Sample records for wall heat fluxes

  1. Comparison of Turbulent Heat-Transfer Results for Uniform Wall Heat Flux and Uniform Wall Temperature

    NASA Technical Reports Server (NTRS)

    Siegel, R.; Sparrow, E. M.

    1960-01-01

    The purpose of this note is to examine in a more precise way how the Nusselt numbers for turbulent heat transfer in both the fully developed and thermal entrance regions of a circular tube are affected by two different wall boundary conditions. The comparisons are made for: (a) Uniform wall temperature (UWT); and (b) uniform wall heat flux (UHF). Several papers which have been concerned with the turbulent thermal entrance region problem are given. 1 Although these analyses have all utilized an eigenvalue formulation for the thermal entrance region there were differences in the choices of eddy diffusivity expressions, velocity distributions, and methods for carrying out the numerical solutions. These differences were also found in the fully developed analyses. Hence when making a comparison of the analytical results for uniform wall temperature and uniform wall heat flux, it was not known if differences in the Nusselt numbers could be wholly attributed to the difference in wall boundary conditions, since all the analytical results were not obtained in a consistent way. To have results which could be directly compared, computations were carried out for the uniform wall temperature case, using the same eddy diffusivity, velocity distribution, and digital computer program employed for uniform wall heat flux. In addition, the previous work was extended to a lower Reynolds number range so that comparisons could be made over a wide range of both Reynolds and Prandtl numbers.

  2. Estimation of transient heat flux density during the heat supply of a catalytic wall steam methane reformer

    NASA Astrophysics Data System (ADS)

    Settar, Abdelhakim; Abboudi, Saïd; Madani, Brahim; Nebbali, Rachid

    2018-02-01

    Due to the endothermic nature of the steam methane reforming reaction, the process is often limited by the heat transfer behavior in the reactors. Poor thermal behavior sometimes leads to slow reaction kinetics, which is characterized by the presence of cold spots in the catalytic zones. Within this framework, the present work consists on a numerical investigation, in conjunction with an experimental one, on the one-dimensional heat transfer phenomenon during the heat supply of a catalytic-wall reactor, which is designed for hydrogen production. The studied reactor is inserted in an electric furnace where the heat requirement of the endothermic reaction is supplied by electric heating system. During the heat supply, an unknown heat flux density, received by the reactive flow, is estimated using inverse methods. In the basis of the catalytic-wall reactor model, an experimental setup is engineered in situ to measure the temperature distribution. Then after, the measurements are injected in the numerical heat flux estimation procedure, which is based on the Function Specification Method (FSM). The measured and estimated temperatures are confronted and the heat flux density which crosses the reactor wall is determined.

  3. FDNS code to predict wall heat fluxes or wall temperatures in rocket nozzles

    NASA Technical Reports Server (NTRS)

    Karr, Gerald R.

    1993-01-01

    This report summarizes the findings on the NASA contract NAG8-212, Task No. 3. The overall project consists of three tasks, all of which have been successfully completed. In addition, some supporting supplemental work, not required by the contract, has been performed and is documented herein. Task 1 involved the modification of the wall functions in the code FDNS to use a Reynolds Analogy-based method. Task 2 involved the verification of the code against experimentally available data. The data chosen for comparison was from an experiment involving the injection of helium from a wall jet. Results obtained in completing this task also show the sensitivity of the FDNS code to unknown conditions at the injection slot. Task 3 required computation of the flow of hot exhaust gases through the P&W 40K subscale nozzle. Computations were performed both with and without film coolant injection. The FDNS program tends to overpredict heat fluxes, but, with suitable modeling of backside cooling, may give reasonable wall temperature predictions. For film cooling in the P&W 40K calorimeter subscale nozzle, the average wall temperature is reduced from 1750 R to about 1050 R by the film cooling. The average wall heat flux is reduced by a factor of three.

  4. Numerical simulation of heat fluxes in a two-temperature plasma at shock tube walls

    NASA Astrophysics Data System (ADS)

    Kuznetsov, E. A.; Poniaev, S. A.

    2015-12-01

    Numerical simulation of a two-temperature three-component Xenon plasma flow is presented. A solver based on the OpenFOAM CFD software package is developed. The heat flux at the shock tube end wall is calculated and compared with experimental data. It is shown that the heat flux due to electrons can be as high as 14% of the total heat flux.

  5. Heat flux microsensor measurements

    NASA Technical Reports Server (NTRS)

    Terrell, J. P.; Hager, J. M.; Onishi, S.; Diller, T. E.

    1992-01-01

    A thin-film heat flux sensor has been fabricated on a stainless steel substrate. The thermocouple elements of the heat flux sensor were nickel and nichrome, and the temperature resistance sensor was platinum. The completed heat flux microsensor was calibrated at the AEDC radiation facility. The gage output was linear with heat flux with no apparent temperature effect on sensitivity. The gage was used for heat flux measurements at the NASA Langley Vitiated Air Test Facility. Vitiated air was expanded to Mach 3.0 and hydrogen fuel was injected. Measurements were made on the wall of a diverging duct downstream of the injector during all stages of the hydrogen combustion tests. Because the wall and the gage were not actively cooled, the wall temperature reached over 1000 C (1900 F) during the most severe test.

  6. Benchmark Wall Heat Flux Data for a GO2/GH2 Single Element Combustor

    NASA Technical Reports Server (NTRS)

    Marshall, William M.; Pal, Sibtosh; Woodward, Roger d.; Santoro, Robert J.

    2005-01-01

    Wall heat flux measurements in a 1.5 in. diameter circular cross-section rocket chamber for a uni-element shear coaxial injector element operating on gaseous oxygen (GOz)/gaseous hydrogen (GH,) propellants are presented. The wall heat flux measurements were made using arrays of Gardon type heat flux gauges and coaxial thermocouple instrumentation. Wall heat flux measurements were made for two cases. For the first case, GOZ/GHz oxidizer-rich (O/F=l65) and fuel-rich preburners (O/F=1.09) integrated with the main chamber were utilized to provide vitiated hot fuel and oxidizer to the study shear coaxial injector element. For the second case, the preburners were removed and ambient temperature gaseous oxygen/gaseous hydrogen propellants were supplied to the study injector. Experiments were conducted at four chamber pressures of 750, 600, 450 and 300psia for each case. The overall mixture ratio for the preburner case was 6.6, whereas for the ambient propellant case, the mixture ratio was 6.0. Total propellant flow was nominally 0.27-0.29 Ibm/s for the 750 psia case with flowrates scaled down linearly for lower chamber pressures. The axial heat flux profile results for both the preburner and ambient propellant cases show peak heat flux levels a t axial locations between 2.0 and 3.0 in. from the injector face. The maximum heat flux level was about two times greater for the preburner case. This is attributed to the higher injector fuel-to-oxidizer momentum flux ratio that promotes mixing and higher initial propellant temperature for the preburner case which results in a shorter reaction zone. The axial heat flux profiles were also scaled with respect to the chamber pressure to the power 0.8. The results at the four chamber pressures for both cases collapsed to a single profile indicating that at least to first approximation, the basic fluid dynamic structures in the flow field are pressure independent as long as the chamber/njector/nozzle geometry and injection velocities

  7. DSMC simulation of rarefied gas flows under cooling conditions using a new iterative wall heat flux specifying technique

    NASA Astrophysics Data System (ADS)

    Akhlaghi, H.; Roohi, E.; Myong, R. S.

    2012-11-01

    Micro/nano geometries with specified wall heat flux are widely encountered in electronic cooling and micro-/nano-fluidic sensors. We introduce a new technique to impose the desired (positive/negative) wall heat flux boundary condition in the DSMC simulations. This technique is based on an iterative progress on the wall temperature magnitude. It is found that the proposed iterative technique has a good numerical performance and could implement both positive and negative values of wall heat flux rates accurately. Using present technique, rarefied gas flow through micro-/nanochannels under specified wall heat flux conditions is simulated and unique behaviors are observed in case of channels with cooling walls. For example, contrary to the heating process, it is observed that cooling of micro/nanochannel walls would result in small variations in the density field. Upstream thermal creep effects in the cooling process decrease the velocity slip despite of the Knudsen number increase along the channel. Similarly, cooling process decreases the curvature of the pressure distribution below the linear incompressible distribution. Our results indicate that flow cooling increases the mass flow rate through the channel, and vice versa.

  8. Effect of Particle Size Distribution on Wall Heat Flux in Pulverized-Coal Furnaces and Boilers

    NASA Astrophysics Data System (ADS)

    Lu, Jun

    A mathematical model of combustion and heat transfer within a cylindrical enclosure firing pulverized coal has been developed and tested against two sets of measured data (one is 1993 WSU/DECO Pilot test data, the other one is the International Flame Research Foundation 1964 Test (Beer, 1964)) and one independent code FURN3D from the Argonne National Laboratory (Ahluwalia and IM, 1992). The model called PILC assumes that the system is a sequence of many well-stirred reactors. A char burnout model combining diffusion to the particle surface, pore diffusion, and surface reaction is employed for predicting the char reaction, heat release, and evolution of char. The ash formation model included relates the ash particle size distribution to the particle size distribution of pulverized coal. The optical constants of char and ash particles are calculated from dispersion relations derived from reflectivity, transmissivity and extinction measurements. The Mie theory is applied to determine the extinction and scattering coefficients. The radiation heat transfer is modeled using the virtual zone method, which leads to a set of simultaneous nonlinear algebraic equations for the temperature field within the furnace and on its walls. This enables the heat fluxes to be evaluated. In comparisons with the experimental data and one independent code, the model is successful in predicting gas temperature, wall temperature, and wall radiative flux. When the coal with greater fineness is burnt, the particle size of pulverized coal has a consistent influence on combustion performance: the temperature peak was higher and nearer to burner, the radiation flux to combustor wall increased, and also the absorption and scattering coefficients of the combustion products increased. The effect of coal particle size distribution on absorption and scattering coefficients and wall heat flux is significant. But there is only a small effect on gas temperature and fuel fraction burned; it is speculated

  9. Heat Flux and Wall Temperature Estimates for the NASA Langley HIFiRE Direct Connect Rig

    NASA Technical Reports Server (NTRS)

    Cuda, Vincent, Jr.; Hass, Neal E.

    2010-01-01

    An objective of the Hypersonic International Flight Research Experimentation (HIFiRE) Program Flight 2 is to provide validation data for high enthalpy scramjet prediction tools through a single flight test and accompanying ground tests of the HIFiRE Direct Connect Rig (HDCR) tested in the NASA LaRC Arc Heated Scramjet Test Facility (AHSTF). The HDCR is a full-scale, copper heat sink structure designed to simulate the isolator entrance conditions and isolator, pilot, and combustor section of the HIFiRE flight test experiment flowpath and is fully instrumented to assess combustion performance over a range of operating conditions simulating flight from Mach 5.5 to 8.5 and for various fueling schemes. As part of the instrumentation package, temperature and heat flux sensors were provided along the flowpath surface and also imbedded in the structure. The purpose of this paper is to demonstrate that the surface heat flux and wall temperature of the Zirconia coated copper wall can be obtained with a water-cooled heat flux gage and a sub-surface temperature measurement. An algorithm was developed which used these two measurements to reconstruct the surface conditions along the flowpath. Determinations of the surface conditions of the Zirconia coating were conducted for a variety of conditions.

  10. CFD Code Validation of Wall Heat Fluxes for a G02/GH2 Single Element Combustor

    NASA Technical Reports Server (NTRS)

    Lin, Jeff; West, Jeff S.; Williams, Robert W.; Tucker, P. Kevin

    2005-01-01

    This paper puts forth the case for the need for improved injector design tools to meet NASA s Vision for Space Exploration goals. Requirements for this improved tool are outlined and discussed. The potential for Computational Fluid Dynamics (CFD) to meet these requirements is noted along with its current shortcomings, especially relative to demonstrated solution accuracy. The concept of verification and validation is introduced as the primary process for building and quantifying the confidence necessary for CFD to be useful as an injector design tool. The verification and validation process is considered in the context of the Marshall Space Flight Center (MSFC) Combustion Devices CFD Simulation Capability Roadmap via the Simulation Readiness Level (SRL) concept. The portion of the validation process which demonstrates the ability of a CFD code to simulate heat fluxes to a rocket engine combustor wall is the focus of the current effort. The FDNS and Loci-CHEM codes are used to simulate a shear coaxial single element G02/GH2 injector experiment. The experiment was conducted a t a chamber pressure of 750 psia using hot propellants from preburners. A measured wall temperature profile is used as a boundary condition to facilitate the calculations. Converged solutions, obtained from both codes by using wall functions with the K-E turbulence model and integrating to the wall using Mentor s baseline turbulence model, are compared to the experimental data. The initial solutions from both codes revealed significant issues with the wall function implementation associated with the recirculation zone between the shear coaxial jet and the chamber wall. The FDNS solution with a corrected implementation shows marked improvement in overall character and level of comparison to the data. With the FDNS code, integrating to the wall with Mentor s baseline turbulence model actually produce a degraded solution when compared to the wall function solution with the K--E model. The Loci

  11. Simplified model for determining local heat flux boundary conditions for slagging wall

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

    Bingzhi Li; Anders Brink; Mikko Hupa

    2009-07-15

    In this work, two models for calculating heat transfer through a cooled vertical wall covered with a running slag layer are investigated. The first one relies on a discretization of the velocity equation, and the second one relies on an analytical solution. The aim is to find a model that can be used for calculating local heat flux boundary conditions in computational fluid dynamics (CFD) analysis of such processes. Two different cases where molten deposits exist are investigated: the black liquor recovery boiler and the coal gasifier. The results show that a model relying on discretization of the velocity equationmore » is more flexible in handling different temperature-viscosity relations. Nevertheless, a model relying on an analytical solution is the one fast enough for a potential use as a CFD submodel. Furthermore, the influence of simplifications to the heat balance in the model is investigated. It is found that simplification of the heat balance can be applied when the radiation heat flux is dominant in the balance. 9 refs., 7 figs., 10 tabs.« less

  12. Self-pressurization of a flightweight liquid hydrogen tank: Effects of fill level at low wall heat flux

    NASA Technical Reports Server (NTRS)

    Vandresar, N. T.; Hasan, M. M.; Lin, C.-S.

    1991-01-01

    Experimental results are presented for the self pressurization and thermal stratification of a 4.89 cu m liquid hydrogen storage tank subjected to low heat flux (2.0 and 3.5 W/sq m) in normal gravity. The test tank was representative of future spacecraft tankage, having a low mass to volume ratio and high performance multilayer thermal insulation. Tests were performed at fill levels of 29 and 49 pcts. (by volume) and complement previous tests at 83 pct. fill. As the heat flux increases, the pressure rise rate at each fill level exceeds the homogeneous rate by an increasing ratio. Herein, this ratio did not exceed a value of 2. The slowest pressure rise rate was observed for the 49 pct. fill level at both heat fluxes. This result is attributed to the oblate spheroidal tank geometry which introduces the variables of wetted wall area, liquid-vapor interfacial area, and ratio of side wall to bottom heating as a function of fill level or liquid depth. Initial tank thermal conditions were found to affect the initial pressure rise rate. Quasi steady pressure rise rates are independent of starting conditions.

  13. Convective heat transfer for a gaseous slip flow in micropipe and parallel-plate microchannel with uniform wall heat flux: effect of axial heat conduction

    NASA Astrophysics Data System (ADS)

    Haddout, Y.; Essaghir, E.; Oubarra, A.; Lahjomri, J.

    2017-12-01

    Thermally developing laminar slip flow through a micropipe and a parallel plate microchannel, with axial heat conduction and uniform wall heat flux, is studied analytically by using a powerful method of self-adjoint formalism. This method results from a decomposition of the elliptic energy equation into a system of two first-order partial differential equations. The advantage of this method over other methods, resides in the fact that the decomposition procedure leads to a selfadjoint problem although the initial problem is apparently not a self-adjoint one. The solution is an extension of prior studies and considers a first order slip model boundary conditions at the fluid-wall interface. The analytical expressions for the developing temperature and local Nusselt number in the thermal entrance region are obtained in the general case. Therefore, the solution obtained could be extended easily to any hydrodynamically developed flow and arbitrary heat flux distribution. The analytical results obtained are compared for select simplified cases with available numerical calculations and they both agree. The results show that the heat transfer characteristics of flow in the thermal entrance region are strongly influenced by the axial heat conduction and rarefaction effects which are respectively characterized by Péclet and Knudsen numbers.

  14. Convective heat transfer for a gaseous slip flow in micropipe and parallel-plate microchannel with uniform wall heat flux: effect of axial heat conduction

    NASA Astrophysics Data System (ADS)

    Haddout, Y.; Essaghir, E.; Oubarra, A.; Lahjomri, J.

    2018-06-01

    Thermally developing laminar slip flow through a micropipe and a parallel plate microchannel, with axial heat conduction and uniform wall heat flux, is studied analytically by using a powerful method of self-adjoint formalism. This method results from a decomposition of the elliptic energy equation into a system of two first-order partial differential equations. The advantage of this method over other methods, resides in the fact that the decomposition procedure leads to a selfadjoint problem although the initial problem is apparently not a self-adjoint one. The solution is an extension of prior studies and considers a first order slip model boundary conditions at the fluid-wall interface. The analytical expressions for the developing temperature and local Nusselt number in the thermal entrance region are obtained in the general case. Therefore, the solution obtained could be extended easily to any hydrodynamically developed flow and arbitrary heat flux distribution. The analytical results obtained are compared for select simplified cases with available numerical calculations and they both agree. The results show that the heat transfer characteristics of flow in the thermal entrance region are strongly influenced by the axial heat conduction and rarefaction effects which are respectively characterized by Péclet and Knudsen numbers.

  15. Progress on performance assessment of ITER enhanced heat flux first wall technology after neutron irradiation

    NASA Astrophysics Data System (ADS)

    Hirai, T.; Bao, L.; Barabash, V.; Chappuis, Ph; Eaton, R.; Escourbiac, F.; Giqcuel, S.; Merola, M.; Mitteau, R.; Raffray, R.; Linke, J.; Loewenhoff, Th; Pintsuk, G.; Wirtz, M.; Boomstra, D.; Magielsen, A.; Chen, J.; Wang, P.; Gervash, A.; Safronov, V.

    2016-02-01

    ITER first wall (FW) panels are irradiated by energetic neutrons during the nuclear phase. Thus, an irradiation and high heat flux testing programme is undertaken by the ITER organization in order to evaluate the effects of neutron irradiation on the performance of enhanced heat flux (EHF) FW components. The test campaign includes neutron irradiation (up to 0.6-0.8 dpa at 200 °C-250 °C) of mock-ups that are representative of the final EHF FW panel design, followed by thermal fatigue tests (up to 4.7 MW m-2). Mock-ups were manufactured by the same manufacturing process as proposed for the series production. After a pre-irradiation thermal screening, eight mock-ups will be selected for the irradiation campaigns. This paper reports the preparatory work of HHF tests and neutron irradiation, assessment results as well as a brief description of mock-up manufacturing and inspection routes.

  16. Experimental study of laminar forced convective heat transfer of deionized water based copper (I) oxide nanofluids in a tube with constant wall heat flux

    NASA Astrophysics Data System (ADS)

    Umer, Asim; Naveed, Shahid; Ramzan, Naveed

    2016-10-01

    Nanofluids, having 1-100 nm size particles in any base fluid are promising fluid for heat transfer intensification due to their enhanced thermal conductivity as compared with the base fluid. The forced convection of nanofluids is the major practical application in heat transfer equipments. In this study, heat transfer enhancements at constant wall heat flux under laminar flow conditions were investigated. Nanofluids of different volume fractions (1, 2 and 4 %) of copper (I) oxide nanoparticles in deionized water were prepared using two step technique under mechanical mixing and ultrasonication. The results were investigated by increasing the Reynolds number of the nanofluids at constant heat flux. The trends of Nusselt number variation with dimensionless length (X/D) and Reynolds numbers were studied. It was observed that heat transfer coefficient increases with increases particles volume concentration and Reynolds number. The maximum enhancement in heat transfer coefficient of 61 % was observed with 4 % particle volume concentration at Reynolds number (Re ~ 605).

  17. Supercritical convection, critical heat flux, and coking characteristics of propane

    NASA Technical Reports Server (NTRS)

    Rousar, D. C.; Gross, R. S.; Boyd, W. C.

    1984-01-01

    The heat transfer characteristics of propane at subcritical and supercritical pressure were experimentally evaluated using electrically heated Monel K-500 tubes. A design correlation for supercritical heat transfer coefficient was established using the approach previously applied to supercritical oxygen. Flow oscillations were observed and the onset of these oscillations at supercritical pressures was correlated with wall-to-bulk temperature ratio and velocity. The critical heat flux measured at subcritical pressure was correlated with the product of velocity and subcooling. Long duration tests at fixed heat flux conditions were conducted to evaluate coking on the coolant side tube wall and coking rates comparable to RP-1 were observed.

  18. The two-dimensional Stefan problem with slightly varying heat flux

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

    Gammon, J.; Howarth, J.A.

    1995-09-01

    The authors solve the two-dimensional stefan problem of solidification in a half-space, where the heat flux at the wall is a slightly varying function of positioning along the wall, by means of a large Stefan number approximation (which turns out to be equivalent to a small time solution), and then by means of the Heat Balance Integral Method, which is valid for all time, and which agrees with the large Stefan number solution for small times. A representative solution is given for a particular form of the heat flux perturbation.

  19. CFD modelling wall heat transfer inside a combustion chamber using ANSYS forte

    NASA Astrophysics Data System (ADS)

    Plengsa-ard, C.; Kaewbumrung, M.

    2018-01-01

    A computational model has been performed to analyze a wall heat transfer in a single cylinder, direct injection and four-stroke diesel engine. A direct integration using detailed chemistry CHEMKIN is employed in a combustion model and the Reynolds Averaged Navier Stokes (RANS) turbulence model is used to simulate the flow in the cylinder. To obtain heat flux results, a modified classical variable-density wall heat transfer model is also performed. The model is validated using experimental data from a CUMMINs engine operated with a conventional diesel combustion. One operating engine condition is simulated. Comparisons of simulated in-cylinder pressure and heat release rates with experimental data shows that the model predicts the cylinder pressure and heat release rates reasonably well. The contour plot of instantaneous temperature are presented. Also, the contours of predicted heat flux results are shown. The magnitude of peak heat fluxes as predicted by the wall heat transfer model is in the range of the typical measure values in diesel combustion.

  20. Heat transfer experiments with a central receiver tube subjected to unsteady and non-uniform heat flux

    NASA Astrophysics Data System (ADS)

    Fernández-Torrijos, María; Marugán-Cruz, Carolina; Sobrino, Celia; Santana, Domingo

    2017-06-01

    In this work, a molten salt test loop to study the heat transfer process in external molten salt receivers is described. The experimental installation is formed by a cylindrical molten salt tank, a pump, a flow meter, and an induction heater to generate the heat flux, which is applied in a small rectangular region of the tube surface. In central tower plants, the external receiver pipe is considered to be under unilateral concentrated solar radiation, because only one side of the pipe receives high heat flux. The main advantage of using an induction heater is the control of heating in different areas of the tube. In order to measure the effects of a non-homogenous and unsteady heat flux on the wall temperature distribution a series of experiments have been carried out. 4 K-type thermocouples have been welded at different axial and azimuthal positions of the pipe to obtain the wall temperature distribution. Different temperature measurements have been made varying the heat flux and water velocity to study their effects on the heat transfer process.

  1. Forced Convection Boiling and Critical Heat Flux of Ethanol in Electrically Heated Tube Tests

    NASA Technical Reports Server (NTRS)

    Meyer, Michael L.; Linne, Diane L.; Rousar, Donald C.

    1998-01-01

    Electrically heated tube tests were conducted to characterize the critical heat flux (transition from nucleate to film boiling) of subcritical ethanol flowing at conditions relevant to the design of a regeneratively cooled rocket engine thrust chamber. The coolant was SDA-3C alcohol (95% ethyl alcohol, 5% isopropyl alcohol by weight), and tests were conducted over the following ranges of conditions: pressure from 144 to 703 psia, flow velocities from 9.7 to 77 ft/s, coolant subcooling from 33 to 362 F, and critical heat fluxes up to 8.7 BTU/in(exp 2)/sec. For the data taken near 200 psia, critical heat flux was correlated as a function of the product of velocity and fluid subcooling to within +/- 20%. For data taken at higher pressures, an additional pressure term is needed to correlate the critical heat flux. It was also shown that at the higher test pressures and/or flow rates, exceeding the critical heat flux did not result in wall burnout. This result may significantly increase the engine heat flux design envelope for higher pressure conditions.

  2. Corrections of Heat Flux Measurements on Launch Vehicles

    NASA Technical Reports Server (NTRS)

    Reinarts, Thomas R.; Matson, Monique L.; Walls, Laurie K.

    2002-01-01

    Knowledge of aerothermally induced convective heat transfer is important in the design of thermal protection systems for launch vehicles. Aerothermal models are typically calibrated via the data from circular, in-flight, flush-mounted surface heat flux gauges exposed to the thermal and velocity boundary layers of the external flow. Typically, copper or aluminum Schmidt- Boelter gauges, which take advantage of the one-dimensional Fourier's law of heat conduction, are used to measure the incident heat flux. This instrumentation, when surrounded by low-conductivity insulation, has a wall temperature significantly lower than the insulation. As a result of this substantial disturbance to the thermal boundary layer, the heat flux incident on the gauge tends to be considerably higher than it would have been on the insulation had the calorimeter not been there. In addition, radial conductive heat transfer from the hotter insulation can cause the calorimeter to indicate heat fluxes higher than actual. An overview of an effort to develop and calibrate gauge correction techniques for both of these effects will be presented.

  3. Calculation of heat flux through a wall containing a cavity: Comparison of several models

    NASA Astrophysics Data System (ADS)

    Park, J. E.; Kirkpatrick, J. R.; Tunstall, J. N.; Childs, K. W.

    1986-02-01

    This paper describes the calculation of the heat transfer through the standard stud wall structure of a residential building. The wall cavity contains no insulation. Results from five test cases are presented. The first four represent progressively more complicated approximations to the heat transfer through and within a hollow wall structure. The fifth adds the model components necessary to severely inhibit the radiative energy transport across the empty cavity. Flow within the wall cavity is calculated from the Navier-Stokes equations and the energy conservation equation for an ideal gas using an improvement to the Implicit-Compressible Eulerian (ICE) algorithm of Harlow and Amsden. An algorithm is described to efficiently couple the fluid flow calculations to the radiation-conduction model for the solid portions of the system. Results indicate that conduction through still plates contributes less than 2% of the total heat transferred through a composite wall. All of the other elements (conduction through wall board, sheathing, and siding; convection from siding and wallboard to am bients; and radiation across the wall cavity) are required to accurately predict the heat transfer through a wall. Addition of a foil liner on one inner surface of the wall cavity reduces the total heat transferred by almost 50%.

  4. Turbulent heat flux measurements in a transitional boundary layer

    NASA Technical Reports Server (NTRS)

    Sohn, K. H.; Zaman, K. B. M. Q.; Reshotko, E.

    1992-01-01

    During an experimental investigation of the transitional boundary layer over a heated flat plate, an unexpected result was encountered for the turbulent heat flux (bar-v't'). This quantity, representing the correlation between the fluctuating normal velocity and the temperature, was measured to be negative near the wall under certain conditions. The result was unexpected as it implied a counter-gradient heat transfer by the turbulent fluctuations. Possible reasons for this anomalous result were further investigated. The possible causes considered for this negative bar-v't' were: (1) plausible measurement error and peculiarity of the flow facility, (2) large probe size effect, (3) 'streaky structure' in the near wall boundary layer, and (4) contributions from other terms usually assumed negligible in the energy equation including the Reynolds heat flux in the streamwise direction (bar-u't'). Even though the energy balance has remained inconclusive, none of the items (1) to (3) appear to be contributing directly to the anomaly.

  5. Experimental study on bubble dynamics and wall heat transfer arising from a single nucleation site at subcooled flow boiling conditions – Part 2: Data analysis on sliding bubble characteristics and associated wall heat transfer

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

    Yooa, Junsoo; Estrada-Perez, Carlos E.; Hassan, Yassin A.

    In this second of two companion papers presents an analysis of sliding bubble and wall heat transfer parameters measured during subcooled boiling in a square, vertical, upward flow channel. Bubbles were generated only from a single nucleation site for better observation of both the sliding bubbles’ characteristics and their impact on wall heat transfer through optical measurement techniques. Specific interests include: (i) bubbles departure and subsequent growth while sliding, (ii) bubbles release frequency, (iii) coalescence of sliding bubbles, (iv) sliding bubbles velocity, (v) bubbles size distribution and (vi) wall heat transfer influenced by sliding bubbles. Our results showed that slidingmore » bubbles involve two distinct growth behaviors: (i) at low mass fluxes, sliding bubbles grew fast near the nucleation site, subsequently shrank, and then grew again, (ii) as mass flux increased, however, sliding bubbles grew more steadily. The bubbles originating from the single nucleation site coalesced frequently while sliding, which showed close relation with bubbles release frequency. The sliding bubble velocity near the nucleation site consistently decreased by increasing mass flux, while the observation often became reversed as the bubbles slid downstream due to the effect of interfacial drag. The sliding bubbles moved faster than the local liquid (i.e., ur<0) at low mass flux conditions, but it became reversed as the mass flux increased. The size distribution of sliding bubbles followed Gaussian distribution well both near and far from the nucleation site. The standard deviation of bubble size varied insignificantly through sliding compared to the changes in mean bubble size. Lastly, the sliding bubbles enhanced the wall heat transfer and the effect became more noticeable as inlet subcooling/mass flux decreased or wall heat flux increased. Particularly, the sliding bubble characteristics such as bubble growth behavior observed near the nucleation site played

  6. Experimental study on bubble dynamics and wall heat transfer arising from a single nucleation site at subcooled flow boiling conditions – Part 2: Data analysis on sliding bubble characteristics and associated wall heat transfer

    DOE PAGES

    Yooa, Junsoo; Estrada-Perez, Carlos E.; Hassan, Yassin A.

    2016-04-28

    In this second of two companion papers presents an analysis of sliding bubble and wall heat transfer parameters measured during subcooled boiling in a square, vertical, upward flow channel. Bubbles were generated only from a single nucleation site for better observation of both the sliding bubbles’ characteristics and their impact on wall heat transfer through optical measurement techniques. Specific interests include: (i) bubbles departure and subsequent growth while sliding, (ii) bubbles release frequency, (iii) coalescence of sliding bubbles, (iv) sliding bubbles velocity, (v) bubbles size distribution and (vi) wall heat transfer influenced by sliding bubbles. Our results showed that slidingmore » bubbles involve two distinct growth behaviors: (i) at low mass fluxes, sliding bubbles grew fast near the nucleation site, subsequently shrank, and then grew again, (ii) as mass flux increased, however, sliding bubbles grew more steadily. The bubbles originating from the single nucleation site coalesced frequently while sliding, which showed close relation with bubbles release frequency. The sliding bubble velocity near the nucleation site consistently decreased by increasing mass flux, while the observation often became reversed as the bubbles slid downstream due to the effect of interfacial drag. The sliding bubbles moved faster than the local liquid (i.e., ur<0) at low mass flux conditions, but it became reversed as the mass flux increased. The size distribution of sliding bubbles followed Gaussian distribution well both near and far from the nucleation site. The standard deviation of bubble size varied insignificantly through sliding compared to the changes in mean bubble size. Lastly, the sliding bubbles enhanced the wall heat transfer and the effect became more noticeable as inlet subcooling/mass flux decreased or wall heat flux increased. Particularly, the sliding bubble characteristics such as bubble growth behavior observed near the nucleation site played

  7. The study of heat flux for disruption on experimental advanced superconducting tokamak

    NASA Astrophysics Data System (ADS)

    Yang, Zhendong; Fang, Jianan; Gong, Xianzu; Gan, Kaifu; Luo, Jiarong; Zhao, Hailin; Cui, Zhixue; Zhang, Bin; Chen, Meiwen

    2016-05-01

    Disruption of the plasma is one of the most dangerous instabilities in tokamak. During the disruption, most of the plasma thermal energy is lost, which causes damages to the plasma facing components. Infrared (IR) camera is an effective tool to detect the temperature distribution on the first wall, and the energy deposited on the first wall can be calculated from the surface temperature profile measured by the IR camera. This paper concentrates on the characteristics of heat flux distribution onto the first wall under different disruptions, including the minor disruption and the vertical displacement events (VDE) disruption. Several minor disruptions have been observed before the major disruption under the high plasma density in experimental advanced superconducting tokamak. During the minor disruption, the heat fluxes are mainly deposited on the upper/lower divertors. The magnetic configuration prior to the minor disruption is a lower single null with the radial distance between the two separatrices in the outer midplane dRsep = -2 cm, while it changes to upper single null (dRsep = 1.4 cm) during the minor disruption. As for the VDE disruption, the spatial distribution of heat flux exhibits strong toroidal and radial nonuniformity, and the maximum heat flux received on the dome plate can be up to 11 MW/m2.

  8. Periodic unsteady effects on turbulent boundary layer transport and heat transfer: An experimental investigation in a cylinder-wall junction flow

    NASA Astrophysics Data System (ADS)

    Xie, Qi

    Heat transfer in a turbulent boundary layer downstream of junction with a cylinder has many engineering applications including controlling heat transfer to the endwall in gas turbine passages and cooling of protruding electronic chips. The main objective of this research is to study the fundamental process of heat transport and wall heat transfer in a turbulent three-dimensional flow superimposed with local large-scale periodic unsteadiness generated by vortex shedding from the cylinder. Direct measurements of the Reynolds heat fluxes (/line{utheta},\\ /line{vtheta}\\ and\\ /line{wtheta}) and time-resolved wall heat transfer rate will provide insight into unsteady flow behavior and data for advanced turbulence models for numerical simulation of complex engineering flows. Experiments were conducted in an open-circuit, low-speed wind tunnel. Reynolds stresses and heat fluxes were obtained from turbulent heat-flux probes which consisted of two hot wires, arranged in an X-wire configuration, and a cold wire located in front of the X-wire. Thin-film surface heat flux sensors were designed for measuring time-resolved wall heat flux. A reference probe and conditional-sampling technique connected the flow field dynamics to wall heat transfer. An event detecting and ensemble-averaging method was developed to separate effects of unsteadiness from those of background turbulence. Results indicate that unsteadiness affects both heat transport and wall heat transfer. The flow behind the cylinder can be characterized by three regions: (1) Wake region, where unsteadiness is observed to have modest effect; (2) Unsteady region, where the strongest unsteadiness effect is found; (3) Outer region, where the flow approaches the two-dimensional boundary-layer behavior. Vortex shedding from both sides of the cylinder contributes to mixing enhancement in the wake region. Unsteadiness contributes up to 51% of vertical and 59% of spanwise turbulent heat fluxes in the unsteady region. The

  9. The study of heat flux for disruption on experimental advanced superconducting tokamak

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

    Yang, Zhendong, E-mail: dongyz@ipp.ac.cn, E-mail: jafang@dhu.edu.cn; Institute of Plasma Physics, Chinese Academy of Sciences, Hefei 230031; Fang, Jianan, E-mail: dongyz@ipp.ac.cn, E-mail: jafang@dhu.edu.cn

    Disruption of the plasma is one of the most dangerous instabilities in tokamak. During the disruption, most of the plasma thermal energy is lost, which causes damages to the plasma facing components. Infrared (IR) camera is an effective tool to detect the temperature distribution on the first wall, and the energy deposited on the first wall can be calculated from the surface temperature profile measured by the IR camera. This paper concentrates on the characteristics of heat flux distribution onto the first wall under different disruptions, including the minor disruption and the vertical displacement events (VDE) disruption. Several minor disruptionsmore » have been observed before the major disruption under the high plasma density in experimental advanced superconducting tokamak. During the minor disruption, the heat fluxes are mainly deposited on the upper/lower divertors. The magnetic configuration prior to the minor disruption is a lower single null with the radial distance between the two separatrices in the outer midplane dR{sub sep} = −2 cm, while it changes to upper single null (dR{sub sep} = 1.4 cm) during the minor disruption. As for the VDE disruption, the spatial distribution of heat flux exhibits strong toroidal and radial nonuniformity, and the maximum heat flux received on the dome plate can be up to 11 MW/m{sup 2}.« less

  10. Unsteady Heat Transfer Behavior of Reinforced Concrete Wall of Cold Storage

    NASA Astrophysics Data System (ADS)

    Nomura, Tomohiro; Murakami, Yuji; Uchikawa, Motoyuki

    The authors had already clarified that the heat transfer behaviors between internal and external insulated reinforced concrete wall of cold storage are different each others when inside and outside temperature of wall is flactuating. From that conclusion, we must consider the application method of wall insulation of cold storages in actual design. The theme of the paper is to get the analyzing method and unsteady heat transfer characteristics of concrete walls of cold storage during daily variation of outside temperature of walls, and to give the basis for efficient design and cost optimization of insulate wall of cold storage. The difference of unsteady heat transfer characteristics between internal and external insulate wall, when outside temperature of the wall follewed daily varation, was clarified in experiment and in situ measurement of practical cold storage. The analyzing method with two dimentional unsteady FEM was introduced. Using this method, it is possible to obtain the time variation of heat flux, which is important basic factor for practical design of cold storage, through the wall.

  11. Explosive Boiling at Very Low Heat Fluxes: A Microgravity Phenomenon

    NASA Technical Reports Server (NTRS)

    Hasan, M. M.; Lin, C. S.; Knoll, R. H.; Bentz, M. D.

    1993-01-01

    The paper presents experimental observations of explosive boiling from a large (relative to bubble sizes) flat heating surface at very low heat fluxes in microgravity. The explosive boiling is characterized as either a rapid growth of vapor mass over the entire heating surface due to the flashing of superheated liquid or a violent boiling spread following the appearance of single bubbles on the heating surface. Pool boiling data with saturated Freon 113 was obtained in the microgravity environment of the space shuttle. The unique features of the experimental results are the sustainability of high liquid superheat for long periods and the occurrence of explosive boiling at low heat fluxes (0.2 to 1.2 kW/sq m). For a heat flux of 1.0 kW/sq m a wall superheat of 17.9 degrees C was attained in ten minutes of heating. This was followed by an explosive boiling accompanied with a pressure spike and a violent bulk liquid motion. However, at this heat flux the vapor blanketing the heating surface could not be sustained. Stable nucleate boiling continued following the explosive boiling.

  12. Enhanced heat sink with geometry induced wall-jet

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

    Hossain, Md. Mahamudul, E-mail: sohel0991@gmail.com; Tikadar, Amitav; Bari, Fazlul

    Mini-channels embedded in solid matrix have already proven to be a very efficient way of electronic cooling. Traditional mini-channel heat sinks consist of single layer of parallel channels. Although mini-channel heat sink can achieve very high heat flux, its pumping requirement for circulating liquid through the channel increase very sharply as the flow velocity increases. The pumping requirements of the heat sink can be reduced by increasing its performance. In this paper a novel approach to increase the thermal performance of the mini-channel heat sink is proposed through geometry induced wall jet which is a passive technique. Geometric irregularities alongmore » the channel length causes abrupt pressure change between the channels which causes cross flow through the interconnections thus one channel faces suction and other channel jet action. This suction and jet action disrupts boundary layer causing enhanced heat transfer performance. A CFD model has been developed using commercially available software package FLUENT to evaluate the technique. A parametric study of the velocities and the effect of the position of the wall-jets have been performed. Significant reduction in thermal resistance has been observed for wall-jets, it is also observed that this reduction in thermal resistance is dependent on the position and shape of the wall jet.« less

  13. Expanding Taylor bubble under constant heat flux

    NASA Astrophysics Data System (ADS)

    Voirand, Antoine; Benselama, Adel M.; Ayel, Vincent; Bertin, Yves

    2016-09-01

    Modelization of non-isothermal bubbles expanding in a capillary, as a contribution to the understanding of the physical phenomena taking place in Pulsating Heat Pipes (PHPs), is the scope of this paper. The liquid film problem is simplified and solved, while the thermal problem takes into account a constant heat flux density applied at the capillary tube wall, exchanging with the liquid film surrounding the bubble and also with the capillary tube outside medium. The liquid slug dynamics is solved using the Lucas-Washburn equation. Mass and energy balance on the vapor phase allow governing equations of bubble expansion to be written. The liquid and vapor phases are coupled only through the saturation temperature associated with the vapor pressure, assumed to be uniform throughout the bubble. Results show an over-heating of the vapor phase, although the particular thermal boundary condition used here always ensures an evaporative mass flux at the liquid-vapor interface. Global heat exchange is also investigated, showing a strong decreasing of the PHP performance to convey heat by phase change means for large meniscus velocities.

  14. Single-side conduction modeling for high heat flux coolant channels

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

    Boyd, R.D. Sr.

    In the development of plasma-facing components (PFCs), most investigators have erroneously postulated negligible water critical heat flux dependence on the coolant channel length-to-diameter (L/D) ratio above a constant value of L/D. Although encouraging results have been obtained in characterizing peaking factors for local two-dimensional boiling curves and critical heat flux, additional experimental data and theoretical model development are needed to validate the applicability to PFCs. Both these and related issues will affect the flow boiling correlation and data reduction associated with the development of PFCs for fusion reactors and other physical problems that are dependent on conduction modeling in themore » heat flux spectrum of applications. Both exact solutions and numerical conjugate analyses are presented for a one-side heated (OSH) geometry. The results show (a) the coexistence of three flow regimes inside an OSH circular geometry, (b) the correlational dependence of the inside wall heat flux and temperature, and (c) inaccuracies that could arise in some data reduction procedures.« less

  15. Latent Heat in Soil Heat Flux Measurements

    USDA-ARS?s Scientific Manuscript database

    The surface energy balance includes a term for soil heat flux. Soil heat flux is difficult to measure because it includes conduction and convection heat transfer processes. Accurate representation of soil heat flux is an important consideration in many modeling and measurement applications. Yet, the...

  16. Wall Area of Influence and Growing Wall Heat Transfer due to Sliding Bubbles in Subcooled Boiling Flow

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

    Yoo, Junsoo; Estrada-Perez, Carlos E.; Hassan, Yassin A.

    A variety of dynamical features of sliding bubbles and their impact on wall heat transfer were observed at subcooled flow boiling conditions in a vertical square test channel. Among the wide range of parameters observed, we particularly focus in this paper on (i) the sliding bubbles’ effect on wall heat transfer (supplemantry discussion to the authors’ previous work in Yoo et al. (2016a,b)) and (ii) the wall area influenced by sliding bubbles in subcooled boiling flow. At first, this study reveals that the degree of wall heat transfer improvement due to sliding bubbles depended less on the wall superheat conditionmore » as the mass flux increased. Also, the sliding bubble trajectory was found to be one of the critical factors in order to properly describe the wall heat transfer associated with sliding bubbles. In particular, the wall area influenced by sliding bubbles depended strongly on both sliding bubble trajectory and sliding bubble size; the sliding bubble trajectory was also observed to be closely related to the sliding bubble size. Importantly, these results indicate the limitation of current approach in CFD analyses especially for the wall area of bubble influence. In addition, the analyses on the temporal fraction of bubbles’ residence (FR) along the heated wall show that the sliding bubbles typically travel through narrow path with high frequency while the opposite was observed downstream. That is, both FR and sliding bubble trajectory depended substantially on the distance from nucleation site, which is expected to be similar for the quenching heat transfer mode induced by sliding bubbles.« less

  17. Investigation of Instabilities and Heat Transfer Phenomena in Supercritical Fuels at High Heat Flux and Temperatures

    NASA Technical Reports Server (NTRS)

    Linne, Diane L.; Meyer, Michael L.; Braun, Donald C.; Keller, Dennis J.

    2000-01-01

    A series of heated tube experiments was performed to investigate fluid instabilities that occur during heating of supercritical fluids. In these tests, JP-7 flowed vertically through small diameter tubes at supercritical pressures. Test section heated length, diameter, mass flow rate, inlet temperature, and heat flux were varied in an effort to determine the range of conditions that trigger the instabilities. Heat flux was varied up to 4 BTU/sq in./s, and test section wall temperatures reached as high as 1950 F. A statistical model was generated to explain the trends and effects of the control variables. The model included no direct linear effect of heat flux on the occurrence of the instabilities. All terms involving inlet temperature were negative, and all terms involving mass flow rate were positive. Multiple tests at conditions that produced instabilities provided inconsistent results. These inconsistencies limit the use of the model as a predictive tool. Physical variables that had been previously postulated to control the onset of the instabilities, such as film temperature, velocity, buoyancy, and wall-to-bulk temperature ratio, were evaluated here. Film temperatures at or near critical occurred during both stable and unstable tests. All tests at the highest velocity were stable, but there was no functional relationship found between the instabilities and velocity, or a combination of velocity and temperature ratio. Finally, all of the unstable tests had significant buoyancy at the inlet of the test section, but many stable tests also had significant buoyancy forces.

  18. Automated Heat-Flux-Calibration Facility

    NASA Technical Reports Server (NTRS)

    Liebert, Curt H.; Weikle, Donald H.

    1989-01-01

    Computer control speeds operation of equipment and processing of measurements. New heat-flux-calibration facility developed at Lewis Research Center. Used for fast-transient heat-transfer testing, durability testing, and calibration of heat-flux gauges. Calibrations performed at constant or transient heat fluxes ranging from 1 to 6 MW/m2 and at temperatures ranging from 80 K to melting temperatures of most materials. Facility developed because there is need to build and calibrate very-small heat-flux gauges for Space Shuttle main engine (SSME).Includes lamp head attached to side of service module, an argon-gas-recirculation module, reflector, heat exchanger, and high-speed positioning system. This type of automated heat-flux calibration facility installed in industrial plants for onsite calibration of heat-flux gauges measuring fluxes of heat in advanced gas-turbine and rocket engines.

  19. Aerodynamic heating effects on wall-modeled large-eddy simulations of high-speed flows

    NASA Astrophysics Data System (ADS)

    Yang, Xiang; Urzay, Javier; Moin, Parviz

    2017-11-01

    Aerospace vehicles flying at high speeds are subject to increased wall-heating rates because of strong aerodynamic heating in the near-wall region. In wall-modeled large-eddy simulations (WMLES), this near-wall region is typically not resolved by the computational grid. As a result, the effects of aerodynamic heating need to be modeled using an LES wall model. In this investigation, WMLES of transitional and fully turbulent high-speed flows are conducted to address this issue. In particular, an equilibrium wall model is employed in high-speed turbulent Couette flows subject to different combinations of thermal boundary conditions and grid sizes, and in transitional hypersonic boundary layers interacting with incident shock waves. Specifically, the WMLES of the Couette-flow configuration demonstrate that the shear-stress and heat-flux predictions made by the wall model show only a small sensitivity to the grid resolution even in the most adverse case where aerodynamic heating prevails near the wall and generates a sharp temperature peak there. In the WMLES of shock-induced transition in boundary layers, the wall model is tested against DNS and experiments, and it is shown to capture the post-transition aerodynamic heating and the overall heat transfer rate around the shock-impingement zone. This work is supported by AFOSR.

  20. Small hydrogen/oxygen rocket flowfield behavior from heat flux measurements

    NASA Technical Reports Server (NTRS)

    Reed, Brian D.

    1993-01-01

    The mixing and heat transfer phenomena in small rocket flow fields with fuel film cooling is not well understood. An instrumented, water-cooled chamber with a gaseous hydrogen/gaseous oxygen injector was used to gather steady-state inner and outer wall temperature profiles. The chamber was tested at 414 kPa (60 psia) chamber pressure, from mixture ratios of 3.41 to 8.36. Sixty percent of the fuel was used for film cooling. These temperature profiles were used as boundary conditions in a finite element analysis program, MSC/NASTRAN, to calculate the local radial and axial heat fluxes in the chamber wall. The normal heat fluxes were then calculated and used as a diagnostic of the rocket's flow field behavior. The normal heat fluxes determined were on the order of 1.0 to 3.0 MW/meters squared (0.6 to 1.8 Btu/sec-inches squared). In the cases where mixture ratio was 5 or above, there was a sharp local heat flux maximum in the barrel section of the chamber. This local maximum seems to indicate a reduction or breakdown of the fuel film cooling layer, possibly due to increased mixing in the shear layer between the film and core flows. However, the flow was thought to be completely laminar, as the throat Reynolds numbers were below 50,000 for all the cases. The increased mixing in the shear layer in the higher mixture ratio cases appeared not to be due to the transition of the flow from laminar to turbulent, but rather due to increased reactions between the hydrogen film and oxidizer-rich core flows.

  1. Solid motor aft closure insulation erosion. [heat flux correlation for rate analysis

    NASA Technical Reports Server (NTRS)

    Stampfl, E.; Landsbaum, E. M.

    1973-01-01

    The erosion rate of aft closure insulation in a number of large solid propellant motors was empirically analyzed by correlating the average ablation rate with a number of variables that had previously been demonstrated to affect heat flux. The main correlating parameter was a heat flux based on the simplified Bartz heat transfer coefficient corrected for two-dimensional effects. A multiplying group contained terms related to port-to-throat ratio, local wall angle, grain geometry and nozzle cant angle. The resulting equation gave a good correlation and is a useful design tool.

  2. Simulation of one-sided heating of boiler unit membrane-type water walls

    NASA Astrophysics Data System (ADS)

    Kurepin, M. P.; Serbinovskiy, M. Yu.

    2017-03-01

    This study describes the results of simulation of the temperature field and the stress-strain state of membrane-type gastight water walls of boiler units using the finite element method. The methods of analytical and standard calculation of one-sided heating of fin-tube water walls by a radiative heat flux are analyzed. The methods and software for input data calculation in the finite-element simulation, including thermoelastic moments in welded panels that result from their one-sided heating, are proposed. The method and software modules are used for water wall simulation using ANSYS. The results of simulation of the temperature field, stress field, deformations and displacement of the membrane-type panel for the boiler furnace water wall using the finite-element method, as well as the results of calculation of the panel tube temperature, stresses and deformations using the known methods, are presented. The comparison of the known experimental results on heating and bending by given moments of membrane-type water walls and numerical simulations is performed. It is demonstrated that numerical results agree with high accuracy with the experimental data. The relative temperature difference does not exceed 1%. The relative difference of the experimental fin mutual turning angle caused by one-sided heating by radiative heat flux and the results obtained in the finite element simulation does not exceed 8.5% for nondisplaced fins and 7% for fins with displacement. The same difference for the theoretical results and the simulation using the finite-element method does not exceed 3% and 7.1%, respectively. The proposed method and software modules for simulation of the temperature field and stress-strain state of the water walls are verified and the feasibility of their application in practical design is proven.

  3. Heat Flux Sensor

    NASA Technical Reports Server (NTRS)

    1994-01-01

    A heat flux microsensor developed under a NASP Small Business Innovation Research (SBIR) has a wide range of potential commercial applications. Vatell Corporation originally designed microsensors for use in very high temperatures. The company then used the technology to develop heat flux sensors to measure the rate of heat energy flowing in and out of a surface as well as readings on the surface temperature. Additional major advantages include response to heat flux in less than 10 microseconds and the ability to withstand temperatures up to 1,200 degrees centigrade. Commercial applications are used in high speed aerodynamics, supersonic combustion, blade cooling, and mass flow measurements, etc.

  4. Latent heat sink in soil heat flux measurements

    USDA-ARS?s Scientific Manuscript database

    The surface energy balance includes a term for soil heat flux. Soil heat flux is difficult to measure because it includes conduction and convection heat transfer processes. Accurate representation of soil heat flux is an important consideration in many modeling and measurement applications. Yet, the...

  5. Two-Dimensional Thermal Boundary Layer Corrections for Convective Heat Flux Gauges

    NASA Technical Reports Server (NTRS)

    Kandula, Max; Haddad, George

    2007-01-01

    This work presents a CFD (Computational Fluid Dynamics) study of two-dimensional thermal boundary layer correction factors for convective heat flux gauges mounted in flat plate subjected to a surface temperature discontinuity with variable properties taken into account. A two-equation k - omega turbulence model is considered. Results are obtained for a wide range of Mach numbers (1 to 5), gauge radius ratio, and wall temperature discontinuity. Comparisons are made for correction factors with constant properties and variable properties. It is shown that the variable-property effects on the heat flux correction factors become significant

  6. Mass ablation and magnetic flux losses through a magnetized plasma-liner wall interface

    NASA Astrophysics Data System (ADS)

    García-Rubio, F.; Sanz, J.

    2017-07-01

    The understanding of energy and magnetic flux losses in a magnetized plasma medium confined by a cold wall is of great interest in the success of magnetized liner inertial fusion (MagLIF). In a MagLIF scheme, the fuel is magnetized and subsonically compressed by a cylindrical liner. Magnetic flux conservation is degraded by the presence of gradient-driven transport processes such as thermoelectric effects (Nernst) and magnetic field diffusion. In previous publications [Velikovich et al., Phys. Plasmas 22, 042702 (2015)], the evolution of a hot magnetized plasma in contact with a cold solid wall (liner) was studied using the classical collisional Braginskii's plasma transport equations in one dimension. The Nernst term degraded the magnetic flux conservation, while both thermal energy and magnetic flux losses were reduced with the electron Hall parameter ωeτe with a power-law asymptotic scaling (ωeτe)-1/2. In the analysis made in the present paper, we consider a similar situation, but with the liner being treated differently. Instead of a cold solid wall acting as a heat sink, we model the liner as a cold dense plasma with low thermal conduction (that could represent the cryogenic fuel layer added on the inner surface of the liner in a high-gain MagLIF configuration). Mass ablation comes into play, which adds notably differences to the previous analysis. The direction of the plasma motion is inverted, but the Nernst term still convects the magnetic field towards the liner. Magnetization suppresses the Nernst velocity and improves the magnetic flux conservation. Thermal energy in the hot plasma is lost in heating the ablated material. When the electron Hall parameter is large, mass ablation scales as (ωeτe)-3/10, while both the energy and magnetic flux losses are reduced with a power-law asymptotic scaling (ωeτe)-7/10.

  7. Maximum Expected Wall Heat Flux and Maximum Pressure After Sudden Loss of Vacuum Insulation on the Stratospheric Observatory for Infrared Astronomy (SOFIA) Liquid Helium (LHe) Dewars

    NASA Technical Reports Server (NTRS)

    Ungar, Eugene K.

    2014-01-01

    The aircraft-based Stratospheric Observatory for Infrared Astronomy (SOFIA) is a platform for multiple infrared observation experiments. The experiments carry sensors cooled to liquid helium (LHe) temperatures. A question arose regarding the heat input and peak pressure that would result from a sudden loss of the dewar vacuum insulation. Owing to concerns about the adequacy of dewar pressure relief in the event of a sudden loss of the dewar vacuum insulation, the SOFIA Program engaged the NASA Engineering and Safety Center (NESC). This report summarizes and assesses the experiments that have been performed to measure the heat flux into LHe dewars following a sudden vacuum insulation failure, describes the physical limits of heat input to the dewar, and provides an NESC recommendation for the wall heat flux that should be used to assess the sudden loss of vacuum insulation case. This report also assesses the methodology used by the SOFIA Program to predict the maximum pressure that would occur following a loss of vacuum event.

  8. Measurements of plasma sheath heat flux in the Alcator C-Mod divertor

    NASA Astrophysics Data System (ADS)

    Brunner, Dan; Labombard, Brian; Terry, Jim; Reinke, Matt

    2010-11-01

    Heat flux is one of the most important parameters controlling the lifetime of first-wall components in fusion experiments and reactors. The sheath heat flux coefficient (γ) is a parameter relating heat flux (from a plasma to a material surface) to the electron temperature and ion saturation current. Being such a simple expression for a kinetic process, it is of great interest to plasma edge fluid modelers. Under the assumptions of equal ion and electron temperatures, no secondary electron emission, and no net current to the surface the value of γ is approximately 7 [1]. Alcator C-Mod provides a unique opportunity among today's experiments to measure reactor-relevant heat fluxes (100's of MW/m^2 parallel to the magnetic field) in reactor-like divertor geometry. Motivated by the DoE 2010 joint milestone to measure heat flux footprints, the lower outer divertor of Alcator has been instrumented with a suite of Langmuir probes, novel surface thermocouples, and calorimeters in tiles purposefully ramped to eliminate shadowing; all within view of an IR camera. Initial results indicate that the experimentally inferred values of γ are found to agree with simple theory in the sheath limited regime and diverges to lower values as the density increases.

  9. Fundamentals of heat measurement. [heat flux transducers

    NASA Technical Reports Server (NTRS)

    Gerashchenko, O. A.

    1979-01-01

    Various methods and devices for obtaining experimental data on heat flux density over wide ranges of temperature and pressure are examined. Laboratory tests and device fabrication details are supplemented by theoretical analyses of heat-conduction and thermoelectric effects, providing design guidelines and information relevant to further research and development. A theory defining the measure of correspondence between transducer signal and the measured heat flux is established for individual (isolated) heat flux transducers subject to space and time-dependent loading. An analysis of the properties of stacked (series-connected) transducers of various types (sandwich-type, plane, and spiral) is used to derive a similarity theory providing general governing relationships. The transducers examined are used in 36 types of derivative devices involving direct heat loss measurements, heat conduction studies, radiation pyrometry, calorimetry in medicine and industry and nuclear reactor dosimetry.

  10. High heat flux loop heat pipes

    NASA Astrophysics Data System (ADS)

    North, Mark T.; Sarraf, David B.; Rosenfeld, John H.; Maidanik, Yuri F.; Vershinin, Sergey

    1997-01-01

    Loop Heat Pipes (LHPs) can transport very large thermal power loads, over long distances, through flexible, small diameter tubes and against high gravitational heads. While recent LHPs have transported as much as 1500 W, the peak heat flux through a LHP's evaporator has been limited to about 0.07 MW/m2. This limitation is due to the arrangement of vapor passages next to the heat load which is one of the conditions necessary to ensure self priming of the device. This paper describes work aimed at raising this limit by threefold to tenfold. Two approaches were pursued. One optimized the vapor passage geometry for the high heat flux conditions. The geometry improved the heat flow into the wick and working fluid. This approach also employed a finer pored wick to support higher vapor flow losses. The second approach used a bidisperse wick material within the circumferential vapor passages. The bidisperse material increased the thermal conductivity and the evaporative surface area in the region of highest heat flux, while providing a flow path for the vapor. Proof-of-concept devices were fabricated and tested for each approach. Both devices operated as designed and both demonstrated operation at a heat flux of 0.70 MW/m2. This performance exceeded the known state of the art by a factor of more than six for both conventional heat pipes and for loop heat pipes using ammonia. In addition, the bidisperse-wick device demonstrated boiling heat transfer coefficients up to 100,000 W/m2.K, and the fine pored device demonstrated an orientation independence with its performance essentially unaffected by whether its evaporator was positioned above, below or level with the condenser.

  11. A low-frequency wave motion mechanism enables efficient energy transport in carbon nanotubes at high heat fluxes.

    PubMed

    Zhang, Xiaoliang; Hu, Ming; Poulikakos, Dimos

    2012-07-11

    The great majority of investigations of thermal transport in carbon nanotubes (CNTs) in the open literature focus on low heat fluxes, that is, in the regime of validity of the Fourier heat conduction law. In this paper, by performing nonequilibrium molecular dynamics simulations we investigated thermal transport in a single-walled CNT bridging two Si slabs under constant high heat flux. An anomalous wave-like kinetic energy profile was observed, and a previously unexplored, wave-dominated energy transport mechanism is identified for high heat fluxes in CNTs, originated from excited low frequency transverse acoustic waves. The transported energy, in terms of a one-dimensional low frequency mechanical wave, is quantified as a function of the total heat flux applied and is compared to the energy transported by traditional Fourier heat conduction. The results show that the low frequency wave actually overtakes traditional Fourier heat conduction and efficiently transports the energy at high heat flux. Our findings reveal an important new mechanism for high heat flux energy transport in low-dimensional nanostructures, such as one-dimensional (1-D) nanotubes and nanowires, which could be very relevant to high heat flux dissipation such as in micro/nanoelectronics applications.

  12. Sensors for Metering Heat Flux Area Density and Metrological Equipment for the Heat Flux Density Measurement

    NASA Astrophysics Data System (ADS)

    Doronin, D. O.

    2018-04-01

    The demand in measuring and studies of heat conduction of various media is very urgent now. This article considers the problem of heat conduction monitoring and measurement in various media and materials in any industries and branches of science as well as metrological support of the heat flux measurement equipment. The main study objects are both the sensors manufactured and facilities onto which these sensors will be installed: different cladding structures of the buildings, awnings, rocket fairings, boiler units, internal combustion engines. The Company develops and manufactures different types of heat flux sensors: thermocouple, thin-film, heterogeneous gradient as well as metrological equipment for the gauging calibration of the heat flux density measurement. The calibration shall be performed using both referencing method in the unit and by fixed setting of the heat flux in the unit. To manufacture heterogeneous heat flux gradient sensors (HHFGS) the Company developed and designed a number of units: diffusion welding unit, HHFGS cutting unit. Rather good quality HHFGS prototypes were obtained. At this stage the factory tests on the equipment for the heat flux density measurement equipment are planned. A high-sensitivity heat flux sensor was produced, now it is tested at the Construction Physics Research Institute (Moscow). It became possible to create thin-film heat flux sensors with the sensitivity not worse than that of the sensors manufactured by Captec Company (France). The Company has sufficient premises to supply the market with a wide range of sensors, to master new sensor manufacture technologies which will enable their application range.

  13. Effects of Crack on Heat Flux in Hypersonic Shock/Boundary-Layer Interaction

    NASA Astrophysics Data System (ADS)

    Ozawa, Hiroshi; Hanai, Katsuhisa; Kitamura, Keiichi; Mori, Koichi; Nakamura, Yoshiaki

    A small crack on body surface led to a tragic accident in 2003, which is the Columbia accident. During the shuttle's re-entry, high temperature gas penetrated crack on leading-edge of the left wing and melted the aluminum structure, finally the Columbia blew up. Since early times, there are many fundamental studies about simple cavity-flow formed on body surface in hypersonic speeds. However, an investigation of Shock/Boundary-Layer Interaction (SBLI) on crack has not been researched. For multistage space transportation vehicle such as TSTO, SBLI is an inevitable problem, and then SBLI on crack becomes a critical issue for TSTO development. In this study, the effects of crack, where SBLI occurs, were investigated for TSTO hypersonic speed (M∞ = 8.1). A square crack locates at SBLI point on the TSTO booster. Results show that a crack and its depth strongly effect on peak heat flux and aerodynamic interaction flow-field. In the cases of shallow crack (d/C ≤ 0.10), there exist two high heat flux regions on crack floor, which locates at a flow reattachment region and a back end wall of crack. In this case, a peak heat flux at flow reattachment region becomes about 2 times as large as the stagnation point heat flux, which value becomes larger compared with a peak heat flux in the case of No-Crack TSTO. While in the case of deep crack (d/C = 0.20), overall heat flux on crack floor decreases to below the stagnation point heat flux. These results provide useful data for a development of TSTO thermal protection system (TPS) such as thermal protection tile.

  14. High heat flux issues for plasma-facing components in fusion reactors

    NASA Astrophysics Data System (ADS)

    Watson, Robert D.

    1993-02-01

    Plasma facing components in tokamak fusion reactors are faced with a number of difficult high heat flux issues. These components include: first wall armor tiles, pumped limiters, diverter plates, rf antennae structure, and diagnostic probes. Peak heat fluxes are 15 - 30 MW/m2 for diverter plates, which will operate for 100 - 1000 seconds in future tokamaks. Disruption heat fluxes can approach 100,000 MW/m2 for 0.1 ms. Diverter plates are water-cooled heat sinks with armor tiles brazed on to the plasma facing side. Heat sink materials include OFHC, GlidcopTM, TZM, Mo-41Re, and niobium alloys. Armor tile materials include: carbon fiber composites, beryllium, silicon carbide, tungsten, and molybdenum. Tile thickness range from 2 - 10 mm, and heat sinks are 1 - 3 mm. A twisted tape insert is used to enhance heat transfer and increase the burnout safety margin from critical heat flux limits to 50 - 60 MW/m2 with water at 10 m/s and 4 MPa. Tests using rastered electron beams have shown thermal fatigue failures from cracks at the brazed interface between tiles and the heat sink after only 1000 cycles at 10 - 15 MW/m2. These fatigue lifetimes need to be increased an order of magnitude to meet future requirements. Other critical issues for plasma facing components include: surface erosion from sputtering and disruption erosion, eddy current forces and runaway electron impact from disruptions, neutron damage, tritium retention and release, remote maintenance of radioactive components, corrosion-erosion, and loss-of-coolant accidents.

  15. Heat Transfer at a Long Electrically-Simulated Water Wall in a Circulating Fluidised Bed

    NASA Astrophysics Data System (ADS)

    Sundaresan, R.; Kolar, Ajit Kumar

    In the present work, heat transfer measurements are reported in a 100mm square, 5.5 m tall, cold CFB. The test section is a 19 mm OD electrically heated heat transfer tube, 4.64 m tall (covering more than 80% of the CFB height), sandwiched between two equally tall dummy tubes of 19mm OD, thus simulating a water wall geometry, forming one wall of the CFB. Narrow cut sand particles of mean diameters 156, 256, and 362 micrometers, and a wide cut sample of mean diameter 265 micrometer were used as the bed material. The superficial gas velocity ranged from 4.2 to 8.2 m/s, and the solids recycle flux varied from 17 to 110 kg/m2s. Local heat transfer coefficient at the simulated water wall varies, as expected from a low value at the top of the riser to a high value at the bottom, with an interesting increasing and decreasing trend in between. The average heat transfer coefficients were compared with those available in open literature. Correlations for average heat transfer coefficient are presented, both in terms of an average suspension density and also in terms of important nondimensional numbers, namely, Froude number, relative solids flux and velocity ratio. Comparisons are also made with predictions of relevant heat transfer models. Based on the present fifty-five experimental data points, the following correlation was presented with a correlation coefficient of 0.862 and maximum error is ± 15 %.

  16. Advanced high temperature heat flux sensors

    NASA Technical Reports Server (NTRS)

    Atkinson, W.; Hobart, H. F.; Strange, R. R.

    1983-01-01

    To fully characterize advanced high temperature heat flux sensors, calibration and testing is required at full engine temperature. This required the development of unique high temperature heat flux test facilities. These facilities were developed, are in place, and are being used for advanced heat flux sensor development.

  17. The Role of the Velocity Gradient in Laminar Convective Heat Transfer through a Tube with a Uniform Wall Heat Flux

    ERIC Educational Resources Information Center

    Wang, Liang-Bi; Zhang, Qiang; Li, Xiao-Xia

    2009-01-01

    This paper aims to contribute to a better understanding of convective heat transfer. For this purpose, the reason why thermal diffusivity should be placed before the Laplacian operator of the heat flux, and the role of the velocity gradient in convective heat transfer are analysed. The background to these analyses is that, when the energy…

  18. Impact of wall hydrophobicity on condensation flow and heat transfer in silicon microchannels

    NASA Astrophysics Data System (ADS)

    Fang, Chen; Steinbrenner, Julie E.; Wang, Fu-Min; Goodson, Kenneth E.

    2010-04-01

    While microchannel condensation has been the subject of several recent studies, the critical impact of wall hydrophobicity on the microchannel condensation flow has received very little attention. The paper experimentally studies steam condensation in a silicon microchannel 286 µm in hydraulic diameter with three different wall hydrophobicities. It is found that the channel surface wettability has a significant impact on the flow pattern, pressure drop and heat transfer characteristic. Spatial flow pattern transition is observed in both hydrophobic and hydrophilic channels. In the hydrophobic channel, the transition from dropwise/slugwise flow to plug flow is induced by the slug instability. In the hydrophilic channel, the flow transition is characterized by the periodic bubble detachment, a process in which pressure evolution is found important. Local temperature measurement is conducted and heat flux distribution in the microchannel is reconstructed. For the same inlet vapor flux and temperature, the hydrophobic microchannel yields higher heat transfer rate and pressure drop compared to the hydrophilic channel. The difference is attributed to the distinction in flow pattern and heat transfer mechanism dictated by the channel hydrophobicity. This study highlights the importance of the channel hydrophobicity control for the optimization of the microchannel condenser.

  19. Pool boiling with high heat flux enabled by a porous artery structure

    NASA Astrophysics Data System (ADS)

    Bai, Lizhan; Zhang, Lianpei; Lin, Guiping; Peterson, G. P.

    2016-06-01

    A porous artery structure utilizing the concept of "phase separation and modulation" is proposed to enhance the critical heat flux of pool boiling. A series of experiments were conducted on a range of test articles in which multiple rectangular arteries were machined directly into the top surface of a 10.0 mm diameter copper rod. The arteries were then covered by a 2.0 mm thickness microporous copper plate through silver brazing. The pool wall was fabricated from transparent Pyrex glass to allow a visualization study, and water was used as the working fluid. Experimental results confirmed that the porous artery structure provided individual flow paths for the liquid supply and vapor venting, and avoided the detrimental effects of the liquid/vapor counter flow. As a result, a maximum heat flux of 610 W/cm2 over a heating area of 0.78 cm2 was achieved with no indication of dryout, prior to reaching the heater design temperature limit. Following the experimental tests, the mechanisms responsible for the boiling critical heat flux and performance enhancement of the porous artery structure were analyzed.

  20. Gas-surface interactions using accommodation coefficients for a dilute and a dense gas in a micro- or nanochannel: heat flux predictions using combined molecular dynamics and Monte Carlo techniques.

    PubMed

    Nedea, S V; van Steenhoven, A A; Markvoort, A J; Spijker, P; Giordano, D

    2014-05-01

    The influence of gas-surface interactions of a dilute gas confined between two parallel walls on the heat flux predictions is investigated using a combined Monte Carlo (MC) and molecular dynamics (MD) approach. The accommodation coefficients are computed from the temperature of incident and reflected molecules in molecular dynamics and used as effective coefficients in Maxwell-like boundary conditions in Monte Carlo simulations. Hydrophobic and hydrophilic wall interactions are studied, and the effect of the gas-surface interaction potential on the heat flux and other characteristic parameters like density and temperature is shown. The heat flux dependence on the accommodation coefficient is shown for different fluid-wall mass ratios. We find that the accommodation coefficient is increasing considerably when the mass ratio is decreased. An effective map of the heat flux depending on the accommodation coefficient is given and we show that MC heat flux predictions using Maxwell boundary conditions based on the accommodation coefficient give good results when compared to pure molecular dynamics heat predictions. The accommodation coefficients computed for a dilute gas for different gas-wall interaction parameters and mass ratios are transferred to compute the heat flux predictions for a dense gas. Comparison of the heat fluxes derived using explicit MD, MC with Maxwell-like boundary conditions based on the accommodation coefficients, and pure Maxwell boundary conditions are discussed. A map of the heat flux dependence on the accommodation coefficients for a dense gas, and the effective accommodation coefficients for different gas-wall interactions are given. In the end, this approach is applied to study the gas-surface interactions of argon and xenon molecules on a platinum surface. The derived accommodation coefficients are compared with values of experimental results.

  1. EU Development of High Heat Flux Components

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

    Linke, J.; Lorenzetto, P.; Majerus, P.

    2005-04-15

    The development of plasma facing components for next step fusion devices in Europe is strongly focused to ITER. Here a wide spectrum of different design options for the divertor target and the first wall have been investigated with tungsten, CFC, and beryllium armor. Electron beam simulation experiments have been used to determine the performance of high heat flux components under ITER specific thermal loads. Beside thermal fatigue loads with power density levels up to 20 MWm{sup -2}, off-normal events are a serious concern for the lifetime of plasma facing components. These phenomena are expected to occur on a time scalemore » of a few milliseconds (plasma disruptions) or several hundred milliseconds (vertical displacement events) and have been identified as a major source for the production of neutron activated metallic or tritium enriched carbon dust which is of serious importance from a safety point of view.The irradiation induced material degradation is another critical concern for future D-T-burning fusion devices. In ITER the integrated neutron fluence to the first wall and the divertor armour will remain in the order of 1 dpa and 0.7 dpa, respectively. This value is low compared to future commercial fusion reactors; nevertheless, a nonnegligible degradation of the materials has been detected, both for mechanical and thermal properties, in particular for the thermal conductivity of carbon based materials. Beside the degradation of individual material properties, the high heat flux performance of actively cooled plasma facing components has been investigated under ITER specific thermal and neutron loads.« less

  2. Influence of condensation on heat flux and pressure measurements in a detonation-based short-duration facility

    NASA Astrophysics Data System (ADS)

    Haase, S.; Olivier, H.

    2017-10-01

    Detonation-based short-duration facilities provide hot gas with very high stagnation pressures and temperatures. Due to the short testing time, complex and expensive cooling techniques of the facility walls are not needed. Therefore, they are attractive for economical experimental investigations of high-enthalpy flows such as the flow in a rocket engine. However, cold walls can provoke condensation of the hot combustion gas at the walls. This has already been observed in detonation tubes close behind the detonation wave, resulting in a loss of tube performance. A potential influence of condensation at the wall on the experimental results, like wall heat fluxes and static pressures, has not been considered so far. Therefore, in this study the occurrence of condensation and its influence on local heat flux and pressure measurements has been investigated in the nozzle test section of a short-duration rocket-engine simulation facility. This facility provides hot water vapor with stagnation pressures up to 150 bar and stagnation temperatures up to 3800 K. A simple method has been developed to detect liquid water at the wall without direct optical access to the flow. It is shown experimentally and theoretically that condensation has a remarkable influence on local measurement values. The experimental results indicate that for the elimination of these influences the nozzle wall has to be heated to a certain temperature level, which exclusively depends on the local static pressure.

  3. Heat fluxes across the Antarctic Circumpolar Current

    NASA Astrophysics Data System (ADS)

    Ferrari, Ramiro; Provost, Christine; Hyang Park, Young; Sennéchael, Nathalie; Garric, Gilles; Bourdallé-Badie, Romain

    2014-05-01

    Determining the processes responsible for the Southern Ocean heat balance is fundamental to our understanding of the weather and climate systems. Therefore, in the last decades, various studies aimed at analyzing the major mechanisms of the oceanic poleward heat flux in this region. Previous works stipulated that the cross-stream heat flux due to the mesoscale transient eddies was responsible for the total meridional heat transport across the Antarctic Circumpolar Current (ACC). Several numerical modelling and current meters data studies have recently challenged this idea. These showed that the heat flux due to the mean flow in the southern part of the Antarctic Circumpolar Current could be larger than the eddy heat flux contribution by two orders of magnitude. Eddy heat flux and heat flux by the mean flow distributions of were examined in Drake Passage using in situ measurements collected during the DRAKE 2006-9 project (from January 2006 to March 2009), available observations from the historical DRAKE 79 experiment and high resolution model outputs (ORCA 12, MERCATOR). The Drake Passage estimations provided a limited view of heat transport in the Southern Ocean. The small spatial scales shown by the model derived heat flux by the mean flow indicate that circumpolar extrapolations from a single point observation are perilous. The importance of the heat flux due by the mean flow should be further investigated using other in situ observations and numerical model outputs. Similar situation has been observed, with important implication for heat flux due to the mean flow, in other topographically constricted regions with strong flow across prominent submarine ridges (choke points). We have estimated the heat flux due to the mean flow revisiting other ACC mooring sites where in situ time series are available, e.g. south of Australia (Tasmania) (Phillips and Rintoul, 2000), southeast of New Zealand (Campbell Plateau) (Bryden and Heath, 1985). Heat fluxes due to the mean

  4. Geometrical correction factors for heat flux meters

    NASA Technical Reports Server (NTRS)

    Baumeister, K. J.; Papell, S. S.

    1974-01-01

    General formulas are derived for determining gage averaging errors of strip-type heat flux meters used in the measurement of one-dimensional heat flux distributions. The local averaging error e(x) is defined as the difference between the measured value of the heat flux and the local value which occurs at the center of the gage. In terms of e(x), a correction procedure is presented which allows a better estimate for the true value of the local heat flux. For many practical problems, it is possible to use relatively large gages to obtain acceptable heat flux measurements.

  5. Effect of Finite Chemical Reaction Rates on Heat Transfer to the Walls of Combustion-Driven Supersonic MHD Generator Channels

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

    DAILY, J. W. ..; RAEDER, J.; ZANKL, G.

    1974-03-01

    The effect of finite-rate homogeneous chemical reactions on the heat transfer rates to the walls of combustion-driven supersonic MHD generators was investigated. Experiments were performed on a 200 kW(e) combustion generator. The density of the heat flux to the wall was measured at various axial positions along both a circular cross section Hall-type channel and a diagonal wall channel with a rectangular cross section. From the results it was concluded that a substantial decrease in heat transfer rate to the walls of a combustion-driven supersonic MHD power generator was ob served which appears to occur because of chemical nonequilibrium inmore » the developing wall boundary layers. (LCL)« less

  6. β-distribution for Reynolds stress and turbulent heat flux in relaxation turbulent boundary layer of compression ramp

    NASA Astrophysics Data System (ADS)

    Hu, YanChao; Bi, WeiTao; Li, ShiYao; She, ZhenSu

    2017-12-01

    A challenge in the study of turbulent boundary layers (TBLs) is to understand the non-equilibrium relaxation process after sep-aration and reattachment due to shock-wave/boundary-layer interaction. The classical boundary layer theory cannot deal with the strong adverse pressure gradient, and hence, the computational modeling of this process remains inaccurate. Here, we report the direct numerical simulation results of the relaxation TBL behind a compression ramp, which reveal the presence of intense large-scale eddies, with significantly enhanced Reynolds stress and turbulent heat flux. A crucial finding is that the wall-normal profiles of the excess Reynolds stress and turbulent heat flux obey a β-distribution, which is a product of two power laws with respect to the wall-normal distances from the wall and from the boundary layer edge. In addition, the streamwise decays of the excess Reynolds stress and turbulent heat flux also exhibit power laws with respect to the streamwise distance from the corner of the compression ramp. These results suggest that the relaxation TBL obeys the dilation symmetry, which is a specific form of self-organization in this complex non-equilibrium flow. The β-distribution yields important hints for the development of a turbulence model.

  7. Heat flux viscosity in collisional magnetized plasmas

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

    Liu, C., E-mail: cliu@pppl.gov; Fox, W.; Bhattacharjee, A.

    2015-05-15

    Momentum transport in collisional magnetized plasmas due to gradients in the heat flux, a “heat flux viscosity,” is demonstrated. Even though no net particle flux is associated with a heat flux, in a plasma there can still be momentum transport owing to the velocity dependence of the Coulomb collision frequency, analogous to the thermal force. This heat-flux viscosity may play an important role in numerous plasma environments, in particular, in strongly driven high-energy-density plasma, where strong heat flux can dominate over ordinary plasma flows. The heat flux viscosity can influence the dynamics of the magnetic field in plasmas through themore » generalized Ohm's law and may therefore play an important role as a dissipation mechanism allowing magnetic field line reconnection. The heat flux viscosity is calculated directly using the finite-difference method of Epperlein and Haines [Phys. Fluids 29, 1029 (1986)], which is shown to be more accurate than Braginskii's method [S. I. Braginskii, Rev. Plasma Phys. 1, 205 (1965)], and confirmed with one-dimensional collisional particle-in-cell simulations. The resulting transport coefficients are tabulated for ease of application.« less

  8. High flux heat exchanger

    NASA Astrophysics Data System (ADS)

    Flynn, Edward M.; Mackowski, Michael J.

    1993-01-01

    This interim report documents the results of the first two phases of a four-phase program to develop a high flux heat exchanger for cooling future high performance aircraft electronics. Phase 1 defines future needs for high flux heat removal in advanced military electronics systems. The results are sorted by broad application categories: (1) commercial digital systems, (2) military data processors, (3) power processors, and (4) radar and optical systems. For applications expected to be fielded in five to ten years, the outlook is for steady state flux levels of 30-50 W/sq cm for digital processors and several hundred W/sq cm for power control applications. In Phase 1, a trade study was conducted on emerging cooling technologies which could remove a steady state chip heat flux of 100 W/sq cm while holding chip junction temperature to 90 C. Constraints imposed on heat exchanger design, in order to reflect operation in a fighter aircraft environment, included a practical lower limit on coolant supply temperature, the preference for a nontoxic, nonflammable, and nonfreezing coolant, the need to minimize weight and volume, and operation in an accelerating environment. The trade study recommended the Compact High Intensity Cooler (CHIC) for design, fabrication, and test in the final two phases of this program.

  9. Heat flux measurements on ceramics with thin film thermocouples

    NASA Technical Reports Server (NTRS)

    Holanda, Raymond; Anderson, Robert C.; Liebert, Curt H.

    1993-01-01

    Two methods were devised to measure heat flux through a thick ceramic using thin film thermocouples. The thermocouples were deposited on the front and back face of a flat ceramic substrate. The heat flux was applied to the front surface of the ceramic using an arc lamp Heat Flux Calibration Facility. Silicon nitride and mullite ceramics were used; two thicknesses of each material was tested, with ceramic temperatures to 1500 C. Heat flux ranged from 0.05-2.5 MW/m2(sup 2). One method for heat flux determination used an approximation technique to calculate instantaneous values of heat flux vs time; the other method used an extrapolation technique to determine the steady state heat flux from a record of transient data. Neither method measures heat flux in real time but the techniques may easily be adapted for quasi-real time measurement. In cases where a significant portion of the transient heat flux data is available, the calculated transient heat flux is seen to approach the extrapolated steady state heat flux value as expected.

  10. Flow regimes and mechanistic modeling of critical heat flux under subcooled flow boiling conditions

    NASA Astrophysics Data System (ADS)

    Le Corre, Jean-Marie

    Thermal performance of heat flux controlled boiling heat exchangers are usually limited by the Critical Heat Flux (CHF) above which the heat transfer degrades quickly, possibly leading to heater overheating and destruction. In an effort to better understand the phenomena, a literature review of CHF experimental visualizations under subcooled flow boiling conditions was performed and systematically analyzed. Three major types of CHF flow regimes were identified (bubbly, vapor clot and slug flow regime) and a CHF flow regime map was developed, based on a dimensional analysis of the phenomena and available data. It was found that for similar geometric characteristics and pressure, a Weber number (We)/thermodynamic quality (x) map can be used to predict the CHF flow regime. Based on the experimental observations and the review of the available CHF mechanistic models under subcooled flow boiling conditions, hypothetical CHF mechanisms were selected for each CHF flow regime, all based on a concept of wall dry spot overheating, rewetting prevention and subsequent dry spot spreading. It is postulated that a high local wall superheat occurs locally in a dry area of the heated wall, due to a cyclical event inherent to the considered CHF two-phase flow regime, preventing rewetting (Leidenfrost effect). The selected modeling concept has the potential to span the CHF conditions from highly subcooled bubbly flow to early stage of annular flow. A numerical model using a two-dimensional transient thermal analysis of the heater undergoing nucleation was developed to mechanistically predict CHF in the case of a bubbly flow regime. In this type of CHF two-phase flow regime, the high local wall superheat occurs underneath a nucleating bubble at the time of bubble departure. The model simulates the spatial and temporal heater temperature variations during nucleation at the wall, accounting for the stochastic nature of the boiling phenomena. The model has also the potential to evaluate

  11. Measurement of local high-level, transient surface heat flux

    NASA Technical Reports Server (NTRS)

    Liebert, Curt H.

    1988-01-01

    This study is part of a continuing investigation to develop methods for measuring local transient surface heat flux. A method is presented for simultaneous measurements of dual heat fluxes at a surface location by considering the heat flux as a separate function of heat stored and heat conducted within a heat flux gage. Surface heat flux information is obtained from transient temperature measurements taken at points within the gage. Heat flux was determined over a range of 4 to 22 MW/sq m. It was concluded that the method is feasible. Possible applications are for heat flux measurements on the turbine blade surfaces of space shuttle main engine turbopumps and on the component surfaces of rocket and advanced gas turbine engines and for testing sensors in heat flux gage calibrators.

  12. Experimental investigation on the thermal performance of heat storage walls coupled with active solar systems

    NASA Astrophysics Data System (ADS)

    Zhao, Chunyu; You, Shijun; Zhu, Chunying; Yu, Wei

    2016-12-01

    This paper presents an experimental investigation of the performance of a system combining a low-temperature water wall radiant heating system and phase change energy storage technology with an active solar system. This system uses a thermal storage wall that is designed with multilayer thermal storage plates. The heat storage material is expanded graphite that absorbs a mixture of capric acid and lauric acid. An experiment is performed to study the actual effect. The following are studied under winter conditions: (1) the temperature of the radiation wall surface, (2) the melting status of the thermal storage material in the internal plate, (3) the density of the heat flux, and (4) the temperature distribution of the indoor space. The results reveal that the room temperature is controlled between 16 and 20 °C, and the thermal storage wall meets the heating and temperature requirements. The following are also studied under summer conditions: (1) the internal relationship between the indoor temperature distribution and the heat transfer within the regenerative plates during the day and (2) the relationship between the outlet air temperature and inlet air temperature in the thermal storage wall in cooling mode at night. The results indicate that the indoor temperature is approximately 27 °C, which satisfies the summer air-conditioning requirements.

  13. Pyrolytic graphite gauge for measuring heat flux

    NASA Technical Reports Server (NTRS)

    Bunker, Robert C. (Inventor); Ewing, Mark E. (Inventor); Shipley, John L. (Inventor)

    2002-01-01

    A gauge for measuring heat flux, especially heat flux encountered in a high temperature environment, is provided. The gauge includes at least one thermocouple and an anisotropic pyrolytic graphite body that covers at least part of, and optionally encases the thermocouple. Heat flux is incident on the anisotropic pyrolytic graphite body by arranging the gauge so that the gauge surface on which convective and radiative fluxes are incident is perpendicular to the basal planes of the pyrolytic graphite. The conductivity of the pyrolytic graphite permits energy, transferred into the pyrolytic graphite body in the form of heat flux on the incident (or facing) surface, to be quickly distributed through the entire pyrolytic graphite body, resulting in small substantially instantaneous temperature gradients. Temperature changes to the body can thereby be measured by the thermocouple, and reduced to quantify the heat flux incident to the body.

  14. Heat flux measurement in SSME turbine blade tester

    NASA Astrophysics Data System (ADS)

    Liebert, Curt H.

    1990-11-01

    Surface heat flux values were measured in the turbine blade thermal cycling tester located at NASA-Marshall. This is the first time heat flux has been measured in a space shuttle main engine turbopump environment. Plots of transient and quasi-steady state heat flux data over a range of about 0 to 15 MW/sq m are presented. Data were obtained with a miniature heat flux gage device developed at NASA-Lewis. The results from these tests are being incorporated into turbine design models. Also, these gages are being considered for airfoil surface heat flux measurement on turbine vanes mounted in SSME turbopump test bed engine nozzles at Marshall. Heat flux effects that might be observed on degraded vanes are discussed.

  15. Heat flux measurement in SSME turbine blade tester

    NASA Astrophysics Data System (ADS)

    Liebert, Curt H.

    Surface heat flux values were measured in the turbine blade thermal cycling tester located at NASA-Marshall. This is the first time heat flux has been measured in a space shuttle main engine turbopump environment. Plots of transient and quasi-steady state heat flux data over a range of about 0 to 15 MW/sq m are presented. Data were obtained with a miniature heat flux gage device developed at NASA-Lewis. The results from these tests are being incorporated into turbine design models. Also, these gages are being considered for airfoil surface heat flux measurement on turbine vanes mounted in SSME turbopump test bed engine nozzles at Marshall. Heat flux effects that might be observed on degraded vanes are discussed.

  16. Heat flux microsensor measurements and calibrations

    NASA Technical Reports Server (NTRS)

    Terrell, James P.; Hager, Jon M.; Onishi, Shinzo; Diller, Thomas E.

    1992-01-01

    A new thin-film heat flux gage has been fabricated specifically for severe high temperature operation using platinum and platinum-10 percent rhodium for the thermocouple elements. Radiation calibrations of this gage were performed at the AEDC facility over the available heat flux range (approx. 1.0 - 1,000 W/cu cm). The gage output was linear with heat flux with a slight increase in sensitivity with increasing surface temperature. Survivability of gages was demonstrated in quench tests from 500 C into liquid nitrogen. Successful operation of gages to surface temperatures of 750 C has been achieved. No additional cooling of the gages is required because the gages are always at the same temperature as the substrate material. A video of oxyacetylene flame tests with real-time heat flux and temperature output is available.

  17. Fabrication of Thin Film Heat Flux Sensors

    NASA Technical Reports Server (NTRS)

    Will, Herbert A.

    1992-01-01

    Prototype thin film heat flux sensors have been constructed and tested. The sensors can be applied to propulsion system materials and components. The sensors can provide steady state and fast transient heat flux information. Fabrication of the sensor does not require any matching of the mounting surface. Heat flux is proportional to the temperature difference across the upper and lower surfaces of an insulation material. The sensor consists of an array of thermocouples on the upper and lower surfaces of a thin insulating layer. The thermocouples for the sensor are connected in a thermopile arrangement. A 100 thermocouple pair heat flux sensor has been fabricated on silicon wafers. The sensor produced an output voltage of 200-400 microvolts when exposed to a hot air heat gun. A 20 element thermocouple pair heat flux sensor has been fabricated on aluminum oxide sheet. Thermocouples are Pt-Pt/Rh with silicon dioxide as the insulating material. This sensor produced an output of 28 microvolts when exposed to the radiation of a furnace operating at 1000 C. Work is also underway to put this type of heat flux sensor on metal surfaces.

  18. Role of surface heat fluxes underneath cold pools

    DOE PAGES

    Gentine, Pierre; Garelli, Alix; Park, Seung -Bu; ...

    2016-01-05

    In this paper, the role of surface heat fluxes underneath cold pools is investigated using cloud–resolving simulations with either interactive or horizontally homogenous surface heat fluxes over an ocean and a simplified land surface. Over the ocean, there are limited changes in the distribution of the cold pool temperature, humidity, and gust front velocity, yet interactive heat fluxes induce more cold pools, which are smaller, and convection is then less organized. Correspondingly, the updraft mass flux and lateral entrainment are modified. Over the land surface, the heat fluxes underneath cold pools drastically impact the cold pool characteristics with more numerousmore » and smaller pools, which are warmer and more humid and accompanied by smaller gust front velocities. The interactive fluxes also modify the updraft mass flux and reduce convective organization. These results emphasize the importance of interactive surface fluxes instead of prescribed flux boundary conditions, as well as the formulation of surface heat fluxes, when studying convection.« less

  19. Role of surface heat fluxes underneath cold pools

    PubMed Central

    Garelli, Alix; Park, Seung‐Bu; Nie, Ji; Torri, Giuseppe; Kuang, Zhiming

    2016-01-01

    Abstract The role of surface heat fluxes underneath cold pools is investigated using cloud‐resolving simulations with either interactive or horizontally homogenous surface heat fluxes over an ocean and a simplified land surface. Over the ocean, there are limited changes in the distribution of the cold pool temperature, humidity, and gust front velocity, yet interactive heat fluxes induce more cold pools, which are smaller, and convection is then less organized. Correspondingly, the updraft mass flux and lateral entrainment are modified. Over the land surface, the heat fluxes underneath cold pools drastically impact the cold pool characteristics with more numerous and smaller pools, which are warmer and more humid and accompanied by smaller gust front velocities. The interactive fluxes also modify the updraft mass flux and reduce convective organization. These results emphasize the importance of interactive surface fluxes instead of prescribed flux boundary conditions, as well as the formulation of surface heat fluxes, when studying convection. PMID:27134320

  20. Development of a real-time system for ITER first wall heat load control

    NASA Astrophysics Data System (ADS)

    Anand, Himank; de Vries, Peter; Gribov, Yuri; Pitts, Richard; Snipes, Joseph; Zabeo, Luca

    2017-10-01

    The steady state heat flux on the ITER first wall (FW) panels are limited by the heat removal capacity of the water cooling system. In case of off-normal events (e.g. plasma displacement during H-L transitions), the heat loads are predicted to exceed the design limits (2-4.7 MW/m2). Intense heat loads are predicted on the FW, even well before the burning plasma phase. Thus, a real-time (RT) FW heat load control system is mandatory from early plasma operation of the ITER tokamak. A heat load estimator based on the RT equilibrium reconstruction has been developed for the plasma control system (PCS). A scheme, estimating the energy state for prescribed gaps defined as the distance between the last closed flux surface (LCFS)/separatrix and the FW is presented. The RT energy state is determined by the product of a weighted function of gap distance and the power crossing the plasma boundary. In addition, a heat load estimator assuming a simplified FW geometry and parallel heat transport model in the scrape-off layer (SOL), benchmarked against a full 3-D magnetic field line tracer is also presented.

