events are assigned to ..nu../sub e/ e/sup -/ scattering. The resulting cross section agrees with standard electroweak theory and rules out the constructive interference between weak charge-current and neutral-current interactions.

  5. Recent Results From BaBar in Tau Physics

    SciTech Connect

    Lewczuk, Mateusz; /Victoria U.

    2009-06-25

    The BaBar collaboration has accumulated over 400 million {tau}-pairs which can be used to study charged leptonic and hadronic weak currents to unprecedented precision. This note presents results on lepton universality, measurements of |V{sub us}|, and searches for {tau} decays which violate lepton flavour conservation, or {tau} decays that proceed through a suppressed second class current.

  6. Recent Results from CHAMP Tracking and Accelerometer Data Analysis

    NASA Technical Reports Server (NTRS)

    Luthcke, S. B.; Rowlands, D. D.; Lemoine, F. G.; Nerem, R. S.; Thompson, B.; Pavlis, E.; Williams, T. A.; Colombo, O. L.; Chao, Benjamin F. (Technical Monitor)

    2002-01-01

    The CHAMP mission's unique combination of sensors and orbit configuration will enable unprecedented improvements in modeling and understanding the Earth's static gravity field and its temporal variations. CHAMP is the first of two missions (GRACE to be launched in the early part of 02') that combine a new generation of Global Positioning System (GPS) receivers, a high precision three-axis accelerometer, and star cameras for the precision attitude determination. In order to isolate the gravity signal for science investigations, it is necessary to perform a detailed reduction and analysis of the GPS and Satellite Laser Ranging (SLR) tracking data in conjunction with the accelerometer and attitude data. Precision orbit determination based on the GPS and SLR tracking data will isolate the orbit perturbations, while the accelerometer data will be used to distinguish the non-gravitational forces from those due to the geopotential (static, and time varying). In preparation for the CHAMP and GRACE missions, extensive modifications have been made to NASA/GSFC's GEODYN orbit determination software to enable the simultaneous reduction of spacecraft tracking (e.g. GPS and SLR), three-axis accelerometer and precise attitude data. Several weeks of CHAMP tracking and accelerometer data have been analyzed and the results will be presented. Precision orbit determination analysis based on tracking data alone in addition to results based on the simultaneous reduction of tracking and accelerometer data will be discussed. Results from a calibration of the accelerometer will be presented along with the results from various orbit determination strategies.

  7. Recent results on pathogen intervention during poultry processing

    Technology Transfer Automated Retrieval System (TEKTRAN)

    Slaughter plant – focus has been on Campylobacter and Salmonella - Transport: Campylobacter cross contamination in live haul cages can be lessened by drying cages between uses - Applied after spray wash results in undetectable levels of Campylobacter: Time (24-48h), absorbent powder (2 h), hot air (...

  8. Recent results on the RIA test in IGR reactor

    SciTech Connect

    Asmolov, V.; Yegorova, L.

    1997-01-01

    At the 23d WRSM meeting the data base characterizing results of VVER high burnup fuel rods tests under reactivity-initiated accident (RIA) conditions was presented. Comparison of PWR and VVER failure thresholds was given also. Additional analysis of the obtained results was being carried out during 1996. The results of analysis show that the two different failure mechanisms were observed for PWR and VVER fuel rods. Some factors which can be as the possible reasons of these differences are presented. First of them is the state of preirradiated cladding. Published test data for PWR high burnup fuel rods demonstrated that the PWR high burnup fuel rods failed at the RIA test are characterized by very high level of oxidation and hydriding for the claddings. Corresponding researches were performed at Institute of Atomic Reactors (RLAR, Dimitrovgrad, Russia) for large set of VVER high burnup fuel rods. Results of these investigations show that preirradiated commercial Zr-1%Nb claddings practically keep their initial levels of oxidation and H{sub 2} concentration. Consequently the VVER preirradiated cladding must keep the high level of mechanical properties. The second reason leading to differences between failure mechanisms for two types of high burnup fuel rods can be the test conditions. Now such kind of analysis have been performed by two methods.

  9. Recent Results of Hadal Investigations in the Southern Mariana Trench

    NASA Astrophysics Data System (ADS)

    Fryer, P. B.; Hellebrand, E.; Sharma, S. K.; Acosta-Maeda, T.; Jicha, B. R.; Cameron, J.

    2014-12-01

    The deepest parts of the southern Mariana Trench have variously been interpreted to 1) indicate strike-slip motion along the trench, 2) contain a series of 3 sediment ponds at greater than 10,900 m depth separated from one another by fault-controlled ridges on the subducting plate, and 3) have an even deeper feature in the western-most pond (Vitiaz Deep). Recent lander deployments in all three ponds and the Deepsea Challenger submersible dive by J. Cameron in 2012 showed that the deepest ponds within the Challenger Deep area have nearly unbroken, flat surfaces. One point explored showed veined serpentinite at a depth of 10,800+ m. The potential for active serpentinite-hosted seeps and vent communities was demonstrated for the Shinkai Vent Field at 5,800m depth. Rocks collected using the Wood Hole Oceanographic Institution's hybrid remotely operated vehicle, Nereus, in 2009 from deep (10,879 m) on the incoming plate south of the Challenger Deep, were recovered from the base of a fault scarp where large, columnar-jointed blocks are draped with sediment. Optical microscopy, electron-microprobe and Raman analysis show that they are partially altered massive diabase with altered interstitial glass and containing microbial tubules in vug-filling secondary phases. The chain of seamounts striking NNW, colinear with the Lyra Trough, has been interpreted as a boundary between the Pacific Plate and the seafloor north of the Caroline Ridge. Sediments, drilled from above postulated basement north of the Caroline Ridge are no older that Oligocene. Ar/Ar age dates completed for one rock collected by Nereus in 2009 give a weighted mean plateau age, based on two experiments, of 24.6 +/- 3.2 Ma. Thus, the igneous basement of the subducting plate south of the Challenger Deep is, far younger than the Jurassic Pacific Plate subducting further east. This represents a previously unidentified tectonic plate. With new vehicles and technologies the future for hadal exploration is ripe.

  10. QCD at DOe: A Review of Recent Results

    SciTech Connect

    Sawyer, Lee

    2011-04-26

    We report a variety of measurements of hadronic final states, ranging from elastic scattering of protons to events with highly energetic jets, based on data taken with the DOe experiment at the Fermilab Tevatron proton-antiproton collider.Starting with the non-perturbative regime, we report measurement of the pp-bar elastic differential scattering cross section, using DOe's Forward Proton Detectors (FPD). We present a new way to describe minimum bias events based on angular distributions in {approx_equal}5 million minimum bias pp-bar collisions collected between April 2002 and February 2006 with the DOe detector. We demonstrate that the distribution of {Delta}{phi} in the detector transverse plane between the leading track and all other tracks is a robust observable that can be used for tuning of multiple color interaction models. Pseudorapidity correlations of the {Delta}{phi} distributions are also studied. In addition, we present a measurement of the effective cross section for events produced by double parton scattering.DOe has produced a wide-variety of analyzes of final states involving jets, using a well-understood and calibrated data sample. Inclusive jet cross-sections, dijet production, and multi-jet production have been studied and compared to next-to-leading order (NLO) perturbative Quantum Chromodynamics (pQCD) predictions. After reviewing several published measurements, including the inclusive jet cross section and extraction of the strong coupleing constant {alpha}{sub s}, and the dijet angular dependence and azimuthal decorrelation, we present several recent analyszes. The differential inclusive dijet as a function of the dijet invariant mass Mjj, and the three-jet cross section as a function of the invariant three-jet mass (M{sub 3jet}), are measured in a data set corresponding to an integrated luminosity of 0.7 fb{sup -1}. NLO pQCD calculations are found to be in a reasonable agreement with the measured cross sections.Based on the same data set

  11. Recent Results of TMD Measurements from Jefferson Lab Hall A

    SciTech Connect

    Jiang, Xiaodong

    2013-10-01

    This slide-show presents results on transverse momentum distributions. The presentation covers: target single-spin asymmetry (SSA) (in parity conserving interactions); • Results of JLab Hall A polarized {sup 3}He target TMD measurement; • Semi-­inclusive deep-inelastic scattering channels (E06-010); • Target single-spin asymmetry A{sub UT}, Collins and Sivers SSA on neutron; • Double-spin asymmetry A{sub LT}, extract TMD g{sub 1T} on neutron; • Inclusive channels SSA (E06-010, E05-015, E07-013) • Target SSA: inclusive {sup 3}He(e,e’) quasi-elastic scattering; • Target SSA: inclusive {sup 3}He(e,e’) deep inelastic-elastic scattering; • New SIDIS experiments planned in Hall-A for JLab-12 GeV.

  12. Recent Flight Results of the TRMM Kalman Filter

    NASA Technical Reports Server (NTRS)

    Andrews, Stephen F.; Bilanow, Stephen; Bauer, Frank (Technical Monitor)

    2002-01-01

    The Tropical Rainfall Measuring Mission (TRMM) spacecraft is a nadir pointing spacecraft that nominally controls the roll and pitch attitude based on the Earth Sensor Assembly (ESA) output. TRMM's nominal orbit altitude was 350 km, until raised to 402 km to prolong mission life. During the boost, the ESA experienced a decreasing signal to noise ratio, until sun interference at 393 km altitude made the ESA data unreliable for attitude determination. At that point, the backup attitude determination algorithm, an extended Kalman filter, was enabled. After the boost finished, TRMM reacquired its nadir-pointing attitude, and continued its mission. This paper will briefly discuss the boost and the decision to turn on the backup attitude determination algorithm. A description of the extended Kalman filter algorithm will be given. In addition, flight results from analyzing attitude data and the results of software changes made onboard TRMM will be discussed. Some lessons learned are presented.

  13. Recent charmed baryon Λc results at BESIII

    NASA Astrophysics Data System (ADS)

    Zhou, Xiaokang

    2016-05-01

    BESIII collected 567 pb-1 samples at √{s }=4.599 GeV, which allows us to perform the double-tag technique to measure the rates in the model-independent way near threshold for the first time. Herein, we present our analysis results on branching fractions for 12 Λc+ hadronic decays, including B(Λc +→p K-π+) . In addition, we also report the first model-independent measurement of the absolute branching fraction B(Λc +→Λe+νe) which is the most accurate result to date and improves the previous precision more than twofold.

  14. NASA Space Radiation Risk Project: Overview and Recent Results

    NASA Technical Reports Server (NTRS)

    Blattnig, Steve R.; Chappell, Lori J.; George, Kerry A.; Hada, Megumi; Hu, Shaowen; Kidane, Yared H.; Kim, Myung-Hee Y.; Kovyrshina, Tatiana; Norman, Ryan B.; Nounu, Hatem N.; Peterson, Leif E.; Plante, Ianik; Pluth, Janice M.; Ponomarev, Artem L.; Scott Carnell, Lisa A.; Slaba, Tony C.; Sridharan, Deepa; Xu, Xiaojing

    2015-01-01

    The NASA Space Radiation Risk project is responsible for integrating new experimental and computational results into models to predict risk of cancer and acute radiation syndrome (ARS) for use in mission planning and systems design, as well as current space operations. The project has several parallel efforts focused on proving NASA's radiation risk projection capability in both the near and long term. This presentation will give an overview, with select results from these efforts including the following topics: verification, validation, and streamlining the transition of models to use in decision making; relative biological effectiveness and dose rate effect estimation using a combination of stochastic track structure simulations, DNA damage model calculations and experimental data; ARS model improvements; pathway analysis from gene expression data sets; solar particle event probabilistic exposure calculation including correlated uncertainties for use in design optimization.

  15. Hadron distributions - recent results from the CERN experiment NA44

    SciTech Connect

    Xu, N.

    1996-09-01

    Proton distributions at midrapidity have been measured for 158A{circ}GeV/c Pb + Pb collisions in the focusing spectrometer experiment NA44 at CERN. A high degree of nuclear stopping is found in the truly heavy ion collisions. Systematic results of single particle transverse momentum distributions of pions, kaons, and protons, of 200A-GeV/c S+S and 158A{circ}GeV/c Pb+Pb central collisions will be addressed within the context of thermalization. By comparing these data with thermal and transport models, freeze-out parameters such as the temperature parameter T{sub fo} and mean collective flow velocity ({Beta}) are extracted. Preliminary results of the particle ratios of K{sup -}/K{sup +} and p/p are discussed in the context of cascade models of RQMD and VENUS.

  16. Recent results on two-particle correlations in ALICE

    NASA Astrophysics Data System (ADS)

    Ohlson, Alice

    2016-01-01

    The discovery of correlations between particles separated by several units of pseudorapidity in high-multiplicity pp and p-Pb collisions, reminiscent of structures observed in Pb-Pb collisions, was a challenge to traditional ideas about collectivity in heavy ion collisions. In order to further explore long-range correlations and provide information to theoretical models, correlations between forward trigger muons and mid-rapidity associated hadrons were measured in p-Pb collisions at √sNN = 5.02 TeV. The results demonstrate that the nearside and awayside ridges extend to Δη ∼ ±5 and that the v2 of muons, obtained from subtracting the correlation functions in high- and low-multiplicity events, is (16 ± 6)% higher in the Pb-going than in the p-going direction. The results are compared with AMPT simulations.

  17. Recent flight-test results of optical airdata techniques

    NASA Technical Reports Server (NTRS)

    Bogue, Rodney K.

    1993-01-01

    Optical techniques for measuring airdata parameters were demonstrated with promising results on high performance fighter aircraft. These systems can measure the airspeed vector, and some are not as dependent on special in-flight calibration processes as current systems. Optical concepts for measuring freestream static temperature and density are feasible for in-flight applications. The best feature of these concepts is that the air data measurements are obtained nonintrusively, and for the most part well into the freestream region of the flow field about the aircraft. Current requirements for measuring air data at high angle of attack, and future need to measure the same information at hypersonic flight conditions place strains on existing techniques. Optical technology advances show outstanding potential for application in future programs and promise to make common use of optical concepts a reality. Results from several flight-test programs are summarized, and the technology advances required to make optical airdata techniques practical are identified.

  18. Recent Results from N* Electroproduction Studies with CLAS

    SciTech Connect

    Hovanes Egiyan

    2006-11-01

    During the last eight years a large amount of data on single and two pion electroproduction have been collected using the CEBAF Large Acceptance Spectrometer (CLAS) at Jefferson Lab. The large kinematical coverage of the detector allowed us to perform isobar model fits to extract the transition form factors for the excited states in the second and third resonance regions. The preliminary results for the photocoupling amplitudes from these analyses were presented in this report.

  19. Survey of Recent Results from the PHOBOS Experiment at RHIC

    NASA Astrophysics Data System (ADS)

    Roland, Christof; Back, B. B.; Baker, M. D.; Barton, D. S.; Betts, R. R.; Ballintijn, M.; Bickley, A. A.; Bindel, R.; Budzanowski, A.; Busza, W.; Carroll, A.; Decowski, M. P.; Garcia, E.; George, N.; Gulbrandsen, K.; Gushue, S.; Halliwell, C.; Hamblen, J.; Heintzelman, G. A.; Henderson, C.; Hofman, D. J.; Hollis, R. S.; Hołyński, R.; Holzman, B.; Iordanova, A.; Johnson, E.; Kane, J. L.; Katzy, J.; Khan, N.; Kucewicz, W.; Kulinich, P.; Kuo, C. M.; Lin, W. T.; Manly, S.; McLeod, D.; Michałowski, J.; Mignerey, A. C.; Nouicer, R.; Olszewski, A.; Pak, R.; Park, I. C.; Pernegger, H.; Reed, C.; Remsberg, L. P.; Reuter, M.; Roland, C.; Roland, G.; Rosenberg, L.; Sarin, P.; Sawicki, P.; Skulski, W.; Steadman, S. G.; Steinberg, P.; Stephans, G. S. F.; Stodulski, M.; Sukhanov, A.; Tang, J.-L.; Teng, R.; Trzupek, A.; Vale, C.; van Nieuwenhuizen, G. J.; Verdier, R.; Wadsworth, B.; Wolfs, F. L. H.; Wosiek, B.; Woźniak, K.; Wuosmaa, A. H.; Wysłouch, B.

    2002-10-01

    We present an overview of the latest results for interactions of Au+Au ions at center-of-mass energies of √SNN of 56, 130 and 200 GeV obtained by the PHOBOS collaboration at the Relativistic Heavy Ion Collider (RHIC). These data have allowed us to perform an extensive study of the pseudorapidity density of primary charged particles as a function of incident energy, centrality and pseudorapidity. Our results show a non-trivial evolution of particle densities with both centrality and collision energy, reaching significantly higher values per participating nucleon than at lower energies or in nucleon-nucleon collisions. Further we present results on the azimuthal asymmetry of particle production observed in the √SNN of 130 GeV data set. The observed strong event anisotropy of v2max > 0.06, reaching beyond the value predicted in hadronic cascade models, indicates a closer approach to local thermal equilibration than at lower collision energies. The measured antiparticle-particle ratios of production rates for pions kaons and protons in central Au+Au interactions at √SNN of 130 GeV are compatible with predictions from statistical models, showing an approach to a baryon free region in mid-rapidity with the increase in collision energy.

  20. Recent results from the Viking Labeled Release experiment on Mars

    NASA Technical Reports Server (NTRS)

    Levin, G. V.; Straat, P. A.

    1977-01-01

    The Labeled Release (LR) life detection experiment seeks detection of heterotrophic metabolism by monitoring radio-active gas evolution following the addition of a radioactive nutrient containing seven C-14 labeled organic substrates to surface material. LR results obtained on Mars prior to conjunction showed rapid evolution of radioactive counts upon addition of the nutrient to a fresh surface sample. The responses at both landing sites were quite similar. The additional results summarized in the present paper provide further information on the gas kinetics following a second injection of nutrient and on the effect of 'cold sterilization' of the Martian surface material. Specifically, it is shown that the production of gas from the LR nutrient is remarkably uniform; after reaction approaches completion, addition of more nutrient results in a net loss of the radioactive gas; the reactant in the Mars soil is completely inhibited by heating the soil to 160 C, and is largely inhibited by heating to 46 C. In contrast, exposure to 18 C for 2 sol (1 sol = 24.6 hr) does not appear to inhibit the reaction.

  1. An overview of recent physics results from NSTX

    SciTech Connect

    Kaye, S. M.; Abrams, T.; Ahn, J. -W.; Allain, J. P.; Andre, R.; Andruczyk, D.; Barchfeld, R.; Battaglia, D.; Bhattacharjee, A.; Bedoya, F.; Bell, R. E.; Belova, E.; Berkery, J.; Berry, L.; Bertelli, N.; Beiersdorfer, P.; Bialek, J.; Bilato, R.; Boedo, J.; Bonoli, P.; Boozer, A.; Bortolon, A.; Boyer, M. D.; Boyle, D.; Brennan, D.; Breslau, J.; Brooks, J.; Buttery, R.; Capece, A.; Canik, J.; Chang, C. S.; Crocker, N.; Darrow, D.; Davis, W.; Delgado-Aparicio, L.; Diallo, A.; D'Ippolito, D.; Domier, C.; Ebrahimi, F.; Ethier, S.; Evans, T.; Ferraro, N.; Ferron, J.; Finkenthal, M.; Fonck, R.; Fredrickson, E.; Fu, G. Y.; Gates, D.; Gerhardt, S.; Glasser, A.; Gorelenkov, N.; Gorelenkova, M.; Goumiri, I.; Gray, T.; Green, D.; Guttenfelder, W.; Harvey, R.; Hassanein, A.; Heidbrink, W.; Hirooka, Y.; Hooper, E. B.; Hosea, J.; Humphreys, D.; Jaeger, E. F.; Jarboe, T.; Jardin, S.; Jaworski, M. A.; Kaita, R.; Kessel, C.; Kim, K.; Koel, B.; Kolemen, E.; Kramer, G.; Ku, S.; Kubota, S.; LaHaye, R. J.; Lao, L.; LeBlanc, B. P.; Levinton, F.; Liu, D.; Lore, J.; Lucia, M.; Jr, N. Luhmann; Maingi, R.; Majeski, R.; Mansfield, D.; Maqueda, R.; McKee, G.; Medley, S.; Meier, E.; Menard, J.; Mueller, D.; Munsat, T.; Muscatello, C.; Myra, J.; Nelson, B.; Nichols, J.; Ono, M.; Osborne, T.; Park, J. -K.; Peebles, W.; Perkins, R.; Phillips, C.; Podesta, M.; Poli, F.; Raman, R.; Ren, Y.; Roszell, J.; Rowley, C.; Russell, D.; Ruzic, D.; Ryan, P.; Sabbagh, S. A.; Schuster, E.; Scotti, F.; Sechrest, Y.; Shaing, K.; Sizyuk, T.; Sizyuk, V.; Skinner, C.; Smith, D.; Snyder, P.; Solomon, W.; Sovenic, C.; Soukhanovskii, V.; Startsev, E.; Stotler, D.; Stratton, B.; Stutman, D.; Taylor, C.; Taylor, G.; Tritz, K.; Walker, M.; Wang, W.; Wang, Z.; White, R.; Wilson, J. R.; Wirth, B.; Wright, J.; Yuan, X.; Yuh, H.; Zakharov, L.; Zweben, S. J.

    2015-03-27

    Currently, the National Spherical Torus Experiment (NSTX) is being upgraded to operate at twice the toroidal field and plasma current (up to 1 T and 2 MA), with a second, more tangentially aimed neutral beam (NB) for current and rotation control, allowing for pulse lengths up to 5 s. Recent NSTX physics analyses have addressed topics that will allow NSTX-Upgrade to achieve the research goals critical to a Fusion Nuclear Science Facility. These include producing stable, 100% non-inductive operation in high-performance plasmas, assessing plasma-material interface (PMI) solutions to handle the high heat loads expected in the next-step devices and exploring the unique spherical torus (ST) parameter regimes to advance predictive capability. Non-inductive operation and current profile control in NSTX-U will be facilitated by co-axial helicity injection (CHI) as well as radio frequency (RF) and NB heating. CHI studies using NIMROD indicate that the reconnection process is consistent with the 2D Sweet-Parker theory. Full-wave AORSA simulations show that RF power losses in the scrape-off layer (SOL) increase significantly for both NSTX and NSTX-U when the launched waves propagate in the SOL. Moreover, Toroidal Alfven eigenmode avalanches and higher frequency Alfven eigenmodes can affect NB-driven current through energy loss and redistribution of fast ions. The inclusion of rotation and kinetic resonances, which depend on collisionality, is necessary for predicting experimental stability thresholds of fast growing ideal wall and resistive wall modes. Neutral beams and neoclassical toroidal viscosity generated from applied 3D fields can be used as actuators to produce rotation profiles optimized for global stability. DEGAS-2 has been used to study the dependence of gas penetration on SOL temperatures and densities for the MGI system being implemented on the Upgrade for disruption mitigation. PMI studies have focused on the effect of ELMs and 3D fields on plasma detachment and

  2. An overview of recent physics results from NSTX

    NASA Astrophysics Data System (ADS)

    Kaye, S. M.; Abrams, T.; Ahn, J.-W.; Allain, J. P.; Andre, R.; Andruczyk, D.; Barchfeld, R.; Battaglia, D.; Bhattacharjee, A.; Bedoya, F.; Bell, R. E.; Belova, E.; Berkery, J.; Berry, L.; Bertelli, N.; Beiersdorfer, P.; Bialek, J.; Bilato, R.; Boedo, J.; Bonoli, P.; Boozer, A.; Bortolon, A.; Boyer, M. D.; Boyle, D.; Brennan, D.; Breslau, J.; Brooks, J.; Buttery, R.; Capece, A.; Canik, J.; Chang, C. S.; Crocker, N.; Darrow, D.; Davis, W.; Delgado-Aparicio, L.; Diallo, A.; D'Ippolito, D.; Domier, C.; Ebrahimi, F.; Ethier, S.; Evans, T.; Ferraro, N.; Ferron, J.; Finkenthal, M.; Fonck, R.; Fredrickson, E.; Fu, G. Y.; Gates, D.; Gerhardt, S.; Glasser, A.; Gorelenkov, N.; Gorelenkova, M.; Goumiri, I.; Gray, T.; Green, D.; Guttenfelder, W.; Harvey, R.; Hassanein, A.; Heidbrink, W.; Hirooka, Y.; Hooper, E. B.; Hosea, J.; Humphreys, D.; Jaeger, E. F.; Jarboe, T.; Jardin, S.; Jaworski, M. A.; Kaita, R.; Kessel, C.; Kim, K.; Koel, B.; Kolemen, E.; Kramer, G.; Ku, S.; Kubota, S.; LaHaye, R. J.; Lao, L.; LeBlanc, B. P.; Levinton, F.; Liu, D.; Lore, J.; Lucia, M.; Luhmann, N., Jr.; Maingi, R.; Majeski, R.; Mansfield, D.; Maqueda, R.; McKee, G.; Medley, S.; Meier, E.; Menard, J.; Mueller, D.; Munsat, T.; Muscatello, C.; Myra, J.; Nelson, B.; Nichols, J.; Ono, M.; Osborne, T.; Park, J.-K.; Peebles, W.; Perkins, R.; Phillips, C.; Podesta, M.; Poli, F.; Raman, R.; Ren, Y.; Roszell, J.; Rowley, C.; Russell, D.; Ruzic, D.; Ryan, P.; Sabbagh, S. A.; Schuster, E.; Scotti, F.; Sechrest, Y.; Shaing, K.; Sizyuk, T.; Sizyuk, V.; Skinner, C.; Smith, D.; Snyder, P.; Solomon, W.; Sovenic, C.; Soukhanovskii, V.; Startsev, E.; Stotler, D.; Stratton, B.; Stutman, D.; Taylor, C.; Taylor, G.; Tritz, K.; Walker, M.; Wang, W.; Wang, Z.; White, R.; Wilson, J. R.; Wirth, B.; Wright, J.; Yuan, X.; Yuh, H.; Zakharov, L.; Zweben, S. J.

    2015-10-01

    The National Spherical Torus Experiment (NSTX) is currently being upgraded to operate at twice the toroidal field and plasma current (up to 1 T and 2 MA), with a second, more tangentially aimed neutral beam (NB) for current and rotation control, allowing for pulse lengths up to 5 s. Recent NSTX physics analyses have addressed topics that will allow NSTX-Upgrade to achieve the research goals critical to a Fusion Nuclear Science Facility. These include producing stable, 100% non-inductive operation in high-performance plasmas, assessing plasma-material interface (PMI) solutions to handle the high heat loads expected in the next-step devices and exploring the unique spherical torus (ST) parameter regimes to advance predictive capability. Non-inductive operation and current profile control in NSTX-U will be facilitated by co-axial helicity injection (CHI) as well as radio frequency (RF) and NB heating. CHI studies using NIMROD indicate that the reconnection process is consistent with the 2D Sweet-Parker theory. Full-wave AORSA simulations show that RF power losses in the scrape-off layer (SOL) increase significantly for both NSTX and NSTX-U when the launched waves propagate in the SOL. Toroidal Alfvén eigenmode avalanches and higher frequency Alfvén eigenmodes can affect NB-driven current through energy loss and redistribution of fast ions. The inclusion of rotation and kinetic resonances, which depend on collisionality, is necessary for predicting experimental stability thresholds of fast growing ideal wall and resistive wall modes. Neutral beams and neoclassical toroidal viscosity generated from applied 3D fields can be used as actuators to produce rotation profiles optimized for global stability. DEGAS-2 has been used to study the dependence of gas penetration on SOL temperatures and densities for the MGI system being implemented on the Upgrade for disruption mitigation. PMI studies have focused on the effect of ELMs and 3D fields on plasma detachment and heat

  3. An overview of recent physics results from NSTX

    DOE PAGESBeta

    Kaye, S. M.; Abrams, T.; Ahn, J. -W.; Allain, J. P.; Andre, R.; Andruczyk, D.; Barchfeld, R.; Battaglia, D.; Bhattacharjee, A.; Bedoya, F.; et al

    2015-03-27

    Currently, the National Spherical Torus Experiment (NSTX) is being upgraded to operate at twice the toroidal field and plasma current (up to 1 T and 2 MA), with a second, more tangentially aimed neutral beam (NB) for current and rotation control, allowing for pulse lengths up to 5 s. Recent NSTX physics analyses have addressed topics that will allow NSTX-Upgrade to achieve the research goals critical to a Fusion Nuclear Science Facility. These include producing stable, 100% non-inductive operation in high-performance plasmas, assessing plasma-material interface (PMI) solutions to handle the high heat loads expected in the next-step devices and exploringmore » the unique spherical torus (ST) parameter regimes to advance predictive capability. Non-inductive operation and current profile control in NSTX-U will be facilitated by co-axial helicity injection (CHI) as well as radio frequency (RF) and NB heating. CHI studies using NIMROD indicate that the reconnection process is consistent with the 2D Sweet-Parker theory. Full-wave AORSA simulations show that RF power losses in the scrape-off layer (SOL) increase significantly for both NSTX and NSTX-U when the launched waves propagate in the SOL. Moreover, Toroidal Alfven eigenmode avalanches and higher frequency Alfven eigenmodes can affect NB-driven current through energy loss and redistribution of fast ions. The inclusion of rotation and kinetic resonances, which depend on collisionality, is necessary for predicting experimental stability thresholds of fast growing ideal wall and resistive wall modes. Neutral beams and neoclassical toroidal viscosity generated from applied 3D fields can be used as actuators to produce rotation profiles optimized for global stability. DEGAS-2 has been used to study the dependence of gas penetration on SOL temperatures and densities for the MGI system being implemented on the Upgrade for disruption mitigation. PMI studies have focused on the effect of ELMs and 3D fields on plasma

  4. Recent results from CDF and status of CDF-II

    SciTech Connect

    C. Pagliarone

    2001-12-07

    The CDF detector collected during 1992-95 (Run I) a data sample of 110 pb{sup -1} p{bar p} collisions at a center of mass energy {radical}s = 1.8 TeV. A large variety of physical studies and measurements has been performed using these data. The current paper wants to review results obtained using this data sample as well as discuss the CDF-II upgrades and physical potential of the upgraded CDF Detector (CDF-II) in the Run II.

  5. Recent results in charm decays from Mark III

    SciTech Connect

    Labs, J.F.

    1990-10-01

    Measurements of D{sup 0} {yields} {bar K}{sup 0}{pi}{sup 0}, {bar K}{sup 0}{eta} and {bar K}{sup 0}{eta}{prime} are reported. Preliminary results of a search for the doubly Cabibbo-suppressed decays D{sup +} {yields} K{sup +}{pi}{sup {minus}}{pi}{sup +} and K{sup +}{pi}{sup 0} are also given. Both analyses used 9.3 {plus minus} 0.47 pb{sup {minus}1} of data collected near the {psi}(3770) at SPEAR.

  6. Recent results on parametric analysis of differential Omega error

    NASA Technical Reports Server (NTRS)

    Baxa, E. G., Jr.; Piserchia, P. V.

    1974-01-01

    Previous tests of the differential Omega concept and an analysis of the characteristics of VLF propagation make it possible to delineate various factors which might contribute to the variation of errors in phase measurements at an Omega receiver site. An experimental investigation is conducted to determine the effect of each of a number of parameters on differential Omega accuracy and to develop prediction equations. The differential Omega error form is considered and preliminary results are presented of the regression analysis used to study differential error.

  7. Recent results from the ARGO-YBJ experiment

    SciTech Connect

    Camarri, P.

    2010-03-26

    The ARGO-YBJ experiment at YangBaJing in Tibet (4300 m a.s.l.) has been taking data with its full layout since October 2007. Here we present the first significant results obtained in gamma-ray astronomy and cosmic-ray physics. Emphasis is placed on the analysis of gamma-ray emission from point-like sources (Crab Nebula, MRK 421), on the preliminary limit on the antiproton/proton flux ratio, on the large-scale cosmic-ray anisotropy and on the proton-air cross section. The performance of the detector is also discussed, and the perspectives of the experiment are outlined.

  8. Recent results in high E{sub T} jet production

    SciTech Connect

    Lamoureux, J.; CDF Collaboration

    1997-02-01

    We present results on high E{sub T} jet measurements from CDF and D0. First we show the inclusive jet cross section and compare it to NLO QCD predictions. Preliminary CDF measurements of the {Sigma} E{sub T} cross section are also shown. In order to place limits on the amount of quark compositeness the data can tolerate, we show the dijet angular distributions. Finally, we discuss the inclusive jet cross section measurement at {radical}s = 0.63 TeV and tests of scaling. 13 refs., 15 figs.

  9. KASCADE-Grande Review, Recent Results, Future Endeavors

    NASA Astrophysics Data System (ADS)

    Schoo, S.; Apel, W. D.; Arteaga-Velázquez, J. C.; Beck, K.; Bertaina, M.; Blümer, J.; Bozdog, H.; Brancus, I. M.; Cantoni, E.; Chiavassa, A.; Cossavella, F.; Daumiller, K.; de Souza, V.; Di Pierro, F.; Doll, P.; Engel, R.; Fuhrmann, D.; Gherghel-Lascu, A.; Gils, H. J.; Glasstetter, R.; Grupen, C.; Haungs, A.; Heck, D.; Hörandel, J. R.; Huber, D.; Huege, T.; Kampert, K.-H.; Kang, D.; Klages, H. O.; Link, K.; Łuczak, P.; Mathes, H. J.; Mayer, H. J.; Milke, J.; Mitrica, B.; Morello, C.; Oehlschläger, J.; Ostapchenko, S.; Palmieri, N.; Petcu, M.; Pierog, T.; Rebel, H.; Roth, M.; Schieler, H.; Schröder, F. G.; Sima, O.; Toma, G.; Trinchero, G. C.; Ulrich, H.; Weindl, A.; Wochele, J.; Zabierowski, J.

    A detailed knowledge of the energy spectrum and composition of cosmic rays (CRs) is the most important source of information for solving the riddle of the origin of CRs. The KASCADE experiment and its extension KASCADE-Grande have contributed much to the current knowledge about both the spectrum and composition in the energy range from around 1 PeV to 1 EeV. One of the most important results of the KASCADE experiment is the connection of the knee at a few PeV to a decrease in the flux of light primaries. Later, KASCADE-Grande found a knee-like structure also in the spectrum of heavy elements at around 90 PeV and an ankle-like feature in the spectrum of light elements just above 100 PeV. In this contribution a short review of the experiment will be followed by an overview on the current results on spectrum and composition of CRs and a summary of the further activities within the KASCADE-Grande collaboration related to both, data analysis and data publication.

  10. Recent Results from High Harmonic Fast Wave Experiments on NSTX

    NASA Astrophysics Data System (ADS)

    Taylor, G.; Bell, R. E.; Hosea, J. C.; Leblanc, B. P.; Phillips, C. K.; Valeo, E. J.; Wilson, J. R.; Berry, L. A.; Jaeger, E. F.; Ryan, P. M.; Wilgen, J. B.; Bonoli, P. T.; Wright, J. C.; Harvey, R. W.; Yuh, H.

    2008-11-01

    30 MHz high harmonic fast wave (HHFW) heating and current drive experiments in NSTX at an axial toroidal field of 0.55 T show significantly improved core power deposition and heating efficiency at lower launched toroidal wavenumbers (k||) compared to operation at or below 0.45 T. In addition, lithium wall conditioning has been effectively used to reduce the edge density resulting in the first observation of HHFW core heating at k|| = 3 m-1 in a deuterium plasma. Record core electron temperatures of 5 keV were reached with 3.1 MW HHFW power, and for the first time core HHFW electron heating of NBI-driven deuterium H-mode plasmas was obtained. Motional Stark effect measurements of the current driven in 0.55 T L-mode helium plasmas are consistent with predictions from AORSA and TORIC full-wave simulations. These improved HHFW heating results are attributed to moving the onset density for perpendicular fast wave propagation in the plasma further from the wall [1]. [1] J.C. Hosea, et al., Phys. Plasmas 15, 056104 (2008)

  11. Complementarity and path distinguishability: Some recent results concerning photon pairs

    NASA Technical Reports Server (NTRS)

    Shimony, Abner; Jaeger, Gregg

    1994-01-01

    Two results concerning photon pairs, one previously reported and one new, are summarized. It was previously shown that if the two photons are prepared in a quantum state formed from bar-A and bar-A' for photon 1 and bar-B and bar-B' for photon 2, then both one- and two-particle interferometry can be studied. If upsilon(sub i) is the visibility of one-photon interference fringes (i = 1,2) and upsilon(sub 12) is the visibility of two-photon fringes (a concept which we explicitly define), then upsilon(sub i) squared + upsilon(sub 12) squared is less than or equal to 1. The second result concerns the distinguishability of the paths of photon 2, using the known 2-photon state. A proposed measure E for path distinguishability is based upon finding an optimum strategy for betting on the outcome of a path measurement. Mandel has also proposed a measure of distinguishability P(sub D), defined in terms of the density operator rho of photon 2. We show that E is greater than or equal to P(sub D) and that upsilon(sub 2) = (1 - E(exp 2))exp 1/2.

  12. [Recent results in research on oscillatory chemical reactions].

    PubMed

    Poros, Eszter; Kurin-Csörgei, Krisztina

    2014-01-01

    The mechanisms of the complicated periodical phenomenas in the nature (e.g. hearth beat, sleep cycle, circadian rhythms, etc) could be understood with using the laws of nonlinear chemical systems. In this article the newest result in the research of the subfield of nonlinear chemical dynamics aimed at constructing oscillatory chemical reactions, which are novel either in composition or in configuration, are presented. In the introductory part the concept of chemical periodicity is defined, then the forms as it can appear in time and space and the methods of their study are discussed. Detailed description of the experimental work that has resulted in two significant discoveries is provided. A method was developed to design pH-oscillators which are capable of operating under close conditions. The batch pH-oscillators are more convenient to use in some proposed applications than the equivalent CSTR variant. A redox oscillator that is new in composition was found. The permanganate oxidation of some amino acids was shown to take place according to oscillatory kinetics in a narrow range of the experimental parameters. The KMnO4 - glycine - Na2HPO4 system represents the first example in the family of manganese based oscillators where amino acids is involved. In the conclusion formal analogies between the simple chemical and some more complicated biological oscillatory phenomena are mentioned and the possibility of modeling periodic processes with the use of information gained from the studies of chemical oscillations is pointed out. PMID:25872277

  13. Recent COMPASS results and future prospects for ALICE

    SciTech Connect

    Chung, Suh-Urk

    2015-04-10

    The COMPASS Collaboration has accumulated the world’s highest statistics on the reaction π{sup −} p → π{sup +}π{sup −}π{sup −} p at 190 GeV/c. The results, presented in Section 1, show that a new state J{sup PC} = 1{sup ++} state never reported before, the a{sub 1}(1420), decaying to f{sub 0}(980)π followed by f{sub 0}(980) → ππ. In addition, the Collaboration reports an exotic J{sup PC} = 1{sup −+} state, the π{sub 1}(1600), which cannot be a quarkonium. Both states are likely to be a tetra-quark, i.e. qq{sup ¯}+qq{sup ¯} or a gluonic hybrid, a qq{sup ¯} object with an excited gluon inside it. Section 2 is devoted to a brief discussion of the central production of resonances, which is being investigated by both COMPASS and ALICE collaborations. However, the results are not yet released, so it is limited to a broad discussion of the central production, with emphasis on different analyses dictated by differences in the experimental setup.

  14. Recent Results of NASA's Space Environments and Effects Program

    NASA Technical Reports Server (NTRS)

    Minor, Jody L.; Brewer, Dana S.

