Sample records for afterburn energy release

  1. Building an Efficient Model for Afterburn Energy Release

    DOE Office of Scientific and Technical Information (OSTI.GOV)

    Alves, S; Kuhl, A; Najjar, F

    2012-02-03

    Many explosives will release additional energy after detonation as the detonation products mix with the ambient environment. This additional energy release, referred to as afterburn, is due to combustion of undetonated fuel with ambient oxygen. While the detonation energy release occurs on a time scale of microseconds, the afterburn energy release occurs on a time scale of milliseconds with a potentially varying energy release rate depending upon the local temperature and pressure. This afterburn energy release is not accounted for in typical equations of state, such as the Jones-Wilkins-Lee (JWL) model, used for modeling the detonation of explosives. Here wemore » construct a straightforward and efficient approach, based on experiments and theory, to account for this additional energy release in a way that is tractable for large finite element fluid-structure problems. Barometric calorimeter experiments have been executed in both nitrogen and air environments to investigate the characteristics of afterburn for C-4 and other materials. These tests, which provide pressure time histories, along with theoretical and analytical solutions provide an engineering basis for modeling afterburn with numerical hydrocodes. It is toward this end that we have constructed a modified JWL equation of state to account for afterburn effects on the response of structures to blast. The modified equation of state includes a two phase afterburn energy release to represent variations in the energy release rate and an afterburn energy cutoff to account for partial reaction of the undetonated fuel.« less

  2. Numerical models for afterburning of TNT detonation products in air

    NASA Astrophysics Data System (ADS)

    Donahue, L.; Zhang, F.; Ripley, R. C.

    2013-11-01

    Afterburning occurs when fuel-rich explosive detonation products react with oxygen in the surrounding atmosphere. This energy release can further contribute to the air blast, resulting in a more severe explosion hazard particularly in confined scenarios. The primary objective of this study was to investigate the influence of the products equation of state (EOS) on the prediction of the efficiency of trinitrotoluene (TNT) afterburning and the times of arrival of reverberating shock waves in a closed chamber. A new EOS is proposed, denoted the Afterburning (AB) EOS. This EOS employs the JWL EOS in the high pressure regime, transitioning to a Variable-Gamma (VG) EOS at lower pressures. Simulations of three TNT charges suspended in a explosion chamber were performed. When compared to numerical results using existing methods, it was determined that the Afterburning EOS delays the shock arrival times giving better agreement with the experimental measurements in the early to mid time. In the late time, the Afterburning EOS roughly halved the error between the experimental measurements and results obtained using existing methods. Use of the Afterburning EOS for products with the Variable-Gamma EOS for the surrounding air further significantly improved results, both in the transient solution and the quasi-static pressure. This final combination of EOS and mixture model is recommended for future studies involving afterburning explosives, particularly those in partial and full confinement.

  3. Post-Detonation Energy Release from TNT-Aluminum Explosives

    NASA Astrophysics Data System (ADS)

    Zhang, Fan; Anderson, John; Yoshinaka, Akio

    2007-06-01

    Detonation and post-detonation energy release from TNT and TNT-aluminum composite have been experimentally studied in an air-filled chamber, 26 m^3 in volume and 3 m in diameter. While TNT has a high oxygen deficiency, experiments with 1.1 kg to 4 kg charges yield energy releases reaching only 86% of theoretical equilibrium values, possibly due to the non-uniform mixing between the detonation products and air. In order to improve mixing and further increase afterburning energy, large mass fractions of large aluminum particles are combined with TNT. The effect of particle distribution is also investigated in two composite configurations, whereby the aluminum particles are uniformly mixed in cast TNT or arranged in a shell surrounding a TNT cylinder. It is shown that the TNT-aluminum composite outperforms pure TNT, while improved performance is achieved for the shell configuration due to enhanced spatial mixing of hot fuels with oxidizing gases. Comparisons with the equilibrium theory and a liquid-based aluminized composite explosive (with an oxygen deficiency less than that of TNT) are conducted to further explore the mixing and afterburning mechanism.

  4. Investigation of Noise Field and Velocity Profiles of an Afterburning Engine

    NASA Technical Reports Server (NTRS)

    North, Warren J.; Callaghan, E. E.; Lanzo, C. D.

    1954-01-01

    Sound pressure levels, frequency spectrum, and jet velocity profiles are presented for an engine-afterburner combination at various values of afterburner fuel - air ratio. At the high fuel-air ratios, severe low-frequency resonance was encountered which represented more than half the total energy in the sound spectrum. At similar thrust conditions, lower sound pressure levels were obtained from a current fighter air craft with a different afterburner configuration. The lower sound pressure levels are attributed to resonance-free afterburner operation and thereby indicate the importance of acoustic considerations in afterburner design.

  5. Post-Detonation Energy Release from Tnt-Aluminum Explosives

    NASA Astrophysics Data System (ADS)

    Zhang, Fan; Anderson, John; Yoshinaka, Akio

    2007-12-01

    TNT and TNT-aluminum composites were experimentally studied in an air-filled 26 m3 chamber for charge masses ranging from 1.1 to 4 kg. Large aluminum mass fractions (35 to 50%wt.) and particle sizes (36 μm) were combined with TNT in two configurations, whereby the aluminum particles were uniformly mixed in cast TNT or arranged into a shell surrounding a cast TNT cylinder. The results show that improved performance is achieved for the shell configuration versus the mixed version during the early afterburning phase (10-40 ms), while both approach the same quasi-static explosion overpressure (QSP) after a long duration. The QSP ratios with respect to TNT in nitrogen are in good agreement with equilibrium predictions. Thus, the large aluminum mass fraction improves spatial mixing of hot fuels with oxidizing gases in the detonation products and chamber air, resulting in more efficient afterburning energy release.

  6. Thermal imaging of afterburning plumes

    NASA Astrophysics Data System (ADS)

    Ajdari, E.; Gutmark, E.; Parr, T. P.; Wilson, K. J.; Schadow, K. C.

    1989-01-01

    Afterburning and nonafterburning exhaust plumes were studied experimentally for underexpanded sonic and supersonic conical circular nozzles. The plume structure was visualized using thermal imaging camera and regular photography. IR emission by the plume is mainly dependent on the presence of afterburning. Temperature and reducing power of the exhaust gases, in addition to the nozzle configuration, determine the structure of the plume core, the location where the afterburning is initiated, its size and intensity. Comparison between single shot and average thermal images of the plume show that afterburning is a highly turbulent combustion process.

  7. Thermodynamic Model of Afterburning in Explosions

    DOE Office of Scientific and Technical Information (OSTI.GOV)

    Kuhl, A L; Howard, M; Fried, L

    2003-04-23

    Thermodynamic states encountered during afterburning of explosion products gases in air were analyzed with the Cheetah code. Results are displayed in the form of Le Chatelier diagrams: the locus of states of specific internal energy versus temperature, for six different condensed explosives charges. Accuracy of the results was confirmed by comparing the fuel and products curves with the heats of detonation and combustion, and species composition as measured in bomb calorimeter experiments. Results were fit with analytic functions u = f ( T ) suitable for specifying the thermodynamic properties required for gas-dynamic models of afterburning in explosions.

  8. Measurement of Afterburning Effect of Underoxidized Explosives by Underwater Explosion Method

    NASA Astrophysics Data System (ADS)

    Cao, Wei; He, Zhongqi; Chen, Wanghua

    2015-04-01

    The afterburning effect of TNT and a desensitized hexogen RDX-Al explosive was studied in a defined gas volume under water. A double-layer container (DLC) filled with different gases (air, oxygen, and nitrogen) was used to control and distinguish the afterburning effect of explosives. After the charges in the DLC were initiated under water, the shock wave signals were collected and analyzed. It is shown that shock wave peak pressures are duly in compliance with explosion similarity law, pressure, and impulse histories for explosions in oxygen and air are greater than those recorded for explosions in nitrogen due to the afterburing reaction. Moreover, the afterburning energy was calculated. Results show that even though there is excess oxygen in the gas volume, the afterburning energy may not reach the theoretically maximum value. This result is different from that in confined explosion, where the presence of excess oxygen in the compressed gas filling a bomb leads to complete combustion of the detonation products.

  9. Simulating Afterburn with LLNL Hydrocodes

    DOE Office of Scientific and Technical Information (OSTI.GOV)

    Daily, L D

    2004-06-11

    Presented here is a working methodology for adapting a Lawrence Livermore National Laboratory (LLNL) developed hydrocode, ALE3D, to simulate weapon damage effects when afterburn is a consideration in the blast propagation. Experiments have shown that afterburn is of great consequence in enclosed environments (i.e. bomb in tunnel scenario, penetrating conventional munition in a bunker, or satchel charge placed in a deep underground facility). This empirical energy deposition methodology simulates the anticipated addition of kinetic energy that has been demonstrated by experiment (Kuhl, et. al. 1998), without explicitly solving the chemistry, or resolving the mesh to capture small-scale vorticity. This effortmore » is intended to complement the existing capability of either coupling ALE3D blast simulations with DYNA3D or performing fully coupled ALE3D simulations to predict building or component failure, for applications in National Security offensive strike planning as well as Homeland Defense infrastructure protection.« less

  10. A method for aircraft afterburner combustion without flameholders

    NASA Astrophysics Data System (ADS)

    Birmaher, Shai

    2009-12-01

    State of the art aircraft afterburners employ spray bars to inject fuel and flameholders to stabilize the combustion process. Such afterburner designs significantly increase the length (and thus weight), pressure losses, and observability of the engine. This thesis presents a feasibility study of a compact 'prime and trigger' (PAT) afterburner concept that eliminates the fuel spray bars and flameholders and, thus, eliminates the above-mentioned problems. In this concept, afterburner fuel is injected just upstream or in between the turbine stages. As the fuel travels through the turbine stages, it evaporates, mixes with the bulk flow, and undergoes some chemical reactions without any significant heat release, a process referred to as 'priming'. Downstream of the turbine stages, combustion could take place through autoignition. However, if fuel autoignition does not occur or if autoignition does not produce a combustion zone that is stable and highly efficient, then a low power pilot, or 'trigger', can be used to control the combustion process. The envisioned trigger for the PAT concept is a jet of product gas from ultra-rich hydrocarbon/air combustion that is injected through the afterburner liner. This 'partial oxidation' (POx) gas, which consists mostly of H2, CO, and diluents, rapidly produces radicals and heat that accelerate the autoignition of the primed mixture and, thus, provide an anchor point for the afterburner combustion process. The objective of this research was to demonstrate the feasibility of the PAT concept by showing that (1) combustion of fuel injected within or upstream of turbine stages can occur only downstream of the turbine stages, and (2) the combustion zone is compact, stable and efficient. This was accomplished using two experimental facilities, a developed theoretical model, and Chemkin simulations. The first facility, termed the Afterburner Facility (AF), simulated the bulk flow temperature, velocity and O2 content through a turbojet

  11. Noise of High-Performance Aircraft at Afterburner

    DTIC Science & Technology

    2015-03-30

    Quarterly progress report 3. DATES COVERED (From - To) 12-15-2014 to 04-03-2015 4. TITLE AND SUBTITLE Noise of High-Performance Aircraft at Afterburner ...generation of a high- performance aircraft operating at afterburner condition. The new noise components are indirect combustion noise produced by the...spectrum is reported 15. SUBJECT TERMS Jet noise at afterburner 16. SECURITY CLASSIFICATION OF: a. REPORT u b. ABSTRACT u c. THIS PAGE u 17

  12. Noise of High-Performance Aircraft at Afterburner

    DTIC Science & Technology

    2015-07-11

    Title : Noise of High-Performance Aircraft at Afterburner Principal Investigator Dr. Christopher Tarn Department of Mathematics Florida State...jet. We found that at intermediate power, the dominant noise components are essentially the same as those of a laboratory jet. However, at afterburner ...useful. The power settings are 80N2 (low power), Mil (military power) and MaxAB ( afterburner ). BII8 BI16 2__Q_il_Q_£l Bill l« C0O3 12 ^ COOS

  13. Noise of High-Performance Aircraft at Afterburner

    DTIC Science & Technology

    2015-10-07

    Naval Research Project Title : Noise of High-Performance Aircraft at Afterburner Principal Investigator Dr. Christopher Tam Department...to 08/14/2015 Noise of High-Performance Aircraft at Afterburner Tam, Christopher Sponsored Research Administratiion Florida State University

  14. Numerical study of combustion processes in afterburners

    NASA Technical Reports Server (NTRS)

    Zhou, Xiaoqing; Zhang, Xiaochun

    1986-01-01

    Mathematical models and numerical methods are presented for computer modeling of aeroengine afterburners. A computer code GEMCHIP is described briefly. The algorithms SIMPLER, for gas flow predictions, and DROPLET, for droplet flow calculations, are incorporated in this code. The block correction technique is adopted to facilitate convergence. The method of handling irregular shapes of combustors and flameholders is described. The predicted results for a low-bypass-ratio turbofan afterburner in the cases of gaseous combustion and multiphase spray combustion are provided and analyzed, and engineering guides for afterburner optimization are presented.

  15. Simulated afterburner performance with hydrogen peroxide injection for thrust augmentation

    NASA Technical Reports Server (NTRS)

    Metzler, Allen J; Grobman, Jack S

    1956-01-01

    Combustion performance of three afterburner configurations was evaluated at simulated altitude flight conditions with liquid augmentation to the primary combustor. Afterburner combustion efficiency and stability were better with injection of high-strength hydrogen peroxide than with no injection or with water injection. Improvements were observed in afterburner configurations with and without flameholders and in a short-length afterburner. At a peroxide-air ratio of 0.3, combustion was stable and 85 to 90 percent efficient in all configurations tested. Calculated augmented net-thrust ratios for peroxide injection with afterburning were approximately 60 percent greater than those for water injection.

  16. Countercurrent flow afterburner

    DOEpatents

    Leggett, Ronald L.; Presse, Donald E.; Smith, Carl J.; Teter, Alton R.

    1976-01-01

    Afterburner apparatus for receiving from an incinerator products of combustion and distributing them through a domed distributor in counterflow manner throughout a housing, in opposition to a stream of combustible gas.

  17. Turbulent Mixing and Afterburn in Post-Detonation Flow with Dense Particle Clouds

    NASA Astrophysics Data System (ADS)

    Menon, Suresh

    2015-06-01

    Reactive metal particles are used as additives in most explosives to enhance afterburn and augment the impact of the explosive. The afterburn is highly dependent on the particle dispersal and mixing in the post-detonation flow. The post-detonation flow is generally characterized by hydrodynamic instabilities emanating from the interaction of the blast waves with the detonation product gases and the ambient air. Further, influenced by the particles, the flow evolves and develops turbulent structures, which play vital role in determining mixing and combustion. Past studies in the field in open literature are reviewed along with some recent studies conducted using three dimensional numerical simulations of particle dispersal and combustion in the post-detonation flow. Spherical nitromethane charges enveloped by particle shells of varying thickness are considered along with dense loading effects. In dense flows, the particles block the flow of the gases and therefore, the role of the inter-particle interactions on particle dispersal cannot be ignored. Thus, both dense and dilute effects must be modeled simultaneously to simulate the post-detonation flow. A hybrid equation of state is employed to study the evolution of flow from detonation initiation till the late time mixing and afterburn. The particle dispersal pattern in each case is compared with the available experimental results. The burn rate and the energy release in each case is quantified and the effect of total mass of the particles and the particle size is analyzed in detail. Strengths and limitations of the various methods used for such studies as well as the uncertainties in the modeling strategies are also highlighted. Supported by Defense Threat Reduction Agency.

  18. Altitude Performance of Modified J71 Afterburner with Revised Engine Operating Conditions

    NASA Technical Reports Server (NTRS)

    Useller, James W.; Russey, Robert E.

    1955-01-01

    An investigation was conducted in an altitude test chamber at the NACA Lewis laboratory to determine the effect of a revision of the rated engine operating conditions and modifications to the afterburner fue1 system, flameholder, and shell cooling on the augmented performance of the J71-A-2 (x-29) turbo jet engine operating at altitude . The afterburner modifications were made by the manufacturer to improve the endurance at sea-level, high-pressure conditions and to reduce the afterburner shell temperatures. The engine operating conditions of rated rotational speed and turbine-outlet gas temperature were increased. Data were obtained at conditions simulating flight at a Mach number of 0.9 and at altitudes from 40,000 to 60,000 feet. The afterburner modifications caused a reduction in afterburner combustion efficiency. The increase in rated engine speed and turbine-outlet temperature coupled with the afterburner modifications resulted in the over-all thrust of the engine and afterburner being unchanged at a given afterburner equivalence ratio, while the specific fuel consumption was increased slightly. A moderate shift in the range of equivalence ratios over which the afterburner would operate was encountered, but the maximum operable altitude remained unaltered. The afterburner-shell temperatures were also slightly reduced because of the modifications to the afterburner.

  19. Abatement of N{sub 2}O emissions from circulating fluidized bed combustion through afterburning

    DOE Office of Scientific and Technical Information (OSTI.GOV)

    Gustavsson, L.; Leckner, B.

    1995-04-01

    A method for the abatement of N{sub 2}O emission from fluidized bed combustion has been investigated. The method consists of burning a secondary fuel after the normal circulating fluidized bed combustor. Liquefied petroleum gas (LPG), fuel oil, pulverized coal, and wood, as well as sawdust, were used as the secondary fuel. Experiments showed that the N{sub 2}O emission can be reduced by 90% or more by this technique. The resulting N{sub 2}O emission was principally a function of the gas temperature achieved in the afterburner and independent of afterburning fuel, but the amount of air in the combustion gases frommore » the primary combustion also influences the results. No negative effects on sulfur capture or on NO or CO emissions were recorded. In the experiments, the primary cyclone of the fluidized bed boiler was used for afterburning. If afterburning is implemented in a plant optimized for this purpose, an amount of secondary fuel corresponding to 10% of the total energy input should remove practically all N{sub 2}O. During the present experiments the secondary fuel consumption was greater than 10% of the total energy input due to various losses.« less

  20. Effects of plume afterburning on infrared spectroscopy

    NASA Astrophysics Data System (ADS)

    Zhu, Xijuan; Xu, Ying; Ma, Jing; Duan, Ran; Wu, Jie

    2017-10-01

    Contains H2, CO and unburned components of high-temperature plume of rocket engine, then injected into the atmosphere, continue to carry out the oxidation reaction in the plume near field region with the volume in the plume of oxygen in the air, two times burning. The afterburning is an important cause of infrared radiation intensification of propellant plume, which increases the temperature of the flame and changes the components of the gas, thus enhancing the infrared radiation intensity of the flame. [1]. Two the combustion numerical using chemical reaction mechanism involving HO2 intermediate reaction, the study confirmed that HO2 is a key intermediate, plays a decisive role to trigger early response, on afterburning temperature and flow concentration distribution effect. A finite rate chemical reaction model is used to describe the two burning phenomenon in high temperature plume[2]. In this paper, a numerical simulation of the flame flow field and radiative transfer is carried out for the afterburning phenomenon. The effects of afterburning on the composition, temperature and infrared radiation of the plume are obtained by comparison.

  1. Effect of Operating Conditions and Design on Afterburner Performance

    NASA Technical Reports Server (NTRS)

    Fleming, W. A.; Gabriel, D. S.; Lundin, B. T.

    1956-01-01

    Afterburners for turbojet engines have, within the past decade, found increasing application in service aircraft. Practically all engines manufactured today are equipped with some form of afterburner, and its use has increased from what was originally a short-period thrust-augmentation application to an essential feature of the turbojet propulsion system for flight at supersonic speeds. The design of these afterburners has been based on extensive research and development effort in expanded laboratory facilities by both the NACA and the American engine industry. Most of the work of the engine industry, however, has either not been published or is not generally available owing to its proprietary nature. Consequently, the main bulk of research information available for summary and discussion is of NACA origin. However, because industrial afterburner development has closely followed NACA research, the omission is more one of technical detail than method or concept. One principal difficulty encountered in summarizing the work in this field is that sufficient knowledge does not yet exist to rationally or directly integrate the available background of basic combustion principles into combustor design. A further difficulty is that most of the experimental investigations that have been conducted were directed chiefly toward the development of specific afterburners for various engines rather than to the accumulation of systematic data. This work has, nonetheless, provided not only substantial improvements in the performance of afterburners but also a large fund of experimental data and an extensive background of experience in the field. Consequently, it is the purpose of the present chapter to summarize the many, and frequently unrelated, experimental investigations that have been conducted rather than to formulate a set of design rules. In the treatment of this material an effort has been made, however, to convey to the reader the "know how" acquired by research engineers

  2. Active chlorine and nitric oxide formation from chemical rocket plume afterburning

    NASA Astrophysics Data System (ADS)

    Leone, D. M.; Turns, S. R.

    Chlorine and oxides of nitrogen (NO(x)) released into the atmosphere contribute to acid rain (ground level or low-altitude sources) and ozone depletion from the stratosphere (high-altitude sources). Rocket engines have the potential for forming or activating these pollutants in the rocket plume. For instance, H2/O2 rockets can produce thermal NO(x) in their plumes. Emphasis, in the past, has been placed on determining the impact of chlorine release on the stratosphere. To date, very little, if any, information is available to understand what contribution NO(x) emissions from ground-based engine testing and actual rocket launches have on the atmosphere. The goal of this work is to estimate the afterburning emissions from chemical rocket plumes and determine their local stratospheric impact. Our study focuses on the space shuttle rocket motors, which include both the solid rocket boosters (SRB's) and the liquid propellant main engines (SSME's). Rocket plume afterburning is modeled employing a one-dimensional model incorporating two chemical kinetic systems: chemical and thermal equilibria with overlayed nitric oxide chemical kinetics (semi equilibrium) and full finite-rate chemical kinetics. Additionally, the local atmospheric impact immediately following a launch is modeled as the emissions diffuse and chemically react in the stratosphere.

  3. Active chlorine and nitric oxide formation from chemical rocket plume afterburning

    NASA Technical Reports Server (NTRS)

    Leone, D. M.; Turns, S. R.

    1994-01-01

    Chlorine and oxides of nitrogen (NO(x)) released into the atmosphere contribute to acid rain (ground level or low-altitude sources) and ozone depletion from the stratosphere (high-altitude sources). Rocket engines have the potential for forming or activating these pollutants in the rocket plume. For instance, H2/O2 rockets can produce thermal NO(x) in their plumes. Emphasis, in the past, has been placed on determining the impact of chlorine release on the stratosphere. To date, very little, if any, information is available to understand what contribution NO(x) emissions from ground-based engine testing and actual rocket launches have on the atmosphere. The goal of this work is to estimate the afterburning emissions from chemical rocket plumes and determine their local stratospheric impact. Our study focuses on the space shuttle rocket motors, which include both the solid rocket boosters (SRB's) and the liquid propellant main engines (SSME's). Rocket plume afterburning is modeled employing a one-dimensional model incorporating two chemical kinetic systems: chemical and thermal equilibria with overlayed nitric oxide chemical kinetics (semi equilibrium) and full finite-rate chemical kinetics. Additionally, the local atmospheric impact immediately following a launch is modeled as the emissions diffuse and chemically react in the stratosphere.

  4. Summary of NACA Research on Afterburners for Turbojet Engines

    NASA Technical Reports Server (NTRS)

    Lundin, Bruce T; Gabriel, David S; Fleming, William A

    1956-01-01

    NACA research on afterburners for turbojet engines during the past 5 years is summarized. Although most of this work has been directed toward the development of specific afterburners for various engines rather than toward the accumulation of systematic data, it has, nevertheless, provided a large fund of experimental data and experience in the field. The references cited present over 1000 afterburner configurations and some 3500 hours of operation. In the treatment of the material of this summary, the principal effort has been to convey to the reader the "know-how" acquired by research engineers in the course of the work rather than to formulate a set of design rules.

  5. Measurement of gaseous emissions from an afterburning turbojet engine at simulated altitude conditions

    NASA Technical Reports Server (NTRS)

    Diehl, L. A.

    1973-01-01

    Gaseous emissions from a J85-GE-13 turbojet engine were measured over a range of fuel-air ratios from idle to full afterburning and simulated altitudes from near sea-level to 12,800 meters (42,000 ft). Without afterburning, carbon monoxide and unburned hydrocarbon emissions were highest at idle and lowest at takeoff; oxides of nitrogen exhibited the reverse trend. With afterburning, carbon monoxide and unburned hydrocarbon emissions were greater than for military power. Carbon monoxide emissions were altitude dependent. Oxides of nitrogen emissions were less at minimum afterburning than at military power. For power levels above minimum afterburning, the oxides of nitrogen emissions were both power level and altitude dependent.

  6. Process of afterburning combustible constituents of exhaust gases from rotary kilns

    DOE Office of Scientific and Technical Information (OSTI.GOV)

    Schnabel, W.; Scheu, E.; Serbent, H.

    1984-03-13

    In order to avoid incrustation and an excessively strong thermal attack on the afterburning chamber, the exhaust gases which contain gaseous and solid constituents which are combustible are afterburned in a plurality of stages, which are connected in series. The rate at which oxygen is supplied to each stage is so controlled that part of the combustible constituents is afterburned in each stage. The gas which is about to enter each succeeding stage is cooled by injected water.

  7. Foamed-metal-based catalytic afterburners in automotive exhaust systems

    DOE Office of Scientific and Technical Information (OSTI.GOV)

    Pestryakov, A.N.; Ametov, V.A.

    1994-08-10

    Properties of exhaust afterburning catalysts based on porous cellular materials (foamed metals) have been investigated. Catalysts containing oxides of base metals provide a two-to-threefold reduction of CO emission. Platinum-containing foamed catalysts lower the toxicity of exhaust by 85-90%. A favorable effect is demonstrated by the combined use of afterburners and a motor oil additive based on ultradispersed copper.

  8. Using Underwater Explosion and Cylinder Expansion Tests to Calibrate Afterburn Models for Aluminized Explosives

    NASA Astrophysics Data System (ADS)

    Wedberg, Rasmus

    2017-06-01

    The study explores the combined use of underwater performance tests and cylinder expansion tests in order to parameterize detonation models for aluminized explosives which exhibit afterburning. The approach is suggested to be used in conjunction with thermochemical computation. A formulation containing RDX and aluminum powder is considered and several charges with varying masses are submerged and detonated. Pressure gauges are employed at horizontal distances scaling with the charge diameter, and the specific shock wave energy is shown to increase with charge mass. This is attributed to the combustion of aluminum particles after the Chapman-Jouguet plane. Cylinder expansion tests are carried out using Photon Doppler Velocimetry to register the wall expansion velocity. The tests are modeled using a multi-material arbitrary Lagrangian-Eulerian approach with the Guirguis-Miller model describing detonation with afterburning. The equation of state and afterburn rate law parameters are adjusted such that the model reproduces the results from the cylinder expansion and underwater tests. The approach seems promising, and might be valuable for aluminized explosive formulations intended to be used in a variety of confinement conditions. Swedish Armed Forces.

  9. Destructive treatment of waste gas by catalytic afterburning and adsorption

    DOE Office of Scientific and Technical Information (OSTI.GOV)

    Eppel, S.A.; Kochetkova, R.P.; Kolisnyk, G.P.

    1983-07-01

    Because of the considerable energy costs involved in the use of catalytic afterburning to clean up waste gases, an alternative method is suggested: adsorption with the use of low-cost adsorbents that are regenerated by destruction of the substances that has been taken up. Activated semicoke (ASK) is proposed as an adsorbent and tested. On the basis of the results, ASK is recommended for the treatment of waste gases to remove oxygen-containing, sulfurcontaining, and tarry compounds.

  10. Analysis of turbojet-engine controls for afterburning starting

    NASA Technical Reports Server (NTRS)

    Phillips, W E , Jr

    1956-01-01

    A simulation procedure is developed for studying the effects of an afterburner start on a controlled turbojet engine. The afterburner start is represented by introducing a step decrease in the effective exhaust-nozzle area, after which the control returns the controlled engine variables to their initial values. The degree and speed with which the control acts are a measure of the effectiveness of the particular control system. Data are presented from five systems investigated using an electronic analog computer and the developed simulation procedure. These systems are compared with respect to steady-state errors, speed of response, and transient deviations of the system variables.

  11. Efficiency of the rocket engines with a supersonic afterburner

    NASA Astrophysics Data System (ADS)

    Sergienko, A. A.

    1992-08-01

    The paper is concerned with the problem of regenerative cooling of the liquid-propellant rocket engine combustion chamber at high pressures of the working fluid. It is shown that high combustion product pressures can be achieved in the liquid-propellant rocket engine with a supersonic afterburner than in a liquid-propellant rocket engine with a conventional subsonic combustion chamber for the same allowable heat flux density. However, the liquid-propellant rocket engine with a supersonic afterburner becomes more economical than the conventional engine only at generator gas temperatures of 1700 K and higher.

  12. Exhaust emission calibration of two J-58 afterburning turbojet engines at simulated high-altitude, supersonic flight conditions

    NASA Technical Reports Server (NTRS)

    Holdeman, J. D.

    1976-01-01

    Emissions of total oxides of nitrogen, nitric oxide, unburned hydrocarbons, carbon monoxide, and carbon dioxide from two J-58 afterburning turbojet engines at simulated high-altitude flight conditions are reported. Test conditions included flight speeds from Mach 2 to 3 at altitudes from 16.0 to 23.5 km. For each flight condition exhaust measurements were made for four or five power levels, from maximum power without afterburning through maximum afterburning. The data show that exhaust emissions vary with flight speed, altitude, power level, and radial position across the exhaust. Oxides of nitrogen emissions decreased with increasing altitude and increased with increasing flight speed. Oxides of nitrogen emission indices with afterburning were less than half the value without afterburning. Carbon monoxide and hydrocarbon emissions increased with increasing altitude and decreased with increasing flight speed. Emissions of these species were substantially higher with afterburning than without.

  13. Method and apparatus for afterburning flue gases

    DOE Office of Scientific and Technical Information (OSTI.GOV)

    Sikander, A.; Bjorkman, A.; Jonsson, G.

    1984-11-13

    A method of afterburning flue gases comprises passing impure gases from, for example, an incineration plant such as a destructor, process furnace, crematory furnace or heating boiler, through a burner in an afterburner where through enforced mixture with combustion gas they undergo complete combustion. The combustion gas, depending on the composition of the flue gases, may comprise air or oxygen or either mixed with petroleum gas. In apparatus for implementation of the method, the flue gases and the combustion gas are introduced into a burner which blows the gas mixture into a flame bowl where temperatures in the range ofmore » from 1,500/sup 0/-2,000/sup 0/ C. can be achieved. In one embodiment, the burner produces a conical basket-shaped flame in which the flue gases undergo complete combustion.« less

  14. Investigating ground effects on mixing and afterburning during a TNT explosion

    NASA Astrophysics Data System (ADS)

    Fedina, E.; Fureby, C.

    2013-05-01

    In this paper, the unconfined and semi-confined condensed phase explosions of TNT will be studied using large eddy simulations based on the unsteady, compressible, reacting, multi-species Navier-Stokes equations to gain further understanding of the physical processes involved in a condensed phase explosion and the effect of confinement on the physical processes involved. The analysis of the mixing and afterburning of TNT explosions in free air (unconfined) and near the ground (semi-confined) indicates that the combustion region of detonation products and air is determined by the vorticity patterns, which are induced by the Richtmeyer-Meshkov instabilities that arise during the explosion. When the explosive is detonated in the vicinity of a surface, the surface affects the shock propagation by creating complex shock systems, thereby changing the orientation of the vorticity, giving the afterburning a mushroom shape, and increasing performance of an explosive charge by prolonging the existence of the mixing layer and thereby the afterburning.

  15. Exhaust emission survey of an F100 afterburning turbofan engine at simulated altitude flight conditions

    NASA Technical Reports Server (NTRS)

    Moss, J. E.; Cullom, R. R.

    1981-01-01

    Emissions of carbon monoxide, total oxides of nitrogen, unburned hydrocarbons, and carbon dioxide from an F100, afterburning, two spool turbofan engine at simulated flight conditions are reported. For each flight condition emission measurements were made for two or three power levels from intermediate power (nonafterburning) through maximum afterburning. The data showed that emissions vary with flight speed, altitude, power level, and radial position across the nozzle. Carbon monoxide emissions were low for intermediate power (nonafterburning) and partial afterburning, but regions of high carbon monoxide were present downstream of the flame holder at maximum afterburning. Unburned hydrocarbon emissions were low for most of the simulated flight conditions. The local NOX concentrations and their variability with power level increased with increasing flight Mach number at constant altitude, and decreased with increasing altitude at constant Mach number. Carbon dioxide emissions were proportional to local fuel air ratio for all conditions.

  16. Simulations of Heterogeneous Detonations and Post Detonation Turbulent Mixing and Afterburning

    NASA Astrophysics Data System (ADS)

    Menon, Suresh; Gottiparthi, Kalyana

    2011-06-01

    Most metal-loaded explosives and thermobaric explosives exploit the afterburning of metals to maintain pressure and temperature conditions.The use of such explosives in complex environment can result in post detonation flow containing many scales of vortical motion, flow jetting and shear, as well as plume-surface interactions due to flow impingement and wall flows. In general, all these interactions can lead to highly turbulent flow fields even if the initial ambient conditions were quiescent. Thus, turbulent mixing can dominate initial mixing and impact the final afterburn. We conduct three-dimensional numerical simulations of the propagation of detonation resulting from metal-loaded (inert or reacting) explosives and analyze the afterburn process as well as the generation of multiple scales of mixing in the post detonation flow field. Impact of the detonation and post-detonation flow field on solid surface is also considered for a variety of initial conditions. Comparison with available data is carried out to demonstrate validity of the simulation method. Supported by Defense Threat Reduction Agency

  17. Increase in the efficiency of electric melting of pellets in an arc furnace with allowance for the energy effect of afterburning of carbon oxide in slag using fuel-oxygen burners

    NASA Astrophysics Data System (ADS)

    Stepanov, V. A.; Krakht, L. N.; Merker, E. E.; Sazonov, A. V.; Chermenev, E. A.

    2015-12-01

    The problems of increasing the efficiency of electric steelmaking using fuel-oxygen burners to supply oxygen for the afterburning of effluent gases in an arc furnace are considered. The application of a new energy-saving regime based on a proposed technology of electric melting is shown to intensify the processes of slag formation, heating, and metal decarburization.

  18. Noise of High-Performance Aircraft at Afterburner

    DTIC Science & Technology

    2016-09-22

    Investigation of the importance of indirect combustion noise as a dominant component of military aircraft noise at afterburner. This quarterly...the combustion process is highly unsteady. This creates large temperature fluctuations resulting in the generation of numerous high and low...flow with significant axial velocity gradients, indirect combustion noise is generated (see figure 1). The present research is to investigate this

  19. Operating condition and geometry effects on low-frequency afterburner combustion instability in a turbofan at altitude

    NASA Technical Reports Server (NTRS)

    Cullom, R. R.; Johnsen, R. L.

    1979-01-01

    Three afterburner configurations were tested in a low-bypass-ratio turbofan engine to determine the effect of various fuel distributions, inlet conditions, flameholder geometry, and fuel injection location on combustion instability. Tests were conducted at simulated flight conditions of Mach 0.75 and 1.3 at altitudes from 11,580 to 14,020 m (38,000 to 46,000 ft). In these tests combustion instability with frequency from 28 to 90 Hz and peak-to-peak pressure amplitude up to 46.5 percent of the afterburner inlet total pressure level was encountered. Combustion instability was suppressed in these tests by varying the fuel distribution in the afterburner.

  20. Process and apparatus for afterburning of combustible pollutants from an internal combustion engine

    DOE Office of Scientific and Technical Information (OSTI.GOV)

    Laurent, P.A.

    1978-07-04

    In a process for the afterburning of the combustible pollutants from an internal combustion engine, in order to automatically reduce the secondary induction rate when power increases without using a controlling valve actuatd by the carburetor venturi depression, there is provided a volumetric efficiency of the secondary air pump linked to and activated by the engine and a volumetric efficiency which decreases when the ratio between its back pressure and suction pressure increases, this reduction being achieved through the proper selection of the pump volumetric compression ratio r: between 0.6 c and 1.3 c when a steeply decreasing trend ismore » required, and above 1.3 c if a slower and slower decreasing trend is required. To perform this process an afterburner apparatus has a nitrogen oxide reducing catalyst placed inside the afterburner reactor on the gas stream immediately at the outlet of a torus, in which the gases are homogenized and their reaction with preinjection air is terminated.« less

  1. Noise of high-performance aircraft at afterburner

    NASA Astrophysics Data System (ADS)

    Tam, Christopher K. W.; Parrish, Sarah A.

    2015-09-01

    The noise from a high-performance aircraft at afterburner is investigated. The main objective is to determine whether the dominant noise components are the same or similar to those of a hot supersonic laboratory jet. For this purpose, measured noise data from F-22A Raptors are analyzed. It is found, based on both spectral and directivity data, that there is a new dominant noise component in addition to the usual turbulent mixing noise. The characteristic features of the new noise component are identified. Measured data indicates that the new noise component is observed only when the rate of fuel burn of the engine is increased significantly above that of the intermediate power setting. This suggests that the new noise component is combustion related. The possibility that it is indirect combustion noise generated by the passage of hot spots from the afterburner through the nozzle of the jet is investigated. Because flow and temperature data were not measured in the F-22A engine tests, to provide support to the proposition, numerical simulations of indirect combustion noise generation due to the passing of an entropy wave pulse (a hot spot) through a military-style nozzle are carried out. Sound generation is observed at the front and at the back of the pulse. This creates a fast and a slow acoustic wave as the sound radiates out from the nozzle exit. Quantitative estimates of the principal directions of acoustic radiation due to the emitted fast and slow acoustic waves are made. It is found that there are reasonably good agreements with measured data. To estimate the intensity level (IL) of the radiated indirect combustion noise, a time-periodic entropy wave train of 15 percent temperature fluctuation is used as a model of the hot spots coming out of the afterburner. This yields an IL of 175.5 dB. This is a fairly intense noise source, well capable of causing the radiation of the new jet noise component.

  2. Altitude test of several afterburner configurations on a turbofan engine with a hydrogen heater to simulate an elevated turbine discharge temperature

    NASA Technical Reports Server (NTRS)

    Johnsen, R. L.; Cullom, R. R.

    1977-01-01

    A performance test of several experimental afterburner configurations was conducted with a mixed-flow turbofan engine in an altitude facility. The simulated flight conditions were for Mach 1.4 at two altitudes, 12,190 and 14,630 meters. Turbine discharge temperatures of 889 and 1056 K were used. A production afterburner was tested for comparison. The research afterburners included partial forced mixers with V-gutter flameholders, a carburetted V-gutter flameholder, and a triple ring V-gutter flameholder with four swirl-can fuel mixers. Fuel injection variations were included. Performance data shown include augmented thrust ratio, thrust specific fuel consumption, combustion efficiency, and total pressure drop across the afterburner.

  3. Thermo-Gas-Dynamic Model of Afterburning in Explosions

    DOE Office of Scientific and Technical Information (OSTI.GOV)

    Kuhl, A L; Ferguson, R E; Bell, J B

    2003-07-27

    A theoretical model of afterburning in explosions created by turbulent mixing of the detonation products from fuel-rich charges with air is described. It contains three key elements: (i) a thermodynamic-equilibrium description of the fluids (fuel, air, and products), (ii) a multi-component gas-dynamic treatment of the flow field, and (iii) a sub-grid model of molecular processes of mixing, combustion and equilibration.

  4. Noise of High Performance Aircraft at Afterburner

    DTIC Science & Technology

    2016-02-10

    Navy F18E and the Air Force F22 aircraft became available to the principal investigator. The present project is to analyze these data to identify...the end of the first year of this project (2015), we were able to clearly identify two new dominant noise components from the F22 at afterburner...F18E and F22 aircraft. Compare the noise spectra with those of laboratory hot supersonic jets. ii. Identify any new dominant noise components emitted

  5. Steam thermolysis of tire shreds: modernization in afterburning of accompanying gas with waste steam

    NASA Astrophysics Data System (ADS)

    Kalitko, V. A.

    2010-03-01

    On the basis of experience in the commercial operation of tire-shred steam thermolysis in EnresTec Inc. (Taiwan) producing high-grade commercial carbon, liquid pyrolysis fuel, and accompanying fuel gas by this method, we have proposed a number of engineering solutions and calculated-analytical substantiations for modernization and intensification of the process by afterburning the accompanying gas with waste steam condensable in the scrubber of water gas cleaning of afterburning products. The condensate is completely freed of the organic pyrolysis impurities and the necessity of separating it from the liquid fuel, as is the case with the active process, is excluded.

  6. Emission calibration of a J-58 afterburning turbojet engine at simulated supersonic stratospheric flight conditions

    NASA Technical Reports Server (NTRS)

    Holdeman, J. D.

    1974-01-01

    Emissions of total oxides of nitrogen, unburned hydrocarbons, and carbon monoxide from a J-58 engine at simulated flight conditions of Mach 2.0, 2.4, and 2.8 at 19.8 km altitude are reported. For each flight condition, measurements were made for four engine power levels from maximum power without afterburning through maximum afterburning. These measurements were made 7 cm downstream of the engine primary nozzle using a single point traversing gas sample probe. Results show that emissions vary with flight speed, engine power level, and with radial position across the exhaust.

  7. Emission calibration of a J-58 afterburning turbojet engine at simulated supersonic, stratospheric flight conditions

    NASA Technical Reports Server (NTRS)

    Holdeman, J. D.

    1974-01-01

    Emissions of total oxides of nitrogen, unburned hydrocarbons, and carbon monoxide from a J-58 engine at simulated flight conditions of Mach 2.0, 2.4, and 2.8 at 19.8 km altitude are reported. For each flight condition, measurements were made for four engine power levels from maximum power without afterburning through maximum afterburning. These measurements were made 7 cm downstream of the engine primary nozzle using a single point traversing gas sample probe. Results show that emissions vary with flight speed, engine power level, and with radial position across the exhaust.

  8. Measurements and predictions of flyover and static noise of a TF30 afterburning turbofan engine

    NASA Technical Reports Server (NTRS)

    Burcham, F. W., Jr.; Lasagna, P. L.; Oas, S. C.

    1978-01-01

    The noise of the TF30 afterburning turbofan engine in an F-111 airplane was determined from static (ground) and flyover tests. A survey was made to measure the exhaust temperature and velocity profiles for a range of power settings. Comparisons were made between predicted and measured jet mixing, internal, and shock noise. It was found that the noise produced at static conditions was dominated by jet mixing noise, and was adequately predicted by current methods. The noise produced during flyovers exhibited large contributions from internally generated noise in the forward arc. For flyovers with the engine at nonafterburning power, the internal noise, shock noise, and jet mixing noise were accurately predicted. During flyovers with afterburning power settings, however, additional internal noise believed to be due to the afterburning process was evident; its level was as much as 8 decibels above the nonafterburning internal noise. Power settings that produced exhausts with inverted velocity profiles appeared to be slightly less noisy than power settings of equal thrust that produced uniform exhaust velocity profiles both in flight and in static testing.

  9. [Experimental determination of the time-dependent extent of after-burning with reference to possibilities of the plastic surgery reconstruction of 3d degree burns].

    PubMed

    Bäumer, F; Henrich, H A; Ussmüller, J

    1986-02-01

    The present experiments try to answer the question as to the time-dependent extent of the after-burning process after full-thickness burn (third degree). For an early plastic surgical treatment it was of interest to determine the most early time of escharotomy. The time-dependent spreading of the after-burning area reached its maximum five days after the burn injury. The after-burning area was marked by intravenous injections of Patentblau which caused distinct intravital colouring. Subsequently no further progress could be observed. In the present experiments we suggest this time as the earliest time for plastic covering in case it would be dependent upon the end of the after-burning process.

  10. Numerical Investigation of Aluminum Burning Behind Blast Waves

    DTIC Science & Technology

    2010-10-01

    Lai, and K.S. Im, “ Afterburning of TNT Explosive Products in Air with Aluminum Particles,” AIAA-2008-1029, 2008 [2] K. Balakrishnan and S. Menon...phase flow was applied. The modeled HE includes a significant percentage of aluminum particles, whose long-time afterburning and energy release must...the physical mechanisms are even more complex. The flow environment is significantly different from bare charge detonation and afterburn . As long

  11. Measurements and predictions of flyover and static noise of an afterburning turbofan engine in an F-111 airplane

    NASA Technical Reports Server (NTRS)

    Burcham, F. W., Jr.

    1979-01-01

    The noise of the TF30 afterburning turbofan engine in an F-111 airplane was determined from static (ground) and flyover tests. Exhaust temperatures and velocity profiles were measured for a range of power settings. Comparisons were made between predicted and measured jet mixing, internal, and shock noise. It was found that the noise produced at static conditions was dominated by jet mixing noise, and was adequately predicted by current methods. The noise produced during flyovers exhibited large contributions from internally generated noise in the forward arc. For flyovers with the engine at nonafterburning power, the internal noise, shock noise, and jet mixing noise were accurately predicted. During flyovers with afterburning power settings, however, additional internal noise believed to be due to the afterburning process was evident; its level was as much as 8 decibels above the nonafterburning internal noise.

  12. Numerical simulation of long-duration blast wave evolution in confined facilities

    NASA Astrophysics Data System (ADS)

    Togashi, F.; Baum, J. D.; Mestreau, E.; Löhner, R.; Sunshine, D.

    2010-10-01

    The objective of this research effort was to investigate the quasi-steady flow field produced by explosives in confined facilities. In this effort we modeled tests in which a high explosive (HE) cylindrical charge was hung in the center of a room and detonated. The HEs used for the tests were C-4 and AFX 757. While C-4 is just slightly under-oxidized and is typically modeled as an ideal explosive, AFX 757 includes a significant percentage of aluminum particles, so long-time afterburning and energy release must be considered. The Lawrence Livermore National Laboratory (LLNL)-produced thermo-chemical equilibrium algorithm, “Cheetah”, was used to estimate the remaining burnable detonation products. From these remaining species, the afterburning energy was computed and added to the flow field. Computations of the detonation and afterburn of two HEs in the confined multi-room facility were performed. The results demonstrate excellent agreement with available experimental data in terms of blast wave time of arrival, peak shock amplitude, reverberation, and total impulse (and hence, total energy release, via either the detonation or afterburn processes.

  13. Modeling of chemical reactions in afterburning for the reduction of N{sub 2}O

    DOE Office of Scientific and Technical Information (OSTI.GOV)

    Gustavsson, L.; Glarborg, P.; Leckner, B.

    1996-08-01

    Afterburning involves burning a secondary fuel in the flue gases from a fluidized bed combustor to raise the temperature, and thereby decrease the emission of N{sub 2}O. Tests in a 12-MW circulating fluidized bed boiler used the cyclone as an afterburning combustor. The results from these tests are analyzed by chemical kinetic calculations with homogeneous hydrocarbon and nitrogen chemistry. Furthermore, a study is made of the influence on the calculation of particles in the flue gases. The deviation between calculated and measured data is small at high temperatures, but increases at the lower temperatures investigated. The influence of particles ismore » predicted to be small under conditions prevailing in the cyclone.« less

  14. Development of burners for afterburning chambers of heat-recovery boilers at cogeneration stations equipped with combined-cycle plants

    NASA Astrophysics Data System (ADS)

    Khomenok, L. A.

    2007-09-01

    Problems related to efficient afterburning of fuel in the medium of gas-turbine unit exhaust gases, as well as new design arrangements of gas-jet burners used in the chambers for afterburning fuel in heat-recovery boilers at cogeneration stations equipped with combined-cycle plants, are considered. Results obtained from comparative experimental investigations of different gas-jet flame stabilizers at a test facility are presented, and the advantages of jet-ejector stabilizers are demonstrated.

  15. The effects of compressor seventh-stage bleed air extraction on performance of the F100-PW-220 afterburning turbofan engine

    NASA Technical Reports Server (NTRS)

    Evans, Alison B.

    1991-01-01

    A study was conducted to determine the effects of seventh-stage compressor bleed on the performance of the F100 afterburning turbofan engine. The effects of bleed on thrust, specific fuel consumption, fan turbine inlet temperature, bleed total pressure, and bleed total temperature were obtained from the engine manufacturer's status deck computer simulation. These effects were determined for power settings of intermediate, partial afterburning, and maximum afterburning for Mach numbers between 0.6 and 2.2 and for altitudes of 30,000, 40,000, and 50,000 ft. It was found that thrust loss and specific fuel consumption increase were approximately linear functions of bleed flow and, based on a percent-thrust change basis, were approximately independent of power setting.

  16. Installation for the catalytic afterburning of exhaust gases in the exhaust gas system of an internal combustion engine

    DOE Office of Scientific and Technical Information (OSTI.GOV)

    Lange, K.

    1974-12-06

    An installation is described for the catalytic afterburning of exhaust gases in an internal combustion engine. The system includes a line by-passing the installation for the catalytic afterburning, in which is arranged a throttle valve actuated in dependence on the temperature of the installation. The throttle valve also can be actuated independently of the temperature of the installation, but in dependence of the oil pressure which continues to exist for a short period of time after turning off the engine.

  17. EMISSIONS OF AIR TOXICS FROM A SIMULATED CHARCOAL KILN EQUIPPED WITH AN AFTERBURNER

    EPA Science Inventory

    The report discusses emissions of air toxics from a simulated charcoal kiln equipped with an afterburner. A laboratory-scale simulator was constructed and tested to determine if it could be used to produce charcoal that was similar to that produced in Missouri-type charcoal kilns...

  18. Effects of entrained water and strong turbulence on afterburning within solid rocket motor plumes

    NASA Technical Reports Server (NTRS)

    Gomberg, R. I.; Wilmoth, R. G.

    1978-01-01

    During the first few seconds of the space shuttle trajectory, the solid rocket boosters will be in the proximity of the launch pad. Because of the launch pad structures and the surface of the earth, the turbulent mixing experienced by the exhaust gases will be greatly increased over that for the free flight situation. In addition, a system will be present, designed to protect the lifting vehicle from launch structure vibrations, which will inject quantities of liquid water into the hot plume. The effects of these two phenomena on the temperatures, chemical composition, and flow field present in the afterburning solid rocket motor exhaust plumes of the space shuttle were studied. Results are included from both a computational model of the afterburning and supporting measurements from Titan 3 exhaust plumes taken at Kennedy Space Center with infrared scanned radiometers.

  19. Surface Temperature Measurements from a Stator Vane Doublet in a Turbine Engine Afterburner Flame Using a YAG:Tm Thermographic Phosphor

    NASA Technical Reports Server (NTRS)

    Eldridge, J. I.; Walker, D. G.; Gollub, S. L.; Jenkins, T. P.; Allison, S. W.

    2015-01-01

    Luminescence-based surface temperature measurements were obtained from a YAG:Tm-coated stator vane doublet exposed to the afterburner flame of a J85 test engine at University of Tennessee Space Institute (UTSI). The objective of the testing was to demonstrate that reliable surface temperatures based on luminescence decay of a thermographic phosphor producing short-wavelength emission could be obtained from the surface of an actual engine component in a high gas velocity, highly radiative afterburner flame environment. YAG:Tm was selected as the thermographic phosphor for its blue emission at 456 nm (1D23F4 transition) and UV emission at 365 nm (1D23H6 transition) because background thermal radiation is lower at these wavelengths, which are shorter than those of many previously used thermographic phosphors. Luminescence decay measurements were acquired using a probe designed to operate in the afterburner flame environment. The probe was mounted on the sidewall of a high-pressure turbine vane doublet from a Honeywell TECH7000 turbine engine coated with a standard electron-beam physical vapor deposited (EB-PVD) 200-m-thick TBC composed of yttria-stabilized zirconia (YSZ) onto which a 25-m-thick YAG:Tm thermographic phosphor layer was deposited by solution precursor plasma spray (SPPS). Spot temperature measurements were obtained by measuring luminescence decay times at different afterburner power settings and then converting decay time to temperature via calibration curves. Temperature measurements using the decays of the 456 and 365 nm emissions are compared. While successful afterburner environment measurements were obtained to about 1300C with the 456 nm emission, successful temperature measurements using the 365 nm emission were limited to about 1100C due to interference by autofluorescence of probe optics at short decay times.

  20. An afterburner-powered methane/steam reformer for a solid oxide fuel cells application

    NASA Astrophysics Data System (ADS)

    Mozdzierz, Marcin; Chalusiak, Maciej; Kimijima, Shinji; Szmyd, Janusz S.; Brus, Grzegorz

    2018-04-01

    Solid oxide fuel cell (SOFC) systems can be fueled by natural gas when the reforming reaction is conducted in a stack. Due to its maturity and safety, indirect internal reforming is usually used. A strong endothermic methane/steam reforming process needs a large amount of heat, and it is convenient to provide thermal energy by burning the remainders of fuel from a cell. In this work, the mathematical model of afterburner-powered methane/steam reformer is proposed. To analyze the effect of a fuel composition on SOFC performance, the zero-dimensional model of a fuel cell connected with a reformer is formulated. It is shown that the highest efficiency of a solid oxide fuel cell is achieved when the steam-to-methane ratio at the reforming reactor inlet is high.

  1. Determining the maximal capacity of a combined-cycle plant operating with afterburning of fuel in the gas conduit upstream of the heat-recovery boiler

    NASA Astrophysics Data System (ADS)

    Borovkov, V. M.; Osmanova, N. M.

    2011-01-01

    The effect gained from afterburning of fuel in the gas conduit upstream of the heat-recovery boiler used as part of a PGU-450T combined-cycle plant is considered. The results obtained from calculations of the electric and thermal power outputs produced by the combined-cycle plant equipped with an afterburning chamber are presented.

  2. Magnetic design of an Apple-X afterburner for the SASE3 undulator of the European XFEL

    NASA Astrophysics Data System (ADS)

    Li, Peng; Wei, Tao; Li, Yuhui; Pflueger, Joachim

    2017-10-01

    In its startup configuration the SASE3 beamline of the European XFEL provides only soft X-ray radiation, linearly polarized in the horizontal plane. In order to enhance capabilities of this beamline an afterburner scheme is proposed. It will be used as a coherent radiator using the micro-bunched electron beam of the linear SASE3 system. Radiation with variable polarization, which covers the full SASE3 wavelength range can be generated. For the radiator a new type of undulator design called Apple-X will be used. In this paper the design is described and magnet parameters, which are compatible with the SASE3 afterburner are determined using RADIA simulations. The end structure of such a device is optimized for minimum 1st field integrals.

  3. Integrated pneumatic transporter-incinerator-afterburner subsystem development. [for spacecraft waste disposal

    NASA Technical Reports Server (NTRS)

    Manning, J. R.

    1974-01-01

    The design and fabrication of a prototype automatic transport system to move wastes to an incinerator onboard a spacecraft are described. The commode and debris collector, subsystems to treat noncondensible gases, oxygen supply to incinerator and afterburner, and removal and ash collection from the incinerator are considered, as well as a zero gravity condenser. In-depth performance testing of a totally integrated incineration system and autoclaving as a waste treatment method are included.

  4. Numerical Investigation on Aerodynamic and Combustion Performance of Chevron Mixer Inside an Afterburner.

    PubMed

    Yong, Shan; JingZhou, Zhang; Yameng, Wang

    2014-11-01

    To improve the performance of the afterburner for the turbofan engine, an innovative type of mixer, namely, the chevron mixer, was considered to enhance the mixture between the core flow and the bypass flow. Computational fluid dynamics (CFD) simulations investigated the aerodynamic performances and combustion characteristics of the chevron mixer inside a typical afterburner. Three types of mixer, namely, CC (chevrons tilted into core flow), CB (chevrons tilted into bypass flow), and CA (chevrons tilted into core flow and bypass flow alternately), respectively, were studied on the aerodynamic performances of mixing process. The chevrons arrangement has significant effect on the mixing characteristics and the CA mode seems to be advantageous for the generation of the stronger streamwise vortices with lower aerodynamic loss. Further investigations on combustion characteristics for CA mode were performed. Calculation results reveal that the local temperature distribution at the leading edge section of flame holder is improved under the action of streamwise vortices shedding from chevron mixers. Consequently, the combustion efficiency increased by 3.5% compared with confluent mixer under the same fuel supply scheme.

  5. Turbofan compressor dynamics during afterburner transients

    NASA Technical Reports Server (NTRS)

    Kurkov, A. P.

    1975-01-01

    The effects of afterburner light-off and shut-down transients on compressor stability were investigated. Experimental results are based on detailed high-response pressure and temperature measurements on the Tf30-p-3 turbofan engine. The tests were performed in an altitude test chamber simulating high-altitude engine operation. It is shown that during both types of transients, flow breaks down in the forward part of the fan-bypass duct. At a sufficiently low engine inlet pressure this resulted in a compressor stall. Complete flow breakdown within the compressor was preceded by a rotating stall. At some locations in the compressor, rotating stall cells initially extended only through part of the blade span. For the shutdown transient, the time between first and last detected occurrence of rotating stall is related to the flow Reynolds number. An attempt was made to deduce the number and speed of propagation of rotating stall cells.

  6. Development of Emissions Measurement Techniques for Afterburning Turbine Engines

    DTIC Science & Technology

    1975-10-01

    are most reactive in the plume, with significant de - creases observed at all afterburning power levels. Cnrhon monoxide call either increas~ e or...Plane) Part B. Near Plume Method (Measurement I’rfc(diLr 3•rC for Sampling at Nozzle Exit Plane) viit ! o E . . LIST uO ILLUSrRATIUNS F igure I1.8.t...36. 1lC Concentration Radial Protile, J79-15 Enghine’ at Mid. :•3 AM B Power Level. 37 (𔃺 \\s. C ( O ) (’onv(ent rat io I m .j 7 4 1- E ngtine aI Mmn. A

  7. A concept for jet noise suppression for an afterburning turbojet engine

    NASA Technical Reports Server (NTRS)

    Chambellan, R. E.; Turek, R. J.

    1972-01-01

    A conceptual design of an afterburner system for turbojet engines which may reduce the jet exhaust noise by approximately 10 decibels is presented in this report. The proposed system consists of an array of swirl-can combustors and jet dividing nozzle tubes. The nozzle tubes translate axially upstream of the swirl cans when not in use. Results of preliminary design calculations and photographs of a kinematic model as applied to a hypothetical turbojet engine are presented.

  8. Polynuclear aromatic hydrocarbon and particulate emissions from two-stage combustion of polystyrene: the effects of the secondary furnace (afterburner) temperature and soot filtration.

    PubMed

    Wang, Jun; Richter, Henning; Howard, Jack B; Levendis, Yiannis A; Carlson, Joel

    2002-02-15

    Laboratory experiments were conducted in a two-stage horizontal muffle furnace in order to monitor emissions from batch combustion of polystyrene (PS) and identify conditions that minimize them. PS is a dominant component of municipal and hospital waste streams. Bench-scale combustion of small samples (0.5 g) of shredded styrofoam cups was conducted in air, using an electrically heated horizontal muffle furnace, kept at Tgas = 1000 degrees C. Upon devolatilization, combustion of the polymer took place in a diffusion flame over the sample. The gaseous combustion products were mixed with additional air in a venturi and were channeled to a secondary muffle furnace (afterburner) kept at Tgas = 900-1100 degrees C; residence time therein varied between 0.6 and 0.8 s. At the exits of the primary and the secondary furnace the emissions of CO, CO2, O2, NOx, particulates as well as volatile and semivolatile hydrocarbons, such as polycyclic aromatic hydrocarbons (PAH), were monitored. Online analyzers, gravimetric techniques, and gas chromatography coupled to mass spectrometry (GC-MS) were used. Experiments were also conducted with a high-temperature barrier filter, placed just before the exit of the primary furnace to prevent the particulates from entering into the secondary furnace. Results demonstrated the beneficial effect of the afterburner in reducing PAH concentrations, including those of mutagenic species such as benzo[a]pyrene. Concentrations of individual PAH exhibited a pronounced after burner temperature dependence, typically ranging from a small decrease at 900 degrees C to a larger degree of consumption at 1100 degrees C. Consumption of PAH was observed to be the dominant feature at 900 degrees C, while significant quantities of benzene and some of its derivatives, captured by means of carbosieve/Carbotrap adsorbents, were formed in the afterburner at a temperature of 1000 degrees C. In the primary furnace, about 30% of the mass of the initial polystyrene was

  9. Laboratory generation of free chlorine from HCl under stratospheric afterburning conditions

    DOE Office of Scientific and Technical Information (OSTI.GOV)

    Burke, M.L.; Zittel, P.F.

    1998-01-01

    Experiments have been conducted using a low pressure laboratory flame apparatus to examine the chemistry of solid rocket motor (SRM) afterburning relevant for stratospheric altitudes. It was found that a significant fraction of the HCl injected into H{sub 2}-O{sub 2} and H{sub 2}-CO-O{sub 2} flames can be consumed, with observed losses of up to 40%. The extent of conversion of HCl was found to increase with increasing oxygen:fuel (O/F) ratio and decreasing pressure; the loss at a given O/F was also higher for flames with equal flows of H{sub 2} and CO compared to flames with no CO in themore » fuel. The major product of HCl reaction was found to be Cl{sub 2}, with no other chlorine-contained products observed via mass spectrometry. Distinct Cl{sub 2} B {yields} X emission bands were observed along with very weak CIO A {yields} C bands and a bright, white continuum emission that apparently arose from one or more chlorine-containing compounds. The general findings concerning the magnitude of HCl conversion and the formation of Cl{sub 2} are consistent with published modeling results for SRM stratospheric afterburning. This formation of free chlorine could lead to catalytic destruction of ozone in regions near the path the launch vehicle follows during boost through the stratosphere.« less

  10. Energy release in solar flares

    NASA Technical Reports Server (NTRS)

    Brown, John C.; Correia, Emilia; Farnik, Frantisek; Garcia, Howard; Henoux, Jean-Claude; La Rosa, Ted N.; Machado, Marcos E. (Compiler); Nakajima, Hiroshi; Priest, Eric R.

    1994-01-01

    Team 2 of the Ottawa Flares 22 Workshop dealt with observational and theoretical aspects of the characteristics and processes of energy release in flares. Main results summarized in this article stress the global character of the flaring phenomenon in active regions, the importance of discontinuities in magnetic connectivity, the role of field-aligned currents in free energy storage, and the fragmentation of energy release in time and space.

  11. Preliminary Altitude Performance Data of J71-A2 Turbojet Engine Afterburner

    NASA Technical Reports Server (NTRS)

    Useller, James W.; Mallett, William E.

    1954-01-01

    The performance and operational characteristics of the J71-A2 turbojet-engine afterburner were investigated for a range of altitudes from 23,000 to 60,000 feet at a flight Mach number of 0,9 and at flight Mach numbers of 0.6, 0.9, and 1.0 at an altitude of 45,000 feet. The combustion performance and altitude operational limits, as well as the altitude starting characteristics have been determined.

  12. Altitude-Test-Chamber Investigation of a Solar Afterburner on the 24C Engine I - Operational Characteristics and Altitude Limits

    NASA Technical Reports Server (NTRS)

    1948-01-01

    An altitude-test-chamber investigation was conducted to determine the operational characteristics and altitude blow-out limits of a Solar afterburner in a 24C engine. At rated engine speed and maximum permissible turbine-discharge temperature, the altitude limit as determined by combustion blow-out occurred as a band of unstable operation of about 8000 feet altitude in width with maximum altitude limits from 32,000 feet at a Mach number of 0.3 to about 42,000 feet at a Mach number of 1.0. The maximum fuel-air ratio of the afterburner, as limited by maximum permissible turbine-discharge gas temperatures at rated engine speed, varied between 0.0295 and 0.0380 over a range of flight Mach numbers from 0.25 to 1.0 and at altitudes of 20,000 and 30,000 feet. Over this range of operating conditions, the fuel-air ratio at which lean blow-out occurred was from 10 to 19 percent below these maximum fuel-air ratios. Combustion was very smooth and uniform during operation; however, ignition of the burner was very difficult throughout the investigation. A failure of the flame holder after 12 hours and 15 minutes of afterburner operation resulted in termination of the investigation.

  13. Quantification of Energy Release in Composite Structures

    NASA Technical Reports Server (NTRS)

    Minnetyan, Levon

    2003-01-01

    Energy release rate is usually suggested as a quantifier for assessing structural damage tolerance. Computational prediction of energy release rate is based on composite mechanics with micro-stress level damage assessment, finite element structural analysis and damage progression tracking modules. This report examines several issues associated with energy release rates in composite structures as follows: Chapter I demonstrates computational simulation of an adhesively bonded composite joint and validates the computed energy release rates by comparison with acoustic emission signals in the overall sense. Chapter II investigates the effect of crack plane orientation with respect to fiber direction on the energy release rates. Chapter III quantifies the effects of contiguous constraint plies on the residual stiffness of a 90 ply subjected to transverse tensile fractures. Chapter IV compares ICAN and ICAN/JAVA solutions of composites. Chapter V examines the effects of composite structural geometry and boundary conditions on damage progression characteristics.

  14. Quantification of Energy Release in Composite Structures

    NASA Technical Reports Server (NTRS)

    Minnetyan, Levon; Chamis, Christos C. (Technical Monitor)

    2003-01-01

    Energy release rate is usually suggested as a quantifier for assessing structural damage tolerance. Computational prediction of energy release rate is based on composite mechanics with micro-stress level damage assessment, finite element structural analysis and damage progression tracking modules. This report examines several issues associated with energy release rates in composite structures as follows: Chapter I demonstrates computational simulation of an adhesively bonded composite joint and validates the computed energy release rates by comparison with acoustic emission signals in the overall sense. Chapter II investigates the effect of crack plane orientation with respect to fiber direction on the energy release rates. Chapter III quantifies the effects of contiguous constraint plies on the residual stiffness of a 90 deg ply subjected to transverse tensile fractures. Chapter IV compares ICAN and ICAN/JAVA solutions of composites. Chapter V examines the effects of composite structural geometry and boundary conditions on damage progression characteristics.

  15. Thrust and pumping characteristics of cylindrical ejectors using afterburning turbojet gas generator

    NASA Technical Reports Server (NTRS)

    Samanich, N. E.; Huntley, S. C.

    1969-01-01

    Static tests of cylindrical ejectors having ejector to primary diameter ratios from 1.1 to 1.6 and ejector length to primary nozzle diameter ratios from 0.9 to 2.1 are reported. Power setting of the J85-13 turbojet engine was varied from part power to maximum afterburning. Corrected secondary weight flow ratio was varied from 0.02 to 0.08 over a range of exhaust nozzle pressure ratios from 2.0 to 9.0. Secondary flow temperature rise and pressure drop characteristics through the nacelle secondary flow passage were also obtained.

  16. Nuclear energy release from fragmentation

    NASA Astrophysics Data System (ADS)

    Li, Cheng; Souza, S. R.; Tsang, M. B.; Zhang, Feng-Shou

    2016-08-01

    It is well known that binary fission occurs with positive energy gain. In this article we examine the energetics of splitting uranium and thorium isotopes into various numbers of fragments (from two to eight) with nearly equal size. We find that the energy released by splitting 230,232Th and 235,238U into three equal size fragments is largest. The statistical multifragmentation model (SMM) is applied to calculate the probability of different breakup channels for excited nuclei. By weighing the probability distributions of fragment multiplicity at different excitation energies, we find the peaks of energy release for 230,232Th and 235,238U are around 0.7-0.75 MeV/u at excitation energy between 1.2 and 2 MeV/u in the primary breakup process. Taking into account the secondary de-excitation processes of primary fragments with the GEMINI code, these energy peaks fall to about 0.45 MeV/u.

  17. High probability neurotransmitter release sites represent an energy efficient design

    PubMed Central

    Lu, Zhongmin; Chouhan, Amit K.; Borycz, Jolanta A.; Lu, Zhiyuan; Rossano, Adam J; Brain, Keith L.; Zhou, You; Meinertzhagen, Ian A.; Macleod, Gregory T.

    2016-01-01

    Nerve terminals contain multiple sites specialized for the release of neurotransmitters. Release usually occurs with low probability, a design thought to confer many advantages. High probability release sites are not uncommon but their advantages are not well understood. Here we test the hypothesis that high probability release sites represent an energy efficient design. We examined release site probabilities and energy efficiency at the terminals of two glutamatergic motor neurons synapsing on the same muscle fiber in Drosophila larvae. Through electrophysiological and ultrastructural measurements we calculated release site probabilities to differ considerably between terminals (0.33 vs. 0.11). We estimated the energy required to release and recycle glutamate from the same measurements. The energy required to remove calcium and sodium ions subsequent to nerve excitation was estimated through microfluorimetric and morphological measurements. We calculated energy efficiency as the number of glutamate molecules released per ATP molecule hydrolyzed, and high probability release site terminals were found to be more efficient (0.13 vs. 0.06). Our analytical model indicates that energy efficiency is optimal (~0.15) at high release site probabilities (~0.76). As limitations in energy supply constrain neural function, high probability release sites might ameliorate such constraints by demanding less energy. Energy efficiency can be viewed as one aspect of nerve terminal function, in balance with others, because high efficiency terminals depress significantly during episodic bursts of activity. PMID:27593375

  18. Afterburning in spherical premixed turbulent explosions

    DOE Office of Scientific and Technical Information (OSTI.GOV)

    Bradley, D.; Lawes, M.; Scott, M.J.

    1994-12-01

    During the early stages of spherical turbulent flame propagation, more than half of the gas behind the visible flame front may be unburned. Previous models of the afterburning of the gas behind the apparent flame front have been extended in the present work, to include the effects of flame quenching, consequent upon localized flame stretch. The predictions of the model cover, the spatial and temporal variations of the fraction burned, the flame propagation rate, and the mass burning rate. They are all in dimensionless form and are well supported by associated experimental measurements in a fan-stirred bomb with controlled turbulence.more » The proportion of the gas that is unburned decreases with time and increases with the product of the Karlovitz stretch factor and the Lewis number. Simultaneous photographs were taken of the spherical schlieren image and of that due to Mie scattering from small seed particles in a thin laser sheet that sectioned the spherical flame. These clearly showed the amount of unburned gas within the sphere and, along with other evidence suggest laminar flamelet burning across a scale of distance which is close to the Taylor confirm the predictions of the fraction of gas unburned and of the rate at which it is burning.« less

  19. Net thrust calculation sensitivity of an afterburning turbofan engine to variations in input parameters

    NASA Technical Reports Server (NTRS)

    Hughes, D. L.; Ray, R. J.; Walton, J. T.

    1985-01-01

    The calculated value of net thrust of an aircraft powered by a General Electric F404-GE-400 afterburning turbofan engine was evaluated for its sensitivity to various input parameters. The effects of a 1.0-percent change in each input parameter on the calculated value of net thrust with two calculation methods are compared. This paper presents the results of these comparisons and also gives the estimated accuracy of the overall net thrust calculation as determined from the influence coefficients and estimated parameter measurement accuracies.

  20. Simulations of heterogeneous detonations and post-detonation turbulent mixing and afterburning

    NASA Astrophysics Data System (ADS)

    Gottiparthi, Kalyana Chakravarthi; Menon, Suresh

    2012-03-01

    We conduct three-dimensional numerical simulations of the propagation of blast waves resulting from detonation of a nitromethane charge of radius 5.9 cm loaded with aluminum particles and analyze the afterburn process as well as the generation of multiple scales ofmixing in the post detonation flow field. In the current study, the particle combustion is observed to be dependent on particle dispersal and mixing of gases in the flow where particle dispersal spreads aluminum within the flow and mixing provides the necessary oxidizer. Thus, 5 μm aluminum particles are burnt more effectively in comparison to 10 μm particles for a fixed initial mass of particles. Also, for a fixed initial particle size, increase in the initial mass of aluminum particles resulted in greater mixing.

  1. High-Energy Aspects of Small-Scale Energy Release at the Sun

    NASA Astrophysics Data System (ADS)

    Glesener, L.; Vievering, J. T.; Wright, P. J.; Hannah, I. G.; Panchapakesan, S. A.; Ryan, D.; Krucker, S.; Hudson, H. S.; Grefenstette, B.; White, S. M.; Smith, D. M.; Marsh, A.; Kuhar, M.; Christe, S.; Buitrago-Casas, J. C.; Musset, S.; Inglis, A. R.

    2017-12-01

    Large, powerful solar flares have been investigated in detail for decades, but it is only recently that high-energy aspects of small flares could be measured. These small-scale energy releases offer the opportunity to examine how particle acceleration characteristics scale down, which is critical for constraining energy transfer theories such as magnetic reconnection. Probing to minuscule flare sizes also brings us closer to envisioning the characteristics of the small "nanoflares" that may be responsible for heating the corona. A new window on small-scale flaring activity is now opening with the use of focusing hard X-ray instruments to observe the Sun. Hard X-rays are emitted by flare-accelerated electrons and strongly heated plasma, providing a relatively direct method of measuring energy release and particle acceleration properties. This work will show the first observations of sub-A class microflares using the FOXSI sounding rocket and the NuSTAR astrophysics spacecraft, both of which directly focus hard X-rays but have limited observing time on the Sun. These instruments serve as precursors to a spacecraft version of FOXSI, which will explore energy release across the entire range of flaring activity.

  2. Highlights of the study of energy release in flares

    NASA Technical Reports Server (NTRS)

    Rust, D. M.; Batchelor, D. A.

    1987-01-01

    From February 26 to March 1, 1979, 32 solar flare investigators attended a workshop at Cambridge, MA to define objectives and devise a scientific program for the study of energy release in flares (SERF) during the coming solar maximum. Herein, some major results of the ensuing five-year effort to observe and understand the flare energy release process and its effects (energetic particle production, coronal and chromospheric heating, electromagnetic radiations, and mass motions and ejections) are reviewed. The central issue - what processes store and release the energy liberated in flares - remains unresolved except in the most general terms (e.g., it is generally agreed that the energy is stored in sheared or stressed magnetic fields and released by field annihilation during some MHD instability). Resolving that issue is still one of the most important goals in solar physics, but the advances during the SERF program have brought it closer.

  3. Microelectromechanical high-density energy storage/rapid release system

    NASA Astrophysics Data System (ADS)

    Rodgers, M. Steven; Allen, James J.; Meeks, Kent D.; Jensen, Brian D.; Miller, Samuel L.

    1999-08-01

    One highly desirable characteristic of electrostatically driven microelectromechanical systems (MEMS) is that they consume very little power. The corresponding drawback is that the force they produce may be inadequate for many applications. It has previously been demonstrated that gear reduction units or microtransmissions can substantially increase the torque generated by microengines. Operating speed, however, is also reduced by the transmission gear ratio. Some applications require both high speed and high force. If this output is only required for a limited period of time, then energy could be stored in a mechanical system and rapidly released upon demand. We have designed, fabricated, and demonstrated a high-density energy storage/rapid release system that accomplishes this task. Built using a 5-level surface micromachining technology, the assembly closely resembles a medieval crossbow. Energy releases on the order of tens of nanojoules have already been demonstrated, and significantly higher energy systems are under development.

  4. Energy Release in Solar Flares,

    DTIC Science & Technology

    1982-10-01

    Plasma Research, Stanford University P. Kaufmanu CRAA/CNPq -Conseiho lacional de Desenvolvimento Cientifico e Tecnologico, Slo Paulo, SP, Brasil D.F...three phases of energy release in solar flares (Sturrock, 1980). However, a recent article by Feldman e a.. (1982) points to a significant

  5. A simplified gross thrust computing technique for an afterburning turbofan engine

    NASA Technical Reports Server (NTRS)

    Hamer, M. J.; Kurtenbach, F. J.

    1978-01-01

    A simplified gross thrust computing technique extended to the F100-PW-100 afterburning turbofan engine is described. The technique uses measured total and static pressures in the engine tailpipe and ambient static pressure to compute gross thrust. Empirically evaluated calibration factors account for three-dimensional effects, the effects of friction and mass transfer, and the effects of simplifying assumptions for solving the equations. Instrumentation requirements and the sensitivity of computed thrust to transducer errors are presented. NASA altitude facility tests on F100 engines (computed thrust versus measured thrust) are presented, and calibration factors obtained on one engine are shown to be applicable to the second engine by comparing the computed gross thrust. It is concluded that this thrust method is potentially suitable for flight test application and engine maintenance on production engines with a minimum amount of instrumentation.

  6. Internal combustion engine having a reactor for afterburning of unburned exhaust gas constituents

    DOE Office of Scientific and Technical Information (OSTI.GOV)

    Maurhoff, G.; Steinwart, J.

    1974-08-07

    An internal combustion engine is described which has an engine housing and a reactor for afterburning of unburned constituents in the exhaust gas. The reactor has a shell with a periphery and contains a heat-insulated, reactor chamber which is freely movable beyond the point of connection to the shell. The reactor has an inlet nozzle extending freely through the shell and connected to an outlet passage of the engine and has an outlet for escape of the exhaust gases from the reactor chamber. The inlet nozzle protrudes freely into the outlet passage, and the shell has a portion around themore » inlet nozzle in contact with the engine housing.« less

  7. Installation for the catalytic afterburning of exhaust gases of a multi-cylinder internal combustion engine

    DOE Office of Scientific and Technical Information (OSTI.GOV)

    Lange, K.

    1974-04-24

    An installation for the catalytic afterburning of exhaust gases of a multi-cylinder internal combustion engine has two cylinder rows with two exhaust gas lines, each of which includes at least one catalyst. A temperature-responsive control is operable during engine start-up to conduct substantially the entire exhaust gas flow from the internal combustion engine during warmup for a predetermined time by way of only one of the two catalyst and then, after a short period of time, to conduct the exhaust gas flow from each row of cylinders by way of its associated gas line and catalyst.

  8. Preliminary Internal Performance Data for a Variable-Ejector Assembly on the XJ79-GE-1 Turbojet Engine. II; Afterburning Configurations

    NASA Technical Reports Server (NTRS)

    Bloomer, Harry E.; Groesbeck, Donald E.

    1957-01-01

    Internal performance of an XJ79-GE-1 variable ejector was experimentally determined with the primary nozzle in two representative after-burning positions. Jet-thrust and air-handling data were obtained in quiescent air for 4 selected ejector configurations over a wide range of secondary to primary airflow ratios and primary-nozzle pressure ratios. The experimental ejector data are presented in both graphical and tabulated form.

  9. Interactive Educational Tool for Turbofan and Afterburning Turbojet Engines

    NASA Technical Reports Server (NTRS)

    Benson, Thomas J.

    1997-01-01

    A workstation-based, interactive educational computer program has been developed at the NASA Lewis Research Center to aid in the teaching and understanding of turbine engine design and analysis. This tool has recently been extended to model the performance of two-spool turbofans and afterburning turbojets. The program solves for the flow conditions through the engine by using classical one-dimensional thermodynamic analysis found in various propulsion textbooks. Either an approximately thermally perfect or calorically perfect gas can be used in the thermodynamic analysis. Students can vary the design conditions through a graphical user interface; engine performance is calculated immediately. A variety of graphical formats are used to present results, including numerical results, moving bar charts, and student-generated temperature versus entropy (Ts), pressure versus specific volume (pv), and engine performance plots. The package includes user-controlled printed output, restart capability, online help screens, and a browser that displays teacher-prepared lessons in turbomachinery. The program runs on a variety of workstations or a personal computer using the UNIX operating system and X-based graphics. It is being tested at several universities in the midwestern United States; the source and executables are available free from the author.

  10. The main beam correction term in kinetic energy release from metastable peaks.

    PubMed

    Petersen, Allan Christian

    2017-12-01

    The correction term for the precursor ion signal width in determination of kinetic energy release is reviewed, and the correction term is formally derived. The derived correction term differs from the traditionally applied term. An experimental finding substantiates the inaccuracy in the latter. The application of the "T-value" to study kinetic energy release is found preferable to kinetic energy release distributions when the metastable peaks are slim and simple Gaussians. For electronically predissociated systems, a "borderline zero" kinetic energy release can be directly interpreted in reaction dynamics with strong curvature in the reaction coordinate. Copyright © 2017 John Wiley & Sons, Ltd.

