National Library of Energy BETA

Sample records for type ii school

  1. n-Linear Algebra of type II

    E-Print Network [OSTI]

    W. B. Vasantha Kandasamy; Florentin Smarandache

    2009-02-01

    This book is a continuation of the book n-linear algebra of type I and its applications. Most of the properties that could not be derived or defined for n-linear algebra of type I is made possible in this new structure: n-linear algebra of type II which is introduced in this book. In case of n-linear algebra of type II we are in a position to define linear functionals which is one of the marked difference between the n-vector spaces of type I and II. However all the applications mentioned in n-linear algebras of type I can be appropriately extended to n-linear algebras of type II. Another use of n-linear algebra (n-vector spaces) of type II is that when this structure is used in coding theory we can have different types of codes built over different finite fields whereas this is not possible in the case of n-vector spaces of type I. Finally in the case of n-vector spaces of type II, we can obtain n-eigen values from distinct fields; hence, the n-characteristic polynomials formed in them are in distinct different fields. An attractive feature of this book is that the authors have suggested 120 problems for the reader to pursue in order to understand this new notion. This book has three chapters. In the first chapter the notion of n-vector spaces of type II are introduced. This chapter gives over 50 theorems. Chapter two introduces the notion of n-inner product vector spaces of type II, n-bilinear forms and n-linear functionals. The final chapter suggests over a hundred problems. It is important that the reader is well-versed not only with linear algebra but also n-linear algebra of type I.

  2. sessions II and High School

    E-Print Network [OSTI]

    Walker, Lawrence R.

    /high school certification. 20 Upper Division Biology Credits 06/12 MATH 95 Introductory Algebra Math Placement Testing ACT MATH 96 Intermediate Algebra Math Placement Testing ACT 20 SAT 500 MPT 12 UNLV; MATH 127 Precalculus I Math Placement Testing ACT 25 SAT 560 MPT 26 MATH 181 Calculus I Math Placement

  3. Type II Seesaw at LHC: the Roadmap

    E-Print Network [OSTI]

    Alejandra Melfo; Miha Nemevsek; Fabrizio Nesti; Goran Senjanovic; Yue Zhang

    2012-12-22

    In this Letter we revisit the type-II seesaw mechanism based on the addition of a weak triplet scalar to the standard model. We perform a comprehensive study of its phenomenology at the LHC energies, complete with the electroweak precision constraints. We pay special attention to the doubly-charged component, object of collider searches for a long time, and show how the experimental bound on its mass depends crucially on the particle spectrum of the theory. Our study can be used as a roadmap for future complete LHC studies.

  4. Type II Seesaw at LHC: the Roadmap

    E-Print Network [OSTI]

    Melfo, Alejandra; Nesti, Fabrizio; Senjanovic, Goran; Zhang, Yue

    2012-01-01

    In this Letter we revisit the type-II seesaw mechanism based on the addition of a weak triplet scalar to the standard model. We perform a comprehensive study of its phenomenology at the LHC energies, complete with the electroweak precision constraints. We pay special attention to the doubly-charged component, object of collider searches for a long time, and show how the experimental bound on its mass depends crucially on the particle spectrum of the theory. Our study can be used as a roadmap for future complete LHC studies.

  5. COLLOQUIUM: Type II Solar Radio Bursts: From Fundamental Plasma...

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    coherent radio emission stimulated by shocks. Type II bursts are widely accepted to be radio emission produced at the electron plasma frequency andor twice that frequency...

  6. Vortex pinning by inhomogeneities in type-II superconductors

    E-Print Network [OSTI]

    Chapman, Jon

    Vortex pinning by inhomogeneities in type-II superconductors S.J. Chapman #3;y G. Richardson zx of a curvilinear vortex in an inhomogeneous type-II superconducting material in the limit as the vortex core radius of the superconducting electrons acts as a pinning potential for the vortex, so that vortices will be attracted

  7. Serum markers for type II diabetes mellitus

    DOE Patents [OSTI]

    Metz, Thomas O; Qian, Wei-Jun; Jacobs, Jon M; Polpitiya, Ashoka D; Camp, II, David G; Smith, Richard D

    2014-03-18

    A method for identifying persons with increased risk of developing type 2 diabetes mellitus utilizing selected biomarkers described hereafter either alone or in combination. The present invention allows for broad based, reliable, screening of large population bases and provides other advantages, including the formulation of effective strategies for characterizing, archiving, and contrasting data from multiple sample types under varying conditions.

  8. BBF RFC 106: A Standard Type IIS Syntax for Plants

    E-Print Network [OSTI]

    Rutten, Virginia

    2015-03-17

    Here we define a standard syntax for assembling standard parts for expression in plant cells, extensible to all other eukaryotes. Variations of the Type IIS mediated cloning method known as Golden Gate Cloning, most notably ...

  9. Trace element geochemistry of ordinary chondrite chondrules: the type I/type II chondrule dichotomy

    E-Print Network [OSTI]

    Jacquet, Emmanuel; Gounelle, Matthieu

    2015-01-01

    We report trace element concentrations of silicate phases in chondrules from LL3 ordinary chondrites Bishunpur and Semarkona. Results are similar to previously reported data for carbonaceous chondrites, with rare earth element (REE) concentrations increasing in the sequence olivine ~ 10 K/h) than type I chondrules. Appreciable Na concentrations (3-221 ppm) are measured in olivine from both chondrule types; type II chondrules seem to have behaved as closed systems, which may require chondrule formation in the vicinity of protoplanets or planetesimals. At any rate, higher solid concentrations in type II chondrule forming regions may explain the higher oxygen fugacities they record compared to type I chondrules. Type I and type II chondrules formed in different environments and the correlation between high solid concentrations and/or oxygen fugacities with rapid cooling rates is a key constraint that chondrule formation models must account for.

  10. Future asymptotics of tilted Bianchi type II cosmologies

    E-Print Network [OSTI]

    Sigbjorn Hervik; Woei Chet Lim; Patrik Sandin; Claes Uggla

    2010-04-21

    In this paper we study the future asymptotics of spatially homogeneous Bianchi type II cosmologies with a tilted perfect fluid with a linear equation of state. By means of Hamiltonian methods we first find a monotone function for a special tilted case, which subsequently allows us to construct a new set of monotone functions for the general tilted type II cosmologies. In the context of a new partially gauge invariant dynamical system, this then leads to a proof for a theorem that for the first time gives a complete description of the future asymptotic states of the general tilted Bianchi type II models. The generality of our arguments suggests how one can produce monotone functions that are useful for determining the asymptotics of other tilted perfect fluid cosmologies, as well as for other sources.

  11. Comparing the host galaxies of type Ia, type II, and type Ibc supernovae

    SciTech Connect (OSTI)

    Shao, X.; Liang, Y. C.; Chen, X. Y.; Zhong, G. H.; Deng, L. C.; Zhang, B.; Shi, W. B.; Zhou, L. [Key Laboratory of Optical Astronomy, National Astronomical Observatories, Chinese Academy of Sciences, 20A Datun Road, Chaoyang District, Beijing 100012 (China); Dennefeld, M. [Institut d'Astrophysique de Paris, CNRS, and Universite P. et M. Curie, 98bis Bd Arago, F-75014 Paris (France); Hammer, F.; Flores, H., E-mail: xshao@bao.ac.cn, E-mail: ycliang@bao.ac.cn [GEPI, Observatoire de Paris-Meudon, F-92195 Meudon (France)

    2014-08-10

    We compare the host galaxies of 902 supernovae (SNe), including SNe Ia, SNe II, and SNe Ibc, which are selected by cross-matching the Asiago Supernova Catalog with the Sloan Digital Sky Survey (SDSS) Data Release 7. We selected an additional 213 galaxies by requiring the light fraction of spectral observations to be >15%, which could represent well the global properties of the galaxies. Among these 213 galaxies, 135 appear on the Baldwin-Phillips-Terlevich diagram, which allows us to compare the hosts in terms of whether they are star-forming (SF) galaxies, active galactic nuclei (AGNs; including composites, LINERs, and Seyfert 2s) or absorption-line galaxies (Absorps; i.e., their related emission lines are weak or non-existent). The diagrams related to the parameters D{sub n}(4000), H?{sub A}, stellar masses, star formation rates (SFRs), and specific SFRs for the SNe hosts show that almost all SNe II and most of the SNe Ibc occur in SF galaxies, which have a wide range of stellar masses and low D{sub n}(4000). The SNe Ia hosts as SF galaxies following similar trends. A significant fraction of SNe Ia occurs in AGNs and absorption-line galaxies, which are massive and have high D{sub n}(4000). The stellar population analysis from spectral synthesis fitting shows that the hosts of SNe II have a younger stellar population than hosts of SNe Ia. These results are compared with those of the 689 comparison galaxies where the SDSS fiber captures less than 15% of the total light. These comparison galaxies appear biased toward higher 12+log(O/H) (?0.1 dex) at a given stellar mass. Therefore, we believe the aperture effect should be kept in mind when the properties of the hosts for different types of SNe are discussed.

  12. -STABILITY AND VORTEX MOTION IN TYPE II SUPERCONDUCTORS

    E-Print Network [OSTI]

    Spirn, Daniel

    -STABILITY AND VORTEX MOTION IN TYPE II SUPERCONDUCTORS MATTHIAS KURZKE AND DANIEL SPIRN Abstract. 1. Introduction 1.1. Physical background. The evolution of a superconducting material is usu- ally of the magnetic field and the electric field potential for a superconducting sample R2 . The parameter

  13. Toroidal Magnetic Fields in Type II Superconducting Neutron Stars

    E-Print Network [OSTI]

    Taner Akgun; Ira Wasserman

    2007-11-01

    We determine constraints on the form of axisymmetric toroidal magnetic fields dictated by hydrostatic balance in a type II superconducting neutron star with a barotropic equation of state. Using Lagrangian perturbation theory, we find the quadrupolar distortions due to such fields for various models of neutron stars with type II superconducting and normal regions. We find that the star becomes prolate and can be sufficiently distorted to display precession with a period of the order of years. We also study the stability of such fields using an energy principle, which allows us to extend the stability criteria established by R. J. Tayler for normal conductors to more general media with magnetic free energy that depends on density and magnetic induction, such as type II superconductors. We also derive the growth rate and instability conditions for a specific instability of type II superconductors, first discussed by P. Muzikar, C. J. Pethick and P. H. Roberts, using a local analysis based on perturbations around a uniform background.

  14. Archived Reference Building Type: Primary school

    Broader source: Energy.gov [DOE]

    Here you will find past versions of the commercial reference building models for existing buildings constructed before 1980, organized by building type and location. A summary ofbuilding types and climate zones is available for reference. Current versions are also available.

  15. Archived Reference Building Type: Primary school

    Broader source: Energy.gov [DOE]

    Here you will find past versions of the commercial reference building models for existing buildings constructed in or after 1980, organized by building type and location. A summary of building types and climate zones is available for reference. Current versions are also available.

  16. Archived Reference Building Type: Secondary school

    Broader source: Energy.gov [DOE]

    Here you will find past versions of the commercial reference building models for existing buildings constructed before 1980, organized by building type and location. A summary ofbuilding types and climate zones is available for reference. Current versions are also available.

  17. Archived Reference Building Type: Secondary school

    Broader source: Energy.gov [DOE]

    Here you will find past versions of the commercial reference building models for existing buildings constructed in or after 1980, organized by building type and location. A summary of building types and climate zones is available for reference. Current versions are also available.

  18. Closed tachyon solitons in type II string theory

    E-Print Network [OSTI]

    Iñaki García-Etxebarria; Miguel Montero; Angel M. Uranga

    2015-05-20

    Type II theories can be described as the endpoint of closed string tachyon condensation in certain orbifolds of supercritical type 0 theories. In this paper, we study solitons of this closed string tachyon and analyze the nature of the resulting defects in critical type II theories. The solitons are classified by the real K-theory groups KO of bundles associated to pairs of supercritical dimensions. For real codimension 4 and 8, corresponding to $KO({\\bf S}^4)={\\bf Z}$ and $KO({\\bf S}^8)={\\bf Z}$, the defects correspond to a gravitational instanton and a fundamental string, respectively. We apply these ideas to reinterpret the worldsheet GLSM, regarded as a supercritical theory on the ambient toric space with closed tachyon condensation onto the CY hypersurface, and use it to describe charged solitons under discrete isometries. We also suggest the possible applications of supercritical strings to the physical interpretation of the matrix factorization description of F-theory on singular spaces.

  19. Reference Buildings by Building Type: Primary school

    Broader source: Energy.gov [DOE]

    In addition to the ZIP file for each building type, you can directly view the "scorecard" spreadsheet that summarizes the inputs and results for each location. This Microsoft Excel spreadsheet is also included in the ZIP file. For version 1.4, only the IDF file is included.

  20. Reference Buildings by Building Type: Secondary school

    Office of Energy Efficiency and Renewable Energy (EERE)

    In addition to the ZIP file for each building type, you can directly view the "scorecard" spreadsheet that summarizes the inputs and results for each location. This Microsoft Excel spreadsheet is also included in the ZIP file. For version 1.4, only the IDF file is included.

  1. Superspace with manifest T-duality from type II superstring

    E-Print Network [OSTI]

    Hatsuda, Machiko; Siegel, Warren

    2014-01-01

    A superspace formulation of type II superstring background with manifest T-duality symmetry is presented. This manifestly T-dual formulation is constructed in a space spanned by two sets of nondegenerate super-Poincare algebra. Supertorsion constraints are obtained from consistency of the kappa-symmetric Virasoro constraints. All superconnections and vielbein fields are solved in terms of a prepotential which is one of the vielbein components. AdS5xS5 background is explained in this formulation.

  2. Superspace with manifest T-duality from type II superstring

    E-Print Network [OSTI]

    Machiko Hatsuda; Kiyoshi Kamimura; Warren Siegel

    2014-05-08

    A superspace formulation of type II superstring background with manifest T-duality symmetry is presented. This manifestly T-dual formulation is constructed in a space spanned by two sets of nondegenerate super-Poincare algebra. Supertorsion constraints are obtained from consistency of the kappa-symmetric Virasoro constraints. All superconnections and vielbein fields are solved in terms of a prepotential which is one of the vielbein components. AdS5xS5 background is explained in this formulation.

  3. Type II and Type III Radio Bursts and their Correlation with Solar Energetic Proton Events

    E-Print Network [OSTI]

    Winter, L M

    2015-01-01

    Using the Wind/WAVES radio observations from 2010-2013, we present an analysis of the 123 decametric-hectometric (DH) type II solar radio bursts during this period, the associated type III burst properties, and their correlation with solar energetic proton (SEP) properties determined from analysis of the Geostationary Operational Environmental Satellite (GOES) observations. We present a useful catalog of the type II burst, type III burst, Langmuir wave, and proton flux properties for these 123 events, which we employ to develop a statistical relationship between the radio properties and peak proton flux that can be used to forecast SEP events. We find that all SEP events with a peak > 10 MeV flux above 15 pfu are associated with a type II burst and virtually all SEP events, 92%, are also associated with a type III radio burst. Based on a principal component analysis, the radio burst properties that are most highly correlated with the occurrence of gradual SEP events and account for the most variance in the ra...

  4. On the nature of rapidly fading Type II supernovae

    E-Print Network [OSTI]

    Moriya, Takashi J; Ergon, Mattias; Blinnikov, Sergei I

    2015-01-01

    It has been suggested that Type II supernovae with rapidly fading light curves (a.k.a. Type IIL supernovae) are explosions of progenitors with low-mass hydrogen-rich envelopes which are of the order of 1 Msun. We investigate light-curve properties of supernovae from such progenitors. We confirm that such progenitors lead to rapidly fading Type II supernovae. We find that the luminosity of supernovae from such progenitors with the canonical explosion energy of 1e51 erg and 56Ni mass of 0.05 Msun can increase temporarily shortly before all the hydrogen in the envelope recombines. As a result, a bump appears in their light curves. The bump appears because the heating from the nuclear decay of 56Ni can keep the bottom of hydrogen-rich layers in the ejecta ionized, and thus the photosphere can stay there for a while. We find that the light-curve bump becomes less significant when we make explosion energy larger (>~ 2e51 erg), 56Ni mass smaller (<~ 0.01 Msun), 56Ni mixed in the ejecta, or the progenitor radius l...

  5. Low Mach Number Modeling of Type Ia Supernovae. II. Energy Evolution

    E-Print Network [OSTI]

    Almgren, Ann S.; Bell, John B.; Rendleman, Charles A.; Zingale, Mike

    2006-01-01

    Number Modeling of Type Ia Supernovae. II. Energy EvolutionIa. Subject headings: supernovae: general — white dwarfs —the ignition of Type Ia supernovae (SNe Ia) is critical to

  6. Relativistic cyclotron resonance condition as applied to Type II interplanetary radio emission

    E-Print Network [OSTI]

    California at Berkeley, University of

    Relativistic cyclotron resonance condition as applied to Type II interplanetary radio emission W. M agreement in many areas including the prediction of ``Zeeman'' splitting of the Type II emission. Based on the character of the high-resolution emission spectrum, we can narrow the Type II source location to the IP

  7. Fermionic and Bosonic Stabilizing Effects for Type I and Type II Dimension Bubbles

    E-Print Network [OSTI]

    J. R. Morris

    2004-05-21

    We consider two types of "dimension bubbles", which are viewed as 4d nontopological solitons that emerge from a 5d theory with a compact extra dimension. The size of the extra dimension varies rapidly within the domain wall of the soliton. We consider the cases of type I (II) bubbles where the size of the extra dimension inside the bubble is much larger (smaller) than outside. Type I bubbles with thin domain walls can be stabilized by the entrapment of various particle modes whose masses become much smaller inside than outside the bubble. This is demonstrated here for the cases of scalar bosons, fermions, and massive vector bosons, including both Kaluza-Klein zero modes and Kaluza-Klein excitation modes. Type II bubbles expel massive particle modes but both types can be stabilized by photons. Plasma filled bubbles containing a variety of massless or nearly massless radiation modes may exist as long-lived metastable states. Furthermore, in contrast to the case with a "gravitational bag", the metric for a fluid-filled dimension bubble does not exhibit a naked singularity at the bubble's center.

  8. Type II superconductivity and magnetic flux transport in neutrons stars

    E-Print Network [OSTI]

    P. B. Jones

    2005-10-13

    The transition to a type II proton superconductor which is believed to occur in a cooling neutron star is accompanied by changes in the equation of hydrostatic equilibrium and by the formation of proton vortices with quantized magnetic flux. Analysis of the electron Boltzmann equation for this system and of the proton supercurrent distribution formed at the transition leads to the derivation of a simple expression for the transport velocity of magnetic flux in the liquid interior of a neutron star. This shows that flux moves easily as a consequence of the interaction between neutron and proton superfluid vortices during intervals of spin-down or spin-up in binary systems. The differences between the present analysis and those of previous workers are reviewed and an error in the paper of Jones (1991) is corrected.

  9. JOURNAL OF GEOPHYSICAL RESEARCH, VOL. ???, XXXX, DOI:10.1029/, Examination of Type II Origin with SOHO/LASCO

    E-Print Network [OSTI]

    JOURNAL OF GEOPHYSICAL RESEARCH, VOL. ???, XXXX, DOI:10.1029/, Examination of Type II Origin.-S. CHO ET AL.: EXAMINATION OF TYPE II ORIGIN Abstract. We examine a possibility that metric-type II solar radio bursts are all caused by CME generated shocks. For this we consider 129 type IIs- flare events

  10. Direct numerical simulations of type Ia supernovae flames II: The rayleigh-taylor instability

    E-Print Network [OSTI]

    Bell, J.B.; Day, M.S.; Rendleman, C.A.; Woosley, S.E.; Zingale, M.

    2004-01-01

    Weaver, T. A. 1994, in Supernovae, Les Houches, Session LIV,Simulations of Type Ia Supernovae Flames II: The Rayleigh-Subject headings: supernovae: general — white dwarfs —

  11. On the cosmic ray spectrum from type II Supernovae

    E-Print Network [OSTI]

    Cardillo, Martina; Blasi, Pasquale

    2015-01-01

    One of the most important challenges for the largely accepted idea that Galactic CRs are accelerated in SNR shocks is the maximum energy at which particles can be accelerated. The resonant streaming instability, long invoked for magnetic field amplification at shocks, can not provide sufficiently high fields and efficient enough scattering so as to ensure particle acceleration up to the knee. Here we discuss the non-resonant version of this instability which, with its faster growth and larger value of the amplified field, increases the achievable maximum energy. Because of their higher explosion rate, we focus on type II SNe expanding in their red supergiant wind and we find that the transition between Ejecta Dominated (ED) and Sedov-Taylor (ST) phases takes place at very early times. In this environment, the accelerated particle spectrum shows no high energy exponential cut-off but a spectral break at the maximum energy (EM). Moreover, the maximum energy of protons can easily reach PeV energies. With this mo...

  12. Smooth double critical state theory for type-II superconductors

    E-Print Network [OSTI]

    H. S. Ruiz; A. Bad\\'\\ia-Majós

    2010-05-30

    Several aspects of the general theory for the critical states of a vortex lattice and the magnetic flux dynamics in type-II superconductors are examined by a direct variational optimisation method and widespread physical principles. Our method allows to unify a number of conventional models describing the complex vortex configurations in the critical state regime. Special attention is given to the discussion of the relation between the flux-line cutting mechanism and the depinning threshold limitation. This is done by using a smooth double critical state concept which incorporates the so-called isotropic, elliptical, T and CT models as well-defined limits of our general treatment. Starting from different initial configurations for a superconducting slab in a 3D magnetic field, we show that the predictions of the theory range from the collapse to zero of transverse magnetic moments in the isotropic model, to nearly force free configurations in which paramagnetic values can arbitrarily increase with the applied field for magnetically anisotropic current voltage laws. Noteworthily, the differences between the several model predictions are minimal for the low applied field regime.

  13. LHC Phenomenology of Type II Seesaw: Nondegenerate Case

    E-Print Network [OSTI]

    Zhi-Long Han; Ran Ding; Yi Liao

    2015-04-29

    In this paper, we thoroughly investigate the LHC phenomenology of the type II seesaw mechanism for neutrino masses in the nondegenerate case where the triplet scalars of various charge ($H^{\\pm\\pm}, H^\\pm, H^0, A^0$) have different masses. Compared with the degenerate case, the cascade decays of scalars lead to many new, interesting signal channels. In the positive scenario where $M_{H^{\\pm\\pm}}sigma$ reach at 14 TeV LHC for $M_{H^{\\pm}}=430 GeV$ with $M_{H^{\\pm\\pm}}=400 GeV$ requires an integrated luminosity of 76/fb. And the six-lepton signal can be used to probe the neutral scalars $H^0/A^0$, which are usually hard to detect in the degenerate case. In the negative scenario where $M_{H^{\\pm\\pm}}>M_{H^\\pm}>M_{H^0/A^0}$, the detection of $H^{\\pm\\pm}$ is more challenging, when the cascade decay $H^{\\pm\\pm}\\to H^{\\pm}W^{\\pm*}$ is dominant. The most important channel is the associated $H^{\\pm}H^0/A^0$ production in the final state $\\ell^\\pm\\cancel{E}_Tb\\bar{b}b\\bar{b}$, which requires a luminosity of 109/fb for a $5\\sigma$ discovery, while the final state $\\ell^\\pm\\cancel{E}_Tb\\bar{b}\\tau^+\\tau^-$ is less promising. Moreover, the associated $H^0A^0$ production can give same signals as the standard model Higgs pair production. With a much larger cross section, the $H^0A^0$ production in the final state $b\\bar{b}\\tau^+\\tau^-$ could reach $3\\sigma$ significance at 14 TeV LHC with a luminosity of 300/fb. In summary, with an integrated luminosity of order 500/fb, the triplet scalars can be fully reconstructed at 14 TeV LHC in the negative scenario.

  14. Nucleosynthesis in the accretion disks of Type II collapsars

    E-Print Network [OSTI]

    Indrani Banerjee; Banibrata Mukhopadhyay

    2013-05-08

    We investigate nucleosynthesis inside the gamma-ray burst (GRB) accretion disks formed by the Type II collapsars. In these collapsars, the core collapse of massive stars first leads to the formation of a proto-neutron star and a mild supernova explosion is driven. However, this supernova ejecta lack momentum and falls back onto the neutron star which gets transformed to a stellar mass black hole. In order to study the hydrodynamics and nucleosynthesis of such an accretion disk formed from the fallback material of the supernova ejecta, we use the well established hydrodynamic models. In such a disk neutrino cooling becomes important in the inner disk where the temperature and density are higher. Higher the accretion rate (dot{M}), higher is the density and temperature in the disks. In this work we deal with accretion disks with relatively low accretion rates: 0.001 M_sun s^{-1} \\lesssim dot{M} \\lesssim 0.01 M_sun s^{-1} and hence these disks are predominantly advection dominated. We use He-rich and Si-rich abundances as the initial condition of nucleosynthesis at the outer disk, and being equipped with the disk hydrodynamics and the nuclear network code, we study the abundance evolution as matter inflows and falls into the central object. We investigate the variation in the nucleosynthesis products in the disk with the change in the initial abundance at the outer disk and also with the change in the mass accretion rate. We report the synthesis of several unusual nuclei like {31}P, {39}K, {43}Sc, {35}Cl, and various isotopes of titanium, vanadium, chromium, manganese and copper. We also confirm that isotopes of iron, cobalt, nickel, argon, calcium, sulphur and silicon get synthesized in the disk, as shown by previous authors. Much of these heavy elements thus synthesized are ejected from the disk via outflows and hence they should leave their signature in observed data.

  15. SMOOTH TYPE II BLOW UP SOLUTIONS TO THE FOUR DIMENSIONAL ENERGY CRITICAL WAVE EQUATION

    E-Print Network [OSTI]

    Raphaël, Pierre

    SMOOTH TYPE II BLOW UP SOLUTIONS TO THE FOUR DIMENSIONAL ENERGY CRITICAL WAVE EQUATION MATTHIEU HILLAIRET AND PIERRE RAPHA¨EL Abstract. We exhibit C type II blow up solutions to the focusing energy critical wave equation in dimension N = 4. These solutions admit near blow up time a decomposiiton u(t, x

  16. Numerical Relaxation Approach for Solving the General Ginzburg-Landau Equations for Type-Ii Superconductors 

    E-Print Network [OSTI]

    WANG, ZD; Hu, Chia-Ren.

    1991-01-01

    A numerical relaxation approach for solving the general Ginzburg-Landau equations for type-II superconductors is developed. It is first applied to an isotropic type-II superconductor near H(c1) in order to establish the reliability and effectiveness...

  17. GaSb/GaAs type II quantum dot solar cells for enhanced infrared spectral response

    E-Print Network [OSTI]

    Jalali. Bahram

    into existing multijunction cells either as a means to increase the current or efficiency by using low band gapGaSb/GaAs type II quantum dot solar cells for enhanced infrared spectral response R. B infrared spectral response of GaAs-based solar cells that incorporate type II GaSb quantum dots QDs formed

  18. Kinematics of ICMEs/shocks: blast wave reconstruction using type II emissions

    E-Print Network [OSTI]

    Corona-Romero, P; Aguilar-Rodriguez, E; de-la-Luz, V; Mejia-Ambriz, J C

    2015-01-01

    We present a physical methodology to reconstruct the trajectory of interplanetary shocks using type II radio emission data. This technique calculates the shock trajectory assuming that the disturbance propagates as a blast wave in the interplanetary medium. We applied this Blast Wave Reconstruction (BWR) technique to analyze eight fast Earth-directed ICMEs/shocks associated with type II emissions. The technique deduces a shock trajectory that reproduces the type II frequency drifts, and calculates shock onset speed, shock transit time and shock speed at 1~AU. There were good agreements comparing the BWR results with the type II spectra, with data from coronagraph images, {\\it in situ} measurements, and interplanetary scintillation (IPS) observations. Perturbations on the type II data affect the accuracy of the BWR technique. This methodology could be applied to track interplanetary shocks causing TII emissions in real-time, to predict the shock arrival time and shock speed at 1~AU.

  19. EnergySmart Schools National Financing Roundtable II - Key Outcomes

    SciTech Connect (OSTI)

    2009-12-01

    This document summarizes the discussion at the Financing Roundtable. It provides an overview of the financing opportunities, challenges, and activities involved in achieving high performance schools, as identified by the participants.

  20. A population study of type II bursts in the Rapid Burster

    E-Print Network [OSTI]

    Bagnoli, T; D'Angelo, C R; Galloway, D K

    2015-01-01

    Type II bursts are thought to arise from instabilities in the accretion flow onto a neutron star in an X-ray binary. Despite having been known for almost 40 years, no model can yet satisfactorily account for all their properties. To shed light on the nature of this phenomenon and provide a reference for future theoretical work, we study the entire sample of Rossi X-ray Timing Explorer data of type II bursts from the Rapid Burster (MXB 1730-335). We find that type II bursts are Eddington-limited in flux, that a larger amount of energy goes in the bursts than in the persistent emission, that type II bursts can be as short as 0.130 s, and that the distribution of recurrence times drops abruptly below 15-18 s. We highlight the complicated feedback between type II bursts and the NS surface thermonuclear explosions known as type I bursts, and between type II bursts and the persistent emission. We review a number of models for type II bursts. While no model can reproduce all the observed burst properties and explain...

  1. Ruptured Aortic Aneurysm From Late Type II Endoleak Treated by Transarterial Embolization

    SciTech Connect (OSTI)

    Gunasekaran, Senthil; Funaki, Brian Lorenz, Jonathan

    2013-02-15

    Endoleak is the most common complication after endovascular aneurysm repair. The most common type of endoleak, a type II endoleak, typically follows a benign course and is only treated when associated with increasing aneurysm size. In this case report, we describe a ruptured abdominal aortic aneurysm due to a late, type II endoleak occurring 10 years after endovascular aneurysm repair that was successfully treated by transarterial embolization.

  2. AC losses in type-II superconductors induced by nonuniform fluctuations of external magnetic field

    E-Print Network [OSTI]

    as the economic gains of implementation of type-II superconductors in power transmission lines, current leads amplitude. The results can be used to estimate the AC losses in flywheels, electric motors, magnetic shields

  3. Supernova progenitor constraints from circumstellar interaction: Type II

    E-Print Network [OSTI]

    Robert J. Cumming; Peter Lundqvist

    1996-10-03

    All types of supernovae (SNe), except Type Ia, have been observed to interact with their immediate circumstellar medium (CSM). This interaction can reveal their progenitor's histories, and constrain our ideas about the evolution of massive stars. As examples of the latest progress in this areas, we present some new results on two SNe: a 3D picture of the triple-ring nebula around SN 1987A, and observations of the less well-known but rather intriguing SN 1994W. In the process we introduce Type IIn supernovae (SN IIn; Schlegel 1990) as an important new probe of massive star evolution.

  4. The effective action of type II Calabi-Yau orientifolds

    E-Print Network [OSTI]

    Thomas W. Grimm

    2007-04-18

    This article first reviews the calculation of the N = 1 effective action for generic type IIA and type IIB Calabi-Yau orientifolds in the presence of background fluxes by using a Kaluza-Klein reduction. The Kahler potential, the gauge kinetic functions and the flux-induced superpotential are determined in terms of geometrical data of the Calabi-Yau orientifold and the background fluxes. As a new result, it is shown that the chiral description directly relates to Hitchin's generalized geometry encoded by special odd and even forms on a threefold, whereas a dual formulation with several linear multiplets makes contact to the underlying N = 2 special geometry. In type IIB setups, the flux-potentials can be expressed in terms of superpotentials, D-terms and, generically, a massive linear multiplet. The type IIA superpotential depends on all geometric moduli of the theory. It is reviewed, how type IIA orientifolds arise as a special limit of M-theory compactified on specific G_2 manifolds by matching the effective actions. In a similar spirit type IIB orientifolds are shown to descend from F-theory on a specific class of Calabi-Yau fourfolds. In addition, mirror symmetry for Calabi-Yau orientifolds is briefly discussed and it is shown that the N = 1 chiral coordinates linearize the appropriate instanton actions.

  5. Generation of polarization-entangled photons using type-II doubly periodically poled lithium niobate waveguides

    E-Print Network [OSTI]

    Boyer, Edmond

    Generation of polarization-entangled photons using type-II doubly periodically poled lithium the issue of the generation of non-degenerate cross-polarization-entangled photon pairs using type-conversion processes, namely ordinary pump photon down- conversion to either extraordinary signal and ordinary idler

  6. Exact Inference for the Two-Parameter Exponential Distribution Under Type-II

    E-Print Network [OSTI]

    Kundu, Debasis

    censoring; two-parameter exponential distribution; joint moment generating function; maximum likelihood is fixed, but the number of failures is random, whereas Part of this work has been supported by grants is random but the number of failures is fixed. A mixture of Type-I and Type-II censoring scheme is known

  7. DIAGNOSTICS ON THE SOURCE PROPERTIES OF A TYPE II RADIO BURST WITH SPECTRAL BUMPS

    SciTech Connect (OSTI)

    Feng, S. W.; Chen, Y.; Kong, X. L.; Li, G.; Song, H. Q. [Institute of Space Sciences and School of Space Science and Physics, Shandong University, Weihai 264209 (China)] [Institute of Space Sciences and School of Space Science and Physics, Shandong University, Weihai 264209 (China); Feng, X. S. [SIGMA Weather Group, State Key laboratory for Space Weather, Center for Space Science and Applied Research, Chinese Academy of Sciences, Beijing 100190 (China)] [SIGMA Weather Group, State Key laboratory for Space Weather, Center for Space Science and Applied Research, Chinese Academy of Sciences, Beijing 100190 (China); Guo, Fan, E-mail: yaochen@sdu.edu.cn [Department of Planetary Sciences and Lunar and Planetary laboratory, University of Arizona, Tucson, AZ 85721 (United States)] [Department of Planetary Sciences and Lunar and Planetary laboratory, University of Arizona, Tucson, AZ 85721 (United States)

    2013-04-10

    In recent studies, we proposed that source properties of type II radio bursts can be inferred through a causal relationship between the special shape of the type II dynamic spectrum (e.g., bump or break) and simultaneous extreme ultraviolet (EUV)/white light imaging observations (e.g., CME-shock crossing streamer structures). As a further extension of these studies, in this paper we examine the coronal mass ejection (CME) event on 2007 December 31 associated with a multiple type II radio burst. We identify the presence of two spectral bump features on the observed dynamic spectrum. By combining observational analyses of the radio spectral observations and the EUV-white light imaging data, we conclude that the two spectral bumps result from a CME-shock propagating across dense streamers on the southern and northern sides of the CME. It is inferred that the corresponding two type II emissions originate separately from the two CME-shock flanks where the shock geometries are likely quasi-perpendicular or oblique. Since the emission lanes are bumped as a whole within a relatively short time, it suggests that the type II radio bursts with bumps of this study are emitted from spatially confined sources (with a projected lateral dimension smaller than 0.05-0.1 R{sub Sun} at a fundamental frequency level of 20-30 MHz).

  8. Archive Reference Buildings by Building Type: Primary school

    Broader source: Energy.gov [DOE]

    Here you will find past versions of the reference buildings for new construction commercial buildings, organized by building type and location. A summary of building types and climate zones is...

  9. Archive Reference Buildings by Building Type: Secondary school

    Broader source: Energy.gov [DOE]

    Here you will find past versions of the reference buildings for new construction commercial buildings, organized by building type and location. A summary of building types and climate zones is...

  10. Neutrinoless Double Beta Decay in Type I+II Seesaw Models

    E-Print Network [OSTI]

    Debasish Borah; Arnab Dasgupta

    2015-09-06

    We study neutrinoless double beta decay in left-right symmetric extension of the standard model with type I and type II seesaw origin of neutrino masses. Due to the enhanced gauge symmetry as well as extended scalar sector, there are several new physics sources of neutrinoless double beta decay in this model. Ignoring the left-right gauge boson mixing and heavy-light neutrino mixing, we first compute the contributions to neutrinoless double beta decay for type I and type II dominant seesaw separately and compare with the standard light neutrino contributions. We then repeat the exercise by considering the presence of both type I and type II seesaw, having non-negligible contributions to light neutrino masses and show the difference in results from individual seesaw cases. Assuming the new gauge bosons and scalars to be around a TeV, we constrain different parameters of the model including both heavy and light neutrino masses from the requirement of keeping the neutrinoless double beta decay amplitude below the upper limit set by the GERDA experiment.

  11. Neutrinoless Double Beta Decay in Type I+II Seesaw Models

    E-Print Network [OSTI]

    Borah, Debasish

    2015-01-01

    We study neutrinoless double beta decay in left-right symmetric extension of the standard model with type I and type II seesaw origin of neutrino masses. Due to the enhanced gauge symmetry as well as extended scalar sector, there are several new physics sources of neutrinoless double beta decay in this model. Ignoring the left-right gauge boson mixing and heavy-light neutrino mixing, we first compute the contributions to neutrinoless double beta decay for type I and type II dominant seesaw separately and compare with the standard light neutrino contributions. We then repeat the exercise by considering the presence of both type I and type II seesaw, having non-negligible contributions to light neutrino masses and show the difference in results from individual seesaw cases. Assuming the new gauge bosons and scalars to be around a TeV, we constrain different parameters of the model including both heavy and light neutrino masses from the requirement of keeping the neutrinoless double beta decay amplitude below th...

  12. In Situ Observation of Type II Solar Radio Burst Source Region: a New Generation Mechanism

    E-Print Network [OSTI]

    mechanisms: non-thermal -- shock waves -- Sun: radio radiation 1. Introduction Electromagnetic waves can by Cluster spacecraft (Escoubet et al. 1997). We observe intense radio waves above the local plasma frequencyIn Situ Observation of Type II Solar Radio Burst Source Region: a New Generation Mechanism M. V

  13. Analysis of Impossible, Integral and Zero-Correlation Attacks on Type-II Generalized

    E-Print Network [OSTI]

    International Association for Cryptologic Research (IACR)

    Analysis of Impossible, Integral and Zero-Correlation Attacks on Type-II Generalized Feistel-correlation distinguishers as well as between zero-correlation and integral distinguishers, we analyze in this paper some of the round function, we show that we can not only find impossible, integral and multidimensional zero

  14. Purification, crystallization and preliminary X-ray diffraction studies of retinal dehydrogenase type II

    E-Print Network [OSTI]

    Lamb, Audrey Lee; Wang, Xianshu; Napoli, Joseph L.; Newcomer, Marcia E.

    1998-07-01

    One enzyme which catalyzes the last step of the formation of the hormone retinoic acid from vitamin A (retinol) is retinal dehydrogenase type II (RalDH2). RalDH2, expressed in the Escherichia coli BL21(DE3) strain, was purified and crystallized...

  15. Bulk superconductivity in Type II superconductors near the second critical field

    E-Print Network [OSTI]

    S. Fournais; B. Helffer

    2008-02-14

    We consider superconductors of Type II near the transition from the 'bulk superconducting' to the 'surface superconducting' state. We prove a new $L^{\\infty}$ estimate on the order parameter in the bulk, i.e. away from the boundary. This solves an open problem posed by Aftalion and Serfaty.

