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1

Max-Planck-Institut fr molekulare Genetik  

E-Print Network (OSTI)

R K F L #12;Max-Planck-Institut für molekulare Genetik EBSV06 The Model Variables #12;MaxMax-Planck-Institut für molekulare Genetik EBSV06 Martin Vingron Max-Planck-Institut für molekulare;Max-Planck-Institut für molekulare Genetik EBSV06 Amino Acid Replacement #12;Max-Planck-Institut für

Spang, Rainer

2

Max-Planck-Institut fr Plasmaphysik  

E-Print Network (OSTI)

.15 is produced externally W R5 350 MJ 10 MJ1 MJ0.2 MJ Courtesy of Tim Hender, Culham #12;Max-Planck-Institut fürMax-Planck-Institut für Plasmaphysik Max-Planck-Institut für Plasmaphysik Wendelsteinstra?e 1 with that of the stellarator." V.D. Shafranov, 1980 #12;Max-Planck-Institut für Plasmaphysik 2/36 The classical stellarator #12

3

Max-Planck-Institut fur Mathematik  

E-Print Network (OSTI)

Max-Planck-Institut f¨ur Mathematik in den Naturwissenschaften Leipzig A Note on Resistance of NPT 2013 #12;#12;A Note on Resistance of NPT to Mixture of Separable States Bobo Hua1 , Xiu-Hong Gao2 of the whole matrix. Hence the positivity of T1 is equivalent to the positivity of T2 . A quantum state

4

PhD positions at the Max Planck Institute for Biophysical Chemistry, Gottingen, Germany.  

E-Print Network (OSTI)

-FRIEDRICH-BONHOEFFER-INSTITUT Computational Biomolecular Dynamics Group MAX-PLANCK-INSTITUT F?R BIOPHYSIKALISCHE CHEMIE #12;

de Groot, Bert

5

Institut Vorname Nachname E-Mail Telefon Max-Planck-Institut fr empirische sthetik  

E-Print Network (OSTI)

.holfelder@mpibp-frankfurt.mpg.de +49 69 6303-3020 Max-Planck-Institut für Chemie (Otto-Hahn- Institut) Dr. Susanne Benner susanne.benner@mpic.de +49 6131 305-3000 Max-Planck-Institut für biophysikalische Chemie (Karl

6

Max-Planck-Institut fur Mathematik  

E-Print Network (OSTI)

]. The absence of physical oscillator excitations of the string also implies that all scattering amplitudes-Mills from the N=2 String by Chandrashekar Devchand and Olaf Lechtenfeld Preprint-Nr.: 39 1997 #12;#12;hep-th/9712043 ITP{UH{31/97 EXTENDED SELF-DUAL YANG-MILLS FROM THE N=2 STRING Chandrashekar Devchand Max

7

Living and working in Germany A guide for international scientists at Max Planck Institutes  

E-Print Network (OSTI)

Living and working in Germany A guide for international scientists at Max Planck Institutes #12 and the hospitality in your town. You will quickly find that Germany is a country of many facets ­ a country Planck Society is Germany's most successful scientific or- ganisation in basic research. Max Planck

8

Keynote speakers Susan E. Trumbore -Max-Planck-Institute for Biogeochemistry Jena, Germany  

E-Print Network (OSTI)

Keynote speakers Susan E. Trumbore - Max-Planck-Institute for Biogeochemistry Jena, Germany http for Landscape Biogeochemistry, Germany http://www.arthur-gessler.de/ PhillippeTortell, University of British

Daniel, Rosenfeld

9

07. September 2007 Julia Ducke 1 Max-Planck-Institut fr  

E-Print Network (OSTI)

07. September 2007 Julia Ducke 1 Max-Planck-Institut für Mikrostrukturphysik HalleWeb 2.0-Workshop Wiki Erfahrungen mit Web 2.0 Erfahrungsbericht aus der Bibliothek des MPI für Mikrostrukturphysik #12;07. September 2007 Julia Ducke 2 Max-Planck-Institut für Mikrostrukturphysik HalleWeb 2.0-Workshop #12

10

Max Planck Institute for Biological Cybernetics, Tbingen, Germany VSS 2002, #18.3 ID501 Spatial updating in virtual environments  

E-Print Network (OSTI)

Max Planck Institute for Biological Cybernetics, Tübingen, Germany VSS 2002, #18.3 ID501 Spatial: What are vestibular cues good for? MPI for Biological Cybernetics, Germany 2 "Voluntary" vs Cybernetics, Germany 3 Methods - Setup · Vestibular stimuli: 6 dof Motion Platform · Visual stimuli: LCD video

11

Max-Planck-Institute for Meteorology, Hamburg, Germany Swedish Meteorological and Hydrological Institute, Norrkoping, Sweden  

E-Print Network (OSTI)

Institute, Norrko?ping, Sweden 3 Finnish Meteorological Institute, Helsinki, Finland 4 Rossby Centre, Norrko?ping, Sweden 5 German Weather Service, Offenbach, Germany 6 Institute for Marine Research, University of Kiel, Sweden A comprehensive model inter-comparison study investigating the water budget during the BALTEX

Lindau, Ralf

12

MagLab - Pioneers in Electricity and Magnetism: Max Planck  

NLE Websites -- All DOE Office Websites (Extended Search)

Max Planck (1858-1947) Max Planck In a career that lasted seven decades, Max Planck achieved an enduring legacy with groundbreaking discoveries involving the relationship between...

13

Max-Planck-Gesellschaft Rede des Prsidenten zur Festversammlung 2011 62. Jahresversammlung der Max-Planck-Gesellschaft  

E-Print Network (OSTI)

Max-Planck-Gesellschaft Rede des Präsidenten zur Festversammlung 2011 1 62. Jahresversammlung der Max-Planck-Gesellschaft Rede des Präsidenten, Prof. Peter Gruss zur Festversammlung der Max #12;Max-Planck-Gesellschaft Rede des Präsidenten zur Festversammlung 2011 2 Wissenschaftler

Falge, Eva

14

Princeton, Max Planck Society launch new research center for...  

NLE Websites -- All DOE Office Websites (Extended Search)

Planck Society President Peter Gruss, and Consul General of the Federal Republic of Germany in New York Busso von Alvensleben meet to sign an agreement launching the new Max...

15

Original Message Subject: [Cisprimary] [jobs] Max Planck Society seeks faculty in Autonomous  

E-Print Network (OSTI)

Original Message Subject: [Cisprimary] [jobs] Max Planck Society seeks faculty in AutonomousVjx@mail.gmail.com> > > Max Planck Society seeks faculty in Autonomous Systems at all levels > > The Max Planck Society is establishing a major new research direction > in "Autonomous Systems" to investigate and understand

Plotkin, Joshua B.

16

The Max Planck Society At home in Germany -present throughout the world  

E-Print Network (OSTI)

1 The Max Planck Society At home in Germany - present throughout the world Internationalisation ­ the Max Planck Society's role in safeguarding Germany's future Cooperation across national borders is one the internationalisation of science, both on its own behalf and also on behalf of Germany as a research location. To do

17

Max-Planck-Institut fur Mathematik  

E-Print Network (OSTI)

.2 Compatibility & incompatibility . . . . . . . . . . . . . . . . . . 5 2.3 Self . Moreover, our arguments illustrate the role of self-accommodation to achieve the minimal scaling

18

Max-Planck-Institut fur Mathematik  

E-Print Network (OSTI)

. In organisms proteins fold into a compact state attaining a well defined biological function by exposing

19

Max-Planck-Institut fur Mathematik  

E-Print Network (OSTI)

-assembly in dif- ferent physico-chemical systems like micelle formation, proteins folding, macro- and microphase

20

Max-Planck-Institut fur Mathematik  

E-Print Network (OSTI)

compact manifolds. When M is noncompact, geometry and analysis on it becomes more complicated. Concretely these findings to Ricci solitons and self-shrinkers. Keywords and phrases: Omori-Yau maximum principle, V-Laplacian, V-harmonic map, Ricci soliton, self-shrinker. MSC 2000: 58E20, 53C27. 1. Introduction

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While these samples are representative of the content of NLEBeta,
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21

Max-Planck-Institut f ur Mathematik  

E-Print Network (OSTI)

as a result of energetic competition . . . . . 11 3 Bulk scalings 14 3.1 The small particle limit . . . . . . . . . . . . . . . . . . . . . . . . 87 8.1.2 Identification of four scaling regimes . . . . . . . . . . 91 8.1.3 Asymptotic identification of the unstable mode in Regime III . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 97 8

22

Max-Planck-Institut fur Mathematik  

E-Print Network (OSTI)

. transfer semiflow ), which is always Date: March 17, 2011. 2000 Mathematics Subject Classification. 34D23

23

Max-Planck-Institut fur Mathematik  

E-Print Network (OSTI)

and the Waewski principle only give us a non-empty positive invariant set. Date: March 17, 2011. 2000 Mathematics

24

Max-Planck-Institut f ur Mathematik  

E-Print Network (OSTI)

; Secondary 81R60. Keywords. Noncommutative Geometry, spectral action principle, standard model of particle physics, generally covariant quantum theory. 1. Introduction The question is not whether god did create covariance, the motion of test particles along geodesics and the assumption that the energy­momentum tensor

25

Max-Planck-Institut fur Mathematik  

E-Print Network (OSTI)

Abstract It is discussed how a probabilistic generalization of classical mechanics of a point-particle mechanics, intrinsically mo- tivates a multi-particle concept. This corresponds to the unattainability The behavior at a node 7 5 Conclusions 11 1 Introduction Perhaps, everybody knows about Einstein's \\god does

26

MaxPlanckInstitut fur Mathematik  

E-Print Network (OSTI)

, 1999 Abstract It is discussed how a probabilistic generalization of classical mechanics of a point­particle mechanics, intrinsically mo­ tivates a multi­particle concept. This corresponds to the unattainability The behavior at a node 7 5 Conclusions 11 1 Introduction Perhaps, everybody knows about Einstein's ``god does

27

MAX-PLANCK-INSTITUT FR QUANTENOPTIK  

E-Print Network (OSTI)

Laserspektroskopie. Hochpräzise Spektroskopie von Wasserstoff stellt einen Test der Theorie der Quantenelektrodynamik Wasserstoff erzielt. Ein neuer Forschungs- schwerpunkt ist die Frequenzkammspektroskopie von Wasserstoff- und

Hänsch, Theodor W.

28

Max-Planck-Institut fur Mathematik  

E-Print Network (OSTI)

and Rose, 1984; Hodgkin and Huxley, 1952; Nagumo et al., 1962), neural mass models (Freeman, 1978; Jansen and Rit, 1995; Jansen et al., 1993; Lopes da Silva et al., 1974; Lopes da Silva et al., 1976; Nunez, 1974

29

Max-Planck-Institut fur Mathematik  

E-Print Network (OSTI)

Finster and J¨urgen Tolksdorf Preprint no.: 12 2012 #12;#12;arXiv:1201.5497v2[math-ph]1May2012 BOSONIC, the solution of the Cauchy problem is expressed in terms of tree diagrams which involve the retarded Green's function and have one outgoing leg. In order to obtain general tree diagrams, we set up a "classical

30

Max-Planck-Institut fur Mathematik  

E-Print Network (OSTI)

distribution. This is a spatial approach which does not describe the intrinsically temporal aspects that we have a system consisting of elementary units #23; 2 V . With each non-empty subsystem S #26; V we that there is a \\composition" map : Q #23;2V O f#23;g ,! O V that de#12;nes how to put ob- jects of the individual units

31

Max-Planck-Institut fur Mathematik  

E-Print Network (OSTI)

. The main results of this paper are formulated in Lemma 1 and Theorem 2. Lemma 1 is proved in Section 2. In Section 3 an example of applications of our result is given. There is a large literature [1, 2, 3||. (11) We assume that a(t) > 0, a(t) ten

32

Max-Planck-Institut fur Mathematik  

E-Print Network (OSTI)

, exponential family, information topology, information projection. AMS Subject Classification: 62F30, 54C10, 52 as for example the International Workshop on Bayesian Inference and Maximum Entropy Methods in Science the relative entropy D(P Q) := X log( dP dQ )dP from Q. Thereby dP dQ is the Radon-Nikodým derivative of P

33

Max-Planck-Institut f ur Mathematik  

E-Print Network (OSTI)

, 2004 Abstract In this paper we show that the Higgs boson of the (minimal) Standard Model has at most) Standard Model the three possible gauge inequivalent ground states of the Higgs boson are shown to fully by the hypercharge of the Higgs boson. In [Tolk'03(c)] it has been shown that the symmetry of electromagnetism under

34

Max-Planck-Institut fur Mathematik  

E-Print Network (OSTI)

, then the corresponding energy is trapping, and orbits, visiting these sup- ports in any prescribed succession, can if the boundary of Hill's region is non-empty and not homeomorphic to a sphere. For non-trapping energies we introduce a topological degree which can be non-trivial for low energies, and for Coulombic and other singu

35

Max-Planck-Institut f ur Mathematik  

E-Print Network (OSTI)

­degenerate representations of O(#) are found. They are labeled by the value of the total electric charge, leading . . . . . . . . . . . . . . . . 9 3.2 Generating the observable algebra from the tree data . . . . . 15 3.3 Functional analytic to realistic gauge theories is still a big challenge. Some partial results in this direction already exist, see

36

Max-Planck-Institut fr molekulare Genetik  

E-Print Network (OSTI)

Large-scale Network Data · Random Graph Model (Erdös-Renyi) · Small-world model (Strogatz Large-scale analysis of protein complexes 1. Cell-lysation 2. tandem affinity-purification 3. gel with complex formation · protein identification through MS Limitations · In vivo · Large-scale, unbiased · 56

Spang, Rainer

37

Max-Planck-Institut fur Mathematik  

E-Print Network (OSTI)

. 2010 Mathematics Subject Classification. 20F65 (54E35,20F18,22E25,05C63). Key words and phrases. metric

38

Paul Blom: Research Director, Max Planck Institute for Polymer...  

NLE Websites -- All DOE Office Websites (Extended Search)

host: Thuc Quyen-Nguyen >>>Video and Slides available after the presentation* Abstract In solar cells, free charge carriers can recombine both via bimolecular (Langevin) and...

39

Curriculum Vitae Arne Max Erich Winguth, Ph.D.  

E-Print Network (OSTI)

in an earth system model", two months summer salary, 2005. [9] Visiting Scientist, Max Planck Institute for Meteorology, Germany, "Development of marine carbon cycle in an earth system model", two months summer salary of marine carbon cycle in an earth system model", two months summer salary, 2003. [12] University

Winguth, Arne

40

Max-Planck-Institute for the Physics of Complex Systems, Dresden, Germany MPI-PKS Institute Retreat  

E-Print Network (OSTI)

Flach Localizing Energy Through Nonlinearity and Discreteness Dining Hall 12:15 - 13:00 © Lunch 13 arrive in Gro? D¨olln 12:30 - 13:15 Check-In Hotel D¨ollnsee-Schorfheide Dining Hall 13:15 - 14:15 Lunch 16:30 - 17:20 Ilya Eremin Routes to Unconventional Superconductivity Dining Hall 18:30 - 19:30 Dinner

Jülicher, Frank

Note: This page contains sample records for the topic "max planck institute" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
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41

MAX PLANCK SOCIETY Press Release  

E-Print Network (OSTI)

in Baltimore, Maryland presented an image in the constellation Fornax equal to the apparent size of the full energy distributions. To construct the image, the team stitched together 78 separate exposures from

42

International Max Planck Research School  

E-Print Network (OSTI)

and February. Please check the web-page http://www.mpi-hd.mpg.de/imprs-ptfs for details. It is expected or English system. Composition of the Universe. What lies behind the mysterious Dark Matter and Dark Energy and how does it lead to the baryon asymme- try of the Universe? What are the properties of Dark Matter

43

1 / 2 0 0 8 M A X P L A N C K F O R S C H U N G 93 MAX PLANCK AKTUELL  

E-Print Network (OSTI)

Abgabe von Wärme stets kontinuierlich erfol- gen. Dagegen hatte Planck herausgefunden, dass die Energie von Wärme und Licht anschaulich nachvollziehen. Wie entsteht Wissen? Dies erfährt der Besucher im

44

AFFILIATIONS: Neggers--Royal Netherlands Meteorological Institute (KNMI), De Bilt, Netherlands; siebesma--Royal  

E-Print Network (OSTI)

AFFILIATIONS: Neggers--Royal Netherlands Meteorological Institute (KNMI), De Bilt, Netherlands; siebesma--Royal Netherlands Meteorological Institute (KNMI), De Bilt, and Delft University of Technology, Delft, Netherlands; Heus--Max Planck Institut für Meteorologie, Hamburg, Germany CORRESPONDING AUTHOR: R

Siebesma, Pier

45

Max Wei  

NLE Websites -- All DOE Office Websites (Extended Search)

Max Wei Max Wei Max Wei Sustainable Energy Systems Group Lawrence Berkeley National Laboratory 1 Cyclotron Road MS 90R2002 Berkeley CA 94720 Office Location: 90-2024L (510) 486-5220 MWei@lbl.gov This publications database is an ongoing project, and not all Division publications are represented here yet. Publications 2013 Wei, Max, James H. Nelson, J. Greenblatt, Ana Mileva, Josiah Johnston, Michael K. Ting, Christopher Yang, Christopher M. Jones, James E. McMahon, and Daniel M. Kammen. "Deep carbon reductions in California require electrification and integration across economic sectors." Environmental Research Letters 8, no. 1 (2013). 2012 Greenblatt, J., Max Wei, and James E. McMahon. California's Energy Future: Buildings and Industrial Efficiency, California Council on Science and

46

Planck 2010  

ScienceCinema (OSTI)

Planck 2010 From the Planck Scale to the ElectroWeak Scale The conference will be the twelfth one in a series of meetings on physics beyond the Standard Model, organized jointly by several European groups: Bonn, CERN, Ecole Polytechnique, ICTP, Madrid, Oxford, Padua, Pisa, SISSA and Warsaw as part of activities in the framework of the European network UNILHC.Topics to be discussed: Supersymmetry Supergravity & string phenomenology Extra dimensions Electroweak symmetry breaking LHC and Tevatron Physics Collider physics Flavor & neutrinos physics Astroparticle & cosmology Gravity & holography Strongly coupled physics & CFT Registration: registration will be open until May 1st. Registration fees amount to 150 CHF and cover the cost of the coffee breaks and the social dinner. Payment has to be made online. The deadline for registration has been postponed to May 7th. However, after May 3th, we shall not accept any talk request any more. The meeting will be partly supported by the Marie Curie Initial Training Network "UNILHC" PITN-GA-2009-23792, the ERC Advanced Grant "MassTeV" 226371, and the CERN-TH unit.

None

2011-10-06T23:59:59.000Z

47

Strings and Planck Oscillators  

E-Print Network (OSTI)

We contrast two theories which both start in one dimension at the Planck scale, viz., Quantum SuperString or M-Theory and a theory of Planck oscillations

B. G. Sidharth

2005-12-23T23:59:59.000Z

48

Proceedings of Institute of Mathematics of NAS of Ukraine 2000, Vol. 30, Part 1, 204209. One-Dimensional FokkerPlanck Equation Invariant  

E-Print Network (OSTI)

Proceedings of Institute of Mathematics of NAS of Ukraine 2000, Vol. 30, Part 1, 204­209. One STOGNII Institute of Mathematics of NAS of Ukraine, 3 Tereshchenkivska Street, Kyiv, Ukraine E-mail: spichak@apmat.freenet.kiev.ua National Technical University of Ukraine "Kyiv Polytechnic Institute

Popovych, Roman

49

80 MaxPlanckForschung 4 | 11 xxxxxxxxxxxx  

E-Print Network (OSTI)

Transport von Feuchtig- keit und Wärme um die Erdkugel. Noch hatte Clau?en die Sahara nicht im Blick. Er

50

34 MaxPlanckForschung 3 | 09 kosmischer Heimatkunde  

E-Print Network (OSTI)

Geschichte. TEXT THOMAS B?HRKE Als Star am Himmel trat im Frühjahr 1997 der strahlend helle Hale-Bopp auf der Hofadel, am nächsten um die Sonne. Weit drau?en, dem Landadel ähnlich, führen die Gas- riesen Bahn der Sonne. Bei der ständig steigenden Tem- peratur verlieren diese Körper immer mehr Gas und Staub

51

Abstract Submitted for the DPP05 Meeting of  

E-Print Network (OSTI)

, Forschungszentrum Juelich, IPP (Germany), F. LEUTERER, Max Planck Institut fuer Plasmaphysik (Germany), E. WESTERHOF

52

Ocean Carbon Cycle Models from the Carbon Dioxide Information Analysis Center (CDIAC)  

DOE Data Explorer (OSTI)

\tPacific data-model intercomparison from Patrick Wetzel (Max Planck Institute for Meteorology, Germany)

53

Atmos. Chem. Phys., 10, 33093319, 2010 www.atmos-chem-phys.net/10/3309/2010/  

E-Print Network (OSTI)

Research Centre Geesthacht, Institute for Coastal Research, Max-Planck-Str. 1, 21502 Geesthacht, Germany 4

Paris-Sud XI, Université de

54

1194 VOLUME 10J O U R N A L O F C L I M A T E 1997 American Meteorological Society  

E-Print Network (OSTI)

, United Kingdom u Institute for Atmospheric Physics, GKSS­Research Center, Max-Planck-Strasse, Geesthacht

Xue, Yongkang

55

Soil Control on Runoff Response to Climate Change in Regional Climate Model Simulations  

E-Print Network (OSTI)

, Switzerland #GKSS Forschungszentrum, Geesthacht, Germany @Max Planck Institute for Meteorology, Hamburg

Haak, Hein

56

Boundary value problems for nonlinear first-order ODEs -constructing generalised solutions via the max-plus algebra  

E-Print Network (OSTI)

the max-plus algebra RICAM Georg Regensburger Johann Radon Institute for Computational and Applied Theory of Differential Equations Heriot-Watt University, Edinburgh, 9 August, 2006 SFB F1322 #12;Max), is a (generalized) solution of (1) Then Max-plus linear combination (Min-plus) #12;Max-plus Interpolation Given

Eilbeck, Chris

57

Planck-Length Phenomenology  

E-Print Network (OSTI)

This author's recent proposal of interferometric tests of Planck-scale-related properties of space-time is here revisited from a strictly phenomenological viewpoint. The results announced previously are rederived using elementary dimensional considerations. The dimensional analysis is then extended to the other two classes of experiments (observations of neutral kaons at particle accelerators and observations of the gamma rays we detect from distant astrophysical sources) which have been recently considered as opportunities to explore "foamy" properties of space-time. The emerging picture suggests that there is an objective and intuitive way to connect the sensitivities of these three experiments with the Planck length. While in previous studies the emphasis was always on some quantum-gravity scenario and the analysis was always primarily aimed at showing that the chosen scenario would leave a trace in a certain class of doable experiments, the analysis here reported takes as starting point the experiments and, by relating in a direct quantitative way the sensitivities to the Planck length, provides a model-independent description of the status of Planck-length phenomenology.

Giovanni Amelino-Camelia

2000-08-04T23:59:59.000Z

58

Institutional  

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institutional Sign In About | Careers | Contact | Investors | bpa.gov Search Policy & Reporting Expand Policy & Reporting EE Sectors Expand EE Sectors Technology & Innovation...

59

MAX Fluid Dynamics facility  

NLE Websites -- All DOE Office Websites (Extended Search)

MAX Fluid Dynamics facility MAX Fluid Dynamics facility Capabilities Engineering Experimentation Reactor Safety Testing and Analysis Overview Nuclear Reactor Severe Accident Experiments MAX NSTF SNAKE Aerosol Experiments System Components Laser Applications Robots Applications Other Facilities Other Capabilities Work with Argonne Contact us For Employees Site Map Help Join us on Facebook Follow us on Twitter NE on Flickr MAX Fluid Dynamics facility Providing high resolution data for development of computational tools that model fluid flow and heat transfer within complex systems such as the core of a nuclear reactor. 1 2 3 4 5 Hot and cold air jets are mixed within a glass tank while laser-based anemometers and a high-speed infrared camera characterize fluid flow and heat transfer behavior. Click on image to view larger size image.

60

CAMD Nanofabrication Links  

NLE Websites -- All DOE Office Websites (Extended Search)

Infrastructure :: News :: Related sites National Nanotechnology Initiative Nano Technology Industries Advanced Materials Research Institute Institute of Physics Max-Planck...

Note: This page contains sample records for the topic "max planck institute" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


61

Kurzfassungen der Meteorologentagung DACH, Vol. 1, DACH2007-A-00083, 2007  

E-Print Network (OSTI)

Forschungszentrum, Geesthacht, (2) Meteorologisches Institut der Universität Hamburg , (3) Max Planck Institut für

Zahn, Matthias

62

Modelling Max-CSP as Partial Max-SAT  

Science Journals Connector (OSTI)

We define a number of original encodings that map Max-CSP instances into partial Max-SAT instances. Our ... the well-known direct and support encodings from CSP into SAT. Then, we report on ... profile of our enc...

Josep Argelich; Alba Cabiscol; Ins Lynce

2008-01-01T23:59:59.000Z

63

Copyright 2004, 2005 WiMAX Forum "WiMAX ForumTM" and "WiMAX Forum CERTIFIEDTM" are  

E-Print Network (OSTI)

Copyright 2004, 2005 WiMAX Forum "WiMAX ForumTM" and "WiMAX Forum CERTIFIEDTM" are registered trademarks of the WiMAX ForumTM. * All trademarks are the properties of their respective owners. WiMAX Forum Internal Use Only WiMAX System Modeling Methodology Raj Jain Professor of Computer Science and Engineering

Jain, Raj

64

ComputerScience,TexasA&MUniversity JetMax: Scalable Max-Min  

E-Print Network (OSTI)

1 ComputerScience,TexasA&MUniversity JetMax: Scalable Max-Min Congestion Control for High- Speed Heterogeneous Networks JetMax: Scalable MaxJetMax: Scalable Max--MinMin Congestion Control for High congestion control and its designed properties · Analysis of existing max-min methods XCP, MKC, and MKC

Loguinov, Dmitri

65

QwMaxSat: A Weighted Partial MaxSAT Solver  

E-Print Network (OSTI)

#12; Koshimura, M., Zhang, T., Fujita, H., & Hasegawa, R. (2012). QMaxSAT: A Partial Max-SAT SolverQwMaxSat: A Weighted Partial MaxSAT Solver 2013725 C304 ERATO #12;Problem Solving with MaxSAT 2 Original Problem MaxSAT Problem MaxSAT Model Max

Banbara, Mutsunori

66

Summary Max Total Units  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

Max Total Units Max Total Units *If All Splits, No Rack Units **If Only FW, AC Splits 1000 52 28 28 2000 87 59 35 3000 61 33 15 4000 61 33 15 Totals 261 153 93 ***Costs $1,957,500.00 $1,147,500.00 $697,500.00 Notes: added several refrigerants removed bins from analysis removed R-22 from list 1000lb, no Glycol, CO2 or ammonia Seawater R-404A only * includes seawater units ** no seawater units included *** Costs = (total units) X (estimate of $7500 per unit) 1000lb, air cooled split systems, fresh water Refrig Voltage Cond Unit IF-CU Combos 2 4 5 28 References Refrig Voltage C-U type Compressor HP R-404A 208/1/60 Hermetic SA 2.5 R-507 230/1/60 Hermetic MA 2.5 208/3/60 SemiHerm SA 1.5 230/3/60 SemiHerm MA 1.5 SemiHerm HA 1.5 1000lb, remote rack systems, fresh water Refrig/system Voltage Combos 12 2 24 References Refrig/system Voltage IF only

67

Improved Approximations for Max Set Splitting and Max NAE SAT  

E-Print Network (OSTI)

Improved Approximations for Max Set Splitting and Max NAE SAT #3; Jiawei Zhang and Yinyu Ye y Nanjing, 210093, P.R.China August 16, 2000, Revised January 22, 2001. #3; This research was supported Fudan University, Shanghai, R.R.China. z This work was done while the author was visiting Computational

Ye, Yinyu

68

Atmos. Chem. Phys., 12, 74657474, 2012 www.atmos-chem-phys.net/12/7465/2012/  

E-Print Network (OSTI)

, Stellenbosch 7599, South Africa 2Helmholtz-Zentrum Geesthacht, Institute of Coastal Research, Max-Planck-Strasse, 21502 Geesthacht, Germany 3Max-Planck-Institut f¨ur Chemie, Hahn-Meitner-Weg 1, 55128 Mainz, Germany

Meskhidze, Nicholas

69

EMSL - climate  

NLE Websites -- All DOE Office Websites (Extended Search)

2014GB004826:

  • Max Planck Institute for Biogeochemistry, Jena, Germany
  • Earth System Modeling Program
  • Max Planck Institute for Intelligent...

70

Atmos. Chem. Phys., 10, 90599223, 2010 www.atmos-chem-phys.net/10/9059/2010/  

E-Print Network (OSTI)

. J. Wallington9 1Max-Planck-Institut f¨ur Chemie, Division of Atmospheric Chemistry, Postfach 3060

Meskhidze, Nicholas

71

MATERIALS AND MOLECULAR RESEARCH DIVISION, ANNUAL REPORT 1976  

E-Print Network (OSTI)

tpresent address: Institut flir Atom-und Festkorper- physik,Max Planck Insi tute flir Festkorperfurschung, Stuttgart,

Authors, Various

2010-01-01T23:59:59.000Z

72

PUBLISHED ONLINE: 22 JANUARY 2012 | DOI: 10.1038/NCLIMATE1372 Detecting regional anthropogenic trends in ocean  

E-Print Network (OSTI)

Palmas de Gran Canaria, Las Palmas de Gran Canaria 35.017, Spain, 8Max Planck Institute for Meteorology

Cobb, Kim

73

A better presentation of Plancks radiation law  

Science Journals Connector (OSTI)

Introductory physics and astronomy courses commonly use Wiens displacement law to explain the colors of blackbodies including the Sun and other stars in terms of their temperatures. We argue here that focusing on the peak of the blackbody spectrum is misleading for three reasons. First the Planck curve is too broad for an individual spectral color to stand out. Second the location of the peak of the Planck curve depends on the choice of the independent variable in the plot. And third Wiens displacement law is seldom used in actual practice to find a temperature and direct fitting to the Planck function is preferable. We discuss these flaws and argue that at the introductory level presentation of blackbody radiation in terms of photon statistics would be more effective pedagogically. The average energy of the emitted photons would then be presented in place of Wiens displacement law and discussion of the Stefan-Boltzmann law would include the total number of photons emitted per second. Finally we suggest that the Planck spectrum is most appropriately plotted as a spectral energy density per fractional bandwidth distribution using a logarithmic scale for the wavelength or frequency.

Jonathan M. Marr; Francis P. Wilkin

2012-01-01T23:59:59.000Z

74

What is Special About the Planck Mass?  

E-Print Network (OSTI)

Planck introduced his famous units of mass, length and time a hundred years ago. The many interesting facets of the Planck mass and length are explored. The Planck mass ubiquitously occurs in astrophysics, cosmology, quantum gravity, string theory, etc. Current aspects of its implications for unification of fundamental interactions, energy dependence of coupling constants, dark energy, etc. are discussed.

C. Sivaram

2007-06-30T23:59:59.000Z

75

Proceedings of the Work-in-Progress Session of the 20th IEEE Real-Time and Embedded Technology and Applications Symposium  

E-Print Network (OSTI)

for Software Systems #12;© Copyright 2014 Max Planck Institute for Software Systems. All rights reserved. The copyright of this collection is with the Max Planck Institute for Software Systems. The copyright, to discuss, and to network. Björn B. Brandenburg Max Planck Institute for Software Systems Kaiserslautern

Ungerer, Theo

76

Planck Surveyor On Its Way to Orbit  

ScienceCinema (OSTI)

An Ariane 5 rocket carried the Planck Surveyor and a companion satellite into space May 14, 2009 from the European Space Agency (ESA) base on the northwest coast of South America. Once in orbit beyond the moon, Planck will produce the most accurate measurements ever made of the relic radiation from the big bang, plus the largest set of CMB data ever recorded. Berkeley Labs long and continuing involvement with Planck began when George Smoot of the Physics Division proposed Plancks progenitor to ESA and continues with preparations for ongoing data analysis for the U.S. Planck team at NERSC, led by Julian Borrill, co-leader of the Computational Cosmology Center.

Borrill, Julian

2013-05-29T23:59:59.000Z

77

Telecommunications WiMAX Order  

E-Print Network (OSTI)

Telecommunications WiMAX Order 1. Fax completed form to 979.847.1111. 2. If you do not receive Approval Signature Date Service Date Desired Telecommunications Office Use Only Service Due Date Print #12;

78

Links  

NLE Websites -- All DOE Office Websites (Extended Search)

Related Sites National Nanotechnology Initiative Nano Technology Industries Advanced Materials Research Institute Institute of Physics Max-Planck Institute for Kohlenforschung The...

79

Crystal Structure of the Minimalist Max-E47 Protein Faraz Ahmadpour1  

E-Print Network (OSTI)

Crystal Structure of the Minimalist Max-E47 Protein Chimera Faraz Ahmadpour1 , Rodolfo Ghirlando2, Canada Abstract Max-E47 is a protein chimera generated from the fusion of the DNA-binding basic region of Max and the dimerization region of E47, both members of the basic region/helix-loop-helix (b

Guarne, Alba

80

Frederic Laquai Seminar: Photocurrent Generation in Low-Bandgap...  

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| 3:30 PM - 4:30 PM Frederic Laquai Head, Max Planck Research Group for Organic Optoelectronics Max Planck Institute for Polymer Research Photocurrent Generation in Low-Bandgap...

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81

Min-max and min-max regret versions of some combinatorial optimization problems : a survey  

E-Print Network (OSTI)

of such events. The purpose of this paper is to review the existing literature on the min-max and min-max rMin-max and min-max regret versions of some combinatorial optimization problems : a survey Hassene Aissi , Cristina Bazgan , and Daniel Vanderpooten Résumé Les critères min-max et min-max regret sont

Boyer, Edmond

82

Cloud Security by Max Garvey  

E-Print Network (OSTI)

Cloud Security Survey by Max Garvey #12;Cloudy Cloud is Cloudy What is the cloud? On Demand Service Network access Resource pooling Elasticity of Resources Measured Service #12;Cloud Types/Variants Iaa Cloud Public Cloud Hybrid Cloud combination. Private cloud with overflow going to public cloud. #12

Tolmach, Andrew

83

Heat Hyperbolic Diffusion in Planck Gas  

E-Print Network (OSTI)

In this paper we investigate the diffusion of the thermal pulse in Planck Gas. We show that the Fourier diffusion equation gives the speed of diffusion, v > c and breaks the causality of the thermal processes in Planck gas .For hyperbolic heat transport v

Miroslaw Kozlowski; Janina Marciak-Kozlowska

2006-07-06T23:59:59.000Z

84

Finitely presented groups 4 Max Neunhffer  

E-Print Network (OSTI)

under rotation and inversion and all r R are reduced. Max Neunhöffer (University of St Andrews.e.: pa, pb R for a, b ^X with a = b. Max Neunhöffer (University of St Andrews) Finitely presented is a piece, we have |p| r|. (|r| is the length in letters). Max Neunhöffer (University of St Andrews

Neunhöffer, Max

85

International Max Planck Research School on Adapting Behavior in a Fundamentally Uncertain World  

E-Print Network (OSTI)

IMPRS Uncertainty Phone: (49) 3641 686 677 Fax: (49) 3641 686 623 Email: imprs@econ.mpg.de Internet of Jena was filled to the very last seat. As it has become a good tradition, lectures Petersen, MPI for Re search on Collective Goods Invited lectures talks given by Sidney Winter, Wharton

86

2 | 10 MaxPlanckForschung 3 das Dilemma scheint unauflsbar: Bis zum Jahr 2030  

E-Print Network (OSTI)

aus, Wasserstoff sicherer und Platz sparender zu speichern; und sie legen die Grundlagen, um Batterien

87

Spezial | 10 MaxPlanckForschung 3 das Dilemma scheint unauflsbar: Bis zum Jahr 2030  

E-Print Network (OSTI)

aus, Wasserstoff sicherer und Platz sparender zu speichern; und sie legen die Grundlagen, um Batterien

88

DOE Awards 265 Million Hours of Supercomputing Time to Advance...  

Office of Environmental Management (EM)

Institute of Standards and Technology; the Max-Planck Institute for Quantum Optics in Germany; CERFACS, the European Center for Research and Advanced Training in Scientific...

