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1

Wakefield Breakdown Test of a Diamond-Loaded Accelerating Structure  

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

WAKEFIELD BREAKDOWN TEST OF A DIAMOND-LOADED ACCELERATING STRUCTURE S. Antipov, C. Jing, A. Kanareykin, P. Schoessow Euclid TechLabs LLC, Solon, OH, 44139 USA M. Conde, W. Gai, S....

2

Wakefield Breakdown Test of a Diamond-loaded Accelerating Structure...  

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

WAKEFIELD BREAKDOWN TEST OF A DIAMOND-LOADED ACCELERATING STRUCTURE AT THE AWA S. Antipov, C. Jing, P. Schoessow, J. E. Butler, S. Zuo and A. Kanareykin, Euclid Techlabs LLC,...

3

untitled  

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

Yusof, 2 A. Kanareykin, 1 and W. Gai 2 1 Euclid Techlabs, LLC, 5900 Harper Road, Solon, Ohio 44139, USA 2 High Energy Physics Division, Argonne National Laboratory, Argonne,...

4

High Frequency High Power RF Generation using a Relativistic...  

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

FREQUENCY HIGH POWER RF GENERATION USING A RELATIVISTIC ELECTRON BEAM C. Jing , S. Antipov, P. Schoessow, and A. Kanareykin, Euclid Techlabs LLC, Solon, OH-44139 J.G. Power, M....

5

Euclid File Systems  

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Request Form Euclid File Systems Euclid has 3 kinds of file systems available to users: home directories, scratch directories and project directories, all provided by the NERSC...

6

Getting Started on Euclid  

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Getting started Getting started Logging In Users can log into Euclid using the Secure Shell (SSH) protocol 2 with the following command: % ssh -l username euclid.nersc.gov When you...

7

Getting Started on Euclid  

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

Getting started Getting started Getting started Logging In Users can log into Euclid using the Secure Shell (SSH) protocol 2 with the following command: % ssh -l username euclid.nersc.gov When you successfully log in you will land in your $HOME directory. Euclid is a one node system. All jobs that run on Euclid, e.g. compiles, edits, user jobs, etc,. run on the same node. Sample Program Code: Parallel Hello World Although Euclid was not intended for production runs of MPI codes, it is possible to run small MPI codes on it. Open a new file called helloWorld.f90 with a text editor such as emacs or vi. Paste the contents of the below code into the file. program helloWorld implicit none include "mpif.h" integer :: myPE, numProcs, ierr call MPI_INIT(ierr) call MPI_COMM_RANK(MPI_COMM_WORLD, myPE, ierr)

8

Running jobs on Euclid  

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Running jobs Running jobs Running jobs Overview and Basic Description Euclid is a single node system with 48 processors. It supports both multiprocessing (MPI) and multithreading programming models. Interactive Jobs All Euclid jobs are interactive. To launch an MPI job, type in this at the shell prompt: % mpirun -np numprocs executable_name where numprocs is the total number of MPI processes that will be executed. Interactive Usage Policy Due to the dynamic and unpredictable nature of visualization and data analysis, NERSC will attempt to provide equitable access to Euclid's resources through the enforcement of certain usage guidelines. The most crucial resources are the processor cores (48) and memory (512 GB). Processor Core Usage Policy No single interactive job should use more than 12 processor cores. A single

9

Euclid's Windows and our Mirrors Review of Euclid's Window by Leonard Mlodinow  

E-Print Network (OSTI)

for the cardboard figures that he paints. Disoriented by ideas and by individuals whose feelings and behavior the author about the material, I certainly found it an occasion to reflect on what I would have liked of reconciling it with the differential geometry of relativity; particles #12; Review of Euclid's Windows 2

Langlands, Robert

10

Experimental Observation of Energy Modulation in Electron Beams...  

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

OBSERVATION OF ENERGY MODULATION IN ELECTRON BEAMS PASSING THROUGH TERAHERTZ DIELECTRIC WAKEFIELD STRUCTURES* S. Antipov , C. Jing, P. Schoessow, and A. Kanareykin, Euclid...

11

--No Title--  

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

in Proceedings of the 2003 Particle Accelerator Conference, pg. 2432-2434, 2003. Transformer Ratio Enhancement Experiment. A.Kanareykin (Euclid Concepts LLC), W. Gai, J.G....

12

Transformer Ratio Enhancement Experiment  

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

TRANSFORMER RATIO ENHANCEMENT EXPERIMENT A. Kanareykin, Euclid Concepts LLC, Solon, OH 44139, USA W. Gai, J. G. Power. ANL, Argonne, IL, 60439, USA E. Nenasheva, Ceramics Ltd., St....

13

EDITED--LS-332-DWA_FEL_August16  

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

32 32 August 2012 A Compact Soft X-ray Free-Electron Laser Facility based on a Dielectric Wakefield Accelerator C. Jing, P. Schoessow, A. Kanareykin, Euclid Techlabs LLC, Solon, OH 44139 J. G. Power, HEP Division, Argonne National Laboratory, Argonne, IL 60439 R. Lindberg, A. Zholents, APS, Argonne National Laboratory, Argonne, IL 60439 P. Piot, Northern Illinois University, Department of Physics, DeKalb, IL 60115 To be published as a Light Source Technical Notes The submitted manuscript has been created by UChicago Argonne, LLC, Operator of Argonne National Laboratory ("Argonne"). Argonne, a U.S. Department of Energy Office of Science laboratory, is operated under Contract No. DE-AC02-06CH11357.

14

South Euclid, Ohio: Energy Resources | Open Energy Information  

Open Energy Info (EERE)

Euclid, Ohio: Energy Resources Euclid, Ohio: Energy Resources Jump to: navigation, search Equivalent URI DBpedia Coordinates 41.5231076°, -81.5184553° 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":41.5231076,"lon":-81.5184553,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

15

Growth Diagnostics for Dark Energy models and EUCLID forecast  

E-Print Network (OSTI)

In this work we introduce a new set of parameters $(r_{g}, s_{g})$ involving the linear growth of matter perturbation that can distinguish and constrain different dark energy models very efficiently. Interestingly, for $\\Lambda$CDM model these parameters take exact value $(1,1)$ at all red shifts whereas for models different from $\\Lambda$CDM, they follow different trajectories in the $(r_{g}, s_{g})$ phase plane. By considering the parametrization for the dark energy equation of state ($w$) and for the linear growth rate ($f_{g}$), we show that different dark energy behaviours with similar evolution of the linear density contrast, can produce distinguishable trajectories in the $(r_{g}, s_{g})$ phase plane. Moreover, one can put stringent constraint on these phase plane using future measurements like EUCLID ruling out some of the dark energy behaviours.