    1998-01-01

    The Space Environments and Effects (SEE) Program is a multi-center multi-agency program managed by the NASA Marshall Space Flight Center. The program evolved from the Long Duration Exposure Facility (LDEF), analysis of LDEF data, and recognition of the importance of the environments and environmental effects on future space missions. It is a very comprehensive and focused approach to understanding the space environments, to define the best techniques for both flight and ground-based experimentation, to update the models which predict both the environments and the environmental effects on spacecraft, and finally to ensure that this information is properly maintained and inserted into spacecraft design programs. Formal funding of the SEE Program began initially in FY95. A NASA Research Announcement (NRA) solicited research proposals in the following categories: 1) Engineering environment definitions; 2) Environments and effects design guidelines; 3) Environments and effects assessment models and databases; and, 4) Flight/ground simulation/technology assessment data. This solicitation resulted in funding for eighteen technology development activities (TDA's). This paper will present and describe technical results rom the first set of TDA's of the SEE Program. It will also describe the second set of technology development activities which are expected to begin in January 1998. These new technology development activities will enable the SEE Program to start numerous new development activities in support of mission customer needs.

  15. Spectacular Results from Recent Spitzer Observations of Cassiopeia A

    NASA Astrophysics Data System (ADS)

    Delaney, Tracey

    2006-02-01

    I will present an overview of some of the exciting results from Spitzer observations of the young supernova remnant Cassiopeia A. The images from the MIPS instrument at 24 and 70 microns are dominated by thermal emission from dust within the remnant and clearly show the counterjet extending in the opposite direction from the well-known North-East jet. One of the most surprising results from the 24 micron observations is the presence of infrared light echoes in the vicinity of Cas A. These are thought to result from interstellar dust heated by the explosion and by flares from the compact central object. Images taken in the four IRAC bands show the presence of synchrotron emission. The spectral indices measured between 6cm and IRAC channel 1 at 3.6 micron are flatter than those measured between 6 cm and 20 cm indicating a curved synchrotron spectrum consistent with cosmic-ray-modified shocks. We have also used the IRS instrument in mapping mode to obtainlow-resolution spectra over nearly the entire extent of Cas A. This is the largest single spectral map yet constructed with Spitzer. The spectra, in conjunction with the IRAC images, show that different dust components are associated with different ejecta/circumstellar media components of the remnant. The distribution and composition of the inhomogeneous ejecta and the associated dust indicate that in each direction different nucleosynthetic layers have reached the reverse shock. We have identified diffuse Si and S emission near the center of the remnant that matches the morphology of the absorption seen in the radio at 74 MHz. This material is thought to be ejecta that has not yet encountered the reverse shock but has been photoionized by X-ray and ultraviolet radiation from the remnant. We are able to identify [Ni II] in the remnant. Since the half-life of 56Ni is only 6 days, this material may not be the remains of the Ni synthesized in the supernova explosion. Finally, we have identified strong Ne emission from

  16. Recent Results from the IR Upgrade FEL at Jefferson Lab

    SciTech Connect

    K. Beard; C. Behre; S. Benson; G. Biallas; J. Boyce; D. Douglas; H. F. Dylla; R. Evans; A. Grippo; J. Gubeli; D. Hardy; C. Hernandez-Garcia; K. Jordan; L. Merminga; N. Nishimori; G. Neil; J. Preble; Michelle D. Shinn; T. Siggins; R. Walker; G. Williams; S. Zhang

    2005-08-21

    After demonstrating 10 kW operation with 1 second pulses, the Jefferson Lab program switched to demonstrating high power operation at short wavelengths using a new 8 cm period wiggler and a THz suppression chicane. We report here on the lasing results to date using this new configuration. We have demonstrated a large reduction in THz heating on the mirrors. We have also eliminated heating in the mirror steering assemblies, making operation at high power much more stable. Finally, we have greatly reduced astigmatism in the optical cavity, allowing operation with a very short Rayleigh range. The laser has been tuned from 0.9 to 3.1 microns using the new wiggler. User experiments commenced in April of 2005 with the FEL Upgrade operating over the 1-3 micron range. We are in the process of installing a 5.5 cm permanent magnet wiggler that will give us even larger tuning range and higher power.

  17. Recent Results from the K2K - Neutrino Oscillation Experiment

    NASA Astrophysics Data System (ADS)

    Hill, James E.

    2002-12-01

    The K2K Long-Baseline neutrino oscillation experiment has been aquiring data since mid-1999 and has analysed those up to July of 2001. Fifty-six fully contained events are observed in the fiducial volume of the far detector where 80.6-8.0+7.3 are expected based partly on measurements near the beam production point. There is virtually no background for the contained event search. The methods established in this experiment are crucial for operation of future similar experiments to probe the nature of mixing in the neutral lepton sector, a necessary step in understanding the nature of family structure and of mass itself. A brief history and a few notes about the future and direction of the field precede the description of the experiment and its results.

  18. Recent Results from the Jlab RSS Spin Physics Program

    SciTech Connect

    Mahbubul Khandaker

    2009-12-01

    The spin physics program in Jefferson Lab’s Hall C concentrates on high precision and high resolution studies of the nucleon spin structure that can be extracted from inclusive polarized scattering experiments. The Resonances Spin Structure - RSS experiment has measured nucleon spin structure functions in the resonances region at an intermediate four-momentum transfer Q2 ~ 1.3 GeV2. The polarized target in Hall C could be polarized longitudinally and transversely, allowing extraction of both spin-dependent structure functions g1 and g2. Results on proton and deuteron spin asymmetries A1 and A2, and spin structure functions g1 and g2, are presented here.

  19. Recent Results in Dark Matter Direct Detection Experiments

    SciTech Connect

    Kelso, Christopher Michael

    2012-08-01

    In this dissertation, we study the original excess of low energy events observed by the Co- GeNT collaboration and the annual modulation reported by the DAMA/LIBRA collaboration, and discuss whether these signals could both be the result of the same elastically scattering dark matter particle. We find that, without channeling but when taking into account uncertainties in the relevant quenching factors, a dark matter candidate with a mass of approximately ~7.0 GeV and a cross section with nucleons of σDM-N ~2 x 10-40 cm2 could account for both of these observations. We also compare the region of parameter space favored by DAMA/LIBRA and CoGeNT to the constraints from XENON 10, XENON 100, and CDMS (Si).

  20. Recent Results from Jefferson Lab RSS Spin Physics Program

    SciTech Connect

    Khandaker, Mahbub

    2009-12-17

    The spin physics program in Jefferson Lab's Hall C concentrates on high precision and high resolution studies of the nucleon spin structure that can be extracted from inclusive polarized scattering experiments. The Resonances Spin Structure - RSS experiment has measured nucleon spin structure functions in the resonances region at an intermediate four-momentum transfer Q{sup 2}{approx_equal}1.3 GeV{sup 2}. The polarized target in Hall C could be polarized longitudinally and transversely, allowing extraction of both spin-dependent structure functions g{sub 1} and g{sub 2}. Results on proton and deuteron spin asymmetries A{sub 1} and A{sub 2}, and spin structure functions g{sub 1} and g{sub 2}, are presented here.

  1. Recent results from cosmology and neutrinoless double beta decay

    NASA Astrophysics Data System (ADS)

    Dell’Oro, Stefano; Marcocci, Simone

    2016-05-01

    We quantify the impact of cosmological surveys on the search for neutrinoless double beta decay (0vββ) within the hypothesis that the 0vββ rate is dominated by the Majorana mass of ordinary neutrinos. In particular, we exploit the potential relevance of the work of Palanque-Delabrouille et al. [JCAP 1502, 045 (2015)], whose result seems to favor the normal hierarchy spectrum for the light neutrino masses. The impact of our analysis for the future generation of 0vββ experiments is quite dramatic and motivates further cosmological studies, both theoretically and experimentally. In fact, the allowed values for the Majorana Effective Mass turn out to be < 75meV at 3σ C.L, lowering down to less than 20 meV at 1σ C.L.

  2. Recent results of k-shell ionization by ion collisions

    SciTech Connect

    Avaldi, L.; Milazzo, M.; Mitchell, I.V.; Trivia, G.

    1983-04-01

    The experimental K-shell ionization cross sections of /sub 48/Cd, /sub 50/Sn, /sub 52/Te, /sub 53/I and /sub 56/Ba for alpha particles, between 2.2 MeV and 2.8 MeV, and of /sub 52/Te for protons, between 1.6 and 3 MeV, are presented. The justification for making these measurements comes, on the one hand, in filling a region where, at present, data are sparse: for example, /sub 52/Te ionization cross sections by alpha particles have never been reported before, and, on the other hand, checking between previously reported and diverging sets of experimental results: for example, for alpha particles on tin. In addition, the K-shell ionization cross sections of /sub 52/Te for protons can be considered as an extension of Khelill's measurements.

  3. Recent results from the AMISR Systems (PFISR and RISR)

    NASA Astrophysics Data System (ADS)

    Heinselman, Craig; Nicolls, Michael

    2010-05-01

    The first face of the Advanced Modular Incoherent Scatter Radar (AMISR) was installed at the Poker Flat Research Range north of Fairbanks, Alaska, and became fully operational in March 2007. This system, a phased-array radar for ionospheric studies, had been under development for the National Science Foundation for several years and that development progressed in a staged manner with several prototype systems fielded and tested at different geographic locations. The first panels of the system were field tested near SRI's facility at the ‘Big Dish' above the Stanford University campus in California. Subsequent system testing occurred at the Jicamarca Radio Observatory in Peru and at the HAARP ionospheric modification facility near Gakona in Alaska. The Poker Flat Incoherent Scatter Radar (PFISR) was the first AMISR implementation with full incoherent scatter capabilities at geophysically interesting integration times. Geomagnetically, it is an auroral zone system. A second AMISR face has now been installed very near the magnetic north pole at Resolute Bay, Nunavut, Canada. This face (called RISR for short) is similar, but not identical to, the Poker Flat installation. In addition to its very different geomagnetic location, Resolute Bay's face is also oriented differently and has a number of system improvements adding to the flexibility and utility of that radar. One of the most interesting attributes of the AMISR systems is their ability to steer on a pulse-by-pulse basis. This rapid redirection of the look direction uniquely supports the separation of temporal and spatial changes in the ionospheric plasma. One of the first experiments performed with the completed RISR utilized this steering capability to estimate latitudinal and temporal variations in the electric fields above and to the North of Resolute Bay. This talk will show some of these early results and discuss the details of the system configuration and post processing needed to produce them. It will

  4. CO2CARE - Site Closure Assessment Research - Recent Results

    NASA Astrophysics Data System (ADS)

    Wipki, Mario; Liebscher, Axel; Kühn, Michael; Lüth, Stefan; Durucan, Sevket; Deflandre, Jean-Pierre; Wollenweber, Jens; Chadwick, Andy; Böhm, Gualtiero

    2013-04-01

    The EU project CO2CARE, which started in January 2011, supports the large scale demonstration of CCS technology by addressing requirements of operators and regulators face in terms of CO2 storage site abandonment. The CO2CARE consortium, consisting of 24 project partners from universities, research institutes, and the industry, investigate technologies and procedures for abandonment and post-closure safety, satisfying the regulatory requirements for the transfer of responsibility. Nine key injections sites in Europe, USA, Japan, and Australia, each with a specific (hydro) geological and environmental character, were selected for investigations. These sites can be divided into the CO2 storage types on-shore, off-shore, natural CO2 reservoir, depleted gas reservoirs, and saline aquifers. The project mainly focuses on three key areas: - well abandonment and long-term integrity; - reservoir management and prediction from closure to the long-term; - risk management methodologies for long-term safety. These key areas are in turn closely linked to the three high-level requirements of the EU Directive 2009/31/EC, Article 18 for CO2 storage which are: (i) absence of any detectable leakage, (ii) conformity of actual behaviour of the injected CO2 with the modeled behaviour, and (iii) the storage site is evolving towards a situation of long-term stability. The identification of criteria and the development of site abandonment procedures and technologies, which guarantee the fulfillment of the high-level requirements, are the major objectives in CO2CARE. These criteria have to be fulfilled prior to subsequent transfer of responsibility to the competent authorities, typically 20 or 30 years after site closure. Finally, the essential results of the different working groups in CO2CARE will feed into overall guidelines for regulatory compliance and "Best Practice" for site abandonment. Dissemination of the results will show policy makers and the general public how site abandonment

  5. Recent Results for Solar-System Tests of General Relativity

    NASA Astrophysics Data System (ADS)

    Anderson, J. D.; Lau, E. L.; Turyshev, S.; Williams, J. G.; Nieto, M. M.

    2002-05-01

    We use the current JPL archive of planetary positional data, along with the data-analysis implementation described by Newhall, Standish, and Williams, to solve for all the conventional parameters included in the JPL planetary ephemerides, plus four more parameters specific to tests of General Relativity. Spacecraft ranging data generated by the Deep Space Network (DSN) for NASA missions, and radar ranging measurements to Mercury and Venus are of primary importance. Venus radar ranging has been calibrated for topography by means of altimetry data from the Pioneer 12 Venus orbiter. Martian ranging data consists of orbiter data from Mariner 9 (1971 to 1972) and Mars Global Surveyor (1998 to 2000), as well as lander data from Viking (1976 to 1982) and Pathfinder (1997). In fitting the data, we weight the separate data sets, except for Mars, such that the assumed standard error for each data set is equal to the RMS residual for that particular set after the fit. For Mars, we use a standard error equal to 5 times the RMS residual for each of the four data sets. This is done to compensate for the systematic error from asteroid perturbations. We interpret the resulting parameter errors after the fit as realistic errors, as opposed to formal errors that would result from setting the Mars standard errors equal to their RMS values. The new values of the PPN parameters β and γ , and the solar gravitational quadrupole moment J2, are: β - 1 = -0.0010 +/- 0.0012, γ - 1 = -0.0015 +/- 0.0021, J2 = (2.3 +/- 5.2) x 10-7. The fourth parameter represents a possible time variation ˙ {G} in the gravitational constant. It is unchanged from what we reported last year at the Pasadena meeting. We conclude that the orbits of the inner planets are consistent with the Newtonian inverse-square law of attraction and with General Relativity at the post-Newtonian order O(v2/c2). This work was sponsored by NASA's Space Astrophysics Research and Analysis (SARA) program and was performed at the

  6. Recent results in the Hard-Tube MILO experiment

    SciTech Connect

    Haworth, M.; Hendricks, K.; Englert, T.

    1997-12-31

    The Hard-Tube MILO (Magnetically Insulated transmission Line Oscillator) is an all stainless steel, brazed version of the gigawatt-class, L-band tube reported by Calico et al. The Calico MILO generated a 1.5-GW, 60-ns FWHM microwave pulse using a 500-kV, 60-kA, 500-ns electron beam, while the Hard-Tube MILO generates a 1.8-GW, 170-ns FWHM microwave pulse using a 500-kV, 60-kA, 300-ns electron beam. The authors show that this improved performance is due to suppression unwanted electron emission from the cathode in the region of the first two tube cavities. They also report on experiments to identify the breakdown mechanism in the vacuum radome for the Vlasov antenna which is used as a high-power microwave load for both MILO experiments. Finally, experimental results are presented for an optimized version of the Hard-Tube MILO that computer simulations have shown should generate over 3.0 GW.

  7. Recent results for the ferritics isotopic tailoring (FIST) experiment

    NASA Astrophysics Data System (ADS)

    Gelles, D. S.; Hamilton, M. L.; Oliver, B. M.; Greenwood, L. R.; Ohnuki, S.; Shiba, K.; Kohno, Y.; Kohyama, A.; Robertson, J. P.

    2002-12-01

    An alloy of F82H prepared using the isotope 54Fe in order to encourage H and He production in a fission reactor has been irradiated in the HFIR JP20 experiment at three temperatures to 7 dpa as TEM disks. Irradiated disks were shear punch tested, examined by TEM, analyzed for He and H content, and compared with previous results in order to quantify irradiation hardening due to transmutation-induced H and He. Hardening due to irradiation is found following irradiation at 300 and 400 °C, that is intermediate between that at lower and higher dose, but hardening is negligible following irradiation at 500 °C. Microstructural examinations show typical behavior of irradiation as a function of irradiation temperature, with moderate swelling after 400 °C irradiation but few bubbles after irradiation at 300 °C. Correlations of change in hardening with He and H content show little indication of transmutation-induced hardening, but measured H levels do not agree with predictions and therefore H production and analysis requires further study.

  8. Recent Results for the Ferritics Isotopic Tailoring (FIST) Experiment

    SciTech Connect

    Gelles, David S.; Hamilton, M L.; Oliver, Brian M.; Greenwood, Lawrence R.; Ohnuki, Somei; Shiba, K; Kohno, Yutaka; Kohyama, Akira; Robertson, J P.

    2002-12-01

    An alloy of F82H prepared using the isotope 54 Fe in order to encourage H and He production in a fission reactor has been irradiated in the HFIR JP20 experiment at three temperatures to 7 dpa as TEM disks. Irradiated disks were shear punch tested, examined by TEM, analyzed for He and H content, and compared with previous results in order to quantify irradiation hardening due to transmutation-induced H and He. Hardening due to irradiation is found following irradiation at 300 and 400 C, that is intermediate between that at lower and higher dose, but hardening is negligible following irradiation at 500 C. Microstructural examinations show typical behavior of irradiation as a function of irradiation temperature, with moderate swelling after 400 C irradiation but few bubbles after irradiation at 300 C. Correlations of change in hardening with He and H content show little indication of transmutation-induced hardening, but measured H levels do not agree with predictions and therefore H production and analysis requires further study.

  9. Recent results from Mark II at SPEAR and PEP

    SciTech Connect

    Strait, J.

    1982-04-01

    Three results are presented: (1) The semi-leptonic branching ratio of the ..lambda../sub c/ has been measured at SPEAR to be B(..lambda../sub c//sup +/ ..-->.. e/sup +/X) = (4.5 +- 1.7)%. (2) Properties of tau-pair production have been measured at PEP at square root S = 29 GeV: sigma/sup tau tau//sigma/sup QED/ = 0.97 +- 0.05 +- 0.06; the forward-backward asymmetry is A/sub tau tau/ = (-3.5 +- 5.0)%; inclusive branching ratios are B(tau ..-->.. 1 Prong) = (86 +- 4)%, B(tau ..-->.. 3 Prongs) = (14 +- 4)%, B(tau ..-->.. 5 Prongs) < 0.6% (95% C.L.). (3) A search has been performed for the pair production of charged, point-like, spin 0 particles. The existence of such particles can be ruled out at a 90% confidence level for 3 approx. < M approx. < 10 GeV/c/sup 2/ and branching ratio into hadrons approx. < 90%.

  10. The EXL project, recent results and future perspectives

    NASA Astrophysics Data System (ADS)

    Kiselev, O. A.; EXL Collaboration

    2015-11-01

    The investigation of light-ion induced reactions with exotic beams in inverse kinematics gives access to a broad range of nuclear structure information in the region far off stability. The future FAIR facility, currently under construction at Darmstadt, will provide new opportunities for studying exotic nuclei. The physics program of the EXL project planned as a part of NUclear STructure, Astrophysics and Reactions at FAIR is outlined. It is proposed as a universal high-precision detector setup surrounding the internal target of the storage ring accompanied by a heavy-ion tagging ring detector and a detector for fast protons and neutrons. Possible realization of the setup is briefly discussed. Earlier feasibility studies with stable stored beams and intensive R&D towards the detectors capable of working in ultra-high vacuum conditions helped preparing the final design of the experimental setup. Results of scattering experiments with the stable ions and a very first reaction experiment performed with radioactive ions in the experimental storage ring (ESR) are presented. Future perspectives of the EXL project with a prototype-setup at the ESR and a possible larger-scale setup are also described.

  11. Recent results about fan noise: Its generation, radiation and suppression

    NASA Technical Reports Server (NTRS)

    Feiler, C. E.

    1982-01-01

    Fan noise including its generation, radiation characteristics, and suppression by acoustic treatment is studied. In fan noise generation, results from engine and fan experiments, using inflow control measures to suppress noise sources related to inflow distortion and turbulence, are described. The suppression of sources related to inflow allows the experiments to focus on the fan or engine internal sources. Some of the experiments incorporated pressure sensors on the fan blades to sample the flow disturbances encountered by the blades. From these data some inferences can be drawn about the origins of the disturbances. Also, hot wire measurements of a fan rotor wake field are presented and related to the fan's noise signature. The radiation and the suppression of fan noise are dependent on the acoustic modes generated by the fan. Fan noise suppression and radiation is described by relating these phenomena to the mode cutoff ratio parameter. In addition to its utility in acoustic treatment design and performance prediction, cutoff ratio was useful in developing a simple description of the radiation pattern for broadband fan noise. Some of the findings using the cutoff ratio parameter are presented.

  12. Recent developments and results of new ultraviolet reflective mirror coatings

    NASA Astrophysics Data System (ADS)

    Moore, Christopher S.; Hennessy, John; Jewell, April D.; Nikzad, Shouleh; France, Kevin

    2014-07-01

    Astronomical observations in the Lyman-ultraviolet (91 - 122 nm) are limited in part by the performance of reflective coatings. Currently, the best reflective mirror options for the UV wavelength range of 90 -122 nm are LiF+Al (R ~ 60% from 102 - 200 nm) and SiC (R ~ 30 % from 90 - 200 nm). Higher reflectivity coatings in the 90 - 122 nm range will improve sensitivity and allow for more complex instrumentation. We are working to develop, laboratory test and eventually space test new reflective UV coatings (R > 70% from 90 - 115 nm) that also preserve high-reflectivity performance (R > 80% from 115 - 800 nm) throughout the longer-wavelength vacuum ultraviolet and visible spectral bands. We present a progress report on our work with new protective thin film deposition techniques of metal fluorides (MgF2 and AlF3) on high intrinsic broadband reflective metal (aluminum) surfaces. We present first test results from both traditional and atomic layer deposition processes. In this paper, we discuss the current status of the deposition process, coating substrates, reflectivity measurements for optical through far-ultraviolet wavelengths as well as environmental storage sensitivities.

  13. Recent Results from Gamma-Ray Energy Tracking Array GRETINA

    NASA Astrophysics Data System (ADS)

    Lee, I.-Yang

    2012-10-01

    The gamma-ray energy tracking array GRETINA uses 28 Ge crystals, each with 36 segments, to cover .5ex1 -.1em/ -.15em.25ex4 of the 4π solid angle. The gamma ray tracking technique uses detailed pulse shape information from each of the segments. These pulses are analyzed to determine the energy, time, and three-dimensional positions of all gamma-ray interactions. This information is then utilized, together with the characteristics of Compton scattering and pair-production processes, to track the scattering sequences of the gamma rays. Tracking arrays will give higher efficiency, better peak-to-total ratio and much higher position resolution, and thus increases the detection sensitivity by factors of several hundred compared to current arrays used in nuclear physics research. Particularly, for fast beam experiments tracking will provide spectra quality comparable to that from a Compton suppressed array, such as Gammasphere, while having the position resolution needed for the accurate Doppler correction comparable to detectors designed for good position resolution such as SeGA. GRETINA construction at the 88-Inch Cyclotron at LBNL was completed in March 2011. Extensive engineering and commissioning runs were carried out using radioactive sources, and beams from the Cyclotron until March 2012. The data obtained have been used to debug and improve its performance. After the commissioning period, GRETINA was moved to NSCL MSU and installed at the target position of the S800 spectrograph. The experimental program with a total of twenty four experiments will start in July 2012 after successful commissioning runs. I will present preliminary results from these runs and discuss future research plans.

  14. Overview of Recent Alcator C-Mod Results

    NASA Astrophysics Data System (ADS)

    Marmar, Earl; Alcator C-Mod Team

    2014-10-01

    Alcator C-Mod research currently emphasizes RF heating, current and flow drive, divertor/PMI issues, non-ELMing pedestal regimes with enhanced confinement, and disruption mitigation/runaway dynamics. Stability analysis of I-mode pedestals shows pressures well below the peeling-ballooning limit, as well as expected kinetic ballooning mode thresholds, consistent with the lack of ELMs. Results with the magnetic field aligned ICRF antenna show reductions in high-Z metallic impurities. Implementation of novel ``mirror-probe'' electronics has enabled simultaneous measurements of Te, ne and φ with 1 μs time response using a single probe tip, revealing important properties of the Quasi-Coherent-Mode (QCM) which regulates edge particle transport in EDA H-mode. An Accelerator-based In-situ Material Surveillance diagnostic has been deployed, providing the first between-shot measurements of surface evolution of the all-metal wall. We have observed suppression of boundary turbulence and τE improvement using LHRF into high-density H-modes, with H-factor increases up to 30%. Upgrades which are ready for construction and near term installation on C-Mod include: an off-midplane LH launcher to test theories of improved current drive at high density and an actively heated (900 K) tungsten DEMO-like outer divertor. We are proposing a new facility, ADX, based on Alcator technology, to access advanced magnetic topologies to solve the divertor PMI problem, combined with high-field launch LHCD and ICRF to extend the tokamak to steady-state with reactor relevant tools. Supported by USDOE.

  15. Curiosity explores the base of Aeolis Mons, Gale crater, Mars: Recent Geological and Geochemical Mission Results

    NASA Astrophysics Data System (ADS)

    Gupta, Sanjeev; Vasavada, Ashwin; Crisp, Joy; Grotzinger, John

    2016-04-01

    The Mars Science Laboratory (MSL) Curiosity rover has been exploring sedimentary rocks at the foothills of Aolis Mons since August 2014. Here, an array of fluvial, lacustrine and aeolian strata that show a complex pattern of post-depositional alteration are present. This presentation will summarize the most recent geological and geochemical findings of the MSL mission. Basal outcrops that form the lowest stratigraphic unit of Aeolis Mons, the Murray formation, are characterized predominantly by mudstones with minor intercalated sandstones. The mudstone facies, originally identified at the Pahrump Hills field site, show abundant fine-scale planar laminations throughout the Murray formation succession and is interpreted to record deposition in an ancient lacustrine system in Gale crater. Interbedded cross-stratified sandstones are considered to record fluvio-deltaic incursions into the lake. The lacustrine deposits of the Murray formation are unconformably overlain by much younger sandstones of the Stimson formation. Orbital mapping and in situ observations indicate that the basal strata of the Stimson formation show complex onlap relationships with the underlying Murray formation strata signifying that there was metre-scale palaeotopographic relief on the unconformity surface upon which the Stimson accumulated. The Stimson formation itself is characterized by cross-bedded sandstones with cross-bed sets tens of centimetres in thickness. Sedimentological observations suggest that the Stimson dominantly records deposition by aeolian dunes. Curiosity has made detailed measurements of the geochemistry of the Murray and Stimson formations and associated diagenetic features. Perhaps most surprising has been the discovery of extensive silica enrichment both within mudstones of the Murray formation, perhaps of primary sedimentary or later diagenetic origin, also in as fracture-related diagenetic halos within the Stimson formation. We will describe the nature of this silica

  16. Microbial diversity and methanogenic activity of Antrim Shale formation waters from recently fractured wells.

    PubMed

    Wuchter, Cornelia; Banning, Erin; Mincer, Tracy J; Drenzek, Nicholas J; Coolen, Marco J L

    2013-01-01

    The Antrim Shale in the Michigan Basin is one of the most productive shale gas formations in the U.S., but optimal resource recovery strategies must rely on a thorough understanding of the complex biogeochemical, microbial, and physical interdependencies in this and similar systems. We used Illumina MiSeq 16S rDNA sequencing to analyze the diversity and relative abundance of prokaryotic communities present in Antrim shale formation water of three closely spaced recently fractured gas-producing wells. In addition, the well waters were incubated with a suite of fermentative and methanogenic substrates in an effort to stimulate microbial methane generation. The three wells exhibited substantial differences in their community structure that may arise from their different drilling and fracturing histories. Bacterial sequences greatly outnumbered those of archaea and shared highest similarity to previously described cultures of mesophiles and moderate halophiles within the Firmicutes, Bacteroidetes, and δ- and ε-Proteobacteria. The majority of archaeal sequences shared highest sequence similarity to uncultured euryarchaeotal environmental clones. Some sequences closely related to cultured methylotrophic and hydrogenotrophic methanogens were also present in the initial well water. Incubation with methanol and trimethylamine stimulated methylotrophic methanogens and resulted in the largest increase in methane production in the formation waters, while fermentation triggered by the addition of yeast extract and formate indirectly stimulated hydrogenotrophic methanogens. The addition of sterile powdered shale as a complex natural substrate stimulated the rate of methane production without affecting total methane yields. Depletion of methane indicative of anaerobic methane oxidation (AMO) was observed over the course of incubation with some substrates. This process could constitute a substantial loss of methane in the shale formation. PMID:24367357

  17. Microbial diversity and methanogenic activity of Antrim Shale formation waters from recently fractured wells

    PubMed Central

    Wuchter, Cornelia; Banning, Erin; Mincer, Tracy J.; Drenzek, Nicholas J.; Coolen, Marco J. L.

    2013-01-01

    The Antrim Shale in the Michigan Basin is one of the most productive shale gas formations in the U.S., but optimal resource recovery strategies must rely on a thorough understanding of the complex biogeochemical, microbial, and physical interdependencies in this and similar systems. We used Illumina MiSeq 16S rDNA sequencing to analyze the diversity and relative abundance of prokaryotic communities present in Antrim shale formation water of three closely spaced recently fractured gas-producing wells. In addition, the well waters were incubated with a suite of fermentative and methanogenic substrates in an effort to stimulate microbial methane generation. The three wells exhibited substantial differences in their community structure that may arise from their different drilling and fracturing histories. Bacterial sequences greatly outnumbered those of archaea and shared highest similarity to previously described cultures of mesophiles and moderate halophiles within the Firmicutes, Bacteroidetes, and δ- and ε-Proteobacteria. The majority of archaeal sequences shared highest sequence similarity to uncultured euryarchaeotal environmental clones. Some sequences closely related to cultured methylotrophic and hydrogenotrophic methanogens were also present in the initial well water. Incubation with methanol and trimethylamine stimulated methylotrophic methanogens and resulted in the largest increase in methane production in the formation waters, while fermentation triggered by the addition of yeast extract and formate indirectly stimulated hydrogenotrophic methanogens. The addition of sterile powdered shale as a complex natural substrate stimulated the rate of methane production without affecting total methane yields. Depletion of methane indicative of anaerobic methane oxidation (AMO) was observed over the course of incubation with some substrates. This process could constitute a substantial loss of methane in the shale formation. PMID:24367357

  18. Mixed Material Plasma-Surface Interactions in ITER: Recent Results from the PISCES Group

    SciTech Connect

    Tynan, George R.; Baldwin, Matthew; Doerner, Russell; Hollmann, Eric; Nishijima, Daisuke; Umstadter, Karl; Yu, Jonathan

    2010-05-20

    This paper summarizes recent PISCES studies focused on the effects associated with mixed species plasmas that are similar in composition to what one might expect in ITER. Formation of nanometer scale whiskerlike features occurs in W surfaces exposed to pure He and mixed D/He plasmas and appears to be associated with the formation of He nanometer-scaled bubbles in the W surface. Studies of Be-W alloy formation in Be-seeded D plasmas suggest that this process may be important in ITER all metal wall operational scenarios. Studies also suggest that BeD formation via chemical sputtering of Be walls may be an important first wall erosion mechanism. D retention in ITER mixed materials has also been studied. The D release behavior from beryllium co-deposits does not appear to be a diffusion dominated process, but instead is consistent with thermal release from a number of variable trapping energy sites. As a result, the amount of tritium remaining in codeposits in ITER after baking will be determined by the maximum temperature achieved, rather than by the duration of the baking cycle.

  19. Formation of recent Pb-Ag-Au mineralization by potential sub-surface microbial activity

    NASA Astrophysics Data System (ADS)

    Tornos, Fernando; Velasco, Francisco; Menor-Salván, César; Delgado, Antonio; Slack, John F.; Escobar, Juan Manuel

    2014-08-01

    Las Cruces is a base-metal deposit in the Iberian Pyrite Belt, one of the world’s best-known ore provinces. Here we report the occurrence of major Pb-Ag-Au mineralization resulting from recent sub-surface replacement of supergene oxyhydroxides by carbonate and sulphide minerals. This is probably the largest documented occurrence of recent microbial activity producing an ore assemblage previously unknown in supergene mineralizing environments. The presence of microbial features in the sulphides suggests that these may be the first-described natural bacteriomorphs of galena. The low δ13C values of the carbonate minerals indicate formation by deep anaerobic microbial processes. Sulphur isotope values of sulphides are interpreted here as reflecting microbial reduction in a system impoverished in sulphate. We suggest that biogenic activity has produced around 3.1 × 109 moles of reduced sulphur and 1010 moles of CO2, promoting the formation of ca. 1.19 Mt of carbonates, 114,000 t of galena, 638 t of silver sulphides and 6.5 t of gold.

  20. Formation of recent Pb-Ag-Au mineralization by potential sub-surface microbial activity.

    PubMed

    Tornos, Fernando; Velasco, Francisco; Menor-Salván, César; Delgado, Antonio; Slack, John F; Escobar, Juan Manuel

    2014-01-01

    Las Cruces is a base-metal deposit in the Iberian Pyrite Belt, one of the world's best-known ore provinces. Here we report the occurrence of major Pb-Ag-Au mineralization resulting from recent sub-surface replacement of supergene oxyhydroxides by carbonate and sulphide minerals. This is probably the largest documented occurrence of recent microbial activity producing an ore assemblage previously unknown in supergene mineralizing environments. The presence of microbial features in the sulphides suggests that these may be the first-described natural bacteriomorphs of galena. The low δ(13)C values of the carbonate minerals indicate formation by deep anaerobic microbial processes. Sulphur isotope values of sulphides are interpreted here as reflecting microbial reduction in a system impoverished in sulphate. We suggest that biogenic activity has produced around 3.1 × 10(9) moles of reduced sulphur and 10(10) moles of CO2, promoting the formation of ca. 1.19 Mt of carbonates, 114,000 t of galena, 638 t of silver sulphides and 6.5 t of gold. PMID:25098677

  1. Recent Galaxy Mergers and Residual Star Formation of Red Sequence Galaxies in Galaxy Clusters

    NASA Astrophysics Data System (ADS)

    Sheen, Yun-Kyeong; Yi, Sukyoung K.; Ree, Chang H.; Jaffé, Yara; Demarco, Ricardo; Treister, Ezequiel

    2016-08-01

    This study explored the Galaxy Evolution Explorer ultraviolet (UV) properties of optical red sequence galaxies in four rich Abell clusters at z≤slant 0.1. In particular, we tried to find a hint of merger-induced recent star formation (RSF) in red sequence galaxies. Using the NUV - r\\prime colors of the galaxies, RSF fractions were derived based on various criteria for post-merger galaxies and normal galaxies. Following k-correction, about 36% of the post-merger galaxies were classified as RSF galaxies with a conservative criterion (NUV - r\\prime ≤slant 5), and that number was doubled (∼72%) when using a generous criterion (NUV - r\\prime ≤slant 5.4). The trend was the same when we restricted the sample to galaxies within 0.5 × R 200. Post-merger galaxies with strong UV emission showed more violent, asymmetric features in the deep optical images. The RSF fractions did not show any trend along the clustocentric distance within R 200. We performed a Dressler–Shectman test to check whether the RSF galaxies had any correlation with the substructures in the galaxy clusters. Within R 200 of each cluster, the RSF galaxies did not appear to be preferentially related to the clusters’ substructures. Our results suggested that only 30% of RSF red sequence galaxies show morphological hints of recent galaxy mergers. This implies that internal processes (e.g., stellar mass loss or hot gas cooling) for the supply of cold gas to early-type galaxies may play a significant role in the residual star formation of early-type galaxies at a recent epoch.

  2. Recent Galaxy Mergers and Residual Star Formation of Red Sequence Galaxies in Galaxy Clusters

    NASA Astrophysics Data System (ADS)

    Sheen, Yun-Kyeong; Yi, Sukyoung K.; Ree, Chang H.; Jaffé, Yara; Demarco, Ricardo; Treister, Ezequiel

    2016-08-01

    This study explored the Galaxy Evolution Explorer ultraviolet (UV) properties of optical red sequence galaxies in four rich Abell clusters at z≤slant 0.1. In particular, we tried to find a hint of merger-induced recent star formation (RSF) in red sequence galaxies. Using the NUV - r\\prime colors of the galaxies, RSF fractions were derived based on various criteria for post-merger galaxies and normal galaxies. Following k-correction, about 36% of the post-merger galaxies were classified as RSF galaxies with a conservative criterion (NUV - r\\prime ≤slant 5), and that number was doubled (˜72%) when using a generous criterion (NUV - r\\prime ≤slant 5.4). The trend was the same when we restricted the sample to galaxies within 0.5 × R 200. Post-merger galaxies with strong UV emission showed more violent, asymmetric features in the deep optical images. The RSF fractions did not show any trend along the clustocentric distance within R 200. We performed a Dressler–Shectman test to check whether the RSF galaxies had any correlation with the substructures in the galaxy clusters. Within R 200 of each cluster, the RSF galaxies did not appear to be preferentially related to the clusters’ substructures. Our results suggested that only 30% of RSF red sequence galaxies show morphological hints of recent galaxy mergers. This implies that internal processes (e.g., stellar mass loss or hot gas cooling) for the supply of cold gas to early-type galaxies may play a significant role in the residual star formation of early-type galaxies at a recent epoch.

  3. Initial Satellite Formation Flight Results from the Magnetospheric Multiscale Mission

    NASA Technical Reports Server (NTRS)

    Williams, Trevor; Ottenstein, Neil; Palmer, Eric; Farahmand, Mitra

    2016-01-01

    This paper describes the underlying dynamics of formation flying in a high-eccentricity orbit such as that of the Magnetospheric Multiscale mission. The GPS-based results used for MMS navigation is summarized, as well as the procedures that are used to design the maneuvers used to place the spacecraft into a tetrahedron formation and then maintain it. The details of how to carry out these maneuvers are then discussed. Finally, the numerical results that have been obtained concerning formation flying for the MMS mission to date (e.g. tetrahedron sizes flown, maneuver execution error, fuel usage, etc.) are presented in detail.

  4. Recent advances in understanding the mechanism of hemozoin (malaria pigment) formation.

    PubMed

    Egan, Timothy J

    2008-01-01

    The recent literature on hemozoin/beta-hematin formation is reviewed, with an emphasis on the mechanism of its formation. Recent findings from unrelated organisms that produce hemozoin, namely the malaria parasite Plasmodium falciparum, the worm Schistosoma mansoni and the kissing bug Rhodnius prolixus all of which consume human hemoglobin show that the formation of this crystalline substance occurs within or at the surface of lipids. Biomimetic experimental models of the lipid-water interface as well as computational studies indicate that these lipid environments are probably extraordinarily efficient at producing hemozoin. A rethink is now needed, with a new emphasis on Fe(III)PPIX in non-aqueous environments that mimic lipids and indeed within the lipid environment itself. These findings are explored and discussed in the context of earlier studies on beta-hematin formation. PMID:18226838

  5. Meteor storm evidence against the recent formation of lunar crater Giordano Bruno

    NASA Astrophysics Data System (ADS)

    Withers, Paul

    2001-04-01

    It has been suggested that the formation of the 22 km diameter lunar crater Giordano Bruno was witnessed in June 1178 A.D. To date, this hypothesis has not been well tested. Such an impact on the Earth would be "civilization threatening". Previous studies have shown that the formation of Giordano Bruno would lead to the arrival of 10 million tonnes of ejecta in the Earth's atmosphere in the following week. I calculate that this would cause a week-long meteor storm potentially comparable to the peak of the 1966 Leonids storm. The lack of any known historical records of such a storm is evidence against the recent formation of Giordano Bruno. Other tests of the hypothesis are also discussed, with emphasis on the lack of corroborating evidence for a very recent formation of the crater.

  6. Open clusters and stellar associations: recent results of the Italian community

    NASA Astrophysics Data System (ADS)

    Sciortino, S.