89

E-Print Network 3.0 - analysen der neuesten Sample Search Results  

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DACH, Vol. 1, DACH2007-A-00083, 2007 Meteorologentagung DACH... Forschungszentrum, Geesthacht, (2) Meteorologisches Institut der Universitt Hamburg , (3) Max Planck Institut...

90

Extended metabolite profile of the human spinal cord Andreas Hock1  

E-Print Network (OSTI)

for Biomedical Engineering, University and ETH Zurich, Zurich, Switzerland, 2 Dept. of Clinical Research Institute of Neuroradiology, University Hospital of Zurich, Zurich, Switzerland, 4 Max Planck Institute

91

The Gauge Hierarchy Problem and Planck Oscillators  

E-Print Network (OSTI)

A longstanding question that has puzzled Physicists is the so called gauge hierarchy problem, that is why is there such a wide gap between the mass of a Planck particle, $10^{-5}gms$ and the mass of a typical elementary particle $\\sim 10^{-25}gms$. We show that the answer to this problem lies in a particular characterization of gravitation. This moreover also provides a picture of a Planck scale underpinning for the entire universe itself.

B. G. Sidharth

2005-08-12T23:59:59.000Z

92

Cautious revolutionaries: Maxwell, Planck, Hubble  

Science Journals Connector (OSTI)

Three scientists exemplified the cautious behavior that we might like all scientists to display: indeed they were so critical of their own ideas that they risked losing credit for them. Nevertheless they finally earned at least as much fame as they deserved leaving historians to wonder about what they really believed. Maxwell initially rejected the kinetic theory of gases because two of its predictions disagreed with experiments; later he revived the theory showed that one of those experiments had been misinterpreted and eventually became known as one of the founders of the modern theory. Planck seems to have intended his 1900 quantum hypothesis as a mathematical device not a physical discontinuity; later he limited it to the emission (not absorption) of radiation thereby discovering zero-point energy. Eventually he accepted the physical quantum hypothesis and became known as its discoverer. Hubble (with Humason) established the distancevelocity law which others used as a basis for the expanding universe theory; later he suggested that redshifts may not be due to motion and appeared to lean toward a static model in place of the expanding universe.

Stephen G. Brush

2002-01-01T23:59:59.000Z

93

ATF Users Meeting 2002 Max.ppt  

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and Fusion Research Division Center for Beam Physics Atto-Second Electron Beam Generation and Characterization Experiment at the ATF Max Zolotorev and Alexander Zholents Center for...

94

Atmos. Chem. Phys., 9, 19571969, 2009 www.atmos-chem-phys.net/9/1957/2009/  

E-Print Network (OSTI)

-Planck-Institut f¨ur Chemie (MPI), Air Chemistry Division, Joh.-J.-Becherweg 27, 55128 Mainz, Germany 2GKSS-Research Centre, Institute for Coastal Research (GKSS), Max-Planck-Str. 1, 21502 Geesthacht, Germany 3Leibniz

Meskhidze, Nicholas

95

Cyclic jobshop problem and (max, +)-algebra August 29, 2011  

E-Print Network (OSTI)

-plus algebra and discrete event systems The (max, +) algebra is the set R - endowed with the max operator 3 / 29 #12;Max-plus algebra and discrete event systems The (max, +) algebra is the set R - endowedCyclic jobshop problem and (max, +)-algebra L. Houssin LAAS-CNRS August 29, 2011 L. Houssin Cyclic

Ingrand, François

96

Planck 2015 results. XIII. Cosmological parameters  

E-Print Network (OSTI)

We present results based on full-mission Planck observations of temperature and polarization anisotropies of the CMB. These data are consistent with the six-parameter inflationary LCDM cosmology. From the Planck temperature and lensing data, for this cosmology we find a Hubble constant, H0= (67.8 +/- 0.9) km/s/Mpc, a matter density parameter Omega_m = 0.308 +/- 0.012 and a scalar spectral index with n_s = 0.968 +/- 0.006. (We quote 68% errors on measured parameters and 95% limits on other parameters.) Combined with Planck temperature and lensing data, Planck LFI polarization measurements lead to a reionization optical depth of tau = 0.066 +/- 0.016. Combining Planck with other astrophysical data we find N_ eff = 3.15 +/- 0.23 for the effective number of relativistic degrees of freedom and the sum of neutrino masses is constrained to Spatial curvature is found to be |Omega_K| < 0.005. For LCDM we find a limit on the tensor-to-scalar ratio of r <0.11 consistent with the B-mode constraints fr...

,

2015-01-01T23:59:59.000Z

97

mixer --maintaining web sites easily Max Neunhoffer  

E-Print Network (OSTI)

mixer -- maintaining web sites easily Max Neunh¨offer max.neunhoeffer@math.rwth-aachen.de 15. Juli 3 4 Notation 3 5 Installation of the mixer 3 6 First steps for a new web site 4 7 Finding the MIXERROOT 4 8 How does the mixer put together web pages? 4 9 Template documents 5 10 What replacements does

St Andrews, University of

98

max kwh | OpenEI Community  

Open Energy Info (EERE)

max kwh max kwh Home Ewilson's picture Submitted by Ewilson(53) Contributor 4 January, 2013 - 08:42 Rates with tier problems max kwh tiers I've detected that the following rates all have the improper number of "Max kWh" values (should be one less than the number of charges, since the highest tier is always "all remaining"). This is likely due to users not understanding the meaning of "Max kWh"--often I see things like: "300, 700, 1000" (derived from "first 300, next 700, greater than 1000") which should be entered as "300, 1000". This is why we need checks on input that prevent users from entering this incorrectly. Here is the list (my script only checked residential rates): Syndicate content 429 Throttled (bot load)

99

Towards a 3D time dependent Fokker-Planck solver for modelling RF heating in realistic tokamak geometry  

E-Print Network (OSTI)

. Hedin, Ion Cyclotron Heating in Toroidal Plasmas, Ph.D. thesis, Royal Institute of Technology StockholmTowards a 3D time dependent Fokker-Planck solver for modelling RF heating in realistic tokamak supercomputers and the need for predictive tools to guide the experiments, modelling radio frequency heating

100

Planck's Radiation Law in the Quantized Universe  

E-Print Network (OSTI)

Physical research looks for clues to quantum properties of the gravitational field. On the basis of the common Schr\\"odinger theory, a simple model of the quantization of a Friedmann universe comprising dust and radiation is investigated. With regard to energy quantization, the result suggests a universal limitation of the energy spacing between neighbouring quantum states by the Planck energy. Applied to black-body radiation, a modified Planck radiation law follows. If this could be verified in the laboratory, it would provide a direct hint at quantum properties of the space-time manifold.

Rainer Collier

2014-09-15T23:59:59.000Z

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101

Astrophysical Bounds on Planck Suppressed Lorentz Violation  

E-Print Network (OSTI)

This article reviews many of the observational constraints on Lorentz symmetry violation (LV). We first describe the GZK cutoff and other phenomena that are sensitive to LV. After a brief historical sketch of research on LV, we discuss the effective field theory description of LV and related questions of principle, technical results, and observational constraints. We focus on constraints from high energy astrophysics on mass dimension five operators that contribute to LV electron and photon dispersion relations at order E/M_Planck. We also briefly discuss constraints on renormalizable operators, and review the current and future contraints on LV at order (E/M_Planck)^2.

Ted Jacobson; Stefano Liberati; David Mattingly

2004-07-30T23:59:59.000Z

102

Copyright 2004, 2005, 2006, 2007 WiMAX Forum "WiMAX ForumTM" and "WiMAX Forum CERTIFIEDTM" are  

E-Print Network (OSTI)

://www.wimaxforum.org/apps/org/workgroup/aatg/ download.php/25704/WiMAX_System_Evaluation_M ethodology_071215R2.pdf #12;Copyright 2004, 2005, 2006, 2007Copyright 2004, 2005, 2006, 2007 WiMAX Forum "WiMAX ForumTM" and "WiMAX Forum CERTIFIEDTM" are registered trademarks of the WiMAX ForumTM. * All trademarks are the properties of their respective owners

Jain, Raj

103

Acceleration radiation and the Planck scale  

E-Print Network (OSTI)

A uniformly accelerating observer perceives the Minkowski vacuum state as a thermal bath of radiation. We point out that this field-theory effect can be derived, for any dimension higher than two, without actually invoking very high energy physics. This supports the view that this phenomenon is robust against Planck-scale physics and, therefore, should be compatible with any underlying microscopic theory.

I. Agullo; J. Navarro-Salas; G. J. Olmo; L. Parker

2008-02-27T23:59:59.000Z

104

Planck Scale Cosmology in Resummed Quantum Gravity  

E-Print Network (OSTI)

We show that, by using resummation techniques based on the extension of the methods of Yennie, Frautschi and Suura to Feynman's formulation of Einstein's theory, we get quantum field theoretic predictions for the UV fixed-point values of the dimensionless gravitational and cosmological constants. Connections to the phenomenological asymptotic safety analysis of Planck scale cosmology by Bonanno and Reuter are discussed.

B. F. L. Ward

2008-08-23T23:59:59.000Z

105

Planck Scale Cosmology and Resummed Quantum Gravity  

E-Print Network (OSTI)

We show that, by using amplitude-based resummation techniques for Feynman's formulation of Einstein's theory, we get quantum field theoretic 'first principles' predictions for the UV fixed-point values of the dimensionless gravitational and cosmological constants. Connections to the phenomenological asymptotic safety analysis of Planck scale cosmology by Bonanno and Reuter are discussed.

B. F. L. Ward

2009-10-13T23:59:59.000Z

106

The MAX IV storage ring project  

Science Journals Connector (OSTI)

The design of the MAX IV 3 GeV ultralow-emittance storage ring is presented and the implementation of solutions to the technological challenges imposed by the compact multi-bend achromat lattice are described.

Tavares, P.F.

2014-08-27T23:59:59.000Z

107

Boolean Max-Co-Clones ANDREI A. BULATOV1  

E-Print Network (OSTI)

on a systematic study of max-co-clones. Intuitively, applying max-quantification to a re- lation R(x1, . . . , xn, y1, . . . , yk) results in the relation max(y1, . . . , yk)R(x1, . . . , xn, y1, . . . , ykBoolean Max-Co-Clones ANDREI A. BULATOV1 Simon Fraser University In our ISMVL 2012 paper we

Bulatov, Andrei

108

Boolean Max-Co-Clones Andrei A. Bulatov  

E-Print Network (OSTI)

on a systematic study of max-co-clones. Intuitively, applying max-quantification to a relation R(x1, . . . , xn, y1, . . . , yk) results in the relation max(y1, . . . , yk)R(x1, . . . , xn, y1, . . . , ykBoolean Max-Co-Clones Andrei A. Bulatov Abstract. In our ISMVL 2012 paper we introduced the notion

Bulatov, Andrei

109

ON CYCLIC CLASSES AND ATTRACTION CONES IN MAX SERGEI SERGEEV  

E-Print Network (OSTI)

of linear algebra developed over the max- times semiring Rmax,? which is the set of nonnegative numbers R-plus semiring Rmax,+ = (R {-}, = max, = +), developed over the set of real numbers R with adjoined element to Rmax,+ and Rmax,?. Another well-known semiring is the max-min semiring Rmax,min = (R {-} {}, = max

Butkovic, Peter

110

E-Print Network 3.0 - arabidopsis thaliana seed Sample Search...  

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Max-Planck-Institut fr Entwicklungsbiologie Collection: Biology and Medicine 26 EMS Mutagenesis 101 From: Methods in Molecular Biology, vol. 323: Arabidopsis Protocols,...

111

E-Print Network 3.0 - arabidopsis thaliana seeds Sample Search...  

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Max-Planck-Institut fr Entwicklungsbiologie Collection: Biology and Medicine 26 EMS Mutagenesis 101 From: Methods in Molecular Biology, vol. 323: Arabidopsis Protocols,...

112

E-Print Network 3.0 - andrei surzhenkov priit Sample Search Results  

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Juan Antonio Navarro Perez and Andrei Voronkov. Proof systems for effec- tively Source: Navarro Prez, Juan Antonio - Max-Planck-Institut fr Softwaresysteme Collection:...

113

Atmos. Chem. Phys., 13, 7359, 2013 www.atmos-chem-phys.net/13/7359/2013/  

E-Print Network (OSTI)

. Jenkin5, A. Mellouki6, M. J. Rossi7, J. Troe8, and T. J. Wallington9 1Max-Planck-Institut f¨ur Chemie

Meskhidze, Nicholas

114

E-Print Network 3.0 - attosecond pulse trains Sample Search Results  

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Trains In HHG... polarized. Therefore, attosecond pulses generally are produced in a train, with two pulses ... Source: Kling, Matthias - Max-Planck-Institut fr Quantenoptik...

115

DOE's Office of Science Awards 95 Million Hours of Supercomputing...  

Office of Environmental Management (EM)

and Atmospheric Administration and the Max-Planck Institute for Quantum Optics in Germany. The Council on Competitiveness is the only non-governmental group of corporate CEOs,...

116

X-ray and neutron scattering studies of the complex compounds...  

NLE Websites -- All DOE Office Websites (Extended Search)

by Dr. Hoyoung Jang, Max Planck Institute for Solid State Research in Stuttgart, Germany In condensed matter physics, in particular a field of complex oxide materials, most...

117

E-Print Network 3.0 - arndt wiessner peter Sample Search Results  

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Renewable Energy ; Geosciences 2 Max Planck Institute for Molecular Genetics, Berlin, Germany Otto Warburg International Summer School and Workshop on Summary: Tobias Muller...

118

Posters  

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San Diego La Jolla, California H. Grassl Max Planck Institute for Meteorology Hamburg, Germany A. Heymsfield National Center for Atmospheric Research Boulder, Colorado J. Spinhirne...

119

Markus Mezger | Center for Gas SeparationsRelevant to Clean Energy...  

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Presently: Project leader, Max Planck Institute for Polymer Research, Mainz, Germany Email: mezger at mpip-mainz.mpg.de Diploma in Physics, Stuttgart University,...

120

Posters  

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California M. Latif and T. Stockdale Max-Planck Institute for Meteorology Hamburg, Germany Introduction The warmest waters found in the open ocean are situated in the...

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121

Solving Protein Structures from Scratch | U.S. DOE Office of...  

Office of Science (SC) Website

Contact Ilme Schlichting Max Planck Institute for Medical Research, Heidelberg, Germany ilme.schlichting@mpimf-heidelberg.mpg.de Funding Portions of this research were...

122

E-Print Network 3.0 - alcohol industries case Sample Search Results  

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1 200607HIGHLIGHT POLICY AND PRACTICE Summary: & Tropical Medicine) and colleagues in Russia and at the Max Planck Institute, Germany, conducted a case... -control study...

123

E-Print Network 3.0 - atomic quantum bits Sample Search Results  

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Dynamics group, Max-Planck-Institut fr Quantenoptik Collection: Physics 19 insight review articles 238 NATURE | VOL 416 | 14 MARCH 2002 | www.nature.com Summary:...

124

E-Print Network 3.0 - attosecond transient recorder Sample Search...  

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. The attosecond transient recorder uses linearly polarized few-cycle infrared laser fields. An attosecond ... Source: Kling, Matthias - Max-Planck-Institut fr Quantenoptik...

125

E-Print Network 3.0 - acvr1 mutation activates Sample Search...  

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Molecular Biology Group, Max-Planck-Institut fr molekulare Genetik Collection: Computer Technologies and Information Sciences ; Biotechnology ; Biology and Medicine 3...

126

Metagenomic and Metaproteomic Analyses of Symbioses between Bacteria and Gutless Marine Worms (2014 DOE JGI Genomics of Energy & Environment Meeting)  

SciTech Connect

Nicole Dubilier of the Max Planck Institute speaks at the 9th Annual Genomics of Energy & Environment Meeting on March 20, 2014 in Walnut Creek, Calif.

Dubilier, Nicole [Max Planck Institute

2014-03-19T23:59:59.000Z

127

E-Print Network 3.0 - az mikroskop robeshi Sample Search Results  

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Stefan W. - Department of NanoBiophotonics, Max-Planck-Institut fr biophysikalische Chemie Collection: Physics ; Materials Science ; Chemistry 3 uni ulm intern 309April 2011...

128

E-Print Network 3.0 - agalactiae strains clues Sample Search...  

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primarily ... Source: de Groot, Bert - Max-Planck-Institut fr biophysikalische Chemie Collection: Biology and Medicine ; Biotechnology 3 Mobile genetic elements provide...

129

E-Print Network 3.0 - antibody--an experimental study Sample...  

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... Source: Grubmller, Helmut - Max-Planck-Institut fr biophysikalische Chemie Collection: Chemistry ; Biology and Medicine 2 File TOC7.doc (Final version, last...

130

E-Print Network 3.0 - amino acid insertion Sample Search Results  

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structural domains. Amino acid insertion and deletion rates in genes associated with elementary biochemical... ... Source: Arndt, Peter - Max-Planck-Institut fr molekulare...

131

Stellarators | Princeton Plasma Physics Lab  

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in stellarators By John Greenwald Researchers at the U.S. Department of Energy's Princeton Plasma Physics Laboratory (PPPL) and the Max Planck Institute of Plasma Physics...

132

International collaborations | Princeton Plasma Physics Lab  

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in stellarators By John Greenwald Researchers at the U.S. Department of Energy's Princeton Plasma Physics Laboratory (PPPL) and the Max Planck Institute of Plasma Physics...

133

Press Releases Archive | Princeton Plasma Physics Lab  

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Plasma Physics Laboratory (PPPL) and the Max Planck Institute of Plasma Physics in Germany have devised a new method for minimizing turbulence in bumpy donut-shaped...

134

E-Print Network 3.0 - alpha-radionuklidov ra pb Sample Search...  

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Steven L. Goldstein Max-Planck Institut ... Source: Rudnick, Roberta L. - Department of Geology, University of Maryland at College Park Collection: Geosciences 16 Mobile...

135

E-Print Network 3.0 - atomos communication system Sample Search...  

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un conjunto numerable L cuyos elementos son llamados atomos; los conectivos Source: Navarro Prez, Juan Antonio - Max-Planck-Institut fr Softwaresysteme Collection: Computer...

136

Application of Planck's law to thermionic conversion  

SciTech Connect

A simple, highly accurate, mathematical model of heat-to-electricity conversion is developed from Planck's law for the distribution of the radiant exitance of heat at a selected temperature. An electrical power curve is calculated by integration of the heat law over a selected range of electromagnetic wavelength corresponding to electrical voltage. A novel wavelength-voltage conversion factor, developed from the known wavelength-electron volt conversion factor, establishes the wavelength ({lambda}) for the integration. The Planck law is integrated within the limits {lambda} to 2{lambda}. The integration provides the ideal electrical power that is available from heat at the emitter temperature. When multiplied by a simple ratio, the calculated ideal power closely matches published thermionic converter experimental data. The thermal power model of thermionic conversion is validated by experiments with thermionic emission of ordinary electron tubes. A theoretical basis for the heat law based model of thermionic conversion is found in linear oscillator theory.

Caldwell, F.

1998-07-01T23:59:59.000Z

137

MAP and Planck vs the Real Universe  

E-Print Network (OSTI)

The Microwave Anisotropy Probe (MAP) and Planck Surveyor satellites promise to provide accurate maps of the sky at a range of frequencies and angular scales, from which it will be possible to extract estimates for cosmological parameters. But the real Universe is a nasty, messy place, full of non-linear astrophysics. It is certainly clear that MAP and Planck will fix the background cosmology at an unprecedented level. However, they will have to contend with everything that the Universe throws at them: multiple foregrounds; structure formation effects; and other complications we haven't even thought of yet. Some examples of such effects will be presented. Only an ideal, theorist's universe can be described by a number of free parameters in the single digits, while in reality it is likely that a greater wealth of information waits to be discovered. These `higher-order' processes should be considered as potentially measurable signals, rather than contaminants. The capabilities of Planck seem ideally suited to fully understanding the physics encoded in the microwave sky.

Douglas Scott

1998-10-21T23:59:59.000Z

138

A simulation pipeline for the Planck mission  

E-Print Network (OSTI)

We describe an assembly of numerical tools to model the output data of the Planck satellite. These start with the generation of a CMB sky in a chosen cosmology, add in various foreground sources, convolve the sky signal with arbitrary, even non-symmetric and polarised beam patterns, derive the time ordered data streams measured by the detectors depending on the chosen satellite-scanning strategy, and include noise signals for the individual detectors and electronic systems. The simulation products are needed to develop, verify, optimise, and characterise the accuracy and performance of all data processing and scientific analysis steps of the Planck mission, including data handling, data integrity checking, calibration, map making, physical component separation, and power spectrum estimation. In addition, the simulations allow detailed studies of the impact of many stochastic and systematic effects on the scientific results. The efficient implementation of the simulation allows the build-up of extended statistics of signal variances and co-variances. Although being developed specifically for the Planck mission, it is expected that the employed framework as well as most of the simulation tools will be of use for other experiments and CMB-related science in general.

Martin Reinecke; Klaus Dolag; Reinhard Hell; Matthias Bartelmann; Torsten Ensslin

2005-08-24T23:59:59.000Z

139

Hardness of Max-2Lin and Max-3Lin over integers, reals, and large cyclic Ryan O'Donnell  

E-Print Network (OSTI)

systems of linear equations. Given a ring R, the Max-kLin(R) problem is defined as follows: An input, this easily implies the same hardness for Max--3Lin(Q) and Max--3Lin(R). In- deed, it shows a kind of "bicriHardness of Max-2Lin and Max-3Lin over integers, reals, and large cyclic groups Ryan O

O'Donnell, Ryan

140

On visualization scaling, subeigenvectors and Kleene stars in max algebra  

E-Print Network (OSTI)

and Kleene stars in max algebra #12;Max Algebra a, b R+ a + b, ab A, B Rm?n + A + B, AB, . a b = max(a, b;(Ar )ij = max (i,j;r) (i, j; r)(A) (I A · · · An-1)ij = max(i.j,r) (i, j; r) : r = 0, . . . n - 1 A definite: (A) = 1 (I A · · · An-1)ij = max(i,j) (i, j) : r = 0, . . . , Hans Schneider based on joint

Schneider, Hans

Note: This page contains sample records for the topic "max planck institute" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


141

Fokker-Planck equation in mirror research  

SciTech Connect

Open confinement systems based on the magnetic mirror principle depend on the maintenance of particle distributions that may deviate substantially from Maxwellian distributions. Mirror research has therefore from the beginning relied on theoretical predictions of non-equilibrium rate processes obtained from solutions to the Fokker-Planck equation. The F-P equation plays three roles: Design of experiments, creation of classical standards against which to compare experiment, and predictions concerning mirror based fusion power systems. Analytical and computational approaches to solving the F-P equation for mirror systems will be reviewed, together with results and examples that apply to specific mirror systems, such as the tandem mirror.

Post, R.F.

1983-08-11T23:59:59.000Z

142

A combinatorial algorithm for MAX CSP  

Science Journals Connector (OSTI)

We consider the problem MAX CSP over multi-valued domains with variables ranging over sets of size si ? s and constraints involving kj ? k variables. We study two algorithms with approximation ratios A ... Keywords: algorithmical approximation, analysis of algorithms, combinatorial problems, databases, design of algorithms, graph algorithms

Mayur Datar; Toms Feder; Aristides Gionis; Rajeev Motwani; Rina Panigrahy

2003-03-01T23:59:59.000Z

143

Fokker-Planck/Transport model for neutral beam driven tokamaks  

SciTech Connect

The application of nonlinear Fokker-Planck models to the study of beam-driven plasmas is briefly reviewed. This evolution of models has led to a Fokker-Planck/Transport (FPT) model for neutral-beam-driven Tokamaks, which is described in detail. The FPT code has been applied to the PLT, PDX, and TFTR Tokamaks, and some representative results are presented.

Killeen, J.; Mirin, A.A.; McCoy, M.G.

1980-01-01T23:59:59.000Z

144

QED corrections to Plancks radiation law and photon thermodynamics  

Science Journals Connector (OSTI)

Leading corrections to Plancks radiation formula and other photon thermodynamic functions arising from the pair-mediated photon-photon interaction are calculated. This interaction is found to be attractive and to cause a small increase in occupation number for all modes and a corresponding correction to the equation of state. The results are valid for the range of temperatures well below Te=5.9 GK, the temperature equivalent to the electron mass, a range for which the photon gas is essentially free of pair-produced electrons and positrons. An interesting effect of these corrections is the behavior of the photon gas as an elastic medium and its ability to propagate density perturbations. It is found that the cosmic photon gas subsequent to electron-positron annihilation would have manifested these elastic properties were it not for the presence of the free electrons and their dominance of the photon thermodynamics.

M. Hossein Partovi

1994-07-15T23:59:59.000Z

145

de r eche r che INSTITUT NATIONAL DE RECHERCHE EN INFORMATIQUE ET EN AUTOMATIQUE  

E-Print Network (OSTI)

'' (R[ f\\Gamma1g; max; +), or the ``tropical semiring'' (N[f+1g;min;+), have been invented'alg??ebre lin??eaire (max,+) R??esum??e : Il s'agit d'une br??eve introduction au semi­anneau (max,+) et autres semiISSN 0249­6399 appo r t de r eche r che INSTITUT NATIONAL DE RECHERCHE EN INFORMATIQUE ET EN

O'Sullivan, Joseph A.

146

MINI REVIEW ARTICLE published: 28 April 2014  

E-Print Network (OSTI)

to individual differences in brain structure? Jenny Gu1 * and Ryota Kanai1,2 1 School of Psychology, University Edited by: Burkhard Pleger, Max Planck Institute for Human Cognitive and Brain Sciences, Germany Reviewed by: Marco Taubert, Max-Planck-Institute for Human Cognitive and Brain Sciences, Germany Christopher J

Sussex, University of

147

Institutional INSTITUTIONAL DATA BOOK  

E-Print Network (OSTI)

that institutions provide for their learning and personal development. The University of Minnesota is an equal ORGANIZATIONAL STRUCTURE UMM Organizational Chart as of August 2009

Minnesota, University of

148

Neurton Damage and MAX Phase Ternary Compounds  

SciTech Connect

The Demands of Gen IV nuclear power plants for long service life under neutron radiation at high temperature are severe. Advanced materials that would withstand high temperatures (up to 1000+ C) to high doses in a neutron field would be ideal for reactor internal structures and would add to the long service life and reliability of the reactors. The objective of this work is to investigate the resonse of a new class of machinable, conductive, layered, ternary transition metal carbides and nitrides - the so-called MAX phases - to low and moderate neutron dose levels.

Barsoum, Michael; Hoffman, Elizabeth; Sindelar, Robert; Garcua-Duaz, Brenda; Kohse, Gordon

2014-06-17T23:59:59.000Z

149

Engineering Institute  

NLE Websites -- All DOE Office Websites (Extended Search)

Institute Engineering Institute Engineering dynamics that include flight, vibration isolation for precision manufacturing, earthquake engineering, blast loading, signal processing,...

150

University of Maryland Wins Max Tech and Beyond Competition for  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

University of Maryland Wins Max Tech and Beyond Competition for University of Maryland Wins Max Tech and Beyond Competition for Ultra-Efficient Clothes Dryer University of Maryland Wins Max Tech and Beyond Competition for Ultra-Efficient Clothes Dryer September 10, 2013 - 12:00pm Addthis The Energy Department announced today that the University of Maryland won the second annual Max Tech and Beyond design competition for ultra-low energy use appliances and equipment for the second year in a row. The team developed a heat pump clothes dryer that is nearly 59% more efficient than a traditional electric dryer. The Max Tech and Beyond competition challenges university teams to go beyond the current "max tech," or maximum technology performance levels, by exploring new design concepts that could become the next generation of

151

Extended Fokker Planck model: properties and solutions  

E-Print Network (OSTI)

In the current paper Fokker Planck model of random walks has been extended to non conservative cases characterized by explicit dependence of diffusion and energy on time. A given generalization allows describing of such non equilibrium processes as Levy flights in a classical differential form without use of fractal PDE. Besides it takes into account mixing properties that are obligatory for a certain class of chaotic systems such as Kolmogorov K system. It was shown that an abnormal transport is a consequence of the equilibrium distortion and not stationary diffusion. The particular case of fixed boundaries was considered. According to the received solutions it was shown that a system structure can resist a weak disturbance in the vicinity of the discrete regimes, defined by a system scale and its nonlinear properties. These regimes correspond to the exponential increase of quasi regular structure fluctuations. Only fast disruption of regime is possible for other states of the system. It leads to an immediate transition to the chaos.

Sergey Kamenshchikov

2014-01-20T23:59:59.000Z

152

Min-max-min robustness - Optimization Online  

E-Print Network (OSTI)

or the minimum spanning tree problem turn NP-hard in the new approach. ..... [9] Melvyn, S., Robust optimization, Ph.D. thesis, Massachusetts Institute of.

2014-11-27T23:59:59.000Z

153

A branch and bound algorithm for numerical Max-CSP  

Science Journals Connector (OSTI)

The Constraint Satisfaction Problem (CSP) framework allows users to define problems in ... no solution is generally unsatisfactory. A Max-CSP ...

Jean-Marie Normand; Alexandre Goldsztejn; Marc Christie; Frdric Benhamou

2010-04-01T23:59:59.000Z

154

Clique Inference Process for Solving Max-CSP  

Science Journals Connector (OSTI)

In this paper we show that the clique concept can be exploited in order to solve Max-CSP. We present a clique inference process which...

Mohand Ou Idir Khemmoudj; Hachemi Bennaceur

2006-01-01T23:59:59.000Z

155

AVTA: 2013 Ford C-MAX HEV Testing Results  

Energy.gov (U.S. Department of Energy (DOE))

VTO's National Laboratories have tested and collected both dynamometer and fleet data for the Ford C-MAX HEV (a hybrid electric vehicle).

156

Planck intermediate results. XXIII. Galactic plane emission components derived from Planck with ancillary data  

E-Print Network (OSTI)

Planck data when combined with ancillary data provide a unique opportunity to separate the diffuse emission components of the inner Galaxy. The purpose of the paper is to elucidate the morphology of the various emission components in the strong star-formation region lying inside the solar radius and to clarify the relationship between the various components. The region of the Galactic plane covered is l=300-0-60deg where star-formation is highest and the emission is strong enough to make meaningful component separation. The latitude widths in this longitude range lie between 1deg and 2deg, which correspond to FWHM z-widths of 100-200pc at a typical distance of 6kpc. The four emission components studied here are synchrotron, free-free, anomalous microwave emission (AME), and thermal (vibrational) dust emission. These components are identified by constructing spectral energy distributions (SEDs) at positions along the Galactic plane using the wide frequency coverage of Planck (28.4-857GHz) in combination with l...

Ade, P A R; Alves, M I R; Arnaud, M; Ashdown, M; Atrio-Barandela, F; Aumont, J; Baccigalupi, C; Banday, A J; Barreiro, R B; Battaner, E; Benabed, K; Benoit-Lvy, A; Bernard, J -P; Bersanelli, M; Bielewicz, P; Bobin, J; Bonaldi, A; Bond, J R; Bouchet, F R; Boulanger, F; Burigana, C; Cardoso, J -F; Catalano, A; Chamballu, A; Chiang, H C; Christensen, P R; Clements, D L; Colombi, S; Colombo, L P L; Combet, C; Couchot, F; Crill, B P; Cuttaia, F; Danese, L; Davies, R D; Davis, R J; de Bernardis, P; de Rosa, A; de Zotti, G; Delabrouille, J; Dickinson, C; Diego, J M; Donzelli, S; Dor, O; Douspis, M; Dupac, X; Efstathiou, G; Enlin, T A; Eriksen, H K; Finelli, F; Forni, O; Frailis, M; Franceschi, E; Galeotta, S; Ganga, K; Gnova-Santos, R T; Ghosh, T; Giard, M; Giardino, G; Giraud-Hraud, Y; Gonzlez-Nuevo, J; Grski, K M; Gregorio, A; Gruppuso, A; Hansen, F K; Harrison, D L; Henrot-Versill, S; Herranz, D; Hildebrandt, S R; Hivon, E; Hobson, M; Hornstrup, A; Hovest, W; Huffenberger, K M; Jaffe, A H; Jaffe, T R; Jones, W C; Keihnen, E; Keskitalo, R; Kisner, T S; Kneissl, R; Knoche, J; Kunz, M; Kurki-Suonio, H; Lagache, G; Lhteenmki, A; Lamarre, J -M; Lasenby, A; Lawrence, C R; Leonardi, R; Liguori, M; Lilje, P B; Linden-Vrnle, M; Lpez-Caniego, M; Lubin, P M; Macas-Prez, J F; Maino, D; Mandolesi, N; Martin, P G; Martnez-Gonzlez, E; Masi, S; Massardi, M; Matarrese, S; Mazzotta, P; Meinhold, P R; Melchiorri, A; Mendes, L; Mennella, A; Migliaccio, M; Mitra, S; Miville-Deschnes, M -A; Moneti, A; Montier, L; Morgante, G; Mortlock, D; Munshi, D; Murphy, J A; Naselsky, P; Nati, F; Natoli, P; Nrgaard-Nielsen, H U; Noviello, F; Novikov, D; Novikov, I; Oxborrow, C A; Pagano, L; Pajot, F; Paladini, R; Paoletti, D; Pasian, F; Pearson, T J; Peel, M; Perdereau, O; Perrotta, F; Piacentini, F; Piat, M; Pierpaoli, E; Pietrobon, D; Plaszczynski, S; Pointecouteau, E; Polenta, G; Ponthieu, N; Popa, L; Pratt, G W; Prunet, S; Puget, J -L; Rachen, J P; Reach, W T; Rebolo, R; Reich, W; Reinecke, M; Remazeilles, M; Renault, C; Ricciardi, S; Riller, T; Ristorcelli, I; Rocha, G; Rosset, C; Roudier, G; Rubio-Martn, J A; Rusholme, B; Sandri, M; Savini, G; Scott, D; Spencer, L D; Stolyarov, V; Strong, A W; Sutton, D; Suur-Uski, A -S; Sygnet, J -F; Tauber, J A; Tavagnacco, D; Terenzi, L; Tibbs, C T; Toffolatti, L; Tomasi, M; Tristram, M; Tucci, M; Valenziano, L; Valiviita, J; Van Tent, B; Varis, J; Vielva, P; Villa, F; Wade, L A; Wandelt, B D; Watson, R; Yvon, D; Zacchei, A; Zonca, A

2014-01-01T23:59:59.000Z

157

Deciding Unambiguity and Sequentiality from a Finitely Ambiguous MaxPlus Automaton  

E-Print Network (OSTI)

with multiplicities in the max­plus semiring R max = (R # {-#},max, +). Roughly speaking, it is an automaton with two tapes: an input tape labelled by a finite alphabet #, and an output tape weighted in R max . The weightDeciding Unambiguity and Sequentiality from a Finitely Ambiguous Max­Plus Automaton Ines Klimann

Fondements et Applications, Université Paris 7

158

Lesson 05 - Working with Autodesk 3ds Max  

Science Journals Connector (OSTI)

If you have completed the first four lessons, you have worked with Autodesk 3ds Max from modeling and animation to materials and rendering. Now is a good time to review some of the user interface concepts that you have used and introduce some new tools in order to provide a more complete overview of how 3ds Max works.

Autodesk

2008-01-01T23:59:59.000Z

159

Implications of SCUBA observations for the Planck Surveyor  

E-Print Network (OSTI)

We investigate the implications for the Planck Surveyor of the recent sub-millimetre number counts obtained using the SCUBA camera. Since it observes at the same frequency as one of the higher frequency science channels on Planck, SCUBA can provide constraints on the point-source contribution to the CMB angular power spectrum, which require no extrapolation in frequency. We have calculated the two-point function of these sub-millimetre sources, using a Poisson model normalized to the observed counts. While the current data are uncertain, under reasonable assumptions the point-source contribution to the anisotropy is comparable to the noise in the 353GHz channel. The clustering of these sources is currently unknown, however if they cluster like the z~3 Lyman-break galaxies their signal would be larger than the primary anisotropy signal on scales smaller than about 10 arcmin. We expect the intensity of these sources to decrease for wavelengths longward of 850 microns. At the next lowest Planck frequency, 217GHz, the contribution from both the clustered and Poisson terms are dramatically reduced. Hence we do not expect these sources to seriously affect Planck's main science goal, the determination of the primordial anisotropy power spectrum. Rather, the potential determination of the distribution of sub-mm sources is a further piece of cosmology that Planck may be able to tackle.