Sampurnanand; Anjan A. Sen

2013-01-06T23:59:59.000Z

16

Division Name Will  

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

Chicago Council on Science and Technology Clean Energy Trust Euclid TechLabs* Exxon Mobil* Illinois Science and Technology Coalition* Illinois Technology Association...

17

The State Energy Program Helps Promote that Bigger IS Better in Euclid,  

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

The State Energy Program Helps Promote that Bigger IS Better in The State Energy Program Helps Promote that Bigger IS Better in Euclid, Ohio The State Energy Program Helps Promote that Bigger IS Better in Euclid, Ohio July 25, 2012 - 11:38am Addthis Compare how Lincoln Electric's wind tower -- the largest capacity wind turbine in Ohio -- measures up to well-known structures from around the world. | Graphic courtesy of Lincoln Electric. Compare how Lincoln Electric's wind tower -- the largest capacity wind turbine in Ohio -- measures up to well-known structures from around the world. | Graphic courtesy of Lincoln Electric. Perry Luksin Communication Specialist, Department of Energy State Energy Program What are the key facts? Lincoln Electric's wind tower measures 443 feet tall and can generate 2.5 MW of electrical energy.

18

PowerPoint Presentation  

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

2007 Euclid Techlabs LLC CVD-diamond Ka-band 5 mm ID cylindrical waveguide * Scanning electron microscope images of a THz diamond microstructure produced using the hot wire...

19

pub2010.htm  

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

Special Topics & Beam Vol. 14, pg. 022801, 2011. ANL-HEP-PR-10-64 Increasing the Transformer Ratio at the AWA C. Jing (Euclid Techlabs, LLC), W. Gai, J. G. Power, M. Conde, W....

20

Process Limits on Euclid  

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

Process Limits Process Limits Limit Hard Soft core file size (blocks) 0 unlimited data seg size (kbytes) unlimited unlimited scheduling priority 0 0 file size (blocks) unlimited...

Note: This page contains sample records for the topic "kanareykin euclid techlabs" 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.


21

Running jobs on Euclid  

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

where numprocs is the total number of MPI processes that will be executed. Interactive Usage Policy Due to the dynamic and unpredictable nature of visualization and data analysis,...

22

Euclid Hardware and Software Configuration  

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

ACML (AMD's Math library) PETSc Development and Performance Tools PAPI Performance API IPM (Integrated Performance Monitoring) NERSC-Provided Applications Science domain...

23

Euclid, Ohio: Energy Resources | Open Energy Information  

Open Energy Info (EERE)

81.5267873° 81.5267873° 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":41.5931049,"lon":-81.5267873,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

24

 

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

Related Links Related Links AWA Home Page AWA Activities AWA Facilities AWA Group Meetings AWA News AWA QR Codes AWA Safety Discussions AWA Safety & Procedure Manual WF Notes AGN Notes (Internal) US High Gradient Collaboration Meeting Other Related Links Security and Privacy Notice AWA-- Related Links 2008 Advanced Accelerator Concepts Workshop Argonne Accelerator Institute Illinois Accelerator Institute 2006 Advanced Accelerator Concepts Workshop American Physical Society -- Division of Physics of Beams Euclid Techlabs Joint Accelerator Conferences Website International Linear Collider (ILC) Northern Illinois Center for Accelerator and Detector Development (NICADD) Other Advanced Accelerator R&D Programs · Accelerator Test Facility at BNL · Center for Beam Physics at LBNL

25

Euclid's Windows and our Mirrors Review of Euclid's Window by Leonard Mlodinow  

E-Print Network (OSTI)

for the cardboard figures that he paints. Disoriented by ideas and by individuals whose feelings and behavior the author about the material, I certainly found it an occasion to reflect on what I would have liked; particles and fields; Kaluza-Klein and the introduction of additional di- mensions; the function of "strings

26

On Euclid's Algorithm and the Computation of Polynomial Greatest ...  

E-Print Network (OSTI)

F C 9[x] are arranged in the order of decreasing exponents, the first term is ..... If the coefficients of F1 and F2 are integers bounded in magnitude by c, then by.

27

WF-NOTE-238  

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

6 6 March 21, 2011 Dielectric Wakefield Accelerator to Drive the Future FEL Light Source C. Jing 1,2 , J. Power 1 , and A. Zholents 3 1. High Energy Physics Division, ANL 2. Euclid Techlabs, LLC 3. Advanced Photon Source, ANL Abstract: X-ray free-electron lasers (FELs) are expensive instruments and a large part of the cost of the entire facility is driven by the accelerator. Using a high-energy gain dielectric wake-field accelerator (DWA) instead of the conventional accelerator may provide a significant cost saving and reduction of the facility size. In this article, we investigate using a collinear dielectric wakefield accelerator to provide a high repetition rate, high current, high energy beam to drive a future FEL x-ray light source. As an

28

BNL | ATF Operations Weekly Summary  

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

Operations Weekly Summary Operations Weekly Summary Week Starts E-beam Status CO2 Status 2013/12/30 Up time: 0 days Down time: 5 days Activity: Maintenance & holiday week Up time: 0 days Down time: 5 days (setup) Activity: OPA work & holiday week 2013/12/23 Up time: 1 days Down time: 4 days (holiday week) Exp: Beam Studies Group: ATF Energy: 57.6 MeV Charge: 500 pC Up time: 0 days Down time: 5 days Activity: OPA work & holiday week 2013/12/16 Up time: Down time: Exp: AE-58, ERL BPM testing + beam studies Group: AE58, BNL (C-AD) / ATF Energy: 57.6 MeV Charge: 500 pC Up time: 0 days Down time: 5 days (setup) Activity: OPA work, EUVL test setup (AE59) and maintenance 2013/12/09 Up time: Down time: Exp: AE-52, Beam Manipulation by self wakefield Group: AE52, Euclid techlabs Energy: 57.6 MeV

29

Bradbury Science Museum gets martian fever  

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

payload on Curiosity. The museum's TechLab will have a dozen videos and animations about the Curiosity rover from NASA and the Jet Propulsion Laboratory. Visitors can...