  16. Parametric spatial solitary waves due to type II second-harmonic generation

    E-Print Network [OSTI]

    Parametric spatial solitary waves due to type II second-harmonic generation Alexander V. Buryak either 1 or 2 is generated). A particular case of this three-wave interaction, formally described analyze (1 1)- and (2 1)-dimensional self-guided beams (spatial solitons) due to three-wave para- metric

  17. Best Entry Points for Structured Document Retrieval Part II: Types, Usage and Effectiveness

    E-Print Network [OSTI]

    Lalmas, Mounia

    Best Entry Points for Structured Document Retrieval ­ Part II: Types, Usage and Effectiveness Jane documents. This paper examines the concept of best entry points, which are document components from which of best entry points in structured document retrieval, and their usage and effectiveness in real

  18. The importance of 56Ni in shaping the light curves of type II supernovae

    E-Print Network [OSTI]

    Nakar, Ehud; Katz, Boaz

    2015-01-01

    What intrinsic properties shape the light curves of Type II supernovae (SNe)? To address this question we derive observational measures that are robust (i.e., insensitive to detailed radiative transfer) and constrain the contribution from 56Ni, as well as a combination of the ejecta mass, progenitor radius, and explosion energy. By applying our methods to a sample of type II SNe from the literature we find that 56Ni contribution is often significant. It is typically the source of about 20% of the radiated energy during the photospheric phase, and in extreme cases it even dominates. We find that the 56Ni relative contribution is anti-correlated with the luminosity decline rate, while it is not significantly correlated with other properties of the light curve. When added to other clues, this in turn suggests that the flat plateaus often observed in type II SNe are not a generic feature of the cooling envelope emission, and that without 56Ni many of the SNe that are classified as II-P would have shown a decline ...

  19. Characterizing the V-band light-curves of hydrogen-rich type II supernovae

    SciTech Connect (OSTI)

    Anderson, Joseph P.; González-Gaitán, Santiago; Hamuy, Mario; Gutiérrez, Claudia P.; Antezana, Roberto; De Jaeger, Thomas; Förster, Francisco; González, Luis [Departamento de Astronomía, Universidad de Chile, Casilla 36-D, Santiago (Chile); Stritzinger, Maximilian D.; Contreras, Carlos [Department of Physics and Astronomy, Aarhus University, Ny Munkegade 120, DK-8000 Aarhus C (Denmark); Olivares E, Felipe [Departamento de Ciencias Fisicas, Universidad Andres Bello, Avda. Republica 252, Santiago (Chile); Phillips, Mark M.; Campillay, Abdo; Castellón, Sergio; Hsiao, Eric [Carnegie Observatories, Las Campanas Observatory, Casilla 601, La Serena (Chile); Schulze, Steve [Instituto de Astrofísica, Facultad de Física, Pontifícia Universidad Católica de Chile, Casilla 306, Santiago 22 (Chile); Bolt, Luis [Argelander Institut für Astronomie, Universität Bonn, Auf dem Hügel 71, D-53111 Bonn (Germany); Folatelli, Gastón [Institute for the Physics and Mathematics of the Universe (IPMU), University of Tokyo, 5-1-5 Kashiwanoha, Kashiwa, Chiba 277-8583 (Japan); Freedman, Wendy L. [Observatories of the Carnegie Institution for Science, Pasadena, CA 91101 (United States); Krzemi?ski, Wojtek, E-mail: janderso@eso.org [N. Copernicus Astronomical Center, ul. Bartycka 18, 00-716 Warszawa (Poland); and others

    2014-05-01

    We present an analysis of the diversity of V-band light-curves of hydrogen-rich type II supernovae. Analyzing a sample of 116 supernovae, several magnitude measurements are defined, together with decline rates at different epochs, and time durations of different phases. It is found that magnitudes measured at maximum light correlate more strongly with decline rates than those measured at other epochs: brighter supernovae at maximum generally have faster declining light-curves at all epochs. We find a relation between the decline rate during the 'plateau' phase and peak magnitudes, which has a dispersion of 0.56 mag, offering the prospect of using type II supernovae as purely photometric distance indicators. Our analysis suggests that the type II population spans a continuum from low-luminosity events which have flat light-curves during the 'plateau' stage, through to the brightest events which decline much faster. A large range in optically thick phase durations is observed, implying a range in progenitor envelope masses at the epoch of explosion. During the radioactive tails, we find many supernovae with faster declining light-curves than expected from full trapping of radioactive emission, implying low mass ejecta. It is suggested that the main driver of light-curve diversity is the extent of hydrogen envelopes retained before explosion. Finally, a new classification scheme is introduced where hydrogen-rich events are typed as simply 'SN II' with an 's {sub 2}' value giving the decline rate during the 'plateau' phase, indicating its morphological type.

  20. Photospheric magnitude diagrams for type II supernovat: A promising tool to compute distances

    SciTech Connect (OSTI)

    Rodríguez, Ósmar; Clocchiatti, Alejandro; Hamuy, Mario, E-mail: olrodrig@astro.puc.cl [Millennium Institute of Astrophysics, Casilla 36-D, Santiago (Chile)

    2014-12-01

    We develop an empirical color-based standardization for Type II supernovae (SNe II), equivalent to the classical surface brightness method given in Wesselink. We calibrate this standardization using SNe II with host galaxy distances measured using Cepheids, and a well-constrained shock breakout epoch and extinction due to the host galaxy. We estimate the reddening with an analysis of the B – V versus V – I color-color curves, similar to that of Natali et al. With four SNe II meeting the above requirements, we build a photospheric magnitude versus color diagram (similar to an H-R diagram) with a dispersion of 0.29 mag. We also show that when using time since shock breakout instead of color as the independent variable, the same standardization gives a dispersion of 0.09 mag. Moreover, we show that the above time-based standardization corresponds to the generalization of the standardized candle method of Hamuy and Pinto for various epochs throughout the photospheric phase. To test the new tool, we construct Hubble diagrams for different subsamples of 50 low-redshift (cz < 10{sup 4} km s{sup –1}) SNe II. For 13 SNe within the Hubble flow (cz {sub CMB} > 3000 km s{sup –1}) and with a well-constrained shock breakout epoch we obtain values of 68-69 km s{sup –1} Mpc{sup –1} for the Hubble constant and a mean intrinsic scatter of 0.12 mag or 6% in relative distances.

  1. An observational revisit of band-split solar type-II radio bursts

    E-Print Network [OSTI]

    Du, Guohui; Chen, Yao; Feng, Shiwei; Wang, Bing; Li, Gang

    2015-01-01

    Band split of solar type II radio bursts, discovered several decades ago, is a fascinating phenomenon with the type-II lanes exhibiting two almost-parallel sub-bands with similar morphology. The underlying split mechanism remains elusive. One popular interpretation is that the splitting bands are emitted from the shock upstream and downstream, respectively, with their frequency ratio ({\\gamma}) determined by the shock compression ratio. This interpretation has been taken as the physical basis for many published references. Here we report an observational analysis of type II events with nice split selected from the ground-based RSTN data from 2001 to 2014, in the metric-decametric wavelength. We investigate the temporal variation and distribution of {\\gamma}, and conduct correlation analyses on the deduced spectral values. It is found that {\\gamma} varies in a very narrow range with >80% of {\\gamma} (one-minute averaged data) being between 1.15 to 1.25. For some well-observed and long-lasting events, {\\gamma} ...

  2. H{sub ?} SPECTRAL DIVERSITY OF TYPE II SUPERNOVAE: CORRELATIONS WITH PHOTOMETRIC PROPERTIES

    SciTech Connect (OSTI)

    Gutiérrez, Claudia P.; Hamuy, Mario; González-Gaitán, Santiago [Millennium Institute of Astrophysics, Casilla 36-D, Santiago (Chile); Anderson, Joseph P. [Departamento de Astronomía, Universidad de Chile, Casilla 36-D, Santiago (Chile); Folatelli, Gastón [Institute for the Physics and Mathematics of the Universe (IPMU), University of Tokyo, 5-1-5 Kashiwanoha, Kashiwa, Chiba 277-8583 (Japan); Morrell, Nidia I.; Phillips, Mark M.; Thomas-Osip, Joanna [Carnegie Observatories, Las Campanas Observatory, Casilla 601, La Serena (Chile); Stritzinger, Maximilian D. [Department of Physics and Astronomy, Aarhus University, Ny Munkegade 120, DK-8000 Aarhus C (Denmark); McCarthy, Patrick [Observatories of the Carnegie Institution for Science, Pasadena, CA 91101 (United States); Suntzeff, Nicholas B., E-mail: cgutierr@das.uchile.cl [George P. and Cynthia Woods Mitchell Institute for Fundamental Physics and Astronomy, Department of Physics and Astronomy, Texas A and M University, College Station, TX 77843 (United States)

    2014-05-10

    We present a spectroscopic analysis of the H{sub ?} profiles of hydrogen-rich Type II supernovae. A total of 52 Type II supernovae having well-sampled optical light curves and spectral sequences were analyzed. Concentrating on the H{sub ?} P-Cygni profile we measure its velocity from the FWHM of the emission and the ratio of absorption to emission (a/e) at a common epoch at the start of the recombination phase, and search for correlations between these spectral parameters and photometric properties of the V-band light curves. Testing the strength of various correlations we find that a/e appears to be the dominant spectral parameter in terms of describing the diversity in our measured supernova properties. It is found that supernovae with smaller a/e have higher H{sub ?} velocities, more rapidly declining light curves from maximum during the plateau and radioactive tail phase, are brighter at maximum light, and have shorter optically thick phase durations. We discuss possible explanations of these results in terms of physical properties of Type II supernovae, speculating that the most likely parameters that influence the morphologies of H{sub ?} profiles are the mass and density profile of the hydrogen envelope, together with additional emission components due to circumstellar interaction.

  3. Type II supernova energetics and comparison of light curves to shock-cooling models

    E-Print Network [OSTI]

    Rubin, Adam; De Cia, Annalisa; Horesh, Assaf; Khazov, Danny; Ofek, Eran O; Kulkarni, S R; Arcavi, Iair; Manulis, Ilan; Yaron, Ofer; Vreeswijk, Paul; Kasliwal, Mansi M; Ben-Ami, Sagi; Perley, Daniel A; Cao, Yi; Cenko, S Bradley; Rebbapragada, Umaa D; Wo?niak, P R; Filippenko, Alexei V; Clubb, K I; Nugent, Peter E; Pan, Y -C; Badenes, C; Howell, D Andrew; Valenti, Stefano; Sand, David; Sollerman, J; Johansson, Joel; Leonard, Douglas C; Horst, J Chuck; Armen, Stephen F; Fedrow, Joseph M; Quimby, Robert M; Mazzali, Paulo; Pian, Elena; Sternberg, Assaf; Matheson, Thomas; Sullivan, M; Maguire, K; Lazarevic, Sanja

    2015-01-01

    During the first few days after explosion, Type II supernovae (SNe) are dominated by relatively simple physics. Theoretical predictions regarding early-time SN light curves in the ultraviolet (UV) and optical bands are thus quite robust. We present, for the first time, a sample of $57$ $R$-band Type II SN light curves that are well monitored during their rise, having $>5$ detections during the first 10 days after discovery, and a well-constrained time of explosion to within $1-3$ days. We show that the energy per unit mass ($E/M$) can be deduced to roughly a factor of five by comparing early-time optical data to the model of Rabinak & Waxman (2011), while the progenitor radius cannot be determined based on $R$-band data alone. We find that Type II SN explosion energies span a range of $E/M=(0.2-20)\\times 10^{51} \\; \\rm{erg/(10 M}_\\odot$), and have a mean energy per unit mass of $\\left\\langle E/M \\right\\rangle = 0.85\\times 10^{51} \\; \\rm{erg/(10 M}_\\odot$), corrected for Malmquist bias. Assuming a small sp...

  4. Structure of the minor pseudopilin XcpW from the Pseudomonas aeruginosa type II secretion system

    SciTech Connect (OSTI)

    Franz, Laura P.; Douzi, Badreddine; Durand, Eric; Dyer, David H.; Voulhouxd, Romé; Forest, Katrina T.

    2012-01-13

    Pseudomonas aeruginosa utilizes the type II secretion machinery to transport virulence factors through the outer membrane into the extracellular space. Five proteins in the type II secretion system share sequence homology with pilin subunits of type IV pili and are called the pseudopilins. The major pseudopilin X{sub cp}T{sub G} assembles into an intraperiplasmic pilus and is thought to act in a piston-like manner to push substrates through an outer membrane secretin. The other four minor pseudopilins, X{sub cp}U{sub H}, X{sub cp}V{sub I}, X{sub cp}W{sub J} and X{sub cp}X{sub K}, play less well defined roles in pseudopilus formation. It was recently discovered that these four minor pseudopilins form a quaternary complex that is presumed to initiate the formation of the pseudopilus and to localize to its tip. Here, the structure of X{sub cp}W{sub J} was refined to 1.85 {angstrom} resolution. The structure revealed the type IVa pilin fold with an embellished variable antiparallel {beta}-sheet as also found in the X{sub cp}W{sub J} homologue enterotoxigenic Escherichia coli G{sub sp}J{sub W} and the X{sub cp}U{sub H} homologue Vibrio cholerae E{sub ps}U{sub H}. It is proposed that the exposed surface of this sheet may cradle the long N-terminal 1 helix of another pseudopilin. The final 31 amino acids of the X{sub cp}W{sub J} structure are instrinsically disordered. Deletion of this unstructured region of X{sub cp}W{sub J} did not prevent type II secretion in vivo.

  5. TEST & EVALUATION REPORT FOR THE HEDGEHOG-II PACKAGING SYSTEMS DOT-7A TYPE A CONTAINER

    SciTech Connect (OSTI)

    KELLY, D.L.

    2003-12-29

    This report documents the US. Department of Transportation Specification 7A (DOT-7A) Type A compliance test and evaluation results for the Hedgehog-II packaging systems. The approved Hedgehog-II packaging configurations provide primary and secondary containment. The approved packaging configurations described within this report are designed to ship Type A quantities of radioactive materials, normal form. Contents may be in solid or liquid form. Liquids transported in the approved 1 L glass bottle assembly shall have a specific gravity of less than or equal to 1.6. Liquids transported in all other approved configurations shall have a specific gravity of less than or equal to 2.0. The solid contents, including packaging, are limited in weight to the gross weight of the as-tested liquids and bottles. The approved Hedgehog-II packaging configurations described in this report may be transported by air, and have been evaluated as meeting the applicable International Air Transport Association/International Civil Aviation Organization (IATA/ICAO) Dangerous Goods Regulations in addition to the DOT requirements.

  6. What Working on this Project Meant to Me from the Karns High School English II Honors Class 2006

    E-Print Network [OSTI]

    Pennycook, Steve

    this project including that Oak Ridge started as a key site of the Manhattan Project.It was great#12;What Working on this Project Meant to Me from the Karns High School English II Honors Class. Thishasbeenagreat experienceforme. ­BrookeMercer This was a rewarding and informative project. I had no idea how

  7. Cosmology with Photometrically-Classified Type Ia Supernovae from the SDSS-II Supernova Survey

    E-Print Network [OSTI]

    Campbell, Heather; Nichol, Robert C; Sako, Masao; Smith, Mathew; Lampeitl, Hubert; Olmstead, Matthew D; Bassett, Bruce; Biswas, Rahul; Brown, Peter; Cinabro, David; Dawson, Kyle S; Dilday, Ben; Foley, Ryan J; Frieman, Joshua A; Garnavich, Peter; Hlozek, Renee; Jha, Saurabh W; Kuhlmann, Steve; Kunz, Martin; Marriner, John; Miquel, Ramon; Richmond, Michael; Riess, Adam; Schneider, Donald P; Sollerman, Jesper; Taylor, Matt; Zhao, Gong-Bo

    2012-01-01

    We present the cosmological analysis of 752 photometrically-classified Type Ia Supernovae (SNe Ia) obtained from the full Sloan Digital Sky Survey II (SDSS-II) Supernova (SN) Survey, supplemented with host-galaxy spectroscopy from the SDSS-III Baryon Oscillation Spectroscopic Survey (BOSS). Our photometric-classification method is based on the SN typing technique of Sako et al. (2011), aided by host galaxy redshifts (0.05typing efficiency of 70.8%, with only 3.9% contamination from core-collapse (non-Ia) SNe. We demonstrate that this level of contamination has no effect on our cosmological constraints. We quantify and correct for our selection effects (e.g., Malmquist bias) using simulations. When fitting to a flat LambdaCDM cosmological model, we find that our photometric sample alone gives omega_m=0.24+0.07-0.05 (statistical errors only). If we relax the constraint on flatness, then our sample provides competitive joint stati...

  8. A numerical study of steady-state vortex configurations and vortex pinning in type-II superconductors 

    E-Print Network [OSTI]

    Kim, Sangbum

    2006-04-12

    In part I, a numerical study of the mixed states in a mesoscopic type-II superconducting cylinder is described. Steady-state configurations and transient behavior of the magnetic vortices for various values of the applied ...

  9. Radiatively Induced Type II seesaw and Vector-like 5/3 Charge Quarks

    E-Print Network [OSTI]

    R. Franceschini; R. N. Mohapatra

    2013-06-26

    Understanding small neutrino masses in type II seesaw models with TeV scale SM triplet Higgs bosons requires that its coupling with the standard model Higgs doublet H be dialed down to be order eV to KeV, which is a fine-tuning by a factor of $10^{-11}-10^{-8}$ with respect to the weak scale. We present a SUSY extension of the type II seesaw model where this dimensionful small coupling is radiatively induced, thus making its smallness natural. This model has an exotic vector-like quark doublet which contains a quark X with electric charge 5/3 and a top partner t'. We discuss in details the phenomenology of the model paying special attention to the consequences of the interactions of the the exotic heavy quarks and the scalars of the model. Implications for neutrinoless double beta decay and for the LHC experiments are discussed in detail. Remarkably, in this model both the seesaw triplet and the heavy quarks can manifest at colliders in a host of different signatures, including some that significantly differ from those of the minimal models. Depending on the choice of the hierarchy of couplings, the decay of the heavy quarks and of the seesaw triplet may be subject to bounds that can be tighter or looser than the bounds from standard LHC searches. Furthermore we point out a new short-distance contribution to neutrinoless double beta decay mediated by the simultaneous propagation of the type II triplet and exotic fermions. Remarkably this contribution to the neutrinoless double beta decay is parametrically quite independent from the scale of the generated neutrino mass.

  10. Neutron Scattering Studies of Vortex Matter in Type-II Superconductors

    SciTech Connect (OSTI)

    Xinsheng Ling

    2012-02-02

    The proposed program is an experimental study of the fundamental properties of Abrikosov vortex matter in type-II superconductors. Most superconducting materials used in applications such as MRI are type II and their transport properties are determined by the interplay between random pinning, interaction and thermal fluctuation effects in the vortex state. Given the technological importance of these materials, a fundamental understanding of the vortex matter is necessary. The vortex lines in type-II superconductors also form a useful model system for fundamental studies of a number of important issues in condensed matter physics, such as the presence of a symmetry-breaking phase transition in the presence of random pinning. Recent advances in neutron scattering facilities such as the major upgrade of the NIST cold source and the Spallation Neutron Source are providing unprecedented opportunities in addressing some of the longstanding issues in vortex physics. The core component of the proposed program is to use small angle neutron scattering and Bitter decoration experiments to provide the most stringent test of the Bragg glass theory by measuring the structure factor in both the real and reciprocal spaces. The proposed experiments include a neutron reflectometry experiment to measure the precise Q-dependence of the structure factor of the vortex lattice in the Bragg glass state. A second set of SANS experiments will be on a shear-strained Nb single crystal for testing a recently proposed theory of the stability of Bragg glass. The objective is to artificially create a set of parallel grain boundaries into a Nb single crystal and use SANS to measure the vortex matter diffraction pattern as a function of the changing angle between the applied magnetic field to the grain boundaries. The intrinsic merits of the proposed work are a new fundamental understanding of type-II superconductors on which superconducting technology is based, and a firm understanding of phases and phase transitions in condensed matter systems with random pinning. The broader impact of the program includes the training of future generation of neutron scientists, and further development of neutron scattering and complementary techniques for studies of superconducting materials. The graduate and undergraduate students participating in this project will learn the state-of-the-art neutron scattering techniques, acquire a wide range of materials research experiences, and participate in the frontier research of superconductivity. This should best prepare the students for future careers in academia, industry, or government.

  11. HGB 11/20/95 component side sketch of "Fastbus Power Supply MK II Type 2"

    E-Print Network [OSTI]

    Berns, Hans-Gerd

    S2 FILTER AC LINE M1 DC 0­30 VOLTS M2 DC 0­300 AMPS S3 RESET CTRL LEDs S1 S4,S5 CB1 POWER ON/OFF HGB 11/20/95 component side sketch of "Fastbus Power Supply MK II Type 2" RELAY BOARD INTERLOCKS TB1: INTERLOCKS IN J2: ANALOG OUT J1: REMOTE SENS IN K3 RELAY PS6 5V / 6A (CTRL) Power supply 'RO105' PS5 ­15V / 2

  12. Pump Spectral Bandwidth, Birefringence, and Entanglement in Type-II Parametric Down Conversion

    DOE Public Access Gateway for Energy & Science Beta (PAGES Beta)

    Erenso, Daniel

    2009-01-01

    The twin photons produced by a type-II spontaneous parametric down conversion are well know as a potential source of photons for quantum teleportation due to the strong entanglement in polarization. This strong entanglement in polarization, however, depends on the spectral composition of the pump photon and the nature of optical isotropy of the crystal. By exact numerical calculation of the concurrence, we have shown that how pump photons spectral width and the birefringence nature of the crystal directly affect the degree of polarization entanglement of the twin photons.

  13. Can first year start other than fall? No Type of school PUBLIC

    E-Print Network [OSTI]

    Scharer, John E.

    inside the library 614 4th year 0 0 0 0 2nd year 1 2 3 1.2 3rd year 0 1 1 0.4 1st year 0 17 17 6.8 JCan first year start other than fall? No Type of school PUBLIC Financial aid deadline 5/1/2013 Term enrolled in independent study 221 0 Number of students who participated in law journals 175 0 Typical first-year

  14. Cosmological parameter uncertainties from SALT-II type Ia supernova light curve models

    SciTech Connect (OSTI)

    Mosher, J.; Sako, M. [Department of Physics and Astronomy, University of Pennsylvania, 209 South 33rd Street, Philadelphia, PA 19104 (United States); Guy, J.; Astier, P.; Betoule, M.; El-Hage, P.; Pain, R.; Regnault, N. [LPNHE, CNRS/IN2P3, Université Pierre et Marie Curie Paris 6, Universié Denis Diderot Paris 7, 4 place Jussieu, F-75252 Paris Cedex 05 (France); Kessler, R.; Frieman, J. A. [Kavli Institute for Cosmological Physics, University of Chicago, 5640 South Ellis Avenue, Chicago, IL 60637 (United States); Marriner, J. [Center for Particle Astrophysics, Fermi National Accelerator Laboratory, P.O. Box 500, Batavia, IL 60510 (United States); Biswas, R.; Kuhlmann, S. [Argonne National Laboratory, 9700 South Cass Avenue, Lemont, IL 60439 (United States); Schneider, D. P., E-mail: kessler@kicp.chicago.edu [Department of Astronomy and Astrophysics, The Pennsylvania State University, University Park, PA 16802 (United States)

    2014-09-20

    We use simulated type Ia supernova (SN Ia) samples, including both photometry and spectra, to perform the first direct validation of cosmology analysis using the SALT-II light curve model. This validation includes residuals from the light curve training process, systematic biases in SN Ia distance measurements, and a bias on the dark energy equation of state parameter w. Using the SN-analysis package SNANA, we simulate and analyze realistic samples corresponding to the data samples used in the SNLS3 analysis: ?120 low-redshift (z < 0.1) SNe Ia, ?255 Sloan Digital Sky Survey SNe Ia (z < 0.4), and ?290 SNLS SNe Ia (z ? 1). To probe systematic uncertainties in detail, we vary the input spectral model, the model of intrinsic scatter, and the smoothing (i.e., regularization) parameters used during the SALT-II model training. Using realistic intrinsic scatter models results in a slight bias in the ultraviolet portion of the trained SALT-II model, and w biases (w {sub input} – w {sub recovered}) ranging from –0.005 ± 0.012 to –0.024 ± 0.010. These biases are indistinguishable from each other within the uncertainty; the average bias on w is –0.014 ± 0.007.

  15. ON THE TEMPORAL EVOLUTION OF THE DISK COUNTERPART OF TYPE II SPICULES IN THE QUIET SUN

    SciTech Connect (OSTI)

    Sekse, D. H.; Rouppe van der Voort, L.; De Pontieu, B.

    2013-02-20

    The newly established type II spicule has been speculated to provide enough hot plasma to play an important role in the mass loading and heating of the solar corona. With the identification of rapid blueshifted excursions (RBEs) as the on-disk counterpart of type II spicules we have analyzed three different high-quality timeseries with the CRisp Imaging SpectroPolarimeter (CRISP) at the Swedish Solar Telescope on La Palma and subjected to an automated detection routine to detect a large number of RBEs for statistical purposes. Our observations are of a quiet-Sun region at disk center and we find lower Doppler velocities, 15-40 km s{sup -1}, and Doppler widths, 2-15 km s{sup -1}, of RBEs than in earlier coronal hole studies, 30-50 km s{sup -1} and 7-23 km s{sup -1}, respectively. In addition, we examine the spatial dependence of Doppler velocities and widths along the RBE axis and conclude that there is no clear trend to this over the field of view or in individual RBEs in the quiet Sun at disk center. These differences with previous coronal hole studies are attributed to the more varying magnetic field configuration in quiet-Sun conditions. Using an extremely high-cadence data set has allowed us to improve greatly on the determination of lifetimes of RBEs, which we find to range from 5 to 60 s with an average lifetime of 30 s, as well as the transverse motions in RBEs, with transverse velocities up to 55 km s{sup -1} and averaging 12 km s{sup -1}. Furthermore, our measurements of the recurrence rates of RBEs provide important new constraints on coronal heating by spicules. We also see many examples of a sinusoidal wave pattern in the transverse motion of RBEs with periods averaging 54 s and amplitudes from 21.5 to 129 km which agrees well with previous studies of wave motion in spicules at the limb. We interpret the appearance of RBEs over their full length within a few seconds as the result of a combination of three kinds of motions as is earlier reported for spicules. Finally, we look at the temporal connection between H{alpha} and Ca II 8542 RBEs and find that Ca II 8542 RBEs in addition to being located closer to the footpoint also appear before the H{alpha} RBEs. This connection between Ca II 8542 and H{alpha} supports the idea that heating is occurring in spicules and contributes more weight to the prominence of spicules as a source for heating and mass loading of the corona.

  16. Persistent C II absorption in the normal type Ia supernova 2002fk

    SciTech Connect (OSTI)

    Cartier, Régis; Zelaya, Paula [Millennium Institute of Astrophysics, Casilla 36-D, Santiago (Chile); Hamuy, Mario; Maza, José; González, Luis; Huerta, Leonor [Departamento de Astronomía, Universidad de Chile, Casilla 36-D, Santiago (Chile); Pignata, Giuliano [Departamento Ciencias Fisicas, Universidad Andres Bello, Av. República 252, Santiago (Chile); Förster, Francisco [Center for Mathematical Modelling, Universidad de Chile, Avenida Blanco Encalada 2120, Piso 7, Santiago (Chile); Folatelli, Gaston [Institute for the Physics and Mathematics of the Universe (IPMU), University of Tokyo, 5-1-5 Kashiwanoha, Kashiwa, Chiba 277-8583 (Japan); Phillips, Mark M.; Morrell, Nidia; Contreras, Carlos; Roth, Miguel; González, Sergio [Carnegie Institution of Washington, Las Campanas Observatory, Colina el Pino s/n, Casilla 601 (Chile); Krisciunas, Kevin; Suntzeff, Nicholas B. [Department of Physics and Astronomy, Texas A and M University, 4242 TAMU, College Station, TX 77843 (United States); Clocchiatti, Alejandro [Departamento de Astronomía y Astrofísica, Pontificia Universidad Católica de Chile, Casilla 306, Santiago (Chile); Coppi, Paolo [Department of Astronomy, Yale University, New Haven, CT 06520-8101 (United States); Koviak, Kathleen, E-mail: rcartier@das.uchile.cl [Carnegie Institution of Washington, 813 Santa Barbara Street, Pasadena, CA 911901 (United States)

    2014-07-01

    We present well-sampled UBVRIJHK photometry of SN 2002fk starting 12 days before maximum light through 122 days after peak brightness, along with a series of 15 optical spectra from –4 to +95 days since maximum. Our observations show the presence of C II lines in the early-time spectra of SN 2002fk, expanding at 11,000 km s{sup –1} and persisting until 8 days past maximum light with a velocity of ?9000 km s{sup –1}. SN 2002fk is characterized by a small velocity gradient of v-dot {sub Si} {sub II}=26 km s{sup –1} day{sup –1}, possibly caused by an off-center explosion with the ignition region oriented toward the observer. The connection between the viewing angle of an off-center explosion and the presence of C II in the early-time spectrum suggests that the observation of C II could be also due to a viewing angle effect. Adopting the Cepheid distance to NGC 1309 we provide the first H {sub 0} value based on near-infrared (near-IR) measurements of a Type Ia supernova (SN) between 63.0 ± 0.8 (±3.4 systematic) and 66.7 ± 1.0 (±3.5 systematic) km s{sup –1} Mpc{sup –1}, depending on the absolute magnitude/decline rate relationship adopted. It appears that the near-IR yields somewhat lower (6%-9%) H {sub 0} values than the optical. It is essential to further examine this issue by (1) expanding the sample of high-quality near-IR light curves of SNe in the Hubble flow, and (2) increasing the number of nearby SNe with near-IR SN light curves and precise Cepheid distances, which affords the promise to deliver a more precise determination of H {sub 0}.

  17. Type-II super-Backlund transformation and integrable defects for the N=1 super sinh-Gordon model

    E-Print Network [OSTI]

    A. R. Aguirre; J. F. Gomes; N. I. Spano; A. H. Zimerman

    2015-06-25

    A new super-Backlund transformation for the N=1 supersymmetric sinh-Gordon equation is constructed. Based on this construction we propose a type-II integrable defect for the supersymmetric sinh-Gordon model consistent with this new transformation through the Lagrangian formalism. Explicit expressions for the modified conserved energy, momentum and supercharges are also computed. In addition, we show for the model that the type-II defect can also been regarded as a pair of fused defects of a previously introduced type. The explicit derivation of the associated defect matrices is also presented as a necessary condition for the integrability of the model.

  18. Type-II super-Backlund transformation and integrable defects for the N=1 super sinh-Gordon model

    E-Print Network [OSTI]

    Aguirre, A R; Spano, N I; Zimerman, A H

    2015-01-01

    A new super-Backlund transformation for the N=1 supersymmetric sinh-Gordon equation is constructed. Based on this construction we propose a type-II integrable defect for the supersymmetric sinh-Gordon model consistent with this new transformation through the Lagrangian formalism. Explicit expressions for the modified conserved energy, momentum and supercharges are also computed. In addition, we show for the model that the type-II defect can also been regarded as a pair of fused defects of a previously introduced type. The explicit derivation of the associated defect matrices is also presented as a necessary condition for the integrability of the model.

  19. Autofib Redshift Survey: II -- The Evolution of the Galaxy Luminosity Function by Spectral Type

    E-Print Network [OSTI]

    Jeremy Heyl; Matthew Colless; Richard S. Ellis; Tom Broadhurst

    1996-10-04

    We determine the evolution of the galaxy luminosity function (LF) as a function of spectral type using the Autofib redshift survey, a compendium of over 1700 galaxy redshifts in various magnitude-limited samples spanning b_J=11.5-24.0. To carry out this analysis we have developed a cross-correlation technique which classifies faint galaxy spectra into one of six types based on local galaxy templates. Tests and simulations show that this technique yields classifications correct to within one type for more than 90% of the galaxies in our sample. We have also developed extensions of the step-wise maximum likelihood method and the STY parametric method for estimating LFs which are applicable to recovering an evolving LF from multiple samples. We find that: (i) The spectra and LF of E/S0 galaxies show no appreciable evolution out to at least z ~ 0.5. (ii) Early-type spirals show modest evolution, characterised by a gradual steepening of the faint end of their LF with redshift. (iii) Out to z ~ 0.5, the overall evolution of the galaxy population is dominated by changes seen in late-type spirals. The characteristic luminosity (L^*) of these galaxies appears to brighten with redshift and there are signs of strong density evolution (a rapid increase in \\phi^*). These effects appear to be luminosity dependent so that the LF steepens at higher redshift. These trends are accompanied by a steep increase in the median [OII] equivalent width, implying a rapid increase in the star-formation rate with redshift at fixed luminosity---a given star-formation rate is found at higher redshift in galaxies of higher luminosity. We find that these conclusions are robust with respect to spectral classification errors and the luminosity function estimator.

  20. ANISOTROPIC THERMAL CONDUCTIVITY IN A DIRTY TYPE II SUPERCONDUCTOR J.P.M. Van der Veeken, P.H. Kes and D. de Klerk

    E-Print Network [OSTI]

    Boyer, Edmond

    ANISOTROPIC THERMAL CONDUCTIVITY IN A DIRTY TYPE II SUPERCONDUCTOR J.P.M. Van der Veeken, P.H. Kes, The results are compared with calculations by Watts - Tobin and Imai. For dirty type II superconductors) of the total conductivities. ii) The theoretical calculations are valid only for BCS - superconductors

  1. Photocapacitance study of type-II GaSb/GaAs quantum ring solar cells

    SciTech Connect (OSTI)

    Wagener, M. C.; Botha, J. R.; Carrington, P. J.; Krier, A.

    2014-01-07

    In this study, the density of states associated with the localization of holes in GaSb/GaAs quantum rings are determined by the energy selective charging of the quantum ring distribution. The authors show, using conventional photocapacitance measurements, that the excess charge accumulated within the type-II nanostructures increases with increasing excitation energies for photon energies above 0.9?eV. Optical excitation between the localized hole states and the conduction band is therefore not limited to the ?(k?=?0) point, with pseudo-monochromatic light charging all states lying within the photon energy selected. The energy distribution of the quantum ring states could consequently be accurately related from the excitation dependence of the integrated photocapacitance. The resulting band of localized hole states is shown to be well described by a narrow distribution centered 407?meV above the GaAs valence band maximum.

  2. PREDICTION OF TYPE II SOLAR RADIO BURSTS BY THREE-DIMENSIONAL MHD CORONAL MASS EJECTION AND KINETIC RADIO EMISSION SIMULATIONS

    SciTech Connect (OSTI)

    Schmidt, J. M.; Cairns, Iver H. [School of Physics, University of Sydney, NSW 2006 (Australia); Hillan, D. S., E-mail: jschmidt@physics.usyd.edu.au [CSIRO Earth Science and Resource Engineering, North Ryde, NSW 2113 (Australia)

    2013-08-20

    Type II solar radio bursts are the primary radio emissions generated by shocks and they are linked with impending space weather events at Earth. We simulate type II bursts by combining elaborate three-dimensional MHD simulations of realistic coronal mass ejections (CMEs) at the Sun with an analytic kinetic radiation theory developed recently. The modeling includes initialization with solar magnetic and active region fields reconstructed from magnetograms of the Sun, a flux rope of the initial CME dimensioned with STEREO spacecraft observations, and a solar wind driven with averaged empirical data. We demonstrate impressive accuracy in time, frequency, and intensity for the CME and type II burst observed on 2011 February 15. This implies real understanding of the physical processes involved regarding the radio emission excitation by shocks and supports the near-term development of a capability to predict and track these events for space weather prediction.

  3. Photometric and polarimetric observations of fast declining Type II supernovae 2013hj and 2014G

    E-Print Network [OSTI]

    Bose, Subhash; Misra, Kuntal; Matsumoto, Katsura; Kumar, Brajesh; Singh, Mridweeka; Fukushima, Daiki; Kawabata, Miho

    2015-01-01

    We present broadband photometric and polarimetric observations of two type II supernovae (SNe) 2013hj and 2014G. SN 2014G is a spectroscopically classified type IIL event, which we also confirm photometrically as its light curve show characteristic features (plateau slope of 2.55 mag (100 d)$ ^{-1} $ in V-band and duration of $ \\sim77 $d) of a generic IIL SN. On the other hand SN 2013hj also shows high plateau decline rate of $ 1.5 $ mag (100 d)$ ^{-1} $ in V-band, similar to SNe IIL, but marginally lower than SNe IIL template light curves. Our high cadence photometric observations of SNe 2013hj and 2014G enables us to cover all characteristic phases up to radioactive tail of optical light curves. Broadband polarimetric observations reveal some polarization in SN 2013hj with subtle enhancement as SN evolves towards plateau end, however the polarization angle remains constant throughout the evolution. This characteristic is consistent with the idea that the evolving SN with recombining hydrogen envelope is slo...

  4. THE CHEMICALLY CONTROLLED SYNTHESIS OF DUST IN TYPE II-P SUPERNOVAE

    SciTech Connect (OSTI)

    Sarangi, Arkaprabha; Cherchneff, Isabelle, E-mail: arkaprabha.sarangi@unibas.ch, E-mail: isabelle.cherchneff@unibas.ch [Departement Physik, Universität Basel, CH-4056 Basel (Switzerland)

    2013-10-20

    We study the formation of molecules and dust clusters in the ejecta of solar metallicity, Type II-P supernovae (SNe) using a chemical kinetic approach. We follow the evolution of molecules and small dust cluster masses from day 100 to day 1500 after explosion. We consider stellar progenitors with initial masses of 12, 15, 19, and 25 M{sub ?} that explode as SNe with stratified ejecta. The molecular precursors to dust grains comprise molecular chains, rings and small clusters of silica, silicates, metal oxides, sulfides and carbides, pure metals, and carbon, where the nucleation of silicate clusters is described by a two-step process of metal and oxygen addition. We study the impact of the {sup 56}Ni mass on the type and amount of synthesized dust. We predict that large masses of molecules including CO, SiO, SiS, O{sub 2}, and SO form in the ejecta. We show that the discrepancy between the small dust masses detected at infrared wavelengths some 500 days post-explosion and the larger amounts of dust recently detected with Herschel in SN remnants can be explained by the non-equilibrium chemistry linked to the formation of molecules and dust clusters in the ejected material. Dust gradually builds up from small (?10{sup –5} M{sub ?}) to large masses (?5 × 10{sup –2} M{sub ?}) over a 5 yr period after explosion. Subsequent dust formation and/or growth is hampered by the shortage of chemical agents participating in the dust nucleation and the long timescale for accretion. The results highlight the dependence of the dust chemical composition and mass on the amount of {sup 56}Ni synthesized during the explosion. This dependence may partly explain the diversity of epochs at which dust forms in SNe. More generally, our results indicate that Type II-P SNe are efficient but moderate dust producers with an upper limit on the mass of synthesized dust ranging from ?0.03 to 0.09 M{sub ?}. Other dust sources must then operate at high redshift to explain the large quantities of dust present in young galaxies in the early universe.

  5. EnergySmart Schools National Financing Roundtable II—Key Outcomes

    SciTech Connect (OSTI)

    2009-11-01

    As a follow-up to the release of its Guide to Financing EnergySmart Schools, the the National Financing Roundtable brought together individuals with diverse knowledge of school building programs and projects to discuss financing issues and options that build upon those described in the first Guide to Financing EnergySmart Schools.

