Sample records for observing system aos

  1. Aerosol Observing System (AOS) Handbook

    SciTech Connect (OSTI)

    Jefferson, A

    2011-01-17T23:59:59.000Z

    The Aerosol Observing System (AOS) is a suite of in situ surface measurements of aerosol optical and cloud-forming properties. The instruments measure aerosol properties that influence the earth’s radiative balance. The primary optical measurements are those of the aerosol scattering and absorption coefficients as a function of particle size and radiation wavelength and cloud condensation nuclei (CCN) measurements as a function of percent supersaturation. Additional measurements include those of the particle number concentration and scattering hygroscopic growth. Aerosol optical measurements are useful for calculating parameters used in radiative forcing calculations such as the aerosol single-scattering albedo, asymmetry parameter, mass scattering efficiency, and hygroscopic growth. CCN measurements are important in cloud microphysical models to predict droplet formation.

  2. Aerosol Observing Systems (AOS), New Capabilities for ASR Researchers Stephen R. Springston (srs@bnl.gov)

    E-Print Network [OSTI]

    of remote access over the internet allows mentors complete control over AOS infrastructure components to erect railing, sampling mast and instrument turn on) o Tolerance for heat/cold, wind o `Turtle' mode/off all subsystems allowing both remote and autonomous restart and shutdown of unit in graded steps o

  3. Air Observe System

    E-Print Network [OSTI]

    Alexander Bolonkin

    2007-01-10T23:59:59.000Z

    This manuscript contains a description and basic principles for observing inaccessible areas using low cost, easily deployed equipment. The basic premise is to suspend a tiny video camera at an altitude of 10 - 200 meters over the area to be surveyed. The TV camera supports at altitude by wind or balloon. The technical challenges regard the means by which the camera is suspended. Such a system may be used by military or police forces or by civil authorities for rescue missions or assessment of natural disasters. The method may be further developed for military applications by integrating the surveillance task with deployment of munitions. Key words: air observer, air suspended system, low altitude video observer.

  4. Stochastic Hybrid Systems with Renewal Transitions Duarte Antunes, Jo~ao P. Hespanha, and Carlos Silvestre

    E-Print Network [OSTI]

    Hespanha, João Pedro

    Stochastic Hybrid Systems with Renewal Transitions Duarte Antunes, Jo~ao P. Hespanha, and Carlos], which motivated us to refer to these systems as stochastic hybrid systems with renewal transitions Silvestre Abstract-- We consider Stochastic Hybrid Systems (SHSs) for which the lengths of times

  5. Design considerations of the AO module for the Gemini South multi-conjugate adaptive optics system

    E-Print Network [OSTI]

    Design considerations of the AO module for the Gemini South multi-conjugate adaptive optics system Observatory, 670 N. A'ohoku Place, Hilo, HI 96720 B. Optical Design Service, 8 S. Bella Vista Drive, Tucson optics system E. Jamesa , C. Boyera , R. A. Buchroederb , B.L. Ellerbroeka , M. Huntena a Gemini

  6. Performance of a MEMS-based AO-OCT system using Fourier Reconstruction

    SciTech Connect (OSTI)

    Evans, J; Zawadzki, R; Jones, S; Olivier, S; Werner, J S

    2009-01-21T23:59:59.000Z

    Adaptive optics (AO) and optical coherence tomography (OCT) are powerful imaging modalities that, when combined, can provide high-resolution (3.5 {micro}m isotropic), 3-D images of the retina. The AO-OCT system at UC Davis has demonstrated the utility of this technology for microscopic, volumetric, in vivo retinal imaging. The current system uses an AOptix bimorph deformable mirror (DM) for low-order, high-stroke correction and a 140-actuator Boston Micromachines DM for high-order correction. Developments to improve performance or functionality of the instrument are on-going. Based on previous work in system characterization we have focused on improved AO control. We present preliminary results and remaining challenges for a newly implemented Fourier transform reconstructor (FTR). The previously reported error budget analysis is also reviewed and updated, with consideration of how to improve both the amount of residual error and the robustness of the system. Careful characterization of the AO system will lead to improved performance and inform the design of future systems.

  7. Methanol Masers Observations in the 3-mm Bandwidth at the Radio Telescope RT-22 CrAO

    E-Print Network [OSTI]

    S. Yu. Zubrin; A. V. Antyufeyev; V. V. Myshenko; V. M. Shulga

    2007-12-10T23:59:59.000Z

    We report the beginning of the astronomical masers investigations in the 3-mm bandwidth at the radio telescope RT-22 (CrAO, Ukraine). For this purpose the special complex for maser lines investigation in 85...115 GHz frequency band is developed. It is made on the base of the low noise cryogenic Shottky-diode receiver and the high resolution Fourier-spectrometer. The cryogenic receiver has the DSB noise temperature less than 100K. The spectral channel separation of the Fourier-spectrometer is about 4kHz and the spectrometer bandwidth is 8 MHz. Results of maser observations of 8$^{0}-7^{1} $A$^{+}$ transition of methanol (95.169 GHz) towards DR-21(OH), DR-21W and NGC7538 are in good agreement with early obtained results by other authors. On the basis of the analysis of the location of masers in the NGC7538 direction we can assume that the origin of all known class I methanol masers in this region is connected with existing molecular outflows from young stars.

  8. Aerosol observing system platform integration and AAF instrumentation

    SciTech Connect (OSTI)

    Springston, S.; Sedlacek, A.

    2010-03-15T23:59:59.000Z

    As part of the federal government’s 2009 American Recovery and Reinvestment Act (ARRA), the U.S. DOE Office of Science allocated funds for the capital upgrade of the Atmospheric Radiation Measurement (ARM) Climate Research Facility to improve and expand observational capabilities related to cloud and aerosol properties. The ARM Facility was established as a national user facility for the global scientific community to conduct a wide range of interdisciplinary science. Part of the ARRA-funded expansion of the ARM Facility includes four new Aerosol Observing Systems (AOS) to be designed, instrumented, and mentored by BNL. The enclosures will be customized SeaTainers. These new platforms ([AMF2]: ARM Mobile Facility-2; [TWP-D]: Tropical Western Pacific at Darwin; and [MAOS-A]/[MAOS-C]: Mobile Aerosol Observing System-Aerosol/-Chemistry) will provide a laboratory environment for fielding instruments to collect data on aerosol life cycle, microphysics, and optical/physical properties. The extensive instrument suite includes both established methods and initial deployments of new techniques to add breadth and depth to the AOS data sets. The platforms are designed: (1) to have all instruments pre-installed before deployment, allowing a higher measurement duty cycle; (2) with a standardized configuration improving the robustness of data inter-comparability; (3) to provide remote access capability for instrument mentors; and (4) to readily accommodate guest instrumentation. The first deployment of the AMF2 platform will be at the upcoming StormVEx campaign held at Steamboat Springs, Colorado, October 15, 2010–March 31, 2011 while the TWP-D AOS will be stationed at the ARM Darwin site. The maiden deployments of the MAOS-A and MAOS-C platforms will be during the Ganges Valley Experiment (GVAX) scheduled for April 2011–April 2012. In addition to the ground-based AOS platforms, thee major instrument builds for the AAF are also being undertaken (new trace gas package [NO, NOx, NOy, CO, O3, and SO2]; Scanning Mobility Particle Sampler [SMPS]; and Particle into Liquid Sampler [PILS]). The current status of the AOS platforms, instrument suites, instituted QA/QC activities, projected AOS VAPs, and inlet design, as well as still-unresolved issues, will be presented.

  9. SEU induced errors observed in microprocessor systems

    SciTech Connect (OSTI)

    Asenek, V.; Underwood, C.; Oldfield, M. [Univ. of Surrey, Guildford (United Kingdom). Surrey Space Centre] [Univ. of Surrey, Guildford (United Kingdom). Surrey Space Centre; Velazco, R.; Rezgui, S.; Cheynet, P. [TIMA Lab., Grenoble (France)] [TIMA Lab., Grenoble (France); Ecoffet, R. [Centre National d`Etudes Spatiales, Toulouse (France)] [Centre National d`Etudes Spatiales, Toulouse (France)

    1998-12-01T23:59:59.000Z

    In this paper, the authors present software tools for predicting the rate and nature of observable SEU induced errors in microprocessor systems. These tools are built around a commercial microprocessor simulator and are used to analyze real satellite application systems. Results obtained from simulating the nature of SEU induced errors are shown to correlate with ground-based radiation test data.

  10. Surface Meteorological Observation System (SMOS) Handbook

    SciTech Connect (OSTI)

    Ritsche, MT

    2008-03-01T23:59:59.000Z

    The Surface Meteorological Observation System (SMOS) mostly uses conventional in situ sensors to obtain 1-minute, 30-minute, and 1440-minute (daily) averages of surface wind speed, wind direction, air temperature, relative humidity (RH), barometric pressure, and precipitation at the Central Facility and many of the extended facilities of the Southern Great Plains (SGP) climate research site. The SMOSs are not calibrated as systems. The sensors and the data logger (which includes the analog-to-digital converter, or A/D) are calibrated separately. All systems are installed using components that have a current calibration. SMOSs have not been installed at extended facilities located within about 10 km of existing surface meteorological stations, such as those of the Oklahoma Mesonet. The Surface Meteorological Observation Systems are used to create climatology for each particular location, and to verify the output of numerical weather forecast and other model output. They are also used to “ground-truth” other remote sensing equipment.

  11. First Light Curve Analyses of Binary Systems AO Aqr, CW Aqr and ASAS 012206-4924.7

    E-Print Network [OSTI]

    Ulas, Burak

    2015-01-01T23:59:59.000Z

    Using the data from the public database of the All Sky Automated Survey ({\\tt ASAS}) we performed the very first light curve analyses of the three eclipsing binary systems \\astrobj{AO~Aqr}, \\astrobj{CW~Aqr} and \\astrobj{ASAS~012206-4924.7}. The physical parameters of the systems were determined by the {\\tt PHOEBE} software. From an analysis of the ASAS data it was concluded that AO~Aqr was found to be a contact binary system while CW~Aqr and ASAS~012206-4924.7 were found to be near--contact and detached binaries, respectively. Finally, the locations of the components, corresponding to the estimated physical parameters, in the HR diagram were also discussed.

  12. The web-PLOP observation prioritisation system

    E-Print Network [OSTI]

    Colin Snodgrass; Yiannis Tsapras; Rachel Street; Daniel Bramich; Keith Horne; Martin Dominik; Alasdair Allan

    2008-05-14T23:59:59.000Z

    We present a description of the automated system used by RoboNet to prioritise follow up observations of microlensing events to search for planets. The system keeps an up-to-date record of all public data from OGLE and MOA together with any existing RoboNet data and produces new PSPL fits whenever new data arrives. It then uses these fits to predict the current or future magnitudes of events, and selects those to observe which will maximise the probability of detecting planets for a given telescope and observing time. The system drives the RoboNet telescopes automatically based on these priorities, but it is also designed to be used interactively by human observers. The prioritisation options, such as telescope/instrument parameters, observing conditions and available time can all be controlled via a web-form, and the output target list can also be customised and sorted to show the parameters that the user desires. The interactive interface is available at http://www.artemis-uk.org/web-PLOP/

  13. Common Cyber Security Vulnerabilities Observed in Control System...

    Energy Savers [EERE]

    Common Cyber Security Vulnerabilities Observed in Control System Assessments by the INL NSTB Program Common Cyber Security Vulnerabilities Observed in Control System Assessments by...

  14. The Observers' Paradox: Apparent Computational Complexity in Physical Systems

    E-Print Network [OSTI]

    Pollack, Jordan B.

    The Observers' Paradox: Apparent Computational Complexity in Physical Systems John F. Kolen Research Department of Computer and Information Sciences The Ohio State University Columbus, OH 43210 kolen

  15. ao cateter vesical: Topics by E-print Network

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    image at NASA Ames testbed (R. Belikov group) 12;12;Subaru facility Adaptive Optics System (AO1 The Subaru Coronagraphic Extreme-AO (SCExAO) system Olivier Guyon (Subaru...

  16. acidentalmente ao cesio-137: Topics by E-print Network

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    image at NASA Ames testbed (R. Belikov group) 12;12;Subaru facility Adaptive Optics System (AO1 The Subaru Coronagraphic Extreme-AO (SCExAO) system Olivier Guyon (Subaru...

  17. ao residuo solido: Topics by E-print Network

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    image at NASA Ames testbed (R. Belikov group) 12;12;Subaru facility Adaptive Optics System (AO1 The Subaru Coronagraphic Extreme-AO (SCExAO) system Olivier Guyon (Subaru...

  18. ao estresse agudo: Topics by E-print Network

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    image at NASA Ames testbed (R. Belikov group) 12;12;Subaru facility Adaptive Optics System (AO1 The Subaru Coronagraphic Extreme-AO (SCExAO) system Olivier Guyon (Subaru...

  19. ao destino comum: Topics by E-print Network

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    image at NASA Ames testbed (R. Belikov group) 12;12;Subaru facility Adaptive Optics System (AO1 The Subaru Coronagraphic Extreme-AO (SCExAO) system Olivier Guyon (Subaru...

  20. ao abastecimento publico: Topics by E-print Network

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    image at NASA Ames testbed (R. Belikov group) 12;12;Subaru facility Adaptive Optics System (AO1 The Subaru Coronagraphic Extreme-AO (SCExAO) system Olivier Guyon (Subaru...

  1. associados aos enfezamentos: Topics by E-print Network

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    image at NASA Ames testbed (R. Belikov group) 12;12;Subaru facility Adaptive Optics System (AO1 The Subaru Coronagraphic Extreme-AO (SCExAO) system Olivier Guyon (Subaru...

  2. atinente ao gas: Topics by E-print Network

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    image at NASA Ames testbed (R. Belikov group) 12;12;Subaru facility Adaptive Optics System (AO1 The Subaru Coronagraphic Extreme-AO (SCExAO) system Olivier Guyon (Subaru...

  3. associado ao arroz: Topics by E-print Network

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    image at NASA Ames testbed (R. Belikov group) 12;12;Subaru facility Adaptive Optics System (AO1 The Subaru Coronagraphic Extreme-AO (SCExAO) system Olivier Guyon (Subaru...

  4. alternativa ao bioensaio: Topics by E-print Network

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    image at NASA Ames testbed (R. Belikov group) 12;12;Subaru facility Adaptive Optics System (AO1 The Subaru Coronagraphic Extreme-AO (SCExAO) system Olivier Guyon (Subaru...

  5. aos bloqueios nervosos: Topics by E-print Network

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    image at NASA Ames testbed (R. Belikov group) 12;12;Subaru facility Adaptive Optics System (AO1 The Subaru Coronagraphic Extreme-AO (SCExAO) system Olivier Guyon (Subaru...

  6. associado ao lenho: Topics by E-print Network

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    image at NASA Ames testbed (R. Belikov group) 12;12;Subaru facility Adaptive Optics System (AO1 The Subaru Coronagraphic Extreme-AO (SCExAO) system Olivier Guyon (Subaru...

  7. ao corante azul: Topics by E-print Network

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    image at NASA Ames testbed (R. Belikov group) 12;12;Subaru facility Adaptive Optics System (AO1 The Subaru Coronagraphic Extreme-AO (SCExAO) system Olivier Guyon (Subaru...

  8. ao dirigir alcoolizado: Topics by E-print Network

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    image at NASA Ames testbed (R. Belikov group) 12;12;Subaru facility Adaptive Optics System (AO1 The Subaru Coronagraphic Extreme-AO (SCExAO) system Olivier Guyon (Subaru...

  9. ao desgaste erosivo: Topics by E-print Network

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    image at NASA Ames testbed (R. Belikov group) 12;12;Subaru facility Adaptive Optics System (AO1 The Subaru Coronagraphic Extreme-AO (SCExAO) system Olivier Guyon (Subaru...

  10. ao fansidar quinina: Topics by E-print Network

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    image at NASA Ames testbed (R. Belikov group) 12;12;Subaru facility Adaptive Optics System (AO1 The Subaru Coronagraphic Extreme-AO (SCExAO) system Olivier Guyon (Subaru...

  11. aos herbicidas inibidores: Topics by E-print Network

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    image at NASA Ames testbed (R. Belikov group) 12;12;Subaru facility Adaptive Optics System (AO1 The Subaru Coronagraphic Extreme-AO (SCExAO) system Olivier Guyon (Subaru...

  12. ao referencial discursivo: Topics by E-print Network

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    image at NASA Ames testbed (R. Belikov group) 12;12;Subaru facility Adaptive Optics System (AO1 The Subaru Coronagraphic Extreme-AO (SCExAO) system Olivier Guyon (Subaru...

  13. ao tolueno estireno: Topics by E-print Network

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    image at NASA Ames testbed (R. Belikov group) 12;12;Subaru facility Adaptive Optics System (AO1 The Subaru Coronagraphic Extreme-AO (SCExAO) system Olivier Guyon (Subaru...

  14. associados ao envolvimento: Topics by E-print Network

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    image at NASA Ames testbed (R. Belikov group) 12;12;Subaru facility Adaptive Optics System (AO1 The Subaru Coronagraphic Extreme-AO (SCExAO) system Olivier Guyon (Subaru...

  15. aos tumores selares: Topics by E-print Network

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    image at NASA Ames testbed (R. Belikov group) 12;12;Subaru facility Adaptive Optics System (AO1 The Subaru Coronagraphic Extreme-AO (SCExAO) system Olivier Guyon (Subaru...

  16. associados ao sedentarismo: Topics by E-print Network

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    image at NASA Ames testbed (R. Belikov group) 12;12;Subaru facility Adaptive Optics System (AO1 The Subaru Coronagraphic Extreme-AO (SCExAO) system Olivier Guyon (Subaru...

  17. adaptada ao fechamento: Topics by E-print Network

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    image at NASA Ames testbed (R. Belikov group) 12;12;Subaru facility Adaptive Optics System (AO1 The Subaru Coronagraphic Extreme-AO (SCExAO) system Olivier Guyon (Subaru...

  18. ao material insuficiente: Topics by E-print Network

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    image at NASA Ames testbed (R. Belikov group) 12;12;Subaru facility Adaptive Optics System (AO1 The Subaru Coronagraphic Extreme-AO (SCExAO) system Olivier Guyon (Subaru...

  19. associado ao superbrotamento: Topics by E-print Network

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    image at NASA Ames testbed (R. Belikov group) 12;12;Subaru facility Adaptive Optics System (AO1 The Subaru Coronagraphic Extreme-AO (SCExAO) system Olivier Guyon (Subaru...

  20. alternativas ao dirigir: Topics by E-print Network

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    image at NASA Ames testbed (R. Belikov group) 12;12;Subaru facility Adaptive Optics System (AO1 The Subaru Coronagraphic Extreme-AO (SCExAO) system Olivier Guyon (Subaru...

  1. alternativas habitacionais ao: Topics by E-print Network

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    image at NASA Ames testbed (R. Belikov group) 12;12;Subaru facility Adaptive Optics System (AO1 The Subaru Coronagraphic Extreme-AO (SCExAO) system Olivier Guyon (Subaru...

  2. associados ao excesso: Topics by E-print Network

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    image at NASA Ames testbed (R. Belikov group) 12;12;Subaru facility Adaptive Optics System (AO1 The Subaru Coronagraphic Extreme-AO (SCExAO) system Olivier Guyon (Subaru...

  3. ao desgaste abrasivo: Topics by E-print Network

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    image at NASA Ames testbed (R. Belikov group) 12;12;Subaru facility Adaptive Optics System (AO1 The Subaru Coronagraphic Extreme-AO (SCExAO) system Olivier Guyon (Subaru...

  4. associados ao sobrepeso: Topics by E-print Network

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    image at NASA Ames testbed (R. Belikov group) 12;12;Subaru facility Adaptive Optics System (AO1 The Subaru Coronagraphic Extreme-AO (SCExAO) system Olivier Guyon (Subaru...

  5. ao desmame precoce: Topics by E-print Network

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    image at NASA Ames testbed (R. Belikov group) 12;12;Subaru facility Adaptive Optics System (AO1 The Subaru Coronagraphic Extreme-AO (SCExAO) system Olivier Guyon (Subaru...

  6. ao desfolhamento afetada: Topics by E-print Network

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    image at NASA Ames testbed (R. Belikov group) 12;12;Subaru facility Adaptive Optics System (AO1 The Subaru Coronagraphic Extreme-AO (SCExAO) system Olivier Guyon (Subaru...

  7. associado ao aspirado: Topics by E-print Network

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    image at NASA Ames testbed (R. Belikov group) 12;12;Subaru facility Adaptive Optics System (AO1 The Subaru Coronagraphic Extreme-AO (SCExAO) system Olivier Guyon (Subaru...

  8. ao preparo convencional: Topics by E-print Network

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    image at NASA Ames testbed (R. Belikov group) 12;12;Subaru facility Adaptive Optics System (AO1 The Subaru Coronagraphic Extreme-AO (SCExAO) system Olivier Guyon (Subaru...

  9. ao estresse salino: Topics by E-print Network

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    image at NASA Ames testbed (R. Belikov group) 12;12;Subaru facility Adaptive Optics System (AO1 The Subaru Coronagraphic Extreme-AO (SCExAO) system Olivier Guyon (Subaru...

  10. ao seguimento preconizado: Topics by E-print Network

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    image at NASA Ames testbed (R. Belikov group) 12;12;Subaru facility Adaptive Optics System (AO1 The Subaru Coronagraphic Extreme-AO (SCExAO) system Olivier Guyon (Subaru...

  11. Navigation System for Ground Vehicles using Temporally Interconnected Observers

    E-Print Network [OSTI]

    navigation technique for an automotive vehicle. This method involves several observers, each designed for a particular type of trajectory, that are turned on and off according to a switching policy. Each observer of observer design of vehicular systems. A typical example of such practices1 is found in the navigation

  12. Version 3.0 Earth Observing System (EOS)

    E-Print Network [OSTI]

    Waliser, Duane E.

    D-33192 Version 3.0 Earth Observing System (EOS) Tropospheric Emission Spectrometer (TES) Data_04 Data November 5, 2007 Version 3.0 ii Earth Observing System (EOS) Tropospheric Emission Spectrometer Jet Propulsion Laboratory #12;TES Validation Report ­ Version F04_04 Data November 5, 2007 Version 3.0

  13. DESIGN OF THE GREAT LAKES OBSERVING SYSTEM ENTERPRISE ARCHITECTURE

    E-Print Network [OSTI]

    DESIGN OF THE GREAT LAKES OBSERVING SYSTEM ENTERPRISE ARCHITECTURE T.J. Dekker1 , J.V. DePinto1 , S, collaborative, and consensus-based enterprise architecture design process was conducted under the direction that will achieve an integrated, comprehensive, and sustainable observing system enterprise for the Great Lakes

  14. Seismic Observation Systems in Nagoya University and Publication of Data

    E-Print Network [OSTI]

    Southern California, University of

    Seismic Observation Systems in Nagoya University and Publication of Data Nobuo Fukuwa,a) Jun Tobita,b) and Hiroaki Kojimac) This paper reports the current situation of the seismic monitoring program conducted by Nagoya University. First, the system for observing seismic ground motion in the Tokai Region is described

  15. Rule-based system architecting of Earth observation satellite systems

    E-Print Network [OSTI]

    Selva Valero, Daniel

    2012-01-01T23:59:59.000Z

    System architecting is concerned with exploring the tradespace of early, high-level, system design decisions with a holistic, value-centric view. In the last few years, several tools and methods have been developed to ...

  16. Integrating spacecraft and aircraft in Earth Observation System architectures

    E-Print Network [OSTI]

    Suarez, Brandon H

    2011-01-01T23:59:59.000Z

    The Global Earth Observation System (GEOS) is the essential data gathering network that enables the advancement of Earth science. In recent years, efforts have been made to understand the major GEOS architectural tradeoffs. ...

  17. A cooperative control algorithm for camera based observational systems.

    SciTech Connect (OSTI)

    Young, Joseph G.

    2012-01-01T23:59:59.000Z

    Over the last several years, there has been considerable growth in camera based observation systems for a variety of safety, scientific, and recreational applications. In order to improve the effectiveness of these systems, we frequently desire the ability to increase the number of observed objects, but solving this problem is not as simple as adding more cameras. Quite often, there are economic or physical restrictions that prevent us from adding additional cameras to the system. As a result, we require methods that coordinate the tracking of objects between multiple cameras in an optimal way. In order to accomplish this goal, we present a new cooperative control algorithm for a camera based observational system. Specifically, we present a receding horizon control where we model the underlying optimal control problem as a mixed integer linear program. The benefit of this design is that we can coordinate the actions between each camera while simultaneously respecting its kinematics. In addition, we further improve the quality of our solution by coupling our algorithm with a Kalman filter. Through this integration, we not only add a predictive component to our control, but we use the uncertainty estimates provided by the filter to encourage the system to periodically observe any outliers in the observed area. This combined approach allows us to intelligently observe the entire region of interest in an effective and thorough manner.

  18. OBSERVING LYAPUNOV EXPONENTS OF INFINITE-DIMENSIONAL DYNAMICAL SYSTEMS

    E-Print Network [OSTI]

    Ott, William

    OBSERVING LYAPUNOV EXPONENTS OF INFINITE-DIMENSIONAL DYNAMICAL SYSTEMS WILLIAM OTT, MAURICIO A. RIVAS, AND JAMES WEST Abstract. Can the Lyapunov exponents of infinite-dimensional dynamical systems spaces generated by evolution partial differential equations. Contents 1. Introduction 1 1.1. Lyapunov

  19. Internal and Boundary Observability Estimates for the Heterogeneous Maxwell's System

    SciTech Connect (OSTI)

    Nicaise, Serge [Universite de Valenciennes et du Hainaut Cambresis, MACS, Institut des Sciences et Techniques de Valenciennes, 59313 Valenciennes Cedex 9 (France)], E-mail: snicaise@univ-valenciennes.fr; Pignotti, Cristina [Dipartimento di Matematica Pura e Applicata, Universita di L'Aquila, Via Vetoio, Loc. Coppito, 67010 L'Aquila (Italy)], E-mail: pignotti@univqaq.it

    2006-06-15T23:59:59.000Z

    Observability estimates for Maxwell's system with variable coefficients are established using the differential geometry method recently developed for scalar wave equations.The main tool is that Maxwell's system is reducible to a perturbed vectorial wave equation with a decoupled principal part.

  20. Time evolution of observable properties of parametrized systems

    E-Print Network [OSTI]

    P. Hajicek

    1996-12-18T23:59:59.000Z

    A short review of some recent work on the problem of time and of observables for the reparametrization invariant systems is given. A talk presented at the Second Meeting on Constraint Dynamics and Quantum Gravity at Santa Marguerita Ligure, September 17--21 1996.

  1. Design of coherent quantum observers for linear quantum systems

    E-Print Network [OSTI]

    Shanon L. Vuglar; Hadis Amini

    2015-01-27T23:59:59.000Z

    Quantum versions of control problems are often more difficult than their classical counterparts because of the additional constraints imposed by quantum dynamics. For example, the quantum LQG and quantum H infinity optimal control problems remain open. To make further progress, new, systematic and tractable methods need to be developed. This paper gives three algorithms for designing coherent observers, i.e., quantum systems that are connected to a quantum plant and their outputs provide information about the internal state of the plant. Importantly, coherent observers avoid measurements of the plant outputs. We compare our coherent observers with a classical (measurement-based) observer by way of an example involving an optical cavity with thermal and vacuum noises as inputs.

  2. ExAO for GMT Olivier Guyon

    E-Print Network [OSTI]

    Guyon, Olivier

    -AO system can be small and cheap ­ does not scale up with telescope size BUT: instrument suite can drive up). Putting a coronagraph on a non-ExAO system which was build for general purpose science doesn't work well to build anything that would work on a telescope. By the time they build something, it won't work

  3. Collaborative process control: Observation of tracks generated by PLM system

    E-Print Network [OSTI]

    Elkadiri, Soumaya; Delattre, Miguel; Bouras, Abdelaziz

    2008-01-01T23:59:59.000Z

    This paper aims at analyzing the problems related to collaborative work using a PLM system. This research is mainly focused on the organisational aspects of SMEs involved in networks composed of large companies, subcontractors and other industrial partners. From this analysis, we propose the deployment of an approach based on an observation process of tracks generated by PLM system. The specific contributions are of two fold. First is to identify the brake points of collaborative work. The second, thanks to the exploitation of generated tracks, it allows reducing risks by reacting in real time to the incidents or dysfunctions that may occur. The overall system architecture based on services technology and supporting the proposed approach is described, as well as associated prototype developed using an industrial PLM system.

  4. Algorithms, Protocols & Systems for Remote Observation Using Networked Robotic Cameras

    E-Print Network [OSTI]

    Qin, Ni

    2010-01-16T23:59:59.000Z

    assist in waste cleanup using Point- and-Direct (PAD) commands. Users point to cleanup locations in a shared image and a robot excavates each location in turn. Recent developments in MOSR systems can be found in [26,27]. In [27] Goldberg et al. propose...ALGORITHMS, PROTOCOLS AND SYSTEMS FOR REMOTE OBSERVATION USING NETWORKED ROBOTIC CAMERAS A Dissertation by NI QIN Submitted to the O?ce of Graduate Studies of Texas A&M University in partial fulflllment of the requirements for the degree of DOCTOR...

  5. ao parto 1999-2001: Topics by E-print Network

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

    image at NASA Ames testbed (R. Belikov group) 12;12;Subaru facility Adaptive Optics System (AO1 The Subaru Coronagraphic Extreme-AO (SCExAO) system Olivier Guyon (Subaru...

  6. ao estadiamento pre-operatorio: Topics by E-print Network

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

    image at NASA Ames testbed (R. Belikov group) 12;12;Subaru facility Adaptive Optics System (AO1 The Subaru Coronagraphic Extreme-AO (SCExAO) system Olivier Guyon (Subaru...

  7. auto-anticorpos dirigidos ao: Topics by E-print Network

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

    image at NASA Ames testbed (R. Belikov group) 12;12;Subaru facility Adaptive Optics System (AO1 The Subaru Coronagraphic Extreme-AO (SCExAO) system Olivier Guyon (Subaru...

  8. ao herbicida amonio-glufosinate: Topics by E-print Network

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

    image at NASA Ames testbed (R. Belikov group) 12;12;Subaru facility Adaptive Optics System (AO1 The Subaru Coronagraphic Extreme-AO (SCExAO) system Olivier Guyon (Subaru...

  9. ao cancro mini-mac: Topics by E-print Network

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

    image at NASA Ames testbed (R. Belikov group) 12;12;Subaru facility Adaptive Optics System (AO1 The Subaru Coronagraphic Extreme-AO (SCExAO) system Olivier Guyon (Subaru...

  10. Observational Techniques for Detecting Planets in Binary Systems

    E-Print Network [OSTI]

    Matthew W. Muterspaugh; Maciej Konacki; Benjamin F. Lane; Eric Pfahl

    2007-05-21T23:59:59.000Z

    Searches for planets in close binary systems explore the degree to which stellar multiplicity inhibits or promotes planet formation. There is a degeneracy between planet formation models when only systems with single stars are studied--several mechanisms appear to be able to produce such a final result. This degeneracy is lifted by searching for planets in binary systems; the resulting detections (or evidence of non-existence) of planets in binaries isolates which models may contribute to how planets form in nature. In this chapter, we consider observational efforts to detect planetary companions to binary stars in two types of hierarchical planet-binary configurations: first ``S-type'' planets which orbit just one of the stars, with the binary period being much longer than the planet's; second, ``P-type'' or circumbinary planets, where the planet simultaneously orbits both stars, and the planetary orbital period is much longer than that of the binary. The S-type planet finding techniques are different for binaries that can or cannot be spatially resolved. For wider systems, techniques reviewed include dualstar interferometric differential astrometry and precision radial velocities. Alternatively, unresolved binaries can be studied using modified dualstar "PHASES-style" differential astrometry or a modification of the radial velocity technique for composite spectra. Should a fortunately aligned--but still long period--binary be found, eclipse timing can also reveal the presence of S-type planets. Methods for detecting P-type planets include the composite-spectra variant of the radial velocity technique and eclipse timing.

  11. Thermodynamic properties of mesoscale convective systems observed during BAMEX

    SciTech Connect (OSTI)

    Correia, James; Arritt, R.

    2008-11-01T23:59:59.000Z

    Dropsonde observations from the Bow-echo and Mesoscale convective vortex EXperiment (BAMEX) are used to document the spatio-temporal variability of temperature, moisture and wind within mesoscale convective systems (MCSs). Onion type sounding structures are found throughout the stratiform region of MCSs but the temperature and moisture variability is large. Composite soundings were constructed and statistics of thermodynamic variability were generated within each sub-region of the MCS. The calculated air vertical velocity helped identify subsaturated downdrafts. We found that lapse rates within the cold pool varied markedly throughout the MCS. Layered wet bulb potential temperature profiles seem to indicate that air within the lowest several km comes from a variety of source regions. We also found that lapse rate transitions across the 0 C level were more common than isothermal, melting layers. We discuss the implications these findings have and how they can be used to validate future high resolution numerical simulations of MCSs.

  12. Observations

    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 RenewableSpeeding accessSpeeding access(SC)Gas and OilPhaseObservation of aof

  13. Observability Criteria and Estimator Design for Stochastic Linear Hybrid Systems

    E-Print Network [OSTI]

    Gummadi, Ramakrishna

    . Alessandri and Coletta [5] proposed a Luenberger observer design methodology for deterministic linear hybrid

  14. A satellite ocean color observation operator system for eutrophication assessment in coastal waters

    E-Print Network [OSTI]

    Fontana, Clément

    A satellite ocean color observation operator system for eutrophication assessment in coastal waters: Satellite ocean color Observation operator Eutrophication Remote sensing Radiative transfer modeling

  15. aos seus limites: Topics by E-print Network

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

    performance via correction of atmospheric turbulence using adaptive optics (AO), to seeing-limited observations. Moreover, the scientific output of the...

  16. aos limites prescritos: Topics by E-print Network

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

    performance via correction of atmospheric turbulence using adaptive optics (AO), to seeing-limited observations. Moreover, the scientific output of the...

  17. Antenna system characteristic and solar radio burst observation

    E-Print Network [OSTI]

    Li, Sha; Chen, Zhijun; Wang, Wei; Liu, Donghao

    2015-01-01T23:59:59.000Z

    Chinese Spectral Radio Heliograph (CSRH) is an advanced aperture synthesis solar radio heliograph, developed by National Astronomical Observatories, Chinese Academy of Sciences independently. It consists of 100 reflector antennas, which are grouped into two antenna arrays (CSRH-I and CSRH-II) for low and high frequency bands respectively. The frequency band of CSRH-I is 0.4-2GHz and for CSRH-II, the frequency band is 2-15GHz. In the antenna and feed system, CSRH uses an Eleven feed to receive signals coming from the Sun, the radiation pattern with lower side lobe and back lobe of the feed is well radiated. The characteristics of gain G and antenna noise temperature T effect the quality of solar radio imaging. For CSRH, measured G is larger than 60 dBi and $ T $ is less than 120K, after CSRH-I was established, we have successfully captured a solar radio burst between 1.2-1.6GHz on November 12, 2010 through this instrument and this event was confirmed through the observation of Solar Broadband Radio Spectromete...

  18. On Optimal Control of a Class of Partially-Observed Discrete Event Systems

    E-Print Network [OSTI]

    Paris-Sud XI, Université de

    On Optimal Control of a Class of Partially-Observed Discrete Event Systems H e rv M a rch a n d theC-observer. Thissubmachineleadstothedesiredsupervisorforthesystem. Keywords: DiscreteEventSystems,SupervisoryControlProblem,Optimality(not) be reached in the controlled system, the Optimal Control under Par- tial Observation problem is solved

  19. Estimation of the WECC System Inertia Using Observed Frequency Transients

    E-Print Network [OSTI]

    David P. Chassin; Zhenyu Huang; Matthew K. Donnelly; Candee Hassler; Enrique Ramirez; Cody Ray

    2004-12-28T23:59:59.000Z

    Computer models being developed to understand the interaction between demand-response technology, power system deregulation and market transformation depend in part on understanding the relationship between system frequency and load-control. Frequency, load, and plant outage events data collected over the last several years have permitted analysis to determine the Western Electricity Coordination Council (WECC) system's inertia during each event. This data was used to evaluate the relationship of system inertia to total load, which is used to model system response to load curtailment programs in next generation power system simulations.

  20. OBSERVED HYBRID OSCILLATIONS IN AN ELECTRICAL DISTRIBUTION SYSTEM Vaibhav Donde

    E-Print Network [OSTI]

    . 1 therefore provide an example of a hybrid limit cycle.1 Analysis of power system large disturbance-changing transformers and switched capacitors. Analysis required a hybrid systems framework, due to the non from usual power system oscillations [1]: 1) behav- iour was quite non-smooth, and 2) the oscillation

  1. Mathematical strategies for filtering complex systems: Regularly spaced sparse observations

    SciTech Connect (OSTI)

    Harlim, J. [Department of Mathematics and Center for Atmosphere and Ocean Science, Courant Institute of Mathematical Sciences, New York University, 251 Mercer Street, New York, NY 10012 (United States)], E-mail: jharlim@cims.nyu.edu; Majda, A.J. [Department of Mathematics and Center for Atmosphere and Ocean Science, Courant Institute of Mathematical Sciences, New York University, 251 Mercer Street, New York, NY 10012 (United States)

    2008-05-01T23:59:59.000Z

    Real time filtering of noisy turbulent signals through sparse observations on a regularly spaced mesh is a notoriously difficult and important prototype filtering problem. Simpler off-line test criteria are proposed here as guidelines for filter performance for these stiff multi-scale filtering problems in the context of linear stochastic partial differential equations with turbulent solutions. Filtering turbulent solutions of the stochastically forced dissipative advection equation through sparse observations is developed as a stringent test bed for filter performance with sparse regular observations. The standard ensemble transform Kalman filter (ETKF) has poor skill on the test bed and even suffers from filter divergence, surprisingly, at observable times with resonant mean forcing and a decaying energy spectrum in the partially observed signal. Systematic alternative filtering strategies are developed here including the Fourier Domain Kalman Filter (FDKF) and various reduced filters called Strongly Damped Approximate Filter (SDAF), Variance Strongly Damped Approximate Filter (VSDAF), and Reduced Fourier Domain Kalman Filter (RFDKF) which operate only on the primary Fourier modes associated with the sparse observation mesh while nevertheless, incorporating into the approximate filter various features of the interaction with the remaining modes. It is shown below that these much cheaper alternative filters have significant skill on the test bed of turbulent solutions which exceeds ETKF and in various regimes often exceeds FDKF, provided that the approximate filters are guided by the off-line test criteria. The skill of the various approximate filters depends on the energy spectrum of the turbulent signal and the observation time relative to the decorrelation time of the turbulence at a given spatial scale in a precise fashion elucidated here.

  2. Observational Analysis of the Predictability of Mesoscale Convective Systems ISRAEL L. JIRAK AND WILLIAM R. COTTON

    E-Print Network [OSTI]

    Observational Analysis of the Predictability of Mesoscale Convective Systems ISRAEL L. JIRAK (Manuscript received 30 December 2005, in final form 4 October 2006) ABSTRACT Mesoscale convective systems of usefulness in operational forecasting. 1. Introduction Mesoscale convective systems (MCSs) frequently de

  3. ao controle quimico: Topics by E-print Network

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

    with Coherent Light Physics Websites Summary: : Exoplanets, Coronagraphy, Adaptive Optics 1. SUBARU CORONAGRAPHIC EXTREME-AO SYSTEM OVERVIEW The Subaru takes advantage of the...

  4. assistencia ao controle: Topics by E-print Network

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

    with Coherent Light Physics Websites Summary: : Exoplanets, Coronagraphy, Adaptive Optics 1. SUBARU CORONAGRAPHIC EXTREME-AO SYSTEM OVERVIEW The Subaru takes advantage of the...

  5. ao controle automatico: Topics by E-print Network

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

    with Coherent Light Physics Websites Summary: : Exoplanets, Coronagraphy, Adaptive Optics 1. SUBARU CORONAGRAPHIC EXTREME-AO SYSTEM OVERVIEW The Subaru takes advantage of the...

  6. aplicado ao controle: Topics by E-print Network

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

    with Coherent Light Physics Websites Summary: : Exoplanets, Coronagraphy, Adaptive Optics 1. SUBARU CORONAGRAPHIC EXTREME-AO SYSTEM OVERVIEW The Subaru takes advantage of the...

  7. Estimation of WECC System Inertia Using Observed Frequency Transients

    SciTech Connect (OSTI)

    Chassin, David P.; Huang, Zhenyu; Donnelly, Matt K.; Hassler, Candee A.; Ramirez, Enrique; Ray, Cody W.