30

Virtual Exhibits  

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

the Museum Exhibitions Norris Bradbury Museum Lobby Defense Gallery Research Gallery History Gallery TechLab Virtual Exhibits invisible utility element Virtual Exhibits Virtual...

31

--No Title--  

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

3, 915-923 (2007). ANL-HEP-PR-07-57 High Transformer Ratios in Collinear Wakefield Accelerators J.G. Power, M. Conde, C. Jing, P. Schoessow and A. Kanareykin Presented at Particle...

32

--No Title--  

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

Vol. 877, 362-369, December, 2006. ANL-HEP-CP-06-70 Observation of Enhanced Transformer Ratio in Collinear Wakefield Acceleration C. Jing, A. Kanareykin, J. Power, M....

33

Lifelong Learning  

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

with our life-size image of the rover The museum's TechLab has a dozen videos and animations about the Curiosity rover from NASA and the Jet Propulsion Laboratory. Follow the...

34

HISTORY GALLERY  

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History Gallery TechLab Virtual Exhibits invisible utility element HISTORY GALLERY The Atomic Age begins The conflict that darkened Europe in the late 1930s at first cast no...

35

Fast 704 MHz Ferroelectric Tuner for Superconducting Cavities  

SciTech Connect

The Omega-P SBIR project described in this Report has as its goal the development, test, and evaluation of a fast electrically-controlled L-band tuner for BNL Energy Recovery Linac (ERL) in the Electron Ion Collider (EIC) upgrade of the Relativistic Heavy Ion Collider (RHIC) at Brookhaven National Laboratory (BNL). The tuner, that employs an electrically-controlled ferroelectric component, is to allow fast compensation to cavity resonance changes. In ERLs, there are several factors which significantly affect the amount of power required from the wall-plug to provide the RF-power level necessary for the operation. When beam loading is small, the power requirements are determined by (i) ohmic losses in cavity walls, (ii) fluctuations in amplitude and/or phase for beam currents, and (iii) microphonics. These factors typically require a substantial change in the coupling between the cavity and the feeding line, which results in an intentional broadening of the cavity bandwidth, which in turn demands a significant amount of additional RF power. If beam loading is not small, there is a variety of beam-drive phase instabilities to be managed, and microphonics will still remain an issue, so there remain requirements for additional power. Moreover ERL performance is sensitive to changes in beam arrival time, since any such change is equivalent to phase instability with its vigorous demands for additional power. In this Report, we describe the new modular coaxial tuner, with specifications suitable for the 704 MHz ERL application. The device would allow changing the RF-coupling during the cavity filling process in order to effect significant RF power savings, and also will provide rapid compensation for beam imbalance and allow for fast stabilization against phase fluctuations caused by microphonics, beam-driven instabilities, etc. The tuner is predicted to allow a reduction of about ten times in the required power from the RF source, as compared to a compensation system with narrower bandwidth. It is planned to build a 704 MHz version of the tuner, to check its underlying principles, and to make high-power tests at power densities aimed towards controlling 50 kW of average power. Steps towards this goal will be limited by, among other factors, losses in the actual ferroelectric elements in the ferroelectric assemblies. As the ferroelectric material loss tangent is reduced through efforts by the supplier Euclid TechLabs LLC, the concomitant power loss in its ferroelectric assemblies will drop, and the average power-handling capability of the Omega-P tuner will rise. It can thus be anticipated that the Phase II development project of the 704 MHz tuner will be iterative, but the pace and ultimate power-handling level of the tuner is difficult to predict at this early stage in Euclid's development program. Fortunately, since Omega-P's conceptual tuner is a simple module (nominally rated for 5 kW), so that the number of modules required in each tuner can be chosen, depending upon the cavity power level needed, plus the power for tuner losses.

Jay L. Hirshfield

2012-04-12T23:59:59.000Z

36

Educational Programs  

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

located at: Argonne Brochure Postdoc Brochure Sponsors mdi logo euclid logo uop logo exxon logo aaas logo ist logo For more information, contact Tina Henne Argonne National...

37

EA-1777: Finding of No Significant Impact | Department of Energy  

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

No Significant Impact EA-1777: Finding of No Significant Impact Lincoln Electric's Wind Energy Project in Euclid, OH DOE prepared an environmental assessment analyzing the...

38

Primal-dual methods for solving infinite-dimensional games  

E-Print Network (OSTI)

(1958), 171-176. http://projecteuclid.org/euclid.pjm/1103040253. [4] Nesterov, Yurii. Primal-dual subgradient methods for convex problems. In: Mathematical.

39

Lincoln Electric Draft Environmental Assessment  

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

APPENDIX E. DRAFT EA COMMENTS AND RESPONSES 2 Lincoln Electric Draft Environmental Assessment Comments and Responses Number Commenter Comment Summary Response 1. Euclid Historical...

40

A first step in the design of a formally verified constraint-based testing tool: focaltest  

Science Conference Proceedings (OSTI)

Constraint-based test data generators rely on SMT or constraint solvers to automatically generate test data (e.g., Pex, Sage, Gatel, PathCrawler, Euclide). However, for some test data generation requests corresponding to particular test objectives, these ...

Matthieu Carlier; Catherine Dubois; Arnaud Gotlieb

2012-05-01T23:59:59.000Z

Note: This page contains sample records for the topic "kanareykin euclid techlabs" 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.


41

Genepool Email Announcements Archive  

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

2008 2007 2006 2005 2004 2003 2002 2001 2000 all Select List: all users mpp jgi hopper edison carver pdsf nug managers Retired Systems: bassi davinci franklin jacquard pvp euclid...