  1. Optical heat flux gauge

    DOEpatents

    Noel, Bruce W.; Borella, Henry M.; Cates, Michael R.; Turley, W. Dale; MaCarthur, Charles D.; Cala, Gregory C.

    1991-01-01

    A heat flux gauge comprising first and second thermographic phosphor layers separated by a layer of a thermal insulator. The gauge may be mounted on a surface with the first thermographic phosphor in contact with the surface. A light source is directed at the gauge, causing the phosphors to luminesce. The luminescence produced by the phosphors is collected and its spectra analyzed in order to determine the heat flux on the surface. First and second phosphor layers must be different materials to assure that the spectral lines collected will be distinguishable.

  2. On the roles of solid wall in the thermal analysis of micro heat pipes

    NASA Astrophysics Data System (ADS)

    Hung, Yew Mun

    Micro heat pipe is a small-scale passive heat transfer device of very high thermal conductance that uses phase change and circulation of its working fluid to transfer thermal energy. Different from conventional heat pipe, a micro heat pipe does not contain any wick structure. In this thesis, a one-dimensional, steady-state mathematical model of a single triangular micro heat pipe is developed, with the main purpose of establishing a series of analytical studies on the roles of the solid wall of micro heat pipes in conjunction with the characterization of the thermal performance under the effects of various design and operational parameters. The energy equation of the solid wall is solved analytically to obtain the temperature distribution. The liquid phase is coupled with the solid wall through the continuity of heat flux at their interface, and the continuity, momentum and energy equations of the liquid and vapour phases, together with the Young-Laplace equation for capillary pressure, are solve numerically to yield the heat and fluid flow characteristics of the micro heat pipe. By coupling this mathematical model with the phase-change interfacial resistance model, the relationships for the axial temperature distributions of the liquid and vapour phases throughout the longitudinal direction of a micro heat pipe are also formulated. Four major aspects associated with the operational performance of micro heat pipes are discussed. Firstly, the investigation of the effects of axial conduction in the solid wall reveals that the presence of the solid wall induces change in the phase-change heat transport of the working fluid besides facilitating axial heat conduction in the solid wall. The analysis also highlights the effects of the thickness and thermal conductivity of the solid wall on the axial temperature distribution of solid wall, in the wake of the effects of the axial heat conduction induced on the phase-change heat transport of the working fluid. Secondly

  3. Thin Film Heat Flux Sensors: Design and Methodology

    NASA Technical Reports Server (NTRS)

    Fralick, Gustave C.; Wrbanek, John D.

    2013-01-01

    Thin Film Heat Flux Sensors: Design and Methodology: (1) Heat flux is one of a number of parameters, together with pressure, temperature, flow, etc. of interest to engine designers and fluid dynamists, (2) The measurement of heat flux is of interest in directly determining the cooling requirements of hot section blades and vanes, and (3)In addition, if the surface and gas temperatures are known, the measurement of heat flux provides a value for the convective heat transfer coefficient that can be compared with the value provided by CFD codes.

  4. Prediction of forced convective heat transfer and critical heat flux for subcooled water flowing in miniature tubes

    NASA Astrophysics Data System (ADS)

    Shibahara, Makoto; Fukuda, Katsuya; Liu, Qiusheng; Hata, Koichi

    2018-02-01

    The heat transfer characteristics of forced convection for subcooled water in small tubes were clarified using the commercial computational fluid dynamic (CFD) code, PHENICS ver. 2013. The analytical model consists of a platinum tube (the heated section) and a stainless tube (the non-heated section). Since the platinum tube was heated by direct current in the authors' previous experiments, a uniform heat flux with the exponential function was given as a boundary condition in the numerical simulation. Two inner diameters of the tubes were considered: 1.0 and 2.0 mm. The upward flow velocities ranged from 2 to 16 m/s and the inlet temperature ranged from 298 to 343 K. The numerical results showed that the difference between the surface temperature and the bulk temperature was in good agreement with the experimental data at each heat flux. The numerical model was extended to the liquid sublayer analysis for the CHF prediction and was evaluated by comparing its results with the experimental data. It was postulated that the CHF occurs when the fluid temperature near the heated wall exceeds the saturated temperature, based on Celata et al.'s superheated layer vapor replenishment (SLVR) model. The suggested prediction method was in good agreement with the experimental data and with other CHF data in literature within ±25%.

  5. Miniature Convection Cooled Plug-type Heat Flux Gauges

    NASA Technical Reports Server (NTRS)

    Liebert, Curt H.

    1994-01-01

    Tests and analysis of a new miniature plug-type heat flux gauge configuration are described. This gauge can simultaneously measure heat flux on two opposed active surfaces when heat flux levels are equal to or greater than about 0.2 MW/m(sup 2). The performance of this dual active surface gauge was investigated over a wide transient and steady heat flux and temperature range. The tests were performed by radiatively heating the front surface with an argon arc lamp while the back surface was convection cooled with air. Accuracy is about +20 percent. The gauge is responsive to fast heat flux transients and is designed to withstand the high temperature (1300 K), high pressure (15 MPa), erosive and corrosive environments in modern engines. This gauge can be used to measure heat flux on the surfaces of internally cooled apparatus such as turbine blades and combustors used in jet propulsion systems and on the surfaces of hypersonic vehicles. Heat flux measurement accuracy is not compromised when design considerations call for various size gauges to be fabricated into alloys of various shapes and properties. Significant gauge temperature reductions (120 K), which can lead to potential gauge durability improvement, were obtained when the gauges were air-cooled by forced convection.

  6. Integrated computational study of ultra-high heat flux cooling using cryogenic micro-solid nitrogen spray

    NASA Astrophysics Data System (ADS)

    Ishimoto, Jun; Oh, U.; Tan, Daisuke

    2012-10-01

    A new type of ultra-high heat flux cooling system using the atomized spray of cryogenic micro-solid nitrogen (SN2) particles produced by a superadiabatic two-fluid nozzle was developed and numerically investigated for application to next generation super computer processor thermal management. The fundamental characteristics of heat transfer and cooling performance of micro-solid nitrogen particulate spray impinging on a heated substrate were numerically investigated and experimentally measured by a new type of integrated computational-experimental technique. The employed Computational Fluid Dynamics (CFD) analysis based on the Euler-Lagrange model is focused on the cryogenic spray behavior of atomized particulate micro-solid nitrogen and also on its ultra-high heat flux cooling characteristics. Based on the numerically predicted performance, a new type of cryogenic spray cooling technique for application to a ultra-high heat power density device was developed. In the present integrated computation, it is clarified that the cryogenic micro-solid spray cooling characteristics are affected by several factors of the heat transfer process of micro-solid spray which impinges on heated surface as well as by atomization behavior of micro-solid particles. When micro-SN2 spraying cooling was used, an ultra-high cooling heat flux level was achieved during operation, a better cooling performance than that with liquid nitrogen (LN2) spray cooling. As micro-SN2 cooling has the advantage of direct latent heat transport which avoids the film boiling state, the ultra-short time scale heat transfer in a thin boundary layer is more possible than in LN2 spray. The present numerical prediction of the micro-SN2 spray cooling heat flux profile can reasonably reproduce the measurement results of cooling wall heat flux profiles. The application of micro-solid spray as a refrigerant for next generation computer processors is anticipated, and its ultra-high heat flux technology is expected

  7. Optical heat flux gauge

    DOEpatents

    Noel, Bruce W.; Borella, Henry M.; Cates, Michael R.; Turley, W. Dale; MacArthur, Charles D.; Cala, Gregory C.

    1991-01-01

    A heat flux gauge comprising first and second thermographic phosphor layers separated by a layer of a thermal insulator wherein each thermographic layer comprises a plurality of respective thermographic phosphors. The gauge may be mounted on a surface with the first thermographic phosphor in contact with the surface. A light source is directed at the gauge, causing the phosphors to luminesce. The luminescence produced by the phosphors is collected and its spectra analyzed in order to determine the heat flux on the surface. First and second phosphor layers must be different materials to assure that the spectral lines collected will be distinguishable.

  8. A heat flux modulator from carbon nanotubes.

    PubMed

    Jiang, Shaohui; Zhang, Guang; Xia, Dan; Liu, Changhong; Fan, Shoushan

    2015-08-28

    For a heat flux modulator, the most difficult problem is that the main carriers named 'phonons' have little response to external fields. Of the existing studies on heat flux modulators, most were theoretical work and the materials systems for the theoretical calculations were artificial lattices. In this paper, we made a heat modulator with ultrathin buckypaper which was made of multi-layer carbon nanotube sheets overlapped together, and achieved an on/off ratio whose value was 1.41 using an pendent block in experiments without special optimizations. When the temperatures of the two sides were of appropriate values, we could even see a negative heat flux. Intuitively, the heat flux was tuned by the gap between the buckypaper and the pendent gate, and we observed that there was heat transferred to the pendent block. The structure of the modulator is similar to a CNT transistor with a contactless gate, hence this type of micromodulator will be easy to manufacture in the future.

  9. Tracking heat flux sensors for concentrating solar applications

    DOEpatents

    Andraka, Charles E; Diver, Jr., Richard B

    2013-06-11

    Innovative tracking heat flux sensors located at or near the solar collector's focus for centering the concentrated image on a receiver assembly. With flux sensors mounted near a receiver's aperture, the flux gradient near the focus of a dish or trough collector can be used to precisely position the focused solar flux on the receiver. The heat flux sensors comprise two closely-coupled thermocouple junctions with opposing electrical polarity that are separated by a thermal resistor. This arrangement creates an electrical signal proportional to heat flux intensity, and largely independent of temperature. The sensors are thermally grounded to allow a temperature difference to develop across the thermal resistor, and are cooled by a heat sink to maintain an acceptable operating temperature.

  10. Structures for handling high heat fluxes

    NASA Astrophysics Data System (ADS)

    Watson, R. D.

    1990-12-01

    The divertor is reconized as one of the main performance limiting components for ITER. This paper reviews the critical issues for structures that are designed to withstand heat fluxes > 5 MW/m 2. High velocity, sub-cooled water with twisted tape inserts for enhanced heat transfer provides a critical heat flux limit of 40-60 MW/m 2. Uncertainties in physics and engineering heat flux peaking factors require that the design heat flux not exceed 10 MW/m 2 to maintain an adequate burnout safety margin. Armor tiles and heat sink materials must have a well matched thermal expansion coefficient to minimize stresses. The divertor lifetime from sputtering erosion is highly uncertain. The number of disruptions specified for ITER must be reduced to achieve a credible design. In-situ plasma spray repair with thick metallic coatings may reduce the problems of erosion. Runaway electrons in ITER have the potential to melt actively cooled components in a single event. A water leak is a serious accident because of steam reactions with hot carbon, beryllium, or tungsten that can mobilize large amounts of tritium and radioactive elements. If the plasma does not shutdown immediately, the divertor can melt in 1-10 s after a loss of coolant accident. Very high reliability of carbon tile braze joints will be required to achieve adequate safety and performance goals. Most of these critical issues will be addressed in the near future by operation of the Tore Supra pump limiters and the JET pumped divertor. An accurate understanding of the power flow out of edge of a DT burning plasma is essential to successful design of high heat flux components.

  11. Investigation of Body Force Effects on Flow Boiling Critical Heat Flux

    NASA Technical Reports Server (NTRS)

    Zhang, Hui; Mudawar, Issam; Hasan, Mohammad M.

    2002-01-01

    The bubble coalescence and interfacial instabilities that are important to modeling critical heat flux (CHF) in reduced-gravity systems can be sensitive to even minute body forces. Understanding these complex phenomena is vital to the design and safe implementation of two-phase thermal management loops proposed for space and planetary-based thermal systems. While reduced gravity conditions cannot be accurately simulated in 1g ground-based experiments, such experiments can help isolate the effects of the various forces (body force, surface tension force and inertia) which influence flow boiling CHF. In this project, the effects of the component of body force perpendicular to a heated wall were examined by conducting 1g flow boiling experiments at different orientations. FC-72 liquid was boiled along one wall of a transparent rectangular flow channel that permitted photographic study of the vapor-liquid interface at conditions approaching CHF. High-speed video imaging was employed to capture dominant CHF mechanisms. Six different CHF regimes were identified: Wavy Vapor Layer, Pool Boiling, Stratification, Vapor Counterflow, Vapor Stagnation, and Separated Concurrent Vapor Flow. CHF showed great sensitivity to orientation for flow velocities below 0.2 m/s, where very small CHF values where measured, especially with downflow and downward-facing heated wall orientations. High flow velocities dampened the effects of orientation considerably. Figure I shows representative images for the different CHF regimes. The Wavy Vapor Layer regime was dominant for all high velocities and most orientations, while all other regimes were encountered at low velocities, in the downflow and/or downward-facing heated wall orientations. The Interfacial Lift-off model was modified to predict the effects of orientation on CHF for the dominant Wavy Vapor Layer regime. The photographic study captured a fairly continuous wavy vapor layer travelling along the heated wall while permitting liquid

  12. Experiments of Transient Condensation Heat Transfer on the Heat Flux Senor

    NASA Astrophysics Data System (ADS)

    Wang, Xuwen; Liu, Qiusheng; Zhu, Zhiqiang; Chen, Xue

    2015-09-01

    The influence of transient heat transfer in different condensation condition was investigated experimentally in the present paper. Getting condensation heat and mass transfer regularity and characteristics in space can provide theoretical basis for thermodynamic device such as heat pipes, loop heat pipes and capillary pumped loops as well as other fluid management engineering designing. In order to study the condensation process in space, an experimental study has been carried out on the ground for space experiment. The results show that transit heat transfer coefficient of film condensation is related to the condensation film width, the flow condition near the two phase interface and the pressure of the vapor and non-condensable gas in chamber. On the ground, the condensation heat flux on vertical surface is higher than it on horizontal surface. The transit heat flux of film condensation is affected by the temperature of superheated vapor, the temperature of condensation surface and non-condensable gas pressure. Condensation heat flux with vapor forced convection is many times more than it with natural convection. All of heat flux for both vapor forced convection and natural convection condensation in limited chamber declines dramatically over time. The present experiment is preliminary work for our future space experiments of the condensation and heat transfer process onboard the Chinese Spacecraft "TZ-1" to be launched in 2016.

  13. Optical heat flux gauge

    DOEpatents

    Noel, Bruce W.; Borella, Henry M.; Cates, Michael R.; Turley, W. Dale; MacArthur, Charles D.; Cala, Gregory C.

    1991-01-01

    A heat flux gauge comprising first and second thermographic phosphor layers separated by a layer of a thermal insulator, wherein each thermographic layer comprises a plurality of respective thermographic sensors in a juxtaposed relationship with respect to each other. The gauge may be mounted on a surface with the first thermographic phosphor in contact with the surface. A light source is directed at the gauge, causing the phosphors to luminesce. The luminescence produced by the phosphors is collected and its spectra analyzed in order to determine the heat flux on the surface. First and second phosphor layers must be different materials to assure that the spectral lines collected will be distinguishable.

  14. Effects of Mixed Layer Shear on Vertical Heat Flux

    DTIC Science & Technology

    2016-12-01

    correlation of ice speed to heat flux (r = .312, p < .001). Relationships between ice speed and shear (r = .107, p < .001), ice speed and inverse ...Richardson number (r = .035, p = .256), inverse Richardson number and heat flux (r = .3, p < .001), heat content and heat flux (r = .084, p < .001) were...correlation of ice speed to heat flux (r = .312, p < .001). Relationships between ice speed and shear (r = .107, p < .001), ice speed and inverse Richardson

  15. Towards Improved Estimates of Ocean Heat Flux

    NASA Astrophysics Data System (ADS)

    Bentamy, Abderrahim; Hollman, Rainer; Kent, Elisabeth; Haines, Keith

    2014-05-01

    Recommendations and priorities for ocean heat flux research are for instance outlined in recent CLIVAR and WCRP reports, eg. Yu et al (2013). Among these is the need for improving the accuracy, the consistency, and the spatial and temporal resolution of air-sea fluxes over global as well as at region scales. To meet the main air-sea flux requirements, this study is aimed at obtaining and analyzing all the heat flux components (latent, sensible and radiative) at the ocean surface over global oceans using multiple satellite sensor observations in combination with in-situ measurements and numerical model analyses. The fluxes will be generated daily and monthly for the 20-year (1992-2011) period, between 80N and 80S and at 0.25deg resolution. Simultaneous estimates of all surface heat flux terms have not yet been calculated at such large scale and long time period. Such an effort requires a wide range of expertise and data sources that only recently are becoming available. Needed are methods for integrating many data sources to calculate energy fluxes (short-wave, long wave, sensible and latent heat) across the air-sea interface. We have access to all the relevant, recently available satellite data to perform such computations. Yu, L., K. Haines, M. Bourassa, M. Cronin, S. Gulev, S. Josey, S. Kato, A. Kumar, T. Lee, D. Roemmich: Towards achieving global closure of ocean heat and freshwater budgets: Recommendations for advancing research in air-sea fluxes through collaborative activities. INTERNATIONAL CLIVAR PROJECT OFFICE, 2013: International CLIVAR Publication Series No 189. http://www.clivar.org/sites/default/files/ICPO189_WHOI_fluxes_workshop.pdf

  16. A novel approach to evaluate soil heat flux calculation: An analytical review of nine methods: Soil Heat Flux Calculation

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

    Gao, Zhongming; Russell, Eric S.; Missik, Justine E. C.

    We evaluated nine methods of soil heat flux calculation using field observations. All nine methods underestimated the soil heat flux by at least 19%. This large underestimation is mainly caused by uncertainties in soil thermal properties.

  17. Infrared thermography with non-uniform heat flux boundary conditions on the rotor endwall of an axial turbine

    NASA Astrophysics Data System (ADS)

    Lazzi Gazzini, S.; Schädler, R.; Kalfas, A. I.; Abhari, R. S.

    2017-02-01

    It is technically challenging to measure heat fluxes on the rotating components of gas turbines, yet accurate knowledge of local heat loads under engine-representative conditions is crucial for ensuring the reliability of the designs. In this work, quantitative image processing tools were developed to perform fast and accurate infrared thermography measurements on 3D-shaped film-heaters directly deposited on the turbine endwalls. The newly developed image processing method and instrumentation were used to measure the heat load on the rotor endwalls of an axial turbine. A step-transient heat flux calibration technique is applied to measure the heat flux generated locally by the film heater, thus eliminating the need for a rigorously iso-energetic boundary condition. On-board electronics installed on the rotor record the temperature readings of RTDs installed in the substrate below the heaters in order to evaluate the conductive losses in the solid. Full maps of heat transfer coefficient and adiabatic wall temperature are produced for two different operating conditions, demonstrating the sensitivity of the technique to local flow features and variations in heat transfer due to Reynolds number effect.

  18. An assessment of CFD-based wall heat transfer models in piston engines

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

    Sircar, Arpan; Paul, Chandan; Ferreyro-Fernandez, Sebastian

    The lack of accurate submodels for in-cylinder heat transfer has been identified as a key shortcoming in developing truly predictive, physics-based computational fluid dynamics (CFD) models that can be used to develop combustion systems for advanced high-efficiency, low-emissions engines. Only recently have experimental methods become available that enable accurate near-wall measurements to enhance simulation capability via advancing models. Initial results show crank-angle dependent discrepancies with respect to previously used boundary-layer models of up to 100%. However, available experimental data is quite sparse (only few data points on engine walls) and limited (available measurements are those of heat flux only). Predictivemore » submodels are needed for medium-resolution ("engineering") LES and for unsteady Reynolds-averaged simulations (URANS). Recently, some research groups have performed DNS studies on engine-relevant conditions using simple geometries. These provide very useful data for benchmarking wall heat transfer models under such conditions. Further, a number of new and more sophisticated models have also become available in the literature which account for these engine-like conditions. Some of these have been incorporated while others of a more complex nature, which include solving additional partial differential equations (PDEs) within the thin boundary layer near the wall, are underway. These models will then be tested against the available DNS/experimental data in both SI (spark-ignition) and CI (compression-ignition) engines.« less

  19. Time and Space Resolved Heat Transfer Measurements Under Nucleate Bubbles with Constant Heat Flux Boundary Conditions

    NASA Technical Reports Server (NTRS)

    Myers, Jerry G.; Hussey, Sam W.; Yee, Glenda F.; Kim, Jungho

    2003-01-01

    Investigations into single bubble pool boiling phenomena are often complicated by the difficulties in obtaining time and space resolved information in the bubble region. This usually occurs because the heaters and diagnostics used to measure heat transfer data are often on the order of, or larger than, the bubble characteristic length or region of influence. This has contributed to the development of many different and sometimes contradictory models of pool boiling phenomena and dominant heat transfer mechanisms. Recent investigations by Yaddanapyddi and Kim and Demiray and Kim have obtained time and space resolved heat transfer information at the bubble/heater interface under constant temperature conditions using a novel micro-heater array (10x10 array, each heater 100 microns on a side) that is semi-transparent and doubles as a measurement sensor. By using active feedback to maintain a state of constant temperature at the heater surface, they showed that the area of influence of bubbles generated in FC-72 was much smaller than predicted by standard models and that micro-conduction/micro-convection due to re-wetting dominated heat transfer effects. This study seeks to expand on the previous work by making time and space resolved measurements under bubbles nucleating on a micro-heater array operated under constant heat flux conditions. In the planned investigation, wall temperature measurements made under a single bubble nucleation site will be synchronized with high-speed video to allow analysis of the bubble energy removal from the wall.

  20. Optical heat flux gauge

    DOEpatents

    Noel, B.W.; Borella, H.M.; Cates, M.R.; Turley, W.D.; MacArthur, C.D.; Cala, G.C.

    1991-04-09

    A heat flux gauge is disclosed comprising first and second thermographic phosphor layers separated by a layer of a thermal insulator, wherein each thermographic layer comprises a plurality of respective thermographic sensors in a juxtaposed relationship with respect to each other. The gauge may be mounted on a surface with the first thermographic phosphor in contact with the surface. A light source is directed at the gauge, causing the phosphors to luminesce. The luminescence produced by the phosphors is collected and its spectra analyzed in order to determine the heat flux on the surface. First and second phosphor layers must be different materials to assure that the spectral lines collected will be distinguishable. 9 figures.

  1. High heat flux measurements and experimental calibrations/characterizations

    NASA Technical Reports Server (NTRS)

    Kidd, Carl T.

    1992-01-01

    Recent progress in techniques employed in the measurement of very high heat-transfer rates in reentry-type facilities at the Arnold Engineering Development Center (AEDC) is described. These advances include thermal analyses applied to transducer concepts used to make these measurements; improved heat-flux sensor fabrication methods, equipment, and procedures for determining the experimental time response of individual sensors; performance of absolute heat-flux calibrations at levels above 2,000 Btu/cu ft-sec (2.27 kW/cu cm); and innovative methods of performing in-situ run-to-run characterizations of heat-flux probes installed in the test facility. Graphical illustrations of the results of extensive thermal analyses of the null-point calorimeter and coaxial surface thermocouple concepts with application to measurements in aerothermal test environments are presented. Results of time response experiments and absolute calibrations of null-point calorimeters and coaxial thermocouples performed in the laboratory at intermediate to high heat-flux levels are shown. Typical AEDC high-enthalpy arc heater heat-flux data recently obtained with a Calspan-fabricated null-point probe model are included.

  2. Investigation of the effects of pressure gradient, temperature and wall temperature ratio on the stagnation point heat transfer for circular cylinders and gas turbine vanes

    NASA Technical Reports Server (NTRS)

    Nagamatsu, H. T.; Duffy, R. E.

    1984-01-01

    Low and high pressure shock tubes were designed and constructed for the purpose of obtaining heat transfer data over a temperature range of 390 to 2500 K, pressures of 0.3 to 42 atm, and Mach numbers of 0.15 to 1.5 with and without pressure gradient. A square test section with adjustable top and bottom walls was constructed to produce the favorable and adverse pressure gradient over the flat plate with heat gages. A water cooled gas turbine nozzle cascade which is attached to the high pressure shock tube was obtained to measuse the heat flux over pressure and suction surfaces. Thin-film platinum heat gages with a response time of a few microseconds were developed and used to measure the heat flux for laminar, transition, and turbulent boundary layers. The laminar boundary heat flux on the shock tube wall agreed with Mirel's flat plate theory. Stagnation point heat transfer for circular cylinders at low temperature compared with the theoretical prediction, but for a gas temperature of 922 K the heat fluxes were higher than the predicted values. Preliminary flat plate heat transfer data were measured for laminar, transition, and turbulent boundary layers with and without pressure gradients for free-stream temperatures of 350 to 2575 K and flow Mach numbers of 0.11 to 1.9. The experimental heat flux data were correlated with the laminar and turbulent theories and the agreement was good at low temperatures which was not the case for higher temperatures.

  3. Structural heat pipe. [for spacecraft wall thermal insulation system

    NASA Technical Reports Server (NTRS)

    Ollendorf, S. (Inventor)

    1974-01-01

    A combined structural reinforcing element and heat transfer member is disclosed for placement between a structural wall and an outer insulation blanket. The element comprises a heat pipe, one side of which supports the outer insulation blanket, the opposite side of which is connected to the structural wall. Heat penetrating through the outer insulation blanket directly reaches the heat pipe and is drawn off, thereby reducing thermal gradients in the structural wall. The element, due to its attachment to the structural wall, further functions as a reinforcing member.

  4. Heat Flux Sensors for Infrared Thermography in Convective Heat Transfer

    PubMed Central

    Carlomagno, Giovanni Maria; de Luca, Luigi; Cardone, Gennaro; Astarita, Tommaso

    2014-01-01

    This paper reviews the most dependable heat flux sensors, which can be used with InfraRed (IR) thermography to measure convective heat transfer coefficient distributions, and some of their applications performed by the authors' research group at the University of Naples Federico II. After recalling the basic principles that make IR thermography work, the various heat flux sensors to be used with it are presented and discussed, describing their capability to investigate complex thermo-fluid-dynamic flows. Several applications to streams, which range from natural convection to hypersonic flows, are also described. PMID:25386758

  5. Dean vortices with wall flux in a curved channel membrane system. 2: The velocity field

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

    Chung, K.Y.; Brewster, M.E.; Belfort, G.

    1996-02-01

    The velocity and pressure fields and the effect of wall flux on these fields in a spiral channel are presented. As fluid flows inward through a spiral channel with constant gap and permeable walls, the streamwise flux decreases while the curvature increases. Thus, by balancing the stabilizing effect of wall suction with the destabilizing effect of increasing curvature, established vortices can be maintained along the spiral channel. This approach is used to prescribe spiral geometries with different wall fluxes. Using a weakly nonlinear stability analysis, the influence of wall flux on the characteristics of Dean vortices is obtained. The criticalmore » Dean number is reduced when suction is through the inner wall only, is slightly reduced when suction is equal through both walls, and is increased when suction is through the outer wall only. The magnitude of change is proportional to a ratio of small numbers that measures the importance of the effect of curvature. In membrane filtration applications the wall flux is typically 2 to 5 orders of magnitude less than the streamwise flow. If the radius of curvature of the channel is of the order of 100 times the channel gap, the effect on the critical Dean number is within 2% of the no-wall flux case. If the radius of curvature is sufficiently large, however, it is possible to observe effects on the critical Dean number that approach O(1) in magnitude for certain parameter ranges.« less

  6. An experimental and numerical study of endwall heat transfer in a turbine blade cascade including tangential heat conduction analysis

    NASA Astrophysics Data System (ADS)

    Ratto, Luca; Satta, Francesca; Tanda, Giovanni

    2018-06-01

    This paper presents an experimental and numerical investigation of heat transfer in the endwall region of a large scale turbine cascade. The steady-state liquid crystal technique has been used to obtain the map of the heat transfer coefficient for a constant heat flux boundary condition. In the presence of two- and three-dimensional flows with significant spatial variations of the heat transfer coefficient, tangential heat conduction could lead to error in the heat transfer coefficient determination, since local heat fluxes at the wall-to-fluid interface tend to differ from point to point and surface temperatures to be smoothed out, thus making the uniform-heat-flux boundary condition difficult to be perfectly achieved. For this reason, numerical simulations of flow and heat transfer in the cascade including the effect of tangential heat conduction inside the endwall have been performed. The major objective of numerical simulations was to investigate the influence of wall heat conduction on the convective heat transfer coefficient determined during a nominal iso-flux heat transfer experiment and to interpret possible differences between numerical and experimental heat transfer results. Results were presented and discussed in terms of local Nusselt number and a convenient wall heat flux function for two values of the Reynolds number (270,000 and 960,000).

  7. Measuring Subsurface Water Fluxes Using a Heat Pulse Sensor

    NASA Astrophysics Data System (ADS)

    Ochsner, T. E.; Wang, Q.; Horton, R.

    2001-12-01

    Subsurface water flux is an important parameter in studies of runoff, infiltration, groundwater recharge, and subsurface chemical transport. Heat pulse sensors have been proposed as promising tools for measuring subsurface water fluxes. Our heat pulse probe consists of three 4-cm stainless-steel needles embedded in a waterproof epoxy body. The needles contain resistance heaters and thermocouples. The probes are connected to an external datalogger and power supply and then installed in soil. To measure the water flux, a 15-s heat pulse is generated at the middle needle using the power supply and the resistance heater, and the temperature increases at the needles 6-mm upstream and downstream from the heater are recorded using the thermocouples and datalogger. To date, heat pulse methods have required cumbersome mathematical analysis to calculate soil water flux from this measured data. We present a new mathematical analysis showing that a simple relationship exists between water flux and the ratio of the temperature increase downstream from the line heat source to the temperature increase upstream from the line heat source. The simplicity of this relationship makes heat pulse sensors a more attractive option for measuring subsurface water fluxes.

  8. Graphical determination of wall temperatures for heat transfers through walls of arbitrary shape

    NASA Technical Reports Server (NTRS)

    Lutz, Otto

    1950-01-01

    A graphical method is given which permits determining of the temperature distribution during heat transfer in arbitrarily shaped walls. Three examples show the application of the method. The further development of heat engines depends to a great extent on the control of the thermal stresses in the walls. The thermal stresses stem from the nonuniform temperature distribution in heat transfer through walls which are, for structural reasons, of various thicknesses and sometimes complicated shape. Thus, it is important to know the temperature distribution in these structural parts. Following, a method is given which permits solution of this problem.

  9. A novel transient wall heat transfer approach for the start-up of SI engines with gasoline direct injection

    NASA Astrophysics Data System (ADS)

    Lejsek, David; Kulzer, André; Hammer, Jürgen

    2010-11-01

    The introduction of CO2-reduction technologies like Start-Stop or the Hybrid-Powertrain and the worldwide stringent emission legislation require a detailed optimization of the engine start-up. The combustion concept development as well as the calibration of the engine control unit makes an explicit thermodynamic analysis of the combustion process during the start-up necessary. Initially, the well-known thermodynamic analysis of in-cylinder pressure at stationary condition was transmitted to the highly non-stationary engine start-up. For this running mode of the engine the current models for calculation of the transient wall heat fluxes were found to be misleading. With a fraction of nearly 45% of the burned fuel energy, the wall heat is very important for the calculation of energy balance and for the combustion process analysis. Based on the measurements of transient wall heat transfer densities during the start-up presented in a former work (Lejsek and Kulzer in Investigations on the transient wall heat transfer at start-up for SI engines with gasoline direct injection. SAE Paper), the paper describes the development of adaptations to the known correlations by Woschni (MTZ 31:491, 1970), Hohenberg (Experimentelle Erfassung der Wandwärme von Kolbenmotoren. TU Graz, Habil., 1980) and Bargende (Ein Gleichungsansatz zur Berechnung der instationären Wandwärmeverluste im Hochdruckteil von Ottomotoren. TH Darmstadt, PhD-Thesis, 1991) for the application during engine start-up. To demonstrate the high accuracy of the model, the results of the cyclic resolved thermodynamic analysis using the presented novel approaches were compared with the results of the measurements. It is shown, that the novel heat flux models for the engine start-up process gives a cyclic resolved thermodynamic analysis to optimize the engine start-up pretty efficient.

  10. Diamond Microchannel Heat Sink Designs For High Heat Flux Thermal Control

    NASA Astrophysics Data System (ADS)

    Corbin, Michael V.; DeBenedictis, Matthew M.; James, David B.; LeBlanc, Stephen P.; Paradis, Leo R.

    2002-08-01

    Directed energy weapons, wide band gap semiconductor based radars, and other powerful systems present significant thermal control challenges to component designers. heat Flux levels approaching 2000 W/cm(2) are encountered at the base of laser diodes, and levels as high as 500 WI /cm(2) are expected in laser slabs and power amplifier tube collectors. These impressive heat flux levels frequently combine with strict operating temperature requirements to further compound the thermal control problem. Many investigators have suggested the use of diamond heat spreaders to reduce flux levels at or near to its source, and some have suggested that diamond microchannel heat sinks ultimately may play a significant role in the solution of these problems. Design engineers at Raytheon Company have investigated the application of all-diamond microchannel heat sinks to representative high heat flux problems and have found the approach promising. Diamond microchannel fabrication feasibility has been demonstrated; integration into packaging systems and the accompanying material compatibility issues have been addressed; and thermal and hydrodynamic performance predictions have been made for selected, possible applications. An example of a practical, all diamond microchannel heat sink has been fabricated, and another is in process and will be performance tested. The heat sink assembly is made entirely of optical quality, CVD diamond and is of sufficient strength to withstand the thermal and pressure-induced mechanical loads associated with manufacture and use in tactical weapons environment. The work presented describes the development program's accomplishments to date, and highlights many of the areas for future study.

  11. Quantitative method for measuring heat flux emitted from a cryogenic object

    DOEpatents

    Duncan, Robert V.

    1993-01-01

    The present invention is a quantitative method for measuring the total heat flux, and of deriving the total power dissipation, of a heat-fluxing object which includes the steps of placing an electrical noise-emitting heat-fluxing object in a liquid helium bath and measuring the superfluid transition temperature of the bath. The temperature of the liquid helium bath is thereafter reduced until some measurable parameter, such as the electrical noise, exhibited by the heat-fluxing object or a temperature-dependent resistive thin film in intimate contact with the heat-fluxing object, becomes greatly reduced. The temperature of the liquid helum bath is measured at this point. The difference between the superfluid transition temperature of the liquid helium bath surrounding the heat-fluxing object, and the temperature of the liquid helium bath when the electrical noise emitted by the heat-fluxing object becomes greatly reduced, is determined. The total heat flux from the heat-fluxing object is determined as a function of this difference between these temperatures. In certain applications, the technique can be used to optimize thermal design parameters of cryogenic electronics, for example, Josephson junction and infra-red sensing devices.

  12. Quantitative method for measuring heat flux emitted from a cryogenic object

    DOEpatents

    Duncan, R.V.

    1993-03-16

    The present invention is a quantitative method for measuring the total heat flux, and of deriving the total power dissipation, of a heat-fluxing object which includes the steps of placing an electrical noise-emitting heat-fluxing object in a liquid helium bath and measuring the superfluid transition temperature of the bath. The temperature of the liquid helium bath is thereafter reduced until some measurable parameter, such as the electrical noise, exhibited by the heat-fluxing object or a temperature-dependent resistive thin film in intimate contact with the heat-fluxing object, becomes greatly reduced. The temperature of the liquid helum bath is measured at this point. The difference between the superfluid transition temperature of the liquid helium bath surrounding the heat-fluxing object, and the temperature of the liquid helium bath when the electrical noise emitted by the heat-fluxing object becomes greatly reduced, is determined. The total heat flux from the heat-fluxing object is determined as a function of this difference between these temperatures. In certain applications, the technique can be used to optimize thermal design parameters of cryogenic electronics, for example, Josephson junction and infrared sensing devices.

  13. Tropical Gravity Wave Momentum Fluxes and Latent Heating Distributions

    NASA Technical Reports Server (NTRS)

    Geller, Marvin A.; Zhou, Tiehan; Love, Peter T.

    2015-01-01

    Recent satellite determinations of global distributions of absolute gravity wave (GW) momentum fluxes in the lower stratosphere show maxima over the summer subtropical continents and little evidence of GW momentum fluxes associated with the intertropical convergence zone (ITCZ). This seems to be at odds with parameterizations forGWmomentum fluxes, where the source is a function of latent heating rates, which are largest in the region of the ITCZ in terms of monthly averages. The authors have examined global distributions of atmospheric latent heating, cloud-top-pressure altitudes, and lower-stratosphere absolute GW momentum fluxes and have found that monthly averages of the lower-stratosphere GW momentum fluxes more closely resemble the monthly mean cloud-top altitudes rather than the monthly mean rates of latent heating. These regions of highest cloud-top altitudes occur when rates of latent heating are largest on the time scale of cloud growth. This, plus previously published studies, suggests that convective sources for stratospheric GW momentum fluxes, being a function of the rate of latent heating, will require either a climate model to correctly model this rate of latent heating or some ad hoc adjustments to account for shortcomings in a climate model's land-sea differences in convective latent heating.

  14. Local Heat Flux Measurements with Single and Small Multi-element Coaxial Element-Injectors

    NASA Technical Reports Server (NTRS)

    Jones, Gregg; Protz, Christopher; Bullard, Brad; Hulka, James

    2006-01-01

    To support NASA's Vision for Space Exploration mission, the NASA Marshall Space Flight Center conducted a program in 2005 to improve the capability to predict local thermal compatibility and heat transfer in liquid propellant rocket engine combustion devices. The ultimate objective was to predict and hence reduce the local peak heat flux due to injector design, resulting in a significant improvement in overall engine reliability and durability. Such analyses are applicable to combustion devices in booster, upper stage, and in-space engines with regeneratively cooled chamber walls, as well as in small thrust chambers with few elements in the injector. In this program, single and three-element injectors were hot-fire tested with liquid oxygen and gaseous hydrogen propellants at The Pennsylvania State University Cryogenic Combustor Laboratory from May to August 2005. Local heat fluxes were measured in a 1-inch internal diameter heat sink combustion chamber using Medtherm coaxial thermocouples and Gardon heat flux gauges, Injector configurations were tested with both shear coaxial elements and swirl coaxial elements. Both a straight and a scarfed single element swirl injector were tested. This paper includes general descriptions of the experimental hardware, instrumentation, and results of the hot-fire testing for three coaxial shear and swirl elements. Detailed geometry and test results the for shear coax elements has already been published. Detailed test result for the remaining 6 swirl coax element for the will be published in a future JANNAF presentation to provide well-defined data sets for development and model validation.

  15. Turbulent flame-wall interaction: a DNS study

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

    Chen, Jackie; Hawkes, Evatt R; Sankaran, Ramanan

    2010-01-01

    A turbulent flame-wall interaction (FWI) configuration is studied using three-dimensional direct numerical simulation (DNS) and detailed chemical kinetics. The simulations are used to investigate the effects of the wall turbulent boundary layer (i) on the structure of a hydrogen-air premixed flame, (ii) on its near-wall propagation characteristics and (iii) on the spatial and temporal patterns of the convective wall heat flux. Results show that the local flame thickness and propagation speed vary between the core flow and the boundary layer, resulting in a regime change from flamelet near the channel centreline to a thickened flame at the wall. This findingmore » has strong implications for the modelling of turbulent combustion using Reynolds-averaged Navier-Stokes or large-eddy simulation techniques. Moreover, the DNS results suggest that the near-wall coherent turbulent structures play an important role on the convective wall heat transfer by pushing the hot reactive zone towards the cold solid surface. At the wall, exothermic radical recombination reactions become important, and are responsible for approximately 70% of the overall heat release rate at the wall. Spectral analysis of the convective wall heat flux provides an unambiguous picture of its spatial and temporal patterns, previously unobserved, that is directly related to the spatial and temporal characteristic scalings of the coherent near-wall turbulent structures.« less

  16. Evaluation of bulk heat fluxes from atmospheric datasets

    NASA Astrophysics Data System (ADS)

    Farmer, Benton

    Heat fluxes at the air-sea interface are an important component of the Earth's heat budget. In addition, they are an integral factor in determining the sea surface temperature (SST) evolution of the oceans. Different representations of these fluxes are used in both the atmospheric and oceanic communities for the purpose of heat budget studies and, in particular, for forcing oceanic models. It is currently difficult to quantify the potential impact varying heat flux representations have on the ocean response. In this study, a diagnostic tool is presented that allows for a straightforward comparison of surface heat flux formulations and atmospheric data sets. Two variables, relaxation time (RT) and the apparent temperature (T*), are derived from the linearization of the bulk formulas. They are then calculated to compare three bulk formulae and five atmospheric datasets. Additionally, the linearization is expanded to the second order to compare the amount of residual flux present. It is found that the use of a bulk formula employing a constant heat transfer coefficient produces longer relaxation times and contains a greater amount of residual flux in the higher order terms of the linearization. Depending on the temperature difference, the residual flux remaining in the second order and above terms can reach as much as 40--50% of the total residual on a monthly time scale. This is certainly a non-negligible residual flux. In contrast, a bulk formula using a stability and wind dependent transfer coefficient retains much of the total flux in the first order term, as only a few percent remain in the residual flux. Most of the difference displayed among the bulk formulas stems from the sensitivity to wind speed and the choice of a constant or spatially varying transfer coefficient. Comparing the representation of RT and T* provides insight into the differences among various atmospheric datasets. In particular, the representations of the western boundary current, upwelling

  17. A new heat flux model for the Antarctic Peninsula incorporating spatially variable upper crustal radiogenic heat production

    NASA Astrophysics Data System (ADS)

    Burton-Johnson, A.; Halpin, J. A.; Whittaker, J. M.; Graham, F. S.; Watson, S. J.