  11. A Microelectromechanical High-Density Energy Storage/Rapid Release System

    DOE Office of Scientific and Technical Information (OSTI.GOV)

    Rodgers, M. Steven; Allen, Jim J.; Meeks, Kent D.

    1999-07-21

    One highly desirable characteristic of electrostatically driven microelectromechanical systems (MEMS) is that they consume very little power. The corresponding drawback is that the force they produce may be inadequate for many applications. It has previously been demonstrated that gear reduction units or microtransmissions can substantially increase the torque generated by microengines. Operating speed, however, is also reduced by the transmission gear ratio. Some applications require both high speed and high force. If this output is only required for a limited period of time, then energy could be stored in a mechanical system and rapidly released upon demand. We have designed,more » fabricated, and demonstrated a high-density energy storage/rapid release system that accomplishes this task. Built using a 5-level surface micromachining technology, the assembly closely resembles a medieval crossbow. Energy releases on the order of tens of nanojoules have already been demonstrated, and significantly higher energy systems are under development.« less

  12. Dark Energy Survey releases early data | News

    Science.gov Websites

    released to the public. Astronomers and astronomy buffs can download the data from the website for the of all the images taken for the Dark Energy Survey. This is good news for the astronomy community, as Optical Astronomy Observatory's Cerro Tololo Inter-American Observatory in Chile. The Dark Energy Survey

  13. Dike propagation energy balance from deformation modeling and seismic release

    NASA Astrophysics Data System (ADS)

