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

E-Print Network [OSTI]

"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

Paris-Sud XI, Université de


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

E-Print Network [OSTI]

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

Koopman, Philip


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

E-Print Network [OSTI]

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

Stern, Robert J.


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

E-Print Network [OSTI]

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

Koopman, Philip


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 on Google Bookmark EERE: Alternative Fuels Data Center Home Page on Office of Inspector GeneralDepartmentAUDIT REPORTOpenWendeGuo Feng Bio EnergyInstituteFunding Jump


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

E-Print Network [OSTI]

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

Kamiya, Kaoru




E-Print Network [OSTI]

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

Paris-Sud XI, Université de


Nommer les aNimaux exotiques de BayBars, d'orieNt eN occideNt 1 thierry Buquet  

E-Print Network [OSTI]

mongol, bars en russe. En arabe et en persan, le tigre est désigné par babr (pl. Bubr), mais de nos jours

Paris-Sud XI, Université de


La mnagerie du nom. Figures animales de Baybars 2 fvrier 2011  

E-Print Network [OSTI]

également nommé bar en mongol, bars en russe. En arabe et en persan, le tigre est désigné par babr (pl. bub

Paris-Sud XI, Université de


The Power of the Voice: Listening to Mexican and Central American Immigrant Experiences (1997-2010)  

E-Print Network [OSTI]

variety of artists, including the Mexican norteo ensemble Los Tigres del Norte, the Salvadoran group Tex Bronco, and the Nicaraguan singer-songwriter Flor Urbina. Finally, my conclusion sets the stage for future work on representations of immigrant...

Thornton, Megan L.



Complex deoxidation equilibria of molten steels by titanium and manganese  

SciTech Connect (OSTI)

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.

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



BioMed Central Page 1 of 13  

E-Print Network [OSTI]

@tigr.org * Corresponding author Abstract Background: The Generalized Hidden Markov Model (GHMM) has proven a useful be accelerated by a factor of two by optimizing their content sensors. We finish with a brief illustration-of-the-art in gene prediction techniques. Background Generalized Hidden Markov Models have seen wide use in recent

Majoros, Bill


www.sciencemag.org/cgi/content/full/1138878/DC1 Supporting Online Material for  

E-Print Network [OSTI]

, Evgeny M. Zdobnov, Neil F. Lobo, Kathryn S. Campbell, Susan E. Brown, Maria F. Bonaldo, Jingsong Zhu, Kurt LaButti, Eduardo Lee, Song Li, Diane D. Lovin, Chunhong Mao, Evan Mauceli, Carlos F. M. Menck be addressed. E-mail: nene@tigr.org (V.N.); severson.1@nd.edu (D.W.S.) Published 17 May 2007 on Science Express

Severson, David


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.


Effects of biofilms, sunlight, and salinity on corrosion potential and corrosion initiation of stainless alloys  

SciTech Connect (OSTI)

This phenomenon of corrosion potential ennoblement on stainless alloys is well known for full strength seawater. This report presents data on the extent to which that process occurs as a function of salinity and sunlight level for: stainless steels S30400 and S31600; stainless alloys S44735 (29-4C), S44660 (Seacure), NO8367 (6XN) and N10276 (C-276); and R50250 (Ti-Gr2). The results showed that natural population biofilms formed from all salinity waters under low light level conditions were capable of ennobling the corrosion potentials of all test alloys, although R50250 was consistently ennobled the least. Both the amount of ennoblement and the highest steady potential reached were maximized in fresh water and decreased for all alloys with increasing salinity. The critical pitting potentials for all test alloys were measured in coastal seawater. In addition, the critical pitting potentials for alloys S30400 and S31600 were measured (or estimated from the literature) as a function of salinity. The effect of ennoblement on the initiation and propagation of crevice corrosion are currently under investigation. The effect of sunlight on corrosion potential ennoblement was examined for the super alloy N10276 (C-276). Mechanisms by which ennoblement may be affected by sunlight were discussed, and it was hypothesized that the phenomenon may be at least partially understood in terms of pH fluctuations within the biofilm under the influence of periodic changes in the rates of photosynthesis and respiration.

Dexter, S.C.; Zhang, H.-J. (Delaware Univ., Lewes, DE (USA). Coll. of Marine Studies)



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

E-Print Network [OSTI]

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 ...

Jack, D; Hauschildt, P H