    Current research on open clusters and stellar associations in the Galaxy aims to answer key scientific questions at the hearth of stellar physics, such as the universality of the IMF and its shape in the sub-stellar regime, the star and disk evolution from the PMS to the MS phase, the role played by high energy radiation in the YSO (Young Stellar Object) evolution, and its coronal vs. accretion shock origin, the truly coeval origin of young cluster members and its implication on the still controversial speed of the star formation process. The study of clusters with age greater than 1 Gyr is crucial for understanding the evolution and enrichment of Galaxy disk and its implication for the occurrence of similar phenomena in outer galaxies. I will review recent selected results obtained by scientists of the Italian community in this research area.

  7. Attitudes toward Individuals with Disabilities: Results of a Recent Survey and Implications of Those Results

    ERIC Educational Resources Information Center

    Goreczny, Anthony J.; Bender, Erin E.; Caruso, Guy; Feinstein, Celia S.

    2011-01-01

    Attitudes toward individuals with disabilities are often negative and deleterious, resulting in decreased opportunity and chances at successful integration into the community for these individuals. The purpose of the current study was to investigate attitudes of a group of 129 individuals attending a state-wide conference aimed toward improving…

  8. The ASCD Healthy School Communities Project: Formative Evaluation Results

    ERIC Educational Resources Information Center

    Valois, Robert F.; Lewallen, Theresa C.; Slade, Sean; Tasco, Adriane N.

    2015-01-01

    Purpose: The purpose of this paper is to report the formative evaluation results from the Association for Supervision and Curriculum Development Healthy School Communities (HSC) pilot project. Design/methodology/approach: This study utilized 11 HSC pilot sites in the USA (eight sites) and Canada (three sites). The evaluation question was…

  9. MAPPING THE RECENT STAR FORMATION HISTORY OF THE DISK OF M51

    SciTech Connect

    Kaleida, Catherine; Scowen, Paul A. E-mail: paul.scowen@asu.ed

    2010-08-15

    Using data acquired as part of a unique Hubble Heritage imaging program of broadband colors of the interacting spiral system M51/NGC 5195, we have conducted a photometric study of the stellar associations across the entire disk of the galaxy in order to assess trends in size, luminosity, and local environment associated with the recent star formation (SF) activity in the system. Starting with a sample of over 900 potential associations, we have produced color-magnitude and color-color diagrams for the 120 associations that were deemed to be single-aged. It has been found that main-sequence (MS) turnoffs are not evident for the vast majority of the stellar associations in our set, potentially due to the overlap of isochronal tracks at the high mass end of the MS, and the limited depth of our images at the distance of M51. In order to obtain ages for more of our sample, we produced model spectral energy distributions (SEDs) to fit to the data from the GALEXEV simple stellar population models of Bruzual and Charlot. These SEDs can be used to determine age, size, mass, metallicity, and dust content of each association via a simple {chi}{sup 2} minimization to each association's B-, V-, and I-band fluxes. The derived association properties are mapped as a function of location, and recent trends in SF history of the galaxy are explored in light of these results. This work is the first phase in a program that will compare these stellar systems with their environments using ultraviolet data from the Galaxy Evolution Explorer and infrared data from Spitzer, and ultimately we plan to apply the same stellar population mapping methodology to other nearby face-on spiral galaxies.

  10. Deep Hubble Space Telescope Imaging of Sextans A. I. The Spatially Resolved Recent Star Formation History

    NASA Astrophysics Data System (ADS)

    Dohm-Palmer, Robbie C.; Skillman, Evan D.; Mateo, Mario; Saha, Abi; Dolphin, Andrew; Tolstoy, Eline; Gallagher, Jay S.; Cole, Andrew A.

    2002-02-01

    We have measured stellar photometry from deep Cycle 7 Hubble Space Telescope/WFPC2 imaging of the dwarf irregular galaxy Sextans A. The imaging was taken in three filters: F555W (V; eight orbits), F814W (I; 16 orbits), and F656N (Hα one orbit). Combining these data with Cycle 5 WFPC2 observations provides nearly complete coverage of the optically visible portion of the galaxy. The Cycle 7 observations are nearly 2 mag more sensitive than the Cycle 5 observations, which provides unambiguous separation of the faint blue helium-burning stars (BHeB stars) from contaminant populations. The depth of the photometry allows us to compare recent star formation histories recovered from both the main-sequence stars and the BHeB stars for the last 300 Myr. The excellent agreement between these independent star formation rate (SFR) calculations is a resounding confirmation for the legitimacy of using the BHeB stars to calculate the recent SFR. Using the BHeB stars we have calculated the global star formation history over the past 700 Myr. The history calculated from the Cycle 7 data is remarkably identical to that calculated from the Cycle 5 data, implying that both halves of the galaxy formed stars in concert. We have also calculated the spatially resolved star formation history, combining the fields from the Cycle 5 and Cycle 7 data. The star-forming regions are found in three major zones of the galaxy. One of these zones is extremely young, consisting of only a single star-forming region that is less than 20 Myr old. Two of these zones are associated with high column density neutral gas, while the third, and oldest, is not. Our interpretation of this pattern of star formation is that it is an orderly stochastic process. Star formation begins on the edge of a gas structure and progressively eats away at the cloud, breaking it up and inducing further star formation. A more quantitative analysis of the star formation process must await a larger sample of galaxies with spatially

  11. Recent Developments in Hardware-in-the-Loop Formation Navigation and Control

    NASA Technical Reports Server (NTRS)

    Mitchell, Jason W.; Luquette, Richard J.

    2005-01-01

    The Formation Flying Test-Bed (FFTB) at NASA Goddard Space Flight Center (GSFC) provides a hardware-in-the-loop test environment for formation navigation and control. The facility is evolving as a modular, hybrid, dynamic simulation facility for end-tc-end guidance, navigation, and control (GN&C) design and analysis of formation flying spacecraft. The core capabilities of the FFTB, as a platform for testing critical hardware and software algorithms in-the-loop, are reviewed with a focus on many recent improvements. Two significant upgrades to the FFTB are a message-oriented middleware (MOM) architecture, and a software crosslink for inter-spacecraft ranging. The MOM architecture provides a common messaging bus for software agents, easing integration, arid supporting the GSFC Mission Services Evolution Center (GMSEC) architecture via software bridge. Additionally, the FFTB s hardware capabilities are expanding. Recently, two Low-Power Transceivers (LPTs) with ranging capability have been introduced into the FFTB. The LPT crosslinks will be connected to a modified Crosslink Channel Simulator (CCS), which applies realistic space-environment effects to the Radio Frequency (RF) signals produced by the LPTs.

  12. Late Pop III Star Formation During the Epoch of Reionization: Results from the Renaissance Simulations

    NASA Astrophysics Data System (ADS)

    Xu, Hao; Norman, Michael L.; O’Shea, Brian W.; Wise, John H.

    2016-06-01

    We present results on the formation of Population III (Pop III) stars at redshift 7.6 from the Renaissance Simulations, a suite of extremely high-resolution and physics-rich radiation transport hydrodynamics cosmological adaptive-mesh refinement simulations of high-redshift galaxy formation performed on the Blue Waters supercomputer. In a survey volume of about 220 comoving Mpc3, we found 14 Pop III galaxies with recent star formation. The surprisingly late formation of Pop III stars is possible due to two factors: (i) the metal enrichment process is local and slow, leaving plenty of pristine gas to exist in the vast volume; and (ii) strong Lyman–Werner radiation from vigorous metal-enriched star formation in early galaxies suppresses Pop III formation in (“not so”) small primordial halos with mass less than ˜3 × 107 M ⊙. We quantify the properties of these Pop III galaxies and their Pop III star formation environments. We look for analogs to the recently discovered luminous Ly α emitter CR7, which has been interpreted as a Pop III star cluster within or near a metal-enriched star-forming galaxy. We find and discuss a system similar to this in some respects, however, the Pop III star cluster is far less massive and luminous than CR7 is inferred to be.

  13. Evidence of authigenic vivianite formation in a recent lake sediment due to an iron amendment

    NASA Astrophysics Data System (ADS)

    Rothe, Matthias; Frederichs, Thomas; Eder, Michaela; Kleeberg, Andreas; Hupfer, Michael

    2014-05-01

    Pore water chemistry and equilibrium calculations indicated supersaturation of the ferrous iron phosphate mineral vivianite throughout the upper 30 cm of the iron-rich lake sediments of dimictic lake Groß-Glienicker See, Berlin (Germany). Phosphorus (P) bound in the crystal lattice of the mineral is supposed to be immobilized since vivianite is stable under anoxic, reducing sedimentary conditions. Thus, vivianite formation can be an important process contributing to P retention during early diagenesis. Application of a heavy-liquid separation enabled to identify vivianite by means of X-ray diffraction. Electron micrographs showed spherical nodules consisting of platy- and needle-shaped crystal aggregates with diameters between 50 and 120 μm. Inclusions of diatom shells and other organic debris confirmed the authigenic origin of the dark blue coloured nodules. Vivianite deposits were restricted to the upper 22 cm of the sediment although supersaturation even increased in subjacent pore waters. The high enrichment of vivianite aggregates after sediment preparation combined with magnetic hysteresis measurements allowed to assess the significance of vivianite formation for P burial in aquatic systems. From our results we conclude that vivianite formation was triggered by an artificial iron amendment more than 20 years ago that aimed at reducing the P content of the lake's water body. Furthermore, our results indicate that vivianite formation is located closely beneath the sediment-water interface and that equilibrium calculations, i.e. supersaturated pore water, alone cannot serve as a reliable predictor for the in situ formation of vivianite.

  14. Recent Star Formation in the Wolf-Rayet BCDG MRK 1094

    NASA Astrophysics Data System (ADS)

    Mendez, D. I.; Cairos, L. M.; Esteban, C.; Vilchez, J. M.

    1998-12-01

    We present preliminary results on high resolution Hα imaging of the Wolf-Rayet blue compact dwarf galaxy (BCDG) Mrk 1094. This galaxy presents a bar-shape structure and is currently undergoing a strong star formation burst distributed in several knots. Spatially resolved photometry of the different knots indicates that star formation seems to be propagating from the center outwards all along the bar. We discuss the different processes that could explain these observational facts. In this sense, Mrk 1094 is the first BCDG in which this kind of phenomena is detected.

  15. RECENT STAR FORMATION IN THE LEADING ARM OF THE MAGELLANIC STREAM

    SciTech Connect

    Casetti-Dinescu, Dana I.; Bidin, Christian Moni; Girard, Terrence M.; Van Altena, William F.; Méndez, Réne A.; Vieira, Katherine; Korchagin, Vladimir I. E-mail: dana.casetti@yale.edu E-mail: william.vanaltena@yale.edu E-mail: ramendez.uchile@gmail.com E-mail: vkorchagin@sfedu.ru

    2014-04-01

    Strongly interacting galaxies undergo a short-lived but dramatic phase of evolution characterized by enhanced star formation, tidal tails, bridges, and other morphological peculiarities. The nearest example of a pair of interacting galaxies is the Magellanic Clouds, whose dynamical interaction produced the gaseous features known as the Magellanic Stream trailing the pair's orbit about the Galaxy, the bridge between the Clouds, and the leading arm (LA), a wide and irregular feature leading the orbit. Young, newly formed stars in the bridge are known to exist, giving witness to the recent interaction between the Clouds. However, the interaction of the Clouds with the Milky Way (MW) is less well understood. In particular, the LA must have a tidal origin; however, no purely gravitational model is able to reproduce its morphology and kinematics. A hydrodynamical interaction with the gaseous hot halo and disk of the Galaxy is plausible as suggested by some models and supporting neutral hydrogen (H I) observations. Here we show for the first time that young, recently formed stars exist in the LA, indicating that the interaction between the Clouds and our Galaxy is strong enough to trigger star formation in certain regions of the LA—regions in the outskirts of the MW disk (R ∼ 18 kpc), far away from the Clouds and the bridge.

  16. The recent formation of Saturn's moonlets from viscous spreading of the main rings.

    PubMed

    Charnoz, Sébastien; Salmon, Julien; Crida, Aurélien

    2010-06-10

    The regular satellites of the giant planets are believed to have finished their accretion concurrent with the planets, about 4.5 Gyr ago. A population of Saturn's small moons orbiting just outside the main rings are dynamically young (less than 10(7) yr old), which is inconsistent with the formation timescale for the regular satellites. They are also underdense ( approximately 600 kg m(-3)) and show spectral characteristics similar to those of the main rings. It has been suggested that they accreted at the rings' edge, but hitherto it has been impossible to model the formation process fully owing to a lack of computational power. Here we report a hybrid simulation in which the viscous spreading of Saturn's rings beyond the Roche limit (the distance beyond which the rings are gravitationally unstable) gives rise to the small moons. The moonlets' mass distribution and orbital architecture are reproduced. The current confinement of the main rings and the existence of the dusty F ring are shown to be direct consequences of the coupling of viscous evolution and satellite formation. Saturn's rings, like a mini protoplanetary disk, may be the last place where accretion was recently active in the Solar System, some 10(6)-10(7) yr ago. PMID:20535205

  17. Recent Results on Charm and Tau Physics from BaBar And Belle

    SciTech Connect

    Salvatore, Fabrizio F.; /Royal Holloway, U. of London

    2007-10-15

    Recent results on charm and tau physics obtained at the BABAR and Belle experiments are presented in this article. The charm section will be focused on the most recent results on D{sup 0}{bar D}{sup 0} mixing at Belle and on the measurement of the pseudoscalar decay constant f{sub Ds} using charm tagged e+e- events at BABAR. In the tau section the recent results on Lepton Flavor Violation from tau decays will be discussed, as well as the recent result on the rare decay {tau}{sup -} {yields} 3{pi}{sup -}2{pi}{sup +}2{pi}{sup 0}{nu}{sub {tau}} at BABAR and the measurement of the {tau} lepton mass at Belle.

  18. Compendium of Test Results of Recent Single Event Effect Tests Conducted by the Jet Propulsion Laboratory

    NASA Technical Reports Server (NTRS)

    McClure, Steven S.; Allen, Gregory R.; Irom, Farokh; Scheick, Leif Z.; Adell, Philippe C.; Miyahira, Tetsuo F.

    2010-01-01

    This paper reports heavy ion and proton-induced single event effect (SEE) results from recent tests for a variety of microelectronic devices. The compendium covers devices tested over the last two years by the Jet Propulsion Laboratory.

  19. Ediacaran paleomagnetic results from feeder dikes of the Catoctin Formation

    NASA Astrophysics Data System (ADS)

    Hankard, F.; Domeier, M. M.; Bentley, C.; Van Der Voo, R.

    2011-12-01

    A paleomagnetic study undertaken sixteen years ago on the Catoctin basalts, feeder dikes and sills (Meert et al, 1994) did not bring firm and strong conclusions about the paleoposition of Laurentia during the Ediacaran period. The results were rather complex and sketchy. In effect, three paleomagnetic directions derived from this study were interpreted as follows: one placed Laurentia at high southerly latitude during Catoctin time while the other two were considered as later "remagnetization" events. One remagnetization was hypothesized to have been acquired in the Late Cambrian, when Laurentia was in an equatorial position, whereas a second one was attributed to Taconian mountain-building during the Ordovician period. In order to attempt to unravel the confusing late Precambrian paleogeography, we conducted a detailed paleomagnetic sampling in the Blue Ridge Province of Central Virginia. We focused on the dikes that fed the 568-555 Ma volcanism of the Catoctin Formation (Southworth et al, 2009) in the Shenandoah National Park, as well as in several locations outside the park, and along the south shore of the Potomac River (Maryland). These new data should help to define unambiguously which (if any) of the magnetization components is primary for the Catoctin Formation.

  20. Preferences on technical report format - Results of a survey

    NASA Technical Reports Server (NTRS)

    Pinelli, T. E.; Cordle, V. M.; Glassman, M.; Vondran, R. F.

    1984-01-01

    A survey of 513 engineers and scientists employed at the National Aeronautics and Space Administration Langley Research Center and 600 engineers and scientists from three professional/technical societies solicited the opinions of report users concerning the format of NASA technical reports. The results indicate that a summary as well as an abstract should be included, that the definitions of symbols and glossary of terms should be located in the front of the report, and that the illustrative material should be integrated with the text rather than grouped at the end of the report. Citation of references by number, one-column, ragged-right-margin layout, and third-person writing style are also preferred by a majority of the respondents.

  1. The ACS Nearby Galaxies Survey Treasury: Recovering Spatially Resolved Recent Star Formation Histories

    NASA Astrophysics Data System (ADS)

    Skillman, Evan D.; ANGST Team

    2006-12-01

    Because the supergiant phase of stellar evolution is short relative to the main sequence phase, it is possible to use them as chronometers to reconstruct the spatially resolved recent star formation histories of galaxies (cf., Dohm-Palmer et al. 1997, AJ, 114, 2514). Under the aegis of a cycle 14 HST program to observe a sample of M81 group dwarf galaxies (GO-HST-10605), we have used the star formation history codes of Dolphin (2002, MNRAS, 332, 91) to re-engineer the programs used in Dohm-Palmer et al. and produced automated codes with a wide range of applicability. The ANGST database will allow us our first opportunity to make the transition from analyzing prototypes to analyzing a statistically meaningful sample of galaxies. This promises real progress in quantifying the role of feedback in the evolution of galaxies. This work is supported by NASA grants HST-GO-10605.01-A and HST-GO-10915.06-A

  2. Gas potential of the Rome Trough in Kentucky: Results of recent Cambrian exploration

    SciTech Connect

    Harris, D.C.; Drahovzal, J.A.

    1996-09-01

    A recent gas discovery in the Rome Trough suggests the need to re-evaluate the deep Cambrian potential of eastern Kentucky. A new phase of Cambrian exploration began in mid-1994 with a new pool discovery by the Carson Associates No. 1 Kazee well in Elliott County, Ky. This well blew out and initially flowed 11 MMcfd of gas from the upper Conasauga Group/Rome Formation at 6,258 to 6,270 feet. After this discovery, a second exploratory well (the Blue Ridge No. 1Greene) was drilled on a separate structure in Elliott County in late 1995. The Blue Ridge well was temporarily abandoned, but had shows of gas and condensate. In early 1996, Carson Associates offset their initial discovery well with the No. 33 Lawson Heirs well. This activity follows a frustrating exploration history in the Rome Trough that is marked by numerous gas and oil shows, but rare commercial production. Only three single-well pools have produced commercial gas from the trough, including the recent Kazee well. Stratigraphic units below the Cambrian-Ordovician Knox Group in the Rome Trough are dramatically thicker than their equivalents on the shelf to the north. The interval in the trough is thought to include rocks as old as Early Cambrian, consisting of a basal sandstone, equivalents of the Shady/Tomstown Dolomite, the Rome Formation, and the Conasauga Formation. Sandstones and fractured shales have been responsible for most of the production to date, but dolostone intervals may also have potential. Limited seismic data indicate possible fan-delta and basin-floor fan deposits that may have reservoir potential.

  3. Recent results of high p(T) physics at the CDF II

    SciTech Connect

    Tsuno, Soushi; /Okayama U.

    2005-02-01

    The Tevatron Run II program has been in progress since 2001. The CDF experiment has accumulated roughly five times as much data as did Run I, with much improved detectors. Preliminary results from the CDF experiment are presented. The authors focus on recent high p{sub T} physics results in the Tevatron Run II program.

  4. Enhanced regeneration of phosphorus during formation of the most recent eastern Mediterranean sapropel (S1)

    NASA Astrophysics Data System (ADS)

    Slomp, Caroline P.; Thomson, John; de Lange, Gert J.

    2002-04-01

    Phosphorus regeneration and burial fluxes during and after formation of the most recent sapropel S1 were determined for two deep-basin, low-sedimentation sites in the eastern Mediterranean Sea. Organic C/P ratios and burial fluxes indicate enhanced regeneration of P relative to C during deposition of sapropel S1. This is largely due to the enhanced release of P from organic matter during sulfate reduction. Release of P from Fe-bound P also increased, but this was only a relatively minor source of dissolved P. Pore-water HPO 42- concentrations remained too low for carbonate fluorapatite formation. An increased burial of biogenic Ca-P (i.e., fish debris) was observed for one site. Estimated benthic fluxes of P during sapropel formation were elevated relative to the present day (˜900 to 2800 vs. ˜70 to 120 μmol m -2 yr -1). The present-day sedimentary P cycle in the deep-basin sediments is characterized by two major zones of reaction: (1) the zone near the sediment-water interface where substantial release of HPO 42- from organic matter takes place, and (2) the oxidation front at the top of the S1 where upward-diffusing HPO 42- from below the sapropel is sorbed to Fe-oxides. The efficiency of aerobic organisms in retaining P is reflected in the low organic C/P ratios in the oxidized part of the sapropel. Burial efficiencies for reactive P were significantly lower during S1 times compared with the present day (˜7 to 15% vs. 64 to 77%). Budget calculations for the eastern Mediterranean Sea demonstrate that the weakening of the antiestuarine circulation and the enhanced regeneration of P both contributed to a significant increase in deep-water HPO 42- concentrations during sapropel S1 times. Provided that sufficient vertical mixing occurred, enhanced regeneration of P at the seafloor may have played a key role in maintaining increased productivity during sapropel S1 formation.

  5. Recent Results of Microstructural Characterization of Irradiated Light Water Reactor Fuels using Scanning and Transmission Electron Microscopy

    NASA Astrophysics Data System (ADS)

    Wiss, T.; Thiele, H.; Janssen, A.; Papaioannou, D.; Rondinella, V. V.; Konings, R. J. M.

    2012-12-01

    Recent electron microscopy investigations are presented with an emphasis on properties related to the safe extended operation of nuclear fuel. In particular, this article considers the formation of the high burnup structure (HBS), the prevailing microstructural aspects associated to spent fuel aging, and the release of fission products under accidental condition. Examples of microstructures associated with transient-tested samples but also with very high burnup fuel or heterogeneous mixed oxides (MOX) are presented together with results on damage formation in UO2 samples doped with 238Pu to study the specific effect of alpha damage on the microstructure during the cooling/storage time of irradiated fuel. Examples of single-effect studies (e.g., on the behavior of tellurium, a typical volatile fission product) using ion implantations are also presented.

  6. Recent Results from Broad-Band Intensity Mapping Measurements of Cosmic Large Scale Structure

    NASA Astrophysics Data System (ADS)

    Zemcov, Michael B.; CIBER, Herschel-SPIRE

    2016-01-01

    Intensity mapping integrates the total emission in a given spectral band over the universe's history. Tomographic measurements of cosmic structure can be performed using specific line tracers observed in narrow bands, but a wealth of information is also available from broad-band observations performed by instruments capable of capturing high-fidelity, wide-angle images of extragalactic emission. Sensitive to the continuum emission from faint and diffuse sources, these broad-band measurements provide a view on cosmic structure traced by components not readily detected in point source surveys. After accounting for measurement effects and astrophysical foregrounds, the angular power spectra of such data can be compared to predictions from models to yield powerful insights into the history of cosmic structure formation. This talk will highlight some recent measurements of large scale structure performed using broad-band intensity mapping methods that have given new insights on faint, distant, and diffuse components in the extragalactic background light.

  7. Dynamical Electroweak Symmetry Breaking with a Heavy Fermion in Light of Recent LHC Results

    DOE PAGESBeta

    Hung, Pham Q.

    2013-01-01

    The recent announcement of a discovery of a possible Higgs-like particle—its spin and parity are yet to be determined—at the LHC with a mass of 126 GeV necessitates a fresh look at the nature of the electroweak symmetry breaking, in particular if this newly-discovered particle will turn out to have the quantum numbers of a Standard Model Higgs boson. Even if it were a 0 + scalar with the properties expected for a SM Higgs boson, there is still the quintessential hierarchy problem that one has to deal with and which, by itself, suggests a new physics energy scale aroundmore » 1 TeV. This paper presents a minireview of one possible scenario: the formation of a fermion-antifermion condensate coming from a very heavy fourth generation, carrying the quantum number of the SM Higgs field, and thus breaking the electroweak symmetry.« less

  8. Recent results on D decays and lepton, photon, (and hadron) production of charm

    SciTech Connect

    Nash, T.

    1983-09-01

    After a brief introduction to the experiments with results included in this review, we will discuss, in turn, production of psi and psi', production of open charm in lepton and photon beams, D decays, and give a brief token mention of recent hadroproduction results. Emphasis will be on results reported since the Paris conference (August, 1982), but we will try to include all results since the last Lepton Photon Conference at Bonn (August, 1981) as well as earlier results when necessary for comparison. 42 references.

  9. Recent Results from Galileo PPR at Io: Orbits I31 and I32

    NASA Technical Reports Server (NTRS)

    Rathbun, J. A.; Spencer, J. R.; Tamppari, L. K.; Martin, T. Z.; Barnard, L.; Travis, L. D.

    2002-01-01

    Recent Galileo PPR (Photo-Polarimeter Radiometer) results will be shown, including global day and nighttime maps, high latitude regional maps, and high-resolution scans across hotspots and from pole to pole. SO2 vapor pressure, global heatflow, and hotspot power outputs are estimated. Additional information is contained in the original extended abstract.

  10. MINE WASTE TECHNOLOGY PROGRAM: RECENT RESULTS: LESSONS LEARNED AND FUTURE OPPORTUNITIES

    EPA Science Inventory

    In the EPA sponsored AML workshop, a number of Mine Waste Technology Program (MWTP) projects will be presented in order to highlight the most successful technology demonstrations. Recent results, lesson learned and future opportunities will be presented. The MWTP projects includ...

  11. Recent results from polarization experiments at the LHEP-JINR Accelerator

    SciTech Connect

    Ladygin, V. P.; Azhgirey, L. S.; Gurchin, Yu. V.; Isupov, A. Yu.; Krasnov, V. A.; Khrenov, A. N.; Kiselev, A. S.; Kizka, V. A.; Kurilkin, A. K.; Kurilkin, P. K.; Livanov, A. N.; Ladygina, N. B.; Malakhov, A. I.; Piyadin, S. M.; Reznikov, S. G.; Shikhalev, M. A.; Vasiliev, T. A.; Uesaka, T.; Kawabata, T.; Sakaguchi, S.

    2008-10-13

    The review of recent results from polarization experiments performed at LHEP-JINR Accelerator Complex in a GeV range is given. The current status of the spin program at Nuclotron as well as its further continuation with new high intensity polarized deuterons ion source is discussed.

  12. Recent results and prospects for high pT physics at D-Zero

    SciTech Connect

    Cecilia Elena Gerber

    2003-09-11

    The author presents recent results from the D0 experiment using {approx} 50 pb{sup -1} of data recorded at the center of mass energy of 1.96 TeV at the Fermilab Tevatron. In addition, the author summarizes prospects for high p{sub T} physics at the Tevatron as a function of integrated luminosity.

  13. RECENT LATTICE RESULTS ON FINITE TEMPERATURE AND DENSITY QCD, PART II.

    SciTech Connect

    KARSCH,F.

    2007-07-09

    We discuss recent progress in studies of QCD thermodynamics with almost physical light quark masses and a physical value of the strange quark mass. We summarize results on the transition temperature in QCD and analyze the relation between deconfinement and chiral symmetry restoration.

  14. Nuclear structure relevant to neutrinoless double beta decay candidate {sup 130}Te and other recent results

    SciTech Connect

    Kay, B. P.

    2013-12-30

    We have undertaken a series of single-nucleon and pair transfer reaction measurements to help constrain calculations of the nuclear matrix elements for neutrinoless double beta decay. In this talk, a short overview of measurements relevant to the {sup 130}Te→{sup 130}Xe system is given. Brief mention is made of other recent and forthcoming results.

  15. Characterization Of Superconducting Samples With SIC System For Thin Film Developments: Status And Recent Results

    SciTech Connect

    Phillips, H. Lawrence; Reece, Charles E.; Valente-Feliciano, Anne-Marie; Xiao, Binping; Eremeev, Grigory V.

    2014-02-01

    Within any thin film development program directed towards SRF accelerating structures, there is a need for an RF characterization device that can provide information about RF properties of small samples. The current installation of the RF characterization device at Jefferson Lab is Surface Impedance Characterization (SIC) system. The data acquisition environment for the system has recently been improved to allow for automated measurement, and the system has been routinely used for characterization of bulk Nb, films of Nb on Cu, MgB{sub 2}, NbTiN, Nb{sub 3}Sn films, etc. We present some of the recent results that illustrate present capabilities and limitations of the system.

  16. Recent results from the Berkeley 0.3-NA microfield exposure tool

    SciTech Connect

    Naulleau, Patrick; Anderson, Christopher N.; Dean, Kim; Denham, Paul; Goldberg, Kenneth A.; Hoef, Brian; La Fontaine, Bruno; Wallow, Tom

    2007-03-01

    Operating as a SEMATECH resist test center, the Berkeley 0.3-NA EUV microfield exposure tool continues to play a crucial role in the advancement of EUV resists and masks. Here we present recent resist-characterization results from the tool as well as tool-characterization data. In particular we present lithographic-based aberration measurements demonstrating the long-term stability of the tool. We also describe a recent upgrade to the tool which involved redesign of the programmable coherence illuminator to provide improved field uniformity as well as a programmable field size.

  17. RECENT LATTICE RESULTS ON FINITE TEMPERATURE AND DENSITY QCD, PART 1.

    SciTech Connect

    KARSCH,F.

    2007-07-09

    We discuss recent progress made studies of bulk thermodynamics of strongly interacting matter through lattice simulations of QCD with an almost physical light and strange quark mass spectrum. We present results on the QCD equation of state at vanishing and non-vanishing quark chemical potential and show first results on baryon number and strangeness fluctuations, which might be measured in event-by-event fluctuations in low energy runs at RHIC as well as at FAIR.

  18. Adverse metabolic effects of dietary fructose: Results from recent epidemiological, clinical, and mechanistic studies

    PubMed Central

    Stanhope, Kimber L.; Schwarz, Jean-Marc; Havel, Peter J.

    2014-01-01

    Purpose of review The effects of dietary sugar on risk factors and processes associated with metabolic disease remains a controversial topic, with recent reviews of the available evidence arriving at widely discrepant conclusions. Recent findings There are many recently published epidemiological studies that provide evidence that sugar consumption is associated with metabolic disease. Three recent clinical studies, which investigated the effects of consuming relevant doses of sucrose or high fructose corn syrup along with ad libitum diets, provide evidence that consumption of these sugars increase risk factors for cardiovascular disease (CVD) and metabolic syndrome. Mechanistic studies suggest that these effects result from the rapid hepatic metabolism of fructose catalyzed by fructokinase C, which generates substrate for de novo lipogenesis and leads to increased uric acid levels. Recent clinical studies investigating the effects of consuming less sugar, via educational interventions or by substitution of sugar-sweetened beverages for non-calorically sweetened beverages, provide evidence that such strategies have beneficial effects on risk factors for metabolic disease or on BMI in children. Summary The accumulating epidemiological evidence, direct clinical evidence, and the evidence suggesting plausible mechanisms support a role for sugar in the epidemics of metabolic syndrome, CVD and type 2 diabetes. PMID:23594708

  19. SDSS IV MaNGA: Gradients in Recent Star Formation Histories as Diagnostics for Galaxy Growth and Death

    NASA Astrophysics Data System (ADS)

    Li, Cheng; MaNGA Team

    2016-01-01

    The spatially resolved spectroscopy from MaNGA allows the radial gradients of recent star formation histories (SFH), as indicated by the 4000Å break (D4000) and the equivalent width of both Hδ absorption line and Hα emission line, to be obtained with high accuracy for a large sample of galaxies in the nearby universe. Analyses of both a dozen galaxies observed by the MaNGA prototype run (P-MaNGA) and ~700 galaxies in the current MaNGA sample have shown that the SFH gradients are useful for understanding disk growth and star formation cessation in local galaxies. We find the SFH gradient of a galaxy to strongly depend on the evolution stage of its central region. Centrally star-forming galaxies generally show very weak or no radial variations. In contrast, centrally quiescent galaxies present significant radial gradients in the sense that Dn(4000) decreases, while both EW(HδA) and EW(Hα) increase from the galactic center outward. This effect is seen mainly for high-mass galaxies with stellar mass above a few ×1010 M⊙, and depends weakly on galaxy morphology type. These results are consistent with a picture in which the cessation of star formation propagates from the center of a galaxy outward as it moves to the red sequence. In this talk I will present these analyses and discuss their implications on galaxy evolution.

  20. CREATING HEALTHY HOME EATING ENVIRONMENTS: RESULTS FROM FORMATIVE RESEARCH

    Technology Transfer Automated Retrieval System (TEKTRAN)

    The federal Expanded Food and Nutrition Education Program (EFNEP) provides nutrition education classes to limited-resource families. This study was conducted to inform a new obesity prevention EFNEP component to help families create healthy home food environments. Two formative research studies were...

  1. Recent results on top, bottom and exotic physics at the Tevatron

    SciTech Connect

    Shaw, N.M. |

    1993-08-01

    A summary of results from the recently concluded 1991--1993 Tevatron run is presented. Selected topics from b physics and exotic particle searches from the CDF and D0 collaborations are reviewed. Preliminary results from the CDF top search, using 12pb{sup {minus}1} from the 1992--1993 run, are given. In particular, the lepton + b-tag and dilepton analyses are discussed. Preliminary results from the CDF dilepton analysis places a lower limit on the top quark mass of 108GeV/c{sup 2} at the 95% C.L.

  2. Ultraviolet through Far-Infrared Spatially Resolved Analysis of the Recent Star Formation in M81 (NGC 3031)

    NASA Astrophysics Data System (ADS)

    Pérez-González, Pablo G.; Kennicutt, Robert C., Jr.; Gordon, Karl D.; Misselt, Karl A.; Gil de Paz, Armando; Engelbracht, Charles W.; Rieke, George H.; Bendo, George J.; Bianchi, Luciana; Boissier, Samuel; Calzetti, Daniela; Dale, Daniel A.; Draine, Bruce T.; Jarrett, Thomas H.; Hollenbach, David; Prescott, Moire K. M.

    2006-09-01

    The recent star formation (SF) in the early-type spiral galaxy M81 is characterized using imaging observations from the far-ultraviolet to the far-infrared. We compare these data with models of the stellar, gas, and dust emission for subgalactic regions. Our results suggest the existence of a diffuse dust emission not directly linked to the recent star formation. We find a radial decrease of the dust temperature and dust mass density, and in the attenuation of the stellar light. The IR emission in M81 can be modeled with three components: (1) cold dust with a temperature c>=18+/-2 K, concentrated near the H II regions but also presenting a diffuse distribution; (2) warm dust with w>=53+/-7 K, directly linked with the H II regions; and (3) aromatic molecules, with diffuse morphology peaking around the H II regions. We derive several relationships to obtain total IR luminosities from IR monochromatic fluxes, and we compare five different star formation rate (SFR) estimators for H II regions in M81 and M51: the UV, Hα, and three estimators based on Spitzer data. We find that the Hα luminosity absorbed by dust correlates tightly with the 24 μm emission. The correlation with the total IR luminosity is not as good. Important variations from galaxy to galaxy are found when estimating the total SFR with the 24 μm or the total IR emission alone. The most reliable estimations of the total SFRs are obtained by combining the Hα emission (or the UV) and an IR luminosity (especially the 24 μm emission), which probe the unobscured and obscured SF, respectively. For the entire M81 galaxy, about 50% of the total SF is obscured by dust. The percentage of obscured SF ranges from 60% in the inner regions of the galaxy to 30% in the outer zones.

  3. Very high energy observations of the Galactic Centre: recent results and perspectives with CTA

    NASA Astrophysics Data System (ADS)

    Terrier, Regis

    2016-07-01

    The central 300 pc of our Galaxy are a major laboratory for high energy astrophysics. They harbor the closest supermassive black hole (SMBH) and are the site of a sustained star formation activity. The energy released by the supernovae on the ambient medium must be very strong. Similarly, albeit extremely faint nowadays, the SMBH must have experienced episodes of intense activity in the past which can influence significantly the central regions and beyond, e.g. powering the Fermi bubbles. I review observational results at very high energies from the central region and discuss their implications and the questions they leave open. I discuss the perspectives CTA offers for Galactic Centre astrophysics.

  4. Actinic review of EUV masks: Status and recent results of the AIMS EUV system

    NASA Astrophysics Data System (ADS)

    Weiss, Markus R.; Hellweg, Dirk; Koch, Markus; Peters, Jan Hendrik; Perlitz, Sascha; Garetto, Anthony; Magnusson, Krister; Capelli, Renzo; Jindal, Vibhu

    2015-03-01

    The EUV mask infrastructure is of key importance for the successful introduction of EUV lithography into volume production. In particular, for the production of defect free masks an actinic review of potential defect sites is required. To realize such an actinic review tool, Carl Zeiss and the SEMATECH EUVL Mask Infrastructure consortium started a development program for an EUV aerial image metrology system, the AIMS™ EUV. In this paper, we discuss the current status of the prototype integration and show recent results.

  5. Recent Results from the Wide Angle Search for Planets (WASP) Prototype

    NASA Astrophysics Data System (ADS)

    Kane, S. R.; Horne, K.; Lister, T.; Collier Cameron, A.; Street, R. A.; Pollacco, D. L.; James, D.; Tsapras, Y.

    2004-12-01

    WASP0 is a prototype for what is intended to become a collection of WASPs whose primary aim is to detect transiting extra-solar planets across the face of their parent star. We present some recent results from the WASP0 camera, including observations of the known transiting planet around HD 209458. The current status of the next generation camera (SuperWASP) located on La Palma is briefly outlined.

  6. Recent Results in Electroweak B Decays from the BaBar Experiment

    SciTech Connect

    Koeneke, Karsten; /MIT, LNS /SLAC

    2006-09-01

    A review of the most recent BABAR results on electroweak penguin B decays is presented. The focus of this paper is on the measurement of observables in the decays B {yields} X{sub s}{gamma}, B {yields} K{sup (*)}l{sup +}l{sup -} B {yields} K{sub s}{sup 0}{pi}{sup 0}{gamma} (time-dependent analysis) and B {yields} ({rho}/{omega}){gamma}.

  7. Recent Astrophysics Results from ORELA and Possible Future Experiments at ORELA and SNS

    NASA Astrophysics Data System (ADS)

    Koehler, P. E.

    2002-12-01

    I present some recent results from experiments at the Oak Ridge Electron Linear Accelerator (ORELA) and discuss their impact in nuclear astrophysics. I then describe some possible future nuclear astrophysics experiments at ORELA and at the Spallation Neutron Source (SNS) being built in Oak Ridge. The SNS and ORELA are complementary, world-class facilities and both will be needed for important future experiments in nuclear astrophysics.

  8. Recent results from the GISS model of the global atmosphere. [circulation simulation for weather forecasting

    NASA Technical Reports Server (NTRS)

    Somerville, R. C. J.

    1975-01-01

    Large numerical atmospheric circulation models are in increasingly widespread use both for operational weather forecasting and for meteorological research. The results presented here are from a model developed at the Goddard Institute for Space Studies (GISS) and described in detail by Somerville et al. (1974). This model is representative of a class of models, recently surveyed by the Global Atmospheric Research Program (1974), designed to simulate the time-dependent, three-dimensional, large-scale dynamics of the earth's atmosphere.

  9. Recent results of X-ray observations from OSO-7 and SAS-3

    NASA Technical Reports Server (NTRS)

    Clark, G. W.

    1978-01-01

    Recent observations bearing on the nature of compact X-ray sources obtained from the MIT instruments aboard OSO-7 and SAS-3 are discussed. Results on the X-ray sky survey, new ultralow-energy X-ray sources, X-ray sources in globular clusters, slow X-ray pulsars, and variability and position of compact X-ray sources in Cen A are discussed. Descriptions of the satellite-borne X-ray instruments are provided.

  10. Scanning L-Band Active Passive (SLAP) - Recent Results from an Airborne Simulator for SMAP

    NASA Technical Reports Server (NTRS)

    Kim, Edward

    2015-01-01

    Scanning L-band Active Passive (SLAP) is a recently-developed NASA airborne instrument specially tailored to simulate the new Soil Moisture Active Passive (SMAP) satellite instrument suite. SLAP conducted its first test flights in December, 2013 and participated in its first science campaign-the IPHEX ground validation campaign of the GPM mission-in May, 2014. This paper will present results from additional test flights and science observations scheduled for 2015.