    2005-04-19T23:59:59.000Z

    As demand for electricity in the western United States increases, stresses upon the aging power grid are intensifying. Computer models based on complex mathematical relationships are being developed to assist in understanding the impact of deregulation and market transformation. Frequency, load, and plant outage events data collected over the last several years. Analysis of these events was performed to determine frequency deviation and the systems inertial constant (M) during each event. Utilizing a theoretical relationship that relates system inertia to power loss, M was calculated for 157 events. The relationship of M to system wide load was then examined.

  8. System architecting of a campaign of earth observing satellites

    E-Print Network [OSTI]

    Colson, Justin M

    2008-01-01T23:59:59.000Z

    Given the current level of concern over anthropogenic climate change, and the ongoing debate worldwide regarding what action should be taken to reduce and reverse future warming, the ability to collect data on Earth system ...

  9. H observer for time-delay systems Application to FDI for irrigation canals

    E-Print Network [OSTI]

    Paris-Sud XI, Université de

    H observer for time-delay systems Application to FDI for irrigation canals N. Bedjaoui, X. Litrico and isolation for time-varying delayed systems. It consists to develop a H observer that generates residuals occur on the regulation gates of an irrigation canal. The observer design uses a simplified approximate

  10. Recycling of quantum information: Multiple observations of quantum systems

    E-Print Network [OSTI]

    Peter Rapcan; John Calsamiglia; Ramon Munoz-Tapia; Emilio Bagan; Vladimir Buzek

    2007-08-08T23:59:59.000Z

    Given a finite number of copies of an unknown qubit state that have already been measured optimally, can one still extract any information about the original unknown state? We give a positive answer to this question and quantify the information obtainable by a given observer as a function of the number of copies in the ensemble, and of the number of independent observers that, one after the other, have independently measured the same ensemble of qubits before him. The optimality of the protocol is proven and extensions to other states and encodings are also studied. According to the general lore, the state after a measurement has no information about the state before the measurement. Our results manifestly show that this statement has to be taken with a grain of salt, specially in situations where the quantum states encode confidential information.

  11. Stochastic Modeling and Optimization for Robust Power Management in a Partially Observable System

    E-Print Network [OSTI]

    Qiu, Qinru

    Stochastic Modeling and Optimization for Robust Power Management in a Partially Observable System and issues control commands periodically. Reference [3] models the similar system using the continuous a full observation of the entire system status. In this paper, we propose a new modeling and optimization

  12. An Augmented Reality System for Astronomical Observations Andrei Lintu

    E-Print Network [OSTI]

    Magnor, Marcus

    , but also depends on the visibility, sky brightness and telescope aper- ture. We propose a system which. For projection, a custom-built video projection mod- ule with high contrast and low maximum luminance value fascinated by the starry sky. It is one of the first natural phenomena that was investi- gated by humans

  13. Simulations of Solar System observations in alternative theories of gravity

    E-Print Network [OSTI]

    A. Hees; B. Lamine; S. Reynaud; M. -T. Jaekel; C. Le Poncin-Lafitte; V. Lainey; A. Füzfa; J. -M. Courty; V. Dehant; P. Wolf

    2013-02-27T23:59:59.000Z

    In this communication, we focus on the possibility to test General Relativity (GR) with radioscience experiments. We present simulations of observables performed in alternative theories of gravity using a software that simulates Range/Doppler signals directly from the space time metric. This software allows one to get the order of magnitude and the signature of the modifications induced by an alternative theory of gravity on radioscience signals. As examples, we present some simulations for the Cassini mission in Post-Einsteinian gravity (PEG) and with Standard Model Extension (SME).

  14. Designing a Stochastic Adaptive Impulsive Observer for Stochastic Linear and Nonlinear Impulsive Systems

    SciTech Connect (OSTI)

    Ayati, Moosa [Department of Applied Mathematics, University of Waterloo, Waterloo, Ontario (Canada); Faculty of Electrical and Computer Engineering, K. N. Toosi University of Technology, Tehran (Iran, Islamic Republic of); Alwan, Mohamad; Liu Xinzhi [Department of Applied Mathematics, University of Waterloo, Waterloo, Ontario (Canada); Khaloozadeh, Hamid [Faculty of Electrical and Computer Engineering, K. N. Toosi University of Technology, Tehran (Iran, Islamic Republic of)

    2011-11-30T23:59:59.000Z

    State observation (estimation) is a very important issue in system analysis and control. This paper develops a new observer called Stochastic Adaptive Impulsive Observer (SAIO) for the state estimation of impulsive systems. The proposed observer is applicable to linear and nonlinear stochastic impulsive systems. In addition, the effect of parametric uncertainty is considered and unknown parameters of the system are estimated by suitable adaptation laws. Impulsive system theory, particularly stochastic Lyapunov-like function, is used to analyze the stability and convergence of the state estimations. The main advantages of the proposed observer are: 1) it gives continuous estimation from discrete time measurements of the system output, and 2) it is useful for state estimation when continuous measurements are impossible or expensive. Simulation results show the effectiveness of the proposed observer and we believe that it has many applications in control and estimation theories.

  15. OBSERVER DESIGN FOR NONLINEAR SYSTEMS BY USING INPUT-TO-STATE STABILITY

    E-Print Network [OSTI]

    Sontag, Eduardo

    OBSERVER DESIGN FOR NONLINEAR SYSTEMS BY USING INPUT-TO-STATE STABILITY A. Alessandri Abstract by solving LMI problems [18]. A. Alessandri is with the Institute of Intelligent Systems for Automation

  16. Integrac ao de Crescimento de Regi ao e Detecc

    E-Print Network [OSTI]

    segmentation, combining region growing and edge detection segmentations. 1 Introducâ?º â? ao A segmentacâ?ºâ?ao deâ??�sticas de similari­ dade dividem a imagem em â?? areas que compartilham pro­ priedades comuns. O resultado da

  17. Impulsive observer-based control for linear systems using irregularly sampled measurements

    E-Print Network [OSTI]

    Paris-Sud XI, Université de

    Impulsive observer-based control for linear systems using irregularly sampled measurements Y linear state feedback controller and an impulsive observer to provide an estimate the non-measured states, which are subsequently fed back in the control algorithm. We consider linear systems that can

  18. A climate sensitivity estimate using Bayesian fusion of instrumental observations and an Earth System model

    E-Print Network [OSTI]

    sensitivity estimate using Bayesian fusion of instrumental observations and an Earth System model, J. Geophys System model Roman Olson,1 Ryan Sriver,1 Marlos Goes,2,3 Nathan M. Urban,4,5 H. Damon Matthews,6 MuraliA climate sensitivity estimate using Bayesian fusion of instrumental observations and an Earth

  19. A nonlinear observer to estimate unknown parameters during the synchronization of chaotic systems

    E-Print Network [OSTI]

    L. Torres

    2014-06-20T23:59:59.000Z

    This paper proposes an Extended-Kalman-Filter-like observer for parameter estimation during synchronization of chaotic systems. The exponential stability of the observer is guaranteed by a persistent excitation condition. This approach is shown to be suitable for various classical chaotic systems and several simulations are presented accordingly.

  20. Development and Demonstration of a Relocatable Ocean OSSE System: Optimizing Ocean Observations for Hurricane Forecast

    E-Print Network [OSTI]

    forecasts for individual storms and improved seasonal forecast of the ocean thermal energy availableDevelopment and Demonstration of a Relocatable Ocean OSSE System: Optimizing Ocean Observations in the Gulf of Mexico is being extended to provide NOAA the ability to evaluate new ocean observing systems

  1. Emissions of crustal material in air quality forecast systems: Use of satellite observations

    E-Print Network [OSTI]

    Menut, Laurent

    Emissions of crustal material in air quality forecast systems: Use of satellite observations) Natural (dust, fires, volcanos) Meteorology: Transport, turbulence Clouds and radiation, precipitations Chemistry-transport model Gas and particles concentrations Use of model outputs: Analysis Direct: model vs

  2. A Search for Additional Planets in the Nasa Epoxi Observations of the Exoplanet System Gj 436

    E-Print Network [OSTI]

    Seager, Sara

    We present time series photometry of the M dwarf transiting exoplanet system GJ 436 obtained with the Extrasolar Planet Observation and Characterization (EPOCh) component of the NASA EPOXI mission. We conduct a search of ...

  3. EMPLOYMENT OPPORTUNITIES Hawaii Ocean Observing System (HiOOS) Employment Opportunities

    E-Print Network [OSTI]

    UHM EMPLOYMENT OPPORTUNITIES Hawaii Ocean Observing System (HiOOS) Employment Opportunities FIELD TECHNICIAN OPPORTUNITY: employment with possible development of a senior thesis project in GESCarlo, edecarlo@soest.hawaii.edu JOB REFERENCE NUMBER ON STUDENT EMPLOYMENT WEBSITE: none Student

  4. OBSERVING SYSTEM SIMULATION EXPERIMENTS ON THE OAH'U REGIONAL OCEAN MODEL

    E-Print Network [OSTI]

    Luther, Douglas S.

    Thermal Energy Conversion (OTEC) site off the south coast of Oah'u as well as the circulation of Mamala analyses of the observing systems were conducted at the outflow plume depth of a potential pilot Ocean

  5. EVALUATION OF ULTRASONIC SNOW DEPTH SENSORS FOR AUTOMATED SURFACE OBSERVING SYSTEMS (ASOS)

    E-Print Network [OSTI]

    i THESIS EVALUATION OF ULTRASONIC SNOW DEPTH SENSORS FOR AUTOMATED SURFACE OBSERVING SYSTEMS (ASOS PREPARED UNDER OUR SUPERVISION BY WENDY ANN BRAZENEC ENTITLED EVALUATION OF ULTRASONIC SNOW DEPTH SENSORS;iii ABSTRACT OF THESIS EVALUATION OF ULTRASONIC SNOW DEPTH SENSORS FOR AUTOMATED SURFACE OBSERVING

  6. Observing System Simulation Experiments (OSSEs) for the Mid-Columbia Basin

    SciTech Connect (OSTI)

    Zack, J; Natenberg, E J; Knowe, G V; Waight, K; Manobianco, J; Hanley, D; Kamath, C

    2011-09-13T23:59:59.000Z

    The overall goal of this multi-phased research project known as WindSENSE is to develop an observation system deployment strategy that would improve wind power generation forecasts. The objective of the deployment strategy is to produce the maximum benefit for 1- to 6-hour ahead forecasts of wind speed at hub-height ({approx}80 m). In this phase of the project the focus is on the Mid-Columbia Basin region, which encompasses the Bonneville Power Administration (BPA) wind generation area (Figure 1) that includes the Klondike, Stateline, and Hopkins Ridge wind plants. There are two tasks in the current project effort designed to validate the Ensemble Sensitivity Analysis (ESA) observational system deployment approach in order to move closer to the overall goal: (1) Perform an Observing System Experiment (OSE) using a data denial approach. The results of this task are presented in a separate report. (2) Conduct a set of Observing System Simulation Experiments (OSSE) for the Mid-Colombia basin region. This report presents the results of the OSSE task. The specific objective is to test strategies for future deployment of observing systems in order to suggest the best and most efficient ways to improve wind forecasting at BPA wind farm locations. OSSEs have been used for many years in meteorology to evaluate the potential impact of proposed observing systems, determine tradeoffs in instrument design, and study the most effective data assimilation methodologies to incorporate the new observations into numerical weather prediction (NWP) models (Atlas 1997; Lord 1997). For this project, a series of OSSEs will allow consideration of the impact of new observing systems of various types and in various locations.

  7. Clementine Observations of the Zodiacal Light and the Dust Content of the Inner Solar System

    E-Print Network [OSTI]

    Hahn, Joseph M.

    Clementine Observations of the Zodiacal Light and the Dust Content of the Inner Solar System Joseph Road 1, Houston, TX 77058 Bonnie Cooper Oceaneering Space Systems, 16665 Space Center Boulevard solar radii to the orbit of Venus. The averaged ecliptic surface brightness of the zodiacal light falls

  8. OBSERVE: Occupancy-Based System for Efficient Reduction of HVAC Energy

    E-Print Network [OSTI]

    Carreira-Perpiñán, Miguel Á.

    OBSERVE: Occupancy-Based System for Efficient Reduction of HVAC Energy Varick L. Erickson, Miguel Á & control General Terms Algorithms, Machine Learning, Measurement Keywords Occupancy, HVAC, Ventilation for heating, ventilation, and air-conditioning (HVAC) systems[2]. Studies suggest that 15% to 25% of HVAC

  9. Progress Toward Observing Quantum Effects in an Optomechanical System in Cryogenics

    E-Print Network [OSTI]

    Harris, Jack

    , placed at 400 mK inside a 3 He fridge. The major goals of this research are: laser cooling the 261 kAbstract Progress Toward Observing Quantum Effects in an Optomechanical System in Cryogenics Cheng Yang 2011 Quantum optomechanical systems use radiation pressure of light to couple the optical field

  10. Dynamical and Observational Constraints on Additional Planets in Highly Eccentric Planetary Systems

    E-Print Network [OSTI]

    Robert A. Wittenmyer; Michael Endl; William D. Cochran; Harold F. Levison

    2007-06-13T23:59:59.000Z

    Long time coverage and high radial velocity precision have allowed for the discovery of additional objects in known planetary systems. Many of the extrasolar planets detected have highly eccentric orbits, which raises the question of how likely those systems are to host additional planets. We investigate six systems which contain a very eccentric (e>0.6) planet: HD 3651, HD 37605, HD 45350, HD 80606, HD 89744, and 16 Cyg B. We present updated radial-velocity observations and orbital solutions, search for additional planets, and perform test particle simulations to find regions of dynamical stability. The dynamical simulations show that short-period planets could exist in the HD 45350 and 16 Cyg B systems, and we use the observational data to set tight detection limits, which rule out additional planets down to a few Neptune masses in the HD 3651, HD 45350, and 16 Cyg B systems.

  11. Testing a Coupled Global-limited-area Data Assimilation System Using Observations from the 2004 Pacific Typhoon Season

    E-Print Network [OSTI]

    Holt, Christina

    2012-10-19T23:59:59.000Z

    by the Statistical Spectral Interpolation, which was the operational data assimilation system of NCEP in 2004. The GFS Operational analysis assimilated a large number of satellite radiance observations in addition to the observations assimilated in our system. All...

  12. High latitude geomagnetically induced current events observed on very low frequency radio wave receiver systems

    E-Print Network [OSTI]

    Otago, University of

    High latitude geomagnetically induced current events observed on very low frequency radio wave induced current (GIC) in the Scottish power system in southern Scotland, during a storm event, and exhibit significantly different amplitude characteristics. Finally, we compared in detail the geomagnetic

  13. Faculty Observations: John Scofield An Energy-Monitoring System for Stanford

    E-Print Network [OSTI]

    Scofield, John H.

    Faculty Observations: John Scofield An Energy-Monitoring System for Stanford University's Leslie buildings use energy, and each year we conducted an energy audit of a local building, most often a house in town. We conducted energy audits of two Oberlin College buildings, the Wright Laboratory of Physics

  14. Observers for Nonlinear-Linear Cascade Systems Hvard Fjr Grip, Ali Saberi, and Tor A. Johansen

    E-Print Network [OSTI]

    Johansen, Tor Arne

    Observers for Nonlinear-Linear Cascade Systems Håvard Fjær Grip, Ali Saberi, and Tor A. Johansen been Håvard Fjær Grip and Ali Saberi are with the School of Electrical Engineering and Computer Science of Håvard Fjær Grip is supported by the Research Council of Norway. The work of Ali Saberi is partially

  15. HF radar in French Mediterranean Sea: an element of MOOSE Mediterranean Ocean Observing System on Environment

    E-Print Network [OSTI]

    Boyer, Edmond

    Sea in the context of climate change and anthropogenic pressure and to supply and maintain longHF radar in French Mediterranean Sea: an element of MOOSE Mediterranean Ocean Observing System , Pascal Guterman2 , Karim Bernardet2 1 Mediterranean Institute of Oceanography (MIO, UM 110, USTV

  16. CONSTRAINING THE PLANETARY SYSTEM OF FOMALHAUT USING HIGH-RESOLUTION ALMA OBSERVATIONS

    SciTech Connect (OSTI)

    Boley, A. C.; Payne, M. J.; Ford, E. B.; Shabram, M. [Department of Astronomy, University of Florida, 211 Bryant Space Science Center, Gainesville, FL 32611 (United States); Corder, S. [North American ALMA Science Center, National Radio Astronomy Observatory, 520 Edgemont Road, Charlottesville, VA 22903 (United States); Dent, W. R. F. [ALMA, Alonso de Cordova 3107, Vitacura, Santiago (Chile)

    2012-05-01T23:59:59.000Z

    The dynamical evolution of planetary systems leaves observable signatures in debris disks. Optical images trace micron-sized grains, which are strongly affected by stellar radiation and need not coincide with their parent body population. Observations of millimeter-sized grains accurately trace parent bodies, but previous images lack the resolution and sensitivity needed to characterize the ring's morphology. Here we present ALMA 350 GHz observations of the Fomalhaut debris ring. These observations demonstrate that the parent body population is 13-19 AU wide with a sharp inner and outer boundary. We discuss three possible origins for the ring and suggest that debris confined by shepherd planets is the most consistent with the ring's morphology.

  17. State observers and Kalman filtering for high performance vibration isolation systems

    SciTech Connect (OSTI)

    Beker, M. G., E-mail: M.Beker@Nikhef.nl; Bertolini, A.; Hennes, E.; Rabeling, D. S. [National Institute for Subatomic Physics Nikhef, Science Park 105, 1098 XG Amsterdam (Netherlands)] [National Institute for Subatomic Physics Nikhef, Science Park 105, 1098 XG Amsterdam (Netherlands); Brand, J. F. J. van den; Bulten, H. J. [National Institute for Subatomic Physics Nikhef, Science Park 105, 1098 XG Amsterdam (Netherlands) [National Institute for Subatomic Physics Nikhef, Science Park 105, 1098 XG Amsterdam (Netherlands); VU University Amsterdam, de Boelelaan 1081, 1081 HV Amsterdam (Netherlands)

    2014-03-15T23:59:59.000Z

    There is a strong scientific case for the study of gravitational waves at or below the lower end of current detection bands. To take advantage of this scientific benefit, future generations of ground based gravitational wave detectors will need to expand the limit of their detection bands towards lower frequencies. Seismic motion presents a major challenge at these frequencies and vibration isolation systems will play a crucial role in achieving the desired low-frequency sensitivity. A compact vibration isolation system designed to isolate in-vacuum optical benches for Advanced Virgo will be introduced and measurements on this system are used to present its performance. All high performance isolation systems employ an active feedback control system to reduce the residual motion of their suspended payloads. The development of novel control schemes is needed to improve the performance beyond what is currently feasible. Here, we present a multi-channel feedback approach that is novel to the field. It utilizes a linear quadratic regulator in combination with a Kalman state observer and is shown to provide effective suppression of residual motion of the suspended payload. The application of state observer based feedback control for vibration isolation will be demonstrated with measurement results from the Advanced Virgo optical bench suspension system.

  18. Optical observations of Be/X-ray transient system KS 1947+300

    E-Print Network [OSTI]

    U. Kiziloglu; A. Baykal; N. Kiziloglu

    2006-08-05T23:59:59.000Z

    ROTSE-IIId observations of the Be/X-ray transient system KS 1947+300 obtained between September 2004 and December 2005 make it possible to study the correlation between optical and X-ray activity. The optical outburst of 0.1 mag was accompanied by an increase in X-ray flux in 2004 observations. Strong correlation between the optical and X-ray light curves suggests that neutron star directly accretes from the outflowing material of Be star. The nearly zero time lag between X-ray and optical light curves suggests a heating of the disk of Be star by X-rays. No optical brightening and X-ray enhancement was seen in 2005 observations. There is no indication of the orbital modulation in the optical light curve.

  19. Urban and land surface effects on the 30 July 2003 mesoscale convective system event observed in the southern Great Plains

    E-Print Network [OSTI]

    Niyogi, Dev

    Urban and land surface effects on the 30 July 2003 mesoscale convective system event observed/Atmosphere Mesoscale Prediction System (COAMPS 1 ) to investigate the impact of urban and land vegetation processes on the prediction of the mesoscale convective system (MCS) observed on 30 July 2003 in the vicinity of Oklahoma City

  20. Transit Timing Observations from Kepler: IV. Confirmation of 4 Multiple Planet Systems by Simple Physical Models

    SciTech Connect (OSTI)

    Fabrycky, Daniel C.; /UC, Santa Cruz; Ford, Eric B.; /Florida U.; Steffen, Jason H.; /Fermilab; Rowe, Jason F.; /SETI Inst., Mtn. View /NASA, Ames; Carter, Joshua A.; /Harvard-Smithsonian Ctr. Astrophys.; Moorhead, Althea V.; /Florida U.; Batalha, Natalie M.; /San Jose State U.; Borucki, William J.; /NASA, Ames; Bryson, Steve; /NASA, Ames; Buchhave, Lars A.; /Bohr Inst. /Copenhagen U.; Christiansen, Jessie L.; /SETI Inst., Mtn. View /NASA, Ames /Caltech

    2012-01-01T23:59:59.000Z

    Eighty planetary systems of two or more planets are known to orbit stars other than the Sun. For most, the data can be sufficiently explained by non-interacting Keplerian orbits, so the dynamical interactions of these systems have not been observed. Here we present 4 sets of lightcurves from the Kepler spacecraft, which each show multiple planets transiting the same star. Departure of the timing of these transits from strict periodicity indicates the planets are perturbing each other: the observed timing variations match the forcing frequency of the other planet. This confirms that these objects are in the same system. Next we limit their masses to the planetary regime by requiring the system remain stable for astronomical timescales. Finally, we report dynamical fits to the transit times, yielding possible values for the planets masses and eccentricities. As the timespan of timing data increases, dynamical fits may allow detailed constraints on the systems architectures, even in cases for which high-precision Doppler follow-up is impractical.

  1. Observation of transient gain without population inversion in a laser-cooled rubidium lambda system

    E-Print Network [OSTI]

    S. R. de Echaniz; Andrew D. Greentree; A. V. Durrant; D. M. Segal; J. P. Marangos; J. A. Vaccaro

    2001-05-17T23:59:59.000Z

    We have observed clear Rabi oscillations of a weak probe in a strongly driven three-level lambda system in laser-cooled rubidium for the first time. When the coupling field is non-adiabatically switched on using a Pockels cell, transient probe gain without population inversion is obtained in the presence of uncoupled absorptions. Our results are supported by three-state computations.

  2. Observational determination of the time delays in gravitational lens system Q2237+030

    E-Print Network [OSTI]

    V. Vakulik; R. Schild; V. Dudinov; S. Nuritdinov; V. Tsvetkova; O. Burkhonov; T. Akhunov

    2005-09-19T23:59:59.000Z

    We present new brightness monitoring observations of the 4 components of gravitationally lensed system Q2237+0305, which show detection of an intrinsic quasar brightness fluctuation at a time of subdued microlensing activity, between June 27 and October 12, 2003. These data were used to determine the time delays between the arrivals of the four images. The measured delays are -6, 35, and 2 hours for images B, C and D relative to A, respectively, so they confirm that the long history of brightness monitoring has produced significant detection of microlensing. However the error bars associated with the delays, of order 2 days, are too large to discriminate between competing macro-imaging models. Moreover, our simulations show that for the amplitude of this intrinsic fluctuation and for photometric errors intrinsic to optical monitoring from our 1.5-m telescope or from the OGLE monitoring, a daily sampled brightness record cannot produce reliable lags for model discrimination. We use our simulations to devise a strategy for future delay determination with optical data. Nevertheless, we regard these first estimates to be significant, since they are the first direct measurements of time delays made for this system from ground-based observations in the visual wavelengths. Our results provide the most convincing confirmation of the gravitational-lens nature of Q2237+0305, and give observational justification to the extensive literature which attributes the quasar's previously observed brightness fluctuations to microlensing.

  3. ARM - AOS Aerosol Properties Plots

    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 3,625 1,006 492 742EnergyOnItemResearchSOLICITATIONIMODI FICATION OF CONTRACTOperations AMF2ViewersAOS Aerosol

  4. Integrac~ao de Crescimento de Regi~ao e Detecc~ao de Arestas atraves de Operadores de Agregac~ao

    E-Print Network [OSTI]

    growing and edge detection segmentations. 1 Introduc¸~ao A segmentac¸~ao de imagens pode ser definida como a imagem em ´areas que compartilham pro- priedades comuns. O resultado da segmentac¸~ao orientada `a regi

  5. Observable Consequences of Planet Formation Models in Systems with Close-in Terrestrial Planets

    E-Print Network [OSTI]

    Sean N. Raymond; Rory Barnes; Avi M. Mandell

    2007-11-13T23:59:59.000Z

    To date, two planetary systems have been discovered with close-in, terrestrial-mass planets (planet; 4) formation from material being shepherded by moving secular resonances during dispersal of the protoplanetary disk; 5) tidal circularization of eccentric terrestrial planets with close-in perihelion distances; and 6) photo-evaporative mass loss of a close-in giant planet. Models 1-4 have been validated in previous work. We show that tidal circularization can form hot Earths, but only for relatively massive planets (> 5 Earth masses) with very close-in perihelion distances (planets of less than about 70 Earth masses, photo-evaporation can remove the planet's envelope and leave behind the solid core on a Gyr timescale, but only for planets inside 0.025-0.05 AU. Using two quantities that are observable by current and upcoming missions, we show that these models each produce unique signatures, and can be observationally distinguished. These observables are the planetary system architecture (detectable with radial velocities, transits and transit-timing) and the bulk composition of transiting close-in terrestrial planets (measured by transits via the planet's radius).

  6. Daily Processing of Solar System Object Observations by Gaia UMR 6202 Cassiope, University of Nice-Sophia Antipolis, CNRS,

    E-Print Network [OSTI]

    Paris-Sud XI, Université de

    complex operations, devoted to obtain the best accuracies in the output. It will operate on data obtainedDaily Processing of Solar System Object Observations by Gaia Tanga, P. UMR 6202 Cassiopée to a selected event. For this reason, a pipeline performing fast processing of Gaia observations of Solar System

  7. Understanding and Improving CRM and GCM Simulations of Cloud Systems with ARM Observations

    SciTech Connect (OSTI)

    Wu, Xiaoqing

    2014-02-25T23:59:59.000Z

    The works supported by this ASR project lay the solid foundation for improving the parameterization of convection and clouds in the NCAR CCSM and the climate simulations. We have made a significant use of CRM simulations and ARM observations to produce thermodynamically and dynamically consistent multi-year cloud and radiative properties; improve the GCM simulations of convection, clouds and radiative heating rate and fluxes using the ARM observations and CRM simulations; and understand the seasonal and annual variation of cloud systems and their impacts on climate mean state and variability. We conducted multi-year simulations over the ARM SGP site using the CRM with multi-year ARM forcing data. The statistics of cloud and radiative properties from the long-term CRM simulations were compared and validated with the ARM measurements and value added products (VAP). We evaluated the multi-year climate simulations produced by the GCM with the modified convection scheme. We used multi-year ARM observations and CRM simulations to validate and further improve the trigger condition and revised closure assumption in NCAR GCM simulations that demonstrate the improvement of climate mean state and variability. We combined the improved convection scheme with the mosaic treatment of subgrid cloud distributions in the radiation scheme of the GCM. The mosaic treatment of cloud distributions has been implemented in the GCM with the original convection scheme and enables the use of more realistic cloud amounts as well as cloud water contents in producing net radiative fluxes closer to observations. A physics-based latent heat (LH) retrieval algorithm was developed by parameterizing the physical linkages of observed hydrometeor profiles of cloud and precipitation to the major processes related to the phase change of atmospheric water.

  8. Observational Properties of Type Ib/c Supernova Progenitors in Binary Systems

    E-Print Network [OSTI]

    Kim, Hyun-Jeong; Koo, Bon-Chul

    2015-01-01T23:59:59.000Z

    In several recent observational studies on Type Ib/c supernovae (SNe Ib/c), the inferred ejecta masses have a peak value of 2.0 -- 4.0 $M_\\odot$, in favor of the binary scenario for their progenitors rather than the Wolf-Rayet star scenario. To investigate the observational properties of relatively low-mass helium stars in binary systems as SN Ib/c progenitors, we constructed atmospheric models with the non-LTE radiative transfer code CMFGEN, using binary star evolution models. We find that these helium stars can be characterized by relatively narrow helium emission lines if the mass-loss rate during the final evolutionary phase is significantly enhanced as implied by many SN Ib/c observations. The optical brightness of helium star progenitors can be meaningfully enhanced with a strong wind for $M \\gtrsim 4.4 M_\\odot$, but hardly affected or slightly weakened for relatively low-mass of $\\sim 3.0 M_\\odot$, compared to the simple estimate using blackbody approximation. We further confirm the previous suggestion...

  9. Heating and Dynamics of Two Flare Loop Systems Observed by AIA and EIS

    E-Print Network [OSTI]

    Li, Y; Ding, M D

    2013-01-01T23:59:59.000Z

    We investigate heating and evolution of flare loops in a C4.7 two-ribbon flare on 2011 February 13. From SDO/AIA imaging observations, we can identify two sets of loops. Hinode/EIS spectroscopic observations reveal blueshifts at the feet of both sets of loops. The evolution and dynamics of the two sets are quite different. The first set of loops exhibits blueshifts for about 25 minutes followed by redshifts, while the second set shows stronger blueshifts, which are maintained for about one hour. The UV 1600 observation by AIA also shows that the feet of the second set of loops brighten twice. These suggest that continuous heating may be present in the second set of loops. We use spatially resolved UV light curves to infer heating rates in the few tens of individual loops comprising the two loop systems. With these heating rates, we then compute plasma evolution in these loops with the "enthalpy-based thermal evolution of loops" (EBTEL) model. The results show that, for the first set of loops, the synthetic EU...

  10. EXERCICIOS INTRODUC ~AO `A TEORIA DOS GRAFOS

    E-Print Network [OSTI]

    Kohayakawa, Yoshiharu

    exerc´icios com data de entrega devem ser resolvidos e entregues. Estes exerc´icios far~ao parte de suaEXERC´ICIOS INTRODUC¸ ~AO `A TEORIA DOS GRAFOS 2O. SEMESTRE DE 2010 Instru¸c~oes: 1. Os problemas e avalia¸c~ao. 2. A entrega dos exerc´icios deve ser feita no come¸co da aula (as datas de entrega ser

  11. A Saturn Ring Observer Mission Using Multi-Mission Radioisotope Power Systems

    SciTech Connect (OSTI)

    Abelson, Robert D.; Spilker, Thomas R.; Shirley, James H. [Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Mail Stop 301-445W, Pasadena, CA 91109-8099 (United States)

    2006-01-20T23:59:59.000Z

    Saturn remains one of the most fascinating planets within the solar system. To better understand the complex ring structure of this planet, a conceptual Saturn Ring Observer (SRO) mission is presented that would spend one year in close proximity to Saturn's A and B rings, and perform detailed observations and measurements of the ring particles and electric and magnetic fields. The primary objective of the mission would be to understand ring dynamics, including the microphysics of individual particles and small scale (meters to a few kilometers) phenomena such as particle agglomeration behavior. This would be accomplished by multispectral imaging of the rings at multiple key locations within the A and B rings, and by ring-particle imaging at an unprecedented resolution of 0.5 cm/pixel. The SRO spacecraft would use a Venus-Earth-Earth-Jupiter Gravity Assist (VEEJGA) and be aerocaptured into Saturn orbit using an advanced aeroshell design to minimize propellant mass. Once in orbit, the SRO would stand off from the ring plane 1 to 1.4 km using chemical thrusters to provide short propulsive maneuvers four times per revolution, effectively causing the SRO vehicle to 'hop' above the ring plane. The conceptual SRO spacecraft would be enabled by the use of a new generation of multi-mission Radioisotope Power Systems (RPSs) currently being developed by NASA and DOE. These RPSs include the Multi-Mission Radioisotope Thermoelectric Generator (MMRTG) and Stirling Radioisotope Generator (SRG). The RPSs would generate all necessary electrical power ({>=}330 We at beginning of life) during the 10-year cruise and 1-year science mission ({approx}11 years total). The RPS heat would be used to maintain the vehicle's operating and survival temperatures, minimizing the need for electrical heaters. Such a mission could potentially launch in the 2015-2020 timeframe, with operations at Saturn commencing in approximately 2030.

  12. High-speed, energy-resolved, STJ observations of the AM Her system V2301 Oph

    E-Print Network [OSTI]

    A. P. Reynolds; G. Ramsay; J. H. J. de Bruijne; M. A. C. Perryman; M. Cropper; C. M. Bridge; A. Peacock

    2005-02-02T23:59:59.000Z

    We present high time-resolution optical energy-resolved photometry of the eclipsing cataclysmic variable V2301 Oph made using the ESA S-Cam detector, an array of photon counting super-conducting tunnel junction (STJ) devices with intrinsic energy resolution. Three eclipses were observed, revealing considerable variation in the eclipse shape, particularly during ingress. The eclipse shape is shown to be understood in terms of AM Her accretion via a bright stream, with very little contribution from the white dwarf photosphere and/or hotspot. About two thirds of the eclipsed light arises in the threading region. Variation in the extent of the threading region can account for most of the variations observed between cycles. Spectral fits to the data reveal a 10,000K blackbody continuum with strong, time-varying emission lines of hydrogen and helium. This is the first time that stellar emission lines have been detected in the optical band using a non-dispersive photon-counting system.

  13. SISTEMA NEURONAL RAPIDO DE DECIS~AO BASEADO EM CALORIMETRIA DE ALTAS ENERGIAS

    E-Print Network [OSTI]

    Anjos, André

    ¸c~ao da informa¸c~ao, obt´em-se, ainda assim, uma elevada efici^encia de discrimina¸c~ao (97% para el for the degree of Master of Science (M.Sc.) FAST NEURAL DECISION SYSTEM BASED ON HIGH ENERGY CALORIMETRY Andr develops a fast neural classifier for high energy particle discrimination (electron/jet) at the second

  14. DEVELOPMENT OF A COASTAL MARGIN OBSERVATION AND ASSESSMENT SYSTEM (CMOAS) TO CAPTURE THE EPISODIC EVENTS IN A SHALLOW BAY

    E-Print Network [OSTI]

    Islam, Mohammad S.

    2010-07-14T23:59:59.000Z

    for the implementation of observational systems in other dynamic ecosystems for characterizing and predicting other episodic events such as harmful algal blooms, accidental oil spills, sediment resuspension events, etc. State-of-the-art sensor technologies are involved...

  15. CLARREO shortwave observing system simulation experiments of the twenty-first century: Simulator design and implementation

    SciTech Connect (OSTI)

    Feldman, D.R.; Algieri, C.A.; Ong, J.R.; Collins, W.D.

    2011-04-01T23:59:59.000Z

    Projected changes in the Earth system will likely be manifested in changes in reflected solar radiation. This paper introduces an operational Observational System Simulation Experiment (OSSE) to calculate the signals of future climate forcings and feedbacks in top-of-atmosphere reflectance spectra. The OSSE combines simulations from the Intergovernmental Panel on Climate Change (IPCC) Fourth Assessment Report for the NCAR Community Climate System Model (CCSM) with the MODTRAN radiative transfer code to calculate reflectance spectra for simulations of current and future climatic conditions over the 21st century. The OSSE produces narrowband reflectances and broadband fluxes, the latter of which have been extensively validated against archived CCSM results. The shortwave reflectance spectra contain atmospheric features including signals from water vapor, liquid and ice clouds, and aerosols. The spectra are also strongly influenced by the surface bidirectional reflectance properties of predicted snow and sea ice and the climatological seasonal cycles of vegetation. By comparing and contrasting simulated reflectance spectra based on emissions scenarios with increasing projected and fixed present-day greenhouse gas and aerosol concentrations, we find that prescribed forcings from increases in anthropogenic sulfate and carbonaceous aerosols are detectable and are spatially confined to lower latitudes. Also, changes in the intertropical convergence zone and poleward shifts in the subsidence zones and the storm tracks are all detectable along with large changes in snow cover and sea ice fraction. These findings suggest that the proposed NASA Climate Absolute Radiance and Refractivity Observatory (CLARREO) mission to measure shortwave reflectance spectra may help elucidate climate forcings, responses, and feedbacks.

  16. Potential Soil Moisture Products from the Aquarius Radiometer and Scatterometer Using an Observing System Simulation Experiment

    SciTech Connect (OSTI)

    Luo, Yan [I.M. Systems Group at NOAA/NCEP/EMC; Feng, Xia [George Mason University; Houser, Paul [George Mason University; Anantharaj, Valentine G [ORNL; Fan, Xingang [Western Kentucky University, Bowling Green; De Lannoy, Gabrielle [Ghent University, Belgium; Zhan, Xiwu [NOAA/NESDIS Center for Satellite Applications and Research; Dabbiru, Lalitha [Mississippi State University (MSU)

    2013-01-01T23:59:59.000Z

    Using an observing system simulation experiment (OSSE), we investigate the potential soil moisture retrieval capability of the National Aeronautics and Space Administration (NASA) Aquarius radiometer (L-band 1.413 GHz) and scatterometer (L-band, 1.260 GHz). We estimate potential errors in soil moisture retrievals and identify the sources that could cause those errors. The OSSE system includes (i) a land surface model in the NASA Land Information System, (ii) a radiative transfer and backscatter model, (iii) a realistic orbital sampling model, and (iv) an inverse soil moisture retrieval model. We execute the OSSE over a 1000 2200 km2 region in the central United States, including the Red and Arkansas river basins. Spatial distributions of soil moisture retrieved from the radiometer and scatterometer are close to the synthetic truth. High root mean square errors (RMSEs) of radiometer retrievals are found over the heavily vegetated regions, while large RMSEs of scatterometer retrievals are scattered over the entire domain. The temporal variations of soil moisture are realistically captured over a sparely vegetated region with correlations 0.98 and 0.63, and RMSEs 1.28% and 8.23% vol/vol for radiometer and scatterometer, respectively. Over the densely vegetated region, soil moisture exhibits larger temporal variation than the truth, leading to correlation 0.70 and 0.67, respectively, and RMSEs 9.49% and 6.09% vol/vol respectively. The domain-averaged correlations and RMSEs suggest that radiometer is more accurate than scatterometer in retrieving soil moisture. The analysis also demonstrates that the accuracy of the retrieved soil moisture is affected by vegetation coverage and spatial aggregation.

  17. IEEE TRANSACTIONS ON POWER SYSTEMS, VOL. 22, NO. 4, NOVEMBER 2007 1881 Analysis of Tap-Induced Oscillations Observed

    E-Print Network [OSTI]

    Hiskens, Ian A.

    analysis, tap-changing transformers, voltage oscillations. I. INTRODUCTION ANUMBER of years ago, voltage-Induced Oscillations Observed in an Electrical Distribution System Vaibhav Donde, Member, IEEE, and Ian A. Hiskens, Fellow, IEEE Abstract--Slow oscillations, with a period of around 15 min, were observed in an 11-k

  18. Limits of control for quantum systems: kinematical bounds on the optimization of observables and the question of dynamical realizability

    E-Print Network [OSTI]

    S. G. Schirmer; J. V. Leahy

    2000-10-07T23:59:59.000Z

    In this paper we investigate the limits of control for mixed-state quantum systems. The constraint of unitary evolution for non-dissipative quantum systems imposes kinematical bounds on the optimization of arbitrary observables. We summarize our previous results on kinematical bounds and show that these bounds are dynamically realizable for completely controllable systems. Moreover, we establish improved bounds for certain partially controllable systems. Finally, the question of dynamical realizability of the bounds for arbitary partially controllable systems is shown to depend on the accessible sets of the associated control system on the unitary group U(N) and the results of a few control computations are discussed briefly.

  19. Visualizac~ao de Objetos Tridimensionais Baseada em Interpolac ~ao Projetiva

    E-Print Network [OSTI]

    ¸~ao Computac¸~ao Gr´afica ´e comumente reconhecidacomo o pro- cesso de gerac¸~ao de imagens atrav´es do a seguir. Para um entendimento melhor sobre o assunto, veja as refer^encias [2, 6]. Síntese de Imagens Análise de Imagens Modelagem Geométrica Processamento de Imagens Imagens Dados Figura 1: Computac¸~ao Gr

  20. Status Update and Closed-Loop Performance of the Magellan Adaptive Optics VisAO Camera

    E-Print Network [OSTI]

    Kopon, Derek; Males, Jared; Gasho, Victor; Morzinski, Katie; Follette, Katherine

    2014-01-01T23:59:59.000Z

    We present laboratory results of the closed-loop performance of the Magellan Adaptive Optics (AO) Adaptive Secondary Mirror (ASM), pyramid wavefront sensor (PWFS), and VisAO visible adaptive optics camera. The Magellan AO system is a 585-actuator low-emissivity high-throughput system scheduled for first light on the 6.5 meter Magellan Clay telescope in November 2012. Using a dichroic beamsplitter near the telescope focal plane, the AO system will be able to simultaneously perform visible (500-1000 nm) AO science with our VisAO camera and either 10 micron or 3-5 micron science using either the BLINC/MIRAC4 or CLIO cameras, respectively. The ASM, PWS, and VisAO camera have undergone final system tests in the solar test tower at the Arcetri Institute in Florence, Italy, reaching Strehls of 37% in i'-band with 400 modes and simulated turbulence of 14 cm ro at v-band. We present images and test results of the assembled VisAO system, which includes our prototype advanced Atmospheric Dispersion Corrector (ADC), prot...

