Sample records for tigre tigrinya timne

  1. Le logiciel "Tigre" en formation PLC 1 Grtice J. Vincent Le logiciel Tigre en formation PLC

    E-Print Network [OSTI]

    Paris-Sud XI, Université de

    "Tigre" en formation PLC 1 Grétice J. Vincent Le logiciel « Tigre » en formation PLC J. Vincent Le;______________________________________________________________________________________ Le logiciel "Tigre" en formation PLC 2 Grétice J. Vincent 1.1. La lecture Voici l'écran d;______________________________________________________________________________________ Le logiciel "Tigre" en formation PLC 3 Grétice J. Vincent Figure 3 1.2. La démonstration Voici l

  2. Tigres

    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: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level: National5Sales for4,645U.S. DOE Office of ScienceandMesa del SolStrengthening a solidSynthesis ofwas publishedThree scientistsDepartment

  3. Selected TIGRE Program Listings This appendix contains abbreviated program listings for TIGRE as

    E-Print Network [OSTI]

    Koopman, Philip

    for TIGRE as implemented in C, VAX assembly language, and MIPS R2000 assembly langauge. B.1. REDUCE VAX /* adapt to VAX assembler kernel */ #define VAX_ASM TRUE #else #define VAX_ASM FALSE #endif #ifdef_TOKEN 255 #define PROGSIZE HEAPSIZE/2 /* max size of initial program */ #if VAX_ASM #define HEAP_STRIDE 3

  4. The Tambien Group, Northern Ethiopia (Tigre) NATHAN R. MILLER1*, DOV AVIGAD2, ROBERT J. STERN3 & MICHAEL BEYTH4

    E-Print Network [OSTI]

    Stern, Robert J.

    Chapter 21 The Tambien Group, Northern Ethiopia (Tigre) NATHAN R. MILLER1*, DOV AVIGAD2, ROBERT J (e-mail: nrmiller@mail.utexas.edu) Abstract: The Tambien Group of northern Ethiopia (Tigre Ethiopia within an intra-oceanic setting that was likely far removed from cratonic hinterlands. More work

  5. Time series of high resolution spectra of SN 2014J observed with the TIGRE telescope

    E-Print Network [OSTI]

    Jack, D; Schroder, K -P; Schmitt, J H M M; Hempelmann, A; Gonzalez-Perez, J N; Trinidad, M A; Rauw, G; Sixto, J M Cabrera

    2015-01-01T23:59:59.000Z

    We present a time series of high resolution spectra of the Type Ia supernova 2014J, which exploded in the nearby galaxy M82. The spectra were obtained with the HEROS echelle spectrograph installed at the 1.2 m TIGRE telescope. We present a series of 33 spectra with a resolution of R = 20, 000, which covers the important bright phases in the evolution of SN 2014J during the period from January 24 to April 1 of 2014. The spectral evolution of SN 2014J is derived empirically. The expansion velocities of the Si II P-Cygni features were measured and show the expected decreasing behaviour, beginning with a high velocity of 14,000 km/s on January 24. The Ca II infrared triplet feature shows a high velocity component with expansion velocities of > 20, 000 km/s during the early evolution apart from the normal component showing similar velocities as Si II. Further broad P-Cygni profiles are exhibited by the principal lines of Ca II, Mg II and Fe II. The TIGRE SN 2014J spectra also resolve several very sharp Na I D doub...

  6. Development of the TIGRE This describes the TIGRE method for combinator graph reduction.

    E-Print Network [OSTI]

    Koopman, Philip

    been previously implemented for the G-Ma- chine graph reduction implementation on a VAX (Peyton Jones 1987). In VAX assembly language, unwinding a node while traversing the stack requires four instructions, on average, processing nodes for stack unwinding costs: (4 * 1.38) + 7 = 12.52 VAX instructions per

  7. Associated Media Holdings Inc formerly EL Tigre Development Corp | Open

    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 onYou are now leaving Energy.gov You are now leaving Energy.gov You are being directedAnnual Siteof EnergyInnovation in Carbon Capture andsoftwareAsianEnergy InformationEnergy

  8. Framing Illegality: Sonic Culture, Power, and the Politics of Representation

    E-Print Network [OSTI]

    Arellano, Gerardo Nunez

    2010-01-01T23:59:59.000Z

    member of Los Tigres Del Norte) With their socially andlyrics, Los Tigres Del Norte have been entrancing audiencesargues that Los Tigres Del Norte and their music can be

  9. Compton Recoil Electron Tracking With the TIGRE Gamma-Ray Balloon Experiment

    E-Print Network [OSTI]

    Kamiya, Kaoru

    2011-01-01T23:59:59.000Z

    AGNs), pulsars, gamma-ray bursts, cosmic ray interactionssensitive to cosmic gamma-ray bursts in the energy range ofGalactic center, a single gamma-ray burst which occurred 10