42

Research Gallery  

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

Research Gallery Research Gallery Inside the Museum Exhibitions Norris Bradbury Museum Lobby Defense Gallery Research Gallery History Gallery TechLab Virtual Exhibits invisible utility element Research Gallery Science serving society The Laboratory conducts leading-edge research in many areas of science and technology to help solve national problems related to energy, the environment, infrastructure, and health. Basic research conducted here enhances national defense and economic security. Exhibits you'll find in this gallery: Understanding Radiation LANSCE: Los Alamos Neutron Science Center Space Science Research Viewspace Environmental Monitoring and Research Nanotechnology: The Science of the Small Algae to Biofuels: Squeezing Power from Pond Scum Living with Wildfire: A Shared Community Experience

43

Cliff Hagan Baseball Stadium  

E-Print Network (OSTI)

DIY DIY DIYS Limestone Nicholasville S Upper Ave of Cham pions Euclid Ave University Dr CooperDr Alumni Dr VirginiaAve Huguelet Dr M axwell Dr WallerAve University Ct W oodland Ave E High St Rose St DIY (3.5 mi) Proposed Shared Use Trail (0.4 mi) !(l Bicycle Rack DIY Bicycle Repair Station 0 1

Hayes, Jane E.

44

Research on Regional Differences of Urban Resident Consumption Structure in China Based on Fuzzy Matter Element Model  

Science Conference Proceedings (OSTI)

Study of residents consumption structure plays an important role in macroeconomic policy formulation. Based on per capita annual consumption expenditure of urban households, the fuzzy matter element model is used to evaluate urban resident consumption ... Keywords: comsumption structure, fuzzy matter-element, Euclid approach degree, government consumption expenditure

Hong Li; Bo Zhou

2010-11-01T23:59:59.000Z

45

Brain atlases and associated databases have great potential as gateways for navigating, accessing, and visualizing a wide  

E-Print Network (OSTI)

. Pechura CM, Martin JB: Mapping the Brain and Its Functions. Washington, DC: National Academy Press; 1991 Department of Anatomy & Neurobiology, Washington University School of Medicine, 660 South Euclid Avenue, St registered Windows on the brain: the emerging role of atlases and databases in neuroscience David C Van Essen

Van Essen, David

46

Increasing the transformer ratio at the Argonne wakefield accelerator.  

SciTech Connect

The transformer ratio is defined as the ratio of the maximum energy gain of the witness bunch to the maximum energy loss experienced by the drive bunch (or a bunch within a multidrive bunch train). This plays an important role in the collinear wakefield acceleration scheme. A high transformer ratio is desirable since it leads to a higher overall efficiency under similar conditions (e.g. the same beam loading, the same structure, etc.). One technique to enhance the transformer ratio beyond the ordinary limit of 2 is to use a ramped bunch train. The first experimental demonstration observed a transformer ratio only marginally above 2 due to the mismatch between the drive microbunch length and the frequency of the accelerating structure [C. Jing, A. Kanareykin, J. Power, M. Conde, Z. Yusof, P. Schoessow, and W. Gai, Phys. Rev. Lett. 98, 144801 (2007)]. Recently, we revisited this experiment with an optimized microbunch length using a UV laser stacking technique at the Argonne Wakefield Accelerator facility and measured a transformer ratio of 3.4. Measurements and data analysis from these experiments are presented in detail.

Power, J.G.; Conde, M.; Liu, W.; Yusof, Z.; Gai, W.; Jing, C.; Kanareykin, A. (High Energy Physics); (Euclid Techlabs, LLC)

2011-01-01T23:59:59.000Z

47

A Methodology for Measuring the Rate of Reaction of CO2 with Brine-Rock Mixtures  

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

Methodology for Measuring the Rate of Reaction of CO Methodology for Measuring the Rate of Reaction of CO 2 with Brine-Rock Mixtures Nicholas B. Janda (nbj2@po.cwru.edu; 216-368-2648) Philip W. Morrison, Jr. (pwm5@po.cwru.edu; 216-368-4238) Department of Chemical Engineering Case Western Reserve University 10900 Euclid Avenue Cleveland, OH 44106-7217 Beverly Z. Saylor (bzs@po.cwru.edu; 216-368-3763) Gerald Matisoff (gxm4@po.cwru.edu; 216-368-3677) Department of Geological Sciences Case Western Reserve University 10900 Euclid Avenue Cleveland, OH 44106-7216 Introduction Storage of carbon dioxide in deep, porous, and permeable reservoir rocks is one of the most promising technologies for reducing emissions of greenhouse gases to the atmosphere. Although oil and gas reservoirs are a sensible first step for sequestration of carbon dioxide in geologic

48

BNL | ATF Beam Schedule  

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

Beam Schedule (pdf) Beam Schedule (pdf) Sunday Monday Tuesday Wednesday Thursday Friday Saturday 22 1/2 Holiday Holiday 28 January Holiday 4 5 Maintenance 11 12 Maintenance 18 19 Holiday AE52 - DWFA (Euclid), BL2 25 February AE52 - DWFA (Euclid), BL2 1 2 AE50 - PWFA in QNR (UCLA), BL2 8 9 AE50 - PWFA in QNR (UCLA), BL2 15 16 Holiday AE50 - PWFA in QNR (UCLA), BL2 22 March 1 2 AE53 - Nonlinear Compton (UCLA) 8 9 AE53 - Nonlinear Compton (UCLA) 15 16 AE53 - Nonlinear Compton (UCLA) 22 23 29 Sunday Monday Tuesday Wednesday Thursday Friday Saturday User operations (E-beam in use) Ions - Ion generation User operations (laser in use) PWFA - Plasma Wakefield Acceleration User operations (E-beam and laser in use)

49

Cliff Hagan Baseball Stadium  

E-Print Network (OSTI)

Arboretum DIY DIY DIY S U pper Ave of Cham pions Euclid Ave University Dr CooperDr Aumni Dr VirginiaAve H uguelet D r E M ain St WallerAve University Ct W oodland Ave E High St R ose St DIY E Vine St POT Trail (0.4 mi) !(l Bicycle Rack DIY Bicycle Repair Station Bicycle FacilitiesBicycle Facilities #12;

Hayes, Jane E.

