Sample records for based fluid modeling

  1. Model identification methodology for fluid-based inerters

    NASA Astrophysics Data System (ADS)

    Liu, Xiaofu; Jiang, Jason Zheng; Titurus, Branislav; Harrison, Andrew

    2018-06-01

    Inerter is the mechanical dual of the capacitor via the force-current analogy. It has the property that the force across the terminals is proportional to their relative acceleration. Compared with flywheel-based inerters, fluid-based forms have advantages of improved durability, inherent damping and simplicity of design. In order to improve the understanding of the physical behaviour of this fluid-based device, especially caused by the hydraulic resistance and inertial effects in the external tube, this work proposes a comprehensive model identification methodology. Firstly, a modelling procedure is established, which allows the topological arrangement of the mechanical networks to be obtained by mapping the damping, inertance and stiffness effects directly to their respective hydraulic counterparts. Secondly, an experimental sequence is followed, which separates the identification of friction, stiffness and various damping effects. Furthermore, an experimental set-up is introduced, where two pressure gauges are used to accurately measure the pressure drop across the external tube. The theoretical models with improved confidence are obtained using the proposed methodology for a helical-tube fluid inerter prototype. The sources of remaining discrepancies are further analysed.

  2. Multiscale turbulence models based on convected fluid microstructure

    NASA Astrophysics Data System (ADS)

    Holm, Darryl D.; Tronci, Cesare

    2012-11-01

    The Euler-Poincaré approach to complex fluids is used to derive multiscale equations for computationally modeling Euler flows as a basis for modeling turbulence. The model is based on a kinematic sweeping ansatz (KSA) which assumes that the mean fluid flow serves as a Lagrangian frame of motion for the fluctuation dynamics. Thus, we regard the motion of a fluid parcel on the computationally resolvable length scales as a moving Lagrange coordinate for the fluctuating (zero-mean) motion of fluid parcels at the unresolved scales. Even in the simplest two-scale version on which we concentrate here, the contributions of the fluctuating motion under the KSA to the mean motion yields a system of equations that extends known results and appears to be suitable for modeling nonlinear backscatter (energy transfer from smaller to larger scales) in turbulence using multiscale methods.

  3. Physically-Based Modelling and Real-Time Simulation of Fluids.

    NASA Astrophysics Data System (ADS)

    Chen, Jim Xiong

    1995-01-01

    Simulating physically realistic complex fluid behaviors presents an extremely challenging problem for computer graphics researchers. Such behaviors include the effects of driving boats through water, blending differently colored fluids, rain falling and flowing on a terrain, fluids interacting in a Distributed Interactive Simulation (DIS), etc. Such capabilities are useful in computer art, advertising, education, entertainment, and training. We present a new method for physically-based modeling and real-time simulation of fluids in computer graphics and dynamic virtual environments. By solving the 2D Navier -Stokes equations using a CFD method, we map the surface into 3D using the corresponding pressures in the fluid flow field. This achieves realistic real-time fluid surface behaviors by employing the physical governing laws of fluids but avoiding extensive 3D fluid dynamics computations. To complement the surface behaviors, we calculate fluid volume and external boundary changes separately to achieve full 3D general fluid flow. To simulate physical activities in a DIS, we introduce a mechanism which uses a uniform time scale proportional to the clock-time and variable time-slicing to synchronize physical models such as fluids in the networked environment. Our approach can simulate many different fluid behaviors by changing the internal or external boundary conditions. It can model different kinds of fluids by varying the Reynolds number. It can simulate objects moving or floating in fluids. It can also produce synchronized general fluid flows in a DIS. Our model can serve as a testbed to simulate many other fluid phenomena which have never been successfully modeled previously.

  4. Self-reconfigurable ship fluid-network modeling for simulation-based design

    NASA Astrophysics Data System (ADS)

    Moon, Kyungjin

    Our world is filled with large-scale engineering systems, which provide various services and conveniences in our daily life. A distinctive trend in the development of today's large-scale engineering systems is the extensive and aggressive adoption of automation and autonomy that enable the significant improvement of systems' robustness, efficiency, and performance, with considerably reduced manning and maintenance costs, and the U.S. Navy's DD(X), the next-generation destroyer program, is considered as an extreme example of such a trend. This thesis pursues a modeling solution for performing simulation-based analysis in the conceptual or preliminary design stage of an intelligent, self-reconfigurable ship fluid system, which is one of the concepts of DD(X) engineering plant development. Through the investigations on the Navy's approach for designing a more survivable ship system, it is found that the current naval simulation-based analysis environment is limited by the capability gaps in damage modeling, dynamic model reconfiguration, and simulation speed of the domain specific models, especially fluid network models. As enablers of filling these gaps, two essential elements were identified in the formulation of the modeling method. The first one is the graph-based topological modeling method, which will be employed for rapid model reconstruction and damage modeling, and the second one is the recurrent neural network-based, component-level surrogate modeling method, which will be used to improve the affordability and efficiency of the modeling and simulation (M&S) computations. The integration of the two methods can deliver computationally efficient, flexible, and automation-friendly M&S which will create an environment for more rigorous damage analysis and exploration of design alternatives. As a demonstration for evaluating the developed method, a simulation model of a notional ship fluid system was created, and a damage analysis was performed. Next, the models

  5. Fluid, solid and fluid-structure interaction simulations on patient-based abdominal aortic aneurysm models.

    PubMed

    Kelly, Sinead; O'Rourke, Malachy

    2012-04-01

    This article describes the use of fluid, solid and fluid-structure interaction simulations on three patient-based abdominal aortic aneurysm geometries. All simulations were carried out using OpenFOAM, which uses the finite volume method to solve both fluid and solid equations. Initially a fluid-only simulation was carried out on a single patient-based geometry and results from this simulation were compared with experimental results. There was good qualitative and quantitative agreement between the experimental and numerical results, suggesting that OpenFOAM is capable of predicting the main features of unsteady flow through a complex patient-based abdominal aortic aneurysm geometry. The intraluminal thrombus and arterial wall were then included, and solid stress and fluid-structure interaction simulations were performed on this, and two other patient-based abdominal aortic aneurysm geometries. It was found that the solid stress simulations resulted in an under-estimation of the maximum stress by up to 5.9% when compared with the fluid-structure interaction simulations. In the fluid-structure interaction simulations, flow induced pressure within the aneurysm was found to be up to 4.8% higher than the value of peak systolic pressure imposed in the solid stress simulations, which is likely to be the cause of the variation in the stress results. In comparing the results from the initial fluid-only simulation with results from the fluid-structure interaction simulation on the same patient, it was found that wall shear stress values varied by up to 35% between the two simulation methods. It was concluded that solid stress simulations are adequate to predict the maximum stress in an aneurysm wall, while fluid-structure interaction simulations should be performed if accurate prediction of the fluid wall shear stress is necessary. Therefore, the decision to perform fluid-structure interaction simulations should be based on the particular variables of interest in a given

  6. Hamiltonian closures in fluid models for plasmas

    NASA Astrophysics Data System (ADS)

    Tassi, Emanuele

    2017-11-01

    This article reviews recent activity on the Hamiltonian formulation of fluid models for plasmas in the non-dissipative limit, with emphasis on the relations between the fluid closures adopted for the different models and the Hamiltonian structures. The review focuses on results obtained during the last decade, but a few classical results are also described, in order to illustrate connections with the most recent developments. With the hope of making the review accessible not only to specialists in the field, an introduction to the mathematical tools applied in the Hamiltonian formalism for continuum models is provided. Subsequently, we review the Hamiltonian formulation of models based on the magnetohydrodynamics description, including those based on the adiabatic and double adiabatic closure. It is shown how Dirac's theory of constrained Hamiltonian systems can be applied to impose the incompressibility closure on a magnetohydrodynamic model and how an extended version of barotropic magnetohydrodynamics, accounting for two-fluid effects, is amenable to a Hamiltonian formulation. Hamiltonian reduced fluid models, valid in the presence of a strong magnetic field, are also reviewed. In particular, reduced magnetohydrodynamics and models assuming cold ions and different closures for the electron fluid are discussed. Hamiltonian models relaxing the cold-ion assumption are then introduced. These include models where finite Larmor radius effects are added by means of the gyromap technique, and gyrofluid models. Numerical simulations of Hamiltonian reduced fluid models investigating the phenomenon of magnetic reconnection are illustrated. The last part of the review concerns recent results based on the derivation of closures preserving a Hamiltonian structure, based on the Hamiltonian structure of parent kinetic models. Identification of such closures for fluid models derived from kinetic systems based on the Vlasov and drift-kinetic equations are presented, and

  7. [Individualized fluid-solid coupled model of intracranial aneurysms based on computed tomography angiography data].

    PubMed

    Wang, Fuyu; Xu, Bainan; Sun, Zhenghui; Liu, Lei; Wu, Chen; Zhang, Xiaojun

    2012-10-01

    To establish an individualized fluid-solid coupled model of intracranial aneurysms based on computed tomography angiography (CTA) image data. The original Dicom format image data from a patient with an intracranial aneurysm were imported into Mimics software to construct the 3D model. The fluid-solid coupled model was simulated with ANSYS and CFX software, and the sensitivity of the model was analyzed. The difference between the rigid model and fluid-solid coupled model was also compared. The fluid-solid coupled model of intracranial aneurysm was established successfully, which allowed direct simulation of the blood flow of the intracranial aneurysm and the deformation of the solid wall. The pressure field, stress field, and distribution of Von Mises stress and deformation of the aneurysm could be exported from the model. A small Young's modulus led to an obvious deformation of the vascular wall, and the walls with greater thicknesses had smaller deformations. The rigid model and the fluid-solid coupled model showed more differences in the wall shear stress and blood flow velocity than in pressure. The fluid-solid coupled model more accurately represents the actual condition of the intracranial aneurysm than the rigid model. The results of numerical simulation with the model are reliable to study the origin, growth and rupture of the aneurysms.

  8. Mesoscopic model for binary fluids

    NASA Astrophysics Data System (ADS)

    Echeverria, C.; Tucci, K.; Alvarez-Llamoza, O.; Orozco-Guillén, E. E.; Morales, M.; Cosenza, M. G.

    2017-10-01

    We propose a model for studying binary fluids based on the mesoscopic molecular simulation technique known as multiparticle collision, where the space and state variables are continuous, and time is discrete. We include a repulsion rule to simulate segregation processes that does not require calculation of the interaction forces between particles, so binary fluids can be described on a mesoscopic scale. The model is conceptually simple and computationally efficient; it maintains Galilean invariance and conserves the mass and energy in the system at the micro- and macro-scale, whereas momentum is conserved globally. For a wide range of temperatures and densities, the model yields results in good agreement with the known properties of binary fluids, such as the density profile, interface width, phase separation, and phase growth. We also apply the model to the study of binary fluids in crowded environments with consistent results.

  9. Hierarchical Bayesian Modeling of Fluid-Induced Seismicity

    NASA Astrophysics Data System (ADS)

    Broccardo, M.; Mignan, A.; Wiemer, S.; Stojadinovic, B.; Giardini, D.

    2017-11-01

    In this study, we present a Bayesian hierarchical framework to model fluid-induced seismicity. The framework is based on a nonhomogeneous Poisson process with a fluid-induced seismicity rate proportional to the rate of injected fluid. The fluid-induced seismicity rate model depends upon a set of physically meaningful parameters and has been validated for six fluid-induced case studies. In line with the vision of hierarchical Bayesian modeling, the rate parameters are considered as random variables. We develop both the Bayesian inference and updating rules, which are used to develop a probabilistic forecasting model. We tested the Basel 2006 fluid-induced seismic case study to prove that the hierarchical Bayesian model offers a suitable framework to coherently encode both epistemic uncertainty and aleatory variability. Moreover, it provides a robust and consistent short-term seismic forecasting model suitable for online risk quantification and mitigation.

  10. Modelling vortex-induced fluid-structure interaction.

    PubMed

    Benaroya, Haym; Gabbai, Rene D

    2008-04-13

    The principal goal of this research is developing physics-based, reduced-order, analytical models of nonlinear fluid-structure interactions associated with offshore structures. Our primary focus is to generalize the Hamilton's variational framework so that systems of flow-oscillator equations can be derived from first principles. This is an extension of earlier work that led to a single energy equation describing the fluid-structure interaction. It is demonstrated here that flow-oscillator models are a subclass of the general, physical-based framework. A flow-oscillator model is a reduced-order mechanical model, generally comprising two mechanical oscillators, one modelling the structural oscillation and the other a nonlinear oscillator representing the fluid behaviour coupled to the structural motion.Reduced-order analytical model development continues to be carried out using a Hamilton's principle-based variational approach. This provides flexibility in the long run for generalizing the modelling paradigm to complex, three-dimensional problems with multiple degrees of freedom, although such extension is very difficult. As both experimental and analytical capabilities advance, the critical research path to developing and implementing fluid-structure interaction models entails-formulating generalized equations of motion, as a superset of the flow-oscillator models; and-developing experimentally derived, semi-analytical functions to describe key terms in the governing equations of motion. The developed variational approach yields a system of governing equations. This will allow modelling of multiple d.f. systems. The extensions derived generalize the Hamilton's variational formulation for such problems. The Navier-Stokes equations are derived and coupled to the structural oscillator. This general model has been shown to be a superset of the flow-oscillator model. Based on different assumptions, one can derive a variety of flow-oscillator models.

  11. Physically based model for extracting dual permeability parameters using non-Newtonian fluids

    NASA Astrophysics Data System (ADS)

    Abou Najm, M. R.; Basset, C.; Stewart, R. D.; Hauswirth, S.

    2017-12-01

    Dual permeability models are effective for the assessment of flow and transport in structured soils with two dominant structures. The major challenge to those models remains in the ability to determine appropriate and unique parameters through affordable, simple, and non-destructive methods. This study investigates the use of water and a non-Newtonian fluid in saturated flow experiments to derive physically-based parameters required for improved flow predictions using dual permeability models. We assess the ability of these two fluids to accurately estimate the representative pore sizes in dual-domain soils, by determining the effective pore sizes of macropores and micropores. We developed two sub-models that solve for the effective macropore size assuming either cylindrical (e.g., biological pores) or planar (e.g., shrinkage cracks and fissures) pore geometries, with the micropores assumed to be represented by a single effective radius. Furthermore, the model solves for the percent contribution to flow (wi) corresponding to the representative macro and micro pores. A user-friendly solver was developed to numerically solve the system of equations, given that relevant non-Newtonian viscosity models lack forms conducive to analytical integration. The proposed dual-permeability model is a unique attempt to derive physically based parameters capable of measuring dual hydraulic conductivities, and therefore may be useful in reducing parameter uncertainty and improving hydrologic model predictions.

  12. SPH modeling of fluid-solid interaction for dynamic failure analysis of fluid-filled thin shells

    NASA Astrophysics Data System (ADS)

    Caleyron, F.; Combescure, A.; Faucher, V.; Potapov, S.

    2013-05-01

    This work concerns the prediction of failure of a fluid-filled tank under impact loading, including the resulting fluid leakage. A water-filled steel cylinder associated with a piston is impacted by a mass falling at a prescribed velocity. The cylinder is closed at its base by an aluminum plate whose characteristics are allowed to vary. The impact on the piston creates a pressure wave in the fluid which is responsible for the deformation of the plate and, possibly, the propagation of cracks. The structural part of the problem is modeled using Mindlin-Reissner finite elements (FE) and Smoothed Particle Hydrodynamics (SPH) shells. The modeling of the fluid is also based on an SPH formulation. The problem involves significant fluid-structure interactions (FSI) which are handled through a master-slave-based method and the pinballs method. Numerical results are compared to experimental data.

  13. An earthquake instability model based on faults containing high fluid-pressure compartments

    USGS Publications Warehouse

    Lockner, D.A.; Byerlee, J.D.

    1995-01-01

    It has been proposed that large strike-slip faults such as the San Andreas contain water in seal-bounded compartments. Arguments based on heat flow and stress orientation suggest that in most of the compartments, the water pressure is so high that the average shear strength of the fault is less than 20 MPa. We propose a variation of this basic model in which most of the shear stress on the fault is supported by a small number of compartments where the pore pressure is relatively low. As a result, the fault gouge in these compartments is compacted and lithified and has a high undisturbed strength. When one of these locked regions fails, the system made up of the neighboring high and low pressure compartments can become unstable. Material in the high fluid pressure compartments is initially underconsolidated since the low effective confining pressure has retarded compaction. As these compartments are deformed, fluid pressure remains nearly unchanged so that they offer little resistance to shear. The low pore pressure compartments, however, are overconsolidated and dilate as they are sheared. Decompression of the pore fluid in these compartments lowers fluid pressure, increasing effective normal stress and shear strength. While this effect tends to stabilize the fault, it can be shown that this dilatancy hardening can be more than offset by displacement weakening of the fault (i.e., the drop from peak to residual strength). If the surrounding rock mass is sufficiently compliant to produce an instability, slip will propagate along the fault until the shear fracture runs into a low-stress region. Frictional heating and the accompanying increase in fluid pressure that are suggested to occur during shearing of the fault zone will act as additional destabilizers. However, significant heating occurs only after a finite amount of slip and therefore is more likely to contribute to the energetics of rupture propagation than to the initiation of the instability. We present

  14. Properties of forced convection experimental with silicon carbide based nano-fluids

    NASA Astrophysics Data System (ADS)

    Soanker, Abhinay

    With the advent of nanotechnology, many fields of Engineering and Science took a leap to the next level of advancements. The broad scope of nanotechnology initiated many studies of heat transfer and thermal engineering. Nano-fluids are one such technology and can be thought of as engineered colloidal fluids with nano-sized colloidal particles. There are different types of nano-fluids based on the colloidal particle and base fluids. Nano-fluids can primarily be categorized into metallic, ceramics, oxide, magnetic and carbon based. The present work is a part of investigation of the thermal and rheological properties of ceramic based nano-fluids. alpha-Silicon Carbide based nano-fluid with Ethylene Glycol and water mixture 50-50% volume concentration was used as the base fluid here. This work is divided into three parts; Theoretical modelling of effective thermal conductivity (ETC) of colloidal fluids, study of Thermal and Rheological properties of alpha-SiC nano-fluids, and determining the Heat Transfer properties of alpha-SiC nano-fluids. In the first part of this work, a theoretical model for effective thermal conductivity (ETC) of static based colloidal fluids was formulated based on the particle size, shape (spherical), thermal conductivity of base fluid and that of the colloidal particle, along with the particle distribution pattern in the fluid. A MATLAB program is generated to calculate the details of this model. The model is specifically derived for least and maximum ETC enhancement possible and thereby the lower and upper bounds was determined. In addition, ETC is also calculated for uniform colloidal distribution pattern. Effect of volume concentration on ETC was studied. No effect of particle size was observed for particle sizes below a certain value. Results of this model were compared with Wiener bounds and Hashin- Shtrikman bounds. The second part of this work is a study of thermal and rheological properties of alpha-Silicon Carbide based nano-fluids

  15. Two-dimensional hybrid Monte Carlo–fluid modelling of dc glow discharges: Comparison with fluid models, reliability, and accuracy

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

    Eylenceoğlu, E.; Rafatov, I., E-mail: rafatov@metu.edu.tr; Kudryavtsev, A. A.

    2015-01-15

    Two-dimensional hybrid Monte Carlo–fluid numerical code is developed and applied to model the dc glow discharge. The model is based on the separation of electrons into two parts: the low energetic (slow) and high energetic (fast) electron groups. Ions and slow electrons are described within the fluid model using the drift-diffusion approximation for particle fluxes. Fast electrons, represented by suitable number of super particles emitted from the cathode, are responsible for ionization processes in the discharge volume, which are simulated by the Monte Carlo collision method. Electrostatic field is obtained from the solution of Poisson equation. The test calculations weremore » carried out for an argon plasma. Main properties of the glow discharge are considered. Current-voltage curves, electric field reversal phenomenon, and the vortex current formation are developed and discussed. The results are compared to those obtained from the simple and extended fluid models. Contrary to reports in the literature, the analysis does not reveal significant advantages of existing hybrid methods over the extended fluid model.« less

  16. Magnetorheological fluid based automotive steer-by-wire systems

    NASA Astrophysics Data System (ADS)

    Ahmadkhanlou, Farzad; Washington, Gregory N.; Bechtel, Stephen E.; Wang, Yingru

    2006-03-01

    The idea of this paper is to design a Magnetorheological (MR) fluid based damper for steer-by-wire systems to provide sensory feedback to the driver. The advantages of using MR fluids in haptic devices stem from the increase in transparency gained from the lightweight semiactive system and controller implementation. The performance of MR fluid based steer-by wire system depends on MR fluid model and specifications, MR damper geometry, and the control algorithm. All of these factors are addressed in this study. The experimental results show the improvements in steer-by-wire by adding force feedback to the system.

  17. Enthalpy-based equation of state for highly porous materials employing modified soft sphere fluid model

    NASA Astrophysics Data System (ADS)

    Nayak, Bishnupriya; Menon, S. V. G.

    2018-01-01

    Enthalpy-based equation of state based on a modified soft sphere model for the fluid phase, which includes vaporization and ionization effects, is formulated for highly porous materials. Earlier developments and applications of enthalpy-based approach had not accounted for the fact that shocked states of materials with high porosity (e.g., porosity more than two for Cu) are in the expanded fluid region. We supplement the well known soft sphere model with a generalized Lennard-Jones formula for the zero temperature isotherm, with parameters determined from cohesive energy, specific volume and bulk modulus of the solid at normal condition. Specific heats at constant pressure, ionic and electronic enthalpy parameters and thermal excitation effects are calculated using the modified approach and used in the enthalpy-based equation of state. We also incorporate energy loss from the shock due to expansion of shocked material in calculating porous Hugoniot. Results obtained for Cu, even up to initial porosities ten, show good agreement with experimental data.

  18. A fluid-mechanic-based model for the sedimentation of flocculated suspensions

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

    Chhabra, R.P.; Prasad, D.

    1991-02-01

    Due to the wide occurrence of the suspensions of fine particles in mineral and chemical processing industries, considerable interest has been shown in modeling the hydrodynamic behavior of such systems. A fluid-mechanic-based analysis is presented for the settling behavior of flocculated4d suspensions. Flocs have been modeled as composite spheres consisting of a solid core embedded in a shell of homogeneous and isotropic porous medium. Theoretical estimates of the rates of sedimentation for flocculated suspensions are obtained by solving the equations of continuity and of motion. The interparticle interactions are incorporated into the analysis by employing the Happel free surface cellmore » model. The results reported embrace wide ranges of conditions of floc size and concentration.« less

  19. VISCOPLASTIC FLUID MODEL FOR DEBRIS FLOW ROUTING.

    USGS Publications Warehouse

    Chen, Cheng-lung

    1986-01-01

    This paper describes how a generalized viscoplastic fluid model, which was developed based on non-Newtonian fluid mechanics, can be successfully applied to routing a debris flow down a channel. The one-dimensional dynamic equations developed for unsteady clear-water flow can be used for debris flow routing if the flow parameters, such as the momentum (or energy) correction factor and the resistance coefficient, can be accurately evaluated. The writer's generalized viscoplastic fluid model can be used to express such flow parameters in terms of the rheological parameters for debris flow in wide channels. A preliminary analysis of the theoretical solutions reveals the importance of the flow behavior index and the so-called modified Froude number for uniformly progressive flow in snout profile modeling.

  20. Particles at fluid-fluid interfaces: A new Navier-Stokes-Cahn-Hilliard surface- phase-field-crystal model.

    PubMed

    Aland, Sebastian; Lowengrub, John; Voigt, Axel

    2012-10-01

    Colloid particles that are partially wetted by two immiscible fluids can become confined to fluid-fluid interfaces. At sufficiently high volume fractions, the colloids may jam and the interface may crystallize. The fluids together with the interfacial colloids form an emulsion with interesting material properties and offer an important route to new soft materials. A promising approach to simulate these emulsions was presented in Aland et al. [Phys. Fluids 23, 062103 (2011)], where a Navier-Stokes-Cahn-Hilliard model for the macroscopic two-phase fluid system was combined with a surface phase-field-crystal model for the microscopic colloidal particles along the interface. Unfortunately this model leads to spurious velocities which require very fine spatial and temporal resolutions to accurately and stably simulate. In this paper we develop an improved Navier-Stokes-Cahn-Hilliard-surface phase-field-crystal model based on the principles of mass conservation and thermodynamic consistency. To validate our approach, we derive a sharp interface model and show agreement with the improved diffuse interface model. Using simple flow configurations, we show that the new model has much better properties and does not lead to spurious velocities. Finally, we demonstrate the solid-like behavior of the crystallized interface by simulating the fall of a solid ball through a colloid-laden multiphase fluid.

  1. Numerical investigation of fluid mud motion using a three-dimensional hydrodynamic and two-dimensional fluid mud coupling model

    NASA Astrophysics Data System (ADS)

    Yang, Xiaochen; Zhang, Qinghe; Hao, Linnan

    2015-03-01

    A water-fluid mud coupling model is developed based on the unstructured grid finite volume coastal ocean model (FVCOM) to investigate the fluid mud motion. The hydrodynamics and sediment transport of the overlying water column are solved using the original three-dimensional ocean model. A horizontal two-dimensional fluid mud model is integrated into the FVCOM model to simulate the underlying fluid mud flow. The fluid mud interacts with the water column through the sediment flux, current, and shear stress. The friction factor between the fluid mud and the bed, which is traditionally determined empirically, is derived with the assumption that the vertical distribution of shear stress below the yield surface of fluid mud is identical to that of uniform laminar flow of Newtonian fluid in the open channel. The model is validated by experimental data and reasonable agreement is found. Compared with numerical cases with fixed friction factors, the results simulated with the derived friction factor exhibit the best agreement with the experiment, which demonstrates the necessity of the derivation of the friction factor.

  2. A new hysteresis model based on force-displacement characteristics of magnetorheological fluid actuators subjected to squeeze mode operation

    NASA Astrophysics Data System (ADS)

    Chen, Peng; Bai, Xian-Xu; Qian, Li-Jun; Choi, Seung-Bok

    2017-06-01

    This paper presents a new hysteresis model based on the force-displacement characteristics of magnetorheological (MR) fluid actuators (or devices) subjected to squeeze mode operation. The idea of the proposed model is originated from experimental observation of the field-dependent hysteretic behavior of MR fluids, which shows that from a view of rate-independence of hysteresis, a gap width-dependent hysteresis is occurred in the force-displacement relationship instead of the typical relationship of the force-velocity. To effectively and accurately portray the hysteresis behavior, the gap width-dependent hysteresis elements, the nonlinear viscous effect and the inertial effect are considered for the formulation of the hysteresis model. Then, a model-based feedforward force tracking control scheme is established through an observer which can estimate the virtual displacement. The effectiveness of the proposed hysteresis model is validated through the identification and prediction of the damping force of MR fluids in the squeeze mode. In addition, it is shown that superior force tracking performance of the feedforward control associated with the proposed hysteresis mode is evaluated by adopting several tracking trajectories.

  3. Design and dynamic modeling of electrorheological fluid-based variable-stiffness fin for robotic fish

    NASA Astrophysics Data System (ADS)

    Bazaz Behbahani, Sanaz; Tan, Xiaobo

    2017-08-01

    Fish actively control their stiffness in different swimming conditions. Inspired by such an adaptive behavior, in this paper we study the design, prototyping, and dynamic modeling of compact, tunable-stiffness fins for robotic fish, where electrorheological (ER) fluid serves as the enabling element. A multi-layer composite fin with an ER fluid core is prototyped and utilized to investigate the influence of electrical field on its performance. Hamilton's principle is used to derive the dynamic equations of motion of the flexible fin, and Lighthill's large-amplitude elongated-body theory is adopted to estimate the hydrodynamic force when the fin undergoes base-actuated rotation. The dynamic equations are then discretized using the finite element method, to obtain an approximate numerical solution. Experiments are conducted on the prototyped flexible ER fluid-filled beam for parameter identification and validation of the proposed model, and for examining the effectiveness of electrically controlled stiffness tuning. In particular, it is found that the natural frequency is increased by almost 40% when the applied electric field changes from 0 to 1.5× {10}6 {{V}} {{{m}}}-1.

  4. Modelling induced seismicity due to fluid injection

    NASA Astrophysics Data System (ADS)

    Murphy, S.; O'Brien, G. S.; Bean, C. J.; McCloskey, J.; Nalbant, S. S.

    2011-12-01

    Injection of fluid into the subsurface alters the stress in the crust and can induce earthquakes. The science of assessing the risk of induced seismicity from such ventures is still in its infancy despite public concern. We plan to use a fault network model in which stress perturbations due to fluid injection induce earthquakes. We will use this model to investigate the role different operational and geological factors play in increasing seismicity in a fault system due to fluid injection. The model is based on a quasi-dynamic relationship between stress and slip coupled with a rate and state fiction law. This allows us to model slip on fault interfaces over long periods of time (i.e. years to 100's years). With the use of the rate and state friction law the nature of stress release during slipping can be altered through variation of the frictional parameters. Both seismic and aseismic slip can therefore be simulated. In order to add heterogeneity along the fault plane a fractal variation in the frictional parameters is used. Fluid injection is simulated using the lattice Boltzmann method whereby pore pressure diffuses throughout a permeable layer from the point of injection. The stress perturbation this causes on the surrounding fault system is calculated using a quasi-static solution for slip dislocation in an elastic half space. From this model we can generate slip histories and seismicity catalogues covering 100's of years for predefined fault networks near fluid injection sites. Given that rupture is a highly non-linear process, comparison between models with different input parameters (e.g. fault network statistics and injection rates) will be based on system wide features (such as the Gutenberg-Richter b-values), rather than specific seismic events. Our ultimate aim is that our model produces seismic catalogues similar to those observed over real injection sites. Such validation would pave the way to probabilistic estimation of reactivation risk for

  5. Particles at fluid-fluid interfaces: A new Navier-Stokes-Cahn-Hilliard surface-phase-field-crystal model

    PubMed Central

    Aland, Sebastian; Lowengrub, John; Voigt, Axel

    2013-01-01

    Colloid particles that are partially wetted by two immiscible fluids can become confined to fluid-fluid interfaces. At sufficiently high volume fractions, the colloids may jam and the interface may crystallize. The fluids together with the interfacial colloids form an emulsion with interesting material properties and offer an important route to new soft materials. A promising approach to simulate these emulsions was presented in Aland et al. [Phys. Fluids 23, 062103 (2011)], where a Navier-Stokes-Cahn-Hilliard model for the macroscopic two-phase fluid system was combined with a surface phase-field-crystal model for the microscopic colloidal particles along the interface. Unfortunately this model leads to spurious velocities which require very fine spatial and temporal resolutions to accurately and stably simulate. In this paper we develop an improved Navier-Stokes-Cahn-Hilliard-surface phase-field-crystal model based on the principles of mass conservation and thermodynamic consistency. To validate our approach, we derive a sharp interface model and show agreement with the improved diffuse interface model. Using simple flow configurations, we show that the new model has much better properties and does not lead to spurious velocities. Finally, we demonstrate the solid-like behavior of the crystallized interface by simulating the fall of a solid ball through a colloid-laden multiphase fluid. PMID:23214691

  6. Fluid and hybrid models for streamers

    NASA Astrophysics Data System (ADS)

    Bonaventura, Zdeněk

    2016-09-01

    Streamers are contracted ionizing waves with self-generated field enhancement that propagate into a low-ionized medium exposed to high electric field leaving filamentary trails of plasma behind. The widely used model to study streamer dynamics is based on drift-diffusion equations for electrons and ions, assuming local field approximation, coupled with Poisson's equation. For problems where presence of energetic electrons become important a fluid approach needs to be extended by a particle model, accompanied also with Monte Carlo Collision technique, that takes care of motion of these electrons. A combined fluid-particle approach is used to study an influence of surface emission processes on a fast-pulsed dielectric barrier discharge in air at atmospheric pressure. It is found that fluid-only model predicts substantially faster reignition dynamics compared to coupled fluid-particle model. Furthermore, a hybrid model can be created in which the population of electrons is divided in the energy space into two distinct groups: (1) low energy `bulk' electrons that are treated with fluid model, and (2) high energy `beam' electrons, followed as particles. The hybrid model is then capable not only to deal with streamer discharges in laboratory conditions, but also allows us to study electron acceleration in streamer zone of lighting leaders. There, the production of fast electrons from streamers is investigated, since these (runaway) electrons act as seeds for the relativistic runaway electron avalanche (RREA) mechanism, important for high-energy atmospheric physics phenomena. Results suggest that high energy electrons effect the streamer propagation, namely the velocity, the peak electric field, and thus also the production rate of runaway electrons. This work has been supported by the Czech Science Foundation research project 15-04023S.

  7. Physics-Based Computational Algorithm for the Multi-Fluid Plasma Model

    DTIC Science & Technology

    2014-06-30

    applying it to study laser - 20 Physics-Based Multi-Fluid Plasma Algorithm Shumlak Figure 6: Blended finite element method applied to the species...separation problem in capsule implosions. Number densities and electric field are shown after the laser drive has compressed the multi-fluid plasma and...6 after the laser drive has started the compression. A separation clearly develops. The solution is found using an explicit advance (CFL=1) for the

  8. Phase-field-based lattice Boltzmann model for incompressible binary fluid systems with density and viscosity contrasts.

    PubMed

    Zu, Y Q; He, S

    2013-04-01

    A lattice Boltzmann model (LBM) is proposed based on the phase-field theory to simulate incompressible binary fluids with density and viscosity contrasts. Unlike many existing diffuse interface models which are limited to density matched binary fluids, the proposed model is capable of dealing with binary fluids with moderate density ratios. A new strategy for projecting the phase field to the viscosity field is proposed on the basis of the continuity of viscosity flux. The new LBM utilizes two lattice Boltzmann equations (LBEs): one for the interface tracking and the other for solving the hydrodynamic properties. The LBE for interface tracking can recover the Chan-Hilliard equation without any additional terms; while the LBE for hydrodynamic properties can recover the exact form of the divergence-free incompressible Navier-Stokes equations avoiding spurious interfacial forces. A series of 2D and 3D benchmark tests have been conducted for validation, which include a rigid-body rotation, stationary and moving droplets, a spinodal decomposition, a buoyancy-driven bubbly flow, a layered Poiseuille flow, and the Rayleigh-Taylor instability. It is shown that the proposed method can track the interface with high accuracy and stability and can significantly and systematically reduce the parasitic current across the interface. Comparisons with momentum-based models indicate that the newly proposed velocity-based model can better satisfy the incompressible condition in the flow fields, and eliminate or reduce the velocity fluctuations in the higher-pressure-gradient region and, therefore, achieve a better numerical stability. In addition, the test of a layered Poiseuille flow demonstrates that the proposed scheme for mixture viscosity performs significantly better than the traditional mixture viscosity methods.

  9. Modeling the migration of fluids in subduction zones

    NASA Astrophysics Data System (ADS)

    Spiegelman, M.; Wilson, C. R.; van Keken, P. E.; Hacker, B. R.

    2010-12-01

    Fluids play a major role in the formation of arc volcanism and the generation of continental crust. Progressive dehydration reactions in the downgoing slab release fluids to the hot overlying mantle wedge, causing flux melting and the migration of melts to the volcanic front. While the qualitative concept is well established the quantitative details of fluid release and especially that of fluid migration and generation of hydrous melting in the wedge is still poorly understood. Here we present new models of the fluid migration through the mantle wedge for subduction zones that span the spectrum of arcs worldwide. We focus on the flow of water and use an existing set of high resolution thermal and metamorphic models (van Keken et al., JGR, in review) to predict the regions of water release from the sediments, upper and lower crust, and upper most mantle. We use this water flux as input for the fluid migration calculation based on new finite element models built on advanced computational libraries (FEniCS/PETSc) for efficient and flexible solution of coupled multi-physics problems. The first generation of these models solves for the evolution of porosity and fluid-pressure/flux throughout the slab and wedge given solid flow, viscosity and thermal fields from the existing thermal models. Fluid flow in the new models depends on both permeability and the rheology of the slab-wedge system as interaction with rheological variability can induce additional pressure gradients that affect the fluid flow pathways. We will explore the sensitivity of fluid flow paths for a range of subduction zones and fluid flow parameters with emphasis on variability of the location of the volcanic arc with respect to flow paths and expected degrees of hydrous melting which can be estimated given a variety of wet-melting parameterizations (e.g. Katz et al, 2003, Kelley et al, 2010). The current models just include dehydration reactions but work continues on the next generation of models which

  10. Computational fluid dynamic modelling of cavitation

    NASA Technical Reports Server (NTRS)

    Deshpande, Manish; Feng, Jinzhang; Merkle, Charles L.