  6. Autophagy protects type II alveolar epithelial cells from Mycobacterium tuberculosis infection

    SciTech Connect (OSTI)

    Guo, Xu-Guang [Center for Clinical Laboratory Medicine of PLA, Xijing Hospital, Fourth Military Medical University, Xi'an (China) [Center for Clinical Laboratory Medicine of PLA, Xijing Hospital, Fourth Military Medical University, Xi'an (China); Department of Laboratory Medicine, The Third Affiliated Hospital of Guangzhou Medical University, Guangzhou (China); Ji, Tian-Xing [Department of Laboratory Medicine, The Second Affiliated Hospital of Guangzhou Medical University, Guangzhou (China)] [Department of Laboratory Medicine, The Second Affiliated Hospital of Guangzhou Medical University, Guangzhou (China); Xia, Yong, E-mail: gysyxy@gmail.com [Center for Clinical Laboratory Medicine of PLA, Xijing Hospital, Fourth Military Medical University, Xi'an (China)] [Center for Clinical Laboratory Medicine of PLA, Xijing Hospital, Fourth Military Medical University, Xi'an (China); Ma, Yue-Yun, E-mail: cmbmayy@fmmu.edu.cn [Center for Clinical Laboratory Medicine of PLA, Xijing Hospital, Fourth Military Medical University, Xi'an (China)] [Center for Clinical Laboratory Medicine of PLA, Xijing Hospital, Fourth Military Medical University, Xi'an (China)

    2013-03-08

    Highlights: ? We investigated the protective effect of autophagy pathway against MTB infection. ? MTB-infected A549 cells had higher LDH release. ? Inhibition of autophagy signaling significantly enhanced the MTB-induced necrosis. ? Autophagy prevents apoptosis and promotes cell survival in infected cells. -- Abstract: This study was designed to investigate the protective effect of the autophagy signaling pathway against Mycobacterium tuberculosis infection in type II alveolar epithelial cells. An in vitro M. tuberculosis system was established using human A549 cells. Infection-induced changes in the expression of the autophagic marker LC3 were assessed by reverse transcription-PCR and Western blotting. Morphological changes in autophagosomes were detected by transmission electron microscopy (TEM). The function of the autophagy signaling pathway during infection was assessed by measuring the level of cell death and the amount of lactate dehydrogenase (LDH) released in the presence or absence of the inhibitor 3-methyladenine (3-MA). In addition, effects on LDH release were assessed after the siRNA-mediated knockdown of the essential autophagosomal structural membrane protein Atg5. LC3 mRNA expression was significantly reduced in M.tuberculosis-infected A549 cells (16888.76 ± 1576.34 vs. uninfected: 12744.29 ± 1089.37; P < 0.05). TEM revealed M.tuberculosis bacilli-containing compartments that were surrounded by double membranes characteristic of the autophagic process. M.tuberculosis-infected A549 cells released more LDH (1.45 ± 0.12 vs. uninfected: 0.45 ± 0.04; P < 0.05). The inhibition of autophagy signaling significantly enhanced M.tuberculosis-induced necrosis (3-MA: 75 ± 5% vs. untreated: 15 ± 1%; P < 0.05) and LDH release (3-MA: 2.50 ± 0.24 vs. untreated: 0.45 ± 0.04; Atg5 knockdown: 3.19 ± 0.29 vs. untreated: 1.28 ± 0.11; P < 0.05). Our results indicate that autophagy signaling pathway prevents apoptosis in type II alveolar epithelial cells infected with M.tuberculosis and may represent a molecular target for promoting cell survival during infection by respiratory pathogens.

  7. Relation Between Type-II ELMs, Edge Localized Turbulence, Washboard Modes and Energy Losses Between ELMs in High Density ELMy H-modes on JET

    E-Print Network [OSTI]

    Relation Between Type-II ELMs, Edge Localized Turbulence, Washboard Modes and Energy Losses Between ELMs in High Density ELMy H-modes on JET

  8. Bias dependent dual band response from InAs/Ga,,In...Sb type II strain layer superlattice detectors

    E-Print Network [OSTI]

    New Mexico, University of

    available readout integrated circuits. © 2007 American Institute of Physics. DOI: 10.1063/1.2824819 Infrared, University of New Mexico, Albuquerque, New Mexico 87106, USA Received 10 October 2007; accepted 23 November photodetectors based on type II InAs/Ga In Sb strain layer superlattices using an nBn heterostructure design

  9. 1 The Petro Problem The Petro Chemical Corporation manufactures two types of chemicals, I and II. One ton

    E-Print Network [OSTI]

    Lee, Carl

    in precise but "non-mathematical" language. 1 #12;2 Lieberknecht Problem The Lieberknecht family operates' Us Problem The Radios 'R' Us electronics company has a contract to deliv1 The Petro Problem The Petro Chemical Corporation manufactures two types of chemicals, I and II

  10. Electronic and optical properties of single excitons and biexcitons in type-II quantum dot nanocrystals

    SciTech Connect (OSTI)

    Koc, Fatih; Sahin, Mehmet E-mail: mehsahin@gmail.com

    2014-05-21

    In this study, a detailed investigation of the electronic and optical properties (i.e., binding energies, absorption wavelength, overlap of the electron-hole wave functions, recombination oscillator strength, etc.) of an exciton and a biexciton in CdTe/CdSe core/shell type-II quantum dot heterostructures has been carried out in the frame of the single band effective mass approximation. In order to determine the electronic properties, we have self-consistently solved the Poisson-Schrödinger equations in the Hartree approximation. We have considered all probable Coulomb interaction effects on both energy levels and also on the corresponding wave functions for both single exciton and biexciton. In addition, we have taken into account the quantum mechanical exchange-correlation effects in the local density approximation between same kinds of particles for biexciton. Also, we have examined the effect of the ligands and dielectric mismatch on the electronic and optical properties. We have used a different approximation proposed by Sahin and Koc [Appl. Phys. Lett. 102, 183103 (2013)] for the recombination oscillator strength of the biexciton for bound and unbound cases. The results obtained have been presented comparatively as a function of the shell thicknesses and probable physical reasons in behind of the results have been discussed in a detail.

  11. Degenerate Higgs bosons decays to ${??}$ and ${Z?}$ in the type II Seesaw Model

    E-Print Network [OSTI]

    M. Chabab; M. C. Peyranere; L. Rahili

    2014-08-11

    Using the most recent results of CMS and ATLAS, we study the Higgs decays to $\\gamma\\gamma$ and $Z\\gamma$ in the scenario where the two CP even Higgs predicted by the type II seesaw model (HTM) are close to mass degenerate with a mass near $125$ GeV. We analyse the effects of the Higgs potential parameters constrained by the full set of perturbative unitarity, boundedness from below (BFB) as well as from precision electroweak measurements on these decay modes. Our analysis demonstrates that the observed excess in the diphoton Higgs decay channel can be interpreted in our scenario within a delineated region controlled by $\\lambda_{1}$ and $\\lambda_{4}$ coupling. We also find a deviation in the Higgs decay to $Z\\gamma$ with respect to the Standard Model prediction and the largest enhancement is found for a ratio $R_{Z\\gamma}$ of the order $1.6$. Furthermore we show that consistency with current ATLAS data on the diphoton decay channel favours a light doubly charged Higgs with mass in the range $92 - 180$~GeV. Finally, we find that the $\\gamma\\gamma$ and $Z \\gamma$ Higgs decay modes are generally correlated and the magnitude of correlation is sensitive to the sign of the $\\lambda_{1}$ parameter.

  12. Spectroscopy and dynamics of charge transfer excitons in type-II band aligned quantum confined heterostructures

    SciTech Connect (OSTI)

    Kushavah, Dushyant; Mohapatra, P. K.; Vasa, P.; Singh, B. P.; Rustagi, K. C.; Bahadur, D.

    2015-05-15

    We illustrate effect of charge transfer (CT) in type-II quantum confined heterostructure by comparing CdSe quantum dots (QDs), CdSe/CdTe heterostructure quantum dots (HQDs) and CdSe/CdTe/CdSe quantum well-quantum dots (QWQDs) heterostructures. CdSe core QDs were synthesized using a kinetic growth method where QD size depends on reaction time. For shell coating we used modified version of successive ionic layer adsorption and reaction (SILAR). Size of different QDs ?5 to 7 nm were measured by transmission electron microscopy (TEM). Strong red shift from ?597 to ?746 nm in photoluminescence (PL) spectra from QDs to QWQDs shows high tunability which is not possible with single constituent semiconductor QDs. PL spectra have been recorded at different temperatures (10K-300K). Room temperature time correlated single photon counting (TCSPC) measurements for QDs to QWQDs show three exponential radiative decay. The slowest component decay constant in QWQDs comes around eight fold to ?51 ns as compared to ?6.5 ns in HQD suggesting new opportunities to tailor the radiative carrier recombination rate of CT excitons.

  13. On the modular structure of the genus-one Type II superstring low energy expansion

    E-Print Network [OSTI]

    Eric D'Hoker; Michael B. Green; Pierre Vanhove

    2015-06-03

    The analytic contribution to the low energy expansion of Type II string amplitudes at genus-one is a power series in space-time derivatives with coefficients that are determined by integrals of modular functions over the complex structure modulus of the world-sheet torus. These modular functions are associated with world-sheet vacuum Feynman diagrams and given by multiple sums over the discrete momenta on the torus. In this paper we exhibit exact differential and algebraic relations for a certain infinite class of such modular functions by showing that they satisfy Laplace eigenvalue equations with inhomogeneous terms that are polynomial in non-holomorphic Eisenstein series. Furthermore, we argue that the set of modular functions that contribute to the coefficients of interactions up to order D**10 R*4 are linear sums of functions in this class and quadratic polynomials in Eisenstein series and odd Riemann zeta values. Integration over the complex structure results in coefficients of the low energy expansion that are rational numbers multiplying monomials in odd Riemann zeta values.

  14. Higgs mechanism with type-II Nambu-Goldstone bosons at finite chemical potential

    SciTech Connect (OSTI)

    Hama, Yusuke [Department of Physics, University of Tokyo, Tokyo 113-0033 (Japan); Hatsuda, Tetsuo [Department of Physics, University of Tokyo, Tokyo 113-0033 (Japan); IPMU, University of Tokyo, Kashiwa 277-8568 (Japan); Theoretical Research Division, Nishina Center, RIKEN, Wako 351-0198 (Japan); Uchino, Shun [Department of Physics, Kyoto University, Kyoto 606-8502 (Japan)

    2011-06-15

    When the spontaneous symmetry breaking occurs for systems without Lorentz covariance, there arises possible mismatch, N{sub NG}type-II NG bosons emerge. We study how the gauge bosons acquire masses through the Higgs mechanism under this mismatch by employing gauge theories with complex scalar field at finite chemical potential and by enforcing ''charge'' neutrality. To separate the physical spectra from unphysical ones, the R{sub {xi}} gauge is adopted. Not only massless NG bosons but also massive scalar bosons generated by the chemical potential are absorbed into spatial components of the gauge bosons. Although the chemical potential induces a nontrivial mixings among the scalar bosons and temporal components of the gauge bosons, it does not affect the structure of the physical spectra, so that the total number of physical modes is not modified even for N{sub NG}

  15. A Parameter Study of Type II Supernova Light Curves Using 6 M_odot He Cores

    E-Print Network [OSTI]

    Timothy R. Young

    2004-09-13

    Results of numerical calculations of Type II supernova light curves are presented. The model progenitor stars have 6 $M{_\\odot}$ cores and various envelopes, originating from a numerically evolved 20 $M{_\\odot}$ star. Five parameters that affect the light curves are examined: the ejected mass, the progenitor radius, the explosion energy, the $^{56}$Ni mass, and the extent of $^{56}$Ni mixing. The following affects have been found: 1) the larger the progenitor radius the brighter the early--time light curve, with little affect on the late--time light curve, 2) the larger the envelope mass the fainter the early light curve and the flatter the slope of the late light curve, 3) the larger the explosion energy the brighter the early light curve and the steeper the slope of the late light curve, 4) the larger the $^{56}$Ni mass the brighter the overall light curve after 20 to 50 days, with no affect on the early light curve, 5) the more extensive the $^{56}$Ni mixing the brighter the early light curve and the steeper the late light curve. The primary parameters affecting the light curve shape are the progenitor radius and the ejected mass. The secondary parameters are the explosion energy, $^{56}$Ni mass and $^{56}$Ni mixing. I find that while in principle the general shape and absolute magnitude of a light curve indicate a unique set of parameters, in practice it is difficult to avoid some ambiguity in the parameters. I find that the nickel--powered diffusion wave and the recombination of helium produce a prominent secondary peak in all our calculations. The feature is less prominent when compositional mixing, both $^{56}$Ni mixing and mixing between the hydrogen and helium layers, occurs. The model photospheric temperatures and velocities are presented, for comparison to observation.

  16. Nucleosynthesis in the outflows associated with accretion disks of Type II collapsars

    E-Print Network [OSTI]

    Indrani Banerjee; Banibrata Mukhopadhyay

    2013-09-04

    We investigate nucleosynthesis inside the outflows from gamma-ray burst (GRB) accretion disks formed by the Type II collapsars. In these collapsars, massive stars undergo core collapse to form a proto-neutron star initially and a mild supernova explosion is driven. The supernova ejecta lack momentum and subsequently this newly formed neutron star gets transformed to a stellar mass black hole via massive fallback. The hydrodynamics and the nucleosynthesis in these accretion disks has been studied extensively in the past. Several heavy elements are synthesized in the disk and much of these heavy elements are ejected from the disk via winds and outflows. We study nucleosynthesis in the outflows launched from these disks by using an adiabatic, spherically expanding outflow model, to understand which of these elements thus synthesized in the disk survive in the outflow. While studying this we find that many new elements like isotopes of titanium, copper, zinc etc. are present in the outflows. 56Ni is abundantly synthesized in most of the cases in the outflow which implies that the outflows from these disks in a majority of cases will lead to an observable supernova explosion. It is mainly present when outflow is considered from the He-rich, 56Ni/54Fe rich zones of the disks. However, outflow from the Si-rich zone of the disk remains rich in silicon. Although, emission lines of many of these heavy elements have been observed in the X-ray afterglows of several GRBs by Chandra, BeppoSAX, XMM-Newton etc., Swift seems to have not detected these lines yet.

  17. NUCLEOSYNTHESIS IN THE OUTFLOWS ASSOCIATED WITH ACCRETION DISKS OF TYPE II COLLAPSARS

    SciTech Connect (OSTI)

    Banerjee, Indrani; Mukhopadhyay, Banibrata, E-mail: indrani@physics.iisc.ernet.in, E-mail: bm@physics.iisc.ernet.in [Department of Physics, Indian Institute of Science, Bangalore 560 012 (India)

    2013-11-20

    We investigate nucleosynthesis inside the outflows from gamma-ray burst (GRB) accretion disks formed by the Type II collapsars. In these collapsars, massive stars undergo core collapse to form a proto-neutron star initially, and a mild supernova (SN) explosion is driven. The SN ejecta lack momentum, and subsequently this newly formed neutron star gets transformed to a stellar mass black hole via massive fallback. The hydrodynamics and the nucleosynthesis in these accretion disks have been studied extensively in the past. Several heavy elements are synthesized in the disk, and much of these heavy elements are ejected from the disk via winds and outflows. We study nucleosynthesis in the outflows launched from these disks by using an adiabatic, spherically expanding outflow model, to understand which of these elements thus synthesized in the disk survive in the outflow. While studying this, we find that many new elements like isotopes of titanium, copper, zinc, etc., are present in the outflows. {sup 56}Ni is abundantly synthesized in most of the cases in the outflow, which implies that the outflows from these disks in a majority of cases will lead to an observable SN explosion. It is mainly present when outflow is considered from the He-rich, {sup 56}Ni/{sup 54}Fe-rich zones of the disks. However, outflow from the Si-rich zone of the disk remains rich in silicon. Although emission lines of many of these heavy elements have been observed in the X-ray afterglows of several GRBs by Chandra, BeppoSAX, XMM-Newton, etc., Swift seems to have not yet detected these lines.

  18. Monitoring of Total Type II Pyrethroid Pesticides in Citrus Oils and Water by Converting to a Common Product 3-Phenoxybenzoic Acid

    E-Print Network [OSTI]

    Hammock, Bruce D.

    Monitoring of Total Type II Pyrethroid Pesticides in Citrus Oils and Water by Converting to a Common Product 3-Phenoxybenzoic Acid Mark R. McCoy, Zheng Yang, Xun Fu,§ Ki Chang Ahn, Shirley J. Gee an alternative method that converts the type II pyrethroids to a common chemical product, 3-phenoxybenzoic acid

  19. II*

    Gasoline and Diesel Fuel Update (EIA)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Homesum_a_epg0_fpd_mmcf_m.xls" ,"Available from WebQuantity of Natural GasAdjustments (Billion Cubic Feet) Wyoming Dry NaturalPrices1Markets See full Hydrocarbon Gas2 II Now

  20. The Outer Disks of Early-Type Galaxies. II. Surface-Brightness Profiles of Unbarred Galaxies and Trends with Hubble Type

    E-Print Network [OSTI]

    Gutierrez, Leonel; Aladro, Rebeca; Beckman, John E

    2011-01-01

    We present azimuthally averaged radial profiles of R-band surface brightness for a complete sample of 47 early-type, unbarred galaxies, as a complement to our previous study of early-type barred galaxies. Following very careful sky subtraction, the profiles can typically be determined down to brightness levels well below 27 mag arcsec^{-2} and in the best cases below 28 mag arcsec^{-2}. We classified the profiles according to the scheme used previously for the barred sample: Type I profiles are single unbroken exponential radial declines in brightness; Type II profiles ("truncations") have an inner shallow slope (usually exponential) which changes at a well defined break radius to a steeper exponential; and Type III profiles ("antitruncations") have an inner exponential that is steeper, giving way to a shallower outer (usually exponential) decline. By combining these profiles with previous studies, we can make the first clear statements about the trends of outer-disk profile types along the Hubble sequence (i...

  1. 2015 Middle School Team Photos

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    Cedar Park Middle School I, Portland, Ore. Cedar Park Middle School II, Portland, Ore. Galaxy Science Club, Bellevue, Wash. George Middle School , Portland, Ore. Harrison Park...

  2. Vortex dynamics : a window into the properties of type-II superconductors

    E-Print Network [OSTI]

    Taylor, Benjamin Jeremy

    2006-01-01

    A. Superconductivity . . . . . . . . . .theory of superconductivity B. Type I . . . . . . . . . . .11] P. G. DeGennes, Superconductivity of Metals and Alloys,

  3. Frequent intragenic deletion of the P gene in Tanzanian patients with Type II oculocutaneous albinism (OCA2)

    SciTech Connect (OSTI)

    Spritz, R.; Fukai, K.; Holmes, S.A.

    1995-06-01

    Type II oculocutaneous albinism (OCA2) is an autosomal recessive disorder in which the biosynthesis of melanin pigment is reduced in the skin, hair, and eyes. OCA2, which results from mutations of the P gene, is the most frequent type of albinism in African and African-American patients. OCA2 is especially frequent in Tanzania, where it occurs with an incidence of {approximately}1/1,400. We have identified abnormalities of the P gene in each of 13 unrelated patients with OCA2 from Tanzania. One of these, a deletion of exon 7, is strongly predominant, accounting for {approximately}77% of mutant alleles in this group of patients. 20 refs., 2 figs.

  4. Synthesis and X-ray Crystal Structures of Palladium(II) and Platinum(II) Complexes of the PCP-Type Chiral

    E-Print Network [OSTI]

    Zhang, Xumu

    Synthesis and X-ray Crystal Structures of Palladium(II) and Platinum(II) Complexes of the PCP-assembly of one- dimensional polymeric organometallic structures.9 Re- cently, palladium complexes with a PCP

  5. The BOSS-WiggleZ overlap region II: dependence of cosmic growth on galaxy type

    E-Print Network [OSTI]

    Marín, Felipe A; Blake, Chris; Koda, Jun; Kazin, Eyal; Schneider, Donald P

    2015-01-01

    The anisotropic galaxy 2-point correlation function (2PCF) allows measurement of the growth of large-scale structures from the effect of peculiar velocities on the clustering pattern. We present new measurements of the auto- and cross- correlation function multipoles of 69,180 WiggleZ and 46,380 BOSS-CMASS galaxies sharing an overlapping volume of ~0.2 (Gpc/h)^3. Analysing the redshift-space distortions (RSD) of galaxy 2-point statistics for these two galaxy tracers, we test for systematic errors in the modelling depending on galaxy type and investigate potential improvements in cosmological constraints. We build a large number of mock galaxy catalogues to examine the limits of different RSD models in terms of fitting scales and galaxy type, and to study the covariance of the measurements when performing joint fits. For the galaxy data, fitting the monopole and quadrupole of the WiggleZ 2PCF on scales 24

  6. Late-Type Dwarf Galaxies in the Virgo Cluster: II. Star Formation Properties

    E-Print Network [OSTI]

    Elchanan Almoznino; Noah Brosch

    1998-04-22

    We study star-formation-inducing mechanisms in galaxies through multi- wavelength measurements of a sample of dwarf galaxies in the Virgo cluster described in paper I. Our main goal is to test how star formation inducing mechanisms depend on several parameters of the galaxies, such as morphological type and hydrogen content. We derive the star formation rate and star formation histories of the galaxies, and check their dependence on other parameters. Comparison of the sample galaxies with population synthesis models shows that these objects have significantly lower metallicity than the Solar value. The colors can generally be explained as a combination of two different stellar populations: a young (3--20 Myr) population which represents the stars currently forming, and an older (0.1--1 Gyr) population of previous stellar generations. This is consistent with the explanation that star formation in this type of objects takes place in short bursts followed by long quiescent periods. No significant relation is found between the star formation properties of the sample galaxies and their hydrogen content. Apparently, when star formation occurs in bursts, other parameters influence the star formation properties more significantly than the amount of hydrogen. No correlation is found between the projected Virgocentric distance and the rate of star formation in the galaxies.

  7. Study of Row Phase Dependent Skew Quadrupole Fields in Apple-II Type EPUs at the ALS

    SciTech Connect (OSTI)

    Steier, C.; Marks, S.; Prestemon, Soren; Robin, David; Schlueter, Ross; Wolski, Andrzej

    2004-05-07

    Since about 5 years, Apple-II type Elliptically Polarizing Undulators (EPU) have been used very successfully at the ALS to generate high brightness photon beams with arbitrary polarization. However, both EPUs installed so far cause significant changes of the vertical beamsize, especially when the row phase is changed to change the polarization of the photons emitted. Detailed measurements indicate this is caused by a row phase dependent skew quadrupole term in the EPUs. Magnetic measurements revealed the same effect for the third EPU to be installed later this year. All measurements to identify and quantify the effect with beam will be presented, as well as some results of magnetic bench measurements and numeric field simulations.

  8. Future non-linear stability for solutions of the Einstein-Vlasov system of Bianchi types II and VI$_0$

    E-Print Network [OSTI]

    Ernesto Nungesser

    2012-08-30

    In a recent paper arXiv:1208.4231 we have treated the future non-linear stability for reflection symmetric solutions of the Einstein-Vlasov system of Bianchi types II and VI$_0$. We have been able now to remove the reflection symmetry assumption, thus treating the non-diagonal case. Apart from the increasing complexity the methods have been essentially the same as in the diagonal case, showing that they are thus quite powerful. Here the challenge was to put the equations in a form that permits the use of the previous results. We are able to conclude that after a possible basis change the future of the non-diagonal spacetimes in consideration is asymptotically diagonal.

  9. L.R.S. Bianchi type II Stiff Fluid cosmological model with Decaying Vacuum Energy Density $?$ in general relativity

    E-Print Network [OSTI]

    Hassan Amirhashchi

    2010-11-26

    Locally rotationally symmetric (L.R.S.) Bianchi type II stiff fluid cosmological model is investigated. To get the deterministic model of the universe, we have assumed a condition $A=B^{m}$ between metric potentials $A,~B$ where $n$ is the constant. It is shown that the vacuum energy density $\\Lambda$ is positive and proportional to $\\frac{1}{t^{2}}$. The values of deceleration parameter $q$, matter-energy density $\\Omega_{m}$ and dark-energy density $\\Omega_{\\Lambda}$ are found to be in good agreement with the values obtain from 5-years WMAP observations. the predicted value of the jerk parameter agrees with the SNLS SNIa and X-ray galaxy cluster distance data but does not with the SNIa gold sample data. In general, the model represent accelerating, shearing and non-rotating universe.The physical and geometrical behavior of these models are also discussed.

  10. Low Mach Number Modeling of Type Ia Supernovae. II. Energy Evolution

    E-Print Network [OSTI]

    A. S. Almgren; J. B. Bell; C. A. Rendleman; M. Zingale

    2006-06-21

    The convective period leading up to a Type Ia supernova (SN Ia) explosion is characterized by very low Mach number flows, requiring hydrodynamical methods well-suited to long-time integration. We continue the development of the low Mach number equation set for stellar scale flows by incorporating the effects of heat release due to external sources. Low Mach number hydrodynamics equations with a time-dependent background state are derived, and a numerical method based on the approximate projection formalism is presented. We demonstrate through validation with a fully compressible hydrodynamics code that this low Mach number model accurately captures the expansion of the stellar atmosphere as well as the local dynamics due to external heat sources. This algorithm provides the basis for an efficient simulation tool for studying the ignition of SNe Ia.

  11. Photon storage in Lambda-type optically dense atomic media. II. Free-space model

    E-Print Network [OSTI]

    Alexey V. Gorshkov; Axel Andre; Mikhail D. Lukin; Anders S. Sorensen

    2007-09-08

    In a recent paper [Gorshkov et al., Phys. Rev. Lett. 98, 123601 (2007)], we presented a universal physical picture for describing a wide range of techniques for storage and retrieval of photon wave packets in Lambda-type atomic media in free space, including the adiabatic reduction of the photon group velocity, pulse-propagation control via off-resonant Raman techniques, and photon-echo based techniques. This universal picture produced an optimal control strategy for photon storage and retrieval applicable to all approaches and yielded identical maximum efficiencies for all of them. In the present paper, we present the full details of this analysis as well some of its extensions, including the discussion of the effects of non-degeneracy of the two lower levels of the Lambda system. The analysis in the present paper is based on the intuition obtained from the study of photon storage in the cavity model in the preceding paper [Gorshkov et al., Phys. Rev. A 76, 033804 (2007)].

  12. Type Ia supernovae from merging white dwarfs. II. Post-merger detonations

    SciTech Connect (OSTI)

    Raskin, Cody; Kasen, Daniel [Nuclear Science Division, Lawrence Berkeley National Laboratory, Berkeley, CA (United States); Moll, Rainer; Woosley, Stan [Department of Physics and Department of Astronomy, University of California, Santa Cruz, CA (United States); Schwab, Josiah [Department of Physics and Department of Astronomy, University of California, Berkeley, CA (United States)

    2014-06-10

    Merging carbon-oxygen (CO) white dwarfs are a promising progenitor system for Type Ia supernovae (SNe Ia), but the underlying physics and timing of the detonation are still debated. If an explosion occurs after the secondary star is fully disrupted, the exploding primary will expand into a dense CO medium that may still have a disk-like structure. This interaction will decelerate and distort the ejecta. Here we carry out multidimensional simulations of 'tamped' SN Ia models, using both particle and grid-based codes to study the merger and explosion dynamics and a radiative transfer code to calculate synthetic spectra and light curves. We find that post-merger explosions exhibit an hourglass-shaped asymmetry, leading to strong variations in the light curves with viewing angle. The two most important factors affecting the outcome are the scale height of the disk, which depends sensitively on the binary mass ratio, and the total {sup 56}Ni yield, which is governed by the central density of the remnant core. The synthetic broadband light curves rise and decline very slowly, and the spectra generally look peculiar, with weak features from intermediate mass elements but relatively strong carbon absorption. We also consider the effects of the viscous evolution of the remnant and show that a longer time delay between merger and explosion probably leads to larger {sup 56}Ni yields and more symmetrical remnants. We discuss the relevance of this class of aspherical 'tamped' SN Ia for explaining the class of 'super-Chandrasekhar' SN Ia.

  13. Optical and ultraviolet observations of a low-velocity type II plateau supernova 2013am in M65

    SciTech Connect (OSTI)

    Zhang, Jujia; Bai, Jinming; Fan, Yufeng; Wang, Jianguo; Yi, Weimin; Wang, Chuanjun; Xin, Yuxin; Liangchang; Zhang, Xiliang; Lun, Baoli; Wang, Xueli; He, Shousheng [Yunnan Observatories (YNAO), Chinese Academy of Sciences, Kunming 650216 (China); Wang, Xiaofeng; Huang, Fang; Mo, Jun [Physics Department and Tsinghua Center for Astrophysics (THCA), Tsinghua University, Beijing 100084 (China); Mazzali, Paolo A.; Bersier, David [Astrophysics Research Institute, Liverpool John Moores University, Liverpool Science Park, 146 Brownlow Hill, Liverpool L3 5RF (United Kingdom); Zhang, Tianmeng [National Astronomical Observatories of China (NAOC), Chinese Academy of Sciences, Beijing 100012 (China); Walker, Emma S., E-mail: jujia@ynao.ac.cn, E-mail: baijinming@ynao.ac.cn, E-mail: wang_xf@mail.tsinghua.edu.cn [Department of Physics, Yale University, New Haven, CT 06520-8121 (United States)

    2014-12-10

    Optical and ultraviolet observations for the nearby type II plateau supernova (SN IIP) 2013am in the nearby spiral galaxy M65 are presented in this paper. The early spectra are characterized by relatively narrow P-Cygni features, with ejecta velocities much lower than observed in normal SNe IIP (i.e., ?2000 km s{sup –1} versus ?5000 km {sup –1} in the middle of the plateau phase). Moreover, prominent Ca II absorptions are also detected in SN 2013am at relatively early phases. These spectral features are reminiscent of those seen in the low-velocity and low-luminosity SN IIP 2005cs. However, SN 2013am exhibits different photometric properties, having shorter plateau phases and brighter light curve tails if compared to SN 2005cs. Adopting R{sub V} = 3.1 and a mean value of total reddening derived from the photometric and spectroscopic methods (i.e., E(B – V) = 0.55 ± 0.19 mag), we find that SN 2013am may have reached an absolute V-band peak magnitude of –15.83 ± 0.71 mag and produced an {sup 56}Ni mass of 0.016{sub ?0.006}{sup +0.010} M {sub ?} in the explosion. These parameters are close to those derived for SN 2008in and SN 2009N, which have been regarded as 'gap-filler' objects linking the faint SNe IIP to the normal ones. This indicates that some low-velocity SNe IIP may not necessarily result from the low-energetic explosions. The low expansion velocities could be due to a lower metallicity of the progenitor stars, a larger envelope mass ejected in the explosion, or the effect of viewing angle where these SNe were observed at an angle away from the polar direction.

  14. Degenerate Higgs bosons decays to ${\\gamma\\gamma}$ and ${Z\\gamma}$ in the type II seesaw Model

    E-Print Network [OSTI]

    Chabab, M; Rahili, L

    2014-01-01

    Using the most recent results of CMS and ATLAS, we study the Higgs decays to $\\gamma\\gamma$ and $Z\\gamma$ in the scenario where the two CP even Higgs predicted by the type II seesaw model (HTM) are close to mass degenerate with a mass near $125$ GeV. We analyse the effects of the Higgs potential parameters constrained by the full set of perturbative unitarity, boundedness from below (BFB) as well as from precision electroweak measurements on these decay modes. Our analysis demonstrates that the observed excess in the diphoton Higgs decay channel can be interpreted in our scenario within a delineated region controlled by $\\lambda_{1}$ and $\\lambda_{4}$ coupling. We also find a deviation in the Higgs decay to $Z\\gamma$ with respect to the Standard Model prediction and the largest enhancement is found for a ratio $R_{Z\\gamma}$ of the order $1.6$. Furthermore we show that consistency with current ATLAS data on the diphoton decay channel favours a light doubly charged Higgs with mass in the range $92 - 180$~GeV. F...

  15. From Rehabilitation to Punishment: The Institutionalization of Suspension Policies in Post-World War II New York City Schools

    E-Print Network [OSTI]

    Lissy, Rachel Ellen

    2015-01-01

    Rights in Postwar New York City (Boston: Harvard University1947-1949, Series 240, New York City Department of Educationthe population of the New York City schools has increased by

  16. From Rehabilitation to Punishment: The Institutionalization of Suspension Policies in Post-World War II New York City Schools

    E-Print Network [OSTI]

    Lissy, Rachel Ellen

    2015-01-01

    for Civil Rights in Postwar New York City (Boston: HarvardBack to School to be Cheated!" New York Amsterdam News, City1947-1949, Series 240, New York City Department of Education

  17. School Composition and Disproportionality in Discipline: A School-Level Analysis of Disciplinary Actions against Various Offense Types in the United States, 2007-2008

    E-Print Network [OSTI]

    Fisher, Julie Diane

    2011-04-11

    in his truck, presumably to go hunting after school, to turn his truck around and take his gun home without any disciplinary punishment. Rural administrators were more likely to overlook this violation as long as the weapon was in the student’s vehicle..., placing them in in-school suspension is an easy alternative so teachers do not have to deal with misbehaving students. In the late 1980s and early 1990s schools began to experience more violence such as guns, drugs, and gangs. In response...

  18. Experimental investigation of amplitude and phase quantum correlations in a type II OPO above threshold: from the non-degenerate to the degenerate operation

    E-Print Network [OSTI]

    Julien Laurat; Thomas Coudreau; Laurent Longchambon; Claude Fabre

    2004-12-14

    We describe a very stable type II optical parametric oscillator operated above threshold which provides 9.7 $\\pm$ 0.5 dB (89%) of quantum noise reduction on the intensity difference of the signal and idler modes. We also report the first experimental study by homodyne detection of the generated bright two-mode state in the case of frequency degenerate operation obtained by introducing a birefringent plate inside the optical cavity.

  19. Nucleosynthesis simulations for the production of the p-nuclei $^{\\text{92}}$Mo and $^{\\text{94}}$Mo in a Supernova type II model

    E-Print Network [OSTI]

    Göbel, Kathrin; Koloczek, Alexander; Pignatari, Marco; Reifarth, René; Schach, René; Sonnabend, Kerstin

    2015-01-01

    We present a nucleosynthesis sensitivity study for the $\\gamma$-process in a Supernova type II model within the NuGrid research platform. The simulations aimed at identifying the relevant local production and destruction rates for the p-nuclei of molybdenum and at determining the sensitivity of the final abundances to these rates. We show that local destruction rates strongly determine the abundance of $^{92}$Mo and $^{94}$Mo, and quantify the impact.

  20. Effect of arsenic on the optical properties of GaSb-based type II quantum wells with quaternary GaInAsSb layers

    SciTech Connect (OSTI)

    Janiak, F. Motyka, M.; S?k, G.; Dyksik, M.; Ryczko, K.; Misiewicz, J.; Weih, R.; Höfling, S.; Kamp, M.; Patriarche, G.

    2013-12-14

    Optical properties of molecular beam epitaxially grown type II “W” shaped GaSb/AlSb/InAs/GaIn(As)Sb/InAs/AlSb/GaSb quantum wells (QWs) designed for the active region of interband cascade lasers have been investigated. Temperature dependence of Fourier-transformed photoluminescence and photoreflectance was employed to probe the effects of addition of arsenic into the original ternary valence band well of GaInSb. It is revealed that adding arsenic provides an additional degree of freedom in terms of band alignment and strain tailoring and allows enhancing the oscillator strength of the active type II transition. On the other hand, however, arsenic incorporation apparently also affects the structural and optical material quality via generating carrier trapping states at the interfaces, which can deteriorate the radiative efficiency. These have been evidenced in several spectroscopic features and are also confirmed by cross-sectional transmission electron microscopy images. While arsenic incorporation into type II QWs is a powerful heterostructure engineering tool for optoelectronic devices, a compromise has to be found between ideal band structure properties and high quality morphological properties.

  1. Type II Cepheids in the Milky Way disc. Chemical composition of two new W Vir stars: DD Vel and HQ Car

    E-Print Network [OSTI]

    Lemasle, B; Bono, G; François, P; Saviane, I; Yegorova, I; Genovali, K; Inno, L; Galazutdinov, G; da Silva, R

    2015-01-01

    A robust classification of Cepheids into their different sub-classes and, in particular, between classical and Type II Cepheids, is necessary to properly calibrate the period-luminosity relations and for populations studies in the Galactic disc. Type II Cepheids are, however, very diverse, and classifications based either on intrinsic (period, light curve) or external parameters (e.g., [Fe/H], |z|) do not provide a unique classification. We want to ascertain the classification of two Cepheids, HQ Car and DD Vel, that are sometimes classified as classical Cepheids and sometimes as Type II Cepheids. To achieve this goal, we examine both their chemical composition and the presence of specific features in their spectra. We find emission features in the H{\\alpha} and in the 5875.64 {\\AA} He I lines that are typical of W Vir stars. The [Na/Fe] (or [Na/Zn]) abundances are typical of thick-disc stars, while BL Her stars are Na-overabundant ([Na/Fe]>+0.5 dex). Finally, the two Cepheids show a possible (HQ Car) or prob...

  2. PROBING THE LOW-REDSHIFT STAR FORMATION RATE AS A FUNCTION OF METALLICITY THROUGH THE LOCAL ENVIRONMENTS OF TYPE II SUPERNOVAE

    SciTech Connect (OSTI)

    Stoll, R.; Stanek, K. Z.; Pogge, R. W. [Department of Astronomy, Ohio State University, 140 West 18th Avenue, Columbus, OH 43210-1173 (United States); Prieto, J. L. [Department of Astrophysical Sciences, Princeton University, 4 Ivy Lane, Peyton Hall, Princeton, NJ 08544 (United States)

    2013-08-10

    Type II supernovae (SNe) can be used as a star formation tracer to probe the metallicity distribution of global low-redshift star formation. We present oxygen and iron abundance distributions of Type II SN progenitor regions that avoid many previous sources of bias. Because iron abundance, rather than oxygen abundance, is of key importance for the late stage evolution of the massive stars that are the progenitors of core-collapse supernovae, and because iron enrichment lags oxygen enrichment, we find a general conversion from oxygen abundance to iron abundance. The distributions we present here are the best yet observational standard of comparison for evaluating how different classes of supernovae depend on progenitor metallicity. We spectroscopically measure the gas-phase oxygen abundance near a representative subsample of the hosts of Type II SNe from the first-year Palomar Transient Factory (PTF) SN search, using a combination of Sloan Digital Sky Survey (SDSS) spectra near the SN location (9 hosts) and new longslit spectroscopy (25 hosts). The median metallicity of these 34 hosts at or near the SN location is 12+log(O/H) = 8.65, with a median error of 0.09. The median host galaxy stellar mass from fits to SDSS photometry is 10{sup 9.9} M{sub Sun }. They do not show a systematic offset in metallicity or mass from a redshift-matched sample of the MPA/JHU value-added catalog. In contrast to previous SN host metallicity studies, this sample is drawn from a single survey. It is also drawn from an areal rather than a targeted survey, so SNe in the lowest-mass galaxies are not systematically excluded. Indeed, the PTF SN search has a slight bias toward following up transients in low mass galaxies. The progenitor region metallicity distribution we find is statistically indistinguishable from the metallicity distribution of Type II SN hosts found by targeted surveys and by samples from multiple surveys with different selection functions. Using the relationship between iron and oxygen abundances found for Milky Way disk, bulge, and halo stars, we translate our distribution of Type II SN environments as a function of oxygen abundance into an estimate of the iron abundance, since iron varies more steeply than oxygen. We find that though this sample spans only 0.65 dex in oxygen abundance, the gap between the iron and oxygen abundance is 50% wider at the low-metallicity end of our sample than at the high-metallicity end.

