Sample records for driver training companion

  1. Alternative Fuel Driver Training Companion Manual

    SciTech Connect (OSTI)

    Not Available

    2005-09-01T23:59:59.000Z

    Training manual serves as a companion to alternative fuel training presentations on the fueling and use of vehicles that run on compressed natural gas, biodiesel, E85, and propane.

  2. Alternative Fuel Driver Training Companion Manual

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level: National5Sales for4,645U.S. DOE Office511041cloth DocumentationProducts (VAP) VAP7-0973ManagedStrategic|AljazeeraO S o'ware a ndManterEPAct

  3. Emergency vehicle driver training by Texas municipal police departments: a descriptive study

    E-Print Network [OSTI]

    Westmoreland, Robert Lawrence

    1994-01-01T23:59:59.000Z

    Because of the increase in the number of monetary civil judgments arising out of police emergency driving situations, law enforcement agencies are taking a critical look at their emergency driver training programs. At the present time...

  4. Drivers of Commercial Building Operator Skills

    E-Print Network [OSTI]

    Domanski, J.

    2011-01-01T23:59:59.000Z

    0 Drivers of Commercial Building Operator Skills C&W OVERVIEW C&W SUSTAINABILITY STRATEGIES GROUP WHAT?S DRIVING THE NEED FOR TRAINING? NECESSARY SKILLS & KNOWLEDGE C&W DEVELOPMENT & TRAINING OPPORTUNITIES International Conference... from: ? Owners/investors 4 DRIVERS ? OWNER/INVESTOR DEMAND ?UN Global Compact / Accenture 2010 CEO survey: ?93% of CEOs believe sustainability is ?critical? ?96% believe should be integrated into core business/operations ?C&W 2011survey...

  5. 9. Driver's Age 13. Driver's Date of Birth 14. Driver's Social Security Number 19. Driver's Telephone

    E-Print Network [OSTI]

    Gering, Jon C.

    of Accident (city, state; if on a highway, give number and nearest community) DRIVER INFORMATION OTHER VEHICLE OR PROPERTY Occupied Unoccupied 17. Driver's Age VEHICLE OPERATED BY UNIVERSITY EMPLOYEE Occupied Unoccupied 8. Driver's Name 16. Driver's Name TRUMAN STATE UNIVERSITY VEHICLE ACCIDENT REPORT NAME AND ADDRESS AREA

  6. Training

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level: National5Sales for4,645U.S. DOE Office of ScienceandMesa del SolStrengthening a solidSynthesisAppliances » TopTours SignTrackingTraining

  7. Utility vehicle safety Operator training program

    E-Print Network [OSTI]

    Minnesota, University of

    Utility vehicle safety Operator training program #12;Permissible use Utility Vehicles may only Utility Vehicle operator · When equipped with the "Required Equipment" · On public roadways within Drivers" · Obey all traffic regulations · Trained; update training every two years · Operate vehicles

  8. Doctoral Program Issues: Commentary on Companion Dissertations

    E-Print Network [OSTI]

    McNamara, James F.; Lara-Alecio, Rafael; Hoyle, John; Irby, Beverly J.

    2010-10-22T23:59:59.000Z

    @shsu.edu A Doctoral Issues Presentation at the National Council of Professors of Educational Administration Lexington, KY, August 2, 2006 Companion Dissertations 2 Doctoral Program Issues: Commentary on Companion Dissertations Companion dissertations... the findings for the unique samples and the summary, conclusions, and recommendations. It is recommended in this model that the chair(s) be the same person. Companion Dissertations 3 A second format is the multiple case study model that may elaborate one...

  9. Design and Evaluation of a Safe Driver Machine Interface ANDREA BONDAVALLI5

    E-Print Network [OSTI]

    Firenze, Università degli Studi di

    Computer (EVC) and the Driver Machine Interface (DMI). The EVC is the core of the on- board ATC system; it supervises the movement of the train by using the information re- ceived from the trackside systems. The DMI is the interface between the EVC and the driver; it acquires driver's commands and transforms EVC commands

  10. Driver eye height measurement

    E-Print Network [OSTI]

    Abrahamson, Anthony Daniel

    1978-01-01T23:59:59.000Z

    DRIVER EYF HEIGHT MFASHRFMENT A Thesis by ANTHONY DANIEL ABRAHAMSON Submitted to the Graduate College of Texas A&M Hniversity in partial fulfillment oi the requirement for the degree of MASTER OF SCIENCE December 1978 Major Subje"t: Civil... Engineering DRIVER EYE HEIGHT MEASUREMENT A Thesis by ANTHONY DANIEL ABRAHAMSON Approved as to style and content by: I (C irman of Committee) (Member) (Memb er ) Head of Department) December 1978 ABSTRACT Driver. Eye Height Neasurement. (December...

  11. Records management training: A strategy for a changing environment

    SciTech Connect (OSTI)

    Ekkebus, S.M.

    1992-09-21T23:59:59.000Z

    This presentation will discuss Records Management Training efforts at Martin Marietta Energy Systems, Inc. Topics covered include: drivers for record management training, targeted audiences, current training efforts, and future plans for program development.

  12. Vehicle Management Driver Safety Program

    E-Print Network [OSTI]

    Machel, Hans

    Vehicle Management and Driver Safety Program Manual Facilities & Operations / Finance & Administration Version 2 April 2012 #12;© 2012 University of Alberta. #12;The Vehicle Management and Driver of employment. Driver Acknowledgement I have received the University of Alberta, Vehicle Management and Driver

  13. Nonlinear transmission line based electron beam driver

    SciTech Connect (OSTI)

    French, David M.; Hoff, Brad W.; Tang Wilkin; Heidger, Susan; Shiffler, Don [Directed Energy Directorate, Air Force Research Laboratory, Kirtland AFB, New Mexico 87117 (United States); Allen-Flowers, Jordan [Program in Applied Mathematics, University of Arizona, Tucson, Arizona 85721 (United States)

    2012-12-15T23:59:59.000Z

    Gated field emission cathodes can provide short electron pulses without the requirement of laser systems or cathode heating required by photoemission or thermionic cathodes. The large electric field requirement for field emission to take place can be achieved by using a high aspect ratio cathode with a large field enhancement factor which reduces the voltage requirement for emission. In this paper, a cathode gate driver based on the output pulse train from a nonlinear transmission line is experimentally demonstrated. The application of the pulse train to a tufted carbon fiber field emission cathode generates short electron pulses. The pulses are approximately 2 ns in duration with emission currents of several mA, and the train contains up to 6 pulses at a frequency of 100 MHz. Particle-in-cell simulation is used to predict the characteristic of the current pulse train generated from a single carbon fiber field emission cathode using the same technique.

  14. Gas-Rich Companions of Isolated Galaxies

    E-Print Network [OSTI]

    Pisano, D J; Wilcots, Eric M.

    1999-01-01T23:59:59.000Z

    We have used the VLA to search for gaseous remnants of the galaxy formation process around six extremely isolated galaxies. We found two distinct HI clouds around each of two galaxies in our sample (UGC 9762 & UGC 11124). These clouds are rotating and appear to have optical counterparts, strongly implying that they are typical dwarf galaxies. The companions are currently weakly interacting with the primary galaxy, but have short dynamical friction timescales (~1 Gyr) suggesting that these triple galaxy systems will shortly collapse into one massive galaxy. Given that the companions are consistent with being in circular rotation about the primary galaxy, and that they have small relative masses, the resulting merger will be a minor one. The companions do, however, contain enough gas that the merger will represent a significant infusion of fuel to drive future star formation, bar formation, or central activity, while building up the mass of the disk thus making these systems important pieces of the galaxy f...

  15. Efficacy, national/international practices and motivational factors of lifelong driver education for the aging population

    E-Print Network [OSTI]

    Israels, Richard (Richard Steven)

    2006-01-01T23:59:59.000Z

    In a society facing a significant increase in its aging population, older driver education/training is emerging as a potential solution to help seniors drive more safely, thus maintaining their mobility and quality of life. ...

  16. Integrated Cognitive Assistive & Domotic Companion Robotic Systems

    E-Print Network [OSTI]

    Baudoin, Geneviève

    mobile robotic companion with the advantages of a stationary smart home environment. 2. Semantic support and cognitive engagement of the elderly. Advantages of the Smart Home ­ Numerous existing for reconstructing the home environment. ­ Allows promising marketing policy: "Rent-a-robot" or "Robots-on- demand

  17. Gas-Rich Companions of Isolated Galaxies

    E-Print Network [OSTI]

    D. J. Pisano; Eric M. Wilcots

    1999-02-01T23:59:59.000Z

    We have used the VLA to search for gaseous remnants of the galaxy formation process around six extremely isolated galaxies. We found two distinct HI clouds around each of two galaxies in our sample (UGC 9762 & UGC 11124). These clouds are rotating and appear to have optical counterparts, strongly implying that they are typical dwarf galaxies. The companions are currently weakly interacting with the primary galaxy, but have short dynamical friction timescales (~1 Gyr) suggesting that these triple galaxy systems will shortly collapse into one massive galaxy. Given that the companions are consistent with being in circular rotation about the primary galaxy, and that they have small relative masses, the resulting merger will be a minor one. The companions do, however, contain enough gas that the merger will represent a significant infusion of fuel to drive future star formation, bar formation, or central activity, while building up the mass of the disk thus making these systems important pieces of the galaxy formation and evolution process.

  18. Approaches to enhance driver situational assessment aids

    E-Print Network [OSTI]

    Jones, Eric M. (Eric Michael)

    2007-01-01T23:59:59.000Z

    Collision warning systems encounter a fundamental trade-off between providing the driver more time in which to respond and alerting the driver unnecessarily. The probability that a driver successfully avoids a hazard ...

  19. LANSCE | Training Office | User Training

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

    header TA-53 Training Office User Specific Training LANL Training Services (Internal) LANL UTRAIN (Internal) LANL EXTRAIN (External) Training Office dotline User Training Below is...

  20. UWB dual burst transmit driver

    DOE Patents [OSTI]

    Dallum, Gregory E. (Livermore, CA); Pratt, Garth C. (Discovery Bay, CA); Haugen, Peter C. (Livermore, CA); Zumstein, James M. (Livermore, CA); Vigars, Mark L. (Livermore, CA); Romero, Carlos E. (Livermore, CA)

    2012-04-17T23:59:59.000Z

    A dual burst transmitter for ultra-wideband (UWB) communication systems generates a pair of precisely spaced RF bursts from a single trigger event. An input trigger pulse produces two oscillator trigger pulses, an initial pulse and a delayed pulse, in a dual trigger generator. The two oscillator trigger pulses drive a gated RF burst (power output) oscillator. A bias driver circuit gates the RF output oscillator on and off and sets the RF burst packet width. The bias driver also level shifts the drive signal to the level that is required for the RF output device.

  1. Authorization and Driving History Form The following information will be retained on file by all agencies on their drivers authorized to operate a

    E-Print Network [OSTI]

    Harms, Kyle E.

    agencies on their drivers authorized to operate a State vehicle, or a private vehicle for state purposes ___________________________________________ Position: Staff_____ Faculty_____ Student_____ Is employee's primary purpose to drive vehicles? Yes_____ No/her private vehicle in the course and scope of employment? Yes_____ No_____ Date of last Driver Training

  2. An investigation of driver behavior at highway-railroad grade crossings

    E-Print Network [OSTI]

    Shull, Lee Anne

    1996-01-01T23:59:59.000Z

    crossing results, in that the presence of a crossing (rather than the presence of a train) is indicated by the location of the crossbucks. The driver is ultimately responsible for achieving safe passage across a passive crossing because no warning devices...

  3. Visualization drivers for Geant4

    SciTech Connect (OSTI)

    Beretvas, Andy; /Fermilab

    2005-10-01T23:59:59.000Z

    This document is on Geant4 visualization tools (drivers), evaluating pros and cons of each option, including recommendations on which tools to support at Fermilab for different applications. Four visualization drivers are evaluated. They are OpenGL, HepRep, DAWN and VRML. They all have good features, OpenGL provides graphic output without an intermediate file. HepRep provides menus to assist the user. DAWN provides high quality plots and even for large files produces output quickly. VRML uses the smallest disk space for intermediate files. Large experiments at Fermilab will want to write their own display. They should proceed to make this display graphics independent. Medium experiment will probably want to use HepRep because of it's menu support. Smaller scale experiments will want to use OpenGL in the spirit of having immediate response, good quality output and keeping things simple.

  4. Unemployed Truck Driver Trains for New Career in Weatherization |

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level: National5Sales for4,645 3,625 1,006 492 742EnergyOn AprilA group current C3E AmbassadorsUS-EU-Japan Working Unclassified 1DOE|Niketa

  5. 4, 615650, 2007 Drivers of storage

    E-Print Network [OSTI]

    Paris-Sud XI, Université de

    BGD 4, 615­650, 2007 Drivers of storage water use in Scots pine H. Verbeeck et al. Title Page drivers of storage water use in Scots pine H. Verbeeck1 , K. Steppe2 , N. Nadezhdina3 , M. Op De Beeck1 Correspondence to: H. Verbeeck (hans.verbeeck@ua.ac.be) 615 #12;BGD 4, 615­650, 2007 Drivers of storage water use

  6. Selected Texas Driver Education Instructors’ Feelings About A Driver Education Cultural Awareness Survey

    E-Print Network [OSTI]

    Saint, Nina Jo

    2012-07-16T23:59:59.000Z

    This study examined what items driver education instructors felt should be included in a cultural awareness survey to assess instructors' preparedness to teach a culturally diverse student clientele. In addition, the study examined the ways driver...

  7. Drivers of Future Energy Demand

    Gasoline and Diesel Fuel Update (EIA)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level: National5Sales for On-Highway4,1,50022,3,,,,6,1,9,1,50022,3,,,,6,1,Decade Year-0E (2001)gasoline353/06) 2Yonthly Energy :and1. Total3.9Drivers

  8. P5 Science Drivers: Theory

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level:Energy: Grid Integration Redefining What's Possible for RenewableSpeedingBiomass and BiofuelsOversight BoardP-GlycoproteiniiiScience Drivers:

  9. Software Support for Improved Driver Reliability

    E-Print Network [OSTI]

    Swift, Michael

    .6.23, 2007 esp.c, a serial port driver static int rs_write(struct tty_struct * tty, const unsigned char *buf

  10. Construction of a driver-vehicle model and identification of the driver model parameters

    E-Print Network [OSTI]

    Su, Jemeng

    1981-01-01T23:59:59.000Z

    CONSTRUCTION OF A DRIVER-VEHICLE MODEL AND IDENTIFICATION OF THE DRIVER MODEL PARAMETERS A Thesis by , JEMENG SU Submitted to the Graduate College of Texas A8M University in partial fulfillment of the requiremr nt for the degree of MASTER... OF SCIENCE December 1981 Major Subject: Mechanical Engineering CONSTRUCTION OF A DRIVER-VEHICLE MODEL AND IDENTIFICATION OF THE DRIVER MODEL PARAMETERS A Thesis by JEMENG SU Approved as to style and content by: (Chairman of Committe ) / I...

  11. Construction of a driver-vehicle model and identification of the driver model parameters 

    E-Print Network [OSTI]

    Su, Jemeng

    1981-01-01T23:59:59.000Z

    CONSTRUCTION OF A DRIVER-VEHICLE MODEL AND IDENTIFICATION OF THE DRIVER MODEL PARAMETERS A Thesis by , JEMENG SU Submitted to the Graduate College of Texas A8M University in partial fulfillment of the requiremr nt for the degree of MASTER... OF SCIENCE December 1981 Major Subject: Mechanical Engineering CONSTRUCTION OF A DRIVER-VEHICLE MODEL AND IDENTIFICATION OF THE DRIVER MODEL PARAMETERS A Thesis by JEMENG SU Approved as to style and content by: (Chairman of Committe ) / I...

  12. Companions around the nearest luminous galaxies: segregation and selection effects

    E-Print Network [OSTI]

    Karachentsev, I D

    2015-01-01T23:59:59.000Z

    Using the "Updated Nearby Galaxy Catalog", we consider different properties of companion galaxies around luminous hosts in the Local Volume. The data on stellar masses, linear diameters,surface brightnesses, HI-richness, specific star formation rate (sSFR), and morphological types are discussed for members of the nearest groups, including the Milky Way and M 31 groups, as a function of their separation from the hosts. Companion galaxies in groups tend to have lower stellar masses, smaller linear diameters and fainter mean surface brightnesses as the distance to their host decreases. The hydrogen-to-stellar mass ratio of the companions increases with their linear projected separation from the dominant luminous galaxy. This tendency is more expressed around the bulge-dominated hosts. While linear separation of the companions decreases, their mean sSFR becomes lower, accompanied with the increasing sSFR scatter. Typical linear projected separation of dSphs around the bulge-dominated hosts, 350 kpc, is substantia...

  13. Social Signal Processing in Companion Systems -Challenges Ahead

    E-Print Network [OSTI]

    suggests that nonverbal interaction plays a key role in steering, controlling and maintaining social focus our investigation on the modeling of visual processing mechanisms, since evidence in literature for artificial companions is captured in the five-star model by [BM08] which incorporates contributions along

  14. Driver comprehension of railroad-highway grade crossings

    E-Print Network [OSTI]

    Messick, Jennifer

    1995-01-01T23:59:59.000Z

    each year; however, collisions at grade crossings are still a major concern. In order to continue improving safety at grade crossings, driver comprehension and driver attitudes must be investigated. This research investigated driver comprehension...

  15. F2010-B-107 MODELING OF THE THS-II SERIES/PARALLEL POWER TRAIN AND

    E-Print Network [OSTI]

    Paris-Sud XI, Université de

    F2010-B-107 MODELING OF THE THS-II SERIES/PARALLEL POWER TRAIN AND ITS ENERGY MANAGEMENT SYSTEM ­ Hybrid power train, power-split eCVT, rule-based control strategy, Toyota Hybrid System, driver-based engineering intuition controller. The model encloses the modeling of the vehicle dynamics, the power train

  16. 9, 1443714473, 2012 Soil carbon drivers

    E-Print Network [OSTI]

    Ickert-Bond, Steffi

    BGD 9, 14437­14473, 2012 Soil carbon drivers and benchmarks in Earth system models K. E. O. Todd if available. Causes of variation in soil carbon predictions from CMIP5 Earth system models and comparison #12;BGD 9, 14437­14473, 2012 Soil carbon drivers and benchmarks in Earth system models K. E. O. Todd

  17. LOW-MASS TERTIARY COMPANIONS TO SPECTROSCOPIC BINARIES. I. COMMON PROPER MOTION SURVEY FOR WIDE COMPANIONS USING 2MASS

    SciTech Connect (OSTI)

    Allen, Peter R. [Department of Physics and Astronomy, P.O. Box 3003, Franklin and Marshall College, Lancaster, PA 17604 (United States); Burgasser, Adam J. [Department of Physics, University of California, San Diego, CA 92093 (United States); Faherty, Jacqueline K. [Department of Astrophysics, American Museum of Natural History, Central Park West at 79th Street, New York, NY 10034 (United States); Kirkpatrick, J. Davy, E-mail: peter.allen@fandm.edu [IPAC, California Institute of Technology, Pasadena, CA 91125 (United States)

    2012-08-15T23:59:59.000Z

    We report the first results of a multi-epoch search for wide (separations greater than a few tens of AU), low-mass tertiary companions of a volume-limited sample of 118 known spectroscopic binaries within 30 pc of the Sun, using the Two Micron All Sky Survey Point Source Catalog and follow-up observations with the KPNO and CTIO 4 m telescopes. Note that this sample is not volume complete but volume limited, and, thus, there is incompleteness in our reported companion rates. We are sensitive to common proper motion companions with separations from roughly 200 AU to 10,000 AU ({approx}10'' {yields} {approx} 10'). From 77 sources followed-up to date, we recover 11 previously known tertiaries, 3 previously known candidate tertiaries, of which 2 are spectroscopically confirmed and 1 rejected, and 3 new candidates, of which 2 are confirmed and 1 rejected. This yields an estimated wide tertiary fraction of 19.5{sup +5.2}{sub -3.7}%. This observed fraction is consistent with predictions set out in star formation simulations where the fraction of wide, low-mass companions to spectroscopic binaries is >10%.

  18. The mathcomp package for using Text Companion fonts in math mode *

    E-Print Network [OSTI]

    Mintmire, John W.

    .g., say \\usepackage[ppl]{mathcomp} to make mathcomp use the Adobe Palatino (ppl) text companion fonts

  19. V-217: Microsoft Windows NAT Driver ICMP Packet Handling Denial...

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

    A vulnerability was reported in the Windows NAT Driver PLATFORM: Windows Server 2012 ABSTRACT: This security update resolves a vulnerability in the Windows NAT Driver in Microsoft...

  20. Vehicle Technologies Office Merit Review 2015: Gate Driver Optimizatio...

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

    Gate Driver Optimization for WBG Applications Vehicle Technologies Office Merit Review 2015: Gate Driver Optimization for WBG Applications Presentation given by Oak Ridge National...

  1. Brazil's Biofuels Scenario: What are the Main Drivers Which will...

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

    Brazil's Biofuels Scenario: What are the Main Drivers Which will Shape Investments in the Long Term? Brazil's Biofuels Scenario: What are the Main Drivers Which will Shape...

  2. Discovery of a Young Substellar Companion in Chamaeleon

    E-Print Network [OSTI]

    Luhman, K L; Brandner, W; Skrutskie, M F; Nelson, M J; Smith, J D; Peterson, D E; Cushing, M C; Young, E

    2006-01-01T23:59:59.000Z

    During an imaging survey of the Chamaeleon I star-forming region with the ACS aboard HST, we have discovered a candidate substellar companion to the young low-mass star CHXR 73 (~2 Myr, M=0.35 Msun). We measure a projected separation of 1.3+/-0.03" for the companion, CHXR 73 B, which corresponds to 210 AU at the distance of the cluster. A near-infrared spectrum of this source obtained with CorMASS at the Magellan II telescope exhibits strong steam absorption that confirms its late-type nature (>=M9.5). In addition, the gravity-sensitive shapes of the H- and K-band continua demonstrate that CHXR 73 B is a young, pre-main-sequence object rather than a field star. The probability that CHXR 73A and B are unrelated members of Chamaeleon I is ~0.001. We estimate the masses of CHXR 73 B and other known substellar companions in young clusters with a method that is consistent with the dynamical measurements of the eclipsing binary brown dwarf 2M 0535-0546, which consists of a comparison of the bolometric luminosities ...

  3. Drawing driver's attention to potentially dangerous objects

    E-Print Network [OSTI]

    Kurugöl, Orc?un

    2008-01-01T23:59:59.000Z

    Drivers often have difficulties noticing potentially dangerous objects due to weather or lighting conditions or when their field of view is restricted. This thesis presents a display method for potentially dangerous objects ...

  4. A Landscape of Driver Mutations in Melanoma

    E-Print Network [OSTI]

    Lander, Eric S.

    Despite recent insights into melanoma genetics, systematic surveys for driver mutations are challenged by an abundance of passenger mutations caused by carcinogenic UV light exposure. We developed a permutation-based ...

  5. Physics at a new Fermilab proton driver

    SciTech Connect (OSTI)

    Geer, Steve; /Fermilab

    2006-04-01T23:59:59.000Z

    In 2004, motivated by the recent exciting developments in neutrino physics, the Fermilab Long Range Planning Committee identified a new high intensity Proton Driver as an attractive option for the future. At the end of 2004 the APS ''Study on the Physics of Neutrinos'' concluded that the future US neutrino program should have, as one of its components, ''A proton driver in the megawatt class or above and neutrino superbeam with an appropriate very large detector capable of observing Cp violation and measuring the neutrino mass-squared differences and mixing parameters with high precision''. The presently proposed Fermilab Proton Driver is designed to accomplish these goals, and is based on, and would help develop, Linear Collider technology. In this paper the Proton Driver parameters are summarized, and the potential physics program is described.

  6. Carbon Price Drivers:Carbon Price Drivers:Carbon Price Drivers:Carbon Price Drivers: AAAAnnnn UpdatedUpdatedUpdatedUpdated Literature ReviewLiterature ReviewLiterature ReviewLiterature Review

    E-Print Network [OSTI]

    Paris-Sud XI, Université de

    , such as unexpected fluctuations in energy demand, energy prices (e.g., oil, gas, coal) and weather conditions1 Carbon Price Drivers:Carbon Price Drivers:Carbon Price Drivers:Carbon Price Drivers: AAAAnnnn the factors that shape the price of carbon, where one European Union Allowance is equal to one ton of CO2

  7. Driver expectancy in locating automotive controls 

    E-Print Network [OSTI]

    Francis, Dawn Suzette

    1990-01-01T23:59:59.000Z

    DRIVER EXPECTANCY IN LOCATING AUTOMOTIVE CONTROLS A Thesis by DAWN SUZETTE FRANCIS Submitted to the Office of Graduate Studies of Texas A&M University in partial fulfillment of the requirements for the degree of MASTER OF SCIENCE May 1990... Major Subject: Industrial Engineering DRIVER EXPECTANCY IN LOCATING AUTOMOTIVE CONTROLS A Thesis by DAWN SUZETTE FRANCIS Approved as to style and content by: R. Dale Huchi son (Chair of Committee) Rodger . . ppa (Member) Waymon L ohnston (M er...

  8. Local Danger Warnings for Drivers: The Effect of Modality and Level of Assistance on Driver Reaction

    E-Print Network [OSTI]

    Theune, Mariët

    Local Danger Warnings for Drivers: The Effect of Modality and Level of Assistance on Driver¨ucken, Germany christian.mueller@dfki.de ABSTRACT Local danger warning is an important function of Advanced presentation) is particularly crucial to a successful danger avoidance. We present a user study investigating

  9. Pre-explosion companion stars in Type Iax supernovae

    E-Print Network [OSTI]

    Liu, Zheng-Wei; Abate, Carlo; Wang, Bo

    2015-01-01T23:59:59.000Z

    Type Iax supernovae (SNe Iax) are proposed as one new sub-class of SNe Ia since they present sufficiently distinct observational properties from the bulk of SNe Ia. SNe Iax are the most common of all types of peculiar SNe by both number and rate, with an estimated rate of occurrence of about 5-30% of the total SN Ia rate. However, the progenitor systems of SNe Iax are still uncertain. Analyzing pre-explosion images at SN Iax positions provides a direct way to place strong constraints on the nature of progenitor systems of SNe Iax. In this work, we predict pre-explosion properties of binary companion stars in a variety of potential progenitor systems by performing detailed binary evolution calculations with the one-dimensional stellar evolution code STARS. This will be helpful for constraining progenitor systems of SNe Iax from their pre-explosion observations. With our binary evolution calculations, it is found that the non-degenerate helium (He) companion star to both a massive C/O WD (> 1.1 solar mass) and ...

  10. A SEARCH FOR GIANT PLANET COMPANIONS TO T TAURI STARS

    SciTech Connect (OSTI)

    Crockett, Christopher J. [U.S. Naval Observatory, 10391 W. Naval Observatory Road, Flagstaff, AZ 86001 (United States); Mahmud, Naved I.; Johns-Krull, Christopher M.; Hartigan, Patrick M. [Department of Physics and Astronomy, Rice University, MS-108, 6100 Main Street, Houston, TX 77005 (United States); Prato, L. [Lowell Observatory, 1400 W Mars Hill Road, Flagstaff, AZ 86001 (United States); Jaffe, Daniel T. [Department of Astronomy, University of Texas, R.L. Moore Hall, Austin, TX 78712 (United States); Beichman, Charles A., E-mail: ccrockett@nofs.navy.mil, E-mail: lprato@lowell.edu, E-mail: naved@rice.edu, E-mail: cmj@rice.edu, E-mail: dtj@astro.as.utexas.edu [Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, CA 91109 (United States)

    2012-12-20T23:59:59.000Z

    We present results from an ongoing multiwavelength radial velocity (RV) survey of the Taurus-Auriga star-forming region as part of our effort to identify pre-main-sequence giant planet hosts. These 1-3 Myr old T Tauri stars present significant challenges to traditional RV surveys. The presence of strong magnetic fields gives rise to large, cool star spots. These spots introduce significant RV jitter which can mimic the velocity modulation from a planet-mass companion. To distinguish between spot-induced and planet-induced RV modulation, we conduct observations at {approx}6700 A and {approx}2.3 {mu}m and measure the wavelength dependence (if any) in the RV amplitude. CSHELL observations of the known exoplanet host Gl 86 demonstrate our ability to detect not only hot Jupiters in the near-infrared but also secular trends from more distant companions. Observations of nine very young stars reveal a typical reduction in RV amplitude at the longer wavelengths by a factor of {approx}2-3. While we cannot confirm the presence of planets in this sample, three targets show different periodicities in the two wavelength regions. This suggests different physical mechanisms underlying the optical and the K-band variability.

  11. TWO WIDE PLANETARY-MASS COMPANIONS TO SOLAR-TYPE STARS IN UPPER SCORPIUS

    SciTech Connect (OSTI)

    Ireland, M. J. [Sydney Institute for Astronomy (SIfA), School of Physics, University of Sydney, NSW 2006 (Australia); Kraus, A. [Institute for Astronomy, University of Hawaii, 2680 Woodlawn Drive, Honolulu, HI 96822 (United States); Martinache, F. [National Astronomical Observatory of Japan, Subaru Telescope, Hilo, HI 96720 (United States); Law, N. [Dunlap Institute for Astronomy and Astrophysics, University of Toronto, 50 St. George Street, Toronto M5S 3H4, Ontario (Canada); Hillenbrand, L. A. [Department of Astrophysics, California Institute of Technology, MC 105-24, Pasadena, CA 91125 (United States)

    2011-01-10T23:59:59.000Z

    At wide separations, planetary-mass and brown dwarf companions to solar-type stars occupy a curious region of parameter space not obviously linked to binary star formation or solar system scale planet formation. These companions provide insight into the extreme case of companion formation (either binary or planetary), and due to their relative ease of observation when compared to close companions, they offer a useful template for our expectations of more typical planets. We present the results from an adaptive optics imaging survey for wide ({approx}50-500 AU) companions to solar-type stars in Upper Scorpius. We report one new discovery of a {approx}14 M{sub J} companion around GSC 06214-00210and confirm that the candidate planetary-mass companion 1RXS J160929.1-210524 detected by Lafreniere et al. is in fact comoving with its primary star. In our survey, these two detections correspond to {approx}4% of solar-type stars having companions in the 6-20 M{sub J} mass and {approx}200-500 AU separation range. This figure is higher than would be expected if brown dwarfs and planetary-mass companions were drawn from an extrapolation of the binary mass function. Finally, we discuss implications for the formation of these objects.

  12. Assessor Training Assessor Qualification &

    E-Print Network [OSTI]

    NVLAP Assessor Training Assessor Qualification & Training Requirements #12;Assessor Training 2009: Qualification & Training Requirements 2 References ·ISO/IEC 17011: Conformity assessment General requirements 2 #12;Assessor Training 2009: Qualification & Training Requirements 3 Assessor Defined ·Lead

  13. Annual Training Plan Template

    Broader source: Energy.gov [DOE]

    The Annual Training Plan Template is used by an organization's training POC to draft their organization's annual training plan.

  14. LANSCE | Training Office

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

    header TA-53 Training Office User Specific Training LANL Training Services (Internal) LANL UTRAIN (Internal) LANL EXTRAIN (External) Training Office dotline Please note current...

  15. Detection of Driver Fatigue Caused by Sleep Deprivation

    E-Print Network [OSTI]

    Coughlin, Joseph F.

    This paper aims to provide reliable indications of driver drowsiness based on the characteristics of driver-vehicle interaction. A test bed was built under a simulated driving environment, and a total of 12 subjects ...

  16. Evaluation of teenage driver understanding of traffic control devices

    E-Print Network [OSTI]

    Ford, Garry Lee

    1999-01-01T23:59:59.000Z

    This research documents the evaluation of teenage graphics. drivers with regards to their understanding of 53 traffic control devices. A multiple choice survey was developed and administered to a group of teenage drivers between 15 and 18 years...

  17. Solar Supply Chain and Market Driver Analysis 

    E-Print Network [OSTI]

    Martinez, Nicholas 1990-

    2012-05-09T23:59:59.000Z

    This study aims to explore the evolution of the photovoltaic supply chain in the United States and the drivers which foster growth of the solar market. The study will gather knowledge on the growth of the solar market and roles of different firms...

  18. MOTOR VEHICLE USE PROGRAM DRIVER SAFETY TIPS

    E-Print Network [OSTI]

    MOTOR VEHICLE USE PROGRAM DRIVER SAFETY TIPS Observe Speed Limits and Traffic Laws ­ Allow - Employees who drive Institute or privately owned vehicles on Institute business must possess and carry person. Insurance - Employees who operate their privately owned vehicles on Institute business shall

  19. Driver expectancy in locating automotive controls

    E-Print Network [OSTI]

    Francis, Dawn Suzette

    1990-01-01T23:59:59.000Z

    Major Subject: Industrial Engineering DRIVER EXPECTANCY IN LOCATING AUTOMOTIVE CONTROLS A Thesis by DAWN SUZETTE FRANCIS Approved as to style and content by: R. Dale Huchi son (Chair of Committee) Rodger . . ppa (Member) Waymon L ohnston (M er... assessment of automotive industry practices in 1971 and concluded that only 50% of controls/displays on various models could be said to have a common location. Perel (1974) reviewed prior research and found that it would be difficult to pinpoint...

  20. Revealing {\\delta} Cephei's Secret Companion and Intriguing Past

    E-Print Network [OSTI]

    Anderson, Richard I; Holl, Berry; Eyer, Laurent; Palaversa, Lovro; Mowlavi, Nami; Süveges, Maria; Roelens, Maroussia

    2015-01-01T23:59:59.000Z

    Classical Cepheid variable stars are crucial calibrators of the cosmic distance scale thanks to a relation between their pulsation periods and luminosities. Their archetype, {\\delta} Cephei, is an important calibrator for this relation. In this paper, we show that {\\delta} Cephei is a spectroscopic binary based on newly-obtained high-precision radial velocities. We combine these new data with literature data to determine the orbit, which has period 2201 days, semi-amplitude 1.5 km/s, and high eccentricity (e = 0.647). We re-analyze Hipparcos intermediate astrometric data to measure {\\delta} Cephei's parallax ($\\varpi = 4.09 \\pm 0.16$ mas) and find tentative evidence for an orbital signature, although we cannot claim detection. We estimate that Gaia will fully determine the astrometric orbit. Using the available information from spectroscopy, velocimetry, astrometry, and Geneva stellar evolution models ($M_{\\delta Cep} ~ 5.0 - 5.25 M_\\odot$), we constrain the companion mass to within $0.2 < M_2 < 1.2 M_\\...

  1. FERPA Training Guide FERPA Training Steps

    E-Print Network [OSTI]

    FERPA Training Guide 1 FERPA Training Steps Graduate committee chairs and co-chairs are encouraged-time FERPA training via TrainTraq (if not previously completed). When trying to access the Graduate Committee Degree Evaluation too, the following screen will display if you have not completed FERPA training

  2. ORISE: Health Physics Training

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

    Health Physics Training Student performs an analysis during an ORAU health physics training course Training and educating a highly skilled workforce that can meet operational...

  3. Training | Advanced Photon Source

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

    Beam Time ESAF Contacts Calendars User Community Scientific Access Site AccessVisit Training See also: Argonne WBT Argonne eJHQ ASDACIS Training Courses Training All core...

  4. IRC+10216 Unveils Her Heart: A Companion in 2011 Seen By Hubble

    E-Print Network [OSTI]

    Kim, Hyosun; Mauron, Nicolas

    2014-01-01T23:59:59.000Z

    For the nearest carbon-rich star IRC+10216 with a very high mass loss rate, there have been observational, indirect indications pointing to the existence of a binary companion, such as a bipolar nebula and a spiral-like circumstellar pattern. However, to date, no companion has been reported. Here, we report that the latest Hubble Space Telescope image at an epoch of 2011 exhibits a dramatic change of its innermost region from at the earlier epochs, revealing a faint point-like object at about 0.5 arcsec from the brightness peak. We interpret the sudden core appearance as due to dissipation of intervening circumstellar dust, in coherence with the brightening trend of the recently released Catalina survey photometric database. We interpret the faint point-like source as the companion and discuss the implications of this discovery, which reinforces the binary-induced mass loss scenarios. IRC+10216 and her orbiting companion deserve careful but confidential monitoring.