  11. Recent results on giant dipole resonance decays in highly excited nuclei

    SciTech Connect

    Snover, K.A.

    1991-12-31

    Some recent results on Giant Dipole Resonance (GDR) decays in highly excited, equilibrated nuclei, are discussed based primarily on work done at Seattle. Four sections address the following topics: oblate shapes of rotating, highly excited Zr--Mo nuclei; adiabatic versus `motionally narrowed` GDR decay; large spin-driven deformations observed in hot medium-mass nuclei; and search for entrance channel effects in GDR decay following {sup 58}Ni {plus} {sup 92}Zr fusion. 22 refs.

  12. Recent results on giant dipole resonance decays in highly excited nuclei

    SciTech Connect

    Snover, K.A.

    1991-01-01

    Some recent results on Giant Dipole Resonance (GDR) decays in highly excited, equilibrated nuclei, are discussed based primarily on work done at Seattle. Four sections address the following topics: oblate shapes of rotating, highly excited Zr--Mo nuclei; adiabatic versus motionally narrowed' GDR decay; large spin-driven deformations observed in hot medium-mass nuclei; and search for entrance channel effects in GDR decay following [sup 58]Ni [plus] [sup 92]Zr fusion. 22 refs.

  13. Recent results and perspectives on cosmology and fundamental physics from microwave surveys

    NASA Astrophysics Data System (ADS)

    Burigana, Carlo; Battistelli, Elia Stefano; Benetti, Micol; Cabass, Giovanni; de Bernardis, Paolo; di Serego Alighieri, Sperello; di Valentino, Eleonora; Gerbino, Martina; Giusarma, Elena; Gruppuso, Alessandro; Liguori, Michele; Masi, Silvia; Norgaard-Nielsen, Hans Ulrik; Rosati, Piero; Salvati, Laura; Trombetti, Tiziana; Vielva, Patricio

    2016-04-01

    Recent cosmic microwave background (CMB) data in temperature and polarization have reached high precision in estimating all the parameters that describe the current so-called standard cosmological model. Recent results about the integrated Sachs-Wolfe (ISW) effect from CMB anisotropies, galaxy surveys, and their cross-correlations are presented. Looking at fine signatures in the CMB, such as the lack of power at low multipoles, the primordial power spectrum (PPS) and the bounds on non-Gaussianities, complemented by galaxy surveys, we discuss inflationary physics and the generation of primordial perturbations in the early universe. Three important topics in particle physics, the bounds on neutrinos masses and parameters, on thermal axion mass and on the neutron lifetime derived from cosmological data are reviewed, with attention to the comparison with laboratory experiment results. Recent results from cosmic polarization rotation (CPR) analyses aimed at testing the Einstein equivalence principle (EEP) are presented. Finally, we discuss the perspectives of next radio facilities for the improvement of the analysis of future CMB spectral distortion experiments.

  14. The Panchromatic Hubble Andromeda Treasury. XI. The Spatially Resolved Recent Star Formation History of M31

    NASA Astrophysics Data System (ADS)

    Lewis, Alexia R.; Dolphin, Andrew E.; Dalcanton, Julianne J.; Weisz, Daniel R.; Williams, Benjamin F.; Bell, Eric F.; Seth, Anil C.; Simones, Jacob E.; Skillman, Evan D.; Choi, Yumi; Fouesneau, Morgan; Guhathakurta, Puragra; Johnson, Lent C.; Kalirai, Jason S.; Leroy, Adam K.; Monachesi, Antonela; Rix, Hans-Walter; Schruba, Andreas

    2015-06-01

    We measure the recent star formation history (SFH) across M31 using optical images taken with the Hubble Space Telescope as part of the Panchromatic Hubble Andromeda Treasury (PHAT). We fit the color-magnitude diagrams in ˜9000 regions that are ˜100 pc × 100 pc in projected size, covering a 0.5 square degree area (˜380 kpc2, deprojected) in the NE quadrant of M31. We show that the SFHs vary significantly on these small spatial scales but that there are also coherent galaxy-wide fluctuations in the SFH back to ˜500 Myr, most notably in M31's 10 kpc star-forming ring. We find that the 10 kpc ring is at least 400 Myr old, showing ongoing star formation (SF) over the past ˜500 Myr. This indicates the presence of molecular gas in the ring over at least 2 dynamical times at this radius. We also find that the ring’s position is constant throughout this time, and is stationary at the level of 1 km s-1, although there is evidence for broadening of the ring due to the diffusion of stars into the disk. Based on existing models of M31's ring features, the lack of evolution in the ring’s position makes a purely collisional ring origin highly unlikely. Besides the well-known 10 kpc ring, we observe two other ring-like features. There is an outer ring structure at 15 kpc with concentrated SF starting ˜80 Myr ago. The inner ring structure at 5 kpc has a much lower star formation rate (SFR) and therefore lower contrast against the underlying stellar disk. It was most clearly defined ˜200 Myr ago, but is much more diffuse today. We find that the global SFR has been fairly constant over the last ˜500 Myr, though it does show a small increase at 50 Myr that is 1.3 times the average SFR over the past 100 Myr. During the last ˜500 Myr, ˜60% of all SF has occurred in the 10 kpc ring. Finally, we find that in the past 100 Myr, the average SFR over the PHAT survey area is 0.28 ± 0.03 {{M}⊙ } y{{r}-1} with an average deprojected intensity of 7.3× {{10}-4} {{M}⊙ } y

  15. Recent Results of Nuclear Mass Measurements at Storage Ring in IMP

    NASA Astrophysics Data System (ADS)

    Xu, H. S.; Zhang, Y. H.

    2014-09-01

    Recent commissioning of the Cooler Storage Ring at the Heavy Ion Research Facility in Lanzhou (HIRFL-CSR) has allowed us for direct mass measurements at the Institute of Modern Physics in Lanzhou (IMP), Chinese Academy of Sciences. A series of isochronous mass measurements have been carried out in the past few years using 78Kr, 86Kr, 58Ni, and 112Sn beams. The main results and the present status are presented in this talk, and the implications of these results with respect to nuclear structures and nucleosynthesis in the rp-process of x-ray bursts are discussed.

  16. The 3D structure of the hadrons: recents results and experimental program at Jefferson Lab

    SciTech Connect

    Munoz Camacho, Carlos

    2014-04-01

    The understanding of Quantum Chromodynamics (QCD) at large distances still remains one of the main outstanding problems of nuclear physics. Studying the internal structure of hadrons provides a way to probe QCD in the non-perturbative domain and can help us unravel the internal structure of the most elementary blocks of matter. Jefferson Lab (JLab) has already delivered results on how elementary quarks and gluons create nucleon structure and properties. The upgrade of JLab to 12 GeV will allow the full exploration of the valence-quark structure of nucleons and the extraction of real threedimensional pictures. I will present recent results and review the future experimental program at JLab.

  17. Recent astrophysical and accelerator-based results on the hadronic equation of state

    NASA Astrophysics Data System (ADS)

    Hartnack, Ch; Oeschler, H.; Aichelin, Jörg

    2006-12-01

    In astrophysics as well as in hadron physics, progress has recently been made on the determination of the hadronic equation of state (EoS) of compressed matter. The results are contradictory, however. Simulations of heavy-ion reactions are now sufficiently robust to predict the stiffness of the EoS from (i) the energy dependence of the ratio of K+ from Au + Au and C + C collisions and (ii) the centrality dependence of the K+ multiplicities. The data are best described with a compressibility coefficient at normal nuclear matter density κ of around 200 MeV, a value which is usually called 'soft'. The recent observation of a neutron star with a mass of twice the solar mass is only compatible with theoretical predictions if the EoS is stiff. We review the present situation.

  18. Recent results in a search for inorganic scintillators for x- and gamma-ray detection

    SciTech Connect

    Moses, W.W.; Weber, M.J.; Derenzo, S.E.; Perry, D.; Berahl, P.

    1997-10-01

    We present recent results from an ongoing search for inorganic scintillators for gamma ray detection in which we measure the scintillation properties (luminous efficiency, decay time, and emission wavelength) of powdered samples excited by brief x-ray pulses. Recent promising candidates include cerium doped lutetium borate (LuBO{sub 3}) and the lutetium double phosphates K{sub 3}Lu(PO{sub 4}){sub 2} and Rb{sub 3}Lu(PO{sub 4}){sub 2}, which have luminous intensities above 25,000 photons/MeV. In order to find scintillators that are compatible with silicon photodetectors, we have tested over 1,100 samples using a photomultiplier tube with a GaAs:Cs photocathode, which is sensitive to emissions from 200-950 nm. While many samples exhibited strong emissions in the 600-900 nm range, all had decay times that were larger than 10 {mu}s.

  19. Recent Analytical and Numerical Results for The Navier-Stokes-Voigt Model and Related Models

    NASA Astrophysics Data System (ADS)

    Larios, Adam; Titi, Edriss; Petersen, Mark; Wingate, Beth

    2010-11-01

    The equations which govern the motions of fluids are notoriously difficult to handle both mathematically and computationally. Recently, a new approach to these equations, known as the Voigt-regularization, has been investigated as both a numerical and analytical regularization for the 3D Navier-Stokes equations, the Euler equations, and related fluid models. This inviscid regularization is related to the alpha-models of turbulent flow; however, it overcomes many of the problems present in those models. I will discuss recent work on the Voigt-regularization, as well as a new criterion for the finite-time blow-up of the Euler equations based on their Voigt-regularization. Time permitting, I will discuss some numerical results, as well as applications of this technique to the Magnetohydrodynamic (MHD) equations and various equations of ocean dynamics.

  20. Investigations of a Combustor Using a 9-Point Swirl-Venturi Fuel Injector: Recent Experimental Results

    NASA Technical Reports Server (NTRS)

    Hicks, Yolanda R.; Heath, Christopher M.; Anderson, Robert C.; Tacina, Kathleen M.

    2012-01-01

    This paper explores recent results obtained during testing in an optically-accessible, JP8-fueled, flame tube combustor using baseline Lean Direct Injection (LDI) research hardware. The baseline LDI geometry has nine fuel/air mixers arranged in a 3 x 3 array. Results from this nine-element array include images of fuel and OH speciation via Planar Laser-Induced Fluorescence (PLIF), which describe fuel spray pattern and reaction zones. Preliminary combustion temperatures derived from Stokes/Anti-Stokes Spontaneous Raman Spectroscopy are also presented. Other results using chemiluminescence from major combustion radicals such as CH* and C2* serve to identify the primary reaction zone, while OH PLIF shows the extent of reaction further downstream. Air and fuel velocities and fuel drop size results are also reported.

  1. Prevention of solids formation: Results of the FY 1999 studies

    SciTech Connect

    Hunt, R.D.; Beahm, E.C.; Chase, C.W.; Collins, J.L.; Dillow, T.A.; Weber, C.F.

    1999-12-01

    Tank farm operations at Hanford and Savannah River have been adversely affected by unintentional solids formations. At Hanford, a new cross-site transfer line had to be built because nearly all the original transfer lines were no longer operational due to plugs. At Savannah River, operations at its evaporator system were suspended while a plug in the gravity drain line was physically removed at considerable expense. The plugs as Hanford and Savannah River, which have been characterized, were primarily due to sodium phosphate and sodium aluminosilicate, respectively.

  2. Fracturing results in diatomaceous earth formations, South Belridge Field, California

    SciTech Connect

    Strubhar, M.K.; Medin, W.L.

    1982-09-01

    Fracturing significantly increases light oil production rates at South Belridge making this an economically successful technique for exploitation of the Reef Ridge reservoir. No fracturing mechanics problems were encountered in any of the treatments. The loosely consolidated formations behaved mechanically much like brittle, elastic rocks. Net oil and gross production is typified by initial high rates and an early rapid decline. The major cause of this early rapid decline is the transient flow effect. This behavior is typical of low permeability oil and gas production. Fractures are vertical, as shown by gamma ray and temperature logs run following several treatments. The fractures grow slightly out of the perforated intervals (10 to 15 feet). Loss of fracture conductivity due to fines migration, scale deposition, and/or fracture healing (imbedment) is not a serious problem. Oil viscosity can vary as much as ten-fold. Some wells produce significant amounts of gas--100 to 200 MCFPD initially. The formation is primarily diatomaceous earth which is very fine particle size siliceous material composed of whole or fragmented diatom tests (skeletons). There is no evidence that clay swelling or dispersion is a problem. Field and laboratory data support this conclusion. Aqueous fracturing fluids were successfully used which confirmed laboratory tests on cores.

  3. A review of recent results in gamma-ray astronomy obtained from high-altitude balloons

    NASA Astrophysics Data System (ADS)

    Teegarden, B. J.

    1994-06-01

    This paper reviews recent results in gamma-ray astronomy obtained from experiments flown on high-altitude balloons. New generation balloon-borne imaging experiments have produced the first gamma-ray maps of the Galactic center (GC) region. Balloon flights of new gamma-ray spectrometers with improved sensitivity have provided important new information on the GC annihilation line. For the first time, the narrow 511 keV line as been resolved (FWHM approx. = 3 keV). A very interesting spectral feature at approximately 170 keV has been attributed to backscattered annihilation, probably from the vicinity of a compact object. New results from the Compton Gamma-Ray Observatory (CGRO)/OSSE and Granat/SIGMA experiments on the annihilation line, when considered together with the recent balloon results, have added greatly to our knowledge and understanding of the origin and distribution of this emission. Balloon-borne instruments have made important measurements of gamma-ray continuum and line emission from SN 1987A. The GRIS spectrometer unambiguously resolved the 847 and 1238 keV line emission from radioactive Co-56 synthesized during the explosion. This data indicated that simple spherically symmetric and homogeneous models did not provide an adequate description of the expanding SN shell.

  4. A review of recent results in gamma-ray astronomy obtained from high-altitude balloons

    NASA Technical Reports Server (NTRS)

    Teegarden, B. J.

    1994-01-01

    This paper reviews recent results in gamma-ray astronomy obtained from experiments flown on high-altitude balloons. New generation balloon-borne imaging experiments have produced the first gamma-ray maps of the Galactic center (GC) region. Balloon flights of new gamma-ray spectrometers with improved sensitivity have provided important new information on the GC annihilation line. For the first time, the narrow 511 keV line as been resolved (FWHM approx. = 3 keV). A very interesting spectral feature at approximately 170 keV has been attributed to backscattered annihilation, probably from the vicinity of a compact object. New results from the Compton Gamma-Ray Observatory (CGRO)/OSSE and Granat/SIGMA experiments on the annihilation line, when considered together with the recent balloon results, have added greatly to our knowledge and understanding of the origin and distribution of this emission. Balloon-borne instruments have made important measurements of gamma-ray continuum and line emission from SN 1987A. The GRIS spectrometer unambiguously resolved the 847 and 1238 keV line emission from radioactive Co-56 synthesized during the explosion. This data indicated that simple spherically symmetric and homogeneous models did not provide an adequate description of the expanding SN shell.

  5. Recent results from the Mainz Microtron MAMI and an outlook for the future

    NASA Astrophysics Data System (ADS)

    Denig, Achim

    2016-05-01

    We present recent results from the Mainz Microtron MAMI, which is a high intensity electron accelerator with (polarized) beam energies up to 1.6 GeV. Currently, two major experiments are operated at MAMI. The A1 spectrometer setup is ideally suited for high-resolution electron scattering experiments, which recently led to highly competitive results on electromagnetic form factors and dark photon searches. The second experiment is the Crystal Ball/TAPS calorimeter setup (A2 collaboration), which is operated at the tagged photon beam line. At A2, the baryon spectrum in the low-energy region is investigated in photo-production experiments. A polarized target for longitudinal and transversal beam polarization in combination with the polarized beam does not only allow for experiments in this field, but also opens the avenue for investigations of the polarizabilities of the nucleons, for which new results are presented in this paper. In addition, the high rate of pseudoscalar mesons produced via photo-production allows for measurements of meson decays as motivated by precision tests of chiral perturbation theory or precision tests of the Standard Model. We also outline the physics opportunities at the accelerator MESA (Mainz Energy-Recovering Superconducting Accelerator), which is currently under construction in Mainz.

  6. Recent results on top quark physics and B physics at CDF

    SciTech Connect

    Kim, S.

    1998-01-01

    We present the recent results on top quark physics and B physics with the Collider Detector at Fermilab (CDF). These results come from analyses using a full data sample at an integrated luminosity of 109 pb{sup -1} cross section in 1.8-TeV p{anti p} collisions. We measure the top quark mass to be 175.8{+-}6.5 GeV/c{sup 2} and the t{anti t} production cross section to be 7.6{sup +1.8}{sub -1.5} pb. We also present measurements of the lifetimes of B-hadrons and the time- dependent B{sup 0}-{anti B}{sup 0} mixing which results in the mass difference between heavy and light B{sup 0}{sub d} mesons ({Delta}m{sub d}) of 0.464{+-}0.030(stat){+-}0.026(syst) ps{sup -1}.

  7. An Overview of Recent Deeply Virtual Compton Scattering Results at HERMES

    SciTech Connect

    Mahon, David Francis

    2009-12-17

    We present recently-released HERMES Deeply Virtual Compton Scattering results of Beam-Helicity (formerly Beam-Spin, BSA) and Beam-Charge (BCA) asymmetries from unpo-larised proton, deuteron and selected heavy nuclear gas targets. A new analysis technique utilising the ability of HERA to produce a longitudinally-polarised lepton beam of both charges has been used to simultaneously extract the BSA and BCA amplitudes arising from the DVCS-squared and Interference terms of the total cross section for proton and deuteron data. Results of the Transverse Target-Spin Asymmetry (TTSA) obtained using this technique have been published for transversely-polarised proton data. These extracted asymmetries are presented, integrated over the kinematic acceptance of the HERMES experiment for this interaction, with their dependences on -t, x{sub B} and Q{sup 2} also shown. The results are compared with asymmetries from a phenomenological model of GPDs based on double distributions.

  8. Spatial variation of stratospheric aerosol acidity and model refractive index - Implications of recent results

    NASA Technical Reports Server (NTRS)

    Russell, P. B.; Hamill, P.

    1984-01-01

    Recent experimental results indicate that little or no solid ammonium sulfate is present in background stratospheric aerosols. Other results allow straightforward calculation of sulfuric acid/water droplet properties (acidity, specific gravity, refractive index) as functions of stratospheric temperature and humidity. These results are combined with a variety of latitudinal and seasonal temperature and humidity profiles to obtain corresponding profiles of droplet properties. These profiles are used to update a previous model of stratospheric aerosol refractive index. The new model retains the simplifying approximation of vertically constant refractive index in the inner stratosphere, but has sulfuric acid/water refractive index values that significantly exceed the previously used room temperature values. Mean conversion ratios (e.g., extinction-to-number, backscatter-to-volume) obtained using Mie scattering calculations with the new refractive indices are very similar to those obtained for the old indices, because the effects of deleting ammonium sulfate and increasing acid indices tend to cancel each other.

  9. How can evolutionary theory accommodate recent empirical results on organismal senescence?

    PubMed

    Mitteldorf, Joshua; Pepper, John W

    2007-08-01

    According to a prominent recent report, guppies collected from sites lacking predators are inferior in every aspect of their life history profile to those evolved in other, nearby sites with predators present. This is an exception to two classical predictions of evolutionary theory: that low extrinsic mortality should be associated with longer life span, and that higher fertility should be associated with shorter life span. Some theorists have tried to accommodate this and other anomalous results within the standard framework, but we argue that the exceptions they carve out do not explain the results at hand. In fact, the findings suggest that population regulation has been selected at the group level, though this is a mechanism that most theorists regard with suspicion. We conclude by relating the present result to other experiments that seem to point in the same direction. PMID:18087751

  10. Recent beauty results from CDF and the Run-II upgrades

    SciTech Connect

    Huffman, B.T.; CDF Collaboration

    1996-09-01

    This paper reports on the most recent results from the Collider Detector Facility (CDF) from 110 pb{sup -1} of data taken at the Fermilab Tevatron from 1992 to 1995. Improved measurements of B meson spectroscopy, lifetimes, and searches for new particle states are presented. Evidence for the effectiveness of same side tagging techniques in the context of mixing measurements is shown with applicability for CP violation studies in Run-II explained. The planned upgrades of importance to {ital b} physics for Run-II are briefly detailed with an emphasis on the expected physics reach in Run-II by CDF.

  11. X-rays from Pre-Main Sequence Stars: Recent Results and Future Challenges

    NASA Astrophysics Data System (ADS)

    Skinner, S.

    2016-08-01

    I will summarize recent results of X-ray observations of pre-main sequence (PMS) stars, focusing on XMM-Newton RGS and Chandra HETG observations of RY Tau. These observations provide the best grating spectra obtained so far of a jet-driving T Tauri star. I will also identify key questions regarding the origin and nature of X-ray emission from PMS stars that have emerged from 16 years of XMM-Newton and Chandra observations and which present challenges for the next decade.

  12. Atmospheric remote sensing and applications from GNSS: Recent results and progress

    NASA Astrophysics Data System (ADS)

    Jin, Shuanggen; Gurbuz, Gokhan; Akgul, Volkan

    2016-07-01

    The atmospheric delay is one of Global Navigation Satellite Systems (GNSS) errors. Nowadays, the total zenith tropospheric delay (ZTD) and ionospheric total electron content (TEC) can be precisely obtained from GNSS, which can be used for weather prediction and atmospheric research as well as space weather. In this paper, recent results and progress on atmospheric remote sensing and applications from GNSS are presented, including ocean tide models and mapping functions effects, high-order ionospheric delay correction, tropoapause variations, ionospheric climatology, seismo-atmospheric anomalies and characteristics. Finally, some possible mechanism on atmospheric anomalies and coupling processes are given and discussed as well as future challenges.

  13. Recent results in photoionization of atoms and ions using undulator radiation

    NASA Astrophysics Data System (ADS)

    Wuilleumier, François J.; Cubaynes, D.; Bizau, J.-M.

    2001-07-01

    Recent progress in the production of photon beams delivered by undulators allowed us to obtain new low- and high-resolution results in photoionization of atoms and ions. Using the 2nd generation Super ACO storage ring, we have measured cross sections for higher-order correlation satellites in lithium and single and double photoionization of multiply-charged ions. With the 3rd generation Advanced Light Source storage ring, we performed highly-resolved angle-integrated and angle-resolved experiments, including the study of correlation satellites and hollow states in alkali-atoms.

  14. Recent fracture mechanics results from NASA research related to the aging commercial transport fleet

    NASA Technical Reports Server (NTRS)

    Harris, Charles E.

    1991-01-01

    NASA is conducting the Airframe Structural Integrity Program in support of the aging commercial transport fleet. This interdisciplinary program is being worked in cooperation with the U.S. airframe manufacturers, airline operators, and the FAA. Advanced analysis methods are under development to predict the fatigue crack growth in complex built-up shell structures. Innovative nondestructive examination technologies are also under development to provide large area inspection capability to detect corrosion, disbonds, and fatigue cracks. Recent fracture mechanics results applicable to predicting the growth of cracks initiating at the rivets of fuselage splice joints are reviewed.

  15. Recent experimental results from a long-pulse J-band relativistic klystron amplifier developmental effort

    SciTech Connect

    Kato, K.G.; Crouch, D.D.; Sar, D.R.; Speciale, R.A.; Carlsten, B.E.; Fazio, M.V.; Haynes, W.B.; Stringfield, R.M.

    1994-12-31

    Recent experimental results, supporting simulations, and design modeling are presented from a developmental effort to a produce a long pulse ({approximately}1{mu}s) J-band (5.85-8.2 GHz) relativistic klystron amplifier (RKA) of the high current NRL genealogy. This RKA is designed to operate at approximately 6.6 GHz, with a desired RF output {approximately}700 MW. Conversion of electron beam energy to microwave energy is obtained by a mock magnetically insulated coaxial converter which, in various incarnations, can be made to be either a cavity gap extractor or an inverse cathode.

  16. Recent results and new hardware developments for protein crystal growth in microactivity

    NASA Technical Reports Server (NTRS)

    Delucas, L. J.; Long, M. M.; Moore, K. M.; Smith, C.; Carson, M.; Narayana, S. V. L.; Carter, D.; Clark, A. D., Jr.; Nanni, R. G.; Ding, J.

    1993-01-01

    Protein crystal growth experiments have been performed on 16 space shuttle missions since April, 1985. The initial experiments utilized vapor diffusion crystallization techniques similar to those used in laboratories for earth-based experiments. More recent experiments have utilized temperature induced crystallization as an alternative method for growing high quality protein crystals in microgravity. Results from both vapor diffusion and temperature induced crystallization experiments indicate that proteins grown in microgravity may be larger, display more uniform morphologies, and yield diffraction data to significantly higher resolutions than the best crystals of these proteins grown on earth.

  17. Community Agency Survey Formative Research Results From the TAAG Study

    PubMed Central

    Saunders, Ruth P.; Moody, Jamie

    2008-01-01

    School and community agency collaboration can potentially increase physical activity opportunities for youth. Few studies have examined the role of community agencies in promoting physical activity, much less in collaboration with schools. This article describes formative research data collection from community agencies to inform the development of the Trial of Activity for Adolescent Girls (TAAG) intervention to provide out-of-school physical activity programs for girls. The community agency survey is designed to assess agency capacity to provide physical activity programs for girls, including resources, programs, and partnerships. Most agency respondents (n = 138) report operations during after-school hours, adequate facilities, and program options for girls, although most are sport oriented. Agency resources and programming vary considerably across the six TAAG field sites. Many agencies report partnerships, some involving schools, although not necessarily related to physical activity. Implications for the TAAG intervention are presented. PMID:16397156

  18. Recent Results From The Nasa Earth Science Terra Mission and Future Possibilities

    NASA Technical Reports Server (NTRS)

    Salomonson, Vincent V.

    2000-01-01

    The NASA Earth Sciences Enterprise has made some remarkable strides in recent times in using developing, implementing, and utilizing spaceborne observations to better understand how the Earth works as a coupled, interactive system of the land, ocean, and atmosphere. Notable examples include the Upper Atmosphere Research (UARS) Satellite, the Topology Ocean Experiment (TOPEX) mission, Landsat-7, SeaWiFS, the Tropical Rainfall Monitoring Mission (TRMM), Quickscatt, the Shuttle Radar Topography Mission (SRTM), and, quite recently, the Terra'/Earth Observing System-1 mission. The Terra mission, for example, represents a major step forward in providing sensors that offer considerable advantages and progress over heritage instruments. The Moderate Resolution Imaging Spectrometer (MODIS), the Multi-angle Imaging SpectroRadiometer (MISR), the Measurements of Pollution in the Troposphere (MOPITT), the Advanced Spaceborne Thermal Emissions and Reflections (ASTER) radiometer, and the Clouds and Earth's Radiant Energy System (CERES) radiometer are the instruments involved. Early indications in March indicate that each of these instruments are working well and will be augmenting data bases from heritage instruments as well as producing new, unprecedented observations of land, ocean, and atmosphere features. Several missions will follow the Terra mission as the Earth Observing mission systems complete development and go into operation. These missions include EOS PM-1/'Aqua', Icesat, Vegetation Canopy Lidar (VCL), Jason/TOPEX Follow-on, the Chemistry mission, etc. As the Earth Observing systems completes its first phase in about 2004 a wealth of data enabling better understanding of the Earth and the management of its resources will have been provided. Considerable thought is beginning to be placed on what advances in technology can be implemented that will enable further advances in the early part of the 21st century; e.g., in the time from of 2020. Concepts such as

  19. Diagnostic impact of routine Lyme serology in recent-onset arthritis: results from the ESPOIR cohort

    PubMed Central

    Guellec, Dewi; Narbonne, Valérie; Cornec, Divi; Marhadour, Thierry; Varache, Sophie; Dougados, Maxime; Daurès, Jean Pierre; Jousse-Joulin, Sandrine; Devauchelle-Pensec, Valérie; Saraux, Alain

    2016-01-01

    Objectives Lyme disease may be considered by rheumatologists in patients with recent-onset arthritis, even in the absence of suggestive symptoms. The aim of this study was to determine the diagnostic impact of routine Lyme serology in a French cohort of patients with recent-onset arthritis affecting at least 2 joints. Methods We performed an ancillary study of a French prospective multicentre cohort established to monitor clinical, biological and radiographic data in patients with inflammatory arthritis in at least 2 joints, lasting for 6 weeks to 6 months. Borrelia IgM and IgG antibodies were sought routinely at baseline, using ELISA tests, independently from the physician's strategy for detecting a spirochetal infection. We recorded the proportion of patients with a final diagnosis of Lyme arthritis and evaluated the diagnostic performance of Lyme serology in this particular context. The clinical and biological characteristics of patients according to the Lyme serology results were analysed. Results Of 810 patients, 657 (81.1%) were negative for IgM and IgG antibodies, 91 (11.2%) had only IgM antibodies, 49 (6%) had only IgG antibodies, and 13 (1.6%) had IgG and IgM antibodies. Thus, 7.6% had IgG positivity, consistent with exposure to Borrelia infection. IgG positivity was significantly more prevalent in the North and North-East regions of France (χ2=14.6, p<0.001). No patients received a definite diagnosis of Lyme arthritis. Conclusions This study does not support routine Lyme serological testing in patients with recent-onset inflammatory arthritis affecting more than 1 joint. PMID:26819751

  20. Stratospheric spectroscopy with the far-infrared spectrometer (FIRS-2) - Overview and recent results

    NASA Technical Reports Server (NTRS)

    Traub, Wesley A.; Chance, Kelly V.; Johnson, David G.; Jucks, Kenneth W.

    1991-01-01

    The Smithsonian Astrophysical Observatory's program of balloon-borne stratospheric spectroscopic measurements is described, including instrumentation, recent scientific results, and future plans. The design and operation of the FIRS-2 far-infrared spectrometer is discussed. The current status of our efforts to recover mixing-ratio profiles with about 1 percent precision is presented. Representative recent results are shown giving mixing-ratio profiles from 20 to 50 km, selected from the suite HOCl, HCl, HF, NO2, N2O, HNO3, OH, HO2, H2O2, H2O (and isotopes), O2 (and isotopes), O3 (and isotopes), and CO2 (and isotopes). The utility of O2 and CO2 spectral lines for information on view angle or temperature and pressure is discussed. Future plans are mentioned, including the use of FIRS-2 on a balloon platform for UARS correlative measurements, the use of FIRS-2 on the NASA DC-8 platform for polar measurements, and the potential benefits of a FIRS instrument on a Shuttle platform.

  1. Recent results with ANTARES, the first undersea neutrino telescope in the Mediterranean Sea

    NASA Astrophysics Data System (ADS)

    Margiotta, Annarita; ANTARES Collaboration

    2016-05-01

    The ANTARES detector is the largest undersea neutrino telescope. It is located at about 2500 m under the sea level in front of the Southern French coast, 40 km from Toulon. Its location in the Mediterranean Sea and the good optical properties of the sea water makes it an excellent tool to search for possible sources of neutrinos in the sky region of the Galactic Plane. Its angular resolution, ~ 0.4°, and the effective area for neutrinos coming from the Southern sky allow to put constraints on the possible interpretation of the recent IceCube cosmic neutrino signal. The ANTARES collaboration has developed a rich program of multi-messenger searches together with experiments sensitive to other cosmic messengers. ANTARES has also produced results on neutrinos coming from the annihilation of Dark Matter particles. In particular, the limits obtained for the spin-dependent WIMP-nucleon cross section overcome the existing direct-detection experiments. An overview of the most interesting and recent results obtained with ANTARES are discussed, together with the future perspectives of analyses.

  2. Estimation of motility parameters from trajectory data. A condensate of our recent results

    NASA Astrophysics Data System (ADS)

    Vestergaard, C. L.; Pedersen, J. N.; Mortensen, K. I.; Flyvbjerg, H.

    2015-07-01

    Given a theoretical model for a self-propelled particle or micro-organism, how does one optimally determine the parameters of the model from experimental data in the form of a time-lapse recorded trajectory? For very long trajectories, one has very good statistics, and optimality may matter little. However, for biological micro-organisms, one may not control the duration of recordings, and then optimality can matter. This is especially the case if one is interested in individuality and hence cannot improve statistics by taking population averages over many trajectories. One can learn much about this problem by studying its simplest case, pure diffusion with no self-propagation. This is an interesting problem also in its own right for the very same reasons: interest in individuality and short trajectories. We summarize our recent results on this latter issue here and speculate about the extent to which similar results may be obtained also for self-propelled particles.

  3. Highlights of recent results from the VERITAS gamma-ray observatory

    NASA Astrophysics Data System (ADS)

    Fortson, Lucy; VERITAS Collaboration

    2016-05-01

    VERITAS is a major ground-based gamma-ray observatory comprising an array of four 12 meter air Cherenkov telescopes operating at the Fred Lawrence Whipple Observatory near Tucson, Arizona. Data taking has continued from 2007 with a major camera upgrade completed in 2012 resulting in the current sensitivity to very-high-energy (VHE) gamma rays between 85 GeV and 30 TeV. VERITAS has detected 54 sources (half of which have been discoveries) leading to many significant contributions to the field of VHE astronomy. These proceedings highlight some of the more recent VERITAS results from the blazar and galactic observing programs as well as measurements of the cosmic-ray electron spectrum, constraints on dark matter and a follow-up program for astrophysical neutrinos.

  4. NEOWISE: Recent Results and Observations of Tiny Near-Earth Objects

    NASA Astrophysics Data System (ADS)

    Mainzer, Amanda K.; Bauer, J.; Grav, T.; Masiero, J.; Nugent, C.; Cutri, R.; Wright, E. L.; NEOWISE Team

    2013-10-01

    The minor planet-hunting portion of the Wide-field Infrared Survey Explorer mission (Wright et al. 2010), known as NEOWISE, has resulted in the creation of an archive of single exposure images and extracted sources collected by this infrared all-sky survey (Mainzer et al. 2011). All data products have now been publicly released through NASA's Infrared Science Archive (Cutri et al. 2012). Along with the single exposure images and source databases, the NEOWISE project supported the development of tools for solar system-friendly queries of the data. We have used these tools to extract mid-infrared observations of near-Earth objects that make extremely close approaches to the Earth. Using these observations, we have computed physical properties for these objects. An overview of these derived properties as well as other recent results and status from the project will be presented.

  5. Recent results on lead-ion accumulation in LEAR for the LHC

    NASA Astrophysics Data System (ADS)

    Baird, S.; Bosser, J.; Broere, J.; Carli, C.; Chanel, M.; Hill, C.; Ley, R.; Lombardi, A.; Maccaferri, R.; Maury, S.; Meshkov, I.; Möhl, D.; Molinari, G.; Mulder, H.; Syresin, E.; Tanke, E.; Tranquille, G.; Varenne, F.; Vretenar, M.

    1997-02-01

    To prepare dense bunches of lead ions for the LHC it has been proposed to accumulate the 4.2 MeV/u linac beam in a storage ring with electron cooling. A series of experiments is being performed in the low-energy ring LEAR to test this technique. First results were already reported at the Beam Crystallisation Workshop in Erice in November 1995. Two more recent runs to complement these investigations were concerned with: further study of the beam lifetime; the dependence of the cooling time on optical settings of the storage ring and on neutralization of the electron beam; and tests in view of multiturn injection. New results obtained in these two runs in December 1995 and in April 1996 will be discussed in this contribution.

  6. P-MaNGA: Gradients in Recent Star Formation Histories as Diagnostics for Galaxy Growth and Death

    NASA Astrophysics Data System (ADS)

    Li, Cheng; Wang, Enci; Lin, Lin; Bershady, Matthew A.; Bundy, Kevin; Tremonti, Christy A.; Xiao, Ting; Yan, Renbin; Bizyaev, Dmitry; Blanton, Michael; Cales, Sabrina; Cherinka, Brian; Cheung, Edmond; Drory, Niv; Emsellem, Eric; Fu, Hai; Gelfand, Joseph; Law, David R.; Lin, Lihwai; MacDonald, Nick; Maraston, Claudia; Masters, Karen L.; Merrifield, Michael R.; Pan, Kaike; Sánchez, S. F.; Schneider, Donald P.; Thomas, Daniel; Wake, David; Wang, Lixin; Weijmans, Anne-Marie; Wilkinson, David; Yoachim, Peter; Zhang, Kai; Zheng, Tiantian

    2015-05-01

    We present an analysis of the data produced by the MaNGA prototype run (P-MaNGA), aiming to test how the radial gradients in recent star formation histories, as indicated by the 4000 Å break (Dn(4000)), Hδ absorption (EW(HδA)), and Hα emission (EW(Hα)) indices, can be useful for understanding disk growth and star formation cessation in local galaxies. We classify 12 galaxies observed on two P-MaNGA plates as either centrally quiescent (CQ) or centrally star-forming (CSF), according to whether Dn(4000) measured in the central spaxel of each datacube exceeds 1.6. For each spaxel we generate both 2D maps and radial profiles of Dn(4000), EW(HδA), and EW(Hα). We find that CSF galaxies generally show very weak or no radial variation in these diagnostics. In contrast, CQ galaxies present significant radial gradients, in the sense that Dn(4000) decreases, while both EW(HδA) and EW(Hα) increase from the galactic center outward. The outer regions of the galaxies show greater scatter on diagrams relating the three parameters than their central parts. In particular, the clear separation between centrally measured quiescent and star-forming galaxies in these diagnostic planes is largely filled in by the outer parts of galaxies whose global colors place them in the green valley, supporting the idea that the green valley represents a transition between blue-cloud and red-sequence phases, at least in our small sample. These results are consistent with a picture in which the cessation of star formation propagates from the center of a galaxy outward as it moves to the red sequence.

  7. Eastern Olympus Mons Basal Scarp and Aureole lobe: Recent Structural Evidence for Formation and Development

    NASA Astrophysics Data System (ADS)

    Weller, M. B.; McGovern, P. J.; Fournier, T.; Morgan, J. K.; Katz, O.

    2012-12-01

    The origin of the Olympus Mons (OM) basal scarp and the adjacent enigmatic aureole lobe deposits have long been controversial, with many hypotheses having been postulated for their linked formation, ranging from sub-glacial eruptions (e.g. Helgason, 1999), to numerous landslide and flank collapse models (e.g. Borgia, 1990; Lopes et al., 1980). While a landslide origin is compelling upon the examination of the OM basal scarp morphology, much of the controversy remains, and the subsurface structure of OM is not well understood. With the release of high resolution Digital Terrain Models (DTMs) of Mars from High Resolution Stereo Camera (HRSC) data, we examine a unique portion of the edifice, the Eastern OM Basal Scarp (EOMBS). The EOMBS exhibits two parallel bounding structures: a nearly 100 km-long up-slope extensional normal fault system, with associated offsets on the order of 10-100m, bordered by radial tear faults; and a 160-200 km-long down-slope contractional wrinkle ridge network of varying vergence, inferred to define the boundaries of a "pop-up" structure, associated offsets are on the order of 100m, and were last inferred to be active in recent geologic time at < 45 Ma (Basilevsky et al., 2006). The wrinkle ridge network extends an additional 60-100 km south of the identified normal fault system. We suggest that these fault systems, within the region of the radial tear faults, may be linked by failure surfaces, that their displacements accommodate downslope movement of the flank, and may be direct evidence linking the "East" aureole lobe to the EOMBS. Calculations based on limit equilibrium principles, and matched to the observed faulting locations and slope geometries, suggests a mechanically weak, pore-fluid saturated detachment layer (e.g. similar to phyllosilicates), at a depth of 0 to -3km below the reference datum, underlies eastern OM, consistent with models of OM as a spreading volcanic edifice (Borgia, 1990; McGovern and Morgan, 2009). Our

  8. Recent results in explosive and s-process nucleosynthesis from measurements on radioactive and stable targets

    SciTech Connect

    Koehler, P.E.; Kaeppeler, F.; Schatz, H.