  3. All-vapor processing of p-type tellurium-containing II-VI semiconductor and ohmic contacts thereof

    DOE Patents [OSTI]

    McCandless, Brian E. (Elkton, MD)

    2001-06-26

    An all dry method for producing solar cells is provided comprising first heat-annealing a II-VI semiconductor; enhancing the conductivity and grain size of the annealed layer; modifying the surface and depositing a tellurium layer onto the enhanced layer; and then depositing copper onto the tellurium layer so as to produce a copper tellurium compound on the layer.

  4. Novel Contrast Mechanism in Cross-Sectional Scanning Tunneling Microscopy of GaSb/GaAs Type-II Nanostructures

    E-Print Network [OSTI]

    Feenstra, Randall

    very interesting both for fundamental physics23 and applications as e.g. charge storage devices24-II Nanostructures R. Timm,1, R. M. Feenstra,2 H. Eisele,1 A. Lenz,1 L. Ivanova,1 E. Lenz,3 and M. D¨ahne1 1, sharply defined contrast of the nanostructure at negative sample bias, but a smoothly broadened contrast

  5. Fuel Cell School Buses: Report to Congress

    Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

    Activities, Progress, and Plans: Report to Congress ii December 2008 Fuel Cell School Buses Report to Congress Fuel Cell School Buses: Report to Congress Preface This Department of...

  6. Low-frequency type II radio detections and coronagraph data to describe and forecast the propagation of 71 CMEs/shocks

    E-Print Network [OSTI]

    Cremades, H; Cyr, O C St; Xie, H; Kaiser, M L; Gopalswamy, N

    2015-01-01

    The vulnerability of technology on which present society relies demands that a solar event, its time of arrival at Earth, and its degree of geoeffectiveness be promptly forecasted. Motivated by improving predictions of arrival times at Earth of shocks driven by coronal mass ejections (CMEs), we have analyzed 71 Earth-directed events in different stages of their propagation. The study is primarily based on approximated locations of interplanetary (IP) shocks derived from type II radio emissions detected by the Wind/WAVES experiment during 1997-2007. Distance-time diagrams resulting from the combination of white-light corona, IP type II radio, and in situ data lead to the formulation of descriptive profiles of each CME's journey toward Earth. Furthermore, two different methods to track and predict the location of CME-driven IP shocks are presented. The linear method, solely based on Wind/WAVES data, arises after key modifications to a pre-existing technique that linearly projects the drifting low-frequency type...

  7. Assignment Types UTS LIBRARY

    E-Print Network [OSTI]

    University of Technology, Sydney

    Assignment Types UTS LIBRARY February 2013 Academic Writing Guide Part 2 ­ Assignment Types: This section outlines the basic types of written assignments, providing structural elements and examples. #12;2 II. Assignment Types 1. Essay Writing

  8. Reprocessing the Hipparcos data for evolved giant stars II. Absolute magnitudes for the R-type carbon stars

    E-Print Network [OSTI]

    G. R. Knapp; D. Pourbaix; A. Jorissen

    2001-03-09

    The Hipparcos Intermediate Astrometric Data for carbon stars have been reprocessed using an algorithm which provides an objective criterion for rejecting anomalous data points and constrains the parallax to be positive. New parallax solutions have been derived for 317 cool carbon stars, mostly of types R and N. In this paper we discuss the results for the R stars. The most important result is that the early R stars (i.e., R0 - R3) have absolute magnitudes and V-K colors locating them among red clump giants in the Hertzsprung-Russell diagram. Stars with subtypes R4 - R9 tend to be cooler and have similar luminosity to the N-type carbon stars, as confirmed by their position in the (J-H, H-K) color-color diagram. The sample of early R-type stars selected from the Hipparcos Catalogue appears to be approximately complete to magnitude K_0 ~ 7, translating into a completeness distance of 600 pc if all R stars had M_K= -2 (400 pc if M_K= -1). With about 30 early R-type stars in that volume, they comprise about 0.04% (0.14% for M_K= -1) of the red clump stars in the solar neighborhood. Identification with the red clump locates these stars at the helium core burning stage of stellar evolution, while the N stars are on the asymptotic giant branch, where helium shell burning occurs. The present analysis suggests that for a small fraction of the helium core burning stars (far lower than the fraction of helium shell-burning stars), carbon produced in the interior is mixed to the atmosphere in sufficient quantities to form a carbon star.

  9. Chap. II : Les structures

    E-Print Network [OSTI]

    Poinsot, Laurent

    Chap. II : Les objets structur´es Laurent Poinsot Chap. II : Les objets structur´es Laurent Poinsot 12 f´evrier 2009 #12;Chap. II : Les objets structur´es Laurent Poinsot Les objets structur´es Pour de types "structur´es". #12;Chap. II : Les objets structur´es Laurent Poinsot Les objets structur´es

  10. Spectroscopic and photometric analysis of the early-type spectroscopic binary HD 161853 in the centre of an H II region

    E-Print Network [OSTI]

    Gamen, R; Barbá, R H; Arias, J I; Apellániz, J Maíz; Walborn, N R; Sota, A; Alfaro, E J

    2015-01-01

    We study the O-type star HD 161853, which has been noted as a probable double-lined spectroscopic binary system. We secured high-resolution spectra of HD 161853 during the past nine years. We separated the two components in the system and measured their respective radial velocities for the first time. We confirm that HD 161853 is an $\\sim$1 Ma old binary system consisting of an O8 V star ($M_{\\rm A,RV} \\geq 22$ M$_\\odot$) and a B1--3 V star ($M_{\\rm B,RV} \\geq 7.2$ M$_\\odot$) at about 1.3 kpc. From the radial velocity curve, we measure an orbital period $P$ = 2.66765$\\pm$0.00001 d and an eccentricity $e$ = 0.121$\\pm$0.007. Its $V$-band light curve is constant within 0.014 mag and does not display eclipses, from which we impose a maximum orbital inclination $i=54$ deg. HD 161853 is probably associated with an H II region and a poorly investigated very young open cluster. In addition, we detect a compact emission region at 50 arcsec to HD 161853 in 22$\\mu$m-WISE and 24$\\mu$m-Spitzer images, which may be identif...

  11. Dilepton events with displaced vertices, double beta decay, and resonant leptogenesis with Type-II seesaw dominance, TeV scale $Z'$ and RH neutrinos

    E-Print Network [OSTI]

    Nayak, Bidyut Prava

    2015-01-01

    In a class of Type-II seesaw dominated $SO(10)$ models proposed recently with heavy neutrinos, extra $Z'$ boson, and resonant leptogenesis, at first we show that the lightest first generation sterile neutrino that mediates dominant contributions to neutrinoless double beta decay also generates the displaced vertex leading to verifiable like-sign di-electron as well as di-muon production events outside the LHC detectors having suppressed standard model back-ground and missing energy. Resonant leptogenesis in this case is implemented by a pair of quasi-degenerate sterile neutrinos of the second and the third generations having masses of ${\\cal O}(500)$ GeV. Then we predict a new alternative scenario where the models allow the second generation sterile neutrino mass to be ${\\cal O}(10)$ GeV capable of mediating the dominant double beta decay as well as the displaced vertices for significantly improved number of like-sign dilepton events in different channels. Resonant leptogenesis in this alternative scenario is...

  12. sessions II and High School

    E-Print Network [OSTI]

    Walker, Lawrence R.

    certification. 20 Upper Division Biology Credits 07/11 MATH 95 Introductory Algebra Math Placement Testing ACT MATH 96 Intermediate Algebra Math Placement Testing ACT 20 SAT 500 MPT 12 UNLV Chemistry; MATH 127 Precalculus I Math Placement Testing ACT 25 SAT 560 MPT 26 MATH 181 Calculus I Math Placement

  13. Nucleosynthesis in Type II Supernovae

    E-Print Network [OSTI]

    K. Nomoto; M. Hashimoto; T. Tsujimoto; F. -K. Thielemann; N. Kishimoto; Y. Kubo

    1997-06-03

    Presupernova evolution and explosive nucleosynthesis in massive stars for main-sequence masses from 13 $M_\\odot$ to 70 $M_\\odot$ are calculated. We examine the dependence of the supernova yields on the stellar mass, $^{12}C(\\alpha, \\gamma) ^{16}O}$ rate, and explosion energy. The supernova yields integrated over the initial mass function are compared with the solar abundances.

  14. Phosphatidylinositol 5-phosphate 4-kinase type II beta is required for vitamin D receptor-dependent E-cadherin expression in SW480 cells

    SciTech Connect (OSTI)

    Kouchi, Zen, E-mail: zkouchi@toyaku.ac.jp [Laboratory of Genome and Biosignals, Tokyo University of Pharmacy and Life Sciences, 1432-1 Horinouchi, Hachioji-city, Tokyo 192-0392 (Japan)] [Laboratory of Genome and Biosignals, Tokyo University of Pharmacy and Life Sciences, 1432-1 Horinouchi, Hachioji-city, Tokyo 192-0392 (Japan); Fujiwara, Yuki [Laboratory of Genome and Biosignals, Tokyo University of Pharmacy and Life Sciences, 1432-1 Horinouchi, Hachioji-city, Tokyo 192-0392 (Japan)] [Laboratory of Genome and Biosignals, Tokyo University of Pharmacy and Life Sciences, 1432-1 Horinouchi, Hachioji-city, Tokyo 192-0392 (Japan); Yamaguchi, Hideki [Division of Metastasis and Invasion Signaling, National Cancer Center Research Institute, 5-1-1 Tsukiji, Chuo-ku, Tokyo 104-0045 (Japan) [Division of Metastasis and Invasion Signaling, National Cancer Center Research Institute, 5-1-1 Tsukiji, Chuo-ku, Tokyo 104-0045 (Japan); PRESTO, Japan Science and Technology Agency, 4-1-8 Honcho, Kawaguchi-city, Saitama 332-0012 (Japan); Nakamura, Yoshikazu; Fukami, Kiyoko [Laboratory of Genome and Biosignals, Tokyo University of Pharmacy and Life Sciences, 1432-1 Horinouchi, Hachioji-city, Tokyo 192-0392 (Japan)] [Laboratory of Genome and Biosignals, Tokyo University of Pharmacy and Life Sciences, 1432-1 Horinouchi, Hachioji-city, Tokyo 192-0392 (Japan)

    2011-05-20

    Highlights: {yields} We analyzed Phosphatidylinositol 5-phosphate kinase II{beta} (PIPKII{beta}) function in cancer. {yields} PIPKII{beta} is required for vitamin D receptor-mediated E-cadherin upregulation in SW480. {yields} PIPKII{beta} suppresses cellular motility through E-cadherin induction in SW480 cells. {yields} Nuclear PIP{sub 2} but not plasma membrane-localized PIP{sub 2} mediates E-cadherin upregulation. -- Abstract: Numerous epidemiological data indicate that vitamin D receptor (VDR) signaling induced by its ligand or active metabolite 1{alpha},25-dihydroxyvitamin D{sub 3} (1{alpha},25(OH){sub 2}D{sub 3}) has anti-cancer activity in several colon cancers. 1{alpha},25(OH){sub 2}D{sub 3} induces the epithelial differentiation of SW480 colon cancer cells expressing VDR (SW480-ADH) by upregulating E-cadherin expression; however, its precise mechanism remains unknown. We found that phosphatidylinositol-5-phosphate 4-kinase type II beta (PIPKII{beta}) but not PIPKII{alpha} is required for VDR-mediated E-cadherin induction in SW480-ADH cells. The syntenin-2 postsynaptic density protein/disc large/zona occludens (PDZ) domain and pleckstrin homology domain of phospholipase C-delta1 (PLC{delta}1 PHD) possess high affinity for phosphatidylinositol-4,5-bisphosphate (PI(4,5)P{sub 2}) mainly localized to the nucleus and plasma membrane, respectively. The expression of syntenin-2 PDZ but not PLC{delta}1 PHD inhibited 1{alpha},25(OH){sub 2}D{sub 3}-induced E-cadherin upregulation, suggesting that nuclear PI(4,5)P{sub 2} production mediates E-cadherin expression through PIPKII{beta} in a VDR-dependent manner. PIPKII{beta} is also involved in the suppression of the cell motility induced by 1{alpha},25(OH){sub 2}D{sub 3}. These results indicate that PIPKII{beta}-mediated PI(4,5)P{sub 2} signaling is important for E-cadherin upregulation and inhibition of cellular motility induced by VDR activation.

  15. Determination of lateral size distribution of type-II ZnTe/ZnSe stacked submonolayer quantum dots via spectral analysis of optical signature of the Aharanov-Bohm excitons

    SciTech Connect (OSTI)

    Ji, Haojie; Dhomkar, Siddharth; Roy, Bidisha; Kuskovsky, Igor L.; Shuvayev, Vladimir; Deligiannakis, Vasilios; Tamargo, Maria C.; Ludwig, Jonathan; Smirnov, Dmitry; Wang, Alice

    2014-10-28

    For submonolayer quantum dot (QD) based photonic devices, size and density of QDs are critical parameters, the probing of which requires indirect methods. We report the determination of lateral size distribution of type-II ZnTe/ZnSe stacked submonolayer QDs, based on spectral analysis of the optical signature of Aharanov-Bohm (AB) excitons, complemented by photoluminescence studies, secondary-ion mass spectroscopy, and numerical calculations. Numerical calculations are employed to determine the AB transition magnetic field as a function of the type-II QD radius. The study of four samples grown with different tellurium fluxes shows that the lateral size of QDs increases by just 50%, even though tellurium concentration increases 25-fold. Detailed spectral analysis of the emission of the AB exciton shows that the QD radii take on only certain values due to vertical correlation and the stacked nature of the QDs.

  16. IEEE TRANSACTIONS ON APPLIED SUPERCONDUCTIVITY, VOL. 14, NO. 1, MARCH 2004 69 AC Losses in Type-II Superconductors Induced by

    E-Print Network [OSTI]

    Prigozhin, Leonid

    -II superconductors in power transmission lines, current leads, fault current limiters, magnetic shields, bearings losses in flywheels, electric motors, magnetic shields, etc. Index Terms--AC losses, asymptotic solution

  17. New approaches for modeling type Ia supernovae

    E-Print Network [OSTI]

    Zingale, Michael; Almgren, Ann S.; Bell, John B.; Day, Marcus S.; Rendleman, Charles A.; Woosley, Stan

    2007-01-01

    runaway in Type Ia supernovae: How to run away? oIgnition in Type Ia Supernovae. II. A Three- dimensionalnumber modeling of type Ia supernovae. I. hydrodynamics.

  18. Carbon abundances of early B-type stars in the solar vicinity. Non-LTE line-formation for C II/III/IV and self-consistent atmospheric parameters

    E-Print Network [OSTI]

    M. F. Nieva; N. Przybilla

    2007-11-23

    Precise determinations of the chemical composition in early B-type stars consitute fundamental observational constraints on stellar and galactochemical evolution. Carbon is one of the most abundant metals in the Universe but analyses in early-type stars show inconclusive results, like large discrepancies between analyses of different lines in C II, a failure to establish the C II/III ionization balance and the derivation of systematically lower abundances than from other objects. We present a comprehensive and robust C II/III/IV model for non-LTE line-formation calculations based on carefully selected atomic data. The model is calibrated with high-S/N spectra of six apparently slow-rotating early B-type dwarfs and giants, which cover a wide parameter range and are randomly distributed in the solar neighbourhood. A self-consistent quantitative spectrum analysis is performed using an extensive iteration scheme to determine stellar atmospheric parameters and to select the appropriate atomic data used for the derivation of chemical abundances. We establish the carbon ionization balance for all sample stars based on a unique set of input atomic data, achieving consistency for all modelled lines. Highly accurate atmospheric parameters and a homogeneous carbon abundance with reduced systematic errors are derived. This results in a present-day stellar carbon abundance in the solar neighbourhood, which is in good agreement with recent determinations of the solar value and with the gas-phase abundance of the Orion H II region. The homogeneous present-day carbon abundance also conforms with predictions of chemical-evolution models for the Galaxy. The present approach allows us to constrain the effects of systematic errors on fundamental parameters and abundances. (abridged)

  19. Approved Module Information for AM20CP, 2014/5 Module Title/Name: Numerical Methods II Module Code: AM20CP

    E-Print Network [OSTI]

    Neirotti, Juan Pablo

    Approved Module Information for AM20CP, 2014/5 Module Title/Name: Numerical Methods II Module Code: AM20CP School: Engineering and Applied Science Module Type: Standard Module New Module? No Module Credits: 10 Module Management Information Module Leader Name Juan Neirotti Email Address neirotjp

  20. Approved Module Information for CE4014, 2014/5 Module Title/Name: Advanced Reaction Engineering II Module Code: CE4014

    E-Print Network [OSTI]

    Neirotti, Juan Pablo

    Approved Module Information for CE4014, 2014/5 Module Title/Name: Advanced Reaction Engineering II Module Code: CE4014 School: Engineering and Applied Science Module Type: Standard Module New Module? No Module Credits: 10 Module Management Information Module Leader Name Feroz Kabir Email Address kabirf

  1. Eight-band k·p modeling of InAs/InGaAsSb type-II W-design quantum well structures for interband cascade lasers emitting in a broad range of mid infrared

    SciTech Connect (OSTI)

    Ryczko, K.; S?k, G.; Misiewicz, J. [Institute of Physics, Wroc?aw University of Technology, Wybrze?e Wyspia?skiego 27, 50-370 Wroc?aw (Poland)

    2013-12-14

    Band structure properties of the type-II W-design AlSb/InAs/GaIn(As)Sb/InAs/AlSb quantum wells have been investigated theoretically in a systematic manner and with respect to their use in the active region of interband cascade laser for a broad range of emission in mid infrared between below 3 to beyond 10??m. Eight-band k·p approach has been utilized to calculate the electronic subbands. The fundamental optical transition energy and the corresponding oscillator strength have been determined in function of the thickness of InAs and GaIn(As)Sb layers and the composition of the latter. There have been considered active structures on two types of relevant substrates, GaSb and InAs, introducing slightly modified strain conditions. Additionally, the effect of external electric field has been taken into account to simulate the conditions occurring in the operational devices. The results show that introducing arsenic as fourth element into the valence band well of the type-II W-design system, and then altering its composition, can efficiently enhance the transition oscillator strength and allow additionally increasing the emission wavelength, which makes this solution prospective for improved performance and long wavelength interband cascade lasers.

  2. Topoisomerase II Structure Suggests Novel DNA Cleavage Mechanism

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    Topoisomerase II Structure Suggests Novel DNA Cleavage Mechanism Print Type II topoisomerases are molecular machines that regulate DNA supercoiling and separate interlocked...

  3. 86 GHz SiO maser survey of late-type stars in the Inner Galaxy II. Infrared photometry of the SiO Target Stars

    E-Print Network [OSTI]

    M. Messineo; H. J. Habing; K. M. Menten; A. Omont; L. O. Sjouwerman

    2004-01-14

    We present a compilation and study of DENIS, 2MASS, ISOGAL, MSX and IRAS 1--25 micron photometry for a sample of 441 late-type stars in the inner Galaxy, which we previously searched for 86 GHz SiO maser emission (Messineo et al.2002). The comparison of the DENIS and 2MASS J and Ks magnitudes shows that most of the SiO targets are indeed variable stars. The MSX colours and the IRAS [12]-[25] colour of our SiO targets are consistent with those of Mira type stars with dust silicate feature at 9.7 micron feature in emission, indicating only a moderate mass-loss rate.

  4. [Type text] Page 1 of 13

    E-Print Network [OSTI]

    Nicholson, Bruce J.

    [Type text] Page 1 of 13 Nguyen, C, April 10, 2009 School of Health Professions Faculty Government BYLAWS OF THE SCHOOL OF HEALTH PROFESSIONS THE UNIVERSITY OF TEXAS HEALTH SCIENCE CENTER AT SAN be the School of Health Professions Faculty Assembly and the School of Health Professions Faculty Council

  5. The Westerbork HI Survey of Spiral and Irregular Galaxies II. R-Band Surface Photometry of Late-type Dwarf Galaxies

    E-Print Network [OSTI]

    R. A. Swaters; M. Balcells

    2002-04-30

    R-band surface photometry is presented for 171 late-type dwarf and irregular galaxies. For a subsample of 46 galaxies B-band photometry is presented as well. We present surface brightness profiles as well as isophotal and photometric parameters including magnitudes, diameters and central surface brightnesses. Absolute photometry is accurate to 0.1 mag or better for 77% of the sample. For over 85% of the galaxies the radial surface brightness profiles are consistent with published data within the measured photometric uncertainty. For most of the galaxies in the sample HI data have been obtained with the Westerbork Synthesis Radio Telescope. The galaxies in our sample are part of the WHISP project (Westerbork HI Survey of Spiral and Irregular Galaxies), which aims at mapping about 500 nearby spiral and irregular galaxies in HI. The availability of HI data makes this data set useful for a wide range of studies of the structure, dark matter content and kinematics of late-type dwarf galaxies.

  6. Effect of sidewall surface recombination on the quantum efficiency in a Y{sub 2}O{sub 3} passivated gated type-II InAs/GaSb long-infrared photodetector array

    SciTech Connect (OSTI)

    Chen, G.; Hoang, A. M.; Bogdanov, S.; Haddadi, A.; Darvish, S. R.; Razeghi, M., E-mail: razeghi@eecs.northwestern.edu [Center for Quantum Devices, Department of Electrical Engineering and Computer Science, Northwestern University, Evanston, Illinois 60208 (United States)

    2013-11-25

    Y{sub 2}O{sub 3} was applied to passivate a long-wavelength infrared type-II superlattice gated photodetector array with 50% cut-off wavelength at 11??m, resulting in a saturated gate bias that was 3 times lower than in a SiO{sub 2} passivated array. Besides effectively suppressing surface leakage, gating technique exhibited its ability to enhance the quantum efficiency of 100?×?100??m size mesa from 51% to 57% by suppressing sidewall surface recombination. At 77?K, the gated photodetector showed dark current density and resistance-area product at ?300?mV of 2.5?×?10{sup ?5} A/cm{sup 2} and 1.3?×?10{sup 4}???cm{sup 2}, respectively, and a specific detectivity of 1.4?×?10{sup 12} Jones.

  7. PRODUCTION OF EXOTIC ATOMS MARK ELLERMANN II

    E-Print Network [OSTI]

    Bertulani, Carlos A. - Department of Physics and Astronomy, Texas A&M University

    #12;PRODUCTION OF EXOTIC ATOMS by MARK ELLERMANN II Submitted to the Faculty of the Graduate School OF SCIENCE December 2010 #12;PRODUCTION OF EXOTIC ATOMS Approved: Adviser Dean of the College of Arts & Science Dean of Graduate Studies and Research ii #12;ABSTRACT PRODUCTION OF EXOTIC ATOMS Mark Ellermann

  8. Calculation of two-centre two-electron integrals over Slater-type orbitals revisited. II. Neumann expansion of the exchange integrals

    E-Print Network [OSTI]

    Micha? Lesiuk; Robert Moszynski

    2015-01-08

    In this paper we consider calculation of two-centre exchange integrals over Slater-type orbitals (STOs). We apply the Neumann expansion of the Coulomb interaction potential and consider calculation of all basic quantities which appear in the resulting expression. Analytical closed-form equations for all auxiliary quantities have already been known but they suffer from large digital erosion when some of the parameters are large or small. We derive two differential equations which are obeyed by the most di?cult basic integrals. Taking them as a starting point, useful series expansions for small parameter values or asymptotic expansions for large parameter values are systematically derived. The resulting novel expansions replace the corresponding analytical expressions when the latter introduce significant cancellations. Additionally, we reconsider numerical integration of some necessary quantities and present a new way to calculate the integrand with a controlled precision. All proposed methods are combined to lead to a general, stable algorithm. We perform extensive numerical tests of the introduced expressions to verify their validity and usefulness. Advances reported here provide methodology to compute two-electron exchange integrals over STOs for a broad range of the nonlinear parameters and large angular momenta.

  9. Photometric and spectroscopic studies of massive binaries in the large Magellanic Cloud. II. Three O-type systems in the 30 Dor region

    SciTech Connect (OSTI)

    Morrell, Nidia I. [Las Campanas Observatory, Carnegie Observatories, Casilla 601, La Serena (Chile); Massey, Philip; Neugent, Kathryn F. [Lowell Observatory, 1400 West Mars Hill Road, Flagstaff, AZ 86001 (United States); Penny, Laura R. [Department of Physics and Astronomy, The College of Charleston, Charleston, SC 29424 (United States); Gies, Douglas R., E-mail: nmorrell@lco.cl, E-mail: phil.massey@lowell.edu, E-mail: kneugent@lowell.edu, E-mail: penny@cofc.edu, E-mail: gies@chara.gsu.edu [Center for High Angular Resolution Astronomy and Department of Physics and Astronomy, Georgia State University, P.O. Box 5060, Atlanta, GA 30302 (United States)

    2014-07-10

    This is the second paper in a series devoted to the study of massive binary systems in the Large Magellanic Cloud (LMC). We mainly aim to provide accurate data that constrains the mass-luminosity relation for the most massive stars but also to address the long lasting problem known as the 'mass discrepancy'. We present here our results for three binaries (LMC 169782, LMC 171520, and [P93] 921) harboring the earliest O-type components—ranging from O4 V to O6.5 V—among our sample of 17 systems. Our photometry provided accurate periods for the studied systems, allowing the spectroscopic observations to be performed at selected phases where the radial velocity separation between binary components is larger. Following the procedure outlined in our first paper of this series, after solving the radial velocity curves for orbital parameters, we used tomographic reconstruction to obtain the individual spectra of each star, from which we determined effective temperatures via a model atmosphere fitting with FASTWIND. This information, combined with the light-curve analysis that was performed with GENSYN, enabled the determination of absolute masses, radii, and bolometric luminosities that are compared with those predicted by modern stellar evolutionary models finding that they agree within the uncertainties. Nevertheless, the comparison seems to confirm the small differences found in the first paper of this series in the sense that the evolutionary masses are slightly larger than the Keplerian ones, with differences averaging ?10%, or alternatively, the stellar evolutionary models predict luminosities that are somewhat lower than observed. Still, the overall agreement between the current evolutionary models and the empirically determined stellar parameters is remarkable.

  10. THE TIP OF THE RED GIANT BRANCH DISTANCES TO TYPE Ia SUPERNOVA HOST GALAXIES. II. M66 AND M96 IN THE LEO I GROUP

    SciTech Connect (OSTI)

    Lee, Myung Gyoon; Jang, In Sung, E-mail: mglee@astro.snu.ac.kr, E-mail: isjang@astro.snu.ac.kr [Astronomy Program, Department of Physics and Astronomy, Seoul National University, Gwanak-gu, Seoul 151-742 (Korea, Republic of)

    2013-08-10

    M66 and M96 in the Leo I Group are nearby spiral galaxies hosting Type Ia supernovae (SNe Ia). We estimate the distances to these galaxies from the luminosity of the tip of the red giant branch (TRGB). We obtain VI photometry of resolved stars in these galaxies from F555W and F814W images in the Hubble Space Telescope archive. From the luminosity function of these red giants, we find the TRGB I-band magnitude to be I{sub TRGB} = 26.20 {+-} 0.03 for M66 and 26.21 {+-} 0.03 for M96. These values yield distance modulus (m - M){sub 0} = 30.12 {+-} 0.03(random) {+-} 0.12(systematic) for M66 and (m - M){sub 0} = 30.15 {+-} 0.03(random) {+-} 0.12(systematic) for M96. These results show that they are indeed the members of the same group. With these results we derive absolute maximum magnitudes of two SNe (SN 1989B in M66 and SN 1998bu in M96). V-band magnitudes of these SNe Ia are {approx}0.2 mag fainter than SN 2011fe in M101, one of the nearest recent SNe Ia. We also derive near-infrared magnitudes for SN 1998bu. Optical magnitudes of three SNe Ia (SN 1989B, SN 1998bu, and SN 2011fe) based on TRGB analysis yield a Hubble constant, H{sub 0} = 68.4 {+-} 2.6(random) {+-} 3.7(systematic) km s{sup -1} Mpc{sup -1}. This value is similar to the values derived from recent WMAP9 results, H{sub 0} = 69.32 {+-} 0.80 km s{sup -1} Mpc{sup -1}, and from Planck results, H{sub 0} = 67.3 {+-} 1.2 km s{sup -1} Mpc{sup -1}, but smaller than other recent determinations based on Cepheid calibration for SNe Ia luminosity, H{sub 0} = 74 {+-} 3 km s{sup -1} Mpc{sup -1}.

  11. swinburne.edu.au VET in Schools

    E-Print Network [OSTI]

    Liley, David

    swinburne.edu.au VET in Schools Certificate II in Engineering Studies (Mechatronics) Course code ­ Civil, Mechanical, Robotics & Mechatronics, or Electrical Advanced Diploma of Electronics and Communications Engineering Bachelor of Engineering ­ Civil, Mechanical, or Robotics & Mechatronics #12;

  12. The Graduate School BME Biomedical Engineering

    E-Print Network [OSTI]

    MacAdam, Keith

    : Consent of instructor. BME 605 BIOMEDICAL SIGNAL PROCESSING I. (3) Continuous and discrete signals 440 or equivalent. BME 615 BIOMEDICAL SIGNAL PROCESSING II. (3) StochasticprocessesThe Graduate School BME Biomedical Engineering KEY: # = new course * = course changed = course

  13. Patterns in Illinois Educational School Data

    E-Print Network [OSTI]

    Stevens, Cacey S; Nagel, Sidney R

    2015-01-01

    We examine Illinois educational data from standardized exams and analyze primary factors affecting the achievement of public school students. We focus on the simplest possible models: representation of data through visualizations and regressions on single variables. Exam scores are shown to depend on school type, location, and poverty concentration. For most schools in Illinois, student test scores decline linearly with poverty concentration. However Chicago must be treated separately. Selective schools in Chicago, as well as some traditional and charter schools, deviate from this pattern based on poverty. For any poverty level, Chicago schools perform better than those in the rest of Illinois. Selective programs for gifted students show high performance at each grade level, most notably at the high school level, when compared to other Illinois school types. The case of Chicago charter schools is more complex. In the last six years, their students' scores overtook those of students in traditional Chicago high...

  14. About APPLE II Operation

    SciTech Connect (OSTI)

    Schmidt, T.; Zimoch, D.

    2007-01-19

    The operation of an APPLE II based undulator beamline with all its polarization states (linear horizontal and vertical, circular and elliptical, and continous variation of the linear vector) requires an effective description allowing an automated calculation of gap and shift parameter as function of energy and operation mode. The extension of the linear polarization range from 0 to 180 deg. requires 4 shiftable magnet arrrays, permitting use of the APU (adjustable phase undulator) concept. Studies for a pure fixed gap APPLE II for the SLS revealed surprising symmetries between circular and linear polarization modes allowing for simplified operation. A semi-analytical model covering all types of APPLE II and its implementation will be presented.

  15. The impact of charter schools in Texas 

    E-Print Network [OSTI]

    Booker, Toby Kevin

    2009-06-02

    This dissertation examines the effects of charter schools in Texas, using data from the Texas Education Agency for 190 charter schools and over 60,000 charter students. In Chapter II we examine charter effect test score gains for charter students...

  16. Photosystem II

    ScienceCinema (OSTI)

    James Barber

    2010-09-01

    James Barber, Ernst Chain Professor of Biochemistry at Imperial College, London, gives a BSA Distinguished Lecture titled, "The Structure and Function of Photosystem II: The Water-Splitting Enzyme of Photosynthesis."

  17. Jonathan Barrera Three types: I, II, III

    E-Print Network [OSTI]

    Brutlag, Doug

    and cataracts Sunscreen #12; Code for proteins that are involved in repairing damaged DNA #12; DNA repair

  18. see Type I decision error see Type II decision error

    E-Print Network [OSTI]

    . M ALARA 2-5; 5-52; 8-21, 27; C-8 to 10 alpha () radiation 4-6, 7; 7-15 analysis 7-22 detection background (radiation) activity 5-10, 11 decommissioning 4-13 detection sensitivity 6-37, 39 to 49 ground to 21; A-5 background radiation 4-13 data points 5-25 to 31 P 5-27 r relative shift WRS test 5

  19. Abstract Data Types 5 Algebraic Theory of Abstract Data Types

    E-Print Network [OSTI]

    Berger, Ulrich

    stack top: stack elts The following is an algebra for the signature STACK. Algebra SeqN Carriers N, N43 Part II Abstract Data Types #12;44 5 Algebraic Theory of Abstract Data Types An Abstract Data Type (ADT) is a collection of objects and functions, that is, an algebra, where one ignores how

  20. Tri College 2011 Middle School Team Div I

    E-Print Network [OSTI]

    Hu, Wen-Chen

    Tri College 2011 Middle School Team Div I 1 Ben Franklin 223 2 Schroder Middle GForks 210 3 Horizon;Middle School Team Div II 1 Dilworth-Glydon-Felton 200 2 Mennewaska 185 3 Park River 184 4 Wheaton 167 5 Middle Moorhead 209 4 Discovery 197 5 Sullivan 190 189 Middle School Ind Div I 188 1 Andrew Hu South GF

  1. School of Engineering -School Requirements School of Engineering

    E-Print Network [OSTI]

    Quan, Long

    School of Engineering - School Requirements School of Engineering School Requirements on Doctor outside their programs offered by the School of Engineering. The 3 credits may be satisfied by courses of the School of Engineering at http://www.seng.ust.hk/pg/. In addition to the program requirements

  2. MI FARM TO SCHOOL GRANTEES 2014-2015 PROGRAM YEAR AND PREVIOUS GRANTEES

    E-Print Network [OSTI]

    MI FARM TO SCHOOL GRANTEES 2014-2015 PROGRAM YEAR AND PREVIOUS GRANTEES FOODSYSTEMS.MSU.EDU 2014-2015 GRANTEES School/ district/ program County Current Grant Years as a grantee A&W Daycare Wayne Planning 1 TO SCHOOL GRANTEES (2011/12 ­ 2013/14) School/ district/ program County Grant Type(s) Grant Years All Aboard

  3. EXPERIMENTS with PHOTOVOLTAIC CELLS for high school science students

    E-Print Network [OSTI]

    Oregon, University of

    EXPERIMENTS with PHOTOVOLTAIC CELLS for high school science students By Dick Erickson ­ Pleasant Activity ­ Testing Photovoltaic Cells ..........................5 Expected Observations: ........................................................................................................8 II. LAB ACTIVITY - TESTING PHOTOVOLTAIC CELLS ..................................9 BEFORE YOU START

  4. Teachers and JLab scientists help middle-school science instructors...

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    scientists help middle-school science instructors prepare to teach physics in the 21st century By John Anderson, II, JLab Public Affairs intern August 11, 2003 As part of Jefferson...

  5. Course Title Type Meeting Days & Times Instructor

    E-Print Network [OSTI]

    Raina, Ramesh

    Units CommentsNbr School of Architecture School of Architecture ARC - Architecture ARC 101 The Art of Architecture # 30191 SEC M001 MWF 11:40AM-12:35PM Linder 3.0 ARC 108 Architectural Design II -- Prereq: ARC 107 Louie Staff 3.0 ARC 208 Architectural Design IV -- Prereq: ARC 182 and 207. # 30013 SEC M001 TThF 01

  6. The role of the superintendent as perceived by school administrators and school board presidents in Texas public schools in Region 20 ESC 

    E-Print Network [OSTI]

    Running, Peter John

    2005-02-17

    This study examined the role of the superintendent as it is perceived by school administrators and school board presidents. The study was limited to public schools in Texas located within Region 20 ESC. Responses to a Likert-type instrument were...

  7. SCHOOL of MEDICINE School of Medicine

    E-Print Network [OSTI]

    California at Riverside, University of

    SCHOOL of MEDICINE School of Medicine A next generation med school for the next generation of med students ABOUT THE UCR SCHOOL OF MEDICINE Built upon more than three decades of medical education experience, the new UCR School of Medicine is committed to expanding and diversifying the physician workforce

  8. Artificial Photosynthesis II -

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    II - Artificial Photosynthesis II - Joint Center for Artificial Photosynthesis (JCAP) Simulations NathanLewis.png Schematic of a photoelectrochemical cell being designed to harness...

  9. General Information for Physical Therapy School: Prerequisites for admission to physical therapy school exhibit extreme variation between

    E-Print Network [OSTI]

    Walker, Lawrence R.

    General Information for Physical Therapy School: Prerequisites for admission to physical therapy Chemistry I and II (CHEM 121/121L, CHEM 122/122L) - General Physics I and II (PHYS 151/151L, PHYS 152, 152L, it is not possible to recommend a uniform curriculum that prepares the student for application to all physical

  10. EBR-II Data Digitization

    SciTech Connect (OSTI)

    Yoon, Su-Jong; Rabiti, Cristian; Sackett, John

    2014-08-01

    1. Objectives To produce a validation database out of those recorded signals it will be necessary also to identify the documents need to reconstruct the status of reactor at the time of the beginning of the recordings. This should comprehends the core loading specification (assemblies type and location and burn-up) along with this data the assemblies drawings and the core drawings will be identified. The first task of the project will be identify the location of the sensors, with respect the reactor plant layout, and the physical quantities recorded by the Experimental Breeder Reactor-II (EBR-II) data acquisition system. This first task will allow guiding and prioritizing the selection of drawings needed to numerically reproduce those signals. 1.1 Scopes and Deliverables The deliverables of this project are the list of sensors in EBR-II system, the identification of storing location of those sensors, identification of a core isotopic composition at the moment of the start of system recording. Information of the sensors in EBR-II reactor system was summarized from the EBR-II system design descriptions listed in Section 1.2.

  11. PROTON INDUCED SWELLING IN TYPE 316 STAINLESS STEEL

    E-Print Network [OSTI]

    Srivastava, A.K.

    2010-01-01

    McDonald, Void Formation in Proton- and Nicke1- Irradiatedowned rights. o -iii- PROTON INDUCED SWELLING IN TYPE 316I. II. Introduction Proton Damage Processes A. B.

  12. 1School of Mathematics School of Mathematics

    E-Print Network [OSTI]

    Birmingham, University of

    1School of Mathematics School of Mathematics Studying Mathematics, the beautiful and intriguing language of the universe, opens doors. Dr Chris Good Internet graph #12;2 School of Mathematics Contents Contact details School of Mathematics University of Birmingham Edgbaston, Birmingham B15 2TT United

  13. Time Entry Form Overtime Eligible Staff & Temporaries Harvard Medical School Harvard School of Dental Medicine

    E-Print Network [OSTI]

    Dorf, Martin E.