  5. Improved gauge driver for the generalized harmonic Einstein system

    SciTech Connect (OSTI)

    Lindblom, Lee; Szilagyi, Bela [Theoretical Astrophysics 350-17, California Institute of Technology, Pasadena, California 91125 (United States)

    2009-10-15T23:59:59.000Z

    A new gauge driver is introduced for the generalized harmonic (GH) representation of Einstein's equation. This new driver allows a rather general class of gauge conditions to be implemented in a way that maintains the hyperbolicity of the combined evolution system. This driver is more stable and effective and, unlike previous drivers, allows stable evolutions using the dual-frame evolution technique. Appropriate boundary conditions for this new gauge driver are constructed, and a new boundary condition for the 'gauge' components of the spacetime metric in the GH Einstein system is introduced. The stability and effectiveness of this new gauge driver are demonstrated through numerical tests, which impose a new damped-wave gauge condition on the evolutions of single black-hole spacetimes.

  6. The rotation speed of the companion star in V395 Car (=2S0921--630)

    E-Print Network [OSTI]

    T. Shahbaz; E. Kuulkers; P. A. Charles; F. van der Hooft; J. Casares; J. van Paradijs

    1998-12-23T23:59:59.000Z

    We have obtained high resolution optical spectroscopy of the accretion disc corona source 2S0921--630 (=V395 Car) that constrains the spectral type of the companion star to be most probably K0III. At 6500A the secondary star is found to contribute ~25% to the observed flux. The absorption line spectrum of the K0III companion star is broadened (compared to template stars) by a projected rotational velocity of 65+/-9 km/s (1 sigma).

  7. WIDE COMPANIONS TO HIPPARCOS STARS WITHIN 67 pc OF THE SUN

    SciTech Connect (OSTI)

    Tokovinin, Andrei [Cerro Tololo Inter-American Observatory, Casilla 603, La Serena (Chile); Lepine, Sebastien, E-mail: atokovinin@ctio.noao.edu, E-mail: lepine@amnh.org [Department of Astrophysics, Division of Physical Sciences, American Museum of Natural History, Central Park West at 79th Street, New York, NY 10024 (United States)

    2012-10-01T23:59:59.000Z

    A catalog of common-proper-motion (CPM) companions to stars within 67 pc of the Sun is constructed based on the SUPERBLINK proper-motion survey. It contains 1392 CPM pairs with angular separations 30'' < {rho} < 1800'', relative proper motion between the two components less than 25 mas yr{sup -1}, and magnitudes and colors of the secondaries consistent with those of dwarfs in the (M{sub V} , V - J) diagram. In addition, we list 21 candidate white dwarf CPM companions with separations under 300'', about half of which should be physical. We estimate a 0.31 fraction of pairs with red dwarf companions to be physical systems (about 425 objects), while the rest (mostly wide pairs) are chance alignments. For each candidate companion, the probability of a physical association is evaluated. The distribution of projected separations s of the physical pairs between 2 kAU and 64 kAU follows f(s){proportional_to}s {sup -1.5}, which decreases faster than Oepik's law. We find that solar-mass dwarfs have no less than 4.4% {+-} 0.3% companions with separations larger than 2 kAU, or 3.8% {+-} 0.3% per decade of orbital separation in the 2-16 kAU range. The distribution of mass ratio of those wide companions is approximately uniform in the 0.1 < q < 1.0 range, although we observe a dip at q {approx_equal} 0.5 which, if confirmed, could be evidence of bimodal distribution of companion masses. New physical CPM companions to two exoplanet host stars are discovered.

  8. Is the X-ray pulsating companion of HD 49798 a possible type Ia supernova progenitor?

    E-Print Network [OSTI]

    Liu, Dong-Dong; Wu, Cheng-Yuan; Wang, Bo

    2015-01-01T23:59:59.000Z

    HD 49798 (a hydrogen depleted subdwarf O6 star) with its massive white dwarf (WD) companion has been suggested to be a progenitor candidate of type Ia supernovae (SNe Ia). However, it is still uncertain whether the companion of HD 49798 is a carbon-oxygen (CO) WD or an oxygen-neon (ONe) WD. A CO WD will explode as an SN Ia when its mass grows approach to Chandrasekhar mass, while the outcome of an accreting ONe WD is likely to be a neutron star. We followed a series of Monte Carlo binary population synthesis approach to simulate the formation of ONe WD + He star systems. We found that there is almost no orbital period as large as HD 49798 with its WD companion in these ONe WD + He star systems based on our simulations, which means that the companion of HD 49798 might not be an ONe WD. We suggest that the companion of HD 49798 is most likely a CO WD, which can be expected to increase its mass to the Chandrasekhar mass limit by accreting He-rich material from HD 49798. Thus, HD 49798 with its companion may prod...

  9. Regulatory Drivers | netl.doe.gov

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level:Energy: Grid Integration Redefining What's PossibleRadiation Protection Technical s o Freiberg and SondershausenRegulatory Drivers In July 7,

  10. Analyzing Fuel Saving Opportunities through Driver Feedback Mechanisms...

    Office of Environmental Management (EM)

    Fuel Saving Opportunities through Driver Feedback Mechanisms 2011 DOE Hydrogen and Fuel Cells Program, and Vehicle Technologies Program Annual Merit Review and Peer...

  11. analysis identifies driver: Topics by E-print Network

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

    et al. 2010 Invasive sensors to monitor physiological signals EEG, ECG, pulse@utdallas.edu MSP - CRSS Long-Term Goal: Monitoring Driver Behavior 5 "%"&'(...

  12. aged drivers: Topics by E-print Network

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

    et al. 2010 Invasive sensors to monitor physiological signals EEG, ECG, pulse@utdallas.edu MSP - CRSS Long-Term Goal: Monitoring Driver Behavior 5 "%"&'(...

  13. Assessor Training Measurement Uncertainty

    E-Print Network [OSTI]

    NVLAP Assessor Training Measurement Uncertainty #12;Assessor Training 2009: Measurement Uncertainty Training 2009: Measurement Uncertainty 3 Measurement Uncertainty ·Calibration and testing labs performing Training 2009: Measurement Uncertainty 4 Measurement Uncertainty ·When the nature of the test precludes

  14. Basic Instructor Training

    Broader source: Energy.gov [DOE]

    The Emergency Operations Training Academy, NA 40.2, Readiness and Training, Albuquerque, NM is pleased to announce site certification by the National Training Center for conduct of the Basic Instructor Training class

  15. CLAIMANT AUTO ACCIDENT REPORT For Completion by Driver

    E-Print Network [OSTI]

    Tullos, Desiree

    CLAIMANT AUTO ACCIDENT REPORT For Completion by Driver D E P A R T M E N T O F A D M I N I S T R Address City State Zip For what purpose was car being used at time of accident? Has damage been repaired signals did you give? Other Driver? Who investigated? Who Cited and Why? Describe Accident CONTINUE

  16. EHSO TRAINING CLASSES Fire Safety Program Training

    E-Print Network [OSTI]

    EHSO TRAINING CLASSES Fire Safety Program Training 1. Fire Safety (60 minutes) Instruction includes an actual fire eperience. 2. Fire Extinguisher Training (30 minutes) A practical demonstration on actual burnable liquid fires. This practical extinguisher training is a critical portion of the fire

  17. Media Training

    ScienceCinema (OSTI)

    None

    2011-10-06T23:59:59.000Z

    With the LHC starting up soon, the world's media are again turning their attention to CERN. We're all likely to be called upon to explain what is happening at CERN to media, friends and neighbours. The seminar will be given by BBC television news journalists Liz Pike and Nadia Marchant, and will deal with the kind of questions we're likely to be confronted with through the restart period. The training is open for everybody. Make sure you arrive early enough to get a seat - there are only 200 seats in the Globe. The session will also be webcast: http://webcast.cern.ch/

  18. Cori Training

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level: National5Sales for4,645 3,625govInstrumentstdmadapInactiveVisitingContract Management Fermi Site Office (FSO) FSOConvertingCopyNaturalTraining

  19. Training Links

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level: National5Sales for4,645U.S. DOE Office of ScienceandMesa del SolStrengthening a solidSynthesisAppliances » TopTours SignTrackingTraining

  20. The HI Companions of HII Galaxies and Low Surface Brightness Dwarf Galaxies

    E-Print Network [OSTI]

    Christopher L. Taylor

    1996-11-18T23:59:59.000Z

    I study the VLA HI survey of HII galaxies by Taylor et al. (1995, ApJS, 99, 427; 1996, ApJS, 102, 189) and the VLA HI survey of low surface brightness (LSB) dwarf galaxies by Taylor et al. (1996, ApJS, in press) to investigate the role of galaxy interactions in triggering the bursts of massive star formation seen in HII galaxies. I find that the companion rate for HII galaxies is more than twice that of LSB dwarfs (p[HII] = 0.57 p[LSB] = 0.24). I examine the completeness of the companion samples detected by the two surveys, finding that because they were observed in identical fashions, there are no relative biases to cause one sample or the other to have more companions. Thus I conclude that the difference in the number of HI rich companions is genuine, and signifies a difference in the local, small scale environments between the two types of galaxy. I search through published galaxy catalogs to study the large scale environments of the two samples, finding that at large separations, the two samples exist in very similar environments on average. The difference in companion rates between HII galaxies and LSB dwarfs supports the idea that the bursts of star formation are triggered by galaxy interactions.

  1. THE ABSENCE OF EX-COMPANIONS IN TYPE Ia SUPERNOVA REMNANTS

    SciTech Connect (OSTI)

    Di Stefano, R. [Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138 (United States); Kilic, Mukremin, E-mail: rd@cfa.harvard.edu, E-mail: kilic@ou.edu [Homer L. Dodge Department of Physics and Astronomy, University of Oklahoma, 440 West Brooks Street, Norman, OK 73019 (United States)

    2012-11-01T23:59:59.000Z

    Type Ia supernovae (SNe Ia) play important roles in our study of the expansion and acceleration of the universe, but because we do not know the exact nature or natures of the progenitors, there is a systematic uncertainty that must be resolved if SNe Ia are to become more precise cosmic probes. No progenitor system has ever been identified either in the pre- or post-explosion images of a Ia event. There have been recent claims for and against the detection of ex-companion stars in several SNe Ia remnants. These studies, however, usually ignore the angular momentum gain of the progenitor white dwarf (WD), which leads to a spin-up phase and a subsequent spin-down phase before explosion. For spin-down timescales greater than 10{sup 5} years, the donor star could be too dim to detect by the time of explosion. Here we revisit the current limits on ex-companion stars to SNR 0509-67.5, a 400-year-old remnant in the Large Magellanic Cloud. If the effects of possible angular momentum gain on the WD are included, a wide range of single-degenerate progenitor models are allowed for this remnant. We demonstrate that the current absence of evidence for ex-companion stars in this remnant, as well as other SNe Ia remnants, does not necessarily provide the evidence of absence for ex-companions. We discuss potential ways to identify such ex-companion stars through deep imaging observations.

  2. Discovery of blue companions to two southern Cepheids: WW Car and FN Vel

    E-Print Network [OSTI]

    Kovtyukh, V; Chekhonadskikh, F; Lemasle, B; Belik, S

    2015-01-01T23:59:59.000Z

    A large number of high-dispersion spectra of classical Cepheids were obtained in the region of the CaII H+K spectral lines. The analysis of these spectra allowed us to detect the presence of a strong Balmer line, H$\\epsilon$, for several Cepheids, interpreted as the signature of a blue companion: the presence of a sufficiently bright blue companion to the Cepheid results in a discernible strengthening of the CaII H + Hepsilon line relative to the CaII K line. We investigated 103 Cepheids, including those with known hot companions (B5-B6 main-sequence stars) in order to test the method. We could confirm the presence of a companion to WW Car and FN Vel (the existence of the former was only suspected before) and we found that these companions are blue hot stars. The method remains efficient when the orbital velocity changes in a binary system cannot be revealed and other methods of binarity detection are not efficient.

  3. Ris Energy Report 5 Global drivers for transformation of energy systems 3 Global drivers for transformation of energy

    E-Print Network [OSTI]

    of greenhouse gases has brought a new political rationale for the development of more climate-friendly energy in the global energy market of rapidly-expanding national economies, notably China and India. TogetherRisø Energy Report 5 Global drivers for transformation of energy systems 3 Global drivers

  4. Design consistency and driver error as reflected by driver workload and accident rates

    E-Print Network [OSTI]

    Wooldridge, Mark Douglas

    1992-01-01T23:59:59.000Z

    primary directions, speed consistency and driver workload. Speed consistency consists of analyzing predicted speeds on a highway and striving to keep those speeds within a narrow range. Several major research studies have provided methodologies... participating in the Texas Department of Transportation's Masters in Civil Engineering (MSCE) program, and performed the research that formed the basis for this report under the auspices of the Texas Transportation Institute. The data used as a basis...

  5. Hydraulic Cooling Tower Driver- The Innovation

    E-Print Network [OSTI]

    Dickerson, J. A.

    -drive eliminates these items from the drive train and puts the same electric motor HP at ground level close coupled to a hydraulic pump, filters, and oil reservoir. Hydraulic lines bring oil pressure to the hydraulic motor, which is more than 75% less weight than...

  6. A Possible Brown Dwarf Companion to the White Dwarf GD1400

    E-Print Network [OSTI]

    J. Farihi; M. Christopher

    2004-07-01T23:59:59.000Z

    An unresolved, likely L dwarf companion to the DA white dwarf GD1400 is reported. This would be only the second such system known, discovered 17 years after the prototype L dwarf, GD165B, was determined to be a companion to a white dwarf. Photometric observations and model predicted stellar parameters of the well studied white dwarf primary indicate that GD1400B has $J-K\\ga2.0$ and $M_K=12.13$ mag. If correct, this would place GD1400B at spectral type L6, and it would be the lowest luminosity unevolved companion known to a white dwarf, and thus a definite brown dwarf. However, a low resolution Keck NIRSPEC $2.1-2.4\\mu$m spectrum may not be consistent with known L dwarfs. Uncertainties in classification remain until the binary is resolved or a trigonometric parallax is measured.

  7. The contact binary GSC 04778-00152 with a visual companion

    E-Print Network [OSTI]

    T. Tuvikene; T. Eenmäe; C. Sterken; E. Brogt

    2008-09-11T23:59:59.000Z

    Photometric and spectroscopic observations of the unstudied 12th-magnitude eclipsing binary GSC 04778-00152 are presented. We report the discovery of a visual companion about 1 mag fainter and 2 arcsec away from the binary. By subtracting the light contribution of the visual companion, we obtain the UBVRI light curves of the binary system alone. The shape of the light curve indicates that GSC 04778-00152 is an A-type W UMa contact binary. From light-curve modeling, we derive parameters of the binary system.

  8. Training and Organizational Development

    E-Print Network [OSTI]

    Stephens, Graeme L.

    Training and Organizational Development Contact: Ellen Audley Assistant, 491-1376, Ellen coordinates training and development opportunities for personal and professional growth for Colorado State. Customized training and organizational development consulting services are also available. Class Locations

  9. Assessor Training Assessment Techniques

    E-Print Network [OSTI]

    NVLAP Assessor Training Assessment Techniques: Communication Skills and Conducting an Assessment listener ·Knowledgeable Assessor Training 2009: Assessment Techniques: Communication Skills & Conducting, truthful, sincere, discrete · Diplomatic · Decisive · Selfreliant Assessor Training 2009: Assessment

  10. Assessor Training Nonconformities

    E-Print Network [OSTI]

    NVLAP Assessor Training Nonconformities #12;Nonconformity ­ nonfulfillment of a specified Assessor Training 2009: Nonconformities 2 Definitions #12;Nonconformities ­ All nonconformities must of the lab. Assessor Training 2009: Nonconformities 3 Implications #12;Specified requirements are defined

  11. Training and Organizational Development

    E-Print Network [OSTI]

    Training and Organizational Development Contact: Ellen Audley Assistant, (970) 491-1376, Ellen 1 of 5 This office coordinates training and development opportunities for personal and professional and state classified personnel. Customized training and orga- nizational development consulting services

  12. Training and Development

    E-Print Network [OSTI]

    California at Santa Cruz, University of

    Training and Development Administration Assistant Vice Chancellor Lori Castro VC Business Senior Manager Conflict Resolution Nancy Heischman Training Coordinator Vacant Principal Technical Training Consultant Frank Widman Health Care Facilitator / Interim Benefits Manager Frank Trueba Disability

  13. Training and Organizational Development

    E-Print Network [OSTI]

    Stephens, Graeme L.

    Training and Organizational Development Contact: Ellen Audley Assistant, 491-1376, Ellen. Customized training and organizational development consulting services are also available. Class Location the top of the page ·Choose the "Training & Organizational Development" from the selection box ·Select

  14. Training and Organizational Development

    E-Print Network [OSTI]

    Rutledge, Steven

    Training and Organizational Development Contacts: Ellen Audley Customer Support, (970) 491-professional staff and state classi- fied personnel. Customized training and organizational development consulting of the page ·Choose the "Training & Organizational Development" from the selection box ·Select the "Login" tab

  15. Training and Organizational Development

    E-Print Network [OSTI]

    Stephens, Graeme L.

    Training and Organizational Development Contact: Ellen Audley Assistant, (970) 491-1376, Ellen and state classified personnel. Customized training and organizational development consulting services the "Register for Workshops" button near the top of the page ·Choose the "Training & Organizational Development

  16. Training and Organizational Development

    E-Print Network [OSTI]

    Stephens, Graeme L.

    Training and Organizational Development Contact: Ellen Audley Assistant, 491-1376, Ellen training and organizational development consulting services are also available. Class Location: Johnson the top of the page ·Choose the "Training & Organizational Development" from the selection box ·Select

  17. Training | Advanced Photon Source

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

    Beam Time ESAF Contacts Calendars User Community Scientific Access Site AccessVisit Training See also: Argonne WBT Argonne eJHQ APS Beamline Shielding ASDACIS Training Courses...

  18. Dealing with power games in a companion modelling process: lessons from community water management in Thailand highlands

    E-Print Network [OSTI]

    Paris-Sud XI, Université de

    with power games in a companion modelling process: lessons from community water management in Thailand facilitation methods that helped to manage power asymmetries and to level the playing field but we also discuss1 Dealing with power games in a companion modelling process: lessons from community water

  19. An Optimization Framework for Driver Feedback Systems

    SciTech Connect (OSTI)

    Malikopoulos, Andreas [ORNL; Aguilar, Juan P. [Georgia Institute of Technology

    2013-01-01T23:59:59.000Z

    Modern vehicles have sophisticated electronic control units that can control engine operation with discretion to balance fuel economy, emissions, and power. These control units are designed for specific driving conditions (e.g., different speed profiles for highway and city driving). However, individual driving styles are different and rarely match the specific driving conditions for which the units were designed. In the research reported here, we investigate driving-style factors that have a major impact on fuel economy and construct an optimization framework to optimize individual driving styles with respect to these driving factors. In this context, we construct a set of polynomial metamodels to reflect the responses produced in fuel economy by changing the driving factors. Then, we compare the optimized driving styles to the original driving styles and evaluate the effectiveness of the optimization framework. Finally, we use this proposed framework to develop a real-time feedback system, including visual instructions, to enable drivers to alter their driving styles in response to actual driving conditions to improve fuel efficiency.

  20. FFAG ACCELERATOR PROTON DRIVER FOR NEUTRINO FACTORY.

    SciTech Connect (OSTI)

    RUGGIERO, A.

    2005-06-21T23:59:59.000Z

    This paper is the summary of a conceptual study of a Proton Driver for Neutrino Factory based on the use of a Fixed-Field Alternating-Gradient (FFAG) Accelerator. The required proton energy range for an optimum neutrino production is 5 to 12 GeV. This can be accomplished with a group of three concentric rings each with 807 m circumference [1]. FFAG Accelerators [2] have the capability to accelerate charged particles over a large momentum range ({+-}30-50%) and the feature of constant bending and focusing fields. Particles can be accelerated very fast at the rate given by the accelerating field of RF cavities placed in proper locations between magnets. The performance of FFAG accelerators is to be placed between that of Super-Conducting Linear Accelerators (SCL), with which they share the fast acceleration rate, and Rapid-Cycling Synchrotrons (RCS), as they allow the beam to re-circulate over fewer revolutions. Brookhaven National Laboratory is involved in the study of feasibility of FFAG Accelerators to accelerate intense beams of protons in the GeV energy range for a variety of applications the most important of which is the Upgrade of the Alternating Gradient Synchrotron (AGS) with a new FFAG injector [3] accelerating from 400 MeV to 1.5 GeV. The ring would be housed in the AGS tunnel and has henceforth a circumference of 807 m.

  1. Threat assessment design for driver assistance system at intersections

    E-Print Network [OSTI]

    Aoude, Georges

    This paper considers the decision-making problem for a human-driven vehicle crossing a road intersection in the presence of other, potentially errant, drivers. Our approach relies on a novel threat assessment module, which ...

  2. active gate driver: Topics by E-print Network

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

    chip for SiC FET-driver chip is intended to drive SiC power FETs in DC-DC converters in a hybrid electric vehicle Tolbert, Leon M. 7 Current Balancing Control for Parallel...

  3. A Retroreflective Sheeting Selection Technique for Nighttime Drivers' Needs

    E-Print Network [OSTI]

    Paulus, Susan C.

    2010-07-14T23:59:59.000Z

    In this thesis, the author developed a retroreflective sheeting selection technique for traffic signs. Previous research was used to determine the luminance needed by drivers (demand luminance). The author used roadways scenarios to determine...

  4. Visual Attention and Driver Performance at Horizontal Curves

    E-Print Network [OSTI]

    Brimley, Bradford K.

    2014-12-02T23:59:59.000Z

    Despite the frequency with which drivers encounter curves on highways, curves are regularly identified as locations that experience disproportionately high crash rates. Crash data suggest that inattention is one of the leading causes of crashes...

  5. ambulance drivers: Topics by E-print Network

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

    Summary: BGD 9, 14437-14473, 2012 Soil carbon drivers and benchmarks in Earth system models K. E. O. Todd if available. Causes of variation in soil carbon predictions from...

  6. Your Role as a Jefferson Lab Fleet Vehicle Driver | Jefferson...

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

    Your Role as a Jefferson Lab Fleet Vehicle Driver Responsibility Number One - Safe Driving As a vehicle operator, it is up to you to drive safely and sensibly to avoid crashes. The...

  7. Shaopeng Zhang, Wei Jeng A Facebook Companion for an Adaptive Social Site

    E-Print Network [OSTI]

    Brusilovsky, Peter

    1 Shaopeng Zhang, Wei Jeng A Facebook Companion for an Adaptive Social. The first alternative is to develop a Facebook application with a wide range of functionalities to view and share event information from Eventur on Facebook platform. While we were discussing with Danielle

  8. ON THE ORIGIN OF THE SUPERGIANT H I SHELL AND PUTATIVE COMPANION IN NGC 6822

    SciTech Connect (OSTI)

    Cannon, John M.; O'Leary, Erin M. [Department of Physics and Astronomy, Macalester College, 1600 Grand Avenue, Saint Paul, MN 55105 (United States); Weisz, Daniel R. [Department of Astronomy, University of Washington, Seattle, WA 98195 (United States); Skillman, Evan D. [Minnesota Institute for Astrophysics, University of Minnesota, Minneapolis, MN 55455 (United States); Dolphin, Andrew E. [Raytheon Company, 1151 East Hermans Road, Tucson, AZ 85706 (United States); Bigiel, Frank [Institut fuer Theoretische Astrophysik, Universitaet Heidelberg, Albert-Ueberle-Str. 2, 69120 Heidelberg (Germany); Cole, Andrew A.; Walter, Fabian [School of Mathematics and Physics, University of Tasmania, Private Bag 37, Hobart 7001, Tasmania (Australia); De Blok, W.J.G., E-mail: jcannon@macalester.edu, E-mail: eoleary@macalester.edu, E-mail: dweisz@astro.washington.edu, E-mail: skillman@astro.umn.edu, E-mail: adolphin@raytheon.com, E-mail: bigiel@uni-heidelberg.de, E-mail: andrew.cole@utas.edu.au, E-mail: edeblok@ast.uct.ac.za, E-mail: walter@mpia.de [Department of Astronomy, University of Cape Town, Rondebosch 7700 (South Africa)

    2012-03-10T23:59:59.000Z

    We present new Hubble Space Telescope Advanced Camera for Surveys imaging of six positions spanning 5.8 kpc of the H I major axis of the Local Group dIrr NGC 6822, including both the putative companion galaxy and the large H I hole. The resulting deep color-magnitude diagrams show that NGC 6822 has formed >50% of its stars in the last {approx}5 Gyr. The star formation histories of all six positions are similar over the most recent 500 Myr, including low-level star formation throughout this interval and a weak increase in star formation rate during the most recent 50 Myr. Stellar feedback can create the giant H I hole, assuming that the lifetime of the structure is longer than 500 Myr; such long-lived structures have now been observed in multiple systems and may be the norm in galaxies with solid-body rotation. The old stellar populations (red giants and red clump stars) of the putative companion are consistent with those of the extended halo of NGC 6822; this argues against the interpretation of this structure as a bona fide interacting companion galaxy and against its being linked to the formation of the H I hole via an interaction. Since there is no evidence in the stellar population of a companion galaxy, the most likely explanation of the extended H I structure in NGC 6822 is a warped disk inclined to the line of sight.

  9. Brown Dwarf Companions to G-type Stars. I: Gliese 417B and Gliese 584C

    E-Print Network [OSTI]

    J. Davy Kirkpatrick; Conard C. Dahn; David G. Monet; I. Neill Reid; John E. Gizis; James Liebert; Adam J. Burgasser

    2001-03-14T23:59:59.000Z

    We present astrometric and spectroscopic observations confirming that two nearby G dwarf systems (Gliese 417 = BD+36 2162 and Gliese 584AB = eta CrB AB) have a widely separated, L dwarf, substellar companion. Using age estimates of the G dwarf primaries, we estimate masses for these L dwarfs from theoretical evolutionary tracks. For the L4.5 dwarf Gl 417B we estimate an age of 0.08-0.3 Gyr and a mass of 0.035+/-0.015 M_sun. For the L8 dwarf Gl 584C we estimate an age of 1.0-2.5 Gyr and a mass of 0.060+/-0.015 M_sun. This latter object also shows evidence of spectrum variability, which may be due to surface inhomogeneities rotating into and out of view. These new companions are also compared to six other L dwarf and T dwarf companions previously recognized. For the L dwarf companions, ages implied by the presence or absence of lithium are consistent with ages inferred from the primaries alone.

  10. Preprint: Nature, 387, 685686. June 12 1997. An asteroidal companion to the Earth

    E-Print Network [OSTI]

    Wiegert, Paul

    Preprint: Nature, 387, 685­686. June 12 1997. An asteroidal companion to the Earth Paul A. Wiegert Near­Earth asteroids (or NEAs) are our closest neighbours in the Solar System--- some of these objects have been known to pass closer to the Earth than the Moon 1 . These objects, which range in size from

  11. Science Drivers and Technical Challenges for Advanced Magnetic Resonance

    SciTech Connect (OSTI)

    Mueller, Karl T.; Pruski, Marek; Washton, Nancy M.; Lipton, Andrew S.

    2013-03-07T23:59:59.000Z

    This report recaps the "Science Drivers and Technical Challenges for Advanced Magnetic Resonance" workshop, held in late 2011. This exploratory workshop's goal was to discuss and address challenges for the next generation of magnetic resonance experimentation. During the workshop, participants from throughout the world outlined the science drivers and instrumentation demands for high-field dynamic nuclear polarization (DNP) and associated magnetic resonance techniques, discussed barriers to their advancement, and deliberated the path forward for significant and impactful advances in the field.

  12. Look-ahead Driver Feedback and Powertrain Management

    SciTech Connect (OSTI)

    Verma, Rajeev

    2014-12-31T23:59:59.000Z

    Commercial medium and heavy vehicles, though only a small portion of total vehicle population, play a significant role in energy consumption. In 2012, these vehicles accounted for about 5775.5 trillion btu of energy consumption and 408.8 million tons of CO2 emissions annually, which is a quarter of the total energy burden of highway transportation in the United States [1]. This number is expected to surpass passenger car fuel use within the next few decades. In the meantime, most commercial vehicle fleets are running at a very low profit margin. It is a wellknown fact that fuel economy can vary significantly between drivers, even when they operate the same vehicle on the same route. According to the US Environmental Protection Agency (EPA) and Natural Resource Canada (NRCan), there is up to 35% fuel economy difference between drivers within the same commercial fleet [2] [3], [4]. Similar results were obtained from a Field Operation Test conducted by Eaton Corporation [5]. During this test as much as 30% fuel economy difference was observed among pick-up-and-delivery drivers and 11% difference was observed among line-haul drivers. The driver variability can be attributed to the fact that different drivers react differently to driving conditions such as road grade, traffic, speed limits, etc. For instance, analysis of over 600k miles of naturalistic heavy duty truck driving data [5] indicates that an experienced driver anticipates a downhill and eases up on the throttle to save fuel while an inexperienced driver lacks this judgment.

  13. Alternative highway sign alphabet styles for older drivers

    E-Print Network [OSTI]

    Tan, Carol Hannah

    1991-01-01T23:59:59.000Z

    ALTERNATIVE HIGHWAY SIGN ALPHABET STYLES FOR OLDER DRIVERS A Thesis by Carol Hannah Tan Submitted to the Office of Graduate Studies of Texas A&M University in partial fulfillment of the requirements for the degree of MASTER OF SCIENCE May... (Member) Jame T. . Yao (Head of partment) May 1991 ABSTRACT Alternative Highway Sign Alphabet Styles for Older Drivers. (May 1991) Carol Hannah Tan, B. S. , Texas A8 M University Chair of Advisory Committee: Dr. Daniel B. Farnbro In the United...

  14. Driver tension responses generated by various levels of intersection illumination

    E-Print Network [OSTI]

    Franklin, Weldon Clifford

    1962-01-01T23:59:59.000Z

    DRIVER TENSION RESPONSES GENERATED BY VARIOUS LEVELS OF INTERSECTION ILLUMINATION A Thesis By WELDON CLIFFORD FRANKLIN Submitted to the Graduate School of the Agricultural and Mechanical College of Texas in partial fulfillment... of the requirements for the degree of MASTER OF SCIENCE August 1962 Major Subj ect: Civil Engineering DRIVER TENSION RESPONSES GENERATED BY VARIOUS LEVELS OF INTERSECTION ILLUMINATION A Thesis By WELDON CLIFFORD FRANKLIN Approved as to style and content by...

  15. National Training and Education Resource Advanced Authoring Training

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

    Advanced Authoring Training Participant Guide NTER Advanced Authoring Training Participant Guide (032012 pw) 2 Contents OBJECTIVES ......

  16. Assessor Training International

    E-Print Network [OSTI]

    NVLAP Assessor Training International Arrangements #12;Assessor Training 2009: International;Assessor Training 2009: International Arrangements 3 2009 is the 10th anniversary of the signing granted by a signatory to the ILAC Arrangement #12;Assessor Training 2009: International Arrangements 4

  17. Assessor Training NVLAP Communications

    E-Print Network [OSTI]

    NVLAP Assessor Training NVLAP Communications #12;Assessor Training 2009: NVLAP Communications 2 of assessment. ·Will also discuss other tools, such as internal database and webbased. #12;Assessor Training of assessors at lab · Assignments occur quarterly, in sync with renewal cycles. #12;Assessor Training 2009

  18. Assessor Training Traceability

    E-Print Network [OSTI]

    NVLAP Assessor Training Traceability #12;Assessor Training 2009: Traceability 2 Important References ·ILAC P10:2002 ·NVLAP Handbook 150:2006, Annex B Assessor Training 2009: Traceability 2 #12;Assessor Training 2009: Traceability 3 ILAC P10:2002 ·Section 1.4: Characteristics of traceability

  19. Professional Training Information Pack

    E-Print Network [OSTI]

    Davies, Christopher

    Intending Professional Training Students Year 2 Information Pack #12;- 1 - Applying for a Professional Training Placement To be allowed to do the Professional Training you must have enrolled on one must talk to Dr J. M. Thompson immediately. General introduction to professional training Students

  20. VERY LOW MASS STELLAR AND SUBSTELLAR COMPANIONS TO SOLAR-LIKE STARS FROM MARVELS. IV. A CANDIDATE BROWN DWARF OR LOW-MASS STELLAR COMPANION TO HIP 67526

    SciTech Connect (OSTI)

    Jiang Peng; Ge Jian; De Lee, Nathan; Fleming, Scott W.; Lee, Brian L.; Ma Bo; Wang, Ji [Astronomy Department, University of Florida, 211 Bryant Space Science Center, P.O. Box 112055, Gainesville, FL 32611 (United States); Cargile, Phillip; Hebb, Leslie; Stassun, Keivan G. [Department of Physics and Astronomy, Vanderbilt University, Nashville, TN 37235 (United States); Crepp, Justin R. [Department of Physics, University of Notre Dame, 225 Nieuwland Science Hall, Notre Dame, IN 46556 (United States); Porto de Mello, Gustavo F.; Ferreira, Leticia D. [Observatorio do Valongo, Universidade Federal do Rio de Janeiro, Ladeira do Pedro Antonio, 43, CEP: 20080-090, Rio de Janeiro, RJ (Brazil); Esposito, Massimiliano; Femenia, Bruno; Gonzalez Hernandez, Jonay I. [Instituto de Astrofisica de Canarias, C/Via Lactea S/N, E-38200 La Laguna (Spain); Gaudi, B. Scott [Department of Astronomy, The Ohio State University, 140 West 18th Avenue, Columbus, OH 43210 (United States); Ghezzi, Luan [Laboratorio Interinstitucional de e-Astronomia (LIneA), Rio de Janeiro, RJ 20921-400 (Brazil); Wisniewski, John P. [Homer L. Dodge Department of Physics and Astronomy, University of Oklahoma, 440 West Brooks Street, Norman, OK 73019 (United States); Agol, Eric, E-mail: jpaty@mail.ustc.edu.cn [Department of Astronomy, University of Washington, Box 351580, Seattle, WA 98195-1580 (United States); and others

    2013-09-15T23:59:59.000Z

    We report the discovery of a candidate brown dwarf (BD) or a very low mass stellar companion (MARVELS-5b) to the star HIP 67526 from the Multi-object Apache point observatory Radial Velocity Exoplanet Large-area Survey (MARVELS). The radial velocity curve for this object contains 31 epochs spread over 2.5 yr. Our Keplerian fit, using a Markov Chain Monte Carlo approach, reveals that the companion has an orbital period of 90.2695{sup +0.0188}{sub -0.0187} days, an eccentricity of 0.4375 {+-} 0.0040, and a semi-amplitude of 2948.14{sup +16.65}{sub -16.55} m s{sup -1}. Using additional high-resolution spectroscopy, we find the host star has an effective temperature T{sub eff} = 6004 {+-} 34 K, a surface gravity log g (cgs) =4.55 {+-} 0.17, and a metallicity [Fe/H] =+0.04 {+-} 0.06. The stellar mass and radius determined through the empirical relationship of Torres et al. yields 1.10 {+-} 0.09 M{sub Sun} and 0.92 {+-} 0.19 R{sub Sun }. The minimum mass of MARVELS-5b is 65.0 {+-} 2.9M{sub Jup}, indicating that it is likely to be either a BD or a very low mass star, thus occupying a relatively sparsely populated region of the mass function of companions to solar-type stars. The distance to this system is 101 {+-} 10 pc from the astrometric measurements of Hipparcos. No stellar tertiary is detected in the high-contrast images taken by either FastCam lucky imaging or Keck adaptive optics imaging, ruling out any star with mass greater than 0.2 M{sub Sun} at a separation larger than 40 AU.