    1993-01-01

    Models in sheet cavitation in cryogenic fluids are developed for use in Euler and Navier-Stokes codes. The models are based upon earlier potential-flow models but enable the cavity inception point, length, and shape to be determined as part of the computation. In the present paper, numerical solutions are compared with experimental measurements for both pressure distribution and cavity length. Comparisons between models are also presented. The CFD model provides a relatively simple modification to an existing code to enable cavitation performance predictions to be included. The analysis also has the added ability of incorporating thermodynamic effects of cryogenic fluids into the analysis. Extensions of the current two-dimensional steady state analysis to three-dimensions and/or time-dependent flows are, in principle, straightforward although geometrical issues become more complicated. Linearized models, however offer promise of providing effective cavitation modeling in three-dimensions. This analysis presents good potential for improved understanding of many phenomena associated with cavity flows.

  11. Segregated Methods for Two-Fluid Models

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

    Prosperetti, Andrea; Sundaresan, Sankaran; Pannala, Sreekanth

    2007-01-01

    The previous chapter, with its direct simulation of the fluid flow and a modeling approach to the particle phase, may be seen as a transition between the methods for a fully resolved simulation described in the first part of this book and those for a coarse grained description based on the averaging approach described in chapter ??. We now turn to the latter, which in practice are the only methods able to deal with the complex flows encountered in most situations of practical interest such as fluidized beds, pipelines, energy generation, sediment transport, and others. This chapter and the nextmore » one are devoted to numerical methods for so-called two-fluid models in which the phases are treated as inter-penetrating continua describing, e.g., a liquid and a gas, or a fluid and a suspended solid phase. These models can be extended to deal with more than two continua and, then, the denomination multi-fluid models might be more appropriate. For example, the commercial code OLGA (Bendiksen et al. 1991), widely used in the oil industry, recognizes three phases, all treated as interpenetrating continua: a continuous liquid, a gas, and a disperse liquid phase present as drops suspended in the gas phase. The more recent PeTra (Petroleum Transport, Larsen et al. 1997) also describes three phases, gas, oil, and water. Recent approaches to the description of complex boiling flows recognize four inter-penetrating phases: a liquid phase present both as a continuum and as a dispersion of droplets, and a gas/vapor phase also present as a continuum and a dispersion of bubbles. Methods for these multi-fluid models are based on those developed for the two-fluid model to which we limit ourselves. In principle, one could simply take the model equations, discretize them, and solve them by a method suitable for non-linear problems, e.g. Newton-Raphson iteration. In practice, the computational cost of such a frontal attack is nearly always prohibitive in terms of storage requirement

  12. Fluids and Combustion Facility: Fluids Integrated Rack Modal Model Correlation

    NASA Technical Reports Server (NTRS)

    McNelis, Mark E.; Suarez, Vicente J.; Sullivan, Timothy L.; Otten, Kim D.; Akers, James C.

    2005-01-01

    The Fluids Integrated Rack (FIR) is one of two racks in the Fluids and Combustion Facility on the International Space Station. The FIR is dedicated to the scientific investigation of space system fluids management supporting NASA s Exploration of Space Initiative. The FIR hardware was modal tested and FIR finite element model updated to satisfy the International Space Station model correlation criteria. The final cross-orthogonality results between the correlated model and test mode shapes was greater than 90 percent for all primary target modes.

  13. Adaptive particle-based pore-level modeling of incompressible fluid flow in porous media: a direct and parallel approach

    NASA Astrophysics Data System (ADS)

    Ovaysi, S.; Piri, M.

    2009-12-01

    We present a three-dimensional fully dynamic parallel particle-based model for direct pore-level simulation of incompressible viscous fluid flow in disordered porous media. The model was developed from scratch and is capable of simulating flow directly in three-dimensional high-resolution microtomography images of naturally occurring or man-made porous systems. It reads the images as input where the position of the solid walls are given. The entire medium, i.e., solid and fluid, is then discretized using particles. The model is based on Moving Particle Semi-implicit (MPS) technique. We modify this technique in order to improve its stability. The model handles highly irregular fluid-solid boundaries effectively. It takes into account viscous pressure drop in addition to the gravity forces. It conserves mass and can automatically detect any false connectivity with fluid particles in the neighboring pores and throats. It includes a sophisticated algorithm to automatically split and merge particles to maintain hydraulic connectivity of extremely narrow conduits. Furthermore, it uses novel methods to handle particle inconsistencies and open boundaries. To handle the computational load, we present a fully parallel version of the model that runs on distributed memory computer clusters and exhibits excellent scalability. The model is used to simulate unsteady-state flow problems under different conditions starting from straight noncircular capillary tubes with different cross-sectional shapes, i.e., circular/elliptical, square/rectangular and triangular cross-sections. We compare the predicted dimensionless hydraulic conductances with the data available in the literature and observe an excellent agreement. We then test the scalability of our parallel model with two samples of an artificial sandstone, samples A and B, with different volumes and different distributions (non-uniform and uniform) of solid particles among the processors. An excellent linear scalability is

  14. Modeling of Non-Isothermal Cryogenic Fluid Sloshing

    NASA Technical Reports Server (NTRS)

    Agui, Juan H.; Moder, Jeffrey P.

    2015-01-01

    A computational fluid dynamic model was used to simulate the thermal destratification in an upright self-pressurized cryostat approximately half-filled with liquid nitrogen and subjected to forced sinusoidal lateral shaking. A full three-dimensional computational grid was used to model the tank dynamics, fluid flow and thermodynamics using the ANSYS Fluent code. A non-inertial grid was used which required the addition of momentum and energy source terms to account for the inertial forces, energy transfer and wall reaction forces produced by the shaken tank. The kinetics-based Schrage mass transfer model provided the interfacial mass transfer due to evaporation and condensation at the sloshing interface. The dynamic behavior of the sloshing interface, its amplitude and transition to different wave modes, provided insight into the fluid process at the interface. The tank pressure evolution and temperature profiles compared relatively well with the shaken cryostat experimental test data provided by the Centre National D'Etudes Spatiales.

  15. Development of Efficient Real-Fluid Model in Simulating Liquid Rocket Injector Flows

    NASA Technical Reports Server (NTRS)

    Cheng, Gary; Farmer, Richard

    2003-01-01

    The characteristics of propellant mixing near the injector have a profound effect on the liquid rocket engine performance. However, the flow features near the injector of liquid rocket engines are extremely complicated, for example supercritical-pressure spray, turbulent mixing, and chemical reactions are present. Previously, a homogeneous spray approach with a real-fluid property model was developed to account for the compressibility and evaporation effects such that thermodynamics properties of a mixture at a wide range of pressures and temperatures can be properly calculated, including liquid-phase, gas- phase, two-phase, and dense fluid regions. The developed homogeneous spray model demonstrated a good success in simulating uni- element shear coaxial injector spray combustion flows. However, the real-fluid model suffered a computational deficiency when applied to a pressure-based computational fluid dynamics (CFD) code. The deficiency is caused by the pressure and enthalpy being the independent variables in the solution procedure of a pressure-based code, whereas the real-fluid model utilizes density and temperature as independent variables. The objective of the present research work is to improve the computational efficiency of the real-fluid property model in computing thermal properties. The proposed approach is called an efficient real-fluid model, and the improvement of computational efficiency is achieved by using a combination of a liquid species and a gaseous species to represent a real-fluid species.

  16. Modeling the Migration of Fluids in Subduction Zones

    NASA Astrophysics Data System (ADS)

    Wilson, C. R.; Spiegelman, M.; Van Keken, P. E.; Vrijmoed, J. C.; Hacker, B. R.

    2011-12-01

    Fluids play a major role in the formation of arc volcanism and the generation of continental crust. Progressive dehydration reactions in the downgoing slab release fluids to the hot overlying mantle wedge, causing flux melting and the migration of melts to the volcanic front. While the qualitative concept is well established, the quantitative details of fluid release and especially that of fluid migration and generation of hydrous melting in the wedge is still poorly understood. Here we present new models of the fluid migration through the mantle wedge for subduction zones. We use an existing set of high resolution metamorphic models (van Keken et al, 2010) to predict the regions of water release from the sediments, upper and lower crust, and upper most mantle. We use this water flux as input for the fluid migration calculation based on new finite element models built on advanced computational libraries (FEniCS/PETSc) for efficient and flexible solution of coupled multi-physics problems. The first generation of one-way coupled models solves for the evolution of porosity and fluid-pressure/flux throughout the slab and wedge given solid flow, viscosity and thermal fields from separate solutions to the incompressible Stokes and energy equations in the mantle wedge. These solutions are verified by comparing to previous benchmark studies (van Keken et al, 2008) and global suites of thermal subduction models (Syracuse et al, 2010). Fluid flow depends on both permeability and the rheology of the slab-wedge system as interaction with rheological variability can induce additional pressure gradients that affect the fluid flow pathways. These non-linearities have been shown to explain laboratory-scale observations of melt band orientation in labratory experiments and numerical simulations of melt localization in shear bands (Katz et al 2006). Our second generation of models dispense with the pre-calculation of incompressible mantle flow and fully couple the now compressible

  17. Modeling fluid transport in 2d paper networks

    NASA Astrophysics Data System (ADS)

    Tirapu Azpiroz, Jaione; Fereira Silva, Ademir; Esteves Ferreira, Matheus; Lopez Candela, William Fernando; Bryant, Peter William; Ohta, Ricardo Luis; Engel, Michael; Steiner, Mathias Bernhard

    2018-02-01

    Paper-based microfluidic devices offer great potential as a low-cost platform to perform chemical and biochemical tests. Commercially available formats such as dipsticks and lateral-flow test devices are widely popular as they are easy to handle and produce fast and unambiguous results. While these simple devices lack precise control over the flow to enable integration of complex functionality for multi-step processes or the ability to multiplex several tests, intense research in this area is rapidly expanding the possibilities. Modeling and simulation is increasingly more instrumental in gaining insight into the underlying physics driving the processes inside the channels, however simulation of flow in paper-based microfluidic devices has barely been explored to aid in the optimum design and prototyping of these devices for precise control of the flow. In this paper, we implement a multiphase fluid flow model through porous media for the simulation of paper imbibition of an incompressible, Newtonian fluid such as when water, urine or serum is employed. The formulation incorporates mass and momentum conservation equations under Stokes flow conditions and results in two coupled Darcy's law equations for the pressures and saturations of the wetting and non-wetting phases, further simplified to the Richard's equation for the saturation of the wetting fluid, which is then solved using a Finite Element solver. The model tracks the wetting fluid front as it displaces the non-wetting fluid by computing the time-dependent saturation of the wetting fluid. We apply this to the study of liquid transport in two-dimensional paper networks and validate against experimental data concerning the wetting dynamics of paper layouts of varying geometries.

  18. Two-Fluid Models and Interfacial Area Transport in Microgravity Condition

    NASA Technical Reports Server (NTRS)

    Ishii, Mamoru; Sun, Xiao-Dong; Vasavada, Shilp

    2004-01-01

    The objective of the present study is to develop a two-fluid model formulation with interfacial area transport equation applicable for microgravity conditions. The new model is expected to make a leapfrog improvement by furnishing the constitutive relations for the interfacial interaction terms with the interfacial area transport equation, which can dynamically model the changes of the interfacial structures. In the first year of this three-year project supported by the U.S. NASA, Office of Biological and Physics Research, the primary focus is to design and construct a ground-based, microgravity two-phase flow simulation facility, in which two immiscible fluids with close density will be used. In predicting the two-phase flow behaviors in any two-phase flow system, the interfacial transfer terms are among the most essential factors in the modeling. These interfacial transfer terms in a two-fluid model specify the rate of phase change, momentum exchange, and energy transfer at the interface between the two phases. For the two-phase flow under the microgravity condition, the stability of the fluid particle interface and the interfacial structures are quite different from those under normal gravity condition. The flow structure may not reach an equilibrium condition and the two fluids may be loosely coupled such that the inertia terms of each fluid should be considered separately by use of the two-fluid model. Previous studies indicated that, unless phase-interaction terms are accurately modeled in the two-fluid model, the complex modeling does not necessarily warrant an accurate solution.

  19. [Kidney, Fluid, and Acid-Base Balance].

    PubMed

    Shioji, Naohiro; Hayashi, Masao; Morimatsu, Hiroshi

    2016-05-01

    Kidneys play an important role to maintain human homeostasis. They contribute to maintain body fluid, electrolytes, and acid-base balance. Especially in fluid control, we, physicians can intervene body fluid balance using fluid resuscitation and diuretics. In recent years, one type of fluid resuscitation, hydroxyl ethyl starch has been extensively studied in the field of intensive care. Although their effects on fluid resuscitation are reasonable, serious complications such as kidney injury requiring renal replacement therapy occur frequently. Now we have to pay more attention to this important complication. Another topic of fluid management is tolvaptan, a selective vasopressin-2 receptor antagonist Recent randomized trial suggested that tolvaptan has a similar supportive effect for fluid control and more cost effective compared to carperitide. In recent years, Stewart approach is recognized as one important tool to assess acid-base balance in critically ill patients. This approach has great value, especially to understand metabolic components in acid-base balance. Even for assessing the effects of kidneys on acid-base balance, this approach gives us interesting insight. We should appropriately use this new approach to treat acid-base abnormality in critically ill patients.

  20. Modeling the cometary environment using a fluid approach

    NASA Astrophysics Data System (ADS)

    Shou, Yinsi

    Comets are believed to have preserved the building material of the early solar system and to hold clues to the origin of life on Earth. Abundant remote observations of comets by telescopes and the in-situ measurements by a handful of space missions reveal that the cometary environments are complicated by various physical and chemical processes among the neutral gases and dust grains released from comets, cometary ions, and the solar wind in the interplanetary space. Therefore, physics-based numerical models are in demand to interpret the observational data and to deepen our understanding of the cometary environment. In this thesis, three models using a fluid approach, which include important physical and chemical processes underlying the cometary environment, have been developed to study the plasma, neutral gas, and the dust grains, respectively. Although models based on the fluid approach have limitations in capturing all of the correct physics for certain applications, especially for very low gas density environment, they are computationally much more efficient than alternatives. In the simulations of comet 67P/Churyumov-Gerasimenko at various heliocentric distances with a wide range of production rates, our multi-fluid cometary neutral gas model and multi-fluid cometary dust model have achieved comparable results to the Direct Simulation Monte Carlo (DSMC) model, which is based on a kinetic approach that is valid in all collisional regimes. Therefore, our model is a powerful alternative to the particle-based model, especially for some computationally intensive simulations. Capable of accounting for the varying heating efficiency under various physical conditions in a self-consistent way, the multi-fluid cometary neutral gas model is a good tool to study the dynamics of the cometary coma with different production rates and heliocentric distances. The modeled H2O expansion speeds reproduce the general trend and the speed's nonlinear dependencies of production rate

  1. Reduced order modeling of fluid/structure interaction.

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

    Barone, Matthew Franklin; Kalashnikova, Irina; Segalman, Daniel Joseph

    2009-11-01

    This report describes work performed from October 2007 through September 2009 under the Sandia Laboratory Directed Research and Development project titled 'Reduced Order Modeling of Fluid/Structure Interaction.' This project addresses fundamental aspects of techniques for construction of predictive Reduced Order Models (ROMs). A ROM is defined as a model, derived from a sequence of high-fidelity simulations, that preserves the essential physics and predictive capability of the original simulations but at a much lower computational cost. Techniques are developed for construction of provably stable linear Galerkin projection ROMs for compressible fluid flow, including a method for enforcing boundary conditions that preservesmore » numerical stability. A convergence proof and error estimates are given for this class of ROM, and the method is demonstrated on a series of model problems. A reduced order method, based on the method of quadratic components, for solving the von Karman nonlinear plate equations is developed and tested. This method is applied to the problem of nonlinear limit cycle oscillations encountered when the plate interacts with an adjacent supersonic flow. A stability-preserving method for coupling the linear fluid ROM with the structural dynamics model for the elastic plate is constructed and tested. Methods for constructing efficient ROMs for nonlinear fluid equations are developed and tested on a one-dimensional convection-diffusion-reaction equation. These methods are combined with a symmetrization approach to construct a ROM technique for application to the compressible Navier-Stokes equations.« less

  2. A new model for fluid velocity slip on a solid surface.

    PubMed

    Shu, Jian-Jun; Teo, Ji Bin Melvin; Chan, Weng Kong

    2016-10-12

    A general adsorption model is developed to describe the interactions between near-wall fluid molecules and solid surfaces. This model serves as a framework for the theoretical modelling of boundary slip phenomena. Based on this adsorption model, a new general model for the slip velocity of fluids on solid surfaces is introduced. The slip boundary condition at a fluid-solid interface has hitherto been considered separately for gases and liquids. In this paper, we show that the slip velocity in both gases and liquids may originate from dynamical adsorption processes at the interface. A unified analytical model that is valid for both gas-solid and liquid-solid slip boundary conditions is proposed based on surface science theory. The corroboration with the experimental data extracted from the literature shows that the proposed model provides an improved prediction compared to existing analytical models for gases at higher shear rates and close agreement for liquid-solid interfaces in general.

  3. Experimental Evaluation of Equivalent-Fluid Models for Melamine Foam

    NASA Technical Reports Server (NTRS)

    Allen, Albert R.; Schiller, Noah H.

    2016-01-01

    Melamine foam is a soft porous material commonly used in noise control applications. Many models exist to represent porous materials at various levels of fidelity. This work focuses on rigid frame equivalent fluid models, which represent the foam as a fluid with a complex speed of sound and density. There are several empirical models available to determine these frequency dependent parameters based on an estimate of the material flow resistivity. Alternatively, these properties can be experimentally educed using an impedance tube setup. Since vibroacoustic models are generally sensitive to these properties, this paper assesses the accuracy of several empirical models relative to impedance tube measurements collected with melamine foam samples. Diffuse field sound absorption measurements collected using large test articles in a laboratory are also compared with absorption predictions determined using model-based and measured foam properties. Melamine foam slabs of various thicknesses are considered.

  4. Numerical modeling of materials processes with fluid-fluid interfaces

    NASA Astrophysics Data System (ADS)

    Yanke, Jeffrey Michael

    A numerical model has been developed to study material processes that depend on the interaction between fluids with a large discontinuity in thermophysical properties. A base model capable of solving equations of mass, momentum, energy conservation, and solidification has been altered to enable tracking of the interface between two immiscible fluids and correctly predict the interface deformation using a volume of fluid (VOF) method. Two materials processes investigated using this technique are Electroslag Remelting (ESR) and plasma spray deposition. ESR is a secondary melting technique that passes an AC current through an electrically resistive slag to provide the heat necessary to melt the alloy. The simulation tracks the interface between the slag and metal. The model was validated against industrial scale ESR ingots and was able to predict trends in melt rate, sump depth, macrosegregation, and liquid sump depth. In order to better understand the underlying physics of the process, several constant current ESR runs simulated the effects of freezing slag in the model. Including the solidifying slag in the imulations was found to have an effect on the melt rate and sump shape but there is too much uncertainty in ESR slag property data at this time for quantitative predictions. The second process investigated in this work is the deposition of ceramic coatings via plasma spray deposition. In plasma spray deposition, powderized coating material is injected into a plasma that melts and carries the powder towards the substrate were it impacts, flattening out and freezing. The impacting droplets pile up to form a porous coating. The model is used to simulate this rain of liquid ceramic particles impacting the substrate and forming a coating. Trends in local solidification time and porosity are calculated for various particle sizes and velocities. The predictions of decreasing porosity with increasing particle velocity matches previous experimental results. Also, a

  5. The Chemical Behavior of Fluids Released during Deep Subduction Based on Fluid Inclusions

    NASA Astrophysics Data System (ADS)

    Frezzotti, M. L.; Ferrando, S.

    2014-12-01

    We present a review of current research on fluid inclusions in (HP-) UHP metamorphic rocks that, combined with existing experimental research and thermodynamic models, allow us to investigate the chemical and physical properties of fluids released during deep subduction, their solvent and element transport capacity, and the subsequent implications for the element recycling in the mantle wedge. An impressive number of fluid inclusion studies indicate three main populations of fluid inclusions in HP and UHP metamorphic rocks: i) aqueous and/or non-polar gaseous fluid inclusions (FI), ii) multiphase solid inclusions (MSI), and iii) melt inclusions (MI). Chemical data from preserved fluid inclusions in rocks match with and implement "model" fluids by experiments and thermodynamics, revealing a continuity behind the extreme variations of physico-chemical properties of subduction-zone fluids. From fore-arc to sub-arc depths, fluids released by progressive devolatilization reactions from slab lithologies change from relatively diluted chloride-bearing aqueous solutions (± N2), mainly influenced by halide ligands, to (alkali) aluminosilicate-rich aqueous fluids, in which polymerization probably governs the solubility and transport of major (e.g., Si and Al) and trace elements (including C). Fluid inclusion data implement the petrological models explaining deep volatile liberation in subduction zones, and their flux into the mantle wedge.

  6. Numerical Cerebrospinal System Modeling in Fluid-Structure Interaction.

    PubMed

    Garnotel, Simon; Salmon, Stéphanie; Balédent, Olivier

    2018-01-01

    Cerebrospinal fluid (CSF) stroke volume in the aqueduct is widely used to evaluate CSF dynamics disorders. In a healthy population, aqueduct stroke volume represents around 10% of the spinal stroke volume while intracranial subarachnoid space stroke volume represents 90%. The amplitude of the CSF oscillations through the different compartments of the cerebrospinal system is a function of the geometry and the compliances of each compartment, but we suspect that it could also be impacted be the cardiac cycle frequency. To study this CSF distribution, we have developed a numerical model of the cerebrospinal system taking into account cerebral ventricles, intracranial subarachnoid spaces, spinal canal and brain tissue in fluid-structure interactions. A numerical fluid-structure interaction model is implemented using a finite-element method library to model the cerebrospinal system and its interaction with the brain based on fluid mechanics equations and linear elasticity equations coupled in a monolithic formulation. The model geometry, simplified in a first approach, is designed in accordance with realistic volume ratios of the different compartments: a thin tube is used to mimic the high flow resistance of the aqueduct. CSF velocity and pressure and brain displacements are obtained as simulation results, and CSF flow and stroke volume are calculated from these results. Simulation results show a significant variability of aqueduct stroke volume and intracranial subarachnoid space stroke volume in the physiological range of cardiac frequencies. Fluid-structure interactions are numerous in the cerebrospinal system and difficult to understand in the rigid skull. The presented model highlights significant variations of stroke volumes under cardiac frequency variations only.

  7. A new hybrid particle/fluid model for cometary dust

    NASA Astrophysics Data System (ADS)

    Shou, Y.; Combi, M. R.; Tenishev, V.; Toth, G.; Hansen, K. C.; Huang, Z.; Gombosi, T. I.; Fougere, N.; Rubin, M.

    2017-12-01

    Cometary dust grains, which originate from comets, are believed to contain clues to the formation and the evolution of comets. They also play an important role in shaping the cometary environment, as they are able to decelerate and heat the gas through collisions, carry charges and interact with the plasma environment, and possibly sublimate gases. Therefore, the loss rate and behavior of dust grains are of interest to scientists. Currently, mainly two types of numerical dust models exist: particle models and fluid models have been developed. Particle models, which keep track of the positions and velocities of all gas and dust particles, allow crossing dust trajectories and a more accurate description of returning dust grains than the fluid model. However, in order to compute the gas drag force, the particle model needs to follow more gas particles than dust particles. A fluid model is usually more computationally efficient and is often used to provide simulations on larger spatial and temporal scales. In this work, a new hybrid model is developed to combine the advantages of both particle and fluid models. In the new approach a fluid model based on the University of Michigan BATSRUS code computes the gas properties, and feeds the gas drag force to the particle model, which is based on the Adaptive Mesh Particle Simulator (AMPS) code, to calculate the motion of dust grains. The coupling is done via the Space Weather Modeling Framework (SWMF). In addition to the capability of simulating the long-term dust phenomena, the model can also designate small active regions on the nucleus for comparison with the temporary fine dust features in observations. With the assistance of the newly developed model, the effect of viewing angles on observed dust jet shapes and the transportation of heavy dust grains from the southern to the northern hemisphere of comet 67P/Churyumov-Gerasimenko will be studied and compared with Rosetta mission images. Preliminary results will be

  8. Geochemical modeling of fluid-fluid and fluid-mineral interactions during geological CO2 storage

    NASA Astrophysics Data System (ADS)

    Zhu, C.; Ji, X.; Lu, P.

    2013-12-01

    The long time required for effective CO2 storage makes geochemical modeling an indispensable tool for CCUS. One area of geochemical modeling research that is in urgent need is impurities in CO2 streams. Permitting impurities, such as H2S, in CO2 streams can lead to potential capital and energy savings. However, predicting the consequences of co-injection of CO2 and impurities into geological formations requires the understanding of the phase equilibrium and fluid-fluid interactions. To meet this need, we developed a statistical associating fluid theory (SAFT)-based equation of state (EOS) for the H2S-CO2-H2O-NaCl system at 373.15 fluid plumes in the reservoir can be simulated. Accurate modeling of fluid-mineral interactions must confront unresolved uncertainties of silicate dissolution - precipitation reaction kinetics. Most prominent among these uncertainties is the well-known lab-field apparent discrepancy in dissolution rates. Although reactive transport models that simulate the interactions between reservoir rocks and brine, and their attendant effects on porosity and permeability changes, have proliferated, whether these results have acceptable uncertainties are unknown. We have conducted a series of batch experiments at elevated temperatures and numerical simulations of coupled dissolution and precipitation reactions. The results show that taking into account

  9. Multiscale Modeling of Multiphase Fluid Flow

    DTIC Science & Technology

    2016-08-01

    the disparate time and length scales involved in modeling fluid flow and heat transfer. Molecular dynamics simulations were carried out to provide a...fluid dynamics methods were used to investigate the heat transfer process in open-cell micro-foam with phase change material; enhancement of natural...Computational fluid dynamics, Heat transfer, Phase change material in Micro-foam, Molecular Dynamics, Multiphase flow, Multiscale modeling, Natural

  10. A New Model for Temperature Jump at a Fluid-Solid Interface

    PubMed Central

    Shu, Jian-Jun; Teo, Ji Bin Melvin; Chan, Weng Kong

    2016-01-01

    The problem presented involves the development of a new analytical model for the general fluid-solid temperature jump. To the best of our knowledge, there are no analytical models that provide the accurate predictions of the temperature jump for both gas and liquid systems. In this paper, a unified model for the fluid-solid temperature jump has been developed based on our adsorption model of the interfacial interactions. Results obtained from this model are validated with available results from the literature. PMID:27764230

  11. Coupled in silico platform: Computational fluid dynamics (CFD) and physiologically-based pharmacokinetic (PBPK) modelling.

    PubMed

    Vulović, Aleksandra; Šušteršič, Tijana; Cvijić, Sandra; Ibrić, Svetlana; Filipović, Nenad

    2018-02-15

    One of the critical components of the respiratory drug delivery is the manner in which the inhaled aerosol is deposited in respiratory tract compartments. Depending on formulation properties, device characteristics and breathing pattern, only a certain fraction of the dose will reach the target site in the lungs, while the rest of the drug will deposit in the inhalation device or in the mouth-throat region. The aim of this study was to link the Computational fluid dynamics (CFD) with physiologically-based pharmacokinetic (PBPK) modelling in order to predict aerolisolization of different dry powder formulations, and estimate concomitant in vivo deposition and absorption of amiloride hydrochloride. Drug physicochemical properties were experimentally determined and used as inputs for the CFD simulations of particle flow in the generated 3D geometric model of Aerolizer® dry powder inhaler (DPI). CFD simulations were used to simulate air flow through Aerolizer® inhaler and Discrete Phase Method (DPM) was used to simulate aerosol particles deposition within the fluid domain. The simulated values for the percent emitted dose were comparable to the values obtained using Andersen cascade impactor (ACI). However, CFD predictions indicated that aerosolized DPI have smaller particle size and narrower size distribution than assumed based on ACI measurements. Comparison with the literature in vivo data revealed that the constructed drug-specific PBPK model was able to capture amiloride absorption pattern following oral and inhalation administration. The PBPK simulation results, based on the CFD generated particle distribution data as input, illustrated the influence of formulation properties on the expected drug plasma concentration profiles. The model also predicted the influence of potential changes in physiological parameters on the extent of inhaled amiloride absorption. Overall, this study demonstrated the potential of the combined CFD-PBPK approach to model inhaled drug

  12. Theoretical models for supercritical fluid extraction.

    PubMed

    Huang, Zhen; Shi, Xiao-Han; Jiang, Wei-Juan

    2012-08-10

    For the proper design of supercritical fluid extraction processes, it is essential to have a sound knowledge of the mass transfer mechanism of the extraction process and the appropriate mathematical representation. In this paper, the advances and applications of kinetic models for describing supercritical fluid extraction from various solid matrices have been presented. The theoretical models overviewed here include the hot ball diffusion, broken and intact cell, shrinking core and some relatively simple models. Mathematical representations of these models have been in detail interpreted as well as their assumptions, parameter identifications and application examples. Extraction process of the analyte solute from the solid matrix by means of supercritical fluid includes the dissolution of the analyte from the solid, the analyte diffusion in the matrix and its transport to the bulk supercritical fluid. Mechanisms involved in a mass transfer model are discussed in terms of external mass transfer resistance, internal mass transfer resistance, solute-solid interactions and axial dispersion. The correlations of the external mass transfer coefficient and axial dispersion coefficient with certain dimensionless numbers are also discussed. Among these models, the broken and intact cell model seems to be the most relevant mathematical model as it is able to provide realistic description of the plant material structure for better understanding the mass-transfer kinetics and thus it has been widely employed for modeling supercritical fluid extraction of natural matters. Copyright © 2012 Elsevier B.V. All rights reserved.

  13. Mathematical modeling of fluid-electrolyte alterations during weightlessness

    NASA Technical Reports Server (NTRS)

    Leonard, J. I.

    1984-01-01

    Fluid electrolyte metabolism and renal endocrine control as it pertains to adaptation to weightlessness were studied. The mathematical models that have been particularly useful are discussed. However, the focus of the report is on the physiological meaning of the computer studies. A discussion of the major ground based analogs of weightlessness are included; for example, head down tilt, water immersion, and bed rest, and a comparison of findings. Several important zero g phenomena are described, including acute fluid volume regulation, blood volume regulation, circulatory changes, longer term fluid electrolyte adaptations, hormonal regulation, and body composition changes. Hypotheses are offered to explain the major findings in each area and these are integrated into a larger hypothesis of space flight adaptation. A conceptual foundation for fluid electrolyte metabolism, blood volume regulation, and cardiovascular regulation is reported.

  14. Magnetorheological properties of sodium sulphonate capped electrolytic iron based MR fluid: a comparison with CI based MR fluid

    NASA Astrophysics Data System (ADS)

    Vinod, Sithara; John, Reji; Philip, John

    2017-02-01

    Magnetorheological fluids have numerous engineering applications due to their interesting field assisted rheological behavior. Most commonly used dispersed phase in MR fluids is carbonyl iron (CI). The relatively high cost of CI warrants the need to develop cheaper alternatives to CI, without compromising rheological properties. With the above goal in mind, we have synthesized sodium sulphonate capped electrolytic iron based MR fluid and studied their magnetorheological properties. The results are compared with that of CI based MR fluid. EI and CI particles of average particle size of ∼10 μm with fumed silica particles additives are used in the present study. The dynamic yield stress for EI and CI based MR fluid were found to vary with field strength with an exponent of roughly 1.2 and 1.24, respectively. The slightly lower static and dynamic yield stress values of EI based MR fluid is attributed to the lower magnetization and polydispersity values. The dynamic yield stress showed a decrease of 18.73% and 61.8% for field strengths of 177 mT and 531 mT, respectively as the temperature was increased from 293 to 323 K. The optorheological studies showed a peak in the loss moduli, close to the crossover point of the storage and loss moduli, due to freely moving large sized aggregates along the shear direction that are dislodged from the rheometer plates at higher strains. Our results suggests that EI based MR fluids have magnetorheological behavior comparable to that of CI based MR fluids. As EI is much cheaper than CI, our findings will have important commercial implications in producing cost effective EI based MR fluids.

  15. A viable dark fluid model

    NASA Astrophysics Data System (ADS)

    Elkhateeb, Esraa

    2018-01-01

    We consider a cosmological model based on a generalization of the equation of state proposed by Nojiri and Odintsov (2004) and Štefančić (2005, 2006). We argue that this model works as a dark fluid model which can interpolate between dust equation of state and the dark energy equation of state. We show how the asymptotic behavior of the equation of state constrained the parameters of the model. The causality condition for the model is also studied to constrain the parameters and the fixed points are tested to determine different solution classes. Observations of Hubble diagram of SNe Ia supernovae are used to further constrain the model. We present an exact solution of the model and calculate the luminosity distance and the energy density evolution. We also calculate the deceleration parameter to test the state of the universe expansion.

  16. Mechanistic Fluid Transport Model to Estimate Gastrointestinal Fluid Volume and Its Dynamic Change Over Time.

    PubMed

    Yu, Alex; Jackson, Trachette; Tsume, Yasuhiro; Koenigsknecht, Mark; Wysocki, Jeffrey; Marciani, Luca; Amidon, Gordon L; Frances, Ann; Baker, Jason R; Hasler, William; Wen, Bo; Pai, Amit; Sun, Duxin

    2017-11-01

    Gastrointestinal (GI) fluid volume and its dynamic change are integral to study drug disintegration, dissolution, transit, and absorption. However, key questions regarding the local volume and its absorption, secretion, and transit remain unanswered. The dynamic fluid compartment absorption and transit (DFCAT) model is proposed to estimate in vivo GI volume and GI fluid transport based on magnetic resonance imaging (MRI) quantified fluid volume. The model was validated using GI local concentration of phenol red in human GI tract, which was directly measured by human GI intubation study after oral dosing of non-absorbable phenol red. The measured local GI concentration of phenol red ranged from 0.05 to 168 μg/mL (stomach), to 563 μg/mL (duodenum), to 202 μg/mL (proximal jejunum), and to 478 μg/mL (distal jejunum). The DFCAT model characterized observed MRI fluid volume and its dynamic changes from 275 to 46.5 mL in stomach (from 0 to 30 min) with mucus layer volume of 40 mL. The volumes of the 30 small intestine compartments were characterized by a max of 14.98 mL to a min of 0.26 mL (0-120 min) and a mucus layer volume of 5 mL per compartment. Regional fluid volumes over 0 to 120 min ranged from 5.6 to 20.38 mL in the proximal small intestine, 36.4 to 44.08 mL in distal small intestine, and from 42 to 64.46 mL in total small intestine. The DFCAT model can be applied to predict drug dissolution and absorption in the human GI tract with future improvements.

  17. An evaluation of Computational Fluid dynamics model for flood risk analysis

    NASA Astrophysics Data System (ADS)

    Di Francesco, Silvia; Biscarini, Chiara; Montesarchio, Valeria

    2014-05-01

    This work presents an analysis of the hydrological-hydraulic engineering requisites for Risk evaluation and efficient flood damage reduction plans. Most of the research efforts have been dedicated to the scientific and technical aspects of risk assessment, providing estimates of possible alternatives and of the risk associated. In the decision making process for mitigation plan, the contribute of scientist is crucial, due to the fact that Risk-Damage analysis is based on evaluation of flow field ,of Hydraulic Risk and on economical and societal considerations. The present paper will focus on the first part of process, the mathematical modelling of flood events which is the base for all further considerations. The evaluation of potential catastrophic damage consequent to a flood event and in particular to dam failure requires modelling of the flood with sufficient detail so to capture the spatial and temporal evolutions of the event, as well of the velocity field. Thus, the selection of an appropriate mathematical model to correctly simulate flood routing is an essential step. In this work we present the application of two 3D Computational fluid dynamics models to a synthetic and real case study in order to evaluate the correct evolution of flow field and the associated flood Risk . The first model is based on a opensource CFD platform called openFoam. Water flow is schematized with a classical continuum approach based on Navier-Stokes equation coupled with Volume of fluid (VOF) method to take in account the multiphase character of river bottom-water- air systems. The second model instead is based on the Lattice Boltzmann method, an innovative numerical fluid dynamics scheme based on Boltzmann's kinetic equation that represents the flow dynamics at the macroscopic level by incorporating a microscopic kinetic approach. Fluid is seen as composed by particles that can move and collide among them. Simulation results from both models are promising and congruent to

  18. SPH modeling of fluid-structure interaction

    NASA Astrophysics Data System (ADS)

    Han, Luhui; Hu, Xiangyu

    2018-02-01

    This work concerns numerical modeling of fluid-structure interaction (FSI) problems in a uniform smoothed particle hydrodynamics (SPH) framework. It combines a transport-velocity SPH scheme, advancing fluid motions, with a total Lagrangian SPH formulation dealing with the structure deformations. Since both fluid and solid governing equations are solved in SPH framework, while coupling becomes straightforward, the momentum conservation of the FSI system is satisfied strictly. A well-known FSI benchmark test case has been performed to validate the modeling and to demonstrate its potential.