Douglas Scott; Martin White

1999-03-18T23:59:59.000Z

160

The MAX facility for CFD code validation  

SciTech Connect

ANL has recently completed construction of a fluid dynamics test facility devised to provide validation data for CFD simulation tools used to evaluate various aspects of nuclear power plant design and safety. Experiments with the facility involve mixing air jets within a 1x1x1.7m long glass tank at atmospheric pressure. A particle image velocimetry system measures flow velocity and turbulence quantities within the tank while a high-speed infrared camera records temperatures across the tank lid. The tandem of high fidelity thermal and turbulence data is particularly useful for benchmarking transient heat transfer phenomena such as thermal striping. This paper describes the MAX facility, preliminary data obtained during shakedown tests, and the results of companion CFD calculations employing RANS-based Star-CCM+ and large eddy simulations with Nek 5000. (authors)

Lomperski, S.; Merzari, E.; Obabko, A.; Pointer, W. D.; Fischer, P. [Argonne National Laboratory, Bldg. 206, 9700 S. Cass Ave, Argonne, IL 60439 (United States)

2012-07-01T23:59:59.000Z

Note: This page contains sample records for the topic "max planck institute" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


161

The Effective Planck Mass and the Scale of Inflation  

E-Print Network (OSTI)

Observable quantities in cosmology are dimensionless, and therefore independent of the units in which they are measured. This is true of all physical quantities associated with the primordial perturbations that source cosmic microwave background anisotropies such as their amplitude and spectral properties. However, if one were to try and \\textit{infer} an absolute energy scale for inflation-- a priori, one of the more immediate corollaries of detecting primordial tensor modes-- one necessarily makes reference to a particular choice of units, the natural choice for which is Planck units. In this note, we discuss various aspects of how inferring the energy scale of inflation is complicated by the fact that the effective Planck mass as seen by inflationary quanta necessarily differs from the effective Planck mass as seen by gravitational experiments at presently accessible scales. The uncertainty in the former relative to the latter has to do with the unknown spectrum of universally coupled particles between lab...

Antoniadis, Ignatios

2014-01-01T23:59:59.000Z

162

Component-based Face Recognition with 3D Morphable Models B. Weyrauch  

E-Print Network (OSTI)

@mpi-sb.mpg.de Honda Research Institute USA, Inc. Max-Planck-Institute for Computer Science Boston, MA Saarbr. In this paper, we combine morphable models and component-based recognition. The morphable model is em- ployed

Poggio, Tomaso

163

Venkatraman Ramakrishnan, Thomas A. Steitz, Ada E. Yonath, and...  

Office of Scientific and Technical Information (OSTI)

led a group from the Weizmann Institute in Israel and the Max Planck Institute in Germany. The second group was led by Venki Ramakrishnan... .'3 'Steitz also performed work at...

164

The detection algorithm work in three steps:The detection algorithm work in three steps: bandpass filtered mslp minima (<-1hPa) arebandpass filtered mslp minima (<-1hPa) are  

E-Print Network (OSTI)

(2) GKSS Research Centre, Institute for Coastal Research, Germany (3) Max-Planck-Institut für simulations with CLM, submitted see:"http://coast.gkss.de/staff/zahn/" or "http://coast.gkss

Zahn, Matthias

165

Technische Universitt Darmstadt Center of Smart Interfaces  

E-Print Network (OSTI)

Mainz, Max-Planck-Institute for Polymer Re- search, Deutsches Kunststoffinstitut, Fraunhofer Institute for innovation and promise for techno- logy transfer to industrial applications can be recognized. A primary

Haller-Dintelmann, Robert

166

Board of Directors : Prof. Alfred Leipertz (Coordinator) Prof. Michael Schmidt (Co-Coordinator)  

E-Print Network (OSTI)

in their respective fields and has as its aim the promotion of innovation and leadership skills in all specialist in the SAOT. · Max Planck Institute for the Science of Light (MPL) · Fraunhofer Institute for Integrated

Fiebig, Peter

167

Atmos. Chem. Phys., 13, 70077021, 2013 www.atmos-chem-phys.net/13/7007/2013/  

E-Print Network (OSTI)

-Zentrum Geesthacht, Institute of Coastal Research, Department for Environmental Chemistry, Max-Planck-Str. 1, 21502 Geesthacht, Germany 5Institute of Environmental Physics, University of Heidelberg, Im Neuenheimer Feld 229

Meskhidze, Nicholas

168

Intensified Southern Hemisphere Westerlies regulated atmospheric CO2 during the last deglaciation  

Science Journals Connector (OSTI)

...Center Julich, 52425 Julich, Germany 4 Institute for Coastal Research, Helmholtz-Zentrum Geesthacht, Max-Planck-Strasse 1, 21502 Geesthacht, Germany 5 Institute of Geography, University of Bremen, Celsiusstrasse FVG-M, 28359 Bremen...

C. Mayr; A. Lcke; S. Wagner; H. Wissel; C. Ohlendorf; T. Haberzettl; M. Oehlerich; F. Schbitz; M. Wille; J. Zhu; B. Zolitschka

169

Figure 2: Pulse sequence: Navigators are applied before inner-volume saturation (IVS), up-/downfield  

E-Print Network (OSTI)

, and Anke Henning1,3 1 Institute for Biomedical Engineering, University and ETH Zurich, Zurich, Switzerland, 2 Institute of Neuroradiology, University Hospital of Zurich, Zurich, Switzerland, 3 Max Planck

170

Making Maps from Planck LFI 30GHz Data with Asymmetric Beams and Cooler Noise  

E-Print Network (OSTI)

J. Ashdown et al. : Making Maps from Planck LFI 30GHz DataJ. Ashdown et al. : Making Maps from Planck LFI 30GHz Datain this study. The hit map is shown in the ecliptic (left)

Ashdown, M.A.J.

2010-01-01T23:59:59.000Z

171

arXiv:astro-ph/0609503v118Sep2006 Observations Supporting the Role of Magnetoconvection in  

E-Print Network (OSTI)

Supply to the Quiescent Solar Atmosphere Scott W. McIntosh, Alisdair R. Davey, Donald M. Hassler USA Werner Curdt, Klaus Wilhelm Max Planck Institute for Solar System Research, Max-Planck-Str. 2 mechanisms behind the production and suste- nance of the quiescent solar corona and solar wind poses two

Lin, Gang

172

Making Maps from Planck LFI 30GHz Data  

E-Print Network (OSTI)

This paper is one of a series describing the performance and accuracy of map-making codes as assessed by the Planck CTP working group. We compare the performance of multiple codes written by different groups for making polarized maps from Planck-sized, all-sky cosmic microwave background (CMB) data. Three of the codes are based on destriping algorithm, whereas the other three are implementations of a maximum-likelihood algorithm. Previous papers in the series described simulations at 100 GHz (Poutanen et al. 2006) and 217 GHz (Ashdown et al. 2006). In this paper we make maps (temperature and polarisation) from the simulated one-year observations of four 30 GHz detectors of Planck Low Frequency Instrument (LFI). We used Planck Level S simulation pipeline to produce the observed time-ordered-data streams (TOD). Our previous studies considered polarisation observations for the CMB only. For this paper we increased the realism of the simulations and included polarized galactic foregrounds to our sky model. Our simulated TODs comprised of dipole, CMB, diffuse galactic emissions, extragalactic radio sources, and detector noise. The strong subpixel signal gradients arising from the foreground signals couple to the output map through the map-making and cause an error (signal error) in the maps. Destriping codes have smaller signal error than the maximum-likelihood codes. We examined a number of schemes to reduce this error. On the other hand, the maximum-likelihood map-making codes can produce maps with lower residual noise than destriping codes.

M. A. J. Ashdown; C. Baccigalupi; A. Balbi; J. G. Bartlett; J. Borrill; C. Cantalupo; G. de Gasperis; K. M. Gorski; V. Heikkila; E. Hivon; E. Keihanen; H. Kurki-Suonio; C. R. Lawrence; P. Natoli; T. Poutanen; S. Prunet; M. Reinecke; R. Stompor; B. Wandelt

2007-02-19T23:59:59.000Z

173

On the Fokker-Planck Equation for Stochastic Hybrid Systems  

E-Print Network (OSTI)

On the Fokker-Planck Equation for Stochastic Hybrid Systems: Application to a Wind Turbine Model- speed wind turbine, with a switching controller that combines stall regulation and pitch control FPE is stated. Then the theory is applied to a variable-speed wind turbine model, yielding

Boyer, Edmond

174

QED Corrections to Planck's Radiation Law and Photon Thermodynamics  

E-Print Network (OSTI)

Leading corrections to Planck's formula and photon thermodynamics arising from the pair-mediated photon-photon interaction are calculated. This interaction is attractive and causes an increase in occupation number for all modes. Possible consequences, including the role of the cosmic photon gas in structure formation, are considered.

M. Hossein Partovi

1993-08-18T23:59:59.000Z

175

Dark energy constraints after the new Planck data  

Science Journals Connector (OSTI)

The Planck Collaboration has recently published maps of the cosmic microwave background radiation with the highest precision. In the standard flat ? cold dark matter framework, Planck data show that the Hubble constant H0 is in tension with that measured by the several direct probes on H0. In this paper, we perform a global analysis from the current observational data in the general dark energy models and find that resolving this tension requires the dark energy model with its equation of state (EOS) w?-1. Firstly, assuming the w to be a constant, the Planck data favor wsurvey compilation. Consequently the value derived on H0, H0=71.32.0??km?s-1?Mpc-1 (68%C.L.) is consistent with that from direct H0 probes. We then investigate the dark energy model with a time-evolving w, and obtain the 68%C.L. constraints w0=-0.810.19 and wa=-1.91.1 from the Planck data and the supernova legacy survey compilation. Current data still slightly favor the quintom dark energy scenario with EOS across the cosmological constant boundary w?-1.

Jun-Qing Xia; Hong Li; Xinmin Zhang

2013-09-03T23:59:59.000Z

176

Max Tech and Beyond Design Competition | Department of Energy  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

Max Tech and Beyond Design Competition Max Tech and Beyond Design Competition Max Tech and Beyond Design Competition The Max Tech and Beyond Design Competition is an annual competition run by the Department of Energy (DOE) and the Lawrence Berkeley National Laboratory (LBNL) that encourages students to tackle challenges in designing energy efficient appliances and test performance to evaluate reductions in energy consumption. The competition challenges 10 - 20 collegiate teams nationwide to design and test appliance innovations with the potential to significantly reduce energy consumption while providing a level of service comparable to or better than current best-on-market products. The winner of the competition will be the team that best demonstrates energy savings potential for viable future products.

177

MaxWest Environmental Systems | Open Energy Information  

Open Energy Info (EERE)

MaxWest Environmental Systems MaxWest Environmental Systems Jump to: navigation, search Name MaxWest Environmental Systems Place Houston, Texas Zip 77057 Product MaxWest Environmental Systems designs, builds, owns and operates gasification systems on a turnkey basis. Coordinates 29.76045°, -95.369784° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":29.76045,"lon":-95.369784,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

178

Property:Incentive/MaxInc | Open Energy Information  

Open Energy Info (EERE)

MaxInc MaxInc Jump to: navigation, search Property Name Incentive/MaxInc Property Type Text Description Maximum Incentive. Pages using the property "Incentive/MaxInc" Showing 25 pages using this property. (previous 25) (next 25) 2 2003 Climate Change Fuel Cell Buy-Down Program (Federal) + lesser of 1,000/kW or one-third total project cost 3 30% Business Tax Credit for Solar (Vermont) + No maximum specified. A AEP (Central and North) - Residential Energy Efficiency Programs (Texas) + SOP TCC: $150,000 (Large Projects); $150,000 (Small Projects); $25,000 (Small Projects Monthly Reservation Limit) SOP TNC: $40,000 (Large Projects); $20,000 (Small Projects); $5,000 (Small Projects Monthly Reservation Limit) SOP TCC (Hard to Reach): $75,000/sponsor SOP TNC (Hard to Reach): $50,000/sponsor

179

Property:Incentive/PVPbiFitMaxKW | Open Energy Information  

Open Energy Info (EERE)

PVPbiFitMaxKW PVPbiFitMaxKW Jump to: navigation, search Property Name Incentive/PVPbiFitMaxKW Property Type String Description The maximum installed PV capacity in kW that is eligible for the PBI or FIT. Ex: We Energies' FIT maximum eligible PV system size is 100 kW. Format: 100.0 [1] References ↑ DSIRE Pages using the property "Incentive/PVPbiFitMaxKW" Showing 25 pages using this property. (previous 25) (next 25) A Alliant Energy (Wisconsin Power and Light) - Advanced Renewables Tariff (Wisconsin) + 20 + Ameren Missouri - Solar Renewable Energy Credits + 100 + Anaheim Public Utilities - PV Buydown Program (California) + 1000 + Austin Energy - Commercial PV Incentive Program (Texas) + 20 + Austin Energy - Value of Solar Residential Rate (Texas) + 20 +

180

Property:Incentive/WindResPercMax | Open Energy Information  

Open Energy Info (EERE)

WindResPercMax WindResPercMax Jump to: navigation, search Property Name Incentive/WindResPercMax Property Type String Description The maximum % of the installed cost of a residential wind system that the rebate may offset. Use this for (1.) rebates calculated in terms of % of capital cost as well as (2.) rebates structured in terms of $/kW or $/kWh that also have a maximum % of costs that can be offset by the rebate. Ex: (1.) DE's rebate is 50% of the project cost; (2.) WI's residential wind incentive is based on annual expected performance, up to 25% of installed cost. Format: 25% [1] References ↑ DSIRE Pages using the property "Incentive/WindResPercMax" Showing 25 pages using this property. (previous 25) (next 25) A AEP Ohio - Renewable Energy Technology Program (Ohio) + 50% +

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181

Anatomic Segmentation of Statistical Shape Models Max Hermann1  

E-Print Network (OSTI)

-289, 2010. [4] M. Hermann, A.C. Schunke, T. Schultz, R. Klein: "A Visual Analytics Approach to StudyAnatomic Segmentation of Statistical Shape Models Max Hermann1 , Anja C. Schunke2 , Reinhard Klein1

Eckmiller, Rolf

182

A 0.5-APPROXIMATION ALGORITHM FOR MAX DICUT WITH GIVEN SIZES OF PARTS  

E-Print Network (OSTI)

(G) ! R+ , the maximum directed cut problem (max dicut) is that of #12;nding a directed cut ?A 0.5-APPROXIMATION ALGORITHM FOR MAX DICUT WITH GIVEN SIZES OF PARTS ALEXANDER AGEEV #3; , REFAEL(X) with maximum total weight. In this paper we consider a version of max dicut|max dicut with given sizes of parts

Ageev, Alexandr

183

New Bounds for MAX-SAT by Clause Learning Alexander S. Kulikov  

E-Print Network (OSTI)

New Bounds for MAX-SAT by Clause Learning Alexander S. Kulikov Konstantin Kutzkov May 3, 2009 c MAX-SAT for formulas with constant clause density; · 2K/6 , where K is the number of clauses, for MAX-2-SAT; · 2N/6.7 for (n, 3)-MAX-2-SAT. All

184

A New Approach to Proving Upper Bounds for MAX-2-SAT Arist Kojevnikov  

E-Print Network (OSTI)

A New Approach to Proving Upper Bounds for MAX-2-SAT Arist Kojevnikov Alexander S. Kulikov problem (MAX-2-SAT). We present a new 2K/5.5 -time algorithm for MAX-2-SAT, where K is the number formula, for a particular case of MAX-2-SAT, where each variable appears in at most three 2-clauses

185

On the integer max-linear programming problem Peter Butkovic1,  

E-Print Network (OSTI)

and the integer max-linear programming problem. In max-algebra, for a, b R = R {-}, we define a b = max(a, b to Elsevier July 22, 2013 #12;A two-sided max-linear system (TSS) is of the form Ax c = Bx d where A, B R m time, and give a method in this case. If f R n , then the function f(x) = fT x is called max

Butkovic, Peter

186

LINEAR-PROGRAMMING DESIGN AND ANALYSIS OF FAST ALGORITHMS FOR MAX 2-CSP  

E-Print Network (OSTI)

AND GREGORY B. SORKIN Abstract. The class Max (r, 2)-CSP (or simply Max 2-CSP) consists of constraint(rm/5) for r- valued problems), making it the fastest for Max Cut, and tied (at the time) for Max 2-Sat(·) notation, which ignores leading polynomial factors, is defined in Section 2.1.) For Max 2-CSP we give an O(r

Scott, Alexander Alexander

187

A Generalized Boltzmann Fokker-Planck (GBFP) Electron Transport Method  

National Nuclear Security Administration (NNSA)

Generalized Boltzmann Fokker-Planck Generalized Boltzmann Fokker-Planck (GBFP) Electron Transport Method Brian C. Franke Leonard J. Lorence Sandia National Laboratories Anil K. Prinja University of New Mexico Joint Russian-American Five-Laboratory Conference on Computational Mathematics / Physics Vienna, Austria June 19-23, 2005 SAND2005-3228C Sandia is a multiprogram laboratory operated by Sandia Corporation, a Lockheed Martin Company, for the United States National Nuclear Security Administration and the Department Energy under contract DE-AC04-94AL85000. 2 Overview GBFP Angular Scattering Approximations - Discrete - Hybrid-Discrete - Hybrid-Exponential Condensed History (CH) Algorithms 3-Dimensional Simulation (2-Dimensional Results) with a Material Interface - High-energy electrons in low-Z materials

188

The Effective Planck Mass and the Scale of Inflation  

E-Print Network (OSTI)

Observable quantities in cosmology are dimensionless, and therefore independent of the units in which they are measured. This is true of all physical quantities associated with the primordial perturbations that source cosmic microwave background anisotropies such as their amplitude and spectral properties. However, if one were to try and \\textit{infer} an absolute energy scale for inflation-- a priori, one of the more immediate corollaries of detecting primordial tensor modes-- one necessarily makes reference to a particular choice of units, the natural choice for which is Planck units. In this note, we discuss various aspects of how inferring the energy scale of inflation is complicated by the fact that the effective Planck mass as seen by inflationary quanta necessarily differs from the effective Planck mass as seen by gravitational experiments at presently accessible scales. The uncertainty in the former relative to the latter has to do with the unknown spectrum of universally coupled particles between laboratory scales and the putative scale of inflation. These intermediate particles could be in hidden as well as visible sectors or could also be associated with Kaluza-Klein resonances associated with a compactification scale below the scale of inflation. We discuss various implications for cosmological observables.

Ignatios Antoniadis; Subodh P. Patil

2014-10-31T23:59:59.000Z

189

Planck's confirmation of the M31 disk and halo rotation  

E-Print Network (OSTI)

Planck's data acquired during the first 15.4 months of observations towards both the disk and halo of the M31 galaxy are analyzed. We confirm the existence of a temperature asymmetry, previously detected by using the 7-year WMAP data, along the direction of the M31 rotation, therefore indicative of a Doppler-induced effect. The asymmetry extends up to about 10 degrees (about 130 kpc) from the M31 center. We also investigate the recent issue raised in Rubin and Loeb (2014) about the kinetic Sunyaev-Zeldovich effect from the diffuse hot gas in the Local Group, predicted to generate a hot spot of a few degrees size in the CMB maps in the direction of M31, where the free electron optical depth gets the maximum value. We also consider the issue whether in the opposite direction with respect to the M31 galaxy the same effect induces a minimum in temperature in the Planck's maps of the sky. We find that the Planck's data at 100 GHz show an effect even larger than that expected.

De Paolis, F; Nucita, A A; Ingrosso, G; Kashin, A L; Khachatryan, H G; Mirzoyan, S; Poghosian, E; Jetzer, Ph; Qadir, A; Vetrugno, D

2014-01-01T23:59:59.000Z

190

The Max Tech and Beyond Competition | Department of Energy  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

The Max Tech and Beyond Competition The Max Tech and Beyond Competition The Max Tech and Beyond Competition Addthis 1 of 5 Team Cal Poly Solar is working to significantly reduce the cost and construction time on their solar concentrator for cooking. Image: Lawrence Berkeley National Laboratory 2 of 5 Professor Dale Dolan's students from California Polytechnic State University San Luis Obispo Electrical Engineering department testing the placement of their Hybrid Solar Photovoltaic Panel for Pool Heating. Image: Lawrence Berkeley National Laboratory 3 of 5 Students from the University of Maryland working hard to make a residential air condition unit more efficient. Image: Lawrence Berkeley National Laboratory 4 of 5 Team Ohio State's vapor compression hybrid air/water conditioning system for residential housing.

191

Engineering Institute  

NLE Websites -- All DOE Office Websites (Extended Search)

Engineering Institute Engineering Institute Engineering Institute Engineering dynamics that include flight, vibration isolation for precision manufacturing, earthquake engineering, blast loading, signal processing, and experimental model analysis. Contact Leader, LANL Charles Farrar Email Leader, UCSD Michael Todd Email LANL Program Administrator Jutta Kayser (505) 663-5649 Email Collaboration for conducting mission-driven, multidisciplinary engineering research and recruiting, revitalization, and retention of current & future staff The Engineering Institute is a collaboration between LANL and the University of California at San Diego (UCSD) Jacobs School of Engineering, whose mission is to develop a comprehensive approach for conducting mission-driven, multidisciplinary engineering research

192

Institutional Controls  

NLE Websites -- All DOE Office Websites (Extended Search)

Institutional Controls Institutional Controls Many major Federal laws (e.g., Atomic Energy Act (AEA), Resource Conservation Recovery Act (RCRA), Comprehensive Environmental Response, Compensation and Liability Act (CERCLA)), Executive Orders, regulations and various other drivers influence the use of institutional controls at DOE sites. Some drivers directly authorize or require the use of institutional controls, while others do not. DOE also uses institutional controls when no specific statutory requirement exists to supplement active remediation, pollution control, public and resource protection, and physical security, or to bolster the integrity of engineered remedies. DOE and its predecessor agencies have conducted activities for over 50 years, using land ownership and access control, environmental monitoring and surveillance, and other tools to support protection efforts at operational and inactive facilities, including radioactive waste burial grounds.

193

Solving RCPSP/max by lazy clause generation  

Science Journals Connector (OSTI)

We present a generic exact method for minimizing the project duration of the resource-constrained project scheduling problem with generalized precedence relations (Rcpsp/max). This is a very general scheduling model with applications areas such as project ... Keywords: Constraint programming, Generalized precedence constraints, Lazy clause generation, Project scheduling, Resource constraints, Time windows

Andreas Schutt; Thibaut Feydy; Peter J. Stuckey; Mark G. Wallace

2013-06-01T23:59:59.000Z

194

Structured Region Graphs: Morphing EP into GBP Max Welling  

E-Print Network (OSTI)

Structured Region Graphs: Morphing EP into GBP Max Welling Dept. of Computer Science UC Irvine@eecs.berkeley.edu Abstract GBP and EP are two successful algo­ rithms for approximate probabilistic infer­ ence, which on these structures allow conversion between EP and GBP free ener­ gies. Thus it is revealed that all EP ap

Welling, Max

195

Structured Region Graphs: Morphing EP into GBP Max Welling  

E-Print Network (OSTI)

Structured Region Graphs: Morphing EP into GBP Max Welling Dept. of Computer Science UC Irvine@eecs.berkeley.edu Abstract GBP and EP are two successful algo- rithms for approximate probabilistic infer- ence, which on these structures allow conversion between EP and GBP free ener- gies. Thus it is revealed that all EP ap

Welling, Max

196

Water Quality for Livestock Max Irsik DVM, MAB  

E-Print Network (OSTI)

Water Quality for Livestock Max Irsik DVM, MAB Beef Cattle Extension Veterinarian University of Florida College of Veterinary Medicine Water is an essential nutrient for humans and livestock and drinking water is the primary source of water for most cattle. The most important aspect of water

Watson, Craig A.

197

From corrosion to batteries: Electrochemical interface studies...  

NLE Websites -- All DOE Office Websites (Extended Search)

From corrosion to batteries: Electrochemical interface studies Thursday, October 18, 2012 - 11:00am SSRL, Bldg. 137, Rm 226 Dr. Frank Uwe Renner Max-Planck-Institut fr...

198

Microsoft Word - aac2012_Li_1_WG4-SLAC-PUB-15212.doc  

Office of Scientific and Technical Information (OSTI)

Laboratory (Menlo Park, CA 94025, U.S.A) b Max Planck Institute for Physics (Munich, Germany) c University of California, Los Angeles (Los Angeles, CA 90095, U.S.A) d University...

199

E-Print Network 3.0 - aqueduto vestibular alargado Sample Search...  

NLE Websites -- All DOE Office Websites (Extended Search)

Page: << < 1 2 3 4 5 > >> 1 Max Planck Institute for Biological Cybernetics, Tbingen, Germany VSS 2002, 18.3 ID501 Spatial updating in virtual environments Summary: updating in...

200

S. R. Lee, A. F. Wright, M. H. Crawford, G. A. Petersen, J. Han...  

Office of Scientific and Technical Information (OSTI)

Guide, Technical Report IPP 9113, Max- Planck-Institut fur Plasmaphysik, Garching, Germany, 1997. " W. M. Yim, E. J. Stofko, P. J. Zanzucchi, M. Ettenberg, and S. L, Gilbert,...

Note: This page contains sample records for the topic "max planck institute" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


201

A freely-moving monkey treadmill model Justin D Foster1  

E-Print Network (OSTI)

, Providence, RI 02912, USA 5 Palo Alto Medical Foundation, Palo Alto, CA 94305, USA 6 Max Planck Institute with the speed of individual steps. On a population level, we find that neural state-space trajectories

Shenoy, Krishna V.

202

7, 52775339, 2007 New CARIBIC system  

E-Print Network (OSTI)

Close Full Screen / Esc Printer-friendly Version Interactive Discussion EGU 4 GKSS-Research Centre, Institute for Coastal Research (GKSS), Max-Planck-Stra?e 1, 21502 Geesthacht, Germany 5 Laboratoire des

Paris-Sud XI, Université de

203

A rapid response nowcast/forecast system using multiply nested ocean models and distributed data systems  

E-Print Network (OSTI)

, Sandro Carnield a GKSS Research Center, Institute for Coastal Research, Max-Planck-Str. 1, 21502: +49 4152 87 1525. E-mail address: onken@gkss.de (R. Onken). 1 Previous affiliation: SACLANT Undersea

Robinson, Allan R.

204

E-Print Network 3.0 - attosecond photoelectron spectroscopy Sample...  

NLE Websites -- All DOE Office Websites (Extended Search)

Max-Planck-Institut fr Quantenoptik Collection: Physics 3 Attosecond Atomic Physics Review of literature Summary: will be oscillating in time. When such a state is ionized by an...

205

Astron. Astrophys. 338, L75L78 (1998) ASTROPHYSICS  

E-Print Network (OSTI)

1 Max-Planck-Institut f¨ur Extraterrestrische Physik, Postfach 1603, D-85740 Garching, Germany 2 on the spectrum of CRs, their composition, details of the nuclear cross sections, and propagation in the Galaxy

Moskalenko, Igor V.

206

astroph/9808084 A&A manuscript no.  

E-Print Network (OSTI)

. Strong 1 and O. Reimer 1 1 Max­Planck­Institut f?ur extraterrestrische Physik, Postfach 1603, D­85740, details of the nuclear cross sections, and propagation in the Galaxy. Because they are secondary, an

Strong, Andrew W.

207

Observations of the Li, Be, and B isotopes and constraints on cosmic-ray propagation  

E-Print Network (OSTI)

, CA 90009, USA g Max-Planck-Institut fu¨r extraterrestrische Physik, Postfach 1603, D-85740 Garching and Be in the model predictions is attributed to uncertainties in the production cross-section data. The latter

Moskalenko, Igor V.

208

Atmos. Chem. Phys., 13, 64216428, 2013 www.atmos-chem-phys.net/13/6421/2013/  

E-Print Network (OSTI)

, PMB 1, Menai, NSW 2234, Australia 4Helmholtz-Zentrum Geesthacht, Institute of Coastal Research, Max-Planck-Strasse, 21502 Geesthacht, Germany Correspondence to: F. Slemr (franz.slemr@mpic.de) Received: 18 February 2013

Meskhidze, Nicholas

209

On the edge of death: Rates of decline and lower thresholds of biochemical condition in food-deprived fish larvae and juveniles  

E-Print Network (OSTI)

Helgoland, Germany i Helmholtz Centre Geesthacht, Centre for Materials and Coastal Research, Institute for Coastal Research, Max-Planck-Stra?e 1, 21502 Geesthacht, Germany j Department of Biology, Lund University

210

Atmos. Chem. Phys., 8, 14451482, 2008 www.atmos-chem-phys.net/8/1445/2008/  

E-Print Network (OSTI)

Fourier, France 11GKSS-Forschungszentrum Geesthacht GmbH, Institute for Coastal Research, Department for Environmental Chemistry, Max-Planck-Str. 1, 21052 Geesthacht, Germany 12G¨oteborg University and Chalmers

Douglas, Thomas A.

211

Design of a nitrogen-implanted titanium-based superelastic alloy with optimized properties for  

E-Print Network (OSTI)

, Bucharest, Romania 5 Institute of Materials Research, Helmholtz-Zentrum Geesthacht -Zentrum für Material- und Küstenforschung GmbH Max-Planck-Stra?e 1, D-21502 Geesthacht, Germany *Corresponding author: Prof

Paris-Sud XI, Université de

212

Atmos. Chem. Phys., 14, 22192231, 2014 www.atmos-chem-phys.net/14/2219/2014/  

E-Print Network (OSTI)

-Zentrum Geesthacht, Institute of Coastal Research, Department for Environmental Chemistry,Max-Planck-Str. 1, 21502 Geesthacht, Germany 4Environment Canada, Science and Technology Branch, 867 Lakeshore Rd, Burlington, Ontario

Meskhidze, Nicholas

213

7, 1083710931, 2007 Polar mercury review  

E-Print Network (OSTI)

) and Universite Joseph Fourier, France 10 GKSS-Forschungszentrum Geesthacht GmbH, Institute for Coastal Research, Department for Environmental Chemistry Max-Planck-Str. 1, 21052 Geesthacht, Germany 11 G¨oteborg University

Paris-Sud XI, Université de

214

Contrasting Diversity Patterns of Crenarchaeal, Bacterial and Fungal Soil Communities in an Alpine Landscape  

E-Print Network (OSTI)

.1371/journal.pone.0019950 Editor: Jack Anthony Gilbert, Argonne National Laboratory, United States of America@zinger.fr ¤ Current address: Microbial Habitat Group, Max Planck Institute for Marine Microbiology, Bremen, Germany

Paris-Sud XI, Université de

215

The ATLAS 3D project XXIV. The intrinsic shape distribution of early-type galaxies  

Science Journals Connector (OSTI)

......European Southern Observatory, Karl-Schwarzschild-Str. 2, D-85748 Garching, Germany...Max-Planck-Institut fur Astrophysik, Karl-Schwarzschild-Str. 1, D-85741 Garching, Germany...given by the measurement errors. We mirror the resulting distribution around psi......

Anne-Marie Weijmans; P. T. de Zeeuw; Eric Emsellem; Davor Krajnovi?; Pierre-Yves Lablanche; Katherine Alatalo; Leo Blitz; Maxime Bois; Frdric Bournaud; Martin Bureau; Michele Cappellari; Alison F. Crocker; Roger L. Davies; Timothy A. Davis; Pierre-Alain Duc; Sadegh Khochfar; Harald Kuntschner; Richard M. McDermid; Raffaella Morganti; Thorsten Naab; Tom Oosterloo; Marc Sarzi; Nicholas Scott; Paolo Serra; Gijs Verdoes Kleijn; Lisa M. Young

2014-01-01T23:59:59.000Z

216

USLHC | Angels & Demons Lecture Night - The Science Revealed...  

NLE Websites -- All DOE Office Websites (Extended Search)

pm Max-Planck-Institute Michael Eppard Michael Eppard May 18 Zurich, Switzerland 6:30 pm ETH Zurich Gunther Dissertori, Ulrich Straumann, Christoph Grab Christoph Grab May 18 San...

217

RESEARCH PAPER The anti-protozoal drug pentamidine blocks  

E-Print Network (OSTI)

, Utrecht, The Netherlands; and 2 The Computational Biomolecular Dynamics Group, Max Planck Institute293 cells 10 min after application. When applied to the cytoplasmic side under inside-out patch clamp

de Groot, Bert

218

PHILOSOPHICAL MAGAZINE LETTERS, 2004 VOL. 84, NO. 10, 631641  

E-Print Network (OSTI)

resist buckling in biological materials? Baohua Ji, Huajian Gaoy Max Planck Institute for Metals Research that the most elementary structure of many biological materials consists of mineral crystals with very large

Hsia, K Jimmy

219

Press Releases | Princeton Plasma Physics Lab  

NLE Websites -- All DOE Office Websites (Extended Search)

the highest strength are shown in yellow. Researchers at the U.S. Department of Energy's Princeton Plasma Physics Laboratory (PPPL) and the Max Planck Institute of Plasma Physics...

220

Press Releases Archive | Princeton Plasma Physics Lab  

NLE Websites -- All DOE Office Websites (Extended Search)

the highest strength are shown in yellow. Researchers at the U.S. Department of Energy's Princeton Plasma Physics Laboratory (PPPL) and the Max Planck Institute of Plasma Physics...

Note: This page contains sample records for the topic "max planck institute" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


221

Events - Seminars  

NLE Websites -- All DOE Office Websites (Extended Search)

Nicholas Cox Max Planck Institute for Chemical Energy Conversion, MlheimRuhr, Germany WHEN: May 20, 2014 at 11:00 AM WHERE: Physical Sci C-101 Abstract EPR spectroscopy...

222

Initializing Decadal Climate Predictions with the GECCO Oceanic Synthesis: Effects on the North Atlantic  

Science Journals Connector (OSTI)

This study aims at improving the forecast skill of climate predictions through the use of ocean synthesis data for initial conditions of a coupled climate model. For this purpose, the coupled model of the Max Planck Institute (MPI) for ...

Holger Pohlmann; Johann H. Jungclaus; Armin Khl; Detlef Stammer; Jochem Marotzke

2009-07-01T23:59:59.000Z

223

TeV Astrophysics Constraints on Planck Scale Lorentz Violation  

E-Print Network (OSTI)

We analyze observational constraints from TeV astrophysics on Lorentz violating nonlinear dispersion for photons and electrons without assuming any a priori equality between the photon and electron parameters. The constraints arise from thresholds for vacuum Cerenkov radiation, photon decay and photo-production of electron-positron pairs. We show that the parameter plane for cubic momentum terms in the dispersion relations is constrained to an order unity region in Planck units. We find that the threshold configuration can occur with an asymmetric distribution of momentum for pair creation, and with a hard photon for vacuum Cerenkov radiation.

Ted Jacobson; Stefano Liberati; David Mattingly

2002-09-24T23:59:59.000Z

224

The use and misuse of V c,max in Earth System Models  

Science Journals Connector (OSTI)

Earth System Models (ESMs) aim to project global change....V c,max, is a key parameter in the FvCB model. This study investigated the derivation of the values of V c,max used to re...

Alistair Rogers

2014-02-01T23:59:59.000Z

225

Sugar++: A SAT-Based MAX-CSP/COP Solver Tomoya Tanjo1  

E-Print Network (OSTI)

Sugar++: A SAT-Based MAX-CSP/COP Solver Tomoya Tanjo1 , Naoyuki Tamura2 , and Mutsunori Banbara2 1 describes some features of Sugar++, a SAT-based MAX- CSP/COP solver entering the Third International CSP Solver Competition. In our approach, a MAX-CSP is translated into a Constraint Optimization Problem (COP

Banbara, Mutsunori

226

DOE FY10_Svc_Cont_Inv 122910 v2 MAX.xlsx | Department of Energy  

Energy Savers (EERE)

DOE FY10SvcContInv 122910 v2 MAX.xlsx DOE FY10SvcContInv 122910 v2 MAX.xlsx DOE FY10SvcContInv 122910 v2 MAX.xlsx More Documents & Publications Service Contract Inventory...