    2017-06-01

    A new method for modeling heat flux shows that the upper crust contributes up to 70% of the Antarctic Peninsula's subglacial heat flux and that heat flux values are more variable at smaller spatial resolutions than geophysical methods can resolve. Results indicate a higher heat flux on the east and south of the Peninsula (mean 81 mW m-2) where silicic rocks predominate, than on the west and north (mean 67 mW m-2) where volcanic arc and quartzose sediments are dominant. While the data supports the contribution of heat-producing element-enriched granitic rocks to high heat flux values, sedimentary rocks can be of comparative importance dependent on their provenance and petrography. Models of subglacial heat flux must utilize a heterogeneous upper crust with variable radioactive heat production if they are to accurately predict basal conditions of the ice sheet. Our new methodology and data set facilitate improved numerical model simulations of ice sheet dynamics.Plain Language SummaryAs the climate changes, the Antarctic ice sheet represents the single largest potential source of sea level rise. However, one key parameter controlling how the ice sheet flows remains poorly constrained: the effect of <span class="hlt">heat</span> derived from the Earth's geology on the base of the ice sheet (known as subglacial <span class="hlt">heat</span> <span class="hlt">flux</span>). Although this may not seem like a lot of <span class="hlt">heat</span>, under slow-flowing ice, this "<span class="hlt">heat</span> <span class="hlt">flux</span>" can control how well the ice sheet can flow over the rocks and even lead to melting of the ice at its base. Current models for Antarctica's <span class="hlt">heat</span> <span class="hlt">flux</span> use geophysics to determine how thin the crust is and consequently how easily <span class="hlt">heat</span> from the Earth's mantle can warm the surface. We show here that <span class="hlt">heat</span> produced by radioactive decay within the Earth's crust can have an even greater and much more variable contribution to the subglacial <span class="hlt">heat</span> <span class="hlt">flux</span> than estimated by these previous models. We present a new methodology allowing this crustal <span class="hlt">heat</span></p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20000003033','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20000003033"><span>Numerical Analysis of a Radiant <span class="hlt">Heat</span> <span class="hlt">Flux</span> Calibration System</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Jiang, Shanjuan; Horn, Thomas J.; Dhir, V. K.</p> <p>1998-01-01</p> <p>A radiant <span class="hlt">heat</span> <span class="hlt">flux</span> gage calibration system exists in the Flight Loads Laboratory at NASA's Dryden Flight Research Center. This calibration system must be well understood if the <span class="hlt">heat</span> <span class="hlt">flux</span> gages calibrated in it are to provide useful data during radiant <span class="hlt">heating</span> ground tests or flight tests of high speed aerospace vehicles. A part of the calibration system characterization process is to develop a numerical model of the flat plate heater element and <span class="hlt">heat</span> <span class="hlt">flux</span> gage, which will help identify errors due to convection, heater element erosion, and other factors. A 2-dimensional mathematical model of the gage-plate system has been developed to simulate the combined problem involving convection, radiation and mass loss by chemical reaction. A fourth order finite difference scheme is used to solve the steady state governing equations and determine the temperature distribution in the gage and plate, incident <span class="hlt">heat</span> <span class="hlt">flux</span> on the gage face, and flat plate erosion. Initial gage <span class="hlt">heat</span> <span class="hlt">flux</span> predictions from the model are found to be within 17% of experimental results.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/963766','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/963766"><span>QUANTIFICATION OF <span class="hlt">HEAT</span> <span class="hlt">FLUX</span> FROM A REACTING THERMITE SPRAY</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>Eric Nixon; Michelle Pantoya</p> <p>2009-07-01</p> <p>Characterizing the combustion behaviors of energetic materials requires diagnostic tools that are often not readily or commercially available. For example, a jet of thermite spray provides a high temperature and pressure reaction that can also be highly corrosive and promote undesirable conditions for the survivability of any sensor. Developing a diagnostic to quantify <span class="hlt">heat</span> <span class="hlt">flux</span> from a thermite spray is the objective of this study. Quick response sensors such as thin film <span class="hlt">heat</span> <span class="hlt">flux</span> sensors can not survive the harsh conditions of the spray, but more rugged sensors lack the response time for the resolution desired. A sensor that willmore » allow for adequate response time while surviving the entire test duration was constructed. The sensor outputs interior temperatures of the probes at known locations and utilizes an inverse <span class="hlt">heat</span> conduction code to calculate <span class="hlt">heat</span> <span class="hlt">flux</span> values. The details of this device are discussed and illustrated. Temperature and <span class="hlt">heat</span> <span class="hlt">flux</span> measurements of various thermite spray conditions are reported. Results indicate that this newly developed energetic material <span class="hlt">heat</span> <span class="hlt">flux</span> sensor provides quantitative data with good repeatability.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1985tehs.nasa...51A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1985tehs.nasa...51A"><span>Development of <span class="hlt">heat</span> <span class="hlt">flux</span> sensors for turbine airfoils</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Atkinson, William H.; Cyr, Marcia A.; Strange, Richard R.</p> <p>1985-10-01</p> <p>The objectives of this program are to develop <span class="hlt">heat</span> <span class="hlt">flux</span> sensors suitable for installation in hot section airfoils of advanced aircraft turbine engines and to experimentally verify the operation of these <span class="hlt">heat</span> <span class="hlt">flux</span> sensors in a cylinder in a cross flow experiment. Embedded thermocouple and Gardon gauge sensors were developed and fabricated into both blades and vanes. These were then calibrated using a quartz lamp bank <span class="hlt">heat</span> source and finally subjected to thermal cycle and thermal soak testing. These sensors were also fabricated into cylindrical test pieces and tested in a burner exhaust to verify <span class="hlt">heat</span> <span class="hlt">flux</span> measurements produced by these sensors. The results of the cylinder in cross flow tests 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_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('http://hdl.handle.net/2060/19880001761','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19880001761"><span>Development of <span class="hlt">heat</span> <span class="hlt">flux</span> sensors for turbine airfoils</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Atkinson, William H.; Cyr, Marcia A.; Strange, Richard R.</p> <p>1985-01-01</p> <p>The objectives of this program are to develop <span class="hlt">heat</span> <span class="hlt">flux</span> sensors suitable for installation in hot section airfoils of advanced aircraft turbine engines and to experimentally verify the operation of these <span class="hlt">heat</span> <span class="hlt">flux</span> sensors in a cylinder in a cross flow experiment. Embedded thermocouple and Gardon gauge sensors were developed and fabricated into both blades and vanes. These were then calibrated using a quartz lamp bank <span class="hlt">heat</span> source and finally subjected to thermal cycle and thermal soak testing. These sensors were also fabricated into cylindrical test pieces and tested in a burner exhaust to verify <span class="hlt">heat</span> <span class="hlt">flux</span> measurements produced by these sensors. The results of the cylinder in cross flow tests are given.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1994usee.work..203D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1994usee.work..203D"><span>Measurement of a surface <span class="hlt">heat</span> <span class="hlt">flux</span> and temperature</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Davis, R. M.; Antoine, G. J.; Diller, T. E.; Wicks, A. L.</p> <p>1994-04-01</p> <p>The <span class="hlt">Heat</span> <span class="hlt">Flux</span> Microsensor is a new sensor which was recently patented by Virginia Tech and is just starting to be marketed by Vatell Corp. The sensor is made using the thin-film microfabrication techniques directly on the material that is to be measured. It consists of several thin-film layers forming a differential thermopile across a thermal resistance layer. The measured <span class="hlt">heat</span> <span class="hlt">flux</span> q is proportional to the temperature difference across the resistance layer q= k(sub g)/delta(sub g) x (t(sub 1) - T(sub 2)), where k(sub g) is the thermal conductivity and delta (sub g) is the thickness of the thermal resistance layer. Because the gages are sputter coated directly onto the surface, their total thickness is less than 2 micrometers, which is two orders of magnitude thinner than previous gages. The resulting temperature difference across the thermal resistance layer (delta is less than 1 micrometer) is very small even at high <span class="hlt">heat</span> <span class="hlt">fluxes</span>. To generate a measurable signal many thermocouple pairs are put in series to form a differential thermopile. The combination of series thermocouple junctions and thin-film design creates a gage with very attractive characteristics. It is not only physically non-intrusive to the flow, but also causes minimal disruption of the surface temperature. Because it is so thin, the response time is less than 20 microsec. Consequently, the frequency response is flat from 0 to over 50 kHz. Moreover, the signal of the <span class="hlt">Heat</span> <span class="hlt">Flux</span> Microsensor is directly proportional to the <span class="hlt">heat</span> <span class="hlt">flux</span>. Therefore, it can easily be used in both steady and transient flows, and it measures both the steady and unsteady components of the surface <span class="hlt">heat</span> <span class="hlt">flux</span>. A version of the <span class="hlt">Heat</span> <span class="hlt">Flux</span> Microsensor has been developed to meet the harsh demands of combustion environments. These gages use platinum and platinum-10 percent rhodium as the thermoelectric materials. The thermal resistance layer is silicon monoxide and a protective coating of Al2O3 is deposited on top of the sensor. The</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19940031900','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19940031900"><span>Measurement of a surface <span class="hlt">heat</span> <span class="hlt">flux</span> and temperature</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Davis, R. M.; Antoine, G. J.; Diller, T. E.; Wicks, A. L.</p> <p>1994-01-01</p> <p>The <span class="hlt">Heat</span> <span class="hlt">Flux</span> Microsensor is a new sensor which was recently patented by Virginia Tech and is just starting to be marketed by Vatell Corp. The sensor is made using the thin-film microfabrication techniques directly on the material that is to be measured. It consists of several thin-film layers forming a differential thermopile across a thermal resistance layer. The measured <span class="hlt">heat</span> <span class="hlt">flux</span> q is proportional to the temperature difference across the resistance layer q= k(sub g)/delta(sub g) x (t(sub 1) - T(sub 2)), where k(sub g) is the thermal conductivity and delta (sub g) is the thickness of the thermal resistance layer. Because the gages are sputter coated directly onto the surface, their total thickness is less than 2 micrometers, which is two orders of magnitude thinner than previous gages. The resulting temperature difference across the thermal resistance layer (delta is less than 1 micrometer) is very small even at high <span class="hlt">heat</span> <span class="hlt">fluxes</span>. To generate a measurable signal many thermocouple pairs are put in series to form a differential thermopile. The combination of series thermocouple junctions and thin-film design creates a gage with very attractive characteristics. It is not only physically non-intrusive to the flow, but also causes minimal disruption of the surface temperature. Because it is so thin, the response time is less than 20 microsec. Consequently, the frequency response is flat from 0 to over 50 kHz. Moreover, the signal of the <span class="hlt">Heat</span> <span class="hlt">Flux</span> Microsensor is directly proportional to the <span class="hlt">heat</span> <span class="hlt">flux</span>. Therefore, it can easily be used in both steady and transient flows, and it measures both the steady and unsteady components of the surface <span class="hlt">heat</span> <span class="hlt">flux</span>. A version of the <span class="hlt">Heat</span> <span class="hlt">Flux</span> Microsensor has been developed to meet the harsh demands of combustion environments. These gages use platinum and platinum-10 percent rhodium as the thermoelectric materials. The thermal resistance layer is silicon monoxide and a protective coating of Al2O3 is deposited on top of the sensor. The</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19940024321','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19940024321"><span><span class="hlt">Heat</span> <span class="hlt">flux</span> instrumentation for Hyflite thermal protection system</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Diller, T. E.</p> <p>1994-01-01</p> <p>Using Thermal Protection Tile core samples supplied by NASA, the surface characteristics of the FRCI, TUFI, and RCG coatings were evaluated. Based on these results, appropriate methods of surface preparation were determined and tested for the required sputtering processes. Sample sensors were fabricated on the RCG coating and adhesion was acceptable. Based on these encouraging results, complete <span class="hlt">Heat</span> <span class="hlt">Flux</span> Microsensors were fabricated on the RCG coating. The issue of lead attachment was addressed with the annnealing and welding methods developed at NASA Lewis. Parallel gap welding appears to be the best method of lead attachment with prior <span class="hlt">heat</span> treatment of the sputtered pads. Sample <span class="hlt">Heat</span> <span class="hlt">Flux</span> Microsensors were submitted for testing in the NASA Ames arc jet facility. Details of the project are contained in two attached reports. One additional item of interest is contained in the attached AIAA paper, which gives details of the transient response of a <span class="hlt">Heat</span> <span class="hlt">Flux</span> Microsensors in a shock tube facility at Virginia Tech. The response of the <span class="hlt">heat</span> <span class="hlt">flux</span> sensor was measured to be faster than 10 micro-s.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19930064218&hterms=engine+step+step&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Dengine%2Bstep%2Bstep','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19930064218&hterms=engine+step+step&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Dengine%2Bstep%2Bstep"><span>Comparison of liquid rocket engine base region <span class="hlt">heat</span> <span class="hlt">flux</span> computations using three turbulence models</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Kumar, Ganesh N.; Griffith, Dwaine O., II; Prendergast, Maurice J.; Seaford, C. M.</p> <p>1993-01-01</p> <p>The flow in the base region of launch vehicles is characterized by flow separation, flow reversals, and reattachment. Computation of the convective <span class="hlt">heat</span> <span class="hlt">flux</span> in the base region and on the nozzle external surface of Space Shuttle Main Engine and Space Transportation Main Engine (STME) is an important part of defining base region thermal environments. Several turbulence models were incorporated in a CFD code and validated for flow and <span class="hlt">heat</span> transfer computations in the separated and reattaching regions associated with subsonic and supersonic flows over backward facing steps. <span class="hlt">Heat</span> <span class="hlt">flux</span> computations in the base region of a single STME engine and a single S1C engine were performed using three different <span class="hlt">wall</span> functions as well as a renormalization-group based k-epsilon model. With the very limited data available, the computed values are seen to be of the right order of magnitude. Based on the validation comparisons, it is concluded that all the turbulence models studied have predicted the reattachment location and the velocity profiles at various axial stations downstream of the step very well.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/865563','DOE-PATENT-XML'); return false;" href="https://www.osti.gov/servlets/purl/865563"><span><span class="hlt">Heat</span> <span class="hlt">flux</span> limiting sleeves</span></a></p> <p><a target="_blank" href="http://www.osti.gov/doepatents">DOEpatents</a></p> <p>Harris, William G.</p> <p>1985-01-01</p> <p>A <span class="hlt">heat</span> limiting tubular sleeve extending over only a portion of a tube having a generally uniform outside diameter, the sleeve being open on both ends, having one end thereof larger in diameter than the other end thereof and having a <span class="hlt">wall</span> thickness which decreases in the same direction as the diameter of the sleeve decreases so that the <span class="hlt">heat</span> transfer through the sleeve and tube is less adjacent the large diameter end of the sleeve than adjacent the other end thereof.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/5275074','DOE-PATENT-XML'); return false;" href="https://www.osti.gov/biblio/5275074"><span>Remote high-temperature insulatorless <span class="hlt">heat-flux</span> gauge</span></a></p> <p><a target="_blank" href="http://www.osti.gov/doepatents">DOEpatents</a></p> <p>Noel, B.W.</p> <p>1993-12-28</p> <p>A remote optical <span class="hlt">heat-flux</span> gauge for use in extremely high temperature environments is described. This application is possible because of the use of thermographic phosphors as the sensing media, and the omission of the need for an intervening layer of insulator between phosphor layers. The gauge has no electrical leads, but is interrogated with ultraviolet or laser light. The luminescence emitted by the two phosphor layers, which is indicative of the temperature of the layers, is collected and analyzed in order to determine the <span class="hlt">heat</span> <span class="hlt">flux</span> incident on the surface being investigated. The two layers of thermographic phosphor must be of different materials to assure that the spectral lines collected will be distinguishable. Spatial <span class="hlt">heat-flux</span> measurements can be made by scanning the light across the surface of the gauge. 3 figures.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/869091','DOE-PATENT-XML'); return false;" href="https://www.osti.gov/servlets/purl/869091"><span>Remote high-temperature insulatorless <span class="hlt">heat-flux</span> gauge</span></a></p> <p><a target="_blank" href="http://www.osti.gov/doepatents">DOEpatents</a></p> <p>Noel, Bruce W.</p> <p>1993-01-01</p> <p>A remote optical <span class="hlt">heat-flux</span> gauge for use in extremely high temperature environments is described. This application is possible because of the use of thermographic phosphors as the sensing media, and the omission of the need for an intervening layer of insulator between phosphor layers. The gauge has no electrical leads, but is interrogated with ultraviolet or laser light. The luminescence emitted by the two phosphor layers, which is indicative of the temperature of the layers, is collected and analyzed in order to determine the <span class="hlt">heat</span> <span class="hlt">flux</span> incident on the surface being investigated. The two layers of thermographic phosphor must be of different materials to assure that the spectral lines collected will be distinguishable. Spatial <span class="hlt">heat-flux</span> measurements can be made by scanning the light across the surface of the gauge.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..19.2080D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..19.2080D"><span>Wind stress and <span class="hlt">heat</span> <span class="hlt">fluxes</span> over a Brazilian Coastal Upwelling</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Dourado, Marcelo; Candella, Rogério</p> <p>2017-04-01</p> <p>Coastal upwelling zones have been intensively studied in the last decades especially due to their importance to the biological cycle. The coastal upwelling system of the Cabo Frio region (east coast of the Rio de Janeiro state, Brazil) keeps the surface water cold during most part of the year, what induces a stable atmospheric boundary layer associated to northeast winds. The main goal of this study is to investigate the wind stress and <span class="hlt">heat</span> <span class="hlt">fluxes</span> exchanges between the ocean and the atmosphere in that area. For this purpose, a set of hourly data meteorological and oceanographic data collected by a Wavescan metocean buoy anchored at 23o59S; 42oW, were used, as well as solar radiation and relative humidity from a terrestrial meteorological station from the Instituto Nacional de Meteorologia (InMet). COARE 3.0 algorithm was used to calculate the latent and sensible <span class="hlt">heat</span> <span class="hlt">fluxes</span>. In this discussion, positive values represent <span class="hlt">fluxes</span> towards the ocean. The average net <span class="hlt">heat</span> <span class="hlt">flux</span> over our study period is 88 W m-2. The reduction of the net <span class="hlt">heat</span> <span class="hlt">flux</span> is due to the increase of the ocean latent <span class="hlt">heat</span> loss, although a reduction in incoming shortwave radiation and an increase in ocean long wave cooling also contributes. The latent <span class="hlt">heat</span> is 20 times larger than the sensible <span class="hlt">heat</span> <span class="hlt">flux</span>, but the mean value of the latent <span class="hlt">heat</span> <span class="hlt">flux</span>, 62 W m-2, is half the typical value found in open ocean. The temporal variability of both sensible and latent <span class="hlt">heat</span> <span class="hlt">fluxes</span> reflects their dependence on wind speed and air-sea temperature differences. When upwelling events, here periods when diurnal SST is lower than 18oC, are compared with undisturbed (without upwelling) events, it can be noted the sensible <span class="hlt">heat</span> <span class="hlt">fluxes</span> are positives and 10 times greater in magnitude. This is related to an increment, during these upwelling events, of the air-sea temperature difference and an increasing of the wind speed. The cold waters of the upwelling increase the air-sea temperature gradient and, also, the horizontal land</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19950037243&hterms=impact+art&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Dimpact%2Bart','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19950037243&hterms=impact+art&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Dimpact%2Bart"><span>The impact of land-surface wetness heterogeneity on mesoscale <span class="hlt">heat</span> <span class="hlt">fluxes</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Chen, Fei; Avissar, Roni</p> <p>1994-01-01</p> <p>Vertical <span class="hlt">heat</span> <span class="hlt">fluxes</span> associated with mesoscale circulations generated by land-surface wetness discontinuities are often stronger than turbulent <span class="hlt">fluxes</span>, especially in the upper part of the atmospheric planetary boundary layer. As a result, they contribute significantly to the subgrid-scale <span class="hlt">fluxes</span> in large-scale atmospheric models. Yet they are not considered in these models. To provide some insights into the possible parameterization of these <span class="hlt">fluxes</span> in large-scale models, a state-of-the-art mesoscale numerical model was used to investigate the relationships between mesoscale <span class="hlt">heat</span> <span class="hlt">fluxes</span> and atmospheric and land-surface characteristics that play a key role in the generation of mesoscale circulations. The distribution of land-surface wetness, the wavenumber and the wavelength of the land-surface discontinuities, and the large-scale wind speed have a significant impact on the mesoscale <span class="hlt">heat</span> <span class="hlt">fluxes</span>. Empirical functions were derived to characterize the relationships between mesoscale <span class="hlt">heat</span> <span class="hlt">fluxes</span> and the spatial distribution of land-surface wetness. The strongest mesoscale <span class="hlt">heat</span> <span class="hlt">fluxes</span> were obtained for a wavelength of forcing corresponding approximately to the local Rossby deformation radius. The mesoscale <span class="hlt">heat</span> <span class="hlt">fluxes</span> are weakened by large-scale background winds but remain significant even with moderate winds.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017E%26ES...60a2028I','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017E%26ES...60a2028I"><span><span class="hlt">Heat</span> transfer characteristics of building <span class="hlt">walls</span> using phase change material</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Irsyad, M.; Pasek, A. D.; Indartono, Y. S.; Pratomo, A. W.</p> <p>2017-03-01</p> <p>Minimizing energy consumption in air conditioning system can be done with reducing the cooling load in a room. <span class="hlt">Heat</span> from solar radiation which passes through the <span class="hlt">wall</span> increases the cooling load. Utilization of phase change material on <span class="hlt">walls</span> is expected to decrease the <span class="hlt">heat</span> rate by storing energy when the phase change process takes place. The stored energy is released when the ambient temperature is low. Temperature differences at noon and evening can be utilized as discharging and charging cycles. This study examines the characteristics of <span class="hlt">heat</span> transfer in <span class="hlt">walls</span> using phase change material (PCM) in the form of encapsulation and using the sleeve as well. <span class="hlt">Heat</span> transfer of bricks containing encapsulated PCM, tested the storage and released the <span class="hlt">heat</span> on the <span class="hlt">walls</span> of the building models were evaluated in this study. Experiments of <span class="hlt">heat</span> transfer on brick consist of time that is needed for <span class="hlt">heat</span> transfer and thermal conductivity test as well. Experiments were conducted on a <span class="hlt">wall</span> coated by PCM which was exposed on a day and night cycle to analyze the <span class="hlt">heat</span> storage and <span class="hlt">heat</span> release. PCM used in these experiments was coconut oil. The measured parameter is the temperature at some points in the brick, <span class="hlt">walls</span> and ambient temperature as well. The results showed that the use of encapsulation on an empty brick can increase the time for thermal <span class="hlt">heat</span> transfer. Thermal conductivity values of a brick containing encapsulated PCM was lower than hollow bricks, where each value was 1.3 W/m.K and 1.6 W/m.K. While the process of <span class="hlt">heat</span> absorption takes place from 7:00 am to 06:00 pm, and the release of <span class="hlt">heat</span> runs from 10:00 pm to 7:00 am. The use of this PCM layer can reduce the surface temperature of the <span class="hlt">walls</span> of an average of 2°C and slows the <span class="hlt">heat</span> into the room.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMGC24C..04C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMGC24C..04C"><span>Improving Global Net Surface <span class="hlt">Heat</span> <span class="hlt">Flux</span> with Ocean Reanalysis</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Carton, J.; Chepurin, G. A.; Chen, L.; Grodsky, S.</p> <p>2017-12-01</p> <p>This project addresses the current level of uncertainty in surface <span class="hlt">heat</span> <span class="hlt">flux</span> estimates. Time mean surface <span class="hlt">heat</span> <span class="hlt">flux</span> estimates provided by atmospheric reanalyses differ by 10-30W/m2. They are generally unbalanced globally, and have been shown by ocean simulation studies to be incompatible with ocean temperature and velocity measurements. Here a method is presented 1) to identify the spatial and temporal structure of the underlying errors and 2) to reduce them by exploiting hydrographic observations and the analysis increments produced by an ocean reanalysis using sequential data assimilation. The method is applied to <span class="hlt">fluxes</span> computed from daily state variables obtained from three widely used reanalyses: MERRA2, ERA-Interim, and JRA-55, during an eight year period 2007-2014. For each of these seasonal <span class="hlt">heat</span> <span class="hlt">flux</span> errors/corrections are obtained. In a second set of experiments the <span class="hlt">heat</span> <span class="hlt">fluxes</span> are corrected and the ocean reanalysis experiments are repeated. This second round of experiments shows that the time mean error in the corrected <span class="hlt">fluxes</span> is reduced to within ±5W/m2 over the interior subtropical and midlatitude oceans, with the most significant changes occuring over the Southern Ocean. The global <span class="hlt">heat</span> <span class="hlt">flux</span> imbalance of each reanalysis is reduced to within a few W/m2 with this single correction. Encouragingly, the corrected forms of the three sets of <span class="hlt">fluxes</span> are also shown to converge. In the final discussion we present experiments beginning with a modified form of the ERA-Int reanalysis, produced by the DAKKAR program, in which state variables have been individually corrected based on independent measurements. Finally, we discuss the separation of <span class="hlt">flux</span> error from model error.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009PhDT........56V','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009PhDT........56V"><span>Modeling of a <span class="hlt">heat</span> sink and high <span class="hlt">heat</span> <span class="hlt">flux</span> vapor chamber</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Vadnjal, Aleksander</p> <p></p> <p>An increasing demand for a higher <span class="hlt">heat</span> <span class="hlt">flux</span> removal capability within a smaller volume for high power electronics led us to focus on a novel cold plate design. A high <span class="hlt">heat</span> <span class="hlt">flux</span> evaporator and micro channel <span class="hlt">heat</span> sink are the main components of a cold plate which is capable of removing couple of 100 W/cm2. In order to describe performance of such porous media device a proper modeling has to be addressed. A universal approach based on the volume average theory (VAT) to transport phenomena in porous media is shown. An approach on how to treat the closure for momentum and energy equations is addressed and a proper definition for friction factors and <span class="hlt">heat</span> transfer coefficients are discussed. A numerical scheme using a solution to Navier-Stokes equations over a representative elementary volume (REV) and the use of VAT is developed to show how to compute friction factors and <span class="hlt">heat</span> transfer coefficients. The calculation show good agreement with the experimental data. For the <span class="hlt">heat</span> transfer coefficient closure, a proper average for both fluid and solid is investigated. Different types of <span class="hlt">heating</span> are also investigated in order to determine how it influences the <span class="hlt">heat</span> transfer coefficient. A higher <span class="hlt">heat</span> <span class="hlt">fluxes</span> in small area condensers led us to the micro channels in contrast to the classical <span class="hlt">heat</span> fin design. A micro channel can have various shapes to enhance <span class="hlt">heat</span> transfer, but the shape that will lead to a higher <span class="hlt">heat</span> <span class="hlt">flux</span> removal with a moderate pumping power needs to be determined. The standard micro-channel terminology is usually used for channels with a simple cross section, e.g. square, round, triangle, etc., but here the micro channel cross section is going to be expanded to describe more complicated and interconnected micro scale channel cross sections. The micro channel geometries explored are pin fins (in-line and staggered) and sintered porous micro channels. The problem solved here is a conjugate problem involving two <span class="hlt">heat</span> transfer mechanisms; (1) porous media</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/1131309-diagnostic-quantifying-heat-flux-from-thermite-spray','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/1131309-diagnostic-quantifying-heat-flux-from-thermite-spray"><span>A diagnostic for quantifying <span class="hlt">heat</span> <span class="hlt">flux</span> from a thermite spray</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>E. P. Nixon; M. L. Pantoya; D. J. Prentice</p> <p>2010-02-01</p> <p>Characterizing the combustion behaviors of energetic materials requires diagnostic tools that are often not readily or commercially available. For example, a jet of thermite spray provides a high temperature and pressure reaction that can also be highly corrosive and promote undesirable conditions for the survivability of any sensor. Developing a diagnostic to quantify <span class="hlt">heat</span> <span class="hlt">flux</span> from a thermite spray is the objective of this study. Quick response sensors such as thin film <span class="hlt">heat</span> <span class="hlt">flux</span> sensors cannot survive the harsh conditions of the spray, but more rugged sensors lack the response time for the resolution desired. A sensor that will allowmore » for adequate response time while surviving the entire test duration was constructed. The sensor outputs interior temperatures of the probes at known locations and utilizes an inverse <span class="hlt">heat</span> conduction code to calculate <span class="hlt">heat</span> <span class="hlt">flux</span> values. The details of this device are discussed and illustrated. Temperature and <span class="hlt">heat</span> <span class="hlt">flux</span> measurements of various thermite sprays are reported. Results indicate that this newly designed <span class="hlt">heat</span> <span class="hlt">flux</span> sensor provides quantitative data with good repeatability suitable for characterizing energetic material combustion.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19910015008','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19910015008"><span>Calibrator tests of <span class="hlt">heat</span> <span class="hlt">flux</span> gauges mounted in SSME blades</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Liebert, Curt H.</p> <p>1989-01-01</p> <p>Measurements of <span class="hlt">heat</span> <span class="hlt">flux</span> to space shuttle main engine (SSME) turbine blade surfaces are being made in the Lewis <span class="hlt">heat</span> <span class="hlt">flux</span> calibration facility. Surface <span class="hlt">heat</span> <span class="hlt">flux</span> information is obtained from transient temperature measurements taken at points within the gauge. A 100-kW Vortek arc lamp is used as a source of thermal radiant energy. Thermoplugs, with diameters of about 0.190 cm and lengths varying from about 0.190 to 0.320 cm, are being investigated. The thermoplug is surrounded on all surfaces except the active surface by a pocket of air located in the circular annulus and under the back cover. Since the thermoplug is insulated, it is assumed that <span class="hlt">heat</span> is conducted in a one-dimensional manner from the hot active surface to the cooler back side of the thermoplug. It is concluded that the miniature plug-type gauge concept is feasible for measurement of blade surface <span class="hlt">heat</span> <span class="hlt">flux</span>. It is suggested that it is important to measure <span class="hlt">heat</span> <span class="hlt">flux</span> near the hub on the suction surface and at the throat on SSME blades rotating in engines because stress and <span class="hlt">heat</span> transfer coefficients are high in this region.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016PhLA..380..452G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016PhLA..380..452G"><span>Understanding of <span class="hlt">flux</span>-limited behaviors of <span class="hlt">heat</span> transport in nonlinear regime</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Guo, Yangyu; Jou, David; Wang, Moran</p> <p>2016-01-01</p> <p>The classical Fourier's law of <span class="hlt">heat</span> transport breaks down in highly nonequilibrium situations as in nanoscale <span class="hlt">heat</span> transport, where nonlinear effects become important. The present work is aimed at exploring the <span class="hlt">flux</span>-limited behaviors based on a categorization of existing nonlinear <span class="hlt">heat</span> transport models in terms of their theoretical foundations. Different saturation <span class="hlt">heat</span> <span class="hlt">fluxes</span> are obtained, whereas the same qualitative variation trend of <span class="hlt">heat</span> <span class="hlt">flux</span> versus exerted temperature gradient is got in diverse nonlinear models. The phonon hydrodynamic model is proposed to act as a standard to evaluate other <span class="hlt">heat</span> <span class="hlt">flux</span> limiters because of its more rigorous physical foundation. A deeper knowledge is thus achieved about the phenomenological generalized <span class="hlt">heat</span> transport models. The present work provides deeper understanding and accurate modeling of nonlocal and nonlinear <span class="hlt">heat</span> transport beyond the diffusive limit.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19750008695','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19750008695"><span><span class="hlt">Wall</span> mounted <span class="hlt">heat</span> exchanger characterization. [cryogenic propellant tanks</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Bullard, B. R.</p> <p>1975-01-01</p> <p>Analytical models are presented for describing the <span class="hlt">heat</span> and mass transfer and the energy distribution in the contents of a cryogenic propellant tank, under varying gravity levels. These models are used to analytically evaluate the effectiveness of a <span class="hlt">wall</span> <span class="hlt">heat</span> exchanger as a means of controlling the pressure in the tank during flight and during fill operations. Pressure and temperature histories are presented for tanks varying in size from 4 to 22.5 feet in diameter and gravity levels from 0-1. Results from the subscale test program, utilizing both non-cryogenic and cryogenic fluid, designed to evaluate a tank <span class="hlt">wall</span> <span class="hlt">heat</span> exchanger are described and compared with the analytical models. Both the model and test results indicate that a passive tank <span class="hlt">wall</span> <span class="hlt">heat</span> exchanger can effectively control tank pressure. However, the weight of such a system is considerably higher than that of an active mixer system.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMGC21G1021K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMGC21G1021K"><span>Causes of Potential Urban <span class="hlt">Heat</span> Island Space Using <span class="hlt">Heat</span> <span class="hlt">flux</span> Budget Under Urban Canopy</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kwon, Y. J.; Lee, D. K.</p> <p>2017-12-01</p> <p>Raised concerns about possible contribution from urban <span class="hlt">heat</span> island to global warming is about 30 percent. Therefore, mitigating urban <span class="hlt">heat</span> island became one of major issues to solve among urban planners, urban designers, landscape architects, urban affair decision makers and etc. Urban <span class="hlt">heat</span> island effect on a micro-scale is influenced by factors such as wind, water vapor and solar radiation. Urban <span class="hlt">heat</span> island effect on a microscale is influenced by factors like wind, water vapor and solar radiation. These microscopic climates are also altered by factors affecting the <span class="hlt">heat</span> content in space, like SVF and aspect ratio depending on the structural characteristics of various urban canyon components. Indicators of <span class="hlt">heat</span> mitigation in urban design stage allows us to create a spatial structure considering the <span class="hlt">heat</span> balance budget. The spatial characteristics affect thermal change by varying <span class="hlt">heat</span> storage, emitting or absorbing the <span class="hlt">heat</span>. The research defines characteristics of the space composed of the factors affecting the <span class="hlt">heat</span> <span class="hlt">flux</span> change as the potential urban <span class="hlt">heat</span> island space. Potential urban <span class="hlt">heat</span> island spaces are that having higher <span class="hlt">heat</span> <span class="hlt">flux</span> than periphery space. The study is to know the spatial characteristics that affects the subsequent temperature rise by the <span class="hlt">heat</span> <span class="hlt">flux</span>. As a research method, four types of potential <span class="hlt">heat</span> island space regions were analyzed. I categorized the spatial types by comparing parameters' value of energy balance in day and night: 1) day severe areas, 2) day comfort areas, 3) night severe areas, 4) night comfort areas. I have looked at these four types of potential urban <span class="hlt">heat</span> island areas from a microscopic perspective and investigated how various forms of <span class="hlt">heat</span> influences on higher <span class="hlt">heat</span> <span class="hlt">flux</span> areas. This research was designed to investigate the <span class="hlt">heat</span> indicators to be reflected in the design of urban canyon for <span class="hlt">heat</span> mitigation. As a result, severe areas in daytime have high SVF rate, sensible <span class="hlt">heat</span> is generated. Day comfort areas have shadow effect</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009HMT....45..999H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009HMT....45..999H"><span>A study of nucleate boiling and critical <span class="hlt">heat</span> <span class="hlt">flux</span> with EHD enhancement</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hristov, Y.; Zhao, D.; Kenning, D. B. R.; Sefiane, K.; Karayiannis, T. G.</p> <p>2009-05-01</p> <p>The paper describes results from an experimental and theoretical study of the effect of an electric field on nucleate boiling and the critical <span class="hlt">heat</span> <span class="hlt">flux</span> (CHF) in pool boiling of R123 at atmospheric pressure on a horizontal <span class="hlt">wall</span> with a smooth surface. Two designs of electrode (parallel rods and wire mesh) were used. The experimental data exhibit some differences from the data obtained by other researchers in similar experiments on a <span class="hlt">wall</span> with a different surface finish and with a slightly different design of wire mesh electrode. The hydrodynamic model for EHD enhancement of CHF cannot reconcile the differences. A theoretical model has been developed for the growth of a single vapour bubble on a superheated <span class="hlt">wall</span> in an electric field, leading to a numerical simulation based on the level-set method. The model includes matching of sub-models for the micro- and macro-regions, conduction in the <span class="hlt">wall</span>, distortion of the electric field by the bubble, the temperature dependence of electrical properties and free-charge generation. In the present form of the model, some of these effects are realised in an approximate form. The capability to investigate dry-spot formation and <span class="hlt">wall</span> temperature changes that might lead to CHF has been demonstrated.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JPhCS.891a2223K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JPhCS.891a2223K"><span>Study on coal char ignition by radiant <span class="hlt">heat</span> <span class="hlt">flux</span>.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Korotkikh, A. G.; Slyusarskiy, K. V.</p> <p>2017-11-01</p> <p>The study on coal char ignition by CO2-continuous laser was carried out. The coal char samples of T-grade bituminous coal and 2B-grade lignite were studied via CO2-laser ignition setup. Ignition delay times were determined at ambient condition in <span class="hlt">heat</span> <span class="hlt">flux</span> density range 90-200 W/cm2. The average ignition delay time value for lignite samples were 2 times lower while this difference is larger in high <span class="hlt">heat</span> <span class="hlt">flux</span> region and lower in low <span class="hlt">heat</span> <span class="hlt">flux</span> region. The kinetic constants for overall oxidation reaction were determined using analytic solution of simplified one-dimensional <span class="hlt">heat</span> transfer equation with radiant <span class="hlt">heat</span> transfer boundary condition. The activation energy for lignite char was found to be less than it is for bituminous coal char by approximately 20 %.</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('https://www.osti.gov/pages/biblio/1185374-high-heat-flux-testing-irradiated-tungsten-based-materials-fusion-applications-using-infrared-plasma-arc-lamps','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1185374-high-heat-flux-testing-irradiated-tungsten-based-materials-fusion-applications-using-infrared-plasma-arc-lamps"><span>High-<span class="hlt">heat-flux</span> testing of irradiated tungsten-based materials for fusion applications using infrared plasma arc lamps</span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Sabau, Adrian S.; Ohriner, Evan K.; Kiggans, Jim; ...</p> <p>2014-11-01</p> <p>Testing of advanced materials and component mock-ups under prototypical fusion high-<span class="hlt">heat-flux</span> conditions, while historically a mainstay of fusion research, has proved to be quite challenging, especially for irradiated materials. A new high-<span class="hlt">heat</span>-flux–testing (HHFT) facility based on water-<span class="hlt">wall</span> plasma arc lamps (PALs) is now introduced for materials and small-component testing. Two PAL systems, utilizing a 12 000°C plasma arc contained in a quartz tube cooled by a spiral water flow over the inside tube surface, provide maximum incident <span class="hlt">heat</span> <span class="hlt">fluxes</span> of 4.2 and 27 MW/m 2 over areas of 9×12 and 1×10 cm 2, respectively. This paper will present the overallmore » design and implementation of a PAL-based irradiated material target station (IMTS). The IMTS is primarily designed for testing the effects of <span class="hlt">heat</span> <span class="hlt">flux</span> or thermal cycling on material coupons of interest, such as those for plasma-facing components. Temperature results are shown for thermal cycling under HHFT of tungsten coupon specimens that were neutron irradiated in HFIR. Finally, radiological surveys indicated minimal contamination of the 36×36×18 cm test section, demonstrating the capability of the new facility to handle irradiated specimens at high temperature.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/111419','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/111419"><span>A comparison of critical <span class="hlt">heat</span> <span class="hlt">flux</span> in tubes and bilaterally <span class="hlt">heated</span> annuli</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>Doerffer, S.; Groeneveld, D.C.; Cheng, S.C.</p> <p>1995-09-01</p> <p>This paper examines the critical <span class="hlt">heat</span> <span class="hlt">flux</span> (CHF) behaviour for annular flow in bilaterally <span class="hlt">heated</span> annuli and compares it to that in tubes and unilaterally <span class="hlt">heated</span> annuli. It was found that the differences in CHF between bilaterally and unilaterally <span class="hlt">heated</span> annuli or tubes strongly depend on pressure and quality. the CHF in bilaterally <span class="hlt">heated</span> annuli can be predicted by tube CHF prediction methods for the simultaneous CHF occurrence at both surfaces, and the following flow conditions: pressure 7-10 MPa, mass <span class="hlt">flux</span> 0.5-4.0 Mg/m{sup 2}s and critical quality 0.23-0.9. The effect on CHF of the outer-to-inner surface <span class="hlt">heat</span> <span class="hlt">flux</span> ratio, wasmore » also examined. The prediction of CHF for bilaterally <span class="hlt">heated</span> annuli was based on the droplet-diffusion model proposed by Kirillov and Smogalev. While their model refers only to CHF occurrence at the inner surface, we extended it to cases where CHF occurs at the outer surface, and simultaneously at both surfaces, thus covering all cases of CHF occurrence in bilaterally <span class="hlt">heated</span> annuli. From the annuli CHF data of Becker and Letzter, we derived empirical functions required by the model. the proposed equations provide good accuracy for the CHF data used in this study. Moreover, the equations can predict conditions at which CHF occurs simultaneously at both surfaces. Also, this method can be used for cases with only one <span class="hlt">heated</span> surface.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017PhLA..381.3621L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017PhLA..381.3621L"><span>Size effects in non-linear <span class="hlt">heat</span> conduction with <span class="hlt">flux</span>-limited behaviors</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Li, Shu-Nan; Cao, Bing-Yang</p> <p>2017-11-01</p> <p>Size effects are discussed for several non-linear <span class="hlt">heat</span> conduction models with <span class="hlt">flux</span>-limited behaviors, including the phonon hydrodynamic, Lagrange multiplier, hierarchy moment, nonlinear phonon hydrodynamic, tempered diffusion, thermon gas and generalized nonlinear models. For the phonon hydrodynamic, Lagrange multiplier and tempered diffusion models, <span class="hlt">heat</span> <span class="hlt">flux</span> will not exist in problems with sufficiently small scale. The existence of <span class="hlt">heat</span> <span class="hlt">flux</span> needs the sizes of <span class="hlt">heat</span> conduction larger than their corresponding critical sizes, which are determined by the physical properties and boundary temperatures. The critical sizes can be regarded as the theoretical limits of the applicable ranges for these non-linear <span class="hlt">heat</span> conduction models with <span class="hlt">flux</span>-limited behaviors. For sufficiently small scale <span class="hlt">heat</span> conduction, the phonon hydrodynamic and Lagrange multiplier models can also predict the theoretical possibility of violating the second law and multiplicity. Comparisons are also made between these non-Fourier models and non-linear Fourier <span class="hlt">heat</span> conduction in the type of fast diffusion, which can also predict <span class="hlt">flux</span>-limited behaviors.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013IJTP...52.3598A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013IJTP...52.3598A"><span>Gravitational Collapse with <span class="hlt">Heat</span> <span class="hlt">Flux</span> and Gravitational Waves</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ahmad, Zahid; Ahmed, Qazi Zahoor; Awan, Abdul Sami</p> <p>2013-10-01</p> <p>In this paper, we investigated the cylindrical gravitational collapse with <span class="hlt">heat</span> <span class="hlt">flux</span> by considering the appropriate geometry of the interior and exterior spacetimes. For this purpose, we matched collapsing fluid to an exterior containing gravitational waves.The effects of <span class="hlt">heat</span> <span class="hlt">flux</span> on gravitational collapse are investigated and matched with the results obtained by Herrera and Santos (Class. Quantum Gravity 22:2407, 2005).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19880003381','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19880003381"><span>Experimental study of thermocapillary flows in a thin liquid layer with <span class="hlt">heat</span> <span class="hlt">fluxes</span> imposed on the free surface</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Lai, Chun-Liang; Greenberg, Paul S.; Chai, An-Ti</p> <p>1988-01-01</p> <p>To study thermocapillary flows in a two-dimensional thin liquid layer with <span class="hlt">heat</span> <span class="hlt">fluxes</span> imposed on the free surface experimentally, a long tray configuration was employed to simulate the infinite layer. The surface temperature distribution due to thermocapillary convective for different flow regimes was measured and compared with theoretical predictions. A short tray configuration was also employed to study the end <span class="hlt">wall</span> effects (insulating or conducting). The results show that for a strong convection flow with an insulating <span class="hlt">wall</span> as the boundary the surface temperature distribution became quite uniform. Consequently, the thermocapillary driving force was greatly reduced. On the other hand, a strong fluid motion always existed adjacent to the conducting <span class="hlt">wall</span> because of the large surface temperature gradient near the <span class="hlt">wall</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22408328-magnetic-flux-heat-losses-diffusive-advective-nernst-effects-magnetized-liner-inertial-fusion-like-plasma','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22408328-magnetic-flux-heat-losses-diffusive-advective-nernst-effects-magnetized-liner-inertial-fusion-like-plasma"><span>Magnetic <span class="hlt">flux</span> and <span class="hlt">heat</span> losses by diffusive, advective, and Nernst effects in magnetized liner inertial fusion-like plasma</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>Velikovich, A. L.; Giuliani, J. L.; Zalesak, S. T.</p> <p></p> <p>The magnetized liner inertial fusion (MagLIF) approach to inertial confinement fusion [Slutz et al., Phys. Plasmas 17, 056303 (2010); Cuneo et al., IEEE Trans. Plasma Sci. 40, 3222 (2012)] involves subsonic/isobaric compression and <span class="hlt">heating</span> of a deuterium-tritium plasma with frozen-in magnetic <span class="hlt">flux</span> by a heavy cylindrical liner. The losses of <span class="hlt">heat</span> and magnetic <span class="hlt">flux</span> from the plasma to the liner are thereby determined by plasma advection and gradient-driven transport processes, such as thermal conductivity, magnetic field diffusion, and thermomagnetic effects. Theoretical analysis based on obtaining exact self-similar solutions of the classical collisional Braginskii's plasma transport equations in one dimension demonstratesmore » that the <span class="hlt">heat</span> loss from the hot compressed magnetized plasma to the cold liner is dominated by transverse <span class="hlt">heat</span> conduction and advection, and the corresponding loss of magnetic <span class="hlt">flux</span> is dominated by advection and the Nernst effect. For a large electron Hall parameter (ω{sub e}τ{sub e}≫1), the effective diffusion coefficients determining the losses of <span class="hlt">heat</span> and magnetic <span class="hlt">flux</span> to the liner <span class="hlt">wall</span> are both shown to decrease with ω{sub e}τ{sub e} as does the Bohm diffusion coefficient cT/(16eB), which is commonly associated with low collisionality and two-dimensional transport. We demonstrate how this family of exact solutions can be used for verification of codes that model the MagLIF plasma dynamics.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017PhST..170a4007B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017PhST..170a4007B"><span>Comparison of <span class="hlt">heat</span> <span class="hlt">flux</span> measurement techniques during the DIII-D metal ring campaign</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Barton, J. L.; Nygren, R. E.; Unterberg, E. A.; Watkins, J. G.; Makowski, M. A.; Moser, A.; Rudakov, D. L.; Buchenauer, D.</p> <p>2017-12-01</p> <p>The <span class="hlt">heat</span> <span class="hlt">fluxes</span> expected in the ITER divertor raise concerns about the damage tolerances of tungsten, especially due to thermal transients caused by edge localized modes (ELMs) as well as frequent temperature cycling from high to low extremes. Therefore we are motivated to understand the <span class="hlt">heat</span> <span class="hlt">flux</span> conditions that can cause not only enhanced erosion but also bulk thermo-mechanical damage to a tungsten divertor. For the metal ring campaign in DIII-D, tungsten-coated TZM tile inserts were installed making two toroidal arrays of metal tile inserts in the lower divertor. This study examines the deposited <span class="hlt">heat</span> <span class="hlt">flux</span> on these rings with embedded thermocouples (TCs) sampling at 10 kHz and compares them to Langmuir probe (LP) and infrared thermography (IRTV) <span class="hlt">heat</span> <span class="hlt">flux</span> measurements. We see agreement of the TC, LP, and IRTV data within 20% of the <span class="hlt">heat</span> <span class="hlt">flux</span> averaged over the entire discharge, and that all three diagnostics suggest parallel <span class="hlt">heat</span> <span class="hlt">flux</span> at the OSP location increases linearly with input <span class="hlt">heating</span> power. The TC and LP <span class="hlt">heat</span> <span class="hlt">flux</span> time traces during the discharge trend together during large changes to the average <span class="hlt">heat</span> <span class="hlt">flux</span>. By subtracting the LP measured inter-ELM <span class="hlt">heat</span> <span class="hlt">flux</span> from TC data, using a rectangular ELM energy pulse shape, and taking the relative size and duration of each ELM from {{D}}α measurements, we extract the ELM <span class="hlt">heat</span> <span class="hlt">fluxes</span> from TC data. This over-estimates the IRTV measured ELM <span class="hlt">heat</span> <span class="hlt">fluxes</span> by a factor of 1.9, and could be due to the simplicity of the TC <span class="hlt">heat</span> <span class="hlt">flux</span> model and the assumed ELM energy pulse shape. ELM <span class="hlt">heat</span> <span class="hlt">fluxes</span> deposited on the inserts are used to model tungsten erosion in this campaign. These TC ELM <span class="hlt">heat</span> <span class="hlt">flux</span> estimates are used in addition to IRTV, especially in cases where the IRTV view to the metal ring is obstructed. We observe that some metal inserts were deformed due to exposed leading edges. The thermal conditions on these inserts are investigated with the thermal modeling code ABAQUS using our <span class="hlt">heat</span> <span class="hlt">flux</span> measurements when these edges</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19850027078','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19850027078"><span>Development of advanced high-temperature <span class="hlt">heat</span> <span class="hlt">flux</span> sensors. Phase 2: Verification testing</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Atkinson, W. H.; Cyr, M. A.; Strange, R. R.</p> <p>1985-01-01</p> <p>A two-phase program is conducted to develop <span class="hlt">heat</span> <span class="hlt">flux</span> sensors capable of making <span class="hlt">heat</span> <span class="hlt">flux</span> measurements throughout the hot section of gas turbine engines. In Phase 1, three types of <span class="hlt">heat</span> <span class="hlt">flux</span> sensors are selected; embedded thermocouple, laminated, and Gardon gauge sensors. A demonstration of the ability of these sensors to operate in an actual engine environment is reported. A segmented liner of each of two combustors being used in the Broad Specification Fuels Combustor program is instrumented with the three types of <span class="hlt">heat</span> <span class="hlt">flux</span> sensors then tested in a high pressure combustor rig. Radiometer probes are also used to measure the radiant <span class="hlt">heat</span> loads to more fully characterize the combustor environment. Test results show the <span class="hlt">heat</span> <span class="hlt">flux</span> sensors to be in good agreement with radiometer probes and the predicted data trends. In general, <span class="hlt">heat</span> <span class="hlt">flux</span> sensors have strong potential for use in combustor development programs.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19940003182&hterms=solar+receiver&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Dsolar%2Breceiver','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19940003182&hterms=solar+receiver&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Dsolar%2Breceiver"><span>SIMPLIFIED CALCULATION OF SOLAR <span class="hlt">FLUX</span> ON THE SIDE <span class="hlt">WALL</span> OF CYLINDRICAL CAVITY SOLAR RECEIVERS</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Bhandari, P.</p> <p>1994-01-01</p> <p>The Simplified Calculation of Solar <span class="hlt">Flux</span> Distribution on the Side <span class="hlt">Wall</span> of Cylindrical Cavity Solar Receivers program employs a simple solar <span class="hlt">flux</span> calculation algorithm for a cylindrical cavity type solar receiver. Applications of this program include the study of solar energy, <span class="hlt">heat</span> transfer, and space power-solar dynamics engineering. The aperture plate of the receiver is assumed to be located in the focal plane of a paraboloidal concentrator, and the geometry is assumed to be axisymmetric. The concentrator slope error is assumed to be the only surface error; it is assumed that there are no pointing or misalignment errors. Using cone optics, the contour error method is utilized to handle the slope error of the concentrator. The <span class="hlt">flux</span> distribution on the side <span class="hlt">wall</span> is calculated by integration of the energy incident from cones emanating from all the differential elements on the concentrator. The calculations are done for any set of dimensions and properties of the receiver and the concentrator, and account for any spillover on the aperture plate. The results of this algorithm compared excellently with those predicted by more complicated programs. Because of the utilization of axial symmetry and overall simplification, it is extremely fast. It can be easily extended to other axi-symmetric receiver geometries. The program was written in Fortran 77, compiled using a Ryan McFarland compiler, and run on an IBM PC-AT with a math coprocessor. It requires 60K of memory and has been implemented under MS-DOS 3.2.1. The program was developed in 1988.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017E%26ES...95d2018S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017E%26ES...95d2018S"><span>Selective Internal <span class="hlt">Heat</span> Distribution in Modified Trombe <span class="hlt">Wall</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Szyszka, Jerzy; Kogut, Janusz; Skrzypczak, Izabela; Kokoszka, Wanda</p> <p>2017-12-01</p> <p>At present, the requirements for thermal insulation of the external <span class="hlt">walls</span> in buildings are being increased. There is a need to reduce energy consumption for <span class="hlt">heating</span> rooms during the winter season. This may be achieved by increasing the thermal resistance of the outer partitions, using solutions that utilize either recuperation or solar radiation. The most popular systems include either solar collectors, or <span class="hlt">heat</span> pump links or ground exchangers. Trombe <span class="hlt">walls</span> (TW) are a very promising passive <span class="hlt">heating</span> system, which requires little or no effort to operate, and may be very convenient in different climate conditions. A typical TW consists of a masonry <span class="hlt">wall</span> painted a dark, <span class="hlt">heat</span> absorbing paint colour and faced with a single or double layer of glass. The principle of operation is based on the photothermal conversion of solar radiation. There are various modifications of TW. They may improve the energy efficiency in relation to the climate conditions in which they operate. The hybrid solutions are also known. The efficiency of <span class="hlt">walls</span> is related to the use of proper materials. In TW, the compromise should be sought between the thermal resistance and the ability to distribute <span class="hlt">heat</span> from the absorbed energy of solar radiation. The paper presents an overview of the most commonly used solutions and discusses its own concept dedicated to the climate conditions of Central Europe.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4646773','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4646773"><span>High geothermal <span class="hlt">heat</span> <span class="hlt">flux</span> measured below the West Antarctic Ice Sheet</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Fisher, Andrew T.; Mankoff, Kenneth D.; Tulaczyk, Slawek M.; Tyler, Scott W.; Foley, Neil</p> <p>2015-01-01</p> <p>The geothermal <span class="hlt">heat</span> <span class="hlt">flux</span> is a critical thermal boundary condition that influences the melting, flow, and mass balance of ice sheets, but measurements of this parameter are difficult to make in ice-covered regions. We report the first direct measurement of geothermal <span class="hlt">heat</span> <span class="hlt">flux</span> into the base of the West Antarctic Ice Sheet (WAIS), below Subglacial Lake Whillans, determined from the thermal gradient and the thermal conductivity of sediment under the lake. The <span class="hlt">heat</span> <span class="hlt">flux</span> at this site is 285 ± 80 mW/m2, significantly higher than the continental and regional averages estimated for this site using regional geophysical and glaciological models. Independent temperature measurements in the ice indicate an upward <span class="hlt">heat</span> <span class="hlt">flux</span> through the WAIS of 105 ± 13 mW/m2. The difference between these <span class="hlt">heat</span> <span class="hlt">flux</span> values could contribute to basal melting and/or be advected from Subglacial Lake Whillans by flowing water. The high geothermal <span class="hlt">heat</span> <span class="hlt">flux</span> may help to explain why ice streams and subglacial lakes are so abundant and dynamic in this region. PMID:26601210</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26601210','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26601210"><span>High geothermal <span class="hlt">heat</span> <span class="hlt">flux</span> measured below the West Antarctic Ice Sheet.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Fisher, Andrew T; Mankoff, Kenneth D; Tulaczyk, Slawek M; Tyler, Scott W; Foley, Neil</p> <p>2015-07-01</p> <p>The geothermal <span class="hlt">heat</span> <span class="hlt">flux</span> is a critical thermal boundary condition that influences the melting, flow, and mass balance of ice sheets, but measurements of this parameter are difficult to make in ice-covered regions. We report the first direct measurement of geothermal <span class="hlt">heat</span> <span class="hlt">flux</span> into the base of the West Antarctic Ice Sheet (WAIS), below Subglacial Lake Whillans, determined from the thermal gradient and the thermal conductivity of sediment under the lake. The <span class="hlt">heat</span> <span class="hlt">flux</span> at this site is 285 ± 80 mW/m(2), significantly higher than the continental and regional averages estimated for this site using regional geophysical and glaciological models. Independent temperature measurements in the ice indicate an upward <span class="hlt">heat</span> <span class="hlt">flux</span> through the WAIS of 105 ± 13 mW/m(2). The difference between these <span class="hlt">heat</span> <span class="hlt">flux</span> values could contribute to basal melting and/or be advected from Subglacial Lake Whillans by flowing water. The high geothermal <span class="hlt">heat</span> <span class="hlt">flux</span> may help to explain why ice streams and subglacial lakes are so abundant and dynamic in this region.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..1914314B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..1914314B"><span>The forgotten component of sub-glacial <span class="hlt">heat</span> flow: Upper crustal <span class="hlt">heat</span> production and resultant total <span class="hlt">heat</span> <span class="hlt">flux</span> on the Antarctic Peninsula</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Burton-Johnson, Alex; Halpin, Jacqueline; Whittaker, Joanne; Watson, Sally</p> <p>2017-04-01</p> <p>Seismic and magnetic geophysical methods have both been employed to produce estimates of <span class="hlt">heat</span> <span class="hlt">flux</span> beneath the Antarctic ice sheet. However, both methods use a homogeneous upper crustal model despite the variable concentration of <span class="hlt">heat</span> producing elements within its composite lithologies. Using geological and geochemical datasets from the Antarctic Peninsula we have developed a new methodology for incorporating upper crustal <span class="hlt">heat</span> production in <span class="hlt">heat</span> <span class="hlt">flux</span> models and have shown the greater variability this introduces in to estimates of crustal <span class="hlt">heat</span> <span class="hlt">flux</span>, with implications for glaciological modelling.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JIEIC..99..151S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JIEIC..99..151S"><span>Conjugate <span class="hlt">Heat</span> Transfer Study in Hypersonic Flows</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sahoo, Niranjan; Kulkarni, Vinayak; Peetala, Ravi Kumar</p> <p>2018-04-01</p> <p>Coupled and decoupled conjugate <span class="hlt">heat</span> transfer (CHT) studies are carried out to imitate experimental studies for <span class="hlt">heat</span> transfer measurement in hypersonic flow regime. The finite volume based solvers are used for analyzing the <span class="hlt">heat</span> interaction between fluid and solid domains. Temperature and surface <span class="hlt">heat</span> <span class="hlt">flux</span> signals are predicted by both coupled and decoupled CHT analysis techniques for hypersonic Mach numbers. These two methodologies are also used to study the effect of different <span class="hlt">wall</span> materials on surface parameters. Effectiveness of these CHT solvers has been verified for the inverse problem of <span class="hlt">wall</span> <span class="hlt">heat</span> <span class="hlt">flux</span> recovery using various techniques reported in the literature. Both coupled and decoupled CHT techniques are seen to be equally useful for prediction of local temperature and <span class="hlt">heat</span> <span class="hlt">flux</span> signals prior to the experiments in hypersonic flows.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFMOS22B..05M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFMOS22B..05M"><span>Atmospheric responses to sensible and latent <span class="hlt">heating</span> <span class="hlt">fluxes</span> over the Gulf Stream</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Minobe, S.; Ida, T.; Takatama, K.</p> <p>2016-12-01</p> <p>Air-sea interaction over mid-latitude oceanic fronts such as the Gulf Stream attracted large attention in the last decade. Observational analyses and modelling studies revealed that atmospheric responses over the Gulf Stream including surface wind convergence, enhanced precipitation and updraft penetrating to middle-to-upper troposphere roughly on the Gulf Stream current axis or on the warmer flank of sea-surface temperature (SST) front of the Gulf Stream . For these atmospheric responses, oceanic information should be transmitted to the atmosphere via turbulent <span class="hlt">heat</span> <span class="hlt">fluxes</span>, and thus the mechanisms for atmospheric responses can be understood better by examining latent and sensible air-sea <span class="hlt">heat</span> <span class="hlt">fluxes</span> more closely. Thus, the roles of the sensible and latent <span class="hlt">heat</span> <span class="hlt">fluxes</span> are examined by conducting a series of numerical experiments using the IPRC Regional Atmospheric Model over the Gulf Stream by applying SST smoothing for latent and sensible <span class="hlt">heating</span> separately. The results indicate that the sensible and latent <span class="hlt">heat</span> <span class="hlt">fluxes</span> affect the atmosphere differently. Sensible <span class="hlt">heat</span> <span class="hlt">flux</span> intensifies surface wind convergence to produce sea-level pressure (SLP) anomaly. Latent <span class="hlt">heat</span> <span class="hlt">flux</span> supplies moistures and maintains enhanced precipitation. The different <span class="hlt">heat</span> <span class="hlt">flux</span> components cause upward wind velocity at different levels.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29624394','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29624394"><span>Ultrahigh <span class="hlt">Flux</span> Thin Film Boiling <span class="hlt">Heat</span> Transfer Through Nanoporous Membranes.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Wang, Qingyang; Chen, Renkun</p> <p>2018-05-09</p> <p>Phase change <span class="hlt">heat</span> transfer is fundamentally important for thermal energy conversion and management, such as in electronics with power density over 1 kW/cm 2 . The critical <span class="hlt">heat</span> <span class="hlt">flux</span> (CHF) of phase change <span class="hlt">heat</span> transfer, either evaporation or boiling, is limited by vapor <span class="hlt">flux</span> from the liquid-vapor interface, known as the upper limit of <span class="hlt">heat</span> <span class="hlt">flux</span>. This limit could in theory be greater than 1 kW/cm 2 on a planar surface, but its experimental realization has remained elusive. Here, we utilized nanoporous membranes to realize a new "thin film boiling" regime that resulted in an unprecedentedly high CHF of over 1.2 kW/cm 2 on a planar surface, which is within a factor of 4 of the theoretical limit, and can be increased to a higher value if mechanical strength of the membranes can be improved (demonstrated with 1.85 kW/cm 2 CHF in this work). The liquid supply is achieved through a simple nanoporous membrane that supports the liquid film where its thickness automatically decreases as <span class="hlt">heat</span> <span class="hlt">flux</span> increases. The thin film configuration reduces the conductive thermal resistance, leads to high frequency bubble departure, and provides separate liquid-vapor pathways, therefore significantly enhances the <span class="hlt">heat</span> transfer. Our work provides a new nanostructuring approach to achieve ultrahigh <span class="hlt">heat</span> <span class="hlt">flux</span> in phase change <span class="hlt">heat</span> transfer and will benefit both theoretical understanding and application in thermal management of high power devices of boiling <span class="hlt">heat</span> transfer.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUOSPO54F3320B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUOSPO54F3320B"><span>Satellite-based Calibration of <span class="hlt">Heat</span> <span class="hlt">Flux</span> at the Ocean Surface</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Barron, C. N.; Dastugue, J. M.; May, J. C.; Rowley, C. D.; Smith, S. R.; Spence, P. L.; Gremes-Cordero, S.</p> <p>2016-02-01</p> <p>Model forecasts of upper ocean <span class="hlt">heat</span> content and variability on diurnal to daily scales are highly dependent on estimates of <span class="hlt">heat</span> <span class="hlt">flux</span> through the air-sea interface. Satellite remote sensing is applied to not only inform the initial ocean state but also to mitigate errors in surface <span class="hlt">heat</span> <span class="hlt">flux</span> and model representations affecting the distribution of <span class="hlt">heat</span> in the upper ocean. Traditional assimilation of sea surface temperature (SST) observations re-centers ocean models at the start of each forecast cycle. Subsequent evolution depends on estimates of surface <span class="hlt">heat</span> <span class="hlt">fluxes</span> and upper-ocean processes over the forecast period. The COFFEE project (Calibration of Ocean Forcing with satellite <span class="hlt">Flux</span> Estimates) endeavors to correct ocean forecast bias through a responsive error partition among surface <span class="hlt">heat</span> <span class="hlt">flux</span> and ocean dynamics sources. A suite of experiments in the southern California Current demonstrates a range of COFFEE capabilities, showing the impact on forecast error relative to a baseline three-dimensional variational (3DVAR) assimilation using Navy operational global or regional atmospheric forcing. COFFEE addresses satellite-calibration of surface <span class="hlt">fluxes</span> to estimate surface error covariances and links these to the ocean interior. Experiment cases combine different levels of <span class="hlt">flux</span> calibration with different assimilation alternatives. The cases may use the original <span class="hlt">fluxes</span>, apply full satellite corrections during the forecast period, or extend hindcast corrections into the forecast period. Assimilation is either baseline 3DVAR or standard strong-constraint 4DVAR, with work proceeding to add a 4DVAR expanded to include a weak constraint treatment of the surface <span class="hlt">flux</span> errors. Covariance of <span class="hlt">flux</span> errors is estimated from the recent time series of forecast and calibrated <span class="hlt">flux</span> terms. While the California Current examples are shown, the approach is equally applicable to other regions. These approaches within a 3DVAR application are anticipated to be useful for global and larger</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009PhPl...16b2501S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009PhPl...16b2501S"><span>Divertor <span class="hlt">heat</span> <span class="hlt">flux</span> mitigation in the National Spherical Torus Experimenta)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Soukhanovskii, V. A.; Maingi, R.; Gates, D. A.; Menard, J. E.; Paul, S. F.; Raman, R.; Roquemore, A. L.; Bell, M. G.; Bell, R. E.; Boedo, J. A.; Bush, C. E.; Kaita, R.; Kugel, H. W.; Leblanc, B. P.; Mueller, D.; NSTX Team</p> <p>2009-02-01</p> <p>Steady-state handling of divertor <span class="hlt">heat</span> <span class="hlt">flux</span> is a critical issue for both ITER and spherical torus-based devices with compact high power density divertors. Significant reduction of <span class="hlt">heat</span> <span class="hlt">flux</span> to the divertor plate has been achieved simultaneously with favorable core and pedestal confinement and stability properties in a highly shaped lower single null configuration in the National Spherical Torus Experiment (NSTX) [M. Ono et al., Nucl. Fusion 40, 557 2000] using high magnetic <span class="hlt">flux</span> expansion at the divertor strike point and the radiative divertor technique. A partial detachment of the outer strike point was achieved with divertor deuterium injection leading to peak <span class="hlt">flux</span> reduction from 4-6MWm-2to0.5-2MWm-2 in small-ELM 0.8-1.0MA, 4-6MW neutral beam injection-<span class="hlt">heated</span> H-mode discharges. A self-consistent picture of the outer strike point partial detachment was evident from divertor <span class="hlt">heat</span> <span class="hlt">flux</span> profiles and recombination, particle <span class="hlt">flux</span> and neutral pressure measurements. Analytic scrape-off layer parallel transport models were used for interpretation of NSTX detachment experiments. The modeling showed that the observed peak <span class="hlt">heat</span> <span class="hlt">flux</span> reduction and detachment are possible with high radiated power and momentum loss fractions, achievable with divertor gas injection, and nearly impossible to achieve with main electron density, divertor neutral density or recombination increases alone.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20170002665&hterms=geomagnetism&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D70%26Ntt%3Dgeomagnetism','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20170002665&hterms=geomagnetism&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D70%26Ntt%3Dgeomagnetism"><span>GEM-CEDAR Challenge: Poynting <span class="hlt">Flux</span> at DMSP and Modeled Joule <span class="hlt">Heat</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Rastaetter, Lutz; Shim, Ja Soon; Kuznetsova, Maria M.; Kilcommons, Liam M.; Knipp, Delores J.; Codrescu, Mihail; Fuller-Rowell, Tim; Emery, Barbara; Weimer, Daniel R.; Cosgrove, Russell; <a style="text-decoration: none; " href="javascript:void(0); " onClick="displayelement('author_20170002665'); toggleEditAbsImage('author_20170002665_show'); toggleEditAbsImage('author_20170002665_hide'); "> <img style="display:inline; width:12px; height:12px; " src="images/arrow-up.gif" width="12" height="12" border="0" alt="hide" id="author_20170002665_show"> <img style="width:12px; height:12px; display:none; " src="images/arrow-down.gif" width="12" height="12" border="0" alt="hide" id="author_20170002665_hide"></p> <p>2016-01-01</p> <p>Poynting <span class="hlt">flux</span> into the ionosphere measures the electromagnetic energy coming from the magnetosphere. This energy <span class="hlt">flux</span> can vary greatly between quiet times and geomagnetic active times. As part of the Geospace Environment Modeling-coupling energetics and dynamics of atmospheric regions modeling challenge, physics-based models of the 3-D ionosphere and ionospheric electrodynamics solvers of magnetosphere models that specify Joule <span class="hlt">heat</span> and empirical models specifying Poynting <span class="hlt">flux</span> were run for six geomagnetic storm events of varying intensity. We compared model results with Poynting <span class="hlt">flux</span> values along the DMSP-15 satellite track computed from ion drift meter and magnetic field observations. Although being a different quantity, Joule <span class="hlt">heat</span> can in practice be correlated to incoming Poynting <span class="hlt">flux</span> because the energy is dissipated primarily in high latitudes where Poynting <span class="hlt">flux</span> is being deposited. Within the physics-based model group, we find mixed results with some models overestimating Joule <span class="hlt">heat</span> and some models agreeing better with observed Poynting <span class="hlt">flux</span> rates as integrated over auroral passes. In contrast, empirical models tend to underestimate integrated Poynting <span class="hlt">flux</span> values. Modeled Joule <span class="hlt">heat</span> or Poynting <span class="hlt">flux</span> patterns often resemble the observed Poynting <span class="hlt">flux</span> patterns on a large scale, but amplitudes can differ by a factor of 2 or larger due to the highly localized nature of observed Poynting <span class="hlt">flux</span> deposition that is not captured by the models. In addition, the positioning of modeled patterns appear to be randomly shifted against the observed Poynting <span class="hlt">flux</span> energy input. This study is the first to compare Poynting <span class="hlt">flux</span> and Joule <span class="hlt">heat</span> in a large variety of models of the ionosphere.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/20770232-investigation-saturated-critical-heat-flux-single-uniformly-heated-microchannel','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/20770232-investigation-saturated-critical-heat-flux-single-uniformly-heated-microchannel"><span>Investigation of saturated critical <span class="hlt">heat</span> <span class="hlt">flux</span> in a single, uniformly <span class="hlt">heated</span> microchannel</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>Wojtan, Leszek; Revellin, Remi; Thome, John R.</p> <p>2006-08-15</p> <p>A series of tests have been performed to determine the saturated critical <span class="hlt">heat</span> <span class="hlt">flux</span> (CHF) in 0.5 and 0.8mm internal diameter microchannel tubes as a function of refrigerant mass velocity, <span class="hlt">heated</span> length, saturation temperature and inlet liquid subcooling. The tested refrigerants were R-134a and R-245fa and the <span class="hlt">heated</span> length of microchannel was varied between 20 and 70mm. The results show a strong dependence of CHF on mass velocity, <span class="hlt">heated</span> length and microchannel diameter but no influence of liquid subcooling (2-15{sup o}C) was observed. The experimental results have been compared to the well-known CHF single-channel correlation of Y. Katto and H.more » Ohno [An improved version of the generalized correlation of critical <span class="hlt">heat</span> <span class="hlt">flux</span> for the forced convective boiling in uniformly <span class="hlt">heated</span> vertical tubes, Int. J. <span class="hlt">Heat</span> and Mass Transfer 27 (9) (1984) 1641-1648] and the multichannel correlation of W. Qu and I. Mudawar [Measurement and correlation of critical <span class="hlt">heat</span> <span class="hlt">flux</span> in two-phase microchannel <span class="hlt">heat</span> sinks, Int. J. <span class="hlt">Heat</span> and Mass Transfer 47 (2004) 2045-2059]. The comparison shows that the correlation of Katto-Ohno predicts microchannel data with a mean absolute error of 32.8% with only 41.2% of the data falling within a +/-15% error band. The correlation of Qu and Mudawar shows the same trends as the CHF data but significantly overpredicts them. Based on the present experimental data, a new microscale version of the Katto-Ohno correlation for the prediction of CHF during saturated boiling in microchannels has been proposed. (author)« 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_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('http://adsabs.harvard.edu/abs/2016AGUFM.A33M..04H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.A33M..04H"><span>An Analysis of Inter-annual Variability and Uncertainty of Continental Surface <span class="hlt">Heat</span> <span class="hlt">Fluxes</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Huang, S. Y.; Deng, Y.; Wang, J.</p> <p>2016-12-01</p> <p>The inter-annual variability and the corresponding uncertainty of land surface <span class="hlt">heat</span> <span class="hlt">fluxes</span> during the first decade of the 21st century are re-evaluated at continental scale based on the <span class="hlt">heat</span> <span class="hlt">fluxes</span> estimated by the maximum entropy production (MEP) model. The MEP model predicted <span class="hlt">heat</span> <span class="hlt">fluxes</span> are constrained by surface radiation <span class="hlt">fluxes</span>, automatically satisfy surface energy balance, and are independent of temperature/moisture gradient, wind speed, and roughness lengths. The surface radiation <span class="hlt">fluxes</span> and temperature data from Clouds and the Earth's Radiant Energy System and the surface specific humidity data from Modern-Era Retrospective analysis for Research and Applications were used to reproduce the global surface <span class="hlt">heat</span> <span class="hlt">fluxes</span> with land-cover data from the NASA Energy and Water cycle Study (NEWS). Our analysis shows that the annual means of continental latent <span class="hlt">heat</span> <span class="hlt">fluxes</span> have increasing trends associated with increasing trends in surface net radiative <span class="hlt">fluxes</span>. The sensible <span class="hlt">heat</span> <span class="hlt">fluxes</span> also have increasing trends over most continents except for South America. Ground <span class="hlt">heat</span> <span class="hlt">fluxes</span> have little trends. The continental-scale analysis of the MEP <span class="hlt">fluxes</span> are compared with other existing global surface <span class="hlt">fluxes</span> data products and the implications of the results for inter-annual to decadal variability of regional surface energy budget are discussed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19920009517','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19920009517"><span>Miniature high temperature plug-type <span class="hlt">heat</span> <span class="hlt">flux</span> gauges</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Liebert, Curt H.</p> <p>1992-01-01</p> <p>The objective is to describe continuing efforts to develop methods for measuring surface <span class="hlt">heat</span> <span class="hlt">flux</span>, gauge active surface temperature, and <span class="hlt">heat</span> transfer coefficient quantities. The methodology involves inventing a procedure for fabricating improved plug-type <span class="hlt">heat</span> <span class="hlt">flux</span> gauges and also for formulating inverse <span class="hlt">heat</span> conduction models and calculation procedures. These models and procedures are required for making indirect measurements of these quantities from direct temperature measurements at gauge interior locations. Measurements of these quantities were made in a turbine blade thermal cycling tester (TBT) located at MSFC. The TBT partially simulates the turbopump turbine environment in the Space Shuttle Main Engine. After the TBT test, experiments were performed in an arc lamp to analyze gauge quality.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1992ThApC..46...53B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1992ThApC..46...53B"><span>Tests of a robust eddy correlation system for sensible <span class="hlt">heat</span> <span class="hlt">flux</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Blanford, J. H.; Gay, L. W.</p> <p>1992-03-01</p> <p>Sensible <span class="hlt">heat</span> <span class="hlt">flux</span> estimates from a simple, one-propeller eddy correlation system (OPEC) were compared with those from a sonic anemometer eddy correlation system (SEC). In accordance with similarity theory, the performance of the OPEC system improved with increasing height of the sensor above the surface. <span class="hlt">Flux</span> totals from the two systems at sites with adequate fetch were in excellent agreement after frequency response corrections were applied. The propeller system appears suitable for long periods of unattended measurement. The sensible <span class="hlt">heat</span> <span class="hlt">flux</span> measurements can be combined with net radiation and soil <span class="hlt">heat</span> <span class="hlt">flux</span> measurements to estimate latent <span class="hlt">heat</span> as a residual in the surface energy balance.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28437986','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28437986"><span>Control and design <span class="hlt">heat</span> <span class="hlt">flux</span> bending in thermal devices with transformation optics.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Xu, Guoqiang; Zhang, Haochun; Jin, Yan; Li, Sen; Li, Yao</p> <p>2017-04-17</p> <p>We propose a fundamental latent function of control <span class="hlt">heat</span> transfer and <span class="hlt">heat</span> <span class="hlt">flux</span> density vectors at random positions on thermal materials by applying transformation optics. The expressions for <span class="hlt">heat</span> <span class="hlt">flux</span> bending are obtained, and the factors influencing them are investigated in both 2D and 3D cloaking schemes. Under certain conditions, more than one degree of freedom of <span class="hlt">heat</span> <span class="hlt">flux</span> bending exists corresponding to the temperature gradients of the 3D domain. The <span class="hlt">heat</span> <span class="hlt">flux</span> path can be controlled in random space based on the geometrical azimuths, radial positions, and thermal conductivity ratios of the selected materials.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1993SPIE.1997..486C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1993SPIE.1997..486C"><span>New low-cost high <span class="hlt">heat</span> <span class="hlt">flux</span> source</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Cheng, Dah Yu</p> <p>1993-11-01</p> <p>Intense <span class="hlt">heat</span> sources are needed to address new manufacturing techniques, such as, the Rapid Thermal Process for silicon wafer manufacturing. The current technology of high <span class="hlt">heat</span> <span class="hlt">flux</span> sources is the laser for its ability to do welding and cutting is well-known. The laser with its coherent radiation allows an image to be focused down to very small sizes to reach extremely high <span class="hlt">heat</span> <span class="hlt">flux</span>. But the laser also has problems: it is inefficient in its use because of its singular wave length and brings up OSHA safety related problems. Also heavy industrial manufacturing requires much higher total energy in addition to the high <span class="hlt">heat</span> <span class="hlt">flux</span> which makes the current laser system too slow to be economical. The system I am proposing starts with a parabolic curve. If the curve is rotated about the axis of the parabola, it generates the classical parabolic reflector as we know it. On the other hand, when the curve is rotated about the chord, a line passing through the focal point and perpendicular to the axis, generates a new surface called the Orthogonal Parabolic Surface. A new optical reflector geometry is presented which integrates a linear white light (continuum spectra) source through a coherent path to be focused to a very small area.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JPhD...51z4001B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JPhD...51z4001B"><span>MHD <span class="hlt">heat</span> <span class="hlt">flux</span> mitigation in hypersonic flow around a blunt body with ablating surface</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bityurin, V. A.; Bocharov, A. N.</p> <p>2018-07-01</p> <p>One of the possible applications of magnetohydrodynamic flow control is considered. Namely, the surface <span class="hlt">heat</span> <span class="hlt">flux</span> mitigation by means of magnetohydrodynamic (MHD) interaction in hypersonic flow around a blunt body. The 2D computational model realizes a coupled solution of chemically non-equilibrium ionized airflow in magnetic field. <span class="hlt">Heat</span>- and mass-transfer due to the ablation of materials from the body surface is taken into account. Two cases of free-stream flow conditions are considered: moderate free-stream velocity (7500 m s‑1) case and high free-stream velocity (11 000 m s‑1) case. It is shown that the first flow case results in moderate ionization in the shock layer, while the second flow case results in high ionization. In the first case, the Hall effect is significant, and effective electrical conductivity in the shock layer is rather low. In the second case, the Hall effect reduces, and effective conductivity is high. Even if the Hall effect is strong, as in the first case, intensive MHD deceleration of the flow behind the shock is provided due to the presence of insulating boundaries, the bow shock front and non-conductive <span class="hlt">wall</span> of the blunt body. In the second case, high effective conductivity provides a high intensity of MHD flow deceleration. In both cases, a strong effect of MHD interaction on the flow structure is observed. As a consequence, a noticeable reduction of the surface <span class="hlt">heat</span> <span class="hlt">flux</span> is revealed for reasonable values of magnetic induction. The new treatment of mechanism for the surface <span class="hlt">heat</span> <span class="hlt">flux</span> reduction is proposed, which is different from commonly used one assuming that MHD interaction increases the bow shock stand-off distance, and, consequently results in a decrease of the mean temperature drop across the shock layer. The new effect of ‘saturation of <span class="hlt">heat</span> flux’ is discussed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70186946','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70186946"><span><span class="hlt">Heat</span> <span class="hlt">flux</span> from magmatic hydrothermal systems related to availability of fluid recharge</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Harvey, M. C.; Rowland, J.V.; Chiodini, G.; Rissmann, C.F.; Bloomberg, S.; Hernandez, P.A.; Mazot, A.; Viveiros, F.; Werner, Cynthia A.</p> <p>2015-01-01</p> <p>Magmatic hydrothermal systems are of increasing interest as a renewable energy source. Surface <span class="hlt">heat</span> <span class="hlt">flux</span> indicates system resource potential, and can be inferred from soil CO2 <span class="hlt">flux</span> measurements and fumarole gas chemistry. Here we compile and reanalyze results from previous CO2 <span class="hlt">flux</span> surveys worldwide to compare <span class="hlt">heat</span> <span class="hlt">flux</span> from a variety of magma-hydrothermal areas. We infer that availability of water to recharge magmatic hydrothermal systems is correlated with <span class="hlt">heat</span> <span class="hlt">flux</span>. Recharge availability is in turn governed by permeability, structure, lithology, rainfall, topography, and perhaps unsurprisingly, proximity to a large supply of water such as the ocean. The relationship between recharge and <span class="hlt">heat</span> <span class="hlt">flux</span> interpreted by this study is consistent with recent numerical modeling that relates hydrothermal system <span class="hlt">heat</span> output to rainfall catchment area. This result highlights the importance of recharge as a consideration when evaluating hydrothermal systems for electricity generation, and the utility of CO2 <span class="hlt">flux</span> as a resource evaluation tool.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19740017702','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19740017702"><span>Model <span class="hlt">wall</span> and recovery temperature effects on experimental <span class="hlt">heat</span> transfer data analysis</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Throckmorton, D. A.; Stone, D. R.</p> <p>1974-01-01</p> <p>Basic analytical procedures are used to illustrate, both qualitatively and quantitatively, the relative impact upon <span class="hlt">heat</span> transfer data analysis of certain factors which may affect the accuracy of experimental <span class="hlt">heat</span> transfer data. Inaccurate knowledge of adiabatic <span class="hlt">wall</span> conditions results in a corresponding inaccuracy in the measured <span class="hlt">heat</span> transfer coefficient. The magnitude of the resulting error is extreme for data obtained at <span class="hlt">wall</span> temperatures approaching the adiabatic condition. High model <span class="hlt">wall</span> temperatures and <span class="hlt">wall</span> temperature gradients affect the level and distribution of <span class="hlt">heat</span> transfer to an experimental model. The significance of each of these factors is examined and its impact upon <span class="hlt">heat</span> transfer data analysis is assessed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.T13B0517B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.T13B0517B"><span>A new <span class="hlt">heat</span> <span class="hlt">flux</span> model for the Antarctic Peninsula incorporating spatially variable upper crustal radiogenic <span class="hlt">heat</span> production</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Burton-Johnson, A.; Halpin, J.; Whittaker, J. M.; Graham, F. S.; Watson, S. J.</p> <p>2017-12-01</p> <p>We present recently published findings (Burton-Johnson et al., 2017) on the variability of Antarctic sub-glacial <span class="hlt">heat</span> <span class="hlt">flux</span> and the impact from upper crustal geology. Our new method reveals that the upper crust contributes up to 70% of the Antarctic Peninsula's subglacial <span class="hlt">heat</span> <span class="hlt">flux</span>, and that <span class="hlt">heat</span> <span class="hlt">flux</span> values are more variable at smaller spatial resolutions than geophysical methods can resolve. Results indicate a higher <span class="hlt">heat</span> <span class="hlt">flux</span> on the east and south of the Peninsula (mean 81 mWm-2) where silicic rocks predominate, than on the west and north (mean 67 mWm-2) where volcanic arc and quartzose sediments are dominant. Whilst the data supports the contribution of HPE-enriched granitic rocks to high <span class="hlt">heat</span> <span class="hlt">flux</span> values, sedimentary rocks can be of comparative importance dependent on their provenance and petrography. Models of subglacial <span class="hlt">heat</span> <span class="hlt">flux</span> must utilize a heterogeneous upper crust with variable radioactive <span class="hlt">heat</span> production if they are to accurately predict basal conditions of the ice sheet. Our new methodology and dataset facilitate improved numerical model simulations of ice sheet dynamics. The most significant challenge faced remains accurate determination of crustal structure, particularly the depths of the HPE-enriched sedimentary basins and the sub-glacial geology away from exposed outcrops. Continuing research (particularly detailed geophysical interpretation) will better constrain these unknowns and the effect of upper crustal geology on the Antarctic ice sheet. Burton-Johnson, A., Halpin, J.A., Whittaker, J.M., Graham, F.S., and Watson, S.J., 2017, A new <span class="hlt">heat</span> <span class="hlt">flux</span> model for the Antarctic Peninsula incorporating spatially variable upper crustal radiogenic <span class="hlt">heat</span> production: Geophysical Research Letters, v. 44, doi: 10.1002/2017GL073596.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19850067082&hterms=Biddle&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3DBiddle','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19850067082&hterms=Biddle&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3DBiddle"><span>Evidence for ion <span class="hlt">heat</span> <span class="hlt">flux</span> in the light ion polar wind</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Biddle, A. P.; Moore, T. E.; Chappell, C. R.</p> <p>1985-01-01</p> <p>Cold flowing hydrogen and helium ions have been observed using the retarding ion mass spectrometer on board the Dynamics Explorer 1 spacecraft in the dayside magnetosphere at subauroral latitudes. The ions show a marked <span class="hlt">flux</span> asymmetry with respect to the relative wind direction. The observed data are fitted by a model of drifting Maxwellian distributions perturbed by a first order-Spritzer-Haerm <span class="hlt">heat</span> <span class="hlt">flux</span> distribution function. It is shown that both ion species are supersonic just equatorward of the auroral zone at L = 14, and the shape of asymmetry and direction of the asymmetry are consistent with the presence of an upward <span class="hlt">heat</span> <span class="hlt">flux</span>. At L = 6, both species evolve smoothly into warmer subsonic upward flows with downward <span class="hlt">heat</span> <span class="hlt">fluxes</span>. In the case of subsonic flows the downward <span class="hlt">heat</span> <span class="hlt">flux</span> implies a significant <span class="hlt">heat</span> source at higher altitudes. Spin curves of the spectrometer count rate versus the spin phase angle are provided.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19930022364','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19930022364"><span>Progress in the measurement of SSME turbine <span class="hlt">heat</span> <span class="hlt">flux</span> with plug-type sensors</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Liebert, Curt H.</p> <p>1991-01-01</p> <p>Data reduction was completed for tests of plug-type <span class="hlt">heat</span> <span class="hlt">flux</span> sensors (gauges) in a turbine blade thermal cycling tester (TBT) that is located at NASA/Marshall Space Flight Center, and a typical gauge is illustrated. This is the first time that <span class="hlt">heat</span> <span class="hlt">flux</span> has been measured in a Space Shuttle Main Engine (SSME) Turbopump Turbine environment. The development of the concept for the gauge was performed in a <span class="hlt">heat</span> <span class="hlt">flux</span> measurement facility at Lewis. In this facility, transient and steady state absorbed surface <span class="hlt">heat</span> <span class="hlt">flux</span> information was obtained from transient temperature measurements taken at points within the gauge. A schematic of the TBT is presented, and plots of the absorbed surface <span class="hlt">heat</span> <span class="hlt">flux</span> measured on the three blades tested in the TBT are presented. High quality <span class="hlt">heat</span> <span class="hlt">flux</span> values were measured on all three blades. The experiments demonstrated that reliable and durable gauges can be repeatedly fabricated into the airfoils. The experiment <span class="hlt">heat</span> <span class="hlt">flux</span> data are being used for verification of SSME analytical stress, boundary layer, and <span class="hlt">heat</span> transfer design models. Other experimental results and future plans are also presented.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFM.A33B0157H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.A33B0157H"><span>Distributed Sensible <span class="hlt">Heat</span> <span class="hlt">Flux</span> Measurements for Wireless Sensor Networks</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Huwald, H.; Brauchli, T.; Lehning, M.; Higgins, C. W.</p> <p>2015-12-01</p> <p>The sensible <span class="hlt">heat</span> <span class="hlt">flux</span> component of the surface energy balance is typically computed using eddy covariance or two point profile measurements while alternative approaches such as the <span class="hlt">flux</span> variance method based on convective scaling has been much less explored and applied. <span class="hlt">Flux</span> variance (FV) certainly has a few limitations and constraints but may be an interesting and competitive method in low-cost and power limited wireless sensor networks (WSN) with the advantage of providing spatio-temporal sensible <span class="hlt">heat</span> <span class="hlt">flux</span> over the domain of the network. In a first step, parameters such as sampling frequency, sensor response time, and averaging interval are investigated. Then we explore the applicability and the potential of the FV method for use in WSN in a field experiment. Low-cost sensor systems are tested and compared against reference instruments (3D sonic anemometers) to evaluate the performance and limitations of the sensors as well as the method with respect to the standard calculations. Comparison experiments were carried out at several sites to gauge the <span class="hlt">flux</span> measurements over different surface types (gravel, grass, water) from the low-cost systems. This study should also serve as an example of spatially distributed sensible <span class="hlt">heat</span> <span class="hlt">flux</span> measurements.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012EGUGA..1412137Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012EGUGA..1412137Z"><span>Urban <span class="hlt">heat</span> <span class="hlt">fluxes</span> in the subsurface of Cologne, Germany</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zhu, K.; Bayer, P.; Blum, P.</p> <p>2012-04-01</p> <p>Urbanization during the last hundred years has led to both environmental and thermal impacts on the subsurface. The urban <span class="hlt">heat</span> island (UHI) effect is mostly described as an atmospheric phenomenon, where the measured aboveground temperatures in cities are elevated in comparison to undisturbed rural regions. However, UHIs can be found below, as well as above ground. A large amount of anthropogenic <span class="hlt">heat</span> migrates into the urban subsurface, which also raises the ground temperature and permanently changes the thermal conditions in shallow aquifers. The main objective of our work is to study and determine the urban <span class="hlt">heat</span> <span class="hlt">fluxes</span> in Cologne, Germany, and to improve our understanding of the dynamics of subsurface energy <span class="hlt">fluxes</span> in UHIs. Ideally, our findings will contribute to strategic and more sustainable geothermal use in cities. For a quantitative analysis of the energy <span class="hlt">fluxes</span> within the subsurface and across the atmospheric boundary, two and three-dimensional coupled numerical flow and <span class="hlt">heat</span> transport models were developed. The simulation results indicate that during the past hundred years, an average vertical urban <span class="hlt">heat</span> <span class="hlt">flux</span> that ranges between 80 and 375 mW m-2 can be deduced. Thermal anomalies have migrated into the local urban aquifer system and they reach a depth of about 150 m. In this context, the influence of the regional groundwater flow on the subsurface <span class="hlt">heat</span> transport and temperature development is comprehensively discussed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/12836556','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/12836556"><span>[A review on research of land surface water and <span class="hlt">heat</span> <span class="hlt">fluxes</span>].</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Sun, Rui; Liu, Changming</p> <p>2003-03-01</p> <p>Many field experiments were done, and soil-vegetation-atmosphere transfer(SVAT) models were stablished to estimate land surface <span class="hlt">heat</span> <span class="hlt">fluxes</span>. In this paper, the processes of experimental research on land surface water and <span class="hlt">heat</span> <span class="hlt">fluxes</span> are reviewed, and three kinds of SVAT model(single layer model, two layer model and multi-layer model) are analyzed. Remote sensing data are widely used to estimate land surface <span class="hlt">heat</span> <span class="hlt">fluxes</span>. Based on remote sensing and energy balance equation, different models such as simplified model, single layer model, extra resistance model, crop water stress index model and two source resistance model are developed to estimate land surface <span class="hlt">heat</span> <span class="hlt">fluxes</span> and evapotranspiration. These models are also analyzed in this paper.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1998JNuM..258..672M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1998JNuM..258..672M"><span>On the use of flat tile armour in high <span class="hlt">heat</span> <span class="hlt">flux</span> components</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Merola, M.; Vieider, G.</p> <p>1998-10-01</p> <p>The possibility to have a flat tile geometry for those high <span class="hlt">heat</span> <span class="hlt">flux</span> components subjected to a convective <span class="hlt">heat</span> <span class="hlt">flux</span> (namely the divertor dump target, lower vertical target, and the limiter) has been investigated. Because of the glancing incidence of the power load, if an armour tile falls off an extremely high <span class="hlt">heat</span> <span class="hlt">flux</span> hits the leading edge of the adjacent tile. As a result a rapid temperature increase occurs in the armour-<span class="hlt">heat</span> sink joint. The <span class="hlt">heat</span> <span class="hlt">flux</span> to the water coolant also increases rapidly up to a factor of 1.7 and 2.3 for a beryllium and CFC armour, respectively, thus causing possible critical <span class="hlt">heat</span> <span class="hlt">flux</span> problems. Thermal stresses in the armour-<span class="hlt">heat</span> sink joint double in less than 0.4 s and triplicate after 1 s thus leading to a possible cascade failure. Therefore the use of a flat tile geometry for these components does not seem to be appropriate. In this case a monoblock geometry gives a much more robust solution.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018ZaMP...69...71B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018ZaMP...69...71B"><span>Systems with a constant <span class="hlt">heat</span> <span class="hlt">flux</span> with applications to radiative <span class="hlt">heat</span> transport across nanoscale gaps and layers</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Budaev, Bair V.; Bogy, David B.</p> <p>2018-06-01</p> <p>We extend the statistical analysis of equilibrium systems to systems with a constant <span class="hlt">heat</span> <span class="hlt">flux</span>. This extension leads to natural generalizations of Maxwell-Boltzmann's and Planck's equilibrium energy distributions to energy distributions of systems with a net <span class="hlt">heat</span> <span class="hlt">flux</span>. This development provides a long needed foundation for addressing problems of nanoscale <span class="hlt">heat</span> transport by a systematic method based on a few fundamental principles. As an example, we consider the computation of the radiative <span class="hlt">heat</span> <span class="hlt">flux</span> between narrowly spaced half-spaces maintained at different temperatures.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/ADA243558','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA243558"><span><span class="hlt">Heat</span> Transfer Enhancement due to Bubble Pumping in FC-72 Near the Saturation Temperature</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>1991-03-01</p> <p>boiling, (2) reducing <span class="hlt">wall</span> superheat during nucleate boiling and (3) enhancing critical <span class="hlt">heat</span> <span class="hlt">flux</span> ( Mudawar , 1990) . Since the <span class="hlt">heat</span> transfer potential of...<span class="hlt">flux</span> from a simulated electronic chip attached to the <span class="hlt">wall</span> of a vertical rectangular channel was determined by Mudawar and Madox (1988). They concluded...Surface Boiling," Industrial and Engineering Chemistry, vol. 41, No. 9, 1949. Mudawar , I., and D.E. Maddox, Critical <span class="hlt">Heat</span> <span class="hlt">Flux</span> in Subcooled Flow Boiling</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/6713305-third-law-thermodynamics-presence-heat-flux','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/6713305-third-law-thermodynamics-presence-heat-flux"><span>Third law of thermodynamics in the presence of a <span class="hlt">heat</span> <span class="hlt">flux</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>Camacho, J.</p> <p>1995-01-01</p> <p>Following a maximum entropy formalism, we study a one-dimensional crystal under a <span class="hlt">heat</span> <span class="hlt">flux</span>. We obtain the phonon distribution function and evaluate the nonequilibrium temperature, the specific <span class="hlt">heat</span>, and the entropy as functions of the internal energy and the <span class="hlt">heat</span> <span class="hlt">flux</span>, in both the quantum and the classical limits. Some analogies between the behavior of equilibrium systems at low absolute temperature and nonequilibrium steady states under high values of the <span class="hlt">heat</span> <span class="hlt">flux</span> are shown, which point to a possible generalization of the third law in nonequilibrium situations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19960023961','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19960023961"><span>An Investigation of the Compatibility of Radiation and Convection <span class="hlt">Heat</span> <span class="hlt">Flux</span> Measurements</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Liebert, Curt H.</p> <p>1996-01-01</p> <p>A method for determining time-resolved absorbed surface <span class="hlt">heat</span> <span class="hlt">flux</span> and surface temperature in radiation and convection environments is described. The method is useful for verification of aerodynamic, <span class="hlt">heat</span> transfer and durability models. A practical <span class="hlt">heat</span> <span class="hlt">flux</span> gage fabrication procedure and a simple one-dimensional inverse <span class="hlt">heat</span> conduction model and calculation procedure are incorporated in this method. The model provides an estimate of the temperature and <span class="hlt">heat</span> <span class="hlt">flux</span> gradient in the direction of <span class="hlt">heat</span> transfer through the gage. This paper discusses several successful time-resolved tests of this method in hostile convective <span class="hlt">heating</span> and cooling environments.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017NucFu..57i2006U','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017NucFu..57i2006U"><span>Baseline high <span class="hlt">heat</span> <span class="hlt">flux</span> and plasma facing materials for fusion</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ueda, Y.; Schmid, K.; Balden, M.; Coenen, J. W.; Loewenhoff, Th.; Ito, A.; Hasegawa, A.; Hardie, C.; Porton, M.; Gilbert, M.</p> <p>2017-09-01</p> <p>In fusion reactors, surfaces of plasma facing components (PFCs) are exposed to high <span class="hlt">heat</span> and particle <span class="hlt">flux</span>. Tungsten and Copper alloys are primary candidates for plasma facing materials (PFMs) and coolant tube materials, respectively, mainly due to high thermal conductivity and, in the case of tungsten, its high melting point. In this paper, recent understandings and future issues on responses of tungsten and Cu alloys to fusion environments (high particle <span class="hlt">flux</span> (including T and He), high <span class="hlt">heat</span> <span class="hlt">flux</span>, and high neutron doses) are reviewed. This review paper includes; Tritium retention in tungsten (K. Schmid and M. Balden), Impact of stationary and transient <span class="hlt">heat</span> loads on tungsten (J.W. Coenen and Th. Loewenhoff), Helium effects on surface morphology of tungsten (Y. Ueda and A. Ito), Neutron radiation effects in tungsten (A. Hasegawa), and Copper and copper alloys development for high <span class="hlt">heat</span> <span class="hlt">flux</span> components (C. Hardie, M. Porton, and M. Gilbert).</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.osti.gov/biblio/22612575-results-high-heat-flux-tests-tungsten-divertor-targets-under-plasma-heat-loads-expected-iter-tokamaks-review','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22612575-results-high-heat-flux-tests-tungsten-divertor-targets-under-plasma-heat-loads-expected-iter-tokamaks-review"><span>Results of high <span class="hlt">heat</span> <span class="hlt">flux</span> tests of tungsten divertor targets under plasma <span class="hlt">heat</span> loads expected in ITER and tokamaks (review)</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>Budaev, V. P., E-mail: budaev@mail.ru</p> <p>2016-12-15</p> <p><span class="hlt">Heat</span> loads on the tungsten divertor targets in the ITER and the tokamak power reactors reach ~10MW m{sup −2} in the steady state of DT discharges, increasing to ~0.6–3.5 GW m{sup −2} under disruptions and ELMs. The results of high <span class="hlt">heat</span> <span class="hlt">flux</span> tests (HHFTs) of tungsten under such transient plasma <span class="hlt">heat</span> loads are reviewed in the paper. The main attention is paid to description of the surface microstructure, recrystallization, and the morphology of the cracks on the target. Effects of melting, cracking of tungsten, drop erosion of the surface, and formation of corrugated and porous layers are observed. Production ofmore » submicron-sized tungsten dust and the effects of the inhomogeneous surface of tungsten on the plasma–<span class="hlt">wall</span> interaction are discussed. In conclusion, the necessity of further HHFTs and investigations of the durability of tungsten under high pulsed plasma loads on the ITER divertor plates, including disruptions and ELMs, is stressed.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1373693-gyrokinetic-projection-divertor-heat-flux-width-from-present-tokamaks-iter','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1373693-gyrokinetic-projection-divertor-heat-flux-width-from-present-tokamaks-iter"><span>Gyrokinetic projection of the divertor <span class="hlt">heat-flux</span> width from present tokamaks to ITER</span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Chang, Choong Seock; Ku, Seung -Hoe; Loarte, Alberto; ...