  1. Uma Implementac~ao Concorrente de Redes Neurais PCA para Compress~ao de Imagens

    E-Print Network [OSTI]

    Pereira, Marcone Corrêa

    Uma Implementac¸~ao Concorrente de Redes Neurais PCA para Compress~ao de Imagens Willian Y. Honda1 comparativo mostra que a proposta, aplicada `a tarefa de compress~ao de imagens, apresenta resultados imagens digitais, j´a que permite reduzir a dimensionalidade de um conjunto de da- dos preservando suas

  2. 2372 IEEE TRANSACTIONS ON AUTOMATIC CONTROL, VOL. 58, NO. 9, SEPTEMBER 2013 Observability of a Linear System Under

    E-Print Network [OSTI]

    Yüksel, Serdar

    notion of controllability, these form the essence of modern linear control theory. In this technical note states intact. Furthermore, with the increasing emphasis on networked control systems, it has been realized that the controllability and observability concepts for linear systems with controllers having

  3. Observers for Interconnected Nonlinear and Linear Systems Havard Fjr Grip a, Ali Saberi a, and Tor A. Johansen b

    E-Print Network [OSTI]

    Johansen, Tor Arne

    Observers for Interconnected Nonlinear and Linear Systems H°avard Fjær Grip a, Ali Saberi a (Esfandiari and Khalil, 1987; Saberi and Sannuti, 1990), and non-left-invertible systems (e.g., Gauthier, Hammouri, and Othman, 1992; Bornard and Hammouri, 2002; Grip and Saberi, 2010); the exploitation

  4. SMA Observations of Class 0 Protostars: A High-Angular Resolution Survey of Protostellar Binary Systems

    E-Print Network [OSTI]

    Chen, Xuepeng; Zhang, Qizhou; Bourke, Tyler L; Launhardt, Ralf; Jorgensen, Jes K; Lee, Chin-Fee; Foster, Jonathan B; Dunham, Michael M; Pineda, Jaime E; Henning, Thomas

    2013-01-01T23:59:59.000Z

    We present high angular resolution 1.3 mm and 850 um dust continuum data obtained with the Submillimeter Array toward 33 Class 0 protostars in nearby clouds (distance < 500 pc), which represents so far the largest survey toward protostellar binary/multiple systems. The median angular resolution in the survey is 2.5 arcsec, while the median linear resolution is approximately 600 AU. Compact dust continuum emission is observed from all sources in the sample. Twenty-one sources in the sample show signatures of binarity/multiplicity, with separations ranging from 50 to 5000 AU. The numbers of singles, binaries, triples, and quadruples in the sample are 12, 14, 5, and 2, respectively. The derived multiplicity frequency (MF) and companion star fraction (CSF) for Class 0 protostars are 0.64+/-0.08 and 0.91+/-0.05, respectively, with no correction for completeness. The derived MF and CSF in this survey are approximately two times higher than the values found in the binary surveys toward Class I YSOs, and approxima...

  5. Effect of the N. Delta. interaction on observables of the. pi. NN and. gamma. NN systems

    SciTech Connect (OSTI)

    Pena, M.T. (Centro de Fisica Nuclear da Universidade de Lisboa (INIC), 1699 Lisboa Codex (Portugal)); Garcilazo, H. (Theoretical Physics, University of Hannover, D-3000 Hannover (Germany)); Oelfke, U. (TRIUMF, 4004 Wesbrook Mall, Vancouver, British Columbia (Canada)); Sauer, P.U. (Theoretical Physics, University of Hannover, D-3000 Hannover (Germany) Nuclear Theory Group, Department of Physics, FM-15, University of Washington , Seattle, Washington 98195 (United States))

    1992-04-01T23:59:59.000Z

    Effects on the hadronic and electromagnetic properties of the two-nucleon system above pion threshold, arising from the interaction of the {Delta} isobar with nucleons, are investigated. The instantaneous nucleon-{Delta} potential is based on the meson exchange. Two-body reactions connecting channels with at most one pion and one photon are studied. Processes leading to a three-body pion-two-nucleon final state are considered in the restricted kinematic domain in which the pion forms the {ital P}{sub 33} resonance with one of the nucleons. The nucleon-{Delta} potential is seen to increase the relative importance of the inelastic strength of two-nucleon spin-triplet states with respect to spin-singlet states, correcting a deficiency common in most existing models. Theoretical predictions are compared with recent experimental data for the various reactions. In particular, the differential cross section and the proton beam asymmetry for {ital pp}{r arrow}{ital n}{Delta}{sup ++} ({ital p}{pi}{sup +}) are calculated, the latter observable being especially sensitive to the nucleon-{Delta} interaction.

  6. Extrac~ao de Padr~oes e Construc~ao de Modelos Simbolicos para Previs~ao de Dados Temporais

    E-Print Network [OSTI]

    Batista, Gustavo

    ~ao-lineares. Os primeiros, assumem que os dados respeitam alguma distribuic¸~ao estat´istica e, com base nessaExtrac¸~ao de Padr~oes e Construc¸~ao de Modelos Simb´olicos para Previs~ao de Dados Temporais,hueidianalee,wufengchung}@gmail.com Resumo. A previs~ao de dados temporais ´e uma tarefa de crescente interesse em distintas ´areas. De modo

  7. Soluc~ao dos Exercicios Capitulo 9

    E-Print Network [OSTI]

    Cipolatti, Rolci

    ) = 0. e Exerc´icio 9.5: Mostre que o sistema abaixo pode ser resolvido com: 1) x, y, u em fun¸c~ao de zSolu¸c~ao dos Exerc´icios Cap´itulo 9 Exerc´icio 9.1: Considere a superf´icie xy-z log y+eyz -e = 0¸c~ao das vari´aveis x e y uma vizinhan¸ca do ponto (0, 1). Exerc´icio 9.2: O ponto P = (1, -1, 2) pertence

  8. Systems and Algorithms for Automated Collaborative Observation using Networked Robotic Cameras 

    E-Print Network [OSTI]

    Xu, Yiliang

    2011-10-21T23:59:59.000Z

    The development of telerobotic systems has evolved from Single Operator Single Robot (SOSR) systems to Multiple Operator Multiple Robot (MOMR) systems. The relationship between human operators and robots follows the ...

  9. Systems and Algorithms for Automated Collaborative Observation using Networked Robotic Cameras

    E-Print Network [OSTI]

    Xu, Yiliang

    2011-10-21T23:59:59.000Z

    The development of telerobotic systems has evolved from Single Operator Single Robot (SOSR) systems to Multiple Operator Multiple Robot (MOMR) systems. The relationship between human operators and robots follows the master-slave control architecture...

  10. Cap'itulo 1 Introduc~ao

    E-Print Network [OSTI]

    simples, como sendo a gera¸c~ao de uma seq¨uâ??encia de imagens que retrata o movimento relativo dos objetos, atrav'es das quais 'e poss'ivel observar um outro disco contendo uma seq¨uâ??encia de imagens. Rotacionando­se os discos na velocidade correta, a sincroniza¸c~ao das janelas com as imagens cria o efeito

  11. SOBRE A COMPLEXIDADE DE COLORAC ~AO MISTA

    E-Print Network [OSTI]

    Boyer, Edmond

    (v), se (u, v) A, e c(u) = c(v), se [u, v] E. O problema de Colorac¸~ao Mista consiste em determinar o n,version1-3Nov2010 Author manuscript, published in "III Encontro Regional de Pesquisa Operacional do-se determinar a menor quantidade de cores para a qual o grafo admite uma colorac¸~ao pr´opria. Essa quantidade

  12. Defeating Network Node Subversion on SCADA Systems Using Probabilistic Packet Observation

    E-Print Network [OSTI]

    Sheldon, Nathan D.

    on SCADA systems was first proposed in [2]. It is assumed an operator has a model of a control system are manipulated. If no such manipulation takes place and the control signal is still anomalous, we can assume Supervisory control and data acquisition (SCADA) systems form a vital part of the critical infrastructure

  13. Passive microwave observations of mesoscale convective systems over the tropical Pacific Ocean

    E-Print Network [OSTI]

    McGaughey, Gary Rae

    1994-01-01T23:59:59.000Z

    This paper presents high resolution passive microwave measurements obtained in the western Pacific warm pool region. These measurements represent the first comprehensive observations of convection over the tropical oceans, and were obtained from...

  14. TRANSIT TIMING OBSERVATIONS FROM KEPLER. VI. POTENTIALLY INTERESTING CANDIDATE SYSTEMS FROM FOURIER-BASED STATISTICAL TESTS

    SciTech Connect (OSTI)

    Steffen, Jason H. [Fermilab Center for Particle Astrophysics, P.O. Box 500, MS 127, Batavia, IL 60510 (United States); Ford, Eric B. [Astronomy Department, University of Florida, 211 Bryant Space Sciences Center, Gainesville, FL 32111 (United States); Rowe, Jason F.; Borucki, William J.; Bryson, Steve; Caldwell, Douglas A.; Jenkins, Jon M.; Koch, David G.; Sanderfer, Dwight T.; Seader, Shawn; Twicken, Joseph D. [NASA Ames Research Center, Moffett Field, CA 94035 (United States); Fabrycky, Daniel C. [UCO/Lick Observatory, University of California, Santa Cruz, CA 95064 (United States); Holman, Matthew J. [Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138 (United States); Welsh, William F. [Astronomy Department, San Diego State University, San Diego, CA 92182-1221 (United States); Batalha, Natalie M. [Department of Physics and Astronomy, San Jose State University, San Jose, CA 95192 (United States); Ciardi, David R. [NASA Exoplanet Science Institute/California Institute of Technology, Pasadena, CA 91125 (United States); Kjeldsen, Hans [Department of Physics and Astronomy, Aarhus University, DK-8000 Aarhus C (Denmark); Prsa, Andrej, E-mail: jsteffen@fnal.gov [Department of Astronomy and Astrophysics, Villanova University, 800 East Lancaster Avenue, Villanova, PA 19085 (United States)

    2012-09-10T23:59:59.000Z

    We analyze the deviations of transit times from a linear ephemeris for the Kepler Objects of Interest (KOI) through quarter six of science data. We conduct two statistical tests for all KOIs and a related statistical test for all pairs of KOIs in multi-transiting systems. These tests identify several systems which show potentially interesting transit timing variations (TTVs). Strong TTV systems have been valuable for the confirmation of planets and their mass measurements. Many of the systems identified in this study should prove fruitful for detailed TTV studies.

  15. LINEAR SYSTEMS WITH SIGN-OBSERVATIONS RENEE KOPLON AND EDUARDO D. SONTAG

    E-Print Network [OSTI]

    Sontag, Eduardo

    relatively simple systems. However, for large-scale problems, controllers resulting from the application, various types of switching controllers, and humans ­or, more re- cently, expert systems,­ in supervisory the interplay of modern control theory with automata theory and other techniques from computer science

  16. Observations of prolific transient luminous event production above a mesoscale convective system in Argentina during

    E-Print Network [OSTI]

    Thomas, Jeremy N.

    in Argentina during the Sprite2006 Campaign in Brazil F. T. São Sabbas,1 M. J. Taylor,2 P.D. Pautet,2 M. Bailey convective system (MCS) over Argentina, as part of the third sprite campaign in Brazil. GOES infrared (IR a mesoscale convective system in Argentina during the Sprite2006 Campaign in Brazil, J. Geophys. Res., 115, A

  17. UM ESTUDO SOBRE A OTIMIZAC ~AO DA OPERAC ~AO DE RESERVAT ORIOS DE USINAS HIDRELETRICAS

    E-Print Network [OSTI]

    Oliveira, Aurélio R. L.

    - SP - Brasil Resumo. No Brasil, a gerac¸~ao de energia el´etrica ´e predominantemente de origem hidra´ivel conceber a falta deste importante insumo em qualquer atividade. No Brasil, a gerac¸~ao de energia el, Av. Albert Einstein, 400, Cidade Universit´aria, 13083-970, Campinas - SP - Brasil¡ Departamento de

  18. Extrac~ao de Malhas Adaptativas com Operac~oes de Simplificac~ao e Refinamento

    E-Print Network [OSTI]

    resolution initial mesh and applies refinement to obtain a multiresolution representation from base mesh outras. Nestas ´areas os dados iniciais s~ao comumente representados como dados volum´etricos, os quais a triangulac¸~ao entre pares de fatias paralelas do dado volum´etrico [Barequet and Sharir, 1996], [Cong

  19. The Earth Observing System (EOS)Aura satellite mission is scheduled to launch in June 2004.

    E-Print Network [OSTI]

    ://cloudsat.atmos.colostate.edu/),which is to be launched in mid-2005 [Stephens et al.,2002]. This group of satellites,including the Centre National d? Total Ozone Mapping Spectrometer (TOMS) observations from 1978 show a strong secular decrease in column the TOMS/SBUV global column and profile ozone trend measurements. What are the sources and processes

  20. Uma Formulac~ao Complexa para o Algoritmo Hebbiano Generalizado Aplicada `a Compress~ao de Imagens \\Lambda

    E-Print Network [OSTI]

    Amaral, José Nelson

    ­ da¸c~ao Coordena¸c~ao de Aperfei¸coamento de Pessoal de N'ivel Superior (CAPES), pelo Conselho Nacio

  1. SST subseasonal variability in the central Benguela upwelling system as inferred from satellite observations (19992009)

    E-Print Network [OSTI]

    Boyer, Edmond

    associated with the eastern flank of the semipermanent South Atlantic Anti- cyclone (SAA). Through Ekman of distinct physical and biological features, the Benguela system can be separated into three zones charac

  2. Observations on A Technology Roadmap for Generation IV Nuclear Energy Systems: Technical Roadmap Report

    Broader source: Energy.gov [DOE]

    The development of advanced nuclear energy systems in the U.S. will depend greatly on the continued success of currently operating light water nuclear power plants and the ordering of new...

  3. Dual-Doppler observations of the formative stage of an asymmetric squall line system

    E-Print Network [OSTI]

    Jamieson, Daniel Richard

    2002-01-01T23:59:59.000Z

    The objective of this study is to document and explain the formation of a large asymmetric squall line system. Despite having a precipitation pattern similar to the conceptual model of an asymmetric squall line, the development and evolution...

  4. Experimental observation of a phase transition in the evolution of many-body systems with dipolar interactions

    E-Print Network [OSTI]

    Gonzalo A. Alvarez; Dieter Suter; Robin Kaiser

    2014-09-16T23:59:59.000Z

    Non-equilibrium dynamics of many-body systems is important in many branches of science, such as condensed matter, quantum chemistry, and ultracold atoms. Here we report the experimental observation of a phase transition of the quantum coherent dynamics of a 3D many-spin system with dipolar interactions, and determine its critical exponents. Using nuclear magnetic resonance (NMR) on a solid-state system of spins at room-temperature, we quench the interaction Hamiltonian to drive the evolution of the system. The resulting dynamics of the system coherence can be localized or extended, depending on the quench strength. Applying a finite-time scaling analysis to the observed time-evolution of the number of correlated spins, we extract the critical exponents v = s = 0.42 around the phase transition separating a localized from a delocalized dynamical regime. These results show clearly that such nuclear-spin based quantum simulations can effectively model the non-equilibrium dynamics of complex many-body systems, such as 3D spin-networks with dipolar interactions.

  5. Algebra of systems: A metalanguage for model synthesis and evaluation

    E-Print Network [OSTI]

    Koo, Benjamin H. Y.

    This paper represents system models as algebraic entities and formulates model transformation activities as algebraic operations. We call this modeling framework ldquoalgebra of systemsrdquo (AoS). To show that AoS can ...

  6. Nonlinear Observer Design for Interconnected Power Systems M. A. Mahmud, Student Member, IEEE, M. J. Hossain, Member, IEEE, and H. R. Pota

    E-Print Network [OSTI]

    Pota, Himanshu Roy

    Nonlinear Observer Design for Interconnected Power Systems M. A. Mahmud, Student Member, IEEE, M. J design method for interconnected power systems. The concepts of nonlinear coordinate transformation, Lie derivative, and relative degree are used to design the observer for power systems. In this proposed design

  7. TRANSIT TIMING OBSERVATIONS FROM KEPLER. IV. CONFIRMATION OF FOUR MULTIPLE-PLANET SYSTEMS BY SIMPLE PHYSICAL MODELS

    SciTech Connect (OSTI)

    Fabrycky, Daniel C. [Department of Astronomy and Astrophysics, University of California, Santa Cruz, Santa Cruz, CA 95064 (United States); Ford, Eric B.; Moorhead, Althea V. [Astronomy Department, University of Florida, 211 Bryant Space Sciences Center, Gainesville, FL 32111 (United States); Steffen, Jason H. [Fermilab Center for Particle Astrophysics, P.O. Box 500, MS 127, Batavia, IL 60510 (United States); Rowe, Jason F.; Christiansen, Jessie L. [SETI Institute, Mountain View, CA 94043 (United States); Carter, Joshua A.; Fressin, Francois; Geary, John [Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138 (United States); Batalha, Natalie M. [Department of Physics and Astronomy, San Jose State University, San Jose, CA 95192 (United States); Borucki, William J.; Bryson, Steve; Haas, Michael R. [NASA Ames Research Center, Moffett Field, CA, 94035 (United States); Buchhave, Lars A. [Department of Astrophysics and Planetary Science, Niels Bohr Institute, University of Copenhagen, DK-2100 Copenhagen (Denmark); Ciardi, David R. [NASA Exoplanet Science Institute/Caltech, Pasadena, CA 91126 (United States); Cochran, William D.; Endl, Michael [McDonald Observatory, The University of Texas, Austin TX 78730 (United States); Fanelli, Michael N. [Bay Area Environmental Research Institute/NASA Ames Research Center, Moffett Field, CA 94035 (United States); Fischer, Debra [Astronomy Department, Yale University, New Haven, CT (United States); Hall, Jennifer R., E-mail: daniel.fabrycky@gmail.com [Orbital Sciences Corporation/NASA Ames Research Center, Moffett Field, CA 94035 (United States); and others

    2012-05-10T23:59:59.000Z

    Eighty planetary systems of two or more planets are known to orbit stars other than the Sun. For most, the data can be sufficiently explained by non-interacting Keplerian orbits, so the dynamical interactions of these systems have not been observed. Here we present four sets of light curves from the Kepler spacecraft, each which of shows multiple planets transiting the same star. Departure of the timing of these transits from strict periodicity indicates that the planets are perturbing each other: the observed timing variations match the forcing frequency of the other planet. This confirms that these objects are in the same system. Next we limit their masses to the planetary regime by requiring the system remain stable for astronomical timescales. Finally, we report dynamical fits to the transit times, yielding possible values for the planets' masses and eccentricities. As the timespan of timing data increases, dynamical fits may allow detailed constraints on the systems' architectures, even in cases for which high-precision Doppler follow-up is impractical.

  8. Codi cac~ao de Imagens Marcelo Coelho Ferraz

    E-Print Network [OSTI]

    Codi cac~ao de Imagens Marcelo Coelho Ferraz TESE SUBMETIDA AO CORPO DOCENTE DO INSTITUTO DE MATEM Codi cac~ao de Imagens". Ao meu pai Inha uma, entre muitas outras raz~oes, por suas grandes contribuic Imagens Marcelo Coelho Ferraz Junho de 1998 Orientador: Jonas de Miranda Gomes Diversos m etodos de codi

  9. university-logo Programac~ao Concorrente e Paralela

    E-Print Network [OSTI]

    Rodriguez, Noemi

    university-logo Programa¸c~ao Concorrente e Paralela Noemi Rodriguez August 19, 2009 Noemi Rodriguez Programa¸c~ao Concorrente e Paralela #12;university-logo Objetivos princ´ipios e t´ecnicas de´iveis de abstra¸c~ao! Noemi Rodriguez Programa¸c~ao Concorrente e Paralela #12;university-logo que princ

  10. This chapter describes observations of continuing change in the Arctic environmental system. It is or-

    E-Print Network [OSTI]

    Bhatt, Uma

    for the longest period and largest area of ice sheet melt since at least 1978, and the highest melt rate since in the Canadian Arctic, where the rate of mass loss from small glaciers and ice caps continued to increase system. It is or- ganized into five broad sections: atmosphere, ocean, sea ice cover, land, and Greenland

  11. An adaptive observer for hyperbolic systems with application to UnderBalanced

    E-Print Network [OSTI]

    Boyer, Edmond

    an UnderBalanced well. While a well is being drilled, a fluid circulates through the drilling system. The drilling fluid cools down the drillbit, and evacuates rock cuttings. More importantly, it pressurizes fluid is controlled by a valve, which enables tighter control of the pressure. UnderBalanced Drilling

  12. Observation and characterization of chimera states in coupled dynamical systems with nonlocal coupling

    E-Print Network [OSTI]

    R. Gopal; V. K. Chandrasekar; A. Venkatesan; M. Lakshmanan

    2014-05-15T23:59:59.000Z

    By developing the concepts of strength of incoherence and discontinuity measure, we show that a distinct quantitative characterization of chimera and multichimera states which occur in networks of coupled nonlinear dynamical systems admitting nonlocal interactions of finite radius can be made. These measures also clearly distinguish between chimera or multichimera states (both stable and breathing types) and coherent and incoherent as well as cluster states....

  13. UV Habitability of Possible Exomoons in Observed F-star Planetary Systems

    E-Print Network [OSTI]

    Sato, Satoko

    2015-01-01T23:59:59.000Z

    In the present study we explore the astrobiological significance of F-type stars of spectral type between F5 V and F9.5 V, which possess Jupiter-type planets within or close to their climatological habitable zones. These planets, or at least a subset of them, may also possess rocky exomoons, which potentially offer habitable environments. Our work considers eight selected systems. The Jupiter-type planets in these systems are in notably different orbits with eccentricities ranging from 0.08 to 0.72. Particularly, we consider the stellar UV environments provided by the photospheric stellar radiation in regard to the circumstellar habitability of the system. According to previous studies, DNA is taken as a proxy for carbon-based macromolecules following the paradigm that extraterrestrial biology might be based on hydrocarbons. Thus, the DNA action spectrum is utilized to represent the impact of the stellar UV radiation. Atmospheric attenuation is taken into account based on parameterized attenuation functions. ...

  14. TRANSIT TIMING OBSERVATIONS FROM KEPLER. II. CONFIRMATION OF TWO MULTIPLANET SYSTEMS VIA A NON-PARAMETRIC CORRELATION ANALYSIS

    SciTech Connect (OSTI)

    Ford, Eric B.; Moorhead, Althea V.; Morehead, Robert C. [Astronomy Department, University of Florida, 211 Bryant Space Sciences Center, Gainesville, FL 32611 (United States); Fabrycky, Daniel C. [UCO/Lick Observatory, University of California, Santa Cruz, CA 95064 (United States); Steffen, Jason H. [Fermilab Center for Particle Astrophysics, P.O. Box 500, MS 127, Batavia, IL 60510 (United States); Carter, Joshua A.; Fressin, Francois; Holman, Matthew J.; Ragozzine, Darin; Charbonneau, David [Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138 (United States); Lissauer, Jack J.; Rowe, Jason F.; Borucki, William J.; Bryson, Stephen T.; Burke, Christopher J.; Caldwell, Douglas A. [NASA Ames Research Center, Moffett Field, CA 94035 (United States); Welsh, William F. [Astronomy Department, San Diego State University, San Diego, CA 92182-1221 (United States); Allen, Christopher [Orbital Sciences Corporation/NASA Ames Research Center, Moffett Field, CA 94035 (United States); Batalha, Natalie M. [Department of Physics and Astronomy, San Jose State University, San Jose, CA 95192 (United States); Buchhave, Lars A., E-mail: eford@astro.ufl.edu [Niels Bohr Institute, Copenhagen University, DK-2100 Copenhagen (Denmark); Collaboration: Kepler Science Team; and others

    2012-05-10T23:59:59.000Z

    We present a new method for confirming transiting planets based on the combination of transit timing variations (TTVs) and dynamical stability. Correlated TTVs provide evidence that the pair of bodies is in the same physical system. Orbital stability provides upper limits for the masses of the transiting companions that are in the planetary regime. This paper describes a non-parametric technique for quantifying the statistical significance of TTVs based on the correlation of two TTV data sets. We apply this method to an analysis of the TTVs of two stars with multiple transiting planet candidates identified by Kepler. We confirm four transiting planets in two multiple-planet systems based on their TTVs and the constraints imposed by dynamical stability. An additional three candidates in these same systems are not confirmed as planets, but are likely to be validated as real planets once further observations and analyses are possible. If all were confirmed, these systems would be near 4:6:9 and 2:4:6:9 period commensurabilities. Our results demonstrate that TTVs provide a powerful tool for confirming transiting planets, including low-mass planets and planets around faint stars for which Doppler follow-up is not practical with existing facilities. Continued Kepler observations will dramatically improve the constraints on the planet masses and orbits and provide sensitivity for detecting additional non-transiting planets. If Kepler observations were extended to eight years, then a similar analysis could likely confirm systems with multiple closely spaced, small transiting planets in or near the habitable zone of solar-type stars.

  15. Transit Timing Observations from Kepler: II. Confirmation of Two Multiplanet Systems via a Non-parametric Correlation Analysis

    SciTech Connect (OSTI)

    Ford, Eric B.; /Florida U.; Fabrycky, Daniel C.; /Lick Observ.; Steffen, Jason H.; /Fermilab; Carter, Joshua A.; /Harvard-Smithsonian Ctr. Astrophys.; Fressin, Francois; /Harvard-Smithsonian Ctr. Astrophys.; Holman, Matthew J.; /Harvard-Smithsonian Ctr. Astrophys.; Lissauer, Jack J.; /NASA, Ames; Moorhead, Althea V.; /Florida U.; Morehead, Robert C.; /Florida U.; Ragozzine, Darin; /Harvard-Smithsonian Ctr. Astrophys.; Rowe, Jason F.; /NASA, Ames /SETI Inst., Mtn. View /San Diego State U., Astron. Dept.

    2012-01-01T23:59:59.000Z

    We present a new method for confirming transiting planets based on the combination of transit timing variations (TTVs) and dynamical stability. Correlated TTVs provide evidence that the pair of bodies are in the same physical system. Orbital stability provides upper limits for the masses of the transiting companions that are in the planetary regime. This paper describes a non-parametric technique for quantifying the statistical significance of TTVs based on the correlation of two TTV data sets. We apply this method to an analysis of the transit timing variations of two stars with multiple transiting planet candidates identified by Kepler. We confirm four transiting planets in two multiple planet systems based on their TTVs and the constraints imposed by dynamical stability. An additional three candidates in these same systems are not confirmed as planets, but are likely to be validated as real planets once further observations and analyses are possible. If all were confirmed, these systems would be near 4:6:9 and 2:4:6:9 period commensurabilities. Our results demonstrate that TTVs provide a powerful tool for confirming transiting planets, including low-mass planets and planets around faint stars for which Doppler follow-up is not practical with existing facilities. Continued Kepler observations will dramatically improve the constraints on the planet masses and orbits and provide sensitivity for detecting additional non-transiting planets. If Kepler observations were extended to eight years, then a similar analysis could likely confirm systems with multiple closely spaced, small transiting planets in or near the habitable zone of solar-type stars.

  16. A case for variational geomagnetic data assimilation: insights from a one-dimensional, nonlinear, and sparsely observed MHD system

    E-Print Network [OSTI]

    Fournier, Alexandre; Alboussière, Thierry

    2007-01-01T23:59:59.000Z

    Secular variations of the geomagnetic field have been measured with a continuously improving accuracy during the last few hundred years, culminating nowadays with satellite data. It is however well known that the dynamics of the magnetic field is linked to that of the velocity field in the core and any attempt to model secular variations will involve a coupled dynamical system for magnetic field and core velocity. Unfortunately, there is no direct observation of the velocity. Independently of the exact nature of the above-mentioned coupled system -- some version being currently under construction -- the question is debated in this paper whether good knowledge of the magnetic field can be translated into good knowledge of core dynamics. Furthermore, what will be the impact of the most recent and precise geomagnetic data on our knowledge of the geomagnetic field of the past and future? These questions are cast into the language of variational data assimilation, while the dynamical system considered in this pape...

  17. Avaliac~ao de Desempenho, Area e Energia de Caches com Controle de Poluic~ao

    E-Print Network [OSTI]

    Hexsel, Roberto A

    Avaliac¸~ao de Desempenho, ´Area e Energia de Caches com Controle de Poluic¸~ao Richard R de Souza´a Curitiba, PR, Brasil {rrs03,giancarlo,renato,roberto}@inf.ufpr.br Resumo Este artigo compara o desempenho, a ´area e o disp^endio de energia de quatro projetos do primeiro n´ivel da hie- rarquia de mem´oria para

  18. Visualizac~ao de Objetos Tridimensionais Baseada em Interpolac ~ao Projetiva

    E-Print Network [OSTI]

    como o processo de gerac¸~ao de imagens atrav´es do computador. Nesse artigo preferimos fazer distinc assunto, veja as refer^encias [Gomes e Velho, 1998, Gomes e Velho, 1994]. Síntese de Imagens Análise de Imagens Modelagem Geométrica Processamento de Imagens Imagens Dados Figura 1: Computac¸ ~ao Gr´afica. S

  19. Explorando Tecnicas de Reduc~ao de Base de Dados na Minerac~ao de Padr~oes Sequenciais

    E-Print Network [OSTI]

    Antwerpen, Universiteit

    Explorando T´ecnicas de Reduc¸~ao de Base de Dados na Minerac¸~ao de Padr~oes Seq¨uenciais Ciro mechanisms. Resumo. Neste trabalho, com o objetivo de reduzir o custo de diversas lei- turas da base de dados iterativos de extrac¸~ao de padr~oes seq¨uenciais, prop~oe-se a reduc¸~ao progressiva da base de dados ao

  20. AOS Solar Inc | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page onYou are now leaving Energy.gov You are now leaving Energy.gov You are beingZealand Jump to:Ezfeedflag JumpID-fTriWildcat 1AMEE Jump to: navigation, search Name: AMEEWindenergieAOS Solar

  1. Authorizing Official (AO) | Department of Energy

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels DataDepartment of Energy Your Density Isn't Your Destiny: The FutureComments from TarasaName4ServicesTribal RenewableAustin Energy(AO)

  2. apoio ao teste: Topics by E-print Network

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

    of the closed-loop performance of the Magellan Adaptive Optics (AO) Adaptive Secondary Mirror (ASM), pyramid wavefront sensor (PWFS), and VisAO visible adaptive optics camera. The...

  3. Cen ario Virtual e Composic ao de Imagens

    E-Print Network [OSTI]

    Cenâ?? ario Virtual e Composicâ?º â? ao de Imagens BRUNO COSTA 1 LUCIA DARSA 1 JONAS GOMES 1 PAULO ROMA poderosa para esse propâ??osito â?? e a combinacâ?ºâ?ao de imagens. Glass­shots, mirror­shots e back­projection sâ?ao algumas das tâ??ecnicas tradicionais de combinacâ?ºâ?ao de imagens. Neste trabalho, descrevemos um sistema

  4. university-logo Modelos de Execuc~ao

    E-Print Network [OSTI]

    Rodriguez, Noemi

    university-logo Modelos de Execu¸c~ao Bolsas de Tarefas November 5, 2009 Modelos de Execu¸c~ao Bolsas de Tarefas #12;university-logo Modelos SPMD/MPI todos os processos executam o mesmo c;university-logo Dificuldades ambientes heterog^eneos ambientes com carga externa `a aplica¸c~ao tarefas om

  5. Aerosol Observing System Upgraded

    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) VAP7-0973 1BP-14Scripting for AdvancedSensitivitySensitivity of2

  6. Correla\\c{c}\\~ao de longa-dura\\c{c}\\~ao e anal\\'ise bayesiana da evolu\\c{c}\\~ao temporal dos terremotos ao longo da falha de samambaia, nordeste do brasil

    E-Print Network [OSTI]

    de Freitas, D B; Pereira, L L S; Pedro, L S; Atanazio, M G N; Vilar, C S

    2013-01-01T23:59:59.000Z

    A Bayesian approach is adopted to analyze the sequence of seismic events and their magnitudes near Jo\\~ao C\\^amara which occurred mainly from 1983 to 1998 along the Samambaia fault. In this work, we choose a Bayesian model for the process of occurrence times conditional on the observed magnitude values following the same procedure suggested by Stavrakakis and Tselentis (1987). The model parameters are determined on the basis of historical and physical information. We generate posterior samples from the joint posterior distribution of the model parameters by using a variant of the Metropolis-Hastings algorithm. We use the results in a variety of ways, including the construction of pointwise posterior confidence bands for the conditional intensity of the point process as a function of time, as well as, a posterior distribuition as a function of the mean of occurrence per unit time.

  7. Explorando a Tecnica de Indexac~ao de Conjuntos Candidatos na Minerac~ao de Conjuntos Frequentes

    E-Print Network [OSTI]

    Antwerpen, Universiteit

    suportes baixos s~ao considerados sobre bases de dados es- parsas. A fim de aprimorar seu desempenho, neste suporte m´inimo) das transac¸~oes em uma base de dados. A extrac¸~ao de tais conjuntos representa a fase t~ao eficiente quando valores baixos de suporte m´inimo s~ao considerados sobre bases de dados

  8. Causes of variation in soil carbon simulations from CMIP5 Earth system models and comparison with observations

    E-Print Network [OSTI]

    2013-01-01T23:59:59.000Z

    and benchmarks in Earth system models sitivity of the Amazonand benchmarks in Earth system models Thornton, P. E. ,simulations from CMIP5 Earth system models and comparison

  9. CCM128 COMPUTAC ~AO II INFORMAC ~OES GERAIS

    E-Print Network [OSTI]

    Kohayakawa, Yoshiharu

    CCM128 COMPUTAC¸ ~AO II INFORMAC¸ ~OES GERAIS Bem-vindos `a edi¸c~ao do 1o. semestre de 2014 de CCM´aticos ser~ao sugeridos durante o semestre. Diferentemente de como foi em CCM118, os exerc´icios de CCM128ii/ccm128 Esta p´agina conter´a algum material de suporte para as aulas. Veja tamb´em o sistema Paca

  10. EXERCICIOS MAC430 ALGORITMOS E COMPLEXIDADE DE COMPUTAC ~AO

    E-Print Network [OSTI]

    Kohayakawa, Yoshiharu

    . Os problemas e exerc´icios com data de entrega devem ser resolvidos e entregues. Estes exerc´iciosEXERC´ICIOS MAC430 ALGORITMOS E COMPLEXIDADE DE COMPUTAC¸ ~AO 2O. SEMESTRE DE 2012 Instru¸c~oes: 1 far~ao parte de sua avalia¸c~ao. 2. A entrega dos exerc´icios deve ser feita no come¸co da aula (as

  11. Dynamics of observables and exactly solvable quantum problems: Using time-dependent density functional theory to control quantum systems

    E-Print Network [OSTI]

    Mehdi Farzanehpour; I. V. Tokatly

    2015-06-29T23:59:59.000Z

    We use analytic (current) density-potential maps of time-dependent (current) density functional theory (TD(C)DFT) to inverse engineer analytically solvable time-dependent quantum problems. In this approach the driving potential (the control signal) and the corresponding solution of the Schr\\"odinger equation are parametrized analytically in terms of the basic TD(C)DFT observables. We describe the general reconstruction strategy and illustrate it with a number of explicit examples. First we consider the real space one-particle dynamics driven by a time-dependent electromagnetic field and recover, from the general TDDFT reconstruction formulas, the known exact solution for a driven oscillator with a time-dependent frequency. Then we use analytic maps of the lattice TD(C)DFT to control quantum dynamics in a discrete space. As a first example we construct a time-dependent potential which generates prescribed dynamics on a tight-binding chain. Then our method is applied to the dynamics of spin-1/2 driven by a time dependent magnetic field. We design an analytic control pulse that transfers the system from the ground to excited state and vice versa. This pulse generates the spin flip thus operating as a quantum NOT gate.

  12. In operando observation system for electrochemical reaction by soft X-ray absorption spectroscopy with potential modulation method

    SciTech Connect (OSTI)

    Nagasaka, Masanari, E-mail: nagasaka@ims.ac.jp; Kosugi, Nobuhiro [Institute for Molecular Science, Myodaiji, Okazaki 444-8585 (Japan); The Graduate University for Advanced Studies, Myodaiji, Okazaki 444-8585 (Japan); Yuzawa, Hayato; Horigome, Toshio [Institute for Molecular Science, Myodaiji, Okazaki 444-8585 (Japan)

    2014-10-15T23:59:59.000Z

    In order to investigate local structures of electrolytes in electrochemical reactions under the same scan rate as a typical value 100 mV/s in cyclic voltammetry (CV), we have developed an in operando observation system for electrochemical reactions by soft X-ray absorption spectroscopy (XAS) with a potential modulation method. XAS spectra of electrolytes are measured by using a transmission-type liquid flow cell with built-in electrodes. The electrode potential is swept with a scan rate of 100 mV/s at a fixed photon energy, and soft X-ray absorption coefficients at different potentials are measured at the same time. By repeating the potential modulation at each fixed photon energy, it is possible to measure XAS of electrochemical reaction at the same scan rate as in CV. We have demonstrated successful measurement of the Fe L-edge XAS spectra of aqueous iron sulfate solutions and of the change in valence of Fe ions at different potentials in the Fe redox reaction. The mechanism of these Fe redox processes is discussed by correlating the XAS results with those at different scan rates.

  13. ao caso brasileiro: Topics by E-print Network

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

    Brasileiro na Dcada de Oitenta University of Kansas - KU ScholarWorks Summary: Montenegro. Por sua vez, o Servio Nacional do Teatro, visando incentivar a ida ao teatro,...

  14. INTRODUC¸ ˜AO `AS TRANSFORMADAS DE RADON 1. Introduç ...

    E-Print Network [OSTI]

    2003-08-11T23:59:59.000Z

    em 1956 quando trabalhava no departamento de radiologia do hospital Groote Schurr (o mesmo onde foi feito o primeiro transplante de coraç˜ao) na cidade do

  15. associadas ao carcinoma: Topics by E-print Network

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

    como objetivos analisar as associaes entre a presena de risco ao desenvolvimento infantil e variveis socioeconmicas, demogrficas, psicossociais e obsttricas, e...

  16. Sistema Composto para Amostragem e Gerac~ao de Luzes a partir de Mapas de Iluminac~ao

    E-Print Network [OSTI]

    ´eticos em cenas reais ´e pre- ciso dispor da iluminac¸~ao do ambiente real onde ser´a feita a inserc

  17. CCM118 COMPUTAC ~AO I INFORMAC ~OES GERAIS

    E-Print Network [OSTI]

    Kohayakawa, Yoshiharu

    CCM118 COMPUTAC¸ ~AO I INFORMAC¸ ~OES GERAIS Bem-vindos `a edi¸c~ao do 2o. semestre de 2013 de CCM://www.ime.usp.br/~yoshi/2013ii/ccm118 Esta p´agina conter´a algum material de suporte para as aulas. Veja tamb´em o sistema

  18. CCM128 COMPUTAC ~AO II INFORMAC ~OES GERAIS

    E-Print Network [OSTI]

    Kohayakawa, Yoshiharu

    CCM128 COMPUTAC¸ ~AO II INFORMAC¸ ~OES GERAIS Bem-vindos `a edi¸c~ao do 1o. semestre de 2010 de CCM://www.ime.usp.br/~yoshi/2010i/ccm128 Esta p´agina conter´a algum material de suporte para as aulas. Veja tamb´em o sistema Paca

  19. CCM118 COMPUTAC ~AO I INFORMAC ~OES GERAIS

    E-Print Network [OSTI]

    Kohayakawa, Yoshiharu

    CCM118 COMPUTAC¸ ~AO I INFORMAC¸ ~OES GERAIS Bem-vindos `a edi¸c~ao do 2o. semestre de 2009 de CCM disciplina: Teremos uma p´agina na rede: http://www.ime.usp.br/~yoshi/2009ii/ccm118 Esta p´agina conter

  20. AO DO FLUXO DE POT ENCIA EM AMBIENTE VETORIAL USANDO

    E-Print Network [OSTI]

    Coutinho, Alvaro L. G. A.