  1. THE IMPACT OF TYPE Ia SUPERNOVA EXPLOSIONS ON HELIUM COMPANIONS IN THE CHANDRASEKHAR-MASS EXPLOSION SCENARIO

    SciTech Connect (OSTI)

    Liu Zhengwei; Wang, B.; Han, Z. W. [Yunnan Observatories, Chinese Academy of Sciences, Kunming 650011 (China); Pakmor, R. [Heidelberger Institut fuer Theoretische Studien, Schloss-Wolfsbrunnenweg 35, D-69118 Heidelberg (Germany); Seitenzahl, I. R.; Hillebrandt, W.; Kromer, M.; Edelmann, P.; Taubenberger, S. [Max-Planck-Institut fuer Astrophysik, Karl-Schwarzschild-Str. 1, D-85741 Garching (Germany); Roepke, F. K. [Institut fuer Theoretische Physik und Astrophysik, Universitaet Wuerzburg, Am Hubland, D-97074 Wuerzburg (Germany); Maeda, K., E-mail: zwliu@ynao.ac.cn [Kavli Institute for the Physics and Mathematics of the Universe (Kavli-IPMU), Todai Institutes for Advanced Study (TODIAS), University of Tokyo, 5-1-5 Kashiwanoha, Kashiwa, Chiba 277-8583 (Japan)

    2013-09-01T23:59:59.000Z

    In the version of the single-degenerate scenario of Type Ia supernovae (SNe Ia) studied here, a carbon-oxygen white dwarf explodes close to the Chandrasekhar limit after accreting material from a non-degenerate helium (He) companion star. In the present study, we employ the STELLAR GADGET code to perform three-dimensional hydrodynamical simulations of the interaction of the SN Ia ejecta with the He companion star taking into account its orbital motion and spin. It is found that only 2%-5% of the initial companion mass is stripped off from the outer layers of He companion stars due to the supernova (SN) impact. The dependence of the unbound mass (or the kick velocity) on the orbital separation can be fitted to a good approximation by a power law for a given companion model. After the SN impact, the outer layers of a He donor star are significantly enriched with heavy elements from the low-expansion-velocity tail of SN Ia ejecta. The total mass of accumulated SN-ejecta material on the companion surface reaches about {approx}> 10{sup -3} M{sub Sun} for different companion models. This enrichment with heavy elements provides a potential way to observationally identify the surviving companion star in SN remnants. Finally, by artificially adjusting the explosion energy of the W7 explosion model, we find that the total accumulation of SN ejecta on the companion surface is also dependent on the explosion energy with a power-law relation to a good approximation.

  2. A comparison of South Australia's driver licensing methods: competency-based training vs. practical examination

    E-Print Network [OSTI]

    examination Greg Roach a,*, M.A.P. Taylor b , Drew Dawson a a Centre for Sleep Research, University of South-mail address: greg.roach@unisa.edu.au (Greg Roach) 1369-8478/99/$ - see front matter Ã? 1999 Elsevier Science

  3. Very Low Mass Stellar and Substellar Companions to Solar-like Stars From MARVELS IV: A Candidate Brown Dwarf or Low-Mass Stellar Companion to HIP 67526

    E-Print Network [OSTI]

    Jiang, Peng; Cargile, Phillip; Crepp, Justin R; De Lee, Nathan; de Mello, Gustavo F Porto; Esposito, Massimiliano; Ferreira, Letícia D; Femenia, Bruno; Fleming, Scott W; Gaudi, B Scott; Ghezzi, Luan; Hernández, Jonay I González; Hebb, Leslie; Lee, Brian L; Ma, Bo; Stassun, Keivan G; Wang, Ji; Wisniewski, John P; Agol, Eric; Bizyaev, Dmitry; Brewington, Howard; Chang, Liang; da Costa, Luiz Nicolaci; Eastman, Jason D; Ebelke, Garrett; Gary, Bruce; Kane, Stephen R; Li, Rui; Liu, Jian; Mahadevan, Suvrath; Maia, Marcio A G; Malanushenko, Viktor; Malanushenko, Elena; Muna, Demitri; Nguyen, Duy Cuong; Ogando, Ricardo L C; Oravetz, Audrey; Oravetz, Daniel; Pan, Kaike; Pepper, Joshua; Paegert, Martin; Prieto, Carlos Allende; Rebolo, Rafael; Santiago, Basilio X; Schneider, Donald P; Bradley, Alaina C Shelden; Sivarani, Thirupathi; Snedden, Stephanie; van Eyken, J C; Wan, Xiaoke; Weaver, Benjamin A; Zhao, Bo

    2013-01-01T23:59:59.000Z

    We report the discovery of a candidate brown dwarf or a very low mass stellar companion (MARVELS-5b) to the star HIP 67526 from the Multi-object APO Radial Velocity Exoplanet Large-area Survey (MARVELS). The radial velocity curve for this object contains 31 epochs spread over 2.5 years. Our Keplerian fit using a Markov Chain Monte Carlo approach, reveals that the companion has an orbital period of $90.2695^{+0.0188}_{-0.0187}$ days, an eccentricity of $0.4375 \\pm 0.0040$ and a semi-amplitude of $2948.14^{+16.65}_{-16.55}$ m s$^{-1}$. Using additional high-resolution spectroscopy, we find the host star has an effective temperature $T_{\\rm{eff}}=6004 \\pm 34$ K, a surface gravity $\\log g$ [cgs] $=4.55 \\pm 0.17$ and a metallicity [Fe/H] $=+0.04 \\pm 0.06$. The stellar mass and radius determined through the empirical relationship of Torres et al. (2010), yields 1.10$\\pm$0.09 $M_{\\sun}$ and 0.92$\\pm$0.19 $R_{\\sun}$. The minimum mass of MARVELS-5b is $65.0 \\pm 2.9 M_{Jup}$, indicating that it is likely to be either a...

  4. Analyzing Vehicle Fuel Saving Opportunities through Intelligent Driver Feedback

    SciTech Connect (OSTI)

    Gonder, J.; Earleywine, M.; Sparks, W.

    2012-06-01T23:59:59.000Z

    Driving style changes, e.g., improving driver efficiency and motivating driver behavior changes, could deliver significant petroleum savings. This project examines eliminating stop-and-go driving and unnecessary idling, and also adjusting acceleration rates and cruising speeds to ideal levels to quantify fuel savings. Such extreme adjustments can result in dramatic fuel savings of over 30%, but would in reality only be achievable through automated control of vehicles and traffic flow. In real-world driving, efficient driving behaviors could reduce fuel use by 20% on aggressively driven cycles and by 5-10% on more moderately driven trips. A literature survey was conducted of driver behavior influences, and pertinent factors from on-road experiments with different driving styles were observed. This effort highlighted important driver influences such as surrounding vehicle behavior, anxiety over trying to get somewhere quickly, and the power/torque available from the vehicle. Existing feedback approaches often deliver efficiency information and instruction. Three recommendations for maximizing fuel savings from potential drive cycle improvement are: (1) leveraging applications with enhanced incentives, (2) using an approach that is easy and widely deployable to motivate drivers, and (3) utilizing connected vehicle and automation technologies to achieve large and widespread efficiency improvements.

  5. EC Driver - 41" Stroke Hydraulic Cylinder

    SciTech Connect (OSTI)

    Jaques, A.; /Fermilab

    1990-05-24T23:59:59.000Z

    It was decided to use a hydraulic cylinder resting on the floor of the argon spill trough in the EC carriage to drive the EC's motion on the center beam. Space was limited due to the spill bellows and their required support and containment system. The 0.0. of the cylinder had to be limited to 3 to 3-1/2 inches, maximum. The weight of a wet EC and carriage is estimated to be 320 tons. The rolling coefficient of friction of the Tychoway rollers chosen to guide the EC and carriage along the hardened centerbeam ways is claimed to be less than 0.0025. The driver will also need to overcome the forces produced by moving (rotating) the numerous bayonets located at the top of the cryostats in the many piping systems. These forces were conservatively estimated at 1000 lbs. The drive force required to overcome these forces was then calculated to be: 320(2,000) x 0.0025 + 1,000 = 2.600 lbs. (min. required). Due to the uncertainty in the actual roller coefficient of friction and the various unknowns in estimating the resistive forces contained in the piping and cabling systems attached to the cryostat, a conservative design factor of 5 was chosen. This should account for any uncertainty in our estimation of the minimum required drive force and also leaves us with a reserve to fall back on in case any unforeseen problems might arise. Thus the desired capacity of the driver was set at: (2,600) x 5 = 13,000 lbs. (design capacity). Assuming a 3 inch O.D. cylinder with a 1/2 inch wall (2 inch bore), we first analyzed a 1-3/8 inch diameter piston rod. Using Shigley & Mischke's 'Mechanical Engineering Design' (5th Ed.) and it's formulas for long columns with central loading, it was determined that a 1-3/8 inch diameter rod would not suffice, given our safety factor of 2. Increasing the piston rod diameter to 1-1/2 inches proved to be sufficient. The maximum allowable load came out to be approximately 17,000 lbs., which is greater than the 13,000 lbs. design capacity. With a 1-1/2 inch rod, a 2 inch bore and 10,000 psi capacity, the maximum return (retraction) force is: ({pi}/4)(2{sup 2}-1.52) x (10,000) = 13,744 lbs. (return force). This meets the desired design capacity of the cylinder. On the extension of the cylinder, the pressure will be limited such to produce only the 13,000 lb. design capacity. Through the use of a regulator on the cylinder extension inlet, the pressure will be limited to: 13,000/[({pi}/4)(2){sup 2}] {approx_equal} 4,200 psi. (regulator setting) and 4,200 x ({pi}/4)(2){sup 2} = 13,195 lbs. (thrust force). Another reference used by some Fermi engineers in designing hydraulic cylinders is the 'Design Engineers Handbook', Bulletin 0224-B1 published by the Parker-Hannifin Corporation. The piston rod-stroke selection table on page b-5 is used to determine the stroke factor. Our setup most approximates Case II of the table which gives a stroke factor of 0.70. Multiplying this by the actual stroke (41-inch) gives us a basic length of 28.7-inch. Using the piston rodstroke selection graph on page b-6, the 1-1/2 inch rod and 28.7-inch basic length indicate an allowable thrust of approximately 13,000 lbs. According to the Chief Application Engineer at the Parker-Hannifin regional sales office in Des Plaines, IL, a min imum safety factor of 4 can be assumed in the piston rod-stroke selection graph, possibly even higher. This would be at least twice as high as our initial safety factor of 2. Thus we feel our cylinder design falls well within the acceptable region of this reference.

  6. Workforce Training Case Study Workforce Training for the Electric...

    Office of Environmental Management (EM)

    Workforce Training Case Study Workforce Training for the Electric Power Sector: Transforming the Nation's Electric Grid by Training Skilled Workers The deployment of a smart...

  7. Behavior of trace and companion elements of ULC-IF steel grades during RH-treatment

    SciTech Connect (OSTI)

    Jungreithmeier, A.; Viertauer, A.; Presslinger, H. [Voest-Alpine Stahl Linz GmbH (Austria)

    1996-12-31T23:59:59.000Z

    A large number of metallurgical reactions are caused by lowering the partial pressure during vacuum treatment. One of these reactions is the volatilization of elements with high vapor pressure. The concentration of trace and companion elements during RH-treatment mostly changes because of cooling scrap, deoxidation agents and ferro-alloy additions, slag/metal reactions, vaporization and also because of reactions with the RH-vessel lining. These changes in the concentration of trace and companion elements during RH-treatment are exemplified for ULC-IF (ultra low carbon--interstitial free) steel grades. The elements which are considered are chromium, nickel, molybdenum, copper, vanadium, tin, zinc, lead, phosphorus, sulfur and nitrogen. Calculations of the theoretical equilibrium solubility using thermodynamic data--in dependence of pressure and temperature--correspond well with the values obtained during steel production operations. 67 refs.

  8. A review of "A Companion to Juan Luis Vives" by Charles Fantazzi

    E-Print Network [OSTI]

    Wright, Elizabeth R.

    2010-01-01T23:59:59.000Z

    Armas Wilson, and Isabel Lozano Renieblas when seeking to understand The Labors of Persiles and Sigismunda. Charles Fantazzi. A Companion to Juan Luis Vives. Leiden and Boston: Brill, 2008. viii + 430 pp. $185.00. Review by elizabeth r. wright..., university of georgia. This volume offers detailed analysis and rigorous contextual- ization of the diverse writings of Juan Luis Vives (Valencia, Spain 1492/93?Bruges, Belgium, 1540). In the course of some sixty differ- ent publications, this Valencian...

  9. A 3D Search for Companions to 12 Nearby M-Dwarfs

    E-Print Network [OSTI]

    Davison, Cassy L; Henry, Todd J; Riedel, Adric R; Jao, Wei-Chun; Bailey, John I; Quinn, Samuel N; Cantrell, Justin R; Subasavage, John P; Winters, Jen G

    2015-01-01T23:59:59.000Z

    We present a carefully vetted equatorial ($\\pm$ 30$^\\circ$ Decl.) sample of all known single (within 4'') mid M-dwarfs (M2.5V-M8.0V) extending out to 10 pc; their proximity and low masses make them ideal targets for planet searches. For this sample of 58 stars, we provide V$_J$, R$_{KC}$, I$_{KC}$ photometry, new low dispersion optical ($6000 - 9000$\\AA) spectra from which uniform spectral types are determined, multi-epoch H$\\alpha$ equivalent widths, and gravity sensitive $Na\\,I$ indices. For 12 of these 58 stars, strict limits are placed on the presence of stellar and sub-stellar companions, based on a pioneering program described here that utilizes precise infrared radial velocities and optical astrometric measurements in an effort to search for Jupiter-mass, brown dwarf and stellar-mass companions. Our infrared radial velocity precision using CSHELL at NASA's IRTF is $\\sim$90 m s$^{-1}$ over timescales from 13 days to 5 years. With our spectroscopic results the mean companion masses that we rule out of ex...

  10. Possible Signatures of Ejecta-Companion Interaction in iPTF 13bvn

    E-Print Network [OSTI]

    Hirai, Ryosuke

    2015-01-01T23:59:59.000Z

    We investigate the possible effects of the supernova ejecta hitting the companion star in iPTF 13bvn, focusing on the observable features when it becomes visible. iPTF 13bvn is a type Ib supernova that may become the first case that its progenitor is identified as a binary by near future observations. According to calculations by Bersten et al. (2014), the progenitor should have a mass $\\approx3.5M_\\odot$ to reproduce the supernova light curve, and such compact stars could only be produced via binary evolution. This is one of the reasons that we expect the progenitor to be a binary, but it should be confirmed by observing the remaining companion after the supernova. Their evolutionary calculations suggest that the companion star will be an overluminous OB star at the moment of supernova. With a combination of hydrodynamical and evolutionary simulations, we find that the secondary star will be heated by the supernova ejecta and expand to have larger luminosities and lower surface effective temperatures. The st...

  11. Periodic Flux Variability of Stars due to the Reflex Doppler Effect Induced by Planetary Companions

    E-Print Network [OSTI]

    Abraham Loeb; B. Scott Gaudi

    2003-03-28T23:59:59.000Z

    Upcoming space-based photometric satellites offer the possibility of detecting continuum flux variability at the micro-magnitude level. We show that the Doppler flux variability induced by the reflex motion of stars due to planetary companions has an amplitude of (3-alpha)K/c, where K is the reflex radial velocity amplitude and alpha is the logarithmic slope of source spectral flux in the observed frequency band. For many of the known close-in planetary systems with periods less than ~0.2 years, the periodic Doppler variability is of order a micromagnitude, and is significant relative to the variability caused by reflected light from the planetary companion. For companions with periods greater than ~0.2 years, the Doppler signal is larger than the reflected light signal. We show that the future photometric satellites should reach the sensitivity to detect this Doppler variability. In particular, the Kepler satellite should have the photon-noise sensitivity to detect at a signal-to-noise ratio > 5, all planets with minimum mass greater than 5 Jupiter masses, and periods less than 0.1 years around the 10,000 main-sequence stars with spectral types A through K and apparent magnitude V<12 in its field-of-view.

  12. HST/COS Detection of the Spectrum of the Subdwarf Companion of KOI-81

    E-Print Network [OSTI]

    Matson, Rachel A; Guo, Zhao; Quinn, Samuel N; Buchhave, Lars A; Latham, David W; Howell, Steve B; Rowe, Jason F

    2015-01-01T23:59:59.000Z

    KOI-81 is a totally eclipsing binary discovered by the Kepler mission that consists of a rapidly rotating B-type star and a small, hot companion. The system was forged through large scale mass transfer that stripped the mass donor of its envelope and spun up the mass gainer star. We present an analysis of UV spectra of KOI-81 that were obtained with the Cosmic Origins Spectrograph on the Hubble Space Telescope that reveal for the first time the spectral features of the faint, hot companion. We present a double-lined spectroscopic orbit for the system that yields mass estimates of 2.92 M_sun and 0.19 M_sun for the B-star and hot subdwarf, respectively. We used a Doppler tomography algorithm to reconstruct the UV spectra of the components, and a comparison of the reconstructed and model spectra yields effective temperatures of 12 kK and 19 - 27 kK for the B-star and hot companion, respectively. The B-star is pulsating, and we identified a number of peaks in the Fourier transform of the light curve, including on...

  13. Piecewise training for structured prediction

    E-Print Network [OSTI]

    Sutton, Charles; McCallum, Andrew

    2009-01-01T23:59:59.000Z

    K. (2006). Accelerated training of conditional random ?eldsmethods for discriminative training of dependency parsers (Sutton, C. (2008). Ef?cient training methods for conditional

  14. NCSU Human Resources Training & Organizational

    E-Print Network [OSTI]

    2011 NCSU Human Resources Training & Organizational Development Spring & Summer 2011 Learning to Training & Organizational Development's new eLearning Training Catalog. This catalog serves as a central

  15. Plans for a proton driver at Fermilab

    SciTech Connect (OSTI)

    Kephart, R.D.; /Fermilab

    2005-01-01T23:59:59.000Z

    During the last several years, stunning experimental results have established that neutrinos have nonzero masses and substantial mixing. The Standard Model must be extended to accommodate neutrino mass terms. The observation that neutrino masses and mass splittings are all many orders of magnitude smaller than those of any of the other fundamental fermions suggests radically new physics, perhaps originating at the GUT or Planck Scale, or perhaps the existence of new spatial dimensions. In some sense we know that the Standard Model is broken, but we don't know how it is broken. Whatever the origin of the observed neutrino masses and mixing, it is likely to require a profound extension to our picture of the physical world. The first steps in understanding this revolutionary new physics are to pin down the measurable parameters and to address the next round of basic questions: (1) Are there only three neutrino flavors, or do light, sterile neutrinos exist? (2) If there are only three generations, there is one angle ({theta}{sub 13}) in the mixing matrix that is unmeasured. How large is it? (3) Which of the two possible orderings of the neutrino mass eigenstates applies? (4) If {theta}{sub 13} is large enough one it may be possible to measure the quantum-mechanical phase {delta}. If {theta}{sub 13} and {delta} are non-zero there will be CP violation in the lepton sector. These questions can be addressed by accelerator based neutrino oscillation experiments. The answers will guide our understanding of what lies beyond the Standard Model, and whether the new physics provides an explanation for the baryon asymmetry of the Universe (via leptogenesis), or provides deep insight into the connection between quark and lepton properties (via Grand Unified Theories), or perhaps leads to an understanding of one of the most profound questions in physics: Why are there three generations of quarks and leptons? The answers may well further challenge our picture of the physical world, and will certainly have important implications for our understanding of cosmology and the evolution of the early Universe. The current Fermilab Program is an important part of the world-wide accelerator based effort to explore and understand the physics of neutrino oscillations. By early 2005, with both MINOS and MiniBooNE taking data, Fermilab will be able to answer some of the most pressing first-round questions raised by the discovery that neutrinos have mass. Fermilab's high-intensity neutrino beams are derived from 8- and 120-GeV proton beams. MiniBooNE is currently taking data using 8 GeV Protons from the Booster. The 120 GeV NuMI beam will start to operate in early 2005 using a 0.25 MW proton beam power from the Main Injector. Future neutrino programs will build on these existing facilities. New short and long baseline experiments have been proposed. There are proposals to increase the available number of protons at 8 and 120 GeV with the goal of addressing the full range of questions presented by neutrino oscillations. Key to that vision is a new intense proton source that usually is referred to as the Proton Driver.

  16. BEAM SIMULATIONS USING VIRTUAL DIAGNOSTICS FOR THE DRIVER LINAC

    SciTech Connect (OSTI)

    R. C. York; X. Wu; Q. Zhao

    2011-12-21T23:59:59.000Z

    End-to-end beam simulations for the driver linac have shown that the design meets the necessary performance requirements including having adequate transverse and longitudinal acceptances. However, to achieve reliable operational performance, the development of appropriate beam diagnostic systems and control room procedures are crucial. With limited R&D funding, beam simulations provide a cost effective tool to evaluate candidate beam diagnostic systems and to provide a critical basis for developing early commissioning and later operational activities. We propose to perform beam dynamic studies and engineering analyses to define the requisite diagnostic systems of the driver linac and through simulation to develop and test commissioning and operational procedures.

  17. Athletic Training Education Program Bachelor of Science in Athletic Training

    E-Print Network [OSTI]

    Saldin, Dilano

    Athletic Training Education Program Bachelor of Science in Athletic Training Department of Kinesiology Athletic training is a health care profession practiced by athletic trainers who collaborate with physicians to optimize activity and participation of patients and clients. Athletic training includes

  18. Training System (CHRIS) | Department of Energy

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

    Training System (CHRIS) Training System (CHRIS) CHRIS Training is the computer system that Federal employees use to request training and view their training histories. Managers use...

  19. Assessments A Training Manual

    E-Print Network [OSTI]

    Modern Industrial Assessments A Training Manual Version 2.0 Sponsored by: Produced by: Dr. Michael. Modern Industrial Assessments: A Training Manual, grew from the desires of the United States Department conservation and waste minimization / pollution prevention training courses and information agencies sponsored

  20. CAPITAL ASSET DOCUMENT TRAINING

    E-Print Network [OSTI]

    KUALI CAPITAL ASSET MANAGEMENT DOCUMENT TRAINING Business and Financial Services, Property Management Presented by: Rachel Drenth #12;Sign On to the Training Site · CSU CAP (Campus Administration://padroni.is.colostate.edu:7778/portal/page/portal/CAPQA (THEN CHOOSE QUAL 2) · Non-production Applications: Training Kuali

  1. TRAINING FOR INFORMATION

    E-Print Network [OSTI]

    June 1998 TRAINING FOR INFORMATION TECHNOLOGY SECURITY: EVALUATING THE EFFECTIVENESS OF RESULTS-BASED LEARNING The basic principles of results-based training for information technology (IT) security were discussed in our April 1998 bulletin, Training Require- ments for Information Technology Security

  2. Foal imprint training

    E-Print Network [OSTI]

    Williams, Jennifer Lee

    2001-01-01T23:59:59.000Z

    "Foal imprint training" is widely used in the horse industry. Because the training sessions occur during the period when a foal is "imprinting on its dam", it is assumed the foal will be easier to handle and train later in life. There have been...

  3. Hazardous Waste Management Training

    E-Print Network [OSTI]

    Dai, Pengcheng

    records. The initial training of Hazardous Waste Management and Waste Minimization is done in a classHazardous Waste Management Training Persons (including faculty, staff and students) working before handling hazardous waste. Departments are re- quired to keep records of training for as long

  4. Federal Employee Training

    Broader source: Directives, Delegations, and Requirements [Office of Management (MA)]

    2001-10-11T23:59:59.000Z

    To plan and establish requirements and assign responsibilities for Department of Energy (DOE) Federal employee training, education, and development (hereafter referred to as "training") under the Government Employees Training Act of 1958. Cancels DOE O 360.1A. Canceled by DOE O 360.1C.

  5. Comparative Oncogenomic Analysis of Copy Number Alterations in Human and Zebrafish Tumors Enables Cancer Driver Discovery

    E-Print Network [OSTI]

    Zhang, GuangJun

    The identification of cancer drivers is a major goal of current cancer research. Finding driver genes within large chromosomal events is especially challenging because such alterations encompass many genes. Previously, we ...

  6. Driver mental workload requirements on horizontal curves based on occluded vision test measurements

    E-Print Network [OSTI]

    Shafer, Mark Anthony

    1994-01-01T23:59:59.000Z

    This thesis documents an evaluation of driver mental workload requirements on horizontal curves based on occluded vision test measurements. Driver workload is an important concept in the design of highway systems. A successful highway design...

  7. Assessment of older driver understanding of certain traffic control devices in Texas

    E-Print Network [OSTI]

    Hulett, Stephanie Renee

    2000-01-01T23:59:59.000Z

    The purpose of this research was to assess older Texas drivers on their understanding of nine traffic control devices and identify the devices that are misunderstood by people 65 years and older. Additionally, older driver education programs were...

  8. Evaluation of driver braking performance to an unexpected object in the roadway 

    E-Print Network [OSTI]

    Picha, Dale Louis

    1994-01-01T23:59:59.000Z

    components, specifically whether the equation accurately reflects driver and vehicle behaviors during a braking maneuver. This research evaluated the two components of the SSD equation. Four field studies were conducted that evaluated driver braking...

  9. Final Report on the Fuel Saving Effectiveness of Various Driver Feedback Approaches

    SciTech Connect (OSTI)

    Gonder, J.; Earleywine, M.; Sparks, W.

    2011-03-01T23:59:59.000Z

    This final report quantifies the fuel-savings opportunities from specific driving behavior changes, identifies factors that influence drivers' receptiveness to adopting fuel-saving behaviors, and assesses various driver feedback approaches.

  10. Evaluation of driver braking performance to an unexpected object in the roadway

    E-Print Network [OSTI]

    Picha, Dale Louis

    1994-01-01T23:59:59.000Z

    components, specifically whether the equation accurately reflects driver and vehicle behaviors during a braking maneuver. This research evaluated the two components of the SSD equation. Four field studies were conducted that evaluated driver braking...

  11. Abramovo Counterterrorism Training Center

    SciTech Connect (OSTI)

    Hayes, Christopher M [ORNL; Ross, Larry [U.S. Department of Energy; Lingenfelter, Forrest E [ORNL; Sokolnikov, Pavel I [ORNL; Kaldenbach, Karen Yvonne [ORNL; Estigneev, Yuri [Eleron; Murievav, Andrey [Eleron

    2011-01-01T23:59:59.000Z

    The U.S. government has been assisting the Russian Federation (RF) Ministry of Defense (MOD) for many years with nuclear weapons transportation security (NWTS) through the provision of specialized guard escort railcars and cargo railcars with integrated physical security and communication systems, armored transport vehicles, and armored escort vehicles. As a natural continuation of the NWTS program, a partnership has been formed to construct a training center that will provide counterterrorism training to personnel in all branches of the RF MOD. The Abramovo Counterterrorism Training Center (ACTC) is a multinational, multiagency project with funding from Canada, RF and the U.S. Departments of Defense and Energy. ACTC will be a facility where MOD personnel can conduct basic through advanced training in various security measures to protect Category IA material against the threat of terrorist attack. The training will enhance defense-in-depth principles by integrating MOD guard force personnel into the overall physical protection systems and improving their overall response time and neutralization capabilities. The ACTC project includes infrastructure improvements, renovation of existing buildings, construction of new buildings, construction of new training facilities, and provision of training and other equipment. Classroom training will be conducted in a renovated training building. Basic and intermediate training will be conducted on three different security training areas where various obstacles and static training devices will be constructed. The central element of ACTC, where advanced training will be held, is the 'autodrome,' a 3 km road along which various terrorist events can be staged to challenge MOD personnel in realistic and dynamic nuclear weapons transportation scenarios. This paper will address the ACTC project elements and the vision for training development and integrating this training into actual nuclear weapons transportation operations.

  12. Termites, elephants and fire are key drivers of tree mortality

    E-Print Network [OSTI]

    mortality: 2 dominated by elephant damage, 2 by termite attack and 1 by fire. Wind and human activity wereTermites, elephants and fire are key drivers of tree mortality 5 plots suffered substantial tree not major causes of tree mortality. Sample sizes are too small to reasonably determine the most significant

  13. Next Story > SC DMV lifting drivers' suspensions this week

    E-Print Network [OSTI]

    Duchowski, Andrew T.

    The State Next Story > SC DMV lifting drivers' suspensions this week Researcher: Zombie fads peak COLUMBIA, S.C. -- Zombies seem to be everywhere these days. In the popular TV series "The Walking Dead at the University of California at Davis. Lauro said she keeps track of zombie movies, TV shows and video games

  14. Energy for 500 million Homes: Drivers and Outlook for

    E-Print Network [OSTI]

    -up analysis of residential building energy consumption in China using data from a wide variety of sourcesLBNL-2417E Energy for 500 million Homes: Drivers and Outlook for Residential Energy Consumption and Outlook for Residential Energy Consumption in China Nan Zhou*, Michael A. McNeil, Mark Levine Keywords

  15. Project: Driver and controller for a thermoelectric cooler

    E-Print Network [OSTI]

    Project: Driver and controller for a thermoelectric cooler Supervisor: Prof. Sam Ben-Yaakov Year solutions. Based on one of the three thermoelectric phenomena ­ the Peltier effect ­ bi-directional control is achieved. The TEC (which is a Thermoelectric Cooler) uses this effect. The direction of the current through

  16. Integrating Concurrency Control and Energy Management in Device Drivers

    E-Print Network [OSTI]

    Levis, Philip

    Integrating Concurrency Control and Energy Management in Device Drivers Kevin Klues , Vlado@cs.berkeley.edu dgay@intel-research.net Abstract Energy management is a critical concern in wireless sensornets. De- spite its importance, sensor network operating systems today pro- vide minimal energy management support

  17. Improved gauge driver for the generalized harmonic Einstein system Lee Lindblom and Bela Szilagyi

    E-Print Network [OSTI]

    Lindblom, Lee

    Improved gauge driver for the generalized harmonic Einstein system Lee Lindblom and Be´la Szila´gyi

  18. Radiological worker training

    SciTech Connect (OSTI)

    NONE

    1998-10-01T23:59:59.000Z

    This Handbook describes an implementation process for core training as recommended in Implementation Guide G441.12, Radiation Safety Training, and as outlined in the DOE Radiological Control Standard (RCS). The Handbook is meant to assist those individuals within the Department of Energy, Managing and Operating contractors, and Managing and Integrating contractors identified as having responsibility for implementing core training recommended by the RCS. This training is intended for radiological workers to assist in meeting their job-specific training requirements of 10 CFR 835. While this Handbook addresses many requirements of 10 CFR 835 Subpart J, it must be supplemented with facility-specific information to achieve full compliance.

  19. T-1 Training Area

    SciTech Connect (OSTI)

    None

    2014-11-07T23:59:59.000Z

    Another valuable homeland security asset at the NNSS is the T-1 training area, which covers more than 10 acres and includes more than 20 separate training venues. Local, County, and State first responders who train here encounter a variety of realistic disaster scenarios. A crashed 737 airliner lying in pieces across the desert, a helicopter and other small aircraft, trucks, buses, and derailed train cars are all part of the mock incident scene. After formal classroom education, first responders are trained to take immediate decisive action to prevent or mitigate the use of radiological or nuclear devices by terrorists. The Counterterrorism Operations Support Center for Radiological Nuclear Training conducts the courses and exercises providing first responders from across the nation with the tools they need to protect their communities. All of these elements provide a training experience that cannot be duplicated anywhere else in the country.

  20. T-1 Training Area

    ScienceCinema (OSTI)

    None

    2015-01-09T23:59:59.000Z

    Another valuable homeland security asset at the NNSS is the T-1 training area, which covers more than 10 acres and includes more than 20 separate training venues. Local, County, and State first responders who train here encounter a variety of realistic disaster scenarios. A crashed 737 airliner lying in pieces across the desert, a helicopter and other small aircraft, trucks, buses, and derailed train cars are all part of the mock incident scene. After formal classroom education, first responders are trained to take immediate decisive action to prevent or mitigate the use of radiological or nuclear devices by terrorists. The Counterterrorism Operations Support Center for Radiological Nuclear Training conducts the courses and exercises providing first responders from across the nation with the tools they need to protect their communities. All of these elements provide a training experience that cannot be duplicated anywhere else in the country.

  1. A method for calibration of bone driver transducers to measure the mastoid impedance Reggie Weecea

    E-Print Network [OSTI]

    Allen, Jont

    bone vibrator transducers for clinical measurements, the transfer of energy from the bone driver by known masses. This absolute calibration is based upon a circuit model of the driver, describing specialized equipment not available in the clinic, and a refined bone driver circuit model is proposed

  2. Research Paper A method for calibration of bone driver transducers to measure the mastoid

    E-Print Network [OSTI]

    Allen, Jont

    vibrator transducers for clinical measurements, the transfer of energy from the bone driver depends. This absolute calibration is based upon a circuit model of the driver, describing it with three frequency in the clinic, and a refined bone driver circuit model is proposed to better capture the observed behaviors. Ã?

  3. Testing Closed-Source Binary Device Drivers with DDT Volodymyr Kuznetsov, Vitaly Chipounov, and George Candea

    E-Print Network [OSTI]

    Candea, George

    Testing Closed-Source Binary Device Drivers with DDT Volodymyr Kuznetsov, Vitaly Chipounov (EPFL), Switzerland Abstract DDT is a system for testing closed-source binary de- vice drivers against think of it as a pesticide against device driver bugs. DDT combines virtualization with a spe- cialized

  4. Journal of Transportation Engineering Modelling Automobile Driver's Toll-Lane Choice Behaviour at a Toll Plaza

    E-Print Network [OSTI]

    Kundu, Debasis

    Journal of Transportation Engineering Modelling Automobile Driver's Toll-Lane Choice Behaviour at a Toll Plaza --Manuscript Draft-- Manuscript Number: TEENG-1181R3 Full Title: Modelling Automobile Driver to develop a random utility based discrete multinomial choice model for the behaviour of automobile drivers

  5. Energy Efficiency Services Sector: Workforce Education and Training Needs

    SciTech Connect (OSTI)

    Goldman, Charles A.; Peters, Jane S.; Albers, Nathaniel; Stuart, Elizabeth; Fuller, Merrian C.

    2010-03-19T23:59:59.000Z

    This report provides a baseline assessment of the current state of energy efficiency-related education and training programs and analyzes training and education needs to support expected growth in the energy efficiency services workforce. In the last year, there has been a significant increase in funding for 'green job' training and workforce development (including energy efficiency), through the American Recovery and Reinvestment Act (ARRA). Key segments of the energy efficiency services sector (EESS) have experienced significant growth during the past several years, and this growth is projected to continue and accelerate over the next decade. In a companion study (Goldman et al. 2009), our research team estimated that the EESS will increase two- to four-fold by 2020, to 220,000 person-years of employment (PYE) (low-growth scenario) or up to 380,000 PYE (high-growth scenario), which may represent as many as 1.3 million individuals. In assessing energy efficiency workforce education and training needs, we focus on energy-efficiency services-related jobs that are required to improve the efficiency of residential and nonresidential buildings. Figure ES-1 shows the market value chain for the EESS, sub-sectors included in this study, as well as the types of market players and specific occupations. Our assessment does not include the manufacturing, wholesale, and retail distribution subsectors, or energy efficiency-focused operations and maintenance performed by facility managers.

  6. A COMPANION AS THE CAUSE OF LATITUDE-DEPENDENT EFFECTS IN THE WIND OF ETA CARINAE

    SciTech Connect (OSTI)

    Groh, J. H. [Geneva Observatory, Geneva University, Chemin des Maillettes 51, CH-1290 Sauverny (Switzerland); Madura, T. I.; Weigelt, G. [Max-Planck-Institut fuer Radioastronomie, Auf dem Huegel 69, D-53121 Bonn (Germany); Hillier, D. J. [Department of Physics and Astronomy, University of Pittsburgh, 3941 O'Hara Street, Pittsburgh, PA 15260 (United States); Kruip, C. J. H., E-mail: jose.groh@unige.ch [Leiden Observatory, Leiden University, Postbus 9513, NL-2300 RA Leiden (Netherlands)

    2012-11-01T23:59:59.000Z

    We analyze spatially resolved spectroscopic observations of the Eta Carinae binary system obtained with the Hubble Space Telescope/STIS. Eta Car is enshrouded by the dusty Homunculus nebula, which scatters light emitted by the central binary and provides a unique opportunity to study a massive binary system from different vantage points. We investigate the latitudinal and azimuthal dependence of H{alpha} line profiles caused by the presence of a wind-wind collision (WWC) cavity created by the companion star. Using two-dimensional radiative transfer models, we find that the wind cavity can qualitatively explain the observed line profiles around apastron. Regions of the Homunculus which scatter light that propagated through the WWC cavity show weaker or no H{alpha} absorption. Regions scattering light that propagated through a significant portion of the primary wind show stronger P Cygni absorption. Our models overestimate the H{alpha} absorption formed in the primary wind, which we attribute to photoionization by the companion, not presently included in the models. We can qualitatively explain the latitudinal changes that occur during periastron, shedding light on the nature of Eta Car's spectroscopic events. Our models support the idea that during the brief period of time around periastron when the primary wind flows unimpeded toward the observer, H{alpha} absorption occurs in directions toward the central object and Homunculus SE pole, but not toward equatorial regions close to the Weigelt blobs. We suggest that observed latitudinal and azimuthal variations are dominated by the companion star via the WWC cavity, rather than by rapid rotation of the primary star.