  19. Numerical Modeling of Fluid Flow in Solid Tumors

    PubMed Central

    Soltani, M.; Chen, P.

    2011-01-01

    A mathematical model of interstitial fluid flow is developed, based on the application of the governing equations for fluid flow, i.e., the conservation laws for mass and momentum, to physiological systems containing solid tumors. The discretized form of the governing equations, with appropriate boundary conditions, is developed for a predefined tumor geometry. The interstitial fluid pressure and velocity are calculated using a numerical method, element based finite volume. Simulations of interstitial fluid transport in a homogeneous solid tumor demonstrate that, in a uniformly perfused tumor, i.e., one with no necrotic region, because of the interstitial pressure distribution, the distribution of drug particles is non-uniform. Pressure distribution for different values of necrotic radii is examined and two new parameters, the critical tumor radius and critical necrotic radius, are defined. Simulation results show that: 1) tumor radii have a critical size. Below this size, the maximum interstitial fluid pressure is less than what is generally considered to be effective pressure (a parameter determined by vascular pressure, plasma osmotic pressure, and interstitial osmotic pressure). Above this size, the maximum interstitial fluid pressure is equal to effective pressure. As a consequence, drugs transport to the center of smaller tumors is much easier than transport to the center of a tumor whose radius is greater than the critical tumor radius; 2) there is a critical necrotic radius, below which the interstitial fluid pressure at the tumor center is at its maximum value. If the tumor radius is greater than the critical tumor radius, this maximum pressure is equal to effective pressure. Above this critical necrotic radius, the interstitial fluid pressure at the tumor center is below effective pressure. In specific ranges of these critical sizes, drug amount and therefore therapeutic effects are higher because the opposing force, interstitial fluid pressure, is low in

  20. Micro-poromechanics model of fluid-saturated chemically active fibrous media.

    PubMed

    Misra, Anil; Parthasarathy, Ranganathan; Singh, Viraj; Spencer, Paulette

    2015-02-01

    We have developed a micromechanics based model for chemically active saturated fibrous media that incorporates fiber network microstructure, chemical potential driven fluid flow, and micro-poromechanics. The stress-strain relationship of the dry fibrous media is first obtained by considering the fiber behavior. The constitutive relationships applicable to saturated media are then derived in the poromechanics framework using Hill's volume averaging. The advantage of this approach is that the resultant continuum model accounts for the discrete nature of the individual fibers while retaining a form suitable for porous materials. As a result, the model is able to predict the influence of micro-scale phenomena, such as the fiber pre-strain caused by osmotic effects and evolution of fiber network structure with loading, on the overall behavior and in particular, on the poromechanics parameters. Additionally, the model can describe fluid-flow related rate-dependent behavior under confined and unconfined conditions and varying chemical environments. The significance of the approach is demonstrated by simulating unconfined drained monotonic uniaxial compression under different surrounding fluid bath molarity, and fluid-flow related creep and relaxation at different loading-levels and different surrounding fluid bath molarity. The model predictions conform to the experimental observations for saturated soft fibrous materials. The method can potentially be extended to other porous materials such as bone, clays, foams and concrete.

  1. Combining Computational Fluid Dynamics and Agent-Based Modeling: A New Approach to Evacuation Planning

    PubMed Central

    Epstein, Joshua M.; Pankajakshan, Ramesh; Hammond, Ross A.

    2011-01-01

    We introduce a novel hybrid of two fields—Computational Fluid Dynamics (CFD) and Agent-Based Modeling (ABM)—as a powerful new technique for urban evacuation planning. CFD is a predominant technique for modeling airborne transport of contaminants, while ABM is a powerful approach for modeling social dynamics in populations of adaptive individuals. The hybrid CFD-ABM method is capable of simulating how large, spatially-distributed populations might respond to a physically realistic contaminant plume. We demonstrate the overall feasibility of CFD-ABM evacuation design, using the case of a hypothetical aerosol release in Los Angeles to explore potential effectiveness of various policy regimes. We conclude by arguing that this new approach can be powerfully applied to arbitrary population centers, offering an unprecedented preparedness and catastrophic event response tool. PMID:21687788

  2. Fluid and Electrolyte Balance model (FEB)

    NASA Technical Reports Server (NTRS)

    Fitzjerrell, D. G.

    1973-01-01

    The effects of various oral input water loads on solute and water distribution throughout the body are presented in the form of a model. The model was a three compartment model; the three compartments being plasma, interstitial fluid and cellular fluid. Sodium, potassium, chloride and urea were the only major solutes considered explicitly. The control of body water and electrolyte distribution was affected via drinking and hormone levels.

  3. Lattice Boltzmann model for three-phase viscoelastic fluid flow

    NASA Astrophysics Data System (ADS)

    Xie, Chiyu; Lei, Wenhai; Wang, Moran

    2018-02-01

    A lattice Boltzmann (LB) framework is developed for simulation of three-phase viscoelastic fluid flows in complex geometries. This model is based on a Rothman-Keller type model for immiscible multiphase flows which ensures mass conservation of each component in porous media even for a high density ratio. To account for the viscoelastic effects, the Maxwell constitutive relation is correctly introduced into the momentum equation, which leads to a modified lattice Boltzmann evolution equation for Maxwell fluids by removing the normal but excess viscous term. Our simulation tests indicate that this excess viscous term may induce significant errors. After three benchmark cases, the displacement processes of oil by dispersed polymer are studied as a typical example of three-phase viscoelastic fluid flow. The results show that increasing either the polymer intrinsic viscosity or the elastic modulus will enhance the oil recovery.

  4. Modeling and comparative study of fluid velocities in heterogeneous rocks

    NASA Astrophysics Data System (ADS)

    Hingerl, Ferdinand F.; Romanenko, Konstantin; Pini, Ronny; Balcom, Bruce; Benson, Sally

    2013-04-01

    permeabilities were then correlated with the ones based on the porosity maps and the Kozeny-Carman relationship. The findings of the comparative modeling study are discussed and its potential impact on the modeling of fluid residence times and kinetic reaction rates of fluid-rock interactions in rocks containing meso-scale heterogeneities are reviewed.

  5. Atomistic Modeling of the Fluid-Solid Interface in Simple Fluids

    NASA Astrophysics Data System (ADS)

    Hadjiconstantinou, Nicolas; Wang, Gerald

    2017-11-01

    Fluids can exhibit pronounced structuring effects near a solid boundary, typically manifested in a layered structure that has been extensively shown to directly affect transport across the interface. We present and discuss several results from molecular-mechanical modeling and molecular-dynamics (MD) simulations aimed at characterizing the structure of the first fluid layer directly adjacent to the solid. We identify a new dimensionless group - termed the Wall number - which characterizes the degree of fluid layering, by comparing the competing effects of wall-fluid interaction and thermal energy. We find that in the layering regime, several key features of the first layer layer - including its distance from the solid, its width, and its areal density - can be described using mean-field-energy arguments, as well as asymptotic analysis of the Nernst-Planck equation. For dense fluids, the areal density and the width of the first layer can be related to the bulk fluid density using a simple scaling relation. MD simulations show that these results are broadly applicable and robust to the presence of a second confining solid boundary, different choices of wall structure and thermalization, strengths of fluid-solid interaction, and wall geometries.

  6. A THC Simulator for Modeling Fluid-Rock Interactions

    NASA Astrophysics Data System (ADS)

    Hamidi, Sahar; Galvan, Boris; Heinze, Thomas; Miller, Stephen

    2014-05-01

    Fluid-rock interactions play an essential role in many earth processes, from a likely influence on earthquake nucleation and aftershocks, to enhanced geothermal system, carbon capture and storage (CCS), and underground nuclear waste repositories. In THC models, two-way interactions between different processes (thermal, hydraulic and chemical) are present. Fluid flow influences the permeability of the rock especially if chemical reactions are taken into account. On one hand solute concentration influences fluid properties while, on the other hand, heat can affect further chemical reactions. Estimating heat production from a naturally fractured geothermal systems remains a complex problem. Previous works are typically based on a local thermal equilibrium assumption and rarely consider the salinity. The dissolved salt in fluid affects the hydro- and thermodynamical behavior of the system by changing the hydraulic properties of the circulating fluid. Coupled thermal-hydraulic-chemical models (THC) are important for investigating these processes, but what is needed is a coupling to mechanics to result in THMC models. Although similar models currently exist (e.g. PFLOTRAN), our objective here is to develop algorithms for implementation using the Graphics Processing Unit (GPU) computer architecture to be run on GPU clusters. To that aim, we present a two-dimensional numerical simulation of a fully coupled non-isothermal non-reactive solute flow. The thermal part of the simulation models heat transfer processes for either local thermal equilibrium or nonequilibrium cases, and coupled to a non-reactive mass transfer described by a non-linear diffusion/dispersion model. The flow process of the model includes a non-linear Darcian flow for either saturated or unsaturated scenarios. For the unsaturated case, we use the Richards' approximation for a mixture of liquid and gas phases. Relative permeability and capillary pressure are determined by the van Genuchten relations

  7. A design methodology of magentorheological fluid damper using Herschel-Bulkley model

    NASA Astrophysics Data System (ADS)

    Liao, Linqing; Liao, Changrong; Cao, Jianguo; Fu, L. J.

    2003-09-01

    Magnetorheological fluid (MR fluid) is highly concentrated suspension of very small magnetic particle in inorganic oil. The essential behavior of MR fluid is its ability to reversibly change from free-flowing, linear viscous liquids to semi-solids having controllable yield strength in milliseconds when exposed to magnetic field. This feature provides simple, quiet, rapid-response interfaces between electronic controls and mechanical systems. In this paper, a mini-bus MR fluid damper based on plate Poiseuille flow mode is typically analyzed using Herschel-Bulkley model, which can be used to account for post-yield shear thinning or thickening under the quasi-steady flow condition. In the light of various value of flow behavior index, the influences of post-yield shear thinning or thickening on flow velocity profiles of MR fluid in annular damping orifice are examined numerically. Analytical damping coefficient predictions also are compared via the nonlinear Bingham plastic model and Herschel-Bulkley constitutive model. A MR fluid damper, which is designed and fabricated according to design method presented in this paper, has tested by electro-hydraulic servo vibrator and its control system in National Center for Test and Supervision of Coach Quality. The experimental results reveal that the analysis methodology and design theory are reasonable and MR fluid damper can be designed according to the design methodology.

  8. Nonlinear multimodal model for TLD of irregular tank geometry and small fluid depth

    NASA Astrophysics Data System (ADS)

    Love, J. S.; Tait, M. J.

    2013-11-01

    Tuned liquid dampers (TLDs) utilize sloshing fluid to absorb and dissipate structural vibrational energy. TLDs of irregular or complex tank geometry may be required in practice to avoid tank interference with fixed structural or mechanical components. The literature offers few analytical models to predict the response of this type of TLD, particularly when the fluid depth is small. In this paper, a multimodal model is developed utilizing a Boussinesq-type modal theory which is valid for small TLD fluid depths. The Bateman-Luke variational principle is employed to develop a system of coupled nonlinear ordinary differential equations which describe the fluid response when the tank is subjected to base excitation. Energy dissipation is incorporated into the model from the inclusion of damping screens. The fluid model is used to describe the response of a 2D structure-TLD system when the structure is subjected to external loading and the TLD tank geometry is irregular.

  9. OpenFLUID: an open-source software environment for modelling fluxes in landscapes

    NASA Astrophysics Data System (ADS)

    Fabre, Jean-Christophe; Rabotin, Michaël; Crevoisier, David; Libres, Aline; Dagès, Cécile; Moussa, Roger; Lagacherie, Philippe; Raclot, Damien; Voltz, Marc

    2013-04-01

    Integrative landscape functioning has become a common concept in environmental management. Landscapes are complex systems where many processes interact in time and space. In agro-ecosystems, these processes are mainly physical processes, including hydrological-processes, biological processes and human activities. Modelling such systems requires an interdisciplinary approach, coupling models coming from different disciplines, developed by different teams. In order to support collaborative works, involving many models coupled in time and space for integrative simulations, an open software modelling platform is a relevant answer. OpenFLUID is an open source software platform for modelling landscape functioning, mainly focused on spatial fluxes. It provides an advanced object-oriented architecture allowing to i) couple models developed de novo or from existing source code, and which are dynamically plugged to the platform, ii) represent landscapes as hierarchical graphs, taking into account multi-scale, spatial heterogeneities and landscape objects connectivity, iii) run and explore simulations in many ways : using the OpenFLUID software interfaces for users (command line interface, graphical user interface), or using external applications such as GNU R through the provided ROpenFLUID package. OpenFLUID is developed in C++ and relies on open source libraries only (Boost, libXML2, GLib/GTK, OGR/GDAL, …). For modelers and developers, OpenFLUID provides a dedicated environment for model development, which is based on an open source toolchain, including the Eclipse editor, the GCC compiler and the CMake build system. OpenFLUID is distributed under the GPLv3 open source license, with a special exception allowing to plug existing models licensed under any license. It is clearly in the spirit of sharing knowledge and favouring collaboration in a community of modelers. OpenFLUID has been involved in many research applications, such as modelling of hydrological network

  10. Dynamic bulk and shear moduli due to grain-scale local fluid flow in fluid-saturated cracked poroelastic rocks: Theoretical model

    NASA Astrophysics Data System (ADS)

    Song, Yongjia; Hu, Hengshan; Rudnicki, John W.

    2016-07-01

    Grain-scale local fluid flow is an important loss mechanism for attenuating waves in cracked fluid-saturated poroelastic rocks. In this study, a dynamic elastic modulus model is developed to quantify local flow effect on wave attenuation and velocity dispersion in porous isotropic rocks. The Eshelby transform technique, inclusion-based effective medium model (the Mori-Tanaka scheme), fluid dynamics and mass conservation principle are combined to analyze pore-fluid pressure relaxation and its influences on overall elastic properties. The derivation gives fully analytic, frequency-dependent effective bulk and shear moduli of a fluid-saturated porous rock. It is shown that the derived bulk and shear moduli rigorously satisfy the Biot-Gassmann relationship of poroelasticity in the low-frequency limit, while they are consistent with isolated-pore effective medium theory in the high-frequency limit. In particular, a simplified model is proposed to quantify the squirt-flow dispersion for frequencies lower than stiff-pore relaxation frequency. The main advantage of the proposed model over previous models is its ability to predict the dispersion due to squirt flow between pores and cracks with distributed aspect ratio instead of flow in a simply conceptual double-porosity structure. Independent input parameters include pore aspect ratio distribution, fluid bulk modulus and viscosity, and bulk and shear moduli of the solid grain. Physical assumptions made in this model include (1) pores are inter-connected and (2) crack thickness is smaller than the viscous skin depth. This study is restricted to linear elastic, well-consolidated granular rocks.

  11. Direct modeling for computational fluid dynamics

    NASA Astrophysics Data System (ADS)

    Xu, Kun

    2015-06-01

    All fluid dynamic equations are valid under their modeling scales, such as the particle mean free path and mean collision time scale of the Boltzmann equation and the hydrodynamic scale of the Navier-Stokes (NS) equations. The current computational fluid dynamics (CFD) focuses on the numerical solution of partial differential equations (PDEs), and its aim is to get the accurate solution of these governing equations. Under such a CFD practice, it is hard to develop a unified scheme that covers flow physics from kinetic to hydrodynamic scales continuously because there is no such governing equation which could make a smooth transition from the Boltzmann to the NS modeling. The study of fluid dynamics needs to go beyond the traditional numerical partial differential equations. The emerging engineering applications, such as air-vehicle design for near-space flight and flow and heat transfer in micro-devices, do require further expansion of the concept of gas dynamics to a larger domain of physical reality, rather than the traditional distinguishable governing equations. At the current stage, the non-equilibrium flow physics has not yet been well explored or clearly understood due to the lack of appropriate tools. Unfortunately, under the current numerical PDE approach, it is hard to develop such a meaningful tool due to the absence of valid PDEs. In order to construct multiscale and multiphysics simulation methods similar to the modeling process of constructing the Boltzmann or the NS governing equations, the development of a numerical algorithm should be based on the first principle of physical modeling. In this paper, instead of following the traditional numerical PDE path, we introduce direct modeling as a principle for CFD algorithm development. Since all computations are conducted in a discretized space with limited cell resolution, the flow physics to be modeled has to be done in the mesh size and time step scales. Here, the CFD is more or less a direct

  12. Modeling of Complex Coupled Fluid-Structure Interaction Systems in Arbitrary Water Depth

    DTIC Science & Technology

    2009-01-01

    basin. For the particle finite- element method ( PFEM ) near-field fluid model we completed: (4) the development of a fully-coupled fluid/flexible...method ( PFEM ) based framework for the ALE-RANS solver [1]. We presented the theory of ALE-RANS with a k- turbulence closure model and several numerical...implemented by PFEM (Task (4)). In this work a universal wall function (UWF) is introduced and implemented to more accurately predict the boundary

  13. Model structure identification for wastewater treatment simulation based on computational fluid dynamics.

    PubMed

    Alex, J; Kolisch, G; Krause, K

    2002-01-01

    The objective of this presented project is to use the results of an CFD simulation to automatically, systematically and reliably generate an appropriate model structure for simulation of the biological processes using CSTR activated sludge compartments. Models and dynamic simulation have become important tools for research but also increasingly for the design and optimisation of wastewater treatment plants. Besides the biological models several cases are reported about the application of computational fluid dynamics ICFD) to wastewater treatment plants. One aim of the presented method to derive model structures from CFD results is to exclude the influence of empirical structure selection to the result of dynamic simulations studies of WWTPs. The second application of the approach developed is the analysis of badly performing treatment plants where the suspicion arises that bad flow behaviour such as short cut flows is part of the problem. The method suggested requires as the first step the calculation of fluid dynamics of the biological treatment step at different loading situations by use of 3-dimensional CFD simulation. The result of this information is used to generate a suitable model structure for conventional dynamic simulation of the treatment plant by use of a number of CSTR modules with a pattern of exchange flows between the tanks automatically. The method is explained in detail and the application to the WWTP Wuppertal Buchenhofen is presented.

  14. Numerical modeling of fluid migration in subduction zones

    NASA Astrophysics Data System (ADS)

    Walter, M. J.; Quinteros, J.; Sobolev, S. V.

    2015-12-01

    It is well known that fluids play a crucial role in subduction evolution. For example, mechanical weakening along tectonic interfaces, due to high fluid pressure, may enable oceanic subduction. Hence, the fluid content seems to be a critical parameter for subduction initiation. Studies have also shown a correlation between the location of slab dehydration and intermediate seismic activity. Furthermore, expelled fluids from the subduction slab affect the melting temperature, consequently, contributing to partial melting in the wedge above the down-going plate and extensive volcanism. In summary, fluids have a great impact on tectonic processes and therefore should be incorporated into geodynamic numerical models. Here we use existing approaches to couple and solve fluid flow equations in the SLIM-3D thermo-mechanical code. SLIM-3D is a three-dimensional thermo-mechanical code capable of simulating lithospheric deformation with elasto-visco-plastic rheology. It has been successfully applied to model geodynamic processes at different tectonic settings, including subduction zones. However, although SLIM-3D already includes many features, fluid migration has not been incorporated into the model yet. To this end, we coupled solid and fluid flow assuming that fluids flow through a porous and deformable solid. Thereby, we introduce a two-phase flow into the model, in which the Stokes flow is coupled with the Darcy law for fluid flow. Ultimately, the evolution of porosity is governed by a compaction pressure and the advection of the porous solid. We show the details of our implementation of the fluid flow into the existing thermo-mechanical finite element code and present first results of benchmarks and experiments. We are especially interested in the coupling of subduction processes and the evolution of the magmatic arc. Thereby, we focus on the key factors controlling magma emplacement and its influence on subduction processes.

  15. Comments on Frequency Swept Rotating Input Perturbation Techniques and Identification of the Fluid Force Models in Rotor/bearing/seal Systems and Fluid Handling Machines

    NASA Technical Reports Server (NTRS)

    Muszynska, Agnes; Bently, Donald E.

    1991-01-01

    Perturbation techniques used for identification of rotating system dynamic characteristics are described. A comparison between two periodic frequency-swept perturbation methods applied in identification of fluid forces of rotating machines is presented. The description of the fluid force model identified by inputting circular periodic frequency-swept force is given. This model is based on the existence and strength of the circumferential flow, most often generated by the shaft rotation. The application of the fluid force model in rotor dynamic analysis is presented. It is shown that the rotor stability is an entire rotating system property. Some areas for further research are discussed.

  16. Numerical modelling of fluid-rock interactions: Lessons learnt from carbonate rocks diagenesis studies

    NASA Astrophysics Data System (ADS)

    Nader, Fadi; Bachaud, Pierre; Michel, Anthony

    2015-04-01

    Quantitative assessment of fluid-rock interactions and their impact on carbonate host-rocks has recently become a very attractive research topic within academic and industrial realms. Today, a common operational workflow that aims at predicting the relevant diagenetic processes on the host rocks (i.e. fluid-rock interactions) consists of three main stages: i) constructing a conceptual diagenesis model including inferred preferential fluids pathways; ii) quantifying the resulted diagenetic phases (e.g. depositing cements, dissolved and recrystallized minerals); and iii) numerical modelling of diagenetic processes. Most of the concepts of diagenetic processes operate at the larger, basin-scale, however, the description of the diagenetic phases (products of such processes) and their association with the overall petrophysical evolution of sedimentary rocks remain at reservoir (and even outcrop/ well core) scale. Conceptual models of diagenetic processes are thereafter constructed based on studying surface-exposed rocks and well cores (e.g. petrography, geochemistry, fluid inclusions). We are able to quantify the diagenetic products with various evolving techniques and on varying scales (e.g. point-counting, 2D and 3D image analysis, XRD, micro-CT and pore network models). Geochemical modelling makes use of thermodynamic and kinetic rules as well as data-bases to simulate chemical reactions and fluid-rock interactions. This can be through a 0D model, whereby a certain process is tested (e.g. the likelihood of a certain chemical reaction to operate under specific conditions). Results relate to the fluids and mineral phases involved in the chemical reactions. They could be used as arguments to support or refute proposed outcomes of fluid-rock interactions. Coupling geochemical modelling with transport (reactive transport model; 1D, 2D and 3D) is another possibility, attractive as it provides forward simulations of diagenetic processes and resulting phases. This

  17. Fluid Dynamics Lagrangian Simulation Model

    NASA Astrophysics Data System (ADS)

    Hyman, Ellis

    1994-02-01

    The work performed by Science Applications International Corporation (SAIC) on this contract, Fluid Dynamics Lagrangian Simulation Model, Contract Number N00014-89-C-2106, SAIC Project Number 01-0157-03-0768, focused on a number of research topics in fluid dynamics. The work was in support of the programs of NRL's Laboratory for Computational Physics and Fluid Dynamics and covered the period from 10 September 1989 to 9 December 1993. In the following sections, we describe each of the efforts and the results obtained. Much of the research work has resulted in journal publications. These are included in Appendices of this report for which the reader is referred for complete details.

  18. On hydrodynamic phase field models for binary fluid mixtures

    NASA Astrophysics Data System (ADS)

    Yang, Xiaogang; Gong, Yuezheng; Li, Jun; Zhao, Jia; Wang, Qi

    2018-05-01

    Two classes of thermodynamically consistent hydrodynamic phase field models have been developed for binary fluid mixtures of incompressible viscous fluids of possibly different densities and viscosities. One is quasi-incompressible, while the other is incompressible. For the same binary fluid mixture of two incompressible viscous fluid components, which one is more appropriate? To answer this question, we conduct a comparative study in this paper. First, we visit their derivation, conservation and energy dissipation properties and show that the quasi-incompressible model conserves both mass and linear momentum, while the incompressible one does not. We then show that the quasi-incompressible model is sensitive to the density deviation of the fluid components, while the incompressible model is not in a linear stability analysis. Second, we conduct a numerical investigation on coarsening or coalescent dynamics of protuberances using the two models. We find that they can predict quite different transient dynamics depending on the initial conditions and the density difference although they predict essentially the same quasi-steady results in some cases. This study thus cast a doubt on the applicability of the incompressible model to describe dynamics of binary mixtures of two incompressible viscous fluids especially when the two fluid components have a large density deviation.

  19. Thermal lattice BGK models for fluid dynamics

    NASA Astrophysics Data System (ADS)

    Huang, Jian

    1998-11-01

    As an alternative in modeling fluid dynamics, the Lattice Boltzmann method has attracted considerable attention. In this thesis, we shall present a general form of thermal Lattice BGK. This form can handle large differences in density, temperature, and high Mach number. This generalized method can easily model gases with different adiabatic index values. The numerical transport coefficients of this model are estimated both theoretically and numerically. Their dependency on the sizes of integration steps in time and space, and on the flow velocity and temperature, are studied and compared with other established CFD methods. This study shows that the numerical viscosity of the Lattice Boltzmann method depends linearly on the space interval, and on the flow velocity as well for supersonic flow. This indicates this method's limitation in modeling high Reynolds number compressible thermal flow. On the other hand, the Lattice Boltzmann method shows promise in modeling micro-flows, i.e., gas flows in micron-sized devices. A two-dimensional code has been developed based on the conventional thermal lattice BGK model, with some modifications and extensions for micro- flows and wall-fluid interactions. Pressure-driven micro- channel flow has been simulated. Results are compared with experiments and simulations using other methods, such as a spectral element code using slip boundary condition with Navier-Stokes equations and a Direct Simulation Monte Carlo (DSMC) method.

  20. A Deep Learning based Approach to Reduced Order Modeling of Fluids using LSTM Neural Networks

    NASA Astrophysics Data System (ADS)

    Mohan, Arvind; Gaitonde, Datta

    2017-11-01

    Reduced Order Modeling (ROM) can be used as surrogates to prohibitively expensive simulations to model flow behavior for long time periods. ROM is predicated on extracting dominant spatio-temporal features of the flow from CFD or experimental datasets. We explore ROM development with a deep learning approach, which comprises of learning functional relationships between different variables in large datasets for predictive modeling. Although deep learning and related artificial intelligence based predictive modeling techniques have shown varied success in other fields, such approaches are in their initial stages of application to fluid dynamics. Here, we explore the application of the Long Short Term Memory (LSTM) neural network to sequential data, specifically to predict the time coefficients of Proper Orthogonal Decomposition (POD) modes of the flow for future timesteps, by training it on data at previous timesteps. The approach is demonstrated by constructing ROMs of several canonical flows. Additionally, we show that statistical estimates of stationarity in the training data can indicate a priori how amenable a given flow-field is to this approach. Finally, the potential and limitations of deep learning based ROM approaches will be elucidated and further developments discussed.

  1. Parametric Modeling for Fluid Systems

    NASA Technical Reports Server (NTRS)

    Pizarro, Yaritzmar Rosario; Martinez, Jonathan

    2013-01-01

    Fluid Systems involves different projects that require parametric modeling, which is a model that maintains consistent relationships between elements as is manipulated. One of these projects is the Neo Liquid Propellant Testbed, which is part of Rocket U. As part of Rocket U (Rocket University), engineers at NASA's Kennedy Space Center in Florida have the opportunity to develop critical flight skills as they design, build and launch high-powered rockets. To build the Neo testbed; hardware from the Space Shuttle Program was repurposed. Modeling for Neo, included: fittings, valves, frames and tubing, between others. These models help in the review process, to make sure regulations are being followed. Another fluid systems project that required modeling is Plant Habitat's TCUI test project. Plant Habitat is a plan to develop a large growth chamber to learn the effects of long-duration microgravity exposure to plants in space. Work for this project included the design and modeling of a duct vent for flow test. Parametric Modeling for these projects was done using Creo Parametric 2.0.

  2. Seismic low-frequency-based calculation of reservoir fluid mobility and its applications

    NASA Astrophysics Data System (ADS)

    Chen, Xue-Hua; He, Zhen-Hua; Zhu, Si-Xin; Liu, Wei; Zhong, Wen-Li

    2012-06-01

    Low frequency content of seismic signals contains information related to the reservoir fluid mobility. Based on the asymptotic analysis theory of frequency-dependent reflectivity from a fluid-saturated poroelastic medium, we derive the computational implementation of reservoir fluid mobility and present the determination of optimal frequency in the implementation. We then calculate the reservoir fluid mobility using the optimal frequency instantaneous spectra at the low-frequency end of the seismic spectrum. The methodology is applied to synthetic seismic data from a permeable gas-bearing reservoir model and real land and marine seismic data. The results demonstrate that the fluid mobility shows excellent quality in imaging the gas reservoirs. It is feasible to detect the location and spatial distribution of gas reservoirs and reduce the non-uniqueness and uncertainty in fluid identification.

  3. Including fluid shear viscosity in a structural acoustic finite element model using a scalar fluid representation

    PubMed Central

    Cheng, Lei; Li, Yizeng; Grosh, Karl

    2013-01-01

    An approximate boundary condition is developed in this paper to model fluid shear viscosity at boundaries of coupled fluid-structure system. The effect of shear viscosity is approximated by a correction term to the inviscid boundary condition, written in terms of second order in-plane derivatives of pressure. Both thin and thick viscous boundary layer approximations are formulated; the latter subsumes the former. These approximations are used to develop a variational formation, upon which a viscous finite element method (FEM) model is based, requiring only minor modifications to the boundary integral contributions of an existing inviscid FEM model. Since this FEM formulation has only one degree of freedom for pressure, it holds a great computational advantage over the conventional viscous FEM formulation which requires discretization of the full set of linearized Navier-Stokes equations. The results from thick viscous boundary layer approximation are found to be in good agreement with the prediction from a Navier-Stokes model. When applicable, thin viscous boundary layer approximation also gives accurate results with computational simplicity compared to the thick boundary layer formulation. Direct comparison of simulation results using the boundary layer approximations and a full, linearized Navier-Stokes model are made and used to evaluate the accuracy of the approximate technique. Guidelines are given for the parameter ranges over which the accurate application of the thick and thin boundary approximations can be used for a fluid-structure interaction problem. PMID:23729844

  4. Including fluid shear viscosity in a structural acoustic finite element model using a scalar fluid representation.

    PubMed

    Cheng, Lei; Li, Yizeng; Grosh, Karl

    2013-08-15

    An approximate boundary condition is developed in this paper to model fluid shear viscosity at boundaries of coupled fluid-structure system. The effect of shear viscosity is approximated by a correction term to the inviscid boundary condition, written in terms of second order in-plane derivatives of pressure. Both thin and thick viscous boundary layer approximations are formulated; the latter subsumes the former. These approximations are used to develop a variational formation, upon which a viscous finite element method (FEM) model is based, requiring only minor modifications to the boundary integral contributions of an existing inviscid FEM model. Since this FEM formulation has only one degree of freedom for pressure, it holds a great computational advantage over the conventional viscous FEM formulation which requires discretization of the full set of linearized Navier-Stokes equations. The results from thick viscous boundary layer approximation are found to be in good agreement with the prediction from a Navier-Stokes model. When applicable, thin viscous boundary layer approximation also gives accurate results with computational simplicity compared to the thick boundary layer formulation. Direct comparison of simulation results using the boundary layer approximations and a full, linearized Navier-Stokes model are made and used to evaluate the accuracy of the approximate technique. Guidelines are given for the parameter ranges over which the accurate application of the thick and thin boundary approximations can be used for a fluid-structure interaction problem.

  5. DNA methylation-based age prediction from various tissues and body fluids

    PubMed Central

    Jung, Sang-Eun; Shin, Kyoung-Jin; Lee, Hwan Young

    2017-01-01

    Aging is a natural and gradual process in human life. It is influenced by heredity, environment, lifestyle, and disease. DNA methylation varies with age, and the ability to predict the age of donor using DNA from evidence materials at a crime scene is of considerable value in forensic investigations. Recently, many studies have reported age prediction models based on DNA methylation from various tissues and body fluids. Those models seem to be very promising because of their high prediction accuracies. In this review, the changes of age-associated DNA methylation and the age prediction models for various tissues and body fluids were examined, and then the applicability of the DNA methylation-based age prediction method to the forensic investigations was discussed. This will improve the understandings about DNA methylation markers and their potential to be used as biomarkers in the forensic field, as well as the clinical field. PMID:28946940

  6. Preliminary model of fluid and solute distribution and transport during hemorrhage.

    PubMed

    Gyenge, C C; Bowen, B D; Reed, R K; Bert, J L

    2003-01-01

    The distribution and transport of fluid, ions, and other solutes (plasma proteins and glucose) are described in a mathematical model of unresuscitated hemorrhage. The model is based on balances of each material in both the circulation and its red blood cells, as well as in a whole-body tissue compartment along with its cells. Exchange between these four compartments occurs by a number of different mechanisms. The hemorrhage model has as its basis a validated model, due to Gyenge et al., of fluid and solute exchange in the whole body of a standard human. Hypothetical but physiologically based features such as glucose and small ion releases along with cell membrane changes are incorporated into the hemorrhage model to describe the system behavior, particularly during larger hemorrhages. Moderate (10%-30% blood volume loss) and large (> 30% blood loss) hemorrhage dynamics are simulated and compared with available data. The model predictions compare well with the available information for both types of hemorrhages and provide a reasonable description of the progression of a large hemorrhage from the compensatory phase through vascular collapse.

  7. Hierarchical calibration and validation of computational fluid dynamics models for solid sorbent-based carbon capture

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

    Lai, Canhai; Xu, Zhijie; Pan, Wenxiao

    2016-01-01

    To quantify the predictive confidence of a solid sorbent-based carbon capture design, a hierarchical validation methodology—consisting of basic unit problems with increasing physical complexity coupled with filtered model-based geometric upscaling has been developed and implemented. This paper describes the computational fluid dynamics (CFD) multi-phase reactive flow simulations and the associated data flows among different unit problems performed within the said hierarchical validation approach. The bench-top experiments used in this calibration and validation effort were carefully designed to follow the desired simple-to-complex unit problem hierarchy, with corresponding data acquisition to support model parameters calibrations at each unit problem level. A Bayesianmore » calibration procedure is employed and the posterior model parameter distributions obtained at one unit-problem level are used as prior distributions for the same parameters in the next-tier simulations. Overall, the results have demonstrated that the multiphase reactive flow models within MFIX can be used to capture the bed pressure, temperature, CO2 capture capacity, and kinetics with quantitative accuracy. The CFD modeling methodology and associated uncertainty quantification techniques presented herein offer a solid framework for estimating the predictive confidence in the virtual scale up of a larger carbon capture device.« less

  8. Computational fluid dynamics modelling in cardiovascular medicine

    PubMed Central

    Morris, Paul D; Narracott, Andrew; von Tengg-Kobligk, Hendrik; Silva Soto, Daniel Alejandro; Hsiao, Sarah; Lungu, Angela; Evans, Paul; Bressloff, Neil W; Lawford, Patricia V; Hose, D Rodney; Gunn, Julian P

    2016-01-01

    This paper reviews the methods, benefits and challenges associated with the adoption and translation of computational fluid dynamics (CFD) modelling within cardiovascular medicine. CFD, a specialist area of mathematics and a branch of fluid mechanics, is used routinely in a diverse range of safety-critical engineering systems, which increasingly is being applied to the cardiovascular system. By facilitating rapid, economical, low-risk prototyping, CFD modelling has already revolutionised research and development of devices such as stents, valve prostheses, and ventricular assist devices. Combined with cardiovascular imaging, CFD simulation enables detailed characterisation of complex physiological pressure and flow fields and the computation of metrics which cannot be directly measured, for example, wall shear stress. CFD models are now being translated into clinical tools for physicians to use across the spectrum of coronary, valvular, congenital, myocardial and peripheral vascular diseases. CFD modelling is apposite for minimally-invasive patient assessment. Patient-specific (incorporating data unique to the individual) and multi-scale (combining models of different length- and time-scales) modelling enables individualised risk prediction and virtual treatment planning. This represents a significant departure from traditional dependence upon registry-based, population-averaged data. Model integration is progressively moving towards ‘digital patient’ or ‘virtual physiological human’ representations. When combined with population-scale numerical models, these models have the potential to reduce the cost, time and risk associated with clinical trials. The adoption of CFD modelling signals a new era in cardiovascular medicine. While potentially highly beneficial, a number of academic and commercial groups are addressing the associated methodological, regulatory, education- and service-related challenges. PMID:26512019

  9. Regulation of amniotic fluid volume: mathematical model based on intramembranous transport mechanisms.

    PubMed

    Brace, Robert A; Anderson, Debra F; Cheung, Cecilia Y

    2014-11-15

    Experimentation in late-gestation fetal sheep has suggested that regulation of amniotic fluid (AF) volume occurs primarily by modulating the rate of intramembranous transport of water and solutes across the amnion into underlying fetal blood vessels. In order to gain insight into intramembranous transport mechanisms, we developed a computer model that allows simulation of experimentally measured changes in AF volume and composition over time. The model included fetal urine excretion and lung liquid secretion as inflows into the amniotic compartment plus fetal swallowing and intramembranous absorption as outflows. By using experimental flows and solute concentrations for urine, lung liquid, and swallowed fluid in combination with the passive and active transport mechanisms of the intramembranous pathway, we simulated AF responses to basal conditions, intra-amniotic fluid infusions, fetal intravascular infusions, urine replacement, and tracheoesophageal occlusion. The experimental data are consistent with four intramembranous transport mechanisms acting in concert: 1) an active unidirectional bulk transport of AF with all dissolved solutes out of AF into fetal blood presumably by vesicles; 2) passive bidirectional diffusion of solutes, such as sodium and chloride, between fetal blood and AF; 3) passive bidirectional water movement between AF and fetal blood; and 4) unidirectional transport of lactate into the AF. Further, only unidirectional bulk transport is dynamically regulated. The simulations also identified areas for future study: 1) identifying intramembranous stimulators and inhibitors, 2) determining the semipermeability characteristics of the intramembranous pathway, and 3) characterizing the vesicles that are the primary mediators of intramembranous transport. Copyright © 2014 the American Physiological Society.