</p> <p>2017-07-11</p> <p>Here, the XGC1 edge gyrokinetic code is used to study the width of the <span class="hlt">heat-flux</span> to divertor plates in attached plasma condition. The <span class="hlt">flux</span>-driven simulation is performed until an approximate power balance is achieved between the <span class="hlt">heat-flux</span> across the steep pedestal pressure gradient and the <span class="hlt">heat-flux</span> on the divertor plates.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/21096099','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/21096099"><span>Theoretical simulation of the dual-<span class="hlt">heat-flux</span> method in deep body temperature measurements.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Huang, Ming; Chen, Wenxi</p> <p>2010-01-01</p> <p>Deep body temperature reveals individual physiological states, and is important in patient monitoring and chronobiological studies. An innovative dual-<span class="hlt">heat-flux</span> method has been shown experimentally to be competitive with the conventional zero-<span class="hlt">heat</span>-flow method in its performance, in terms of measurement accuracy and step response to changes in the deep temperature. We have utilized a finite element method to model and simulate the dynamic process of a dual-<span class="hlt">heat-flux</span> probe in deep body temperature measurements to validate the fundamental principles of the dual-<span class="hlt">heat-flux</span> method theoretically, and to acquire a detailed quantitative description of the thermal profile of the dual-<span class="hlt">heat-flux</span> probe. The simulation results show that the estimated deep body temperature is influenced by the ambient temperature (linearly, at a maximum rate of 0.03 °C/°C) and the blood perfusion rate. The corresponding depth of the estimated temperature in the skin and subcutaneous tissue layer is consistent when using the dual-<span class="hlt">heat-flux</span> probe. Insights in improving the performance of the dual-<span class="hlt">heat-flux</span> method were discussed for further studies of dual-<span class="hlt">heat-flux</span> probes, taking into account structural and geometric considerations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.fs.usda.gov/treesearch/pubs/23962','TREESEARCH'); return false;" href="https://www.fs.usda.gov/treesearch/pubs/23962"><span>A modified force-restore approach to modeling snow-surface <span class="hlt">heat</span> <span class="hlt">fluxes</span></span></a></p> <p><a target="_blank" href="http://www.fs.usda.gov/treesearch/">Treesearch</a></p> <p>Charles H. Luce; David G. Tarboton</p> <p>2001-01-01</p> <p>Accurate modeling of the energy balance of a snowpack requires good estimates of the snow surface temperature. The snow surface temperature allows a balance between atmospheric <span class="hlt">heat</span> <span class="hlt">fluxes</span> and the conductive <span class="hlt">flux</span> into the snowpack. While the dependency of atmospheric <span class="hlt">fluxes</span> on surface temperature is reasonably well understood and parameterized, conduction of <span class="hlt">heat</span> from...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2002mwoc.conf...39M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2002mwoc.conf...39M"><span>Contagious Coronal <span class="hlt">Heating</span> from Recurring Emergence of Magnetic <span class="hlt">Flux</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Moore, R. L.; Falconer, D. A.; Sterling, A. C.</p> <p>2002-01-01</p> <p>For each of six old bipolar active regions, we present and interpret Yohkoh/SXT and SOHO/MDI observations of the development, over several days, of enhanced coronal <span class="hlt">heating</span> in and around the old bipole in response to new magnetic <span class="hlt">flux</span> emergence within the old bipole. The observations show: 1. In each active region, new <span class="hlt">flux</span> emerges in the equatorward side of the old bipole, around a lone remaining leading sunspot and/or on the equatorward end of the neutral line of the old bipole. 2. The emerging field is marked by intense internal coronal <span class="hlt">heating</span>, and enhanced coronal <span class="hlt">heating</span> occurs in extended loops stemming from the emergence site. 3. In five of the six cases, a "rooster tail" of coronal loops in the poleward extent of the old bipole also brightens in response to the <span class="hlt">flux</span> emergence. 4. There are episodes of enhanced coronal <span class="hlt">heating</span> in surrounding magnetic fields that are contiguous with the old bipole but are not directly connected to the emerging field. From these observations, we suggest that the accommodation of localized newly emerged <span class="hlt">flux</span> within an old active region entails far reaching adjustments in the 3D magnetic field throughout the active region and in surrounding fields in which the active region is embedded, and that these adjustments produce the extensive enhanced coronal <span class="hlt">heating</span>. We Also Note That The Reason For The recurrence of <span class="hlt">flux</span> emergence in old active regions may be that active-region <span class="hlt">flux</span> tends to emerge in giant-cell convection downflows. If so, the poleward "rooster tail" is a coronal flag of a long-lasting downflow in the convection zone. This work was funded by NASA's Office of Space Science through the Solar Physics Supporting Research and Technology Program and the Sun-Earth Connection Guest Investigator Program.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20020022350&hterms=Magnetic+Flux&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3DMagnetic%2BFlux','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20020022350&hterms=Magnetic+Flux&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3DMagnetic%2BFlux"><span>Contagious Coronal <span class="hlt">Heating</span> from Recurring Emergence of Magnetic <span class="hlt">Flux</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Moore, Ronald L.; Falconer, David; Sterling, Alphonse; Whitaker, Ann F. (Technical Monitor)</p> <p>2001-01-01</p> <p>For each of six old bipolar active regions, we present and interpret Yohkoh/SXT and SOHO/MDI observations of the development, over several days, of enhanced coronal <span class="hlt">heating</span> in and around the old bipole in response to new magnetic <span class="hlt">flux</span> emerge= within the old bipole. The observations show: 1. In each active region, new <span class="hlt">flux</span> emerges in the equatorward side of the old bipole, around a lone remaining leading sunspot and/or on the equatorward end of the neutral line of the old bipole. 2. The emerging field is marked by intense internal coronal <span class="hlt">heating</span>, and enhanced coronal <span class="hlt">heating</span> occurs in extended loops stemming from the emergence site. 3. In five of the six cases, a "rooster tail" of coronal loops in the poleward extent of the old bipole also brightens in response to the <span class="hlt">flux</span> emergence. 4. There are episodes of enhanced coronal <span class="hlt">heating</span> in surrounding magnetic fields that are contiguous with the old bipole but are not directly connected to the emerging field. From these observations, we suggest that the accommodation of localized newly emerged <span class="hlt">flux</span> within an old active region entails far reaching adjustments in the 3D magnetic field throughout the active region and in surrounding fields in which the active region is embedded, and that these adjustments produce the extensive enhanced coronal <span class="hlt">heating</span>. We also note that the reason for the recurrence of <span class="hlt">flux</span> emergence in old active regions may be that active region <span class="hlt">flux</span> tends to emerge in giant-cell convection downflows. If so, the poleward "rooster tail" is a coronal flag of a long-lasting downflow in the convection zone. This work was funded by NASA's Office of Space Science through the Solar Physics Supporting Research and Technology Program and the Sun-Earth Connection Guest Investigator Program.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19840023491','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19840023491"><span>Electroless-plating technique for fabricating thin-<span class="hlt">wall</span> convective <span class="hlt">heat</span>-transfer models</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Avery, D. E.; Ballard, G. K.; Wilson, M. L.</p> <p>1984-01-01</p> <p>A technique for fabricating uniform thin-<span class="hlt">wall</span> metallic <span class="hlt">heat</span>-transfer models and which simulates a Shuttle thermal protection system tile is described. Two 6- by 6- by 2.5-in. tiles were fabricated to obtain local <span class="hlt">heat</span> transfer rates. The fabrication process is not limited to any particular geometry and results in a seamless thin-<span class="hlt">wall</span> <span class="hlt">heat</span>-transfer model which uses a one-wire thermocouple to obtain local cold-<span class="hlt">wall</span> <span class="hlt">heat</span>-transfer rates. The tile is relatively fragile because of the brittle nature of the material and the structural weakness of the flat-sided configuration; however, a method was developed and used for repairing a cracked tile.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015APS..DPPJO5002H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015APS..DPPJO5002H"><span><span class="hlt">Heat-Flux</span> Measurements from Collective Thomson-Scattering Spectra</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Henchen, R. J.; Hu, S. X.; Katz, J.; Froula, D. H.; Rozmus, W.</p> <p>2015-11-01</p> <p>Collective Thomson scattering was used to measure <span class="hlt">heat</span> <span class="hlt">flux</span> in coronal plasmas. The relative amplitude of the Thomson-scattered power into the up- and downshifted electron plasma wave features was used to determine the <span class="hlt">flux</span> of electrons moving along the temperature gradient at three to four times the electron thermal velocity. Simultaneously, the ion-acoustic wave features were measured. Their relative amplitude is used to measure the <span class="hlt">flux</span> of the return-current electrons. The frequencies of these ion-acoustic and electron plasma wave features provide local measurements of the electron temperature and density. These spectra were obtained at five locations along the temperature gradient in a laser-produced blowoff plasma. These measurements of plasma parameters are used to infer the Spitzer -Härm <span class="hlt">flux</span> <m:mfenced close=")" open="(" separators="">qSH = - κ∇Te </m:mfenced> and are in good agreement with the values of the <span class="hlt">heat</span> <span class="hlt">flux</span> measured from the scattering-feature asymmetries. This material is based upon work supported by the Department of Energy National Nuclear Security Administration under Award Number DE-NA0001944.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/21233734-measurement-gas-species-temperatures-coal-burnout-wall-heat-fluxes-mwe-lignite-fired-boiler-different-overfire-air-damper-openings','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/21233734-measurement-gas-species-temperatures-coal-burnout-wall-heat-fluxes-mwe-lignite-fired-boiler-different-overfire-air-damper-openings"><span>Measurement of gas species, temperatures, coal burnout, and <span class="hlt">wall</span> <span class="hlt">heat</span> <span class="hlt">fluxes</span> in a 200 MWe lignite-fired boiler with different overfire air damper openings</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>Jianping Jing; Zhengqi Li; Guangkui Liu</p> <p></p> <p>Measurements were performed on a 200 MWe, <span class="hlt">wall</span>-fired, lignite utility boiler. For different overfire air (OFA) damper openings, the gas temperature, gas species concentration, coal burnout, release rates of components (C, H, and N), furnace temperature, and <span class="hlt">heat</span> <span class="hlt">flux</span> and boiler efficiency were measured. Cold air experiments for a single burner were conducted in the laboratory. The double-swirl flow pulverized-coal burner has two ring recirculation zones starting in the secondary air region in the burner. As the secondary air flow increases, the axial velocity of air flow increases, the maxima of radial velocity, tangential velocity and turbulence intensity all increase,more » and the swirl intensity of air flow and the size of recirculation zones increase slightly. In the central region of the burner, as the OFA damper opening widens, the gas temperature and CO concentration increase, while the O{sub 2} concentration, NOx concentration, coal burnout, and release rates of components (C, H, and N) decrease, and coal particles ignite earlier. In the secondary air region of the burner, the O{sub 2} concentration, NOx concentration, coal burnout, and release rates of components (C, H, and N) decrease, and the gas temperature and CO concentration vary slightly. In the sidewall region, the gas temperature, O{sub 2} concentration, and NOx concentration decrease, while the CO concentration increases and the gas temperature varies slightly. The furnace temperature and <span class="hlt">heat</span> <span class="hlt">flux</span> in the main burning region decrease appreciably, but increase slightly in the burnout region. The NOx emission decreases from 1203.6 mg/m{sup 3} (6% O{sub 2}) for a damper opening of 0% to 511.7 mg/m{sup 3} (6% O{sub 2}) for a damper opening of 80% and the boiler efficiency decreases from 92.59 to 91.9%. 15 refs., 17 figs., 3 tabs.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19860002759','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19860002759"><span>Turbine blade and vane <span class="hlt">heat</span> <span class="hlt">flux</span> sensor development, phase 2</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Atkinson, W. H.; Cyr, M. A.; Strange, R. R.</p> <p>1985-01-01</p> <p>The development of <span class="hlt">heat</span> <span class="hlt">flux</span> sensors for gas turbine blades and vanes and the demonstration of <span class="hlt">heat</span> transfer measurement methods are reported. The performance of the <span class="hlt">heat</span> <span class="hlt">flux</span> sensors was evaluated in a cylinder in cross flow experiment and compared with two other <span class="hlt">heat</span> <span class="hlt">flux</span> measurement methods, the slug calorimeter and a dynamic method based on fluctuating gas and surface temperature. Two cylinders, each instrumented with an embedded thermocouple sensor, a Gardon gauge, and a slug calorimeter, were fabricated. Each sensor type was calibrated using a quartz lamp bank facility. The instrumented cylinders were then tested in an atmospheric pressure combustor rig at conditions up to gas stream temperatures of 1700K and velocities to Mach 0.74. The test data are compared to other measurements and analytical prediction.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMGC21D0970Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMGC21D0970Z"><span>Two-wavelength Method Estimates <span class="hlt">Heat</span> <span class="hlt">fluxes</span> over Heterogeneous Surface in North-China</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zhang, G.; Zheng, N.; Zhang, J.</p> <p>2017-12-01</p> <p><span class="hlt">Heat</span> <span class="hlt">fluxes</span> is a key process of hydrological and <span class="hlt">heat</span> transfer of soil-plant-atmosphere continuum (SPAC), and now it is becoming an important topic in meteorology, hydrology, ecology and other related research areas. Because the temporal and spatial variation of <span class="hlt">fluxes</span> at regional scale is very complicated, it is still difficult to measure <span class="hlt">fluxes</span> at the kilometer scale over a heterogeneous surface. A technique called "two-wavelength method" which combines optical scintillometer with microwave scintillometer is able to measure both sensible and latent <span class="hlt">heat</span> <span class="hlt">fluxes</span> over large spatial scales at the same time. The main purpose of this study is to investigate the <span class="hlt">fluxes</span> over non-uniform terrain in North-China. Estimation of <span class="hlt">heat</span> <span class="hlt">fluxes</span> was carried out with the optical-microwave scintillometer and an eddy covariance (EC) system over heterogeneous surface in Tai Hang Mountains, China. EC method was set as a benchmark in the study. Structure parameters obtained from scintillometer showed that the typical measurement values of Cn2 are around 10-13 m-2/3 for microwave scintillometer, and values of Cn2 were around 10-15 m-2/3 for optical scintillometer. The correlation of <span class="hlt">heat</span> <span class="hlt">fluxes</span> (H) derived from scintillometer and EC system showed as a ratio of 1.05,and with R2=0.75, while the correlation of latent <span class="hlt">heat</span> <span class="hlt">fluxes</span> (LE) showed as 1.29 with R2=0.67. It was also found that <span class="hlt">heat</span> <span class="hlt">fluxes</span> derived from the two system showed good agreement (R2=0.9 for LE, R2=0.97 for H) when the Bowen ratio (β) was 1.03, while discrepancies showed significantly when β=0.75, and RMSD in H was 139.22 W/m2, 230.85 W/m2 in LE respectively.Experiment results in our research shows that, the two-wavelength method gives a larger <span class="hlt">heat</span> <span class="hlt">fluxes</span> over the study area, and a deeper study should be conduct. We expect that our investigate and analysis can be promoted the application of scintillometry method in regional evapotranspiration measurements and relevant disciplines.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/21401346-experimental-investigation-heat-transfer-frictional-characteristics-vertical-upward-rifled-tube-supercritical-cfb-boiler','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/21401346-experimental-investigation-heat-transfer-frictional-characteristics-vertical-upward-rifled-tube-supercritical-cfb-boiler"><span>Experimental investigation on <span class="hlt">heat</span> transfer and frictional characteristics of vertical upward rifled tube in supercritical CFB boiler</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>Yang, Dong; Pan, Jie; Zhu, Xiaojing</p> <p>2011-02-15</p> <p>Water <span class="hlt">wall</span> design is a key issue for supercritical Circulating Fluidized Bed (CFB) boiler. On account of the good <span class="hlt">heat</span> transfer performance, rifled tube is applied in the water <span class="hlt">wall</span> design of a 600 MW supercritical CFB boiler in China. In order to investigate the <span class="hlt">heat</span> transfer and frictional characteristics of the rifled tube with vertical upward flow, an in-depth experiment was conducted in the range of pressure from 12 to 30 MPa, mass <span class="hlt">flux</span> from 230 to 1200 kg/(m{sup 2} s), and inner <span class="hlt">wall</span> <span class="hlt">heat</span> <span class="hlt">flux</span> from 130 to 720 kW/m{sup 2}. The <span class="hlt">wall</span> temperature distribution and pressure dropmore » in the rifled tube were obtained in the experiment. The normal, enhanced and deteriorated <span class="hlt">heat</span> transfer characteristics were also captured. In this paper, the effects of pressure, inner <span class="hlt">wall</span> <span class="hlt">heat</span> <span class="hlt">flux</span> and mass <span class="hlt">flux</span> on <span class="hlt">heat</span> transfer characteristics are analyzed, the <span class="hlt">heat</span> transfer mechanism and the frictional resistance performance are discussed, and the corresponding empirical correlations are presented. The experimental results show that the rifled tube can effectively prevent the occurrence of departure from nucleate boiling (DNB) and keep the tube <span class="hlt">wall</span> temperature in a permissible range under the operating condition of supercritical CFB boiler. (author)« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018HMT....54.2089I','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018HMT....54.2089I"><span>Studies on <span class="hlt">heat</span> transfer and pressure drop in turbulent flow of silver - water nanofluids through a circular tube at constant <span class="hlt">wall</span> <span class="hlt">heat</span> <span class="hlt">flux</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Iyahraja, S.; Rajadurai, J. Selwin; Rajesh, S.; Pandian, R. Seeni Thangaraj; Kumaran, M. Selva; Selvakumar, G.</p> <p>2018-07-01</p> <p>In the present study, performance of convective <span class="hlt">heat</span> transfer and friction factor of silver-water nanofluids in a horizontal circular pipe under turbulent flow were investigated experimentally under uniform <span class="hlt">heat</span> <span class="hlt">flux</span> condition. The volume concentration of silver nanoparticles is varied as 0.01, 0.05 and 0.1%. <span class="hlt">Heat</span> transfer coefficient and friction factor of nanofluids were measured experimentally by varying the Reynolds number from 3000 to 21,000. It is observed that the addition of even low volume fraction of silver nanoparticles increases both Nusselt number and <span class="hlt">heat</span> transfer coefficient of the nanofluid significantly. Nusselt number of silver-water nanofluid increases up to 32.6% for 0.1% volume fraction at Reynolds number of 21,000. However, the addition of nanoparticles in the base fluid increases the friction factor slightly. New empirical correlations are also proposed for the estimation of Nusselt number and friction factor of silver-water nanofluid based on the data of present experimental investigation. The proposed correlations of Nusselt number and friction factor show good agreement with their experimental data.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018HMT...tmp...38I','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018HMT...tmp...38I"><span>Studies on <span class="hlt">heat</span> transfer and pressure drop in turbulent flow of silver - water nanofluids through a circular tube at constant <span class="hlt">wall</span> <span class="hlt">heat</span> <span class="hlt">flux</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Iyahraja, S.; Rajadurai, J. Selwin; Rajesh, S.; Pandian, R. Seeni Thangaraj; Kumaran, M. Selva; Selvakumar, G.</p> <p>2018-02-01</p> <p>In the present study, performance of convective <span class="hlt">heat</span> transfer and friction factor of silver-water nanofluids in a horizontal circular pipe under turbulent flow were investigated experimentally under uniform <span class="hlt">heat</span> <span class="hlt">flux</span> condition. The volume concentration of silver nanoparticles is varied as 0.01, 0.05 and 0.1%. <span class="hlt">Heat</span> transfer coefficient and friction factor of nanofluids were measured experimentally by varying the Reynolds number from 3000 to 21,000. It is observed that the addition of even low volume fraction of silver nanoparticles increases both Nusselt number and <span class="hlt">heat</span> transfer coefficient of the nanofluid significantly. Nusselt number of silver-water nanofluid increases up to 32.6% for 0.1% volume fraction at Reynolds number of 21,000. However, the addition of nanoparticles in the base fluid increases the friction factor slightly. New empirical correlations are also proposed for the estimation of Nusselt number and friction factor of silver-water nanofluid based on the data of present experimental investigation. The proposed correlations of Nusselt number and friction factor show good agreement with their experimental data.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19930022365','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19930022365"><span>Thin film <span class="hlt">heat</span> <span class="hlt">flux</span> sensor for Space Shuttle Main Engine turbine environment</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Will, Herbert</p> <p>1991-01-01</p> <p>The Space Shuttle Main Engine (SSME) turbine environment stresses engine components to their design limits and beyond. The extremely high temperatures and rapid temperature cycling can easily cause parts to fail if they are not properly designed. Thin film <span class="hlt">heat</span> <span class="hlt">flux</span> sensors can provide <span class="hlt">heat</span> loading information with almost no disturbance of gas flows or of the blade. These sensors can provide steady state and transient <span class="hlt">heat</span> <span class="hlt">flux</span> information. A thin film <span class="hlt">heat</span> <span class="hlt">flux</span> sensor is described which makes it easier to measure small temperature differences across very thin insulating layers.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/761855','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/761855"><span>Recent High <span class="hlt">Heat</span> <span class="hlt">Flux</span> Tests on W-Rod-Armored Mockups</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>NYGREN,RICHARD E.; YOUCHISON,DENNIS L.; MCDONALD,JIMMIE M.</p> <p>2000-07-18</p> <p>In the authors initial high <span class="hlt">heat</span> <span class="hlt">flux</span> tests on small mockups armored with W rods, done in the small electron beam facility (EBTS) at Sandia National Laboratories, the mockups exhibited excellent thermal performance. However, to reach high <span class="hlt">heat</span> <span class="hlt">fluxes</span>, they reduced the <span class="hlt">heated</span> area to only a portion ({approximately}25%) of the sample. They have now begun tests in their larger electron beam facility, EB 1200, where the available power (1.2 MW) is more than enough to <span class="hlt">heat</span> the entire surface area of the small mockups. The initial results indicate that, at a given power, the surface temperatures of rods inmore » the EB 1200 tests is somewhat higher than was observed in the EBTS tests. Also, it appears that one mockup (PW-10) has higher surface temperatures than other mockups with similar height (10mm) W rods, and that the previously reported values of absorbed <span class="hlt">heat</span> <span class="hlt">flux</span> on this mockup were too high. In the tests in EB 1200 of a second mockup, PW-4, absorbed <span class="hlt">heat</span> <span class="hlt">fluxes</span> of {approximately}22MW/m{sup 2} were reached but the corresponding surface temperatures were somewhat higher than in EBTS. A further conclusion is that the simple 1-D model initially used in evaluating some of the results from the EBTS testing was not adequate, and 3-D thermal modeling will be needed to interpret the results.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/6080374-comparison-heat-exchanger-solar-block-wall-swine-nursery','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/6080374-comparison-heat-exchanger-solar-block-wall-swine-nursery"><span>Comparison of <span class="hlt">heat</span> exchanger and solar block <span class="hlt">wall</span> in a swine nursery</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>Jones, D.D.; Friday, W.H.; Thieme, R.H.</p> <p>1984-01-01</p> <p>A pig nursery building was divided into two equal rooms, one with a <span class="hlt">heat</span> exchanger and one with a solar block <span class="hlt">wall</span>. The average air inlet temperatures were 16.4/sup 0/C in the <span class="hlt">heat</span> exchanger room and 11.9/sup 0/C in the solar <span class="hlt">heated</span> room. Supplemental <span class="hlt">heating</span> costs were 67% higher in the solar block <span class="hlt">wall</span> room.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JGRC..122.4569M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JGRC..122.4569M"><span>Mixing rates and vertical <span class="hlt">heat</span> <span class="hlt">fluxes</span> north of Svalbard from Arctic winter to spring</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Meyer, Amelie; Fer, Ilker; Sundfjord, Arild; Peterson, Algot K.</p> <p>2017-06-01</p> <p>Mixing and <span class="hlt">heat</span> <span class="hlt">flux</span> rates collected in the Eurasian Basin north of Svalbard during the N-ICE2015 drift expedition are presented. The observations cover the deep Nansen Basin, the Svalbard continental slope, and the shallow Yermak Plateau from winter to summer. Mean quiescent winter <span class="hlt">heat</span> <span class="hlt">flux</span> values in the Nansen Basin are 2 W m-2 at the ice-ocean interface, 3 W m-2 in the pycnocline, and 1 W m-2 below the pycnocline. Large <span class="hlt">heat</span> <span class="hlt">fluxes</span> exceeding 300 W m-2 are observed in the late spring close to the surface over the Yermak Plateau. The data consisting of 588 microstructure profiles and 50 days of high-resolution under-ice turbulence measurements are used to quantify the impact of several forcing factors on turbulent dissipation and <span class="hlt">heat</span> <span class="hlt">flux</span> rates. Wind forcing increases turbulent dissipation seven times in the upper 50 m, and doubles <span class="hlt">heat</span> <span class="hlt">fluxes</span> at the ice-ocean interface. The presence of warm Atlantic Water close to the surface increases the temperature gradient in the water column, leading to enhanced <span class="hlt">heat</span> <span class="hlt">flux</span> rates within the pycnocline. Steep topography consistently enhances dissipation rates by a factor of four and episodically increases <span class="hlt">heat</span> <span class="hlt">flux</span> at depth. It is, however, the combination of storms and shallow Atlantic Water that leads to the highest <span class="hlt">heat</span> <span class="hlt">flux</span> rates observed: ice-ocean interface <span class="hlt">heat</span> <span class="hlt">fluxes</span> average 100 W m-2 during peak events and are associated with rapid basal sea ice melt, reaching 25 cm/d.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2004SuMi...35..543M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2004SuMi...35..543M"><span><span class="hlt">Heat</span> transfer behaviours of nanofluids in a uniformly <span class="hlt">heated</span> tube</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Maı̈ga, Sidi El Bécaye; Nguyen, Cong Tam; Galanis, Nicolas; Roy, Gilles</p> <p>2004-03-01</p> <p>In the present work, we consider the problem of the forced convection flow of water- γAl 2O 3 and ethylene glycol- γAl 2O 3 nanofluids inside a uniformly <span class="hlt">heated</span> tube that is submitted to a constant and uniform <span class="hlt">heat</span> <span class="hlt">flux</span> at the <span class="hlt">wall</span>. In general, it is observed that the inclusion of nanoparticles has increased considerably the <span class="hlt">heat</span> transfer at the tube <span class="hlt">wall</span> for both the laminar and turbulent regimes. Such improvement of <span class="hlt">heat</span> transfer becomes more pronounced with the increase of the particle concentration. On the other hand, the presence of particles has produced adverse effects on the <span class="hlt">wall</span> friction that also increases with the particle volume concentration. Results have also shown that the ethylene glycol- γAl 2O 3 mixture gives a far better <span class="hlt">heat</span> transfer enhancement than the water- γAl 2O 3 mixture.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..1917050Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..1917050Z"><span>Mesoscale eddies control meridional <span class="hlt">heat</span> <span class="hlt">flux</span> variability in the subpolar North Atlantic</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zhao, Jian; Bower, Amy; Yang, Jiayan; Lin, Xiaopei; Zhou, Chun</p> <p>2017-04-01</p> <p>The meridional <span class="hlt">heat</span> <span class="hlt">flux</span> in the subpolar North Atlantic is vital to the climate of the high-latitude North Atlantic. For the basinwide <span class="hlt">heat</span> <span class="hlt">flux</span> across a section between Greenland and Scotland, much of the variability occurs in the Iceland basin, where the North Atlantic Current (NAC) carries relatively warm and salty water northward. As a component of the Overturning in the Subpolar North Atlantic Program (OSNAP), WHOI and OUC are jointly operating gliders in the Iceland Basin to continuously monitor the circulation and corresponding <span class="hlt">heat</span> <span class="hlt">flux</span> in this eddy-rich region. Based on one year of observations, two circulation regimes in the Iceland basin have been identified: a mesoscale eddy like circulation pattern and northward NAC circulation pattern. When a mesoscale eddy is generated, the rotational currents associated with the eddy lead to both northward and southward flow in the Iceland basin. This is quite different from the broad northward flow associated with the NAC when there is no eddy. The transition between the two regimes coupled with the strong temperature front in the Iceland basin can modify the meridional <span class="hlt">heat</span> <span class="hlt">flux</span> on the order of 0.3PW, which is the dominant source for the <span class="hlt">heat</span> <span class="hlt">flux</span> change the Iceland Basin. According to high-resolution numerical model results, the Iceland Basin has the largest contribution to the meridional <span class="hlt">heat</span> <span class="hlt">flux</span> variability along the section between Greenland and Scotland. Therefore, mesoscale eddies in the Iceland Basin provide important dynamics to control the meridional <span class="hlt">heat</span> <span class="hlt">flux</span> variability in the subpolar North Atlantic.</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('https://www.ncbi.nlm.nih.gov/pubmed/27285827','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27285827"><span>Experimental Methodology for Estimation of Local <span class="hlt">Heat</span> <span class="hlt">Fluxes</span> and Burning Rates in Steady Laminar Boundary Layer Diffusion Flames.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Singh, Ajay V; Gollner, Michael J</p> <p>2016-06-01</p> <p>Modeling the realistic burning behavior of condensed-phase fuels has remained out of reach, in part because of an inability to resolve the complex interactions occurring at the interface between gas-phase flames and condensed-phase fuels. The current research provides a technique to explore the dynamic relationship between a combustible condensed fuel surface and gas-phase flames in laminar boundary layers. Experiments have previously been conducted in both forced and free convective environments over both solid and liquid fuels. A unique methodology, based on the Reynolds Analogy, was used to estimate local mass burning rates and flame <span class="hlt">heat</span> <span class="hlt">fluxes</span> for these laminar boundary layer diffusion flames utilizing local temperature gradients at the fuel surface. Local mass burning rates and convective and radiative <span class="hlt">heat</span> feedback from the flames were measured in both the pyrolysis and plume regions by using temperature gradients mapped near the <span class="hlt">wall</span> by a two-axis traverse system. These experiments are time-consuming and can be challenging to design as the condensed fuel surface burns steadily for only a limited period of time following ignition. The temperature profiles near the fuel surface need to be mapped during steady burning of a condensed fuel surface at a very high spatial resolution in order to capture reasonable estimates of local temperature gradients. Careful corrections for radiative <span class="hlt">heat</span> losses from the thermocouples are also essential for accurate measurements. For these reasons, the whole experimental setup needs to be automated with a computer-controlled traverse mechanism, eliminating most errors due to positioning of a micro-thermocouple. An outline of steps to reproducibly capture near-<span class="hlt">wall</span> temperature gradients and use them to assess local burning rates and <span class="hlt">heat</span> <span class="hlt">fluxes</span> is provided.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1164318','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/1164318"><span>Institute for High <span class="hlt">Heat</span> <span class="hlt">Flux</span> Removal (IHHFR). Phases I, II, and III</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>Boyd, Ronald D.</p> <p>2014-08-31</p> <p>The IHHFR focused on interdisciplinary applications as it relates to high <span class="hlt">heat</span> <span class="hlt">flux</span> engineering issues and problems which arise due to engineering systems being miniaturized, optimized, or requiring increased high <span class="hlt">heat</span> <span class="hlt">flux</span> performance. The work in the IHHFR focused on water as a coolant and includes: (1) the development, design, and construction of the high <span class="hlt">heat</span> <span class="hlt">flux</span> flow loop and facility; (2) test section development, design, and fabrication; and, (3) single-side <span class="hlt">heat</span> <span class="hlt">flux</span> experiments to produce 2-D boiling curves and 3-D conjugate <span class="hlt">heat</span> transfer measurements for single-side <span class="hlt">heated</span> test sections. This work provides data for comparisons with previously developed andmore » new single-side <span class="hlt">heated</span> correlations and approaches that address the single-side <span class="hlt">heated</span> effect on <span class="hlt">heat</span> transfer. In addition, this work includes the addition of single-side <span class="hlt">heated</span> circular TS and a monoblock test section with a helical wire insert. Finally, the present work includes: (1) data base expansion for the monoblock with a helical wire insert (only for the latter geometry), (2) prediction and verification using finite element, (3) monoblock model and methodology development analyses, and (4) an alternate model development for a hypervapotron and related conjugate <span class="hlt">heat</span> transfer controlling parameters.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012AGUFM.C43A0587P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012AGUFM.C43A0587P"><span><span class="hlt">Heat</span> <span class="hlt">flux</span> variations over sea-ice observed at the coastal area of the Sejong Station, Antarctica</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Park, S.; Choi, T.; Kim, S.</p> <p>2012-12-01</p> <p>This study presents variations of sensible <span class="hlt">heat</span> <span class="hlt">flux</span> and latent <span class="hlt">heat</span> <span class="hlt">flux</span> over sea-ice observed in 2011 from the 10-m <span class="hlt">flux</span> tower located at the coast of the Sejong Station on King George Island, Antarctica. A period from June to November was divided into three parts: "Freezing", "Frozen", and "Melting" periods based on daily monitoring of sea state and hourly photos looking at the Marian Cove in front of the Sejong Station. The division of periods enabled us to look into the <span class="hlt">heat</span> <span class="hlt">flux</span> variations depending on the sea-ice conditions. Over freezing sea surface during the freezing period of late June, daily mean sensible <span class="hlt">heat</span> <span class="hlt">flux</span> was -11.9 Wm-2 and daily mean latent <span class="hlt">heat</span> <span class="hlt">flux</span> was +16.3 Wm-2. Over the frozen sea-ice, daily mean sensible <span class="hlt">heat</span> <span class="hlt">flux</span> was -10.4 Wm-2 while daily mean latent <span class="hlt">heat</span> <span class="hlt">flux</span> was +2.4 Wm-2. During the melting period of mid-October to early November, magnitudes of sensible <span class="hlt">heat</span> <span class="hlt">flux</span> increased to -14.2 Wm-2 and latent <span class="hlt">heat</span> <span class="hlt">flux</span> also increased to +13.5 Wm-2. In short, latent <span class="hlt">heat</span> <span class="hlt">flux</span> was usually upward over sea-ice most of the time while sensible <span class="hlt">heat</span> <span class="hlt">flux</span> was downward from atmosphere to sea-ice. Magnitudes of the <span class="hlt">fluxes</span> were small but increased when freezing or melting of sea-ice was occurring. Especially, latent <span class="hlt">heat</span> <span class="hlt">flux</span> increased five to six times compared to that of "frozen" period implying that early melting of sea-ice may cause five to six times larger supply of moisture to the atmosphere.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/1130204-interaction-between-marine-boundary-layer-cellular-cloudiness-surface-heat-fluxes','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/1130204-interaction-between-marine-boundary-layer-cellular-cloudiness-surface-heat-fluxes"><span>On the Interaction between Marine Boundary Layer Cellular Cloudiness and Surface <span class="hlt">Heat</span> <span class="hlt">Fluxes</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>Kazil, J.; Feingold, G.; Wang, Hailong</p> <p>2014-01-02</p> <p>The interaction between marine boundary layer cellular cloudiness and surface uxes of sensible and latent <span class="hlt">heat</span> is investigated. The investigation focuses on the non-precipitating closed-cell state and the precipitating open-cell state at low geostrophic wind speed. The Advanced Research WRF model is used to conduct cloud-system-resolving simulations with interactive surface <span class="hlt">fluxes</span> of sensible <span class="hlt">heat</span>, latent <span class="hlt">heat</span>, and of sea salt aerosol, and with a detailed representation of the interaction between aerosol particles and clouds. The mechanisms responsible for the temporal evolution and spatial distribution of the surface <span class="hlt">heat</span> <span class="hlt">fluxes</span> in the closed- and open-cell state are investigated and explained. Itmore » is found that the horizontal spatial structure of the closed-cell state determines, by entrainment of dry free tropospheric air, the spatial distribution of surface air temperature and water vapor, and, to a lesser degree, of the surface sensible and latent <span class="hlt">heat</span> <span class="hlt">flux</span>. The synchronized dynamics of the the open-cell state drives oscillations in surface air temperature, water vapor, and in the surface <span class="hlt">fluxes</span> of sensible and latent <span class="hlt">heat</span>, and of sea salt aerosol. Open-cell cloud formation, cloud optical depth and liquid water path, and cloud and rain water path are identified as good predictors of the spatial distribution of surface air temperature and sensible <span class="hlt">heat</span> <span class="hlt">flux</span>, but not of surface water vapor and latent <span class="hlt">heat</span> <span class="hlt">flux</span>. It is shown that by enhancing the surface sensible <span class="hlt">heat</span> <span class="hlt">flux</span>, the open-cell state creates conditions by which it is maintained. While the open-cell state under consideration is not depleted in aerosol, and is insensitive to variations in sea-salt <span class="hlt">fluxes</span>, it also enhances the sea-salt <span class="hlt">flux</span> relative to the closed-cell state. In aerosol-depleted conditions, this enhancement may replenish the aerosol needed for cloud formation, and hence contribute to the perpetuation of the open-cell state as well. Spatial homogenization of the surface <span class="hlt">fluxes</span> is found</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018MicNa...4....1H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018MicNa...4....1H"><span>Nanoporous membrane device for ultra high <span class="hlt">heat</span> <span class="hlt">flux</span> thermal management</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hanks, Daniel F.; Lu, Zhengmao; Sircar, Jay; Salamon, Todd R.; Antao, Dion S.; Bagnall, Kevin R.; Barabadi, Banafsheh; Wang, Evelyn N.</p> <p>2018-02-01</p> <p>High power density electronics are severely limited by current thermal management solutions which are unable to dissipate the necessary <span class="hlt">heat</span> <span class="hlt">flux</span> while maintaining safe junction temperatures for reliable operation. We designed, fabricated, and experimentally characterized a microfluidic device for ultra-high <span class="hlt">heat</span> <span class="hlt">flux</span> dissipation using evaporation from a nanoporous silicon membrane. With 100 nm diameter pores, the membrane can generate high capillary pressure even with low surface tension fluids such as pentane and R245fa. The suspended ultra-thin membrane structure facilitates efficient liquid transport with minimal viscous pressure losses. We fabricated the membrane in silicon using interference lithography and reactive ion etching and then bonded it to a high permeability silicon microchannel array to create a biporous wick which achieves high capillary pressure with enhanced permeability. The back side consisted of a thin film platinum heater and resistive temperature sensors to emulate the <span class="hlt">heat</span> dissipation in transistors and measure the temperature, respectively. We experimentally characterized the devices in pure vapor-ambient conditions in an environmental chamber. Accordingly, we demonstrated <span class="hlt">heat</span> <span class="hlt">fluxes</span> of 665 ± 74 W/cm2 using pentane over an area of 0.172 mm × 10 mm with a temperature rise of 28.5 ± 1.8 K from the <span class="hlt">heated</span> substrate to ambient vapor. This <span class="hlt">heat</span> <span class="hlt">flux</span>, which is normalized by the evaporation area, is the highest reported to date in the pure evaporation regime, that is, without nucleate boiling. The experimental results are in good agreement with a high fidelity model which captures <span class="hlt">heat</span> conduction in the suspended membrane structure as well as non-equilibrium and sub-continuum effects at the liquid-vapor interface. This work suggests that evaporative membrane-based approaches can be promising towards realizing an efficient, high <span class="hlt">flux</span> thermal management strategy over large areas for high-performance electronics.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19970000389','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19970000389"><span>Evaporation on/in Capillary Structures of High <span class="hlt">Heat</span> <span class="hlt">Flux</span> Two-Phase Devices</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Faghri, Amir; Khrustalev, Dmitry</p> <p>1996-01-01</p> <p>Two-phase devices (<span class="hlt">heat</span> pipes, capillary pumped loops, loop <span class="hlt">heat</span> pipes, and evaporators) have become recognized as key elements in thermal control systems of space platforms. Capillary and porous structures are necessary and widely used in these devices, especially in high <span class="hlt">heat</span> <span class="hlt">flux</span> and zero-g applications, to provide fluid transport and enhanced <span class="hlt">heat</span> transfer during vaporization and condensation. However, some unexpected critical phenomena, such as dryout in long <span class="hlt">heat</span> pipe evaporators and high thermal resistance of loop <span class="hlt">heat</span> pipe evaporators with high <span class="hlt">heat</span> <span class="hlt">fluxes</span>, are possible and have been encountered in the use of two-phase devices in the low gravity environment. Therefore, a detailed fundamental investigation is proposed to better understand the fluid behavior in capillary-porous structures during vaporization at high <span class="hlt">heat</span> <span class="hlt">fluxes</span>. The present paper addresses some theoretical aspects of this investigation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1995SPIE.2586..241X','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1995SPIE.2586..241X"><span><span class="hlt">Heat</span> <span class="hlt">flux</span> exchange estimation by using ATSR SST data in TOGA area</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Xue, Yong; Lawrence, Sean P.; Llewellyn-Jones, David T.</p> <p>1995-12-01</p> <p>The study of phenomena such as ENSO requires consideration of the dynamics and thermodynamics of the coupled ocean-atmosphere system. The dynamic and thermal properties of the atmosphere and ocean are directly affected by air-sea transfers of <span class="hlt">fluxes</span> of momentum, <span class="hlt">heat</span> and moisture. In this paper, we present results of turbulent <span class="hlt">heat</span> <span class="hlt">fluxes</span> calculated by using two years (1992 and 1993) monthly average TOGA data and ATSR SST data in TOGA area. A comparison with published results indicates good qualitative agreement. Also, we compared the results of <span class="hlt">heat</span> <span class="hlt">flux</span> exchange by using ATSR SST data and by using the TOGA bucket SST data. The ATSR SST data set has been shown to be useful in helping to estimate the large space scale <span class="hlt">heat</span> <span class="hlt">flux</span> exchange.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70190499','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70190499"><span>Viscous relaxation of Ganymede's impact craters: Constraints on <span class="hlt">heat</span> <span class="hlt">flux</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>Bland, Michael T.; Singer, Kelsi N.; McKinnon, William B.; Schenk, Paul M.</p> <p>2017-01-01</p> <p>Measurement of crater depths in Ganymede’s dark terrain have revealed substantial numbers of unusually shallow craters indicative of viscous relaxation [see companion paper: Singer, K.N., Schenk, P. M., Bland, M.T., McKinnon, W.B., (2017). Relaxed impact craters on Ganymede: Regional variations and high <span class="hlt">heat</span> flow. Icarus, submitted]. These viscously relaxed craters provide insight into the thermal history of the dark terrain: the rate of relaxation depends on the size of the crater and the thermal structure of the lithosphere. Here we use finite element simulations of crater relaxation to constrain the <span class="hlt">heat</span> <span class="hlt">flux</span> within the dark terrain when relaxation occurred. We show that the degree of viscous relaxation observed cannot be achieved through radiogenic <span class="hlt">heating</span> alone, even if all of the relaxed craters are ancient and experienced the high radiogenic <span class="hlt">fluxes</span> present early in the satellite’s history. For craters with diameter ≥ 10 km, <span class="hlt">heat</span> <span class="hlt">fluxes</span> of 40–50 mW m-2−2"> can reproduce the observed crater depths, but only if the <span class="hlt">fluxes</span> are sustained for ∼1 Gyr. These craters can also be explained by shorter-lived “<span class="hlt">heat</span> pulses” with magnitudes of ∼100 mW m-2−2"> and timescales of 10–100 Myr. At small crater diameters (4 km) the observed shallow depths are difficult to achieve even when <span class="hlt">heat</span> <span class="hlt">fluxes</span> as high as 150 mW m-2−2"> are sustained for 1 Gyr. The extreme thermal conditions required to viscously relax small craters may indicate that mechanisms other than viscous relaxation, such as topographic degradation, are also in play at small crater diameters. The timing of the relaxation event(s) is poorly constrained due to the sparsity of adequate topographic information, though it likely occurred in Ganymede’s middle history (neither recently, nor shortly after satellite formation). The consistency between the timing and magnitude of the <span class="hlt">heat</span> <span class="hlt">fluxes</span> derived here and those inferred from other tectonic features suggests that a single event</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017Icar..296..275B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017Icar..296..275B"><span>Viscous relaxation of Ganymede's impact craters: Constraints on <span class="hlt">heat</span> <span class="hlt">flux</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bland, Michael T.; Singer, Kelsi N.; McKinnon, William B.; Schenk, Paul M.</p> <p>2017-11-01</p> <p>Measurement of crater depths in Ganymede's dark terrain have revealed substantial numbers of unusually shallow craters indicative of viscous relaxation [see companion paper: Singer, K.N., Schenk, P. M., Bland, M.T., McKinnon, W.B., (2017). Relaxed impact craters on Ganymede: Regional variations and high <span class="hlt">heat</span> flow. Icarus, submitted]. These viscously relaxed craters provide insight into the thermal history of the dark terrain: the rate of relaxation depends on the size of the crater and the thermal structure of the lithosphere. Here we use finite element simulations of crater relaxation to constrain the <span class="hlt">heat</span> <span class="hlt">flux</span> within the dark terrain when relaxation occurred. We show that the degree of viscous relaxation observed cannot be achieved through radiogenic <span class="hlt">heating</span> alone, even if all of the relaxed craters are ancient and experienced the high radiogenic <span class="hlt">fluxes</span> present early in the satellite's history. For craters with diameter ≥ 10 km, <span class="hlt">heat</span> <span class="hlt">fluxes</span> of 40-50 mW m-2 can reproduce the observed crater depths, but only if the <span class="hlt">fluxes</span> are sustained for ∼1 Gyr. These craters can also be explained by shorter-lived "<span class="hlt">heat</span> pulses" with magnitudes of ∼100 mW m-2 and timescales of 10-100 Myr. At small crater diameters (4 km) the observed shallow depths are difficult to achieve even when <span class="hlt">heat</span> <span class="hlt">fluxes</span> as high as 150 mW m-2 are sustained for 1 Gyr. The extreme thermal conditions required to viscously relax small craters may indicate that mechanisms other than viscous relaxation, such as topographic degradation, are also in play at small crater diameters. The timing of the relaxation event(s) is poorly constrained due to the sparsity of adequate topographic information, though it likely occurred in Ganymede's middle history (neither recently, nor shortly after satellite formation). The consistency between the timing and magnitude of the <span class="hlt">heat</span> <span class="hlt">fluxes</span> derived here and those inferred from other tectonic features suggests that a single event caused both Ganymede's tectonic deformation and</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017MsT.........14P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017MsT.........14P"><span>Mold <span class="hlt">Flux</span> Crystallization and Mold Thermal Behavior</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Peterson, Elizabeth Irene</p> <p></p> <p>Mold <span class="hlt">flux</span> plays a small but critical role in the continuous casting of steel. The carbon-coated powder is added at the top of the water-cooled copper mold, over time it melts and infiltrates the gap between the copper mold and the solidifying steel strand. Mold powders serve five primary functions: (1) chemical insulation, (2) thermal insulation, (3) lubrication between the steel strand and mold, (4) absorption of inclusions, and (5) promotion of even <span class="hlt">heat</span> <span class="hlt">flux</span>. All five functions are critical to slab casting, but surface defect prevention is primarily controlled through even <span class="hlt">heat</span> <span class="hlt">flux</span>. Glassy <span class="hlt">fluxes</span> have high <span class="hlt">heat</span> transfer and result in a thicker steel shell. Steels with large volumetric shrinkage on cooling must have a crystalline <span class="hlt">flux</span> to reduce the radiative <span class="hlt">heat</span> transfer and avoid the formation of cracks in the shell. Crystallinity plays a critical role in steel shell formation, therefore it is important to study the thermal conditions that promote each phase and its morphology. Laboratory tests were performed to generate continuous cooling transformation (CCT) and time-temperature-transformation (TTT) diagrams. Continuous cooling transformation tests were performed in an instrumented eight cell step chill mold. Results showed that cuspidine was the only phase formed in conventional <span class="hlt">fluxes</span> and all observed structures were dendritic. An isothermal tin bath quench method was also developed to isothermally age glassy samples. Isothermal tests yielded different microstructures and different phases than those observed by continuous cooling. Comparison of aged tests with industrial <span class="hlt">flux</span> films indicates similar faceted structures along the mold <span class="hlt">wall</span>, suggesting that mold <span class="hlt">flux</span> first solidifies as a glass along the mold <span class="hlt">wall</span>, but the elevated temperature devitrifies the glassy structure forming crystals that cannot form by continuous cooling.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20040111369&hterms=Hassan&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAuthor-Name%26N%3D0%26No%3D60%26Ntt%3DHassan','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20040111369&hterms=Hassan&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAuthor-Name%26N%3D0%26No%3D60%26Ntt%3DHassan"><span>Role of Turbulent Prandtl Number on <span class="hlt">Heat</span> <span class="hlt">Flux</span> at Hypersonic Mach Number</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Xiao, X.; Edwards, J. R.; Hassan, H. A.</p> <p>2004-01-01</p> <p>Present simulation of turbulent flows involving shock wave/boundary layer interaction invariably overestimates <span class="hlt">heat</span> <span class="hlt">flux</span> by almost a factor of two. One possible reason for such a performance is a result of the fact that the turbulence models employed make use of Morkovin's hypothesis. This hypothesis is valid for non-hypersonic Mach numbers and moderate rates of <span class="hlt">heat</span> transfer. At hypersonic Mach numbers, high rates of <span class="hlt">heat</span> transfer exist in regions where shock wave/boundary layer interactions are important. As a result, one should not expect traditional turbulence models to yield accurate results. The goal of this investigation is to explore the role of a variable Prandtl number formulation in predicting <span class="hlt">heat</span> <span class="hlt">flux</span> in flows dominated by strong shock wave/boundary layer interactions. The intended applications involve external flows in the absence of combustion such as those encountered in supersonic inlets. This can be achieved by adding equations for the temperature variance and its dissipation rate. Such equations can be derived from the exact Navier-Stokes equations. Traditionally, modeled equations are based on the low speed energy equation where the pressure gradient term and the term responsible for energy dissipation are ignored. It is clear that such assumptions are not valid for hypersonic flows. The approach used here is based on the procedure used in deriving the k-zeta model, in which the exact equations that governed k, the variance of velocity, and zeta, the variance of vorticity, were derived and modeled. For the variable turbulent Prandtl number, the exact equations that govern the temperature variance and its dissipation rate are derived and modeled term by term. The resulting set of equations are free of damping and <span class="hlt">wall</span> functions and are coordinate-system independent. Moreover, modeled correlations are tensorially consistent and invariant under Galilean transformation. The final set of equations will be given in the paper.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009PhST..138a4059H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009PhST..138a4059H"><span>Experiences with tungsten coatings in high <span class="hlt">heat</span> <span class="hlt">flux</span> tests and under plasma load in ASDEX Upgrade</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Herrmann, A.; Greuner, H.; Fuchs, J. C.; de Marné, P.; Neu, R.; ASDEX Upgrade Team</p> <p>2009-12-01</p> <p>ASDEX Upgrade was operated with about 6400 s plasma discharge during the scientific program in 2007/2008 exploring tungsten as a first <span class="hlt">wall</span> material in tokamaks. In the first phase, the <span class="hlt">heating</span> power was restricted to 10 MW. It was increased to 15 MW in the second phase. During this operational period, a delamination of the 200 μm W-VPS coating happened at 2 out of 128 tiles of the outer divertor and an unscheduled opening was required. In the third phase, ASDEX Upgrade was operated with partly predamaged tiles and up to 15 MW <span class="hlt">heating</span> power. The target load was actively controlled by N2-seeding. This paper presents the screening test of target tiles in the high <span class="hlt">heat</span> <span class="hlt">flux</span> test facility GLADIS, experiences with operation and detected damages of the outer divertor as well as the <span class="hlt">heat</span> load to the outer divertor and the reasons for the toroidal asymmetry of the divertor load.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/542197-flux-fluctuation-energy-collisional-grain-flow-flat-frictional-wall','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/542197-flux-fluctuation-energy-collisional-grain-flow-flat-frictional-wall"><span>On the <span class="hlt">flux</span> of fluctuation energy in a collisional grain flow at a flat, frictional <span class="hlt">wall</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>Jenkins, J.T.; Louge, M.Y.</p> <p></p> <p>We consider a flow of colliding spheres that interacts with a flat, frictional <span class="hlt">wall</span> and calculate the <span class="hlt">flux</span> of fluctuation energy in two limits. In the first limit, all spheres slide upon contact with the <span class="hlt">wall</span>. Here, we refine the calculations of Jenkins [J. Appl. Mech. {bold 59}, 120 (1992)] and show that a correlation between two orthogonal components of the fluctuation velocity of the point of contact of the grains with the <span class="hlt">wall</span> provides a substantial correction to the <span class="hlt">flux</span> originally predicted. In the other limit, the granular material is agitated but the mean velocity of the contact pointsmore » with respect to the <span class="hlt">wall</span> is zero and Jenkins{close_quote} earlier calculation is improved by distinguishing between those contacts that slide in a collision and those that stick. The new expressions for the <span class="hlt">flux</span> agree well with the computer simulations of Louge [Phys. Fluids {bold 6}, 2253 (1994)]. Finally, we extend the expression for zero mean sliding to incorporate small sliding and obtain an approximate expression for the <span class="hlt">flux</span> between the two limits. {copyright} {ital 1997 American Institute of Physics.}« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19940010290','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19940010290"><span>DNS and modeling of the interaction between turbulent premixed flames and <span class="hlt">walls</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Poinsot, T. J.; Haworth, D. C.</p> <p>1992-01-01</p> <p>The interaction between turbulent premixed flames and <span class="hlt">walls</span> is studied using a two-dimensional full Navier-Stokes solver with simple chemistry. The effects of <span class="hlt">wall</span> distance on the local and global flame structure are investigated. Quenching distances and maximum <span class="hlt">wall</span> <span class="hlt">heat</span> <span class="hlt">fluxes</span> during quenching are computed in laminar cases and are found to be comparable to experimental and analytical results. For turbulent cases, it is shown that quenching distances and maximum <span class="hlt">heat</span> <span class="hlt">fluxes</span> remain of the same order as for laminar flames. Based on simulation results, a 'law-of-the-<span class="hlt">wall</span>' model is derived to describe the interaction between a turbulent premixed flame and a <span class="hlt">wall</span>. This model is constructed to provide reasonable behavior of flame surface density near a <span class="hlt">wall</span> under the assumption that flame-<span class="hlt">wall</span> interaction takes place at scales smaller than the computational mesh. It can be implemented in conjunction with any of several recent flamelet models based on a modeled surface density equation, with no additional constraints on mesh size or time step.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009HMT....45..967S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009HMT....45..967S"><span>Flow boiling <span class="hlt">heat</span> transfer of R134a and R404A in a microfin tube at low mass <span class="hlt">fluxes</span> and low <span class="hlt">heat</span> <span class="hlt">fluxes</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Spindler, Klaus; Müller-Steinhagen, Hans</p> <p>2009-05-01</p> <p>An experimental investigation of flow boiling <span class="hlt">heat</span> transfer in a commercially available microfin tube with 9.52 mm outer diameter has been carried out. The microfin tube is made of copper with a total fin number of 55 and a helix angle of 15°. The fin height is 0.24 mm and the inner tube diameter at fin root is 8.95 mm. The test tube is 1 m long and is electrically <span class="hlt">heated</span>. The experiments have been performed at saturation temperatures between 0 and -20°C. The mass <span class="hlt">flux</span> was varied between 25 and 150 kg/m2s, the <span class="hlt">heat</span> <span class="hlt">flux</span> from 15,000 W/m2 down to 1,000 W/m2. All measurements have been performed at constant inlet vapour quality ranging from 0.1 to 0.7. The measured <span class="hlt">heat</span> transfer coefficients range from 1,300 to 15,700 W/m2K for R134a and from 912 to 11,451 W/m2K for R404A. The mean <span class="hlt">heat</span> transfer coefficient of R134a is in average 1.5 times higher than for R404A. The mean <span class="hlt">heat</span> transfer coefficient has been compared with the correlations by Koyama et al. and by Kandlikar. The deviations are within ±30% and ±15%, respectively. The influence of the mass <span class="hlt">flux</span> on the <span class="hlt">heat</span> transfer is most significant between 25 and 62.5 kg/m2s, where the flow pattern changes from stratified wavy flow to almost annular flow. This flow pattern transition is shifted to lower mass <span class="hlt">fluxes</span> for the microfin tube compared to the smooth tube.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1183661','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/1183661"><span>Critical <span class="hlt">Heat</span> <span class="hlt">Flux</span> Phenomena at HighPressure & Low Mass <span class="hlt">Fluxes</span>: NEUP Final Report Part I: Experiments</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>Corradini, Michael; Wu, Qiao</p> <p>2015-04-30</p> <p>This report is a preliminary document presenting an overview of the Critical <span class="hlt">Heat</span> <span class="hlt">Flux</span> (CHF) phenomenon, the High Pressure Critical <span class="hlt">Heat</span> <span class="hlt">Flux</span> facility (HPCHF), preliminary CHF data acquired, and the future direction of the research. The HPCHF facility has been designed and built to study CHF at high pressure and low mass <span class="hlt">flux</span> ranges in a rod bundle prototypical of conceptual Small Modular Reactor (SMR) designs. The rod bundle is comprised of four electrically <span class="hlt">heated</span> rods in a 2x2 square rod bundle with a prototypic chopped-cosine axial power profile and equipped with thermocouples at various axial and circumferential positions embeddedmore » in each rod for CHF detection. Experimental test parameters for CHF detection range from pressures of ~80 – 160 bar, mass <span class="hlt">fluxes</span> of ~400 – 1500 kg/m2s, and inlet water subcooling from ~30 – 70°C. The preliminary data base established will be further extended in the future along with comparisons to existing CHF correlations, models, etc. whose application ranges may be applicable to the conditions of SMRs.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19840024719','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19840024719"><span>Turbine blade and vane <span class="hlt">heat</span> <span class="hlt">flux</span> sensor development, phase 1</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Atkinson, W. H.; Cyr, M. A.; Strange, R. R.</p> <p>1984-01-01</p> <p><span class="hlt">Heat</span> <span class="hlt">flux</span> sensors available for installation in the hot section airfoils of advanced aircraft gas turbine engines were developed. Two <span class="hlt">heat</span> <span class="hlt">flux</span> sensors were designed, fabricated, calibrated, and tested. Measurement techniques are compared in an atmospheric pressure combustor rig test. Sensors, embedded thermocouple and the Gordon gauge, were fabricated that met the geometric and fabricability requirements and could withstand the hot section environmental conditions. Calibration data indicate that these sensors yielded repeatable results and have the potential to meet the accuracy goal of measuring local <span class="hlt">heat</span> <span class="hlt">flux</span> to within 5%. Thermal cycle tests and thermal soak tests indicated that the sensors are capable of surviving extended periods of exposure to the environment conditions in the turbine. Problems in calibration of the sensors caused by severe non-one dimensional <span class="hlt">heat</span> flow were encountered. Modifications to the calibration techniques are needed to minimize this problem and proof testing of the sensors in an engine is needed to verify the designs.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1984pwa..rept.....A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1984pwa..rept.....A"><span>Turbine blade and vane <span class="hlt">heat</span> <span class="hlt">flux</span> sensor development, phase 1</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Atkinson, W. H.; Cyr, M. A.; Strange, R. R.</p> <p>1984-08-01</p> <p><span class="hlt">Heat</span> <span class="hlt">flux</span> sensors available for installation in the hot section airfoils of advanced aircraft gas turbine engines were developed. Two <span class="hlt">heat</span> <span class="hlt">flux</span> sensors were designed, fabricated, calibrated, and tested. Measurement techniques are compared in an atmospheric pressure combustor rig test. Sensors, embedded thermocouple and the Gordon gauge, were fabricated that met the geometric and fabricability requirements and could withstand the hot section environmental conditions. Calibration data indicate that these sensors yielded repeatable results and have the potential to meet the accuracy goal of measuring local <span class="hlt">heat</span> <span class="hlt">flux</span> to within 5%. Thermal cycle tests and thermal soak tests indicated that the sensors are capable of surviving extended periods of exposure to the environment conditions in the turbine. Problems in calibration of the sensors caused by severe non-one dimensional <span class="hlt">heat</span> flow were encountered. Modifications to the calibration techniques are needed to minimize this problem and proof testing of the sensors in an engine is needed to verify the designs.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19910029831&hterms=Hot+papers&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D80%26Ntt%3DHot%2Bpapers','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19910029831&hterms=Hot+papers&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D80%26Ntt%3DHot%2Bpapers"><span>A unique high <span class="hlt">heat</span> <span class="hlt">flux</span> facility for testing hypersonic engine components</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Melis, Matthew E.; Gladden, Herbert J.</p> <p>1990-01-01</p> <p>This paper describes the Hot Gas Facility, a unique, reliable, and cost-effective high-<span class="hlt">heat-flux</span> facility for testing hypersonic engine components developed at the NASA Lewis Research Center. The Hot Gas Facility is capable of providing <span class="hlt">heat</span> <span class="hlt">fluxes</span> ranging from 200 Btu/sq ft per sec on flat surfaces up to 8000 Btu/sq ft per sec at a leading edge stagnation point. The usefulness of the Hot Gas Facility for the NASP community was demonstrated by testing hydrogen-cooled structures over a range of temperatures and pressures. Ranges of the Reynolds numbers, Prandtl numbers, enthalpy, and <span class="hlt">heat</span> <span class="hlt">fluxes</span> similar to those expected during hypersonic flights were achieved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017ThEng..64..301S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017ThEng..64..301S"><span>Nanoparticle coating of a microchannel surface is an effective method for increasing the critical <span class="hlt">heat</span> <span class="hlt">flux</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Shustov, M. V.; Kuzma-Kichta, Yu. A.; Lavrikov, A. V.</p> <p>2017-04-01</p> <p>Results are presented of an investigation into water boiling in a single microchannel 0.2 mm high, 3 mm wide, and 13.7 mm long with a smooth <span class="hlt">heating</span> surface or with a coating from aluminum oxide nanoparticles. The experimental procedure and the test setup are described. The top <span class="hlt">wall</span> of the microchannel is made of glass so that video recording in the reflected light of the process can be made. A coating of Al2O3 particles is applied onto the <span class="hlt">heating</span> surface before the experiments using a method developed by the authors of the paper. The experiments yielded data on <span class="hlt">heat</span> transfer and void fraction and its fluctuations for the bubble and transient boiling in the microchannel. The dependence was established of the <span class="hlt">heat</span> <span class="hlt">flux</span> on the temperature of the microchannel <span class="hlt">wall</span> with a smooth surface or a surface with Al2O3 nanoparticle coating for various mass flows in the microchannel. The boiling crisis has been found to occur in the microchannel with a nanoparticle coating at a considerably higher <span class="hlt">heat</span> <span class="hlt">flux</span> than that in the channel without coating. The experimental data also suggest that the nanoparticle coating improves <span class="hlt">heat</span> transfer in the transition boiling region. Processing of the data obtained using a high-speed video revealed void fraction fluctuations enabling us to describe two-phase flow regimes with the flow boiling in a microchannel. It has been found that a return flow occurs in the microchannel under certain conditions. A hypothesis for its causes is proposed. The dependence of the void fraction on the steam quality in the microchannel with or without a nanoparticle coating was determined from the video records. The experimental data on void fraction for boiling in the microchannel without coating are approximated by an empirical correlation. The experiments demonstrate that the void fraction during boiling in the microchannel with a nanoparticle coating is higher than during boiling in the channel without coating (where φ and x are the void fraction and 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_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/2015PhRvA..91b2121L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015PhRvA..91b2121L"><span><span class="hlt">Heat</span> <span class="hlt">flux</span> and quantum correlations in dissipative cascaded systems</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lorenzo, Salvatore; Farace, Alessandro; Ciccarello, Francesco; Palma, G. Massimo; Giovannetti, Vittorio</p> <p>2015-02-01</p> <p>We study the dynamics of <span class="hlt">heat</span> <span class="hlt">flux</span> in the thermalization process of a pair of identical quantum systems that interact dissipatively with a reservoir in a cascaded fashion. Despite that the open dynamics of the bipartite system S is globally Lindbladian, one of the subsystems "sees" the reservoir in a state modified by the interaction with the other subsystem and hence it undergoes a non-Markovian dynamics. As a consequence, the <span class="hlt">heat</span> flow exhibits a nonexponential time behavior which can greatly deviate from the case where each party is independently coupled to the reservoir. We investigate both thermal and correlated initial states of S and show that the presence of correlations at the beginning can considerably affect the <span class="hlt">heat-flux</span> rate. We carry out our study in two paradigmatic cases—a pair of harmonic oscillators with a reservoir of bosonic modes and two qubits with a reservoir of fermionic modes—and compare the corresponding behaviors. In the case of qubits and for initial thermal states, we find that the trace distance discord is at any time interpretable as the correlated contribution to the total <span class="hlt">heat</span> <span class="hlt">flux</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014APS..DPPTP8051M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014APS..DPPTP8051M"><span>Turbulent transport regimes and the SOL <span class="hlt">heat</span> <span class="hlt">flux</span> width</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Myra, J. R.; D'Ippolito, D. A.; Russell, D. A.</p> <p>2014-10-01</p> <p>Understanding the responsible mechanisms and resulting scaling of the scrape-off layer (SOL) <span class="hlt">heat</span> <span class="hlt">flux</span> width is important for predicting viable operating regimes in future tokamaks, and for seeking possible mitigation schemes. Simulation and theory results using reduced edge/SOL turbulence models have produced SOL widths and scalings in reasonable accord with experiments in many cases. In this work, we attempt to qualitatively and conceptually understand various regimes of edge/SOL turbulence and the role of turbulent transport in establishing the SOL <span class="hlt">heat</span> <span class="hlt">flux</span> width. Relevant considerations include the type and spectral characteristics of underlying instabilities, the location of the gradient drive relative to the SOL, the nonlinear saturation mechanism, and the parallel <span class="hlt">heat</span> transport regime. Recent SOLT turbulence code results are employed to understand the roles of these considerations and to develop analytical scalings. We find a <span class="hlt">heat</span> <span class="hlt">flux</span> width scaling with major radius R that is generally positive, consistent with older results reviewed in. The possible relationship of turbulence mechanisms to the heuristic drift mechanism is considered, together with implications for future experiments. Work supported by US DOE grant DE-FG02-97ER54392.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19880001849','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19880001849"><span>Enhancement of surface-atmosphere <span class="hlt">fluxes</span> by desert-fringe vegetation through reduction of surface albedo and of soil <span class="hlt">heat</span> <span class="hlt">flux</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Otterman, J.</p> <p>1987-01-01</p> <p>Under the arid conditions prevailing at the end of the dry season in the western Negev/northern Sinai region, vegetation causes a sharp increase relative to bare soil in the daytime sensible <span class="hlt">heat</span> <span class="hlt">flux</span> from the surface to the atmosphere. Two mechanisms are involved: the increase in the surface absorptivity and a decrease in the surface <span class="hlt">heat</span> <span class="hlt">flux</span>. By increasing the sensible <span class="hlt">heat</span> <span class="hlt">flux</span> to the atmosphere through the albedo and the soil <span class="hlt">heat</span> <span class="hlt">flux</span> reductions, the desert-fringe vegetation increases the daytime convection and the growth of the planetary boundary layer. Removal of vegetation by overgrazing, by reducing the sensible <span class="hlt">heat</span> <span class="hlt">flux</span>, tends to reduce daytime convective precipitation, producing higher probabilities of drought conditions. This assessment of overgrazing is based on observations in the Sinai/Negev, where the soil albedo is high and where overgrazing produces an essential bare soil. Even if the assessment for the Sinai/Negev does not quantitatively apply throughout Africa, the current practice in many African countries of maintaining a large population of grazing animals, can contribute through the mesoscale mechanisms described to reduce daytime convective precipitation, perpetuating higher probabilities of drought. Time-of-day analysis of precipitation in Africa appears worthwhile, to better assess the role of the surface conditions in contributing to drought.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015EGUGA..17.6733B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015EGUGA..17.6733B"><span>Ground <span class="hlt">heat</span> <span class="hlt">flux</span> and power sources of low-enthalpy geothermal systems</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bayer, Peter; Blum, Philipp; Rivera, Jaime A.</p> <p>2015-04-01</p> <p>Geothermal <span class="hlt">heat</span> pumps commonly extract energy from the shallow ground at depths as low as approximately 400 m. Vertical borehole <span class="hlt">heat</span> exchangers are often applied, which are seasonally operated for decades. During this lifetime, thermal anomalies are induced in the ground and surface-near aquifers, which often grow over the years and which alleviate the overall performance of the geothermal system. As basis for prediction and control of the evolving energy imbalance in the ground, focus is typically set on the ground temperatures. This is reflected in regulative temperature thresholds, and in temperature trends, which serve as indicators for renewability and sustainability. In our work, we examine the fundamental <span class="hlt">heat</span> <span class="hlt">flux</span> and power sources, as well as their temporal and spatial variability during geothermal <span class="hlt">heat</span> pump operation. The underlying rationale is that for control of ground temperature evolution, knowledge of the primary <span class="hlt">heat</span> sources is fundamental. This insight is also important to judge the validity of simplified modelling frameworks. For instance, we reveal that vertical <span class="hlt">heat</span> <span class="hlt">flux</span> from the surface dominates the basal <span class="hlt">heat</span> <span class="hlt">flux</span> towards a borehole. Both <span class="hlt">fluxes</span> need to be accounted for as proper vertical boundary conditions in the model. Additionally, the role of horizontal groundwater advection is inspected. Moreover, by adopting the ground energy deficit and long-term replenishment as criteria for system sustainability, an uncommon perspective is adopted that is based on the primary parameter rather than induced local temperatures. In our synthetic study and dimensionless analysis, we demonstrate that time of ground energy recovery after system shutdown may be longer than what is expected from local temperature trends. In contrast, unrealistically long recovery periods and extreme thermal anomalies are predicted without account for vertical ground <span class="hlt">heat</span> <span class="hlt">fluxes</span> and only when the energy content of the geothermal reservoir is considered.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017PhST..170a4071S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017PhST..170a4071S"><span>Progress in extrapolating divertor <span class="hlt">heat</span> <span class="hlt">fluxes</span> towards large fusion devices</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sieglin, B.; Faitsch, M.; Eich, T.; Herrmann, A.; Suttrop, W.; Collaborators, JET; the MST1 Team; the ASDEX Upgrade Team</p> <p>2017-12-01</p> <p><span class="hlt">Heat</span> load to the plasma facing components is one of the major challenges for the development and design of large fusion devices such as ITER. Nowadays fusion experiments can operate with <span class="hlt">heat</span> load mitigation techniques, e.g. sweeping, impurity seeding, but do not generally require it. For large fusion devices however, <span class="hlt">heat</span> load mitigation will be essential. This paper presents the current progress of the extrapolation of steady state and transient <span class="hlt">heat</span> loads towards large fusion devices. For transient <span class="hlt">heat</span> loads, so-called edge localized modes are considered a serious issue for the lifetime of divertor components. In this paper, the ITER operation at half field (2.65 T) and half current (7.5 MA) will be discussed considering the current material limit for the divertor peak energy fluence of 0.5 {MJ}/{{{m}}}2. Recent studies were successful in describing the observed energy fluence in the JET, MAST and ASDEX Upgrade using the pedestal pressure prior to the ELM crash. Extrapolating this towards ITER results in a more benign <span class="hlt">heat</span> load compared to previous scalings. In the presence of magnetic perturbation, the axisymmetry is broken and a 2D <span class="hlt">heat</span> <span class="hlt">flux</span> pattern is induced on the divertor target, leading to local increase of the <span class="hlt">heat</span> <span class="hlt">flux</span> which is a concern for ITER. It is shown that for a moderate divertor broadening S/{λ }{{q}}> 0.5 the toroidal peaking of the <span class="hlt">heat</span> <span class="hlt">flux</span> disappears.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016PEPI..250...35S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016PEPI..250...35S"><span>Dynamos driven by weak thermal convection and heterogeneous outer boundary <span class="hlt">heat</span> <span class="hlt">flux</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sahoo, Swarandeep; Sreenivasan, Binod; Amit, Hagay</p> <p>2016-01-01</p> <p>We use numerical dynamo models with heterogeneous core-mantle boundary (CMB) <span class="hlt">heat</span> <span class="hlt">flux</span> to show that lower mantle lateral thermal variability may help support a dynamo under weak thermal convection. In our reference models with homogeneous CMB <span class="hlt">heat</span> <span class="hlt">flux</span>, convection is either marginally supercritical or absent, always below the threshold for dynamo onset. We find that lateral CMB <span class="hlt">heat</span> <span class="hlt">flux</span> variations organize the flow in the core into patterns that favour the growth of an early magnetic field. <span class="hlt">Heat</span> <span class="hlt">flux</span> patterns symmetric about the equator produce non-reversing magnetic fields, whereas anti-symmetric patterns produce polarity reversals. Our results may explain the existence of the geodynamo prior to inner core nucleation under a tight energy budget. Furthermore, in order to sustain a strong geomagnetic field, the lower mantle thermal distribution was likely dominantly symmetric about the equator.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19900010105','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19900010105"><span>The influence of a <span class="hlt">wall</span> function on turbine blade <span class="hlt">heat</span> transfer prediction</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Whitaker, Kevin W.</p> <p>1989-01-01</p> <p>The second phase of a continuing investigation to improve the prediction of turbine blade <span class="hlt">heat</span> transfer coefficients was completed. The present study specifically investigated how a numeric <span class="hlt">wall</span> function in the turbulence model of a two-dimensional boundary layer code, STAN5, affected <span class="hlt">heat</span> transfer prediction capabilities. Several sources of inaccuracy in the <span class="hlt">wall</span> function were identified and then corrected or improved. <span class="hlt">Heat</span> transfer coefficient predictions were then obtained using each one of the modifications to determine its effect. Results indicated that the modifications made to the <span class="hlt">wall</span> function can significantly affect the prediction of <span class="hlt">heat</span> transfer coefficients on turbine blades. The improvement in accuracy due the modifications is still inconclusive and is still being investigated.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018PEPI..277...10L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018PEPI..277...10L"><span>Linking lowermost mantle structure, core-mantle boundary <span class="hlt">heat</span> <span class="hlt">flux</span> and mantle plume formation</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Li, Mingming; Zhong, Shijie; Olson, Peter</p> <p>2018-04-01</p> <p>The dynamics of Earth's lowermost mantle exert significant control on the formation of mantle plumes and the core-mantle boundary (CMB) <span class="hlt">heat</span> <span class="hlt">flux</span>. However, it is not clear if and how the variation of CMB <span class="hlt">heat</span> <span class="hlt">flux</span> and mantle plume activity are related. Here, we perform geodynamic model experiments that show how temporal variations in CMB <span class="hlt">heat</span> <span class="hlt">flux</span> and pulses of mantle plumes are related to morphologic changes of the thermochemical piles of large-scale compositional heterogeneities in Earth's lowermost mantle, represented by the large low shear velocity provinces (LLSVPs). We find good correlation between the morphologic changes of the thermochemical piles and the time variation of CMB <span class="hlt">heat</span> <span class="hlt">flux</span>. The morphology of the thermochemical piles is significantly altered during the initiation and ascent of strong mantle plumes, and the changes in pile morphology cause variations in the local and the total CMB <span class="hlt">heat</span> <span class="hlt">flux</span>. Our modeling results indicate that plume-induced episodic variations of CMB <span class="hlt">heat</span> <span class="hlt">flux</span> link geomagnetic superchrons to pulses of surface volcanism, although the relative timing of these two phenomena remains problematic. We also find that the density distribution in thermochemical piles is heterogeneous, and that the piles are denser on average than the surrounding mantle when both thermal and chemical effects are included.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4927748','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4927748"><span>Experimental Methodology for Estimation of Local <span class="hlt">Heat</span> <span class="hlt">Fluxes</span> and Burning Rates in Steady Laminar Boundary Layer Diffusion Flames</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Singh, Ajay V.; Gollner, Michael J.</p> <p>2016-01-01</p> <p>Modeling the realistic burning behavior of condensed-phase fuels has remained out of reach, in part because of an inability to resolve the complex interactions occurring at the interface between gas-phase flames and condensed-phase fuels. The current research provides a technique to explore the dynamic relationship between a combustible condensed fuel surface and gas-phase flames in laminar boundary layers. Experiments have previously been conducted in both forced and free convective environments over both solid and liquid fuels. A unique methodology, based on the Reynolds Analogy, was used to estimate local mass burning rates and flame <span class="hlt">heat</span> <span class="hlt">fluxes</span> for these laminar boundary layer diffusion flames utilizing local temperature gradients at the fuel surface. Local mass burning rates and convective and radiative <span class="hlt">heat</span> feedback from the flames were measured in both the pyrolysis and plume regions by using temperature gradients mapped near the <span class="hlt">wall</span> by a two-axis traverse system. These experiments are time-consuming and can be challenging to design as the condensed fuel surface burns steadily for only a limited period of time following ignition. The temperature profiles near the fuel surface need to be mapped during steady burning of a condensed fuel surface at a very high spatial resolution in order to capture reasonable estimates of local temperature gradients. Careful corrections for radiative <span class="hlt">heat</span> losses from the thermocouples are also essential for accurate measurements. For these reasons, the whole experimental setup needs to be automated with a computer-controlled traverse mechanism, eliminating most errors due to positioning of a micro-thermocouple. An outline of steps to reproducibly capture near-<span class="hlt">wall</span> temperature gradients and use them to assess local burning rates and <span class="hlt">heat</span> <span class="hlt">fluxes</span> is provided. PMID:27285827</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1305850-broadening-divertor-heat-flux-profile-increasing-number-elm-filaments-nstx','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1305850-broadening-divertor-heat-flux-profile-increasing-number-elm-filaments-nstx"><span>Broadening of divertor <span class="hlt">heat</span> <span class="hlt">flux</span> profile with increasing number of ELM filaments in NSTX</span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Ahn, J. -W.; Maingi, R.; Canik, J. M.; ...</p> <p>2014-11-13</p> <p>Edge localized modes (ELMs) represent a challenge to future fusion devices, owing to cyclical high peak <span class="hlt">heat</span> <span class="hlt">fluxes</span> on divertor plasma facing surfaces. One ameliorating factor has been that the <span class="hlt">heat</span> <span class="hlt">flux</span> characteristic profile width has been observed to broaden with the size of the ELM, as compared with the inter-ELM <span class="hlt">heat</span> <span class="hlt">flux</span> profile. In contrast, the <span class="hlt">heat</span> <span class="hlt">flux</span> profile has been observed to narrow during ELMs under certain conditions in NSTX. Here we show that the ELM <span class="hlt">heat</span> <span class="hlt">flux</span> profile width increases with the number of filamentary striations observed, i.e., profile narrowing is observed with zero or very fewmore » striations. Because NSTX often lies on the long wavelength current-driven mode side of ideal MHD instabilities, few filamentary structures can be expected under many conditions. Lastly, ITER is also projected to lie on the current driven low-n stability boundary, and therefore detailed projections of the unstable modes expected in ITER and the <span class="hlt">heat</span> <span class="hlt">flux</span> driven in ensuing filamentary structures is needed.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009APS..DPPPP8020L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009APS..DPPPP8020L"><span>Initial results from divertor <span class="hlt">heat-flux</span> instrumentation on Alcator C-Mod</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Labombard, B.; Brunner, D.; Payne, J.; Reinke, M.; Terry, J. L.; Hughes, J. W.; Lipschultz, B.; Whyte, D.</p> <p>2009-11-01</p> <p>Physics-based plasma transport models that can accurately simulate the <span class="hlt">heat-flux</span> power widths observed in the tokamak boundary are lacking at the present time. Yet this quantity is of fundamental importance for ITER and most critically important for DEMO, a reactor similar to ITER but with ˜4 times the power exhaust. In order to improve our understanding, C-Mod, DIII-D and NSTX will aim experiments in FY10 towards characterizing the divertor ``footprint'' and its connection to conditions ``upstream'' in the boundary and core plasmas [2]. Standard IR-based <span class="hlt">heat-flux</span> measurements are particularly difficult in C-Mod, due to its vertical-oriented divertor targets. To overcome this, a suite of embedded <span class="hlt">heat-flux</span> sensor probes (tile thermocouples, calorimeters, surface thermocouples) combined with IR thermography was installed during the FY09 opening, along with a new divertor bolometer system. This paper will report on initial experiments aimed at unfolding the <span class="hlt">heat-flux</span> dependencies on plasma operating conditions. [2] a proposed US DoE Joint Facilities Milestone.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFMGC34B..06G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFMGC34B..06G"><span>Capabilities of VOS-based <span class="hlt">fluxes</span> for estimating ocean <span class="hlt">heat</span> budget and its variability</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Gulev, S.; Belyaev, K.</p> <p>2016-12-01</p> <p>We consider here the perspective of using VOS observations by merchant ships available form the ICOADS data for estimating ocean surface <span class="hlt">heat</span> budget at different time scale. To this purpose we compute surface turbulent <span class="hlt">heat</span> <span class="hlt">fluxes</span> as well as short- and long-wave radiative <span class="hlt">fluxes</span> from the ICOADS reports for the last several decades in the North Atlantic mid latitudes. Turbulent <span class="hlt">fluxes</span> were derived using COARE-3 algorithm and for computation of radiative <span class="hlt">fluxes</span> new algorithms accounting for cloud types were used. Sampling uncertainties in the VOS-based <span class="hlt">fluxes</span> were estimated by sub-sampling of the recomputed reanalysis (ERA-Interim) <span class="hlt">fluxes</span> according to the VOS sampling scheme. For the turbulent <span class="hlt">heat</span> <span class="hlt">fluxes</span> we suggest an approach to minimize sampling uncertainties. The approach is based on the integration of the turbulent <span class="hlt">heat</span> <span class="hlt">fluxes</span> in the coordinates of steering parameters (vertical surface temperature and humidity gradients on one hand and wind speed on the other) for which theoretical probability distributions are known. For short-wave radiative <span class="hlt">fluxes</span> sampling uncertainties were minimized by "rotating local observation time around the clock" and using probability density functions for the cloud cover occurrence distributions. Analysis was performed for the North Atlantic latitudinal band from 25 N to 60 N, for which also estimates of the meridional <span class="hlt">heat</span> transport are available from the ocean cross-sections. Over the last 35 years turbulent <span class="hlt">fluxes</span> within the region analysed increase by about 6 W/m2 with the major growth during the 1990s and early 2000s. Decreasing incoming short wave radiation during the same time (about 1 W/m2) implies upward change of the ocean surface <span class="hlt">heat</span> loss by about 7-8 W/m2. We discuss different sources of uncertainties of computations as well as potential of the application of the analysis concept to longer time series going back to 1920s.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2008MicST..20..193H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2008MicST..20..193H"><span>Experimental Study of the Relation Between <span class="hlt">Heat</span> Transfer and Flow Behavior in a Single Microtube</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Huang, Shih-Che; Kawanami, Osamu; Kawakami, Kazunari; Honda, Itsuro; Kawashima, Yousuke; Ohta, Haruhiko</p> <p>2008-09-01</p> <p>The flow boiling <span class="hlt">heat</span> transfer in microchannels have become important issue because it is extremely high-performance <span class="hlt">heat</span> exchanger for electronic devices. For a detailed study on flow boiling <span class="hlt">heat</span> transfer in a microtube, we have used a transparent <span class="hlt">heated</span> microtube, which is coated with a thin gold film on its inner <span class="hlt">wall</span>. The gold film is used as a resistance thermometer to directly evaluate the inner <span class="hlt">wall</span> temperature averaged over the entire temperature measurement length. At the same time, the transparency of the film enables the observation of fluid behavior. Flow boiling experiments have been carried out using the microtube under the following conditions; mass velocity of 105 kg/m2 s, tube diameter of 1 mm, <span class="hlt">heat</span> <span class="hlt">flux</span> in the range of 10 380 kW/m2 s, and the test fluid used is ionized water. Under low <span class="hlt">heat</span> <span class="hlt">flux</span> conditions, the fluctuations in the inner <span class="hlt">wall</span> temperature and mass velocity are closely related; the frequency of these fluctuations is the same. However, the fluctuations in the inner <span class="hlt">wall</span> temperature and <span class="hlt">heat</span> transfer coefficient are found to be independent of the fluctuation in the mass velocity under high <span class="hlt">heat</span> <span class="hlt">flux</span> conditions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018HMT...tmp..114M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018HMT...tmp..114M"><span>A combined ANN-GA and experimental based technique for the estimation of the unknown <span class="hlt">heat</span> <span class="hlt">flux</span> for a conjugate <span class="hlt">heat</span> transfer problem</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>M K, Harsha Kumar; P S, Vishweshwara; N, Gnanasekaran; C, Balaji</p> <p>2018-05-01</p> <p>The major objectives in the design of thermal systems are obtaining the information about thermophysical, transport and boundary properties. The main purpose of this paper is to estimate the unknown <span class="hlt">heat</span> <span class="hlt">flux</span> at the surface of a solid body. A constant area mild steel fin is considered and the base is subjected to constant <span class="hlt">heat</span> <span class="hlt">flux</span>. During <span class="hlt">heating</span>, natural convection <span class="hlt">heat</span> transfer occurs from the fin to ambient. The direct solution, which is the forward problem, is developed as a conjugate <span class="hlt">heat</span> transfer problem from the fin and the steady state temperature distribution is recorded for any assumed <span class="hlt">heat</span> <span class="hlt">flux</span>. In order to model the natural convection <span class="hlt">heat</span> transfer from the fin, an extended domain is created near the fin geometry and air is specified as a fluid medium and Navier Stokes equation is solved by incorporating the Boussinesq approximation. The computational time involved in executing the forward model is then reduced by developing a neural network (NN) between <span class="hlt">heat</span> <span class="hlt">flux</span> values and temperatures based on back propagation algorithm. The conjugate <span class="hlt">heat</span> transfer NN model is now coupled with Genetic algorithm (GA) for the solution of the inverse problem. Initially, GA is applied to the pure surrogate data, the results are then used as input to the Levenberg- Marquardt method and such hybridization is proven to result in accurate estimation of the unknown <span class="hlt">heat</span> <span class="hlt">flux</span>. The hybrid method is then applied for the experimental temperature to estimate the unknown <span class="hlt">heat</span> <span class="hlt">flux</span>. A satisfactory agreement between the estimated and actual <span class="hlt">heat</span> <span class="hlt">flux</span> is achieved by incorporating the hybrid method.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/467948','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/467948"><span>A preliminary assessment of the effects of <span class="hlt">heat</span> <span class="hlt">flux</span> distribution and penetration on the creep rupture of a reactor vessel lower head</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>Chu, T.Y.; Bentz, J.; Simpson, R.</p> <p>1997-02-01</p> <p>The objective of the Lower Head Failure (LHF) Experiment Program is to experimentally investigate and characterize the failure of the reactor vessel lower head due to thermal and pressure loads under severe accident conditions. The experiment is performed using 1/5-scale models of a typical PWR pressure vessel. Experiments are performed for various internal pressure and imposed <span class="hlt">heat</span> <span class="hlt">flux</span> distributions with and without instrumentation guide tube penetrations. The experimental program is complemented by a modest modeling program based on the application of vessel creep rupture codes developed in the TMI Vessel Investigation Project. The first three experiments under the LHF programmore » investigated the creep rupture of simulated reactor pressure vessels without penetrations. The <span class="hlt">heat</span> <span class="hlt">flux</span> distributions for the three experiments are uniform (LHF-1), center-peaked (LHF-2), and side-peaked (LHF-3), respectively. For all the experiments, appreciable vessel deformation was observed to initiate at vessel <span class="hlt">wall</span> temperatures above 900K and the vessel typically failed at approximately 1000K. The size of failure was always observed to be smaller than the <span class="hlt">heated</span> region. For experiments with non-uniform <span class="hlt">heat</span> <span class="hlt">flux</span> distributions, failure typically occurs in the region of peak temperature. A brief discussion of the effect of penetration is also presented.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19890000356&hterms=Rhodium&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3DRhodium','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19890000356&hterms=Rhodium&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3DRhodium"><span><span class="hlt">Heat-Flux</span> Sensor For Hot Engine Cylinders</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Kim, Walter S.; Barrows, Richard F.; Smith, Floyd A.; Koch, John</p> <p>1989-01-01</p> <p><span class="hlt">Heat-flux</span> sensor includes buried wire thermocouple and thin-film surface thermocouple, made of platinum and platinum with 13 percent rhodium. Sensor intended for use in ceramic-insulated, low-<span class="hlt">heat</span>-rejection diesel engine at temperatures of about 1,000 K. Thermocouple junction resists environment in cylinder of advanced high-temperature diesel engine created by depositing overlapping films of Pt and 0.87 Pt/0.13 Rh on iron plug. Plug also contains internal thermocouple.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015APS..DPPJP2043P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015APS..DPPJP2043P"><span>Scaling Relationships for ELM Diverter <span class="hlt">Heat</span> <span class="hlt">Flux</span> on DIII D</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Peters, E. A.; Makowski, M. A.; Leonard, A. W.</p> <p>2015-11-01</p> <p>Edge Localized Modes (ELMs) are periodic plasma instabilities that occur during H-mode operation in tokamaks. Left unmitigated, these instabilities result in concentrated particle and <span class="hlt">heat</span> <span class="hlt">fluxes</span> at the divertor and stand to cause serious damage to the plasma facing components of tokamaks. The purpose of this research is to find scaling relationships that predict divertor <span class="hlt">heat</span> <span class="hlt">flux</span> due to ELMs based on plasma parameters at the time of instability. This will be accomplished by correlating characteristic ELM parameters with corresponding plasma measurements and analyzing the data for trends. One early assessment is the effect of the <span class="hlt">heat</span> transmission coefficient ? on the in/out asymmetry of the calculated ELM <span class="hlt">heat</span> <span class="hlt">fluxes</span>. Using IR camera data, further assessments in this study will continue to emphasize in/out asymmetry in ELMs, as this has important implications for ITER operation. Work supported in part by the US DOE, DE-AC52-07NA27344, DE-FC02-04ER54698, Office of Workforce Development for Teachers and Scientists (WDTS) under the Science Undergraduate Laboratory Internships Program (SULI).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017NucFu..57k6016X','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017NucFu..57k6016X"><span>Divertor <span class="hlt">heat</span> <span class="hlt">flux</span> simulations in ELMy H-mode discharges of EAST</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Xia, T. Y.; Xu, X. Q.; Wu, Y. B.; Huang, Y. Q.; Wang, L.; Zheng, Z.; Liu, J. B.; Zang, Q.; Li, Y. Y.; Zhao, D.; EAST Team</p> <p>2017-11-01</p> <p>This paper presents <span class="hlt">heat</span> <span class="hlt">flux</span> simulations for the ELMy H-mode on the Experimental Advanced Superconducting Tokamak (EAST) using a six-field two-fluid model in BOUT++. Three EAST ELMy H-mode discharges with different plasma currents I p and geometries are studied. The trend of the scrape-off layer width λq with I p is reproduced by the simulation. The simulated width is only half of that derived from the EAST scaling law, but agrees well with the international multi-machine scaling law. Note that there is no radio-frequency (RF) <span class="hlt">heating</span> scheme in the simulations, and RF <span class="hlt">heating</span> can change the boundary topology and increase the <span class="hlt">flux</span> expansion. Anomalous electron transport is found to contribute to the divertor <span class="hlt">heat</span> <span class="hlt">fluxes</span>. A coherent mode is found in the edge region in simulations. The frequency and poloidal wave number kθ are in the range of the edge coherent mode in EAST. The magnetic fluctuations of the mode are smaller than the electric field fluctuations. Statistical analysis of the type of turbulence shows that the turbulence transport type (blobby or turbulent) does not influence the <span class="hlt">heat</span> <span class="hlt">flux</span> width scaling. The two-point model differs from the simulation results but the drift-based model shows good agreement with simulations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMNG21A0138D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMNG21A0138D"><span>The Influence of <span class="hlt">Heat</span> <span class="hlt">Flux</span> Boundary Heterogeneity on <span class="hlt">Heat</span> Transport in Earth's Core</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Davies, C. J.; Mound, J. E.</p> <p>2017-12-01</p> <p>Rotating convection in planetary systems can be subjected to large lateral variations in <span class="hlt">heat</span> <span class="hlt">flux</span> from above; for example, due to the interaction between the metallic cores of terrestrial planets and their overlying silicate mantles. The boundary anomalies can significantly reorganise the pattern of convection and influence global diagnostics such as the Nusselt number. We have conducted a suite of numerical simulations of rotating convection in a spherical shell geometry comparing convection with homogeneous boundary conditions to that with two patterns of <span class="hlt">heat</span> <span class="hlt">flux</span> variation at the outer boundary: one hemispheric pattern, and one derived from seismic tomographic imaging of Earth's lower mantle. We consider Ekman numbers down to 10-6 and <span class="hlt">flux</span>-based Rayleigh numbers up to 800 times critical. The heterogeneous boundary conditions tend to increase the Nusselt number relative to the equivalent homogeneous case by altering both the flow and temperature fields, particularly near the top of the convecting region. The enhancement in Nusselt number tends to increase as the amplitude and wavelength of the boundary heterogeneity is increased and as the system becomes more supercritical. In our suite of models, the increase in Nusselt number can be as large as 25%. The slope of the Nusselt-Rayleigh scaling also changes when boundary heterogeneity is included, which has implications when extrapolating to planetary conditions. Additionally, regions of effective thermal stratification can develop when strongly heterogeneous <span class="hlt">heat</span> <span class="hlt">flux</span> conditions are applied at the outer boundary.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19900000468&hterms=solar+receiver&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Dsolar%2Breceiver','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19900000468&hterms=solar+receiver&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Dsolar%2Breceiver"><span>Simplified Calculation Of Solar <span class="hlt">Fluxes</span> In Solar Receivers</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Bhandari, Pradeep</p> <p>1990-01-01</p> <p>Simplified Calculation of Solar <span class="hlt">Flux</span> Distribution on Side <span class="hlt">Wall</span> of Cylindrical Cavity Solar Receivers computer program employs simple solar-<span class="hlt">flux</span>-calculation algorithm for cylindrical-cavity-type solar receiver. Results compare favorably with those of more complicated programs. Applications include study of solar energy and transfer of <span class="hlt">heat</span>, and space power/solar-dynamics engineering. Written in FORTRAN 77.</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('http://hdl.handle.net/2060/19730019076','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19730019076"><span>Extended hydrodynamic theory of the peak and minimum pool boiling <span class="hlt">heat</span> <span class="hlt">fluxes</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Linehard, J. H.; Dhir, V. K.</p> <p>1973-01-01</p> <p>The hydrodynamic theory of the extreme pool boiling <span class="hlt">heat</span> <span class="hlt">fluxes</span> is expanded to embrace a variety of problems that have not previously been analyzed. These problems include the prediction of the peak <span class="hlt">heat</span> <span class="hlt">flux</span> on a variety of finite heaters, the influence of viscosity on the Taylor and Helmoltz instability mechanisms with application to film boiling and to the peak <span class="hlt">heat</span> <span class="hlt">flux</span> in viscous liquids, the formalization of the analogy between high-current-density electrolysis and boiling, and the description of boiling in the low-gravity limit. The predictions are verified with a large number of new data.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.fs.usda.gov/treesearch/pubs/19747','TREESEARCH'); return false;" href="https://www.fs.usda.gov/treesearch/pubs/19747"><span>An inverse method to estimate stem surface <span class="hlt">heat</span> <span class="hlt">flux</span> in wildland fires</span></a></p> <p><a target="_blank" href="http://www.fs.usda.gov/treesearch/">Treesearch</a></p> <p>Anthony S. Bova; Matthew B. Dickinson</p> <p>2009-01-01</p> <p>Models of wildland fire-induced stem <span class="hlt">heating</span> and tissue necrosis require accurate estimates of inward <span class="hlt">heat</span> <span class="hlt">flux</span> at the bark surface. Thermocouple probes or <span class="hlt">heat</span> <span class="hlt">flux</span> sensors placed at a stem surface do not mimic the thermal response of tree bark to flames.We show that data from thin thermocouple probes inserted just below the bark can be used, by means of a one-...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/4144121','DOE-PATENT-XML'); return false;" href="https://www.osti.gov/biblio/4144121"><span><span class="hlt">HEAT</span> TRANSFER METHOD</span></a></p> <p><a target="_blank" href="http://www.osti.gov/doepatents">DOEpatents</a></p> <p>Gambill, W.R.; Greene, N.D.</p> <p>1960-08-30</p> <p>A method is given for increasing burn-out <span class="hlt">heat</span> <span class="hlt">fluxes</span> under nucleate boiling conditions in <span class="hlt">heat</span> exchanger tubes without incurring an increase in pumping power requirements. This increase is achieved by utilizing a spinning flow having a rotational velocity sufficient to produce a centrifugal acceleration of at least 10,000 g at the tube <span class="hlt">wall</span>. At this acceleration the <span class="hlt">heat</span>-transfer rate at burn out is nearly twice the rate which can be achieved in a similar tube utilizing axial flow at the same pumping power. At higher accelerations the improvement over axial flow is greater, and <span class="hlt">heat</span> <span class="hlt">fluxes</span> in excess of 50 x 10/sup 6/ Btu/hr/sq ft can be achieved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19890065910&hterms=burnout&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D70%26Ntt%3Dburnout','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19890065910&hterms=burnout&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D70%26Ntt%3Dburnout"><span>A new hydrodynamic prediction of the peak <span class="hlt">heat</span> <span class="hlt">flux</span> from horizontal cylinders in low speed upflow</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Ungar, E. K.; Eichhorn, R.</p> <p>1988-01-01</p> <p>Flow-boiling data have been obtained for horizontal cylinders in saturated acetone, isopropanol, and water, yielding <span class="hlt">heat</span> <span class="hlt">flux</span> vs. <span class="hlt">wall</span> superheat boiling curves for the organic liquids. A region of low speed upflow is identified in which long cylindrical bubbles break off from the wake with regular frequency. The Strouhal number of bubble breakoff is a function only of the Froude number in any liquid, and the effective wake thickness in all liquids is a function of the density ratio and the Froude number. A low speed flow boiling burnout prediction procedure is presented which yields accurate results in widely dissimilar liquids.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015PlST...17..792C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015PlST...17..792C"><span>Numerical Study of High <span class="hlt">Heat</span> <span class="hlt">Flux</span> Performances of Flat-Tile Divertor Mock-ups with Hypervapotron Cooling Concept</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Chen, Lei; Liu, Xiang; Lian, Youyun; Cai, Laizhong</p> <p>2015-09-01</p> <p>The hypervapotron (HV), as an enhanced <span class="hlt">heat</span> transfer technique, will be used for ITER divertor components in the dome region as well as the enhanced <span class="hlt">heat</span> <span class="hlt">flux</span> first <span class="hlt">wall</span> panels. W-Cu brazing technology has been developed at SWIP (Southwestern Institute of Physics), and one W/CuCrZr/316LN component of 450 mm×52 mm×166 mm with HV cooling channels will be fabricated for high <span class="hlt">heat</span> <span class="hlt">flux</span> (HHF) tests. Before that a relevant analysis was carried out to optimize the structure of divertor component elements. ANSYS-CFX was used in CFD analysis and ABAQUS was adopted for thermal-mechanical calculations. Commercial code FE-SAFE was adopted to compute the fatigue life of the component. The tile size, thickness of tungsten tiles and the slit width among tungsten tiles were optimized and its HHF performances under International Thermonuclear Experimental Reactor (ITER) loading conditions were simulated. One brand new tokamak HL-2M with advanced divertor configuration is under construction in SWIP, where ITER-like flat-tile divertor components are adopted. This optimized design is expected to supply valuable data for HL-2M tokamak. supported by the National Magnetic Confinement Fusion Science Program of China (Nos. 2011GB110001 and 2011GB110004)</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/ADA469754','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA469754"><span>Electromagnetic Control of High <span class="hlt">Heat-Flux</span> Spray Impingement Boiling Under Microgravity Conditions</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>2007-03-01</p> <p>impingement boiling ( Mudawar , 2000; Chow et al., 1997; Tilton, 1989). With water as the working fluid, spray cooling has achieved a <span class="hlt">heat</span> <span class="hlt">flux</span> on the...Stebbins, C. J., and Mudawar , I., 1996. "Mapping of Impact and <span class="hlt">Heat</span> Transfer Regimes of Water Drops Impinging on a Polished Surface," Int. J. <span class="hlt">Heat</span> and Mass...34 Proceedings of SAE 2004 Power Systems Conference, 2004-01-3204, Reno NV, November, pp. 309-317. Mudawar , 1., 2000. "Assessment of High-<span class="hlt">heat</span> <span class="hlt">Flux</span></p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1356713-analysis-edge-stability-models-heat-flux-width','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1356713-analysis-edge-stability-models-heat-flux-width"><span>Analysis of edge stability for models of <span class="hlt">heat</span> <span class="hlt">flux</span> width</span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Makowski, Michael A.; Lasnier, Charles J.; Leonard, Anthony W.; ...</p> <p>2017-05-12</p> <p>Detailed measurements of the n e, and T e, and T i profiles in the vicinity of the separatrix of ELMing H-mode discharges have been used to examine plasma stability at the extreme edge of the plasma and assess stability dependent models of the <span class="hlt">heat</span> <span class="hlt">flux</span> width. The results are strongly contrary to the critical gradient model, which posits that a ballooning instability determines a gradient scale length related to the <span class="hlt">heat</span> <span class="hlt">flux</span> width. The results of this analysis are not sensitive to the choice of location to evaluate stability. Significantly, it is also found that the results are completelymore » consistent with the heuristic drift model for the <span class="hlt">heat</span> <span class="hlt">flux</span> width. Here the edge pressure gradient scales with plasma density and is proportional to the pressure gradient inferred from the equilibrium in accordance with the predictions of that theory.