50

MEMOCODE 2003 Panel Stephen A. Edwards  

E-Print Network (OSTI)

MEMOCODE 2003 Panel Stephen A. Edwards Department of Computer Science, Columbia University www-level synthesis and validation. #12;Euclid's Algorithm on the PDP-11 .globl _gcd GPRs: r0-r7 .text r7=PC, r6=SP, r5=FP _gcd: jsr r5, rsave Save SP in FP L2: mov 4(r5), r1 r1 = n sxt r0 sign extend div 6(r5), r0 r0

51

PRECISION COSMOGRAPHY WITH STACKED VOIDS  

SciTech Connect

We present a purely geometrical method for probing the expansion history of the universe from the observation of the shape of stacked voids in spectroscopic redshift surveys. Our method is an Alcock-Paczynski (AP) test based on the average sphericity of voids posited on the local isotropy of the universe. It works by comparing the temporal extent of cosmic voids along the line of sight with their angular, spatial extent. We describe the algorithm that we use to detect and stack voids in redshift shells on the light cone and test it on mock light cones produced from N-body simulations. We establish a robust statistical model for estimating the average stretching of voids in redshift space and quantify the contamination by peculiar velocities. Finally, assuming that the void statistics that we derive from N-body simulations is preserved when considering galaxy surveys, we assess the capability of this approach to constrain dark energy parameters. We report this assessment in terms of the figure of merit (FoM) of the dark energy task force and in particular of the proposed Euclid mission which is particularly suited for this technique since it is a spectroscopic survey. The FoM due to stacked voids from the Euclid wide survey may double that of all other dark energy probes derived from Euclid data alone (combined with Planck priors). In particular, voids seem to outperform baryon acoustic oscillations by an order of magnitude. This result is consistent with simple estimates based on mode counting. The AP test based on stacked voids may be a significant addition to the portfolio of major dark energy probes and its potentialities must be studied in detail.

Lavaux, Guilhem [Department of Physics, University of Illinois at Urbana-Champaign, 1002 West Green Street, Urbana, IL 61801 (United States); Wandelt, Benjamin D. [UPMC Univ Paris 06, UMR 7095, Institut d'Astrophysique de Paris, 98 bis, boulevard Arago, 75014 Paris (France)

2012-08-01T23:59:59.000Z

52

PETSc: External Software  

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

External Software External Software Home Download Features Documentation Applications/Publications Miscellaneous External Software Developers Site PETSc interfaces to the following optional external software (installing packages) (manual pages): ADIFOR - automatic differentiation for the computation of sparse Jacobians. AMD - Approximate minimum degree orderings. AnaMod - a library of matrix analysis modules; part of the Salsa project. BLAS and LAPACK Chaco - a graph partitioning package. ESSL - IBM's math library for fast sparse direct LU factorization. Euclid - parallel ILU(k) developed by David Hysom, accessed through the Hypre interface. FFTW - Fastest Fourier Transform in the West, developed at MIT by Matteo Frigo and Steven G. Johnson. Hypre - the LLNL preconditioner library.

53

Dark energy constraints from a space-based supernova survey  

E-Print Network (OSTI)

We present a forecast of dark energy constraints that could be obtained from a large sample of distances to Type Ia supernovae detected and measured from space. We simulate the supernova events as they would be observed by a EUCLID-like telescope with its two imagers, assuming those would be equipped with 4 visible and 3 near infrared swappable filters. We account for known systematic uncertainties affecting the cosmological constraints, including those arising through the training of the supernova model used to fit the supernovae light curves. Using conservative assumptions and Planck priors, we find that a 18 month survey would yield constraints on the dark energy equation of state comparable to the cosmic shear approach in EUCLID: a variable two-parameter equation of state can be constrained to ~0.03 at z~0.3. These constraints are derived from distances to about 13,000 supernovae out to z=1.5, observed in two cones of 10 and 50 deg^2. These constraints do not require measuring a nearby supernova sample fr...

Astier, P; Pain, R; Balland, C

2010-01-01T23:59:59.000Z

54

Medical Facilities With Experience Evaluating CBD  

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

/25/11 /25/11 Medical Facilities With Experience Evaluating Chronic Beryllium Disease Cleveland Clinic Foundation Raid Dweik, M.D., FACP, F.C.C.P. Pulmonary and Critical Care Medicine 9500 Euclid Avenue Cleveland, OH 44195 Contact: Jessica Phone: 216-445-5763 East Tennessee Pulmonary Associates R. Hal Hughes, M.D. East Tennessee Pulmonary Associates 800 Oak Ridge Turnpike Oak Ridge, TN 37830-9657 Phone: 865-483-3594 Philip Harber, M.D. 7230 Medical Center Drive, Ste 300 West Hills, CA 91307 Contact: Samantha Phone: 310-433-5342 Harborview Medical Center University of Washington Jordan Firestone, M.D.; Victor VanHee, M.D.; Szerre Vedal, M.D.; David Bonauto, M.D.; or June Spector, M.D. Occupational & Environmental Medicine Program Box 359739

55

Secretary Chu to Visit Cleveland | Department of Energy  

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

Cleveland Cleveland Secretary Chu to Visit Cleveland January 17, 2012 - 2:24pm Addthis Washington D.C. - U.S. Energy Secretary Steven Chu will travel to Cleveland, Ohio, tomorrow to deliver a speech at the City Club of Cleveland on the importance of strengthening U.S. competitiveness in the global clean energy race and how Ohio is helping to lead the way. Following the event, Secretary Chu will tour Case Western Reserve University's Research Laboratories and meet with community business leaders. Speech at the City Club of Cleveland WHAT: Energy Secretary Steven Chu to deliver speech at City Club of Cleveland WHEN: Wednesday, January 18 12:30 PM EST WHERE: City Club of Cleveland, Cleveland, Ohio 850 Euclid Ave. The City Club Building, 2nd Floor