  10. Regulation of amniotic fluid volume: mathematical model based on intramembranous transport mechanisms

    PubMed Central

    Anderson, Debra F.; Cheung, Cecilia Y.

    2014-01-01

    Experimentation in late-gestation fetal sheep has suggested that regulation of amniotic fluid (AF) volume occurs primarily by modulating the rate of intramembranous transport of water and solutes across the amnion into underlying fetal blood vessels. In order to gain insight into intramembranous transport mechanisms, we developed a computer model that allows simulation of experimentally measured changes in AF volume and composition over time. The model included fetal urine excretion and lung liquid secretion as inflows into the amniotic compartment plus fetal swallowing and intramembranous absorption as outflows. By using experimental flows and solute concentrations for urine, lung liquid, and swallowed fluid in combination with the passive and active transport mechanisms of the intramembranous pathway, we simulated AF responses to basal conditions, intra-amniotic fluid infusions, fetal intravascular infusions, urine replacement, and tracheoesophageal occlusion. The experimental data are consistent with four intramembranous transport mechanisms acting in concert: 1) an active unidirectional bulk transport of AF with all dissolved solutes out of AF into fetal blood presumably by vesicles; 2) passive bidirectional diffusion of solutes, such as sodium and chloride, between fetal blood and AF; 3) passive bidirectional water movement between AF and fetal blood; and 4) unidirectional transport of lactate into the AF. Further, only unidirectional bulk transport is dynamically regulated. The simulations also identified areas for future study: 1) identifying intramembranous stimulators and inhibitors, 2) determining the semipermeability characteristics of the intramembranous pathway, and 3) characterizing the vesicles that are the primary mediators of intramembranous transport. PMID:25186112

  11. Network-Theoretic Modeling of Fluid Flow

    DTIC Science & Technology

    2015-07-29

    Final Report STIR: Network-Theoretic Modeling of Fluid Flow ARO Grant W911NF-14-1-0386 Program manager: Dr. Samuel Stanton ( August 1, 2014–April 30...Morzyński, M., and Comte , P., “A finite-time thermodynamics of unsteady fluid flows,” Journal of Non-Equilibrium Thermody- namics, Vol. 33, No. 2

  12. Computational fluid dynamics investigation of turbulence models for non-newtonian fluid flow in anaerobic digesters.

    PubMed

    Wu, Binxin

    2010-12-01

    In this paper, 12 turbulence models for single-phase non-newtonian fluid flow in a pipe are evaluated by comparing the frictional pressure drops obtained from computational fluid dynamics (CFD) with those from three friction factor correlations. The turbulence models studied are (1) three high-Reynolds-number k-ε models, (2) six low-Reynolds-number k-ε models, (3) two k-ω models, and (4) the Reynolds stress model. The simulation results indicate that the Chang-Hsieh-Chen version of the low-Reynolds-number k-ε model performs better than the other models in predicting the frictional pressure drops while the standard k-ω model has an acceptable accuracy and a low computing cost. In the model applications, CFD simulation of mixing in a full-scale anaerobic digester with pumped circulation is performed to propose an improvement in the effective mixing standards recommended by the U.S. EPA based on the effect of rheology on the flow fields. Characterization of the velocity gradient is conducted to quantify the growth or breakage of an assumed floc size. Placement of two discharge nozzles in the digester is analyzed to show that spacing two nozzles 180° apart with each one discharging at an angle of 45° off the wall is the most efficient. Moreover, the similarity rules of geometry and mixing energy are checked for scaling up the digester.

  13. Biomechanically based simulation of brain deformations for intraoperative image correction: coupling of elastic and fluid models

    NASA Astrophysics Data System (ADS)

    Hagemann, Alexander; Rohr, Karl; Stiehl, H. Siegfried

    2000-06-01

    In order to improve the accuracy of image-guided neurosurgery, different biomechanical models have been developed to correct preoperative images w.r.t. intraoperative changes like brain shift or tumor resection. All existing biomechanical models simulate different anatomical structures by using either appropriate boundary conditions or by spatially varying material parameter values, while assuming the same physical model for all anatomical structures. In general, this leads to physically implausible results, especially in the case of adjacent elastic and fluid structures. Therefore, we propose a new approach which allows to couple different physical models. In our case, we simulate rigid, elastic, and fluid regions by using the appropriate physical description for each material, namely either the Navier equation or the Stokes equation. To solve the resulting differential equations, we derive a linear matrix system for each region by applying the finite element method (FEM). Thereafter, the linear matrix systems are linked together, ending up with one overall linear matrix system. Our approach has been tested using synthetic as well as tomographic images. It turns out from experiments, that the integrated treatment of rigid, elastic, and fluid regions significantly improves the prediction results in comparison to a pure linear elastic model.

  14. Fluid casting of particle-based articles

    DOEpatents

    Menchhofer, Paul

    1995-01-01

    A method for the production of articles made of a particle-based material; e.g., ceramics and sintered metals. In accordance with one aspect of the invention, a thermally settable slurry containing a relatively high concentration of the particles is introduced into an immiscible, heated fluid. The slurry sets or hardens into a shape determined by the physical characteristics of the fluid and the manner of introduction of the slurry into the fluid. For example, the slurry is pulse injected into the fluid to provide spherical articles. The hardened spheres may then be sintered to consolidate the particles and provide a high density product.

  15. Fluid casting of particle-based articles

    DOEpatents

    Menchhofer, P.

    1995-03-28

    A method is disclosed for the production of articles made of a particle-based material; e.g., ceramics and sintered metals. In accordance with one aspect of the invention, a thermally settable slurry containing a relatively high concentration of the particles is introduced into an immiscible, heated fluid. The slurry sets hardens into a shape determined by the physical characteristics of the fluid and the manner of introduction of the slurry into the fluid. For example, the slurry is pulse injected into the fluid to provide spherical articles. The hardened spheres may then be sintered to consolidate the particles and provide a high density product. 1 figure.

  16. Numerical modeling of fluid migration in subduction zones

    NASA Astrophysics Data System (ADS)

    Walter, Marius J.; Quinteros, Javier; Sobolev, Stephan V.

    2015-04-01

    It is well known that fluids play a crucial role in subduction evolution. For example, excess mechanical weakening along tectonic interfaces, due to excess fluid pressure, may enable oceanic subduction. Hence, the fluid content seems to be a critical parameter for subduction initiation. Studies have also shown a correlation between the location of slab dehydration and intermediate seismic activity. Furthermore, expelled fluids from the subduction slab affect the melting temperature, consequently, contributing to partial melting in the wedge above the downgoing plate, and resulting in chemical changes in earth interior and extensive volcanism. In summary, fluids have a great impact on tectonic processes and therefore should be incorporated into geodynamic numerical models. Here we use existing approaches to couple and solve fluid flow equations in the SLIM-3D thermo-mechanical code. SLIM-3D is a three-dimensional thermo-mechanical code capable of simulating lithospheric deformation with elasto-visco-plastic rheology. It incorporates an arbitrary Lagrangian Eulerian formulation, free surface, and changes in density and viscosity, due to endothermic and exothermic phase transitions. It has been successfully applied to model geodynamic processes at different tectonic settings, including subduction zones. However, although SLIM-3D already includes many features, fluid migration has not been incorporated into the model yet. To this end, we coupled solid and fluid flow assuming that fluids flow through a porous and deformable solid. Thereby, we introduce a two-phase flow into the model, in which the Stokes flow is coupled with the Darcy law for fluid flow. This system of equations becomes, however, nonlinear, because the rheology and permeability are depended on the porosity (fluid fraction of the matrix). Ultimately, the evolution of porosity is governed by the compaction pressure and the advection of the porous solid. We show the details of our implementation of the

  17. Modeling of Fluid-Membrane Interaction in Cellular Microinjection Process

    NASA Astrophysics Data System (ADS)

    Karzar-Jeddi, Mehdi; Diaz, Jhon; Olgac, Nejat; Fan, Tai-Hsi

    2009-11-01

    Cellular microinjection is a well-accepted method to deliver matters such as sperm, nucleus, or macromolecules into biological cells. To improve the success rate of in vitro fertilization and to establish the ideal operating conditions for a novel computer controlled rotationally oscillating intracytoplasmic sperm injection (ICSI) technology, we investigate the fluid-membrane interactions in the ICSI procedure. The procedure consists of anchoring the oocyte (a developing egg) using a holding pipette, penetrating oocyte's zona pellucida (the outer membrane) and the oolemma (the plasma or inner membrane) using an injection micropipette, and finally to deliver sperm into the oocyte for fertilization. To predict the large deformation of the oocyte membranes up to the piercing of the oolemma and the motion of fluids across both membranes, the dynamic fluid-pipette-membrane interactions are formulated by the coupled Stokes' equations and the continuum membrane model based on Helfrich's energy theory. A boundary integral model is developed to simulate the transient membrane deformation and the local membrane stress induced by the longitudinal motion of the injection pipette. The model captures the essential features of the membranes shown on optical images of ICSI experiments, and is capable of suggesting the optimal deformation level of the oolemma to start the rotational oscillations for piercing into the oolemma.

  18. Modeling of Complex Coupled Fluid-Structure Interaction Systems in Arbitrary Water Depth

    DTIC Science & Technology

    2008-01-01

    model in a particle finite element method ( PFEM ) based framework for the ALE-RANS solver and submitted a journal paper recently [1]. In the paper, we...developing a fluid-flexible structure interaction model without free surface using ALE-RANS and k-ε turbulence closure model implemented by PFEM . In...the ALE_RANS and k-ε turbulence closure model based on the particle finite element Method ( PFEM ) and obtained some satisfying results [1-2]. The

  19. Methods for simulation-based analysis of fluid-structure interaction.

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

    Barone, Matthew Franklin; Payne, Jeffrey L.

    2005-10-01

    Methods for analysis of fluid-structure interaction using high fidelity simulations are critically reviewed. First, a literature review of modern numerical techniques for simulation of aeroelastic phenomena is presented. The review focuses on methods contained within the arbitrary Lagrangian-Eulerian (ALE) framework for coupling computational fluid dynamics codes to computational structural mechanics codes. The review treats mesh movement algorithms, the role of the geometric conservation law, time advancement schemes, wetted surface interface strategies, and some representative applications. The complexity and computational expense of coupled Navier-Stokes/structural dynamics simulations points to the need for reduced order modeling to facilitate parametric analysis. The proper orthogonalmore » decomposition (POD)/Galerkin projection approach for building a reduced order model (ROM) is presented, along with ideas for extension of the methodology to allow construction of ROMs based on data generated from ALE simulations.« less

  20. Collisional transport across the magnetic field in drift-fluid models

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

    Madsen, J., E-mail: jmad@fysik.dtu.dk; Naulin, V.; Nielsen, A. H.

    2016-03-15

    Drift ordered fluid models are widely applied in studies of low-frequency turbulence in the edge and scrape-off layer regions of magnetically confined plasmas. Here, we show how collisional transport across the magnetic field is self-consistently incorporated into drift-fluid models without altering the drift-fluid energy integral. We demonstrate that the inclusion of collisional transport in drift-fluid models gives rise to diffusion of particle density, momentum, and pressures in drift-fluid turbulence models and, thereby, obviates the customary use of artificial diffusion in turbulence simulations. We further derive a computationally efficient, two-dimensional model, which can be time integrated for several turbulence de-correlation timesmore » using only limited computational resources. The model describes interchange turbulence in a two-dimensional plane perpendicular to the magnetic field located at the outboard midplane of a tokamak. The model domain has two regions modeling open and closed field lines. The model employs a computational expedient model for collisional transport. Numerical simulations show good agreement between the full and the simplified model for collisional transport.« less

  1. The fluid events model: Predicting continuous task action change.

    PubMed

    Radvansky, Gabriel A; D'Mello, Sidney; Abbott, Robert G; Morgan, Brent; Fike, Karl; Tamplin, Andrea K

    2015-01-01

    The fluid events model is a behavioural model aimed at predicting the likelihood that people will change their actions in ongoing, interactive events. From this view, not only are people responding to aspects of the environment, but they are also basing responses on prior experiences. The fluid events model is an attempt to predict the likelihood that people will shift the type of actions taken within an event on a trial-by-trial basis, taking into account both event structure and experience-based factors. The event-structure factors are: (a) changes in event structure, (b) suitability of the current action to the event, and (c) time on task. The experience-based factors are: (a) whether a person has recently shifted actions, (b) how often a person has shifted actions, (c) whether there has been a dip in performance, and (d) a person's propensity to switch actions within the current task. The model was assessed using data from a series of tasks in which a person was producing responses to events. These were two stimulus-driven figure-drawing studies, a conceptually driven decision-making study, and a probability matching study using a standard laboratory task. This analysis predicted trial-by-trial action switching in a person-independent manner with an average accuracy of 70%, which reflects a 34% improvement above chance. In addition, correlations between overall switch rates and actual switch rates were remarkably high (mean r = .98). The experience-based factors played a more major role than the event-structure factors, but this might be attributable to the nature of the tasks.

  2. State-of-the-art review of computational fluid dynamics modeling for fluid-solids systems

    NASA Astrophysics Data System (ADS)

    Lyczkowski, R. W.; Bouillard, J. X.; Ding, J.; Chang, S. L.; Burge, S. W.

    1994-05-01

    As the result of 15 years of research (50 staff years of effort) Argonne National Laboratory (ANL), through its involvement in fluidized-bed combustion, magnetohydrodynamics, and a variety of environmental programs, has produced extensive computational fluid dynamics (CFD) software and models to predict the multiphase hydrodynamic and reactive behavior of fluid-solids motions and interactions in complex fluidized-bed reactors (FBR's) and slurry systems. This has resulted in the FLUFIX, IRF, and SLUFIX computer programs. These programs are based on fluid-solids hydrodynamic models and can predict information important to the designer of atmospheric or pressurized bubbling and circulating FBR, fluid catalytic cracking (FCC) and slurry units to guarantee optimum efficiency with minimum release of pollutants into the environment. This latter issue will become of paramount importance with the enactment of the Clean Air Act Amendment (CAAA) of 1995. Solids motion is also the key to understanding erosion processes. Erosion rates in FBR's and pneumatic and slurry components are computed by ANL's EROSION code to predict the potential metal wastage of FBR walls, intervals, feed distributors, and cyclones. Only the FLUFIX and IRF codes will be reviewed in the paper together with highlights of the validations because of length limitations. It is envisioned that one day, these codes with user-friendly pre- and post-processor software and tailored for massively parallel multiprocessor shared memory computational platforms will be used by industry and researchers to assist in reducing and/or eliminating the environmental and economic barriers which limit full consideration of coal, shale, and biomass as energy sources; to retain energy security; and to remediate waste and ecological problems.

  3. Comparing fluid mechanics models with experimental data.

    PubMed Central

    Spedding, G R

    2003-01-01

    The art of modelling the physical world lies in the appropriate simplification and abstraction of the complete problem. In fluid mechanics, the Navier-Stokes equations provide a model that is valid under most circumstances germane to animal locomotion, but the complexity of solutions provides strong incentive for the development of further, more simplified practical models. When the flow organizes itself so that all shearing motions are collected into localized patches, then various mathematical vortex models have been very successful in predicting and furthering the physical understanding of many flows, particularly in aerodynamics. Experimental models have the significant added convenience that the fluid mechanics can be generated by a real fluid, not a model, provided the appropriate dimensionless groups have similar values. Then, analogous problems can be encountered in making intelligible but independent descriptions of the experimental results. Finally, model predictions and experimental results may be compared if, and only if, numerical estimates of the likely variations in the tested quantities are provided. Examples from recent experimental measurements of wakes behind a fixed wing and behind a bird in free flight are used to illustrate these principles. PMID:14561348

  4. A watershed model of individual differences in fluid intelligence.

    PubMed

    Kievit, Rogier A; Davis, Simon W; Griffiths, John; Correia, Marta M; Cam-Can; Henson, Richard N

    2016-10-01

    Fluid intelligence is a crucial cognitive ability that predicts key life outcomes across the lifespan. Strong empirical links exist between fluid intelligence and processing speed on the one hand, and white matter integrity and processing speed on the other. We propose a watershed model that integrates these three explanatory levels in a principled manner in a single statistical model, with processing speed and white matter figuring as intermediate endophenotypes. We fit this model in a large (N=555) adult lifespan cohort from the Cambridge Centre for Ageing and Neuroscience (Cam-CAN) using multiple measures of processing speed, white matter health and fluid intelligence. The model fit the data well, outperforming competing models and providing evidence for a many-to-one mapping between white matter integrity, processing speed and fluid intelligence. The model can be naturally extended to integrate other cognitive domains, endophenotypes and genotypes. Copyright © 2016 The Authors. Published by Elsevier Ltd.. All rights reserved.

  5. Two-fluid models of turbulence

    NASA Technical Reports Server (NTRS)

    Spalding, D. B.

    1985-01-01

    The defects of turbulence models are summarized and the importance of so-called nongradient diffusion in turbulent fluxes is discussed. The mathematical theory of the flow of two interpenetrating continua is reviewed, and the mathematical formulation of the two fluid model is outlined. Results from plane wake, axisymmetric jet, and combustion studies are shown.

  6. Modeling and control of magnetorheological fluid dampers using neural networks

    NASA Astrophysics Data System (ADS)

    Wang, D. H.; Liao, W. H.

    2005-02-01

    Due to the inherent nonlinear nature of magnetorheological (MR) fluid dampers, one of the challenging aspects for utilizing these devices to achieve high system performance is the development of accurate models and control algorithms that can take advantage of their unique characteristics. In this paper, the direct identification and inverse dynamic modeling for MR fluid dampers using feedforward and recurrent neural networks are studied. The trained direct identification neural network model can be used to predict the damping force of the MR fluid damper on line, on the basis of the dynamic responses across the MR fluid damper and the command voltage, and the inverse dynamic neural network model can be used to generate the command voltage according to the desired damping force through supervised learning. The architectures and the learning methods of the dynamic neural network models and inverse neural network models for MR fluid dampers are presented, and some simulation results are discussed. Finally, the trained neural network models are applied to predict and control the damping force of the MR fluid damper. Moreover, validation methods for the neural network models developed are proposed and used to evaluate their performance. Validation results with different data sets indicate that the proposed direct identification dynamic model using the recurrent neural network can be used to predict the damping force accurately and the inverse identification dynamic model using the recurrent neural network can act as a damper controller to generate the command voltage when the MR fluid damper is used in a semi-active mode.

  7. A two-fluid model for avalanche and debris flows.

    PubMed

    Pitman, E Bruce; Le, Long

    2005-07-15

    Geophysical mass flows--debris flows, avalanches, landslides--can contain O(10(6)-10(10)) m(3) or more of material, often a mixture of soil and rocks with a significant quantity of interstitial fluid. These flows can be tens of meters in depth and hundreds of meters in length. The range of scales and the rheology of this mixture presents significant modelling and computational challenges. This paper describes a depth-averaged 'thin layer' model of geophysical mass flows containing a mixture of solid material and fluid. The model is derived from a 'two-phase' or 'two-fluid' system of equations commonly used in engineering research. Phenomenological modelling and depth averaging combine to yield a tractable set of equations, a hyperbolic system that describes the motion of the two constituent phases. If the fluid inertia is small, a reduced model system that is easier to solve may be derived.

  8. Transport of fluid and solutes in the body I. Formulation of a mathematical model.

    PubMed

    Gyenge, C C; Bowen, B D; Reed, R K; Bert, J L

    1999-09-01

    A compartmental model of short-term whole body fluid, protein, and ion distribution and transport is formulated. The model comprises four compartments: a vascular and an interstitial compartment, each with an embedded cellular compartment. The present paper discusses the assumptions on which the model is based and describes the equations that make up the model. Fluid and protein transport parameters from a previously validated model as well as ionic exchange parameters from the literature or from statistical estimation [see companion paper: C. C. Gyenge, B. D. Bowen, R. K. Reed, and J. L. Bert. Am. J. Physiol. 277 (Heart Circ. Physiol. 46): H1228-H1240, 1999] are used in formulating the model. The dynamic model has the ability to simulate 1) transport across the capillary membrane of fluid, proteins, and small ions and their distribution between the vascular and interstitial compartments; 2) the changes in extracellular osmolarity; 3) the distribution and transport of water and ions associated with each of the cellular compartments; 4) the cellular transmembrane potential; and 5) the changes of volume in the four fluid compartments. The validation and testing of the proposed model against available experimental data are presented in the companion paper.

  9. Stability of stationary solutions for inflow problem on the micropolar fluid model

    NASA Astrophysics Data System (ADS)

    Yin, Haiyan

    2017-04-01

    In this paper, we study the asymptotic behavior of solutions to the initial boundary value problem for the micropolar fluid model in a half-line R+:=(0,∞). We prove that the corresponding stationary solutions of the small amplitude to the inflow problem for the micropolar fluid model are time asymptotically stable under small H1 perturbations in both the subsonic and degenerate cases. The microrotation velocity brings us some additional troubles compared with Navier-Stokes equations in the absence of the microrotation velocity. The proof of asymptotic stability is based on the basic energy method.

  10. Numerical Modeling of Conjugate Heat Transfer in Fluid Network

    NASA Technical Reports Server (NTRS)

    Majumdar, Alok

    2004-01-01

    Fluid network modeling with conjugate heat transfer has many applications in Aerospace engineering. In modeling unsteady flow with heat transfer, it is important to know the variation of wall temperature in time and space to calculate heat transfer between solid to fluid. Since wall temperature is a function of flow, a coupled analysis of temperature of solid and fluid is necessary. In cryogenic applications, modeling of conjugate heat transfer is of great importance to correctly predict boil-off rate in propellant tanks and chill down of transfer lines. In TFAWS 2003, the present author delivered a paper to describe a general-purpose computer program, GFSSP (Generalized Fluid System Simulation Program). GFSSP calculates flow distribution in complex flow circuit for compressible/incompressible, with or without heat transfer or phase change in all real fluids or mixtures. The flow circuit constitutes of fluid nodes and branches. The mass, energy and specie conservation equations are solved at the nodes where as momentum conservation equations are solved at the branches. The proposed paper describes the extension of GFSSP to model conjugate heat transfer. The network also includes solid nodes and conductors in addition to fluid nodes and branches. The energy conservation equations for solid nodes solves to determine the temperatures of the solid nodes simultaneously with all conservation equations governing fluid flow. The numerical scheme accounts for conduction, convection and radiation heat transfer. The paper will also describe the applications of the code to predict chill down of cryogenic transfer line and boil-off rate of cryogenic propellant storage tank.

  11. A double medium model for diffusion in fluid-bearing rock

    NASA Astrophysics Data System (ADS)

    Wang, H. F.

    1993-09-01

    The concept of a double porosity medium to model fluid flow in fractured rock has been applied to model diffusion in rock containing a small amount of a continuous fluid phase that surrounds small volume elements of the solid matrix. The model quantifies the relative role of diffusion in the fluid and solid phases of the rock. The fluid is the fast diffusion path, but the solid contains the volumetrically significant amount of the diffusing species. The double medium model consists of two coupled differential equations. One equation is the diffusion equation for the fluid concentration; it contains a source term for change in the average concentration of the diffusing species in the solid matrix. The second equation represents the assumption that the change in average concentration in a solid element is proportional to the difference between the average concentration in the solid and the concentration in the fluid times the solid-fluid partition coefficient. The double medium model is shown to apply to laboratory data on iron diffusion in fluid-bearing dunite and to measured oxygen isotope ratios at marble-metagranite contacts. In both examples, concentration profiles are calculated for diffusion taking place at constant temperature, where a boundary value changes suddenly and is subsequently held constant. Knowledge of solid diffusivities can set a lower bound to the length of time over which diffusion occurs, but only the product of effective fluid diffusivity and time is constrained for times longer than the characteristic solid diffusion time. The double medium results approach a local, grain-scale equilibrium model for times that are large relative to the time constant for solid diffusion.

  12. Modeling mechanical properties of a shear thickening fluid damper based on phase transition theory

    NASA Astrophysics Data System (ADS)

    Wei, Minghai; Lin, Kun; Guo, Qian

    2018-03-01

    Shear thickening fluids (STFs) are highly concentrated colloidal suspensions consisting of monodisperse nano-particles suspended in a carrying fluid, and have the capacity to display both flowable and rigid behaviors, when subjected to sudden stimuli. In that process, the external energy that acts on an STF can be dissipated quickly. The aim of this study is to present a dynamic model of a damper filled with STF that can be directly used in control engineering fields. To this end, shear stress during phase transition of the STF material is chosen as an internal variable. A non-convex function with bifurcation behavior is used to describe the phase transitioning of STF by determining the relationship between the behavioral characteristics of the microscopic phase and macroscopic damping force. This model is able to predict force-velocity and force-displacement relationships as functions of the loading frequency. Efficacy of the model is demonstrated via comparison with experimental results from previous studies. In addition, the results confirm the hypothesis regarding the occurrence of STF phase transitioning when subject to shear stress.

  13. Refining the Subseafloor Circulation Model of the Middle Valley Hydrothermal System Using Fluid Geochemistry

    NASA Astrophysics Data System (ADS)

    Inderbitzen, K. E.; Wheat, C. G.; Baker, P. A.; Fisher, A. T.

    2014-12-01

    Currently, fluid circulation patterns and the evolution of rock/fluid compositions as circulation occurs in subseafloor hydrothermal systems are poorly constrained. Sedimented spreading centers provide a unique opportunity to study subsurface flow because sediment acts as an insulating blanket that traps heat from the cooling magma body and limits: (a) potential flow paths for seawater to recharge the aquifer in permeable upper basaltic basement and (b) points of altered fluid egress. This also allows for a range of thermal and geochemical gradients to exist near the sediment-water interface. Models of fluid circulation patterns in this type of hydrologic setting have been generated (eg. Stein and Fisher, 2001); however fluid chemistry datasets have not previously been used to test the model's viability. We address this issue by integrating the existing circulation model with fluid compositional data collected from sediment pore waters and high temperature hydrothermal vents located in Middle Valley on the Juan de Fuca Ridge. Middle Valley hosts a variety of hydrologic regimes: including areas of fluid recharge (Site 855), active venting (Site 858/1036; Dead Dog vent field), recent venting (Site 856/1035; Bent Hill Massive Sulfide deposit) and a section of heavily sedimented basement located between recharge and discharge sites (Site 857). We will present new results based on thermal and geochemical data from the area of active venting (Sites 858 and 1036), that was collected during Ocean Drilling Program Legs 139 and 169 and a subsequent heat flow/gravity coring effort. These results illuminate fine scale controls on secondary recharge and fluid flow within the sediment section at Site 858/1036. The current status of high temperature vents in this area (based on observations made in July, 2014) will also be outlined.

  14. Computational fluid dynamics modelling in cardiovascular medicine.

    PubMed

    Morris, Paul D; Narracott, Andrew; von Tengg-Kobligk, Hendrik; Silva Soto, Daniel Alejandro; Hsiao, Sarah; Lungu, Angela; Evans, Paul; Bressloff, Neil W; Lawford, Patricia V; Hose, D Rodney; Gunn, Julian P

    2016-01-01

    This paper reviews the methods, benefits and challenges associated with the adoption and translation of computational fluid dynamics (CFD) modelling within cardiovascular medicine. CFD, a specialist area of mathematics and a branch of fluid mechanics, is used routinely in a diverse range of safety-critical engineering systems, which increasingly is being applied to the cardiovascular system. By facilitating rapid, economical, low-risk prototyping, CFD modelling has already revolutionised research and development of devices such as stents, valve prostheses, and ventricular assist devices. Combined with cardiovascular imaging, CFD simulation enables detailed characterisation of complex physiological pressure and flow fields and the computation of metrics which cannot be directly measured, for example, wall shear stress. CFD models are now being translated into clinical tools for physicians to use across the spectrum of coronary, valvular, congenital, myocardial and peripheral vascular diseases. CFD modelling is apposite for minimally-invasive patient assessment. Patient-specific (incorporating data unique to the individual) and multi-scale (combining models of different length- and time-scales) modelling enables individualised risk prediction and virtual treatment planning. This represents a significant departure from traditional dependence upon registry-based, population-averaged data. Model integration is progressively moving towards 'digital patient' or 'virtual physiological human' representations. When combined with population-scale numerical models, these models have the potential to reduce the cost, time and risk associated with clinical trials. The adoption of CFD modelling signals a new era in cardiovascular medicine. While potentially highly beneficial, a number of academic and commercial groups are addressing the associated methodological, regulatory, education- and service-related challenges. Published by the BMJ Publishing Group Limited. For permission

  15. Rock deformation models and fluid leak-off in hydraulic fracturing

    NASA Astrophysics Data System (ADS)

    Yarushina, Viktoriya M.; Bercovici, David; Oristaglio, Michael L.

    2013-09-01

    Fluid loss into reservoir rocks during hydraulic fracturing is modelled via a poro-elastoplastic pressure diffusion equation in which the total compressibility is a sum of fluid, rock and pore space compressibilities. Inclusion of pore compressibility and porosity-dependent permeability in the model leads to a strong pressure dependence of leak-off (i.e. drainage rate). Dilation of the matrix due to fluid invasion causes higher rates of fluid leak-off. The present model is appropriate for naturally fractured and tight gas reservoirs as well as for soft and poorly consolidated formations whose mechanical behaviour departs from simple elastic laws. Enhancement of the leak-off coefficient by dilation, predicted by the new model, may help explain the low percentage recovery of fracturing fluid (usually between 5 and 50 per cent) in shale gas stimulation by hydraulic fracturing.

  16. Classical analogous of quantum cosmological perfect fluid models

    NASA Astrophysics Data System (ADS)

    Batista, A. B.; Fabris, J. C.; Gonçalves, S. V. B.; Tossa, J.

    2001-05-01

    Quantization in the minisuperspace of a gravity system coupled to a perfect fluid, leads to a solvable model which implies singularity free solutions through the construction of a superposition of the wavefunctions. We show that such models are equivalent to a classical system where, besides the perfect fluid, a repulsive fluid with an equation of state pQ= ρQ is present. This leads to speculate on the true nature of this quantization procedure. A perturbative analysis of the classical system reveals the condition for the stability of the classical system in terms of the existence of an anti-gravity phase.

  17. Improving students’ conceptions on fluid dynamics through peer teaching model with PDEODE (PTM-PDEODE)

    NASA Astrophysics Data System (ADS)

    Samsudin, A.; Fratiwi, N.; Amin, N.; Wiendartun; Supriyatman; Wibowo, F.; Faizin, M.; Costu, B.

    2018-05-01

    This study based on an importance of improving students’ conceptions and reduces students’ misconceptions on fluid dynamics concepts. Consequently, should be done the study through combining Peer Teaching Model (PTM) and PDEODE (Prediction, Discuss, Explain, Observe, Discuss and Explain) learning strategy (PTM-PDEODE). For the research methods, we used the 4D model (Defining, Designing, Developing, and Disseminating). The samples are 38 students (their ages were an average of 17 years-old) at one of the senior high schools in Bandung. The improvement of students’ conceptions was diagnosed through a four-tier test of fluid dynamics. At the disseminating phase, students’ conceptions of fluid dynamics concepts are increase after the use of PTM-PDEODE. In conclusion, the development of PTM-PDEODE is respectable enough to improve students’ conceptions on dinamics fluid.

  18. Comparison of fluid neutral models for one-dimensional plasma edge modeling with a finite volume solution of the Boltzmann equation

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

    Horsten, N., E-mail: niels.horsten@kuleuven.be; Baelmans, M.; Dekeyser, W.

    2016-01-15

    We derive fluid neutral approximations for a simplified 1D edge plasma model, suitable to study the neutral behavior close to the target of a nuclear fusion divertor, and compare its solutions to the solution of the corresponding kinetic Boltzmann equation. The plasma is considered as a fixed background extracted from a detached 2D simulation. We show that the Maxwellian equilibrium distribution is already obtained very close to the target, justifying the use of a fluid approximation. We compare three fluid neutral models: (i) a diffusion model; (ii) a pressure-diffusion model (i.e., a combination of a continuity and momentum equation) assumingmore » equal neutral and ion temperatures; and (iii) the pressure-diffusion model coupled to a neutral energy equation taking into account temperature differences between neutrals and ions. Partial reflection of neutrals reaching the boundaries is included in both the kinetic and fluid models. We propose two methods to obtain an incident neutral flux boundary condition for the fluid models: one based on a diffusion approximation and the other assuming a truncated Chapman-Enskog distribution. The pressure-diffusion model predicts the plasma sources very well. The diffusion boundary condition gives slightly better results overall. Although including an energy equation still improves the results, the assumption of equal ion and neutral temperature already gives a very good approximation.« less

  19. A Fluid-driven Earthquake Cycle, Omori's Law, and Fluid-driven Aftershocks

    NASA Astrophysics Data System (ADS)

    Miller, S. A.

    2015-12-01

    Few models exist that predict the Omori's Law of aftershock rate decay, with rate-state friction the only physically-based model. ETAS is a probabilistic model of cascading failures, and is sometimes used to infer rate-state frictional properties. However, the (perhaps dominant) role of fluids in the earthquake process is being increasingly realised, so a fluid-based physical model for Omori's Law should be available. In this talk, I present an hypothesis for a fluid-driven earthquake cycle where dehydration and decarbonization at depth provides continuous sources of buoyant high pressure fluids that must eventually make their way back to the surface. The natural pathway for fluid escape is along plate boundaries, where in the ductile regime high pressure fluids likely play an integral role in episodic tremor and slow slip earthquakes. At shallower levels, high pressure fluids pool at the base of seismogenic zones, with the reservoir expanding in scale through the earthquake cycle. Late in the cycle, these fluids can invade and degrade the strength of the brittle crust and contribute to earthquake nucleation. The mainshock opens permeable networks that provide escape pathways for high pressure fluids and generate aftershocks along these flow paths, while creating new pathways by the aftershocks themselves. Thermally activated precipitation then seals up these pathways, returning the system to a low-permeability environment and effective seal during the subsequent tectonic stress buildup. I find that the multiplicative effect of an exponential dependence of permeability on the effective normal stress coupled with an Arrhenius-type, thermally activated exponential reduction in permeability results in Omori's Law. I simulate this scenario using a very simple model that combines non-linear diffusion and a step-wise increase in permeability when a Mohr Coulomb failure condition is met, and allow permeability to decrease as an exponential function in time. I show very

  20. Three-dimensional vortex-induced vibrations of supported pipes conveying fluid based on wake oscillator models

    NASA Astrophysics Data System (ADS)

    Wang, L.; Jiang, T. L.; Dai, H. L.; Ni, Q.