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19910063111&hterms=heat+stress&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3Dheat%2Bstress','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19910063111&hterms=heat+stress&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3Dheat%2Bstress"><span>Reynolds shear stress and <span class="hlt">heat</span> <span class="hlt">flux</span> calculations in a fully developed turbulent duct flow</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Antonia, R. A.; Kim, J.</p> <p>1991-01-01</p> <p>The use of a modified form of the Van Driest mixing length for a fully developed turbulent channel flow leads to mean velocity and Reynolds stress distributions that are in close agreement with data obtained either from experiments or direct numerical simulations. The calculations are then extended to a nonisothermal flow by assuming a constant turbulent Prandtl number, the value of which depends on the molecular Prandtl number. Calculated distributions of mean temperature and lateral <span class="hlt">heat</span> <span class="hlt">flux</span> are in reasonable agreement with the simulations. The extension of the calculations to higher Reynolds numbers provides some idea of the Reynolds number required for scaling on <span class="hlt">wall</span> variables to apply in the inner region of the flow.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011APS..DPPPI2005M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011APS..DPPPI2005M"><span>Analysis of a Multi-Machine Database on Divertor <span class="hlt">Heat</span> <span class="hlt">Fluxes</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Makowski, M. A.</p> <p>2011-10-01</p> <p>A coordinated effort to measure divertor <span class="hlt">heat</span> <span class="hlt">flux</span> characteristics in fully attached, similarly shaped H-mode plasmas on C-Mod, DIII-D and NSTX was carried out in 2010 in order to construct a predictive scaling relation applicable to next step devices including ITER, FNSF, and DEMO. Few published scaling laws are available and those that have been published were obtained under widely varying conditions and divertor geometries, leading to conflicting predictions for this critically important quantity. This study was designed to overcome these deficiencies. Corresponding plasma parameters were systematically varied in each tokamak, resulting in a combined data set in which Ip varies by a factor 3, Bt varies by a factor of 14.5, and major radius varies by a factor of 2.6. The derived scaling relation consistently predicts narrower <span class="hlt">heat</span> <span class="hlt">flux</span> widths than relations currently in use. Analysis of the combined data set reveals that the primary dependence of the parallel <span class="hlt">heat</span> <span class="hlt">flux</span> width is robustly inverse with Ip. All three tokamaks independently demonstrate this dependence. The midplane SOL profiles in DIII-D are also found to steepen with higher Ip, similar to the divertor <span class="hlt">heat</span> <span class="hlt">flux</span> profiles. Weaker dependencies on the toroidal field and normalized Greenwald density, fGW, are also found, but vary across devices and with the measure of the <span class="hlt">heat</span> <span class="hlt">flux</span> width used, either FWHM or integral width. In the combined data set, the strongest size scaling is with minor radius resulting in an approximately linear dependence on a /Ip . This suggests a scaling correlated with the inverse of the poloidal field, as would be expected for critical gradient or drift-based transport. Supported by the US DOE under DE-AC52-07NA27344 and DE-FC02-04ER54698.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/11874138','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/11874138"><span>Methodology for estimation of time-dependent surface <span class="hlt">heat</span> <span class="hlt">flux</span> due to cryogen spray cooling.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Tunnell, James W; Torres, Jorge H; Anvari, Bahman</p> <p>2002-01-01</p> <p>Cryogen spray cooling (CSC) is an effective technique to protect the epidermis during cutaneous laser therapies. Spraying a cryogen onto the skin surface creates a time-varying <span class="hlt">heat</span> <span class="hlt">flux</span>, effectively cooling the skin during and following the cryogen spurt. In previous studies mathematical models were developed to predict the human skin temperature profiles during the cryogen spraying time. However, no studies have accounted for the additional cooling due to residual cryogen left on the skin surface following the spurt termination. We formulate and solve an inverse <span class="hlt">heat</span> conduction (IHC) problem to predict the time-varying surface <span class="hlt">heat</span> <span class="hlt">flux</span> both during and following a cryogen spurt. The IHC formulation uses measured temperature profiles from within a medium to estimate the surface <span class="hlt">heat</span> <span class="hlt">flux</span>. We implement a one-dimensional sequential function specification method (SFSM) to estimate the surface <span class="hlt">heat</span> <span class="hlt">flux</span> from internal temperatures measured within an in vitro model in response to a cryogen spurt. Solution accuracy and experimental errors are examined using simulated temperature data. <span class="hlt">Heat</span> <span class="hlt">flux</span> following spurt termination appears substantial; however, it is less than that during the spraying time. The estimated time-varying <span class="hlt">heat</span> <span class="hlt">flux</span> can subsequently be used in forward <span class="hlt">heat</span> conduction models to estimate temperature profiles in skin during and following a cryogen spurt and predict appropriate timing for onset of the laser pulse.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19930032422&hterms=thin+film+fabrication&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Dthin%2Bfilm%2Bfabrication','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19930032422&hterms=thin+film+fabrication&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Dthin%2Bfilm%2Bfabrication"><span>Fabrication of thin film <span class="hlt">heat</span> <span class="hlt">flux</span> sensors</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Will, Herbert</p> <p>1991-01-01</p> <p>Thin-film <span class="hlt">heat-flux</span> sensors have been constructed in the form of arrays of thermocouples on upper and lower surfaces of an insulating layer, so that <span class="hlt">flux</span> values are proportional to the temperature difference across the upper and lower surface of the insulation material. The sensor thermocouples are connected in thermopile arrangement, and the structure is patterned with photolithographic techniques. Both chromel-alumel and Pt-Pt/Rh thermocouples have been devised; the later produced 28 microvolts when exposed to the radiation of a 1000 C furnace.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017APS..DPPBO7015H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017APS..DPPBO7015H"><span><span class="hlt">Heat-Flux</span> Measurements in Laser-Produced Plasmas Using Thomson Scattering from Electron Plasma Waves</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Henchen, R. J.; Goncharov, V. N.; Cao, D.; Katz, J.; Froula, D. H.; Rozmus, W.</p> <p>2017-10-01</p> <p>An experiment was designed to measure <span class="hlt">heat</span> <span class="hlt">flux</span> in coronal plasmas using collective Thomson scattering. Adjustments to the electron distribution function resulting from <span class="hlt">heat</span> <span class="hlt">flux</span> affect the shape of the collective Thomson scattering features through wave-particle resonance. The amplitude of the Spitzer-Härm electron distribution function correction term (f1) was varied to match the data and determines the value of the <span class="hlt">heat</span> <span class="hlt">flux</span>. Independent measurements of temperature and density obtained from Thomson scattering were used to infer the classical <span class="hlt">heat</span> <span class="hlt">flux</span> (q = - κ∇Te) . Time-resolved Thomson-scattering data were obtained at five locations in the corona along the target normal in a blowoff plasma formed from a planar Al target with 1.5 kJ of 351-nm laser light in a 2-ns square pulse. The <span class="hlt">flux</span> measured through the Thomson-scattering spectra is a factor of 5 less than the κ∇Te measurements. The lack of collisions of <span class="hlt">heat</span>-carrying electrons suggests a nonlocal model is needed to accurately describe the <span class="hlt">heat</span> <span class="hlt">flux</span>. This material is based upon work supported by the Department of Energy National Nuclear Security Administration under Award Number DE-NA0001944.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.fs.usda.gov/treesearch/pubs/34711','TREESEARCH'); return false;" href="https://www.fs.usda.gov/treesearch/pubs/34711"><span>Fine fuel <span class="hlt">heating</span> by radiant <span class="hlt">flux</span></span></a></p> <p><a target="_blank" href="http://www.fs.usda.gov/treesearch/">Treesearch</a></p> <p>David Frankman; Brent W. Webb; Bret W. Butler; Don J. Latham</p> <p>2010-01-01</p> <p>Experiments were conducted wherein wood shavings and Ponderosa pine needles in quiescent air were subjected to a steady radiation <span class="hlt">heat</span> <span class="hlt">flux</span> from a planar ceramic burner. The internal temperature of these particles was measured using fine diameter (0.076mm diameter) type K thermocouples. A narrow angle radiometer was used to determine the emissive power generated by the...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/813610','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/813610"><span>Infrared Camera Diagnostic for <span class="hlt">Heat</span> <span class="hlt">Flux</span> Measurements on NSTX</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>D. Mastrovito; R. Maingi; H.W. Kugel</p> <p>2003-03-25</p> <p>An infrared imaging system has been installed on NSTX (National Spherical Torus Experiment) at the Princeton Plasma Physics Laboratory to measure the surface temperatures on the lower divertor and center stack. The imaging system is based on an Indigo Alpha 160 x 128 microbolometer camera with 12 bits/pixel operating in the 7-13 {micro}m range with a 30 Hz frame rate and a dynamic temperature range of 0-700 degrees C. From these data and knowledge of graphite thermal properties, the <span class="hlt">heat</span> <span class="hlt">flux</span> is derived with a classic one-dimensional conduction model. Preliminary results of <span class="hlt">heat</span> <span class="hlt">flux</span> scaling are reported.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013APJAS..49..443P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013APJAS..49..443P"><span><span class="hlt">Heat</span> <span class="hlt">flux</span> variations over sea ice observed at the coastal area of the Sejong Station, Antarctica</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Park, Sang-Jong; Choi, Tae-Jin; Kim, Seong-Joong</p> <p>2013-08-01</p> <p>This study presents variations of sensible <span class="hlt">heat</span> <span class="hlt">flux</span> and latent <span class="hlt">heat</span> <span class="hlt">flux</span> over sea ice observed in 2011 from the 10-m <span class="hlt">flux</span> tower located at the coast of the Sejong Station on King George Island, Antarctica. A period from July to September was selected as a sea ice period based on daily record of sea state and hourly photos looking at the Marian Cove in front of the Sejong Station. For the sea ice period, mean sensible <span class="hlt">heat</span> <span class="hlt">flux</span> is about -11 Wm-2, latent <span class="hlt">heat</span> <span class="hlt">flux</span> is about +2 W m-2, net radiation is -12 W m-2, and residual energy is -3 W m-2 with clear diurnal variations. Estimated mean values of surface exchange coefficients for momentum, <span class="hlt">heat</span> and moisture are 5.15 × 10-3, 1.19 × 10-3, and 1.87 × 10-3, respectively. The observed exchange coefficients of <span class="hlt">heat</span> shows clear diurnal variations while those of momentum and moisture do not show diurnal variation. The parameterized exchange coefficients of <span class="hlt">heat</span> and moisture produces <span class="hlt">heat</span> <span class="hlt">fluxes</span> which compare well with the observed diurnal variations of <span class="hlt">heat</span> <span class="hlt">fluxes</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19820009925','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19820009925"><span>Sensitivity of a climatologically-driven sea ice model to the ocean <span class="hlt">heat</span> <span class="hlt">flux</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Parkinson, C. L.; Good, M. R.</p> <p>1982-01-01</p> <p>Ocean <span class="hlt">heat</span> <span class="hlt">flux</span> sensitivity was studied on a numerical model of sea ice covering the Weddell Sea region of the southern ocean. The model is driven by mean monthly climatological atmospheric variables. For each model run, the ocean <span class="hlt">heat</span> <span class="hlt">flux</span> is uniform in both space and time. Ocean <span class="hlt">heat</span> <span class="hlt">fluxes</span> below 20 W m to the minus 2 power do not provide sufficient energy to allow the ice to melt to its summertime thicknesses and concentrations by the end of the 14 month simulation, whereas ocean <span class="hlt">heat</span> <span class="hlt">fluxes</span> of 30 W m to the minus 2 power and above result in too much ice melt, producing the almost total disappearance of ice in the Weddell Sea by the end of the 14 months. These results are dependent on the atmospheric forcing fields.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19930036197&hterms=modeling+transfer+heat&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3Dmodeling%2Btransfer%2Bheat','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19930036197&hterms=modeling+transfer+heat&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3Dmodeling%2Btransfer%2Bheat"><span>On the assumption of vanishing temperature fluctuations at the <span class="hlt">wall</span> for <span class="hlt">heat</span> transfer modeling</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Sommer, T. P.; So, R. M. C.; Zhang, H. S.</p> <p>1993-01-01</p> <p>Boundary conditions for fluctuating <span class="hlt">wall</span> temperature are required for near-<span class="hlt">wall</span> <span class="hlt">heat</span> transfer modeling. However, their correct specifications for arbitrary thermal boundary conditions are not clear. The conventional approach is to assume zero fluctuating <span class="hlt">wall</span> temperature or zero gradient for the temperature variance at the <span class="hlt">wall</span>. These are idealized specifications and the latter condition could lead to an ill posed problem for fully-developed pipe and channel flows. In this paper, the validity and extent of the zero fluctuating <span class="hlt">wall</span> temperature condition for <span class="hlt">heat</span> transfer calculations is examined. The approach taken is to assume a Taylor expansion in the <span class="hlt">wall</span> normal coordinate for the fluctuating temperature that is general enough to account for both zero and non-zero value at the <span class="hlt">wall</span>. Turbulent conductivity is calculated from the temperature variance and its dissipation rate. <span class="hlt">Heat</span> transfer calculations assuming both zero and non-zero fluctuating <span class="hlt">wall</span> temperature reveal that the zero fluctuating <span class="hlt">wall</span> temperature assumption is in general valid. The effects of non-zero fluctuating <span class="hlt">wall</span> temperature are limited only to a very small region near the <span class="hlt">wall</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1175154','DOE-PATENT-XML'); return false;" href="https://www.osti.gov/servlets/purl/1175154"><span>Local <span class="hlt">wall</span> <span class="hlt">heat</span> <span class="hlt">flux</span>/temperature meter for convective flow and method of utilizing same</span></a></p> <p><a target="_blank" href="http://www.osti.gov/doepatents">DOEpatents</a></p> <p>Boyd, Ronald D.; Ekhlassi, Ali; Cofie, Penrose</p> <p>2004-11-30</p> <p>According to one embodiment of the invention, a method includes providing a conduit having a fluid flowing therethrough, disposing a plurality of temperature measurement devices inside a <span class="hlt">wall</span> of the conduit, positioning at least some of the temperature measurement devices proximate an inside surface of the <span class="hlt">wall</span> of the conduit, positioning at least some of the temperature measurement devices at different radial positions at the same circumferential location within the <span class="hlt">wall</span>, measuring a plurality of temperatures of the <span class="hlt">wall</span> with respective ones of the temperature measurement devices to obtain a three-dimensional temperature topology of the <span class="hlt">wall</span>, determining the temperature dependent thermal conductivity of the conduit, and determining a multi-dimensional thermal characteristic of the inside surface of the <span class="hlt">wall</span> of the conduit based on extrapolation of the three-dimensional temperature topology and the temperature dependent thermal conductivities.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20080005138','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20080005138"><span>Local <span class="hlt">wall</span> <span class="hlt">heat</span> <span class="hlt">flux</span>/temperature meter for convective flow and method of utilizing same</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Cofie, Penrose (Inventor); Ekhlassi, Ali (Inventor); Boyd, Ronald D. (Inventor)</p> <p>2004-01-01</p> <p>According to one embodiment of the invention, a method includes providing a conduit having a fluid flowing therethrough, disposing a plurality of temperature measurement devices inside a <span class="hlt">wall</span> of the conduit, positioning at least some of the temperature measurement devices proximate an inside surface of the <span class="hlt">wall</span> of the conduit, positioning at least some of the temperature measurement devices at different radial positions at the same circumferential location within the <span class="hlt">wall</span>, measuring a plurality of temperatures of the <span class="hlt">wall</span> with respective ones of the temperature measurement devices to obtain a three-dimensional temperature topology of the <span class="hlt">wall</span>, determining the temperature dependent thermal conductivity of the conduit, and determining a multi-dimensional thermal characteristic of the inside surface of the <span class="hlt">wall</span> of the conduit based on extrapolation of the three-dimensional temperature topology and the temperature dependent thermal conductivities.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19920019509','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19920019509"><span><span class="hlt">Heat</span> exchanger with oscillating flow</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Scotti, Stephen J. (Inventor); Blosser, Max L. (Inventor); Camarda, Charles J. (Inventor)</p> <p>1992-01-01</p> <p>Various <span class="hlt">heat</span> exchange apparatuses are described in which an oscillating flow of primary coolant is used to dissipate an incident <span class="hlt">heat</span> <span class="hlt">flux</span>. The oscillating flow may be imparted by a reciprocating piston, a double action twin reciprocating piston, fluidic oscillators, or electromagnetic pumps. The oscillating fluid flows through at least one conduit in either an open loop or a closed loop. A secondary flow of coolant may be used to flow over the outer <span class="hlt">walls</span> of at least one conduit to remove <span class="hlt">heat</span> transferred from the primary coolant to the <span class="hlt">walls</span> of the conduit.</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('http://hdl.handle.net/2060/19940016022','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19940016022"><span><span class="hlt">Heat</span> exchanger with oscillating flow</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Scotti, Stephen J. (Inventor); Blosser, Max L. (Inventor); Camarda, Charles J. (Inventor)</p> <p>1993-01-01</p> <p>Various <span class="hlt">heat</span> exchange apparatuses are described in which an oscillating flow of primary coolant is used to dissipate an incident <span class="hlt">heat</span> <span class="hlt">flux</span>. The oscillating flow may be imparted by a reciprocating piston, a double action twin reciprocating piston, fluidic oscillators or electromagnetic pumps. The oscillating fluid flows through at least one conduit in either an open loop or a closed loop. A secondary flow of coolant may be used to flow over the outer <span class="hlt">walls</span> of at least one conduit to remove <span class="hlt">heat</span> transferred from the primary coolant to the <span class="hlt">walls</span> of the conduit.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JGRC..122..726R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JGRC..122..726R"><span>Surface <span class="hlt">flux</span> and ocean <span class="hlt">heat</span> transport convergence contributions to seasonal and interannual variations of ocean <span class="hlt">heat</span> content</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Roberts, C. D.; Palmer, M. D.; Allan, R. P.; Desbruyeres, D. G.; Hyder, P.; Liu, C.; Smith, D.</p> <p>2017-01-01</p> <p>We present an observation-based <span class="hlt">heat</span> budget analysis for seasonal and interannual variations of ocean <span class="hlt">heat</span> content (H) in the mixed layer (Hmld) and full-depth ocean (Htot). Surface <span class="hlt">heat</span> <span class="hlt">flux</span> and ocean <span class="hlt">heat</span> content estimates are combined using a novel Kalman smoother-based method. Regional contributions from ocean <span class="hlt">heat</span> transport convergences are inferred as a residual and the dominant drivers of Hmld and Htot are quantified for seasonal and interannual time scales. We find that non-Ekman ocean <span class="hlt">heat</span> transport processes dominate Hmld variations in the equatorial oceans and regions of strong ocean currents and substantial eddy activity. In these locations, surface temperature anomalies generated by ocean dynamics result in turbulent <span class="hlt">flux</span> anomalies that drive the overlying atmosphere. In addition, we find large regions of the Atlantic and Pacific oceans where <span class="hlt">heat</span> transports combine with local air-sea <span class="hlt">fluxes</span> to generate mixed layer temperature anomalies. In all locations, except regions of deep convection and water mass transformation, interannual variations in Htot are dominated by the internal rearrangement of <span class="hlt">heat</span> by ocean dynamics rather than the loss or addition of <span class="hlt">heat</span> at the surface. Our analysis suggests that, even in extratropical latitudes, initialization of ocean dynamical processes could be an important source of skill for interannual predictability of Hmld and Htot. Furthermore, we expect variations in Htot (and thus thermosteric sea level) to be more predictable than near surface temperature anomalies due to the increased importance of ocean <span class="hlt">heat</span> transport processes for full-depth <span class="hlt">heat</span> budgets.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20140016851','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20140016851"><span>Impacts of Soil-aquifer <span class="hlt">Heat</span> and Water <span class="hlt">Fluxes</span> on Simulated Global Climate</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Krakauer, N.Y.; Puma, Michael J.; Cook, B. I.</p> <p>2013-01-01</p> <p>Climate models have traditionally only represented <span class="hlt">heat</span> and water <span class="hlt">fluxes</span> within relatively shallow soil layers, but there is increasing interest in the possible role of <span class="hlt">heat</span> and water exchanges with the deeper subsurface. Here, we integrate an idealized 50m deep aquifer into the land surface module of the GISS ModelE general circulation model to test the influence of aquifer-soil moisture and <span class="hlt">heat</span> exchanges on climate variables. We evaluate the impact on the modeled climate of aquifer-soil <span class="hlt">heat</span> and water <span class="hlt">fluxes</span> separately, as well as in combination. The addition of the aquifer to ModelE has limited impact on annual-mean climate, with little change in global mean land temperature, precipitation, or evaporation. The seasonal amplitude of deep soil temperature is strongly damped by the soil-aquifer <span class="hlt">heat</span> <span class="hlt">flux</span>. This not only improves the model representation of permafrost area but propagates to the surface, resulting in an increase in the seasonal amplitude of surface air temperature of >1K in the Arctic. The soil-aquifer water and <span class="hlt">heat</span> <span class="hlt">fluxes</span> both slightly decrease interannual variability in soil moisture and in landsurface temperature, and decrease the soil moisture memory of the land surface on seasonal to annual timescales. The results of this experiment suggest that deepening the modeled land surface, compared to modeling only a shallower soil column with a no-<span class="hlt">flux</span> bottom boundary condition, has limited impact on mean climate but does affect seasonality and interannual persistence.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3995107','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3995107"><span>Estimation of Surface <span class="hlt">Heat</span> <span class="hlt">Flux</span> and Surface Temperature during Inverse <span class="hlt">Heat</span> Conduction under Varying Spray Parameters and Sample Initial Temperature</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Aamir, Muhammad; Liao, Qiang; Zhu, Xun; Aqeel-ur-Rehman; Wang, Hong</p> <p>2014-01-01</p> <p>An experimental study was carried out to investigate the effects of inlet pressure, sample thickness, initial sample temperature, and temperature sensor location on the surface <span class="hlt">heat</span> <span class="hlt">flux</span>, surface temperature, and surface ultrafast cooling rate using stainless steel samples of diameter 27 mm and thickness (mm) 8.5, 13, 17.5, and 22, respectively. Inlet pressure was varied from 0.2 MPa to 1.8 MPa, while sample initial temperature varied from 600°C to 900°C. Beck's sequential function specification method was utilized to estimate surface <span class="hlt">heat</span> <span class="hlt">flux</span> and surface temperature. Inlet pressure has a positive effect on surface <span class="hlt">heat</span> <span class="hlt">flux</span> (SHF) within a critical value of pressure. Thickness of the sample affects the maximum achieved SHF negatively. Surface <span class="hlt">heat</span> <span class="hlt">flux</span> as high as 0.4024 MW/m2 was estimated for a thickness of 8.5 mm. Insulation effects of vapor film become apparent in the sample initial temperature range of 900°C causing reduction in surface <span class="hlt">heat</span> <span class="hlt">flux</span> and cooling rate of the sample. A sensor location near to quenched surface is found to be a better choice to visualize the effects of spray parameters on surface <span class="hlt">heat</span> <span class="hlt">flux</span> and surface temperature. Cooling rate showed a profound increase for an inlet pressure of 0.8 MPa. PMID:24977219</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/491560','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/491560"><span>Critical <span class="hlt">heat</span> <span class="hlt">flux</span> (CHF) phenomenon on a downward facing curved surface</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>Cheung, F.B.; Haddad, K.H.; Liu, Y.C.</p> <p>1997-06-01</p> <p>This report describes a theoretical and experimental study of the boundary layer boiling and critical <span class="hlt">heat</span> <span class="hlt">flux</span> phenomena on a downward facing curved <span class="hlt">heating</span> surface, including both hemispherical and toroidal surfaces. A subscale boundary layer boiling (SBLB) test facility was developed to measure the spatial variation of the critical <span class="hlt">heat</span> <span class="hlt">flux</span> and observe the underlying mechanisms. Transient quenching and steady-state boiling experiments were performed in the SBLB facility under both saturated and subcooled conditions to obtain a complete database on the critical <span class="hlt">heat</span> <span class="hlt">flux</span>. To complement the experimental effort, an advanced hydrodynamic CHF model was developed from the conservation lawsmore » along with sound physical arguments. The model provides a clear physical explanation for the spatial variation of the CHF observed in the SBLB experiments and for the weak dependence of the CHF data on the physical size of the vessel. Based upon the CHF model, a scaling law was established for estimating the local critical <span class="hlt">heat</span> <span class="hlt">flux</span> on the outer surface of a <span class="hlt">heated</span> hemispherical vessel that is fully submerged in water. The scaling law, which compares favorably with all the available local CHF data obtained for various vessel sizes, can be used to predict the local CHF limits on large commercial-size vessels. This technical information represents one of the essential elements that is needed in assessing the efficacy of external cooling of core melt by cavity flooding as a severe accident management strategy. 83 figs., 3 tabs.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/ADA266086','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA266086"><span>Boiling <span class="hlt">Heat</span>-Transfer Processes and Their Application in the Cooling of High <span class="hlt">Heat</span> <span class="hlt">Flux</span> Devices</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>1993-06-01</p> <p>1991, pp. 395-397. 385. Galloway, J. E. and Mudawar , 1. "Critical <span class="hlt">Heat</span> <span class="hlt">Flux</span> Enhancement by Means of Liquid Subcooling and Centrifugal Force Induced...Flow Boiling <span class="hlt">Heat</span> Transfer for a Spirally Fluted Tube." <span class="hlt">Heat</span> Tran~ler Engineering, Vol. 13, No.1, 1992, pp. 42-52. 390. Willingham, T. C. and Mudawar</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1985PhFl...28.3333S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1985PhFl...28.3333S"><span>Magnetic <span class="hlt">flux</span> trapping during field reversal in the formation of a field-reversed configuration</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Steinhauer, Loren C.</p> <p>1985-11-01</p> <p>The flow of plasma and magnetic <span class="hlt">flux</span> toward a <span class="hlt">wall</span> is examined in a slab geometry where the magnetic field is parallel to the <span class="hlt">wall</span>. Magnetohydrodynamic (MHD) flow with a quasisteady approximation is assumed that reduces the problem to three coupled ordinary differential equations. The calculated behavior shows that a thin current sheath is established at the <span class="hlt">wall</span> in which a variety of phenomena appear, including significant resistive <span class="hlt">heating</span> and rapid deceleration of the plasma flow. The sheath physics determines the speed at which <span class="hlt">flux</span> and plasma flow toward the <span class="hlt">wall</span>. The model has been applied to the field-reversal phase of a field-reversed theta pinch, during which the reduced magnetic field near the <span class="hlt">wall</span> drives an outward flow of plasma and magnetic <span class="hlt">flux</span>. The analysis leads to approximate expressions for the instantaneous flow speed, the loss of magnetic <span class="hlt">flux</span> during the field reversal phase, the integrated <span class="hlt">heat</span> flow to the <span class="hlt">wall</span>, and the highest possible magnetic <span class="hlt">flux</span> retained after reversal. Predictions from this model are compared with previous time-dependent MHD calculations and with experimental results from the TRX-1 [Proceedings of the 4th Symposium on the Physics and Technology of Compact Toroids, 27-29 October 1981 (Lawrence Livermore National Laboratory, Livermore, CA, 1982), p. 61] and TRX-2 [Proceedings of the 6th U.S. Symposium on Compact Toroid Research, 20-23 February, 1984 (Princeton Plasma Physics Laboratory, Princeton, NJ, 1984), p. 154] experiments.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19850046194&hterms=magnetic+cooling&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D80%26Ntt%3Dmagnetic%2Bcooling','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19850046194&hterms=magnetic+cooling&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D80%26Ntt%3Dmagnetic%2Bcooling"><span>On the <span class="hlt">heating</span> mechanism of magnetic <span class="hlt">flux</span> loops in the solar atmosphere</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Song, M. T.; Wu, S. T.</p> <p>1984-01-01</p> <p>An investigation is conducted of physical <span class="hlt">heating</span> mechanisms due to the ponderomotive forces exerted by turbulent waves along the solar atmosphere's curved magnetic <span class="hlt">flux</span> loops. Results indicate that the temperature difference between the inside and outside of the <span class="hlt">flux</span> loop can be classified into three parts, two of which represent the cooling or <span class="hlt">heating</span> effect exerted by the ponderomotive force, while the third is the <span class="hlt">heating</span> effect due to turbulent energy conversion from the localized plasma. This <span class="hlt">heating</span> mechanism is used to illustrate solar atmospheric <span class="hlt">heating</span> by means of an example that leads to the formulation of plages.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22596746-influence-joule-heating-current-induced-domain-wall-depinning','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22596746-influence-joule-heating-current-induced-domain-wall-depinning"><span>Influence of Joule <span class="hlt">heating</span> on current-induced domain <span class="hlt">wall</span> depinning</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>Moretti, Simone, E-mail: simone.moretti@usal.es; Raposo, Victor; Martinez, Eduardo</p> <p>2016-06-07</p> <p>The domain <span class="hlt">wall</span> depinning from a notch in a Permalloy nanostrip on top of a SiO{sub 2}/Si substrate is studied theoretically under application of static magnetic fields and the injection of short current pulses. The influence of Joule <span class="hlt">heating</span> on current-induced domain <span class="hlt">wall</span> depinning is explored self-consistently by coupling the magnetization dynamics in the ferromagnetic strip to the <span class="hlt">heat</span> transport throughout the system. Our results indicate that Joule <span class="hlt">heating</span> plays a remarkable role in these processes, resulting in a reduction in the critical depinning field and/or in a temporary destruction of the ferromagnetic order for typically injected current pulses. Inmore » agreement with experimental observations, similar pinning-depinning phase diagrams can be deduced for both current polarities when the Joule <span class="hlt">heating</span> is taken into account. These observations, which are incompatible with the sole contribution of spin transfer torques, provide a deeper understanding of the physics underlying these processes and establish the real scope of the spin transfer torque. They are also relevant for technological applications based on current-induced domain-<span class="hlt">wall</span> motion along soft strips.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/17443543','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/17443543"><span>Double <span class="hlt">wall</span> versus single <span class="hlt">wall</span> incubator for reducing <span class="hlt">heat</span> loss in very low birth weight infants in incubators.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Laroia, N; Phelps, D L; Roy, J</p> <p>2007-04-18</p> <p>Studies have shown improved survival of newborn infants maintained in the thermoneutral range. The concept of an incubator with additional insulation, a double plexiglass <span class="hlt">wall</span>, is appealing for very low birth weight infants as it may help to provide a thermoneutral environment. To assess the effects of double <span class="hlt">walled</span> incubator versus a single <span class="hlt">wall</span> incubator on insensible water loss, rate of oxygen consumption, episodes of hypothermia, time to regain birth weight, duration of hospitalization and infant mortality in premature infants. The standard search strategy of the Cochrane Neonatal Review Group was used. This included searches of electronic databases: Oxford Database of Perinatal Trials, Cochrane Central Register of Controlled Trials (CENTRAL, The Cochrane Library, Issue 1, 2006), MEDLINE (1966 - 2006), EMBASE, previous reviews including cross references, abstracts, conference and symposia proceedings, expert informants in all published languages, and CINAHL (1982 - 2006). Only studies using random or quasi-random methods of allocation were considered for this review. Eligible studies assessed at least one of the outcome variables identified as important to this topic. Independent data extraction and quality assessment of included trials was conducted by the review authors. Data were analyzed using generic inverse variance methodology and weighted mean difference (WMD). Results are presented with 95% confidence intervals. Meta-analysis was undertaken using a fixed effect model. Three studies met the criteria. Four other studies were excluded, as they did not compare double versus single <span class="hlt">wall</span> incubators (details of the studies are given in the included and excluded studies section). Double <span class="hlt">wall</span> incubators have the advantage of decreasing <span class="hlt">heat</span> loss, decreasing <span class="hlt">heat</span> production and decreasing radiant <span class="hlt">heat</span> loss when compared to single <span class="hlt">wall</span> incubators. There is also the advantage of reduced oxygen consumption. A minimal increase in conductive <span class="hlt">heat</span> loss was noted when</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28410347','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28410347"><span>Accuracy of Zero-<span class="hlt">Heat-Flux</span> Cutaneous Temperature in Intensive Care Adults.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Dahyot-Fizelier, Claire; Lamarche, Solène; Kerforne, Thomas; Bénard, Thierry; Giraud, Benoit; Bellier, Rémy; Carise, Elsa; Frasca, Denis; Mimoz, Olivier</p> <p>2017-07-01</p> <p>To compare accuracy of a continuous noninvasive cutaneous temperature using zero-<span class="hlt">heat-flux</span> method to esophageal temperature and arterial temperature. Prospective study. ICU and NeuroICU, University Hospital. Fifty-two ICU patients over a 4-month period who required continuous temperature monitoring were included in the study, after informed consent. All patients had esophageal temperature probe and a noninvasive cutaneous device to monitor their core temperature continuously. In seven patients who required cardiac output monitoring, continuous iliac arterial temperature was collected. Simultaneous core temperatures were recorded from 1 to 5 days. Comparison to the esophageal temperature, considered as the reference in this study, used the Bland and Altman method with adjustment for multiple measurements per patient. The esophageal temperature ranged from 33°C to 39.7°C, 61,298 pairs of temperature using zero-<span class="hlt">heat-flux</span> and esophageal temperature were collected and 1,850 triple of temperature using zero-<span class="hlt">heat-flux</span>, esophageal temperature, and arterial temperature. Bias and limits of agreement for temperature using zero-<span class="hlt">heat-flux</span> were 0.19°C ± 0.53°C compared with esophageal temperature with an absolute difference of temperature pairs equal to or lower than 0.5°C of 92.6% (95% CI, 91.9-93.4%) of cases and equal to or lower than 1°C for 99.9% (95% CI, 99.7-100.0%) of cases. Compared with arterial temperature, bias and limits of agreement were -0.00°C ± 0.36°C with an absolute difference of temperature pairs equal to or lower than 0.5°C of 99.8% (95% CI, 95.3-100%) of cases. All absolute difference of temperature pairs between temperature using zero-<span class="hlt">heat-flux</span> and arterial temperature and between arterial temperature and esophageal temperature were equal to or lower than 1°C. No local or systemic serious complication was observed. These results suggest a comparable reliability of the cutaneous sensor using the zero-<span class="hlt">heat-flux</span> method compared with esophageal or</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5381797','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5381797"><span>Darcy-Forchheimer flow with Cattaneo-Christov <span class="hlt">heat</span> <span class="hlt">flux</span> and homogeneous-heterogeneous reactions</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Hayat, Tasawar; Haider, Farwa; Alsaedi, Ahmed</p> <p>2017-01-01</p> <p>Here Darcy-Forchheimer flow of viscoelastic fluids has been analyzed in the presence of Cattaneo-Christov <span class="hlt">heat</span> <span class="hlt">flux</span> and homogeneous-heterogeneous reactions. Results for two viscoelastic fluids are obtained and compared. A linear stretching surface has been used to generate the flow. Flow in porous media is characterized by considering the Darcy-Forchheimer model. Modified version of Fourier's law through Cattaneo-Christov <span class="hlt">heat</span> <span class="hlt">flux</span> is employed. Equal diffusion coefficients are employed for both reactants and auto catalyst. Optimal homotopy scheme is employed for solutions development of nonlinear problems. Solutions expressions of velocity, temperature and concentration fields are provided. Skin friction coefficient and <span class="hlt">heat</span> transfer rate are computed and analyzed. Here the temperature and thermal boundary layer thickness are lower for Cattaneo-Christov <span class="hlt">heat</span> <span class="hlt">flux</span> model in comparison to classical Fourier's law of <span class="hlt">heat</span> conduction. Moreover, the homogeneous and heterogeneous reactions parameters have opposite behaviors for concentration field. PMID:28380014</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016APS..DPPNO6011L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016APS..DPPNO6011L"><span>Particle-In-Cell simulation concerning <span class="hlt">heat-flux</span> mitigation using electromagnetic fields</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lüskow, Karl Felix; Duras, Julia; Kemnitz, Stefan; Kahnfeld, Daniel; Matthias, Paul; Bandelow, Gunnas; Schneider, Ralf; Konigorski, Detlev</p> <p>2016-10-01</p> <p>In space missions enormous amount of money is spent for the thermal protection system for re-entry. To avoid complex materials and save money one idea is to reduce the <span class="hlt">heat-flux</span> towards the spacecraft. The partially-ionized gas can be controlled by electromagnetic fields. For first-principle tests partially ionized argon flow from an arc-jet was used to measure the <span class="hlt">heat-flux</span> mitigation created by an external magnetic field. In the successful experiment a reduction of 85% was measured. In this work the Particle-in-Cell (PIC) method was used to simulate this experiment. PIC is able to reproduce the <span class="hlt">heat</span> <span class="hlt">flux</span> mitigation qualitatively. The main mechanism is identified as a changed electron transport and by this, modified electron density due to the reaction to the applied magnetic field. Ions follow due to quasi-neutrality and influence then strongly by charge exchange collisions the neutrals dynamics and <span class="hlt">heat</span> deposition. This work was supported by the German Space Agency DLR through Project 50RS1508.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015PhPl...22d2516M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015PhPl...22d2516M"><span>Turbulent transport regimes and the scrape-off layer <span class="hlt">heat</span> <span class="hlt">flux</span> width</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Myra, J. R.; D'Ippolito, D. A.; Russell, D. A.</p> <p>2015-04-01</p> <p>Understanding the responsible mechanisms and resulting scaling of the scrape-off layer (SOL) <span class="hlt">heat</span> <span class="hlt">flux</span> width is important for predicting viable operating regimes in future tokamaks and for seeking possible mitigation schemes. In this paper, we present a qualitative and conceptual framework for understanding various regimes of edge/SOL turbulence and the role of turbulent transport as the mechanism for establishing the SOL <span class="hlt">heat</span> <span class="hlt">flux</span> width. Relevant considerations include the type and spectral characteristics of underlying instabilities, the location of the gradient drive relative to the SOL, the nonlinear saturation mechanism, and the parallel <span class="hlt">heat</span> transport regime. We find a <span class="hlt">heat</span> <span class="hlt">flux</span> width scaling with major radius R that is generally positive, consistent with the previous findings [Connor et al., Nucl. Fusion 39, 169 (1999)]. The possible relationship of turbulence mechanisms to the neoclassical orbit width or heuristic drift mechanism in core energy confinement regimes known as low (L) mode and high (H) mode is considered, together with implications for the future experiments.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/16711925','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/16711925"><span>Effect of <span class="hlt">heat</span> <span class="hlt">flux</span> on differential rotation in turbulent convection.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Kleeorin, Nathan; Rogachevskii, Igor</p> <p>2006-04-01</p> <p>We studied the effect of the turbulent <span class="hlt">heat</span> <span class="hlt">flux</span> on the Reynolds stresses in a rotating turbulent convection. To this end we solved a coupled system of dynamical equations which includes the equations for the Reynolds stresses, the entropy fluctuations, and the turbulent <span class="hlt">heat</span> <span class="hlt">flux</span>. We used a spectral tau approximation in order to close the system of dynamical equations. We found that the ratio of the contributions to the Reynolds stresses caused by the turbulent <span class="hlt">heat</span> <span class="hlt">flux</span> and the anisotropic eddy viscosity is of the order of approximately 10(L rho/l0)2, where l0 is the maximum scale of turbulent motions and L rho is the fluid density variation scale. This effect is crucial for the formation of the differential rotation and should be taken into account in the theories of the differential rotation of the Sun, stars, and planets. In particular, we demonstrated that this effect may cause the differential rotation which is comparable with the typical solar differential rotation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JThSc..26..166X','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JThSc..26..166X"><span>The effect of <span class="hlt">heating</span> direction on flow boiling <span class="hlt">heat</span> transfer of R134a in micro-channels</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Xu, Mingchen; Jia, Li; Dang, Chao; Peng, Qi</p> <p>2017-04-01</p> <p>This paper presents effects of <span class="hlt">heating</span> directions on <span class="hlt">heat</span> transfer performance of R134a flow boiling in micro- channel <span class="hlt">heat</span> sink. The <span class="hlt">heat</span> sink has 30 parallel rectangular channels with cross-sectional dimensions of 500μm width 500μm depth and 30mm length. The experimental operation condition ranges of the <span class="hlt">heat</span> <span class="hlt">flux</span> and the mass <span class="hlt">flux</span> were 13.48 to 82.25 W/cm2 and 373.3 to 1244.4 kg/m2s respectively. The vapor quality ranged from 0.07 to 0.93. The <span class="hlt">heat</span> transfer coefficients of top <span class="hlt">heating</span> and bottom <span class="hlt">heating</span> both were up to 25 kW/m2 K. Two dominate transfer mechanisms of nucleate boiling and convection boiling were observed according to boiling curves. The experimental results indicated that the <span class="hlt">heat</span> transfer coefficient of bottom <span class="hlt">heating</span> was 13.9% higher than top <span class="hlt">heating</span> in low <span class="hlt">heat</span> <span class="hlt">flux</span>, while in high <span class="hlt">heat</span> <span class="hlt">flux</span>, the <span class="hlt">heat</span> transfer coefficient of bottom <span class="hlt">heating</span> was 9.9%.higher than the top <span class="hlt">heating</span>, because bubbles were harder to divorce the <span class="hlt">heating</span> <span class="hlt">wall</span>. And a modified correlation was provided to predict <span class="hlt">heat</span> transfer of top <span class="hlt">heating</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22597986-design-calibration-novel-transient-radiative-heat-flux-meter-spacecraft-thermal-test','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22597986-design-calibration-novel-transient-radiative-heat-flux-meter-spacecraft-thermal-test"><span>Design and calibration of a novel transient radiative <span class="hlt">heat</span> <span class="hlt">flux</span> meter for a spacecraft thermal test</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>Sheng, Chunchen; Hu, Peng, E-mail: hupeng@ustc.edu.cn; Cheng, Xiaofang</p> <p>2016-06-15</p> <p>Radiative <span class="hlt">heat</span> <span class="hlt">flux</span> measurement is significantly important for a spacecraft thermal test. To satisfy the requirements of both high accuracy and fast response, a novel transient radiative <span class="hlt">heat</span> <span class="hlt">flux</span> meter was developed. Its thermal receiver consists of a central thermal receiver and two thermal guarded annular plates, which ensure the temperature distribution of the central thermal receiver to be uniform enough for reasonably applying lumped <span class="hlt">heat</span> capacity method in a transient radiative <span class="hlt">heat</span> <span class="hlt">flux</span> measurement. This novel transient radiative <span class="hlt">heat</span> <span class="hlt">flux</span> meter design can also take accurate measurements regardless of spacecraft surface temperature and incident radiation spectrum. The measurement principlemore » was elaborated and the coefficients were calibrated. Experimental results from testing a blackbody furnace and an Xenon lamp show that this novel transient radiative <span class="hlt">heat</span> <span class="hlt">flux</span> meter can be used to measure transient radiative <span class="hlt">heat</span> <span class="hlt">flux</span> up to 1400 W/m{sup 2} with high accuracy and the response time of less than 10 s.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19870006083','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19870006083"><span>Comparison of measured and modeled radiation, <span class="hlt">heat</span> and water vapor <span class="hlt">fluxes</span>: FIFE pilot study</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Blad, Blaine L.; Hubbard, Kenneth G.; Verma, Shashi B.; Starks, Patrick; Norman, John M.; Walter-Shea, Elizabeth</p> <p>1987-01-01</p> <p>The feasibility of using radio frequency receivers to collect data from automated weather stations to model <span class="hlt">fluxes</span> of latent <span class="hlt">heat</span>, sensible <span class="hlt">heat</span>, and radiation using routine weather data collected by automated weather stations was tested and the estimated <span class="hlt">fluxes</span> were compared with <span class="hlt">fluxes</span> measured over wheat. The model Cupid was used to model the <span class="hlt">fluxes</span>. Two or more automated weather stations, interrogated by radio frequency and other means, were utilized to examine some of the climatic variability of the First ISLSCP (International Satellite Land-Surface Climatology Project) Field Experiment (FIFE) site, to measure and model reflected and emitted radiation streams from various locations at the site and to compare modeled latent and sensible <span class="hlt">heat</span> <span class="hlt">fluxes</span> with measured values. Some bidirectional reflected and emitted radiation data were collected from 23 locations throughout the FIFE site. Analysis of these data along with analysis of the measured sensible and latent <span class="hlt">heat</span> <span class="hlt">fluxes</span> is just beginning.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018PhRvE..97b2122S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018PhRvE..97b2122S"><span>Hyperbolic <span class="hlt">heat</span> conduction, effective temperature, and third law for nonequilibrium systems with <span class="hlt">heat</span> <span class="hlt">flux</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sobolev, S. L.</p> <p>2018-02-01</p> <p>Some analogies between different nonequilibrium <span class="hlt">heat</span> conduction models, particularly random walk, the discrete variable model, and the Boltzmann transport equation with the single relaxation time approximation, have been discussed. We show that, under an assumption of a finite value of the <span class="hlt">heat</span> carrier velocity, these models lead to the hyperbolic <span class="hlt">heat</span> conduction equation and the modified Fourier law with relaxation term. Corresponding effective temperature and entropy have been introduced and analyzed. It has been demonstrated that the effective temperature, defined as a geometric mean of the kinetic temperatures of the <span class="hlt">heat</span> carriers moving in opposite directions, acts as a criterion for thermalization and is a nonlinear function of the kinetic temperature and <span class="hlt">heat</span> <span class="hlt">flux</span>. It is shown that, under highly nonequilibrium conditions when the <span class="hlt">heat</span> <span class="hlt">flux</span> tends to its maximum possible value, the effective temperature, <span class="hlt">heat</span> capacity, and local entropy go to zero even at a nonzero equilibrium temperature. This provides a possible generalization of the third law to nonequilibrium situations. Analogies and differences between the proposed effective temperature and some other definitions of a temperature in nonequilibrium state, particularly for active systems, disordered semiconductors under electric field, and adiabatic gas flow, have been shown and discussed. Illustrative examples of the behavior of the effective temperature and entropy during nonequilibrium <span class="hlt">heat</span> conduction in a monatomic gas and a strong shockwave have been analyzed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JIEIC.tmp..264S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JIEIC.tmp..264S"><span>Prediction of Experimental Surface <span class="hlt">Heat</span> <span class="hlt">Flux</span> of Thin Film Gauges using ANFIS</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sarma, Shrutidhara; Sahoo, Niranjan; Unal, Aynur</p> <p>2018-05-01</p> <p>Precise quantification of surface <span class="hlt">heat</span> <span class="hlt">fluxes</span> in highly transient environment is of paramount importance from the design point of view of several engineering equipment like thermal protection or cooling systems. Such environments are simulated in experimental facilities by exposing the surface with transient <span class="hlt">heat</span> loads typically step/impulsive in nature. The surface <span class="hlt">heating</span> rates are then determined from highly transient temperature history captured by efficient surface temperature sensors. The classical approach is to use thin film gauges (TFGs) in which temperature variations are acquired within milliseconds, thereby allowing calculation of surface <span class="hlt">heat</span> <span class="hlt">flux</span>, based on the theory of one-dimensional <span class="hlt">heat</span> conduction on a semi-infinite body. With recent developments in the soft computing methods, the present study is an attempt for the application of intelligent system technique, called adaptive neuro fuzzy inference system (ANFIS) to recover surface <span class="hlt">heat</span> <span class="hlt">fluxes</span> from a given temperature history recorded by TFGs without having the need to solve lengthy analytical equations. Experiments have been carried out by applying known quantity of `impulse <span class="hlt">heat</span> load' through laser beam on TFGs. The corresponding voltage signals have been acquired and surface <span class="hlt">heat</span> <span class="hlt">fluxes</span> are estimated through classical analytical approach. These signals are then used to `train' the ANFIS model, which later predicts output for `test' values. Results from both methods have been compared and these surface <span class="hlt">heat</span> <span class="hlt">fluxes</span> are used to predict the non-linear relationship between thermal and electrical properties of the gauges that are exceedingly pertinent to the design of efficient TFGs. Further, surface plots have been created to give an insight about dimensionality effect of the non-linear dependence of thermal/electrical parameters on each other. Later, it is observed that a properly optimized ANFIS model can predict the impulsive <span class="hlt">heat</span> profiles with significant accuracy. This paper thus shows 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_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('http://adsabs.harvard.edu/abs/2017MMTB...48.1951Y','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017MMTB...48.1951Y"><span>Controlling Radiative <span class="hlt">Heat</span> Transfer Across the Mold <span class="hlt">Flux</span> Layer by the Scattering Effect of the Borosilicate Mold <span class="hlt">Flux</span> System with Metallic Iron</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Yoon, Dae-Woo; Cho, Jung-Wook; Kim, Seon-Hyo</p> <p>2017-08-01</p> <p>The present study proposes a countermeasure for regulating total <span class="hlt">heat</span> <span class="hlt">flux</span> through the mold <span class="hlt">flux</span> layer by designed mold <span class="hlt">flux</span> with additive metallic iron particles. The <span class="hlt">heat</span> <span class="hlt">flux</span> through the B2O3-CaO-SiO2-Na2O-CaF2-Fe system was investigated using the infrared emitter technique to evaluate total <span class="hlt">flux</span> density across the mold <span class="hlt">flux</span> film. Both scanning electron microscope (SEM) and X-ray diffraction analysis were employed in order to identify the morphological and compositional changes of the crystalline phase, according to increasing iron contents in the mold <span class="hlt">flux</span>. It was confirmed that the crystalline layer of studied mold <span class="hlt">fluxes</span> does not have a meaningful effect on the total <span class="hlt">heat</span> <span class="hlt">flux</span> density due to the similar structure and fraction of the crystalline phase. The extinction coefficient was measured for glassy mold <span class="hlt">fluxes</span> using an ultraviolet/visible and a Fourier transformation-infrared ray spectrometer in the range of 0.5 to 5 μm. For analyzing the scattering behavior of iron particles on the extinction coefficient, the number density and diameter of particles were observed by an automated SEM (auto-SEM). With these data, Mie scattering theory is adopted to define the scattering behavior of dispersed iron droplets in glassy matrix. It was found that the theoretical scattering coefficient demonstrated about 1623 to 3295 m-1, which is in accordance with the experimental results. In doing so, this study successfully achieves the strong scattering behavior that would contribute greatly to the optimization of overall <span class="hlt">heat</span> <span class="hlt">flux</span> through the mold <span class="hlt">flux</span> film during the casting process.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011MeScT..22j5402O','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011MeScT..22j5402O"><span>High-resolution hot-film measurement of surface <span class="hlt">heat</span> <span class="hlt">flux</span> to an impinging jet</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>O'Donovan, T. S.; Persoons, T.; Murray, D. B.</p> <p>2011-10-01</p> <p>To investigate the complex coupling between surface <span class="hlt">heat</span> transfer and local fluid velocity in convective <span class="hlt">heat</span> transfer, advanced techniques are required to measure the surface <span class="hlt">heat</span> <span class="hlt">flux</span> at high spatial and temporal resolution. Several established flow velocity techniques such as laser Doppler anemometry, particle image velocimetry and hot wire anemometry can measure fluid velocities at high spatial resolution (µm) and have a high-frequency response (up to 100 kHz) characteristic. Equivalent advanced surface <span class="hlt">heat</span> transfer measurement techniques, however, are not available; even the latest advances in high speed thermal imaging do not offer equivalent data capture rates. The current research presents a method of measuring point surface <span class="hlt">heat</span> <span class="hlt">flux</span> with a hot film that is flush mounted on a <span class="hlt">heated</span> flat surface. The film works in conjunction with a constant temperature anemometer which has a bandwidth of 100 kHz. The bandwidth of this technique therefore is likely to be in excess of more established surface <span class="hlt">heat</span> <span class="hlt">flux</span> measurement techniques. Although the frequency response of the sensor is not reported here, it is expected to be significantly less than 100 kHz due to its physical size and capacitance. To demonstrate the efficacy of the technique, a cooling impinging air jet is directed at the <span class="hlt">heated</span> surface, and the power required to maintain the hot-film temperature is related to the local <span class="hlt">heat</span> <span class="hlt">flux</span> to the fluid air flow. The technique is validated experimentally using a more established surface <span class="hlt">heat</span> <span class="hlt">flux</span> measurement technique. The thermal performance of the sensor is also investigated numerically. It has been shown that, with some limitations, the measurement technique accurately measures the surface <span class="hlt">heat</span> transfer to an impinging air jet with improved spatial resolution for a wide range of experimental parameters.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1321430-nonlinear-fluid-simulation-particle-heat-fluxes-during-burst-elms-diii-bout++-code-fluid-simulation-particle-heat-fluxes-during-burst-elms-diid-bout++-code','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1321430-nonlinear-fluid-simulation-particle-heat-fluxes-during-burst-elms-diii-bout++-code-fluid-simulation-particle-heat-fluxes-during-burst-elms-diid-bout++-code"><span>Nonlinear fluid simulation of particle and <span class="hlt">heat</span> <span class="hlt">fluxes</span> during burst of ELMs on DIII-D with BOUT++ code [Fluid Simulation of Particle and <span class="hlt">Heat</span> <span class="hlt">Fluxes</span> during Burst of ELMs on DIID with BOUT++ code</span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Xia, T. Y.; Xu, X. Q.</p> <p>2015-09-01</p> <p>In order to study the distribution and evolution of the transient particle and <span class="hlt">heat</span> <span class="hlt">fluxes</span> during edge-localized mode (ELM) bursts, a BOUT++ six-field two-fluid model based on the Braginskii equations with non-ideal physics effects is used to simulate pedestal collapse in divertor geometry. We used the profiles from the DIII-D H-mode discharge #144382 with fast target <span class="hlt">heat</span> <span class="hlt">flux</span> measurements as the initial conditions for the simulations. Moreover, a <span class="hlt">flux</span>-limited parallel thermal conduction is used with three values of the <span class="hlt">flux</span>-limiting coefficientmore » $${{\\alpha}_{j}}$$ , free streaming model with $${{\\alpha}_{j}}=1$$ , sheath-limit with $${{\\alpha}_{j}}=0.05$$ , and one value in between. The studies show that a 20 times increase in $${{\\alpha}_{j}}$$ leads to ~6 times increase in the <span class="hlt">heat</span> <span class="hlt">flux</span> amplitude to both the inner and outer targets, and the widths of the <span class="hlt">fluxes</span> are also expanded. The sheath-limit model of <span class="hlt">flux</span>-limiting coefficient is found to be the most appropriate one, which shows ELM sizes close to the measurements. The evolution of the density profile during the burst of ELMs of DIII-D discharge #144382 is simulated, and the collapse in width and depth of $${{n}_{\\text{e}}}$$ are reproduced at different time steps. The growing process of the profiles for the <span class="hlt">heat</span> <span class="hlt">flux</span> at divertor targets during the burst of ELMs measured by IRTV (infrared television) is also reproduced by this model. The widths of <span class="hlt">heat</span> <span class="hlt">fluxes</span> towards targets are a little narrower, and the peak amplitudes are twice the measurements possibly due to the lack of a model of divertor radiation which can effectively reduce the <span class="hlt">heat</span> <span class="hlt">fluxes</span>. The magnetic flutter combined with parallel thermal conduction is found to be able to increase the total <span class="hlt">heat</span> loss by around 33% since the magnetic flutter terms provide the additional conductive <span class="hlt">heat</span> transport in the radial direction. Finally, the <span class="hlt">heat</span> <span class="hlt">flux</span> profile at both the inner and outer targets is obviously broadened by magnetic flutter. The</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28063826','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28063826"><span>Evaluation of <span class="hlt">Heat</span> <span class="hlt">Flux</span> Measurement as a New Process Analytical Technology Monitoring Tool in Freeze Drying.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Vollrath, Ilona; Pauli, Victoria; Friess, Wolfgang; Freitag, Angelika; Hawe, Andrea; Winter, Gerhard</p> <p>2017-05-01</p> <p>This study investigates the suitability of <span class="hlt">heat</span> <span class="hlt">flux</span> measurement as a new technique for monitoring product temperature and critical end points during freeze drying. The <span class="hlt">heat</span> <span class="hlt">flux</span> sensor is tightly mounted on the shelf and measures non-invasively (no contact with the product) the <span class="hlt">heat</span> transferred from shelf to vial. <span class="hlt">Heat</span> <span class="hlt">flux</span> data were compared to comparative pressure measurement, thermocouple readings, and Karl Fischer titration as current state of the art monitoring techniques. The whole freeze drying process including freezing (both by ramp freezing and controlled nucleation) and primary and secondary drying was considered. We found that direct measurement of the transferred <span class="hlt">heat</span> enables more insights into thermodynamics of the freezing process. Furthermore, a vial <span class="hlt">heat</span> transfer coefficient can be calculated from <span class="hlt">heat</span> <span class="hlt">flux</span> data, which ultimately provides a non-invasive method to monitor product temperature throughout primary drying. The end point of primary drying determined by <span class="hlt">heat</span> <span class="hlt">flux</span> measurements was in accordance with the one defined by thermocouples. During secondary drying, <span class="hlt">heat</span> <span class="hlt">flux</span> measurements could not indicate the progress of drying as monitoring the residual moisture content. In conclusion, <span class="hlt">heat</span> <span class="hlt">flux</span> measurements are a promising new non-invasive tool for lyophilization process monitoring and development using energy transfer as a control parameter. Copyright © 2017 American Pharmacists Association®. Published by Elsevier Inc. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018AIPC.1959e0009D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018AIPC.1959e0009D"><span>Investigation of <span class="hlt">heat</span> <span class="hlt">flux</span> on aerodynamic body in supersonic gas flow with local energy deposition</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Dobrov, Y. V.; Lashkov, V. A.; Mashek, I. Ch.; Khoronzhuk, R. S.</p> <p>2018-05-01</p> <p>Existence and intensive growth of <span class="hlt">heat</span> <span class="hlt">flux</span> on a vehicle is one of the main problems in hypersonic flight. Experimental study of <span class="hlt">heat</span> <span class="hlt">flux</span> in the stagnation point of a blunt cylinder in supersonic flow was made using gradient <span class="hlt">heat</span> <span class="hlt">flux</span> sensor. It was found that a transfer function of the measuring system should be used for obtaining data at fast-changing <span class="hlt">heat</span> <span class="hlt">flux</span> measurements. It was established that it was possible to produce a short-term <span class="hlt">heat</span> transfer from the surface of streamlined body with the help of microwave discharge. Numerical simulation showed that it is possible to change nature of the flow by means of local energy deposition in case of streamlined wedge.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20060047645','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20060047645"><span>Local <span class="hlt">Heat</span> <span class="hlt">Flux</span> Measurements with Single Element Coaxial Injectors</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Jones, Gregg; Protz, Christopher; Bullard, Brad; Hulka, James</p> <p>2006-01-01</p> <p>To support the mission for the NASA Vision for Space Exploration, the NASA Marshall Space Flight Center conducted a program in 2005 to improve the capability to predict local thermal compatibility and <span class="hlt">heat</span> transfer in liquid propellant rocket engine combustion devices. The ultimate objective was to predict and hence reduce the local peak <span class="hlt">heat</span> <span class="hlt">flux</span> due to injector design, resulting in a significant improvement in overall engine reliability and durability. Such analyses are applicable to combustion devices in booster, upper stage, and in-space engines, as well as for small thrusters with few elements in the injector. In this program, single element and three-element injectors were hot-fire tested with liquid oxygen and ambient temperature gaseous hydrogen propellants at The Pennsylvania State University Cryogenic Combustor Laboratory from May to August 2005. Local <span class="hlt">heat</span> <span class="hlt">fluxes</span> were measured in a 1-inch internal diameter <span class="hlt">heat</span> sink combustion chamber using Medtherm coaxial thermocouples and Gardon <span class="hlt">heat</span> <span class="hlt">flux</span> gauges. Injectors were tested with shear coaxial and swirl coaxial elements, including recessed, flush and scarfed oxidizer post configurations, and concentric and non-concentric fuel annuli. This paper includes general descriptions of the experimental hardware, instrumentation, and results of the hot-fire testing for three of the single element injectors - recessed-post shear coaxial with concentric fuel, flush-post swirl coaxial with concentric fuel, and scarfed-post swirl coaxial with concentric fuel. Detailed geometry and test results will be published elsewhere to provide well-defined data sets for injector development and model validatation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20090008662','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20090008662"><span>Thermal Capacitance (Slug) Calorimeter Theory Including <span class="hlt">Heat</span> Losses and Other Decaying Processes</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Hightower, T. Mark; Olivares, Ricardo A.; Philippidis, Daniel</p> <p>2008-01-01</p> <p>A mathematical model, termed the Slug Loss Model, has been developed for describing thermal capacitance (slug) calorimeter behavior when <span class="hlt">heat</span> losses and other decaying processes are not negligible. This model results in the temperature time slope taking the mathematical form of exponential decay. When data is found to fit well to this model, it allows a <span class="hlt">heat</span> <span class="hlt">flux</span> value to be calculated that corrects for the losses and may be a better estimate of the cold <span class="hlt">wall</span> fully catalytic <span class="hlt">heat</span> <span class="hlt">flux</span>, as is desired in arc jet testing. The model was applied to the data from a copper slug calorimeter inserted during a particularly severe high <span class="hlt">heating</span> rate arc jet run to illustrate its use. The Slug Loss Model gave a cold <span class="hlt">wall</span> <span class="hlt">heat</span> <span class="hlt">flux</span> 15% higher than the value of 2,250 W/sq cm obtained from the conventional approach to processing the data (where no correction is made for losses). For comparison, a Finite Element Analysis (FEA) model was created and applied to the same data, where conduction <span class="hlt">heat</span> losses from the slug were simulated. The <span class="hlt">heat</span> <span class="hlt">flux</span> determined by the FEA model was found to be in close agreement with the <span class="hlt">heat</span> <span class="hlt">flux</span> determined by the Slug Loss Model.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.A53G2359A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.A53G2359A"><span>Multi Seasonal and Diurnal Characterization of Sensible <span class="hlt">Heat</span> <span class="hlt">Flux</span> in an Arid Land Environment</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Al-Mashharawi, S.; Aragon, B.; McCabe, M.</p> <p>2017-12-01</p> <p>In sparsely vegetated arid and semi-arid regions, the available energy is transformed primarily into sensible <span class="hlt">heat</span>, with little to no energy partitioned into latent <span class="hlt">heat</span>. The characterization of bare soil arid environments are rather poorly understood in the context of both local, regional and global energy budgets. Using data from a long-term surface layer scintillometer and co-located meteorological installation, we examine the diurnal and seasonal patterns of sensible <span class="hlt">heat</span> <span class="hlt">flux</span> and the net radiation to soil <span class="hlt">heat</span> <span class="hlt">flux</span> ratio. We do this over a bare desert soil located adjacent to an irrigated agricultural field in the central region of Saudi Arabia. The results of this exploratory analysis can be used to inform upon remote sensing techniques for surface <span class="hlt">flux</span> estimation, to derive and monitor soil <span class="hlt">heat</span> <span class="hlt">flux</span> dynamics, estimate the <span class="hlt">heat</span> transfer resistance and the thermal roughness length over bare soils, and to better inform efforts that model the advective effects that complicate the accurate representation of agricultural energy budgets in the arid zone.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/25045862','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25045862"><span>An evaluation of a zero-<span class="hlt">heat-flux</span> cutaneous thermometer in cardiac surgical patients.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Eshraghi, Yashar; Nasr, Vivian; Parra-Sanchez, Ivan; Van Duren, Albert; Botham, Mark; Santoscoy, Thomas; Sessler, Daniel I</p> <p>2014-09-01</p> <p>Although core temperature can be measured invasively, there are currently no widely available, reliable, noninvasive thermometers for its measurement. We thus compared a prototype zero-<span class="hlt">heat-flux</span> thermometer with simultaneous measurements from a pulmonary artery catheter. Specifically, we tested the hypothesis that zero-<span class="hlt">heat-flux</span> temperatures are sufficiently accurate for routine clinical use. Core temperature was measured from the thermistor of a standard pulmonary artery catheter and with a prototype zero-<span class="hlt">heat-flux</span> deep-tissue thermometer in 105 patients having nonemergent cardiac surgery. Zero-<span class="hlt">heat-flux</span> probes were positioned on the lateral forehead and lateral neck. Skin surface temperature probes were attached to the forehead just adjacent to the zero-<span class="hlt">heat-flux</span> probe. Temperatures were recorded at 1-minute intervals, excluding the period of cardiopulmonary bypass, and for the first 4 postoperative hours. Zero-<span class="hlt">heat-flux</span> and pulmonary artery temperatures were compared with bias analysis; differences exceeding 0.5°C were considered to be potentially clinically important. The mean duration in the operating room was 279 ± 75 minutes, and the mean cross-clamp time was 118 ± 50 minutes. All subjects were monitored for an additional 4 hours in the intensive care unit. The average overall difference between forehead zero-<span class="hlt">heat-flux</span> and pulmonary artery temperatures (i.e., forehead minus pulmonary artery) was -0.23°C (95% limits of agreement of ±0.82); 78% of the differences were ≤0.5°C. The average intraoperative temperature difference was -0.08°C (95% limits of agreement of ±0.88); 84% of the differences were ≤0.5°C. The average postoperative difference was -0.32°C (95% limits of agreement of ±0.75); 84% of the differences were ≤0.5°C. Bias and precision values for neck site were similar to the forehead values. Uncorrected forehead skin temperature showed an increasing negative bias as core temperature decreased. Core temperature can be noninvasively</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010AGUFM.B11D0379L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010AGUFM.B11D0379L"><span>A Semi-parametric Multivariate Gap-filling Model for Eddy Covariance Latent <span class="hlt">Heat</span> <span class="hlt">Flux</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Li, M.; Chen, Y.</p> <p>2010-12-01</p> <p>Quantitative descriptions of latent <span class="hlt">heat</span> <span class="hlt">fluxes</span> are important to study the water and energy exchanges between terrestrial ecosystems and the atmosphere. The eddy covariance approaches have been recognized as the most reliable technique for measuring surface <span class="hlt">fluxes</span> over time scales ranging from hours to years. However, unfavorable micrometeorological conditions, instrument failures, and applicable measurement limitations may cause inevitable <span class="hlt">flux</span> gaps in time series data. Development and application of suitable gap-filling techniques are crucial to estimate long term <span class="hlt">fluxes</span>. In this study, a semi-parametric multivariate gap-filling model was developed to fill latent <span class="hlt">heat</span> <span class="hlt">flux</span> gaps for eddy covariance measurements. Our approach combines the advantages of a multivariate statistical analysis (principal component analysis, PCA) and a nonlinear interpolation technique (K-nearest-neighbors, KNN). The PCA method was first used to resolve the multicollinearity relationships among various hydrometeorological factors, such as radiation, soil moisture deficit, LAI, and wind speed. The KNN method was then applied as a nonlinear interpolation tool to estimate the <span class="hlt">flux</span> gaps as the weighted sum latent <span class="hlt">heat</span> <span class="hlt">fluxes</span> with the K-nearest distances in the PCs’ domain. Two years, 2008 and 2009, of eddy covariance and hydrometeorological data from a subtropical mixed evergreen forest (the Lien-Hua-Chih Site) were collected to calibrate and validate the proposed approach with artificial gaps after standard QC/QA procedures. The optimal K values and weighting factors were determined by the maximum likelihood test. The results of gap-filled latent <span class="hlt">heat</span> <span class="hlt">fluxes</span> conclude that developed model successful preserving energy balances of daily, monthly, and yearly time scales. Annual amounts of evapotranspiration from this study forest were 747 mm and 708 mm for 2008 and 2009, respectively. Nocturnal evapotranspiration was estimated with filled gaps and results are comparable with other studies</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/7377945','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/7377945"><span>Wheelchair cushion effect on skin temperature, <span class="hlt">heat</span> <span class="hlt">flux</span>, and relative humidity.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Stewart, S F; Palmieri, V; Cochran, G V</p> <p>1980-05-01</p> <p>For patients subject to decubitus ulcers, wheelchair cushions should be prescribed with knowledge of the cushion's effect on the thermal as well as mechanical environment of the skin. To define thermal effects that may be encountered during routine use, tests werr made on 24 commercially available cushions. Skin temperature, <span class="hlt">heat</span> <span class="hlt">flux</span> and relative humidity were measured under the ischial tuberosities of a normal 24-year-old man during a 1-hour period of sitting on each cushion. After 1 hour, skin temperatures increased by means of 3.4 C and 2.8 C on foams and viscoelastic foams and there were slight decreases in <span class="hlt">heat</span> <span class="hlt">flux</span> as compared with control values in air. On gels, skin temperatures remained constant and <span class="hlt">heat</span> <span class="hlt">flux</span> increased, while water "floatation" pads caused a mean skin temperature decreased of 2.7 C along with a marked increase in <span class="hlt">heat</span> <span class="hlt">flux</span>. Relative humidity at the skin cushion interface increased by 10.4%, 22.8% and 19.8% on foams, gels and water floatation pads, as compared with room air values. Representative cushions from each of the general types (foam, viscoelastic foam, gel and water floatation) also were subjected to 2-hour tests which indicated the measured parameters continued to change asymptotically.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUOSPO23A..03S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUOSPO23A..03S"><span><span class="hlt">Heat</span> and salt budgets over the Gulf Stream North <span class="hlt">Wall</span> during LatMix survey in winter 2012.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sanchez-Rios, A.; Shearman, R. K.; D'Asaro, E. A.; Lee, C.; Gula, J.; Klymak, J. M.</p> <p>2016-02-01</p> <p>As part of the ONR-sponsored LatMix Experiment, ship-based and glider-based observations following a Lagrangian float are used to examine the evolution of temperature, salinity and density along the Gulf Stream north <span class="hlt">wall</span> in wintertime. Satellite observations during the survey and the in-situ measurements showed the presence of submesoscale (<10 km) features along the front. Models have successfully reproduced similar features, but observations are lacking, particularly at the small scales needed to understand their role in the transport of <span class="hlt">heat</span> and salt across the front and out of the mixed layer. Calculating the trend in time at each depth and cross-front location we found an increase of <span class="hlt">heat</span> and salinity in regions where the strongest cross-front gradients of velocity were observed at the mixed layer and around 150m depth, these changes are density compensated and suggest isopycnal mixing and a connection between the mixed layer and subsurface layers. The large Rossby number (Ro>1) calculated for this regions corroborates the possibility of submesoscale dynamics. Using a <span class="hlt">heat</span> and salinity budget, we show that surface forcing, entrainment from below and advection by the mean flow velocities are not sufficient to explain the observed rate of change of <span class="hlt">heat</span> and salinity in the mixed layer. Although confidence estimates prevent an accurate <span class="hlt">flux</span> divergence calculation, Reynold <span class="hlt">flux</span> estimates are consistent with a cross-frontal exchange that can reproduce the observed temporal trends.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19890001997','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19890001997"><span>Comparison of measured and modeled radiation, <span class="hlt">heat</span> and water vapor <span class="hlt">fluxes</span>: FIFE pilot study</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Blad, Blaine L.; Verma, Shashi B.; Hubbard, Kenneth G.; Starks, Patrick; Hays, Cynthia; Norman, John M.; Waltershea, Elizabeth</p> <p>1988-01-01</p> <p>The primary objectives of the 1985 study were to test the feasibility of using radio frequency receivers to collect data from automated weather stations and to evaluate the use of the data collected by the automated weather stations for modeling the <span class="hlt">fluxes</span> of latent <span class="hlt">heat</span>, sensible <span class="hlt">heat</span>, and radiation over wheat. The model Cupid was used to calculate these <span class="hlt">fluxes</span> which were compared with <span class="hlt">fluxes</span> of these entities measured using micrometeorological techniques. The primary objectives of the 1986 study were to measure and model reflected and emitted radiation streams at a few locations within the First International Satellite Land-Surface Climatology Project Field Experiment (FIFE) site and to compare modeled and measured latent <span class="hlt">heat</span> and sensible <span class="hlt">heat</span> <span class="hlt">fluxes</span> from the prairie vegetation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016APS..DPPYO8001H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016APS..DPPYO8001H"><span>Classical <span class="hlt">Heat-Flux</span> Measurements in Coronal Plasmas from Collective Thomson-Scattering Spectra</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Henchen, R. J.; Hu, S. X.; Katz, J.; Froula, D. H.; Rozmus, W.</p> <p>2016-10-01</p> <p>Collective Thomson scattering was used to measure <span class="hlt">heat</span> <span class="hlt">flux</span> in coronal plasmas. The relative amplitude of the Thomson-scattered power into the up- and downshifted electron plasma wave features was used to determine the <span class="hlt">flux</span> of electrons moving along the temperature gradient at three to four times the electron thermal velocity. Simultaneously, the ion-acoustic wave features were measured. Their relative amplitude was used to measure the <span class="hlt">flux</span> of the return-current electrons. The frequencies of these ion-acoustic and electron plasma wave features provide local measurements of the electron temperature and density. These spectra were obtained at five locations along the temperature gradient in a laser-produced blowoff plasma. These measurements of plasma parameters are used to infer the Spitzer-Härm <span class="hlt">flux</span> (qSH = - κ∇Te ) and are in good agreement with the values of the <span class="hlt">heat</span> <span class="hlt">flux</span> measured from the scattering-feature asymmetries. Additional experiments probed plasma waves perpendicular to the temperature gradient. The data show small effects resulting from <span class="hlt">heat</span> <span class="hlt">flux</span> compared to probing waves along the temperature gradient. This material is based upon work supported by the Department of Energy National Nuclear Security Administration under Award Number DE-NA0001944.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19660000530','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19660000530"><span>Light-intensity modulator withstands high <span class="hlt">heat</span> <span class="hlt">fluxes</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Maples, H. G.; Strass, H. K.</p> <p>1966-01-01</p> <p>Mechanism modulates and controls the intensity of luminous radiation in light beams associated with high-intensity <span class="hlt">heat</span> <span class="hlt">flux</span>. This modulator incorporates two fluid-cooled, externally grooved, contracting metal cylinders which when rotated about their longitudinal axes present a circular aperture of varying size depending on the degree of rotation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20120003896&hterms=max+planck&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3Dmax%2Bplanck','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20120003896&hterms=max+planck&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3Dmax%2Bplanck"><span>Global Intercomparison of 12 Land Surface <span class="hlt">Heat</span> <span class="hlt">Flux</span> Estimates</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Jimenez, C.; Prigent, C.; Mueller, B.; Seneviratne, S. I.; McCabe, M. F.; Wood, E. F.; Rossow, W. B.; Balsamo, G.; Betts, A. K.; Dirmeyer, P. A.; <a style="text-decoration: none; " href="javascript:void(0); " onClick="displayelement('author_20120003896'); toggleEditAbsImage('author_20120003896_show'); toggleEditAbsImage('author_20120003896_hide'); "> <img style="display:inline; width:12px; height:12px; " src="images/arrow-up.gif" width="12" height="12" border="0" alt="hide" id="author_20120003896_show"> <img style="width:12px; height:12px; display:none; " src="images/arrow-down.gif" width="12" height="12" border="0" alt="hide" id="author_20120003896_hide"></p> <p>2011-01-01</p> <p>A global intercomparison of 12 monthly mean land surface <span class="hlt">heat</span> <span class="hlt">flux</span> products for the period 1993-1995 is presented. The intercomparison includes some of the first emerging global satellite-based products (developed at Paris Observatory, Max Planck Institute for Biogeochemistry, University of California Berkeley, University of Maryland, and Princeton University) and examples of <span class="hlt">fluxes</span> produced by reanalyses (ERA-Interim, MERRA, NCEP-DOE) and off-line land surface models (GSWP-2, GLDAS CLM/ Mosaic/Noah). An intercomparison of the global latent <span class="hlt">heat</span> <span class="hlt">flux</span> (Q(sub le)) annual means shows a spread of approx 20 W/sq m (all-product global average of approx 45 W/sq m). A similar spread is observed for the sensible (Q(sub h)) and net radiative (R(sub n)) <span class="hlt">fluxes</span>. In general, the products correlate well with each other, helped by the large seasonal variability and common forcing data for some of the products. Expected spatial distributions related to the major climatic regimes and geographical features are reproduced by all products. Nevertheless, large Q(sub le)and Q(sub h) absolute differences are also observed. The <span class="hlt">fluxes</span> were spatially averaged for 10 vegetation classes. The larger Q(sub le) differences were observed for the rain forest but, when normalized by mean <span class="hlt">fluxes</span>, the differences were comparable to other classes. In general, the correlations between Q(sub le) and R(sub n) were higher for the satellite-based products compared with the reanalyses and off-line models. The <span class="hlt">fluxes</span> were also averaged for 10 selected basins. The seasonality was generally well captured by all products, but large differences in the <span class="hlt">flux</span> partitioning were observed for some products and basins.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20030067911','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20030067911"><span>Investigation of Critical <span class="hlt">Heat</span> <span class="hlt">Flux</span> in Reduced Gravity Using Photomicrographic Techniques</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Mudawar, Issam; Zhang, Hui</p> <p>2003-01-01</p> <p>Experiments were performed to examine the effects of body force on flow boiling critical <span class="hlt">heat</span> <span class="hlt">flux</span> (CHF). FC-72 was boiled along one <span class="hlt">wall</span> of a transparent rectangular flow channel that permitted photographic study of the vapor-liquid interface just prior to CHF. High-speed video imaging techniques were used to identify dominant CHF mechanisms corresponding to different flow orientations and liquid velocities. Six different CHF regimes were identified: Wavy Vapor Layer, Pool Boiling, Stratification, Vapor Counterflow, Vapor Stagnation, and Separated Concurrent Vapor Flow. CHF showed significant sensitivity to orientation for flow velocities below 0.2 m/s, where extremely low CHF values where measured, especially with downward-facing <span class="hlt">heated</span> <span class="hlt">wall</span> and downflow orientations. High flow velocities dampened the effects of orientation considerably. The CHF data were used to assess the suitability of previous CHF models and correlations. It is shown the Interfacial Lift-off Model is very effective at predicting CHF for high velocities at all orientations. The flooding limit, on the other hand, is useful at estimating CHF at low velocities and for downflow orientations. A new method consisting of three dimensionless criteria is developed for determining the minimum flow velocity required to overcome body force effects on near-saturated flow boiling CHF. Vertical upflow boiling experiments were performed in pursuit of identifying the trigger mechanism for subcooled flow boiling CHF. While virtually all prior studies on flow boiling CHF concern the prediction or measurement of conditions that lead to CHF, this study was focused on events that take place during the CHF transient. High-speed video imaging and photomicrographic techniques were used to record the transient behavior of interfacial features from the last steady-state power level before CHF until the moment of power cut-off following CHF. The video records show the development of a wavy vapor layer which propagates</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.H54C..03L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.H54C..03L"><span>Mapping surface <span class="hlt">heat</span> <span class="hlt">fluxes</span> by assimilating GOES land surface temperature and SMAP products</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lu, Y.; Steele-Dunne, S. C.; Van De Giesen, N.</p> <p>2017-12-01</p> <p>Surface <span class="hlt">heat</span> <span class="hlt">fluxes</span> significantly affect the land-atmosphere interaction, but their modelling is often hindered by the lack of in-situ measurements and the high spatial heterogeneity. Here, we propose a hybrid particle assimilation strategy to estimate surface <span class="hlt">heat</span> <span class="hlt">fluxes</span> by assimilating GOES land surface temperature (LST) data and SMAP products into a simple dual-source surface energy balance model, in which the requirement for in-situ data is minimized. The study aims to estimate two key parameters: a neutral bulk <span class="hlt">heat</span> transfer coefficient (CHN) and an evaporative fraction (EF). CHN scales the sum of surface energy <span class="hlt">fluxes</span>, and EF represents the partitioning between <span class="hlt">flux</span> components. To bridge the huge resolution gap between GOES and SMAP data, SMAP data are assimilated using a particle filter to update soil moisture which constrains EF, and GOES data are assimilated with an adaptive particle batch smoother to update CHN. The methodology is applied to an area in the US Southern Great Plains with forcing data from NLDAS-2 and the GPM mission. Assessment against in-situ observations suggests that the sensible and latent <span class="hlt">heat</span> <span class="hlt">flux</span> estimates are greatly improved at both daytime and 30-min scale after assimilation, particularly for latent <span class="hlt">heat</span> <span class="hlt">fluxes</span>. Comparison against an LST-only assimilation case demonstrates that despite the coarse resolution, assimilating SMAP data is not only beneficial but also crucial for successful and robust <span class="hlt">flux</span> estimation, particularly when the modelling uncertainties are large. Since the methodology is independent on in-situ data, it can be easily applied to other areas.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/864118','DOE-PATENT-XML'); return false;" href="https://www.osti.gov/servlets/purl/864118"><span>Method and apparatus for determining vertical <span class="hlt">heat</span> <span class="hlt">flux</span> of geothermal field</span></a></p> <p><a target="_blank" href="http://www.osti.gov/doepatents">DOEpatents</a></p> <p>Poppendiek, Heinz F.</p> <p>1982-01-01</p> <p>A method and apparatus for determining vertical <span class="hlt">heat</span> <span class="hlt">flux</span> of a geothermal field, and mapping the entire field, is based upon an elongated <span class="hlt">heat-flux</span> transducer (10) comprised of a length of tubing (12) of relatively low thermal conductivity with a thermopile (20) inside for measuring the thermal gradient between the ends of the transducer after it has been positioned in a borehole for a period sufficient for the tube to reach thermal equilibrium. The transducer is thermally coupled to the surrounding earth by a fluid annulus, preferably water or mud. A second transducer comprised of a length of tubing of relatively high thermal conductivity is used for a second thermal gradient measurement. The ratio of the first measurement to the second is then used to determine the earth's thermal conductivity, k.sub..infin., from a precalculated graph, and using the value of thermal conductivity thus determined, then determining the vertical earth temperature gradient, b, from predetermined steady state <span class="hlt">heat</span> balance equations which relate the undisturbed vertical earth temperature distributions at some distance from the borehole and earth thermal conductivity to the temperature gradients in the transducers and their thermal conductivity. The product of the earth's thermal conductivity, k.sub..infin., and the earth's undisturbed vertical temperature gradient, b, then determines the earth's vertical <span class="hlt">heat</span> <span class="hlt">flux</span>. The process can be repeated many times for boreholes of a geothermal field to map vertical <span class="hlt">heat</span> <span class="hlt">flux</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUOSHE12A..03H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUOSHE12A..03H"><span>Energy and variance budgets of a diffusive staircase with implications for <span class="hlt">heat</span> <span class="hlt">flux</span> scaling</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hieronymus, M.; Carpenter, J. R.</p> <p>2016-02-01</p> <p>Diffusive convection, the mode of double-diffusive convection that occur when both temperature and salinity increase with increasing depth, is commonplace throughout the high latitude oceans and diffusive staircases constitute an important <span class="hlt">heat</span> transport process in the Arctic Ocean. <span class="hlt">Heat</span> and buoyancy <span class="hlt">fluxes</span> through these staircases are often estimated using <span class="hlt">flux</span> laws deduced either from laboratory experiments, or from simplified energy or variance budgets. We have done direct numerical simulations of double-diffusive convection at a range of Rayleigh numbers and quantified the energy and variance budgets in detail. This allows us to compare the <span class="hlt">fluxes</span> in our simulations to those derived using known <span class="hlt">flux</span> laws and to quantify how well the simplified energy and variance budgets approximate the full budgets. The <span class="hlt">fluxes</span> are found to agree well with earlier estimates at high Rayleigh numbers, but we find large deviations at low Rayleigh numbers. The close ties between the <span class="hlt">heat</span> and buoyancy <span class="hlt">fluxes</span> and the budgets of thermal variance and energy have been utilized to derive <span class="hlt">heat</span> <span class="hlt">flux</span> scaling laws in the field of thermal convection. The result is the so called GL-theory, which has been found to give accurate <span class="hlt">heat</span> <span class="hlt">flux</span> scaling laws in a very wide parameter range. Diffusive convection has many similarities to thermal convection and an extension of the GL-theory to diffusive convection is also presented and its predictions are compared to the results from our numerical simulations.</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('http://adsabs.harvard.edu/abs/2017EPJC...77..251S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EPJC...77..251S"><span>Dynamics of charged bulk viscous collapsing cylindrical source with <span class="hlt">heat</span> <span class="hlt">flux</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Shah, S. M.; Abbas, G.</p> <p>2017-04-01</p> <p>In this paper, we have explored the effects of dissipation on the dynamics of charged bulk viscous collapsing cylindrical source which allows the out-flow of <span class="hlt">heat</span> <span class="hlt">flux</span> in the form of radiations. The Misner-Sharp formalism has been implemented to drive the dynamical equation in terms of proper time and radial derivatives. We have investigated the effects of charge and bulk viscosity on the dynamics of collapsing cylinder. To determine the effects of radial <span class="hlt">heat</span> <span class="hlt">flux</span>, we have formulated the <span class="hlt">heat</span> transport equations in the context of Müller-Israel-Stewart theory by assuming that thermodynamics viscous/<span class="hlt">heat</span> coupling coefficients can be neglected within some approximations. In our discussion, we have introduced the viscosity by the standard (non-causal) thermodynamics approach. The dynamical equations have been coupled with the <span class="hlt">heat</span> transport equation; the consequences of the resulting coupled <span class="hlt">heat</span> equation have been analyzed in detail.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017SPIE10444E..1PN','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017SPIE10444E..1PN"><span>Satellite data based approach for the estimation of anthropogenic <span class="hlt">heat</span> <span class="hlt">flux</span> over urban areas</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Nitis, Theodoros; Tsegas, George; Moussiopoulos, Nicolas; Gounaridis, Dimitrios; Bliziotis, Dimitrios</p> <p>2017-09-01</p> <p>Anthropogenic effects in urban areas influence the thermal conditions in the environment and cause an increase of the atmospheric temperature. The cities are sources of <span class="hlt">heat</span> and pollution, affecting the thermal structure of the atmosphere above them which results to the urban <span class="hlt">heat</span> island effect. In order to analyze the urban <span class="hlt">heat</span> island mechanism, it is important to estimate the anthropogenic <span class="hlt">heat</span> <span class="hlt">flux</span> which has a considerable impact on the urban energy budget. The anthropogenic <span class="hlt">heat</span> <span class="hlt">flux</span> is the result of man-made activities (i.e. traffic, industrial processes, <span class="hlt">heating</span>/cooling) and thermal releases from the human body. Many studies have underlined the importance of the Anthropogenic <span class="hlt">Heat</span> <span class="hlt">Flux</span> to the calculation of the urban energy budget and subsequently, the estimation of mesoscale meteorological fields over urban areas. Therefore, spatially disaggregated anthropogenic <span class="hlt">heat</span> <span class="hlt">flux</span> data, at local and city scales, are of major importance for mesoscale meteorological models. The main objectives of the present work are to improve the quality of such data used as input for mesoscale meteorological models simulations and to enhance the application potential of GIS and remote sensing in the fields of climatology and meteorology. For this reason, the Urban Energy Budget concept is proposed as the foundation for an accurate determination of the anthropogenic <span class="hlt">heat</span> discharge as a residual term in the surface energy balance. The methodology is applied to the cities of Athens and Paris using the Landsat ETM+ remote sensing data. The results will help to improve our knowledge on Anthropogenic <span class="hlt">Heat</span> <span class="hlt">Flux</span>, while the potential for further improvement of the methodology is also discussed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27176779','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27176779"><span>A Comparative Study for Flow of Viscoelastic Fluids with Cattaneo-Christov <span class="hlt">Heat</span> <span class="hlt">Flux</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Hayat, Tasawar; Muhammad, Taseer; Alsaedi, Ahmed; Mustafa, Meraj</p> <p>2016-01-01</p> <p>This article examines the impact of Cattaneo-Christov <span class="hlt">heat</span> <span class="hlt">flux</span> in flows of viscoelastic fluids. Flow is generated by a linear stretching sheet. Influence of thermal relaxation time in the considered <span class="hlt">heat</span> <span class="hlt">flux</span> is seen. Mathematical formulation is presented for the boundary layer approach. Suitable transformations lead to a nonlinear differential system. Convergent series solutions of velocity and temperature are achieved. Impacts of various influential parameters on the velocity and temperature are sketched and discussed. Numerical computations are also performed for the skin friction coefficient and <span class="hlt">heat</span> transfer rate. Our findings reveal that the temperature profile has an inverse relationship with the thermal relaxation parameter and the Prandtl number. Further the temperature profile and thermal boundary layer thickness are lower for Cattaneo-Christov <span class="hlt">heat</span> <span class="hlt">flux</span> model in comparison to the classical Fourier's law of <span class="hlt">heat</span> conduction.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20030062133&hterms=Magnetic+Flux&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3DMagnetic%2BFlux','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20030062133&hterms=Magnetic+Flux&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3DMagnetic%2BFlux"><span>Solar Coronal <span class="hlt">Heating</span> and the Magnetic <span class="hlt">Flux</span> Content of the Network</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Falconer, D. A.; Moore, R. L.; Porter, J. G.; Hathaway, D. H.</p> <p>2003-01-01</p> <p>We investigate the <span class="hlt">heating</span> of the quiet corona by measuring the increase of coronal luminosity with the amount of magnetic <span class="hlt">flux</span> in the underlying network at solar minimum when there were no active regions on the face of the Sun. The coronal luminosity is measured from Fe IX/X-Fe XII pairs of coronal images from SOHO/EIT. The network magnetic <span class="hlt">flux</span> content is measured from SOHO/MDI magnetograms. We find that the luminosity of the corona in our quiet regions increases roughly in proportion to the square root of the magnetic <span class="hlt">flux</span> content of the network and roughly in proportion to the length of the perimeter of the network magnetic <span class="hlt">flux</span> clumps. From (1) this result, (2) other observations of many fine-scale explosive events at the edges of network <span class="hlt">flux</span> clumps, and (3) a demonstration that it is energetically feasible for the <span class="hlt">heating</span> of the corona in quiet regions to be driven by explosions of granule-sized sheared-core magnetic bipoles embedded in the edges of network <span class="hlt">flux</span> clumps, we infer that in quiet regions that are not influenced by active regions the corona is mainly <span class="hlt">heated</span> by such magnetic activity in the edges of the network <span class="hlt">flux</span> clumps. Our observational results together with our feasibility analysis allow us to predict that (1) at the edges of the network <span class="hlt">flux</span> clumps there are many transient sheared-core bipoles of the size and lifetime of granules and having transverse field strengths > approx. 100 G, (2) approx. 30 of these bipoles are present per supergranule, and (3) most spicules are produced by explosions of these bipoles.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20030062034&hterms=Magnetic+Flux&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3DMagnetic%2BFlux','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20030062034&hterms=Magnetic+Flux&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3DMagnetic%2BFlux"><span>Solar Coronal <span class="hlt">Heating</span> and the Magnetic <span class="hlt">Flux</span> Content of the Network</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Moore, R. L.; Falconer, D. A.; Porter, J. G.; Hathaway, D. H.</p> <p>2003-01-01</p> <p>We investigate the <span class="hlt">heating</span> of the quiet corona by measuring the increase of coronal luminosity with the amount of magnetic <span class="hlt">flux</span> in the underlying network at solar minimum when there were no active regions on the face of the Sun. The coronal luminosity is measured from Fe IX/X-Fe XII pairs of coronal images from SOHO/EIT. The network magnetic <span class="hlt">flux</span> content is measured from SOHO/MDI magnetograms. We find that the luminosity of the corona in our quiet regions increases roughly in proportion to the square root of the magnetic <span class="hlt">flux</span> content of the network and roughly in proportion to the length of the perimeter of the network magnetic <span class="hlt">flux</span> clumps. From (1) this result, (2) other observations of many fine-scale explosive events at the edges of network <span class="hlt">flux</span> clumps, and (3) a demonstration that it is energetically feasible for the <span class="hlt">heating</span> of the corona in quiet regions to be driven by explosions of granule-sized sheared-core magnetic bipoles embedded in the edges of network <span class="hlt">flux</span> clumps, we infer that in quiet regions that are not influenced by active regions the corona is mainly <span class="hlt">heated</span> by such magnetic activity in the edges of the network <span class="hlt">flux</span> clumps. Our observational results together with our feasibility analysis allow us to predict that (1) at the edges of the network <span class="hlt">flux</span> clumps there are many transient sheared-core bipoles of the size and lifetime of granules and having transverse field strengths greater than approximately - 100 G, (2) approximately 30 of these bipoles are present per supergranule, and (3) most spicules are produced by explosions of these bipoles.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014EGUGA..16.6056N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014EGUGA..16.6056N"><span>Laboratory experiments of <span class="hlt">heat</span> and moisture <span class="hlt">fluxes</span> through supraglacial debris</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Nicholson, Lindsey; Mayer, Christoph; Wirbel, Anna</p> <p>2014-05-01</p> <p>Inspired by earlier work (Reznichenko et al., 2010), we have carried out experiments within a climate chamber to explore the best ways to measure the <span class="hlt">heat</span> and moisture <span class="hlt">fluxes</span> through supraglacial debris. Sample ice blocks were prepared with debris cover of varying lithology, grain size and thickness and were instrumented with a combination of Gemini TinyTag temperature/relative humidity sensors and Decagon soil moisture sensors in order to monitor the <span class="hlt">heat</span> and moisture <span class="hlt">fluxes</span> through the overlying debris material when the experiment is exposed to specified solar lamp radiation and laminar airflow within the temperature-controlled climate chamber. Experimental results can be used to determine the optimal set up for numerical models of <span class="hlt">heat</span> and moisture <span class="hlt">flux</span> through supraglacial debris and also indicate the performance limitations of such sensors that can be expected in field installations. Reznichenko, N., Davies, T., Shulmeister, J. and McSaveney, M. (2010) Effects of debris on ice-surface melting rates: an experimental study. Journal of Glaciology, Volume 56, Number 197, 384-394.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19870053663&hterms=worlds+oceans&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D90%26Ntt%3Dworlds%2Boceans','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19870053663&hterms=worlds+oceans&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D90%26Ntt%3Dworlds%2Boceans"><span>Mass, <span class="hlt">heat</span> and freshwater <span class="hlt">fluxes</span> in the South Indian Ocean</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Fu, Lee-Lueng</p> <p>1986-01-01</p> <p>Six hydrographic sections were used to examine the circulation and property <span class="hlt">fluxes</span> in the South Indian Ocean from 10 to 32 deg S. The calculations were made by applying an inverse method to the data. In the interior of the South Indian Ocean, the geostrophic flow is generally northward. At 18 deg S, the northward interior mass <span class="hlt">flux</span> is balanced by the southward Ekman mass <span class="hlt">flux</span> at the surface, whereas at 32 deg S the northward interior mass <span class="hlt">flux</span> is balanced by the southward mass <span class="hlt">flux</span> of the Agulhas Current. There is a weak, southward mass <span class="hlt">flux</span> of 6 x 10 to the 9th kg/s in the Mozambique Channel. The rate of water exchange between the Pacific Ocean and the Indian Ocean is dependent on the choice of the initial reference level used in the inverse calculation. The choice of 1500 m, the depth of the deep oxygen minimum, has led to a <span class="hlt">flux</span> of water from the Pacific Ocean to the Indian Ocean at a rate of 6.6 x 10 to the 9th kg/s. <span class="hlt">Heat</span> <span class="hlt">flux</span> calculations indicate that the Indian Ocean is exporting <span class="hlt">heat</span> to the rest of the world's oceans at a rate of -0.69 x 10 to the 15th W at 18 deg S and -0.25 x 10 to the 15th W at 32 deg S (negative values being southward).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017ZNatA..72..151B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017ZNatA..72..151B"><span>Thermotronics: Towards Nanocircuits to Manage Radiative <span class="hlt">Heat</span> <span class="hlt">Flux</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ben-Abdallah, Philippe; Biehs, Svend-Age</p> <p>2017-02-01</p> <p>The control of electric currents in solids is at the origin of the modern electronics revolution that has driven our daily life since the second half of 20th century. Surprisingly, to date, there is no thermal analogue for a control of <span class="hlt">heat</span> <span class="hlt">flux</span>. Here, we summarise the very last developments carried out in this direction to control <span class="hlt">heat</span> exchanges by radiation both in near and far-field in complex architecture networks.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19720018905','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19720018905"><span>Combined buoyancy and flow direction effects on saturated boiling critical <span class="hlt">heat</span> <span class="hlt">flux</span> in liquid nitrogen</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Papell, S. S.</p> <p>1972-01-01</p> <p>Buoyancy effects on the critical <span class="hlt">heat</span> <span class="hlt">flux</span> and general data trends for a liquid nitrogen internal flow system were determined by comparison of upflow and downflow data under identical test conditions. The test section had a 1.28 cm diameter flow passage and a 30.5 cm <span class="hlt">heated</span> length which was subjected to uniform <span class="hlt">heat</span> <span class="hlt">fluxes</span> through resistance <span class="hlt">heating</span>. Test conditions covered a range of pressures from 3.4 to 10.2 atm, inlet velocities from 0.23 to 3.51 m/sec, with the liquid nitrogen temperature at saturated inlet conditions. Data comparisons showed that the critical <span class="hlt">heat</span> <span class="hlt">flux</span> for downflow could be up to 36 percent lower than for upflow. A nonmonotonic relationship between the critical <span class="hlt">heat</span> <span class="hlt">flux</span> and velocity was determined for upflow but not for downflow. A limiting inlet velocity of 4.12 m/sec was determined to be the minimum velocity required to completely suppress the influence of buoyancy on the critical <span class="hlt">heat</span> <span class="hlt">flux</span> for this saturated inlet flow system. A correlation of this limiting fluid velocity is presented that was developed from previously published subcooled liquid nitrogen data and the saturated data of this investigation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19900018410','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19900018410"><span>Apparatus for measuring high-<span class="hlt">flux</span> <span class="hlt">heat</span> transfer in radiatively <span class="hlt">heated</span> compact exchangers</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Olson, Douglas A.</p> <p>1989-01-01</p> <p>An apparatus is described which can deliver uniform <span class="hlt">heat</span> <span class="hlt">flux</span> densities of up to 80 W/sq cm over an area 7.8 cm x 15.2 cm for use in measuring the <span class="hlt">heat</span> transfer and pressure drop in thin (6 mm or less), compact <span class="hlt">heat</span> exchangers. Helium gas at flow rates of 0 to 40 kg/h and pressures to 6.9 MPa (1000 psi) is the working fluid. The instrumentation used in the apparatus and the methods for analyzing the data is described. The apparatus will be used initially to test the performance of prototype cooling jackets for the engine struts of the National Aerospace Plane (NASP).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/23521268','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/23521268"><span>How the propagation of <span class="hlt">heat-flux</span> modulations triggers E × B flow pattern formation.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Kosuga, Y; Diamond, P H; Gürcan, O D</p> <p>2013-03-08</p> <p>We propose a novel mechanism to describe E×B flow pattern formation based upon the dynamics of propagation of <span class="hlt">heat-flux</span> modulations. The E × B flows of interest are staircases, which are quasiregular patterns of strong, localized shear layers and profile corrugations interspersed between regions of avalanching. An analogy of staircase formation to jam formation in traffic flow is used to develop an extended model of <span class="hlt">heat</span> avalanche dynamics. The extension includes a <span class="hlt">flux</span> response time, during which the instantaneous <span class="hlt">heat</span> <span class="hlt">flux</span> relaxes to the mean <span class="hlt">heat</span> <span class="hlt">flux</span>, determined by symmetry constraints. The response time introduced here is the counterpart of the drivers' response time in traffic, during which drivers adjust their speed to match the background traffic flow. The finite response time causes the growth of mesoscale temperature perturbations, which evolve to form profile corrugations. The length scale associated with the maximum growth rate scales as Δ(2) ~ (v(thi)/λT(i))ρ(i)sqrt[χ(neo)τ], where λT(i) is a typical <span class="hlt">heat</span> pulse speed, χ(neo) is the neoclassical thermal diffusivity, and τ is the response time of the <span class="hlt">heat</span> <span class="hlt">flux</span>. The connection between the scale length Δ(2) and the staircase interstep scale is discussed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016amsf.conf..335Y','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016amsf.conf..335Y"><span>Effect of Na2O on Crystallisation Behaviour and <span class="hlt">Heat</span> Transfer of Fluorine-Free Mould <span class="hlt">Fluxes</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Yang, Jian; Zhang, Jianqiang; Sasaki, Yasushi; Ostrovski, Oleg; Zhang, Chen; Cai, Dexiang; Kashiwaya, Yoshiaki</p> <p></p> <p>Most of the commercial mould <span class="hlt">fluxes</span> contain fluorides which bring about serious environmental problems. The major challenge in the application of fluorine-free mould <span class="hlt">fluxes</span> is to control the <span class="hlt">heat</span> transfer from the strand to copper mould which is closely related to crystallisation behaviour. In this study, the effects of Na2O on the crystallisation behaviour and <span class="hlt">heat</span> transfer of CaO-SiO2-Na2O-B2O3-TiO2-Al2O3-MgO-Li2O mould <span class="hlt">fluxes</span> were investigated using single /double hot thermocouple technique (SHTT/DHTT) and infrared emitter technique (IET), respectively. Continuous cooling transformation (CCT) and time-temperature transformation (TTT) diagrams constructed using SHTT showed that the increase of Na2O concentration led to higher critical cooling rate and shorter incubation time. The crystallisation behaviour in a thermal gradient was examined using DHTT. The <span class="hlt">heat</span> <span class="hlt">flux</span> measured by IET showed that the increase of Na2O concentration decreased the <span class="hlt">heat</span> <span class="hlt">flux</span> when Na2O was lower than 9 mass% but the further increase of Na2O raised the <span class="hlt">heat</span> <span class="hlt">flux</span>. The relationship between <span class="hlt">flux</span> crystallisation and <span class="hlt">heat</span> transfer was also discussed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20120003981','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20120003981"><span>Analysis of the Pressure Rise in a Partially Filled Liquid Tank in Microgravity with Low <span class="hlt">Wall</span> <span class="hlt">Heat</span> <span class="hlt">Flux</span> and Simultaneous Boiling and Condensation</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Hasan, Mohammad M.; Balasubramaniam, R.