    --970, Brasil. Resumo Este trabalho apresenta um m'etodo de solu¸c~ao do problema de Fluxo de Potâ??encia usando o¸c~ao de energia el'etrica, assim como in'umeros problemas em engenharia e ou­ tras ciâ??encias, requer

  1. Optimally Robust Kalman Filtering at Work: AO-, IO-, and Simultaneously IO-and AO-Robust Filters

    E-Print Network [OSTI]

    Ruckdeschel, Peter

    Optimally Robust Kalman Filtering at Work: AO-, IO-, and Simultaneously IO- and AO- Robust Filters Abstract We take up optimality results for robust Kalman filtering from Ruckdeschel (2001, 2010) where. (2006), Fried et al. (2007). Keywords: robustness, Kalman Filter, innovation outlier, additive outlier

  2. DEVELOPMENT OF A COASTAL MARGIN OBSERVATION AND ASSESSMENT SYSTEM (CMOAS) TO CAPTURE THE EPISODIC EVENTS IN A SHALLOW BAY 

    E-Print Network [OSTI]

    Islam, Mohammad S.

    2010-07-14T23:59:59.000Z

    in real-time monitoring of hydrodynamic, meteorological and water quality parameters in the bay. Three different platform types used for the installation of sensor systems are: 1) Fixed Robotic, 2) Mobile, and 3) Remote. An automated profiler system...

  3. U and Th zonation in apatite observed by laser ablation ICPMS, and implications for the (UTh)/He system

    E-Print Network [OSTI]

    Shuster, David L.

    U and Th zonation in apatite observed by laser ablation ICPMS, and implications for the (U A laser-ablation inductively-coupled plasma mass spectrometry technique was developed to measure U, Th

  4. New Observations of Extra-Disk Molecular Gas in Interacting Galaxy Systems, Including a Two-Component System in Stephan's Quintet

    E-Print Network [OSTI]

    B. J. Smith; C. Struck

    2000-11-03T23:59:59.000Z

    We present new CO (1 - 0) observations of eleven extragalactic tails and bridges in nine interacting galaxy systems, almost doubling the number of such features with sensitive CO measurements. Eight of these eleven features were undetected in CO to very low CO/HI limits, with the most extreme case being the NGC 7714/5 bridge. This bridge contains luminous H II regions and has a very high HI column density (1.6 X 10^21 cm^-2 in the 55" CO beam), yet was undetected in CO to rms T(R)* = 2.4 mK. The HI column density is higher than standard H2 and CO self-shielding limits for solar-metallicity gas, suggesting that the gas in this bridge is metal-poor and has an enhanced N(H2)/I(CO) ratio compared to the Galactic value. Only one of the eleven features in our sample was unambiguously detected in CO, a luminous HI-rich star formation region near an optical tail in the compact group Stephan's Quintet. We detect CO at two widely separated velocities in this feature, at ~6000 km/s and ~6700 km/s. Both of these components have HI and H-alpha counterparts. These velocities correspond to those of galaxies in the group, suggesting that this gas is material that has been removed from two galaxies in the group. The CO/HI/H-alpha ratios for both components are similar to global values for spiral galaxies.

  5. Event-Triggered Observer-based Output-Feedback Stabilization of Linear System with Communication Delays in the Measurements

    E-Print Network [OSTI]

    Boyer, Edmond

    Department of GIPSA-lab, CNRS, Univ. of Grenoble, Grenoble, France. Institute of Engineering, UNAM, Mexico City, Mexico. Faculty of Electronics, Autonomous University of Puebla (BUAP), Puebla, Mexico. E, miniaturized and interconnected systems, there is a growing interest in Net- worked Control Systems (NCSs

  6. Development of a high dynamic range spectroscopic system for observation of neutral hydrogen atom density distribution in Large Helical Device core plasma

    SciTech Connect (OSTI)

    Fujii, K., E-mail: fujii@me.kyoto-u.ac.jp; Atsumi, S.; Watanabe, S.; Shikama, T.; Hasuo, M. [Department of Mechanical Engineering and Science, Graduate School of Engineering, Kyoto University, Kyoto 606-8540 (Japan)] [Department of Mechanical Engineering and Science, Graduate School of Engineering, Kyoto University, Kyoto 606-8540 (Japan); Goto, M.; Morita, S. [National Institute for Fusion Science, Toki 509-5292 (Japan)] [National Institute for Fusion Science, Toki 509-5292 (Japan)

    2014-02-15T23:59:59.000Z

    We report development of a high dynamic range spectroscopic system comprising a spectrometer with 30% throughput and a camera with a low-noise fast-readout complementary metal-oxide semiconductor sensor. The system achieves a 10{sup 6} dynamic range (?20 bit resolution) and an instrumental function approximated by a Voigt profile with Gauss and Lorentz widths of 31 and 0.31 pm, respectively, for 656 nm light. The application of the system for line profile observations of the Balmer-? emissions from high temperature plasmas generated in the Large Helical Device is also presented. In the observed line profiles, emissions are detected in far wings more than 1.0 nm away from the line center, equivalent to neutral hydrogen atom kinetic energies above 1 keV. We evaluate atom density distributions in the core plasma by analyzing the line profiles.

  7. ao trauma perineal: Topics by E-print Network

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

    painful information that clients are not yet ready to confront or divulge. Ann S. Uhler; Olga V. Parker, Ph.D. 67 Logica Computacional Verificac ao com Logicas Temporais...

  8. ao-assisted integral-field observations: Topics by E-print Network

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

    SINFONI at the ESO Very Large Telescope in the near-infrared (K-band), using adaptive optics to correct for the blurring effect of the earth atmosphere. The data have a spatial...

  9. Observed Characteristics of Clouds and Precipitating Systems Associated with the Tropical Circulation in Global Models and Reanalyses

    E-Print Network [OSTI]

    Stachnik, Justin Paul

    2013-03-25T23:59:59.000Z

    This dissertation presents a series of work related to the representation of the Hadley circulation (HC) in atmospheric reanalyses and general circulation models (GCMs), with connections to the underlying tropical and subtropical cloud systems...

  10. Reconstruc~ao de Imagens de Resson^ancia Magnetica de Fluxo com Compressed Sensing

    E-Print Network [OSTI]

    Carvalho, João Luiz

    ´obitos no Brasil. A visualiza¸c~ao e quantifica¸c~ao do fluxo cardiovascular trazem informa) reconstru¸c~ao por energia m´inima, (d) reconstru¸c~ao por CS [3]. s~ao as diferen¸cas finitas nas dire a energia do sinal esteja fortemente concentrada em

  11. Collaborative Research: Focusing Attention to Improve the Performance of Citizen Science Systems -Beautiful Images and Perceptive Observers

    E-Print Network [OSTI]

    Crowston, Kevin

    Collaborative Research: Focusing Attention to Improve the Performance of Citizen Science Systems unable to replicate the successes of human pattern recognition. The growth of citizen science on the web-computational citizen science platform that combines the efforts of human classifiers with those of computational

  12. A.O. Smith: Demonstrate Underutilized micro-CHP - 2015 Peer Review...

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

    A.O. Smith: Demonstrate Underutilized micro-CHP - 2015 Peer Review A.O. Smith: Demonstrate Underutilized micro-CHP - 2015 Peer Review Presenter: Kris Jorgensen, A.O. Smith View the...

  13. Harmonic QPOs and Thick Accretion Disk Oscillations in BL Lac Object AO 0235+164

    E-Print Network [OSTI]

    F. K. Liu; G. Zhao; Xue-Bing Wu

    2006-06-27T23:59:59.000Z

    Periodic outbursts are observed in many AGNs and usually explained with a supermassive black hole binary (SMBHB) scenario. However, multiple periods are observed in some AGNs and cannot be explained with it. Here we analyze the periodicity of the radio light curves of AO 0235+164 at multi-frequencies and report the discovery of six QPOs in integer ratio 1:2:3:4:5:6 of QPO frequencies, of which the second with period $P_2 = (5.46 \\pm 0.47) {\\rm yr}$ is the strongest. We fit the radio light curves and show that the initial phases of six QPOs have zero or $\\pi$ differences relative to each other. We suggest a harmonic relationship of QPOs. The centroid frequency, relative strength, harmonic relationship and relative initial phases of QPOs are independent of radio frequency. The harmonic QPOs are likely due to the quasi-periodic injection of plasma from an oscillating accretion disk into the jet. We estimate the supermassive black hole mass $M_{\\rm BH} \\simeq (4.72\\pm 2.04) \\times 10^8 M_\\odot$ and the accretion rate $\\dot{m}\\simeq 0.007$. With the knowledge of accretion disk, it implies that the inner region of accretion disk of AO 0235+164 is a radiatively inefficient accretion flow. The oscillation accretion is due to the p-mode oscillation of the thick disk probably excited by a SMBHB. The theoretical predications of fundamental oscillation frequency and the harmonics are well consistent with the observations. Harmonic QPOs would be absent when the thick disk becomes geometrically thin due to the increase of accretion rate. We discuss the observations of AO 0235+164 basing on the SMBHB-thick disk oscillation scenario.

  14. The formation and maintenance of single-thread tie channels entering floodplain lakes: observations from three diverse river systems

    SciTech Connect (OSTI)

    Rowland, Joel C [Los Alamos National Laboratory; Dietrich, William E [UC BERKELEY; Day, Geoff [NEWCREST MINING; Parker, Gary [UNIV OF ILLINOIS

    2009-01-01T23:59:59.000Z

    Tie channels connect rivers to floodplain lakes on many lowland rivers and thereby play a central role in floodplain sedimentology and ecology, yet they are generally unrecognized and little studied. here we report the results of field studies focused on tie channel origin and morphodynamics in three contrasting systems: the Middle Fly River, Papua New Guinea, the Lower Mississippi River, and Birch Creek in Alaska. Across these river systems, tie channels vary by an order of magnitude in size but exhibit the same characteristic morphology and appear to develop and evolve by a similar set of processes. In all three systems, the channels are characterized by a narrow, leveed single-thread morphology with maximum width approximately one tenth the width of the mainstem river. The channels typically have a V shaped cross-section, unlike most fluvial channels. These channels develop as lakes become isolated from the river by sedimentation. Narrowing of the connection between river and lake causes a sediment-laden jet to develop. Levees develop along the margins of the jet leading to channel emergence and eventual levee aggradation to the height of the mainstem levees. Bi-directional flow in these channels is common. Outflows from the lake scour sediment and prevent channel blockage. We propose that channel geometry and size are then controlled by a dynamic balance between channel narrowing by suspended sediment deposition and incision and widening by mass failure of banks during outflows. Tie channels are laterally stable and may convey flow for hundreds to a few thousand of years.

  15. Hoje sera disponiblizada a Lista de Exercicios 4: combinac~ao linear, vetores LI e LD, base, dimens~ao, produto

    E-Print Network [OSTI]

    Dutenhefner, Francisco

    . Terceira prova: 15/junho - 10:00 horas - ICEx. #12;Combina¸c~ao Linear, base e dimens~ao Sejam dados V1 modo V = x1V1 + x2V2 + · · · + xkVk. #12;Combina¸c~ao Linear, base e dimens~ao Sejam dados V1 as combina¸c~oes lineares de V1, . . . , Vk. #12;Combina¸c~ao Linear, base e dimens~ao Sejam dados V1

  16. Spectrum of wind speed fluctuations encountered by a rotating blade of a wind energy conversion system: observations and theory

    SciTech Connect (OSTI)

    Connell, J.R.

    1981-11-01T23:59:59.000Z

    This report proves that the characteristics of turbulence that are experienced by a rotating wind turbine rotor blade are in principle and in practice very different than those experienced by a nonrotating rotor blade. Thus conventional wind characteristics, which are formulated for the nonrotating frame of reference, are more inaccurate than generally supposed. The measurements and mathematical model that are presented for turbulence observed in the rotating frame of reference represent the third phase of the Pacific Northwest Laboratory work aimed at providing an accurate turbulence description for use in the design and evaluation of the performance of wind turbines. The first phase of work was the measurement of wind with a vertical plane array of anemometers. The second phase was the physical interpretation of the measurements in terms of implications for wind turbine rotors and initiation of development of a model of wind/wind turbine interaction. The third phase involved measurement of turbulence by rotating sensors and mathematical development of a physical model of this representation of turbulence as independent checks and expansions of the vertical plane array results. A fourth phase, to correlate real wind turbine response with rotationally measured turbulence and thereby understand the wind/wind turbine interaction, is in progress and preliminary results are quite promising.

  17. THE EVOLUTION OF CIRCUMPLANETARY DISKS AROUND PLANETS IN WIDE ORBITS: IMPLICATIONS FOR FORMATION THEORY, OBSERVATIONS, AND MOON SYSTEMS

    SciTech Connect (OSTI)

    Shabram, Megan; Boley, Aaron C. [Department of Astronomy, University of Florida, 211 Bryant Space Center, Gainesville, FL 32611 (United States)] [Department of Astronomy, University of Florida, 211 Bryant Space Center, Gainesville, FL 32611 (United States)

    2013-04-10T23:59:59.000Z

    Using radiation hydrodynamics simulations, we explore the evolution of circumplanetary disks around wide-orbit proto-gas giants. At large distances from the star ({approx}100 AU), gravitational instability followed by disk fragmentation can form low-mass substellar companions (massive gas giants and/or brown dwarfs) that are likely to host large disks. We examine the initial evolution of these subdisks and their role in regulating the growth of their substellar companions, as well as explore consequences of their interactions with circumstellar material. We find that subdisks that form in the context of GIs evolve quickly from a very massive state. Long-term accretion rates from the subdisk onto the proto-gas giant reach {approx}0.3 Jupiter masses kyr{sup -1}. We also find consistency with previous simulations, demonstrating that subdisks are truncated at {approx}1/3 of the companion's Hill radius and are thick, with (h/r) of {approx}> 0.2. The thickness of subdisks draws to question the use of thin-disk approximations for understanding the behavior of subdisks, and the morphology of subdisks has implications for the formation and extent of satellite systems. These subdisks create heating events in otherwise cold regions of the circumstellar disk and serve as planet formation beacons that can be detected by instruments such as ALMA.

  18. Exercicios de Calculo Numerico Integrac~ao Numerica

    E-Print Network [OSTI]

    Cabral, Marco

    Exerc´icios de C´alculo Num´erico Integra¸c~ao Num´erica 1. Calcule as integrais abaixo pela regra(x, y, z) = (xy)z . Calcule valor num´erico de cada integral usando as f´ormulas anteriores, com passo h

  19. FSE IPSE (2014 AO Admission) Faculty of Science and Engineering

    E-Print Network [OSTI]

    Kaji, Hajime

    ability who are grounded in science and engineering knowledge such as math in addition to humanitiesFSE IPSE (2014 AO Admission) Faculty of Science and Engineering School of Fundamental Science and Engineering School of Creative Science and Engineering School of Advanced Science and Engineering WASEDA

  20. ao gas natural: Topics by E-print Network

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

    ao gas natural First Page Previous Page 1 2 3 4 5 6 7 8 9 10 11 12 13 14 15 16 17 18 19 20 21 22 23 24 25 Next Page Last Page Topic Index 1 NATURAL GAS MARKET ASSESSMENT Energy...

  1. ao acordo nuclear: Topics by E-print Network

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

    ao acordo nuclear First Page Previous Page 1 2 3 4 5 6 7 8 9 10 11 12 13 14 15 16 17 18 19 20 21 22 23 24 25 Next Page Last Page Topic Index 1 UIIVERSIDADE DA CORUA ACORDO ENTRE O...

  2. GOALS, STRATEGIES AND FIRST DISCOVERIES OF AO327, THE ARECIBO ALL-SKY 327 MHz DRIFT PULSAR SURVEY

    SciTech Connect (OSTI)

    Deneva, J. S. [Arecibo Observatory, HC3 Box 53995, Arecibo, PR 00612 (United States); Stovall, K.; Martinez, J. G.; Jenet, F. [Center for Advanced Radio Astronomy, Department of Physics and Astronomy, University of Texas at Brownsville, Brownsville, TX 78520 (United States); McLaughlin, M. A.; Bates, S. D.; Bagchi, M. [Department of Physics, West Virginia University, 111 White Hall, Morgantown, WV 26506 (United States); Freire, P. C. C. [Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, D-53121 Bonn (Germany)

    2013-09-20T23:59:59.000Z

    We report initial results from AO327, a drift survey for pulsars with the Arecibo telescope at 327 MHz. The first phase of AO327 will cover the sky at declinations of –1° to 28°, excluding the region within 5° of the Galactic plane, where high scattering and dispersion make low-frequency surveys sub-optimal. We record data from a 57 MHz bandwidth with 1024 channels and 125 ?s sampling time. The 60 s transit time through the AO327 beam means that the survey is sensitive to very tight relativistic binaries even with no acceleration searches. To date we have detected 44 known pulsars with periods ranging from 3 ms to 2.21 s and discovered 24 new pulsars. The new discoveries include 3 ms pulsars, three objects with periods of a few tens of milliseconds typical of young as well as mildly recycled pulsars, a nuller, and a rotating radio transient. Five of the new discoveries are in binary systems. The second phase of AO327 will cover the sky at declinations of 28°-38°. We compare the sensitivity and search volume of AO327 to the Green Bank North Celestial Cap survey and the GBT350 drift survey, both of which operate at 350 MHz.

  3. Partial Observers

    E-Print Network [OSTI]

    Thomas Marlow

    2006-10-20T23:59:59.000Z

    We attempt to dissolve the measurement problem using an anthropic principle which allows us to invoke rational observers. We argue that the key feature of such observers is that they are rational (we need not care whether they are `classical' or `macroscopic' for example) and thus, since quantum theory can be expressed as a rational theory of probabilistic inference, the measurement problem is not a problem.

  4. Segmentac~ao e Classificac~ao de Padr~oes Visuais Baseadas em Campos Receptivos e Inibitorios

    E-Print Network [OSTI]

    Lewiner, Thomas (Thomas Lewiner)

    on Receptive Fields (SCRF). O outro ´e uma nova rede neural, chamada I-PyraNet. A I-PyraNet ´e uma implementac modelo SCRF e a I-PyraNet foram aplicados juntos num problema de detecc¸~ao de floresta em imagens de sat on the concepts of receptive fields, called Segmentation and Classification Based on Receptive Fields (SCRF

  5. Sobre a viagem de Enrico Fermi ao Brasil em 1934

    E-Print Network [OSTI]

    Caruso, Francisco

    2014-01-01T23:59:59.000Z

    Enrico Fermi was one of the greater physicists of the XX century. In 1934, he gave several lectures in Brazil. Invited by Theodoro Ramos to work in S\\~ao Paulo, he preferred to stay in Rome and went to the USA in 1938. However, Fermi recommended Gleb Wataghin to come in his place. Wataghin made history in Brazil, becoming one of the first Professors of the future S\\~ao Paulo University. Besides his relevance to the History of Science, Fermi eventually leaved an indelible mark on the creation and institutionalization of national scientific research due to the indication of Wataghin. Despite this fact, very little is known about Fermi's trip to Brazil. This work tries to reconstruct the fullest possible steps of the famous Italian physicist in our lands.

  6. ARM - Mobile Aerosol Observing System

    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 3,625govInstrumentstdmadap Documentation TDMADAP : XDCnarrowbandheat flux ARMMeasurementsMethane Gas

  7. ARM - Surface Aerosol Observing System

    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 3,625govInstrumentstdmadap Documentation TDMADAP :ProductsVaisalaAlaskaInstruments NSASteering

  8. Maoming Zhong ao Wind Power Co Ltd | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page onYou are now leaving Energy.gov You are now leaving Energy.gov You are being directedAnnual Siteof Energy 2,AUDIT REPORTEnergyFarmsPower CoLongxing WindMaoming Zhong ao Wind Power Co

  9. SMIT: Uma Arquitetura Tolerante a Intrus~oes Baseada em Virtualizac~ao

    E-Print Network [OSTI]

    Correia, Miguel

    . Sistemas financeiros, de controle de gerac¸~ao e distribuic¸~ao de energia, de controle de dispositivos a necessidade de, no m´inimo, 3f + 1 r´eplicas para tolerar faltas bizantinas [Lamport et al. 1982

  10. Reconstruc~ao de Objetos 3D usando Modelos Deform aveis Rosana Marques da Silva

    E-Print Network [OSTI]

    ~ao A reconstruc~ao de modelos 3D a partir de imagens pode ser, convenientemente, separado em dois est a- gios. O amostrados nas imagens, enquanto o segundo concentra-se na transformac~ao dessas in- formac~oes em um modelo equilibrio energia m nima. As forcas externas s~ao estimadas a partir de informac~oes extra das das imagens

  11. Reconstruc~ao de Imagens de Resson^ancia Magnetica de Fluxo com Imageamento Paralelo

    E-Print Network [OSTI]

    Carvalho, João Luiz

    paralelo para a reconstru¸c~ao de dados reais e dados simulados em computador (phantoms num´ericos amostrados completamente. Reconstru¸c~ao de um phantom num´erico usando SOS e dados amostrados completamente um phantom num´erico usando algoritmo SOS e dados subamostrados. Reconstru¸c~ao de um conjunto de

  12. RECONSTRU C~AO DE IMAGENS DE RESSON^ANCIA MAGNETICA DE FLUXO COM IMAGEAMENTO PARALELO

    E-Print Network [OSTI]

    Carvalho, João Luiz

    RECONSTRU ¸C~AO DE IMAGENS DE RESSON^ANCIA MAGN´ETICA DE FLUXO COM IMAGEAMENTO PARALELO Davi Marco o objetivo de permitir uma correta reconstru¸c~ao de imagens. T´ecnicas de imageamento paralelo como paralelo, SENSE, gridding, subamostragem, spiral FVE 1 Introdu¸c~ao O uso de imagens m´edicas vem sendo bem

  13. Visualizac~ao de Panoramas Virtuais Andr'e Machado de Matos

    E-Print Network [OSTI]

    visualizacao em tempo real, deformacao de imagens, gerenciamento de cache e imagens em multiresolucao Abstract¸c~ao Baseada em Imagens . . . . . . . . . . . 12 2.5.3 Convers~ao entre Descri¸c~oes e M'etodos H Renderiza¸c~ao Baseada em Imagens 15 3.1 Origens

  14. Field observations and lessons learned

    SciTech Connect (OSTI)

    Nielsen, Joh B [Los Alamos National Laboratory

    2010-01-01T23:59:59.000Z

    This presentation outlines observations and lessons learned from the Megaports program. It provides: (1) details of field and technical observations collected during LANL field activities at ports around the world and details of observations collected during radiation detections system testing at Los Alamos National Laboratory; (2) provides suggestions for improvement and efficiency; and (3) discusses possible program execution changes for more effective operations.

  15. ESTIMATIVAS DA AREA DE ATRAC~AO DE SISTEMAS N~AO LINEARES COM INCERTEZAS VARIANTES NO TEMPO POR MEIO DE UMA CLASSE DE

    E-Print Network [OSTI]

    Pota, Himanshu Roy

    ~ao diferencial linear. Usando-se esta representa¸c~ao do sistema original, prop~oe-se um algoritmo num´erico´ivel. Um exemplo num´erico ´e apresentado para demonstrar a validade da abordagem proposta. Palavras (?) e sistemas de pot^encia (?). Recentemente, m´etodos num´ericos tem sido desenvolvidos para an

  16. arXiv:0905.3759v3[nlin.AO]27Jan2010 Evolving networks and the development of neural

    E-Print Network [OSTI]

    Johnson, Samuel

    arXiv:0905.3759v3[nlin.AO]27Jan2010 Evolving networks and the development of neural systems Samuel Johnson, J. Marro and Joaqu´in J. Torres Departamento de Electromagnetismo y F´isica de la Materia Granada, Spain. E-mail: samuel@onsager.ugr.es, jmarro@ugr.es and jtorres@onsager.ugr.es Abstract

  17. Impacto das politicas de replicac~ao na disponibilidade de documentos em redes P2P sob ataques DoS

    E-Print Network [OSTI]

    Guedes, Dorgival

    to detect and to prevent. That has led to studies on attack-tolerant systems, usually based on P2P networks empresas. Os tipos mais comuns de ataques maliciosos, devido `a dificuldade de defesa, s~ao os ataques de

  18. Grids Computacionais: da Computac~ao de Alto Desempenho a Servicos sob Demanda

    E-Print Network [OSTI]

    Cirne, Walfredo

    a HP Brasil P&D e conta com suporte do CNPq. #12;1.1. Introduc¸~ao Grids Computacionais s~ao atualmente A Rede El´etrica (The Electric Grid) [1]. A Rede El´etrica disponibiliza energia el´etrica sob demanda e esconde do usu´ario detalhes como a origem da energia e a complexidade da malha de transmiss~ao e

  19. ao 138-7 experiment: Topics by E-print Network

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

    mask, which should offer a highly stable solution for telescopes without adaptive optics (AO) for wavefront correction in space missions. The primary aim of this work was to...

  20. Estudantes universitrios devem mais de 200 milhes de euros aos bancos

    E-Print Network [OSTI]

    Instituto de Sistemas e Robotica

    , de 25 anos, no quarto ano da licenciatura em Enfer- magem, recorreu ao empréstimo de- vido à difícil

  1. MAC323 EXERCICIO-PROGRAMA 3 LOCALIZAC~AO DE PALAVRAS I

    E-Print Network [OSTI]

    Kohayakawa, Yoshiharu

    /6/2013 (23:55) 1. Introdu¸c~ao Nos EPs 3 e 4, voc^e far´a alguns exerc´icios simples envolvendo textos e PLN (por exemplo, dado T, determinar as senten¸cas que com- p~oe T) ser~ao resolvidos usando um

  2. Departamento de Matematica do IST, Secc~ao de Algebra e Analise Analise Matematica III

    E-Print Network [OSTI]

    Granja, Gustavo

    ´iveis na web, s~ao uma excelente introdu¸c~ao `a mat´eria. Exerc´icios Resolvidos: Na webpage da cadeira encontram-se links para listas de exerc´icios resolvidos assim como para enunciados e algumas resolu/ou exames resolvidos. (Encontram-se por vezes `a venda listas de exerc´icios resolvidos de qualidade duvi

  3. Reconstruc~ao Paralelizada de Dados de Resson^ancia Magnetica de Fluxo em

    E-Print Network [OSTI]

    Carvalho, João Luiz

    imagens desejadas exige um processamento computacional, chamado de reconstru¸c~ao. Existem diversas t desenvolver algoritmos r´apidos para a reconstru¸c~ao de imagens de RM, por meio do uso de n´ucleos de tratamento mais eficiente. As imagens de fluxo permitem a an´alise de muitas dessas doen¸cas. No entanto, o

  4. Visualizac~ao de Panoramas Virtuais Andr e Machado de Matos

    E-Print Network [OSTI]

    visualizacao em tempo real, deformacao de imagens, gerenciamento de cache e imagens em multiresolucao Abstract em Imagens . . . . . . . . . . . 12 2.5.3 Convers~ao entre Descric~oes e M etodos H bridos Renderizac~ao Baseada em Imagens 15 3.1 Origens

  5. arXiv:1408.2487v2[physics.ao-ph]22Aug2014 Ising model for melt ponds on Arctic sea ice

    E-Print Network [OSTI]

    Golden, Kenneth M.

    arXiv:1408.2487v2[physics.ao-ph]22Aug2014 Ising model for melt ponds on Arctic sea ice Yi-Ping Ma,1, USA The albedo of melting Arctic sea ice, a key parameter in climate modeling, is determined by pools of water on the ice surface. Recent observations show an onset of pond complexity at a critical area

  6. Analysis of Cloud-resolving Simulations of a Tropical Mesoscale Convective System Observed during TWP-ICE: Vertical Fluxes and Draft Properties in Convective and Stratiform Regions

    SciTech Connect (OSTI)

    Mrowiec, Agnieszka A.; Rio, Catherine; Fridlind, Ann; Ackerman, Andrew; Del Genio, Anthony D.; Pauluis, Olivier; Varble, Adam; Fan, Jiwen

    2012-10-02T23:59:59.000Z

    We analyze three cloud-resolving model simulations of a strong convective event observed during the TWP-ICE campaign, differing in dynamical core, microphysical scheme or both. Based on simulated and observed radar reflectivity, simulations roughly reproduce observed convective and stratiform precipitating areas. To identify the characteristics of convective and stratiform drafts that are difficult to observe but relevant to climate model parameterization, independent vertical wind speed thresholds are calculated to capture 90% of total convective and stratiform updraft and downdraft mass fluxes. Convective updrafts are fairly consistent across simulations (likely owing to fixed large-scale forcings and surface conditions), except that hydrometeor loadings differ substantially. Convective downdraft and stratiform updraft and downdraft mass fluxes vary notably below the melting level, but share similar vertically uniform draft velocities despite differing hydrometeor loadings. All identified convective and stratiform downdrafts contain precipitation below ~10 km and nearly all updrafts are cloudy above the melting level. Cold pool properties diverge substantially in a manner that is consistent with convective downdraft mass flux differences below the melting level. Despite differences in hydrometeor loadings and cold pool properties, convective updraft and downdraft mass fluxes are linearly correlated with convective area, the ratio of ice in downdrafts to that in updrafts is ~0.5 independent of species, and the ratio of downdraft to updraft mass flux is ~0.5-0.6, which may represent a minimum evaporation efficiency under moist conditions. Hydrometeor loading in stratiform regions is found to be a fraction of hydrometeor loading in convective regions that ranges from ~10% (graupel) to ~90% (cloud ice). These findings may lead to improved convection parameterizations.

  7. 846 IEEE TRANSACTIONS ON NEURAL NETWORKS ON LEARNING SYSTEMS, VOL. 23, NO. 5, MAY 2012 [9] D. Cheng and H. Qi, "Controllability and observability of Boolean

    E-Print Network [OSTI]

    Vermont, University of

    . 3, pp. 512­521, Mar. 2009. [31] D. Cheng, H. Qi, and Z. Li, Analysis and Control of Boolean Networks: A Semi-Tensor Product Approach. London, U.K.: Springer-Verlag, 2011. [32] D. Cheng, H. Qi, and Z. Li846 IEEE TRANSACTIONS ON NEURAL NETWORKS ON LEARNING SYSTEMS, VOL. 23, NO. 5, MAY 2012 [9] D. Cheng

  8. Observation and Control for Debugging Distributed Computations

    E-Print Network [OSTI]

    Garg, Vijay

    Observation and Control for Debugging Distributed Computations Vijay K. Garg \\Lambda Parallel and Distributed Systems Laboratory, Electrical and Computer Engineering Department The University of Texas for observing and controlling a distributed computation and its applications to distributed debugging

  9. Observation and Control for Debugging Distributed Computations

    E-Print Network [OSTI]

    Garg, Vijay

    Observation and Control for Debugging Distributed Computations Vijay K. Garg Parallel and Distributed Systems Laboratory, Electrical and Computer Engineering Department The University of Texas for observing and controlling a distributed computation and its applications to distributed debugging

  10. Elementos de Teoria da Informac~ao Mario A. T. Figueiredo

    E-Print Network [OSTI]

    Figueiredo, Mário A. T.

    . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 31 2.6 Codifica¸c~ao com Modelo Errado . . . . . . . . . . . . . . . . . . . . . . . . . . . 33 2´etica . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 47 3 #12;4 CONTE ´UDO 3 Fontes Discretas com Mem´oria 51 3.1 Processos Estoc´asticos Discretos em

  11. http://www.opticsinfobase.org/abstract.cfm?uri=ao-22-1-95

    National Nuclear Security Administration (NNSA)

    dust particle size measurements R. G. Pinnick, G. Fernandez, and B. D. Hinds Applied Optics, Vol. 22, Issue 1, pp. 95-102 (1983) doi:10.1364AO.22.000095 View Full Text:...

  12. A system to test the effects of materials on the electron drift lifetime in liquid argon and observations on the effect of water

    SciTech Connect (OSTI)

    Andrews, R.; Jaskierny, W.; Jostlein, H.; Kendziora, C.; Pordes, S.; Tope, T.; /Fermilab; ,

    2009-07-01T23:59:59.000Z

    A materials test system (MTS) has been developed at FNAL to assess the suitability of materials for use in a large liquid argon time projection chamber. During development of the MTS, it was noted that controlling the cryostat pressure with a 'raining' condenser reduced the electron drift lifetime in the liquid argon. The effect of condensing has been investigated using a series of passive materials to filter the condensate. We report the results of these studies and of tests on different candidate materials for detector construction. The inferred reduction of electron drift lifetime by water concentrations in the parts per trillion is of particular interest.

  13. Simulac~ao de Sistemas Embarcados utilizando ArchC Andreia Aparecida Barbiero

    E-Print Network [OSTI]

    Hexsel, Roberto A

    Federal do Paran´a Departamento de Inform´atica CEP 81.531-990 ­ Curitiba, PR, Brasil andreia@c3sl.531-990 ­ Curitiba, PR, Brasil roberto@inf.ufpr.br Resumo O ritmo do mercado de produc¸~ao de hardware e software equi- pamentos eletr^onicos. Estes produtos s~ao projetados sob restric¸~oes de recursos como energia

  14. Elementos de apoio `as aulas de Detecc~ao Remota ISA Primeiro Ciclo

    E-Print Network [OSTI]

    . O sinal detectado pelo sensor pode ser devido a energia ­ de origem solar ou proveniente de um´etica As observa¸c~oes por detec~ao remota implicam algum tipo de transmiss~ao de energia entre o alvo e o sensor emissor artificial ­ reflectida pela superf´icie ou energia emitida pela pr´opria superf´icie. Em geral

  15. Uma Interface Grafica para Algoritmos de Detecc~ao de Diferencas entre Documentos XML

    E-Print Network [OSTI]

    Hara, Carmem Satie

    ^ancia singular, pois atrav´es destas os usu´arios e administradores de base de dados semi-estruturados podem) tem sido cada vez mais difundida para troca de dados na Web. Com a XML tornando-se um padr~ao para publicac¸~ao e transporte de dados via Web faz-se necess´ario o desenvolvimento de algumas ferramentas que

  16. CCM0128 -Computac~ao II -2012 Exercicio Programa 1b -Intervalos Disjuntos

    E-Print Network [OSTI]

    Mascarenhas, Walter Figueiredo

    neste EP ´e fazer um programa que, dados os hor´arios de come¸co e fim das aulas em um certo dia da ordenar as aulas. No entanto, voc^e ainda n~ao tem certeza sobre qual par^ametro deve servir de base para dura¸c~ao Implemente o quicksort e utilize um algoritmo guloso que o utilize com base em um dos tr

  17. UNIVERSITY OF WISCONSIN-MADISON, Madison, WI. Assistant Professor, tenure track, beginning August 2013. AOS: Philosophy of Mind.

    E-Print Network [OSTI]

    Wisconsin at Madison, University of

    2013. AOS: Philosophy of Mind. AOC: Open. Four courses per year at the undergraduate and graduate level

  18. Cenario Virtual e Composic~ao de Imagens BRUNO COSTA1 LUCIA DARSA1 JONAS GOMES1

    E-Print Network [OSTI]

    Cen´ario Virtual e Composic¸~ao de Imagens BRUNO COSTA1 LUCIA DARSA1 JONAS GOMES1 PAULO ROMA2 LUIZ a combinac¸~ao de imagens. Glass-shots, mirror-shots e back-projection s~ao algumas das t´ecnicas tradicionais de combinac¸~ao de imagens. Neste trabalho, descrevemos um sistema baseado em t´ecnicas de rob

  19. Evolutionary outcomes for pairs of planets undergoing orbital migration and circularization: second order resonances and observed period ratios in Kepler's planetary systems

    E-Print Network [OSTI]

    Xiang-Gruess, M

    2015-01-01T23:59:59.000Z

    In order to study the origin of the architectures of low mass planetary systems, we perform numerical surveys of the evolution of pairs of coplanar planets in the mass range $(1-4)\\ \\rmn{M}_{\\oplus}.$ These evolve for up to $2\\times10^7 \\rmn{yr}$ under a range of orbital migration torques and circularization rates assumed to arise through interaction with a protoplanetary disc. Near the inner disc boundary, significant variations of viscosity, interaction with density waves or with the stellar magnetic field could occur and halt migration, but allow ircularization to continue. This was modelled by modifying the migration and circularization rates. Runs terminated without an extended period of circularization in the absence of migration torques gave rise to either a collision, or a system close to a resonance. These were mostly first order with a few $\\%$ terminating in second order resonances. Both planetary eccentricities were small $< 0.1$ and all resonant angles liberated. This type of survey produced o...

  20. Real-time Coastal Observation Network (ReCON)

    E-Print Network [OSTI]

    research. Deploy observations systems on portable, low cost buoys and fixed platforms of opportunity systems. The project will establish a test bed for observing system network design studies and develop

  1. Use of ARM observations and numerical models to determine radiative and latent heating profiles of mesoscale convective systems for general circulation models

    SciTech Connect (OSTI)

    Houze, Jr., Robert A. [University of Washington Dept. of Atmospheric Sciences

    2013-11-13T23:59:59.000Z

    We examined cloud radar data in monsoon climates, using cloud radars at Darwin in the Australian monsoon, on a ship in the Bay of Bengal in the South Asian monsoon, and at Niamey in the West African monsoon. We followed on with a more in-depth study of the continental MCSs over West Africa. We investigated whether the West African anvil clouds connected with squall line MCSs passing over the Niamey ARM site could be simulated in a numerical model by comparing the observed anvil clouds to anvil structures generated by the Weather Research and Forecasting (WRF) mesoscale model at high resolution using six different ice-phase microphysical schemes. We carried out further simulations with a cloud-resolving model forced by sounding network budgets over the Niamey region and over the northern Australian region. We have devoted some of the effort of this project to examining how well satellite data can determine the global breadth of the anvil cloud measurements obtained at the ARM ground sites. We next considered whether satellite data could be objectively analyzed to so that their large global measurement sets can be systematically related to the ARM measurements. Further differences were detailed between the land and ocean MCS anvil clouds by examining the interior structure of the anvils with the satellite-detected the CloudSat Cloud Profiling Radar (CPR). The satellite survey of anvil clouds in the Indo-Pacific region was continued to determine the role of MCSs in producing the cloud pattern associated with the MJO.

  2. Optical and radio variability of the BL Lac object AO 0235+16: a possible 5-6 year periodicity

    E-Print Network [OSTI]

    C. M. Raiteri; M. Villata; H. D. Aller; M. F. Aller; J. Heidt; O. M. Kurtanidze; L. Lanteri; M. Maesano; E. Massaro; F. Montagni; R. Nesci; K. Nilsson; M. G. Nikolashvili; P. Nurmi; L. Ostorero; T. Pursimo; R. Rekola; A. Sillanpaa; L. O. Takalo; H. Terasranta; G. Tosti; T. J. Balonek; M. Feldt; E. J. McGrath; A. Heines; C. Heisler; J. Hu; M. Kidger; J. R. Mattox; A. Pati; R. Robb; A. C. Sadun; P. Shastri; S. J. Wagner; J. Wei; X. Wu

    2001-08-09T23:59:59.000Z

    New optical and radio data on the BL Lacertae object AO 0235+16 have been collected in the last four years by a wide international collaboration, which confirm the intense activity of this source. The optical data also include the results of the Whole Earth Blazar Telescope (WEBT) first-light campaign organized in November 1997. The optical spectrum is observed to basically steepen when the source gets fainter. We have investigated the existence of typical variability time scales and of possible correlations between the optical and radio emissions by means of visual inspection, Discrete Correlation Function analysis, and Discrete Fourier Transform technique. The major radio outbursts are found to repeat quasi-regularly with a periodicity of about 5.7 years; this period is also in agreement with the occurrence of some of the major optical outbursts, but not all of them.