    Bonaccorso, Alessandro; Aoki, Yosuke; Rivalta, Eleonora

    2017-06-01

    Magma is transported in the crust mainly by dike intrusions. In volcanic areas, dikes can ascend toward the free surface and also move by lateral propagation, eventually feeding flank eruptions. Understanding dike mechanics is a key to forecasting the expected propagation and associated hazard. Several studies have been conducted on dike mechanisms and propagation; however, a less in-depth investigated aspect is the relation between measured dike-induced deformation and the seismicity released during its propagation. We individuated a simple x that can be used as a proxy of the expected mechanical energy released by a propagating dike and is related to its average thickness. For several intrusions around the world (Afar, Japan, and Mount Etna), we correlate such mechanical energy to the seismic moment released by the induced earthquakes. We obtain an empirical law that quantifies the expected seismic energy released before arrest. The proposed approach may be helpful to predict the total seismic moment that will be released by an intrusion and thus to control the energy status during its propagation and the time of dike arrest.Plain Language SummaryDike propagation is a dominant mechanism for magma ascent, transport, and eruptions. Besides being an intriguing physical process, it has critical hazard implications. After the magma intrusion starts, it is difficult to predict when and where a specific horizontal dike is going to halt and what its final length will be. In our study, we singled an equation that can be used as a proxy of the expected mechanical <span class="hlt">energy</span> to be <span class="hlt">released</span> by the opening dike. We related this expected <span class="hlt">energy</span> to the seismic moment of several eruptive intrusions around the world (Afar region, Japanese volcanoes, and Mount Etna). The proposed novel approach is helpful to estimate the total seismic moment to be <span class="hlt">released</span>, therefore allowing potentially predicting when the dike will end its propagation</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.eia.gov/outlooks/archive/aeo10/carbon_dioxide.html','EIAPUBS'); return false;" href="https://www.eia.gov/outlooks/archive/aeo10/carbon_dioxide.html"><span>Accounting for Carbon Dioxide Emissions from Biomass <span class="hlt">Energy</span> Combustion (<span class="hlt">released</span> in AEO2010)</span></a></p> <p><a target="_blank" href="http://www.eia.doe.gov/reports/">EIA Publications</a></p> <p></p> <p>2010-01-01</p> <p>Carbon Dioxide (CO2) emissions from the combustion of biomass to produce <span class="hlt">energy</span> are excluded from the <span class="hlt">energy</span>-related CO2 emissions reported in Annual <span class="hlt">Energy</span> Outlook 2010. According to current international convention, carbon <span class="hlt">released</span> through biomass combustion is excluded from reported <span class="hlt">energy</span>-related emissions. The <span class="hlt">release</span> of carbon from biomass combustion is assumed to be balanced by the uptake of carbon when the feedstock is grown, resulting in zero net emissions over some period of time]. However, analysts have debated whether increased use of biomass <span class="hlt">energy</span> may result in a decline in terrestrial carbon stocks, leading to a net positive <span class="hlt">release</span> of carbon rather than the zero net <span class="hlt">release</span> assumed by its exclusion from reported <span class="hlt">energy</span>-related emissions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22679462-simulation-radiation-energy-release-air-showers','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22679462-simulation-radiation-energy-release-air-showers"><span>Simulation of radiation <span class="hlt">energy</span> <span class="hlt">release</span> in air showers</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Glaser, Christian; Erdmann, Martin; Hörandel, Jörg R.</p> <p>2016-09-01</p> <p>A simulation study of the <span class="hlt">energy</span> <span class="hlt">released</span> by extensive air showers in the form of MHz radiation is performed using the CoREAS simulation code. We develop an efficient method to extract this radiation <span class="hlt">energy</span> from air-shower simulations. We determine the longitudinal profile of the radiation <span class="hlt">energy</span> <span class="hlt">release</span> and compare it to the longitudinal profile of the <span class="hlt">energy</span> deposit by the electromagnetic component of the air shower. We find that the radiation <span class="hlt">energy</span> corrected for the geometric dependence of the geomagnetic emission scales quadratically with the <span class="hlt">energy</span> in the electromagnetic component of the air shower with a second-order dependence on themore » atmospheric density at the position of the maximum shower development X {sub max}. In a measurement where X {sub max} is not accessible, this second order dependence can be approximated using the zenith angle of the incoming direction of the air shower with only a minor loss in accuracy. Our method results in an intrinsic uncertainty of 4% in the determination of the <span class="hlt">energy</span> in the electromagnetic air-shower component, which is well below current experimental uncertainties.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/7328736-control-installation-proportioning-secondary-air-quantity-improvement-combustion-internal-combustion-engines-afterburning-exhaust-gases-internal-combustion-engines','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/7328736-control-installation-proportioning-secondary-air-quantity-improvement-combustion-internal-combustion-engines-afterburning-exhaust-gases-internal-combustion-engines"><span>Control installation for the proportioning of a secondary air quantity for improvement of the combustion in internal combustion engines or the <span class="hlt">afterburning</span> of the exhaust gases of internal combustion engines</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Bockelmann, W.; Groezinger, H.; Woebky, P.U.</p> <p>1977-01-04</p> <p>A control installation is described for the dosing or proportioning of a secondary air quantity for the improvement of combustion in internal combustion engines, or the <span class="hlt">after-burning</span> of the exhaust gases of internal combustion engines. An auxiliary arrangement is responsive to an emergency signal for effecting the prompt shutting-off of the secondary air. The emergency signal may be initiated in response to a failure in the ignition voltage of the internal combustion engine; an increase in the hydrocarbon content of the exhaust gases; a disparity between the position of the mixture dosing element and the engine rotational speed; the exceedingmore » of a limiting temperature in the exhaust gas manifold; or the exceeding of a limiting temperature in the <span class="hlt">afterburner</span>.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JGRA..123.2513Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JGRA..123.2513Z"><span>Coronal Flux Rope Catastrophe Associated With Internal <span class="hlt">Energy</span> <span class="hlt">Release</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zhuang, Bin; Hu, Youqiu; Wang, Yuming; Zhang, Quanhao; Liu, Rui; Gou, Tingyu; Shen, Chenglong</p> <p>2018-04-01</p> <p>Magnetic <span class="hlt">energy</span> during the catastrophe was predominantly studied by the previous catastrophe works since it is believed to be the main <span class="hlt">energy</span> supplier for the solar eruptions. However, the contribution of other types of <span class="hlt">energies</span> during the catastrophe cannot be neglected. This paper studies the catastrophe of the coronal flux rope system in the solar wind background, with emphasis on the transformation of different types of <span class="hlt">energies</span> during the catastrophe. The coronal flux rope is characterized by its axial and poloidal magnetic fluxes and total mass. It is shown that a catastrophe can be triggered by not only an increase but also a decrease of the axial magnetic flux. Moreover, the internal <span class="hlt">energy</span> of the rope is found to be <span class="hlt">released</span> during the catastrophe so as to provide <span class="hlt">energy</span> for the upward eruption of the flux rope. As far as the magnetic <span class="hlt">energy</span> is concerned, it provides only part of the <span class="hlt">energy</span> <span class="hlt">release</span>, or even increases during the catastrophe, so the internal <span class="hlt">energy</span> may act as the dominant or even the unique <span class="hlt">energy</span> supplier during the catastrophe.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018SPIE10595E..10K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018SPIE10595E..10K"><span><span class="hlt">Energy</span> <span class="hlt">release</span> for the actuation and deployment of muscle-inspired asymmetrically multistable chains</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kidambi, Narayanan; Zheng, Yisheng; Harne, Ryan L.; Wang, K. W.</p> <p>2018-03-01</p> <p>Animal locomotion and movement requires <span class="hlt">energy</span>, and the elastic potential <span class="hlt">energy</span> stored in skeletal muscle can facilitate movements that are otherwise energetically infeasible. A significant proportion of this <span class="hlt">energy</span> is captured and stored in the micro- and nano-scale constituents of muscle near the point of instability between asymmetric equilibrium states. This <span class="hlt">energy</span> may be quickly <span class="hlt">released</span> to enable explosive macroscopic motions or to reduce the metabolic cost of cyclic movements. Inspired by these behaviors, this research explores modular metastructures of bistable element chains and develops methods to <span class="hlt">release</span> the <span class="hlt">energy</span> stored in higher-potential system configurations. Quasi-static investigations reveal the role of state-transition pathways on the overall efficiency of the deployment event. It is shown that sequential, local <span class="hlt">release</span> of <span class="hlt">energy</span> from the bistable elements is more efficient than concurrent <span class="hlt">energy</span> <span class="hlt">release</span> achieved by applying a force at the free end of the structure. From dynamic analyses and experiments, it is shown that that the <span class="hlt">energy</span> <span class="hlt">released</span> from one bistable element can be used to activate the <span class="hlt">release</span> of <span class="hlt">energy</span> from subsequent links, reducing the actuation <span class="hlt">energy</span> required to extend or deploy the chain below that required for quasi-static deployment. This phenomenon is influenced by the level of asymmetry in the bistable constituents and the location of the impulse that initiates the deployment of the structure. The results provide insight into the design and behavior of asymmetrically multistable chains that can leverage stored potential <span class="hlt">energy</span> to enable efficient and effective system deployment and length change.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1999PhDT.......198W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1999PhDT.......198W"><span>Triggered instabilities in rocket motors and active combustion control for an incinerator <span class="hlt">afterburner</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wicker, Josef M.</p> <p>1999-11-01</p> <p>Two branches of research are conducted in this thesis. The first deals with nonlinear combustion response as a mechanism for triggering combustion instabilities in solid rocket motors. A nonlinear wave equation is developed to study a wide class of combustion response functions to second-order in fluctuation amplitude. Conditions for triggering are derived from analysis of limit cycles, and regions of triggering are found in parametric space. Introduction of linear cross-coupling and quadratic self-coupling among the acoustic modes appears to be how the nonlinear combustion response produces triggering to a stable limit cycle. Regions of initial conditions corresponding to stable pulses were found, suggesting that stability depends on initial phase angle and harmonic content, as well as the composite amplitude, of the pulse. Also, dependence of nonlinear stability upon system parameters is considered. The second part of this thesis presents research for a controller to improve the emissions of an incinerator <span class="hlt">afterburner</span>. The developed controller was experimentally tested at the Naval Air Warfare Center (NAWC), on a 50kW-scale model of an <span class="hlt">afterburner</span> for Naval shipboard incinerator applications. Acoustic forcing of the combustor's reacting shear layer is used to control the formation of coherent vortical structures, within which favorable fuel-air mixing and efficient combustion can occur. Laser-based measurements of CO emissions are used as the performance indicator for the combustor. The controller algorithm is based on the downhill simplex method and adjusts the shear layer forcing parameters in order to minimize the CO emissions. The downhill simplex method was analyzed with respect to its behavior in the face of time-variation of the plant and noise in the sensor signal, and was modified to account for these difficulties. The control system has experimentally demonstrated the ability (1) to find optimal control action for single- and multi-variable control, (2</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19770008588','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19770008588"><span>A computer simulation of the <span class="hlt">afterburning</span> processes occurring within solid rocket motor plumes in the troposphere</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Gomberg, R. I.; Stewart, R. B.</p> <p>1976-01-01</p> <p>As part of a continuing study of the environmental effects of solid rocket motor (SRM) operations in the troposphere, a numerical model was used to simulate the <span class="hlt">afterburning</span> processes occurring in solid rocket motor plumes and to predict the quantities of potentially harmful chemical species which are created. The calculations include the effects of finite-rate chemistry and turbulent mixing. It is found that the amount of NO produced is much less than the amount of HCl present in the plume, that chlorine will appear predominantly in the form of HCl although some molecular chlorine is present, and that combustion is complete as is evident from the predominance of carbon dioxide over carbon monoxide.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_3");'>3</a></li> <li><a href="#" onclick='return showDiv("page_4");'>4</a></li> <li class="active"><span>5</span></li> <li><a href="#" onclick='return showDiv("page_6");'>6</a></li> <li><a href="#" onclick='return showDiv("page_7");'>7</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_5 --> <div id="page_6" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_4");'>4</a></li> <li><a href="#" onclick='return showDiv("page_5");'>5</a></li> <li class="active"><span>6</span></li> <li><a href="#" onclick='return showDiv("page_7");'>7</a></li> <li><a href="#" onclick='return showDiv("page_8");'>8</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="101"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19740004458','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19740004458"><span>Spontaneous ignition in <span class="hlt">afterburner</span> segment tests at an inlet temperature of 1240 K and a pressure of 1 atmosphere with ASTM jet-A fuel</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Schultz, D. F.; Branstetter, J. R.</p> <p>1973-01-01</p> <p>A brief testing program was undertaken to determine if spontaneous ignition and stable combustion could be obtained in a jet engine <span class="hlt">afterburning</span> operating with an inlet temperature of 1240 K and a pressure of 1 atmosphere with ASTM Jet-A fuel. Spontaneous ignition with 100-percent combustion efficiency and stable burning was obtained using water-cooled fuel spraybars as flameholders.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28521230','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28521230"><span><span class="hlt">Energy</span> consumption and water-soluble protein <span class="hlt">release</span> by cell wall disruption of Nannochloropsis gaditana.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Safi, C; Cabas Rodriguez, L; Mulder, W J; Engelen-Smit, N; Spekking, W; van den Broek, L A M; Olivieri, G; Sijtsma, L</p> <p>2017-09-01</p> <p>Several cell disruption methods were tested on Nannochloropsis gaditana, to evaluate their efficiency in terms of cell disintegration, <span class="hlt">energy</span> input and <span class="hlt">release</span> of soluble proteins. High-pressure homogenization (HPH) and bead milling were the most efficient with >95% cell disintegration, ±50% (w/w) <span class="hlt">release</span> of total proteins and low <span class="hlt">energy</span> input (<0.5kWh.kg -1 biomass ). Enzymatic treatment required low <span class="hlt">energy</span> input (<0.34kWh.kg -1 biomass ), but it only <span class="hlt">released</span> ±35% protein (w/w). Pulsed Electric Field (PEF) was neither <span class="hlt">energy</span>-efficient (10.44kWh.kg -1 biomass ) nor successful for protein <span class="hlt">release</span> (only 10% proteins w/w) and cell disintegration. The <span class="hlt">release</span> of proteins after applying HPH and bead milling always required less intensive operating conditions for cell disruption. The <span class="hlt">energy</span> cost per unit of <span class="hlt">released</span> protein ranged from 0.15-0.25 €.kg Protein -1 in case of HPH, and up to 2-20 €.kg Protein -1 in case of PEF. Copyright © 2017 Elsevier Ltd. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/1402583-miniature-bulge-test-energy-release-rate-hiped-aluminum-aluminum-interfacial-fracture','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/1402583-miniature-bulge-test-energy-release-rate-hiped-aluminum-aluminum-interfacial-fracture"><span>Miniature bulge test and <span class="hlt">energy</span> <span class="hlt">release</span> rate in HIPed aluminum/aluminum interfacial fracture</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Liu, C.; Lovato, M. L.; Clarke, K. D.</p> <p></p> <p>We summarize the development of a technique of using miniature bulge test combined with three-dimensional digital image correlation (3D-DIC) for measuring <span class="hlt">energy</span> <span class="hlt">release</span> rate or fracture toughness of bimaterial interface of thin metal foils. Furthermore, the <span class="hlt">energy</span> <span class="hlt">release</span> rate associated with the HIPed aluminum/aluminum interfacial delamination is determined experimentally using the proposed technique. Detailed discussions of the schemes of preparing and conducting the bulge test, and computing various quantities required for the determination of the <span class="hlt">energy</span> <span class="hlt">release</span> rate are presented.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1402583-miniature-bulge-test-energy-release-rate-hiped-aluminum-aluminum-interfacial-fracture','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1402583-miniature-bulge-test-energy-release-rate-hiped-aluminum-aluminum-interfacial-fracture"><span>Miniature bulge test and <span class="hlt">energy</span> <span class="hlt">release</span> rate in HIPed aluminum/aluminum interfacial fracture</span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Liu, C.; Lovato, M. L.; Clarke, K. D.; ...</p> <p>2017-10-13</p> <p>We summarize the development of a technique of using miniature bulge test combined with three-dimensional digital image correlation (3D-DIC) for measuring <span class="hlt">energy</span> <span class="hlt">release</span> rate or fracture toughness of bimaterial interface of thin metal foils. Furthermore, the <span class="hlt">energy</span> <span class="hlt">release</span> rate associated with the HIPed aluminum/aluminum interfacial delamination is determined experimentally using the proposed technique. Detailed discussions of the schemes of preparing and conducting the bulge test, and computing various quantities required for the determination of the <span class="hlt">energy</span> <span class="hlt">release</span> rate are presented.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19870052744&hterms=Magnetic+energy&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3DMagnetic%2Benergy','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19870052744&hterms=Magnetic+energy&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3DMagnetic%2Benergy"><span>Observed form and action of the magnetic <span class="hlt">energy</span> <span class="hlt">release</span> in flares</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Machado, Marcos E.; Moore, Ronald L.</p> <p>1986-01-01</p> <p>The observable spatio-temporal characteristics of the <span class="hlt">energy</span> <span class="hlt">release</span> in flares and their association with the magnetic environment and tracers of field dynamics are reviewed. The observations indicate that impulsive phase manifestations, like particle acceleration, may be related to the formation of neutral sheets at the interface between interacting bipoles, but that the site for the bulk of the <span class="hlt">energy</span> <span class="hlt">release</span> is within closed loops rather than at the interaction site.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19730020187','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19730020187"><span><span class="hlt">Afterburner</span> performance of film-vaporizing V-gutters for inlet temperatures up to 1255 K</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Branstetter, J. R.; Reck, G. M.</p> <p>1973-01-01</p> <p>Combustion tests of five variations of an integral, spray-bar - flameholder combination were conducted in a 0.49-m-diameter duct. Emphasis was on low levels of augmentation. Fuel impinged on guide plates, mixed with a controlled amount of inlet air, vaporized, and was guided into the V-gutter wake. Combustor length was 0.92 m. Good performance was demonstrated at fuel-air ratios less than 0.025 for inlet temperatures of 920 to 1255 K. Maximum combustion efficiency occured in the vicinity of fuel-air ratios of 0.02 and was 92 to 100 percent, depending on the inlet temperature. Lean blowout fuel-air ratios were in the vicinity of 0.005. Improvements in rich-limit blowout resulted from enlarging the guide-flow passageway areas. Other means of extending the operating range are suggested. A simplified <span class="hlt">afterburner</span> concept for application to advanced engines is described.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19850022925','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19850022925"><span>Residual thermal and moisture influences on the strain <span class="hlt">energy</span> <span class="hlt">release</span> rate analysis of edge delamination</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Obrien, T. K.; Raju, I. S.; Garber, D. P.</p> <p>1985-01-01</p> <p>A laminated plate theory analysis is developed to calculate the strain <span class="hlt">energy</span> <span class="hlt">release</span> rate associated with edge delamination growth in a composite laminate. The analysis includes the contribution of residual thermal and moisture stresses to the strain <span class="hlt">energy</span> <span class="hlt">released</span>. The strain <span class="hlt">energy</span> <span class="hlt">release</span> rate, G, increased when residual thermal effects were combined with applied mechanical strains, but then decreased when increasing moisture content was included. A quasi-three-dimensional finite element analysis indicated identical trends and demonstrated these same trends for the individual strain <span class="hlt">energy</span> <span class="hlt">release</span> rate components, G sub I and G sub II, associated with interlaminar tension and shear. An experimental study indicated that for T300/5208 graphite-epoxy composites, the inclusion of residual thermal and moisture stresses did not significantly alter the calculation of interlaminar fracture toughness from strain <span class="hlt">energy</span> <span class="hlt">release</span> rate analysis of edge delamination data taken at room temperature, ambient conditions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/1418771-total-kinetic-energy-release-fast-neutron-induced-fission','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/1418771-total-kinetic-energy-release-fast-neutron-induced-fission"><span>The total kinetic <span class="hlt">energy</span> <span class="hlt">release</span> in the fast neutron-induced fission of 232Th</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>King, Jonathan; Yanez, Ricardo; Loveland, Walter</p> <p></p> <p>Here, the post-emission total kinetic <span class="hlt">energy</span> <span class="hlt">release</span> (TKE) in the neutron-induced fission of 232Th was measured (using white spectrum neutrons from LANSCE) for neutron <span class="hlt">energies</span> from E n=3 to 91MeV. In this <span class="hlt">energy</span> range the average post-neutron total kinetic <span class="hlt">energy</span> <span class="hlt">release</span> decreases from 162.3±0.3 at E n=3 MeV to 154.9±0.3 MeV at E n=91 MeV. Analysis of the fission mass distributions indicates that the decrease in TKE with increasing neutron <span class="hlt">energy</span> is a combination of increasing yields of symmetric fission (which has a lower associated TKE) and a decrease in the TKE <span class="hlt">release</span> in asymmetric fission.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1418771-total-kinetic-energy-release-fast-neutron-induced-fission','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1418771-total-kinetic-energy-release-fast-neutron-induced-fission"><span>The total kinetic <span class="hlt">energy</span> <span class="hlt">release</span> in the fast neutron-induced fission of 232Th</span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>King, Jonathan; Yanez, Ricardo; Loveland, Walter; ...</p> <p>2017-12-15</p> <p>Here, the post-emission total kinetic <span class="hlt">energy</span> <span class="hlt">release</span> (TKE) in the neutron-induced fission of 232Th was measured (using white spectrum neutrons from LANSCE) for neutron <span class="hlt">energies</span> from E n=3 to 91MeV. In this <span class="hlt">energy</span> range the average post-neutron total kinetic <span class="hlt">energy</span> <span class="hlt">release</span> decreases from 162.3±0.3 at E n=3 MeV to 154.9±0.3 MeV at E n=91 MeV. Analysis of the fission mass distributions indicates that the decrease in TKE with increasing neutron <span class="hlt">energy</span> is a combination of increasing yields of symmetric fission (which has a lower associated TKE) and a decrease in the TKE <span class="hlt">release</span> in asymmetric fission.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19740019462','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19740019462"><span>Development of integrated, zero-G pneumatic transporter/rotating paddle incinerator/catalytic <span class="hlt">afterburner</span> subsystem for processing human wastes on board spacecraft</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Fields, S. F.; Labak, L. J.; Honegger, R. J.</p> <p>1974-01-01</p> <p>A four component system was developed which consists of a particle size reduction mechanism, a pneumatic waste transport system, a rotating-paddle incinerator, and a catalytic <span class="hlt">afterburner</span> to be integrated into a six-man, zero-g subsystem for processing human wastes on board spacecraft. The study included the development of different concepts or functions, the establishment of operational specifications, and a critical evaluation for each of the four components. A series of laboratory tests was run, and a baseline subsystem design was established. An operational specification was also written in preparation for detailed design and testing of this baseline subsystem.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19820051443&hterms=1044&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3D%2526%25231044','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19820051443&hterms=1044&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3D%2526%25231044"><span>Evaluation of a simplified gross thrust calculation method for a J85-21 <span class="hlt">afterburning</span> turbojet engine in an altitude facility</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Baer-Riedhart, J. L.</p> <p>1982-01-01</p> <p>A simplified gross thrust calculation method was evaluated on its ability to predict the gross thrust of a modified J85-21 engine. The method used tailpipe pressure data and ambient pressure data to predict the gross thrust. The method's algorithm is based on a one-dimensional analysis of the flow in the <span class="hlt">afterburner</span> and nozzle. The test results showed that the method was notably accurate over the engine operating envelope using the altitude facility measured thrust for comparison. A summary of these results, the simplified gross thrust method and requirements, and the test techniques used are discussed in this paper.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017SPIE10237E..0ZL','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017SPIE10237E..0ZL"><span>Magnetic force study for the helical <span class="hlt">afterburner</span> for the European XFEL</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Li, Peng; Wei, Tao; Li, Yuhui; Pflueger, Joachim</p> <p>2017-05-01</p> <p>At present the SASE3 undulator line at the European XFEL is using a planar undulator producing linear polarized soft Xray radiation only. In order to satisfy the demand for circular polarized radiation a helical undulator system, the so-called <span class="hlt">afterburner</span> is in construction. It will be operated as a radiator using the pre-bunched beam of the SASE3 undulator system. Among several options for the magnetic structure the Apple-X geometry was chosen. This is a pure permanent magnet undulator using NdFeB material. Four magnet arrays are arranged symmetrically the beam axis. Polarization can be changed by adjusting the phase shift (PS) between the two orthogonal structures. The field strength can be adjusted either by gap adjustment or alternatively by the amplitude shift (AS) scheme. For an engineering design the maximum values of forces and torques on each of the components under worst case operational conditions are important. The superposition principle is used to reduce calculation time. It is found that the maximum forces Fx, Fy and Fz for a 2m long Apple-X undulator are 1.8*104N, 2.4*104N and 2.3*104N, respectively. More results are presented in this paper.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27762047','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27762047"><span>A Responsive Battery with Controlled <span class="hlt">Energy</span> <span class="hlt">Release</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Wang, Xiaopeng; Gao, Jian; Cheng, Zhihua; Chen, Nan; Qu, Liangti</p> <p>2016-11-14</p> <p>A new type of responsive battery with the fascinating feature of pressure perceptibility has been developed, which can spontaneously, timely and reliably control the power outputs (e.g., current and voltage) in response to pressure changes. The device design is based on the structure of the Zn-air battery, in which graphene-coated sponge serves as pressure-sensitive air cathode that endows the whole system with the capability of self-controlled <span class="hlt">energy</span> <span class="hlt">release</span>. The responsive batteries exhibit superior battery performance with high open-circuit voltage (1.3 V), and competitive areal capacity of 1.25 mAh cm -2 . This work presents an important move towards next-generation intelligent <span class="hlt">energy</span> storage devices with <span class="hlt">energy</span> management function. © 2016 Wiley-VCH Verlag GmbH & Co. KGaA, Weinheim.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018AAS...23121901C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018AAS...23121901C"><span>The Dark <span class="hlt">Energy</span> Survey First Data <span class="hlt">Release</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Carrasco Kind, Matias</p> <p>2018-01-01</p> <p>In this talk I will announce and highlight the main components of the first public data <span class="hlt">release</span> (DR1) coming from the Dark <span class="hlt">Energy</span> Survey (DES).In January 2016, the DES survey made available, in a simple unofficial <span class="hlt">release</span> to the astronomical community, the first set of products. This data was taken and studied during the DES Science Verification period consisting on roughly 250 sq. degrees and 25 million objects at a mean depth of i=23.7 that led to over 80 publications from DES scientist.The DR1 <span class="hlt">release</span> is the first official <span class="hlt">release</span> from the main survey and it consists on the observations taken during the first 3 seasons from August 2013 to February 2016 (about 100 nights each season) of the survey which cover the entire DES footprint. All of the Single Epoch Images and the Year 3 Coadded images distributed in 10223 tiles are available for download in this <span class="hlt">release</span>. The catalogs provide astrometry, photometry and basic classification for near 400M objects in roughly 5000 sq. degrees on the southern hemisphere with a approximate mean depth of i=23.3. Complementary footprint, masking and depth information is also available. All of the software used during the generation of these products are open sourced and have been made available through the Github DES Organization. Images, data and other sub products have been possible through the international and collaborative effort of all 25 institutions involved in DES and are available for exploration and download through the interfaces provided by a partnership between NCSA, NOAO and LIneA.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28508907','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28508907"><span>An effective trigger for <span class="hlt">energy</span> <span class="hlt">release</span> of vinylheptafulvene-based solar heat batteries.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Cacciarini, Martina; Vlasceanu, Alexandru; Jevric, Martyn; Nielsen, Mogens Brøndsted</p> <p>2017-05-30</p> <p>Stoichiometric copper(i) tetrakis(acetonitrile) is found to activate the thermal ring-closure reaction of a series of high-<span class="hlt">energy</span> vinylheptafulvene isomers to the corresponding low-<span class="hlt">energy</span> and photoactive dihydroazulenes, allowing the <span class="hlt">release</span> of <span class="hlt">energy</span> upon request.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018AcAau.147..281C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018AcAau.147..281C"><span>Numerical analysis and design optimization of supersonic <span class="hlt">after-burning</span> with strut fuel injectors for scramjet engines</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Candon, M. J.; Ogawa, H.</p> <p>2018-06-01</p> <p>Scramjets are a class of hypersonic airbreathing engine that offer promise for economical, reliable and high-speed access-to-space and atmospheric transport. The expanding flow in the scramjet nozzle comprises of unburned hydrogen. An <span class="hlt">after-burning</span> scheme can be used to effectively utilize the remaining hydrogen by supplying additional oxygen into the nozzle, aiming to augment the thrust. This paper presents the results of a single-objective design optimization for a strut fuel injection scheme considering four design variables with the objective of maximizing thrust augmentation. Thrust is found to be augmented significantly owing to a combination of contributions from aerodynamic and combustion effects. Further understanding and physical insights have been gained by performing variance-based global sensitivity analysis, scrutinizing the nozzle flowfields, analyzing the distributions and contributions of the forces acting on the nozzle wall, and examining the combustion efficiency.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20140001072','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20140001072"><span>The Role of Compressibility in <span class="hlt">Energy</span> <span class="hlt">Release</span> by Magnetic Reconnection</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Birn, J.; Borovosky, J. E.; Hesse, M.</p> <p>2012-01-01</p> <p>Using resistive compressible magnetohydrodynamics, we investigate the <span class="hlt">energy</span> <span class="hlt">release</span> and transfer by magnetic reconnection in finite (closed or periodic) systems. The emphasis is on the magnitude of <span class="hlt">energy</span> <span class="hlt">released</span> and transferred to plasma heating in configurations that range from highly compressible to incompressible, based on the magnitude of the background beta (ratio of plasma pressure over magnetic pressure) and of a guide field in two-dimensional reconnection. As expected, the system becomes more incompressible, and the role of compressional heating diminishes, with increasing beta or increasing guide field. Nevertheless, compressional heating may dominate over Joule heating for values of the guide field of 2 or 3 (in relation to the reconnecting magnetic field component) and beta of 5-10. This result stems from the strong localization of the dissipation near the reconnection site, which is modeled based on particle simulation results. Imposing uniform resistivity, corresponding to a Lundquist number of 10(exp 3) to 10(exp 4), leads to significantly larger Ohmic heating. Increasing incompressibility greatly reduces the magnetic flux transfer and the amount of <span class="hlt">energy</span> <span class="hlt">released</span>, from approx. 10% of the <span class="hlt">energy</span> associated with the reconnecting field component, for zero guide field and low beta, to approx. 0.2%-0.4% for large values of the guide field B(sub y0) > 5 or large beta. The results demonstrate the importance of taking into account plasma compressibility and localization of dissipation in investigations of heating by turbulent reconnection, possibly relevant for solar wind or coronal heating.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFMMR51B2708M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFMMR51B2708M"><span>Strain Rate Dependency of Fracture Toughness, <span class="hlt">Energy</span> <span class="hlt">Release</span> Rate and Geomechanical Attributes of Select Indian Shales</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Mahanta, B.; Vishal, V.; Singh, T. N.; Ranjith, P.</p> <p>2016-12-01</p> <p>In addition to modern improved technology, it requires detailed understanding of rock fractures for the purpose of enhanced <span class="hlt">energy</span> extraction through hydraulic fracturing of gas shales and geothermal <span class="hlt">energy</span> systems. The understanding of rock fracture behavior, patterns and properties such as fracture toughness; <span class="hlt">energy</span> <span class="hlt">release</span> rate; strength and deformation attributes during fracturing hold significance. Environmental factors like temperature, pressure, humidity, water vapor and experimental condition such as strain rate influence the estimation of these properties. In this study, the effects of strain rates on fracture toughness, <span class="hlt">energy</span> <span class="hlt">release</span> rate as well as geomechanical properties like uniaxial compressive strength, Young's modulus, failure strain, tensile strength, and brittleness index of gas shales were investigated. In addition to the rock-mechanical parameters, the fracture toughness and the <span class="hlt">energy</span> <span class="hlt">release</span> rates were measured for three different modes viz. mode I, mixed mode (I-II) and mode II. Petrographic and X-ray diffraction (XRD) analyses were performed to identify the mineral composition of the shale samples. Scanning electron microscope (SEM) analyses were conducted to have an insight about the strain rate effects on micro-structure of the rock. The results suggest that the fracture toughness; the <span class="hlt">energy</span> <span class="hlt">release</span> rate as well as other geomechanical properties are a function of strain rates. At high strain rates, the strength and stiffness of shale increases which in turn increases the fracture toughness and the <span class="hlt">energy</span> <span class="hlt">release</span> rate of shale that may be due to stress redistribution during grain fracturing. The fracture toughness and the strain <span class="hlt">energy</span> <span class="hlt">release</span> rates for all the modes (I/I-II/II) are comparable at lower strain rates, but they vary considerably at higher strain rates. In all the cases, mode I and mode II fracturing requires minimum and maximum applied <span class="hlt">energy</span>, respectively. Mode I <span class="hlt">energy</span> <span class="hlt">release</span> rate is maximum, compared to the other modes.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/7347667-apparatus-afterburning-exhaust-gases-internal-combustion-engine-remove-pollutants-therefrom','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/7347667-apparatus-afterburning-exhaust-gases-internal-combustion-engine-remove-pollutants-therefrom"><span>Apparatus for <span class="hlt">afterburning</span> the exhaust gases of an internal combustion engine to remove pollutants therefrom</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Laurent, P.A.</p> <p>1976-09-28</p> <p>An apparatus is described for <span class="hlt">afterburning</span> the combustible pollutants from the exhaust gases of an internal combustion engine in a reactor, in which secondary air is introduced. Upstream of the reactor, a chamber in the form of a torus is provided, through which the exhaust gases from a maximum number of cylinders flow before entering the reactor. A first obstacle, acting as a flame holder is disposed inside the torus. The reactor comprises a chamber whose inner surface is approximately a surface of revolution, and mounted inside of which is a second obstacle, acting as flame holder, substantially along themore » axis of revolution. The second flame holder has a diameter large enough to provide a contact time of 1 to 3 x 10/sup -3/ seconds of the gas flow in a recirculation zone surrounding the second flame holder, the diameter of the second flame holder being 15 to 40 percent of the reactor diameter.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017ASPC..510..289P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017ASPC..510..289P"><span>Flare <span class="hlt">Energy</span> <span class="hlt">Release</span>: Internal Conflict, Contradiction with High Resolution Observations, Possible Solutions</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Pustilnik, L.</p> <p>2017-06-01</p> <p>All accepted paradigm of solar and stellar flares <span class="hlt">energy</span> <span class="hlt">release</span> based on 2 whales: 1. Source of <span class="hlt">energy</span> is free <span class="hlt">energy</span> of non-potential force free magnetic field in atmosphere above active region; 2. Process of ultrafast dissipation of magnetic fields is Reconnection in Thin Turbulent Current Sheet (RTTCS). Progress in observational techniques in last years provided ultra-high spatial resolution and in physics of turbulent plasma showed that real situation is much more complicated and standard approach is in contradiction both with observations and with problem of RTTCS stability. We present critical analysis of classic models of pre-flare <span class="hlt">energy</span> accumulation and its dissipation during flare <span class="hlt">energy</span> <span class="hlt">release</span> from pioneer works Giovanelli (1939, 1947) up to topological reconnection. We show that all accepted description of global force-free fields as source of future flare cannot be agreed with discovered in last years fine and ultra-fine current-magnetic structure included numerouse arcs-threads with diameters up to 100 km with constant sequence from photosphere to corona. This magnetic skeleton of thin current magnetic threads with strong interaction between them is main source of reserved magnetic <span class="hlt">energy</span> insolar atmosphere. Its dynamics will be controlled by percolation of magnetic stresses through network of current-magnetic threads with transition to flare state caused by critical value of global current. We show that thin turbulent current sheet is absolutely unstable configuration both caused by splitting to numerous linear currents by dissipative modes like to tearing, and as sequence of suppress of plasma turbulence caused by anomalous heating of turbulent plasma. In result of these factors primary RTTCS will be disrupted in numerous turbulent and normal plasma domains like to resistors network. Current propagation through this network will have percolation character with all accompanied properties of percolated systems: self-organization with formation power</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_4");'>4</a></li> <li><a href="#" onclick='return showDiv("page_5");'>5</a></li> <li class="active"><span>6</span></li> <li><a href="#" onclick='return showDiv("page_7");'>7</a></li> <li><a href="#" onclick='return showDiv("page_8");'>8</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_6 --> <div id="page_7" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_5");'>5</a></li> <li><a href="#" onclick='return showDiv("page_6");'>6</a></li> <li class="active"><span>7</span></li> <li><a href="#" onclick='return showDiv("page_8");'>8</a></li> <li><a href="#" onclick='return showDiv("page_9");'>9</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="121"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19770035709&hterms=Magnetic+energy&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D90%26Ntt%3DMagnetic%2Benergy','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19770035709&hterms=Magnetic+energy&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D90%26Ntt%3DMagnetic%2Benergy"><span><span class="hlt">Energy</span> <span class="hlt">released</span> by the interaction of coronal magnetic fields</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Sheeley, N. R., Jr.</p> <p>1976-01-01</p> <p>Comparisons between coronal spectroheliograms and photospheric magnetograms are presented to support the idea that as coronal magnetic fields interact, a process of field-line reconnection usually takes place as a natural way of preventing magnetic stresses from building up in the lower corona. This suggests that the <span class="hlt">energy</span> which would have been stored in stressed fields is continuously <span class="hlt">released</span> as kinetic <span class="hlt">energy</span> of material being driven aside to make way for the reconnecting fields. However, this kinetic <span class="hlt">energy</span> is negligible compared with the thermal <span class="hlt">energy</span> of the coronal plasma. Therefore, it appears that these slow adjustments of coronal magnetic fields cannot account for even the normal heating of the corona, much less the energetic events associated with solar flares.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/22745740','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/22745740"><span>Blast shock wave mitigation using the hydraulic <span class="hlt">energy</span> redirection and <span class="hlt">release</span> technology.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Chen, Yun; Huang, Wei; Constantini, Shlomi</p> <p>2012-01-01</p> <p>A hydraulic <span class="hlt">energy</span> redirection and <span class="hlt">release</span> technology has been developed for mitigating the effects of blast shock waves on protected objects. The technology employs a liquid-filled plastic tubing as a blast overpressure transformer to transfer kinetic <span class="hlt">energy</span> of blast shock waves into hydraulic <span class="hlt">energy</span> in the plastic tubings. The hydraulic <span class="hlt">energy</span> is redirected through the plastic tubings to the openings at the lower ends, and then is quickly <span class="hlt">released</span> with the liquid flowing out through the openings. The samples of the specifically designed body armor in which the liquid-filled plastic tubings were installed vertically as the outer layer of the body armor were tested. The blast test results demonstrated that blast overpressure behind the body armor samples was remarkably reduced by 97% in 0.2 msec after the liquid flowed out of its appropriate volume through the openings. The results also suggested that a volumetric liquid surge might be created when kinetic <span class="hlt">energy</span> of blast shock wave was transferred into hydraulic <span class="hlt">energy</span> to cause a rapid physical movement or displacement of the liquid. The volumetric liquid surge has a strong destructive power, and can cause a noncontact, remote injury in humans (such as blast-induced traumatic brain injury and post-traumatic stress disorder) if it is created in cardiovascular system. The hydraulic <span class="hlt">energy</span> redirection and <span class="hlt">release</span> technology can successfully mitigate blast shock waves from the outer surface of the body armor. It should be further explored as an innovative approach to effectively protect against blast threats to civilian and military personnel.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3379975','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3379975"><span>Blast Shock Wave Mitigation Using the Hydraulic <span class="hlt">Energy</span> Redirection and <span class="hlt">Release</span> Technology</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Chen, Yun; Huang, Wei; Constantini, Shlomi</p> <p>2012-01-01</p> <p>A hydraulic <span class="hlt">energy</span> redirection and <span class="hlt">release</span> technology has been developed for mitigating the effects of blast shock waves on protected objects. The technology employs a liquid-filled plastic tubing as a blast overpressure transformer to transfer kinetic <span class="hlt">energy</span> of blast shock waves into hydraulic <span class="hlt">energy</span> in the plastic tubings. The hydraulic <span class="hlt">energy</span> is redirected through the plastic tubings to the openings at the lower ends, and then is quickly <span class="hlt">released</span> with the liquid flowing out through the openings. The samples of the specifically designed body armor in which the liquid-filled plastic tubings were installed vertically as the outer layer of the body armor were tested. The blast test results demonstrated that blast overpressure behind the body armor samples was remarkably reduced by 97% in 0.2 msec after the liquid flowed out of its appropriate volume through the openings. The results also suggested that a volumetric liquid surge might be created when kinetic <span class="hlt">energy</span> of blast shock wave was transferred into hydraulic <span class="hlt">energy</span> to cause a rapid physical movement or displacement of the liquid. The volumetric liquid surge has a strong destructive power, and can cause a noncontact, remote injury in humans (such as blast-induced traumatic brain injury and post-traumatic stress disorder) if it is created in cardiovascular system. The hydraulic <span class="hlt">energy</span> redirection and <span class="hlt">release</span> technology can successfully mitigate blast shock waves from the outer surface of the body armor. It should be further explored as an innovative approach to effectively protect against blast threats to civilian and military personnel. PMID:22745740</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017APS..MARH16003I','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017APS..MARH16003I"><span>Unleashing elastic <span class="hlt">energy</span>: dynamics of <span class="hlt">energy</span> <span class="hlt">release</span> in rubber bands and impulsive biological systems</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ilton, Mark; Cox, Suzanne; Egelmeers, Thijs; Patek, S. N.; Crosby, Alfred J.</p> <p></p> <p>Impulsive biological systems - which include mantis shrimp, trap-jaw ants, and venus fly traps - can reach high speeds by using elastic elements to store and rapidly <span class="hlt">release</span> <span class="hlt">energy</span>. The material behavior and shape changes critical to achieving rapid <span class="hlt">energy</span> <span class="hlt">release</span> in these systems are largely unknown due to limitations of materials testing instruments operating at high speed and large displacement. In this work, we perform fundamental, proof-of-concept measurements on the tensile retraction of elastomers. Using high speed imaging, the kinematics of retraction are measured for elastomers with varying mechanical properties and geometry. Based on the kinematics, the rate of <span class="hlt">energy</span> dissipation in the material is determined as a function of strain and strain-rate, along with a scaling relation which describes the dependence of maximum velocity on material properties. Understanding this scaling relation along with the material failure limits of the elastomer allows the prediction of material properties required for optimal performance. We demonstrate this concept experimentally by optimizing for maximum velocity in our synthetic model system, and achieve retraction velocities that exceed those in biological impulsive systems. This model system provides a foundation for future work connecting continuum performance to molecular architecture in impulsive systems.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19870011944','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19870011944"><span>Convergence of strain <span class="hlt">energy</span> <span class="hlt">release</span> rate components for edge-delaminated composite laminates</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Raju, I. S.; Crews, J. H., Jr.; Aminpour, M. A.</p> <p>1987-01-01</p> <p>Strain <span class="hlt">energy</span> <span class="hlt">release</span> rates for edge delaminated composite laminates were obtained using quasi 3 dimensional finite element analysis. The problem of edge delamination at the -35/90 interfaces of an 8-ply composite laminate subjected to uniform axial strain was studied. The individual components of the strain <span class="hlt">energy</span> <span class="hlt">release</span> rates did not show convergence as the delamination tip elements were made smaller. In contrast, the total strain <span class="hlt">energy</span> <span class="hlt">release</span> rate converged and remained unchanged as the delamination tip elements were made smaller and agreed with that calculated using a classical laminated plate theory. The studies of the near field solutions for a delamination at an interface between two dissimilar isotropic or orthotropic plates showed that the imaginary part of the singularity is the cause of the nonconvergent behavior of the individual components. To evaluate the accuracy of the results, an 8-ply laminate with the delamination modeled in a thin resin layer, that exists between the -35 and 90 plies, was analyzed. Because the delamination exists in a homogeneous isotropic material, the oscillatory component of the singularity vanishes.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011ShWav..21..425Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011ShWav..21..425Z"><span>Simplified modeling of blast waves from metalized heterogeneous explosives</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zarei, Z.; Frost, D. L.</p> <p>2011-09-01</p> <p>The detonation of a metalized explosive generates a complex multiphase flow field. Modeling the subsequent propagation of the blast front requires a detailed knowledge of the metal particle dynamics and reaction rate. Given the uncertainties in modeling these phenomena, a much simpler, 1D compressible flow model is used to illustrate the general effects of secondary <span class="hlt">energy</span> <span class="hlt">release</span> due to particle reaction on the blast front properties. If the total <span class="hlt">energy</span> <span class="hlt">release</span> is held constant, the blast pressure and impulse are primarily dependent on the following parameters: the proportion of secondary <span class="hlt">energy</span> <span class="hlt">released</span> due to <span class="hlt">afterburning</span>, the rate of <span class="hlt">energy</span> <span class="hlt">release</span>, the location the secondary <span class="hlt">energy</span> <span class="hlt">release</span> begins, and the range over which it occurs. <span class="hlt">Releasing</span> the total <span class="hlt">energy</span> over a longer time period in general reduces the peak blast overpressure at a given distance. However, secondary <span class="hlt">energy</span> <span class="hlt">release</span> reduces the rate of decay of the shock pressure, increases the local gas temperature and hence increases the velocity of the secondary shock front. As a result, for certain values of the above parameters, the peak blast impulse may be increased by a factor of about two in a region near the charge. The largest augmentation to the near-field peak impulse results when the secondary <span class="hlt">energy</span> is <span class="hlt">released</span> immediately behind the shock front rather than uniformly within the combustion products.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009EGUGA..11.2323R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009EGUGA..11.2323R"><span>Influence of LOD variations on seismic <span class="hlt">energy</span> <span class="hlt">release</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Riguzzi, F.; Krumm, F.; Wang, K.; Kiszely, M.; Varga, P.</p> <p>2009-04-01</p> <p>Tidal friction causes significant time variations of geodynamical parameters, among them geometrical flattening. The axial despinning of the Earth due to tidal friction through the change of flattening generates incremental meridional and azimuthal stresses. The stress pattern in an incompressible elastic upper mantle and crust is symmetric to the equator and has its inflection points at the critical latitude close to ±45°. Consequently the distribution of seismic <span class="hlt">energy</span> <span class="hlt">released</span> by strong, shallow focus earthquakes should have also sharp maxima at this latitude. To investigate the influence of length of day (LOD) variations on earthquake activity an earthquake catalogue of strongest seismic events (M>7.0) was completed for the period 1900-2007. It is shown with the use of this catalogue that for the studied time-interval the catalogue is complete and consists of the seismic events responsible for more than 90% of <span class="hlt">released</span> seismic <span class="hlt">energy</span>. Study of the catalogue for earthquakes M>7.0 shows that the seismic <span class="hlt">energy</span> discharged by the strongest seismic events has significant maxima at ±45°, what renders probably that the seismic activity of our planet is influenced by an external component, i.e. by the tidal friction, which acts through the variation of the hydrostatic figure of the Earth caused by it. Distribution along the latitude of earthquake numbers and <span class="hlt">energies</span> was investigated also for the case of global linear tectonic structures, such as mid ocean ridges and subduction zones. It can be shown that the number of the shallow focus shocks has a repartition along the latitude similar to the distribution of the linear tectonic structures. This means that the position of foci of seismic events is mainly controlled by the tectonic activity.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20130014383','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20130014383"><span>Surface Temperature Measurements from a Stator Vane Doublet in a Turbine Engine <span class="hlt">Afterburner</span> Flame using Ultra-Bright Cr-Doped GdAlO3 Thermographic Phosphor</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Eldridge, Jeffrey I.; Jenkins, Thomas P.; Allison, Stephen W.; Wolfe, Douglas E.; Howard, Robert P.</p> <p>2013-01-01</p> <p>Luminescence-based surface temperature measurements from an ultra-bright Cr-doped GdAlO3 perovskite (GAP:Cr) coating were successfully conducted on an air-film-cooled stator vane doublet exposed to the <span class="hlt">afterburner</span> flame of a J85 test engine at University of Tennessee Space Institute (UTSI). The objective of the testing at UTSI was to demonstrate that reliable thermal barrier coating (TBC) surface temperatures based on luminescence decay of a thermographic phosphor could be obtained from the surface of an actual engine component in an aggressive <span class="hlt">afterburner</span> flame environment and to address the challenges of a highly radiant background and high velocity gases. A high-pressure turbine vane doublet from a Honeywell TECH7000 turbine engine was coated with a standard electron-beam physical vapor deposited (EB-PVD) 200-m-thick TBC composed of yttria-stabilized zirconia (YSZ) onto which a 25-m-thick GAP:Cr thermographic phosphor layer was deposited by EB-PVD. The ultra-bright broadband luminescence from the GAP:Cr thermographic phosphor is shown to offer the advantage of over an order-of-magnitude greater emission intensity compared to rare-earth-doped phosphors in the engine test environment. This higher emission intensity was shown to be very desirable for overcoming the necessarily restricted probe light collection solid angle and for achieving high signal-to-background levels. Luminescence-decay-based surface temperature measurements varied from 500 to over 1000C depending on engine operating conditions and level of air film cooling.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016MeScT..27l5205E','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016MeScT..27l5205E"><span>Surface temperature measurements from a stator vane doublet in a turbine <span class="hlt">afterburner</span> flame using a YAG:Tm thermographic phosphor</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Eldridge, Jeffrey I.; Allison, Stephen W.; Jenkins, Thomas P.; Gollub, Sarah L.; Hall, Carl A.; Walker, D. Greg</p> <p>2016-12-01</p> <p>Phosphor thermometry measurements in turbine engine environments can be difficult because of high background radiation levels. To address this challenge, luminescence lifetime-based phosphor thermometry measurements were obtained using thulium-doped Y3Al5O12 (YAG:Tm) to take advantage of the emission wavelengths at 365 nm (1D2  →  3H6 transition) and at 456 nm (1D2  →  3F4 transition). At these wavelengths, turbine engine radiation background is reduced compared with emission from longer wavelength phosphors. Temperature measurements of YAG:Tm coatings were demonstrated using decay of both the 365 and 456 nm emission bands in a furnace environment up to 1400 °C. To demonstrate that reliable surface temperatures based on short-wavelength YAG:Tm emission could be obtained from the surface of an actual engine component in a high gas velocity, highly radiative environment, measurements were obtained from a YAG:Tm-coated Honeywell stator vane doublet placed in the <span class="hlt">afterburner</span> flame exhaust stream of the augmenter-equipped General Electric J85 turbojet test engine at the University of Tennessee Space Institute (UTSI). Using a probe designed for engine insertion, spot temperature measurements were obtained by measuring luminescence decay times over a range of steady state throttle settings as well as during an engine throttle acceleration. YAG:Tm phosphor thermometry measurements of the stator vane surface in the <span class="hlt">afterburner</span> exhaust stream using the decay of the 456 nm emission band were successfully obtained at temperatures up to almost 1300 °C. Phosphor thermometry measurements acquired with the engine probe using the decay of the 365 nm emission band were not successful at usefully high temperatures because the probe design allowed transmission of intense unfiltered silica Raman scattering that produced photomultiplier tube saturation with extended recovery times. Recommendations are made for probe modifications that will enable</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/ADA532274','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA532274"><span>Utilizing CFD for Prediction of HD1.3 Pressure Loads in a Cell with Venting</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>2010-07-01</p> <p>room. The gas load is a result of the heat <span class="hlt">released</span> during the explosion and <span class="hlt">afterburning</span> of explosives that was not consumed by the initial...Structural Systems Design Guide HNDED-CS-93-72 specifies that all HD 1.3 in a room will be summed and converted to an equivalent TNT mass (based on...the H2 and CO are shown in Table 5. The Pre- <span class="hlt">Afterburning</span> quantities are based on the chemical equilibrium calculations performed in the AFCESI code</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19910020966','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19910020966"><span>Residual thermal and moisture influences on the strain <span class="hlt">energy</span> <span class="hlt">release</span> rate analysis of local delaminations from matrix cracks</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Obrien, T. K.</p> <p>1991-01-01</p> <p>An analysis utilizing laminated plate theory is developed to calculate the strain <span class="hlt">energy</span> <span class="hlt">release</span> rate associated with local delaminations originating at off-axis, single ply, matrix cracks in laminates subjected to uniaxial loads. The analysis includes the contribution of residual thermal and moisture stresses to the strain <span class="hlt">energy</span> <span class="hlt">released</span>. Examples are calculated for the strain <span class="hlt">energy</span> <span class="hlt">release</span> rate associated with local delaminations originating at 90 degrees and angle-ply (non-90 degrees) matrix ply cracks in glass epoxy and graphite epoxy laminates. The solution developed may be used to assess the relative contribution of mechanical, residual thermal, and moisture stresses on the strain <span class="hlt">energy</span> <span class="hlt">release</span> rate for local delamination for a variety of layups and materials.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/865965','DOE-PATENT-XML'); return false;" href="https://www.osti.gov/servlets/purl/865965"><span>Method of achieving the controlled <span class="hlt">release</span> of thermonuclear <span class="hlt">energy</span></span></a></p> <p><a target="_blank" href="http://www.osti.gov/doepatents">DOEpatents</a></p> <p>Brueckner, Keith A.</p> <p>1986-01-01</p> <p>A method of achieving the controlled <span class="hlt">release</span> of thermonuclear <span class="hlt">energy</span> by illuminating a minute, solid density, hollow shell of a mixture of material such as deuterium and tritium with a high intensity, uniformly converging laser wave to effect an extremely rapid build-up of <span class="hlt">energy</span> in inwardly traveling shock waves to implode the shell creating thermonuclear conditions causing a reaction of deuterons and tritons and a resultant high <span class="hlt">energy</span> thermonuclear burn. Utilizing the resulting <span class="hlt">energy</span> as a thermal source and to breed tritium or plutonium. The invention also contemplates a laser source wherein the flux level is increased with time to reduce the initial shock heating of fuel and provide maximum compression after implosion; and, in addition, computations and an equation are provided to enable the selection of a design having a high degree of stability and a dependable fusion performance by establishing a proper relationship between the laser <span class="hlt">energy</span> input and the size and character of the selected material for the fusion capsule.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20060056392','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20060056392"><span>Influence of Finite Element Software on <span class="hlt">Energy</span> <span class="hlt">Release</span> Rates Computed Using the Virtual Crack Closure Technique</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Krueger, Ronald; Goetze, Dirk; Ransom, Jonathon (Technical Monitor)</p> <p>2006-01-01</p> <p>Strain <span class="hlt">energy</span> <span class="hlt">release</span> rates were computed along straight delamination fronts of Double Cantilever Beam, End-Notched Flexure and Single Leg Bending specimens using the Virtual Crack Closure Technique (VCCT). Th e results were based on finite element analyses using ABAQUS# and ANSYS# and were calculated from the finite element results using the same post-processing routine to assure a consistent procedure. Mixed-mode strain <span class="hlt">energy</span> <span class="hlt">release</span> rates obtained from post-processing finite elem ent results were in good agreement for all element types used and all specimens modeled. Compared to previous studies, the models made of s olid twenty-node hexahedral elements and solid eight-node incompatible mode elements yielded excellent results. For both codes, models made of standard brick elements and elements with reduced integration did not correctly capture the distribution of the <span class="hlt">energy</span> <span class="hlt">release</span> rate acr oss the width of the specimens for the models chosen. The results suggested that element types with similar formulation yield matching results independent of the finite element software used. For comparison, m ixed-mode strain <span class="hlt">energy</span> <span class="hlt">release</span> rates were also calculated within ABAQUS#/Standard using the VCCT for ABAQUS# add on. For all specimens mod eled, mixed-mode strain <span class="hlt">energy</span> <span class="hlt">release</span> rates obtained from ABAQUS# finite element results using post-processing were almost identical to re sults calculated using the VCCT for ABAQUS# add on.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018CG....113....1Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018CG....113....1Z"><span>Forecasting of future earthquakes in the northeast region of India considering <span class="hlt">energy</span> <span class="hlt">released</span> concept</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zarola, Amit; Sil, Arjun</p> <p>2018-04-01</p> <p>This study presents the forecasting of time and magnitude size of the next earthquake in the northeast India, using four probability distribution models (Gamma, Lognormal, Weibull and Log-logistic) considering updated earthquake catalog of magnitude Mw ≥ 6.0 that occurred from year 1737-2015 in the study area. On the basis of past seismicity of the region, two types of conditional probabilities have been estimated using their best fit model and respective model parameters. The first conditional probability is the probability of seismic <span class="hlt">energy</span> (e × 1020 ergs), which is expected to <span class="hlt">release</span> in the future earthquake, exceeding a certain level of seismic <span class="hlt">energy</span> (E × 1020 ergs). And the second conditional probability is the probability of seismic <span class="hlt">energy</span> (a × 1020 ergs/year), which is expected to <span class="hlt">release</span> per year, exceeding a certain level of seismic <span class="hlt">energy</span> per year (A × 1020 ergs/year). The logarithm likelihood functions (ln L) were also estimated for all four probability distribution models. A higher value of ln L suggests a better model and a lower value shows a worse model. The time of the future earthquake is forecasted by dividing the total seismic <span class="hlt">energy</span> expected to <span class="hlt">release</span> in the future earthquake with the total seismic <span class="hlt">energy</span> expected to <span class="hlt">release</span> per year. The epicentre of recently occurred 4 January 2016 Manipur earthquake (M 6.7), 13 April 2016 Myanmar earthquake (M 6.9) and the 24 August 2016 Myanmar earthquake (M 6.8) are located in zone Z.12, zone Z.16 and zone Z.15, respectively and that are the identified seismic source zones in the study area which show that the proposed techniques and models yield good forecasting accuracy.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/ADA026455','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA026455"><span>The LRCM: (the Long-Range Strategic Cruise Missile) Asymmetries, Deterrence and SAL (Strategic Arms Limitation)</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>1976-03-01</p> <p>about the same pro- portion of the useful payload. The J-85-4A non- <span class="hlt">afterburning</span> turbojet engines installed in the F5 aircraft occupy about 25% of the...about one kiloton TNT equivalent yield per 1 5 Pretty and Archer, op. cit. 32 pound of warhead weight. Thus, a 200 KT warhead will weigh about 200...explosion is equivalent to a conventional unit of <span class="hlt">energy</span> <span class="hlt">release</span> equal to one thousand short tons of TNT , or about 10 calories, 1.15 x 10 kilowatt</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2000ShWav..10..127W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2000ShWav..10..127W"><span>Visualization of turbulent combustion of TNT detonation products in a steel vessel</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wolański, P.; Gut, Z.; Trzciński, W. A.; Szymańczyk, L.; Paszula, J.</p> <p></p> <p>Mixing and <span class="hlt">afterburning</span> of TNT detonation products in a steel vessel are recorded by the use of the Schlieren visualization system and high speed photography. The vessel is filled with air or 50% oxygen enriched air. Overpressure histories at the vessel wall are also recorded by using pressure transducers. In these experiments nitrogen, air or 50% oxygen enriched air are used as vessel fillers. The Oppenheim-Kuhl theory of thermodynamics of closed systems is applied to estimate the <span class="hlt">released</span> <span class="hlt">energy</span> on the basis of pressure histories.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26410785','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26410785"><span>Highly fluorescent carbon dots for visible sensing of doxorubicin <span class="hlt">release</span> based on efficient nanosurface <span class="hlt">energy</span> transfer.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Wang, Beibei; Wang, Shujun; Wang, Yanfang; Lv, Yan; Wu, Hao; Ma, Xiaojun; Tan, Mingqian</p> <p>2016-01-01</p> <p>To prepare fluorescent carbon dots for loading cationic anticancer drug through donor-quenched nanosurface <span class="hlt">energy</span> transfer in visible sensing of drug <span class="hlt">release</span>. Highly fluorescent carbon dots (CDs) were prepared by a facile hydrothermal approach from citric acid and o-phenylenediamine. The obtained CDs showed a high quantum yield of 46 % and exhibited good cytocompatibility even at 1 mg/ml. The cationic anticancer drug doxorubicin (DOX) can be loaded onto the negatively charged CDs through electrostatic interactions. Additionally, the fluorescent CDs feature reversible donor-quenched mode nanosurface <span class="hlt">energy</span> transfer. When loading the <span class="hlt">energy</span> receptor DOX, the donor CDs' fluorescence was switched "off", while it turned "on" again after DOX <span class="hlt">release</span> from the surface through endocytic uptake. Most DOX molecules were <span class="hlt">released</span> from the CDs after 6 h incubation and entered cell nuclear region after 8 h, suggesting the drug delivery system may have potential for visible sensing in drug <span class="hlt">release</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1426668','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/1426668"><span>The Dark <span class="hlt">Energy</span> Survey Data <span class="hlt">Release</span> 1</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Abbott, T.M.C.; et al.</p> <p></p> <p>We describe the first public data <span class="hlt">release</span> of the Dark <span class="hlt">Energy</span> Survey, DES DR1, consisting of reduced single epoch images, coadded images, coadded source catalogs, and associated products and services assembled over the first three years of DES science operations. DES DR1 is based on optical/near-infrared imaging from 345 distinct nights (August 2013 to February 2016) by the Dark <span class="hlt">Energy</span> Camera mounted on the 4-m Blanco telescope at Cerro Tololo Inter-American Observatory in Chile. We <span class="hlt">release</span> data from the DES wide-area survey covering ~5,000 sq. deg. of the southern Galactic cap in five broad photometric bands, grizY. DES DR1 hasmore » a median delivered point-spread function of g = 1.12, r = 0.96, i = 0.88, z = 0.84, and Y = 0.90 arcsec FWHM, a photometric precision of < 1% in all bands, and an astrometric precision of 151 mas. The median coadded catalog depth for a 1.95" diameter aperture at S/N = 10 is g = 24.33, r = 24.08, i = 23.44, z = 22.69, and Y = 21.44 mag. DES DR1 includes nearly 400M distinct astronomical objects detected in ~10,000 coadd tiles of size 0.534 sq. deg. produced from ~39,000 individual exposures. Benchmark galaxy and stellar samples contain ~310M and ~ 80M objects, respectively, following a basic object quality selection. These data are accessible through a range of interfaces, including query web clients, image cutout servers, jupyter notebooks, and an interactive coadd image visualization tool. DES DR1 constitutes the largest photometric data set to date at the achieved depth and photometric precision.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013JPhCS.451a2014M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013JPhCS.451a2014M"><span>Dynamic <span class="hlt">energy</span> <span class="hlt">release</span> rate in couple-stress elasticity</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Morini, L.; Piccolroaz, A.; Mishuris, G.</p> <p>2013-07-01</p> <p>This paper is concerned with <span class="hlt">energy</span> <span class="hlt">release</span> rate for dynamic steady state crack problems in elastic materials with microstructures. A Mode III semi-infinite crack subject to loading applied on the crack surfaces is considered. The micropolar behaviour of the material is described by the theory of couple-stress elasticity developed by Koiter. A general expression for the dynamic J-integral including both traslational and micro-rotational inertial contributions is derived, and the conservation of this integral on a path surrounding the crack tip is demonstrated.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JAP...121x3101K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JAP...121x3101K"><span>Analyzing the effect of slotted foil on radiation pulse profile in a mode locked <span class="hlt">afterburner</span> X-ray free electron laser</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kumar, Sandeep; Hur, Min Sup; Chung, Moses</p> <p>2017-06-01</p> <p>Extremely short X-ray pulses in the attosecond (as) range are important tools for ultrafast dynamics, high resolution microscopy, and nuclear dynamics study. In this paper, we numerically examine the generation of gigawatt (GW) mode-locked (ML) multichromatic X-rays using the parameters of the Pohang Accelerator Laboratory (PAL)-X-ray free electron laser (XFEL), the Korean XFEL. In this vein, we analyze the ML-FEL [Thompson and McNeil, Phys. Rev. Lett. 100, 203901 (2008)] and mode-locked <span class="hlt">afterburner</span> (MLAB) FEL [Dunning et al., Phys. Rev. Lett. 110, 104801 (2013)] schemes on the hard X-ray beamline of the PAL-XFEL. Using the ML scheme, we numerically demonstrate a train of radiation pulses in the hard X-ray (photon <span class="hlt">energy</span> ˜12.4 keV) with 3.5 GW power and 16 as full-width half maximum (FWHM) pulse duration. On the other hand, using the MLAB scheme, a train of radiation pulses with 3 GW power and 1 as FWHM (900 zs in RMS) pulse duration has been obtained at 12.4 keV photon <span class="hlt">energy</span>. Both schemes generate broadband, discrete, and coherent spectrum compared to the XFEL's narrowband spectrum. Furthermore, the effect of slotted foil is also studied first time on the MLAB-FEL output. Numerical comparisons show that the temporal structure of the MLAB-FEL output can be improved significantly by the use of the slotted foil. Such short X-ray pulses at XFEL facilities will allow the studies of electron-nuclear and nuclear dynamics in atoms or molecules, and the broadband radiation will substantially improve the efficiency of the experimental techniques such as X-ray crystallography and spectroscopy, paving the way for outstanding progress in biology and material science.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_5");'>5</a></li> <li><a href="#" onclick='return showDiv("page_6");'>6</a></li> <li class="active"><span>7</span></li> <li><a href="#" onclick='return showDiv("page_8");'>8</a></li> <li><a href="#" onclick='return showDiv("page_9");'>9</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_7 --> <div id="page_8" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_6");'>6</a></li> <li><a href="#" onclick='return showDiv("page_7");'>7</a></li> <li class="active"><span>8</span></li> <li><a href="#" onclick='return showDiv("page_9");'>9</a></li> <li><a href="#" onclick='return showDiv("page_10");'>10</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="141"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010PhPl...17a2109B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010PhPl...17a2109B"><span><span class="hlt">Energy</span> <span class="hlt">release</span> and transfer in guide field reconnection</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Birn, J.; Hesse, M.</p> <p>2010-01-01</p> <p>Properties of <span class="hlt">energy</span> <span class="hlt">release</span> and transfer by magnetic reconnection in the presence of a guide field are investigated on the basis of 2.5-dimensional magnetohydrodynamic (MHD) and particle-in-cell (PIC) simulations. Two initial configurations are considered: a plane current sheet with a uniform guide field of 80% of the reconnecting magnetic field component and a force-free current sheet in which the magnetic field strength is constant but the field direction rotates by 180° through the current sheet. The onset of reconnection is stimulated by localized, temporally limited compression. Both MHD and PIC simulations consistently show that the outgoing <span class="hlt">energy</span> fluxes are dominated by (redirected) Poynting flux and enthalpy flux, whereas bulk kinetic <span class="hlt">energy</span> flux and heat flux (in the PIC simulation) are small. The Poynting flux is mainly associated with the magnetic <span class="hlt">energy</span> of the guide field which is carried from inflow to outflow without much alteration. The conversion of annihilated magnetic <span class="hlt">energy</span> to enthalpy flux (that is, thermal <span class="hlt">energy</span>) stems mainly from the fact that the outflow occurs into a closed field region governed by approximate force balance between Lorentz and pressure gradient forces. Therefore, the <span class="hlt">energy</span> converted from magnetic to kinetic <span class="hlt">energy</span> by Lorentz force acceleration becomes immediately transferred to thermal <span class="hlt">energy</span> by the work done by the pressure gradient force. Strong similarities between late stages of MHD and PIC simulations result from the fact that conservation of mass and entropy content and footpoint displacement of magnetic flux tubes, imposed in MHD, are also approximately satisfied in the PIC simulations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2003EAEJA.....9933F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2003EAEJA.....9933F"><span>Carbon dioxide degassing and thermal <span class="hlt">energy</span> <span class="hlt">release</span> at Vesuvio (Italy)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Frondini, F.; Chiodini, G.; Caliro, S.; Cardellini, C.; Granieri, D.</p> <p>2003-04-01</p> <p>At Vesuvio, basing on the data of the CO2 flux surveys carried out in April and May 2000, are discharged about 130 t d-1 of CO2 through soil diffuse degassing. In the crater area the distribution of the soil temperatures show a general correspondence between the CO2 flux anomalies and the high temperatures, suggesting that the heating of the soil is mainly due to the condensation of the rising volcanic-hydrothermal fluids. Considering that the original H2O/CO2 ratio of hydrothermal fluids is recorded by fumarolic effluents, the steam associated to the CO2 output has been computed and amount to is 475 t d-1. The <span class="hlt">energy</span> produced by the steam condensation and cooling of the liquid phase is 1.26 1012 J d-1 (14.6 MW). The amounts of gas and <span class="hlt">energy</span> <span class="hlt">released</span> by Vesuvio are comparable to those <span class="hlt">released</span> by other volcanic degassing areas of the world and their estimates, through periodical CO2 flux surveys, can constitute a powerful tool to monitor the activity of the volcano.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/897937','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/897937"><span>Kinetic Modeling of Slow <span class="hlt">Energy</span> <span class="hlt">Release</span> in Non-Ideal Carbon Rich Explosives</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Vitello, P; Fried, L; Glaesemann, K</p> <p>2006-06-20</p> <p>We present here the first self-consistent kinetic based model for long time-scale <span class="hlt">energy</span> <span class="hlt">release</span> in detonation waves in the non-ideal explosive LX-17. Non-ideal, insensitive carbon rich explosives, such as those based on TATB, are believed to have significant late-time slow <span class="hlt">release</span> in <span class="hlt">energy</span>. One proposed source of this <span class="hlt">energy</span> is diffusion-limited growth of carbon clusters. In this paper we consider the late-time <span class="hlt">energy</span> <span class="hlt">release</span> problem in detonation waves using the thermochemical code CHEETAH linked to a multidimensional ALE hydrodynamics model. The linked CHEETAH-ALE model dimensional treats slowly reacting chemical species using kinetic rate laws, with chemical equilibrium assumed for speciesmore » coupled via fast time-scale reactions. In the model presented here we include separate rate equations for the transformation of the un-reacted explosive to product gases and for the growth of a small particulate form of condensed graphite to a large particulate form. The small particulate graphite is assumed to be in chemical equilibrium with the gaseous species allowing for coupling between the instantaneous thermodynamic state and the production of graphite clusters. For the explosive burn rate a pressure dependent rate law was used. Low pressure freezing of the gas species mass fractions was also included to account for regions where the kinetic coupling rates become longer than the hydrodynamic time-scales. The model rate parameters were calibrated using cylinder and rate-stick experimental data. Excellent long time agreement and size effect results were achieved.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22661301-observable-signatures-energy-release-braided-coronal-loops','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22661301-observable-signatures-energy-release-braided-coronal-loops"><span>Observable Signatures of <span class="hlt">Energy</span> <span class="hlt">Release</span> in Braided Coronal Loops</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Pontin, D. I.; Janvier, M.; Tiwari, S. K.</p> <p></p> <p>We examine the turbulent relaxation of solar coronal loops containing non-trivial field line braiding. Such field line tangling in the corona has long been postulated in the context of coronal heating models. We focus on the observational signatures of <span class="hlt">energy</span> <span class="hlt">release</span> in such braided magnetic structures using MHD simulations and forward modeling tools. The aim is to answer the following question: if <span class="hlt">energy</span> <span class="hlt">release</span> occurs in a coronal loop containing braided magnetic flux, should we expect a clearly observable signature in emissions? We demonstrate that the presence of braided magnetic field lines does not guarantee a braided appearance to themore » observed intensities. Observed intensities may—but need not necessarily—reveal the underlying braided nature of the magnetic field, depending on the degree and pattern of the field line tangling within the loop. However, in all cases considered, the evolution of the braided loop is accompanied by localized heating regions as the loop relaxes. Factors that may influence the observational signatures are discussed. Recent high-resolution observations from Hi-C have claimed the first direct evidence of braided magnetic fields in the corona. Here we show that both the Hi-C data and some of our simulations give the appearance of braiding at a range of scales.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010JEnM...28....1T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010JEnM...28....1T"><span>Chemical <span class="hlt">Energy</span> <span class="hlt">Release</span> in Several Recently Discovered Detonation and Deflagration Flows</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Tarver, Craig M.</p> <p>2010-10-01</p> <p>Several recent experiments on complex detonation and deflagration flows are analyzed in terms of the chemical <span class="hlt">energy</span> <span class="hlt">release</span> required to sustain these flows. The observed double cellular structures in detonating gaseous nitromethane-oxygen and NO2-fuel (H2, CH4, and C2H6) mixtures are explained by the amplification of two distinct pressure wave frequencies by two exothermic reactions, the faster reaction forming vibrationally excited NO* and the slower reaction forming highly vibrationally excited N2**. The establishment of a Chapman-Jouguet (C-J) deflagration behind a weak shock wave, the C-J detonation established after a head-on collision with a shock front, and the C-J detonation conditions established in reactive supersonic flows are quantitatively calculated using the chemical <span class="hlt">energy</span> <span class="hlt">release</span> of a H2 + Cl2 mixture. For these three reactive flows, these calculations illustrate that different fractions of the exothermic chemical <span class="hlt">energy</span> are used to sustain steady-state propagation. C-J detonation calculations on the various initial states using the CHEETAH chemical equilibrium code are shown to be in good agreement with experimental detonation velocity measurements for the head-on collision and supersonic flow detonations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19930054261&hterms=solar+energy&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3Dsolar%2Benergy','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19930054261&hterms=solar+energy&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3Dsolar%2Benergy"><span>Numerical modeling of the <span class="hlt">energy</span> storage and <span class="hlt">release</span> in solar flares</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Wu, S. T.; Weng, F. S.</p> <p>1993-01-01</p> <p>This paper reports on investigation of the photospheric magnetic field-line footpoint motion (usually referred to as shear motion) and magnetic flux emerging from below the surface in relation to <span class="hlt">energy</span> storage in a solar flare. These causality relationships are demonstrated by using numerical magnetohydrodynamic simulations. From these results, one may conclude that the <span class="hlt">energy</span> stored in solar flares is in the form of currents. The dynamic process through which these currents reach a critical value is discussed as well as how these currents lead to <span class="hlt">energy</span> <span class="hlt">release</span>, such as the explosive events of solar flares.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19830014615','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19830014615"><span>The <span class="hlt">energy</span> <span class="hlt">release</span> in earthquakes, and subduction zone seismicity and stress in slabs. Ph.D. Thesis</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Vassiliou, M. S.</p> <p>1983-01-01</p> <p><span class="hlt">Energy</span> <span class="hlt">release</span> in earthquakes is discussed. Dynamic <span class="hlt">energy</span> from source time function, a simplified procedure for modeling deep focus events, static <span class="hlt">energy</span> estimates, near source <span class="hlt">energy</span> studies, and <span class="hlt">energy</span> and magnitude are addressed. Subduction zone seismicity and stress in slabs are also discussed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1154960','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/1154960"><span>Explosive Products EOS: Adjustment for detonation speed and <span class="hlt">energy</span> <span class="hlt">release</span></span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Menikoff, Ralph</p> <p>2014-09-05</p> <p>Propagating detonation waves exhibit a curvature effect in which the detonation speed decreases with increasing front curvature. The curvature effect is due to the width of the wave profile. Numerically, the wave profile depends on resolution. With coarse resolution, the wave width is too large and results in a curvature effect that is too large. Consequently, the detonation speed decreases as the cell size is increased. We propose a modification to the products equation of state (EOS) to compensate for the effect of numerical resolution; i.e., to increase the CJ pressure in order that a simulation propagates a detonation wavemore » with a speed that is on average correct. The EOS modification also adjusts the <span class="hlt">release</span> isentrope to correct the <span class="hlt">energy</span> <span class="hlt">release</span>.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1992JCoMa..26.2028R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1992JCoMa..26.2028R"><span>Method for computing <span class="hlt">energy</span> <span class="hlt">release</span> rate using the elastic work factor approach</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Rhee, K. Y.; Ernst, H. A.</p> <p>1992-01-01</p> <p>The elastic work factor eta(el) concept was applied to composite structures for the calculation of total <span class="hlt">energy</span> <span class="hlt">release</span> rate by using a single specimen. Cracked lap shear specimens with four different unidirectional fiber orientation were used to examine the dependence of eta(el) on the material properties. Also, three different thickness ratios (lap/strap) were used to determine how geometric conditions affect eta(el). The eta(el) values were calculated in two different ways: compliance method and crack closure method. The results show that the two methods produce comparable eta(el) values and, while eta(el) is affected significantly by geometric conditions, it is reasonably independent of material properties for the given geometry. The results also showed that the elastic work factor can be used to calculate total <span class="hlt">energy</span> <span class="hlt">release</span> rate using a single specimen.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20140013397','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20140013397"><span><span class="hlt">Energy</span> <span class="hlt">Release</span> from Impacting Prominence Material Following the 2011 June 7 Eruption</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Gilbert, H. R.; Inglis, A. R.; Mays, M. L.; Ofman, L.; Thompson, B. J.; Young, C. A.</p> <p>2013-01-01</p> <p>Solar filaments exhibit a range of eruptive-like dynamic activity, ranging from the full or partial eruption of the filament mass and surrounding magnetic structure as a coronal mass ejection to a fully confined or failed eruption. On 2011 June 7, a dramatic partial eruption of a filament was observed by multiple instruments on board the Solar Dynamics Observatory (SDO) and Solar-Terrestrial Relations Observatory. One of the interesting aspects of this event is the response of the solar atmosphere as non-escaping material falls inward under the influence of gravity. The impact sites show clear evidence of brightening in the observed extreme ultraviolet wavelengths due to <span class="hlt">energy</span> <span class="hlt">release</span>. Two plausible physical mechanisms for explaining the brightening are considered: heating of the plasma due to the kinetic <span class="hlt">energy</span> of impacting material compressing the plasma, or reconnection between the magnetic field of low-lying loops and the field carried by the impacting material. By analyzing the emission of the brightenings in several SDO/Atmospheric Imaging Assembly wavelengths, and comparing the kinetic <span class="hlt">energy</span> of the impacting material (7.6 × 10(exp 26) - 5.8 × 10(exp 27) erg) to the radiative <span class="hlt">energy</span> (approx. 1.9 × 10(exp 25) - 2.5 × 10(exp 26) erg), we find the dominant mechanism of <span class="hlt">energy</span> <span class="hlt">release</span> involved in the observed brightening is plasma compression.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EPJWC.15307007T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EPJWC.15307007T"><span>Precise calculation of neutron-capture reactions contribution in <span class="hlt">energy</span> <span class="hlt">release</span> for different types of VVER-1000 fuel assemblies</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Tikhomirov, Georgy; Bahdanovich, Rynat; Pham, Phu</p> <p>2017-09-01</p> <p>Precise calculation of <span class="hlt">energy</span> <span class="hlt">release</span> in a nuclear reactor is necessary to obtain the correct spatial power distribution and predict characteristics of burned nuclear fuel. In this work, previously developed method for calculation neutron-capture reactions - capture component - contribution in effective <span class="hlt">energy</span> <span class="hlt">release</span> in a fuel core of nuclear reactor is discussed. The method was improved and implemented to the different models of VVER-1000 reactor developed for MCU 5 and MCNP 4 computer codes. Different models of equivalent cell and fuel assembly in the beginning of fuel cycle were calculated. These models differ by the geometry, fuel enrichment and presence of burnable absorbers. It is shown, that capture component depends on fuel enrichment and presence of burnable absorbers. Its value varies for different types of hot fuel assemblies from 3.35% to 3.85% of effective <span class="hlt">energy</span> <span class="hlt">release</span>. Average capture component contribution in effective <span class="hlt">energy</span> <span class="hlt">release</span> for typical serial fresh fuel of VVER-1000 is 3.5%, which is 7 MeV/fission. The method will be used in future to estimate the dependency of capture <span class="hlt">energy</span> on fuel density, burn-up, etc.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22522197-energy-release-initiation-sunquake-class-flare','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22522197-energy-release-initiation-sunquake-class-flare"><span><span class="hlt">ENERGY</span> <span class="hlt">RELEASE</span> AND INITIATION OF A SUNQUAKE IN A C-CLASS FLARE</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Sharykin, I. N.; Kosovichev, A. G.; Zimovets, I. V.</p> <p></p> <p>We present an analysis of the C7.0 solar flare from 2013 February 17, revealing a strong helioseismic response (sunquake) caused by a compact impact observed with the Helioseismic and Magnetic Imager on board the Solar Dynamics Observatory (SDO) in the low atmosphere. This is the weakest known C-class flare generating a sunquake event. To investigate the possible mechanisms of this event and understand the role of accelerated charged particles and photospheric electric currents, we use data from three space observatories: RHESSI, SDO, and Geostationary Operational Environmental Satellite. We find that the photospheric flare impact does not spatially correspond to themore » strongest hard X-ray emission source, but both of these events are parts of the same <span class="hlt">energy</span> <span class="hlt">release</span>. Our analysis reveals a close association of the flare <span class="hlt">energy</span> <span class="hlt">release</span> with a rapid increase in the electric currents and suggests that the sunquake initiation is unlikely to be caused by the impact of high-<span class="hlt">energy</span> electrons, but may be associated with rapid current dissipation or a localized impulsive Lorentz force in the lower layers of the solar atmosphere.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19730010239','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19730010239"><span><span class="hlt">Afterburner</span> Performance of Circular V-Gutters and a Sector of Parallel V-Gutters for a Range of Inlet Temperatures to 1255 K (1800 F)</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Brandstetter, J. Robert; Reck, Gregory M.</p> <p>1973-01-01</p> <p>Combustion tests of two V-gutter types were conducted in a 19.25-in. diameter duct using vitiated air. Fuel spraybars were mounted in line with the V-gutters. Combustor length was set by flame-quench water sprays which were part of a calorimeter for measuring combustion efficiency. Although the levels of performance of the parallel and circular array <span class="hlt">afterburners</span> were different, the trends with geometry variations were consistent. Therefore, parallel arrays can be used for evaluating V-gutter geometry effects on combustion performance. For both arrays, the highest inlet temperature produced combustion efficiencies near 100 percent. A 5-in. spraybar - to - V-gutter spacing gave higher efficiency and better lean blowout performance than a spacing twice as large. Gutter durability was good.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFMSH14B..05K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFMSH14B..05K"><span>Triggers and Manifestations of Flare <span class="hlt">Energy</span> <span class="hlt">Release</span> in the Low Atmosphere</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kosovichev, A. G.; Sharykin, I. N.; Sadykov, V. M.; Vargas, S.; Zimovets, I. V.</p> <p>2016-12-01</p> <p>The main goal is to understand triggers and manifestations of the flare <span class="hlt">energy</span> <span class="hlt">release</span> in the lower layers of the solar atmosphere (the photosphere and chromosphere) using high-resolution optical observations and magnetic field measurements. As a case study we present results for an M-class flare. We analyze optical images, HMI Dopplergrams and vector magnetograms, and use Non-Linear Force-Free Field (NLFFF) extrapolation for reconstruction of the magnetic topology. The NLFFF modelling reveals interaction of oppositely directed magnetic flux-tubes in the Polarity Inversion Line (PIL). These two interacting magnetic flux tubes are observed as a compact sheared arcade along the PIL in the high-resolution broad-band continuum images from New Solar Telescope (NST). In the vicinity of the PIL, the NST H-alpha observations reveal formation of a thin three-ribbon structure corresponding to the small-scale photospheric magnetic arcade. Magnetic reconnection is triggered by two interacting magnetic flux tubes with forming current sheet extended along the PIL. Presented observational results evidence in favor of location of the primary <span class="hlt">energy</span> <span class="hlt">release</span> site in the dense chromosphere where plasma is partially ionized in the region of strong electric currents concentrated near the polarity inversion line.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19790006996','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19790006996"><span>Enclosure fire hazard analysis using relative <span class="hlt">energy</span> <span class="hlt">release</span> criteria. [burning rate and combustion control</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Coulbert, C. D.</p> <p>1978-01-01</p> <p>A method for predicting the probable course of fire development in an enclosure is presented. This fire modeling approach uses a graphic plot of five fire development constraints, the relative <span class="hlt">energy</span> <span class="hlt">release</span> criteria (RERC), to bound the heat <span class="hlt">release</span> rates in an enclosure as a function of time. The five RERC are flame spread rate, fuel surface area, ventilation, enclosure volume, and total fuel load. They may be calculated versus time based on the specified or empirical conditions describing the specific enclosure, the fuel type and load, and the ventilation. The calculation of these five criteria, using the common basis of <span class="hlt">energy</span> <span class="hlt">release</span> rates versus time, provides a unifying framework for the utilization of available experimental data from all phases of fire development. The plot of these criteria reveals the probable fire development envelope and indicates which fire constraint will be controlling during a criteria time period. Examples of RERC application to fire characterization and control and to hazard analysis are presented along with recommendations for the further development of the concept.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017PhDT.......113D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017PhDT.......113D"><span>Understanding the Relationships Between Architecture, Chemistry, and <span class="hlt">Energy</span> <span class="hlt">Release</span> of Energetic Nanocomposites</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>DeLisio, Jeffery Brandon</p> <p></p> <p>Energetic nanocomposites are a class of reactive material that incorporate nanosized materials or features in order to enhance reaction kinetics and <span class="hlt">energy</span> densities. Typically, these systems employ metal nanoparticles as the fuel source and have demonstrated reactivities orders of magnitude larger than more traditionally used micron-sized metal fuels. One drawback of using nanosized metals is that the nascent oxide shell comprises a significant weight percent as the particle size decreases. This shell also complicates the understanding of oxidation mechanisms of nanosized metal fuels. In this dissertation, I apply a two-fold approach to understanding the relationships between architecture, chemistry, and <span class="hlt">energy</span> <span class="hlt">release</span> of energetic nanocomposites by 1) investigating alternative metal fuels to develop a deeper understanding of the reaction mechanisms of energetic nanocomposites and 2) creating unique microstructures to tailor macroscopic properties allowing for customizability of energetic performance. In order to accurately study these systems, new analytical techniques capable of high heating rate analysis were developed. The oxidation mechanisms of tantalum nanoparticles was first probed using high heating rate TEM and Temperature-Jump Time-of-Flight Mass Spectrometry (T-Jump TOFMS) and shell crystallization was found to plan an important role in the mechanism. An air-sensitive sample holder was developed and employed to analyze the decomposition and oxidation of molecular aluminum compounds, which theoretically can achieve similar <span class="hlt">energy</span> <span class="hlt">release</span> rates to monomolecular explosives in addition to much higher <span class="hlt">energy</span> densities. In order to obtain simultaneous thermal and speciation data at high heating rates, a nanocalorimeter was integrated into the TOFMS system and measurements were performed on Al/CuO nanolaminates to probe the effect of bilayer thickness on <span class="hlt">energy</span> <span class="hlt">release</span>. An electrospray based approach to creating energetic nanocomposites with tunable</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19990078564','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19990078564"><span>A Method for Calculating Strain <span class="hlt">Energy</span> <span class="hlt">Release</span> Rates in Preliminary Design of Composite Skin/Stringer Debonding Under Multi-Axial Loading</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Krueger, Ronald; Minguet, Pierre J.; OBrien, T. Kevin</p> <p>1999-01-01</p> <p>Three simple procedures were developed to determine strain <span class="hlt">energy</span> <span class="hlt">release</span> rates, G, in composite skin/stringer specimens for various combinations of unaxial and biaxial (in-plane/out-of-plane) loading conditions. These procedures may be used for parametric design studies in such a way that only a few finite element computations will be necessary for a study of many load combinations. The results were compared with mixed mode strain <span class="hlt">energy</span> <span class="hlt">release</span> rates calculated directly from nonlinear two-dimensional plane-strain finite element analyses using the virtual crack closure technique. The first procedure involved solving three unknown parameters needed to determine the <span class="hlt">energy</span> <span class="hlt">release</span> rates. Good agreement was obtained when the external loads were used in the expression derived. This superposition technique was only applicable if the structure exhibits a linear load/deflection behavior. Consequently, a second technique was derived which was applicable in the case of nonlinear load/deformation behavior. The technique involved calculating six unknown parameters from a set of six simultaneous linear equations with data from six nonlinear analyses to determine the <span class="hlt">energy</span> <span class="hlt">release</span> rates. This procedure was not time efficient, and hence, less appealing. A third procedure was developed to calculate mixed mode <span class="hlt">energy</span> <span class="hlt">release</span> rates as a function of delamination lengths. This procedure required only one nonlinear finite element analysis of the specimen with a single delamination length to obtain a reference solution for the <span class="hlt">energy</span> <span class="hlt">release</span> rates and the scale factors. The delamination was extended in three separate linear models of the local area in the vicinity of the delamination subjected to unit loads to obtain the distribution of G with delamination lengths. This set of sub-problems was Although additional modeling effort is required to create the sub- models, this local technique is efficient for parametric studies.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018CPL...693...66H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018CPL...693...66H"><span>Tunneling and reflection in unimolecular reaction kinetic <span class="hlt">energy</span> <span class="hlt">release</span> distributions</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hansen, K.</p> <p>2018-02-01</p> <p>The kinetic <span class="hlt">energy</span> <span class="hlt">release</span> distributions in unimolecular reactions is calculated with detailed balance theory, taking into account the tunneling and the reflection coefficient in three different types of transition states; (i) a saddle point corresponding to a standard RRKM-type theory, (ii) an attachment Langevin cross section, and (iii) an absorbing sphere potential at short range, without long range interactions. Corrections are significant in the one dimensional saddle point states. Very light and lightly bound absorbing systems will show measurable effects in decays from the absorbing sphere, whereas the Langevin cross section is essentially unchanged.