    Time Entry Form ­ Overtime Eligible Staff & Temporaries Harvard Medical School Harvard School of Dental Medicine Action: Reported Time Prior Period Adjustment Name: Week Ending: Employee ID: Job Title: Dept: Job Rcd #: Sun Mon Tue Wed Thu Fri Sat Time Type Tub Org Fund Activity Sub-Act Root Rate Comments

  14. School of Public Service School of Public Service Statement on Research

    E-Print Network [OSTI]

    Barrash, Warren

    seamlessly incorporate both types of research into their professional lives, and we should expectSchool of Public Service School of Public Service Statement on Research The creation of the SPS offers an opportunity to redefine the scope of research activities for faculty members, professional

  15. SEARCHING FOR NEW HYPERCOMPACT H II REGIONS

    SciTech Connect (OSTI)

    Sanchez-Monge, Alvaro [Osservatorio Astrofisico di Arcetri, INAF, Largo E. Fermi 5, I-50125 Firenze (Italy); Pandian, Jagadheep D. [Institute for Astronomy, University of Hawaii, 2680 Woodlawn Dr., Honolulu, HI 96822 (United States); Kurtz, Stan, E-mail: asanchez@arcetri.astro.it [Centro de RadioastronomIa y Astrofisica, Universidad Nacional Autonoma de Mexico, Apdo. Postal 3-72, 58090 Morelia, Michoacan (Mexico)

    2011-09-20

    Hypercompact (HC) H II regions are, by nature, very young H II regions, associated with the earliest stages of massive star formation. They may represent the transition phase as an early B-type star grows into an O-type star. Unfortunately, so few HC H II regions are presently known that their general attributes and defining characteristics are based on small number statistics. A larger sample is needed for detailed studies and good statistics. Class II methanol masers are one of the best indicators of the early stages of massive star formation. Using the Arecibo Methanol Maser Galactic Plane Survey-the most sensitive blind survey for 6.7 GHz methanol masers to date-we selected 24 HC H II region candidates. We made Expanded Very Large Array continuum observations at 3.6 and 1.3 cm to search for HC H II regions associated with these masers. We identified six potential HC H II regions in our sample based on the presence of optically thick free-free emission. Overall, we find that 30% of the methanol masers have an associated centimeter radio continuum source (separation less than 0.1 pc), which is in general agreement with previous studies.

  16. Sloan Digital Sky Survey II (SDSS-II) Supernova Data

    DOE Data Explorer [Office of Scientific and Technical Information (OSTI)]

    The Sloan Digital Sky Survey (SDSS) is a series of three interlocking imaging and spectroscopic surveys, carried out over an eight-year period with a dedicated 2.5m telescope located at Apache Point Observatory in Southern New Mexico. The SDSS Supernova Survey was one of those three components of SDSS and SDSS-II, a 3-year extension of the original SDSS that operated from July 2005 to July 2008. The Supernova Survey was a time-domain survey, involving repeat imaging of the same region of sky every other night, weather permitting. The primary scientific motivation was to detect and measure light curves for several hundred supernovae through repeat scans of the SDSS Southern equatorial stripe 82 (about 2.5? wide by ~120? long). Over the course of three 3-month campaigns SDSS-II SN discovered and measured multi-band lightcurves for ~500 spectroscopically confirmed Type Ia supernovae in the redshift range z=0.05-0.4. In addition, the project harvested a few hundred light curves for SNe Ia and discovered about 80 spectroscopically confirmed core-collapse supernovae (supernova types Ib/c and II).

  17. STELLAR KINEMATICS AND STRUCTURAL PROPERTIES OF VIRGO CLUSTER DWARF EARLY-TYPE GALAXIES FROM THE SMAKCED PROJECT. II. THE SURVEY AND A SYSTEMATIC ANALYSIS OF KINEMATIC ANOMALIES AND ASYMMETRIES

    SciTech Connect (OSTI)

    Toloba, E.; Guhathakurta, P. [UCO/Lick Observatory, University of California, Santa Cruz, 1156 High Street, Santa Cruz, CA 95064 (United States); Peletier, R. F. [Kapteyn Astronomical Institute, Postbus 800, 9700 AV Groningen (Netherlands); Boselli, A. [Laboratoire d'Astrophysique de Marseille-LAM, Université d'Aix-Marseille and CNRS, UMR 7326, 38 rue F. Joliot-Curie, 13388 Marseille Cedex 13 (France); Lisker, T. [Astronomisches Rechen-Institut, Zentrum für Astronomie der Universität Heidelberg, Mönchhofstraße 12-14, D-69120 Heidelberg (Germany); Falcón-Barroso, J.; Ry?, A. [Instituto de Astrofísica de Canarias, Vía Láctea s/n, La Laguna, Tenerife (Spain); Simon, J. D. [Observatories of the Carnegie Institution for Science, 813 Santa Barbara Street, Pasadena, CA 91101 (United States); Van de Ven, G. [Max Planck Institute for Astronomy, Königstuhl 17, D-69117 Heidelberg (Germany); Paudel, S. [Korea Astronomy and Space Science Institute, Daejeon 305-348 (Korea, Republic of); Emsellem, E. [European Southern Observatory, Karl-Schwarzschild-Strasse 2, D-85748, Garching (Germany); Janz, J. [Centre for Astrophysics and Supercomputing, Swinburne University, Hawthorn, VIC 3122 (Australia); Den Brok, M. [Department of Physics and Astronomy, University of Utah, Salt Lake City, UT 84112 (United States); Gorgas, J. [Departamento de Astrofísica y Física de la Atmósfera, Universidad Complutense de Madrid, E-28040, Madrid (Spain); Hensler, G. [Department of Astrophysics, University of Vienna, Türkenschanzstraße 17, 1180 Vienna (Austria); Laurikainen, E.; Salo, H. [Division of Astronomy, Department of Physics, PO Box 3000, FI-90014 University of Oulu (Finland); Niemi, S.-M., E-mail: toloba@ucolick.org [Mullard Space Science Laboratory, University College London, Holmbury St. Mary, Dorking, Surrey RH5 6NT (United Kingdom)

    2015-01-01

    We present spatially resolved kinematics and global stellar populations and mass-to-light ratios for a sample of 39 dwarf early-type (dE) galaxies in the Virgo cluster studied as part of the SMAKCED stellar absorption-line spectroscopy and imaging survey. This sample is representative of the early-type population in the Virgo cluster in the absolute magnitude range –19.0 < M{sub r} < –16.0 and of all morphological subclasses found in this galaxy population. For each dE, we measure the rotation curve and velocity dispersion profile and fit an analytic function to the rotation curve. We study the significance of the departure of the rotation curve from the best-fit analytic function (poorly fit) and of the difference between the approaching and receding sides of the rotation curve (asymmetry). Our sample includes two dEs with kinematically decoupled cores that have been previously reported. We find that 62 ± 8% (23 out of the 39) of the dEs have a significant anomaly in their rotation curve. Analysis of the images reveals photometric anomalies for most galaxies. However, there is no clear correlation between the significance of the photometric and kinematic anomalies. We measure age-sensitive (H{sub ?} and H{sub ?A}) and metallicity sensitive (Fe4668 and Mgb) Lick spectral indices in the LIS-5 Å system. This population of galaxies exhibits a wide range of ages and metallicities; we also find that 4 dEs show clear evidence of emission partially filling in the Balmer absorption lines. Finally, we estimate the total masses and dark matter fractions of the dEs and plot them in the mass-size, the mass-velocity dispersion, and the fundamental plane scaling relations. The dEs seem to be the bridge between massive early-type galaxies and dSphs, and have a median total mass within the R{sub e} of log M{sub e} = 9.1 ± 0.2 and a median dark matter fraction within the R{sub e} of f {sub DM} = 46 ± 18%. Any formation model for the dE galaxy class must account for this diversity of kinematic and photometric anomalies and stellar populations.

  18. Deep-Sea Research II 52 (2005) 26982714 Mechanisms regulating large-scale seasonal fluctuations in

    E-Print Network [OSTI]

    McGillicuddy Jr., Dennis J.

    2005-01-01

    Deep-Sea Research II 52 (2005) 2698­2714 Mechanisms regulating large-scale seasonal fluctuations Hole, MA 02543, USA b Thayer School of Engineering, Dartmouth College, Hanover, NH 03755, USA c School by ocean currents. Third, the organism is capable of directed motion through the water by virtue of its

  19. 3F6 -Software Engineering and Design Design Patterns (II)

    E-Print Network [OSTI]

    Young, Steve

    3F6 - Software Engineering and Design Handout 7 Design Patterns (II) With Markup Steve Young #12;Design Patterns (II) 1 Observer Pattern Problem We want our drawing editor to be able to store for a shape in the drawing. These include typing in values for Red, Green and Blue, selecting a colour from

  20. Blood Types

    E-Print Network [OSTI]

    Hacker, Randi; Tsutsui, William

    2007-03-14

    Sox spent a hundred mil to acquire pitcher Daisuke Matsuzaka; they probably weren't even aware that he is a Type O and that they make the best bankers, politicians and... you guessed it... professional baseball players. #ceas #hacker #japan #tsutsuien...

  1. GREEN FUNCTIONS ASSOCIATED TO COMPLEX REFLECTION GROUPS, II

    E-Print Network [OSTI]

    Shoj, Toshiaki

    be described completely in terms of various "Gre* *en functions" of type Bn0. However, note that the Green GREEN FUNCTIONS ASSOCIATED TO COMPLEX REFLECTION GROUPS, II University of Tokyo Noda, Chiba 278-8510, Japan Abstract. Green functions

  2. ACRA-II

    Energy Science and Technology Software Center (OSTI)

    003089IBMPC00 ACRA-II: Kernel Integration Code System for Estimation of Radiation Doses Caused by a Hypothetical Reactor Accident   

  3. Essays on School Choice and the Returns to School Quality

    E-Print Network [OSTI]

    Ajayi, Kehinde Funmilola

    2011-01-01

    me to track the secondary school performance of students whoyears stay in same school performance on SSCE core subjects2007): “Elite Schools and Academic Performance,” Institute

  4. Derived Types What Are Derived Types?

    E-Print Network [OSTI]

    Collett Jr., Jeffrey L.

    Derived Types #12;What Are Derived Types? As usual, a hybrid of two, unrelated concepts C++, Python orientation comes in #12;Simple Derived Types TYPE Wheel INTEGER :: spokes REAL :: diameter, width CHARACTER(LEN=15) :: material END TYPE Wheel That defines a derived type Wheel Using derived types needs a special

  5. Derived Types What Are Derived Types?

    E-Print Network [OSTI]

    Collett Jr., Jeffrey L.

    Derived Types #12;What Are Derived Types? As usual, a hybrid of two, unrelated concepts C object orientation comes in This course will only describe the former. #12;Simple Derived Types TYPE That defines a derived type Wheel Using derived types needs a special syntax TYPE(Wheel) :: w1 #12;More

  6. Impact of Middle School Scheduling Structure on Student Achievement in Math and Science, as Defined by AEIS Indicators, on Selected Demographic Student Groups in Urban Texas Middle Schools 

    E-Print Network [OSTI]

    Coburn, Joseph Ryan

    2015-05-01

    type on math and science achievement school-wide when accounting for the factors of minority student population and teacher experience. There was a statistically significant interaction at the p < .05 level for schedule type and teacher experience...

  7. Type: Renewal

    Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on Delicious RankADVANCEDInstallers/ContractorsPhotovoltaicsStateof Energy TwoEvent at the Pu Facility,Type IV COPV1

  8. Garbage Collection Based on a Linear Type System Atsushi Igarashi

    E-Print Network [OSTI]

    Science Graduate School of Arts and Sciences University of Tokyo igarashi@graco.c.u-tokyo.ac.jp Naoki and Linear Type Systems Automatic memory management, one of the important features of modern high expressions are given type Int under the assumption that x is given type Int, written as follows: x: Int ` x

  9. LABORATORY II MECHANICAL OSCILLATIONS

    E-Print Network [OSTI]

    Minnesota, University of

    Lab II - 1 LABORATORY II MECHANICAL OSCILLATIONS Most of the laboratory problems so far have was constant. In this set of laboratory problems, the total force acting on an object, and thus its's oscillation frequency. OBJECTIVES: After successfully completing this laboratory, you should be able to

  10. G-TEAMS at Mountain View High School Jennifer Hendryx, Mathias Reynolds

    E-Print Network [OSTI]

    Lega, Joceline

    G-TEAMS at Mountain View High School Jennifer Hendryx, Mathias Reynolds Who are we? Jennifer: Math teacher at Mountain View High school; teaches Alg. II, College Ready Math, and SpEd Alg. I. Goals in physics, Jennifer has been able to participate in Mountain View's Ac Dec as the science coach

  11. Out of School and Off Track: The Overuse of Suspensions in American Middle and High Schools

    E-Print Network [OSTI]

    Losen, Daniel J; Martinez, Tia E

    2013-01-01

    School Board, LA (26) 9. Detroit City School District, MI (School Board, LA (26) 9. Detroit City School District, MI (

  12. EnergySmart Schools Case Study: Northern Guilford Middle School

    SciTech Connect (OSTI)

    2009-09-01

    An EnergySmart Schools Case Study on the Northern Guilford Middle School in Greensboro, North Carolina

  13. Summer School Programs

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    Summer Institute IS&T Data Science at Scale Summer School IS&T Co-Design Summer School RELATED LINKS Affiliated Links IS&T Pillars New Mexico Consortium PRObE UCSC ISSDM...

  14. sustainable school of sustainable

    E-Print Network [OSTI]

    systems engineering School Director Ronald G. Askin Personalized learning Educational gaming Energy and product lifecycle analysis Earth systems engineering Water purification Resource-climate interactions Underground Infrastructure Construction Management school of electrical, computer and energy engineering

  15. Explaining Charter School Effectiveness

    E-Print Network [OSTI]

    Angrist, Joshua

    Lottery estimates suggest Massachusetts' urban charter schools boost achievement well beyond that of traditional urban public schools students, while nonurban charters reduce achievement from a higher baseline. The fact ...

  16. Planning for school choice

    E-Print Network [OSTI]

    Williams, Barika X. (Barika Xaviera)

    2010-01-01

    The image of the picturesque urban schoolhouse is increasingly becoming a thing of the past. City schools were viewed with fear or disdain. The urban school's image shifted to an unruly coop for 'dangerous' unteachable ...

  17. Cost Comparison of Public Elementary School Construction Costs Based on Project Delivery System in the State of Texas 

    E-Print Network [OSTI]

    Reinisch, Ashley

    2012-02-14

    the relationship between cost and project delivery systems. A survey was sent to all school superintendents in Texas requesting recent data on elementary school enrollment, project delivery type and construction costs. One hundred and thirty six responses were...

  18. The Three-Dimensional Structural Basis of Type II Hyperprolinemia...

    Office of Scientific and Technical Information (OSTI)

    crystal structure of HsP5CDH was determined using experimental phasing. Structures of the mutant enzymes S352A (2.4 angstrom) and S352L (2.85 angstrom) were...

  19. Engineering the angiotensin II type 1 receptor for structural studies

    E-Print Network [OSTI]

    Thomas, Jennifer Ann

    2015-02-03

    signal-regulated kinases (ERKs) and promote the internalisation of ?2AR through clathrin-coated pits. Adapted from 3. Conformational changes in the activation of GPCRs Initially, all GPCR structures were of receptors in the inactive conformation...

  20. Type II Migration: Varying Planet Mass and Disc Viscosity

    E-Print Network [OSTI]

    Richard G. Edgar

    2008-07-03

    This paper continues an earlier study of giant planet migration, examining the effect of planet mass and disc viscosity on the migration rate. We find that the migration rate of a gap-opening planet varies systematically with the planet's mass, as predicted in our earlier work. However, the variation with disc viscosity appears to be much weaker than expected.

  1. Phenomenology of heterotic and type II orientifold string models 

    E-Print Network [OSTI]

    Mayes, Van Eric

    2009-05-15

    Cryptons are metastable bound states of fractionally-charged particles that arise generically in the hidden sectors of models derived from heterotic string. We study their properties and decay modes in a speci?c ?ipped ...

  2. Type II Opsins: Evolutionary Origin by Internal Domain Duplication?

    E-Print Network [OSTI]

    California at Santa Barbara, University of

    Science+Business Media, LLC 2008 Abstract Opsins are a large group of proteins with seven transmembrane evolutionary origin, in which both groups of opsins evolved a seven-TM structure and light sensitivity independently. This convergence may indicate an impor- tant role for seven-TM protein structure for retinal

  3. Preliminary PBFA II design

    SciTech Connect (OSTI)

    Johnson, D. L.; VanDevender, J. P.; Martin, T. H.

    1980-01-01

    The upgrade of Sandia National Laboratories particle beam fusion accelerator, PBFA I, to PBFA II presents several interesting and challenging pulsed power design problems. PBFA II requires increasing the PBFA I output parameters from 2 MV, 30 TW, 1 MJ to 4 MV, 100 TW, 3.5 MJ with the constraint of using much of the same PBFA I hardware. The increased PBFA II output will be obtained by doubling the number of modules (from 36 to 72), increasing the primary energy storage (from 4 MJ to 15 MJ), lowering the pulse forming line (PFL) output impedance, and adding a voltage doubling network.

  4. Relativistic Quaternionic Wave Equation II

    E-Print Network [OSTI]

    Schwartz, Charles

    2007-01-01

    Relativistic quaternionic wave equation. II J. Math. Phys.Relativistic quaternionic wave equation. II Charles Schwartzcomponent quaternionic wave equation recently introduced. A

  5. Earth Science The Wiess School of Natural Sciences

    E-Print Network [OSTI]

    Richards-Kortum, Rebecca

    143 Earth Science The Wiess School of Natural Sciences CHAIR Alan Levander PROFESSORS John B Physics I and II with lab ESCI 321 Earth System Evolution and Cycles ESCI 322 Earth Chemistry and Materials ESCI 323 Earth Structure and Deformation with lab ESCI 324 Earth's Interior ESCI Degrees Offered

  6. Teachers’ and Administrators’ Perceptions of the Antecedents of School Dropout among English Language Learners at Selected Texas Schools 

    E-Print Network [OSTI]

    Doll, Jonathan Jacob

    2011-08-08

    stream_source_info DOLL-DISSERTATION.pdf.txt stream_content_type text/plain stream_size 430135 Content-Encoding ISO-8859-1 stream_name DOLL-DISSERTATION.pdf.txt Content-Type text/plain; charset=ISO-8859-1 i... TEACHERS? AND ADMINISTRATORS? PERCEPTIONS OF THE ANTECEDENTS OF SCHOOL DROPOUT AMONG ENGLISH LANGUAGE LEARNERS AT SELECTED TEXAS SCHOOLS A Dissertation by JONATHAN JACOB DOLL Submitted to the Office of Graduate Studies of Texas A...

  7. GREEN FUNCTIONS ASSOCIATED TO COMPLEX REFLECTION GROUPS, II

    E-Print Network [OSTI]

    Shoj, Toshiaki

    , that the Green functions of type D n can be described completely in terms of various ``Green functions'' of typeGREEN FUNCTIONS ASSOCIATED TO COMPLEX REFLECTION GROUPS, II TOSHIAKI SHOJI Department of Mathematics Science University of Tokyo Noda, Chiba 278­8510, Japan Abstract. Green functions associated

  8. _Part II - Contract Clauses

    National Nuclear Security Administration (NNSA)

    M0572 dated 3215 Contract DE-AC04-94AL85000 Modification No. M202 Page I - 1 Part II - Contract Clauses Section I TABLE OF CONTENTS 1. FAR 52.202-1 DEFINITIONS (JAN 2012)...

  9. Wind for Schools (Poster)

    SciTech Connect (OSTI)

    Baring-Gould, I.

    2010-05-01

    As the United States dramatically expands wind energy deployment, the industry is challenged with developing a skilled workforce and addressing public resistance. Wind Powering America's Wind for Schools project addresses these issues by developing Wind Application Centers (WACs) at universities; WAC students assist in implementing school wind turbines and participate in wind courses, by installing small wind turbines at community "host" schools, by implementing teacher training with interactive curricula at each host school. This poster provides an overview of the first two years of the Wind for Schools project, primarily supporting activities in Colorado, Kansas, Nebraska, South Dakota, Montana, and Idaho.

  10. Hydrogen in Type Ic Supernovae?

    E-Print Network [OSTI]

    David Branch; David J. Jeffery; Timothy R. Young; E. Baron

    2006-05-09

    By definition, a Type Ic supernova (SN Ic) does not have conspicuous lines of hydrogen or helium in its optical spectrum. SNe Ic usually are modelled in terms of the gravitational collapse of bare carbon-oxygen cores. We consider the possibility that the spectra of ordinary (SN 1994I-like) SNe Ic have been misinterpreted, and that SNe Ic eject hydrogen. An absorption feature usually attributed to a blend of Si II 6355 and C II 6580 may be produced by H-alpha. If SN 1994I-like SNe Ic eject hydrogen, the possibility that hypernova (SN 1998bw-like) SNe Ic, some of which are associated with gamma-ray bursts, also eject hydrogen should be considered. The implications of hydrogen for SN Ic progenitors and explosion models are briefly discussed.

  11. High School if required

    E-Print Network [OSTI]

    Walker, Lawrence R.

    or below, take in same semester as MATH 126 GEOL 221 3 Introduction to Optical Mineralogy and Petrography and Metamorphic Petrology/ Petrography PHYS 152 General Physics II CHEM 122 General Chemistry II CHEM AP 4-5 Lab

  12. Centrifuge workers study. Phase II, completion report

    SciTech Connect (OSTI)

    Wooten, H.D.

    1994-09-01

    Phase II of the Centrifuge Workers Study was a follow-up to the Phase I efforts. The Phase I results had indicated a higher risk than expected among centrifuge workers for developing bladder cancer when compared with the risk in the general population for developing this same type of cancer. However, no specific agent could be identified as the causative agent for these bladder cancers. As the Phase II Report states, Phase I had been limited to workers who had the greatest potential for exposure to substances used in the centrifuge process. Phase II was designed to expand the survey to evaluate the health of all employees who had ever worked in Centrifuge Program Departments 1330-1339 but who had not been interviewed in Phase I. Employees in analytical laboratories and maintenance departments who provided support services for the Centrifuge Program were also included in Phase II. In December 1989, the Oak Ridge Associated Universities (ORAU), now known as Oak Ridge Institute for Science and Education (ORISE), was contracted to conduct a follow-up study (Phase II). Phase H of the Centrifuge Workers Study expanded the survey to include all former centrifuge workers who were not included in Phase I. ORISE was chosen because they had performed the Phase I tasks and summarized the corresponding survey data therefrom.

  13. STUDY TYPES What is a "Study Type"?

    E-Print Network [OSTI]

    Dorf, Martin E.

    #12;STUDY TYPES What is a "Study Type"? A Study Type is a defined business process. Study Types work together to streamline workflow, track data & keep users informed. There are 2 Study Types in eCOMS: COMS and IACUC. The COMS Study: The COMS Study is an online form that a Principal Investigator fills

  14. 18 March 2015 Medical School MBChB Student Records Management Procedures

    E-Print Network [OSTI]

    Banaji,. Murad

    , religious beliefs, health, sexual health and criminal records. The table below sets out the types18 March 2015 Medical School MBChB Student Records Management Procedures The Medical School holdsRecord%20Retention%20Schedule%20R01.pdf. Information type Explanation Where and how stored Accessibility

  15. Program School/ Career: Descripton ISIS Program Codes

    E-Print Network [OSTI]

    Wisconsin at Madison, University of

    Program School/ Career: Descripton ISIS Program Codes Program Career: Descripton College School;Program School/ Career: Descripton ISIS Program Codes Program Career: Descripton College School/ College 1

  16. Solar Schools Assessment and Implementation Project: Financing Options for Solar Installations on K-12 Schools

    SciTech Connect (OSTI)

    Coughlin, J.; Kandt, A.

    2011-10-01

    This report focuses on financial options developed specifically for renewable energy and energy efficiency projects in three California public school districts. Solar energy systems installed on public schools have a number of benefits that include utility bill savings, reductions in greenhouse gas emissions (GHGs) and other toxic air contaminants, job creation, demonstrating environmental leadership, and creating learning opportunities for students. In the 2011 economic environment, the ability to generate general-fund savings as a result of reducing utility bills has become a primary motivator for school districts trying to cut costs. To achieve meaningful savings, the size of the photovoltaic (PV) systems installed (both individually on any one school and collectively across a district) becomes much more important; larger systems are required to have a material impact on savings. Larger PV systems require a significant financial commitment and financing therefore becomes a critical element in the transaction. In simple terms, school districts can use two primary types of ownership models to obtain solar installations and cost savings across a school district. The PV installations can be financed and owned directly by the districts themselves. Alternatively, there are financing structures whereby another entity, such as a solar developer or its investors, actually own and operate the PV systems on behalf of the school district. This is commonly referred to as the 'third-party ownership model.' Both methods have advantages and disadvantages that should be weighed carefully.

  17. Longfellow Middle School Wins Virginia Middle School Science...

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    Wins Virginia Middle School Science Bowl on March 7 2014 Virginia Middle School Science Bowl At the end of the day, the team from Longfellow Middle School, Falls Church, won the...

  18. High Performance Schools Policy

    Broader source: Energy.gov [DOE]

    The Executive Order also requires that the New Jersey Economic Development Authority establish a subsidiary corporation, The New Jersey Schools Construction Corporation (SCC), to be responsible...

  19. Type Ia Supernova Carbon Footprints

    E-Print Network [OSTI]

    Thomas, R C; Aragon, C; Antilogus, P; Bailey, S; Baltay, C; Bongard, S; Buton, C; Canto, A; Childress, M; Chotard, N; Copin, Y; Fakhouri, H K; Gangler, E; Hsiao, E Y; Kerschhaggl, M; Kowalski, M; Loken, S; Nugent, P; Paech, K; Pain, R; Pecontal, E; Pereira, R; Perlmutter, S; Rabinowitz, D; Rigault, M; Rubin, D; Runge, K; Scalzo, R; Smadja, G; Tao, C; Weaver, B A; Wu, C; Brown, P J; Milne, P A

    2011-01-01

    We present convincing evidence of unburned carbon at photospheric velocities in new observations of 5 Type Ia supernovae (SNe Ia) obtained by the Nearby Supernova Factory. These SNe are identified by examining 346 spectra from 124 SNe obtained before +2.5 d relative to maximum. Detections are based on the presence of relatively strong C II 6580 absorption "notches" in multiple spectra of each SN, aided by automated fitting with the SYNAPPS code. Four of the 5 SNe in question are otherwise spectroscopically unremarkable, with ions and ejection velocities typical of SNe Ia, but spectra of the fifth exhibits high-velocity (v > 20,000 km/s) Si II and Ca II features. On the other hand, the light curve properties are preferentially grouped, strongly suggesting a connection between carbon-positivity and broad band light curve/color behavior: Three of the 5 have relatively narrow light curves but also blue colors, and a fourth may be a dust-reddened member of this family. Accounting for signal-to-noise and phase, we ...

  20. North Newton School Corp | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on QA:QA J-E-1 SECTION J APPENDIXsourceII Jump to:Information 3rd| OpenInformation 9thNorthNewton School Corp Jump

  1. Tridiagonal pairs of Krawtchouk type

    E-Print Network [OSTI]

    Ito, Tatsuro

    2007-01-01

    Let $K$ denote an algebraically closed field with characteristic 0 and let $V$ denote a vector space over $K$ with finite positive dimension. Let $A,A^*$ denote a tridiagonal pair on $V$ with diameter $d$. We say that $A,A^*$ has Krawtchouk type whenever the sequence $\\lbrace d-2i\\rbrace_{i=0}^d$ is a standard ordering of the eigenvalues of $A$ and a standard ordering of the eigenvalues of $A^*$. Assume $A,A^*$ has Krawtchouk type. We show that there exists a nondegenerate symmetric bilinear form $$ on $V$ such that $= $ and $= $ for $u,v\\in V$. We show that the following tridiagonal pairs are isomorphic: (i) $A,A^*$; (ii) $-A,-A^*$; (iii) $A^*,A$; (iv) $-A^*,-A$. We give a number of related results and conjectures.

  2. (MATH 1302) Calculus II

    E-Print Network [OSTI]

    Huang, Haiying

    (MATH 1302) MATH 1426 Calculus I MATH 2425 Calculus II MATH 2326 Calculus III IE 3312 PHYS 1443 PHYS 1444 IE 3301 EE 2440 Circuits MATH 3319 ENGL 1301 ENGL 1302 (1310) (Intro) 1320 C/C++ 2312 Ass Sw Des Pat *4321 Testing *4322 Sw Mgmt (CHEM 1300) CHEM 1441 Math Placement Test / Advising (MATH

  3. Smog Check II Evaluation Part II: Overview of Vehicle

    E-Print Network [OSTI]

    Denver, University of

    Smog Check II Evaluation Part II: Overview of Vehicle Emissions . . . . . . . . . . . . Prepared in Later Sections ____________________ 1 3. Older Vehicles Have Higher Emissions on Average _____________ 3 ___________________________________ 12 7. Emissions of Individual Vehicles Vary from Test to Test ________ 15 8. Total Emissions

  4. Jefferson Lab hosts 19 schools for Virginia Regional High School...

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    Feb. 10, to compete in the Virginia Regional High School Science Bowl. Nineteen teams, representing high schools from across the region are participating in this year's...

  5. Annual Report School of Engineering

    E-Print Network [OSTI]

    Alpay, S. Pamir

    Annual Report 1999-2000 School of Engineering University of Connecticut #12;#12;University of Connecticut School of Engineering Annual Report 1999-2000 Table of Contents School of Engineering Annual Departments Chemical Engineering Annual Report Summary

  6. Kinard Core Knowledge Middle School

    High Performance Buildings Database

    Fort Collins, CO Located on the outskirts of Fort Collins, the Kinard school has established an impressive benchmark for high performance school buildings. Not only was the school designed with low energy use in mind: it's actually achieving these goals.

  7. Identifying Effective School Principals 

    E-Print Network [OSTI]

    Fernandez, Kandyce; Flores, Santa; Huang, Emily; Igwe, Carolyn; McDonald, Leslie; Stroud, Ryan; Willis, Rebecca; Dugat, Amber

    2007-01-01

    -1 PRINCIPAL PERFORMANCE IN TEXAS: TOOLS FOR MEASURING EFFECTIVE SCHOOL LEADERSHIP KANDYCE FERNANDEZ SANTA FLORES EMILY HUANG CAROLYN IGWE LESLIE MCDONALD RYAN STROUD REBECCA WILLIS AMBER DUGAT FACULTY ADVISOR: DR. LORI TAYLOR MAY.........................................................................................................................................15 Influences of School Characteristics on Student Performance ..........................................................................17 Student Performance Conclusion...

  8. Howe School Alliance for

    E-Print Network [OSTI]

    Yang, Eui-Hyeok

    BEST PRACTICES. BETTER RESULTS. Howe School Alliance for Technology Management "The biggest value of the Alliance, for me, is that it gives me a break from daily problem solving and creates an opportunity companies join the Howe School Alliance for Technology Management. Come learn what sets us apart and how we

  9. INFORMATION IIT SCHOOL OF

    E-Print Network [OSTI]

    Heller, Barbara

    INFORMATION TECHNOLOGY AND MANAGEMENT IIT SCHOOL OF APPLIED TECHNOLOGY CYBER SECURITY an undergraduate degree in Information Technology and Management (ITM) from Illinois Tech's School of Applied. · You'll learn relevant skills so you can integrate information technology and management into your

  10. Middle School Teacher's Guide

    E-Print Network [OSTI]

    Patterson, Bruce D.

    of animals that also includes humans. All mammals are vertebrates and endothermic, warm-blooded. They alsoMiddle School Teacher's Guide ANATOMY Major Sponsor: #12;MIDDLE SCHOOL | EDUCATOR | ANATOMY VIRTUAL of content areas. All materials in this module are optional but designed to enrich your students' Virtual

  11. Giant Protease TPP II's Structure, Mechanism Uncovered

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    Giant Protease TPP II's Structure, Mechanism Uncovered Print Tripeptidyl peptidase II (TPP II), the largest known eukaryotic enzyme that breaks down proteins (a protease), is...

  12. Los Alamos Dynamics Summer School

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    School Los Alamos Dynamics Summer School Overview Contact Institute Director Charles Farrar (505) 663-5330 Email Professional Staff Assistant Jutta Kayser (505) 663-5649 Email...

  13. Portsmouth Abbey School Wind Turbine Wind Farm | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on QA:QA J-E-1 SECTION J APPENDIXsourceII JumpQuarterly SmartDB-2, Blue MountainSchoolPrairiePonder,Abbey School Wind

  14. 5) Management ii) Mechanical methods

    E-Print Network [OSTI]

    Nowak, Robert S.

    5) Management c) Control ii) Mechanical methods = manually or mechanically damaging plants #12;5) Management c) Control ii) Mechanical methods Advantages · Generally much less public opposition #12;5) Management c) Control ii) Mechanical methods Advantages · Generally much less public opposition · Works well

  15. A Typed Operational Semantics for Type Theory 

    E-Print Network [OSTI]

    Goguen, Healfdene

    Untyped reduction provides a natural operational semantics for type theory. Normalization results say that such a semantics is sound. However, this reduction does not take type information into account and gives no information ...

  16. Ribosomal Database Project II

    DOE Data Explorer [Office of Scientific and Technical Information (OSTI)]

    The Ribosomal Database Project (RDP) provides ribosome related data and services to the scientific community, including online data analysis and aligned and annotated Bacterial small-subunit 16S rRNA sequences. As of March 2008, RDP Release 10 is available and currently (August 2009) contains 1,074,075 aligned 16S rRNA sequences. Data that can be downloaded include zipped GenBank and FASTA alignment files, a histogram (in Excel) of the number of RDP sequences spanning each base position, data in the Functional Gene Pipeline Repository, and various user submitted data. The RDP-II website also provides numerous analysis tools.[From the RDP-II home page at http://rdp.cme.msu.edu/index.jsp

  17. 1 School of Nursing SCHOOL OF NURSING

    E-Print Network [OSTI]

    Vertes, Akos

    . The SON educates students in the art and science of assisting patients, families, and communities to achieve their highest level of health. The school promotes leadership, quality, knowledge, collaboration, students at SON's Foggy Bottom campus are immersed in current events involving health care policy

  18. 2001 Participating Schools Abraham Wing School

    E-Print Network [OSTI]

    School of Humanities Teacher: Ms. Vivian Hansen Students: Catherine Calsolaro Lusonta Harvin Shaharazod, Mrs. Miller and Mrs. Stokes Students: Jordan Adderly Mariah Brown Antonio Davis Raven Dixon Jabril Teachers: Mr. Gerald Germano, Ms. Karen Lasky and Mrs. Joy G. Sokero Students: Miranda Allen Cassie Card

  19. Successes in School Energy Management - Energy Monitoring 

    E-Print Network [OSTI]

    Corbitt, C.

    2012-01-01

    stream_source_info ESL-KT-12-10-27.pdf.txt stream_content_type text/plain stream_size 2031 Content-Encoding ISO-8859-1 stream_name ESL-KT-12-10-27.pdf.txt Content-Type text/plain; charset=ISO-8859-1 Successes in School... Energy Management ? Energy Monitoring Chad Corbitt, CEM, ATEM Energy Manager, Klein ISD jcorbitt1@kleinisd.net Wednesday, October 10, 2012 Keys to Energy Monitoring ? Develop an Energy Monitoring plan ? Define the why, what, how and who...

  20. The power graph of a finite group, II Peter J. Cameron

    E-Print Network [OSTI]

    Cameron, Peter

    The power graph of a finite group, II Peter J. Cameron School of Mathematical Sciences Queen Mary, University of London Mile End Road London E1 4NS, U.K. Abstract The directed power graph of a group G is the digraph with vertex set G, having an arc from y to x whenever x is a power of y; the undirected power

  1. Improved Yield and Diverse Finished Bacterial Genomes using Pacific Biosciences RS II SMRT Sequencing

    E-Print Network [OSTI]

    Weber, David J.

    Improved Yield and Diverse Finished Bacterial Genomes using Pacific Biosciences RS II SMRT-Cruz, Alvaro Godinez, Luke J. Tallon Institute for Genome Sciences, University of Maryland School of Medicine, effective, and highly accurate platform for generation of complete microbial genome sequences. As early

  2. School of International Graduate Studies

    E-Print Network [OSTI]

    School of International Graduate Studies 1 SCHOOL OF INTERNATIONAL GRADUATE STUDIES Information Brief Last revision: 5/11 #12;School of International Graduate Studies 2 NPS Facts · Worldwide Outreach · Fully accredited #12;School of International Graduate Studies 3 SIGS Objectives · Provide graduate

  3. School of International Graduate Studies

    E-Print Network [OSTI]

    School of International Graduate Studies 1 SCHOOL OF INTERNATIONAL GRADUATE STUDIES Information Brief Last revision: 10/09 #12;School of International Graduate Studies 2 SIGS Objectives · Provide Security · Support U.S. defense and foreign policy #12;School of International Graduate Studies 3

  4. 07SCHOOL OF MECHANICAL ENGINEERING

    E-Print Network [OSTI]

    Dimitrova, Vania

    07SCHOOL OF MECHANICAL ENGINEERING UNDERGRADUATE DEGREES School of Mechanical Engineering FACULTY OF ENGINEERING Undergraduate Degrees 2015 #12;www.engineering.leeds.ac.uk/mechanical UNDERGRADUATE DEGREES SCHOOL OF MECHANICAL ENGINEERING The School of Mechanical Engineering offers both a broad mechanical engineering degree

  5. Benchmark specifications for EBR-II shutdown heat removal tests

    SciTech Connect (OSTI)

    Sofu, T.; Briggs, L. L.

    2012-07-01

    Argonne National Laboratory (ANL) is hosting an IAEA-coordinated research project on benchmark analyses of sodium-cooled fast reactor passive safety tests performed at the Experimental Breeder Reactor-II (EBR-II). The benchmark project involves analysis of a protected and an unprotected loss of flow tests conducted during an extensive testing program within the framework of the U.S. Integral Fast Reactor program to demonstrate the inherently safety features of EBR-II as a pool-type, sodium-cooled fast reactor prototype. The project is intended to improve the participants' design and safety analysis capabilities for sodium-cooled fast reactors through validation and qualification of safety analysis codes and methods. This paper provides a description of the EBR-II tests included in the program, and outlines the benchmark specifications being prepared to support the IAEA-coordinated research project. (authors)

  6. This study was supported in part by NSF Grant IIS 97-32799 and by a grant from the Office of the Dean at the School of Information Studies, Syracuse University. The authors thank the unnamed real estate agents and other real estate professionals for their

    E-Print Network [OSTI]

    Crowston, Kevin

    estate agents and other real estate professionals for their time and insight, and the anonymous reviewers THE RESIDENTIAL REAL ESTATE INDUSTRY1 Kevin Crowston School of Information Studies Syracuse University U are exploringhow informationand communicationtechnology (ICT) use affects the work lives of real estate agents

  7. Building Energy Efficient Schools 

    E-Print Network [OSTI]

    McClure, J. D.; Estes, J. M.

    1985-01-01

    Many new school buildings consume only half the energy required by similar efficient structures designed without energy performance as a design criterion. These are comfortable and efficient while construction costs remain about the same as those...

  8. School quality and wages 

    E-Print Network [OSTI]

    Speakman, Robert B., Jr.