    2018-05-01

    The present study develops a new three-dimensional nonlinear model for investigating vortex-induced vibrations (VIV) of flexible pipes conveying internal fluid flow. The unsteady hydrodynamic forces associated with the wake dynamics are modeled by two distributed van der Pol wake oscillators. In particular, the nonlinear partial differential equations of motion of the pipe and the wake are derived, taking into account the coupling between the structure and the fluid. The nonlinear equations of motion for the coupled system are then discretized by means of the Galerkin technique, resulting in a high-dimensional reduced-order model of the system. It is shown that the natural frequencies for in-plane and out-of-plane motions of the pipe may be different at high internal flow velocities beyond the threshold of buckling instability. The orientation angle of the postbuckling configuration is time-varying due to the disturbance of hydrodynamic forces, thus yielding sometimes unexpected results. For a buckled pipe with relatively low cross-flow velocity, interestingly, examining the nonlinear dynamics of the pipe indicates that the combined effects of the cross-flow-induced resonance of the in-plane first mode and the internal-flow-induced buckling on the IL and CF oscillation amplitudes may be significant. For higher cross-flow velocities, however, the effect of internal fluid flow on the nonlinear VIV responses of the pipe is not pronounced.

  1. Hydromechanical Modeling of Fluid Flow in the Lower Crust

    NASA Astrophysics Data System (ADS)

    Connolly, J.

    2011-12-01

    The lower crust lies within an ambiguous rheological regime between the brittle upper crust and ductile sub-lithospheric mantle. This ambiguity has allowed two schools of thought to develop concerning the nature of fluid flow in the lower crust. The classical school holds that lower crustal rocks are inviscid and that any fluid generated by metamorphic devolatilization is squeezed out of rocks as rapidly as it is produced. According to this school, permeability is a dynamic property and fluid flow is upward. In contrast, the modern school uses concepts from upper crustal hydrology that presume implicitly, if not explicitly, that rocks are rigid or, at most, brittle. For the modern school, the details of crustal permeability determine fluid flow and as these details are poorly known almost anything is possible. Reality, to the extent that it is reflected by inference from field studies, offers some support to both schools. In particular, evidence of significant lateral and channelized fluid flow are consistent with flow in rigid media, while evidence for short (104 - 105 y) grain-scale fluid-rock interaction during much longer metamorphic events, suggests that reaction-generated grain-scale permeability is sealed rapidly by compaction; a phenomenon that is also essential to prevent extensive retrograde metamorphism. These observations provide a compelling argument for recognizing in conceptual models of lower crustal fluid flow that rocks are neither inviscid nor rigid, but compact by viscous mechanisms on a finite time-scale. This presentation will review the principle consequences of, and obstacles to, incorporating compaction in such models. The role of viscous compaction in the lower crust is extraordinarily uncertain, but ignoring this uncertainty in models of lower crustal fluid flow does not make the models any more certain. Models inevitably invoke an initial steady state hydraulic regime. This initial steady state is critical to model outcomes because it

  2. GEOSIM: A numerical model for geophysical fluid flow simulation

    NASA Technical Reports Server (NTRS)

    Butler, Karen A.; Miller, Timothy L.; Lu, Huei-Iin

    1991-01-01

    A numerical model which simulates geophysical fluid flow in a wide range of problems is described in detail, and comparisons of some of the model's results are made with previous experimental and numerical studies. The model is based upon the Boussinesq Navier-Stokes equations in spherical coordinates, which can be reduced to a cylindrical system when latitudinal walls are used near the pole and the ratio of latitudinal length to the radius of the sphere is small. The equations are approximated by finite differences in the meridional plane and spectral decomposition in the azimuthal direction. The user can specify a variety of boundary and initial conditions, and there are five different spectral truncation options. The results of five validation cases are presented: (1) the transition between axisymmetric flow and baroclinic wave flow in the side heated annulus; (2) the steady baroclinic wave of the side heated annulus; (3) the wave amplitude vacillation of the side heated annulus; (4) transition to baroclinic wave flow in a bottom heated annulus; and (5) the Spacelab Geophysical Fluid Flow Cell (spherical) experiment.

  3. The Kantowski-Sachs Quantum Model with Stiff Matter Fluid

    NASA Astrophysics Data System (ADS)

    Alvarenga, F. G.; Fracalossi, R.; Freitas, R. C.; Gonçalves, S. V. B.

    2018-05-01

    In this paper, we study the quantum cosmological Kantowski-Sachs model and we solve the Wheeler-DeWitt equation in minisuperspace to obtain the wave function of the corresponding universe. The perfect fluid is described by Schutz's canonical formalism, which allows to attribute dynamical degrees of freedom to matter. The time is introduced phenomenologically using the fluid's degrees of freedom. In particular, we adopt a stiff matter fluid. The viability of this model is analyzed and discussed.

  4. Modeling of magnetorheological fluid in quasi-static squeeze flow mode

    NASA Astrophysics Data System (ADS)

    Horak, Wojciech

    2018-06-01

    This work presents a new nonlinear model to describe MR fluid behavior in the squeeze flow mode. The basis for deriving the model were the principles of continuum mechanics and the theory of tensor transformation. The analyzed case concerned quasi-static squeeze with a constant area, between two parallel plates with non-slip boundary conditions. The developed model takes into account the rheological properties or MR fluids as a viscoplastic material for which yield stress increases due to compression. The model also takes into account the formation of normal force in the MR fluid as a result of the magnetic field impact. Moreover, a new parameter has been introduced which characterizes the behavior of MR fluid subjected to compression. The proposed model has been experimentally validated and the obtained results suggest that the assumptions made in the model development are reasonable, as good model compatibility with the experiments was obtained.

  5. The Blended Finite Element Method for Multi-fluid Plasma Modeling

    DTIC Science & Technology

    2016-07-01

    Briefing Charts 3. DATES COVERED (From - To) 07 June 2016 - 01 July 2016 4. TITLE AND SUBTITLE The Blended Finite Element Method for Multi-fluid Plasma...BLENDED FINITE ELEMENT METHOD FOR MULTI-FLUID PLASMA MODELING Éder M. Sousa1, Uri Shumlak2 1ERC INC., IN-SPACE PROPULSION BRANCH (RQRS) AIR FORCE RESEARCH...MULTI-FLUID PLASMA MODEL 2 BLENDED FINITE ELEMENT METHOD Blended Finite Element Method Nodal Continuous Galerkin Modal Discontinuous Galerkin Model

  6. [Preparation and characterization of a polyvinylpyrrolidone water-based magnetic fluid].

    PubMed

    Xie, Jian-feng; Zhang, Yang-de; Zeng, Zhao-wu; Wang, Xiao-li; Liu, Xing-yan; Zhou, Wei-hua

    2008-03-01

    To prepare a stable water-based magnetic fluid. A water-based magnetic fluid was prepared by addition of polyvinylpyrrolidone (PVP) as the coating agent for the magnetic particles. After preparation of Fe3O4 by co-precipitation method, PVP was added for its coating, followed by ultrasonic agitation and purification. The magnetic nanoparticles of homogeneously small size and water-based magnetic fluid were obtained, which had good dispersion in water with strong magnetism. PVP can be used as a surfactant to stabilize the magnetic fluid.

  7. Modelling fluid accumulation in the neck using simple baseline fluid metrics: implications for sleep apnea.

    PubMed

    Vena, Daniel; Yadollahi, A; Bradley, T Douglas

    2014-01-01

    Obstructive sleep apnea (OSA) is a common respiratory disorder among adults. Recently we have shown that sedentary lifestyle causes an increase in diurnal leg fluid volume (LFV), which can shift into the neck at night when lying down to sleep and increase OSA severity. The purpose of this work was to investigate various metrics that represent baseline fluid retention in the legs and examine their correlation with neck fluid volume (NFV) and to develop a robust model for predicting fluid accumulation in the neck. In 13 healthy awake non-obese men, LFV and NFV were recorded continuously and simultaneously while standing for 5 minutes and then lying supine for 90 minutes. Simple regression was used to examine correlations between baseline LFV, baseline neck circumference (NC) and change in LFV with the outcome variables: change in NC (ΔNC) and in NFV (ΔNFV90) after lying supine for 90 minutes. An exhaustive grid search was implemented to find combinations of input variables which best modeled outcomes. We found strong positive correlations between baseline LFV (supine and standing) and ΔNFV90. Models developed for predicting ΔNFV90 included baseline standing LFV, baseline NC combined with change in LFV after lying supine for 90 minutes. These correlations and the developed models suggest that a greater baseline LFV might contribute to increased fluid accumulation in the neck. These results give more evidence that sedentary lifestyle might play a role in the pathogenesis of OSA by increasing the baseline LFV. The best models for predicting ΔNC include baseline LFV and NC; they improved accuracies of estimating ΔNC over individual predictors, suggesting that a combination of baseline fluid metrics is a good predictor of the change in NC while lying supine. Future work is aimed at adding additional baseline demographic features to improve model accuracy and eventually use it as a screening tool to predict severity of OSA prior to sleep.

  8. One-dimension modeling on the parallel-plate ion extraction process based on a non-electron-equilibrium fluid model

    NASA Astrophysics Data System (ADS)

    Li, He-Ping; Chen, Jian; Guo, Heng; Jiang, Dong-Jun; Zhou, Ming-Sheng; Department of Engineering Physics Team

    2017-10-01

    Ion extraction from a plasma under an externally applied electric field involve multi-particle and multi-field interactions, and has wide applications in the fields of materials processing, etching, chemical analysis, etc. In order to develop the high-efficiency ion extraction methods, it is indispensable to establish a feasible model to understand the non-equilibrium transportation processes of the charged particles and the evolutions of the space charge sheath during the extraction process. Most of the previous studies on the ion extraction process are mainly based on the electron-equilibrium fluid model, which assumed that the electrons are in the thermodynamic equilibrium state. However, it may lead to some confusions with neglecting the electron movement during the sheath formation process. In this study, a non-electron-equilibrium model is established to describe the transportation of the charged particles in a parallel-plate ion extraction process. The numerical results show that the formation of the Child-Langmuir sheath is mainly caused by the charge separation. And thus, the sheath shielding effect will be significantly weakened if the charge separation is suppressed during the extraction process of the charged particles.

  9. Surface tension driven flow in glass melts and model fluids

    NASA Technical Reports Server (NTRS)

    Mcneil, T. J.; Cole, R.; Subramanian, R. S.

    1982-01-01

    Surface tension driven flow has been investigated analytically and experimentally using an apparatus where a free column of molten glass or model fluids was supported at its top and bottom faces by solid surfaces. The glass used in the experiments was sodium diborate, and the model fluids were silicone oils. In both the model fluid and glass melt experiments, conclusive evidence was obtained to prove that the observed flow was driven primarily by surface tension forces. The experimental observations are in qualitative agreement with predictions from the theoretical model.

  10. Mathematical modeling of impact of two metal plates using two-fluid approach

    NASA Astrophysics Data System (ADS)

    Utkin, P. S.; Fortova, S. V.

    2018-01-01

    The paper is devoted to the development of the two-fluid mathematical model and the computational algorithm for the modeling of two metal plates impact. In one-dimensional case the governing system of equations comprises seven equations: three conservation laws for each fluid and transfer equation for the volume fraction of one of the fluids. Both fluids are considered to be compressible and equilibrium on velocities. Pressures equilibrium is used as fluids interface condition. The system has hyperbolic type but could not be written in the conservative form because of nozzling terms in the right-hand side of the equations. The algorithm is based on the Harten-Lax-van Leer numerical flux function. The robust computation in the presence of the interface boundary is carried out due to the special pressure relaxation procedure. The problem is solved using stiffened gas equations of state for each fluid. The parameters in the equations of state are calibrated using the results of computations using wide-range equations of state for the metals. In simulations of metal plates impact we get two shocks after the initial impact that propagate to the free surfaces of the samples. The characteristics of shock waves are close (maximum relative error in characteristics of shocks is not greater than 7%) to the data from the wide-range equations of states computations.

  11. Optimization of decoupling performance of underwater acoustic coating with cavities via equivalent fluid model

    NASA Astrophysics Data System (ADS)

    Huang, Lingzhi; Xiao, Yong; Wen, Jihong; Zhang, Hao; Wen, Xisen

    2018-07-01

    Acoustic coatings with periodically arranged internal cavities have been successfully applied in submarines for the purpose of decoupling water from vibration of underwater structures, and thus reducing underwater sound radiation. Previous publications on decoupling acoustic coatings with cavities are mainly focused on the case of coatings with specific shaped cavities, including cylindrical and conical cavities. To explore better decoupling performance, an optimal design of acoustic coating with complex shaped cavities is attempted in this paper. An equivalent fluid model is proposed to characterize coatings with general axisymmetrical cavities. By employing the equivalent fluid model, an analytical vibroacoustic model is further developed for the prediction of sound radiation from an infinite plate covered with an equivalent fluid layer (as a replacement of original coating) and immersed in water. Numerical examples are provided to verify the equivalent fluid model. Based on a combining use of the analytical vibroacoustic model and a differential evolution algorithm, optimal designs for acoustic coatings with cavities are conducted. Numerical results demonstrate that the decoupling performance of acoustic coating can be significantly improved by employing special axisymmetrical cavities as compared to traditional cylindrical cavities.

  12. Breakdown of single spin-fluid model in the heavily hole-doped superconductor CsFe2As2

    NASA Astrophysics Data System (ADS)

    Zhao, D.; Li, S. J.; Wang, N. Z.; Li, J.; Song, D. W.; Zheng, L. X.; Nie, L. P.; Luo, X. G.; Wu, T.; Chen, X. H.

    2018-01-01

    Although Fe-based superconductors are correlated electronic systems with multiorbital, previous nuclear magnetic resonance (NMR) measurement suggests that a single spin-fluid model is sufficient to describe its spin behavior. Here, we first observed the breakdown of single spin-fluid model in a heavily hole-doped Fe-based superconductor CsFe2As2 by site-selective NMR measurement. At high-temperature regime, both Knight shift and nuclear spin-lattice relaxation at 133Cs and 75As nuclei exhibit distinct temperature-dependent behavior, suggesting the breakdown of the single spin-fluid model in CsFe2As2 . This is ascribed to the coexistence of both localized and itinerant spin degree of freedom at 3 d orbitals, which is consistent with the orbital-selective Mott phase. With decreasing temperature, the single spin-fluid behavior is recovered below T*˜75 K due to a coherent state among 3 d orbitals. The Kondo liquid scenario is proposed to understand the low-temperature coherent state.

  13. Modeling the relaxation dynamics of fluids in nanoporous materials

    NASA Astrophysics Data System (ADS)

    Edison, John R.

    Mesoporous materials are being widely used in the chemical industry in various environmentally friendly separation processes and as catalysts. Our research can be broadly described as an effort to understand the behavior of fluids confined in such materials. More specifically we try to understand the influence of state variables like temperature and pore variables like size, shape, connectivity and structural heterogeneity on both the dynamic and equilibrium behavior of confined fluids. The dynamic processes associated with the approach to equilibrium are largely unexplored. It is important to look into the dynamic behavior for two reasons. First, confined fluids experience enhanced metastabilities and large equilibration times in certain classes of mesoporous materials, and the approach to the metastable/stable equilibrium is of tremendous interest. Secondly, understanding the transport resistances in a microscopic scale will help better engineer heterogeneous catalysts and separation processes. Here we present some of our preliminary studies on dynamics of fluids in ideal pore geometries. The tool that we have used extensively to investigate the relaxation dynamics of fluids in pores is the dynamic mean field theory (DMFT) as developed by Monson [P. A. Monson, J. Chem. Phys., 128, 084701 (2008)]. The theory is based on a lattice gas model of the system and can be viewed as a highly computationally efficient approximation to the dynamics averaged over an ensemble of Kawasaki dynamics Monte Carlo trajectories of the system. It provides a theory of the dynamics of the system consistent with the thermodynamics in mean field theory. The nucleation mechanisms associated with confined fluid phase transitions are emergent features in the calculations. We begin by describing the details of the theory and then present several applications of DMFT. First we present applications to three model pore networks (a) a network of slit pores with a single pore width; (b) a network

  14. Experimental and analytical study on fluid whirl and fluid whip modes

    NASA Technical Reports Server (NTRS)

    Muszynska, Agnes

    1994-01-01

    Fluid whirl and fluid whip are rotor self-excited, lateral vibrations which occur due to rotor interactions with the surrounding fluid. There exist various modes of fluid whirl and fluid whip. These modes are close to rotor modes corresponding to free vibrations (based on the linear model). Small differences are due to nonlinearities in the system. This paper presents experimental and analytical results on the lowest modes of fluid whirls and fluid whip. Examples of rotors supported in fluid lubricated bearings show the variations of rotor deflection amplitudes and phases in the whirl and whip modes with changes of rotative speeds and/or changes in lumped mass locations along the shaft.

  15. Modelling of reactive fluid transport in deformable porous rocks

    NASA Astrophysics Data System (ADS)

    Yarushina, V. M.; Podladchikov, Y. Y.

    2009-04-01

    One outstanding challenge in geology today is the formulation of an understanding of the interaction between rocks and fluids. Advances in such knowledge are important for a broad range of geologic settings including partial melting and subsequent migration and emplacement of a melt into upper levels of the crust, or fluid flow during regional metamorphism and metasomatism. Rock-fluid interaction involves heat and mass transfer, deformation, hydrodynamic flow, and chemical reactions, thereby necessitating its consideration as a complex process coupling several simultaneous mechanisms. Deformation, chemical reactions, and fluid flow are coupled processes. Each affects the others. Special effort is required for accurate modelling of the porosity field through time. Mechanical compaction of porous rocks is usually treated under isothermal or isoentropic simplifying assumptions. However, joint consideration of both mechanical compaction and reactive porosity alteration requires somewhat greater than usual care about thermodynamic consistency. Here we consider the modelling of multi-component, multi-phase systems, which is fundamental to the study of fluid-rock interaction. Based on the conservation laws for mass, momentum, and energy in the form adopted in the theory of mixtures, we derive a thermodynamically admissible closed system of equations describing the coupling of heat and mass transfer, chemical reactions, and fluid flow in a deformable solid matrix. Geological environments where reactive transport is important are located at different depths and accordingly have different rheologies. In the near surface, elastic or elastoplastic properties would dominate, whereas viscoplasticity would have a profound effect deeper in the lithosphere. Poorly understood rheologies of heterogeneous porous rocks are derived from well understood processes (i.e., elasticity, viscosity, plastic flow, fracturing, and their combinations) on the microscale by considering a

  16. A New 3D Multi-fluid Model: A Study of Kinetic Effects and Variations of Physical Conditions in the Cometary Coma

    NASA Astrophysics Data System (ADS)

    Shou, Y.; Combi, M.; Toth, G.; Tenishev, V.; Fougere, N.; Jia, X.; Rubin, M.; Huang, Z.; Hansen, K.; Gombosi, T.; Bieler, A.

    2016-12-01

    Physics-based numerical coma models are desirable whether to interpret the spacecraft observations of the inner coma or to compare with the ground-based observations of the outer coma. In this work, we develop a multi-neutral-fluid model based on the BATS-R-US code of the University of Michigan, which is capable of computing both the inner and outer coma and simulating time-variable phenomena. It treats H2O, OH, H2, O, and H as separate fluids and each fluid has its own velocity and temperature, with collisions coupling all fluids together. The self-consistent collisional interactions decrease the velocity differences, re-distribute the excess energy deposited by chemical reactions among all species, and account for the varying heating efficiency under various physical conditions. Recognizing that the fluid approach has limitations in capturing all of the correct physics for certain applications, especially for very low density environment, we applied our multi-fluid coma model to comet 67P/Churyumov-Gerasimenko at various heliocentric distances and demonstrated that it yields comparable results to the Direct Simulation Monte Carlo (DSMC) model, which is based on a kinetic approach that is valid under these conditions. Therefore, our model may be a powerful alternative to the particle-based model, especially for some computationally intensive simulations. In addition, by running the model with several combinations of production rates and heliocentric distances, we characterize the cometary H2O expansion speeds and demonstrate the nonlinear dependencies of production rate and heliocentric distance. Our results are also compared to previous modeling work and remote observations, which serve as further validation of our model.

  17. Microscope-Based Fluid Physics Experiments in the Fluids and Combustion Facility on ISS

    NASA Technical Reports Server (NTRS)

    Doherty, Michael P.; Motil, Susan M.; Snead, John H.; Malarik, Diane C.

    2000-01-01

    At the NASA Glenn Research Center, the Microgravity Science Program is planning to conduct a large number of experiments on the International Space Station in both the Fluid Physics and Combustion Science disciplines, and is developing flight experiment hardware for use within the International Space Station's Fluids and Combustion Facility. Four fluids physics experiments that require an optical microscope will be sequentially conducted within a subrack payload to the Fluids Integrated Rack of the Fluids and Combustion Facility called the Light Microscopy Module, which will provide the containment, changeout, and diagnostic capabilities to perform the experiments. The Light Microscopy Module is planned as a fully remotely controllable on-orbit microscope facility, allowing flexible scheduling and control of experiments within International Space Station resources. This paper will focus on the four microscope-based experiments, specifically, their objectives and the sample cell and instrument hardware to accommodate their requirements.

  18. Advanced computation for modeling fluid-solid dynamics in subduction zones

    NASA Astrophysics Data System (ADS)

    Spiegelman, Marc; Wilson, Cian; van Keken, Peter; Kelemen, Peter; Hacker, Bradley

    2014-05-01

    Arc volcanism associated with subduction is generally considered to occur by a process where hydrous fluids are released from the slab, interact with the overlying mantle wedge to produce silicate rich magmas which are then transported to the arc. However, the quantitative details of fluid release, migration, melt generation and transport in the wedge remain poorly understood. In particular, there are two fundamental observations that defy quantitative modeling. The first is the location of the volcanic front with respect to intermediate depth earthquakes (e.g. 100 ± 40 km). This observation is remarkably robust yet insensitive to subduction parameters. This contrasts with new estimates on the variability of fluid release in global subduction zones which suggest a significant sensitivity of fluid release to slab thermal conditions. Reconciling these results implies some mechanism for focusing fluids and/or melts toward the wedge corner. The second observation is the global existence of thermally hot erupted basalts and andesites that, if derived from flux melting of the mantle requires sub-arc mantle temperatures of 1300 degrees C over shallow pressures of 1-2 GPa comparable to P-T estimates for the dry solidus beneath mid-ocean ridges. These observations impose significant challenges for geodynamic models of subduction zones, and in particular for those that do not include the explicit transport of fluids and melts. We present a range of high-resolution models that include a more complete description of coupled fluid and solid mechanics (allowing the fluid to interact with solid rheological variations) together with rheologically consistent solution for temperature and solid flow. We discuss how successful these interactions are at focusing both fluids and hot solids to sub-arc regions worldwide. We also evaluate the efficacy of current wet melting parameterizations in these models. When driven by buoyancy alone, fluid migrates through the mantle wedge along

  19. The dynamic two-fluid model OLGA; Theory and application

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

    Bendiksen, K.H.; Maines, D.; Moe, R.

    1991-05-01

    Dynamic two-fluid models have found a wide range of application in the simulation of two-phase-flow systems, particularly for the analysis of steam/water flow in the core of a nuclear reactor. Until quite recently, however, very few attempts have been made to use such models in the simulation of two-phase oil and gas flow in pipelines. This paper presents a dynamic two-fluid model, OLGA, in detail, stressing the basic equations and the two-fluid models applied. Predictions of steady-state pressure drop, liquid hold-up, and flow-regime transitions are compared with data from the SINTEF Two-Phase Flow Laboratory and from the literature. Comparisons withmore » evaluated field data are also presented.« less

  20. Numerical Modelling of Three-Fluid Flow Using The Level-set Method

    NASA Astrophysics Data System (ADS)

    Li, Hongying; Lou, Jing; Shang, Zhi

    2014-11-01

    This work presents a numerical model for simulation of three-fluid flow involving two different moving interfaces. These interfaces are captured using the level-set method via two different level-set functions. A combined formulation with only one set of conservation equations for the whole physical domain, consisting of the three different immiscible fluids, is employed. Numerical solution is performed on a fixed mesh using the finite volume method. Surface tension effect is incorporated using the Continuum Surface Force model. Validation of the present model is made against available results for stratified flow and rising bubble in a container with a free surface. Applications of the present model are demonstrated by a variety of three-fluid flow systems including (1) three-fluid stratified flow, (2) two-fluid stratified flow carrying the third fluid in the form of drops and (3) simultaneous rising and settling of two drops in a stationary third fluid. The work is supported by a Thematic and Strategic Research from A*STAR, Singapore (Ref. #: 1021640075).

  1. A collaborative exercise on DNA methylation based body fluid typing.

    PubMed

    Jung, Sang-Eun; Cho, Sohee; Antunes, Joana; Gomes, Iva; Uchimoto, Mari L; Oh, Yu Na; Di Giacomo, Lisa; Schneider, Peter M; Park, Min Sun; van der Meer, Dieudonne; Williams, Graham; McCord, Bruce; Ahn, Hee-Jung; Choi, Dong Ho; Lee, Yang Han; Lee, Soong Deok; Lee, Hwan Young

    2016-10-01

    A collaborative exercise on DNA methylation based body fluid identification was conducted by seven laboratories. For this project, a multiplex methylation SNaPshot reaction composed of seven CpG markers was used for the identification of four body fluids, including blood, saliva, semen, and vaginal fluid. A total of 30 specimens were prepared and distributed to participating laboratories after thorough testing. The required experiments included four increasingly complex tasks: (1) CE of a purified single-base extension reaction product, (2) multiplex PCR and multiplex single-base extension reaction of bisulfite-modified DNA, (3) bisulfite conversion of genomic DNA, and (4) extraction of genomic DNA from body fluid samples. In tasks 2, 3 and 4, one or more mixtures were analyzed, and specimens containing both known and unknown body fluid sources were used. Six of the laboratories generated consistent body fluid typing results for specimens of bisulfite-converted DNA and genomic DNA. One laboratory failed to set up appropriate conditions for capillary analysis of reference single-base extension products. In general, variation in the values obtained for DNA methylation analysis between laboratories increased with the complexity of the required experiments. However, all laboratories concurred on the interpretation of the DNA methylation profiles produced. Although the establishment of interpretational guidelines on DNA methylation based body fluid identification has yet to be performed, this study supports the addition of DNA methylation profiling to forensic body fluid typing. © 2016 WILEY-VCH Verlag GmbH & Co. KGaA, Weinheim.

  2. Cognitive components underpinning the development of model-based learning.

    PubMed

    Potter, Tracey C S; Bryce, Nessa V; Hartley, Catherine A

    2017-06-01

    Reinforcement learning theory distinguishes "model-free" learning, which fosters reflexive repetition of previously rewarded actions, from "model-based" learning, which recruits a mental model of the environment to flexibly select goal-directed actions. Whereas model-free learning is evident across development, recruitment of model-based learning appears to increase with age. However, the cognitive processes underlying the development of model-based learning remain poorly characterized. Here, we examined whether age-related differences in cognitive processes underlying the construction and flexible recruitment of mental models predict developmental increases in model-based choice. In a cohort of participants aged 9-25, we examined whether the abilities to infer sequential regularities in the environment ("statistical learning"), maintain information in an active state ("working memory") and integrate distant concepts to solve problems ("fluid reasoning") predicted age-related improvements in model-based choice. We found that age-related improvements in statistical learning performance did not mediate the relationship between age and model-based choice. Ceiling performance on our working memory assay prevented examination of its contribution to model-based learning. However, age-related improvements in fluid reasoning statistically mediated the developmental increase in the recruitment of a model-based strategy. These findings suggest that gradual development of fluid reasoning may be a critical component process underlying the emergence of model-based learning. Copyright © 2016 The Authors. Published by Elsevier Ltd.. All rights reserved.

  3. Electrostatically frequency tunable micro-beam-based piezoelectric fluid flow energy harvester

    NASA Astrophysics Data System (ADS)

    Rezaee, Mousa; Sharafkhani, Naser

    2017-07-01

    This research investigates the dynamic behavior of a sandwich micro-beam based piezoelectric energy harvester with electrostatically adjustable resonance frequency. The system consists of a cantilever micro-beam immersed in a fluid domain and is subjected to the simultaneous action of cross fluid flow and nonlinear electrostatic force. Two parallel piezoelectric laminates are extended along the length of the micro-beam and connected to an external electric circuit which generates an output power as a result of the micro-beam oscillations. The fluid-coupled structure is modeled using Euler-Bernoulli beam theory and the equivalent force terms for the fluid flow. Fluid induced forces comprise the added inertia force which is evaluated using equivalent added mass and the drag and lift forces which are evaluated using relative velocity and Van der Pol equation. In addition to flow velocity and fluid density, the influence of several design parameters such as external electrical resistance, piezo layer position, and dc voltage on the generated power are investigated by using Galerkin and step by step linearization method. It is shown that for given flowing fluid parameters, i.e., density and velocity, one can adjust the applied dc voltage to tune resonance frequency so that the lock-in phenomenon with steady large amplitude oscillations happens, also by adjusting the harvester parameters including the mechanical and electrical ones, the maximal output power of the harvester becomes possible.

  4. Tribological and Rheological Properties of a Synovial Fluid Model

    NASA Astrophysics Data System (ADS)

    Klossner, Rebecca; Liang, Jing; Krause, Wendy

    2010-03-01

    Hyaluronic acid (HA) and the plasma proteins, albumin and globulins, are the most abundant macromolecules in synovial fluid, the fluid that lubricates freely moving joints. In previous studies, bovine synovial fluid, a synovial fluid model (SFM) and albumin in phosphate buffered saline (PBS) were observed to be rheopectic---viscosity increases over time under constant shear. Additionally, steady shear experiments have a strong shear history dependence in protein-containing solutions, whereas samples of HA in PBS behaved as a ``typical'' polyelectrolyte. The observed rheopexy and shear history dependence are indicative of structure building in solution, which is most likely caused by protein aggregation. The tribology of the SFM was also investigated using nanoindenter-based scratch tests. The coefficient of frictions (μ) between the diamond nanoindenter tip and a polyethylene surface was measured in the presence of the SFM and solutions with varied protein and HA concentrations. The lowest μ is observed in the SFM, which most closely mimics a healthy joint. Finally, an anti-inflammatory drug, hydroxychloroquine, was shown to inhibit protein interactions in the SFM in rheological studies, and thus the tribological response was examined. We hypothesize that the rheopectic behavior is important in lubrication regimes and therefore, the rheological and tribological properties of these solutions will be correlated.

  5. Modeling and test of a kinaesthetic actuator based on MR fluid for haptic applications.

    PubMed

    Yang, Tae-Heon; Koo, Jeong-Hoi; Kim, Sang-Youn; Kwon, Dong-Soo

    2017-03-01

    Haptic display units have been widely used for conveying button sensations to users, primarily employing vibrotactile actuators. However, the human feeling for pressing buttons mainly relies on kinaesthetic sensations (rather than vibrotactile sensations), and little studies exist on small-scale kinaesthetic haptic units. Thus, the primary goals of this paper are to design a miniature kinaesthetic actuator based on Magneto-Rheological (MR) fluid that can convey various button-clicking sensations and to experimentally evaluate its haptic performance. The design focuses of the proposed actuator were to produce sufficiently large actuation forces (resistive forces) for human users in a given size constraint and to offer a wide range of actuation forces for conveying vivid haptic sensations to users. To this end, this study first performed a series of parametric studies using mathematical force models for multiple operating modes of MR fluid in conjunction with finite element electromagnetism analysis. After selecting design parameters based on parametric studies, a prototype actuator was constructed, and its performance was evaluated using a dynamic mechanical analyzer. It measured the actuator's resistive force with a varying stroke (pressed depth) up to 1 mm and a varying input current from 0 A to 200 mA. The results show that the proposed actuator creates a wide range of resistive forces from around 2 N (off-state) to over 9.5 N at 200 mA. In order to assess the prototype's performance in the terms of the haptic application prospective, a maximum force rate was calculated to determine just noticeable difference in force changes for the 1 mm stoke of the actuator. The results show that the force rate is sufficient to mimic various levels of button sensations, indicating that the proposed kinaesthetic actuator can offer a wide range of resistive force changes that can be conveyed to human operators.

  6. Laszlo Tisza and the two-fluid model of superfluidity

    NASA Astrophysics Data System (ADS)

    Balibar, Sébastien

    2017-11-01

    The "two-fluid model" of superfluidity was first introduced by Laszlo Tisza in 1938. On that year, Tisza published the principles of his model as a brief note in Nature and two articles in French in the Comptes rendus de l'Académie des sciences, followed in 1940 by two other articles in French in the Journal de physique et le Radium. In 1941, the two-fluid model was reformulated by Lev Landau on a more rigorous basis. Successive experiments confirmed the revolutionary idea introduced by Tisza: superfluid helium is indeed a surprising mixture of two fluids with independent velocity fields. His prediction of the existence of heat waves, a consequence of his model, was also confirmed. Then, it took several decades for the superfluidity of liquid helium to be fully understood.

  7. Cognitive Components Underpinning the Development of Model-Based Learning

    PubMed Central

    Potter, Tracey C.S.; Bryce, Nessa V.; Hartley, Catherine A.

    2016-01-01

    Reinforcement learning theory distinguishes “model-free” learning, which fosters reflexive repetition of previously rewarded actions, from “model-based” learning, which recruits a mental model of the environment to flexibly select goal-directed actions. Whereas model-free learning is evident across development, recruitment of model-based learning appears to increase with age. However, the cognitive processes underlying the development of model-based learning remain poorly characterized. Here, we examined whether age-related differences in cognitive processes underlying the construction and flexible recruitment of mental models predict developmental increases in model-based choice. In a cohort of participants aged 9–25, we examined whether the abilities to infer sequential regularities in the environment (“statistical learning”), maintain information in an active state (“working memory”) and integrate distant concepts to solve problems (“fluid reasoning”) predicted age-related improvements in model-based choice. We found that age-related improvements in statistical learning performance did not mediate the relationship between age and model-based choice. Ceiling performance on our working memory assay prevented examination of its contribution to model-based learning. However, age-related improvements in fluid reasoning statistically mediated the developmental increase in the recruitment of a model-based strategy. These findings suggest that gradual development of fluid reasoning may be a critical component process underlying the emergence of model-based learning. PMID:27825732

  8. A new model of cavern diameter based on a validated CFD study on stirring of a highly shear-thinning fluid.

    PubMed

    Story, Anna; Jaworski, Zdzisław

    2017-01-01

    Results of numerical simulations of momentum transfer for a highly shear-thinning fluid (0.2% Carbopol) in a stirred tank equipped with a Prochem Maxflo T type impeller are presented. The simulation results were validated using LDA data and both tangential and axial force measurements in the laminar and early transitional flow range. A good agreement between the predicted and experimental results of the local fluid velocity components was found. From the predicted and experimental values of both tangential and axial forces, the power number, Po , and thrust number, Th , were also calculated. Values of the absolute relative deviations were below 4.0 and 10.5%, respectively, for Po and Th , which confirms a satisfactory agreement with experiments. An intensive mixing zone, known as cavern, was observed near the impeller. In this zone, the local values of fluid velocity, strain rate, Metzner-Otto coefficient, shear stress and intensity of energy dissipation were all characterized by strong variability. Based on the results of experimental study a new model using non-dimensional impeller force number was proposed to predict the cavern diameter. Comparative numerical simulations were also carried out for a Newtonian fluid (water) and their results were similarly well verified using LDA measurements, as well as experimental power number values.

  9. Sphere based fluid systems

    NASA Technical Reports Server (NTRS)

    Elleman, Daniel D. (Inventor); Wang, Taylor G. (Inventor)

    1989-01-01

    Systems are described for using multiple closely-packed spheres. In one system for passing fluid, a multiplicity of spheres lie within a container, with all of the spheres having the same outside diameter and with the spheres being closely nested in one another to create multiple interstitial passages of a known size and configuration and smooth walls. The container has an inlet and outlet for passing fluid through the interstitial passages formed between the nested spheres. The small interstitial passages can be used to filter out material, especially biological material such as cells in a fluid, where the cells can be easily destroyed if passed across sharp edges. The outer surface of the spheres can contain a material that absorbs a constitutent in the flowing fluid, such as a particular contamination gas, or can contain a catalyst to chemically react the fluid passing therethrough, the use of multiple small spheres assuring a large area of contact of these surfaces of the spheres with the fluid. In a system for storing and releasing a fluid such as hydrogen as a fuel, the spheres can include a hollow shell containing the fluid to be stored, and located within a compressable container that can be compressed to break the shells and release the stored fluid.