</p> <p>2012-01-01</p> <p>Experiments performed with Freon 113 in the space shuttle have shown that in a pro- cess of very slow <span class="hlt">heating</span>, high liquid superheats can be sustained for a long period in microgravity. In a closed system explosive vaporization of superheated liquid resulted in pressure spikes of varying magnitudes. In this paper, we analyze the pressure rise in a partially lled closed tank in which a large vapor bubble (i.e., ullage) is initially present, and the liquid is subjected to a low <span class="hlt">wall</span> <span class="hlt">heat</span> ux. The liquid layer adjacent to the <span class="hlt">wall</span> becomes superheated until the temperature for nucleation of the bubbles (or the incipience of boiling) is achieved. In the absence of the gravity-induced convection large quantities of superheated liquid can accumulate over time near the <span class="hlt">heated</span> surface. Once the incipience temperature is attained, explosive boiling occurs and the vapor bubbles that are produced on the heater surface tend to quickly raise the tank pressure. The liquid-vapor saturation temperature increases as well. These two e ects tend to induce condensation of the large ullage bubble that is initially present, and tends to mitigate the tank pressure rise. As a result, the tank pressure is predicted to rise sharply, attain a maximum, and subsequently decay slowly. The predicted pressure rise is compared with experimental results obtained in the microgravity environments of the space shuttle for Freon 113. The analysis is appli- cable, in general to <span class="hlt">heating</span> of liquid in closed containers in microgravity and to cryogenic fuel tanks, in particular where small <span class="hlt">heat</span> leaks into the tank are unavoidable.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19890052278&hterms=heat+exchange&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D80%26Ntt%3Dheat%2Bexchange','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19890052278&hterms=heat+exchange&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D80%26Ntt%3Dheat%2Bexchange"><span>A study of oceanic surface <span class="hlt">heat</span> <span class="hlt">fluxes</span> in the Greenland, Norwegian, and Barents Seas</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Hakkinen, Sirpa; Cavalieri, Donald J.</p> <p>1989-01-01</p> <p>This study examines oceanic surface <span class="hlt">heat</span> <span class="hlt">fluxes</span> in the Norwegian, Greenland, and Barents seas using the gridded Navy Fleet Numerical Oceanography Central surface analysis and the First GARP Global Experiment (FGGE) IIc cloudiness data bases. Monthly and annual means of net and turbulent <span class="hlt">heat</span> <span class="hlt">fluxes</span> are computed for the FGGE year 1979. The FGGE IIb data base consisting of individual observations provides particularly good data coverage in this region for a comparison with the gridded Navy winds and air temperatures. The standard errors of estimate between the Navy and FGGE IIb winds and air temperatures are 3.6 m/s and 2.5 C, respectively. The computations for the latent and sensible <span class="hlt">heat</span> <span class="hlt">fluxes</span> are based on bulk formulas with the same constant <span class="hlt">heat</span> exchange coefficient of 0.0015. The results show extremely strong wintertime <span class="hlt">heat</span> <span class="hlt">fluxes</span> in the northern Greenland Sea and especially in the Barents Sea in contrast to previous studies.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70016282','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70016282"><span>Spectral estimates of net radiation and soil <span class="hlt">heat</span> <span class="hlt">flux</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>Daughtry, C.S.T.; Kustas, William P.; Moran, M.S.; Pinter, P. J.; Jackson, R. D.; Brown, P.W.; Nichols, W.D.; Gay, L.W.</p> <p>1990-01-01</p> <p>Conventional methods of measuring surface energy balance are point measurements and represent only a small area. Remote sensing offers a potential means of measuring outgoing <span class="hlt">fluxes</span> over large areas at the spatial resolution of the sensor. The objective of this study was to estimate net radiation (Rn) and soil <span class="hlt">heat</span> <span class="hlt">flux</span> (G) using remotely sensed multispectral data acquired from an aircraft over large agricultural fields. Ground-based instruments measured Rn and G at nine locations along the flight lines. Incoming <span class="hlt">fluxes</span> were also measured by ground-based instruments. Outgoing <span class="hlt">fluxes</span> were estimated using remotely sensed data. Remote Rn, estimated as the algebraic sum of incoming and outgoing <span class="hlt">fluxes</span>, slightly underestimated Rn measured by the ground-based net radiometers. The mean absolute errors for remote Rn minus measured Rn were less than 7%. Remote G, estimated as a function of a spectral vegetation index and remote Rn, slightly overestimated measured G; however, the mean absolute error for remote G was 13%. Some of the differences between measured and remote values of Rn and G are associated with differences in instrument designs and measurement techniques. The root mean square error for available energy (Rn - G) was 12%. Thus, methods using both ground-based and remotely sensed data can provide reliable estimates of the available energy which can be partitioned into sensible and latent <span class="hlt">heat</span> under nonadvective conditions. ?? 1990.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015HMT....51.1747N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015HMT....51.1747N"><span>Simultaneous <span class="hlt">heat</span> and mass transfer inside a vertical channel in evaporating a <span class="hlt">heated</span> falling glycols liquid film</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Nait Alla, Abderrahman; Feddaoui, M'barek; Meftah, Hicham</p> <p>2015-12-01</p> <p>The interactive effects of <span class="hlt">heat</span> and mass transfer in the evaporation of ethylene and propylene glycol flowing as falling films on vertical channel was investigated. The liquid film falls along a left plate which is externally subjected to a uniform <span class="hlt">heat</span> <span class="hlt">flux</span> while the right plate is the dry <span class="hlt">wall</span> and is kept thermally insulated. The model solves the coupled governing equations in both phases together with the boundary and interfacial conditions. The systems of equations obtained by using an implicit finite difference method are solved by Tridiagonal Matrix Algorithm. The influence of the inlet liquid flow, Reynolds number in the gas flow and the <span class="hlt">wall</span> <span class="hlt">heat</span> <span class="hlt">flux</span> on the intensity of <span class="hlt">heat</span> and mass transfers are examined. A comparison between the results obtained for studied glycols and water in the same conditions is made. The results indicate that water evaporates in more intense way in comparison to glycols and the increase of gas flow rate tends to improve slightly the evaporation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19980148003','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19980148003"><span>Design, Construction, and Qualification of a Microscale Heater Array for Use in Boiling <span class="hlt">Heat</span> Transfer</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Rule, T. D.; Kim, J.; Kalkur, T. S.</p> <p>1998-01-01</p> <p>Boiling <span class="hlt">heat</span> transfer is an efficient means of <span class="hlt">heat</span> transfer because a large amount of <span class="hlt">heat</span> can be removed from a surface using a relatively small temperature difference between the surface and the bulk liquid. However, the mechanisms that govern boiling <span class="hlt">heat</span> transfer are not well understood. Measurements of <span class="hlt">wall</span> temperature and <span class="hlt">heat</span> <span class="hlt">flux</span> near the <span class="hlt">wall</span> would add to the database of knowledge which is necessary to understand the mechanisms of nucleate boiling. A heater array has been developed which contains 96 heater elements within a 2.5 mm square area. The temperature of each heater element is held constant by an electronic control system similar to a hot-wire anemometer. The voltage that is being applied to each heater element can be measured and digitized using a high-speed A/D converter, and this digital information can be compiled into a series of <span class="hlt">heat-flux</span> maps. Information for up to 10,000 <span class="hlt">heat</span> <span class="hlt">flux</span> maps can be obtained each second. The heater control system, the A/D system and the heater array construction are described in detail. Results are presented which show that this is an effective method of measuring the local <span class="hlt">heat</span> <span class="hlt">flux</span> during nucleate and transition boiling. <span class="hlt">Heat</span> <span class="hlt">flux</span> maps are obtained for pool boiling in FC-72 on a horizontal surface. Local <span class="hlt">heat</span> <span class="hlt">flux</span> variations are shown to be three to six times larger than variations in the spatially averaged <span class="hlt">heat</span> <span class="hlt">flux</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19740003624','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19740003624"><span>Effect of gage size on the measurement of local <span class="hlt">heat</span> <span class="hlt">flux</span>. [formulas for determining gage averaging errors</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Baumeister, K. J.; Papell, S. S.</p> <p>1973-01-01</p> <p>General formulas are derived for determining gage averaging errors of strip-type <span class="hlt">heat</span> <span class="hlt">flux</span> meters used in the measurement of one-dimensional <span class="hlt">heat</span> <span class="hlt">flux</span> distributions. In addition, a correction procedure is presented which allows a better estimate for the true value of the local <span class="hlt">heat</span> <span class="hlt">flux</span>. As an example of the technique, the formulas are applied to the cases of <span class="hlt">heat</span> transfer to air slot jets impinging on flat and concave surfaces. It is shown that for many practical problems, the use of very small <span class="hlt">heat</span> <span class="hlt">flux</span> gages is often unnecessary.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011A%26A...531A.162K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011A%26A...531A.162K"><span>Reynolds stress and <span class="hlt">heat</span> <span class="hlt">flux</span> in spherical shell convection</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Käpylä, P. J.; Mantere, M. J.; Guerrero, G.; Brandenburg, A.; Chatterjee, P.</p> <p>2011-07-01</p> <p>Context. Turbulent <span class="hlt">fluxes</span> of angular momentum and enthalpy or <span class="hlt">heat</span> due to rotationally affected convection play a key role in determining differential rotation of stars. Their dependence on latitude and depth has been determined in the past from convection simulations in Cartesian or spherical simulations. Here we perform a systematic comparison between the two geometries as a function of the rotation rate. Aims: Here we want to extend the earlier studies by using spherical wedges to obtain turbulent angular momentum and <span class="hlt">heat</span> transport as functions of the rotation rate from stratified convection. We compare results from spherical and Cartesian models in the same parameter regime in order to study whether restricted geometry introduces artefacts into the results. In particular, we want to clarify whether the sharp equatorial profile of the horizontal Reynolds stress found in earlier Cartesian models is also reproduced in spherical geometry. Methods: We employ direct numerical simulations of turbulent convection in spherical and Cartesian geometries. In order to alleviate the computational cost in the spherical runs, and to reach as high spatial resolution as possible, we model only parts of the latitude and longitude. The rotational influence, measured by the Coriolis number or inverse Rossby number, is varied from zero to roughly seven, which is the regime that is likely to be realised in the solar convection zone. Cartesian simulations are performed in overlapping parameter regimes. Results: For slow rotation we find that the radial and latitudinal turbulent angular momentum <span class="hlt">fluxes</span> are directed inward and equatorward, respectively. In the rapid rotation regime the radial <span class="hlt">flux</span> changes sign in accordance with earlier numerical results, but in contradiction with theory. The latitudinal <span class="hlt">flux</span> remains mostly equatorward and develops a maximum close to the equator. In Cartesian simulations this peak can be explained by the strong "banana cells". Their effect in the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19940023156','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19940023156"><span>Numerical and experimental analyses of the radiant <span class="hlt">heat</span> <span class="hlt">flux</span> produced by quartz <span class="hlt">heating</span> systems</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Turner, Travis L.; Ash, Robert L.</p> <p>1994-01-01</p> <p>A method is developed for predicting the radiant <span class="hlt">heat</span> <span class="hlt">flux</span> distribution produced by tungsten filament, tubular fused-quartz envelope <span class="hlt">heating</span> systems with reflectors. The method is an application of Monte Carlo simulation, which takes the form of a random walk or ray tracing scheme. The method is applied to four systems of increasing complexity, including a single lamp without a reflector, a single lamp with a Hat reflector, a single lamp with a parabolic reflector, and up to six lamps in a six-lamp contoured-reflector <span class="hlt">heating</span> unit. The application of the Monte Carlo method to the simulation of the thermal radiation generated by these systems is discussed. The procedures for numerical implementation are also presented. Experiments were conducted to study these quartz <span class="hlt">heating</span> systems and to acquire measurements of the corresponding empirical <span class="hlt">heat</span> <span class="hlt">flux</span> distributions for correlation with analysis. The experiments were conducted such that several complicating factors could be isolated and studied sequentially. Comparisons of the experimental results with analysis are presented and discussed. Good agreement between the experimental and simulated results was obtained in all cases. This study shows that this method can be used to analyze very complicated quartz <span class="hlt">heating</span> systems and can account for factors such as spectral properties, specular reflection from curved surfaces, source enhancement due to reflectors and/or adjacent sources, and interaction with a participating medium in a straightforward manner.</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/2017PhyE...85..271F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017PhyE...85..271F"><span>Different nano-particles volume fraction and Hartmann number effects on flow and <span class="hlt">heat</span> transfer of water-silver nanofluid under the variable <span class="hlt">heat</span> <span class="hlt">flux</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Forghani-Tehrani, Pezhman; Karimipour, Arash; Afrand, Masoud; Mousavi, Sayedali</p> <p>2017-01-01</p> <p>Nanofluid flow and <span class="hlt">heat</span> transfer composed of water-silver nanoparticles is investigated numerically inside a microchannel. Finite volume approach (FVM) is applied and the effects of gravity are ignored. The whole length of Microchannel is considered in three sections as l1=l3=0.151 and l2=0.71. The linear variable <span class="hlt">heat</span> <span class="hlt">flux</span> affects the microchannel <span class="hlt">wall</span> in the length of l2 while a magnetic field with strength of B0 is considered over the whole domain of it. The influences of different values of Hartmann number (Ha=0, 10, 20), volume fraction of the nanoparticles (ɸ=0, 0.02, 0.04) and Reynolds number (Re=10, 50, 200) on the hydrodynamic and thermal properties of flow are reported. The investigation of slip velocity variations under the effects of a magnetic field are presented for the first time (to the best knowledge of author) while the non-dimensional slip coefficient are selected as B=0.01, 0.05, 0.1 at different states.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19890056315&hterms=dropout&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Ddropout','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19890056315&hterms=dropout&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Ddropout"><span>Electron <span class="hlt">heat</span> <span class="hlt">flux</span> dropouts in the solar wind - Evidence for interplanetary magnetic field reconnection?</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Mccomas, D. J.; Gosling, J. T.; Phillips, J. L.; Bame, S. J.; Luhmann, J. G.; Smith, E. J.</p> <p>1989-01-01</p> <p>An examination of ISEE-3 data from 1978 reveal 25 electron <span class="hlt">heat</span> <span class="hlt">flux</span> dropout events ranging in duration from 20 min to over 11 hours. The <span class="hlt">heat</span> <span class="hlt">flux</span> dropouts are found to occur in association with high plasma densities, low plasma velocities, low ion and electron temperatures, and low magnetic field magnitudes. It is suggested that the <span class="hlt">heat</span> <span class="hlt">flux</span> dropout intervals may indicate that the spacecraft is sampling plasma regimes which are magnetically disconnected from the sun and instead are connected to the outer heliosphere at both ends.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014NucFu..54l3004W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014NucFu..54l3004W"><span>Experimental and numerical investigation of HyperVapotron <span class="hlt">heat</span> transfer</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wang, Weihua; Deng, Haifei; Huang, Shenghong; Chu, Delin; Yang, Bin; Mei, Luoqin; Pan, Baoguo</p> <p>2014-12-01</p> <p>The divertor first <span class="hlt">wall</span> and neutral beam injection (NBI) components of tokamak devices require high <span class="hlt">heat</span> <span class="hlt">flux</span> removal up to 20-30 MW m-2 for future fusion reactors. The water cooled HyperVapotron (HV) structure, which relies on internal grooves or fins and boiling <span class="hlt">heat</span> transfer to maximize the <span class="hlt">heat</span> transfer capability, is the most promising candidate. The HV devices, that are able to transfer large amounts of <span class="hlt">heat</span> (1-20 MW m-2) efficiently, have therefore been developed specifically for this application. Until recently, there have been few attempts to observe the detailed bubble characteristics and vortex evolvement of coolant flowing inside their various parts and understand of the internal two-phase complex <span class="hlt">heat</span> transfer mechanism behind the vapotron effect. This research builds the experimental facilities of HyperVapotron Loop-I (HVL-I) and Pressure Water HyperVapotron Loop-II (PWHL-II) to implement the subcooled boiling principle experiment in terms of typical flow parameters, geometrical parameters of test section and surface <span class="hlt">heat</span> <span class="hlt">flux</span>, which are similar to those of the ITER-like first <span class="hlt">wall</span> and NBI components (EAST and MAST). The multiphase flow and <span class="hlt">heat</span> transfer phenomena on the surface of grooves and triangular fins when the subcooled water flowed through were observed and measured with the planar laser induced fluorescence (PLIF) and high-speed photography (HSP) techniques. Particle image velocimetry (PIV) was selected to reveal vortex formation, the flow structure that promotes the vapotron effect during subcooled boiling. The coolant flow data for contributing to the understanding of the vapotron phenomenon and the assessment of how the design and operational conditions that might affect the thermal performance of the devices were collected and analysed. The subcooled flow boiling model and methods of HV <span class="hlt">heat</span> transfer adopted in the considered computational fluid dynamics (CFD) code were evaluated by comparing the calculated <span class="hlt">wall</span> temperatures with the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMGP41A0954M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMGP41A0954M"><span>New geothermal <span class="hlt">heat</span> <span class="hlt">flux</span> map of Greenland and the Iceland hotspot track</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Martos, Y. M.; Jordan, T. A.; Catalan, M.; Jordan, T. M.; Bamber, J. L.; Vaughan, D. G.</p> <p>2017-12-01</p> <p>Greenland is the second largest reservoir of water on Earth and about 80% of its surface is covered by ice. It is mainly composed of Archean blocks that collided during the Early Proterozoic. Indirect methods have been used to study its subglacial thermal conditions, geology and lithospheric structure. Numerous regions of basal melting are identified in the central and north Greenland but their relationship with geothermal <span class="hlt">heat</span> <span class="hlt">flux</span> is not yet clear. Crustal thickness derived by seismology and gravity data are consistent, showing no significant lateral variations, and providing average values of about 40 and 36 km respectively. Even though Greenland is considered a craton its crust has been affected by the presume passage of the Iceland hotspot since at least 100 Ma. Here we present the newest and highest resolution Curie Depth and geothermal <span class="hlt">heat</span> <span class="hlt">flux</span> maps for Greenland as well as their associated uncertainties. For estimating the Curie Depths we applied spectral methods to aeromagnetic data from the World Digital Magnetic Anomaly Map WDMAM2.0. Calculated Curie Depths vary from 25 to 50 km with shallower values located to the east. A thermal model is built based on the 1D <span class="hlt">heat</span> conduction equation and considering steady state conditions. The thermal parameters are then optimized using local values derived from direct measurements, temperature profiles and more indirect methods such as radar imaging. The <span class="hlt">heat</span> <span class="hlt">flux</span> distribution shows higher spatial variability and a very different pattern than previously proposed and with values of 50-80 mW/m2. We identify a NW-SE high <span class="hlt">heat</span> <span class="hlt">flux</span> feature crossing Greenland which we correlate with the Iceland hotspot track. Additionally, to evaluate the lithospheric structure we calculate the Bouguer anomaly from GOCO5s satellite free air data and construct several gravity models across the proposed hotspot track. We show that a dense lower crust body in the same location the high <span class="hlt">heat</span> <span class="hlt">flux</span> trend is permissible from a gravimetric</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/872555','DOE-PATENT-XML'); return false;" href="https://www.osti.gov/servlets/purl/872555"><span>Method of fission <span class="hlt">heat</span> <span class="hlt">flux</span> determination from experimental data</span></a></p> <p><a target="_blank" href="http://www.osti.gov/doepatents">DOEpatents</a></p> <p>Paxton, Frank A.</p> <p>1999-01-01</p> <p>A method is provided for determining the fission <span class="hlt">heat</span> <span class="hlt">flux</span> of a prime specimen inserted into a specimen of a test reactor. A pair of thermocouple test specimens are positioned at the same level in the holder and a determination is made of various experimental data including the temperature of the thermocouple test specimens, the temperature of bulk water channels located in the test holder, the gamma scan count ratios for the thermocouple test specimens and the prime specimen, and the thicknesses of the outer clads, the fuel fillers, and the backclad of the thermocouple test specimen. Using this experimental data, the absolute value of the fission <span class="hlt">heat</span> <span class="hlt">flux</span> for the thermocouple test specimens and prime specimen can be calculated.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/8885256','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/8885256"><span>The role of <span class="hlt">heat</span> shock proteins in protection and pathophysiology of the arterial <span class="hlt">wall</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Xu, Q; Wick, G</p> <p>1996-09-01</p> <p>The arterial <span class="hlt">wall</span> is an integrated functional component of the circulatory system that is continually remodelling in response to various stressors, including localized injury, toxins, smoking and hypercholesterolaemia. These stimuli directly or indirectly cause changes in blood pressure and damage to the vessel <span class="hlt">wall</span>, and eventually induce arterial stiffness and obstruction. To maintain the homeostasis of the vessel <span class="hlt">wall</span>, the vascular cells produce a high level of stress proteins, also known as <span class="hlt">heat</span> shock proteins, which protect against damage during haemodynamic stress. However, an immune reaction to <span class="hlt">heat</span> shock proteins might contribute to the development of atherosclerosis. We hypothesize that the induction of <span class="hlt">heat</span> shock proteins is beneficial in the arterial <span class="hlt">wall</span>'s response to stress but is harmful in certain other circumstances.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19840016704','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19840016704"><span>Performance of thermal barrier coatings in high <span class="hlt">heat</span> <span class="hlt">flux</span> environments</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Miller, R. A.; Berndt, C. C.</p> <p>1984-01-01</p> <p>Thermal barrier coatings were exposed to the high temperature and high <span class="hlt">heat</span> <span class="hlt">flux</span> produced by a 30 kW plasma torch. Analysis of the specimen <span class="hlt">heating</span> rates indicates that the temperature drop across the thickness of the 0.038 cm ceramic layer was about 1100 C after 0.5 sec in the flame. An as-sprayed ZrO2-8%Y2O3 specimens survived 3000 of the 0.5 sec cycles with failing. Surface spalling was observed when 2.5 sec cycles were employed but this was attributed to uneven <span class="hlt">heating</span> caused by surface roughness. This surface spalling was prevented by smoothing the surface with silicon carbide paper or by laser glazing. A coated specimen with no surface modification but which was <span class="hlt">heat</span> treated in argon also did not surface spall. <span class="hlt">Heat</span> treatment in air led to spalling in as early as 2 cycle from <span class="hlt">heating</span> stresses. Failures at edges were investigated and shown to be a minor source of concern. Ceramic coatings formed from ZrO2-12%Y2O3 or ZrO2-20%Y2O3 were shown to be unsuited for use under the high <span class="hlt">heat</span> <span class="hlt">flux</span> conditions of this study.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/24360191','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/24360191"><span>Assessment of land surface temperature and <span class="hlt">heat</span> <span class="hlt">fluxes</span> over Delhi using remote sensing data.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Chakraborty, Surya Deb; Kant, Yogesh; Mitra, Debashis</p> <p>2015-01-15</p> <p>Surface energy processes has an essential role in urban weather, climate and hydrosphere cycles, as well in urban <span class="hlt">heat</span> redistribution. The research was undertaken to analyze the potential of Landsat and MODIS data in retrieving biophysical parameters in estimating land surface temperature & <span class="hlt">heat</span> <span class="hlt">fluxes</span> diurnally in summer and winter seasons of years 2000 and 2010 and understanding its effect on anthropogenic <span class="hlt">heat</span> disturbance over Delhi and surrounding region. Results show that during years 2000-2010, settlement and industrial area increased from 5.66 to 11.74% and 4.92 to 11.87% respectively which in turn has direct effect on land surface temperature (LST) and <span class="hlt">heat</span> <span class="hlt">fluxes</span> including anthropogenic <span class="hlt">heat</span> <span class="hlt">flux</span>. Based on the energy balance model for land surface, a method to estimate the increase in anthropogenic <span class="hlt">heat</span> <span class="hlt">flux</span> (Has) has been proposed. The settlement and industrial areas has higher amounts of energy consumed and has high values of Has in all seasons. The comparison of satellite derived LST with that of field measured values show that Landsat estimated values are in close agreement within error of ±2 °C than MODIS with an error of ±3 °C. It was observed that, during 2000 and 2010, the average change in surface temperature using Landsat over settlement & industrial areas of both seasons is 1.4 °C & for MODIS data is 3.7 °C. The seasonal average change in anthropogenic <span class="hlt">heat</span> <span class="hlt">flux</span> (Has) estimated using Landsat & MODIS is up by around 38 W/m(2) and 62 W/m(2) respectively while higher change is observed over settlement and concrete structures. The study reveals that the dynamic range of Has values has increased in the 10 year period due to the strong anthropogenic influence over the area. The study showed that anthropogenic <span class="hlt">heat</span> <span class="hlt">flux</span> is an indicator of the strength of urban <span class="hlt">heat</span> island effect, and can be used to quantify the magnitude of the urban <span class="hlt">heat</span> island effect. Copyright © 2013 Elsevier Ltd. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009DPS....41.1409P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009DPS....41.1409P"><span>Solar <span class="hlt">Flux</span> Deposition And <span class="hlt">Heating</span> Rates In Jupiter's Atmosphere</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Perez-Hoyos, Santiago; Sánchez-Lavega, A.</p> <p>2009-09-01</p> <p>We discuss here the solar downward net <span class="hlt">flux</span> in the 0.25 - 2.5 µm range in the atmosphere of Jupiter and the associated <span class="hlt">heating</span> rates under a number of vertical cloud structure scenarios focusing in the effect of clouds and hazes. Our numerical model is based in the doubling-adding technique to solve the radiative transfer equation and it includes gas absorption by CH4, NH3 and H2, in addition to Rayleigh scattering by a mixture of H2 plus He. Four paradigmatic Jovian regions have been considered (hot-spots, belts, zones and Polar Regions). The hot-spots are the most transparent regions with downward net <span class="hlt">fluxes</span> of 2.5±0.5 Wm-2 at the 6 bar level. The maximum solar <span class="hlt">heating</span> is 0.04±0.01 K/day and occurs above 1 bar. Belts and zones characterization result in a maximum net downward <span class="hlt">flux</span> of 0.5 Wm-2 at 2 bar and 0.015 Wm-2 at 6 bar. <span class="hlt">Heating</span> is concentrated in the stratospheric and tropospheric hazes. Finally, Polar Regions are also explored and the results point to a considerable stratospheric <span class="hlt">heating</span> of 0.04±0.02 K/day. In all, these calculations suggest that the role of the direct solar forcing in the Jovian atmospheric dynamics is limited to the upper 1 - 2 bar of the atmosphere except in the hot-spot areas. Acknowledgments: This work has been funded by Spanish MEC AYA2006-07735 with FEDER support and Grupos Gobierno Vasco IT-464-07.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018GeoJI.214..265V','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018GeoJI.214..265V"><span>Temperature and <span class="hlt">heat</span> <span class="hlt">flux</span> scaling laws for isoviscous, infinite Prandtl number mixed <span class="hlt">heating</span> convection</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Vilella, Kenny; Deschamps, Frédéric</p> <p>2018-07-01</p> <p>Thermal evolution of terrestrial planets is controlled by <span class="hlt">heat</span> transfer through their silicate mantles. A suitable framework for modelling this <span class="hlt">heat</span> transport is a system including bottom <span class="hlt">heating</span> (from the core) and internal <span class="hlt">heating</span>, for example, generated by secular cooling or by the decay of radioactive isotopes. The mechanism of <span class="hlt">heat</span> transfer depends on the physical properties of the system. In systems where convection is able to operate, two different regimes are possible depending on the relative amount of bottom and internal <span class="hlt">heating</span>. For moderate internal <span class="hlt">heating</span> rates, the system is composed of active hot upwellings and cold downwellings. For large internal <span class="hlt">heating</span> rates, the bottom <span class="hlt">heat</span> <span class="hlt">flux</span> becomes negative and the system is only composed of active cold downwellings. Here, we build theoretical scaling laws for both convective regimes following the approach of Vilella & Kaminski (2017), which links the surface <span class="hlt">heat</span> <span class="hlt">flux</span> and the temperature jump across both the top and the bottom thermal boundary layer (TBL) to the Rayleigh number and the dimensionless internal <span class="hlt">heating</span> rate. Theoretical predictions are then verified against numerical simulations performed in 2-D and 3-D Cartesiangeometry, and covering a large range of the parameter space. Our theoretical scaling laws are more successful in predicting the thermal structure of systems with large internal <span class="hlt">heating</span> rates than that of systems with no or moderate internal <span class="hlt">heating</span>. The differences between moderate and large internal <span class="hlt">heating</span> rates are interpreted as differences in the mechanisms generating thermal instabilities. We identified three mechanisms: conductive growth of the TBL, instability impacting, and TBL erosion, the last two being present only for moderate internal <span class="hlt">heating</span> rates, in which hot plumes are generated at the bottom of the system and are able to reach the surface. Finally, we apply our scaling laws to the evolution of the early Earth, proposing a new model for the cooling of the primordial</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018GeoJI.tmp..134V','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018GeoJI.tmp..134V"><span>Temperature and <span class="hlt">heat</span> <span class="hlt">flux</span> scaling laws for isoviscous, infinite Prandtl number mixed <span class="hlt">heating</span> convection.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Vilella, Kenny; Deschamps, Frederic</p> <p>2018-04-01</p> <p>Thermal evolution of terrestrial planets is controlled by <span class="hlt">heat</span> transfer through their silicate mantles. A suitable framework for modelling this <span class="hlt">heat</span> transport is a system including bottom <span class="hlt">heating</span> (from the core) and internal <span class="hlt">heating</span>, e.g., generated by secular cooling or by the decay of radioactive isotopes. The mechanism of <span class="hlt">heat</span> transfer depends on the physical properties of the system. In systems where convection is able to operate, two different regimes are possible depending on the relative amount of bottom and internal <span class="hlt">heating</span>. For moderate internal <span class="hlt">heating</span> rates, the system is composed of active hot upwellings and cold downwellings. For large internal <span class="hlt">heating</span> rates, the bottom <span class="hlt">heat</span> <span class="hlt">flux</span> becomes negative and the system is only composed of active cold downwellings. Here, we build theoretical scaling laws for both convective regimes following the approach of Vilella & Kaminski (2017), which links the surface <span class="hlt">heat</span> <span class="hlt">flux</span> and the temperature jump across both the top and bottom thermal boundary layer (TBL) to the Rayleigh number and the dimensionless internal <span class="hlt">heating</span> rate. Theoretical predictions are then verified against numerical simulations performed in 2D and 3D-Cartesian geometry, and covering a large range of the parameter space. Our theoretical scaling laws are more successful in predicting the thermal structure of systems with large internal <span class="hlt">heating</span> rates than that of systems with no or moderate internal <span class="hlt">heating</span>. The differences between moderate and large internal <span class="hlt">heating</span> rates are interpreted as differences in the mechanisms generating thermal instabilities. We identified three mechanisms: conductive growth of the TBL, instability impacting, and TBL erosion, the last two being present only for moderate internal <span class="hlt">heating</span> rates, in which hot plumes are generated at the bottom of the system and are able to reach the surface. Finally, we apply our scaling laws to the evolution of the early Earth, proposing a new model for the cooling of the primordial magma ocean</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..18.3373A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..18.3373A"><span>Estimating sensible <span class="hlt">heat</span> <span class="hlt">flux</span> in agricultural screenhouses by the <span class="hlt">flux</span>-variance and half-order time derivative methods</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Achiman, Ori; Mekhmandarov, Yonatan; Pirkner, Moran; Tanny, Josef</p> <p>2016-04-01</p> <p>Previous studies have established that the eddy covariance (EC) technique is reliable for whole canopy <span class="hlt">flux</span> measurements in agricultural crops covered by porous screens, i.e., screenhouses. Nevertheless, the eddy covariance technique remains difficult to apply in the farm due to costs, operational complexity, and post-processing of data - thereby inviting alternative techniques to be developed. The subject of this research was estimating the sensible <span class="hlt">heat</span> <span class="hlt">flux</span> by two turbulent transport techniques, namely, <span class="hlt">Flux</span>-Variance (FV) and Half-order Time Derivative (HTD) whose instrumentation needs and operational demands are not as elaborate as the EC. The FV is based on the standard deviation of high frequency temperature measurements and a similarity constant CT. The HTD method requires mean air temperature and air velocity data. Measurements were carried out in two types of screenhouses: (i) a banana plantation in a light shading (8%) screenhouse; (ii) a pepper crop in a dense insect-proof (50-mesh) screenhouse. In each screenhouse an EC system was deployed for reference and high frequency air temperature measurements were conducted using miniature thermocouples installed at several levels to identify the optimal measurement height. Quality control analysis showed that turbulence development and flow stationarity conditions in the two structures were suitable for <span class="hlt">flux</span> measurements by the EC technique. Energy balance closure slopes in the two screenhouses were larger than 0.71, in agreement with results for open fields. Regressions between sensible <span class="hlt">heat</span> <span class="hlt">flux</span> measured by EC and estimated by FV resulted with CT values that were usually larger than 1, the typical value for open field. In both shading and insect-proof screenhouses the CT value generally increased with height. The optimal measurement height, defined as the height with maximum R2 of the regression between EC and FV sensible <span class="hlt">heat</span> <span class="hlt">fluxes</span>, was just above the screen. CT value at optimal height was 2.64 and 1.52 for</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016JGRC..121.8419K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016JGRC..121.8419K"><span>Reconciling estimates of the ratio of <span class="hlt">heat</span> and salt <span class="hlt">fluxes</span> at the ice-ocean interface</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Keitzl, T.; Mellado, J. P.; Notz, D.</p> <p>2016-12-01</p> <p>The <span class="hlt">heat</span> exchange between floating ice and the underlying ocean is determined by the interplay of diffusive <span class="hlt">fluxes</span> directly at the ice-ocean interface and turbulent <span class="hlt">fluxes</span> away from it. In this study, we examine this interplay through direct numerical simulations of free convection. Our results show that an estimation of the interface <span class="hlt">flux</span> ratio based on direct measurements of the turbulent <span class="hlt">fluxes</span> can be difficult because the <span class="hlt">flux</span> ratio varies with depth. As an alternative, we present a consistent evaluation of the <span class="hlt">flux</span> ratio based on the total <span class="hlt">heat</span> and salt <span class="hlt">fluxes</span> across the boundary layer. This approach allows us to reconcile previous estimates of the ice-ocean interface conditions. We find that the ratio of <span class="hlt">heat</span> and salt <span class="hlt">fluxes</span> directly at the interface is 83-100 rather than 33 as determined by previous turbulence measurements in the outer layer. This can cause errors in the estimated ice-ablation rate from field measurements of up to 40% if they are based on the three-equation formulation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19950065587&hterms=burning+plasma&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3Dburning%2Bplasma','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19950065587&hterms=burning+plasma&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3Dburning%2Bplasma"><span>Measuring <span class="hlt">Fluxes</span> Of <span class="hlt">Heat</span> To A Plasma-Arc Anode</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Sankovic, John M.; Menart, James A.; Pfender, Emil; Heberlein, Joachim</p> <p>1995-01-01</p> <p>Three probes constructed to provide measurements indicative of conductive, convective, and radiative transfer of <span class="hlt">heat</span> from free-burning plasma arc to water-cooled copper anode used in generating arc. Each probe consists mainly of copper body with two thermocouples embedded at locations 4 mm apart along length. Thermocouples provide measure of rate of conduction of <span class="hlt">heat</span> along probe and transfers of <span class="hlt">heat</span> from plasma to sensing surface at tip of probe. Probes identical except sensing surface of one uncoated and other two coated with different materials to make them sensitive to different components of overall <span class="hlt">flux</span> of <span class="hlt">heat</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19850007787','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19850007787"><span>High temperature thermocouple and <span class="hlt">heat</span> <span class="hlt">flux</span> gauge using a unique thin film-hardware hot juncture</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Liebert, C. H.; Holanda, R.; Hippensteele, S. A.; Andracchio, C. A.</p> <p>1984-01-01</p> <p>A special thin film-hardware material thermocouple (TC) and <span class="hlt">heat</span> <span class="hlt">flux</span> gauge concept for a reasonably high temperature and high <span class="hlt">flux</span> flat plate <span class="hlt">heat</span> transfer experiment was fabricated and tested to gauge temperatures of 911 K. This concept was developed for minimal disturbance of boundary layer temperature and flow over the plates and minimal disturbance of <span class="hlt">heat</span> <span class="hlt">flux</span> through the plates. Comparison of special <span class="hlt">heat</span> <span class="hlt">flux</span> gauge Stanton number output at steady-state conditions with benchmark literature data was good and agreement was within a calculated uncertainty of the measurement system. Also, good agreement of special TC and standard TC outputs was obtained and the results are encouraging. Oxidation of thin film thermoelements was a primary failure mode after about 5 of operation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19860028321&hterms=911&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D80%26Ntt%3D911','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19860028321&hterms=911&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D80%26Ntt%3D911"><span>High-temperature thermocouple and <span class="hlt">heat</span> <span class="hlt">flux</span> gauge using a unique thin film-hardware hot junction</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Liebert, C. H.; Holanda, R.; Hippensteele, S. A.; Andracchio, C. A.</p> <p>1985-01-01</p> <p>A special thin film-hardware material thermocouple (TC) and <span class="hlt">heat</span> <span class="hlt">flux</span> gauge concept for a reasonably high temperature and high <span class="hlt">flux</span> flat plate <span class="hlt">heat</span> transfer experiment was fabricated and tested to gauge temperatures of 911 K. This concept was developed for minimal disturbance of boundary layer temperature and flow over the plates and minimal disturbance of <span class="hlt">heat</span> <span class="hlt">flux</span> through the plates. Comparison of special <span class="hlt">heat</span> <span class="hlt">flux</span> gauge Stanton number output at steady-state conditions with benchmark literature data was good and agreement was within a calculated uncertainty of the measurement system. Also, good agreement of special TC and standard TC outputs was obtained and the results are encouraging. Oxidation of thin film thermoelements was a primary failure mode after about 5 of operation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/111422','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/111422"><span>General correlation for prediction of critical <span class="hlt">heat</span> <span class="hlt">flux</span> ratio in water cooled channels</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>Pernica, R.; Cizek, J.</p> <p>1995-09-01</p> <p>The paper present the general empirical Critical <span class="hlt">Heat</span> <span class="hlt">Flux</span> Ration (CHFR) correlation which is valid for vertical water upflow through tubes, internally <span class="hlt">heated</span> concentric annuli and rod bundles geometries with both wide and very tight square and triangular rods lattices. The proposed general PG correlation directly predicts the CHFR, it comprises axial and radial non-uniform <span class="hlt">heating</span>, and is valid in a wider range of thermal hydraulic conditions than previously published critical <span class="hlt">heat</span> <span class="hlt">flux</span> correlations. The PG correlation has been developed using the critical <span class="hlt">heat</span> <span class="hlt">flux</span> Czech data bank which includes more than 9500 experimental data on tubes, 7600 data onmore » rod bundles and 713 data on internally <span class="hlt">heated</span> concentric annuli. Accuracy of the CHFR prediction, statistically assessed by the constant dryout conditions approach, is characterized by the mean value nearing 1.00 and the standard deviation less than 0.06. Moverover, a subchannel form of the PG correlations is statistically verified on Westinghouse and Combustion Engineering rod bundle data bases, i.e. more than 7000 experimental CHF points of Columbia University data bank were used.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70032127','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70032127"><span>Using <span class="hlt">heat</span> to characterize streambed water <span class="hlt">flux</span> variability in four stream reaches</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Essaid, H.I.; Zamora, C.M.; McCarthy, K.A.; Vogel, J.R.; Wilson, J.T.</p> <p>2008-01-01</p> <p>Estimates of streambed water <span class="hlt">flux</span> are needed for the interpretation of streambed chemistry and reactions. Continuous temperature and head monitoring in stream reaches within four agricultural watersheds (Leary Weber Ditch, IN; Maple Creek, NE; DR2 Drain, WA; and Merced River, CA) allowed <span class="hlt">heat</span> to be used as a tracer to study the temporal and spatial variability of <span class="hlt">fluxes</span> through the streambed. Synoptic methods (seepage meter and differential discharge measurements) were compared with estimates obtained by using <span class="hlt">heat</span> as a tracer. Water <span class="hlt">flux</span> was estimated by modeling one-dimensional vertical flow of water and <span class="hlt">heat</span> using the model VS2DH. <span class="hlt">Flux</span> was influenced by physical heterogeneity of the stream channel and temporal variability in stream and ground-water levels. During most of the study period (April-December 2004), <span class="hlt">flux</span> was upward through the streambeds. At the IN, NE, and CA sites, high-stage events resulted in rapid reversal of flow direction inducing short-term surface-water flow into the streambed. During late summer at the IN site, regional ground-water levels dropped, leading to surface-water loss to ground water that resulted in drying of the ditch. Synoptic measurements of <span class="hlt">flux</span> generally supported the model <span class="hlt">flux</span> estimates. Water flow through the streambed was roughly an order of magnitude larger in the humid basins (IN and NE) than in the arid basins (WA and CA). Downward <span class="hlt">flux</span>, in response to sudden high streamflows, and seasonal variability in <span class="hlt">flux</span> was most pronounced in the humid basins and in high conductivity zones in the streambed. Copyright ?? 2008 by the American Society of Agronomy, Crop Science Society of America, and Soil Science Society of America. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20150018534','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20150018534"><span><span class="hlt">Heat</span> Transfer to Longitudinal Laminar Flow Between Cylinders</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Sparrow, Ephraim M.; Loeffler, Albert L. Jr.; Hubbard, H. A.</p> <p>1960-01-01</p> <p>Consideration is given to the fully developed <span class="hlt">heat</span> transfer characteristics for longitudinal laminar flow between cylinders arranged in an equilateral triangular array. The analysis is carried out for the condition of uniform <span class="hlt">heat</span> transfer per unit length. Solutions are obtained for the temperature distribution, and from these, Nusselt numbers are derived for a wide range of spacing-to-diameter ratios. It is found that as the spacing ratio increases, so also does the <span class="hlt">wall</span>-to-bulk temperature difference for a fixed <span class="hlt">heat</span> transfer per unit length. Corresponding to a uniform surface temperature around the circumference of a cylinder, the circumferential variation of the local <span class="hlt">heat</span> <span class="hlt">flux</span> is computed. For spacing ratios of 1.5 - 2.0 and greater, uniform peripheral <span class="hlt">wall</span> temperature and uniform peripheral <span class="hlt">heat</span> <span class="hlt">flux</span> are simultaneously achieved. A simplified analysis which neglects circumferential variations is also carried out, and the results are compared with those from the more exact formulation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/19880733','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/19880733"><span>Transectional <span class="hlt">heat</span> transfer in thermoregulating bigeye tuna (Thunnus obesus) - a 2D <span class="hlt">heat</span> <span class="hlt">flux</span> model.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Boye, Jess; Musyl, Michael; Brill, Richard; Malte, Hans</p> <p>2009-11-01</p> <p>We developed a 2D <span class="hlt">heat</span> <span class="hlt">flux</span> model to elucidate routes and rates of <span class="hlt">heat</span> transfer within bigeye tuna Thunnus obesus Lowe 1839 in both steady-state and time-dependent settings. In modeling the former situation, we adjusted the efficiencies of <span class="hlt">heat</span> conservation in the red and the white muscle so as to make the output of the model agree as closely as possible with observed cross-sectional isotherms. In modeling the latter situation, we applied the <span class="hlt">heat</span> exchanger efficiencies from the steady-state model to predict the distribution of temperature and <span class="hlt">heat</span> <span class="hlt">fluxes</span> in bigeye tuna during their extensive daily vertical excursions. The simulations yielded a close match to the data recorded in free-swimming fish and strongly point to the importance of the <span class="hlt">heat</span>-producing and <span class="hlt">heat</span>-conserving properties of the white muscle. The best correspondence between model output and observed data was obtained when the countercurrent <span class="hlt">heat</span> exchangers in the blood flow pathways to the red and white muscle retained 99% and 96% (respectively) of the <span class="hlt">heat</span> produced in these tissues. Our model confirms that the ability of bigeye tuna to maintain elevated muscle temperatures during their extensive daily vertical movements depends on their ability to rapidly modulate <span class="hlt">heating</span> and cooling rates. This study shows that the differential cooling and <span class="hlt">heating</span> rates could be fully accounted for by a mechanism where blood flow to the swimming muscles is either exclusively through the <span class="hlt">heat</span> exchangers or completely shunted around them, depending on the ambient temperature relative to the body temperature. Our results therefore strongly suggest that such a mechanism is involved in the extensive physiological thermoregulatory abilities of endothermic bigeye tuna.</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('http://adsabs.harvard.edu/abs/2018PhFl...30b5103K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018PhFl...30b5103K"><span>Mixed convection <span class="hlt">heat</span> transfer enhancement in a cubic lid-driven cavity containing a rotating cylinder through the introduction of artificial roughness on the <span class="hlt">heated</span> <span class="hlt">wall</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kareem, Ali Khaleel; Gao, Shian</p> <p>2018-02-01</p> <p>The aim of the present numerical investigation is to comprehensively analyse and understand the <span class="hlt">heat</span> transfer enhancement process using a roughened, <span class="hlt">heated</span> bottom <span class="hlt">wall</span> with two artificial rib types (R-s and R-c) due to unsteady mixed convection <span class="hlt">heat</span> transfer in a 3D moving top <span class="hlt">wall</span> enclosure that has a central rotating cylinder, and to compare these cases with the smooth bottom <span class="hlt">wall</span> case. These different cases (roughened and smooth bottom <span class="hlt">walls</span>) are considered at various clockwise and anticlockwise rotational speeds, -5 ≤ Ω ≤ 5, and Reynolds numbers of 5000 and 10 000. The top and bottom <span class="hlt">walls</span> of the lid-driven cavity are differentially <span class="hlt">heated</span>, whilst the remaining cavity <span class="hlt">walls</span> are assumed to be stationary and adiabatic. A standard k-ɛ model for the Unsteady Reynolds-Averaged Navier-Stokes equations is used to deal with the turbulent flow. The <span class="hlt">heat</span> transfer improvement is carefully considered and analysed through the detailed examinations of the flow and thermal fields, the turbulent kinetic energy, the mean velocity profiles, the <span class="hlt">wall</span> shear stresses, and the local and average Nusselt numbers. It has been concluded that artificial roughness can strongly affect the thermal fields and fluid flow patterns. Ultimately, the <span class="hlt">heat</span> transfer rate has been dramatically increased by involving the introduced artificial rips. Increasing the cylinder rotational speed or Reynolds number can enhance the <span class="hlt">heat</span> transfer process, especially when the <span class="hlt">wall</span> roughness exists.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EPJWC.14302079N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EPJWC.14302079N"><span>Visualization of various working fluids flow regimes in gravity <span class="hlt">heat</span> pipe</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Nemec, Patrik</p> <p></p> <p><span class="hlt">Heat</span> pipe is device working with phase changes of working fluid inside hermetically closed pipe at specific pressure. The phase changes of working fluid from fluid to vapour and vice versa help <span class="hlt">heat</span> pipe to transport high <span class="hlt">heat</span> <span class="hlt">flux</span>. Amount of <span class="hlt">heat</span> <span class="hlt">flux</span> transferred by <span class="hlt">heat</span> pipe, of course depends on kind of working fluid. The article deal about visualization of various working fluids flow regimes in glass gravity <span class="hlt">heat</span> pipe by high speed camera and processes casing inside during <span class="hlt">heat</span> pipe operation. Experiment working fluid flow visualization is performed with two glass <span class="hlt">heat</span> pipes with different inner diameter (13 mm and 22 mm) filled with water, ethanol and fluorinert FC 72. The working fluid flow visualization explains the phenomena as a working fluid boiling, nucleation of bubbles, and vapour condensation on the <span class="hlt">wall</span>, vapour and condensate flow interaction, flow down condensate film thickness on the <span class="hlt">wall</span> occurred during the <span class="hlt">heat</span> pipe operation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20040161241','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20040161241"><span>Effects of <span class="hlt">Heat</span> <span class="hlt">Flux</span>, Oxygen Concentration and Glass Fiber Volume Fraction on Pyrolysate Mass <span class="hlt">Flux</span> from Composite Solids</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Rich, D. B.; Lautenberger, C. W.; Yuan, Z.; Fernandez-Pello, A. C.</p> <p>2004-01-01</p> <p>Experimental work on the effects of <span class="hlt">heat</span> <span class="hlt">flux</span>, oxygen concentration and glass fiber volume fraction on pyrolysate mass <span class="hlt">flux</span> from samples of polypropylene/glass fiber composite (PP/G) is underway. The research is conducted as part of a larger project to develop a test methodology for flammability of materials, particularly composites, in the microgravity and variable oxygen concentration environment of spacecraft and space structures. Samples of PP/G sized at 30 x 30 x 10 mm are flush mounted in a flow tunnel, which provides a flow of oxidizer over the surface of the samples at a fixed value of 1 m/s and oxygen concentrations varying between 18 and 30%. Each sample is exposed to a constant external radiant <span class="hlt">heat</span> <span class="hlt">flux</span> at a given value, which varies between tests from 10 to 24 kW/sq m. Continuous sample mass loss and surface temperature measurements are recorded for each test. Some tests are conducted with an igniter and some are not. In the former case, the research goal is to quantify the critical mass <span class="hlt">flux</span> at ignition for the various environmental and material conditions described above. The later case generates a wider range of mass <span class="hlt">flux</span> rates than those seen prior to ignition, providing an opportunity to examine the protective effects of blowing on oxidative pyrolysis and <span class="hlt">heating</span> of the surface. Graphs of surface temperature and sample mass loss vs. time for samples of 30% PPG at oxygen concentrations of 18 and 21% are presented in the figures below. These figures give a clear indication of the lower pyrolysis rate and extended time to ignition that accompany a lower oxygen concentration. Analysis of the mass <span class="hlt">flux</span> rate at the time of ignition gives good repeatability but requires further work to provide a clear indication of mass <span class="hlt">flux</span> trends accompanying changes in environmental and material properties.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20040084193','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20040084193"><span>Effects of <span class="hlt">Heat</span> <span class="hlt">Flux</span>, Oxygen Concentration and Glass Fiber Volume Fraction on Pyrolysate Mass <span class="hlt">Flux</span> from Composite Solids</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Rich, D. B.; Lautenberger, C. W.; Yuan, Z.; Fernandez-Pello, A. C.</p> <p>2004-01-01</p> <p>Experimental work on the effects of <span class="hlt">heat</span> <span class="hlt">flux</span>, oxygen concentration and glass fiber volume fraction on pyrolysate mass <span class="hlt">flux</span> from samples of polypropylene/glass fiber composite (PP/G) is underway. The research is conducted as part of a larger project to develop a test methodology for flammability of materials, particularly composites, in the microgravity and variable oxygen concentration environment of spacecraft and space structures. Samples of PP/G sized at 30x30x10 mm are flush mounted in a flow tunnel, which provides a flow of oxidizer over the surface of the samples at a fixed value of 1 m/s and oxygen concentrations varying between 18 and 30%. Each sample is exposed to a constant external radiant <span class="hlt">heat</span> <span class="hlt">flux</span> at a given value, which varies between tests from 10 to 24 kW/m2. Continuous sample mass loss and surface temperature measurements are recorded for each test. Some tests are conducted with an igniter and some are not. In the former case, the research goal is to quantify the critical mass <span class="hlt">flux</span> at ignition for the various environmental and material conditions described above. The later case generates a wider range of mass <span class="hlt">flux</span> rates than those seen prior to ignition, providing an opportunity to examine the protective effects of blowing on oxidative pyrolysis and <span class="hlt">heating</span> of the surface. Graphs of surface temperature and sample mass loss vs. time for samples of 30% PPG at oxygen concentrations of 18 and 21% are presented in the figures below. These figures give a clear indication of the lower pyrolysis rate and extended time to ignition that accompany a lower oxygen concentration. Analysis of the mass <span class="hlt">flux</span> rate at the time of ignition gives good repeatability but requires further work to provide a clear indication of mass <span class="hlt">flux</span> trends accompanying changes in environmental and material properties.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017ClDy...49.1531H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017ClDy...49.1531H"><span>Revisiting the global surface energy budgets with maximum-entropy-production model of surface <span class="hlt">heat</span> <span class="hlt">fluxes</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Huang, Shih-Yu; Deng, Yi; Wang, Jingfeng</p> <p>2017-09-01</p> <p>The maximum-entropy-production (MEP) model of surface <span class="hlt">heat</span> <span class="hlt">fluxes</span>, based on contemporary non-equilibrium thermodynamics, information theory, and atmospheric turbulence theory, is used to re-estimate the global surface <span class="hlt">heat</span> <span class="hlt">fluxes</span>. The MEP model predicted surface <span class="hlt">fluxes</span> automatically balance the surface energy budgets at all time and space scales without the explicit use of near-surface temperature and moisture gradient, wind speed and surface roughness data. The new MEP-based global annual mean <span class="hlt">fluxes</span> over the land surface, using input data of surface radiation, temperature data from National Aeronautics and Space Administration-Clouds and the Earth's Radiant Energy System (NASA CERES) supplemented by surface specific humidity data from the Modern-Era Retrospective Analysis for Research and Applications (MERRA), agree closely with previous estimates. The new estimate of ocean evaporation, not using the MERRA reanalysis data as model inputs, is lower than previous estimates, while the new estimate of ocean sensible <span class="hlt">heat</span> <span class="hlt">flux</span> is higher than previously reported. The MEP model also produces the first global map of ocean surface <span class="hlt">heat</span> <span class="hlt">flux</span> that is not available from existing global reanalysis products.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1993eash.book.....A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1993eash.book.....A"><span>Experimental and analytical studies of high <span class="hlt">heat</span> <span class="hlt">flux</span> components for fusion experimental reactor</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Araki, Masanori</p> <p>1993-03-01</p> <p>In this report, the experimental and analytical results concerning the development of plasma facing components of ITER are described. With respect to developing high <span class="hlt">heat</span> removal structures for the divertor plates, an externally-finned swirl tube was developed based on the results of critical <span class="hlt">heat</span> <span class="hlt">flux</span> (CHF) experiments on various tube structures. As the result, the burnout <span class="hlt">heat</span> <span class="hlt">flux</span>, which also indicates incident CHF, of 41 (+/-) 1 MW/sq m was achieved in the externally-finned swirl tube. The applicability of existing CHF correlations based on uniform <span class="hlt">heating</span> conditions was evaluated by comparing the CHF experimental data with the smooth and the externally-finned tubes under one-sided <span class="hlt">heating</span> condition. As the results, experimentally determined CHF data for straight tube show good agreement, for the externally-finned tube, no existing correlations are available for prediction of the CHF. With respect to the evaluation of the bonds between carbon-based material and <span class="hlt">heat</span> sink metal, results of brazing tests were compared with the analytical results by three dimensional model with temperature-dependent thermal and mechanical properties. Analytical results showed that residual stresses from brazing can be estimated by the analytical three directional stress values instead of the equivalent stress value applied. In the analytical study on the separatrix sweeping for effectively reducing surface <span class="hlt">heat</span> <span class="hlt">fluxes</span> on the divertor plate, thermal response of the divertor plate was analyzed under ITER relevant <span class="hlt">heat</span> <span class="hlt">flux</span> conditions and has been tested. As the result, it has been demonstrated that application of the sweeping technique is very effective for improvement in the power handling capability of the divertor plate and that the divertor mock-up has withstood a large number of additional cyclic <span class="hlt">heat</span> loads.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20110008740','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20110008740"><span>Monitoring Delamination of Thermal Barrier Coatings During Interrupted High-<span class="hlt">Heat-Flux</span> Laser Testing using Luminescence Imaging</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.; Zhu, Dongming; Wolfe, Douglas E.</p> <p>2011-01-01</p> <p>This presentation showed progress made in extending luminescence-base delamination monitoring to TBCs exposed to high <span class="hlt">heat</span> <span class="hlt">fluxes</span>, which is an environment that much better simulates actual turbine engine conditions. This was done by performing upconversion luminescence imaging during interruptions in laser testing, where a high-power CO2 laser was employed to create the desired <span class="hlt">heat</span> <span class="hlt">flux</span>. Upconverison luminescence refers to luminescence where the emission is at a higher energy (shorter wavelength) than the excitation. Since there will be negligible background emission at higher energies than the excitation, this methods produces superb contrast. Delamination contrast is produced because both the excitation and emission wavelengths are reflected at delamination cracks so that substantially higher luminescence intensity is observed in regions containing delamination cracks. Erbium was selected as the dopant for luminescence specifically because it exhibits upconversion luminescence. The high power CO2 10.6 micron wavelength laser facility at NASA GRC was used to produce the <span class="hlt">heat</span> <span class="hlt">flux</span> in combination with forced air backside cooling. Testing was performed at a lower (95 W/sq cm) and higher (125 W/sq cm) <span class="hlt">heat</span> <span class="hlt">flux</span> as well as furnace cycling at 1163C for comparison. The lower <span class="hlt">heat</span> <span class="hlt">flux</span> showed the same general behavior as furnace cycling, a gradual, "spotty" increase in luminescence associated with debond progression; however, a significant difference was a pronounced incubation period followed by acceleration delamination progression. These results indicate that extrapolating behavior from furnace cycling measurements will grossly overestimate remaining life under high <span class="hlt">heat</span> <span class="hlt">flux</span> conditions. The higher <span class="hlt">heat</span> <span class="hlt">flux</span> results were not only accelerated, but much different in character. Extreme bond coat rumpling occurred, and delamination propagation extended over much larger areas before precipitating macroscopic TBC failure. This indicates that under the higher <span class="hlt">heat</span> <span class="hlt">flux</span> (and</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMGC21D0969Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMGC21D0969Z"><span>Uncertainty analysis of scintillometers methods in measuring sensible <span class="hlt">heat</span> <span class="hlt">fluxes</span> of forest ecosystem</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zheng, N.</p> <p>2017-12-01</p> <p>Sensible <span class="hlt">heat</span> <span class="hlt">flux</span> (H) is one of the driving factors of surface turbulent motion and energy exchange. Therefore, it is particularly important to measure sensible <span class="hlt">heat</span> <span class="hlt">flux</span> accurately at the regional scale. However, due to the heterogeneity of the underlying surface, hydrothermal regime, and different weather conditions, it is difficult to estimate the represented <span class="hlt">flux</span> at the kilometer scale. The scintillometer have been developed into an effective and universal equipment for deriving <span class="hlt">heat</span> <span class="hlt">flux</span> at the regional-scale which based on the turbulence effect of light in the atmosphere since the 1980s. The parameter directly obtained by the scintillometer is the structure parameter of the refractive index of air based on the changes of light intensity fluctuation. Combine with parameters such as temperature structure parameter, zero-plane displacement, surface roughness, wind velocity, air temperature and the other meteorological data <span class="hlt">heat</span> <span class="hlt">fluxes</span> can be derived. These additional parameters increase the uncertainties of <span class="hlt">flux</span> because the difference between the actual feature of turbulent motion and the applicable conditions of turbulence theory. Most previous studies often focused on the constant <span class="hlt">flux</span> layers that are above the rough sub-layers and homogeneous flat surfaces underlying surfaces with suitable weather conditions. Therefore, the criteria and modified forms of key parameters are invariable. In this study, we conduct investment over the hilly area of northern China with different plants, such as cork oak, cedar-black and locust. On the basis of key research on the threshold and modified forms of saturation with different turbulence intensity, modified forms of Bowen ratio with different drying-and-wetting conditions, universal function for the temperature structure parameter under different atmospheric stability, the dominant sources of uncertainty will be determined. The above study is significant to reveal influence mechanism of uncertainty and explore influence</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19720004950','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19720004950"><span>Dynamics of <span class="hlt">heat</span>-pipe reactors</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Niederauer, G. F.</p> <p>1971-01-01</p> <p>A split-core <span class="hlt">heat</span> pipe reactor, fueled with either U(233)C or U(235)C in a tungsten cermet and cooled by 7-Li-W <span class="hlt">heat</span> pipes, was examined for the effects of the <span class="hlt">heat</span> pipes on reactor while trying to safely absorb large reactivity inputs through inherent shutdown mechanisms. Limits on ramp reactivity inputs due to fuel melting temperature and <span class="hlt">heat</span> pipe <span class="hlt">wall</span> <span class="hlt">heat</span> <span class="hlt">flux</span> were mapped for the reactor in both startup and at-power operating modes.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4882143','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4882143"><span>Calibration of High <span class="hlt">Heat</span> <span class="hlt">Flux</span> Sensors at NIST</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Murthy, A. V.; Tsai, B. K.; Gibson, C. E.</p> <p>1997-01-01</p> <p>An ongoing program at the National Institute of Standards and Technology (NIST) is aimed at improving and standardizing <span class="hlt">heat-flux</span> sensor calibration methods. The current calibration needs of U.S. science and industry exceed the current NIST capability of 40 kW/m2 irradiance. In achieving this goal, as well as meeting lower-level non-radiative <span class="hlt">heat</span> <span class="hlt">flux</span> calibration needs of science and industry, three different types of calibration facilities currently are under development at NIST: convection, conduction, and radiation. This paper describes the research activities associated with the NIST Radiation Calibration Facility. Two different techniques, transfer and absolute, are presented. The transfer calibration technique employs a transfer standard calibrated with reference to a radiometric standard for calibrating the sensors using a graphite tube blackbody. Plans for an absolute calibration facility include the use of a spherical blackbody and a cooled aperture and sensor-housing assembly to calibrate the sensors in a low convective environment. PMID:27805156</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19910011011','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19910011011"><span>Self-pressurization of a flightweight liquid hydrogen storage tank subjected to low <span class="hlt">heat</span> <span class="hlt">flux</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Hasan, M. M.; Lin, C. S.; Vandresar, N. T.</p> <p>1991-01-01</p> <p>Results are presented for an experimental investigation of self-pressurization and thermal stratification of a 4.89 cu m liquid hydrogen (LH2) storage tank subjected to low <span class="hlt">heat</span> <span class="hlt">flux</span> (0.35, 2.0, and 3.5 W/sq m) under normal gravity conditions. Tests were performed at fill levels of 83 to 84 percent (by volume). The LH2 tank was representative of future spacecraft tankage, having a low mass-to-volume ratio and high performance multilayer thermal insulation. Results show that the pressure rise rate and thermal stratification increase with increasing <span class="hlt">heat</span> <span class="hlt">flux</span>. At the lowest <span class="hlt">heat</span> <span class="hlt">flux</span>, the pressure rise rate is comparable to the homogenous rate, while at the highest <span class="hlt">heat</span> <span class="hlt">flux</span>, the rate is more than three times the homogeneous rate. It was found that initial conditions have a significant impact on the initial pressure rise rate. The quasi-steady pressure rise rates are nearly independent of the initial condition after an initial transient period has passed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AGUFM.P53A1845G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFM.P53A1845G"><span>Counterintuitive Constraints on Chaos Formation Set by <span class="hlt">Heat</span> <span class="hlt">Flux</span> through Europa's Ocean</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Goodman, J. C.</p> <p>2013-12-01</p> <p>Models for the formation of disruptive chaos features on the icy surface of Europa fall into two broad categories: either chaos is formed when basal <span class="hlt">heating</span> causes localized melting and thinning of the ice shell, or basal <span class="hlt">heating</span> drives diapiric convection within the ice shell. We argue that in both of these cases, <span class="hlt">heating</span> of the ice shell from below does not lead to chaos formation at the location of <span class="hlt">heating</span>. If chaos is formed when a localized oceanic <span class="hlt">heat</span> source, such as a hydrothermal plume, "melts through" the ice crust, we must consider what happens to the melted liquid. If Europa's ocean is salty, the melt will form a buoyant pool inside the melted cavity, leading to a stable interface between cold fresh meltwater and warm salty seawater. This stable interface acts like an ablative <span class="hlt">heat</span> shield, protecting the ice from further damage. Some <span class="hlt">heat</span> can be transferred across the stable layer by double diffusion, but this transfer is very inefficient. We calculate that local ocean <span class="hlt">heating</span> cannot be balanced by local <span class="hlt">flux</span> through the stable layer: instead, the warm ocean water must spread laterally until it is delivering <span class="hlt">heat</span> to the ice base on a regional or global scale (a <span class="hlt">heating</span> zone hundreds or thousands of km across, for conservative parameters.) If chaos is formed by diapiric solid-state convection within the ice shell, many investigators have assumed that diapirism and chaos should be most prevalent where the basal <span class="hlt">heat</span> <span class="hlt">flux</span> is strongest. We argue that this is not the case. In Rayleigh-Benard convection, increasing the <span class="hlt">heat</span> <span class="hlt">flux</span> will make convection more vigorous --- if and only if the convecting layer thickness does not change. We argue that increased basal <span class="hlt">heat</span> <span class="hlt">flux</span> will thin the ice shell, reducing its Rayleigh number and making convection less likely, not more. This insight allows us to reverse the logic of recent discussions of the relationship between ocean circulation and chaos (for instance, Soderlund et al, 2013 LPSC). We argue that global oceanic</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/20527160','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/20527160"><span>[Characteristics of CO2 <span class="hlt">flux</span> before and in the <span class="hlt">heating</span> period at urban complex underlying surface area].</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Jia, Qing-yu; Zhou, Guang-sheng; Wang, Yu; Liu, Xiao-mei</p> <p>2010-04-01</p> <p>Urban areas were significant contributors to global carbon dioxide emissions. The eddy covariance (EC) was used to measure carbon dioxide (CO2) concentration and <span class="hlt">flux</span> data at urban area in Shenyang. This research analyzed the characteristics of atmospheric CO2 concentration and <span class="hlt">flux</span> in October 2008 to November 2008 period before and in the <span class="hlt">heating</span> period. The results showed that the daily variation of CO2 concentration was two-peak curve. The first peak time appeared as same as sunrise time, while the second peak time impacted by vehicles and <span class="hlt">heating</span>. The result of CO2 <span class="hlt">flux</span> showed that urban atmospheric CO2 was net emissions, vegetation photosynthesis absorbed CO2 of traffic, the CO2 <span class="hlt">flux</span> peak appeared at 17:15-18:15 in the <span class="hlt">heating</span> period, CO2 emission increased 29.37 g x (m2 x d)(-1) in the <span class="hlt">heating</span> period than that before the <span class="hlt">heating</span> period; there was corresponding relationship between CO2 <span class="hlt">flux</span> and the time when temperature peak and sensible <span class="hlt">heating</span> <span class="hlt">flux</span> (Hc) turn positive. The results also indicated that atmospheric CO2 concentration and its <span class="hlt">flux</span> were affected seriously by both wind direction and carbon sources.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMSH32A..04S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMSH32A..04S"><span>Control Mechanisms of the Electron <span class="hlt">Heat</span> <span class="hlt">Flux</span> in the Solar Wind: Observations in Comparison to Numerical Simulations</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Stverak, S.; Hellinger, P.; Landi, S.; Travnicek, P. M.; Maksimovic, M.</p> <p>2017-12-01</p> <p>Recent understanding of the <span class="hlt">heat</span> transport and dissipation in the expanding solar wind propose number of complex control mechanisms down to the electron kinetic scales. We investigate the evolution of electron <span class="hlt">heat</span> <span class="hlt">flux</span> properties and constraints along the expansion using in situ observations from Helios spacecraft in comparison to numerical kinetic simulations. In particular we focus on the roles of Coulomb collisions and wave-particle interactions in shaping the electron velocity distribution functions and thus controlling the <span class="hlt">heat</span> transported by the electron <span class="hlt">heat</span> <span class="hlt">flux</span>. We show the general evolution of the electron <span class="hlt">heat</span> <span class="hlt">flux</span> to be driven namely by the Coulomb collisions. Locally we demonstrate the wave-particle interactions related to the kinetic plasma instabilities to be providing effective constraints in case of extreme <span class="hlt">heat</span> <span class="hlt">flux</span> levels.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017RPFSU..25..123H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017RPFSU..25..123H"><span>The Effect of the <span class="hlt">Heat</span> <span class="hlt">Flux</span> on the Self-Ignition of Oriented Strand Board</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hirle, Siegfried; Balog, Karol</p> <p>2017-06-01</p> <p>This article deals with the initiation phase of flaming and smouldering burning of oriented strand board. The influence of <span class="hlt">heat</span> <span class="hlt">flux</span> on thermal degradation of OSB boards, time to ignition, <span class="hlt">heat</span> release rate and mass loss rate using thermal analysis and vertical electrical radiation panel methods were studied. Significant information on the influence of the <span class="hlt">heat</span> <span class="hlt">flux</span> density and the thickness of the material on time to ignition was obtained.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19720011318','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19720011318"><span>Pyrotechnic hazards classification and evaluation program test report. <span class="hlt">Heat</span> <span class="hlt">flux</span> study of deflagrating pyrotechnic munitions</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Fassnacht, P. O.</p> <p>1971-01-01</p> <p>A <span class="hlt">heat</span> <span class="hlt">flux</span> study of deflagrating pyrotechnic munitions is presented. Three tests were authorized to investigate whether <span class="hlt">heat</span> <span class="hlt">flux</span> measurements may be used as effective hazards evaluation criteria to determine safe quantity distances for pyrotechnics. A passive sensor study was conducted simultaneously to investigate their usefulness in recording events and conditions. It was concluded that <span class="hlt">heat</span> <span class="hlt">flux</span> measurements can effectively be used to evaluate hazards criteria and that passive sensors are an inexpensive tool to record certain events in the vicinity of deflagrating pyrotechnic stacks.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/16118893','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/16118893"><span>Finger <span class="hlt">heat</span> <span class="hlt">flux</span>/temperature as an indicator of thermal imbalance with application for extravehicular activity.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Koscheyev, Victor S; Leon, Gloria R; Coca, Aitor</p> <p>2005-11-01</p> <p>The designation of a simple, non-invasive, and highly precise method to monitor the thermal status of astronauts is important to enhance safety during extravehicular activities (EVA) and onboard emergencies. Finger temperature (Tfing), finger <span class="hlt">heat</span> <span class="hlt">flux</span>, and indices of core temperature (Tc) [rectal (Tre), ear canal (Tec)] were assessed in 3 studies involving different patterns of <span class="hlt">heat</span> removal/insertion from/to the body by a multi-compartment liquid cooling/warming garment (LCWG). Under both uniform and nonuniform temperature conditions on the body surface, Tfing and finger <span class="hlt">heat</span> <span class="hlt">flux</span> were highly correlated with garment <span class="hlt">heat</span> <span class="hlt">flux</span>, and also highly correlated with each other. Tc responses did not adequately reflect changes in thermal balance during the ongoing process of <span class="hlt">heat</span> insertion/removal from the body. Overall, Tfing/finger <span class="hlt">heat</span> <span class="hlt">flux</span> adequately reflected the initial destabilization of thermal balance, and therefore appears to have significant potential as a useful index for monitoring and maintaining thermal balance and comfort in extreme conditions in space as well as on Earth. c2005 Elsevier Ltd. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19930036590&hterms=carbon+footprint&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Dcarbon%2Bfootprint','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19930036590&hterms=carbon+footprint&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Dcarbon%2Bfootprint"><span>Aircraft- and tower-based <span class="hlt">fluxes</span> of carbon dioxide, latent, and sensible <span class="hlt">heat</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Desjardins, R. L.; Hart, R. L.; Macpherson, J. I.; Schuepp, P. H.; Verma, S. B.</p> <p>1992-01-01</p> <p><span class="hlt">Fluxes</span> of carbon dioxide, water vapor, and sensible <span class="hlt">heat</span> obtained over a grassland ecosystem, during the First International Satellite Land Surface Climatology Project (ISLSCP) Field Experiment (FIFE), using an aircraft- and two tower-based systems are compared for several days in 1987 and in 1989. The tower-based cospectral estimates of CO2, sensible <span class="hlt">heat</span>, water vapor, and momentum, expressed as a function of wavenumber K times sampling height z, are relatively similar to the aircraft-based estimates for K x z greater than 0.1. A measurable contribution to the <span class="hlt">fluxes</span> is observed by tower-based systems at K x z less than 0.01 but not by the aircraft-based system operating at an altitude of approximately 100 m over a 15 x 15 km area. Using all available simultaneous aircraft and tower data, <span class="hlt">flux</span> estimates by both systems were shown to be highly correlated. As expected from the spatial variations of the greenness index, surface extrapolation of airborne <span class="hlt">flux</span> estimates tended to lie between those of the two tower sites. The average <span class="hlt">fluxes</span> obtained, on July 11, 1987, and August 4, 1989, by flying a grid pattern over the FIFE site agreed with the two tower data sets for CO2, but sensible and latent <span class="hlt">heat</span> were smaller than those obtained by the tower-based systems. However, in general, except for a small underestimation due to the long wavelength contributions and due to <span class="hlt">flux</span> divergence with height, the differences between the aircraft- and tower-based surface estimates of <span class="hlt">fluxes</span> appear to be mainly attributable to differences in footprint, that is, differences in the area contributing to the surface <span class="hlt">flux</span> estimates.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20130000651','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20130000651"><span>Surface Catalysis and Oxidation on Stagnation Point <span class="hlt">Heat</span> <span class="hlt">Flux</span> Measurements in High Enthalpy Arc Jets</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Nawaz, Anuscheh; Driver, David M.; Terrazas-Salinas</p> <p>2013-01-01</p> <p><span class="hlt">Heat</span> <span class="hlt">flux</span> sensors are routinely used in arc jet facilities to determine <span class="hlt">heat</span> transfer rates from plasma plume. The goal of this study is to assess the impact of surface composition changes on these <span class="hlt">heat</span> <span class="hlt">flux</span> sensors. Surface compositions can change due to oxidation and material deposition from the arc jet. Systematic surface analyses of the sensors were conducted before and after exposure to plasma. Currently copper is commonly used as surface material. Other surface materials were studied including nickel, constantan gold, platinum and silicon dioxide. The surfaces were exposed to plasma between 0.3 seconds and 3 seconds. Surface changes due to oxidation as well as copper deposition from the arc jets were observed. Results from changes in measured <span class="hlt">heat</span> <span class="hlt">flux</span> as a function of surface catalycity is given, along with a first assessment of enthalpy for these measurements. The use of cupric oxide is recommended for future <span class="hlt">heat</span> <span class="hlt">flux</span> measurements, due to its consistent surface composition arc jets.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMSH41C..02G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMSH41C..02G"><span>Chromospheric <span class="hlt">Heating</span> Driven by Cancellations of Internetwork Magnetic <span class="hlt">Flux</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Gosic, M.; de la Cruz Rodriguez, J.; De Pontieu, B.; Bellot Rubio, L.; Esteban Pozuelo, S.; Ortiz-Carbonell, A. N.</p> <p>2017-12-01</p> <p>The <span class="hlt">heating</span> of the solar chromosphere remains to be one of the most important questions in solar physics. It is believed that this phenomenon may significantly be supported by small-scale internetwork (IN) magnetic fields. Indeed, cancellations of IN magnetic <span class="hlt">flux</span> can generate transient brightenings in the chromosphere and transition region. These bright structures might be the signature of energy release and plasma <span class="hlt">heating</span>, probably driven by magnetic reconnection of IN field lines. Using high resolution, multiwavelength, coordinated observations recorded with the Interface Region Imaging Spectrograph (IRIS) and the Swedish 1-m Solar Telescope (SST), we analyzed cancellations of IN <span class="hlt">flux</span> and their impact on the energetics and dynamics of the quiet Sun atmosphere. From their temporal and spatial evolution, we determine that these events can <span class="hlt">heat</span> locally the upper atmospheric layers. However, employing multi-line inversions of the Mg II h & k lines, we show that cancellations, although occurring ubiquitously over IN regions, are not capable of sustaining the total radiative losses of the quiet Sun chromosphere.</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('http://adsabs.harvard.edu/abs/2012RScI...83c3501B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012RScI...83c3501B"><span>Surface thermocouples for measurement of pulsed <span class="hlt">heat</span> <span class="hlt">flux</span> in the divertor of the Alcator C-Mod tokamak</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Brunner, D.; LaBombard, B.</p> <p>2012-03-01</p> <p>A novel set of thermocouple sensors has been developed to measure <span class="hlt">heat</span> <span class="hlt">fluxes</span> arriving at divertor surfaces in the Alcator C-Mod tokamak, a magnetic confinement fusion experiment. These sensors operate in direct contact with the divertor plasma, which deposits <span class="hlt">heat</span> <span class="hlt">fluxes</span> in excess of ˜10 MW/m2 over an ˜1 s pulse. Thermoelectric EMF signals are produced across a non-standard bimetallic junction: a 50 μm thick 74% tungsten-26% rhenium ribbon embedded in a 6.35 mm diameter molybdenum cylinder. The unique coaxial geometry of the sensor combined with its single-point electrical ground contact minimizes interference from the plasma/magnetic environment. Incident <span class="hlt">heat</span> <span class="hlt">fluxes</span> are inferred from surface temperature evolution via a 1D thermal <span class="hlt">heat</span> transport model. For an incident <span class="hlt">heat</span> <span class="hlt">flux</span> of 10 MW/m2, surface temperatures rise ˜1000 °C/s, corresponding to a <span class="hlt">heat</span> <span class="hlt">flux</span> flowing along the local magnetic field of ˜200 MW/m2. Separate calorimeter sensors are used to independently confirm the derived <span class="hlt">heat</span> <span class="hlt">fluxes</span> by comparing total energies deposited during a plasma pulse. Langmuir probes in close proximity to the surface thermocouples are used to test plasma-sheath <span class="hlt">heat</span> transmission theory and to identify potential sources of discrepancies among physical models.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19840020949','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19840020949"><span>Methane <span class="hlt">heat</span> transfer investigation</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p></p> <p>1984-01-01</p> <p>Future high chamber pressure LOX/hydrocarbon booster engines require copper base alloy main combustion chamber coolant channels similar to the SSME to provide adequate cooling and reusable engine life. Therefore, it is of vital importance to evaluate the <span class="hlt">heat</span> transfer characteristics and coking thresholds for LNG (94% methane) cooling, with a copper base alloy material adjacent to he fuel coolant. High pressure methane cooling and coking characteristics recently evaluated at Rocketdyne using stainless steel <span class="hlt">heated</span> tubes at methane bulk temperatures and coolant <span class="hlt">wall</span> temperatures typical of advanced engine operation except at lower <span class="hlt">heat</span> <span class="hlt">fluxes</span> as limited by the tube material. As expected, there was no coking observed. However, coking evaluations need be conducted with a copper base surface exposed to the methane coolant at higher <span class="hlt">heat</span> <span class="hlt">fluxes</span> approaching those of future high chamber pressure engines.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19900063454&hterms=equilibrium+liquid+vapors&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3Dequilibrium%2Bliquid%2Bvapors','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19900063454&hterms=equilibrium+liquid+vapors&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3Dequilibrium%2Bliquid%2Bvapors"><span>An analysis of the vapor flow and the <span class="hlt">heat</span> conduction through the liquid-wick and pipe <span class="hlt">wall</span> in a <span class="hlt">heat</span> pipe with single or multiple <span class="hlt">heat</span> sources</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Chen, Ming-Ming; Faghri, Amir</p> <p>1990-01-01</p> <p>A numerical analysis is presented for the overall performance of <span class="hlt">heat</span> pipes with single or multiple <span class="hlt">heat</span> sources. The analysis includes the <span class="hlt">heat</span> conduction in the <span class="hlt">wall</span> and liquid-wick regions as well as the compressibility effect of the vapor inside the <span class="hlt">heat</span> pipe. The two-dimensional elliptic governing equations in conjunction with the thermodynamic equilibrium relation and appropriate boundary conditions are solved numerically. The solutions are in agreement with existing experimental data for the vapor and <span class="hlt">wall</span> temperatures at both low and high operating temperatures.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/863792','DOE-PATENT-XML'); return false;" href="https://www.osti.gov/servlets/purl/863792"><span><span class="hlt">Heat</span> exchanger with leak detecting double <span class="hlt">wall</span> tubes</span></a></p> <p><a target="_blank" href="http://www.osti.gov/doepatents">DOEpatents</a></p> <p>Bieberbach, George; Bongaards, Donald J.; Lohmeier, Alfred; Duke, James M.</p> <p>1981-01-01</p> <p>A straight shell and tube <span class="hlt">heat</span> exchanger utilizing double <span class="hlt">wall</span> tubes and three tubesheets to ensure separation of the primary and secondary fluid and reliable leak detection of a leak in either the primary or the secondary fluids to further ensure that there is no mixing of the two fluids.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/20643911-role-electron-heat-flux-guide-field-magnetic-reconnection','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/20643911-role-electron-heat-flux-guide-field-magnetic-reconnection"><span>The role of electron <span class="hlt">heat</span> <span class="hlt">flux</span> in guide-field magnetic reconnection</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>Hesse, Michael; Kuznetsova, Masha; Birn, Joachim</p> <p>2004-12-01</p> <p>A combination of analytical theory and particle-in-cell simulations are employed in order to investigate the electron dynamics near and at the site of guide field magnetic reconnection. A detailed analysis of the contributions to the reconnection electric field shows that both bulk inertia and pressure-based quasiviscous processes are important for the electrons. Analytic scaling demonstrates that conventional approximations for the electron pressure tensor behavior in the dissipation region fail, and that <span class="hlt">heat</span> <span class="hlt">flux</span> contributions need to be accounted for. Based on the evolution equation of the <span class="hlt">heat</span> <span class="hlt">flux</span> three tensor, which is derived in this paper, an approximate form ofmore » the relevant <span class="hlt">heat</span> <span class="hlt">flux</span> contributions to the pressure tensor is developed, which reproduces the numerical modeling result reasonably well. Based on this approximation, it is possible to develop a scaling of the electron current layer in the central dissipation region. It is shown that the pressure tensor contributions become important at the scale length defined by the electron Larmor radius in the guide magnetic field.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20080006072','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20080006072"><span>High-<span class="hlt">Heat-Flux</span> Cyclic Durability of Thermal and Environmental Barrier Coatings</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Zhu, Dongming; Ghosn, Louis L.; Miller, Robert A.</p> <p>2007-01-01</p> <p>Advanced ceramic thermal and environmental barrier coatings will play an increasingly important role in future gas turbine engines because of their ability to protect the engine components and further raise engine temperatures. For the supersonic vehicles currently envisioned in the NASA fundamental aeronautics program, advanced gas turbine engines will be used to provide high power density thrust during the extended supersonic flight of the aircraft, while meeting stringent low emission requirements. Advanced ceramic coating systems are critical to the performance, life and durability of the hot-section components of the engine systems. In this work, the laser and burner rig based high-<span class="hlt">heat-flux</span> testing approaches were developed to investigate the coating cyclic response and failure mechanisms under simulated supersonic long-duration cruise mission. The accelerated coating cracking and delamination mechanism under the engine high-<span class="hlt">heat-flux</span>, and extended supersonic cruise time conditions will be addressed. A coating life prediction framework may be realized by examining the crack initiation and propagation in conjunction with environmental degradation under high-<span class="hlt">heat-flux</span> test conditions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2007AIPC..936..659P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2007AIPC..936..659P"><span>Numerical Simulation of <span class="hlt">Wall</span> <span class="hlt">Heat</span> Load in Combustor Flow</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Panara, D.; Hase, M.; Krebs, W.; Noll, B.</p> <p>2007-09-01</p> <p>Due to the major mechanism of NOx generation, there is generally a temperature trade off between improved cycle efficiency, material constraints and low NOx emission. The cycle efficiency is proportional to the highest cycle temperature, but unfortunately also the NOx production increases with increasing combustion temperature. For this reason, the modern combustion chamber design has been oriented towards lean premixed combustion system and more and more attention must be focused on the cooling air management. The challenge is to ensure sufficiently low temperature of the combustion liner with very low amount of film or effusion cooling air. Correct numerical prediction of temperature fields and <span class="hlt">wall</span> <span class="hlt">heat</span> load are therefore of critical interest in the modern combustion chamber design. Moreover, lean combustion technology has shown the appearance of thermo-acoustic instabilities which have to be taken into account in the simulation and, more in general, in the design of reliable combustion systems. In this framework, the present investigation addresses the capability of a commercial multiphysics code (ANSYS CFX) to correctly predict the <span class="hlt">wall</span> <span class="hlt">heat</span> load and the core flow temperature field in a scaled power generation combustion chamber with a simplified ceramic liner. Comparison are made with the experimental results from the ITS test rig at the University of Karlsruhe [1] and with a previous numerical campaign from [2]. In addition the effect of flow unsteadyness on the <span class="hlt">wall</span> <span class="hlt">heat</span> load is discussed showing some limitations of the traditional steady state flow thermal design.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19730022520','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19730022520"><span>Viscous hydrodynamic instability theory of the peak and minimum pool boiling <span class="hlt">heat</span> <span class="hlt">fluxes</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Dhir, V. K.</p> <p>1972-01-01</p> <p>Liquid viscosity was included in the Bellman-Pennington theory of the Taylor wave in a liquid vapor interface. Predictions of the most susceptible wavelength, and of the wave frequency, were made as a function of a liquid viscosity parameter and the Bond number. The stability of a gas jet in a viscous liquid was studied and the result is used to predict the peak <span class="hlt">heat</span> <span class="hlt">flux</span> on large horizontal heaters. Experimental measurements of the dominant Taylor wave and its growth rate were made during the film boiling of cyclohexanol on cylindrical heaters. The results bear out the predictions quite well. The thickness of the vapor blanket surrounding a cylindrical heater was measured and a correlation suggested. The effect of large <span class="hlt">fluxes</span> of vapor volume on the dominant wavelength was also noted. Theoretical results of the peak <span class="hlt">heat</span> <span class="hlt">flux</span> are compared with the experimental data, and the effect of finite geometry of flat plate heaters on the peak <span class="hlt">heat</span> <span class="hlt">flux</span> is also discussed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20160003590&hterms=strengthening&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D80%26Ntt%3Dstrengthening','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20160003590&hterms=strengthening&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D80%26Ntt%3Dstrengthening"><span>The Impact of Trends in the Large Scale Atmospheric Circulation on Mediterranean Surface Turbulent <span class="hlt">Heat</span> <span class="hlt">Fluxes</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Romanski, Joy; Hameed, Sultan</p> <p>2015-01-01</p> <p>Interannual variations of latent <span class="hlt">heat</span> <span class="hlt">fluxes</span> (LHF) and sensible <span class="hlt">heat</span> <span class="hlt">fluxes</span> (SHF) over the Mediterranean for the boreal winter season (DJF) show positive trends during 1958-2011. Using reanalysis and satellite-based products, the variability and trends in the <span class="hlt">heat</span> <span class="hlt">fluxes</span> are compared with variations in three atmospheric teleconnection patterns: the North Atlantic Oscillation (NAO), the pressure and position of the Azores High (AH), and the East Atlantic-West Russia teleconnection pattern (EAWR). Comparison of correlations between the <span class="hlt">heat</span> <span class="hlt">fluxes</span> and teleconnections, along with analysis of composites of surface temperature, humidity, and wind fields for different teleconnection states, demonstrates that the AH explains the <span class="hlt">heat</span> <span class="hlt">flux</span> changes more successfully than NAO and EAWR. Trends in pressure and longitude of the Azores High show a strengthening and an eastward shift. Variations of the Azores High occur along an axis defined by lower pressure and westward location at one extreme and higher pressure and eastward location at the other extreme. The shift of the AH from predominance of the low/west state to the high/east state induces trends in Mediterranean Sea surface winds, temperature, and moisture. These, combined with sea surface warming trends, produce trends in wintertime sensible and latent <span class="hlt">heat</span> <span class="hlt">fluxes</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017ApJ...846..165U','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017ApJ...846..165U"><span>Modeling Coronal Response in Decaying Active Regions with Magnetic <span class="hlt">Flux</span> Transport and Steady <span class="hlt">Heating</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ugarte-Urra, Ignacio; Warren, Harry P.; Upton, Lisa A.; Young, Peter R.</p> <p>2017-09-01</p> <p>We present new measurements of the dependence of the extreme ultraviolet (EUV) radiance on the total magnetic <span class="hlt">flux</span> in active regions as obtained from the Atmospheric Imaging Assembly (AIA) and the Helioseismic and Magnetic Imager on board the Solar Dynamics Observatory. Using observations of nine active regions tracked along different stages of evolution, we extend the known radiance—magnetic <span class="hlt">flux</span> power-law relationship (I\\propto {{{Φ }}}α ) to the AIA 335 Å passband, and the Fe xviii 93.93 Å spectral line in the 94 Å passband. We find that the total unsigned magnetic <span class="hlt">flux</span> divided by the polarity separation ({{Φ }}/D) is a better indicator of radiance for the Fe xviii line with a slope of α =3.22+/- 0.03. We then use these results to test our current understanding of magnetic <span class="hlt">flux</span> evolution and coronal <span class="hlt">heating</span>. We use magnetograms from the simulated decay of these active regions produced by the Advective <span class="hlt">Flux</span> Transport model as boundary conditions for potential extrapolations of the magnetic field in the corona. We then model the hydrodynamics of each individual field line with the Enthalpy-based Thermal Evolution of Loops model with steady <span class="hlt">heating</span> scaled as the ratio of the average field strength and the length (\\bar{B}/L) and render the Fe xviii and 335 Å emission. We find that steady <span class="hlt">heating</span> is able to partially reproduce the magnitudes and slopes of the EUV radiance—magnetic <span class="hlt">flux</span> relationships and discuss how impulsive <span class="hlt">heating</span> can help reconcile the discrepancies. This study demonstrates that combined models of magnetic <span class="hlt">flux</span> transport, magnetic topology, and <span class="hlt">heating</span> can yield realistic estimates for the decay of active region radiances with time.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018HMT....54..985A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018HMT....54..985A"><span>Thermal performance analysis of a flat <span class="hlt">heat</span> pipe working with carbon nanotube-water nanofluid for cooling of a high <span class="hlt">heat</span> <span class="hlt">flux</span> heater</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Arya, A.; Sarafraz, M. M.; Shahmiri, S.; Madani, S. A. H.; Nikkhah, V.; Nakhjavani, S. M.</p> <p>2018-04-01</p> <p>Experimental investigation on the thermal performance of a flat <span class="hlt">heat</span> pipe working with carbon nanotube nanofluid is conducted. It is used for cooling a heater working at high <span class="hlt">heat</span> <span class="hlt">flux</span> conditions up to 190 kW/m2. The <span class="hlt">heat</span> pipe is fabricated from aluminium and is equipped with rectangular fin for efficient cooling of condenser section. Inside the <span class="hlt">heat</span> pipe, a screen mesh was inserted as a wick structure to facilitate the capillary action of working fluid. Influence of different operating parameters such as <span class="hlt">heat</span> <span class="hlt">flux</span>, mass concentration of carbon nanotubes and filling ratio of working fluid on thermal performance of <span class="hlt">heat</span> pipe and its thermal resistance are investigated. Results showed that with an increase in <span class="hlt">heat</span> <span class="hlt">flux</span>, the <span class="hlt">heat</span> transfer coefficient in evaporator section of the <span class="hlt">heat</span> pipe increases. For filling ratio, however, there is an optimum value, which was 0.8 for the test <span class="hlt">heat</span> pipe. In addition, CNT/water enhanced the <span class="hlt">heat</span> transfer coefficient up to 40% over the deionized water. Carbon nanotubes intensified the thermal performance of wick structure by creating a fouling layer on screen mesh structure, which changes the contact angle of liquid with the surface, intensifying the capillary forces.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19980206267','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19980206267"><span>Experimental Performance of a Micromachined <span class="hlt">Heat</span> <span class="hlt">Flux</span> Sensor</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Stefanescu, S.; DeAnna, R. G.; Mehregany, M.</p> <p>1998-01-01</p> <p>Steady-state and frequency response calibration of a microfabricated <span class="hlt">heat-flux</span> sensor have been completed. This sensor is batch fabricated using standard, micromachining techniques, allowing both miniaturization and the ability to create arrays of sensors and their corresponding interconnects. Both high-frequency and spatial response is desired, so the sensors are both thin and of small cross-sectional area. Thin-film, temperature-sensitive resistors are used as the active gauge elements. Two sensor configurations are investigated: (1) a Wheatstone-bridge using four resistors; and (2) a simple, two-resistor design. In each design, one resistor (or pair) is covered by a thin layer (5000 A) thermal barrier; the other resistor (or pair) is covered by a thick (5 microns) thermal barrier. The active area of a single resistor is 360 microns by 360 microns; the total gauge area is 1.5 mm square. The resistors are made of 2000 A-thick metal; and the entire gauge is fabricated on a 25 microns-thick flexible, polyimide substrate. <span class="hlt">Heat</span> <span class="hlt">flux</span> through the surface changes the temperature of the resistors and produces a corresponding change in resistance. Sensors were calibrated using two radiation <span class="hlt">heat</span> sources: (1) a furnace for steady-state, and (2) a light and chopper for frequency response.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20120002868','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20120002868"><span>Characterization of Turbulent Latent and Sensible <span class="hlt">Heat</span> <span class="hlt">Flux</span> Exchange Between the Atmosphere and Ocean in MERRA</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Robert, J. Brent; Robertson, Franklin R.; Clayson, Carol Anne; Bosilovich, Michael G.</p> <p>2012-01-01</p> <p>Turbulent <span class="hlt">fluxes</span> of <span class="hlt">heat</span> and moisture across the atmosphere-ocean interface are fundamental components of the Earth's energy and water balance. Characterizing both the spatiotemporal variability and the fidelity of these exchanges of <span class="hlt">heat</span> and moisture is critical to understanding the global water and energy cycle variations, quantifying atmosphere-ocean feedbacks, and improving model predictability. This study examines the veracity of the recently completed NASA Modern-Era Retrospective analysis for Research and Applications (MERRA) product with respect to its representation of the surface turbulent <span class="hlt">heat</span> <span class="hlt">fluxes</span>. A validation of MERRA turbulent <span class="hlt">heat</span> <span class="hlt">fluxes</span> and near-surface bulk variables at local, high-resolution space and time scales is achieved by making comparisons to a large suite of direct observations. Both in situ and satellite-observed gridded surface <span class="hlt">heat</span> <span class="hlt">flux</span> estimates are employed to investigate the spatial and temporal variability of the surface <span class="hlt">fluxes</span> with respect to their annual mean climatologies, their seasonal covariability of near-surface bulk parameters, and their representation of extremes. The impact of data assimilation on the near-surface parameters is assessed through evaluation of incremental analysis update tendencies produced by the assimilation procedure. It is found that MERRA turbulent surface <span class="hlt">heat</span> <span class="hlt">fluxes</span> are relatively accurate for typical conditions but have systematically weak vertical gradients in moisture and temperature and have a weaker covariability between the near-surface gradients and wind speed than found in observations. This results in an underestimate of the surface latent and sensible <span class="hlt">heat</span> <span class="hlt">fluxes</span> over the western boundary current and storm track regions. The assimilation of observations mostly acts to bring MERRA closer to observational products by increasing moisture and temperature near the surface and decreasing the near-surface wind speeds. The major patterns of spatial and temporal variability of the turbulent <span class="hlt">heat</span></p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20120007430','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20120007430"><span>Characterization of Turbulent Latent and Sensible <span class="hlt">Heat</span> <span class="hlt">Flux</span> Exchange Between the Atmosphere and Ocean in MERRA</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Roberts, J. Brent; Robertson, Franklin R.; Clayson, Carol Anne; Bosilovich, Michael G.