    1993-07-01

    Measurements of (n,p) and (n,{alpha}) cross sections are crucial for a better understanding of many scenarios of nucleosynthesis. Current problems in which such reactions play a roll include the possible synthesis of heavy element during the big bang. The production of several rare isotopes in explosive nucleosynthesis, and a better understanding of the role of the s process in the synthesis of light and intermediate mass nuclei. We have recently completed measurements of several (n,p) and (n,{alpha}) cross sections of importance to nuclear astrophysics. The cross sections were measured in the range from thermal energy to approximately 1 MeV by using the white neutron source at the Manuel Lujan, Jr. Neutron Scattering Center (LANSCE) in Los Alamos. We have also made complementary measurements at the Karlsruhe Van de Graaff and at thee Oak Ridge Electron Linear Accelerator (ORELA). We discuss the impact of the results on nuclear astrophysics as well as recent improvements and future plans.

  9. Recent Star Formation in the Lupus Clouds as Seen by Herschel

    NASA Astrophysics Data System (ADS)

    Rygl, Kazi L. J.; Benedettini, Milena

    We present a study of the star formation histories of the Lupus I, III, and IV clouds using the Herschel 70-500 μm maps obtained by the Herschel Gould Belt Survey Key-Project. By combining the new Herschel data with the existing Spitzer catalog we obtained an unprecedented census of prestellar sources and young stellar objects in the Lupus clouds, which allowed us to study the overall star formation rate (SFR) and efficiency (SFE). The high SFE of Lupus III and its decreasing SFR suggest that Lupus III is the most evolved cloud, that after having experienced a major star formation event, is now approaching the end of its current star-forming cycle. Lupus I is currently undergoing a large star formation event, apparent by the increasing SFR. Also Lupus IV has an increasing SFR, however, the relative number of prestellar sources is much lower than in Lupus I, suggesting that its star formation has not yet reached its peak.

  10. Involvement of the Anterior Cingulate Cortex in Formation, Consolidation, and Reconsolidation of Recent and Remote Contextual Fear Memory

    ERIC Educational Resources Information Center

    Einarsson, Einar O.; Nader, Karim

    2012-01-01

    It has been suggested that memories become more stable and less susceptible to the disruption of reconsolidation over weeks after learning. Here, we test this by targeting the anterior cingulate cortex (ACC) and test its involvement in the formation, consolidation, and reconsolidation of recent and remote contextual fear memory. We found that…

  11. Recent results on central Pb+Pb collisions from experiment NA49

    NASA Astrophysics Data System (ADS)

    Appelshäuser, H.; Bächler, J.; Bailey, S. J.; Barnby, L. S.; Bartke, J.; Barton, R. A.; Biał Kowska, H.; Billmeier, A.; Blyth, C. O.; Bock, R.; Bormann, C.; Brady, F. P.; Brockmann, R.; Brun, R.; Bunč Ić , P.; Caines, H. L.; Cebra, D.; Cooper, G. E.; Cramer, J. G.; Csato, P.; Dunn, J.; Eckardt, V.; Eckhardt, F.; Ferguson, M. I.; Fischer, H. G.; Flierl, D.; Fodor, Z.; Foka, P.; Freund, P.; Friese, V.; Fuchs, M.; Gabler, F.; Gal, J.; Gaź Dzicki, M.; Gł Adysz, E.; Grebieszkow, J.; Günther, J.; Harris, J. W.; Hegyi, S.; Henkel, T.; Hill, L. A.; Huang, I.; Hümmler, H.; Igo, G.; Irmscher, D.; Jacobs, P.; Jones, P. G.; Kadija, K.; Kolesnikov, V. I.; Kowalski, M.; Lasiuk, B.; Lévai, P.; Malakhov, A. I.; Margetis, S.; Markert, C.; Melkumov, G. L.; Mock, A.; Molnár, J.; Nelson, J. M.; Oldenburg, M.; Odyniec, G.; Palla, G.; Panagiotou, A. D.; Petridis, A.; Piper, A.; Porter, R. J.; Poskanzer, A. M.; Poziombka, S.; Prindle, D. J.; Pühlhofer, F.; Rauch, W.; Reid, J. G.; Renfordt, R.; Retyk, W.; Ritter, H. G.; Röhrich, D.; Roland, C.; Roland, G.; Rudolph, H.; Rybicki, A.; Sandoval, A.; Sann, H.; Semenov, A. Yu.; Schäfer, E.; Schmischke, D.; Schmitz, N.; Schönfelder, S.; Seyboth, P.; Seyerlein, J.; Sikler, F.; Skrzypczak, E.; Squier, G. T. A.; Stock, R.; Ströbele, H.; Szentpetery, I.; Sziklai, J.; Szymanski, P.; Toy, M.; Trainor, T. A.; Trentalange, S.; Ullrich, T.; Vassiliou, M.; Vesztergombi, G.; Vranić , D.; Wang, F.; Weerasundara, D. D.; Wenig, S.; Whitten, C.; Wienold, T.; Wood, L.; Yates, T. A.; Zimanyi, J.; Zhu, X.-Z.; Zybert, R.

    1998-08-01

    In this paper we present recent results from experiment NA49 on single- and multiparticle distributions obtained for Pb+Pb collisions at 158GeV/nucleon at the CERN SPS. NA49 aims at a complete description of the hadronic final state of nuclear collisions, which will eventually allow us to establish whether an equilibrated, deconfined state of partonic matter, the quark gluon plasma (QGP), is created in the early stages of these collisions. New experimental results regarding the evolution of the hadron source through transverse expansion to chemical and thermal freeze-out are presented. We find that the available data can be understood in terms of simple physical pictures, indicating that sufficient energy densities for QGP creation are indeed reached in the early stage of the collision. The NA49 results on particle abundances are discussed in comparison with nuclear collisions at lower energy and elementary collisions at various energies. This comparison demonstrates that simple extrapolation from these systems fails to describe the results for Pb+Pb collisions at the CERN SPS.

  12. Recent Results from a Laboratory Study of Charging Mechanisms in a Dusty Plasma

    NASA Technical Reports Server (NTRS)

    Venturini, Catherine C.; Spann, James F., Jr.; Comfort, Richard H.

    1998-01-01

    A laboratory investigation has been developed to experimentally study the interaction of micron sized particles with plasmas and electromagnetic radiation. The intent is to investigate under what conditions particles of various compositions and sizes become charged, or discharged, while exposed to an electron beam and UV radiation. This investigation uses a unique laboratory technique known as electrodynamic suspension of particles. Here, a single charged micron size particle is suspended in a quadrupole trap and then subjected to a controlled environment. In this paper, we will discuss recent results from this experiment in which different materials including polystyrene and aluminum oxide, and sizes ranging from 10 microns to 1 micron have been used to determine charge to mass ratios and then subjected to an electron beam and /or UV radiation. In each instance, the particle's charge as well as beam current flux and radiation intensity flux is measured. These results will be compared with initial results using salt crystals. It was found that a negatively charged salt crystal exposed for 30 minutes to a 500 eV electron beam with primary electron beam current of -3.06 x 10(exp -5) picoamps yielded a secondary electron current of 3.23 x 10(exp -5) picoamps. Additionally, the particle was observed to be steadily losing charge over this time interval. By studying the microphysics of one particle, a better understanding of theoretical models and other laboratory results associated with particle charging mechanisms can be achieved.

  13. Modeling of dust halo formation following comet outbursts Preliminary results

    NASA Technical Reports Server (NTRS)

    Gombosi, T. I.; Horanyi, M.

    1986-01-01

    Evolution of gas and dust distributions following a spatially and temporally localized comet outburst was calculated using a hybrid kinetic - hydrodynamic method. It was found that a comet outburst resulted in significantly increased dust terminal velocities. As these higher terminal velocity values result in larger apex distances, therefore the outburst generates distinct dust envelopes in front of the regular dust coma. Such envelopes were observed at several comets (cf. comet Donati).

  14. Recent Results from the Wide Angle Search for Planets (WASP) Prototype

    NASA Astrophysics Data System (ADS)

    Kane, S. R.; Horne, K.; Street, R. A.; Pollaco, D. L.; James, D.; Tsapras, Y.; Collier Cameron, A.

    WASP0 is a prototype for what is intended to become a collection of WASPs whose primary aim is to detect transiting extrasolar planets across the face of their parent star. The WASP0 instrument is a wide-field (9-degree) 6.3 cm aperture F/2.8 Apogee 10 CCD camera (2Kx2K chip, 16-arcsec pixels). The camera is mounted piggy-back on a commercial 10-inch Meade telescope. We present some recent results from the WASP camera, including observations from La Palma of the known transiting planet around HD 209458 and preliminary analysis of other stars located in the same field. We also outline further problems which restrict the ability to achieve photon limited precision with a wide-field commercial CCD.

  15. The Trojan Horse method for nuclear astrophysics: Recent results for direct reactions

    SciTech Connect

    Tumino, A.; Gulino, M.; Spitaleri, C.; Cherubini, S.; Romano, S.; Cognata, M. La; Pizzone, R. G.; Rapisarda, G. G.; Lamia, L.

    2014-05-09

    The Trojan Horse method is a powerful indirect technique to determine the astrophysical factor for binary rearrangement processes A+x→b+B at astrophysical energies by measuring the cross section for the Trojan Horse (TH) reaction A+a→B+b+s in quasi free kinematics. The Trojan Horse Method has been successfully applied to many reactions of astrophysical interest, both direct and resonant. In this paper, we will focus on direct sub-processes. The theory of the THM for direct binary reactions will be shortly presented based on a few-body approach that takes into account the off-energy-shell effects and initial and final state interactions. Examples of recent results will be presented to demonstrate how THM works experimentally.

  16. Neutron detection with noble gas scintillation: a review of recent results

    NASA Astrophysics Data System (ADS)

    Lavelle, C. M.; Coplan, Michael; Miller, Eric C.; Thompson, Alan K.; Kowler, Alex; Vest, Rob; Yue, Andrew; Koeth, Tim; Al-Sheikhly, Mohammad; Clark, Charles

    2015-08-01

    Thermal neutron detection is of vital importance to many disciplines, including neutron scattering, workplace monitoring, and homeland protection. We survey recent results from our collaboration which couple low-pressure noble gas scintillation with novel approaches to neutron absorbing materials and geometries to achieve potentially advantageous detector concepts. Noble gas scintillators were used for neutron detection as early as the late 1950's. Modern use of noble gas scintillation includes liquid and solid forms of argon and xenon in the dark matter and neutron physics experiments and commercially available high pressure applications have achieved high resolution gamma ray spectroscopy. Little attention has been paid to the overlap between low pressure noble gas scintillation and thermal neutron detection, for which there are many potential benefits.

  17. Recent Results of Semi-inclusive DIS Experiments at Jefferson Lab

    SciTech Connect

    Allada, Kalyan

    2015-09-01

    Semi-inclusive deep inelastic scattering (SIDIS) is a powerful tool to explore the 3-d structure of nucleon in momentum space. Through a combination of polarized or unpolarized lepton beam and nucleon target one can study various transverse-momentum dependent parton distribution functions (TMDs) that appear in the SIDIS cross-section. TMDs provide a description of nucleon structure in terms of parton’s transverse momentum and its transverse spin, which enables us to study the quark orbital angular momentum effects in the nucleon. Several SIDIS experiments were performed in three experimental halls at JLab with 6 GeV electron beam using both polarized or upolarized beam and target combinations. The kinematic range was mainly focued on valence quark region. In this proceeding we will discuss some of the recent results from JLab 6 GeV run.

  18. Recent Results of Target Single-Spin Asymmetry Experiments at Jefferson Lab

    SciTech Connect

    Jiang, Xiaodong

    2013-08-01

    We report recent results from Jefferson Lab Hall A “Neutron Transversity” experiment (E06-010). Transversely polarized target single-spin asymmetry AUT and beam-target double-spin asymmetry A{sub LT} have been measured in semi-inclusive deep-inelastic scattering (SIDIS) reactions on a polarized neutron ({sup 3}He) target. Collins-type and Sivers-type asymmetries have been extracted from A{sub UT} for charged pion SIDIS productions, which are sensitive to quark transversity and Sivers distributions, correspondingly. Double spin asymmetry A{sub LT} is sensitive to a specific quark transverse momentum dependent parton distribution (TMD), the so-called “ transverse helicity” (g{sub 1T} ) distributions. In addition, target single-spin asymmetries A{sub y} in inclusive electron scattering on a transversely polarized {sup 3}He target in quasi-elastic and deep inelastic kinematics were also measured in Hall A.

  19. Recent results from ArgoNeuT and status of MicroBooNE

    SciTech Connect

    Szelc, A. M.

    2015-07-15

    Liquid Argon Time Projection Chambers (LArTPCs) are a novel detector technology for neutrino detection experiments. Their fine granularity combined with calorimetric capabilities allows for precision measurements that will answer the outstanding questions about the role of neutrinos in the Standard Model of Particle physics and beyond it. Here, we discuss the development effort underway in the framework of the US based LArTPC program, which ties improving the reach of the technology with relevant physics measurements of beam neutrinos at Fermilab. Examples of experiments in this program are ArgoNeuT which ran on the NuMI beam line and acquired 1.35×10{sup 20} POT and MicroBooNE which is set to run on the Booster neutrino beamline at the beginning of 2015. Recent results from the ArgoNeuT experiment will be discussed as well as the status and prospects for MicroBooNE.

  20. Actinic review of EUV masks: status and recent results of the AIMSTM EUV system

    NASA Astrophysics Data System (ADS)

    Perlitz, Sascha; Peters, Jan Hendrik; Weiss, Markus; Hellweg, Dirk; Capelli, Renzo; Magnusson, Krister; Malloy, Matt; Wurm, Stefan

    2015-10-01

    Key enabler of the successful introduction of EUV lithography into volume production is the EUV mask infrastructure. For the production of defect free masks, actinic review of potential defect sites to decide on the need for repair or compensation is required. Also, the repair or compensation with the ZEISS MERiT electron beam repair tool needs actinic verification in a closed loop mask repair solution. For the realization of actinic mask review, ZEISS and the SEMATECH EUVL Mask Infrastructure consortium started a development program for an EUV aerial image metrology system, the AIMSTM EUV, with realization of a prototype tool. The development and prototype realization of the AIMSTM EUV has entered the tool calibration and qualification phase utilizing the achieved capabilities of EUV aerial image acquisition and EUV mask handling. In this paper, we discuss the current status of the prototype qualification and show recent measurement results.

  1. Recent results from the EBIT and Super EBIT at Lawrence Livermore National Laboratory

    SciTech Connect

    Marrs, R.E.

    1996-10-07

    The electron beam ion trap (EBIT), and the higher-energy Super EBIT at Lawrence Livermore National Laboratory can produce any highly charged ion. These highly charged ions are used in a variety of research programs. Recent results from four different experiments are reviewed here. K-shell ionization cross sections have been measured for the hydrogenlike ions of several elements, and L-shell ionization cross sections have been measured for uranium ions. A measurement of the ground-state hyperfine transition in hydrogenlike {sup 165}H{sup 66+} is notable because of the complete absence of Doppler shifts. A cryogenic Penning trap, injected with EBIT ions, has been used to observe a single highly charged ion as it recombines by sequential electron capture from H{sub 2} gas. A large sputtered ion yield, suggesting a surface Coulomb explosion, has been observed from insulators bombarded with very highly charged EBIT ions. 21 refs., 11 figs.

  2. The Trojan Horse method for nuclear astrophysics: Recent results for direct reactions

    NASA Astrophysics Data System (ADS)

    Tumino, A.; Spitaleri, C.; Cherubini, S.; Gulino, M.; La Cognata, M.; Lamia, L.; Pizzone, R. G.; Rapisarda, G. G.; Romano, S.

    2014-05-01

    The Trojan Horse method is a powerful indirect technique to determine the astrophysical factor for binary rearrangement processes A+x→b+B at astrophysical energies by measuring the cross section for the Trojan Horse (TH) reaction A+a→B+b+s in quasi free kinematics. The Trojan Horse Method has been successfully applied to many reactions of astrophysical interest, both direct and resonant. In this paper, we will focus on direct sub-processes. The theory of the THM for direct binary reactions will be shortly presented based on a few-body approach that takes into account the off-energy-shell effects and initial and final state interactions. Examples of recent results will be presented to demonstrate how THM works experimentally.

  3. Cascade Spectroscopy and Recent Xi* Photo-production Results from CLAS

    SciTech Connect

    John T. Goetz

    2010-08-01

    Doubly-strange baryon resonances provide new insights into baryon structure. The standard QCD Lagrangian implies that for every N* and Delta* resonance, there should be a corresponding Xi (cascade resonance). This is due to the flavor symmetry of the strong force. Therefore, one can investigate baryon structure by observing aspects of the doubly-strange baryons like regularities such as parity doublets. At energies above approximately 1.5 GeV, the light-quark baryon resonances are broad and overlap while the cascades in this range are narrow and therefore more readily observed. An overview of the world cascade spectrum and a comparison to the lighter baryon spectra will be presented. Recent results from an on-going analysis from the G12 (5.4 GeV) photo-production experiment using the CLAS detector at JLab will be highlighted.

  4. "The open sky rhinoplasty" for correction of secondary cleft lip nose deformity, Technique and recent results.

    PubMed

    Tschopp, H M

    1988-01-01

    The typical nose deformity after cleft-lip repair still represents great challenge for the plastic surgeon in this field. Many methods have been designed in attempts to correct the deformity, either during primary closure of the lip or as a secondary procedure when growth of the nose is complete. In this paper the author's own technique of secondary rhinoseptoplasty in cleft-lip patients is presented. The different cartilaginous and osseous structures are approached through a transcolumellar incision and the skin of the nose completely reflected upwards. This so-called "open sky view" gives a total perspective on the entire pathology of the cleft-lip nose deformity and makes it possible to correct it accordingly. Emphasis is put on some important surgical manoeuvers. Recent results are presented and the pros and cons of this procedure discussed. PMID:3187450

  5. Recent Results from the Relativistic Electron Proton Telescope (REPT) onboard the Van Allen Probes Mission

    NASA Astrophysics Data System (ADS)

    Kanekal, S. G.; Baker, D. N.; Elkington, S. R.; Hoxie, V. C.; Li, X.; Spence, H. E.

    2013-05-01

    We describe recent results from the REPT instruments on board Van Allen Probes mission launched on 30 August 2012. The twin spacecraft comprising the Van Allen probes mission are identically instrumented and carry a comprehensive suite of sensors characterizing magnetospheric charged particle populations, electric and magnetic fields and plasma waves. The REPT instruments comprise a well-shielded silicon solid state detector stack, with a state of the art electronics and measure electrons of ~1.5 to > 20 MeV and protons of ~17 to > 100 MeV. The instruments were commissioned 3 days after launch and continue to provide high quality measurements. We describe the Van Allen probes and the REPT instrument and report on the new and unexpected features of the outer zone electron populations observed by REPT.

  6. Recent Results from the SPLASH Survey: Chemical Abundances and Kinematics of Andromeda's Stellar Halo

    NASA Astrophysics Data System (ADS)

    Gilbert, Karoline

    2015-08-01

    Large scale surveys of Andromeda's resolved stellar populations have revolutionized our view of this galaxy over the past decade. The combination of large-scale, contiguous photometric surveys and pointed spectroscopic surveys has been particularly powerful for discovering and following up new substructures and disentangling the structural components of Andromeda. The SPLASH (Spectroscopic and Photometric Landscape of Andromeda's Stellar Halo) survey consists of broad- and narrow-band imaging and spectroscopy of red giant branch stars in lines of sight throughout the M31 system, ranging in distance from 3 kpc to more than 200 kpc from Andromeda's center. I will present recent results from the SPLASH survey on the structure of Andromeda's stellar halo and the origin of tidal debris features, including measurements of the kinematics and chemical abundances of Andromeda's halo stars.

  7. Recent Multispectral Imaging Results from the Pancam Instruments on the Mars Exploration Rovers Spirit and Opportunity

    NASA Astrophysics Data System (ADS)

    Bell, J. F.

    2006-12-01

    As of early September 2006, the Mars Exploration Rover Panoramic Camera (Pancam) instruments have acquired more than 57,000 and 52,000 multispectral images, respectively, from the rovers' landing sites and traverse paths within Gusev crater and Meridiani Planum. These observations include more than 950 and 600 full multispectral imaging observations, respectively, in the 11 distinct near-UV to near-IR wavelengths sampled by the Pancams. Both rovers have faced challenges in their exploration activities during 2006 because of power restrictions imposed by the low-Sun, southern hemisphere winter conditions. Still, major science campaigns have been conducted at both landing sites. At Gusev, Pancam imaging documented major geomorphic and color units during the Spirit rover's traverse down the south side of Husband Hill and across the Southern Basin to the possible volcanic or impact feature known as Home Plate. More recently, at Spirit's "Winter Haven" stationary location in Gusev crater, a full-resolution, 360 degree, low-compression panorama (the "McMurdo" panorama) has been obtained using all of Pancam's filters. In Meridiani, the geology and color properties of the terrain during Opportunity's traverse south from Erebus crater to its current location at the rim of Victoria crater has been documented in detail by Pancam multispectral imaging, including a number of albedo measurements and other coordinated observations with orbiting NASA and ESA spacecraft designed to enhance surface-orbital "ground truth" connections. Panoramas, mosaics, and multispectral analysis results from these recent Pancam data sets will be summarized and discussed in terms of their geologic context and complimentarity to other MER remote sensing and in situ investigations and results obtained during this past year.

  8. Recent results in single-pixel compressive imaging using selective measurement strategies

    NASA Astrophysics Data System (ADS)

    Herman, Matthew A.; Weston, Tyler; McMackin, Lenore; Li, Yun; Chen, Jianbo; Kelly, Kevin F.

    2015-05-01

    This paper reports an overview of recent results in compressive imaging and detection using a single-pixel camera. These applications use a digital micromirror device to spatially modulate the light from an observed scene using binary sensing patterns. The patterns are obtained from a special Hadamard matrix that contains blocks of rows of which each has a common local signature pattern. The blocks partition the Hadamard spectrum, thus permitting analysis of the scene in terms of these local signature patterns. In contrast, Hadamard patterns are typically described in terms of their sequency, which is a global property of each individual row. The proposed local-signature, row-block point of view can be beneficial since it permits us to adaptively select the best blocks with which to sense the signal/scene of interest, or to select the best blocks based on a priori information. As a result, in imaging applications more fine-scale detail can be extracted from the scene, and in detection applications fewer false positives can result. Note, this signature row-block partitioning is a general mathematical technique that can be applied to the Kronecker product of any two matrices, of any size. For example, in our imaging application, we extend this idea to a Hadamard matrix that is not a power of two, yet whose block-signatures possess the familiar Sylvester-Walsh power-of-two sequency patterns.

  9. Signatures of Recent Asteroid Disruptions in the Formation and Evolution of Solar System Dust Bands

    NASA Astrophysics Data System (ADS)

    Espy Kehoe, A. J.; Kehoe, T. J. J.; Colwell, J. E.; Dermott, S. F.

    2015-09-01

    We have performed detailed dynamical modeling of the structure of a faint dust band observed in coadded InfraRed Astronomical Satellite data at an ecliptic latitude of 17° that convincingly demonstrates that it is the result of a relatively recent (significantly less than 1 Ma) disruption of an asteroid and is still in the process of forming. We show here that young dust bands retain information on the size distribution and cross-sectional area of dust released in the original asteroid disruption, before it is lost to orbital and collisional decay. We find that the Emilkowalski cluster is the source of this partial band and that the dust released in the disruption would correspond to a regolith layer ∼3 m deep on the ∼10 km diameter source body's surface. The dust in this band is described by a cumulative size-distribution inverse power-law index with a lower bound of 2.1 (implying domination of cross-sectional area by small particles) for dust particles with diameters ranging from a few μm up to a few cm. The coadded observations show that the thermal emission of the dust band structure is dominated by large (mm–cm size) particles. We find that dust particle ejection velocities need to be a few times the escape velocity of the Emilkowalski cluster source body to provide a good fit to the inclination dispersion of the observations. We discuss the implications that such a significant release of material during a disruption has for the temporal evolution of the structure, composition, and magnitude of the zodiacal cloud.

  10. Modelling of groundwater mound formation resulting from transient recharge

    NASA Astrophysics Data System (ADS)

    Rai, S. N.; Ramana, D. V.; Thiagarajan, S.; Manglik, A.

    2001-06-01

    An analytical solution of a linearized Boussinesq equation is obtained to predict water table fluctuations as a result of time varying recharge from a strip basin for any number of recharge cycles. The analytical solution is obtained by using finite Fourier sine transform. Applications of the solution for the prediction of water table fluctuations and sensitivity analysis are demonstrated with the help of example problems.

  11. Recent results from the University of Washington's 38 mm ram accelerator

    NASA Astrophysics Data System (ADS)

    de Turenne, J. A.; Chew, G.; Bruckner, A. P.

    1992-07-01

    The ram accelerator is a propulsive device that accelerates projectiles using gasdynamic cycles similar to those which generate thrust in airbreathing ramjets. The projectile, analogous to the centerbody of a ramjet, travels supersonically through a stationary tube containing a gaseous fuel and oxidizer mixture. The projectile itself carries no onboard propellant. A combustion zone follows the projectile and stabilizes the shock structure. The resulting pressure distribution continuously accelerates the projectile. Several modes of ram accelerator operation have been investigated experimentally and theoretically. At velocities below the Chapman-Jouguet (C-J) detonation speed of the propellant mixture, the thermally choked propulsion mode accelerates the projectiles. At projectile velocities between approximately 90 and 110 percent of the C-J speed, a transdetonative propulsion mode occurs. At velocities beyond 110 percent of the C-J speed, projectiles experience superdetonative propulsion. This paper presents recent experimental results from these propulsion modes obtained with the University of Washington's 38-mm bore ram accelerator. Data from investigations with hydrogen diluted-gas mixtures are also introduced.

  12. Recent Advances and Some Results in Plasma-Based Accelerator Modeling

    NASA Astrophysics Data System (ADS)

    Mori, W. B.

    2002-12-01

    Simulation, using particle-in-cell (PIC) methods, has played a critical role in the evolution of the field of plasma-based acceleration. Early on, simulations allowed the testing of new ideas using so-called cartoon parameters. These simulations were done in either one or two-dimensions using single processor supercomputers. Through the development of new algorithms and parallel computing, today, we can now use PIC simulations to model the full-scale of ongoing experiments in three-dimensions. These experiments are attempting to accelerate electrons to ˜1 GeV. In this article, I will present recent results in which simulation results are compared to experiment and I will discuss the future challenges in advanced accelerator modeling. Principally, these are 1.) to be able to model a 100+ on 100+ GeV collider in three-dimensions and, 2.) to develop more efficient, yet still accurate, algorithms so that simulation can be used for real-time feedback with experiment.

  13. High-Resolution Spectroscopy of Mars: Recent Results and Implications for Atmospheric Evolution

    NASA Technical Reports Server (NTRS)

    Krasnopolsky, V. A.; Owen, T. C.; Maillard, J. P.

    1999-01-01

    It is believed that Earth, Venus, and Mars were formed by the same rocky and icy planetesimals, which resembled meteorites and comets in their composition, respectively. These planets are thus expected to have initially had the same chemical and isotope composition. Scaling the mass of the terrestrial ocean by the planetary mass ratio, the expected initial H2O abundance on Mars is a layer of about 1 km thick. Scaling the abundance of CO2 on Venus, the expected initial CO2 abundance on Mars is 15 bars. Evidently, significant parts of the initial H2O and CO2 abundances have been lost. Intense meteorite impact erosion and hydrodynamic escape of hydrogen (which could drag to escape more heavy species) were dominant loss processes in the first 0.8 Byr. Later, atmospheric sputtering by O+ ions resulted in the dissociation of CO2 and massive losses of O, C, and H. Formation of carbonates also reduced CO2 to its present abundance which currently exists in the atmosphere, on the polar caps, and is absorbed by regolith. Water loss is currently due to thermal escape of H and nonthermal escape of O, both formed by photodissociation of H2O. All loss processes resulted in fractionation of the H, O, and C isotopes. Therefore, the current isotope ratios in H2O and CO2 are clues to the history of volatiles on Mars. There are three tools to study H2O and CO2 isotopes in the martian atmosphere: (i) mass spectrometry from landing probes, (ii) analyses of Mars' gases trapped in the SNC meteorites which were ejected from Mars, and (iii) high-resolution spectroscopy of the H2O andCO2 bands. Method (i) is the best but is the most expensive. Mass spectrometers to be used should be designed for high-precision isotope measurements. Method (ii) makes it possible to reach an uncertainty +/- 0.1%. However, the obtained results are affected by some uncontrolled interactions: isotope fractionations of (1) trapped gases and (2) those released in pyrolysis, (3) contribution of the impactor, isotope

  14. Results of Gamma-Ray Measurements from a Recent Demonstration for Russian Technical Experts

    SciTech Connect

    Luke, S J; Archer, D E; Gosnell, T B; Lochner, R T; Morgan, J F; White, G K; Weitz, R

    2001-06-01

    In August 2001, a group of U.S. technical experts demonstrated an Attribute Measurement System with an Information Barrier (AMSIB) for a delegation of Russian technical experts. The purpose of the demonstration was to show that attributes of a classified plutonium item of potential interest to arms control and nonproliferation transparency regimes could be ascertained without releasing any sensitive information. For this demonstration, both gamma-ray and neutron attributes were determined. We consider only the gamma-ray attributes here. The specific plutonium attributes measured were the isotopic ratio of {sup 240}Pu to {sup 239}Pu, the ''age'' of the plutonium (time elapsed since the most recent chemical purification of the plutonium), and the absence of plutonium oxide in the item's storage container. In this paper, we briefly review the technologies employed for the attribute measurements used in the gamma-ray portion of the demonstration, concentrating on the results of the test measurements of the isotopic and age attributes made on unclassified items.

  15. Characteristics of the strongly Interacting Quark Gluon Plasma -- implications of recent flow results

    NASA Astrophysics Data System (ADS)

    Petersen, Hannah

    2012-03-01

    Recent measurements of higher order flow coefficients offer a more complete understanding of how hot and dense QCD matter is created in relativistic heavy ion collisions and what its properties are. In addition to providing new constraints on the viscosity of the quark gluon plasma, anisotropic flow is sensitive to the structure of the initial state. As elliptic flow (v2) is generated by the difference in pressure gradients that result from the initial almond shape of the reaction region in non-central collisions, higher order coefficients encode more detailed information about the event-by-event fluctuating initial state profile. In my talk, I will present an overview of theoretical work aimed at understanding the correlations between initial state structures and final state correlations and their origin and discuss the current status of initial state models. I will outline how the new experimental findings at RHIC and LHC can be used towards characterize the dynamical evolution of relativistic heavy ion collisions with special emphasis on the role of event-by-event approaches and sophisticated multi-parameter fits to achieve this goal.

  16. Highlights of recent results from the VERITAS Active Galactic Nuclei Observing Program

    NASA Astrophysics Data System (ADS)

    Abeysekara, Udara; VERITAS Collaboration

    2016-03-01

    Active Galactic Nuclei (AGN) are the dominant class of the Very High Energy (VHE) gamma-ray sources. The VERITAS Observatory dedicates about 430 hr/year of dark time and 200 hr/year of observations under moonlight, on the AGN observing program. VERITAS is located at the Fred Lawrence Whipple Observatory near Tucson, Arizona, and is sensitive to gamma rays with energies between of 85 GeV and 30 TeV. VERITAS became fully operational in 2007, and has since then detected 34 very high energy (VHE) AGN. The majority of the detected galaxies are blazars, in addition to a few radio galaxies. The VHE emission mechanism, and the location of the VHE emission zone of AGN are still poorly understood. Detailed observations of VHE AGN are necessary for understanding these uncertainties. AGN are plausible source candidates for ultra-high-energy cosmic rays and astrophysical neutrinos. VHE gamma-rays from AGN can also be used as probes to place limits on extragalactic background light density. This presentation will report the most recent results from the VERITAS AGN program including newly discovered AGN, and VHE flares of known TeV AGN. Udara Abeysekara for the VERITAS Collaboration.

  17. Recent research results in stereo 3-D pictorial displays at Langley Research Center

    NASA Technical Reports Server (NTRS)

    Parrish, Russell V.; Busquets, Anthony M.; Williams, Steven P.

    1990-01-01

    Recent results from a NASA-Langley program which addressed stereo 3D pictorial displays from a comprehensive standpoint are reviewed. The program dealt with human factors issues and display technology aspects, as well as flight display applications. The human factors findings include addressing a fundamental issue challenging the application of stereoscopic displays in head-down flight applications, with the determination that stereoacuity is unaffected by the short-term use of stereo 3D displays. While stereoacuity has been a traditional measurement of depth perception abilities, it is a measure of relative depth, rather than actual depth (absolute depth). Therefore, depth perception effects based on size and distance judgments and long-term stereo exposure remain issues to be investigated. The applications of stereo 3D to pictorial flight displays within the program have repeatedly demonstrated increases in pilot situational awareness and task performance improvements. Moreover, these improvements have been obtained within the constraints of the limited viewing volume available with conventional stereo displays. A number of stereo 3D pictorial display applications are described, including recovery from flight-path offset, helicopter hover, and emulated helmet-mounted display.

  18. Recent Results From a Si/CdTe Semiconductor Compton Telescope

    SciTech Connect

    Tanaka, T.; Watanabe, S.; Takeda, S.; Oonuki, K.; Mitani, T.; Nakazawa, K.; Takashima, T.; Takahashi, T.; Tajima, H.; Sawamoto, N.; Fukazawa, Y.; Nomachi, M.; /JAXA, Sagamihara /Tokyo U. /SLAC /Hiroshima U. /Osaka U.

    2007-01-23

    We are developing a Compton telescope based on high resolution Si and CdTe detectors for astrophysical observations in sub-MeV/MeV gamma-ray region. Recently, we constructed a prototype Compton telescope which consists of six layers of double-sided Si strip detectors and CdTe pixel detectors to demonstrate the basic performance of this new technology. By irradiating the detector with gamma-rays from radio isotope sources, we have succeeded in Compton reconstruction of images and spectra. The obtained angular resolution is 3.9{sup o} (FWHM) at 511 keV, and the energy resolution is 14 keV (FWHM) at the same energy. In addition to the conventional Compton reconstruction, i.e., drawing cones in the sky, we also demonstrated a full reconstruction by tracking Compton recoil electrons using the signals detected in successive Si layers. By irradiating {sup 137}Cs source, we successfully obtained an image and a spectrum of 662 keV line emission with this method. As a next step, development of larger double-sided Si strip detectors with a size of 4 cm x 4 cm is underway to improve the effective area of the Compton telescope. We are also developing a new low-noise analog ASIC to handle the increasing number of channels. Initial results from these two new technologies are presented in this paper as well.

  19. Overview and Recent Results from the ZaP Flow Z-Pinch

    NASA Astrophysics Data System (ADS)

    Shumlak, U.

    2005-10-01

    The ZaP Flow Z-Pinch Experiment at the University of Washington investigates sheared flow stabilization in an otherwise unstable configuration. An axially flowing Z-pinch is generated with a coaxial accelerator coupled to a pinch assembly chamber. Magnetic probes measure the fluctuation levels of the azimuthal modes m = 1, 2, and 3. The plasma is magnetically confined for an extended quiescent period where the mode activity is significantly reduced. Multichord Doppler shift measurements of impurity lines show a large, sheared flow during the quiescent period and low shear profiles during periods of high mode activity. The plasma has a sheared axial flow that exceeds the theoretical threshold for stability during the quiescent period and is lower than the threshold during periods of high mode activity. The Z-pinch plasmas are globally stable for approximately 2000 growth times. The end of the quiescent period corresponds to a drop in plasma density and a decrease in plasma acceleration. Recent experimental results suggest a means to extend the experiment to quasi steady state operation.

  20. Results from recent hydrogen pellet acceleration studies with a 2-m railgun

    SciTech Connect

    Kim, K.; Zhang, D.J.; King, T.; Haywood, R.; Manns, W.; Venneri, F.

    1989-12-01

    A new 3.2-mm-diameter, two-stage, fuseless, plasma-arc-driven electromagnetic railgun has been designed, constructed, and successfully operated to achieve a record velocity of 2.67 km/s({sup b}) for 3.2 mmD {times} 4 mmL solid hydrogen pellet. The first stage of this hydrogen pellet injector is a combination of a hydrogen pellet generator and a gas fun. The second stage is a 2-m-long railgun which serves as a booster accelerator. The gas fun accelerates a frozen hydrogen pellet to a medium velocity and injects it into the railgun through a perforated coupling piece, which also serves a pressure-relieving mechanism. An electrical breakdown of the propellant gas, which has followed the pellet from the gas fun into the railgun, forms a conducting plasma-arc armature immediately behind the pellet allowing for fuseless operation of the railgun. Study of the pressure profile and the behavior of the plasma-arc armature inside the railgun bore led to elimination of spurious arcing, which prevents operation of the railgun at high voltages (and, therefore, at high currents). A timing circuit that can automatically measure the pellet input velocity and allows for accurate control of arc initiation behind the pellet helps prevent pellet disintegration and mistriggering of the arc initiation circuit. Results from the recent cryogenic operation of the two-stage pellet acceleration system are reported. 11 refs., 2 figs., 1 tab.

  1. A Summary of the NASA Lightning Nitrogen Oxides Model (LNOM) and Recent Results

    NASA Technical Reports Server (NTRS)

    Koshak, William; Peterson, Harld

    2011-01-01

    The NASA Marshall Space Flight Center introduced the Lightning Nitrogen Oxides Model (LNOM) a couple of years ago to combine routine state-of-the-art measurements of lightning with empirical laboratory results of lightning NOx production. The routine measurements included VHF lightning source data [such as from the North Alabama Lightning Mapping Array (LMA)], and ground flash location, peak current, and stroke multiplicity data from the National Lightning Detection Network(TradeMark) (NLDN). Following these initial runs of LNOM, the model was updated to include several non-return stroke lightning NOx production mechanisms, and provided the impact of lightning NOx on an August 2006 run of CMAQ. In this study, we review the evolution of the LNOM in greater detail and discuss the model?s latest upgrades and applications. Whereas previous applications were limited to five summer months of data for North Alabama thunderstorms, the most recent LNOM analyses cover several years. The latest statistics of ground and cloud flash NOx production are provided.

  2. Recent results in the radiation synthesis and modification of polymers for special applications

    SciTech Connect

    Hummel, D.O.

    1980-01-01

    Certain economic considerations relative to production of radicals on a large-industrial scale using different types of radiation indicate that current use of electron accelerators in at least 9 out of 10 radiation-chemical processes reflects use of the most economical method of irradiation. Fluorine-containing monomers and monomer mixtures belong to a class of systems intensively studied for the radiation-initiated synthesis of polymers with good thermal, mechanical, and chemical properties. Results of detailed investigations of the vinylfluoride-vinylidene-fluoride system and subsequent grafting with hydrophylic monomers are presented. Studies of grafting in the system polyethylene-hexafluoroacetone was found to follow a chain mechanism, with the branches consisting of only one monomer unit each. Cationic grafting was observed during irradiation of ..cap alpha..-methylstyrene, vinylbutylether, or isobutene in the presence of polyethylene, polytetrafluoroethylene, or PVC. Grafting of the fiber/monomer systems, cellulose with styrene, vinylfluoride, ethylacrylate or acrylamide; wool with styrene; polypropylene with vinylchloride and vinylidenechloride; poly(ethylene terephthalate) with styrene, acrylic and methacrylic acid, acrylic acid plus acrylonitrile, and N-vinylpyrrolidone have all been investigated recently. Radiation synthesis and modification of membranes and resins and the radiation-grafting of enzymes have also been reported. 75 references. (BLM)

  3. Recent Results from the Lunar Reconnaissance Orbiter Mission and Plans for the Extended Science Phase

    NASA Technical Reports Server (NTRS)

    Vondrak, Richard; Keller, John W.; Chin, Gordon; Petro, Noah; Garvin, James B.; Rice, James W.