  7. Direct Detection of the Close Companion of Polaris with the Hubble Space Telescope

    E-Print Network [OSTI]

    Nancy Remage Evans; Gail H. Schaefer; Howard E. Bond; Giuseppe Bono; Margarita Karovska; Edmund Nelan; Dimitar Sasselov; Brian D. Mason

    2008-06-30T23:59:59.000Z

    Polaris, the nearest and brightest classical Cepheid, is a single-lined spectroscopic binary with an orbital period of 30 years. Using the High Resolution Channel of the Advanced Camera for Surveys onboard the Hubble Space Telescope (HST) at a wavelength of ~2255\\AA, we have directly detected the faint companion at a separation of 0\\farcs17. A second HST observation 1.04 yr later confirms orbital motion in a retrograde direction. By combining our two measures with the spectroscopic orbit of Kamper and an analysis of the Hipparcos and FK5 proper motions by Wielen et al., we find a mass for Polaris Aa of 4.5^{+2.2}_{-1.4} M_\\odot--the first purely dynamical mass determined for any Cepheid. For the faint companion Polaris Ab we find a dynamical mass of 1.26^{+0.14}_{-0.07} M_\\odot, consistent with an inferred spectral type of F6 V and with the flux difference of 5.4 mag observed at 2255\\AA. The magnitude difference at the V band is estimated to be 7.2 mag. Continued HST observations will significantly reduce the mass errors, which are presently still too large to provide critical constraints on the roles of convective overshoot, mass loss, rotation, and opacities in the evolution of intermediate-mass stars. Our astrometry, combined with two centuries of archival measurements, also confirms that the well-known, more distant (18") visual companion, Polaris B, has a nearly common proper motion with that of the Aa,Ab pair. This is consistent with orbital motion in a long-period bound system. The ultraviolet brightness of Polaris B is in accordance with its known F3 V spectral type if it has the same distance as Polaris Aa,Ab.

  8. VERY LOW MASS STELLAR AND SUBSTELLAR COMPANIONS TO SOLAR-LIKE STARS FROM MARVELS. II. A SHORT-PERIOD COMPANION ORBITING AN F STAR WITH EVIDENCE OF A STELLAR TERTIARY AND SIGNIFICANT MUTUAL INCLINATION

    SciTech Connect (OSTI)

    Fleming, Scott W.; Ge Jian; De Lee, Nathan; Jiang Peng; Lee, Brian; Nelson, Ben [Department of Astronomy, University of Florida, 211 Bryant Space Science Center, Gainesville, FL 2611-2055 (United States); Barnes, Rory [Department of Astronomy, University of Washington, P.O. Box 351580, Seattle, WA 98195 (United States); Beatty, Thomas G.; Gaudi, B. Scott; Shappee, Benjamin J. [Department of Astronomy, Ohio State University, 140 West 18th Avenue, Columbus, OH 43210 (United States); Crepp, Justin R. [Department of Astronomy, California Institute of Technology, 1200 E. California Blvd., Pasadena, CA 91125 (United States); Esposito, Massimiliano; Femenia, Bruno; Gonzalez Hernandez, Jonay I. [Instituto de Astrofisica de Canarias (IAC), E-38205 La Laguna, Tenerife (Spain); Ferreira, Leticia; Porto de Mello, Gustavo F. [Observatorio do Valongo, Universidade Federal do Rio de Janeiro, Ladeira do Pedro Antonio, 43, CEP: 20080-090, Rio de Janeiro, RJ (Brazil); Gary, Bruce; Hebb, Leslie; Stassun, Keivan [Department of Physics and Astronomy, Vanderbilt University, Nashville, TN 37235 (United States); Ghezzi, Luan, E-mail: scfleming@psu.edu [Laboratorio Interinstitucional de e-Astronomia, LIneA, Rua Gal. Jose Cristino 77, Rio de Janeiro, RJ-20921-400 (Brazil); and others

    2012-09-15T23:59:59.000Z

    We report the discovery via radial velocity (RV) measurements of a short-period (P = 2.430420 {+-} 0.000006 days) companion to the F-type main-sequence star TYC 2930-00872-1. A long-term trend in the RV data also suggests the presence of a tertiary stellar companion with P > 2000 days. High-resolution spectroscopy of the host star yields T{sub eff} = 6427 {+-} 33 K, log g = 4.52 {+-} 0.14, and [Fe/H] = -0.04 {+-} 0.05. These parameters, combined with the broadband spectral energy distribution (SED) and a parallax, allow us to infer a mass and radius of the host star of M{sub 1} = 1.21 {+-} 0.08 M{sub Sun} and R{sub 1} = 1.09{sup +0.15}{sub -0.13} R{sub Sun }. The minimum mass of the inner companion is below the hydrogen-burning limit; however, the true mass is likely to be substantially higher. We are able to exclude transits of the inner companion with high confidence. Further, the host star spectrum exhibits a clear signature of Ca H and K core emission, indicating stellar activity, but a lack of photometric variability and small vsin I suggest that the primary's spin axis is oriented in a pole-on configuration. The rotational period of the primary estimated through an activity-rotation relation matches the orbital period of the inner companion to within 1.5 {sigma}, suggesting that the primary and inner companion are tidally locked. If the inner companion's orbital angular momentum vector is aligned with the stellar spin axis as expected through tidal evolution, then it has a stellar mass of {approx}0.3-0.4 M{sub Sun }. Direct imaging limits the existence of stellar companions to projected separations <30 AU. No set of spectral lines and no significant flux contribution to the SED from either companion are detected, which places individual upper mass limits of M{sub {l_brace}2,3{r_brace}} {approx}< 1.0 M{sub Sun }, provided they are not stellar remnants. If the tertiary is not a stellar remnant, then it likely has a mass of {approx}0.5-0.6 M{sub Sun }, and its orbit is likely significantly inclined from that of the secondary, suggesting that the Kozai-Lidov mechanism may have driven the dynamical evolution of this system.

  9. Know the Star, Know the Planet. III. Discovery of Late-Type Companions to Two Exoplanet Host Stars

    E-Print Network [OSTI]

    Roberts,, Lewis C; Mason, Brian D; Riddle, Reed L; Hartkopf, William I; Law, Nicholas M; Baranec, Christoph

    2015-01-01T23:59:59.000Z

    We discuss two multiple star systems that host known exoplanets: HD 2638 and 30 Ari B. Adaptive optics imagery revealed an additional stellar companion to both stars. We collected multi-epoch images of the systems with Robo-AO and the PALM-3000 adaptive optics systems at Palomar Observatory and provide relative photometry and astrometry. The astrometry indicates that the companions share common proper motion with their respective primaries. Both of the new companions have projected separations less than 30 AU from the exoplanet host star. Using the projected separations to compute orbital periods of the new stellar companions, HD 2638 has a period of 130 yrs and 30 Ari B has a period of 80 years. Previous studies have shown that the true period is most likely within a factor of three of these estimated values. The additional component to the 30 Ari makes it the second confirmed quadruple system known to host an exoplanet. HD 2638 hosts a hot Jupiter and the discovery of a new companion strengthens the connect...

  10. ORISE: Epidemiology Training

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

    Epidemiology Training Epidemiological studies can provide valuable insight into health trends for workers and the public at large. Once a study is complete, however, it must be...

  11. Training | Advanced Photon Source

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

    Argonne's receiving staff will refuse to accept the shipment: See the APS Safety and Training page for details on a variety of hazardous materials and special instructions from...

  12. ORISE: Training and Tools

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

    cancer afflict more people every year and have resulted in increased demand for trained health care providers and accessible health information. Because health care workers and...

  13. Training and Drills

    Broader source: Directives, Delegations, and Requirements [Office of Management (MA)]

    1997-08-21T23:59:59.000Z

    The volume offers a framework for effective management of emergency response training and drills. Canceled by DOE G 151.1-3.

  14. Radiation Safety Training Materials

    Broader source: Energy.gov [DOE]

    The following Handbooks and Standard provide recommended hazard specific training material for radiological workers at DOE facilities and for various activities.

  15. Training | Department of Energy

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

    Brush up on power purchase agreements (PPAs) by taking FEMP's newly revised eTraining course. Read more New course introduces best practices for establishing partnerships with...

  16. Ellipsoidal Oscillations Induced by Substellar Companions: A Prospect for the Kepler Mission

    E-Print Network [OSTI]

    Eric Pfahl; Phil Arras; Bill Paxton

    2007-04-15T23:59:59.000Z

    Hundreds of substellar companions to solar-type stars will be discovered with the Kepler satellite. Kepler's extreme photometric precision gives access to low-amplitude stellar variability contributed by a variety of physical processes. We discuss in detail the periodic flux modulations arising from the tidal force on the star due to a substellar companion. An analytic expression for the variability is derived in the equilibrium-tide approximation. We demonstrate analytically and through numerical solutions of the linear, nonadiabatic stellar oscillation equations that the equilibrium-tide formula works extremely well for stars of mass <1.4 Msun with thick surface convection zones. More massive stars with largely radiative envelopes do not conform to the equilibrium-tide approximation and can exhibit flux variations $\\ga$10 times larger than naive estimates. Over the full range of stellar masses considered, we treat the oscillatory response of the convection zone by adapting a prescription that A. J. Brickhill developed for pulsating white dwarfs. Compared to other sources of periodic variability, the ellipsoidal lightcurve has a distinct dependence on time and system parameters. We suggest that ellipsoidal oscillations induced by giant planets may be detectable from as many as ~100 of the 10^5 Kepler target stars. (Abridged)

  17. An astrometric companion to the nearby metal-poor, low-mass star LHS 1589

    E-Print Network [OSTI]

    Sebastien Lepine; R. Michael Rich; Michael M. Shara; Kelle L. Cruz; Andrew Skemer

    2007-07-20T23:59:59.000Z

    We report the discovery of a companion to the high proper motion star LHS 1589, a nearby high-velocity, low-mass subdwarf. The companion (LHS 1589B) is located 0.224+/-0.004" to the southwest of the primary (LHS 1589A), and is 0.5 magnitude fainter than the primary in the K_s band. The pair was resolved with the IRCAL infrared camera at Lick Observatory, operating with the Laser Guide Star Adaptive Optics system. A low-resolution spectrum of the unresolved pair obtained at the MDM observatory shows the source to be consistent with a cool subdwarf of spectral subtype sdK7.5. A photometric distance estimate places the metal-poor system at a distance d=81+/-18 parsecs from the Sun. We also measure a radial velocity V_rad=67+/-8 km/s which, together with the proper motion and estimated distance, suggests that the pair is roaming the inner Galactic halo on a highly eccentric orbit. With a projected orbital separation s=18.1+/-4.8 AU, and a crude estimate of the system's total mass, we estimate the orbital period of the system to be in the range 75 yr metal-poor, low-mass stars.

  18. On the nature of the tertiary companion to FW Tau: ALMA CO observations and SED modeling

    E-Print Network [OSTI]

    Caceres, Claudio; Schreiber, Matthias R; Canovas, Hector; Cieza, Lucas A; Williams, Jonathan P; Hales, Antonio; Pinte, Christophe; Menard, Francois; Wahhaj, Zahed

    2015-01-01T23:59:59.000Z

    It is thought that planetary mass companions may form through gravitational disk instabilities or core accretion. Identifying such objects in the process of formation would provide the most direct test for the competing formation theories. One of the most promising candidates for a planetary mass object still in formation is the third object in the FWTau system. We here present ALMA cycle 1 observations confirming the recently published 1.3 mm detection of a dust disk around this third object and present for the first time a clear detection of a single peak 12CO(2-1) line, providing direct evidence for the simultaneous existence of a gas disk. We perform radiative transfer modeling of the third object in FW Tau and find that current observations are consistent with a planetary mass object embedded in a disk which is externally irradiated by the binary companion and seen at an inclination of i<15 deg. However, we also find that a near edge-on disk around a more massive substellar object can explain the obse...

  19. Observable fractions of core-collapse supernova light curves brightened by binary companions

    E-Print Network [OSTI]

    Moriya, Takashi J; Izzard, Robert G

    2015-01-01T23:59:59.000Z

    Many core-collapse supernova progenitors are presumed to be in binary systems. If a star explodes in a binary system, the early supernova light curve can be brightened by the collision of the supernova ejecta with the companion star. The early brightening can be observed when the observer is in the direction of the hole created by the collision. Based on a population synthesis model, we estimate the fractions of core-collapse supernovae in which the light-curve brightening by the collision can be observed. We find that 0.19% of core-collapse supernova light curves can be observed with the collisional brightening. Type Ibc supernova light curves are more likely to be brightened by the collision (0.53%) because of the high fraction of the progenitors being in binary systems and their proximity to the companion stars. Type II and IIb supernova light curves are less affected (~1e-3% and ~1e-2%, respectively). Although the early, slow light-curve declines of some Type IIb and Ibc supernovae are argued to be caused...

  20. BGSU BLACKBOARD TRAINING TUTORIAL BGSU Blackboard Training 2

    E-Print Network [OSTI]

    Moore, Paul A.

    BGSU BLACKBOARD TRAINING TUTORIAL #12;BGSU Blackboard Training 2 T A B L E O F C O N T E N T S 1 BGSU Blackboard Training 3 #12;BGSU Blackboard Training 4 Adding An Item ­ Used to upload different Course BGSU Blackboard Training 5 #12;Once you are done adding your questions to the Test Canvas, click

  1. Low-jitter, hydrogen thyratron Pockels cell driver

    SciTech Connect (OSTI)

    Oicles, J.A.; Kitchin, H.D.

    1983-06-01T23:59:59.000Z

    The requirements to be met by Pockels cell drivers for incorporation into the Novette and Nova Laser systems are presented, and critical aspects of the specification examined. A high-performance pulse generator has been developed to meet these requirements using new thyratron technology from the English Electric Valve Co. Ltd. Two closely related versions have been built; a 10KV output unit with 9 nsec risetime into five parallel 50-ohm loads and a faster 5KV output driver with 3.5 nsec risetime into a single 50-ohm load. The design approach for optimizing performance, using the new tubes in relation to the LLNL specification is described, including the techniques used for control of electromagnetic interference.

  2. automobile driver examination: Topics by E-print Network

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

    training vs. practical examination Physics Websites Summary: examination Greg Roach a,*, M.A.P. Taylor b , Drew Dawson a a Centre for Sleep Research, University of...

  3. Stability analysis and testing of a train of centrifugal compressors for high pressure gas injection

    SciTech Connect (OSTI)

    Memmott, E.A. [Dresser-Rand Co., Olean, NY (United States)

    1999-07-01T23:59:59.000Z

    This paper describes the rotor dynamic stability analysis and the PTC-10 Class 1 test of a three body centrifugal compressor train for high pressure natural gas injection services. This train had a full load full pressure string test on hydrocarbon gases to a final discharge pressure of 500 BAR (7250 PSIA). Each compressor is of the back to back configuration, and is equipped with tilting pad seals, damper bearings, and a honeycomb labyrinth at the division wall with shunt holes. The driver is a gas turbine.

  4. Simple SPICE model for comparison of CMOS output driver circuits

    E-Print Network [OSTI]

    Hermann, John Karl

    1993-01-01T23:59:59.000Z

    to monitor the ground nodes of output driver circuits for noise. Both relative performance and noise levels are generated through the simulations. A test device was built to confirm that the model was effective in speed and noise comparisons. Values were... on CMOS technologies. Journal model is IEEE 'I?ansactions on Automatic Control. A. Literature Survey Research has been done in the past concerning noise generated by digital logic de- vices. In particular, Advanced CMOS Logic (ACL) integrated circuits...

  5. 59136 Federal Register / Vol. 75, No. 186 / Monday, September 27, 2010 / Rules and Regulations (c) Certain farm vehicle drivers. The

    E-Print Network [OSTI]

    ) Certain farm vehicle drivers. The rules in this part except for § 391.15(e) do not apply to a farm vehicle driver except a farm vehicle driver who drives an articulated (combination) commercial motor vehicle, as defined in § 390.5. For limited exemptions for farm vehicle drivers of articulated commercial motor

  6. Training for Records and Information Management

    Broader source: Energy.gov [DOE]

    Records Management Training:  NARA Records Management Training   NARA Targeted Assistance NARA Brochures Training Presentation:  Information Collection Requests/PRA (pdf)  

  7. Training Management Information System

    SciTech Connect (OSTI)

    Rackley, M.P.

    1989-01-01T23:59:59.000Z

    The Training Management Information System (TMIS) is an integrated information system for all training related activities. TMIS is at the leading edge of training information systems used in the nuclear industry. The database contains all the necessary records to confirm the department's adherence to accreditation criteria and houses all test questions, student records and information needed to evaluate the training process. The key to the TMIS system is that the impact of any change (i.e., procedure change, new equipment, safety incident in the commercial nuclear industry, etc.) can be tracked throughout the training process. This ensures the best training can be performed that meets the needs of the employees. TMIS is comprised of six functional areas: Job and Task Analysis, Training Materials Design and Development, Exam Management, Student Records/Scheduling, Evaluation, and Commitment Tracking. The system consists of a VAX 6320 Cluster with IBM and MacIntosh computers tied into an ethernet with the VAX. Other peripherals are also tied into the system: Exam Generation Stations to include mark sense readers for test grading, Production PC's for Desk-Top Publishing of Training Material, and PC Image Workstations. 5 figs.

  8. Federal Employee Training Manual

    Broader source: Directives, Delegations, and Requirements [Office of Management (MA)]

    2001-10-11T23:59:59.000Z

    This Manual provides detailed requirements to supplement DOE O 360.1B, FEDERAL EMPLOYEE TRAINING. The information in this Manual is intended to assist in improving Federal workforce performance under Department of Energy (DOE) managed Federal employee training. Cancels DOE M 360.1A-1. Canceled by DOE O 360.1C.

  9. Federal Employee Training Manual

    Broader source: Directives, Delegations, and Requirements [Office of Management (MA)]

    1999-09-21T23:59:59.000Z

    This Manual provides detailed requirements to supplement DOE O 360.1A, Federal Employee Training, dated 9-21-99. The information in this Manual is intended to assist in improving Federal workforce performance under Department of Energy (DOE) managed Federal employee training. Canceled by DOE M 360.1-1B.

  10. Federal Employee Training

    Broader source: Directives, Delegations, and Requirements [Office of Management (MA)]

    1999-09-21T23:59:59.000Z

    To plan and establish requirements and assign responsibilities for Department of Energy (DOE) Federal employee training, education, and development under the Government Employees Training Act of 1958, as amended. Cancels DOE O 360.1. Canceled by DOE O 360.1B.

  11. SS# L# NSHE# Athletic Training

    E-Print Network [OSTI]

    Hemmers, Oliver

    SS# L# NSHE# Athletic Training Admitted Date: Date Advised: Credits Semester Grade ENG 101 identified. Number of Transfer credits, 2-year Athletic Training Specialization or KIN 245) for admission into the Athletic Training Program. Admission process

  12. _____________________________ Environment, Health, & Safety _________ __________________ Training Program

    E-Print Network [OSTI]

    _________ __________________ Training Program EHS 370 Lockout/Tagout for Authorized Persons Course Syllabus Subject Category: Electrical participants with training on Lockout/Tagout responsibilities, acceptable practices, and procedures, and line management and supervision responsibilities. Course Objectives: After completing this training

  13. VERY LOW MASS STELLAR AND SUBSTELLAR COMPANIONS TO SOLAR-LIKE STARS FROM MARVELS. I. A LOW-MASS RATIO STELLAR COMPANION TO TYC 4110-01037-1 IN A 79 DAY ORBIT

    E-Print Network [OSTI]

    Stassun, Keivan

    TYC 4110-01037-1 has a low-mass stellar companion, whose small mass ratio and short orbital period are atypical among binary systems with solar-like (T [subscript eff] [< over ~] 6000 K) primary stars. Our analysis of TYC ...

  14. H-BAND IMAGE OF A PLANETARY COMPANION AROUND HR 8799 IN 2002

    SciTech Connect (OSTI)

    Fukagawa, Misato; Fujita, Yutaka; Shibai, Hiroshi [Department of Earth and Space Science, Graduate School of Science, Osaka University, 1-1 Machikaneyama, Toyonaka, Osaka 560-0043 (Japan); Itoh, Yoichi; Oasa, Yumiko [Graduate School of Science, Kobe University, 1-1 Rokkodai, Nada, Kobe, Hyogo 657-8501 (Japan); Tamura, Motohide [Department of Astronomical Science, Graduate University for Advanced Studies (SOKENDAI), 2-21-1 Osawa, Mitaka, Tokyo 181-8588 (Japan); Hayashi, Saeko S.; Hayashi, Masahiko [National Astronomical Observatory of Japan, 2-21-1 Osawa, Mitaka, Tokyo 181-8588 (Japan)

    2009-05-01T23:59:59.000Z

    The discovery of three planetary companions around HR 8799 marked a significant epoch in direct imaging of extrasolar planets. Given the importance of this system, we re-analyzed H-band images of HR 8799 obtained with the Subaru 36-elements adaptive optics (AO) in 2002 July. The low-order AO imaging combined with the classical point-spread function (PSF) subtractions even revealed the extrasolar planet, HR 8799b. Our observations in 2002 confirmed that it has been orbiting HR 8799 in a counterclockwise direction. The flux of HR 8799b was consistent with those in the later epochs within the uncertainty of 0.25 mag, further supporting the planetary mass estimate by Marois et al.

  15. Constraints on the formation mechanism of the planetary mass companion of 2MASS 1207334-393254

    E-Print Network [OSTI]

    G. Lodato; E. Delgado-Donate; C. J. Clarke

    2005-09-26T23:59:59.000Z

    In this paper we discuss the nature and the possible formation scenarios of the companion of the brown dwarf 2MASS 1207334-393254. We initially discuss the basic physical properties of this object and conclude that, although from its absolute mass ($5M_{\\rm Jup}$), it is a planetary object, in terms of its mass ratio $q$ and of its separation $a$ with respect to the primary brown dwarf, it is consistent with the statistical properties of binaries with higher primary mass. We then explore the possible formation mechanism for this object. We show that the standard planet formation mechanism of core accretion is far too slow to form this object within 10 Myr, the observed age of the system. On the other hand, the alternative mechanism of gravitational instability (proposed both in the context of planet and of binary formation) may, in principle, work and form a system with the observed properties.

  16. ORISE: Training and Technology Support

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

    Training and Technology Support ORISE helps train all levels of government personnel for natural disasters and man-made emergencies using latest technology The Oak Ridge Institute...

  17. ORISE: Training and Qualification Programs

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

    Training and Qualification Programs As a core part of providing effective communication and training to protect the safety of workers, the Oak Ridge Institute for Science and...

  18. _____________________________ Environment, Health, & Safety _________ __________________ Training Program

    E-Print Network [OSTI]

    Eisen, Michael

    Program EHS 369 Lockout/Tagout Practical Refresher Training For Qualified Electrical Workers Course functions. The course is designed to provide employees with hands on training on Lockout

  19. Training of nuclear facility personnel

    SciTech Connect (OSTI)

    Not Available

    1981-04-01T23:59:59.000Z

    Separate abstracts are included for each of the papers presented concerning certification and standards; operations training; the human element; and non-licensed training.

  20. THE TRENDS HIGH-CONTRAST IMAGING SURVEY. III. A FAINT WHITE DWARF COMPANION ORBITING HD 114174

    SciTech Connect (OSTI)

    Crepp, Justin R. [Department of Physics, University of Notre Dame, 225 Nieuwland Science Hall, Notre Dame, IN 46556 (United States); Johnson, John Asher [Department of Planetary Science, California Institute of Technology, 1200 E. California Blvd., Pasadena, CA 91125 (United States); Howard, Andrew W. [Institute for Astronomy, University of Hawaii, 2680 Woodlawn Drive, Honolulu, HI 96822 (United States); Marcy, Geoffrey W. [Department of Astronomy, University of California, Berkeley, CA 94720 (United States); Gianninas, Alexandros; Kilic, Mukremin [Department of Physics and Astronomy, University of Oklahoma, Norman, OK 73019 (United States); Wright, Jason T., E-mail: jcrepp@nd.edu [Department of Astronomy and Astrophysics, Pennsylvania State University, University Park, PA 16802 (United States)

    2013-09-01T23:59:59.000Z

    The nearby Sun-like star HD 114174 exhibits a strong and persistent Doppler acceleration indicating the presence of an unseen distant companion. We have acquired high-contrast imaging observations of this star using NIRC2 at Keck and report the direct detection of the body responsible for causing the ''trend''. HD 114174 B has a projected separation of 692 {+-} 9 mas (18.1 AU) and is 10.75 {+-} 0.12 mag (contrast of 5 Multiplication-Sign 10{sup -5}) fainter than its host in the K-band, requiring aggressive point-spread function subtraction to identify. Our astrometric time baseline of 1.4 yr demonstrates physical association through common proper motion. We find that the companion has absolute magnitude, M{sub J} = 13.97 {+-} 0.11, and colors, J - K = 0.12 {+-} 0.16 mag. These characteristics are consistent with an Almost-Equal-To T3 dwarf, initially leading us to believe that HD 114174 B was a substellar object. However, a dynamical analysis that combines radial velocity measurements with available imaging data indicates a minimum mass of 0.260 {+-} 0.010 M{sub Sun }. We conclude that HD 114174 B must be a white dwarf. Assuming a hydrogen-rich composition, atmospheric and evolutionary model fits yield an effective temperature T{sub eff} = 8200 {+-} 4000 K, surface gravity log g = 8.90 {+-} 0.02, and cooling age of t{sub c} Almost-Equal-To 3.4 Gyr, which is consistent with the 4.7{sup +2.3}{sub -2.6} Gyr host star isochronal age estimate. HD 114174 B is a benchmark object located only 26.14 {+-} 0.37 pc from the Sun. It may be studied at a level of detail comparable to Sirius and Procyon, and used to understand the link between the mass of white dwarf remnants with that of their progenitors.

  1. Limits on additional planetary companions to OGLE-2005-BLG-390L

    E-Print Network [OSTI]

    D. Kubas; A. Cassan; M. Dominik; D. Bennett

    2008-02-27T23:59:59.000Z

    We investigate constraints on additional planets orbiting the distant M-dwarf star OGLE-2005-BLG-390L, around which photometric microlensing data has revealed the existence of the sub-Neptune-mass planet OGLE-2005-BLG-390Lb. We specifically aim to study potential Jovian companions and compare our findings with predictions from core-accretion and disc-instability models of planet formation. We also obtain an estimate of the detection probability for sub-Neptune mass planets similar to OGLE-2005-BLG-390Lb using a simplified simulation of a microlensing experiment. We compute the efficiency of our photometric data for detecting additional planets around OGLE-2005-BLG-390L, as a function of the microlensing model parameters and convert it into a function of the orbital axis and planet mass by means of an adopted model of the Milky Way. We find that more than 50 % of potential planets with a mass in excess of 1 M_J between 1.1 and 2.3 AU around OGLE-2005-BLG-390L would have revealed their existence, whereas for gas giants above 3 M_J in orbits between 1.5 and 2.2 AU, the detection efficiency reaches 70 %; however, no such companion was observed. Our photometric microlensing data therefore do not contradict the existence of gas giant planets at any separation orbiting OGLE-2005-BLG-390L. Furthermore we find a detection probability for an OGLE-2005-BLG-390Lb-like planet of around 2-5 %. In agreement with current planet formation theories, this quantitatively supports the prediction that sub-Neptune mass planets are common around low-mass stars.

  2. Know The Star, Know the Planet. IV. A Stellar Companion to the Host star of the Eccentric Exoplanet HD 8673b

    E-Print Network [OSTI]

    Roberts,, Lewis C; Neyman, Christopher R; Wu, Yanqin; Riddle, Reed L; Shelton, J Christopher; Angione, John; Baranec, Christoph; Bouchez, Antonin; Bui, Khanh; Burruss, Rick; Burse, Mahesh; Chordia, Pravin; Croner, Ernest; Das, Hillol; Dekany, Richard G; Guiwits, Stephen; Hale, David; Henning, John; Law, Shrinivas Kulkarni Nicholas; McKenna, Dan; Milburn, Jennifer; Palmer, Dean; Punnadi, Sujit; Ramaprakash, A N; Roberts, Jennifer E; Tendulkar, Shriharsh P; Trinh, Thang; Troy, Mitchell; Truong, Tuan; Zolkower, Jeff

    2015-01-01T23:59:59.000Z

    HD 8673 hosts a massive exoplanet in a highly eccentric orbit (e=0.723). Based on two epochs of speckle interferometry a previous publication identi?ed a candidate stellar companion. We observed HD 8673 multiple times with the 10 m Keck II telescope, the 5 m Hale telescope, the 3.63 m AEOS telescope and the 1.5m Palomar telescope in a variety of ?lters with the aim of con?rming and characterizing the stellar companion. We did not detect the candidate companion, which we now conclude was a false detection, but we did detect a fainter companion. We collected astrometry and photometry of the companion on six epochs in a variety of ?lters. The measured di?erential photometry enabled us to determine that the companion is an early M dwarf with a mass estimate of 0.33-0.45 M?. The companion has a projected separation of 10 AU, which is one of the smallest projected separations of an exoplanet host binary system. Based on the limited astrometry collected, we are able to constrain the orbit of the stellar companion to...

  3. The effects of driver gas contamination on shock tube test time

    E-Print Network [OSTI]

    Hawkins, Garry Owen

    1970-01-01T23:59:59.000Z

    THE EFFECTS OF DRIVER GAS CONTAMINATION ON SHOCK TUBE TEST TIME A Thesis by CARRY OWEN HAWKINS Approved as to style and content by: (Chairman of Committee) (Head of Department) (Memb e r) (Member) (Member) (Membe r) (Member) December 1970... AB S TRACT The Effects of Driver Gas Contamination on Shock Tube Test Time. (December 1970) Garry 0. Hawkins, B. S. , Texas A&M University; Directed by: Dr. Richard E. Thomas The effects of driver gas contamination are manifested in a change...

  4. Robust high-contrast companion detection from interferometric observations. The CANDID algorithm and an application to six binary Cepheids

    E-Print Network [OSTI]

    Gallenne, A; Kervella, P; Monnier, J D; Schaefer, G H; Baron, F; Breitfelder, J; Bouquin, J B Le; Roettenbacher, R M; Gieren, W; Pietrzynski, G; McAlister, H; Brummelaar, T ten; Sturmann, J; Sturmann, L; Turner, N; Ridgway, S; Kraus, S

    2015-01-01T23:59:59.000Z

    Long-baseline interferometry is an important technique to spatially resolve binary or multiple systems in close orbits. By combining several telescopes together and spectrally dispersing the light, it is possible to detect faint components around bright stars. Aims. We provide a rigorous and detailed method to search for high-contrast companions around stars, determine the detection level, and estimate the dynamic range from interferometric observations. We developed the code CANDID (Companion Analysis and Non-Detection in Interferometric Data), a set of Python tools that allows us to search systematically for point-source, high-contrast companions and estimate the detection limit. The search pro- cedure is made on a N x N grid of fit, whose minimum needed resolution is estimated a posteriori. It includes a tool to estimate the detection level of the companion in the number of sigmas. The code CANDID also incorporates a robust method to set a 3{\\sigma} detection limit on the flux ratio, which is based on an a...

  5. ULAS J141623.94+134836.3: A BLUE T DWARF COMPANION TO A BLUE L DWARF

    E-Print Network [OSTI]

    Burgasser, Adam J.

    We confirm the substellar nature of ULAS J141623.94+134836.3 (aka SDSS J1416+1348B), a common proper motion companion to the blue L dwarf SDSS J141624.08+134826.7 identified by Burningham et al. and Scholz. Low-resolution ...

  6. Discovery of a Low-Mass Companion to a Metal-Rich F Star with the MARVELS Pilot Project

    E-Print Network [OSTI]

    Fleming, Scott W; Mahadevan, Suvrath; Lee, Brian; Eastman, Jason D; Siverd, Robert J; Gaudi, B Scott; Niedzielski, Andrzej; Sivarani, Thirupathi; Stassun, Keivan; Wolszczan, Alex; Barnes, Rory; Gary, Bruce; Nguyen, Duy Cuong; Morehead, Robert C; Wan, Xiaoke; Zhao, Bo; Liu, Jian; Guo, Pengcheng; Kane, Stephen R; van Eyken, Julian C; De Lee, Nathan M; Crepp, Justin R; Shelden, Alaina C; Laws, Chris; Wisniewski, John P; Schneider, Donald P; Pepper, Joshua; Snedden, Stephanie A; Pan, Kaike; Bizyaev, Dmitry; Brewington, Howard; Malanushenko, Olena; Malanushenko, Viktor; Oravetz, Daniel; Simmons, Audrey; Watters, Shannon

    2010-01-01T23:59:59.000Z

    We report the discovery of a low-mass companion orbiting the metal-rich, main sequence F star TYC 2949-00557-1 during the MARVELS (Multi-object APO Radial Velocity Exoplanet Large-area Survey) Pilot Project. The host star has an effective temperature T_eff = 6135 +/- 40 K, log(g) = 4.4 +/- 0.1 and [Fe/H] = 0.32 +/- 0.01, indicating a mass of M = 1.25 +/- 0.09 M_\\odot and R = 1.15 +/- 0.15 R_\\odot. The companion has an orbital period of 5.69449 +/- 0.00023 days and straddles the hydrogen burning limit with a minimum mass of 64 M_J, and may thus be an example of the rare class of brown dwarfs orbiting at distances comparable to those of "Hot Jupiters." We present relative photometry that demonstrates the host star is photometrically stable at the few millimagnitude level on time scales of hours to years, and rules out transits for a companion of radius greater than 0.8 R_J at the 95% confidence level. Tidal analysis of the system suggests that the star and companion are likely in a double synchronous state wher...

  7. P5 Science Drivers: Accelerator Experiments Panagiotis Spentzouris

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level:Energy: Grid Integration Redefining What's Possible for RenewableSpeedingBiomass and BiofuelsOversight BoardP-GlycoproteiniiiScience Drivers:

  8. Philips Light Sources & Electronics is Developing an Efficient, Smaller, Cost-Effective Family of LED Drivers

    Broader source: Energy.gov [DOE]

    With the help of DOE funding, Philips Light Sources & Electronics is developing a new family of LED drivers that are more efficient and cost-effective as well as smaller in size than currently available drivers. The new drivers are switch-mode power supplies that are similar to today's drivers, but with an improved design. In addition, they have a different topology—boost plus LLC—for wattages of 40W and above, but they retain the commonly used flyback topology at lower wattages.

  9. Factors Associated with Hit-and-Run Pedestrian Fatalities and Driver Identification

    E-Print Network [OSTI]

    MacLeod, Kara E.; Griswold, Julia; Arnold, Lindsay S.; Ragland, David R

    2010-01-01T23:59:59.000Z

    Hit-and-run Crashes. Accident Analysis and Prevention, Vol.Circumstances and Drivers. Accident Analysis and Prevention,Hit-and-run Crashes. Accident Analysis and Prevention, Vol.

  10. Radiation Safety Training Basic Radiation Safety Training for

    E-Print Network [OSTI]

    Dai, Pengcheng

    Radiation Safety Training Basic Radiation Safety Training for Sealed Source Users for Physics 461 Protocol Title: Training for Sealed Source Users Drafted By: Chris Millsaps, RSS Reviewers: ZB, TU, GS Purpose: To provide basic radiation safety training to the users of sealed sources located

  11. AMIS-Training Material iReport Training Part 2

    E-Print Network [OSTI]

    Farritor, Shane

    AMIS- Training Material iReport Training ­Part 2 (iReport-3.0.0) Topic: Parameters · Open a report- Training Material · Open the `Document structure' Page 2 of 7 6/27/2008 Institutional Research and Planning University of Nebraska-Lincoln #12;AMIS- Training Material · Right click on `Parameters' > Add > Parameter

  12. Radiation Safety Training Basic Radiation Safety Training for

    E-Print Network [OSTI]

    Dai, Pengcheng

    Radiation Safety Training Basic Radiation Safety Training for X-ray Users for Physics 461 & 462 Protocol Title: Basic Radiation Safety Training for X-ray Users Drafted By: Chris Millsaps, RSS Reviewers: ZB, TU, GS Purpose: To provide basic radiation safety training to the users of x-ray producing

  13. Training Session: Frederick, MD

    Broader source: Energy.gov [DOE]

    This 3.5-hour training provides builders with a comprehensive review of zero net-energy-ready home construction including the business case, detailed specifications, and opportunities to be...

  14. DVU Featured Training & Events ...

    Energy Savers [EERE]

    Featured Training & Events Form Please complete this form in its entirety and email to AskTheDvu@hq.doe.gov 1. Course Title: 2. Course StartEnd Date: 3. StartEnd Time (Time zone...

  15. Computerized training management system

    DOE Patents [OSTI]

    Rice, H.B.; McNair, R.C.; White, K.; Maugeri, T.