  10. UN REGALO PARA HISTORIA. A CMERA DE UM "TIGRE DO SAARA" RETRATA TEMPOS DE ESCURIDO NA REPBLICA ORIENTAL DEL URUGUAY.

    E-Print Network [OSTI]

    Paris-Sud XI, Université de

    ORIENTAL DEL URUGUAY. Marco Antônio VARGAS VILLALOBOS Pontifícia Universidade Católica do Rio Grande do Sul González. El fotógrafo nacido en Marruecos en la época del protectorado español, llegó a Uruguay como

  11. PPaAJ~f~-"'

    Office of Legacy Management (LM)

    ,ioeelble eve;ltualty of valuable m&ala other timn pnnium bsLc recoaorinl flwi these pII& reeiduom durLy or incIdental td the rooovcly of UlWllW? . Af%r consldemtion of the...

  12. Complex deoxidation equilibria of molten steels by titanium and manganese

    SciTech Connect (OSTI)

    Morita, K.; Morioka, Y.; Tsukihashi, F.; Sano, N. [Univ. of Tokyo (Japan). Dept. of Metallurgy

    1996-12-31T23:59:59.000Z

    The relationship between the equilibrium composition of Fe-Ti-Mn melts and that of coexisting oxides has been investigated by employing a cold crucible melting at 1,873 K. Using metal compositions and the Gibbs energies of formation of component oxides, iso-activity contours of FeO and MnO for the FeO-TiO{sub 1.5}-MnO melts at 1,873 K were evaluated. The optimal conditions for practical deoxidation processes with Ti-Mn alloys are discussed.

  13. Construction of a minimal tiling path across the euchromatic arms of sorghum chromosome 3 and comparative analysis with the rice chromosome 1 pseudomolecule

    E-Print Network [OSTI]

    Zhou, Bin

    2009-05-15T23:59:59.000Z

    pools orthologous to a 5.1 Mb region of rice chromosome 1 were constructed and sequence skimmed. Alignment of the sorghum skim sequences to the TIGR rice gene models revealed ~62% colinearity between the two orthologous regions. In addition, colinearity...

  14. An assessment of the validity of cerium oxide as a surrogate for plutonium oxide gallium removal studies

    SciTech Connect (OSTI)

    Kolman, D.G.; Park, Y.; Stan, M.; Hanrahan, R.J. Jr.; Butt, D.P.

    1999-03-01T23:59:59.000Z

    Methods for purifying plutonium metal have long been established. These methods use acid solutions to dissolve and concentrate the metal. However, these methods can produce significant mixed waste, that is, waste containing both radioactive and chemical hazards. The volume of waste produced from the aqueous purification of thousands of weapons would be expensive to treat and dispose. Therefore, a dry method of purification is highly desirable. Recently, a dry gallium removal research program commenced. Based on initial calculations, it appeared that a particular form of gallium (gallium suboxide, Ga{sub 2}O) could be evaporated from plutonium oxide in the presence of a reducing agent, such as small amounts of hydrogen dry gas within an inert environment. Initial tests using ceria-based material (as a surrogate for PuO{sub 2}) showed that thermally-induced gallium removal (TIGR) from small samples (on the order of one gram) was indeed viable. Because of the expense and difficulty of optimizing TIGR from plutonium dioxide, TIGR optimization tests using ceria have continued. This document details the relationship between the ceria surrogate tests and those conducted using plutonia.

  15. TIGRFAMS: The TIGRFAMs database of protein families

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

    TIGRFAMs are protein families based on Hidden Markov Models or HMMs. Use this page to see the curated seed alignmet for each TIGRFam, the full alignment of all family members and the cutoff scores for inclusion in each of the TIGRFAMs. Also use this page to search through the TIGRFAMs and HMMs for text in the TIGRFAMs Text Search or search for specific sequences in the TIGRFAMs Sequence Search.[Copied from the Overview at http://www.jcvi.org/cms/research/projects/tigrfams/overview/] See also TIGRFAMs ordered by the roles they play at http://cmr.jcvi.org/tigr-scripts/CMR/shared/EvidenceList.cgi?ev_type=TIGRFAM&order_type=role.