227

An Approximation Algorithm for MAX DICUT with Given Sizes of Parts  

E-Print Network (OSTI)

function w : E(G) ! R+ , the maximum directed cut problem (max dicut) is that of #12;nding a directed cut ? weight function w : E(G) ! R+ , the maximum directed cut problem (max dicut) is that of #12;ndingAn Approximation Algorithm for MAX DICUT with Given Sizes of Parts Alexander Ageev #3; Sobolev

Sviridenko, Maxim

228

Computing Reliability Distributions of Windowed Max-log-map (MLM) Detectors : ISI Channels  

E-Print Network (OSTI)

Computing Reliability Distributions of Windowed Max-log-map (MLM) Detectors : ISI Channels Fabian provide exact expressions for both i) the joint distribution of the MLM symbol reliabilities, and ii--detection, intersymbol inteference, max-log- map, probability distribution, reliability I. INTRODUCTION The max

Kavcic, Aleksandar

229

Joint Planck and WMAP Assessment of Low CMB Multipoles  

E-Print Network (OSTI)

The remarkable progress in cosmic microwave background (CMB) studies over past decade has led to the era of precision cosmology in striking agreement with the $\\Lambda$CDM model. However, the lack of power in the CMB temperature anisotropies at large angular scales (low-$\\ell$), as has been confirmed by the recent Planck data also (up to $\\ell=40$), is still an open problem. One can avoid to seek an explanation for this problem by attributing the lack of power to cosmic variance or can look for explanations i.e., different inflationary potentials or initial conditions for inflation to begin with, non-trivial topology, ISW effect etc. Features in the primordial power spectrum (PPS) motivated by the early universe physics has been the most common solution to address this problem. In the present work we also follow this approach and consider a set of PPS which have features and constrain the parameters of those using WMAP 9 year and Planck data employing Markov-Chain Monte Carlo (MCMC) analysis. The prominent fe...

Iqbal, Asif; Souradeep, Tarun; Malik, Manzoor A

2015-01-01T23:59:59.000Z

230

Modeling and Algorithm for DynamicModeling and Algorithm for Dynamic Multi-Objective Max-CSPsMulti-Objective Max-CSPs  

E-Print Network (OSTI)

_n is blow m. ­ e.g. m=5 : No (3,3) / Yes (4,1) #12;Multi-Objective Max-CSP (Properties) For a cost vector RModeling and Algorithm for DynamicModeling and Algorithm for Dynamic Multi-Objective Max-CSPsMulti-Objective Max-CSPs Tenda Okimoto ¹², Tony Rebeiro ³, Maxime Clement and Katsumi Inoue ² ¹ Transdisciplinary

Banbara, Mutsunori

231

Hamilton Eye Institute Neuroscience Institute  

E-Print Network (OSTI)

Care Neonatology & Maternal Fetal Pediatric Heart Institute Steve J. Schwab, MD Musculoskeletal A New of Radiology · Mari Assumes Leadership of OB/GYN city attractioNs Levitt Shell Revived Feature Vision

Cui, Yan

232

Lawrence Berkeley National Laboratory report LBNL-50634 Min-max Identities on Boundaries of  

E-Print Network (OSTI)

in their interiors, then min x bd(K) max f bd(L) f(x) = r0 = min f bd(L) max x bd(K) f(x) . (1) This identity (1) is given by max {r : rL K} = r0 = max {r : rK L } , (2) where K is the polar set of K. Finally, the pairs (x0, f0) R ? (Rn ) that solve both min-max problems in equation (1) have x0 r0 bd(L) bd

233

Theorem: L : Z List. ( p :{Z Z | let m, i = p in max_seg_sum(m; L) max_initseg_sum(i; L)}) L:Z List. (p:{Z Z| let m,i = p in max_seg_sum(m;L) max_initseg_sum(i;L)})  

E-Print Network (OSTI)

(u;u + p2) initseg_sum(r;[u; u1 / v]) )) 2 #12;Theorem: L : Z List. ( p :{Z ? Z | let m, i = p in maxTheorem: L : Z List. ( p :{Z ? Z | let m, i = p in max_seg_sum(m; L) max_initseg_sum(i; L)}) L:Z List. (p:{Z ? Z| let m,i = p in max_seg_sum(m;L) max_initseg_sum(i;L)}) | BY (D 0 THENA Auto) | 1. L

234

A New Approach to Computing Max Flows using Electrical Flows  

E-Print Network (OSTI)

A New Approach to Computing Max Flows using Electrical Flows Yin Tat Lee (MIT) Satish Rao (UC-Kelner-Madry-Spielman-Teng'11]: approximate flow in time Uses electrical flows. 7 #12;Electrical Flows 3 1 S t 8 #12;Electrical Flows Identify Graph with Resistor Network R(e)=1/w(e) 1/3 S t 1 9 #12;Electrical Flows Electrical flow

Rajamani, Sriram K.

235

The Unknown Max Weber: A Note on Missing Translations  

E-Print Network (OSTI)

shabbily treated of all Weber's works, on "sociology and social policy" (1924b), which includes much of his most "empirical" research. Again, until recently (1971) only one small essay (on socialism) had become available to Americans. This sorry condition... of Social Rights and the Western Welfare State: A Weberian Perspective (Uni versity of North Carolina Press, 1981); Ronald Glassman and Vatro Murvar, eds., Max Weber's Political Sociology (Greenwood, 1984); ]urgen Habermas, The Theory of Communicative...

Sica, Alan

1984-01-01T23:59:59.000Z

236

Quantum Institute  

NLE Websites -- All DOE Office Websites (Extended Search)

Quantum Institute Quantum Institute Quantum Institute A new research frontier awaits! Our door is open and we thrive on mutually beneficial partnerships, collaborations that drive innovations and new technologies. Contact Leader Malcolm Boshier (505) 665-8892 Email Two of LANL's most successful quantum technology initiatives: quantum cryptography and the race for quantum computer The area of quantum information, science, and technology is rapidly evolving, with important applications in the areas of quantum cryptography, quantum computing, quantum metrology, and advanced quantum-based sensors, some of which are directly relevant to the Laboratory's national security mission. Mission Foster a vigorous intellectual environment at LANL Define and develop strategic thrusts Target and pursue funding opportunities

237

42 MaxPlanckForschung 4 | 13 Turbulence is omnipresent: it plays an important role during planet formation, mixes fuel and air  

E-Print Network (OSTI)

on aircraft wings or car bodies, for example, is feared because it push- es up the fuel consumption. And tur formation, mixes fuel and air in the cylinder of an engine, but also increases the energy needed for pumps PHENOMENON In our blood vessels, the steady blood flow also switches time and again to turbulent motion

Falge, Eva

238

Planck's quantum-driven integer quantum Hall effect in chaos  

E-Print Network (OSTI)

The integer quantum Hall effect (IQHE) and chaos are commonly conceived as being unrelated. Contrary to common wisdoms, we find in a canonical chaotic system, the kicked spin-$1/2$ rotor, a Planck's quantum($h_e$)-driven phenomenon bearing a firm analogy to IQHE but of chaos origin. Specifically, the rotor's energy growth is unbounded ('metallic' phase) for a discrete set of critical $h_e$-values, but otherwise bounded ('insulating' phase). The latter phase is topological in nature and characterized by a quantum number ('quantized Hall conductance'). The number jumps by unity whenever $h_e$ decreases passing through each critical value. Our findings, within the reach of cold-atom experiments, indicate that rich topological quantum phenomena may emerge from chaos.

Yu Chen; Chushun Tian

2014-09-18T23:59:59.000Z

239

Irreversible Thermodynamics of the Universe: Constraints from Planck Data  

E-Print Network (OSTI)

The present work deals with irreversible Universal thermodynamics. The homogenous and isotropic flat model of the universe is chosen as open thermodynamical system and non-equilibrium thermodynamics comes into picture due to the mechanism of particle creation. For simplicity, entropy flow is considered only due to heat conduction. Further, due to Maxwell-Cattaneo modified Fourier law for non-equilibrium phenomenon, the temperature satisfies damped wave equation instead of heat conduction equation. Validity of generalized second law of thermodynamics (GSLT) has been investigated for Universe bounded by apparent or event horizon with cosmic substrutum as perfect fluid with constant or variable equation of state or interacting dark species. Finally, we have used three Planck data sets to constrain the thermal conductivity \\lambda and the coupling parameter b^2. These constraints must be satisfied in order for GSLT to hold for Universe bounded by apparent or event horizons.

Subhajit Saha; Atreyee Biswas; Subenoy Chakraborty

2014-04-04T23:59:59.000Z

240

Planck Scale Cosmology and Asymptotic Safety in Resummed Quantum Gravity  

E-Print Network (OSTI)

In Weinberg's asymptotic safety approach, a finite dimensional critical surface for a UV stable fixed point generates a theory of quantum gravity with a finite number of physical parameters. We argue that, in an extension of Feynman's original formulation of the theory, we recover this fixed-point UV behavior from an exact re-arrangement of the respective perturbative series. Our results are consistent with the exact field space Wilsonian renormalization group results of Reuter {\\it et al.} and with recent Hopf- algebraic Dyson-Schwinger renormalization theory results of Kreimer. We obtain the first "first principles" predictions of the dimensionless gravitational and cosmological constants and our results support the Planck scale cosmology of Bonanno and Reuter. We conclude with an estimate for the currently observed value of the cosmological constant.

B. F. L. Ward

2010-12-13T23:59:59.000Z

Note: This page contains sample records for the topic "max planck institute" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


241

Probing Planck scale physics with IceCube  

Science Journals Connector (OSTI)

Neutrino oscillations can be affected by decoherence induced e.g. by Planck scale suppressed interactions with the space-time foam predicted in some approaches to quantum gravity. We study the prospects for observing such effects at IceCube, using the likely flux of TeV antineutrinos from the Cygnus spiral arm. We formulate the statistical analysis for evaluating the sensitivity to quantum decoherence in the presence of the background from atmospheric neutrinos, as well as from plausible cosmic neutrino sources. We demonstrate that IceCube will improve the sensitivity to decoherence effects of O(E2/MPl) by 17 orders of magnitude over present limits and, moreover, that it can probe decoherence effects of O(E3/MPl2) which are well beyond the reach of other experiments.

Luis A. Anchordoqui; Haim Goldberg; M. C. Gonzalez-Garcia; Francis Halzen; Dan Hooper; Subir Sarkar; Thomas J. Weiler

2005-09-28T23:59:59.000Z

242

Hypersonic expansion of the Fokker--Planck equation  

SciTech Connect

A systematic study of the hypersonic limit of a heavy species diluted in a much lighter gas is made via the Fokker--Planck equation governing its velocity distribution function. In particular, two different hypersonic expansions of the Fokker--Planck equation are considered, differing from each other in the momentum equation of the heavy gas used as the basis of the expansion: in the first of them, the pressure tensor is neglected in that equation while, in the second expansion, the pressure tensor term is retained. The expansions are valid when the light gas Mach number is O(1) or larger and the difference between the mean velocities of light and heavy components is small compared to the light gas thermal speed. They can be applied away from regions where the spatial gradient of the distribution function is very large, but it is not restricted with respect to the temporal derivative of the distribution function. The hydrodynamic equations corresponding to the lowest order of both expansions constitute two different hypersonic closures of the moment equations. For the subsequent orders in the expansions, closed sets of moment equations (hydrodynamic equations) are given. Special emphasis is made on the order of magnitude of the errors of the lowest-order hydrodynamic quantities. It is shown that if the heat flux vanishes initially, these errors are smaller than one might have expected from the ordinary scaling of the hypersonic closure. Also it is found that the normal solution of both expansions is a Gaussian distribution at the lowest order.

Fernandez-Feria, R.

1989-02-01T23:59:59.000Z

243

RATAN-600 and PLANCK Mission: new results after First General Meeting  

E-Print Network (OSTI)

We present activity at RATAN-600 connected with future PLANCK mission. It includes special radio telescope upgrading, multi-frequencies observations in the 0.6GHz-30GHz band with 40 channels, new results, connected with synchrotron, spinning dust and polarized Galaxy emission at small scales. Much lower limits were found than expected before the First Planck meeting. New deep sub-mJy survey of the 100 sq.deg. field at cm. waves demonstrated, that NVSS objects will dominate at LFI frequencies, and new, invisible by NVSS population will be below PLANCK sensitivity limit with only few exceptions. Preparation to the next generation experiments, connected with PLANCK mission we describe as well. They include high l polarization, SZ- blind survey, and test observations of the cosmological highly redshifted lines at small scales.

Yu. Parijskij; I. Novikov

2004-02-17T23:59:59.000Z

244

Forecasting neutrino masses from galaxy clustering in the Dark Energy Survey combined with the Planck measurements  

Science Journals Connector (OSTI)

......from galaxy clustering in the Dark Energy Survey combined with the Planck measurements...photometric redshift shells of the Dark Energy Survey (DES) over a volume of 20...in the photometric redshift survey Dark Energy Survey (DES), combined with......

Ofer Lahav; Angeliki Kiakotou; Filipe B. Abdalla; Chris Blake

2010-06-11T23:59:59.000Z

245

Holographic Noise in Michelson Interferometers: A Direct Experimental Probe of Unification at the Planck Scale  

ScienceCinema (OSTI)

Classical spacetime and quantum mass-energy form the basis of all of physics. They become inconsistent at the Planck scale, 5.4 times 10^{-44} seconds, which may signify a need for reconciliation in a unified theory. Although proposals for unified theories exist, a direct experimental probe of this scale, 16 orders of magnitude above Tevatron energy, has seemed hopelessly out of reach. However in a particular interpretation of holographic unified theories, derived from black hole evaporation physics, a world assembled out of Planck-scale waves displays effects of unification with a new kind of uncertainty in position at the Planck diffraction scale, the geometric mean of the Planck length and the apparatus size. In this case a new phenomenon may measurable, an indeterminacy of spacetime position that appears as noise in interferometers. The colloquium will discuss the theory of the effect, and our plans to build a holographic interferometer at Fermilab to measure it.

Craig Hogan

2010-01-08T23:59:59.000Z

246

New constraints on coupled dark energy from the Planck satellite experiment  

Science Journals Connector (OSTI)

We present new constraints on coupled dark energy from the recent measurements of the cosmic microwave background anisotropies from the Planck satellite mission. We found that a coupled dark energy model is fully compatible with the Planck measurements, deriving a weak bound on the dark matterdark energy coupling parameter ?=-0.49-0.31+0.19 at 68%C.L. Moreover if Planck data are fitted to a coupled dark energy scenario, the constraint on the Hubble constant is relaxed to H0=72.1-2.3+3.2??km/s/Mpc, solving the tension with the Hubble Space Telescope (HST) value. We show that a combined PLANCK+HST analysis provides significant evidence for coupled dark energy finding a nonzero value for the coupling parameter ?, with -0.90Survey, the Sloan Digital Sky Survey and the Baron Oscillation Spectroscopic Survey.

Valentina Salvatelli; Andrea Marchini; Laura Lopez-Honorez; Olga Mena

2013-07-24T23:59:59.000Z

247

Design and Analysis of Stochastic Dynamical Systems with Fokker-Planck Equation  

E-Print Network (OSTI)

Monte-Carlo techniques. Spectral analysis of the discretized Fokker- Planck operator, followed by spurious mode rejection is employed to construct a new semi-analytical algorithm to obtain near real-time approximations of transient FPE response of high...

Kumar, Mrinal

2011-02-22T23:59:59.000Z

248

text in "Max kWh" fields | OpenEI Community  

Open Energy Info (EERE)

text in "Max kWh" fields text in "Max kWh" fields Home > Groups > Utility Rate Ewilson's picture Submitted by Ewilson(51) Contributor 3 January, 2013 - 09:57 I noticed that a warning appears if you enter text only in the "Max kWh" field. However an entry like "text 1234" does not give a warning. I think it should as we are trying to prevent users from writing "less than X", "greater than Y", etc. and follow the intention of the "Max kWh" field. Also there should be a warning if the number of "Max kWh" fields with values is not correct--it should be one less than the number of charge fields with values. There should also be a warning if the "Max kWh" fields do not increase from top to bottom. These checks on input would save lots of trouble when using json files for

249

Deciding Unambiguity and Sequentiality from a Finitely Ambiguous MaxPlus Automaton  

E-Print Network (OSTI)

­anneau max­plus. Le r??esultat principal est le suivant : on peut d??ecider si une s??erie reconnue par unDeciding Unambiguity and Sequentiality from a Finitely Ambiguous Max­Plus Automaton Ines Klimann with weights in the max­plus semiring are considered. The main result is: it is decidable whether a series

Fondements et Applications, Université Paris 7

250

Reducible spectral theory with applications to the robustness of matrices in max algebra  

E-Print Network (OSTI)

.Butkoviµcy R.A.Cuninghame-Greenz S.Gaubertx July 25, 2008 Abstract Let a b = max(a; b) and a b = a + b for a; b 2 R := R [ f 1g. By max-algebra we understand the analogue of linear algebra developed for the pair: The max-algebraic eigenvalue-eigenvector problem is the following: Given A 2 R n n , ...nd all 2 R and x 2

Butkovic, Peter

251

CSR EXPANSIONS OF MATRIX POWERS IN MAX ALGEBRA SERGEi SERGEEV AND HANS SCHNEIDER  

E-Print Network (OSTI)

that for t 3n2, the powers At can be expanded in max-algebraic sums of terms of the form CStR, where C and R the max-times semiring Rmax,? which is the set of nonnegative numbers R+ equipped with the operations-algebraic powers of nonnegative matrices, the main object of our study. The max-plus semiring Rmax,+ = (R

Schneider, Hans

252

Non-linear programs with max-linear constraints: A heuristic approach  

E-Print Network (OSTI)

5, 2009 Abstract Let a b = max(a, b) and a b = a + b for a, b R and extend the pair of operations = max(a, b) and a b = a + b for a, b R and extend the pair of operations to matrices and vectors bkj = maxk(aik + bkj) for all i, j. Also, if R then A = ( aij). Max-algebra has been studied

Butkovic, Peter

253

MSC-E Technical Report 1/2003 Intercomparison Study of Numerical Models for  

E-Print Network (OSTI)

-Planck-Strasse 1, D-21502 Geesthacht Germany fax: 49 41 52 87 23 66 e-mail: ebinghaus@dvmc10.gkss.de Ilia ILYIN - Research Centre, Institute of Hydrophysics Max-Planck-Strasse 1 D-21502 Geesthacht GERMANY tel: 49 41 52 87

254

Reconciliation of High Energy Scale Models of Inflation with Planck  

E-Print Network (OSTI)

The inflationary cosmology paradigm is very successful in explaining the CMB anisotropy to the percent level. Besides the dependence on the inflationary model, the power spectra, spectral tilt and non-Gaussianity of the CMB temperature fluctuations also depend on the initial state of inflation. Here, we examine to what extent these observables are affected by our ignorance in the initial condition for inflationary perturbations, due to unknown new physics at a high scale $M$. For initial states that satisfy constraints from backreaction, we find that the amplitude of the power spectra could still be significantly altered, while the modification in bispectrum remains small. For such initial states, $M$ has an upper bound of a few tens of $H$, with $H$ being the Hubble parameter during inflation. We show that for $M\\sim 20 H$, such initial states always (substantially) suppress the tensor to scalar ratio. In particular we show that a general choice of initial conditions can satisfactorily reconcile the simple $1/2 m^2 \\phi^2$ chaotic model with the Planck data.

Amjad Ashoorioon; Konstantinos Dimopoulos; M. M. Sheikh-Jabbari; Gary Shiu

2014-02-06T23:59:59.000Z

255

Axion cold dark matter: status after Planck and BICEP2  

E-Print Network (OSTI)

We investigate the axion dark matter scenario (ADM), in which axions account for all of the dark matter in the Universe, in light of the most recent cosmological data. In particular, we use the Planck temperature data, complemented by WMAP E-polarization measurements, as well as the recent BICEP2 observations of B-modes. Baryon Acoustic Oscillation data, including those from the Baryon Oscillation Spectroscopic Survey, are also considered in the numerical analyses. We find that, in the minimal ADM scenario, the full dataset implies that the axion mass m_a = 82.2 pm 1.1 {\\mu}eV (corresponding to the Peccei-Quinn symmetry being broken at a scale f_a = (7.54 pm 0.10)*10^10 GeV), or m_a = 76.6 pm 2.6 {\\mu}eV (f_a = (8.08 pm 0.27)*10^10 GeV) when we allow for a non- standard effective number of relativistic species Neff . We also find a 2{\\sigma} preference for Neff > 3.046. The limit on the sum of neutrino masses is Sum m_{\

E. Di Valentino; E. Giusarma; M. Lattanzi; A. Melchiorri; O. Mena

2014-05-08T23:59:59.000Z

256

California Institute of Technology  

NLE Websites -- All DOE Office Websites (Extended Search)

California Institute of Technology o Ivan Celanovic, Principal Research Scientist, Massachusetts Institute of Technology o Geoffrey Kinsey, Director, Photovoltaic...

257

Institute of Design Institute of Design  

E-Print Network (OSTI)

Institute of Design Institute of Design 350 N. LaSalle St. Chicago, IL 60610 312.595.4900 design The Institute of Design has continuously explored emerg- ing ideas about how design interacts with society languages and use of new media and material. The school was renamed the Institute of Design (ID) in 1944

Heller, Barbara

258

CURRICULUM VITAE Svante Pbo  

E-Print Network (OSTI)

of Munich, Germany. 1997- Director, Max-Planck-Institute for Evolutionary Anthropology, Leipzig, Germany. 1999- Honorary Professor of Genetics and Evolutionary Biology, University of Leipzig, Germany. 2003 Lecture, Heidelberg, Germany. 1998 Member, Academia Europaea. Max Delbrück Medal, Berlin, Germany. 1999

Pääbo, Svante

259

MiniMAX: A Compact, Portable X-Ray System For Field Inspection  

NLE Websites -- All DOE Office Websites (Extended Search)

MiniMAX: A Compact, Portable X-Ray System For Field Inspection MiniMAX: A Compact, Portable X-Ray System For Field Inspection MiniMAX: A Compact, Portable X-Ray System For Field Inspection MiniMAX takes x-ray images that are as detailed or even better than conventional hospital systems. However, unlike such systems, MiniMAX is easy to use, portable, lightweight, and inexpensive. MiniMAX takes advantage of the form factor of x-ray film, the physics of computed radiography (CR), and the compact technology of digital radiography (DR) panels to implement the benefits of each in a very simple, reliable, and compact system. July 11, 2013 Complete , 6.5lb, MiniMAX portable radiography system including Leica M9 camera, Jenoptik lens, JDSU dichroic filter, LED flash, CsBr storage phosphor, and 57-Co source. Complete, 6.5lb, MiniMAX portable radiography system including Leica M9

260

A characterisation of the complexity of forbidding subproblems in binary Max-CSP  

Science Journals Connector (OSTI)

Tractable classes of binary CSP and binary Max-CSP have recently been discovered by studying classes of instances defined by excluding subproblems. In this paper we characterise the complexity of all classes of binary Max-CSP instances defined by forbidding ...

Martin C. Cooper; Guillaume Escamocher; Stanislav ivn

2012-10-01T23:59:59.000Z

Note: This page contains sample records for the topic "max planck institute" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


261

The use and misuse of Vc,max in Earth System Models Alistair Rogers  

E-Print Network (OSTI)

REVIEW The use and misuse of Vc,max in Earth System Models Alistair Rogers Received: 18 November Dordrecht (outside the USA) 2013 Abstract Earth System Models (ESMs) aim to project global change. Central Á Vc,max Á Leaf nitrogen Á Earth System Models Introduction The primary goal of Earth System Models

Rogers, Alistair

262

Visualization in max algebra: An application of diagonal scaling of matrices.  

E-Print Network (OSTI)

Visualization in max algebra: An application of diagonal scaling of matrices. Hans Schneider Schneider with some results from joint work with Peter Butkovic and Sergei SergeevVisualization in max > 0 Definition path in G(A) i(0) i(1) · · · i(k) (i, j), ((i, j; r)) path from i to j (length r

Schneider, Hans

263

An 0.5-Approximation Algorithm for MAX DICUT with Given Sizes of Parts  

E-Print Network (OSTI)

An 0.5-Approximation Algorithm for MAX DICUT with Given Sizes of Parts Alexander Ageev Refael Hassin Maxim Sviridenko Abstract Given a directed graph G and an edge weight function w : E(G) R+, the maximum directed cut problem (max dicut) is that of finding a directed cut (X) with maximum total weight

Atkinson, Katie

264

Journal de la Socit Franaise de Statistique Spatial extremes: Max-stable processes at work  

E-Print Network (OSTI)

and conditional simulation of max-stable processes. The paper ends with the modeling of extreme wind gustsSubmission Journal de la Société Française de Statistique Spatial extremes: Max-stable processes many developments to the functional extreme value theory have been made during the last decades

Ribatet, Mathieu

265

Planck early results: Spectral energy distributions and radio continuum spectra of northern extragalactic radio sources  

E-Print Network (OSTI)

Spectral energy distributions (SEDs) and radio continuum spectra are presented for a northern sample of 104 extragalactic radio sources, based on the Planck Early Release Compact Source Catalog (ERCSC) and simultaneous multifrequency data. The nine Planck frequencies, from 30 to 857 GHz, are complemented by a set of simultaneous observations ranging from radio to gamma-rays. This is the first extensive frequency coverage in the radio and millimetre domains for an essentially complete sample of extragalactic radio sources, and it shows how the individual shocks, each in their own phase of development, moving in the relativistic jet, shape the radio spectra. The SEDs presented in this paper were fitted with second and third degree polynomials to estimate the frequencies of the synchrotron and inverse Compton (IC) peaks, and the spectral indices of low and high frequency radio data, including the Planck ERCSC data, were calculated. SED modelling methods are discussed, with an emphasis on proper, physical modelli...

Aatrokoski, J; Aghanim, N; Aller, H D; Aller, M F; Angelakis, E; Arnaud, M; Ashdown, M; Aumont, J; Baccigalupi, C; Balbi, A; Banday, A J; Barreiro, R B; Bartlett, J G; Battaner, E; Benabed, K; Benot, A; Berdyugin, A; Bernard, J -P; Bersanelli, M; Bhatia, R; Bonaldi, A; Bonavera, L; Bond, J R; Borrill, J; Bouchet, F R; Bucher, M; Burigana, C; Burrows, D N; Cabella, P; Capalbi, M; Cappellini, B; Cardoso, J -F; Catalano, A; Cavazzuti, E; Cayn, L; Challinor, A; Chamballu, A; Chary, R -R; Chiang, L -Y; Christensen, P R; Clements, D L; Colafrancesco, S; Colombi, S; Couchot, F; Coulais, A; Cutini, S; Cuttaia, F; Danese, L; Davies, R D; Davis, R J; de Bernardis, P; de Gasperis, G; de Rosa, A; de Zotti, G; Delabrouille, J; Delouis, J -M; Dickinson, C; Dole, H; Donzelli, S; Dor, O; Drl, U; Douspis, M; Dupac, X; Efstathiou, G; Enlin, T A; Finelli, F; Forni, O; Frailis, M; Franceschi, E; Fuhrmann, L; Galeotta, S; Ganga, K; Gargano, F; Gasparrini, D; Gehrels, N; Giard, M; Giardino, G; Giglietto, N; Giommi, P; Giordano, F; Giraud-Hraud, Y; Gonzlez-Nuevo, J; Grski, K M; Gratton, S; Gregorio, A; Gruppuso, A; Harrison, D; Henrot-Versill, S; Herranz, D; Hildebrandt, S R; Hivon, E; Hobson, M; Holmes, W A; Hovest, W; Hoyland, R J; Huffenberger, K M; Jaffe, A H; Juvela, M; Keihnen, E; Keskitalo, R; King, O; Kisner, T S; Kneissl, R; Knox, L; Krichbaum, T P; Kurki-Suonio, H; Lagache, G; Lhteenmki, A; Lamarre, J -M; Lasenby, A; Laureijs, R J; Lavonen, N; Lawrence, C R; Leach, S; Leonardi, R; Len-Tavares, J; Linden-V\\ornle, M; Lindfors, E; Lpez-Caniego, M; Lubin, P M; Macas-Prez, J F; Maffei, B; Maino, D; Mandolesi, N; Mann, R; Maris, M; Martnez-Gonzlez, E; Masi, S; Massardi, M; Matarrese, S; Matthai, F; Max-Moerbeck, W; Mazziotta, M N; Mazzotta, P; Melchiorri, A; Mendes, L; Mennella, A; Michelson, P F; Mingaliev, M; Mitra, S; Miville-Deschnes, M -A; Moneti, A; Monte, C; Montier, L; Morgante, G; Mortlock, D; Munshi, D; Murphy, A; Naselsky, P; Natoli, P; Nestoras, I; Netterfield, C B; Nieppola, E; Nilsson, K; N\\orgaard-Nielsen, H U; Noviello, F; Novikov, D; Novikov, I; O'Dwyer, I J; Osborne, S; Pajot, F; Partridge, B; Pasian, F; Patanchon, G; Pavlidou, V; Pearson, T J; Perdereau, O; Perotto, L; Perri, M; Perrotta, F; Piacentini, F; Piat, M; Plaszczynski, S; Platania, P; Pointecouteau, E; Polenta, G; Ponthieu, N; Poutanen, T; Przeau, G; Prunet, S; Puget, J -L; Rachen, J P; Rain, S; Reach, W T; Readhead, A; Rebolo, R; Reeves, R; Reinecke, M; Reinthal, R; Renault, C; Ricciardi, S; Richards, J; Riller, T; Riquelme, D; Ristorcelli, I; Rocha, G; Rosset, C; Rowan-Robinson, M; Rubi\; Rusholme, B; Saarinen, J; Sandri, M; Savolainen, P; Scott, D; Seiffert, M D; Sievers, A; Sillanp, A; Smoot, G F; Sotnikova, Y; Starck, J -L; Stevenson, M; Stivoli, F; Stolyarov, V; Sudiwala, R; Sygnet, J -F; Takalo, L; Tammi, J; Tauber, J A; Terenzi, L; Thompson, D J; Toffolatti, L; Tomasi, M; Tornikoski, M; Torre, J -P; Tosti, G; Tramacere, A; Tristram, M; Tuovinen, J; Trler, M; Turunen, M; Umana, G; Ungerechts, H; Valenziano, L; Valtaoja, E; Varis, J; Verrecchia, F; Vielva, P; Villa, F; Vittorio, N; Wandelt, B D; Wu, J; Yvon, D; Zacchei, A; Zensus, J A; Zhou, X; Zonca, A

2011-01-01T23:59:59.000Z

266

Boltzmann-Fokker-Planck calculations using standard discrete-ordinates codes  

SciTech Connect

The Boltzmann-Fokker-Planck (BFP) equation can be used to describe both neutral and charged-particle transport. Over the past several years, the author and several collaborators have developed methods for representing Fokker-Planck operators with standard multigroup-Legendre cross-section data. When these data are input to a standard S/sub n/ code such as ONETRAN, the code actually solves the Boltzmann-Fokker-Planck equation rather than the Boltzmann equation. This is achieved wihout any modification to the S/sub n/ codes. Because BFP calculations can be more demanding from a numerical viewpoint than standard neutronics calculations, we have found it useful to implement new quadrature methods ad convergence acceleration methods in the standard discrete-ordinates code, ONETRAN. We discuss our BFP cross-section representation techniques, our improved quadrature and acceleration techniques, and present results from BFP coupled electron-photon transport calculations performed with ONETRAN. 19 refs., 7 figs.

Morel, J.E.

1987-01-01T23:59:59.000Z

267

Planck Scale Induced Speed of Sound in a Trapped Bose-Einstein Condensate  

E-Print Network (OSTI)

In the present work, we analyze the corrections caused by an anomalous dispersion relation, suggested in several quantum gravity models, upon the speed of sound in a weakly interacting Bose--Einstein Condensate, trapped in a potential of the form $V(r)\\sim r^{2}$. We show that the corresponding ground state energy and consequently, the associated speed of sound, present corrections respect to the usual case, which may be used to explore the sensitivity to Planck--scale effects on these relevant properties associated with the condensate. Indeed, we stress that this type of macroscopic bodies may be more sensitive, under certain conditions, to Planck--scale manifestations than its constituents. In addition, we prove that the inclusion of a trapping potential, together with many--body contributions, improves the sensitivity to Planck--scale signals, compared to the homogeneous system.

E. Castellanos; J. I. Rivas; V. Domnguez-Rocha

2014-07-11T23:59:59.000Z

268

Intracellular Measurements of Spatial Integration and the MAX Operation in Complex Cells of the Cat Primary Visual Cortex  

E-Print Network (OSTI)

Intracellular Measurements of Spatial Integration and the MAX Operation in Complex Cells of the Cat. Intracellular measurements of spatial integration and the MAX operation in complex cells of the cat primary by a maximum operation (MAX)-like computation, as suggested by Riesenhuber and Poggio's model of object

Riesenhuber, Maximilian

269

The Singular-Value Decomposition in the Extended Max Algebra* Bart De Schutter+ and Bart De Moor*  

E-Print Network (OSTI)

numbers and the extended max algebra to define the sing&r-value decomposition of a matrix in the extendedThe Singular-Value Decomposition in the Extended Max Algebra* Bart De Schutter+ and Bart De Moor ABSTRACT First we establish a connection between the field of the real numbers and the extended max algebra

270

A summary of the Planck constant measurements using a watt balance with a superconducting solenoid at NIST  

E-Print Network (OSTI)

Researchers at the National Institute of Standards and Technology have been using a watt balance, NIST-3, to measure the Planck constant $h$ for over ten years. Two recently published values disagree by more than one standard uncertainty. The motivation for the present manuscript is twofold. First, we correct the latest published number to take into account a recently discovered systematic error in mass dissemination at the Bureau International des Poids et Mesures (BIPM). Second, we provide guidance on how to combine the two numbers into one final result. In order to adequately reflect the discrepancy, we added an additional systematic uncertainty to the published uncertainty budgets. The final value of $h$ measured with NIST-3 is $h = 6.626\\,069\\,36(37)\\times 10^{-34}\\,\\mbox{J\\,s}$. This result is $77(57) \\times 10^{-9}$ fractionally higher than $h_{\\mathrm{90}}$. Each number in parentheses gives the value of the standard uncertainty in the last two digits of the respective value and $h_{\\mathrm{90}}$ is th...

Schlamminger, S; Haddad, D; Newell, D B; Seifert, F; Chao, L S; Liu, R; Williams, E R; Pratt, J R

2015-01-01T23:59:59.000Z

271

Transient finite element analysis of electric double layer using Nernst-Planck-Poisson equations with a modified stern layer  

E-Print Network (OSTI)

Finite element analysis of electric double layer capacitors using a transient nonlinear Nernst-Planck-Poisson (NPP) model and Nernst-Planck-Poisson-modified Stern layer (NPPMS) model are presented in 1D and 2D. The NPP model provided unrealistic ion...

Lim, Jong Il

2007-04-25T23:59:59.000Z

272

Entropy production in irreversible systems described by a Fokker-Planck equation Tnia Tom and Mrio J. de Oliveira  

E-Print Network (OSTI)

Entropy production in irreversible systems described by a Fokker-Planck equation Tânia Tomé and the entropy production in nonequilibrium interacting particle systems described by a Fokker-Planck equation equilibrium there will be no production of entropy. A non- equilibrium thermodynamic system in the stationary

de Oliveira, Mário José

273

Development of the Schrodinger equation for attosecond laser pulse interaction with Planck gas  

E-Print Network (OSTI)

The creation of the new particles by the interaction of the ultrarelativistic ions,from Large Hadron Collider(LHC), and attosecond laser pulse open new possibilities for laser physicists community .In this paper we propose the hyperbolic Schr\\"odinger equation (HSE) for gas of the "classical" particles "i.e. particles with mass= Planck mass We discuss the inclusion of the gravity to the HSE The solution of the HSE for a particle in a box is obtained. It is shown that for particles with m greater than Mp the energy spectrum is independent of the mass of particle. Key words: attosecond laser pulses, Schrodinger equation, Planck particles, thermal processes

M. Kozlowski; J. Marciak-Kozlowska; Josef Pilsudski

2011-09-04T23:59:59.000Z

274

Emergent gravity by tuning the effective Planck length in Bose-Einstein Condensate  

E-Print Network (OSTI)

We show that at lowest energy nonlocal interactions, the tuning of s-wave scattering length can enable a systematic control over the quantum pressure term in a Bose-Einstein condensate (BEC). We derive the equation for the massless free excitations in an analogue curved space-time by controlling the effective Planck length. Our controlled derivation indicates a breakdown of this dynamics at length scales comparable to effective Planck length. We also specify the correction that one has to take into account at a larger length scale in a flat space-time due to the emergent gravity at intermediate length scales.