    2012-01-01

    The Lunar Reconnaissance Orbiter spacecraft (LRO), launched on June 18, 2009, began with the goal of seeking safe landing sites for future robotic missions or the return of humans to the Moon as part of NASA's Exploration Systems Mission Directorate (ESMD). In addition, LRO's objectives included the search for surface resources and to investigate the Lunar radiation environment. After spacecraft commissioning, the ESMD phase of the mission began on September 15, 2009 and completed on September 15, 2010 when operational responsibility for LRO was transferred to NASA's Science Mission Directorate (SMD). The SMD mission was scheduled for 2 years and completed in September, 2012. The LRO mission has been extended for two years under SMD. The extended mission focuses on a new set of goals related to understanding the geologic history of the Moon, its current state, and what it can tell us about the evolution Of the Solar System. Here we will review the major results from the LRO mission for both exploration and science and discuss plans and objectives going forward including plans for the extended science phase out to 2014. Results from the LRO mission include but are not limited to the development of comprehensive high resolution maps and digital terrain models of the lunar surface; discoveries on the nature of hydrogen distribution, and by extension water, at the lunar poles; measurement of the day and night time temperature of the lunar surface including temperature down below 30 K in permanently shadowed regions (PSRs); direct measurement of Hg, H2, and CO deposits in the PSRs, evidence for recent tectonic activity on the Moon, and high resolution maps of the illumination conditions as the poles. The objectives for the second and extended science phases of the mission under SMD include: 1) understanding the bombardment history of the Moon, 2) interpreting Lunar geologic processes, 3) mapping the global Lunar regolith, 4) identifying volatiles on the Moon, and 5

  4. Linear and circular polarimetry of recent comets: Observational results for eight comets

    NASA Astrophysics Data System (ADS)

    Rosenbush, V.; Ivanova, A.; Kiselev, N.; Afanasiev, V.; Kolesnikov, S.; Shakhovskoy, D.

    2014-07-01

    We present the results of polarimetric observations for a number of recent comets carried out at the 6-m telescope of the Special Astrophysical Observatory (Russia) and the 2.6-m telescope of the Crimean Astrophysical Observatory (Ukraine) during 2011--2013. Comets 103P/Hartley 2, C/2009 P1 (Garradd), C/2011 L4 (PANSTARRS), C/2012 S1 (ISON), C/2013 R1 (Lovejoy), 29P/Schwassmann-Wachmann 1, C/2010 S1 (LINEAR), and C/2011 R1 (McNaught) were observed at different distances from the Sun (0.9--6.3 au) and at different phase angles (6.2--83.5 deg). The results obtained are compared with the phase-angle dependencies of linear polarization typical for the high-polarization and low-polarization comets. The linear polarization of comet S1 (LINEAR) and Schwassmann-Wachmann 1 are the first ever measured at the heliocentric distances larger than 6 au. The maps of circular polarization over the coma and its variations with the distance from the nucleus of comets P1 (Garradd), L4 (PANSTARRS), R1 (McNaught), and Schwassmann-Wachmann 1 are obtained. In all cases, left-handed circular polarization is detected and its value is within the range from -0.04 % up to -0.3 %. Detection of left-handed circular polarization in these comets has confirmed our previous conclusion that circular polarization of comets is predominantly left-handed. We will discuss the possible reasons for the diversity and similarity of linear and circular polarization in comets.

  5. Recent results on modelling the spatial and temporal structure of the Earth's gravity field.

    PubMed

    Moore, P; Zhang, Q; Alothman, A

    2006-04-15

    The Earth's gravity field plays a central role in sea-level change. In the simplest application a precise gravity field will enable oceanographers to capitalize fully on the altimetric datasets collected over the past decade or more by providing a geoid from which absolute sea-level topography can be recovered. However, the concept of a static gravity field is now redundant as we can observe temporal variability in the geoid due to mass redistribution in or on the total Earth system. Temporal variability, associated with interactions between the land, oceans and atmosphere, can be investigated through mass redistributions with, for example, flow of water from the land being balanced by an increase in ocean mass. Furthermore, as ocean transport is an important contributor to the mass redistribution the time varying gravity field can also be used to validate Global Ocean Circulation models. This paper will review the recent history of static and temporal gravity field recovery, from the 1980s to the present day. In particular, mention will be made of the role of satellite laser ranging and other space tracking techniques, satellite altimetry and in situ gravity which formed the basis of gravity field determination until the last few years. With the launch of Challenging Microsatellite Payload and Gravity and Circulation Experiment (GRACE) our knowledge of the spatial distribution of the Earth's gravity field is taking a leap forward. Furthermore, GRACE is now providing insight into temporal variability through 'monthly' gravity field solutions. Prior to this data we relied on satellite tracking, Global Positioning System and geophysical models to give us insight into the temporal variability. We will consider results from these methodologies and compare them to preliminary results from the GRACE mission. PMID:16537153

  6. Paleomagnetism of the Todos Santos Formation in the Maya Block, Chiapas, Mexico: Preliminary Results

    NASA Astrophysics Data System (ADS)

    Godinez-Urban, A.; Molina-Garza, R. S.; Iriondo, A.; Geissman, J. W.

    2008-12-01

    Preliminary results of a paleomagnetic study on jurassic volcanic rocks (U-Pb 188.8 +/- 3.2Ma) locally interbedded with red beds assigned to the Todos Santos Formation, sampled in the Homoclinal Tectonic Province of the Neogene Fold Belt, Chiapas-Mexico, reveal multi component magnetizations acquired during pre- and post- folding of these rocks. The samples responded well to thermal demagnetization, but not so to AF demagnetization, suggesting that a high coercivity mineral phase like hematite is the main remanence carrier. The post-folding B-component direction of Dec=174.3 Inc=-30.6 (k=46; alpha95=13.6; N=4) represents a recent Tertiary? overprint; while the pre-folding C-component direction of Dec=329.9 Inc=7.8 (k=12.5; alpha95=16.3; N=8) is in agreement with a previously reported small data set for the Todos Santos Formation. When compared to the North American reference direction (Jurassic Kayenta Formation) the observed direction indicates a counterclockwise rotation of 35.9 +/- 16.6 degrees, and moderate north to south latitudinal displacement. If a reference pole from NE North America is used, the amount of counterclockwise rotation and latitudinal displacement are both slightly reduced. If the assumption that Jurassic strata in Chiapas reflect displacement of the Maya Block, then these data are consistent with reconstructions of the Maya Block in the Gulf of Mexico region. Other sites sampled in Jurassic strata suggest that in addition to the interpreted regional rotation, local (vertical-axis) rotations may have affected the region in more recent times.

  7. Recent advances with generalized entropy theory of glass-formation in polymers

    NASA Astrophysics Data System (ADS)

    Freed, Karl

    The generalized entropy theory (GET) of glass-formation in polymers is a combination of the lattice cluster theory (LCT) for the configurational entropy density with the Adam-Gibbs (AG) theory for the structural relaxation time. A greatly simplified form of the GET (whose expression for the free energy is roughly double that of Flory-Huggins theory) accurately reproduces the four characteristic temperatures of glass-formation (the onset, crossover, glass transition, and Kauzmann temperatures) of the full GET to within 4K for a series of models of polymers composed of semi-flexible chains having the structure of poly(n-alpha olefins). The theory is now simple enough to be used in courses in polymer physics. Although the successes of the GET provide a strong validation of the final form of the AG theory provided the configurational entropy is used, the physical basis of the AG theory has remained an enigma. Hence, we have developed a new, more general, statistical mechanical derivation of AG theory that explains the previously perplexing observations that the string-like elementary excitations have the mass and temperature dependence of systems undergoing equilibrium self-assembly. This work is supported by the (U.S.) Department of Energy (DOE), Office of Basic Energy Sciences, Division of Materials Sciences and Engineering under Award No. DE- SC0008631.

  8. Semiconductor Nanostructures in High Magnetic Fields:. Recent Results at Hfml Nijmegen

    NASA Astrophysics Data System (ADS)

    Christianen, Peter C. M.

    A short overview of the current experimental facilities at the HFML Nijmegen, including an update on the planned development of a 45 T Hybrid magnet in conjunction with a Free Electron Laser, was presented. That was followed by a brief highlight of recent results on the high field physical properties of semiconductor nanostructures, such as quantum rings1 and dots,2 graphene3,4 and organic nanostructures.5 The majority of the talk was devoted to the investigation of negatively charged excitons (negative trions, two electrons bound to one hole) in semiconductor quantum wells in high magnetic fields. A comprehensive overview of photoluminescence (PL) experiments on GaAs and CdTe quantum wells (QWs) of variable well widths, containing a low density electron gas (2DEG) was presented. Particular interest was given to the magnetic field range where the ground state of negative trions is changing from a singlet (both electrons having opposite spin) to a triplet (parallel electron spins) state. Using polarized magneto-PL (excitation) and reflectivity spectroscopy we have identified (for both GaAs and CdTe QWs) the four typical excitonic peaks, usually denoted as the singlet, dark triplet and bright triplet trion peaks, as well as the neutral exciton peak. All peaks exhibit a pronounced dependence on polarization, 2DEG density and temperature. CdTe QWs exhibit all four peaks at the entire field range used (< 44 T), whereas the dark triplet emission disappears at high fields for GaAs QWs. We have determined the field strength at which the singlet-triplet crossover occurs for all QWs, which allows us to critically compare our experimental results with theoretical predictions. Remarkably, the actual singlet-triplet transition is hidden in GaAs QWs and a narrow (12 nm) CdTe QW. Since the PL emission energy equals the energy difference between the initial (trion) and final (electron) states, the PL lines themselves do not cross at the singlet-triplet crossover as a result of the

  9. Davis Strait and Ungava Fault Zone: First Results From a Recent Geophysical Survey

    NASA Astrophysics Data System (ADS)

    Ehrhardt, A.; Gohl, K.; Neben, S.; Volkmar, D.; Funck, T.; Gerlings, J.

    2008-12-01

    The Davis Strait is a bathymetric high that separates the southern Baffin Bay and the northern Labrador Sea. These basins are the result of Cretaceous and Paleogene rifting and seafloor spreading between the North American plate and Greenland. Being one of the main tectonic features of the Davis Strait, the Ungava Fault Zone is associated with transform motion related to a northward movement of Greenland relative to North America during rifting and seafloor spreading in Baffin Bay and Labrador Sea. The plate tectonic reconstruction of the Davis Strait contributes significantly to the understanding of the geodynamic history of the North-American - Greenland plates, not only the Davis Strait area but also the area of Lancaster Sound and Nares Strait, where it could shed light into the so-called Nares Strait Conflict. It is still under debate whether the spreading between Greenland and Baffin Island was compensated by sinistral transform motion along the proposed Wegener-Fault. Thus Nares Strait (trace of the Wegener Fault) and Lancaster Sound (failed arm rift) are relicts of this scenario. The lack of evidence for transform motion between Greenland and Ellesmere Island contradicts this model and provokes the conflict. As major compression along the Eurekan Fold Belt overprinted the proposed transform motion along the Wegener Fault, the Ungava Fault Zone in the Davis Strait could give the missing information for the plate tectonic reconstruction. The onshore-offshore geology and structural setting of Baffin Island is analysed by recent publications that show an essentially non-volcanic continental margin at Baffin Island that is interrupted by a volcanic-style margin around Cape Dyer. Intensive magmatic activity during the initial opening phase is indicated by widespread seaward-dipping-reflector sequences (SDRS) north of Cape Dyer. On the other hand, the structural setting of the Greenland margin side is unclear. The identification of the corresponding conjugate

  10. Dentin bonding performance using Weibull statistics and evaluation of acid-base resistant zone formation of recently introduced adhesives.

    PubMed

    Guan, Rui; Takagaki, Tomohiro; Matsui, Naoko; Sato, Takaaki; Burrow, Michael F; Palamara, Joseph; Nikaido, Toru; Tagami, Junji

    2016-07-30

    Dentin bonding durability of recently introduced dental adhesives: Clearfil SE Bond 2 (SE2), Optibond XTR (XTR), and Scotchbond Universal (SBU) was investigated using Weibull analysis as well as analysis of the micromorphological features of the acid-base resistant zone (ABRZ) created for the adhesives. The bonding procedures of SBU were divided into three subgroups: self-etch (SBS), phosphoric acid (PA) etching on moist (SBM) or dry dentin (SBD). All groups were thermocycled for 0, 5,000 and 10,000 cycles followed by microtensile bond strength testing. Acid-base challenge was undertaken before SEM and TEM observations of the adhesive interface. The etch-and-rinse method with SBU (SBM and SBD) created inferior interfaces on the dentin surface which resulted in reduced bond durability. ABRZ formation was detected with the self-etch adhesive systems; SE2, XTR and SBS. In the PA etching protocols of SBM and SBD, a thick hybrid layer but no ABRZ was detected, which might affect dentin bond durability. PMID:27335136

  11. Studies on the tempo of bubble formation in recently cavitated vessels: a model to predict the pressure of air bubbles.

    PubMed

    Wang, Yujie; Pan, Ruihua; Tyree, Melvin T

    2015-06-01

    A cavitation event in a vessel replaces water with a mixture of water vapor and air. A quantitative theory is presented to argue that the tempo of filling of vessels with air has two phases: a fast process that extracts air from stem tissue adjacent to the cavitated vessels (less than 10 s) and a slow phase that extracts air from the atmosphere outside the stem (more than 10 h). A model was designed to estimate how water tension (T) near recently cavitated vessels causes bubbles in embolized vessels to expand or contract as T increases or decreases, respectively. The model also predicts that the hydraulic conductivity of a stem will increase as bubbles collapse. The pressure of air bubbles trapped in vessels of a stem can be predicted from the model based on fitting curves of hydraulic conductivity versus T. The model was validated using data from six stem segments each of Acer mono and the clonal hybrid Populus 84 K (Populus alba × Populus glandulosa). The model was fitted to results with root mean square error less than 3%. The model provided new insight into the study of embolism formation in stem tissue and helped quantify the bubble pressure immediately after the fast process referred to above. PMID:25907963

  12. Immunotherapy in gastrointestinal cancer: Recent results, current studies and future perspectives.

    PubMed

    Moehler, Markus; Delic, Maike; Goepfert, Katrin; Aust, Daniela; Grabsch, Heike I; Halama, Niels; Heinrich, Bernd; Julie, Catherine; Lordick, Florian; Lutz, Manfred P; Mauer, Murielle; Alsina Maqueda, Maria; Schild, Hansjoerg; Schimanski, Carl C; Wagner, Anna-Dorothea; Roth, Arnaud; Ducreux, Michel

    2016-05-01

    The new therapeutic approach of using immune checkpoint inhibitors as anticancer agents is a landmark innovation. Early studies suggest that immune checkpoint inhibition might also be effective in patients with gastrointestinal cancer. To improve the efficacy of immunotherapy, different strategies are currently under evaluation. This review summarises the discussion during the European Organisation for Research and Treatment of Cancer Gastrointestinal Tract Cancer Translational Research Meeting in Mainz in November 2014 and provides an update on the most recent results of immune therapy in gastrointestinal cancers. Knowledge of potential relationships between tumour cells and their microenvironment including the immune system will be essential in gastrointestinal malignancies. In this context, the density of T cell infiltration within colorectal cancer metastases has been associated with response to chemotherapy, and a high expression of programmed cell death ligand 1 (PD-L1) in advanced gastric cancer has been related with poor prognosis. Effective targets might include neo-antigens encoded from genes carrying tumour-specific somatic mutations. Tailored immunotherapy based on such mutations could enable the effective targeting of an individual patient's tumour with vaccines produced on demand. Other strategies considering checkpoint inhibitors have shown efficacy by targeting cytotoxic T-lymphocyte-associated protein 4 and PD-1 or PD-L1. DNA mismatch repair-deficient tumours appear to be potentially the best candidates for these therapies. Finally, the combination of oncolytic viruses with immunotherapy might boost antitumour activity as well. Further evaluation of these promising immunological therapeutic approaches will require large prospective clinical studies. PMID:27039171

  13. Recent Progress in Understanding Natural-Hazards-Generated TEC Perturbations: Measurements and Modeling Results

    NASA Astrophysics Data System (ADS)

    Komjathy, A.; Yang, Y. M.; Meng, X.; Verkhoglyadova, O. P.; Mannucci, A. J.; Langley, R. B.

    2015-12-01

    Natural hazards, including earthquakes, volcanic eruptions, and tsunamis, have been significant threats to humans throughout recorded history. The Global Positioning System satellites have become primary sensors to measure signatures associated with such natural hazards. These signatures typically include GPS-derived seismic deformation measurements, co-seismic vertical displacements, and real-time GPS-derived ocean buoy positioning estimates. Another way to use GPS observables is to compute the ionospheric total electron content (TEC) to measure and monitor post-seismic ionospheric disturbances caused by earthquakes, volcanic eruptions, and tsunamis. Research at the University of New Brunswick (UNB) laid the foundations to model the three-dimensional ionosphere at NASA's Jet Propulsion Laboratory by ingesting ground- and space-based GPS measurements into the state-of-the-art Global Assimilative Ionosphere Modeling (GAIM) software. As an outcome of the UNB and NASA research, new and innovative GPS applications have been invented including the use of ionospheric measurements to detect tiny fluctuations in the GPS signals between the spacecraft and GPS receivers caused by natural hazards occurring on or near the Earth's surface.We will show examples for early detection of natural hazards generated ionospheric signatures using ground-based and space-borne GPS receivers. We will also discuss recent results from the U.S. Real-time Earthquake Analysis for Disaster Mitigation Network (READI) exercises utilizing our algorithms. By studying the propagation properties of ionospheric perturbations generated by natural hazards along with applying sophisticated first-principles physics-based modeling, we are on track to develop new technologies that can potentially save human lives and minimize property damage. It is also expected that ionospheric monitoring of TEC perturbations might become an integral part of existing natural hazards warning systems.

  14. Terrestrial Gamma-ray Flashes: Twentieth Anniversary and Recent Fermi GBM Results

    NASA Astrophysics Data System (ADS)

    Briggs, Michael

    2014-05-01

    The TGF field has advanced remarkably in the twenty years since the publication of the paper "Discovery of intense gamma-ray flashes of atmospheric origin" by G. J. Fishman et al. I will review the BATSE observations and how the following space-based observations of RHESSI, AGILE and Fermi advanced the field. BATSE discovered TGFs, including multi-pulse ones, and established the correlation of TGFs with thunderstorms. Retrospective analysis of BATSE data identified electron-beam events. RHESSI observations extended the spectra to higher energies and indicated a lower source altitude. The shape of the spectrum measured with AGILE challenges the predictions of the large-scale relativistic runaway electron avalanche (RREA) model. Much progress has been made with the combination of space-based gamma-ray and ground-based radio observations. Finally, I will review Fermi GBM results. The high effective area of GBM enables improved measurements of pulse profiles. Some multi-pulse events have separations as short as 1/4 ms, so that the pulses partially overlap. Short events are typically asymmetric, consistent with a Compton tail, while longer events are commonly symmetric, consistent with the Compton tail being hidden within the longer pulse. GBM also found electron-beam events to include positrons. Recent ground-based search of individual photon data uncovered fainter and shorter TGFs. Radio observations of GBM TGFs and a strong TGF duration / radio-detection anti-correlation show that the radio detections that are very close in time (< tens of microseconds) to a TGF are due to the TGF itself rather than from lightning. Analysis of the first year of continuous individual photon data found more than 800 TGFs.

  15. Developing Improved Water Velocity and Flux Estimation from AUVs - Results From Recent ASTEP Field Programs

    NASA Astrophysics Data System (ADS)

    Kinsey, J. C.; Yoerger, D. R.; Camilli, R.; German, C. R.

    2010-12-01

    Water velocity measurements are crucial to quantifying fluxes and better understanding water as a fundamental transport mechanism for marine chemical and biological processes. The importance of flux to understanding these processes makes it a crucial component of astrobiological exploration to moons possessing large bodies of water, such as Europa. Present technology allows us to obtain submerged water velocity measurements from stationary platforms; rarer are measurements from submerged vehicles which possess the ability to autonomously survey tens of kilometers over extended periods. Improving this capability would also allow us to obtain co-registered water velocity and other sensor data (e.g., mass spectrometers, temperature, oxygen, etc) and significantly enhance our ability to estimate fluxes. We report results from 4 recent expeditions in which we measured water velocities from autonomous underwater vehicles (AUVs) to help quantify flux in three different oceanographic contexts: hydrothermal vent plumes; an oil spill cruise responding to the 2010 Deepwater Horizon blowout; and two expeditions investigating naturally occurring methane seeps. On all of these cruises, we directly measured the water velocities with an acoustic Doppler current profiler (ADCP) mounted on the AUV. Vehicle motion was corrected for using bottom-lock Doppler tracks when available and, in the absence of bottom-lock, estimates of vehicle velocity based on dynamic models. In addition, on the methane seep cruises, we explored the potential of using acoustic mapping sonars, such as multi-beam and sub-bottom profiling systems, to localize plumes and indirectly quantify flux. Data obtained on these expeditions enhanced our scientific investigations and provides data for future development of algorithms for autonomously processing, identifying, and classifying water velocity and flux measurements. Such technology will be crucial in future astrobiology missions where highly constrained

  16. Benchmarking MELCOR 1.8.2 for ITER Against Recent EVITA Results

    SciTech Connect

    Merrill, Brad J

    2007-11-01

    A version of MELCOR 1.8.2 modified for use in ITER Preliminary Safety Report analyses was validated against recent data from the EVITA facility located in Cadarache, France. EVITA Test Series 7 was used for this study to verify MELCOR’s ability to predict the pressures, temperatures, cryoplate ice mass, and vaccum vessel (VV) condensate mass for test conditions in EVITA that include injections of steam, nitrogen, and water in to the EVITA VV after the walls had been heated to 165 ºC and the cryoplate had been cooled to -193 ºC. In general, the ability of MELCOR to predict the VV pressure and wall temperatures for the steam only and water only injection tests was very good. Predicted ice layer masses where larger than reported for the EVITA cryoplate, in particular for the steam only injection tests (~40% too high), and the predicted condensate masses were less that measured in EVITA. Both of these descrpancies can be explained by ice porosity. The modified MELCOR 1.8.2 over predicts the EVITA VV pressure for the co-injection tests (e.g., steam plus nitrogen, or water plus nitrogen injections) by almost a factor of two. Based on parametric runs that where made by increasing the predicted cryoplate condensation rate, it is believed that this pressure over prediction is a result of an under predicted cryoplate condensation rate. The particulars of this study are documented in this report as well as conclusions about the impact this study has regarding the use of this verions of MELCOR for consequence analyses for ITER safety reports.

  17. Review of the ACE-FTS measurements and recent results for the troposphere and UTLS

    NASA Astrophysics Data System (ADS)

    Bernath, Peter

    The ACE satellite mission goals are: (1) to measure and to understand the chemical and dynamical processes that control the distribution of ozone in the upper troposphere and stratosphere, with a particular emphasis on the Arctic region; (2) to explore the relationship between atmospheric chemistry and climate change; (3) to study the effects of biomass burning in the free troposphere; and (4) to measure aerosol number density, size distribution and composition in order to reduce the uncertainties in their effects on the global energy balance. ACE is making a comprehensive set of simultaneous measurements of trace gases, thin clouds, aerosols, and temperature by solar occultation from a satellite in low earth orbit. A high inclination (74 degrees) low earth orbit (650 km) gives ACE coverage of tropical, mid-latitudes and polar regions. A high-resolution (0.02 cm-1 ) infrared Fourier Transform Spectrometer (FTS) operating from 2 to 13 microns (750-4400 cm-1 ) is measuring the vertical distribution of trace gases, and the meteorological variables of temperature and pressure. Aerosols and clouds are being monitored using the extinction of solar radiation at 0.525 and 1.02 microns as measured by two filtered imagers as well as by their infrared spectra. A dual spectrograph called MAESTRO was added to the mission to extend the wavelength coverage to the 280-1000 nm spectral region. The principal investigator for MAESTRO is T. McElroy of the Meteorological Service of Canada. The FTS and imagers have been built by ABB-Bomem in Quebec City, while the satellite bus has been made by Bristol Aerospace in Winnipeg. ACE was selected in the Canadian Space Agency's SCISAT-1 program, and was successfully launched by NASA on August 12, 2003 for a nominal 2-year mission. The first results of ACE have been presented in a special issue of Geophysics Research Letters in 2005 and recently a special issue on ACE validation has been prepared for Atmospheric Chemistry and Physics by K

  18. Recent Results of Ambient Ozone Monitoring in Southern Sierra Nevada and White Mountains, California

    NASA Astrophysics Data System (ADS)

    Burley, J. D.; Bytnerowicz, A.; Cisneros, R.; Schweizer, D.

    2014-12-01

    numerous violations of the California health standard. These results will be discussed from a perspective of other monitoring campaigns conducted by our team in the Sierra Nevada, and they will be compared to concurrent results from nearby low elevation sites. We will also discuss effects of the recent Sierra Nevada wildland fires on ozone levels and distribution.

  19. Recent Observational Results of Seafloor Crustal Deformation Along the Suruga-Nankai Trough, Japan

    NASA Astrophysics Data System (ADS)

    Tadokoro, K.; Sugimoto, S.; Watanabe, T.; Muto, D.; Kimoto, A.; Okuda, T.; Ikuta, R.; Sayanagi, K.; Kuno, M.

    2008-12-01

    The Suruga-Nankai Trough is one of the active plate boundaries in the world. The Philippine Sea plate is subducting beneath the Amurian (Eurasian) plate along the tough, and major subduction earthquakes, Nankai and Tonankai earthquakes, have repeatedly occurred with intervals of about 100-150 years. The 1944 Tonankai and 1946 Nankai earthquakes are the most recent significant earthquakes along the trough. Therefore, the 50-years probabilities of the next major earthquakes are estimated at 80-90% by Headquarters for Earthquake Research Promotion, Japanese Government. It is, therefore, necessary to start monitoring crustal deformation above the source regions of the major earthquakes where in the ocean area. We developed a new system composed of the precise acoustic ranging and kinematic GPS positioning techniques for monitoring of seafloor crustal deformation [Tadokoro et al., 2006, GRL; Ikuta et al., 2008, JGR]. We had installed seven seafloor benchmarks for acoustic ranging at the Suruga-Nankai Trough region between 2002 and 2004. The water depths at the benchmarks are about 800 to 2000 m. We installed a new seafloor benchmark at the eastern margin of the Kumano Basin on June 23, 2008. Three seafloor benchmarks had been aligned perpendicular to the trough axis. In contrast, the new benchmark was installed eastward relative to the pre-installed benchmarks, and we can monitor lateral variations in crustal deformation at the region. We started the repeated measurements at four benchmarkes (two at the Kumano Basin named KMN and KMS, and the other two at the Suruga Bay named SNW and SNE) in 2005. The number of times we have measured are seven, eleven, three and nine times at KMN, KMS, SNW and SNE, respectively. Recent results of the repeated measurements show the following horizontal velocities with relative to the Amurian Plate: 6.4 cm/yr, N86W at KMN; 5.3 cm/yr, N71W at KMS; 3.3 cm/yr, N57W at SNE. The errors of the horizontal velocities are 1-3 cm/yr. Unfortunately

  20. OVERVIEW OF RECENT EXPERIMENTAL RESULTS FROM THE DIII-D ADVANCED TOKAMAK PROGRAM

    SciTech Connect

    BURRELL,KH

    2002-11-01

    OAK A271 OVERVIEW OF RECENT EXPERIMENTAL RESULTS FROM THE DIII-D ADVANCED TOKAMAK PROGRAM. The DIII-D research program is developing the scientific basis for advanced tokamak (AT) modes of operation in order to enhance the attractiveness of the tokamak as an energy producing system. Since the last International Atomic Energy Agency (IAEA) meeting, the authors have made significant progress in developing the building blocks needed for AT operation: (1) the authors have doubled the magnetohydrodynamic (MHD) stable tokamak operating space through rotational stabilization of the resistive wall mode; (2) using this rotational stabilization, they have achieved {beta}{sub N}H{sub 89} {le} 10 for 4 {tau}{sub E} limited by the neoclassical tearing mode; (3) using real-time feedback of the electron cyclotron current drive (ECCD) location, they have stabilized the (m,n) = (3,2) neoclassical tearing mode and then increased {beta}{sub T} by 60%; (4) they have produced ECCD stabilization of the (2,1) neoclassical tearing mode in initial experiments; (5) they have made the first integrated AT demonstration discharges with current profile control using ECCD; (6) ECCD and electron cyclotron heating (ECH) have been used to control the pressure profile in high performance plasmas; and (7) they have demonstrated stationary tokamak operation for 6.5 s (36 {tau}{sub E}) at the same fusion gain parameter of {beta}{sub N}H{sub 89}/q{sub 95}{sup 2} {approx} 0.4 as ITER but at much higher q{sub 95} = 4.2. They have developed general improvements applicable to conventional and advanced tokamak operating modes: (1) they have an existence proof of a mode of tokamak operation, quiescent H-mode, which has no pulsed, ELM heat load to the divertor and which can run for long periods of time (3.8 s or 25 {tau}{sub E}) with constant density and constant radiation power; (2) they have demonstrated real-time disruption detection and mitigation for vertical disruption events using high pressure gas jet

  1. Recent results from the first polar direct drive plastic capsule implosions on NIF

    NASA Astrophysics Data System (ADS)

    Schmitt, Mark J.

    2012-10-01

    Polar direct drive (PDD) offers a simplified platform for conducting strongly driven implosions on NIF to investigate mix, hydro-burn and ignition-relevant physics. Its successful use necessitates a firm understanding and predictive capability of its implosion characteristics including hydro performance, symmetry and yield. To assess this capability, the first two PDD implosions of deuterium filled CH capsules were recently conducted at NIF. The P2 Legendre mode symmetry seen in these implosions agreed with pre-shot predictions even though the 700kJ drive energy produced intensities that far exceeded thresholds for both Raman and Brillouin stimulated scattering. These shots were also the first to employ image backlighting driven by two laser quads. Preliminary results indicate that the yield from the uncoated 2.25 mm diameter, 42 μm thick, CH shells was reduced by about a factor of two owing to as-shot laser drive asymmetries. Similarly, a small (sim50 μm) centroid offset between the upper and lower shell hemispheres seen in the first shot appears to be indicative of the laser quad energies. Overall, the implosion trajectories agreed with pre-shot predictions of bangtime. The second shot incorporated an 80 ?m wide,10 ?m deep depression encircling the equator of the capsule. This engineered feature was imposed to test our capability to predict the effect of high-mode features on yield and mix. A predicted yield reduction factor of 3 was not observed.[4pt] In collaboration with P. A. Bradley, J. A. Cobble, P. Hakel, S. C. Hsu, N. S. Krasheninnikova, G. A. Kyrala, G. R. Magelssen, T. J. Murphy, K. A. Obrey, R. C. Shah, I. L. Tregillis and F. J. Wysocki of Los Alamos National Laboratory; M. Marinak, R. Wallace, T. Parham, M. Cowan, S. Glenn, R. Benedetti and the NIF Operations Team of Lawrence Livermore National Laboratory; R. S. Craxton and P. W. McKenty of the Univ. Rochester; P. Fitzsimmons and A. Nikroo of General Atomics; H. Rinderknecht, M. Rosenberg, and M. G

  2. The massive star population in M101. II. Spatial variations in the recent star formation history

    SciTech Connect

    Grammer, Skyler; Humphreys, Roberta M. E-mail: roberta@umn.edu

    2014-09-01

    We investigate star formation history (SFH) as a function of radius in M101 using archival Hubble Space Telescope Advanced Camera for Surveys photometry. We derive the SFH from the resolved stellar populations in five 2' wide annuli. Binning the SFH into time frames corresponding to stellar populations traced by Hα, far-ultraviolet, and near-ultraviolet emission, we find that the fraction of stellar populations young enough to contribute in Hα is 15%-35% in the inner regions, compared to less than 5% in the outer regions. This provides a sufficient explanation for the lack of Hα emission at large radii. We also model the blue to red supergiant ratio in our five annuli, examine the effects that a metallicity gradient and variable SFH have on the predicted ratios, and compare to the observed values. We find that the radial behavior of our modeled blue to red supergiant ratios is highly sensitive to both spatial variations in the SFH and metallicity. Incorporating the derived SFH into modeled ratios, we find that we are able to reproduce the observed values at large radii (low metallicity), but at small radii (high metallicity) the modeled and observed ratios are discrepant.

  3. Recent Ocean Literacy Research in United States Public Schools: Results and Implications

    ERIC Educational Resources Information Center

    Plankis, Brian J.; Marrero, Meghan E.

    2010-01-01

    Recent research conducted on adults in the United States indicates low ocean literacy (Ocean Project, 2009b, 1999), but there is a dearth of peer-reviewed research on K-12 students' ocean literacy. This paper presents two research studies that examined the ocean and environmental literacy of 464 K-12 students in five states. Like the majority of…

  4. Hydrogen Station Cost Estimates: Comparing Hydrogen Station Cost Calculator Results with other Recent Estimates

    SciTech Connect

    Melaina, M.; Penev, M.

    2013-09-01

    This report compares hydrogen station cost estimates conveyed by expert stakeholders through the Hydrogen Station Cost Calculation (HSCC) to a select number of other cost estimates. These other cost estimates include projections based upon cost models and costs associated with recently funded stations.

  5. Recent results on high rate growth of KDP-type crystals for power laser systems

    NASA Astrophysics Data System (ADS)

    Bespalov, Viktor I.; Bredikhin, Vladimir I.; Ershov, V. P.; Zilberberg, Victor V.

    1996-02-01

    The two types of high rate growth technology of KDP-type crystal are observed. This technology will be used for effective producing of crystal elements for high-energy laser systems. The recent achievements (in particular the obtaining of 380 by 230 by 50 mm Z-plate from KDP crystal) are reported.

  6. Early-type galaxies at intermediate redshift observed with Hubble space telescope WFC3: perspectives on recent star formation

    SciTech Connect

    Rutkowski, Michael J.; Jeong, Hyunjin; Yi, Sukyoung K.; Cohen, Seth H.; Windhorst, Rogier A.; Kaviraj, Sugata; Ryan, Russell E. Jr.; Koekemoer, Anton; Hathi, Nimish P.; Dopita, Michael A.

    2014-12-01

    We present an analysis of the stellar populations of 102 visually selected early-type galaxies (ETGs) with spectroscopic redshifts (0.35 ≲ z ≲ 1.5) from observations in the Early Release Science program with the Wide Field Camera 3 (WFC3) on the Hubble Space Telescope (HST). We fit one- and two-component synthetic stellar models to the ETGs UV-optical-near-IR spectral energy distributions and find that a large fraction (∼40%) are likely to have experienced a minor (f{sub YC} ≲ 10% of stellar mass) burst of recent (t{sub YC} ≲ 1 Gyr) star formation. The measured age and mass fraction of the young stellar populations do not strongly trend with measurements of galaxy morphology. We note that massive (M > 10{sup 10.5} M {sub ☉}) recent star-forming ETGs appear to have larger sizes. Furthermore, high-mass, quiescent ETGs identified with likely companions populate a distinct region in the size-mass parameter space, in comparison with the distribution of massive ETGs with evidence of recent star formation (RSF). We conclude that both mechanisms of quenching star formation in disk-like ETGs and (gas-rich, minor) merger activity contribute to the formation of young stars and the size-mass evolution of intermediate redshift ETGs. The number of ETGs for which we have both HST WFC3 panchromatic (especially UV) imaging and spectroscopically confirmed redshifts is relatively small, therefore, a conclusion about the relative roles of both of these mechanisms remains an open question.

  7. Land-atmosphere interactions and climate change: Recent results and new perspectives (Invited)

    NASA Astrophysics Data System (ADS)

    Seneviratne, S. I.; Davin, E. L.; Greve, P.; Gudmundsson, L.; Guillod, B.; Hirschi, M.; Mittelbach, H.; Mueller, B.; Mystakidis, S.; Orlowsky, B.; Orth, R.; Wilhelm, M.

    2013-12-01

    Land-atmosphere interactions play a key role in the climate system. In particular, soil moisture-climate interactions have been shown to affect the occurrence of extreme events in both present and future (e.g. Seneviratne et al. 2006, 2010). This presentation will provide an overview on recent results highlighting the impact of soil moisture-temperature feedbacks on hot extremes (e.g. Hirschi et al. 2010, Mueller and Seneviratne 2012, Seneviratne et al. 2013). Furthermore, it will also address new findings in the area of soil moisture-precipitation and land albedo-climate feedbacks (Guillod et al. 2013, Davin et al. 2013). The representation of these feedbacks in current climate models will be discussed, based on analyses of CMIP5 simulations. We will especially highlight systematic biases found in some key relationships underlying these feedbacks (e.g. Mueller and Seneviratne 2013). Finally, we will address the question of terrestrial climate engineering through targeted modifications of the land surface. References: Davin, E.L., S.I. Seneviratne, P. Ciais, A. Olioso, and T. Wang, 2013: Preferential cooling of hot extremes from cropland albedo management. Submitted. Guillod, B., et al., 2013: Land surface controls on afternoon precipitation diagnosed from observational data: Uncertainties, confounding factors and the possible role of interception storage. Manuscript in preparation. Hirschi, M., S.I. Seneviratne, V. Alexandrov, F. Boberg, C. Boroneant, O.B. Christensen, H. Formayer, B. Orlowsky, and P. Stepanek, 2011: Observational evidence for soil-moisture impact on hot extremes in southeastern Europe. Nature Geoscience, 4, 17-21, doi:10.1038/ngeo1032. Mueller, B., and S.I. Seneviratne, 2012: Hot days induced by precipitation deficits at the global scale. Proceedings of the National Academy of Sciences, 109 (31), 12398-12403, doi: 10.1073/pnas.1204330109. Mueller, B., and S.I. Seneviratne 2013: Systematic land climate and evapotranspiration biases in CMIP5

  8. High-latitude Recent Surface Mantle On Mars: New Results From Mola and Moc

    NASA Astrophysics Data System (ADS)

    Kreslavsky, M. A.; Head, J. W.

    The latitudinal trend of MGS-MOLA-derived kilometer-scale surface roughness on Mars has been interpreted as the presence of a geologically young several-meter-thick mantle at high-latitudes, which has a specific ten-meter-scale "basketball" surface pattern in MGS MOC images (Kreslavsky and Head, J. Geophys. Res., 105, 26695- 26711, 2000). A specific dissected pattern seen in MOC images in narrow mid-latitude zones has been interpreted as evidence for ongoing desiccation of ground ice (Mus- tard et al., Nature, 412, 411-414, 2001). This pattern can be interpreted as peripheral degrading part of the high-latitude mantle. We present new maps of MOLA-derived statistical characteristics of kilometer-scale topographic pattern showing the global distribution of the mantle and its distal dissected parts in the northern lowlands. We use a selection of high-quality MOC images of the northern lowlands to characterize the variability of the small-scale morphology of the mantle deposits and their strati- graphic relationship with other young features around the polar cap: dunes of dif- ferent types, dune fields, layered terrains, Chasma Boreale-related deposits, etc. We discuss possible ice content in the mantle, possible mechanisms of mantle formation and degradation, and possible time scales of these processes. Formation and degrada- tion of the mantle could follow obliquity oscillations at 0.05 Myr time scale. It is also possible that the mantle is more inert and its formation and degradation is controlled by 2-5-Myr-scale chaotic obliquity wander.