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016PhDT........44P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016PhDT........44P"><span>Combustion instability and active control: Alternative fuels, augmentors, and modeling heat <span class="hlt">release</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Park, Sammy Ace</p> <p></p> <p>Experimental and analytical studies were conducted to explore thermo-acoustic coupling during the onset of combustion instability in various air-breathing combustor configurations. These include a laboratory-scale 200-kW dump combustor and a 100-kW augmentor featuring a v-gutter flame holder. They were used to simulate main combustion chambers and <span class="hlt">afterburners</span> in aero engines, respectively. The three primary themes of this work includes: 1) modeling heat <span class="hlt">release</span> fluctuations for stability analysis, 2) conducting active combustion control with alternative fuels, and 3) demonstrating practical active control for augmentor instability suppression. The phenomenon of combustion instabilities remains an unsolved problem in propulsion engines, mainly because of the difficulty in predicting the fluctuating component of heat <span class="hlt">release</span> without extensive testing. A hybrid model was developed to describe both the temporal and spatial variations in dynamic heat <span class="hlt">release</span>, using a separation of variables approach that requires only a limited amount of experimental data. The use of sinusoidal basis functions further reduced the amount of data required. When the mean heat <span class="hlt">release</span> behavior is known, the only experimental data needed for detailed stability analysis is one instantaneous picture of heat <span class="hlt">release</span> at the peak pressure phase. This model was successfully tested in the dump combustor experiments, reproducing the correct sign of the overall Rayleigh index as well as the remarkably accurate spatial distribution pattern of fluctuating heat <span class="hlt">release</span>. Active combustion control was explored for fuel-flexible combustor operation using twelve different jet fuels including bio-synthetic and Fischer-Tropsch types. Analysis done using an actuated spray combustion model revealed that the combustion response times of these fuels were similar. Combined with experimental spray characterizations, this suggested that controller performance should remain effective with various alternative fuels</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22314728-procedure-recovery-pin-pin-fields-energy-release-core-vver-type-reactor-bipr-code','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22314728-procedure-recovery-pin-pin-fields-energy-release-core-vver-type-reactor-bipr-code"><span>Procedure of recovery of pin-by-pin fields of <span class="hlt">energy</span> <span class="hlt">release</span> in the core of VVER-type reactor for the BIPR-8 code</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Gordienko, P. V., E-mail: gorpavel@vver.kiae.ru; Kotsarev, A. V.; Lizorkin, M. P.</p> <p>2014-12-15</p> <p>The procedure of recovery of pin-by-pin <span class="hlt">energy-release</span> fields for the BIPR-8 code and the algorithm of the BIPR-8 code which is used in nodal computation of the reactor core and on which the recovery of pin-by-pin fields of <span class="hlt">energy</span> <span class="hlt">release</span> is based are briefly described. The description and results of the verification using the module of recovery of pin-by-pin <span class="hlt">energy-release</span> fields and the TVS-M program are given.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_6");'>6</a></li> <li><a href="#" onclick='return showDiv("page_7");'>7</a></li> <li class="active"><span>8</span></li> <li><a href="#" onclick='return showDiv("page_9");'>9</a></li> <li><a href="#" onclick='return showDiv("page_10");'>10</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_8 --> <div id="page_9" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_7");'>7</a></li> <li><a href="#" onclick='return showDiv("page_8");'>8</a></li> <li class="active"><span>9</span></li> <li><a href="#" onclick='return showDiv("page_10");'>10</a></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="161"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/25615343','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25615343"><span>Fluctuations of global <span class="hlt">energy</span> <span class="hlt">release</span> and crackling in nominally brittle heterogeneous fracture.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Barés, J; Hattali, M L; Dalmas, D; Bonamy, D</p> <p>2014-12-31</p> <p>The temporal evolution of mechanical <span class="hlt">energy</span> and spatially averaged crack speed are both monitored in slowly fracturing artificial rocks. Both signals display an irregular burstlike dynamics, with power-law distributed fluctuations spanning a broad range of scales. Yet, the elastic power <span class="hlt">released</span> at each time step is proportional to the global velocity all along the process, which enables defining a material-constant fracture <span class="hlt">energy</span>. We characterize the intermittent dynamics by computing the burst statistics. This latter displays the scale-free features signature of crackling dynamics, in qualitative but not quantitative agreement with the depinning interface models derived for fracture problems. The possible sources of discrepancies are pointed out and discussed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27802110','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27802110"><span>Base <span class="hlt">Release</span> and Modification in Solid-Phase DNA Exposed to Low-<span class="hlt">Energy</span> Electrons.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Choofong, Surakarn; Cloutier, Pierre; Sanche, Léon; Wagner, J Richard</p> <p>2016-11-01</p> <p>Ionization generates a large number of secondary low-<span class="hlt">energy</span> electrons (LEEs) with a most probable <span class="hlt">energy</span> of approximately 10 eV, which can break DNA bonds by dissociative electron attachment (DEA) and lead to DNA damage. In this study, we investigated radiation damage to dry DNA induced by X rays (1.5 keV) alone on a glass substrate or X rays combined with extra LEEs (average <span class="hlt">energy</span> of 5.8 eV) emitted from a tantalum (Ta) substrate under an atmosphere of N 2 and standard ambient conditions of temperature and pressure. The targets included calf-thymus DNA and double-stranded synthetic oligonucleotides. We developed analytical methods to measure the <span class="hlt">release</span> of non-modified DNA bases from DNA and the formation of several base modifications by LC-MS/MS with isotopic dilution for precise quantification. The results show that the yield of non-modified bases as well as base modifications increase by 20-30% when DNA is deposited on a Ta substrate compared to that on a glass substrate. The order of base <span class="hlt">release</span> (Gua > Ade > Thy ∼ Cyt) agrees well with several theoretical studies indicating that Gua is the most susceptible site toward sugar-phosphate cleavage. The formation of DNA damage by LEEs is explained by DEA leading to the <span class="hlt">release</span> of non-modified bases involving the initial cleavage of N1-C1', C3'-O3' or C5'-O5' bonds. The yield of base modifications was lower than the <span class="hlt">release</span> of non-modified bases. The main LEE-induced base modifications include 5,6-dihydrothymine (5,6-dHT), 5,6-dihydrouracil (5-dHU), 5-hydroxymethyluracil (5-HmU) and 5-formyluracil (5-ForU). The formation of base modifications by LEEs can be explained by DEA and cleavage of the C-H bond of the methyl group of Thy (giving 5-HmU and 5-ForU) and by secondary reactions of H atoms and hydride anions that are generated by primary LEE reactions followed by subsequent reaction with Cyt and Thy (giving 5,6-dHU and 5,6-dHT).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19790006995','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19790006995"><span>Application of the relative <span class="hlt">energy</span> <span class="hlt">release</span> criteria to enclosure fire testing. [aircraft compartments</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Roschke, E. J.; Coulbert, C. D.</p> <p>1979-01-01</p> <p>The five relative <span class="hlt">energy</span> <span class="hlt">release</span> criteria (RERC) which are a first step towards formulating a unified concept that can be applied to the development of fires in enclosures, place upper bounds on the rate and amount of <span class="hlt">energy</span> <span class="hlt">released</span> during a fire. They are independent, calculated readily, and may be applied generally to any enclosure regardless of size. They are useful in pretest planning and for interpreting experimental data. Data from several specific fire test programs were examined to evaluate the potential use of RERC to provide test planning guidelines. The RERC were compared with experimental data obtained in full-scale enclosures. These results confirm that in general the RERC do identify the proper limiting constraints on enclosure fire development and determine the bounds of the fire development envelope. Plotting actual fire data against the RERC reveals new valid insights into fire behavior and reveals the controlling constraints in fire development. The RERC were calculated and plotted for several descrpitions of full-scale fires in various aircraft compartments.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017IAUS..327...94D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017IAUS..327...94D"><span>Understanding the connection between the <span class="hlt">energy</span> <span class="hlt">released</span> during solar flares and their emission in the lower atmosphere</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>da Costa, F. Rubio</p> <p>2017-10-01</p> <p>While progress has been made on understanding how <span class="hlt">energy</span> is <span class="hlt">released</span> and deposited along the solar atmosphere during explosive events such as solar flares, the chromospheric and coronal heating through the sudden <span class="hlt">release</span> of magnetic <span class="hlt">energy</span> remain an open problem in solar physics. Recent hydrodynamic models allow to investigate the <span class="hlt">energy</span> deposition along a flare loop and to study the response of the chromosphere. These results have been improved with the consideration of transport and acceleration of particles along the loop. RHESSI and Fermi/GBM X-ray and gamma-ray observations help to constrain the spectral properties of the injected electrons. The excellent spatial, spectral and temporal resolution of IRIS will also help us to constrain properties of explosive events, such as the continuum emission during flares or their emission in the chromosphere.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017PAN....80.1683K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017PAN....80.1683K"><span>Computer Simulation of Compression and <span class="hlt">Energy</span> <span class="hlt">Release</span> upon Laser Irradiation of Cylindrically Symmetric Target</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kuzenov, V. V.</p> <p>2017-12-01</p> <p>The paper is devoted to the theoretical and computational study of compression and <span class="hlt">energy</span> <span class="hlt">release</span> for magneto-inertial plasma confinement. This approach makes it possible to create new high-density plasma sources, apply them in materials science experiments, and use them in promising areas of power engineering.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1226128','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/1226128"><span>Fission Fragment Mass Distributions and Total Kinetic <span class="hlt">Energy</span> <span class="hlt">Release</span> of 235-Uranium and 238-Uranium in Neutron-Induced Fission at Intermediate and Fast Neutron <span class="hlt">Energies</span></span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Duke, Dana Lynn</p> <p>2015-11-12</p> <p>This Ph.D. dissertation describes a measurement of the change in mass distributions and average total kinetic <span class="hlt">energy</span> (TKE) <span class="hlt">release</span> with increasing incident neutron <span class="hlt">energy</span> for fission of 235U and 238U. Although fission was discovered over seventy-five years ago, open questions remain about the physics of the fission process. The <span class="hlt">energy</span> of the incident neutron, En, changes the division of <span class="hlt">energy</span> <span class="hlt">release</span> in the resulting fission fragments, however, the details of <span class="hlt">energy</span> partitioning remain ambiguous because the nucleus is a many-body quantum system. Creating a full theoretical model is difficult and experimental data to validate existing models are lacking. Additional fissionmore » measurements will lead to higher-quality models of the fission process, therefore improving applications such as the development of next-generation nuclear reactors and defense. This work also paves the way for precision experiments such as the Time Projection Chamber (TPC) for fission cross section measurements and the Spectrometer for Ion Determination in Fission (SPIDER) for precision mass yields.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19890038958&hterms=end+theory&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3DThe%2Bend%2Btheory','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19890038958&hterms=end+theory&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3DThe%2Bend%2Btheory"><span>Strain <span class="hlt">energy</span> <span class="hlt">release</span> rate analysis of the end-notched flexure specimen using the finite-element method</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Salpekar, S. A.; Raju, I. S.; O'Brien, T. K.</p> <p>1988-01-01</p> <p>Two-dimensional finite-element analysis of the end-notched flexure specimen was performed using 8-node isoparametric, parabolic elements to evaluate compliance and mode II strain <span class="hlt">energy</span> <span class="hlt">release</span> rates, G sub II. The G sub II values were computed using two different techniques: the virtual crack-closure technique (VCCT) and the rate of change of compliance with crack length (compliance derivative method). The analysis was performed for various crack-length-to-semi-span (a/L) ratios ranging from 0.2 to 0.9. Three material systems representing a wide range of material properties were analyzed. The compliance and strain <span class="hlt">energy</span> <span class="hlt">release</span> rates of the specimen calculated with the present finite-element analysis agree very well with beam theory equations including transverse shear. The G sub II values calculated using the compliance derivative method compared extremely well with those calculated using the VCCT. The G sub II values obtained by the compliance derivative method using the top or bottom beam deflections agreed closely with each other. The strain <span class="hlt">energy</span> <span class="hlt">release</span> rates from a plane-stress analysis were higher than the plane-strain values by only a small percentage, indicating that either assumption may be used in the analysis. The G sub II values for one material system calculated from the finte-element analysis agreed with one solution in the literature and disagreed with the other solution in the literature.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19880004353','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19880004353"><span>Strain-<span class="hlt">energy-release</span> rate analysis of the end-notched flexure specimen using the finite-element method</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Salpekar, S. A.; Raju, I. S.; Obrien, T. K.</p> <p>1987-01-01</p> <p>Two-dimensional finite-element analysis of the end-notched flexure specimen was performed using 8-node isoparametric, parabolic elements to evaluate compliance and mode II strain <span class="hlt">energy</span> <span class="hlt">release</span> rates, G sub II. The G sub II values were computed using two different techniques: the virtural crack-closure technique (VCCT) and the rate of change of compliance with crack length (compliance derivative method). The analysis was performed for various crack-length-to-semi-span (a/L) ratios ranging from 0.2 to 0.9. Three material systems representing a wide range of material properties were analyzed. The compliance and strain <span class="hlt">energy</span> <span class="hlt">release</span> rates of the specimen calculated with the present finite-element analysis agree very well with beam theory equations including transverse shear. The G sub II values calculated using the compliance derivative method compared extremely well with those calculated using the VCCT. The G sub II values obtained by the compliance derivative method using the top or bottom beam deflections agreed closely with each other. The strain <span class="hlt">energy</span> <span class="hlt">release</span> rates from a plane-stress analysis were higher than the plane-strain values by only a small percentage, indicating that either assumption may be used in the analysis. The G sub II values for one material system calculated from the finite-element analysis agreed with one solution in the literature and disagreed with the other solution in the literature.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.fs.usda.gov/treesearch/pubs/32776','TREESEARCH'); return false;" href="https://www.fs.usda.gov/treesearch/pubs/32776"><span>Relationships between <span class="hlt">energy</span> <span class="hlt">release</span>, fuel mass loss, and trace gas and aerosol emissions during laboratory biomass fires</span></a></p> <p><a target="_blank" href="http://www.fs.usda.gov/treesearch/">Treesearch</a></p> <p>Patrick H. Freeborn; Martin J. Wooster; Wei Min Hao; Cecily A. Nordgren Ryan; Stephen P. Baker; Charles Ichoku</p> <p>2008-01-01</p> <p>Forty-four small-scale experimental fires were conducted in a combustion chamber to examine the relationship between biomass consumption, smoke production, convective <span class="hlt">energy</span> <span class="hlt">release</span>, and middle infrared (MIR) measurements of fire radiative <span class="hlt">energy</span> (FRE). Fuel bed weights, trace gas and aerosol particle concentrations, stack flow rate and temperature, and concurrent...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018AIPA....8c5013J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018AIPA....8c5013J"><span>The effect of explosive percentage on underwater explosion <span class="hlt">energy</span> <span class="hlt">release</span> of hexanitrohexaazaisowurtzitane and octogen based aluminized explosives</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Jiao, Qingjie; Wang, Qiushi; Nie, Jianxin; Guo, Xueyong; Zhang, Wei; Fan, Wenqi</p> <p>2018-03-01</p> <p>To control the explosion <span class="hlt">energy</span> output by optimizing explosive components is a key requirement in a number of different application areas. The effect of different Al/O Ratio on underwater explosion of aluminized explosives has been studied detailedly. However, the effect of explosive percentage in the same Al/O Ratio is rarely researched, especially for Hexanitrohexaazaisowurtzitane (CL-20) based aluminized explosives. In this study, we performed the underwater explosion experiments with 1.2-kilogram explosives in order to investigate the explosion <span class="hlt">energy</span> <span class="hlt">released</span> from CL-20 and Octogen (HMX) based aluminized explosives. The percentage of the explosive varied from 5% to 30% and it is shown that: the shockwave peak pressure (pm) grows gradually; shock wave <span class="hlt">energy</span> (Es) continues increasing, bubble <span class="hlt">energy</span> (Eb) increases then decreases peaking at 15% for both formulas, and the total <span class="hlt">energy</span> (E) and <span class="hlt">energy</span> <span class="hlt">release</span> rate (η) peak at 20% for CL-20 and 15% for HMX. This paper outlines the physical mechanism of Eb change under the influence of an aluminium initial reaction temperature and reaction active detonation product percentage coupling. The result shows that CL-20 is superior as a new high explosive and has promising application prospects in the regulation of explosive <span class="hlt">energy</span> output for underwater explosives.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/15259957','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/15259957"><span>Sludge thermal oxidation processes: mineral recycling, <span class="hlt">energy</span> impact, and greenhouse effect gases <span class="hlt">release</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Guibelin, E</p> <p>2004-01-01</p> <p>Different treatment routes have been studied for a mixed sludge: the conventional agricultural use is compared with the thermal oxidation processes, including incineration (in gaseous phase) and wet air oxidation (in liquid phase). The interest of a sludge digestion prior to the final treatment has been also considered according to the two major criteria, which are the fossil <span class="hlt">energy</span> utilisation and the greenhouse effect gases (CO2, CH4, N2O) <span class="hlt">release</span>. Thermal <span class="hlt">energy</span> has to be recovered on thermal processes to make these processes environmentally friendly, otherwise their main interest is to extract or destroy micropollutants and pathogens from the carbon cycle. In case of continuous <span class="hlt">energy</span> recovery, incineration can produce more <span class="hlt">energy</span> than it consumes. Digestion is especially interesting for agriculture: according to these two schemes, the <span class="hlt">energy</span> final balance can also be in excess. As to wet air oxidation, it is probably one of the best ways to minimize greenhouse effect gases emission.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20150010747&hterms=corona&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3Dcorona','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20150010747&hterms=corona&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3Dcorona"><span>Spatiotemporal Organization of <span class="hlt">Energy</span> <span class="hlt">Release</span> Events in the Quiet Solar Corona</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Uritsky, Vadim M.; Davila, Joseph M.</p> <p>2014-01-01</p> <p>Using data from the STEREO and SOHO spacecraft, we show that temporal organization of <span class="hlt">energy</span> <span class="hlt">release</span> events in the quiet solar corona is close to random, in contrast to the clustered behavior of flaring times in solar active regions. The locations of the quiet-Sun events follow the meso- and supergranulation pattern of the underling photosphere. Together with earlier reports of the scale-free event size statistics, our findings suggest that quiet solar regions responsible for bulk coronal heating operate in a driven self-organized critical state, possibly involving long-range Alfvenic interactions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29133908','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29133908"><span>Optically-controlled long-term storage and <span class="hlt">release</span> of thermal <span class="hlt">energy</span> in phase-change materials.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Han, Grace G D; Li, Huashan; Grossman, Jeffrey C</p> <p>2017-11-13</p> <p>Thermal <span class="hlt">energy</span> storage offers enormous potential for a wide range of <span class="hlt">energy</span> technologies. Phase-change materials offer state-of-the-art thermal storage due to high latent heat. However, spontaneous heat loss from thermally charged phase-change materials to cooler surroundings occurs due to the absence of a significant <span class="hlt">energy</span> barrier for the liquid-solid transition. This prevents control over the thermal storage, and developing effective methods to address this problem has remained an elusive goal. Herein, we report a combination of photo-switching dopants and organic phase-change materials as a way to introduce an activation <span class="hlt">energy</span> barrier for phase-change materials solidification and to conserve thermal <span class="hlt">energy</span> in the materials, allowing them to be triggered optically to <span class="hlt">release</span> their stored latent heat. This approach enables the retention of thermal <span class="hlt">energy</span> (about 200 J g -1 ) in the materials for at least 10 h at temperatures lower than the original crystallization point, unlocking opportunities for portable thermal <span class="hlt">energy</span> storage systems.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMSH43A2805I','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMSH43A2805I"><span><span class="hlt">Energy</span> <span class="hlt">release</span> from a stream of infalling prominence debris on 2011 September 7-8</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Inglis, A. R.; Gilbert, H. R.; Ofman, L.</p> <p>2017-12-01</p> <p>In recent years high-resolution and high-cadence EUV imaging has revealed a new phenomenon, impacting prominence debris, where prominence material from failed or partial eruptions can impact the lower atmosphere and <span class="hlt">release</span> <span class="hlt">energy</span>. We present a clear example of this phenomenon occurring on 2011 September 7-8. The initial eruption of prominence material was associated with an X1.8-class flare from AR11283, occurring at 22:30 UT on 2011 September 7, resulting in a semi-continuous stream of this material returning to the solar surface between 00:20 - 00:40 UT on 2011 September 8. A substantial area remote from the original active region experienced brightening in multiple EUV channels observed by SDO/AIA. Using the differential emission measure, we estimated the energetic properties of this event. We found that the radiated <span class="hlt">energy</span> of the impacted plasma was of order 10^27 ergs, while the upper limit on the thermal <span class="hlt">energy</span> peaked at 10^28 ergs. Based on these estimates we were able to determine the mass content of the debris to be in the range 2x10^14 < m < 2x10^15 g. Given typical promimence masses, the likely debris mass is towards the lower end of this range. This clear example of a prominence debris event shows that significant <span class="hlt">energy</span> <span class="hlt">release</span> takes place during these events, and that such impacts may be used as a novel diagnostic tool for investigating prominence material properties.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010AGUFM.B41E0368K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010AGUFM.B41E0368K"><span>Influence of ultrasonic <span class="hlt">energy</span> on dispersion of aggregates and <span class="hlt">released</span> amounts of organic matter and polyvalent cations</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kaiser, M.; Kleber, M.; Berhe, A. A.</p> <p>2010-12-01</p> <p>Aggregates play important roles in soil carbon storage and stabilization. Identification of scale-dependent mechanisms of soil aggregate formation and stability is necessary to predict and eventually manage the flow of carbon through terrestrial ecosystems. Application of ultrasonic <span class="hlt">energy</span> is a common tool to disperse soil aggregates. In this study, we used ultra sonic <span class="hlt">energy</span> (100 to 2000 J cm-3) to determine the amount of polyvalent cations and organic matter involved in aggregation processes in three arable and three forest soils that varied in soil mineral composition. To determine the amount of organic matter and cations <span class="hlt">released</span> after application of different amount of ultrasonic <span class="hlt">energy</span>, we removed the coarse fraction (>250 µm). The remaining residue (<250 µm) was mixed with water and ultrasonically dispersed by application of 100, 200, 400, 500, 1000, 1500 and 2000 J cm-3 <span class="hlt">energy</span>. After centrifugation the supernatant was filtered and the solid residue freeze dried before we analyzed the amounts of water-extracted organic carbon (OC), Fe, Al, Ca, Mn, and Mg in the filtrates. The extracted OM and solid residues were further characterized by Fourier Transformed Infra Red spectroscopy and Scanning Electron Microscopy. Our results show a linear increase in amount of dissolved OC with increasing amounts of ultra sonic <span class="hlt">energy</span> up to 1500 J cm-3 indicating maximum dispersion of soil aggregates at this <span class="hlt">energy</span> level independent from soil type or land use. In contrast to Mn, and Mg, the amounts of dissolved Ca, Fe, and Al increase with increasing ultra sonic <span class="hlt">energy</span> up to 1500 J cm-3. At 1500 J cm-3, the absolute amounts of OC, Ca, Fe, and Al <span class="hlt">released</span> were specific for each soil type, likely indicating differences in type of OM-mineral interactions involved in micro-scaled aggregation processes. The amounts of dissolved Fe, and Al <span class="hlt">released</span> after an application of 1500 J cm-3 are not related to oxalate- and dithionite- extractable, or total Al content indicating less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19720019047','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19720019047"><span>Liquid rocket performance computer model with distributed <span class="hlt">energy</span> <span class="hlt">release</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Combs, L. P.</p> <p>1972-01-01</p> <p>Development of a computer program for analyzing the effects of bipropellant spray combustion processes on liquid rocket performance is described and discussed. The distributed <span class="hlt">energy</span> <span class="hlt">release</span> (DER) computer program was designed to become part of the JANNAF liquid rocket performance evaluation methodology and to account for performance losses associated with the propellant combustion processes, e.g., incomplete spray gasification, imperfect mixing between sprays and their reacting vapors, residual mixture ratio striations in the flow, and two-phase flow effects. The DER computer program begins by initializing the combustion field at the injection end of a conventional liquid rocket engine, based on injector and chamber design detail, and on propellant and combustion gas properties. It analyzes bipropellant combustion, proceeding stepwise down the chamber from those initial conditions through the nozzle throat.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19900052352&hterms=solar+energy&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Dsolar%2Benergy','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19900052352&hterms=solar+energy&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Dsolar%2Benergy"><span>Observational clues to the <span class="hlt">energy</span> <span class="hlt">release</span> process in impulsive solar bursts</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Batchelor, David</p> <p>1990-01-01</p> <p>The nature of the <span class="hlt">energy</span> <span class="hlt">release</span> process that produces impulsive bursts of hard X-rays and microwaves during solar flares is discussed, based on new evidence obtained using the method of Crannell et al. (1978). It is shown that the hard X-ray spectral index gamma is negatively correlated with the microwave peak frequency, suggesting a common source for the microwaves and X-rays. The thermal and nonthermal models are compared. It is found that the most straightforward explanations for burst time behavior are shock-wave particle acceleration in the nonthermal model and thermal conduction fronts in the thermal model.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22614032-energy-release-temperature-field-ultracold-neutron-source-wwr-reactor-petersburg-nuclear-physics-institute','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22614032-energy-release-temperature-field-ultracold-neutron-source-wwr-reactor-petersburg-nuclear-physics-institute"><span>The <span class="hlt">energy</span> <span class="hlt">release</span> and temperature field in the ultracold neutron source of the WWR-M reactor at the Petersburg Nuclear Physics Institute</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Serebrov, A. P., E-mail: serebrov@pnpi.spb.ru; Kislitsin, B. V.; Onegin, M. S.</p> <p>2016-12-15</p> <p>Results of calculations of <span class="hlt">energy</span> <span class="hlt">releases</span> and temperature fields in the ultracold neutron source under design at the WWR-M reactor are presented. It is shown that, with the reactor power of 18 MW, the power of <span class="hlt">energy</span> <span class="hlt">release</span> in the 40-L volume of the source with superfluid helium will amount to 28.5 W, while 356 W will be <span class="hlt">released</span> in a liquid-deuterium premoderator. The lead shield between the reactor core and the source reduces the radiative heat <span class="hlt">release</span> by an order of magnitude. A thermal power of 22 kW is <span class="hlt">released</span> in it, which is removed by passage of water.more » The distribution of temperatures in all components of the vacuum structure is presented, and the temperature does not exceed 100°C at full reactor power. The calculations performed make it possible to go to design of the source.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/ADA516406','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA516406"><span>Short Term Innovative Research Program: Nanoengineered Reactive Materials for Tunable Ignition and <span class="hlt">Energy</span> <span class="hlt">Release</span></span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>2009-01-01</p> <p>Background Most conventional explosives can be roughly categorized into two classes – molecular materials and intermolecular composites. Molecular...materials refer to species such as the nitroalkanes (e.g. nitromethane ) and cyclic nitramines (e.g. TNAZ, RDX, HMX) that <span class="hlt">release</span> chemical <span class="hlt">energy</span>...alternative to conventional explosives that has been gaining increasing interest have been termed reactive materials, and are defined as systems in</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/1184278-linear-free-energy-correlations-fission-product-release-from-fukushima-daiichi-nuclear-accident','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/1184278-linear-free-energy-correlations-fission-product-release-from-fukushima-daiichi-nuclear-accident"><span>Linear Free <span class="hlt">Energy</span> Correlations for Fission Product <span class="hlt">Release</span> from the Fukushima-Daiichi Nuclear Accident</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Abrecht, David G.; Schwantes, Jon M.</p> <p></p> <p>This paper extends the preliminary linear free <span class="hlt">energy</span> correlations for radionuclide <span class="hlt">release</span> performed by Schwantes, et al., following the Fukushima-Daiichi Nuclear Power Plant accident. Through evaluations of the molar fractionations of radionuclides deposited in the soil relative to modeled radionuclide inventories, we confirm the source of the radionuclides to be from active reactors rather than the spent fuel pool. Linear correlations of the form ln χ = -α (ΔG rxn°(T C))/(RT C)+β were obtained between the deposited concentration and the reduction potential of the fission product oxide species using multiple reduction schemes to calculate ΔG° rxn(T C). These models allowedmore » an estimate of the upper bound for the reactor temperatures of T C between 2130 K and 2220 K, providing insight into the limiting factors to vaporization and <span class="hlt">release</span> of fission products during the reactor accident. Estimates of the <span class="hlt">release</span> of medium-lived fission products 90Sr, 121mSn, 147Pm, 144Ce, 152Eu, 154Eu, 155Eu, 151Sm through atmospheric venting and <span class="hlt">releases</span> during the first month following the accident were performed, and indicate large quantities of 90Sr and radioactive lanthanides were likely to remain in the damaged reactor cores.« less</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_7");'>7</a></li> <li><a href="#" onclick='return showDiv("page_8");'>8</a></li> <li class="active"><span>9</span></li> <li><a href="#" onclick='return showDiv("page_10");'>10</a></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_9 --> <div id="page_10" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_8");'>8</a></li> <li><a href="#" onclick='return showDiv("page_9");'>9</a></li> <li class="active"><span>10</span></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="181"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.nrel.gov/news/press/1997/update2.html','SCIGOVWS'); return false;" href="https://www.nrel.gov/news/press/1997/update2.html"><span>Start Your <span class="hlt">Energy</span> Conversion Devices</span></a></p> <p><a target="_blank" href="http://www.science.gov/aboutsearch.html">Science.gov Websites</a></p> <p></p> <p></p> <p>:37 a.m. and 1:33 p.m. MIT's car took only 1 hour, 37 minutes and 8 seconds to travel the 65 <em>miles</em> at an average speed of 40.60 <em>miles</em> per hour. Closely following was Stanford University/University of California-Berkeley's <span class="hlt">Afterburner</span> II coming in at 1:37:25, with an average speed of 40.48 <em>miles</em> per hour</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010EGUGA..1210096K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010EGUGA..1210096K"><span>Soft computing analysis of the possible correlation between temporal and <span class="hlt">energy</span> <span class="hlt">release</span> patterns in seismic activity</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Konstantaras, Anthony; Katsifarakis, Emmanouil; Artzouxaltzis, Xristos; Makris, John; Vallianatos, Filippos; Varley, Martin</p> <p>2010-05-01</p> <p>This paper is a preliminary investigation of the possible correlation of temporal and <span class="hlt">energy</span> <span class="hlt">release</span> patterns of seismic activity involving the preparation processes of consecutive sizeable seismic events [1,2]. The background idea is that during periods of low-level seismic activity, stress processes in the crust accumulate <span class="hlt">energy</span> at the seismogenic area whilst larger seismic events act as a decongesting mechanism <span class="hlt">releasing</span> considerable <span class="hlt">energy</span> [3,4]. A dynamic algorithm is being developed aiming to identify and cluster pre- and post- seismic events to the main earthquake following on research carried out by Zubkov [5] and Dobrovolsky [6,7]. This clustering technique along with <span class="hlt">energy</span> <span class="hlt">release</span> equations dependent on Richter's scale [8,9] allow for an estimate to be drawn regarding the amount of the <span class="hlt">energy</span> being <span class="hlt">released</span> by the seismic sequence. The above approach is being implemented as a monitoring tool to investigate the behaviour of the underlying <span class="hlt">energy</span> management system by introducing this information to various neural [10,11] and soft computing models [1,12,13,14]. The incorporation of intelligent systems aims towards the detection and simulation of the possible relationship between <span class="hlt">energy</span> <span class="hlt">release</span> patterns and time-intervals among consecutive sizeable earthquakes [1,15]. Anticipated successful training of the imported intelligent systems may result in a real-time, on-line processing methodology [1,16] capable to dynamically approximate the time-interval between the latest and the next forthcoming sizeable seismic event by monitoring the <span class="hlt">energy</span> <span class="hlt">release</span> process in a specific seismogenic area. Indexing terms: pattern recognition, long-term earthquake precursors, neural networks, soft computing, earthquake occurrence intervals References [1] Konstantaras A., Vallianatos F., Varley M.R. and Makris J. P.: ‘Soft computing modelling of seismicity in the southern Hellenic arc', IEEE Geoscience and Remote Sensing Letters, vol. 5 (3), pp. 323-327, 2008 [2] Eneva M. and</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3946412','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3946412"><span>Noninvasive Fluorescence Resonance <span class="hlt">Energy</span> Transfer Imaging of in vivo Premature Drug <span class="hlt">Release</span> from Polymeric Nanoparticles</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Zou, Peng; Chen, Hongwei; Paholak, Hayley J.; Sun, Duxin</p> <p>2013-01-01</p> <p>Understanding in vivo drug <span class="hlt">release</span> kinetics is critical for the development of nanoparticle-based delivery systems. In this study, we developed a fluorescence resonance <span class="hlt">energy</span> transfer (FRET) imaging approach to noninvasively monitor in vitro and in vivo cargo <span class="hlt">release</span> from polymeric nanoparticles. The FRET donor dye (DiO or DiD) and acceptor dye (DiI or DiR) were individually encapsulated into poly(ethylene oxide)-b-polystyrene (PEO-PS) nanoparticles. When DiO (donor) nanoparticles and DiI (acceptor) nanoparticles were co-incubated with cancer cells for 2 h, increased FRET signals were observed from cell membranes, suggesting rapid <span class="hlt">release</span> of DiO and DiI to cell membranes. Similarly, increased FRET ratios were detected in nude mice after intravenous co-administration of DiD (donor) nanoparticles and DiR (acceptor) nanoparticles. In contrast, another group of nude mice i.v. administrated with DiD/DiR co-loaded nanoparticles showed decreased FRET ratios. Based on the difference in FRET ratios between the two groups, in vivo DiD/DiR <span class="hlt">release</span> half-life from PEO-PS nanoparticles was determined to be 9.2 min. In addition, it was observed that the presence of cell membranes facilitated burst <span class="hlt">release</span> of lipophilic cargos while incorporation of oleic acid-coated iron oxide into PEO-PS nanoparticles slowed the <span class="hlt">release</span> of DiD/DiR to cell membranes. The developed in vitro and in vivo FRET imaging techniques can be used to screening stable nano-formulations for lipophilic drug delivery. PMID:24033270</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.eia.gov/consumption/manufacturing/reports/2010/early_estimates.cfm','EIAPUBS'); return false;" href="https://www.eia.gov/consumption/manufacturing/reports/2010/early_estimates.cfm"><span>Early-<span class="hlt">release</span> Estimates From the 2010 MECS Show That <span class="hlt">Energy</span> Consumption In the Manufacturing Sector Decreased Between 2006 and 2010</span></a></p> <p><a target="_blank" href="http://www.eia.doe.gov/reports/">EIA Publications</a></p> <p></p> <p>2012-01-01</p> <p><span class="hlt">Energy</span> consumption in the U.S. manufacturing sector fell from 21,098 trillion Btu (tBtu) in 2006 to 19,062 tBtu in 2010, a decline of almost 10% , based on preliminary estimates <span class="hlt">released</span> from the 2010 Manufacturing <span class="hlt">Energy</span> Consumption Survey (MECS). This decline continues the downward trend in manufacturing <span class="hlt">energy</span> use since the 1998 MECS report.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19990028196','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19990028196"><span>"2001: A Space Odyssey" Revisited--The Feasibility of 24 Hour Commuter Flights to the Moon Using NTR Propulsion with LUNOX <span class="hlt">Afterburners</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Borowski, Stanley K.; Dudzinski, Leonard A.</p> <p>1998-01-01</p> <p>The prospects for "24 hour" commuter flights to the Moon, similar to that portrayed in 2001: A Space Odyssey but on a more Spartan scale, are examined using two near term, "high leverage" technologies--liquid oxygen (LOX)-augmented nuclear thermal rocket (NTR) propulsion and "lunar-derived" oxygen (LUNOX) production. Ironrich volcanic glass, or "orange soil," discovered during the Apollo 17 mission to Taurus-Littrow, has produced a 4% oxygen yield in recent NASA experiments using hydrogen reduction. LUNOX development and utilization would eliminate the need to transport oxygen supplies from Earth and is expected to dramatically reduce the size, cost and complexity of space transportation systems. The LOX-augmented NTR concept (LANTR) exploits the high performance capability of the conventional liquid hydrogen (LH2)-cooled NTR and the mission leverage provided by LUNOX in a unique way, LANTR utilizes the large divergent section of its nozzle as an "<span class="hlt">afterburner</span>" into which oxygen is injected and supersonically combusted with nuclear preheated hydrogen emerging front the engine's choked sonic throat--essentially "scramjet propulsion in reverse." By varying the oxygen-to-hydrogen mixture ratio, the LANTR engine can operate over a wide range of thrust and specific impulse (Isp) values while the reactor core power level remains relatively constant. The thrust augmentation feature of LANTR means that "big engine" performance can be obtained using smaller, more affordable, easier to test NTR engines. The use of high-density LOX in place of low-density LH2 also reduces hydrogen mass and tank volume resulting in smaller space vehicles. An implementation strategy and evolutionary lunar mission architecture is outlined which requires only Shuttle C or "in-line" Shuttle-derived launch vehicles, and utilizes conventional NTR-powered lunar transfer vehicles (LTVs), operating in an "expendable mode" initially, to maximize delivered surface payload on each mission. The increased</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.A41F2363C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.A41F2363C"><span>Advancing Knowledge on Fugitive Natural Gas from <span class="hlt">Energy</span> Resource Development at a Controlled <span class="hlt">Release</span> Field Observatory</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Cahill, A. G.; Chao, J.; Forde, O.; Prystupa, E.; Mayer, K. U.; Black, T. A.; Tannant, D. D.; Crowe, S.; Hallam, S.; Mayer, B.; Lauer, R. M.; van Geloven, C.; Welch, L. A.; Salas, C.; Levson, V.; Risk, D. A.; Beckie, R. D.</p> <p>2017-12-01</p> <p>Fugitive gas, comprised primarily of methane, can be unintentionally <span class="hlt">released</span> from upstream oil and gas development either at surface from leaky infrastructure or in the subsurface through failure of <span class="hlt">energy</span> well bore integrity. For the latter, defective cement seals around <span class="hlt">energy</span> well casings may permit buoyant flow of natural gas from the deeper subsurface towards shallow aquifers, the ground surface and potentially into the atmosphere. Concerns associated with fugitive gas <span class="hlt">release</span> at surface and in the subsurface include contributions to greenhouse gas emissions, subsurface migration leading to accumulation in nearby infrastructure and impacts to groundwater quality. Current knowledge of the extent of fugitive gas leakage including how to best detect and monitor over time, and particularly its migration and fate in the subsurface, is incomplete. We have established an experimental field observatory for evaluating fugitive gas leakage in an area of historic and ongoing hydrocarbon resource development within the Montney Resource Play of the Western Canadian Sedimentary Basin, British Columbia, Canada. Natural gas will be intentionally <span class="hlt">released</span> at surface and up to 25 m below surface at various rates and durations. Resulting migration patterns and impacts will be evaluated through examination of the geology, hydrogeology, hydro-geochemistry, isotope geochemistry, hydro-geophysics, vadose zone and soil gas processes, microbiology, and atmospheric conditions. The use of unmanned aerial vehicles and remote sensors for monitoring and detection of methane will also be assessed for suitability as environmental monitoring tools. Here we outline the experimental design and describe initial research conducted to develop a detailed site conceptual model of the field observatory. Subsequently, results attained from pilot surface and sub-surface controlled natural gas <span class="hlt">releases</span> conducted in late summer 2017 will be presented as well as results of numerical modelling conducted</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.nrel.gov/news/press/1996/','SCIGOVWS'); return false;" href="https://www.nrel.gov/news/press/1996/"><span>1996 News <span class="hlt">Releases</span> | NREL</span></a></p> <p><a target="_blank" href="http://www.science.gov/aboutsearch.html">Science.gov Websites</a></p> <p></p> <p></p> <p>6 News <span class="hlt">Releases</span> Access news stories about the laboratory and renewable <em><span class="hlt">energy</span></em> and <em><span class="hlt">energy</span></em> efficiency Facility Slashes <em><span class="hlt">Energy</span></em> Use by 66 Percent - (10/3/96) Agreement Moves Nevada Solar Plant Step Closer to Converter Wins National Award - (7/25/96) Solar <em><span class="hlt">Energy</span></em> to Help Heat Major Commercial Facility - (6/21/96</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013JPhB...46x5201R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013JPhB...46x5201R"><span>Ion-polycyclic aromatic hydrocarbon collisions: kinetic <span class="hlt">energy</span> <span class="hlt">releases</span> for specific fragmentation channels</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Reitsma, G.; Zettergren, H.; Boschman, L.; Bodewits, E.; Hoekstra, R.; Schlathölter, T.</p> <p>2013-12-01</p> <p>We report on 30 keV He2 + collisions with naphthalene (C10H8) molecules, which leads to very extensive fragmentation. To unravel such complex fragmentation patterns, we designed and constructed an experimental setup, which allows for the determination of the full momentum vector by measuring charged collision products in coincidence in a recoil ion momentum spectrometer type of detection scheme. The determination of fragment kinetic <span class="hlt">energies</span> is found to be considerably more accurate than for the case of mere coincidence time-of-flight spectrometers. In fission reactions involving two cationic fragments, typically kinetic <span class="hlt">energy</span> <span class="hlt">releases</span> of 2-3 eV are observed. The results are interpreted by means of density functional theory calculations of the reverse barriers. It is concluded that naphthalene fragmentation by collisions with keV ions clearly is much more violent than the corresponding photofragmentation with energetic photons. The ion-induced naphthalene fragmentation provides a feedstock of various small hydrocarbonic species of different charge states and kinetic <span class="hlt">energy</span>, which could influence several molecule formation processes in the cold interstellar medium and facilitates growth of small hydrocarbon species on pre-existing polycyclic aromatic hydrocarbons.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/21251711','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/21251711"><span>Intracellularly monitoring/imaging the <span class="hlt">release</span> of doxorubicin from pH-responsive nanoparticles using Förster resonance <span class="hlt">energy</span> transfer.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Chen, Ko-Jie; Chiu, Ya-Ling; Chen, Yu-Ming; Ho, Yi-Cheng; Sung, Hsing-Wen</p> <p>2011-04-01</p> <p>Stimuli-responsive nanoparticles (NPs) have been receiving much attention as a drug-delivery vehicle for therapeutic applications; once internalized into cells, the intracellular fate of NPs and their drug <span class="hlt">release</span> behavior in response to local stimuli must be understood for efficient delivery of therapeutics. In this study, we prepared pH-responsive doxorubicin (DOX)-loaded NPs, made of N-palmitoyl chitosan bearing a Cy5 moiety (Cy5-NPCS), as an anticancer delivery device. The results of our molecular dynamic simulations showed that the ability of Cy5-NPCS to self-associate offered the close proximity between the donor (DOX) and the acceptor (Cy5) required for Förster resonance <span class="hlt">energy</span> transfer (FRET), while the pH-driven structure transition prescribed the on-to-off switch of the <span class="hlt">energy</span> transfer. The caveolae-mediated pathway played a major role in the internalization of NPCS NPs. Using the concept of FRET, we found that the DOX fluorescence in the cytosol was first seen when NPCS NPs were present in the slightly acidic early endosomes. Following NPCS NPs trafficking into a more acidic organelle (late endosomes/lysosomes), a more evident <span class="hlt">release</span> of DOX into the cytosol was observed; the <span class="hlt">released</span> DOX was then gradually accumulated in the cell nuclei, leading to a significant cytotoxicity. Understanding the fate of NPs with respect to their intracellular localization and drug <span class="hlt">release</span> behavior is crucial for the rational design of drug carriers. Copyright © 2010 Elsevier Ltd. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20030067859','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20030067859"><span>2001: A Space Odyssey Revisited: The Feasibility of 24 Hour Commuter Flights to the Moon Using NTR Propulsion with LUNOX <span class="hlt">Afterburners</span>. Revised</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Borowski, Stanley; Dudzinski, Leonard A.</p> <p>2003-01-01</p> <p>The prospects for 24 hour commuter flights to the Moon, similar to that portrayed in 2001: A Space Odyssey but on a more Spartan scale, are examined using two near term, high leverage technologies: liquid oxygen (LOX)-augmented nuclear thermal rocket (NTR) propulsion and lunar-derived oxygen (LUNOX) production. Iron-rich volcanic glass, or orange soil, discovered during the Apollo 17 mission to Taurus-Littrow, has produced a 4 percent oxygen yield in recent NASA experiments using hydrogen reduction. LUNOX development and utilization would eliminate the need to transport oxygen supplies from Earth and is expected to dramatically reduce the size, cost and complexity of space transportation systems. The LOX-augmented NTR concept (LANTR) exploits the high performance capability of the conventional liquid hydrogen (LH2)-cooled NTR and the mission leverage provided by LUNOX in a unique way. LANTR utilizes the large divergent section of its nozzle as an <span class="hlt">afterburner</span> into which oxygen is injected and supersonically combusted with nuclear preheated hydrogen emerging from the engine's choked sonic throat, essentially scramjet propulsion in reverse. By varying the oxygen-to-hydrogen mixture ratio, the LANTR engine can operate over a wide range of thrust and specific impulse (Isp) values while the reactor core power level remains relatively constant. The thrust augmentation feature of LANTR means that big engine performance can be obtained using smaller, more affordable, easier to test NTR engines. The use of high-density LOX in place of low density LH2 also reduces hydrogen mass and tank volume resulting in smaller space vehicles. An implementation strategy and evolutionary lunar mission architecture is outlined which requires only Shuttle C or in-line Shuttle-derived launch vehicles, and utilizes conventional NTR-powered lunar transfer vehicles (LTVs), operating in an expendable mode initially, to maximize delivered surface payload on each mission. The increased payload is</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20020022207','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20020022207"><span>"2001: A Space Odyssey" Revisited: The Feasibility of 24 Hour Commuter Flights to the Moon Using NTR Propulsion with LUNOX <span class="hlt">Afterburners</span>. Revised</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Borowski, Stanley K.; Dudzinski, Leonard A.</p> <p>2001-01-01</p> <p>The prospects for "24 hour" commuter flights to the Moon. similar to that portrayed in 2001: A Space Odyssey but on a more Spartan scale. are examined using two near term. "high leverage" technologies-liquid oxygen (LOX)-augmented nuclear thermal rocket (NTR) propulsion and "lunar-derived" oxygen (LUNOX) production. Iron-rich volcanic glass. or "orange soil," discovered during the Apollo 17 mission to Taurus-Littrow. has produced a 4% oxygen yield in recent NASA experiments using hydrogen reduction. LUNOX development and utilization would eliminate the need to transport oxygen supplies from Earth and is expected to dramatically reduce the size, cost and complexity of space transportation systems. The LOX-augmented NTR concept (LANTR) exploits the high performance capability of the conventional liquid hydrogen (LH2)-cooled NTR and the mission leverage provided by LUNOX in a unique way. LANTR utilizes the large divergent section of its nozzle as an "<span class="hlt">afterburner</span>" into which oxygen is injected and supersonically combusted with nuclear preheated hydrogen emerging from the engine's choked sonic throat-essentially "scramjet propulsion in reverse." By varying the oxygen-to-hydrogen mixture ratio, the LANTR engine can operate over a wide range of thrust and specific impulse (Isp) values while the reactor core power level remains relatively constant. The thrust augmentation feature of LANTR means that "big engine" performance can be obtained using smaller. more affordable. easier to test NTR engines. The use of high-density LOX in place of low-density LH2 also reduces hydrogen mass and tank volume resulting in smaller space vehicles. An implementation strategy and evolutionary lunar mission architecture is outlined which requires only Shuttle C or "in-line" Shuttle-derived launch vehicles, and utilizes conventional NTR-powered lunar transfer vehicles (LTVs), operating in an "expendable mode" initially, to maximize delivered surface payload on each mission. The increased</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/ADA588136','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA588136"><span>Optical Pressure Measurements of Explosions</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>2013-09-01</p> <p>near field detonation product gases can have a significant effect upon <span class="hlt">afterburn</span> ignition times (4). The implication being that <span class="hlt">afterburning</span> times...can be tuned to bring detonation product <span class="hlt">afterburning</span> into proximity of the leading shock, influencing brisance, and explosive impulse on target. 3...R. Z.; McAndrew, B. A. <span class="hlt">Afterburn</span> Ignition Delay and Shock Augmentation in Fuel Rich Solid Explosives. Propellants, Explosives, Pyrotechnics 2010</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AIPC.1683b0121L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AIPC.1683b0121L"><span>DEM code-based modeling of <span class="hlt">energy</span> accumulation and <span class="hlt">release</span> in structurally heterogeneous rock masses</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lavrikov, S. V.; Revuzhenko, A. F.</p> <p>2015-10-01</p> <p>Based on discrete element method, the authors model loading of a physical specimen to describe its capacity to accumulate and <span class="hlt">release</span> elastic <span class="hlt">energy</span>. The specimen is modeled as a packing of particles with viscoelastic coupling and friction. The external elastic boundary of the packing is represented by particles connected by elastic springs. The latter means introduction of an additional special potential of interaction between the boundary particles, that exercises effect even when there is no direct contact between the particles. On the whole, the model specimen represents an element of a medium capable of accumulation of deformation <span class="hlt">energy</span> in the form of internal stresses. The data of the numerical modeling of the physical specimen compression and the laboratory testing results show good qualitative consistency.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/25675358','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25675358"><span>Linear free <span class="hlt">energy</span> correlations for fission product <span class="hlt">release</span> from the Fukushima-Daiichi nuclear accident.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Abrecht, David G; Schwantes, Jon M</p> <p>2015-03-03</p> <p>This paper extends the preliminary linear free <span class="hlt">energy</span> correlations for radionuclide <span class="hlt">release</span> performed by Schwantes et al., following the Fukushima-Daiichi Nuclear Power Plant accident. Through evaluations of the molar fractionations of radionuclides deposited in the soil relative to modeled radionuclide inventories, we confirm the initial source of the radionuclides to the environment to be from active reactors rather than the spent fuel pool. Linear correlations of the form In χ = −α ((ΔGrxn°(TC))/(RTC)) + β were obtained between the deposited concentrations, and the reduction potentials of the fission product oxide species using multiple reduction schemes to calculate ΔG°rxn (TC). These models allowed an estimate of the upper bound for the reactor temperatures of TC between 2015 and 2060 K, providing insight into the limiting factors to vaporization and <span class="hlt">release</span> of fission products during the reactor accident. Estimates of the <span class="hlt">release</span> of medium-lived fission products 90Sr, 121mSn, 147Pm, 144Ce, 152Eu, 154Eu, 155Eu, and 151Sm through atmospheric venting during the first month following the accident were obtained, indicating that large quantities of 90Sr and radioactive lanthanides were likely to remain in the damaged reactor cores.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/21298168','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/21298168"><span>Determination of differential cross sections and kinetic <span class="hlt">energy</span> <span class="hlt">release</span> of co-products from central sliced images in photo-initiated dynamic processes.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Chen, Kuo-mei; Chen, Yu-wei</p> <p>2011-04-07</p> <p>For photo-initiated inelastic and reactive collisions, dynamic information can be extracted from central sliced images of state-selected Newton spheres of product species. An analysis framework has been established to determine differential cross sections and the kinetic <span class="hlt">energy</span> <span class="hlt">release</span> of co-products from experimental images. When one of the reactants exhibits a high recoil speed in a photo-initiated dynamic process, the present theory can be employed to analyze central sliced images from ion imaging or three-dimensional sliced fluorescence imaging experiments. It is demonstrated that the differential cross section of a scattering process can be determined from the central sliced image by a double Legendre moment analysis, for either a fixed or continuously distributed recoil speeds in the center-of-mass reference frame. Simultaneous equations which lead to the determination of the kinetic <span class="hlt">energy</span> <span class="hlt">release</span> of co-products can be established from the second-order Legendre moment of the experimental image, as soon as the differential cross section is extracted. The intensity distribution of the central sliced image, along with its outer and inner ring sizes, provide all the clues to decipher the differential cross section and the kinetic <span class="hlt">energy</span> <span class="hlt">release</span> of co-products.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19810004372','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19810004372"><span>Gas <span class="hlt">release</span> and conductivity modification studies</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Linson, L. M.; Baxter, D. C.</p> <p>1979-01-01</p> <p>The behavior of gas clouds produced by <span class="hlt">releases</span> from orbital velocity in either a point <span class="hlt">release</span> or venting mode is described by the modification of snowplow equations valid in an intermediate altitude regime. Quantitative estimates are produced for the time dependence of the radius of the cloud, the average internal <span class="hlt">energy</span>, the translational velocity, and the distance traveled. The dependence of these quantities on the assumed density profile, the internal <span class="hlt">energy</span> of the gas, and the ratio of specific heats is examined. The new feature is the inclusion of the effect of the large orbital velocity. The resulting gas cloud models are used to calculate the characteristics of the field line integrated Pedersen conductivity enhancements that would be produced by the <span class="hlt">release</span> of barium thermite at orbital velocity in either the point <span class="hlt">release</span> or venting modes as a function of <span class="hlt">release</span> altitude and chemical payload weight.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AcAau.112..182L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AcAau.112..182L"><span><span class="hlt">Energy</span> <span class="hlt">release</span> properties of amorphous boron and boron-based propellant primary combustion products</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Liang, Daolun; Liu, Jianzhong; Xiao, Jinwu; Xi, Jianfei; Wang, Yang; Zhang, Yanwei; Zhou, Junhu</p> <p>2015-07-01</p> <p>The microstructure of amorphous boron and the primary combustion products of boron-based fuel-rich propellant (hereafter referred to as primary combustion products) was analyzed by scanning electron microscope. Composition analysis of the primary combustion products was carried out by X-ray diffraction and X-ray photoelectron spectroscopy. The <span class="hlt">energy</span> <span class="hlt">release</span> properties of amorphous boron and the primary combustion products were comparatively studied by laser ignition experimental system and thermogravimetry-differential scanning calorimetry. The primary combustion products contain B, C, Mg, Al, B4C, B13C2, BN, B2O3, NH4Cl, H2O, and so on. The <span class="hlt">energy</span> <span class="hlt">release</span> properties of primary combustion products are different from amorphous boron, significantly. The full-time spectral intensity of primary combustion products at a wavelength of 580 nm is ~2% lower than that of amorphous boron. The maximum spectral intensity of the former at full wave is ~5% higher than that of the latter. The ignition delay time of primary combustion products is ~150 ms shorter than that of amorphous boron, and the self-sustaining combustion time of the former is ~200 ms longer than that of the latter. The thermal oxidation process of amorphous boron involves water evaporation (weight loss) and boron oxidation (weight gain). The thermal oxidation process of primary combustion products involves two additional steps: NH4Cl decomposition (weight loss) and carbon oxidation (weight loss). CL-20 shows better combustion-supporting effect than KClO4 in both the laser ignition experiments and the thermal oxidation experiments.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2002SPIE.4562..593M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2002SPIE.4562..593M"><span>Low surface <span class="hlt">energy</span> polymeric <span class="hlt">release</span> coating for improved contact print lithography</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Mancini, David P.; Resnick, Douglas J.; Gehoski, Kathleen A.; Popovich, Laura L.; Chang, Daniel</p> <p>2002-03-01</p> <p>Contact printing has been used for decades in many various lithography applications in the microelectronic industry. While vacuum contact printing processes offer sub-micron resolution and high throughput, they often suffer from some important drawbacks. One of the most common problems is degradation in both resolution and defect density which occurs when the same mask si used for multiple exposures without frequent mask cleans. This is largely due to the relatively high surface <span class="hlt">energy</span> of both quartz and chrome and the tendency of most photoresists to adhere to these surfaces. As a result, when a mask and wafer are pressed into intimate contact, resist will tend to stick to the mask creating a defect on the wafer, effectively propagating defects to subsequent wafers. In this study, DuPont Teflon AF 1601S is used as a photomask coating and evaluated for its ability to act as a <span class="hlt">release</span> agent and reduce defects while maintaining resolution for multiple exposures. Teflon AF is an amorphous, transparent, low surface <span class="hlt">energy</span>, polymeric material that can be spin coated into a thin conformal film. Tests have shown that when using an uncoated mask in vacuum contact, resolution of 0.75 micrometers dense lines is severely degraded after less than 10 consecutive exposures. However, when the mask is coated, 0.75 micrometers dense lines were successfully resolved using vacuum contact for over 200 exposures without cleaning. In addition, it has been demonstrated that Teflon AF coatings impart to a mask a self-cleaning capability, since particles tend to stick to the photoresist rather than the mask. A coated mask, which was purposefully contaminated with particulates, resolved 0.75 micrometers dense lines on all but the first wafer of a series of 25 consecutive exposures. The patented mask <span class="hlt">releases</span> layer process has successfully been demonstrated with a positive novolak resist. Additional data which describes the system chemistry, dilution and coating process, and film morphology</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19900016760','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19900016760"><span>Strain <span class="hlt">energy</span> <span class="hlt">release</span> rate analysis of delamination in a tapered laminate subjected to tension load</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Salpekar, S. A.; Raju, I. S.; Obrien, T. K.</p> <p>1990-01-01</p> <p>A tapered composite laminate subjected to tension load was analyzed using the finite-element method. The glass/epoxy laminate has a (+ or - 45)sub 3 group of plies dropped in three distinct steps, each 20 ply-thicknesses apart, thus forming a taper angle of 5.71 degrees. Steep gradients of interlaminar normal and shear stress on a potential delamination interface suggest the existence of stress singularities at the points of material and geometric discontinuities created by the internal plydrops. The delamination was assumed to initiate at the thin end of the taper on a -45/+45 interface and the delamination growth was simulated in both directions, i.e., along the taper and into the thin region. The strain-<span class="hlt">energy-release</span> rate for a delamination growing into the thin laminate consisted predominantly of mode I (opening) component. For a delamination growing along the tapered region, the strain-<span class="hlt">energy-release</span> rate was initially all mode I, but the proportion of mode I decreased with increase in delamination size until eventually total G was all mode II. The total G for both delamination tips increased with increase in delamination size, indicating that a delamination initiating at the end of the taper will grow unstably along the taper and into the thin laminate simultaneously.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017BVol...79...84M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017BVol...79...84M"><span>Volatiles and <span class="hlt">energy</span> <span class="hlt">released</span> by Puracé volcano</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Maldonado, Luisa Fernanda Meza; Inguaggiato, Salvatore; Jaramillo, Marco Tulio; Valencia, Gustavo Garzón; Mazot, Agnes</p> <p>2017-12-01</p> <p>Total CO2 output of Puracé volcano (Colombia) was estimated on the basis of fluids discharged by fumaroles, soil gases, and dissolved carbon species in the aquifer. The soil CO2 emission was computed from a field survey of 512 points of CO2 soil flux measurements at the main degassing areas of Puracé volcano. The CO2 flux from Puracé's plume was estimated using an indirect method, that used the SO2 plume flux and CO2/SO2 ratio of the main high temperature fumarole. The total output of CO2 was estimated at ≅ 1500 t/day. The main contribution of CO2 comes from the plume (summit degassing) and from soil degassing that emit 673 and 812 t/day, respectively. The contributions of summit and soil degassing areas are comparable, indicating an intermediate degassing style partitioned between closed and open conduit systems. The estimated water vapor discharge (as derived from the chemical composition of the fumaroles, the H2O/CO2 ratio, and the SO2 plume flux) allowed calculation of the total thermal <span class="hlt">energy</span> (fumarolic, soil degassing, and aquifer) <span class="hlt">released</span> from the Puracé volcanic system. This was 360 MW.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_8");'>8</a></li> <li><a href="#" onclick='return showDiv("page_9");'>9</a></li> <li class="active"><span>10</span></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_10 --> <div id="page_11" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_9");'>9</a></li> <li><a href="#" onclick='return showDiv("page_10");'>10</a></li> <li class="active"><span>11</span></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="201"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1992PApGe.139..293T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1992PApGe.139..293T"><span>Time-lag of the earthquake <span class="hlt">energy</span> <span class="hlt">release</span> between three seismic regions</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Tsapanos, Theodoros M.; Liritzis, Ioannis</p> <p>1992-06-01</p> <p>Three complete data sets of strong earthquakes ( M≥5.5), which occurred in the seismic regions of Chile, Mexico and Kamchatka during the time period 1899 1985, have been used to test the existence of a time-lag in the seismic <span class="hlt">energy</span> <span class="hlt">release</span> between these regions. These data sets were cross-correlated in order to determine whether any pair of the sets are correlated. For this purpose statistical tests, such as the T-test, the Fisher's transformation and probability distribution have been applied to determine the significance of the obtained correlation coefficients. The results show that the time-lag between Chile and Kamchatka is -2, which means that Kamchatka precedes Chile by 2 years, with a correlation coefficient significant at 99.80% level, a weak correlation between Kamchatka-Mexico and noncorrelation for Mexico-Chile.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017ApJ...835..214P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017ApJ...835..214P"><span>Stochastic Fermi Energization of Coronal Plasma during Explosive Magnetic <span class="hlt">Energy</span> <span class="hlt">Release</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Pisokas, Theophilos; Vlahos, Loukas; Isliker, Heinz; Tsiolis, Vassilis; Anastasiadis, Anastasios</p> <p>2017-02-01</p> <p>The aim of this study is to analyze the interaction of charged particles (ions and electrons) with randomly formed particle scatterers (e.g., large-scale local “magnetic fluctuations” or “coherent magnetic irregularities”) using the setup proposed initially by Fermi. These scatterers are formed by the explosive magnetic <span class="hlt">energy</span> <span class="hlt">release</span> and propagate with the Alfvén speed along the irregular magnetic fields. They are large-scale local fluctuations (δB/B ≈ 1) randomly distributed inside the unstable magnetic topology and will here be called Alfvénic Scatterers (AS). We constructed a 3D grid on which a small fraction of randomly chosen grid points are acting as AS. In particular, we study how a large number of test particles evolves inside a collection of AS, analyzing the evolution of their <span class="hlt">energy</span> distribution and their escape-time distribution. We use a well-established method to estimate the transport coefficients directly from the trajectories of the particles. Using the estimated transport coefficients and solving the Fokker-Planck equation numerically, we can recover the <span class="hlt">energy</span> distribution of the particles. We have shown that the stochastic Fermi energization of mildly relativistic and relativistic plasma can heat and accelerate the tail of the ambient particle distribution as predicted by Parker & Tidman and Ramaty. The temperature of the hot plasma and the tail of the energetic particles depend on the mean free path (λsc) of the particles between the scatterers inside the energization volume.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29055333','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29055333"><span>Anisotropic kinetic <span class="hlt">energy</span> <span class="hlt">release</span> and gyroscopic behavior of CO2 super rotors from an optical centrifuge.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Murray, Matthew J; Ogden, Hannah M; Mullin, Amy S</p> <p>2017-10-21</p> <p>An optical centrifuge is used to generate an ensemble of CO 2 super rotors with oriented angular momentum. The collision dynamics and <span class="hlt">energy</span> transfer behavior of the super rotor molecules are investigated using high-resolution transient IR absorption spectroscopy. New multipass IR detection provides improved sensitivity to perform polarization-dependent transient studies for rotational states with 76 ≤ J ≤ 100. Polarization-dependent measurements show that the collision-induced kinetic <span class="hlt">energy</span> <span class="hlt">release</span> is spatially anisotropic and results from both near-resonant <span class="hlt">energy</span> transfer between super rotor molecules and non-resonant <span class="hlt">energy</span> transfer between super rotors and thermal molecules. J-dependent studies show that the extent and duration of the orientational anisotropy increase with rotational angular momentum. The super rotors exhibit behavior akin to molecular gyroscopes, wherein molecules with larger amounts of angular momentum are less likely to change their angular momentum orientation through collisions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JChPh.147o4309M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JChPh.147o4309M"><span>Anisotropic kinetic <span class="hlt">energy</span> <span class="hlt">release</span> and gyroscopic behavior of CO2 super rotors from an optical centrifuge</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Murray, Matthew J.; Ogden, Hannah M.; Mullin, Amy S.</p> <p>2017-10-01</p> <p>An optical centrifuge is used to generate an ensemble of CO2 super rotors with oriented angular momentum. The collision dynamics and <span class="hlt">energy</span> transfer behavior of the super rotor molecules are investigated using high-resolution transient IR absorption spectroscopy. New multipass IR detection provides improved sensitivity to perform polarization-dependent transient studies for rotational states with 76 ≤ J ≤ 100. Polarization-dependent measurements show that the collision-induced kinetic <span class="hlt">energy</span> <span class="hlt">release</span> is spatially anisotropic and results from both near-resonant <span class="hlt">energy</span> transfer between super rotor molecules and non-resonant <span class="hlt">energy</span> transfer between super rotors and thermal molecules. J-dependent studies show that the extent and duration of the orientational anisotropy increase with rotational angular momentum. The super rotors exhibit behavior akin to molecular gyroscopes, wherein molecules with larger amounts of angular momentum are less likely to change their angular momentum orientation through collisions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.fs.usda.gov/treesearch/pubs/14162','TREESEARCH'); return false;" href="https://www.fs.usda.gov/treesearch/pubs/14162"><span>Impact of <span class="hlt">Released</span> Fual Moisture on Atmospheric Dynamics</span></a></p> <p><a target="_blank" href="http://www.fs.usda.gov/treesearch/">Treesearch</a></p> <p>Brian E. Potter</p> <p>2003-01-01</p> <p>A common component of fire incident reports and prescribed burn preparations is an estimate of the <span class="hlt">energy</span> that was or will be <span class="hlt">released</span> by the fire. Typically, this is based on the <span class="hlt">energy</span> <span class="hlt">released</span> by combustion of the fuel load, reduced to account for the <span class="hlt">energy</span> that is required to evaporate moisture in the fuel materials. (e.g., Byram 1959, Anderson 1968, Simard et al...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/ADA595424','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA595424"><span>United States Air Force F-35A Operational Basing Environmental Impact Statement. Appendix E: Responses</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>2013-09-01</p> <p>R0287, R0549, R0662, R0740 Concerned that the <span class="hlt">afterburner</span> was not factored into the noise zone equation. <span class="hlt">Afterburner</span> takeoffs were factored into...the noise assessment. The F-35s at Burlington International Airport are proposed to use <span class="hlt">afterburners</span> on only 5 percent of their takeoffs (vice the...90 percent done now by F-16s). However, the <span class="hlt">afterburner</span> would be turned off shortly after the aircraft becomes airborne, much prior to crossing the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1992MTA....23.2339A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1992MTA....23.2339A"><span>Theoretical models for the combustion of alloyable materials</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Armstrong, Robert</p> <p>1992-09-01</p> <p>The purpose of this work is to extend a theoretical model of layered (laminar) media for SHS combustion presented in an earlier article [1] to explore possible mechanisms for <span class="hlt">after-burning</span> in SHS ( i.e., gasless) combustion. As before, our particular interest is how the microscopic geometry of the solid reactants is reflected in the combustion wave and in the reaction product. The model is constructed from alternating lamina of two pure reactants that interdiffuse exothermically to form a product. Here, the laminar model is extended to contain layers of differing thicknesses. Using asymptotic theory, it was found that under certain conditions, the combustion wave can become “detached,” and an initial thin flame propagates through the media, leaving a slower, thicker flame following behind ( i.e., <span class="hlt">afterburning</span>). Thin laminae are consumed in the initial flame and are thick in the secondary. The thin flame has a width determined by the inverse of the activation <span class="hlt">energy</span> of diffusion, as found previously. The width of the <span class="hlt">afterburning</span> zone, however, is determined by the absolute time of diffusion for the thicker laminae. Naturally, when the laminae are all the same thickness, there is only one thin flame. The condition for the appearance of <span class="hlt">afterburning</span> is found to be contingent on the square of the ratio of smallestto-largest thicknesses being considerably less than unity.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JPhCS.908a2018K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JPhCS.908a2018K"><span>Influence of ceramic dental crown coating substrate thickness ratio on strain <span class="hlt">energy</span> <span class="hlt">release</span> rate</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Khasnulhadi, K.; Daud, R.; Mat, F.; Noor, S. N. F. M.; Basaruddin, K. S.; Sulaiman, M. H.</p> <p>2017-10-01</p> <p>This paper presents the analysis of coating substrate thickness ratio effect on the crown coating fracture behaviour. The bi-layer material is examined under four point bending with pre-crack at the bottom of the core material by using finite element. Three different coating thickness of core/substrate was tested which is 1:1, 1:2 and 2:1. The fracture parameters are analysed based on bilayer and homogenous elastic interaction. The result shows that the ratio thickness of core/veneer provided a significant effect on <span class="hlt">energy</span> <span class="hlt">release</span> rate.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/2907251','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/2907251"><span>[The post-burn process--a determinant in local surgical treatment of deep burns].</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Bäumer, F; Henrich, H A</p> <p>1988-12-01</p> <p><span class="hlt">Afterburning</span> has been studied in the animal experiment by use of intravital dye indicators and by measuring partial oxygen pressure. After third degree burn the oxygen conduction of the damaged skin increased. The <span class="hlt">afterburning</span> was seen to be finished on the 5th day after the burn trauma. The histological changes in the depth of the <span class="hlt">afterburn</span> area reaches to the subcutis. The extend of the <span class="hlt">afterburn</span> area was not related to the applied temperature or the duration of the experimental burn injury.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EPJD...70..130R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EPJD...70..130R"><span>Kinetic-<span class="hlt">energy</span> <span class="hlt">release</span> distributions of fragment anions from collisions of potassium atoms with D-Ribose and tetrahydrofuran*</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Rebelo, André; Cunha, Tiago; Mendes, Mónica; da Silva, Filipe Ferreira; García, Gustavo; Limão-Vieira, Paulo</p> <p>2016-06-01</p> <p>Kinetic-<span class="hlt">energy</span> <span class="hlt">release</span> distributions have been obtained from the width and shapes of the time-of-flight (TOF) negative ion mass peaks formed in collisions of fast potassium atoms with D-Ribose (DR) and tetrahydrofuran (THF) molecules. Recent dissociative ion-pair formation experiments yielding anion formation have shown that the dominant fragment from D-Ribose is OH- [D. Almeida, F. Ferreira da Silva, G. García, P. Limão-Vieira, J. Chem. Phys. 139, 114304 (2013)] whereas in the case of THF is O- [D. Almeida, F. Ferreira da Silva, S. Eden, G. García, P. Limão-Vieira, J. Phys. Chem. A 118, 690 (2014)]. The results for DR and THF show an <span class="hlt">energy</span> distribution profile reminiscent of statistical degradation via vibrational excitation and partly due to direct transformation of the excess <span class="hlt">energy</span> in translational <span class="hlt">energy</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20120008792&hterms=ply&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3D.ply','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20120008792&hterms=ply&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3D.ply"><span>Adhesive-Bonded Composite Joint Analysis with Delaminated Surface Ply Using Strain-<span class="hlt">Energy</span> <span class="hlt">Release</span> Rate</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Chadegani, Alireza; Yang, Chihdar; Smeltzer, Stanley S. III</p> <p>2012-01-01</p> <p>This paper presents an analytical model to determine the strain <span class="hlt">energy</span> <span class="hlt">release</span> rate due to an interlaminar crack of the surface ply in adhesively bonded composite joints subjected to axial tension. Single-lap shear-joint standard test specimen geometry with thick bondline is followed for model development. The field equations are formulated by using the first-order shear-deformation theory in laminated plates together with kinematics relations and force equilibrium conditions. The stress distributions for the adherends and adhesive are determined after the appropriate boundary and loading conditions are applied and the equations for the field displacements are solved. The system of second-order differential equations is solved to using the symbolic computation tool Maple 9.52 to provide displacements fields. The equivalent forces at the tip of the prescribed interlaminar crack are obtained based on interlaminar stress distributions. The strain <span class="hlt">energy</span> <span class="hlt">release</span> rate of the crack is then determined by using the crack closure method. Finite element analyses using the J integral as well as the crack closure method are performed to verify the developed analytical model. It has been shown that the results using the analytical method correlate well with the results from the finite element analyses. An attempt is made to predict the failure loads of the joints based on limited test data from the literature. The effectiveness of the inclusion of bondline thickness is justified when compared with the results obtained from the previous model in which a thin bondline and uniform adhesive stresses through the bondline thickness are assumed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2000JGR...10519111R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2000JGR...10519111R"><span>Surface displacements and <span class="hlt">energy</span> <span class="hlt">release</span> rates for constant stress drop slip zones in joined elastic quarter spaces</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Rodgers, Michael J.; Wen, Shengmin; Keer, Leon M.</p> <p>2000-08-01</p> <p>A three-dimensional quasi-static model of faulting in an elastic half-space with a horizontal change of material properties (i.e., joined elastic quarter spaces) is considered. A boundary element method is used with a stress drop slip zone approach so that the fault surface relative displacements as well as the free surface displacements are approximated in elements over their respective domains. Stress intensity factors and free surface displacements are calculated for a variety of cases to show the phenomenological behavior of faulting in such a medium. These calculations showed that the behavior could be distinguished from a uniform half-space. Slip in a stiffer material increases, while slip in a softer material decreases the <span class="hlt">energy</span> <span class="hlt">release</span> rate and the free surface displacements. Also, the 1989 Kalapana earthquake was located on the basis of a series of forward searches using this method and leveling data. The located depth is 8 km, which is the closer to the seismically inferred depth than that determined from other models. Finally, the <span class="hlt">energy</span> <span class="hlt">release</span> rate, which can be used as a fracture criterion for fracture at this depth, is calculated to be 11.1×106 J m-2.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19870004360','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19870004360"><span>Q3DG: A computer program for strain-<span class="hlt">energy-release</span> rates for delamination growth in composite laminates</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Raju, I. S.</p> <p>1986-01-01</p> <p>The Q3DG is a computer program developed to perform a quasi-three-dimensional stress analysis for composite laminates which may contain delaminations. The laminates may be subjected to mechanical, thermal, and hygroscopic loads. The program uses the finite element method and models the laminates with eight-noded parabolic isoparametric elements. The program computes the strain-<span class="hlt">energy-release</span> components and the total strain-<span class="hlt">energy</span> <span class="hlt">release</span> in all three modes for delamination growth. A rectangular mesh and data file generator, DATGEN, is included. The DATGEN program can be executed interactively and is user friendly. The documentation includes sections dealing with the Q3D analysis theory, derivation of element stiffness matrices and consistent load vectors for the parabolic element. Several sample problems with the input for Q3DG and output from the program are included. The capabilities of the DATGEN program are illustrated with examples of interactive sessions. A microfiche of all the examples is included. The Q3DG and DATGEN programs have been implemented on CYBER 170 class computers. Q3DG and DATGEN were developed at the Langley Research Center during the early eighties and documented in 1984 to 1985.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28773009','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28773009"><span>Understanding Drug <span class="hlt">Release</span> Data through Thermodynamic Analysis.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Freire, Marjorie Caroline Liberato Cavalcanti; Alexandrino, Francisco; Marcelino, Henrique Rodrigues; Picciani, Paulo Henrique de Souza; Silva, Kattya Gyselle de Holanda E; Genre, Julieta; Oliveira, Anselmo Gomes de; Egito, Eryvaldo Sócrates Tabosa do</p> <p>2017-06-13</p> <p>Understanding the factors that can modify the drug <span class="hlt">release</span> profile of a drug from a Drug-Delivery-System (DDS) is a mandatory step to determine the effectiveness of new therapies. The aim of this study was to assess the Amphotericin-B (AmB) kinetic <span class="hlt">release</span> profiles from polymeric systems with different compositions and geometries and to correlate these profiles with the thermodynamic parameters through mathematical modeling. Film casting and electrospinning techniques were used to compare behavior of films and fibers, respectively. <span class="hlt">Release</span> profiles from the DDSs were performed, and the mathematical modeling of the data was carried out. Activation <span class="hlt">energy</span>, enthalpy, entropy and Gibbs free <span class="hlt">energy</span> of the drug <span class="hlt">release</span> process were determined. AmB <span class="hlt">release</span> profiles showed that the relationship to overcome the enthalpic barrier was PVA-fiber > PVA-film > PLA-fiber > PLA-film. Drug <span class="hlt">release</span> kinetics from the fibers and the films were better fitted on the Peppas-Sahlin and Higuchi models, respectively. The thermodynamic parameters corroborate these findings, revealing that the AmB <span class="hlt">release</span> from the evaluated systems was an endothermic and non-spontaneous process. Thermodynamic parameters can be used to explain the drug kinetic <span class="hlt">release</span> profiles. Such an approach is of utmost importance for DDS containing insoluble compounds, such as AmB, which is associated with an erratic bioavailability.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5554032','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5554032"><span>Understanding Drug <span class="hlt">Release</span> Data through Thermodynamic Analysis</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Freire, Marjorie Caroline Liberato Cavalcanti; Alexandrino, Francisco; Marcelino, Henrique Rodrigues; Picciani, Paulo Henrique de Souza; Silva, Kattya Gyselle de Holanda e; Genre, Julieta; de Oliveira, Anselmo Gomes; do Egito, Eryvaldo Sócrates Tabosa</p> <p>2017-01-01</p> <p>Understanding the factors that can modify the drug <span class="hlt">release</span> profile of a drug from a Drug-Delivery-System (DDS) is a mandatory step to determine the effectiveness of new therapies. The aim of this study was to assess the Amphotericin-B (AmB) kinetic <span class="hlt">release</span> profiles from polymeric systems with different compositions and geometries and to correlate these profiles with the thermodynamic parameters through mathematical modeling. Film casting and electrospinning techniques were used to compare behavior of films and fibers, respectively. <span class="hlt">Release</span> profiles from the DDSs were performed, and the mathematical modeling of the data was carried out. Activation <span class="hlt">energy</span>, enthalpy, entropy and Gibbs free <span class="hlt">energy</span> of the drug <span class="hlt">release</span> process were determined. AmB <span class="hlt">release</span> profiles showed that the relationship to overcome the enthalpic barrier was PVA-fiber > PVA-film > PLA-fiber > PLA-film. Drug <span class="hlt">release</span> kinetics from the fibers and the films were better fitted on the Peppas–Sahlin and Higuchi models, respectively. The thermodynamic parameters corroborate these findings, revealing that the AmB <span class="hlt">release</span> from the evaluated systems was an endothermic and non-spontaneous process. Thermodynamic parameters can be used to explain the drug kinetic <span class="hlt">release</span> profiles. Such an approach is of utmost importance for DDS containing insoluble compounds, such as AmB, which is associated with an erratic bioavailability. PMID:28773009</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018PASJ..tmp....6S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018PASJ..tmp....6S"><span>Observational study on the fine structure and dynamics of a solar jet. II. <span class="hlt">Energy</span> <span class="hlt">release</span> process revealed by spectral analysis</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sakaue, Takahito; Tei, Akiko; Asai, Ayumi; Ueno, Satoru; Ichimoto, Kiyoshi; Shibata, Kazunari</p> <p>2018-01-01</p> <p>We report on a solar jet phenomenon associated with the C5.4 class flare on 2014 November 11. The data of the jet was provided by the Solar Dynamics Observatory, the X-Ray Telescope (XRT) aboard Hinode, and the Interface Region Imaging Spectrograph and Domeless Solar Telescope (DST) at Hida Observatory, Kyoto University. These plentiful data enabled us to present this series of papers to discuss all the processes of the observed phenomena, including <span class="hlt">energy</span> storage, event trigger, and <span class="hlt">energy</span> <span class="hlt">release</span>. In this paper, we focus on the <span class="hlt">energy</span> <span class="hlt">release</span> process of the observed jet, and mainly describe our spectral analysis on the Hα data of DST to investigate the internal structure of the Hα jet and its temporal evolution. This analysis reveals that in the physical quantity distributions of the Hα jet, such as line-of-sight velocity and optical thickness, there is a significant gradient in the direction crossing the jet. We interpret this internal structure as the consequence of the migration of the <span class="hlt">energy</span> <span class="hlt">release</span> site, based on the idea of ubiquitous reconnection. Moreover, by measuring the horizontal flow of the fine structures in the jet, we succeeded in deriving the three-dimensional velocity field and the line-of-sight acceleration field of the Hα jet. The analysis result indicates that part of the ejecta in the Hα jet experienced additional acceleration after it had been ejected from the lower atmosphere. This secondary acceleration was found to occur in the vicinity of the intersection between the trajectories of the Hα jet and the X-ray jet observed by Hinode/XRT. We propose that a fundamental cause of this phenomenon is magnetic reconnection involving the plasmoid in the observed jet.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/25433200','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25433200"><span>Relationships between surface free <span class="hlt">energy</span>, surface texture parameters and controlled drug <span class="hlt">release</span> in hydrophilic matrices.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Saurí, J; Suñé-Negre, J M; Díaz-Marcos, J; Vilana, J; Millán, D; Ticó, J R; Miñarro, M; Pérez-Lozano, P; García-Montoya, E</p> <p>2015-01-15</p> <p>The study of controlled <span class="hlt">release</span> and drug <span class="hlt">release</span> devices has been dominated by considerations of the bulk or average properties of material or devices. Yet the outermost surface atoms play a central role in their performance. The objective of this article has been to characterize the surface of hydrophilic matrix tablets using the contact angle (CA) method to ascertain the surface free <span class="hlt">energy</span>, and atomic force microscopy (AFM) and confocal microscopy (CM) for the physical characterization of the surface of the hydrophilic matrix. The surface free <span class="hlt">energy</span> results obtained show that hydroxypropylmethylcellulose K15M hinders the spreading of water on the surface of the tablet, such that the concentration of HPMC K15M increases the reaction rate of the hydrophobic interactions between the chains of HPMC K15M which increases with respect to the rate of penetration of water into the tablet. In this study, we developed a new method to characterize the swelling of the tablets and established a relationship between the new method based on microswelling and the swelling ratio parameter. The surface texture parameters have been determined and the morphology of the tablets of the different formulations and the evolution of the surface morphology after interacting with the water, swelling and forming a gel layer were characterized. This work represents significant progress in the characterization of matrix tablets. Copyright © 2014 Elsevier B.V. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/16965044','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/16965044"><span>High translational <span class="hlt">energy</span> <span class="hlt">release</span> in H2 (D2) associative desorption from H (D) chemisorbed on C(0001).</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Baouche, S; Gamborg, G; Petrunin, V V; Luntz, A C; Baurichter, A; Hornekaer, L</p> <p>2006-08-28</p> <p>Highly energetic translational <span class="hlt">energy</span> distributions are reported for hydrogen and deuterium molecules desorbing associatively from the atomic chemisorption states on highly oriented pyrolytic graphite (HOPG). Laser assisted associative desorption is used to measure the time of flight of molecules desorbing from a hydrogen (deuterium) saturated HOPG surface produced by atomic exposure from a thermal atom source at around 2100 K. The translational <span class="hlt">energy</span> distributions normal to the surface are very broad, from approximately 0.5 to approximately 3 eV, with a peak at approximately 1.3 eV. The highest translational <span class="hlt">energy</span> measured is close to the theoretically predicted barrier height. The angular distribution of the desorbing molecules is sharply peaked along the surface normal and is consistent with thermal broadening contributing to <span class="hlt">energy</span> <span class="hlt">release</span> parallel to the surface. All results are in qualitative agreement with recent density functional theory calculations suggesting a lowest <span class="hlt">energy</span> para-type dimer recombination path.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JAP...122b4104X','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JAP...122b4104X"><span>Effect of temperature-driven phase transition on <span class="hlt">energy</span>-storage and -<span class="hlt">release</span> properties of Pb0.97La0.02[Zr0.55Sn0.30Ti0.15]O3 ceramics</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Xu, Ran; Tian, Jingjing; Zhu, Qingshan; Feng, Yujun; Wei, Xiaoyong; Xu, Zhuo</p> <p>2017-07-01</p> <p>Temperature-driven phase transition of Pb0.97La0.02[Zr0.55Sn0.30Ti0.15]O3 ceramics was studied, and the consecutive ferroelectric-antiferroelectric-paraelectric (FE-AFE-PE) switching was confirmed. The materials have better dielectric tunability (-82% to 50%) in the AFE state than in the FE state. Also, the phase transition influences the <span class="hlt">energy</span>-storage and -<span class="hlt">release</span> performance significantly. A sharp increase in <span class="hlt">releasable</span> <span class="hlt">energy</span> density and efficiency was observed due to the temperature-driven FE-AFE transition. Highest <span class="hlt">releasable</span> <span class="hlt">energy</span> density, current density, and peak power density were achieved at 130 °C, which was attributed to the highest backward transition field. The stored charge was <span class="hlt">released</span> completely in AFE and PE states in the microseconds scale, while only a small part of it was <span class="hlt">released</span> in the FE state. The above results indicate the huge impact of temperature-driven phase transition on dielectrics' performance, which is significant when developing AFE materials working in a wide temperature range.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/ADA244082','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA244082"><span>Engineering and Development Support of General Decon Technology for the DARCOM Installation Restoration Program. Task 2. Treatment of Explosives Contaminated Lagoon Sediment. Phase I. Literature Review and Evaluation</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>1980-11-01</p> <p>hr incineration rate are presented in Table 15. These costs include dredging equipment, flat bed trailer and <span class="hlt">afterburners</span> and venturi scrubbers where...require further treatment before they can be <span class="hlt">released</span> into the environment, i.e. biological degradation for the liquid and specific scrubbers for the...The wet-air units are equipped with wet scrubbers to remove air emissions. Air emissions are expected to contain at a minimum CO, C0 2 ,N2 , 0, and</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_9");'>9</a></li> <li><a href="#" onclick='return showDiv("page_10");'>10</a></li> <li class="active"><span>11</span></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_11 --> <div id="page_12" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_10");'>10</a></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li class="active"><span>12</span></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="221"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018EPJWC.16900024T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018EPJWC.16900024T"><span>Fission fragment yields and total kinetic <span class="hlt">energy</span> <span class="hlt">release</span> in neutron-induced fission of235,238U,and239Pu</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Tovesson, F.; Duke, D.; Geppert-Kleinrath, V.; Manning, B.; Mayorov, D.; Mosby, S.; Schmitt, K.</p> <p>2018-03-01</p> <p>Different aspects of the nuclear fission process have been studied at Los Alamos Neutron Science Center (LANSCE) using various instruments and experimental techniques. Properties of the fragments emitted in fission have been investigated using Frisch-grid ionization chambers, a Time Projection Chamber (TPC), and the SPIDER instrument which employs the 2v-2E method. These instruments and experimental techniques have been used to determine fission product mass yields, the <span class="hlt">energy</span> dependent total kinetic <span class="hlt">energy</span> (TKE) <span class="hlt">release</span>, and anisotropy in neutron-induced fission of U-235, U-238 and Pu-239.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/CFR-2011-title10-vol1/pdf/CFR-2011-title10-vol1-sec20-2003.pdf','CFR2011'); return false;" href="https://www.gpo.gov/fdsys/pkg/CFR-2011-title10-vol1/pdf/CFR-2011-title10-vol1-sec20-2003.pdf"><span>10 CFR 20.2003 - Disposal by <span class="hlt">release</span> into sanitary sewerage.</span></a></p> <p><a target="_blank" href="http://www.gpo.gov/fdsys/browse/collectionCfr.action?selectedYearFrom=2011&page.go=Go">Code of Federal Regulations, 2011 CFR</a></p> <p></p> <p>2011-01-01</p> <p>... 10 <span class="hlt">Energy</span> 1 2011-01-01 2011-01-01 false Disposal by <span class="hlt">release</span> into sanitary sewerage. 20.2003 Section 20.2003 <span class="hlt">Energy</span> NUCLEAR REGULATORY COMMISSION STANDARDS FOR PROTECTION AGAINST RADIATION Waste Disposal § 20.2003 Disposal by <span class="hlt">release</span> into sanitary sewerage. (a) A licensee may discharge licensed...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/CFR-2013-title10-vol1/pdf/CFR-2013-title10-vol1-sec20-2003.pdf','CFR2013'); return false;" href="https://www.gpo.gov/fdsys/pkg/CFR-2013-title10-vol1/pdf/CFR-2013-title10-vol1-sec20-2003.pdf"><span>10 CFR 20.2003 - Disposal by <span class="hlt">release</span> into sanitary sewerage.</span></a></p> <p><a target="_blank" href="http://www.gpo.gov/fdsys/browse/collectionCfr.action?selectedYearFrom=2013&page.go=Go">Code of Federal Regulations, 2013 CFR</a></p> <p></p> <p>2013-01-01</p> <p>... 10 <span class="hlt">Energy</span> 1 2013-01-01 2013-01-01 false Disposal by <span class="hlt">release</span> into sanitary sewerage. 20.2003 Section 20.2003 <span class="hlt">Energy</span> NUCLEAR REGULATORY COMMISSION STANDARDS FOR PROTECTION AGAINST RADIATION Waste Disposal § 20.2003 Disposal by <span class="hlt">release</span> into sanitary sewerage. (a) A licensee may discharge licensed...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/CFR-2010-title10-vol1/pdf/CFR-2010-title10-vol1-sec20-2003.pdf','CFR'); return false;" href="https://www.gpo.gov/fdsys/pkg/CFR-2010-title10-vol1/pdf/CFR-2010-title10-vol1-sec20-2003.pdf"><span>10 CFR 20.2003 - Disposal by <span class="hlt">release</span> into sanitary sewerage.</span></a></p> <p><a target="_blank" href="http://www.gpo.gov/fdsys/browse/collectionCfr.action?selectedYearFrom=2010&page.go=Go">Code of Federal Regulations, 2010 CFR</a></p> <p></p> <p>2010-01-01</p> <p>... 10 <span class="hlt">Energy</span> 1 2010-01-01 2010-01-01 false Disposal by <span class="hlt">release</span> into sanitary sewerage. 20.2003 Section 20.2003 <span class="hlt">Energy</span> NUCLEAR REGULATORY COMMISSION STANDARDS FOR PROTECTION AGAINST RADIATION Waste Disposal § 20.2003 Disposal by <span class="hlt">release</span> into sanitary sewerage. (a) A licensee may discharge licensed...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/CFR-2014-title10-vol1/pdf/CFR-2014-title10-vol1-sec20-2003.pdf','CFR2014'); return false;" href="https://www.gpo.gov/fdsys/pkg/CFR-2014-title10-vol1/pdf/CFR-2014-title10-vol1-sec20-2003.pdf"><span>10 CFR 20.2003 - Disposal by <span class="hlt">release</span> into sanitary sewerage.</span></a></p> <p><a target="_blank" href="http://www.gpo.gov/fdsys/browse/collectionCfr.action?selectedYearFrom=2014&page.go=Go">Code of Federal Regulations, 2014 CFR</a></p> <p></p> <p>2014-01-01</p> <p>... 10 <span class="hlt">Energy</span> 1 2014-01-01 2014-01-01 false Disposal by <span class="hlt">release</span> into sanitary sewerage. 20.2003 Section 20.2003 <span class="hlt">Energy</span> NUCLEAR REGULATORY COMMISSION STANDARDS FOR PROTECTION AGAINST RADIATION Waste Disposal § 20.2003 Disposal by <span class="hlt">release</span> into sanitary sewerage. (a) A licensee may discharge licensed...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/CFR-2012-title10-vol1/pdf/CFR-2012-title10-vol1-sec20-2003.pdf','CFR2012'); return false;" href="https://www.gpo.gov/fdsys/pkg/CFR-2012-title10-vol1/pdf/CFR-2012-title10-vol1-sec20-2003.pdf"><span>10 CFR 20.2003 - Disposal by <span class="hlt">release</span> into sanitary sewerage.</span></a></p> <p><a target="_blank" href="http://www.gpo.gov/fdsys/browse/collectionCfr.action?selectedYearFrom=2012&page.go=Go">Code of Federal Regulations, 2012 CFR</a></p> <p></p> <p>2012-01-01</p> <p>... 10 <span class="hlt">Energy</span> 1 2012-01-01 2012-01-01 false Disposal by <span class="hlt">release</span> into sanitary sewerage. 20.2003 Section 20.2003 <span class="hlt">Energy</span> NUCLEAR REGULATORY COMMISSION STANDARDS FOR PROTECTION AGAINST RADIATION Waste Disposal § 20.2003 Disposal by <span class="hlt">release</span> into sanitary sewerage. (a) A licensee may discharge licensed...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AGUFMSH21A2064G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFMSH21A2064G"><span>Intermittent Flare <span class="hlt">Energy</span> <span class="hlt">Release</span>: A Signature of Contracting Magnetic Islands from Reconnection?</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Guidoni, S. E.; Karpen, J. T.; DeVore, C.</p> <p>2013-12-01</p> <p>Many flares show short-lived enhancements of emission that protrude above their smooth underlying emission. These spikes have been observed over a vast <span class="hlt">energy</span> spectrum, from radio to hard x-rays. In hard X-rays, for example, their duration ranges from 0.2 to 2 s, with the majority occurring during the flare impulsive phase (Cheng 2012). In most cases, this intermittent <span class="hlt">energy</span> <span class="hlt">release</span> is situated at the footpoints of flare arcades where ionized particles, previously accelerated to high <span class="hlt">energies</span> at coronal heights, are decelerated by the dense solar surface. It is not yet understood what mechanisms accelerate ionized particles to the <span class="hlt">energies</span> required to produce the observed emission spikes. Drake et al. (2006) proposed a kinetic mechanism for accelerating electrons from contracting magnetic islands that form as reconnection proceeds, analogous to the <span class="hlt">energy</span> gain of a ball bouncing between converging walls. They estimated that multi-island regions of macroscopic dimensions might account for the required acceleration rates in flares, but at this time it is impractical to simulate large-scale systems in kinetic models. On the other hand, our recent high-resolution MHD simulations of a breakout eruptive flare (Karpen et al. 2012) allow us to resolve in detail the generation and evolution of macroscopic magnetic islands in a flare current sheet. Incorporating a rigorous kinetic model into our global simulations is not feasible at present. However, we intend to breach the gap between kinetic and fluid models by characterizing the contractions of islands as they move away from the main reconnection site, to determine their plausibility as candidates for the observed bursts of radiation. With our null-tracking capabilities, we follow the creation and evolution of the X- and O-type (island) nulls that result from spatially and temporally localized reconnection. Different regimes of current-sheet reconnection (slow/fast), island sizes, rates of island coalescence, and rates</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26512339','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26512339"><span>Effects of High-Intensity Training on Anaerobic and Aerobic Contributions to Total <span class="hlt">Energy</span> <span class="hlt">Release</span> During Repeated Supramaximal Exercise in Obese Adults.