Sarkar, Supratik

2014-01-01T23:59:59.000Z

275

Higher order mixed moment approximations for the Fokker-Planck equation in one space dimension  

E-Print Network (OSTI)

We study mixed-moment models (full zeroth moment, half higher moments) for a Fokker-Planck equation in one space dimension. Mixed-moment minimum-entropy models are known to overcome the zero net-flux problem of full-moment minimum entropy Mn models. Realizability theory for these mixed moments of arbitrary order is derived, as well as a new closure, which we refer to as Kershaw closures. They provide non-negative distribution functions combined with an analytical closure. Numerical tests are performed with standard first-order finite volume schemes and compared with a finite-difference Fokker-Planck scheme.

Florian Schneider; Graham Alldredge; Martin Frank; Axel Klar

2014-05-21T23:59:59.000Z

276

Supervised Learning of Image Restoration with Convolutional Networks Viren Jain1  

E-Print Network (OSTI)

Institute of Technology, Cambridge, MA, USA 2 Howard Hughes Medical Institute, Cambridge, MA, USA 3 Biomedical Optics, Max Planck Institute for Medical Research, Heidelberg, Germany Abstract Convolutional, the images are clean enough to be used for segmentation, whereas the other approaches fail in this respect

Gabrieli, John

277

5, 10751099, 2014 Uncertainty in crop  

E-Print Network (OSTI)

Resources and Energy Directorate, Oslo, Norway 16 International Institute for Applied System Analysis, New York, USA 24 Institute for Sustainable Economic Development, Vienna, Austria 25 Max Planck of Bonn, Bonn, Germany 28 Santa Fe Institute, Santa Fe, New Mexico, USA Received: 28 July 2014 ­ Accepted

Levermann, Anders

278

The Excellence Initiative of the German Federal Ministry of Education and Research and the German Research Foundation  

E-Print Network (OSTI)

Mikrotechnik Mainz, Max-Planck-Institute for Polymer Research, Fraunhofer-Institute for Structural Du- rability and System Reliability, Deutsches Kunststoff-Institut). The Center of Smart Interfaces focuses on phase of Smart Interfaces Experimental Interface Physics #12;Innovative Environment Workforce: 1 Research group

Haller-Dintelmann, Robert

279

The Excellence Initiative of the German Federal Ministry of Education and Research and the German Research Foundation  

E-Print Network (OSTI)

Mikrotechnik Mainz, Max-Planck-Institute for Polymer Research, Fraunhofer-Institute for Structural Du- rability and System Reliability, Deutsches Kunststoff-Institut). The Center of Smart Interfaces focuses on phase of innovative combustion concepts and characterisation of components in energy technologies ­ Numerical

Haller-Dintelmann, Robert

280

Institute of Design Institute of Design  

E-Print Network (OSTI)

Institute of Design Institute of Design 350 N. LaSalle St. Chicago, IL 60610 312.595.4900 main 312.595.4906 graduate study information 312.595.4901 fax design@id.iit.edu www.id.iit.edu Dean: Patrick F. Whitney The Institute of Design (ID) is defined by a legacy of experimentation joined with unique academic programs

Heller, Barbara

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We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


281

Southern Research Institute Visit  

NLE Websites -- All DOE Office Websites (Extended Search)

initiates collaboration between Southern Research Institute(SRI) and LSU CAMD hosted visitors from the Southern Research Institute in Birmingham, Alabama, and researchers from LSU...

282

Consistency tests for Planck and WMAP in the low multipole domain  

SciTech Connect

Recently, full sky maps from Planck have been made publicly available. In this paper, we do consistency tests for the three Planck CMB sky maps. We assume that the difference between two maps represents the contributions from systematics, noise, foregrounds and other sources, and that a precise representation of the Cosmic Microwave Background should be uncorrelated with it. We investigate the cross correlation in pixel space between the difference maps and the various Planck maps and find no significant correlations, in comparison to 10000 random Gaussian simulated maps. Additionally we investigate the difference map between the WMAP ILC 9 year map and the ILC 7 year map. We perform cross correlations between this difference map, and the ILC9 and ILC7, and find significant correlations only for the ILC9, at more than the 99.99% level. Likewise, a comparison between the Planck NILC map and the WMAP ILC9 map, shows a strong correlation for the ILC9 map with the difference map, also at more than the 99.99% level. Thus the ILC9 appears to be more contaminated than the ILC7, which should be taken into consideration when using WMAP maps for cosmological analyses.

Frejsel, A.; Hansen, M.; Liu, H., E-mail: frejsel@nbi.dk, E-mail: kirstejn@nbi.dk, E-mail: liuhao@nbi.dk [Niels Bohr Institute and Discovery Center, Blegdamsvej 17, 2100 Copenhagen (Denmark)

2013-06-01T23:59:59.000Z

283

Poisson-Nernst-Planck systems for narrow tubular-like membrane and Bixiang Wang  

E-Print Network (OSTI)

membrane channels, transport of holes and electrons in semiconductors (see, e.g., [1, 2, 24, 4, 6, 7, 8, 17, 25]). In the context of ion flow through membrane channels, it is physicallyPoisson-Nernst-Planck systems for narrow tubular-like membrane channels Weishi Liu and Bixiang Wang

Liu, Weishi

284

Ground states of 2d J Ising spin glasses via stationary FokkerPlanck sampling  

E-Print Network (OSTI)

of the individual variables that enter the cost function. Moreover, the influence of the cost function on the search disciplines [1, 2]. Among those, stochastic search strategies like e.g. simulated annealing [3, 4], parallel function. Langevin dynamics can also be cast in terms of a Fokker­Planck equation as evolution equation

Peinke, Joachim

285

Planck CMB Anomalies: Astrophysical and Cosmological Foregrounds and the Curse of Masking  

E-Print Network (OSTI)

Understanding the origin of reported anomalies in the CMB is fundamental to either validate the standard model of cosmology or to explore new physics. Their confirmation with Planck data suggests they are not due to a problem in WMAP or Planck data. We investigate three other possible issues: 1) the trade-off between minimising systematics due to foreground contamination (with a conservative mask) and minimising systematics due to masking, 2) astrophysical foregrounds (the kinetic Doppler quadrupole and kinetic Sunyaev-Zel'dovich effect), and 3) secondary cosmological signals (the integrated Sachs-Wolfe effect). We address the masking issue by considering new procedures that use both WMAP and Planck to produce higher quality full-sky maps using the sparsity methodology (LGMCA maps). We show the impact of masking is dominant over that of residual foregrounds, and the LGMCA full-sky maps can be used without further processing to study anomalies. We consider four official Planck PR1 and two LGMCA CMB maps. Analy...

Rassat, A; Paykari, P; Sureau, F; Bobin, J

2014-01-01T23:59:59.000Z

286

Tunnel effect and symmetries for Kramers Fokker-Planck type operators  

E-Print Network (OSTI)

- values. R´esum´e Nous ´etudions des op´erateurs de type Kramers-Fokker-Planck dans la lim- ite semi are real and exponentially small, and establish the complete semiclassical asymptotics for these eigen ´etablissons leur asymp- totique semi-classique compl`ete. Contents 1 Introduction 3 2 Review of some results

Hérau, Frédéric

287

SpeeDP: A new algorithm to compute the SDP relaxations of Max ...  

E-Print Network (OSTI)

Oct 15, 2010 ... matrix A of a weighted graph G = (V,E), the Max-Cut problem calls for a ...... Further, in [21] the authors report a comparison of a matlab.

2010-10-15T23:59:59.000Z

288

Topic Assignment as of 1/29/2011 Android hardware API (max # of presenter)  

E-Print Network (OSTI)

Topic Assignment as of 1/29/2011 Android hardware API (max # of presenter) 1. Taking a picture) Sevada Abraamyan; Other Android API 7. Android search framework (1) Dillon Kearns; 8. Web

289

ARM - Field Campaign - 2006 MAX-Mex-Megacity Aerosol eXperiment - Mexico  

NLE Websites -- All DOE Office Websites (Extended Search)

6 MAX-Mex-Megacity Aerosol eXperiment - Mexico City 6 MAX-Mex-Megacity Aerosol eXperiment - Mexico City Comments? We would love to hear from you! Send us a note below or call us at 1-888-ARM-DATA. Send Campaign : 2006 MAX-Mex-Megacity Aerosol eXperiment - Mexico City 2006.03.03 - 2006.03.28 Lead Scientist : Jeffrey Gaffney For data sets, see below. Description A 4-week field campaign was conducted in and downwind of Mexico City during March 2006. The Megacity Aerosol eXperiment - MEXico City (MAX-MEX) characterized aerosol formation and changes in aerosol composition, size distribution, light scattering coefficient, absorption coefficient, optical depth, soot-specific absorption, and radiative fluxes at selected vertical and horizontal locations in the outflow from a well-characterized urban core. Detailed analyses were made of the meteorological conditions during

290

Petroleum Institute Scholarly Publications  

E-Print Network (OSTI)

Abu Dhabi The Petroleum Institute Scholarly Publications January 1st ­ December 31st 2007 #12;The Petroleum Institute Scholarly Publications January 1st ­ December 31st 2007 v #12;- 2 - Scholarly Publications 2007 | The Petroleum Institute #12;- 3 - Scholarly Publications 2007 | The Petroleum Institute

291

Petroleum Institute Scholarly Publications  

E-Print Network (OSTI)

Abu Dhabi The Petroleum Institute Scholarly Publications 2010 #12;#12;The Petroleum Institute Belhaj Petroleum Engineering Sadoon Morad Petroleum Geosciences Sivakumar Sivasubramaniam College of Arts departments within the Petroleum Institute. Names in bold show Petroleum Institute faculty who are attached

292

Institut National des Tlcommunications Advanced Telecommunications Research Institute  

E-Print Network (OSTI)

Institut National des Télécommunications Advanced Telecommunications Research Institute Rapport de

Ray, Thomas S.

293

Vol. 167: 25-36, 1998 MARINE ECOLOGY PROGRESS SERIES  

E-Print Network (OSTI)

Gewasserphysik, Max-Planck-Strasse, D-21502 Geesthacht, Germany ABSTRACT: Macrofaunal samples were collected

Dippner, Joachim W.

294

Biogeosciences, 5, 171201, 2008 www.biogeosciences.net/5/171/2008/  

E-Print Network (OSTI)

Research, GKSS Research Center, Geesthacht, Max-Planck-Str., 21502 Geesthacht, Germany 7Center for Hydro

Stramski, Dariusz

295

ELSEVIER Atmospheric Research 39 (1995) 91-111 ATMOSPHERIC  

E-Print Network (OSTI)

Geesthacht, Institutfiir Physik, Max-Planck-Strafle, D-21502 GeesthachtGermany Received 6 April 1994

Moelders, Nicole

296

4, 34533530, 2007 Particulate organic  

E-Print Network (OSTI)

Research, GKSS Research Center, Geesthacht, Max-Planck-Str., 21502 Geesthacht, Germany 7 Center for Hydro

Paris-Sud XI, Université de

297

THE INSTITUTE OF ELECTRONICS, INFORMATION AND COMMUNICATION ENGINEERS  

E-Print Network (OSTI)

] Adaptive Processing [9] (FV ) Online Methods for Voltage and Frequency Control [10] Thrifty Barrier [5 PG1 MT4 MT7 MT9 PG2 time MT Margin MTi Ti ( MTG) TT MG [6] TMT G = Tm + Tn + ... + max1(...) + max2(...) + ... 1 TMT G = T1 + max(T8, T9) + max(T2 + T5, T6 +max(T2, T3), T7 + max(T3, T4)) Ti MTi MTG TMT G

Kasahara, Hironori

298

An Analog Cellular Automaton Model of Gravitation: Planck-Scale Black Holes Randall C. O'Reilly  

E-Print Network (OSTI)

An Analog Cellular Automaton Model of Gravitation: Planck-Scale Black Holes Randall C. O by Randall C. O'Reilly, initially published online at URL listed below on 12/28/05 (Dated: December 28, 2005

O'Reilly, Randall C.

299

Petroleum Institute Scholarly Publications  

E-Print Network (OSTI)

Abu Dhabi The Petroleum Institute Scholarly Publications 2008 #12.. AAkkgguunn Petroleum Engineering SS.. MMoorraadd Petroleum Geosciences RR.. NNuunnnn &&SS indicate Petroleum Institute faculty who are attached to the program shown. Every effort has been made

300

SLAC X-ray Identifies Mystery Atom Critical to Food Supply | Department of  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

X-ray Identifies Mystery Atom Critical to Food Supply X-ray Identifies Mystery Atom Critical to Food Supply SLAC X-ray Identifies Mystery Atom Critical to Food Supply November 18, 2011 - 10:05am Addthis Serena DeBeer of Cornell University and the Max Planck Institute for Bioinorganic Chemistry, led the the team that performed crucial experiments at SLAC. Dr. DeBeer is pictured above with Michael Roemelt and Frank Neese, also of the Max Planck Institute. Click here to see a photo of the nitrogenase enzyme. Serena DeBeer of Cornell University and the Max Planck Institute for Bioinorganic Chemistry, led the the team that performed crucial experiments at SLAC. Dr. DeBeer is pictured above with Michael Roemelt and Frank Neese,

Note: This page contains sample records for the topic "max planck institute" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


301

Moment-Preserving SN Discretizations for the One-Dimensional Fokker-Planck Equation  

SciTech Connect

The Fokker-Planck equation: (1) Describes the transport and interactions of charged particles, (2) Many small-angle scattering collisions, (3) Asymptotic limit of the Boltzmann equation (Pomraning, 1992), and (4) The Boltzmann collision operator becomes the angular Laplacian. SN angular discretization: (1) Angular flux is collocated at the SN quadrature points, (2) The second-order derivatives in the Laplacian term must be discretized, and (3) Weighted finite-difference method preserves zeroth and first moments (Morel, 1985). Moment-preserving methods: (1) Collocate the Fokker-Planck operator at the SN quadrature points, (2) Develop several related and/or equivalent methods, and (3) Motivated by discretizations for the angular derivative appearing in the transport equation in one-dimensional spherical coordinates.

Warsa, James S. [Los Alamos National Laboratory; Prinja, Anil K. [Los Alamos National Laboratory

2012-06-14T23:59:59.000Z

302

Una interpretaci\\'on f\\'isica de la constante de Planck  

E-Print Network (OSTI)

According to the commonly accepted interpretation of Quantum Mechanics, it is only possible to talk about the existence of elementary particles when they are detected by an experiment or by a classical measurement device. This has led to distortions with regard to the objective existence of reality, since it would be necessary an observer to materialize the elementary particle. This issue is solved when the elementary particle is placed in permanent interaction with the rest of the universe, so its existence would not depend on any intelligent observer and thus the objective range of elementary particles would be recovered. This article explores the interaction between elementary particles and a background action field of stochastic character and it is also determined that the standard deviation of the particle-background field interaction is essentially the Planck constant, since the expressions of the energy according to the Planck postulate and the momentum according to the Louis de Broglie thesis follow i...

Alvarez-Samaniego, Wilson P; Moya-Alvarez, Douglas

2013-01-01T23:59:59.000Z

303

Detectability of Planck-Scale-Induced Blurring with Gamma-Ray Bursts  

E-Print Network (OSTI)

Microscopic fluctuations inherent to the fuzziness of spacetime at the Planck scale might accumulate in wavefronts propagating a cosmological distance and lead to noticeable blurring in an image of a pointlike source. Distant quasars viewed in the optical and ultraviolet with Hubble Space Telescope (HST} may show this weakly, and if real suggests a stronger effect should be seen for Gamma-Ray Bursts (GRBs) in X-rays and gamma-rays. Those telescopes, however, operate far from their diffraction limits. A description of how Planck-scale-induced blurring could be sensed at high energy, even with cosmic rays, while still agreeing with the HST results is discussed. It predicts dilated apparent source size and inflated uncertainties in positional centroids, effectively a threshold angular accuracy restricting knowledge of source location on the sky. These outcomes are found to be consistent with an analysis of the 10 highest-redshift GRB detections reported for the Fermi satellite. Confusion with photon cascade and ...

Steinbring, Eric

2015-01-01T23:59:59.000Z

304

Astrophysics in relative unites as conformal unified theory without Planck absolutes  

E-Print Network (OSTI)

Astrophysical data on the Supernova luminosity-distance - redshift relations, recalculated in terms of relative measurement standards, is utilized as a justification of conformal-invariant unified theory, where all masses, including masses of the Planck and Higgs, become the present- day values of dynamic variable of evolution of the universe in a regime of the dominances of a free scalar field. Planck epoch with the primordial fireball of the Hot Universe Scenario is substituted by the epoch of cosmological creation from physical vacuum of W-, Z-bosons. Arguments for the benefit of existence of initial data of the cosmic evolution which describe all visible matter including CMB radiation as product of decays of the primordial bosons in the framework of Standard Model are listed.

Barbashov, B M; Pervushin, V N; Zorin, A G

2002-01-01T23:59:59.000Z

305

The Institute of Petroleum  

E-Print Network (OSTI)

The Institute of Petroleum Engineering The Institute of Petroleum Engineering (IPE) is a world leading, specialised centre in research, training and teaching, with the largest petroleum engineering and teaching. Our vision is to be the international institute of choice for research and teaching in petroleum

Painter, Kevin

306

The National Cancer Institute,  

E-Print Network (OSTI)

The National Cancer Institute, International Cancer Information Center Bldg. 82, Rm 123 Bethesda, MD 20892 The National Cancer Institute (NCI) is part of the Federal Government. NCI coordinates the government's cancer research program. It is the largest of the 17 biomedical research institutes and centers

307

institution Service Fin  

E-Print Network (OSTI)

with the up eed to have: eferred institut mary DUNS nu me, title, and em enter the infor ded verificatio st universit earching on th e n institution is r "List of Comp ent, or search for the institut thorized. Not Listed? ted, it may still uctions with th n or entity can HScompliant F o determine if i cies

Hutcheon, James M.

308

Policy for Institutional Consultants  

Science Journals Connector (OSTI)

Policy for Institutional Consultants ... The Association of Consulting Chemists and Chemical Engineers, therefore, offers "A Statement of Research Policy Suggested for Inclusion in Research Policies of Educational Institutions" which is the result of a study of a cross section of institutional policies now in ... ...

1946-06-10T23:59:59.000Z

309

OIL & GAS INSTITUTE Introduction  

E-Print Network (OSTI)

OIL & GAS INSTITUTE CONTENTS Introduction Asset Integrity Underpinning Capabilities 2 4 4 6 8 9 10 COMPETITIVENESS UNIVERSITY of STRATHCLYDE OIL & GAS INSTITUTE OIL & GAS EXPERTISE AND PARTNERSHIPS #12;1 The launch of the Strathclyde Oil & Gas Institute represents an important step forward for the University

Mottram, Nigel

310

INSTITUTE OF BIOMEDICAL ENGINEERING  

E-Print Network (OSTI)

INSTITUTE OF BIOMEDICAL ENGINEERING Innovation,Translation, Impact University College London Gower Street London WC1E 6BT UK www.ibme.ucl.ac.uk DesignbyHype!hype.co.uk UCL Institute of Biomedical Engineering #12;Innovating MedTech The Institute of Biomedical Engineering (IBME) provides a much-needed focus

Saunders, Mark

311

The Planck energy-mass source as an alternative to the Big Bang  

E-Print Network (OSTI)

The general theory of relativity is used to show that the total energy-mass of the visible Universe could be produced by an energy-mass source with the Planck power. The source was supposedly born at the phase of cosmic inflation and acts continuously throughout the lifetime of our Universe. The model allows one to treat dark energy as a real form of energy without using the hypothesis of anti-gravity.

Serge F. Timashev

2008-04-17T23:59:59.000Z

312

The Simultaneous Medicina-Planck Experiment (SiMPlE): data acquisition, reduction and first results  

E-Print Network (OSTI)

The Simultaneous Medicina-{\\it Planck} Experiment (SiMPlE) is aimed at observing a selected sample of 263 extragalactic and Galactic sources with the Medicina 32-m single dish radio telescope in the same epoch as the Planck satellite observations. The data acquired with a frequency coverage down to 5 GHz, also combined with Planck at frequencies above 30 GHz, will constitute a useful reference catalogue of bright sources over the whole Northern hemisphere. Furthermore, source observations performed in different epochs and comparison with other catalogues allow the investigation of source variabilities on different timescales. In this work, we describe the sample selection, the on-going data acquisition campaign, the data reduction procedures, the developed tools, and the comparison with other data-sets. We present the data at 5 and 8.3 GHz for the SiMPlE Northern Sample consisting of 79 sources with $\\delta \\geq 45^\\circ$ selected in our catalogue and observed during the first 6 months of the project. A first...

Procopio, P; Righini, S; Zanichelli, A; Ricciardi, S; Libardi, P; Burigana, C; Cuttaia, F; Mack, K -H; Terenzi, L; Villa, F; Bonavera, L; Morgante, G; Trigilio, C; Trombetti, T; Umana, G

2011-01-01T23:59:59.000Z

313

Reconstruction of the primordial power spectra with Planck and BICEP2 data  

Science Journals Connector (OSTI)

By using the cubic spline interpolation method, we reconstruct the shape of the primordial scalar and tensor power spectra from the recently released Planck temperature and BICEP2 polarization cosmic microwave background data. We find that the vanishing scalar index running (dns/dlnk) model is strongly disfavored at more than 3? confidence level on the k=0.0002??Mpc?1 scale. Furthermore, the power-law parametrization gives a blue-tilt tensor spectrum, no matter using only the first five bandpowers nt=1.20?0.64+0.56(95%??C.L.) or the full nine bandpowers nt=1.24?0.58+0.51(95%??C.L.) of BICEP2 data sets. Unlike the large tensor-to-scalar ratio value (r?0.20) under the scale-invariant tensor spectrum assumption, our interpolation approach gives r0.002<0.060(95%??C.L.) by using the first five bandpowers of BICEP2 data. After comparing the results with/without BICEP2 data, we find that Planck temperature with small tensor amplitude signals and BICEP2 polarization data with large tensor amplitude signals dominate the tensor spectrum reconstruction on the large and small scales, respectively. Hence, the resulting blue tensor tilt actually reflects the tension between Planck and BICEP2 data.

Bin Hu; Jian-Wei Hu; Zong-Kuan Guo; Rong-Gen Cai

2014-07-30T23:59:59.000Z

314

Radial Fokker-Planck model for plasmas confined by magnetic mirror fields  

SciTech Connect

A time-dependent computer model has been developed for the spatially dependent distribution function f(r,v,t). An orbit averaged Fokker-Planck equation treats Coulomb collisions and various atomic physics processes. The motivation for the present code is to provide an accurate treatment of gyro-radius effects and realistic beam geometries which have been neglected in previous Fokker-Planck codes. Finite width beams may be offset from the plasma center to determine beam injection for build-up studies. The inclusion of a finite gyro-radius is essential for studying radial transport due to both quasilinear fluctuations and charge exchange collisions. Charge exchange with energetic beam atoms and plasma erosion due to charge-exchange collisions with thermal gas are both included. Quasilinear diffusion terms include the effects of turbulent diffusion in the model. The model has been used to study particle and energy confinement times in the 2XIIB experiment and in the mirror plug of the TMX experiment. Calculated values of T/sub e/ decrease from classical Fokker-Planck values (1000 eV for 2XIIB) to the 50 eV to 200 eV range observed in 2XIIB and TMX experiments. Radial density profiles and n tau scaling with plasma radius and magnetic field agree with experimental data.

Futch, A.H.

1986-05-01T23:59:59.000Z

315

Towards more realistic Ion Cyclotron Resonance Heating Fokker-Planck modelling  

SciTech Connect

Recent theoretical work allows accounting for a number of effects previously not or not fully accounted for but potentially playing an important role to understand the wave-particle interaction underlying Ion Cyclotron Resonance Heating. In [1] a semi-analytical method was proposed to evaluate the dielectric response of a plasma to electromagnetic waves in the ion cyclotron domain of frequencies accounting for drift orbit effects in an axisymmetric tokamak. It relies on subdividing the orbit into elementary segments in which the integrations can be performed analytically or by tabulation. Using the coefficients evaluated using this semi-analytical method, a 3-D Fokker-Planck code is being developed. The underlying equations and their implementation, as well as some results of this new 3-D Fokker-Planck code are briefly presented. The adopted numerical resolution technique relies on a subdivision of the integration domain in tetrahedrons. This specific shape of the elementary volumes allows imposing the boundary conditions along curved surfaces - in particular the 'bi-local' conditions across the curved trapped/passing boundary connecting one trapped to two passing orbits - elegantly. Results are presented of Fokker-Planck modelling accounting for the actual electric field wave structure, particle orbits and tokamak geometry. A discussion is also provided on the feasibility of further upgrading the description.

Van Eester, D. [Laboratory for Plasma Physics, Association 'EURATOM - Belgian State', Koninklijke Militaire School - Ecole Royale Militaire, Trilateral Euregio Cluster, Brussels (Belgium)

2006-11-30T23:59:59.000Z

316

Institutional Change for Sustainability | Department of Energy  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

Institutional Change for Sustainability Institutional Change for Sustainability Institutional Change Continuous Improvement Cycle Institutional Change Continuous Improvement Cycle...

317

Atmos. Chem. Phys., 14, 957968, 2014 www.atmos-chem-phys.net/14/957/2014/  

E-Print Network (OSTI)

. Lelieveld1,2 1The Cyprus Institute, P.O. Box 27456, 1645 Nicosia, Cyprus 2Max Planck Institute for Chemistry 1 Introduction Increased levels of fine particles in the air from anthro- pogenic and natural origin parts of the lungs and the smallest ones even the alveoli, the gas exchange cavities of the lungs

Meskhidze, Nicholas

318

Integrability and disorder in mesoscopic systems: Application to orbital magnetism  

E-Print Network (OSTI)

komplexer Systeme, 01187 Dresden, Germany Denis Ullmoa) Bell Laboratories, Lucent Technologies, 1D-265, 600 Institut fu¨r Physik, Memminger Strasse. 6, 86135 Augsburg, Germany and Max-Planck-Institut fu¨r Physik functions. We dem- onstrate that the anomalously large zero-field susceptibility characteristic of clean

Ullmo, Denis

319

Atmos. Chem. Phys., 10, 93199331, 2010 www.atmos-chem-phys.net/10/9319/2010/  

E-Print Network (OSTI)

Biogeochemistry Department, Max Planck Institute for Chemistry, Mainz, Germany *present address: Institute of Sciences of Ukraine, Kharkov, Ukraine ***present address: Cordis Corporation, Analytical Technology, Spring burning), a transition period, and the onset of the wet season (clean conditions). In the present study

Meskhidze, Nicholas

320

Atmos. Chem. Phys., 7, 43294373, 2007 www.atmos-chem-phys.net/7/4329/2007/  

E-Print Network (OSTI)

Quality Research Branch, Environment Canada, Downsview, Ontario, Canada 9W. M. Keck Laboratories, Cambridge, Massachusetts, USA 15School of Chemistry, University of Leeds, Leeds, LS2 9JT, UK 16Institute, Ontario, Canada 22Air Chemistry Department, Max-Planck Institute of Chemistry, P.O. Box 3060, 55020 Mainz

Paris-Sud XI, Université de

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321

Physics Issues in the Design of Low Aspect-Ratio, High-, Quasi-Axisymmetric Stellarators  

E-Print Network (OSTI)

, Lausanne, Switzerland 5 Max Planck Institute for Plasma Physics,Greifswald, Germany 6 Kurchatov InstitutePhysics Issues in the Design of Low Aspect-Ratio, High-, Quasi-Axisymmetric Stellarators M Princeton Plasma Physics Laboratory, Princeton, NJ 08543 USA 2 Oak Ridge National Laboratory, Oak Ridge, TN

Lin, Zhihong

322

H Goldschmidt Abstracts 2011  

Science Journals Connector (OSTI)

...electron pool in ROS reactions. [1] Morones et al. (2005) Nanotechnology 16, 2346. [2] Hwang et al. (2008) Small 4, 746...correspondence: aheuser@uni-bonn.de) 2 Institute of Aerospace Medicine, German Aerospace Center (DLR), K ln, Germany 3 Max-Planck-Institut...

323

German public-private partnership breaks ground  

Science Journals Connector (OSTI)

... history, Germany's Max Planck Society (MPS) is setting up a new institute using private money 200 million (US$317 million) of it. On 15 July, ... The institute is set to start work by the end of this year. Publicprivate research is a well established concept in the United States, but not yet in ...

2008-07-23T23:59:59.000Z

324

State of the Arctic Coast 2010 Scientific Review and Outlook  

E-Print Network (OSTI)

International Permafrost Association Published by: Helmholtz-Zentrum Geesthacht LOICZ International Project Office Institute of Coastal Research Max-Planck-Strasse 1 D-21502 Geesthacht, Germany April 2011 The Land and financially supported by the Institute of Coastal Research, at the Helmholtz-Zentrum Geesthacht, Germany

Douglas, Thomas A.

325

Linear Structures in the Core of the Coma Cluster of Galaxies  

Science Journals Connector (OSTI)

...0HA, UK.3Max-Planck-Institut fur Astrophysik, Karl-Schwarzschild-Strasse 1, 85748 Garching, Germany.4Space Research Institute...for Cosmology and Astrophysics (10) and X-ray Multi-Mirror Mission (XMM-Newton) (11) (Fig. 3). The arms are...

J. S. Sanders; A. C. Fabian; E. Churazov; A. A. Schekochihin; A. Simionescu; S. A. Walker; N. Werner

2013-09-20T23:59:59.000Z

326

3, 24652497, 2003 Nudged GCM tracer  

E-Print Network (OSTI)

et al. Title Page Abstract Introduction Conclusions References Tables Figures Back Close Full Screen, The Netherlands 2 Space Research Organisation of the Netherlands (SRON), Utrecht, The Netherlands 3 Royal Netherlands Meteorological Institute (KNMI), De Bilt, The Netherlands 4 Max Planck Institut f¨ur Chemie (MPI

Paris-Sud XI, Université de

327

DOE Joint Genome Institute Completes Soybean Genome- Data Released to  

NLE Websites -- All DOE Office Websites (Extended Search)

Press Release: December 8, 2008 Press Release: December 8, 2008 DOE Joint Genome Institute Completes Soybean Genome- Data Released to Advance Biofuel, Food, & Feed Research WALNUT CREEK, CA- The U.S. Department of Energy Joint Genome Institute (DOE JGI) has released a complete draft assembly of the soybean (Glycine max) genetic code, making it widely available to the research community to advance new breeding strategies for one of the world's most valuable plant commodities. Soybean not only accounts for 70 percent of the world's edible protein, but also is an emerging feedstock for biodiesel production. Soybean is second only to corn as an agricultural commodity and is the leading U.S. agricultural export. DOE JGI's interest in sequencing the soybean centers on its use for biodiesel, a renewable, alternative fuel with the highest energy content of

328

Onshore wind max capacity 50.4% - what wind farm, what year? | OpenEI  

Open Energy Info (EERE)

Onshore wind max capacity 50.4% - what wind farm, what year? Onshore wind max capacity 50.4% - what wind farm, what year? Home How can I find more specific information about wind capacity? I can get the max/min/media stuff from the bar graphs. Is there any way to see individual wind farm capacity per year or get examples of performance? I'm helping run a tech site and some specific information would be helpful in dealing with skeptical individuals. Is there any more detailed information on capacity other than the graph summary statistics? (I do not know my way around this site, but I'm willing to learn.) Submitted by Bob Wallace on 15 June, 2013 - 00:23 1 answer Points: 0 Hi Bob- Thank you for posting your question. It seems that your question developed after viewing/using the Transparent Cost Database, however, I

329

Chromidio: an interface for color tracking with key frames in Max and Nato  

E-Print Network (OSTI)

separate mtr file to be loaded into any Max patch utilizing Max's mtr, or multi-track recorder, object. File Management A n important goal in software application development is to incorporate some basic file management functions so that projects can... 3 ? total matching pixels 0 7 6 8 0 0 |"5~ fT27~ [T27~ | 127 127 \\TzT 127 359 | 127 output 49 76 332 127 playback Fig. 16. The Recording and Playback window and related controls. From bottom left: Clear Mtr, Load Mtr File, Save Mtr...

Tucker, Amy Rebecca

2012-06-07T23:59:59.000Z

330

Modeling Max-Min Fairness for Elastic Flows in Telecommunication Alain Dupuisa, Fabrice Guillemina and Philippe Robertb  

E-Print Network (OSTI)

r0 allocated to some other data ow r0 such that r0 r. Max-min fairness can be formulated in terms1 Modeling Max-Min Fairness for Elastic Flows in Telecommunication Networks Alain Dupuisa, Fabrice Guillemina and Philippe Robertb aFrance Telecom R&D, 2, Avenue Pierre Marzin, 22300 Lannion France b

Guillemin, Fabrice

331

Understanding the Link Between Bicyclists and Light Rail Survey Results from Bicycle Riders on MAX in Portland, Oregon  

E-Print Network (OSTI)

Understanding the Link Between Bicyclists and Light Rail Survey Results from Bicycle Riders on MAX Introduction 1 Portland Bicycle Master Plan, Section V 2 History of Bicycles on MAX 3 Benefits of the Bicycle is a bicycle friendly city. In 1995 and 1998, Bicycling Magazine named Portland the best city for bicycling

Bertini, Robert L.

332

From max-plus algebra to nonexpansive mappings: a nonlinear theory for discrete event systems  

Science Journals Connector (OSTI)

Discrete event systems provide a useful abstraction for modelling a wide variety of systems: digital circuits, communication networks, manufacturing plants, etc. Their dynamics--stability, equilibrium states, cyclical behaviour, asymptotic average delays--are ... Keywords: cycle time, discrete event system, fixed point, max-plus semiring, nonexpansive map, nonlinear eigenvalue, nonnegative matrix, topical function

Jeremy Gunawardena

2003-02-01T23:59:59.000Z

333

The new ambient-pressure X-ray photoelectron spectroscopy instrument at MAX-lab  

Science Journals Connector (OSTI)

The new instrument for ambient-pressure X-ray photoelectron spectroscopy at the Swedish synchrotron radiation facility MAX IV Laboratory is presented. The instrument is based on the use of a retractable and exchangeable high-pressure cell, which implies that ultrahigh-vacuum conditions are retained in the analysis chamber and that dual ambient pressure and ultrahigh-vacuum use is possible.

Schnadt, J.

2012-08-07T23:59:59.000Z

334

A Power-Law Formulation of Laminar Flow in Short Pipes Max Sherman  

E-Print Network (OSTI)

A Power-Law Formulation of Laminar Flow in Short Pipes Max Sherman Indoor Environment Program ABSTRACT This report develops a theoretical description of the hydrodynamic relationship based on a power pipes can be described with a simple power law dependence on pressure, but that the exponent

335

Defining Development Standards for Reusable User Interface Max Mulawa, Rich Picking and Vic Grout  

E-Print Network (OSTI)

for standard aware development. · Constraints on API of the component. · Documentation structure. · IntegrationDefining Development Standards for Reusable User Interface Components Max Mulawa, Rich Picking.NET user-interface components. This standard aims to assess the quality of implemented components

Grout, Vic

336

Queue-Length Proportional and Max-Min Fair Bandwidth Allocation for Best Effort Flows  

E-Print Network (OSTI)

and fairness principles. In this paper, we propose sequential and parallel algorithms to allocate bandwidth the max-min fairness principle, which maximizes bandwidth utilization and maintains fairness among flows. We first formulate the problem based on the allocation criterion and fairness principle. Then, we

Pan, Deng

337

Copper: An Essential Micronutrient for Beef Cattle Max Irsik DVM, MAB  

E-Print Network (OSTI)

Copper: An Essential Micronutrient for Beef Cattle Max Irsik DVM, MAB Beef Cattle Extension Veterinarian University of Florid College of Veterinary Medicine Throughout the world copper deficiency limits of phosphorous, copper deficiency is the most sever mineral limitation to grazing livestock throughout extensive

Watson, Craig A.

338

CONDENSATION OF HOMOMORPHISM SPACES KLAUS LUX, MAX NEUNHOFFER, AND FELIX NOESKE  

E-Print Network (OSTI)

CONDENSATION OF HOMOMORPHISM SPACES KLAUS LUX, MAX NEUNH¨OFFER, AND FELIX NOESKE Abstract. We present an efficient algorithm for the condensation of homo- morphism spaces. This provides an improvement is a special case of what has become known as "condensation". The precise connection is as follows: Let F

St Andrews, University of

339

Extremal shot noises, heavy tails and max-stable random fields.  