  10. Aortic dissection simulation models for clinical support: fluid-structure interaction vs. rigid wall models.

    PubMed

    Alimohammadi, Mona; Sherwood, Joseph M; Karimpour, Morad; Agu, Obiekezie; Balabani, Stavroula; Díaz-Zuccarini, Vanessa

    2015-04-15

    The management and prognosis of aortic dissection (AD) is often challenging and the use of personalised computational models is being explored as a tool to improve clinical outcome. Including vessel wall motion in such simulations can provide more realistic and potentially accurate results, but requires significant additional computational resources, as well as expertise. With clinical translation as the final aim, trade-offs between complexity, speed and accuracy are inevitable. The present study explores whether modelling wall motion is worth the additional expense in the case of AD, by carrying out fluid-structure interaction (FSI) simulations based on a sample patient case. Patient-specific anatomical details were extracted from computed tomography images to provide the fluid domain, from which the vessel wall was extrapolated. Two-way fluid-structure interaction simulations were performed, with coupled Windkessel boundary conditions and hyperelastic wall properties. The blood was modelled using the Carreau-Yasuda viscosity model and turbulence was accounted for via a shear stress transport model. A simulation without wall motion (rigid wall) was carried out for comparison purposes. The displacement of the vessel wall was comparable to reports from imaging studies in terms of intimal flap motion and contraction of the true lumen. Analysis of the haemodynamics around the proximal and distal false lumen in the FSI model showed complex flow structures caused by the expansion and contraction of the vessel wall. These flow patterns led to significantly different predictions of wall shear stress, particularly its oscillatory component, which were not captured by the rigid wall model. Through comparison with imaging data, the results of the present study indicate that the fluid-structure interaction methodology employed herein is appropriate for simulations of aortic dissection. Regions of high wall shear stress were not significantly altered by the wall motion

  11. Modeling Two-Phase Flow and Vapor Cycles Using the Generalized Fluid System Simulation Program

    NASA Technical Reports Server (NTRS)

    Smith, Amanda D.; Majumdar, Alok K.

    2017-01-01

    This work presents three new applications for the general purpose fluid network solver code GFSSP developed at NASA's Marshall Space Flight Center: (1) cooling tower, (2) vapor-compression refrigeration system, and (3) vapor-expansion power generation system. These systems are widely used across engineering disciplines in a variety of energy systems, and these models expand the capabilities and the use of GFSSP to include fluids and features that are not part of its present set of provided examples. GFSSP provides pressure, temperature, and species concentrations at designated locations, or nodes, within a fluid network based on a finite volume formulation of thermodynamics and conservation laws. This paper describes the theoretical basis for the construction of the models, their implementation in the current GFSSP modeling system, and a brief evaluation of the usefulness of the model results, as well as their applicability toward a broader spectrum of analytical problems in both university teaching and engineering research.

  12. A Generalized Fluid System Simulation Program to Model Flow Distribution in Fluid Networks

    NASA Technical Reports Server (NTRS)

    Majumdar, Alok; Bailey, John W.; Schallhorn, Paul; Steadman, Todd

    1998-01-01

    This paper describes a general purpose computer program for analyzing steady state and transient flow in a complex network. The program is capable of modeling phase changes, compressibility, mixture thermodynamics and external body forces such as gravity and centrifugal. The program's preprocessor allows the user to interactively develop a fluid network simulation consisting of nodes and branches. Mass, energy and specie conservation equations are solved at the nodes; the momentum conservation equations are solved in the branches. The program contains subroutines for computing "real fluid" thermodynamic and thermophysical properties for 33 fluids. The fluids are: helium, methane, neon, nitrogen, carbon monoxide, oxygen, argon, carbon dioxide, fluorine, hydrogen, parahydrogen, water, kerosene (RP-1), isobutane, butane, deuterium, ethane, ethylene, hydrogen sulfide, krypton, propane, xenon, R-11, R-12, R-22, R-32, R-123, R-124, R-125, R-134A, R-152A, nitrogen trifluoride and ammonia. The program also provides the options of using any incompressible fluid with constant density and viscosity or ideal gas. Seventeen different resistance/source options are provided for modeling momentum sources or sinks in the branches. These options include: pipe flow, flow through a restriction, non-circular duct, pipe flow with entrance and/or exit losses, thin sharp orifice, thick orifice, square edge reduction, square edge expansion, rotating annular duct, rotating radial duct, labyrinth seal, parallel plates, common fittings and valves, pump characteristics, pump power, valve with a given loss coefficient, and a Joule-Thompson device. The system of equations describing the fluid network is solved by a hybrid numerical method that is a combination of the Newton-Raphson and successive substitution methods. This paper also illustrates the application and verification of the code by comparison with Hardy Cross method for steady state flow and analytical solution for unsteady flow.

  13. Two-fluid model for locomotion under self-confinement

    NASA Astrophysics Data System (ADS)

    Reigh, Shang Yik; Lauga, Eric

    2017-09-01

    The bacterium Helicobacter pylori causes ulcers in the stomach of humans by invading mucus layers protecting epithelial cells. It does so by chemically changing the rheological properties of the mucus from a high-viscosity gel to a low-viscosity solution in which it may self-propel. We develop a two-fluid model for this process of swimming under self-generated confinement. We solve exactly for the flow and the locomotion speed of a spherical swimmer located in a spherically symmetric system of two Newtonian fluids whose boundary moves with the swimmer. We also treat separately the special case of an immobile outer fluid. In all cases, we characterize the flow fields, their spatial decay, and the impact of both the viscosity ratio and the degree of confinement on the locomotion speed of the model swimmer. The spatial decay of the flow retains the same power-law decay as for locomotion in a single fluid but with a decreased magnitude. Independent of the assumption chosen to characterize the impact of confinement on the actuation applied by the swimmer, its locomotion speed always decreases with an increase in the degree of confinement. Our modeling results suggest that a low-viscosity region of at least six times the effective swimmer size is required to lead to swimming with speeds similar to locomotion in an infinite fluid, corresponding to a region of size above ≈25 μ m for Helicobacter pylori.

  14. Microfluidic-based Broadband Measurements of Fluid Permittivity and Permeability to 100 GHz

    NASA Astrophysics Data System (ADS)

    Little, Charles A. E.

    This dissertation concerns the development of unique microfluidic microwave devices and associated microwave calibrations to quantitatively extract the broadband permittivity and permeability of fluids between 100 kHz and 110 GHz. The devices presented here consist of SU-8- and PDMS-based microfluidic channels integrated lithographically with coplanar waveguides (CPWs), measured via an external vector network analyzer (VNA). By applying our hybrid set of microwave calibrations to the raw data we extract distributed circuit parameters, representative of the electromagnetic response of the microfluidic channel. We then correlate these parameters to the permittivity and permeability of the fluid within the channels. We are primarily focused on developing devices, calibrations, and analyses to characterize various chemical and biological systems. The small fluid volumes and overall scale of our devices lends the technique to point-of-care blood and cell analysis, as well as to the analysis of high-value chemicals. Broadband microwave microfluidics is sensitive to three primary categories of phenomena: Ionic, dipolar, and magnetic resonances. All three can occur in complex fluids such as blood, proteins and particle suspensions. In order to make quantitative measurements, we need to be able to model and separate all three types of responses. Here we first measure saline solutions (NaCl and water) as an ideal system to better understanding both the ionic and dipolar response. Specifically, we are targeting the electrical double-layer (EDL) response, an ionic effect, which dominates over the intrinsic fluid response at lower frequencies. We have found that the EDL response for saline obeys a strict Debye-type relaxation model, the frequency response of which is dependent solely on the conductivity of the solution. To develop a better understanding of the magnetic response, we first measure magnetic nanoparticles; showing it is possible to detect the magnetic resonances of

  15. A unified approach to fluid-flow, geomechanical, and seismic modelling

    NASA Astrophysics Data System (ADS)

    Yarushina, Viktoriya; Minakov, Alexander

    2016-04-01

    The perturbations of pore pressure can generate seismicity. This is supported by observations from human activities that involve fluid injection into rocks at high pressure (hydraulic fracturing, CO2 storage, geothermal energy production) and natural examples such as volcanic earthquakes. Although the seismic signals that emerge during geotechnical operations are small both in amplitude and duration when compared to natural counterparts. A possible explanation for the earthquake source mechanism is based on a number of in situ stress measurements suggesting that the crustal rocks are close to its plastic yield limit. Hence, a rapid increase of the pore pressure decreases the effective normal stress, and, thus, can trigger seismic shear deformation. At the same time, little attention has been paid to the fact that the perturbation of fluid pressure itself represents an acoustic source. Moreover, non-double-couple source mechanisms are frequently reported from the analysis of microseismicity. A consistent formulation of the source mechanism describing microseismic events should include both a shear and isotropic component. Thus, improved understanding of the interaction between fluid flow and seismic deformation is needed. With this study we aim to increase the competence in integrating real-time microseismic monitoring with geomechanical modelling such that there is a feedback loop between monitored deformation and stress field modelling. We propose fully integrated seismic, geomechanical and reservoir modelling. Our mathematical formulation is based on fundamental set of force balance, mass balance, and constitutive poro-elastoplastic equations for two-phase media consisting of deformable solid rock frame and viscous fluid. We consider a simplified 1D modelling setup for consistent acoustic source and wave propagation in poro-elastoplastic media. In this formulation the seismic wave is generated due to local changes of the stress field and pore pressure induced by

  16. Salt tectonics and shallow subseafloor fluid convection: Models of coupled fluid-heat-salt transport

    USGS Publications Warehouse

    Wilson, A.; Ruppel, C.

    2007-01-01

    Thermohaline convection associated with salt domes has the potential to drive significant fluid flow and mass and heat transport in continental margins, but previous studies of fluid flow associated with salt structures have focused on continental settings or deep flow systems of importance to petroleum exploration. Motivated by recent geophysical and geochemical observations that suggest a convective pattern to near-seafloor pore fluid flow in the northern Gulf of Mexico (GoMex), we devise numerical models that fully couple thermal and chemical processes to quantify the effects of salt geometry and seafloor relief on fluid flow beneath the seafloor. Steady-state models that ignore halite dissolution demonstrate that seafloor relief plays an important role in the evolution of shallow geothermal convection cells and that salt at depth can contribute a thermal component to this convection. The inclusion of faults causes significant, but highly localized, increases in flow rates at seafloor discharge zones. Transient models that include halite dissolution show the evolution of flow during brine formation from early salt-driven convection to later geothermal convection, characteristics of which are controlled by the interplay of seafloor relief and salt geometry. Predicted flow rates are on the order of a few millimeters per year or less for homogeneous sediments with a permeability of 10−15 m2, comparable to compaction-driven flow rates. Sediment permeabilities likely fall below 10−15 m2 at depth in the GoMex basin, but such thermohaline convection can drive pervasive mass transport across the seafloor, affecting sediment diagenesis in shallow sediments. In more permeable settings, such flow could affect methane hydrate stability, seafloor chemosynthetic communities, and the longevity of fluid seeps.

  17. Validation of an All-Pressure Fluid Drop Model: Heptane Fluid Drops in Nitrogen

    NASA Technical Reports Server (NTRS)

    Harstad, K.; Bellan, J.; Bulzan, Daniel L. (Technical Monitor)

    2000-01-01

    Despite the fact that supercritical fluids occur both in nature and in industrial situations, the fundamentals of their behavior is poorly understood because supercritical fluids combine the characteristics of both liquids and gases, and therefore their behavior is not intuitive. There are several specific reasons for the lack of understanding: First, data from (mostly optical) measurements can be very misleading because regions of high density thus observed are frequently identified with liquids. A common misconception is that if in an experiment one can optically identify "drops" and "ligaments", the observed fluid must be in a liquid state. This inference is incorrect because in fact optical measurements detect any large change (i.e. gradients) in density. Thus, the density ratio may be well below Omicron(10(exp 3)) that characterizes its liquid/gas value, but the measurement will still identify a change in the index of refraction providing that the change is sudden (steep gradients). As shown by simulations of supercritical fluids, under certain conditions the density gradients may remain large during the supercritical binary fluids mixing, thus making them optically identifiable. Therefore, there is no inconsistency between the optical observation of high density regions and the fluids being in a supercritical state. A second misconception is that because a fluid has a liquid-like density, it is appropriate to model it as a liquid. However, such fluids may have liquid-like densities while their transport properties differ from those of a liquid. Considering that the critical pressure of most fuel hydrocarbons used in Diesel and gas turbine engines is in the range of 1.5 - 3 MPa, and the fact that the maximum pressure attained in these engines is about 6 Mps, it is clear that the fuel in the combustion chamber will experience both subcritical and supercritical conditions. Studies of drop behavior over a wide range of pressures were performed in the past

  18. Modelling Transcapillary Transport of Fluid and Proteins in Hemodialysis Patients

    PubMed Central

    Pietribiasi, Mauro; Waniewski, Jacek; Załuska, Alicja; Załuska, Wojciech; Lindholm, Bengt

    2016-01-01

    Background The kinetics of protein transport to and from the vascular compartment play a major role in the determination of fluid balance and plasma refilling during hemodialysis (HD) sessions. In this study we propose a whole-body mathematical model describing water and protein shifts across the capillary membrane during HD and compare its output to clinical data while evaluating the impact of choosing specific values for selected parameters. Methods The model follows a two-compartment structure (vascular and interstitial space) and is based on balance equations of protein mass and water volume in each compartment. The capillary membrane was described according to the three-pore theory. Two transport parameters, the fractional contribution of large pores (αLP) and the total hydraulic conductivity (LpS) of the capillary membrane, were estimated from patient data. Changes in the intensity and direction of individual fluid and solute flows through each part of the transport system were analyzed in relation to the choice of different values of small pores radius and fractional conductivity, lymphatic sensitivity to hydraulic pressure, and steady-state interstitial-to-plasma protein concentration ratio. Results The estimated values of LpS and αLP were respectively 10.0 ± 8.4 mL/min/mmHg (mean ± standard deviation) and 0.062 ± 0.041. The model was able to predict with good accuracy the profiles of plasma volume and serum total protein concentration in most of the patients (average root-mean-square deviation < 2% of the measured value). Conclusions The applied model provides a mechanistic interpretation of fluid transport processes induced by ultrafiltration during HD, using a minimum of tuned parameters and assumptions. The simulated values of individual flows through each kind of pore and lymphatic absorption rate yielded by the model may suggest answers to unsolved questions on the relative impact of these not-measurable quantities on total vascular refilling and

  19. A FOUR-FLUID MHD MODEL OF THE SOLAR WIND/INTERSTELLAR MEDIUM INTERACTION WITH TURBULENCE TRANSPORT AND PICKUP PROTONS AS SEPARATE FLUID

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

    Usmanov, Arcadi V.; Matthaeus, William H.; Goldstein, Melvyn L., E-mail: arcadi.usmanov@nasa.gov

    2016-03-20

    We have developed a four-fluid, three-dimensional magnetohydrodynamic model of the solar wind interaction with the local interstellar medium. The unique features of the model are: (a) a three-fluid description for the charged components of the solar wind and interstellar plasmas (thermal protons, electrons, and pickup protons), (b) the built-in turbulence transport equations based on Reynolds decomposition and coupled with the mean-flow Reynolds-averaged equations, and (c) a solar corona/solar wind model that supplies inner boundary conditions at 40 au by computing solar wind and magnetic field parameters outward from the coronal base. The three charged species are described by separate energy equationsmore » and are assumed to move with the same velocity. The fourth fluid in the model is the interstellar hydrogen which is treated by separate continuity, momentum, and energy equations and is coupled with the charged components through photoionization and charge exchange. We evaluate the effects of turbulence transport and pickup protons on the global heliospheric structure and compute the distribution of plasma, magnetic field, and turbulence parameters throughout the heliosphere for representative solar minimum and maximum conditions. We compare our results with Voyager 1 observations in the outer heliosheath and show that the relative amplitude of magnetic fluctuations just outside the heliopause is in close agreement with the value inferred from Voyager 1 measurements by Burlaga et al. The simulated profiles of magnetic field parameters in the outer heliosheath are in qualitative agreement with the Voyager 1 observations and with the analytical model of magnetic field draping around the heliopause of Isenberg et al.« less

  20. Dynamic dielectrophoresis model of multi-phase ionic fluids.

    PubMed

    Yan, Ying; Luo, Jing; Guo, Dan; Wen, Shizhu

    2015-01-01

    Ionic-based dielectrophoretic microchips have attracted significant attention due to their wide-ranging applications in electro kinetic and biological experiments. In this work, a numerical method is used to simulate the dynamic behaviors of ionic droplets in a microchannel under the effect of dielectrophoresis. When a discrete liquid dielectric is encompassed within a continuous fluid dielectric placed in an electric field, an electric force is produced due to the dielectrophoresis effect. If either or both of the fluids are ionic liquids, the magnitude and even the direction of the force will be changed because the net ionic charge induced by an electric field can affect the polarization degree of the dielectrics. However, using a dielectrophoresis model, assuming ideal dielectrics, results in significant errors. To avoid the inaccuracy caused by the model, this work incorporates the electrode kinetic equation and defines a relationship between the polarization charge and the net ionic charge. According to the simulation conditions presented herein, the electric force obtained in this work has an error exceeding 70% of the actual value if the false effect of net ionic charge is not accounted for, which would result in significant issues in the design and optimization of experimental parameters. Therefore, there is a clear motivation for developing a model adapted to ionic liquids to provide precise control for the dielectrophoresis of multi-phase ionic liquids.

  1. Variable flexure-based fluid filter

    DOEpatents

    Brown, Steve B.; Colston, Jr., Billy W.; Marshall, Graham; Wolcott, Duane

    2007-03-13

    An apparatus and method for filtering particles from a fluid comprises a fluid inlet, a fluid outlet, a variable size passage between the fluid inlet and the fluid outlet, and means for adjusting the size of the variable size passage for filtering the particles from the fluid. An inlet fluid flow stream is introduced to a fixture with a variable size passage. The size of the variable size passage is set so that the fluid passes through the variable size passage but the particles do not pass through the variable size passage.

  2. New hydrologic model of fluid migration in deep porous media

    NASA Astrophysics Data System (ADS)

    Dmitrievsky, A.; Balanyuk, I.

    2009-04-01

    The authors present a new hydrological model of mantle processes that effect on formation of oil-and-gas bearing basins, fault tectonics and thermal convection. Any fluid migration is initially induced by lateral stresses in the crust and lithosphere which result from global geodynamic processes related to the mantle convection. The global processes are further transformed into regional movements in weakness zones. Model of porous media in deep fractured zones and idea of self-oscillation processes in mantle layers and fractured zones of the crust at different depths was used as the basis for developed concept. The content of these notions resides in the fact that there are conditions of dynamic balance in mantle layers originating as a result of combination and alternate actions of compaction and dilatance mechanisms. These mechanisms can be manifested in different combinations and under different conditions as well as can be complemented by other processes influencing on regime of fluid migration. They can act under condition of passive margin, ocean rift and ocean subduction zones as well as in consolidated platform and sheet. Self-oscillation regime, sub vertical direction of fluid flows, anomalously high layer pressure, and high level of anomalies of various geophysical fields are common for them. A certain class of fluid dynamic models describing consolidation of sedimentary basins, free oscillation processes slow and quick (at the final stage) fluid dynamic processes of the evolution of a sedimentary basin in subduction zones is considered for the first time. The last model of quick fluid dynamic processes reflects the process of formation of hydrocarbon deposits in the zones of collision of lithosphere plates. The results of numerical simulation and diagrams reflecting consecutive stages of the gas-fluid dynamic front propagation are assessed of the Pri-Caspian depression as the example. Calculations with this model will simultaneously be carried out for

  3. Fluid identification based on P-wave anisotropy dispersion gradient inversion for fractured reservoirs

    NASA Astrophysics Data System (ADS)

    Zhang, J. W.; Huang, H. D.; Zhu, B. H.; Liao, W.

    2017-10-01

    Fluid identification in fractured reservoirs is a challenging issue and has drawn increasing attentions. As aligned fractures in subsurface formations can induce anisotropy, we must choose parameters independent with azimuths to characterize fractures and fluid effects such as anisotropy parameters for fractured reservoirs. Anisotropy is often frequency dependent due to wave-induced fluid flow between pores and fractures. This property is conducive for identifying fluid type using azimuthal seismic data in fractured reservoirs. Through the numerical simulation based on Chapman model, we choose the P-wave anisotropy parameter dispersion gradient (PADG) as the new fluid factor. PADG is dependent both on average fracture radius and fluid type but independent on azimuths. When the aligned fractures in the reservoir are meter-scaled, gas-bearing layer could be accurately identified using PADG attribute. The reflection coefficient formula for horizontal transverse isotropy media by Rüger is reformulated and simplified according to frequency and the target function for inverting PADG based on frequency-dependent amplitude versus azimuth is derived. A spectral decomposition method combining Orthogonal Matching Pursuit and Wigner-Ville distribution is used to prepare the frequency-division data. Through application to synthetic data and real seismic data, the results suggest that the method is useful for gas identification in reservoirs with meter-scaled fractures using high-qualified seismic data.

  4. Physically-Based Rendering of Particle-Based Fluids with Light Transport Effects

    NASA Astrophysics Data System (ADS)

    Beddiaf, Ali; Babahenini, Mohamed Chaouki

    2018-03-01

    Recent interactive rendering approaches aim to efficiently produce images. However, time constraints deeply affect their output accuracy and realism (many light phenomena are poorly or not supported at all). To remedy this issue, in this paper, we propose a physically-based fluid rendering approach. First, while state-of-the-art methods focus on isosurface rendering with only two refractions, our proposal (1) considers the fluid as a heterogeneous participating medium with refractive boundaries, and (2) supports both multiple refractions and scattering. Second, the proposed solution is fully particle-based in the sense that no particles transformation into a grid is required. This interesting feature makes it able to handle many particle types (water, bubble, foam, and sand). On top of that, a medium with different fluids (color, phase function, etc.) can also be rendered.

  5. Molecular modeling the microstructure and phase behavior of bulk and inhomogeneous complex fluids

    NASA Astrophysics Data System (ADS)

    Bymaster, Adam

    Accurate prediction of the thermodynamics and microstructure of complex fluids is contingent upon a model's ability to capture the molecular architecture and the specific intermolecular and intramolecular interactions that govern fluid behavior. This dissertation makes key contributions to improving the understanding and molecular modeling of complex bulk and inhomogeneous fluids, with an emphasis on associating and macromolecular molecules (water, hydrocarbons, polymers, surfactants, and colloids). Such developments apply broadly to fields ranging from biology and medicine, to high performance soft materials and energy. In the bulk, the perturbed-chain statistical associating fluid theory (PC-SAFT), an equation of state based on Wertheim's thermodynamic perturbation theory (TPT1), is extended to include a crossover correction that significantly improves the predicted phase behavior in the critical region. In addition, PC-SAFT is used to investigate the vapor-liquid equilibrium of sour gas mixtures, to improve the understanding of mercaptan/sulfide removal via gas treating. For inhomogeneous fluids, a density functional theory (DFT) based on TPT1 is extended to problems that exhibit radially symmetric inhomogeneities. First, the influence of model solutes on the structure and interfacial properties of water are investigated. The DFT successfully describes the hydrophobic phenomena on microscopic and macroscopic length scales, capturing structural changes as a function of solute size and temperature. The DFT is used to investigate the structure and effective forces in nonadsorbing polymer-colloid mixtures. A comprehensive study is conducted characterizing the role of polymer concentration and particle/polymer size ratio on the structure, polymer induced depletion forces, and tendency towards colloidal aggregation. The inhomogeneous form of the association functional is used, for the first time, to extend the DFT to associating polymer systems, applicable to any

  6. FluidCam 1&2 - UAV-based Fluid Lensing Instruments for High-Resolution 3D Subaqueous Imaging and Automated Remote Biosphere Assessment of Reef Ecosystems

    NASA Astrophysics Data System (ADS)

    Chirayath, V.; Instrella, R.

    2016-02-01

    We present NASA ESTO FluidCam 1 & 2, Visible and NIR Fluid-Lensing-enabled imaging payloads for Unmanned Aerial Vehicles (UAVs). Developed as part of a focused 2014 earth science technology grant, FluidCam 1&2 are Fluid-Lensing-based computational optical imagers designed for automated 3D mapping and remote sensing of underwater coastal targets from airborne platforms. Fluid Lensing has been used to map underwater reefs in 3D in American Samoa and Hamelin Pool, Australia from UAV platforms at sub-cm scale, which has proven a valuable tool in modern marine research for marine biosphere assessment and conservation. We share FluidCam 1&2 instrument validation and testing results as well as preliminary processed data from field campaigns. Petabyte-scale aerial survey efforts using Fluid Lensing to image at-risk reefs demonstrate broad applicability to large-scale automated species identification, morphology studies and reef ecosystem characterization for shallow marine environments and terrestrial biospheres, of crucial importance to improving bathymetry data for physical oceanographic models and understanding climate change's impact on coastal zones, global oxygen production, carbon sequestration.

  7. FluidCam 1&2 - UAV-Based Fluid Lensing Instruments for High-Resolution 3D Subaqueous Imaging and Automated Remote Biosphere Assessment of Reef Ecosystems

    NASA Astrophysics Data System (ADS)

    Chirayath, V.

    2015-12-01

    We present NASA ESTO FluidCam 1 & 2, Visible and NIR Fluid-Lensing-enabled imaging payloads for Unmanned Aerial Vehicles (UAVs). Developed as part of a focused 2014 earth science technology grant, FluidCam 1&2 are Fluid-Lensing-based computational optical imagers designed for automated 3D mapping and remote sensing of underwater coastal targets from airborne platforms. Fluid Lensing has been used to map underwater reefs in 3D in American Samoa and Hamelin Pool, Australia from UAV platforms at sub-cm scale, which has proven a valuable tool in modern marine research for marine biosphere assessment and conservation. We share FluidCam 1&2 instrument validation and testing results as well as preliminary processed data from field campaigns. Petabyte-scale aerial survey efforts using Fluid Lensing to image at-risk reefs demonstrate broad applicability to large-scale automated species identification, morphology studies and reef ecosystem characterization for shallow marine environments and terrestrial biospheres, of crucial importance to improving bathymetry data for physical oceanographic models and understanding climate change's impact on coastal zones, global oxygen production, carbon sequestration.

  8. A model of fluid and solute exchange in the human: validation and implications.

    PubMed

    Bert, J L; Gyenge, C C; Bowen, B D; Reed, R K; Lund, T

    2000-11-01

    In order to understand better the complex, dynamic behaviour of the redistribution and exchange of fluid and solutes administered to normal individuals or to those with acute hypovolemia, mathematical models are used in addition to direct experimental investigation. Initial validation of a model developed by our group involved data from animal experiments (Gyenge, C.C., Bowen, B.D., Reed, R.K. & Bert, J.L. 1999b. Am J Physiol 277 (Heart Circ Physiol 46), H1228-H1240). For a first validation involving humans, we compare the results of simulations with a wide range of different types of data from two experimental studies. These studies involved administration of normal saline or hypertonic saline with Dextran to both normal and 10% haemorrhaged subjects. We compared simulations with data including the dynamic changes in plasma and interstitial fluid volumes VPL and VIT respectively, plasma and interstitial colloid osmotic pressures PiPL and PiIT respectively, haematocrit (Hct), plasma solute concentrations and transcapillary flow rates. The model predictions were overall in very good agreement with the wide range of experimental results considered. Based on the conditions investigated, the model was also validated for humans. We used the model both to investigate mechanisms associated with the redistribution and transport of fluid and solutes administered following a mild haemorrhage and to speculate on the relationship between the timing and amount of fluid infusions and subsequent blood volume expansion.

  9. Dynamic modeling method for infrared smoke based on enhanced discrete phase model

    NASA Astrophysics Data System (ADS)

    Zhang, Zhendong; Yang, Chunling; Zhang, Yan; Zhu, Hongbo

    2018-03-01

    The dynamic modeling of infrared (IR) smoke plays an important role in IR scene simulation systems and its accuracy directly influences the system veracity. However, current IR smoke models cannot provide high veracity, because certain physical characteristics are frequently ignored in fluid simulation; simplifying the discrete phase as a continuous phase and ignoring the IR decoy missile-body spinning. To address this defect, this paper proposes a dynamic modeling method for IR smoke, based on an enhanced discrete phase model (DPM). A mathematical simulation model based on an enhanced DPM is built and a dynamic computing fluid mesh is generated. The dynamic model of IR smoke is then established using an extended equivalent-blackbody-molecule model. Experiments demonstrate that this model realizes a dynamic method for modeling IR smoke with higher veracity.

  10. Cloud fluid models of gas dynamics and star formation in galaxies

    NASA Technical Reports Server (NTRS)

    Struck-Marcell, Curtis; Scalo, John M.; Appleton, P. N.

    1987-01-01

    The large dynamic range of star formation in galaxies, and the apparently complex environmental influences involved in triggering or suppressing star formation, challenges the understanding. The key to this understanding may be the detailed study of simple physical models for the dominant nonlinear interactions in interstellar cloud systems. One such model is described, a generalized Oort model cloud fluid, and two simple applications of it are explored. The first of these is the relaxation of an isolated volume of cloud fluid following a disturbance. Though very idealized, this closed box study suggests a physical mechanism for starbursts, which is based on the approximate commensurability of massive cloud lifetimes and cloud collisional growth times. The second application is to the modeling of colliding ring galaxies. In this case, the driving processes operating on a dynamical timescale interact with the local cloud processes operating on the above timescale. The results is a variety of interesting nonequilibrium behaviors, including spatial variations of star formation that do not depend monotonically on gas density.

  11. A two-phase solid/fluid model for dense granular flows including dilatancy effects

    NASA Astrophysics Data System (ADS)

    Mangeney, Anne; Bouchut, Francois; Fernandez-Nieto, Enrique; Koné, El-Hadj; Narbona-Reina, Gladys

    2016-04-01

    Describing grain/fluid interaction in debris flows models is still an open and challenging issue with key impact on hazard assessment [{Iverson et al.}, 2010]. We present here a two-phase two-thin-layer model for fluidized debris flows that takes into account dilatancy effects. It describes the velocity of both the solid and the fluid phases, the compression/dilatation of the granular media and its interaction with the pore fluid pressure [{Bouchut et al.}, 2016]. The model is derived from a 3D two-phase model proposed by {Jackson} [2000] based on the 4 equations of mass and momentum conservation within the two phases. This system has 5 unknowns: the solid and fluid velocities, the solid and fluid pressures and the solid volume fraction. As a result, an additional equation inside the mixture is necessary to close the system. Surprisingly, this issue is inadequately accounted for in the models that have been developed on the basis of Jackson's work [{Bouchut et al.}, 2015]. In particular, {Pitman and Le} [2005] replaced this closure simply by imposing an extra boundary condition at the surface of the flow. When making a shallow expansion, this condition can be considered as a closure condition. However, the corresponding model cannot account for a dissipative energy balance. We propose here an approach to correctly deal with the thermodynamics of Jackson's model by closing the mixture equations by a weak compressibility relation following {Roux and Radjai} [1998]. This relation implies that the occurrence of dilation or contraction of the granular material in the model depends on whether the solid volume fraction is respectively higher or lower than a critical value. When dilation occurs, the fluid is sucked into the granular material, the pore pressure decreases and the friction force on the granular phase increases. On the contrary, in the case of contraction, the fluid is expelled from the mixture, the pore pressure increases and the friction force diminishes. To

  12. A new 3D multi-fluid model: a study of kinetic effects and variations of physical conditions in the cometary coma

    NASA Astrophysics Data System (ADS)

    Shou, Yinsi; Combi, Michael R.; Toth, Gabor; Huang, Zhenguang; Jia, Xianzhe; Fougere, Nicolas; Tenishev, Valeriy; Gombosi, T. I.; Hansen, Kenneth C.; Bieler, Andre

    2016-10-01

    Physics-based numerical coma models are desirable whether to interpret the spacecraft observations of the inner coma or to compare with the ground-based observations of the outer coma. In this work, we develop a multi-neutral-fluid model based on BATS-R-US in the University of Michigan's SWMF (Space Weather Modeling Framework), which is capable of computing both the inner and the outer coma and simulating time-variable phenomena. It treats H2O, OH, H2, O, and H as separate fluids and each fluid has its own velocity and temperature, with collisions coupling all fluids together. The self-consistent collisional interactions decrease the velocity differences, re-distribute the excess energy deposited by chemical reactions among all species, and account for the varying heating efficiency under various physical conditions. Recognizing that the fluid approach has limitations in capturing all of the correct physics for certain applications, especially for very low density environment, we applied our multi-fluid coma model to comet 67P/Churyumov-Gerasimenko (CG) at various heliocentric distances and demonstrated that it is able to yield comparable results as the Direct Simulation Monte Carlo (DSMC) model, which is based on a kinetic approach that is valid under these conditions. Therefore, our model may be a powerful alternative to the particle-based model, especially for some computationally intensive simulations. In addition, by running the model with several combinations of production rates and heliocentric distances, we can characterize the cometary H2O expansion speeds and demonstrate the nonlinear effect of production rates or photochemical heating. Our results are also compared to previous modeling work (e.g., Bockelee-Morvan & Crovisier 1987) and remote observations (e.g., Tseng et al. 2007), which serve as further validation of our model. This work has been partially supported by grant NNX14AG84G from the NASA Planetary Atmospheres Program, and US Rosetta contracts

  13. New mathematics for old physics: The case of lattice fluids

    NASA Astrophysics Data System (ADS)

    Barberousse, Anouk; Imbert, Cyrille

    2013-08-01

    We analyze the effects of the introduction of new mathematical tools on an old branch of physics by focusing on lattice fluids, which are cellular automata (CA)-based hydrodynamical models. We examine the nature of these discrete models, the type of novelty they bring about within scientific practice and the role they play in the field of fluid dynamics. We critically analyze Rohrlich's, Fox Keller's and Hughes' claims about CA-based models. We distinguish between different senses of the predicates "phenomenological" and "theoretical" for scientific models and argue that it is erroneous to conclude, as they do, that CA-based models are necessarily phenomenological in any sense of the term. We conversely claim that CA-based models of fluids, though at first sight blatantly misrepresenting fluids, are in fact conservative as far as the basic laws of statistical physics are concerned and not less theoretical than more traditional models in the field. Based on our case-study, we propose a general discussion of the prospect of CA for modeling in physics. We finally emphasize that lattice fluids are not just exotic oddities but do bring about new advantages in the investigation of fluids' behavior.

  14. Computational Fluid Dynamic Modeling of Rocket Based Combined Cycle Engine Flowfields

    NASA Technical Reports Server (NTRS)

    Daines, Russell L.; Merkle, Charles L.

    1994-01-01

    Computational Fluid Dynamic techniques are used to study the flowfield of a fixed geometry Rocket Based Combined Cycle engine operating in rocket ejector mode. Heat addition resulting from the combustion of injected fuel causes the subsonic engine flow to choke and go supersonic in the slightly divergent combustor-mixer section. Reacting flow computations are undertaken to predict the characteristics of solutions where the heat addition is determined by the flowfield. Here, adaptive gridding is used to improve resolution in the shear layers. Results show that the sonic speed is reached in the unheated portions of the flow first, while the heated portions become supersonic later. Comparison with results from another code show reasonable agreement. The coupled solutions show that the character of the combustion-based thermal choking phenomenon can be controlled reasonably well such that there is opportunity to optimize the length and expansion ratio of the combustor-mixer.

  15. Numerical Modeling of Pressurization of Cryogenic Propellant Tank for Integrated Vehicle Fluid System

    NASA Technical Reports Server (NTRS)

    Majumdar, Alok K.; LeClair, Andre C.; Hedayat, Ali

    2016-01-01

    This paper presents a numerical model of pressurization of a cryogenic propellant tank for the Integrated Vehicle Fluid (IVF) system using the Generalized Fluid System Simulation Program (GFSSP). The IVF propulsion system, being developed by United Launch Alliance, uses boiloff propellants to drive thrusters for the reaction control system as well as to run internal combustion engines to develop power and drive compressors to pressurize propellant tanks. NASA Marshall Space Flight Center (MSFC) has been running tests to verify the functioning of the IVF system using a flight tank. GFSSP, a finite volume based flow network analysis software developed at MSFC, has been used to develop an integrated model of the tank and the pressurization system. This paper presents an iterative algorithm for converging the interface boundary conditions between different component models of a large system model. The model results have been compared with test data.

  16. Modeling Microgravity Induced Fluid Redistribution Autoregulatory and Hydrostatic Enhancements

    NASA Technical Reports Server (NTRS)

    Myers, J. G.; Werner, C.; Nelson, E. S.; Feola, A.; Raykin, J.; Samuels, B.; Ethier, C. R.