    1998-08-04T23:59:59.000Z

    A Computerized Training Management System (CTMS) is disclosed for providing a procedurally defined process that is employed to develop accreditable performance based training programs for job classifications that are sensitive to documented regulations and technical information. CTMS is a database that links information needed to maintain a five-phase approach to training-analysis, design, development, implementation, and evaluation independent of training program design. CTMS is designed using R-Base{trademark}, an-SQL compliant software platform. Information is logically entered and linked in CTMS. Each task is linked directly to a performance objective, which, in turn, is linked directly to a learning objective; then, each enabling objective is linked to its respective test items. In addition, tasks, performance objectives, enabling objectives, and test items are linked to their associated reference documents. CTMS keeps all information up to date since it automatically sorts, files and links all data; CTMS includes key word and reference document searches. 18 figs.

  16. Computerized training management system

    DOE Patents [OSTI]

    Rice, Harold B. (Franklin Furnace, OH); McNair, Robert C. (East Setauket, NY); White, Kenneth (Shirley, NY); Maugeri, Terry (Wading River, NY)

    1998-08-04T23:59:59.000Z

    A Computerized Training Management System (CTMS) for providing a procedurally defined process that is employed to develop accreditable performance based training programs for job classifications that are sensitive to documented regulations and technical information. CTMS is a database that links information needed to maintain a five-phase approach to training-analysis, design, development, implementation, and evaluation independent of training program design. CTMS is designed using R-Base.RTM., an-SQL compliant software platform. Information is logically entered and linked in CTMS. Each task is linked directly to a performance objective, which, in turn, is linked directly to a learning objective; then, each enabling objective is linked to its respective test items. In addition, tasks, performance objectives, enabling objectives, and test items are linked to their associated reference documents. CTMS keeps all information up to date since it automatically sorts, files and links all data; CTMS includes key word and reference document searches.

  17. NUG 2014 Training Presentations

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

    David Turner, NERSC | Download File: 08-FileSystems2.pdf | pdf | 1 MB New User Training: Introduction to NERSC February 3, 2014 | Author(s): Harvey Wasserman, NERSC |...

  18. NUG 2014 Training Presentations

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

    Cholia, NERSC | Download File: 06-WebPortals-NUG2014.pdf | pdf | 1.3 MB New User Training: Introduction to NERSC February 3, 2014 | Author(s): Harvey Wasserman, NERSC |...

  19. Training Session: Carbondale, CO

    Broader source: Energy.gov [DOE]

    This 3.5-hour training provides builders with a comprehensive review of zero energy-ready home construction including the business case, detailed specifications, and opportunities to be recognized...

  20. Worker Training Program (Nebraska)

    Broader source: Energy.gov [DOE]

    The Worker Training Program is a business incentive program to support the retraining and upgrading of Nebraska’s current workforce. The amount of grant funding available quarterly is distributed...

  1. Training Session: Buffalo, NY

    Broader source: Energy.gov [DOE]

    This 3.5-hour training provides builders with a comprehensive review of zero energy-ready home construction including the business case, detailed specifications, and opportunities to be recognized...

  2. ZERH Training: Harrisonburg, VA

    Broader source: Energy.gov [DOE]

    This 3.5-hour training provides builders with a comprehensive review of zero energy-ready home construction including the business case, detailed specifications, and opportunities to be recognized...

  3. Training and Organizational Development

    E-Print Network [OSTI]

    Training and Organizational Development Contact: Ellen Audley Assistant, (970) 491-1376, Ellen & Organizational Development" from the selection box ·Select the "Login" tab and login ·Select the "Add Class" tab

  4. Training Session: Euless, TX

    Broader source: Energy.gov [DOE]

    This 3.5-hour training provides builders with a comprehensive review of zero energy-ready home construction including the business case, detailed specifications, and opportunities to be recognized...

  5. Assessor Training Internal Audits and

    E-Print Network [OSTI]

    NVLAP Assessor Training Internal Audits and Management Reviews #12;Assessor Training 2009, quarterly, etc., schedule throughout the year #12;Assessor Training 2009: Internal Audits and Management a copy of the full internal audit schedule. #12;Assessor Training 2009: Internal Audits and Management

  6. Training for Early Career Researchers

    E-Print Network [OSTI]

    Greifswald, Ernst-Moritz-Arndt-Universität

    Training for Early Career Researchers Research Management Training for 16 ­ 17 September 2014 training in an intensive, yet effective workshop form over two days. There is a strong emphasis on European Management Training for Early Career Researchers 16 ­ 17 September 2014 in Hamburg #12;

  7. Assessor Training Annex A: Referencing

    E-Print Network [OSTI]

    NVLAP Assessor Training Annex A: Referencing NVLAP Accreditation #12;Assessor Training: Annex · NVLAP reserves the right to control its use #12;Assessor Training: Annex A (rev. 2012-07-31) 33 · NVLAP of technical competence #12;Assessor Training: Annex A (rev. 2012-07-31) 44 · It is NVLAP's responsibility

  8. Assessor Training NVLAP Assessment Forms

    E-Print Network [OSTI]

    NVLAP Assessor Training NVLAP Assessment Forms #12;Assessor Training 2009: NVLAP Assessment Forms 2 Summary ·Test Method Review Summary ·ProgramSpecific Checklists Examples #12;Assessor Training 2009: NVLAP are completed · Assessor Names, Dates, Lab Code #12;Assessor Training 2009: NVLAP Assessment Forms 4 NIST

  9. Academic Training (J-1 Student)

    E-Print Network [OSTI]

    Heller, Barbara

    Academic Training (J-1 Student) International Center D E F I N I T I O N : J-1 students Training. Such employment can only be in a field of study indicated on the student's DS-2019. C O N D I T I months of academic training (post-doctoral research/teaching positions only). Academic training can

  10. Training Program Environmental Health & Safety

    E-Print Network [OSTI]

    Jia, Songtao

    Training Program Overview Environmental Health & Safety VISION STATEMENT We provide expert guidance University Medical Center 212-854-8749 Morningside Campus 212-854-8749 Introduction Training&S offers a wide range of training programs, presented by subject matter experts in multiple formats

  11. University of Rochester Respirator Training

    E-Print Network [OSTI]

    Mahon, Bradford Z.

    (SCBA) UofR Respirator Training 8 #12;Air Purifying Respirators (Particulate) Tight-fitting respirator

  12. UWB multi-burst transmit driver for averaging receivers

    DOE Patents [OSTI]

    Dallum, Gregory E

    2012-11-20T23:59:59.000Z

    A multi-burst transmitter for ultra-wideband (UWB) communication systems generates a sequence of precisely spaced RF bursts from a single trigger event. There are two oscillators in the transmitter circuit, a gated burst rate oscillator and a gated RF burst or RF power output oscillator. The burst rate oscillator produces a relatively low frequency, i.e., MHz, square wave output for a selected transmit cycle, and drives the RF burst oscillator, which produces RF bursts of much higher frequency, i.e., GHz, during the transmit cycle. The frequency of the burst rate oscillator sets the spacing of the RF burst packets. The first oscillator output passes through a bias driver to the second oscillator. The bias driver conditions, e.g., level shifts, the signal from the first oscillator for input into the second oscillator, and also controls the length of each RF burst. A trigger pulse actuates a timing circuit, formed of a flip-flop and associated reset time delay circuit, that controls the operation of the first oscillator, i.e., how long it oscillates (which defines the transmit cycle).

  13. Gaz de France ordering high-efficiency drivers

    SciTech Connect (OSTI)

    de Biasi, V.

    1980-11-01T23:59:59.000Z

    For natural gas transmission, distribution, and storage operations, Gaz de France is installing Creusot-Loire's new line of high-efficiency gas-turbine packages, powered by Allison 501 and 570 generators for compressor speeds exceeding 10,000 rpm. The Type CA.3 driver comprises a 501 generator coupled to a two-stage power turbine; the ISO base rating is 3265 kW on gas fuel with a heat rate of 12,050 Btu/kWhr. The CA.5 driver with the stronger 570 gas-turbine engine is base-rated at 4805 kW with a heat rate of 11,360 Btu/kWhr. Designed for direct-drive, with no intermediary gearing, the high-speed compressor operates on the 13,820-rpm output shaft speed of the CA.3 for baseload requirements or on 11,500 rpm for the more powerful CA.5 set. These compressor packages will serve as boosters for the transmission and storage of regasified LNG from Algeria and natural gas from the North Sea, USSR, and France's own Lacq fields.

  14. Mentoring and Job Training in the Field for Newly Trained Contractors...

    Energy Savers [EERE]

    Mentoring and Job Training in the Field for Newly Trained Contractors Mentoring and Job Training in the Field for Newly Trained Contractors Better Buildings Neighborhood Program...

  15. Shaping the output pulse of a linear-transformer-driver module W. A. Stygar,1

    E-Print Network [OSTI]

    Shaping the output pulse of a linear-transformer-driver module W. A. Stygar,1 W. E. Fowler,1 K. R a linear-transformer- driver (LTD) module that drives an internal water-insulated transmission line-insulated radial-transmission-line impedance transformers [Phys. Rev. ST Accel. Beams 11, 030401 (2008)]. DOI: 10

  16. Submitted to Vehicle System Dynamics An Adaptive Lateral Preview Driver Model

    E-Print Network [OSTI]

    Peng, Huei

    of the vehicle. The proposed driver model is developed using the adaptive predictive control (APC) framework inspires our interest in understanding human steering actions and the development of a driver model on the response of the vehicle. These tests can be performed with a steering and speed control robot, and thus can

  17. 1 Drivers of the projected changes to the Pacific Ocean 2 equatorial circulation

    E-Print Network [OSTI]

    Paris-Sud XI, Université de

    1 Drivers of the projected changes to the Pacific Ocean 2 equatorial circulation 3 A. Sen Gupta,1 A), 29 Drivers of the projected changes to the Pacific Ocean equatorial 30 circulation, Geophys. Res. Lett., 39, LXXXXX, doi:10.1029/ 31 2012GL051447. 32 1. Introduction 33 [2] The equatorial Pacific Ocean

  18. AABBSSTTRRAACCTT MA, RUIQI. The Effect of In-Vehicle Automation and Reliability on Driver Situation

    E-Print Network [OSTI]

    Kaber, David B.

    AABBSSTTRRAACCTT MA, RUIQI. The Effect of In-Vehicle Automation and Reliability on Driver Situation by automation and in- vehicle device use. Specifically, this study investigated the implications of adaptive; investigate the effect of varying reliability of in-vehicle automation (navigation aids) on driver SA

  19. Nighttime driver needs: an analysis of sign usage based on luminance

    E-Print Network [OSTI]

    Clark, Jerremy Eugene

    2007-09-17T23:59:59.000Z

    ? With brighter signs being visible from farther away, there is an increased opportunity for the driver to look at the sign. This thesis assesses the impact of sign brightness on the nighttime driver�s sign viewing behavior; such as the number of glances...

  20. Expert Recommendation based on Social Drivers, Social Network Analysis, and Semantic Data Representation

    E-Print Network [OSTI]

    Fox, Mark S.

    Expert Recommendation based on Social Drivers, Social Network Analysis, and Semantic Data-Theoretical Multi-Level (MTML) framework which investigates social drivers for network formation in the communities computational techniques from social network analysis and representational techniques from the semantic web

  1. UC SANTA BARBARA POLICY AND PROCEDURE Driving Records for Designated Employees and Drivers

    E-Print Network [OSTI]

    Bigelow, Stephen

    when employees are convicted of motor vehicle violations and when actions are taken against a driver a special certificate (ambulance, private school bus, farm labor vehicle, special construction equipment with this policy. C. There are criminal penalties for employing or continuing to employ as a driver a person who

  2. Catadioptric Sensor for a Simultaneous Tracking of the Driver's Face and the Road Scene

    E-Print Network [OSTI]

    Paris-Sud XI, Université de

    using head mounted devices but these systems are too intrusive in the driving task. The most popular non-intrusive to be non-intrusive and compact (to avoid distracting the driver in his task), able to observe the driver on Omnidirectional Vision, Camera Networks and Non-classical Cameras - OMNIVIS (2008)" #12;2 J-F. Layerle, X

  3. STATE OF CALIFORNIA -GENERAL SERVICES -RISK AND INSURANCE MANAGEMENT STATE DRIVER ACCIDENT REVIEW

    E-Print Network [OSTI]

    Ponce, V. Miguel

    STATE OF CALIFORNIA - GENERAL SERVICES - RISK AND INSURANCE MANAGEMENT STATE DRIVER ACCIDENT REVIEW STD. 274 (REV. 1/2003) PLEASE PRINT OR TYPE SUPERVISOR'S REVIEW - FOR DEPARTMENTAL ACCIDENT PREVENTION PURPOSE: To have supervisor investigate each driver accident, report facts and circumstances, confirm

  4. PSR J1311-3430: A HEAVYWEIGHT NEUTRON STAR WITH A FLYWEIGHT HELIUM COMPANION

    SciTech Connect (OSTI)

    Romani, Roger W. [Department of Physics, Stanford University, Stanford, CA 94305 (United States); Filippenko, Alexei V.; Silverman, Jeffrey M.; Cenko, S. Bradley [Department of Astronomy, University of California, Berkeley, CA 94720-3411 (United States); Greiner, Jochen; Rau, Arne; Elliott, Jonathan [Max-Planck-Instituet fuer Extraterrestrische Physik, D-85748 Garching (Germany); Pletsch, Holger J., E-mail: rwr@astro.stanford.edu [Max-Planck-Instituet fuer Gravitationsphysik (Albert-Einstein-Instituet), D-30167 Hannover (Germany)

    2012-12-01T23:59:59.000Z

    We have obtained initial spectroscopic observations and additional photometry of the newly discovered P{sub b} = 94 minute {gamma}-ray black-widow pulsar PSR J1311-3430. The Keck spectra show a He-dominated, nearly H-free photosphere and a large radial-velocity amplitude of 609.5 {+-} 7.5 km s{sup -1}. Simultaneous seven-color GROND photometry further probes the heating of this companion, and shows the presence of a flaring infrared excess. We have modeled the quiescent light curve, constraining the orbital inclination and masses. Simple heated light-curve fits give M{sub NS} = 2.7 M{sub Sun }, but show systematic light-curve differences. Adding extra components allows a larger mass range to be fit, but all viable solutions have M{sub NS} > 2.1 M{sub Sun }. If confirmed, such a large M{sub NS} substantially constrains the equation of state of matter at supernuclear densities.

  5. Training discriminative computer vision models with weak supervision

    E-Print Network [OSTI]

    Babenko, Boris

    2012-01-01T23:59:59.000Z

    during training. . . . . . . . . . . . . . . . . . . . . .of the image. Prior to training, T overlapping regions arefor training . . . . . . . . . . . . . . . . . . . . . . . .

  6. Training | Department of Energy

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level:Energy: Grid Integration Redefining What'sis Taking Over OurThe Iron Spin Transition in2, 2003Tool ofTopoCarbon DioxideTraining Training The

  7. Training | The Ames Laboratory

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level: National5Sales for4,645U.S. DOE Office of ScienceandMesa del SolStrengthening a solidSynthesisAppliances » TopToursTraining WorksheetTraining

  8. Marketplace Training Marketplace offers several training opportunities below. To request a dedicated training for your department or group, or for

    E-Print Network [OSTI]

    Tsien, Roger Y.

    Marketplace Training Marketplace offers several training opportunities below. To request a dedicated training for your department or group, or for general questions about Marketplace please contact

  9. Linac-Based Proton Driver for a Neutrino Factory

    E-Print Network [OSTI]

    Garoby, R; Aiba, M; Meddahi, M

    2009-01-01T23:59:59.000Z

    A Neutrino Factory Proton Driver based on a superconducting proton linac has been designed in the CERN context. The 5 GeV/4 MW H- beam from the linac is accumulated using charge exchange injection in a fixed-energy synchrotron and afterwards transferred to a compressor ring, where bunch rotation takes place. The lattices of the accumulator and compressor are described, as well as magnet technology and RF manipulations. Critical issues related to charge-exchange injection, space-charge effects in the compressor and beam stability in the accumulator, are addressed. The analysis is focused on the baseline scenario, which provides 6 bunches on the target. Results of preliminary analysis of options with less bunches (three and one) are also presented.

  10. Recirculating induction accelerators as drivers for heavy ion fusion

    SciTech Connect (OSTI)

    Barnard, J.J.; Deadrick, F.; Friedman, A.; Grote, D.P.; Griffith, L.V.; Kirbie, H.C.; Neil, V.K.; Newton, M.A.; Paul, A.C.; Sharp, W.M.; Shay, H.D. (Lawrence Livermore National Laboratory, Livermore, California 94550 (United States)); Bangerter, R.O.; Faltens, A.; Fong, C.G.; Judd, D.L.; Lee, E.P.; Reginato, L.L.; Yu, S.S. (Lawrence Berkeley Laboratory, Berkeley, California 94720 (United States)); Godlove, T.F. (FM Technologies, Inc., 10529-B Braddock Rd., Fairfax, Virginia 22302 (United States))

    1993-07-01T23:59:59.000Z

    A two-year study of recirculating induction heavy ion accelerators as low-cost driver for inertial-fusion energy applications was recently completed. The projected cost of a 4 MJ accelerator was estimated to be about $500 M (million) and the efficiency was estimated to be 35%. The principal technology issues include energy recovery of the ramped dipole magnets, which is achieved through use of ringing inductive/capacitive circuits, and high repetition rates of the induction cell pulsers, which is accomplished through arrays of field effect transistor (FET) switches. Principal physics issues identified include minimization of particle loss from interactions with the background gas, and more demanding emittance growth and centroid control requirements associated with the propagation of space-charge-dominated beams around bends and over large path lengths. In addition, instabilities such as the longitudinal resistive instability, beam-breakup instability and betatron-orbit instability were found to be controllable with careful design.

  11. A Shared Population of Epidemic Methicillin-Resistant Staphylococcus aureus 15 Circulates in Humans and Companion Animals

    E-Print Network [OSTI]

    Harrison, Ewan M.; Weinert, Lucy A.; Holden, Matthew T. G.

    2014-05-13T23:59:59.000Z

    and Environmental Sciences, University of Hull, Hull, United Kingdomf; Centre for Preventive Medicine, Animal Health Trust, Kentford, Newmarket, Suffolk, United Kingdomg ABSTRACT Methicillin-resistant Staphylococcus aureus (MRSA) is a global human health problem... causing infections in both hos- pitals and the community. Companion animals, such as cats, dogs, and horses, are also frequently colonized by MRSA and can become infected. We sequenced the genomes of 46 multilocus sequence type (ST) 22 MRSA isolates from...

  12. VERY LOW MASS STELLAR AND SUBSTELLAR COMPANIONS TO SOLAR-LIKE STARS FROM MARVELS. I. A LOW-MASS RATIO STELLAR COMPANION TO TYC 4110-01037-1 IN A 79 DAY ORBIT

    SciTech Connect (OSTI)

    Wisniewski, John P.; Agol, Eric; Barnes, Rory [Astronomy Department, University of Washington, Box 351580, Seattle, WA 98195 (United States); Ge, Jian; De Lee, Nathan; Fleming, Scott W.; Lee, Brian L.; Chang, Liang [Department of Astronomy, University of Florida, 211 Bryant Space Science Center, Gainesville, FL 32611-2055 (United States); Crepp, Justin R. [Department of Astrophysics, California Institute of Technology, 1200 E. California Blvd., Pasadena, CA 91125 (United States); Eastman, Jason; Gaudi, B. Scott [Department of Astronomy, Ohio State University, 140 West 18th Avenue, Columbus, OH 43210 (United States); Esposito, Massimiliano; Gonzalez Hernandez, Jonay I.; Prieto, Carlos Allende [Instituto de Astrofisica de Canarias (IAC), E-38205 La Laguna, Tenerife (Spain); Ghezzi, Luan; Da Costa, Luiz N.; Porto De Mello, G. F. [Laboratorio Interinstitucional de e-Astronomia-LIneA, Rio de Janeiro, RJ 20921-400 (Brazil); Stassun, Keivan G.; Cargile, Phillip [Department of Physics and Astronomy, Vanderbilt University, Nashville, TN 37235 (United States); Bizyaev, Dmitry, E-mail: jwisnie@u.washington.edu [Apache Point Observatory, P.O. Box 59, Sunspot, NM 88349-0059 (United States); and others

    2012-05-15T23:59:59.000Z

    TYC 4110-01037-1 has a low-mass stellar companion, whose small mass ratio and short orbital period are atypical among binary systems with solar-like (T{sub eff} {approx}< 6000 K) primary stars. Our analysis of TYC 4110-01037-1 reveals it to be a moderately aged ({approx}<5 Gyr) solar-like star having a mass of 1.07 {+-} 0.08 M{sub Sun} and radius of 0.99 {+-} 0.18 R{sub Sun }. We analyze 32 radial velocity (RV) measurements from the SDSS-III MARVELS survey as well as 6 supporting RV measurements from the SARG spectrograph on the 3.6 m Telescopio Nazionale Galileo telescope obtained over a period of {approx}2 years. The best Keplerian orbital fit parameters were found to have a period of 78.994 {+-} 0.012 days, an eccentricity of 0.1095 {+-} 0.0023, and a semi-amplitude of 4199 {+-} 11 m s{sup -1}. We determine the minimum companion mass (if sin i = 1) to be 97.7 {+-} 5.8 M{sub Jup}. The system's companion to host star mass ratio, {>=}0.087 {+-} 0.003, places it at the lowest end of observed values for short period stellar companions to solar-like (T{sub eff} {approx}< 6000 K) stars. One possible way to create such a system would be if a triple-component stellar multiple broke up into a short period, low q binary during the cluster dispersal phase of its lifetime. A candidate tertiary body has been identified in the system via single-epoch, high contrast imagery. If this object is confirmed to be comoving, we estimate it would be a dM4 star. We present these results in the context of our larger-scale effort to constrain the statistics of low-mass stellar and brown dwarf companions to FGK-type stars via the MARVELS survey.

  13. A HIGHLY INCLINED ORBIT FOR THE 110 DAY PERIOD M-DWARF COMPANION KOI-368.01

    SciTech Connect (OSTI)

    Zhou, George [Research School of Astronomy and Astrophysics, Australian National University, Cotter Road, Weston Creek, ACT 2611 (Australia)] [Research School of Astronomy and Astrophysics, Australian National University, Cotter Road, Weston Creek, ACT 2611 (Australia); Huang, Chelsea X., E-mail: george@mso.anu.edu.au [Department of Astrophysical Sciences, 4 Ivy Lane, Peyton Hall, Princeton University, Princeton, NJ 08544 (United States)

    2013-10-20T23:59:59.000Z

    We report the detection of asymmetry in the transit light curves of the 110 day period companion to KOI-368, a rapidly rotating A-dwarf. The significant distortion in the transit light curve is attributed to spin-orbit misalignment between the transiting companion and the gravity darkened host star. Our analysis was based on 11 long cadence and 2 short cadence transits of KOI-368.01 from the Kepler mission, as well as stellar parameters determined from our follow-up spectroscopic observation. We measured the true obliquity between the orbit normal and the stellar rotation axis to be 69{sub -10}{sup +9o}. We also find a secondary eclipse event with depth 29 ± 3 ppm at phase 0.59, from which the temperature of the companion is constrained to 3060 ± 50 K, indicating that KOI-368.01 is a late M-dwarf. The eccentricity is also calculated from the eclipse to be 0.1429 ± 0.0007. The long period, high obliquity, and low eccentricity of KOI-368.01 allow us to limit a number of proposed theories for the misalignment of binary systems.

  14. A Close Companion Search around L Dwarfs using Aperture Masking Interferometry and Palomar Laser Guide Star Adaptive Optics

    E-Print Network [OSTI]

    Bernat, David; Ireland, Michael; Tuthill, Peter; Martinache, Frantz; Angione, John; Burruss, Rick S; Cromer, John L; Dekany, Richard G; Guiwits, Stephen R; Henning, John R; Hickey, Jeff; Kibblewhite, Edward; McKenna, Daniel L; Moore, Anna M; Petrie, Harold L; Roberts, Jennifer; Shelton, J Chris; Thicksten, Robert P; Trinh, Thang; Tripathi, Renu; Troy, Mitchell; Truong, Tuan; Velur, Viswa; Lloyd, James P

    2010-01-01T23:59:59.000Z

    We present a close companion search around sixteen known early-L dwarfs using aperture masking interferometry with Palomar laser guide star adaptive optics. The use of aperture masking allows the detection of close binaries, corresponding to projected physical separations of 0.6-10.0 AU for the targets of our survey. This survey achieved median contrast limits of Delta_K ~ 2.3 for separations between 1.2 - 4 lambda/D, and Delta_K ~ 1.4 at (2/3)lambda/D. We present four candidate binaries detected with moderate to high confidence (90-98%). Two have projected physical separations less than 1.5 AU. This may indicate that tight-separation binaries contribute more significantly to the binary fraction than currently assumed, consistent with spectroscopic and photometric overluminosity studies. Ten targets of this survey have previously been observed with the Hubble Space Telescope as part of companion searches. We use the increased resolution of aperture masking to search for close or dim companions that would be o...

  15. A CLOSE COMPANION SEARCH AROUND L DWARFS USING APERTURE MASKING INTERFEROMETRY AND PALOMAR LASER GUIDE STAR ADAPTIVE OPTICS

    SciTech Connect (OSTI)

    Bernat, David [Department of Astronomy, Cornell University, Ithaca, NY 14853 (United States); Bouchez, Antonin H.; Cromer, John L.; Dekany, Richard G.; Moore, Anna M. [California Institute of Technology, Pasadena, CA 91125 (United States); Ireland, Michael; Tuthill, Peter [Sydney Institute for Astrophysics, School of Physics, University of Sydney (Australia); Martinache, Frantz [National Astronomical Observatory of Japan, Subaru Telescope, Hilo, HI 96720 (United States); Angione, John; Burruss, Rick S.; Guiwits, Stephen R.; Henning, John R.; Hickey, Jeff; Kibblewhite, Edward; McKenna, Daniel L.; Petrie, Harold L.; Roberts, Jennifer; Shelton, J. Chris; Thicksten, Robert P.; Trinh, Thang [Palomar Laser Guide Star Adaptive Optics Team, Palomar Observatory, California Institute of Technology, Palomar Mountain, CA 92060 (United States)

    2010-06-01T23:59:59.000Z

    We present a close companion search around 16 known early L dwarfs using aperture masking interferometry with Palomar laser guide star adaptive optics (LGS AO). The use of aperture masking allows the detection of close binaries, corresponding to projected physical separations of 0.6-10.0 AU for the targets of our survey. This survey achieved median contrast limits of {Delta}K {approx} 2.3 for separations between 1.2 {lambda}/D-4{lambda}/D and {Delta}K {approx} 1.4 at 2/3 {lambda}/D. We present four candidate binaries detected with moderate-to-high confidence (90%-98%). Two have projected physical separations less than 1.5 AU. This may indicate that tight-separation binaries contribute more significantly to the binary fraction than currently assumed, consistent with spectroscopic and photometric overluminosity studies. Ten targets of this survey have previously been observed with the Hubble Space Telescope as part of companion searches. We use the increased resolution of aperture masking to search for close or dim companions that would be obscured by full aperture imaging, finding two candidate binaries. This survey is the first application of aperture masking with LGS AO at Palomar. Several new techniques for the analysis of aperture masking data in the low signal-to-noise regime are explored.

  16. Training and Reading Level

    E-Print Network [OSTI]

    Bishop, D. l.

    1982-01-01T23:59:59.000Z

    In preparing training materials, we often assume that the personnel for whom we are preparing the materials have a working knowledge of what we are teaching them. This is not often true (regardless of what we would like to think). In fact, they may...

  17. Making Training Effective

    E-Print Network [OSTI]

    Bishop, D. L.

    1980-01-01T23:59:59.000Z

    Several years ago, a training session was being held at an electric generating plant in the Midwest. One of the subjects covered in the session was steamline drain traps. One of the trainees checked several of the steam traps when he went back...

  18. Federal Employee Training

    Broader source: Directives, Delegations, and Requirements [Office of Management (MA)]

    2011-07-06T23:59:59.000Z

    This Order establishes requirements and responsibilities for DOE Federal employee training in accordance with Chapter 41 of Title 5, United States Code (U.S.C.). Cancels DOE O 360.1B and DOE M 360.1-1B.

  19. Athletic Training 2013-14 Name: ______________________________________________________________________

    E-Print Network [OSTI]

    Boyce, Richard L.

    Curriculum Athletic Training 2013-14 Name ______________ ______________ __________________ Pre-Athletic Training F Sp ATP 280 ______________ ______________ __________________ Basic Recognition ______________ ______________ __________________ Counseling Psychology F Sp PSY 405 ______________ ______________ __________________ Athletic Training Courses

  20. Behavioral and Neural Effects of Reasoning Training

    E-Print Network [OSTI]

    Mackey, Allyson

    2012-01-01T23:59:59.000Z

    et al. (2010). Putting brain training to the test. Nature. PE. , et al. (2007). Training-induced functional activationin children with abacus training. Human Brain Mapping, 32,

  1. Medical students' perspectives on clinical empathy training.

    E-Print Network [OSTI]

    Afghani, Behnoosh; Besimanto, Shabnam; Amin, Alpesh; Shapiro, Johanna

    2011-01-01T23:59:59.000Z

    on Clinical Empathy Training B Afghani 1 , S Besimanto 2 , Aon Clinical Empathy Training Education for Health, Volumethe barriers to empathy training from the perspective of

  2. Workforce Development Training Program (South Dakota)

    Broader source: Energy.gov [DOE]

    The Workforce Development Training Program funds industry-education partnerships through which customized training programs and short-term, job-specific training is delivered. The Workforce...

  3. Renewable Energy Training | Department of Energy

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

    Training Renewable Energy Training Federal Energy Management Program (FEMP) training is available on demand to help Federal agencies understand and meet Federal energy management...

  4. DEPARTMENT OF ENERGY Privacy Awareness Training | Department...

    Energy Savers [EERE]

    DEPARTMENT OF ENERGY Privacy Awareness Training DEPARTMENT OF ENERGY Privacy Awareness Training DEPARTMENT OF ENERGY Privacy Awareness Training DEPARTMENT OF ENERGY Privacy...

  5. Electric vehicle drive train with rollback detection and compensation

    DOE Patents [OSTI]

    Konrad, Charles E. (Roanoke, VA)

    1994-01-01T23:59:59.000Z

    An electric vehicle drive train includes a controller for detecting and compensating for vehicle rollback, as when the vehicle is started upward on an incline. The vehicle includes an electric motor rotatable in opposite directions corresponding to opposite directions of vehicle movement. A gear selector permits the driver to select an intended or desired direction of vehicle movement. If a speed and rotational sensor associated with the motor indicates vehicle movement opposite to the intended direction of vehicle movement, the motor is driven to a torque output magnitude as a nonconstant function of the rollback speed to counteract the vehicle rollback. The torque function may be either a linear function of speed or a function of the speed squared.

  6. Electric vehicle drive train with rollback detection and compensation

    DOE Patents [OSTI]

    Konrad, C.E.

    1994-12-27T23:59:59.000Z

    An electric vehicle drive train includes a controller for detecting and compensating for vehicle rollback, as when the vehicle is started upward on an incline. The vehicle includes an electric motor rotatable in opposite directions corresponding to opposite directions of vehicle movement. A gear selector permits the driver to select an intended or desired direction of vehicle movement. If a speed and rotational sensor associated with the motor indicates vehicle movement opposite to the intended direction of vehicle movement, the motor is driven to a torque output magnitude as a nonconstant function of the rollback speed to counteract the vehicle rollback. The torque function may be either a linear function of speed or a function of the speed squared. 6 figures.

  7. Sandia Energy - Education and Training

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

    Security for Electric Infrastructure National Supervisory Control and Data Acquisition (SCADA) Education and Training Education and TrainingTara Camacho-Lopez2015-05-11T18:41:05+00...

  8. Job Training Assistance Programs (Tennessee)

    Broader source: Energy.gov [DOE]

    The Job Training Assistance Programs in Tennessee are a combination of three programs: The FastTrack Job Training Assistance Program (FJTAP), The Tennessee Job Skills Program (TJS), and The Job...

  9. Sliding Mode Pulsed Averaging IC Drivers for High Brightness Light Emitting Diodes

    SciTech Connect (OSTI)

    Dr. Anatoly Shteynberg, PhD

    2006-08-17T23:59:59.000Z

    This project developed new Light Emitting Diode (LED) driver ICs associated with specific (uniquely operated) switching power supplies that optimize performance for High Brightness LEDs (HB-LEDs). The drivers utilize a digital control core with a newly developed nonlinear, hysteretic/sliding mode controller with mixed-signal processing. The drivers are flexible enough to allow both traditional microprocessor interface as well as other options such as “on the fly” adjustment of color and brightness. Some other unique features of the newly developed drivers include • AC Power Factor Correction; • High power efficiency; • Substantially fewer external components should be required, leading to substantial reduction of Bill of Materials (BOM). Thus, the LED drivers developed in this research : optimize LED performance by increasing power efficiency and power factor. Perhaps more remarkably, the LED drivers provide this improved performance at substantially reduced costs compared to the present LED power electronic driver circuits. Since one of the barriers to market penetration for HB-LEDs (in particular “white” light LEDs) is cost/lumen, this research makes important contributions in helping the advancement of SSL consumer acceptance and usage.

  10. CSAT Role-Based/Core Competency Training Program | Department...

    Energy Savers [EERE]

    Services Training Cybersecurity Training Warehouse DOE Training & Education CSAT Role-BasedCore Competency Training Program CSAT Role-BasedCore Competency Training...

  11. Sandia Energy - SCADA Training Courses

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

    Training Courses Home Stationary Power Safety, Security & Resilience of Energy Infrastructure Grid Modernization Cyber Security for Electric Infrastructure National Supervisory...

  12. Training for hazardous waste workers

    SciTech Connect (OSTI)

    Favel, K.

    1990-10-26T23:59:59.000Z

    This implementation plan describes the system and provides the information and schedules that are necessary to comply with the Department of Energy (DOE) Albuquerque Operations Office (AL) Memorandum, Reference EPD dated September 11, 1990, Training for Hazardous Waste Workers. The memo establishes the need for identifying employees requiring environmental training, ensuring that the training is received, and meeting documentation and recordkeeping requirements for the training.

  13. QU Car: a very high luminosity nova-like binary with a carbon-enriched companion

    E-Print Network [OSTI]

    J. E. Drew; L. E. Hartley; K. S. Long; J. van der Walt

    2002-09-16T23:59:59.000Z

    QU Car is listed in cataclysmic variable star catalogues as a nova-like variable. This little-studied, yet bright interacting binary is re-appraised here in the light of new high-quality ultraviolet (UV) interstellar line data obtained with STIS on board the Hubble Space Telescope. The detection of a component of interstellar absorption at a mean LSR velocity of $-$14 km s$^{-1}$ indicates that the distance to QU Car may be $\\sim$2 kpc or more -- a considerable increase on the previous lower-limiting distance of 500 pc. If so, the bolometric luminosity of QU Car could exceed $10^{37}$ ergs s$^{-1}$. This would place this binary in the luminosity domain occupied by known compact-binary supersoft X-ray sources. Even at a 500 pc, QU Car appears to be the most luminous nova-like variable known. New intermediate dispersion optical spectroscopy of QU Car spanning 3800--7000 \\AA is presented. These data yield the discovery that C{\\sc iv} $\\lambda\\lambda$5801,12 is present as an unusually prominent emission line in an otherwise low-contrast line spectrum. Using measurements of this and other lines in a recombination line analysis, it is shown that the C/He abundance as proxied by the n(C$^{4+}$)/n(He$^{2+}$) ratio may be as high as 0.06 (an order of magnitude higher than the solar ratio). Furthermore, the C/O abundance ratio is estimated to be greater than 1. These findings suggest that the companion in QU Car is a carbon star. If so, it would be the first example of a carbon star in such a binary. An early-type R star best matches the required abundance pattern and could escape detection at optical wavelengths provided the distance to QU Car is $\\sim$2 kpc or more.