E-Print Network (OSTI)

Extremal shot noises, heavy tails and max-stable random fields. Cl´ement Dombry May 31, 2010 Abstract We consider the extremal shot noise defined by M(y) = sup{mh(y - x); (x, m) }, where. Extremal shot noises naturally appear in extreme value theory as a model for spatial extremes and serve

Paris-Sud XI, Université de

340

Institute for Advanced Studies  

NLE Websites -- All DOE Office Websites (Extended Search)

Institute for Advanced Studies Institute for Advanced Studies Institute for Advanced Studies NMC leverages the strengths of three research universities to build joint programs, develop strategic partnerships, provide common organization and facilities. Contact Leader TBD LANL Program Administrator Pam Hundley (505) 663-5453 Email Building regional partnerships in education, leveraging strengths of three research universities The Institute for Advanced Studies (IAS) works with the three New Mexico research universities (University of New Mexico, New Mexico Tech, and New Mexico State University) to develop research and educational collaborations and partnerships. To facilitate interactions between the universities and LANL, the three New Mexico schools established the New Mexico Consortium (NMC), a nonprofit

Note: This page contains sample records for the topic "max planck institute" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


341

INSTITUTE COLLOQUIA AND SEMINARS  

NLE Websites -- All DOE Office Websites (Extended Search)

National Laboratory, Berkeley, California Production of Transactinide Elements in Cold Fusion Reactions at LBNL February 20 Mr. Thomas Henry, Cyclotron Institute, Texas A&M...

342

Graduate Studies - Cyclotron Institute  

NLE Websites -- All DOE Office Websites (Extended Search)

the Department of Chemistry, but may elect to work with any Institute faculty research advisor, irrespective of that advisor's departmental affiliation. Research programs at the...

343

Michigan Institute Science and  

E-Print Network (OSTI)

Michigan Institute for Plasma Science and Engineering Seminar Onset of Fast Magnetic Reconnection's magnetosphere, and solar flares. These observations place strong constraints on theory, which must explain

Shyy, Wei

344

Michigan Institute Plasma Science  

E-Print Network (OSTI)

Michigan Institute Plasma Science and Engineering Seminar Neutral Atom Imaging of the Terrestrial re- search includes ion heating in the solar corona, electric double layers, magne- tosphere neutral

Shyy, Wei

345

INSTITUTE OF COMPUTER SCIENCE  

E-Print Network (OSTI)

Institute of Computer Science, Academy of Sciences of the Czech Republic. Pod vodrenskou v 2, 182 07 Prague 8, Czech Republic. phone: (+420)266052083...

346

The Norwegian Polar Institute  

Science Journals Connector (OSTI)

... ON March 1, the Norwegian Polar Institute (Norsk Polarinstitutt) was established in Oslo in order to continue and expand the activity of ...

1948-06-19T23:59:59.000Z

347

Commitment Institutional Change Principle  

Energy.gov (U.S. Department of Energy (DOE))

Commitment can be a crucial element that helps Federal agencies inject and emphasize sustainability in their organizational culture. Institutions and people change when they have made definite...

348

Research - Cyclotron Institute  

NLE Websites -- All DOE Office Websites (Extended Search)

Overview Viewing gamma ray spectra. The Institute research program focuses on the atomic nucleus, a many-body system of strongly interacting constituents bound together by the...

349

Massachusetts Institute of Technology  

NLE Websites -- All DOE Office Websites (Extended Search)

132011 Teppei Katori, MIT 1 Teppei Katori for MiniBooNE collaboration Massachusetts Institute of Technology Short baseline neutrino workshop, Fermilab, Batavia, IL, May 13, 2011...

350

Constraining the dynamical dark energy parameters: Planck-2013 vs WMAP9  

E-Print Network (OSTI)

We determine the best-fit values and confidence limits for dynamical dark energy parameters together with other cosmological parameters on the basis of different datasets which include WMAP9 or Planck-2013 results on CMB anisotropy, BAO distance ratios from recent galaxy surveys, magnitude-redshift relations for distant SNe Ia from SNLS3 and Union2.1 samples and the HST determination of the Hubble constant. We use a Markov Chain Monte Carlo routine to map out the likelihood in the multi-dimensional parameter space. We show that the most precise determination of cosmological parameters with the narrowest confidence limits is obtained for the Planck{+}HST{+}BAO{+}SNLS3 dataset. The best-fit values and 2$\\sigma$ confidence limits for cosmological parameters in this case are $\\Omega_{de}=0.718\\pm0.022$, $w_0=-1.15^{+0.14}_{-0.16}$, $c_a^2=-1.15^{+0.02}_{-0.46}$, $\\Omega_bh^2=0.0220\\pm0.0005$, $\\Omega_{cdm}h^2=0.121\\pm0.004$, $h=0.713\\pm0.027$, $n_s=0.958^{+0.014}_{-0.010}$, $A_s=(2.215^{+0.093}_{-0.101})\\cdot10^{-9}$, $\\tau_{rei}=0.093^{+0.022}_{-0.028}$. For this dataset, the $\\Lambda$CDM model is just outside the 2$\\sigma$ confidence region, while for the dataset WMAP9{+}HST{+}BAO{+}SNLS3 the $\\Lambda$CDM model is only 1$\\sigma$ away from the best fit. The tension in the determination of some cosmological parameters on the basis of two CMB datasets WMAP9 and Planck-2013 is highlighted.

B. Novosyadlyj; O. Sergijenko; R. Durrer; V. Pelykh

2013-12-23T23:59:59.000Z

351

COUNTRY INSTITUTION SIGNING DATE  

E-Print Network (OSTI)

COUNTRY INSTITUTION SIGNING DATE /RENEWAL WEB SITE ALBANIA University of Tirana 11.12.2001 www /RENEWAL WEB SITE FINLAND JAMK University of Applied Sciences 29.10.2009 www.jamk.fi/ FRANCE ?cole INSTITUTION SIGNING DATE /RENEWAL WEB SITE MACEDONIA St. Cyril and Methodius" University of Skopje 11

Di Pillo, Gianni

352

Nuclear Energy Institutes  

Science Journals Connector (OSTI)

Nuclear Energy Institutes ... The Atomic Energy Commission and the American Society for Engineering Education offer their nuclear energy courses for engineering and science teachers again in the summer of 1960. ... At least 160 college and university teachers will study nuclear science in the seven institutes scheduled. ...

1960-01-11T23:59:59.000Z

353

National Institutes of Health National Institute of Mental Health  

E-Print Network (OSTI)

National Institutes of Health National Institute of Mental Health Department of Health and HumanNational Institute of Mental Health Division of Intramural Research Programs http://intramural.nimh.nih.gov/ [NIMH of Fellowship Training] National Institutes of Health National Institute of Mental Health Department of Health

Baker, Chris I.

354

Deposit Description (for FIS, max 30 characters) Outd $ PSU ID/Acct #, Name(Last, First, MI), or other comments Cards $  

E-Print Network (OSTI)

Cash $ Deposit Description (for FIS, max 30 characters) Outd $ Checks $ PSU ID/Acct #, Name documentation attached. Must equal 0: PSU Miscellaneous Deposit Form Cash $ Deposit Description (for FIS, max 30 Deposit Form Cash $ Deposit Description (for FIS, max 30 characters) Outd $ Checks $ PSU ID/Acct #, Name

Caughman, John

355

156 IEEE JOURNAL ON SELECTED AREAS IN COMMUNICATIONS, VOL. 27, NO. 2, FEBRUARY 2009 Scheduling in IEEE 802.16e Mobile WiMAX  

E-Print Network (OSTI)

in IEEE 802.16e Mobile WiMAX Networks: Key Issues and a Survey Chakchai So-In, Student Member, IEEE, Raj times. IEEE 802.16e based WiMAX networks promise the best available quality of experience for mobile data service users. Unlike wireless LANs, WiMAX networks incorporate several quality of service (Qo

Jain, Raj

356

Bohr - Planck quantum theory, (Tesla) magnetic monopoles and fine structure constant  

E-Print Network (OSTI)

In this work we apply Bohr-Planck (Old quantum atomic and radiation) theory, i.e. and quasi-classical methods for analysis of the magnetic monopoles and other problems. We reproduce exactly some basic elements of the Dirac magnetic monopoles theory, especially Dirac electric/magnetic charge quantization condition. Also, we suggest a new, effective, simply called Tesla model (for analogy with positions of the solenoids by Tesla inductive motor) of the magnetic monopole instead of usual effective Dirac model (half-infinite, very tinny solenoid) of the magnetic monopole. In our, i.e. Tesla model we use three equivalent tiny solenoids connected in series with a voltage source. One end of any solenoid is placed at the circumference of a circle and solenoids are directed radial toward circle center. Length of any solenoid is a bit smaller than finite circle radius so that other end of any solenoid is very close to the circle center. Angles between neighboring solenoids equal $120^{\\circ}$. All this implies that, practically, there is no magnetic field, or, magnetic pole, e.g. $S$, in the circle center, and that whole system holds only other, $N$ magnetic pole, at the ends of the solenoids at circle circumference. Finally, we reproduce relatively satisfactory value of the fine structure constant using Planck, i.e. Bose-Einstein statistics and Wien displacement law.

Vladan Pankovic; Darko V. Kapor; Stevica Djurovic; Miodrag Krmar

2014-10-17T23:59:59.000Z

357

Planck 2015 results. IV. Low Frequency Instrument beams and window functions  

E-Print Network (OSTI)

This paper presents the characterization of the in-flight beams, the beam window functions, and the associated uncertainties for the Planck Low Frequency Instrument (LFI). The structure of the paper is similar to that presented in the 2013 Planck release; the main differences concern the beam normalization and the delivery of the window functions to be used for polarization analysis. The in-flight assessment of the LFI main beams relies on measurements performed during observations of Jupiter. By stacking data from seven Jupiter transits, the main beam profiles are measured down to -25 dB at 30 and 44 GHz, and down to -30 dB at 70 GHz. The agreement between the simulated beams and the measured beams is confirmed to be better than 1% at each LFI frequency band (within the 20 dB contour from the peak, the rms values are: 0.1% at 30 and 70 GHz; 0.2% at 44 GHz). Simulated polarized beams are used for the computation of the effective beam window functions. The error budget for the window functions is estimated fro...

Ade, P A R; Ashdown, M; Aumont, J; Baccigalupi, C; Banday, A J; Barreiro, R B; Bartolo, N; Battaner, E; Benabed, K; Benot, A; Benoit-Lvy, A; Bernard, J -P; Bersanelli, M; Bielewicz, P; Bonaldi, A; Bonavera, L; Bond, J R; Borrill, J; Bouchet, F R; Bucher, M; Burigana, C; Butler, R C; Calabrese, E; Cardoso, J -F; Catalano, A; Chamballu, A; Christensen, P R; Colombi, S; Colombo, L P L; Crill, B P; Curto, A; Cuttaia, F; Danese, L; Davies, R D; Davis, R J; de Bernardis, P; de Rosa, A; de Zotti, G; Delabrouille, J; Dickinson, C; Diego, J M; Dole, H; Donzelli, S; Dor, O; Douspis, M; Ducout, A; Dupac, X; Efstathiou, G; Elsner, F; Enlin, T A; Eriksen, H K; Fergusson, J; Finelli, F; Forni, O; Frailis, M; Franceschi, E; Frejsel, A; Galeotta, S; Galli, S; Ganga, K; Giard, M; Giraud-Hraud, Y; Gjerlw, E; Gonzlez-Nuevo, J; Grski, K M; Gratton, S; Gregorio, A; Gruppuso, A; Hansen, F K; Hanson, D; Harrison, D L; Henrot-Versill, S; Herranz, D; Hildebrandt, S R; Hivon, E; Hobson, M; Holmes, W A; Hornstrup, A; Hovest, W; Huffenberger, K M; Hurier, G; Jaffe, A H; Jaffe, T R; Juvela, M; Keihnen, E; Keskitalo, R; Kiiveri, K; Kisner, T S; Knoche, J; Kunz, M; Kurki-Suonio, H; Lhteenmki, A; Lamarre, J -M; Lasenby, A; Lattanzi, M; Lawrence, C R; Leahy, J P; Leonardi, R; Lesgourgues, J; Levrier, F; Liguori, M; Lilje, P B; Linden-Vrnle, M; Lindholm, V; Lpez-Caniego, M; Lubin, P M; Macas-Prez, J F; Maggio, G; Maino, D; Mandolesi, N; Mangilli, A; Martin, P G; Martnez-Gonzlez, E; Masi, S; Matarrese, S; Mazzotta, P; McGehee, P; Meinhold, P R; Melchiorri, A; Mendes, L; Mennella, A; Migliaccio, M; Mitra, S; Montier, L; Morgante, G; Mortlock, D; Moss, A; Munshi, D; Murphy, J A; Naselsky, P; Nati, F; Natoli, P; Netterfield, C B; Nrgaard-Nielsen, H U; Novikov, D; Novikov, I; Paci, F; Pagano, L; Paoletti, D; Partridge, B; Pasian, F; Patanchon, G; Pearson, T J; Perdereau, O; Perotto, L; Perrotta, F; Pettorino, V; Piacentini, F; Pierpaoli, E; Pietrobon, D; Pointecouteau, E; Polenta, G; Pratt, G W; Przeau, G; Prunet, S; Puget, J -L; Rachen, J P; Rebolo, R; Reinecke, M; Remazeilles, M; Renzi, A; Rocha, G; Rosset, C; Rossetti, M; Roudier, G; Rubio-Martn, J A; Rusholme, B; Sandri, M; Santos, D; Savelainen, M; Scott, D; Seiffert, M D; Shellard, E P S; Spencer, L D; Stolyarov, V; Sutton, D; Suur-Uski, A -S; Sygnet, J -F; Tauber, J A; Terenzi, L; Toffolatti, L; Tomasi, M; Tristram, M; Tucci, M; Tuovinen, J; Umana, G; Valenziano, L; Valiviita, J; Van Tent, B; Vassallo, T; Vielva, P; Villa, F; Wade, L A; Wandelt, B D; Watson, R; Wehus, I K; Yvon, D; Zacchei, A; Zonca, A

2015-01-01T23:59:59.000Z

358

Argonne Accelerator Institute  

NLE Websites -- All DOE Office Websites (Extended Search)

AAI Home AAI Home Welcome Accelerators at Argonne Mission Organization History Document Collection Conferences & Workshops Beams and Applications Seminar Argonne-Fermilab Collaboration Lee Teng Scholarship Program Useful Links Organization The Argonne Accelerator Institute is a matrixed organization. Its members and fellows reside in programmatic Argonne divisions. The Institute reports to the Associate Laboratory Director for Photon Science), and the administrative functions of the Institute are within the PSC directorate. Director: Rodney Gerig Associate Director: Hendrik Weerts ( Director of High Energy Physics Division) Associate Director: Sasha Zholents (Director of Accelerator Systems Division) Associate Director: Robert Janssens ( Director of Argonne Physics Division)

359

Argonne Accelerator Institute  

NLE Websites -- All DOE Office Websites (Extended Search)

Useful Links Useful Links Argonne National Laboratory Accelerator Sites Conferences Advanced Photon Source (APS) Argonne Wakefield Accelerator (AWA) Argonne Tandem Linear Accelerator System (ATLAS) High Energy Physics Division RIA (????) Link to JACoW (Joint Accelerator Conferences Website) Fermi National Accelerator Laboratory Fermilab-Argonne Collaboration Accelerator Physics Center Workshops Other Accelerator Institutes Energy Recovering Linacs Center for Advance Studies of Accelerators (Jefferson Labs) Center for Beam Physics (LBNL) Accelerator Test Facility (BNL) The Cockcroft Institute (Daresbury, UK) John Adams Institute (Rutherford, UK) ERL2009 to be held at Cornell ERL2007 ERL2005 DOE Laboratory with Accelerators Fermilab Stanford Linear Accelerator Center Brookhaven National Laboratory

360

DOE - Office of Legacy Management -- Max Zuckerman and Sons Inc - MD 04  

Office of Legacy Management (LM)

Inc - MD 04 Inc - MD 04 FUSRAP Considered Sites Site: MAX ZUCKERMAN & SONS, INC. (MD.04 ) Eliminated from consideration under FUSRAP Designated Name: Not Designated Alternate Name: Maryland Alloys Corporation MD.04-1 Location: 5245 Fairlawn Avenue , Baltimore , Maryland MD.04-2 Evaluation Year: 1994 MD.04-1 MD.04-3 Site Operations: Scrap metals broker that arranged purchases of materials for third party buyers. MD.04-2 MD.04-4 Site Disposition: Eliminated - Potential for contamination remote MD.04-3 Radioactive Materials Handled: Yes Primary Radioactive Materials Handled: Uranium (Q-11) Oxide/Residue MD.04-2 MD.04-4 Radiological Survey(s): Yes MD.04-1 Site Status: Eliminated from consideration under FUSRAP MD.04-3 Also see Documents Related to MAX ZUCKERMAN & SONS, INC.

Note: This page contains sample records for the topic "max planck institute" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
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We encourage you to perform a real-time search of NLEBeta
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361

Joint Theory Institute  

NLE Websites -- All DOE Office Websites (Extended Search)

Program General Info Program General Info Registration Info Directions to Argonne Dynamics of Symmetry Breaking A Workshop sponsored by the ANL/UChicago Joint Theory Institute April 13-17, 2009 Argonne National Laboratory, IL The Joint Theory Institute (JTI) is a multi-disciplinary research institution jointly supported at the University of Chicago and Argonne National Laboratory to enhance collaborative research between both institutions in the broad area of theory. This year JTI sponsors a workshop the aim of which is to explore the dynamics of symmetry breaking in a broad range of systems from nuclear physics to string theory, using theoretical insights such as Dyson-Schwinger equations formalism, gauge/gravity duality and lattice QCD. We will focus on systems which exhibit dynamical symmetry breaking and will cover topics essential for understanding nonperturbative QCD and physics of quark-gluon plasma.

362

Petroleum Institute Scholarly Publications  

E-Print Network (OSTI)

Abu Dhabi The Petroleum Institute Scholarly Publications 2009 #12 Mechanical Engineering HHaaddii BBeellhhaajj Petroleum Engineering SSaaddoooonn MMoorraadd Petroleum LLaannggiillllee Advanced University Placement Editors' notes: Names in bold in citations indicate Petroleum

363

Critical Materials Institute  

ScienceCinema (OSTI)

Ames Laboratory Director Alex King talks about the goals of the Critical Materials Institute in diversifying the supply of critical materials, developing substitute materials, developing tools and techniques for recycling critical materials, and forecasting materials needs to avoid future shortages.

Alex King

2013-06-05T23:59:59.000Z

364

INSTITUTE COLLOQUIA AND SEMINARS  

NLE Websites -- All DOE Office Websites (Extended Search)

April 16 M. Sanchez-Vega and V. E. Jacob, Cyclotron Institute, Texas A&M University Test of the Unitarity of the CKM Matrix via Superallowed + decay. April 23 Dr. Subrata...

365

Determine Institutional Change Sustainability Goals | Department...  

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

Determine Institutional Change Sustainability Goals Determine Institutional Change Sustainability Goals Institutional Change Continuous Improvement Cycle The first step in the...

366

Institutional Change for Sustainability Contacts | Department...  

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

Institutional Change for Sustainability Contacts Institutional Change for Sustainability Contacts For more information about institutional change for sustainability, contact: Jerry...

367

Institutional Change Process for Sustainability  

Energy.gov (U.S. Department of Energy (DOE))

For establishing institutional change in a Federal agency to achieve sustainability or other energy efficiency goals, follow the five-step institutional change process. In accordance with the...

368

Strategies for Achieving Institutional Change  

Energy.gov (U.S. Department of Energy (DOE))

Many strategiesincluding those derived from Institutional Change Principlesmay be used to effect institutional change in support of energy and sustainability objectives.

369

Property:OpenEI/UtilityRate/DemandRateStructure/Tier3Max | Open Energy  

Open Energy Info (EERE)

Max" Max" Showing 13 pages using this property. 4 4b524791-bef2-49b1-850b-458730755203 + 5 + 4b524791-bef2-49b1-850b-458730755203 + 5 + 4b524791-bef2-49b1-850b-458730755203 + 6 + 4b524791-bef2-49b1-850b-458730755203 + 7 + 4b524791-bef2-49b1-850b-458730755203 + 3 +, 4 +, 5 +, ... 4b524791-bef2-49b1-850b-458730755203 + 9 + 4b524791-bef2-49b1-850b-458730755203 + 3 + 4b524791-bef2-49b1-850b-458730755203 + 30 + 4b524791-bef2-49b1-850b-458730755203 + 4 + 4b524791-bef2-49b1-850b-458730755203 + 36 + E E40880ac-c27b-4cbf-a011-b0d7d6e10fe9 + 200 + E40880ac-c27b-4cbf-a011-b0d7d6e10fe9 + 200 + E40880ac-c27b-4cbf-a011-b0d7d6e10fe9 + 200 + Retrieved from "http://en.openei.org/w/index.php?title=Property:OpenEI/UtilityRate/DemandRateStructure/Tier3Max&oldid=539747

370

J A H R E S B E R I C H T | A N N U A L R E P O R T bericht des Prsidenten  

E-Print Network (OSTI)

J A H R E S B E R I C H T | A N N U A L R E P O R T 2 0 0 9 #12;2 bericht des Präsidenten Lese an Umweltveränderungen kOOPeratiOnsPrOgramme Partnergruppen Max Planck Fellows Kooperation mit der Fraunhofer-Gesellschaft Tandemprojekte Institutsübergreifende Forschungsinitiativen nachwuchsFörderung Minerva-Programm Max

Falge, Eva

371

Inflationary generalized Chaplygin gas and dark energy in the light of the Planck and BICEP2 experiments  

E-Print Network (OSTI)

In this work, we study an inflationary scenario in the presence of Generalized Chaplygin Gas (GCG). We show that in Einstein gravity, GCG is not a suitable candidate for inflation; but in a five dimensional brane world scenario, it can work as a viable inflationary model. We calculate the relevant quantities such as $n_{s}$, $r$ and $A_{s}$ related to the primordial scalar and tensor fluctuations, and using their recent bounds from Planck and BICEP2, we constrain the model parameters as well as the five-dimensional Planck mass. But as a slow-roll inflationary model with a power-law type scalar primordial power spectrum, GCG as an inflationary model can not resolve the tension between results from BICEP2 and Planck with a concordance $\\Lambda$CDM Universe. We show that going beyond the concordance $\\Lambda$CDM model and incorporating more general dark energy behaviour, this tension may be eased. We also obtain the constraints on the $n_{s}$ and $r$ and the GCG model parameters using Planck+WP+BICEP2 data considering the CPL dark energy behaviour.

Bikash R Dinda; Sumit Kumar; Anjan A. Sen

2014-10-21T23:59:59.000Z

372

The effect of a spatially varying Galactic spectral index on the maximum entropy reconstruction of Planck Surveyor satellite data  

E-Print Network (OSTI)

We study the effect of Galactic foregrounds with spatially varying spectral indices on analysis of simulated data from the Planck Satellite. We also briefly mention the effect the extra-galactic point sources have on the data analysis and summarise the most recent constraints on Galactic emission at GHz frequencies.

A. W. Jones; M. P. Hobson; P. Mukherjee; A. N. Lasenby

1998-10-15T23:59:59.000Z

373

Ion Fokker-Planck simulation of D-{sup 3}He gas target implosions  

SciTech Connect

Recently performed inertial confinement fusion implosion experiments involving D-{sup 3}He gas-filled microballoons have shown discrepancies between expected and measured nuclear fusion yields as the relative abundances of D and {sup 3}He are varied. The latter have been tentatively attributed to a sedimentation, or stratification phenomenon occurring in the target core. This work investigates the possibility of ion species sedimentation in a detailed way through multi-species ion-kinetic Vlasov-Fokker-Planck simulations of the implosion process. A noticeable amount of sedimentation is found to build up during the main shock propagation to the target center, but then disappears as the implosion proceeds. As a result, only the yield of the first burst of neutrons, associated with shock convergence, is appreciably modified, leaving the main neutron production phase during fuel compression and stagnation unaffected. The sedimentation of fuel ion species found, thus, cannot explain the experimental discrepancies.

Larroche, O. [CEA DIF, Bruyeres le Chatel, 91297 Arpajon Cedex (France)

2012-12-15T23:59:59.000Z

374

Fokker-Planck Dynamics and Entropies for the Normalized Ricci Flow  

E-Print Network (OSTI)

We consider some elementary aspects of the geometry of the space of probability measures endowed with Wasserstein distance. In such a setting, we discuss the various terms entering Perelman's shrinker entropy, and characterize two new monotonic functionals for the volume-normalized Ricci flow. One is obtained by a rescaling of the curvature term in the shrinker entropy. The second is associated with a gradient flow obtained by adding a curvature-drift to Perelman's backward heat equation. We show that the resulting Fokker-Planck PDE is the natural diffusion flow for probability measures absolutely continuous with respect to the Ricci-evolved Riemannian measure, we discuss its exponential trend to equilibrium, and its relation with the viscous Hamilton-Jacobi equation.

Mauro Carfora

2005-07-15T23:59:59.000Z

375

Constraints on the extensions to the base $?$CDM model from BICEP2, Planck and WMAP  

E-Print Network (OSTI)

Recently Background Imaging of Cosmic Extragalactic Polarization (B2) discovered the relic gravitational waves at $7.0\\sigma$ confidence level. However, the other cosmic microwave background (CMB) data, for example Planck data released in 2013 (P13), prefer a much smaller amplitude of the primordial gravitational waves spectrum if a power-law spectrum of adiabatic scalar perturbations is assumed in the six-parameter $\\Lambda$CDM cosmology. In this paper, we explore whether the $w$CDM model and the running spectral index can relax the tension between B2 and other CMB data. In particular, we find that a positive running of running of spectral index is preferred at $1.7\\sigma$ level from the combination of B2, P13 and WMAP Polarization data.

Cheng Cheng; Qing-Guo Huang; Wen Zhao

2014-05-02T23:59:59.000Z

376

Hypersharp Resonant Capture of Neutrinos as a Laboratory Probe of the Planck Length  

E-Print Network (OSTI)

The 18.6 keV antineutrino line from 2-body decay of 3H in crystals can be emitted with natural width because of motional averaging by lattice vibrations despite the very long lifetime of 3H and contrary to commonly held views of linewidths in such a case. It can be resonantly captured in 3He with geometrical cross section sigma ~10-17 cm2. Using its hypersharp sensitivity DELTAE/E ~10-29 and the method of time-filtered resonance, the basic energy width ~10-24 eV expected of the 3H state can be measured to test if ultimate nuclear widths are limited by the Planck length rather than time-energy uncertainty.

R. S. Raghavan

2009-03-04T23:59:59.000Z

377

Simultaneous Planck, Swift, and Fermi observations of X-ray and gamma-ray selected blazars  

E-Print Network (OSTI)

We present simultaneous Planck, Swift, Fermi, and ground-based data for 105 blazars belonging to three samples with flux limits in the soft X-ray, hard X-ray, and gamma-ray bands. Our unique data set has allowed us to demonstrate that the selection method strongly influences the results, producing biases that cannot be ignored. Almost all the BL Lac objects have been detected by Fermi-LAT, whereas ~40% of the flat-spectrum radio quasars (FSRQs) in the radio, soft X-ray, and hard X-ray selected samples are still below the gamma-ray detection limit even after integrating 27 months of Fermi-LAT data. The radio to sub-mm spectral slope of blazars is quite flat up to ~70GHz, above which it steepens to ~-0.65. BL Lacs have significantly flatter spectra than FSRQs at higher frequencies. The distribution of the rest-frame synchrotron peak frequency (\

Giommi, P; Lahteenmaki, A; Thompson, D J; Capalbi, M; Cutini, S; Gasparrini, D; Gonzalez-Nuevo, J; Leon-Tavares, J; Lopez-Caniego, M; Mazziotta, M N; Monte, C; Perri, M; Raino, S; Tosti, G; Tramacere, A; Verrecchia, F; Aller, H D; Aller, M F; Angelakis, E; Bastieri, D; Berdyugin, A; Bonaldi, A; Bonavera, L; Burigana, C; Burrows, D N; Buson, S; Cavazzuti, E; Chincarini, G; Colafrancesco, S; Costamante, L; Cuttaia, F; D'Ammando, F; de Zotti, G; Frailis, M; Fuhrmann, L; Galeotta, S; Gargano, F; Gehrels, N; Giglietto, N; Giordano, F; Giroletti, M; Keihanen, E; King, O; Krichbaum, T P; Lasenby, A; Lavonen, N; Lawrence, C R; Leto, C; Lindfors, E; Mandolesi, N; Massardi, M; Max-Moerbeck, W; Michelson, P F; Mingaliev, M; Natoli, P; Nestoras, I; Nieppola, E; Nilsson, K; Partridge, B; Pavlidou, V; Pearson, T J; Procopio, P; Rachen, J P; Readhead, A; Reeves, R; Reimer, A; Reinthal, R; Ricciardi, S; Richards, J; Riquelme, D; Saarinen, J; Sajina, A; Sandri, M; Savolainen, P; Sievers, A; Sillanpaa, A; Sotnikova, Y; Stevenson, M; Tagliaferri, G; Takalo, L; Tammi, J; Tavagnacco, D; Terenzi, L; Toffolatti, L; Tornikoski, M; Trigilio, C; Turunen, M; Umana, G; Ungerechts, H; Villa, F; Wu, J; Zacchei, A; Zensus, J A; Zhou, X

2011-01-01T23:59:59.000Z

378

Making Maps from Planck LFI 30GHz Data with Asymmetric Beams and Cooler Noise  

SciTech Connect

The Planck satellite will observe the full sky at nine frequencies from 30 to 857 GHz. Temperature and polarization frequency maps made from these observations are prime deliverables of the Planck mission. The goal of this paper is to examine the effects of four realistic instrument systematics in the 30 GHz frequency maps: non-axially-symmetric beams, sample integration, sorption cooler noise, and pointing errors. They simulated one year long observations of four 30 GHz detectors. The simulated timestreams contained CMB, foreground component (both galactic and extra-galactic), instrument nolise (correlated and white), and the four instrument systematic effects. They made maps from the timelines and examined the magnitudes of the systematics effects in the maps and their angular power spectra. They also compared the maps of different mapmaking codes to see how they performed. They used five mapmaking codes (two destripers and three optimal codes). None of their mapmaking codes makes an attempt to deconvolve the beam from its output map. Therefore all our maps had similar smoothing due to beams and sample integration. This is a complicated smoothing, because every map pixel has its own effective beam. Temperature to polarization cross-coupling due to beam mismatch causes a detectable bias in the TE spectrum of the CMB map. The effects of cooler noise and pointing errors did not appear to be major concerns for the 30 GHz channel. The only essential difference found so far between mapmaking codes that affects accuracy (in terms of residual RMS) is baseline length. All optimal codes give essentially indistiguishable results. A destriper gives the same result as the optimal codes when the baseline is set short enough (Madam). For longer baselines destripers (Springtide and Madam) require less computing resources but deliver a noisier map.

The Planck CTP Working Group; Ashdown, M.A.J.; Baccigalupi, C.; Bartlett, J.G.; Borrill, J.; Cantalupo, C.; de Gasperis, G.; Gorski, K.M.; Hivon, E.; Huffenberger, K.; Keihanen, E.; Keskitalo, R.; Kisner, T.; Hurki-Suonio, H.; Lawrence, C.R.; Natoli, P.; Poutanen, T.; Prezeau, G.; Reinecke, M.; Rocha, G.; Sandri, M.; Stompor, R..; Villa, F.; Wandelt, B.; de Troia, G.

2008-06-19T23:59:59.000Z

379

National Institute of Agricultural Botany  

Science Journals Connector (OSTI)

... D. M. Wills, directed attention to the value of the Institute's system of substations. By means of this organization the Institute is able to make recommendations to farmers ... and Scarborough. There are at present two defective links in the Institute's chain of substationsthe Fens and Walesand the Institute hopes that these defects will shortly be remedied ...

1937-11-13T23:59:59.000Z

380

INSTITUTE ON ASSETS & SOCIAL POLICY  

E-Print Network (OSTI)

INSTITUTE ON ASSETS & SOCIAL POLICY LIVING LONGER ON LESS IN MASSACHUSETTS: THE NEW ECONOMIC (IN)SECURITY OF SENIORS Tatjana Meschede Laura Sullivan Thomas Shapiro #12;About the Institute on Assets and Social Policy The Institute on Assets and Social Policy (IASP), a research institute at the Heller School for Social Policy

Snider, Barry B.

Note: This page contains sample records for the topic "max planck institute" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


381

Argonne Accelerator Institute  

NLE Websites -- All DOE Office Websites (Extended Search)

Mission Mission The mission of the Argonne Accelerator Institute is centered upon the following related goals: Locate next generation accelerator facilities in Northern Illinois Advance accelerator technology Oversee a selected, strategic, lab-wide, and acclaimed accelerator R&D portfolio In order to accomplish the above goals, the institute has established five objectives. These are coupled to programmatic objectives, and are dependent on each other, but they serve to identify important areas for the institute to focus its activities. Educate the "next generation" of accelerator physicists and engineers Work with area Universities to establish Joint Appointments and Adjunct Professorships Identify students Provide research opportunities at Argonne Work with the US Particle Accelerator School

382

Surface Science 430 (1999) L515L520 www.elsevier.nl/locate/susc Surface Science Letters  

E-Print Network (OSTI)

of Science and Technology, 790-784 Pohang, South Korea b Fritz-Haber-Institut der Max-Planck-Gesellschaft, Faradayweg 4-6, 14195 Berlin-Dahlem, Germany Received 14 October 1998; accepted for publication 11 January. This substrate was chosen since the clean W(001)* Corresponding author. Fax: +82-562-279-3099. E-mail address

383

Interaction between hydrogen molecules and metallofullerenes Mina Yoon,1,2,3,a  

E-Print Network (OSTI)

and Zhenyu Zhang1,3 1 Materials Science and Technology Division, Oak Ridge National Laboratory, Oak Ridge, Tennessee 37831, USA 2 Fritz-Haber-Institut der Max-Planck-Gesellschaft, 14195 Berlin, Germany 3 Department have been made in exploring hydrogen as a potential energy carrier for efficient, clean, and renewable

384

Point Defect Configurations of Supersaturated Au Atoms Inside Si  

E-Print Network (OSTI)

, Dhananjay Kumar,, Sokrates T. Pantelides,,# and Stephen J. Pennycook,# Materials Science and Technology Di, Spain, Max Planck Institute of Microstructure Physics, Weinberg 2, 06120 Halle, Germany, and Department of stable silicides in the Au-Si phase diagram suggests growth of clean Si nanowires might be possible

Pennycook, Steve

385

A Cubic Fe4Mo4 Oxo Framework and Its Reversible Four-Electron Redox Chemistry  

Science Journals Connector (OSTI)

Max Planck Institute for Chemical Energy Conversion (formerly Bioinorganic Chemistry), Stiftstrae 34?36, 45470 Mlheim, Germany ... Indeed, a salt with a FeII2FeIII2MoVI4 constellation, [Fe4Mo4](TCNQ)2 (2), could be isolated after treatment with TCNQ. ... data indicate that the binding energies of all the elements in the title compds. ...