  3. Climate Dynamics Observational, Theoretical and

    E-Print Network [OSTI]

    Dong, Xiquan

    1 23 Climate Dynamics Observational, Theoretical and Computational Research on the Climate System.6, and -22.5 Wm-2 , respectively, indicating a net cooling effect of clouds on the TOA radiation budget-2 , respectively, resulting in a larger net cooling effect of 2.9 Wm-2 in the model simu- lations

  4. Belief space planning assuming maximum likelihood observations

    E-Print Network [OSTI]

    Lozano-Perez, Tomas

    observations are modelled as Gaussian noise. Given this model of the dynamics, two planning and control methods-locating the sensors with the contacts this way complicates planning and control because it forces the system to trade of the partially observable control problem, often modeled as a partially observable Markov decision process (POMDP

  5. JPL D-33509 Earth Observing System (EOS)

    E-Print Network [OSTI]

    . Cofield, David T. Cuddy, Lucien Froidevaux, Ryan A Fuller, Robert F. Jarnot, Jonathan H. Jiang, Yibo B

  6. JPL D-33509 Earth Observing System (EOS)

    E-Print Network [OSTI]

    . Cuddy, Lucien Froidevaux, Ryan A Fuller, Robert F. Jarnot, Jonathan H. Jiang, Yibo B. Jiang, Brian W

  7. JPL D-33509 Earth Observing System (EOS)

    E-Print Network [OSTI]

    1000 1200 FWHM / km Nathaniel J. Livesey, William G. Read, Lucien Froidevaux, Alyn Lambert, Gloria L

  8. JPL D-28534 Earth Observing System (EOS)

    E-Print Network [OSTI]

    .0 June 15, 2004 National Aeronautics and Space Administration Jet Propulsion Laboratory California . . . . . . . . . . . . . . . . . . . . . . 4 1.1.4 Zeeman Splitting . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 5 1.2 Magnetic . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 7 1.3 Tensor magnetic susceptibility . . . . . . . . . . . . . . . . . . . . . . . . . . . 9 2

  9. GEO Secretariat Global Earth Observing System of

    E-Print Network [OSTI]

    ­ 2009-11 Work Plan Objective: to improve the management and protection of terrestrial, coastal Survey #12;© GEO Secretariat Trees are so much more sensible than people, steadier and more enduring and Epidemiology 3. Energy Management 4. Climate Variability & Change 5. Water Management 6. Weather Forecasting 7

  10. Automated Surface Observing System: Standby Power Options

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels DataDepartment of Energy Your Density Isn't Your Destiny: The FutureComments from TarasaName4ServicesTribalWorkplaceAutomated SteelAutomated

  11. Regras de Avaliac~ao de CDI-II (Leic-A, 1o s 2010/2011)

    E-Print Network [OSTI]

    Baia, Margarida

    lista bi-semanal de exerc´icios propostos. Estes exerc´icios devem ser resolvidos pelos alunos antes das prepara¸c~ao pr´evia dos exerc´icios de cada ficha, e sobre o desempenho em deter- minados exerc´icios finalizar a resolu¸c~ao dos exerc´icios, recorrendo ao docente para esclarecer eventuais d´uvidas. Em cada

  12. Blind identification of MISO-FIR channels Carlos Est^ev~ao R. Fernandes

    E-Print Network [OSTI]

    Boyer, Edmond

    Blind identification of MISO-FIR channels Carlos Est^ev~ao R. Fernandes , Pierre Comon , G, vol.90 Abstract In this paper, we address the problem of determining the order of MISO channels to false alarm. Afterwards, we introduce the concept of MISO channel nested detectors based on a deflation

  13. Acustica submarina em alta frequ^encia: teoria, simulac~ao e resultados experimentais1

    E-Print Network [OSTI]

    Jesus, Sérgio M.

    ~oes, peso, consumo de energia e custo dos equipamentos normalmente utilizados para transmiss~ao e recep Acústica Submarina - Rio de Janeiro, Brasil, 21-23 de novembro de 2007 #12;77 num´ericos podem calcular

  14. Conselho de Ministros abre porta das salas de aulas aos bolseiros

    E-Print Network [OSTI]

    Instituto de Sistemas e Robotica

    permite que os bolseiros de investigação lecionem, ape- sar de diversas limitações impostas pelo Governo O Governo aprovou a alteração ao Estatuto do Bolseiro de Investiga- ção que permite que todos os bol- seiros mesmo a pedir "diversos pareceres jurídicos" sobre os ajus- tes promovidos pelo Governo. Um dos

  15. Cursos de dois anosGoverno vai apresentar a proposta, que agrada aos Institutos Politcnicos.

    E-Print Network [OSTI]

    Instituto de Sistemas e Robotica

    Cursos de dois anos·Governo vai apresentar a proposta, que agrada aos Institutos Politécnicos. ·0 apresentada pelo Governo dentro de semanas. Institutos Politécnicos aplaudem a possibilidade. CARLA MARINA Qualidade. Governo quer ver aumentar o número de diplomados em Portugal #12;

  16. RICHARD REMPEL DE SOUZA AVALIAC~AO DE CACHES ESPECIALIZADAS PARA

    E-Print Network [OSTI]

    Hexsel, Roberto A

    apresentem os melhores resultados. Para tanto, os dados obtidos, a partir do trabalho base, para essa comando do Benchmark . . . . . . . . . . . . . . . . . . . . . . . . 26 B Script para cria¸c~ao da base de dados 27 C Script AWK 40 1 #12;Lista de Tabelas 2.1 Modelos de CPU

  17. CCM0128 -Computac~ao II -2012 Exercicio Programa 1a -Subsequ^encia de Soma Maxima

    E-Print Network [OSTI]

    Mascarenhas, Walter Figueiredo

    CCM0128 - Computa¸c~ao II - 2012 Exerc´icio Programa 1a - Subsequ^encia de Soma M´axima E-mail do

  18. Esquema Hibrido para Amostragem de Mapas de Iluminac~ao em renderizac~oes foto-realistas

    E-Print Network [OSTI]

    ´eticos em cenas reais ´e pre- ciso dispor da iluminac¸~ao do ambiente real onde ser´a feita a inserc

  19. Gabarito da Prova Final de Calculo Diferencial e Integral III Eng. Produc~ao 06/12/2007

    E-Print Network [OSTI]

    Cipolatti, Rolci

    movimento ´e retil´ineo na dire¸c~ao do vetor (4, 4, ) e o vetor velocidade ´e d dt - (t) = 32t 152 (4, 4

  20. VLT/UVES observations of extremely strong intervening damped Lyman-alpha systems: Molecular hydrogen and excited carbon, oxygen and silicon at log N(HI)=22.4

    E-Print Network [OSTI]

    Noterdaeme, P; Rahmani, H; Petitjean, P; Pâris, I; Ledoux, C; Gupta, N; López, S

    2015-01-01T23:59:59.000Z

    We present a detailed analysis of three extremely strong intervening DLAs (log N(HI)>=21.7) observed towards quasars with VLT/UVES. We measure overall metallicities of [Zn/H]~-1.2, -1.3 and -0.7 at respectively zabs=2.34 towards SDSS J2140-0321 (log N(HI) = 22.4+/-0.1), zabs=3.35 towards SDSS J1456+1609 (log N(HI) = 21.7+/-0.1) and zabs=2.25 towards SDSS J0154+1935 (log N(HI) = 21.75+/-0.15). We detect H2 towards J2140-0321 (log N(H2) = 20.13+/-0.07) and J1456+1609 (log N(H2) = 17.10+/-0.09) and argue for a tentative detection towards J0154+1935. Absorption from the excited fine-structure levels of OI, CI and SiII are detected in the system towards J2140-0321, that has the largest HI column density detected so far in an intervening DLA. This is the first detection of OI fine-structure lines in a QSO-DLA, that also provides us a rare possibility to study the chemical abundances of less abundant atoms like Co and Ge. Simple single phase photo-ionisation models fail to reproduce all the observed quantities. Inst...

  1. Spectrum of Controlling and Observing Complex Networks

    E-Print Network [OSTI]

    Yan, Gang; Barzel, Baruch; Slotine, Jean-Jacques; Liu, Yang-Yu; Barabasi, Albert-Laszlo

    2015-01-01T23:59:59.000Z

    Observing and controlling complex networks are of paramount interest for understanding complex physical, biological and technological systems. Recent studies have made important advances in identifying sensor or driver nodes, through which we can observe or control a complex system. Yet, the observation uncertainty induced by measurement noise and the energy cost required for control continue to be significant challenges in practical applications. Here we show that the control energy cost and the observation uncertainty vary widely in different directions of the state space. In particular, we find that if all nodes are directly driven, control is energetically feasible, as the maximum energy cost increases sublinearly with the system size. If, however, we aim to control a system by driving only a single node, control in some directions is energetically prohibitive, increasing exponentially with the system size. For the cases in between, the maximum energy decays exponentially if we increase the number of driv...

  2. Atomic Collapse Observed

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

    Scientists Observe Atomic Collapse State Quantum Mechanics Prediction Confirmed in Graphene Using NERSC's Hopper April 26, 2013 | Tags: Hopper, Materials Science Contact: Linda...

  3. Hot Pot Field Observations

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

    Lane, Michael

    Map of field observations including depressions, springs, evidence of former springs, travertine terraces and vegetation patterns. Map also contains interpretation of possible spring alignments.

  4. Hot Pot Field Observations

    SciTech Connect (OSTI)

    Lane, Michael

    2013-06-28T23:59:59.000Z

    Map of field observations including depressions, springs, evidence of former springs, travertine terraces and vegetation patterns. Map also contains interpretation of possible spring alignments.

  5. Observing the next galactic supernova

    SciTech Connect (OSTI)

    Adams, Scott M.; Kochanek, C. S.; Beacom, John F.; Stanek, K. Z. [Department of Astronomy, The Ohio State University, 140 West 18th Avenue, Columbus, OH 43210 (United States); Vagins, Mark R. [Kavli Institute for the Physics and Mathematics of the Universe (WPI), Todai Institutes for Advanced Study, University of Tokyo, 5-1-5 Kashiwanoha, Kashiwa, Chiba 277-8583 (Japan)

    2013-12-01T23:59:59.000Z

    No supernova (SN) in the Milky Way has been observed since the invention of the optical telescope, instruments for other wavelengths, neutrino detectors, or gravitational wave observatories. It would be a tragedy to miss the opportunity to fully characterize the next one. To aid preparations for its observations, we model the distance, extinction, and magnitude probability distributions of a successful Galactic core-collapse supernova (ccSN), its shock breakout radiation, and its massive star progenitor. We find, at very high probability (? 100%), that the next Galactic SN will easily be detectable in the near-IR and that near-IR photometry of the progenitor star very likely (? 92%) already exists in the Two Micron All Sky Survey. Most ccSNe (98%) will be easily observed in the optical, but a significant fraction (43%) will lack observations of the progenitor due to a combination of survey sensitivity and confusion. If neutrino detection experiments can quickly disseminate a likely position (?3°), we show that a modestly priced IR camera system can probably detect the shock breakout radiation pulse even in daytime (64% for the cheapest design). Neutrino experiments should seriously consider adding such systems, both for their scientific return and as an added and internal layer of protection against false triggers. We find that shock breakouts from failed ccSNe of red supergiants may be more observable than those of successful SNe due to their lower radiation temperatures. We review the process by which neutrinos from a Galactic ccSN would be detected and announced. We provide new information on the EGADS system and its potential for providing instant neutrino alerts. We also discuss the distance, extinction, and magnitude probability distributions for the next Galactic Type Ia supernova (SN Ia). Based on our modeled observability, we find a Galactic ccSN rate of 3.2{sub ?2.6}{sup +7.3} per century and a Galactic SN Ia rate of 1.4{sub ?0.8}{sup +1.4} per century for a total Galactic SN rate of 4.6{sub ?2.7}{sup +7.4} per century is needed to account for the SNe observed over the last millennium, which implies a Galactic star formation rate of 3.6{sub ?3.0}{sup +8.3} M {sub ?} yr{sup –1}.

  6. Systems

    E-Print Network [OSTI]

    Chapter 1. Systems. 1.1. On Line. In this introductory section we will pose no exercises, but instead, will detail. how to use Maple to solve problems in linear ...

  7. 27/10/2010 12:48AGU: Highlatitude geomagnetically induced current events observed on very low frequency radio wave receiver systems Page 1 of 2http://europa.agu.org/?view=article&uri=/journals/rs/rs1002/2009RS004215/2009RS004215.xml&t=

    E-Print Network [OSTI]

    Ulich, Thomas

    27/10/2010 12:48AGU: Highlatitude geomagnetically induced current events observed on very low Abstract Highlatitude geomagnetically induced current events observed on very low frequency radio wave characteristics. Finally, we compared in detail the geomagnetic induced current (GIC) in the Scottish power system

  8. Exercicios-Desafio de AMIV Nota Importante: N~ao e recomendavel e e altamente desaconselhado o investimento de

    E-Print Network [OSTI]

    Natário, José

    investimento de tempo na tentativa de resolu¸c~ao destes exerc´icios por quem ainda n~ao tenha resolvido com su- cesso e relativa facilidade os exerc´icios-teste semanais e uma quantidade bastante substancial de exerc´icios

  9. Segmentac~ao da Parede da Aorta em Imagens de Resson^ancia Magnetica de Tempo Real

    E-Print Network [OSTI]

    Carvalho, João Luiz

    Segmenta¸c~ao da Parede da Aorta em Imagens de Resson^ancia Magn´etica de Tempo Real Gustavo Maia no plano. Metodologia O processamento de imagens e c´alculos computacionais foram feitos no software MATLAB´alculo do centro de massa da combina¸c~ao de imagens binarizadas definidas pelas caracter´isticas da imagem

  10. Near-Infrared Observations April 9, 2009

    E-Print Network [OSTI]

    Harrison, Thomas

    idea: correct wavefront distortions using a deformable secondary mirror · can achieve better correction;Energy Generation · what are we seeing when we observe solar system objects in the NIR? · reflected

  11. OBSERVATIONS OF TWO TRANSIENT LUMINOUS EVENT-

    E-Print Network [OSTI]

    Rutledge, Steven

    OBSERVATIONS OF TWO TRANSIENT LUMINOUS EVENT- PRODUCING MESOSCALE CONVECTIVE SYSTEMS Timothy LangC by positive cloud-to-ground (+CG) lightning can lead to transient luminous events (TLEs; Williams 1998; Lyons

  12. ChainReaction: uma Variante de Replicac~ao em Cadeia com Coer^encia Causal+

    E-Print Network [OSTI]

    Rodrigues, Luís E.T.

    , o ChainReaction serve de base a um futuro sistema para Geo-replica¸c~ao (v´arios centros de dados desafios no desenho de sistemas de armazenamento de dados para suporte a aplica¸c~oes na nuvem. Por este propostas nos ´ultimos anos. Este artigo prop~oe um novo sis- tema de armazenamento de dados, chamado Chain

  13. VII Seminrio tcnico-cientifico de anlise dos dados referentes ao

    E-Print Network [OSTI]

    protegidas da Amazônia pode agüentar a pressão do desflorestamento? #12;Métodos · Base de dados ­ Limite dasVII Seminário técnico-cientifico de análise dos dados referentes ao desmatamento na Amazônia Legal;Desflorestamento no entorno #12;10 km 30 km #12;10 km 30 km #12;Banco de dados ­ 1997 - 2008 ACUMULADO #12;BANCO DE

  14. Observational learning in horses

    E-Print Network [OSTI]

    Baer, Katherine Louise

    1979-01-01T23:59:59.000Z

    . One group served as control subjects while the other group functioned as a treated group (observers). The observers were allowed to watch a correctly performed discrimination task prior to testing of a learning response using the same task.... Discrimination testing was conducted on all horses daily for 14 days with criterion set at seven out of eight responses correct with the last five consecutively correct. The maximum number of trials performed without reaching set criterion was limited...

  15. If physics is an information science, what is an observer?

    E-Print Network [OSTI]

    Chris Fields

    2012-02-11T23:59:59.000Z

    Interpretations of quantum theory have traditionally assumed a "Galilean" observer, a bare "point of view" implemented physically by a quantum system. This paper investigates the consequences of replacing such an informationally-impoverished observer with an observer that satisfies the requirements of classical automata theory, i.e. an observer that encodes sufficient prior information to identify the system being observed and recognize its acceptable states. It shows that with reasonable assumptions about the physical dynamics of information channels, the observations recorded by such an observer will display the typical characteristics predicted by quantum theory, without requiring any specific assumptions about the observer's physical implementation.

  16. Observations of the Icy Universe

    E-Print Network [OSTI]

    Boogert, Adwin; Whittet, Douglas

    2015-01-01T23:59:59.000Z

    Freeze-out of the gas phase elements onto cold grains in dense interstellar and circumstellar media builds up ice mantles consisting of molecules that are mostly formed in situ (H2O, NH3, CO2, CO, CH3OH, and more). This review summarizes the detected infrared spectroscopic ice features and compares the abundances across Galactic, extragalactic, and solar system environments. A tremendous amount of information is contained in the ice band profiles. Laboratory experiments play a critical role in the analysis of the observations. Strong evidence is found for distinct ice formation stages, separated by CO freeze out at high densities. The ice bands have proven to be excellent probes of the thermal history of their environment. The evidence for the long-held idea that processing of ices by energetic photons and cosmic rays produces complex molecules is weak. Recent state of the art observations show promise for much progress in this area with planned infrared facilities.

  17. Observer-based fault detection for nuclear reactors

    E-Print Network [OSTI]

    Li, Qing, 1972-

    2001-01-01T23:59:59.000Z

    This is a study of fault detection for nuclear reactor systems. Basic concepts are derived from fundamental theories on system observers. Different types of fault- actuator fault, sensor fault, and system dynamics fault ...

  18. Would be the photon a composed particle? / Sobre a possibilidade da quantiza\\c{c}\\~ao dos fluxos de campo na radia\\c{c}\\~ao eletromagn\\'etica

    E-Print Network [OSTI]

    Duarte, Celso de Araujo

    2013-01-01T23:59:59.000Z

    Here it is made a comparative analysis between the classical and the quantum expressions for the energy of electromagnetic radiation (ER). The comparison points to the possibility of the quantization of the magnetic and the electric field fluxes in the ER. ----- Apresenta-se uma an\\'alise comparativa entre as express\\~oes cl\\'assica e qu\\^antica para a energia da radia\\c{c}\\~ao eletromagn\\'etica (RE). A compara\\c{c}\\~ao nos aponta para a possibilidade de haver uma quantiza\\c{c}\\~ao dos fluxos dos campos magn\\'etico e el\\'etrico na RE.

  19. Observing Massive Galaxy Formation

    E-Print Network [OSTI]

    Christopher J. Conselice

    2002-12-20T23:59:59.000Z

    A major goal of contemporary astrophysics is understanding the origin of the most massive galaxies in the universe, particularly nearby ellipticals and spirals. Theoretical models of galaxy formation have existed for many decades, although low and high redshift observations are only beginning to put constraints on different ideas. We briefly describe these observations and how they are revealing the methods by which galaxies form by contrasting and comparing fiducial rapid collapse and hierarchical formation model predictions. The available data show that cluster ellipticals must have rapidly formed at z > 2, and that up to 50% of all massive galaxies at z ~ 2.5 are involved in major mergers. While the former is consistent with the monolithic collapse picture, we argue that hierarchal formation is the only model that can reproduce all the available observations.

  20. Automated Surface Observing System (ASOS) General System Description

    E-Print Network [OSTI]

    ;ACU Option Comparison Battery Bank to power Hydrogen Fuel Engine Generator the existing UPS Cell Special battery venting to outside required; difficult to replenish Must be stored outside; easy cost Quarterly testing; Batteries replaced every 4 - 5 yrs (> $8.5K) Limited maintenance costs yearly

  1. Academic Writing Observation Papers

    E-Print Network [OSTI]

    a particular action and did not notice something about the people involved. Note what you did not notice observations. People: If the setting is crowded, choose a particular group (or groups) or focus on random paper around a research question: For example, you may be interested in power relations, interactions

  2. Academic Writing Observation Papers

    E-Print Network [OSTI]

    a particular action and did not notice something about the people involved. Note what you did not notice observations. People: If the setting is crowded, choose a particular group (or groups) or focus on random in power relations, interactions between interpersonal communication processes and other media, or other

  3. Global Warming Observations

    E-Print Network [OSTI]

    Schofield, Jeremy

    Global Warming Observations: 1. Global temperature has been gradually rising in recent years #15 in range 8000 12000 nm { CFC's, methane and N 2 O important for global warming even though concentra- tions in concentration of \\greenhouse gases" like CO 2 What determines global temperature? Energy budget of earth: 1

  4. XXVII SIMP OSIO BRASILEIRO DE TELECOMUNICAC ~OES -SBrT 2009, DE 29 DE SETEMBRO A 2 DE OUTUBRO DE 2009, BLUMENAU, SC Super-resoluc~ao de video usando quadros chave

    E-Print Network [OSTI]

    de Queiroz, Ricardo L.

    -resoluc¸~ao o conjunto de processos capaz de gerar imagens de alta resoluc¸~ao a partir de imagens de baixa contraposic¸~ao, imagens de alta resoluc¸~ao s~ao aquelas em que a densidade de pixels ´e elevada, assim como imagens de baixa resoluc¸~ao e deve process´a-las de modo a se obter uma imagem em maior resoluc¸~ao. Na

  5. Grupo fundamental e espacos de recobrimento, ver~ao 2011, Lista 2 Professor: H. Bursztyn

    E-Print Network [OSTI]

    Bursztyn, Henrique

    caminhos a, b, c, d : I X dados por: a(s) = F(s, 0), b(s) = F(1, s), c(s) = F(0, s), d(s) = F(1, s que o grupo fundamental de um grupo topol´ogico ´e abeliano. Dica: dados la¸cos a, b : I G com ponto base 1 G, use o problema 1 para F(s, t) = m(a(s), b(t))... Problema 3: Mostre que s~ao equivalentes

  6. Calculo Numerico -Exame -10/07/07 Considere a func~ao f(x) = xe-x

    E-Print Network [OSTI]

    Sussner, Peter

    C´alculo Num´erico - Exame - 10/07/07 1 Considere a fun¸c~ao f(x) = xe-x - e-3 . (a) Esbo¸ce o gr

  7. Observational Mishaps - a Database

    E-Print Network [OSTI]

    Kaspar von Braun; Kristin Chiboucas; Denise Hurley-Keller

    1999-06-11T23:59:59.000Z

    We present a World-Wide-Web-accessible database of astronomical images which suffer from a variety of observational problems, ranging from common occurences, such as dust grains on filters and/or the dewar window, to more exotic phenomena, such as loss of primary mirror support due to the deflation of the support airbags. Apart from its educational usefulness, the purpose of this database is to assist astronomers in diagnosing and treating errant images at the telescope, thus saving valuable telescope time. Every observational mishap contained in this on-line catalog is presented in the form of a GIF image, a brief explanation of the problem, and, when possible, a suggestion for improving the image quality.

  8. Identificac~ao da Doenca de Chagas Baseada em Analise de Sinais de Variabilidade da Frequ^encia Cardiaca

    E-Print Network [OSTI]

    Carvalho, João Luiz

    ´etrica Universidade de Bras´ilia, Bras´ilia­DF, Brasil GDPSGrupo de Processamento Digital de Sinais Introdu as energias de atividade simp´atica (de baixa frequ^encia, 0,05 a 0,15 Hz) e parassimp´atica (de alta frequ de varia¸c~ao versus coeficiente de regress~ao; RMSSD versus energia de baixa frequ^encia. Figura 5

  9. Rintoul, S.R., M.P. Meredith, O. Schofield, and L. Newman. 2012. The Southern Ocean Observing System. Oceanography 25(3):6869, http://dx.doi.org/10.5670/oceanog.2012.76.

    E-Print Network [OSTI]

    in the stability of the Antarctic ice sheets and their contributions to sea level rise 4. The future observations. recognition of this need motivated the community to develop a strategy for a Southern Ocean large impact on the remote and poorly observed Southern Ocean. Argo has already collected many more

  10. ARM Observations Projected

    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) VAP Update Information on new, existing, andObservations Projected

  11. Observations of Edge Turbulence

    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 RenewableSpeeding accessSpeeding access(SC)Gas and OilPhaseObservation ofEdge

  12. Observing the Inflationary Reheating

    E-Print Network [OSTI]

    Jerome Martin; Christophe Ringeval; Vincent Vennin

    2014-10-29T23:59:59.000Z

    Reheating is the the epoch which connects inflation to the subsequent hot Big-Bang phase. Conceptually very important, this era is however observationally poorly known. We show that the current Planck satellite measurements of the Cosmic Microwave Background (CMB) anisotropies constrain the kinematic properties of the reheating era for most of the inflationary models. This result is obtained by deriving the marginalized posterior distributions of the reheating parameter for about 200 models taken in Encyclopaedia Inflationaris. Weighted by the statistical evidence of each model to explain the data, we show that the Planck 2013 measurements induce an average reduction of the posterior-to-prior volume by 40%. Making some additional assumptions on reheating, such as specifying a mean equation of state parameter, or focusing the analysis on peculiar scenarios, can enhance or reduce this constraint. Our study also indicates that the Bayesian evidence of a model can substantially be affected by the reheating properties. The precision of the current CMB data is therefore such that estimating the observational performance of a model now requires to incorporate information about its reheating history.

  13. Observations on European Agriculture.

    E-Print Network [OSTI]

    Fraps, G. S. (George Stronach)

    1911-01-01T23:59:59.000Z

    of Manure ............................................. 9 ........................................ ~pplication of Manure 11 ............................ ............. dffects of Manure -- 12 ............................... rhird-Purchase of Imported....i& includes leguminous crops to gather nitrogen from the air, and thereby enrich the soil. The crops are never turned under but q fed and the manure saved. Second, it is due to a general use of a system of grain and live. stock farming in which all...

  14. Observing alternatives to inflation

    E-Print Network [OSTI]

    P. Peter

    2009-12-07T23:59:59.000Z

    We discuss the possibility that the inflationary paradigm, undoubtfully today's best framework to understand all the present cosmological data, may still have some viable challengers. The underlying idea for such discussions is that although inflation already passed quite a large number of tests, indeed enough to make it part of the so-called ``standard model'' of cosmology, it has always been through indirect measurements: there is not a chance that we may ever directly check its validity, and therefore, in order to assert its factuality with increasing level of confidence, it is required that we compare its predictions not only to observations, but also to as many contenders as possible. Among other categories of possible models, we wish to put the emphasis in particular on bouncing cosmologies that, however not as complete as the inflation paradigm might be, could still represent a reasonnable way of explaining the current data. Hopefully, future data will be able to discriminate between these various sets of theories.

  15. Correlation between human observer performance and model observer performance in differential phase contrast CT

    SciTech Connect (OSTI)

    Li, Ke; Garrett, John [Department of Medical Physics, University of Wisconsin-Madison, 1111 Highland Avenue, Madison, Wisconsin 53705 (United States)] [Department of Medical Physics, University of Wisconsin-Madison, 1111 Highland Avenue, Madison, Wisconsin 53705 (United States); Chen, Guang-Hong [Department of Medical Physics, University of Wisconsin-Madison, 1111 Highland Avenue, Madison, Wisconsin 53705 and Department of Radiology, University of Wisconsin-Madison, 600 Highland Avenue, Madison, Wisconsin 53792 (United States)] [Department of Medical Physics, University of Wisconsin-Madison, 1111 Highland Avenue, Madison, Wisconsin 53705 and Department of Radiology, University of Wisconsin-Madison, 600 Highland Avenue, Madison, Wisconsin 53792 (United States)

    2013-11-15T23:59:59.000Z

    Purpose: With the recently expanding interest and developments in x-ray differential phase contrast CT (DPC-CT), the evaluation of its task-specific detection performance and comparison with the corresponding absorption CT under a given radiation dose constraint become increasingly important. Mathematical model observers are often used to quantify the performance of imaging systems, but their correlations with actual human observers need to be confirmed for each new imaging method. This work is an investigation of the effects of stochastic DPC-CT noise on the correlation of detection performance between model and human observers with signal-known-exactly (SKE) detection tasks.Methods: The detectabilities of different objects (five disks with different diameters and two breast lesion masses) embedded in an experimental DPC-CT noise background were assessed using both model and human observers. The detectability of the disk and lesion signals was then measured using five types of model observers including the prewhitening ideal observer, the nonprewhitening (NPW) observer, the nonprewhitening observer with eye filter and internal noise (NPWEi), the prewhitening observer with eye filter and internal noise (PWEi), and the channelized Hotelling observer (CHO). The same objects were also evaluated by four human observers using the two-alternative forced choice method. The results from the model observer experiment were quantitatively compared to the human observer results to assess the correlation between the two techniques.Results: The contrast-to-detail (CD) curve generated by the human observers for the disk-detection experiments shows that the required contrast to detect a disk is inversely proportional to the square root of the disk size. Based on the CD curves, the ideal and NPW observers tend to systematically overestimate the performance of the human observers. The NPWEi and PWEi observers did not predict human performance well either, as the slopes of their CD curves tended to be steeper. The CHO generated the best quantitative agreement with human observers with its CD curve overlapping with that of human observer. Statistical equivalence between CHO and humans can be claimed within 11% of the human observer results, including both the disk and lesion detection experiments.Conclusions: The model observer method can be used to accurately represent human observer performance with the stochastic DPC-CT noise for SKE tasks with sizes ranging from 8 to 128 pixels. The incorporation of the anatomical noise remains to be studied.

  16. Satellite Observations towards the Agriculture applications

    E-Print Network [OSTI]

    Satellite Observations towards the Agriculture applications Osamu Ochiai Japan Aerospace Exploration Agency #12;7/30/2006 IGARSS_2006 Integrated Systems for Agriculture 2 Convergence of Evidence, All Gov't Policy Makers Reference Model: USDA Foreign Agricultural Service PECAD:Production Estimates

  17. Observations and simulations improve space weather models

    E-Print Network [OSTI]

    - 1 - Observations and simulations improve space weather models June 25, 2014 Los Alamos with fast-moving particles and a space weather system that varies in response to incoming energy computer simulations of the space weather that can affect vital technology, communication and navigation

  18. Effect of linear lumping on controllability and observability

    E-Print Network [OSTI]

    Tóth, János

    Effect of linear lumping on controllability and observability Zs´ofia Horv´ath October 2006 Email to reduce the number of state variables on controllability and observability of linear differential the effect of linear lumping on such properties of the system as controllability and observability and apply

  19. 62 Bureau of Meteorology Annual Report 201314 Observations and infrastructure

    E-Print Network [OSTI]

    Greenslade, Diana

    . · The development of a risk-based asset replacement plan for 2014­15 and beyond was commenced, and an Asset Life-cycle, the Observing System Strategy has been developed and will be supported by an accompanying roadmap monitoring and review of the Bureau's observing systems is undertaken to assess performance and fitness

  20. A SURVEY OF RECENT RESULTS IN NETWORKED CONTROL SYSTEMS Jo~ao P. Hespanha Payam Naghshtabrizi Yonggang Xu

    E-Print Network [OSTI]

    Liebling, Michael

    air vehicles (UAVs) due to stealth requirements, power-starved vehicles such as planetary rovers, long are addressed in [31], which obtains a general extension of Bode's integral inequality. This material is based

  1. Reconstruc~ao Paralelizada de Dados de Resson^ancia Magnetica de Fluxo em Processadores Multi-nucleo

    E-Print Network [OSTI]

    Carvalho, João Luiz

    multidimensionais: m(x, y, z, v, t) RF Gz Gx Gy a b c d Sequ^encia de pulso FVE espiral [1] Reconstru¸c~ao: NUFFT [3/corte (256 batimentos card´iacos a 105 bpm) 120 -120 0 0 500 velocidade(cm/s) tempo (ms) 120 -120 0 0 500 120

  2. Uma Experi^encia de Sincronizac~ao de Bases de Dados Relacionais Utilizando SyncML

    E-Print Network [OSTI]

    Hara, Carmem Satie

    Uma Experi^encia de Sincronizac¸~ao de Bases de Dados Relacionais Utilizando SyncML Alison L. B}@inf.ufpr.br Abstract. This paper describes SBDML, a SyncML-based middleware to repli- cate and synchonize data between sincronizar dados de um banco de dados relacional com outro banco de dados relacional ou com dispositivos m

  3. The Latin Music Database: Uma Base de Dados Para a Classificac~ao Automatica de G^eneros Musicais

    E-Print Network [OSTI]

    Kent, University of

    The Latin Music Database: Uma Base de Dados Para a Classificac¸~ao Autom´atica de G^eneros Musicais base de dados nova e in´edita, que foi originalmente criada para experimentos relacionados- senvolvido que garante que a base de dados seja facilmente expans´ivel e tenha todas as caracter

  4. AoM 2007 ID Number : 12323 NEW PRODUCT DEVELOPMENT IN A PLATFORM-DRIVEN ORGANIZATION : TOWARDS PLATFORM

    E-Print Network [OSTI]

    Paris-Sud XI, Université de

    AoM 2007 ID Number : 12323 NEW PRODUCT DEVELOPMENT IN A PLATFORM-DRIVEN ORGANIZATION : TOWARDS PLATFORM LIFECYCLE MANAGEMENT. SYLVAIN LENFLE, SIHEM JOUINI, CAROLINE DERROUSSEAUX CENTRE DE RECHERCHE EN GESTION, ECOLE POLYTECHNIQUE ABSTRACT Platform product development is now widely used to tackle the cost

  5. Reconstruc~ao de Objetos 3D usando Modelos Deform'aveis Rosana Marques da Silva \\Lambda Wu, ShinTing

    E-Print Network [OSTI]

    ¸c~ao A reconstru¸c~ao de modelos 3D a partir de imagens pode ser, convenientemente, separado em dois est'a­ gios. O¸c~ao, de pontos amostrados nas imagens, enquanto o segundo concentra­se na transforma¸c~ao dessas in­ forma a partir de informa¸c~oes extra'idas das imagens. O m'etodo proposto por n'os est'a baseado no modelo de

  6. Apparatus for observing a hostile environment

    DOE Patents [OSTI]

    Nance, Thomas A. (Aiken, SC); Boylston, Micah L. (Williston, SC); Robinson, Casandra W. (Trenton, SC); Sexton, William C. (Aiken, SC); Heckendorn, Frank M. (Aiken, SC)

    2000-01-01T23:59:59.000Z

    An apparatus is provided for observing a hostile environment, comprising a housing and a camera capable of insertion within the housing. The housing is a double wall assembly with an inner and outer wall with an hermetically sealed chamber therebetween. A housing for an optical system used to observe a hostile environment is provided, comprising a transparent, double wall assembly. The double wall assembly has an inner wall and an outer wall with an hermetically sealed chamber therebetween. The double wall assembly has an opening and a void area in communication with the opening. The void area of the housing is adapted to accommodate the optical system within said void area. An apparatus for protecting an optical system used to observe a hostile environment is provided comprising a housing; a tube positioned within the housing; and a base for supporting the housing and the tube. The housing comprises a double wall assembly having an inner wall and an outerwall with an hermetically sealed chamber therebetween. The tube is adapted to house the optical system therein.

  7. Observable Proxies For 26 Al Enhancement

    SciTech Connect (OSTI)

    Fryer, Christopher L [Los Alamos National Laboratory; Young, Patrick A [Los Alamos National Laboratory; Ellinger, Carola I [ASU; Arnett, William D [UNIV ARIZONA

    2008-01-01T23:59:59.000Z

    We consider the cospatial production of elements in supernova explosions to find observationally detectable proxies for enhancement of {sup 26}Al in supernova ejecta and stellar systems. Using four progenitors we explore a range of 1D explosions at different energies and an asymmetric 3D explosion. We find that the most reliable indicator of the presence of {sup 26}Al in unmixed ejecta is a very low S/Si ratio ({approx} 0.05). Production of N in O/S/Si-rich regions is also indicative. The biologically important element P is produced at its highest abundance in the same regions. Proxies should be detectable in supernova ejecta with high spatial resolution multi wavelength observations, but the small absolute abundance of material injected into a proto-planetary disk makes detection unlikely in existing or forming stellar/planetary systems.

  8. Observation

    Office of Scientific and Technical Information (OSTI)

    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 742EnergyOnItem Not Found Item Not Found TheHotSpeedingSpeedingSpeedingSpeedingSpeedingSpeedingOTYa

  9. Observation

    Office of Scientific and Technical Information (OSTI)

    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 742EnergyOnItem Not Found Item Not Found

  10. Observation

    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 RenewableSpeeding accessSpeeding access(SC)Gas and Oil ResearchPublictearing mode

  11. Observation

    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 RenewableSpeeding accessSpeeding access(SC)Gas and Oil ResearchPublictearing

  12. NS&T MANAGEMENT OBSERVATIONS

    SciTech Connect (OSTI)

    Gianotto, David

    2014-06-01T23:59:59.000Z

    The INL Management Observation Program (MOP) is designed to improve managers and supervisors understanding of work being performed by employees and the barriers impacting their success. The MOP also increases workers understanding of managements’ expectations as they relate to safety, security, quality, and work performance. Management observations (observations) are designed to improve the relationship and trust between employees and managers through increased engagement and interactions between managers and researchers in the field. As part of continuous improvement, NS&T management took initiative to focus on the participation and quality of observations in FY 14. This quarterly report is intended to (a) summarize the participation and quality of management’s observations, (b) assess observations for commonalities or trends related to facility or process barriers impacting research, and (c) provide feedback and make recommendations for improvements NS&T’s MOP.

  13. XXVII SIMP OSIO BRASILEIRO DE TELECOMUNICAC ~OES -SBrT 2009, DE 29 DE SETEMBRO A 2 DE OUTUBRO DE 2009, BLUMENAU, SC Arquitetura de resoluc~ao mista para codificac~ao

    E-Print Network [OSTI]

    de Queiroz, Ricardo L.

    aplicac¸~oes de baixo consumo de energia, como em sistemas de seguranc¸a com m´ultiplas c^ameras para uma´ilia, Bras´ilia, Brasil. E-mails: {diogo,queiroz}@image.unb.br. Camilo C. D´orea e Bruno Macchiavello, Departamento de Ci^encia da Computac¸~ao, Universidade de Bras´ilia, Bras´ilia, Brasil. E-mails: {camilo

  14. TEXTOS DE APOIO AO PROFESSOR DE FSICA IF UFRGS MARQUES, N. L. R. & ARAUJO, I. S. v.20 n 5 TEXTOS DE APOIO AO PROFESSOR DE FSICA IF UFRGS MARQUES, N. L. R. & ARAUJO, I. S. v.20 n 5

    E-Print Network [OSTI]

    dos Santos, C.A.

    no estudo mais amplo dos fenômenos térmicos, incluindo o conceito de energia, energia interna, calor, aquecedor solar e garrafa térmica, entre outros. Apesar do texto ter sido construído visando aos alunos do ­ MARQUES, N. L. R. & ARAUJO, I. S. ­ v.20 nº 5 5 SUMÁRIO I ­ ENERGIA

  15. Calculo Numerico -Segunda Prova -29/11/05 Considere a populac~ao dos E.U.A. em milhares de pessoas dada pela tabela seguinte

    E-Print Network [OSTI]

    Sussner, Peter

    C´alculo Num´erico - Segunda Prova - 29/11/05 1 Considere a popula¸c~ao dos E.U.A. em milhares de erro global, erro local, e ordem de um m´etodo num´erico para a resolu¸c~ao de PVI's. [0, 75 pts] 4

  16. 1 Introduc~ao A Mec^anica Estatistica usa como premissas basicas o conhecimento de alguns detalhes mi-

    E-Print Network [OSTI]

    Kik, Pieter

    a descri¸c~ao de propriedades e fen^omenos em escala termodin^amica, como equa¸c~oes de estado´iculas que formam um sistema pode mudar radi- calmente as propriedades termodin^amicas. Al´em de abrir: Termodin^amica Neste cap´itulo n´os nos preocuparemos em usar apenas conceitos e leis da Termodin^amica. O

  17. 8, 88178846, 2008 Observed boundary-

    E-Print Network [OSTI]

    Paris-Sud XI, Université de

    ACPD 8, 8817­8846, 2008 Observed boundary- layer/mesoscale impacts on Saharan dust J. H. Marsham et and Enviroment, University of Leeds, Leeds, UK 2 Institut f¨ur Meteorologie und Klimaforschung, Universit@env.leeds.ac.uk) 8817 #12;ACPD 8, 8817­8846, 2008 Observed boundary- layer/mesoscale impacts on Saharan dust J. H

  18. rK6)ao>x -^ i D) Ris-M-2906(ENf

    E-Print Network [OSTI]

    , but sold at the normal price. Replacements, if they can be issued, will be available for purchase of fuel savings and power supply capabilities for a number of system configu

  19. Observable signatures of general relativistic dynamics in compact binaries

    E-Print Network [OSTI]

    Lang, Ryan N. (Ryan Nathan)

    2009-01-01T23:59:59.000Z

    The effects of general relativity (GR) in astrophysical systems are often difficult to calculate, but they can have important consequences for observables. This thesis considers the impact of previously-ignored GR effects ...

  20. Power line harmonic radiation (PLHR) observed by the DEMETER spacecraft

    E-Print Network [OSTI]

    Santolik, Ondrej

    Power line harmonic radiation (PLHR) observed by the DEMETER spacecraft F. Nemec,1,2 O. Santoli´k,3 January 2006; published 22 April 2006. [1] Results of a systematic survey of Power Line Harmonic Radiation from the electric power systems which are magnetically conjugated with the place of observation

  1. What is the reference frame of an accelerated observer?

    E-Print Network [OSTI]

    K. -P. Marzlin

    1998-03-12T23:59:59.000Z

    The general construction of extended refrence frames for noninertial observers in flat space is studied. It is shown that, if the observer moves inertially before and after an arbitrary acceleration and rotation, the region where reference frames can coincide with an inertial system is bounded for final velocities exceeding 0.6 c.

  2. Nembhard (2002) 1 Individual Observation Process Monitoring Charts

    E-Print Network [OSTI]

    Nembhard, Harriet Black

    observations. The Shewhart chart has been well-discussed in the literature and introductory texts on SPC (seeNembhard (2002) 1 Individual Observation Process Monitoring Charts for Systems with Response Lags Engineering April 2002 Abstract Previously, it has been held that statistical process control (SPC

  3. Kalman Filtering with Intermittent Observations

    E-Print Network [OSTI]

    Jordan, Michael I.