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Jabbour, Georges; Iancu, Horia-Daniel; Paulin, Anne</p> <p></p> <p>Studying relative anaerobic and aerobic metabolism contributions to total <span class="hlt">energy</span> <span class="hlt">release</span> during exercise may be valuable in understanding exercise energetic demands and the energetic adaptations that occur in response to acute or chronic exercise in obese adults. The aim of the present study is to evaluate the effects of 6 weeks of high-intensity training (HIT) on relative anaerobic and aerobic contributions to total <span class="hlt">energy</span> <span class="hlt">release</span> and on peak power output during repeated supramaximal cycling exercises (SCE) in obese adults. Twenty-four obese adults (body mass index = ± 33 kg.m -2 ) were randomized into a control group ( n  = 12) and an HIT group ( n  = 12). Accumulated oxygen deficits (ml.min -1 ) and anaerobic and aerobic contributions (%) were measured in all groups before and after training via repeated SCE. In addition, the peak power output performed during SCE was determined using the force-velocity test. Before HIT, anaerobic contributions to repeated SCE did not differ between the groups and decreased significantly during the third and fourth repetitions. After HIT, anaerobic contributions increased significantly in the HIT group (+11 %, p  < 0.01) and were significantly higher than those of the control group ( p  < 0.01). Moreover, the peak power obtained during SCE increased significantly in the HIT group (+110 W.kg -1 , p  < 0.01) and correlated positively with increases in anaerobic contributions ( r  = 0.9, p  < 0.01). In obese adults, HIT increased anaerobic contributions to <span class="hlt">energy</span> <span class="hlt">release</span> which were associated with peak power enhancement in response to repeated SCE. Consequently, HIT may be an appropriate approach for improving <span class="hlt">energy</span> contributions and muscle power among obese adults.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.eia.gov/outlooks/archive/aeo10/demand.html','EIAPUBS'); return false;" href="https://www.eia.gov/outlooks/archive/aeo10/demand.html"><span><span class="hlt">Energy</span> Demand (<span class="hlt">released</span> in AEO2010)</span></a></p> <p><a target="_blank" href="http://www.eia.doe.gov/reports/">EIA Publications</a></p> <p></p> <p>2010-01-01</p> <p>Growth in U.S. <span class="hlt">energy</span> use is linked to population growth through increases in demand for housing, commercial floorspace, transportation, manufacturing, and services. This affects not only the level of <span class="hlt">energy</span> use, but also the mix of fuels and consumption by sector.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014APS..MARS26013H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014APS..MARS26013H"><span>Effect of slow <span class="hlt">energy</span> <span class="hlt">releasing</span> on divergent detonation of Insensitive High Explosives</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hu, Xiaomian; Pan, Hao; Huang, Yong; Wu, Zihui</p> <p>2014-03-01</p> <p>There exists a slow <span class="hlt">energy</span> <span class="hlt">releasing</span> (SER) process in the slow reaction zone located behind the detonation wave due to the carbon cluster in the detonation products of Insensitive High Explosives (IHEs), and the process will affect the divergent detonation wave's propagation and the driving process of the explosives. To study the potential effect, a new artificial burn model including the SER process based on the programmed burn model is proposed in the paper. Quasi-steady analysis of the new model indicates that the nonlinearity of the detonation speed as a function of front curvature owes to the significant change of the reaction rate and the reaction zone length at the sonic state. What's more, in simulating the detonation of IHE JB-9014, the new model including the slow reaction can predict a slower jump-off velocity, in good agreement with the result of the test.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/5450442-radioactive-materials-released-from-nuclear-power-plants','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/5450442-radioactive-materials-released-from-nuclear-power-plants"><span>Radioactive materials <span class="hlt">released</span> from nuclear power plants</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Tichler, J.; Benkovitz, C.</p> <p></p> <p><span class="hlt">Releases</span> of radioactive materials in airborne and liquid effluents from commercial light water reactors during 1979 have been compiled and reported. Data on solid waste shipments as well as selected operating information have been included. This report supplements earlier annual reports issued by the former Atomic <span class="hlt">Energy</span> Commission and the Nuclear Regulatory Commission. The 1979 <span class="hlt">release</span> data are compared with previous year's <span class="hlt">releases</span> in tabular form. Data covering specific radionuclides are summarized.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27455513','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27455513"><span>Effects of levomilnacipran extended-<span class="hlt">release</span> on motivation/<span class="hlt">energy</span> and functioning in adults with major depressive disorder.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Thase, Michael E; Gommoll, Carl; Chen, Changzheng; Kramer, Kenneth; Sambunaris, Angelo</p> <p>2016-11-01</p> <p>The objective of this post-hoc analysis was to investigate the relationship between motivation/<span class="hlt">energy</span> and functional impairment in patients with major depressive disorder (MDD). Data were taken from a phase 3 trial of levomilnacipran extended-<span class="hlt">release</span> (ER) in adults with MDD (NCT01034462; N=429) that used the 18-item Motivation and <span class="hlt">Energy</span> Inventory (MEI) to assess motivation/<span class="hlt">energy</span>. Two subgroups with lower and higher motivation/<span class="hlt">energy</span> were defined using baseline MEI total scores (≤28 and >28, respectively). Change from baseline in the Sheehan Disability Scale (SDS) total score was analyzed in the intent-to-treat (ITT) population and both subgroups. Path analyses were carried out in the ITT population and a lower MEI subgroup to assess the direct and indirect effects of levomilnacipran ER on SDS total score change. In the ITT population and the lower MEI subgroup, significant differences were found between levomilnacipran ER and placebo for changes in the SDS total score (-2.6 and -3.9, both P<0.01), but not in the higher MEI subgroup. The indirect effect of levomilnacipran ER on SDS total score improvement, as mediated by MEI total score change, was 79.9% in the lower MEI subgroup and 67.2% in the ITT population. Levomilnacipran ER was previously shown to improve motivation/<span class="hlt">energy</span> in adults with MDD. The current analysis indicates that improvements in functional impairment were considerably mediated by improvements in motivation/<span class="hlt">energy</span>, particularly in patients with lower motivation/<span class="hlt">energy</span> at baseline.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19830009328','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19830009328"><span>Strain <span class="hlt">energy</span> <span class="hlt">release</span> rate analysis of cyclic delamination growth in compressively loaded laminates</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Whitcomb, J. D.</p> <p>1983-01-01</p> <p>Delamination growth in compressively loaded composite laminates was studied analytically and experimentally. The configuration used was a laminate with an across-the-width delamination. An approximate super-position stress analysis was developed to quantify the effects of various geometric, material, and load parameters on mode 2 and mode 2 strain <span class="hlt">energy</span> <span class="hlt">release</span> rates G sub/1 and G sub 2, respectively. Calculated values of G sub 1 and G sub 2 were then compared with measured cyclic delamination growth rates to determine the relative importance of G sub 1 and G sub 2. High growth rates were observed only when G sub 1 was large. However, slow growth was observed even when G sub 1 was negligibly small. This growth apparently was due to a large value of G sub 2.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018AIPC.1959d0008E','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018AIPC.1959d0008E"><span><span class="hlt">Energy</span> <span class="hlt">release</span> estimation for fragmenting meteoroid</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Egorova, L. A.; Lokhin, V. V.</p> <p>2018-05-01</p> <p>It is known that for the adequate interpretation of fireball observations it is necessary to take into account its fragmentation in the Earth's atmosphere. Various models for large cosmic body destruction in the atmosphere are known. Presented work continues our previous research on the fragmentation of fireballs. Proposing a model for the destruction of a fireball we also submit a model for the transition of its kinetic <span class="hlt">energy</span> to thermal one. The meteoroid destruction under consideration is similar to the destruction of a solid body during an explosion. The kinetic <span class="hlt">energy</span> of the moving particles of the crashing meteoric body transform into the thermal <span class="hlt">energy</span> of the gas volume in which their motion occurs.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/ADA582523','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA582523"><span>University Capstone Project: Enhanced Initiation Techniques for Thermochemical <span class="hlt">Energy</span> Conversion</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>2013-03-01</p> <p>technologies such as scramjets, gas turbine engines (relight and <span class="hlt">afterburner</span> ignition), and pulsed detonation engines ( PDEs ) because of the limited...events in a flow tube were recorded, and the PDE engine was fired while monitoring ignition time and wave speed throughout the detonation process...long steel tube fitted with a 36” long, 2” x 2” square polycarbonate test section is used in place of the instrumented detonation tube. The PDE</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.nrel.gov/news/program/2018/new-open-source-version-of-floris-released.html','SCIGOVWS'); return false;" href="https://www.nrel.gov/news/program/2018/new-open-source-version-of-floris-released.html"><span>New Open-Source Version of FLORIS <span class="hlt">Released</span> | News | NREL</span></a></p> <p><a target="_blank" href="http://www.science.gov/aboutsearch.html">Science.gov Websites</a></p> <p></p> <p></p> <p>New <em>Open</em>-Source Version of FLORIS <span class="hlt">Released</span> New <em>Open</em>-Source Version of FLORIS <span class="hlt">Released</span> January 26 , 2018 National Renewable <span class="hlt">Energy</span> Laboratory (NREL) researchers recently <span class="hlt">released</span> an updated <em>open</em>-source simplified and documented. Because of the living, <em>open</em>-source nature of the newly updated utility, NREL</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014cosp...40E3437U','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014cosp...40E3437U"><span>The statistical analysis of <span class="hlt">energy</span> <span class="hlt">release</span> in small-scale coronal structures</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ulyanov, Artyom; Kuzin, Sergey; Bogachev, Sergey</p> <p></p> <p>We present the results of statistical analysis of impulsive flare-like brightenings, which numerously occur in the quiet regions of solar corona. For our study, we utilized high-cadence observations performed with two EUV-telescopes - TESIS/Coronas-Photon and AIA/SDO. In total, we processed 6 sequences of images, registered throughout the period between 2009 and 2013, covering the rising phase of the 24th solar cycle. Based on high-speed DEM estimation method, we developed a new technique to evaluate the main parameters of detected events (geometrical sizes, duration, temperature and thermal <span class="hlt">energy</span>). We then obtained the statistical distributions of these parameters and examined their variations depending on the level of solar activity. The results imply that near the minimum of the solar cycle the <span class="hlt">energy</span> <span class="hlt">release</span> in quiet corona is mainly provided by small-scale events (nanoflares), whereas larger events (microflares) prevail on the peak of activity. Furthermore, we investigated the coronal conditions that had specified the formation and triggering of registered flares. By means of photospheric magnetograms obtained with MDI/SoHO and HMI/SDO instruments, we examined the topology of local magnetic fields at different stages: the pre-flare phase, the peak of intensity and the ending phase. To do so, we introduced a number of topological parameters including the total magnetic flux, the distance between magnetic sources and their mutual arrangement. The found correlation between the change of these parameters and the formation of flares may offer an important tool for application of flare forecasting.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28565910','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28565910"><span>Photochemical <span class="hlt">Energy</span> Storage and Electrochemically Triggered <span class="hlt">Energy</span> <span class="hlt">Release</span> in the Norbornadiene-Quadricyclane System: UV Photochemistry and IR Spectroelectrochemistry in a Combined Experiment.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Brummel, Olaf; Waidhas, Fabian; Bauer, Udo; Wu, Yanlin; Bochmann, Sebastian; Steinrück, Hans-Peter; Papp, Christian; Bachmann, Julien; Libuda, Jörg</p> <p>2017-07-06</p> <p>The two valence isomers norbornadiene (NBD) and quadricyclane (QC) enable solar <span class="hlt">energy</span> storage in a single molecule system. We present a new photoelectrochemical infrared reflection absorption spectroscopy (PEC-IRRAS) experiment, which allows monitoring of the complete <span class="hlt">energy</span> storage and <span class="hlt">release</span> cycle by in situ vibrational spectroscopy. Both processes were investigated, the photochemical conversion from NBD to QC using the photosensitizer 4,4'-bis(dimethylamino)benzophenone (Michler's ketone, MK) and the electrochemically triggered cycloreversion from QC to NBD. Photochemical conversion was obtained with characteristic conversion times on the order of 500 ms. All experiments were performed under full potential control in a thin-layer configuration with a Pt(111) working electrode. The vibrational spectra of NBD, QC, and MK were analyzed in the fingerprint region, permitting quantitative analysis of the spectroscopic data. We determined selectivities for both the photochemical conversion and the electrochemical cycloreversion and identified the critical steps that limit the reversibility of the storage cycle.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/ADA071312','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA071312"><span>Peak Overpressures for Internal Blast</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>1979-06-01</p> <p>fuels that also are oxygen- deficient (trinitrotoluene ( TNT ), for example), the initial detonation is followed by combustion in an <span class="hlt">afterburn</span> ; it is...and consequently show lesser <span class="hlt">afterburn</span> effects. Figure 8 shows overpressures for reference internal explo- sions with TNT , an oxygen-deficient...excplosive (oxygen balance of -14% to C02 and -257 to CO) 8 with pronounced <span class="hlt">afterburn</span> effects that depend on the TNT -air ratio. Shown for compari- soa are</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5049949','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5049949"><span>Effects of levomilnacipran extended-<span class="hlt">release</span> on motivation/<span class="hlt">energy</span> and functioning in adults with major depressive disorder</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Gommoll, Carl; Chen, Changzheng; Kramer, Kenneth; Sambunaris, Angelo</p> <p>2016-01-01</p> <p>The objective of this post-hoc analysis was to investigate the relationship between motivation/<span class="hlt">energy</span> and functional impairment in patients with major depressive disorder (MDD). Data were taken from a phase 3 trial of levomilnacipran extended-<span class="hlt">release</span> (ER) in adults with MDD (NCT01034462; N=429) that used the 18-item Motivation and <span class="hlt">Energy</span> Inventory (MEI) to assess motivation/<span class="hlt">energy</span>. Two subgroups with lower and higher motivation/<span class="hlt">energy</span> were defined using baseline MEI total scores (≤28 and >28, respectively). Change from baseline in the Sheehan Disability Scale (SDS) total score was analyzed in the intent-to-treat (ITT) population and both subgroups. Path analyses were carried out in the ITT population and a lower MEI subgroup to assess the direct and indirect effects of levomilnacipran ER on SDS total score change. In the ITT population and the lower MEI subgroup, significant differences were found between levomilnacipran ER and placebo for changes in the SDS total score (−2.6 and −3.9, both P<0.01), but not in the higher MEI subgroup. The indirect effect of levomilnacipran ER on SDS total score improvement, as mediated by MEI total score change, was 79.9% in the lower MEI subgroup and 67.2% in the ITT population. Levomilnacipran ER was previously shown to improve motivation/<span class="hlt">energy</span> in adults with MDD. The current analysis indicates that improvements in functional impairment were considerably mediated by improvements in motivation/<span class="hlt">energy</span>, particularly in patients with lower motivation/<span class="hlt">energy</span> at baseline. PMID:27455513</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_10");'>10</a></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li class="active"><span>12</span></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_12 --> <div id="page_13" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li class="active"><span>13</span></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="241"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19910048398&hterms=process+accounting&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3Dprocess%2Baccounting','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19910048398&hterms=process+accounting&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3Dprocess%2Baccounting"><span>Collisionless coupling processes in AMPTE <span class="hlt">releases</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Lui, A. T. Y.</p> <p>1990-01-01</p> <p>An evaluation is made of results obtained to date by in situ measurements, numerical simulations, and theoretical considerations of Active Magnetospheric Particle Tracer Explorer chemical <span class="hlt">releases</span> bearing on the nature of collisionless coupling processes. It is noted that both laminar and turbulent forces act to couple the solar wind momentum and <span class="hlt">energy</span> to the <span class="hlt">release</span> cloud; the magnetic field compression formed in this interaction plays an important intermediary role in coupling the two plasmas, and the intense electrostatic turbulence generated enhances the interaction. A scenario accounting for several features in the observed evolution of the December 27, 1984 artificial comet <span class="hlt">release</span> is presented.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..19.9188M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..19.9188M"><span>The use of Remotely Piloted Aircraft Systems for the Innovative Methodologies in thermal <span class="hlt">Energy</span> <span class="hlt">Release</span> monitoring</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Marotta, Enrica; Avino, Rosario; Avvisati, Gala; Belviso, Pasquale; Caliro, Stefano; Caputo, Teresa; Carandente, Antonio; Peluso, Rosario; Sangianantoni, Agata; Sansivero, Fabio; Vilardo, Giuseppe</p> <p>2017-04-01</p> <p>Last years have been characterized by a fast development of Remotely Piloted Aircraft Systems which are becoming cheaper, lighter and more powerful. The concurrent development of high resolution, lightweight and <span class="hlt">energy</span> saving sensors sometimes specifically designed for air-borne applications are together rapidly changing the way in which it is possible to perform monitoring and surveys in hazardous environments such as volcanoes. An example of this convergence is the new methodology we are currently developing at the INGV-Osservatorio Vesuviano for the estimation of the thermal <span class="hlt">energy</span> <span class="hlt">release</span> of volcanic diffuse degassing areas using the ground temperatures from thermal infrared images. Preliminary experiments, carried out during many-years campaigns performed inside at La Solfatara crater by using thermal infrared images and K type thermocouples inserted into the ground at various depths, found a correlation between surface temperature and shallow gradient. Due to the large extent of areas affected by thermal anomalies, an effective and expedite tool to acquire the IR images is a RPAS equipped with high-resolution thermal and visible cameras. These acquisitions allow to quickly acquire the data to produce a heat <span class="hlt">release</span> map. This map is then orthorectified and geocoded in order to be superimposed on digital terrain models or on the orthophotogrammetric mosaic obtained after processing photos acquired by RPAS. Such expedite maps of heat flux, taking in account accurate filtering of atmospheric influence, represents a useful tool for volcanic surveillance monitoring purposes. In order to start all the activities of these drones we had to acquire all necessary permissions required by the complex Italian normative.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/20122847','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/20122847"><span>Metabolic and stress-related roles of prolactin-<span class="hlt">releasing</span> peptide.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Onaka, Tatsushi; Takayanagi, Yuki; Leng, Gareth</p> <p>2010-05-01</p> <p>In the modern world, improvements in human health can be offset by unhealthy lifestyle factors, including the deleterious consequences of stress and obesity. For <span class="hlt">energy</span> homeostasis, humoral factors and neural afferents from the gastrointestinal tract, in combination with long-term nutritional signals, communicate information to the brain to regulate <span class="hlt">energy</span> intake and expenditure. <span class="hlt">Energy</span> homeostasis and stress interact with each other, and stress affects both food intake and <span class="hlt">energy</span> expenditure. Prolactin-<span class="hlt">releasing</span> peptide, synthesized in discrete neuronal populations in the hypothalamus and brainstem, plays an important role in integrating these responses. This review describes how prolactin-<span class="hlt">releasing</span> peptide neurons receive information concerning both internal metabolic states and environmental conditions, and play a key role in <span class="hlt">energy</span> homeostasis and stress responses. 2010 Elsevier Ltd. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1028083','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/1028083"><span>Metering Best Practices, A Guide to Achieving Utility Resource Efficiency, <span class="hlt">Release</span> 2.0</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Sullivan, Greg; Hunt, W. D.; Pugh, Ray</p> <p>2011-08-31</p> <p>This <span class="hlt">release</span> is an update and expansion of the information provided in <span class="hlt">Release</span> 1.0 of the Metering Best Practice Guide that was issued in October 2007. This <span class="hlt">release</span>, as was the previous <span class="hlt">release</span>, was developed under the direction of the U.S. Department of <span class="hlt">Energy</span>'s Federal <span class="hlt">Energy</span> Management Program (FEMP). The mission of FEMP is to facilitate the Federal Government's implementation of sound cost-effective <span class="hlt">energy</span> management and investment practices to enhance the nation's <span class="hlt">energy</span> security and environmental stewardship. Each of these activities is directly related to achieving requirements set forth in the <span class="hlt">Energy</span> Policy Acts of 1992 and 2005, the Energymore » Independence and Security Act (EISA) of 2007, and the goals that have been established in Executive Orders 13423 and 13514 - and also those practices that are inherent in sound management of Federal financial and personnel resources.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/ADA603843','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA603843"><span>U.S. Air Force Bomber Sustainment and Modernization: Background and Issues for Congress</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>2014-06-04</p> <p>turbofan Thrust: Each engine up to 17,000 pounds Wingspan: 185 feet (56.4 meters) Length: 159 feet, 4 inches (48.5 meters) Height: 40 feet, 8...precision and non-precision weapons. Features The B-1B’s blended wing and body configuration, variable-geometry wings, and turbofan <span class="hlt">afterburning</span> engines... turbofan engine with <span class="hlt">afterburner</span> Thrust: 30,000-plus pounds with <span class="hlt">afterburner</span>, per engine Wingspan: 137 feet (41.8 meters) extended forward, 79 feet</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013SPIE.8779E..1MS','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013SPIE.8779E..1MS"><span>Microstructured snow targets for high <span class="hlt">energy</span> quasi-monoenergetic proton acceleration</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Schleifer, E.; Nahum, E.; Eisenmann, S.; Botton, M.; Baspaly, A.; Pomerantz, I.; Abricht, F.; Branzel, J.; Priebe, G.; Steinke, S.; Andreev, A.; Schnuerer, M.; Sandner, W.; Gordon, D.; Sprangle, P.; Ledingham, K. W. D.; Zigler, A.</p> <p>2013-05-01</p> <p>Compact size sources of high <span class="hlt">energy</span> protons (50-200MeV) are expected to be key technology in a wide range of scientific applications 1-8. One promising approach is the Target Normal Sheath Acceleration (TNSA) scheme 9,10, holding record level of 67MeV protons generated by a peta-Watt laser 11. In general, laser intensity exceeding 1018 W/cm2 is required to produce MeV level protons. Another approach is the Break-Out <span class="hlt">Afterburner</span> (BOA) scheme which is a more efficient acceleration scheme but requires an extremely clean pulse with contrast ratio of above 10-10. Increasing the <span class="hlt">energy</span> of the accelerated protons using modest <span class="hlt">energy</span> laser sources is a very attractive task nowadays. Recently, nano-scale targets were used to accelerate ions 12,13 but no significant enhancement of the accelerated proton <span class="hlt">energy</span> was measured. Here we report on the generation of up to 20MeV by a modest (5TW) laser system interacting with a microstructured snow target deposited on a Sapphire substrate. This scheme relax also the requirement of high contrast ratio between the pulse and the pre-pulse, where the latter produces the highly structured plasma essential for the interaction process. The plasma near the tip of the snow target is subject to locally enhanced laser intensity with high spatial gradients, and enhanced charge separation is obtained. Electrostatic fields of extremely high intensities are produced, and protons are accelerated to MeV-level <span class="hlt">energies</span>. PIC simulations of this targets reproduce the experimentally measured <span class="hlt">energy</span> scaling and predict the generation of 150 MeV protons from laser power of 100TW laser system18.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27916951','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27916951"><span>Silica-Based and Borate-Based, Titania-Containing Bioactive Coatings Characterization: Critical Strain <span class="hlt">Energy</span> <span class="hlt">Release</span> Rate, Residual Stresses, Hardness, and Thermal Expansion.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Rodriguez, Omar; Matinmanesh, Ali; Phull, Sunjeev; Schemitsch, Emil H; Zalzal, Paul; Clarkin, Owen M; Papini, Marcello; Towler, Mark R</p> <p>2016-12-01</p> <p>Silica-based and borate-based glass series, with increasing amounts of TiO₂ incorporated, are characterized in terms of their mechanical properties relevant to their use as metallic coating materials. It is observed that borate-based glasses exhibit CTE (Coefficient of Thermal Expansion) closer to the substrate's (Ti6Al4V) CTE, translating into higher mode I critical strain <span class="hlt">energy</span> <span class="hlt">release</span> rates of glasses and compressive residual stresses and strains at the coating/substrate interface, outperforming the silica-based glasses counterparts. An increase in the content of TiO₂ in the glasses results in an increase in the mode I critical strain <span class="hlt">energy</span> <span class="hlt">release</span> rate for both the bulk glass and for the coating/substrate system, proving that the addition of TiO₂ to the glass structure enhances its toughness, while decreasing its bulk hardness. Borate-based glass BRT3, with 15 mol % TiO₂ incorporated, exhibits superior properties overall compared to the other proposed glasses in this work, as well as 45S5 Bioglass ® and Pyrex.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5197991','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5197991"><span>Silica-Based and Borate-Based, Titania-Containing Bioactive Coatings Characterization: Critical Strain <span class="hlt">Energy</span> <span class="hlt">Release</span> Rate, Residual Stresses, Hardness, and Thermal Expansion</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Rodriguez, Omar; Matinmanesh, Ali; Phull, Sunjeev; Schemitsch, Emil H.; Zalzal, Paul; Clarkin, Owen M.; Papini, Marcello; Towler, Mark R.</p> <p>2016-01-01</p> <p>Silica-based and borate-based glass series, with increasing amounts of TiO2 incorporated, are characterized in terms of their mechanical properties relevant to their use as metallic coating materials. It is observed that borate-based glasses exhibit CTE (Coefficient of Thermal Expansion) closer to the substrate’s (Ti6Al4V) CTE, translating into higher mode I critical strain <span class="hlt">energy</span> <span class="hlt">release</span> rates of glasses and compressive residual stresses and strains at the coating/substrate interface, outperforming the silica-based glasses counterparts. An increase in the content of TiO2 in the glasses results in an increase in the mode I critical strain <span class="hlt">energy</span> <span class="hlt">release</span> rate for both the bulk glass and for the coating/substrate system, proving that the addition of TiO2 to the glass structure enhances its toughness, while decreasing its bulk hardness. Borate-based glass BRT3, with 15 mol % TiO2 incorporated, exhibits superior properties overall compared to the other proposed glasses in this work, as well as 45S5 Bioglass® and Pyrex. PMID:27916951</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017PhRvL.118o5101K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017PhRvL.118o5101K"><span>Turbulent Kinetic <span class="hlt">Energy</span> in the <span class="hlt">Energy</span> Balance of a Solar Flare</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kontar, E. P.; Perez, J. E.; Harra, L. K.; Kuznetsov, A. A.; Emslie, A. G.; Jeffrey, N. L. S.; Bian, N. H.; Dennis, B. R.</p> <p>2017-04-01</p> <p>The <span class="hlt">energy</span> <span class="hlt">released</span> in solar flares derives from a reconfiguration of magnetic fields to a lower <span class="hlt">energy</span> state, and is manifested in several forms, including bulk kinetic <span class="hlt">energy</span> of the coronal mass ejection, acceleration of electrons and ions, and enhanced thermal <span class="hlt">energy</span> that is ultimately radiated away across the electromagnetic spectrum from optical to x rays. Using an unprecedented set of coordinated observations, from a suite of instruments, we here report on a hitherto largely overlooked <span class="hlt">energy</span> component—the kinetic <span class="hlt">energy</span> associated with small-scale turbulent mass motions. We show that the spatial location of, and timing of the peak in, turbulent kinetic <span class="hlt">energy</span> together provide persuasive evidence that turbulent <span class="hlt">energy</span> may play a key role in the transfer of <span class="hlt">energy</span> in solar flares. Although the kinetic <span class="hlt">energy</span> of turbulent motions accounts, at any given time, for only ˜(0.5 - 1 )% of the <span class="hlt">energy</span> <span class="hlt">released</span>, its relatively rapid (˜1 - 10 s ) energization and dissipation causes the associated throughput of <span class="hlt">energy</span> (i.e., power) to rival that of major components of the <span class="hlt">released</span> <span class="hlt">energy</span> in solar flares, and thus presumably in other astrophysical acceleration sites.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28452537','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28452537"><span>Turbulent Kinetic <span class="hlt">Energy</span> in the <span class="hlt">Energy</span> Balance of a Solar Flare.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Kontar, E P; Perez, J E; Harra, L K; Kuznetsov, A A; Emslie, A G; Jeffrey, N L S; Bian, N H; Dennis, B R</p> <p>2017-04-14</p> <p>The <span class="hlt">energy</span> <span class="hlt">released</span> in solar flares derives from a reconfiguration of magnetic fields to a lower <span class="hlt">energy</span> state, and is manifested in several forms, including bulk kinetic <span class="hlt">energy</span> of the coronal mass ejection, acceleration of electrons and ions, and enhanced thermal <span class="hlt">energy</span> that is ultimately radiated away across the electromagnetic spectrum from optical to x rays. Using an unprecedented set of coordinated observations, from a suite of instruments, we here report on a hitherto largely overlooked <span class="hlt">energy</span> component-the kinetic <span class="hlt">energy</span> associated with small-scale turbulent mass motions. We show that the spatial location of, and timing of the peak in, turbulent kinetic <span class="hlt">energy</span> together provide persuasive evidence that turbulent <span class="hlt">energy</span> may play a key role in the transfer of <span class="hlt">energy</span> in solar flares. Although the kinetic <span class="hlt">energy</span> of turbulent motions accounts, at any given time, for only ∼(0.5-1)% of the <span class="hlt">energy</span> <span class="hlt">released</span>, its relatively rapid (∼1-10  s) energization and dissipation causes the associated throughput of <span class="hlt">energy</span> (i.e., power) to rival that of major components of the <span class="hlt">released</span> <span class="hlt">energy</span> in solar flares, and thus presumably in other astrophysical acceleration sites.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015PhDT.......150M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015PhDT.......150M"><span>Light activated nitric oxide <span class="hlt">releasing</span> materials</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Muizzi Casanas, Dayana Andreina</p> <p></p> <p>The ability to control the location and dosage of biologically active molecules inside the human body can be critical to maximizing effective treatment of cardiovascular diseases like angina. The current standard of treatment relies on the metabolism of organonitrate drugs into nitric oxide (NO), which are not specific, and also show problems with densitization with long-term use. There is a need then to create a treatment method that gives targeted <span class="hlt">release</span> of NO. Metal-nitrosyl (M-NO) complexes can be used for delivery of NO since the <span class="hlt">release</span> of NO can be controlled with light. However, the NO-<span class="hlt">releasing</span> drug must be activated with red light to ensure maximum penetration of light through tissue. However, the <span class="hlt">release</span> of NO from M-NO complexes with red-light activation is a significant challenge since the <span class="hlt">energy</span> required to break the metal-NO bond is usually larger than the <span class="hlt">energy</span> provided by red light. The goal of this project was to create red- sensitive, NO-<span class="hlt">releasing</span> materials based on Ru-salen-nitrosyl compounds. Our approach was to first modify Ru salen complexes to sensitize the photochemistry for <span class="hlt">release</span> of NO after red light irradiation. Next, we pursued polymerization of the Ru-salen complexes. We report the synthesis and quantitative photochemical characterization of a series of ruthenium salen nitrosyl complexes. These complexes were modified by incorporating electron donating groups in the salen ligand structure at key locations to increase electron density on the Ru. Complexes with either an --OH or --OCH3 substituent showed an improvement in the quantum yield of <span class="hlt">release</span> of NO upon blue light irradiation compared to the unmodified salen. These --OH and --OCH3 complexes were also sensitized for NO <span class="hlt">release</span> after red light activation, however the red-sensitive complexes were unstable and showed ligand substitution on the order of minutes. The substituted complexes remained sensitive for NO <span class="hlt">release</span>, but only after blue light irradiation. The Ru</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19950026596','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19950026596"><span>Maximum thrust mode evaluation</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Orme, John S.; Nobbs, Steven G.</p> <p>1995-01-01</p> <p>Measured reductions in acceleration times which resulted from the application of the F-15 performance seeking control (PSC) maximum thrust mode during the dual-engine test phase is presented as a function of power setting and flight condition. Data were collected at altitudes of 30,000 and 45,000 feet at military and maximum <span class="hlt">afterburning</span> power settings. The time savings for the supersonic acceleration is less than at subsonic Mach numbers because of the increased modeling and control complexity. In addition, the propulsion system was designed to be optimized at the mid supersonic Mach number range. Recall that even though the engine is at maximum <span class="hlt">afterburner</span>, PSC does not trim the <span class="hlt">afterburner</span> for the maximum thrust mode. Subsonically at military power, time to accelerate from Mach 0.6 to 0.95 was cut by between 6 and 8 percent with a single engine application of PSC, and over 14 percent when both engines were optimized. At maximum <span class="hlt">afterburner</span>, the level of thrust increases were similar in magnitude to the military power results, but because of higher thrust levels at maximum <span class="hlt">afterburner</span> and higher aircraft drag at supersonic Mach numbers the percentage thrust increase and time to accelerate was less than for the supersonic accelerations. Savings in time to accelerate supersonically at maximum <span class="hlt">afterburner</span> ranged from 4 to 7 percent. In general, the maximum thrust mode has performed well, demonstrating significant thrust increases at military and maximum <span class="hlt">afterburner</span> power. Increases of up to 15 percent at typical combat-type flight conditions were identified. Thrust increases of this magnitude could be useful in a combat situation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1993IJFr...59...69L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1993IJFr...59...69L"><span>Variation of the <span class="hlt">energy</span> <span class="hlt">release</span> rate as a crack approaches and passes through an elastic inclusion</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Li, Rongshun; Chudnovsky, A.</p> <p>1993-02-01</p> <p>The variation of the <span class="hlt">energy</span> <span class="hlt">release</span> rate (ERP) at the tip of a crack penetrating an elastic inclusion is analyzed using an approach involving modeling the random array of microcracks or other defects by an elastic inclusion with effective elastic properties. Computations are carried out using a finite element procedure. The eight-noded isoparametric serendipity element with the shift of the midpoint to the quarter-point is used to simulate the singularity at the crack tip, and the crack growth is accommodated by implementing a mesh regeneration technique. The ERP values were calculated for various crack tip positions which simulate the process of the crack approaching and penetrating the inclusion.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19930060443&hterms=ERP&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3DERP','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19930060443&hterms=ERP&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3DERP"><span>Variation of the <span class="hlt">energy</span> <span class="hlt">release</span> rate as a crack approaches and passes through an elastic inclusion</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Li, Rongshun; Chudnovsky, A.</p> <p>1993-01-01</p> <p>The variation of the <span class="hlt">energy</span> <span class="hlt">release</span> rate (ERP) at the tip of a crack penetrating an elastic inclusion is analyzed using an approach involving modeling the random array of microcracks or other defects by an elastic inclusion with effective elastic properties. Computations are carried out using a finite element procedure. The eight-noded isoparametric serendipity element with the shift of the midpoint to the quarter-point is used to simulate the singularity at the crack tip, and the crack growth is accommodated by implementing a mesh regeneration technique. The ERP values were calculated for various crack tip positions which simulate the process of the crack approaching and penetrating the inclusion.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27523328','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27523328"><span>Kinetic <span class="hlt">Energy</span> <span class="hlt">Release</span> of the Singly and Doubly Charged Methylene Chloride Molecule: The Role of Fast Dissociation.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Alcantara, K F; Rocha, A B; Gomes, A H A; Wolff, W; Sigaud, L; Santos, A C F</p> <p>2016-09-01</p> <p>The center of mass kinetic <span class="hlt">energy</span> <span class="hlt">release</span> distribution (KERD) spectra of selected ionic fragments, formed through dissociative single and double photoionization of CH2Cl2 at photon <span class="hlt">energies</span> around the Cl 2p edge, were extracted from the shape and width of the experimentally obtained time-of-flight (TOF) distributions. The KERD spectra exhibit either smooth profiles or structures, depending on the moiety and photon <span class="hlt">energy</span>. In general, the heavier the ionic fragments, the lower their average KERDs are. In contrast, the light H(+) fragments are observed with kinetic <span class="hlt">energies</span> centered around 4.5-5.5 eV, depending on the photon <span class="hlt">energy</span>. It was observed that the change in the photon <span class="hlt">energy</span> involves a change in the KERDs, indicating different processes or transitions taking place in the breakup process. In the particular case of double ionization with the ejection of two charged fragments, the KERDs present have characteristics compatible with the Coulombic fragmentation model. Intending to interpret the experimental data, singlet and triplet states at Cl 2p edge of the CH2Cl2 molecule, corresponding to the Cl (2p → 10a1*) and Cl (2p → 4b1*) transitions, were calculated at multiconfigurational self-consistent field (MCSCF) level and multireference configuration interaction (MRCI). These states were selected to form the spin-orbit coupling matrix elements, which after diagonalization result in a spin-orbit manifold. Minimum <span class="hlt">energy</span> pathways for dissociation of the molecule were additionally calculated aiming to give support to the presence of the ultrafast dissociation mechanism in the molecular breakup.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/20002674-compact-closed-loop-controlled-waste-incinerator','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/20002674-compact-closed-loop-controlled-waste-incinerator"><span>Compact, closed-loop controlled waste incinerator</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Schadow, K.C.; Seeker, W.R.</p> <p>1999-07-01</p> <p>Technologies for solid and liquid waste destruction in compact incinerators are being developed in collaboration between industry, universities, and a Government laboratory. This paper reviews progress on one technology, namely active combustion control to achieve efficient and controlled <span class="hlt">afterburning</span> of air-starved reaction products. This technology which uses synchronized waste gas injection into acoustically stabilized air vortices was transitioned to a simplified <span class="hlt">afterburner</span> design and practical operational conditions. The full-scale, simplified <span class="hlt">afterburner</span>, which achieved CO and NO{sub x} emissions of about 30 ppm with a residence time of less than 50 msec, was integrated with a commercially available marine incinerator tomore » increase throughput and reduce emissions. Closed-loop active control with diode laser sensors and novel control strategies was demonstrated on a sub-scale <span class="hlt">afterburner</span>.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19850004196','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19850004196"><span>Dynamic compression and volatile <span class="hlt">release</span> of carbonates</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Tyburczy, J. A.; Ahrens, T. J.</p> <p>1984-01-01</p> <p>Particle velocity profiles upon shock compression and isentropic <span class="hlt">releases</span> were measured for polycrystalline calcite. The Solenhofen limestone <span class="hlt">release</span> paths lie, close to the Hugoniot. Calcite 3 to 2 transition, upon <span class="hlt">release</span>, was observed, but rarefaction shocks were not detected. The equation of state is used to predict the fraction of material devolatilized upon isentropic <span class="hlt">release</span> as a function of shock pressure. The effect of ambient partial pressure of CO2 on the calculations is demonstrated and considered in models of atmospheric evolution by impact induced mineral devolatilization. The radiative characteristics of shocked calcite indicate that localization of thermal <span class="hlt">energy</span> occurs under shock compression. Shock entropy calculations result in a minimum estimate of 90% devolatilization upon complete <span class="hlt">release</span> from 10 GPa. Isentropic <span class="hlt">release</span> paths from calculated continuum Hugoniot temperatures cross into the CaO (solid) + CO2 (vapor) field at improbably low pressures. It is found that <span class="hlt">release</span> paths from measured shock temperatures cross into the melt plus vapor field at pressures greater than .5 GPa, which suggests that devolatilization is initiated at the shear banding sites.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/978409','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/978409"><span>Reactive Blast Waves from Composite Charges</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Kuhl, A L; Bell, J B; Beckner, V E</p> <p>2009-10-16</p> <p>Investigated here is the performance of composite explosives - measured in terms of the blast wave they drive into the surrounding environment. The composite charge configuration studied here was a spherical booster (1/3 charge mass), surrounded by aluminum (Al) powder (2/3 charge mass) at an initial density of {rho}{sub 0} = 0.604 g/cc. The Al powder acts as a fuel but does not detonate - thereby providing an extreme example of a 'non-ideal' explosive (where 2/3 of the charge does not detonate). Detonation of the booster charge creates a blast wave that disperses the Al powder and ignites the ensuingmore » Al-air mixture - thereby forming a two-phase combustion cloud embedded in the explosion. <span class="hlt">Afterburning</span> of the booster detonation products with air also enhances and promotes the Al-air combustion process. Pressure waves from such reactive blast waves have been measured in bomb calorimeter experiments. Here we describe numerical simulations of those experiments. A Heterogeneous Continuum Model was used to model the dispersion and combustion of the Al particle cloud. It combines the gasdynamic conservation laws for the gas phase with a dilute continuum model for the dispersed phase, as formulated by Nigmatulin. Inter-phase mass, momentum and <span class="hlt">energy</span> exchange are prescribed by phenomenological models of Khasainov. It incorporates a combustion model based on mass conservation laws for fuel, air and products; source/sink terms are treated in the fast-chemistry limit appropriate for such gasdynamic fields, along with a model for mass transfer from the particle phase to the gas. The model takes into account both the <span class="hlt">afterburning</span> of the detonation products of the booster with air, and the combustion of the Al particles with air. The model equations were integrated by high-order Godunov schemes for both the gas and particle phases. Adaptive Mesh Refinement (AMR) was used to capture the <span class="hlt">energy</span>-bearing scales of the turbulent flow on the computational grid, and to track</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JPhCS.908a2016S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JPhCS.908a2016S"><span><span class="hlt">Energy</span> <span class="hlt">release</span> rate analysis on the interface cracks of enamel-cement-bracket fracture using virtual crack closure technique</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Samshuri, S. F.; Daud, R.; Rojan, M. A.; Mat, F.; Basaruddin, K. S.; Hassan, R.</p> <p>2017-10-01</p> <p>This paper presents the <span class="hlt">energy</span> method to evaluate fracture behavior of enamel-cement-bracket system based on cement thickness. Finite element (FE) model of enamel-cement-bracket was constructed by using ANSYS Parametric Design Language (APDL). Three different thickness were used in this study, 0.05, 0.2, and 0.271 mm which assigned as thin, medium and thick for both enamel-cement and cement bracket interface cracks. Virtual crack closure technique (VCCT) was implemented as a simulation method to calculated <span class="hlt">energy</span> <span class="hlt">release</span> rate (ERR). Simulation results were obtained for each thickness are discussed by using Griffith’s <span class="hlt">energy</span> balance approach. ERR for thin thickness are found to be the lowest compared to medium and thick. Peak value of ERR also showed a significant different between medium and thick thickness. Therefore, weakest bonding occurred at low cement thickness because less load required to produce enough <span class="hlt">energy</span> to detach the bracket. For medium and thick thickness, both increased rapidly in <span class="hlt">energy</span> value at about the mid-point of the enamel-cement interface. This behavior occurred because of the increasing in mechanical and surface <span class="hlt">energy</span> when the cracks are increasing. However, result for thick thickness are higher at mid-point compared to thin thickness. In conclusion, fracture behavior of enamel cracking process for medium most likely the safest to avoid enamel fracture and withstand bracket debonding.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/5492188','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/5492188"><span>Radioactive materials <span class="hlt">released</span> from nuclear power plants</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Tichler, J.; Norden, K.; Congemi, J.</p> <p></p> <p><span class="hlt">Releases</span> of radioactive materials in airborne and liquid effluents from commercial light water reactors during 1987 have been compiled and reported. Data on solid waste shipments as well as selected operating information have been included. This report supplements earlier annual reports issued by the former Atomic <span class="hlt">Energy</span> Commission and the Nuclear Regulatory Commission. The 1987 <span class="hlt">release</span> data are summarized in tabular form. Data covering specific radionuclides are summarized. 16 tabs.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li class="active"><span>13</span></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_13 --> <div id="page_14" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li class="active"><span>14</span></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="261"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/5667195','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/5667195"><span>Radioactive materials <span class="hlt">released</span> from nuclear power plants</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Tichler, J.; Norden, K.; Congemi, J.</p> <p></p> <p><span class="hlt">Releases</span> of radioactive materials in airborne and liquid effluents from commercial light water reactors during 1988 have been compiled and reported. Data on solid waste shipments as well as selected operating information have been included. This report supplements earlier annual reports issued by the former Atomic <span class="hlt">Energy</span> Commission and the Nuclear Regulatory Commission. The 1988 <span class="hlt">release</span> data are summarized in tabular form. Data covering specific radionuclides are summarized. 16 tabs.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/CFR-2010-title10-vol1/pdf/CFR-2010-title10-vol1-sec14-43.pdf','CFR'); return false;" href="https://www.gpo.gov/fdsys/pkg/CFR-2010-title10-vol1/pdf/CFR-2010-title10-vol1-sec14-43.pdf"><span>10 CFR 14.43 - Acceptance of payment constitutes <span class="hlt">release</span>.</span></a></p> <p><a target="_blank" href="http://www.gpo.gov/fdsys/browse/collectionCfr.action?selectedYearFrom=2010&page.go=Go">Code of Federal Regulations, 2010 CFR</a></p> <p></p> <p>2010-01-01</p> <p>... 10 <span class="hlt">Energy</span> 1 2010-01-01 2010-01-01 false Acceptance of payment constitutes <span class="hlt">release</span>. 14.43 Section... Commission Action and Authority § 14.43 Acceptance of payment constitutes <span class="hlt">release</span>. Acceptance by the claimant, his agent, or legal representative, of any award, compromise, or settlement made under the provisions...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20070038346','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20070038346"><span>A Semi-Analytical Method for Determining the <span class="hlt">Energy</span> <span class="hlt">Release</span> Rate of Cracks in Adhesively-Bonded Single-Lap Composite Joints</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Yang, Charles; Sun, Wenjun; Tomblin, John S.; Smeltzer, Stanley S., III</p> <p>2007-01-01</p> <p>A semi-analytical method for determining the strain <span class="hlt">energy</span> <span class="hlt">release</span> rate due to a prescribed interface crack in an adhesively-bonded, single-lap composite joint subjected to axial tension is presented. The field equations in terms of displacements within the joint are formulated by using first-order shear deformable, laminated plate theory together with kinematic relations and force equilibrium conditions. The stress distributions for the adherends and adhesive are determined after the appropriate boundary and loading conditions are applied and the equations for the field displacements are solved. Based on the adhesive stress distributions, the forces at the crack tip are obtained and the strain <span class="hlt">energy</span> <span class="hlt">release</span> rate of the crack is determined by using the virtual crack closure technique (VCCT). Additionally, the test specimen geometry from both the ASTM D3165 and D1002 test standards are utilized during the derivation of the field equations in order to correlate analytical models with future test results. The system of second-order differential field equations is solved to provide the adherend and adhesive stress response using the symbolic computation tool, Maple 9. Finite element analyses using J-integral as well as VCCT were performed to verify the developed analytical model. The finite element analyses were conducted using the commercial finite element analysis software ABAQUS. The results determined using the analytical method correlated well with the results from the finite element analyses.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1014667','DOE-PATENT-XML'); return false;" href="https://www.osti.gov/servlets/purl/1014667"><span>Storing and transporting <span class="hlt">energy</span></span></a></p> <p><a target="_blank" href="http://www.osti.gov/doepatents">DOEpatents</a></p> <p>McClaine, Andrew W.; Brown, Kenneth</p> <p>2010-09-07</p> <p>Among other things, hydrogen is <span class="hlt">released</span> from water at a first location using <span class="hlt">energy</span> from a first <span class="hlt">energy</span> source; the <span class="hlt">released</span> hydrogen is stored in a metal hydride slurry; and the metal hydride slurry is transported to a second location remote from the first location.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/543282','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/543282"><span>Stored <span class="hlt">energy</span> in irradiated silicon carbide</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Snead, L.L.; Burchell, T.D.</p> <p>1997-04-01</p> <p>This report presents a short review of the phenomenon of Wigner stored <span class="hlt">energy</span> <span class="hlt">release</span> from irradiated graphite and discusses it in relation to neutron irradiation of silicon carbide. A single published work in the area of stored <span class="hlt">energy</span> <span class="hlt">release</span> in SiC is reviewed and the results are discussed. It appears from this previous work that because the combination of the comparatively high specific heat of SiC and distribution in activation <span class="hlt">energies</span> for recombining defects, the stored <span class="hlt">energy</span> <span class="hlt">release</span> of SiC should only be a problem at temperatures lower than those considered for fusion devices. The conclusion of this preliminary reviewmore » is that the stored <span class="hlt">energy</span> <span class="hlt">release</span> in SiC will not be sufficient to cause catastrophic heating in fusion reactor components, though further study would be desirable.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/23974798','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/23974798"><span>Fluoride <span class="hlt">releasing</span> and enamel demineralization around orthodontic brackets by fluoride-<span class="hlt">releasing</span> composite containing nanoparticles.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Melo, Mary A S; Morais, Weslanny A; Passos, Vanara F; Lima, Juliana P M; Rodrigues, Lidiany K A</p> <p>2014-05-01</p> <p>Fluoride-containing materials have been suggested to control enamel demineralization around orthodontic brackets during the treatment with fixed appliances. The improvement of their properties has been made through innovations, such as the application of nanotechnology by incorporation of nanofillers. This in vitro study evaluated the capacity of fluoride <span class="hlt">releasing</span> and enamel demineralization inhibition of fluoride-<span class="hlt">releasing</span> nanofilled cement around orthodontic brackets using an artificial caries biofilm model. Forty bovine enamel discs were selected by evaluating surface microhardness and randomized into four groups (n = 10): non-fluoride-<span class="hlt">releasing</span> microfilled composite, fluoride-<span class="hlt">releasing</span> microfilled composite, resin-modified glass ionomer cement (RMGI), and fluoride-<span class="hlt">releasing</span> nanofilled composite (FN). After brackets bonding in each disc, the specimens were subjected to a cariogenic challenge through a Streptococcus mutans biofilm model. After the experimental period, the biofilm formed around the brackets was collected for fluoride analysis and the mineral loss around the brackets was determined by integrated demineralization via cross-sectional microhardness measurement at 20 and 70 μm from the bracket margin. Additionally, samples of each group were subjected to <span class="hlt">energy</span>-dispersive X-ray spectroscopy (EDX) analysis examined under a scanning electron microscopy (SEM). ANOVA followed by Tukey test were applied for fluoride concentration and mineral loss data, respectively. At both distances, only RMGI statistically differed from the other groups presenting the lowest demineralization, although there was a trend to a lower demineralization of enamel around brackets in FN group. Similar condition was found to fluoride concentration and EDX/SEM analysis. Under the cariogenic exposure condition of this study, the fluoride-<span class="hlt">releasing</span> nanofilled material had similar performance to fluoride-<span class="hlt">releasing</span> microfilled materials. The presence of nanofillers in the fluoride-<span class="hlt">releasing</span></p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/5095587','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/5095587"><span>Radioactive materials <span class="hlt">released</span> from nuclear power plants. Annual report 1978</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Tichler, J.; Benkovitz, C.</p> <p></p> <p><span class="hlt">Releases</span> of radioactive materials in airborne and liquid effluents from commerical light water reactors during 1978 have been compiled and reported. Data on soild waste shipments as well as selected operating information have been included. This report supplements earlier annual reports by the former Atomic <span class="hlt">Energy</span> Commission and the Nuclear Regulatory Commission. The 1978 <span class="hlt">release</span> data are compared with previous years <span class="hlt">releases</span> in tabular form. Data covering specific radionuclides are summarized.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29514078','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29514078"><span>Mechanism of Mg2+-Accompanied Product <span class="hlt">Release</span> in Sugar Nucleotidyltransferases.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Vithani, Neha; Ankush Jagtap, Pravin Kumar; Verma, Sunil Kumar; Tripathi, Ravi; Awasthi, Shalini; Nair, Nisanth N; Prakash, Balaji</p> <p>2018-03-06</p> <p>The nucleotidyl transfer reaction, catalyzed by sugar nucleotidyltransferases (SNTs), is assisted by two active site Mg 2+ ions. While studying this reaction using X-ray crystallography, we captured snapshots of the pyrophosphate (product) as it exits along a pocket. Surprisingly, one of the active site Mg 2+ ions remains coordinated to the exiting pyrophosphate. This hints at the participation of Mg 2+ in the process of product <span class="hlt">release</span>, besides its role in catalyzing nucleotidyl transfer. These observations are further supported by enhanced sampling molecular dynamics simulations. Free <span class="hlt">energy</span> computations suggest that the product <span class="hlt">release</span> is likely to be rate limiting in SNTs, and the origin of the high free <span class="hlt">energy</span> barrier for product <span class="hlt">release</span> could be traced back to the "slow" conformational change of an Arg residue at the exit end of the pocket. These results establish a dual role for Mg 2+ , and propose a general mechanism of product <span class="hlt">release</span> during the nucleotidyl transfer by SNTs. Copyright © 2018 Elsevier Ltd. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19870033836&hterms=astronomia+espacio&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3Dastronomia%2By%2Bespacio','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19870033836&hterms=astronomia+espacio&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3Dastronomia%2By%2Bespacio"><span>Spatial and temporal characteristics of flare <span class="hlt">energy</span> <span class="hlt">release</span> determined from X-ray and radio imaging observations</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Hernandez, A. M.; Machado, M. E.; Vilmer, N.; Trottet, G.</p> <p>1986-01-01</p> <p>Using the Hard X-ray Imaging Spectrometer (HXIS) from the Solar Maximum Mission Satellite, the morphological aspects and temporal evolution of three major flares which occurred on June 29, 1980 are studied. One of these events, observed at 10:40 UT, is analyzed in particular detail, including Hard X-ray Burst Spectrometer (HXRBS) data and metric wavelength data from the Nancay radioheliograph. The flares occurred during the interaction of two distinct magnetic structures. There is an early onset phase during which there is a weak level of particle acceleration, perhaps accompanied by strong heating within the magnetic interaction region. The impulsive phase of high power <span class="hlt">energy</span> <span class="hlt">release</span> is associated with a major interaction between the two structures and accompanied by strong acceleration and heating.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/7070382-computer-model-predictions-local-effects-large-solid-fuel-rocket-motors-stratospheric-ozone-technical-report','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/7070382-computer-model-predictions-local-effects-large-solid-fuel-rocket-motors-stratospheric-ozone-technical-report"><span>Computer model predictions of the local effects of large, solid-fuel rocket motors on stratospheric ozone. Technical report</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Zittel, P.F.</p> <p>1994-09-10</p> <p>The solid-fuel rocket motors of large space launch vehicles <span class="hlt">release</span> gases and particles that may significantly affect stratospheric ozone densities along the vehicle's path. In this study, standard rocket nozzle and flowfield computer codes have been used to characterize the exhaust gases and particles through the <span class="hlt">afterburning</span> region of the solid-fuel motors of the Titan IV launch vehicle. The models predict that a large fraction of the HCl gas exhausted by the motors is converted to Cl and Cl2 in the plume <span class="hlt">afterburning</span> region. Estimates of the subsequent chemistry suggest that on expansion into the ambient daytime stratosphere, the highlymore » reactive chlorine may significantly deplete ozone in a cylinder around the vehicle track that ranges from 1 to 5 km in diameter over the altitude range of 15 to 40 km. The initial ozone depletion is estimated to occur on a time scale of less than 1 hour. After the initial effects, the dominant chemistry of the problem changes, and new models are needed to follow the further expansion, or closure, of the ozone hole on a longer time scale.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/ADA956432','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA956432"><span>Proposed Department of Defense Policy on Air Installations Compatible Use Zones</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>1973-06-01</p> <p>34 F-3 HIOHT MOW • 1! F-100 <span class="hlt">afterburner</span> 2A B-52H military 2C-5 ! F-101 F-6 C/KC-135A... <span class="hlt">afterburner</span> F-6 F-89 MONT MOW 10 F-8 F-94 F-ll T-38 B^7 military 2D A-5 B-58 military mONT MOW • HMNT MOUP * F-SO...imlitarv 2B-5 F S4F F MG F-104 military 2A-5 F-10« F-86E, F. H F-4B. C " F-86V \\ F-K HMNT MOW 4 B-67 F-3 <span class="hlt">afterburner</span></p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1395882','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/1395882"><span><span class="hlt">Energy</span>Plus™</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p></p> <p></p> <p>Originally developed in 1999, an updated version 8.8.0 with bug fixes was <span class="hlt">released</span> on September 30th, 2017. <span class="hlt">Energy</span>Plus™ is a whole building <span class="hlt">energy</span> simulation program that engineers, architects, and researchers use to model both <span class="hlt">energy</span> consumption—for heating, cooling, ventilation, lighting and plug and process loads—and water use in buildings. <span class="hlt">Energy</span>Plus is a console-based program that reads input and writes output to text files. It ships with a number of utilities including IDF-Editor for creating input files using a simple spreadsheet-like interface, EP-Launch for managing input and output files and performing batch simulations, and EP-Compare for graphically comparing the results ofmore » two or more simulations. Several comprehensive graphical interfaces for <span class="hlt">Energy</span>Plus are also available. DOE does most of its work with <span class="hlt">Energy</span>Plus using the OpenStudio® software development kit and suite of applications. DOE <span class="hlt">releases</span> major updates to <span class="hlt">Energy</span>Plus twice annually.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19950021867','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19950021867"><span>Static and dynamic strain <span class="hlt">energy</span> <span class="hlt">release</span> rates in toughened thermosetting composite laminates</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Cairns, Douglas S.</p> <p>1992-01-01</p> <p>In this work, the static and dynamic fracture properties of several thermosetting resin based composite laminates are presented. Two classes of materials are explored. These are homogeneous, thermosetting resins and toughened, multi-phase, thermosetting resin systems. Multi-phase resin materials have shown enhancement over homogenous materials with respect to damage resistance. The development of new dynamic tests are presented for composite laminates based on Width Tapered Double Cantilevered Beam (WTDCB) for Mode 1 fracture and the End Notched Flexure (ENF) specimen. The WTDCB sample was loaded via a low inertia, pneumatic cylinder to produce rapid cross-head displacements. A high rate, piezo-electric load cell and an accelerometer were mounted on the specimen. A digital oscilloscope was used for data acquisition. Typical static and dynamic load versus displacement plots are presented. The ENF specimen was impacted in three point bending with an instrumented impact tower. Fracture initiation and propagation <span class="hlt">energies</span> under static and dynamic conditions were determined analytically and experimentally. The test results for Mode 1 fracture are relatively insensitive to strain rate effects for the laminates tested in this study. The test results from Mode 2 fracture indicate that the toughened systems provide superior fracture initiation and higher resistance to propagation under dynamic conditions. While the static fracture properties of the homogeneous systems may be relatively high, the apparent Mode 2 dynamic critical strain <span class="hlt">energy</span> <span class="hlt">release</span> rate drops significantly. The results indicate that static Mode 2 fracture testing is inadequate for determining the fracture performance of composite structures subjected to conditions such as low velocity impact. A good correlation between the basic Mode 2 dynamic fracture properties and the performance is a combined material/structural Compression After Impact (CAI) test is found. These results underscore the importance of</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017MS%26E..283a2002C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017MS%26E..283a2002C"><span>Amphiphilic polymer based on fluoroalkyl and PEG side chains for fouling <span class="hlt">release</span> coating</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Cong, W. W.; Wang, K.; Yu, X. Y.; Zhang, H. Q.; Lv, Z.; Gui, T. J.</p> <p>2017-12-01</p> <p>Under static conditions, fouling <span class="hlt">release</span> coating could not express good <span class="hlt">release</span> property to marine organisms. Amphiphilic polymer with mixture of fluorinated monomer and short side group of polyethylene glycol (PEG) was synthesized. And also we studied the ability of amphiphilic polymer to influence the surface properties and how it controlled the adhesion of marine organisms to coated surfaces. By incorporating fluorinated monomer and PEG side chain into the polymer, the effect of incorporating both polar and non-polar groups on fouling-<span class="hlt">release</span> coating could be studied. The dry surface was characterized by three-dimensional digital microscopy and scanning electron microscopy (SEM), and the morphology of the amphiphilic fouling <span class="hlt">release</span> coating showed just like flaky petal. The amphiphilic polymer in fouling <span class="hlt">release</span> coating tended to reconstruct in water, and the ability was examined by static contact angle, which was smaller than the PDMS (polydimethylsiloxane) fouling <span class="hlt">release</span> coating. Also surface <span class="hlt">energy</span> was calculated by three solvents, and surface <span class="hlt">energy</span> of amphiphilic fouling <span class="hlt">release</span> coating was higher than that of the PDMS fouling <span class="hlt">release</span> coating. To understand more about its fouling <span class="hlt">release</span> property, seawater exposure method was adopted in gulf of Qingdao port. Fewer diatoms Navicula were found in biofilm after using amphiphilic fouling <span class="hlt">release</span> coating. In general, coating containing both PEG and fluorinated side chain possessed certain fouling <span class="hlt">release</span> property.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27914784','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27914784"><span><span class="hlt">Energy</span> efficient bead milling of microalgae: Effect of bead size on disintegration and <span class="hlt">release</span> of proteins and carbohydrates.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Postma, P R; Suarez-Garcia, E; Safi, C; Yonathan, K; Olivieri, G; Barbosa, M J; Wijffels, R H; Eppink, M H M</p> <p>2017-01-01</p> <p>The disintegration of three industry relevant algae (Chlorella vulgaris, Neochloris oleoabundans and Tetraselmis suecica) was studied in a lab scale bead mill at different bead sizes (0.3-1mm). Cell disintegration, proteins and carbohydrates <span class="hlt">released</span> into the water phase followed a first order kinetics. The process is selective towards proteins over carbohydrates during early stages of milling. In general, smaller beads led to higher kinetic rates, with a minimum specific <span class="hlt">energy</span> consumption of ⩽0.47kWhkg DW -1 for 0.3mm beads. After analysis of the stress parameters (stress number and stress intensity), it appears that optimal disintegration and <span class="hlt">energy</span> usage for all strains occurs in the 0.3-0.4mm range. During the course of bead milling, the native structure of the marker protein Rubisco was retained, confirming the mildness of the disruption process. Copyright © 2016 The Authors. Published by Elsevier Ltd.. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/6529113-installation-burning-out-scrap-metal','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/6529113-installation-burning-out-scrap-metal"><span>Installation for burning-out scrap metal</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Gutschmidt, P.</p> <p>1982-08-24</p> <p>Disclosed is an installation for burning-out scrap metal goods for the purpose of reclaiming scrap metal, comprising at least one furnace wagon, which is capable of being loaded with the scrap metal goods to be burned out; at least one burning-out chamber into which the furnace wagon is movable for burning-out the scrap metal goods to produce scrap steel; means for heating the burning-out chamber to a temperature of at least about 600* C.; at least one <span class="hlt">afterburning</span> chamber communicating with the burning-out chamber for <span class="hlt">afterburning</span> flue gases produced in the burning-out chamber at a temperature from about 1100* tomore » 1200* C.; a waste gas purifying plant communicating with the <span class="hlt">afterburning</span> chamber for eliminating the flue gas impurities and for the scrubbing of the flue-gases originating from the <span class="hlt">afterburning</span> chamber; and at least one cooling chamber arranged adjacent to and in selective communication with the burning-out chamber for cooling the burned-out material.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1046791','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/1046791"><span>Numerical Simulations of Thermobaric Explosions</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Kuhl, A L; Bell, J B; Beckner, V E</p> <p>2007-05-04</p> <p>A Model of the <span class="hlt">energy</span> evolution in thermobaric explosions is presented. It is based on the two-phase formulation: conservation laws for the gas and particle phases along with inter-phase interaction terms. It incorporates a Combustion Model based on the mass conservation laws for fuel, air and products; source/sink terms are treated in the fast-chemistry limit appropriate for such gas dynamic fields. The Model takes into account both the <span class="hlt">afterburning</span> of the detonation products of the booster with air, and the combustion of the fuel (Al or TNT detonation products) with air. Numerical simulations were performed for 1.5-g thermobaric explosions inmore » five different chambers (volumes ranging from 6.6 to 40 liters and length-to-diameter ratios from 1 to 12.5). Computed pressure waveforms were very similar to measured waveforms in all cases - thereby proving that the Model correctly predicts the <span class="hlt">energy</span> evolution in such explosions. The computed global fuel consumption {mu}(t) behaved as an exponential life function. Its derivative {dot {mu}}(t) represents the global rate of fuel consumption. It depends on the rate of turbulent mixing which controls the rate of <span class="hlt">energy</span> <span class="hlt">release</span> in thermobaric explosions.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3205187','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3205187"><span>Regulation of gonadotropin-<span class="hlt">releasing</span> hormone neurons by glucose</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Roland, Alison V.; Moenter, Suzanne M.</p> <p>2011-01-01</p> <p>Reproduction is influenced by <span class="hlt">energy</span> balance, but the physiological pathways mediating their relationship have not been fully elucidated. As the central regulators of fertility, gonadotropin-<span class="hlt">releasing</span> hormone (GnRH) neurons integrate numerous physiological signals, including metabolic cues. Circulating glucose levels regulate GnRH <span class="hlt">release</span> and may in part mediate the effects of negative <span class="hlt">energy</span> balance on fertility. Existing evidence suggests that neural pathways originating in the hindbrain, as well as in the hypothalamic feeding nuclei, transmit information concerning glucose availability to GnRH neurons. Here we review recent evidence suggesting that GnRH neurons may directly sense changes in glucose availability by a mechanism involving adenosine monophosphate-activated protein kinase (AMPK). These findings expand our understanding of how metabolic signaling in the brain regulates reproduction. PMID:21855365</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AIPC.1800d0003D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AIPC.1800d0003D"><span>Throttle pneumatic impact mechanism equipped with <span class="hlt">afterburner</span> idle-stroke chamber</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Dedov, Alexey; Frantseva, Eleanor; Dmitriev, Mikhail</p> <p>2017-01-01</p> <p>Pneumatic impact mechanisms are widely used in construction, mining and other economic sectors of a country. Such mechanisms are a base for a wide range of machines of various types and dimensions from hand-held tools to mounted piling hammers with impact <span class="hlt">energy</span> up to 10 000 J. This paper is aimed at creation of pneumatic impact mechanism with the improved characteristics, including operation, <span class="hlt">energy</span> use, weight and size which is especially important in space-limited working conditions. The research methods include development of computer mathematical model that can solve equations system and test a prototype model at the experimental stand. As a result of conducted research the pneumatic impact mechanism with the improved characteristics was developed. An engineering method for calculating throttle pneumatic impact mechanisms with a preset value of impact <span class="hlt">energy</span> from 1 to 20 000 was investigated. This method allows creating percussive machines of a wide range of application.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/808226','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/808226"><span>Environmental <span class="hlt">Releases</span> for Calendar Year 2001</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>DYEKMAN, D L</p> <p>2002-08-01</p> <p>This report fulfills the annual reporting requirements of US Department of <span class="hlt">Energy</span> (DOE) Order 5400.1, General Environmental Protection Program. The report contains tabular data summaries on air emissions and liquid effluents <span class="hlt">released</span> to the environment as well as nonroutine <span class="hlt">releases</span> during calendar year (CY) 2001. These <span class="hlt">releases</span>, bearing radioactive and hazardous substances, were from Bechtel Hanford, Inc. (BHI), CH2M HILL Hanford Group, Inc. (CHG), and Fluor Hanford (FH) managed facilities and activities. These data were obtained from direct sampling and analysis and from estimates based upon approved <span class="hlt">release</span> factors. This report further serves as a supplemental resource to the Hanfordmore » Site Environmental Report (HSER PNNL-13910), published by the Pacific Northwest National Laboratory. HSER includes a yearly accounting of the impacts on the surrounding populace and environment from major activities at the Hanford Site. HSER also summarizes the regulatory compliance status of the Hanford Site. Tables ES-1 through ES-5 display comprehensive data summaries of CY2001 air emission and liquid effluent <span class="hlt">releases</span>. The data displayed in these tables compiles the following: Radionuclide air emissions; Nonradioactive air emissions; Radionuclides in liquid effluents discharged to ground; Total volumes and flow rates of radioactive liquid effluents discharged to ground; and Radionuclides discharged to the Columbia River.« less</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li class="active"><span>14</span></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_14 --> <div id="page_15" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li class="active"><span>15</span></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="281"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=EC98-44817-2&hterms=learn+better+video&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D60%26Ntt%3Dlearn%2Bbetter%2Bvideo','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=EC98-44817-2&hterms=learn+better+video&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D60%26Ntt%3Dlearn%2Bbetter%2Bvideo"><span>SR-71A on Ramp with Dual Max <span class="hlt">Afterburner</span> Engines Firing</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p></p> <p>1998-01-01</p> <p>This night shot shows one of NASA's SR-71 Blackbird research aircraft on the ramp at the Dryden Flight Research Center, Edwards, California, with both engines running in max <span class="hlt">afterburner</span>. Two SR-71 aircraft have been used by NASA as testbeds for high-speed and high-altitude aeronautical research. The aircraft, an SR-71A and an SR-71B pilot trainer aircraft, have been based here at NASA's Dryden Flight Research Center, Edwards, California. They were transferred to NASA after the U.S. Air Force program was cancelled. As research platforms, the aircraft can cruise at Mach 3 for more than one hour. For thermal experiments, this can produce heat soak temperatures of over 600 degrees Fahrenheit (F). This operating environment makes these aircraft excellent platforms to carry out research and experiments in a variety of areas -- aerodynamics, propulsion, structures, thermal protection materials, high-speed and high-temperature instrumentation, atmospheric studies, and sonic boom characterization. The SR-71 was used in a program to study ways of reducing sonic booms or over pressures that are heard on the ground, much like sharp thunderclaps, when an aircraft exceeds the speed of sound. Data from this Sonic Boom Mitigation Study could eventually lead to aircraft designs that would reduce the 'peak' overpressures of sonic booms and minimize the startling affect they produce on the ground. One of the first major experiments to be flown in the NASA SR-71 program was a laser air data collection system. It used laser light instead of air pressure to produce airspeed and attitude reference data, such as angle of attack and sideslip, which are normally obtained with small tubes and vanes extending into the airstream. One of Dryden's SR-71s was used for the Linear Aerospike Rocket Engine, or LASRE Experiment. Another earlier project consisted of a series of flights using the SR-71 as a science camera platform for NASA's Jet Propulsion Laboratory in Pasadena, California. An upward</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/6537727-cavity-actuated-supersonic-mixing-combustion-control','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/6537727-cavity-actuated-supersonic-mixing-combustion-control"><span>Cavity-actuated supersonic mixing and combustion control</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Yu, K.H.; Schadow, K.C.</p> <p>1994-11-01</p> <p>Compressible shear layers in supersonic jets are quite stable and spread very slowly compared with incompressible shear layers. In this paper, a novel use of a cavity-actuated forcing technique is demonstrated for increasing the spreading rate of compressible shear layers. Periodic modulations were applied to Mach 2.0 reacting and nonreacting jets using the cavities that were attached at the exit of a circular supersonic nozzle. The effect of cavity-actuated forcing was studied as a function of the cavity geometry, in particular, the length and the depth of the cavity. When the cavities were tuned to certain frequencies, large-scale highly coherentmore » structures were produced in the shear layers substantially increasing the growth rate. The cavity excitation was successfully applied to both cold and hot supersonic jets. When applied to cold Mach 2.0 air jets. the cavity-actuated forcing increased the spreading rate of the initial shear layers with the convective Mach number (M[sub C]) of 0.85 by a factor of three. For high-temperature Mach 2.0 jets with M[sub C] of 1.4, a 50% increase in the spreading rate was observed with the forcing. Finally, the cavity-actuated forcing was applied to reacting supersonic jets with ethylene-oxygen <span class="hlt">afterburning</span>. For this case, the forcing caused a 20%--30% reduction in the <span class="hlt">afterburning</span> flame length and modified the <span class="hlt">afterburning</span> intensity significantly. The direction of the modification depended on the characteristics of the <span class="hlt">afterburning</span> flames. The intensity was reduced with forcing for unstable flames with weak <span class="hlt">afterburning</span> while it was increased for stable flames with strong <span class="hlt">afterburning</span>.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://eric.ed.gov/?q=drama+AND+therapy&pg=3&id=ED381701','ERIC'); return false;" href="https://eric.ed.gov/?q=drama+AND+therapy&pg=3&id=ED381701"><span>Emotional <span class="hlt">Release</span> for Children: Repairing the Past--Preparing the Future.</span></a></p> <p><a target="_blank" href="http://www.eric.ed.gov/ERICWebPortal/search/extended.jsp?_pageLabel=advanced">ERIC Educational Resources Information Center</a></p> <p>Pearson, Mark; Nolan, Patricia</p> <p></p> <p>Emotional <span class="hlt">Release</span> Counselling (ERC) is based on the simple premise that to feel emotions and <span class="hlt">energy</span> and to let them be expressed keeps us mentally healthy. ERC works to help a child be deeply connected to the sensation within the body, to develop self-awareness. The book explains the concept of emotional <span class="hlt">release</span> counseling and provides specific…</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19880041571&hterms=Magnetic+energy&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D60%26Ntt%3DMagnetic%2Benergy','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19880041571&hterms=Magnetic+energy&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D60%26Ntt%3DMagnetic%2Benergy"><span>The observed characteristics of flare <span class="hlt">energy</span> <span class="hlt">release</span>. I - Magnetic structure at the <span class="hlt">energy</span> <span class="hlt">release</span> site</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Machado, Marcos E.; Moore, Ronald L.; Hagyard, Mona J.; Hernandez, Ana M.; Rovira, Marta G.</p> <p>1988-01-01</p> <p>It is shown that flaring activity as seen in X-rays usually encompasses two or more interacting magnetic bipoles within an active region. Soft and hard X-ray spatiotemporal evolution is considered as well as the time dependence of the thermal <span class="hlt">energy</span> content in different magnetic bipoles participating in the flare, the hardness and impulsivity of the hard X-ray emission, and the relationship between the X-ray behavior and the strength and 'observable shear' of the magnetic field. It is found that the basic structure of a flare usually consists of an initiating closed bipole plus one or more adjacent closed bipoles impacted against it.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009Nanot..20r5103B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009Nanot..20r5103B"><span>A multifunctional magnetic nanocarrier bearing fluorescent dye for targeted drug delivery by enhanced two-photon triggered <span class="hlt">release</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Banerjee, Shashwat S.; Chen, Dong-Hwang</p> <p>2009-05-01</p> <p>We report a novel nanoformulation for targeted drug delivery which utilizes nanophotonics through the fusion of nanotechnology with biomedical application. The approach involves an <span class="hlt">energy</span>-transferring magnetic nanoscopic co-assembly fabricated of rhodamine B (RDB) fluorescent dye grafted gum arabic modified Fe3O4 magnetic nanoparticle and photosensitive linker by which dexamethasone drug is conjugated to the magnetic nano-assembly. The advantage offered by this nanoformulation is the indirect photo-triggered-on-demand drug <span class="hlt">release</span> by efficient up-converting <span class="hlt">energy</span> of the near-IR (NIR) light to higher <span class="hlt">energy</span> and intraparticle <span class="hlt">energy</span> transfer from the dye grafted magnetic nanoparticle to the linker for drug <span class="hlt">release</span> by cleavage. The synthesized nanoparticles were found to be of ultra-small size (13.33 nm) and are monodispersed in an aqueous suspension. Dexamethasone (Dexa) drug conjugated to RDB-GAMNP by photosensitive linker showed appreciable <span class="hlt">release</span> of Dexa by photo-triggered response on exposure to radiation having a wavelength in the NIR region whereas no detectable <span class="hlt">release</span> was observed in the dark. Photo-triggered response for the nanoformulation not bearing the rhodamine B dye was drastically less as less Dexa was <span class="hlt">released</span> on exposure to NIR radiation which suggest that the photo-cleavage of linker and <span class="hlt">release</span> of Dexa mainly originated from the indirect excitation through the uphill <span class="hlt">energy</span> conversions based on donor-acceptor model FRET. The promising pathway of nanophotonics for the on-demand <span class="hlt">release</span> of the drug makes this nanocarrier very promising for applications in nanomedicine.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/25272025','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25272025"><span>Probing the kinetic <span class="hlt">energy-release</span> dynamics of H-atom products from the gas-phase reaction of O(3P) with vinyl radical C2H3.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Jang, Su-Chan; Choi, Jong-Ho</p> <p>2014-11-21</p> <p>The gas-phase radical-radical reaction dynamics of ground-state atomic oxygen O((3)P) with vinyl radicals C2H3 has been studied by combining the results of vacuum-ultraviolet laser-induced fluorescence spectroscopy in a crossed beam configuration with ab initio calculations. The two radical reactants O((3)P) and C2H3 were produced by photolysis of NO2 and supersonic flash pyrolysis of C2H3I, respectively. Doppler profile analysis of the kinetic <span class="hlt">energy</span> <span class="hlt">release</span> of the nascent H-atom products from the title reaction O((3)P) + C2H3→ H((2)S) + CH2CO (ketene) revealed that the average translational <span class="hlt">energy</span> of the products and the average fraction of the total available <span class="hlt">energy</span> were 7.03 ± 0.30 kcal mol(-1) and 7.2%. The empirical data combined with CBS-QB3 level ab initio theory and statistical calculations demonstrated that the title oxygen-hydrogen exchange reaction is a major reaction channel, through an addition-elimination mechanism involving the formation of a short-lived, dynamical complex on the doublet potential <span class="hlt">energy</span> surface. On the basis of systematic comparison with several exchange reactions of hydrocarbon radicals, the observed kinetic <span class="hlt">energy</span> <span class="hlt">release</span> can be explained in terms of the weak impulse at the moment of decomposition in the loose transition state with a product-like geometry and a small reverse barrier along the exit channel.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018ApJ...854..178N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018ApJ...854..178N"><span>Two-stage <span class="hlt">Energy</span> <span class="hlt">Release</span> Process of a Confined Flare with Double HXR Peaks</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ning, Hao; Chen, Yao; Wu, Zhao; Su, Yang; Tian, Hui; Li, Gang; Du, Guohui; Song, Hongqiang</p> <p>2018-02-01</p> <p>A complete understanding of the onset and subsequent evolution of confined flares has not been achieved. Earlier studies mainly analyzed disk events so as to reveal their magnetic topology and the cause of confinement. In this study, taking advantage of a tandem of instruments working at different wavelengths of X-rays, EUVs, and microwaves, we present dynamic details about a confined flare observed on the northwestern limb of the solar disk on 2016 July 24. The entire dynamic evolutionary process starting from its onset is consistent with a loop–loop interaction scenario. The X-ray profiles manifest an intriguing double-peak feature. From the spectral fitting, it has been found that the first peak is nonthermally dominated, while the second peak is mostly multithermal with a hot (∼10 MK) and a super-hot (∼30 MK) component. This double-peak feature is unique in that the two peaks are clearly separated by 4 minutes, and the second peak reaches up to 25–50 keV in addition, at <span class="hlt">energy</span> bands above 3 keV, the X-ray fluxes decline significantly between the two peaks. This, together with other available imaging and spectral data, manifest a two-stage <span class="hlt">energy</span> <span class="hlt">release</span> process. A comprehensive analysis is carried out to investigate the nature of this two-stage process. We conclude that the second stage with the hot and super-hot sources mainly involves direct heating through a loop–loop reconnection at a relatively high altitude in the corona. The uniqueness of the event characteristics and the complete dataset make the study a nice addition to present literature on solar flares.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/24726419','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/24726419"><span>Experimental and modeling studies of ultrasound-assisted <span class="hlt">release</span> of phenolics from oak chips into model wine.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Tao, Yang; Zhang, Zhihang; Sun, Da-Wen</p> <p>2014-09-01</p> <p>The enhancement of <span class="hlt">release</span> of oak-related compounds from oak chips during wine aging with oak chips may interest the winemaking industry. In this study, the 25-kHz ultrasound waves were used to intensify the mass transfer of phenolics from oak chips into a model wine. The influences of acoustic <span class="hlt">energy</span> density (6.3-25.8 W/L) and temperature (15-25 °C) on the <span class="hlt">release</span> kinetics of total phenolics were investigated systematically. The results exhibited that the total phenolic yield <span class="hlt">released</span> was not affected by acoustic <span class="hlt">energy</span> density significantly whereas it increased with the increase of temperature during sonication. Furthermore, to describe the mechanism of mass transfer of phenolics in model wine under ultrasonic field, the <span class="hlt">release</span> kinetics of total phenolics was simulated by both a second-order kinetic model and a diffusion model. The modeling results revealed that the equilibrium concentration of total phenolics in model wine, the initial <span class="hlt">release</span> rate and effective diffusivity of total phenolics generally increased with acoustic <span class="hlt">energy</span> density and temperature. In addition, temperature had a negative effect on the second-order <span class="hlt">release</span> rate constant whereas acoustic <span class="hlt">energy</span> density had an opposite effect. Copyright © 2014 Elsevier B.V. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19890011915','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19890011915"><span>Strain <span class="hlt">energy</span> <span class="hlt">release</span> rate as a function of temperature and preloading history utilizing the edge delamination fatique test method</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Zimmerman, Richard S.; Adams, Donald F.</p> <p>1989-01-01</p> <p>Static laminate and tension-tension fatigue tests of IM7/8551-7 composite materials was performed. The Edge Delamination Test (EDT) was utilized to evaluate the temperature and preloading history effect on the critical strain <span class="hlt">energy</span> <span class="hlt">release</span> rate. Static and fatigue testing was performed at room temperature and 180 F (82 C). Three preloading schemes were used to precondition fatigue test specimens prior to performing the normal tension-tension fatigue EDT testing. Computer software was written to perform all fatigue testing while monitoring the dynamic modulus to detect the onset of delamination and record the test information for later retrieval and reduction.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1327951','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/1327951"><span><span class="hlt">Energy</span> by the Numbers: An <span class="hlt">Energy</span> Revolution</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>None</p> <p></p> <p>The U.S. Department of <span class="hlt">Energy</span> (DOE) today <span class="hlt">released</span> a new report that highlights the accelerated deployment of five clean <span class="hlt">energy</span> technologies: wind turbines, solar technologies for both utility-scale and distributed photovoltaic (PV), electric vehicles (EVs) and light-emitting diodes (LEDs). The report, Revolution…Now, was announced by <span class="hlt">Energy</span> Secretary Ernest Moniz during a discussion at The Atlantic’s Washington Ideas Forum.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3350736','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3350736"><span>Impact of <span class="hlt">release</span> dynamics of laser-irradiated polymer micropallets on the viability of selected adherent cells</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Ma, Huan; Mismar, Wael; Wang, Yuli; Small, Donald W.; Ras, Mat; Allbritton, Nancy L.; Sims, Christopher E.; Venugopalan, Vasan</p> <p>2012-01-01</p> <p>We use time-resolved interferometry, fluorescence assays and computational fluid dynamics (CFD) simulations to examine the viability of confluent adherent cell monolayers to selection via laser microbeam <span class="hlt">release</span> of photoresist polymer micropallets. We demonstrate the importance of laser microbeam pulse <span class="hlt">energy</span> and focal volume position relative to the glass–pallet interface in governing the threshold <span class="hlt">energies</span> for pallet <span class="hlt">release</span> as well as the pallet <span class="hlt">release</span> dynamics. Measurements using time-resolved interferometry show that increases in laser pulse <span class="hlt">energy</span> result in increasing pallet <span class="hlt">release</span> velocities that can approach 10 m s−1 through aqueous media. CFD simulations reveal that the pallet motion results in cellular exposure to transient hydrodynamic shear stress amplitudes that can exceed 100 kPa on microsecond timescales, and which produces reduced cell viability. Moreover, CFD simulation results show that the maximum shear stress on the pallet surface varies spatially, with the largest shear stresses occurring on the pallet periphery. Cell viability of confluent cell monolayers on the pallet surface confirms that the use of larger pulse <span class="hlt">energies</span> results in increased rates of necrosis for those cells situated away from the pallet centre, while cells situated at the pallet centre remain viable. Nevertheless, experiments that examine the viability of these cell monolayers following pallet <span class="hlt">release</span> show that proper choices for laser microbeam pulse <span class="hlt">energy</span> and focal volume position lead to the routine achievement of cell viability in excess of 90 per cent. These laser microbeam parameters result in maximum pallet <span class="hlt">release</span> velocities below 6 m s−1 and cellular exposure of transient hydrodynamic shear stresses below 20 kPa. Collectively, these results provide a mechanistic understanding that relates pallet <span class="hlt">release</span> dynamics and associated transient shear stresses with subsequent cellular viability. This provides a quantitative, mechanistic basis for determining</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/22158840','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/22158840"><span>Impact of <span class="hlt">release</span> dynamics of laser-irradiated polymer micropallets on the viability of selected adherent cells.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Ma, Huan; Mismar, Wael; Wang, Yuli; Small, Donald W; Ras, Mat; Allbritton, Nancy L; Sims, Christopher E; Venugopalan, Vasan</p> <p>2012-06-07</p> <p>We use time-resolved interferometry, fluorescence assays and computational fluid dynamics (CFD) simulations to examine the viability of confluent adherent cell monolayers to selection via laser microbeam <span class="hlt">release</span> of photoresist polymer micropallets. We demonstrate the importance of laser microbeam pulse <span class="hlt">energy</span> and focal volume position relative to the glass-pallet interface in governing the threshold <span class="hlt">energies</span> for pallet <span class="hlt">release</span> as well as the pallet <span class="hlt">release</span> dynamics. Measurements using time-resolved interferometry show that increases in laser pulse <span class="hlt">energy</span> result in increasing pallet <span class="hlt">release</span> velocities that can approach 10 m s(-1) through aqueous media. CFD simulations reveal that the pallet motion results in cellular exposure to transient hydrodynamic shear stress amplitudes that can exceed 100 kPa on microsecond timescales, and which produces reduced cell viability. Moreover, CFD simulation results show that the maximum shear stress on the pallet surface varies spatially, with the largest shear stresses occurring on the pallet periphery. Cell viability of confluent cell monolayers on the pallet surface confirms that the use of larger pulse <span class="hlt">energies</span> results in increased rates of necrosis for those cells situated away from the pallet centre, while cells situated at the pallet centre remain viable. Nevertheless, experiments that examine the viability of these cell monolayers following pallet <span class="hlt">release</span> show that proper choices for laser microbeam pulse <span class="hlt">energy</span> and focal volume position lead to the routine achievement of cell viability in excess of 90 per cent. These laser microbeam parameters result in maximum pallet <span class="hlt">release</span> velocities below 6 m s(-1) and cellular exposure of transient hydrodynamic shear stresses below 20 kPa. Collectively, these results provide a mechanistic understanding that relates pallet <span class="hlt">release</span> dynamics and associated transient shear stresses with subsequent cellular viability. This provides a quantitative, mechanistic basis for determining optimal</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19780002743','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19780002743"><span>Mechanical <span class="hlt">energy</span> storage device for hip disarticulation</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Vallotton, W. C. (Inventor)</p> <p>1977-01-01</p> <p>An artificial leg including a trunk socket, a thigh section hingedly coupled to the trunk socket, a leg section hingedly coupled to the thigh section and a foot section hingedly coupled to the leg section is outlined. A mechanical <span class="hlt">energy</span> storage device is operatively associated with the artificial leg for storage and <span class="hlt">release</span> of <span class="hlt">energy</span> during the normal walking stride of the user. <span class="hlt">Energy</span> is stored in the mechanical <span class="hlt">energy</span> storage device during a weight-bearing phase of the walking stride when the user's weight is on the artificial leg. <span class="hlt">Energy</span> is <span class="hlt">released</span> during a phase of the normal walking stride, when the user's weight is removed from the artificial leg. The stored <span class="hlt">energy</span> is <span class="hlt">released</span> from the <span class="hlt">energy</span> storage device to pivot the thigh section forwardly about the hinged coupling to the trunk socket.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.nrel.gov/news/press/2014/15409.html','SCIGOVWS'); return false;" href="https://www.nrel.gov/news/press/2014/15409.html"><span>NREL and Army Validate <span class="hlt">Energy</span> Savings for Net Zero <span class="hlt">Energy</span> Installations |</span></a></p> <p><a target="_blank" href="http://www.science.gov/aboutsearch.html">Science.gov Websites</a></p> <p></p> <p></p> <p>News | NREL</A> and Army Validate <em><span class="hlt">Energy</span></em> Savings for Net Zero <em><span class="hlt">Energy</span></em> Installations News <span class="hlt">Release</span> : NREL and Army Validate <em><span class="hlt">Energy</span></em> Savings for Net Zero <em><span class="hlt">Energy</span></em> Installations October 27, 2014 The U.S. Army (Army) has partnered with the <em><span class="hlt">Energy</span></em> Department's National Renewable <em><span class="hlt">Energy</span></em> Laboratory (NREL) to</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.nrel.gov/esif/news.html','SCIGOVWS'); return false;" href="https://www.nrel.gov/esif/news.html"><span><span class="hlt">Energy</span> Systems Integration Facility News | <span class="hlt">Energy</span> Systems Integration</span></a></p> <p><a target="_blank" href="http://www.science.gov/aboutsearch.html">Science.gov Websites</a></p> <p></p> <p></p> <p>, 2018 News <span class="hlt">Release</span>: NREL Taps Young to Oversee <em>Geothermal</em> <em><span class="hlt">Energy</span></em> Program In her new role, Young will work closely with NREL management to establish the lab's <em>geothermal</em> <em><span class="hlt">energy</span></em> portfolio, including research and development geared toward advancing the use of <em>geothermal</em> <em><span class="hlt">energy</span></em> as a renewable power source</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1419730','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/1419730"><span>MCNP Version 6.2 <span class="hlt">Release</span> Notes</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Werner, Christopher John; Bull, Jeffrey S.; Solomon, C. J.</p> <p></p> <p>Monte Carlo N-Particle or MCNP ® is a general-purpose Monte Carlo radiation-transport code designed to track many particle types over broad ranges of <span class="hlt">energies</span>. This MCNP Version 6.2 follows the MCNP6.1.1 beta version and has been <span class="hlt">released</span> in order to provide the radiation transport community with the latest feature developments and bug fixes for MCNP. Since the last <span class="hlt">release</span> of MCNP major work has been conducted to improve the code base, add features, and provide tools to facilitate ease of use of MCNP version 6.2 as well as the analysis of results. These <span class="hlt">release</span> notes serve as a general guidemore » for the new/improved physics, source, data, tallies, unstructured mesh, code enhancements and tools. For more detailed information on each of the topics, please refer to the appropriate references or the user manual which can be found at http://mcnp.lanl.gov. This <span class="hlt">release</span> of MCNP version 6.2 contains 39 new features in addition to 172 bug fixes and code enhancements. There are still some 33 known issues the user should familiarize themselves with (see Appendix).« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.eia.gov/outlooks/archive/aeo10/intensity_trends.html','EIAPUBS'); return false;" href="https://www.eia.gov/outlooks/archive/aeo10/intensity_trends.html"><span><span class="hlt">Energy</span> Intensity Trends in AEO2010 (<span class="hlt">released</span> in AEO2010)</span></a></p> <p><a target="_blank" href="http://www.eia.doe.gov/reports/">EIA Publications</a></p> <p></p> <p>2010-01-01</p> <p><span class="hlt">Energy</span> intensity (<span class="hlt">energy</span> consumption per dollar of real GDP) indicates how much <span class="hlt">energy</span> a country uses to produce its goods and services. From the early 1950s to the early 1970s, U.S. total primary <span class="hlt">energy</span> consumption and real GDP increased at nearly the same annual rate. During that period, real oil prices remained virtually flat. In contrast, from the mid-1970s to 2008, the relationship between <span class="hlt">energy</span> consumption and real GDP growth changed, with primary <span class="hlt">energy</span> consumption growing at less than one-third the previous average rate and real GDP growth continuing to grow at its historical rate. The decoupling of real GDP growth from <span class="hlt">energy</span> consumption growth led to a decline in <span class="hlt">energy</span> intensity that averaged 2.8% per year from 1973 to 2008. In the Annual <span class="hlt">Energy</span> Outlook 2010 Reference case, <span class="hlt">energy</span> intensity continues to decline, at an average annual rate of 1.9% from 2008 to 2035.