</p> <p>2012-01-01</p> <p>Turbulent <span class="hlt">fluxes</span> of <span class="hlt">heat</span> and moisture across the atmosphere-ocean interface are fundamental components of the Earth s energy and water balance. Characterizing both the spatiotemporal variability and the fidelity of these exchanges of <span class="hlt">heat</span> and moisture is critical to understanding the global water and energy cycle variations, quantifying atmosphere-ocean feedbacks, and improving model predictability. This study examines the veracity of the recently completed NASA Modern-Era Retrospective analysis for Research and Applications (MERRA) product with respect to its representation of the surface turbulent <span class="hlt">heat</span> <span class="hlt">fluxes</span>. A validation of MERRA turbulent <span class="hlt">heat</span> <span class="hlt">fluxes</span> and near-surface bulk variables at local, high-resolution space and time scales is achieved by making comparisons to a large suite of direct observations. Both in situ and satellite-observed gridded surface <span class="hlt">heat</span> <span class="hlt">flux</span> estimates are employed to investigate the spatial and temporal variability of the surface <span class="hlt">fluxes</span> with respect to their annual mean climatologies, their seasonal covariability of near-surface bulk parameters, and their representation of extremes. The impact of data assimilation on the near-surface parameters is assessed through evaluation of incremental analysis update tendencies produced by the assimilation procedure. It is found that MERRA turbulent surface <span class="hlt">heat</span> <span class="hlt">fluxes</span> are relatively accurate for typical conditions but have systematically weak vertical gradients in moisture and temperature and have a weaker covariability between the near-surface gradients and wind speed than found in observations. This results in an underestimate of the surface latent and sensible <span class="hlt">heat</span> <span class="hlt">fluxes</span> over the western boundary current and storm track regions. The assimilation of observations mostly acts to bring MERRA closer to observational products by increasing moisture and temperature near the surface and decreasing the near-surface wind speeds. The major patterns of spatial and temporal variability of the turbulent <span class="hlt">heat</span></p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1990PhDT........67B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1990PhDT........67B"><span><span class="hlt">Heat</span> Deposition and <span class="hlt">Heat</span> Removal in the UCLA Continuous Current Tokamak</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Brown, Michael Lee</p> <p>1990-01-01</p> <p>Energy transfer processes in a steady-state tokamak are examined both theoretically and experimentally in order to determine the patterns of plasma <span class="hlt">heat</span> deposition to material surfaces and the methods of <span class="hlt">heat</span> removal. <span class="hlt">Heat</span> transfer experiments involving actively cooled limiters and <span class="hlt">heat</span> <span class="hlt">flux</span> probes were performed in the UCLA Continuous Current Tokamak (CCT). The simple exponential model of plasma power deposition was extended to describe the global <span class="hlt">heat</span> deposition to the first <span class="hlt">wall</span> of a steady-state tokamak. The <span class="hlt">heat</span> <span class="hlt">flux</span> distribution in CCT was determined from measurements of <span class="hlt">heat</span> flow to 32 large-area water-cooled Faraday shield panels. Significant toroidal and poloidal asymmetries were observed, with the maximum <span class="hlt">heat</span> <span class="hlt">fluxes</span> tending to fall on the lower outside panels. <span class="hlt">Heat</span> deposition to the water-cooled guard limiters of an ion Bernstein wave antenna in CCT was measured during steady-state operation. Very strong asymmetries were observed. The <span class="hlt">heat</span> distribution varied greatly with magnetic field. Copper <span class="hlt">heat</span> <span class="hlt">flux</span> sensors incorporating internal thermocouples were developed to measure plasma power deposition to exterior probe surfaces and <span class="hlt">heat</span> removal from water -cooled interior surfaces. The resulting inverse <span class="hlt">heat</span> conduction problem was solved using the function specification method. Cooling by an impinging liquid jet was investigated. One end of a cylindrical copper <span class="hlt">heat</span> <span class="hlt">flux</span> sensor was <span class="hlt">heated</span> by a DC electrical arc and the other end was cooled by a low velocity water jet at 1 atm. Critical <span class="hlt">heat</span> <span class="hlt">flux</span> (CHF) values for the 55-80 ^circC sub-cooled free jets were typically 2.5 times published values for saturated free jets. For constrained jets, CHF values were about 20% lower. <span class="hlt">Heat</span> deposition and <span class="hlt">heat</span> removal in thick (3/4 inch diameter) cylindrical metal probes (SS304 or copper) inserted into a steady-state tokamak plasma were measured for a broad range of <span class="hlt">heat</span> loads. The probes were cooled internally by a constrained jet of either air or water. Steady -state <span class="hlt">heat</span></p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1214444-modeling-effect-lithium-induced-pedestal-profiles-scrape-off-layer-turbulence-heat-flux-width','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1214444-modeling-effect-lithium-induced-pedestal-profiles-scrape-off-layer-turbulence-heat-flux-width"><span>Modeling the effect of lithium-induced pedestal profiles on scrape-off-layer turbulence and the <span class="hlt">heat</span> <span class="hlt">flux</span> width</span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Russell, David A.; D'Ippolito, Daniel A.; Myra, James R.; ...</p> <p>2015-09-01</p> <p>The effect of lithium (Li) <span class="hlt">wall</span> coatings on scrape-off-layer (SOL) turbulence in the National Spherical Torus Experiment (NSTX) is modeled with the Lodestar SOLT (“SOL Turbulence”) code. Specifically, the implications for the SOL <span class="hlt">heat</span> <span class="hlt">flux</span> width of experimentally observed, Li-induced changes in the pedestal profiles are considered. The SOLT code used in the modeling has been expanded recently to include ion temperature evolution and ion diamagnetic drift effects. This work focuses on two NSTX discharges occurring pre- and with-Li deposition. The simulation density and temperature profiles are constrained, inside the last closed <span class="hlt">flux</span> surface only, to match those measured inmore » the two experiments, and the resulting drift-interchange-driven turbulence is explored. The effect of Li enters the simulation only through the pedestal profile constraint: Li modifies the experimental density and temperature profiles in the pedestal, and these profiles affect the simulated SOL turbulence. The power entering the SOL measured in the experiments is matched in the simulations by adjusting “free” dissipation parameters (e.g., diffusion coefficients) that are not measured directly in the experiments. With power-matching, (a) the <span class="hlt">heat</span> <span class="hlt">flux</span> SOL width is smaller, as observed experimentally by infra-red thermography, and (b) the simulated density fluctuation amplitudes are reduced with Li, as inferred for the experiments as well from reflectometry analysis. The instabilities and saturation mechanisms that underlie the SOLT model equilibria are also discussed.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2007APS..DPPBI1005S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2007APS..DPPBI1005S"><span>Divertor <span class="hlt">Heat</span> <span class="hlt">Flux</span> Reduction and Detachment in the National Spherical Torus eXperiment.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Soukhanovskii, Vsevolod</p> <p>2007-11-01</p> <p>Steady-state handling of the <span class="hlt">heat</span> <span class="hlt">flux</span> is a critical divertor issue for both the International Thermonuclear Experimental Reactor and spherical torus (ST) devices. Because of an inherently compact divertor, it was thought that ST-based devices might not be able to fully utilize radiative and dissipative divertor techniques based on induced power and momentum loss. However, initial experiments conducted in the National Spherical Torus Experiment in an open geometry horizontal carbon plate divertor using 0.8 MA 2-6 MW NBI-<span class="hlt">heated</span> lower single null H-mode plasmas at the lower end of elongations κ=1.8-2.4 and triangularities δ=0.45-0.75 demonstrated that high divertor peak <span class="hlt">heat</span> <span class="hlt">fluxes</span>, up to 6-10 MW/ m^2, could be reduced by 50-75% using a high-recycling radiative divertor regime with D2 injection. Furthermore, similar reduction was obtained with a partially detached divertor (PDD) at high D2 injection rates, however, it was accompanied by an X-point MARFE that quickly led to confinement degradation. Another approach takes advantage of the ST relation between strong shaping and high performance, and utilizes the poloidal magnetic <span class="hlt">flux</span> expansion in the divertor region. Up to 60 % reduction in divertor peak <span class="hlt">heat</span> <span class="hlt">flux</span> was achieved at similar levels of scrape-off layer power by varying plasma shaping and thereby increasing the outer strike point (OSP) poloidal <span class="hlt">flux</span> expansion from 4-6 to 18-22. In recent experiments conducted in highly-shaped 1.0-1.2 MA 6 MW NBI <span class="hlt">heated</span> H-mode plasmas with divertor D2 injection at rates up to 10^22 s-1, a PDD regime with OSP peak <span class="hlt">heat</span> <span class="hlt">flux</span> 0.5-1.5 MW/m^2 was obtained without noticeable confinement degradation. Calculations based on a two point scrape-off layer model with parameterized power and momentum losses show that the short parallel connection length at the OSP sets the upper limit on the radiative exhaust channel, and both the impurity radiation and large momentum sink achievable only at high divertor neutral pressures are required</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20160007555','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20160007555"><span>Comparison of <span class="hlt">Heat</span> <span class="hlt">Flux</span> Gages for High Enthalpy Flows - NASA Ames and IRS</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Loehle, Stefan; Nawaz, Anuscheh; Herdrich, Georg; Fasoulas, Stefanos; Martinez, Edward; Raiche, George</p> <p>2016-01-01</p> <p>This article is a companion to a paper on <span class="hlt">heat</span> <span class="hlt">flux</span> measurements as initiated under a Space Act Agreement in 2011. The current focus of this collaboration between the Institute of Space Systems (IRS) of the University of Stuttgart and NASA Ames Research Center is the comparison and refinement of diagnostic measurements. A first experimental campaign to test different <span class="hlt">heat</span> <span class="hlt">flux</span> gages in the NASA Interaction <span class="hlt">Heating</span> Facility (IHF) and the Plasmawindkanaele (PWK) at IRS was established. This paper focuses on the results of the measurements conducted at IRS. The tested gages included a at face and hemispherical probe head, a 4" hemispherical slug calorimeter, a null-point calorimeter from Ames and a null-point calorimeter developed for this purpose at IRS. The Ames null-point calorimeter was unfortunately defective upon arrival. The measured <span class="hlt">heat</span> <span class="hlt">fluxes</span> agree fairly well with each other. The reason for discrepancies can be attributed to signal-to-noise levels and the probe geometry.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012AIPC.1448..242P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012AIPC.1448..242P"><span>Experimental study on the <span class="hlt">heat</span> transfer characteristics of a nuclear reactor containment <span class="hlt">wall</span> cooled by gravitationally falling water</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Pasek, Ari D.; Umar, Efrison; Suwono, Aryadi; Manalu, Reinhard E. E.</p> <p>2012-06-01</p> <p>Gravitationally falling water cooling is one of mechanism utilized by a modern nuclear Pressurized Water Reactor (PWR) for its Passive Containment Cooling System (PCCS). Since the cooling is closely related to the safety, water film cooling characteristics of the PCCS should be studied. This paper deals with the experimental study of laminar water film cooling on the containment model <span class="hlt">wall</span>. The influences of water mass flow rate and <span class="hlt">wall</span> <span class="hlt">heat</span> rate on the <span class="hlt">heat</span> transfer characteristic were studied. This research was started with design and assembly of a containment model equipped with the water cooling system, and calibration of all measurement devices. The containment model is a scaled down model of AP 1000 reactor. Below the containment steam is generated using electrical heaters. The steam <span class="hlt">heated</span> the containment <span class="hlt">wall</span>, and then the temperatures of the <span class="hlt">wall</span> in several positions were measure transiently using thermocouples and data acquisition. The containment was then cooled by falling water sprayed from the top of the containment. The experiments were done for various <span class="hlt">wall</span> <span class="hlt">heat</span> rate and cooling water flow rate. The objective of the research is to find the temperature profile along the <span class="hlt">wall</span> before and after the water cooling applied, prediction of the water film characteristic such as means velocity, thickness and their influence to the <span class="hlt">heat</span> transfer coefficient. The result of the experiments shows that the <span class="hlt">wall</span> temperatures significantly drop after being sprayed with water. The thickness of water film increases with increasing water flow rate and remained constant with increasing <span class="hlt">wall</span> <span class="hlt">heat</span> rate. The <span class="hlt">heat</span> transfer coefficient decreases as film mass flow rate increase due to the increases of the film thickness which causes the increasing of the thermal resistance. The <span class="hlt">heat</span> transfer coefficient increases slightly as the <span class="hlt">wall</span> <span class="hlt">heat</span> rate increases. The experimental results were then compared with previous theoretical studied.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/CFR-2010-title16-vol2/pdf/CFR-2010-title16-vol2-part1209-subpartA-app8.pdf','CFR'); return false;" href="https://www.gpo.gov/fdsys/pkg/CFR-2010-title16-vol2/pdf/CFR-2010-title16-vol2-part1209-subpartA-app8.pdf"><span>16 CFR Figure 8 to Subpart A of... - Standard Radiant <span class="hlt">Heat</span> Energy <span class="hlt">Flux</span> Profile</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>... 16 Commercial Practices 2 2010-01-01 2010-01-01 false Standard Radiant <span class="hlt">Heat</span> Energy <span class="hlt">Flux</span> Profile 8... PRODUCT SAFETY ACT REGULATIONS INTERIM SAFETY STANDARD FOR CELLULOSE INSULATION The Standard Pt. 1209, Subpt. A, Fig. 8 Figure 8 to Subpart A of Part 1209—Standard Radiant <span class="hlt">Heat</span> Energy <span class="hlt">Flux</span> Profile EC03OC91...</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://www.gpo.gov/fdsys/pkg/CFR-2011-title16-vol2/pdf/CFR-2011-title16-vol2-part1209-subpartA-app8.pdf','CFR2011'); return false;" href="https://www.gpo.gov/fdsys/pkg/CFR-2011-title16-vol2/pdf/CFR-2011-title16-vol2-part1209-subpartA-app8.pdf"><span>16 CFR Figure 8 to Subpart A of... - Standard Radiant <span class="hlt">Heat</span> Energy <span class="hlt">Flux</span> Profile</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>... 16 Commercial Practices 2 2011-01-01 2011-01-01 false Standard Radiant <span class="hlt">Heat</span> Energy <span class="hlt">Flux</span> Profile 8... PRODUCT SAFETY ACT REGULATIONS INTERIM SAFETY STANDARD FOR CELLULOSE INSULATION The Standard Pt. 1209, Subpt. A, Fig. 8 Figure 8 to Subpart A of Part 1209—Standard Radiant <span class="hlt">Heat</span> Energy <span class="hlt">Flux</span> Profile EC03OC91...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/CFR-2013-title16-vol2/pdf/CFR-2013-title16-vol2-part1209-subpartA-app8.pdf','CFR2013'); return false;" href="https://www.gpo.gov/fdsys/pkg/CFR-2013-title16-vol2/pdf/CFR-2013-title16-vol2-part1209-subpartA-app8.pdf"><span>16 CFR Figure 8 to Subpart A of... - Standard Radiant <span class="hlt">Heat</span> Energy <span class="hlt">Flux</span> Profile</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>... 16 Commercial Practices 2 2013-01-01 2013-01-01 false Standard Radiant <span class="hlt">Heat</span> Energy <span class="hlt">Flux</span> Profile 8... PRODUCT SAFETY ACT REGULATIONS INTERIM SAFETY STANDARD FOR CELLULOSE INSULATION The Standard Pt. 1209, Subpt. A, Fig. 8 Figure 8 to Subpart A of Part 1209—Standard Radiant <span class="hlt">Heat</span> Energy <span class="hlt">Flux</span> Profile EC03OC91...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/CFR-2012-title16-vol2/pdf/CFR-2012-title16-vol2-part1209-subpartA-app8.pdf','CFR2012'); return false;" href="https://www.gpo.gov/fdsys/pkg/CFR-2012-title16-vol2/pdf/CFR-2012-title16-vol2-part1209-subpartA-app8.pdf"><span>16 CFR Figure 8 to Subpart A of... - Standard Radiant <span class="hlt">Heat</span> Energy <span class="hlt">Flux</span> Profile</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>... 16 Commercial Practices 2 2012-01-01 2012-01-01 false Standard Radiant <span class="hlt">Heat</span> Energy <span class="hlt">Flux</span> Profile 8... PRODUCT SAFETY ACT REGULATIONS INTERIM SAFETY STANDARD FOR CELLULOSE INSULATION The Standard Pt. 1209, Subpt. A, Fig. 8 Figure 8 to Subpart A of Part 1209—Standard Radiant <span class="hlt">Heat</span> Energy <span class="hlt">Flux</span> Profile EC03OC91...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/CFR-2014-title16-vol2/pdf/CFR-2014-title16-vol2-part1209-subpartA-app8.pdf','CFR2014'); return false;" href="https://www.gpo.gov/fdsys/pkg/CFR-2014-title16-vol2/pdf/CFR-2014-title16-vol2-part1209-subpartA-app8.pdf"><span>16 CFR Figure 8 to Subpart A of... - Standard Radiant <span class="hlt">Heat</span> Energy <span class="hlt">Flux</span> Profile</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>... 16 Commercial Practices 2 2014-01-01 2014-01-01 false Standard Radiant <span class="hlt">Heat</span> Energy <span class="hlt">Flux</span> Profile 8... PRODUCT SAFETY ACT REGULATIONS INTERIM SAFETY STANDARD FOR CELLULOSE INSULATION The Standard Pt. 1209, Subpt. A, Fig. 8 Figure 8 to Subpart A of Part 1209—Standard Radiant <span class="hlt">Heat</span> Energy <span class="hlt">Flux</span> Profile EC03OC91...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20000056863','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20000056863"><span>Critical <span class="hlt">Heat</span> <span class="hlt">Flux</span> in Pool Boiling on Metal-Graphite Composite Surfaces</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Zhang, Nengli; Yang, Wen-Jei; Chao, David F.; Chao, David F. (Technical Monitor)</p> <p>2000-01-01</p> <p>A study is conducted on high <span class="hlt">heat-flux</span> pool boiling of pentane on micro-configured composite surfaces. The boiling surfaces are copper-graphite (Cu-Gr) and aluminum-graphite (Al-Gr) composites with a fiber volume concentration of 50%. The micro-graphite fibers embedded in the matrix contribute to a substantial enhancement in boiling <span class="hlt">heat</span>-transfer performance. Correlation equations are obtained for both the isolated and coalesced bubble regimes, utilizing a mathematical model based on a metal-graphite, two-tier configuration with the aid of experimental data. A new model to predict the critical <span class="hlt">heat</span> <span class="hlt">flux</span> (CHF) on the composites is proposed to explain the fundamental aspects of the boiling phenomena. Three different factors affecting the CHF are considered in the model. Two of them are expected to become the main agents driving vapor volume detachment under microgravity conditions, using the metal-graphite composite surfaces as the <span class="hlt">heating</span> surface and using liquids with an unusual Marangoni effect as the working fluid.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2000BoLMe..95..271O','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2000BoLMe..95..271O"><span>Stability Effects on <span class="hlt">Heat</span> and Moisture <span class="hlt">Fluxes</span> at Sea</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Oost, W. A.; Jacobs, C. M. J.; van Oort, C.</p> <p></p> <p>During the 1996 ASGAMAGE experiment we measured windspeed, air temperature Ta, watertemperature Ts, humidity and the momentum,<span class="hlt">heat</span> and moisture <span class="hlt">fluxes</span> at a research platform offthe Dutch coast. For each quantity we used several(sets of) instruments simultaneously. This allowed usto make an extensive assessment of the quality of themeasurements and to find optimal values for thevarious quantities for each run. From these values wecalculated CH and CE, theStanton and Dalton numbers, and reduced them to 10-mheight and neutral conditions. For this reductionwe made a separate analysis for the effect ofinclusion or non-inclusion of the assumption that theroughness length for <span class="hlt">heat</span> or moisture is the same forthe neutral and non-neutral cases. Differences inthe reduced data due to this assumption turned out tobe well within the measurement error.For CH we distinguished three separategroups of data: stable (A), unstable witha s (B) and unstablewith thetas;a > s (C), with indicating the potential temperature.The stable data separate into two groups, depending onwater temperature and/or the wave field. The data ofgroup B showed a relation with wave age. The data ofgroup C consistently gave negative values forCH, a result that might indicate conversion oflatent <span class="hlt">heat</span> into sensible <span class="hlt">heat</span> through condensation ofwater vapour just above the water surface. An attemptto re-analyse the data in terms of density <span class="hlt">fluxes</span>,combining the effects of <span class="hlt">heat</span> and moisture, still gavenegative transfer coefficients for group C.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1999PhDT.......232H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1999PhDT.......232H"><span>Critical <span class="hlt">heat</span> <span class="hlt">flux</span> in subcooled flow boiling</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hall, David Douglas</p> <p></p> <p>The critical <span class="hlt">heat</span> <span class="hlt">flux</span> (CHF) phenomenon was investigated for water flow in tubes with particular emphasis on the development of methods for predicting CHF in the subcooled flow boiling regime. The Purdue University Boiling and Two-Phase Flow Laboratory (PU-BTPFL) CHF database for water flow in a uniformly <span class="hlt">heated</span> tube was compiled from the world literature dating back to 1949 and represents the largest CHF database ever assembled with 32,544 data points from over 100 sources. The superiority of this database was proven via a detailed examination of previous databases. The PU-BTPFL CHF database is an invaluable tool for the development of CHF correlations and mechanistic models that are superior to existing ones developed with smaller, less comprehensive CHF databases. In response to the many inaccurate and inordinately complex correlations, two nondimensional, subcooled CHF correlations were formulated, containing only five adjustable constants and whose unique functional forms were determined without using a statistical analysis but rather using the parametric trends observed in less than 10% of the subcooled CHF data. The correlation based on inlet conditions (diameter, <span class="hlt">heated</span> length, mass velocity, pressure, inlet quality) was by far the most accurate of all known subcooled CHF correlations, having mean absolute and root-mean-square (RMS) errors of 10.3% and 14.3%, respectively. The outlet (local) conditions correlation was the most accurate correlation based on local CHF conditions (diameter, mass velocity, pressure, outlet quality) and may be used with a nonuniform axial <span class="hlt">heat</span> <span class="hlt">flux</span>. Both correlations proved more accurate than a recent CHF look-up table commonly employed in nuclear reactor thermal hydraulic computer codes. An interfacial lift-off, subcooled CHF model was developed from a consideration of the instability of the vapor-liquid interface and the fraction of <span class="hlt">heat</span> required for liquid-vapor conversion as opposed to that for bulk liquid <span class="hlt">heating</span>. Severe</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JGRC..122.4068S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JGRC..122.4068S"><span>Air-sea <span class="hlt">heat</span> <span class="hlt">flux</span> climatologies in the Mediterranean Sea: Surface energy balance and its consistency with ocean <span class="hlt">heat</span> storage</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Song, Xiangzhou; Yu, Lisan</p> <p>2017-05-01</p> <p>This study provides an analysis of the Mediterranean Sea surface energy budget using nine surface <span class="hlt">heat</span> <span class="hlt">flux</span> climatologies. The ensemble mean estimation shows that the net downward shortwave radiation (192 ± 19 W m-2) is balanced by latent <span class="hlt">heat</span> <span class="hlt">flux</span> (-98 ± 10 W m-2), followed by net longwave radiation (-78 ± 13 W m-2) and sensible <span class="hlt">heat</span> <span class="hlt">flux</span> (-13 ± 4 W m-2). The resulting net <span class="hlt">heat</span> budget (Qnet) is 2 ± 12 W m-2 into the ocean, which appears to be warm biased. The annual-mean Qnet should be -5.6 ± 1.6 W m-2 when estimated from the observed net transport through the Strait of Gibraltar. To diagnose the uncertainty in nine Qnet climatologies, we constructed Qnet from the <span class="hlt">heat</span> budget equation by using historic hydrological observations to determine the <span class="hlt">heat</span> content changes and advective <span class="hlt">heat</span> <span class="hlt">flux</span>. We also used the Qnet from a data-assimilated global ocean state estimation as an additional reference. By comparing with the two reference Qnet estimates, we found that seven products (NCEP 1, NCEP 2, CFSR, ERA-Interim, MERRA, NOCSv2.0, and OAFlux+ISCCP) overestimate Qnet, with magnitude ranging from 6 to 27 W m-2, while two products underestimate Qnet by -6 W m-2 (JRA55) and -14 W m-2 (CORE.2). Together with the previous warm pool work of Song and Yu (2013), we show that CFSR, MERRA, NOCSv2.0, and OAFlux+ISCCP are warm-biased not only in the western Pacific warm pool but also in the Mediterranean Sea, while CORE.2 is cold-biased in both regions. The NCEP 1, 2, and ERA-Interim are cold-biased over the warm pool but warm-biased in the Mediterranean Sea.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.fs.usda.gov/treesearch/pubs/5978','TREESEARCH'); return false;" href="https://www.fs.usda.gov/treesearch/pubs/5978"><span>Charring rate of wood exposed to a constant <span class="hlt">heat</span> <span class="hlt">flux</span></span></a></p> <p><a target="_blank" href="http://www.fs.usda.gov/treesearch/">Treesearch</a></p> <p>R. H. White; H. C. Tran</p> <p>1996-01-01</p> <p>A critical factor in the fire endurance of a wood member is its rate of charring. Most available charring rate data have been obtained using the time-temperature curves of the standard fire resistance tests (ASTM E 119 and ISO 834) to define the fire exposure. The increased use of <span class="hlt">heat</span> release calorimeters using exposures of constant <span class="hlt">heat</span> <span class="hlt">flux</span> levels has broadened the...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/1038927-heat-flux-analysis-reacting-thermite-spray-impingent-substrate','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/1038927-heat-flux-analysis-reacting-thermite-spray-impingent-substrate"><span><span class="hlt">Heat</span> <span class="hlt">Flux</span> Analysis of a Reacting Thermite Spray Impingent on a Substrate</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>Eric S. Collins; Michelle L. Pantoya; Michael A. Daniels</p> <p>2012-03-01</p> <p>Spray combustion from a thermite reaction is a new area of research relevant to localized energy generation applications, such as welding or cutting. In this study, we characterized the <span class="hlt">heat</span> <span class="hlt">flux</span> of combustion spray impinging on a target from a nozzle for three thermite mixtures. The reactions studied include aluminum (Al) with iron oxide (Fe2O3), Al with copper oxide (CuO), and Al with molybdenum oxide (MoO3). Several standoff distances (i.e., distance from the nozzle exit to the target) were analyzed. A fast response <span class="hlt">heat</span> <span class="hlt">flux</span> sensor was engineered for this purpose and is discussed in detail. Results correlated substrate damagemore » to a threshold <span class="hlt">heat</span> <span class="hlt">flux</span> of 4550 W/cm2 for a fixed-nozzle configuration. Also, higher gas-generating thermites were shown to produce a widely dispersed spray and be less effective at imparting kinetic energy damage to a target. These results provide an understanding of the role of thermal and physical properties (i.e., such as <span class="hlt">heat</span> of combustion, gas generation, and particle size) on thermite spray combustion performance measured by damaging a target substrate.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015PhRvE..92e3006K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015PhRvE..92e3006K"><span><span class="hlt">Heat</span> transfer enhancement induced by <span class="hlt">wall</span> inclination in turbulent thermal convection</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kenjereš, Saša</p> <p>2015-11-01</p> <p>We present a series of numerical simulations of turbulent thermal convection of air in an intermediate range or Rayleigh numbers (106≤Ra ≤109 ) with different configurations of a thermally active lower surface. The geometry of the lower surface is designed in such a way that it represents a simplified version of a mountain slope with different inclinations (i.e., "Λ "- and "V "-shaped geometry). We find that different <span class="hlt">wall</span> inclinations significantly affect the local <span class="hlt">heat</span> transfer by imposing local clustering of instantaneous thermal plumes along the inclination peaks. The present results reveal that significant enhancement of the integral <span class="hlt">heat</span> transfer can be obtained (up to 32%) when compared to a standard Rayleigh-Bénard configuration with flat horizontal <span class="hlt">walls</span>. This is achieved through combined effects of the enlargement of the <span class="hlt">heated</span> surface and reorganization of the large-scale flow structures.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1353402-error-field-measurement-correction-heat-flux-balancing-wendelstein','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1353402-error-field-measurement-correction-heat-flux-balancing-wendelstein"><span>Error field measurement, correction and <span class="hlt">heat</span> <span class="hlt">flux</span> balancing on Wendelstein 7-X</span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Lazerson, Samuel A.; Otte, Matthias; Jakubowski, Marcin; ...</p> <p>2017-03-10</p> <p>The measurement and correction of error fields in Wendelstein 7-X (W7-X) is critical to long pulse high beta operation, as small error fields may cause overloading of divertor plates in some configurations. Accordingly, as part of a broad collaborative effort, the detection and correction of error fields on the W7-X experiment has been performed using the trim coil system in conjunction with the <span class="hlt">flux</span> surface mapping diagnostic and high resolution infrared camera. In the early commissioning phase of the experiment, the trim coils were used to open an n/m = 1/2 island chain in a specially designed magnetic configuration. Themore » <span class="hlt">flux</span> surfacing mapping diagnostic was then able to directly image the magnetic topology of the experiment, allowing the inference of a small similar to 4 cm intrinsic island chain. The suspected main sources of the error field, slight misalignment and deformations of the superconducting coils, are then confirmed through experimental modeling using the detailed measurements of the coil positions. Observations of the limiters temperatures in module 5 shows a clear dependence of the limiter <span class="hlt">heat</span> <span class="hlt">flux</span> pattern as the perturbing fields are rotated. Plasma experiments without applied correcting fields show a significant asymmetry in neutral pressure (centered in module 4) and light emission (visible, H-alpha, CII, and CIII). Such pressure asymmetry is associated with plasma-<span class="hlt">wall</span> (limiter) interaction asymmetries between the modules. Application of trim coil fields with n = 1 waveform correct the imbalance. Confirmation of the error fields allows the assessment of magnetic fields which resonate with the n/m = 5/5 island chain.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1984PhFl...27.1545M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1984PhFl...27.1545M"><span>Plasma <span class="hlt">wall</span> sheath contributions to <span class="hlt">flux</span> retention during the formation of field-reversed configurations</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Milroy, R. D.; Slough, J. T.; Hoffman, A. L.</p> <p>1984-06-01</p> <p><span class="hlt">Flux</span> loss during field reversal on the TRX-1 field-reversed θ pinch is found to be much less than predicted by the inertial model of Green and Newton. This can be explained by a pressure bearing, conducting sheath which naturally forms at the <span class="hlt">wall</span> and limits the <span class="hlt">flux</span> loss. A one-dimensional (r-t) magnetohydrodynamic (MHD) numerical model has been used to study the formation and effectiveness of the sheath. The calculations are in excellent agreement with experimental measurements over a wide range of operating parameters. The results indicate that good <span class="hlt">flux</span> trapping can be achieved through the field reversal phase of FRC formation with much slower external field reversal rates than in current experiments.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19990008950','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19990008950"><span>Remote <span class="hlt">Heat</span> <span class="hlt">Flux</span> Using a Self Calibration Multiwavelength Pyrometer and a Transparent Material</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Ng, Daniel</p> <p>1998-01-01</p> <p>A self calibrating multiwavelength pyrometer was used to conduct remote <span class="hlt">heat</span> <span class="hlt">flux</span> measurements using a transparent sapphire disk by determining the sapphire disk's front and back surface temperatures. Front surface temperature (Tfs) was obtained from detection of surface emitted radiation at long wavelengths (k = 6 gm). Back surface temperature (Tbs) was obtained from short wavelength (1 to 5 gm) radiation transmitted through the sapphire disk. The thermal conductivity of the sapphire disk and the <span class="hlt">heat</span> transfer coefficients h, and h2 of its surfaces are determined experimentally. An analysis of the <span class="hlt">heat</span> <span class="hlt">flux</span> measurement is presented.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011WRR....47.5545M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011WRR....47.5545M"><span>Estimation of evaporation and sensible <span class="hlt">heat</span> <span class="hlt">flux</span> from open water using a large-aperture scintillometer</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>McJannet, D. L.; Cook, F. J.; McGloin, R. P.; McGowan, H. A.; Burn, S.</p> <p>2011-05-01</p> <p>The use of scintillometers to determine sensible and latent <span class="hlt">heat</span> <span class="hlt">flux</span> is becoming increasingly common because of their ability to quantify convective <span class="hlt">fluxes</span> over distances of hundreds of meters to several kilometers. The majority of investigations using scintillometry have focused on processes above land surfaces, but here we propose a new methodology for obtaining sensible and latent <span class="hlt">heat</span> <span class="hlt">fluxes</span> from a scintillometer deployed over open water. This methodology has been tested by comparison with eddy covariance measurements and through comparison with alternative scintillometer calculation approaches that are commonly used in the literature. The methodology is based on linearization of the Bowen ratio, which is a common assumption in models such as Penman's model and its derivatives. Comparison of latent <span class="hlt">heat</span> <span class="hlt">flux</span> estimates from the eddy covariance system and the scintillometer showed excellent agreement across a range of weather conditions and <span class="hlt">flux</span> rates, giving a high level of confidence in scintillometry-derived latent <span class="hlt">heat</span> <span class="hlt">fluxes</span>. The proposed approach produced better estimates than other scintillometry calculation methods because of the reliance of alternative methods on measurements of water temperature or water body <span class="hlt">heat</span> storage, which are both notoriously hard to quantify. The proposed methodology requires less instrumentation than alternative scintillometer calculation approaches, and the spatial scales of required measurements are arguably more compatible. In addition to scintillometer measurements of the structure parameter of the refractive index of air, the only measurements required are atmospheric pressure, air temperature, humidity, and wind speed at one height over the water body.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010EGUGA..12.7262B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010EGUGA..12.7262B"><span>Anthropogenic <span class="hlt">heat</span> <span class="hlt">fluxes</span> over Moscow agglomeration and other Russian and world cities</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Belova, Iya; Ginzburg, Alexander</p> <p>2010-05-01</p> <p>Urbanization, particularly with respect to its sustainability, remains to be a great challenge in all regions of the world. Urbanization has an influence on soils, hydrology, and climate, these changes have effect on global climate, pollution, increase of anthropogenic greenhouse gases in the earth's atmosphere and human health. Thus anthropogenic <span class="hlt">heat</span> <span class="hlt">flux</span> is an important factor for estimation of development of global climate. The simple formula for anthropogenic <span class="hlt">heat</span> <span class="hlt">fluxes</span> (AHF) was proposed in the EGU General Assembly 2008 presentation [1] AHF = k × PD × EC, were PD is urban population density and EC is total energy consumption per capita. It was estimated that two of the world megacities - Seoul and Moscow - have the highest AHF values - 83 and 56 W/m2 correspondently. In presented paper it was studied the reasons of such high anthropogenic <span class="hlt">heat</span> <span class="hlt">fluxes</span> within Moscow region as well as AHF over the major Russian cities. It was shown that main reason of this circumstance is the administrative divisions in Moscow region. Moscow is ringed by Moscow circle motor road. Accordingly the city has sharply defined boundaries and densely populated residential suburbs are cut off and don't included in Moscow city administrative area. It was constructed the special graph to illuminate why Moscow city has such a high anthropogenic <span class="hlt">heat</span> factor and how much Moscow agglomeration AHF could be if consider not only Moscow city itself but also the nearest suburb towns. Using the data from World Bank [2] and Russian governmental statistic agency [3] anthropogenic <span class="hlt">heat</span> <span class="hlt">fluxes</span> for Russian cities with population more than 500 000 were estimated. Energy consumption data for different Russian regions were calculated by special routine using in the Web-atlas [4]. This research is supported by RAS Fundamental Research Project 'Influence of anthropogenic <span class="hlt">heat</span> <span class="hlt">fluxes</span> and aerosol pollution on <span class="hlt">heat</span> balance and climate of urbanized areas'. Other results of this project is presented in paper [5</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/865136','DOE-PATENT-XML'); return false;" href="https://www.osti.gov/servlets/purl/865136"><span>Method for braze-joining spirally wound tapes to inner <span class="hlt">walls</span> of <span class="hlt">heat</span> exchanger tubes</span></a></p> <p><a target="_blank" href="http://www.osti.gov/doepatents">DOEpatents</a></p> <p>Garrison, Melton E.</p> <p>1984-01-01</p> <p>The present invention is directed to a method of fabricating <span class="hlt">heat</span> exchanger tubes in which twisted tapes are utilized for promoting turbulence and <span class="hlt">heat</span> transfer. The method of the present invention provides for the brazing of the tapes to the inner <span class="hlt">walls</span> of the tubes for enhancing <span class="hlt">heat</span> transfer between the fluid within the conduit and a fluid medium outside of the conduit by conduction through the tape. The braze joint of the present invention is coextensive with the tape over the entire length thereof within the conduit. The practice of the present invention is achieved by placing a filler wire of brazing metal along the tape at a location removed from the side <span class="hlt">walls</span> and then <span class="hlt">heating</span> the conduit and tape sufficiently to effect the displacement of the filler metal by wicking to the contact point between the tape and the conduit <span class="hlt">wall</span> to form a braze joint coextensive with the length of the tape within the conduit. This arrangement provides maximum <span class="hlt">heat</span> transfer and assures that the tape is in contact with the conduit over the entire common length thereof.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/5607539','DOE-PATENT-XML'); return false;" href="https://www.osti.gov/biblio/5607539"><span>Method for braze-joining spirally wound tapes to inner <span class="hlt">walls</span> of <span class="hlt">heat</span> exchanger tubes</span></a></p> <p><a target="_blank" href="http://www.osti.gov/doepatents">DOEpatents</a></p> <p>Garrison, M.E.</p> <p>1982-09-03</p> <p>The present invention is directed to a method of fabricating <span class="hlt">heat</span> exchanger tubes in which twisted tapes are utilized for promoting turbulence and <span class="hlt">heat</span> transfer. The method of the present invention provides for the brazing of the tapes to the inner <span class="hlt">walls</span> of the tubes for enhancing <span class="hlt">heat</span> transfer between the fluid within the conduit and a fluid medium outside of the conduit by conduction through the tape. The braze joint of the present invention is coextensive with the tape over the entire length thereof within the conduit. The practice of the present invention is achieved by placing a filler wire of brazing metal along the tape at a location removed from the side <span class="hlt">walls</span> and then <span class="hlt">heating</span> the conduit and tape sufficiently to effect the displacement of the filler metal by wicking to the contact point between the tape and the conduit <span class="hlt">wall</span> to form a braze joint coextensive with the length of the tape within the conduit. This arrangement provides maximum <span class="hlt">heat</span> transfer and assures that the tape is in contact with the conduit over the entire common length thereof.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29749202','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29749202"><span>[Characteristics of water and <span class="hlt">heat</span> <span class="hlt">fluxes</span> and its footprint climatology on farmland in low hilly region of red soil].</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Li, Yang; Jing, Yuan Shu; Qin, Ben Ben</p> <p>2017-01-01</p> <p>The analysis of the characteristics and footprint climatology of farmland water and <span class="hlt">heat</span> <span class="hlt">fluxes</span> has great significance to strengthen regional climate resource management and improve the hydrothermal resource utilization in the region of red soil. Based on quality controlled data from large aperture scintillometer and automatic meteorological station in hilly region of red soil, this paper analyzed in detail the characteristics of farmland water and <span class="hlt">heat</span> <span class="hlt">fluxes</span> at different temporal scales and the corresponding source area distribution of <span class="hlt">flux</span> measurement in the non-rainy season and crop growth period in hilly region of red soil. The results showed that the diurnal variation of water and <span class="hlt">heat</span> <span class="hlt">fluxes</span> showed a unimodal trend, but compared with the sunny day, the diurnal variation curves fluctuated more complicatedly on cloudy day. In the whole, either ten-day periods or month scale, the water and <span class="hlt">heat</span> <span class="hlt">fluxes</span> were greater in August than in September, while the net radiation <span class="hlt">flux</span> was more distributed to latent <span class="hlt">heat</span> exchange. The proportion of net radiation to latent <span class="hlt">heat</span> <span class="hlt">flux</span> decreased in September compared to August, but the sensible <span class="hlt">heat</span> <span class="hlt">flux</span> was vice versa. With combined effects of weather conditions (particularly wind), stability, and surface condition, the source areas of <span class="hlt">flux</span> measurement at different temporal scales showed different distribution characteristics. Combined with the underlying surface crops, the source areas at different temporal scales also had different contribution sources.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011PhFl...23c0601G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011PhFl...23c0601G"><span>Investigation of the ellipsoidal-statistical Bhatnagar-Gross-Krook kinetic model applied to gas-phase transport of <span class="hlt">heat</span> and tangential momentum between parallel <span class="hlt">walls</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Gallis, M. A.; Torczynski, J. R.</p> <p>2011-03-01</p> <p>The ellipsoidal-statistical Bhatnagar-Gross-Krook (ES-BGK) kinetic model is investigated for steady gas-phase transport of <span class="hlt">heat</span>, tangential momentum, and mass between parallel <span class="hlt">walls</span> (i.e., Fourier, Couette, and Fickian flows). This investigation extends the original study of Cercignani and Tironi, who first applied the ES-BGK model to <span class="hlt">heat</span> transport (i.e., Fourier flow) shortly after this model was proposed by Holway. The ES-BGK model is implemented in a molecular-gas-dynamics code so that results from this model can be compared directly to results from the full Boltzmann collision term, as computed by the same code with the direct simulation Monte Carlo (DSMC) algorithm of Bird. A gas of monatomic molecules is considered. These molecules collide in a pairwise fashion according to either the Maxwell or the hard-sphere interaction and reflect from the <span class="hlt">walls</span> according to the Cercignani-Lampis-Lord model with unity accommodation coefficients. Simulations are performed at pressures from near-free-molecular to near-continuum. Unlike the BGK model, the ES-BGK model produces <span class="hlt">heat-flux</span> and shear-stress values that both agree closely with the DSMC values at all pressures. However, for both interactions, the ES-BGK model produces molecular-velocity-distribution functions that are qualitatively similar to those determined for the Maxwell interaction from Chapman-Enskog theory for small <span class="hlt">wall</span> temperature differences and moment-hierarchy theory for large <span class="hlt">wall</span> temperature differences. Moreover, the ES-BGK model does not produce accurate values of the mass self-diffusion coefficient for either interaction. Nevertheless, given its reasonable accuracy for <span class="hlt">heat</span> and tangential-momentum transport, its sound theoretical foundation (it obeys the H-theorem), and its available extension to polyatomic molecules, the ES-BGK model may be a useful method for simulating certain classes of single-species noncontinuum gas flows, as Cercignani suggested.</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('https://www.osti.gov/biblio/20997132-steady-state-film-boiling-heat-transfer-simulated-trace-v4','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/20997132-steady-state-film-boiling-heat-transfer-simulated-trace-v4"><span>Steady State Film Boiling <span class="hlt">Heat</span> Transfer Simulated With Trace V4.160</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>Audrius Jasiulevicius; Rafael Macian-Juan</p> <p>2006-07-01</p> <p>This paper presents the results of the assessment and analysis of TRACE v4.160 <span class="hlt">heat</span> transfer predictions in the post-CHF (critical <span class="hlt">heat</span> <span class="hlt">flux</span>) region and discusses the possibilities to improve the TRACE v4.160 code predictions in the film boiling <span class="hlt">heat</span> transfer when applying different film boiling correlations. For this purpose, the TRACE v4.160-calculated film boiling <span class="hlt">heat</span> <span class="hlt">flux</span> and the resulting maximum inner <span class="hlt">wall</span> temperatures during film boiling in single tubes were compared with experimental data obtained at the Royal Institute of Technology (KTH) in Stockholm, Sweden. The experimental database included measurements for pressures ranging from 30 to 200 bar and coolantmore » mass <span class="hlt">fluxes</span> from 500 to 3000 kg/m{sup 2}s. It was found that TRACE v4.160 does not produce correct predictions of the film boiling <span class="hlt">heat</span> <span class="hlt">flux</span>, and consequently of the maximum inner <span class="hlt">wall</span> temperature in the test section, under the wide range of conditions documented in the KTH experiments. In particular, it was found that the standard TRACE v4.160 under-predicts the film boiling <span class="hlt">heat</span> transfer coefficient at low pressure-low mass <span class="hlt">flux</span> and high pressure-high mass <span class="hlt">flux</span> conditions. For most of the rest of the investigated range of parameters, TRACE v4.160 over-predicts the film boiling <span class="hlt">heat</span> transfer coefficient, which can lead to non-conservative predictions in applications to nuclear power plant analyses. Since no satisfactory agreement with the experimental database was obtained with the standard TRACE v4.160 film boiling <span class="hlt">heat</span> transfer correlations, we have added seven film boiling correlations to TRACE v4.160 in order to investigate the possibility to improve the code predictions for the conditions similar to the KTH tests. The film boiling correlations were selected among the most commonly used film boiling correlations found in the open literature, namely Groeneveld 5.7, Bishop (2 correlations), Tong, Konkov, Miropolskii and Groeneveld-Delorme correlations. The only correlation among the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EL....11964001P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EL....11964001P"><span>Local rectification of <span class="hlt">heat</span> <span class="hlt">flux</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Pons, M.; Cui, Y. Y.; Ruschhaupt, A.; Simón, M. A.; Muga, J. G.</p> <p>2017-09-01</p> <p>We present a chain-of-atoms model where <span class="hlt">heat</span> is rectified, with different <span class="hlt">fluxes</span> from the hot to the cold baths located at the chain boundaries when the temperature bias is reversed. The chain is homogeneous except for boundary effects and a local modification of the interactions at one site, the “impurity”. The rectification mechanism is due here to the localized impurity, the only asymmetrical element of the structure, apart from the externally imposed temperature bias, and does not rely on putting in contact different materials or other known mechanisms such as grading or long-range interactions. The effect survives if all interaction forces are linear except the ones for the impurity.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017ClDy...48.1089L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017ClDy...48.1089L"><span>A multi-model ensemble view of winter <span class="hlt">heat</span> <span class="hlt">flux</span> dynamics and the dipole mode in the Mediterranean Sea</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Liguori, Giovanni; Di Lorenzo, Emanuele; Cabos, William</p> <p>2017-02-01</p> <p>Changes in surface <span class="hlt">heat</span> <span class="hlt">fluxes</span> affect several climate processes controlling the Mediterranean climate. These include the winter formation of deep waters, which is the primary driver of the Mediterranean Sea overturning circulation. Previous studies that characterize the spatial and temporal variability of surface <span class="hlt">heat</span> <span class="hlt">flux</span> anomalies over the basin reveal the existence of two statistically dominant patterns of variability: a monopole of uniform sign and an east-west dipole of opposite signs. In this work, we use the 12 regional climate model ensemble from the EU-FP6 ENSEMBLES project to diagnose the large-scale atmospheric processes that control the variability of <span class="hlt">heat</span> <span class="hlt">fluxes</span> over the Mediterranean Sea from interannual to decadal timescales (here defined as timescales > 6 year). Our findings suggest that while the monopole structure captures variability in the winter-to-winter domain-average net <span class="hlt">heat</span> <span class="hlt">flux</span>, the dipole pattern tracks changes in the Mediterranean climate that are connected to the East Atlantic/Western Russia (EA/WR) atmospheric teleconnection pattern. Furthermore, while the monopole exhibits significant differences in the spatial structure across the multi-model ensemble, the dipole pattern is very robust and more clearly identifiable in the anomaly maps of individual years. A <span class="hlt">heat</span> budget analysis of the dipole pattern reveals that changes in winds associated with the EA/WR pattern exert dominant control through both a direct effect on the latent <span class="hlt">heat</span> <span class="hlt">flux</span> (i.e., wind speed) and an indirect effect through specific humidity (e.g., wind advection). A simple reconstruction of the <span class="hlt">heat</span> <span class="hlt">flux</span> variability over the deep-water formation regions of the Gulf of Lion and the Aegean Sea reveals that the combination of the monopole and dipole time series explains over 90 % of the <span class="hlt">heat</span> <span class="hlt">flux</span> variance in these regions. Given the important role that surface <span class="hlt">heat</span> <span class="hlt">flux</span> anomalies play in deep-water formation and the regional climate, improving our knowledge on the dynamics</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1999PhDT........27O','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1999PhDT........27O"><span>An experimental investigation of the effects of spiral angle on the evaporation <span class="hlt">heat</span> transfer coefficients in microfin tubes with visualization technique</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Oh, Se-Yoon</p> <p></p> <p>A smooth tube and five microfin tubes were tested, and evaporation <span class="hlt">heat</span> transfer coefficients were measured and compared for mass <span class="hlt">fluxes</span>, 50, 100 and 200 kg/m2 s, and <span class="hlt">heat</span> <span class="hlt">fluxes</span>, 5, 10 and 20 kW/m 2, with Refrigerant 134a as a working fluid. The evaporation <span class="hlt">heat</span> transfer coefficients at quality 0.5 were compared among the smooth and five microfin tubes with spiral angles 6, 12, 18, 25 and 44 degrees. The effect of the spiral angle on the <span class="hlt">heat</span> transfer coefficients was examined. It was found that the optimal spiral angle where the maximum <span class="hlt">heat</span> transfer coefficient occurs, mainly depends on mass <span class="hlt">flux</span>. The optimal spiral angle was 18 degrees for G=50 kg/m2 s, and 6 degrees for G=100 and 200 kg/m 2 s. A borescope was used to visualize the flow on the inside <span class="hlt">wall</span> of test tubes. The purpose was to find out the effect of the grooves on the liquid flow in microfin tubes and to explain the mechanism of <span class="hlt">heat</span> transfer enhancement. Temperatures on the tube <span class="hlt">wall</span> were measured at the same axial location as the imaging sensor of the borescope, and were related to the behavior of the liquid flow on the inside <span class="hlt">wall</span> of the tubes. The liquid flow in the grooves on the <span class="hlt">wall</span> was found to be the most important factor in enhancing <span class="hlt">heat</span> transfer coefficients. The liquid flowed upward along the grooves and covered the upper inside <span class="hlt">wall</span> of the microfin tubes at G=50 kg/m2 s. When <span class="hlt">heat</span> <span class="hlt">flux</span> increases, the liquid flow was found at a higher position. Both liquid viscosity and surface tension decrease, when temperature increases. Thus, the lower viscosity at higher <span class="hlt">heat</span> <span class="hlt">flux</span> facilitated the upward motion of the liquid flow in the grooves, so that the momentum force as well as the capillary effect was found to push the liquid along the grooves.* *A CD is included with dissertation containing video clips in avi format which can be viewed with media player.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016JGRD..121.7853K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016JGRD..121.7853K"><span>Re-examining the roles of surface <span class="hlt">heat</span> <span class="hlt">flux</span> and latent <span class="hlt">heat</span> release in a "hurricane-like" polar low over the Barents Sea</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kolstad, Erik W.; Bracegirdle, Thomas J.; Zahn, Matthias</p> <p>2016-07-01</p> <p>Polar lows are intense mesoscale cyclones that occur at high latitudes in both hemispheres during winter. Their sometimes evidently convective nature, fueled by strong surface <span class="hlt">fluxes</span> and with cloud-free centers, have led to some polar lows being referred to as "arctic hurricanes." Idealized studies have shown that intensification by hurricane development mechanisms is theoretically possible in polar winter atmospheres, but the lack of observations and realistic simulations of actual polar lows have made it difficult to ascertain if this occurs in reality. Here the roles of surface <span class="hlt">heat</span> <span class="hlt">fluxes</span> and latent <span class="hlt">heat</span> release in the development of a Barents Sea polar low, which in its cloud structures showed some similarities to hurricanes, are studied with an ensemble of sensitivity experiments, where latent <span class="hlt">heating</span> and/or surface <span class="hlt">fluxes</span> of sensible and latent <span class="hlt">heat</span> were switched off before the polar low peaked in intensity. To ensure that the polar lows in the sensitivity runs did not track too far away from the actual environmental conditions, a technique known as spectral nudging was applied. This was shown to be crucial for enabling comparisons between the different model runs. The results presented here show that (1) no intensification occurred during the mature, postbaroclinic stage of the simulated polar low; (2) surface <span class="hlt">heat</span> <span class="hlt">fluxes</span>, i.e., air-sea interaction, were crucial processes both in order to attain the polar low's peak intensity during the baroclinic stage and to maintain its strength in the mature stage; and (3) latent <span class="hlt">heat</span> release played a less important role than surface <span class="hlt">fluxes</span> in both stages.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19990080915','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19990080915"><span>Diffusion, <span class="hlt">Fluxes</span>, Friction Forces, and Joule <span class="hlt">Heating</span> in Two-Temperature Multicomponent Magnetohydrodynamics</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Chang, C. H.</p> <p>1999-01-01</p> <p>The relationship between Joule <span class="hlt">heating</span>, diffusion <span class="hlt">fluxes</span>, and friction forces has been studied for both total and electron thermal energy equations, using general expressions for multicomponent diffusion in two-temperature plasmas with the velocity dependent Lorentz force acting on charged species in a magnetic field. It is shown that the derivation of Joule <span class="hlt">heating</span> terms requires both diffusion <span class="hlt">fluxes</span> and friction between species which represents the resistance experienced by the species moving at different relative velocities. It is also shown that the familiar Joule <span class="hlt">heating</span> term in the electron thermal energy equation includes artificial effects produced by switching the convective velocity from the species velocity to the mass-weighted velocity, and thus should not be ignored even when there is no net energy dissipation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.A33B2351M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.A33B2351M"><span>Development of a New Methodology for Computing Surface Sensible <span class="hlt">Heat</span> <span class="hlt">Fluxes</span> using Thermal Imagery</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Morrison, T. J.; Calaf, M.; Fernando, H. J.; Price, T. A.; Pardyjak, E.</p> <p>2017-12-01</p> <p>Current numerical weather predication models utilize similarity to characterize momentum, moisture, and <span class="hlt">heat</span> <span class="hlt">fluxes</span>. Such formulations are only valid under the ideal assumptions of spatial homogeneity, statistical stationary, and zero subsidence. However, recent surface temperature measurements from the Mountain Terrain Atmospheric Modeling and Observations (MATERHORN) Program on the Salt Flats of Utah's West desert, show that even under the most a priori ideal conditions, heterogeneity of the aforementioned variables exists. We present a new method to extract spatially-distributed measurements of surface sensible <span class="hlt">heat</span> <span class="hlt">flux</span> from thermal imagery. The approach consists of using a surface energy budget, where the ground <span class="hlt">heat</span> <span class="hlt">flux</span> is easily computed from limited measurements using a force-restore-type methodology, the latent <span class="hlt">heat</span> <span class="hlt">fluxes</span> are neglected, and the energy storage is computed using a lumped capacitance model. Preliminary validation of the method is presented using experimental data acquired from a nearby sonic anemometer during the MATERHORN campaign. Additional evaluation is required to confirm the method's validity. Further decomposition analysis of on-site instrumentation (thermal camera, cold-hotwire probes, and sonic anemometers) using Proper Orthogonal Decomposition (POD), and wavelet analysis, reveals time scale similarity between the flow and surface fluctuations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018PhRvB..97t5414O','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018PhRvB..97t5414O"><span>Circular <span class="hlt">heat</span> and momentum <span class="hlt">flux</span> radiated by magneto-optical nanoparticles</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ott, A.; Ben-Abdallah, P.; Biehs, S.-A.</p> <p>2018-05-01</p> <p>In the present article we investigate the <span class="hlt">heat</span> and momentum <span class="hlt">fluxes</span> radiated by a hot magneto-optical nanoparticle in its surroundings under the action of an external magnetic field. We show that the <span class="hlt">flux</span> lines circulate in a confined region at a nanometric distance from the particle around the axis of the magnetic field in a vortexlike configuration. Moreover we prove that the spatial orientation of these vortices (clockwise or counterclockwise) is associated with the contribution of optical resonances with topological charges m =+1 or m =-1 to the thermal emission. This work paves the way for a geometric description of <span class="hlt">heat</span> and momentum transport in lattices of magneto-optical particles. Moreover it could have important applications in the field of energy storage as well as in thermal management at nanoscale.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1076472-reduced-model-simulations-scrape-off-layer-heat-flux-width-comparison-experiment','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1076472-reduced-model-simulations-scrape-off-layer-heat-flux-width-comparison-experiment"><span>Reduced model simulations of the scrape-off-layer <span class="hlt">heat-flux</span> width and comparison with experiment</span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Myra, J. R.; Russell, D. A.; D’Ippolito, D. A.; ...</p> <p>2011-01-01</p> <p>Reduced model simulations of turbulence in the edge and scrape-off-layer (SOL) region of a spherical torus or tokamak plasma are employed to address the physics of the scrape-off-layer <span class="hlt">heat</span> <span class="hlt">flux</span> width. The simulation model is an electrostatic two-dimensional fluid turbulence model, applied in the plane perpendicular to the magnetic field at the outboard midplane of the torus. The model contains curvature-driven-interchange modes, sheath losses, and both perpendicular turbulent diffusive and convective (blob) transport. These transport processes compete with classical parallel transport to set the SOL width. Midplane SOL profiles of density, temperature and parallel <span class="hlt">heat</span> <span class="hlt">flux</span> are obtained from themore » simulation and compared with experimental results from the National Spherical Torus Experiment (NSTX) to study the scaling of the <span class="hlt">heat</span> <span class="hlt">flux</span> width with power and plasma current. It is concluded that midplane turbulence is the main contributor to the SOL <span class="hlt">heat</span> <span class="hlt">flux</span> width for the low power H-mode discharges studied, while additional physics is required to explain the plasma current scaling of the SOL <span class="hlt">heat</span> <span class="hlt">flux</span> width observed experimentally in higher power discharges. Intermittent separatrix spanning convective cells are found to be the main mechanism that sets the near-SOL width in the simulations. The roles of sheared flows and blob trapping vs. emission are discussed.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JARS...11d6012L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JARS...11d6012L"><span>Estimation of land surface <span class="hlt">heat</span> <span class="hlt">fluxes</span> based on visible infrared imaging radiometer suite data: case study in northern China</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Li, Xiaojun; Xin, Xiaozhou; Peng, Zhiqing; Zhang, Hailong; Li, Li; Shao, Shanshan; Liu, Qinhuo</p> <p>2017-10-01</p> <p>Evapotranspiration (ET) plays an important role in surface-atmosphere interactions and can be monitored using remote sensing data. The visible infrared imaging radiometer suite (VIIRS) sensor is a generation of optical satellite sensors that provide daily global coverage at 375- to 750-m spatial resolutions with 22 spectral channels (0.412 to 12.05 μm) and capable of monitoring ET from regional to global scales. However, few studies have focused on methods of acquiring ET from VIIRS images. The objective of this study is to introduce an algorithm that uses the VIIRS data and meteorological variables to estimate the energy budgets of land surfaces, including the net radiation, soil <span class="hlt">heat</span> <span class="hlt">flux</span>, sensible <span class="hlt">heat</span> <span class="hlt">flux</span>, and latent <span class="hlt">heat</span> <span class="hlt">fluxes</span>. A single-source model that based on surface energy balance equation is used to obtain surface <span class="hlt">heat</span> <span class="hlt">fluxes</span> within the Zhangye oasis in China. The results were validated using observations collected during the HiWATER (Heihe Watershed Allied Telemetry Experimental Research) project. To facilitate comparison, we also use moderate resolution imaging spectrometer (MODIS) data to retrieve the regional surface <span class="hlt">heat</span> <span class="hlt">fluxes</span>. The validation results show that it is feasible to estimate the turbulent <span class="hlt">heat</span> <span class="hlt">flux</span> based on the VIIRS sensor and that these data have certain advantages (i.e., the mean bias error of sensible <span class="hlt">heat</span> <span class="hlt">flux</span> is 15.23 W m-2) compared with MODIS data (i.e., the mean bias error of sensible <span class="hlt">heat</span> <span class="hlt">flux</span> is -29.36 W m-2). Error analysis indicates that, in our model, the accuracies of the estimated sensible <span class="hlt">heat</span> <span class="hlt">fluxes</span> rely on the errors in the retrieved surface temperatures and the canopy heights.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20040034110','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20040034110"><span>A Comparison of Latent <span class="hlt">Heat</span> <span class="hlt">Fluxes</span> over Global Oceans for Four <span class="hlt">Flux</span> Products</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Chou, Shu-Hsien; Nelkin, Eric; Ardizzone, Joe; Atlas, Robert M.</p> <p>2003-01-01</p> <p>To improve our understanding of global energy and water cycle variability, and to improve model simulations of climate variations, it is vital to have accurate latent <span class="hlt">heat</span> <span class="hlt">fluxes</span> (LHF) over global oceans. Monthly LHF, 10-m wind speed (U10m), 10-m specific humidity (Q10h), and sea-air humidity difference (Qs-Q10m) of GSSTF2 (version 2 Goddard Satellite-based Surface Turbulent <span class="hlt">Fluxes</span>) over global Oceans during 1992-93 are compared with those of HOAPS (Hamburg Ocean Atmosphere Parameters and <span class="hlt">Fluxes</span> from Satellite Data), NCEP (NCEP/NCAR reanalysis). The mean differences, standard deviations of differences, and temporal correlation of these monthly variables over global Oceans during 1992-93 between GSSTF2 and each of the three datasets are analyzed. The large-scale patterns of the 2yr-mean fields for these variables are similar among these four datasets, but significant quantitative differences are found. The temporal correlation is higher in the northern extratropics than in the south for all variables, with the contrast being especially large for da Silva as a result of more missing ship data in the south. The da Silva has extremely low temporal correlation and large differences with GSSTF2 for all variables in the southern extratropics, indicating that da Silva hardly produces a realistic variability in these variables. The NCEP has extremely low temporal correlation (0.27) and large spatial variations of differences with GSSTF2 for Qs-Q10m in the tropics, which causes the low correlation for LHF. Over the tropics, the HOAPS LHF is significantly smaller than GSSTF2 by approx. 31% (37 W/sq m), whereas the other two datasets are comparable to GSSTF2. This is because the HOAPS has systematically smaller LHF than GSSTF2 in space, while the other two datasets have very large spatial variations of large positive and negative LHF differences with GSSTF2 to cancel and to produce smaller regional-mean differences. Our analyses suggest that the GSSTF2 latent <span class="hlt">heat</span> <span class="hlt">flux</span></p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27387899','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27387899"><span>Additional double-<span class="hlt">wall</span> roof in single-<span class="hlt">wall</span>, closed, convective incubators: Impact on body <span class="hlt">heat</span> loss from premature infants and optimal adjustment of the incubator air temperature.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Delanaud, Stéphane; Decima, Pauline; Pelletier, Amandine; Libert, Jean-Pierre; Stephan-Blanchard, Erwan; Bach, Véronique; Tourneux, Pierre</p> <p>2016-09-01</p> <p>Radiant <span class="hlt">heat</span> loss is high in low-birth-weight (LBW) neonates. Double-<span class="hlt">wall</span> or single-<span class="hlt">wall</span> incubators with an additional double-<span class="hlt">wall</span> roof panel that can be removed during phototherapy are used to reduce Radiant <span class="hlt">heat</span> loss. There are no data on how the incubators should be used when this second roof panel is removed. The aim of the study was to assess the <span class="hlt">heat</span> exchanges in LBW neonates in a single-<span class="hlt">wall</span> incubator with and without an additional roof panel. To determine the optimal thermoneutral incubator air temperature. Influence of the additional double-<span class="hlt">wall</span> roof was assessed by using a thermal mannequin simulating a LBW neonate. Then, we calculated the optimal incubator air temperature from a cohort of human LBW neonate in the absence of the additional roof panel. Twenty-three LBW neonates (birth weight: 750-1800g; gestational age: 28-32 weeks) were included. With the additional roof panel, R was lower but convective and evaporative skin <span class="hlt">heat</span> losses were greater. This difference can be overcome by increasing the incubator air temperature by 0.15-0.20°C. The benefit of an additional roof panel was cancelled out by greater body <span class="hlt">heat</span> losses through other routes. Understanding the <span class="hlt">heat</span> transfers between the neonate and the environment is essential for optimizing incubators. Copyright © 2016 IPEM. Published by Elsevier Ltd. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20060033621&hterms=neural+networks&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D90%26Ntt%3Dneural%2Bnetworks','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20060033621&hterms=neural+networks&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D90%26Ntt%3Dneural%2Bnetworks"><span>A neural network to retrieve the mesoscale instantaneous latent <span class="hlt">heat</span> <span class="hlt">flux</span> over oceans from SSM/I observations</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Bourras, D.; Eymard, L.; Liu, W. T.</p> <p>2000-01-01</p> <p>The turbulent latent and sensible <span class="hlt">heat</span> <span class="hlt">fluxes</span> are necessary to study <span class="hlt">heat</span> budget of the upper ocean or initialize ocean general circulation models. In order to retrieve the latent <span class="hlt">heat</span> <span class="hlt">flux</span> from satellite observations authors mostly use a bulk approximation of the <span class="hlt">flux</span> whose parameters are derived from different instrument. In this paper, an approach based on artificial neural networks is proposed and compared to the bulk method on a global data set and 3 local data sets.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016ResPh...6..139M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016ResPh...6..139M"><span>Effect of radiator position and mass <span class="hlt">flux</span> on the dryer room <span class="hlt">heat</span> transfer rate</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Mirmanto, M.; Sulistyowati, E. D.; Okariawan, I. D. K.</p> <p></p> <p>A room radiator as usually used in cold countries, is actually able to be used as a <span class="hlt">heat</span> source to dry goods, especially in the rainy season where the sun seldom shines due to much rain and cloud. Experiments to investigate effects of radiator position and mass <span class="hlt">flux</span> on <span class="hlt">heat</span> transfer rate were performed. This study is to determine the best position of the radiator and the optimum mass <span class="hlt">flux</span>. The radiator used was a finned radiator made of copper pipes and aluminum fins with an overall dimension of 220 mm × 50 mm × 310 mm. The prototype room was constructed using plywood and wood frame with an overall size of 1000 mm × 1000 mm × 1000 mm. The working fluid was <span class="hlt">heated</span> water flowing inside the radiator and air circulating naturally inside the prototype room. The nominal mass <span class="hlt">fluxes</span> employed were 800, 900 and 1000 kg/m2 s. The water was kept at 80 °C at the radiator entrance, while the initial air temperature inside the prototype room was 30 °C. Three positions of the radiator were examined. The results show that the effect of the mass <span class="hlt">flux</span> on the forced and free convection <span class="hlt">heat</span> transfer rate is insignificant but the radiator position strongly affects the <span class="hlt">heat</span> transfer rate for both forced and free convection.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JAP...122f3302G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JAP...122f3302G"><span>Material impacts and <span class="hlt">heat</span> <span class="hlt">flux</span> characterization of an electrothermal plasma source with an applied magnetic field</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Gebhart, T. E.; Martinez-Rodriguez, R. A.; Baylor, L. R.; Rapp, J.; Winfrey, A. L.</p> <p>2017-08-01</p> <p>To produce a realistic tokamak-like plasma environment in linear plasma device, a transient source is needed to deliver <span class="hlt">heat</span> and particle <span class="hlt">fluxes</span> similar to those seen in an edge localized mode (ELM). ELMs in future large tokamaks will deliver <span class="hlt">heat</span> <span class="hlt">fluxes</span> of ˜1 GW/m2 to the divertor plasma facing components at a few Hz. An electrothermal plasma source can deliver <span class="hlt">heat</span> <span class="hlt">fluxes</span> of this magnitude. These sources operate in an ablative arc regime which is driven by a DC capacitive discharge. An electrothermal source was configured with two pulse lengths and tested under a solenoidal magnetic field to determine the resulting impact on liner ablation, plasma parameters, and delivered <span class="hlt">heat</span> <span class="hlt">flux</span>. The arc travels through and ablates a boron nitride liner and strikes a tungsten plate. The tungsten target plate is analyzed for surface damage using a scanning electron microscope.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017ClDy...49..391C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017ClDy...49..391C"><span>ENSO related SST anomalies and relation with surface <span class="hlt">heat</span> <span class="hlt">fluxes</span> over south Pacific and Atlantic</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Chatterjee, S.; Nuncio, M.; Satheesan, K.</p> <p>2017-07-01</p> <p>The role of surface <span class="hlt">heat</span> <span class="hlt">fluxes</span> in Southern Pacific and Atlantic Ocean SST anomalies associated with El Nino Southern Oscillation (ENSO) is studied using observation and ocean reanalysis products. A prominent dipole structure in SST anomaly is found with a positive (negative) anomaly center over south Pacific (65S-45S, 120W-70W) and negative (positive) one over south Atlantic (50S-30S, 30W-0E) during austral summer (DJF) of El Nino (LaNina). During late austral spring-early summer (OND) of El Nino (LaNina), anomalous northerly (southerly) meridional moisture transport and a positive (negative) sea level pressure anomaly induces a suppressed (enhanced) latent <span class="hlt">heat</span> <span class="hlt">flux</span> from the ocean surface over south Pacific. This in turn results in a shallower than normal mixed layer depth which further helps in development of the SST anomaly. Mixed layer thins further due to anomalous shortwave radiation during summer and a well developed SST anomaly evolves. The south Atlantic pole exhibits exactly opposite characteristics at the same time. The contribution from the surface <span class="hlt">heat</span> <span class="hlt">fluxes</span> to mixed layer temperature change is found to be dominant over the advective processes over both the basins. Net surface <span class="hlt">heat</span> <span class="hlt">fluxes</span> anomaly is also found to be maximum during late austral spring-early summer period, with latent <span class="hlt">heat</span> <span class="hlt">flux</span> having a major contribution to it. The anomalous latent <span class="hlt">heat</span> <span class="hlt">fluxes</span> between atmosphere and ocean surface play important role in the growth of observed summertime SST anomaly. Sea-surface height also shows similar out-of-phase signatures over the two basins and are well correlated with the ENSO related SST anomalies. It is also observed that the magnitude of ENSO related anomalies over the southern ocean are weaker in LaNina years than in El Nino years, suggesting an intensified tropics-high latitude tele-connection during warm phases of ENSO.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017PhyA..470...20A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017PhyA..470...20A"><span>Effects of finite <span class="hlt">wall</span> thickness and sinusoidal <span class="hlt">heating</span> on convection in nanofluid-saturated local thermal non-equilibrium porous cavity</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Alsabery, A. I.; Chamkha, A. J.; Saleh, H.; Hashim, I.; Chanane, B.</p> <p>2017-03-01</p> <p>The effects of finite <span class="hlt">wall</span> thickness and sinusoidal <span class="hlt">heating</span> on convection in a nanofluid-saturated local thermal non-equilibrium (LTNE) porous cavity are studied numerically using the finite difference method. The finite thickness vertical <span class="hlt">wall</span> of the cavity is maintained at a constant temperature and the right <span class="hlt">wall</span> is <span class="hlt">heated</span> sinusoidally. The horizontal insulated <span class="hlt">walls</span> allow no <span class="hlt">heat</span> transfer to the surrounding. The Darcy law is used along with the Boussinesq approximation for the flow. Water-based nanofluids with Cu nanoparticles are chosen for investigation. The results of this study are obtained for various parameters such as the Rayleigh number, periodicity parameter, nanoparticles volume fraction, thermal conductivity ratio, ratio of <span class="hlt">wall</span> thickness to its height and the modified conductivity ratio. Explanation for the influence of the various above-mentioned parameters on the streamlines, isotherms, local Nusselt number and the weighted average <span class="hlt">heat</span> transfer is provided with regards to the thermal conductivities of nanoparticles suspended in the pure fluid and the porous medium. It is shown that the overall <span class="hlt">heat</span> transfer is significantly increased with the relative non-uniform <span class="hlt">heating</span>. Further, the convection <span class="hlt">heat</span> transfer is shown to be inhibited by the presence of the solid <span class="hlt">wall</span>. The results have possible applications in the <span class="hlt">heat</span>-storage fluid-saturated porous systems and the applications of the high power <span class="hlt">heat</span> transfer.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19910021158','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19910021158"><span>A laser-induced <span class="hlt">heat</span> <span class="hlt">flux</span> technique for convective <span class="hlt">heat</span> transfer measurements in high speed flows</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Porro, A. R.; Keith, T. G., Jr.; Hingst, W. R.</p> <p>1991-01-01</p> <p>A technique is developed to measure the local convective <span class="hlt">heat</span> transfer coefficient on a model surface in a supersonic flow field. The technique uses a laser to apply a discrete local <span class="hlt">heat</span> <span class="hlt">flux</span> at the model test surface, and an infrared camera system determines the local temperature distribution due to the <span class="hlt">heating</span>. From this temperature distribution and an analysis of the <span class="hlt">heating</span> process, a local convective <span class="hlt">heat</span> transfer coefficient is determined. The technique was used to measure the local surface convective <span class="hlt">heat</span> transfer coefficient distribution on a flat plate at nominal Mach numbers of 2.5, 3.0, 3.5, and 4.0. The flat plate boundary layer initially was laminar and became transitional in the measurement region. The experimentally determined convective <span class="hlt">heat</span> transfer coefficients were generally higher than the theoretical predictions for flat plate laminar boundary layers. However, the results indicate that this nonintrusive optical measurement technique has the potential to measure surface convective <span class="hlt">heat</span> transfer coefficients in high speed flow fields.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19920071694&hterms=transfer+techniques&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3Dtransfer%2Btechniques','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19920071694&hterms=transfer+techniques&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3Dtransfer%2Btechniques"><span>A laser-induced <span class="hlt">heat</span> <span class="hlt">flux</span> technique for convective <span class="hlt">heat</span> transfer measurements in high speed flows</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Porro, A. R.; Keith, T. G., Jr.; Hingst, W. R.</p> <p>1991-01-01</p> <p>A technique is developed to measure the local convective <span class="hlt">heat</span> transfer coefficient on a model surface in a supersonic flow field. The technique uses a laser to apply a discrete local <span class="hlt">heat</span> <span class="hlt">flux</span> at the model test surface, and an infrared camera system determines the local temperature distribution due to the <span class="hlt">heating</span>. From this temperature distribution and an analysis of the <span class="hlt">heating</span> process, a local convective <span class="hlt">heat</span> transfer coefficient is determined. The technique was used to measure the local surface convective <span class="hlt">heat</span> transfer coefficient distribution on a flat plate at nominal Mach numbers of 2.5, 3.0, 3.5, and 4.0. The flat plate boundary layer initially was laminar and became transitional in the measurement region. The experimentally determined convective <span class="hlt">heat</span> transfer coefficients were generally higher than the theoretical predictions for flat plate laminar boundary layers. However, the results indicate that this nonintrusive optical measurement technique has the potential to measure surface convective <span class="hlt">heat</span> transfer coefficients in high-speed flowfields.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014AGUFMGC13C0652T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AGUFMGC13C0652T"><span>Southern Ocean air-sea <span class="hlt">heat</span> <span class="hlt">flux</span>, SST spatial anomalies, and implications for multi-decadal upper ocean <span class="hlt">heat</span> content trends.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Tamsitt, V. M.; Talley, L. D.; Mazloff, M. R.</p> <p>2014-12-01</p> <p>The Southern Ocean displays a zonal dipole (wavenumber one) pattern in sea surface temperature (SST), with a cool zonal anomaly in the Atlantic and Indian sectors and a warm zonal anomaly in the Pacific sector, associated with the large northward excursion of the Malvinas and southeastward flow of the Antarctic Circumpolar Current (ACC). To the north of the cool Indian sector is the warm, narrow Agulhas Return Current (ARC). Air-sea <span class="hlt">heat</span> <span class="hlt">flux</span> is largely the inverse of this SST pattern, with ocean <span class="hlt">heat</span> gain in the Atlantic/Indian, cooling in the southeastward-flowing ARC, and cooling in the Pacific, based on adjusted <span class="hlt">fluxes</span> from the Southern Ocean State Estimate (SOSE), a ⅙° eddy permitting model constrained to all available in situ data. This <span class="hlt">heat</span> <span class="hlt">flux</span> pattern is dominated by turbulent <span class="hlt">heat</span> loss from the ocean (latent and sensible), proportional to perturbations in the difference between SST and surface air temperature, which are maintained by ocean advection. Locally in the Indian sector, intense <span class="hlt">heat</span> loss along the ARC is contrasted by ocean <span class="hlt">heat</span> gain of 0.11 PW south of the ARC. The IPCC AR5 50 year depth-averaged 0-700 m temperature trend shows surprising similarities in its spatial pattern, with upper ocean warming in the ARC contrasted by cooling to the south. Using diagnosed <span class="hlt">heat</span> budget terms from the most recent (June 2014) 6-year run of the SOSE we find that surface cooling in the ARC is balanced by <span class="hlt">heating</span> from south-eastward advection by the current whereas <span class="hlt">heat</span> gain in the ACC is balanced by cooling due to northward Ekman transport driven by strong westerly winds. These results suggest that spatial patterns in multi-decadal upper ocean temperature trends depend on regional variations in upper ocean dynamics.</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('http://hdl.handle.net/2060/19930022671','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19930022671"><span>Hypersonic engine component experiments in high <span class="hlt">heat</span> <span class="hlt">flux</span>, supersonic flow environment</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Gladden, Herbert J.; Melis, Matthew E.</p> <p>1993-01-01</p> <p>A major concern in advancing the state-of-the-art technologies for hypersonic vehicles is the development of an aeropropulsion system capable of withstanding the sustained high thermal loads expected during hypersonic flight. Even though progress has been made in the computational understanding of fluid dynamics and the physics/chemistry of high speed flight, there is also a need for experimental facilities capable of providing a high <span class="hlt">heat</span> <span class="hlt">flux</span> environment for testing component concepts and verifying/calibrating these analyses. A hydrogen/oxygen rocket engine <span class="hlt">heat</span> source was developed at the NASA Lewis Research Center as one element in a series of facilities at national laboratories designed to fulfill this need. This 'Hot Gas Facility' is capable of providing <span class="hlt">heat</span> <span class="hlt">fluxes</span> up to 450 w/sq cm on flat surfaces and up to 5,000 w/sq cm at the leading edge stagnation point of a strut in a supersonic flow stream. Gas temperatures up to 3050 K can also be attained. Two recent experimental programs conducted in this facility are discussed. The objective of the first experiment is to evaluate the erosion and oxidation characteristics of a coating on a cowl leading edge (or strut leading edge) in a supersonic, high <span class="hlt">heat</span> <span class="hlt">flux</span> environment. Macrophotographic data from a coated leading edge model show progressive degradation over several thermal cycles at aerothermal conditions representative of high Mach number flight. The objective of the second experiment is to assess the capability of cooling a porous surface exposed to a high temperature, high velocity flow environment and to provide a <span class="hlt">heat</span> transfer data base for a design procedure. Experimental results from transpiration cooled surfaces in a supersonic flow environment are presented.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19820011907','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19820011907"><span>Estimating ocean-air <span class="hlt">heat</span> <span class="hlt">fluxes</span> during cold air outbreaks by satellite</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Chou, S. H.; Atlas, D.</p> <p>1981-01-01</p> <p>Nomograms of mean column <span class="hlt">heating</span> due to surface sensible and latent <span class="hlt">heat</span> <span class="hlt">fluxes</span> were developed. Mean sensible <span class="hlt">heating</span> of the cloud free region is related to the cloud free path (CFP, the distance from the shore to the first cloud formation) and the difference between land air and sea surface temperatures, theta sub 1 and theta sub 0, respectively. Mean latent <span class="hlt">heating</span> is related to the CFP and the difference between land air and sea surface humidities q sub 1 and q sub 0 respectively. Results are also applicable to any path within the cloud free region. Corresponding <span class="hlt">heat</span> <span class="hlt">fluxes</span> may be obtained by multiplying the mean <span class="hlt">heating</span> by the mean wind speed in the boundary layer. The sensible <span class="hlt">heating</span> estimated by the present method is found to be in good agreement with that computed from the bulk transfer formula. The sensitivity of the solutions to the variations in the initial coastal soundings and large scale subsidence is also investigated. The results are not sensitive to divergence but are affected by the initial lapse rate of potential temperature; the greater the stability, the smaller the <span class="hlt">heating</span>, other things being equal. Unless one knows the lapse rate at the shore, this requires another independent measurement. For this purpose the downwind slope of the square of the boundary layer height is used, the mean value of which is also directly proportional to the mean sensible <span class="hlt">heating</span>. The height of the boundary layer should be measurable by future spaceborn lidar systems.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015JGRD..12011957A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015JGRD..12011957A"><span>Recent trends (2003-2013) of land surface <span class="hlt">heat</span> <span class="hlt">fluxes</span> on the southern side of the central Himalayas, Nepal</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Amatya, Pukar Man; Ma, Yaoming; Han, Cunbo; Wang, Binbin; Devkota, Lochan Prasad</p> <p>2015-12-01</p> <p>Novice efforts have been made in order to study the regional distribution of land surface <span class="hlt">heat</span> <span class="hlt">fluxes</span> on the southern side of the central Himalayas utilizing high-resolution remotely sensed products, but these have been on instantaneous scale. In this study the Surface Energy Balance System model is used to obtain annual averaged maps of the land surface <span class="hlt">heat</span> <span class="hlt">fluxes</span> for 11 years (2003-2013) and study their annual trends on the central Himalayan region. The maps were derived at 5 km resolution using monthly input products ranging from satellite derived to Global Land Data Assimilation System meteorological data. It was found that the net radiation <span class="hlt">flux</span> is increasing as a result of decreasing precipitation (drier environment). The sensible <span class="hlt">heat</span> <span class="hlt">flux</span> did not change much except for the northwestern High Himalaya and High Mountains. In northwestern High Himalaya sensible <span class="hlt">heat</span> <span class="hlt">flux</span> is decreasing because of decrease in wind speed, ground-air temperature difference, and increase in winter precipitation, whereas in High Mountains it is increasing due to increase in ground-air temperature difference and high rate of deforestation. The latent <span class="hlt">heat</span> <span class="hlt">flux</span> has an overall increasing trend with increase more pronounced in the lower regions compared to high elevated regions. It has been reported that precipitation is decreasing with altitude in this region. Therefore, the increasing trend in latent <span class="hlt">heat</span> <span class="hlt">flux</span> can be attributed to increase in net radiation <span class="hlt">flux</span> under persistent forest cover and irrigation land used for agriculture.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20150023475','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20150023475"><span>The Impact of Trends in the Large Scale Atmospheric Circulation on Mediterranean Surface Turbulent <span class="hlt">Heat</span> <span class="hlt">Fluxes</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Romanski, Joy; Hameed, Sultan</p> <p>2015-01-01</p> <p>Interannual variations of latent <span class="hlt">heat</span> <span class="hlt">fluxes</span> (LHF) and sensible <span class="hlt">heat</span> <span class="hlt">fluxes</span> (SHF) over the Mediterranean for the boreal winter season (DJF) show positive trends during 1958-2011. Comparison of correlations between the <span class="hlt">heat</span> <span class="hlt">fluxes</span> and the intensity and location of the Azores High (AH), and the NAO and East Atlantic-West Russia (EAWR) teleconnections, along with analysis of composites of surface temperature, humidity and wind fields for different teleconnection states, demonstrates that variations of the AH are found to explain the <span class="hlt">heat</span> <span class="hlt">flux</span> changes more successfully than the NAO and the EAWR. Trends in sea level pressure and longitude of the Azores High during DJF show a strengthening, and an eastward shift. DJF Azores High pressure and longitude are shown to co-vary such that variability of the Azores High occurs along an axis defined by lower pressure and westward location at one extreme, and higher pressure and eastward location at the other extreme. The shift of the Azores High from predominance of the low/west state to the high/east state induces trends in Mediterranean Sea surface winds, temperature and moisture. These, combined with sea surface warming trends, produce trends in wintertime Mediterranean Sea sensible and latent <span class="hlt">heat</span> <span class="hlt">fluxes</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1367091-heat-flux-modeling-using-ion-drift-effects-diii-mode-plasmas-resonant-magnetic-perturbations','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1367091-heat-flux-modeling-using-ion-drift-effects-diii-mode-plasmas-resonant-magnetic-perturbations"><span><span class="hlt">Heat</span> <span class="hlt">flux</span> modeling using ion drift effects in DIII-D H-mode plasmas with resonant magnetic perturbations</span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Wingen, Andreas; Schmitz, Oliver; Evans, Todd E.; ...</p> <p>2014-01-01</p> <p>The <span class="hlt">heat</span> <span class="hlt">flux</span> patterns measured in low-collisionality DIII-D H-mode plasmas strongly deviate from simultaneously measured CII emission patterns, used as indicator of particle <span class="hlt">flux</span>, during applied resonant magnetic perturbations. While the CII emission clearly shows typical striations, which are similar to magnetic footprint patterns obtained from vacuum field line tracing, the <span class="hlt">heat</span> <span class="hlt">flux</span> is usually dominated by one large peak at the strike point position. The vacuum approximation, which only considers applied magnetic fields and neglects plasma response and plasma effects, cannot explain the shape of the observed <span class="hlt">heat</span> <span class="hlt">flux</span> pattern. One possible explanation is the effect of particle drifts.more » This is included in the field line equations and the results are discussed with reference to the measurement. Electrons and ions show di fferent drift motions at thermal energy levels in a guiding center approximation. While electrons hardly deviate from the field lines, ions can drift several centimetres away from field line <span class="hlt">flux</span> surfaces. A model is presented in which an ion <span class="hlt">heat</span> <span class="hlt">flux</span>, based on the ion drift motion from various kinetic energies as they contribute to a thermal Maxwellian distribution, is calculated. The simulated <span class="hlt">heat</span> <span class="hlt">flux</span> is directly compared to measurements with a varying edge safety factor q95. This analysis provides evidence for the dominate e ect of high-energy ions in carrying <span class="hlt">heat</span> from the plasma inside the separatrix to the target. High-energy ions are deposited close to the unperturbed strike line while low-energy ions can travel into the striated magnetic topology.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2004JNuM..329..687L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2004JNuM..329..687L"><span>High <span class="hlt">heat</span> <span class="hlt">flux</span> properties of pure tungsten and plasma sprayed tungsten coatings</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Liu, X.; Tamura, S.; Tokunaga, K.; Yoshida, N.; Noda, N.; Yang, L.; Xu, Z.</p> <p>2004-08-01</p> <p>High <span class="hlt">heat</span> <span class="hlt">flux</span> properties of pure tungsten and plasma sprayed tungsten coatings on carbon substrates have been studied by annealing and cyclic <span class="hlt">heat</span> loading. The recrystallization temperature and an activation energy QR=126 kJ/mol for grain growth of tungsten coating by vacuum plasma spray (VPS) were estimated, and the microstructural changes of multi-layer tungsten and rhenium interface pre-deposited by physical vapor deposition (PVD) with anneal temperature were investigated. Cyclic load tests indicated that pure tungsten and VPS-tungsten coating could withstand 1000 cycles at 33-35 MW/m 2 <span class="hlt">heat</span> <span class="hlt">flux</span> and 3 s pulse duration, and inert gas plasma spray (IPS)-tungsten coating showed local cracks by 300 cycles but did not induce failure by further cycles. However, the failure of pure tungsten and VPS-tungsten coating by fatigue cracking was observed under higher <span class="hlt">heat</span> load (55-60 MW/m 2) for 420 and 230 cycles, respectively.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JThSc..26..160G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JThSc..26..160G"><span>Inverse <span class="hlt">heat</span> conduction estimation of inner <span class="hlt">wall</span> temperature fluctuations under turbulent penetration</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Guo, Zhouchao; Lu, Tao; Liu, Bo</p> <p>2017-04-01</p> <p>Turbulent penetration can occur when hot and cold fluids mix in a horizontal T-junction pipe at nuclear plants. Caused by the unstable turbulent penetration, temperature fluctuations with large amplitude and high frequency can lead to time-varying <span class="hlt">wall</span> thermal stress and even thermal fatigue on the inner <span class="hlt">wall</span>. Numerous cases, however, exist where inner <span class="hlt">wall</span> temperatures cannot be measured and only outer <span class="hlt">wall</span> temperature measurements are feasible. Therefore, it is one of the popular research areas in nuclear science and engineering to estimate temperature fluctuations on the inner <span class="hlt">wall</span> from measurements of outer <span class="hlt">wall</span> temperatures without damaging the structure of the pipe. In this study, both the one-dimensional (1D) and the two-dimensional (2D) inverse <span class="hlt">heat</span> conduction problem (IHCP) were solved to estimate the temperature fluctuations on the inner <span class="hlt">wall</span>. First, numerical models of both the 1D and the 2D direct <span class="hlt">heat</span> conduction problem (DHCP) were structured in MATLAB, based on the finite difference method with an implicit scheme. Second, both the 1D IHCP and the 2D IHCP were solved by the steepest descent method (SDM), and the DHCP results of temperatures on the outer <span class="hlt">wall</span> were used to estimate the temperature fluctuations on the inner <span class="hlt">wall</span>. Third, we compared the temperature fluctuations on the inner <span class="hlt">wall</span> estimated by the 1D IHCP with those estimated by the 2D IHCP in four cases: (1) when the maximum disturbance of temperature of fluid inside the pipe was 3°C, (2) when the maximum disturbance of temperature of fluid inside the pipe was 30°C, (3) when the maximum disturbance of temperature of fluid inside the pipe was 160°C, and (4) when the fluid temperatures inside the pipe were random from 50°C to 210°C.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014ExFl...55.1647G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014ExFl...55.1647G"><span>Teflon probing for the flow characterization of arc-<span class="hlt">heated</span> wind tunnel facilities</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Gulli, Stefano; Ground, Cody; Crisanti, Matthew; Maddalena, Luca</p> <p>2014-02-01</p> <p>The experimental flow characterization of the arc-<span class="hlt">heated</span> wind tunnel of the University of Texas at Arlington is investigated in this work using ablative Teflon probes in combination with total pressure measurements. A parallel analytical work, focused on the dimensional analysis of the ablation process, has been conducted with the purpose of improving existing semi-empirical correlations for the <span class="hlt">heat</span> blockage due to the mass injection inside the boundary layer. A control volume analysis at the receding surface of the specimens is used to calculate the <span class="hlt">wall</span> <span class="hlt">heat</span> transfer for a non-ablating probe by including the blockage effect. The new correlations, obtained for the convective blockage, show an improvement of the correlation coefficient of 110 % with respect to those available in literature, once a new blowing parameter containing the stagnation pressure is introduced. A correlation developed by NASA during the Round-Robin program, which relates the Teflon mass loss rate to the total pressure and cold-<span class="hlt">wall</span> <span class="hlt">heat</span> <span class="hlt">flux</span> measured experimentally, is also used to predict the <span class="hlt">wall</span> <span class="hlt">heat</span> transfer referred to the ablation temperature of Teflon. For both approaches, a simplified stagnation point convective <span class="hlt">heat</span> transfer equation allows the average stagnation enthalpy to be calculated. Several locations downstream of the nozzle exit have been surveyed, and selected points of the facility's performance map have been used for the experimental campaign. The results show that both approaches provide similar results in terms of stagnation <span class="hlt">heat</span> <span class="hlt">flux</span> and enthalpy prediction with uncertainties comparable to those provided by standard intrusive <span class="hlt">heat</span> <span class="hlt">flux</span> probes ( δ q max < 25 %). The analysis of the Teflon's ablated surface does not reveal significant flow non-uniformities, and a 1.14 <span class="hlt">heat</span> <span class="hlt">flux</span> enhancement factor due to the shock-shock interaction is detectable at x = 3.5 in. from the nozzle exit plane. The results show the use of ablative probes for the flow characterization of arc</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010APS..DPPTP9070P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010APS..DPPTP9070P"><span>Kinetic studies of divertor <span class="hlt">heat</span> <span class="hlt">fluxes</span> in Alcator C-Mod</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Pankin, A. Y.; Bateman, G.; Kritz, A. H.; Rafiq, T.; Park, G. Y.; Chang, C. S.; Brunner, D.; Hughes, J. W.; Labombard, B.; Terry, J.</p> <p>2010-11-01</p> <p>The kinetic XGC0 code [C.S. Chang et al, Phys. Plasmas 11 (2004) 2649] is used to model the H- mode pedestal and SOL regions in Alcator C-Mod discharges. The self-consistent simulations in this study include kinetic neoclassical physics and anomalous transport models along with the ExB flow shear effects. The <span class="hlt">heat</span> <span class="hlt">fluxes</span> on the divertor plates are computed and the <span class="hlt">fluxes</span> to the outer plate are compared with experimental observations. The dynamics of the radial electric field near the separatrix and in the SOL region are computed with the XGC0 code, and the effect of the anomalous transport on the <span class="hlt">heat</span> <span class="hlt">fluxes</span> in the SOL region is investigated. In particular, the particle and thermal diffusivities obtained in the analysis mode are compared with predictions from the theory-based anomalous transport models such as MMM95 [G. Bateman et al, Phys. Plasmas 5 (1998) 1793] and DRIBM [T. Rafiq et al, to appear in Phys. Plasmas (2010)]. It is found that there is a notable pinch effect in the inner separatrix region. Possible physical mechanisms for the particle and thermal pinches are discussed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1376436-material-impacts-heat-flux-characterization-electrothermal-plasma-source-applied-magnetic-field','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1376436-material-impacts-heat-flux-characterization-electrothermal-plasma-source-applied-magnetic-field"><span>Material impacts and <span class="hlt">heat</span> <span class="hlt">flux</span> characterization of an electrothermal plasma source with an applied magnetic field</span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Gebhart, T. E.; Martinez-Rodriguez, R. A.; Baylor, L. R.; ...</p> <p>2017-08-11</p> <p>To produce a realistic tokamak-like plasma environment in linear plasma device, a transient source is needed to deliver <span class="hlt">heat</span> and particle <span class="hlt">fluxes</span> similar to those seen in an edge localized mode (ELM). ELMs in future large tokamaks will deliver <span class="hlt">heat</span> <span class="hlt">fluxes</span> of ~1 GW/m 2 to the divertor plasma facing components at a few Hz. An electrothermal plasma source can deliver <span class="hlt">heat</span> <span class="hlt">fluxes</span> of this magnitude. These sources operate in an ablative arc regime which is driven by a DC capacitive discharge. An electrothermal source was configured in this paper with two pulse lengths and tested under a solenoidal magneticmore » field to determine the resulting impact on liner ablation, plasma parameters, and delivered <span class="hlt">heat</span> <span class="hlt">flux</span>. The arc travels through and ablates a boron nitride liner and strikes a tungsten plate. Finally, the tungsten target plate is analyzed for surface damage using a scanning electron microscope.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/1376436-material-impacts-heat-flux-characterization-electrothermal-plasma-source-applied-magnetic-field','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/1376436-material-impacts-heat-flux-characterization-electrothermal-plasma-source-applied-magnetic-field"><span>Material impacts and <span class="hlt">heat</span> <span class="hlt">flux</span> characterization of an electrothermal plasma source with an applied magnetic field</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>Gebhart, T. E.; Martinez-Rodriguez, R. A.; Baylor, L. R.</p> <p></p> <p>To produce a realistic tokamak-like plasma environment in linear plasma device, a transient source is needed to deliver <span class="hlt">heat</span> and particle <span class="hlt">fluxes</span> similar to those seen in an edge localized mode (ELM). ELMs in future large tokamaks will deliver <span class="hlt">heat</span> <span class="hlt">fluxes</span> of ~1 GW/m 2 to the divertor plasma facing components at a few Hz. An electrothermal plasma source can deliver <span class="hlt">heat</span> <span class="hlt">fluxes</span> of this magnitude. These sources operate in an ablative arc regime which is driven by a DC capacitive discharge. An electrothermal source was configured in this paper with two pulse lengths and tested under a solenoidal magneticmore » field to determine the resulting impact on liner ablation, plasma parameters, and delivered <span class="hlt">heat</span> <span class="hlt">flux</span>. The arc travels through and ablates a boron nitride liner and strikes a tungsten plate. Finally, the tungsten target plate is analyzed for surface damage using a scanning electron microscope.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018E%26ES..140a2111U','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018E%26ES..140a2111U"><span><span class="hlt">Heat</span> Conductivity Resistance of Concrete <span class="hlt">Wall</span> Panel by Water Flowing in Different Orientations of Internal PVC pipe</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Umi, N. N.; Norazman, M. N.; Daud, N. M.; Yusof, M. A.; Yahya, M. A.; Othman, M.</p> <p>2018-04-01</p> <p>Green building technology and sustainability development is current focus in the world nowadays. In Malaysia and most tropical countries the maximum temperature recorded typically at 35°C. Air-conditioning system has become a necessity in occupied buildings, thereby increasing the cost of electric consumption. The aim of this study is to find out the solution in minimizing <span class="hlt">heat</span> transfer from the external environment and intentions towards going green. In this study, the experimental work includes testing three types of concrete <span class="hlt">wall</span> panels. The main <span class="hlt">heat</span> intervention material in this research is 2 inch diameter Polyvinyl Chloride (PVC) pipe embedded at the center of the concrete <span class="hlt">wall</span> panel, while the EPS foam beads were added to the cement content in the concrete mix forming the outer layer of the <span class="hlt">wall</span> panel. Water from the rainwater harvesting system is regulated in the PVC pipe to intervene with the <span class="hlt">heat</span> conductivity through the <span class="hlt">wall</span> panel. Results from the experimental works show that the internal surface temperature of these <span class="hlt">heat</span> resistance <span class="hlt">wall</span> panels is to 3□C lower than control <span class="hlt">wall</span> panel from plain interlocking bricks.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018ResPh...8..341H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018ResPh...8..341H"><span>Effect of Cattaneo-Christov <span class="hlt">heat</span> <span class="hlt">flux</span> on Jeffrey fluid flow with variable thermal conductivity</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hayat, Tasawar; Javed, Mehwish; Imtiaz, Maria; Alsaedi, Ahmed</p> <p>2018-03-01</p> <p>This paper presents the study of Jeffrey fluid flow by a rotating disk with variable thickness. Energy equation is constructed by using Cattaneo-Christov <span class="hlt">heat</span> <span class="hlt">flux</span> model with variable thermal conductivity. A system of equations governing the model is obtained by applying boundary layer approximation. Resulting nonlinear partial differential system is transformed to ordinary differential system. Homotopy concept leads to the convergent solutions development. Graphical analysis for velocities and temperature is made to examine the influence of different involved parameters. Thermal relaxation time parameter signifies that temperature for Fourier's <span class="hlt">heat</span> law is more than Cattaneo-Christov <span class="hlt">heat</span> <span class="hlt">flux</span>. A constitutional analysis is made for skin friction coefficient and <span class="hlt">heat</span> transfer rate. Effects of Prandtl number on temperature distribution and <span class="hlt">heat</span> transfer rate are scrutinized. It is observed that larger Reynolds number gives illustrious temperature distribution.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/1020790-model-heat-transfer-sapwood-implications-sap-flux-density-measurements-using-thermal-dissipation-probes','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/1020790-model-heat-transfer-sapwood-implications-sap-flux-density-measurements-using-thermal-dissipation-probes"><span>A model of <span class="hlt">heat</span> transfer in sapwood and implications for sap <span class="hlt">flux</span> density measurements using thermal dissipation probes</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>Wullschleger, Stan D; Childs, Kenneth W; King, Anthony Wayne</p> <p>2011-01-01</p> <p>A variety of thermal approaches are used to estimate sap <span class="hlt">flux</span> density in stems of woody plants. Models have proven valuable tools for interpreting the behavior of <span class="hlt">heat</span> pulse, <span class="hlt">heat</span> balance, and <span class="hlt">heat</span> field deformation techniques, but have seldom been used to describe <span class="hlt">heat</span> transfer dynamics for the <span class="hlt">heat</span> dissipation method. Therefore, to better understand the behavior of <span class="hlt">heat</span> dissipation probes, a model was developed that takes into account the thermal properties of wood, the physical dimensions and thermal characteristics of the probes, and the conductive and convective <span class="hlt">heat</span> transfer that occurs due to water flow in the sapwood. Probesmore » were simulated as aluminum tubes 20 mm in length and 2 mm in diameter, whereas sapwood, heartwood, and bark each had a density and water fraction that determined their thermal properties. Base simulations assumed a constant sap <span class="hlt">flux</span> density with sapwood depth and no wounding or physical disruption of xylem beyond the 2 mm diameter hole drilled for probe installation. Simulations across a range of sap <span class="hlt">flux</span> densities showed that the dimensionless quantity k defined as ( Tm T)/ T where Tm is the temperature differential ( T) between the <span class="hlt">heated</span> and unheated probe under zero flow conditions was dependent on the thermal conductivity of the sapwood. The relationship between sap <span class="hlt">flux</span> density and k was also sensitive to radial gradients in sap <span class="hlt">flux</span> density and to xylem disruption near the probe. Monte Carlo analysis in which 1000 simulations were conducted while simultaneously varying thermal conductivity and wound diameter revealed that sap <span class="hlt">flux</span> density and k showed considerable departure from the original calibration equation used with this technique. The departure was greatest for abrupt patterns of radial variation typical of ring-porous species. Depending on the specific combination of thermal conductivity and wound diameter, use of the original calibration equation resulted in an 81% under- to 48% over-estimation of sap <span class="hlt">flux</span></p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22611415-mhd-effects-heat-transfer-ucm-fluid-along-joule-heating-thermal-radiation-using-cattaneo-christov-heat-flux-model','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22611415-mhd-effects-heat-transfer-ucm-fluid-along-joule-heating-thermal-radiation-using-cattaneo-christov-heat-flux-model"><span>MHD effects and <span class="hlt">heat</span> transfer for the UCM fluid along with Joule <span class="hlt">heating</span> and thermal radiation using Cattaneo-Christov <span class="hlt">heat</span> <span class="hlt">flux</span> model</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>Shah, S., E-mail: sajidshah313@yahoo.com; Hussain, S.; Sagheer, M.</p> <p>2016-08-15</p> <p>Present study examines the numerical analysis of MHD flow of Maxwell fluid with thermal radiation and Joule <span class="hlt">heating</span> by considering the recently developed Cattaneo-Christov <span class="hlt">heat</span> <span class="hlt">flux</span> model which explains the time relaxation characteristics for the <span class="hlt">heat</span> <span class="hlt">flux</span>. The objective is to analyze the governing parameters such as viscoelastic fluid parameter, Magnetic parameter, Eckert and Prandtl number’s impact on the velocity and temperature profiles through graphs and tables. Suitable similarity transformations have been used to reduce the formulated PDEs into a system of coupled non-linear ODEs. Shooting technique has been invoked for finding the numerical solutions of the dimensionless velocity andmore » temperature profiles. Additionally, the MATLAB built-in routine bvp4c has also been used to verify and strengthen the results obtained by shooting method. From some special cases of the present work, a comparison with the previously published results has been presented.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29358631','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29358631"><span>High geothermal <span class="hlt">heat</span> <span class="hlt">flux</span> in close proximity to the Northeast Greenland Ice Stream.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Rysgaard, Søren; Bendtsen, Jørgen; Mortensen, John; Sejr, Mikael K</p> <p>2018-01-22</p> <p>The Greenland ice sheet (GIS) is losing mass at an increasing rate due to surface melt and flow acceleration in outlet glaciers. Currently, there is a large disagreement between observed and simulated ice flow, which may arise from inaccurate parameterization of basal motion, subglacial hydrology or geothermal <span class="hlt">heat</span> sources. Recently it was suggested that there may be a hidden <span class="hlt">heat</span> source beneath GIS caused by a higher than expected geothermal <span class="hlt">heat</span> <span class="hlt">flux</span> (GHF) from the Earth's interior. Here we present the first direct measurements of GHF from beneath a deep fjord basin in Northeast Greenland. Temperature and salinity time series (2005-2015) in the deep stagnant basin water are used to quantify a GHF of 93 ± 21 mW m -2 which confirm previous indirect estimated values below GIS. A compilation of <span class="hlt">heat</span> <span class="hlt">flux</span> recordings from Greenland show the existence of geothermal <span class="hlt">heat</span> sources beneath GIS and could explain high glacial ice speed areas such as the Northeast Greenland ice stream.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017E%26ES...61a2003Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017E%26ES...61a2003Z"><span>Unsteady <span class="hlt">heat</span> transfer performance of <span class="hlt">heat</span> pipe with axially swallow-tailed microgrooves</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zhang, R. P.