56

Performance and Optimization  

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

Hyper-Threading Hyper-Threading Core Specialization Technology Documentation Cray XC30 Documentation Known issues News and Updates Cray XC30 Press Release Euclid - Retired 01/31/2013 Franklin - Retired 04/30/12 Data & File Systems Network Connections Queues and Scheduling Job Logs & Analytics Training & Tutorials Software Accounts & Allocations Policies Data Analytics & Visualization Data Management Policies Science Gateways User Surveys NERSC Users Group User Announcements Help Operations for: Passwords & Off-Hours Status 1-800-66-NERSC, option 1 or 510-486-6821 Account Support https://nim.nersc.gov accounts@nersc.gov 1-800-66-NERSC, option 2 or 510-486-8612 Consulting http://help.nersc.gov consult@nersc.gov 1-800-66-NERSC, option 3 or 510-486-8611 Home » For Users » Computational Systems » Retired Systems » Edison

57

Case Western University (Vestas) | Open Energy Information  

Open Energy Info (EERE)

University (Vestas) University (Vestas) Jump to: navigation, search Name Case Western University (Vestas) Facility Case Western University (Vestas) Sector Wind energy Facility Type Community Wind Facility Status In Service Owner Case Western University Developer Case Western University Energy Purchaser Sopko & Sons - excess to First Energy Location Euclid OH Coordinates 41.60216607°, -81.49763346° 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":41.60216607,"lon":-81.49763346,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

58

Case Western University (Nordex) | Open Energy Information  

Open Energy Info (EERE)

University (Nordex) University (Nordex) Jump to: navigation, search Name Case Western University (Nordex) Facility Case Western University (Nordex) Sector Wind energy Facility Type Community Wind Facility Status In Service Owner Case Western University Developer Case Western University Energy Purchaser Stamco Inc - excess to First Energy Location Euclid OH Coordinates 41.60213398°, -81.49688244° 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":41.60213398,"lon":-81.49688244,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

59

Lincoln Electric | Open Energy Information  

Open Energy Info (EERE)

Lincoln Electric Lincoln Electric Facility Lincoln Electric Sector Wind energy Facility Type Commercial Scale Wind Facility Status In Service Owner Lincoln Electric Developer Lincoln Electric Energy Purchaser Lincoln Electric Location Euclid OH Coordinates 41.58468216°, -81.52579665° 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":41.58468216,"lon":-81.52579665,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

60

Genepool Email Announcements Archive  

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

Email Announcements Archive Email Announcements Archive Genepool Email Announcements Archive Year: 2014 Select Year: 2014 2013 2012 2011 2010 2009 2008 2007 2006 2005 2004 2003 2002 2001 2000 all Select List: all users mpp jgi hopper edison carver pdsf nug managers Retired Systems: bassi davinci franklin jacquard pvp euclid seaborg Search Announcements Body and Title Search Subject Date Author Re: [Edison-users] [usgc] Edison will be reserved for system debugging every other day starting from 10/10/2013 Thursday 16:00 PDT 2014-01-10 15:57:24 Zhengji Zhao [Jgi-users] Jenkins talk today at Noon (Dial-in for JGI participants) 2014-01-10 09:45:33 Douglas Jacobsen [Jgi-users] Please complete the NERSC 2013 User Survey 2014-01-09 17:48:50 Douglas Jacobsen

Note: This page contains sample records for the topic "kanareykin euclid techlabs" 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

NERSC Announcements  

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

Announcements Announcements Announcements Email Announcement Archive Year: 2014 Select Year: 2014 2013 2012 2011 2010 2009 2008 2007 2006 2005 2004 2003 2002 2001 2000 all Select List: all users mpp jgi hopper edison carver pdsf nug managers Retired Systems: bassi davinci franklin jacquard pvp euclid seaborg Search Announcements Body and Title Search Subject Date Author Re: [Edison-users] [usgc] Edison will be reserved for system debugging every other day starting from 10/10/2013 Thursday 16:00 PDT 2014-01-10 15:57:24 Zhengji Zhao [Jgi-users] Jenkins talk today at Noon (Dial-in for JGI participants) 2014-01-10 09:45:33 Douglas Jacobsen [Jgi-users] Please complete the NERSC 2013 User Survey 2014-01-09 17:48:50 Douglas Jacobsen

62

ReliOn | Open Energy Information  

Open Energy Info (EERE)

ReliOn ReliOn Jump to: navigation, search Name ReliOn Address 15913 E. Euclid Avenue Place Spokane, WA Zip 99216 Sector Hydrogen Product Fuel cells for backup and grid-supplement power Year founded 1995 Number of employees 11-50 Phone number 509-228-6500 Website http://www.relion-inc.com Region Pacific Northwest Area References ReliOn[1] LinkedIn Connections CrunchBase Profile No CrunchBase profile. Create one now! This article is a stub. You can help OpenEI by expanding it. ReliOn is a company based in Spokane, Washington. References ↑ "ReliOn" Retrieved from "http://en.openei.org/w/index.php?title=ReliOn&oldid=616700" Categories: Companies Energy Generation Organizations Clean Energy Organizations Organizations Stubs What links here Related changes

63

Notice of Record of Decision and Floodplain Statement of Findings for the San Luis Rio Colorado Project (DOE/EIS  

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

4 Federal Register 4 Federal Register / Vol. 72, No. 197 / Friday, October 12, 2007 / Notices * Hawthorne, Nevada. Hawthorne Convention Center, 932 E. Street, November 13, 2007, from 4 to 7 p.m. * Caliente, Nevada. Caliente Youth Center, U.S. Highway 93, November 15, 2007, from 5:30 to 8 p.m. * Reno/Sparks, Nevada. Reno-Sparks Convention Center, 4590 S. Virginia Street, November 19, 2007, from 4 to 7 p.m. * Town of Amargosa Valley, Nevada. Longstreet Inn & Casino, Highway 373, November 26, 2007, from 4 to 7 p.m. * Goldfield, Nevada. Goldfield School Gymnasium, Hall & Euclid, November 27, 2007, from 4 to 7 p.m. * Lone Pine, California. Statham Hall, 138 N. Jackson Street, November 29, 2007, from 4 to 7 p.m. * Las Vegas, Nevada. Cashman Center, 850 Las Vegas Blvd., December