  9. Recent developments in the way forward for alternative methods: Formation of national consensus platforms in Europe

    SciTech Connect

    Rogiers, Vera . E-mail: vrogiers@fafy.vub.ac.be

    2005-09-01

    Ecopa, the European Consensus Platform on 3R-Alternatives, is an international not-for-profit organization that wants to stimulate the development of 3R-alternatives, increase awareness among the public, scientists and regulatory bodies, and help their implementation into the different national legislations. This is done by networking and bringing together National Consensus Platforms on 3R-alternatives. Consensus means that all parties concerned are represented, namely, animal welfare, industry, academia, and governmental institutions. Actually, 14 Member State Platforms exist. Fully complying with the criteria, set by ecopa, are the platforms of Austria, Belgium, the Czech Republic, Finland, Germany, Italy, the Netherlands, Spain, Sweden, Switzerland, and the United Kingdom. Under development are the platforms of Denmark, Norway, and Poland. To reach its goals, ecopa uses conventional scientific tools such as workshops and meetings but it also makes scientific-political statements. A recent realization in particular is the involvement of ecopa in several European projects of the Sixth Framework Programme, either as coordinator, research partner, or board member.

  10. Recent developments in the way forward for alternative methods: formation of national consensus platforms in Europe.

    PubMed

    Rogiers, Vera

    2005-09-01

    Ecopa, the European Consensus Platform on 3R-Alternatives, is an international not-for-profit organization that wants to stimulate the development of 3R-alternatives, increase awareness among the public, scientists and regulatory bodies, and help their implementation into the different national legislations. This is done by networking and bringing together National Consensus Platforms on 3R-alternatives. Consensus means that all parties concerned are represented, namely, animal welfare, industry, academia, and governmental institutions. Actually, 14 Member State Platforms exist. Fully complying with the criteria, set by ecopa, are the platforms of Austria, Belgium, the Czech Republic, Finland, Germany, Italy, the Netherlands, Spain, Sweden, Switzerland, and the United Kingdom. Under development are the platforms of Denmark, Norway, and Poland. To reach its goals, ecopa uses conventional scientific tools such as workshops and meetings but it also makes scientific-political statements. A recent realization in particular is the involvement of ecopa in several European projects of the Sixth Framework Programme, either as coordinator, research partner, or board member. PMID:16055162

  11. Sensitivity analysis and multidisciplinary optimization for aircraft design - Recent advances and results

    NASA Technical Reports Server (NTRS)

    Sobieszczanski-Sobieski, Jaroslaw

    1988-01-01

    Optimization by decomposition, complex system sensitivity analysis, and a rapid growth of disciplinary sensitivity analysis are some of the recent developments that hold promise of a quantum jump in the support engineers receive from computers in the quantitative aspects of design. Review of the salient points of these techniques is given and illustrated by examples from aircraft design as a process that combines the best of human intellect and computer power to manipulate data.

  12. Sensitivity analysis and multidisciplinary optimization for aircraft design: Recent advances and results

    NASA Technical Reports Server (NTRS)

    Sobieszczanski-Sobieski, Jaroslaw

    1988-01-01

    Optimization by decomposition, complex system sensitivity analysis, and a rapid growth of disciplinary sensitivity analysis are some of the recent developments that hold promise of a quantum jump in the support engineers receive from computers in the quantitative aspects of design. Review of the salient points of these techniques is given and illustrated by examples from aircraft design as a process that combines the best of human intellect and computer power to manipulate data.

  13. Biomarker validation of reports of recent sexual activity: results of a randomized controlled study in Zimbabwe.

    PubMed

    Minnis, Alexandra M; Steiner, Markus J; Gallo, Maria F; Warner, Lee; Hobbs, Marcia M; van der Straten, Ariane; Chipato, Tsungai; Macaluso, Maurizio; Padian, Nancy S

    2009-10-01

    Challenges in the accurate measurement of sexual behavior in human immunodeficiency virus (HIV) prevention research are well documented and have prompted discussion about whether valid assessments are possible. Audio computer-assisted self-interviewing (ACASI) may increase the validity of self-reported behavioral data. In 2006-2007, Zimbabwean women participated in a randomized, cross-sectional study that compared self-reports of recent vaginal sex and condom use collected through ACASI or face-to-face interviewing (FTFI) with a validated objective biomarker of recent semen exposure (prostate-specific antigen (PSA) levels). Of 910 study participants, 196 (21.5%) tested positive for PSA, an indication of semen exposure during the previous 2 days. Of these 196 participants, 23 (11.7%) reported no sex in the previous 2 days, with no difference in reported sexual activity between interview modes (12.5% ACASI vs. 10.9% FTFI; Fisher's exact test: P = 0.72). In addition, 71 PSA-positive participants (36.2%) reported condom-protected vaginal sex only; their reports also indicated no difference between interview modes (33.7% ACASI vs. 39.1% FTFI; P = 0.26). Only 52% of PSA-positive participants reported unprotected sex during the previous 2 days. Self-report was a poor predictor of recent sexual activity and condom use in this study, regardless of interview mode, providing evidence that such data should be interpreted cautiously. PMID:19741042

  14. Biomarker Validation of Reports of Recent Sexual Activity: Results of a Randomized Controlled Study in Zimbabwe

    PubMed Central

    Steiner, Markus J.; Gallo, Maria F.; Warner, Lee; Hobbs, Marcia M.; van der Straten, Ariane; Chipato, Tsungai; Macaluso, Maurizio; Padian, Nancy S.

    2009-01-01

    Challenges in the accurate measurement of sexual behavior in human immunodeficiency virus (HIV) prevention research are well documented and have prompted discussion about whether valid assessments are possible. Audio computer-assisted self-interviewing (ACASI) may increase the validity of self-reported behavioral data. In 2006–2007, Zimbabwean women participated in a randomized, cross-sectional study that compared self-reports of recent vaginal sex and condom use collected through ACASI or face-to-face interviewing (FTFI) with a validated objective biomarker of recent semen exposure (prostate-specific antigen (PSA) levels). Of 910 study participants, 196 (21.5%) tested positive for PSA, an indication of semen exposure during the previous 2 days. Of these 196 participants, 23 (11.7%) reported no sex in the previous 2 days, with no difference in reported sexual activity between interview modes (12.5% ACASI vs. 10.9% FTFI; Fisher's exact test: P = 0.72). In addition, 71 PSA-positive participants (36.2%) reported condom-protected vaginal sex only; their reports also indicated no difference between interview modes (33.7% ACASI vs. 39.1% FTFI; P = 0.26). Only 52% of PSA-positive participants reported unprotected sex during the previous 2 days. Self-report was a poor predictor of recent sexual activity and condom use in this study, regardless of interview mode, providing evidence that such data should be interpreted cautiously. PMID:19741042

  15. Recent results from the Microscopic Imagers on the Mars Exploration Rovers

    NASA Astrophysics Data System (ADS)

    Herkenhoff, K. E.; Ashley, J. W.; Cabrol, N. A.

    2009-12-01

    objects under the rover, the out-of-focus data still show what appears to be a rock touching the belly. Opportunity MI observations in Victoria crater show that hematite concretions are generally smaller and less spherical than those observed farther north on Meridiani Planum, despite similarities in the chemical composition of the rocks. This change in the concretions may be due to lateral differences in depositional environment or diagenesis, or may reflect vertical stratigraphic variations as Opportunity traversed up section. As Opportunity traverses south from Victoria crater, the MI has observed multiple outcrops and cobbles. Some of the cobbles, such as “Santorini” and “Kasos,” show textures that are consistent with the interpretation, based on chemical data, that they are meteorites. More recently, Opportunity studied the boulder “Block Island,” an iron-nickel meteorite. MI images of “Block Island” show triangular features that are interpreted as Widmanstätten patterns, commonly observed in this type of meteorite. The MI has also imaged skeleton-like metal protrusions on “Block Island” that appear to be the result of preferential weathering of interstitial material.

  16. OVERVIEW OF RECENT EXPERIMENTAL RESULTS FROM THE DIII-D ADVANCED TOKAMAK PROGRAM

    SciTech Connect

    BURRELL,HK

    2002-11-01

    OAK A271 OVERVIEW OF RECENT EXPERIMENTAL RESULTS FROM THE DIII-D ADVANCED TOKAMAK PROGRAM. The DIII-D research program is developing the scientific basis for advanced tokamak (AT) modes of operation in order to enhance the attractiveness of the tokamak as an energy producing system. Since the last International Atomic Energy Agency (IAEA) meeting, they have made significant progress in developing the building blocks needed for AT operation: (1) they have doubled the magnetohydrodynamic (MHD) stable tokamak operating space through rotational stabilization of the resistive wall mode; (2) using this rotational stabilization, they have achieved {beta}{sub N}H{sub 89} {ge} 10 for 4 {tau}{sub E} limited by the neoclassical tearing mode; (3) using real-time feedback of the electron cyclotron current drive (ECCD) location, they have stabilized the (m,n) = (3,2) neoclassical tearing mode and then increased {beta}{sub T} by 60%; (4) they have produced ECCD stabilization of the (2,1) neoclassical tearing mode in initial experiments; (5) they have made the first integrated AT demonstration discharges with current profile control using ECCD; (6) ECCD and electron cyclotron heating (ECH) have been used to control the pressure profile in high performance plasmas; and (7) they have demonstrated stationary tokamak operation for 6.5 s (36 {tau}{sub E}) at the same fusion gain parameter of {beta}{sub N}H{sub 89}/q{sub 95}{sup 2} {approx} 0.4 as ITER but at much higher q{sub 95} = 4.2. The authors have developed general improvements applicable to conventional and advanced tokamak operating modes: (1) they have an existence proof of a mode of tokamak operation, quiescent H-mode, which has no pulsed, ELM heat load to the divertor and which can run for long periods of time (3.8 s or 25 {tau}{sub E}) with constant density and constant radiated power; (2) they have demonstrated real-time disruption detection and mitigation for vertical disruption events using high pressure gas jet

  17. Evidence from SOFIA Imaging of Polycyclic Aromatic Hydrocarbon Formation along a Recent Outflow in NGC 7027

    NASA Astrophysics Data System (ADS)

    Lau, Ryan M.; Werner, Michael W.; Sahai, Raghvendra; Ressler, Michael E.

    2016-06-01

    We report spatially resolved (FWHM ~ 3.8 - 4.6'') mid-IR imaging observations of the planetary nebula (PN) NGC 7027 taken with the 2.5-m telescope aboard the Stratospheric Observatory for Infrared Astronomy (SOFIA). Images of NGC 7027 were acquired at 6.3, 6.6, 11.1, 19.7, 24.2, 33.6, and 37.1 μm using the Faint Object Infrared Camera for the SOFIA Telescope (FORCAST). The observations reveal emission from Polycyclic Aromatic Hydrocarbon (PAH) and warm dust (TD ~ 90 K) from the ionized inner edge of the molecular envelope surrounding the central star of the planetary nebula (CSPN). The DustEM code was used to fit the spectral energy distribution of fluxes obtained by FORCAST and the archival infrared spectrum of NGC 7027 acquired by the Short Wavelength Spectrometer (SWS) on the Infrared Space Observatory (ISO). Best-fit dust models reveal a total dust mass of ~6 × 10-3 M⊙, where carbonaceous large (a = 1.5 μm) and very small (a ~ 12 Å) grains, and PAHs (3.1 Å < a <12 Å) compose 96.5, 2.2, and 1.3% of the dust by mass, respectively. The 37 μm optical depth map reveals minima in the dust column density at regions in the envelope that are coincident with a previously identified highly collimated outflow from the CSPN. The column density minima are also spatially coincident with enhancements in the 6.2 μm PAH feature, which is derived from the 6.3 and 6.6 μm maps. We interpret the spatial anti-correlation of the dust column density and PAH 6.2 μm feature strength and their alignment with the outflow from the CSPN as evidence of dust processing and rapid PAH formation via grain-grain collisions in the post-shock environment of the dense photo-dissociation region (PDR) and molecular envelope.

  18. The formation of recent and remote memory is associated with time-dependent formation of dendritic spines in the hippocampus and anterior cingulate cortex.

    PubMed

    Restivo, Leonardo; Vetere, Gisella; Bontempi, Bruno; Ammassari-Teule, Martine

    2009-06-24

    Although hippocampal-cortical interactions are crucial for the formation of enduring declarative memories, synaptic events that govern long-term memory storage remain mostly unclear. We present evidence that neuronal structural changes, i.e., dendritic spine growth, develop sequentially in the hippocampus and anterior cingulate cortex (aCC) during the formation of recent and remote contextual fear memory. We found that mice placed in a conditioning chamber for one 7 min conditioning session and exposed to five footshocks (duration, 2 s; intensity, 0.7 mA; interstimulus interval, 60 s) delivered through the grid floor exhibited robust fear response when returned to the experimental context 24 h or 36 d after the conditioning. We then observed that their fear response at the recent, but not the remote, time point was associated with an increase in spine density on hippocampal neurons, whereas an inverse temporal pattern of spine density changes occurred on aCC neurons. At each time point, hippocampal or aCC structural alterations were achieved even in the absence of recent or remote memory tests, thus suggesting that they were not driven by retrieval processes. Furthermore, ibotenic lesions of the hippocampus impaired remote memory and prevented dendritic spine growth on aCC neurons when they were performed immediately after the conditioning, whereas they were ineffective when performed 24 d later. These findings reveal that gradual structural changes modifying connectivity in hippocampal-cortical networks underlie the formation and expression of remote memory, and that the hippocampus plays a crucial but time-limited role in driving structural plasticity in the cortex. PMID:19553460

  19. Amazonis Planitia: The role of geologically recent volcanism and sedimentation in the formation of the smoothest plains on Mars

    NASA Astrophysics Data System (ADS)

    Fuller, Elizabeth R.; Head, James W.

    2002-10-01

    presence of rough lava flow surfaces underlying the sedimentary debris. These data thus suggest that the unique smoothness of Amazonis Planitia is the result of deposition of thin fluid lava flows and fluvial sediments in an enclosed basin. Crater counts suggest that the most recent resurfacing may have occurred in the latest Amazonian Period, in the last 1% of the history of Mars. In light of its unique history, it is somewhat ironic to note that Amazonis Planitia was originally thought to be a typical young Martian surface and therefore used to name the Amazonian era.

  20. Recent insight on the control of enzymes involved in estrogen formation and transformation in human breast cancer.

    PubMed

    Pasqualini, Jorge R; Chetrite, Gérard S

    2005-02-01

    The great majority of breast cancers are in their early stage hormone-dependent and it is well accepted that estradiol (E2) plays an important role in the genesis and evolution of this tumor. Human breast cancer tissues contain all the enzymes: estrone sulfatase, 17beta-hydroxysteroid dehydrogenase, aromatase involved in the last steps of E2 bioformation. Sulfotransferases which convert estrogens into the biologically inactive estrogen sulfates are also present in this tissue. Quantitative data show that the 'sulfatase pathway', which transforms estrogen sulfates into the bioactive unconjugated E2, is 100-500 times higher than the 'aromatase pathway', which converts androgens into estrogens. The treatment of breast cancer patients with anti-aromatases is largely developed with very positive results. However, the formation of E2 via the 'sulfatase pathway' is very important in the breast cancer tissue. In recent years it was found that antiestrogens (e.g. tamoxifen, 4-hydroxytamoxifen), various progestins (e.g. promegestone, nomegestrol acetate, medrogestone, dydrogesterone, norelgestromin), tibolone and its metabolites, as well as other steroidal (e.g. sulfamates) and non-steroidal compounds, are potent sulfatase inhibitors. In another series of studies, it was found that E2 itself has a strong anti-sulfatase action. This paradoxical effect of E2 adds a new biological response of this hormone and could be related to estrogen replacement therapy in which it was observed to have either no effect or to decrease breast cancer mortality in postmenopausal women. Interesting information is that high expression of steroid sulfatase mRNA predicts a poor prognosis in patients with +ER. These progestins, as well as tibolone, can also block the conversion of estrone to estradiol by the inhibition of the 17beta-hydroxysteroid dehydrogenase type I (17beta-HSD-1). High expressison of 17beta-HSD-1 can be an indicator of adverse prognosis in ER-positive patients. It was shown that

  1. R&D on chalcopyrite based solar cells in Europe: Recent result and developments

    SciTech Connect

    Schock, H.W.; Stolt, L. |

    1996-01-01

    The present developments related to Chalcopyrite-based thin film solar cells are reported. Recent achievement include CuInS{sub 2} based solar cells with efficiencies in the order of 12{percent} and the development of Cd free devices with efficiencies of more than 15{percent}. Submodules based on coevaporation with areas up to 100 cm{sup 2} have been developed and aperture area efficiencies up to 10.2{percent} have been achieved. Reactors for the deposition of submodules with an area of 30{times}30 cm{sup 2} are put into operation. {copyright} {ital 1996 American Institute of Physics.}

  2. Approach to SSME health monitoring. III - Exhaust plume emission spectroscopy: Recent results and detailed analysis

    NASA Astrophysics Data System (ADS)

    Tejwani, Gopal D.; van Dyke, David B.; Bircher, Felix E.

    1993-06-01

    Spectral data for two recent A-1 test firings, 901-717 and 901-718, obtained from an Optical Multichannel Analyzer and an Optical Plume Anomaly Detector, are presented. The spectral data encompasses the database of SSME critical components and materials and the spectral database for the SSME related elements and materials. Relatively strong and continuous emissions from Cr and Fe atomic transitions were observed starting at engine start plus 494 s and persisting until the engine shut off at engine start plus 520 s. These emissions are considered to be emanated from the SSME material AISI 440C, which is traced to high pressure turbopump bearings.

  3. Wavefront correction with a ferrofluid deformable mirror: experimental results and recent developments

    NASA Astrophysics Data System (ADS)

    Brousseau, Denis; Borra, Ermanno F.; Thibault, Simon; Ritcey, Anna M.; Parent, Jocelyn; Seddiki, Omar; Déry, Jean-Philippe; Faucher, Luc; Vassallo, Julien; Naderian, Azadeh

    2008-07-01

    We present the research status of a deformable mirror made of a magnetic liquid whose surface is actuated by a triangular array of small current carrying coils. We demonstrate that the mirror can correct a 11 μm low order aberrated wavefront to a residual RMS wavefront error 0.05 μm. Recent developments show that these deformable mirrors can reach a frequency response of several hundred hertz. A new method for linearizing the response of these mirrors is also presented.

  4. Overview of recent results on Heating and Current Drive in JET

    SciTech Connect

    Ongena, J.; Durodie, F.; Lerche, E.; Eester, D. van; Vrancken, M.; Baranov, Yu.; Challis, C. D.; Jacquet, Ph.; Jenkins, I.; Kiptily, V.; Kirov, K.; Mailloux, J.; Mayoral, M. L.; Monakhov, I.; Nightingale, M.; Walden, A.; Bobkov, V.; Lennholm, M.; Colas, L.; Ekedahl, A.

    2007-09-28

    Recent progress on heating and current drive on JET is reported. Topics discussed are: high power coupling of ICRF/LH at ITER relevant antenna/launcher-separatrix distances, succesfull demonstration of 3 dB couplers for ELM tolerance of the ICRF system, influence of ICRF on LH operation, rotation studies in plasma without external momentum with standard and enhanced JET toriodal field ripple, studies of different ICRF heating schemes and of NTM avoidance schemes using Ion Cyclotron Current Drive. A brief outlook on future plans for experiments at JET is given.

  5. Approach to SSME health monitoring. III - Exhaust plume emission spectroscopy: Recent results and detailed analysis

    NASA Technical Reports Server (NTRS)

    Tejwani, Gopal D.; Van Dyke, David B.; Bircher, Felix E.

    1993-01-01

    Spectral data for two recent A-1 test firings, 901-717 and 901-718, obtained from an Optical Multichannel Analyzer and an Optical Plume Anomaly Detector, are presented. The spectral data encompasses the database of SSME critical components and materials and the spectral database for the SSME related elements and materials. Relatively strong and continuous emissions from Cr and Fe atomic transitions were observed starting at engine start plus 494 s and persisting until the engine shut off at engine start plus 520 s. These emissions are considered to be emanated from the SSME material AISI 440C, which is traced to high pressure turbopump bearings.

  6. Advanced turboprop noise prediction: Development of a code at NASA Langley based on recent theoretical results

    NASA Technical Reports Server (NTRS)

    Farassat, F.; Dunn, M. H.; Padula, S. L.

    1986-01-01

    The development of a high speed propeller noise prediction code at Langley Research Center is described. The code utilizes two recent acoustic formulations in the time domain for subsonic and supersonic sources. The structure and capabilities of the code are discussed. Grid size study for accuracy and speed of execution on a computer is also presented. The code is tested against an earlier Langley code. Considerable increase in accuracy and speed of execution are observed. Some examples of noise prediction of a high speed propeller for which acoustic test data are available are given. A brisk derivation of formulations used is given in an appendix.

  7. The emigration potential of Czechoslovakia, Hungary, Lithuania, Poland and Russia: recent survey results.

    PubMed

    Brym, R J

    1992-12-01

    The author reviews recent evidence concerning the emigration potential of Russia and Eastern Europe, using data from a 1991 survey of 4,269 respondents. "It is demonstrated that the proportion of adults wishing to emigrate from each of these countries in February 1991 varied from a low of 2 per cent in Lithuania to a high of 13 per cent in Poland. Total emigration potential from the region is estimated to have been between 10.2 and 16.7 million....A multiple regression analysis indicates that age and pessimism concerning democracy are the main factors that were independently associated with desire to emigrate." PMID:12179890

  8. Recent Results using a 28 GHz EBW Heating and Current Drive System on MAST

    NASA Astrophysics Data System (ADS)

    Bigelow, Tim; Caughman, John; Peng, Martin; Diem, Stephanie; Hawes, Julian; Gurl, Chris; Griffiths, Jonathan; Shevchenko, Vladimir; Finburg, Paul; Mailloux, Joelle; Taylor, Gary

    2013-10-01

    Improvements to a high power 28 GHz gyrotron system have been made to the MAST Electron Bernstein Wave (EBW) heating, start up, and current drive system in the past few years as collaborative research between ORNL and CCFE. Recent EBW heating and CD experiments on MAST have improved upon previous RF generated plasma current levels. The goals of the research were to extend the initial EBW CD study by increasing substantially the power level and pulse length of the gyrotron hardware and improve transmission line efficiency used in initial experiments. A dummy-load power level of up to 200 kW and a pulse length approaching 0.5 s has been achieved. Arcing, localized to the launcher box, has been observed to limit the launched power level to ~80 kW for up to 450 ms. Several days of high power plasma operation have been recently completed with good progress in increasing the previously attainable solenoid-free plasma current levels. Up to 75 kA of plasma current was achieved at this injected power level. This manuscript has been authored by UT-Battelle, LLC, under Contract No. DE-AC05-00OR22725 with the U.S. Department of Energy.

  9. Health effects of carbon-containing particulate matter: focus on sources and recent research program results.

    PubMed

    Rohr, Annette; McDonald, Jacob

    2016-02-01

    Air pollution is a complex mixture of gas-, vapor-, and particulate-phase materials comprised of inorganic and organic species. Many of these components have been associated with adverse health effects in epidemiological and toxicological studies, including a broad spectrum of carbonaceous atmospheric components. This paper reviews recent literature on the health impacts of organic aerosols, with a focus on specific sources of organic material; it is not intended to be a comprehensive review of all the available literature. Specific emission sources reviewed include engine emissions, wood/biomass combustion emissions, biogenic emissions and secondary organic aerosol (SOA), resuspended road dust, tire and brake wear, and cooking emissions. In addition, recent findings from large toxicological and epidemiological research programs are reviewed in the context of organic PM, including SPHERES, NPACT, NERC, ACES, and TERESA. A review of the extant literature suggests that there are clear health impacts from emissions containing carbon-containing PM, but difficulty remains in apportioning responses to certain groupings of carbonaceous materials, such as organic and elemental carbon, condensed and gas phases, and primary and secondary material. More focused epidemiological and toxicological studies, including increased characterization of organic materials, would increase understanding of this issue. PMID:26635181

  10. Overview and Recent Results from the ZaP Flow Z-Pinch

    NASA Astrophysics Data System (ADS)

    Shumlak, U.; Neslon, B. A.; Adams, C. S.; den Hartog, D. J.; Golingo, R. P.; Knecht, S. D.; Munson, K. A.; Newman, J.; Pasko, J.; Schmuland, D.; Sybouts, M.; Vogman, G.

    2006-10-01

    The ZaP Flow Z-Pinch Experiment at the University of Washington investigates a magnetic confinement configuration that relies on sheared flow for stability in an otherwise unstable configuration. An axially flowing Z-pinch is generated with a coaxial accelerator coupled to a pinch assembly chamber. Magnetic probes measure fluctuation levels. The plasma is magnetically confined for an extended quiescent period where the mode activity is reduced. Multichord Doppler shift measurements of impurity lines show a sub-Alfvenic, sheared flow during the quiescent period and low shear profiles during periods of high mode activity. The plasma has a sheared axial flow that exceeds the theoretical threshold for stability during the quiescent period and is lower than the threshold during periods of high mode activity. A holographic interferometer measures a radially peaked density profile during the quiescent period. Density profiles are analyzed to determine magnetic field and temperature profiles. Internal magnetic fields have been recently determined by measuring the Zeeman splitting of impurity carbon emission. The measurements are consistent with a magnetically confined pinch plasma. Recent experimental measurements will be presented. This work is supported by a grant from DOE.

  11. Key Recent Scientific Results from the Opportunity Rover's Exploration of Endeavour Crater, Mars

    NASA Technical Reports Server (NTRS)

    Arvidson, R. E.; Squyres, S. W.; Gellert, R.; Herkenhoff, K.; Mittlefehldt, D.; Crumpler, L.; McLennan, S.; Farrand, W. H.; Joliff, B. L.; Morris, R. V.

    2015-01-01

    The Opportunity Rover is currently in its 11th year of operations, exploring the rim of the approximately 22 km wide Noachian-age Endeavour Crater. Opportunity spent its 5th winter season in Cook Haven, a gentle swale along Murray Ridge. Two small rocks serendipitously overturned by rover wheel motions show evidence for aqueous precipitation of sulfates, and interaction with a strong oxidant (e.g., O2) to form a thin, high valence state Mn oxide coating. After the winter, Opportunity headed south to Cape Tribulation and explored Shoemaker formation impact breccias, finding numerous Ca-sulfate veins cutting across outcrops. A key target for Opportunity's measurements has been the Spirit of Saint Louis crater (SoSL), which is approximately 25 m wide, oval in plan view, shallow, flat-floored, and has a slightly raised rim. SoSL crater is surrounded by an apron of bright, polygonally-shaped outcrops and is superimposed on a gentle swale in Cape Tribulation. Rocks in a thin reddish zone on the rim are enriched in hematite, Si, and Ge, and depleted in Fe, relative to surrounding rocks. Apron rocks include an outcrop also enriched in Si and Ge, and slightly depleted in Fe. In general rocks in the crater and apron have elevated S relative to Shoemaker formation breccias, tracking values observed in the Cook Haven and the Hueytown (fracture running perpendicular to Cape Tribulation) outcrops. SoSL crater lies just to the west of Marathon Valley, a key target for exploration by Opportunity because five separate CRISM observations indicate the presence of Fe/Mg smectites on the upper valley floor. Opportunity data show that low relief, relatively bright polygonal outcrops dominate the valley floor where not covered by scree and soil shed from surrounding walls. Initial reconnaissance shows that the outcrops are breccias with compositions similar to the typical SoSL crater apron and floor rocks, although only the very upper portion of the valley has been explored as of August

  12. Carbon dioxide formation and elimination in man. Recent theories and possible consequences.

    PubMed

    Wiklund, L

    1996-01-01

    Systemic metabolism results in a production of not only carbon dioxide, water and urea but also bicarbonate ions. Most of these bicarbonate ions are generated during the catabolism of glutamine. In order to be eliminated as carbon dioxide in the lungs bicarbonate ions must be protonised. This protonisation of the bicarbonate ion seems to take place in a number of tissue compartments in which acid-base balance is maintained. One of the most important processes for protonisation of the bicarbonate ion is the hepatic ureagenesis from ammonia/ammonium ions. A substantial part of the ammonia/ammonium ions are generated during the catabolism of amino acids. Terminal oxidation of glutamine in the gut seems to be of great significance for this process. In certain conditions the enteric generation of ammonium ions seems so important that an ATP-driven enterohepatic recirculation of ammonium ions/urea constituting an amplifying mechanism for the protonisation of the bicarbonate ion is motivated. PMID:8740926

  13. Recent results and prospects of exotic hadrons at B-factories

    NASA Astrophysics Data System (ADS)

    Wang, Xiaolong

    2016-05-01

    The recent measurement on e+e- → π+π-ψ(2S) via initial-state-radiation from the Belle experiment is reviewed. This measurement improves the determination of the properties of Y(4360) and Y(4660). Y(4260) → π+π-ψ(2S) is also studied. The significance of Y(4260) is less than 3σ, however, this state has a significant affect on determining parameters of Y(4360) and Y(4660). Evidence for a charged charmoniumlike structure at 4.05 GeV/c2 is observed in the π±ψ(2S) intermediate state in the Y(4360) decays. Finally, we review the promise of the Belle II in understanding the nature of exotic states.

  14. Recent HERMES results from inclusive and semi-inclusive hadron production

    NASA Astrophysics Data System (ADS)

    Van Hulse, Charlotte

    2015-01-01

    Hermes collected a wealth of data using the 27.6 GeV polarized Hera lepton beam and various pure, polarized and unpolarized, gaseous targets. This unique data set opens the door to various measurements sensitive to the multi-dimensional structure of the nucleon. Among them are two-hadron production in semi-inclusive deep-inelastic scattering on a transversely polarized target, providing access to different transverse-momentum-dependent distribution and fragmentation functions in a way complementary to single-hadron production. Also transverse-target single-spin asymmetries in inclusive electroproduction of charged pions and kaons have been recently extracted, complementing data from proton-proton collisions, where large, so far unexplained, asymmetries have been observed. From inclusive measurements on various nuclear targets, the Λ polarization is extracted, also here complementing measurements in proton-proton collisions.

  15. Recent results from operation of the ANTARES deep-sea neutrino telescope

    NASA Astrophysics Data System (ADS)

    Hallewell, G. D.

    2014-12-01

    The ANTARES neutrino telescope is currently the largest operating water Cherenkov detector and the largest neutrino detector in the Northern hemisphere. It comprises 885 optical modules distributed on 12 detection lines anchored at a depth of 2.5 km in the Mediterranean Sea near Toulon, France; at a latitude that accesses a large part of the Galactic Plane, including the Galactic Centre. Its main scientific target is the detection of multi-TeV neutrinos predicted in charged cosmic particle acceleration mechanisms. In addition, ANTARES has developed a range of multi-messenger search strategies to look for correlations with optical counterparts and other cosmic messengers including γ-rays and charged cosmic rays. Other topics of investigation include the search for neutrinos from dark matter annihilation, searches for exotic particles and the measurement of neutrino oscillations. Details of the telescope are discussed together with examples of recently-conducted searches.

  16. Recent results from the TwinSol low-energy RIB facility

    NASA Astrophysics Data System (ADS)

    Becchetti, F. D.; Kolata, J. J.

    2016-06-01

    We report on some of the recent developments and experimental work done at the twin-solenoid low-energy radioactive-ion-beam (RIB) facility TwinSol installed at the U Notre Dame 10 MV FN tandem accelerator. The TwinSol facility is a joint project of the University of Michigan (UM) and the University of Notre Dame (UND), and includes several U.S. and foreign collaborators. A number of significant experiments including RIB-induced transfer reactions, elastic scattering, resonant scattering, and fusion at energies near and well below the Coulomb barrier have been performed with this facility. Several of these as well as future work and upgrades planned will be described.

  17. Recent results on reactions with radioactive beams at RIBRAS (Radioactive Ion Beams in Brazil)

    NASA Astrophysics Data System (ADS)

    Lépine-Szily, A.; Lichtenthäler, R.; Guimarães, V.; Arazi, A.; Barioni, A.; Benjamim, E. A.; de Faria, P. N.; Descouvemont, P.; Gasques, L. R.; E; Leistenschneider; Mendes, D. R., Jr.; Morais, M. C.; Morcelle, V.; Moro, A. M.; Pampa Condori, R.; Pires, K. C. C.; Rodriguez-Gallardo, M.; Scarduelli, V.; Shorto, J. M. B.; Zamora, J. C.

    2015-04-01

    We present a quick description of RIBRAS (Radioactive Ion beams in Brazil), which is a superconducting double solenoid system, installed at the Pelletron Laboratory of the University of São Paulo and extends the capabilities of the original Pelletron Tandem Accelerator of 8MV terminal voltage (8UD) by producing secondary beams of unstable nuclei. The experimental program of the RIBRAS covers the study of elastic and inelastic scattering with the objective to study the interaction potential and the reaction mechanisms between weakly bound (RIB) and halo (6He and 8B) projectiles on light, medium and heavy mass targets. With highly purified beams, the study of resonant elastic scattering and resonant transfer reactions, using inverse kinematics and thick targets, have also been included in our recent experimental program.

  18. Recent results from the Tara tandem mirror and Constance-B mirror

    SciTech Connect

    Post, R.S.; Brau, K.; Casey, J.; Chen, X.; Coleman, J.; Garner, R.; Golovato, S.; Gerver, M.; Goodman, D.; Guss, W.

    1986-11-01

    The Tara tandem mirror program has studied anchor and ponderomotive stabilization, axicell plugging with ECH and ICRF, sloshing ion buildup in the axicells, and halo formation and stabilization by an axisymmetric divertor. Central cell plasma parameters achieved by midplane fueling and slow wave ICRF heating from a local magnetic hill are ..beta.. = 1.2%, n/sub e/ = 3 x 10/sup 12/ cm/sup -3/. The plasma is stabilized both by anchor ion ..beta.. and by ponderomotive stabilization with the central cell ICRF in combination with a magnetic divertor, realizing a completely axisymmetric configuration. Anchor ICRF creates non-Boltzman potential plugging of central cell ions. Neutral beam injection establishes a sloshing ion distribution for a cold dense central cell stream; the hot ion confinement is classical and dominated by electron drag. Axicell ECH plugging experiments lead to near total reduction in endloss, but also to a decrease in the central cell density, indicating increased radial losses. Single-ended ECH plugging shows no increase in opposite endloss. Single-ended plugging with axicell ICRF produces 50% reduction in ion endloss, with about half of the reflected ions observed in the opposite endloss. In the Constance-B quadrupole mirror the hot electron pressure profile is peaked off-axis and has the shape of a baseball seam.

  19. Overview and Recent Results from the HyperV Plasma Gun

    NASA Astrophysics Data System (ADS)

    Witherspoon, F. Douglas; Case, Andrew; Messer, Sarah; Bomgardner, Richard; Phillips, Michael; van Doren, David; Elton, Raymond; Uzun-Kaymak, Ilker

    2007-11-01

    We present an overview of research at HyperV to develop high velocity dense plasma jets for application to fusion and HEDP. The approach uses symmetrical pulsed injection of high density plasma into a coaxial EM accelerator having a cross-section tailored to prevent formation of the blow-by instability. Two development paths are followed to accomplish this injection step: we compare large arrays of capillary discharges to sparkgaps arranged in a toroidal configuration. Experiments on three test fixtures are described: a 2pi configuration with 64 capillary injectors, a 32 injector prototype gun designed to drive rotation in the Maryland MCX experiment, and a second gun using 112 sparkgap electrodes for injection. Data is presented from visible light spectroscopy, fast optical imaging, Rogowski coils, pressure probes, Bdot probes, photodiodes, and a laser interferometer. Ballistic pendulum tests indicate plasma jets with mass 160 micrograms at 70 km/s have been achieved with plasma density above 10^15 cm-3.

  20. Results from Recent Observations and Modeling of Saharan Dust interaction with Hurricane Nadine (2012)

    NASA Astrophysics Data System (ADS)

    Shi, J. J.; Braun, S. A.; Tao, W. K.; Tao, Z.; Sippel, J. A.; Matsui, T.; Peters-Lidard, C. D.

    2015-12-01

    The Hurricane and Severe Storm Sentinel (HS3) was a multiyear field campaign with the goal of improving understanding of hurricane formation and intensity change. One of HS3's primary science goals was to obtain measurements to help determine the extent to which the Saharan air layer impacts storm intensification. This presentation will focus on environmental observations obtained by one of the Global Hawks (dropsonde derived profiles of temperature, humidity, wind speed and wind direction; interferometer derived profiles of temperature and humidity in the clear air; and lidar derived profiles of Saharan dust and clouds) during the early stages of Hurricane Nadine (2012) when it interacted with the Saharan air layer. In addition, the Goddard Space Flight Center version of the Weather Research and Forecasting model with interactive aerosol-cloud-radiation physics is used to generate 30-member ensemble simulations of Nadine with and without the aerosol interactions. Preliminary conclusions related to the impact of the Saharan air layer on the evolution of Nadine will be described.

  1. Results of NASA's First Autonomous Formation Flying Experiment: Earth Observing-1 (EO-1)

    NASA Technical Reports Server (NTRS)

    Folta, David; Hawkins, Albin; Bauer, Frank (Technical Monitor)

    2002-01-01

    NASA's first autonomous formation flying mission completed its primary goal of demonstrating an advanced technology called enhanced formation flying. To enable this technology, the Flight Dynamics Analysis Branch at the Goddard Space Flight Center implemented a universal 3-axis formation flying algorithm in an autonomous executive flight code onboard the New Millennium Program's (NMP) Earth Observing-1 (EO-1) spacecraft. This paper describes the mathematical background of the autonomous formation flying algorithm, the onboard flight design and the validation results of this unique system. Results from fully autonomous maneuver control are presented as comparisons between the onboard EO-1 operational autonomous control system called AutoCon, its ground-based predecessor used in operations, and the original standalone algorithm. Maneuvers discussed encompass reactionary, routine formation maintenance, and inclination control. Orbital data is also examined to verify that all formation flying requirements were met.

  2. Results Of NASA's First Autonomous Formation Flying Experiment: Earth Observing-1 (EO-1)

    NASA Technical Reports Server (NTRS)

    Folta, David; Hawkins, Albin

    2002-01-01

    NASA's first autonomous formation flying mission completed its primary goal of demonstrating an advanced technology called Enhanced Formation Flying. To enable this technology, a team at the Goddard Space Flight Center implemented a universal 3-axis formation flying algorithm in an autonomous executive flight code onboard the New Millennium Program's (NMP) Earth Observing-1 (EO-1) spacecraft. This paper describes the mathematical background of the autonomous formation flying algorithm, the onboard flight design and the validation results of this unique system. Results from fully autonomous maneuver control are presented as comparisons between the onboard EO-1 operational autonomous control system called AutoCon(trademark), its ground-based predecessor used in operations, and the original standalone algorithm. Maneuvers discussed encompass reactionary, routine formation maintenance, and inclination control. Orbital data is also examined to verify that all formation flying requirements were met.

  3. Gulf of Alaska continental slope morphology: Evidence for recent trough mouth fan formation

    NASA Astrophysics Data System (ADS)

    Swartz, John M.; Gulick, Sean P. S.; Goff, John A.

    2015-01-01

    continental shelves are host to numerous morphologic features that help understand past glacier dynamics. Southeastern Alaska is home to the St. Elias mountains, an active orogen that also hosts temperate marine glaciers. During glacial periods ice streams advance across the continental shelf, carving shelf-crossing troughs that reach the shelf edge. We use high-resolution multibeam data to develop the relationship between the Yakutat and Alsek Sea Valleys and the resulting continental slope morphology. The shelf and slope geomorphology can be divided into statistical groupings that relate to the relative balance of erosion and deposition. Our analysis indicates that only the Yakutat system has been able to build an incipient trough-mouth fan. The extreme sediment supply from this region was able to overwhelm the steep initial topography of the transform margin while further to the east sediment slope-bypass dominates. This analysis provides an extreme end member to existing studies of temperate glaciation along continental margins. The unique interplay between rapid uplift due to ongoing collision and the massive erosion caused by temperate glaciers provides for sedimentary flux far above most other systems.