</p> <p>2017-04-01</p> <p>A mathematical model is developed for predicting the transient <span class="hlt">heat</span> transfer and fluid flow of <span class="hlt">heat</span> pipe with axially swallow-tailed microgrooves. The effects of liquid convective <span class="hlt">heat</span> transfer in the microgrooves, liquid-vapor interfacial phase-change <span class="hlt">heat</span> transfer and liquid-vapor interfacial shear stress are accounted for in the present model. The coupled non-linear control equations are solved numerically. Mass flow rate at the interface is obtained from the application of kinetic theory. Time variation of <span class="hlt">wall</span> temperature is studied from the initial startup to steady state. The numerical results are verified by experiments. Time constants for startup and shutdown operation are defined to determine how fast a <span class="hlt">heat</span> pipe responds to an applied input <span class="hlt">heat</span> <span class="hlt">flux</span>, which slightly decreases with increasing <span class="hlt">heat</span> load.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011E%26PSL.306..205Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011E%26PSL.306..205Z"><span><span class="hlt">Heat</span> <span class="hlt">fluxes</span> at the Earth's surface and core-mantle boundary since Pangea formation and their implications for the geomagnetic superchrons</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zhang, Nan; Zhong, Shijie</p> <p>2011-06-01</p> <p>The Earth's surface and core-mantle boundary (CMB) <span class="hlt">heat</span> <span class="hlt">fluxes</span> are controlled by mantle convection and have important influences on Earth's thermal evolution and geodynamo processes in the core. However, the long-term variations of the surface and CMB <span class="hlt">heat</span> <span class="hlt">fluxes</span> remain poorly understood, particularly in response to the supercontinent Pangea — likely the most significant global tectonic event in the last 500 Ma. In this study, we reconstruct temporal evolution of the surface and CMB <span class="hlt">heat</span> <span class="hlt">fluxes</span> since the Paleozoic by formulating three-dimensional spherical models of mantle convection with plate motion history for the last 450 Ma that includes the assembly and break-up of supercontinent Pangea. Our models reproduce well present-day observations of the surface <span class="hlt">heat</span> <span class="hlt">flux</span> and seafloor age distribution. Our models show that the present-day CMB <span class="hlt">heat</span> <span class="hlt">flux</span> is low below the central Pacific and Africa but high elsewhere due to subducted slabs, particularly when chemically dense piles are present above the CMB. We show that while the surface <span class="hlt">heat</span> <span class="hlt">flux</span> may not change significantly in response to Pangea assembly, it increases by ~ 16% from 200 to 120 Ma ago as a result of Pangea breakup and then decreases for the last 120 Ma to approximately the pre-200 Ma value. As consequences of the assembly and breakup of Pangea, equatorial CMB <span class="hlt">heat</span> <span class="hlt">flux</span> reaches minimum at ~ 270 Ma and again at ~ 100 Ma ago, while global CMB <span class="hlt">heat</span> <span class="hlt">flux</span> is a maximum at ~ 100 Ma ago. These extrema in CMB <span class="hlt">heat</span> <span class="hlt">fluxes</span> coincide with the Kiaman (316-262 Ma) and Cretaceous (118-83 Ma) Superchrons, respectively, and may be responsible for the Superchrons.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20090035866&hterms=spacex&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D90%26Ntt%3Dspacex','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20090035866&hterms=spacex&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D90%26Ntt%3Dspacex"><span>Validation of PICA Ablation and Thermal-Response Model at Low <span class="hlt">Heat</span> <span class="hlt">Flux</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Milos, Frank S.; Chen, Yih-Kanq</p> <p>2009-01-01</p> <p>Phenolic Impregnated Carbon Ablator (PICA) was the forebody heatshield material on the Stardust sample-return capsule and is also a primary candidate material for the Mars Science Lander (MSL), the Orion Crew Module, and the SpaceX Dragon vehicle. As part of the heatshield qualification for Orion, physical and thermal properties of virgin and charred PICA were measured, and an ablation and thermal response model was developed. We validated the model by comparing it with recession and temperature data from stagnation arcjet tests conducted over a wide range of stagnation <span class="hlt">heat</span> <span class="hlt">flux</span> of 107 to 1102 W/sq cm. The effect of orthotropic thermal conductivity was evident in the thermal response of the arcjet models. In general, model predictions compared well with the data; however, the uncertainty of the recession prediction was greatest for <span class="hlt">heat</span> <span class="hlt">fluxes</span> below 200 W/sq cm. More recent MSL testing focused on the low <span class="hlt">heat</span> <span class="hlt">flux</span> regime of 45 to 250 W/sq cm. The new results confirm the recession uncertainty, especially for pressures below 6 kPa. In this work we focus on improving the model predictions for MSL and Orion tests below 250 W/sq cm.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014AGUFMSA41A4056H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AGUFMSA41A4056H"><span>Direct measurements of vertical <span class="hlt">heat</span> <span class="hlt">flux</span> and Na <span class="hlt">flux</span> in the mesosphere and lower thermosphere by lidar at Boulder (40°N, 105°W), Colorado</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Huang, W.; Chu, X.; Gardner, C. S.; Barry, I. F.; Smith, J. A.; Fong, W.; Yu, Z.; Chen, C.</p> <p>2014-12-01</p> <p>The vertical transport of <span class="hlt">heat</span> and constituent by gravity waves and tides plays a fundamental role in establishing the thermal and constituent structures of the mesosphere and lower thermosphere (MLT), but has not been thoroughly investigated by observations. In particular, direct measurements of vertical <span class="hlt">heat</span> <span class="hlt">flux</span> and metal constituent <span class="hlt">flux</span> caused by dissipating waves are extremely rare, which demand precise measurements with high spatial and temporal resolutions over a long period. Such requirements are necessary to overcome various uncertainties to reveal the small quantities of the <span class="hlt">heat</span> and constituent <span class="hlt">fluxes</span> induced by dissipating waves. So far such direct observations have only been reported for vertical <span class="hlt">heat</span> and Na <span class="hlt">fluxes</span> using a Na Doppler lidar at Starfire Optical Range (SOR) in Albuquerque, New Mexico. Furthermore, estimate of eddy <span class="hlt">heat</span> and constituent <span class="hlt">fluxes</span> from the turbulent mixing generated by breaking waves is even more challenging due to the even smaller temporal and spatial scales of the eddy. Consequently, the associated coefficients of thermal (kH) and constituent (kzz) diffusion have not been well characterized and remain as large uncertainties in models. We attempt to address these issues with direct measurements by a Na Doppler lidar with exceptional high-resolution measurement capabilities. Since summer 2010, we have been operating a Na Doppler lidar at Boulder, Colorado. The efficiency of the lidar has been greatly improved in summer of 2011 and achieved generally over 1000 counts of Na signal per lidar pulse in winter. In 2013, we made extensive Na lidar observations in 98 nights. These data covering each month of a full year will be used to characterize the seasonal variations of <span class="hlt">heat</span> and Na <span class="hlt">fluxes</span> and to be compared with the pioneering observations at SOR. In November 2013, we further upgraded the lidar with two new frequency shifters and a new data acquisition scheme, which are optimized for estimating eddy <span class="hlt">fluxes</span> and reducing 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_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('http://hdl.handle.net/2060/20100015631','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20100015631"><span>Thin Film <span class="hlt">Heat</span> <span class="hlt">Flux</span> Sensor Development for Ceramic Matrix Composite (CMC) Systems</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Wrbanek, John D.; Fralick, Gustave C.; Hunter, Gary W.; Zhu, Dongming; Laster, Kimala L.; Gonzalez, Jose M.; Gregory, Otto J.</p> <p>2010-01-01</p> <p>The NASA Glenn Research Center (GRC) has an on-going effort for developing high temperature thin film sensors for advanced turbine engine components. Stable, high temperature thin film ceramic thermocouples have been demonstrated in the lab, and novel methods of fabricating sensors have been developed. To fabricate thin film <span class="hlt">heat</span> <span class="hlt">flux</span> sensors for Ceramic Matrix Composite (CMC) systems, the rough and porous nature of the CMC system posed a significant challenge for patterning the fine features required. The status of the effort to develop thin film <span class="hlt">heat</span> <span class="hlt">flux</span> sensors specifically for use on silicon carbide (SiC) CMC systems with these new technologies is described.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19810020846','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19810020846"><span>Influence of thermal boundary conditions on <span class="hlt">heat</span> transfer from a cylinder in cross flow</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Papell, S. S.</p> <p>1981-01-01</p> <p>Local <span class="hlt">heat</span> transfer data over the leading surface of a cylinder in crossflow were obtained for a Reynolds number range of 50,000. The cylinder was operated at both uniform-<span class="hlt">wall</span>-temperature and uniform-<span class="hlt">heat-flux</span> thermal ance of 80 deg from the front stagnation point, the uniform-<span class="hlt">wall</span>-temperature <span class="hlt">heat</span> transfer coefficients were as much as 66 percent lower than the uniform-<span class="hlt">heat-flux</span> data. Between the stagnation point and 60 deg around the cylinder, there were no significant differences in the data. This region of the cylinder is within the cylindrical curvature region of the front end of a real turbine so it was concluded that either thermal boundary condition could be used to model turbine flow over that region of the blade. Results of evaluating the exponent x in the fundamental relationship Nu=f(Re) sup x, which is used in data correlation show the exponent varies as a function of local position on the cylinder even in the laminar flow region. The value of x increases linearly from 0.50 at the stagnation point to 0.59 at 60 deg around the cylinder. This linear trend continued into the separation region at 80 deg for the uniform-<span class="hlt">wall</span>-temperature data, but x increased markedly in the separation region for the uniform-<span class="hlt">heat-flux</span> data.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1981STIN...8129384P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1981STIN...8129384P"><span>Influence of thermal boundary conditions on <span class="hlt">heat</span> transfer from a cylinder in cross flow</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Papell, S. S.</p> <p>1981-08-01</p> <p>Local <span class="hlt">heat</span> transfer data over the leading surface of a cylinder in crossflow were obtained for a Reynolds number range of 50,000. The cylinder was operated at both uniform-<span class="hlt">wall</span>-temperature and uniform-<span class="hlt">heat-flux</span> thermal ance of 80 deg from the front stagnation point, the uniform-<span class="hlt">wall</span>-temperature <span class="hlt">heat</span> transfer coefficients were as much as 66 percent lower than the uniform-<span class="hlt">heat-flux</span> data. Between the stagnation point and 60 deg around the cylinder, there were no significant differences in the data. This region of the cylinder is within the cylindrical curvature region of the front end of a real turbine so it was concluded that either thermal boundary condition could be used to model turbine flow over that region of the blade. Results of evaluating the exponent x in the fundamental relationship Nu=f(Re) sup x, which is used in data correlation show the exponent varies as a function of local position on the cylinder even in the laminar flow region. The value of x increases linearly from 0.50 at the stagnation point to 0.59 at 60 deg around the cylinder. This linear trend continued into the separation region at 80 deg for the uniform-<span class="hlt">wall</span>-temperature data, but x increased markedly in the separation region for the uniform-<span class="hlt">heat-flux</span> data.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018E3SWC..3302002P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018E3SWC..3302002P"><span>Effect of aerated concrete blockwork joints on the <span class="hlt">heat</span> transfer performance uniformity</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Pukhkal, Viktor; Murgul, Vera</p> <p>2018-03-01</p> <p>Analysis of data on the effect of joints of the aerated concrete blocks on the <span class="hlt">heat</span> transfer uniformity of exterior <span class="hlt">walls</span> was carried out. It was concluded, that the values of the <span class="hlt">heat</span> transfer performance uniformity factor in the literature sources were obtained for the regular fragment of a <span class="hlt">wall</span> construction by approximate addition of thermal conductivities. <span class="hlt">Heat</span> flow patterns for the aerated concrete exterior <span class="hlt">walls</span> amid different values of the thermal conductivity factors and design ambient air temperature of -26 °C were calculated with the use of "ELCUT" software for modelling of thermal patterns by finite element method. There were defined the values for the <span class="hlt">heat</span> transfer performance uniformity factor, reduced total thermal resistance and <span class="hlt">heat-flux</span> density for the exterior <span class="hlt">walls</span>. The calculated values of the <span class="hlt">heat</span> transfer performance uniformity factors, as a function of the coefficient of thermal conductivity of aerated concrete blocks, differ from the known data by a more rigorous thermal and physical substantiation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018PhRvB..97r4306S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018PhRvB..97r4306S"><span>Electric control of the <span class="hlt">heat</span> <span class="hlt">flux</span> through electrophononic effects</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Seijas-Bellido, Juan Antonio; Aramberri, Hugo; Íñiguez, Jorge; Rurali, Riccardo</p> <p>2018-05-01</p> <p>We demonstrate a fully electric control of the <span class="hlt">heat</span> <span class="hlt">flux</span>, which can be continuously modulated by an externally applied electric field in PbTiO3, a prototypical ferroelectric perovskite, revealing the mechanisms by which experimentally accessible fields can be used to tune the thermal conductivity by as much as 50% at room temperature.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016MMTB...47.2447Y','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016MMTB...47.2447Y"><span>Crystallization Behavior and <span class="hlt">Heat</span> Transfer of Fluorine-Free Mold <span class="hlt">Fluxes</span> with Different Na2O Concentration</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Yang, Jian; Zhang, Jianqiang; Sasaki, Yasushi; Ostrovski, Oleg; Zhang, Chen; Cai, Dexiang; Kashiwaya, Yoshiaki</p> <p>2016-08-01</p> <p>In this study, the crystallization behavior and <span class="hlt">heat</span> transfer of CaO-SiO2-Na2O-B2O3-TiO2-Al2O3-MgO-Li2O fluorine-free mold <span class="hlt">fluxes</span> with different Na2O contents (5 to 11 mass pct) were studied using single/double hot thermocouple technique (SHTT/DHTT) and infrared emitter technique (IET), respectively. Continuous cooling transformation (CCT) and time-temperature transformation (TTT) diagrams constructed using SHTT showed that crystallization temperature increased and incubation time shortened with the increase of Na2O concentration, indicating an enhanced crystallization tendency. The crystallization process of mold <span class="hlt">fluxes</span> in the temperature field simulating the casting condition was also investigated using DHTT. X-ray diffraction (XRD) analysis of the quenched mold <span class="hlt">fluxes</span> showed that the dominant phase changed from CaSiO3 to Ca11Si4B2O22 with the increasing concentration of Na2O. The <span class="hlt">heat</span> transfer examined by IET showed that the increase of Na2O concentration reduced the responding <span class="hlt">heat</span> <span class="hlt">flux</span> when Na2O was lower than 9 mass pct but the further increase of Na2O to 11 mass pct enhanced the <span class="hlt">heat</span> <span class="hlt">flux</span>. The correlation between crystallinity and <span class="hlt">heat</span> transfer was discussed in terms of crystallization tendency and crystal morphology.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22390828-magnetic-flux-heat-losses-diffusive-advective-nernst-effects-maglif-like-plasma','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22390828-magnetic-flux-heat-losses-diffusive-advective-nernst-effects-maglif-like-plasma"><span>Magnetic <span class="hlt">flux</span> and <span class="hlt">heat</span> losses by diffusive, advective, and Nernst effects in MagLIF-like plasma</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>Velikovich, A. L., E-mail: sasha.velikovich@nrl.navy.mil; Giuliani, J. L., E-mail: sasha.velikovich@nrl.navy.mil; Zalesak, S. T.</p> <p>2014-12-15</p> <p>The MagLIF approach to inertial confinement fusion involves subsonic/isobaric compression and <span class="hlt">heating</span> of a DT plasma with frozen-in magnetic <span class="hlt">flux</span> by a heavy cylindrical liner. The losses of <span class="hlt">heat</span> and magnetic <span class="hlt">flux</span> from the plasma to the liner are thereby determined by plasma advection and gradient-driven transport processes, such as thermal conductivity, magnetic field diffusion and thermomagnetic effects. Theoretical analysis based on obtaining exact self-similar solutions of the classical collisional Braginskii's plasma transport equations in one dimension demonstrates that the <span class="hlt">heat</span> loss from the hot plasma to the cold liner is dominated by the transverse <span class="hlt">heat</span> conduction and advection, andmore » the corresponding loss of magnetic <span class="hlt">flux</span> is dominated by advection and the Nernst effect. For a large electron Hall parameter ω{sub e}τ{sub e} effective diffusion coefficients determining the losses of <span class="hlt">heat</span> and magnetic <span class="hlt">flux</span> are both shown to decrease with ω{sub e}τ{sub e} as does the Bohm diffusion coefficient, which is commonly associated with low collisionality and two-dimensional transport. This family of exact solutions can be used for verification of codes that model the MagLIF plasma dynamics.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19830001774','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19830001774"><span>Development of advanced high-temperature <span class="hlt">heat</span> <span class="hlt">flux</span> sensors</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Atkinson, W. H.; Strange, R. R.</p> <p>1982-01-01</p> <p>Various configurations of high temperature, <span class="hlt">heat</span> <span class="hlt">flux</span> sensors were studied to determine their suitability for use in experimental combustor liners of advanced aircraft gas turbine engines. It was determined that embedded thermocouple sensors, laminated sensors, and Gardon gauge sensors, were the most viable candidates. Sensors of all three types were fabricated, calibrated, and endurance tested. All three types of sensors met the fabricability survivability, and accuracy requirements established for their application.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.P43D2905H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.P43D2905H"><span>The <span class="hlt">Heat</span> <span class="hlt">Flux</span> through the Ice Shell on Europa, Constraints from Measurements in Terrestrial Conditions</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hruba, J.; Kletetschka, G.</p> <p>2017-12-01</p> <p><span class="hlt">Heat</span> transport across the ice shell of Europa controls the thermal evolution of its interior. Such process involves energy sources that drive ice resurfacing (1). More importantly, <span class="hlt">heat</span> <span class="hlt">flux</span> through the ice shell controls the thickness of the ice (2), that is poorly constrained between 1 km to 30+ km (3). Thin ice would allow ocean water to be affected by radiation from space. Thick ice would limit the <span class="hlt">heat</span> ocean sources available to the rock-ocean interface at the ocean's bottom due to tidal dissipation and potential radioactive sources. The <span class="hlt">heat</span> <span class="hlt">flux</span> structures control the development of geometrical configurations on the Europa's surface like double ridges, ice diapirs, chaos regions because the rheology of ice is temperature dependent (4).Analysis of temperature record of growing ice cover over a pond and water below revealed the importance of solar radiation during the ice growth. If there is no snow cover, a sufficient amount of solar radiation can penetrate through the ice and <span class="hlt">heat</span> the water below. Due to temperature gradient, there is a <span class="hlt">heat</span> <span class="hlt">flux</span> from the water to the ice (Qwi), which may reduce ice growth at the bottom. Details and variables that constrain the <span class="hlt">heat</span> <span class="hlt">flux</span> through the ice can be utilized to estimate the ice thickness. We show with this analog analysis provides the forth step towards measurement strategy on the surface of Europa. We identify three types of thermal profiles (5) and fourth with combination of all three mechanisms.References:(1) Barr, A. C., A. P. Showman, 2009, <span class="hlt">Heat</span> transfer in Europa's icy shell, University of Arizona Press, p. 405-430.(2) Ruiz, J., J. A. Alvarez-Gómez, R. Tejero, and N. Sánchez, 2007, <span class="hlt">Heat</span> flow and thickness of a convective ice shell on Europa for grain size-dependent rheologies: Icarus, v. 190, p. 145-154.(3) Billings, S. E., S. A. Kattenhorn, 2005, The great thickness debate: Ice shell thickness models for Europa and comparisons with estimates based on flexure at ridges: Icarus, v. 177, p. 397-412.(4) Quick</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/ADA549369','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA549369"><span>Physics-Based Modeling and Measurement of High-<span class="hlt">Flux</span> Condensation <span class="hlt">Heat</span> Transfer</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>2011-09-01</p> <p>TRANSFER (Contract No. N000140811139) by Prof. Issam Mudawar Sung-Min Kim Joseph Kim Boiling and Two-Phase Flow Laboratory School of...Final 01-10-2008 to 30-09-2011 Physics-Based Modeling and Measurement of High-<span class="hlt">Flux</span> Condensation <span class="hlt">Heat</span> Transfer NA N00014-08-1-1139 NA NA NA NA Mudawar ...respectively. phase change, condensation, electronics cooling, micro-channel, high-<span class="hlt">flux</span> U U U UU 107 Mudawar , Issam 765-494-5705 Reset PHYSICS-BASED</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AcAau.138..168H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AcAau.138..168H"><span>Drag and <span class="hlt">heat</span> <span class="hlt">flux</span> reduction mechanism of blunted cone with aerodisks</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Huang, Wei; Li, Lang-quan; Yan, Li; Zhang, Tian-tian</p> <p>2017-09-01</p> <p>The major challenge among a number of design requirements for hypersonic vehicles is the reduction of drag and aerodynamic <span class="hlt">heating</span>. Of all these techniques of drag and <span class="hlt">heat</span> <span class="hlt">flux</span> reduction, application of forward facing aerospike conceived in 1950s is an effective and simpler technique to reduce the drag as well as the <span class="hlt">heat</span> transfer rate for blunt nosed bodies at hypersonic Mach numbers. In this paper, the flow fields around a blunt cone with and without aerodisk flying at hypersonic Mach numbers are computed numerically, and the numerical simulations are conducted by specifying the freestream velocity, static pressure and static temperatures at the inlet of the computational domain with a three-dimensional, steady, Reynolds-averaged Navier-Stokes equation. An aerodisk is attached to the tip of the rod to reduce the drag and <span class="hlt">heat</span> <span class="hlt">flux</span> further. The influences of the length of rod and the diameter of aerodisk on the drag and <span class="hlt">heat</span> <span class="hlt">flux</span> reduction mechanism are analyzed comprehensively, and eight configurations are taken into consideration in the current study. The obtained results show that for all aerodisks, the reduction in drag of the blunt body is proportional to the extent of the recirculation dead air region. For long rods, the aerodisk is found not that beneficial in reducing the drag, and an aerodisk is more effective than an aerospike. The spike produces a region of recirculation separated flow that shields the blunt-nosed body from the incoming flow, and the recirculation region is formed around the root of the spike up to the reattachment point of the flow at the shoulder of the blunt body. The dynamic pressure in the recirculation area is highly reduced and thus leads to the decrease in drag and <span class="hlt">heat</span> load on the surface of the blunt body. Because of the reattachment of the shear layer on the shoulder of the blunt body, the pressure near that point becomes large.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016Cryo...78....1H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016Cryo...78....1H"><span>Numerical investigation of supercritical LNG convective <span class="hlt">heat</span> transfer in a horizontal serpentine tube</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Han, Chang-Liang; Ren, Jing-Jie; Dong, Wen-Ping; Bi, Ming-Shu</p> <p>2016-09-01</p> <p>The submerged combustion vaporizer (SCV) is indispensable general equipment for liquefied natural gas (LNG) receiving terminals. In this paper, numerical simulation was conducted to get insight into the flow and <span class="hlt">heat</span> transfer characteristics of supercritical LNG on the tube-side of SCV. The SST model with enhanced <span class="hlt">wall</span> treatment method was utilized to handle the coupled <span class="hlt">wall</span>-to-LNG <span class="hlt">heat</span> transfer. The thermal-physical properties of LNG under supercritical pressure were used for this study. After the validation of model and method, the effects of mass <span class="hlt">flux</span>, outer <span class="hlt">wall</span> temperature and inlet pressure on the <span class="hlt">heat</span> transfer behaviors were discussed in detail. Then the non-uniformity <span class="hlt">heat</span> transfer mechanism of supercritical LNG and effect of natural convection due to buoyancy change in the tube was discussed based on the numerical results. Moreover, different flow and <span class="hlt">heat</span> transfer characteristics inside the bend tube sections were also analyzed. The obtained numerical results showed that the local surface <span class="hlt">heat</span> transfer coefficient attained its peak value when the bulk LNG temperature approached the so-called pseudo-critical temperature. Higher mass <span class="hlt">flux</span> could eliminate the <span class="hlt">heat</span> transfer deteriorations due to the increase of turbulent diffusion. An increase of outer <span class="hlt">wall</span> temperature had a significant influence on diminishing <span class="hlt">heat</span> transfer ability of LNG. The maximum surface <span class="hlt">heat</span> transfer coefficient strongly depended on inlet pressure. Bend tube sections could enhance the <span class="hlt">heat</span> transfer due to secondary flow phenomenon. Furthermore, based on the current simulation results, a new dimensionless, semi-theoretical empirical correlation was developed for supercritical LNG convective <span class="hlt">heat</span> transfer in a horizontal serpentine tube. The paper provided the mechanism of <span class="hlt">heat</span> transfer for the design of high-efficiency SCV.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/21021096-impact-different-correlations-tracev4-predicted-critical-heat-flux','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/21021096-impact-different-correlations-tracev4-predicted-critical-heat-flux"><span>Impact of Different Correlations on TRACEv4.160 Predicted Critical <span class="hlt">Heat</span> <span class="hlt">Flux</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>Jasiulevicius, A.; Macian-Juan, R.</p> <p>2006-07-01</p> <p>This paper presents an independent assessment of the Critical <span class="hlt">Heat</span> <span class="hlt">Flux</span> (CHF) models implemented in TRACEv4.160 with data from the experiments carried out at the Royal Institute of Technology (RIT) in Stockholm, Sweden, with single vertical uniformly <span class="hlt">heated</span> 7.0 m long tubes. In previous CHF assessment studies with TRACE, it was noted that, although the overall code predictions in long single tubes with inner diameters of 1.0 to 2.49 cm agreed rather well with the results of experiments (with r.m.s. error being 25.6%), several regions of pressure and coolant mass <span class="hlt">flux</span> could be identified, in which the code strongly under-predictsmore » or over-predicts the CHF. In order to evaluate the possibility of improving the code performance, some of the most widely used and assessed CHF correlations were additionally implemented in TRACEv4.160, namely Bowring, Levitan - Lantsman, and Tong-W3. The results obtained for the CHF predictions in single tubes with uniform axial <span class="hlt">heat</span> <span class="hlt">flux</span> by using these correlations, were compared to the results produced with the standard TRACE correlations (Biasi and CISE-GE), and with the experimental data from RIT, which covered a broad range of pressures (3-20 MPa) and coolant mass <span class="hlt">fluxes</span> (500-3000 kg/m{sup 2}s). Several hundreds of experimental points were calculated to cover the parameter range mentioned above for the evaluation of the newly implemented correlations in the TRACEv4.160 code. (author)« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/887481','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/887481"><span>Validation experiments to determine radiation partitioning of <span class="hlt">heat</span> <span class="hlt">flux</span> to an object in a fully turbulent fire.</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>Ricks, Allen; Blanchat, Thomas K.; Jernigan, Dann A.</p> <p>2006-06-01</p> <p>It is necessary to improve understanding and develop validation data of the <span class="hlt">heat</span> <span class="hlt">flux</span> incident to an object located within the fire plume for the validation of SIERRA/ FUEGO/SYRINX fire and SIERRA/CALORE. One key aspect of the validation data sets is the determination of the relative contribution of the radiative and convective <span class="hlt">heat</span> <span class="hlt">fluxes</span>. To meet this objective, a cylindrical calorimeter with sufficient instrumentation to measure total and radiative <span class="hlt">heat</span> <span class="hlt">flux</span> had been designed and fabricated. This calorimeter will be tested both in the controlled radiative environment of the Penlight facility and in a fire environment in the FLAME/Radiant Heatmore » (FRH) facility. Validation experiments are specifically designed for direct comparison with the computational predictions. Making meaningful comparisons between the computational and experimental results requires careful characterization and control of the experimental features or parameters used as inputs into the computational model. Validation experiments must be designed to capture the essential physical phenomena, including all relevant initial and boundary conditions. A significant question of interest to modeling <span class="hlt">heat</span> <span class="hlt">flux</span> incident to an object in or near a fire is the contribution of the radiation and convection modes of <span class="hlt">heat</span> transfer. The series of experiments documented in this test plan is designed to provide data on the radiation partitioning, defined as the fraction of the total <span class="hlt">heat</span> <span class="hlt">flux</span> that is due to radiation.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20160009728','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20160009728"><span>Hybrid <span class="hlt">Heat</span> Pipes for Lunar and Martian Surface and High <span class="hlt">Heat</span> <span class="hlt">Flux</span> Space Applications</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Ababneh, Mohammed T.; Tarau, Calin; Anderson, William G.; Farmer, Jeffery T.; Alvarez-Hernandez, Angel R.</p> <p>2016-01-01</p> <p>Novel hybrid wick <span class="hlt">heat</span> pipes are developed to operate against gravity on planetary surfaces, operate in space carrying power over long distances and act as thermosyphons on the planetary surface for Lunar and Martian landers and rovers. These hybrid <span class="hlt">heat</span> pipes will be capable of operating at the higher <span class="hlt">heat</span> <span class="hlt">flux</span> requirements expected in NASA's future spacecraft and on the next generation of polar rovers and equatorial landers. In addition, the sintered evaporator wicks mitigate the start-up problems in vertical gravity aided <span class="hlt">heat</span> pipes because of large number of nucleation sites in wicks which will allow easy boiling initiation. ACT, NASA Marshall Space Flight Center, and NASA Johnson Space Center, are working together on the Advanced Passive Thermal experiment (APTx) to test and validate the operation of a hybrid wick VCHP with warm reservoir and HiK"TM" plates in microgravity environment on the ISS.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017WRR....5310858L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017WRR....5310858L"><span>Mapping Surface <span class="hlt">Heat</span> <span class="hlt">Fluxes</span> by Assimilating SMAP Soil Moisture and GOES Land Surface Temperature Data</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lu, Yang; Steele-Dunne, Susan C.; Farhadi, Leila; van de Giesen, Nick</p> <p>2017-12-01</p> <p>Surface <span class="hlt">heat</span> <span class="hlt">fluxes</span> play a crucial role in the surface energy and water balance. In situ measurements are costly and difficult, and large-scale <span class="hlt">flux</span> mapping is hindered by surface heterogeneity. Previous studies have demonstrated that surface <span class="hlt">heat</span> <span class="hlt">fluxes</span> can be estimated by assimilating land surface temperature (LST) and soil moisture to determine two key parameters: a neutral bulk <span class="hlt">heat</span> transfer coefficient (CHN) and an evaporative fraction (EF). Here a methodology is proposed to estimate surface <span class="hlt">heat</span> <span class="hlt">fluxes</span> by assimilating Soil Moisture Active Passive (SMAP) soil moisture data and Geostationary Operational Environmental Satellite (GOES) LST data into a dual-source (DS) model using a hybrid particle assimilation strategy. SMAP soil moisture data are assimilated using a particle filter (PF), and GOES LST data are assimilated using an adaptive particle batch smoother (APBS) to account for the large gap in the spatial and temporal resolution. The methodology is implemented in an area in the U.S. Southern Great Plains. Assessment against in situ observations suggests that soil moisture and LST estimates are in better agreement with observations after assimilation. The RMSD for 30 min (daytime) <span class="hlt">flux</span> estimates is reduced by 6.3% (8.7%) and 31.6% (37%) for H and LE on average. Comparison against a LST-only and a soil moisture-only assimilation case suggests that despite the coarse resolution, assimilating SMAP soil moisture data is not only beneficial but also crucial for successful and robust <span class="hlt">flux</span> estimation, particularly when the uncertainties in the model estimates are large.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19990025912','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19990025912"><span>Experimental Studies of the <span class="hlt">Heat</span> Transfer to RBCC Rocket Nozzles for CFD Application to Design Methodologies</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Santoro, Robert J.; Pal, Sibtosh</p> <p>1999-01-01</p> <p>Rocket thrusters for Rocket Based Combined Cycle (RBCC) engines typically operate with hydrogen/oxygen propellants in a very compact space. Packaging considerations lead to designs with either axisymmetric or two-dimensional throat sections. Nozzles tend to be either two- or three-dimensional. <span class="hlt">Heat</span> transfer characteristics, particularly in the throat, where the peak <span class="hlt">heat</span> <span class="hlt">flux</span> occurs, are not well understood. <span class="hlt">Heat</span> transfer predictions for these small thrusters have been made with one-dimensional analysis such as the Bartz equation or scaling of test data from much larger thrusters. The current work addresses this issue with an experimental program that examines the <span class="hlt">heat</span> transfer characteristics of a gaseous oxygen (GO2)/gaseous hydrogen (GH2) two-dimensional compact rocket thruster. The experiments involved measuring the axial <span class="hlt">wall</span> temperature profile in the nozzle region of a water-cooled gaseous oxygen/gaseous hydrogen rocket thruster at a pressure of 3.45 MPa. The <span class="hlt">wall</span> temperature measurements in the thruster nozzle in concert with Bartz's correlation are utilized in a one-dimensional model to obtain axial profiles of nozzle <span class="hlt">wall</span> <span class="hlt">heat</span> <span class="hlt">flux</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/111415','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/111415"><span>A formal approach for the prediction of the critical <span class="hlt">heat</span> <span class="hlt">flux</span> in subcooled water</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>Lombardi, C.</p> <p>1995-09-01</p> <p>The critical <span class="hlt">heat</span> <span class="hlt">flux</span> (CHF) in subcooled water at high mass <span class="hlt">fluxes</span> are not yet satisfactory correlated. For this scope a formal approach is here followed, which is based on an extension of the parameters and the correlation used for the dryout prediction for medium high quality mixtures. The obtained correlation, in spite of its simplicity and its explicit form, yields satisfactory predictions, also when applied to more conventional CHF data at low-medium mass <span class="hlt">fluxes</span> and high pressures. Further improvements are possible, if a more complete data bank will be available. The main and general open item is the definitionmore » of a criterion, depending only on independent parameters, such as mass <span class="hlt">flux</span>, pressure, inlet subcooling and geometry, to predict whether the <span class="hlt">heat</span> transfer crisis will result as a DNB or a dryout phenomenon.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016ClDy...47.1497S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016ClDy...47.1497S"><span>AMOC sensitivity to surface buoyancy <span class="hlt">fluxes</span>: Stronger ocean meridional <span class="hlt">heat</span> transport with a weaker volume transport?</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sévellec, Florian; Fedorov, Alexey V.</p> <p>2016-09-01</p> <p>Oceanic northward <span class="hlt">heat</span> transport is commonly assumed to be positively correlated with the Atlantic meridional overturning circulation (AMOC). For example, in numerical "water-hosing" experiments, imposing anomalous freshwater <span class="hlt">fluxes</span> in the northern Atlantic leads to a slow-down of the AMOC and the corresponding reduction of oceanic northward <span class="hlt">heat</span> transport. Here, we study the sensitivity of the ocean <span class="hlt">heat</span> and volume transports to surface <span class="hlt">heat</span> and freshwater <span class="hlt">fluxes</span> using a generalized stability analysis. For the sensitivity to surface freshwater <span class="hlt">fluxes</span>, we find that, while the direct relationship between the AMOC volume and <span class="hlt">heat</span> transports holds on shorter time scales, it can reverse on timescales longer than 500 years or so. That is, depending on the model surface boundary conditions, reduction in the AMOC volume transport can potentially lead to a stronger <span class="hlt">heat</span> transport on long timescales, resulting from the gradual increase in ocean thermal stratification. We discuss the implications of these results for the problem of steady state (statistical equilibrium) in ocean and climate GCM as well as paleoclimate problems including millennial climate variability.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1437164','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/1437164"><span>AMOC sensitivity to surface buoyancy <span class="hlt">fluxes</span>: Stronger ocean meridional <span class="hlt">heat</span> transport with a weaker volume transport?</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>Sevellec, Florian; Fedorov, Alexey V.</p> <p></p> <p>Oceanic northward <span class="hlt">heat</span> transport is commonly assumed to be positively correlated with the Atlantic meridional overturning circulation (AMOC). For example, in numerical "water-hosing" experiments, imposing anomalous freshwater <span class="hlt">fluxes</span> in the northern Atlantic leads to a slow-down of the AMOC and the corresponding reduction of oceanic northward <span class="hlt">heat</span> transport. Here, we study the sensitivity of the ocean <span class="hlt">heat</span> and volume transports to surface <span class="hlt">heat</span> and freshwater <span class="hlt">fluxes</span> using a generalized stability analysis. For the sensitivity to surface freshwater <span class="hlt">fluxes</span>, we find that, while the direct relationship between the AMOC volume and <span class="hlt">heat</span> transports holds on shorter time scales, it can reversemore » on timescales longer than 500 years or so. That is, depending on the model surface boundary conditions, reduction in the AMOC volume transport can potentially lead to a stronger <span class="hlt">heat</span> transport on long timescales, resulting from the gradual increase in ocean thermal stratification. Finally, we discuss the implications of these results for the problem of steady state (statistical equilibrium) in ocean and climate GCM as well as paleoclimate problems including millennial climate variability.« 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_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.osti.gov/pages/biblio/1437164-amoc-sensitivity-surface-buoyancy-fluxes-stronger-ocean-meridional-heat-transport-weaker-volume-transport','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1437164-amoc-sensitivity-surface-buoyancy-fluxes-stronger-ocean-meridional-heat-transport-weaker-volume-transport"><span>AMOC sensitivity to surface buoyancy <span class="hlt">fluxes</span>: Stronger ocean meridional <span class="hlt">heat</span> transport with a weaker volume transport?</span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Sevellec, Florian; Fedorov, Alexey V.</p> <p>2016-01-04</p> <p>Oceanic northward <span class="hlt">heat</span> transport is commonly assumed to be positively correlated with the Atlantic meridional overturning circulation (AMOC). For example, in numerical "water-hosing" experiments, imposing anomalous freshwater <span class="hlt">fluxes</span> in the northern Atlantic leads to a slow-down of the AMOC and the corresponding reduction of oceanic northward <span class="hlt">heat</span> transport. Here, we study the sensitivity of the ocean <span class="hlt">heat</span> and volume transports to surface <span class="hlt">heat</span> and freshwater <span class="hlt">fluxes</span> using a generalized stability analysis. For the sensitivity to surface freshwater <span class="hlt">fluxes</span>, we find that, while the direct relationship between the AMOC volume and <span class="hlt">heat</span> transports holds on shorter time scales, it can reversemore » on timescales longer than 500 years or so. That is, depending on the model surface boundary conditions, reduction in the AMOC volume transport can potentially lead to a stronger <span class="hlt">heat</span> transport on long timescales, resulting from the gradual increase in ocean thermal stratification. Finally, we discuss the implications of these results for the problem of steady state (statistical equilibrium) in ocean and climate GCM as well as paleoclimate problems including millennial climate variability.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018RScI...89f4901D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018RScI...89f4901D"><span>Development of a radiative <span class="hlt">heating</span> facility for studying flow and <span class="hlt">heat</span> transfer in hydrocarbon-cooled structures</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Dong, Da; Lu, Yang; Yuan, Yueming; Fan, Xuejun</p> <p>2018-06-01</p> <p>An experimental facility was designed to simulate the <span class="hlt">heat</span> exchange between the hot gas and the fuel-cooled <span class="hlt">wall</span> in a scramjet combustor. Thermal radiation from an electrically <span class="hlt">heated</span> graphite plate is employed to unilaterally <span class="hlt">heat</span> up a multi-channeled cooling plate. A maximum <span class="hlt">heat</span> <span class="hlt">flux</span> of over 0.8 MW/m2 was achieved for an effective <span class="hlt">heating</span> area up to 1000 mm × 40 mm. Precise control of the back pressure of a coolant (up to 5 MPa) in a unique way was also demonstrated. With this facility, studies of flow and <span class="hlt">heat</span> transfer in hydrocarbon-cooled structures can be performed under a well-controlled manner.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012IJAEO..17...76S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012IJAEO..17...76S"><span>A revised surface resistance parameterisation for estimating latent <span class="hlt">heat</span> <span class="hlt">flux</span> from remotely sensed data</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Song, Yi; Wang, Jiemin; Yang, Kun; Ma, Mingguo; Li, Xin; Zhang, Zhihui; Wang, Xufeng</p> <p>2012-07-01</p> <p>Estimating evapotranspiration (ET) is required for many environmental studies. Remote sensing provides the ability to spatially map latent <span class="hlt">heat</span> <span class="hlt">flux</span>. Many studies have developed approaches to derive spatially distributed surface energy <span class="hlt">fluxes</span> from various satellite sensors with the help of field observations. In this study, remote-sensing-based λE mapping was conducted using a Landsat Thematic Mapper (TM) image and an Enhanced Thematic Mapper Plus (ETM+) image. The remotely sensed data and field observations employed in this study were obtained from Watershed Allied Telemetry Experimental Research (WATER). A biophysics-based surface resistance model was revised to account for water stress and temperature constraints. The precision of the results was validated using 'ground truth' data obtained by eddy covariance (EC) system. Scale effects play an important role, especially for parameter optimisation and validation of the latent <span class="hlt">heat</span> <span class="hlt">flux</span> (λE). After considering the footprint of EC, the λE derived from the remote sensing data was comparable to the EC measured value during the satellite's passage. The results showed that the revised surface resistance parameterisation scheme was useful for estimating the latent <span class="hlt">heat</span> <span class="hlt">flux</span> over cropland in arid regions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19950053067&hterms=TIDE+POOLS&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3DTIDE%2BPOOLS','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19950053067&hterms=TIDE+POOLS&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3DTIDE%2BPOOLS"><span>Tidal and atmospheric forcing of the upper ocean in the Gulf of California. 2: Surface <span class="hlt">heat</span> <span class="hlt">flux</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Paden, Cynthia A.; Winant, Clinton D.; Abbott, Mark R.</p> <p>1993-01-01</p> <p>Satellite infrared imagery and coastal meteorological data for March 1984 through February 1985 are used to estimate the net annual surface <span class="hlt">heat</span> <span class="hlt">flux</span> for the northern Gulf of California. The average annual surface <span class="hlt">heat</span> <span class="hlt">flux</span> for the area north of Guaymas and Santa Rosalia is estimated to be +74 W/sq m for the 1984-1985 time period. This is comparable to the +20-50 W/sq m previously obtained from <span class="hlt">heat</span> and freshwater transport estimates made with hydrographic surveys from different years and months. The spatial distribution of the net surface <span class="hlt">heat</span> <span class="hlt">flux</span> shows a net gain of <span class="hlt">heat</span> over the whole northern gulf. Except for a local maximum near San Esteban Island, the largest <span class="hlt">heat</span> gain (+110-120 W/sq m) occurs in the Ballenas and Salsipuedes channels, where strong tidal mixing produces anomalously cold sea surface temperatures (SSTs) over much of the year. The lowest <span class="hlt">heat</span> gain occurs in the Guayamas Basin (+40-50 W/sq m), where SSTs are consistently warmer. In the relatively shallow northern basin the net surface <span class="hlt">heat</span> <span class="hlt">flux</span> is farily uniform, with a net annual gain of approxmately +70 W/sq m. A local minimum in <span class="hlt">heat</span> gain (approximately +60 W/sq m) is observed over the shelf in the northwest, where spring and summer surface temperatures are particularly high. A similar minimum in <span class="hlt">heat</span> gain over the shelf was observed in a separate study in which historical SSTs and 7 years (1979-1986) of meteorological data from Puerto Penasco were used to estimate the net surface <span class="hlt">heat</span> <span class="hlt">flux</span> for the northern basin. In that study, however, the <span class="hlt">heat</span> <span class="hlt">fluxes</span> were higher, with a gain of +100 W/sq m over the shelf and +114 W/sq m in the northern basin. These larger values are directly attributable to the higher humidities in the 1979-1986 study compared to the 1984-1985 satellite study. High humidities reduce evaporation and the associated latent <span class="hlt">heat</span> loss, promoting a net annual <span class="hlt">heat</span> gain. In the norther Gulf of California, however, tidal mixing appears to play a key role in the observed gain of</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017APS..DPPCO4002B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017APS..DPPCO4002B"><span>Boundary plasma <span class="hlt">heat</span> <span class="hlt">flux</span> width measurements for poloidal magnetic fields above 1 Tesla in the Alcator C-Mod tokamak</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Brunner, Dan; Labombard, Brian; Kuang, Adam; Terry, Jim; Alcator C-Mod Team</p> <p>2017-10-01</p> <p>The boundary <span class="hlt">heat</span> <span class="hlt">flux</span> width, along with the total power flowing into the boundary, sets the power exhaust challenge for tokamaks. A multi-machine boundary <span class="hlt">heat</span> <span class="hlt">flux</span> width database found that the <span class="hlt">heat</span> <span class="hlt">flux</span> width in H-modes scaled inversely with poloidal magnetic field (Bp) and was independent of machine size. The maximum Bp in the database was 0.8 T, whereas the ITER 15 MA, Q =10 scenario will be 1.2 T. New measurements of the boundary <span class="hlt">heat</span> <span class="hlt">flux</span> width in Alcator C-Mod extend the international database to plasmas with Bp up to 1.3 T. C-Mod was the only experiment able to operate at ITER-level Bp. These new measurements are from over 300 plasma shots in L-, I-, and EDA H-modes spanning essentially the whole operating space in C-Mod. We find that the inverse-Bp dependence of the <span class="hlt">heat</span> <span class="hlt">flux</span> width in H-modes continues to ITER-level Bp, further reinforcing the empirical projection of 500 μm <span class="hlt">heat</span> <span class="hlt">flux</span> width for ITER. We find 50% scatter around the inverse-Bp scaling and are searching for the `hidden variables' causing this scatter. Supported by USDoE award DE-FC02-99ER54512.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19960047459','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19960047459"><span>A Computational Fluid Dynamic and <span class="hlt">Heat</span> Transfer Model for Gaseous Core and Gas Cooled Space Power and Propulsion Reactors</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Anghaie, S.; Chen, G.</p> <p>1996-01-01</p> <p>A computational model based on the axisymmetric, thin-layer Navier-Stokes equations is developed to predict the convective, radiation and conductive <span class="hlt">heat</span> transfer in high temperature space nuclear reactors. An implicit-explicit, finite volume, MacCormack method in conjunction with the Gauss-Seidel line iteration procedure is utilized to solve the thermal and fluid governing equations. Simulation of coolant and propellant flows in these reactors involves the subsonic and supersonic flows of hydrogen, helium and uranium tetrafluoride under variable boundary conditions. An enthalpy-rebalancing scheme is developed and implemented to enhance and accelerate the rate of convergence when a <span class="hlt">wall</span> <span class="hlt">heat</span> <span class="hlt">flux</span> boundary condition is used. The model also incorporated the Baldwin and Lomax two-layer algebraic turbulence scheme for the calculation of the turbulent kinetic energy and eddy diffusivity of energy. The Rosseland diffusion approximation is used to simulate the radiative energy transfer in the optically thick environment of gas core reactors. The computational model is benchmarked with experimental data on flow separation angle and drag force acting on a suspended sphere in a cylindrical tube. The <span class="hlt">heat</span> transfer is validated by comparing the computed results with the standard <span class="hlt">heat</span> transfer correlations predictions. The model is used to simulate flow and <span class="hlt">heat</span> transfer under a variety of design conditions. The effect of internal <span class="hlt">heat</span> generation on the <span class="hlt">heat</span> transfer in the gas core reactors is examined for a variety of power densities, 100 W/cc, 500 W/cc and 1000 W/cc. The maximum temperature, corresponding with the <span class="hlt">heat</span> generation rates, are 2150 K, 2750 K and 3550 K, respectively. This analysis shows that the maximum temperature is strongly dependent on the value of <span class="hlt">heat</span> generation rate. It also indicates that a <span class="hlt">heat</span> generation rate higher than 1000 W/cc is necessary to maintain the gas temperature at about 3500 K, which is typical design temperature required to achieve high</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/5384790-transformations-fluxes-forces-describing-simultaneous-transport-water-heat-unsaturated-porous-media','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/5384790-transformations-fluxes-forces-describing-simultaneous-transport-water-heat-unsaturated-porous-media"><span>Transformations of <span class="hlt">fluxes</span> and forces describing the simultaneous transport of water and <span class="hlt">heat</span> in unsaturated porous media</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>Raats, P.A.C.</p> <p>1975-12-01</p> <p>Balances of mass for the water in N distinct phases and a balance of <span class="hlt">heat</span> for the medium as a whole were formulated. Following Philip and de Vries, it was assumed that the <span class="hlt">flux</span> of water in each phase is proportional to the gradient of the pressure in that phase and that the diffusive component of the <span class="hlt">flux</span> of <span class="hlt">heat</span> is proportional to the gradient of the temperature. Clapeyron equations were used to express the gradient of the pressure in any phase in terms of the gradient of the pressure in a reference state and of the temperature. The referencemore » state may be the water in one of the phases or the water in some measuring device such as a tensiometer or a psychrometer. Expressions for the total <span class="hlt">flux</span> of water and for the diffusive <span class="hlt">flux</span> of <span class="hlt">heat</span> plus the convective <span class="hlt">flux</span> of <span class="hlt">heat</span> associated with the conversion from any phase to the reference state were shown to satisfy the onsager reciprocal relations. A theorem due to Meixner was used to delineate the class of <span class="hlt">fluxes</span> and forces that preserves these relations. In particular, it was shown that if the gradients of water content and temperature are used as the driving forces, the onsager relations are no longer satisfied.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/ADA578387','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA578387"><span>Surface De-Wetting Based Critical <span class="hlt">Heat</span> <span class="hlt">Flux</span> Model Development and Validation</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>2013-02-05</p> <p>the onset of CHF. When the process of dewetting occurs at contact line and micro region, the temperature of dry spots increases, hence dryout areas...increase and the CHF occurs. Finally, we proposed the CHF mechanism based on the surface dewetting and experimental data. 15. SUBJECT TERMS spray...determines the overall <span class="hlt">heat</span> transfer, contact line <span class="hlt">heat</span> transfer <span class="hlt">wall</span> is critically important to trigger the onset of CHF. When the process of dewetting</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013EGUGA..1511209H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013EGUGA..1511209H"><span>Seasonal cycle of oceanic mixed layer and upper-ocean <span class="hlt">heat</span> <span class="hlt">fluxes</span> in the Mediterranean Sea from in-situ observations.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Houpert, Loïc; Testor, Pierre; Durrieu de Madron, Xavier; Estournel, Claude; D'Ortenzio, Fabrizio</p> <p>2013-04-01</p> <p><span class="hlt">Heat</span> <span class="hlt">fluxes</span> across the ocean-atmosphere interface play a crucial role in the upper turbulent mixing. The depth reached by this turbulent mixing is indicated by an homogenization of seawater properties in the surface layer, and is defined as the Mixed Layer Depth (MLD). The thickness of the mixed layer determines also the <span class="hlt">heat</span> content of the layer that directly interacts with the atmosphere. The seasonal variability of these air-sea <span class="hlt">fluxes</span> is crucial in the calculation of <span class="hlt">heat</span> budget. An improvement in the estimate of these <span class="hlt">fluxes</span> is needed for a better understanding of the Mediterranean ocean circulation and climate, in particular in Regional Climate Models. There are few estimations of surface <span class="hlt">heat</span> <span class="hlt">fluxes</span> based on oceanic observations in the Mediterranean, and none of them are based on mixed layer observations. So, we proposed here new estimations of these upper-ocean <span class="hlt">heat</span> <span class="hlt">fluxes</span> based on mixed layer. We present high resolution Mediterranean climatology (0.5°) of the mean MLD based on a comprehensive collection of temperature profiles of last 43 years (1969-2012). The database includes more than 150,000 profiles, merging CTD, XBT, ARGO Profiling floats, and gliders observations. This dataset is first used to describe the seasonal cycle of the mixed layer depth on the whole Mediterranean on a monthly climatological basis. Our analysis discriminates several regions with coherent behaviors, in particular the deep water formation sites, characterized by significant differences in the winter mixing intensity. <span class="hlt">Heat</span> storage rates (HSR) were calculated as the time rate of change of the <span class="hlt">heat</span> content integrated from the surface down to a specific depth that is defined as the MLD plus an integration constant. Monthly climatology of net <span class="hlt">heat</span> <span class="hlt">flux</span> (NHF) from ERA-Interim reanalysis was balanced by the 1°x1° resolution <span class="hlt">heat</span> storage rate climatology. Local <span class="hlt">heat</span> budget balance and seasonal variability in the horizontal <span class="hlt">heat</span> <span class="hlt">flux</span> are then discussed by taking into account</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014APS..DPPGI1003A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014APS..DPPGI1003A"><span>Broadening of the divertor <span class="hlt">heat</span> <span class="hlt">flux</span> footprint with increasing number of ELM filaments in NSTX</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ahn, Joon-Wook</p> <p>2014-10-01</p> <p>We report on the broadening (narrowing) of the ELM <span class="hlt">heat</span> <span class="hlt">flux</span> footprint with increasing (decreasing) number of filamentary striations from in-depth thermography measurements in NSTX. Edge localized modes (ELMs) represent a challenge to future fusion devices, due to the high <span class="hlt">heat</span> <span class="hlt">fluxes</span> on plasma facing surfaces. One ameliorating factor has been that the divertor <span class="hlt">heat</span> <span class="hlt">flux</span> characteristic profile width (λq) has been observed to broaden with the size of ELM, as compared with the inter-ELM λq, which keeps the peak <span class="hlt">heat</span> <span class="hlt">flux</span> (qpeak) from increasing. In contrast, λq has been observed to narrow during ELMs under certain conditions in NSTX, for both naturally occurring and 3-D fields triggered ELMs. Fast thermographic measurements and detailed analysis demonstrate that the ELM λq increases with the number of observed filamentary striations, i . e . , profile narrowing (broadening) occurs when the number of striations is smaller (larger) than 3-4. With profile narrowing, qpeak at ELM peak times is inversely related (proportional) to λq (the ELM size), exacerbating the <span class="hlt">heat</span> <span class="hlt">flux</span> problem. Edge stability analysis shows that NSTX ELMs almost always lie on the current-driven kink/peeling mode side with low toroidal mode number (n = 1--5), consistent with the typical numbers of striations in NSTX (0-8) in comparison 10--15 striations are normally observed in intermediate-n peeling-ballooning ELMs, e.g., from JET. The NSTX characteristics may translate directly to ITER, which is also projected to lie on the low-n kink/peeling stability boundary. This work was supported by the U.S. DOE, Contract DE-AC05-00OR22725 (ORNL) and DE-AC02-09CH11466 (PPPL).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19990023320','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19990023320"><span>Bubble Dynamics, Two-Phase Flow, and Boiling <span class="hlt">Heat</span> Transfer in Microgravity</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Chung, Jacob N.</p> <p>1998-01-01</p> <p> <span class="hlt">wall</span> temperature and <span class="hlt">heat</span> <span class="hlt">flux</span> near the <span class="hlt">wall</span> would add to the database of knowledge which is necessary to understand the mechanisms of nucleate boiling. A heater array has been developed which contains 96 heater elements within a 2.5 mm square area. The temperature of each heater element is held constant by an electronic control system similar to a hot-wire anemometer. The voltage that is being applied to each heater element can be measured and digitized using a high-speed Analog to Digital (A/D) converter, and this digital information can be compiled into a series of <span class="hlt">heat-flux</span> maps. Information for up to 10,000 <span class="hlt">heat</span> <span class="hlt">flux</span> maps can be obtained each second. The heater control system, the A/D system and the heater array construction are described in detail. Results are presented which show that this is an effective method of measuring the local <span class="hlt">heat</span> <span class="hlt">flux</span> during nucleate and transition boiling. <span class="hlt">Heat</span> <span class="hlt">flux</span> maps are obtained for pool boiling in FC-72 on a horizontal surface. Local <span class="hlt">heat</span> <span class="hlt">flux</span> variations are shown to be three to six times larger than variations in the spatially averaged <span class="hlt">heat</span> <span class="hlt">flux</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20100005642','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20100005642"><span>Fabrication and Testing of a Thin-Film <span class="hlt">Heat</span> <span class="hlt">Flux</span> Sensor for a Stirling Convertor</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Wilson, Scott D.; Fralick, Gus c.; Wrbanek, John D.; Sayir, Ali</p> <p>2010-01-01</p> <p>The NASA Glenn Research Center (GRC) has been testing high-efficiency free-piston Stirling convertors for potential use in radioisotope power systems since 1999. Stirling convertors are being operated for many years to demonstrate a radioisotope power system capable of providing reliable power for potential multiyear missions. Techniques used to monitor the convertors for change in performance include measurements of temperature, pressure, energy addition, and energy rejection. Micro-porous bulk insulation is used in the Stirling convertor test setup to minimize the loss of thermal energy from the electric <span class="hlt">heat</span> source to the environment. The insulation is characterized before extended operation, enabling correlation of the net thermal energy addition to the convertor. Aging micro-porous bulk insulation changes insulation efficiency, introducing errors in the correlation for net thermal energy addition. A thin-film <span class="hlt">heat</span> <span class="hlt">flux</span> sensor was designed and fabricated to directly measure the net thermal energy addition to the Stirling convertor. The fabrication techniques include slipcasting and using Physical Vapor Deposition (PVD). One-micron-thick noble metal thermocouples measure temperature on the surface of an alumina ceramic disk and <span class="hlt">heat</span> <span class="hlt">flux</span> is calculated. Fabrication, integration, and test results of a thin-film <span class="hlt">heat</span> <span class="hlt">flux</span> sensor are presented.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016APS..DPPN10136L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016APS..DPPN10136L"><span>Momentum transport and non-local transport in <span class="hlt">heat-flux</span>-driven magnetic reconnection in HEDP</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Liu, Chang; Fox, Will; Bhattacharjee, Amitava</p> <p>2016-10-01</p> <p>Strong magnetic fields are readily generated in high-energy-density plasmas and can affect the <span class="hlt">heat</span> confinement properties of the plasma. Magnetic reconnection can in turn be important as an inverse process, which destroys or reconfigures the magnetic field. Recent theory has demonstrated a novel physics regime for reconnection in high-energy-density plasmas where the magnetic field is advected into the reconnection layer by plasma <span class="hlt">heat</span> <span class="hlt">flux</span> via the Nernst effect. In this work we elucidate the physics of the electron dissipation layer in this <span class="hlt">heat-flux</span>-driven regime. Through fully kinetic simulation and a new generalized Ohm's law, we show that momentum transport due to the <span class="hlt">heat-flux</span>-viscosity effect provides the dissipation mechanism to allow magnetic field line reconnection. Scaling analysis and simulations show that the characteristic width of the current sheet in this regime is several electron mean-free-paths. These results additionally show a coupling between non-local transport and momentum transport, which in turn affects the dynamics of the magnetic field. This work was supported by the U.S. Department of Energy under Contract No. DE-SC0008655.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20030063051','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20030063051"><span>Momentum and <span class="hlt">Heat</span> <span class="hlt">Flux</span> Measurements in the Exhaust of VASIMR using Helium Propellant</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Chavers, D. Gregory; Chang-Diaz, Franklin R.; Irvine, Claude; Squire, Jared P.</p> <p>2003-01-01</p> <p>Interplanetary travel requires propulsion systems that can provide high specific impulse (Isp), while also having sufficient thrust to rapidly accelerate large payloads. One such propulsion system is the Variable Specific Impulse Magneto-plasma Rocket (VASIMR), which creates, <span class="hlt">heats</span>, and ejects plasma to provide variable thrust and Isp, designed to optimally meet the mission requirements. The fraction of the total energy invested in creating the plasma, as compared to the plasma's total kinetic energy, is an important factor in determining the overall system efficiency. In VASIMR, this 'frozen flow loss' is appreciable when at high thrust, but negligible at high Isp. The loss applies to other electric thrusters as well. If some of this energy could be recovered through recombination processes, and reinjected as neutral kinetic energy, the efficiency of VASIMR, in its low Isp/high thrust mode may be improved. An experiment is being conducted to investigate the possibility of recovering some of the energy used to create the plasma by studying the flow characteristics of the charged and neutral particles in the exhaust of the thruster. This paper will cover the measurements of momentum <span class="hlt">flux</span> and <span class="hlt">heat</span> <span class="hlt">flux</span> in the exhaust of the VASIMR test facility using helium as the propellant where the <span class="hlt">heat</span> <span class="hlt">flux</span> is comprised of both kinetic and plasma recombination energy. The <span class="hlt">flux</span> measurements also assist in diagnosing and verifying the plasma conditions in the existing experiment.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018PhFl...30a5108A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018PhFl...30a5108A"><span>Effects of spatial gradients in thermophysical properties on the topology of turbulence in <span class="hlt">heated</span> channel flow of supercritical fluids</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Azih, Chukwudi; Yaras, Metin I.</p> <p>2018-01-01</p> <p>The current literature suggests that large spatial gradients of thermophysical properties, which occur in the vicinity of the pseudo-critical thermodynamic state, may result in significant variations in forced-convection <span class="hlt">heat</span> transfer rates. Specifically, these property gradients induce inertia- and buoyancy-driven phenomena that may enhance or deteriorate the turbulence-dominated <span class="hlt">heat</span> convection process. Through direct numerical simulations, the present study investigates the role of coherent flow structures in channel geometries for non-buoyant and buoyant flows of supercritical water, with buoyant configurations involving <span class="hlt">wall</span>-normal oriented gravitational acceleration and downstream-oriented gravitational acceleration. This sequence of simulations enables the evaluation of the relative contributions of inertial and buoyancy phenomena to <span class="hlt">heat</span> transfer variations. In these simulations, the state of the working fluid is in the vicinity of the pseudo-critical point. The uniform <span class="hlt">wall</span> <span class="hlt">heat</span> <span class="hlt">flux</span> and the channel mass <span class="hlt">flux</span> are specified such that the <span class="hlt">heat</span> to mass <span class="hlt">flux</span> ratio is 3 kJ/kg, with an inflow Reynolds number of 12 000 based on the channel hydraulic diameter, the area-averaged inflow velocity, and fluid properties evaluated at the bulk temperature and pressure of the inflow plane. In the absence of buoyancy forces, notable reductions in the density and viscosity in close proximity of the <span class="hlt">heated</span> <span class="hlt">wall</span> are observed to promote generation of small-scale vortices, with resultant breakdown into smaller scales as they interact with preexisting larger near-<span class="hlt">wall</span> vortices. This interaction results in a reduction in the overall thermal mixing at particular <span class="hlt">wall</span>-normal regions of the channel. Under the influence of <span class="hlt">wall</span>-normal gravitational acceleration, the <span class="hlt">wall</span>-normal density gradients are noted to enhance ejection motions due to baroclinic vorticity generation on the lower <span class="hlt">wall</span>, thus providing additional <span class="hlt">wall</span>-normal thermal mixing. Along the upper <span class="hlt">wall</span>, the same mechanism</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19880009508','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19880009508"><span>Prototype thin-film thermocouple/<span class="hlt">heat-flux</span> sensor for a ceramic-insulated diesel engine</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Kim, Walter S.; Barrows, Richard F.</p> <p>1988-01-01</p> <p>A platinum versus platinum-13 percent rhodium thin-film thermocouple/<span class="hlt">heat-flux</span> sensor was devised and tested in the harsh, high-temperature environment of a ceramic-insulated, low-<span class="hlt">heat</span>-rejection diesel engine. The sensor probe assembly was developed to provide experimental validation of <span class="hlt">heat</span> transfer and thermal analysis methodologies applicable to the insulated diesel engine concept. The thin-film thermocouple configuration was chosen to approximate an uninterrupted chamber surface and provide a 1-D <span class="hlt">heat-flux</span> path through the probe body. The engine test was conducted by Purdue University for Integral Technologies, Inc., under a DOE-funded contract managed by NASA Lewis Research Center. The thin-film sensor performed reliably during 6 to 10 hr of repeated engine runs at indicated mean surface temperatures up to 950 K. However, the sensor suffered partial loss of adhesion in the thin-film thermocouple junction area following maximum cyclic temperature excursions to greater than 1150 K.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018PhPl...25e5905C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018PhPl...25e5905C"><span>Progress towards modeling tokamak boundary plasma turbulence and understanding its role in setting divertor <span class="hlt">heat</span> <span class="hlt">flux</span> widths</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Chen, B.; Xu, X. Q.; Xia, T. Y.; Li, N. M.; Porkolab, M.; Edlund, E.; LaBombard, B.; Terry, J.; Hughes, J. W.; Ye, M. Y.; Wan, Y. X.</p> <p>2018-05-01</p> <p>The <span class="hlt">heat</span> <span class="hlt">flux</span> distributions on divertor targets in H-mode plasmas are serious concerns for future devices. We seek to simulate the tokamak boundary plasma turbulence and <span class="hlt">heat</span> transport in the edge localized mode-suppressed regimes. The improved BOUT++ model shows that not only Ip but also the radial electric field Er plays an important role on the turbulence behavior and sets the <span class="hlt">heat</span> <span class="hlt">flux</span> width. Instead of calculating Er from the pressure gradient term (diamagnetic Er), it is calculated from the plasma transport equations with the sheath potential in the scrape-off layer and the plasma density and temperature profiles inside the separatrix from the experiment. The simulation results with the new Er model have better agreement with the experiment than using the diamagnetic Er model: (1) The electromagnetic turbulence in enhanced Dα H-mode shows the characteristics of quasi-coherent modes (QCMs) and broadband turbulence. The mode spectra are in agreement with the phase contrast imaging data and almost has no change in comparison to the cases which use the diamagnetic Er model; (2) the self-consistent boundary Er is needed for the turbulence simulations to get the consistent <span class="hlt">heat</span> <span class="hlt">flux</span> width with the experiment; (3) the frequencies of the QCMs are proportional to Er, while the divertor <span class="hlt">heat</span> <span class="hlt">flux</span> widths are inversely proportional to Er; and (4) the BOUT++ turbulence simulations yield a similar <span class="hlt">heat</span> <span class="hlt">flux</span> width to the experimental Eich scaling law and the prediction from the Goldston heuristic drift model.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1175043','DOE-PATENT-XML'); return false;" href="https://www.osti.gov/servlets/purl/1175043"><span>Method and apparatus for active control of combustion rate through modulation of <span class="hlt">heat</span> transfer from the combustion chamber <span class="hlt">wall</span></span></a></p> <p><a target="_blank" href="http://www.osti.gov/doepatents">DOEpatents</a></p> <p>Roberts, Jr., Charles E.; Chadwell, Christopher J.</p> <p>2004-09-21</p> <p>The flame propagation rate resulting from a combustion event in the combustion chamber of an internal combustion engine is controlled by modulation of the <span class="hlt">heat</span> transfer from the combustion flame to the combustion chamber <span class="hlt">walls</span>. In one embodiment, <span class="hlt">heat</span> transfer from the combustion flame to the combustion chamber <span class="hlt">walls</span> is mechanically modulated by a movable member that is inserted into, or withdrawn from, the combustion chamber thereby changing the shape of the combustion chamber and the combustion chamber <span class="hlt">wall</span> surface area. In another embodiment, <span class="hlt">heat</span> transfer from the combustion flame to the combustion chamber <span class="hlt">walls</span> is modulated by cooling the surface of a portion of the combustion chamber <span class="hlt">wall</span> that is in close proximity to the area of the combustion chamber where flame speed control is desired.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016RScI...87b3504B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016RScI...87b3504B"><span>Feedback system for divertor impurity seeding based on real-time measurements of surface <span class="hlt">heat</span> <span class="hlt">flux</span> in the Alcator C-Mod tokamak</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Brunner, D.; Burke, W.; Kuang, A. Q.; LaBombard, B.; Lipschultz, B.; Wolfe, S.</p> <p>2016-02-01</p> <p>Mitigation of the intense <span class="hlt">heat</span> <span class="hlt">flux</span> to the divertor is one of the outstanding problems in fusion energy. One technique that has shown promise is impurity seeding, i.e., the injection of low-Z gaseous impurities (typically N2 or Ne) to radiate and dissipate the power before it arrives to the divertor target plate. To this end, the Alcator C-Mod team has created a first-of-its-kind feedback system to control the injection of seed gas based on real-time surface <span class="hlt">heat</span> <span class="hlt">flux</span> measurements. Surface thermocouples provide real-time measurements of the surface temperature response to the plasma <span class="hlt">heat</span> <span class="hlt">flux</span>. The surface temperature measurements are inputted into an analog computer that "solves" the 1-D <span class="hlt">heat</span> transport equation to deliver accurate, real-time signals of the surface <span class="hlt">heat</span> <span class="hlt">flux</span>. The surface <span class="hlt">heat</span> <span class="hlt">flux</span> signals are sent to the C-Mod digital plasma control system, which uses a proportional-integral-derivative (PID) algorithm to control the duty cycle demand to a pulse width modulated piezo valve, which in turn controls the injection of gas into the private <span class="hlt">flux</span> region of the C-Mod divertor. This paper presents the design and implementation of this new feedback system as well as initial results using it to control divertor <span class="hlt">heat</span> <span class="hlt">flux</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26931846','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26931846"><span>Feedback system for divertor impurity seeding based on real-time measurements of surface <span class="hlt">heat</span> <span class="hlt">flux</span> in the Alcator C-Mod tokamak.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Brunner, D; Burke, W; Kuang, A Q; LaBombard, B; Lipschultz, B; Wolfe, S</p> <p>2016-02-01</p> <p>Mitigation of the intense <span class="hlt">heat</span> <span class="hlt">flux</span> to the divertor is one of the outstanding problems in fusion energy. One technique that has shown promise is impurity seeding, i.e., the injection of low-Z gaseous impurities (typically N2 or Ne) to radiate and dissipate the power before it arrives to the divertor target plate. To this end, the Alcator C-Mod team has created a first-of-its-kind feedback system to control the injection of seed gas based on real-time surface <span class="hlt">heat</span> <span class="hlt">flux</span> measurements. Surface thermocouples provide real-time measurements of the surface temperature response to the plasma <span class="hlt">heat</span> <span class="hlt">flux</span>. The surface temperature measurements are inputted into an analog computer that "solves" the 1-D <span class="hlt">heat</span> transport equation to deliver accurate, real-time signals of the surface <span class="hlt">heat</span> <span class="hlt">flux</span>. The surface <span class="hlt">heat</span> <span class="hlt">flux</span> signals are sent to the C-Mod digital plasma control system, which uses a proportional-integral-derivative (PID) algorithm to control the duty cycle demand to a pulse width modulated piezo valve, which in turn controls the injection of gas into the private <span class="hlt">flux</span> region of the C-Mod divertor. This paper presents the design and implementation of this new feedback system as well as initial results using it to control divertor <span class="hlt">heat</span> <span class="hlt">flux</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_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/2018ResPh...8..569I','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018ResPh...8..569I"><span>Three dimensional rotating flow of Powell-Eyring nanofluid with non-Fourier's <span class="hlt">heat</span> <span class="hlt">flux</span> and non-Fick's mass <span class="hlt">flux</span> theory</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ibrahim, Wubshet</p> <p>2018-03-01</p> <p>This article numerically examines three dimensional boundary layer flow of a rotating Powell-Eyring nanofluid. In modeling <span class="hlt">heat</span> transfer processes, non-Fourier <span class="hlt">heat</span> <span class="hlt">flux</span> theory and for mass transfer non-Fick's mass <span class="hlt">flux</span> theory are employed. This theory is recently re-initiated and it becomes the active research area to resolves some drawback associated with the famous Fourier <span class="hlt">heat</span> <span class="hlt">flux</span> and mass <span class="hlt">flux</span> theory. The mathematical model of the flow problem is a system of non-linear partial differential equations which are obtained using the boundary layer analysis. The non-linear partial differential equations have been transformed into non-linear high order ordinary differential equations using similarity transformation. Employing bvp4c algorithm from matlab software routine, the numerical solution of the transformed ordinary differential equations is obtained. The governing equations are constrained by parameters such as rotation parameter λ , the non-Newtonian parameter N, dimensionless thermal relaxation and concentration relaxation parameters δt and δc . The impacts of these parameters have been discussed thoroughly and illustrated using graphs and tables. The findings show that thermal relaxation time δt reduces the thermal and concentration boundary layer thickness. Further, the results reveal that the rotational parameter λ has the effect of decreasing the velocity boundary layer thickness in both x and y directions. Further examination pinpoints that the skin friction coefficient along x-axis is an increasing and skin friction coefficient along y-axis is a decreasing function of rotation parameter λ . Furthermore, the non-Newtonian fluid parameter N has the characteristic of reducing the amount of local Nusselt numbers -f″ (0) and -g″ (0) both in x and y -directions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016ApPhL.108d2405R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016ApPhL.108d2405R"><span>Domain <span class="hlt">wall</span> dynamics along curved strips under current pulses: The influence of Joule <span class="hlt">heating</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Raposo, Victor; Moretti, Simone; Hernandez, Maria Auxiliadora; Martinez, Eduardo</p> <p>2016-01-01</p> <p>The current-induced domain <span class="hlt">wall</span> dynamics along curved ferromagnetic strips is studied by coupling the magnetization dynamics to the <span class="hlt">heat</span> transport. Permalloy strips with uniform and non-uniform cross section are evaluated, taking into account the influence of the electrical contacts used to inject the current pulses and the substrate on top of which the ferromagnetic strip is sited. Micromagnetic simulations indicate that the geometry and the non-ferromagnetic materials in the system play a significant role in the current-induced domain <span class="hlt">wall</span> dynamics. Due to the natural pinning, domain <span class="hlt">walls</span> are hardly affected by the spin-transfer torques when placed in uniform cross section strips under current pulses with reduced magnitude. On the contrary, the current-induced domain <span class="hlt">wall</span> displacement is significantly different in strips with non-uniform cross section, where thermal gradients emerge as due to the Joule <span class="hlt">heating</span>. It is found that these thermal gradients can assist or act against the pure spin-transfer torques, in agreement with the recent experimental observations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015SJCE...23b..19H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015SJCE...23b..19H"><span>Thermal Response Of An Aerated Concrete <span class="hlt">Wall</span> With Micro-Encapsulated Phase Change Material</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Halúzová, Dušana</p> <p>2015-06-01</p> <p>For many years Phase Change Materials (PCM) have attracted attention due to their ability to store large amounts of thermal energy. This property makes them a candidate for the use of passive <span class="hlt">heat</span> storage. In many applications, they are used to avoid the overheating of the temperature of an indoor environment. This paper describes the behavior of phase change materials that are inbuilt in aerated concrete blocks. Two building samples of an aerated concrete <span class="hlt">wall</span> were measured in laboratory equipment called "twin-boxes". The first box consists of a traditional aerated concrete <span class="hlt">wall</span>; the second one has additional PCM micro-encapsulated in the <span class="hlt">wall</span>. The <span class="hlt">heat</span> <span class="hlt">flux</span> through the <span class="hlt">wall</span> was measured and compared to simulation results modeled in the ESP-r program. This experimental measurement provides a foundation for a model that can be used to analyze further building constructions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018MicST.tmp...45F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018MicST.tmp...45F"><span>Numerical Study of Single Bubble Growth on and Departure from a Horizontal Superheated <span class="hlt">Wall</span> by Three-dimensional Lattice Boltzmann Method</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Feng, Yuan; Li, Hui-Xiong; Guo, Kai-Kai; Zhao, Jian-Fu; Wang, Tai</p> <p>2018-05-01</p> <p>A three-dimensional hybrid lattice Boltzmann method was used to simulate the progress of a single bubble's growth and departure from a horizontal superheated <span class="hlt">wall</span>. The evolutionary process of the bubble shapes and also the temperature fields during pool nucleate boiling were obtained and the influence of the gravitational acceleration on the bubble departure diameter (BDD), the bubble release frequency (BRF) and the <span class="hlt">heat</span> <span class="hlt">flux</span> on the superheated <span class="hlt">wall</span> was analyzed. The simulation results obtained by the present three-dimensional numerical studies demonstrate that the BDD is proportional to g^{-0.301}, the BRF is proportional to g^{-0.58}, and the averaged <span class="hlt">wall</span> <span class="hlt">heat</span> <span class="hlt">flux</span> is proportional to g^{0.201}, where g is the gravitational acceleration. These results are in good agreement with the common-used experimental correlations, indicating the rationality of the present numerical model and results.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2005JNuM..337..761L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2005JNuM..337..761L"><span>Simulation of tokamak armour erosion and plasma contamination at intense transient <span class="hlt">heat</span> <span class="hlt">fluxes</span> in ITER</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Landman, I. S.; Bazylev, B. N.; Garkusha, I. E.; Loarte, A.; Pestchanyi, S. E.; Safronov, V. M.</p> <p>2005-03-01</p> <p>For ITER, the potential material damage of plasma facing tungsten-, CFC-, or beryllium components during transient processes such as ELMs or mitigated disruptions are simulated numerically using the MHD code FOREV-2D and the melt motion code MEMOS-1.5D for a <span class="hlt">heat</span> deposition in the range of 0.5-3 MJ/m 2 on the time scale of 0.1-1 ms. Such loads can cause significant evaporation at the target surface and a contamination of the SOL by the ions of evaporated material. Results are presented on carbon plasma dynamics in toroidal geometry and on radiation <span class="hlt">fluxes</span> from the SOL carbon ions obtained with FOREV-2D. The validation of MEMOS-1.5D against the plasma gun tokamak simulators MK-200UG and QSPA-Kh50, based on the tungsten melting threshold, is described. Simulations with MEMOS-1.5D for a beryllium first <span class="hlt">wall</span> that provide important details about the melt motion dynamics and typical features of the damage are reported.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1240418-lattice-boltzmann-modeling-boiling-heat-transfer-boiling-curve-effects-wettability','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1240418-lattice-boltzmann-modeling-boiling-heat-transfer-boiling-curve-effects-wettability"><span>Lattice Boltzmann modeling of boiling <span class="hlt">heat</span> transfer: The boiling curve and the effects of wettability</span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Li, Q.; Kang, Q. J.; Francois, M. M.; ...</p> <p>2015-03-03</p> <p>A hybrid thermal lattice Boltzmann (LB) model is presented to simulate thermal multiphase flows with phase change based on an improved pseudopotential LB approach (Li et al., 2013). The present model does not suffer from the spurious term caused by the forcing-term effect, which was encountered in some previous thermal LB models for liquid–vapor phase change. Using the model, the liquid–vapor boiling process is simulated. The boiling curve together with the three boiling stages (nucleate boiling, transition boiling, and film boiling) is numerically reproduced in the LB community for the first time. The numerical results show that the basic featuresmore » and the fundamental characteristics of boiling <span class="hlt">heat</span> transfer are well captured, such as the severe fluctuation of transient <span class="hlt">heat</span> <span class="hlt">flux</span> in the transition boiling and the feature that the maximum <span class="hlt">heat</span> transfer coefficient lies at a lower <span class="hlt">wall</span> superheat than that of the maximum <span class="hlt">heat</span> <span class="hlt">flux</span>. Moreover, the effects of the <span class="hlt">heating</span> surface wettability on boiling <span class="hlt">heat</span> transfer are investigated. It is found that an increase in contact angle promotes the onset of boiling but reduces the critical <span class="hlt">heat</span> <span class="hlt">flux</span>, and makes the boiling process enter into the film boiling regime at a lower <span class="hlt">wall</span> superheat, which is consistent with the findings from experimental studies.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20120015092','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20120015092"><span>Convective <span class="hlt">Heat</span> Transfer Scaling of Ignition Delay and Burning Rate with <span class="hlt">Heat</span> <span class="hlt">Flux</span> and Stretch Rate in the Equivalent Low Stretch Apparatus</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Olson, Sandra</p> <p>2011-01-01</p> <p>To better evaluate the buoyant contributions to the convective cooling (or <span class="hlt">heating</span>) inherent in normal-gravity material flammability test methods, we derive a convective <span class="hlt">heat</span> transfer correlation that can be used to account for the forced convective stretch effects on the net radiant <span class="hlt">heat</span> <span class="hlt">flux</span> for both ignition delay time and burning rate. The Equivalent Low Stretch Apparatus (ELSA) uses an inverted cone heater to minimize buoyant effects while at the same time providing a forced stagnation flow on the sample, which ignites and burns as a ceiling fire. Ignition delay and burning rate data is correlated with incident <span class="hlt">heat</span> <span class="hlt">flux</span> and convective <span class="hlt">heat</span> transfer and compared to results from other test methods and fuel geometries using similarity to determine the equivalent stretch rates and thus convective cooling (or <span class="hlt">heating</span>) rates for those geometries. With this correlation methodology, buoyant effects inherent in normal gravity material flammability test methods can be estimated, to better apply the test results to low stretch environments relevant to spacecraft material selection.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013EGUGA..15.8245V','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013EGUGA..15.8245V"><span>Estimating Antarctic Geothermal <span class="hlt">Heat</span> <span class="hlt">Flux</span> using Gravity Inversion</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Vaughan, Alan P. M.; Kusznir, Nick J.; Ferraccioli, Fausto; Leat, Phil T.; Jordan, Tom A. R. M.; Purucker, Michael E.; Golynsky, A. V.; Sasha Rogozhina, Irina</p> <p>2013-04-01</p> <p>Geothermal <span class="hlt">heat</span> <span class="hlt">flux</span> (GHF) in Antarctica is very poorly known. We have determined (Vaughan et al. 2012) top basement <span class="hlt">heat</span>-flow for Antarctica and adjacent rifted continental margins using gravity inversion mapping of crustal thickness and continental lithosphere thinning (Chappell & Kusznir 2008). Continental lithosphere thinning and post-breakup residual thicknesses of continental crust determined from gravity inversion have been used to predict the preservation of continental crustal radiogenic <span class="hlt">heat</span> productivity and the transient lithosphere <span class="hlt">heat</span>-flow contribution within thermally equilibrating rifted continental and oceanic lithosphere. The sensitivity of present-day Antarctic top basement <span class="hlt">heat</span>-flow to initial continental radiogenic <span class="hlt">heat</span> productivity, continental rift and margin breakup age has been examined. Knowing GHF distribution for East Antarctica and the Gamburtsev Subglacial Mountains (GSM) region in particular is critical because: 1) The GSM likely acted as key nucleation point for the East Antarctic Ice Sheet (EAIS); 2) the region may contain the oldest ice of the EAIS - a prime target for future ice core drilling; 3) GHF is important to understand proposed ice accretion at the base of the EAIS in the GSM and its links to sub-ice hydrology (Bell et al. 2011). An integrated multi-dataset-based GHF model for East Antarctica is planned that will resolve the wide range of estimates previously published using single datasets. The new map and existing GHF distribution estimates available for Antarctica will be evaluated using direct ice temperature measurements obtained from deep ice cores, estimates of GHF derived from subglacial lakes, and a thermodynamic ice-sheet model of the Antarctic Ice Sheet driven by past climate reconstructions and each of analysed <span class="hlt">heat</span> flow maps, as has recently been done for the Greenland region (Rogozhina et al. 2012). References Bell, R.E., Ferraccioli, F., Creyts, T.T., Braaten, D., Corr, H., Das, I., Damaske, D., Frearson, N</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27910364','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27910364"><span>Spectroscopic imaging of limiter <span class="hlt">heat</span> and particle <span class="hlt">fluxes</span> and the resulting impurity sources during Wendelstein 7-X startup plasmas.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Stephey, L; Wurden, G A; Schmitz, O; Frerichs, H; Effenberg, F; Biedermann, C; Harris, J; König, R; Kornejew, P; Krychowiak, M; Unterberg, E A</p> <p>2016-11-01</p> <p>A combined IR and visible camera system [G. A. Wurden et al., "A high resolution IR/visible imaging system for the W7-X limiter," Rev. Sci. Instrum. (these proceedings)] and a filterscope system [R. J. Colchin et al., Rev. Sci. Instrum. 74, 2068 (2003)] were implemented together to obtain spectroscopic data of limiter and first <span class="hlt">wall</span> recycling and impurity sources during Wendelstein 7-X startup plasmas. Both systems together provided excellent temporal and spatial spectroscopic resolution of limiter 3. Narrowband interference filters in front of the camera yielded C-III and H α photon <span class="hlt">flux</span>, and the filterscope system provided H α , H β , He-I, He-II, C-II, and visible bremsstrahlung data. The filterscopes made additional measurements of several points on the W7-X vacuum vessel to yield <span class="hlt">wall</span> recycling <span class="hlt">fluxes</span>. The resulting photon <span class="hlt">flux</span> from both the visible camera and filterscopes can then be compared to an EMC3-EIRENE synthetic diagnostic [H. Frerichs et al., "Synthetic plasma edge diagnostics for EMC3-EIRENE, highlighted for Wendelstein 7-X," Rev. Sci. Instrum. (these proceedings)] to infer both a limiter particle <span class="hlt">flux</span> and <span class="hlt">wall</span> particle <span class="hlt">flux</span>, both of which will ultimately be used to infer the complete particle balance and particle confinement time τ P .</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5784416','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5784416"><span>Hindcasting the Madden‐Julian Oscillation With a New Parameterization of Surface <span class="hlt">Heat</span> <span class="hlt">Fluxes</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>Wang, Jingfeng; Lin, Wenshi</p> <p>2017-01-01</p> <p>Abstract The recently developed maximum entropy production (MEP) model, an alternative parameterization of surface <span class="hlt">heat</span> <span class="hlt">fluxes</span>, is incorporated into the Weather Research and Forecasting (WRF) model. A pair of WRF cloud‐resolving experiments (5 km grids) using the bulk transfer model (WRF default) and the MEP model of surface <span class="hlt">heat</span> <span class="hlt">fluxes</span> are performed to hindcast the October Madden‐Julian oscillation (MJO) event observed during the 2011 Dynamics of the MJO (DYNAMO) field campaign. The simulated surface latent and sensible <span class="hlt">heat</span> <span class="hlt">fluxes</span> in the MEP and bulk transfer model runs are in general consistent with in situ observations from two research vessels. Compared to the bulk transfer model, the convection envelope is strengthened in the MEP run and shows a more coherent propagation over the Maritime Continent. The simulated precipitable water in the MEP run is in closer agreement with the observations. Precipitation in the MEP run is enhanced during the active phase of the MJO with significantly reduced regional dry and wet biases. Large‐scale ocean evaporation is stronger in the MEP run leading to stronger boundary layer moistening to the east of the convection center, which facilitates the eastward propagation of the MJO. PMID:29399269</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19780018913&hterms=heat+exchange&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D90%26Ntt%3Dheat%2Bexchange','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19780018913&hterms=heat+exchange&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D90%26Ntt%3Dheat%2Bexchange"><span><span class="hlt">Heat</span> transfer evaluation in a plasma core reactor</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Smith, D. E.; Smith, T. M.; Stoenescu, M. L.</p> <p>1976-01-01</p> <p>Numerical evaluations of <span class="hlt">heat</span> transfer in a fissioning uranium plasma core reactor cavity, operating with seeded hydrogen propellant, was performed. A two-dimensional analysis is based on an assumed flow pattern and cavity <span class="hlt">wall</span> <span class="hlt">heat</span> exchange rate. Various iterative schemes were required by the nature of the radiative field and by the solid seed vaporization. Approximate formulations of the radiative <span class="hlt">heat</span> <span class="hlt">flux</span> are generally used, due to the complexity of the solution of a rigorously formulated problem. The present work analyzes the sensitivity of the results with respect to approximations of the radiative field, geometry, seed vaporization coefficients and flow pattern. The results present temperature, <span class="hlt">heat</span> <span class="hlt">flux</span>, density and optical depth distributions in the reactor cavity, acceptable simplifying assumptions, and iterative schemes. The present calculations, performed in cartesian and spherical coordinates, are applicable to any most general <span class="hlt">heat</span> transfer problem.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018InvPr..34g5008I','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018InvPr..34g5008I"><span>Ensemble-marginalized Kalman filter for linear time-dependent PDEs with noisy boundary conditions: application to <span class="hlt">heat</span> transfer in building <span class="hlt">walls</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Iglesias, Marco; Sawlan, Zaid; Scavino, Marco; Tempone, Raúl; Wood, Christopher</p> <p>2018-07-01</p> <p>In this work, we present the ensemble-marginalized Kalman filter (EnMKF), a sequential algorithm analogous to our previously proposed approach (Ruggeri et al 2017 Bayesian Anal. 12 407–33, Iglesias et al 2018 Int. J. <span class="hlt">Heat</span> Mass Transfer 116 417–31), for estimating the state and parameters of linear parabolic partial differential equations in initial-boundary value problems when the boundary data are noisy. We apply EnMKF to infer the thermal properties of building <span class="hlt">walls</span> and to estimate the corresponding <span class="hlt">heat</span> <span class="hlt">flux</span> from real and synthetic data. Compared with a modified ensemble Kalman filter (EnKF) that is not marginalized, EnMKF reduces the bias error, avoids the collapse of the ensemble without needing to add inflation, and converges to the mean field posterior using or less of the ensemble size required by EnKF. According to our results, the marginalization technique in EnMKF is key to performance improvement with smaller ensembles at any fixed time.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2003EAEJA.....5126S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2003EAEJA.....5126S"><span>Evaluation of parameterization for turbulent <span class="hlt">fluxes</span> of momentum and <span class="hlt">heat</span> in stably stratified surface layers</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sodemann, H.; Foken, Th.</p> <p>2003-04-01</p> <p>General Circulation Models calculate the energy exchange between surface and atmosphere by means of parameterisations for turbulent <span class="hlt">fluxes</span> of momentum and <span class="hlt">heat</span> in the surface layer. However, currently implemented parameterisations after Louis (1979) create large discrepancies between predictions and observational data, especially in stably stratified surface layers. This work evaluates a new surface layer parameterisation proposed by Zilitinkevich et al. (2002), which was specifically developed to improve energy <span class="hlt">flux</span> predictions in stable stratification. The evaluation comprises a detailed study of important surface layer characteristics, a sensitivity study of the parameterisation, and a direct comparison to observational data from Antarctica and predictions by the Louis (1979) parameterisation. The stability structure of the stable surface layer was found to be very complex, and strongly influenced <span class="hlt">fluxes</span> in the surface layer. The sensitivity study revealed that the new parameterisation depends strongly on the ratio between roughness length and roughness temperature, which were both observed to be very variable parameters. The comparison between predictions and measurements showed good agreement for momentum <span class="hlt">fluxes</span>, but large discrepancies for <span class="hlt">heat</span> <span class="hlt">fluxes</span>. A stability dependent evaluation of selected data showed better agreement for the new parameterisation of Zilitinkevich et al. (2002) than for the Louis (1979) scheme. Nevertheless, this comparison underlines the need for more detailed and physically sound concepts for parameterisations of <span class="hlt">heat</span> <span class="hlt">fluxes</span> in stably stratified surface layers. Zilitinkevich, S. S., V. Perov and J. C. King (2002). "Near-surface turbulent <span class="hlt">fluxes</span> in stable stratification: Calculation techniques for use in General Circulation Models." Q. J. R. Meteorol. Soc. 128(583): 1571--1587. Louis, J. F. (1979). "A Parametric Model of Vertical Eddy <span class="hlt">Fluxes</span> in the Atmosphere." Bound.-Layer Meteor. 17(2): 187--202.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70033363','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70033363"><span>Modern perspectives on measuring and interpreting seafloor <span class="hlt">heat</span> <span class="hlt">flux</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>Harris, Reid N.; Fisher, A.; Ruppel, C.; Martinez, F.</p> <p>2008-01-01</p> <p>There has been a resurgence of interest in marine <span class="hlt">heat</span> flow in the past 10–15 years, coinciding with fundamental achievements in understanding the Earth's thermal state and quantifying the dynamics and impacts of material and energy <span class="hlt">fluxes</span> within and between the lithosphere and hydrosphere. At the same time, technical capabilities have dwindled to the point that no U.S. academic institution currently operates a seagoing <span class="hlt">heat</span> flow capacity.In September 2007, a workshop was convened in Salt Lake City with sponsorship from the U.S. National Science Foundation (NSF) and participation by scientists and engineers from North America, Europe, and Asia. The primary goals of the workshop were to (1) assess high-priority scientific and technical needs and (2) to evaluate options for developing and maintaining essential capabilities in marine <span class="hlt">heat</span> flow for the U.S. scientific community.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4199907','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4199907"><span>Estimating Energy Expenditure Using <span class="hlt">Heat</span> <span class="hlt">Flux</span> Measured at Single Body Site</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Lyden, Kate; Swibas, Tracy; Catenacci, Victoria; Guo, Ruixin; Szuminsky, Neil; Melanson, Edward L.</p> <p>2014-01-01</p> <p>Introduction The Personal Calorie Monitor (PCM) is a portable direct calorimeter that estimates energy expenditure (EE) from measured <span class="hlt">heat</span> <span class="hlt">flux</span> (i.e. the sum of conductive, convective, radiative, and evaporative). Purpose The primary aim of this study was to compare EE estimated from measures of <span class="hlt">heat</span> <span class="hlt">flux</span> to indirect calorimetry in a thermoneutral environment (26°C). A secondary aim was to determine if exposure to ambient temperature below thermoneutral (19°C) influences the accuracy of the PCM. Methods 34 Adults (mean±SD, age = 28±5 y, body mass index = 22.9±2.6 kg.m2) were studied for 5 h in a whole-room indirect calorimeter (IC) in thermoneutral and cool conditions. Participants wore the PCM on their upper arm and completed two, 20-minute treadmill-walking bouts (0% grade, 3 mph). The remaining time was spent sedentary (e.g., watching television, using a computer). Results In thermoneutral, EE (mean (95% CI)) measured by IC and PCM was 560.0 (526.5, 593.5) and 623.3 (535.5, 711.1) kcals, respectively. In cool, EE measured by IC and PCM was 572.5 (540.9, 604.0) and 745.5 (668.1, 822.8) kcals, respectively. Under thermoneutral conditions, mean PCM minute-by-minute EE tracked closely with IC, resulting in a small, non-significant bias (63 kcals (−5.8, 132.4)). During cool conditions, mean PCM minute-by-minute EE did not track IC, resulting in a large bias (173.0 (93.9, 252.1)) (p<0.001). Conclusion This study demonstrated the validity of using measured <span class="hlt">heat</span> <span class="hlt">flux</span> to estimate EE. However, accuracy may be impaired in cool conditions, possibly due to excess <span class="hlt">heat</span> loss from the exposed limbs. PMID:24811326</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19950024426','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19950024426"><span>Diamond thin film temperature and <span class="hlt">heat-flux</span> sensors</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Aslam, M.; Yang, G. S.; Masood, A.; Fredricks, R.</p> <p>1995-01-01</p> <p>Diamond film temperature and <span class="hlt">heat-flux</span> sensors are developed using a technology compatible with silicon integrated circuit processing. The technology involves diamond nucleation, patterning, doping, and metallization. Multi-sensor test chips were designed and fabricated to study the thermistor behavior. The minimum feature size (device width) for 1st and 2nd generation chips are 160 and 5 micron, respectively. The p-type diamond thermistors on the 1st generation test chip show temperature and response time ranges of 80-1270 K and 0.29-25 microseconds, respectively. An array of diamond thermistors, acting as <span class="hlt">heat</span> <span class="hlt">flux</span> sensors, was successfully fabricated on an oxidized Si rod with a diameter of 1 cm. Some problems were encountered in the patterning of the Pt/Ti ohmic contacts on the rod, due mainly to the surface roughness of the diamond film. The use of thermistors with a minimum width of 5 micron (to improve the spatial resolution of measurement) resulted in lithographic problems related to surface roughness of diamond films. We improved the mean surface roughness from 124 nm to 30 nm by using an ultra high nucleation density of 10(exp 11)/sq cm. To deposit thermistors with such small dimensions on a curved surface, a new 3-D diamond patterning technique is currently under development. This involves writing a diamond seed pattern directly on the curved surface by a computer-controlled nozzle.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015EGUGA..17.1791W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015EGUGA..17.1791W"><span>Modelling storm development and the impact when introducing waves, sea spray and <span class="hlt">heat</span> <span class="hlt">fluxes</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wu, Lichuan; Rutgersson, Anna; Sahlée, Erik</p> <p>2015-04-01</p> <p>In high wind speed conditions, sea spray generated due to intensity breaking waves have big influence on the wind stress and <span class="hlt">heat</span> <span class="hlt">fluxes</span>. Measurements show that drag coefficient will decrease in high wind speed. Sea spray generation function (SSGF), an important term of wind stress parameterization in high wind speed, usually treated as a function of wind speed/friction velocity. In this study, we introduce a wave state depended SSGG and wave age depended Charnock number into a high wind speed wind stress parameterization (Kudryavtsev et al., 2011; 2012). The proposed wind stress parameterization and sea spray <span class="hlt">heat</span> <span class="hlt">fluxes</span> parameterization from Andreas et al., (2014) were applied to an atmosphere-wave coupled model to test on four storm cases. Compared with measurements from the FINO1 platform in the North Sea, the new wind stress parameterization can reduce the forecast errors of wind in high wind speed range, but not in low wind speed. Only sea spray impacted on wind stress, it will intensify the storms (minimum sea level pressure and maximum wind speed) and lower the air temperature (increase the errors). Only the sea spray impacted on the <span class="hlt">heat</span> <span class="hlt">fluxes</span>, it can improve the model performance on storm tracks and the air temperature, but not change much in the storm intensity. If both of sea spray impacted on the wind stress and <span class="hlt">heat</span> <span class="hlt">fluxes</span> are taken into account, it has the best performance in all the experiment for minimum sea level pressure and maximum wind speed and air temperature. Andreas, E. L., Mahrt, L., and Vickers, D. (2014). An improved bulk air-sea surface <span class="hlt">flux</span> algorithm, including spray-mediated transfer. Quarterly Journal of the Royal Meteorological Society. Kudryavtsev, V. and Makin, V. (2011). Impact of ocean spray on the dynamics of the marine atmospheric boundary layer. Boundary-layer meteorology, 140(3):383-410. Kudryavtsev, V., Makin, V., and S, Z. (2012). On the sea-surface drag and <span class="hlt">heat</span>/mass transfer at strong winds. Technical report, Royal</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016APS..DPPT10081S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016APS..DPPT10081S"><span>Particle and <span class="hlt">heat</span> <span class="hlt">flux</span> estimates in Proto-MPEX in Helicon Mode with IR imaging</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Showers, M. A.; Biewer, T. M.; Caughman, J. B. O.; Donovan, D. C.; Goulding, R. H.; Rapp, J.</p> <p>2016-10-01</p> <p>The Prototype Material Plasma Exposure eXperiment (Proto-MPEX) at Oak Ridge National Laboratory (ORNL) is a linear plasma device developing the plasma source concept for the Material Plasma Exposure eXperiment (MPEX), which will address plasma material interaction (PMI) science for future fusion reactors. To better understand how and where energy is being lost from the Proto-MPEX plasma during ``helicon mode'' operations, particle and <span class="hlt">heat</span> <span class="hlt">fluxes</span> are quantified at multiple locations along the machine length. Relevant diagnostics include infrared (IR) cameras, four double Langmuir probes (LPs), and in-vessel thermocouples (TCs). The IR cameras provide temperature measurements of Proto-MPEX's plasma-facing dump and target plates, located on either end of the machine. The change in surface temperature is measured over the duration of the plasma shot to determine the <span class="hlt">heat</span> <span class="hlt">flux</span> hitting the plates. The IR cameras additionally provide 2-D thermal load distribution images of these plates, highlighting Proto-MPEX plasma behaviors, such as hot spots. The LPs and TCs provide additional plasma measurements required to determine particle and <span class="hlt">heat</span> <span class="hlt">fluxes</span>. Quantifying axial variations in <span class="hlt">fluxes</span> will help identify machine operating parameters that will improve Proto-MPEX's performance, increasing its PMI research capabilities. This work was supported by the U.S. D.O.E. contract DE-AC05-00OR22725.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20050217477','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20050217477"><span>Flow-Boiling Critical <span class="hlt">Heat</span> <span class="hlt">Flux</span> Experiments Performed in Reduced Gravity</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Hasan, Mohammad M.; Mudawar, Issam</p> <p>2005-01-01</p> <p>Poor understanding of flow boiling in microgravity has recently emerged as a key obstacle to the development of many types of power generation and advanced life support systems intended for space exploration. The critical <span class="hlt">heat</span> <span class="hlt">flux</span> (CHF) is perhaps the most important thermal design parameter for boiling systems involving both heatflux-controlled devices and intense <span class="hlt">heat</span> removal. Exceeding the CHF limit can lead to permanent damage, including physical burnout of the <span class="hlt">heat</span>-dissipating device. The importance of the CHF limit creates an urgent need to develop predictive design tools to ensure both the safe and reliable operation of a two-phase thermal management system under the reduced-gravity (like that on the Moon and Mars) and microgravity environments of space. At present, very limited information is available on flow-boiling <span class="hlt">heat</span> transfer and the CHF under these conditions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015ThEng..62...88B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015ThEng..62...88B"><span>Critical <span class="hlt">heat</span> <span class="hlt">flux</span> for water boiling in channels. Modern state, typical regularities, unsolved problems, and ways for solving them (a review)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bobkov, V. P.</p> <p>2015-02-01</p> <p>Some general matters concerned with description of burnout in channels are outlined. Data obtained from experimental investigations on critical <span class="hlt">heat</span> <span class="hlt">fluxes</span> (CHF) in different channels, CHF data banks, the main determining parameters, CHF basic dependences, and a system of correction functions are discussed. Two methods for estimating the CHF description errors are analyzed. The influence of operating parameters, transverse sizes of channels, and conditions at their inlet are analyzed. The effects of <span class="hlt">heat</span>-transfer surface shape and <span class="hlt">heat</span> supply arrangement are considered for concentric annular channels. The notions of a thermal boundary layer and an elementary thermal cell during burnout in channels with an intricate cross section are defined. New notions for describing CHF in rod assemblies are introduced: bundle effect, thermal misalignment, assembly-section-averaged and local parameters (for an elementary cell), cell-wise CHF analysis in bundles, and standard and nonstandard cells. Possible influence of <span class="hlt">wall</span> thermophysical properties on CHF in dense assemblies and other effects are considered. Thermal interaction of nonequivalent cells and the effect of <span class="hlt">heat</span> supply arrangement over the cell perimeter are analyzed. Special attention is paid to description of the effect the <span class="hlt">heat</span> release nonuniformity along the channels has on CHF. Objectives to be pursued by studies of CHF in channels of different cross-section shapes are formulated.</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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