    2017-01-01

    Space flight induces a marked cephalad (headward) redistribution of blood and interstitial fluid potentially resulting in a loss of venous tone and reduction in heart muscle efficiency upon introduction into the microgravity environment. Using various types of computational models, we are investigating how this fluid redistribution may induce intracranial pressure changes, relevant to reported reductions in astronaut visual acuity, part of the Visual Impairment and Intracranial Pressure (VIIP) syndrome. Methods: We utilize a lumped parameter cardiovascular system (CVS) model, augmented by compartments comprising the cerebral spinal fluid (CSF) space, as the primary tool to describe how microgravity, and the associated lack of hydrostatic gradient, impacts fluid redistribution. Models of ocular fluid pressures and biomechanics then accept the output of the above model as boundary condition input to allow more detailed, local analysis (see IWS Abstract by Ethier et al.). Recently, we enhanced the capabilities our previously reported CVS model through the implementation of robust autoregulatory mechanisms and a more fundamental approach to the implementation of hydrostatic mechanisms. Modifying the approach of Blanco et al., we implemented auto-regulation in a quasi-static manner, as an averaged effect across the span of one heartbeat. This approach reduced the higher frequency perturbations from the regulatory mechanism and was intended to allow longer simulation times (days) than models that implement within-beat regulatory mechanisms (minutes). A more fundamental approach to hydrostatics was implemented by a quasi-1D approach, in which compartment descriptions include compartment length, orientation and relative position, allowed for modeling of body orientation, relative body positioning and, in the future, alternative gravity environments. At this time the inclusion of hydrostatic mechanisms supplies additional capabilities to train and validate the CVS model

  17. Coupled incompressible Smoothed Particle Hydrodynamics model for continuum-based modelling sediment transport

    NASA Astrophysics Data System (ADS)

    Pahar, Gourabananda; Dhar, Anirban

    2017-04-01

    A coupled solenoidal Incompressible Smoothed Particle Hydrodynamics (ISPH) model is presented for simulation of sediment displacement in erodible bed. The coupled framework consists of two separate incompressible modules: (a) granular module, (b) fluid module. The granular module considers a friction based rheology model to calculate deviatoric stress components from pressure. The module is validated for Bagnold flow profile and two standardized test cases of sediment avalanching. The fluid module resolves fluid flow inside and outside porous domain. An interaction force pair containing fluid pressure, viscous term and drag force acts as a bridge between two different flow modules. The coupled model is validated against three dambreak flow cases with different initial conditions of movable bed. The simulated results are in good agreement with experimental data. A demonstrative case considering effect of granular column failure under full/partial submergence highlights the capability of the coupled model for application in generalized scenario.

  18. Balanced Fluid Versus Saline-Based Fluid in Post-operative Severe Traumatic Brain Injury Patients: Acid-Base and Electrolytes Assessment

    PubMed Central

    Hassan, Mohamad Hasyizan; Hassan, Wan Mohd Nazaruddin Wan; Zaini, Rhendra Hardy Mohd; Shukeri, Wan Fadzlina Wan Muhd; Abidin, Huda Zainal; Eu, Chong Soon

    2017-01-01

    Background Normal saline (NS) is a common fluid of choice in neurosurgery and neuro-intensive care unit (ICU), but it does not contain other electrolytes and has the potential to cause hyperchloremic metabolic acidosis with prolonged infusion. These problems may be reduced with the availability of balanced fluid (BF), which becomes a more physiological isotonic solution with the presence of complete electrolyte content. This study aimed to compare the changes in electrolytes and acid–base between NS and BF (Sterofundin® ISO) therapy for post-operative severe traumatic brain injury (TBI) patients in neuro-ICU. Methods Sixty-six severe TBI patients who required emergency craniotomy or craniectomy and were planned for post-operative ventilation were randomised into NS (n = 33) and BF therapy groups (n = 33). The calculation of maintenance fluid given was based on the Holliday-Segar method. The electrolytes and acid–base parameters were assessed at an 8 h interval for 24 h. The data were analysed using repeated measures ANOVA. Results The NS group showed a significant lower base excess (−3.20 versus −1.35, P = 0.049), lower bicarbonate level (22.03 versus 23.48 mmol/L, P = 0.031), and more hyperchloremia (115.12 versus 111.74 mmol/L, P < 0.001) and hypokalemia (3.36 versus 3.70 mmol/L, P < 0.001) than the BF group at 24 h of therapy. The BF group showed a significantly higher level of calcium (1.97 versus 1.79 mmol/L, P = 0.003) and magnesium (0.94 versus 0.80 mmol/L, P < 0.001) than the NS group at 24 h of fluid therapy. No significant differences were found in pH, pCO2, lactate, and sodium level. Conclusion BF therapy showed better effects in maintaining higher electrolyte parameters and reducing the trend toward hyperchloremic metabolic acidosis than the NS therapy during prolonged fluid therapy for postoperative TBI patients. PMID:29386975

  19. Balanced Fluid Versus Saline-Based Fluid in Post-operative Severe Traumatic Brain Injury Patients: Acid-Base and Electrolytes Assessment.

    PubMed

    Hassan, Mohamad Hasyizan; Hassan, Wan Mohd Nazaruddin Wan; Zaini, Rhendra Hardy Mohd; Shukeri, Wan Fadzlina Wan Muhd; Abidin, Huda Zainal; Eu, Chong Soon

    2017-10-01

    Normal saline (NS) is a common fluid of choice in neurosurgery and neuro-intensive care unit (ICU), but it does not contain other electrolytes and has the potential to cause hyperchloremic metabolic acidosis with prolonged infusion. These problems may be reduced with the availability of balanced fluid (BF), which becomes a more physiological isotonic solution with the presence of complete electrolyte content. This study aimed to compare the changes in electrolytes and acid-base between NS and BF (Sterofundin® ISO) therapy for post-operative severe traumatic brain injury (TBI) patients in neuro-ICU. Sixty-six severe TBI patients who required emergency craniotomy or craniectomy and were planned for post-operative ventilation were randomised into NS ( n = 33) and BF therapy groups ( n = 33). The calculation of maintenance fluid given was based on the Holliday-Segar method. The electrolytes and acid-base parameters were assessed at an 8 h interval for 24 h. The data were analysed using repeated measures ANOVA. The NS group showed a significant lower base excess (-3.20 versus -1.35, P = 0.049), lower bicarbonate level (22.03 versus 23.48 mmol/L, P = 0.031), and more hyperchloremia (115.12 versus 111.74 mmol/L, P < 0.001) and hypokalemia (3.36 versus 3.70 mmol/L, P < 0.001) than the BF group at 24 h of therapy. The BF group showed a significantly higher level of calcium (1.97 versus 1.79 mmol/L, P = 0.003) and magnesium (0.94 versus 0.80 mmol/L, P < 0.001) than the NS group at 24 h of fluid therapy. No significant differences were found in pH, pCO 2 , lactate, and sodium level. BF therapy showed better effects in maintaining higher electrolyte parameters and reducing the trend toward hyperchloremic metabolic acidosis than the NS therapy during prolonged fluid therapy for postoperative TBI patients.

  20. A hybridizable discontinuous Galerkin method for modeling fluid-structure interaction

    NASA Astrophysics Data System (ADS)

    Sheldon, Jason P.; Miller, Scott T.; Pitt, Jonathan S.

    2016-12-01

    This work presents a novel application of the hybridizable discontinuous Galerkin (HDG) finite element method to the multi-physics simulation of coupled fluid-structure interaction (FSI) problems. Recent applications of the HDG method have primarily been for single-physics problems including both solids and fluids, which are necessary building blocks for FSI modeling. Utilizing these established models, HDG formulations for linear elastostatics, a nonlinear elastodynamic model, and arbitrary Lagrangian-Eulerian Navier-Stokes are derived. The elasticity formulations are written in a Lagrangian reference frame, with the nonlinear formulation restricted to hyperelastic materials. With these individual solid and fluid formulations, the remaining challenge in FSI modeling is coupling together their disparate mathematics on the fluid-solid interface. This coupling is presented, along with the resultant HDG FSI formulation. Verification of the component models, through the method of manufactured solutions, is performed and each model is shown to converge at the expected rate. The individual components, along with the complete FSI model, are then compared to the benchmark problems proposed by Turek and Hron [1]. The solutions from the HDG formulation presented in this work trend towards the benchmark as the spatial polynomial order and the temporal order of integration are increased.

  1. Four phases of intravenous fluid therapy: a conceptual model.

    PubMed

    Hoste, E A; Maitland, K; Brudney, C S; Mehta, R; Vincent, J-L; Yates, D; Kellum, J A; Mythen, M G; Shaw, A D

    2014-11-01

    I.V. fluid therapy plays a fundamental role in the management of hospitalized patients. While the correct use of i.v. fluids can be lifesaving, recent literature demonstrates that fluid therapy is not without risks. Indeed, the use of certain types and volumes of fluid can increase the risk of harm, and even death, in some patient groups. Data from a recent audit show us that the inappropriate use of fluids may occur in up to 20% of patients receiving fluid therapy. The delegates of the 12th Acute Dialysis Quality Initiative (ADQI) Conference sought to obtain consensus on the use of i.v. fluids with the aim of producing guidance for their use. In this article, we review a recently proposed model for fluid therapy in severe sepsis and propose a framework by which it could be adopted for use in most situations where fluid management is required. Considering the dose-effect relationship and side-effects of fluids, fluid therapy should be regarded similar to other drug therapy with specific indications and tailored recommendations for the type and dose of fluid. By emphasizing the necessity to individualize fluid therapy, we hope to reduce the risk to our patients and improve their outcome. © The Author 2014. Published by Oxford University Press on behalf of the British Journal of Anaesthesia. All rights reserved. For Permissions, please email: journals.permissions@oup.com.

  2. Fluid Analysis and Improved Structure of an ATEG Heat Exchanger Based on Computational Fluid Dynamics

    NASA Astrophysics Data System (ADS)

    Tang, Z. B.; Deng, Y. D.; Su, C. Q.; Yuan, X. H.

    2015-06-01

    In this study, a numerical model has been employed to analyze the internal flow field distribution in a heat exchanger applied for an automotive thermoelectric generator based on computational fluid dynamics. The model simulates the influence of factors relevant to the heat exchanger, including the automotive waste heat mass flow velocity, temperature, internal fins, and back pressure. The result is in good agreement with experimental test data. Sensitivity analysis of the inlet parameters shows that increase of the exhaust velocity, compared with the inlet temperature, makes little contribution (0.1 versus 0.19) to the heat transfer but results in a detrimental back pressure increase (0.69 versus 0.21). A configuration equipped with internal fins is proved to offer better thermal performance compared with that without fins. Finally, based on an attempt to improve the internal flow field, a more rational structure is obtained, offering a more homogeneous temperature distribution, higher average heat transfer coefficient, and lower back pressure.

  3. Hydraulic fracturing fluid migration in the subsurface: A review and expanded modeling results

    NASA Astrophysics Data System (ADS)

    Birdsell, Daniel T.; Rajaram, Harihar; Dempsey, David; Viswanathan, Hari S.

    2015-09-01

    Understanding the transport of hydraulic fracturing (HF) fluid that is injected into the deep subsurface for shale gas extraction is important to ensure that shallow drinking water aquifers are not contaminated. Topographically driven flow, overpressured shale reservoirs, permeable pathways such as faults or leaky wellbores, the increased formation pressure due to HF fluid injection, and the density contrast of the HF fluid to the surrounding brine can encourage upward HF fluid migration. In contrast, the very low shale permeability and capillary imbibition of water into partially saturated shale may sequester much of the HF fluid, and well production will remove HF fluid from the subsurface. We review the literature on important aspects of HF fluid migration. Single-phase flow and transport simulations are performed to quantify how much HF fluid is removed via the wellbore with flowback and produced water, how much reaches overlying aquifers, and how much is permanently sequestered by capillary imbibition, which is treated as a sink term based on a semianalytical, one-dimensional solution for two-phase flow. These simulations include all of the important aspects of HF fluid migration identified in the literature review and are performed in five stages to faithfully represent the typical operation of a hydraulically fractured well. No fracturing fluid reaches the aquifer without a permeable pathway. In the presence of a permeable pathway, 10 times more fracturing fluid reaches the aquifer if well production and capillary imbibition are not included in the model.

  4. Thermal conductivity of the Lennard-Jones chain fluid model.

    PubMed

    Galliero, Guillaume; Boned, Christian

    2009-12-01

    Nonequilibrium molecular dynamics simulations have been performed to estimate, analyze, and correlate the thermal conductivity of a fluid composed of short Lennard-Jones chains (up to 16 segments) over a large range of thermodynamic conditions. It is shown that the dilute gas contribution to the thermal conductivity decreases when the chain length increases for a given temperature. In dense states, simulation results indicate that the residual thermal conductivity of the monomer increases strongly with density, but is weakly dependent on the temperature. Compared to the monomer value, it has been noted that the residual thermal conductivity of the chain was slightly decreasing with its length. Using these results, an empirical relation, including a contribution due to the critical enhancement, is proposed to provide an accurate estimation of the thermal conductivity of the Lennard-Jones chain fluid model (up to 16 segments) over the domain 0.8fluid model merge on the same "universal" curve when plotted as a function of the excess entropy. Furthermore, it is shown that the reduced configurational thermal conductivity of the Lennard-Jones chain fluid model is approximately proportional to the reduced excess entropy for all fluid states and all chain lengths.

  5. A computational model for doctoring fluid films in gravure printing

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

    Hariprasad, Daniel S., E-mail: dshari@unm.edu; Grau, Gerd; Schunk, P. Randall

    2016-04-07

    The wiping, or doctoring, process in gravure printing presents a fundamental barrier to resolving the micron-sized features desired in printed electronics applications. This barrier starts with the residual fluid film left behind after wiping, and its importance grows as feature sizes are reduced, especially as the feature size approaches the thickness of the residual fluid film. In this work, various mechanical complexities are considered in a computational model developed to predict the residual fluid film thickness. Lubrication models alone are inadequate, and deformation of the doctor blade body together with elastohydrodynamic lubrication must be considered to make the model predictivemore » of experimental trends. Moreover, model results demonstrate that the particular form of the wetted region of the blade has a significant impact on the model's ability to reproduce experimental measurements.« less

  6. A Well-Posed, Objective and Dynamic Two-Fluid Model

    NASA Astrophysics Data System (ADS)

    Chetty, Krishna; Vaidheeswaran, Avinash; Sharma, Subash; Clausse, Alejandro; Lopez de Bertodano, Martin

    The transition from dispersed to clustered bubbly flows due to wake entrainment is analyzed with a well-posed and objective one-dimensional (1-D) Two-Fluid Model, derived from variational principles. Modeling the wake entrainment force using the variational technique requires formulation of the inertial coupling coefficient, which defines the kinetic coupling between the phases. The kinetic coupling between a pair of bubbles and the liquid is obtained from potential flow over two-spheres and the results are validated by comparing the virtual mass coefficients with existing literature. The two-body interaction kinetic coupling is then extended to a lumped parameter model for viscous flow over two cylindrical bubbles, to get the Two-Fluid Model for wake entrainment. Linear stability analyses comprising the characteristics and the dispersion relation and non-linear numerical simulations are performed with the 1-D variational Two-Fluid Model to demonstrate the wake entrainment instability leading to clustering of bubbles. Finally, the wavelengths, amplitudes and propagation velocities of the void waves from non-linear simulations are compared with the experimental data.

  7. Numerical Modeling of Multiphase Fluid Flow in Ore-Forming Hydrothermal Systems

    NASA Astrophysics Data System (ADS)

    Weis, P.; Driesner, T.; Coumou, D.; Heinrich, C. A.

    2007-12-01

    Two coexisting fluid phases - a variably saline liquid and a vapor phase - are ubiquitous in ore-forming and other hydrothermal systems. Understanding the dynamics of phase separation and the distinct physical and chemical evolution of the two fluids probably plays a key role in generating different ore deposit types, e.g. porphyry type, high and low sulfidation Cu-Mo-Au deposits. To this end, processes within hydrothermal systems have been studied with a refined numerical model describing fluid flow in transient porous media (CSP~5.0). The model is formulated on a mass, energy and momentum conserving finite-element-finite-volume (FEFV) scheme and is capable of simulating multiphase flow of NaCl-H20 fluids. Fluid properties are computed from an improved equation of state (SOWAT~2.0). It covers conditions with temperatures of up to 1000 degrees~C, pressures of up to 500 MPa, and fluid salinities of 0~to 100%~NaCl. In particular, the new set-up allows for a more accurate description of fluid phase separation during boiling of hydrothermal fluids into a vapor and a brine phase. The geometric flexibility of the FEFV-meshes allows for investigations of a large variety of geological settings, ranging from ore-forming processes in magmatic hydrothermal system to the dynamics of black smokers at mid-ocean ridges. Simulations demonstrated that hydrothermal convection patterns above cooling plutons are primarily controlled by the system-scale permeability structure. In porphyry systems, high fluid pressures develop in a stock rising from the magma chamber which can lead to rock failure and, eventually, an increase in permeability due to hydrofracturing. Comparisons of the thermal evolution as inferred from modeling studies with data from fluid inclusion studies of the Pb-Zn deposits of Madan, Bulgaria are in a strikingly good agreement. This indicates that cross-comparisons of field observations, analytical data and numerical simulations will become a powerful tool towards a

  8. Assessment of WENO-extended two-fluid modelling in compressible multiphase flows

    NASA Astrophysics Data System (ADS)

    Kitamura, Keiichi; Nonomura, Taku

    2017-03-01

    The two-fluid modelling based on an advection-upwind-splitting-method (AUSM)-family numerical flux function, AUSM+-up, following the work by Chang and Liou [Journal of Computational Physics 2007;225: 840-873], has been successfully extended to the fifth order by weighted-essentially-non-oscillatory (WENO) schemes. Then its performance is surveyed in several numerical tests. The results showed a desired performance in one-dimensional benchmark test problems: Without relying upon an anti-diffusion device, the higher-order two-fluid method captures the phase interface within a fewer grid points than the conventional second-order method, as well as a rarefaction wave and a very weak shock. At a high pressure ratio (e.g. 1,000), the interpolated variables appeared to affect the performance: the conservative-variable-based characteristic-wise WENO interpolation showed less sharper but more robust representations of the shocks and expansions than the primitive-variable-based counterpart did. In two-dimensional shock/droplet test case, however, only the primitive-variable-based WENO with a huge void fraction realised a stable computation.

  9. Instabilities and diffusion in a hydrodynamic model of a fluid membrane coupled to a thin active fluid layer.

    PubMed

    Sarkar, N; Basu, A

    2012-11-01

    We construct a coarse-grained effective two-dimensional (2d hydrodynamic theory as a theoretical model for a coupled system of a fluid membrane and a thin layer of a polar active fluid in its ordered state that is anchored to the membrane. We show that such a system is prone to generic instabilities through the interplay of nonequilibrium drive, polar order and membrane fluctuation. We use our model equations to calculate diffusion coefficients of an inclusion in the membrane and show that their values depend strongly on the system size, in contrast to their equilibrium values. Our work extends the work of S. Sankararaman and S. Ramaswamy (Phys. Rev. Lett., 102, 118107 (2009)) to a coupled system of a fluid membrane and an ordered active fluid layer. Our model is broadly inspired by and should be useful as a starting point for theoretical descriptions of the coupled dynamics of a cell membrane and a cortical actin layer anchored to it.

  10. Modeling quantum fluid dynamics at nonzero temperatures

    PubMed Central

    Berloff, Natalia G.; Brachet, Marc; Proukakis, Nick P.

    2014-01-01

    The detailed understanding of the intricate dynamics of quantum fluids, in particular in the rapidly growing subfield of quantum turbulence which elucidates the evolution of a vortex tangle in a superfluid, requires an in-depth understanding of the role of finite temperature in such systems. The Landau two-fluid model is the most successful hydrodynamical theory of superfluid helium, but by the nature of the scale separations it cannot give an adequate description of the processes involving vortex dynamics and interactions. In our contribution we introduce a framework based on a nonlinear classical-field equation that is mathematically identical to the Landau model and provides a mechanism for severing and coalescence of vortex lines, so that the questions related to the behavior of quantized vortices can be addressed self-consistently. The correct equation of state as well as nonlocality of interactions that leads to the existence of the roton minimum can also be introduced in such description. We review and apply the ideas developed for finite-temperature description of weakly interacting Bose gases as possible extensions and numerical refinements of the proposed method. We apply this method to elucidate the behavior of the vortices during expansion and contraction following the change in applied pressure. We show that at low temperatures, during the contraction of the vortex core as the negative pressure grows back to positive values, the vortex line density grows through a mechanism of vortex multiplication. This mechanism is suppressed at high temperatures. PMID:24704874

  11. A Two-Fluid, MHD Coronal Model

    NASA Technical Reports Server (NTRS)

    Suess, Steven T.; Wang, A.-H.; Wu, S. T.; Poletto, G.; McComas, D. J.

    1998-01-01

    We describe first results from a numerical two-fluid MHD model of the global structure of the solar corona. The model is two-fluid in the sense that it accounts for the collisional energy exchange between protons and electrons. As in our single-fluid model, volumetric heat and momentum sources are required to produce high speed wind from coronal holes, low speed wind above streamers, and mass fluxes similar to the empirical solar wind. By specifying different proton and electron heating functions we obtain a high proton temperature in the coronal hole and a relatively low proton temperature in the streamer (in comparison with the electron temperature). This is consistent with inferences from SOHO/UVCS, and with the Ulysses/SWOOPS proton and electron temperature measurements which we show from the fast latitude scan. The density in the coronal hole between 2 solar radii and 5 solar radii (2RS and 5RS) is similar to the density reported from SPARTAN 201-01 measurements by Fisher and Guhathakurta. The proton mass flux scaled to 1 AU is 2.4 x 10(exp 8)/sq cm s, which is consistent with Ulysses observations. Inside the closed field region, the density is sufficiently high so that the simulation gives equal proton and electron temperatures due to the high collision rate. In open field regions (in the coronal hole and above the streamer) the proton and electron temperatures differ by varying amounts. In the streamer, the temperature and density are similar to those reported empirically by Li et al and the plasma beta is larger than unity everywhere above approx. 1.5 R(sub s), as it is in all other MHD coronal streamer models.

  12. Validation of model predictions of pore-scale fluid distributions during two-phase flow

    NASA Astrophysics Data System (ADS)

    Bultreys, Tom; Lin, Qingyang; Gao, Ying; Raeini, Ali Q.; AlRatrout, Ahmed; Bijeljic, Branko; Blunt, Martin J.

    2018-05-01

    Pore-scale two-phase flow modeling is an important technology to study a rock's relative permeability behavior. To investigate if these models are predictive, the calculated pore-scale fluid distributions which determine the relative permeability need to be validated. In this work, we introduce a methodology to quantitatively compare models to experimental fluid distributions in flow experiments visualized with microcomputed tomography. First, we analyzed five repeated drainage-imbibition experiments on a single sample. In these experiments, the exact fluid distributions were not fully repeatable on a pore-by-pore basis, while the global properties of the fluid distribution were. Then two fractional flow experiments were used to validate a quasistatic pore network model. The model correctly predicted the fluid present in more than 75% of pores and throats in drainage and imbibition. To quantify what this means for the relevant global properties of the fluid distribution, we compare the main flow paths and the connectivity across the different pore sizes in the modeled and experimental fluid distributions. These essential topology characteristics matched well for drainage simulations, but not for imbibition. This suggests that the pore-filling rules in the network model we used need to be improved to make reliable predictions of imbibition. The presented analysis illustrates the potential of our methodology to systematically and robustly test two-phase flow models to aid in model development and calibration.

  13. Continuum Model of Gas Uptake for Inhomogeneous Fluids

    DOE PAGES

    Ihm, Yungok; Cooper, Valentino R.; Vlcek, Lukas; ...

    2017-07-20

    We describe a continuum model of gas uptake for inhomogeneous fluids (CMGIF) and use it to predict fluid adsorption in porous materials directly from gas-substrate interaction energies determined by first principles calculations or accurate effective force fields. The method uses a perturbation approach to correct bulk fluid interactions for local inhomogeneities caused by gas substrate interactions, and predicts local pressure and density of the adsorbed gas. The accuracy and limitations of the model are tested by comparison with the results of Grand Canonical Monte Carlo simulations of hydrogen uptake in metal-organic frameworks (MOFs). We show that the approach provides accuratemore » predictions at room temperature and at low temperatures for less strongly interacting materials. As a result, the speed of the CMGIF method makes it a promising candidate for high-throughput materials discovery in connection with existing databases of nano-porous materials.« less

  14. Working fluid selection for space-based two-phase heat transport systems

    NASA Technical Reports Server (NTRS)

    Mclinden, Mark O.

    1988-01-01

    The working fluid for externally-mounted, space-based two-phase heat transport systems is considered. A sequence of screening criteria involving freezing and critical point temperatures and latent heat of vaporization and vapor density are applied to a data base of 860 fluids. The thermal performance of the 52 fluids which pass this preliminary screening are then ranked according to their impact on the weight of a reference system. Upon considering other nonthermal criteria (flammability, toxicity, and chemical stability) a final set of 10 preferred fluids is obtained. The effects of variations in system parameters is investigated for these 10 fluids by means of a factorial design.

  15. A new mixed subgrid-scale model for large eddy simulation of turbulent drag-reducing flows of viscoelastic fluids

    NASA Astrophysics Data System (ADS)

    Li, Feng-Chen; Wang, Lu; Cai, Wei-Hua

    2015-07-01

    A mixed subgrid-scale (SGS) model based on coherent structures and temporal approximate deconvolution (MCT) is proposed for turbulent drag-reducing flows of viscoelastic fluids. The main idea of the MCT SGS model is to perform spatial filtering for the momentum equation and temporal filtering for the conformation tensor transport equation of turbulent flow of viscoelastic fluid, respectively. The MCT model is suitable for large eddy simulation (LES) of turbulent drag-reducing flows of viscoelastic fluids in engineering applications since the model parameters can be easily obtained. The LES of forced homogeneous isotropic turbulence (FHIT) with polymer additives and turbulent channel flow with surfactant additives based on MCT SGS model shows excellent agreements with direct numerical simulation (DNS) results. Compared with the LES results using the temporal approximate deconvolution model (TADM) for FHIT with polymer additives, this mixed SGS model MCT behaves better, regarding the enhancement of calculating parameters such as the Reynolds number. For scientific and engineering research, turbulent flows at high Reynolds numbers are expected, so the MCT model can be a more suitable model for the LES of turbulent drag-reducing flows of viscoelastic fluid with polymer or surfactant additives. Project supported by the China Postdoctoral Science Foundation (Grant No. 2011M500652), the National Natural Science Foundation of China (Grant Nos. 51276046 and 51206033), and the Specialized Research Fund for the Doctoral Program of Higher Education of China (Grant No. 20112302110020).

  16. Modeling of viscoelastic properties of nonpermeable porous rocks saturated with highly viscous fluid at seismic frequencies at the core scale

    NASA Astrophysics Data System (ADS)