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27775347','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27775347"><span>Molecular Dynamics and Free <span class="hlt">Energy</span> Simulations of Phenylacetate and CO2 <span class="hlt">Release</span> from AMDase and Its G74C/C188S Mutant: A Possible Rationale for the Reduced Activity of the Latter.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Karmakar, Tarak; Balasubramanian, Sundaram</p> <p>2016-11-17</p> <p>Arylmalonate decarboxylase (AMDase) catalyzes the decarboxylation of α-aryl-α-methyl malonates to produce optically pure α-arylpropionates of industrial and medicinal importance. Herein, atomistic molecular dynamics simulations have been carried out to delineate the mechanism of the <span class="hlt">release</span> of product molecules phenylacetate (PAC) and carbon dioxide (CO 2 ), from the wild-type (WT) and its G74C/C188S mutant enzymes. Both of the product molecules follow a crystallographically characterized solvent-accessible channel to come out of the protein interior. A higher free <span class="hlt">energy</span> barrier for the <span class="hlt">release</span> of PAC from G74C/C188S compared to that in the WT is consistent with the experimentally observed compromised efficiency of the mutant. The <span class="hlt">release</span> of CO 2 precedes that of PAC; free <span class="hlt">energy</span> barriers for CO 2 and PAC <span class="hlt">release</span> in the WT enzyme are calculated to be ∼1-2 and ∼23 kcal/mol, respectively. Postdecarboxylation, CO 2 moves toward a hydrophobic pocket formed by Pro 14, Leu 38, Leu 40, Leu 77, and the side chain of Tyr 48 which serves as its temporary "reservoir". CO 2 <span class="hlt">releases</span> following a channel mainly decorated by apolar residues, unlike in the case of oxalate decarboxylase where polar residues mediate its transport.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/CFR-2014-title10-vol4/pdf/CFR-2014-title10-vol4-sec1707-208.pdf','CFR2014'); return false;" href="https://www.gpo.gov/fdsys/pkg/CFR-2014-title10-vol4/pdf/CFR-2014-title10-vol4-sec1707-208.pdf"><span>10 CFR 1707.208 - Restrictions that apply to <span class="hlt">released</span> records.</span></a></p> <p><a target="_blank" href="http://www.gpo.gov/fdsys/browse/collectionCfr.action?selectedYearFrom=2014&page.go=Go">Code of Federal Regulations, 2014 CFR</a></p> <p></p> <p>2014-01-01</p> <p>... 10 <span class="hlt">Energy</span> 4 2014-01-01 2014-01-01 false Restrictions that apply to <span class="hlt">released</span> records. 1707.208 Section 1707.208 <span class="hlt">Energy</span> DEFENSE NUCLEAR FACILITIES SAFETY BOARD TESTIMONY BY DNFSB EMPLOYEES AND PRODUCTION OF OFFICIAL RECORDS IN LEGAL PROCEEDINGS Requests for Testimony and Production of Documents § 1707...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/CFR-2012-title10-vol4/pdf/CFR-2012-title10-vol4-sec1707-208.pdf','CFR2012'); return false;" href="https://www.gpo.gov/fdsys/pkg/CFR-2012-title10-vol4/pdf/CFR-2012-title10-vol4-sec1707-208.pdf"><span>10 CFR 1707.208 - Restrictions that apply to <span class="hlt">released</span> records.</span></a></p> <p><a target="_blank" href="http://www.gpo.gov/fdsys/browse/collectionCfr.action?selectedYearFrom=2012&page.go=Go">Code of Federal Regulations, 2012 CFR</a></p> <p></p> <p>2012-01-01</p> <p>... 10 <span class="hlt">Energy</span> 4 2012-01-01 2012-01-01 false Restrictions that apply to <span class="hlt">released</span> records. 1707.208 Section 1707.208 <span class="hlt">Energy</span> DEFENSE NUCLEAR FACILITIES SAFETY BOARD TESTIMONY BY DNFSB EMPLOYEES AND PRODUCTION OF OFFICIAL RECORDS IN LEGAL PROCEEDINGS Requests for Testimony and Production of Documents § 1707...</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li class="active"><span>15</span></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_15 --> <div id="page_16" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li class="active"><span>16</span></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="301"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/CFR-2011-title10-vol4/pdf/CFR-2011-title10-vol4-sec1707-208.pdf','CFR2011'); return false;" href="https://www.gpo.gov/fdsys/pkg/CFR-2011-title10-vol4/pdf/CFR-2011-title10-vol4-sec1707-208.pdf"><span>10 CFR 1707.208 - Restrictions that apply to <span class="hlt">released</span> records.</span></a></p> <p><a target="_blank" href="http://www.gpo.gov/fdsys/browse/collectionCfr.action?selectedYearFrom=2011&page.go=Go">Code of Federal Regulations, 2011 CFR</a></p> <p></p> <p>2011-01-01</p> <p>... 10 <span class="hlt">Energy</span> 4 2011-01-01 2011-01-01 false Restrictions that apply to <span class="hlt">released</span> records. 1707.208 Section 1707.208 <span class="hlt">Energy</span> DEFENSE NUCLEAR FACILITIES SAFETY BOARD TESTIMONY BY DNFSB EMPLOYEES AND PRODUCTION OF OFFICIAL RECORDS IN LEGAL PROCEEDINGS Requests for Testimony and Production of Documents § 1707...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/CFR-2010-title10-vol4/pdf/CFR-2010-title10-vol4-sec1707-208.pdf','CFR'); return false;" href="https://www.gpo.gov/fdsys/pkg/CFR-2010-title10-vol4/pdf/CFR-2010-title10-vol4-sec1707-208.pdf"><span>10 CFR 1707.208 - Restrictions that apply to <span class="hlt">released</span> records.</span></a></p> <p><a target="_blank" href="http://www.gpo.gov/fdsys/browse/collectionCfr.action?selectedYearFrom=2010&page.go=Go">Code of Federal Regulations, 2010 CFR</a></p> <p></p> <p>2010-01-01</p> <p>... 10 <span class="hlt">Energy</span> 4 2010-01-01 2010-01-01 false Restrictions that apply to <span class="hlt">released</span> records. 1707.208 Section 1707.208 <span class="hlt">Energy</span> DEFENSE NUCLEAR FACILITIES SAFETY BOARD TESTIMONY BY DNFSB EMPLOYEES AND PRODUCTION OF OFFICIAL RECORDS IN LEGAL PROCEEDINGS Requests for Testimony and Production of Documents § 1707...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/CFR-2013-title10-vol4/pdf/CFR-2013-title10-vol4-sec1707-208.pdf','CFR2013'); return false;" href="https://www.gpo.gov/fdsys/pkg/CFR-2013-title10-vol4/pdf/CFR-2013-title10-vol4-sec1707-208.pdf"><span>10 CFR 1707.208 - Restrictions that apply to <span class="hlt">released</span> records.</span></a></p> <p><a target="_blank" href="http://www.gpo.gov/fdsys/browse/collectionCfr.action?selectedYearFrom=2013&page.go=Go">Code of Federal Regulations, 2013 CFR</a></p> <p></p> <p>2013-01-01</p> <p>... 10 <span class="hlt">Energy</span> 4 2013-01-01 2013-01-01 false Restrictions that apply to <span class="hlt">released</span> records. 1707.208 Section 1707.208 <span class="hlt">Energy</span> DEFENSE NUCLEAR FACILITIES SAFETY BOARD TESTIMONY BY DNFSB EMPLOYEES AND PRODUCTION OF OFFICIAL RECORDS IN LEGAL PROCEEDINGS Requests for Testimony and Production of Documents § 1707...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19820017379','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19820017379"><span>Exhaust emissions survey of a turbofan engine for flame holder swirl type augmentors at simulated altitude flight conditions</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Moss, J. E., Jr.</p> <p>1981-01-01</p> <p>Emissions of carbon dioxide, total oxides of nitrogen, unburned hydrocarbons, and carbon monoxide from an F100 <span class="hlt">afterburning</span> two spool turbofan engine at simulated flight conditions are reported. Tests were run at Mach 0.8 at altitudes of 10.97 and 13.71 km (36,000 and 45,000 ft), and at Mach 1.2 at 13.71 km (45,000 ft). Emission measurements were made from intermediate power (nonafterburning) through maximum <span class="hlt">afterburning</span>, using a single point gas sample probe traversed across the horizontal diameter of the exhaust nozzle. The data show that emissions vary with flight speed, altitude, power level, and radial position across the nozzle. Carbon monoxide emissions were low for intermediate and partial <span class="hlt">afterburning</span> power. Unburned hydrocarbons were near zero for most of the simulated flight conditions. At maximum <span class="hlt">afterburning</span>, there were regions of NOx deficiency in regions of high CO. The results suggest that the low NOx levels observed in the tests are a result of interaction with high CO in the thermal converter. CO2 emissions were proportional to local fuel air ratio for all test conditions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/24619858','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/24619858"><span>Low effective activation <span class="hlt">energies</span> for oxygen <span class="hlt">release</span> from metal oxides: evidence for mass-transfer limits at high heating rates.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Jian, Guoqiang; Zhou, Lei; Piekiel, Nicholas W; Zachariah, Michael R</p> <p>2014-06-06</p> <p>Oxygen <span class="hlt">release</span> from metal oxides at high temperatures is relevant to many thermally activated chemical processes, including chemical-looping combustion, solar thermochemical cycles and energetic thermite reactions. In this study, we evaluated the thermal decomposition of nanosized metal oxides under rapid heating (~10(5) K s(-1)) with time-resolved mass spectrometry. We found that the effective activation-<span class="hlt">energy</span> values that were obtained using the Flynn-Wall-Ozawa isoconversional method are much lower than the values found at low heating rates, indicating that oxygen transport might be rate-determining at a high heating rate. © 2014 WILEY-VCH Verlag GmbH & Co. KGaA, Weinheim.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19950004113&hterms=thermal+energy&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3Dthermal%2Benergy','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19950004113&hterms=thermal+energy&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3Dthermal%2Benergy"><span>TES (Thermal <span class="hlt">Energy</span> Storage) Video News <span class="hlt">Release</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p></p> <p>1994-01-01</p> <p>TES is an in-space technology experiment that flew on STS-62. Its intent is to investigate the behavior of two different thermal <span class="hlt">energy</span> storage materials as they undergo repeated melting and freezing in the microgravity environment.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017Natur.551...40M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017Natur.551...40M"><span>Theoretical physics: Quarks fuse to <span class="hlt">release</span> <span class="hlt">energy</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Miller, Gerald A.</p> <p>2017-11-01</p> <p>In nuclear fusion, <span class="hlt">energy</span> is produced by the rearrangement of protons and neutrons. The discovery of an analogue of this process involving particles called quarks has implications for both nuclear and particle physics. See Letter p.89</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017APS..SHK.K6001H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017APS..SHK.K6001H"><span>Measurements of the Shock <span class="hlt">Release</span> Of Quartz and Paralyene-N</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hawreliak, James; Karasik, Max; Oh, Jaechul; Aglitskiy, Yefim</p> <p>2017-06-01</p> <p>The shock and <span class="hlt">release</span> properties of Quartz and hydrocarbons are important to high <span class="hlt">energy</span> density (HED) research and inertial confinement fusion (ICF) science. The bulk of HED material research studies single shock or multiple shock conditions. The challenge with measuring <span class="hlt">release</span> properties is unlike shocks which have a single interface from which to measure the properties, the <span class="hlt">release</span> establishes gradients in the sample. The streaked x-ray imaging capability of the NIKE laser allow the interface between quartz and CH to be measured during the <span class="hlt">release</span>, giving measurements of the interface velocity and CH density. Here, we present experimental results from the NIKE laser where quartz and parylene-N are shock compressed to high pressure and temperature and the <span class="hlt">release</span> state is measured through x-ray imaging. The shock state is characterized by shock front velocity measurements using VISAR and the <span class="hlt">release</span> state is characterized by using side-on streaked x-ray radiography Work supported by DOE/NNSA.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/445804-formation-emission-nitrogen-oxide-gas-turbine-engines-plume-effluent-characteristics-tf3o-p111+-tf33-p9-engines-final-technical-report-november-december','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/445804-formation-emission-nitrogen-oxide-gas-turbine-engines-plume-effluent-characteristics-tf3o-p111+-tf33-p9-engines-final-technical-report-november-december"><span>Formation and emission of nitrogen oxide in gas turbine engines: plume effluent characteristics of TF3O-P111+ and TF33-P9 engines. Final technical report, 1 November-17 December 1993</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Dill, J.W.; Sowa, W.A.; Samuelsen, G.S.</p> <p>1996-06-30</p> <p>Phase I of this project focused on the creation of a spatial emissions map of the plume effluent in the exhaust stream directly behind the engine in a jet engine test cell (JETC). Both <span class="hlt">afterburning</span> TF30-P111+ and non-after-burning TF33-P9 engines were tested. Measurements were taken in conjunction with actual engine tests for validity of the data. Temperature, oxides of nitrogen (NOx), carbon monoxide (CO) concentration, and velocity were among the characteristics measured radially and axially in the plume for each engine type. The main focus of this study was on NOx, consisting of nitric oxide (NO) and nitrogen dioxide (NO2).more » Measurements in the P111+ plume reveal levels of NOx above 300 ppm along the centerline of the effluent. A dip in the NOx emissions at <span class="hlt">afterburner</span> shows signs of a reburning and/or dilution effect by the atmospheric combustion in the effluent. Significant amounts of NO2 are present in the effluent over the entire power range. Temperatures at military power reach 1100 deg F along the centerline, and CO values are below 80 ppm. Carbon monoxide concentrations decrease from idle to military power (full power, no <span class="hlt">afterburner</span>), then rise sharply in <span class="hlt">afterburner</span>. The CO peaks shift outward from centerline as do the temperatures due to the radial geometry of the <span class="hlt">afterburner</span> combustion (over 10 percent CO at 2850 deg F).« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/6457776','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/6457776"><span>Radioactive materials <span class="hlt">released</span> from nuclear power plants. Annual report, 1980</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Tichler, J.; Benkovitz, C.</p> <p></p> <p><span class="hlt">Releases</span> of radioactive materials in airborne and liquid effluents from commercial light water reactors during 1980 have been compiled and reported. Data on solid waste shipments as well as selected operating information have been included. This report supplements earlier annual reports issued by the former Atomic <span class="hlt">Energy</span> Commission and the Nuclear Regulatory Commission. The 1980 <span class="hlt">release</span> data are summarized in tabular form. Data covering specific radionuclides are summarized.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/6346354','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/6346354"><span>Radioactive materials <span class="hlt">released</span> from nuclear power plants: Annual report, 1984</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Tichler, J.; Norden, K.; Congemi, J.</p> <p></p> <p><span class="hlt">Releases</span> of radioactive materials in airborne and liquid effluents from commercial light water reactors during 1984 have been compiled and reported. Data on solid waste shipments as well as selected operating information have been included. This report supplements earlier annual reports issued by the former Atomic <span class="hlt">Energy</span> Commission and the Nuclear Regulatory Commission. The 1984 <span class="hlt">release</span> data are summarized in tabular form. Data covering specific radionuclides are summarized.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/5489623','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/5489623"><span>Radioactive materials <span class="hlt">released</span> from nuclear power plants: Annual report, 1985</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Tichler, J.; Norden, K.; Congemi, J.</p> <p></p> <p><span class="hlt">Releases</span> of radioactive materials in airborne and liquid effluents from commercial light water reactors during 1985 have been compiled and reported. Data on solid waste shipments as well as selected operating information have been included. This report supplements earlier annual reports issued by the former Atomic <span class="hlt">Energy</span> Commission and the Nuclear Regulatory Commission. The 1985 <span class="hlt">release</span> data are summarized in tabular form. Data covering specific radionuclides are summarized.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/17514753','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/17514753"><span>Ultrasound enhanced glucose <span class="hlt">release</span> from corn in ethanol plants.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Khanal, Samir Kumar; Montalbo, Melissa; van Leeuwen, J; Srinivasan, Gowrishankar; Grewell, David</p> <p>2007-12-01</p> <p>This work evaluated the use of high power ultrasonic <span class="hlt">energy</span> to treat corn slurry in dry corn milling ethanol plants to enhance liquefaction and saccharification for ethanol production. Corn slurry samples obtained before and after jet cooking were subjected to ultrasonic pretreatment for 20 and 40 s at amplitudes of vibration ranging from 180 to 299 microm(pp) (peak to peak amplitude in microm). The resulting samples were then exposed to enzymes (alpha-amylase and glucoamylase) to convert cornstarch into glucose. A comparison of scanning electron micrographs of raw and sonicated samples showed the development of micropores and the disruption of cell walls in corn mash. The corn particle size declined nearly 20-fold following ultrasonic treatment at high power settings. The glucose <span class="hlt">release</span> rate from sonicated samples increased as much as threefold compared to the control group. The efficiency of ultrasound exceeded 100% in terms of <span class="hlt">energy</span> gain from the sugar <span class="hlt">released</span> over the ultrasonic <span class="hlt">energy</span> supplied. Enzymatic activity was enhanced when the corn slurry was sonicated with simultaneous addition of enzymes. This finding suggests that the ultrasonic <span class="hlt">energy</span> did not degrade or denature the enzymes during the pretreatment.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/18823012','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/18823012"><span>Mechanistic evaluation of alginate-HEC gelisphere compacts for controlled intrastriatal nicotine <span class="hlt">release</span> in Parkinson's disease.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Choonara, Yahya E; Pillay, Viness; Khan, Riaz A; Singh, Neha; du Toit, Lisa C</p> <p>2009-06-01</p> <p>This study focused on elucidating a mechanistic understanding in support of the multiple mechanisms which govern the formation of crosslinked alginate-hydroxyethylcellulose (Alg-HEC) gelispheres intended for the controlled intrastriatal <span class="hlt">release</span> of nicotine as a neuroprotectant in Parkinson's Disease. HEC was incorporated as a reinforcing "protective" colloidal polymer to induce interactions between the free carboxyl groups of alginate with hydroxylated HEC monomers. Gelispheres were compressed within an external poly(lactic-co-glycolic acid) (PLGA) matrix to further prolong the <span class="hlt">release</span> of nicotine. Sol-gel interconversion mechanisms, matrix deformability moduli, matrix fracture <span class="hlt">energies</span> and chemometric models of the associated <span class="hlt">energy</span> paradigms were analyzed for their influence on the mechanism and extent of nicotine <span class="hlt">release</span>. Textural profiling demonstrated higher fracture <span class="hlt">energies</span> (7.94-26.69 x 10(-4) J) and lower deformability moduli (12.24-58.36 N/mm) when gelispheres were cured in 2 M HCl as a postcuring step. Ba(2+) crosslinked gelispheres resulted in superiorly compact matrices with an increase in volume of 201-329% as compared to the Ca(2+) and Zn(2+) crosslinked matrices. The order of matrix compactness was as follows: Zn(2+) < Ca(2+) < Ba(2+). Molecular mechanisms of formation, interaction, conversion, and stability of sol-gel transitions depended on the type of crosslinker, crosslinking time, <span class="hlt">energy</span> transactions, and interactions with molecules of the hydration medium. Ba(2+) crosslinked gelispheres <span class="hlt">released</span> nicotine slower than Ca(2+) and Zn(2+) crosslinked gelispheres due to the higher <span class="hlt">energy</span> requirement for interconversion to sol while the <span class="hlt">energy</span> requirements for Ca(2+) and Zn(2+) was at a lower demand. Ba(2+) crosslinked gelispheres within PLGA matrices therefore retarded nicotine <span class="hlt">release</span> in a pseudo-zero-order manner over 21 days. (c) 2008 Wiley-Liss, Inc.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19800034194&hterms=fusion+energy&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Dfusion%2Benergy','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19800034194&hterms=fusion+energy&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Dfusion%2Benergy"><span>Development of thermal <span class="hlt">energy</span> storage units for spacecraft cryogenic coolers</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Richter, R.; Mahefkey, E. T.</p> <p>1980-01-01</p> <p>Thermal <span class="hlt">Energy</span> Storage Units were developed for storing thermal <span class="hlt">energy</span> required for operating Vuilleumier cryogenic space coolers. In the course of the development work the thermal characteristics of thermal <span class="hlt">energy</span> storage material was investigated. By three distinctly different methods it was established that ternary salts did not <span class="hlt">release</span> fusion <span class="hlt">energy</span> as determined by ideality at the melting point of the eutectic salt. Phase change <span class="hlt">energy</span> was <span class="hlt">released</span> over a relatively wide range of temperature with a large change in volume. This strongly affects the amount of thermal <span class="hlt">energy</span> that is available to the Vuilleumier cryogenic cooler at its operating temperature range and the amount of thermal <span class="hlt">energy</span> that can be stored and <span class="hlt">released</span> during a single storage cycle.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/25087974','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25087974"><span>Sustained <span class="hlt">release</span> carrier for adenosine triphosphate as signaling molecule.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Wischke, Christian; Weigel, Judith; Bulavina, Larisa; Lendlein, Andreas</p> <p>2014-12-10</p> <p>Adenosine triphosphate (ATP) is a molecule with a fascinating variety of intracellular and extracellular biological functions that go far beyond <span class="hlt">energy</span> metabolism. Due to its limited passive diffusion through biological membranes, controlled <span class="hlt">release</span> systems may allow to interact with ATP-mediated extracellular processes. In this study, two <span class="hlt">release</span> systems were explored to evaluate the capacity for either long-term or short-term <span class="hlt">release</span>: (i) Poly[(rac-lactide)-co-glycolide] (PLGA) implant rods were capable of ATP <span class="hlt">release</span> over days to weeks, depending on the PLGA molecular weight and end-group capping, but were also associated with partial hydrolytic degradation of ATP to ADP and AMP, but not adenosine. (ii) Thermosensitive methylcellulose hydrogels with a gelation occurring at body temperature allowed combining adjustable loading levels and the capacity for injection, with injection forces less than 50N even for small 27G needles. Finally, a first in vitro study illustrated purinergic-triggered response of primary murine microglia to ATP <span class="hlt">released</span> from hydrogels, demonstrating the potential relevance for biomedical applications. Copyright © 2014 Elsevier B.V. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017ApSS..407..137K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017ApSS..407..137K"><span>Rapid fabrication of superhydrophobic Al/Fe2O3 nanothermite film with excellent <span class="hlt">energy-release</span> characteristics and long-term storage stability</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ke, Xiang; Zhou, Xiang; Hao, Gaozi; Xiao, Lei; Liu, Jie; Jiang, Wei</p> <p>2017-06-01</p> <p>One of the challenges for the application of energetic materials is their <span class="hlt">energy</span>-retaining capabilities after long-term storage. In this study, we report a facile method to fabricate superhydrophobic Al/Fe2O3 nanothermite film by combining electrophoretic deposition and surface modification technologies. Different concentrations of dispersion solvents and additives are investigated to optimize the deposition parameters. Meanwhile, the dependence of deposition rates on nanoparticle concentrations is also studied. The surface morphology and chemical composition are characterized by field-emission scanning electron microscopy, X-ray diffraction, X-ray <span class="hlt">energy</span>-dispersive spectroscopy, and X-ray photoelectron spectroscopy. A static contact angles as high as 156° shows the superhydrophobicity of the nanothermite film. Natural and accelerated aging tests are performed and the thermal behavior is analyzed. Thermal analysis shows that the surface modification contributes to significantly improved <span class="hlt">energy-release</span> characteristics for both fresh and aged samples, which is supposed to be attributed to the preignition reaction between Al2O3 shell and FAS-17. Superhydrophobic Al/Fe2O3 nanothermite film exhibits excellent long-time storage stability with 83.4% of <span class="hlt">energy</span> left in natural aging test and 60.5% in accelerated aging test. This study is instructive to the practical applications of nanothermites, especially in highly humid environment.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013RMRE...46..859Y','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013RMRE...46..859Y"><span>Microseism Induced by Transient <span class="hlt">Release</span> of In Situ Stress During Deep Rock Mass Excavation by Blasting</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Yang, Jianhua; Lu, Wenbo; Chen, Ming; Yan, Peng; Zhou, Chuangbing</p> <p>2013-07-01</p> <p>During deep rock mass excavation with the method of drill and blast, accompanying the secession of rock fragments and the formation of a new free surface, in situ stress on this boundary is suddenly <span class="hlt">released</span> within several milliseconds, which is termed the transient <span class="hlt">release</span> of in situ stress. In this process, enormous strain <span class="hlt">energy</span> around the excavation face is instantly <span class="hlt">released</span> in the form of kinetic <span class="hlt">energy</span> and it inevitably induces microseismic events in surrounding rock masses. Thus, blasting excavation-induced microseismic vibrations in high-stress rock masses are attributed to the combined action of explosion and the transient <span class="hlt">release</span> of in situ stress. The intensity of stress <span class="hlt">release</span>-induced microseisms, which depends mainly on the magnitude of the in situ stress and the dimension of the excavation face, is comparable to that of explosion-induced vibrations. With the methods of time-<span class="hlt">energy</span> density analysis, amplitude spectrum analysis, and finite impulse response (FIR) digital filter, microseismic vibrations induced by the transient <span class="hlt">release</span> of in situ stress were identified and separated from recorded microseismic signals during a blast of deep rock masses in the Pubugou Hydropower Station. The results show that the low-frequency component in the microseismic records results mainly from the transient <span class="hlt">release</span> of in situ stress, while the high-frequency component originates primarily from explosion. In addition, a numerical simulation was conducted to demonstrate the occurrence of microseismic events by the transient <span class="hlt">release</span> of in situ stress, and the results seem to have confirmed fairly well the separated vibrations from microseismic records.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28069223','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28069223"><span>Sustained <span class="hlt">release</span> formulations of citronella oil nanoemulsion using cavitational techniques.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Agrawal, Naveen; Maddikeri, Ganesh L; Pandit, Aniruddha B</p> <p>2017-05-01</p> <p>Nanoemulsion synthesis has proven to be an effective way for transportation of immobile, insoluble bioactive compounds. Citronella Oil (lemongrass oil), a natural plant extract, can be used as a mosquito repellent and has less harmful effects compared to its available market counterpart DEET (N, N-Diethyl-meta-toluamide). Nanoemulsion of citronella oil in water was prepared using cavitation-assisted techniques while investigating the effect of system parameters like HLB (Hydrophilic Lipophilic Balance), surfactant concentration, input <span class="hlt">energy</span> density and mode of power input on emulsion quality. The present work also examines the effect of emulsification on <span class="hlt">release</span> rate to understand the relationship between droplet size and the <span class="hlt">release</span> rate. Minimum droplet size (60nm) of the emulsion was obtained at HLB of 14, S/O 1 ratio of 1.0, ultrasound amplitude of 50% and irradiation time of 5min. This study revealed that hydrodynamic cavitation-assisted emulsification is more <span class="hlt">energy</span> efficient compared to ultrasonic emulsification. It was also found that the <span class="hlt">release</span> rate of nanoemulsion enhanced as the droplet size of emulsion reduced. Copyright © 2016 Elsevier B.V. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2002JNuM..307.1418O','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2002JNuM..307.1418O"><span>Hydrogen <span class="hlt">release</span> from 800 MeV proton-irradiated tungsten</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Oliver, B. M.; Venhaus, T. J.; Causey, R. A.; Garner, F. A.; Maloy, S. A.</p> <p>2002-12-01</p> <p>Tungsten irradiated in spallation neutron sources, such as those proposed for the accelerator production of tritium (APT) project, will contain large quantities of generated helium and hydrogen gas. Tungsten used in proposed fusion reactors will also be exposed to neutrons, and the generated protium will be accompanied by deuterium and tritium diffusing in from the plasma-facing surface. The <span class="hlt">release</span> kinetics of these gases during various off-normal scenarios involving loss of coolant and after heat-induced rises in temperature are of particular interest for both applications. To determine the <span class="hlt">release</span> kinetics of hydrogen from tungsten, tungsten rods irradiated with 800 MeV protons in the Los Alamos Neutron Science Center (LANSCE) to high exposures as part of the APT project have been examined. Hydrogen evolution from the tungsten has been measured using a dedicated mass-spectrometer system by subjecting the specimens to an essentially linear temperature ramp from ˜300 to ˜1500 K. <span class="hlt">Release</span> profiles are compared with predictions obtained using the Tritium Migration Analysis Program (TMAP4). The measurements show that for high proton doses, the majority of the hydrogen is <span class="hlt">released</span> gradually, starting at about 900 K and reaching a maximum at about 1400 K, where it drops fairly rapidly. Comparisons with TMAP show quite reasonable agreement using a trap <span class="hlt">energy</span> of 1.4 eV and a trap density of ˜7%. There is a small additional <span class="hlt">release</span> fraction occurring at ˜550 K, which is believed to be associated with low-<span class="hlt">energy</span> trapping at or near the surface, and, therefore, was not included in the bulk TMAP model.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li class="active"><span>16</span></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_16 --> <div id="page_17" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li class="active"><span>17</span></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="321"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2004PApGe.161.2405Y','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2004PApGe.161.2405Y"><span>Load-Unload Response Ratio (LURR), Accelerating Moment/<span class="hlt">Energy</span> <span class="hlt">Release</span> (AM/ER) and State Vector Saltation as Precursors to Failure of Rock Specimens</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Yin, Xiang-Chu; Yu, Huai-Zhong; Kukshenko, Victor; Xu, Zhao-Yong; Wu, Zhishen; Li, Min; Peng, Keyin; Elizarov, Surgey; Li, Qi</p> <p>2004-12-01</p> <p>In order to verify some precursors such as LURR (Load/Unload Response Ratio) and AER (Accelerating <span class="hlt">Energy</span> <span class="hlt">Release</span>) before large earthquakes or macro-fracture in heterogeneous brittle media, four acoustic emission experiments involving large rock specimens under tri-axial stress, have been conducted. The specimens were loaded in two ways: monotonous or cycling. The experimental results confirm that LURR and AER are precursors of macro-fracture in brittle media. A new measure called the state vector has been proposed to describe the damage evolution of loaded rock specimens.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/19905150','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/19905150"><span>Binding free <span class="hlt">energy</span> and counterion <span class="hlt">release</span> for adsorption of the antimicrobial peptide lactoferricin B on a POPG membrane.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Tolokh, Igor S; Vivcharuk, Victor; Tomberli, Bruno; Gray, C G</p> <p>2009-09-01</p> <p>Molecular dynamics (MD) simulations are used to study the interaction of an anionic palmitoyl-oleoyl-phosphatidylglycerol (POPG) bilayer with the cationic antimicrobial peptide bovine lactoferricin (LFCinB) in a 100 mM NaCl solution at 310 K. The interaction of LFCinB with a POPG bilayer is employed as a model system for studying the details of membrane adsorption selectivity of cationic antimicrobial peptides. Seventy eight 4 ns MD production run trajectories of the equilibrated system, with six restrained orientations of LFCinB at 13 different separations from the POPG membrane, are generated to determine the free <span class="hlt">energy</span> profile for the peptide as a function of the distance between LFCinB and the membrane surface. To calculate the profile for this relatively large system, a variant of constrained MD and thermodynamic integration is used. A simplified method for relating the free <span class="hlt">energy</span> profile to the LFCinB-POPG membrane binding constant is employed to predict a free <span class="hlt">energy</span> of adsorption of -5.4+/-1.3 kcal/mol and a corresponding maximum adsorption binding force of about 58 pN. We analyze the results using Poisson-Boltzmann theory. We find the peptide-membrane attraction to be dominated by the entropy increase due to the <span class="hlt">release</span> of counterions and polarized water from the region between the charged membrane and peptide, as the two approach each other. We contrast these results with those found earlier for adsorption of LFCinB on the mammalianlike palmitoyl-oleoyl-phosphatidylcholine membrane.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009PhRvE..80c1911T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009PhRvE..80c1911T"><span>Binding free <span class="hlt">energy</span> and counterion <span class="hlt">release</span> for adsorption of the antimicrobial peptide lactoferricin B on a POPG membrane</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Tolokh, Igor S.; Vivcharuk, Victor; Tomberli, Bruno; Gray, C. G.</p> <p>2009-09-01</p> <p>Molecular dynamics (MD) simulations are used to study the interaction of an anionic palmitoyl-oleoyl-phosphatidylglycerol (POPG) bilayer with the cationic antimicrobial peptide bovine lactoferricin (LFCinB) in a 100 mM NaCl solution at 310 K. The interaction of LFCinB with a POPG bilayer is employed as a model system for studying the details of membrane adsorption selectivity of cationic antimicrobial peptides. Seventy eight 4 ns MD production run trajectories of the equilibrated system, with six restrained orientations of LFCinB at 13 different separations from the POPG membrane, are generated to determine the free <span class="hlt">energy</span> profile for the peptide as a function of the distance between LFCinB and the membrane surface. To calculate the profile for this relatively large system, a variant of constrained MD and thermodynamic integration is used. A simplified method for relating the free <span class="hlt">energy</span> profile to the LFCinB-POPG membrane binding constant is employed to predict a free <span class="hlt">energy</span> of adsorption of -5.4±1.3kcal/mol and a corresponding maximum adsorption binding force of about 58 pN. We analyze the results using Poisson-Boltzmann theory. We find the peptide-membrane attraction to be dominated by the entropy increase due to the <span class="hlt">release</span> of counterions and polarized water from the region between the charged membrane and peptide, as the two approach each other. We contrast these results with those found earlier for adsorption of LFCinB on the mammalianlike palmitoyl-oleoyl-phosphatidylcholine membrane.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/ADA563470','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA563470"><span><span class="hlt">Energy</span> & Energetics</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>2012-06-22</p> <p>mechanical and structural failure and decomposition in ultra-fast time regimes. Our research teams are exploring novel ways to convert mechanical ...<span class="hlt">energy</span> to thermal <span class="hlt">energy</span> by examining initiation mechanisms , multi-phase combustion, detonation and the mechanisms that lead to the <span class="hlt">release</span> of <span class="hlt">energy</span>...understanding of the mechanisms of structural stability by doping Fe in LiCoPO4 and effectiveness of HFiP in stopping further oxidation of electrolytes are</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.eia.gov/consumption/commercial/reports/2012/energyusage/','EIAPUBS'); return false;" href="https://www.eia.gov/consumption/commercial/reports/2012/energyusage/"><span>2012 Commercial Buildings <span class="hlt">Energy</span> Consumption Survey: <span class="hlt">Energy</span> Usage Summary</span></a></p> <p><a target="_blank" href="http://www.eia.doe.gov/reports/">EIA Publications</a></p> <p></p> <p>2016-01-01</p> <p>EIA has <span class="hlt">released</span> summary tables providing <span class="hlt">energy</span> consumption estimates from the 2012 CBECS. The data show that despite a 14% increase in total buildings and a 22% increase in total floorspace since 2003, <span class="hlt">energy</span> use in the estimated 5.6 million U.S. commercial buildings was up just 7% during the same period.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFMMR41B2704B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFMMR41B2704B"><span>Real-time noble gas <span class="hlt">release</span> signaling rock deformation</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bauer, S. J.; Gardner, W. P.; Lee, H.</p> <p>2016-12-01</p> <p>We present empirical results/relationships of rock strain, microfracture density, acoustic emissions, and noble gas <span class="hlt">release</span> from laboratory triaxial experiments for a granite and basalt. Noble gases are contained in most crustal rock at inter/intra granular sites, their <span class="hlt">release</span> during natural and manmade stress and strain changes represents a signal of brittle/semi brittle deformation. The gas composition depends on lithology, geologic history and age, fluids present, and uranium, thorium and potassium-40 concentrations in the rocks that affect radiogenic noble gases (helium, argon) production. Noble gas emission and its relationship to crustal processes have been studied, including correlations to tectonic velocities and qualitative estimates of deep permeability from surface measurements, finger prints of nuclear weapon detonation, and as potential precursory signals to earthquakes attributed to gas <span class="hlt">release</span> due to pre-seismic stress, dilatancy and/or rock fracturing. Helium emission has been shown as a precursor of volcanic activity. Real-time noble gas <span class="hlt">release</span> is observed using an experimental system utilizing mass spectrometers to measure gases <span class="hlt">released</span> during triaxial rock deformation. Noble gas <span class="hlt">release</span> is shown to represent a sensitive precursor signal of rock deformation by relating real-time noble gas <span class="hlt">release</span> to stress-strain state changes and acoustic emissions. We propose using noble gas <span class="hlt">release</span> to also signal rock deformation in boreholes, mines and nuclear waste repositories. We postulate each rock exhibits a gas <span class="hlt">release</span> signature which is microstructure, stress/strain state, and or permanent deformation dependent. Such relationships, when calibrated, may be used to sense rock deformation and then develop predictive models. Sandia National Laboratories is a multi-program laboratory managed and operated by Sandia Corporation, a wholly owned subsidiary of Lockheed Martin Corp., for the US Dept. of <span class="hlt">Energy</span>'s National Nuclear Security Administration under</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1990RuCRv..59..989M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1990RuCRv..59..989M"><span>Procedures for making gaseous industrial waste safe</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Matros, Yu Sh; Noskov, Aleksandr S.</p> <p>1990-10-01</p> <p>The application of various methods (adsorption, absorption, thermal <span class="hlt">afterburning</span>, catalytic purification, and others) for the removal of sulphur and nitrogen oxides, toxic organic compounds, hydrogen sulphide, and carbon monoxide from industrial waste gases is described. Much attention is devoted to the catalytic procedure for making the gases safe using an <span class="hlt">energy</span> collecting non-stationary method (reversible process). The advantages and limitations of various gas purification methods are considered. The bibliography includes 279 references.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=1302732','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=1302732"><span>Forces and Pressures in DNA Packaging and <span class="hlt">Release</span> from Viral Capsids</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Tzlil, Shelly; Kindt, James T.; Gelbart, William M.; Ben-Shaul, Avinoam</p> <p>2003-01-01</p> <p>In a previous communication (Kindt et al., 2001) we reported preliminary results of Brownian dynamics simulation and analytical theory which address the packaging and ejection forces involving DNA in bacteriophage capsids. In the present work we provide a systematic formulation of the underlying theory, featuring the energetic and structural aspects of the strongly confined DNA. The free <span class="hlt">energy</span> of the DNA chain is expressed as a sum of contributions from its encapsidated and <span class="hlt">released</span> portions, each expressed as a sum of bending and interstrand <span class="hlt">energies</span> but subjected to different boundary conditions. The equilibrium structure and <span class="hlt">energy</span> of the capsid-confined and free chain portions are determined, for each ejected length, by variational minimization of the free <span class="hlt">energy</span> with respect to their shape profiles and interaxial spacings. Numerical results are derived for a model system mimicking the λ-phage. We find that the fully encapsidated genome is highly compressed and strongly bent, forming a spool-like condensate, storing enormous elastic <span class="hlt">energy</span>. The elastic stress is rapidly <span class="hlt">released</span> during the first stage of DNA injection, indicating the large force (tens of pico Newtons) needed to complete the (inverse) loading process. The second injection stage sets in when ∼1/3 of the genome has been <span class="hlt">released</span>, and the interaxial distance has nearly reached its equilibrium value (corresponding to that of a relaxed torus in solution); concomitantly the encapsidated genome begins a gradual morphological transformation from a spool to a torus. We also calculate the loading force, the average pressure on the capsid's walls, and the anisotropic pressure profile within the capsid. The results are interpreted in terms of the (competing) bending and interaction components of the packing <span class="hlt">energy</span>, and are shown to be in good agreement with available experimental data. PMID:12609865</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/12609865','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/12609865"><span>Forces and pressures in DNA packaging and <span class="hlt">release</span> from viral capsids.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Tzlil, Shelly; Kindt, James T; Gelbart, William M; Ben-Shaul, Avinoam</p> <p>2003-03-01</p> <p>In a previous communication (Kindt et al., 2001) we reported preliminary results of Brownian dynamics simulation and analytical theory which address the packaging and ejection forces involving DNA in bacteriophage capsids. In the present work we provide a systematic formulation of the underlying theory, featuring the energetic and structural aspects of the strongly confined DNA. The free <span class="hlt">energy</span> of the DNA chain is expressed as a sum of contributions from its encapsidated and <span class="hlt">released</span> portions, each expressed as a sum of bending and interstrand <span class="hlt">energies</span> but subjected to different boundary conditions. The equilibrium structure and <span class="hlt">energy</span> of the capsid-confined and free chain portions are determined, for each ejected length, by variational minimization of the free <span class="hlt">energy</span> with respect to their shape profiles and interaxial spacings. Numerical results are derived for a model system mimicking the lambda-phage. We find that the fully encapsidated genome is highly compressed and strongly bent, forming a spool-like condensate, storing enormous elastic <span class="hlt">energy</span>. The elastic stress is rapidly <span class="hlt">released</span> during the first stage of DNA injection, indicating the large force (tens of pico Newtons) needed to complete the (inverse) loading process. The second injection stage sets in when approximately 1/3 of the genome has been <span class="hlt">released</span>, and the interaxial distance has nearly reached its equilibrium value (corresponding to that of a relaxed torus in solution); concomitantly the encapsidated genome begins a gradual morphological transformation from a spool to a torus. We also calculate the loading force, the average pressure on the capsid's walls, and the anisotropic pressure profile within the capsid. The results are interpreted in terms of the (competing) bending and interaction components of the packing <span class="hlt">energy</span>, and are shown to be in good agreement with available experimental data.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29944181','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29944181"><span>Photocontrol of Drug <span class="hlt">Release</span> from Supramolecular Hydrogels with Green Light.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Karcher, Johannes; Pianowski, Zbigniew</p> <p>2018-06-26</p> <p>Photoresponsive smart materials transform light <span class="hlt">energy</span> into sophisticated functions. They find increasing biomedical applications in light-induced drug <span class="hlt">release</span> and photopharmacology, as they can locally provide the desired therapeutic effect due to precise spatiotemporal dosage control. However, the majority of reported studies rely on cytotoxic UV light that poorly penetrates tissues. Here we report the first drug-<span class="hlt">releasing</span> system based on photochromic low molecular weight supramolecular hydrogels that is triggered with visible light. We demonstrated green-light-induced <span class="hlt">release</span> of structurally unmodified antibiotic, anticancer, and anti-inflammatory drugs under physiological conditions. Using the antibiotic-loaded gel, we selectively inhibited bacterial growth with green light. © 2018 WILEY-VCH Verlag GmbH & Co. KGaA, Weinheim.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/864314','DOE-PATENT-XML'); return false;" href="https://www.osti.gov/servlets/purl/864314"><span>Method of generating electricity using an endothermic coal gasifier and MHD generator</span></a></p> <p><a target="_blank" href="http://www.osti.gov/doepatents">DOEpatents</a></p> <p>Marchant, David D.; Lytle, John M.</p> <p>1982-01-01</p> <p>A system and method of generating electrical power wherein a mixture of carbonaceous material and water is heated to initiate and sustain the endothermic reaction of carbon and water thereby providing a gasified stream containing carbon monoxide, hydrogen and nitrogen and waste streams of hydrogen sulfide and ash. The gasified stream and an ionizing seed material and pressurized air from a preheater go to a burner for producing ionized combustion gases having a temperature of about 5000.degree. to about 6000.degree. F. which are accelerated to a velocity of about 1000 meters per second and passed through an MHD generator to generate DC power and thereafter through a diffuser to reduce the velocity. The gases from the diffuser go to an <span class="hlt">afterburner</span> and from there in heat exchange relationship with the gasifier to provide heat to sustain the endothermic reaction of carbon and water and with the preheater to preheat the air prior to combustion with the gasified stream. <span class="hlt">Energy</span> from the <span class="hlt">afterburner</span> can also be used to energize other parts of the system.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMMR43D0492B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMMR43D0492B"><span>Noble Gas <span class="hlt">Release</span> Signal as a Precursor to Fracture</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bauer, S. J.; Lee, H.; Gardner, W. P.</p> <p>2017-12-01</p> <p>We present empirical results of rock strain, microfracturing, acoustic emissions, and noble gas <span class="hlt">release</span> from laboratory triaxial experiments for a granite, basalt, shale and bedded rock salt. Noble gases are <span class="hlt">released</span> and measured real-time during deformation using mass spectrometry. The gas <span class="hlt">release</span> represents a precursive signal to macrofracture. Gas <span class="hlt">release</span> is associated with increased acoustic emissions indicating that microfracturing is required to <span class="hlt">release</span> gas and create pathways for the gas to be sensed. The gas <span class="hlt">released</span> depends on initial gas content, pore structure and its evolution during deformation, the deformation amount, matrix permeability, deformation style and the stress/strain history. Gases are <span class="hlt">released</span> from inter and intracrystalline sites; <span class="hlt">release</span> rate increases as strain and microfracturing increases. The gas composition depends on lithology, geologic history and age, fluids present, and radioisotope concentrations that affect radiogenic noble gas isotope (e.g. 4He,40Ar) production. Noble gas emission and its relationship to crustal processes such as seismicity and volcanism, tectonic velocities, qualitative estimates of deep permeability, age dating of groundwater, and a signature of nuclear weapon detonation. Our result show that mechanical deformation of crustal materials is an important process controlling gas <span class="hlt">release</span> from rocks and minerals, and should be considered in techniques which utilize gas <span class="hlt">release</span> and/or accumulation. We propose using noble gas <span class="hlt">release</span> to signal rock deformation in boreholes, mines and waste repositories. We postulate each rock exhibits a gas <span class="hlt">release</span> signature which is microstructure, stress, strain, and/or permanent deformation dependent. Calibration of such relationships, for example relating gas <span class="hlt">release</span> per rock unit volume to strain may be used to quantify rock deformation and develop predictive models.Sandia National Laboratories is a multimission laboratory managed and operated by National Technology and</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19930053293&hterms=barium&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3Dbarium','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19930053293&hterms=barium&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3Dbarium"><span>Measurements of the time constant for steady ionization in shaped-charge barium <span class="hlt">releases</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Hoch, Edward L.; Hallinan, Thomas J.</p> <p>1993-01-01</p> <p>Quantitative measurements of three solar illuminated shaped-charge barium <span class="hlt">releases</span> injected at small angles to the magnetic field were made using a calibrated color television camera. Two of the <span class="hlt">releases</span> were from 1989. The third <span class="hlt">release</span>, a reanalysis of an event included in Hallinan's 1988 study of three 1986 <span class="hlt">releases</span>, was included to provide continuity between the two studies. Time constants for ionization, measured during the first 25 s of each <span class="hlt">release</span>, were found to vary considerably. The two 1989 time constants differed substantially, and both were significantly less than any of the 1986 time constants. On the basis of this variability, we conclude that the two 1989 <span class="hlt">releases</span> showed evidence of continuous nonsolar ionization. One <span class="hlt">release</span> showed nonsolar ionization which could not he attributed to Alfven's critical ionization velocity process, which requires a component of velocity perpendicular to the magnetic field providing a perpendicular <span class="hlt">energy</span> greater than the ionization potential.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28756281','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28756281"><span>Quantifying the mode II critical strain <span class="hlt">energy</span> <span class="hlt">release</span> rate of borate bioactive glass coatings on Ti6Al4V substrates.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Matinmanesh, A; Li, Y; Clarkin, O; Zalzal, P; Schemitsch, E H; Towler, M R; Papini, M</p> <p>2017-11-01</p> <p>Bioactive glasses have been used as coatings for biomedical implants because they can be formulated to promote osseointegration, antibacterial behavior, bone formation, and tissue healing through the incorporation and subsequent <span class="hlt">release</span> of certain ions. However, shear loading on coated implants has been reported to cause the delamination and loosening of such coatings. This work uses a recently developed fracture mechanics testing methodology to quantify the critical strain <span class="hlt">energy</span> <span class="hlt">release</span> rate under nearly pure mode II conditions, G IIC , of a series of borate-based glass coating/Ti6Al4V alloy substrate systems. Incorporating increasing amounts of SrCO 3 in the glass composition was found to increase the G IIC almost twofold, from 25.3 to 46.9J/m 2 . The magnitude and distribution of residual stresses in the coating were quantified, and it was found that the residual stresses in all cases distributed uniformly over the cross section of the coating. The crack was driven towards, but not into, the glass/Ti6Al4V substrate interface due to the shear loading. This implied that the interface had a higher fracture toughness than the coating itself. Copyright © 2017 Elsevier Ltd. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3339652','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3339652"><span>Role of GABA <span class="hlt">Release</span> From Leptin Receptor-Expressing Neurons in Body Weight Regulation</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Xu, Yuanzhong; O'Brien, William G.; Lee, Cheng-Chi; Myers, Martin G.</p> <p>2012-01-01</p> <p>It is well established that leptin regulates <span class="hlt">energy</span> balance largely through isoform B leptin receptor-expressing neurons (LepR neurons) in the brain and that leptin activates one subset of LepR neurons (leptin-excited neurons) while inhibiting the other (leptin-inhibited neurons). However, the neurotransmitters <span class="hlt">released</span> from LepR neurons that mediate leptin action in the brain are not well understood. Previous results demonstrate that leptin mainly acts on γ-aminobutyric acid (GABA)ergic neurons to reduce body weight, and that leptin activates proopiomelanocortin neuron activity by reducing GABA <span class="hlt">release</span> onto these neurons, suggesting a body weight-promoting role for GABA <span class="hlt">released</span> from leptin-inhibited neurons. To directly examine the role of GABA <span class="hlt">release</span> from LepR neurons in body weight regulation, mice with disruption of GABA <span class="hlt">release</span> specifically from LepR neurons were generated by deletion of vesicular GABA transporter in LepR neurons. Interestingly, these mice developed mild obesity on chow diet and were sensitive to diet-induced obesity, which were associated with higher food intake and lower <span class="hlt">energy</span> expenditure. Moreover, these mice showed blunted responses in both food intake and body weight to acute leptin administration. These results demonstrate that GABA plays an important role in mediating leptin action. In combination with the previous studies that leptin reduces GABA <span class="hlt">release</span> onto proopiomelanocortin neurons through leptin-inhibited neurons and that disruption of GABA <span class="hlt">release</span> from agouti gene-related protein neurons, one subset of LepR-inhibited neurons, leads to a lean phenotype, our results suggest that, under our experimental conditions, GABA <span class="hlt">release</span> from leptin-excited neuron dominates over leptin-inhibited ones. PMID:22334723</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3075550','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3075550"><span>INSECT FAT BODY: <span class="hlt">ENERGY</span>, METABOLISM, AND REGULATION</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Arrese, Estela L.; Soulages, Jose L.</p> <p>2010-01-01</p> <p>The fat body plays major roles in the life of insects. It is a dynamic tissue involved in multiple metabolic functions. One of these functions is to store and <span class="hlt">release</span> <span class="hlt">energy</span> in response to the <span class="hlt">energy</span> demands of the insect. Insects store <span class="hlt">energy</span> reserves in the form of glycogen and triglycerides in the adipocytes, the main fat body cell. Insect adipocytes can store a great amount of lipid reserves as cytoplasmic lipid droplets. Lipid metabolism is essential for growth and reproduction and provides <span class="hlt">energy</span> needed during extended nonfeeding periods. This review focuses on <span class="hlt">energy</span> storage and <span class="hlt">release</span> and summarizes current understanding of the mechanisms underlying these processes in insects. PMID:19725772</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1996NIMPB.126..170L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1996NIMPB.126..170L"><span><span class="hlt">Release</span> from ISOLDE molten metal targets under pulsed proton beam conditions</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lettry, J.; Catherall, R.; Cyvoct, G.; Evensen, A. H. M.; Lindroos, M.; Jonsson, O. C.; Kugler, E.; Schindl, K.; Ravn, H.; Wildner, E.; Drumm, P.; Obert, J.; Putaux, J. C.; Sauvage, J.</p> <p>1996-04-01</p> <p>By moving the ISOLDE mass separators from the 600 MeV Synchrocyclotron (SC) to the 1 GeV Proton-Synchrotron-Booster (PS) the instantaneous <span class="hlt">energy</span> density of the proton beam went up by 3 orders of magnitude. The developments of the molten metal target units and the optimization of the PS proton beam to cope with the effects of the thermal shocks induced by the proton beam are described. The <span class="hlt">energy</span> density of the PS proton beam was reduced by spatial defocusing and time staggered extraction of the four PS-accelerators. The <span class="hlt">release</span> from lanthanum, lead and tin targets is discussed for different settings of the proton beam and compared to the <span class="hlt">release</span> observed at ISOLDE-SC. The yields of Hg isotopes are presented.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015JPhCS.664b2006B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015JPhCS.664b2006B"><span>The ALICE Software <span class="hlt">Release</span> Validation cluster</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Berzano, D.; Krzewicki, M.</p> <p>2015-12-01</p> <p>One of the most important steps of software lifecycle is Quality Assurance: this process comprehends both automatic tests and manual reviews, and all of them must pass successfully before the software is approved for production. Some tests, such as source code static analysis, are executed on a single dedicated service: in High <span class="hlt">Energy</span> Physics, a full simulation and reconstruction chain on a distributed computing environment, backed with a sample “golden” dataset, is also necessary for the quality sign off. The ALICE experiment uses dedicated and virtualized computing infrastructures for the <span class="hlt">Release</span> Validation in order not to taint the production environment (i.e. CVMFS and the Grid) with non-validated software and validation jobs: the ALICE <span class="hlt">Release</span> Validation cluster is a disposable virtual cluster appliance based on CernVM and the Virtual Analysis Facility, capable of deploying on demand, and with a single command, a dedicated virtual HTCondor cluster with an automatically scalable number of virtual workers on any cloud supporting the standard EC2 interface. Input and output data are externally stored on EOS, and a dedicated CVMFS service is used to provide the software to be validated. We will show how the <span class="hlt">Release</span> Validation Cluster deployment and disposal are completely transparent for the <span class="hlt">Release</span> Manager, who simply triggers the validation from the ALICE build system's web interface. CernVM 3, based entirely on CVMFS, permits to boot any snapshot of the operating system in time: we will show how this allows us to certify each ALICE software <span class="hlt">release</span> for an exact CernVM snapshot, addressing the problem of Long Term Data Preservation by ensuring a consistent environment for software execution and data reprocessing in the future.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/6453450-modeling-energy-release-systems-from-otec-plants','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/6453450-modeling-energy-release-systems-from-otec-plants"><span>Modeling of <span class="hlt">energy</span> <span class="hlt">release</span> systems from OTEC plants</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Denno, K.</p> <p>1983-12-01</p> <p>This paper presents analytical scope for the controlling functions of OTEC operation for the ultimate production of sizable bulk ..delta..T as well as H/sub 2/, N/sub 2/ and NH/sub 3/. The controlling parametric functions include the oceanic and ammonia Reynolds numbers which depend implicitly and explicitly on the ocean water velocity, mass-volume, duration of ..delta..T extraction, and the inlet and outlet water temperatures internally and externally. Solutions for the oceanic and amonia Reynolds numbers have been established setting the deciding constraints on water velocity, boundary temperatures, mass-volume as well as other plant parameters. Linkage between OTEC plant and other conventionalmore » as well as advanced <span class="hlt">energy</span> systems has been expressed in terms of a set of balance and coordinating <span class="hlt">energy</span> equations.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/CFR-2011-title10-vol1/pdf/CFR-2011-title10-vol1-sec50-83.pdf','CFR2011'); return false;" href="https://www.gpo.gov/fdsys/pkg/CFR-2011-title10-vol1/pdf/CFR-2011-title10-vol1-sec50-83.pdf"><span>10 CFR 50.83 - <span class="hlt">Release</span> of part of a power reactor facility or site for unrestricted use.</span></a></p> <p><a target="_blank" href="http://www.gpo.gov/fdsys/browse/collectionCfr.action?selectedYearFrom=2011&page.go=Go">Code of Federal Regulations, 2011 CFR</a></p> <p></p> <p>2011-01-01</p> <p>... 10 <span class="hlt">Energy</span> 1 2011-01-01 2011-01-01 false <span class="hlt">Release</span> of part of a power reactor facility or site for... of a power reactor facility or site for unrestricted use. (a) Prior written NRC approval is required... <span class="hlt">release</span>. Nuclear power reactor licensees seeking NRC approval shall— (1) Evaluate the effect of <span class="hlt">releasing</span>...</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li class="active"><span>17</span></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_17 --> <div id="page_18" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li class="active"><span>18</span></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="341"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/CFR-2010-title10-vol1/pdf/CFR-2010-title10-vol1-sec50-83.pdf','CFR'); return false;" href="https://www.gpo.gov/fdsys/pkg/CFR-2010-title10-vol1/pdf/CFR-2010-title10-vol1-sec50-83.pdf"><span>10 CFR 50.83 - <span class="hlt">Release</span> of part of a power reactor facility or site for unrestricted use.</span></a></p> <p><a target="_blank" href="http://www.gpo.gov/fdsys/browse/collectionCfr.action?selectedYearFrom=2010&page.go=Go">Code of Federal Regulations, 2010 CFR</a></p> <p></p> <p>2010-01-01</p> <p>... 10 <span class="hlt">Energy</span> 1 2010-01-01 2010-01-01 false <span class="hlt">Release</span> of part of a power reactor facility or site for... of a power reactor facility or site for unrestricted use. (a) Prior written NRC approval is required... <span class="hlt">release</span>. Nuclear power reactor licensees seeking NRC approval shall— (1) Evaluate the effect of <span class="hlt">releasing</span>...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/23708563','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/23708563"><span>Potential <span class="hlt">release</span> scenarios for carbon nanotubes used in composites.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Nowack, Bernd; David, Raymond M; Fissan, Heinz; Morris, Howard; Shatkin, Jo Anne; Stintz, Michael; Zepp, Richard; Brouwer, Derk</p> <p>2013-09-01</p> <p> exposure. A possibility for significant <span class="hlt">release</span> also exists during recycling operations when the polymers containing CNTs are handled together with other polymers and mainly occupational users would be exposed. It can be concluded that in general, significant <span class="hlt">release</span> of CNTs from products and articles is unlikely except in manufacturing and subsequent processing, tires, recycling, and potentially in textiles. However except for high <span class="hlt">energy</span> machining processes, most likely the resulting exposure for these scenarios will be low and to a non-pristine form of CNTs. Actual exposure studies, which quantify the amount of material <span class="hlt">released</span> should be conducted to provide further evidence for this conclusion. Copyright © 2013 The Authors. Published by Elsevier Ltd.. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/21203885','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/21203885"><span>The effect of toxins on inorganic phosphate <span class="hlt">release</span> during actin polymerization.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Vig, Andrea; Ohmacht, Róbert; Jámbor, Eva; Bugyi, Beáta; Nyitrai, Miklós; Hild, Gábor</p> <p>2011-05-01</p> <p>During the polymerization of actin, hydrolysis of bound ATP occurs in two consecutive steps: chemical cleavage of the high-<span class="hlt">energy</span> nucleotide and slow <span class="hlt">release</span> of the γ-phosphate. In this study the effect of phalloidin and jasplakinolide on the kinetics of P(i) <span class="hlt">release</span> was monitored during the formation of actin filaments. An enzyme-linked assay based spectrophotometric technique was used to follow the liberation of inorganic phosphate. It was verified that jasplakinolide reduced the P(i) <span class="hlt">release</span> in the same way as phalloidin. It was not possible to demonstrate long-range allosteric effects of the toxins by <span class="hlt">release</span> of P(i) from F-actin. The products of ATP hydrolysis were <span class="hlt">released</span> by denaturation of the actin filaments. HPLC analysis of the samples revealed that the ATP in the toxin-bound region was completely hydrolysed into ADP and P(i). The effect of both toxins can be sufficiently explained by local and mechanical blockade of P(i) dissociation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29580414','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29580414"><span>Natural gum-type biopolymers as potential modified nonpolar drug <span class="hlt">release</span> systems.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Salamanca, Constain H; Yarce, Cristhian J; Moreno, Roger A; Prieto, Vanessa; Recalde, Juanita</p> <p>2018-06-01</p> <p>In this work, the relationship between surface properties and drug <span class="hlt">release</span> mechanism from binary composition tablets formed by quetiapine fumarate and biopolymer materials was studied. The biopolymers correspond to xanthan and tragacanth gums, which are projected as modified drug <span class="hlt">release</span> systems. The surface studies were carried out by the sessile drop method, while the surface free <span class="hlt">energy</span> (SFE) was determinate through Young-Dupree and OWRK semi-empirical models. On the other hand, the drug <span class="hlt">release</span> studies were performed by in vitro dissolution tests, where the data were analyzed through kinetic models of zero order, first order, Higuchi, and Korsmeyer-Peppas. The results showed that depending on the type and the proportion of biopolymer, surface properties, and the drug <span class="hlt">release</span> processes are significantly affected, wherein tragacanth gum present a usual erosion mechanism, while xanthan gum describes a swelling mechanism that controls the <span class="hlt">release</span> of the drug. Copyright © 2018 Elsevier Ltd. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19920068569&hterms=Free+energy&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3DFree%2Benergy','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19920068569&hterms=Free+energy&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3DFree%2Benergy"><span>Relationship between wave <span class="hlt">energy</span> and free <span class="hlt">energy</span> from pickup ions in the Comet Halley environment</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Huddleston, D. E.; Johnstone, A. D.</p> <p>1992-01-01</p> <p>The free <span class="hlt">energy</span> available from the implanted heavy ion population at Comet Halley is calculated by assuming that the initial unstable velocity space ring distribution of the ions evolves toward a bispherical shell. Ultimately this free <span class="hlt">energy</span> adds to the turbulence in the solar wind. Upstream and downstream free <span class="hlt">energies</span> are obtained separately for the conditions observed along the Giotto spacecraft trajectory. The results indicate that the waves are mostly upstream propagating in the solar wind frame. The total free <span class="hlt">energy</span> density always exceeds the measured wave <span class="hlt">energy</span> density because, as expected in the nonlinear process of ion scattering, the available <span class="hlt">energy</span> is not all immediately <span class="hlt">released</span>. An estimate of the amount which has been <span class="hlt">released</span> can be obtained from the measured oxygen ion distributions and again it exceeds that observed. The theoretical analysis is extended to calculate the k spectrum of the cometary-ion-generated turbulence.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.loc.gov/pictures/collection/hh/item/ca3243.photos.194678p/','SCIGOV-HHH'); return false;" href="https://www.loc.gov/pictures/collection/hh/item/ca3243.photos.194678p/"><span>16. EAST ELEVATION OF FLOAT HOUSE AND FISH WATER <span class="hlt">RELEASE</span> ...</span></a></p> <p><a target="_blank" href="http://www.loc.gov/pictures/collection/hh/">Library of Congress Historic Buildings Survey, Historic Engineering Record, Historic Landscapes Survey</a></p> <p></p> <p></p> <p>16. EAST ELEVATION OF FLOAT HOUSE AND FISH WATER <span class="hlt">RELEASE</span> OUTLET. PART OF <span class="hlt">ENERGY</span> DISSIPATING BAFFLE PIER SYSTEM IS VISIBLE AT LEFT. - Pit 4 Diversion Dam, Pit River west of State Highway 89, Big Bend, Shasta County, CA</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/8622791','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/8622791"><span>Changes in brain amino acid content induced by hyposmolar stress and <span class="hlt">energy</span> deprivation.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Haugstad, T S; Valø, E T; Langmoen, I A</p> <p>1995-12-01</p> <p>The changes in endogenous amino acids in brain extracellular and intracellular compartments evoked by hyposmotic stress and <span class="hlt">energy</span> deprivation were compared. Tissue content and <span class="hlt">release</span> of ten amino acids were measured simultaneously in rat hippocampal slices by means of high performance liquid chromatography. Hyposmotic stress induced a large <span class="hlt">release</span> of taurine (25568 pmol mg-1 protein), and a smaller <span class="hlt">release</span> of glutamate, accompanied by an inverse change in tissue content. Adding mannitol to correct osmolarity, blocked these changes. <span class="hlt">Energy</span> deprivation caused an increase in the <span class="hlt">release</span> of all amino acids except glutamine. The <span class="hlt">release</span> was particularly large for glutamate and GABA (31141 and 13282 pmol mg-1, respectively). The intracellular concentrations were generally reduced, but the total amount of the <span class="hlt">released</span> amino acids increased In contrast to the effect seen during hyposmolar stress, mannitol enhanced the changes due to <span class="hlt">energy</span> deprivation. The results show that hyposmolar stress and <span class="hlt">energy</span> deprivation cause different content and <span class="hlt">release</span> profiles, suggesting that the mechanisms involved in the two situations are either different or modulated in different ways. The intracellular amino acid depletion seen during <span class="hlt">energy</span> deprivation shows that increased outward transport is probably a primary event, and increased amino acid formation likely secondary to this <span class="hlt">release</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1046745','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/1046745"><span>Solar Thermal <span class="hlt">Energy</span> Storage Device: Hybrid Nanostructures for High-<span class="hlt">Energy</span>-Density Solar Thermal Fuels</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>None</p> <p>2012-01-09</p> <p>HEATS Project: MIT is developing a thermal <span class="hlt">energy</span> storage device that captures <span class="hlt">energy</span> from the sun; this <span class="hlt">energy</span> can be stored and <span class="hlt">released</span> at a later time when it is needed most. Within the device, the absorption of sunlight causes the solar thermal fuel’s photoactive molecules to change shape, which allows <span class="hlt">energy</span> to be stored within their chemical bonds. A trigger is applied to <span class="hlt">release</span> the stored <span class="hlt">energy</span> as heat, where it can be converted into electricity or used directly as heat. The molecules would then revert to their original shape, and can be recharged using sunlight to begin themore » process anew. MIT’s technology would be 100% renewable, rechargeable like a battery, and emissions-free. Devices using these solar thermal fuels—called Hybrisol—can also be used without a grid infrastructure for applications such as de-icing, heating, cooking, and water purification.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/19182389','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/19182389"><span>Sustained-<span class="hlt">release</span> progesterone vaginal suppositories 1--development of sustained-<span class="hlt">release</span> granule--.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Nakayama, Ayako; Sunada, Hisakazu; Okamoto, Hirokazu; Furuhashi, Kaoru; Ohno, Yukiko; Ito, Mikio</p> <p>2009-02-01</p> <p>Progesterone (P) is an important hormone for the establishment of pregnancy, and its administration is useful for luteal insufficiency. Considering the problems of commercially available oral and injection drugs, hospital-formulated vaginal suppositories are clinically used. However, since the half-life of P suppositories is short, it is difficult to maintain its constant blood concentration. To sustain drug efficacy and prevent side-effects, we are attempting to develop sustained-<span class="hlt">release</span> suppositories by examining the degree of sustained-<span class="hlt">release</span> of active ingredients. In this study, we examined the combinations of granulation methods and <span class="hlt">release</span> systems for the preparation of sustained-<span class="hlt">release</span> granules of P, and produced 13 types of sustained-<span class="hlt">release</span> granules. We also examined the diameter, content, and dissolution of each type of granules, and confirmed that the sustained-<span class="hlt">release</span> of all types of granules was satisfactory. Among the sustained-<span class="hlt">release</span> granules, we selected granules with a content and a degree of sustained-<span class="hlt">release</span> suitable for sustained-<span class="hlt">release</span> suppositories.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4703894','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4703894"><span>ATP hydrolysis assists phosphate <span class="hlt">release</span> and promotes reaction ordering in F1-ATPase</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Li, Chun-Biu; Ueno, Hiroshi; Watanabe, Rikiya; Noji, Hiroyuki; Komatsuzaki, Tamiki</p> <p>2015-01-01</p> <p>F1-ATPase (F1) is a rotary motor protein that can efficiently convert chemical <span class="hlt">energy</span> to mechanical work of rotation via fine coordination of its conformational motions and reaction sequences. Compared with reactant binding and product <span class="hlt">release</span>, the ATP hydrolysis has relatively little contributions to the torque and chemical <span class="hlt">energy</span> generation. To scrutinize possible roles of ATP hydrolysis, we investigate the detailed statistics of the catalytic dwells from high-speed single wild-type F1 observations. Here we report a small rotation during the catalytic dwell triggered by the ATP hydrolysis that is indiscernible in previous studies. Moreover, we find in freely rotating F1 that ATP hydrolysis is followed by the <span class="hlt">release</span> of inorganic phosphate with low synthesis rates. Finally, we propose functional roles of the ATP hydrolysis as a key to kinetically unlock the subsequent phosphate <span class="hlt">release</span> and promote the correct reaction ordering. PMID:26678797</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27097108','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27097108"><span>Indocyanine Green-Loaded Liposomes for Light-Triggered Drug <span class="hlt">Release</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Lajunen, Tatu; Kontturi, Leena-Stiina; Viitala, Lauri; Manna, Moutusi; Cramariuc, Oana; Róg, Tomasz; Bunker, Alex; Laaksonen, Timo; Viitala, Tapani; Murtomäki, Lasse; Urtti, Arto</p> <p>2016-06-06</p> <p>Light-triggered drug delivery systems enable site-specific and time-controlled drug <span class="hlt">release</span>. In previous work, we have achieved this with liposomes containing gold nanoparticles in the aqueous core. Gold nanoparticles absorb near-infrared light and <span class="hlt">release</span> the <span class="hlt">energy</span> as heat that increases the permeability of the liposomal bilayer, thus <span class="hlt">releasing</span> the contents of the liposome. In this work, we replaced the gold nanoparticles with the clinically approved imaging agent indocyanine green (ICG). The ICG liposomes were stable at storage conditions (4-22 °C) and at body temperature, and fast near-infrared (IR) light-triggered drug <span class="hlt">release</span> was achieved with optimized phospholipid composition and a 1:50 ICG-to-lipid molar ratio. Encapsulated small molecular calcein and FITC-dextran (up to 20 kDa) were completely <span class="hlt">released</span> from the liposomes after light exposure for 15 s. Location of ICG in the PEG layer of the liposomes was simulated with molecular dynamics. ICG has important benefits as a light-triggering agent in liposomes: fast content <span class="hlt">release</span>, improved stability, improved possibility of liposomal size control, regulatory approval to use in humans, and the possibility of imaging the in vivo location of the liposomes based on the fluorescence of ICG. Near-infrared light used as a triggering mechanism has good tissue penetration and safety. Thus, ICG liposomes are an attractive option for light-controlled and efficient delivery of small and large drug molecules.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/14659427','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/14659427"><span>Dioxins and furans formation in pilot incineration tests of sewage sludge spiked with organic chlorine.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Mininni, Giuseppe; Sbrilli, Andrea; Guerriero, Ettore; Rotatori, Mauro</p> <p>2004-03-01</p> <p>The factors affecting polychlorinated dibenzo-p-dioxins (PCDD) and polychlorinated dibenzofurans (PCDF) formation were studied in sewage sludge incineration tests carried out on a demonstrative plant. The plant includes a circulating fluidised bed furnace (FBF) and a rotary kiln furnace (RKF), operating alternatively. During the tests sewage sludge was spiked with chlorinated hydrocarbons and the operating parameters of the <span class="hlt">afterburning</span> chamber were varied. PCDD/F were sampled in each test before the bag filter, thus collecting the above contaminants before abatement systems. From the tests it appeared that PCDD/F were always produced in more abundance in the tests carried out by FBF than by RKF. The higher PCDD/F concentrations in the tests by FBF were reached when sewage sludge was spiked with a high dosage of a surrogate organic mixture of chlorinated hydrocarbons and when the <span class="hlt">afterburning</span> chamber was used only as transit equipment with the burner off. The distribution of the different PCDD/F homologues was compared. P5CDFs were generally the prevalent fraction, with very few exceptions for the tests by RKF at high temperature of the <span class="hlt">afterburning</span> chamber. As for FBF tests, it was found that the PCDD/F homologue profile depends on the <span class="hlt">afterburning</span> chamber temperature.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/24994533','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/24994533"><span>The destiny of Ca(2+) <span class="hlt">released</span> by mitochondria.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Takeuchi, Ayako; Kim, Bongju; Matsuoka, Satoshi</p> <p>2015-01-01</p> <p>Mitochondrial Ca(2+) is known to regulate diverse cellular functions, for example <span class="hlt">energy</span> production and cell death, by modulating mitochondrial dehydrogenases, inducing production of reactive oxygen species, and opening mitochondrial permeability transition pores. In addition to the action of Ca(2+) within mitochondria, Ca(2+) <span class="hlt">released</span> from mitochondria is also important in a variety of cellular functions. In the last 5 years, the molecules responsible for mitochondrial Ca(2+) dynamics have been identified: a mitochondrial Ca(2+) uniporter (MCU), a mitochondrial Na(+)-Ca(2+) exchanger (NCLX), and a candidate for a mitochondrial H(+)-Ca(2+) exchanger (Letm1). In this review, we focus on the mitochondrial Ca(2+) <span class="hlt">release</span> system, and discuss its physiological and pathophysiological significance. Accumulating evidence suggests that the mitochondrial Ca(2+) <span class="hlt">release</span> system is not only crucial in maintaining mitochondrial Ca(2+) homeostasis but also participates in the Ca(2+) crosstalk between mitochondria and the plasma membrane and between mitochondria and the endoplasmic/sarcoplasmic reticulum.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/10159717','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/10159717"><span>Radioactive materials <span class="hlt">released</span> from nuclear power plants. Annual report 1991, Volume 12</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Tichler, J.; Doty, K.; Congemi, J.</p> <p></p> <p><span class="hlt">Releases</span> of radioactive materials in airborne and liquid effluents from commercial light water reactors during 1991 have been compiled and reported. Data on solid waste shipments as well as selected operating information have been included. This report supplements earlier annual reports issued by the former Atomic <span class="hlt">Energy</span> Commission and the Nuclear Regulatory Commission. The 1991 <span class="hlt">release</span> data are summarized in tabular form. Data Covering specific radionuclides are summarized.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/6095021','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/6095021"><span>Radioactive materials <span class="hlt">released</span> from nuclear power plants. Annual report, 1982. Volume 3</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Tichler, J.; Norden, K.</p> <p></p> <p><span class="hlt">Releases</span> of radioactive materials in airborne and liquid effluents from commercial light water reactors during 1982 have been compiled and reported. Data on solid waste shipments as well as selected operating information have been included. This report supplements earlier annual reports issued by the former Atomic <span class="hlt">Energy</span> Commission and the Nuclear Regulatory Commission. The 1982 <span class="hlt">release</span> data are summarized in tabular form. Data covering specific radionuclides are summarized.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/10189046','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/10189046"><span>Radioactive materials <span class="hlt">released</span> from nuclear power plants. Volume 11: Annual report, 1990</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Tichler, J.; Doty, K.; Congemi, J.</p> <p></p> <p><span class="hlt">Releases</span> of radioactive materials in airborne and liquid effluents from commercial light water reactors during 1990 have been compiled and reported. Data on solid waste shipments as well as selected operating information have been included. This report supplements earlier annual reports issued by the former Atomic <span class="hlt">Energy</span> Commission and the Nuclear Regulatory Commission. The 1990 <span class="hlt">release</span> data are summarized in tabular form. Data covering specific radionuclides are summarized.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/7030462','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/7030462"><span>Radioactive materials <span class="hlt">released</span> from nuclear power plants. Annual report 1981. Vol. 2</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Tichler, J.; Benkovitz, C.</p> <p></p> <p><span class="hlt">Releases</span> of radioactive materials in airborne and liquid effluents from commercial light water reactors during 1981 have been compiled and reported. Data on solid waste shipments as well as selected operating information have been included. This report supplements earlier annual reports issued by the former Atomic <span class="hlt">Energy</span> Commission and the Nuclear Regulatory Commission. The 1981 <span class="hlt">release</span> data are summarized in tabular form. Data covering specific radionuclides are summarized.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/5359493','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/5359493"><span>Radioactive materials <span class="hlt">released</span> from nuclear power plants. Annual report, 1983. Volume 4</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Tichler, J.; Norden, K.</p> <p></p> <p><span class="hlt">Releases</span> of radioactive materials in airborne and liquid effluents from commercial light water reactors during 1983 have been compiled and reported. Data on solid waste shipments as well as selected operating information have been included. This report supplements earlier annual reports issued by the former Atomic <span class="hlt">Energy</span> Commission and the Nuclear Regulatory Commission. The 1983 <span class="hlt">release</span> data are summarized in tabular form. Data covering specific radionuclides are summarized.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/CFR-2011-title10-vol2/pdf/CFR-2011-title10-vol2-sec61-41.pdf','CFR2011'); return false;" href="https://www.gpo.gov/fdsys/pkg/CFR-2011-title10-vol2/pdf/CFR-2011-title10-vol2-sec61-41.pdf"><span>10 CFR 61.41 - Protection of the general population from <span class="hlt">releases</span> of radioactivity.</span></a></p> <p><a target="_blank" href="http://www.gpo.gov/fdsys/browse/collectionCfr.action?selectedYearFrom=2011&page.go=Go">Code of Federal Regulations, 2011 CFR</a></p> <p></p> <p>2011-01-01</p> <p>... 10 <span class="hlt">Energy</span> 2 2011-01-01 2011-01-01 false Protection of the general population from <span class="hlt">releases</span> of radioactivity. 61.41 Section 61.41 <span class="hlt">Energy</span> NUCLEAR REGULATORY COMMISSION (CONTINUED) LICENSING REQUIREMENTS FOR LAND DISPOSAL OF RADIOACTIVE WASTE Performance Objectives § 61.41 Protection of the general population...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/CFR-2010-title10-vol2/pdf/CFR-2010-title10-vol2-sec61-41.pdf','CFR'); return false;" href="https://www.gpo.gov/fdsys/pkg/CFR-2010-title10-vol2/pdf/CFR-2010-title10-vol2-sec61-41.pdf"><span>10 CFR 61.41 - Protection of the general population from <span class="hlt">releases</span> of radioactivity.</span></a></p> <p><a target="_blank" href="http://www.gpo.gov/fdsys/browse/collectionCfr.action?selectedYearFrom=2010&page.go=Go">Code of Federal Regulations, 2010 CFR</a></p> <p></p> <p>2010-01-01</p> <p>... 10 <span class="hlt">Energy</span> 2 2010-01-01 2010-01-01 false Protection of the general population from <span class="hlt">releases</span> of radioactivity. 61.41 Section 61.41 <span class="hlt">Energy</span> NUCLEAR REGULATORY COMMISSION (CONTINUED) LICENSING REQUIREMENTS FOR LAND DISPOSAL OF RADIOACTIVE WASTE Performance Objectives § 61.41 Protection of the general population...</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li class="active"><span>18</span></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_18 --> <div id="page_19" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li class="active"><span>19</span></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="361"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/CFR-2012-title10-vol2/pdf/CFR-2012-title10-vol2-sec61-41.pdf','CFR2012'); return false;" href="https://www.gpo.gov/fdsys/pkg/CFR-2012-title10-vol2/pdf/CFR-2012-title10-vol2-sec61-41.pdf"><span>10 CFR 61.41 - Protection of the general population from <span class="hlt">releases</span> of radioactivity.</span></a></p> <p><a target="_blank" href="http://www.gpo.gov/fdsys/browse/collectionCfr.action?selectedYearFrom=2012&page.go=Go">Code of Federal Regulations, 2012 CFR</a></p> <p></p> <p>2012-01-01</p> <p>... 10 <span class="hlt">Energy</span> 2 2012-01-01 2012-01-01 false Protection of the general population from <span class="hlt">releases</span> of radioactivity. 61.41 Section 61.41 <span class="hlt">Energy</span> NUCLEAR REGULATORY COMMISSION (CONTINUED) LICENSING REQUIREMENTS FOR LAND DISPOSAL OF RADIOACTIVE WASTE Performance Objectives § 61.41 Protection of the general population...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/CFR-2014-title10-vol2/pdf/CFR-2014-title10-vol2-sec61-41.pdf','CFR2014'); return false;" href="https://www.gpo.gov/fdsys/pkg/CFR-2014-title10-vol2/pdf/CFR-2014-title10-vol2-sec61-41.pdf"><span>10 CFR 61.41 - Protection of the general population from <span class="hlt">releases</span> of radioactivity.</span></a></p> <p><a target="_blank" href="http://www.gpo.gov/fdsys/browse/collectionCfr.action?selectedYearFrom=2014&page.go=Go">Code of Federal Regulations, 2014 CFR</a></p> <p></p> <p>2014-01-01</p> <p>... 10 <span class="hlt">Energy</span> 2 2014-01-01 2014-01-01 false Protection of the general population from <span class="hlt">releases</span> of radioactivity. 61.41 Section 61.41 <span class="hlt">Energy</span> NUCLEAR REGULATORY COMMISSION (CONTINUED) LICENSING REQUIREMENTS FOR LAND DISPOSAL OF RADIOACTIVE WASTE Performance Objectives § 61.41 Protection of the general population...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/CFR-2013-title10-vol2/pdf/CFR-2013-title10-vol2-sec61-41.pdf','CFR2013'); return false;" href="https://www.gpo.gov/fdsys/pkg/CFR-2013-title10-vol2/pdf/CFR-2013-title10-vol2-sec61-41.pdf"><span>10 CFR 61.41 - Protection of the general population from <span class="hlt">releases</span> of radioactivity.</span></a></p> <p><a target="_blank" href="http://www.gpo.gov/fdsys/browse/collectionCfr.action?selectedYearFrom=2013&page.go=Go">Code of Federal Regulations, 2013 CFR</a></p> <p></p> <p>2013-01-01</p> <p>... 10 <span class="hlt">Energy</span> 2 2013-01-01 2013-01-01 false Protection of the general population from <span class="hlt">releases</span> of radioactivity. 61.41 Section 61.41 <span class="hlt">Energy</span> NUCLEAR REGULATORY COMMISSION (CONTINUED) LICENSING REQUIREMENTS FOR LAND DISPOSAL OF RADIOACTIVE WASTE Performance Objectives § 61.41 Protection of the general population...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016APS..DPPN10144H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016APS..DPPN10144H"><span>Measuring the properties of shock <span class="hlt">released</span> Quartz and Parylene-N</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hawreliak, James; Karasik, Max; Oh, Jaechul; Aglitskiy, Yefim</p> <p>2016-10-01</p> <p>The high pressure and temperature properties of Quartz and hydrocarbons are important to high <span class="hlt">energy</span> density (HED) research and inertial confinement fusion (ICF) science. The bulk of HED material research studies the single shock Hugoniot. Here, we present experimental results from the NIKE laser where quartz and parylene-N are shock compressed to high pressure and temperature and the <span class="hlt">release</span> state is measured through x-ray imaging. The shock state is characterized by shock front velocity measurements using VISAR and the <span class="hlt">release</span> state is characterized by using side-on streaked x-ray radiography.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22308371-low-energy-electron-induced-cytosine-base-release-deoxycytidine-monophosphate-via-glycosidic-bond-cleavage-time-dependent-wavepacket-study','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22308371-low-energy-electron-induced-cytosine-base-release-deoxycytidine-monophosphate-via-glycosidic-bond-cleavage-time-dependent-wavepacket-study"><span>Low <span class="hlt">energy</span> electron induced cytosine base <span class="hlt">release</span> in 2′-deoxycytidine-3′-monophosphate via glycosidic bond cleavage: A time-dependent wavepacket study</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Bhaskaran, Renjith; Sarma, Manabendra, E-mail: msarma@iitg.ernet.in</p> <p>2014-09-14</p> <p>Low <span class="hlt">energy</span> electron (LEE) induced cytosine base <span class="hlt">release</span> in a selected pyrimidine nucleotide, viz., 2′-deoxycytidine-3′-monophosphate is investigated using ab initio electronic structure methods and time dependent quantum mechanical calculations. It has been noted that the cytosine base scission is comparatively difficult process than the 3′ C–O bond cleavage from the lowest π{sup *} shape resonance in <span class="hlt">energy</span> region <1 eV. This is mainly due to the high activation <span class="hlt">energy</span> barrier associated with the electron transfer from the π{sup *} orbital of the base to the σ{sup *} orbital of the glycosidic N–C bond. In addition, the metastable state formed aftermore » impinging LEE (0–1 eV) has very short lifetime (10 fs) which may decay in either of the two competing auto-detachment or dissociation process simultaneously. On the other hand, the selected N–C mode may cleave to form the cytosine base anion at higher <span class="hlt">energy</span> regions (>2 eV) via tunneling of the glycosidic bond. Resonance states generated within this <span class="hlt">energy</span> regime will exist for a duration of ∼35–55 fs. Comparison of salient features of the two dissociation events, i.e., 3′ C–O single strand break and glycosidic N–C bond cleavage in 3′-dCMPH molecule are also provided.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017PhDT.......119S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017PhDT.......119S"><span>Ultrasound Stimulation of Insulin <span class="hlt">Release</span> from Pancreatic Beta Cells</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Suarez Castellanos, Ivan M.</p> <p></p> <p>Type 2 diabetes (T2D) mellitus is a complex metabolic disease that has reached epidemic proportions in the United States and around the world. Controlling T2D is often difficult as pharmacological management routinely requires complex therapy with multiple medications, and loses its effectiveness over time. The objective of this dissertation was to explore a novel, non-pharmacological approach that utilizes the application of ultrasound <span class="hlt">energy</span> to stimulate insulin <span class="hlt">release</span>. Our experiments have focused on determination of effectiveness and safety of ultrasound application in stimulation of insulin <span class="hlt">release</span> from the pancreatic beta cells. Our results showed that ultrasound treatment, applied at frequencies of 800 kHz and 1 MHz and intensities of 0.5 W/cm2 and 1 W/cm2, did not produce any significant effects on cell viability compared to sham group as assessed with trypan blue dye exclusion test and MTT cytotoxicity assay. ELISA quantification of insulin <span class="hlt">release</span> from beta cells resulting from ultrasound treatment showed clinically-significant amounts of <span class="hlt">released</span> insulin as compared to sham-treated beta cells. Carbon fiber amperometry detection of secretory events from dopamine-loaded beta cells treated with ultrasound showed that <span class="hlt">release</span> of secretory content could be temporally controlled by careful selection of ultrasound parameters. Both ELISA and amperometry experiments demonstrated that ultrasound-stimulated insulin <span class="hlt">release</span> is a calcium-dependent process, potentially mediated by the mechanical effects of ultrasound. This study demonstrated that therapeutic ultrasound is a technique capable of stimulating the <span class="hlt">release</span> of insulin from pancreatic beta cells in a safe, effective and controlled manner.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27432081','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27432081"><span>Genipin crosslinker <span class="hlt">releasing</span> sutures for improving the mechanical/repair strength of damaged connective tissue.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Sundararaj, Sharath; Slusarewicz, Paul; Brown, Matt; Hedman, Thomas</p> <p>2017-11-01</p> <p>The most common mode of surgical repair of ruptured tendons and ligaments involves the use of sutures for reattachment. However, there is a high incidence of rerupture and repair failure due to pulling out of the suture material from the damaged connective tissue. The main goal of this research was to achieve a localized delivery of crosslinking agent genipin (GP) from rapid-<span class="hlt">release</span> biodegradable coatings on sutures, for strengthening the repair of ruptured connective tissue. Our hypothesis is that GP <span class="hlt">released</span> from the suture coating will lead to exogenous crosslinking of native connective tissue resulting in beneficial effects on clinically relevant mechanical parameters such as tear resistance, tissue strength, and <span class="hlt">energy</span> required to rupture the tissue (toughness). Sutures were successfully coated with a biodegradable polymer layer loaded with the crosslinking agent genipin, without compromising the mechanical properties of the suture. The rapid-<span class="hlt">release</span> of genipin was achieved under both in vitro and ex vivo conditions. Exogenous crosslinking using these genipin <span class="hlt">releasing</span> sutures was demonstrated using equine tendons. The tendons treated with genipin <span class="hlt">releasing</span> sutures showed significant improvement in failure load, <span class="hlt">energy</span> required for pull-out failure, and stiffness. © 2016 Wiley Periodicals, Inc. J Biomed Mater Res Part B: Appl Biomater, 105B: 2199-2205, 2017. © 2016 Wiley Periodicals, Inc.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28801266','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28801266"><span>Lipogels responsive to near-infrared light for the triggered <span class="hlt">release</span> of therapeutic agents.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Martín-Saavedra, Francisco; Ruiz-Hernández, Eduardo; Escudero-Duch, Clara; Prieto, Martín; Arruebo, Manuel; Sadeghi, Negar; Deckers, Roel; Storm, Gert; Hennink, Wim E; Santamaría, Jesús; Vilaboa, Nuria</p> <p>2017-10-01</p> <p>Here we report a composite system based on fibrin hydrogels that incorporate in their structure near-infrared (NIR) responsive nanomaterials and thermosensitive liposomes (TSL). Polymerized fibrin networks entrap simultaneously gold-based nanoparticles (NPs) capable of transducing NIR photon <span class="hlt">energy</span> into heat, and lysolipid-incorporated TSL (LTSL) loaded with doxorubicin hydrochloride (DOX). NIR irradiation of the resulting hydrogels (referred to as "lipogels") with 808nm laser light increased the temperature of the illuminated areas, leading to the <span class="hlt">release</span> of the liposomal cargo. Levels of DOX that <span class="hlt">release</span> from the "smart" composites were dependent on the concentration of NIR nanotransducers loaded in the lipogel, the intensity of the electromagnetic <span class="hlt">energy</span> deposited and the irradiation regime. <span class="hlt">Released</span> DOX retained its bioactivity, as shown in cultures of epithelial carcinoma cells. Finally, the developed drug delivery platform was refined by using NIR-photoabsorbers based on copper sulfide NPs to generate completely biodegradable composites as well as through the incorporation of cholesterol (Ch) in LTSL formulation, which lessens leakiness of the liposomal cargo at physiological temperature. This remotely controlled system may suit well for those therapies that require precise control over the dose of delivered drug in a defined spatiotemporal framework. Hydrogels composed of fibrin embedding nanoparticles responsive to near infrared (NIR) <span class="hlt">energy</span> and thermosensitive liposomes loaded with doxorubicin hydrochloride (DOX), were prepared by in situ polymerization. NIR-light irradiation of these constructs, referred to as "NIR responsive lipogels", results in the controlled <span class="hlt">release</span> of DOX to the surrounding medium. This technology may use fully degradable components and can preserve the bioactivity of liposomal cargo after remote triggering to finely regulate the dose and bioavailability of delivered payloads. NIR responsive lipogels technology overcomes the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/22686344','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/22686344"><span>Accelerated in-vitro <span class="hlt">release</span> testing methods for extended-<span class="hlt">release</span> parenteral dosage forms.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Shen, Jie; Burgess, Diane J</p> <p>2012-07-01</p> <p>This review highlights current methods and strategies for accelerated in-vitro drug <span class="hlt">release</span> testing of extended-<span class="hlt">release</span> parenteral dosage forms such as polymeric microparticulate systems, lipid microparticulate systems, in-situ depot-forming systems and implants. Extended-<span class="hlt">release</span> parenteral dosage forms are typically designed to maintain the effective drug concentration over periods of weeks, months or even years. Consequently, 'real-time' in-vitro <span class="hlt">release</span> tests for these dosage forms are often run over a long time period. Accelerated in-vitro <span class="hlt">release</span> methods can provide rapid evaluation and therefore are desirable for quality control purposes. To this end, different accelerated in-vitro <span class="hlt">release</span> methods using United States Pharmacopeia (USP) apparatus have been developed. Different mechanisms of accelerating drug <span class="hlt">release</span> from extended-<span class="hlt">release</span> parenteral dosage forms, along with the accelerated in-vitro <span class="hlt">release</span> testing methods currently employed are discussed. Accelerated in-vitro <span class="hlt">release</span> testing methods with good discriminatory ability are critical for quality control of extended-<span class="hlt">release</span> parenteral products. Methods that can be used in the development of in-vitro-in-vivo correlation (IVIVC) are desirable; however, for complex parenteral products this may not always be achievable. © 2012 The Authors. JPP © 2012 Royal Pharmaceutical Society.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3408959','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3408959"><span>Accelerated in vitro <span class="hlt">release</span> testing methods for extended <span class="hlt">release</span> parenteral dosage forms</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Shen, Jie; Burgess, Diane J.</p> <p>2012-01-01</p> <p>Objectives This review highlights current methods and strategies for accelerated in vitro drug <span class="hlt">release</span> testing of extended <span class="hlt">release</span> parenteral dosage forms such as polymeric microparticulate systems, lipid microparticulate systems, in situ depot-forming systems, and implants. Key findings Extended <span class="hlt">release</span> parenteral dosage forms are typically designed to maintain the effective drug concentration over periods of weeks, months or even years. Consequently, “real-time” in vitro <span class="hlt">release</span> tests for these dosage forms are often run over a long time period. Accelerated in vitro <span class="hlt">release</span> methods can provide rapid evaluation and therefore are desirable for quality control purposes. To this end, different accelerated in vitro <span class="hlt">release</span> methods using United States Pharmacopoeia (USP) apparatus have been developed. Different mechanisms of accelerating drug <span class="hlt">release</span> from extended <span class="hlt">release</span> parenteral dosage forms, along with the accelerated in vitro <span class="hlt">release</span> testing methods currently employed are discussed. Conclusions Accelerated in vitro <span class="hlt">release</span> testing methods with good discriminatory ability are critical for quality control of extended <span class="hlt">release</span> parenteral products. Methods that can be used in the development of in vitro-in vivo correlation (IVIVC) are desirable, however for complex parenteral products this may not always be achievable. PMID:22686344</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/25246129','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25246129"><span><span class="hlt">Energy</span> independent uptake and <span class="hlt">release</span> of polystyrene nanoparticles in primary mammalian cell cultures.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Fiorentino, Ilaria; Gualtieri, Roberto; Barbato, Vincenza; Mollo, Valentina; Braun, Sabrina; Angrisani, Alberto; Turano, Mimmo; Furia, Maria; Netti, Paolo A; Guarnieri, Daniela; Fusco, Sabato; Talevi, Riccardo</p> <p>2015-01-15</p> <p>Nanoparticle (NPs) delivery systems in vivo promises to overcome many obstacles associated with the administration of drugs, vaccines, plasmid DNA and RNA materials, making the study of their cellular uptake a central issue in nanomedicine. The uptake of NPs may be influenced by the cell culture stage and the NPs physical-chemical properties. So far, controversial data on NPs uptake have been derived owing to the heterogeneity of NPs and the general use of immortalized cancer cell lines that often behave differently from each other and from primary mammalian cell cultures. Main aims of the present study were to investigate the uptake, endocytosis pathways, intracellular fate and <span class="hlt">release</span> of well standardized model particles, i.e. fluorescent 44 nm polystyrene NPs (PS-NPs), on two primary mammalian cell cultures, i.e. bovine oviductal epithelial cells (BOEC) and human colon fibroblasts (HCF) by confocal microscopy and spectrofluorimetric analysis. Different drugs and conditions that inhibit specific internalization routes were used to understand the mechanisms that mediate PS-NP uptake. Our data showed that PS-NPs are rapidly internalized by both cell types 1) with similar saturation kinetics; 2) through ATP-independent processes, and 3) quickly <span class="hlt">released</span> in the culture medium. Our results suggest that PS-NPs are able to rapidly cross the cell membrane through passive translocation during both uptake and <span class="hlt">release</span>, and emphasize the need to carefully design NPs for drug delivery, to ensure their selective uptake and to optimize their retainment in the targeted cells. Copyright © 2014 Elsevier Inc. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/1441352-expanding-capability-reaction-diffusion-codes-using-pseudo-traps-temperature-partitioning-applied-hydrogen-uptake-release-from-tungsten','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/1441352-expanding-capability-reaction-diffusion-codes-using-pseudo-traps-temperature-partitioning-applied-hydrogen-uptake-release-from-tungsten"><span>Expanding the capability of reaction-diffusion codes using pseudo traps and temperature partitioning: Applied to hydrogen uptake and <span class="hlt">release</span> from tungsten</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Simmonds, M. J.; Yu, J. H.; Wang, Y. Q.</p> <p></p> <p>Simulating the implantation and thermal desorption evolution in a reaction-diffusion model requires solving a set of coupled differential equations that describe the trapping and <span class="hlt">release</span> of atomic species in Plasma Facing Materials (PFMs). These fundamental equations are well outlined by the Tritium Migration Analysis Program (TMAP) which can model systems with no more than three active traps per atomic species. To overcome this limitation, we have developed a Pseudo Trap and Temperature Partition (PTTP) scheme allowing us to lump multiple inactive traps into one pseudo trap, simplifying the system of equations to be solved. For all temperatures, we show themore » trapping of atoms from solute is exactly accounted for when using a pseudo trap. However, a single effective pseudo trap <span class="hlt">energy</span> can not well replicate the <span class="hlt">release</span> from multiple traps, each with its own detrapping <span class="hlt">energy</span>. However, atoms held in a high <span class="hlt">energy</span> trap will remain trapped at relatively low temperatures, and thus there is a temperature range in which <span class="hlt">release</span> from high <span class="hlt">energy</span> traps is effectively inactive. By partitioning the temperature range into segments, a pseudo trap can be defined for each segment to account for multiple high <span class="hlt">energy</span> traps that are actively trapping but are effectively not <span class="hlt">releasing</span> atoms. With increasing temperature, as in controlled thermal desorption, the lowest <span class="hlt">energy</span> trap is nearly emptied and can be removed from the set of coupled equations, while the next higher <span class="hlt">energy</span> trap becomes an actively <span class="hlt">releasing</span> trap. Each segment is thus calculated sequentially, with the last time step of a given segment solution being used as an initial input for the next segment as only the pseudo and actively <span class="hlt">releasing</span> traps are modeled. This PTTP scheme is then applied to experimental thermal desorption data for tungsten (W) samples damaged with heavy ions, which display six distinct <span class="hlt">release</span> peaks during thermal desorption. Without modifying the TMAP7 source code the PTTP scheme is shown</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1441352-expanding-capability-reaction-diffusion-codes-using-pseudo-traps-temperature-partitioning-applied-hydrogen-uptake-release-from-tungsten','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1441352-expanding-capability-reaction-diffusion-codes-using-pseudo-traps-temperature-partitioning-applied-hydrogen-uptake-release-from-tungsten"><span>Expanding the capability of reaction-diffusion codes using pseudo traps and temperature partitioning: Applied to hydrogen uptake and <span class="hlt">release</span> from tungsten</span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Simmonds, M. J.; Yu, J. H.; Wang, Y. Q.; ...</p> <p>2018-06-04</p> <p>Simulating the implantation and thermal desorption evolution in a reaction-diffusion model requires solving a set of coupled differential equations that describe the trapping and <span class="hlt">release</span> of atomic species in Plasma Facing Materials (PFMs). These fundamental equations are well outlined by the Tritium Migration Analysis Program (TMAP) which can model systems with no more than three active traps per atomic species. To overcome this limitation, we have developed a Pseudo Trap and Temperature Partition (PTTP) scheme allowing us to lump multiple inactive traps into one pseudo trap, simplifying the system of equations to be solved. For all temperatures, we show themore » trapping of atoms from solute is exactly accounted for when using a pseudo trap. However, a single effective pseudo trap <span class="hlt">energy</span> can not well replicate the <span class="hlt">release</span> from multiple traps, each with its own detrapping <span class="hlt">energy</span>. However, atoms held in a high <span class="hlt">energy</span> trap will remain trapped at relatively low temperatures, and thus there is a temperature range in which <span class="hlt">release</span> from high <span class="hlt">energy</span> traps is effectively inactive. By partitioning the temperature range into segments, a pseudo trap can be defined for each segment to account for multiple high <span class="hlt">energy</span> traps that are actively trapping but are effectively not <span class="hlt">releasing</span> atoms. With increasing temperature, as in controlled thermal desorption, the lowest <span class="hlt">energy</span> trap is nearly emptied and can be removed from the set of coupled equations, while the next higher <span class="hlt">energy</span> trap becomes an actively <span class="hlt">releasing</span> trap. Each segment is thus calculated sequentially, with the last time step of a given segment solution being used as an initial input for the next segment as only the pseudo and actively <span class="hlt">releasing</span> traps are modeled. This PTTP scheme is then applied to experimental thermal desorption data for tungsten (W) samples damaged with heavy ions, which display six distinct <span class="hlt">release</span> peaks during thermal desorption. Without modifying the TMAP7 source code the PTTP scheme is shown</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20080012200&hterms=Renewable+energy&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3DRenewable%2Benergy','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20080012200&hterms=Renewable+energy&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3DRenewable%2Benergy"><span>Surface meteorology and Solar <span class="hlt">Energy</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Stackhouse, Paul W. (Principal Investigator)</p> <p></p> <p>The <span class="hlt">Release</span> 5.1 Surface meteorology and Solar <span class="hlt">Energy</span> (SSE) data contains parameters formulated for assessing and designing renewable <span class="hlt">energy</span> systems. Parameters fall under 11 categories including: Solar cooking, solar thermal applications, solar geometry, tilted solar panels, <span class="hlt">energy</span> storage systems, surplus product storage systems, cloud information, temperature, wind, other meteorological factors, and supporting information. This latest <span class="hlt">release</span> contains new parameters based on recommendations by the renewable <span class="hlt">energy</span> industry and it is more accurate than previous <span class="hlt">releases</span>. On-line plotting capabilities allow quick evaluation of potential renewable <span class="hlt">energy</span> projects for any region of the world. The SSE data set is formulated from NASA satellite- and reanalysis-derived insolation and meteorological data for the 10-year period July 1983 through June 1993. Results are provided for 1 degree latitude by 1 degree longitude grid cells over the globe. Average daily and monthly measurements for 1195 World Radiation Data Centre ground sites are also available. [Mission Objectives] The SSE project contains insolation and meteorology data intended to aid in the development of renewable <span class="hlt">energy</span> systems. Collaboration between SSE and technology industries such as the Hybrid Optimization Model for Electric Renewables ( HOMER ) may aid in designing electric power systems that employ some combination of wind turbines, photovoltaic panels, or diesel generators to produce electricity. [Temporal_Coverage: Start_Date=1983-07-01; Stop_Date=1993-06-30] [Spatial_Coverage: Southernmost_Latitude=-90; Northernmost_Latitude=90; Westernmost_Longitude=-180; Easternmost_Longitude=180].</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010JMPSo..58....1M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010JMPSo..58....1M"><span>The <span class="hlt">energy-release</span> rate and “self-force” of dynamically expanding spherical and plane inclusion boundaries with dilatational eigenstrain</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Markenscoff, Xanthippi; Ni, Luqun</p> <p>2010-01-01</p> <p>In the context of the linear theory of elasticity with eigenstrains, the radiated field including inertia effects of a spherical inclusion with dilatational eigenstrain radially expanding is obtained on the basis of the dynamic Green's function, and one of the half-space inclusion boundary (with dilatational eigenstrain) moving from rest in general subsonic motion is obtained by a limiting process from the spherically expanding inclusion as the radius tends to infinity while the eigenstrain remains constrained, and this is the minimum <span class="hlt">energy</span> solution. The global <span class="hlt">energy-release</span> rate required to move the plane inclusion boundary and to create an incremental region of eigenstrain is defined analogously to the one for moving cracks and dislocations and represents the mechanical rate of work needed to be provide for the expansion of the inclusion. The calculated value, which is the "self-force" of the expanding inclusion, has a static component plus a dynamic one depending only on the current value of the velocity, while in the case of the spherical boundary, there is an additional contribution accounting for the jump in the strain at the farthest part at the back of the inclusion having the time to reach the front boundary, thus making the dynamic "self-force" history dependent.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.eia.gov/outlooks/archive/aeo10/arra.html','EIAPUBS'); return false;" href="https://www.eia.gov/outlooks/archive/aeo10/arra.html"><span>American Recovery and Reinvestment Act of 2009: Summary of Provisions (<span class="hlt">released</span> in AEO2010)</span></a></p> <p><a target="_blank" href="http://www.eia.doe.gov/reports/">EIA Publications</a></p> <p></p> <p>2010-01-01</p> <p>The American Recovery and Reinvestment Act of 2009 (ARRA), signed into law in mid-February 2009, provides significant new federal funding, loan guarantees, and tax credits to stimulate investments in <span class="hlt">energy</span> efficiency and renewable <span class="hlt">energy</span>. The provisions of ARRA were incorporated initially as part of a revision to the Annual <span class="hlt">Energy</span> Outlook 2009 Reference case that was <span class="hlt">released</span> in April 2009, and they also are included in Annual <span class="hlt">Energy</span> Outlook 2010.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/4098692','DOE-PATENT-XML'); return false;" href="https://www.osti.gov/biblio/4098692"><span>ELECTROMAGNETIC <span class="hlt">RELEASE</span> MECHANISM</span></a></p> <p><a target="_blank" href="http://www.osti.gov/doepatents">DOEpatents</a></p> <p>Michelson, C.</p> <p>1960-09-13</p> <p>An electromagnetic <span class="hlt">release</span> mechanism is offered that may be used, for example, for supporting a safety rod for a nuclear reactor. The <span class="hlt">release</span> mechanism is designed to have a large excess holding force and a rapid, uniform, and dependable <span class="hlt">release</span>. The fast <span class="hlt">release</span> is accomplished by providing the electromagnet with slotttd polts separated by an insulating potting resin, and by constructing the poles with a ferro-nickel alloy. The combination of these two features materially reduces the eddy current power density whenever the magnetic field changes during a <span class="hlt">release</span> operation. In addition to these features, the design of the armature is such as to provide ready entrance of fluid into any void that might tend to form during <span class="hlt">release</span> of the armature. This also improves the <span class="hlt">release</span> time for the mechanism. The large holding force for the mechanism is accomplished by providing a small, selected, uniform air gap between the inner pole piece and the armature.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015APS..APR.X4007K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015APS..APR.X4007K"><span>Measurement of the Total Kinetic <span class="hlt">Energy</span> <span class="hlt">Release</span> (TKE) in 232 Th(n,f) with En = 2.59 - 87.31 MeV</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>King, Jonathan; Yanez, Ricardo; Barrett, Jonathan; Loveland, Walter; Tovesson, Fredrik; Fotiades, Nick; Lee, Hye Young</p> <p>2015-04-01</p> <p>Experimental results for the Total Kinetic <span class="hlt">Energy</span> <span class="hlt">Release</span> (TKE) of 232 Th(n,f) with En = 2.59 - 87.31 MeV will be presented. The experiment was performed at the 15R beamline at the Weapons Neutron Research(WNR) facility at LANL-LANSCE. WNR provides a white spectrum of neutrons peaking at 2 MeV and reaching up to 800 MeV, with neutron <span class="hlt">energies</span> being deduced from measurements of the neutron time of flight (TOF). A thin-backed 232 ThF4 target of 2 cm diameter with a thorium areal density of 178.9 μg/cm2 was placed between two arrays of Hammamatsu PIN diodes (active area 4 cm2 each). The beam was collimated to 1 cm diameter. The target was placed 45 degrees off of the beam axis, with the detectors at 60 degrees and 120 degrees from the beam axis. Over 25,000 fission fragment coincidence events were recorded, allowing for sixteen <span class="hlt">energy</span> bins between 2.59 and 87.31 MeV. We believe that this will be the most comprehensive published measurement of the TKE for 232 Th(n,f) with En = 2.59 - 87.31 MeV. This work was supported in part by the Director, Office of <span class="hlt">Energy</span> Research, Division of Nuclear Physics of the Office of High <span class="hlt">Energy</span> and Nuclear Physics of the USDoE under Grant DE-FG06-97ER41026. This work has benefited from the use of the Los Alamos Neutron Science Center at the Los Alamos National Laboratory. This facility is funded by the USDoE under DOE Contract No. DE-AC52-06NA25396.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/65434','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/65434"><span>Complement-induced histamine <span class="hlt">release</span> from human basophils. III. Effect of pharmacologic agents.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Hook, W A; Siraganian, R P</p> <p>1977-02-01</p> <p>Human serum activated with zymosan generates a factor (C5a) that <span class="hlt">releases</span> histamine from autologous basophils. Previously we have presented evidence that this mechanism for C5a-induced <span class="hlt">release</span> differs from IgE-mediated reactions. The effect of several pharmacologic agents known to alter IgE-mediated <span class="hlt">release</span> was studied to determine whether they have a similar action on serum-induced <span class="hlt">release</span>. Deuterium oxide (D2O), which enhances allergic <span class="hlt">release</span>, inhibited in a concentration-dependent fashion the serum-induced reaction at incubation temperatures of 25 and 32 degrees C. The colchicine-induced inhibition was not reversed by D2O. Cytochalasin B, which gives a variable enhancement of IgE-mediated <span class="hlt">release</span>, had a marked enhancing effect on the serum-induced reaction in all subjects tested. The following agents known to inhibit the IgE-mediated reaction also inhibited serum-induced <span class="hlt">release</span> at 25 degrees C: colchicine, dibutyryl cyclic AMP, aminophylline, isoproterenol, cholera toxin, chlorphenesin, diethylcarbamazine, and 2-deoxy-D-glucose. These results suggest that the serum-induced <span class="hlt">release</span> is modulated by intracellular cyclic AMP, requires <span class="hlt">energy</span>, and is enhanced by the disruption of microfilaments. The lack of an effect by D2O would suggest that microtubular stabilization is not required. The data can be interpreted to indicate that IgE- and C5a-mediated reactions diverge at a late stage in the histamine <span class="hlt">release</span> pathway.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19750014904','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19750014904"><span>Parametric studies with an atmospheric diffusion model that assesses toxic fuel hazards due to the ground clouds generated by rocket launches</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Stewart, R. B.; Grose, W. L.</p> <p>1975-01-01</p> <p>Parametric studies were made with a multilayer atmospheric diffusion model to place quantitative limits on the uncertainty of predicting ground-level toxic rocket-fuel concentrations. Exhaust distributions in the ground cloud, cloud stabilized geometry, atmospheric coefficients, the effects of exhaust plume <span class="hlt">afterburning</span> of carbon monoxide CO, assumed surface mixing-layer division in the model, and model sensitivity to different meteorological regimes were studied. Large-scale differences in ground-level predictions are quantitatively described. Cloud alongwind growth for several meteorological conditions is shown to be in error because of incorrect application of previous diffusion theory. In addition, rocket-plume calculations indicate that almost all of the rocket-motor carbon monoxide is <span class="hlt">afterburned</span> to carbon dioxide CO2, thus reducing toxic hazards due to CO. The <span class="hlt">afterburning</span> is also shown to have a significant effect on cloud stabilization height and on ground-level concentrations of exhaust products.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li class="active"><span>19</span></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_19 --> <div id="page_20" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li class="active"><span>20</span></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="381"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19950038654&hterms=hydrodynamic+electron+flow&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26Nf%3DPublication-Date%257CBTWN%2B19900101%2B20001231%26N%3D0%26No%3D90%26Ntt%3Dhydrodynamic%2Belectron%2Bflow','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19950038654&hterms=hydrodynamic+electron+flow&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26Nf%3DPublication-Date%257CBTWN%2B19900101%2B20001231%26N%3D0%26No%3D90%26Ntt%3Dhydrodynamic%2Belectron%2Bflow"><span><span class="hlt">Energy</span> transport and dynamics</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Schmieder, Brigitte; Peres, Giovanni; Enome, Shinzo; Falciani, Roberto; Heinzel, Petr; Henoux, Jean-Claude; Mariska, John T.; Reale, Fabio; Rilee, Mike L.; Rompolt, Bogdan</p> <p>1994-01-01</p> <p>We report findings concerning <span class="hlt">energy</span> transport and dynamics in flares during the impulsive and gradual phases based on new ground-based and space observations (notably from Yohkoh). A preheating sometimes occurs during the impulsive phase. Ca XIX line shifts are confirmed to be good tracers of bulk plasma motions, although strong blue shifts are not as frequent as previously claimed. They often appear correlated with hard X-rays but, for some events, the concept that electron beams provide the whole <span class="hlt">energy</span> input to the thermal component seems not to apply. Theory now yields: new diagnostics of low-<span class="hlt">energy</span> proton and electric beams; accurate hydrodynamical modeling of pulse beam heating of the atmosphere; possible diagnostics of microflares (based on X-ray line ratio or on loop variability); and simulated images of chromospheric evaporation fronts. For the gradual phase, the continual reorganization of magnetic field lines over active regions determines where and when magnetic reconnection, the mechanism favored for <span class="hlt">energy</span> <span class="hlt">release</span>, will occur. Spatial and temporal fragmentation of the <span class="hlt">energy</span> <span class="hlt">release</span>, observed at different wavelengths, is considered to be a factor as well in <span class="hlt">energy</span> transport and plasma dynamics.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2008PhDT.......100F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2008PhDT.......100F"><span>Sol-gel encapsulation for controlled drug <span class="hlt">release</span> and biosensing</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Fang, Jonathan</p> <p></p> <p>The main focus of this dissertation is to investigate the use of sol-gel encapsulation of biomolecules for controlled drug <span class="hlt">release</span> and biosensing. Controlled drug <span class="hlt">release</span> has advantages over conventional therapies in that it maintains a constant, therapeutic drug level in the body for prolonged periods of time. The anti-hypertensive drug Captopril was encapsulated in sol-gel materials of various forms, such as silica xerogels and nanoparticles. The primary objective was to show that sol-gel silica materials are promising drug carriers for controlled <span class="hlt">release</span> by <span class="hlt">releasing</span> Captopril at a <span class="hlt">release</span> rate that is within a therapeutic range. We were able to demonstrate desired <span class="hlt">release</span> for over a week from Captopril-doped silica xerogels and overall <span class="hlt">release</span> from Captopril-doped silica nanoparticles. As an aside, the antibiotic Vancomycin was also encapsulated in these porous silica nanoparticles and desired <span class="hlt">release</span> was obtained for several days in-vitro. The second part of the dissertation focuses on immobilizing antibodies and proteins in sol-gel to detect various analytes, such as hormones and amino acids. Sol-gel competitive immunoassays on antibody-doped silica xerogels were used for hormone detection. Calibration for insulin and C-peptide in standard solutions was obtained in the nM range. In addition, NASA-Ames is also interested in developing a reagentless biosensor using bacterial periplasmic binding proteins (bPBPs) to detect specific biomarkers, such as amino acids and phosphate. These bPBPs were doubly labeled with two different fluorophores and encapsulated in silica xerogels. Ligand-binding experiments were performed on the bPBPs in solution and in sol-gel. Ligand-binding was monitored by fluorescence resonance <span class="hlt">energy</span> transfer (FRET) between the two fluorophores on the bPBP. Titration data show that one bPBP has retained its ligand-binding properties in sol-gel.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/7253429','DOE-PATENT-XML'); return false;" href="https://www.osti.gov/biblio/7253429"><span>Method and apparatus for thermal <span class="hlt">energy</span> storage. [Patent application</span></a></p> <p><a target="_blank" href="http://www.osti.gov/doepatents">DOEpatents</a></p> <p>Gruen, D.M.</p> <p>1975-08-19</p> <p>A method and apparatus for storing <span class="hlt">energy</span> by converting thermal <span class="hlt">energy</span> to potential chemically bound <span class="hlt">energy</span> in which a first metal hydride is heated to dissociation temperature, liberating hydrogen gas which is compressed and reacted with a second metal to form a second metal hydride while <span class="hlt">releasing</span> thermal <span class="hlt">energy</span>. Cooling the first metal while warming the second metal hydride to dissociation temperature will reverse the flow of hydrogen gas back to the first metal, <span class="hlt">releasing</span> additional thermal <span class="hlt">energy</span>. The method and apparatus are particularly useful for the storage and conversion of thermal <span class="hlt">energy</span> from solar heat sources and for the utilization of this <span class="hlt">energy</span> for space heating purposes, such as for homes or offices.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018AcAau.143..193L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018AcAau.143..193L"><span>Mixing and combustion enhancement of Turbocharged Solid Propellant Ramjet</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Liu, Shichang; Li, Jiang; Zhu, Gen; Wang, Wei; Liu, Yang</p> <p>2018-02-01</p> <p>Turbocharged Solid Propellant Ramjet is a new concept engine that combines the advantages of both solid rocket ramjet and Air Turbo Rocket, with a wide operation envelope and high performance. There are three streams of the air, turbine-driving gas and augment gas to mix and combust in the <span class="hlt">afterburner</span>, and the coaxial intake mode of the <span class="hlt">afterburner</span> is disadvantageous to the mixing and combustion. Therefore, it is necessary to carry out mixing and combustion enhancement research. In this study, the numerical model of Turbocharged Solid Propellant Ramjet three-dimensional combustion flow field is established, and the numerical simulation of the mixing and combustion enhancement scheme is conducted from the aspects of head region intake mode to injection method in <span class="hlt">afterburner</span>. The results show that by driving the compressed air to deflect inward and the turbine-driving gas to maintain strong rotation, radial and tangential momentum exchange of the two streams can be enhanced, thereby improving the efficiency of mixing and combustion in the <span class="hlt">afterburner</span>. The method of injecting augment gas in the transverse direction and making sure the injection location is as close as possible to the head region is beneficial to improve the combustion efficiency. The outer combustion flow field of the <span class="hlt">afterburner</span> is an oxidizer-rich environment, while the inner is a fuel-rich environment. To improve the efficiency of mixing and combustion, it is necessary to control the injection velocity of the augment gas to keep it in the oxygen-rich zone of the outer region. The numerical simulation for different flight conditions shows that the optimal mixing and combustion enhancement scheme can obtain high combustion efficiency and have excellent applicability in a wide working range.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4730898','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4730898"><span>Strain <span class="hlt">Release</span> Amination</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Gianatassio, Ryan; Lopchuk, Justin M.; Wang, Jie; Pan, Chung-Mao; Malins, Lara R.; Prieto, Liher; Brandt, Thomas A.; Collins, Michael R.; Gallego, Gary M.; Sach, Neal W.; Spangler, Jillian E.; Zhu, Huichin; Zhu, Jinjiang; Baran, Phil S.</p> <p>2015-01-01</p> <p>To optimize drug candidates, modern medicinal chemists are increasingly turning to an unconventional structural motif: small, strained ring systems. However, the difficulty of introducing substituents such as bicyclo[1.1.1]pentanes, azetidines, or cyclobutanes often outweighs the challenge of synthesizing the parent scaffold itself. Thus, there is an urgent need for general methods to rapidly and directly append such groups onto core scaffolds. Here we report a general strategy to harness the embedded potential <span class="hlt">energy</span> of effectively spring-loaded C–C and C–N bonds with the most oft-encountered nucleophiles in pharmaceutical chemistry, amines. Strain <span class="hlt">release</span> amination can diversify a range of substrates with a multitude of desirable bioisosteres at both the early and late-stages of a synthesis. The technique has also been applied to peptide labeling and bioconjugation. PMID:26816372</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1047928','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/1047928"><span>Assessment of the U.S. Department of <span class="hlt">Energy</span>'s Home <span class="hlt">Energy</span> Scoring Tool</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Roberts, David; Merket, Noel; Polly, Ben</p> <p>2012-07-01</p> <p>The National Renewable <span class="hlt">Energy</span> Laboratory (NREL) conducted a series of assessments of the U.S. Department of <span class="hlt">Energy</span>'s (DOE) proposed Home <span class="hlt">Energy</span> Scoring Tool (HEST). This report is an assessment of the 4/27/2012 <span class="hlt">release</span> of HEST. Predictions of electric and natural gas consumption were compared with weather-normalized utility billing data for a mixture of newer and older homes located in Oregon, Wisconsin, Minnesota, North Carolina and Texas.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016NatSR...636476Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016NatSR...636476Z"><span>Rechargeable calcium phosphate orthodontic cement with sustained ion <span class="hlt">release</span> and re-<span class="hlt">release</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zhang, Ling; Weir, Michael D.; Chow, Laurence C.; Reynolds, Mark A.; Xu, Hockin H. K.</p> <p>2016-11-01</p> <p>White spot lesions (WSL) due to enamel demineralization are major complications for orthodontic treatments. Calcium phosphate (CaP) dental resins with Ca and P ion <span class="hlt">releases</span> are promising for remineralization. However, previous Ca and P <span class="hlt">releases</span> lasted for only weeks. Experimental orthodontic cements were developed using pyromellitic glycerol dimethacrylate (PMGDM) and ethoxylated bisphenol A dimethacrylate (EBPADMA) at mass ratio of 1:1 (PE); and PE plus 10% of 2-hydroxyethyl methacrylate (HEMA) and 5% of bisphenol A glycidyl dimethacrylate (BisGMA) (PEHB). Particles of amorphous calcium phosphate (ACP) were incorporated into PE and PEHB at 40% filler level. Specimens were tested for bracket-enamel shear bond strength, water sorption, CaP <span class="hlt">release</span>, and ion recharge and re-<span class="hlt">release</span>. PEHB+40ACP had higher bracket-enamel bond strength and ion <span class="hlt">release</span> and rechargeability than PE+40ACP. ACP incorporation into the novel orthodontic cement did not adversely affect the bracket-enamel bond strength. Ion <span class="hlt">release</span> and re-<span class="hlt">release</span> from the novel ACP orthodontic cement indicated favorable <span class="hlt">release</span> and re-<span class="hlt">release</span> patterns. The recharged orthodontic cement could <span class="hlt">release</span> CaP ions continuously for four weeks without further recharge. Novel rechargeable orthodontic cement containing ACP was developed with a high bracket-enamel bond strength and the ability to be repeatedly recharged to maintain long-term high levels of CaP ion <span class="hlt">releases</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5093739','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5093739"><span>Rechargeable calcium phosphate orthodontic cement with sustained ion <span class="hlt">release</span> and re-<span class="hlt">release</span></span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Zhang, Ling; Weir, Michael D.; Chow, Laurence C.; Reynolds, Mark A.; Xu, Hockin H. K.</p> <p>2016-01-01</p> <p>White spot lesions (WSL) due to enamel demineralization are major complications for orthodontic treatments. Calcium phosphate (CaP) dental resins with Ca and P ion <span class="hlt">releases</span> are promising for remineralization. However, previous Ca and P <span class="hlt">releases</span> lasted for only weeks. Experimental orthodontic cements were developed using pyromellitic glycerol dimethacrylate (PMGDM) and ethoxylated bisphenol A dimethacrylate (EBPADMA) at mass ratio of 1:1 (PE); and PE plus 10% of 2-hydroxyethyl methacrylate (HEMA) and 5% of bisphenol A glycidyl dimethacrylate (BisGMA) (PEHB). Particles of amorphous calcium phosphate (ACP) were incorporated into PE and PEHB at 40% filler level. Specimens were tested for bracket-enamel shear bond strength, water sorption, CaP <span class="hlt">release</span>, and ion recharge and re-<span class="hlt">release</span>. PEHB+40ACP had higher bracket-enamel bond strength and ion <span class="hlt">release</span> and rechargeability than PE+40ACP. ACP incorporation into the novel orthodontic cement did not adversely affect the bracket-enamel bond strength. Ion <span class="hlt">release</span> and re-<span class="hlt">release</span> from the novel ACP orthodontic cement indicated favorable <span class="hlt">release</span> and re-<span class="hlt">release</span> patterns. The recharged orthodontic cement could <span class="hlt">release</span> CaP ions continuously for four weeks without further recharge. Novel rechargeable orthodontic cement containing ACP was developed with a high bracket-enamel bond strength and the ability to be repeatedly recharged to maintain long-term high levels of CaP ion <span class="hlt">releases</span>. PMID:27808251</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/18495391','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/18495391"><span>Wax-based sustained <span class="hlt">release</span> matrix pellets prepared by a novel freeze pelletization technique II. In vitro drug <span class="hlt">release</span> studies and <span class="hlt">release</span> mechanisms.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Cheboyina, Sreekhar; Wyandt, Christy M</p> <p>2008-07-09</p> <p>A novel freeze pelletization technique was evaluated for the preparation of wax-based sustained <span class="hlt">release</span> matrix pellets. Pellets containing water-soluble drugs were successfully prepared using a variety of waxes. The drug <span class="hlt">release</span> significantly depended on the wax type used and the aqueous drug solubility. The drug <span class="hlt">release</span> decreased as the hydrophobicity of wax increased and the drug <span class="hlt">release</span> increased as the aqueous drug solubility increased. In glyceryl monostearate (GMS) pellets, drug <span class="hlt">release</span> rate decreased as the loading of theophylline increased. On the contrary, the <span class="hlt">release</span> rate increased as the drug loading of diltiazem HCl increased in Precirol pellets. Theophylline at low drug loads existed in a dissolved state in GMS pellets and the <span class="hlt">release</span> followed desorption kinetics. At higher loads, theophylline existed in a crystalline state and the <span class="hlt">release</span> followed dissolution-controlled constant <span class="hlt">release</span> for all the waxes studied. However, with the addition of increasing amounts of Brij 76, theophylline <span class="hlt">release</span> rate increased and the <span class="hlt">release</span> mechanism shifted to diffusion-controlled square root time kinetics. But the <span class="hlt">release</span> of diltiazem HCl from Precirol pellets at all drug loads, followed diffusion-controlled square root time kinetics. Therefore, pellets capable of providing a variety of <span class="hlt">release</span> profiles for different drugs can be prepared using this freeze pelletization technique by suitably modifying the pellet forming matrix compositions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20140006468','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20140006468"><span>A Comparison of Three Algorithms for Orion Drogue Parachute <span class="hlt">Release</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Matz, Daniel A.; Braun, Robert D.</p> <p>2015-01-01</p> <p>The Orion Multi-Purpose Crew Vehicle is susceptible to ipping apex forward between drogue parachute <span class="hlt">release</span> and main parachute in ation. A smart drogue <span class="hlt">release</span> algorithm is required to select a drogue <span class="hlt">release</span> condition that will not result in an apex forward main parachute deployment. The baseline algorithm is simple and elegant, but does not perform as well as desired in drogue failure cases. A simple modi cation to the baseline algorithm can improve performance, but can also sometimes fail to identify a good <span class="hlt">release</span> condition. A new algorithm employing simpli ed rotational dynamics and a numeric predictor to minimize a rotational <span class="hlt">energy</span> metric is proposed. A Monte Carlo analysis of a drogue failure scenario is used to compare the performance of the algorithms. The numeric predictor prevents more of the cases from ipping apex forward, and also results in an improvement in the capsule attitude at main bag extraction. The sensitivity of the numeric predictor to aerodynamic dispersions, errors in the navigated state, and execution rate is investigated, showing little degradation in performance.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19880051672&hterms=direct+energy&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Ddirect%2Benergy','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19880051672&hterms=direct+energy&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Ddirect%2Benergy"><span>The roles of direct input of <span class="hlt">energy</span> from the solar wind and unloading of stored magnetotail <span class="hlt">energy</span> in driving magnetospheric substorms</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Rostoker, G.; Akasofu, S. I.; Baumjohann, W.; Kamide, Y.; Mcpherron, R. L.</p> <p>1987-01-01</p> <p>The contributions to the substorm expansive phase of direct <span class="hlt">energy</span> input from the solar wind and from <span class="hlt">energy</span> stored in the magnetotail which is <span class="hlt">released</span> in an unpredictable manner are considered. Two physical processes for the dispensation of the <span class="hlt">energy</span> input from the solar wind are identified: (1) a driven process in which <span class="hlt">energy</span> supplied from the solar wind is directly dissipated in the ionosphere; and (2) a loading-unloading process in which <span class="hlt">energy</span> from the solar wind is first stored in the magnetotail and then is suddenly <span class="hlt">released</span> to be deposited in the ionosphere. The pattern of substorm development in response to changes in the interplanetary medium has been elucidated for a canonical isolated substorm.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018PhRvC..97f4901S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018PhRvC..97f4901S"><span>Particle production at <span class="hlt">energies</span> available at the CERN Large Hadron Collider within an evolutionary model</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sinyukov, Yu. M.; Shapoval, V. M.</p> <p>2018-06-01</p> <p>The particle yields and particle number ratios in Pb+Pb collisions at the CERN Large Hadron Collider (LHC) <span class="hlt">energy</span> √{sN N}=2.76 TeV are described within the integrated hydrokinetic model (iHKM) at two different equations of state (EoS) for quark-gluon matter and the two corresponding hadronization temperatures T =165 MeV and T =156 MeV. The role of particle interactions at the final <span class="hlt">afterburner</span> stage of the collision in the particle production is investigated by means of comparison of the results of full iHKM simulations with those where the annihilation and other inelastic processes (except for resonance decays) are switched off after hadronization/particlization, similarly as in the thermal models. An analysis supports the picture of continuous chemical freeze-out in the sense that the corrections to the sudden chemical freeze-out results, which arise because of the inelastic reactions at the subsequent evolution times, are noticeable and improve the description of particle number ratios. An important observation is that, although the particle number ratios with switched-off inelastic reactions are quite different at different particlization temperatures which are adopted for different equations of state to reproduce experimental data, the complete iHKM calculations bring very close results in both cases.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5131847','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5131847"><span>Magnetotail <span class="hlt">energy</span> dissipation during an auroral substorm</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Panov, E.V.; Baumjohann, W.; Wolf, R.A.; Nakamura, R.; Angelopoulos, V.; Weygand, J. M.; Kubyshkina, M.V.</p> <p>2016-01-01</p> <p>Violent <span class="hlt">releases</span> of space plasma <span class="hlt">energy</span> from the Earth’s magnetotail during substorms produce strong electric currents and bright aurora. But what modulates these currents and aurora and controls dissipation of the <span class="hlt">energy</span> <span class="hlt">released</span> in the ionosphere? Using data from the THEMIS fleet of satellites and ground-based imagers and magnetometers, we show that plasma <span class="hlt">energy</span> dissipation is controlled by field-aligned currents (FACs) produced and modulated during magnetotail topology change and oscillatory braking of fast plasma jets at 10-14 Earth radii in the nightside magnetosphere. FACs appear in regions where plasma sheet pressure and flux tube volume gradients are non-collinear. Faster tailward expansion of magnetotail dipolarization and subsequent slower inner plasma sheet restretching during substorm expansion and recovery phases cause faster poleward then slower equatorward movement of the substorm aurora. Anharmonic radial plasma oscillations build up displaced current filaments and are responsible for discrete longitudinal auroral arcs that move equatorward at a velocity of about 1km/s. This observed auroral activity appears sufficient to dissipate the <span class="hlt">released</span> <span class="hlt">energy</span>. PMID:27917231</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19870016747','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19870016747"><span>Product <span class="hlt">energy</span> distributions and <span class="hlt">energy</span> partitioning in O atom reactions on surfaces</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Halpern, Bret; Kori, Moris</p> <p>1987-01-01</p> <p>Surface reactions involving O atoms are likely to be highly exoergic, with different consequences if <span class="hlt">energy</span> is channeled mostly to product molecules or surface modes. Thus the surface may become a source of excited species which can react elsewhere, or a sink for localized heat deposition which may disrupt the surface. The vibrational <span class="hlt">energy</span> distribution of the product molecule contains strong clues about the flow of <span class="hlt">released</span> <span class="hlt">energy</span>. Two instructive examples of <span class="hlt">energy</span> partitioning at surfaces are the Pt catalyzed oxidations: (1) C(ads) + O(ads) yields CO* (T is greater than 1000 K); and (2) CO(ads) + O(gas) yields CO2* (T is approx. 300 K). The infrared emission spectra of the excited product molecules were recorded and the vibrational population distributions were determined. In reaction 1, <span class="hlt">energy</span> appeared to be statistically partitioned between the product CO and several Pt atoms. In reaction 2, partitioning was non-statistical; the CO2 asymmetric stretch distribution was inverted. In gas reactions these results would indicate a long lived and short lived activated complex. The requirement that Pt be heated in O atoms to promote reaction of atomic O and CO at room temperature is specifically addressed. Finally, the fraction of <span class="hlt">released</span> <span class="hlt">energy</span> that is deposited in the catalyst is estimated.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/97030','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/97030"><span>Radioactive materials <span class="hlt">released</span> from nuclear power plants. Volume 13, Annual report 1992</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Tichler, J.; Doty, K.; Lucadamo, K.</p> <p></p> <p><span class="hlt">Releases</span> of radioactive materials in airborne and liquid effluents from commercial light water reactors during 1992 have been compiled and reported. The summary data for the years 1973 through 1991 are included for comparison. Data on solid waste shipments as well as selected operating information have been included. This report supplements earlier annual reports issued by the former Atomic <span class="hlt">Energy</span> Commission and the Nuclear Regulatory Commission. The 1992 <span class="hlt">release</span> data are summarized in tabular form. Data covering specific radionuclides are summarized.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/10183473','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/10183473"><span>Radioactive materials <span class="hlt">released</span> from nuclear power plants. Annual report 1989: Volume 10</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Tichler, J.; Norden, K.; Congemi, J.</p> <p></p> <p><span class="hlt">Releases</span> of radioactive materials in airborne and liquid effluents from commercial light water reactors during 1989 have been compiled and reported. The summary data for the years 1970 through 1988 are included for comparison. Data on solid waste shipments as well as selected operating information have been included. This report supplements earlier annual reports issued by the former Atomic <span class="hlt">Energy</span> Commission and the Nuclear Regulatory Commission. The 1989 <span class="hlt">release</span> data are summarized in tabular form. Data covering specific radionuclides are summarized.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/179179','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/179179"><span>Radioactive materials <span class="hlt">released</span> from nuclear power plants: Annual report, 1993. Volume 14</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Tichler, J.; Doty, K.; Lucadamo, K.</p> <p></p> <p><span class="hlt">Releases</span> of radioactive materials in airborne and liquid effluents from commercial light water reactors during 1993 have been compiled and reported. The summary data for the years 1974 through 1992 are included for comparison. Data on solid waste shipments as well as selected operating information have been included. This report supplements earlier annual reports issued by the former Atomic <span class="hlt">Energy</span> Commission and the Nuclear Regulatory Commission. The 1993 <span class="hlt">release</span> data are summarized in tabular form. Data covering specific radionuclides are summarized.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017PhRvF...2f4802K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017PhRvF...2f4802K"><span>Partial-depth lock-<span class="hlt">release</span> flows</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Khodkar, M. A.; Nasr-Azadani, M. M.; Meiburg, E.</p> <p>2017-06-01</p> <p>We extend the vorticity-based modeling concept for stratified flows introduced by Borden and Meiburg [Z. Borden and E. Meiburg, J. Fluid Mech. 726, R1 (2013), 10.1017/jfm.2013.239] to unsteady flow fields that cannot be rendered quasisteady by a change of reference frames. Towards this end, we formulate a differential control volume balance for the conservation of mass and vorticity in the fully unsteady parts of the flow, which we refer to as the differential vorticity model. We furthermore show that with the additional assumptions of locally uniform parallel flow within each layer, the unsteady vorticity modeling approach reproduces the familiar two-layer shallow-water equations. To evaluate its accuracy, we then apply the vorticity model approach to partial-depth lock-<span class="hlt">release</span> flows. Consistent with the shallow water analysis of Rottman and Simpson [J. W. Rottman and J. E. Simpson, J. Fluid Mech. 135, 95 (1983), 10.1017/S0022112083002979], the vorticity model demonstrates the formation of a quasisteady gravity current front, a fully unsteady expansion wave, and a propagating bore that is present only if the lock depth exceeds half the channel height. When this bore forms, it travels with a velocity that does not depend on the lock height and the interface behind it is always at half the channel depth. We demonstrate that such a bore is <span class="hlt">energy</span> conserving. The differential vorticity model gives predictions for the height and velocity of the gravity current and the bore, as well as for the propagation velocities of the edges of the expansion fan, as a function of the lock height. All of these predictions are seen to be in good agreement with the direct numerical simulation data and, where available, with experimental results. An <span class="hlt">energy</span> analysis shows lock-<span class="hlt">release</span> flows to be <span class="hlt">energy</span> conserving only for the case of a full lock, whereas they are always dissipative for partial-depth locks.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/24978099','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/24978099"><span>Observations of the <span class="hlt">release</span> of non-methane hydrocarbons from fractured shale.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Sommariva, Roberto; Blake, Robert S; Cuss, Robert J; Cordell, Rebecca L; Harrington, Jon F; White, Iain R; Monks, Paul S</p> <p>2014-01-01</p> <p>The organic content of shale has become of commercial interest as a source of hydrocarbons, owing to the development of hydraulic fracturing ("fracking"). While the main focus is on the extraction of methane, shale also contains significant amounts of non-methane hydrocarbons (NMHCs). We describe the first real-time observations of the <span class="hlt">release</span> of NMHCs from a fractured shale. Samples from the Bowland-Hodder formation (England) were analyzed under different conditions using mass spectrometry, with the objective of understanding the dynamic process of gas <span class="hlt">release</span> upon fracturing of the shale. A wide range of NMHCs (alkanes, cycloalkanes, aromatics, and bicyclic hydrocarbons) are <span class="hlt">released</span> at parts per million or parts per billion level with temperature- and humidity-dependent <span class="hlt">release</span> rates, which can be rationalized in terms of the physicochemical characteristics of different hydrocarbon classes. Our results indicate that higher <span class="hlt">energy</span> inputs (i.e., temperatures) significantly increase the amount of NMHCs <span class="hlt">released</span> from shale, while humidity tends to suppress it; additionally, a large fraction of the gas is <span class="hlt">released</span> within the first hour after the shale has been fractured. These findings suggest that other hydrocarbons of commercial interest may be extracted from shale and open the possibility to optimize the "fracking" process, improving gas yields and reducing environmental impacts.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1169641','DOE-PATENT-XML'); return false;" href="https://www.osti.gov/servlets/purl/1169641"><span>Systems and methods for solar <span class="hlt">energy</span> storage, transportation, and conversion utilizing photochemically active organometallic isomeric compounds and solid-state catalysts</span></a></p> <p><a target="_blank" href="http://www.osti.gov/doepatents">DOEpatents</a></p> <p>Vollhardt, K. Peter C.; Segalman, Rachel A; Majumdar, Arunava; Meier, Steven</p> <p>2015-02-10</p> <p>A system for converting solar <span class="hlt">energy</span> to chemical <span class="hlt">energy</span>, and, subsequently, to thermal <span class="hlt">energy</span> includes a light-harvesting station, a storage station, and a thermal <span class="hlt">energy</span> <span class="hlt">release</span> station. The system may include additional stations for converting the <span class="hlt">released</span> thermal <span class="hlt">energy</span> to other <span class="hlt">energy</span> forms, e.g., to electrical <span class="hlt">energy</span> and mechanical work. At the light-harvesting station, a photochemically active first organometallic compound, e.g., a fulvalenyl diruthenium complex, is exposed to light and is photochemically converted to a second, higher-<span class="hlt">energy</span> organometallic compound, which is then transported to a storage station. At the storage station, the high-<span class="hlt">energy</span> organometallic compound is stored for a desired time and/or is transported to a desired location for thermal <span class="hlt">energy</span> <span class="hlt">release</span>. At the thermal <span class="hlt">energy</span> <span class="hlt">release</span> station, the high-<span class="hlt">energy</span> organometallic compound is catalytically converted back to the photochemically active organometallic compound by an exothermic process, while the <span class="hlt">released</span> thermal <span class="hlt">energy</span> is captured for subsequent use.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li class="active"><span>20</span></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_20 --> <div id="page_21" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li class="active"><span>21</span></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="401"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20010055267','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20010055267"><span><span class="hlt">Energy</span> Absorbing Protective Shroud</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Schneider, William C. (Inventor)</p> <p>2001-01-01</p> <p>The present invention is a dissipating protection <span class="hlt">energy</span> system designed to receive and safely dissipate the kinetic <span class="hlt">energy</span> from high <span class="hlt">energy</span> fragments. The <span class="hlt">energy</span> dissipation system dissipates <span class="hlt">energy</span> transferred to it by the incremental and progressive rupturing at an approximately constant force of strategically placed sacrificial stitching applied to a number of high strength straps, such as an aromatic polyimide fiber of extremely high tensile strength. Thus, the <span class="hlt">energy</span> dissipation system provides a lightweight device for controlling and dissipating the dangerous and destructive <span class="hlt">energy</span> stored in high strength fragments <span class="hlt">released</span> by catastrophic failures of machinery minimizing damage to other critical components.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=1574041','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=1574041"><span>Lack of CB1 receptors increases noradrenaline <span class="hlt">release</span> in vas deferens without affecting atrial noradrenaline <span class="hlt">release</span> or cortical acetylcholine <span class="hlt">release</span></span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Schlicker, Eberhard; Redmer, Agnes; Werner, André; Kathmann, Markus</p> <p>2003-01-01</p> <p>We studied whether cannabinoid CB1 receptor gene disruption (to yield CB1−/− mice) affects the electrically evoked tritium overflow from vas deferens and atrial pieces preincubated with [3H]-noradrenaline (NA) (‘noradrenaline <span class="hlt">release</span>') and from cerebral cortex slices preincubated with [3H]-choline (‘acetylcholine <span class="hlt">release</span>'). NA <span class="hlt">release</span> was higher by 37% in vas deferens from CB1−/− mice than in vas deferens from CB1+/+ mice. The cannabinoid receptor agonist WIN 55,212-2 inhibited, and the CB1 receptor inverse agonist/antagonist SR 141716, increased NA <span class="hlt">release</span> in vas deferens from CB1+/+ mice without affecting it in vas deferens from CB1−/− mice. Atrial NA <span class="hlt">release</span> did not differ between CB1+/+ and CB1−/− mice nor did WIN 55,212-2 affect NA <span class="hlt">release</span> in either strain. Cortical acetylcholine (Ach) <span class="hlt">release</span> did not differ between CB1+/+ and CB1−/− mice. WIN 55,212-2 inhibited, but SR 141716 did not affect, Ach <span class="hlt">release</span> in the cortex from CB1+/+ mice. Both drugs did not alter Ach <span class="hlt">release</span> in the cortex from CB1−/− mice. Tritium content did not differ between CB1+/+ and CB1−/− mice in any preparation. In conclusion, the increase in NA <span class="hlt">release</span> associated with CB1 receptor deficiency in the vas deferens, which cannot be ascribed to an alteration of tritium content of the preparations, suggests an endogenous tone at the CB1 receptors of CB1+/+ mice in this tissue. Furthermore, the effect of WIN 55,212-2 on NA <span class="hlt">release</span> in the vas deferens and on cortical Ach <span class="hlt">release</span> involves CB1 receptors, whereas the involvement of non-CB1–non-CB2 receptors can be excluded. PMID:12970076</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMNH21C0187H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMNH21C0187H"><span>Electromagnetic <span class="hlt">Energy</span> <span class="hlt">Released</span> in the Subduction (Benioff) Zone in Weeks Previous to Earthquake Occurrence in Central Peru and the Estimation of Earthquake Magnitudes.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Heraud, J. A.; Centa, V. A.; Bleier, T.</p> <p>2017-12-01</p> <p>During the past four years, magnetometers deployed in the Peruvian coast have been providing evidence that the ULF pulses received are indeed generated at the subduction or Benioff zone and are connected with the occurrence of earthquakes within a few kilometers of the source of such pulses. This evidence was presented at the AGU 2015 Fall meeting, showing the results of triangulation of pulses from two magnetometers located in the central area of Peru, using data collected during a two-year period. Additional work has been done and the method has now been expanded to provide the instantaneous <span class="hlt">energy</span> <span class="hlt">released</span> at the stress areas on the Benioff zone during the precursory stage, before an earthquake occurs. Collected data from several events and in other parts of the country will be shown in a sequential animated form that illustrates the way <span class="hlt">energy</span> is <span class="hlt">released</span> in the ULF part of the electromagnetic spectrum. The process has been extended in time and geographical places. Only pulses associated with the occurrence of earthquakes are taken into account in an area which is highly associated with subduction-zone seismic events and several pulse parameters have been used to estimate a function relating the magnitude of the earthquake with the value of a function generated with those parameters. The results shown, including the animated data video, constitute additional work towards the estimation of the magnitude of an earthquake about to occur, based on electromagnetic pulses that originated at the subduction zone. The method is providing clearer evidence that electromagnetic precursors in effect conveys physical and useful information prior to the advent of a seismic event</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016Tectp.682..147V','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016Tectp.682..147V"><span>Stress <span class="hlt">release</span> model and proxy measures of earthquake size. Application to Italian seismogenic sources</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Varini, Elisa; Rotondi, Renata; Basili, Roberto; Barba, Salvatore</p> <p>2016-07-01</p> <p>This study presents a series of self-correcting models that are obtained by integrating information about seismicity and fault sources in Italy. Four versions of the stress <span class="hlt">release</span> model are analyzed, in which the evolution of the system over time is represented by the level of strain, moment, seismic <span class="hlt">energy</span>, or <span class="hlt">energy</span> scaled by the moment. We carry out the analysis on a regional basis by subdividing the study area into eight tectonically coherent regions. In each region, we reconstruct the seismic history and statistically evaluate the completeness of the resulting seismic catalog. Following the Bayesian paradigm, we apply Markov chain Monte Carlo methods to obtain parameter estimates and a measure of their uncertainty expressed by the simulated posterior distribution. The comparison of the four models through the Bayes factor and an information criterion provides evidence (to different degrees depending on the region) in favor of the stress <span class="hlt">release</span> model based on the <span class="hlt">energy</span> and the scaled <span class="hlt">energy</span>. Therefore, among the quantities considered, this turns out to be the measure of the size of an earthquake to use in stress <span class="hlt">release</span> models. At any instant, the time to the next event turns out to follow a Gompertz distribution, with a shape parameter that depends on time through the value of the conditional intensity at that instant. In light of this result, the issue of forecasting is tackled through both retrospective and prospective approaches. Retrospectively, the forecasting procedure is carried out on the occurrence times of the events recorded in each region, to determine whether the stress <span class="hlt">release</span> model reproduces the observations used in the estimation procedure. Prospectively, the estimates of the time to the next event are compared with the dates of the earthquakes that occurred after the end of the learning catalog, in the 2003-2012 decade.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20020024843&hterms=ssto&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Dssto','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20020024843&hterms=ssto&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Dssto"><span>Feasibility Study of SSTO Base Heating Simulation in Pulsed-Type Facilities</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Park, Chung Sik; Sharma, Surendra; Edwards, Thomas A. (Technical Monitor)</p> <p>1995-01-01</p> <p>A laboratory simulation of the base heating environment of the proposed reusable Single-Stage-To-Orbit vehicle during its ascent flight was proposed. The rocket engine produces CO2 and H2, which are the main combustible components of the exhaust effluent. The burning of these species, known as <span class="hlt">afterburning</span>, enhances the base region gas temperature as well as the base heating. To determine the heat flux on the SSTO vehicle, current simulation focuses on the thermochemistry of the <span class="hlt">afterburning</span>, thermophysical properties of the base region gas, and ensuing radiation from the gas. By extrapolating from the Saturn flight data, the Damkohler number for the <span class="hlt">afterburning</span> of SSTO vehicle is estimated to be of the order of 10. The limitations on the material strengths limit the laboratory simulation of the flight Damkohler number as well as other flow parameters. A plan is presented in impulse facilities using miniature rocket engines which generate the simulated rocket plume by electric ally-heating a H2/CO2 mixture.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20020033017&hterms=Combustible&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D70%26Ntt%3DCombustible','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20020033017&hterms=Combustible&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D70%26Ntt%3DCombustible"><span>Feasibility Study of Laboratory Simulation of Single-Stage-to-Orbit Vehicle Base Heating</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Park, Chung Sik; Sharma, Surendra; Edwards, Thomas A. (Technical Monitor)</p> <p>1995-01-01</p> <p>The feasibility of simulating in a laboratory the heating environment of the base region of the proposed reusable single-stage-to-orbit vehicle during its ascent is examined. The propellant is assumed to consist of hydrocarbon (RP1), liquid hydrogen (LH2), and liquid oxygen (LO2), which produces CO and H2 as the main combustible components of the exhaust effluent. Since <span class="hlt">afterburning</span> in the recirculating region can dictate the temperature of the base flowfield and ensuing heating phenomena, laboratory simulation focuses on the thermochemistry of the <span class="hlt">afterburning</span>. By extrapolating the Saturn V flight data, the Damkohler number, in the base region with <span class="hlt">afterburning</span> for SSTO vehicle, is estimated to be between 30 and 140. It is shown that a flow with a Damkohler number of 1.8 to 25 can be produced in an impulse ground test facility. Even with such a reduced Damkohler number, the experiment can adequately reproduce the main features of the flight environment.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/6057821-alternative-fuels-multiple-hearth-furnaces','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/6057821-alternative-fuels-multiple-hearth-furnaces"><span>Alternative fuels for multiple-hearth furnaces</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Bracken, B.D.; Lawson, T.U.</p> <p>1980-04-01</p> <p>A study of alternative procedures for reducing the consumption of No. 2 fuel oil at the Lower Molonglo Water Quality Control Centre near Canberra, Aust., indicated that in comparison with the present system of incineration with heat supplied by burning fuel oil, the installation of a sludge drying operation, consisting of a rotary dryer heated by furnace exhaust gases with the dried sludge used to fuel the furnace, would become economically desirable by 1985 if <span class="hlt">afterburning</span> is not required, and would be justified immediately if <span class="hlt">afterburning</span> is required to meet air pollution control regulations. The substitution of any of fourmore » waste fuels (refuse-derived fuel, waste paper, wood waste, or waste oil) or of coal for the No. 2 fuel oil would not be cost-effective through 1989. The furnace system, including <span class="hlt">afterburning</span> and fuel oil requirements, the envisioned alternative fuel use systems, sludge processing alternatives, heat balance results, and economics are discussed.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/5661843-leading-edge-combining-maturity-advanced-technology-f404-turbofan-engine','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/5661843-leading-edge-combining-maturity-advanced-technology-f404-turbofan-engine"><span>On the leading edge; Combining maturity and advanced technology on the F404 turbofan engine</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Powel, S.F. IV</p> <p>1991-01-01</p> <p>In this paper the overall design concept of the F404 <span class="hlt">afterburning</span> turbofan engine is reviewed together with some of the lessons learned from over 2 million flight hours in service. GE Aircraft Engines' derivative and growth plans for the F404 family are then reviewed including the Building Block component development approach. Examples of advanced technologies under development for introduction into new F404 derivative engine models are presented in the areas of materials, digital and fiber optic controls systems, and vectoring exhaust nozzles. The design concept and details of the F404-GE-402, F412-GE-400, and other derivative engines under full-scale development are described.more » Studies for future growth variants and the benefits of the F404 derivative approach to development of <span class="hlt">afterburning</span> engines in the 18,000-24,000 lb (80--107 kN) thrust class and non- <span class="hlt">afterburning</span> engines in the 12,000--19,000 lb (53--85 kN) class are discussed.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMMR12A..02Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMMR12A..02Z"><span>Mechanisms of iodine <span class="hlt">release</span> from iodoapatite in aqueous solution</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zhang, Z.; Wang, J.</p> <p>2017-12-01</p> <p>Immobilization of iodine-129 with waste forms in geological setting is challenging due to its extremely long half-life and high volatility in the environment. To evaluate the long-term performance of waste form, it is imperative to determine the <span class="hlt">release</span> mechanism of iodine hosted in the waste form materials. This study investigated the iodine <span class="hlt">released</span> from apatite structured waste form Pb9.85 (VO4)6 I1.7 to understand how diffusion and dissolution control the durability of apatite waste form. A standard semi-dynamic leach test was adopted in this study. Samples were exposed in fresh leachant periodically and the leachant was replaced after each interval. Each experiment was carried out in cap-sealed Teflon vessels under constant temperature (e.g. 90 °C). ICP-MS analysis on the reacted leachates shows that Pb and V were <span class="hlt">released</span> constantly and congruently with the stoichiometric ratio of Pb/V. However, iodine <span class="hlt">release</span> is incongruent and time dependent. The iodine <span class="hlt">release</span> rate starts significantly higher than the corresponding stoichiometric value and gradually decreases, approaching the stoichiometric value. Therefore, a dual-mode mechanism is proposed to account for the iodine <span class="hlt">release</span> from apatite, which is dominated by short-term diffusion and long-term dissolution processes. Additional tests show that the element <span class="hlt">release</span> rates depend on a number of test parameters, including sample surface to solution volume ratio (m-1), interval (day), temperature (°C), and solution pH. This study provides a quantitative characterization of iodine <span class="hlt">release</span> mechanism. The activation <span class="hlt">energy</span> of iodine leaching 21±1.6 kJ/mol was obtained by varying the test temperature. At the test conditions of to neutral pH and 90 °C, the long-term iodine <span class="hlt">release</span> rate 3.3 mg/(m2 • day) is projected by normalizing sample surface area to solution volume ratio (S/V) to 1.0 m-1 and interval to 1 day. These findings demonstrate i) the feasibility of our approach to quantify the <span class="hlt">release</span> mechanism</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012A%26A...540A..24B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012A%26A...540A..24B"><span>Using SDO's AIA to investigate <span class="hlt">energy</span> transport from a flare's <span class="hlt">energy</span> <span class="hlt">release</span> site to the chromosphere</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Brosius, J. W.; Holman, G. D.</p> <p>2012-04-01</p> <p>Context. Coordinated observations of a GOES B4.8 microflare with SDO's Atmospheric Imaging Assembly (AIA) and the Ramaty High <span class="hlt">Energy</span> Solar Spectroscopic Imager (RHESSI) on 2010 July 31 show that emission in all seven of AIA's EUV channels brightened simultaneously nearly 6 min before RHESSI or GOES detected emission from plasma at temperatures around 10 MK. Aims: To help interpret these and AIA flare observations in general, we characterized the expected temporal responses of AIA's 94, 131, 171, 193, 211, and 335 Å channels to solar flare brightenings by combining (1) AIA's nominal temperature response functions available through SSWIDL with (2) EUV spectral line data observed in a flare loop footpoint on 2001 April 24 with the Coronal Diagnostic Spectrometer (CDS) on timescales comparable to AIA's image cadence. Methods: The nine emission lines observed by CDS cover a wide range of formation temperature from about 0.05 to 8 MK. Line brightenings observed early during the CDS flare occurred at temperatures less than about 0.7 MK, with the largest values around 0.1 MK. These brightenings were consistent with the flare's <span class="hlt">energy</span> transport being dominated by nonthermal particle beams. Because all of AIA's EUV channels are sensitive to emission from plasma in the 0.1 to 0.7 MK temperature range, we show that all of AIA's EUV channels will brighten simultaneously during flares like this, in which <span class="hlt">energy</span> transport is dominated by nonthermal particle beams. Results: The 2010 July 31 flare observed by AIA and RHESSI displays this behavior, so we conclude that such beams likely dominated the flare's <span class="hlt">energy</span> transport early during the event. When thermal conduction from a reconnection-heated, hot (~10 MK) plasma dominates the <span class="hlt">energy</span> transport, the AIA channels that are sensitive to emission from such temperatures (particularly the 94 and 131 Å channels) will brighten earlier than the channels that are not sensitive to such temperatures (171 and 211 Å). Conclusions: Thus</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2008AIPC..973..907N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2008AIPC..973..907N"><span>Multicomponent Implant <span class="hlt">Releasing</span> Dexamethasone</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Nikkola, L.; Vapalahti, K.; Ashammakhi, N.</p> <p>2008-02-01</p> <p>Several inflammatory conditions are usually treated with corticosteroids. There are various problems like side effects with traditional applications of steroids, e.g. topical, or systemic routes. Local drug delivery systems have been studied and developed to gain more efficient administration with fewer side effects. Earlier, we reported on developing Dexamethasone (DX) <span class="hlt">releasing</span> biodegradable fibers. However, their drug <span class="hlt">release</span> properties were not satisfactory in terms of onset of drug <span class="hlt">release</span>. Thus, we assessed the development of multicomponent (MC) implant to enhance earlier drug <span class="hlt">release</span> from such biodegradable fibers. Poly (lactide-co-glycolide) (PLGA) and 2 wt-% and 8 wt-% DX were compounded and extruded with twin-screw extruder to form of fibers. Some of the fibers were sterilized to obtain a change in drug <span class="hlt">release</span> properties. Four different fiber classes were studied: 2 wt-%, 8 wt-%, sterilized 2 wt-%, and sterilized 8 wt-%. 3×4 different DX-<span class="hlt">releasing</span> fibers were then heat-pressed to form one multicomponent rod. Half of the rods where sterilized. Drug <span class="hlt">release</span> was measured from initial fibers and multicomponent rods using a UV/VIS spectrometer. Shear strength and changes in viscosity were also measured. Drug <span class="hlt">release</span> studies showed that drug <span class="hlt">release</span> commenced earlier from multicomponent rods than from component fibers. Drug <span class="hlt">release</span> from multicomponent rods lasted from day 30 to day 70. The <span class="hlt">release</span> period of sterilized rods extended from day 23 to day 57. When compared to the original component fibers, the drug <span class="hlt">release</span> from MC rods commenced earlier. The initial shear strength of MC rods was 135 MPa and decreased to 105 MPa during four weeks of immersion in phosphate buffer solution. Accordingly, heat pressing has a positive effect on drug <span class="hlt">release</span>. After four weeks in hydrolysis, no disintegration was observed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3048762','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3048762"><span>Bone Cell–materials Interactions and Ni Ion <span class="hlt">Release</span> of Anodized Equiatomic NiTi Alloy</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Bernard, Sheldon A.; Balla, Vamsi Krishna; Davies, Neal M.; Bose, Susmita; Bandyopadhyay, Amit</p> <p>2011-01-01</p> <p>Laser processed NiTi alloy was anodized for different durations in H2SO4 electrolyte with varying pH to create biocompatible surfaces with low Ni ion <span class="hlt">release</span> as well as bioactive surfaces to enhance biocompatibility and bone cell-materials interactions. The anodized surfaces were assessed for their in vitro cell-materials interactions using human fetal osteoblast (hFOB) cells for 3, 7 and 11 days, and Ni ion <span class="hlt">release</span> up to 8 weeks in simulated body fluids. The results were correlated with surface morphologies of anodized surfaces characterized using field-emission scanning electron microscopy (FESEM). The results show that the anodization creates a surface with nano/micro roughness depending on anodization conditions. The hydrophilicity of NiTi surface was found to improve after anodization due to lower contact angles in cell media, which dropped from 32° to < 5°. The improved wettability of anodized surfaces is further corroborated by their high surface <span class="hlt">energy</span> comparable to that of cp Ti. Relatively high surface <span class="hlt">energy</span>, especially polar component, and nano/micro surface features of anodized surfaces significantly increased the number of living cells and their adherence and growth on these surfaces. Finally, a significant drop in Ni ion <span class="hlt">release</span> from 268 ± 11 to 136 ± 15 ppb was observed for NiTi surfaces after anodization. This work indicates that anodization of NiTi alloy has a positive influence on the surface <span class="hlt">energy</span> and surface morphology, which in turn improve bone cell-materials interactions and reduce Ni ion <span class="hlt">release</span> in vitro. PMID:21232641</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19810006442','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19810006442"><span>Chemical <span class="hlt">release</span> module facility</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Reasoner, D. L.</p> <p>1980-01-01</p> <p>The chemical <span class="hlt">release</span> module provides the capability to conduct: (1) thermite based metal vapor <span class="hlt">releases</span>; (2) pressurized gas <span class="hlt">releases</span>; (3) dispersed liquid <span class="hlt">releases</span>; (4) shaped charge <span class="hlt">releases</span> from ejected submodules; and (5) diagnostic measurements with pi supplied instruments. It also provides a basic R-F and electrical system for: (1) receiving and executing commands; (2) telemetering housekeeping data; (3) tracking; (4) monitoring housekeeping and control units; and (5) ultrasafe disarming and control monitoring.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1993graz.iafcQR...K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1993graz.iafcQR...K"><span>Solar thermal rocket engine (STRE) thrust characteristics at the change of engine operation mode and of the flight vehicle attitude in the solar system</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kudrin, O. I.</p> <p>1993-10-01</p> <p>Relationships are presented which describe changes in the thrust and specific impulse of a solar thermal rocket engine due to a change in the flow rate of the working fluid (hydrogen). Expressions are also presented which describe the variation of the STRE thrust and specific impulse with the distance between the flight vehicle and the sun. Results of calculations are presented for an STRE with <span class="hlt">afterburning</span> of the working fluid (hydrogen + oxygen) using hydrogen heating by solar <span class="hlt">energy</span> to a temperature of 2360 K.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.eia.gov/consumption/archive/rtecs/nhts_survey/2001/','EIAPUBS'); return false;" href="https://www.eia.gov/consumption/archive/rtecs/nhts_survey/2001/"><span>Household Vehicles <span class="hlt">Energy</span> Use: Latest Data and Trends</span></a></p> <p><a target="_blank" href="http://www.eia.doe.gov/reports/">EIA Publications</a></p> <p></p> <p>2005-01-01</p> <p>This report provides newly available national and regional data and analyzes the nation's <span class="hlt">energy</span> use by light-duty vehicles. This <span class="hlt">release</span> represents the analytical component of the report, with a data component having been <span class="hlt">released</span> in early 2005.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/1130682-quantification-kinetic-rate-law-parameters-uranium-release-from-sodium-autunite-function-aqueous-bicarbonate-concentrations','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/1130682-quantification-kinetic-rate-law-parameters-uranium-release-from-sodium-autunite-function-aqueous-bicarbonate-concentrations"><span>Quantification of Kinetic Rate Law Parameters of Uranium <span class="hlt">Release</span> from Sodium Autunite as a Function of Aqueous Bicarbonate Concentrations</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Gudavalli, Ravi; Katsenovich, Yelena; Wellman, Dawn M.</p> <p>2013-09-05</p> <p>ABSTRACT: Hydrogen carbonate is one of the most significant components within the uranium geochemical cycle. In aqueous solutions, hydrogen carbonate forms strong complexes with uranium. As such, aqueous bicarbonate may significantly increase the rate of uranium <span class="hlt">release</span> from uranium minerals. Quantifying the relationship of aqueous hydrogen carbonate solutions to the rate of uranium <span class="hlt">release</span> during dissolution is critical to understanding the long-term fate of uranium within the environment. Single-pass flow-through (SPTF) experiments were conducted to estimate the rate of uranium <span class="hlt">release</span> from Na meta-autunite as a function of bicarbonate solutions (0.0005-0.003 M) under the pH range of 6-11 and temperaturesmore » of 5-60oC. Consistent with the results of previous investigation, the rate of uranium <span class="hlt">release</span> from sodium autunite exhibited minimal dependency on temperature; but were strongly dependent on pH and increasing concentrations of bicarbonate solutions. Most notably at pH 7, the rate of uranium <span class="hlt">release</span> exhibited 370 fold increases relative to the rate of uranium <span class="hlt">release</span> in the absence of bicarbonate. However, the effect of increasing concentrations of bicarbonate solutions on the <span class="hlt">release</span> of uranium was significantly less under higher pH conditions. It is postulated that at high pH values, surface sites are saturated with carbonate, thus the addition of more bicarbonate would have less effect on uranium <span class="hlt">release</span>. Results indicate the activation <span class="hlt">energies</span> were unaffected by temperature and bicarbonate concentration variations, but were strongly dependent on pH conditions. As pH increased from 6 to 11, activation <span class="hlt">energy</span> values were observed to decrease from 29.94 kJ mol-1 to 13.07 kJ mol-1. The calculated activation <span class="hlt">energies</span> suggest a surface controlled dissolution mechanism.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1399265','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/1399265"><span>Hawaii <span class="hlt">Energy</span> Sustainable Program</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Rocheleau, Richard; Turn, Scott; Griffin, James</p> <p></p> <p>The objective of HESP was to support the development and deployment of distributed <span class="hlt">energy</span> resource (DER) technologies to facilitate increased penetration of renewable <span class="hlt">energy</span> resources and reduced use of fossil fuels in Hawaii’s power grids. All deliverables, publications and other public <span class="hlt">releases</span> have been submitted to the DOE in accordance with the award and subsequent award modifications.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19940008670','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19940008670"><span>Analysis of gas turbine engines using water and oxygen injection to achieve high Mach numbers and high thrust</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Henneberry, Hugh M.; Snyder, Christopher A.</p> <p>1993-01-01</p> <p>An analysis of gas turbine engines using water and oxygen injection to enhance performance by increasing Mach number capability and by increasing thrust is described. The liquids are injected, either separately or together, into the subsonic diffuser ahead of the engine compressor. A turbojet engine and a mixed-flow turbofan engine (MFTF) are examined, and in pursuit of maximum thrust, both engines are fitted with <span class="hlt">afterburners</span>. The results indicate that water injection alone can extend the performance envelope of both engine types by one and one-half Mach numbers at which point water-air ratios reach 17 or 18 percent and liquid specific impulse is reduced to some 390 to 470 seconds, a level about equal to the impulse of a high <span class="hlt">energy</span> rocket engine. The envelope can be further extended, but only with increasing sacrifices in liquid specific impulse. Oxygen-airflow ratios as high as 15 percent were investigated for increasing thrust. Using 15 percent oxygen in combination with water injection at high supersonic Mach numbers resulted in thrust augmentation as high as 76 percent without any significant decrease in liquid specific impulse. The stoichiometric <span class="hlt">afterburner</span> exit temperature increased with increasing oxygen flow, reaching 4822 deg R in the turbojet engine at a Mach number of 3.5. At the transonic Mach number of 0.95 where no water injection is needed, an oxygen-air ratio of 15 percent increased thrust by some 55 percent in both engines, along with a decrease in liquid specific impulse of 62 percent. <span class="hlt">Afterburner</span> temperature was approximately 4700 deg R at this high thrust condition. Water and/or oxygen injection are simple and straightforward strategies to improve engine performance and they will add little to engine weight. However, if large Mach number and thrust increases are required, liquid flows become significant, so that operation at these conditions will necessarily be of short duration.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.epa.gov/nsr/revised-seasonal-afterburner-policy','PESTICIDES'); return false;" href="https://www.epa.gov/nsr/revised-seasonal-afterburner-policy"><span>Revised Seasonal <span class="hlt">Afterburner</span> Policy</span></a></p> <p><a target="_blank" href="http://www.epa.gov/pesticides/search.htm">EPA Pesticide Factsheets</a></p> <p></p> <p></p> <p>This document may be of assistance in applying the New Source Review (NSR) air permitting regulations including the Prevention of Significant Deterioration (PSD) requirements. This document is part of the NSR Policy and Guidance Database. Some documents in the database are a scanned or retyped version of a paper photocopy of the original. Although we have taken considerable effort to quality assure the documents, some may contain typographical errors. Contact the office that issued the document if you need a copy of the original.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014EGUGA..1612959G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014EGUGA..1612959G"><span>Pyroclast acceleration and <span class="hlt">energy</span> partitioning in fake explosive eruptions</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Gaudin, Damien; Taddeucci, Jacopo; Scheu, Bettina; Valentine, Greg; Capponi, Antonio; Kueppers, Ulrich; Graettiger, Allison; Sonder, Ingo</p> <p>2014-05-01</p> <p>Explosive eruptions are characterized by the fast <span class="hlt">release</span> of <span class="hlt">energy</span>, with gas expansion playing a lead role. An excess of pressure may be generated either by the exsolution and accumulation of volatiles (e.g., vulcanian and strombolian explosions) or by in situ vaporization of water (e.g., phreato-magmatic explosions). The <span class="hlt">release</span> of pressurized gas ejects magma and country rock pyroclasts at velocities that can reach several hundred of meters per second. The amount and velocity of pyroclasts is determined not only by the total <span class="hlt">released</span> <span class="hlt">energy</span>, but also by the system-specific dynamics of the <span class="hlt">energy</span> transfer from gas to pyroclasts. In this context, analogue experiments are crucial, since the amount of available <span class="hlt">energy</span> is determined. Here, we analyze three different experiments, designed to reproduce different aspects of explosive volcanism, focusing on the acceleration phase of the pyroclasts, in order to compare how the potential <span class="hlt">energy</span> is transferred to the pyroclasts in different systems. In the first, shock-tube-type experiment, salt crystals resting in a pressurized Plexiglas cylinder are accelerated when a diaphragm set is suddenly opened, <span class="hlt">releasing</span> the gas. In the second experiment, a pressurized air bubble is <span class="hlt">released</span> in a water-filled Plexiglas pipe; diaphragm opening causes sudden expansion and bursting of the bubble and ejection of water droplets. In the last experiment, specifically focusing on phreatomagmatic eruptions, buried explosive charges accelerate the overlying loose material. All experiments were monitored by multiple high speed cameras and a variety of sensors. Despite the largely differing settings and processes, particle ejection velocity above the vent from the three experiments share a non-linear decay over time. Fitting this decay allows to estimate a characteristic depth that is related to the specific acceleration processes. Given that the initial available <span class="hlt">energy</span> is experimentally controlled a priori, the information on the</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li class="active"><span>21</span></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_21 --> <div id="page_22" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li class="active"><span>22</span></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li><a href="#" onclick='return showDiv("page_24");'>24</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="421"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/20623984','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/20623984"><span>[Oral controlled <span class="hlt">release</span> dosage forms].</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Mehuys, Els; Vervaet, Chris</p> <p>2010-06-01</p> <p>Several technologies to control drug <span class="hlt">release</span> from oral dosage forms have been developed. Drug <span class="hlt">release</span> can be regulated in several ways: sustained <span class="hlt">release</span>, whereby the drug is <span class="hlt">released</span> slowly over a prolonged period of time, postponed <span class="hlt">release</span>, whereby drug <span class="hlt">release</span> is delayed until passage from the stomach into the intestine (via enteric coating), and targeted <span class="hlt">release</span>, whereby the drug is targeted to a specific location of the gastrointestinal tract. This article reviews the various oral controlled <span class="hlt">release</span> dosage forms on the market.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1046671','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/1046671"><span>High <span class="hlt">Energy</span> Density Capacitors</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>None</p> <p>2010-07-01</p> <p>BEEST Project: Recapping is developing a capacitor that could rival the <span class="hlt">energy</span> storage potential and price of today’s best EV batteries. When power is needed, the capacitor rapidly <span class="hlt">releases</span> its stored <span class="hlt">energy</span>, similar to lightning being discharged from a cloud. Capacitors are an ideal substitute for batteries if their <span class="hlt">energy</span> storage capacity can be improved. Recapping is addressing storage capacity by experimenting with the material that separates the positive and negative electrodes of its capacitors. These separators could significantly improve the <span class="hlt">energy</span> density of electrochemical devices.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19720022304','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19720022304"><span>A study of an advanced confined linear <span class="hlt">energy</span> source</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Anderson, M. C.; Heidemann, W. B.</p> <p>1971-01-01</p> <p>A literature survey and a test program to develop and evaluate an advanced confined linear <span class="hlt">energy</span> source were conducted. The advanced confined linear <span class="hlt">energy</span> source is an explosive or pyrotechnic X-Cord (mild detonating fuse) supported inside a confining tube capable of being hermetically sealed and retaining all products of combustion. The <span class="hlt">energy</span> <span class="hlt">released</span> by initiation of the X-Cord is transmitted through the support material to the walls of the confining tube causing an appreciable change in cross sectional configuration and expansion of the tube. When located in an assembly that can accept and use the <span class="hlt">energy</span> of the tube expansion, useful work is accomplished through fracture of a structure, movement of a load, reposition of a pin, <span class="hlt">release</span> of a restraint, or similar action. The tube assembly imparts that <span class="hlt">energy</span> without <span class="hlt">release</span> of debris or gases from the device itself. This facet of the function is important to the protection of men or equipment located in close proximity to the system during the time of function.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29845080','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29845080"><span>Sustained <span class="hlt">Release</span> of Green Tea Polyphenols from Liposomal Nanoparticles; <span class="hlt">Release</span> Kinetics and Mathematical Modelling.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Prakash Upputuri, Ravi Theaj; Azad Mandal, Abul Kalam</p> <p>2017-01-01</p> <p>Background: Green tea polyphenols (GTP) are known to have several health benefits. In spite of these benefits, its application as a therapeutic agent is limited due to some of its limitations such as stability, bioavailability, and biotransformation. To overcome these limitations, liposomal nanoparticles have been used as a carrier of the GTP. Objective: Encapsulation of GTP to the liposomal nanoparticles in order to achieve a sustained <span class="hlt">release</span> of the GTP and to determine the drug <span class="hlt">release</span> kinetics and the mechanism of the <span class="hlt">release</span>. Materials and Methods: GTP encapsulated liposomal nanoparticles were prepared using phosphatidyl choline and cholesterol. The synthesized particles were characterized for their particle size and morphology. In vitro <span class="hlt">release</span> studies were carried out, followed by drug <span class="hlt">release</span> kinetics, and determining the mechanism of <span class="hlt">release</span>. In vitro , antioxidant assay was determined following 2,2-diphenyl-1-picrylhydrazyl (DPPH) method. Results: Atomic force microscope (AFM) and high resolution scanning electron microscope (HR SEM) images showed spherical particles of the size of 64.5 and 252 nm. An encapsulation efficiency as high as 77.7% was observed with GTP concentration of 5 mg.mL -1 . In vitro <span class="hlt">release</span> studies showed that the loading concentrations of GTP were independent to the cumulative percentage of the drug <span class="hlt">release</span>. GTP <span class="hlt">release</span> by varying the pH and temperature showed a direct correlation between the <span class="hlt">release</span> parameter and the percentage of drug <span class="hlt">release</span>. The higher the pH and temperature, the higher was the percentage of the drug <span class="hlt">release</span>. The <span class="hlt">release</span> data showed a good correlation with Zero order kinetics and the mechanism of the <span class="hlt">release</span> being anomalous mode. Radical scavenging activity of the <span class="hlt">released</span> GTP showed a potent scavenging activity. Conclusion: GTP encapsulated liposomal nanoparticles could be used as a delivery vehicle for achieving a sustained <span class="hlt">release</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EPJC...77..554G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EPJC...77..554G"><span>Dilaton field <span class="hlt">released</span> under collision of dilatonic black holes with Gauss-Bonnet term</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Gwak, Bogeun; Ro, Daeho</p> <p>2017-08-01</p> <p>We investigate the upper limit of the gravitational radiation <span class="hlt">released</span> upon the collision of two dilatonic black holes by analyzing the Gauss-Bonnet term. Dilatonic black holes have a dilaton hair coupled with this term. Using the laws of thermodynamics, the upper limit of the radiation is obtained, which reflected the effects of the dilaton hair. The amount of radiation <span class="hlt">released</span> is greater than that emitted by a Schwarzschild black hole due to the contribution from the dilaton hair. In the collision, most of the dilaton hair can be <span class="hlt">released</span> through radiation, where the <span class="hlt">energy</span> radiated by the dilaton hair is maximized when the horizon of one black hole is minimized for a fixed second black hole.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1041255','DOE-PATENT-XML'); return false;" href="https://www.osti.gov/servlets/purl/1041255"><span>Metal ferrite spinel <span class="hlt">energy</span> storage devices and methods for making and using same</span></a></p> <p><a target="_blank" href="http://www.osti.gov/doepatents">DOEpatents</a></p> <p>Weimer, Alan W [Niwot, CO; Perkins, Christopher [Boulder, CO; Scheffe, Jonathan [Westminster, CO; George, Steven M [Boulder, CO; Lichty, Paul [Westminster, CO</p> <p>2012-05-29</p> <p>1-100 nm metal ferrite spinel coatings are provided on substrates, preferably by using an atomic layer deposition process. The coatings are able to store <span class="hlt">energy</span> such as solar <span class="hlt">energy</span>, and to <span class="hlt">release</span> that stored <span class="hlt">energy</span>, via a redox reaction. The coating is first thermally or chemically reduced. The reduced coating is then oxidized in a second step to <span class="hlt">release</span> <span class="hlt">energy</span> and/or hydrogen, carbon monoxide or other reduced species.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1083041','DOE-PATENT-XML'); return false;" href="https://www.osti.gov/servlets/purl/1083041"><span>Metal ferrite spinel <span class="hlt">energy</span> storage devices and methods for making and using same</span></a></p> <p><a target="_blank" href="http://www.osti.gov/doepatents">DOEpatents</a></p> <p>Weimer, Alan W.; Perkins, Christopher; Scheffe, Jonathan; George, Steven M.; Lichty, Paul</p> <p>2013-03-19</p> <p>1-100 nm metal ferrite spinel coatings are provided on substrates, preferably by using an atomic layer deposition process. The coatings are able to store <span class="hlt">energy</span> such as solar <span class="hlt">energy</span>, and to <span class="hlt">release</span> that stored <span class="hlt">energy</span>, via a redox reaction. The coating is first thermally or chemically reduced. The reduced coating is then oxidized in a second step to <span class="hlt">release</span> <span class="hlt">energy</span> and/or hydrogen, carbon monoxide or other reduced species.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22475652-light-stimulated-cargo-release-from-coreshell-structured-nanocomposite-site-specific-delivery','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22475652-light-stimulated-cargo-release-from-coreshell-structured-nanocomposite-site-specific-delivery"><span>Light-stimulated cargo <span class="hlt">release</span> from a core–shell structured nanocomposite for site-specific delivery</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Cai, Yun; Ling, Li; Li, Xiaofang</p> <p></p> <p>This paper reported a core–shell structured site-specific delivery system with a light switch triggered by low <span class="hlt">energy</span> light (λ=510 nm). Its core was composed of supermagnetic Fe{sub 3}O{sub 4} nanoparticles for magnetic guiding and targeting. Its outer shell consisted of mesoporous silica molecular sieve MCM-41 which offered highly ordered hexagonal tunnels for cargo capacity. A light switch N1-(4aH-cyclopenta[1,2-b:5,4-b′]dipyridin-5(5aH)-ylidene)benzene-1, 4-diamine (CBD) was covalently grafted into these hexagonal tunnels, serving as light stimuli acceptor with loading content of 1.1 μM/g. This composite was fully characterized and confirmed by SEM, TEM, XRD patterns, N{sub 2} adsorption/desorption, thermogravimetric analysis, IR, UV–vis absorption and emissionmore » spectra. Experimental data suggested that this composite had a core as wide as 150 nm and could be magnetically guided to specific sites. Its hexagonal tunnels were as long as 180 nm. Upon light stimuli of “on” and “off” states, controllable <span class="hlt">release</span> was observed with short <span class="hlt">release</span> time of ~900 s (90% capacity). - Graphical abstract: A core–shell structured site-specific delivery system with a light switch triggered by yellow light was constructed. Controllable <span class="hlt">release</span> was observed with short <span class="hlt">release</span> time of ~900 s (90% capacity). - Highlights: • A core–shell structured site-specific delivery system was constructed. • It consisted of Fe{sub 3}O{sub 4} core and MCM-41 shell grafted with light switch. • This delivery system was triggered by low <span class="hlt">energy</span> light. • Controllable <span class="hlt">release</span> was observed with short <span class="hlt">release</span> time of ~900 s.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4501354','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4501354"><span>Magnetically stimulated ciprofloxacin <span class="hlt">release</span> from polymeric microspheres entrapping iron oxide nanoparticles</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Sirivisoot, Sirinrath; Harrison, Benjamin S</p> <p>2015-01-01</p> <p>To extend the external control capability of drug <span class="hlt">release</span>, iron oxide nanoparticles (NPs) encapsulated into polymeric microspheres were used as magnetic media to stimulate drug <span class="hlt">release</span> using an alternating magnetic field. Chemically synthesized iron oxide NPs, maghemite or hematite, and the antibiotic ciprofloxacin were encapsulated together within polycaprolactone microspheres. The polycaprolactone microspheres entrapping ciprofloxacin and magnetic NPs could be triggered for immediate drug <span class="hlt">release</span> by magnetic stimulation at a maximum value of 40%. Moreover, the microspheres were cytocompatible with fibroblasts in vitro with a cell viability percentage of more than 100% relative to a nontreated control after 24 hours of culture. Macrophage cell cultures showed no signs of increased inflammatory responses after in vitro incubation for 56 hours. Treatment of Staphylococcus aureus with the magnetic microspheres under an alternating (isolating) magnetic field increased bacterial inhibition further after 2 days and 5 days in a broth inhibition assay. The findings of the present study indicate that iron oxide NPs, maghemite and hematite, can be used as media for stimulation by an external magnetic <span class="hlt">energy</span> to activate immediate drug <span class="hlt">release</span>. PMID:26185446</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JPhCS.830a2162M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JPhCS.830a2162M"><span>Investigation of the <span class="hlt">Energy</span> Balance in the Spark Discharge Generator for Nanoparticles Synthesis</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Mylnikov, D. A.; Efimov, A. A.; Ivanov, V. V.</p> <p>2017-07-01</p> <p>In this paper we investigate the balance of <span class="hlt">energy</span> in the discharge circuit of a spark discharge generator (SDG) for nanoparticles synthesis. The <span class="hlt">released</span> <span class="hlt">energy</span> consists of several parts: the <span class="hlt">energy</span> in a discharge gap and the <span class="hlt">energy</span> dissipated in the other elements of the circuit. In turn, in the gap a one part of the <span class="hlt">energy</span> <span class="hlt">releases</span> in preanode and precathode regions and the other part in an arc between electrodes. We measured these parts and proposed ways to optimize <span class="hlt">energy</span> efficiency of the nanoparticles production.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27951520','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27951520"><span>Corticotropin-<span class="hlt">releasing</span> hormone and dopamine <span class="hlt">release</span> in healthy individuals.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Payer, Doris; Williams, Belinda; Mansouri, Esmaeil; Stevanovski, Suzanna; Nakajima, Shinichiro; Le Foll, Bernard; Kish, Stephen; Houle, Sylvain; Mizrahi, Romina; George, Susan R; George, Tony P; Boileau, Isabelle</p> <p>2017-02-01</p> <p>Corticotropin-<span class="hlt">releasing</span> hormone (CRH) is a key component of the neuroendocrine response to stress. In animal models, CRH has been shown to modulate dopamine <span class="hlt">release</span>, and this interaction is believed to contribute to stress-induced relapse in neuropsychiatric disorders. Here we investigated whether CRH administration induces dopamine <span class="hlt">release</span> in humans, using positron emission tomography (PET). Eight healthy volunteers (5 female, 22-48 years old) completed two PET scans with the dopamine D 2/3 receptor radioligand [ 11 C]-(+)-PHNO: once after saline injection, and once after injection of corticorelin (synthetic human CRH). We also assessed subjective reports and measured plasma levels of endocrine hormones (adrenocorticotropic hormone and cortisol). Relative to saline, corticorelin administration decreased binding of the D 2/3 PET probe [ 11 C]-(+)-PHNO, suggesting dopamine <span class="hlt">release</span>. Endocrine stress markers were also elevated, in line with activation of the hypothalamic-pituitary-adrenal axis, but we detected no changes in subjective ratings. Preliminary results from this proof-of-concept study suggests that CRH challenge in combination with [ 11 C]-(+)-PHNO PET may serve as an assay of dopamine <span class="hlt">release</span>, presenting a potential platform for evaluating CRH/dopamine interactions in neuropsychiatric disorders and CRH antagonists as potential treatment avenues. Copyright © 2016 Elsevier Ltd. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5127786','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5127786"><span>Thermosensitive liposomes for localized delivery and triggered <span class="hlt">release</span> of chemotherapy</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Ta, Terence; Porter, Tyrone M.</p> <p>2016-01-01</p> <p>Liposomes are a promising class of nanomedicine with the potential to provide site-specific chemotherapy, thus improving the quality of cancer patient care. First-generation liposomes have emerged as one of the first nanomedicines used clinically for localized delivery of chemotherapy. Second-generation liposomes, i.e. stimuli-responsive liposomes, have the potential to not only provide site-specific chemotherapy, but also triggered drug <span class="hlt">release</span> and thus greater spatial and temporal control of therapy. Temperature-sensitive liposomes are an especially attractive option, as tumors can be heated in a controlled and predictable manner with external <span class="hlt">energy</span> sources. Traditional thermosensitive liposomes are composed of lipids that undergo a gel-to-liquid phase transition at several degrees above physiological temperature. More recently, temperature-sensitization of liposomes has been demonstrated with the use of lysolipids and synthetic temperature-sensitive polymers. The design, drug <span class="hlt">release</span> behavior, and clinical potential of various temperature-sensitive liposomes, as well as the various heating modalities used to trigger <span class="hlt">release</span>, are discussed in this review. PMID:23583706</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4498003','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4498003"><span>Modulating dopamine <span class="hlt">release</span> by optogenetics in transgenic mice reveals terminal dopaminergic dynamics</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Lu, Yao; Driscoll, Nicolette; Ozden, Ilker; Yu, Zeyang; Nurmikko, Arto V.</p> <p>2015-01-01</p> <p>Abstract. Dopamine (DA) <span class="hlt">release</span> and uptake dynamics in the nucleus accumbens (NAc) have important implications for neurological diseases and mammalian animal behaviors. We demonstrate here the use of cell-type-specific optogenetic targeting in conjunction with fast-scan cyclic voltammetry applied to brain slices prepared from specifically tailored transgenic mice, which conditionally express channelrhodopsin-2 (ChR2) through dopamine transporter (DAT)-Cre. Terminal dopaminergic dynamics and the direct manipulation of induced DA <span class="hlt">release</span> level by controlling light intensity, pulse width, and the shape of stimulation waveforms were studied. Effective cell terminal-targeting optogenetic induction of DA <span class="hlt">release</span> at physiological levels in NAc is demonstrated and discussed. It was found that delivering more light <span class="hlt">energy</span> by increasing stimulation intensity and length is not the only way to control DA <span class="hlt">release</span>; the temporal shape of the stimulus waveform at light onset is also critically related to induced DA concentrations. In addition, DA uptake dynamics as well as the recovery of the presynaptic <span class="hlt">releasable</span> DA pool are studied and modeled. More broadly, our experimental findings provide important further evidence for effectively applying optogenetics to induce neurotransmitter <span class="hlt">release</span> in the behaviorally relevant region of the brain in a highly cell-type selective context. PMID:26171413</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/CFR-2010-title10-vol1/pdf/CFR-2010-title10-vol1-sec50-34a.pdf','CFR'); return false;" href="https://www.gpo.gov/fdsys/pkg/CFR-2010-title10-vol1/pdf/CFR-2010-title10-vol1-sec50-34a.pdf"><span>10 CFR 50.34a - Design objectives for equipment to control <span class="hlt">releases</span> of radioactive material in effluents-nuclear...</span></a></p> <p><a target="_blank" href="http://www.gpo.gov/fdsys/browse/collectionCfr.action?selectedYearFrom=2010&page.go=Go">Code of Federal Regulations, 2010 CFR</a></p> <p></p> <p>2010-01-01</p> <p>... 10 <span class="hlt">Energy</span> 1 2010-01-01 2010-01-01 false Design objectives for equipment to control <span class="hlt">releases</span> of..., Certifications, and Regulatory Approvals; Form; Contents; Ineligibility of Certain Applicants § 50.34a Design objectives for equipment to control <span class="hlt">releases</span> of radioactive material in effluents—nuclear power reactors. (a...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/CFR-2013-title10-vol1/pdf/CFR-2013-title10-vol1-sec50-34a.pdf','CFR2013'); return false;" href="https://www.gpo.gov/fdsys/pkg/CFR-2013-title10-vol1/pdf/CFR-2013-title10-vol1-sec50-34a.pdf"><span>10 CFR 50.34a - Design objectives for equipment to control <span class="hlt">releases</span> of radioactive material in effluents-nuclear...</span></a></p> <p><a target="_blank" href="http://www.gpo.gov/fdsys/browse/collectionCfr.action?selectedYearFrom=2013&page.go=Go">Code of Federal Regulations, 2013 CFR</a></p> <p></p> <p>2013-01-01</p> <p>... 10 <span class="hlt">Energy</span> 1 2013-01-01 2013-01-01 false Design objectives for equipment to control <span class="hlt">releases</span> of..., Certifications, and Regulatory Approvals; Form; Contents; Ineligibility of Certain Applicants § 50.34a Design objectives for equipment to control <span class="hlt">releases</span> of radioactive material in effluents—nuclear power reactors. (a...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/CFR-2011-title10-vol1/pdf/CFR-2011-title10-vol1-sec50-34a.pdf','CFR2011'); return false;" href="https://www.gpo.gov/fdsys/pkg/CFR-2011-title10-vol1/pdf/CFR-2011-title10-vol1-sec50-34a.pdf"><span>10 CFR 50.34a - Design objectives for equipment to control <span class="hlt">releases</span> of radioactive material in effluents-nuclear...</span></a></p> <p><a target="_blank" href="http://www.gpo.gov/fdsys/browse/collectionCfr.action?selectedYearFrom=2011&page.go=Go">Code of Federal Regulations, 2011 CFR</a></p> <p></p> <p>2011-01-01</p> <p>... 10 <span class="hlt">Energy</span> 1 2011-01-01 2011-01-01 false Design objectives for equipment to control <span class="hlt">releases</span> of..., Certifications, and Regulatory Approvals; Form; Contents; Ineligibility of Certain Applicants § 50.34a Design objectives for equipment to control <span class="hlt">releases</span> of radioactive material in effluents—nuclear power reactors. (a...