64

Edison Programming Environment  

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

Technology Documentation Technology Documentation Cray XC30 Documentation Known issues News and Updates Cray XC30 Press Release Euclid - Retired 01/31/2013 Franklin - Retired 04/30/12 Data & File Systems Network Connections Queues and Scheduling Job Logs & Analytics Training & Tutorials Software Accounts & Allocations Policies Data Analytics & Visualization Data Management Policies Science Gateways User Surveys NERSC Users Group User Announcements Help Operations for: Passwords & Off-Hours Status 1-800-66-NERSC, option 1 or 510-486-6821 Account Support https://nim.nersc.gov accounts@nersc.gov 1-800-66-NERSC, option 2 or 510-486-8612 Consulting http://help.nersc.gov consult@nersc.gov 1-800-66-NERSC, option 3 or 510-486-8611 Home » For Users » Computational Systems » Retired Systems » Edison

65

Transferring Data  

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

Transferring Data Transferring Data to and from NERSC Yushu Yao 1 Tuesday, March 8, 2011 Overview 2 * Structure of NERSC Systems and Disks * Data Transfer Nodes * Transfer Data from/to NERSC - scp/sftp - bbcp - GridFTP * Sharing Data Within NERSC Tuesday, March 8, 2011 Systems and Disks 3 System Hopper Franklin Carver Euclid Data Transfer Node PDSF Global Home ($HOME) Global Scratch ($GSCRATCH) Project Directory Local Non-shared Scratch Data transfer nodes can access most of the disks, suggested for transferring data in/out NERSC Tuesday, March 8, 2011 Data Transfer Nodes * Two Servers Available Now: - dtn01.nersc.gov and dtn02.nersc.gov - Accessible by all NERSC users * Designed to Transfer Data: - High speed connection to HPSS and NGF (Global Home, Project, and Global Scratch) - High speed ethernet to wide area network

66

Complementarity of weak lensing and peculiar velocity measurements in testing general relativity  

SciTech Connect

We explore the complementarity of weak lensing and galaxy peculiar velocity measurements to better constrain modifications to General Relativity. We find no evidence for deviations from General Relativity on cosmological scales from a combination of peculiar velocity measurements (for Luminous Red Galaxies in the Sloan Digital Sky Survey) with weak lensing measurements (from the Canadian France Hawaii Telescope Legacy Survey). We provide a Fisher error forecast for a Euclid-like space-based survey including both lensing and peculiar velocity measurements and show that the expected constraints on modified gravity will be at least an order of magnitude better than with present data, i.e. we will obtain {approx_equal}5% errors on the modified gravity parametrization described here. We also present a model-independent method for constraining modified gravity parameters using tomographic peculiar velocity information, and apply this methodology to the present data set.

Song, Yong-Seon [Korea Institute for Advanced Study, Dongdaemun-gu, Seoul 130-722 (Korea, Republic of); Institute of Cosmology and Gravitation, University of Portsmouth, Dennis Sciama Building, Portsmouth, PO1 3FX (United Kingdom); Zhao Gongbo; Bacon, David; Koyama, Kazuya; Nichol, Robert C. [Institute of Cosmology and Gravitation, University of Portsmouth, Dennis Sciama Building, Portsmouth, PO1 3FX (United Kingdom); Pogosian, Levon [Department of Physics, Simon Fraser University, Burnaby, BC, V5A 1S6 (Canada)

2011-10-15T23:59:59.000Z

67

Constraints on primordial non-Gaussianity from WMAP7 and luminous red galaxies power spectrum and forecast for future surveys  

Science Conference Proceedings (OSTI)

We place new constraints on the primordial local non-Gaussianity parameter f{sub NL} using recent cosmic microwave background anisotropy and galaxy clustering data. We model the galaxy power spectrum according to the halo model, accounting for a scale-dependent bias correction proportional to f{sub NL}/k{sup 2}. We first constrain f{sub NL} in a full 13 parameters analysis that includes 5 parameters of the halo model and 7 cosmological parameters. Using the WMAP7 CMB data and the SDSS DR4 galaxy power spectrum, we find f{sub NL}=171{sub -139}{sup +140} at 68% C.L. and -69forecast the constraints on f{sub NL} from future surveys as EUCLID and from CMB missions as Planck showing that their combined analysis could detect f{sub NL{approx}}5.

De Bernardis, Francesco [Physics Department and INFN, Universita di Roma 'La Sapienza', Ple Aldo Moro 2, 00185, Rome (Italy); Center for Cosmology, Department of Physics and Astronomy, University of California Irvine, Irvine, California 92697 (United States); Serra, Paolo; Cooray, Asantha [Center for Cosmology, Department of Physics and Astronomy, University of California Irvine, Irvine, California 92697 (United States); Melchiorri, Alessandro [Physics Department and INFN, Universita di Roma 'La Sapienza', Ple Aldo Moro 2, 00185, Rome (Italy)

2010-10-15T23:59:59.000Z

68

Cray IO COE  

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

IO COE IO COE Performance of MPIIO on DVS+GPFS Yushu Yao Collaboration with: Mike Aamodt, Katie Antypas, Tina Butler, Mark Cruciani, Jason Hick, David Knaak, Rei Lee, Rose Olson, Mike Welcome 1 Wednesday, July 25, 12 WHY 2 Wednesday, July 25, 12 Scratch 35GB/S LSI 7900 OSS OSS OSS OSS OSS OSS ... ... LSI 7900 LSI 7900 ... ... LSI 7900 LSI 7900 ... ... DDN DDN DDN DDN PROJECT DVS DDN DDN DDN DDN GSCRATCH Data Analysis Visualization ... ... PNSD PNSD PNSD CMP CMP CMP ... CMP CMP CMP ... ... ... ... Carver ... Euclid ... ... Reason 1. Users Love Global File Systems FAST MPIIO!!! 3 Wednesday, July 25, 12 0 3 6 9 12 Carver FilePerProc Hopper FilePerProc Carver MPIIO Hopper MPIIO 1.8 7 11 11 0.8 11 12 12 Read Write GB/Sec Performance using IOR (Jan 2012) 20 nodes with 4PE/node Reason 2. Well, DVS+MPIIO Was Super SLOW

69

Pacific Fuel Cell Corporation | Open Energy Information  

Open Energy Info (EERE)