    2007-04-25

    This dissertation examines the literature that attempts to measure the relationship between school quality and earnings. I begin by developing a simple economic model that predicts that, everything else being equal and with comparisons being made...

  9. Difwind II Wind Farm | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on QA:QA J-E-1 SECTION J APPENDIX ECoopButtePower VenturesInformation9)ask queries TypeDeveloper|WindsDifwind I WindII

  10. PART II - CONTRACT CLAUSES

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Homesum_a_epg0_fpd_mmcf_m.xls" ,"Available from WebQuantityBonneville Power Administration wouldMass mapSpeeding access toOctoberConsumptionPoweredE Contract No.No. 330 J.2-1 ContractII

  11. PARS II TRAINING

    Energy Savers [EERE]

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on DeliciousMathematicsEnergyInterested PartiesBuilding energy codes have a more than 20-yearPAE EvaluationPARS II13,

  12. Questions about Cori II

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Homesum_a_epg0_fpd_mmcf_m.xls" ,"Available from WebQuantity ofkandz-cm11 Outreach Home RoomPreservation of Fe(II) by Carbon-RichProton Delivery and RemovalQuantumdefault Sign In About

  13. Types of Commissioning

    Broader source: Energy.gov [DOE]

    Several commissioning types exist to address the specific needs of equipment and systems across both new and existing buildings. The following commissioning types provide a good overview.

  14. Postdoc Appointment Types

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    Appointment Types Postdoc Appointment Types Most postdocs will be offered a postdoctoral research associate appointment. Each year, approximately 30 Postdoctoral Fellow...

  15. Citrus bioactive compounds influencing phase II detoxifying enzymes: potential for cancer chemoprevention 

    E-Print Network [OSTI]

    Perez, Jose Luis

    2009-05-15

    Several cell culture and animal studies demonstrated that citrus limonoids have protective effects against certain types of cancer. These chemopreventive properties of citrus limonoids are attributed to the induction of phase II enzyme, glutathione...

  16. NSBA Endorses EnergySmart Schools

    SciTech Connect (OSTI)

    2008-01-01

    EnergySmart Schools fact sheet on the EnergySmart Schools program that is endorsed by the National School Board Association (NSBA).

  17. High schools that bridge the achievement gap

    E-Print Network [OSTI]

    Hargrove, Michael S.

    2007-01-01

    statewide patterns of high school performance as measured byFusarelli, 2004). School performance is strongly associatedon publicly available school performance, demographic, and

  18. Are We Closing the School Discipline Gap?

    E-Print Network [OSTI]

    Losen, Daniel; Hodson, Cheri; Keith II, Michael A; Morrison, Katrina; Belway, Shakti

    2015-01-01

    an indicator of school performance or achievement. Becausepart of reporting on school performance and accountability,used to evaluate school and district performance and for

  19. Does Schooling Give Us Rational Expectations?

    E-Print Network [OSTI]

    Shenoy, Ajay

    2015-01-01

    of Edmund S. Phelps :25. DOES SCHOOLING GIVE US RATIONALDoes Schooling Give Us Rational Expectations? Ajay Shenoy ?from four years to six. DOES SCHOOLING GIVE US RATIONAL

  20. Types of Lights Types of Lights

    E-Print Network [OSTI]

    1 Types of Lights Types of Lights q So far we have studied point lights ­ Radiate in all direc7ons q Other lights ­ Direc7onal lights (posi7on-independent) ­ Spotlights #12;2 Direc1onal Lights q Shine in a single, uniform direc7on q All rays

  1. Supernovae. Part II: The aftermath

    E-Print Network [OSTI]

    Trimble, V; Trimble, V

    1983-01-01

    R. Viswanathan, 1980, As- Supernovae. Part II ExperimentalSmith, 1982, Astrophys. Supernovae. Chevalier, R. A. , andC. B. , 1974, Ed. , Supernovae and Supernova Rem- nants,

  2. 8. SQL II 8-1 Part 8: SQL II

    E-Print Network [OSTI]

    Brass, Stefan

    8. SQL II 8-1 Part 8: SQL II References: · Elmasri/Navathe:Fundamentals of Database Systems, 3rd Edition, 1999. Chap. 8, "SQL -- The Relational Database Standard" (Sect. 8.2, 8.3.3, part of 8.3.4.) · Silberschatz/Korth/Sudarshan: Database System Concepts, 3rd Edition. McGraw-Hill, 1999: Chapter 4: "SQL

  3. A Study of Prevention and Retention Strategies for Successful Urban Secondary High School Hispanic Students 

    E-Print Network [OSTI]

    Lopez, Roberto I

    2013-01-14

    Hispanic high school students have a dropout rate that ranges from 35 percent to 55 percent depending on what type of report you may be referencing. Add rates for all high school students. Hispanic youth endure the challenges of language barriers...

  4. Phase II Final Report

    SciTech Connect (OSTI)

    Schuknecht, Nate; White, David; Hoste, Graeme

    2014-09-11

    The SkyTrough DSP will advance the state-of-the-art in parabolic troughs for utility applications, with a larger aperture, higher operating temperature, and lower cost. The goal of this project was to develop a parabolic trough collector that enables solar electricity generation in the 2020 marketplace for a 216MWe nameplate baseload power plant. This plant requires an LCOE of 9¢/kWhe, given a capacity factor of 75%, a fossil fuel limit of 15%, a fossil fuel cost of $6.75/MMBtu, $25.00/kWht thermal storage cost, and a domestic installation corresponding to Daggett, CA. The result of our optimization was a trough design of larger aperture and operating temperature than has been fielded in large, utility scale parabolic trough applications: 7.6m width x 150m SCA length (1,118m2 aperture), with four 90mm diameter × 4.7m receivers per mirror module and an operating temperature of 500°C. The results from physical modeling in the System Advisory Model indicate that, for a capacity factor of 75%: The LCOE will be 8.87¢/kWhe. SkyFuel examined the design of almost every parabolic trough component from a perspective of load and performance at aperture areas from 500 to 2,900m2. Aperture-dependent design was combined with fixed quotations for similar parts from the commercialized SkyTrough product, and established an installed cost of $130/m2 in 2020. This project was conducted in two phases. Phase I was a preliminary design, culminating in an optimum trough size and further improvement of an advanced polymeric reflective material. This phase was completed in October of 2011. Phase II has been the detailed engineering design and component testing, which culminated in the fabrication and testing of a single mirror module. Phase II is complete, and this document presents a summary of the comprehensive work.

  5. Pomeroy II (08) Wind Farm | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on QA:QA J-E-1 SECTION J APPENDIXsourceII JumpQuarterly SmartDB-2, Blue MountainSchoolPrairie JumpPolytechnic

  6. Pomeroy II (4Q07) Wind Farm | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on QA:QA J-E-1 SECTION J APPENDIXsourceII JumpQuarterly SmartDB-2, Blue MountainSchoolPrairie JumpPolytechnic4Q07) Wind

  7. Indiana University School of Library and Information Science S604/S764 : Information Networks

    E-Print Network [OSTI]

    Indiana University

    Indiana University School of Library and Information Science S604/S764. But what is a network? What types of networks exist? Why are they interesting of Library and Information Science, Indiana University, on November 11, 1996

  8. QUANTUM MECHANICS II Physics 342

    E-Print Network [OSTI]

    Rosner, Jonathan L.

    QUANTUM MECHANICS II Physics 342 KPTC 103 9:00 ­ 10:20 a.m. 1 Tues., Thurs. ­ Winter Quarter 2011 quantum mechanics at the graduate level. The text for Quantum Mechanics II will be J. J. Sakurai and Jim Napolitano, Modern Quantum Mechanics, Second Edition (Addison-Wesley, San Francisco, 2011). For supplemental

  9. II JORNADAS "PUBLICAR EN REVISTAS

    E-Print Network [OSTI]

    Escolano, Francisco

    II JORNADAS "PUBLICAR EN REVISTAS DE IMPACTO" 20 de Septiembre 2011 Facultad de Ciencias de la Salud #12;Taller: "Elaboración de Manuscritos y Proceso Editorial en Revistas Indexadas: el Caso del: Secretaría. Departamento de Psicología de la Salud II JORNADAS "PUBLICAR EN REVISTAS DE IMPACTO" 20 de

  10. National Synchrotron Light Source II

    ScienceCinema (OSTI)

    Steve Dierker

    2010-01-08

    The National Synchrotron Light Source II (NSLS-II) at the U.S. Department of Energy's Brookhaven National Laboratory is a proposed new state-of-the-art medium energy storage ring designed to deliver world-leading brightness and flux with top-off operation

  11. Sist. Lin. II Aps Escalonamento

    E-Print Network [OSTI]

    Cabral, Marco

    Lineares ­ 2a Parte Paulo Goldfeld Marco Cabral Departamento de Matemática Aplicada Universidade Federal do Rio de Janeiro Álgebra Linear II 2008/2 Prof. Marco Cabral & Prof. Paulo Goldfeld DMA / IM / UFRJ 1 conjunto-solução = { } sistema inconsistente Álgebra Linear II 2008/2 Prof. Marco Cabral & Prof. Paulo

  12. Unit II-5 Interpolation 1 Interpolation

    E-Print Network [OSTI]

    Birkett, Stephen

    Unit II-5 Interpolation 1 Unit II-5 Interpolation Unit II-5 Interpolation 2 Interpolation outside the range of values of xi use extrapolation Unit II-5 Interpolation 3 Basic ideas · given: n+1 in tabular format Unit II-5 Interpolation 4 Basis functions · n basis functions 1, 2, ... , n can be used

  13. Career Break Record of Contact Days Staff on a career break may, by agreement with their Head of School/Unit, undertake a number of days'

    E-Print Network [OSTI]

    Brierley, Andrew

    with their Head of School/Unit, undertake a number of days' paid work during their career break ("contact days"). The type of work undertaken is a matter of agreement between the member of staff and the Head of School/Unit: _________________________________________________________________ Staff ID/NI Number/ Date of Birth:_________________________________________ School/Unit

  14. Wind for Schools Curriculum Brief

    SciTech Connect (OSTI)

    None

    2010-08-01

    This fact sheet provides an overview of wind energy curricula as it relates to the Wind for Schools project.

  15. School of Mines Undergraduate Bulletin

    E-Print Network [OSTI]

    is for your use as a source of continuing reference. Please save it. Published by Colorado School of Mines

  16. School of Mines Graduate Bulletin

    E-Print Network [OSTI]

    is for your use as a source of continuing reference. Please save it. Published by Colorado School of Mines

  17. MATH0370: Introduction to Applied Mathematics 2 c School of Mathematics, University of Leeds

    E-Print Network [OSTI]

    Rucklidge, Alastair

    MATH0370: Introduction to Applied Mathematics 2 c School of Mathematics, University of Leeds and Vectors, Cambridge, 1986. #12;ii Useful resources · Course web page: http://www.maths.leeds.ac.uk/~alastair/MATH a Maths drop-in service open every day during term. They can be found at 15 Blenheim Terrace; see http

  18. Types of Reuse

    Broader source: Energy.gov [DOE]

    The following provides greater detail regarding the types of reuse pursued for LM sites. It should be noted that many actual reuses combine several types of the uses listed below.

  19. SCHOOL OF MEDICINE CURRICULUM GUIDE

    E-Print Network [OSTI]

    Finley Jr., Russell L.

    SCHOOL OF MEDICINE YEAR 2 CURRICULUM GUIDE WAYNE STATE UNIVERSITY SCHOOL OF MEDICINE 2015-2016 PLEASE READ THE INTRODUCTORY PAGES VERY CAREFULLY. THEY CONTAIN IMPORTANT POLICY GUIDELINES. Curriculum guides are subject to revision. Updated versions of the Curriculum Guide will be posted on the School

  20. SCHOOL OF MEDICINE CURRICULUM GUIDE

    E-Print Network [OSTI]

    Finley Jr., Russell L.

    SCHOOL OF MEDICINE YEAR IV CURRICULUM GUIDE WAYNE STATE UNIVERSITY SCHOOL OF MEDICINE 2014-2015 Curriculum Guides are subject to revision. Updates will be posted to the electronic version of this Curriculum Guide that can be found on the School of Medicine website. Curriculum Guide 2014-2015 Revised 03

  1. LMS Undergraduate Summer School 2015

    E-Print Network [OSTI]

    Abrahams, I. David

    LMS Undergraduate Summer School 2015 Application form for the LMS Undergraduate Summer School 2015 of LMS Undergraduate Summer Schools. The aim is to introduce to modern mathematics the best UK Maths on the recommendation of the Head of Department and LMS representative. If you would like to participate, please discuss

  2. LMS Undergraduate Summer School 2015

    E-Print Network [OSTI]

    Haase, Markus

    LMS Undergraduate Summer School 2015 The London Mathematical Society, De Morgan House, 57 and is a charity registered with the Charity Commissioners. Registered number: 252660 http://www.lms.ac.uk/events/lms-summer-schools This Summer School is part of the LMS 150th Anniversary celebrations. http://www.lms.ac.uk/2015 Loughborough

  3. #winchesterart Winchester School of Art

    E-Print Network [OSTI]

    Molinari, Marc

    #winchesterart Winchester School of Art University of Southampton Park Ave, Winchester, Hampshire School of Art 6 Introducing Winchester School of Art 7 Executive Team 8 Showcasing our Talent 9 Fashion Marketing/Management 40 BA Fine Art 48 BA Graphic Arts 58 BA Games Design and Art 60 MA Fashion

  4. School of Accounting Highlights -2013

    E-Print Network [OSTI]

    Tipple, Brett

    School of Accounting Highlights - 2013 The School of Accounting: · The School of Accounting's Masters of Accounting program and Undergraduate program were both ranked 22nd in the Nation by the Public Accounting Report in 2013 for all accounting programs across the nation. · Both the undergraduate and Masters

  5. Master's of School Administration (MSA)

    E-Print Network [OSTI]

    Olszewski Jr., Edward A.

    Master's of School Administration (MSA) Program and Add-On Licensure Handbook #12;2 TABLE OF EDUCATION UNIVERSITY OF NORTH CAROLINA WILMINGTON MASTER OF SCHOOL ADMINISTRATION Graduates of the Master of School Administration (M.S.A.) program will be effective educational leaders who can inspire, engage

  6. School of Medicine Degree options

    E-Print Network [OSTI]

    Brierley, Andrew

    126 School of Medicine Medicine Degree options BSc (Single Honours Degree) Medicine Entrance level. HNC Applied Sciences`Pathway to Medicine'at Perth College The School of Medicine has formed at St Andrews. More information can be found on the School of Medicine webpages or from Perth College T

  7. School of Medicine Degree options

    E-Print Network [OSTI]

    Brierley, Andrew

    136 School of Medicine Medicine Degree options BSc (Single Honours Degree) Medicine Entrance Applied Sciences`Pathway to Medicine'at Perth College The School of Medicine has formed a partnership Andrews. More information can be found on the School of Medicine web pages ( http://medicine

  8. SCHOOL OF MEDICINE RESEARCH ROADMAP

    E-Print Network [OSTI]

    Chapman, Michael S.

    SCHOOL OF MEDICINE RESEARCH ROADMAP October 2011 #12;OHSU School of Medicine Research Roadmap internal and external stakeholders and the public. #12;OHSU School of Medicine Research Roadmap October human health and well-being. At the Research Roadmap Retreat in December 2010, I issued a charge

  9. Building Energy-Efficient Schools

    E-Print Network [OSTI]

    energy efficiency in the rebuilding and renovating of New Orleans K-12 schools after Hurricanes Katrina certification; a goal was also set for schools undergoing major renovation to achieve 25% energy savingsBuilding Energy- Efficient Schools in New Orleans Lessons Learned #12;2 #12;3 The devastation

  10. Nottingham Business School Biofuels Market and Policy Governance

    E-Print Network [OSTI]

    Evans, Paul

    Nottingham Business School Biofuels Market and Policy Governance The last decade has seen a dramatic growth in the global production and consumption of biofuels, as a rapidly- rising number triggered growing concerns about the downsides from different types of biofuel. This, in turn, presents

  11. Optimal Newton-type algorithms for nonconvex smooth optimization

    E-Print Network [OSTI]

    Sidorov, Nikita

    Optimal Newton-type algorithms for nonconvex smooth optimization Coralia Cartis Mathematical-HPC Workshop on New Directions in Nonlinear Optimization University of Manchester, School of Mathematics, March 19, 2014 New Directions in Nonlinear Optimization: Manchester, 2014 ­ p. 1/33 #12;Unconstrained

  12. Doctoral school COURSE PROPOSAL

    E-Print Network [OSTI]

    Jeanjean, Louis

    Doctoral school COURSE PROPOSAL ED SPIM / Course proposal Page 1/2 2013 Title: The Web of data This course will give an overview of the principles of Linked Data along with the Web of Data, as it emerged architectures. This course also presents the concepts and definitions related to the Semantic Web (or Web

  13. international summer school 2015

    E-Print Network [OSTI]

    Wirosoetisno, Djoko

    in the National Student Survey. Our inclusion in the Russell Group has cemented our reputation as one) · International Relations: Security, Conflict and Peace · Introduction to Accounting · Introduction to English Law The Summer School gave me the opportunity to see the United Kingdom in varying and interesting perspectives I

  14. Phase II Planning for Niall Gaffney

    E-Print Network [OSTI]

    Phase II Planning for the HET Niall Gaffney March 6, 1997 #12;#12;Phase II Planning for the HET 3 ................................................................................................................................. 38 Plan Templates .............................................................................................................................................. 47 Example Plans

  15. Phase II Planning for Niall Gaffney

    E-Print Network [OSTI]

    Phase II Planning for the HET Niall Gaffney March 6, 1997 #12; #12; Phase II Planning for the HET 3 ................................................................................................................................. 38 Plan Templates .............................................................................................................................................. 47 Example Plans

  16. Quantitative comparison between Type Ia supernova spectra at low and high redshifts: A case study

    E-Print Network [OSTI]

    Garavini, G.; Supernova Cosmology Project

    2008-01-01

    Highlight - The Physics of Supernovae, ESO/MPA/MPE Workshop,Evolution in high-redshift supernovae Fig. 8 “Ca ii H&K”SN 1991T/SN 1999aa-like supernovae. 1. Introduction Type Ia

  17. High School if required

    E-Print Network [OSTI]

    Walker, Lawrence R.

    ; contact Physics *CHEM 474 3 Biochemistry I *CHEM 475 3 Biochemistry II CHEM 355 & 355L 3+2 Quantitative *CHEM 447 2 Advanced Synthesis Lab *CHEM 455 & 455L 3+2 Instrumental Analysis *CHEM 472 2 Biochemistry AP 4-5 Lab required @ UNLV; contact Chemistry PHYS 182 & 182L Engineering Physics III PHYS 180 & 180L

  18. High School if required

    E-Print Network [OSTI]

    Walker, Lawrence R.

    as MATH 126 CHEM 474 3 Biochemistry I CHEM 355 & 355L 3+2 Quantitative Analysis CHEM 402 1 Scientific 182 & 182L Engineering Physics III PHYS 180 & 180L Engineering Physics I Physics C - E & M 4 required (prerequisites vary by major) *CHEM 475 3 Biochemistry II *CHEM 472 2 Biochemistry Laboratory co

  19. Options Study - Phase II

    SciTech Connect (OSTI)

    R. Wigeland; T. Taiwo; M. Todosow; W. Halsey; J. Gehin

    2010-09-01

    The Options Study has been conducted for the purpose of evaluating the potential of alternative integrated nuclear fuel cycle options to favorably address the issues associated with a continuing or expanding use of nuclear power in the United States. The study produced information that can be used to inform decisions identifying potential directions for research and development on such fuel cycle options. An integrated nuclear fuel cycle option is defined in this study as including all aspects of the entire nuclear fuel cycle, from obtaining natural resources for fuel to the ultimate disposal of used nuclear fuel (UNF) or radioactive wastes. Issues such as nuclear waste management, especially the increasing inventory of used nuclear fuel, the current uncertainty about used fuel disposal, and the risk of nuclear weapons proliferation have contributed to the reluctance to expand the use of nuclear power, even though it is recognized that nuclear power is a safe and reliable method of producing electricity. In this Options Study, current, evolutionary, and revolutionary nuclear energy options were all considered, including the use of uranium and thorium, and both once-through and recycle approaches. Available information has been collected and reviewed in order to evaluate the ability of an option to clearly address the challenges associated with the current implementation and potential expansion of commercial nuclear power in the United States. This Options Study is a comprehensive consideration and review of fuel cycle and technology options, including those for disposal, and is not constrained by any limitations that may be imposed by economics, technical maturity, past policy, or speculated future conditions. This Phase II report is intended to be used in conjunction with the Phase I report, and much information in that report is not repeated here, although some information has been updated to reflect recent developments. The focus in this Options Study was to identify any nuclear fuel cycle technology or option that may result in a significant beneficial impact to the issues as compared to the current U.S. approach of once-through use of nuclear fuel in LWRs or similar reactors followed by direct disposal of UNF. This approach was taken because incremental differences may be difficult to clearly identify and justify due to the large uncertainties that can be associated with the specific causes of the issues. Phase II of this Options Study continued the review of nuclear fuel cycle options that was initiated and documented during Phase I, concentrating on reviewing and summarizing the potential of integrated nuclear fuel cycles. However, based on the reviews of previous studies and available data, it was not always possible to clearly determine sufficiently large differences between the various fuel cycle and technology options for some of the issues or evaluation measures, for example, in cases where only incremental differences with respect to the issues might be achieved regardless of the fuel cycle option or technologies being considered, or where differences were insufficient to clearly rise above the uncertainties.

  20. Does School Count? School Climate and Behavior Problems for Youth With ASD, ID, or TD

    E-Print Network [OSTI]

    Murphy, Marina E.

    2015-01-01

    Ben-Avie, M. (1997). School climate as a factor in studentof school emotional climate on student psychopathology.J. (2001). School social climate and individual differences

  1. Identity and the pursuit of school success understandings of intelligence and effort in three high schools

    E-Print Network [OSTI]

    Nunn, Lisa Michele

    2009-01-01

    performance in school and performance on intelligence tests.Intelligence and School Performance." Journal of EducationalDifferences in School Performance." American Sociological

  2. Out of School and Off Track: The Overuse of Suspensions in American Middle and High Schools

    E-Print Network [OSTI]

    Losen, Daniel J; Martinez, Tia E

    2013-01-01

    and undermining overall school performance. Moreover, as ourmeasure the performance of secondary schools, and as “earlymeasure the performance of secondary schools, and as “early

  3. by popular demand: Addiction II

    E-Print Network [OSTI]

    Niv, Yael

    by popular demand: Addiction II PSY/NEU338:Animal learning and decision making: Psychological, size of other non-drug rewards, and cost (but ultimately the demand is inelastic, or at least

  4. Experience with capture cavity II

    SciTech Connect (OSTI)

    Koeth, T.; /Fermilab /Rutgers U., Piscataway; Branlard, J.; Edwards, H.; Fliller, R.; Harms, E.; Hocker, A.; McGee, M.; Pischalnikov, Y.; Prieto, P.; Reid, J.; /Fermilab

    2007-06-01

    Valuable experience in operating and maintaining superconducting RF cavities in a horizontal test module has been gained with Capture Cavity II. We report on all facets of our experience to date.

  5. TYPES OF NONIMMIGRANT VISAS Type Description

    E-Print Network [OSTI]

    for pleasure and cannot receive any type of payments. C-1*, Aliens in travel status while travelling directly through the C-2*, United States. C-3* D-1 Alien crewman on shore leave or transferring to another vessel is grounds for deportation. E-1 Aliens who conduct trade or inventories between the United States

  6. Run II Jet Physics Proceedings of the Run II QCD and Weak Boson Physics Workshop

    E-Print Network [OSTI]

    Blazey, G C; Ellis, S D; Elvira, V D; Frame, K C; Grinstein, S; Hirosky, R; Piegaia, R; Schellman, H; Snihur, R; Sorin, V; Zeppenfeld, Dieter; Blazey, Gerald C.; Dittmann, Jay R.; Ellis, Stephen D.; Hirosky, Robert; Zeppenfeld, Dieter

    2000-01-01

    The Run II jet physics group includes the Jet Algorithms, Jet Shape/Energy Flow, and Jet Measurements/Correlations subgroups. The main goal of the jet algorithm subgroup was to explore and define standard Run II jet finding procedures for CDF and DO. The focus of the jet shape/energy flow group was the study of jets as objects and the energy flows around these objects. The jet measurements/correlations subgroup discussed measurements at different beam energies; strong coupling constant measurements; and LO, NLO, NNLO, and threshold jet calculations. As a practical matter the algorithm and shape/energy flow groups merged to concentrate on the development of Run II jet algorithms that are both free of theoretical and experimental difficulties and able to reproduce Run I measurements. Starting from a review of the experience gained during Run I, the group considered a variety of cone algorithms and KT algorithms. The current understanding of both types of algorithms, including calibration issues, are discussed i...

  7. N-Type Thermoelectric Performance of Functionalized Carbon Nanotube-Filled Polymer Composites 

    E-Print Network [OSTI]

    Freeman, Dallas

    2012-07-16

    -TYPE THERMOELECTRIC PERFORMANCE OF FUNCTIONALIZED CARBON NANOTUBE-FILLED POLYMER COMPOSITES A Thesis by DALLAS D. FREEMAN II Submitted to the Office of Graduate Studies of Texas A&M University in partial fulfillment of the requirements for the degree... of MASTER OF SCIENCE May 2012 Major Subject: Mechanical Engineering N-Type Thermoelectric Performance of Functionalized Carbon Nanotube-Filled Polymer Composites Copyright 2012 Dallas D. Freeman II...

  8. Development of youth leadership life skills of Texas youth as San Antonio Livestock Exposition school tour guides 

    E-Print Network [OSTI]

    Real, Laura A; Real, Laura A.

    2005-02-17

    training. The target population was Texas 4-H, FFA, and FCCLA members who served as school tour guides at the San Antonio Livestock Exposition. School tour guides referred to the 4-H, FFA, FCCLA members who imparted their personal knowledge... guide, and previous leadership skills training. 5 CHAPTER II REVIEW OF LITERATURE This literature review provides a foundation of previous research regarding the relationship between youth leadership life skills development (YLLSD...

  9. Responding to budget concerns: Hewlett-Woodmere School District's community budget advisory committee's first year's work, October 1989-1990 

    E-Print Network [OSTI]

    Sweeney, Erin Elizabeth Marie

    1990-01-01

    those to which they have opened my eyes, ears, heart, mind and opportunities for success. TABLE OF CONTENTS Page ABSTRACT . ACKNOWLEDGEMENTS TABLE OF CONTENTS lv INTRODUCTION History of the District The Process The Problem The Project II... the proposed School District budget. The successive defeats forced the School District to adopt an austerity budget for the ttrst time in its ninety-one year history. Austerity is a state mandated contingency program that goes into effect when voters cannot...

  10. Ponnequin phase I and II (PSCo) Wind Farm | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on QA:QA J-E-1 SECTION J APPENDIXsourceII JumpQuarterly SmartDB-2, Blue MountainSchoolPrairiePonder, Texas:I and II (PSCo)

  11. Under consideration for publication in Math. Struct. in Comp. Science Equilibrium and Termination II: the case of

    E-Print Network [OSTI]

    Danos, Vincent - Laboratoire Preuves, Programmes et Systèmes, Université Paris 7

    II: the case of Petri nets Vincent Danos and Nicolas Oury School of Informatics, University class of Petri nets equipped with stochastic mass action semantics. We establish a simple algebraic the detailed balance condition familiar from the thermodynamics of reaction networks. We also find that when

  12. Sedbergh School - The Mind

    E-Print Network [OSTI]

    Macfarlane, Alan

    2015-06-16

    SEDBERGH DAYS THE DEVELOPMENT OF THE MIND School Library – posed photo 1959 - 2 CONTENTS GENERAL Prolegomena to study of intellectual developments 3 Thoughts on intellectual development 22 Civics and other... are accomplished with reasonable success, and probably with the added pleasure of co- captain Jamie Bruce-Lockhart and his brother Sandy, we will then have a set of detailed materials for three children over the first 25 years or so of their lives...

  13. Single superpartner production at Tevatron Run II

    E-Print Network [OSTI]

    F. Deliot; G. Moreau; C. Royon

    2000-07-25

    We study the single productions of supersymmetric particles at Tevatron Run II which occur in the $2 \\to 2-body$ processes involving R-parity violating couplings of type $\\l'_{ijk} L_i Q_j D_k^c$. We focus on the single gaugino productions which receive contributions from the resonant slepton productions. We first calculate the amplitudes of the single gaugino productions. Then we perform analyses of the single gaugino productions based on the three charged leptons and like sign dilepton signatures. These analyses allow to probe supersymmetric particles masses beyond the present experimental limits, and many of the $\\l'_{ijk}$ coupling constants down to values smaller than the low-energy bounds. Finally, we show that the studies of the single gaugino productions offer the opportunity to reconstruct the $\\tilde \\chi^0_1$, $\\tilde \\chi^{\\pm}_1$, $\\tilde \

  14. High School Girls Honored for Math, Science Achievements at Sandia...

    Broader source: Energy.gov (indexed) [DOE]

    Tabatha Barrington, East Union High School Suman Tripathy, Foothill High School Carmen Jimenez, Fremont High School Morgan Correia, Granada High School Megan Kristovich, Livermore...

  15. Thomas Jefferson High School for Science & Technology National...

    Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

    Hill School, Kansas City, Mo. Santa Monica High School, Santa Monica, Calif. Smoky Hill High School, Aurora, Colo. State College Are High School, State College, Pa. Sycamore...

  16. COLLEGE OF HEALTH & HUMAN SERVICES SCHOOL OF NURSING SCHOOL OF HEALTH AND APPLIED HUMAN SCIENCES SCHOOL OF SOCIAL WORK

    E-Print Network [OSTI]

    Olszewski Jr., Edward A.

    Telling: Building Self Efficacy, Optimism and Enhancing School Performance with Middle School StudentsCOLLEGE OF HEALTH & HUMAN SERVICES SCHOOL OF NURSING SCHOOL OF HEALTH AND APPLIED HUMAN SCIENCES SCHOOL OF SOCIAL WORK CHHS SUCCESS April/May 2013 The College of Health and Human Services is dedicated

  17. Thermostable purified endoglucanase II from Acidothermus cellulolyticus ATCC

    DOE Patents [OSTI]

    Adney, William S. (Golden, CO); Thomas, Steven R. (Denver, CO); Nieves, Rafael A. (Lakewood, CO); Himmel, Michael E. (Littleton, CO)

    1994-01-01

    A purified low molecular weight endoglucanase II from Acidothermus cellulolyticus (ATCC 43068) is disclosed. The endoglucanase is water soluble, possesses both C.sub.1, and C.sub.x types of enzyme activity, a high degree of stability toward heat, and exhibits optimum temperature activity at about 81.degree. C. at pH's from about 2 to about 9, and at a inactivation temperature of about 100.degree. C. at pH's from about 2 to about 9.

  18. Thermostable purified endoglucanase II from Acidothermus cellulolyticus ATCC

    DOE Patents [OSTI]

    Adney, W.S.; Thomas, S.R.; Nieves, R.A.; Himmel, M.E.

    1994-11-22

    A purified low molecular weight endoglucanase II from Acidothermus cellulolyticus (ATCC 43068) is disclosed. The endoglucanase is water soluble, possesses both C[sub 1], and C[sub x] types of enzyme activity, a high degree of stability toward heat, and exhibits optimum temperature activity at about 81 C at pH's from about 2 to about 9, and at a inactivation temperature of about 100 C at pH's from about 2 to about 9. 9 figs.

  19. School Energy Management 

    E-Print Network [OSTI]

    Wine, D.

    2011-01-01

    stream_source_info ESL-KT-11-11-59.pdf.txt stream_content_type text/plain stream_size 0 Content-Encoding UTF-8 stream_name ESL-KT-11-11-59.pdf.txt Content-Type text/plain; charset=UTF-8 ...

  20. Typed Self-Optimization

    E-Print Network [OSTI]

    Brown, Matt

    2013-01-01

    type T y[O]. The operator IsIs is self-applicative, in thatargument t is any of Is[O] or IsIs, and otherwise behavesproof constant introduced by IsIs proves that the type of t

  1. Department for Education: Secondary School Accountability Consultation

    E-Print Network [OSTI]

    Rambaut, Andrew

    aspects of schools' performance cannot easily be measured but are nevertheless important. School1 Department for Education: Secondary School Accountability Consultation Response by the Wellcome for schools. We have embarked on a programme of work to help improve school governance ­ details can be found

  2. NAVAL POSTGRADUATE SCHOOL Monterey, California

    E-Print Network [OSTI]

    #12;Thesis F2lJ6 NAVAL POSTGRADUATE SCHOOL Monterey, California THESIS AN ANALYSIS OF HYPERSPECTRAL;DUDLEY K~OX LlRRARY NAVAL -0 SCHOOL MONTE"ev C.A ;:I3~~5101 #12;5. FlJNDING NUMBERS 8, PERFOR"TE IN SYSTEMS TF.CHNOLOGY (SPACE SYSTEMS OPERATJONS) from the NAVAL POSTGRADUATE SCHOOL J. . . . Matthew

  3. SMB 2014 - Imaging Summer School

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    ranges. The school will address topics that are not commonly included in text books or class lectures, and typically obtained only through on-the-experiment training....

  4. Clemson University School of Architecture

    E-Print Network [OSTI]

    Stuart, Steven J.

    ) 0.2 Curriculum Requirement: Fulfills Architecture Technology Requirement1 Clemson University School of Architecture Clemson Architecture Center Charleston. South Carolina 29401 1. Course Description Architectural craft lab

  5. Los Alamos Dynamics Summer School

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    School Program Information and Application Process Contact Institute Director Charles Farrar (505) 663-5330 Email Professional Staff Assistant Jutta Kayser (505) 663-5649 Email...

  6. summer school flyer.indd

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    The summer school includes a wide range of topics such as: * Ring current and radiation belts * Magnetosphere-ionosphere coupling * Solar wind dynamics * Spacecraft charging *...

  7. School of Engineering Annual Report

    E-Print Network [OSTI]

    Alpay, S. Pamir

    Activities............................. Civil & Environmental Engineering.......... PROGRAMS Engineering Diversity Program....................................... Environmental EngineeringSchool of Engineering 1 9 9 9 Annual Report #12;University of ConnecticutUniversity of Connecticut

  8. 2015 High School Team Photos

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    High-School-Team-Photos- Sign In About | Careers | Contact | Investors | bpa.gov Search News & Us Expand News & Us Projects & Initiatives Expand Projects & Initiatives...

  9. Coligand-regulated assembly, fluorescence, and magnetic properties of Co(II) and Cd(II) complexes with a non-coplanar dicarboxylate

    SciTech Connect (OSTI)

    Xin, Ling-Yun; Liu, Guang-Zhen; Ma, Lu-Fang; Wang, Li-Ya

    2013-10-15

    A non-coplanar dicarboxylate ndca (H{sub 2}ndca=5-norbornene-2,3-dicarboxylic acid), combining with various dipyridyl-typed tectons, constructs six Cd(II)/Co(II) coordination polymers under hydrothermal conditions, namely [Co(ndca)(H{sub 2}O)]{sub n} (1), ([Co(ndca)(bpe)(H{sub 2}O)]·H{sub 2}O){sub n} (2), [Co(ndca)(bpa){sub 0.5}(H{sub 2}O)]{sub n} (3), [Cd(ndca)(bpe)(H{sub 2}O)]{sub n} (4), ([Cd(ndca)(bpa)(H{sub 2}O)]·0.5H{sub 2}O){sub n} (5), and ([Cd(ndca)(bpp) (H{sub 2}O)]·H{sub 2}O){sub n} (6) (bpe=1,2-di(4-pyridyl)ethylene, bpa=1,2-bi(4-pyridyl)ethane, and bpp=1,3-bis(4-pyridyl)propane). All these compounds contain various metal(II)–carboxylate motifs, including carboxylate binuclear (2, 4, 5), carboxylate chain (1, 6) and carboxylate layer (3), which are further extended by dipyridyl-typed coligands to afford a vast diversity of the structures with 2D pyknotic layers (1, 6), 2D open layer (5), 2D?3D interpenetrated networks (2,4), and 3D pillared-layer framework (3), respectively. In addition, fluorescent spectra of Cd(II) complexes and magnetic properties of Co(II) complexes are also given. - Graphical abstract: Six various cadmium(II)/cobalt(II)–organic frameworks were constructed by 5-norbornene-2,3-dicarboxylic acid and different bis(pyridine) rod-like tectons, and Cd (II) complexes exhibit blue–violet emissions, whereas Co (II) complexes show antiferromagnetic behaviours. Display Omitted.

  10. COLLEGE OF HEALTH & HUMAN SERVICES SCHOOL OF NURSING SCHOOL OF HEALTH AND APPLIED HUMAN SCIENCES SCHOOL OF SOCIAL WORK

    E-Print Network [OSTI]

    Olszewski Jr., Edward A.

    COLLEGE OF HEALTH & HUMAN SERVICES SCHOOL OF NURSING SCHOOL OF HEALTH AND APPLIED HUMAN SCIENCES SCHOOL OF SOCIAL WORK "Improving Health and Quality of Life Globally and in NC" Jock Brandis The Full

  11. Forster-Type Nonradiative Energy Transfer for Assemblies of Arrayed Nanostructures: Confinement Dimension vs Stacking Dimension

    E-Print Network [OSTI]

    Demir, Hilmi Volkan

    Forster-Type Nonradiative Energy Transfer for Assemblies of Arrayed Nanostructures: Confinement Demir*,, LUMINOUS! Center of Excellence for Semiconductor Lighting and Display, School of Electrical-type nonradiative energy transfer (NRET) provides us with the ability to transfer excitation energy between proximal

  12. Nevada High School Wind Farm | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on QA:QA J-E-1 SECTION J APPENDIXsourceII Jump to: navigation,National MarineUSAID ClimateState Lands Jump to:High School

  13. Norfolk Public Schools Wind Project | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on QA:QA J-E-1 SECTION J APPENDIXsourceII Jump to:Information 3rd| Open Energy InformationPublic Schools Wind

  14. Pipestone School District Wind Farm | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on QA:QA J-E-1 SECTION J APPENDIXsourceII JumpQuarterly SmartDB-2, Blue MountainSchool District Wind Farm Jump to:

  15. Pleasanton Public Schools Wind Project | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on QA:QA J-E-1 SECTION J APPENDIXsourceII JumpQuarterly SmartDB-2, Blue MountainSchool DistrictPlaxica Limited Jump

  16. Pocatello Community Charter School Wind Project | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on QA:QA J-E-1 SECTION J APPENDIXsourceII JumpQuarterly SmartDB-2, Blue MountainSchoolPrairie Jump to: navigation,

  17. Ponderosa High School Wind Project | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on QA:QA J-E-1 SECTION J APPENDIXsourceII JumpQuarterly SmartDB-2, Blue MountainSchoolPrairiePonder, Texas:

  18. John A. Burns School of Medicine (JABSOM) Doctor of Medicine Early Acceptance Program (DMEAP) for Entering Hawaii Resident Freshman

    E-Print Network [OSTI]

    John A. Burns School of Medicine (JABSOM) Doctor of Medicine Early Acceptance Program (DMEAP: _____________________________________ Date of Birth (mm/dd/yyyy): _________________ Describe why you want to pursue a career in medicine (Please type) Print Form #12;John A. Burns School of Medicine (JABSOM) Doctor of Medicine Early Acceptance

  19. University of Tennessee School of Music

    E-Print Network [OSTI]

    Grissino-Mayer, Henri D.