    1 Kalman Filtering with Intermittent Observations Bruno Sinopoli, Luca Schenato, Massimo within sensor networks, we consider the prob- lem of performing Kalman filtering with intermittent be neglected. We address this problem starting from the discrete Kalman filtering formulation, and modelling

  4. Radio Observations of Supernova Remnants

    E-Print Network [OSTI]

    W. Reich

    2002-08-28T23:59:59.000Z

    Supernovae release an enormous amount of energy into the interstellar medium. Their remnants can observationally be traced up to several ten-thousand years. So far more than 230 Galactic supernova remnants (SNRs) have been identified in the radio range. Detailed studies of the different types of SNRs give insight into the interaction of the blast wave with the interstellar medium. Shock accelerated particles are observed, but also neutron stars left from the supernova explosion make their contribution. X-ray observations in conjunction with radio data constrain models of supernova evolution. A brief review of the origin and evolution of SNRs is given, which are compared with supernova statistics and observational limitations. In addition the morphology and characteristics of the different types of SNRs are described, including some recent results and illustrated by SNRs images mostly obtained with the Effelsberg 100-m telescope.

  5. Baryon Resonances Observed at BES

    E-Print Network [OSTI]

    B. S. Zou

    2008-02-01T23:59:59.000Z

    The $\\psi$ decays provide a novel way to explore baryon spectroscopy and baryon structure. The baryon resonances observed from $\\psi$ decays at BES are reviewed. The implications and prospects at upgraded BESIII/BEPCII are discussed.

  6. Jet observables without jet algorithms

    E-Print Network [OSTI]

    Bertolini, Daniele

    We introduce a new class of event shapes to characterize the jet-like structure of an event. Like traditional event shapes, our observables are infrared/collinear safe and involve a sum over all hadrons in an event, but ...

  7. Resilient Detection in the Presence of Integrity Attacks , Jo~ao Hespanha

    E-Print Network [OSTI]

    Hespanha, João Pedro

    critical plants and processes, including manufacturing, water and gas treatment and This researchReview Only 2 distribution, facility control and power grids. A successful attack to such kind of systems may infrastructures susceptible to cyber security threats. The research community has acknowledged the importance

  8. Single-Camera Visual Servoing 1 Jo~ao P. Hespanha

    E-Print Network [OSTI]

    Hespanha, João Pedro

    -loop system. However, it is possible to design a controller that drives the robot to the goal, provided to the #12;rst and passing through the goal point. The Cartesian coordinates of the robot are de- noted by (x deals with the problem of driving the po- sition of a point-robot to a goal point, using measure- ments

  9. Kalman filter data assimilation: Targeting observations and parameter estimation

    SciTech Connect (OSTI)

    Bellsky, Thomas, E-mail: bellskyt@asu.edu; Kostelich, Eric J.; Mahalov, Alex [School of Mathematical and Statistical Sciences, Arizona State University, Tempe, Arizona 85287 (United States)] [School of Mathematical and Statistical Sciences, Arizona State University, Tempe, Arizona 85287 (United States)

    2014-06-15T23:59:59.000Z

    This paper studies the effect of targeted observations on state and parameter estimates determined with Kalman filter data assimilation (DA) techniques. We first provide an analytical result demonstrating that targeting observations within the Kalman filter for a linear model can significantly reduce state estimation error as opposed to fixed or randomly located observations. We next conduct observing system simulation experiments for a chaotic model of meteorological interest, where we demonstrate that the local ensemble transform Kalman filter (LETKF) with targeted observations based on largest ensemble variance is skillful in providing more accurate state estimates than the LETKF with randomly located observations. Additionally, we find that a hybrid ensemble Kalman filter parameter estimation method accurately updates model parameters within the targeted observation context to further improve state estimation.

  10. Tailoring Strong Lensing Cosmographic Observations

    E-Print Network [OSTI]

    Linder, Eric V

    2015-01-01T23:59:59.000Z

    Strong lensing time delay cosmography has excellent complementarity with other dark energy probes, and will soon have abundant systems detected. We investigate two issues in the imaging and spectroscopic followup required to obtain the time delay distance. The first is optimization of spectroscopic resources. We develop a code to optimize the cosmological leverage under the constraint of constant spectroscopic time, and find that sculpting the lens system redshift distribution can deliver a 40% improvement in dark energy figure of merit. The second is the role of systematics, correlated between different quantities of a given system or model errors common to all systems. We show how the levels of different systematics affect the cosmological parameter estimation, and derive guidance for the fraction of double image vs quad image systems to follow as a function of differing systematics between them.

  11. Mid-Infrared Imaging of the Post-AGB Star AC Herculis with the MMT Adaptive Optics System

    E-Print Network [OSTI]

    Laird M. Close; Beth Biller; William F. Hoffmann; Phil M. Hinz; John H. Bieging; Francois Wildi; Michael Lloyd-Hart; Guido Brusa; Don Fisher; Doug Miller; Roger Angel

    2003-10-20T23:59:59.000Z

    We utilized the MMT's unique deformable secondary adaptive optics system to produce high-resolution (FWHM=0.3"), very high Strehl mid-infrared (9.8, 11.7 & 18 micron) images of the post-AGB star AC Her. The very high (98+/-2%) Strehls achieved with Mid-IR AO led naturally to an ultra-stable PSF independent of airmass, seeing, or location on the sky. We find no significant difference between AC Her's morphology and our unresolved PSF calibration stars (mu UMa & alpha Her) at 9.8, 11.7, & 18 microns. Our current observations do not confirm any extended Mid-IR structure around AC Her. These observations are in conflict with previously reported Keck (seeing-limited) 11.7 and 18 micron images which suggested the presence of a resolved ~0.6" edge-on circumbinary disk. We conclude that AC Her has no extended Mid-IR structure on scales greater than 0.2" (R<75 AU). These first results of Mid-IR AO science are very encouraging for future high accuracy Mid-IR imaging with this technique.

  12. European Photovoltaic Solar Energy Conference, Valencia, Spain, 6-10 September 2010, 2AO.1.6 INDUSTRIALLY RELEVANT Al2O3 DEPOSITION TECHNIQUES

    E-Print Network [OSTI]

    25th European Photovoltaic Solar Energy Conference, Valencia, Spain, 6-10 September 2010, 2AO.1 Al2O3 passivation layers degrade to SRVs larger than 100 cm/s af- ter firing. Hence, the firing

  13. X-ray Observations of Mrk 231

    E-Print Network [OSTI]

    T. J. Turner

    1998-08-10T23:59:59.000Z

    This paper presents new X-ray observations of Mrk 231, an active galaxy of particular interest due to its large infrared luminosity and the presence of several blueshifted broad absorption line (BAL) systems, a phenomenon observed in a small fraction of QSOs. A ROSAT HRI image of Mrk 231 is presented, this shows an extended region of soft X-ray emission, covering several tens of kpc, consistent with the extent of the host galaxy. An ASCA observation of Mrk 231 is also presented. Hard X-rays are detected but the data show no significant variability in X-ray flux. The hard X-ray continuum is heavily attenuated and X-ray column estimates range from ~ 2 x 10^{22} - 10^{23} cm^{-2} depending on whether the material is assumed to be neutral or ionized, and on the model assumed for the extended X-ray component. These ASCA data provide only the second hard X-ray spectrum of a BAL AGN presented to date. The broad-band spectral-energy-distribution of the source is discussed. While Mrk 231 is X-ray weak compared to Seyfert 1 galaxies, it has an optical-to-X-ray spectrum typical of a QSO.

  14. OBSERVED HYBRID OSCILLATIONS IN AN ELECTRICAL DISTRIBUTION SYSTEM Vaibhav Donde

    E-Print Network [OSTI]

    Hiskens, Ian A.

    reported in [2]. The paper therefore provides, in Section 2, a brief dis- cussion of modelling extensions due to the discreteness of transformer taps and capac- itors respectively. Accurate modelling must>0) Tap decrement logic (y2>0) (y2

  15. Campaign-level science traceability for Earth observation system architecting

    E-Print Network [OSTI]

    Seher, Theodore K. (Theodore Kimball)

    2009-01-01T23:59:59.000Z

    The Earth Sciences Decadal Survey of 2007 presented a comprehensive vision for the evolution of space-based Earth Science resources. The practical development of the Decadal campaign, however, has highlighted four challenges ...

  16. Observing ocean changes at the nation's first SWAC system

    E-Print Network [OSTI]

    (conductivity, temperature, pressure) · + oxygen, fluorescence and turbidity · ADCP: 300kHz · Nitrate sensor-2 years operational Items of note and path forward Photo: Christopher Pala, www.onewater.org Mahalo

  17. Regularized Nonlinear Moving Horizon Observer for Detectable Systems

    E-Print Network [OSTI]

    Johansen, Tor Arne

    ], Alessandri et al. [2008] for different formulation relying on somewhat different assumptions. Such a moving

  18. Observations of englacial water passages: a fracture-dominated system

    E-Print Network [OSTI]

    Jacobel, Robert W.

    hydraulics of glaciers have focused on the subglacial regime. In temperate alpine glaciers and ice caps controls the spatial distribution of water at the bed, which may affect local ice movement. These passages and the outward melting of the ice walls due to the frictional heat produced by the flowing water. The processes

  19. Common Cyber Security Vulnerabilities Observed in Control System

    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 33 111 1,613PortsmouthBartlesville EnergyDepartment. CashDay-JuneOffice of

  20. Common Cyber Security Vulnerabilities Observed in Control System

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels DataDepartment of Energy Your Density Isn't Your Destiny: Theof"Wave the WhiteNational| Department ofCommittee Report for

  1. Automated Surface Observing System: Standby Power Options | Department of

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page onYouTube YouTube Note: Since the YouTube platform is alwaysISOSource1-01 Audit LetterYear 2015Energy Automated

  2. CX Lyrae 2008 Observing Campaign

    E-Print Network [OSTI]

    de Ponthiere, Pierre; Hambsch, Franz-Josef

    2012-01-01T23:59:59.000Z

    The Blazhko effect in CX Lyr has been reported for the first time by Le Borgne et al. (2007). The authors have pointed out that the Blazhko period was not evaluated accurately due to dataset scarcity. The possible period values announced were 128 or 227 days. A newly conducted four-month observing campaign in 2008 (fifty-nine observation nights) has provided fourteen times of maximum. From a period analysis of measured times of maximum, a Blazhko period of 62 +/- 2 days can be suggested. However, the present dataset is still not densely sampled enough to exclude that the measured period is still a modulation of the real Blazhko period. Indeed the shape of the (O-C) curve does not repeat itself exactly during the campaign duration.

  3. Observation of an Antimatter Hypernucleus

    SciTech Connect (OSTI)

    STAR Collaboration; Abelev, Betty

    2010-07-05T23:59:59.000Z

    Nuclear collisions recreate conditions in the universe microseconds after the Big Bang. Only a very small fraction of the emitted fragments are light nuclei, but these states are of fundamental interest. We report the observation of antihypertritons - composed of an antiproton, antineutron, and antilambda hyperon - produced by colliding gold nuclei at high energy. Our analysis yields 70 {+-} 17 antihypertritons ({sub {bar {Lambda}}}{sup 3}{bar H}) and 157 {+-} 30 hypertritons ({sub {Lambda}}{sup 3}H). The measured yields of {sub {Lambda}}{sup 3}H ({sub {bar {Lambda}}}{sup 3}{bar H}) and {sup 3}He ({sup 3}{ovr He}) are similar, suggesting an equilibrium in coordinate and momentum space populations of up, down, and strange quarks and antiquarks, unlike the pattern observed at lower collision energies. The production and properties of antinuclei, and nuclei containing strange quarks, have implications spanning nuclear/particle physics, astrophysics, and cosmology.

  4. Odds of observing the multiverse

    SciTech Connect (OSTI)

    Dahlen, A. [Joseph Henry Laboratories, Department of Physics, Princeton University, Princeton, New Jersey 08544 (United States)

    2010-03-15T23:59:59.000Z

    Eternal inflation predicts that our observable universe lies within a bubble (or pocket universe) embedded in a volume of inflating space. The interior of the bubble undergoes inflation and standard cosmology, while the bubble walls expand outward and collide with other neighboring bubbles. The collisions provide either an opportunity to make a direct observation of the multiverse or, if they produce unacceptable anisotropy, a threat to inflationary theory. The probability of an observer in our bubble detecting the effects of collisions has an absolute upper bound set by the odds of being in the part of our bubble that lies in the forward light cone of a collision; in the case of collisions with bubbles of identical vacua, this bound is given by the bubble nucleation rate times (H{sub O}/H{sub I}){sup 2}, where H{sub O} is the Hubble scale outside the bubbles and H{sub I} is the scale of the second round of inflation that occurs inside our bubble. Similar results were obtained by Freigovel et al. using a different method for the case of collisions with bubbles of much larger cosmological constant; here, it is shown to hold in the case of collisions with identical bubbles as well.

  5. Odds of observing the multiverse

    E-Print Network [OSTI]

    Alex Dahlen

    2010-01-11T23:59:59.000Z

    Eternal inflation predicts our observable universe lies within a bubble (or pocket universe) embedded in a volume of inflating space. The interior of the bubble undergoes inflation and standard cosmology, while the bubble walls expand outward and collide with other neighboring bubbles. The collisions provide either an opportunity to make a direct observation of the multiverse or, if they produce unacceptable anisotropy, a threat to inflationary theory. The probability of an observer in our bubble detecting the effects of collisions has an absolute upper bound set by the odds of being in the part of our bubble that lies in the forward light-cone of a collision; in the case of collisions with bubbles of identical vacua, this bound given by the bubble nucleation rate times ($H_{\\rm{O}}/H_{\\rm{I}})^2$, where $H_{\\rm{O}}$ is the Hubble scale outside the bubbles and $H_{\\rm{I}}$ is the scale of the second round of inflation that occurs inside our bubble. Similar results were obtained by Freigovel \\emph{et al.} using a different method for the case of collisions with bubbles of much larger cosmological constant; here it is shown to hold in the case of collisions with identical bubbles as well. A significant error in a previous draft was corrected in order to arrive at this result.

  6. Spitzer observations of hydrogen deuteride

    E-Print Network [OSTI]

    David A. Neufeld; Joel D. Green; David J. Hollenbach; Paule Sonnentrucker; Gary J. Melnick; Edwin A. Bergin; Ronald L. Snell; William J. Forrest; Dan M. Watson; Michael J. Kaufman

    2006-06-26T23:59:59.000Z

    We report the detection of interstellar hydrogen deuteride (HD) toward the supernova remnant IC443, and the tentative detection of HD toward the Herbig Haro objects HH54 and HH7 and the star forming region GGD37 (Cepheus A West). Our detections are based upon spectral line mapping observations of the R(3) and R(4) rotational lines of HD, at rest wavelengths of 28.502 and 23.034 micron respectively, obtained using the Infrared Spectrograph onboard the Spitzer Space Telescope. The HD R(4)/R(3) line intensity ratio promises to be a valuable probe of the gas pressure in regions where it can be observed. The derived HD/H2 abundance ratios are 1.19(+0.35/-0.24)E-5, 1.80(+0.54/-0.32)E-5, and 1.41(+0.46/-0.33)E-5 respectively (68.3% confidence limits, based upon statistical errors alone) for IC443 (clump C), HH54, and HH7. If HD is the only significant reservoir of gas-phase deuterium in these sources, the inferred HD/H2 ratios are all consistent with a gas-phase elemental abundance [n(D)/n(H)](gas) ~ 7.5E-6, a factor 2 - 3 below the values obtained previously from observations of atomic deuterium in the local bubble and the Galactic halo. However, similarly low gas-phase deuterium abundances have been inferred previously for molecular gas clouds in the Orion region, and in atomic clouds along sight-lines within the Galactic disk to stars more distant than 500 pc from the Sun.

  7. Magnetars: the physics behind observations

    E-Print Network [OSTI]

    Turolla, Roberto; Watts, Anna

    2015-01-01T23:59:59.000Z

    Magnetars are the strongest magnets in the present universe and the combination of extreme magnetic field, gravity and density makes them unique laboratories to probe current physical theories (from quantum electrodynamics to general relativity) in the strong field limit. Magnetars are observed as peculiar, burst--active X-ray pulsars, the Anomalous X-ray Pulsars (AXPs) and the Soft Gamma Repeaters (SGRs); the latter emitted also three "giant flares," extremely powerful events during which luminosities can reach up to 10^47 erg/s for about one second. The last five years have witnessed an explosion in magnetar research which has led, among other things, to the discovery of transient, or "outbursting," and "low-field" magnetars. Substantial progress has been made also on the theoretical side. Quite detailed models for explaining the magnetars' persistent X-ray emission, the properties of the bursts, the flux evolution in transient sources have been developed and confronted with observations. New insight on neu...

  8. Conformal Relativity: Theory and Observations

    E-Print Network [OSTI]

    V. Pervushin; V. Zinchuk; A. Zorin

    2004-11-22T23:59:59.000Z

    Theoretical and observational arguments are listed in favor of a new principle of relativity of units of measurements as the basis of a conformal-invariant unification of General Relativity and Standard Model by replacement of all masses with a scalar (dilaton) field. The relative units mean conformal observables: the coordinate distance, conformal time, running masses, and constant temperature. They reveal to us a motion of a universe along its hypersurface in the field space of events like a motion of a relativistic particle in the Minkowski space, where the postulate of the vacuum as a state with minimal energy leads to arrow of the geometric time. In relative units, the unified theory describes the Cold Universe Scenario, where the role of the conformal dark energy is played by a free minimal coupling scalar field in agreement with the most recent distance-redshift data from type Ia supernovae. In this Scenario, the evolution of the Universe begins with the effect of intensive creation of primordial W-Z-bosons explaining the value of CMBR temperature, baryon asymmetry, tremendous deficit of the luminosity masses in the COMA-type superclusters and large-scale structure of the Universe.

  9. Spitzer observations of hydrogen deuteride

    E-Print Network [OSTI]

    Neufeld, D A; Hollenbach, D J; Sonnentrucker, P; Melnick, G J; Bergin, E A; Snell, R L; Forrest, W J; Watson, D M; Kaufman, M J; Neufeld, David A.; Green, Joel D.; Hollenbach, David J.; Sonnentrucker, Paule; Melnick, Gary J.; Bergin, Edwin A.; Snell, Ronald L.; Forrest, William J.; Watson, Dan M.; Kaufman, and Michael J.

    2006-01-01T23:59:59.000Z

    We report the detection of interstellar hydrogen deuteride (HD) toward the supernova remnant IC443, and the tentative detection of HD toward the Herbig Haro objects HH54 and HH7 and the star forming region GGD37 (Cepheus A West). Our detections are based upon spectral line mapping observations of the R(3) and R(4) rotational lines of HD, at rest wavelengths of 28.502 and 23.034 micron respectively, obtained using the Infrared Spectrograph onboard the Spitzer Space Telescope. The HD R(4)/R(3) line intensity ratio promises to be a valuable probe of the gas pressure in regions where it can be observed. The derived HD/H2 abundance ratios are 1.19(+0.35/-0.24)E-5, 1.80(+0.54/-0.32)E-5, and 1.41(+0.46/-0.33)E-5 respectively (68.3% confidence limits, based upon statistical errors alone) for IC443 (clump C), HH54, and HH7. If HD is the only significant reservoir of gas-phase deuterium in these sources, the inferred HD/H2 ratios are all consistent with a gas-phase elemental abundance [n(D)/n(H)](gas) ~ 7.5E-6, a facto...

  10. Fluid observers and tilting cosmology

    E-Print Network [OSTI]

    A. A. Coley; S. Hervik; W. C. Lim

    2006-05-24T23:59:59.000Z

    We study perfect fluid cosmological models with a constant equation of state parameter $\\gamma$ in which there are two naturally defined time-like congruences, a geometrically defined geodesic congruence and a non-geodesic fluid congruence. We establish an appropriate set of boost formulae relating the physical variables, and consequently the observed quantities, in the two frames. We study expanding spatially homogeneous tilted perfect fluid models, with an emphasis on future evolution with extreme tilt. We show that for ultra-radiative equations of state (i.e., $\\gamma>4/3$), generically the tilt becomes extreme at late times and the fluid observers will reach infinite expansion within a finite proper time and experience a singularity similar to that of the big rip. In addition, we show that for sub-radiative equations of state (i.e., $\\gamma < 4/3$), the tilt can become extreme at late times and give rise to an effective quintessential equation of state. To establish the connection with phantom cosmology and quintessence, we calculate the effective equation of state in the models under consideration and we determine the future asymptotic behaviour of the tilting models in the fluid frame variables using the boost formulae. We also discuss spatially inhomogeneous models and tilting spatially homogeneous models with a cosmological constant.

  11. Autonomous observing strategies for the ocean carbon cycle

    SciTech Connect (OSTI)

    Bishop, James K.; Davis, Russ E.

    2000-07-26T23:59:59.000Z

    Understanding the exchanges of carbon between the atmosphere and ocean and the fate of carbon delivered to the deep sea is fundamental to the evaluation of ocean carbon sequestration options. An additional key requirement is that sequestration must be verifiable and that environmental effects be monitored and minimized. These needs can be addressed by carbon system observations made from low-cost autonomous ocean-profiling floats and gliders. We have developed a prototype ocean carbon system profiler based on the Sounding Oceanographic Lagrangian Observer (SOLO; Davis et al., 1999). The SOLO/ carbon profiler will measure the two biomass components of the carbon system and their relationship to physical variables, such as upper ocean stratification and mixing. The autonomous observations within the upper 1500 m will be made on daily time scales for periods of months to seasons and will be carried out in biologically dynamic locations in the world's oceans that are difficult to access with ships (due to weather) or observe using remote sensing satellites (due to cloud cover). Such an observational capability not only will serve an important role in carbon sequestration research but will provide key observations of the global ocean's natural carbon cycle.

  12. Laser frequency combs for astronomical observations

    E-Print Network [OSTI]

    Tilo Steinmetz; Tobias Wilken; Constanza Araujo-Hauck; Ronald Holzwarth; Theodor W. Hänsch; Luca Pasquini; Antonio Manescau; Sandro D'Odorico; Michael T. Murphy; Thomas Kentischer; Wolfgang Schmidt; Thomas Udem

    2008-09-09T23:59:59.000Z

    A direct measurement of the universe's expansion history could be made by observing in real time the evolution of the cosmological redshift of distant objects. However, this would require measurements of Doppler velocity drifts of about 1 centimeter per second per year, and astronomical spectrographs have not yet been calibrated to this tolerance. We demonstrate the first use of a laser frequency comb for wavelength calibration of an astronomical telescope. Even with a simple analysis, absolute calibration is achieved with an equivalent Doppler precision of approximately 9 meters per second at about 1.5 micrometers - beyond state-of-the-art accuracy. We show that tracking complex, time-varying systematic effects in the spectrograph and detector system is a particular advantage of laser frequency comb calibration. This technique promises an effective means for modeling and removal of such systematic effects to the accuracy required by future experiments to see direct evidence of the universe's putative acceleration.

  13. Disk Evolution in Young Binaries: from Observations to Theory

    E-Print Network [OSTI]

    J. -L. Monin; C. J. Clarke; L. Prato; C. McCabe

    2006-04-03T23:59:59.000Z

    The formation of a binary system surrounded by disks is the most common outcome of stellar formation. Hence studying and understanding the formation and the evolution of binary systems and associated disks is a cornerstone of star formation science. Moreover, since the components within binary systems are coeval and the sizes of their disks are fixed by the tidal truncation of their companion, binary systems provide an ideal "laboratory" in which to study disk evolution under well defined boundary conditions. In this paper, we review observations of several inner disk diagnostics in multiple systems, including hydrogen emission lines (indicative of ongoing accretion), $K-L$ and $K-N$ color excesses (evidence of warm inner disks), and polarization (indicative of the relative orientations of the disks around each component). We examine to what degree these properties are correlated within binary systems and how this degree of correlation depends on parameters such as separation and binary mass ratio. These findings will be interpreted both in terms of models that treat each disk as an isolated reservoir and those in which the disks are subject to re-supply from some form of circumbinary reservoir, the observational evidence for which we will also critically review. The planet forming potential of multiple star systems is discussed in terms of the relative lifetimes of disks around single stars, binary primaries and binary secondaries. Finally, we summarize several potentially revealing observational problems and future projects that could provide further insight into disk evolution in the coming decade

  14. High-resolution radio observations of X-ray binaries

    E-Print Network [OSTI]

    James Miller-Jones

    2008-09-15T23:59:59.000Z

    I present an overview of important results obtained using high-resolution very long baseline interferometry (VLBI) observations of X-ray binary systems. These results derive from both astrometric observations and resolved imaging of sources, from black holes to neutron star and even white dwarf systems. I outline a number of upcoming developments in instrumentation, both new facilities and ongoing upgrades to existing VLBI instruments, and I conclude by identifying a number of important areas of investigation where VLBI will be crucial in advancing our understanding of X-ray binaries.

  15. Quintom Cosmology: Theoretical implications and observations

    E-Print Network [OSTI]

    Yi-Fu Cai; Emmanuel N. Saridakis; Mohammad R. Setare; Jun-Qing Xia

    2010-04-22T23:59:59.000Z

    We review the paradigm of quintom cosmology. This scenario is motivated by the observational indications that the equation of state of dark energy across the cosmological constant boundary is mildly favored, although the data are still far from being conclusive. As a theoretical setup we introduce a no-go theorem existing in quintom cosmology, and based on it we discuss the conditions for the equation of state of dark energy realizing the quintom scenario. The simplest quintom model can be achieved by introducing two scalar fields with one being quintessence and the other phantom. Based on the double-field quintom model we perform a detailed analysis of dark energy perturbations and we discuss their effects on current observations. This type of scenarios usually suffer from a manifest problem due to the existence of a ghost degree of freedom, and thus we review various alternative realizations of the quintom paradigm. The developments in particle physics and string theory provide potential clues indicating that a quintom scenario may be obtained from scalar systems with higher derivative terms, as well as from non-scalar systems. Additionally, we construct a quintom realization in the framework of braneworld cosmology, where the cosmic acceleration and the phantom divide crossing result from the combined effects of the field evolution on the brane and the competition between four and five dimensional gravity. Finally, we study the outsets and fates of a universe in quintom cosmology. In a scenario with null energy condition violation one may obtain a bouncing solution at early times and therefore avoid the Big Bang singularity. Furthermore, if this occurs periodically, we obtain a realization of an oscillating universe. Lastly, we comment on several open issues in quintom cosmology and their connection to future investigations.

  16. First Observation of Plasmarons in Graphene

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

    First Observation of Plasmarons in Graphene First Observation of Plasmarons in Graphene Print Wednesday, 30 June 2010 00:00 An international team of scientists performing...

  17. Interpreting observed northern hemisphere snow trends with large ensembles of climate simulations

    E-Print Network [OSTI]

    for Atmospheric Research's Community Earth System Model. Two 40-member ensembles driven by historical radiative for Atmospheric Research's Community Earth System Model (CCSM4), in comparison with observations. Each ensemble

  18. Optical monitor for observing turbulent flow

    DOE Patents [OSTI]

    Albrecht, Georg F. (Livermore, CA); Moore, Thomas R. (Rochester, NY)

    1992-01-01T23:59:59.000Z

    The present invention provides an apparatus and method for non-invasively monitoring turbulent fluid flows including anisotropic flows. The present invention uses an optical technique to filter out the rays travelling in a straight line, while transmitting rays with turbulence induced fluctuations in time. The output is two dimensional, and can provide data regarding the spectral intensity distribution, or a view of the turbulence in real time. The optical monitor of the present invention comprises a laser that produces a coherent output beam that is directed through a fluid flow, which phase-modulates the beam. The beam is applied to a temporal filter that filters out the rays in the beam that are straight, while substantially transmitting the fluctuating, turbulence-induced rays. The temporal filter includes a lens and a photorefractive crystal such as BaTiO.sub.3 that is positioned in the converging section of the beam near the focal plane. An imaging system is used to observe the filtered beam. The imaging system may take a photograph, or it may include a real time camera that is connected to a computer. The present invention may be used for many purposes including research and design in aeronautics, hydrodynamics, and combustion.

  19. INTEGRAL observations of Galaxy Clusters

    E-Print Network [OSTI]

    Goldoni, P; Laurent, P; Cassé, M; Paul, J; Sarazin, C L

    2000-01-01T23:59:59.000Z

    Cluster of galaxies are the largest concentrations of visible mass in the Universe and therefore a fundamental topic of cosmology and astrophysics. Recent radio, EUV, and X-ray observations suggest that clusters contain large populations of diffuse nonthermal relativistic and/or superthermal particles. These particles may be produced by acceleration in cluster merger shocks, AGNs, and/or supernovae in cluster galaxies. Models for the nonthermal populations in clusters indicate that they should produce substantial hard X-ray and $\\gamma$ luminosities. The possible role of nonthermal particles in the dynamics of clusters is one of the greatest uncertainties in their use as cosmological probes. INTEGRAL offers, for the first time, the possibility of simultaneous medium resolution imaging (~ 12 arcmin) and high resolution spectroscopy (DeltaE/E ~ 2 keV @ 1.3 MeV) with exceptional sensitivity in the hard X-ray/soft gamma-ray band. The spatial resolution will allow discrete sources, such as AGNs, to be separated fr...

  20. Impact of Wind Turbine Penetration on the Dynamic Performance of Interconnected Power Systems

    E-Print Network [OSTI]

    Pota, Himanshu Roy

    Impact of Wind Turbine Penetration on the Dynamic Performance of Interconnected Power Systems M. J School of S ~ao Carlos, Brazil. Email: ramos@sel.eese.usp.br Abstract--The complexity of power systems, such as wind generators. This changing nature of power systems has considerable effect on its dynamic behaviour

  1. 12 August 2005 Observing Optical Transition

    E-Print Network [OSTI]

    Anlage, Steven

    12 August 2005 Observing Optical Transition Radiation from 10keV Electrons 1 #12;12 August 2005 Observing Optical Transition Radiation from 10keV Electrons 2 #12;12 August 2005 Observing Optical Transition Radiation from 10keV Electrons 3 #12;12 August 2005 Observing Optical Transition Radiation from 10

  2. Programming Infinite Objects by Observations Andreas Abel

    E-Print Network [OSTI]

    Abel, Andreas

    ), and observe its result (behavior). Application is the defining principle of functions [Granstr¨om

  3. Programming Infinite Objects by Observations Andreas Abel

    E-Print Network [OSTI]

    Abel, Andreas

    (experiment), and observe its result (behavior). Application is the defining principle of functions [Granstr¨om

  4. ARM - Campaign Instrument - aos

    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 3,625 1,006 492 742EnergyOnItemResearchSOLICITATIONIMODI FICATIONCLASICgovInstrumentsaod Comments? We would love

  5. ARM - Datastreams - aos

    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 3,625 1,006 492air Comments? We would love torwpprecipmom Documentation

  6. ARM - Instrument - aos

    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 3,625 1,006Datastreamstwrcam40m DocumentationJanuary 9, 2009 [Events,Forms IngestgovInstrumentsamc Documentation

  7. Hengill geothermal volcanic complex (Iceland) characterized by integrated geophysical observations

    E-Print Network [OSTI]

    Paris-Sud XI, Université de

    Hengill geothermal volcanic complex (Iceland) characterized by integrated geophysical observations be used to infer the location of magma chambers or productive geothermal areas. The Hengill volcanic triple-junction complex has a well-developed geothermal system, which is being exploited to extract hot

  8. Future prospects in n-nuclear interactions. [Polarization observables

    SciTech Connect (OSTI)

    Moss, J.M.

    1982-01-01T23:59:59.000Z

    I examine in detail two research areas, polarization observables and antiproton-nucleus reactions, which should have near-term future impact on our understanding of the interaction of medium-energy nucleons in nuclei. More speculative future experiments employing cooled beams, double spectrometer systems, and large Q-valure low momentum-transfer reactions are also discussed.

  9. Observation of Bogoliubov excitations in exciton-polariton condensates

    E-Print Network [OSTI]

    Loss, Daniel

    LETTERS Observation of Bogoliubov excitations in exciton-polariton condensates S. UTSUNOMIYA1 predicted the occurrence of Bose­Einstein condensation (BEC) in an ideal gas of non-interacting bosonic Bose condensed system was developed by Bogoliubov in 1947, which predicted the phonon-like excitation

  10. Observation of the negative muonium ion in vacuum

    SciTech Connect (OSTI)

    Kuang, Yunan

    1989-05-01T23:59:59.000Z

    The negative muonium ion (M/sup /minus//), which is the bound system of a positive muon and two electrons, has been produced and observed for the first time. Its counterpart H/sup /minus// is well known, and spectroscopy and collision studies with H/sup /minus// have yielded many fruitful results. Noteworthy are recent investigations of the photoionization of a relativistic H/sup /minus// beam. The negative positronium ion has also been formed and observed. The discovery of M/sup /minus// provides us with a new leptonic system for spectroscopy and collision studies, which may reveal interesting physics associated with mass effects. Since M/sup /minus// is a charged particle, it can also be used to produce a beam of exotic atoms with a small phase space. This dissertation is a detailed account of the observation of M/sup /minus//. 93 refs., 54 figs., 18 tabs.

  11. The Arctic Lower Troposphere Observed Structure (ALTOS) Campaign

    SciTech Connect (OSTI)

    Verlinde, J

    2010-10-18T23:59:59.000Z

    The ALTOS campaign focuses on operating a tethered observing system for routine in situ sampling of low-level (< 2 km) Arctic clouds. It has been a long-term hope to fly tethered systems at Barrow, Alaska, but it is clear that the Federal Aviation Administration (FAA) will not permit in-cloud tether systems at Barrow, even if unmanned aerial vehicle (UAV) operations are allowed in the future. We have provided the scientific rationale for long-term, routine in situ measurements of cloud and aerosol properties in the Arctic. The existing restricted air space at Oliktok offers an opportunity to do so.

  12. Observation of Entanglement-Dependent Two-Particle Holonomic Phase

    E-Print Network [OSTI]

    J. C. Loredo; M. A. Broome; D. H. Smith; A. G. White

    2015-06-18T23:59:59.000Z

    Holonomic phases---geometric and topological---have long been an intriguing aspect of physics. They are ubiquitous, ranging from observations in particle physics to applications in fault tolerant quantum computing. However, their exploration in particles sharing genuine quantum correlations lack in observations. Here we experimentally demonstrate the holonomic phase of two entangled-photons evolving locally, which nevertheless gives rise to an entanglement-dependent phase. We observe its transition from geometric to topological as the entanglement between the particles is tuned from zero to maximal, and find this phase to behave more resilient to evolution changes with increasing entanglement. Furthermore, we theoretically show that holonomic phases can directly quantify the amount of quantum correlations between the two particles. Our results open up a new avenue for observations of holonomic phenomena in multi-particle entangled quantum systems.

  13. I Congresso de Estatistica e Investigac~ao Operacional da Galiza e Norte de Portugal VII Congreso Galego de Estatistica e Investigacion de Operacions

    E-Print Network [OSTI]

    Soares, João Luís Cardoso

    Galego de Estat´istica e Investigaci´on de Operaci´ons Guimar~aes 26, 27 e 28 de Outubro de 2005 SOLVINGI Congresso de Estat´istica e Investiga¸c~ao Operacional da Galiza e Norte de Portugal VII Congreso

  14. arXiv:0901.3725v1[physics.ao-ph]23Jan2009 A Brief Tutorial on the Ensemble Kalman Filter

    E-Print Network [OSTI]

    Mandel, Jan

    arXiv:0901.3725v1[physics.ao-ph]23Jan2009 A Brief Tutorial on the Ensemble Kalman Filter Jan Mandel February 2007, updated January 2009 Abstract The ensemble Kalman filter (EnKF) is a recursive filter equations in geophysical models. The EnKF originated as a version of the Kalman filter for large problems

  15. Performance and evaluation of the infrared AO sensor CALICO Leander H. Mehrgan*, Siegfried Eschbaumer, Gert Finger, Manfred Meyer, and Joerg Stegmeier

    E-Print Network [OSTI]

    Liske, Jochen

    Performance and evaluation of the infrared AO sensor CALICO , Leander H. Mehrgan*, Siegfried and to investigate the best unit cell circuit for future infrared wavefront sensors, ESO has teamed up with CALTECH-Schwarzschild Str. 2, D-85748 Garching, Germany ABSTRACT The CALICO sensor is a pathfinder for the development

  16. Mapeamento em Aneis para uma Separac~ao Neuronal Eletron-Jato usando Calorimetros Multi-camadas e Multi-segmentados

    E-Print Network [OSTI]

    Anjos, André

    reduzir o imenso fluxo de dados de eventos pre- visto, o experimento contar´a com um sistema de filtra -May use all info from all detectors -RoI based process -PC farms and fast networks -OO programming dados do evento ser~ao analizados como um todo. Neste n´ivel, para cada part´icula detetada, uma regi

  17. Observing and modeling Earths energy flows

    SciTech Connect (OSTI)

    Stevens B.; Schwartz S.

    2012-05-11T23:59:59.000Z

    This article reviews, from the authors perspective, progress in observing and modeling energy flows in Earth's climate system. Emphasis is placed on the state of understanding of Earth's energy flows and their susceptibility to perturbations, with particular emphasis on the roles of clouds and aerosols. More accurate measurements of the total solar irradiance and the rate of change of ocean enthalpy help constrain individual components of the energy budget at the top of the atmosphere to within {+-}2 W m{sup -2}. The measurements demonstrate that Earth reflects substantially less solar radiation and emits more terrestrial radiation than was believed even a decade ago. Active remote sensing is helping to constrain the surface energy budget, but new estimates of downwelling surface irradiance that benefit from such methods are proving difficult to reconcile with existing precipitation climatologies. Overall, the energy budget at the surface is much more uncertain than at the top of the atmosphere. A decade of high-precision measurements of the energy budget at the top of the atmosphere is providing new opportunities to track Earth's energy flows on timescales ranging from days to years, and at very high spatial resolution. The measurements show that the principal limitation in the estimate of secular trends now lies in the natural variability of the Earth system itself. The forcing-feedback-response framework, which has developed to understand how changes in Earth's energy flows affect surface temperature, is reviewed in light of recent work that shows fast responses (adjustments) of the system are central to the definition of the effective forcing that results from a change in atmospheric composition. In many cases, the adjustment, rather than the characterization of the compositional perturbation (associated, for instance, with changing greenhouse gas concentrations, or aerosol burdens), limits accurate determination of the radiative forcing. Changes in clouds contribute importantly to this adjustment and thus contribute both to uncertainty in estimates of radiative forcing and to uncertainty in the response. Models are indispensable to calculation of the adjustment of the system to a compositional change but are known to be flawed in their representation of clouds. Advances in tracking Earth's energy flows and compositional changes on daily through decadal timescales are shown to provide both a critical and constructive framework for advancing model development and evaluation.

  18. Oasis A New System to Acquire and Display the Analog Signals for LHC

    E-Print Network [OSTI]

    Deghaye, S; Kozar, J; Serrano, J

    2003-01-01T23:59:59.000Z

    To cope with the user requirements for the Large Hadron Collider (LHC) era, a new system has to be developed for the acquisition and display of analog signals in the accelerator domain. OASIS, the Open Analog Signals Information System, extends the capabilities of the existing 'new Analogue observation system' (nAos) in many fronts : new acquisition hardware is supported to provide higher analog bandwidth to the users, a new distributed triggering scheme has been designed for greater flexibility and the software has been completely redesigned with openness in mind to allow easy upgrading and maintainability. This paper describes the architecture chosen to satisfy the new user requirements. The solution involves three tiers and makes use of the J2EE platform to communicate between the GUI and the middle tier. The front-end tier runs on Linux PCs in CompactPCI format, to support fast digitizer modules. A first prototype system, used for the extraction tests from the Super Proton Synchrotron (SPS) to the LHC, is...

  19. Ornithological Observations 1 GUIDELINES TO AUTHORS

    E-Print Network [OSTI]

    de Villiers, Marienne

    Ornithological Observations 1 GUIDELINES TO AUTHORS Ornithological Observations is a semi flush left (no tabs or indents) and paragraphs must be separated by a line space. Authors are requested

  20. Terrestrial Carbon Observations: Protocols for Vegetation Sampling

    E-Print Network [OSTI]

    GTOS GTOS 55 Terrestrial Carbon Observations: Protocols for Vegetation Sampling and Data Submission Shashi Verma #12;(intentionally blank) #12;Terrestrial Carbon Observations: Protocols for Vegetation Forestry University, Bejing 100083, China 5 University of Wisconsin, Milwaukee, WI 6 Microsoft Research

  1. Observation of Bloch oscillations in molecular rotation

    E-Print Network [OSTI]

    Johannes Floß; Andrei Kamalov; Ilya Sh. Averbukh; Philip H. Bucksbaum

    2015-04-26T23:59:59.000Z

    The periodically kicked quantum rotor is known for non-classical effects such as quantum localisation in angular momentum space or quantum resonances in rotational excitation. These phenomena have been studied in diverse systems mimicking the kicked rotor, such as cold atoms in optical lattices, or coupled photonic structures. Recently, it was predicted that several solid state quantum localisation phenomena - Anderson localisation, Bloch oscillations, and Tamm-Shockley surface states - may manifest themselves in the rotational dynamics of laser-kicked molecules. Here, we report the first observation of rotational Bloch oscillations in a gas of nitrogen molecules kicked by a periodic train of femtosecond laser pulses. A controllable detuning from the quantum resonance creates an effective accelerating potential in angular momentum space, inducing Bloch-like oscillations of the rotational excitation. These oscillations are measured via the temporal modulation of the refractive index of the gas. Our results introduce room-temperature laser-kicked molecules as a new laboratory for studies of localisation phenomena in quantum transport.