Jan P. Falkenhagen; Beatrice Braun; Eckhard Bill; Dominik Sattler; Christian Limberg

2014-07-01T23:59:59.000Z

386

JT-60 Modification Plan for Long Pulse Advanced Tokamak Research  

E-Print Network (OSTI)

JT-60 Modification Plan for Long Pulse Advanced Tokamak Research Colloquium of Max Planck Institute as one step to DEMO · Advanced tokamak researches · Scientific achievements of JT-60 and its phase Tokamak Commercializa tion pease JT-60 Decision system of prototype reactor Electricity Generation

387

Dynamics and Steady States in Excitable Mobile Agent Systems Fernando Peruani1,2  

E-Print Network (OSTI)

. Sibona1,3 1 Max Planck Institute for the Physics of Complex Systems, No¨thnitzer Stra?e 38, 01187 Dresden-agent contact rate (CR) becomes crucial to understand the excitation dynamics, which exhibits three regimes. In an excitable system, agents typically have three states, quies- cent, excited, and refractory, and pass through

Peruani, Fernando

388

The Universe Viewed in Gamma-Rays 1 The Future of the MAGIC Project: Phase II  

E-Print Network (OSTI)

and even become very important. We are trying to quantify the rate of muons which will pass the selection for the MAGIC Collaboration Max-Planck-Institute for Physics, Foehringer Ring 6, 80805 Munich, Germany Abstract will be discussed. 1. Introduction Seven and a half years have passed since the first presentations

Enomoto, Ryoji

389

Review of the formulation of present1 generation stratospheric chemistry climate1  

E-Print Network (OSTI)

of Water and Atmospheric Research, Lauder, New Zealand. 2 Max Planck Institut für Meteorologie, HamburgReview of the formulation of present1 generation stratospheric chemistry climate1 modelsBE647 #12;Review of the formulation of present generation stratospheric chemistry climate models

Wirosoetisno, Djoko

390

arXiv:physics/0603142v117Mar2006 Brownian Motion after Einstein  

E-Print Network (OSTI)

arXiv:physics/0603142v117Mar2006 Brownian Motion after Einstein: Some new applications and new-4000 Roskilde, Denmark 2 Department of Biological Physics, E¨otv¨os Lor´and University (ELTE), H-1117 Budapest, Hungary 3 Max Planck Institute for the Physics of Complex Systems, N¨othnitzer Strasse 38, D

391

Supplement to: The CO2 release and Oxygen uptake from Fossil Fuel Emission  

E-Print Network (OSTI)

, C. Minejima2,4 , H. Mukai2 1 Max Planck Institute for Biogeochemistry, Jena, Germany 2 Center to observations at the station Ochsenkopf in Germany. #12;EDGAR 3.2 usage type Corresponding UN usage type(s) code, refineries, etc.) 0911 0914 0924 121 084 Consumption by mining industry Consumption by biogas plants

Meskhidze, Nicholas

392

Wolfgang Ketterle Education Pre-diploma (Vordiplom), Physics, University of Heidelberg, Germany, 1978  

E-Print Network (OSTI)

Wolfgang Ketterle Education · Pre-diploma (Vordiplom), Physics, University of Heidelberg, Germany, Germany, 1982. · Ph.D., Physics, Ludwig-Maximilians University of Munich and Max-Planck Institute for Quantum Optics, Garching, Germany, 1986. Employment 1982-88 Research assistant (1982-85) and staff

393

The 32nd International Electric Propulsion Conference, Wiesbaden, Germany September 11 15, 2011  

E-Print Network (OSTI)

The 32nd International Electric Propulsion Conference, Wiesbaden, Germany September 11 ­ 15, 2011 1 Electric Propulsion Conference, Wiesbaden · Germany September 11 ­ 15, 2011 K. Matyash1 , Max-Planck-Institut für Plasmaphysik, EURATOM Association, Greifswald, D-17491, Germany R. Schneider2 , Greifswald

394

2, 181212, 2002 The flux of carbonyl  

E-Print Network (OSTI)

, coal combustion, sulfur recovery, etc.), and is removed by terrestrial vegetation, soils, pho-25/181/ c European Geophysical Society 2002 Atmospheric Chemistry and Physics Discussions The flux, 60054 Frankfurt am Main, Germany * now at Max Planck Institute for Chemistry, Mainz, Germany Received: 9

Paris-Sud XI, Université de

395

Atmos. Chem. Phys., 3, 17431757, 2003 www.atmos-chem-phys.org/acp/3/1743/ Atmospheric  

E-Print Network (OSTI)

by an Analytical Scanning Electron Microscope (ASEM) confirm the influence of coal combustion on the carbona- ceousAtmos. Chem. Phys., 3, 1743­1757, 2003 www.atmos-chem-phys.org/acp/3/1743/ Atmospheric Chemistry, and N. Mihalopoulos3 1Department of Biogeochemistry, Max-Planck-Institute for Chemistry, Mainz, Germany

Paris-Sud XI, Université de

396

Astronomy & Astrophysics manuscript no. HUGSv11 c ESO 2014 September 26, 2014  

E-Print Network (OSTI)

Astronomy & Astrophysics manuscript no. HUGSv11 c ESO 2014 September 26, 2014 The Hawk-I UDS for Astronomy, University of Edinburgh, Royal Observatory, Edinburgh EH9 3HJ, UK 3 Department of Physics and Astronomy, Sonoma State University, Rohnert Park, CA, SA 4 Max-Planck-Institut fur extraterrestrische Physik

Faraon, Andrei

397

EUROGRAPHICS 2007 / D. Cohen-Or and P. Slavk (Guest Editors)  

E-Print Network (OSTI)

A Bidirectional Light Field - Hologram Transform Remo Ziegler1, Simon Bucheli1, Lukas Ahrenberg2, Marcus Magnor3, Markus Gross1 1ETH Zurich, Switzerland 2Max-Planck-Institute für Informatik, Germany 3TU Braunschweig the notion of conventional image-based rendering, our framework makes joint use of both light fields

Magnor, Marcus

398

The effect of expertise on the quality of forest standards implementation: The case of FSC forest certification in Russia  

E-Print Network (OSTI)

certification in Russia Olga Maletz a, , Maria Tysiachniouk b,1 a Max Planck Institute for the Study, Office 301, St. Petersburg 191040, Russia a b s t r a c ta r t i c l e i n f o Keywords: Expertise in the forestry sector. Specifically we analyze the experience of two large forest companies in Russia

399

Multi-Class Video Co-Segmentation with a Generative Multi-Video Model Wei-Chen Chiu Mario Fritz  

E-Print Network (OSTI)

Multi-Class Video Co-Segmentation with a Generative Multi-Video Model Wei-Chen Chiu Mario Fritz Max Planck Institute for Informatics, Saarbr¨ucken, Germany {walon,mfritz}@mpi-inf.mpg.de Abstract Video data in videos and recent advances in video segmentation has shown great progress in exploiting these addition

400

Proton MR Spectroscopy at 7 Tesla in the Macaque monkey J. Pfeuffer1  

E-Print Network (OSTI)

Proton MR Spectroscopy at 7 Tesla in the Macaque monkey J. Pfeuffer1 , C. Juchem1 , H. Merkle2 , N was demonstrated to provide significant sensitivity and resolution gains at high magnetic field [1,2]. MR imaging. K. Logothetis1 1 Max Planck Institute for biological Cybernetics, Tuebingen, D, Germany, 2 LFMI, NIH

Jegelka, Stefanie

Note: This page contains sample records for the topic "max planck institute" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


401

Localized 1H MR Spectroscopy in the alert monkey at 7 Tesla J. Pfeuffer1  

E-Print Network (OSTI)

Localized 1H MR Spectroscopy in the alert monkey at 7 Tesla J. Pfeuffer1 , C. Juchem1 , H. Merkle2-voxel 1 H MRS in the alert monkey using a 7 T MR system with a vertical bore. Typically , N. K. Logothetis1 1 Department Physiology of Cognitive Processes, Max Planck Institute

Jegelka, Stefanie

402

Functional MR imaging of the awake monkey in a novel vertical large-bore 7 Tesla setup J. Pfeuffer1  

E-Print Network (OSTI)

Functional MR imaging of the awake monkey in a novel vertical large-bore 7 Tesla setup J. Pfeuffer1 , J. Pauls1 , M. Augath1 , T. Steudel1 , H. Merkle2 , N. K. Logothetis1 1 Max Planck InstituteMRI results in the awake trained monkey (Macaca mulatta) using a novel vertical 7T/60cm MR system are reported

Jegelka, Stefanie

403

A&A manuscript no. (will be inserted by hand later)  

E-Print Network (OSTI)

Max­Planck­Institut f¨ur extraterrestrische Physik, Postfach 1603, D--85740 Garching, Germany 3 ISO for the grating sections are ??=ffi?? ¸ 10000. Any remaining errors in the wavelength scale are dominated is described in Schaeidt et al (1996). Pre­flight the wavelength calibration of the two grat­ ing sections

404

A&A manuscript no. (will be inserted by hand later)  

E-Print Network (OSTI)

source in Orion M.Pohl Max­Planck­Institut f?ur extraterrestrische Physik, Postfach 1603, 85740 Garching and Dermer 1995). In the next section I will show that the observed emission from the Orion region can

Pohl, Martin Karl Wilhelm

405

Organotextile Catalysis  

Science Journals Connector (OSTI)

...1242196 Ji-Woong Lee Thomas Mayer-Gall Klaus Opwis Choong Eui Song Jochen Stefan Gutmann Benjamin List 1Max-Planck-Institut...Catalysis Ji-Woong Lee, Thomas Mayer-Gall, Klaus Opwis, Choong Eui Song, Jochen Stefan Gutmann, Benjamin List Materials/Methods...

Ji-Woong Lee; Thomas Mayer-Gall; Klaus Opwis; Choong Eui Song; Jochen Stefan Gutmann; Benjamin List

2013-09-13T23:59:59.000Z

406

Project funded by the European Union under the 7th Framework Programme  

E-Print Network (OSTI)

Project cost: 4,287,529 Project funding: 3,424,534 Max-Planck-Institut für biologische Kybernetik #12Project funded by the European Union under the 7th Framework Programme http://www.mycopter.eu my a Personal Aerial Transportation System (PATS) #12;http://www.mycopter.eu Rationale for the project Money

407

PHILOSOPHICALMAGAZINEB, 1994, zyxwvutVOL.69, No. 4, 655-669 Plan-view and profile imaging of sulphided platinum particles  

E-Print Network (OSTI)

of sulphided platinum particles By M. A. GRIBELWK~,P. J. F. HARRIS$and J. L. HUTCHISON Department of Materials}faceting of the particles(Harris 1986b).These faceted crystallites provide almost ideal candidates for surface work on specimens of this type (Jefferson and Harris 1988, t Present address: Max-Planck-Institut fur

Harris, Peter J F

408

Introduction to special section on the Phoenix Mission: Landing Site Characterization Experiments, Mission Overviews, and  

E-Print Network (OSTI)

braking strategy. After a safe landing, twin fan-like solar panels are unfurled and provide the energy lander with a science payload inherited from MPL and 2001 instruments gives significant advantages, University of Ottawa, Ottawa, Ontario, Canada. 10 Max Planck Institute for Solar System Research, Katlenburg

Duck, Thomas J.

409

erlangen graduate school in advanced optical technologies  

E-Print Network (OSTI)

to the SAOT. The SAOT provides an interdisciplinary research and education programme in which innovation Centre (BLZ) · Fraunhofer Institute for Integrated Systems and Device Technology (IISB) · Max Planck framework for scientific enterprise with important scope for innovation at the inter- faces between

Fiebig, Peter

410

Plasticity of the human brain " We never use the same brain twice" Arno Villringer and Burkhard Pleger  

E-Print Network (OSTI)

Plasticity of the human brain " We never use the same brain twice" Arno Villringer and Burkhard Pleger Max Planck Institute for Human Brain and Cognitive Sciences, Leipzig Summary With the advent of noninvasive neuroimaging the human brain has become accessible for invivo

411

Atmos. Chem. Phys., 7, 211222, 2007 www.atmos-chem-phys.net/7/211/2007/  

E-Print Network (OSTI)

and the influence of sulfuric acid M. Ehn1, T. Pet¨aj¨a1, H. Aufmhoff2, P. Aalto1, K. H¨ameri1,3, F. Arnold2, A properties of ultrafine aerosol particles in the boreal forest: diurnal variation, solubility 64, 00014 University of Helsinki, Finland 2Max-Planck Institute for Nuclear Physics (MPIK

Boyer, Edmond

412

Project funded by the European Union under the 7th Framework Programme  

E-Print Network (OSTI)

Aerial Transportation System (PATS) Our vision: travel between home and work on short distances 27 for vehicle automation and control Social and technological impact of a PATS 27/06/2011 5Heinrich Bülthoff, Max Planck Institute for Biological Cybernetics Automation of aerial vehicles PAVs should

413

Biogeosciences, 11, 12151259, 2014 www.biogeosciences.net/11/1215/2014/  

E-Print Network (OSTI)

, B. Wehrli15, and F. Wenzhöfer2,3 1Helmholtz Zentrum Geesthacht Center for Materials and Coastal Research, Max-Planck Str. 1, 21502 Geesthacht, Germany 2Alfred Wegener Institute Helmholtz Center for Polar U1987, Perth, WA 6845, Australia fpresent address: Helmholtz Zentrum Geesthacht Center for Materials

Wehrli, Bernhard

414

Peculiar early-type galaxies in the Sloan Digital Sky Survey Stripe82  

Science Journals Connector (OSTI)

......fuelling the starburst, allowing it to then reform a disc. It is possible that the galaxy...Science Foundation, the US Department of Energy, the National Aeronautics and Space Administration...Max-Planck-Institute for Astrophysics (MPA), New Mexico State University, Ohio State University......

Sugata Kaviraj

2010-07-21T23:59:59.000Z

415

Influence of tissue conductivity anisotropy on EEG/MEG field and return current computation in a realistic head model  

E-Print Network (OSTI)

brain using potential differences and/or magnetic fluxes measured non- invasively directly from the head in a realistic head model: A simulation and visualization study using high-resolution finite element modeling C 3493, Salt Lake City, UT 84112, USA c Max Planck Institute for Human Cognitive and Brain Sciences

Utah, University of

416

Supporting Information: Nanoparticle Tension Probes Patterned at the Nanoscale  

E-Print Network (OSTI)

was obtained from a Nanopure water purification system with a UV sterilization unit and showed a resistivity and Biosystems, Max Planck Institute for Intelligent Systems, Stuttgart, Germany Corresponding Author: k%), cytochalasin D ( 98%) were purchased from Sigma-Aldrich (St. Louis, MO) and used without further purification

Salaita, Khalid

417

Curriculum Vitae for Richard Kleeman 1 Education  

E-Print Network (OSTI)

in a coupled ocean-atmosphere model due to atmospheric noise", Tellus A Vol 46, pp529-540. 14. Power S.B., A.B. Power, 1995,"A simple atmospheric model of heat flux for ocean model studies", J. Phys. Oceanogr. Vol 25 Hybrid Coupled Tropi- cal Atmosphere Ocean Model: Sensitivities and Hindcast Skill"; Max Planck Institut

Mohri, Mehryar

418

Two-dimensional Electron Liquid State at Oxide Interfaces J. Mannhart  

E-Print Network (OSTI)

Two-dimensional Electron Liquid State at Oxide Interfaces J. Mannhart Max Planck InstituteAlO3 #12;LaAlO3 - SrTiO3 YBa2Cu3O7 G. Hammerl #12;Interfaces with Standard Semiconductors: Space Charge;Conductance-voltage characteristics It/ Vs Vs were measured using a standard lock-in technique.24 Simulta

Yeh, Nai-Chang

419

International Journal of Primatology ( C 2006) DOI: 10.1007/s10764-005-9013-0  

E-Print Network (OSTI)

and Habitat Use in the Goualougo Triangle, Republic of Congo David Morgan,1 Crickette Sanz,2 Jean Robert in the Republic of Congo, and in an adjacent area in which se- lective logging will take place in the near future University, Wildlife Conservation Society, Congo. 2Max Planck, Institute for Evolutionary Anthropology

420

The ATLAS3D project XXIX. The new look of early-type galaxies and surrounding fields disclosed by extremely deep optical images  

Science Journals Connector (OSTI)

......European Southern Observatory, Karl-Schwarzschild-Str. 2, D-85748 Garching, Germany...Max-Planck-Institut fur Astrophysik, Karl-Schwarzschild-Str. 1, NL-85741 Garching, Germany...obstructing support spider of the telescope mirror (see Fig.-5). As mentioned earlier......

Pierre-Alain Duc; Jean-Charles Cuillandre; Emin Karabal; Michele Cappellari; Katherine Alatalo; Leo Blitz; Frdric Bournaud; Martin Bureau; Alison F. Crocker; Roger L. Davies; Timothy A. Davis; P. T. de Zeeuw; Eric Emsellem; Sadegh Khochfar; Davor Krajnovi?; Harald Kuntschner; Richard M. McDermid; Leo Michel-Dansac; Raffaella Morganti; Thorsten Naab; Tom Oosterloo; Sanjaya Paudel; Marc Sarzi; Nicholas Scott; Paolo Serra; Anne-Marie Weijmans; Lisa M. Young

2015-01-01T23:59:59.000Z

Note: This page contains sample records for the topic "max planck institute" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


421

Results from the Wilkinson Microwave Anisotropy Probe  

Science Journals Connector (OSTI)

......Max-Planck-Institut fur Astrophysik, Karl-Schwarzschild-Strabetae 1, 85740 Garching...WMAP has two back-to-back mirrors to focus the incoming electromagnetic...each other. The size of each mirror is , providing substantially...COBE, which did not have mirrors but only horn antennas. The......

Eiichiro Komatsu; Charles L. Bennett (on behalf of the WMAP science team)

2014-06-01T23:59:59.000Z

422

Spectroscopic study of the open cluster NGC 6811  

Science Journals Connector (OSTI)

......Max-Planck-Institute for Astrophysics, Karl-Schwarzschild-Str. 1, D-85741 Garching, Germany...Hectochelle spectrograph at the Multiple Mirror Telescope and classified 139 of them...Hectochelle spectrograph on the Multiple Mirror Telescope, through 0.19 dex, derived......

J. Molenda-Zakowicz; K. Brogaard; E. Niemczura; M. Bergemann; A. Frasca; T. Arentoft; F. Grundahl

2014-01-01T23:59:59.000Z

423

E Goldschmidt Abstracts 2011  

Science Journals Connector (OSTI)

...KAY-CHRISTIAN EMEIS1, BIRGIT NAGEL1 AND NIKO LAHAJNAR2 1 Institute of Coastal Research, Helmholtz Center Geesthacht, Max-Planck-Str. 1, 21502 Geesthacht, Germany (Kay.emeis@zmaw.de, Birgit.nagel@hzg.de) 2 KlimaCampus, Bundesstr...

424

November 01, 2012 CURRICULUM VITAE  

E-Print Network (OSTI)

of Idaho 2008 Kavli Foundation Fellow, National Academy of Sciences - Alexander von Humboldt Stiftung 2008, PLoS Genetics 2012-2015 Scientific Advisory Committee, Max Planck Institute for Chemical Ecology 2011-2012 Vice President, American Society of Naturalists 2010 Scientific Advisory Committee, Uppsala Centre

Hoekstra, Hopi E.

425

February 2013 CURRICULUM VITAE  

E-Print Network (OSTI)

of Idaho 2008 Kavli Foundation Fellow, National Academy of Sciences - Alexander von Humboldt Stiftung 2008S Genetics 2012-2015 Scientific Advisory Committee, Max Planck Institute for Chemical Ecology 2011-2012 Vice President, American Society of Naturalists 2010 Scientific Advisory Committee, Uppsala Centre

Hoekstra, Hopi E.

426

Interfacial behaviour of Catanionic surfactants Antonio Stocco,*,1,  

E-Print Network (OSTI)

tension, high surface concentration and high viscoelastic compression moduli, as measured with rising the concentration of free surfactant ions (CTA+ ). The equilibrium surface tension is reached faster for non surface tension, multiple light scattering, foam. Present address: Max Planck Institute of Colloids

Boyer, Edmond

427

Nuclear Physics A 687 (2001) 405434 www.elsevier.nl/locate/npe  

E-Print Network (OSTI)

Nuclear Physics A 687 (2001) 405­434 www.elsevier.nl/locate/npe Spectral ergodicity and normal Fisicas, UNAM, Apartado, Postal 48-3, Cuernavaca, Mexico c Max-Planck-Institut für Kernphysik, Postfach reveals that spectral ergodicity is not broken, but that different energy scales of the spectra

Mejía-Monasterio, Carlos

428

The Landscape of the Traveling Salesman Problem Peter F. Stadler y  

E-Print Network (OSTI)

The Landscape of the Traveling Salesman Problem Peter F. Stadler y Max Planck Institut f The landscapes of Traveling Salesman Problems are investigated by ran­ dom walk techniques. The autocorrelation functions for different metrics on the space of tours are calculated. The landscape turns out to be AR(1

Stadler, Peter F.

429

Nonlinear alternating current responses of dipolar fluids J. P. Huang  

E-Print Network (OSTI)

Nonlinear alternating current responses of dipolar fluids J. P. Huang Max Planck Institute Mechanics Group, Laboratory of Computational Engineering, Helsinki University of Technology, P. O. Box 9203-dependent nonlinear dielectric increment of dipolar fluids in nonpolar fluids is often mea- sured by using

Huang, Ji-Ping

430

Effects of molecular rotation in low-energy electron collisions of  

Science Journals Connector (OSTI)

...First studies on the nuclear spin symmetry influencing...to the rovibrational nuclear degrees of freedom...RF) high-energy accelerator at an energy of 5...magnetic storage ring at a vacuum of ca 311mbar. The...Max-Planck Institute of Nuclear Physics in Heidelberg...

2006-01-01T23:59:59.000Z

431

MORTEN H. CHRISTIANSEN Department of Psychology  

E-Print Network (OSTI)

Phone: (607) 255-3834 (dept) Fax: (607) 255-8433 Email: christiansen@cornell.edu Departmental web page for Psycholinguistics, Nijmegen, the Netherlands. 2009 6-week visit at the Max Planck Institute for Psycholinguistics, Nijmegen, the Netherlands. 2007 9-week sabbatical visit in the Department of Developmental and Comparative

432

Prevalence of Small-scale Jets from the Network Structures of the Solar Transition Region and  

E-Print Network (OSTI)

furnace model Funnels from networks Tu et al. 2005 #12;Implication for solar wind origin (II) · Mass lossPrevalence of Small-scale Jets from the Network Structures of the Solar Transition Region-Smithsonian Center for Astrophysics 2Lockheed Martin Solar and Astrophysics Laboratory 3Max Planck Institute

433

Geophys. J. Int. (2008) 173, 793801 doi: 10.1111/j.1365-246X.2008.03764.x GJIPlanetaryscience  

E-Print Network (OSTI)

of Alberta, Edmonton, AB T6G 1V6, Canada 3Physics Division, US Coast Guard Academy, New London, CT 06320, USA 4Max Planck Institute for Solar System Research, 37191 Katlenburg-Lindau, Germany Accepted 2008 of inte- rior heat and reradiated solar energy. Since the net outward heat flow exceeds solar deposition

434

Comparative Microbial Genomics group CenterforBiologicalSequenceanalysisDepartmentofSystemsBiology,TechnicalUniversityofDenmark  

E-Print Network (OSTI)

Comparative Microbial Genomics group CenterforBiologicalSequenceanalysisDepartmentofSystemsBiology,TechnicalUniversityofDenmark Burkholderia Pan-genomics Dave Ussery Max Planck Institut fur Terrestrial Microbiology Marburg, Germany 26 May, 2008 - or - What can we learn from more than 50 sequenced genomes? #12;Comparative Microbial Genomics

Ussery, David W.

435

Potential of metabolomics as a functional genomics tool  

E-Print Network (OSTI)

Potential of metabolomics as a functional genomics tool Raoul J. Bino1,2,3 , Robert D. Hall2 3 Centre for BioSystems Genomics, POB 98, 6700 AB Wageningen, The Netherlands 4 Max-Planck Institute Australian Centre for Plant Functional Genomics, School of Botany, University of Melbourne, Victoria 3010

Wurtele, Eve Syrkin

436

Ann. Geophys., 26, 23832394, 2008 www.ann-geophys.net/26/2383/2008/  

E-Print Network (OSTI)

with the geomagnetic field, and allow energy and momentum to be transferred from the solar wind into the magnetosphere 2008 Annales Geophysicae What is the best method to calculate the solar wind propagation delay? B, University Iasi, Romania 3University of Bergen, Norway *also at: Max-Planck Institute for Solar Systems

Bergen, Universitetet i

437

Argonne Accelerator Institute  

NLE Websites -- All DOE Office Websites (Extended Search)

AAI Home AAI Home Welcome Accelerators at Argonne Mission Organization History Document Collection Conferences & Workshops Beams and Applications Seminar Argonne-Fermilab Collaboration Lee Teng Scholarship Program Useful Links Argonne Accelerator Institute In 2006, Argonne Laboratory Director Robert Rosner formed the AAI as a focal point for accelerator initiatives. The institute works to utilize Argonne's extensive accelerator resources, to enhance existing facilities, to determine the future of accelerator development and construction, and to oversee a dynamic and acclaimed accelerator physics portfolio. More Information for: Members * Students Industrial Collaborators - Working with Argonne Link to: Accelerators for America's Future Upcoming Events and News 4th International Particle Accelerator Conference (IPAC'13)

438

Institut Farman 6eme Journe  

E-Print Network (OSTI)

Institut Farman 6eme Journée Institut Farman Jeudi 22 Novembre 2012 FR3311 CNRS www.farman.ens-cachan.fr #12;Institut Farman Les projets Farman ont donné lieu depuis 2007 à 28 projets dont 10 en cours ASTECH (2 thèses en co-direction LMT/SATIE) #12;Institut Farman L'Institut Farman c'est aussi : Equipex

439

~max0006  

National Nuclear Security Administration (NNSA)

Safety, and lIealth -The NNSA functional leader for ES&H is the Senior ES&H Advisor. This functional area includes all ES&H requirements except nuclear safety...

440

Perimeter Institute Cosmic Acceleration  

E-Print Network (OSTI)

Wayne Hu Perimeter Institute April 2010 Cosmic Acceleration Dark Energy v. Modified Gravity #12;Outline · Dark Energy vs Modified Gravity · Three Regimes of Modified Gravity · Worked (Toy) Models: f 1998 Discovery #12;Mercury or Pluto? General relativity says Gravity = Geometry And Geometry = Matter-Energy

Hu, Wayne

Note: This page contains sample records for the topic "max planck institute" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


441

Cancer Research Beckman Institute  

E-Print Network (OSTI)

Cancer Research Beckman Institute FOR ADVANCED SCIENCE AND TECHNOLOGY #12;T The medical and scientific worlds have known for many years that in order to truly understand and treat cancer, the fight has and cancerous tumors have to first be visualized at the smallest scales possible, and then treated in the most

Illinois at Urbana-Champaign, University of

442

Michigan Institute Science and  

E-Print Network (OSTI)

Michigan Institute for Plasma Science and Engineering Seminar Universal Magnetic Structures Prof. Mark Moldwin Dept. of Atmospheric, Oceanic and Space Sciences University of Michigan Thursday, 19 Nov and provide examples on how thinking about discrete structures can add to our understanding of the solar

Shyy, Wei

443

Pulsed electrospark deposition of MAX phase Cr2AlC based coatings on titanium alloy  

Science Journals Connector (OSTI)

Abstract Coatings with a high amount of MAX phase were obtained onto Ti substrate using the pulsed electrospark deposition (PED) technique and Cr2AlC electrode material (??). The structure and phase formation of the coatings generated at different modes were studied. It was found, that a layer of titanium carbide was formed during the initial stage of the deposition at the interface as a result of chemical reaction between Cr2AlC electrode and Ti substrate which further acts as a diffusion barrier.

E.I. Zamulaeva; E.A. Levashov; T.A. Sviridova; N.V. Shvyndina; M.I. Petrzhik

2013-01-01T23:59:59.000Z

444

Institution Name Institution Name Address Place Zip Notes Website Region  

Open Energy Info (EERE)

Institute for the Built Environment CSU Institute for the Built Institute for the Built Environment CSU Institute for the Built Environment Oval Drive Fort Collins Colorado http www ibe colostate edu Rockies Area Colorado Renewable Energy Collaboratory Colorado Renewable Energy Collaboratory th Street Suite Denver Colorado http www coloradocollaboratory org Rockies Area Colorado School of Mines Colorado Energy Research Institute Colorado School of Mines Colorado Energy Research Institute Illinois Street Golden Colorado http www ceri mines org Rockies Area Denver University International Institute for Environment and Enterprise Denver University International Institute for Environment and Enterprise S University Blvd Denver Colorado http www du edu enviro Research htm Rockies Area EverSealed Windows Inc EverSealed Windows Inc Interlocken Drive Evergreen

445

Mirant: Case 67a: Units 3 & 4 & 5 at Max Load for 12 hours and at Min Load  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

Mirant: Case 67a: Units 3 & 4 & 5 at Max Load for 12 hours and at Mirant: Case 67a: Units 3 & 4 & 5 at Max Load for 12 hours and at Min Load for 12 hours Mirant: Case 67a: Units 3 & 4 & 5 at Max Load for 12 hours and at Min Load for 12 hours Docket No. EO-05-01. Mirant: Case 67a: Units 3 & 4 & 5 at Max Load for 12 hours and at Min Load for 12 hours. Arial photograph showing plant and location of predicted SO2 violations, predicted in 2000. Mirant: Case 67a: Units 3 & 4 & 5 at Max Load for 12 hours and at Min Load for 12 hours More Documents & Publications Mirant Potomac, Alexandria, Virginia: Maximum Impacts Predicted by AERMOD-PRIME, Units 3, 1, 2 SO2 Case Mirant Potomac, Alexandria, Virginia: Maximum Impacts Predicted by AERMOD-PRIME, Units 4, 1, 2 SO2 Case Mirant Potomac, Alexandria, Virginia: Maximum Impacts Predicted by

446

Electronic structure and optical conductivities of 20 MAX-phase compounds  

Science Journals Connector (OSTI)

The electronic structure and optical conductivities of 20 so-called MAX phases Ti3AC2 (A = Al, Si, Ge), Ti2AC (A = Al, Ga, In, Si, Ge, Sn, P, As, S), Ti2AlN, M2AlC (M = V, Nb, Cr), and Tan+1AlCn (n = 1 to 4) are studied using the first-principles orthogonalized linear combination of atomic orbitals (OLCAO) method. The calculated results include total and partial density of states, effective charge on each atom, and quantitative bond order values. Also calculated are directionally resolved interband optical conductivities. By analyzing such results regarding these phases (that have different atomic compositions and layered structures) several important features on structural stability and electrical conductivities are identified and compared with experimental data. We confirm the trend of increasing N(Ef) (total density of states at the Fermi level Ef) as the number of valence electrons of the composing elements increases. The local feature of total density of states (TDOS) near Ef is used to predict structural stability. The calculated effective charge on each atom shows that the M (transition-metal) atoms always lose charge to the X (C or N) atoms, whereas the A-group atoms mostly gain charge but some lose charge. Bond order values are obtained and critically analyzed for all types of interatomic bonds in all the 20 MAX phases.

Yuxiang Mo; Paul Rulis; W. Y. Ching

2012-10-16T23:59:59.000Z

447

Low-energy asymptotic expansion of the Green function for one-dimensional Fokker-Planck and Schrdinger equations  

E-Print Network (OSTI)

We consider Schr\\"odinger equations and Fokker-Planck equations in one dimension, and study the low-energy asymptotic behavior of the Green function using a new method. In this method, the coefficient of the expansion in powers of the wave number can be systematically calculated to arbitrary order, and the behavior of the remainder term can be analyzed on the basis of an expression in terms of transmission and reflection coefficients.

Toru Miyazawa

2011-12-26T23:59:59.000Z

448

High-energy asymptotic expansion of the Green function for one-dimensional Fokker-Planck and Schrdinger equations  

E-Print Network (OSTI)

A new formalism is presented for high-energy analysis of the Green function for Fokker-Planck and Schr\\"odinger equations in one dimension. Formulas for the asymptotic expansion in powers of the inverse wave number are derived, and conditions for the validity of the expansion are studied through the analysis of the remainder term. The short-time expansion of the Green function is also discussed.

Toru Miyazawa

2011-12-26T23:59:59.000Z

449

Application of the non-Markovian Fokker-Planck equation to the resonant activation of a Josephson junction  

Science Journals Connector (OSTI)

The non-Markovian Fokker-Planck equation in the energy variable for a system with a driving force is employed to find the escape rate of a particle in a potential well. The energy-dependent diffusion coefficient is the integral of the spectral densities of the applied force and the velocity of the system. The escape-rate formula is applied to resonant activation of a Josephson junction by a microwave driving current with a good comparison to experimental results.

Ted Hesselroth

1993-07-01T23:59:59.000Z

450

List of all HEP Institutions  

NLE Websites -- All DOE Office Websites (Extended Search)

Top 500 Top 500 HEP and Astrophysics Institutions by Country This document lists the 500 major high-energy physics and astrophysics institutions, sorted by country. Each listing will show a [SPIRES Entry] which gives the full address and phone/fax/url of the institution in addition to links to papers in HEP and people in HEPNAMES. The [Home page], where known, takes you directly to the departmental home page. Alternatively try our INSTITUTIONS search page. This list of the top 500 institutions is chosen by the number of papers from each institution in the past 5 years. Click here for the full list of HEP institutions. Please send any comments, corrections, updates or information on new institutions to: inst@slac.stanford.edu. Last modified at 17:12:32 on 06/30/04.

451

BEEKEEPING INSTITUTE Young Harris College  

E-Print Network (OSTI)

2008 BEEKEEPING INSTITUTE May 15-17 Young Harris College Young Harris, Georgia #12;Young Harris, section comb honey, mead, and beekeeping gadgets. We urge students to participate in the Institute Honey

Delaplane, Keith S.

452

PRITZKER INSTITUTE FOR BIOMEDICAL SCIENCE  

E-Print Network (OSTI)

PRITZKER INSTITUTE FOR BIOMEDICAL SCIENCE AND ENGINEERING Strategic Plan Summary #12;Pritzker Institute for Biomedical Science and Engineering for Strategic Plan Summary | 1 PRITZKER INSTITUTE FOR BIOMEDICAL SCIENCE AND ENGINEERING STRATEGIC PLAN SUMMARY 1. Grow the student body · Provide financial

Heller, Barbara

453

Planck 2015 results. VIII. High Frequency Instrument data processing: Calibration and maps  

E-Print Network (OSTI)

This paper describes the processing applied to the Planck High Frequency Instrument (HFI) cleaned, time-ordered information to produce photometrically calibrated maps in temperature and (for the first time) in polarization. The data from the 2.5 year full mission include almost five independent full-sky surveys. HFI observes the sky over a broad range of frequencies, from 100 to 857 GHz. To get the best accuracy on the calibration over such a large range, two different photometric calibration schemes have been used. The 545 and 857 GHz data are calibrated using models of planetary atmospheric emission. The lower frequencies (from 100 to 353 GHz) are calibrated using the time-variable cosmological microwave background dipole which we call the orbital dipole. This source of calibration only depends on the satellite velocity with respect to the solar system and permits an independent measurement of the amplitude of the CMB solar dipole (3364.5 +/- 0.8 \\mu K) which is 1\\sigma\\ higher than the WMAP measurement wit...