Fuel Cell Corporation Fuel Cell Corporation Jump to: navigation, search Name Pacific Fuel Cell Corporation Address 26985 Lakeland Blvd. Place Euclid, Ohio Zip 44132 Sector Buildings, Efficiency, Renewable Energy, Services Product Consulting; Engineering/architectural/design; Maintenance and repair;Manufacturing;Raw materials/extraction; Research and development;Retail product sales and distribution;Trainining and education Phone number 216-731-0906 Website http://www.pacificfuelcell.com Coordinates 41.603828°, -81.494011° 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":41.603828,"lon":-81.494011,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

70

The Renaissance Group, A Conserve First Company | Open Energy Information  

Open Energy Info (EERE)

Group, A Conserve First Company Group, A Conserve First Company Jump to: navigation, search Name The Renaissance Group, A Conserve First Company Address 8281 Euclid Chardon Road Place Kirtland, Ohio Zip 44094 Sector Buildings, Efficiency, Hydro, Renewable Energy, Solar, Wind energy Product Agriculture; Consulting;Energy audits/weatherization; Engineering/architectural/design;Installation;Investment/finances;Maintenance and repair;Manufacturing; Research and development;Retail product sales and distribution;Trainining and education Phone number 440-256-2800 Website http://www.ConserveFirst.com Coordinates 41.584344°, -81.346526° 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":41.584344,"lon":-81.346526,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

71

The concept of primes and the algorithm for counting the greatest common divisor in Ancient China  

E-Print Network (OSTI)

When people mention the number theoretical achievements in Ancient China, the famous Chinese Remainder Theorem always springs to mind. But, two more of them--the concept of primes and the algorithm for counting the greatest common divisor, are rarely spoken. Some scholars even think that Ancient China has not the concept of primes. The aim of this paper is to show that the concept of primes in Ancient China can be traced back to the time of Confuciusor (about 500 B.C.) or more ago. This implies that the concept of primes in Ancient China is much earlier than the concept of primes in Euclid's \\emph{Elements}(about 300 B.C.) of Ancient Greece. We also shows that the algorithm for counting the greatest common divisor in Ancient China is essentially the Euclidean algorithm or the binary gcd algorithm. Donald E. Knuth said that "the binary gcd algorithm was discovered by J. Stein in 1961". Nevertheless, Knuth was wrong. The ancient Chinese algorithm is clearly much earlier than J. Stein's algorithm.

Zhang, Shaohua

2009-01-01T23:59:59.000Z

72

Bulk flows from galaxy luminosities: application to 2MASS redshift survey and forecast for next-generation datasets  

E-Print Network (OSTI)

We present a simple method for measuring cosmological bulk flows from large redshift surveys, based on the apparent dimming or brightening of galaxies due to their peculiar motion. It is aimed at estimating bulk flows of cosmological volumes containing large numbers of galaxies. Constraints on the bulk flow are obtained by minimizing systematic variations in galaxy luminosities with respect to a reference luminosity function measured from the whole survey. This method offers two advantages over more popular bulk flow estimators: it is independent of error-prone distance indicators and of the poorly-known galaxy bias. We apply the method to the 2MASS redshift survey (2MRS) to measure the local bulk flows of spherical shells centered on the Milky Way (MW). The result is consistent with that obtained by Nusser and Davis (2011) using the SFI++ catalogue of Tully-Fisher distance indicators. We also make an assessment of the ability of the method to constrain bulk flows at larger redshifts ($z=0.1-0.5$) from next generation datasets. As a case study we consider the planned EUCLID survey. Using this method we will be able to measure a bulk motion of $ \\sim 200 \\kms$ of $10^6$ galaxies with photometric redshifts, at the $3\\sigma$ level for both $z\\sim 0.15$ and $z\\sim 0.5$. Thus the method will allow us to put strong constraints on dark energy models as well as alternative theories for structure formation.

Adi Nusser; Enzo Branchini; Marc Davis

2011-02-21T23:59:59.000Z

73

RECONSTRUCTING REDSHIFT DISTRIBUTIONS WITH CROSS-CORRELATIONS: TESTS AND AN OPTIMIZED RECIPE  

SciTech Connect

Many of the cosmological tests to be performed by planned dark energy experiments will require extremely well-characterized photometric redshift measurements. Current estimates for cosmic shear are that the true mean redshift of the objects in each photo-z bin must be known to better than 0.002(1 + z), and the width of the bin must be known to {approx}0.003(1 + z) if errors in cosmological measurements are not to be degraded significantly. A conventional approach is to calibrate these photometric redshifts with large sets of spectroscopic redshifts. However, at the depths probed by Stage III surveys (such as DES), let alone Stage IV (LSST, JDEM, and Euclid), existing large redshift samples have all been highly (25%-60%) incomplete, with a strong dependence of success rate on both redshift and galaxy properties. A powerful alternative approach is to exploit the clustering of galaxies to perform photometric redshift calibrations. Measuring the two-point angular cross-correlation between objects in some photometric redshift bin and objects with known spectroscopic redshift, as a function of the spectroscopic z, allows the true redshift distribution of a photometric sample to be reconstructed in detail, even if it includes objects too faint for spectroscopy or if spectroscopic samples are highly incomplete. We test this technique using mock DEEP2 Galaxy Redshift survey light cones constructed from the Millennium Simulation semi-analytic galaxy catalogs. From this realistic test, which incorporates the effects of galaxy bias evolution and cosmic variance, we find that the true redshift distribution of a photometric sample can, in fact, be determined accurately with cross-correlation techniques. We also compare the empirical error in the reconstruction of redshift distributions to previous analytic predictions, finding that additional components must be included in error budgets to match the simulation results. This extra error contribution is small for surveys that sample large areas of sky (>{approx}10{sup 0}-100{sup 0}), but dominant for {approx}1 deg{sup 2} fields. We conclude by presenting a step-by-step, optimized recipe for reconstructing redshift distributions from cross-correlation information using standard correlation measurements.

Matthews, Daniel J.; Newman, Jeffrey A., E-mail: djm70@pitt.ed, E-mail: janewman@pitt.ed [Department of Physics and Astronomy, University of Pittsburgh, 3941 O'Hara Street, Pittsburgh, PA 15260 (United States)

2010-09-20T23:59:59.000Z