  14. Rights of Way Pesticide Training

    E-Print Network [OSTI]

    Ishida, Yuko

    Rights of Way Pesticide Training This class will provide informa on for people doing Rights of Way than 5 business days prior to training by 5:00PM. LATE CANCELLATIONS = NO REFUNDS ~ NO CREDITS ~ NO ROLLING FORWARD ~ NO EXCEPTIONS. The SBE Training Center reserves the right to cancel class due to low

  15. Spring 2014 Organization Development & Training

    E-Print Network [OSTI]

    Wu, Shin-Tson

    Spring 2014 Organization Development & Training Catalog University of Central Florida Office of Organization Development & Training 3280 Progress Drive Orlando, FL 32826-2912 (407) 823-0440 February 7, 2014 Volume 2, Number 3 The current Catalog is published at http://www.hr.ucf.edu/web/training

  16. 3, 285297, 2006 Optimising training

    E-Print Network [OSTI]

    Paris-Sud XI, Université de

    HESSD 3, 285­297, 2006 Optimising training data for ANNs with Genetic Algorithms R. G. Kamp and H and Earth System Sciences Optimising training data for ANNs with Genetic Algorithms R. G. Kamp 1,2 and H. H­297, 2006 Optimising training data for ANNs with Genetic Algorithms R. G. Kamp and H. H. G. Savenije Title

  17. _____________________________ Environment, Health, & Safety _________ __________________ Training Program

    E-Print Network [OSTI]

    Eisen, Michael

    _________ __________________ Training Program EHS 359 Lockout/Tagout Practical Training Course Syllabus Subject Category: Electrical Safety Course Prerequisite: EHS0358 Lockout/Tagout Verification Course Length: 4 hours Medical Approval is designed to provide employees with hands on training on Lockout/Tagout responsibilities, acceptable

  18. _____________________________ Environment, Health, & Safety _________ __________________ Training Program

    E-Print Network [OSTI]

    Lee, Jason R.

    _________ __________________ Training Program EHS 379 Subcontractors Lockout/Tagout Orientation Course Syllabus Subject Category work involving lockout/tagout. The training explains the subcontractor LBNL Lockout/Tagout process so this training, participants will be able to: · Recall the purpose of lockout/tagout · Identify conditions

  19. IMMIGRANT LEADERSHIP TRAINING Juliette Steadman

    E-Print Network [OSTI]

    de Lijser, Peter

    IMMIGRANT LEADERSHIP TRAINING CURRICULUM by Eric Cohen Juliette Steadman and Rufus Whitley 2000 94103 #12;IMMIGRANT LEADERSHIP TRAINING CURRICULUM by Eric Cohen Juliette Steadman Rufus Whitley of the Missionary Oblates of Mary Immaculate. #12;#12;#12;UPDATE TO THE IMMIGRANT LEADERSHIP TRAINING CURRICULUM

  20. CLEAN ENERGY WORKFORCE TRAINING PROGRAM

    E-Print Network [OSTI]

    #12;CLEAN ENERGY WORKFORCE TRAINING PROGRAM $90 million Multi-agency initiative to: Identify clean energy workforce needs Build regional capacity in clean energy sector development Deliver industry relevant training for displaced workers and new workforce entrants #12;CLEAN ENERGY WORKFORCE TRAINING

  1. NIH Extramural Research Training Programs

    E-Print Network [OSTI]

    Grishok, Alla

    1 NIH Extramural Research Training Programs Rodney Ulane, Ph.D. NIH Research Training Officer;2 Predoctoral Individual NRSA (F31) Predoctoral Individual MD/PhD NRSA (F30) Postdoctoral Institutional Training Grant (T32) Postdoctoral Individual NRSA (F32) Small Grant (R03) Research Project Grant (R01

  2. APPLICATION OF A DAMPED LOCALLY OPTIMIZED COMBINATION OF IMAGES METHOD TO THE SPECTRAL CHARACTERIZATION OF FAINT COMPANIONS USING AN INTEGRAL FIELD SPECTROGRAPH

    SciTech Connect (OSTI)

    Pueyo, Laurent [Department of Physics and Astronomy, Johns Hopkins University, 366 Bloomberg Center, 3400 N. Charles Street, Baltimore, MD 21218 (United States); Crepp, Justin R.; Hinkley, Sasha; Hillenbrand, Lynne; Dekany, Richard; Bouchez, Antonin; Roberts, Jenny [California Institute of Technology, 1200 E. California Blvd., Pasadena, CA 91125 (United States); Vasisht, Gautam; Roberts, Lewis C.; Shao, Mike; Burruss, Rick [Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, CA 91109 (United States); Brenner, Douglas; Oppenheimer, Ben R.; Zimmerman, Neil [American Museum of Natural History, Central Park West at 79th Street, New York, NY 10024 (United States); Parry, Ian [Institute of Astronomy, University of Cambridge, Madingley Rd., Cambridge, CB3 0HA (United Kingdom); Beichman, Charles [NASA Exoplanet Science Institute, 770 S. Wilson Avenue, Pasadena, CA 91225 (United States); Soummer, Remi, E-mail: lap@pha.jhu.edu [Space Telescope Science Institute, 3700 San Marin Drive, Baltimore, MD 21218 (United States)

    2012-03-01T23:59:59.000Z

    High-contrast imaging instruments are now being equipped with integral field spectrographs (IFSs) to facilitate the detection and characterization of faint substellar companions. Algorithms currently envisioned to handle IFS data, such as the Locally Optimized Combination of Images (LOCI) algorithm, rely on aggressive point-spread function (PSF) subtraction, which is ideal for initially identifying companions but results in significantly biased photometry and spectroscopy owing to unwanted mixing with residual starlight. This spectrophotometric issue is further complicated by the fact that algorithmic color response is a function of the companion's spectrum, making it difficult to calibrate the effects of the reduction without using iterations involving a series of injected synthetic companions. In this paper, we introduce a new PSF calibration method, which we call 'damped LOCI', that seeks to alleviate these concerns. By modifying the cost function that determines the weighting coefficients used to construct PSF reference images, and also forcing those coefficients to be positive, it is possible to extract companion spectra with a precision that is set by calibration of the instrument response and transmission of the atmosphere, and not by post-processing. We demonstrate the utility of this approach using on-sky data obtained with the Project 1640 IFS at Palomar. Damped LOCI does not require any iterations on the underlying spectral type of the companion, nor does it rely on priors involving the chromatic and statistical properties of speckles. It is a general technique that can readily be applied to other current and planned instruments that employ IFSs.

  3. BANYAN. VI. Discovery of a companion at the brown dwarf/planet-mass limit to a Tucana-Horologium M dwarf

    E-Print Network [OSTI]

    Artigau, Étienne; Faherty, Jacqueline; Malo, Lison; Naud, Marie-Eve; Doyon, René; Lafrenière, David; Beletsky, Yuri

    2015-01-01T23:59:59.000Z

    We report the discovery of a substellar companion to 2MASS J02192210-3925225, a young M6 $\\gamma$ candidate member of the Tucana-Horologium association (30 - 40 Myr). This L4 $\\gamma$ companion has been discovered with seeing-limited direct imaging observations; at a 4" separation (160AU) and a modest contrast ratio, it joins the very short list of young low-mass companions amenable to study without the aid of adaptive optics, enabling its characterization with a much wider suite of instruments than is possible for companions uncovered by high-contrast imaging surveys. With a model-dependent mass of 12-15MJup, it straddles the boundary between the planet and brown dwarf mass regimes. We present near-infrared spectroscopy of this companion and compare it to various similar objects uncovered in the last few years. The J0219-3925 system falls in a sparsely populated part of the host mass versus mass ratio diagram for binaries; the dearth of known similar companions may be due to observational biases in previous ...

  4. Mid Career Training of Indian Forest Service Officers: International Training Program

    E-Print Network [OSTI]

    Phase III Mid Career Training of Indian Forest Service Officers: International Training Program and Training #12;Acknowledgments The Indian Forest Service Officer Training program coordinators at Colorado University Center for Protected Area Management and Training · Colorado State University Warner College

  5. Training & Technology Solutions Queens College ~ Office of Converging Technologies ~ Training & Technology Solutions

    E-Print Network [OSTI]

    Johnson Jr.,, Ray

    Training & Technology Solutions Queens College ~ Office of Converging Technologies ~ Training & Technology Solutions 718-997-4875 ~ training@qc.cuny.edu ~ I-Bldg 214 Advisor Center Navigation: Login #12;Training & Technology Solutions Queens College ~ Office of Converging Technologies ~ Training

  6. Information Technology Security Training Requirements Appendix E --Training Cross Reference E-1

    E-Print Network [OSTI]

    Information Technology Security Training Requirements APPENDIX E Appendix E -- Training Cross Reference E-1 #12;Information Technology Security Training Requirements Appendix E -- Training Cross Reference E-2 #12;Information Technology Security Training Requirements APPENDIX E -- JOB FUNCTION

  7. __________________________________ Environment, Health, & Safety ________________________________ Training Program

    E-Print Network [OSTI]

    Eisen, Michael

    commercial drivers license endorsement to transport radioactive or hazardous waste. Course Objectives: After to transport Radioactive materials to an offsite location. Recall who is allowed to prepare and package radioactive materials for delivery to an offsite locations Select an appropriate vehicle for transporting

  8. Athletic Training Admissions Procedures Truman State University

    E-Print Network [OSTI]

    Gering, Jon C.

    Athletic Training Admissions Procedures Truman State University Admission to the athletic training major is competitive and selective. Students interested in majoring in athletic training must complete Athletic Training as their major area of study on the University's application for admission

  9. Factors Involved in Search Dog Training

    E-Print Network [OSTI]

    Alexander, Michael B.

    2010-07-14T23:59:59.000Z

    involved in training competent search dogs. Obedience training methods, age training was initiated, previous handler canine training experience, and handler perception and emotional attachment to their search dog were examined through a sixty-six question...

  10. Human Resources Organizational Development and Training 1

    E-Print Network [OSTI]

    Dennett, Daniel

    Human Resources Organizational Development and Training 1 Development Guide for Tufts Leadership Competencies Human Resources Training, Learning and Development Copyright © 2013 Tufts University Developed with Copperbeech Group Inc. #12;Human Resources Training, Learning and Development 2 #12;Human Resources Training

  11. Physics at an upgraded proton driver at Fermilab

    SciTech Connect (OSTI)

    Steve Geer

    2004-07-28T23:59:59.000Z

    The accelerator-based particle physics program in the US is entering a period of transition. This is particularly true at Fermilab which for more than two decades has been the home of the Tevatron Proton-Antiproton Collider, the World's highest energy hadron collider. In a few years time the energy frontier will move to the LHC at CERN. Hence, if an accelerator-based program is to survive at Fermilab, it must evolve. Fermilab is fortunate in that, in addition to hosting the Tevatron Collider, the laboratory also hosts the US accelerator-based neutrino program. The recent discovery that neutrino flavors oscillate has opened a new exciting world for us to explore, and has created an opportunity for the Fermilab accelerator complex to continue to address the cutting-edge questions of particle physics beyond the Tevatron Collider era. The presently foreseen neutrino oscillation experiments at Fermilab (MiniBooNE [1] and MINOS [2]) will enable the laboratory to begin contributing to the Global oscillation physics program in the near future, and will help us better understand the basic parameters describing the oscillations. However, this is only a first step. To be able to pin down all of the oscillation parameters, and hopefully make new discoveries along the way, we will need high statistics experiments, which will require a very intense neutrino beam, and one or more very massive detectors. In particular we will require new MW-scale primary proton beams and perhaps ultimately a Neutrino Factory [3]. Plans to upgrade the Fermilab Proton Driver are presently being developed [4]. The upgrade project would replace the Fermilab Booster with a new 8 GeV accelerator with 0.5-2 MW beam power, a factor of 15-60 more than the current Booster. It would also make the modifications needed to the Fermilab Main Injector (MI) to upgrade it to simultaneously provide 120 GeV beams of 2 MW. This would enable a factor of 5-10 increase in neutrino beam intensities at the MI, while also supporting a vigorous 8 GeV fixed-target program. In addition, a Proton Driver might also serve as a stepping-stone to future accelerators, both as an R&D test bed and as an injector, with connections to the Linear Collider, Neutrino Factories, and a VLHC. Hence, although neutrino physics would provide the main thrust for the science program at an upgraded Fermilab proton source, the new facility would also offer exciting opportunities for other fixed-target particle physics (kaons, muons, neutrons, antiprotons, etc.) and a path towards new accelerators in the future.

  12. MFRC Training Development & Delivery Program - Bloodstain & Toxicology...

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

    MFRC Training Development & Delivery Program - Bloodstain & Toxicology DESCRIPTION: The Midwest Forensics Resource Center (MFRC) Training Development and Delivery Program increases...

  13. Training For Radiation Emergencies, First Responder Operations...

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

    Training For Radiation Emergencies, First Responder Operations - Instructors Guide Training For Radiation Emergencies, First Responder Operations - Instructors Guide COURSE...

  14. Tribal Leader Training Session: NCAI Conference | Department...

    Energy Savers [EERE]

    Training Session: NCAI Conference Tribal Leader Training Session: NCAI Conference 111101NCAIpresentationfinal.pdf More Documents & Publications Key Renewable Energy...

  15. eRA Training Team1 Terminations

    E-Print Network [OSTI]

    Baker, Chris I.

    eRA Training Team1 xTrain Terminations Electronic Research Administration Sponsored by: The National Institutions of Health, Office of Extramural Research April 2010 #12;eRA Training Team2 xTrain General Information xTrain Overview The following section provides general information on the xTrain

  16. eRA Training Team1 Terminations

    E-Print Network [OSTI]

    Baker, Chris I.

    eRA Training Team1 xTrain Terminations Electronic Research Administration Sponsored by: The National Institutes of Health, Office of Extramural Research March 2012 #12;eRA Training Team2 xTrain General Information xTrain Overview The following section provides general information on the xTrain

  17. Dynamic analysis of policy drivers for bioenergy commodity markets

    SciTech Connect (OSTI)

    Robert F. Jeffers; Jacob J. Jacobson; Erin M. Searcy

    2001-01-01T23:59:59.000Z

    Biomass is increasingly being considered as a feedstock to provide a clean and renewable source of energy in the form of both liquid fuels and electric power. In the United States, the biofuels and biopower industries are regulated by different policies and have different drivers which impact the maximum price the industries are willing to pay for biomass. This article describes a dynamic computer simulation model that analyzes future behavior of bioenergy feedstock markets given policy and technical options. The model simulates the long-term dynamics of these markets by treating advanced biomass feedstocks as a commodity and projecting the total demand of each industry as well as the market price over time. The model is used for an analysis of the United States bioenergy feedstock market that projects supply, demand, and market price given three independent buyers: domestic biopower, domestic biofuels, and foreign exports. With base-case assumptions, the biofuels industry is able to dominate the market and meet the federal Renewable Fuel Standard (RFS) targets for advanced biofuels. Further analyses suggest that United States bioenergy studies should include estimates of export demand in their projections, and that GHG-limiting policy would partially shield both industries from exporter dominance.

  18. Temperature as a driver for the expansion of the microalga Gonyostomum semen in Swedish lakes

    E-Print Network [OSTI]

    Temperature as a driver for the expansion of the microalga Gonyostomum semen in Swedish lakes Karin is an example of invasive harmful microalgae (Neilan et al., 2003). Another presumably invasive species

  19. Fourth Annual Ethical Leadership Conference Panel Drivers, Challenges, and Strategies for Future of Corporate

    E-Print Network [OSTI]

    Lin, Xiaodong

    Fourth Annual Ethical Leadership Conference Panel Drivers, Challenges, and Strategies for Future, Academy of Management Review, Academy of Management Perspectives, Business & Society, Long Range Planning Social Responsibility for Hess Corporation, a global integrated energy company based in New York City

  20. Summary of sessions B and F: High intensity linacs and frontend & proton drivers

    SciTech Connect (OSTI)

    Ferdinand, R.; /Saclay; Chou, W.; /Fermilab; Galambos, J.; /Oak Ridge

    2005-01-01T23:59:59.000Z

    This paper summarizes the sessions B&F of the 33rd ICFA Advanced Beam Dynamics Workshop on High Intensity & High Brightness Hadron Beams held in Bensheim, Germany. It covers high intensity linacs, front ends and proton driver topics.

  1. The physics issues that determine inertial confinement fusion target gain and driver requirements: A tutorial*

    E-Print Network [OSTI]

    with simple models for hohlraum wall energy loss to predict coupling efficiencies and a simple one into running the driver. More- over, the unrecycled portion of energy produced must be sufficient to sell

  2. Vehicle Technologies Office Merit Review 2014: Look-Ahead Driver Feedback and Powertrain Management

    Broader source: Energy.gov [DOE]

    Presentation given by Eaton at 2014 DOE Hydrogen and Fuel Cells Program and Vehicle Technologies Office Annual Merit Review and Peer Evaluation Meeting about look-ahead driver feedback and...

  3. active-load laser driver: Topics by E-print Network

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

    Summary: BGD 9, 14437-14473, 2012 Soil carbon drivers and benchmarks in Earth system models K. E. O. Todd if available. Causes of variation in soil carbon predictions from...

  4. Age and cross-cultural comparison of drivers' cognitive workload and performance in simulated urban driving

    E-Print Network [OSTI]

    Son, J.

    Driving demands significant psychomotor attention and requires even more when drivers are engaged in secondary tasks that increase cognitive workload and divert attention. It is well established that age influences driving ...

  5. A review of "The Cambridge Companion to Velázquez." by Suzanne L. Stratton-Pruitt, ed.

    E-Print Network [OSTI]

    Tanya J. Tiffany

    2003-01-01T23:59:59.000Z

    ?zquez?s oeuvre in concert with the artistic practices and traditions of his time. In an excellent discussion of artists? training in Spain, Zahira V?liz examines Vel?zquez?s apprenticeship in the studio of the eru- dite painter, Francisco Pacheco, and analyzes..., and analyzes how the pious reputations of beatas and other holy women served as justifications for their proposed correctives to the monarchies? policies. Sara T. Nalle then provides a useful synopsis of religious beliefs and practices in Vel?zquez?s Spain...

  6. Adaptacin de un driver WLAN Linux a una arquitectura NIOS-Avalon

    E-Print Network [OSTI]

    Autònoma de Barcelona, Universitat

    Adaptación de un driver WLAN Linux a una arquitectura NIOS-Avalon B. Martínez , I. Tarruella, D de un driver Linux se realiza un mapeo sobre una arquitectura basada en un procesador integrado dentro de un SoC. La elección de la partición Hw/Sw y de ciertos parámetros de la arquitectura se

  7. Review of a Spoke-Cavity Design Option for the RIA Driver Linac

    SciTech Connect (OSTI)

    Petr Ostroumov; Kenneth Shepard; Jean Delayen

    2005-05-16T23:59:59.000Z

    A design option for the 1.4 GV, multiple-charge-state driver linac required for the U. S. Rare Isotope Accelerator Project based on 345 MHz, 3-cell spoke-loaded cavities has been previously discussed [1]. This paper updates consideration of design options for the RIA driver, including recent results from numerically-modeling the multi-charge-state beam dynamics and also cold test results for prototype superconducting niobium 3-cell spoke-loaded cavities.

  8. NUG 2014 Training Presentations

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level: National5Sales for4,645U.S. DOE Office of Science (SC)Integrated CodesTransparency VisitSilver Toyota PriusNSR Key NumberGettingTraining

  9. NUG Training 2012

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level: National5Sales for4,645U.S. DOE Office of Science (SC)Integrated CodesTransparency VisitSilver Toyota PriusNSR KeyNUG 2015 NUG Training 2012

  10. Complete Safety Training

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level: National5Sales for4,645 3,625govInstrumentstdmadapInactiveVisiting theCommercialization and Innovation2010 2010AboutComplete Safety Training

  11. DVU Training News Form

    Office of Environmental Management (EM)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level: National5Sales for4,645 3,625 1,006 492 742 33 1112011AT&T,Office of Policy, OAPMMilestone | DepartmentEA Featured Training &

  12. ORISE: Training and Tools

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level: National5Sales for4,645U.S. DOE Office of Science (SC)Integrated CodesTransparencyDOENurseResourcesThe Value of IndependenceTraining and

  13. Training | Department of Energy

    Office of Environmental Management (EM)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level: National5Sales for4,645 3,625 1,006 492 742 33Frequently AskedEnergyIssuesEnergy SolarRadioactiveI DisposalFiveTrainingEnergy

  14. Training Worksheet Job Aid

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level: National5Sales for4,645U.S. DOE Office of ScienceandMesa del SolStrengthening a solidSynthesisAppliances » TopToursTraining Worksheet Job Aid

  15. DRIVERS OF H I TURBULENCE IN DWARF GALAXIES

    SciTech Connect (OSTI)

    Stilp, Adrienne M.; Dalcanton, Julianne J. [Department of Astronomy, University of Washington, Box 351580, Seattle, WA 98195 (United States); Skillman, Evan [Minnesota Institute for Astrophysics, University of Minnesota, 116 Church Street SE, Minneapolis, MN 55455 (United States); Warren, Steven R. [Department of Astronomy, University of Maryland, CSS Building, Room 1024, Stadium Drive, College Park, MD 20742-2421 (United States); Ott, Juergen [National Radio Astronomy Observatory, P.O. Box O, 1003 Lopezville Road, Socorro, NM 87801 (United States); Koribalski, Baerbel [Australia Telescope National Facility, CSIRO Astronomy and Space Science, P.O. Box 76, Epping, NSW 1710 (Australia)

    2013-08-20T23:59:59.000Z

    Neutral hydrogen (H I) velocity dispersions are believed to be set by turbulence in the interstellar medium (ISM). Although turbulence is widely believed to be driven by star formation, recent studies have shown that this driving mechanism may not be dominant in regions of low star formation surface density ({Sigma}{sub SFR}), such those as found in dwarf galaxies or the outer regions of spirals. We have generated average H I line profiles in a number of nearby dwarfs and low-mass spirals by co-adding H I spectra in subregions with either a common radius or {Sigma}{sub SFR}. We find that the individual spatially resolved ''superprofiles'' are composed of a central narrow peak ({approx}5-15 km s{sup -1}) with higher velocity wings to either side, similar to their global counterparts as calculated for the galaxy as a whole. Under the assumption that the central peak reflects the H I turbulent velocity dispersion, we compare measures of H I kinematics determined from the superprofiles to local ISM properties, including surface mass densities and measures of star formation. The shape of the wings of the superprofiles do not show any correlation with local ISM properties, which indicates that they may be an intrinsic feature of H I line-of-sight spectra. On the other hand, the H I velocity dispersion is correlated most strongly with baryonic and H I surface mass density, which points toward a gravitational origin for turbulence, but it is unclear which, if any, gravitational instabilities are able to operate efficiently in these systems. Star formation energy is typically produced at a level sufficient to drive H I turbulent motions at realistic coupling efficiencies in regimes where {Sigma}{sub SFR} {approx}> 10{sup -4} M{sub Sun} yr{sup -1} kpc{sup -2}, as is typically found in inner spiral disks. At low star formation intensities, on the other hand, star formation cannot supply enough energy to drive the observed turbulence, nor does it uniquely determine the turbulent velocity dispersion. Nevertheless, even at low intensity, star formation does appear to provide a lower threshold for H I velocity dispersions. We find a pronounced decrease in coupling efficiency with increasing {Sigma}{sub SFR}, which would be consistent with a picture where star formation couples to the ISM with constant efficiency, but that less of that energy is found in the neutral phase at higher {Sigma}{sub SFR}. We have examined a number of potential drivers of H I turbulence, including star formation, gravitational instabilities, the magneto-rotational instability, and accretion-driven turbulence, and found that, individually, none of these drivers is capable of driving the observed levels of turbulence in the low {Sigma}{sub SFR} regime. We discuss possible solutions to this conundrum.

  16. A sustainable model for training teachers to use pivotal response training

    E-Print Network [OSTI]

    Suhrheinrich, Jessica Brooke

    2010-01-01T23:59:59.000Z

    J. R. , (1995). Pyramidal staff training in the extension ofvia pivotal response training and the individualization ofof pivotal response training. Journal of Speech, Language

  17. Stockpile Dismantlement Database Training Materials

    SciTech Connect (OSTI)

    Not Available

    1993-11-01T23:59:59.000Z

    This document, the Stockpile Dismantlement Database (SDDB) training materials is designed to familiarize the user with the SDDB windowing system and the data entry steps for Component Characterization for Disposition. The foundation of information required for every part is depicted by using numbered graphic and text steps. The individual entering data is lead step by step through generic and specific examples. These training materials are intended to be supplements to individual on-the-job training.

  18. Environment, Health, & Safety Training Program

    E-Print Network [OSTI]

    Eisen, Michael

    Radiological Training (GERT) Course Syllabus Subject Category: Radiation Protection Course or facility. Participant Evaluation: No Written Exam: No Practical Exam: No Retraining

  19. Rediness Review Team Member Training

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

    MEMBER TRAINING Idaho National Engineering Laboratory Michael Hillman DOE HQ - HSS Idaho National Engineering Laboratory Dan M. Stover, PE Technical And Professional Services, Inc....

  20. Developing Alaskan Sustainable Housing Training

    Broader source: Energy.gov [DOE]

    Hosted by the Association of Alaska Housing Authorities (AAHA), this three-day training event covers strategies and technical issues related to sustainable housing development.

  1. DOCUMENTATION SPECIFIC TASK TRAINING PROGRAM

    E-Print Network [OSTI]

    Illinois at Urbana-Champaign, University of

    DOCUMENTATION APPENDIX SPECIFIC TASK TRAINING PROGRAM Conducted by the ILLINOIS CENTER ............................................................. Coordination of Contract Documents Art.105.05 Appendix Page 14

  2. A LIKELY CLOSE-IN LOW-MASS STELLAR COMPANION TO THE TRANSITIONAL DISK STAR HD 142527

    SciTech Connect (OSTI)

    Biller, Beth; Benisty, Myriam; Chauvin, Gael; Olofsson, Johan; Pott, Joerg-Uwe; Mueller, Andre; Bonnefoy, Mickaeel; Henning, Thomas [Max-Planck-Institut fuer Astronomie, Koenigstuhl 17, 69117 Heidelberg (Germany); Lacour, Sylvestre; Thebault, Philippe [LESIA, CNRS/UMR-8109, Observatoire de Paris, UPMC, Universite Paris Diderot, 5 place Jules Janssen, 92195 Meudon (France); Juhasz, Attila [Leiden Observatory, Leiden University, P.O. Box 9513, 2300 RA Leiden (Netherlands); Sicilia-Aguilar, Aurora [Departamento de Fisica Teorica, Facultad de Ciencias, Universidad Autonoma de Madrid, 28049 Cantoblanco, Madrid (Spain); Tuthill, Peter [School of Physics, University of Sydney, NSW 2006 (Australia); Crida, Aurelien, E-mail: biller@mpia.de [Universite de Nice - Sophia antipolis/C.N.R.S./Observatoire de la Cote d'Azur, Laboratoire Lagrange (UMR 7293), Boulevard de l'Observatoire, B.P. 4229 06304 NICE cedex 04 (France)

    2012-07-10T23:59:59.000Z

    With the uniquely high contrast within 0.''1 ({Delta}mag(L') = 5-6.5 mag) available using Sparse Aperture Masking with NACO at Very Large Telescope, we detected asymmetry in the flux from the Herbig Fe star HD 142527 with a barycenter emission situated at a projected separation of 88 {+-} 5 mas (12.8 {+-} 1.5 AU at 145 pc) and flux ratios in H, K, and L' of 0.016 {+-} 0.007, 0.012 {+-} 0.008, and 0.0086 {+-} 0.0011, respectively (3{sigma} errors), relative to the primary star and disk. After extensive closure-phase modeling, we interpret this detection as a close-in, low-mass stellar companion with an estimated mass of {approx}0.1-0.4 M{sub Sun }. HD 142527 has a complex disk structure, with an inner gap imaged in both the near and mid-IR as well as a spiral feature in the outer disk in the near-IR. This newly detected low-mass stellar companion may provide a critical explanation of the observed disk structure.

  3. Clinical Training Opportunities in NINDS Clinical Training Opportunities

    E-Print Network [OSTI]

    Levin, Judith G.

    Clinical Training Opportunities in NINDS #12;Clinical Training Opportunities National Institute of Neurological Disorders and Stroke (NINDS) National Institutes of Health (NIH) The NINDS intramural clinical in Basic Science Laboratories and Clinical Branches of the nineteen NIH institutes and centers. The campus

  4. Training Program Handbook: A systematic approach to training

    SciTech Connect (OSTI)

    Not Available

    1994-08-01T23:59:59.000Z

    This DOE handbook describes a systematic method for establishing and maintaining training programs that meet the requirements and expectations of DOE Orders 5480.18B and 5480.20. The systematic approach to training includes 5 phases: Analysis, design, development, implementation, and evaluation.

  5. Large Synoptic Survey Telescope: From Science Drivers to Reference Design

    SciTech Connect (OSTI)

    Ivezic, Z.; Axelrod, T.; Brandt, W.N.; Burke, D.L.; Claver, C.F.; Connolly, A.; Cook, K.H.; Gee, P.; Gilmore, D.K.; Jacoby, S.H.; Jones, R.L.; Kahn, S.M.; Kantor, J.P.; Krabbendam, V.; Lupton, R.H.; Monet, D.G.; Pinto, P.A.; Saha, A.; Schalk, T.L.; Schneider, D.P.; Strauss, Michael A.; /Washington U., Seattle, Astron. Dept. /LSST Corp. /Penn State U., Astron. Astrophys. /KIPAC, Menlo Park /NOAO, Tucson /LLNL, Livermore /UC, Davis /Princeton U., Astrophys. Sci. Dept. /Naval Observ., Flagstaff /Arizona U., Astron. Dept. - Steward Observ. /UC, Santa Cruz /Harvard U. /Johns Hopkins U. /Illinois U., Urbana

    2011-10-14T23:59:59.000Z

    In the history of astronomy, major advances in our understanding of the Universe have come from dramatic improvements in our ability to accurately measure astronomical quantities. Aided by rapid progress in information technology, current sky surveys are changing the way we view and study the Universe. Next-generation surveys will maintain this revolutionary progress. We focus here on the most ambitious survey currently planned in the visible band, the Large Synoptic Survey Telescope (LSST). LSST will have unique survey capability in the faint time domain. The LSST design is driven by four main science themes: constraining dark energy and dark matter, taking an inventory of the Solar System, exploring the transient optical sky, and mapping the Milky Way. It will be a large, wide-field ground-based system designed to obtain multiple images covering the sky that is visible from Cerro Pachon in Northern Chile. The current baseline design, with an 8.4 m (6.5 m effective) primary mirror, a 9.6 deg{sup 2} field of view, and a 3,200 Megapixel camera, will allow about 10,000 square degrees of sky to be covered using pairs of 15-second exposures in two photometric bands every three nights on average. The system is designed to yield high image quality, as well as superb astrometric and photometric accuracy. The survey area will include 30,000 deg{sup 2} with {delta} < +34.5{sup o}, and will be imaged multiple times in six bands, ugrizy, covering the wavelength range 320-1050 nm. About 90% of the observing time will be devoted to a deep-wide-fast survey mode which will observe a 20,000 deg{sup 2} region about 1000 times in the six bands during the anticipated 10 years of operation. These data will result in databases including 10 billion galaxies and a similar number of stars, and will serve the majority of science programs. The remaining 10% of the observing time will be allocated to special programs such as Very Deep and Very Fast time domain surveys. We describe how the LSST science drivers led to these choices of system parameters.

  6. Potty Training Gone Terribly Wrong

    E-Print Network [OSTI]

    Hacker, Randi; Tsutsui, William

    2006-05-31T23:59:59.000Z

    -intestinal tract," that is, "drastic toilet training". Happily, Western understanding of Japan has improved over the years and today no one would suggest that Pearl Harbor was the result of potty training gone terribly wrong. At least not in public... #ceas...

  7. _____________________________ Environment, Health, & Safety _________ __________________ Training Program

    E-Print Network [OSTI]

    Eisen, Michael

    Program EHS 369 Lockout/Tagout Practical Refresher Training for Non-Qualified Electrical Workers Course to provide employees with Lockout/Tagout responsibilities, acceptable practices, and procedures with respect within lockout tagout activities as a non-qualified electrical worker. Web Resource: EH&S Training

  8. _____________________________ Environment, Health, & Safety _________ __________________ Training Program

    E-Print Network [OSTI]

    Eisen, Michael

    _________ __________________ Training Program EHS 258 Lockout/Tagout Refresher Training Course Syllabus Subject Category: General Course Prerequisite: EHS0358 Lockout/Tagout Verification Course Length: 1 hour Medical Approval: None Delivery Mode Lockout/Tagout responsibilities, acceptable practices, and procedures with respect to safety

  9. _____________________________ Environment, Health, & Safety _________ __________________ Training Program

    E-Print Network [OSTI]

    _________ __________________ Training Program EHS 372 Lockout/Tagout Awareness for Line Managers Course Syllabus Subject Category perform Lockout/Tagout (LOTO). This training provides an awareness of the LOTO process and the different, participants will be able to: · Describe what LOTO is · Identify requirements for performing Lockout

  10. The Geant4 Visualisation System - a multi-driver graphics system

    E-Print Network [OSTI]

    John Allison; Laurent Garnier; Akinori Kimura; Joseph Perl

    2012-12-31T23:59:59.000Z

    From the beginning the Geant4 Visualisation System was designed to support several simultaneous graphics systems written to common abstract interfaces. Today it has matured into a powerful diagnostic and presentational tool. It comes with a library of models that may be added to the current scene and which include the representation of the Geant4 geometry hierarchy, simulated trajectories and user-written hits and digitisations. The workhorse is the OpenGL suite of drivers for X, Xm, Qt and Win32. There is an Open Inventor driver. Scenes can be exported in special graphics formats for offline viewing in the DAWN, VRML, HepRApp and gMocren browsers. PostScript can be generated through OpenGL, Open Inventor, DAWN and HepRApp. Geant4's own tracking algorithms are used by the Ray Tracer. Not all drivers support all features but all drivers bring added functionality of some sort. This paper describes the interfaces and details the individual drivers.

  11. Microsoft PowerPoint - IGCA Training 2011-OPAM | Department of...

    Office of Environmental Management (EM)

    - IGCA Training 2011-OPAM Microsoft PowerPoint - IGCA Training 2011-OPAM IGCA Inventory Data Collection Tool Training 2011 Microsoft PowerPoint - IGCA Training 2011-OPAM...

  12. PARS II Training Workbook (Course 103) | Department of Energy

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

    PARS II Training Workbook (Course 103) PARS II Training Workbook (Course 103) PARS II More Documents & Publications PARS II TRAINING PARS II TRAINING PARS II 104 Contractor Monthly...

  13. PIA - Savannah River Nuclear Solutions Training Records and Informatio...

    Office of Environmental Management (EM)

    Nuclear Solutions Training Records and Information Network (TRAIN) PIA - Savannah River Nuclear Solutions Training Records and Information Network (TRAIN) PIA - Savannah River...

  14. EPA Tribal Training and Outreach Support for the American Indian...

    Office of Environmental Management (EM)

    Tribal Training and Outreach Support for the American Indian Air Quality Training Program EPA Tribal Training and Outreach Support for the American Indian Air Quality Training...

  15. TRADE (Training Resources and Data Exchange): Nontechnical training programs inventory: Volume 1, Management skills training programs, Supervisory skills trainings programs

    SciTech Connect (OSTI)

    Not Available

    1986-09-01T23:59:59.000Z

    In a continuing effort to facilitate communications and resource exchange among the DOE contractors, the TRADE (Training Resources and Data Exchange) Committee has compiled the Training Programs Inventories listed below which, taken together, total over 2800 courses and reflect the range and focus of in-house training programs being offered throughout the DOE GOCO system by approximately 50 contractors. The Nontechnical Training Programs Inventories includes those programs or courses designed specifically for in-house employees and which provide development and practical information about job-related subjects not included in the technical training area. The focus of the Inventories is on targeted audiences, resources, and course design. The contact person is listed with each course.

  16. STARS Training Needs Assessment Learner Instructions 07/2009 1 STARS Training Needs Assessment

    E-Print Network [OSTI]

    Ford, James

    STARS Training Needs Assessment Learner Instructions 07/2009 1 STARS Training Needs Assessment. · Click the STARS (Training) tab. · Click My Training Needs in the left menu. · Click the secure link to continue to My Training Needs. On the Training Needs Assessment page, click the box to the left of every

  17. Co-training and Self-training for Word Sense Disambiguation Rada Mihalcea

    E-Print Network [OSTI]

    Mihalcea, Rada

    Co-training and Self-training for Word Sense Disambiguation Rada Mihalcea Department of Computer the application of co- training and self-training to word sense disam- biguation. Optimal and empirical parameter se- lection methods for co-training and self-training are investigated, with various degrees of error

  18. Large-Scale Wind Training Program

    SciTech Connect (OSTI)

    Porter, Richard L. [Hudson Valley Community College

    2013-07-01T23:59:59.000Z

    Project objective is to develop a credit-bearing wind technician program and a non-credit safety training program, train faculty, and purchase/install large wind training equipment.