Adam, R; Aghanim, N; Arnaud, M; Ashdown, M; Aumont, J; Baccigalupi, C; Banday, A J; Barreiro, R B; Bartolo, N; Battaner, E; Benabed, K; Benot, A; Benoit-Lvy, A; Bernard, J -P; Bersanelli, M; Bertincourt, B; Bielewicz, P; Bonavera, L; Bond, J R; Borrill, J; Bouchet, F R; Boulanger, F; Bucher, M; Burigana, C; Calabrese, E; Cardoso, J -F; Catalano, A; Challinor, A; Chamballu, A; Chiang, H C; Christensen, P R; Clements, D L; Colombi, S; Colombo, L P L; Combet, C; Couchot, F; Coulais, A; Crill, B P; Curto, A; Cuttaia, F; Danese, L; Davies, R D; Davis, R J; de Bernardis, P; de Rosa, A; de Zotti, G; Delabrouille, J; Delouis, J -M; Dsert, F -X; Diego, J M; Dole, H; Donzelli, S; Dor, O; Douspis, M; Ducout, A; Dupac, X; Efstathiou, G; Elsner, F; Enlin, T A; Eriksen, H K; Falgarone, E; Fergusson, J; Finelli, F; Forni, O; Frailis, M; Fraisse, A A; Franceschi, E; Frejsel, A; Galeotta, S; Galli, S; Ganga, K; Ghosh, T; Giard, M; Giraud-Hraud, Y; Gjerlw, E; Gonzlez-Nuevo, J; Grski, K M; Gratton, S; Gruppuso, A; Gudmundsson, J E; Hansen, F K; Hanson, D; Harrison, D L; Henrot-Versill, S; Herranz, D; Hildebrandt, S R; Hivon, E; Hobson, M; Holmes, W A; Hornstrup, A; Hovest, W; Huffenberger, K M; Hurier, G; Jaffe, A H; Jaffe, T R; Jones, W C; Juvela, M; Keihnen, E; Keskitalo, R; Kisner, T S; Kneissl, R; Knoche, J; Kunz, M; Kurki-Suonio, H; Lagache, G; Lamarre, J -M; Lasenby, A; Lattanzi, M; Lawrence, C R; Jeune, M Le; Leahy, J P; Lellouch, E; Leonardi, R; Lesgourgues, J; Levrier, F; Liguori, M; Lilje, P B; Linden-Vrnle, M; Lpez-Caniego, M; Lubin, P M; Macas-Prez, J F; Maggio, G; Maino, D; Mandolesi, N; Mangilli, A; Martin, P G; Martnez-Gonzlez, E; Masi, S; Matarrese, S; Mazzotta, P; McGehee, P; Melchiorri, A; Mendes, L; Mennella, A; Migliaccio, M; Mitra, S; Miville-Deschnes, M -A; Moneti, A; Montier, L; Moreno, R; Morgante, G; Mortlock, D; Moss, A; Mottet, S; Munshi, D; Murphy, J A; Naselsky, P; Nati, F; Natoli, P; Netterfield, C B; Nrgaard-Nielsen, H U; Noviello, F; Novikov, D; Novikov, I; Oxborrow, C A; Paci, F; Pagano, L; Pajot, F; Paoletti, D; Pasian, F; Patanchon, G; Pearson, T J; Perdereau, O; Perotto, L; Perrotta, F; Pettorino, V; Piacentini, F; Piat, M; Pierpaoli, E; Pietrobon, D; Plaszczynski, S; Pointecouteau, E; Polenta, G; Pratt, G W; Przeau, G; Prunet, S; Puget, J -L; Rachen, J P; Reinecke, M; Remazeilles, M; Renault, C; Renzi, A; Ristorcelli, I; Rocha, G; Rosset, C; Rossetti, M; Roudier, G; Rusholme, B; Sandri, M; Santos, D; Sauv, A; Savelainen, M; Savini, G; Scott, D; Seiffert, M D; Shellard, E P S; Spencer, L D; Stolyarov, V; Stompor, R; Sudiwala, R; Sutton, D; Suur-Uski, A -S; Sygnet, J -F; Tauber, J A; Terenzi, L; Toffolatti, L; Tomasi, M; Tristram, M; Tucci, M; Tuovinen, J; Valenziano, L; Valiviita, J; Van Tent, B; Vielva, P; Villa, F; Wade, L A; Wandelt, B D; Watson, R; Wehus, I K; Yvon, D; Zacchei, A; Zonca, A

2015-01-01T23:59:59.000Z

454

Neutrinos help reconcile Planck measurements with both Early and Local Universe  

E-Print Network (OSTI)

In light of the recent BICEP2 B-mode polarization detection, which implies a large inflationary tensor-to-scalar ratio r_{0.05}=0.2^{+0.07}_{-0.05}, we re-examine the evidence for an extra sterile massive neutrino, originally invoked to account for the tension between the cosmic microwave background (CMB) temperature power spectrum and local measurements of the expansion rate H0 and cosmological structure. With only the standard active neutrinos and power-law scalar spectra, this detection is in tension with the upper limit of rgravitational waves. An extra sterile species with the same energy density as is needed to reconcile the CMB data with H0 measurements can also alleviate this new tension. By combining data from the Planck and ACT/SPT temperature spectra, WMAP9 polarization, H_0, baryon acoustic oscillation and local cluster abundance measurements with BICEP2 data, we find the joint evidence for a sterile massive neutrino increases to DeltaNeff=0.98\\pm 0.26 for the effective number and ms= 0.52\\pm 0.13 eV for the effective mass or 3.8 sigma and 4 sigma evidence respectively. We caution the reader that these results correspond to a joint statistical evidence and, in addition, astrophysical systematic errors in the clusters and H0 measurements, and small-scale CMB data could weaken our conclusions.

Cora Dvorkin; Mark Wyman; Douglas H. Rudd; Wayne Hu

2014-09-17T23:59:59.000Z

455

Self-Consistent Fokker-Planck Treatment Of Particle Distributions in Astrophysical Plasmas  

E-Print Network (OSTI)

High-energy, multi-component plasmas in which pair creation and annihilation, lepton-lepton scattering, lepton-proton scattering, and Comptonization all contribute to establishing the particle and photon distributions, are present in a broad range of compact astrophysical objects. Earlier work has included much of the microphysics needed to account for electron-photon and electron-proton interactions, but little has been done to handle the redistribution of the particles as a result of their Coulomb interaction with themselves in an arbitrary case. Our goal here is to use a Fokker-Planck approach in order to develop a fully self-consistent theory for the interaction of arbitrarily distributed particles and radiation to arrive at an accurate representation of the high-energy plasma in these sources. We conduct several tests representative of two dominant segments of parameter space and discuss physical implications of the non-Maxwellian distribution function. Approximate analytical forms for the electron distribution in the case of strongly non-Maxwellian plasmas are given.

Sergei Nayakshin; Fulvio Melia

1997-05-03T23:59:59.000Z

456

On the significance of power asymmetries in Planck CMB data at all scales  

E-Print Network (OSTI)

We perform an analysis of the CMB temperature data taken by the Planck satellite investigating if there is any significant deviation from cosmological isotropy. We look for differences between two opposite hemispheres with respect to particular directions, comparing with simulations. We apply a mask symmetrized in antipodal directions to avoid possible biases and smoothed on a 10' scale to avoid spurious extra power on small scales induced by sharp edges. We properly take into account of Doppler and aberration effects due to our peculiar velocity and of the anisotropy of the noise, since these effects induce a significant "hemispherical asymmetry". We are thus able to probe scales all the way to $\\ell = 2000$. After such treatment we find no evidence for significant hemispherical anomalies along any of the analyzed directions (i.e., deviations are less than 2$\\sigma$ in the full range of $\\ell$). Then we find results on a "dipolar modulation" of the the power spectrum of amplitude $A_{mod}$. Along the most as...

Quartin, Miguel

2014-01-01T23:59:59.000Z

457

Constraining models of $f(R)$ gravity with Planck and WiggleZ power spectrum data  

E-Print Network (OSTI)

In order to explain cosmic acceleration without invoking "dark" physics, we consider $f(R)$ modified gravity models, which replace the standard Einstein-Hilbert action in General Relativity with a higher derivative theory. We use data from the WiggleZ Dark Energy survey to probe the formation of structure on large scales which can place tight constraints on these models. We combine the large-scale structure data with measurements of the cosmic microwave background from the Planck surveyor. After parameterising the modification of the action using the Compton wavelength parameter $B_0$, we constrain this parameter using ISiTGR, assuming an initial non-informative log prior probability distribution of this cross-over scale. We find that the addition of the WiggleZ power spectrum provides the tightest constraints to date on $B_0$ by an order of magnitude, giving ${\\rm log}_{10}(B_0) < -4.07$ at 95% confidence limit. Finally, we test whether the effect of adding the lensing amplitude $A_{\\rm Lens}$ and the sum...

Dossett, Jason; Parkinson, David

2014-01-01T23:59:59.000Z

458

Constraining models of $f(R)$ gravity with Planck and WiggleZ power spectrum data  

E-Print Network (OSTI)

In order to explain cosmic acceleration without invoking "dark" physics, we consider $f(R)$ modified gravity models, which replace the standard Einstein-Hilbert action in General Relativity with a higher derivative theory. We use data from the WiggleZ Dark Energy survey to probe the formation of structure on large scales which can place tight constraints on these models. We combine the large-scale structure data with measurements of the cosmic microwave background from the Planck surveyor. After parameterising the modification of the action using the Compton wavelength parameter $B_0$, we constrain this parameter using ISiTGR, assuming an initial non-informative log prior probability distribution of this cross-over scale. We find that the addition of the WiggleZ power spectrum provides the tightest constraints to date on $B_0$ by an order of magnitude, giving ${\\rm log}_{10}(B_0) < -4.07$ at 95% confidence limit. Finally, we test whether the effect of adding the lensing amplitude $A_{\\rm Lens}$ and the sum of the neutrino mass $\\sum m_\

Jason Dossett; Bin Hu; David Parkinson

2014-01-16T23:59:59.000Z

459

An Efficient Fokker-Planck Solver and its Application to Stochastic Particle Acceleration in Galaxy Clusters  

E-Print Network (OSTI)

Particle acceleration by turbulence plays a role in many astrophysical environments. The non- linear evolution of the underlying cosmic-ray spectrum is complex and can be described by a Fokker-Planck equation, which in general has to be solved numerically. We present here an implementation to compute the evolution of a cosmic-ray spectrum coupled to turbulence considering isotropic particle pitch-angle distributions and taking into account the relevant particle energy gains and losses. Our code can be used in run time and post-processing to very large astrophysical fluid simulations. We also propose a novel method to compress cosmic- ray spectra by a factor of ten, to ease the memory demand in very large simulations. We show a number of code tests, which firmly establish the correctness of the code. In this paper we focus on relativistic electrons, but our code and methods can be easily extended to the case of hadrons. We apply our pipeline to the relevant problem of particle acceleration in galaxy clusters. ...

Donnert, Julius

2014-01-01T23:59:59.000Z

460

return 2i + 1 Max-heap property is A[Parent(i)] A[i] for  

E-Print Network (OSTI)

[Parent(i)] A[i] for every node i other than the root. Max-Heapify(A, i) l Left(i) r Right(i) if l heap1 Heapsort Parent(i) return i/2 Left(i) return 2i Right(i) return 2i + 1 Max-heap property is A-size[A] and A[l] > A[i] then largest l else largest i if r heap-size[A] and A[r] > A[largest] then largest r

Bylander, Tom

Note: This page contains sample records for the topic "max planck institute" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


461

Form:Research Institution | Open Energy Information  

Open Energy Info (EERE)

Institution Jump to: navigation, search Add a Research or Development Institution Input your research or development institution name below to add to the registry. If your research...

462

Home About Thomson Reuters Press Room Contact Us ScienceWatch Home  

E-Print Network (OSTI)

: Max Planck Inst Extraterr Phys, Postfach 1603, D-85740 Garching, Germany. Max Planck Inst Extraterr of the interstellar dust, radiation, and magnetic fields, and improved particle and nuclear cross-section data

Moskalenko, Igor V.

463

Cold Gas Traps for Ice Particle Formation  

Science Journals Connector (OSTI)

...GKSS-Forschungszentrum, Max-Planck-Strasse 1, D-21502 Geesthacht, Germany. Water, with the characteristic angular structure...GKSS-Forschungszentrum, Max-Planck-Strabetae 1, D-21502 Geesthacht, Germany. *To whom correspondence should be addressed...

S. Bauerecker; B. Neidhart

1998-12-18T23:59:59.000Z

464

Multiple equilibria on planet Dune: climatevegetation dynamics on a sandy planet  

E-Print Network (OSTI)

Torino, Torino, Italy; 2 International Max Planck Research School on Earth System Modelling, Hamburg.cresto-aleina@zmaw.de $Now at: International Max Planck Research School on Earth System Modelling, H

D'Andrea, Fabio

465

Argonne Accelerator Institute  

NLE Websites -- All DOE Office Websites (Extended Search)

Fermilab Collaboration Fermilab Collaboration Lee Teng Scholarship Program Useful Links The Argonne Accelerator Institute Historical Document Collection Document Access Guide The documents in this collection are held in several repositories, some of which have restricted access. This guide explains the different types of access, and specifies the access levels for each repository. Repositories Name Access Argonne National Laboratory Document Open Access Argonne Research Library Hard Copy Only Beam Dynamics Newsletter Open Access DOE Information Bridge Open Access IEEE Xplore Library Subscription Required JACoW Open Access Journal of Applied Physics Subscription Required Nuclear Instruments & Methods in Physics Research, Section A Subscription Required Physical Review A Subscription Required

466

www.wapa.gov/sn/environment/Docs/FINAL MAX OBN CX 10-11-2011.pdf  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

Maxwell - Maxwell - O'Banion opaw Requested By: David Young Date Submitted: 9/1112011 Descl'iption of the Projcct: Purpose and Need Mail Code: N1410 Phone: 916-353-4542 Date Required: 9/20/2011 The Western Area Power Administration (Western), Sierra Nevada Region (SNR), is responsible for the operation and maintenance (O&M) of federally owned and operated transmission lines, Switchyards, and facilities throughout California. Western and Reclamation must comply with the National Electric Safety Code, Western States Coordinating Council (WECC), and internal directives for protecting human safety, the physical environment, and maintaining the reliable operation of the transmission system. Western is proposing to put Optical Oround Wire (OPOW) on its existing Maxwell O'Banion (MAX-OBN) transmission line. The need for

467

2012 CERTS R&M Peer Review - Dynamic Energy and Environmental Dispatch - Max Zhang  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

Dispatch: Dispatch: Achieving co-benefits of power systems reliability and air quality K. Max Zhang, Richard Schuler, Monica Nguyen, Crystal Chen, Santiago Palacio, and Keenan Valentine Acknowledgement: Collaborations with Mike Swider and Wesley Hall at NYISO; Valuable discussions with Tim Mount, Bill Schulze, Bob Thomas, Dan Shawhan and Ray Zimmerman. High Electric Demand Days (HEDD): A "peak" problem * Heat Waves * Power Systems - Reliability is compromised - Cost of electricity is high: expensive peaking generators * Environment - High ozone air pollution - Double threats to public health: heat and air pollution New York City Temperature 81 89 84 94 94 88 93 93 94 89 96 100 Washington DC Metropolitan Area June 2012 July 2012 Get Creative!

468

Curriculum vitae Bernd Knll  

E-Print Network (OSTI)

Curriculum vitae Bernd Knöll Schulbildung 1985 ­ 1992 Max-Planck-Gymnasium Gro?-Umstadt Zivildienst

Ulm, Universität

469

E-Print Network 3.0 - abfallhaltung von natuerlicher Sample Search...  

NLE Websites -- All DOE Office Websites (Extended Search)

Universitt Hamburg Summary: Prof. Dr. Hans von Storch GKSS-Forschungszentrum Geesthacht Max-Planck-Strae 21502 Geesthacht Prof. Dr... - - - - - - - - - - - - - - - - - -...

470

Matthias Zahn1,2 , Ralf Weisse1  

E-Print Network (OSTI)

for Coastal Research, MaxPlanckStr.1, 21502 Geesthacht, Germany #12;Outline: · Introduction · Reconstruction

Zahn, Matthias

471

Remote Sens. 2014, 6, 4190-4216; doi:10.3390/rs6054190 remote sensing  

E-Print Network (OSTI)

Brockmann Consult, Max-Planck-Str. 2, 21502 Geesthacht, Germany; E-Mails: tom.block@brockmann-consult.de (T

Myneni, Ranga B.

472

meteorological synthesizing centre -east Convention on Long-Range Transboundary Air Pollution  

E-Print Network (OSTI)

of Hydrophysics Max-Planck-Strasse 1 D-21502 Geesthacht GERMANY tel: 49 41 52871847; fax: 49 41 52871888 e

473

Atmos. Chem. Phys., 11, 47794787, 2011 www.atmos-chem-phys.net/11/4779/2011/  

E-Print Network (OSTI)

, Stellenbosch 7599, South Africa 3GKSS Forschungszentrum Geesthacht GmbH, Max-Planck-Strasse, 21502 Geesthacht

Meskhidze, Nicholas

474

J A H R E S B E R I C H T | A N N U A L R E P O R T Vorwort des Prsidenten  

E-Print Network (OSTI)

2 0 1 0 J A H R E S B E R I C H T | A N N U A L R E P O R T #12;Vorwort des Präsidenten Lese, soziale Interaktion und Solidarität kooPerationsProgramme Partnergruppen Max Planck Center Max Planck Forschungsinitiativen nachwuchsFörderung Minerva-Programm Max-Planck-Forschungsgruppen International Max Planck Research

Falge, Eva

475

Boride-based nano-laminates with MAX-phase-like behaviour  

SciTech Connect

MAX-phases being usually composed of transition metals, group A elements and carbon/nitrogen are considered interesting materials for many applications because of their tremendous bulk modulus, 'reversible' plasticity, and machinability. This is mainly due to their unique kind of bonding comprising covalent, ionic as well as metallic bonds providing 'easy' planes of rupture and deformability due to the layered crystal structures. In transition metal boride systems, similar types of bonding are available. In particular the W{sub 2}B{sub 5}-structure type and its stacking variations allow the synthesis of strongly layered crystal structures exhibiting unique delamination phenomena. The paper presents ab initio calculations showing the similarities of bonding between the ternary carbides and the corresponding ternary or quaternary borides. Formation of boride-based nano-laminates from auxiliary liquid phases, from the melt as well as during sintering and precipitation from supersaturated solid solutions will be discussed by means of SEM and TEM studies. The role of impurities weakening the interlayer bonding will be addressed in particular. The pronounced cleavage parallel to the basal plane gives rise for crack deflection and pull-out mechanisms if the laminates are dispersed in brittle matrices such as boron carbide, silicon carbide or other transition metal borides. - Graphical abstract: Some transition metal borides crystallise in a layered structure of alternating stacks of metal and boron atoms giving rise for strongly anisotropic properties. Their preferred cleavage parallel and the deformability perpendicular to the basal plan are similar to the peculiar mechanical behaviour recently described for MAX-phases. Ab initio calculations of the crystal structure prove the weak bonds between the layers for a variety of borides which can be used to reinforce ceramic materials on a nano-scale level.

Telle, Rainer [Institut fuer Gesteinshuettenkunde (Mineral Engineering), Chair of Ceramics and Refractory Materials, RWTH Aachen, Mauerstrasse 5, D-52056 Aachen (Germany)]. E-mail: telle@ghi.rwth-aachen.de; Momozawa, Ai [Institut fuer Gesteinshuettenkunde (Mineral Engineering), Chair of Ceramics and Refractory Materials, RWTH Aachen, Mauerstrasse 5, D-52056 Aachen (Germany); Music, Denis [Materials Chemistry, RWTH Aachen (Germany); Schneider, Jochen M. [Materials Chemistry, RWTH Aachen (Germany)

2006-09-15T23:59:59.000Z

476

Property:OpenEI/UtilityRate/DemandRateStructure/Tier2Max | Open Energy  

Open Energy Info (EERE)

Max" Max" Showing 25 pages using this property. (previous 25) (next 25) 2 2ed23a51-907f-47a4-aa12-930fdab46ff6 + 100 + 2ed23a51-907f-47a4-aa12-930fdab46ff6 + 100 + 2ed23a51-907f-47a4-aa12-930fdab46ff6 + 100 + 3 33829b61-e8a8-4227-9d74-c6d82b9a7439 + 5,000 + 33829b61-e8a8-4227-9d74-c6d82b9a7439 + 5,000 + 33829b61-e8a8-4227-9d74-c6d82b9a7439 + 5,000 + 4 41b62cce-5d88-4f82-9cec-9def23ca54f0 + 5,000 + 41b62cce-5d88-4f82-9cec-9def23ca54f0 + 5,000 + 41b62cce-5d88-4f82-9cec-9def23ca54f0 + 5,000 + 4b524791-bef2-49b1-850b-458730755203 + 20 + 4b524791-bef2-49b1-850b-458730755203 + 3 + 4b524791-bef2-49b1-850b-458730755203 + 24 + 4b524791-bef2-49b1-850b-458730755203 + 3 + 4b524791-bef2-49b1-850b-458730755203 + 4 + 4b524791-bef2-49b1-850b-458730755203 + 4 + 4b524791-bef2-49b1-850b-458730755203 + 5 +

477

DOE Solar Decathlon: New York Institute of Technology: Instituting  

NLE Websites -- All DOE Office Websites (Extended Search)

New York Institute of Technology's solar house in its permanent location at the U.S. Merchant Marine Academy. New York Institute of Technology's solar house in its permanent location at the U.S. Merchant Marine Academy. Enlarge image Green Machine/Blue Space relies on a hydrogen fuel cell to convert and store energy collected by the house's photovoltaic system. (Courtesy of Kevin Rodgers/U.S. Merchant Marine Academy) Who: New York Institute of Technology What: Green Machine/ Blue Space Where: U.S. Merchant Marine Academy 300 Steamboat Road Kings Point, NY 11024 Map This House Public tours: Not available Solar Decathlon 2005 New York Institute of Technology: Instituting Technology New York Institute of Technology partnered with the U.S. Merchant Marine Academy to develop a solar-powered house for the U.S. Department of Energy Solar Decathlon 2005. The house, called Green Machine/Blue Space, was

478

Institution Name Institution Name Address Place Zip Notes Website Region  

Open Energy Info (EERE)

Institution Name Institution Name Address Place Zip Notes Website Region Institution Name Institution Name Address Place Zip Notes Website Region ARCH Venture Partners Texas ARCH Venture Partners Texas Bridgepoint Parkway Bldg Suite Austin Texas http www archventure com Texas Area ARCH Venture Partners Washington ARCH Venture Partners Washington Second Avenue Suite Seattle Washington http www archventure com Pacific Northwest Area African Wind Energy Association South Africa African Wind Energy Association South Africa South Africa http www afriwea org en south africa htm Alternative Energy Institute Alternative Energy Institute russell long blvd Canyon Texas http www windenergy org Texas Area Applied Process Engineering Laboratory Applied Process Engineering Laboratory Hills Street Suite Richland Washington http www apel org

479

Tokyo Institute of Technology Tokyo Institute of Technology  

E-Print Network (OSTI)

Tokyo Institute of Technology 2004 #12; Tokyo Institute of Technology k O(n-k/2) (Efron et al 1996) 2O(B) (Shimodaira 2002, 2004) O(B) #12; Tokyo Institute of Technology of Technology 1 2 3 4 5 1 2 3 4 5 1 2 3 4 5 1 23 4 5 1 2 3 4 5 1 2 3 4 5 1 2 3 4 5 1 23 4 5 1 2 3 4 5

Shimodaira, Hidetoshi

480

Minority Educational Institution Student Partnership Program...  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

Development Minority Educational Institution Student Partnership Program (MEISPP) Minority Educational Institution Student Partnership Program (MEISPP) Our Minority Educational...

Note: This page contains sample records for the topic "max planck institute" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


481

Joint Genome Institute's Automation Approach and History  

E-Print Network (OSTI)

Joint Genome Institutes Automation Approach and Historythroughput environment; automation does not necessarilyissues Islands of Automation modular instruments with

Roberts, Simon

2006-01-01T23:59:59.000Z

482

Plumbing Manufacturer's Institute Ex Parte Communication Regarding...  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

Plumbing Manufacturer's Institute Ex Parte Communication Regarding Showerheads Plumbing Manufacturer's Institute Ex Parte Communication Regarding Showerheads Letter to Department...

483

Structure of pre-Supervisory Committee Meeting (PRE-SCM) report: Abstract of work to date (250 words max)  

E-Print Network (OSTI)

Appendix B Structure of pre-Supervisory Committee Meeting (PRE-SCM) report: Abstract of work to date (250 words max) An abstract of the work to date, providing general background and explaining how the work fits in the field of your project. This abstract can be very similar to the one submitted

Woodgett, Jim

484

Making Maps from Planck LFI 30GHz Data with Asymmetric Beams and Cooler Noise  

E-Print Network (OSTI)

The Planck satellite will observe the full sky at nine frequencies from 30 to 857 GHz. The goal of this paper is to examine the effects of four realistic instrument systematics in the 30 GHz frequency maps: non-axially-symmetric beams, sample integration, sorption cooler noise, and pointing errors. We simulated one year long observations of four 30 GHz detectors. The simulated timestreams contained CMB, foreground components (both galactic and extra-galactic), instrument noise (correlated and white), and the four instrument systematic effects. We made maps from the timelines and examined the magnitudes of the systematics effects in the maps and their angular power spectra. We also compared the maps of different mapmaking codes to see how they performed. We used five mapmaking codes (two destripers and three optimal codes). None of our mapmaking codes makes an attempt to deconvolve the beam from its output map. Therefore all our maps had similar smoothing due to beams and sample integration. Temperature to polarization cross-coupling due to beam mismatch causes a detectable bias in the TE spectrum of the CMB map. The effects of cooler noise and pointing errors did not appear to be major concerns for the 30 GHz channel. The only essential difference found so far between mapmaking codes that affects accuracy (in terms of residual RMS) is baseline length. All optimal codes give essentially indistinguishable results. A destriper gives the same result as the optimal codes when the baseline is set short enough. For longer baselines destripers require less computing resources but deliver a noisier map.

M. A. J. Ashdown; C. Baccigalupi; J. G. Bartlett; J. Borrill; C. Cantalupo; G. de Gasperis; G. de Troia; K. M. Gorski; E. Hivon; K. Huffenberger; E. Keihanen; R. Keskitalo; T. Kisner; H. Kurki-Suonio; C. R. Lawrence; P. Natoli; T. Poutanen; G. Prezeau; M. Reinecke; G. Rocha; M. Sandri; R. Stompor; F. Villa; B. Wandelt

2009-04-09T23:59:59.000Z

485

Homogenization of the Poisson-Nernst-Planck Equations for Ion Transport in Charged Porous Media  

E-Print Network (OSTI)

Effective Poisson-Nernst-Planck (PNP) equations are derived for macroscopic ion transport in charged porous media under periodic fluid flow by an asymptotic multi-scale expansion with drift. The microscopic setting is a two-component periodic composite consisting of a dilute electrolyte continuum (described by standard PNP equations) and a continuous dielectric matrix, which is impermeable to the ions and carries a given surface charge. Four new features arise in the upscaled equations: (i) the effective ionic diffusivities and mobilities become tensors, related to the microstructure; (ii) the effective permittivity is also a tensor, depending on the electrolyte/matrix permittivity ratio and the ratio of the Debye screening length to the macroscopic length of the porous medium; (iii) the microscopic fluidic convection is replaced by a diffusion-dispersion correction in the effective diffusion tensor; and (iv) the surface charge per volume appears as a continuous "background charge density", as in classical membrane models. The coefficient tensors in the upscaled PNP equations can be calculated from periodic reference cell problems. For an insulating solid matrix, all gradients are corrected by the same tensor, and the Einstein relation holds at the macroscopic scale, which is not generally the case for a polarizable matrix, unless the permittivity and electric field are suitably defined. In the limit of thin double layers, Poisson's equation is replaced by macroscopic electroneutrality (balancing ionic and surface charges). The general form of the macroscopic PNP equations may also hold for concentrated solution theories, based on the local-density and mean-field approximations. These results have broad applicability to ion transport in porous electrodes, separators, membranes, ion-exchange resins, soils, porous rocks, and biological tissues.

Markus Schmuck; Martin Z. Bazant

2014-07-14T23:59:59.000Z

486

DOE SciDACs Earth System Grid Center for Enabling Technologies Final Report for University of Southern California Information Sciences Institute  

SciTech Connect

The mission of the Earth System Grid Federation (ESGF) is to provide the worldwide climate-research community with access to the data, information, model codes, analysis tools, and intercomparison capabilities required to make sense of enormous climate data sets. Its specific goals are to (1) provide an easy-to-use and secure web-based data access environment for data sets; (2) add value to individual data sets by presenting them in the context of other data sets and tools for comparative analysis; (3) address the specific requirements of participating organizations with respect to bandwidth, access restrictions, and replication; (4) ensure that the data are readily accessible through the analysis and visualization tools used by the climate research community; and (5) transfer infrastructure advances to other domain areas. For the ESGF, the U.S. Department of Energys (DOEs) Earth System Grid Center for Enabling Technologies (ESG-CET) team has led international development and delivered a production environment for managing and accessing ultra-scale climate data. This production environment includes multiple national and international climate projects (such as the Community Earth System Model and the Coupled Model Intercomparison Project), ocean model data (such as the Parallel Ocean Program), observation data (Atmospheric Radiation Measurement Best Estimate, Carbon Dioxide Information and Analysis Center, Atmospheric Infrared Sounder, etc.), and analysis and visualization tools, all serving a diverse user community. These data holdings and services are distributed across multiple ESG-CET sites (such as ANL, LANL, LBNL/NERSC, LLNL/PCMDI, NCAR, and ORNL) and at unfunded partner sites, such as the Australian National University National Computational Infrastructure, the British Atmospheric Data Centre, the National Oceanic and Atmospheric Administration Geophysical Fluid Dynamics Laboratory, the Max Planck Institute for Meteorology, the German Climate Computing Centre, the National Aeronautics and Space Administration Jet Propulsion Laboratory, and the National Oceanic and Atmospheric Administration. The ESGF software is distinguished from other collaborative knowledge systems in the climate community by its widespread adoption, federation capabilities, and broad developer base. It is the leading source for present climate data holdings, including the most important and largest data sets in the globalclimate community, andassuming its development continueswe expect it to be the leading source for future climate data holdings as well. Recently, ESG-CET extended its services beyond data-file access and delivery to include more detailed information products (scientific graphics, animations, etc.), secure binary data-access services (based upon the OPeNDAP Data Access Protocol), and server-side analysis. The latter capabilities allow users to request data subsets transformed through commonly used analysis and intercomparison procedures. As we transition from development activities to production and operations, the ESG-CET team is tasked with making data available to all users seeking to understand, process, extract value from, visualize, and/or communicate it to othersthis is of course if funding continues at some level. This ongoing effort, though daunting in scope and complexity, would greatly magnify the value of numerical climate model outputs and climate observations for future national and international climate-assessment reports. The ESG-CET team also faces substantial technical challenges due to the rapidly increasing scale of climate simulation and observational data, which will grow, for example, from less than 50 terabytes for the last Intergovernmental Panel on Climate Change (IPCC) assessment to multiple Petabytes for the next IPCC assessment. In a world of exponential technological change and rapidly growing sophistication in climate data analysis, an infrastructure such as ESGF must constantly evolve if it is to remain relevant and useful.

Chervenak, Ann Louise [University of Southern California] [University of Southern California

2013-12-19T23:59:59.000Z

487

Partnering Institution Name Partnering Institution Name Place Type  

Open Energy Info (EERE)

Partnering Institution Name Partnering Institution Name Place Type Partnering Institution Name Partnering Institution Name Place Type of Partnership Partner Center Partner Year Partner Description Link Technologies Technologies North Lexington Massachusetts Incubator National Center for Photovoltaics M M St Paul Minnesota CRADA http www nrel gov pv pv manufacturing html A O Smith A O Smith Milwaukee Wisconsin Test Evaluation Partner Electricity Resources Building Systems Integration A123Systems A123Systems Watertown Massachusetts CRADA Transportation Technologies and Systems http www nrel gov news press html AAON AAON Tulsa Oklahoma Test Evaluation Partner Electricity Resources Building Systems Integration AQUA Products AQUA Products Prosperity South Carolina Test Evaluation Partner Electricity Resources Building Systems Integration

488

Institution Name Institution Name Address Place Zip Notes Website...  

Open Energy Info (EERE)

IEn Institute of Power Engineering IEn Warsaw Poland http www ien com pl home Jordan National Energy Research Center Jordan National Energy Research Center P O Box Al...

489

Argonne Accelerator Institute  

NLE Websites -- All DOE Office Websites (Extended Search)

Welcome Welcome In 2006, Argonne laboratory director Robert Rosner formed the AAI as a focal point for accelerator initiatives. The institute works to utilize Argonne's extensive accelerator resources, to enhance existing facilities, to determine the future of accelerator development and construction, and to oversee a dynamic and acclaimed accelerator physics portfolio. I invite you to look around the content of this web site. Accelerators at Argonne describes our rich heritage in this field, particularly with respect to the development and support of user facilities. Initiatives describes the things we are hoping to do, and Research & Development discusses our research portfolio. If you are a graduate or undergraduate student wishing to pursue a career in accelerator science or technology, please see Educational

490

Argonne Accelerator Institute  

NLE Websites -- All DOE Office Websites (Extended Search)

ZGS -- Zero Gradient Synchrotron (operation: 1963 - 1979) ZGS -- Zero Gradient Synchrotron (operation: 1963 - 1979) The ZGS was a 12 GeV weak-focusing proton synchrotron. It was the first high energy physics accelerator located between the U.S. coasts. The ZGS was also the first synchrotron to accelerate spin polarized protons and the first to use H-minus injection. Other noteworthy features of the ZGS program were the large number of university-based users and the pioneering development of large superconducting magnets for bubble chambers and beam transport. References - Document Access Guide History of the ZGS, Argonne, 1979, American Institute of Physics, AIP Conference Proceedings No. 60 (1980). (Located in the Argonne Research Library) High Energy Physics at Argonne National Laboratory, A. Crewe, R.

491

Argonne Accelerator Institute  

NLE Websites -- All DOE Office Websites (Extended Search)

The Argonne Accelerator History Document Collection The Argonne Accelerator History Document Collection The Argonne Accelerator Institute (AAI) has established a special collection of archived documents which describe notable Argonne accelerator work of the past 50 years. A list of such Argonne Accelerator Projects is given below. Each project is described briefly, with links to archived documents in this collection. This collection includes important Argonne accelerator documents which may have become difficult to locate, as well as ones which have broad scope. In keeping with its historical purpose, this collection only covers work done 10 or more years ago. Many of the listed documents are available online. We hope to make more of them available online in the future. [For several of the projects, interesting additional online documents can be found by

492

Cyclotron Institute Upgrade Project  

SciTech Connect

The Cyclotron Institute at Texas A&M University has upgraded its accelerator facilities to extend research capabilities with both stable and radioactive beams. The upgrade is divided into three major tasks: (1) re-commission the K-150 (88) cyclotron, couple it to existing beam lines to provide intense stable beams into the K-500 experimental areas and use it as a driver to produce radioactive beams; (2) develop light ion and heavy ion guides for stopping radioactive ions created with the K-150 beams; and (3) transport 1+ ions from the ion guides into a charge-breeding electron-cyclotron-resonance ion source (CB-ECR) to produce highly-charged radioactive ions for acceleration in the K-500 cyclotron. When completed, the upgraded facility will provide high-quality re-accelerated secondary beams in a unique energy range in the world.

Clark, Henry [Texas A& M University; Yennello, Sherry [Texas A& M University; Tribble, Robert [Texas A& M University

2014-08-26T23:59:59.000Z

493

J A H R E S B E R I C H T | A N N U A L R E P O R T VORWORT DES PRSIDENTEN  

E-Print Network (OSTI)

J A H R E S B E R I C H T | A N N U A L R E P O R T 2 0 0 6 #12;VORWORT DES PR?SIDENTEN FOREWORD COOPERATION PROGRAMS Partnergruppen Partner Groups Max Planck Fellows Max Planck Fellows Kooperation mit-Program Selbständige Nachwuchsgruppen Independent Junior Research Groups International Max Planck Research

Falge, Eva

494

Accounting Fraud and Institutional Investors.  

E-Print Network (OSTI)

??This dissertation examines institutional investors' trading behavior in a sample of 322 firms alleged in Accounting, Auditing, and Enforcement Releases to have manipulated their accounting (more)

Larson, Chad R.

2008-01-01T23:59:59.000Z

495

Research and Institutional Integrity Office  

NLE Websites -- All DOE Office Websites (Extended Search)

The Research and Institutional Integrity Office (RIIO) serves as a focal point for ethics and compliance assurance at the Berkeley Lab in three main areas of responsibility:...

496

Fundamental Interactions - Research - Cyclotron Institute  

NLE Websites -- All DOE Office Websites (Extended Search)

Cyclotron Institute, but also exploit the facilities at the University of Jyvaskyla in Finland and at the TRIUMF Laboratory in Canada. Nuclear reactions can be used to synthesize...

497

Institut fr Werkzeugmaschinen und Fabrikbetrieb  

E-Print Network (OSTI)

Institut für Werkzeugmaschinen und Fabrikbetrieb Fachgebiet Montagetechnik und Fabrikbetrieb Univ h/Monat) Ausschreibungsnummer: MF-13-RH-01 Die Arbeiten im Fachgebiet Montagetechnik und

Berlin,Technische Universität

498

Continuous Change Institutional Change Principle  

Energy.gov (U.S. Department of Energy (DOE))

Because it takes time to establish institutional change, Federal agencies need multiyear plans that continuously work to achieve, reinforce, and improve significant and persistent sustainability...

499

News Releases | Critical Materials Institute  

NLE Websites -- All DOE Office Websites (Extended Search)

Releases CMI hosts EU, Japan to discuss global critical materials strategy, September 10, 2014 Five Critical Materials Institute researchers named Most Influential Scientific Minds...

500

SKIN CANCER INSTITUTE THE CANCER INSTITUTES AT NORTHWESTERN MEDICINE  

E-Print Network (OSTI)

SKIN CANCER INSTITUTE THE CANCER INSTITUTES AT NORTHWESTERN MEDICINE Melanoma The Most Lethal Form advances in nanotechnology to increase our understanding of melanoma and to develop new tools into controllable cells or target them for destruction. Investigators also are using nanotechnology to understand

Engman, David M.