  2. Rhodium Mossbauer Superradiance of Observable Gravitational Effect

    E-Print Network [OSTI]

    Yao Cheng; Bing Xia

    2007-11-18T23:59:59.000Z

    We summarize the experimental observations of three case studies on the long-lived rhodium Mossbauer Effect. Extraordinary observations reported in this work manifest the open-up of photonic band gap in analogy to the superconducting gap. Observable gravitational effect is manifested by the superradiance of different sample orientations corresponding to the earth gravity. These observations are of potential importance for detecting gravitational waves and development of the two-photon gamma laser.

  3. JAXA's Earth Observation Program Osamu Ochiai

    E-Print Network [OSTI]

    JAXA's Earth Observation Program Osamu Ochiai Japan Aerospace Exploration Agency #12;1 Disasters Health Energy Climate Water 1 Japanese Main Activities of Earth Observation Weather MTSAT (JMA) Eco Earth Observation Targets (JFY) 2006 2007 2008 2009 2010 2011 2012 2013 2014 2015 2016 2017 2018

  4. Observation of diamond turned OFHC copper using Scanning Tunneling Microscopy

    SciTech Connect (OSTI)

    Grigg, D.A.; Russell, P.E.; Dow, T.A.

    1988-12-01T23:59:59.000Z

    Diamond turned OFHC copper samples have been observed within the past few months using the Scanning Tunneling Microscope. Initial results have shown evidence of artifacts which may be used to better understand the diamond turning process. The STM`s high resolution capability and three dimensional data representation allows observation and study of surface features unobtainable with conventional profilometry systems. Also, the STM offers a better quantitative means by which to analyze surface structures than the SEM. This paper discusses findings on several diamond turned OFHC copper samples having different cutting conditions. Each sample has been cross referenced using STM and SEM.

  5. Natural geometric representation for electron local observables

    SciTech Connect (OSTI)

    Minogin, V.G., E-mail: minogin@isan.troitsk.ru

    2014-03-15T23:59:59.000Z

    An existence of the quartic identities for the electron local observables that define orthogonality relations for the 3D quantities quadratic in the electron observables is found. It is shown that the joint solution of the quartic and bilinear identities for the electron observables defines a unique natural representation of the observables. In the natural representation the vector type electron local observables have well-defined fixed positions with respect to a local 3D orthogonal reference frame. It is shown that the natural representation of the electron local observables can be defined in six different forms depending on a choice of the orthogonal unit vectors. The natural representation is used to determine the functional dependence of the electron wave functions on the local observables valid for any shape of the electron wave packet. -- Highlights: •Quartic identities that define the orthogonality relations for the electron local observables are found. •Joint solution of quartic and bilinear identities defines a unique natural representation of the electron local observables. •Functional dependence of the electron wave functions on the electron local observables is determined.

  6. arXiv:1012.0722v1[nlin.AO]3Dec2010 Topological stability criteria for synchronized coupled systems of non-identical

    E-Print Network [OSTI]

    . This indicates that be- side global structural measures of the network also the local and mesoscale that occur in subgraphs on the mesoscale. We then formulate and numerically confirm a conjecture that extends be possible to understand the in- terplay between local, global, and mesoscale constraints on stability

  7. VERITAS OBSERVATIONS OF THE NOVA IN V407 CYGNI

    SciTech Connect (OSTI)

    Aliu, E. [Department of Physics and Astronomy, Barnard College, Columbia University, NY 10027 (United States); Archambault, S. [Physics Department, McGill University, Montreal, QC H3A 2T8 (Canada); Arlen, T. [Department of Physics and Astronomy, University of California, Los Angeles, CA 90095 (United States); Aune, T.; Bouvier, A. [Santa Cruz Institute for Particle Physics and Department of Physics, University of California, Santa Cruz, CA 95064 (United States); Beilicke, M.; Buckley, J. H.; Bugaev, V.; Dickherber, R. [Department of Physics, Washington University, St. Louis, MO 63130 (United States); Benbow, W. [Fred Lawrence Whipple Observatory, Harvard-Smithsonian Center for Astrophysics, Amado, AZ 85645 (United States); Bradbury, S. M. [School of Physics and Astronomy, University of Leeds, Leeds LS2 9JT (United Kingdom); Byrum, K. [Argonne National Laboratory, 9700 South Cass Avenue, Argonne, IL 60439 (United States); Cannon, A.; Collins-Hughes, E. [School of Physics, University College Dublin, Belfield, Dublin 4 (Ireland); Cesarini, A.; Connolly, M. P. [School of Physics, National University of Ireland Galway, University Road, Galway (Ireland); Ciupik, L. [Astronomy Department, Adler Planetarium and Astronomy Museum, Chicago, IL 60605 (United States); Cui, W. [Department of Physics, Purdue University, West Lafayette, IN 47907 (United States); Decerprit, G. [DESY, Platanenallee 6, 15738 Zeuthen (Germany); Duke, C., E-mail: daniel-d-gall@uiowa.edu, E-mail: kazuma-tsurusaki@uiowa.edu [Department of Physics, Grinnell College, Grinnell, IA 50112-1690 (United States); and others

    2012-07-20T23:59:59.000Z

    We report on very high energy (E > 100 GeV) gamma-ray observations of V407 Cygni, a symbiotic binary that underwent a nova outburst producing 0.1-10 GeV gamma rays during 2010 March 10-26. Observations were made with the Very Energetic Radiation Imaging Telescope Array System during 2010 March 19-26 at relatively large zenith angles due to the position of V407 Cyg. An improved reconstruction technique for large zenith angle observations is presented and used to analyze the data. We do not detect V407 Cygni and place a differential upper limit on the flux at 1.6 TeV of 2.3 Multiplication-Sign 10{sup -12} erg cm{sup -2} s{sup -1} (at the 95% confidence level). When considered jointly with data from Fermi-LAT, this result places limits on the acceleration of very high energy particles in the nova.

  8. Process Cooling Pumping Systems Analysis

    E-Print Network [OSTI]

    Sherman, C.

    2008-01-01T23:59:59.000Z

    An analysis of the mill water pumping systems at a North American manufacturing facility was conducted late las year and the following issues were observed: 1. Overpumping – Both systems were overpumped to a significant degree against...

  9. Self-potential observations during hydraulic fracturing

    E-Print Network [OSTI]

    Moore, J R; Glaser, Steven D

    2007-01-01T23:59:59.000Z

    potential measurements during hydraulic fracturing of BunterSP response during hydraulic fracturing. Citation: Moore, J.observations during hydraulic fracturing, J. Geophys. Res. ,

  10. EA-1964: National Ecological Observation Network (NEON)

    Broader source: Energy.gov [DOE]

    The National Science Foundation (NSF) prepared an EA that evaluated potential environmental impacts of the proposed National Ecological Observation Network (NEON), a continental-scale network of...

  11. Observational Window Functions in Planet Transit Searches

    E-Print Network [OSTI]

    Kaspar von Braun; David R. Ciardi

    2008-01-17T23:59:59.000Z

    Window functions describe, as a function of orbital period, the probability that an existing planetary transit is detectable in one's data for a given observing strategy. We show the dependence of this probability upon several strategy and astrophysical parameters, such as length of observing run, observing cadence, length of night, and transit duration. The ability to detect a transit is directly related to the intrinsic noise of the observations. In our simulations of the window function, we explicitly address non-correlated (gaussian or white) noise and correlated (red) noise and discuss how these two different noise components affect window functions in different manners.

  12. Sandia National Laboratories: Marginal Ice Zone Observations...

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

    Marginal Ice Zone Observations and Processes Experiment mission Sierra Unmanned Aerial Vehicle to Begin Flights Over Arctic Sea Ice On July 25, 2013, in Climate, Customers &...

  13. Direct Observation of Aggregative Nanoparticle Growth: Kinetic...

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

    Aggregative Nanoparticle Growth: Kinetic Modeling of the Size Distribution and Growth Rate. Direct Observation of Aggregative Nanoparticle Growth: Kinetic Modeling of the Size...

  14. First Observation of Plasmarons in Graphene

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

    First Observation of Plasmarons in Graphene Print An international team of scientists performing angle-resolved photoemission spectroscopy (ARPES) experiments at ALS Beamline 7.0.1...

  15. CCD Observing Manual 49 Bay State Road

    E-Print Network [OSTI]

    Ellingson, Steven W.

    Stars 5.6. Supernovae/Novae Patrols 5.7. Designing Your Own: Using AAVSO VSX 6.0 Observing Techniques 6

  16. A general perspective on time observables

    E-Print Network [OSTI]

    Bryan W. Roberts

    2014-04-19T23:59:59.000Z

    I propose a general geometric framework in which to discuss the existence of time observables. This frameworks allows one to describe a local sense in which time observables always exist, and a global sense in which they can sometimes exist subject to a restriction on the vector fields that they generate. Pauli's prohibition on quantum time observables is derived as a corollary to this result. I will then discuss how time observables can be regained in modest extensions of quantum theory beyond its standard formulation.

  17. CAN REMOTE OBSERVING BE GOOD OBSERVING? REFLECTIONS ON PROCRUSTES AND ANTAEUS 1

    E-Print Network [OSTI]

    Lockman, Jay

    CAN REMOTE OBSERVING BE GOOD OBSERVING? REFLECTIONS ON PROCRUSTES AND ANTAEUS 1 Felix J. Lockman National Radio Astronomy Observatory Green Bank, WV 24944 USA ABSTRACT Remote observing seeks to simulate, written in 1992 for a conference proceedings on remote observing, is reprinted here with only slight

  18. Quantum mechanical observer and superstring/M theory

    E-Print Network [OSTI]

    M. Dance

    2008-12-31T23:59:59.000Z

    Terms are suggested for inclusion in a Lagrangian density as seen by an observer O2, to represent the dynamics of a quantum mechanical observer O1 that is an initial stage in an observation process. This paper extends an earlier paper which suggested that the centre-of-mass kinetic energy of O1 could correspond to, and possibly underlie, the Lagrangian density for bosonic string theory, where the worldsheet coordinates are the coordinates which O1 can observe. The present paper considers a fermion internal to O1, in addition to O1's centre of mass. It is suggested that quantum mechanical uncertainties in the transformation between O1's and O2's reference systems might require O2 to use $d$ spinor fields for this fermion, where $d$ is the number of spacetime dimensions. If this is the case, and if the symmetry/observability arguments in arXiv:hep-th/0601104 apply, the resulting Lagrangian density for the dynamics of O1 might resemble, or even underlie, superstring/M theory.

  19. Direct Observation of Polymer Sheathing in Carbon

    E-Print Network [OSTI]

    Direct Observation of Polymer Sheathing in Carbon Nanotube-Polycarbonate Composites W. Ding, A (MWCNT)-polycarbonate composites are presented. This sheathing was observed in images of the composite properties, increases in electrical conductivity3 and improved thermal properties4 are obtained with small

  20. Observation of Parametric Instability in Advanced LIGO

    E-Print Network [OSTI]

    Evans, Matthew; Fritschel, Peter; Miller, John; Barsotti, Lisa; Martynov, Denis; Brooks, Aidan; Coyne, Dennis; Abbott, Rich; Adhikari, Rana; Arai, Koji; Bork, Rolf; Kells, Bill; Rollins, Jameson; Smith-Lefebvre, Nicolas; Vajente, Gabriele; Yamamoto, Hiroaki; Derosa, Ryan; Effler, Anamaria; Kokeyama, Keiko; Betzweiser, Joseph; Frolov, Valera; Mullavey, Adam; O`Reilly, Brian; Dwyer, Sheila; Izumi, Kiwamu; Kawabe, Keita; Landry, Michael; Sigg, Daniel; Ballmer, Stefan; Massinger, Thomas J; Staley, Alexa; Mueller, Chris; Grote, Hartmut; Ward, Robert; King, Eleanor; Blair, David; Ju, Li; Zhao, Chunnong

    2015-01-01T23:59:59.000Z

    Parametric instabilities have long been studied as a potentially limiting effect in high-power interferometric gravitational wave detectors. Until now, however, these instabilities have never been observed in a kilometer-scale interferometer. In this work we describe the first observation of parametric instability in an Advanced LIGO detector, and the means by which it has been removed as a barrier to progress.

  1. Spectroscopic observation of the rotational Doppler effect

    E-Print Network [OSTI]

    S. Barreiro; J. W. R. Tabosa; H. Failache; A. Lezama

    2006-07-26T23:59:59.000Z

    We report on the first spectroscopic observation of the rotational Doppler shift associated with light beams carrying orbital angular momentum. The effect is evidenced as the broadening of a Hanle/EIT coherence resonance on Rb vapor when the two incident Laguerre-Gaussian laser beams have opposite topological charges. The observations closely agree with theoretical predictions.

  2. ISO SPECTROSCOPIC OBSERVATIONS OF SHORTPERIOD COMETS \\Lambda

    E-Print Network [OSTI]

    Demoulin, Pascal

    1 ISO SPECTROSCOPIC OBSERVATIONS OF SHORT­PERIOD COMETS \\Lambda J. Crovisier 1 , T. Encrenaz 1 , E 4 , E. van Dishoeck 5 , R. Knacke 6 , T.Y. Brooke 7 1 Observatoire de Paris, Meudon, France 2 ISO are found in a short­period comet. The ISO observations of the Jupiter­family comet P/Hartley 2, presum

  3. Towards observable signatures of other bubble universes

    SciTech Connect (OSTI)

    Aguirre, Anthony; Johnson, Matthew C.; Shomer, Assaf [SCIPP, University of California, Santa Cruz, California 95064 (United States)

    2007-09-15T23:59:59.000Z

    We evaluate the possibility of observable effects arising from collisions between vacuum bubbles in a universe undergoing false-vacuum eternal inflation. Contrary to conventional wisdom, we find that under certain assumptions most positions inside a bubble should have access to a large number of collision events. We calculate the expected number and angular size distribution of such collisions on an observer's 'sky', finding that for typical observers the distribution is anisotropic and includes many bubbles, each of which will affect the majority of the observer's sky. After a qualitative discussion of the physics involved in collisions between arbitrary bubbles, we evaluate the implications of our results, and outline possible detectable effects. In an optimistic sense, then, the present paper constitutes a first step in an assessment of the possible effects of other bubble universes on the cosmic microwave background and other observables.

  4. Mueller Matrix Parameters for Radio Telescopes and their Observational Determination

    E-Print Network [OSTI]

    Carl Heiles; Phil Perillat; Michael Nolan; Duncan Lorimer; Ramesh Bhat; Tapasi Ghosh; Murray Lewis; Karen O'Neil; Chris Salter; Snezana Stanimirovic

    2001-07-18T23:59:59.000Z

    Modern digital crosscorrelators permit the simultaneous measurement of all four Stokes parameters. However, the results must be calibrated to correct for the polarization transfer function of the receiving system. The transfer function for any device can be expressed by its Mueller matrix. We express the matrix elements in terms of fundamental system parameters that describe the voltage transfer functions (known as the Jones matrix) of the various system devices in physical terms and thus provide a means for comparing with engineering calculations and investigating the effects of design changes. We describe how to determine these parameters with astronomical observations. We illustrate the method by applying it to some of the receivers at the Arecibo Observatory.

  5. Hybrid Modeling of Communication Networks Using Modelica Daniel Farnqvist, Katrin Strandemar, Karl Henrik Johansson, and Jo~ao Pedro Hespanha

    E-Print Network [OSTI]

    Hespanha, João Pedro

    Hybrid Modeling of Communication Networks Using Modelica Daniel F¨arnqvist, Katrin Strandemar networks using Modelica is discussed. Congestion control in packet-switched networks, such as the Internet, by develop- ing a model library based on a recent hybrid systems model, that Modelica provides an efficient

  6. Subscriber access provided by TEL AVIV UNIV (AO) ACS Nano is published by the American Chemical Society. 1155 Sixteenth Street

    E-Print Network [OSTI]

    Hod, Oded

    radicals,34 and chemical impurities.30,40,43 A unique mechanism for spin ordering in graphene-based systems is related to the appearance of edge states.18 29,42,46 51,53,54,56 When cutting a graphene sheet along its zigzag axis to form a narrow and elongated graphene nanorib- bon (GNR), distinct electronic states ap

  7. Observational and evolutionary studies of neutron star X-ray binaries

    E-Print Network [OSTI]

    Lin, Jinrong, Ph. D. Massachusetts Institute of Technology

    2011-01-01T23:59:59.000Z

    In this thesis, we present our observational and evolutionary studies of neutron stars in X-ray binary systems. A variety of topics are discussed, which are all related by a single scientific theme, namely, helping to set ...

  8. Retrieval of Non-Spherical Dust Aerosol Properties from Satellite Observations

    E-Print Network [OSTI]

    Huang, Xin

    2013-08-01T23:59:59.000Z

    An accurate and generalized global retrieval algorithm from satellite observations is a prerequisite to understand the radiative effect of atmospheric aerosols on the climate system. Current operational aerosol retrieval algorithms are limited...

  9. Time changes in gradient and observed winds 

    E-Print Network [OSTI]

    Carlson, Ronald Dale

    1972-01-01T23:59:59.000Z

    TIME CHANGES IN GRADIENT AND OBSERVED WINDS A Thesis by RONALD DALE CARLSON Submitted to the Graduate College of Texas A&M University in partial fulfillm=n of the requirement for the degree of MASTER OF SCIENCE MAY 1972 Major Subject...: Meteorology TIME CHANGES IN GRADIENT AND OBSERVED WINDS A Thesis by RONALD D. CARLSON Approved as to style and content by: (Chairman of Co , ee) (Member) (Member) May 1972 ABSTRACT Time Changes in Gradient and Observed Winds. (May 1972) Ronald Dale...

  10. Power line harmonic radiation observed by satellite: Properties and propagation through the ionosphere

    E-Print Network [OSTI]

    Santolik, Ondrej

    Power line harmonic radiation observed by satellite: Properties and propagation through of power line harmonic radiation events observed by the low-altitude DEMETER spacecraft. Altogether, 88 with the largest intensities often occur off exact multiples of base power system frequency. This can be explained

  11. Satellite observations of the seasonal cycles of absorbing aerosols in Africa

    E-Print Network [OSTI]

    Graaf, Martin de

    Satellite observations of the seasonal cycles of absorbing aerosols in Africa related to monsoon system and aerosol loading is studied using multi-year satellite observations of UV-absorbing aerosols and rain gauge measurements. The seasonal variation of the aerosol distribution is clearly linked

  12. Observational Analysis of Cloud and Precipitation in Midlatitude Cyclones: Northern versus Southern Hemisphere Warm Fronts

    E-Print Network [OSTI]

    Satellite Observations (CALIPSO), and Advanced Microwave Scanning Radiometer for Earth Observing System Extratropical cyclones produce the bulk of the cold- season precipitation in middle and high latitudes and are key contributors to the meridional transport of energy between the equator and the poles. Though

  13. Video Observations Inside Channels of Erupting Geysers, Geyser Valley, A.Belousov1

    E-Print Network [OSTI]

    Belousov, Alexander

    Video Observations Inside Channels of Erupting Geysers, Geyser Valley, Russia A.Belousov1 , M on the internal plumbing of geyser systems. Here we present data based on video observations of interior conduit lowered a video camera (with thermal and water insulation) into the conduits of four erupting geysers

  14. Magnetospheric line radiation event observed simultaneously on board Cluster 1, Cluster 2 and DEMETER spacecraft

    E-Print Network [OSTI]

    Santolik, Ondrej

    be related to power line harmonic radiation (PLHR, an electromagnetic radiation from electric power systemsMagnetospheric line radiation event observed simultaneously on board Cluster 1, Cluster 2., O. Santolík, M. Parrot, and J. S. Pickett (2012), Magnetospheric line radiation event observed

  15. Observing motor learning produces somatosensory change Nicol F. Bernardi,1,2

    E-Print Network [OSTI]

    Malfait, Nicole

    Observing motor learning produces somatosensory change Nicolò F. Bernardi,1,2 Mohammad Darainy,1, Darainy M, Bricolo E, Ostry DJ. Observing motor learning produces somatosensory change. J Neurophysiol 110 of others has been shown to affect motor learning, but does it have effects on sensory systems as well

  16. Initial Helioseismic Observations by Hinode/SOT

    E-Print Network [OSTI]

    Takashi Sekii; Alexander G. Kosovichev; Junwei Zhao; Saku Tsuneta; Hiromoto Shibahashi; Thomas E. Berger; Kiyoshi Ichimoto; Yukio Katsukawa; Bruce W. Lites; Shin'ichi Nagata; Toshifumi Shimizu; Richard A. Shine; Yoshinori Suematsu; Theodore D. Tarbell; Alan M. Title

    2007-09-12T23:59:59.000Z

    Results from initial helioseismic observations by Solar Optical Telescope onboard Hinode are reported. It has been demonstrated that intensity oscillation data from Broadband Filter Imager can be used for various helioseismic analyses. The k-omega power spectra, as well as corresponding time-distance cross-correlation function that promises high-resolution time-distance analysis below 6-Mm travelling distance, were obtained for G-band and CaII-H data. Subsurface supergranular patterns have been observed from our first time-distance analysis. The results show that the solar oscillation spectrum is extended to much higher frequencies and wavenumbers, and the time-distance diagram is extended to much shorter travel distances and times than they were observed before, thus revealing great potential for high-resolution helioseismic observations from Hinode.

  17. NASA Launches New Earth Observation Satellite

    E-Print Network [OSTI]

    Christian, Eric

    Goddard View The Weekly ­ 2 NASA Launches New Earth Observation Satellite ­ 3 3-D printing Creates Complex free online access to the information. This revolution has al- lowed scientists to detect changes over

  18. INTEGRAL observations of HER X-1

    E-Print Network [OSTI]

    D. Klochkov; R. Staubert; S. Tsygankov; A. Lutovinov; K. P. Postnov; N. I. Shakura; S. A. Potanin; C. Ferrigno; I. Kreykenbohm; J. Wilms

    2007-04-23T23:59:59.000Z

    First results of observations of the low mass X-ray binary Her X-1/HZ Her performed by the INTEGRAL satellite in July-August 2005 are presented. A significant part of one 35 day main-on state was covered. The cyclotron line in the X-ray spectrum is well observed and its position and shape, as well as its variability with time and phase of the 1.24 s pulsation are explored. X-ray pulse profiles for different energy bands are studied throughout the observation. The pulse period is found to vary on short time scales revealing a dynamical spin-up/spin-down behavior. Results of simultaneous optical observations of HZ Her are also discussed.

  19. Gamma-Ray Line Observations with RHESSI

    E-Print Network [OSTI]

    David M. Smith

    2004-04-30T23:59:59.000Z

    The Reuven Ramaty High Energy Solar Spectroscopic Imager (RHESSI) has been observing gamma-ray lines from the Sun and the Galaxy since its launch in February 2002. Here I summarize the status of RHESSI observations of solar lines (nuclear de-excitation, neutron capture, and positron annihilation), the lines of $^{26}$Al and $^{60}$Fe from the inner Galaxy, and the search for positron annihilation in novae.

  20. Infrasonic observations of the Northridge, California, earthquake

    SciTech Connect (OSTI)

    Mutschlecner, J.P.; Whitaker, R.W.

    1994-09-01T23:59:59.000Z

    Infrasonic waves from the Northridge, California, earthquake of 17 January 1994 were observed at the St. George, Utah, infrasound array of the Los Alamos National Laboratory. The distance to the epicenter was 543 kilometers. The signal shows a complex character with many peaks and a long duration. An interpretation is given in terms of several modes of signal propagation and generation including a seismic-acoustic secondary source mechanism. A number of signals from aftershocks are also observed.

  1. Mass Parameterizations and Predictions of Isotopic Observables

    E-Print Network [OSTI]

    S. R. Souza; P. Danielewicz; S. Das Gupta; R. Donangelo; W. A. Friedman; W. G. Lynch; W. P. Tan; M. B. Tsang

    2003-03-24T23:59:59.000Z

    We discuss the accuracy of mass models for extrapolating to very asymmetric nuclei and the impact of such extrapolations on the predictions of isotopic observables in multifragmentation. We obtain improved mass predictions by incorporating measured masses and extrapolating to unmeasured masses with a mass formula that includes surface symmetry and Coulomb terms. We find that using accurate masses has a significant impact on the predicted isotopic observables.

  2. MMT/AO 5 micron Imaging Constraints on the Existence of Giant Planets Orbiting Fomalhaut at ~13-40 AU

    E-Print Network [OSTI]

    Matthew A. Kenworthy; Eric E. Mamajek; Philip M. Hinz; Michael R. Meyer; Aren N. Heinze; Douglas L. Miller; Suresh Sivanandam; Melanie Freed

    2008-11-17T23:59:59.000Z

    A candidate secondary mirror. Our images are sensitive to giant planets at orbital radii comparable to the outer solar system (~5-40 AU). Comparing our 5-sigma M-band photometric limits to theoretical evolutionary tracks for substellar objects, our results rule out the existence of planets with masses greater than 2 Jupiter masses, from ~13-40 AU and objects greater than 13 Jupiter masses from ~8-40 AU.

  3. MMT/AO 5 micron Imaging Constraints on the Existence of Giant Planets Orbiting Fomalhaut at ~13-40 AU

    E-Print Network [OSTI]

    Kenworthy, Matthew A; Hinz, Philip M; Meyer, Michael R; Heinze, Aren N; Miller, Douglas L; Sivanandam, Suresh; Freed, Melanie

    2008-01-01T23:59:59.000Z

    A candidate secondary mirror. Our images are sensitive to giant planets at orbital radii comparable to the outer solar system (~5-40 AU). Comparing our 5-sigma M-band photometric limits to theoretical evolutionary tracks for substellar objects, our results rule out the existence of planets with masses greater than 2 Jupiter masses, from ~13-40 AU and objects greater than 13 Jupiter masses from ~8-40 AU.

  4. VERITAS OBSERVATIONS OF GAMMA-RAY BURSTS DETECTED BY SWIFT

    SciTech Connect (OSTI)

    Acciari, V. A.; Benbow, W. [Fred Lawrence Whipple Observatory, Harvard-Smithsonian Center for Astrophysics, Amado, AZ 85645 (United States); Aliu, E.; Errando, M. [Department of Physics and Astronomy, Barnard College, Columbia University, NY 10027 (United States); Arlen, T. [Department of Physics and Astronomy, University of California, Los Angeles, CA 90095 (United States); Aune, T. [Santa Cruz Institute for Particle Physics and Department of Physics, University of California, Santa Cruz, CA 95064 (United States); Beilicke, M.; Buckley, J. H.; Bugaev, V. [Department of Physics, Washington University, St. Louis, MO 63130 (United States); Bradbury, S. M. [School of Physics and Astronomy, University of Leeds, Leeds, LS2 9JT (United Kingdom); Byrum, K. [Argonne National Laboratory, 9700 S. Cass Avenue, Argonne, IL 60439 (United States); Cannon, A.; Collins-Hughes, E. [School of Physics, University College Dublin, Belfield, Dublin 4 (Ireland); Cesarini, A.; Connolly, M. P. [School of Physics, National University of Ireland Galway, University Road, Galway (Ireland); Christiansen, J. L. [Physics Department, California Polytechnic State University, San Luis Obispo, CA 94307 (United States); Ciupik, L. [Astronomy Department, Adler Planetarium and Astronomy Museum, Chicago, IL 60605 (United States); Cui, W. [Department of Physics, Purdue University, West Lafayette, IN 47907 (United States); Duke, C. [Department of Physics, Grinnell College, Grinnell, IA 50112-1690 (United States); Falcone, A. [Department of Astronomy and Astrophysics, 525 Davey Lab, Pennsylvania State University, University Park, PA 16802 (United States); and others

    2011-12-10T23:59:59.000Z

    We present the results of 16 Swift-triggered Gamma-ray burst (GRB) follow-up observations taken with the Very Energetic Radiation Imaging Telescope Array System (VERITAS) telescope array from 2007 January to 2009 June. The median energy threshold and response time of these observations were 260 GeV and 320 s, respectively. Observations had an average duration of 90 minutes. Each burst is analyzed independently in two modes: over the whole duration of the observations and again over a shorter timescale determined by the maximum VERITAS sensitivity to a burst with a t{sup -1.5} time profile. This temporal model is characteristic of GRB afterglows with high-energy, long-lived emission that have been detected by the Large Area Telescope on board the Fermi satellite. No significant very high energy (VHE) gamma-ray emission was detected and upper limits above the VERITAS threshold energy are calculated. The VERITAS upper limits are corrected for gamma-ray extinction by the extragalactic background light and interpreted in the context of the keV emission detected by Swift. For some bursts the VHE emission must have less power than the keV emission, placing constraints on inverse Compton models of VHE emission.

  5. Observation of Dirac Monopoles in a Synthetic Magnetic Field

    E-Print Network [OSTI]

    Ray, M W; Kandel, S; Möttönen, M; Hall, D S

    2014-01-01T23:59:59.000Z

    Magnetic monopoles --- particles that behave as isolated north or south magnetic poles --- have been the subject of speculation since the first detailed observations of magnetism several hundred years ago. Numerous theoretical investigations and hitherto unsuccessful experimental searches have followed Dirac's 1931 development of a theory of monopoles consistent with both quantum mechanics and the gauge invariance of the electromagnetic field. The existence of even a single Dirac magnetic monopole would have far-reaching physical consequences, most famously explaining the quantization of electric charge. Although analogues of magnetic monopoles have been found in exotic spin-ices and other systems, there has been no direct experimental observation of Dirac monopoles within a medium described by a quantum field, such as superfluid helium-3. Here we demonstrate the controlled creation of Dirac monopoles in the synthetic magnetic field produced by a spinor Bose-Einstein condensate. Monopoles are identified, in b...

  6. PMU Placement for Enhancing Dynamic Observability of a Power Grid

    SciTech Connect (OSTI)

    Du, Pengwei; Huang, Zhenyu; Diao, Ruisheng; Lee, Barry; Anderson, Kevin K.

    2010-09-27T23:59:59.000Z

    Power grids are operated in an increasingly complicated environment. However, operators lack effective and accurate tools for real-time monitoring and control of power systems. The U.S. Department of Energy, along with several utilities and system operators, is making a major $108 million investment in the Western Interconnection for phasor measurement unit (PMU) installation and phasor application development. This phasor measurement network opens up many opportunities for the estimation and prediction of power system states in real time, which enable operators to evaluate the system dynamic security in advance and allow them more time to respond to disturbances. Kalman filter based dynamic state estimation offers a solution suitable for this purpose. Our work indicates that the performance of Kalman filters in dynamic state estimation would degrade if PMU measurements cannot adequately capture the system dynamics. This paper develops a framework to identify how to place PMUs to improve dynamic observability of the power grid. Simulation results validate the concept, and the guidelines for PMU placement are derived.

  7. Causa Efficiens versus Causa Formalis: origens da discuss\\~ao moderna sobre a dimensionalidade do espa\\c{c}o

    E-Print Network [OSTI]

    Caruso, Francisco

    2015-01-01T23:59:59.000Z

    Metascientific criteria used for explaining or constraining physical space dimensionality and their historical relationship to prevailing causal systems are discussed. The important contributions by Aristotle, Kant and Ehrenfest to the dimensionality of space problem are considered and shown to be grounded on different causal explanations: {\\it causa materialis} for Aristotle, {\\it causa efficiens} for young Kant and an ingenious combination of {\\it causa efficiens} and {\\it causa formalis} for Ehrenfest. The prominent and growing r\\^ole played by {\\it causa formalis} in modern physical approaches to this problem is emphasized.

  8. XXX SIMP OSIO BRASILEIRO DE TELECOMUNICAC ~OES -SBrT'12, 13-16 DE SETEMBRO DE 2012, BRASILIA, DF Codificac~ao de Video H.264/AVC em Tempo Real e

    E-Print Network [OSTI]

    de Queiroz, Ricardo L.

    ´ilia-DF, Brasil, E-mail: queiroz@ieee.org tem oferecido novas arquiteturas com forte vi´es de economia de energia´ILIA, DF Codificac¸~ao de V´ideo H.264/AVC em Tempo Real e Restrita por Energia Tiago A. da Fonseca e maior e, portanto, maior consumo de energia. Para permitir soluc¸~oes verdes de codificac¸~ao de v

  9. Simultaneous state and unknown inputs estimation with PI and PMI observers for Takagi Sugeno model with unmeasurable premise

    E-Print Network [OSTI]

    Paris-Sud XI, Université de

    Simultaneous state and unknown inputs estimation with PI and PMI observers for Takagi Sugeno model-- In this paper, a proportional integral (PI) and a proportional multiple integral observer (PMI) are proposed and PMI observers developed for linear systems. The state estimation error is written as a perturbed

  10. OBSERVING CORONAL NANOFLARES IN ACTIVE REGION MOSS

    SciTech Connect (OSTI)

    Testa, Paola; DeLuca, Ed; Golub, Leon; Korreck, Kelly; Weber, Mark [Smithsonian Astrophysical Observatory, 60 Garden street, MS 58, Cambridge, MA 02138 (United States); De Pontieu, Bart; Martinez-Sykora, Juan; Title, Alan [Lockheed Martin Solar and Astrophysics Lab, Org. A021S, Bldg. 252, 3251 Hanover Street, Palo Alto, CA 94304 (United States); Hansteen, Viggo [Institute of Theoretical Astrophysics, University of Oslo, P.O. Box 1029 Blindern, N-0315 Oslo (Norway); Cirtain, Jonathan; Winebarger, Amy; Kobayashi, Ken [NASA Marshall Space Flight Center, ZP 13, Huntsville, AL 35812 (United States); Kuzin, Sergey [P. N. Lebedev Physical institute of the Russian Academy of Sciences, Leninskii prospekt, 53, 119991 Moscow (Russian Federation); Walsh, Robert [University of Central Lancashire, Lancashire, Preston PR1 2HE (United Kingdom); DeForest, Craig, E-mail: ptesta@cfa.harvard.edu [Southwest Research Institute, 1050 Walnut Street, Suite 300, Boulder, CO 80302 (United States)

    2013-06-10T23:59:59.000Z

    The High-resolution Coronal Imager (Hi-C) has provided Fe XII 193A images of the upper transition region moss at an unprecedented spatial ({approx}0.''3-0.''4) and temporal (5.5 s) resolution. The Hi-C observations show in some moss regions variability on timescales down to {approx}15 s, significantly shorter than the minute-scale variability typically found in previous observations of moss, therefore challenging the conclusion of moss being heated in a mostly steady manner. These rapid variability moss regions are located at the footpoints of bright hot coronal loops observed by the Solar Dynamics Observatory/Atmospheric Imaging Assembly in the 94 A channel, and by the Hinode/X-Ray Telescope. The configuration of these loops is highly dynamic, and suggestive of slipping reconnection. We interpret these events as signatures of heating events associated with reconnection occurring in the overlying hot coronal loops, i.e., coronal nanoflares. We estimate the order of magnitude of the energy in these events to be of at least a few 10{sup 23} erg, also supporting the nanoflare scenario. These Hi-C observations suggest that future observations at comparable high spatial and temporal resolution, with more extensive temperature coverage, are required to determine the exact characteristics of the heating mechanism(s).

  11. Observations of the Askaryan Effect in Ice

    SciTech Connect (OSTI)

    Gorham, P.W.

    2007-01-16T23:59:59.000Z

    We report on the first observations of the Askaryan effect in ice: coherent impulsive radio Cherenkov radiation from the charge asymmetry in an electromagnetic (EM) shower. Such radiation has been observed in silica sand and rock salt, but this is the first direct observation from an EM shower in ice. These measurements are important since the majority of experiments to date that rely on the effect for ultra-high energy neutrino detection are being performed using ice as the target medium. As part of the complete validation process for the Antarctic Impulsive Transient Antenna (ANITA) experiment, we performed an experiment at the Stanford Linear Accelerator Center (SLAC) in June 2006 using a 7.5 metric ton ice target, yielding results fully consistent with theoretical expectations.

  12. Observations of the Askaryan Effect in Ice

    E-Print Network [OSTI]

    ANITA collaboration; P. W. Gorham; S. W. Barwick; J. J. Beatty; D. Z. Besson; W. R. Binns; C. Chen; P. Chen; J. M. Clem; A. Connolly; P. F. Dowkontt; M. A. DuVernois; R. C. Field; D. Goldstein; A. Goodhue; C. Hast; C. L. Hebert; S. Hoover; M. H. Israel; J. Kowalski; J. G. Learned; K. M. Liewer; J. T. Link; E. Lusczek; S. Matsuno; B. Mercurio; C. Miki; P. Miocinovic; J. Nam; C. J. Naudet; J. Ng; R. Nichol; K. Palladino; K. Reil; A. Romero-Wolf; M. Rosen; D. Saltzberg; D. Seckel; G. S. Varner; D. Walz; F. Wu

    2007-01-12T23:59:59.000Z

    We report on the first observations of the Askaryan effect in ice: coherent impulsive radio Cherenkov radiation from the charge asymmetry in an electromagnetic (EM) shower. Such radiation has been observed in silica sand and rock salt, but this is the first direct observation from an EM shower in ice. These measurements are important since the majority of experiments to date that rely on the effect for ultra-high energy neutrino detection are being performed using ice as the target medium. As part of the complete validation process for the Antarctic Impulsive Transient Antenna (ANITA) experiment, we performed an experiment at the Stanford Linear Accelerator Center (SLAC) in June 2006 using a 7.5 metric ton ice target, yielding results fully consistent with theoretical expectations.

  13. Workshop on observations of recent comets (1990)

    SciTech Connect (OSTI)

    Huebner, W.F.; Wehinger, P.A.; Rahe, J.; Konno, I.

    1990-01-01T23:59:59.000Z

    Potential interpretations are presented for observations of four comets: Brorsen-Metcalf (1989o), Okazaki-Levy-Rudenko (1989r), Aarseth-Brewington (1989a1), and Austin (1989o1). The relationship of minor species with each other and possible parents as well as with dust are being pursued in a number of investigations. Of particular interest are the abundance ratios of CH{sub 4} to CO and NH{sub 3} to N{sub 2}. The need for closer collaboration betwen observing teams and modelers is examined. The need for dust size distribution as a function of cometocentric distance to be analyzed in closer collaboration between observers and modelers is discussed.

  14. Observations of the Askaryan Effect in Ice

    E-Print Network [OSTI]

    Barwick, S W; Besson, D Z; Binns, W R; Chen, P; Clem, J M; Connolly, A; Dowkontt, P F; Duvernois, M A; Field, R C; Goldstein, D; Goodhue, A; Gorham, P W; Hast, C; Hebert, C L; Hoover, S; Israel, M H; Kowalski, J; Learned, J G; Liewer, K M; Link, J T; Lusczek, E; Matsuno, S; Mercurio, B; Miki, C; Miocinovic, P; Nam, J; Naudet, C J; Ng, J; Nichol, R; Palladino, K J; Reil, K; Romero-Wolf, A; Rosen, M; Saltzberg, D; Secke, D; Varner, G S; Walz, D; Wu, F

    2006-01-01T23:59:59.000Z

    We report on the first observations of the Askaryan effect in ice: coherent impulsive radio Cherenkov radiation from the charge asymmetry in an electromagnetic (EM) shower. Such radiation has been observed in silica sand and rock salt, but this is the first direct observation from an EM shower in ice. These measurements are important since the majority of experiments to date that rely on the effect for ultra-high energy neutrino detection are being performed using ice as the target medium. As part of the complete validation process for the Antarctic Impulsive Transient Antenna (ANITA) experiment, we performed an experiment at the Stanford Linear Accelerator Center (SLAC) in June 2006 using a 7.5 metric ton ice target, yielding results fully consistent with theoretical expectations.

  15. Rhodium Mossbauer Superradiance of Observable Gravitational Effect

    E-Print Network [OSTI]

    Cheng, Yao

    2007-01-01T23:59:59.000Z

    We report the direct observations of the entangled superradiance from rhodium nuclei oriented along the long edge of the polycrystalline sample. The long-lived rhodium Mossbauer effect is sensitive to the earth gravity, which opens up novel approaches of detecting the gravitational waves. Superradiance and exciton diffusion are enhanced by liquid-nitrogen cooling. Gravitational effect attributed to multipolar nuclear transition of the atto-eV natural linewidth is manifested by emissions from different sample orientations corresponding to the earth gravity. The long-range gamma coupling across grain boundaries despite the temperature variation inside sample is manifested by the observed dependence on macroscopic sample size.