  19. Job Training Tax Credit (Rhode Island)

    Broader source: Energy.gov [DOE]

    Companies who invest in training opportunities for new or existing employees may take a corporate income tax credit equal to 50% of eligible training expenditures through the Job Training Tax...

  20. Grid Parity for Residential Photovoltaics in the United States: Key Drivers and Sensitivities; Preprint

    SciTech Connect (OSTI)

    Ong, S.; Denholm, P.; Clark, N.

    2012-08-01T23:59:59.000Z

    In this report, we analyze PV break-even costs for U.S. residential customers. We evaluate some key drivers of grid parity both regionally and over time. We also examine the impact of moving from flat to time-of-use (TOU) rates, and we evaluate individual components of the break-even cost, including effect of rate structure and various incentives. Finally, we examine how PV markets might evolve on a regional basis considering the sensitivity of the break-even cost to four major drivers: technical performance, financing parameters, electricity prices and rates, and policies. We find that electricity price rather than technical parameters are in general the key drivers of the break-even cost of PV. Additionally, this analysis provides insight about the potential viability of PV markets.

  1. The ALICE analysis train system

    E-Print Network [OSTI]

    Markus Zimmermann; for the ALICE collaboration

    2015-02-23T23:59:59.000Z

    In the ALICE experiment hundreds of users are analyzing big datasets on a Grid system. High throughput and short turn-around times are achieved by a centralized system called the LEGO trains. This system combines analysis from different users in so-called analysis trains which are then executed within the same Grid jobs thereby reducing the number of times the data needs to be read from the storage systems. The centralized trains improve the performance, the usability for users and the bookkeeping in comparison to single user analysis. The train system builds upon the already existing ALICE tools, i.e. the analysis framework as well as the Grid submission and monitoring infrastructure. The entry point to the train system is a web interface which is used to configure the analysis and the desired datasets as well as to test and submit the train. Several measures have been implemented to reduce the time a train needs to finish and to increase the CPU efficiency.

  2. Athletic Training Coordinator Hometown: Colorado Springs, CO

    E-Print Network [OSTI]

    Van Stryland, Eric

    WHO WE ARE Gaby Bell Athletic Training Coordinator Hometown: Colorado Springs, CO Certifications Athletic Training Graduate Assistant Jonathan Hodapp Student Athletic Trainer Mike Carlson Student Athletic

  3. Microsoft PowerPoint - IGCA Training 2011

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

    Procurement and Assistance Management Department of Energy IGCA Inventory Data Collection Tool Training Collection Tool Training 2011 Office of Procurement and Assistance...

  4. Supervisory Training Requirements | Department of Energy

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

    Requirements The Office of Learning and Workforce Development has developed an inventory of training and developmental activities that will meet the supervisory training...

  5. BNL | CFN Operations Safety Awareness (COSA) Training

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

    CFN Operations Safety Awareness (COSA) Training All users at the CFN must complete the CFN Operations Safety Awareness (COSA) Training before they can access the facilities. COSA...

  6. TQP Qualifying Official Training Approaches - Livermore Site...

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

    TQP Qualifying Official Training Approaches - Livermore Site Office TQP Qualifying Official Training Approaches - Livermore Site Office A QO is an individual who has the technical...

  7. User Facility Training | Advanced Photon Source

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

    See Also: Argonne WBT Argonne eJHQ ACIS Training APS Beamline Shielding Argonne National Laboratory User Facility Training Core Courses: These courses require your badge number and...

  8. Voluntary Initiative on Incentives: Toolkit Training Webinar...

    Energy Savers [EERE]

    Voluntary Initiative on Incentives: Toolkit Training Webinar Voluntary Initiative on Incentives: Toolkit Training Webinar March 26, 2015 12:30PM to 2:0...

  9. Funding Opportunity Announcement: Solar Training and Education...

    Energy Savers [EERE]

    Training and Education for Professionals (STEP) Funding Opportunity Announcement: Solar Training and Education for Professionals (STEP) Funding Number: DE-FOA-0001329 Funding...

  10. RELIABILITY IMPROVEMENT OF BART TRAIN CONTROL

    E-Print Network [OSTI]

    Turner, D.B.

    2011-01-01T23:59:59.000Z

    2) of the BART Automatic Train Control System. BART 74-111,systems. The unique level of sophistication automatic train controls

  11. CarSafe: A Driver Safety App that Detects Dangerous Driving Behavior using Dual-Cameras on Smartphones

    E-Print Network [OSTI]

    Campbell, Andrew T.

    CarSafe: A Driver Safety App that Detects Dangerous Driving Behavior using Dual}@cs.dartmouth.edu ABSTRACT Driving while being tired or distracted is dangerous. We are developing the CafeSafe app on the phone to detect and alert drivers to dangerous driving conditions inside and outside the car. Car

  12. 1 Managed by UT-Battelle for the U.S. Department of Energy Global and regional drivers of

    E-Print Network [OSTI]

    1 Managed by UT-Battelle for the U.S. Department of Energy Global and regional drivers to climate change #12;2 Managed by UT-Battelle for the U.S. Department of Energy Global and regional drivers

  13. Abstract--There are two types of drivers in production machine systems: constant velocity (CV) motor and servo-motor.

    E-Print Network [OSTI]

    Zhang, WJ "Chris"

    ) motor and servo-motor. If a system contains two drivers or more, among which some are of the CV motor while the other are the servo-motor, the system has the so-called hybrid driver architecture is stable. A simulation is performed to show verify the proposed controller. The CV motor has the velocity

  14. GSC 07396-00759 = V4046 Sgr C[D]: A WIDE-SEPARATION COMPANION TO THE CLOSE T TAURI BINARY SYSTEM V4046 Sgr AB

    E-Print Network [OSTI]

    Kastner, J. H.

    We explore the possibility that GSC 07396-00759 (spectral type M1e) is a widely separated (~2[' over .]82, or projected separation ~12,350 AU) companion to the "old" (age ~12 Myr) classical T Tauri binary system V4046 Sgr ...

  15. For Release: 9:20 a.m. PST, January 9, 2007 CHANDRA X-RAY TELESCOPE DISCOVERS COMPANION TO BRIGHT STAR IN THE

    E-Print Network [OSTI]

    Cohen, David

    : Australia, Brazil, New Zealand, Papua New Guinea, and Samoa. The companion star was discovered accidentally the highly supersonic stellar winds of hot, luminous stars produce x-rays, and we were surprised to see two that of the Sun, is very luminous (giving off about 34,000 times as much energy as our Sun every second

  16. TWO PLANETARY COMPANIONS AROUND THE K7 DWARF GJ 221: A HOT SUPER-EARTH AND A CANDIDATE IN THE SUB-SATURN DESERT RANGE

    SciTech Connect (OSTI)

    Arriagada, Pamela; Minniti, Dante [Department of Astronomy, Pontificia Universidad Catolica de Chile, Casilla 306, Santiago 22 (Chile); Anglada-Escude, Guillem; Butler, R. Paul [Department of Terrestrial Magnetism, Carnegie Institution of Washington, 5241 Broad Branch Road NW, Washington, DC 20015-1305 (United States); Crane, Jeffrey D.; Shectman, Stephen A.; Thompson, Ian [The Observatories of the Carnegie Institution of Washington, 813 Santa Barbara Street, Pasadena, CA 91101 (United States); Wende, Sebastian, E-mail: parriaga@astro.puc.cl [Institut fuer Astrophysik, Universitaet Goettingen, Friedrich-Hund-Platz 1, D-37077 Goettingen (Germany)

    2013-07-01T23:59:59.000Z

    We report two low-mass companions orbiting the nearby K7 dwarf GJ 221 that have emerged from reanalyzing 4.4 yr of publicly available HARPS spectra complemented with 2 years of high-precision Doppler measurements with Magellan/PFS. The HARPS measurements alone contain the clear signal of a low-mass companion with a period of 125 days and a minimum mass of 53.2 M{sub Circled-Plus} (GJ 221b), falling in a mass range where very few planet candidates have been found (sub-Saturn desert). The addition of 17 PFS observations allows the confident detection of a second low-mass companion (6.5 M{sub Circled-Plus }) in a hot orbit (3.87 day period, GJ 221c). Spectroscopic and photometric calibrations suggest that GJ 221 is slightly depleted ([Fe/H] {approx} -0.1) compared to the Sun, so the presence of two low-mass companions in the system confirms the trend that slightly reduced stellar metallicity does not prevent the formation of planets in the super-Earth to sub-Saturn mass regime.

  17. The CORALIE survey for southern extra-solar planets VII. Two short-period Saturnian companions to HD108147 and HD168746

    E-Print Network [OSTI]

    F. Pepe; M. Mayor; F. Galland; D. Naef; D. Queloz; N. C. Santos; S. Udry; M. Burnet

    2002-03-26T23:59:59.000Z

    We present the discovery of two Saturn-mass companions to HD108147 and HD168746. Both belong to the lightest ever discovered planets. The minimum mass of the companion to HD168746 is of only 0.77 the mass of Saturn and its orbital period is 6.4 days. The companion to HD108147 orbits its parent star in 10.9 days and its minimum mass is 1.34 that of Saturn. Its orbit is characterized by a high eccentricity, e=0.50, indicating possibly the presence of a second companion. The detection of Saturn-mass planets by means of the Doppler technique demands high radial-velocity measurement precision. The two new candidates were discovered by means of the CORALIE echelle spectrograph. The instrumental accuracy of CORALIE combined with the simultaneous ThAr-reference technique has reached a level better than 3m/s. On many observed objects the precision is now limited by photon noise. We present in this paper the weighted cross-correlation technique, which leads to an improvement in the photon noise of the computed radial velocity. We discuss as well a modification of the numerical cross-correlation mask which reduces significantly the residual perturbation effects produced by telluric absorption lines.

  18. Characterization of Low-mass, Wide-separation Substellar Companions to Stars in Upper Scorpius: Near-infrared Photometry and Spectroscopy

    E-Print Network [OSTI]

    Lachapelle, François-René; Gagné, Jonathan; Jayawardhana, Ray; Janson, Markus; Helling, Christiane; Witte, Soeren

    2015-01-01T23:59:59.000Z

    We present new 0.9-2.45 $\\mu$m spectroscopy ($R \\sim 1000$), and $Y$, $J$, $H$, $K_s$, $L^\\prime$ photometry, obtained at Gemini North, of three low-mass brown dwarf companions on wide orbits around young stars of the Upper Scorpius OB association: HIP 78530 B, [PGZ2001] J161031.9-191305 B, and GSC 06214-00210 B. We use these data to assess the companions' spectral type, temperature, surface gravity and mass, as well as the ability of the BT-Settl and Drift-Phoenix atmosphere models to reproduce the spectral features of young substellar objects. For completeness, we also analyze the archival spectroscopy and photometry of the Upper Scorpius planetary mass companion 1RXS J160929.1-210524 b. Based on a comparison with model spectra we find that the companions, in the above order, have effective temperatures of 2700, 2500, 2300 and 1700 K. These temperatures are consistent with our inferred spectral types, respectively M7 $\\beta$, M9 $\\gamma$, M9 $\\gamma$, and L4 $\\gamma$. From bolometric luminosities estimated ...

  19. Mon. Not. R. Astron. Soc. 402, 26092616 (2010) doi:10.1111/j.1365-2966.2009.16085.x Radio emissions from substellar companions of evolved cool stars

    E-Print Network [OSTI]

    Luttermoser, Donald G.

    2010-01-01T23:59:59.000Z

    A number of substellar companions to evolved cool stars have now been reported. Cool giants are distinct instability (CMI) mechanism. Our study leads to the following two observational prospects. First, for coronal; however, much brighter flux densities may be achievable when CMI is considered. Key words: stars: late

  20. _____________________________ Environment, Health, & Safety _________ __________________ Training Program

    E-Print Network [OSTI]

    Eisen, Michael

    _________ __________________ Training Program EHS 0368 Asbestos Class III Refresher Course Syllabus Subject Category: Occupational · Recognize the health effects associated with asbestos, and measure used to control exposure · Identify work practices and controls for incidental disturbance of asbestos containing building materials. Course

  1. Training Session: West Chester, PA

    Broader source: Energy.gov [DOE]

    This 3.5-hour training provides builders with a comprehensive review of zero net-energy-ready home construction including the business case, detailed specifications, and opportunities to be...

  2. ZERH Training: San Diego, CA

    Broader source: Energy.gov [DOE]

    This 3.5-hour training provides builders with a comprehensive review of zero energy-ready home construction including the business case, detailed specifications, and opportunities to be recognized...

  3. Plain Language Training Class 01

    Broader source: Energy.gov [DOE]

    Registration link:  CHRIS https://mis.doe.gov/ess/index.cfm   002357/0017 and https://powerpedia.energy.gov/wiki/Plain_Writing_Training_Class_October_...Course Type: Classroom   Course Location:...

  4. Stillwell Avenue Terminal Train Shed

    High Performance Buildings Database

    New York, NY Coney Island's Stillwell Avenue Terminal is the largest above-ground station in New York City's subway system. After years of deferred maintenance, the 90-year-old station was redesigned by New York City Transit's in-house design staff. The train shed's new arched-truss structure covers four platforms and eight tracks. The train shed was designed to meet demanding maintenance, durability, and operations requirements.

  5. Training For Radiation Emergencies, First Responder Operations- Course Presentation

    Broader source: Energy.gov [DOE]

    Presentation slides use in the Training For Radiation Emergencies, First Responder Operations refresher training course.

  6. Alternative systematic approaches to training

    SciTech Connect (OSTI)

    Not Available

    1995-01-01T23:59:59.000Z

    This handbook is approved for use by all DOE Components and contractors. The handbook was prepared primarily for DOE nuclear facilities, but the information can be effectively used by any other type of facility. DOE nuclear, DOE non-nuclear, commercial nuclear reactor, fuel fabrication, chemical processing, or other types of facilities may also apply the principles of this approach and find it useful and applicable to local needs. The handbook provides DOE and contractor operating organizations with concepts and guidance regarding the use of alternative techniques to implement a systematic approach to training (SAT). The techniques described in this handbook are endorsed by DOE and use of the guidance in this handbook is appropriate for establishment of technical training programs at DOE nuclear facilities. The use of guidance on selection and implementation of appropriate training approaches after consideration of job complexity, the consequences of error based on risk/hazard potential, and available training media should result in effective and efficient training programs. The information presented in this handbook can be used to grade the level of effort and formality used in developing training programs.

  7. Efficient high density train operations

    DOE Patents [OSTI]

    Gordon, Susanna P. (Oakland, CA); Evans, John A. (Hayward, CA)

    2001-01-01T23:59:59.000Z

    The present invention provides methods for preventing low train voltages and managing interference, thereby improving the efficiency, reliability, and passenger comfort associated with commuter trains. An algorithm implementing neural network technology is used to predict low voltages before they occur. Once voltages are predicted, then multiple trains can be controlled to prevent low voltage events. Further, algorithms for managing inference are presented in the present invention. Different types of interference problems are addressed in the present invention such as "Interference. During Acceleration", "Interference Near Station Stops", and "Interference During Delay Recovery." Managing such interference avoids unnecessary brake/acceleration cycles during acceleration, immediately before station stops, and after substantial delays. Algorithms are demonstrated to avoid oscillatory brake/acceleration cycles due to interference and to smooth the trajectories of closely following trains. This is achieved by maintaining sufficient following distances to avoid unnecessary braking/accelerating. These methods generate smooth train trajectories, making for a more comfortable ride, and improve train motor reliability by avoiding unnecessary mode-changes between propulsion and braking. These algorithms can also have a favorable impact on traction power system requirements and energy consumption.

  8. UA researchers develop develop a device for moving industrial vehicles without drivers

    E-Print Network [OSTI]

    Escolano, Francisco

    in settings with extreme human conditions (cold storage, waste management , etc....) The device is availableUA researchers develop develop a device for moving industrial vehicles without drivers Researchers Localization And Mapping). This technology is applicable to any business or industrial environment where

  9. Design and characterization of a signal insulation coreless transformer integrated in a CMOS gate driver chip

    E-Print Network [OSTI]

    Paris-Sud XI, Université de

    Design and characterization of a signal insulation coreless transformer integrated in a CMOS gate the implementation of numerous distinct power transistor gate drivers, the control signal insulation is becoming more results will be shown in order to validate the functionality. I. INTRODUCTION An insulation system

  10. Stochastic Behaviour of the Electricity Bid Stack: from Fundamental Drivers to Power Prices

    E-Print Network [OSTI]

    Howison, Sam

    Stochastic Behaviour of the Electricity Bid Stack: from Fundamental Drivers to Power Prices Michael@maths.ox.ac.uk (01865 280613) Sam Howison Oxford-Man Institute, University of Oxford, Blue Boar Court, 9 Alfred Street on stochastic processes for underlying factors (fuel prices, power demand and generation capacity availability

  11. Refueling Behavior of Flexible Fuel Vehicle Drivers in the Federal Fleet

    SciTech Connect (OSTI)

    Daley, R.; Nangle, J.; Boeckman, G.; Miller, M.

    2014-05-01T23:59:59.000Z

    Federal fleets are a frequent subject of legislative and executive efforts to lead a national transition to alternative fuels and advanced vehicle technologies. Section 701 of the Energy Policy Act of 2005 requires that all dual-fueled alternative fuel vehicles in the federal fleet be operated on alternative fuel 100% of the time when they have access to it. However, in Fiscal Year (FY) 2012, drivers of federal flex fuel vehicles (FFV) leased through the General Services Administration refueled with E85 24% of the time when it was available--falling well short of the mandate. The U.S. Department of Energy's National Renewable Energy Laboratory completed a 2-year Laboratory Directed Research and Development project to identify the factors that influence the refueling behavior of federal FFV drivers. The project began with two primary hypotheses. First, information scarcity increases the tendency to miss opportunities to purchase E85. Second, even with perfect information, there are limits to how far drivers will go out of their way to purchase E85. This paper discusses the results of the project, which included a June 2012 survey of federal fleet drivers and an empirical analysis of actual refueling behavior from FY 2009 to 2012. This research will aid in the design and implementation of intervention programs aimed at increasing alternative fuel use and reducing petroleum consumption.

  12. A fuel economy optimization system with applications in vehicles with human drivers and autonomous vehicles

    E-Print Network [OSTI]

    Wu, Changxu (Sean)

    A fuel economy optimization system with applications in vehicles with human drivers and autonomous University of New York, Buffalo, USA a r t i c l e i n f o Keywords: Vehicle fuel economy Eco-driving Human developed and validated a new fuel-economy optimization system (FEOS), which receives input from vehicle

  13. IMPACT OF BEAM TRANSPORT METHOD ON CHAMBER AND DRIVER DESIGN FOR

    E-Print Network [OSTI]

    IMPACT OF BEAM TRANSPORT METHOD ON CHAMBER AND DRIVER DESIGN FOR HEAVY ION INERTIAL FUSION ENERGY D propagate in thick-liquid-wall, wetted-wall, and dry-wall chambers. KEYWORDS: heavy ion fusion, ion beam transport, reactor chamber design I. INTRODUCTION The U.S. heavy ion fusion ~HIF! program is working toward

  14. DRIVER ASSISTED CONTROL STRATEGIES: THEORY AND EXPERIMENT Mark DePoorter

    E-Print Network [OSTI]

    Brennan, Sean

    performance is specified as a Reference Model. The driver maintains nominal control of the vehicle by direct actuation of the front steering inputs. The controller then determines the appropriate rear steer inputs. An appropriate vehicle model is developed and a polynomial pole placement technique is used to control

  15. Megafauna biomass tradeoff as a driver of Quaternary and future extinctions

    E-Print Network [OSTI]

    California at Berkeley, University of

    Megafauna biomass tradeoff as a driver of Quaternary and future extinctions Anthony D. Barnosky,000 and 3,000 years ago. Estimates of megafauna biomass (including hu- mans as a megafauna species) for before, during, and after the extinction episode suggest that growth of human biomass largely matched

  16. Multimodal Presentation of Local Danger Warnings for Drivers: A Situation-Dependent Assessment of Usability

    E-Print Network [OSTI]

    Theune, Mariët

    Multimodal Presentation of Local Danger Warnings for Drivers: A Situation-Dependent Assessment danger warning function. To achieve high-quality assistance, the communication mode needs to be adaptive. Moreover, regardless of communication mode, the local danger warning function was considered as the most

  17. Hydrology as a driver of biodiversity: Controls on carrying capacity, niche formation, and dispersal

    E-Print Network [OSTI]

    Konar, Megan

    Hydrology as a driver of biodiversity: Controls on carrying capacity, niche formation Centre for Hydrology, ``Dino Tonini'', Padua, Italy a r t i c l e i n f o Article history: Available online 3 March 2012 Keywords: Hydrology Biodiversity Dispersal Carrying capacity Niches Climate change

  18. 2002-21-0041 Performance Driver Information Systems, Enhancing the Fun-to-Drive Equation

    E-Print Network [OSTI]

    in automobiles today display vehicle speed, fluid levels, fluid temperatures, and some basic diagnostic information (warnings, panel lamps). Optional driver information systems add to this list by offering fuel to be very complex. Essentially, all that is required is a speedometer and a fuel gauge. The speedometer

  19. A method for calibration of bone driver transducers to measure the mastoid Reggie Weece a

    E-Print Network [OSTI]

    Allen, Jont

    2010 Available online xxxx a b s t r a c t When using bone vibrator transducers for clinical a circuit model of the driver, describing it with three frequency-dependent parameters. Once these three circuit model is proposed to better capture the observed behaviors. Ã? 2010 Published by Elsevier B.V. 1

  20. Offshore Wind Turbine Design: Addressing Uncertainty Drivers Sten Frandsen Niels Jacob Tarp-Johansen

    E-Print Network [OSTI]

    the next generation of offshore wind farms are designed. The aim of this paper is to discuss existingOffshore Wind Turbine Design: Addressing Uncertainty Drivers Sten Frandsen Niels Jacob Tarp@civil.auc.dk leje@elsam-eng.com Abstract: Current offshore wind turbine design methods have matured to a 1st

  1. Young drivers and the efficacy of the Texas drug and alcohol driving awareness program

    E-Print Network [OSTI]

    Darnell, Richard

    2009-05-15T23:59:59.000Z

    The purpose of this study was to examine the efficacy of the Texas Drug and Alcohol Driving Awareness Program (TDADAP) in relation to alcohol-related offenses among young drivers. Participants in this study were students in pre-license programs...

  2. What kind of charging infrastructure do Chevrolet Volts Drivers in The EV Project use?

    SciTech Connect (OSTI)

    John Smart

    2013-09-01T23:59:59.000Z

    This report summarizes key conclusions from analysis of data collected from Chevrolet Volts participating in The EV Project. Topics include how much Volt drivers charge at level 1 vs. level 2 rates and how much they charge at home vs. away from home.

  3. Perception Drivers for Treated Wood by U.S. South Homebuilders and Remodelers

    E-Print Network [OSTI]

    Wu, Qinglin

    Perception Drivers for Treated Wood by U.S. South Homebuilders and Remodelers Sanna M. Kallioranta1 for the use of treated wood products in construction is considerable, especially in the U.S. South for termite protection and to mitigate moisture related decay. This research investigates the perception about treated

  4. Evolution styles: using architectural knowledge as an evolution driver Carlos E. Cuesta1

    E-Print Network [OSTI]

    Perry, Dewayne E.

    Evolution styles: using architectural knowledge as an evolution driver Carlos E. Cuesta1 , Elena+D, 02006, Albacete, Spain ABSTRACT Software evolution is an increasingly challenging and compelling concern software evolution is carried out, software architecture emerges as one of the cornerstones that should

  5. Evolution on a Restless Planet: Were Environmental Variability and Environmental Change Major Drivers of Human Evolution?

    E-Print Network [OSTI]

    Richerson, Peter J.

    223 7 Evolution on a Restless Planet: Were Environmental Variability and Environmental Change Major Drivers of Human Evolution? Peter J. Richerson, Robert L. Bettinger, and Robert Boyd 7.1 Introduction Two kinds of factors set the tempo and direction of organic and cultural evolution, those external to biotic

  6. Setup, tests and results for the ATLAS TileCal Read Out Driver production

    E-Print Network [OSTI]

    Valero, Alberto; Castillo, V; Cuenca, C; Ferrer, A; Fullana, E; González, V; Higón, E; Munar, A; Poveda, J; Ruiz-Martínez, A; Salvachúa, B; Sanchís, E; Solans, C; Soret, J; Torres, J; Valls, J A

    2007-01-01T23:59:59.000Z

    In this paper we describe the performance and test results of the production of the 38 ATLAS TileCal Read Out Drivers (RODs). We first describe the basic hardware specifications and firmware functionality of the modules, the test-bench setup used for production and the test procedure to qualify the boards. We then finally show and discuss the performance results.

  7. HIGH INTENSITY LINAC DRIVER FOR THE SPIRAL-2 PROJECT : DESIGN OF SUPERCONDUCTING 88 MHZ QUARTER WAVE

    E-Print Network [OSTI]

    Paris-Sud XI, Université de

    . For the high-energy section of the linac, a superconducting 88 MHz Quarter Wave Resonator (beta 0.12) has been WAVE RESONATORS (BETA 0.12), POWER COUPLERS AND CRYOMODULES T. Junquera, G. Olry, H. Saugnac, J Abstract A superconducting linac driver, delivering deuterons with an energy up to 40 MeV (5 mA) and heavy

  8. Using Vision-Based Driver Assistance to Augment Vehicular Ad-Hoc Network Communication

    E-Print Network [OSTI]

    Beauchemin, Steven S.

    a Vision-Based Driver Assistance (VBDA) system that monitors the environment surrounding the vehicle using in the surrounding environment. The concept of a CCWS has been introduced, studied and validated by a number adoption of the Wireless Access in Vehicular Environments (WAVE) set of standards in production vehicles

  9. Linearity -statistics 1.1B training

    E-Print Network [OSTI]

    Linearity - statistics IPAT 1.1B training 300M training D0 resolution is evaluated using 100k single muon events (same events in all 3 plots). Red is the default 11L FTK bank trained using 300M muons on narrow beam of muons (central eta, fixed phi, high fixed pT). Using two types of training: default FTK

  10. Centre for Smoking Cessation and Training

    E-Print Network [OSTI]

    Saunders, Mark

    Centre for Smoking Cessation and Training The NHS Centre for Smoking Cessation and Training (NCSCT and commissioners commission and provide training and continuing support to allow staff to achieve the required of training courses advise the Department of Health on issues relating to the Stop Smoking Services

  11. Assessor Training Evaluating OnSite Reports

    E-Print Network [OSTI]

    NVLAP Assessor Training Evaluating OnSite Reports and Corrective Actions #12;Assessor Training 2009Site Report form ·NVLAP OnSite Assessment Review form #12;Assessor Training 2009: Evaluating OnSite Reports · Nonconformities cited #12;Assessor Training 2009: Evaluating OnSite Reports & Corrective Actions 44 Evaluating

  12. Training for Emergencies Panel: Chris Reed

    E-Print Network [OSTI]

    Training for Emergencies Panel: Chris Reed Ben Berman Immanuel Barshi It's very important to have pilots sharing ideas with other instructor pilots. IB: In aviation there is a lot of mentor training. Instructor pilots are not trained trainers; they are aviators who are providing training. When things

  13. Arizona Foundation Expands Weatherization Training Center

    Broader source: Energy.gov [DOE]

    Read about one weatherization training center that's looking forward to an onslaught of new trainees.

  14. Special Clinical Staff Training Specialized Radiation Safety

    E-Print Network [OSTI]

    Baker, Chris I.

    Special Clinical Staff Training Specialized Radiation Safety Training Courses for: Nurses these training courses by contacting the Radiation Safety Training Office at 496-2255. Radiation Safety for Clinical Center Employees A great introduction to radiation and radioactive material for new Clinical

  15. 2014 Veteran Employment and USERRA Mandatory Training

    Broader source: Energy.gov [DOE]

    Annual Mandatory Training for Managers, Supervisors and Human Resource Professionals on Veteran Employment and USERRA

  16. Training for Emergencies Need for some uniformity of training across airlines. Concern is especially about

    E-Print Network [OSTI]

    Training for Emergencies · Need for some uniformity of training across airlines. Concern is especially about variability in amount of training for emergencies. Not enough training in general for emergencies. · What are the criteria for training for success. · Try a "hypertext" approach to simulator

  17. Training Request Form Administration Training Services, Organizational Effectiveness/OHR 612-626-1373 ULearn

    E-Print Network [OSTI]

    Minnesota, University of

    Training Request Form Administration Training Services, Organizational Effectiveness/OHR · 612-626-1373 ULearn www.umn.edu/ohr/trainingservices 5-17-12 A Training Request Forms are designed to obtain additional information from a learner when requesting training in ULearn. The Training Request Form

  18. VIRTUAL TRAINING CENTRE FOR SHOE DESIGN: A SAMPLE VIRTUAL TRAINING ENVIRONMENT

    E-Print Network [OSTI]

    Aristomenis, Antoniadis

    VIRTUAL TRAINING CENTRE FOR SHOE DESIGN: A SAMPLE VIRTUAL TRAINING ENVIRONMENT Aura Mihai1 , Mehmet@tex.tuiasi.ro Abstract It is a fact that virtual training has become a key issue in training. There are numerous virtual learning and training environments and, in parallel with this, there are various approaches and tools

  19. DOE's BestPractices Steam End User Training Steam End User Training

    E-Print Network [OSTI]

    Oak Ridge National Laboratory

    DOE's BestPractices Steam End User Training Steam End User Training Introduction Module - 1 8/27/2010 Steam End User Training Introduction Module Slide 1 - Introduction Title Page Hello, and welcome to the Steam System End User training. In this training, we will investigate how to assess, evaluate

  20. PERSONAL TRAINING RECORD Guidance on using the Personal Safety Training Record

    E-Print Network [OSTI]

    Cambridge, University of

    PERSONAL TRAINING RECORD Guidance on using the Personal Safety Training Record What safety training adequate health and safety training on induction, when there is exposure to new or increased risks and to repeat the training periodically where appropriate. Members of the University are required to attend any

  1. DOE's BestPractices Steam End User Training Steam End User Training

    E-Print Network [OSTI]

    Oak Ridge National Laboratory

    DOE's BestPractices Steam End User Training Steam End User Training Steam Distribution Losses Module 1 June 29, 2010 Steam EndUser Training Steam Distribution System Losses Module Slide 1 pressure. #12;DOE's BestPractices Steam End User Training Steam End User Training Steam Distribution

  2. TTU RCR Training Certification RCR_TrainingCert Page 1 of 1 8/26/2010

    E-Print Network [OSTI]

    Rock, Chris

    TTU RCR Training Certification RCR_TrainingCert Page 1 of 1 8/26/2010 Background: Your: Name of trainee R number eRaider name UG G PD 1 semester Safety training CITI training by this award have received RCR training as required No additonal students or postdoctoral trainees are or were

  3. DOE's BestPractices Steam End User Training Steam End User Training

    E-Print Network [OSTI]

    Oak Ridge National Laboratory

    DOE's BestPractices Steam End User Training Steam End User Training Welcome Module - 1 8/27/2010 Steam End User Training Welcome Module Slide 1 ­ Steam End User Training Welcome to the Department of Energy's Industrial Technologies Program BestPractices Steam End-User Training. The Department of Energy

  4. What is Personal Training? Personal Training offers a one-on-one

    E-Print Network [OSTI]

    McConnell, Terry

    PERSONAL TRAINING What is Personal Training? Personal Training offers a one-on-one private workout program, your Personal Trainer will help you reach your goals. Learn the different weight training will begin your Personal Training program with a fitness assessment, which will give the trainer

  5. Training & Technology Solutions Queens College ~ Office of Converging Technologies ~ Training & Technology Solutions

    E-Print Network [OSTI]

    Johnson Jr.,, Ray

    Training & Technology Solutions Queens College ~ Office of Converging Technologies ~ Training & Technology Solutions 718-997-4875 ~ training@qc.cuny.edu ~ I-Bldg 214 CUNYfirst Faculty Center Navigation;Training & Technology Solutions Queens College ~ Office of Converging Technologies ~ Training & Technology

  6. ALARA training at DOE contractor facilities

    SciTech Connect (OSTI)

    Neeser, J.L.

    1992-05-22T23:59:59.000Z

    ALARA training is an important element of a sound ALARA program. ALARA training at a nuclear facility needs to be conducted for all occupational workers, for radiation workers, for radiation protection technicians, and for all other employees who have ALARA responsibilities. Each of these groups needs to receive ALARA training specific to their responsibilities. This report describes how to develop this training. It also outlines what should be included in an acceptable ALARA training program.

  7. Training Program Handbook: A Systematic Approach to Training

    Office of Environmental Management (EM)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level: National5Sales for4,645 3,625 1,006 492 742 33Frequently AskedEnergyIssuesEnergy SolarRadioactiveI DisposalFiveTraining News Training

  8. Does Brain-Training Make You Smarter? Evidence from Working Memory Training Studies

    E-Print Network [OSTI]

    Rose, Michael R.

    Does Brain-Training Make You Smarter? Evidence from Working Memory Training Studies Guest Lecture by Claudia von Bastian Psychology & Neuroscience be improved through cognitive training? This question is still highly controversial

  9. The Perceived Impact of Cognitive Developmental Training on the Perceptions of University and District Trained Mentors

    E-Print Network [OSTI]

    Williams, Jennifer Beth

    2011-08-08T23:59:59.000Z

    The purpose of this study is to investigate differences found in self-efficacy perceptions regarding mentoring of trained mentors who were trained using a cognitive developmental model of mentor training, with mentor teachers who have received...

  10. Planets Around Low-Mass Stars (PALMS). III. A Young Dusty L Dwarf Companion at the Deuterium-Burning Limit

    E-Print Network [OSTI]

    Bowler, Brendan P; Shkolnik, Evgenya L; Dupuy, Trent J

    2013-01-01T23:59:59.000Z

    We report the discovery of an L-type companion to the young M3.5V star 2MASS J01225093-2439505 at a projected separation of 1.45" (~52 AU) as part of our adaptive optics imaging search for extrasolar giant planets around young low-mass stars. 2MASS 0122-2439 B has very red near-infrared colors similar to the HR 8799 planets and the reddest known young/dusty L dwarfs in the field. Moderate-resolution (R~3800) 1.5-2.4 $\\mu$m spectroscopy reveals a near-infrared spectral type of L4-L6 and an angular H-band shape, confirming its cool temperature and young age. The kinematics of 2MASS 0122-2439 AB are marginally consistent with members of the ~120 Myr AB Dor young moving group based on the photometric distance to the primary (36 +/- 4 pc) and our radial velocity measurement of 2MASS 0122-2439 A from Keck/HIRES. We adopt the AB Dor group age for the system, but the high energy emission, lack of Li I $\\lambda$6707 absorption, and spectral shape of 2MASS 0122-2439 B suggest a range of ~10-120 Myr is possible. The age...

  11. Detection of the radial velocity curve of the B5-A0 supergiant companion star of Cir X-1?

    E-Print Network [OSTI]

    Jonker, P G; Bassa, C G

    2006-01-01T23:59:59.000Z

    In this Paper we report on phase resolved I-band optical spectroscopic and photometric observations of Cir X-1 obtained with the Very Large Telescope. The spectra are dominated by Paschen absorption lines at nearly all orbital phases except near phase zero (coinciding with the X-ray dip) when the absorption lines are filled-in by broad Paschen emission lines. The radial velocity curve of the absorption lines corresponds to an eccentric orbit (e=0.45) whose period and time of periastron passage are consistent with the period and phase predicted by the most recent X-ray dip ephemeris. We found that the I-band magnitude is consistent with being constant at I=17.6 in the binary phase interval 0.1-0.6. The source-brightness peaks at I=16.7-16.9 at phase 0.9-1.0. This I-band brightening coincides in phase with the X-ray dip. Even though it is likely that the absorption line spectrum is associated with the companion star of Cir X-1, we cannot exclude the possibility that the spectrum originates in the accretion disc...

  12. Newly Determined Explosion Center of Tycho's Supernova and the Implications for Proposed Ex-Companion Stars of the Progenitor

    E-Print Network [OSTI]

    Xue, Zhichao

    2015-01-01T23:59:59.000Z

    `Star G', near the center of the supernova remnant of Tycho's SN1572, has been claimed to be the ex-companion star of the exploding white dwarf, thus pointing to the progenitor being like a recurrent nova. This claim has been controversial, but there have been no confident proofs or disproofs. Previously, no has seriously addressed the question as to the exact explosion site in 1572. We now provide accurate measures of the supernova position by two radically different methods. Our first method is to use the 42 measured angular distances between the supernova in 1572 and bright nearby stars, with individual measures being as good as 84 arc-seconds, and all resulting in a position with a 1-$\\sigma$ error radius of 39 arc-seconds (including systematic uncertainties). Our second method is to use a detailed and realistic expansion model for 19 positions around the edge of the remnant, where the swept-up material has measured densities, and we determine the center of expansion with a chi-square fit to the 19 measur...