  4. Recent Results from the Spirit Rover at Home Plate and "Silica Valley"

    NASA Astrophysics Data System (ADS)

    Squyres, S. W.

    2007-12-01

    right front wheel excavated a small patch of high albedo soil. Mini-TES spectra of this soil were well fit by amorphous silica, and subsequent investigation with the APXS showed a composition that was more than 90% SiO2. The deposits are also enriched in Ti. Mini-TES spectra of nearby rocks also show a strong signature of amorphous silica, and APXS spectra of these rocks also confirm a high silica content. We consider two hypotheses for the formation of these silica-rich deposits. One is that they developed via precipitation from hydrothermal fluids. Siliceous sinter deposits are common in terrestrial hydrothermal environments where fluids dissolve Si from host rocks at high temperatures and then reprecipitate silica at lower temperatures. Alternatively, the Si-rich materials may represent the remnants of formerly basaltic materials that have been extensively leached in a fumarolic environment under acid sulfate conditions. In either case, the proximity to Home Plate is consistent with formation via the interaction of basaltic volcanism with groundwater. The astrobiological implications of these Si-rich deposits may be significant. Both hydrothermal systems and fumaroles are capable of supporting microbial ecosystems on Earth, and precipitated silica deposits in both environments can preserve strong textural evidence of microbial life.

  5. Key Recent Scientific Results from the Opportunity Rover's Exploration of Cape Tribulation, Endeavour Crater, Mars

    NASA Astrophysics Data System (ADS)

    Arvidson, R. E.; Squyres, S. W.; Gellert, R.; Herkenhoff, K. E.; Mittlefehldt, D. W.; Crumpler, L. S.; McLennan, S. M.; Farrand, W. H.; Jolliff, B. L.; Morris, R. V.

    2015-12-01

    The Opportunity Rover is in its 11th year of exploration, currently exploring the Cape Tribulation rim segment of the ~22 km wide Noachian Endeavour Crater and its tilted and fractured outcrops. A key target for Opportunity's measurements has been the Spirit of Saint Louis crater (SoSL), which is ~25 m wide, oval in plan view, shallow, flat-floored, and has a slightly raised rim. SoSL crater is surrounded by an apron of bright, polygonally-shaped outcrops and is superimposed on a gentle swale in Cape Tribulation. Rocks in a thin reddish zone on the rim are enriched in hematite, Si, and Ge, and depleted in Fe, relative to surrounding rocks. Apron rocks include an outcrop also enriched in Si and Ge, and slightly depleted in Fe. In general rocks in the crater and apron have elevated S levels relative to Shoemaker formation breccias, tracking values observed in the Cook Haven (gentle swale superimposed on Murray Ridge and site of Opportunity's 5th winter site) and the Hueytown fracture (running perpendicular to Cape Tribulation) outcrops. SoSL crater lies just to the west of Marathon Valley, a key target for exploration by Opportunity because five separate CRISM observations indicate the presence of Fe/Mg smectites on the upper valley floor. Opportunity data show that low relief, relatively bright, wind-scoured outcrops dominate the valley floor where not covered by scree and soil shed from surrounding walls. Initial reconnaissance shows that the outcrops are breccias with compositions similar to the typical SoSL crater apron and floor rocks, although only the very upper portion of the valley has been explored as of August 2015. Pervasive but modest aqueous alteration of Endeavour's rim is implied by the combination of CRISM and Opportunity data, providing insight into early aqueous processes dominated in this location by relatively low water to rock ratios, and at least in part associated with enhanced fluid flow along fractures.

  6. Recent results in search for new physics at the Tevatron (Run I)

    SciTech Connect

    John Zhou

    2004-01-12

    We present some new results on searches for new physics at the Tevatron Run 1 (1992-1996). The topics covered are searches for R-Parity violating and conserving mSUGRA, large extra dimensions in di-photon and monojet channels, leptoquark in jets + E{sub T} channel, and two model independent searches. All results were finalized during the past year.

  7. Recent results on eta and eta-prime photoproduction on the proton

    SciTech Connect

    Barry Ritchie

    2004-06-01

    The experimental situation on eta and eta' photoproduction on the proton is reviewed, emphasizing progress made since 2001. New preliminary results for eta' photoproduction on the proton from Jefferson Lab are presented. Experimental results are compared with several theoretical approaches, with an emphasis on consequences for understanding baryon spectroscopy.

  8. Formation of gullies on Mars: link to recent climate history and insolation microenvironments implicate surface water flow origin.

    PubMed

    Head, James W; Marchant, David R; Kreslavsky, Mikhail A

    2008-09-01

    Features seen in portions of a typical midlatitude Martian impact crater show that gully formation follows a geologically recent period of midlatitude glaciation. Geological evidence indicates that, in the relatively recent past, sufficient snow and ice accumulated on the pole-facing crater wall to cause glacial flow and filling of the crater floor with debris-covered glaciers. As glaciation waned, debris-covered glaciers ceased flowing, accumulation zones lost ice, and newly exposed wall alcoves continued as the location for limited snow/frost deposition, entrapment, and preservation. Analysis of the insolation geometry of this pole-facing crater wall, and similar occurrences in other craters at these latitudes on Mars, shows that they are uniquely favored for accumulation of snow and ice, and a relatively more rapid exposure to warmer summer temperatures. We show that, after the last glaciation, melting of residual snow and ice in alcoves could have formed the fluvial channels and sedimentary fans of the gullies. Recent modeling shows that top-down melting can occur in these microenvironments under conditions similar to those currently observed on Mars, if small amounts of snow or frost accumulate in alcoves and channels. Accumulation and melting is even more favored in the somewhat wetter, relatively recent geological past of Mars, after the period of active glaciation. PMID:18725636

  9. Formation of gullies on Mars: Link to recent climate history and insolation microenvironments implicate surface water flow origin

    PubMed Central

    Head, James W.; Marchant, David R.; Kreslavsky, Mikhail A.

    2008-01-01

    Features seen in portions of a typical midlatitude Martian impact crater show that gully formation follows a geologically recent period of midlatitude glaciation. Geological evidence indicates that, in the relatively recent past, sufficient snow and ice accumulated on the pole-facing crater wall to cause glacial flow and filling of the crater floor with debris-covered glaciers. As glaciation waned, debris-covered glaciers ceased flowing, accumulation zones lost ice, and newly exposed wall alcoves continued as the location for limited snow/frost deposition, entrapment, and preservation. Analysis of the insolation geometry of this pole-facing crater wall, and similar occurrences in other craters at these latitudes on Mars, shows that they are uniquely favored for accumulation of snow and ice, and a relatively more rapid exposure to warmer summer temperatures. We show that, after the last glaciation, melting of residual snow and ice in alcoves could have formed the fluvial channels and sedimentary fans of the gullies. Recent modeling shows that top-down melting can occur in these microenvironments under conditions similar to those currently observed on Mars, if small amounts of snow or frost accumulate in alcoves and channels. Accumulation and melting is even more favored in the somewhat wetter, relatively recent geological past of Mars, after the period of active glaciation. PMID:18725636

  10. [Homeless and mentally ill. Review of recent research and results on a doubly disadvantaged minority].

    PubMed

    Kellinghaus, C; Eikelmann, B; Ohrmann, P; Reker, T

    1999-03-01

    There are about 200,000 homeless persons in Germany, 35,000 of them living on the streets. They suffer from unemployment, poverty, social isolation and physical impairments. More than two-thirds of them suffer from mental illness as well. Substance abuse predominates, but also schizophrenic and affective disorders and personality disorders show a higher prevalence than among the general population. Comorbidity is found frequently. However, mental disorders are just one of several factors contributing to the process of becoming homeless. Due to the complex combination of mental, physical, social and economic problems of the homeless mentally ill psychiatric care is not sufficient. Yet recent US studies show that a combination of multimodal clinical measures and a network of outpatient assistance can improve both physical and mental health and the social situation. Having established reliable epidemiological data, future research should concentrate on analysing the influence of homelessness on mental health, and on planning and evaluating specific programmes for the homeless mentally ill. PMID:10214555

  11. Clinical development of gene therapy: results and lessons from recent successes

    PubMed Central

    Kumar, Sandeep RP; Markusic, David M; Biswas, Moanaro; High, Katherine A; Herzog, Roland W

    2016-01-01

    Therapeutic gene transfer holds the promise of providing lasting therapies and even cures for diseases that were previously untreatable or for which only temporary or suboptimal treatments were available. For some time, clinical gene therapy was characterized by some impressive but rare examples of successes and also several setbacks. However, effective and long-lasting treatments are now being reported from gene therapy trials at an increasing pace. Positive outcomes have been documented for a wide range of genetic diseases (including hematological, immunological, ocular, and neurodegenerative and metabolic disorders) and several types of cancer. Examples include restoration of vision in blind patients, eradication of blood cancers for which all other treatments had failed, correction of hemoglobinopathies and coagulation factor deficiencies, and restoration of the immune system in children born with primary immune deficiency. To date, about 2,000 clinical trials for various diseases have occurred or are in progress, and many more are in the pipeline. Multiple clinical studies reported successful treatments of pediatric patients. Design of gene therapy vectors and their clinical development are advancing rapidly. This article reviews some of the major successes in clinical gene therapy of recent years. PMID:27257611

  12. StarDriver: Recent results on beam smoothing and LPI mitigation

    NASA Astrophysics Data System (ADS)

    Eimerl, D.; Skupsky, S.; Campbell, E. M.

    2016-05-01

    StarDriver was recently proposed as a highly flexible laser driver for inertial confinement fusion and high energy density physics. It envisions a laser drive consisting of very many beams at an aperture and energy where the optical technology is well-developed, used in concert to create a large scale laser driver system. In this paper we describe a StarDriver-class laser with 5120 physical beamlets disposed about the target chamber in 80 evenly spaced ports, each port containing 64 beamlets, each beamlet having about ∼1.5THz of 2D SSD bandwidth and suitable phase plates, an aperture of ∼65mm, an energy of 80J, and frequency-converted to ∼351nm.many beamlets at an aperture where optical technology is well-developed, and each beamlet has energy ∼100J in a several times diffraction limited beam. The ensemble of beamlets has frequency bandwidth 2%-10%, thereby providing significant control of both hydrodynamic and laser-plasma instabilities The drive at the target is ∼400kJ, has a well-behaved low L-mode spectrum, and smooths very rapidly, reaching an asymptotic smoothness of <1% in less than Ins.

  13. [European surveillance of tuberculosis: description of the network and recent results].

    PubMed

    Infuso, A; Falzon, D

    2005-05-01

    A network for the surveillance of tuberculosis covering the WHO European Region was set up in 1996. It aims to improve the contribution of surveillance to TB control, promoting standardised methods to compare countries. Standardized individual or aggregate data on notified TB cases is provided annually from national surveillance institutions. In the enlarged European Union (EU), overall TB notification rates decreased in recent years (14/100 000 in 2002), but leveled off in some countries including France and the United Kingdom, partly due to increasing numbers of patients from high TB incidence areas (30% in 2002). Multidrug resistance (MDR) was much more frequent in the Baltic States (21% in 2002) than in other countries (1.7%; range: 0-3.7%). Treatment of new pulmonary TB cases notified in 2001 was completed within 12 months in 74% of cases, ongoing in 3%, interrupted due to death in 7%, and interrupted for other reasons or unknown in 15%. In the Balkans and Turkey, notification rates ranged between 20 and 62 per 100 000 in 2002, and decreasing or stable except for Romania (153 in 2002). In the East (former Soviet Union), TB surveillance data, although incomplete, shows an increasing incidence (97/100 000 in 2002), high prevalence of primary MDR (14% in Kazakhstan), and frequent treatment failures (10% in new cases). At the time of EU enlargement, European TB surveillance covering the whole WHO European Region should continue, with support of TB control in the East as a regional priority. PMID:15885956

  14. Clinical development of gene therapy: results and lessons from recent successes.

    PubMed

    Kumar, Sandeep Rp; Markusic, David M; Biswas, Moanaro; High, Katherine A; Herzog, Roland W

    2016-01-01

    Therapeutic gene transfer holds the promise of providing lasting therapies and even cures for diseases that were previously untreatable or for which only temporary or suboptimal treatments were available. For some time, clinical gene therapy was characterized by some impressive but rare examples of successes and also several setbacks. However, effective and long-lasting treatments are now being reported from gene therapy trials at an increasing pace. Positive outcomes have been documented for a wide range of genetic diseases (including hematological, immunological, ocular, and neurodegenerative and metabolic disorders) and several types of cancer. Examples include restoration of vision in blind patients, eradication of blood cancers for which all other treatments had failed, correction of hemoglobinopathies and coagulation factor deficiencies, and restoration of the immune system in children born with primary immune deficiency. To date, about 2,000 clinical trials for various diseases have occurred or are in progress, and many more are in the pipeline. Multiple clinical studies reported successful treatments of pediatric patients. Design of gene therapy vectors and their clinical development are advancing rapidly. This article reviews some of the major successes in clinical gene therapy of recent years. PMID:27257611

  15. Recent Results in the Top Quark Sector from the D0 Experiment

    SciTech Connect

    None, None

    2015-04-10

    In these proceedings, I review recent measurements in the top quark sector in pp-bar collisions at a centre-of-mass energy of √s = 1.96 TeV in Run II of the Fermilab Tevatron Collider using the D0 detector. I will present the differential measurement of the tt-bar production cross section and the Tevatron combination of inclusive tt-bar cross section measurements; the first evidence of the production of single top quarks in the s-channel by D0 and the observation in combination with CDF. Furthermore, I will review the measurements of the forward-backward asymmetry in tt-bar events, and conclude with the world’s most precise single measurement of the top quark mass, which is a fundamental parameter of the standard model, and present the Tevatron combination, which is the world’s most precise determination of the top quark mass, with a relative precision of 0.37%.

  16. Recent results on materials aspects of the investigation of new topological states of matter

    NASA Astrophysics Data System (ADS)

    Cava, Robert

    Investigation of the electronic states of matter that are determined by topological physics has exploded in recent years through parallel progress in theory, experimental characterization, device fabrication and new materials development. In our group working in this area, the speaker has been responsible for the development of new materials to allow the experimentalists to probe the emergence of new topological properties, and to help embody the concepts of our theorists in real materials. The field is fast-moving, with particular thrusts at the present time toward Weyl and Dirac semimetals, and in this talk I will describe the materials aspects of our work in the past year in these areas, specifically as they are related to our strong collaborations with the groups of N.P. Ong, A. Yazdani, and B.A. Bernevig at Princeton, T. Valla and J. Tao at Brookhaven, and A. Vishwanath at Berkeley. The support of our work in this area by the NSF through its MRSEC program, Grant DMR 1420541, and the ARO through its MURI on topological insulators, Grant W911NF-12-1-0461, is gratefully acknowledged.

  17. Development of Compact Resonant Diplexers for Ecrh:. Design, Recent Results, and Plans

    NASA Astrophysics Data System (ADS)

    Kasparek, W.; Plaum, B.; Brand, P.; Lechte, C.; Saliba, M.; Wang, Y.; Erckmann, V.; Hollmann, F.; Michel, G.; Noke, F.; Purps, F.; Stober, J.; Wagner, D.; Petelin, M.; Koposova, E.; Lubyako, L.; Doelman, N.; van den Braber, R.; Bruschi, A.; Bongers, W.; Thoen, D. J.

    2011-02-01

    High-power diplexers can be used in ECRH systems as power or beam combiners (BC), slow and fast directional switches (FADIS) to toggle the power from continuously operating gyrotrons between two launchers, and discriminators of low-power ECE signals from high-power ECRH in launchers used for in-line ECE. In the paper, design options for resonant diplexers are presented, and detailed low-power investigations on transmission characteristics and insertion losses are discussed. Two types, a purely quasi-optical and a compact waveguide-compatible diplexer, respectively, have been tested with high-power in the 140 GHz ECRH system for the stellarator W7-X. Fast switching, arbitrary distribution of the gyrotron power to two outputs, as well as power combination could be demonstrated with the first prototype. In recent experiments with a compact design, a mirror drive for tracking of the resonator to the gyrotron frequency was implemented; first long-pulse tests on transmission characteristics are shown. Finally, plans for implementation of this diplexer in the ECRH at ASDEX Upgrade are described.

  18. D0 dimuon charge asymmetry from Bs system with Z' couplings and the recent LHCb result

    NASA Astrophysics Data System (ADS)

    Kim, Hyung Do; Kim, Sung-Gi; Shin, Seodong

    2013-07-01

    The D0 collaboration has announced the observation of the like-sign dimuon charge asymmetry since 2010, which has a difference of more than 3σ from the Standard Model prediction. One of the promising explanations is considering the existence of flavor-changing Z' couplings to the b and s quarks which can contribute to the off-diagonal decay width in the Bs-B¯s mixing. Model construction is highly constrained by the recent LHCb data of 1fb-1 integrated luminosity. In this paper, we analyze the experimental constraints on constructing new physics models to explain the dimuon charge asymmetry from the CP violation of the Bs system. We present limits on Z' couplings and show that it is impossible to obtain the 1σ range of the dimuon charge asymmetry without the new contribution in the Bd system. Even with an arbitrary contribution in the Bd system, the new couplings must be in the fine-tuned region.

  19. Radition belt dynamics : Recent results from van Allen Probes and future observations from CeREs

    NASA Astrophysics Data System (ADS)

    Kanekal, Shrikanth; O'Brien, Paul; Baker, Daniel N.; Ogasawara, Keiichi; Fennell, Joseph; Christian, Eric; Claudepierre, Seth; Livi, Stefano; Desai, Mihir; Li, Xinlin; Jaynes, Allison; Turner, Drew; Jones, Ashley; Schiller, Quintin

    2016-07-01

    We describe recent observations of the Earth's radiation belts made by instruments on board the Van Allen Probes mission, particularly the Relativistic Electron Proton Telescope (REPT) and the Magnetic Electron Ion spectrometer (MagEIS). These observations have significantly advanced our understanding of terrestrial radiation belt dynamics. The Van Allen Probes mission comprises two identically instrumented spacecraft which were launched 31 August, 2012 into low-inclination lapping equatorial orbits. The orbit periods are about 9 hours, with perigees and apogees of of ~600 km and 5.8 RE respectively. We discuss the new scientific findings of the Van Allen Probes mission regarding the physics of energization and loss of relativistic electrons and their implications for future low-cost missions, especially CubeSats. We describe the CeREs (a Compact Radiation belt Explorer) CubeSat mission currently being built at the Goddard Space Flight Center, and carrying on board, an innovative instrument, the Miniaturized Electron Proton Telescope (MERiT). The MERiT is a compact low-mass low-power instrument measuring electrons from a few keV to tens of MeV in multiple differential channels. MERiT is optimized to measure electron microbursts with a high time resolution of a few milliseconds. We present and discuss possible future scientific contributions from CeREs.

  20. Exploring 100+ Year Variability with DASCH: Statistical Methods and Recent Results.

    NASA Astrophysics Data System (ADS)

    Miller, George Franklin; Grindlay, Jonathan E.; Los, Edward

    2014-06-01

    The Digital Access to a Sky Century at Harvard (DASCH) project is currently digitizing the roughly 500,000 photographic plates maintained by the Harvard College Observatory. The Harvard plate collection covers each point of the sky roughly 500 to 3000 times from 1885 to 1992, with limiting magnitudes ranging from B=14-18 mag and photometric accuracy within ±0.1 mag. Production scanning (roughly 400 plates/day) is proceeding in Galactic coordinates from the North Galactic Pole and is currently at roughly 40 degrees galactic latitude. The vastness of these data makes DASCH unique in its ability to systematically study variability on decade-long time scales across the entire sky. We are developing new statistical mining techniques to predictively identify the many classes of stellar variability and explore their long-term behavior, as well as discover new unusual cases/classes of variability. Most recently, we are working to implement wavelet-based algorithms into our mining routines, better allowing us to analyze localized non-periodic signals. Here we report on the progress of our mining and machine learning routines, as well as share several of the exciting new discoveries that are being made with DASCH. We gratefully acknowledge support from NSF grants AST-0407380, AST-0909073 and AST-1313370.

  1. Compendium of Recent Test Results of Single Event Effects Conducted by the Jet Propulsion Laboratory

    NASA Technical Reports Server (NTRS)

    Allen, Gregory R.; Guertin, Steven M.; Scheick, Leif Z.; Irom, Farokh; Zajac, Stephanie

    2012-01-01

    This paper reports heavy ion, proton, and laser induced single event effects results for a variety of microelectronic devices targeted for possible use in NASA spacecrafts. The compendium covers devices tested within the years of 2010 through 2012.

  2. RECENT RESULTS OF RADIATION HYDRODYNAMICS AND TURBULENCE EXPERIMENTS IN CYLINDRICAL GEOMETRY.

    SciTech Connect

    Magelssen G. R.; Scott, J. M.; Batha, S. H.; Holmes, R. L.; Lanier, N. E.; Tubbs, D. L.; Elliott, N. E.; Dunne, A. M.; Rothman, S.; Parker, K. W.; Youngs, D.

    2001-01-01

    Cylindrical implosion experiments at the University of Rochester laser facility, OMEGA, were performed to study radiation hydrodynamics and compressible turbulence in convergent geometry. Laser beams were used to directly drive a cylinder with either a gold (AU) or dichloropolystyrene (C6H8CL2) marker layer placed between a solid CH ablator and a foam cushion. When the cylinder is imploded the Richtmyer-Meshkov instability and convergence cause the marker layer to increase in thickness. Marker thickness measurements were made by x-ray backlighting along the cylinder axis. Experimental results of the effect of surface roughness will be presented. Computational results with an AMR code are in good agreement with the experimental results from targets with the roughest surface. Computational results suggest that marker layer 'end effects' and bowing increase the effective thickness of the marker layer at lower levels of roughness.

  3. The maturation of research into the avian hippocampal formation: Recent discoveries from one of the nature's foremost navigators.

    PubMed

    Herold, Christina; Coppola, Vincent J; Bingman, Verner P

    2015-11-01

    For more than 30 years, a growing number of researchers have been attracted to the challenge of understanding the neurobiological organization of the avian hippocampal formation (HF) and its relationship to the remarkable spatial cognitive abilities of birds. In this selective review, we highlight recent anatomical and developmental findings that reveal a HF design that defies any simple comparison to the mammalian hippocampus and leaves unanswered the seemingly enduring question of whether a dentate gyrus homologue is to be found in HF. From a functional perspective, we highlight the recent discoveries that implicate HF in the use of space for memory pattern segregation and continued interest in the role HF neurogenesis may play in supporting memory function and its relationship to memory decline in aging birds. We also summarize data that nurture a fundamental reinterpretation of the role of HF in spatial cognition by suggesting HF involvement in spatial perception antecedent to any memory formation. Given the disproportionate adaptive significance of space for birds, which has led to the evolution of their exceptional navigational and memory abilities, there is little doubt that the avian HF will continue to provide important and unexpected insights into the neural basis of spatial cognition. PMID:25850561

  4. Recent Selected Ion Flow Tube (SIFT) Studies Concerning the Formation of Amino Acids in the Gas Phase

    NASA Technical Reports Server (NTRS)

    Jackson, Douglas M.; Adams, Nigel G.; Babcock, Lucia M.

    2006-01-01

    Recently the simplest amino acid, glycine, has been detected in interstellar clouds, ISC, although this has since been contested. In order to substantiate either of these claims, plausible routes to amino acids need to be investigated. For gas phase synthesis, the SIFT technique has been employed to study simple amino acids via ion-molecule reactions of several ions of interstellar interest with methylamine, ethylamine, formic acid, acetic acid, and methyl formate. Carboxylic acid type ions were considered in the reactions involving the amines. In reactions where the carboxylic acid and methyl formate neutrals were studied, the reactant ions were primarily amine ion fragments. It was observed that the amines and acids preferentially fragment or accept a proton whenever energetically possible. NH3(+), however, uniquely reacted with the neutrals via atom abstraction to form NH4(+). These studies yielded a body of data relevant to astrochemistry, supplementing the available literature. However, the search for gas phase routes to amino acids using conventional molecules has been frustrated. Our most recent research investigates the fragmentation patterns of several amino acids and several possible routes have been suggested for future study.

  5. Microstructural Analysis of Irradiated U-Mo Fuel Plates: Recent Results

    SciTech Connect

    D. D. Keiser, Jr.; J. Jue; B. D. Miller; J. Gan; A. B. Robinson; P. V. Medvedev

    2012-03-01

    Microstructural characterization of irradiated dispersion and monolithic RERTR fuel plates using scanning electron microscopy (SEM) is being performed in the Electron Microscopy Laboratory at the Idaho National Laboratory. The SEM analysis of samples from U-Mo dispersion fuel plates focuses primarily on the behavior of the Si that has been added to the Al matrix to improve the irradiation performance of the fuel plate and on the overall behavior of fission gases (e.g., Xe and Kr) that develop as bubbles in the fuel microstructure. For monolithic fuel plates, microstructural features of interest, include those found in the U-Mo foil and at the U-Mo/Zr and Zr/6061 Al cladding interfaces. For both dispersion and monolithic fuel plates, samples have been produced using an SEM equipped with a Focused Ion Beam (FIB). These samples are of very high quality and can be used to uncover some very unique microstructural features that are typically not observed when characterizing samples produced using more conventional techniques. Overall, for the dispersion fuel plates with matrices that contained Si, narrower fuel/matrix interaction layers are typically observed compared to the fuel plates with pure Al matrix, and for the monolithic fuel plates microstructural features have been observed in the U-10Mo foil that are similar to what have been observed in the fuel particles found in U-Mo dispersion fuels. Most recently, more prototypic monolithic fuel samples have been characterized and this paper describes the microstructures that have been observed in these samples.

  6. Some recent results using spin echo resolved grazing incidence scattering (SERGIS)

    NASA Astrophysics Data System (ADS)

    Pynn, Roger; Ashkar, Rana; Stonaha, P.; Washington, A. L.

    2011-06-01

    The advantages of neutrons for probing bulk structures are well known: they provide statistically averaged correlation functions over a large range of length scales and they are sensitive to light atoms such as hydrogen. These same qualities are, in principle, useful in the study of surfaces and buried morphologies in thin films, especially when the films are polymeric or biological. However, because of the limited sample volume for such systems, the scattering is weak, especially if the neutron beam has to be severely collimated in order to resolve distances of interest (typically 10 to several 100 nm parallel to the surface of the sample). SERGIS is a technique that can potentially overcome these limitations by allowing high resolution measurements of lateral surface structure without requiring tight beam collimation. In this paper we discuss recent progress towards implementing SERGIS both at the Low Energy Neutron Source at Indiana University and on the Asterix reflectometer at the Los Alamos Neutron Science Center (LANSCE). The architecture we use exploits a robust symmetry-related cancellation of Larmor phase aberrations. The spatial resolution it achieves closely mimics that of the ideal magnetic Wollaston prisms. To make progress in understanding SERGIS, we have applied it to the measurement of simple diffraction gratings and developed a dynamical theory that accounts quantitatively and without adjustable parameters for all of the data sets we have measured to date. We argue here that, if SERGIS is to be applied to the study of weakly scattering thin films, it will be necessary to develop the technique of dark-field spin echo scattering angle measurement.

  7. Water in Star-forming Regions with Herschel (WISH): recent results and trends

    NASA Astrophysics Data System (ADS)

    van Dishoeck, E. F.

    2012-03-01

    Water is a key molecule in the physics and chemistry of star- and planet-forming regions. In the `Water in Star-forming Regions with Herschel' (WISH) Key Program, we have obtained a comprehensive set of water data toward a large sample of well-characterized protostars, covering a wide range of masses and luminosities --from the lowest to the highest mass protostars--, as well as evolutionary stages --from pre-stellar cores to disks. Lines of both ortho- and para-H_2O and their isotopologues, as well as chemically related hydrides, are observed with the HIFI and PACS instruments. The data elucidate the physical processes responsible for the warm gas, probe dynamical processes associated with forming stars and planets (outflow, infall, expansion), test basic chemical processes and reveal the chemical evolution of water and the oxygen-reservoir into planet-forming disks. In this brief talk a few recent WISH highlights will be presented, including determinations of the water abundance in each of the different physical components (inner and outer envelope, outflow) and constraints on the ortho/para ratio. Special attention will be given to trends found across the sample, especially the similarity in profiles from low to high-mass protostars and the evolution of the gas-phase water abundance from prestellar cores to disks. More details can be found at http://www.strw.leidenuniv.nl/WISH, whereas overviews are given in van Dishoeck et al. (2011, PASP 123, 138), Kristensen & van Dishoeck (2011, Astronomische Nachrichten 332, 475) and Bergin & van Dishoeck (2012, Phil. Trans. Royal Soc. A).

  8. Development and recent results from the Subaru coronagraphic extreme adaptive optics system

    NASA Astrophysics Data System (ADS)

    Jovanovic, N.; Guyon, O.; Martinache, F.; Clergeon, C.; Singh, G.; Kudo, T.; Newman, K.; Kuhn, J.; Serabyn, E.; Norris, B.; Tuthill, P.; Stewart, P.; Huby, E.; Perrin, G.; Lacour, S.; Vievard, S.; Murakami, N.; Fumika, O.; Minowa, Y.; Hayano, Y.; White, J.; Lai, O.; Marchis, F.; Duchene, G.; Kotani, T.; Woillez, J.

    2014-07-01

    The Subaru Coronagraphic Extreme Adaptive Optics (SCExAO) instrument is one of a handful of extreme adaptive optics systems set to come online in 2014. The extreme adaptive optics correction is realized by a combination of precise wavefront sensing via a non-modulated pyramid wavefront sensor and a 2000 element deformable mirror. This system has recently begun on-sky commissioning and was operated in closed loop for several minutes at a time with a loop speed of 800 Hz, on ~150 modes. Further suppression of quasi-static speckles is possible via a process called "speckle nulling" which can create a dark hole in a portion of the frame allowing for an enhancement in contrast, and has been successfully tested on-sky. In addition to the wavefront correction there are a suite of coronagraphs on board to null out the host star which include the phase induced amplitude apodization (PIAA), the vector vortex, 8 octant phase mask, 4 quadrant phase mask and shaped pupil versions which operate in the NIR (y-K bands). The PIAA and vector vortex will allow for high contrast imaging down to an angular separation of 1 λ/D to be reached; a factor of 3 closer in than other extreme AO systems. Making use of the left over visible light not used by the wavefront sensor is VAMPIRES and FIRST. These modules are based on aperture masking interferometry and allow for sub-diffraction limited imaging with moderate contrasts of ~100-1000:1. Both modules have undergone initial testing on-sky and are set to be fully commissioned by the end of 2014.

  9. RESULTS OF RECENT HIGH TEMPERATURE COELECTROLYSIS STUDIES AT THE IDAHO NATIONAL LABORATORY

    SciTech Connect

    Carl Stoots; James O'Brien; Joseph Hartvigsen

    2009-05-01

    Some results of CO2 / H2O electrolysis experiments performed to date using button cells and three different 10-cell planar solid oxide stacks are presented and discussed. These results include electrolysis performance at various temperatures, gas mixtures, and electrical settings. Product gas compositions, as measured via an in-line micro gas chromatograph (GC), are compared to predictions obtained from an INL-developed chemical equilibrium coelectrolysis model (CECM). Better understanding of the feasibility of producing syngas using high temperature electrolysis may initiate the systematic investigation of nuclear-powered synfuel production as a bridge to the future hydrogen economy and ultimate independence from foreign energy resources.

  10. Best Practices in Grid Integration of Variable Wind Power: Summary of Recent US Case Study Results and Mitigation Measures

    SciTech Connect

    Smith, J. Charles; Parsons, Brian; Acker, Thomas; Milligan, Michael; Zavidil, Robert; Schuerger, Matthew; DeMeo, Edgar

    2010-01-22

    This paper will summarize results from a number of utility wind integration case studies conducted recently in the US, and outline a number of mitigation measures based on insights from those studies.

  11. Implications of Bt Traits on Mycotoxin Contamination in Maize: Overview and Recent Experimental Results

    Technology Transfer Automated Retrieval System (TEKTRAN)

    Methods are becoming available to control mycotoxin-producing fungi in pre-harvest crops, including biocontrol and host plant resistance. While published reports since 1999 have associated Bt expression in corn with reduced mycotoxin levels, subsequent field results have been inconsistent. There i...

  12. Recent results for bonding S-65C grade Be to copper alloys

    SciTech Connect

    Dombrowski, D.W.

    1995-09-01

    Novel processes for bonding beryllium to copper alloys without the use of a silver bonding aid have been developed at Brush Wellman. Tensile strength results will be presented at room temperature and elevated temperatures. A comparison will be made between bond strengths derived from rectangular tensile specimens and reduced section tensile specimens. Failure modes of the specimens at various temperatures will be shown.

  13. Mammary carcinogenesis in rats: basic facts and recent results in Brookhaven

    SciTech Connect

    Shellabarger, C.J.; Stone, J.P.; Holtzman, s.

    1982-01-01

    Some research results from experiments investigating neutron-induced mammary carcinogenesis in rats are presented. The additive effects of neutrons and 3-methylcholanthrene on mammary adenocarcinoma were determined. Synergism between diethylstilbestrol and neutrons was likewise studied. Differences in mammary neoplastic response between strains of laboratory rats was also investigated. (ACR)

  14. Recent Simulation Results on Ring Current Dynamics Using the Comprehensive Ring Current Model

    NASA Technical Reports Server (NTRS)

    Zheng, Yihua; Zaharia, Sorin G.; Lui, Anthony T. Y.; Fok, Mei-Ching

    2010-01-01

    Plasma sheet conditions and electromagnetic field configurations are both crucial in determining ring current evolution and connection to the ionosphere. In this presentation, we investigate how different conditions of plasma sheet distribution affect ring current properties. Results include comparative studies in 1) varying the radial distance of the plasma sheet boundary; 2) varying local time distribution of the source population; 3) varying the source spectra. Our results show that a source located farther away leads to a stronger ring current than a source that is closer to the Earth. Local time distribution of the source plays an important role in determining both the radial and azimuthal (local time) location of the ring current peak pressure. We found that post-midnight source locations generally lead to a stronger ring current. This finding is in agreement with Lavraud et al.. However, our results do not exhibit any simple dependence of the local time distribution of the peak ring current (within the lower energy range) on the local time distribution of the source, as suggested by Lavraud et al. [2008]. In addition, we will show how different specifications of the magnetic field in the simulation domain affect ring current dynamics in reference to the 20 November 2007 storm, which include initial results on coupling the CRCM with a three-dimensional (3-D) plasma force balance code to achieve self-consistency in the magnetic field.

  15. Hadron distributions — Recent results from the CERN experiment NA44

    NASA Astrophysics Data System (ADS)

    Xu, Nu; Bearden, I. G.; Bøggild, H.; Boissevain, J.; Dodd, J.; Erazmus, B.; Esumi, S.; Fabjan, C. W.; Ferenc, D.; Fields, D. E.; Franz, A.; Gaardhøje, J. J.; Hansen, O.; Hardtke, D.; van Hecke, H.; Holzer, E. B.; Humanic, T.; Hummel, P.; Jacak, B. V.; Jayanti, R.; Kaneta, M.; Kopytine, M.; Leltchouk, M.; Ljubicic, T.; Lörstad, B.; Maeda, N.; Medvedev, A.; Murray, M.; Nishimura, S.; Ohnishi, H.; Paic, G.; Pandey, S. U.; Piuz, F.; Pluta, J.; Polychronakos, V.; Potekhin, M.; Poulard, G.; Sakaguchi, A.; Simon-Gillo, J.; Schmidt-Sørensen, J.; Sondheim, W.; Spegel, M.; Sugitate, T.; Sullivan, J. P.; Sumi, Y.; Willis, W. J.; Wolf, K.; Xu, N.; Zachary, D. S.; NA44 Collaboration

    1996-02-01

    Proton distributions at midrapidity have been measured for 158A·GeV Pb+Pb collisions in the focusing spectrometer experiment NA44 at CERN. A high degree of nuclear stopping is found in the truly heavy ion collisions. Systematic results of single particle transverse momentum distributions of pions, kaons, and protons, of 200A·GeV S+S and 158A·GeV Pb+Pb central collisions will be addressed within the context of thermalization. By comparing these data with thermal and transport models, freeze-out parameters such as the temperature parameter Tfo and mean collective flow velocity <β> are extracted. Preliminary results of the particle ratios of {K -}/{K +} and {overlinep}/{p} are discussed in the context of cascade models of RQMD and VENUS.

  16. Recent results on the nucleon resonance spectrum and structure from the CLAS detector

    NASA Astrophysics Data System (ADS)

    Mokeev, V. I.; Aznauryan, I. G.; Burkert, V. D.; Gothe, R. W.

    2016-03-01

    The CLAS detector at Jefferson Lab has provided the dominant part of all available worldwide data on exclusive meson electroproduction off protons in the resonance region. New results on the γυpN* transition amplitudes (electrocouplings) are available from analyses of the CLAS data and will be presented. Their impact on understanding of hadron structure will be discussed emphasizing the credible access to the dressed quark mass function that has been achieved for the first time by a combined analysis of the experimental results on the electromagnetic nucleon elastic and N → N* transition form factors. We will also discuss further convincing evidences for a new baryon state N' (1720)3/2+ found in a combined analysis of charged double pion photo- and electroproduction cross sections off the protons.

  17. Airborne Carbon Dioxide Laser Absorption Spectrometer for IPDA Measurements of Tropospheric CO2: Recent Results

    NASA Technical Reports Server (NTRS)

    Spiers, Gary D.; Menzies, Robert T.

    2008-01-01

    The National Research Council's decadal survey on Earth Science and Applications from Space[1] recommended the Active Sensing of CO2 Emissions over Nights, Days, and Seasons (ASCENDS) mission for launch in 2013-2016 as a logical follow-on to the Orbiting Carbon Observatory (OCO) which is scheduled for launch in late 2008 [2]. The use of a laser absorption measurement technique provides the required ability to make day and night measurements of CO2 over all latitudes and seasons. As a demonstrator for an approach to meeting the instrument needs for the ASCENDS mission we have developed the airborne Carbon Dioxide Laser Absorption Spectrometer (CO2LAS) which uses the Integrated Path Differential Absorption (IPDA) Spectrometer [3] technique operating in the 2 micron wavelength region.. During 2006 a short engineering checkout flight of the CO2LAS was conducted and the results presented previously [4]. Several short flight campaigns were conducted during 2007 and we report results from these campaigns.

  18. Recent Results on Two-Photon Physics at BaBar

    SciTech Connect

    Druzhinin, Vladimir P.; /Novosibirsk, IYF

    2011-12-02

    The authors present measurements of the {gamma}{gamma}* {yields} {pi}{sup 0} transition form factor for the momentum transfer range Q{sup 2} = 4-40 GeV{sup 2} and the {gamma}{gamma}* {yields} {eta}{sub c} transition form factor for the range Q{sup 2} = 2-50 GeV{sup 2}. The results of the measurement of the {eta}{sub c} mass, total and two-photon widths are also presented.

  19. High speed turboprops for executive aircraft, potential and recent test results

    NASA Technical Reports Server (NTRS)

    Mikkelson, D. C.; Mitchell, G. A.

    1980-01-01

    Four high speed propeller models were designed and tested in an 8x6 foot wind tunnel in order to evaluate the potential of advanced propeller technology. Results from these tests show that the combination of: increased blade number, aerodynamically integrated propeller/nacelles, reduced blade thickness, spinner area ruling, and blade sweep are important in achieving high propeller efficiency at the high cruise speeds.

  20. Recent results at the N = Z line with GASP and EUROBALL

    SciTech Connect

    Farnea, E.

    2004-02-27

    Valuable information on the validity of the isospin symmetry was obtained by studying nuclei close to the N = Z line with the GASP and EUROBALL {gamma}-ray spectrometres coupled to ancillary devices. Here a few selected results on the study of mirror nuclei are presented, together with an estimate of the isospin mixing probability through the measurement of a forbidden E1 transition in 64Ge.