    University of Tennessee School of Music Ambassador Application Return your completed application to the School of Music Office. Please Read the Information Below before Applying: The School of Music Student Ambassadors

  20. 10th LANSCE School on Neutron Scattering

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    10th LANSCE School on Neutron Scattering LANSCE 10th LANSCE School on Neutron Scattering Home Abstract Lecturers Hands-On Experiments Free Day About the School Sponsors FAQ's...

  1. University of Connecticut School of Medicine

    E-Print Network [OSTI]

    Oliver, Douglas L.

    University of Connecticut School of Medicine Department of Psychiatry University of Connecticut Health Center, John Dempsey Hospital, Farmington CT University of Connecticut School of Medicine, Department of Psychiatry, UHP Outpatient Clinic, West Hartford CT University of Connecticut School

  2. Cardiff School of Planning and Geography

    E-Print Network [OSTI]

    Martin, Ralph R.

    Cardiff School of Planning and Geography Undergraduate Degree Programmes Entry 2015 www Cardiff School of Planning and Geography Teaching excellence Culturally diverseSupportive Friendly #12 Contents Cardiff School of Planning and Geography is a leading international centre for teaching

  3. Characterization of Corrosion Products and Microbes on Various Types of Metal Coupons Using Beamline 1.4.3

    E-Print Network [OSTI]

    Characterization of Corrosion Products and Microbes on Various Types of Metal Coupons Using of California, Irvine and Mackay School of Mines, University of Nevada, Reno Microbes primarily exist in complex

  4. 02 College of Information Science, School of InformaticsCollege of Information Science, School of InformaticsCollege of Information Science, School of InformaticsCollege of Information Science, School of InformaticsCollege of Information Science, School o

    E-Print Network [OSTI]

    Tanaka, Jiro

    of Information Science, School of InformaticsCollege of Information Science, School of InformaticsCollege of Information Science, School of InformaticsCollege of Information Science, School of InformaticsCollege of Information Science, School of InformaticsCollege of Information Science, School of Informatics

  5. Hybrid type checking

    E-Print Network [OSTI]

    Flanagan, C

    2006-01-01

    O’Callahan and J. -D. Choi. Hybrid dynamic data race detec-subtyping is sound, the hybrid compilation algorithmHybrid Type Checking Cormac Flanagan Department of Computer

  6. Fejer-type inequalities

    E-Print Network [OSTI]

    Mitroi, F C

    2011-01-01

    The aim of this paper is to present some new Fejer-type results for convex functions. Improvements of Young's inequality (the arithmetic-geometric mean inequality) and other applications to special means are pointed as well.

  7. EMPLOYMENT OVERVIEW HARVARD KENNEDY SCHOOL

    E-Print Network [OSTI]

    Schrag, Daniel

    EMPLOYMENT OVERVIEW HARVARD KENNEDY SCHOOL CAREER ADVANCEMENT 617-495-1161t career_advancement@hks.harvard.edut www.hks.harvard.edu/careert Class of 2013 HARVARD KENNEDY SCHOOL CLASS OF 2013 EMPLOYMENT OVERVIEWt in an educational program as of October. This overview reflects the diverse employment choices of Harvard Kennedy

  8. Graduate School Per Veritatem Vis

    E-Print Network [OSTI]

    Gereau, Robert W. IV

    . Hance, Jr. Robert E. Hernreich Priscilla L. Hill-Ardoin Thomas J. Hillman Louis G. Hutt, Jr. Donald A University 5 Board of Trustees 6 OfficersoftheUniversity 8 Deans of the Schools 9 Graduate School of Arts was edited in July 2012 by Associ- ate Dean Nancy P. Pope, stays in effect through July 2015. Credits

  9. School of Environment and Sustainability

    E-Print Network [OSTI]

    Saskatchewan, University of

    School of Environment and Sustainability Room 323, Kirk Hall 117 Science Place Saskatoon, SK S7N 5C8 Telephone: (306) 966-1985 E-mail: sens.info@usask.ca Master of Environment and Sustainability (MES) Opportunity Sustainability Science in the Delta Dialogue Network The School of Environment and Sustainability

  10. University Graduate School Academic Bulletin

    E-Print Network [OSTI]

    Indiana University

    's role in encouraging a creative environ- ment for scholarship, research, teaching and learning scholars. Through its connections with national higher education organizations, it serves as a resource of Library and Information Science, the School of Optometry, and the School of Public and Environmental

  11. International School on Energy Systems

    E-Print Network [OSTI]

    Daraio, Chiara

    Hier neuer QR-Code ISES 2015 International School on Energy Systems Training Course on Energy Systems for Young Researchers and Professionals The International School on Energy Systems ­ ISES 2015 and future energy systems. The program comprises presentations and discussions on the following subjects

  12. 3rd Elgersburg School 2011

    E-Print Network [OSTI]

    Knobloch,Jürgen

    Nonlinear Control 3rd Elgersburg School 2011 Nonlinear Control 3rd Elgersburg School 2011 Randy Freeman Professor Department of Electrical Engineering & Computer Science #12;Nonlinear Control 3rd Fabian Wirth Sponsor: Exercises and discussions by Dr. Robert Gregg #12;Nonlinear Control 3rd Elgersburg

  13. Nickel(II) and Copper(I,II)-based Metal-Organic Frameworks Incorporati...

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    Nickel(II) and Copper(I,II)-based Metal-Organic Frameworks Incorporating an Extended Trispyrazolate Linker Previous Next List Tabacaru, Aurel; Galli, Simona; Pettinari, Claudio;...

  14. The Graduate School New Mexico State University

    E-Print Network [OSTI]

    Johnson, Eric E.

    The Graduate School New Mexico State University Educational Services Building, Suite 301 PO Box Form and supporting documentation. #12;The Graduate School New Mexico State University Educational

  15. School Bus Emissions Study | Department of Energy

    Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

    School Bus Emissions Study School Bus Emissions Study 2003 DEER Conference Presentation: international Truck and Engine Corporation deer2003slodowske.pdf More Documents &...

  16. 11th LANSCE School on Neutron Scattering

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    11th LANSCE School on Neutron Scattering LANSCE 11th LANSCE School on Neutron Scattering Home Abstract Lecturers Lecturer Abstracts Hands-On Experiments Free Day About the...

  17. Energy Efficient Schools Initiative - Grants | Department of...

    Broader source: Energy.gov (indexed) [DOE]

    Maximum Rebate Varies by school district Program Info Sector Name State Administrator Energy Efficient Schools Initiative Website http:www.tn.goveesifinanceinc.shtml...

  18. School science project 'demystifies' Portsmouth Gaseous Diffusion...

    Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

    School science project 'demystifies' Portsmouth Gaseous Diffusion Plant Site School science project 'demystifies' Portsmouth Gaseous Diffusion Plant Site June 2, 2015 - 10:40am...

  19. Financing an EnergySmart School

    SciTech Connect (OSTI)

    2008-01-01

    EnergySmart Schools fact sheet on choosing an EnergySmart approach to school construction to increase the number of attractive financing options available.

  20. Financing an EnergySmart School

    Office of Energy Efficiency and Renewable Energy (EERE)

    EnergySmart Schools fact sheet on choosing an EnergySmart approach to school construction to increase the number of attractive financing options available.

  1. Los Alamos Space Weather Summer School

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    Non-U.S Citizens Mentors, Projects Papers, Reports Photos NSEC IGPPS Space Weather Summer School Los Alamos Space Weather Summer School June 1 - July 24, 2015 Contacts...

  2. HELIOPHYSICS II. ENERGY CONVERSION PROCESSES

    E-Print Network [OSTI]

    Hudson, Hugh

    with the term "solar flare" dominate our thinking about energy conversion from magnetic storage to other formsHELIOPHYSICS II. ENERGY CONVERSION PROCESSES edited by CAROLUS J. SCHRIJVER Lockheed Martin of a solar flare 11 2.3.1 Flare luminosity and mechanical energy 11 2.3.2 The impulsive phase (hard X

  3. Assignment II Saha & Boltzmann equations

    E-Print Network [OSTI]

    Spoon, Henrik

    Assignment II Saha & Boltzmann equations January 21, 2002 This assignment is meant to give you some practical experience in using the Saha and Boltzmann equations that govern the level populations in atoms;s =kT the partition function of ionization stage r. The Saha equation: N r+1 N r = 2U r+1 U r P e #18

  4. Green Schools Project Final Report

    SciTech Connect (OSTI)

    Verdict, M.

    2000-09-27

    The Alliance to Save Energy has responded to interest in the Green Schools concept from the New England states of Maine, New Hampshire and Vermont. The Alliance conducted a train-the-trainers workshop in Augusta, Maine March 17--18, 1999. This work is part of a Green Schools replication project leveraged by funds from another source, NORDAX, which contributed $80,000 to provide partial support to staff at the Maine Energy Education Project (MEEP), Vermont Energy Education Program (VEEP), and New Hampshire Governor's Office to develop Green Schools Projects. DOE funds were used to conduct training, develop a network of state and local government, business and school partners to support school efficiency activities in those three states.

  5. 2005 Graduate School of Information Science and Technology 1 How to Register for Subjects on the Web CAMPUS SQUARE

    E-Print Network [OSTI]

    Yamamoto, Hirosuke

    2005 Graduate School of Information Science and Technology 1 How to Register for Subjects. - Symbols can be used. II. Register for Subjects 1. Step 1: Click " (Register)" on Top Menu to enter. Enter the registration page. 3. Search subjects which meet your conditions. Step 3-1: Select your department. Step 3

  6. ORIGINAL PAPER Caspase-3 feeds back on caspase-8, Bid and XIAP in type I Fas

    E-Print Network [OSTI]

    Timmer, Jens

    ORIGINAL PAPER Caspase-3 feeds back on caspase-8, Bid and XIAP in type I Fas signaling in primary and activation of caspase-3 as compared to the type II pathway which first requires caspase- 8-mediated Bid into the fully processed p18 species. Our data do not discriminate if p18 positively or negatively influences Fas

  7. Mittwoch, 28.05.2014 Zeit H17, NW II H18, NW II H20, NW II

    E-Print Network [OSTI]

    Ott, Albrecht

    Beliefs and Fracking Gebäude Audimax 09:40 (Gebäudewechsel Audimax -> NW II) 10:00 "Hydrogeologie von

  8. FSP Index Top Performing Schools http://www.academicanalytics.com/TopSchools/TopSchools.aspx 1 of 3 2/12/2008 5:13 PM

    E-Print Network [OSTI]

    Tesanovic, Zlatko

    FSP Index Top Performing Schools http://www.academicanalytics.com/TopSchools/TopSchools.aspx 1 of 3 2/12/2008 5:13 PM Tuesday, February 12, 2008 | 5:13 PM EST FSP Index Top Performing Schools 2006 University of Iowa Brown University #12;FSP Index Top Performing Schools http://www.academicanalytics.com/TopSchools/TopSchools

  9. Effects on School Enrollment and Performance of a Conditional Transfers Program in Mexico

    E-Print Network [OSTI]

    Dubois, Pierre; de Janvry, Alain; Sadoulet, Elisabeth

    2003-01-01

    schooling decisions, school performance, dynamic decisions,enroll- ment and school performance determine educationalthe determinants of school performance is particularly

  10. WASTES II model storage requirements benchmark testing

    SciTech Connect (OSTI)

    Shay, M.R.; Walling, R.C.; Altenhofen, M.K.

    1986-09-01

    A study was conducted to benchmark results obtained from using the Waste System Transportation and Economic Simulation - Version II (WASTES II) model against information published in the ''Spent Fuel Storage Requirements'' report (DOE/RL-84-1). The WASTES model was developed by PNL for use in evaluating the spent-fuel storage and transportation requirements and costs for the US Department of Energy (DOE). The ''Spent Fuel Storage Requirements'' report is issued annually by the DOE and provides both historical/projected spent fuel inventory data and storage requirements data based on information supplied directly from utilities. The objective of this study is to compare the total inventory and storage requirements documented in the ''Spent Fuel Storage Requirements'' report with similar data that results from use of the WASTES model. Three differences have been identified as a result of benchmark testing. Two minor differences are present in the total inventory projected and the equivalent metric tons of uranium of spent fuel requiring storage. These differences result from the way reinserted spent fuel is handled and the methods used to calculate mass equivalents. A third difference is found in the storage requirements for the case that uses intra-utility transshipment. This discrepancy is due to the Oyster Creek reactor, which is shown to not require additional storage in the Spent Fuel Storage Requirements report, even though there is no destination reactor of the same type within its utility. The discrepancy was corrected soon after the 1984 ''Spent Fuel Storage Requirements report was issued and does not appear in more recent documents (DOE/RL-85-2).

  11. Swift Progress on NSLS-II Booster

    ScienceCinema (OSTI)

    None

    2013-07-17

    Get an inside look around the booster ring at the National Synchrotron Light Source II. The booster is part of the injector complex for NSLS-II, now under construction at Brookhaven Lab.

  12. PARS II Training Materials | Department of Energy

    Energy Savers [EERE]

    Training Materials PARS II Training Materials PARS II presentation hand-outs and step-by-step "how to" exercises for each course are available for download. Users who are attending...

  13. Investigating the Distribution of Teacher Quality by Race/Ethnicity and Socioeconomic Status of Students by School in One Large School District 

    E-Print Network [OSTI]

    McGlohn, Robin

    2012-07-16

    large school district. The population for this study included 69 schools during the 2007-2008 school year within one large suburban school district. Included in this study were 47 elementary schools, 14 middle schools, and 8 high schools...

  14. COLLEGE OF HEALTH & HUMAN SERVICES SCHOOL OF NURSING SCHOOL OF HEALTH/APPLIED HUMAN SCIENCES SCHOOL OF SOCIAL WORK

    E-Print Network [OSTI]

    Olszewski Jr., Edward A.

    COLLEGE OF HEALTH & HUMAN SERVICES SCHOOL OF NURSING SCHOOL OF HEALTH/APPLIED HUMAN SCIENCES SCHOOL OF SOCIAL WORK Faculty Scholarly and Research Interests 2012-2014 School of Health/Applied Human Sciences Personnel Physical Activity/exercise levels. Licensure to teach K-12 HPE. K-12 Healthful Living Curriculum

  15. Nilpotence and Stable Homotopy Theory II

    E-Print Network [OSTI]

    1997-12-14

    Nilpotence and Stable Homotopy. Theory II. Michael J. Hopkins. ?. Jeffrey H. Smith. †. Massachusetts Institute of Technology, Cambridge Massachusetts.

  16. Type Ia Supernovae

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Homesum_a_epg0_fpd_mmcf_m.xls" ,"Available from WebQuantity ofkandz-cm11 Outreach Home RoomPreservationBio-Inspired SolarAbout /Two Electron Holes in HematiteType Ia Supernovae Type Ia

  17. Agreement Type Union

    National Nuclear Security Administration (NNSA)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Homesum_a_epg0_fpd_mmcf_m.xls" ,"Available from WebQuantity of NaturalDukeWakefield Municipal Gas &SCE-SessionsSouthReporteeo | National Nucleara min [Type the abstract of theType

  18. Basics, types Evolution

    E-Print Network [OSTI]

    Crenshaw, Michael

    to nuclear fusion. · Novae radiate primarily in the UV to X-ray region. · Types: ­ Classical Novae: only one is hot enough for explosive fusion. For classical novae, this happens on a time scale of 103 ­ 105 years. · Thermonuclear runaway (TNR): capture of protons by heavy elements (CNO cycle), happens in seconds #12;5 Novae

  19. EISCAT Radar School, Kiruna, 2005 Outrigger in

    E-Print Network [OSTI]

    into regional fibre network, sharing costs with schools, health centres etc. #12;Bo Thidé EISCAT Radar School Thidé EISCAT Radar School, Kiruna,, 200515 LOFAR Phase 2 into Lower Saxony, Schleswig in innovative ways #12;Bo Thidé EISCAT Radar School, Kiruna,, 200524 LOFAR was conceived by the astrophysics

  20. May 15, 2014 1 School of Science

    E-Print Network [OSTI]

    May 15, 2014 1 School of Science Welcome to the School of Science at IUPUI! The School of Science and staff on a campus with a multitude of resources to help students succeed. The School of Science offers. In addition to preparing students for science or technology-related careers and for advanced study in graduate

  1. A New School of Thought University of South Carolina School of Medicine Greenville

    E-Print Network [OSTI]

    Almor, Amit

    A New School of Thought University of South Carolina School of Medicine Greenville #12;There's a new kind of medical school in the Upstate of South Carolina, a place where tomorrow's doctors and the community. The UNIVERSITY OF SOUTH CAROLINA SCHOOL OF MEDICINE GREENVILLE is a four-year medical school

  2. GOVERNANCE OF THE GRADUATE SCHOOL OF THE GRADUATE SCHOOL AND UNIVERSITY CENTER

    E-Print Network [OSTI]

    Johnson Jr.,, Ray

    graduate programs of The Graduate School, to set standards of admission and academic performance1 GOVERNANCE OF THE GRADUATE SCHOOL OF THE GRADUATE SCHOOL AND UNIVERSITY CENTER THE CITY of The Graduate School and University Center, hereafter referred to as The Graduate School, is the chief academic

  3. GOVERNANCE OF THE GRADUATE SCHOOL OF THE GRADUATE SCHOOL AND UNIVERSITY CENTER

    E-Print Network [OSTI]

    Artemov, Sergei N.

    graduate programs of The Graduate School, to set standards of admission and academic performance1 GOVERNANCE OF THE GRADUATE SCHOOL OF THE GRADUATE SCHOOL AND UNIVERSITY CENTER THE CITY School and University Center, hereafter referred to as The Graduate School, is the chief academic

  4. SPECTROSCOPY OF TYPE Ia SUPERNOVAE BY THE CARNEGIE SUPERNOVA PROJECT

    SciTech Connect (OSTI)

    Folatelli, Gaston [Kavli Institute for the Physics and Mathematics of the Universe (Kavli IPMU, WPI), Todai Institutes for Advanced Study, the University of Tokyo, 277-8583 Kashiwa (Japan); Morrell, Nidia; Phillips, Mark M.; Hsiao, Eric; Campillay, Abdo; Contreras, Carlos; Castellon, Sergio; Roth, Miguel [Las Campanas Observatory, Carnegie Observatories, Casilla 601, La Serena (Chile); Hamuy, Mario; Anderson, Joseph P. [Departamento de Astronomia, Universidad de Chile, Casilla 36-D, Santiago (Chile); Krzeminski, Wojtek [N. Copernicus Astronomical Center, ul. Bartycka 18, 00-716 Warszawa (Poland); Stritzinger, Maximilian [Department of Physics and Astronomy, Aarhus University, Ny Munkegade 120, DK-8000 Aarhus C (Denmark); Burns, Christopher R.; Freedman, Wendy L.; Madore, Barry F.; Murphy, David; Persson, S. E. [Observatories of the Carnegie Institution of Washington, 813 Santa Barbara Street, Pasadena, CA 91101 (United States); Prieto, Jose L. [Department of Astrophysical Sciences, Princeton University, 4 Ivy Ln., Princeton, NJ 08544 (United States); Suntzeff, Nicholas B.; Krisciunas, Kevin, E-mail: gaston.folatelli@ipmu.jp [George P. and Cynthia Woods Mitchell Institute for Fundamental Physics and Astronomy, Department of Physics and Astronomy, Texas A and M University, College Station, TX 77843 (United States); and others

    2013-08-10

    This is the first release of optical spectroscopic data of low-redshift Type Ia supernovae (SNe Ia) by the Carnegie Supernova Project including 604 previously unpublished spectra of 93 SNe Ia. The observations cover a range of phases from 12 days before to over 150 days after the time of B-band maximum light. With the addition of 228 near-maximum spectra from the literature, we study the diversity among SNe Ia in a quantitative manner. For that purpose, spectroscopic parameters are employed such as expansion velocities from spectral line blueshifts and pseudo-equivalent widths (pW). The values of those parameters at maximum light are obtained for 78 objects, thus providing a characterization of SNe Ia that may help to improve our understanding of the properties of the exploding systems and the thermonuclear flame propagation. Two objects, namely, SNe 2005M and 2006is, stand out from the sample by showing peculiar Si II and S II velocities but otherwise standard velocities for the rest of the ions. We further study the correlations between spectroscopic and photometric parameters such as light-curve decline rate and color. In agreement with previous studies, we find that the pW of Si II absorption features are very good indicators of light-curve decline rate. Furthermore, we demonstrate that parameters such as pW2 (Si II 4130) and pW6 (Si II 5972) provide precise calibrations of the peak B-band luminosity with dispersions of Almost-Equal-To 0.15 mag. In the search for a secondary parameter in the calibration of peak luminosity for SNe Ia, we find a Almost-Equal-To 2{sigma}-3{sigma} correlation between B-band Hubble residuals and the velocity at maximum light of S II and Si II lines.

  5. Energy.gov Page Types

    Broader source: Energy.gov [DOE]

    Learn about the standard page types available in the Energy.gov Drupal content management system. For information about other available page types, or to request a new kind of page type, contact...

  6. Practical pluggable types for Java

    E-Print Network [OSTI]

    Papi, Matthew M

    2008-01-01

    This paper introduces the Checker Framework, which supports adding pluggable type systems to the Java language in a backward-compatible way. A type system designer defines type qualifiers and their semantics, and a compiler ...

  7. Window Types | Department of Energy

    Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

    aluminum or vinyl cladding reduces maintenance requirements. Types of Window Glazing or Glass In addition to choosing a frame type, you will need to consider what type of glazing...

  8. Law School Event Composting Guide

    E-Print Network [OSTI]

    Wolfe, Patrick J.

    Law School Event Composting Guide HLS SUSTAINABILITY PROGRAM JANUARY 2011 Thank you for your interest in event composting! Separating materials for composting is easy, and organic materials comprise a significant portion of event waste. Composting instead

  9. Clemson University School Of Architecture

    E-Print Network [OSTI]

    Stuart, Steven J.

    Clemson University School Of Architecture Clemson Architecture Center in Charleston 400 Graduate and Undergraduate Architecture 0.2 Curriculum Requirements: ARCH;between architecture, site, and context, this studio may be located in Clemson

  10. High Performance Computing School COMSC

    E-Print Network [OSTI]

    Martin, Ralph R.

    High Performance Computing School COMSC This module aims to provide the students with fundamental knowledge and understanding of techniques associated with High Performance Computing and its practical' skills in analysing and evaluating High Performance Computing and will be structured around

  11. Guidelines for Energy Efficient Schools 

    E-Print Network [OSTI]

    McClure, J. D.; Estes, J. M.; Bicknell, K. N.; Estes, M. C.

    1988-01-01

    Operational experience of several schools designed with energy efficiency as a design criteria is discussed in this paper. Actual monthly energy usage and cost are provided. Annual energy cost performance ($/ft^2-yr) and energy performance (BTU/FT^2...

  12. School of Mines Graduate Bulletin

    E-Print Network [OSTI]

    is for your use as a source of continuing reference. Please save it. Published by Colorado School of Mines & Divisions. . . . . . . . . . . . . . . . 5 General Information . . . . . . . . . . . . . . . . . . . . . 6 Mission and Goals . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 6 Institutional Values

  13. School of Mines Graduate Bulletin

    E-Print Network [OSTI]

    : This Bulletin is for your use as a source of continuing reference. Please save it. Published by Colorado School & Divisions. . . . . . . . . . . . . . . . 5 General Information . . . . . . . . . . . . . . . . . . . . . 6 Mission and Goals . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 6 Institutional Values

  14. School of Mines Graduate Bulletin

    E-Print Network [OSTI]

    is for your use as a source of continuing reference. Please save it. Published by Colorado School of Mines . . . . . . . . . . . . . . . . . 5 Academic Departments & Divisions . . . . . . . . . . . . 5 General Information 6 Mission and Goals . . . . . . . . . . . . . . . . . . . . . . . . . . 6 Institutional Values and Principles

  15. School of Mines Graduate Bulletin

    E-Print Network [OSTI]

    is for your use as a source of continuing reference. Please save it. Published by Colorado School of Mines General Information . . . . . . . . . . . . . . . . . . . . . 6 Mission and Goals . . . . . . . . . . . . . . . . . . . . . . . . . . 6 Institutional Values and Principles . . . . . . . . . . . . . . 6 History of CSM

  16. Missouri School District Charges Up

    Broader source: Energy.gov [DOE]

    Missouri's Lee's Summit R-7 school district's distribution fleet was tired. Many of the vehicles had racked up more than 300,000 miles and made frequent trips to the shop to repair the 20 plus-year-old parts.

  17. BEF- Solar 4R Schools

    Broader source: Energy.gov [DOE]

    The school agrees to: own and maintain the solar system, provide access to a network in order to transfer solar data and offer and implement an educational and/or public outreach strategy. Solar ...

  18. National Nuclear Chemistry Summer School

    Broader source: Energy.gov [DOE]

    he Division of Nuclear Chemistry and Technology of the American Chemical Society (ACS) is sponsoring two INTENSIVE six-week Summer Schools in Nuclear and Radiochemistry for undergraduates. Funding...

  19. National Nuclear Chemistry Summer School

    Broader source: Energy.gov [DOE]

    The Division of Nuclear Chemistry and Technology of the American Chemical Society (ACS) is sponsoring two INTENSIVE six-week Summer Schools in Nuclear and Radiochemistry for undergraduates. Funding is provided by the US Department of Energy.

  20. Development projects: Secondary school, Arnold 

    E-Print Network [OSTI]

    Anonymous

    This BULLETIN describes a secondary school at Arnold, Nottinghamshire, designed by the Development Group of the Architects and Building Branch of the Ministry of Education in collaboration with the Local Education Authority. It was the sixth...

  1. IIT SCHOOL OF APPLIED TECHNOLOGY

    E-Print Network [OSTI]

    Heller, Barbara

    . MANUFACTURINGTECHNOLOGY. #12;BE A LEADER OF THE NEXT INDUSTRIAL REVOLUTION. An undergraduate degree in IndustrialINDUSTRIAL TECHNOLOGY AND MANAGEMENT IIT SCHOOL OF APPLIED TECHNOLOGY INDUSTRIAL OPERATIONS. RESOURCE MANAGEMENT. INDUSTRIAL FACILITIES. SUPPLY CHAIN MANAGEMENT. SUSTAINABILITY

  2. Second generation Research Reactor Fuel Container (RRFC-II).

    SciTech Connect (OSTI)

    Abhold, M. E.; Baker, M. C.; Bourret, S. C.; Harker, W. C.; Pelowitz, D. G.; Polk, P. J.

    2001-01-01

    The second generation Research Reactor Fuel Counter (RRFC-II) has been developed to measure the remaining {sup 235}U content in foreign spent Material Test Reactor (MTR)-type fuel being returned to the Westinghouse Savannah River Site (WSRS) for interim storage and subsequent disposal. The fuel to be measured started as fresh fuel nominally with 93% enriched Uraniuin alloyed with A1 clad in Al. The fuel was irradiated to levels of up to 65% burnup. The RRFC-II, which will be located in the L-Basin spent fuel pool, is intended to assay the {sup 235}U content using a combination of passive neutron coincidence counting, active neutron coincidence counting, and active-multiplicity analysis. Measurements will be done underwater, eliminating the need for costly and hazardous handling operations of spent fuel out of water. The underwater portion of the RRFC-II consists of a watertight stainless steel housing containing neutron and gamma detectors and a scanning active neutron source. The portion of the system that resides above water consists of data-processing electronics; electromechanical drive electronics; a computer to control the operation of the counter, to collect, and to analyze data; and a touch screen interface located at the equipment rack. The RRFC-II is an improved version of the Los Alamos-designed RRFC already installed in the SRS Receipts Basin for Offsite Fuel. The RRFC-II has been fabricated and is scheduled for installation in late FY 2001 pending acceptance testing by Savannah River Site personnel.

  3. Educating the Nation: I. Schools

    E-Print Network [OSTI]

    Mandler, P.

    2014-01-01

    Education’, Comparative Education Review 29 (1985), 145-70, quote at 147-8; Fabrice Murtin and Martina Viarengo, ‘The Expansion and Convergence of Compulsory Schooling in Western Europe, 1950-2000’, Economica 78 (2011), 501-22. 7 Michael Sanderson... sensitive commentators, interpret rapid comprehensivization by Labour authorities as evidence of a lack of a noisy ‘grammar-school constituency’ (Stoke, Leeds) and/or the presence of ‘working-class communities with relatively few education...

  4. II

    Office of Legacy Management (LM)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Homesum_a_epg0_fpd_mmcf_m.xls" ,"Available from WebQuantity of NaturalDukeWakefield Municipal Gas &SCE-SessionsSouth DakotaRobbins and700, 1.Reports1E~ S·D3GraniteS T A/ I' Il7aa AMY

  5. II

    Office of Legacy Management (LM)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Homesum_a_epg0_fpd_mmcf_m.xls" ,"Available from WebQuantity of NaturalDukeWakefield Municipal Gas &SCE-SessionsSouth DakotaRobbins and700, 1.Reports1E~ S·D3GraniteS T A/ I' Il7aa AMY

  6. II

    Office of Legacy Management (LM)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Homesum_a_epg0_fpd_mmcf_m.xls" ,"Available from WebQuantity of NaturalDukeWakefield Municipal Gas &SCE-SessionsSouth DakotaRobbins and700, 1.Reports1E~ S·D3GraniteS T A/ I' Il7aa

  7. II

    Office of Legacy Management (LM)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Homesum_a_epg0_fpd_mmcf_m.xls" ,"Available from WebQuantity of NaturalDukeWakefield Municipal Gas &SCE-SessionsSouth DakotaRobbins and700, 1.Reports1E~ S·D3GraniteS T A/ I' Il7aa :

  8. II

    Office of Legacy Management (LM)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Homesum_a_epg0_fpd_mmcf_m.xls" ,"Available from WebQuantity of NaturalDukeWakefield Municipal Gas &SCE-SessionsSouthReport for the t-) S/,,5 'a C O M P R E H E N SGwen} ;im1 * I

  9. II

    Gasoline and Diesel Fuel Update (EIA)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Homesum_a_epg0_fpd_mmcf_m.xls" ,"Available from WebQuantity of Natural GasAdjustments (Billion Cubic Feet) Wyoming Dry NaturalPrices1Markets See full Hydrocarbon Gas LiquidsENERGYww0,

  10. Dust around Type Ia supernovae

    E-Print Network [OSTI]

    Wang, Lifan

    2005-01-01

    Dust around Type Ia supernovae Lifan Wang 1,2 LawrenceIa. Subject headings: Supernovae: General, Dust, Extinctionline) bands for Type Ia supernovae. (a), upper panel, shows

  11. School's out for summer 

    E-Print Network [OSTI]

    Churchill, Caitlin

    2009-01-01

    education and rainwater harvesting were also included in the basic curriculum last summer, but Whittlesey said these topics have been expanded to create a separate Water Academy that includes lessons on watersheds, water systems, properties of water.... Students learn about collecting water from roof surface areas and various types of rainwater harvesting collection devices. 4. Texas AgriLife Extension specialist Larry Hysmith instructs students on how to collect water samples and aquatic life from Lake...

  12. The impact of teacher leadership on school effectiveness in selected exemplary secondary schools 

    E-Print Network [OSTI]

    Hook, David Paul

    2006-08-16

    This qualitative study used naturalistic inquiry methodology to study the impact that teacher leadership has on school effectiveness. Two suburban high schools were chosen for this study. Both of these schools had been ...

  13. School of Engineering Code Approved February 2, 2009 School of Engineering

    E-Print Network [OSTI]

    School of Engineering Code Approved February 2, 2009 Code of the School of Engineering University of Kansas Engineering Senate Revised May 29, 2009 #12;The School of Engineering Code Approved February 2 .......................................................................................................... 4 ARTICLE III THE ENGINEERING SENATE

  14. Johnny Walks to School - Does Jane? Sex Differences in Children's Active Travel to School

    E-Print Network [OSTI]

    McMillan, Tracy; Day, Kristen; Boarnet, Marlon; Alfonzo, Mariela; Anderson, Craig

    2006-01-01

    Johnny Walks to School—Does Jane? Sex Differences… Osborne,at Johnny Walks to School—Does Jane? Sex Differences… theBehavior Johnny Walks to School—Does Jane? Sex Differences…

  15. School of Engineering | University of Connecticut Annual Report School of Engineering Annual Report 1

    E-Print Network [OSTI]

    Alpay, S. Pamir

    2000 2001 School of Engineering | University of Connecticut Annual Report #12;School of Engineering Annual Report 1 University of ConnecticutUniversity of Connecticut School of Engineering Annual Report

  16. Organizational, financial and demographic characteristics of charter schools in Texas and their relationship to school performance 

    E-Print Network [OSTI]

    D'Lorm, Raul

    2007-04-25

    The deepening dissatisfaction with traditional public schools has inspired changes in the educational system. In less than a decade charter schools have gone from nonexistent to widespread. Charter schools are different from other reforms because...

  17. The Assembly of the Belle II TOP Counter

    E-Print Network [OSTI]

    Boqun Wang; for the Belle II PID Group

    2015-01-13

    A new type of ring-imaging Cherenkov counter, called TOP counter, has been developed for particle identification at the Belle II experiment to run at the SuperKEKB accelerator in KEK, Japan. The detector consists of 16 identical modules arranged azimuthally around the beam line. The assembly procedure for a TOP module is described. This procedure includes acceptance testing of the quartz mirror, prism, and quartz bar radiators. The acceptance tests include a chip search and measurements of bulk transmittance and total internal reflectance. The process for aligning and gluing the optical components together is described.

  18. Thomas Jefferson High School for Science & Technology Wins...

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    School, Richmond, Takes Second NEWPORT NEWS, Va., Feb. 27, 2010 - The Thomas Jefferson High School for Science and Technology from Alexandria beat out St. Christopher's School...

  19. North Carolina School of Science and Mathematics from Durham...

    Broader source: Energy.gov (indexed) [DOE]

    at the National Building Museum in Washington. North Carolina School of Science and Mathematics beat Mira Loma High School from Sacramento CA in the high school national...

  20. School Culture and Performance at Different Middle Level Structures

    E-Print Network [OSTI]

    Gomez, Martin Omar

    2010-01-01

    behaviors raise school performance would be immenselyG. A. (1996b). School culture and performance: Testing thesignificant in explaining school performance. The purpose of

  1. Anti-Lemons: School Reputation and Educational Quality

    E-Print Network [OSTI]

    MacLeod, Bentley

    2009-01-01

    and information on school performance: Lessons from Chile,”and information on school performance: Lessons from Chile,”will unambiguously raise school performance and student

  2. Boulder Valley School District (Colorado) Power Purchase Agreement...

    Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

    Boulder Valley School District (Colorado) Power Purchase Agreement Case Study Boulder Valley School District (Colorado) Power Purchase Agreement Case Study Boulder Valley School...

  3. 2012 LANSCE Neutron Scattering School | Los Alamos National Laboratory

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    2 LANSCE Neutron Scattering School LANSCE 2012 LANSCE Neutron Scattering School Home About the School Hands-On Experiments Quick Links Application - Closed Schedule Poster...

  4. 2012 LANSCE Neutron Scattering School | Los Alamos National Laboratory

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    1 LANSCE Neutron Scattering School LANSCE 2011 LANSCE Neutron Scattering School Home NSS 2011 About the School Lecturers Hands-On Experiments Quick Links Application Schedule...

  5. Energy Design Guidelines for High Performance Schools: Hot and...

    Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

    Design Guidelines for High Performance Schools: Hot and Humid Climates Energy Design Guidelines for High Performance Schools: Hot and Humid Climates School districts around the...

  6. Building Energy-Efficient Schools in New Orleans: Lessons Learned...

    Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

    Energy- Efficient Schools in New Orleans Lessons Learned 2 3 The devastation of schools in New Orleans from the hurricanes was exacerbated by many years of deferred school...