  16. Black Holes: from Speculations to Observations

    E-Print Network [OSTI]

    Thomas W. Baumgarte

    2006-04-13T23:59:59.000Z

    This paper provides a brief review of the history of our understanding and knowledge of black holes. Starting with early speculations on ``dark stars'' I discuss the Schwarzschild "black hole" solution to Einstein's field equations and the development of its interpretation from "physically meaningless" to describing the perhaps most exotic and yet "most perfect" macroscopic object in the universe. I describe different astrophysical black hole populations and discuss some of their observational evidence. Finally I close by speculating about future observations of black holes with the new generation of gravitational wave detectors.

  17. Observation of superdeformation in sup 191 Hg

    SciTech Connect (OSTI)

    Moore, E.F.; Janssens, R.V.F.; Chasman, R.R.; Ahmad, I.; Khoo, T.L.; Wolfs, F.L.H. (Argonne National Laboratory, Argonne, Illinois 60439 (US)); Ye, D. (Argonne National Laboratory, Argonne, Illinois 60439 (US)); Beard, K.B. (Argonne National Laboratory, Argonne, Illinois 60439 (US)); Garg, U. (University of Notre Dame, Notre Dame, Indiana 46556); Drigert, M.W. (Idaho National Engineering Laboratory, EG G Idaho Inc., Idaho Falls, Idaho 83415); and others

    1989-07-24T23:59:59.000Z

    The first observation of superdeformation in the mass region {ital A}{congruent}190 is reported. A rotational band of twelve transitions with an average energy spacing of 37 keV, an average moment of inertia {ital scrF}{sup (2)} of 110 {h bar}{sup 2} MeV{sup {minus}1}, and an average quadrupole moment of 18{plus minus}3 {ital e} b has been observed in {sup 191}Hg; this band persists at low rotational frequency. These results are in excellent agreement with a calculation that predicts an ellipsoidal axis ratio of 1.65:1 for the superdeformed shape in this nucleus.

  18. Experimental Observation of a Generalized Gibbs Ensemble

    E-Print Network [OSTI]

    Tim Langen; Sebastian Erne; Remi Geiger; Bernhard Rauer; Thomas Schweigler; Maximilian Kuhnert; Wolfgang Rohringer; Igor E. Mazets; Thomas Gasenzer; Jörg Schmiedmayer

    2014-11-26T23:59:59.000Z

    The connection between the non-equilibrium dynamics of isolated quantum many-body systems and statistical mechanics is a fundamental open question. It is generally believed that the unitary quantum evolution of a sufficiently complex system leads to an apparent maximum-entropy state that can be described by thermodynamical ensembles. However, conventional ensembles fail to describe the large class of systems that exhibit non-trivial conserved quantities. Instead, generalized ensembles have been predicted to maximize entropy in these systems. In our experiments we explicitly show that a degenerate one-dimensional Bose gas relaxes to a state that can be described by such a generalized ensemble. This is verified through a detailed study of correlation functions up to 10th order. The applicability of the generalized ensemble description for isolated quantum many-body systems points to a natural emergence of classical statistical properties from the microscopic unitary quantum evolution.

  19. Braking system

    DOE Patents [OSTI]

    Norgren, D.U.

    1982-09-23T23:59:59.000Z

    A balanced braking system comprising a plurality of braking assemblies located about a member to be braked. Each of the braking assemblies consists of a spring biased piston of a first material fitted into a body of a different material which has a greater contraction upon cooling than the piston material. The piston is provided with a recessed head portion over which is positioned a diaphragm and forming a space therebetween to which is connected a pressurized fluid supply. The diaphragm is controlled by the fluid in the space to contact or withdraw from the member to be braked. A cooling means causes the body within which the piston is fitted to contract more than the piston, producing a tight shrink fit therebetween. The braking system is particularly applicable for selectively braking an arbor of an electron microscope which immobilizes, for example, a vertically adjustable low temperature specimen holder during observation. The system provides balanced braking forces which can be easily removed and re-established with minimal disturbance to arbor location.

  20. Recurrence properties of quantum observables in wave packet dynamics

    E-Print Network [OSTI]

    Sudheesh, C; Balakrishnan, V

    2009-01-01T23:59:59.000Z

    We investigate the recurrence properties of the time series of quantum mechanical expectation values, in terms of two representative models for a single-mode radiation field interacting with a nonlinear medium. From recurrence-time distributions, return maps and recurrence plots, we conclude that the dynamics of appropriate observables pertaining to the field can vary from quasiperiodicity to hyperbolicity, depending on the extent of the nonlinearity and of the departure from coherence of the initial state of the field. We establish that, in a simple bipartite model in which the field is effectively an open quantum system, a decaying exponential recurrence-time distribution, characteristic of a hyperbolic dynamical system, is associated with chaotic temporal evolution as characterized by a positive Liapunov exponent.

  1. Recurrence properties of quantum observables in wave packet dynamics

    E-Print Network [OSTI]

    C. Sudheesh; S. Lakshmibala; V. Balakrishnan

    2009-12-29T23:59:59.000Z

    We investigate the recurrence properties of the time series of quantum mechanical expectation values, in terms of two representative models for a single-mode radiation field interacting with a nonlinear medium. From recurrence-time distributions, return maps and recurrence plots, we conclude that the dynamics of appropriate observables pertaining to the field can vary from quasiperiodicity to hyperbolicity, depending on the extent of the nonlinearity and of the departure from coherence of the initial state of the field. We establish that, in a simple bipartite model in which the field is effectively an open quantum system, a decaying exponential recurrence-time distribution, characteristic of a hyperbolic dynamical system, is associated with chaotic temporal evolution as characterized by a positive Liapunov exponent.

  2. Belief Revision with Unreliable Observations Craig Boutilier

    E-Print Network [OSTI]

    Halpern, Joseph Y.

    Belief Revision with Unreliable Observations Craig Boutilier Dept. Computer Science University of British Columbia Vancouver, British Columbia Canada, V6T 1W5 cebly@cs.ubc.ca Nir Friedman ¡£¢ Computer Research in belief revision has been dominated by work that lies firmly within the classic AGM paradigm

  3. OH Maser Observations of Planetary Nebulae Precursors

    E-Print Network [OSTI]

    R. M. Deacon; J. M. Chapman; A. J. Green

    2004-06-08T23:59:59.000Z

    We present OH maser observations at 1612, 1665, 1667, and 1720 MHz for 86 post-asymptotic giant branch (post-AGB) stars selected from a survey of 1612 MHz maser sources in the Galactic Plane. The observations were taken with the Parkes Telescope and the Australia Telescope Compact Array between 2002 September and 2003 August. Post-AGB stars are the precursors to planetary nebulae, the diverse morphological range of which is unexplained. The maser observations were taken to investigate the onset and incidence of wind asymmetries during the post-AGB phase. We re-detected all 86 sources at 1612 MHz while 27 sources were detected at 1665 and 45 at 1667 MHz. One source was re-detected at 1720 MHz. We present a classification scheme for the maser profiles and show that 25% of sources in our sample are likely to have asymmetric or bipolar outflows. From a comparison of the maser and far-infrared properties we find that there is a likely trend in the shape of the maser profiles with some sources evolving from double-peaked to irregular to fully bipolar profiles. A subset of higher-mass sources stand out as having almost no mainline emission and mostly double-peaked profiles. At least 25% of sources in the sample are variable at one or more of the frequencies observed. We also confirm a previously-noted 1667 MHz overshoot phenomenon.

  4. INVENTORY MANAGEMENT WITH PARTIALLY OBSERVED NONSTATIONARY DEMAND

    E-Print Network [OSTI]

    Ludkovski, Mike

    INVENTORY MANAGEMENT WITH PARTIALLY OBSERVED NONSTATIONARY DEMAND ERHAN BAYRAKTAR AND MICHAEL LUDKOVSKI Abstract. We consider a continuous-time model for inventory management with Markov mod- ulated non inventory level. We then solve this equivalent formulation and directly characterize an optimal inventory

  5. 8) Stratospheric equatorial variability a) Observations

    E-Print Network [OSTI]

    Lott, Francois

    speed. Phase lines inclined eastward when altitude increases indicating upward propation Signal field) Westward phase propagation but eastward group propagation Phase lines inclined westward Signal;5 Satellites wind observations (UARS, Swinbak et Ortland 1997) The Quasi-Biennial Oscillation (low stratosphere

  6. Observation of energetic electrons within magnetic islands

    E-Print Network [OSTI]

    Loss, Daniel

    that energetic electron fluxes peak at sites of compressed density within islands, which imposes a new constraintLETTERS Observation of energetic electrons within magnetic islands L.-J. CHEN1 *, A. BHATTACHARJEE1, University of New Hampshire, Durham, New Hampshire 03824, USA 2 National Astronomical Observatory of Japan, 2

  7. Finding slowly decaying observables Gary Froyland \\Lambda

    E-Print Network [OSTI]

    Froyland, Gary

    Finding slowly decaying observables Gary Froyland \\Lambda Department of Mathematical Engineering initial transient behaviour to disappear. We present a rigorous numerical method for (i) estimating distribution on M ; that is, if you plot the orbit on a computer, you see the same distribution of dots. We

  8. Uncertain Probabilistic Roadmaps with Observations Richard Dearden

    E-Print Network [OSTI]

    Yao, Xin

    Uncertain Probabilistic Roadmaps with Observations Richard Dearden School of Computer Science Science University of Birmingham Birmingham, B15 2TT, UK mlk@cs.bham.ac.uk Abstract Probabilistic roadmaps. Introduction Probabilistic Roadmaps (PRM) are a popular technique for path planning in high dimensional spaces

  9. Energy flow observables in hadronic collisions

    E-Print Network [OSTI]

    F. Hautmann

    2012-05-24T23:59:59.000Z

    We present recent QCD calculations of energy flow distributions associated with the production of jets at wide rapidity separations in high-energy hadron collisions, and discuss the role of these observables to analyze contributions from parton showering and from multiple parton collisions.

  10. Observation-based test set generation

    E-Print Network [OSTI]

    Cobb, Jeffrey Lee

    2013-02-22T23:59:59.000Z

    . Current test set generation relies primarily on the "stuck-at" model, which both excites and observes every site of the circuit. However, a test set with good stuck-at fault coverage will not necessarily find all the defects in a circuit. Other models...

  11. 7, 79077932, 2007 ACE-FTS observation

    E-Print Network [OSTI]

    Boyer, Edmond

    , D. Hauglustaine5 , C. D. Boone6 , and P. F. Bernath6,7 1 Spectroscopie de l'atmosph`ere, Chimie Center, Mail Stop 401A, Hampton, VA 23681-2199, USA 4 Earth Observation Science, Space Research Centre Laboratoire des Sciences du Climat et de l'Environnement (LSCE)/Institut Pierre-Simon Laplace, CEA-CNRS, F

  12. Atmospheric Noise in Single Dish Observations

    E-Print Network [OSTI]

    Militzer, Burkhard

    the errors in a wideband total power measurement. Noise con­ tributions come from thermal noise consider total power measurements with a single dish radiometer. The measured total power, p[K] = g \\Theta for extended sources. For wideband total power observations, the maximum integration time ¸ 0.1 s in order

  13. An Observational Look at Rotating Stars

    E-Print Network [OSTI]

    Wiita, Paul J.

    . The Doppler Effect induces a shift at each end of the star's spectrum as one limb recedes, while the other radial velocities and the resulting shifts in wavelength from the various parts of the star (Kaler 1989 be calculated, or perhaps even the angular velocity" (Abney 1877). The component of the radial velocity observed

  14. Relativistic particle: Dirac observables and Feynman propagator

    SciTech Connect (OSTI)

    Freidel, Laurent; Girelli, Florian; Livine, Etera R. [Perimeter Institute, 31 Caroline St North, Waterloo, ON, N2L 2Y5 (Canada); SISSA, Via Beirut 2-4, 34014 Trieste (Italy); INFN, Sezione di Trieste (Italy); Laboratoire de Physique, ENS Lyon, CNRS UMR 5672, 46 Allee d'Italie, 69364 Lyon Cedex 07 (France)

    2007-05-15T23:59:59.000Z

    We analyze the algebra of Dirac observables of the relativistic particle in four space-time dimensions. We show that the position observables become noncommutative and the commutation relations lead to a structure very similar to the noncommutative geometry of deformed special relativity (DSR). In this framework, it appears natural to consider the 4D relativistic particle as a five-dimensional massless particle. We study its quantization in terms of wave functions on the 5D light cone. We introduce the corresponding five-dimensional action principle and analyze how it reproduces the physics of the 4D relativistic particle. The formalism is naturally subject to divergences (due to the 5D representation), and we show that DSR arises as a natural regularization: the 5D light cone is regularized as the de Sitter space. We interpret the fifth coordinate as the particle's proper time while the fifth moment can be understood as the mass. Finally, we show how to formulate the Feynman propagator and the Feynman amplitudes of quantum field theory in this context in terms of Dirac observables. This provides new insights for the construction of observables and scattering amplitudes in DSR.

  15. Observability of Neuronal Network Motifs (Invited Paper)

    E-Print Network [OSTI]

    Brennan, Sean

    Observability of Neuronal Network Motifs (Invited Paper) Andrew J. Whalen*t, Sean N. Brennan Engineering, + Engineering Science and Mechanics, Neurosurgery, and Physics, Penn State University, University) neuronal networks as a function of 1) the connection topology and sym metry, 2) the measured nodes, and 3

  16. Power Counting to Better Jet Observables

    E-Print Network [OSTI]

    Andrew J. Larkoski; Ian Moult; Duff Neill

    2014-09-22T23:59:59.000Z

    Optimized jet substructure observables for identifying boosted topologies will play an essential role in maximizing the physics reach of the Large Hadron Collider. Ideally, the design of discriminating variables would be informed by analytic calculations in perturbative QCD. Unfortunately, explicit calculations are often not feasible due to the complexity of the observables used for discrimination, and so many validation studies rely heavily, and solely, on Monte Carlo. In this paper we show how methods based on the parametric power counting of the dynamics of QCD, familiar from effective theory analyses, can be used to design, understand, and make robust predictions for the behavior of jet substructure variables. As a concrete example, we apply power counting for discriminating boosted Z bosons from massive QCD jets using observables formed from the n-point energy correlation functions. We show that power counting alone gives a definite prediction for the observable that optimally separates the background-rich from the signal-rich regions of phase space. Power counting can also be used to understand effects of phase space cuts and the effect of contamination from pile-up, which we discuss. As these arguments rely only on the parametric scaling of QCD, the predictions from power counting must be reproduced by any Monte Carlo, which we verify using Pythia8 and Herwig++. We also use the example of quark versus gluon discrimination to demonstrate the limits of the power counting technique.

  17. INTEGRAL observations of Her X-1

    E-Print Network [OSTI]

    D. Klochkov; R. Staubert; K. Postnov; N. Shakura; A. Santangelo; S. Tsygankov; A. Lutovinov; I. Kreykenbohm; J. Wilms

    2008-02-08T23:59:59.000Z

    Aims: We investigate the X-ray spectral and timing properties of the accreting X-ray pulsar Her X-1 observed with the INTEGRAL satellite in July-August 2005. Methods: The data analyzed in this work cover a substantial part of one main-on state of the source. The short-time scale pulse period development is measured. X-ray pulse profiles for different energy ranges and time intervals are constructed. Pulse-averaged and pulse-phase resolved broad band X-ray spectra are studied. Spectral changes during X-ray dips are explored. Results: The X-ray pulse profiles are found to change significantly during the period of observations. For the first time a strong spinup is measured within one 35 d cycle. Spectral characteristics observed during the X-ray dips are consistent with their interpretaion as due to partial covering as has been reported by several authors. The fundamental cyclotron absorption line is firmly observed in both pulse-averaged and pulse-phase resolved X-ray spectra. The energy, width, and the depth of the line are found to vary significantly with pulse phase.

  18. Direct observation of temperature dependent magnetic domain structure of the multiferroic La{sub 0.66}Sr{sub 0.34}MnO{sub 3}/BiFeO{sub 3} bilayer system by x-ray linear dichroism- and x-ray magnetic circular dichroism-photoemission electron microscopy

    SciTech Connect (OSTI)

    Mix, C.; Finizio, S.; Jakob, G.; Kläui, M. [Institut für Physik, Johannes Gutenberg Universität Mainz, Staudingerweg 7, D-55128 Mainz (Germany); Buzzi, M.; Nolting, F. [Swiss Light Source, Paul Scherrer Institut, CH-5232 Villigen PSI (Switzerland); Kronast, F. [Helmholtz-Zentrum-Berlin für Materialien und Energie GmbH, Albert-Einstein Straße 15, D-12489 Berlin (Germany)

    2014-05-21T23:59:59.000Z

    Low-thickness La{sub 0.66}Sr{sub 0.34}MnO{sub 3} (LSMO)/BiFeO{sub 3} (BFO) thin film samples deposited on SrTiO{sub 3} were imaged by high resolution x-ray microscopy at different temperatures. The ultra-thin thickness of the top layer allows to image both the ferromagnetic domain structure of LSMO and the multiferroic domain structure of the buried BFO layer, opening a path to a direct observation of coupling at the interface on a microscopic level. By comparing the domain size and structure of the BFO and LSMO, we observed that, in contrast to LSMO single layers, LSMO/BFO multilayers show a strong temperature dependence of the ferromagnetic domain structure of the LSMO. Particularly, at 40?K, a similar domain size for BFO and LSMO is observed. This indicates a persistence of exchange coupling on the microscopic scale at a temperature, where the exchange bias as determined by magnetometer measurements is vanishing.

  19. ISO observations of four active galaxies

    E-Print Network [OSTI]

    Michel Dennefeld; Thomas Boller; Dimitra Rigopoulou; Henrik Spoon

    2003-12-12T23:59:59.000Z

    We present ISO PHOT-S spectra of four galaxies known or suspected to host a central AGN, selected from the initial Iras/Rosat sample of Boller et al. (1992). Two of them had no obvious Seyfert features in their previous optical spectra: IRAS 14201+2956, and IRAS 21582+1018. The latter was bright enough to also allow SWS observations around selected neon lines, to establish its excitation. While both PHOT-S spectra are characteristic of starburst-dominated galaxies, the neon line ratios in IRAS 21582+1018 indicate the presence of a hard excitation source. New, high-resolution, optical spectra show only a weak, broad component around Halpha, classifying now these two objects as Sey 1.9 galaxies. The two other galaxies observed are the NLS1 galaxies Mrk 359 and Mrk 1388. Their ISO spectra however do not reveal the typical, strong PAH features found in the starburst galaxies and are more like those of standard Seyferts. These results show therefore that, although IR observations were expected to be able to always reveal the presence of an active nucleus by piercing through the central obscuration, the result may be ambiguous: the broad band IR energy distribution can still be dominated by starburts located in a circumnuclear region, and the AGN appear only in specific observations (high-excitation lines in the IR, or optical spectra with better quality than classification spectra). The obscuration needs however to be patchy rather than complete, to explain the detection of the high-excitation lines or broad Balmer wings. Only high-energy observations can then establish the strength of the central AGN and the amount of extinction with certainty.

  20. APOSTLE: 11 TRANSIT OBSERVATIONS OF TrES-3b

    SciTech Connect (OSTI)

    Kundurthy, P.; Becker, A. C.; Agol, E.; Barnes, R.; Williams, B. [Astronomy Department, University of Washington, Seattle, WA 98195 (United States)] [Astronomy Department, University of Washington, Seattle, WA 98195 (United States)

    2013-02-10T23:59:59.000Z

    The Apache Point Survey of Transit Lightcurves of Exoplanets (APOSTLE) observed 11 transits of TrES-3b over two years in order to constrain system parameters and look for transit timing and depth variations. We describe an updated analysis protocol for APOSTLE data, including the reduction pipeline, transit model, and Markov Chain Monte Carlo analyzer. Our estimates of the system parameters for TrES-3b are consistent with previous estimates to within the 2{sigma} confidence level. We improved the errors (by 10%-30%) on system parameters such as the orbital inclination (i {sub orb}), impact parameter (b), and stellar density ({rho}{sub *}) compared to previous measurements. The near-grazing nature of the system, and incomplete sampling of some transits, limited our ability to place reliable uncertainties on individual transit depths and hence we do not report strong evidence for variability. Our analysis of the transit timing data shows no evidence for transit timing variations and our timing measurements are able to rule out super-Earth and gas giant companions in low-order mean motion resonance with TrES-3b.

  1. Faraday Rotation Observations of Magnetic Fields in galaxy Clusters

    E-Print Network [OSTI]

    Tracy E. Clarke

    2004-12-10T23:59:59.000Z

    The presence of magnetic fields in the intracluster medium in clusters of galaxies has been revealed through several different observational techniques. These fields may be dynamically important in clusters as they will provide additional pressure support to the intracluster medium as well as inhibit transport mechanisms such as thermal conduction. Here, we review the current observational state of Faraday rotation measure studies of the cluster fields. The fields are generally found to be a few to 10 microG in non-cooling core clusters and ordered on scales of 10-20 kpc. Studies of sources at large impact parameters show that the magnetic fields extend from cluster cores to radii of at least 500 kpc. In central regions of cooling core systems the field strengths are often somewhat higher (10-40 microG) and appear to be ordered on smaller scales of a few to 10 kpc. We also review some of the recent work on interpreting Faraday rotation measure observations through theory and numerical simulations. These techniques allow us to build up a much more detailed view of the strength and topology of the fields.

  2. Extraplanar Dust in Spiral Galaxies: Observations and Implications

    E-Print Network [OSTI]

    J. Christopher Howk

    1999-10-05T23:59:59.000Z

    Recent optical and submillimeter observations have begun to probe the existence of dust grains in the halos of spiral galaxies. I review our own work in this area which employs high-resolution optical images of edge-on spiral galaxies to trace high-z dust in absorption against the background stellar light of the galaxies. We have found that a substantial fraction of such galaxies (>50%) show extensive webs of dust-bearing clouds to heights z>2 kpc. Extraplanar dust in galaxies is statistically correlated with extraplanar diffuse ionized gas, though there is no evidence for a direct, physical relationship between these two phases of the high-z interstellar medium. The dense high-z clouds individually have masses estimated to be >10^5} to 10^6 solar masses. The detailed properties of the observed dust structures suggest the clouds seen in our images may represent the dense phase of a multiphase ISM at high-z. Such dense clouds can have an important effect on the observed light distribution in spiral galaxies. I discuss the effects such high-z dust can have on quantitative measures of the vertical structure of stars and ionized gas in edge-on systems.

  3. Observation of incomplete fusion reactions at l < l {sub crit}

    SciTech Connect (OSTI)

    Yadav, Abhishek, E-mail: abhishekyadav117@gmail.com; Sharma, Vijay R., E-mail: abhishekyadav117@gmail.com; Singh, Devendra P., E-mail: abhishekyadav117@gmail.com; Unnati,; Singh, B. P.; Prasad, R. [Department of Physics, Aligarh Muslim University, Aligarh (UP) - 202 002 (India); Singh, Pushpendra P. [GSI-Helmholtz Centre for Heavy Ion Research GmbH, D-64291 Darmstadt (Germany); Bala, Indu; Kumar, R.; Muralithar, S.; Singh, R. P. [NP-Group: Inter-University Accelerator Center, Aruna Asaf Ali Marg, New Delhi - 110 067 (India); Sharma, M. K. [Department of Physics, S. V. College, Aligarh- 202 001 (India)

    2014-08-14T23:59:59.000Z

    In order to understand the presence of incomplete fusion at low energies i.e. 4-7MeV/nucleon and also to study its dependence on various entrance-channel parameters, the two type of measurements (i) excitation function for {sup 12}C+{sup 159}Tb, and (ii) forward recoil ranges for {sup 12}C+{sup 159}Tb systems have been performed. The experimentally measured excitation functions have been analyzed within the framework of compound nucleus decay using statistical model code PACE4. Analysis of data suggests the production of xn/px)n-channels via complete fusion, as these are found to be well reproduced by PACE4 predictions, while, a significant enhancement in the excitation functions of ?-emitting channels has been observed over the theoretical ones, which has been attributed due to the incomplete fusion processes. Further, the incomplete fusion events observed in case of forward recoil range measurements have been explained on the basis of the breakup fusion model, where these events may be attributed to the fusion of {sup 8}Be and/or {sup 4}He from {sup 12}C projectile to the target nucleus. In the present work, the SUMRULE model calculations are found to highly underestimate the observed incomplete fusion cross-sections which indicate that the l-values lower than l {sub crit} (limit of complete fusion) significantly contribute to the incomplete fusion reactions.

  4. Observation of Dirac Monopoles in a Synthetic Magnetic Field

    E-Print Network [OSTI]

    M. W. Ray; E. Ruokokoski; S. Kandel; M. Möttönen; D. S. Hall

    2014-08-13T23:59:59.000Z

    Magnetic monopoles --- particles that behave as isolated north or south magnetic poles --- have been the subject of speculation since the first detailed observations of magnetism several hundred years ago. Numerous theoretical investigations and hitherto unsuccessful experimental searches have followed Dirac's 1931 development of a theory of monopoles consistent with both quantum mechanics and the gauge invariance of the electromagnetic field. The existence of even a single Dirac magnetic monopole would have far-reaching physical consequences, most famously explaining the quantization of electric charge. Although analogues of magnetic monopoles have been found in exotic spin-ices and other systems, there has been no direct experimental observation of Dirac monopoles within a medium described by a quantum field, such as superfluid helium-3. Here we demonstrate the controlled creation of Dirac monopoles in the synthetic magnetic field produced by a spinor Bose-Einstein condensate. Monopoles are identified, in both experiments and matching numerical simulations, at the termini of vortex lines within the condensate. By directly imaging such a vortex line, the presence of a monopole may be discerned from the experimental data alone. These real-space images provide conclusive and long-awaited experimental evidence of the existence of Dirac monopoles. Our result provides an unprecedented opportunity to observe and manipulate these quantum-mechanical entities in a controlled environment.

  5. Brown Dwarfs as Ejected Stellar Embryos: Observational Perspectives

    E-Print Network [OSTI]

    Bo Reipurth; Cathie Clarke

    2002-08-31T23:59:59.000Z

    We discuss a scenario in which brown dwarfs are formed like stars, except that their full collapse phases are interrupted through dynamical interactions in small multiple systems, leading to the ejection of the lightest member. This disintegration is a stochastic process, often resulting in the expulsion of newborn low mass stars, but when it occurs early enough the ejected stellar embryo will be a substellar object. This process may be so common at early ages that a large fraction of the ubiquitous brown dwarfs could have formed in this manner. Detailed gas dynamical simulations are required in order to better understand the details of the decay of small newborn multiple systems. We discuss the observational consequences of the ejection hypothesis, noting especially the importance of binaries with brown dwarf components as an observational test. Finally, we note that brown dwarfs that have recently been ejected may be so disturbed, by infall from the collapsing core and also by heavy accretion from perturbed circumstellar disks, that traditional spectral and luminosity criteria may fail to identify their substellar nature.

  6. WTERT-India Observations from India's Crisis Ranjith Annepu Observations from India's Crisis

    E-Print Network [OSTI]

    as the city could not find a new landfill site. Author Ranjith Annepu, WTERT ­ India Date February 04, 2013WTERT- India Observations from India's Crisis Ranjith Annepu Observations from India's Crisis Waste-to-Energy Research and Technology Council (WTERT) ­ India, 89-B, NEERI Mumbai Zonal Lab, Worli

  7. CAN REMOTE OBSERVING BE GOOD OBSERVING? REFLECTIONS ON PROCRUSTES AND ANTAEUS 1

    E-Print Network [OSTI]

    Groppi, Christopher

    CAN REMOTE OBSERVING BE GOOD OBSERVING? REFLECTIONS ON PROCRUSTES AND ANTAEUS 1 Felix J. Lockman 2 National Radio Astronomy Observatory 520 Edgemont Rd. Charlottesville, Va. 22903 USA ABSTRACT Remote tales of Procrustes and Antaeus. This article considers some of the human factors involved in remote

  8. Observation of Single Top Quark Production

    SciTech Connect (OSTI)

    Abazov, V.M.; /Dubna, JINR; Abbott, B.; /Oklahoma U.; Abolins, M.; /Michigan State U.; Acharya, Bannanje Sripath; /Tata Inst.; Adams, M.; /Illinois U., Chicago; Adams, T.; /Florida State U.; Aguilo, E.; /Alberta U. /Simon Fraser U. /York U., Canada /McGill U.; Ahsan, M.; /Kansas State U.; Alexeev, G.D.; /Dubna, JINR; Alkhazov, Georgiy D.; /St. Petersburg, INP; Alton, Andrew K.; /Michigan State U. /Northeastern U.

    2009-03-01T23:59:59.000Z

    We report first observation of the electroweak production of single top quarks in p{bar p} collisions at {radical}s = 1.96 TeV based on 2.3 fb{sup ?1} of data collected by the D0 detector at the Fermilab Tevatron Collider. Using events containing an isolated electron or muon and missing transverse energy, together with jets originating from the fragmentation of b quarks, we measure a cross section of {sigma}(p{bar p} {yields} tb + X, tqb + X) = 3.94 {+-} 0.88 pb. The probability to measure a cross section at this value or higher in the absence of signal is 2.5 x 10{sup ?7}, corresponding to a 5.0 standard deviation significance for the observation.

  9. Fermi Observations of Gamma-ray Bursts

    SciTech Connect (OSTI)

    Ohno, Masanori [Institute of Space and Astronautical Science, JAXA, 3-1-1 Yoshinodai, Chuo-ku, Sagamihara, Kanagawa 252-5210 (Japan)

    2010-10-15T23:59:59.000Z

    The gamma-ray emission mechanism of Gamma-ray bursts (GRBs) are still unknown. Fermi Gamma-ray Space Telescope successfully detected high-energy (> 100 MeV) emission from 17 GRBs since its launch. Fermi revealed the distinct temporal behaviors and extra spectral component from high-energy emission. These new observational results are driving many theoretical implications, such as leptonic, hadronic and afterglow origin. The highest energy photon detected by Fermi gives a constraint on the bulk Lorentz factor of the ultra-relativistic jets of GRBs. The impact of the Fermi GRB observations extends not only to the GRB-related issues but also to the outside GRB physics, such as quantum gravity and model of the extra galactic background light.

  10. Electron Cloud observation in the LHC

    E-Print Network [OSTI]

    Rumolo, G; Baglin, V; Bartosik, H; Biancacci, N; Baudrenghien, P; Bregliozzi, G; Chiggiato, P; Claudet, S; De Maria, R; Esteban-Muller, J; Favier, M; Hansen, C; Höfle, W; Jimenez, J M; Kain, V; Lanza, G; Li, K S B; Maury Cuna, G H I; Métral, E; Papotti, G; Pieloni, T; Roncarolo, F; Salvant, B; Shaposhnikova, E N; Steinhagen, R J; Tavian, L J; Valuch, D; Venturini Delsolaro, W; Zimmermann, F; Iriso, U; Dominguez, O; Koukovini-Platia, E; Mounet, N; Zannini, C; Bhat, C M

    2011-01-01T23:59:59.000Z

    Operation of LHC with bunch trains at different spacings has revealed the formation of an electron cloud inside the machine. The main observations of electron cloud build up are the pressure rise measured at the vacuum gauges in the warm regions, as well as the increase of the beam screen temperature in the cold regions due to an additional heat load. The effects of the electron cloud were also visible as instability and emittance growth affecting the last bunches of longer trains, which could be improved running with higher chromaticity or larger transverse emittances. A summary of the 2010 and 2011 observations and measurements and a comparison with models will be presented. The efficiency of scrubbing to improve the machine running performance will be briefly discussed.

  11. Observational constraints on braneworld chaotic inflation

    E-Print Network [OSTI]

    Andrew R Liddle; Anthony J Smith

    2003-08-13T23:59:59.000Z

    We examine observational constraints on chaotic inflation models in the Randall-Sundrum Type II braneworld. If inflation takes place in the high-energy regime, the perturbations produced by the quadratic potential are further from scale-invariance than in the standard cosmology, in the quartic case more or less unchanged, while for potentials of greater exponent the trend is reversed. We test these predictions against a data compilation including the WMAP measurements of microwave anisotropies and the 2dF galaxy power spectrum. While in the standard cosmology the quartic potential is at the border of what the data allow and all higher powers excluded, we find that in the high-energy regime of braneworld inflation even the quadratic case is under strong observational pressure. We also investigate the intermediate regime where the brane tension is comparable to the inflationary energy scale, where the deviations from scale-invariance prove to be greater.

  12. Constraining the Braneworld with Gravitational Wave Observations

    SciTech Connect (OSTI)

    McWilliams, Sean T. [Gravitational Astrophysics Laboratory, NASA Goddard Space Flight Center, 8800 Greenbelt Road, Greenbelt Maryland 20771 (United States)

    2010-04-09T23:59:59.000Z

    Some braneworld models may have observable consequences that, if detected, would validate a requisite element of string theory. In the infinite Randall-Sundrum model (RS2), the AdS radius of curvature, l, of the extra dimension supports a single bound state of the massless graviton on the brane, thereby reproducing Newtonian gravity in the weak-field limit. However, using the AdS/CFT correspondence, it has been suggested that one possible consequence of RS2 is an enormous increase in Hawking radiation emitted by black holes. We utilize this possibility to derive two novel methods for constraining l via gravitational wave measurements. We show that the EMRI event rate detected by LISA can constrain l at the {approx}1 {mu}m level for optimal cases, while the observation of a single galactic black hole binary with LISA results in an optimal constraint of l{<=}5 {mu}m.

  13. SALT observations of southern post-novae

    E-Print Network [OSTI]

    Tomov, T; Mikolajewski, M; Ilkiewicz, K

    2015-01-01T23:59:59.000Z

    We report on recent optical observations of the stellar and the nebular remnants of 22 southern post-novae. In this study, for each of our targets, we obtained and analysed long-slit spectra in the spectral range 3500-6600 A and in H$\\alpha$+NII narrow-band images. The changes in the emission lines' equivalent widths with the time since the outburst agree with earlier published results of other authors. We estimated an average value $\\alpha$=2.37 for the exponent of the power law fitted to the post-novae continua. Our observations clearly show the two-component structure of the V842 Cen expanding nebulae, owing to the different velocities of the ejected matter. We discovered an expanding shell around V382 Vel with an outer diameter of about 12 arcsec.

  14. First direct observation of muon antineutrino disappearance

    DOE Public Access Gateway for Energy & Science Beta (PAGES Beta)

    Adamson, P [Fermilab; Andreopoulos, C [Rutherford; Auty, D J [Sussex U.; Ayres, D S [Argonne; Backhouse, C [Oxford U.; Barr, G [Oxford U.; Bishai, M [Brookhaven; Blake, A [Cambridge U.; Bock, G J [Fermilab; Boehnlein, D J [/Fermilab; Bogert, D [Fermilab; Harvard U., Phys. Dept.

    2011-07-05T23:59:59.000Z

    This letter reports the first direct observation of muon antineutrino disappearance. The MINOS experiment has taken data with an accelerator beam optimized for ??? production, accumulating an exposure of 1.71 x 1020 protons on target. In the Far Detector, 97 charged current ??? events are observed. The no-oscillation hypothesis predicts 156 events and is excluded at 6.3?. The best fit to oscillation yields |?m?2| = (3.36-0.40 +0.46(stat.) ± 0.06(syst.)) x 10-3 eV2, sin2(2 ??) = 0.86-0.12+0.11 (stat.) ± 0.01(syst.). The MINOS ?? and ??? measurements are consistent at the 2.0% confidence level, assuming identical underlying oscillation parameters.

  15. RHESSI and SphinX Common Observations

    E-Print Network [OSTI]

    Mrozek, Tomasz

    ) energy range: 3-8 keV (16 energy bands, E=0.3 keV) #12;Fluxes comparison SphinX DRM conversion factors possible. In 2009 we had three instruments that observed the Sun in similar energy band: SphinX, RHESSI, design & manufacture - energy range: 1.2 ­ 15 keV - time resolution: ~0.00001 s - sensitivity: 100x

  16. LNG Observer: Second Qatargas train goes onstream

    SciTech Connect (OSTI)

    NONE

    1997-01-01T23:59:59.000Z

    The January-February, 1997 issue of the LNG Observer is presented. The following topics are discussed: second Qatargas train goes onstream; financing for the eighth Indonesian liquefaction train; Koreans take stakes in Oman LNG; US imports and exports of LNG in 1996; A 60% increase in proved reserves on the North West Shelf; proposals for Indian LNG terminal CEDIGAZ forecasts world LNG trade by 2010; growth for North African gas production and exports; and new forecast sees strong growth for Asian gas.

  17. Posters Ground-Based Radiometric Observations

    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 forPortsmouth/Paducah Project Office PressPostdoctoraldecadal observations719 Posters117

  18. Correlation between model observer and human observer performance in CT imaging when lesion location is uncertain

    SciTech Connect (OSTI)

    Leng, Shuai; Yu, Lifeng; Zhang, Yi; McCollough, Cynthia H. [Department of Radiology, Mayo Clinic, 200 First Street Southwest, Rochester, Minnesota 55905 (United States)] [Department of Radiology, Mayo Clinic, 200 First Street Southwest, Rochester, Minnesota 55905 (United States); Carter, Rickey [Department of Biostatistics, Mayo Clinic, 200 First Street Southwest, Rochester, Minnesota 55905 (United States)] [Department of Biostatistics, Mayo Clinic, 200 First Street Southwest, Rochester, Minnesota 55905 (United States); Toledano, Alicia Y. [Biostatistics Consulting, LLC, 10606 Wheatley Street, Kensington, Maryland 20895 (United States)] [Biostatistics Consulting, LLC, 10606 Wheatley Street, Kensington, Maryland 20895 (United States)

    2013-08-15T23:59:59.000Z

    Purpose: The purpose of this study was to investigate the correlation between model observer and human observer performance in CT imaging for the task of lesion detection and localization when the lesion location is uncertain.Methods: Two cylindrical rods (3-mm and 5-mm diameters) were placed in a 35 × 26 cm torso-shaped water phantom to simulate lesions with ?15 HU contrast at 120 kV. The phantom was scanned 100 times on a 128-slice CT scanner at each of four dose levels (CTDIvol = 5.7, 11.4, 17.1, and 22.8 mGy). Regions of interest (ROIs) around each lesion were extracted to generate images with signal-present, with each ROI containing 128 × 128 pixels. Corresponding ROIs of signal-absent images were generated from images without lesion mimicking rods. The location of the lesion (rod) in each ROI was randomly distributed by moving the ROIs around each lesion. Human observer studies were performed by having three trained observers identify the presence or absence of lesions, indicating the lesion location in each image and scoring confidence for the detection task on a 6-point scale. The same image data were analyzed using a channelized Hotelling model observer (CHO) with Gabor channels. Internal noise was added to the decision variables for the model observer study. Area under the curve (AUC) of ROC and localization ROC (LROC) curves were calculated using a nonparametric approach. The Spearman's rank order correlation between the average performance of the human observers and the model observer performance was calculated for the AUC of both ROC and LROC curves for both the 3- and 5-mm diameter lesions.Results: In both ROC and LROC analyses, AUC values for the model observer agreed well with the average values across the three human observers. The Spearman's rank order correlation values for both ROC and LROC analyses for both the 3- and 5-mm diameter lesions were all 1.0, indicating perfect rank ordering agreement of the figures of merit (AUC) between the average performance of the human observers and the model observer performance.Conclusions: In CT imaging of different sizes of low-contrast lesions (?15 HU), the performance of CHO with Gabor channels was highly correlated with human observer performance for the detection and localization tasks with uncertain lesion location in CT imaging at four clinically relevant dose levels. This suggests the ability of Gabor CHO model observers to meaningfully assess CT image quality for the purpose of optimizing scan protocols and radiation dose levels in detection and localization tasks for low-contrast lesions.

  19. Library System Library System

    E-Print Network [OSTI]

    Cinabro, David

    Library System #12;Library System 5150 Anthony Wayne Drive David Adamany Undergraduate Library that for the current fiscal year, we've been given an additional $600,000 for our library materials budget. We're very subscriptions. The Wayne State University Libraries are deeply committed to providing our faculty and students

  20. MICRO-CHP System for Residential Applications

    SciTech Connect (OSTI)

    Joseph Gerstmann

    2009-01-31T23:59:59.000Z

    This is the final report of progress under Phase I of a project to develop and commercialize a micro-CHP system for residential applications that provides electrical power, heating, and cooling for the home. This is the first phase of a three-phase effort in which the residential micro-CHP system will be designed (Phase I), developed and tested in the laboratory (Phase II); and further developed and field tested (Phase III). The project team consists of Advanced Mechanical Technology, Inc. (AMTI), responsible for system design and integration; Marathon Engine Systems, Inc. (MES), responsible for design of the engine-generator subsystem; AO Smith, responsible for design of the thermal storage and water heating subsystems; Trane, a business of American Standard Companies, responsible for design of the HVAC subsystem; and AirXchange, Inc., responsible for design of the mechanical ventilation and dehumidification subsystem.