  16. Manganese containing layer for magnetic recording media

    DOE Patents [OSTI]

    Lambeth, David N. (Pittsburgh, PA); Lee, Li-Lien (Santa Clara, CA); Laughlin, David E. (Pittsburgh, PA)

    1999-01-01T23:59:59.000Z

    The present invention provides for a magnetic recording media incorporating Mn-containing layers between a substrate and a magnetic layer to provide media having increased coercivity and lower noise. The Mn-containing layer can be incorporated in a rotating, translating or stationary recording media to operate in conjunction with magnetic transducing heads for recording and reading of magnetic data, as well as other applications. The magnetic recording medium of the invention preferably includes a Co or Co alloy film magnetic layer, and Mn-containing layer, preferably comprised of VMn, TiMn, MnZn, CrMnMo, CrMnW, CrMnV, and CrMnTi, and most preferably a CrMn alloy, disposed between the substrate and the magnetic layer to promote an epitaxial crystalline structure in the magnetic layer. The medium can further include seed layers, preferably polycrystalline MgO for longitudinal media, underlayers, and intermediate layers. Underlayers and intermediate layers are comprised of materials having either an A2 structure or a B2-ordered crystalline structure disposed between the seed layer and the magnetic layer. Materials having an A2 structure are preferably Cr or Cr alloys, such as CrV, CrMo, CrW and CrTi. Materials having a B2-ordered structure having a lattice constant that is substantially comparable to that of Cr, such as those preferably selected from the group consisting of NiAl, AILCo, FeAl, FeTi, CoFe, CoTi, CoHf, CoZr, NiTi, CuBe, CuZn, A-LMn, AlRe, AgMg, and Al.sub.2 FeMn.sub.2, and is most preferably FeAl or NiAl.

  17. Tensile Hoop Behavior of Irradiated Zircaloy-4 Nuclear Fuel Cladding

    SciTech Connect (OSTI)

    Jaramillo, Roger A [ORNL; Hendrich, WILLIAM R [ORNL; Packan, Nicolas H [ORNL

    2007-03-01T23:59:59.000Z

    A method for evaluating the room temperature ductility behavior of irradiated Zircaloy-4 nuclear fuel cladding has been developed and applied to evaluate tensile hoop strength of material irradiated to different levels. The test utilizes a polyurethane plug fitted within a tubular cladding specimen. A cylindrical punch is used to compress the plug axially, which generates a radial displacement that acts upon the inner diameter of the specimen. Position sensors track the radial displacement of the specimen outer diameter as the compression proceeds. These measurements coupled with ram force data provide a load-displacement characterization of the cladding response to internal pressurization. The development of this simple, cost-effective, highly reproducible test for evaluating tensile hoop strain as a function of internal pressure for irradiated specimens represents a significant advance in the mechanical characterization of irradiated cladding. In this project, nuclear fuel rod assemblies using Zircaloy-4 cladding and two types of mixed uranium-plutonium oxide (MOX) fuel pellets were irradiated to varying levels of burnup. Fuel pellets were manufactured with and without thermally induced gallium removal (TIGR) processing. Fuel pellets manufactured by both methods were contained in fuel rod assemblies and irradiated to burnup levels of 9, 21, 30, 40, and 50 GWd/MT. These levels of fuel burnup correspond to fast (E > 1 MeV) fluences of 0.27, 0.68, 0.98, 1.4 and 1.7 1021 neutrons/cm2, respectively. Following irradiation, fuel rod assemblies were disassembled; fuel pellets were removed from the cladding; and the inner diameter of cladding was cleaned to remove residue materials. Tensile hoop strength of this cladding material was tested using the newly developed method. Unirradiated Zircaloy-4 cladding was also tested. With the goal of determining the effect of the two fuel types and different neutron fluences on clad ductility, tensile hoop strength tests were performed on cladding for these varying conditions. Experimental data revealed negligible performance differences for cladding containing TIGR vs non-TIGR processed fuel pellets. Irradiation hardening was observed in tensile hoop data as the strength of the cladding increased with increasing neutron dose and appeared to saturate for a fast fluence of 1.7 1021 neutrons/cm2.

  18. Identification of the feature that causes the I-band secondary maximum of a type Ia supernova

    E-Print Network [OSTI]

    Jack, D; Hauschildt, P H

    2015-01-01T23:59:59.000Z

    We obtained a time series of spectra covering the secondary maximum in the I-band of the bright Type Ia supernova 2014J in M82 with the TIGRE telescope. Comparing the observations with theoretical models calculated with the time dependent extension of the PHOENIX code, we identify the feature that causes the secondary maximum in the I-band light curve. Fe II 3d6(3D)4s-3d6(5D)4p and similar high excitation transitions produce a blended feature at 7500 {\\AA}, which causes the rise of the light curve towards the secondary maximum. The series of observed spectra of SN 2014J and archival data of SN 2011fe confirm this conclusion. We further studied the plateau phase of the Rband light curve of SN 2014J and searched for features which contribute to the flux. The theoretical models do not clearly indicate a new feature that may cause the Rband plateau phase. However, Co II features in the range of 6500 - 7000 {\\AA} and the Fe II feature of the I-band are clearly seen in the theoretical spectra, but do not appear to ...