  7. Belle II Technical Design Report

    E-Print Network [OSTI]

    T. Abe; I. Adachi; K. Adamczyk; S. Ahn; H. Aihara; K. Akai; M. Aloi; L. Andricek; K. Aoki; Y. Arai; A. Arefiev; K. Arinstein; Y. Arita; D. M. Asner; V. Aulchenko; T. Aushev; T. Aziz; A. M. Bakich; V. Balagura; Y. Ban; E. Barberio; T. Barvich; K. Belous; T. Bergauer; V. Bhardwaj; B. Bhuyan; S. Blyth; A. Bondar; G. Bonvicini; A. Bozek; M. Bracko; J. Brodzicka; O. Brovchenko; T. E. Browder; G. Cao; M. -C. Chang; P. Chang; Y. Chao; V. Chekelian; A. Chen; K. -F. Chen; P. Chen; B. G. Cheon; C. -C. Chiang; R. Chistov; K. Cho; S. -K. Choi; K. Chung; A. Comerma; M. Cooney; D. E. Cowley; T. Critchlow; J. Dalseno; M. Danilov; A. Dieguez; A. Dierlamm; M. Dillon; J. Dingfelder; R. Dolenec; Z. Dolezal; Z. Drasal; A. Drutskoy; W. Dungel; D. Dutta; S. Eidelman; A. Enomoto; D. Epifanov; S. Esen; J. E. Fast; M. Feindt; M. Fernandez Garcia; T. Fifield; P. Fischer; J. Flanagan; S. Fourletov; J. Fourletova; L. Freixas; A. Frey; M. Friedl; R. Fruehwirth; H. Fujii; M. Fujikawa; Y. Fukuma; Y. Funakoshi; K. Furukawa; J. Fuster; N. Gabyshev; A. Gaspar de Valenzuela Cueto; A. Garmash; L. Garrido; Ch. Geisler; I. Gfall; Y. M. Goh; B. Golob; I. Gorton; R. Grzymkowski; H. Guo; H. Ha; J. Haba; K. Hara; T. Hara; T. Haruyama; K. Hayasaka; K. Hayashi; H. Hayashii; M. Heck; S. Heindl; C. Heller; T. Hemperek; T. Higuchi; Y. Horii; W. -S. Hou; Y. B. Hsiung; C. -H. Huang; S. Hwang; H. J. Hyun; Y. Igarashi; C. Iglesias; Y. Iida; T. Iijima; M. Imamura; K. Inami; C. Irmler; M. Ishizuka; K. Itagaki; R. Itoh; M. Iwabuchi; G. Iwai; M. Iwai; M. Iwasaki; M. Iwasaki; Y. Iwasaki; T. Iwashita; S. Iwata; H. Jang; X. Ji; T. Jinno; M. Jones; T. Julius; T. Kageyama; D. H. Kah; H. Kakuno; T. Kamitani; K. Kanazawa; P. Kapusta; S. U. Kataoka; N. Katayama; M. Kawai; Y. Kawai; T. Kawasaki; J. Kennedy; H. Kichimi; M. Kikuchi; C. Kiesling; B. K. Kim; G. N. Kim; H. J. Kim; H. O. Kim; J. -B. Kim; J. H. Kim; M. J. Kim; S. K. Kim; K. T. Kim; T. Y. Kim; K. Kinoshita; K. Kishi; B. Kisielewski; K. Kleese van Dam; J. Knopf; B. R. Ko; M. Koch; P. Kodys; C. Koffmane; Y. Koga; T. Kohriki; S. Koike; H. Koiso; Y. Kondo; S. Korpar; R. T. Kouzes; Ch. Kreidl; M. Kreps; P. Krizan; P. Krokovny; H. Krueger; A. Kruth; W. Kuhn; T. Kuhr; R. Kumar; T. Kumita; S. Kupper; A. Kuzmin; P. Kvasnicka; Y. -J. Kwon; C. Lacasta; J. S. Lange; I. -S. Lee; M. J. Lee; M. W. Lee; S. -H. Lee; M. Lemarenko; J. Li; W. D. Li; Y. Li; J. Libby; A. Limosani; C. Liu; H. Liu; Y. Liu; Z. Liu; D. Liventsev; A. Lopez Virto; Y. Makida; Z. P. Mao; C. Marinas; M. Masuzawa; D. Matvienko; W. Mitaroff; K. Miyabayashi; H. Miyata; Y. Miyazaki; T. Miyoshi; R. Mizuk; G. B. Mohanty; D. Mohapatra; A. Moll; T. Mori; A. Morita; Y. Morita; H. -G. Moser; D. Moya Martin; T. Mueller; D. Muenchow; J. Murakami; S. S. Myung; T. Nagamine; I. Nakamura; T. T. Nakamura; E. Nakano; H. Nakano; M. Nakao; H. Nakazawa; S. -H. Nam; Z. Natkaniec; E. Nedelkovska; K. Negishi; S. Neubauer; C. Ng; J. Ninkovic; S. Nishida; K. Nishimura; E. Novikov; T. Nozaki; S. Ogawa; K. Ohmi; Y. Ohnishi; T. Ohshima; N. Ohuchi; K. Oide; S. L. Olsen; M. Ono; Y. Ono; Y. Onuki; W. Ostrowicz; H. Ozaki; P. Pakhlov; G. Pakhlova; H. Palka; H. Park; H. K. Park; L. S. Peak; T. Peng; I. Peric; M. Pernicka; R. Pestotnik; M. Petric; L. E. Piilonen; A. Poluektov; M. Prim; K. Prothmann; K. Regimbal; B. Reisert; R. H. Richter; J. Riera-Babures; A. Ritter; A. Ritter; M. Ritter; M. Roehrken; J. Rorie; M. Rosen; M. Rozanska; L. Ruckman; S. Rummel; V. Rusinov; R. M. Russell; S. Ryu; H. Sahoo; K. Sakai; Y. Sakai; L. Santelj; T. Sasaki; N. Sato; Y. Sato; J. Scheirich; J. Schieck; C. Schwanda; A. J. Schwartz; B. Schwenker; A. Seljak; K. Senyo; O. -S. Seon; M. E. Sevior; M. Shapkin; V. Shebalin; C. P. Shen; H. Shibuya; S. Shiizuka; J. -G. Shiu; B. Shwartz; F. Simon; H. J. Simonis; J. B. Singh; R. Sinha; M. Sitarz; P. Smerkol; A. Sokolov; E. Solovieva; S. Stanic; M. Staric; J. Stypula; Y. Suetsugu; S. Sugihara; T. Sugimura; K. Sumisawa; T. Sumiyoshi; K. Suzuki; S. Y. Suzuki; H. Takagaki; F. Takasaki; H. Takeichi; Y. Takubo; M. Tanaka; S. Tanaka; N. Taniguchi; E. Tarkovsky; G. Tatishvili; M. Tawada; G. N. Taylor; Y. Teramoto; I. Tikhomirov; K. Trabelsi; T. Tsuboyama; K. Tsunada; Y. -C. Tu; T. Uchida; S. Uehara; K. Ueno; T. Uglov; Y. Unno; S. Uno; P. Urquijo; Y. Ushiroda; Y. Usov; S. Vahsen; M. Valentan; P. Vanhoefer; G. Varner; K. E. Varvell; P. Vazquez; I. Vila; E. Vilella; A. Vinokurova; J. Visniakov; M. Vos; C. H. Wang; J. Wang; M. -Z. Wang; P. Wang; A. Wassatch; M. Watanabe; Y. Watase; T. Weiler; N. Wermes; R. E. Wescott; E. White; J. Wicht; L. Widhalm; K. M. Williams; E. Won; H. Xu; B. D. Yabsley; H. Yamamoto; H. Yamaoka; Y. Yamaoka; M. Yamauchi; Y. Yin; H. Yoon; J. Yu; C. Z. Yuan; Y. Yusa; D. Zander; M. Zdybal; Z. P. Zhang; J. Zhao; L. Zhao; Z. Zhao; V. Zhilich; P. Zhou; V. Zhulanov; T. Zivko; A. Zupanc; O. Zyukova

    2010-11-01

    The Belle detector at the KEKB electron-positron collider has collected almost 1 billion Y(4S) events in its decade of operation. Super-KEKB, an upgrade of KEKB is under construction, to increase the luminosity by two orders of magnitude during a three-year shutdown, with an ultimate goal of 8E35 /cm^2 /s luminosity. To exploit the increased luminosity, an upgrade of the Belle detector has been proposed. A new international collaboration Belle-II, is being formed. The Technical Design Report presents physics motivation, basic methods of the accelerator upgrade, as well as key improvements of the detector.

  8. Luz II | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on QA:QAsource History View NewTexas:Montezuma, Arizona:Oregon:Lowell Point, Alaska:Vermont:Lutz, Florida:II Jump to:

  9. SECTION II: HEAVY ION REACTIONS

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Homesum_a_epg0_fpd_mmcf_m.xls" ,"Available from WebQuantityBonneville Power AdministrationRobust, High-Throughput Analysis of Protein1-0845* Storage Systems INTERACTIONSTemperatureII:

  10. Harvest II | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on QA:QA J-E-1 SECTION J APPENDIXsource History View NewGuam: Energy Resources JumpConsultingHarfordHarvard,BioFuelsII

  11. Limon II | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on QA:QA J-E-1 SECTION J APPENDIXsource History ViewInformationWinds JumpOxiranchem IncLighthouseLigninLimon I JumpII

  12. Majestic II | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on QA:QA J-E-1 SECTION J APPENDIXsource HistoryScenarios Towards 2050EnermarGenerationMainsa Instalaciones JumpMajestic II

  13. Musselshell II | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on QA:QA J-E-1 SECTION J APPENDIXsourceII Jump to: navigation, searchsourceEnergyTexas: Energy Resources JumpMuskegonIII

  14. Penascal II | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on QA:QA J-E-1 SECTION J APPENDIXsourceII JumpQuarterly Smart GridNorth Carolina:ParamountEnergy GroupPeetz

  15. Cooperative Effects in the Binding of Substrates to Nickel(II) and Nickel(III) Complexes with a Bis(macrocyclic) Ligand

    E-Print Network [OSTI]

    Nazarenko, Alexander

    II/I Introduction Mannich-type, metal-ion-assisted condensation reactions of cis-disposed primary amines. However, in the copper(II)-assisted condensation the [a] Universität Heidelberg, Anorganisch at Buffalo, 1300 Elmwood Ave, Buffalo, NY 14222-1095, USA [d] Institute of Physical Chemistry, Polish Academy

  16. The Antecedents and Consequences of Ethnically Diverse Early Adolescents' School Belonging and Academic Identity in Middle School

    E-Print Network [OSTI]

    Kogachi, Kara Heidi Akemi

    2013-01-01

    discrimination, and school performance among children ofin motivation and school performance are quite normative ateffects on the school performance of ethnic minority youth (

  17. BNL ATF II beamlines design

    SciTech Connect (OSTI)

    Fedurin, M.; Jing, Y.; Stratakis, D.; Swinson, C.

    2015-05-03

    The Brookhaven National Laboratory. Accelerator Test Facility (BNL ATF) is currently undergoing a major upgrade (ATF-II). Together with a new location and much improved facilities, the ATF will see an upgrade in its major capabilities: electron beam energy and quality and CO2 laser power. The electron beam energy will be increased in stages, first to 100-150 MeV followed by a further increase to 500 MeV. Combined with the planned increase in CO2 laser power (from 1-100 TW), the ATF-II will be a powerful tool for Advanced Accelerator research. A high-brightness electron beam, produced by a photocathode gun, will be accelerated and optionally delivered to multiple beamlines. Besides the energy range (up to a possible 500 MeV in the final stage) the electron beam can be tailored to each experiment with options such as: small transverse beam size (<10 um), short bunch length (<100 fsec) and, combined short and small bunch options. This report gives a detailed overview of the ATFII capabilities and beamlines configuration.

  18. Airborne concentrations of asbestos in 71 school buildings

    SciTech Connect (OSTI)

    Corn, M.; Crump, K.; Farrar, D.B.; Lee, R.J.; McFee, D.R. (Johns Hopkins Univ., Baltimore, MD (USA))

    1991-02-01

    A total of 473 air samples from 71 schools scheduled for abatement (328 indoor static samples, 51 personal samples, and 94 outdoor samples) were analyzed by transmission electron microscopy techniques. Six measures of asbestos-in-air concentration were considered: (1) total asbestos structures per cubic centimeter: (2) chrysotile structures per cubic centimeter; (3) amphibole structures per cubic centimeter; (4) structures per cubic centimeter at least 0.5 micron long and at least five times wide; (5) structures per cubic centimeter at least 5 microns long; and (6) structures per cubic centimeter at least 5 microns long and at least 0.2 micron wide. The average concentration of chrysotile structures in indoor air samples was 0.017 structures/cm{sup 3}; the average concentration of amphibole structures was 0.0015 structure/cm{sup 3}. Ninety-five percent of structures found were chrysotile. The average concentrations of all structures were significantly higher indoors than outdoors (P less than 0.001). The average concentration of structures more than 5 microns long indoors was 0.00023 structure/cm{sup 3}. None of the following factors were significantly correlated with asbestos concentrations in air: type of asbestos-containing materials (ACM) present, condition of ACM, accessibility of ACM to students, whether ACM were covered, air flow, or whether sweeping was noted during sample collection. In addition, asbestos-in-air concentrations were not significantly different in different types of schools (high, intermediate or elementary) or in schools constructed in different time periods. Lastly, there was no correlation between the mineral type of asbestos found in the air and the type found in samples of bulk material.

  19. Radiological Release Accident Investigation Report (Phase II...

    Broader source: Energy.gov (indexed) [DOE]

    Investigation Report (Phase II Report) More Documents & Publications Central Characterization Program (CCP) Los Alamos National Laboratory (LANL) Interface Document Oak Ridge...

  20. Concrete Pour in NSLS-II Ring

    ScienceCinema (OSTI)

    Bruno Semon

    2013-07-22

    The mezzanine floor of the ring building tunnel for NSLS-II was completed when the last concrete was placed in February 2011.

  1. Giant Protease TPP II's Structure, Mechanism Uncovered

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    longer, and could lead to feeling satisfied after smaller portions, lowering overall food intake, which could help treat obesity. Knowing the mechanism of action for TPP II...

  2. Advanced Energy Retrofit Guide: Practical Ways to Improve Energy Performance, K-12 Schools (Book)

    SciTech Connect (OSTI)

    Not Available

    2013-12-01

    The U.S. Department of Energy developed the Advanced Energy Retrofit Guides (AERGs) to provide specific methodologies, information, and guidance to help energy managers and other stakeholders plan and execute energy efficiency improvements. Detailed technical discussion is fairly limited. Instead, we emphasize actionable information, practical methodologies, diverse case studies, and unbiased evaluations of the most promising retrofit energy efficiency measures for each building type. A series of AERGs is under development, addressing key segments of the commercial building stock. K-12 schools were selected as one of the highest priority building sectors, because schools affect the lives of most Americans. They also represent approximately 8% of the energy use and 10% of the floor area in commercial buildings nationwide. U.S. K-12 school districts spend more than $8 billion each year on energy - more than they spend on computers and textbooks combined. Most occupy older buildings that often have poor operational performance - more than 30% of schools were built before 1960. The average age of a school is about 42 years - which is nearly the expected serviceable lifespan of the building. K-12 schools offer unique opportunities for deep, cost-effective energy efficiency improvements, and this guide provides convenient and practical guidance for exploiting these opportunities in the context of public, private, and parochial schools.

  3. Pluggable type-checking for custom type qualifiers in Java

    E-Print Network [OSTI]

    Papi, Matthew M.

    2007-09-17

    We have created a framework for adding custom type qualifiers to the Javalanguage in a backward-compatible way. The type system designer definesthe qualifiers and creates a compiler plug-in that enforces theirsemantics. ...

  4. Thomas Jefferson High School for Science & Technology Takes 2015...

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    high school and middle school students will compete in 70 high school and 50 middle school regional Science Bowl tournaments. Students, in teams of four or five, compete in the...

  5. High School Co-op Program Recruitment Calendar

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    High School Jory Medina TBD Los Alamos High School Tammy Seidel, Michelle Vargas-Jimenez Thurs, Feb 5 McCurdy High School Dolores Salazar Wed, Feb 18 Mesa Vista High School...

  6. COLLEGE OF HEALTH & HUMAN SERVICES SCHOOL OF NURSING SCHOOL OF HEALTH AND APPLIED HUMAN SCIENCES SCHOOL OF SOCIAL WORK

    E-Print Network [OSTI]

    Olszewski Jr., Edward A.

    COLLEGE OF HEALTH & HUMAN SERVICES SCHOOL OF NURSING SCHOOL OF HEALTH AND APPLIED HUMAN SCIENCES SCHOOL OF SOCIAL WORK CHHS SUCCESS Fall 2013 The College of Health and Human Services is dedicated't think any of us will forget the power of the Alumni Keynote presented by SHAHS alum Chad Porter

  7. COLLEGE OF HEALTH & HUMAN SERVICES SCHOOL OF NURSING SCHOOL OF HEALTH AND APPLIED HUMAN SCIENCES SCHOOL OF SOCIAL WORK

    E-Print Network [OSTI]

    Olszewski Jr., Edward A.

    COLLEGE OF HEALTH & HUMAN SERVICES SCHOOL OF NURSING SCHOOL OF HEALTH AND APPLIED HUMAN SCIENCES SCHOOL OF SOCIAL WORK CHHS SUCCESS Spring 2014 The College of Health and Human Services is dedicated to enhancing the health and quality of life of individuals, families and communities in Southeastern North

  8. COLLEGE OF HEALTH & HUMAN SERVICES SCHOOL OF NURSING SCHOOL OF HEALTH/APPLIED HUMAN SCIENCES SCHOOL OF SOCIAL WORK

    E-Print Network [OSTI]

    Olszewski Jr., Edward A.

    COLLEGE OF HEALTH & HUMAN SERVICES SCHOOL OF NURSING SCHOOL OF HEALTH/APPLIED HUMAN SCIENCES SCHOOL OF SOCIAL WORK Implementing Cultural Competency Training Throughout an Entire Health System March 26, 2013 3 competency training. He is a fellow of the Health Research and Education Trust Cultural Competency Leadership

  9. Policies and outcomes for UK sustainable schools

    E-Print Network [OSTI]

    Moncaster, A.M.; Simmons, P.

    2015-02-11

    , economic and environmental sustainability were increasing during the same period, leading to stated new aspirations from 2004 for the schools to be ‘models of sustainable development’. The key political discourses for ‘sustainable schools’ during this era...

  10. The Graduate School New Mexico State University

    E-Print Network [OSTI]

    Johnson, Eric E.

    The Graduate School New Mexico State University Educational Services Building, Suite 301 PO Box at 646-5745. #12;The Graduate School New Mexico State University Educational Services Building, Suite 301

  11. Early Childhood Education and School Readiness: Conceptual

    E-Print Network [OSTI]

    Rau, Don C.

    Early Childhood Education and School Readiness: Conceptual Models, Constructs, and Measures and Evaluation. #12;Early Childhood Education and School Readiness Workshop, June 17-18, 2002 TABLE OF CONTENTS .................................................................................................................................................13 Language and Early Literacy

  12. New Orleans Schools Implement Energy Efficiency

    Office of Energy Efficiency and Renewable Energy (EERE)

    After Hurricanes Katrina and Rita in 2007, the U.S. Department of Energy (DOE) and the National Renewable Energy Laboratory (NREL), provided technical assistance to New Orleans’ schools to improve energy efficiency and reduce school operating costs.

  13. Discipline Policies, Successful Schools, and Racial Justice

    E-Print Network [OSTI]

    Losen, Daniel

    2011-01-01

    used to evaluate school performance. These lower achieversfor monitoring school performance. In addition, it isschools was related to (a) reduction in office disciplinary referrals, (b) reduction in suspensions, and (c) improved fifth grade academic performance:

  14. School of Civil & Environmental Engineering August 2009

    E-Print Network [OSTI]

    Jacobs, Laurence J.

    GRADUATE HANDBOOK School of Civil & Environmental Engineering August 2009 #12;2 #12;3 GRADUATE HANDBOOK School of Civil & Environmental Engineering - Georgia Tech TABLE OF CONTENTS CHAPTER I 7 INTRODUCTION TO CIVIL & ENVIRONMENTAL ENGINEERING.............................................................7

  15. School of Healthcare Sciences Undergraduate Degree Programmes

    E-Print Network [OSTI]

    Martin, Ralph R.

    9 Midwifery 10 Adult Nursing 11 Children's Nursing 12 Mental Health Nursing 13 Occupational Therapy is a new School, made up of the former Schools of Nursing and Midwifery and Healthcare Studies. As such

  16. The Streit Council School of Public Policy

    E-Print Network [OSTI]

    The Streit Council and the School of Public Policy George Mason University Transatlantic Policy, George Mason University, 3351 Fairfax Drive, Arlington, Virginia 22201 (two blocks east, Streit Council Moderator: Desmond Dinan, School of Public Policy, George Mason University Speakers: Mark

  17. Lecturer, Management Lally School of Management

    E-Print Network [OSTI]

    Salama, Khaled

    Lecturer, Management Lally School of Management Rensselaer Polytechnic Institute The enterprise management and organization area of The Lally School of Management at Rensselaer Polytechnic Institute degree equivalent in management, strategy, organization behavior, or an appropriate related field

  18. UNIVERSITY OF CONNECTICUT SCHOOL OF MEDICINE

    E-Print Network [OSTI]

    UNIVERSITY OF CONNECTICUT SCHOOL OF MEDICINE SCHOOL OF DENTAL MEDICINE Summer Fellowship Program Application The University of Connecticut Health Center Office of Student Affairs Farmington Connecticut 06030-1905 Deadline for application: March 15th #12;College Undergraduate

  19. Highcliffe School Woodfuel Innovative heating for a Leicestershire Primary School

    E-Print Network [OSTI]

    to adapt coal boilers enabling them to run on wood pellets. In addition to supporting the local economy school through the simple act of replacing an ageing, coal-fired boiler with a modern, wood-fuelled version. The new boiler utilises wood chips supplied by a local farmer. However, in time, some of the fuel

  20. PICTURE GROUPS OF FINITE TYPE AND COHOMOLOGY IN TYPE An

    E-Print Network [OSTI]

    Igusa, Kiyoshi

    PICTURE GROUPS OF FINITE TYPE AND COHOMOLOGY IN TYPE An KIYOSHI IGUSA, KENT ORR, GORDANA TODOROV a picture group. We construct a finite CW complex which is shown in another paper [10] to be a K(, 1) for this picture group. In [5] another independent proof was given for this fact in the special case of type

  1. Foster-Glocester Regional School District (Rhode Island) - Financing Profile

    SciTech Connect (OSTI)

    none,

    2008-12-01

    This document is an EnergySmart Schools Financing Profile of Foster-Glocester Regional School District in Rhode Island

  2. University of Connecticut Health Center School of Dental Medicine

    E-Print Network [OSTI]

    Oliver, Douglas L.

    University of Connecticut Health Center School of Dental Medicine Application for Admission of Connecticut School of Dental Medicine

  3. Lead(ii) Detection An Exceptionally Selective Lead(ii)-Regulatory

    E-Print Network [OSTI]

    He, Chuan

    Lead(ii) Detection An Exceptionally Selective Lead(ii)-Regulatory Protein from Ralstonia Metallidurans: Development of a Fluorescent Lead(ii) Probe** Peng Chen, Bill Greenberg, Safiyh Taghavi, Christine Romano, Daniel van der Lelie, and Chuan He* Lead contamination is a serious threat to human health

  4. 9-MONTH SAMPLE MULTI-YEAR OFFER LETTER TEACHING FACULTY II, RESEARCH FACULTY II,

    E-Print Network [OSTI]

    McQuade, D. Tyler

    9-MONTH SAMPLE MULTI-YEAR OFFER LETTER TEACHING FACULTY II, RESEARCH FACULTY II, INSTRUCTIONAL SPECIALIST II OR ASSOCIATE IN RESEARCH APPOINTMENT Dear Dr. xxx: I am pleased to offer you an ["in://facultyhandbook.fsu.edu/). This offer is also contingent upon your providing the necessary documents to prove your identity

  5. 12-MONTH SAMPLE MULTI-YEAR OFFER LETTER TEACHING FACULTY II, RESEARCH FACULTY II,

    E-Print Network [OSTI]

    McQuade, D. Tyler

    12-MONTH SAMPLE MULTI-YEAR OFFER LETTER TEACHING FACULTY II, RESEARCH FACULTY II, INSTRUCTIONAL SPECIALIST II OR ASSOCIATE IN RESEARCH APPOINTMENT Dear Dr. xxx: I am pleased to offer you an ["in://facultyhandbook.fsu.edu). This offer is also contingent upon your providing the necessary documents to prove your identity

  6. SWAMI II technology transfer plan

    SciTech Connect (OSTI)

    Ward, C.R.; Peterson, K.D.; Harpring, L.J.; Immel, D.M.; Jones, J.D.; Mallet, W.R.

    1995-12-31

    Thousands of drums of radioactive/hazardous/mixed waste are currently stored at DOE sites throughout US; they are stored in warehouse facilities on an interim basis, pending final disposition. Recent emphasis on anticipated decommissioning of facilities indicates that many more drums of waste will be generated, requiring additional storage. Federal and state regulations dictate that hazardous waste covered by RCRA be inspected periodically for container degradation and to verify inventories. All known DOE waste storage facilities are currently inspected manually. A system to perform robotic inspection of waste drums is under development by the SRTC Robotics Group of WSRC; it is called the Stored Waste Autonomous Mobile Inspector (SWAMI). The first version, SWAMI I, was developed by the Savannah River Technology Center (SRTC) as a proof of principle system for autonomous inspection of drums in a warehouse. SWAMI I was based on the Transitions Research Corporation (TRC) HelpMate mobile robot. TRC modified the Helpmate to navigate in aisles of drums. SRTC added subsystems to SWAMI I to determine its position in open areas, read bar code labels on the drums up to three levels high, capture images of the drums and perform a radiation survey of the floor in the aisles. The radiation survey was based on SRTC patented technology first implemented on the Semi-Intelligent Mobile Observing Navigator (SIMON). The radiation survey is not essential for the inspection of drums, but is an option that can increase the utility and effectiveness of SWAMI in warehouses with radioactive and/or mixed waste. All the sensors on SWAMI I were fixed on the vehicle. From the success of SWAMI I, a second version, SWAMI II, was developed; it will be evaluated at Fernald and tested with two other mobile robots. Intent is to transfer the technology developed for SWAMI I and II to industry so that it can supply additional units for purchase for drum inspection.

  7. School of Civil and Environmental Engineering School of Civil and Environmental Engineering

    E-Print Network [OSTI]

    Gaucher, Eric

    School of Civil and Environmental Engineering School of Civil and Environmental Engineering Atlanta", and "making a difficult subject interesting". 1 #12;School of Civil and Environmental Engineering School of Civil and Environmental Engineering Atlanta, GA 30332-0355 U.S.A. Phone 404-894-2201 Fax 404

  8. School of Civil and Environmental Engineering School of Civil and Environmental Engineering

    E-Print Network [OSTI]

    Gaucher, Eric

    School of Civil and Environmental Engineering School of Civil and Environmental Engineering Atlanta Engineering School of Civil and Environmental Engineering Atlanta, GA 30332-0355 U.S.A. Phone 404-894-2201 Fax stand-alone transit courses and modules in introductory #12;School of Civil and Environmental

  9. 1 School of Engineering and Applied Science SCHOOL OF ENGINEERING AND

    E-Print Network [OSTI]

    Vertes, Akos

    1 School of Engineering and Applied Science SCHOOL OF ENGINEERING AND APPLIED SCIENCE Dean D.S. Dolling Associate Deans B. Narahari, C.E. Korman, R. Riffat The School of Engineering and Applied Science to accept women for degree candidacy in engineering. While the organization and offerings of the school have

  10. UCD School of Veterinary Medicine Strategic Plan 2012-2017 School of Veterinary Medicine

    E-Print Network [OSTI]

    California at Davis, University of

    UCD School of Veterinary Medicine ­ Strategic Plan 2012-2017 - 0 - School of Veterinary Medicine University of California, Davis 2012-2017 Strategic Plan #12;UCD School of Veterinary Medicine ­ Strategic School of Veterinary Medicine ­ Strategic Plan 2012-2017 - 2 - The Strategic Planning Process · Planning

  11. Ecological Factors Affecting Hispanic Urban Middle School and High School Adolescents’ College and Career Aspirations 

    E-Print Network [OSTI]

    Hostrup, Judy Ann

    2011-08-08

    Program Enrollment ............... 49 9 Hispanic Middle School Adolescents? College Aspirations ............. 50 10 Hispanic Middle School Adolescents? Common Career Choices (Percentages... in previous years (Gottlieb, 2006). 11 Adolescents: Middle and high school grade-level students who are approximately 10 to 18 years old (American Psychological Association, 2002). Middle School Students: Usually grades seven and eight, but sometimes...

  12. Smog Check II Executive Summary

    E-Print Network [OSTI]

    Denver, University of

    to reduce air pollution emissions from vehicles by encouraging better ongoing maintenance of vehicles. Smog Check targets three types of pollution from vehicles: hydrocarbons (HC), nitrogen oxides (NOx, and ensuring the repair of vehicles with excessive emissions and broken or tampered emissions control systems

  13. Inheritance and association of oil content and seed coat type in sesame, Sesamum indicum L 

    E-Print Network [OSTI]

    Culp, T. W

    1953-01-01

    INHERITANCE AND ASSOCIATION OF OIL CONTENT AND SEED COAT TYPE IN SESAHE~ SESAMUH INDICUH L, A Thesis THOHAS W. CULP Approved as to style and content by: Chairman of Committee Head o e Department of Agronomy January, 1953 INHERITANCE... AND ASSOCIATION OF OIL CONTENT AND SEED COAT TYPE IN SESAME~ SESAIKM INDICUM L, THOMAS V GULP A Thesis Submitted to the Graduate School of the Agricultural and Mechanical College of Texas in partial fulfillment of the requirements for the degree of MASTERS...

  14. Top for economics Rank Business School

    E-Print Network [OSTI]

    Lin, Xiaodong

    Top for economics Rank Business School 1 University of Chicago: Booth Rutgers Business School of Strathclyde Business School University of Pretoria, Gibs IMD 2 3 4 5 6 7 8 9 10 1 2 3 4 5 6 7 8 9 10 Top/WHU Beisheim Tsinghua University/Insead Top for international business Rank Business School 1 2 3 4 5 6 7 8 9

  15. Procurement Card Program COLORADO SCHOOL OF MINES

    E-Print Network [OSTI]

    . The School uses a web-based program called Access Online for all reallocations of transactions made through

  16. http://get. School of Gr

    E-Print Network [OSTI]

    deYoung, Brad

    . udience: uthority of the rmation contac on the School ool of Graduat alterations. No latest versi l

  17. School of Information Technologies Undergraduate Scholarship (11275) The School of Information Technologies Undergraduate Scholarship is a one-year scholarship,

    E-Print Network [OSTI]

    Selvadurai, Selvakennedy

    School of Information Technologies Undergraduate Scholarship (11275) The School of Information of the scholarship shall be the School of Information Technologies Undergraduate Scholarship. b. The scholarship of schooling to enter ­ Bachelor of Computer Science and Technology (Advanced) Bachelor of Information

  18. PREPARING URBAN STUDENTS FOR COLLEGE-LEVEL WRITING: A NARRATIVE INQUIRY AND SPATIAL ANALYSIS OF TWO HIGH SCHOOL ENGLISH TEACHERS' PROFESSIONAL KNOWLEDGE

    E-Print Network [OSTI]

    Burdick, Melanie Nichole

    2011-07-28

    PREPARING URBAN STUDENTS FOR COLLEGE-LEVEL WRITING: A NARRATIVE INQUIRY AND SPATIAL ANALYSIS OF TWO HIGH SCHOOL ENGLISH TEACHERS? PROFESSIONAL KNOWLEDGE BY Copyright 2011 Melanie Nichole Burdick Submitted... Date defended: July 22, 2011 ii The Dissertation Committee for Melanie Nichole Burdick certifies That this is the approved version of the following dissertation...

  19. Entering Fall 2014 -BS in IM&T: Program Requirements To graduate with the Bachelor of Science in Information Management and Technology from the School of

    E-Print Network [OSTI]

    Crowston, Kevin

    in Information Management and Technology from the School of Information Studies, you must complete 120 credits. Information Management and Technology Primary Core (24-25 Credits): IST 101 Freshman Forum IST 195 IST 233 Management and Technology Electives (15 Credits): Concentration I 9 credits Concentration II 9 credits

  20. The Outer Disks of Early-Type Galaxies. I. Surface-Brightness Profiles of Barred Galaxies

    E-Print Network [OSTI]

    Peter Erwin; Michael Pohlen; John E. Beckman

    2007-09-21

    We present a study of 66 barred, early-type (S0-Sb) disk galaxies, focused on the disk surface brightness profile outside the bar region and the nature of Freeman Type I and II profiles, their origins, and their possible relation to disk truncations. This paper discusses the data and their reduction, outlines our classification system, and presents $R$-band profiles and classifications for all galaxies in the sample. The profiles are derived from a variety of different sources, including the Sloan Digital Sky Survey (Data Release 5). For about half of the galaxies, we have profiles derived from more than one telescope; this allows us to check the stability and repeatability of our profile extraction and classification. The vast majority of the profiles are reliable down to levels of mu_R ~ 27 mag arcsec^-2; in exceptional cases, we can trace profiles down to mu_R > 28. We can typically follow disk profiles out to at least 1.5 times the traditional optical radius R_25; for some galaxies, we find light extending to ~ 3 R_25. We classify the profiles into three main groups: Type I (single-exponential), Type II (down-bending), and Type III (up-bending). The frequencies of these types are approximately 27%, 42%, and 24%, respectively, plus another 6% which are combinations of Types II and III. We further classify Type II profiles by where the break falls in relation to the bar length, and in terms of the postulated mechanisms for breaks at large radii ("classical trunction" of star formation versus the influence of the Outer Lindblad Resonance of the bar). We also classify the Type III profiles by the probable morphology of the outer light (disk or spheroid). Illustrations are given for all cases. (Abridged)

  1. CHAPTER 3: CONTRACTS Policy 3-1 SCHOOL CONTRACTS

    E-Print Network [OSTI]

    ­ School as Buyer; · Settlement Agreements; · Energy Performance Contracts; · Solar Host AgreementsCHAPTER 3: CONTRACTS Policy 3-1 SCHOOL CONTRACTS 1. Categories 2. Policy 3. Content of School Contracts 4. Approved School Contract Forms 5. School Contract Approvals 6. School Contract Legal Review 7

  2. Department of Geophysics Colorado School of Mines

    E-Print Network [OSTI]

    Department of Geophysics Colorado School of Mines Golden, CO 80401 http://www.geophysics Colorado School of Mines CGEM Alisa Marie Green #12;Department of Geophysics Colorado School of Mines Golden, CO 80401 http://www.geophysics.mines.edu/cgem Defended: November 06, 2003 Advisor: Dr. Yaoguo Li

  3. Department of Geophysics Colorado School of Mines

    E-Print Network [OSTI]

    Department of Geophysics Colorado School of Mines Golden, CO 80401 http://www.geophysics Colorado School of Mines CGEM Dongjie Cheng #12;#12;Department of Geophysics Colorado School of Mines Golden, CO 80401 http://www.geophysics.mines.edu/cgem Defended: December 2003 Advisor: Dr. Yaoguo Li (GP

  4. STATE OF THE SCHOOL OF ENGINEERING

    E-Print Network [OSTI]

    Maurer,. Edwin P.

    ... MECH: smart water heater, autonomous robots, nanosat testing ... INTER: extreme environment exploration is not a spectator sport! SCHOOL OF ENGINEERING - 2014 Solar Decathlon ENGR 1 Final Civil Engineering Lab Collaborative Study #12;SCHOOL OF ENGINEERING Solar Decathlon ­ unrivaled experience SCHOOL OF ENGINEERING

  5. School of Architecture Montana State University

    E-Print Network [OSTI]

    Maxwell, Bruce D.

    School of Architecture Montana State University Strategic Planning Document Condensed Outline May 24, 2013 School of Architecture Vision Recognizing that architecture is a basic human need, we strive to play an essential and innovative role in enhancing the human condition. School of Architecture Mission

  6. Montana State University 1 School of Art

    E-Print Network [OSTI]

    Maxwell, Bruce D.

    Montana State University 1 School of Art 213 Haynes Hall Bozeman, MT 59717-3680 406-994-4501 Email: art@montana.edu The School of Art, fully accredited by the National Association of Schools of Arts and Design, was established in 1893 and its first graduate degree was conferred in 1932. We

  7. COLORADO SCHOOL OF MINES PERFORMANCE MANAGEMENT PROGRAM

    E-Print Network [OSTI]

    1 COLORADO SCHOOL OF MINES PERFORMANCE MANAGEMENT PROGRAM Revised October 1, 2008 I. HISTORY Since change, the Colorado School of Mine's (CSM) Performance Management Steering Committee was established the administration in the development and implementation of the School's Performance Pay Program. The original

  8. Annual Report 2008 School of Management

    E-Print Network [OSTI]

    Nagurney, Anna

    School, for the exceptional performance of its Massachusetts Export Center. The Importance of Alumnix Isenberg Annual Report 2008 School of Management University of Massachusetts Amherst Building The Isenberg Advantage Jack '57 and Suzy Welch with The Isenberg School's Jack Welch Scholars Building

  9. Isenberg School of Management Annual Report

    E-Print Network [OSTI]

    Nagurney, Anna

    and innovation. That is reflected in the School's exemplary performance in national surveys. In BusinessIsenberg School of Management Annual Report 2006-07 #12;Dear Alumni and Friends: As every page of this report indicates, the Isenberg School is a vibrant community with a culture that fosters learning

  10. Strategic Plan The School of Engineering

    E-Print Network [OSTI]

    10-Year Strategic Plan 2003-2013 The School of Engineering at the University of Kansas KU School of Engineering 1 Eaton Hall (785) 864-2930 (voice) (785) 864-5445 (fax) sbell@ku.edu #12;Executive Summary In 2002-2003,The KU School of Engineering identified, and has since refined, four specific objectives

  11. Faculty of Social Sciences School of Psychology

    E-Print Network [OSTI]

    St Andrews, University of

    Faculty of Social Sciences School of Psychology Undergraduate and Postgraduate Courses #12;Opposite: One of the School of Psychology's Eye Tracking Laboratories. Contents 02 Welcome to the School of Psychology 03 Why Study with Us? 04 Research Informed Teaching 05 A Graduate's Experience Our Undergraduate

  12. Undergraduate Courses in School of Psychology

    E-Print Network [OSTI]

    Banaji,. Murad

    Psychology Undergraduate Courses in School of Psychology Undergraduate Courses in #12;The School has an excellent reputation for Psychology, which is important as I intend to continue in this field that. Zoe, BSc Psychology Contents 3 Welcome to the School of Psychology 4 Why choose Psychology

  13. SCHOOL OF ENGINEERING FIELDWORK SAFETY HANDBOOK

    E-Print Network [OSTI]

    Neri, Peter

    UNIVERSITY OF ABERDEEN SCHOOL OF ENGINEERING FIELDWORK SAFETY HANDBOOK January 2014 #12;Contents A .................................................................................................................................. 26 Engineering Fieldwork Safety Handbook 2 January 2014 #12;A. Introduction The School's commitment and · individual projects carried out by students in the field. This handbook describes how the School gives

  14. Approved November 16, 2010 SCHOOL OF MANAGEMENT

    E-Print Network [OSTI]

    Pittendrigh, Barry

    Approved November 16, 2010 SCHOOL OF MANAGEMENT KRANNERT GRADUATE SCHOOL OF MANAGEMENT PURDUE;Approved November 16, 2010 Vision: The Krannert School of Management will focus on the management at Krannert in many different ways - Innovation in the classroom ­ through state of the art cases, theory

  15. Harvard Law School Recording License Agreement

    E-Print Network [OSTI]

    Schrag, Daniel

    Harvard Law School Recording License Agreement This is the paper version of the Harvard Law School Recording License Agreement. With it, individuals who give presentations or are recorded on campus (at: Harvard Law School Recording License Agreement The Author named above authorizes

  16. Faculty of Medicine Graduate School of Medicine

    E-Print Network [OSTI]

    Miyashita, Yasushi

    2009--2010 Faculty of Medicine Graduate School of Medicine PROSPECTUS The University of Tokyo #12;#12;A Message From the Dean of Faculty and Graduate School of Medicine, the University of Tokyo Takao Shimizu Dean, Faculty and Graduate School of Medicine The University of Tokyo Faculty of Medicine

  17. Faculty of Medicine Graduate School of Medicine

    E-Print Network [OSTI]

    Miyashita, Yasushi

    2015 2016 Faculty of Medicine Graduate School of Medicine PROSPECTUS The University of Tokyo #12;#12;A Message From the Dean of Faculty and Graduate School of Medicine, the University of Tokyo Kohei Miyazono Dean, Faculty and Graduate School of Medicine The University of Tokyo Faculty of Medicine

  18. Faculty of Medicine Graduate School of Medicine

    E-Print Network [OSTI]

    Miyashita, Yasushi

    2011--2012 Faculty of Medicine Graduate School of Medicine PROSPECTUS The University of Tokyo #12;#12;A Message From the Dean of Faculty and Graduate School of Medicine, the University of Tokyo Kohei Miyazono Dean, Faculty and Graduate School of Medicine The University of Tokyo Faculty of Medicine

  19. Faculty of Medicine Graduate School of Medicine

    E-Print Network [OSTI]

    Miyashita, Yasushi

    2005--2006 Faculty of Medicine Graduate School of Medicine PROSPECTUS The University of Tokyo #12;#12;Welcome to Faculty of Medicine, Graduate School of Medicine The University of Tokyo Nobutaka Hirokawa Dean, Faculty of Medicine, Graduate School of Medicine The University of Tokyo The University of Tokyo Graduate

  20. Faculty of Medicine Graduate School of Medicine

    E-Print Network [OSTI]

    Miyashita, Yasushi

    2007--2008 Faculty of Medicine Graduate School of Medicine PROSPECTUS The University of Tokyo #12;#12;Welcome to Faculty of Medicine, Graduate School of Medicine The University of Tokyo Takao Shimizu Dean, Faculty of Medicine, Graduate School of Medicine The University of Tokyo The Faculty of Medicine