  13. The Water Abundance of the Directly Imaged Substellar Companion {\\kappa} And b Retrieved from a Near Infrared Spectrum

    E-Print Network [OSTI]

    Todorov, Kamen O; Pineda, Jaime E; Meyer, Michael R; Quanz, Sascha P; Hinkley, Sasha; Fortney, Jonathan J

    2015-01-01T23:59:59.000Z

    Recently, spectral retrieval has proven to be a powerful tool for constraining the physical properties and atmospheric compositions of extrasolar planet atmospheres from observed spectra, primarily for transiting objects but also increasingly for directly imaged planets and brown dwarfs. Despite its strengths, this approach has been applied to only about a dozen targets. Determining the abundances of the main carbon and oxygen-bearing compounds in a planetary atmosphere can lead to the C/O ratio of the object, which is crucial in understanding its formation and migration history. We present a retrieval analysis on the published near-infrared spectrum of {\\kappa} And b, a directly imaged substellar companion to a young B9 star. We fit the emission spectrum model utilizing a Markov Chain Monte Carlo algorithm. We estimate the abundance of water vapor, and its uncertainty, in the atmosphere of the object. We also place upper limits on the abundances of carbon dioxide and methane and constrain the pressure-temper...

  14. Pruning and Training Peach Orchards

    E-Print Network [OSTI]

    Price, R. H.

    1901-01-01T23:59:59.000Z

    is directing the growth of succeeding branches. The idea of correct train- ing should come befo~e successful pruning. we prune in olrder to train a tree according to some preconceived ideal of form. We also prune, , less frequently, to remove dead wood...- wards. No one should prune a peach tree without fully understanding the necessity of the operation and also what results such an ope~ation of surgery would have upon the future growth of the tree. The best form of top for a given locality...

  15. Bishop Paiute Weatherization Training Program

    SciTech Connect (OSTI)

    Carlos Hernandez

    2010-01-28T23:59:59.000Z

    The DOE Weatherization Training Grant assisted Native American trainees in developing weatherization competencies, creating employment opportunities for Bishop Paiute tribal members in a growing field. The trainees completed all the necessary training and certification requirements and delivered high-quality weatherization services on the Bishop Paiute Reservation. Six tribal members received all three certifications for weatherization; four of the trainees are currently employed. The public benefit includes (1) development of marketable skills by low-income Native individuals, (2) employment for low-income Native individuals in a growing industry, and (3) economic development opportunities that were previously not available to these individuals or the Tribe.

  16. Training | National Nuclear Security Administration

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level:Energy: Grid Integration Redefining What'sis Taking Over OurThe Iron Spin Transition in2, 2003Tool ofTopoCarbon DioxideTraining Training

  17. Training News | Department of Energy

    Office of Environmental Management (EM)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level: National5Sales for4,645 3,625 1,006 492 742 33Frequently AskedEnergyIssuesEnergy SolarRadioactiveI DisposalFiveTraining News Training News

  18. EPA Tribal Training and Outreach Support for the American Indian Air Quality Training Program

    Broader source: Energy.gov [DOE]

    The U.S. Environmental Protection Agency (EPA) is accepting applications to provide training, and technical and outreach support for the American Indian Air Quality Training Program.

  19. Training new operators - the first six months

    SciTech Connect (OSTI)

    Worthel, B.; /Fermilab

    2010-04-01T23:59:59.000Z

    The Fermilab Operations Department takes about two years to train a new Operator. The Operator's introductory (Concepts) On-the-Job-Training (OJT) gives him or her an overview of the laboratory, teaches the basic facts about all the accelerators, and it also teaches the new operator the training process used for all the rest of their OJT training. The Concepts OJT takes about four to six months for most people to complete. This paper will explain how this first six months of training sets the new employee on their path to becoming a fully trained Operator.

  20. MODELING THE INFRARED SPECTRUM OF THE EARTH-MOON SYSTEM: IMPLICATIONS FOR THE DETECTION AND CHARACTERIZATION OF EARTHLIKE EXTRASOLAR PLANETS AND THEIR MOONLIKE COMPANIONS

    SciTech Connect (OSTI)

    Robinson, Tyler D., E-mail: robinson@astro.washington.edu [NASA Astrobiology Institute. (United States)

    2011-11-01T23:59:59.000Z

    The Moon maintains large surface temperatures on its illuminated hemisphere and can contribute significant amounts of flux to spatially unresolved thermal infrared (IR) observations of the Earth-Moon system, especially at wavelengths where Earth's atmosphere is absorbing. In this paper we investigate the effects of an unresolved companion on IR observations of Earthlike exoplanets. For an extrasolar twin Earth-Moon system observed at full phase at IR wavelengths, the Moon consistently comprises about 20% of the total signal, approaches 30% of the signal in the 9.6 {mu}m ozone band and the 15 {mu}m carbon dioxide band, makes up as much as 80% of the signal in the 6.3 {mu}m water band, and more than 90% of the signal in the 4.3 {mu}m carbon dioxide band. These excesses translate to inferred brightness temperatures for Earth that are too large by 20-40 K and demonstrate that the presence of undetected satellites can have significant impacts on the spectroscopic characterization of exoplanets. The thermal flux contribution from an airless companion depends strongly on phase, implying that observations of exoplanets should be taken when the star-planet-observer angle (i.e., phase angle) is as large as feasibly possible if contributions from companions are to be minimized. We show that, by differencing IR observations of an Earth twin with a companion taken at both gibbous and crescent phases, Moonlike satellites may be detectable by future exoplanet characterization missions for a wide range of system inclinations.

  1. Accounting for the Variation of Driver Aggression in the Simulation of Conventional and Advanced Vehicles

    SciTech Connect (OSTI)

    Neubauer, J.; Wood, E.

    2013-01-01T23:59:59.000Z

    Hybrid electric vehicles, plug-in hybrid electric vehicles, and battery electric vehicles offer the potential to reduce both oil imports and greenhouse gases, as well as to offer a financial benefit to the driver. However, assessing these potential benefits is complicated by several factors, including the driving habits of the operator. We focus on driver aggression, i.e., the level of acceleration and velocity characteristic of travel, to (1) assess its variation within large, real-world drive datasets, (2) quantify its effect on both vehicle efficiency and economics for multiple vehicle types, (3) compare these results to those of standard drive cycles commonly used in the industry, and (4) create a representative drive cycle for future analyses where standard drive cycles are lacking.

  2. Accounting for the Variation of Driver Aggression in the Simulation of Conventional and Advanced Vehicles: Preprint

    SciTech Connect (OSTI)

    Neubauer, J.; Wood, E.

    2013-03-01T23:59:59.000Z

    Hybrid electric vehicles, plug-in hybrid electric vehicles, and battery electric vehicles offer the potential to reduce both oil imports and greenhouse gases, as well as to offer a financial benefit to the driver. However, assessing these potential benefits is complicated by several factors, including the driving habits of the operator. We focus on driver aggression, i.e., the level of acceleration and velocity characteristic of travel, to (1) assess its variation within large, real-world drive datasets, (2) quantify its effect on both vehicle efficiency and economics for multiple vehicle types, (3) compare these results to those of standard drive cycles commonly used in the industry, and (4) create a representative drive cycle for future analyses where standard drive cycles are lacking.

  3. OPERATION AND COMMISSIONING OF THE JEFFERSON LAB UV FEL USING AN SRF DRIVER ERL

    SciTech Connect (OSTI)

    R. Legg; S. Benson; G. Biallas; K. Blackburn; J. Boyce; D. Bullard; J. Coleman; C. Dickover; D. Douglas; F. Ellingsworth; P. Evtushenko; F. Hannon; C. Hernandez-Garcia; C. Gould; J. Gubeli; D. Hardy; K. Jordan; M. Klopf; J. Kortze; M. Marchlik; W. Moore; G. Neil; T. Powers; D. Sexton; Michelle D. Shinn; C. Tennant; R. Walker; G. Wilson

    2011-03-01T23:59:59.000Z

    We describe the operation and commissioning of the Jefferson Lab UV FEL using a CW SRF ERL driver. Based on the same 135 MeV linear accelerator as the Jefferson Lab 10 kW IR Upgrade FEL, the UV driver ERL uses a bypass geometry to provide transverse phase space control, bunch length compression, and nonlinear aberration compensation necessitating a unique set of commissioning and operational procedures. Additionally, a novel technique to initiate lasing is described. To meet these constraints and accommodate a challenging installation schedule, we adopted a staged commissioning plan with alternating installation and operation periods. This report addresses these issues and presents operational results from on-going beam operations.

  4. Discovery of a Brown Dwarf Companion to Gliese 570ABC: A 2MASS T Dwarf Significantly Cooler than Gliese 229B

    E-Print Network [OSTI]

    A. J. Burgasser; J. D. Kirkpatrick; R. M. Cutri; H. McCallon; G. Kopan; J. E. Gizis; J. Liebert; I. N. Reid; M. E. Brown; D. G. Monet; C. C. Dahn; C. A. Beichman; M. F. Skrutskie

    2000-01-11T23:59:59.000Z

    We report the discovery of a widely separated (258$\\farcs3\\pm0\\farcs$4) T dwarf companion to the Gl 570ABC system. This new component, Gl 570D, was initially identified from the Two Micron All Sky Survey (2MASS). Its near-infrared spectrum shows the 1.6 and 2.2 $\\micron$ CH$_4$ absorption bands characteristic of T dwarfs, while its common proper motion with the Gl 570ABC system confirms companionship. Gl 570D (M$_J$ = 16.47$\\pm$0.07) is nearly a full magnitude dimmer than the only other known T dwarf companion, Gl 229B, and estimates of L = (2.8$\\pm$0.3)x10$^{-6}$ L$_{\\sun}$ and T$_{eff}$ = 750$\\pm$50 K make it significantly cooler and less luminous than any other known brown dwarf companion. Using evolutionary models by Burrows et al. and an adopted age of 2-10 Gyr, we derive a mass estimate of 50$\\pm$20 M$_{Jup}$ for this object.

  5. _____________________________ Environment, Health, & Safety _________ __________________ Training Program

    E-Print Network [OSTI]

    Eisen, Michael

    _________ __________________ Training Program EHS 365 ~ Asbestos Containment Entry Course Syllabus Subject Category: Occupational Health: This course is designed for personnel who may need to enter asbestos containments, but not for the purpose on an annual basis with the exception of EH&S personnel. Entry is limited to entering asbestos containments

  6. _____________________________ Environment, Health, & Safety _________ __________________ Training Program

    E-Print Network [OSTI]

    Eisen, Michael

    Program EHS 364 ~ Asbestos Class III 4 Hour Training Course Syllabus Subject Category: Occupational Health class participation on asbestos control work practices · Copy of power point slides · Interactive employees, or other employees, who incidentally disturb small amounts of asbestos containing building

  7. Radiation Safety Annual Refresher Training

    E-Print Network [OSTI]

    Thomas, David D.

    Radiation Safety Annual Refresher Training Radiation Protection Division Department of Environmental Health & Safety #12;Topics in Radiation Safety (applicable RPD Manual sections indicated) User;Topics in Radiation Safety (applicable RPD Manual sections indicated) User and Non-user topics Types

  8. Modularized training for technical editors

    SciTech Connect (OSTI)

    Murphy, P.W.

    1988-09-08T23:59:59.000Z

    This paper outlines the editorial services provided at the Lawrence Livermore National Laboratory (LLNL), sketches a syllabus of basic training for technical editors, describes the approach being used to develop this cost-effective individualized instruction for editors (experienced or not) new to work at LLNL, and enumerates the advantages of this approach. 8 refs.

  9. UNCG Security Awareness Training & Instructions

    E-Print Network [OSTI]

    Saidak, Filip

    UNCG Security Awareness Training & Instructions 02.09.2010 Page 1 of 4 Educating UNCG faculty and staff with respect to security best practices is essential in securing the University's information University employee that works with restricted or financial data. UNCG engaged Fishnet Security, a nationally

  10. _____________________________ Environment, Health, & Safety _________ __________________ Training Program

    E-Print Network [OSTI]

    _________ __________________ Training Program EHS 373 Lockout/Tagout for Responsible Individuals Course Syllabus Subject Category with an understanding of Lockout/Tagout responsibilities and acceptable practices. It will also address management will be able to: · Identify requirements for performing lockout/tagout · Identify four exceptions to LOTO

  11. _____________________________ Environment, Health, & Safety _________ __________________ Training Program

    E-Print Network [OSTI]

    Knowles, David William

    Prerequisite: None Course Length: 20 minutes Medical Approval: None Delivery Mode: Web-based Training Frequency Expert: Lorraine Dowling Web-based Instructional Designer: Brooke Vaughn Course Instructional Materials: Web-based course and a PDF downloadable version of the course is available within the web- based

  12. Health and Safety Training Reciprocity

    Broader source: Directives, Delegations, and Requirements [Office of Management (MA)]

    2014-04-14T23:59:59.000Z

    Establishes a policy for reciprocity of employee health and safety training among DOE entities responsible for employee health and safety at DOE sites and facilities to increase efficiency and effectiveness of Departmental operations while meeting established health and safety requirements. Does not cancel other directives.

  13. E Procurement Training for Non-

    E-Print Network [OSTI]

    E Procurement Training for Non- Pilot departments Provided by: BIDSYNC Sponsored by: DGS #12;What is eProcurement (eP)? eProcurement is an online requisition and solicitation development tool e, and LPA search engine will only be accessible via eProcurement at go-live on March 16, 2009 This session

  14. Testing, Training, and Signature Devices | Y-12 National Security...

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

    Testing, Training, and ... Testing, Training, and Signature Devices Y-12 manufactures specialized uranium testing, training, and signature devices to support the nuclear detection...

  15. NERSC Online Training May 3: Navigating NERSC File Systems

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

    Online Training May 3: Navigating NERSC File Systems NERSC Online Training May 3: Navigating NERSC File Systems April 26, 2011 by Richard Gerber A NERSC training event, "Navigating...

  16. DOE Cybersecurity Training and Education | Department of Energy

    Office of Environmental Management (EM)

    Training and Education DOE Cybersecurity Training and Education The DOE Cybersecurity Awareness and Training (CSAT) program provides the Department an opportunity to leverage its...

  17. Cognitive training in schizophrenia: a neuroscience-based approach

    E-Print Network [OSTI]

    Vinogradov, Sophia

    2010-01-01T23:59:59.000Z

    No. 3 . 2010 Cognitive training in schizophrenia - Genevskyspecific social skills training programmes for schizophreniaA review of cognitive training in schizophrenia. Schizophr

  18. Commercial Building Energy Asset Scoring Tool 2013 Pilot Training...

    Office of Environmental Management (EM)

    Scoring Tool 2013 Pilot Training Session Commercial Building Energy Asset Scoring Tool 2013 Pilot Training Session overview of the June 18, 2013 pilot training session for the...

  19. athletic training students: Topics by E-print Network

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

    department specific O'Toole, Alice J. 5 Athletic Training Education Program Bachelor of Science in Athletic Training Physics Websites Summary: Athletic Training Education Program...

  20. Renewable Energy Training and Education | Department of Energy

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

    Renewable Energy Training and Education Renewable Energy Training and Education October 16, 2013 - 5:17pm Addthis Multiple resources exist to train Federal agency personnel to...

  1. Managing the Drivers of Air Flow and Water Vapor Transport in Existing Single Family Homes (Revised)

    SciTech Connect (OSTI)

    Cummings, J.; Withers, C.; Martin, E.; Moyer, N.

    2012-10-01T23:59:59.000Z

    This document focuses on managing the driving forces which move air and moisture across the building envelope. While other previously published Measure Guidelines focus on elimination of air pathways, the ultimate goal of this Measure Guideline is to manage drivers which cause air flow and water vapor transport across the building envelope (and also within the home), control air infiltration, keep relative humidity (RH) within acceptable limits, avoid combustion safety problems, improve occupant comfort, and reduce house energy use.

  2. Evaluation of four selected servo hand controls for severely handicapped drivers

    E-Print Network [OSTI]

    Sexton, Donna Jean

    1979-01-01T23:59:59.000Z

    OF SCIENCE December 1979 Major Subject: Industrial Engineering EVALUATION OF FOUR SELECTED SERVO HAND CONTROLS FOR SEVERELY HANDICAPPED DRIVERS A Thesis by DONNA JEAN SEXTON Approved as to style and content by: (Co-Chairman of Committee) (Co... CURRENT TRENDS IN AUTOMOTIVE ADAPTIVE CONTROLS Mechanical Adaptive Controls Power Assist Adaptive Controls Joystick Controls METHOD Subjects The Tracking Task Apparatus DATA REDUCTION Analog to Digital Conversion Data Cleanup Calculation...

  3. Studies of a Linac Driver for a High Repetition Rate X-Ray FEL

    SciTech Connect (OSTI)

    Venturini, M.; Corlett, J.; Doolittle, L.; Filippetto, D.; Papadopoulos, C.; Penn, G.; Prosnitz, D.; Qiang, J.; Reinsch, M.; Ryne, R.; Sannibale, F.; Staples, J.; Wells, R.; Wurtele, J.; Zolotorev, M.; Zholents, A.

    2011-06-01T23:59:59.000Z

    We report on on-going studies of a superconducting CW linac driver intended to support a high repetition rate FEL operating in the soft x-rays spectrum. We present a pointdesign for a 1.8 GeV machine tuned for 300 pC bunches and delivering low-emittance, low-energy spread beams as needed for the SASE and seeded beamlines.

  4. DRIVER ACCELERATOR DESIGN FOR THE 10 KW UPGRADE OF THE JEFFERSON LAB IR FEL

    E-Print Network [OSTI]

    DRIVER ACCELERATOR DESIGN FOR THE 10 KW UPGRADE OF THE JEFFERSON LAB IR FEL D. Douglas, S. V, Newport News, VA23606, USA Abstract An upgrade of the Jefferson Lab IR FEL [1] is now un- der construction. It will provide 10 kW output light power in a wavelength range of 2­10 µm. The FEL will be driven by a modest

  5. Where do Nissan Leaf drivers in The EV Project charge when they have the opportunity to charge at work?

    SciTech Connect (OSTI)

    John Smart; Don Scoffield

    2014-03-01T23:59:59.000Z

    This paper invesigates where Nissan Leaf drivers in the EV Project charge when they have the opportunity to charge at work. Do they charge at work, home, or some other location?

  6. Where do Chevrolet Volt drivers in The EV Project charge when they have the opportunity to charge at work?

    SciTech Connect (OSTI)

    John Smart; Don Scoffield

    2014-03-01T23:59:59.000Z

    This paper investigates where Chevy Volt drivers in the EV Project charge when they have the opportunity to charge at work. Do they charge at home, work, or some other location.

  7. Analytic Framework for Evaluation of State Energy Efficiency and Renewable Energy Policies with Reference to Stakeholder Drivers

    SciTech Connect (OSTI)

    Brown, E.; Mosey, G.

    2008-07-01T23:59:59.000Z

    This report presents the framework that was developed to analyze energy efficiency and renewable energy policies on the state level based on how well they meet the stakeholder drivers.

  8. Compact, Intelligent, Digitally Controlled IGBT Gate Drivers for a PEBB-Based ILC Marx Modulator

    SciTech Connect (OSTI)

    Nguyen, M.N.; Burkhart, C.; Olsen, J.J.; Macken, K.; /SLAC; ,

    2010-06-07T23:59:59.000Z

    SLAC National Accelerator Laboratory has built and is currently operating a first generation prototype Marx klystron modulator to meet ILC specifications. Under development is a second generation prototype, aimed at improving overall performance, serviceability, and manufacturability as compared to its predecessor. It is designed around 32 cells, each operating at 3.75 kV and correcting for its own capacitor droop. Due to the uniqueness of this application, high voltage gate drivers needed to be developed for the main 6.5 kV and droop correction 1.7 kV IGBTs. The gate driver provides vital functions such as protection of the IGBT from over-voltage and over-current, detection of gate-emitter open and short circuit conditions, and monitoring of IGBT degradation (based on collector-emitter saturation voltage). Gate drive control, diagnostic processing capabilities, and communication are digitally implemented using an FPGA. This paper details the design of the gate driver circuitry, component selection, and construction layout. In addition, experimental results are included to illustrate the effectiveness of the protection circuit.

  9. Break-Even Cost for Residential Photovoltaics in the United States: Key Drivers and Sensitivities

    SciTech Connect (OSTI)

    Denholm, P.; Margolis, R. M.; Ong, S.; Roberts, B.

    2009-12-01T23:59:59.000Z

    Grid parity--or break-even cost--for photovoltaic (PV) technology is defined as the point where the cost of PV-generated electricity equals the cost of electricity purchased from the grid. Break-even cost is expressed in $/W of an installed system. Achieving break-even cost is a function of many variables. Consequently, break-even costs vary by location and time for a country, such as the United States, with a diverse set of resources, electricity prices, and other variables. In this report, we analyze PV break-even costs for U.S. residential customers. We evaluate some key drivers of grid parity both regionally and over time. We also examine the impact of moving from flat to time-of-use (TOU) rates, and we evaluate individual components of the break-even cost, including effect of rate structure and various incentives. Finally, we examine how PV markets might evolve on a regional basis considering the sensitivity of the break-even cost to four major drivers: technical performance, financing parameters, electricity prices and rates, and policies. We find that local incentives rather than ?technical? parameters are in general the key drivers of the break-even cost of PV. Additionally, this analysis provides insight about the potential viability of PV markets.

  10. Highway crash rates and age-related driver limitations: Literature review and evaluation of data bases

    SciTech Connect (OSTI)

    Hu, P.S. [Oak Ridge National Lab., TN (United States)] [Oak Ridge National Lab., TN (United States); Young, J.R. [Tennessee Univ., Knoxville, TN (United States)] [Tennessee Univ., Knoxville, TN (United States); Lu, An [Oak Ridge Associated Universities, Inc., TN (United States)] [Oak Ridge Associated Universities, Inc., TN (United States)

    1993-08-01T23:59:59.000Z

    American society is undergoing a major demographic transformation that is resulting in a larger proportion of older individuals in the population. Moreover, recent travel surveys show that an increasing number of older individuals are licensed to drive and that they drive more than their same age cohort a decade ago. However, they continue to take shorter trips than younger drivers and they avoid driving during congested hours. This recent demographic transformation in our society, the graying of America, coupled with the increasing mobility of the older population impose a serious highway safety issue that cannot be overlooked. Some of the major concerns are the identification of ``high-risk`` older drivers and the establishment of licensing guidelines and procedures that are based on conclusive scientific evidence. Oak Ridge National Laboratory`s (ORNL) objectives in this project can be characterized by the following tasks: Review and evaluate the 1980 American Association of Motor Vehicle Administrators (AAMVA) and National Highway Traffic Safety Administration (NHTSA) licensing guidelines. Determine whether the license restriction recommended in the 1980 AAMVA and NHTSA guidelines was based on scientific evidence or on judgement of medical advisors. Identify in the scientific literature any medical conditions which are found to be highly associated with highway crashes, and which are not mentioned in the 1980 guidelines. Summarize States` current licensing practices for drivers with age-related physical and mental limitations. Identify potential data sources to establish conclusive evidence on age-related functional impairments and highway crashes.

  11. Analysis of the Ultra-fast Switching Dynamics in a Hybrid MOSFET/Driver

    SciTech Connect (OSTI)

    Tang, T.; Burkhart, C.; /SLAC

    2011-08-17T23:59:59.000Z

    The turn-on dynamics of a power MOSFET during ultra-fast, {approx} ns, switching are discussed in this paper. The testing was performed using a custom hybrid MOSFET/Driver module, which was fabricated by directly assembling die-form components, power MOSFET and drivers, on a printed circuit board. By using die-form components, the hybrid approach substantially reduces parasitic inductance, which facilitates ultra-fast switching. The measured turn on time of the hybrid module with a resistive load is 1.2 ns with an applied voltage of 1000 V and drain current of 33 A. Detailed analysis of the switching waveforms reveals that switching behavior must be interpreted differently in the ultra-fast regime. For example, the gate threshold voltage to turn on the device is observed to increase as the switching time decreases. Further analysis and simulation of MOSFET switching behavior shows that the minimum turn on time scales with the product of the drain-source on resistance and drain-source capacitance, R{sub DS(on)}C{sub OSS}. This information will be useful in power MOSFET selection and gate driver design for ultra-fast switching applications.

  12. Survey of Laser Markets Relevant to Inertial Fusion Energy Drivers, information for National Research Council

    SciTech Connect (OSTI)

    Bayramian, A J; Deri, R J; Erlandson, A C

    2011-02-24T23:59:59.000Z

    Development of a new technology for commercial application can be significantly accelerated by leveraging related technologies used in other markets. Synergies across multiple application domains attract research and development (R and D) talent - widening the innovation pipeline - and increases the market demand in common components and subsystems to provide performance improvements and cost reductions. For these reasons, driver development plans for inertial fusion energy (IFE) should consider the non-fusion technology base that can be lveraged for application to IFE. At this time, two laser driver technologies are being proposed for IFE: solid-state lasers (SSLs) and KrF gas (excimer) lasers. This document provides a brief survey of organizations actively engaged in these technologies. This is intended to facilitate comparison of the opportunities for leveraging the larger technical community for IFE laser driver development. They have included tables that summarize the commercial organizations selling solid-state and KrF lasers, and a brief summary of organizations actively engaged in R and D on these technologies.

  13. Accounting for the Variation of Driver Aggression in the Simulation of Conventional and Advanced Vehicles (Presentation)

    SciTech Connect (OSTI)

    Neubauer, J.; Wood, E.

    2013-05-01T23:59:59.000Z

    This presentation discusses a method of accounting for realistic levels of driver aggression to higher-level vehicle studies, including the impact of variation in real-world driving characteristics (acceleration and speed) on vehicle energy consumption and different powertrains (e.g., conventionally powered vehicles versus electrified drive vehicles [xEVs]). Aggression variation between drivers can increase fuel consumption by more than 50% or decrease it by more than 20% from average. The normalized fuel consumption deviation from average as a function of population percentile was found to be largely insensitive to powertrain. However, the traits of ideal driving behavior are a function of powertrain. In conventional vehicles, kinetic losses dominate rolling resistance and aerodynamic losses. In xEVs with regenerative braking, rolling resistance and aerodynamic losses dominate. The relation of fuel consumption predicted from real-world drive data to that predicted by the industry-standard HWFET, UDDS, LA92, and US06 drive cycles was not consistent across powertrains, and varied broadly from the mean, median, and mode of real-world driving. A drive cycle synthesized by NREL's DRIVE tool accurately and consistently reproduces average real-world for multiple powertrains within 1%, and can be used to calculate the fuel consumption effects of varying levels of driver aggression.

  14. Use of the National Driver Register in the U.S. Department of Energy Human Reliability Program

    SciTech Connect (OSTI)

    Phillip M. Kannan, Center for Human Reliability Studies

    2007-01-01T23:59:59.000Z

    The National Driver Register (NDR) is a complex information network established and maintained by the Secretary of the Department of Transportation (DOT) under the National Driver Register Act of 1982. This report analyzes the question of whether information from the NDR is available to officials making Human Reliability Program (HRP) certification and recertification decisions and to Department of Energy (DOE) personnel security specialists making access authorization determinations.

  15. Fill in the following information: Mediation Training

    E-Print Network [OSTI]

    Arnold, Jonathan

    Fill in the following information: Mediation Training Fall 2014 Registration Form GENERAL / CIVIL:30 pm) Select training date(s): 3 1 2 Mail check or money order to: J.W. Fanning Institute

  16. The Weatherization Training program at Pennsylvania College

    SciTech Connect (OSTI)

    Meville, Jeff; Wilson, Jack; Manz, John; Gannett, Kirk; Smith, Franzennia

    2010-01-01T23:59:59.000Z

    A look into some of the remarkable work being done in the Weatherization Training program at Pennsylvania College. Penn College's program has served as the model for six other training centers in Pennsylvania alone.

  17. Making Education and Training Impact on Industry

    E-Print Network [OSTI]

    Cohen, K. C.

    1980-01-01T23:59:59.000Z

    Making education and training impact on anyone these days seems to be an increasing difficult problem. Perhaps one of the reasons we see this growing problem and our relative failure in attempts to make education and training more effective...

  18. Discovering the Value of "Gaining Through Training"

    E-Print Network [OSTI]

    Lee, R. C.; Hahn, G. E.

    This paper is dedicated to five situations where unrecognized needs were discovered while general and generic training was being conducted. The initial training classes were on the proper use and importance of steam energy in many different types...

  19. The Weatherization Training program at Pennsylvania College

    ScienceCinema (OSTI)

    Meville, Jeff; Wilson, Jack; Manz, John; Gannett, Kirk; Smith, Franzennia;

    2013-05-29T23:59:59.000Z

    A look into some of the remarkable work being done in the Weatherization Training program at Pennsylvania College. Penn College's program has served as the model for six other training centers in Pennsylvania alone.

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    E-Print Network [OSTI]

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  1. Federal Buildings Personnel Training Act of 2010

    Broader source: Energy.gov [DOE]

    On December 14, 2010, President Obama signed the Federal Buildings Personnel Training Act of 2010 into law. This legislation will have an important impact on Federal agency training programs geared...

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    Broader source: Energy.gov [DOE]

    The Nebraska Customized Job Training Advantage is a flexible job training program with grants from $800-$4000 per qualified new job. Additional grant funding may be available for jobs created in...

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    SciTech Connect (OSTI)

    NONE

    1998-02-01T23:59:59.000Z

    This handbook contains recommended training materials consistent with DOE standardized core radiological training material. These materials consist of a program management guide, instructor`s guide, student guide, and overhead transparencies.

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

    Steam Systems Training: Steam Systems April 16, 2014 - 6:31pm Addthis Learn about the diverse training sessions offered. The courses are taught by highly qualified instructors who...

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    E-Print Network [OSTI]

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    participants had received prior US training. The primaryassessment scores between training groups are depicted indifferences between the training groups’ FAST image

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    E-Print Network [OSTI]

    Jensen, Ric

    2008-01-01T23:59:59.000Z

    by the Texas Water Resources Institute (TWRI). TWRI is working with Texas A&M Uni- versity?s Spatial Sciences Laboratory (SSL), Zachry Department of Civil Engineering, and the Texas AgriLife Blackland Research and Extension Center at Temple to market...,? said Wurbs, who will teach the WRAP courses. ?Training courses allow practitioners to efficiently gain proficiency in applying new innovations in technology, computer modeling, and water management strategies.? Dr. Raghavan Srinivasan, SSL...

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    E-Print Network [OSTI]

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    E-Print Network [OSTI]

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    Safety Training Policy Virginia Tech Chemistry Department Approved by the Executive Committee on 06 at specific training sessions or programs is mandatory. Tenure-track faculty members may choose their level research are exempt, as their safety training is incorporated into their laboratory courses. The first step

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    ENVIRONMENT, SAFETY & HEALTH DIVISION Chapter 24: Training Quick Start Summary Product ID: 520-group.slac.stanford.edu/esh/eshmanual/references/trainingQuickstart.pdf 1 Who needs to know about these requirements The requirements of Training apply to all persons on-site, employees and non-employees, their SLAC

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    2011 TRAINING DATES January 10-12 March 1-3 April 11-13 June 7-9 July 26-28 September 6-8 November: Tools and Functionality Professional Development Training Course OVERVIEW ArcGIS Desktop II: Tools come- first serve basis. · The workshop registration cost is $650. Payment is due prior to the training

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    CPR/AED Training Payment Form This form must be completed and submitted along with payment in order to participate in TxClass PN 900 CPR/AED Training. Cost to participate is $30. Payment may be in the form of IDT account or check payable to UT Austin. Upon receipt of payment and completion of training class

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    E-Print Network [OSTI]

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    E-Print Network [OSTI]

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    MAKE THE RIGHT MOVE Corporate Training On-Site · Online · Global IMPROVE YOUR COMPETITIVE ADVANTAGE WITH WORLD-CLASS ON-SITE AND ONLINE SOLUTIONS TAILORED TO MEET YOUR BUSINESS AND EMPLOYEE TRAINING NEEDS a competitive advantage depends on how well your staff executes. UCIrvineExtension's Corporate Training helps

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    E-Print Network [OSTI]

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    DOE's BestPractices Steam End User Training Steam EndUser Training Resource Utilization End User Training Resource Utilization Analysis Module 1 June 28, 2010 #12; DOE's BestPractices Steam End User Training Slide 3 Fuel Selection 1 Fuel purchases typically dominate the operating cost

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    E-Print Network [OSTI]

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    Equality and Diversity E-training Guidance How do I access the training? You are already registered as a user on the system. You can access the training and save your progress in four quick steps. 1. Firstly, access the training through the following link: https://abdn.marshallacmtraining.co.uk/courselist. 2

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    E-Print Network [OSTI]

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    DOE's BestPractices Steam End User Training Steam End User Training Navigational Tutorial - 1 8/27/2010 Steam End User Training Navigational Tutorial Module Slide 1 ­ Introduction Hello, and welcome to the Steam End User Training. I would like to take a few minutes to show you how to navigate through

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    E-Print Network [OSTI]

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    ACADEMIC TRAINING FOR J-1 STUDENTS - 5 SAMPLE ADVISOR'S LETTER FOR ACADEMIC TRAINING must Services FROM: Name Title RE: Recommendation for Academic Training for ___________________________ DATE ____________________________ ______________________________________________________. This student has an opportunity to pursue academic training with the employer indicated below. I have discussed

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    E-Print Network [OSTI]

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    DOE's BestPractices Steam End User Training Steam End User Training Steam Generation Efficiency Module Efficiency Definition - 1 8/30/2010 Steam End-User Training Steam Generation Efficiency Module will be discussed. [Slide Visual ­ Contents of Module Sections] Banner: DOE's BestPractices Steam End User Training

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    E-Print Network [OSTI]

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    E-Print Network [OSTI]

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    E-Print Network [OSTI]

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    E-Print Network [OSTI]

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    Training History Report Training Services, Organizational Effectiveness/OHR · 612-626-1373 UMReports www.umn.edu/ohr/trainingservices 1-30-13 Following are the steps to view one's training history. A report will be run in UMReports which displays training courses for one Emplid or by department

  9. UMBC Training Centers Partners with EC-Council, to Deliver Online Cybersecurity Training Programs

    E-Print Network [OSTI]

    Maryland, Baltimore County, University of

    UMBC Training Centers Partners with EC-Council, to Deliver Online Cybersecurity Training Programs "iClasses offer Students the option of live, instructor lead online security training virtually anywhere with access to the internet." March 21, 2011 - UMBC Training Centers, long time partner of the EC

  10. DOE's BestPractices Steam End User Training Steam End User Training

    E-Print Network [OSTI]

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  11. How do I get my training transcripts? 1. HR Training Transcript

    E-Print Network [OSTI]

    Howitt, Ivan

    How do I get my training transcripts? 1. HR Training Transcript There are two ways to access your HR Training Transcript ­ either through Banner Self Service or 49er Express. I) Using Banner Self credentials, then select the "Employee" tab Select the "Human Resources Training Courses Completed" link II

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    E-Print Network [OSTI]

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    2004-09-30T23:59:59.000Z

    Due to a variety of reasons, one of the most common types of training found at companies is safety and health training. As part of a comprehensive health and safety training program there is usually an ergonomics training course. These courses...

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    E-Print Network [OSTI]

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    Training & Technology Solutions Queens College ~ Office of Converging Technologies ~ Training & Technology Solutions 718-997-4875 ~ training@qc.cuny.edu ~ I-Bldg 214 How to Pay Your Tuition Using E be navigated to your Student Center page. John Smith 23145678 John's Student Center #12;Training & Technology

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    E-Print Network [OSTI]

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    E-Print Network [OSTI]

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    E-Print Network [OSTI]

    Fig. 1 Training within the interdepartmental Biotechnology and Bioengineering Center (BBC). POSTDOCTORAL TRAINING PROGRAM OPPORTUNITIES BIOTECHNOLOGY AND BIOENGINEERING CENTER MEDICAL COLLEGE OF WISCONSIN o Contact Apply Overview Essential Program Features Training Program Activities Mentors (Training

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    E-Print Network [OSTI]

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  18. CRAD, Training - Los Alamos National Laboratory Waste Characterization...

    Office of Environmental Management (EM)

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  19. area doe training: Topics by E-print Network

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

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    E-Print Network [OSTI]

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