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/CFR-2012-title10-vol1/pdf/CFR-2012-title10-vol1-sec50-34a.pdf','CFR2012'); return false;" href="https://www.gpo.gov/fdsys/pkg/CFR-2012-title10-vol1/pdf/CFR-2012-title10-vol1-sec50-34a.pdf"><span>10 CFR 50.34a - Design objectives for equipment to control <span class="hlt">releases</span> of radioactive material in effluents-nuclear...</span></a></p> <p><a target="_blank" href="http://www.gpo.gov/fdsys/browse/collectionCfr.action?selectedYearFrom=2012&page.go=Go">Code of Federal Regulations, 2012 CFR</a></p> <p></p> <p>2012-01-01</p> <p>... 10 <span class="hlt">Energy</span> 1 2012-01-01 2012-01-01 false Design objectives for equipment to control <span class="hlt">releases</span> of..., Certifications, and Regulatory Approvals; Form; Contents; Ineligibility of Certain Applicants § 50.34a Design objectives for equipment to control <span class="hlt">releases</span> of radioactive material in effluents—nuclear power reactors. (a...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/CFR-2014-title10-vol1/pdf/CFR-2014-title10-vol1-sec50-34a.pdf','CFR2014'); return false;" href="https://www.gpo.gov/fdsys/pkg/CFR-2014-title10-vol1/pdf/CFR-2014-title10-vol1-sec50-34a.pdf"><span>10 CFR 50.34a - Design objectives for equipment to control <span class="hlt">releases</span> of radioactive material in effluents-nuclear...</span></a></p> <p><a target="_blank" href="http://www.gpo.gov/fdsys/browse/collectionCfr.action?selectedYearFrom=2014&page.go=Go">Code of Federal Regulations, 2014 CFR</a></p> <p></p> <p>2014-01-01</p> <p>... 10 <span class="hlt">Energy</span> 1 2014-01-01 2014-01-01 false Design objectives for equipment to control <span class="hlt">releases</span> of..., Certifications, and Regulatory Approvals; Form; Contents; Ineligibility of Certain Applicants § 50.34a Design objectives for equipment to control <span class="hlt">releases</span> of radioactive material in effluents—nuclear power reactors. (a...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26700879','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26700879"><span>The thermodynamics of endosomal escape and DNA <span class="hlt">release</span> from lipoplexes.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Avital, Yotam Y; Grønbech-Jensen, Niels; Farago, Oded</p> <p>2016-01-28</p> <p>Complexes of cationic and neutral lipids and DNA (lipoplexes) are emerging as promising vectors for gene therapy applications. Their appeal stems from their non pathogenic nature and the fact that they self-assemble under conditions of thermal equilibrium. Lipoplex adhesion to the cell plasma membrane initiates a three-stage process termed transfection, consisting of (i) endocytosis, (ii) lipoplex breakdown, and (iii) DNA <span class="hlt">release</span> followed by gene expression. As successful transfection requires lipoplex degradation, it tends to be hindered by the lipoplex thermodynamic stability; nevertheless, it is known that the transfection process may proceed spontaneously. Here, we use a simple model to study the thermodynamic driving forces governing transfection. We demonstrate that after endocytosis [stage (i)], the lipoplex becomes inherently unstable. This instability, which is triggered by interactions between the cationic lipids of the lipoplex and the anionic lipids of the enveloping plasma membrane, is entropically controlled involving both remixing of the lipids and counterions <span class="hlt">release</span>. Our detailed calculation shows that the free <span class="hlt">energy</span> gain during stage (ii) is approximately linear in Φ+, the mole fraction of cationic lipids in the lipoplex. This free <span class="hlt">energy</span> gain, ΔF, reduces the barrier for fusion between the enveloping and the lipoplex bilayers, which produces a hole allowing for DNA <span class="hlt">release</span> [stage (iii)]. The linear relationship between ΔF and the fraction of cationic lipids explains the experimentally observed exponential increase of transfection efficiency with Φ+ in lamellar lipoplexes.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28853891','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28853891"><span>Investigation of the Iron(II) <span class="hlt">Release</span> Mechanism of Human H-Ferritin as a Function of pH.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Sala, Davide; Ciambellotti, Silvia; Giachetti, Andrea; Turano, Paola; Rosato, Antonio</p> <p>2017-09-25</p> <p>We investigated the kinetics of the <span class="hlt">release</span> of iron(II) ions from the internal cavity of human H-ferritin as a function of pH. Extensive molecular dynamics simulations of the entire 24-mer ferritin provided atomic-level information on the <span class="hlt">release</span> mechanism. Double protonation of His residues at pH 4 facilitates the removal of the iron ligands within the C3 channel through the formation of salt bridges, resulting in a significantly lower <span class="hlt">release</span> <span class="hlt">energy</span> barrier than pH 9.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li class="active"><span>22</span></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li><a href="#" onclick='return showDiv("page_24");'>24</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_22 --> <div id="page_23" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li class="active"><span>23</span></li> <li><a href="#" onclick='return showDiv("page_24");'>24</a></li> <li><a href="#" onclick='return showDiv("page_25");'>25</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="441"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.nrel.gov/esif/esi-news-201608.html','SCIGOVWS'); return false;" href="https://www.nrel.gov/esif/esi-news-201608.html"><span><span class="hlt">Energy</span> Systems Integration News | <span class="hlt">Energy</span> Systems Integration Facility |</span></a></p> <p><a target="_blank" href="http://www.science.gov/aboutsearch.html">Science.gov Websites</a></p> <p></p> <p></p> <p>power grid modeling scenarios <em>Study</em> Shows Eastern U.S. Power Grid Can Support Upwards of 30% Wind and newly <span class="hlt">released</span> Eastern Renewable <span class="hlt">Energy</span> Integration <em>Study</em> (ERGIS) shows that the power grid of the -based <em>study</em> of four potential wind and PV futures and associated operational impacts in the Eastern</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://eric.ed.gov/?q=Fuel+AND+co2&pg=2&id=EJ853417','ERIC'); return false;" href="https://eric.ed.gov/?q=Fuel+AND+co2&pg=2&id=EJ853417"><span>Low <span class="hlt">Energy</span> Schools in Ireland</span></a></p> <p><a target="_blank" href="http://www.eric.ed.gov/ERICWebPortal/search/extended.jsp?_pageLabel=advanced">ERIC Educational Resources Information Center</a></p> <p>Heffernan, Martin</p> <p>2004-01-01</p> <p>Out of a commitment to reducing carbon dioxide emissions, Ireland's Department of Education and Science has designed and constructed two low <span class="hlt">energy</span> schools, in Tullamore, County Offaly, and Raheen, County Laois. With <span class="hlt">energy</span> use in buildings responsible for approximately 55% of the CO[subscript 2] <span class="hlt">released</span> into the atmosphere and a major…</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015Nanos...710340L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015Nanos...710340L"><span>Real-time investigation of cytochrome c <span class="hlt">release</span> profiles in living neuronal cells undergoing amyloid beta oligomer-induced apoptosis</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lee, Jae Young; Park, Younggeun; Pun, San; Lee, Sung Sik; Lo, Joe F.; Lee, Luke P.</p> <p>2015-06-01</p> <p>Intracellular Cyt c <span class="hlt">release</span> profiles in living human neuroblastoma undergoing amyloid β oligomer (AβO)-induced apoptosis, as a model Alzheimer's disease-associated pathogenic molecule, were analysed in a real-time manner using plasmon resonance <span class="hlt">energy</span> transfer (PRET)-based spectroscopy.Intracellular Cyt c <span class="hlt">release</span> profiles in living human neuroblastoma undergoing amyloid β oligomer (AβO)-induced apoptosis, as a model Alzheimer's disease-associated pathogenic molecule, were analysed in a real-time manner using plasmon resonance <span class="hlt">energy</span> transfer (PRET)-based spectroscopy. Electronic supplementary information (ESI) available. See DOI: 10.1039/c5nr02390d</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19930087885','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19930087885"><span>Altitude Wind Tunnel Investigation of XJ34-WE-32 Engine Performance Without Electronic Control</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Bloomer, Harry E; Walker, William J; Pantages, George L</p> <p>1953-01-01</p> <p>An investigation was conducted in the NACA Lewis altitude wind tunnel to evaluate the performance characteristics of an XJ34-WE-32 turbojet engine which was equipped with an <span class="hlt">afterburner</span>, a variable-area exhaust nozzle, and an integrated electronic control. The data were obtained with the <span class="hlt">afterburner</span> and electronic control inoperative. Performance data were obtained at altitudes from 5000 to 55,000 feet and flight Mach numbers from 0.28 to 1.06 for a complete range of operable engine speeds at each of four fixed positions of the variable-area exhaust nozzle.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19910009227&hterms=ionospheric+modification&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Dionospheric%2Bmodification','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19910009227&hterms=ionospheric+modification&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Dionospheric%2Bmodification"><span>Ionospheric chemical <span class="hlt">releases</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Bernhardt, Paul A.; Scales, W. A.</p> <p>1990-01-01</p> <p>Ionospheric plasma density irregularities can be produced by chemical <span class="hlt">releases</span> into the upper atmosphere. F-region plasma modification occurs by: (1) chemically enhancing the electron number density; (2) chemically reducing the electron population; or (3) physically convecting the plasma from one region to another. The three processes (production, loss, and transport) determine the effectiveness of ionospheric chemical <span class="hlt">releases</span> in subtle and surprising ways. Initially, a chemical <span class="hlt">release</span> produces a localized change in plasma density. Subsequent processes, however, can lead to enhanced transport in chemically modified regions. Ionospheric modifications by chemical <span class="hlt">releases</span> excites artificial enhancements in airglow intensities by exothermic chemical reactions between the newly created plasma species. Numerical models were developed to describe the creation and evolution of large scale density irregularities and airglow clouds generated by artificial means. Experimental data compares favorably with theses models. It was found that chemical <span class="hlt">releases</span> produce transient, large amplitude perturbations in electron density which can evolve into fine scale irregularities via nonlinear transport properties.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27694233','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27694233"><span>Freshwater bacteria <span class="hlt">release</span> methane as a byproduct of phosphorus acquisition.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Yao, Mengyin; Henny, Cynthia; Maresca, Julia A</p> <p>2016-09-30</p> <p>Freshwater lakes emit large amounts of methane, some of which is produced in oxic surface waters. Two potential pathways for aerobic methane production exist: methanogenesis in oxygenated water, which has been observed in some lakes, or demethylation of small organic molecules. Although methane is produced via demethylation in oxic marine environments, this mechanism of methane <span class="hlt">release</span> has not yet been demonstrated in freshwater systems. Genes related to the C-P lyase pathway, which cleaves C-P bonds in phosphonate compounds, were found in a metagenomic survey of the surface water of Lake Matano, which is chronically P-starved and methane-rich. We demonstrate that four bacterial isolates from Lake Matano obtain P from methylphosphonate and <span class="hlt">release</span> methane, and that this activity is repressed by phosphate. We further demonstrate that expression of phnJ, which encodes the enzyme that <span class="hlt">releases</span> methane, is higher in the presence of methylphosphonate and lower when both methylphosphonate and phosphate are added. This gene is also found in most of the metagenomic data sets from freshwater environments. These experiments link methylphosphonate degradation and methane production with gene expression and phosphate availability in freshwater organisms, and suggest that some of the excess methane in the Lake Matano surface water, and in other methane-rich lakes, may be produced by P-starved bacteria. Methane is an important greenhouse gas, and contributes substantially to global warming. Although freshwater environments are known to <span class="hlt">release</span> methane into the atmosphere, estimates of the amount of methane emitted by freshwater lakes vary from 8 to 73 Tg per year. Methane emissions are difficult to predict in part because the source of the methane can vary: it is the end product of the <span class="hlt">energy</span>-conserving pathway in methanogenic archaea, which predominantly live in anoxic sediments or waters, but have also been identified in some oxic freshwater environments. More recently</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/21232641','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/21232641"><span>Bone cell-materials interactions and Ni ion <span class="hlt">release</span> of anodized equiatomic NiTi alloy.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Bernard, Sheldon A; Balla, Vamsi Krishna; Davies, Neal M; Bose, Susmita; Bandyopadhyay, Amit</p> <p>2011-04-01</p> <p>A laser processed NiTi alloy was anodized for different times in H(2)SO(4) electrolyte with varying pH to create biocompatible surfaces with low Ni ion <span class="hlt">release</span> as well as bioactive surfaces to enhance biocompatibility and bone cell-material interactions. The anodized surfaces were assessed for their in vitro cell-material interactions using human fetal osteoblast (hFOB) cells for 3, 7 and 11 days, and Ni ion <span class="hlt">release</span> up to 8 weeks in simulated body fluids. The results were correlated with the surface morphologies of anodized surfaces characterized using field-emission scanning electron microscopy (FESEM). The results show that anodization creates a surface with nano/micro-roughness depending on the anodization conditions. The hydrophilicity of the NiTi surface was found to improve after anodization, as shown by the lower contact angles in cell medium, which dropped from 32° to <5°. The improved wettability of anodized surfaces is further corroborated by their high surface <span class="hlt">energy</span>, comparable with that of commercially pure Ti. Relatively high surface <span class="hlt">energies</span>, especially the polar component, and nano/micro surface features of anodized surfaces significantly increased the number of living cells and their adherence and growth on these surfaces. Finally, a significant drop in Ni ion <span class="hlt">release</span> from 268±11 to 136±15 ppb was observed for NiTi surfaces after anodization. This work indicates that anodization of a NiTi alloy has a positive influence on the surface <span class="hlt">energy</span> and surface morphology, which in turn improves bone cell-material interactions and reduces Ni ion <span class="hlt">release</span> in vitro. Copyright © 2011 Acta Materialia Inc. Published by Elsevier Ltd. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://eric.ed.gov/?q=%22short+film%22&pg=7&id=EJ214121','ERIC'); return false;" href="https://eric.ed.gov/?q=%22short+film%22&pg=7&id=EJ214121"><span>Short Films--Sure Winners: A Select List of the Best of the Recent <span class="hlt">Releases</span>.</span></a></p> <p><a target="_blank" href="http://www.eric.ed.gov/ERICWebPortal/search/extended.jsp?_pageLabel=advanced">ERIC Educational Resources Information Center</a></p> <p>Reingoldas, Elena; And Others</p> <p>1979-01-01</p> <p>Lists and offers brief descriptions of 47 recently <span class="hlt">released</span> short films, arranged in the following categories: literary adaptations, profiles and personal growth, <span class="hlt">energy</span> and technology, upbeat and positive, and human concerns. (FL)</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4363105','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4363105"><span>The heat <span class="hlt">released</span> during catalytic turnover enhances the diffusion of an enzyme</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Riedel, Clement; Gabizon, Ronen; Wilson, Christian A. M.; Hamadani, Kambiz; Tsekouras, Konstantinos; Marqusee, Susan; Pressé, Steve; Bustamante, Carlos</p> <p>2015-01-01</p> <p>Recent studies have shown that the diffusivity of enzymes increases in a substrate-dependent manner during catalysis1,2. Although this observation has been reported and characterized for several different systems3–10, the precise origin of this phenomenon is unknown. Calorimetric methods are often used to determine enthalpies from enzyme-catalysed reactions and can therefore provide important insight into their reaction mechanisms11,12. The ensemble averages involved in traditional bulk calorimetry cannot probe the transient effects that the <span class="hlt">energy</span> exchanged in a reaction may have on the catalyst. Here we obtain single-molecule fluorescence correlation spectroscopy data and analyse them within the framework of a stochastic theory to demonstrate a mechanistic link between the enhanced diffusion of a single enzyme molecule and the heat <span class="hlt">released</span> in the reaction. We propose that the heat <span class="hlt">released</span> during catalysis generates an asymmetric pressure wave that results in a differential stress at the protein–solvent interface that transiently displaces the centre-of-mass of the enzyme (chemoacoustic effect). This novel perspective on how enzymes respond to the <span class="hlt">energy</span> <span class="hlt">released</span> during catalysis suggests a possible effect of the heat of reaction on the structural integrity and internal degrees of freedom of the enzyme. PMID:25487146</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1257853-heat-released-during-catalytic-turnover-enhances-diffusion-enzyme','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1257853-heat-released-during-catalytic-turnover-enhances-diffusion-enzyme"><span>The heat <span class="hlt">released</span> during catalytic turnover enhances the diffusion of an enzyme</span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Riedel, Clement; Gabizon, Ronen; Wilson, Christian A. M.; ...</p> <p>2014-12-10</p> <p>Recent studies have shown that the diffusivity of enzymes increases in a substrate-dependent manner during catalysis. Although this observation has been reported and characterized for several different systems, the precise origin of this phenomenon is unknown. Calorimetric methods are often used to determine enthalpies from enzyme-catalysed reactions and can therefore provide important insight into their reaction mechanisms. The ensemble averages involved in traditional bulk calorimetry cannot probe the transient effects that the <span class="hlt">energy</span> exchanged in a reaction may have on the catalyst. Here we obtain single-molecule fluorescence correlation spectroscopy data and analyse them within the framework of a stochastic theorymore » to demonstrate a mechanistic link between the enhanced diffusion of a single enzyme molecule and the heat <span class="hlt">released</span> in the reaction. We propose that the heat <span class="hlt">released</span> during catalysis generates an asymmetric pressure wave that results in a differential stress at the protein-solvent interface that transiently displaces the centre-of-mass of the enzyme (chemoacoustic effect). We find this novel perspective on how enzymes respond to the <span class="hlt">energy</span> <span class="hlt">released</span> during catalysis suggests a possible effect of the heat of reaction on the structural integrity and internal degrees of freedom of the enzyme.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=1309440','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=1309440"><span>Characteristics of renin <span class="hlt">release</span> from isolated superfused glomeruli in vitro.</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Blendstrup, K; Leyssac, P P; Poulsen, K; Skinner, S L</p> <p>1975-01-01</p> <p>1. A method is described for studying renin <span class="hlt">release</span> from superfused rat glomeruli following their rapid isolation by a magnetic iron-oxide technique. 2. Microscopically selected glomeruli were free of tubular components. Some possessed vascular pole protrusions of up to 20 mum, unrelated to renin content. 3. Renin content of 102 batches, each of 400 glomeruli, was 1.34 plus or minus 0.08 times 10-4 Goldblatt hog units per 100 glomeruli (plus or minus S.E. of mean). Different osmolarities (305, 355 and 400 m-osmole/1.), sodium concentrations (110 and 135 mM) and buffer compositions of the preparation solution did not alter this value. Renin content per glomerulus in intact kidney was 100-fold higher. 4. At 30 degrees C the contained juxtaglomerular cells <span class="hlt">released</span> renin at consistent but decreasing rates over 4-6 hr. Initial <span class="hlt">release</span> rate in 110 mM sodium, 305 m-osmole/1. solutions were 0.86 plus or minus 0.068 times 10-6 units per 100 glomeruli per 30 min (plus or minus S.E. of mean, n = 42) or 0.546 plus or minus 0.046 percent of content per 30 min. In 135 mM sodium, 305 m-osmole/1. solutions, <span class="hlt">release</span> was 2.4-fold higher (P less than 0.001) and remained elevated for at least 3 hr. When related to renin content per glomerulus resting <span class="hlt">release</span> rate in vitro was higher by at most one order of magnitude than calculated in vivo values. 5. <span class="hlt">Release</span> was augmented by gentle physical agitation of the glomeruli. 6. <span class="hlt">Release</span> rate was inversely ralated to temperature. On reducing temperature from 30 degrees C, <span class="hlt">release</span> increased 2.6-fold at 20 degrees C and 6.7-fold at 10 degrees C (P less than 0.001, n = 11). The response was reversible. 7. 3 mM sodium cyanide plus 3 mM sodium iodoacetate caused a variable <span class="hlt">release</span> of renin associated with depletion of content within 4 hr. The response was progressive and reached a peak after 60 min. 8. Sensitivity of renin <span class="hlt">release</span> to temperature and metabolic blockade indicates that <span class="hlt">energy</span> is required for retention of renin by the cell. This</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JPhCS.843a2004K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JPhCS.843a2004K"><span>Theoretical prediction of <span class="hlt">energy</span> <span class="hlt">release</span> rate for interface crack initiation by thermal stress in environmental barrier coatings for ceramics</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kawai, E.; Umeno, Y.</p> <p>2017-05-01</p> <p>As weight reduction of turbines for aircraft engines is demanded to improve fuel consumption and curb emission of carbon dioxide, silicon carbide (SiC) fiber reinforced SiC matrix composites (SiC/SiC) are drawing enormous attention as high-pressure turbine materials. For preventing degradation of SiC/SiC, environmental barrier coatings (EBC) for ceramics are deposited on the composites. The purpose of this study is to establish theoretical guidelines for structural design which ensures the mechanical reliability of EBC. We conducted finite element method (FEM) analysis to calculate <span class="hlt">energy</span> <span class="hlt">release</span> rates (ERRs) for interface crack initiation due to thermal stress in EBC consisting of Si-based bond coat, Mullite and Ytterbium (Yb)-silicate layers on a SiC/SiC substrate. In the FEM analysis, the thickness of one EBC layer was changed from 25 μm to 200 μm while the thicknesses of the other layers were fixed at 25 μm, 50 μm and 100 μm. We compared ERRs obtained by the FEM analysis and a simple theory for interface crack in a single-layered structure where ERR is estimated as nominal strain <span class="hlt">energy</span> in the coating layers multiplied by a constant factor (independent of layer thicknesses). We found that, unlike the case of single-layered structures, the multiplication factor is no longer a constant but is determined by the combination of consisting coating layer thicknesses.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017PPCF...59g5003P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017PPCF...59g5003P"><span>Heavy ion acceleration in the radiation pressure acceleration and breakout <span class="hlt">afterburner</span> regimes</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Petrov, G. M.; McGuffey, C.; Thomas, A. G. R.; Krushelnick, K.; Beg, F. N.</p> <p>2017-07-01</p> <p>We present a theoretical study of heavy ion acceleration from ultrathin (20 nm) gold foil irradiated by high-intensity sub-picosecond lasers. Using two-dimensional particle-in-cell simulations, three laser systems are modeled that cover the range between femtosecond and picosecond pulses. By varying the laser pulse duration we observe a transition from radiation pressure acceleration (RPA) to the relativistic induced transparency (RIT) regime for heavy ions akin to light ions. The underlying physics of beam formation and acceleration is similar for light and heavy ions, however, nuances of the acceleration process make the heavy ions more challenging. A more detailed study involving variation of peak laser intensity I 0 and pulse duration τFWHM revealed that the transition point from RPA to RIT regime depends on the peak laser intensity on target and occurs for pulse duration {τ }{{F}{{W}}{{H}}{{M}}}{{R}{{P}}{{A}}\\to {{R}}{{I}}{{T}}}[{{f}}{{s}}]\\cong 210/\\sqrt{{I}0[{{W}} {{{cm}}}-2]/{10}21}. The most abundant gold ion and charge-to-mass ratio are Au51+ and q/M ≈ 1/4, respectively, half that of light ions. For ultrathin foils, on the order of one skin depth, we established a linear scaling of the maximum <span class="hlt">energy</span> per nucleon (E/M)max with (q/M)max, which is more favorable than the quadratic one found previously. The numerical simulations predict heavy ion beams with very attractive properties for applications: high directionality (<10° half-angle), high fluxes (>1011 ions sr-1) and <span class="hlt">energy</span> (>20 MeV/nucleon) from laser systems delivering >20 J of <span class="hlt">energy</span> on target.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.osti.gov/sciencecinema/biblio/1046043','SCIGOVIMAGE-SCICINEMA'); return false;" href="http://www.osti.gov/sciencecinema/biblio/1046043"><span>Rad-<span class="hlt">Release</span></span></a></p> <p><a target="_blank" href="http://www.osti.gov/sciencecinema/">ScienceCinema</a></p> <p>None</p> <p>2017-12-09</p> <p>The R&D 100 Award winning Rad-<span class="hlt">Release</span> Chemical Decontamination Technology is a highly effective (up to 99% removal rate), affordable, patented chemical-foam-clay decontamination process tailored to specific radiological and metal contaminants, which is applicable to a wide variety of substrates. For more information about this project, visit http://www.inl.gov/rd100/2011/rad-<span class="hlt">release</span>/</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3836820','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3836820"><span>How tendons buffer <span class="hlt">energy</span> dissipation by muscle</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Roberts, Thomas J.; Konow, Nicolai</p> <p>2013-01-01</p> <p>To decelerate the body and limbs, muscles actively lengthen to dissipate <span class="hlt">energy</span>. During rapid <span class="hlt">energy</span>-dissipating events, tendons buffer the work done on muscle by temporarily storing elastic <span class="hlt">energy</span>, then <span class="hlt">releasing</span> this <span class="hlt">energy</span> to do work on the muscle. This elastic mechanism may reduce the risk of muscle damage by reducing peak forces and lengthening rates of active muscle. PMID:23873133</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017PPN....48..691B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017PPN....48..691B"><span>Low-<span class="hlt">energy</span> nuclear reactions in crystal structures</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bagulya, A. V.; Dalkarov, O. D.; Negodaev, M. A.; Rusetskii, A. S.</p> <p>2017-09-01</p> <p>Results of studying low-<span class="hlt">energy</span> nuclear reactions at the HELIS facility (LPI) are presented. Investigations of yields from DD reactions in deuterated crystal structures at deuteron <span class="hlt">energies</span> of 10 to 25 keV show a considerable enhancement effect. It is shown that exposure of the deuterated targets to the H+ (proton) and Ne+ beams with <span class="hlt">energies</span> from 10 to 25 keV and an X-ray beam with the <span class="hlt">energy</span> of 20 to 30 keV stimulates DD reaction yields. For the CVD diamond target, it is shown that its orientation with respect to the deuteron beam affects the neutron yield. The D+ beam is shown to cause much higher heat <span class="hlt">release</span> in the TiDx target than the H+ and Ne+ beams, and this heat <span class="hlt">release</span> depends on the deuterium concentration in the target and the current density of the deuteron beam.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/515488','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/515488"><span>Final voluntary <span class="hlt">release</span> assessment/corrective action report</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>NONE</p> <p>1996-11-12</p> <p>The US Department of <span class="hlt">Energy</span>, Carlsbad Area Office (DOE-CAO) has completed a voluntary <span class="hlt">release</span> assessment sampling program at selected Solid Waste Management Units (SWMUs) at the Waste Isolation Pilot Plant (WIPP). This Voluntary <span class="hlt">Release</span> Assessment/Corrective Action (RA/CA) report has been prepared for final submittal to the Environmental protection Agency (EPA) Region 6, Hazardous Waste Management Division and the New Mexico Environment Department (NMED) Hazardous and Radioactive Materials Bureau to describe the results of voluntary <span class="hlt">release</span> assessment sampling and proposed corrective actions at the SWMU sites. The Voluntary RA/CA Program is intended to be the first phase in implementing the Resourcemore » Conservation and Recovery Act (RCRA) Facility Investigation (RFI) and corrective action process at the WIPP. Data generated as part of this sampling program are intended to update the RCRA Facility Assessment (RFA) for the WIPP (Assessment of Solid Waste Management Units at the Waste Isolation Pilot Plant), NMED/DOE/AIP 94/1. This Final Voluntary RA/CA Report documents the results of <span class="hlt">release</span> assessment sampling at 11 SWMUs identified in the RFA. With this submittal, DOE formally requests a No Further Action determination for these SWMUs. Additionally, this report provides information to support DOE`s request for No Further Action at the Brinderson and Construction landfill SWMUs, and to support DOE`s request for approval of proposed corrective actions at three other SWMUs (the Badger Unit Drill Pad, the Cotton Baby Drill Pad, and the DOE-1 Drill Pad). This information is provided to document the results of the Voluntary RA/CA activities submitted to the EPA and NMED in August 1995.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19730057131&hterms=whales&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D90%26Ntt%3Dwhales','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19730057131&hterms=whales&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D90%26Ntt%3Dwhales"><span>Geophysical disturbance environment during the NASA/MPE barium <span class="hlt">release</span> at 5 earth radii on September 21, 1971.</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Davis, T. N.; Stanley, G. M.; Boyd, J. S.</p> <p>1973-01-01</p> <p>The geophysical disturbance environment was quiet during the NASA/MPE barium <span class="hlt">release</span> at 5 earth radii on September 21, 1971. At the time of the <span class="hlt">release</span>, the magnetosphere was in the late recovery phase of a principal magnetic storm, the provisional Dst value was -13 gammas, and the local horizontal disturbance at Great Whale River was near zero. Riometer and other observations indicated low-level widespread precipitation of high-<span class="hlt">energy</span> electrons at Great Whale River before, during, and after the <span class="hlt">release</span>. Cloudy sky at this station prevented optical observation of aurora. No magnetic or ionospheric effects attributable to the barium <span class="hlt">release</span> were detected at Great Whale River.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/25913320','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25913320"><span>Equilibrium and kinetic models for colloid <span class="hlt">release</span> under transient solution chemistry conditions.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Bradford, Scott A; Torkzaban, Saeed; Leij, Feike; Simunek, Jiri</p> <p>2015-10-01</p> <p>We present continuum models to describe colloid <span class="hlt">release</span> in the subsurface during transient physicochemical conditions. Our modeling approach relates the amount of colloid <span class="hlt">release</span> to changes in the fraction of the solid surface area that contributes to retention. Equilibrium, kinetic, equilibrium and kinetic, and two-site kinetic models were developed to describe various rates of colloid <span class="hlt">release</span>. These models were subsequently applied to experimental colloid <span class="hlt">release</span> datasets to investigate the influence of variations in ionic strength (IS), pH, cation exchange, colloid size, and water velocity on <span class="hlt">release</span>. Various combinations of equilibrium and/or kinetic <span class="hlt">release</span> models were needed to describe the experimental data depending on the transient conditions and colloid type. <span class="hlt">Release</span> of Escherichia coli D21g was promoted by a decrease in solution IS and an increase in pH, similar to expected trends for a reduction in the secondary minimum and nanoscale chemical heterogeneity. The retention and <span class="hlt">release</span> of 20nm carboxyl modified latex nanoparticles (NPs) were demonstrated to be more sensitive to the presence of Ca(2+) than D21g. Specifically, retention of NPs was greater than D21g in the presence of 2mM CaCl2 solution, and <span class="hlt">release</span> of NPs only occurred after exchange of Ca(2+) by Na(+) and then a reduction in the solution IS. These findings highlight the limitations of conventional interaction <span class="hlt">energy</span> calculations to describe colloid retention and <span class="hlt">release</span>, and point to the need to consider other interactions (e.g., Born, steric, and/or hydration forces) and/or nanoscale heterogeneity. Temporal changes in the water velocity did not have a large influence on the <span class="hlt">release</span> of D21g for the examined conditions. This insensitivity was likely due to factors that reduce the applied hydrodynamic torque and/or increase the resisting adhesive torque; e.g., macroscopic roughness and grain-grain contacts. Our analysis and models improve our understanding and ability to describe the amounts</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26432265','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26432265"><span>Effects of artemisinin sustained-<span class="hlt">release</span> granules on mixed alga growth and microcystins production and <span class="hlt">release</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Ni, Lixiao; Li, Danye; Hu, Shuzhen; Wang, Peifang; Li, Shiyin; Li, Yiping; Li, Yong; Acharya, Kumud</p> <p>2015-12-01</p> <p>To safely and effectively apply artemisinin sustained-<span class="hlt">release</span> granules to control and prevent algal water-blooms, the effects of artemisinin and its sustained-<span class="hlt">release</span> granules on freshwater alga (Scenedesmus obliquus (S. obliquus) and Microcystis aeruginosa (M. aeruginosa)), as well as the production and <span class="hlt">release</span> of microcystins (MCs) were studied. The results showed that artemisinin sustained-<span class="hlt">release</span> granules inhibited the growth of M. aeruginosa (above 95% IR) and S. obliquus (about 90% IR), with M. aeruginosa more sensitive. The artemisinin sustained-<span class="hlt">release</span> granules had a longer inhibition effect on growth of pure algae and algal coexistence than direct artemisinin dosing. The artemisinin sustained-<span class="hlt">release</span> granules could decrease the production and <span class="hlt">release</span> of algal toxins due to the continued stress of artemisinin <span class="hlt">released</span> from artemisinin sustained-<span class="hlt">release</span> granules. There was no increase in the total amount of MC-LR in the algal cell culture medium.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li class="active"><span>23</span></li> <li><a href="#" onclick='return showDiv("page_24");'>24</a></li> <li><a href="#" onclick='return showDiv("page_25");'>25</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_23 --> <div id="page_24" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li class="active"><span>24</span></li> <li><a href="#" onclick='return showDiv("page_25");'>25</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="461"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/19349044','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/19349044"><span>Effects of anthropogenic heat <span class="hlt">release</span> upon the urban climate in a Japanese megacity.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Narumi, Daisuke; Kondo, Akira; Shimoda, Yoshiyuki</p> <p>2009-05-01</p> <p>This report presents results of investigations of the influence of anthropogenic heat <span class="hlt">release</span> in Japanese megacity (Keihanshin district) upon the urban climate, using the <span class="hlt">energy</span> database [Shimoda et al., 1999. Estimation and evaluation of artificial waste heat in urban area. Selected Papers from the Conference ICB-ICUC'99 WCASP-50 WMO/TD no. 1026] as a part of the land-surface boundary conditions of a mesoscale meteorological simulation model. The calculated results related to atmospheric temperature distribution were similar to observed values not only for daily averages but also for amplitudes and phases of diurnal change. To reproduce accurately, it is essential to reproduce urban characteristics such as an urban canopy and anthropogenic heat <span class="hlt">release</span> in a fine resolution mesh. We attempted an analysis using current data for anthropogenic heat and under uniform heat <span class="hlt">release</span> conditions, to investigate temporal and spatial characteristics in relation to the influence of anthropogenic heat <span class="hlt">release</span> on the urban climate. The results of investigation into the influence of anthropogenic heat <span class="hlt">release</span> on atmospheric temperature using current data indicate that the amount of heat <span class="hlt">released</span> is lower at night than during the day, but the temperature rise is nearly 3 times greater. Results of investigation into the influence of anthropogenic heat <span class="hlt">release</span> on wind systems using current data indicate that the onset of land breezes is delayed, particularly in a coastal area. Investigation into the temporal characteristics related to the influence of anthropogenic heat <span class="hlt">release</span> under uniform heat <span class="hlt">release</span> conditions showed a maximum influence on temperature during the predawn period.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70012003','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70012003"><span>Gravitational potential as a source of earthquake <span class="hlt">energy</span></span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Barrows, L.; Langer, C.J.</p> <p>1981-01-01</p> <p>Some degree of tectonic stress within the earth originates from gravity acting upon density structures. The work performed by this "gravitational tectonics stress" must have formerly existed as gravitational potential <span class="hlt">energy</span> contained in the stress-causing density structure. According to the elastic rebound theory (Reid, 1910), the <span class="hlt">energy</span> of earthquakes comes from an elastic strain field built up by fairly continuous elastic deformation in the period between events. For earthquakes resulting from gravitational tectonic stress, the elastic rebound theory requires the transfer of <span class="hlt">energy</span> from the gravitational potential of the density structures into an elastic strain field prior to the event. An alternate theory involves partial gravitational collapse of the stress-causing density structures. The earthquake <span class="hlt">energy</span> comes directly from a net decrease in gravitational potential <span class="hlt">energy</span>. The gravitational potential <span class="hlt">energy</span> <span class="hlt">released</span> at the time of the earthquake is split between the <span class="hlt">energy</span> <span class="hlt">released</span> by the earthquake, including work done in the fault zone and an increase in stored elastic strain <span class="hlt">energy</span>. The stress associated with this elastic strain field should oppose further fault slip. ?? 1981.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20080012141&hterms=Renewable+energy&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3DRenewable%2Benergy','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20080012141&hterms=Renewable+energy&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3DRenewable%2Benergy"><span>Surface Meteorology and Solar <span class="hlt">Energy</span> (SSE) Data <span class="hlt">Release</span> 5.1</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Stackhouse, Paul W. (Principal Investigator)</p> <p></p> <p>The Surface meteorology and Solar <span class="hlt">Energy</span> (SSE) data set contains over 200 parameters formulated for assessing and designing renewable <span class="hlt">energy</span> systems.The SSE data set is formulated from NASA satellite- and reanalysis-derived insolation and meteorological data for the 10-year period July 1983 through June 1993. Results are provided for 1 degree latitude by 1 degree longitude grid cells over the globe. Average daily and monthly measurements for 1195 World Radiation Data Centre ground sites are also available. [Location=GLOBAL] [Temporal_Coverage: Start_Date=1983-07-01; Stop_Date=1993-06-30] [Spatial_Coverage: Southernmost_Latitude=-90; Northernmost_Latitude=90; Westernmost_Longitude=-180; Easternmost_Longitude=180] [Data_Resolution: Latitude_Resolution=1 degree; Longitude_Resolution=1 degree].</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/17112658','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/17112658"><span>Modeling the <span class="hlt">release</span>, spreading, and burning of LNG, LPG, and gasoline on water.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Johnson, David W; Cornwell, John B</p> <p>2007-02-20</p> <p>Current interest in the shipment of liquefied natural gas (LNG) has renewed the debate about the safety of shipping large volumes of flammable fuels. The size of a spreading pool following a <span class="hlt">release</span> of LNG from an LNG tank ship has been the subject of numerous papers and studies dating back to the mid-1970s. Several papers have presented idealized views of how the LNG would be <span class="hlt">released</span> and spread across a quiescent water surface. There is a considerable amount of publicly available material describing these idealized <span class="hlt">releases</span>, but little discussion of how other flammable fuels would behave if <span class="hlt">released</span> from similar sized ships. The purpose of this paper is to determine whether the models currently available from the United States Federal <span class="hlt">Energy</span> Regulatory Commission (FERC) can be used to simulate the <span class="hlt">release</span>, spreading, vaporization, and pool fire impacts for materials other than LNG, and if so, identify which material-specific parameters are required. The review of the basic equations and principles in FERC's LNG <span class="hlt">release</span>, spreading, and burning models did not reveal a critical fault that would prevent their use in evaluating the consequences of other flammable fluid <span class="hlt">releases</span>. With the correct physical data, the models can be used with the same level of confidence for materials such as LPG and gasoline as they are for LNG.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/10102372','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/10102372"><span>Consequence assessment for Airborne <span class="hlt">Releases</span> of SO{sub 2} from the Y-12 Pilot Dechlorination Facility</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Pendergrass, W.R.</p> <p></p> <p>The Atmospheric Turbulence and Diffusion Division was requested by the Department of <span class="hlt">Energy`s</span> Oak Ridge Operations Office to conduct a consequence assessment for potential atmospheric <span class="hlt">releases</span> of SO{sub 2} from the Y-12 Pilot Dechlorination Facility. The focus of the assessment was to identify ``worst`` case meteorology which posed the highest concentration exposure potential for both on-site as well as off-site populations. A series of plausible SO{sub 2} <span class="hlt">release</span> scenarios were provided by Y-12 for the consequence assessment. Each scenario was evaluated for predictions of downwind concentration, estimates of a five-minute time weighted average, and estimate of the dimension of themore » puff. The highest hazard potential was associated with Scenario 1, in which a total of eight SO{sub 2} cylinders are <span class="hlt">released</span> internally to the Pilot Facility and exhausted through the emergency venting system. A companion effort was also conducted to evaluate the potential for impact of <span class="hlt">releases</span> of SO{sub 2} from the Pilot Facility on the population of Oak Ridge. While specific transport trajectory data is not available for the Pilot Facility, extrapolations based on the Oak Ridge Site Survey and climatological records from the Y-12 meteorological program does not indicate the potential for impact on the city of Oak Ridge. Steering by the local topographical features severely limits the potential impact ares. Due to the lack of specific observational data, both tracer and meteorological, only inferences can be made concerning impact zones. It is recommended tat the Department of <span class="hlt">Energy</span> Oak Ridge Operations examine the potential for off-site impact and develop the background data to prepare impact zones for <span class="hlt">releases</span> of hazardous materials from the Y-12 facility.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/23017121','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/23017121"><span>Anoxia-induced <span class="hlt">release</span> of colloid- and nanoparticle-bound phosphorus in grassland soils.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Henderson, R; Kabengi, N; Mantripragada, N; Cabrera, M; Hassan, S; Thompson, A</p> <p>2012-11-06</p> <p>Particle-facilitated transport is a key mechanism of phosphorus (P) loss in agroecosystems. We assessed contributions of colloid- and nanoparticle-bound P (nPP; 1-415 nm) to total P <span class="hlt">released</span> from grassland soils receiving biannual poultry litter applications since 1995. In laboratory incubations, soils were subjected to 7 days of anoxic conditions or equilibrated at pH 6 and 8 under oxic conditions and then the extract was size fractionated by differential centrifugation/ultrafiltration for analysis of P, Al, Fe, Si, Ti, and Ca. Selected samples were characterized by transmission electron microscopy-<span class="hlt">energy</span> dispersive spectroscopy (TEM-EDS) and field flow fractionation (FFF-ICP-MS). Particles <span class="hlt">released</span> were present as nanoaggregates with a mean diameter of 200-250 nm, composed of ~50-nm aluminosilicate flakes studded with Fe and Ti-rich clusters (<10 nm) that contained most of the P detected by EDS. Anoxic incubation of stimulated nPP <span class="hlt">release</span> with seasonally saturated soils <span class="hlt">released</span> more nPP and Fe(2+)(aq) than well-drained soils; whereas, nonreductive particle dispersion, accomplished by raising the pH, yielded no increase in nPP <span class="hlt">release</span>. This suggests Fe acts as a cementing agent, binding to the bulk soil P-bearing colloids that can be <span class="hlt">released</span> during reducing conditions. Furthermore, it suggests prior periodic exposure to anoxic conditions increases susceptibility to redox-induced P mobilization.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27993048','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27993048"><span>Kinetics of Brominated Flame Retardant (BFR) <span class="hlt">Releases</span> from Granules of Waste Plastics.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Sun, Bingbing; Hu, Yuanan; Cheng, Hefa; Tao, Shu</p> <p>2016-12-20</p> <p>Plastic components of e-waste contain high levels of brominated flame retardants (BFRs), whose <span class="hlt">releases</span> cause environmental and human health concerns. This study characterized the <span class="hlt">release</span> kinetics of polybrominated diphenyl ethers (PBDEs) from millimeter-sized granules processed from the plastic exteriors of two scrap computer displays at environmentally relevant temperatures. The <span class="hlt">release</span> rate of a substitute of PBDEs, 1,2-bis(2,4,6-tribromophenoxy)ethane (BTBPE), from the waste plastics, was reported for the first time. Deca-BDE was the most abundant PBDE congeners in both materials (87-89%), while BTBPE was also present at relatively high contents. The <span class="hlt">release</span> kinetics of BFRs could be modeled as one-dimensional diffusion, while the temperature dependence of diffusion coefficients was well described by the Arrhenius equation. The diffusion coefficients of BFRs (at 30 °C) in the plastic matrices were estimated to be in the range of 10 -27.16 to 10 -19.96 m 2 ·s -1 , with apparent activation <span class="hlt">energies</span> between 88.4 and 154.2 kJ·mol -1 . The half-lives of BFR <span class="hlt">releases</span> (i.e., 50% depletion) from the plastic granules ranged from thousands to tens of billions of years at ambient temperatures. These findings suggest that BFRs are <span class="hlt">released</span> very slowly from the matrices of waste plastics through molecular diffusion, while their emissions can be significantly enhanced with wear-and-tear and pulverization.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27253462','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27253462"><span>Solar Thermal <span class="hlt">Energy</span> Storage in a Photochromic Macrocycle.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Vlasceanu, Alexandru; Broman, Søren L; Hansen, Anne S; Skov, Anders B; Cacciarini, Martina; Kadziola, Anders; Kjaergaard, Henrik G; Mikkelsen, Kurt V; Nielsen, Mogens Brøndsted</p> <p>2016-07-25</p> <p>The conversion and efficient storage of solar <span class="hlt">energy</span> is recognized to hold significant potential with regard to future <span class="hlt">energy</span> solutions. Molecular solar thermal batteries based on photochromic systems exemplify one possible technology able to harness and apply this potential. Herein is described the synthesis of a macrocycle based on a dimer of the dihydroazulene/vinylheptafulvene (DHA/VHF) photo/thermal couple. By taking advantage of conformational strain, this DHA-DHA macrocycle presents an improved ability to absorb and store incident light <span class="hlt">energy</span> in chemical bonds (VHF-VHF). A stepwise <span class="hlt">energy</span> <span class="hlt">release</span> over two sequential ring-closing reactions (VHF→DHA) combines the advantages of an initially fast discharge, hypothetically addressing immediate <span class="hlt">energy</span> consumption needs, followed by a slow process for consistent, long-term use. This exemplifies another step forward in the molecular engineering and design of functional organic materials towards solar thermal <span class="hlt">energy</span> storage and <span class="hlt">release</span>. © 2016 WILEY-VCH Verlag GmbH & Co. KGaA, Weinheim.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26454181','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26454181"><span>Competitive interactions and controlled <span class="hlt">release</span> of a natural antioxidant from halloysite nanotubes.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Hári, József; Gyürki, Ádám; Sárközi, Márk; Földes, Enikő; Pukánszky, Béla</p> <p>2016-01-15</p> <p>Halloysite nanotubes used as potential carrier material for a controlled <span class="hlt">release</span> stabilizer in polyethylene were thoroughly characterized with several techniques including the measurement of specific surface area, pore volume and surface <span class="hlt">energy</span>. The high surface <span class="hlt">energy</span> of the halloysite results in the strong bonding of the additive to the surface. Dissolution experiments carried out with eight different solvents for the determination of the effect of solvent characteristics on the amount of irreversibly bonded quercetin proved that adsorption and dissolution depend on competitive interactions prevailing in the system. Solvents with low polarity dissolve only surplus quercetin adsorbed in multilayers. Polyethylene is a very apolar polymer forming weak interactions with every substance; quercetin dissolves into it from the halloysite surface only above a critical surface coverage. Stabilization experiments confirmed that strong adhesion prevents dissolution and results in limited stabilization efficiency. At larger adsorbed amounts better stability and extended effect were measured indicating dissolution and controlled <span class="hlt">release</span>. Copyright © 2015 Elsevier Inc. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28913542','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28913542"><span>Metal <span class="hlt">release</span> profiles of orthodontic bands, brackets, and wires: an in vitro study.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Wendl, B; Wiltsche, H; Lankmayr, E; Winsauer, H; Walter, A; Muchitsch, A; Jakse, N; Wendl, M; Wendl, T</p> <p>2017-11-01</p> <p>The present study evaluated the temporal <span class="hlt">release</span> of Co Cr, Mn, and Ni from the components of a typical orthodontic appliance during simulated orthodontic treatment. Several commercially available types of bands, brackets, and wires were exposed to an artificial saliva solution for at least 44 days and the metals <span class="hlt">released</span> were quantified in regular intervals using inductively coupled plasma quadrupole mass spectrometry (ICP-MS, Elan DRC+, Perkin Elmer, USA). Corrosion products encountered on some products were investigated by a scanning electron microscope equipped with an <span class="hlt">energy</span> dispersive X-ray microanalyzer (EDX). Bands <span class="hlt">released</span> the largest quantities of Co, Cr, Mn, and Ni, followed by brackets and wires. Three different temporal metal <span class="hlt">release</span> profiles were observed: (1) constant, though not necessarily linear <span class="hlt">release</span>, (2) saturation (metal <span class="hlt">release</span> stopped after a certain time), and (3) an intermediate <span class="hlt">release</span> profile that showed signs of saturation without reaching saturation. These temporal metal liberation profiles were found to be strongly dependent on the individual test pieces. The corrosion products which developed on some of the bands after a 6-month immersion in artificial saliva and the different metal <span class="hlt">release</span> profiles of the investigated bands were traced back to different attachments welded onto the bands. The use of constant <span class="hlt">release</span> rates will clearly underestimate metal intake by the patient during the first couple of days and overestimate exposure during the remainder of the treatment which is usually several months long. While our data are consistent with heavy metal <span class="hlt">release</span> by orthodontic materials at levels well below typical dietary intake, we nevertheless recommend the use of titanium brackets and replacement of the band with a tube in cases of severe Ni or Cr allergy.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/25976094','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25976094"><span>Differential involvement of IL-6 in the early and late phase of 1-methylnicotinamide (MNA) <span class="hlt">release</span> in Concanavalin A-induced hepatitis.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Sternak, Magdalena; Jakubowski, Andrzej; Czarnowska, Elzbieta; Slominska, Ewa M; Smolenski, Ryszard T; Szafarz, Malgorzata; Walczak, Maria; Sitek, Barbara; Wojcik, Tomasz; Jasztal, Agnieszka; Kaminski, Karol; Chlopicki, Stefan</p> <p>2015-09-01</p> <p>Exogenous 1-methylnicotinamide (MNA) displays anti-inflammatory activity. The aim of this work was to characterize the profile of <span class="hlt">release</span> of endogenous MNA during the initiation and progression of murine hepatitis induced by Concanavalin A (ConA). In particular we aimed to clarify the role of interleukin-6 (IL-6) as well as the <span class="hlt">energy</span> state of hepatocytes in MNA <span class="hlt">release</span> in early and late phases of ConA-induced hepatitis in mice. Hepatitis was induced by ConA in IL-6(+/+) and IL-6(-/-) mice, and various parameters of liver inflammation and injury, as well as the <span class="hlt">energy</span> state of hepatocytes, were analysed in relation to MNA <span class="hlt">release</span>. The decrease in ATP/ADP and NADH/NAD ratios, cytokine <span class="hlt">release</span> (IL-6, IFN-ɤ), acute phase response (e.g. haptoglobin) and liver injury (alanine aminotransaminase, ALT) were all blunted in ConA-induced hepatitis in IL-6(-/-) mice as compared to IL-6(+/+) mice. The <span class="hlt">release</span> of MNA in response to Con A was also significantly blunted in IL-6(-/-) mice as compared to IL-6(+/+) mice in the early stage of ConA-induced hepatitis. In turn, nicotinamide N-methyltransferase (NNMT) and aldehyde oxidase (AO) activities were blunted in the liver and MNA plasma concentration was elevated to similar degree in the late stage after Concanavalin A in IL-6(+/+) and IL-6(-/-) mice. In conclusion, we demonstrated that in ConA-induced hepatitis, early, but not late MNA <span class="hlt">release</span> was IL-6-dependent. Our results suggest that in the initiation and early hepatitis, MNA <span class="hlt">release</span> is linked to the <span class="hlt">energy</span> deficit/impaired redox status in hepatocytes, while in a later phase, MNA <span class="hlt">release</span> is rather linked to the systemic inflammation. Copyright © 2015 Elsevier B.V. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19710000079','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19710000079"><span>High-reliability <span class="hlt">release</span> mechanism</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Paradise, J. J.</p> <p>1971-01-01</p> <p><span class="hlt">Release</span> mechanism employing simple clevis fitting in combination with two pin-pullers achieves high reliability degree through active mechanical redundancy. Mechanism <span class="hlt">releases</span> solar arrays. It is simple and inexpensive and performs effectively. It adapts to other <span class="hlt">release</span>-system applications with variety of pin-puller devices.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1986IJTJE...2..263T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1986IJTJE...2..263T"><span>Spray characteristics of two combined jet atomizers</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Tambour, Y.; Portnoy, D.</p> <p></p> <p>The downstream changes in droplet volume concentration of a vaporizing fuel spray produced by two jet atomizers which form an overlapping zone of influence is theoretically analyzed, employing experimental data of Yule et al. (1982) for a single jet atomizer as initial conditions. One of the atomizers is located below the other at a certain distance downstream. Such an injection geometry can be found in <span class="hlt">afterburners</span> of modern jet engines. The influence of various vertical and horizontal distances between the two atomizers on the downstream spray characteristics is investigated for a vaporizing kerosene spray in a 'cold' (293 K) and a 'hot' (450 K) environment. The analysis shows how one can control the downstream spray characteristics via the geometry of injection. Such geometrical considerations may be of great importance in the design of <span class="hlt">afterburner</span> wall geometry and in the reduction of wall thermal damage. The injection geometry may also affect the intensity of the spray distribution which determines the mode of droplet group combustion. The latter plays an important role in improving <span class="hlt">afterburner</span> combustion efficiency.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/17536177','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/17536177"><span>Mechanisms of HSP72 <span class="hlt">release</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Asea, Alexzander</p> <p>2007-04-01</p> <p>Currently two mechanisms are recognized by which heat shock proteins (HSP) are <span class="hlt">released</span> from cells; a passive <span class="hlt">release</span> mechanism, including necrotic cell death, severe blunt trauma, surgery and following infection with lytic viruses, and an active <span class="hlt">release</span> mechanism which involves the non classical protein <span class="hlt">release</span> pathway. HSPs are <span class="hlt">released</span> both as free HSP and within exosomes. This review covers recent findings on the mechanism by which stress induces the <span class="hlt">release</span> of HSP72 into the circulation and the biological significance of circulating HSP72 to host defense against disease.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.C41D1266C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.C41D1266C"><span>Seismic Signatures of Brine <span class="hlt">Release</span> at Blood Falls, Taylor Glacier, Antarctica</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Carr, C. G.; Pettit, E. C.; Carmichael, J.</p> <p>2017-12-01</p> <p>Blood Falls is created by the <span class="hlt">release</span> of subglacially-sourced, iron-rich brine at the surface of Taylor Glacier, McMurdo Dry Valleys, Antarctica. The supraglacial portion of this hydrological feature is episodically active. Englacial liquid brine flow occurs despite ice temperatures of -17°C and we document supraglacial liquid brine <span class="hlt">release</span> despite ambient air temperatures average -20°C. In this study, we use data from a seismic network, time-lapse cameras, and publicly available weather station data to address the questions: what are the characteristics of seismic events that occur during Blood Falls brine <span class="hlt">release</span> and how do these compare with seismic events that occur during times of Blood Falls quiescence? How are different processes observable in the time-lapse imagery represented in the seismic record? Time-lapse photography constrains the timing of brine <span class="hlt">release</span> events during the austral winter of 2014. We use a noise-adaptive digital power detector to identify seismic events and cluster analysis to identify repeating events based on waveform similarity across the network. During the 2014 wintertime brine <span class="hlt">release</span>, high-<span class="hlt">energy</span> repeated seismic events occurred proximal to Blood Falls. We investigate the ground motions associated with these clustered events, as well as their spatial distribution. We see evidence of possible tremor during the brine <span class="hlt">release</span> periods, an indicator of fluid movement. If distinctive seismic signatures are associated with Blood Falls brine <span class="hlt">release</span> they could be identified based solely on seismic data without any aid from time-lapse cameras. Passive seismologic monitoring has the benefit of continuity during the polar night and other poor visibility conditions, which make time-lapse imagery unusable.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AIPC.1731e0130T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AIPC.1731e0130T"><span>Computational study of a calcium <span class="hlt">release</span>-activated calcium channel</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Talukdar, Keka; Shantappa, Anil</p> <p>2016-05-01</p> <p>The naturally occurring proteins that form hole in membrane are commonly known as ion channels. They play multiple roles in many important biological processes. Deletion or alteration of these channels often leads to serious problems in the physiological processes as it controls the flow of ions through it. The proper maintenance of the flow of ions, in turn, is required for normal health. Here we have investigated the behavior of a calcium <span class="hlt">release</span>-activated calcium ion channel with pdb entry 4HKR in Drosophila Melanogaster. The equilibrium <span class="hlt">energy</span> as well as molecular dynamics simulation is performed first. The protein is subjected to molecular dynamics simulation to find their <span class="hlt">energy</span> minimized value. Simulation of the protein in the environment of water and ions has given us important results too. The solvation <span class="hlt">energy</span> is also found using Charmm potential.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22225153-remedial-investigation-hanford-site-releases-columbia-river','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22225153-remedial-investigation-hanford-site-releases-columbia-river"><span>Remedial Investigation of Hanford Site <span class="hlt">Releases</span> to the Columbia River - 13603</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Lerch, J.A.; Hulstrom, L.C.; Sands, J.P.</p> <p>2013-07-01</p> <p>In south-central Washington State, the Columbia River flows through the U.S. Department of <span class="hlt">Energy</span> Hanford Site. A primary objective of the Hanford Site cleanup mission is protection of the Columbia River, through remediation of contaminated soil and groundwater that resulted from its weapons production mission. Within the Columbia River system, surface water, sediment, and biota samples related to potential Hanford Site hazardous substance <span class="hlt">releases</span> have been collected since the start of Hanford operations. The impacts from <span class="hlt">release</span> of Hanford Site radioactive substances to the Columbia River in areas upstream, within, and downstream of the Hanford Site boundary have been previouslymore » investigated as mandated by the U.S. Department of <span class="hlt">Energy</span> requirements under the Atomic <span class="hlt">Energy</span> Act. The Remedial Investigation Work Plan for Hanford Site <span class="hlt">Releases</span> to the Columbia River [1] was issued in 2008 to initiate assessment of the impacts under the Comprehensive Environmental Response, Compensation, and Liability Act of 1980 [2]. The work plan established a phased approach to characterize contaminants, assess current risks, and determine whether or not there is a need for any cleanup actions. Field investigation activities over a 120-mile stretch of the Columbia River began in October 2008 and were completed in 2010. Sampled media included surface water, pore water, surface and core sediment, island soil, and fish (carp, walleye, whitefish, sucker, small-mouth bass, and sturgeon). Information and sample results from the field investigation were used to characterize current conditions within the Columbia River and assess whether current conditions posed a risk to ecological or human receptors that would merit additional study or response actions under CERCLA. The human health and ecological risk assessments are documented in reports that were published in 2012 [3, 4]. Conclusions from the risk assessment reports are being summarized and integrated with remedial investigation</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28238734','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28238734"><span>Drug <span class="hlt">releasing</span> nanoplatforms activated by alternating magnetic fields.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Mertz, Damien; Sandre, Olivier; Bégin-Colin, Sylvie</p> <p>2017-06-01</p> <p>The use of an alternating magnetic field (AMF) to generate non-invasively and spatially a localized heating from a magnetic nano-mediator has become very popular these last years to develop magnetic hyperthermia (MH) as a promising therapeutic modality already used in the clinics. AMF has become highly attractive this last decade over others radiations, as AMF allows a deeper penetration in the body and a less harmful ionizing effect. In addition to pure MH which induces tumor cell death through local T elevation, this AMF-generated magneto-thermal effect can also be exploited as a relevant external stimulus to trigger a drug <span class="hlt">release</span> from drug-loaded magnetic nanocarriers, temporally and spatially. This review article is focused especially on this concept of AMF induced drug <span class="hlt">release</span>, possibly combined with MH. The design of such magnetically responsive drug delivery nanoplatforms requires two key and complementary components: a magnetic mediator which collects and turns the magnetic <span class="hlt">energy</span> into local heat, and a thermoresponsive carrier ensuring thermo-induced drug <span class="hlt">release</span>, as a consequence of magnetic stimulus. A wide panel of magnetic nanomaterials/chemistries and processes are currently developed to achieve such nanoplatforms. This review article presents a broad overview about the fundamental concepts of drug <span class="hlt">releasing</span> nanoplatforms activated by AMF, their formulations, and their efficiency in vitro and in vivo. This article is part of a Special Issue entitled "Recent Advances in Bionanomaterials" Guest Editors: Dr. Marie-Louise Saboungi and Dr. Samuel D. Bader. Copyright © 2017 Elsevier B.V. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/25373951','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25373951"><span><span class="hlt">Energy</span> balance during underwater implosion of ductile metallic cylinders.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Chamberlin, Ryan E; Guzas, Emily L; Ambrico, Joseph M</p> <p>2014-11-01</p> <p><span class="hlt">Energy</span>-based metrics are developed and applied to a numerical test case of implosion of an underwater pressure vessel. The <span class="hlt">energy</span> metrics provide estimates of the initial <span class="hlt">energy</span> in the system (potential <span class="hlt">energy</span>), the <span class="hlt">energy</span> <span class="hlt">released</span> into the fluid as a pressure pulse, the <span class="hlt">energy</span> absorbed by the imploding structure, and the <span class="hlt">energy</span> absorbed by air trapped within the imploding structure. The primary test case considered is the implosion of an aluminum cylinder [diameter: 2.54 cm (1 in.), length: 27.46 cm (10.81 in.)] that collapses flat in a mode-2 shape with minimal fracture. The test case indicates that the structure absorbs the majority (92%) of the initial <span class="hlt">energy</span> in the system. Consequently, the <span class="hlt">energy</span> emitted as a pressure pulse into the fluid is a small fraction, approximately 5%, of the initial <span class="hlt">energy</span>. The <span class="hlt">energy</span> absorbed by the structure and the <span class="hlt">energy</span> emitted into the fluid are calculated for additional simulations of underwater pressure vessel implosions. For all cases investigated, there is minimal fracture in the collapse, the structure absorbs more than 80% of the initial <span class="hlt">energy</span> of the system, and the <span class="hlt">released</span> pressure pulse carries away less than 6% of the initial <span class="hlt">energy</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014AGUFM.H24E..01B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AGUFM.H24E..01B"><span>Equilibrium and Kinetic Models for Colloid <span class="hlt">Release</span> Under Transient Solution Chemistry Conditions</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bradford, S. A.; Torkzaban, S.; Leij, F. J.; Simunek, J.</p> <p>2014-12-01</p> <p>Colloid retention and <span class="hlt">release</span> is well known to depend on a wide variety of physical, chemical, and microbiological factors that may vary temporally in the subsurface environment. We present equilibrium, kinetic, combined equilibrium and kinetic, and two-site kinetic models of colloid <span class="hlt">release</span> during transient physicochemical conditions. Our mathematical modeling approach relates colloid <span class="hlt">release</span> under transient conditions to changes in the fraction of the solid surface area that contributes to retention. The developed models were subsequently applied to experimental colloid <span class="hlt">release</span> datasets to investigate the influence of variations in ionic strength (IS), pH, cation exchange, colloid size, and water velocity on <span class="hlt">release</span>. Various combinations of equilibrium and/or kinetic <span class="hlt">release</span> models were needed to describe the experimental data depending on the transient conditions and colloid type. <span class="hlt">Release</span> of E. coli D21g was promoted by a decrease in solution IS and an increase in pH, similar to expected trends for a reduction in the secondary minimum and nanoscale chemical heterogeneity, respectively. The retention and <span class="hlt">release</span> of 20 nm carboxyl modified latex nanoparticles (NPs) were demonstrated to be more sensitive to the presence of Ca2+ than D21g. Specifically, retention of NPs was greater than D21g in the presence of 2 mM CaCl2 solution, and <span class="hlt">release</span> of NPs only occurred after exchange of Ca2+ by Na+ and then a reduction in the solution IS. These findings highlight the limitations of conventional interaction <span class="hlt">energy</span> calculations to describe colloid retention and <span class="hlt">release</span>, and point to the need to consider Born repulsion and nanoscale heterogeneity. Temporal changes in the water velocity did not have a large influence on the <span class="hlt">release</span> of D21g. This insensitivity was likely due to factors that reduce the applied hydrodynamic torque and/or increase the resisting adhesive torque. Collectively, experimental and modeling results indicate that episodic colloid transport in the</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li class="active"><span>24</span></li> <li><a href="#" onclick='return showDiv("page_25");'>25</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_24 --> <div id="page_25" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li><a href="#" onclick='return showDiv("page_24");'>24</a></li> <li class="active"><span>25</span></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="481"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013PhDT.......281B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013PhDT.......281B"><span>Implementation of a Thermodynamic Solver within a Computer Program for Calculating Fission-Product <span class="hlt">Release</span> Fractions</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Barber, Duncan Henry</p> <p></p> <p>During some postulated accidents at nuclear power stations, fuel cooling may be impaired. In such cases, the fuel heats up and the subsequent increased fission-gas <span class="hlt">release</span> from the fuel to the gap may result in fuel sheath failure. After fuel sheath failure, the barrier between the coolant and the fuel pellets is lost or impaired, gases and vapours from the fuel-to-sheath gap and other open voids in the fuel pellets can be vented. Gases and steam from the coolant can enter the broken fuel sheath and interact with the fuel pellet surfaces and the fission-product inclusion on the fuel surface (including material at the surface of the fuel matrix). The chemistry of this interaction is an important mechanism to model in order to assess fission-product <span class="hlt">releases</span> from fuel. Starting in 1995, the computer program SOURCE 2.0 was developed by the Canadian nuclear industry to model fission-product <span class="hlt">release</span> from fuel during such accidents. SOURCE 2.0 has employed an early thermochemical model of irradiated uranium dioxide fuel developed at the Royal Military College of Canada. To overcome the limitations of computers of that time, the implementation of the RMC model employed lookup tables to pre-calculated equilibrium conditions. In the intervening years, the RMC model has been improved, the power of computers has increased significantly, and thermodynamic subroutine libraries have become available. This thesis is the result of extensive work based on these three factors. A prototype computer program (referred to as SC11) has been developed that uses a thermodynamic subroutine library to calculate thermodynamic equilibria using Gibbs <span class="hlt">energy</span> minimization. The Gibbs <span class="hlt">energy</span> minimization requires the system temperature (T) and pressure (P), and the inventory of chemical elements (n) in the system. In order to calculate the inventory of chemical elements in the fuel, the list of nuclides and nuclear isomers modelled in SC11 had to be expanded from the list used by SOURCE 2.0. A</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://eric.ed.gov/?q=fossils&pg=6&id=EJ967535','ERIC'); return false;" href="https://eric.ed.gov/?q=fossils&pg=6&id=EJ967535"><span><span class="hlt">ENERGY</span> STAR and Green Buildings--Using <span class="hlt">ENERGY</span> STAR Resources for Green Building Rating Systems: LEED[R], Green Globes[R] and CHPS</span></a></p> <p><a target="_blank" href="http://www.eric.ed.gov/ERICWebPortal/search/extended.jsp?_pageLabel=advanced">ERIC Educational Resources Information Center</a></p> <p>Utebay, Kudret</p> <p>2011-01-01</p> <p>Every building, from the smallest school to the tallest skyscraper, uses <span class="hlt">energy</span>. This <span class="hlt">energy</span> is most often generated by burning fossil fuels, which <span class="hlt">releases</span> greenhouse gases into the atmosphere and contributes to climate change. Existing commercial buildings offer a significant opportunity for low-cost, immediate emissions and <span class="hlt">energy</span> cost…</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29869670','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29869670"><span>Yield of reversible colloidal gels during flow start-up: <span class="hlt">release</span> from kinetic arrest.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Johnson, Lilian C; Landrum, Benjamin J; Zia, Roseanna N</p> <p>2018-06-05</p> <p>Yield of colloidal gels during start-up of shear flow is characterized by an overshoot in shear stress that accompanies changes in network structure. Prior studies of yield of reversible colloidal gels undergoing strong flow model the overshoot as the point at which network rupture permits fluidization. However, yield under weak flow, which is of interest in many biological and industrial fluids shows no such disintegration. The mechanics of reversible gels are influenced by bond strength and durability, where ongoing rupture and re-formation impart aging that deepens kinetic arrest [Zia et al., J. Rheol., 2014, 58, 1121], suggesting that yield be viewed as <span class="hlt">release</span> from kinetic arrest. To explore this idea, we study reversible colloidal gels during start-up of shear flow via dynamic simulation, connecting rheological yield to detailed measurements of structure, bond dynamics, and potential <span class="hlt">energy</span>. We find that pre-yield stress grows temporally with the changing roles of microscopic transport processes: early time behavior is set by Brownian diffusion; later, advective displacements permit relative particle motion that stretches bonds and stores <span class="hlt">energy</span>. Stress accumulates in stretched, oriented bonds until yield, which is a tipping point to <span class="hlt">energy</span> <span class="hlt">release</span>, and is passed with a fully intact network, where the loss of very few bonds enables relaxation of many, easing glassy arrest. This is immediately followed by a reversal to growth in potential <span class="hlt">energy</span> during bulk plastic deformation and condensation into larger particle domains, supporting the view that yield is an activated <span class="hlt">release</span> from kinetic arrest. The continued condensation of dense domains and shrinkage of network surfaces, along with a decrease in the potential <span class="hlt">energy</span>, permit the gel to evolve toward more complete phase separation, supporting our view that yield of weakly sheared gels is a 'non-equilibrium phase transition'. Our findings may be particularly useful for industrial or other coatings, where weak</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28419724','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28419724"><span>A Reversed Photosynthesis-like Process for Light-Triggered CO2 Capture, <span class="hlt">Release</span>, and Conversion.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Wang, Dingguan; Liao, Shenglong; Zhang, Shiming; Wang, Yapei</p> <p>2017-06-22</p> <p>Materials for CO 2 capture have been extensively exploited for climate governance and gas separation. However, their regeneration is facing the problems of high <span class="hlt">energy</span> cost and secondary CO 2 contamination. Herein, a reversed photosynthesis-like process is proposed, in which CO 2 is absorbed in darkness while being <span class="hlt">released</span> under light illumination. The process is likely supplementary to natural photosynthesis of plants, in which, on the contrary, CO 2 is <span class="hlt">released</span> during the night. Remarkably, the material used here is able to capture 9.6 wt.% CO 2 according to its active component. Repeatable CO 2 capture at room temperature and <span class="hlt">release</span> under light irradiation ensures its convenient and cost-effective regeneration. Furthermore, CO 2 <span class="hlt">released</span> from the system is successfully converted into a stable compound in tandem with specific catalysts. © 2017 Wiley-VCH Verlag GmbH & Co. KGaA, Weinheim.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/22582904','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/22582904"><span>Optimization of propranolol HCl <span class="hlt">release</span> kinetics from press coated sustained <span class="hlt">release</span> tablets.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Ali, Adel Ahmed; Ali, Ahmed Mahmoud</p> <p>2013-01-01</p> <p>Press-coated sustained <span class="hlt">release</span> tablets offer a valuable, cheap and easy manufacture alternative to the highly expensive, multi-step manufacture and filling of coated beads. In this study, propranolol HCl press-coated tablets were prepared using hydroxylpropylmethylcellulose (HPMC) as tablet coating material together with carbopol 971P and compressol as <span class="hlt">release</span> modifiers. The prepared formulations were optimized for zero-order <span class="hlt">release</span> using artificial neural network program (INForm, Intelligensys Ltd, North Yorkshire, UK). Typical zero-order <span class="hlt">release</span> kinetics with extended <span class="hlt">release</span> profile for more than 12 h was obtained. The most important variables considered by the program in optimizing formulations were type and proportion of polymer mixture in the coat layer and distribution ratio of drug between core and coat. The key elements found were; incorporation of 31-38 % of the drug in the coat, fixing the amount of polymer in coat to be not less than 50 % of coat layer. Optimum zero-order <span class="hlt">release</span> kinetics (linear regression r2 = 0.997 and Peppas model n value > 0.80) were obtained when 2.5-10 % carbopol and 25-42.5% compressol were incorporated into the 50 % HPMC coat layer.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29337660','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29337660"><span>Guidance for Evaluating the Safety of Experimental <span class="hlt">Releases</span> of Mosquitoes, Emphasizing Mark-<span class="hlt">Release</span>-Recapture Techniques.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Benedict, Mark Q; Charlwood, J Derek; Harrington, Laura C; Lounibos, L Philip; Reisen, William K; Tabachnick, Walter J</p> <p>2018-01-01</p> <p>Experimental <span class="hlt">releases</span> of mosquitoes are performed to understand characteristics of populations related to the biology, ability to transmit pathogens, and ultimately their control. In this article, we discuss considerations related to the safety of experimental <span class="hlt">releases</span> of living mosquitoes, applying principles of good practice in vector biology that protect human health and comfort. We describe specific factors of experimental <span class="hlt">releases</span> of mosquitoes that we believe are critical to inform institutional biosafety committees and similar review boards to which proposals to conduct mosquito <span class="hlt">release</span> experiments have been submitted. In this study, "experimental <span class="hlt">releases</span>" means those that do not significantly increase vector capacity or nuisance biting relative to the unperturbed natural baseline. This document specifically does not address <span class="hlt">releases</span> of mosquitoes for ongoing control programs or trials of new control methods for which broader assessments of risk are required. It also does not address <span class="hlt">releases</span> of transgenic or exotic (non-native) mosquito species, both of which require particular regulatory approval. Experimental <span class="hlt">releases</span> may include females and males and evaluation must consider their effects based on the number <span class="hlt">released</span>, their genotype and phenotype, the environment into which they are <span class="hlt">released</span>, and postrelease collection activities. We consider whether increases of disease transmission and nuisance biting might result from proposed experimental <span class="hlt">releases</span> against the backdrop of natural population size variation. We recommend that experimental <span class="hlt">releases</span> be conducted in a manner that can be reasonably argued to have insignificant negative effects. Reviewers of proposals for experimental <span class="hlt">releases</span> should expect applicants to provide such an argument based on evidence from similar studies and their planned activities. This document provides guidance for creating and evaluating such proposals.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4046803','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4046803"><span>Near-Infrared-Induced Heating of Confined Water in Polymeric Particles for Efficient Payload <span class="hlt">Release</span></span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p></p> <p>2015-01-01</p> <p>Near-infrared (NIR) light-triggered <span class="hlt">release</span> from polymeric capsules could make a major impact on biological research by enabling remote and spatiotemporal control over the <span class="hlt">release</span> of encapsulated cargo. The few existing mechanisms for NIR-triggered <span class="hlt">release</span> have not been widely applied because they require custom synthesis of designer polymers, high-powered lasers to drive inefficient two-photon processes, and/or coencapsulation of bulky inorganic particles. In search of a simpler mechanism, we found that exposure to laser light resonant with the vibrational absorption of water (980 nm) in the NIR region can induce <span class="hlt">release</span> of payloads encapsulated in particles made from inherently non-photo-responsive polymers. We hypothesize that confined water pockets present in hydrated polymer particles absorb electromagnetic <span class="hlt">energy</span> and transfer it to the polymer matrix, inducing a thermal phase change. In this study, we show that this simple and highly universal strategy enables instantaneous and controlled <span class="hlt">release</span> of payloads in aqueous environments as well as in living cells using both pulsed and continuous wavelength lasers without significant heating of the surrounding aqueous solution. PMID:24717072</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/24717072','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/24717072"><span>Near-infrared-induced heating of confined water in polymeric particles for efficient payload <span class="hlt">release</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Viger, Mathieu L; Sheng, Wangzhong; Doré, Kim; Alhasan, Ali H; Carling, Carl-Johan; Lux, Jacques; de Gracia Lux, Caroline; Grossman, Madeleine; Malinow, Roberto; Almutairi, Adah</p> <p>2014-05-27</p> <p>Near-infrared (NIR) light-triggered <span class="hlt">release</span> from polymeric capsules could make a major impact on biological research by enabling remote and spatiotemporal control over the <span class="hlt">release</span> of encapsulated cargo. The few existing mechanisms for NIR-triggered <span class="hlt">release</span> have not been widely applied because they require custom synthesis of designer polymers, high-powered lasers to drive inefficient two-photon processes, and/or coencapsulation of bulky inorganic particles. In search of a simpler mechanism, we found that exposure to laser light resonant with the vibrational absorption of water (980 nm) in the NIR region can induce <span class="hlt">release</span> of payloads encapsulated in particles made from inherently non-photo-responsive polymers. We hypothesize that confined water pockets present in hydrated polymer particles absorb electromagnetic <span class="hlt">energy</span> and transfer it to the polymer matrix, inducing a thermal phase change. In this study, we show that this simple and highly universal strategy enables instantaneous and controlled <span class="hlt">release</span> of payloads in aqueous environments as well as in living cells using both pulsed and continuous wavelength lasers without significant heating of the surrounding aqueous solution.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=1192992','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=1192992"><span>Canine bombesin-like gastrin <span class="hlt">releasing</span> peptides stimulate gastrin <span class="hlt">release</span> and acid secretion in the dog.</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Bunnett, N W; Clark, B; Debas, H T; Del Milton, R C; Kovacs, T O; Orloff, M S; Pappas, T N; Reeve, J R; Rivier, J E; Walsh, J H</p> <p>1985-01-01</p> <p>The synthetic mammalian bombesin-like peptides, canine gastrin <span class="hlt">releasing</span> peptide 27, 23 and 10, and porcine gastrin <span class="hlt">releasing</span> peptide 27 were compared with amphibian bombesin 14 and 10 during intravenous infusions into six conscious dogs with chronic gastric cannulae. Gastrin and gastrin <span class="hlt">releasing</span> peptide were measured in peripherally sampled venous blood by radioimmunoassay and gastric acid secretions were collected. All forms of gastrin <span class="hlt">releasing</span> peptide stimulated gastrin <span class="hlt">release</span> and gastric acid secretion in a dose-dependent manner. The larger canine and porcine peptides were more potent than the decapeptide. Bombesin 14 was more potent than bombesin 10. A rise in the venous concentration of immunoreactive gastrin <span class="hlt">releasing</span> peptide of only 20 fmol ml-1 stimulated gastrin <span class="hlt">release</span> to about 50% of maximal. Gastrin <span class="hlt">releasing</span> peptide 10 was cleared from the circulation three times faster than the larger forms and this may account for the apparent differences in potency. PMID:3839849</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/19124230','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/19124230"><span>IDM <span class="hlt">release</span> behavior and surface characteristics of the novel Cu/IDM/LDPE nanocomposite for intrauterine device.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Yang, Zhihong; Xie, Changsheng; Xiang, Hua; Feng, Jinqing; Xia, Xianping; Cai, Shuizhou</p> <p>2009-03-01</p> <p>Copper/indomethacin/low-density polyethylene (Cu/IDM/LDPE) nanocomposite was prepared as a novel material for intra-uterine device (IUD). IDM <span class="hlt">release</span> profile of the nanocomposite was investigated by using spectrophotometer. The results show that IDM <span class="hlt">release</span> rate of Cu/IDM/LDPE nanocomposite is higher in simulated uterine solution than that in methanol, confirming that the <span class="hlt">release</span> process of IDM is dominated mainly by pore diffusion. The decrease in copper particle size and the increase in copper mass content all accelerate IDM <span class="hlt">release</span>, indicating that IDM <span class="hlt">release</span> rate can be adjusted by changing copper loading or copper particle size. The surface of the incubated nanocomposite was characterized by X-ray diffraction, scanning electron microscopy and <span class="hlt">energy</span> dispersive X-ray microanalysis. A few deposits composed of P, Cl, Ca, Cu and O were observed on the nanocomposite surface, which may be related to the presence of IDM particles with large particle size.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/1977904','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/1977904"><span>Calcium <span class="hlt">released</span> by photolysis of DM-nitrophen stimulates transmitter <span class="hlt">release</span> at squid giant synapse.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Delaney, K R; Zucker, R S</p> <p>1990-07-01</p> <p>1. Transmitter <span class="hlt">release</span> at the squid giant synapse was stimulated by photolytic <span class="hlt">release</span> of Ca2+ from the 'caged' Ca2+ compound DM-nitrophen (Kaplan & Ellis-Davies, 1988) inserted into presynaptic terminals. 2. Competing binding reactions cause the amount of Ca2+ <span class="hlt">released</span> by DM-nitrophen photolysis to depend on the concentrations of DM-nitrophen, total Ca2+, Mg+, ATP and native cytoplasmic Ca2+ buffer. Measurements of presynaptic [Ca2+] changes by co-injection of the fluorescent indicator dye Fura-2 show that DM-nitrophen photolysis causes a transient rise in Ca2+ followed by decay within about 150 ms to an increased steady-state level. 3. Rapid photolysis of Ca2(+)-loaded nitrophen within the presynaptic terminal was followed in less than a millisecond by depolarization of the postsynaptic membrane. As with action potential-evoked excitatory postsynaptic potentials (EPSPs), the light-evoked response was partially and reversibly blocked by 1-3 mM-kainic acid which desensitizes postsynaptic glutamate receptors. 4. <span class="hlt">Release</span> was similar in magnitude and rate to normal action potential-mediated EPSPs. 5. The <span class="hlt">release</span> of transmitter by photolysis of Ca2(+)-loaded DM-nitrophen was not affected by removal of Ca2+ from the saline or addition of tetrodotoxin. Photolysis of DM-nitrophen injected into presynaptic terminals without added Ca2+ did not stimulate <span class="hlt">release</span> of transmitter nor did it interfere with normal action potential-mediated <span class="hlt">release</span>. 6. Stimulation of presynaptic action potentials in Ca2(+)-free saline during the light-evoked response did not elicit increased <span class="hlt">release</span> of transmitter if the ganglion was bathed in Ca2(+)-free saline, i.e. in the absence of Ca2+ influx. Increasing the intensity of the light or stimulating presynaptic action potentials in Ca2(+)-containing saline increased the <span class="hlt">release</span> of transmitter. Therefore the failure of presynaptic voltage change to increase transmitter <span class="hlt">release</span> resulting from <span class="hlt">release</span> of caged Ca2+ was not due to saturation or</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/22610467','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/22610467"><span><span class="hlt">Release</span> behavior of tanshinone IIA sustained-<span class="hlt">release</span> pellets based on crack formation theory.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Liu, Pan; Li, Jin; Liu, Jianping; Yang, Jikun; Fan, Yongqing</p> <p>2012-08-01</p> <p>The objective of this study was to investigate the drug <span class="hlt">release</span> mechanism and in vivo performance of Tanshinone IIA sustained-<span class="hlt">release</span> pellets, coated with blends of polyvinyl acetate (PVAc) and poly(vinyl alcohol)-poly(ethylene glycol) (PVA-PEG) graft copolymer. A formulation screening study showed that pellets coated with PVAc-PVA-PEG at a ratio of 70:30 (w/w) succeeded in achieving a 24 h sustained <span class="hlt">release</span>, irrespective of the coating weight (from 2% to 10%). Both the microscopic observation and mathematical model gave further insight into the underlying <span class="hlt">release</span> mechanism, indicating that diffusion through water-filled cracks was dominant for the control of drug <span class="hlt">release</span>. In vivo test showed that the maximum plasma concentration of sustained-<span class="hlt">release</span> pellets was decreased from 82.13 ± 17.05 to 40.50 ± 11.72 ng mL as that of quick-<span class="hlt">release</span> pellets. The time of maximum concentration, half time, and mean residence time were all prolonged from 3.80 ± 0.40 to 8.02 ± 0.81 h, 4.28 ± 1.21 to 8.18 ± 2.06 h, and 8.60 ± 1.59 to 17.50 ± 2.78 h, compared with uncoated preparations. A good in vitro-in vivo correlation was characterized by a high coefficient of determination (r = 0.9772). In conclusion, pellets coated with PVAc-PVA-PEG could achieve a satisfactory sustained-<span class="hlt">release</span> behavior based on crack formation theory. Copyright © 2012 Wiley Periodicals, Inc.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/ADP000437','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADP000437"><span>Yield and Blast Analyses with a Unified Theory of Explosions</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>1982-08-01</p> <p>and <span class="hlt">afterburning</span> of PBXN 103. The ambient conditions are for the test site at Socorro, NM, altitude -- 5200 feet. The input mass was 1038 pounds...essentially the warhead, most of which is PBXN -103. This was the very first test of the code. The relative yield is plFj.ed as T (time). The TOA yield, .90...YO =YO*1.0 ’Relative yields from earlier runs or fits 52 ’ 1 G = 106 cal = 4pi/3*le6 kg m^2/m^3/sec^2 53 AB=.00 ’<span class="hlt">Afterburning</span> fraction 56 YO = Y0*(I</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19910004943','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19910004943"><span>Kinetics of hydrogen <span class="hlt">release</span> from lunar soil</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Bustin, Roberta</p> <p>1990-01-01</p> <p>With increasing interest in a lunar base, there is a need for extensive examination of possible lunar resources. Hydrogen will be needed on a lunar base for many activities including providing fuel, making water, and serving as a reducing agent in the extraction of oxygen from its ores. Previous studies have shown the solar wind has implanted hydrogen in the lunar regolith and that hydrogen is present not only in the outer layer of soil but to considerable depths, depending on the sampling site. If this hydrogen is to be mined and used on the lunar surface, a number of questions need to be answered. How much <span class="hlt">energy</span> must be expended in order to <span class="hlt">release</span> the hydrogen from the soil. What temperatures must be attained, and how long must the soil be heated. This study was undertaken to provide answers to practical questions such as these. Hydrogen was determined using a Pyrolysis/GC technique in which hydrogen was <span class="hlt">released</span> by heating the soil sample contained in a quartz tube in a resistance wire furnace, followed by separation and quantitative determination using a gas chromatograph with a helium ionization detector. Heating times and temperatures were varied, and particle separates were studied in addition to bulk soils. The typical sample size was 10 mg of lunar soil. All of the soils used were mature soils with similar hydrogen abundances. Pre-treatments with air and steam were used in an effort to find a more efficient way of <span class="hlt">releasing</span> hydrogen.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012PhDT.......382B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012PhDT.......382B"><span>Fluoride <span class="hlt">release</span>, recharge, and re-<span class="hlt">release</span> from four orthodontic bonding systems</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bouvier, Amy Johanna</p> <p></p> <p>Objectives: To determine the amount of initial fluoride <span class="hlt">release</span> from four orthodontic bonding systems over a period of four weeks, and then to subject these materials to an external source of fluoride for recharge in order to measure the amount of fluoride re-<span class="hlt">release</span> over another four-week interval. Additionally the surface morphology of these materials was analyzed under the scanning electron microscope in order to identify microscopic changes in the materials that may have occurred during the experiment. Methods: Four orthodontic adhesives: Fuji Ortho LC (GC America, Alsip, IL), Transbond XT (3M Unitek, Monrovia, CA), Illuminate Light Cure (Ortho Organizers, Carlsbad, CA), and Opal Seal with Opal Bond MV (Ultradent, South Jordan, UT), n=120 (30/material) were tested for fluoride <span class="hlt">release</span> at 1 hour, 24 hours, 3 days, 1 week, 2 weeks, 3 weeks and 4 weeks. Samples (10/subgroup/material) were then recharged with an external source of fluoride (toothpaste, foam, or varnish), and retested for fluoride re-<span class="hlt">release</span> at 1 hour, 24 hours, 3 days, 1 week, 2 weeks, 3 weeks and 4 weeks. The scanning electron microscope was utilized in order to assess each material's surface morphology before testing and after completion of the experiment (n=16). Descriptive statistics, means and standard deviations were calculated for all four materials and their subgroups at each time interval. A mixed model two-way ANOVA was run, using a level of significance of 0.05. Bonferroni multiple comparison tests were conducted using if groups were found to be statistically significantly different. To determine significant differences between fluoride <span class="hlt">release</span> and re-<span class="hlt">release</span> for each recharge subgroup within each material group, paired t-tests were performed for the time intervals of 24 hours, 2 weeks, and 4 weeks. For the paired t-tests, the level of significance used was 0.02 to allow for Bonferroni correction. Results: During the initial 24 hours the fluoride measurements (in mg/L or ppm) were as</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5846569','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5846569"><span>Guidance for Evaluating the Safety of Experimental <span class="hlt">Releases</span> of Mosquitoes, Emphasizing Mark-<span class="hlt">Release</span>-Recapture Techniques</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Charlwood, J. Derek; Harrington, Laura C.; Lounibos, L. Philip; Reisen, William K.; Tabachnick, Walter J.</p> <p>2018-01-01</p> <p>Abstract Experimental <span class="hlt">releases</span> of mosquitoes are performed to understand characteristics of populations related to the biology, ability to transmit pathogens, and ultimately their control. In this article, we discuss considerations related to the safety of experimental <span class="hlt">releases</span> of living mosquitoes, applying principles of good practice in vector biology that protect human health and comfort. We describe specific factors of experimental <span class="hlt">releases</span> of mosquitoes that we believe are critical to inform institutional biosafety committees and similar review boards to which proposals to conduct mosquito <span class="hlt">release</span> experiments have been submitted. In this study, “experimental releases” means those that do not significantly increase vector capacity or nuisance biting relative to the unperturbed natural baseline. This document specifically does not address <span class="hlt">releases</span> of mosquitoes for ongoing control programs or trials of new control methods for which broader assessments of risk are required. It also does not address <span class="hlt">releases</span> of transgenic or exotic (non-native) mosquito species, both of which require particular regulatory approval. Experimental <span class="hlt">releases</span> may include females and males and evaluation must consider their effects based on the number <span class="hlt">released</span>, their genotype and phenotype, the environment into which they are <span class="hlt">released</span>, and postrelease collection activities. We consider whether increases of disease transmission and nuisance biting might result from proposed experimental <span class="hlt">releases</span> against the backdrop of natural population size variation. We recommend that experimental <span class="hlt">releases</span> be conducted in a manner that can be reasonably argued to have insignificant negative effects. Reviewers of proposals for experimental <span class="hlt">releases</span> should expect applicants to provide such an argument based on evidence from similar studies and their planned activities. This document provides guidance for creating and evaluating such proposals. PMID:29337660</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5381730','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5381730"><span>Dendritic <span class="hlt">release</span> of neurotransmitters</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Ludwig, Mike; Apps, David; Menzies, John; Patel, Jyoti C.; Rice, Margaret E.</p> <p>2017-01-01</p> <p><span class="hlt">Release</span> of neuroactive substances by exocytosis from dendrites is surprisingly widespread and is not confined to a particular class of transmitters: it occurs in multiple brain regions, and includes a range of neuropeptides, classical neurotransmitters and signaling molecules such as nitric oxide, carbon monoxide, ATP and arachidonic acid. This review is focused on hypothalamic neuroendocrine cells that <span class="hlt">release</span> vasopressin and oxytocin and midbrain neurons that <span class="hlt">release</span> dopamine. For these two model systems, the stimuli, mechanisms and physiological functions of dendritic <span class="hlt">release</span> have been explored in greater detail than is yet available for other neurons and neuroactive substances. PMID:28135005</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19790014029','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19790014029"><span>Source of <span class="hlt">released</span> carbon fibers</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Bell, V. L.</p> <p>1979-01-01</p> <p>The potential for the <span class="hlt">release</span> of carbon fibers from aircraft crashes/fires is addressed. Simulation of the conditions of aircraft crash fires in order to predict the quantities and forms of fibrous materials which might be <span class="hlt">released</span> from civilian aircraft crashes/fires is considered. Figures are presented which describe some typical fiber <span class="hlt">release</span> test activities together with some very preliminary results of those activities. The state of the art of carbon fiber <span class="hlt">release</span> is summarized as well as some of the uncertainties concerning accidental fiber <span class="hlt">release</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19930006524','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19930006524"><span>CRRES: The combined <span class="hlt">release</span> and radiation effects satellite program directory</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Layman, Laura D.; Miller, George P.</p> <p>1992-01-01</p> <p>As a result of natural processes, plasma clouds are often injected into the magnetosphere. These chemical <span class="hlt">releases</span> can be used to study many aspects of such injections. When a dense plasma is injected into the inner magnetosphere, it is expected to take up the motion of the ambient plasma. However, it has been observed in previous <span class="hlt">releases</span> at moderate altitudes that the cloud preserved its momentum for some time following the <span class="hlt">release</span> and that parts of the cloud peeled off from the main cloud presumable due to the action of an instability. As one moves outward into the magnetosphere, the mirror force becomes less dominant and the initial conditions following a <span class="hlt">release</span> are dominated by the formation of a diamagnetic cavity since the initial plasma pressure from the injected Ba ions is greater than the magnetic field <span class="hlt">energy</span> density. A previous high-altitude <span class="hlt">release</span> (31,300 km) showed this to be the case initially, but at later times there was evidence for acceleration of the Ba plasma to velocities corresponding to 60,000 K. This effect is not explained. This series of experiments is therefore designed to inject plasma clouds into the magnetosphere under widely varying conditions of magnetic field strength and ambient plasma density. In this way the coupling of injected clouds to the ambient plasma and magnetic field, the formation of striations due to instabilities, and possible heating and acceleration of the injected Ba plasma can be studied over a wide range of magnetosphere parameters. Adding to the scientific yield will be the availability of measurements for the DOD/SPACERAD instruments which can monitor plasma parameters, electric and magnetic fields, and waves before, during and after the <span class="hlt">releases</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.eia.gov/consumption/residential/reports/2009/16-states.cfm','EIAPUBS'); return false;" href="https://www.eia.gov/consumption/residential/reports/2009/16-states.cfm"><span>EIA Household <span class="hlt">Energy</span> Use Data Now Includes Detail on 16 States</span></a></p> <p><a target="_blank" href="http://www.eia.doe.gov/reports/">EIA Publications</a></p> <p></p> <p>2011-01-01</p> <p>The <span class="hlt">Energy</span> Information Administration (EIA) is <span class="hlt">releasing</span> new benchmark estimates for home <span class="hlt">energy</span> use for the year 2009 that include detailed data for 16 states, 12 more than in past EIA residential <span class="hlt">energy</span> surveys.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li><a href="#" onclick='return showDiv("page_24");'>24</a></li> <li class="active"><span>25</span></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_25 --> <div class="footer-extlink text-muted" style="margin-bottom:1rem; text-align:center;">Some links on this page may take you to non-federal websites. 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