    Wang, Zizhen; Schmitt, Douglas R.; Wang, Ruihe

    2017-08-01

    A core scale modeling method for viscoelastic properties of rocks saturated with viscous fluid at low frequencies is developed based on the stress-strain method. The elastic moduli dispersion of viscous fluid is described by the Maxwell's spring-dash pot model. Based on this modeling method, we numerically test the effects of frequency, fluid viscosity, porosity, pore size, and pore aspect ratio on the storage moduli and the stress-strain phase lag of saturated rocks. And we also compared the modeling results to the Hashin-Shtrikman bounds and the coherent potential approximation (CPA). The dynamic moduli calculated from the modeling are lower than the predictions of CPA, and both of these fall between the Hashin-Shtrikman bounds. The modeling results indicate that the frequency and the fluid viscosity have similar effects on the dynamic moduli dispersion of fully saturated rocks. We observed the Debye peak in the phase lag variation with the change of frequency and viscosity. The pore structure parameters, such as porosity, pore size, and aspect ratio affect the rock frame stiffness and result in different viscoelastic behaviors of the saturated rocks. The stress-strain phase lags are larger with smaller stiffness contrasts between the rock frame and the pore fluid. The viscoelastic properties of saturated rocks are more sensitive to aspect ratio compared to other pore structure parameters. The results suggest that significant seismic dispersion (at about 50-200 Hz) might be expected for both compressional and shear waves passing through rocks saturated with highly viscous fluids.Plain Language SummaryWe develop a core scale <span class="hlt">modeling</span> method to simulate the viscoelastic properties of rocks saturated with viscous <span class="hlt">fluid</span> at low frequencies <span class="hlt">based</span> on the stress-strain method. The elastic moduli dispersion of viscous <span class="hlt">fluid</span> is described by the Maxwell's spring-dash pot <span class="hlt">model</span>. By using this <span class="hlt">modeling</span> method, we numerically test</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29225490','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29225490"><span><span class="hlt">Fluid</span> flow in porous media using image-<span class="hlt">based</span> <span class="hlt">modelling</span> to parametrize Richards' equation.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Cooper, L J; Daly, K R; Hallett, P D; Naveed, M; Koebernick, N; Bengough, A G; George, T S; Roose, T</p> <p>2017-11-01</p> <p>The parameters in Richards' equation are usually calculated from experimentally measured values of the soil-water characteristic curve and saturated hydraulic conductivity. The complex pore structures that often occur in porous media complicate such parametrization due to hysteresis between wetting and drying and the effects of tortuosity. Rather than estimate the parameters in Richards' equation from these indirect measurements, image-<span class="hlt">based</span> <span class="hlt">modelling</span> is used to investigate the relationship between the pore structure and the parameters. A three-dimensional, X-ray computed tomography image stack of a soil sample with voxel resolution of 6 μm has been used to create a computational mesh. The Cahn-Hilliard-Stokes equations for two-<span class="hlt">fluid</span> flow, in this case water and air, were applied to this mesh and solved using the finite-element method in COMSOL Multiphysics. The upscaled parameters in Richards' equation are then obtained via homogenization. The effect on the soil-water retention curve due to three different contact angles, 0°, 20° and 60°, was also investigated. The results show that the pore structure affects the properties of the flow on the large scale, and different contact angles can change the parameters for Richards' equation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20090040000&hterms=propylene+glycol&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3Dpropylene%2Bglycol','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20090040000&hterms=propylene+glycol&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3Dpropylene%2Bglycol"><span>Evaluation of Propylene Glycol-<span class="hlt">Based</span> <span class="hlt">Fluids</span> for Constellation Habitats and Vehicles</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Lee, Steve</p> <p>2009-01-01</p> <p>Two <span class="hlt">fluid</span> life tests have been conducted to evaluate propylene glycol-<span class="hlt">based</span> <span class="hlt">fluids</span> for use in Constellation habitats and vehicles. The first test was conducted from November 2008 to January 2009 to help determine the compatibility of the propylene glycol-<span class="hlt">based</span> <span class="hlt">fluid</span> selected for Orion at the time. When the first test uncovered problems with the <span class="hlt">fluid</span> selection, an investigation and selection of a new <span class="hlt">fluid</span> were conducted. A second test was started in March 2010 to evaluate the new selection. For the first test, the <span class="hlt">fluid</span> was subjected to a thermal <span class="hlt">fluid</span> loop that had flight-like properties, as compared to Orion. The <span class="hlt">fluid</span> loop had similar wetted materials, temperatures, flow rates, and aluminum wetted surface area to <span class="hlt">fluid</span> volume ratio. The test was designed to last for 10 years, the life expectancy of the lunar habitat. However, the test lasted less than two months. System filters became clogged with precipitate, rendering the <span class="hlt">fluid</span> system inoperable. Upon examination of the precipitate, it was determined that the precipitate composition contained aluminum, which could have only come from materials in the test stand, as aluminum is not part of the original <span class="hlt">fluid</span> composition. Also, the <span class="hlt">fluid</span> pH was determined to have increased from 10.1, at the first test sample, to 12.2, at the completion of the test. This high of a pH is corrosive to aluminum and was certainly a contributing factor to the development of precipitate. Due to the problems encountered during this test, the <span class="hlt">fluid</span> was rejected as a coolant candidate for Orion. A new propylene glycol-<span class="hlt">based</span> <span class="hlt">fluid</span> was selected by the Orion project for use in the Orion vehicle. The Orion project has conducted a series of screening tests to help verify that there will be no problems with the new <span class="hlt">fluid</span> selection. To compliment testing performed by the Orion project team, a new life test was developed to test the new <span class="hlt">fluid</span>. The new test bed was similar to the original test bed, but with some improvements <span class="hlt">based</span> on experience</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017APS..DPPP11084B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017APS..DPPP11084B"><span>Linear instabilities near the DIII-D edge simulated in <span class="hlt">fluid</span> <span class="hlt">models</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bass, Eric; Holland, Christopher</p> <p>2017-10-01</p> <p>The linear instability spectrum is reported near the DIII-D edge (within the separatrix) for L-mode and H-mode shots using the new eigenvalue solver FluTES (<span class="hlt">Fluid</span> Toroidal Eigenvalue Solver). FluTES circumvents difficulties with convergence to clean linear eigenmodes (required for diagnosis of nonlinear simulations in codes such as BOUT++) often encountered with <span class="hlt">fluid</span> initial-value solvers. FluTES is well-verified in analytic cases and against a BOUT++/ELITE benchmark toroidal case. We report results for both a 3-field, one-<span class="hlt">fluid</span> <span class="hlt">model</span> (the well-known ``elm-pb'' <span class="hlt">model</span>) and a 5-field, two-<span class="hlt">fluid</span> <span class="hlt">model</span>. For the peeling-ballooning-dominated H-mode, the two solutions are qualitatively the same. In the driftwave-dominated L-mode edge, only the two-<span class="hlt">fluid</span> solution gives robust instabilities which occur primarily at n > 50 . FluTES is optimized for this regime (near-flutelike limit, toroidally spectral). Cross-separatrix, coupled <span class="hlt">fluid</span> and drift instabilities may play a role in explaining the gyrokinetic L-mode edge transport shortfall. Extension of FluTES into the open-field-line region is underway. Prepared by UCSD under Contract Number DE-FG02-06ER54871.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20160014682','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20160014682"><span>Physics-<span class="hlt">Based</span> Fragment Acceleration <span class="hlt">Modeling</span> for Pressurized Tank Burst Risk Assessments</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Manning, Ted A.; Lawrence, Scott L.</p> <p>2014-01-01</p> <p>As part of comprehensive efforts to develop physics-<span class="hlt">based</span> risk assessment techniques for space systems at NASA, coupled computational <span class="hlt">fluid</span> and rigid body dynamic simulations were carried out to investigate the flow mechanisms that accelerate tank fragments in bursting pressurized vessels. Simulations of several configurations were compared to analyses <span class="hlt">based</span> on the industry-standard Baker explosion <span class="hlt">model</span>, and were used to formulate an improved version of the <span class="hlt">model</span>. The standard <span class="hlt">model</span>, which neglects an external <span class="hlt">fluid</span>, was found to agree best with simulation results only in configurations where the internal-to-external pressure ratio is very high and fragment curvature is small. The improved <span class="hlt">model</span> introduces terms that accommodate an external <span class="hlt">fluid</span> and better account for variations <span class="hlt">based</span> on circumferential fragment count. Physics-<span class="hlt">based</span> analysis was critical in increasing the <span class="hlt">model</span>'s range of applicability. The improved tank burst <span class="hlt">model</span> can be used to produce more accurate risk assessments of space vehicle failure modes that involve high-speed debris, such as exploding propellant tanks and bursting rocket engines.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_8");'>8</a></li> <li><a href="#" onclick='return showDiv("page_9");'>9</a></li> <li class="active"><span>10</span></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_10 --> <div id="page_11" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_9");'>9</a></li> <li><a href="#" onclick='return showDiv("page_10");'>10</a></li> <li class="active"><span>11</span></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="201"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015EGUGA..1714629M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015EGUGA..1714629M"><span>A Two-Phase Solid/<span class="hlt">Fluid</span> <span class="hlt">Model</span> for Dense Granular Flows Including Dilatancy Effects</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Mangeney, Anne; Bouchut, Francois; Fernandez-Nieto, Enrique; Narbona-Reina, Gladys</p> <p>2015-04-01</p> <p>We propose a thin layer depth-averaged two-phase <span class="hlt">model</span> to describe solid-<span class="hlt">fluid</span> mixtures such as debris flows. It describes the velocity of the two phases, the compression/dilatation of the granular media and its interaction with the pore <span class="hlt">fluid</span> pressure, that itself modifies the friction within the granular phase (Iverson et al., 2010). The <span class="hlt">model</span> is derived from a 3D two-phase <span class="hlt">model</span> proposed by Jackson (2000) <span class="hlt">based</span> on the 4 equations of mass and momentum conservation within the two phases. This system has 5 unknowns: the solid and <span class="hlt">fluid</span> velocities, the solid and <span class="hlt">fluid</span> pressures and the solid volume fraction. As a result, an additional equation inside the mixture is necessary to close the system. Surprisingly, this issue is inadequately accounted for in the <span class="hlt">models</span> that have been developed on the basis of Jackson's work (Bouchut et al., 2014). In particular, Pitman and Le replaced this closure simply by imposing an extra boundary condition at the surface of the flow. When making a shallow expansion, this condition can be considered as a closure condition. However, the corresponding <span class="hlt">model</span> cannot account for a dissipative energy balance. We propose here an approach to correctly deal with the thermodynamics of Jackson's equations. We close the mixture equations by a weak compressibility relation involving a critical density, or equivalently a critical pressure. Moreover, we relax one boundary condition, making it possible for the <span class="hlt">fluid</span> to escape the granular media when compression of the granular mass occurs. Furthermore, we introduce second order terms in the equations making it possible to describe the evolution of the pore <span class="hlt">fluid</span> pressure in response to the compression/dilatation of the granular mass without prescribing an extra ad-hoc equation for the pore pressure. We prove that the energy balance associated with this Jackson closure is dissipative, as well as its thin layer associated <span class="hlt">model</span>. We present several numerical tests for the 1D case that are compared to the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014AGUFMEP41D..04M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AGUFMEP41D..04M"><span>A Two-Phase Solid/<span class="hlt">Fluid</span> <span class="hlt">Model</span> for Dense Granular Flows Including Dilatancy Effects</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Mangeney, A.; Bouchut, F.; Fernández-Nieto, E. D.; Narbona-Reina, G.; Kone, E. H.</p> <p>2014-12-01</p> <p>We propose a thin layer depth-averaged two-phase <span class="hlt">model</span> to describe solid-<span class="hlt">fluid</span> mixtures such as debris flows. It describes the velocity of the two phases, the compression/dilatation of the granular media and its interaction with the pore <span class="hlt">fluid</span> pressure, that itself modifies the friction within the granular phase (Iverson et al., 2010). The <span class="hlt">model</span> is derived from a 3D two-phase <span class="hlt">model</span> proposed by Jackson (2000) <span class="hlt">based</span> on the 4 equations of mass and momentum conservation within the two phases. This system has 5 unknowns: the solid and <span class="hlt">fluid</span> velocities, the solid and <span class="hlt">fluid</span> pressures and the solid volume fraction. As a result, an additional equation inside the mixture is necessary to close the system. Surprisingly, this issue is inadequately accounted for in the <span class="hlt">models</span> that have been developed on the basis of Jackson's work (Bouchut et al., 2014). In particular, Pitman and Le replaced this closure simply by imposing an extra boundary condition at the surface of the flow. When making a shallow expansion, this condition can be considered as a closure condition. However, the corresponding <span class="hlt">model</span> cannot account for a dissipative energy balance. We propose here an approach to correctly deal with the thermodynamics of Jackson's equations. We close the mixture equations by a weak compressibility relation involving a critical density, or equivalently a critical pressure. Moreover, we relax one boundary condition, making it possible for the <span class="hlt">fluid</span> to escape the granular media when compression of the granular mass occurs. Furthermore, we introduce second order terms in the equations making it possible to describe the evolution of the pore <span class="hlt">fluid</span> pressure in response to the compression/dilatation of the granular mass without prescribing an extra ad-hoc equation for the pore pressure. We prove that the energy balance associated with this Jackson closure is dissipative, as well as its thin layer associated <span class="hlt">model</span>. We present several numerical tests for the 1D case that are compared to the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19920015092','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19920015092"><span>Acoustic intensity calculations for axisymmetrically <span class="hlt">modeled</span> <span class="hlt">fluid</span> regions</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Hambric, Stephen A.; Everstine, Gordon C.</p> <p>1992-01-01</p> <p>An algorithm for calculating acoustic intensities from a time harmonic pressure field in an axisymmetric <span class="hlt">fluid</span> region is presented. Acoustic pressures are computed in a mesh of NASTRAN triangular finite elements of revolution (TRIAAX) using an analogy between the scalar wave equation and elasticity equations. Acoustic intensities are then calculated from pressures and pressure derivatives taken over the mesh of TRIAAX elements. Intensities are displayed as vectors indicating the directions and magnitudes of energy flow at all mesh points in the acoustic field. A prolate spheroidal shell is <span class="hlt">modeled</span> with axisymmetric shell elements (CONEAX) and submerged in a <span class="hlt">fluid</span> region of TRIAAX elements. The <span class="hlt">model</span> is analyzed to illustrate the acoustic intensity method and the usefulness of energy flow paths in the understanding of the response of <span class="hlt">fluid</span>-structure interaction problems. The structural-acoustic analogy used is summarized for completeness. This study uncovered a NASTRAN limitation involving numerical precision issues in the CONEAX stiffness calculation causing large errors in the system matrices for nearly cylindrical cones.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/23005525','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/23005525"><span><span class="hlt">Fluid</span> mechanics in <span class="hlt">fluids</span> at rest.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Brenner, Howard</p> <p>2012-07-01</p> <p>Using readily available experimental thermophoretic particle-velocity data it is shown, contrary to current teachings, that for the case of compressible flows independent dye- and particle-tracer velocity measurements of the local <span class="hlt">fluid</span> velocity at a point in a flowing <span class="hlt">fluid</span> do not generally result in the same <span class="hlt">fluid</span> velocity measure. Rather, tracer-velocity equality holds only for incompressible flows. For compressible <span class="hlt">fluids</span>, each type of tracer is shown to monitor a fundamentally different <span class="hlt">fluid</span> velocity, with (i) a dye (or any other such molecular-tagging scheme) measuring the <span class="hlt">fluid</span>'s mass velocity v appearing in the continuity equation and (ii) a small, physicochemically and thermally inert, macroscopic (i.e., non-Brownian), solid particle measuring the <span class="hlt">fluid</span>'s volume velocity v(v). The term "compressibility" as used here includes not only pressure effects on density, but also temperature effects thereon. (For example, owing to a liquid's generally nonzero isobaric coefficient of thermal expansion, nonisothermal liquid flows are to be regarded as compressible despite the general perception of liquids as being incompressible.) Recognition of the fact that two independent <span class="hlt">fluid</span> velocities, mass- and volume-<span class="hlt">based</span>, are formally required to <span class="hlt">model</span> continuum <span class="hlt">fluid</span> behavior impacts on the foundations of contemporary (monovelocity) <span class="hlt">fluid</span> mechanics. Included therein are the Navier-Stokes-Fourier equations, which are now seen to apply only to incompressible <span class="hlt">fluids</span> (a fact well-known, empirically, to experimental gas kineticists). The findings of a difference in tracer velocities heralds the introduction into <span class="hlt">fluid</span> mechanics of a general bipartite theory of <span class="hlt">fluid</span> mechanics, bivelocity hydrodynamics [Brenner, Int. J. Eng. Sci. 54, 67 (2012)], differing from conventional hydrodynamics in situations entailing compressible flows and reducing to conventional hydrodynamics when the flow is incompressible, while being applicable to both liquids and gases.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015APS..DFDL23009R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015APS..DFDL23009R"><span><span class="hlt">Fluid</span>-Structure Interaction <span class="hlt">Modeling</span> of Intracranial Aneurysm Hemodynamics: Effects of Different Assumptions</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Rajabzadeh Oghaz, Hamidreza; Damiano, Robert; Meng, Hui</p> <p>2015-11-01</p> <p>Intracranial aneurysms (IAs) are pathological outpouchings of cerebral vessels, the progression of which are mediated by complex interactions between the blood flow and vasculature. Image-<span class="hlt">based</span> computational <span class="hlt">fluid</span> dynamics (CFD) has been used for decades to investigate IA hemodynamics. However, the commonly adopted simplifying assumptions in CFD (e.g. rigid wall) compromise the simulation accuracy and mask the complex physics involved in IA progression and eventual rupture. Several groups have considered the wall compliance by using <span class="hlt">fluid</span>-structure interaction (FSI) <span class="hlt">modeling</span>. However, FSI simulation is highly sensitive to numerical assumptions (e.g. linear-elastic wall material, Newtonian <span class="hlt">fluid</span>, initial vessel configuration, and constant pressure outlet), the effects of which are poorly understood. In this study, a comprehensive investigation of the sensitivity of FSI simulations in patient-specific IAs is investigated using a multi-stage approach with a varying level of complexity. We start with simulations incorporating several common simplifications: rigid wall, Newtonian <span class="hlt">fluid</span>, and constant pressure at the outlets, and then we stepwise remove these simplifications until the most comprehensive FSI simulations. Hemodynamic parameters such as wall shear stress and oscillatory shear index are assessed and compared at each stage to better understand the sensitivity of in FSI simulations for IA to <span class="hlt">model</span> assumptions. Supported by the National Institutes of Health (1R01 NS 091075-01).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017APS..MAR.K4013W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017APS..MAR.K4013W"><span><span class="hlt">Fluid</span>-Structure <span class="hlt">Model</span> of Lymphatic Valve and Vessel</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wolf, Ki; Ballard, Matthew; Nepiyushchikh, Zhanna; Razavi, Mohammad; Dixon, Brandon; Alexeev, Alexander</p> <p></p> <p>The lymphatic system is a part of the circulatory system that performs a range of important functions such as transportation of interstitial <span class="hlt">fluid</span>, fatty acid, and immune cells. The lymphatic vessels are composed of contractile walls to pump lymph against adverse pressure gradient and lymphatic valves that prevent back flow. Despite the importance of lymphatic system, the contribution of mechanical and geometric changes of lymphatic valves and vessels in pathologies of lymphatic dysfunction, such as lymphedema, is not well understood. We developed a coupled <span class="hlt">fluid</span>-solid computational <span class="hlt">model</span> to simultaneously simulate a lymphatic vessel, valve, and flow. A lattice Boltzmann <span class="hlt">model</span> is used to represent the <span class="hlt">fluid</span> component, while lattice spring <span class="hlt">model</span> is used for the solid component of the lymphatic vessel, whose mechanical properties are derived experimentally. Behaviors such as lymph flow pattern and lymphatic valve performance against backflow and adverse pressure gradient under varied parameters of lymphatic valve and vessel geometry and mechanical properties are investigated to provide a better insight into the dynamics of lymphatic vessels, valves, and system and give insight into how they might fail in disease. NSF CMMI-1635133.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/22233045','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/22233045"><span>[Study on the dynamic <span class="hlt">model</span> with supercritical CO2 <span class="hlt">fluid</span> extracting the lipophilic components in Panax notoginseng].</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Duan, Xian-Chun; Wang, Yong-Zhong; Zhang, Jun-Ru; Luo, Huan; Zhang, Heng; Xia, Lun-Zhu</p> <p>2011-08-01</p> <p>To establish a dynamics <span class="hlt">model</span> for extracting the lipophilic components in Panax notoginseng with supercritical carbon dioxide (CO2). <span class="hlt">Based</span> on the theory of counter-flow mass transfer and the molecular mass transfer between the material and the supercritical CO2 <span class="hlt">fluid</span> under differential mass-conservation equation, a dynamics <span class="hlt">model</span> was established and computed to compare forecasting result with the experiment process. A dynamics <span class="hlt">model</span> has been established for supercritical CO2 to extract the lipophilic components in Panax notoginseng, the computed result of this <span class="hlt">model</span> was consistent with the experiment process basically. The supercritical <span class="hlt">fluid</span> extract dynamics <span class="hlt">model</span> established in this research can expound the mechanism in the extract process of which lipophilic components of Panax notoginseng dissolve the mass transfer and is tallied with the actual extract process. This provides certain instruction for the supercritical CO2 <span class="hlt">fluid</span> extract' s industrialization enlargement.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22525150-spherically-symmetric-einstein-aether-perfect-fluid-models','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22525150-spherically-symmetric-einstein-aether-perfect-fluid-models"><span>Spherically symmetric Einstein-aether perfect <span class="hlt">fluid</span> <span class="hlt">models</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>Coley, Alan A.; Latta, Joey; Leon, Genly</p> <p></p> <p>We investigate spherically symmetric cosmological <span class="hlt">models</span> in Einstein-aether theory with a tilted (non-comoving) perfect <span class="hlt">fluid</span> source. We use a 1+3 frame formalism and adopt the comoving aether gauge to derive the evolution equations, which form a well-posed system of first order partial differential equations in two variables. We then introduce normalized variables. The formalism is particularly well-suited for numerical computations and the study of the qualitative properties of the <span class="hlt">models</span>, which are also solutions of Horava gravity. We study the local stability of the equilibrium points of the resulting dynamical system corresponding to physically realistic inhomogeneous cosmological <span class="hlt">models</span> and astrophysicalmore » objects with values for the parameters which are consistent with current constraints. In particular, we consider dust <span class="hlt">models</span> in (β−) normalized variables and derive a reduced (closed) evolution system and we obtain the general evolution equations for the spatially homogeneous Kantowski-Sachs <span class="hlt">models</span> using appropriate bounded normalized variables. We then analyse these <span class="hlt">models</span>, with special emphasis on the future asymptotic behaviour for different values of the parameters. Finally, we investigate static <span class="hlt">models</span> for a mixture of a (necessarily non-tilted) perfect <span class="hlt">fluid</span> with a barotropic equations of state and a scalar field.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.H51C1492N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.H51C1492N"><span>Phase field <span class="hlt">modeling</span> of crack propagations in <span class="hlt">fluid</span>-saturated porous media with anisotropic surface energy</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Na, S.; Sun, W.; Yoon, H.; Choo, J.</p> <p>2016-12-01</p> <p>Directional mechanical properties of layered geomaterials such as shale are important on evaluating the onset and growth of fracture for engineering applications such as hydraulic fracturing, geologic carbon storage, and geothermal recovery. In this study, a continuum phase field <span class="hlt">modeling</span> is conducted to demonstrate the initiation and pattern of cracks in <span class="hlt">fluid</span>-saturated porous media. The discontinuity of sharp cracks is formulated using diffusive crack phase field <span class="hlt">modeling</span> and the anisotropic surface energy is incorporated to account for the directional fracture toughness. In particular, the orientation of bedding in geomaterials with respect to the loading direction is represented by the directional critical energy release rate. Interactions between solid skeleton and <span class="hlt">fluid</span> are also included to analyze the mechanical behavior of <span class="hlt">fluid</span>-saturated geologic materials through the coupled hydro-mechanical <span class="hlt">model</span>. <span class="hlt">Based</span> on the linear elastic phase field <span class="hlt">modeling</span>, we also addressed how the plasticity in crack phase field influences the crack patterns by adopting the elasto-plastic <span class="hlt">model</span> with Drucker-Prager yield criterion. Numerical examples exhibit the features of anisotropic surface energy, the interactions between solid and <span class="hlt">fluid</span> and the effects of plasticity on crack propagations.Sandia National Laboratories is a multi-program laboratory managed and operated by Sandia Corporation, a wholly owned subsidiary of Lockheed Martin Corporation, for the U.S. Department of Energy's National Nuclear Security Administration under contract DE-AC04-94AL85000.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20120001214','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20120001214"><span><span class="hlt">Base</span> Flow <span class="hlt">Model</span> Validation</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Sinha, Neeraj; Brinckman, Kevin; Jansen, Bernard; Seiner, John</p> <p>2011-01-01</p> <p>A method was developed of obtaining propulsive <span class="hlt">base</span> flow data in both hot and cold jet environments, at Mach numbers and altitude of relevance to NASA launcher designs. The <span class="hlt">base</span> flow data was used to perform computational <span class="hlt">fluid</span> dynamics (CFD) turbulence <span class="hlt">model</span> assessments of <span class="hlt">base</span> flow predictive capabilities in order to provide increased confidence in <span class="hlt">base</span> thermal and pressure load predictions obtained from computational <span class="hlt">modeling</span> efforts. Predictive CFD analyses were used in the design of the experiments, available propulsive <span class="hlt">models</span> were used to reduce program costs and increase success, and a wind tunnel facility was used. The data obtained allowed assessment of CFD/turbulence <span class="hlt">models</span> in a complex flow environment, working within a building-block procedure to validation, where cold, non-reacting test data was first used for validation, followed by more complex reacting <span class="hlt">base</span> flow validation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015ChPhB..24h4401Y','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015ChPhB..24h4401Y"><span>Direct numerical simulation of viscoelastic-<span class="hlt">fluid-based</span> nanofluid turbulent channel flow with heat transfer</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Yang, Juan-Cheng; Li, Feng-Chen; Cai, Wei-Hua; Zhang, Hong-Na; Yu, Bo</p> <p>2015-08-01</p> <p>Our previous experimental studies have confirmed that viscoelastic-<span class="hlt">fluid-based</span> nanofluid (VFBN) prepared by suspending nanoparticles in a viscoelastic <span class="hlt">base</span> <span class="hlt">fluid</span> (VBF, behaves drag reduction at turbulent flow state) can reduce turbulent flow resistance as compared with water and enhance heat transfer as compared with VBF. Direct numerical simulation (DNS) is performed in this study to explore the mechanisms of heat transfer enhancement (HTE) and flow drag reduction (DR) for the VFBN turbulent flow. The Giesekus <span class="hlt">model</span> is used as the constitutive equation for VFBN. Our previously proposed thermal dispersion <span class="hlt">model</span> is adopted to take into account the thermal dispersion effects of nanoparticles in the VFBN turbulent flow. The DNS results show similar behaviors for flow resistance and heat transfer to those obtained in our previous experiments. Detailed analyses are conducted for the turbulent velocity, temperature, and conformation fields obtained by DNSs for different <span class="hlt">fluid</span> cases, and for the friction factor with viscous, turbulent, and elastic contributions and heat transfer rate with conductive, turbulent and thermal dispersion contributions of nanoparticles, respectively. The mechanisms of HTE and DR of VFBN turbulent flows are then discussed. <span class="hlt">Based</span> on analogy theory, the ratios of Chilton-Colburn factor to friction factor for different <span class="hlt">fluid</span> flow cases are investigated, which from another aspect show the significant enhancement in heat transfer performance for some cases of water-<span class="hlt">based</span> nanofluid and VFBN turbulent flows. Project supported by the National Natural Science Foundation of China (Grant No. 51276046), the Specialized Research Fund for the Doctoral Program of Higher Education of China (Grant No. 20112302110020), the China Postdoctoral Science Foundation (Grant No. 2014M561037), and the President Fund of University of Chinese Academy of Sciences, China (Grant No. Y3510213N00).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/21996162','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/21996162"><span>Magnetic <span class="hlt">fluid-modeled</span> microgravity: a novel way to treat tumor.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Chen, Jun; Yan, Zhiqiang; Liu, Rongrong; Wang, Nanding; Li, Jing; Wang, Zongren</p> <p>2011-12-01</p> <p>With the advances of nanotechnology in recent years, our understanding of the therapy of cancers has deepened and the development of new technologies for cancer diseases has emerged. Here, with the recent discoveries of nanomagnetic <span class="hlt">fluids</span> as well as microgravity effects upon cancerous cells, we suggest an innovative method of treating tumor using magnetic <span class="hlt">fluid-modeled</span> microgravity. Magnetic <span class="hlt">fluids</span> are delivered by outside magnetic field to tumor issue either intravenously or through direct injection, and this is followed by application of an uniform external magnetic field that causes microgravity. The <span class="hlt">modeled</span> microgravity is to inhibit cancerous cells growth and invasion. Copyright © 2011. Published by Elsevier Ltd.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017IJGMM..1450183S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017IJGMM..1450183S"><span>Cosmological <span class="hlt">models</span> constructed by van der Waals <span class="hlt">fluid</span> approximation and volumetric expansion</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Samanta, G. C.; Myrzakulov, R.</p> <p></p> <p>The universe <span class="hlt">modeled</span> with van der Waals <span class="hlt">fluid</span> approximation, where the van der Waals <span class="hlt">fluid</span> equation of state contains a single parameter ωv. Analytical solutions to the Einstein’s field equations are obtained by assuming the mean scale factor of the metric follows volumetric exponential and power-law expansions. The <span class="hlt">model</span> describes a rapid expansion where the acceleration grows in an exponential way and the van der Waals <span class="hlt">fluid</span> behaves like an inflation for an initial epoch of the universe. Also, the <span class="hlt">model</span> describes that when time goes away the acceleration is positive, but it decreases to zero and the van der Waals <span class="hlt">fluid</span> approximation behaves like a present accelerated phase of the universe. Finally, it is observed that the <span class="hlt">model</span> contains a type-III future singularity for volumetric power-law expansion.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016MinPe.110..515M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016MinPe.110..515M"><span>Mass transfer and <span class="hlt">fluid</span> evolution in late-metamorphic veins, Rhenish Massif (Germany): insight from alteration geochemistry and <span class="hlt">fluid</span>-mineral equilibria <span class="hlt">modeling</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Marsala, Achille; Wagner, Thomas</p> <p>2016-08-01</p> <p>Element mobility and <span class="hlt">fluid</span>-rock interaction related to the formation of late-metamorphic quartz veins have been studied by combination of mineral chemistry, whole-rock geochemistry, mass balance analysis and <span class="hlt">fluid</span>-mineral equilibria <span class="hlt">modeling</span>. The quartz veins are hosted by very low-grade metasedimentary rocks of the fold-and-thrust belt of the Rhenish Massif (Germany). The veins record two stages of evolution, a massive vein filling assemblage with elongate-blocky quartz, chlorite, apatite and albite, and a later open space filling assemblage with euhedral crystals of quartz, ankerite-dolomite and minor calcite and sulfides. Detailed mass balance analysis of an alteration profile adjacent to a representative quartz vein demonstrates that element mobility is restricted to the proximal zone. The most important element changes are gain of Ca, Fe, Mg, Mn, P and CO2, and loss of Si, K and Na. The data demonstrate that wall-rock carbonation is one of the main alteration features, whereas mobility of Si, K and Na are related to dissolution of quartz and destruction of detrital feldspar and muscovite. The whole-rock geochemical data, in conjunction with <span class="hlt">fluid</span> composition data and pressure-temperature estimates, were used as input for <span class="hlt">fluid</span>-mineral equilibria <span class="hlt">modeling</span> in the system Si-Al-Fe-Mg-Ca-Na-K-C-S-O-H-B-F-Cl. <span class="hlt">Modeling</span> involved calculation of rock-buffered <span class="hlt">fluid</span> compositions over the temperature interval 100-500 °C, and reaction-path simulations where a rock-buffered high-temperature <span class="hlt">fluid</span> reacts with fresh host-rocks at temperatures of 400, 300 and 200 °C. Calculated rock-buffered <span class="hlt">fluid</span> compositions demonstrate that retrograde silica solubility is a strong driving force for quartz leaching in the temperature-pressure window of 380-450 °C and 0.5 kbar. These conditions overlap with the estimated temperatures for the initial stage of vein formation. Reaction-path <span class="hlt">models</span> show that high-temperature alteration can produce the observed silica leaching, suggesting that</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018PhRvE..97b2109P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018PhRvE..97b2109P"><span>Vapor-liquid phase behavior of a size-asymmetric <span class="hlt">model</span> of ionic <span class="hlt">fluids</span> confined in a disordered matrix: The collective-variables-<span class="hlt">based</span> approach</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Patsahan, O. V.; Patsahan, T. M.; Holovko, M. F.</p> <p>2018-02-01</p> <p>We develop a theory <span class="hlt">based</span> on the method of collective variables to study the vapor-liquid equilibrium of asymmetric ionic <span class="hlt">fluids</span> confined in a disordered porous matrix. The approach allows us to formulate the perturbation theory using an extension of the scaled particle theory for a description of a reference system presented as a two-component hard-sphere <span class="hlt">fluid</span> confined in a hard-sphere matrix. Treating an ionic <span class="hlt">fluid</span> as a size- and charge-asymmetric primitive <span class="hlt">model</span> (PM) we derive an explicit expression for the relevant chemical potential of a confined ionic system which takes into account the third-order correlations between ions. Using this expression, the phase diagrams for a size-asymmetric PM are calculated for different matrix porosities as well as for different sizes of matrix and <span class="hlt">fluid</span> particles. It is observed that general trends of the coexistence curves with the matrix porosity are similar to those of simple <span class="hlt">fluids</span> under disordered confinement, i.e., the coexistence region gets narrower with a decrease of porosity and, simultaneously, the reduced critical temperature Tc* and the critical density ρi,c * become lower. At the same time, our results suggest that an increase in size asymmetry of oppositely charged ions considerably affects the vapor-liquid diagrams leading to a faster decrease of Tc* and ρi,c * and even to a disappearance of the phase transition, especially for the case of small matrix particles.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018PhPl...25f1206R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018PhPl...25f1206R"><span>Three dimensional <span class="hlt">fluid</span>-kinetic <span class="hlt">model</span> of a magnetically guided plasma jet</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ramos, Jesús J.; Merino, Mario; Ahedo, Eduardo</p> <p>2018-06-01</p> <p>A <span class="hlt">fluid</span>-kinetic <span class="hlt">model</span> of the collisionless plasma flow in a convergent-divergent magnetic nozzle is presented. The <span class="hlt">model</span> combines the leading-order Vlasov equation and the <span class="hlt">fluid</span> continuity and perpendicular momentum equation for magnetized electrons, and the <span class="hlt">fluid</span> equations for cold ions, which must be solved iteratively to determine the self-consistent plasma response in a three-dimensional magnetic field. The kinetic electron solution identifies three electron populations and provides the plasma density and pressure tensor. The far downstream asymptotic behavior shows the anisotropic cooling of the electron populations. The <span class="hlt">fluid</span> equations determine the electric potential and the <span class="hlt">fluid</span> velocities. In the small ion-sound gyroradius case, the solution is constructed one magnetic line at a time. In the large ion-sound gyroradius case, ion detachment from magnetic lines makes the problem fully three-dimensional.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28551193','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28551193"><span>Drivers of choice for <span class="hlt">fluid</span> milk versus plant-<span class="hlt">based</span> alternatives: What are consumer perceptions of <span class="hlt">fluid</span> milk?</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>McCarthy, K S; Parker, M; Ameerally, A; Drake, S L; Drake, M A</p> <p>2017-08-01</p> <p><span class="hlt">Fluid</span> milk consumption has declined for decades while consumption of nondairy alternatives has increased. A better understanding of why consumers purchase <span class="hlt">fluid</span> milk or nondairy alternatives is needed to assist increased sales of milk or maintain sales without further decline. The objective of this study was to determine the extrinsic attributes that drive purchase within each product category. The second objective was to determine the personal values behind the purchase of each beverage type to give further understanding why particular attributes are important. An online conjoint survey was launched with 702 dairy consumers, 172 nondairy consumers, and 125 consumers of both beverages. Individual means-end chain interviews were conducted with <span class="hlt">fluid</span> milk consumers (n = 75), plant-<span class="hlt">based</span> alternative consumers (n = 68), and consumers of both beverages (n = 78). Fat content was the most important attribute for dairy milk followed by package size and label claims. Consumers of <span class="hlt">fluid</span> milk preferred 1 or 2% fat content, gallon, or half-gallon packaging, conventionally pasteurized store-brand milk. Sugar level was the most important attribute for plant-<span class="hlt">based</span> beverages, followed by plant source and package size. Almond milk was the most desirable plant source, and half-gallon packaging was the most preferred packaging. Means-end chain interviews results suggested that maintaining a balanced diet and healthy lifestyle was important to all consumer groups. Lactose free was an important attribute for plant-<span class="hlt">based</span> alternative consumers and consumers of both dairy and nondairy. A distinguishing characteristic of those who only drank nondairy plant-<span class="hlt">based</span> alternatives was that plant-<span class="hlt">based</span> beverages contributed to a goal to consume less animal products, beliefs about animal mistreatment, and perceived lesser effect on the environment than <span class="hlt">fluid</span> milk. Unique to <span class="hlt">fluid</span> milk consumers was that <span class="hlt">fluid</span> milk was perceived as a staple food item. These results suggest that the dairy industry</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018PhRvL.120c4501D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018PhRvL.120c4501D"><span>Covariant Structure of <span class="hlt">Models</span> of Geophysical <span class="hlt">Fluid</span> Motion</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Dubos, Thomas</p> <p>2018-01-01</p> <p>Geophysical <span class="hlt">models</span> approximate classical <span class="hlt">fluid</span> motion in rotating frames. Even accurate approximations can have profound consequences, such as the loss of inertial frames. If geophysical <span class="hlt">fluid</span> dynamics are not strictly equivalent to Newtonian hydrodynamics observed in a rotating frame, what kind of dynamics are they? We aim to clarify fundamental similarities and differences between relativistic, Newtonian, and geophysical hydrodynamics, using variational and covariant formulations as tools to shed the necessary light. A space-time variational principle for the motion of a perfect <span class="hlt">fluid</span> is introduced. The geophysical action is interpreted as a synchronous limit of the relativistic action. The relativistic Levi-Civita connection also has a finite synchronous limit, which provides a connection with which to endow geophysical space-time, generalizing Cartan (1923). A covariant mass-momentum budget is obtained using covariance of the action and metric-preserving properties of the connection. Ultimately, geophysical <span class="hlt">models</span> are found to differ from the standard compressible Euler <span class="hlt">model</span> only by a specific choice of a metric-Coriolis-geopotential tensor akin to the relativistic space-time metric. Once this choice is made, the same covariant mass-momentum budget applies to Newtonian and all geophysical hydrodynamics, including those <span class="hlt">models</span> lacking an inertial frame. Hence, it is argued that this mass-momentum budget provides an appropriate, common fundamental principle of dynamics. The postulate that Euclidean, inertial frames exist can then be regarded as part of the Newtonian theory of gravitation, which some <span class="hlt">models</span> of geophysical hydrodynamics slightly violate.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28284415','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28284415"><span>Sampling guidelines for oral <span class="hlt">fluid-based</span> surveys of group-housed animals.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Rotolo, Marisa L; Sun, Yaxuan; Wang, Chong; Giménez-Lirola, Luis; Baum, David H; Gauger, Phillip C; Harmon, Karen M; Hoogland, Marlin; Main, Rodger; Zimmerman, Jeffrey J</p> <p>2017-09-01</p> <p>Formulas and software for calculating sample size for surveys <span class="hlt">based</span> on individual animal samples are readily available. However, sample size formulas are not available for oral <span class="hlt">fluids</span> and other aggregate samples that are increasingly used in production settings. Therefore, the objective of this study was to develop sampling guidelines for oral <span class="hlt">fluid-based</span> porcine reproductive and respiratory syndrome virus (PRRSV) surveys in commercial swine farms. Oral <span class="hlt">fluid</span> samples were collected in 9 weekly samplings from all pens in 3 barns on one production site beginning shortly after placement of weaned pigs. Samples (n=972) were tested by real-time reverse-transcription PCR (RT-rtPCR) and the binary results analyzed using a piecewise exponential survival <span class="hlt">model</span> for interval-censored, time-to-event data with misclassification. Thereafter, simulation studies were used to study the barn-level probability of PRRSV detection as a function of sample size, sample allocation (simple random sampling vs fixed spatial sampling), assay diagnostic sensitivity and specificity, and pen-level prevalence. These studies provided estimates of the probability of detection by sample size and within-barn prevalence. Detection using fixed spatial sampling was as good as, or better than, simple random sampling. Sampling multiple barns on a site increased the probability of detection with the number of barns sampled. These results are relevant to PRRSV control or elimination projects at the herd, regional, or national levels, but the results are also broadly applicable to contagious pathogens of swine for which oral <span class="hlt">fluid</span> tests of equivalent performance are available. Copyright © 2017 The Authors. Published by Elsevier B.V. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/15160901','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/15160901"><span>Evaluation of generic types of drilling <span class="hlt">fluid</span> using a risk-<span class="hlt">based</span> analytic hierarchy process.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Sadiq, Rehan; Husain, Tahir; Veitch, Brian; Bose, Neil</p> <p>2003-12-01</p> <p>The composition of drilling muds is <span class="hlt">based</span> on a mixture of clays and additives in a <span class="hlt">base</span> <span class="hlt">fluid</span>. There are three generic categories of <span class="hlt">base</span> <span class="hlt">fluid</span>--water, oil, and synthetic. Water-<span class="hlt">based</span> <span class="hlt">fluids</span> (WBFs) are relatively environmentally benign, but drilling performance is better with oil-<span class="hlt">based</span> <span class="hlt">fluids</span> (OBFs). The oil and gas industry developed synthetic-<span class="hlt">based</span> <span class="hlt">fluids</span> (SBFs), such as vegetable esters, olefins, ethers, and others, which provide drilling performance comparable to OBFs, but with lower environmental and occupational health effects. The primary objective of this paper is to present a methodology to guide decision-making in the selection and evaluation of three generic types of drilling <span class="hlt">fluids</span> using a risk-<span class="hlt">based</span> analytic hierarchy process (AHP). In this paper a comparison of drilling <span class="hlt">fluids</span> is made considering various activities involved in the life cycle of drilling <span class="hlt">fluids</span>. This paper evaluates OBFs, WBFs, and SBFs <span class="hlt">based</span> on four major impacts--operations, resources, economics, and liabilities. Four major activities--drilling, discharging offshore, loading and transporting, and disposing onshore--cause the operational impacts. Each activity involves risks related to occupational injuries (safety), general public health, environmental impact, and energy use. A multicriteria analysis strategy was used for the selection and evaluation of drilling <span class="hlt">fluids</span> using a risk-<span class="hlt">based</span> AHP. A four-level hierarchical structure is developed to determine the final relative scores, and the SBFs are found to be the best option.</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('https://www.ncbi.nlm.nih.gov/pubmed/26492498','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26492498"><span>Soy Protein Isolate As <span class="hlt">Fluid</span> Loss Additive in Bentonite-Water-<span class="hlt">Based</span> Drilling <span class="hlt">Fluids</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Li, Mei-Chun; Wu, Qinglin; Song, Kunlin; Lee, Sunyoung; Jin, Chunde; Ren, Suxia; Lei, Tingzhou</p> <p>2015-11-11</p> <p>Wellbore instability and formation collapse caused by lost circulation are vital issues during well excavation in the oil industry. This study reports the novel utilization of soy protein isolate (SPI) as <span class="hlt">fluid</span> loss additive in bentonite-water <span class="hlt">based</span> drilling <span class="hlt">fluids</span> (BT-WDFs) and describes how its particle size and concentration influence on the filtration property of SPI/BT-WDFs. It was found that high pressure homogenization (HPH)-treated SPI had superior filtration property over that of native SPI due to the improved ability for the plugging pore throat. HPH treatment also caused a significant change in the surface characteristic of SPI, leading to a considerable surface interaction with BT in aqueous solution. The concentration of SPI had a significant impact on the dispersion state of SPI/BT mixtures in aquesous solution. At low SPI concentrations, strong aggregations were created, resulting in the formation of thick, loose, high-porosity and high-permeability filter cakes and high <span class="hlt">fluid</span> loss. At high SPI concentrations, intercatlated/exfoliated structures were generated, resulting in the formation of thin, compact, low-porosity and low-permeability filter cakes and low <span class="hlt">fluid</span> loss. The SPI/BT-WDFs exhibited superior filtration property than pure BT-WDFs at the same solid concentraion, demonstrating the potential utilization of SPI as an effective, renewable, and biodegradable <span class="hlt">fluid</span> loss reducer in well excavation applications.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4698250','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4698250"><span>Magnetic Capture of a Molecular Biomarker from Synovial <span class="hlt">Fluid</span> in a Rat <span class="hlt">Model</span> of Knee Osteoarthritis</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Yarmola, Elena G.; Shah, Yash; Arnold, David P.; Dobson, Jon; Allen, Kyle D.</p> <p>2015-01-01</p> <p>Biomarker development for osteoarthritis (OA) often begins in rodent <span class="hlt">models</span>, but can be limited by an inability to aspirate synovial <span class="hlt">fluid</span> from a rodent stifle (similar to the human knee). To address this limitation, we have developed a magnetic nanoparticle-<span class="hlt">based</span> technology to collect biomarkers from a rodent stifle, termed magnetic capture. Using a common OA biomarker - the c-terminus telopeptide of type II collagen (CTXII) - magnetic capture was optimized in vitro using bovine synovial <span class="hlt">fluid</span> and then tested in a rat <span class="hlt">model</span> of knee OA. Anti-CTXII antibodies were conjugated to the surface of superparamagnetic iron oxide-containing polymeric particles. Using these anti-CTXII particles, magnetic capture was able to estimate the level of CTXII in 25 µL aliquots of bovine synovial <span class="hlt">fluid</span>; and under controlled conditions, this estimate was unaffected by synovial <span class="hlt">fluid</span> viscosity. Following in vitro testing, anti-CTXII particles were tested in a rat monoiodoacetate <span class="hlt">model</span> of knee OA. CTXII could be magnetically captured from a rodent stifle without the need to aspirate <span class="hlt">fluid</span> and showed 10 fold changes in CTXII levels from OA-affected joints relative to contralateral control joints. Combined, these data demonstrate the ability and sensitivity of magnetic capture for post-mortem analysis of OA biomarkers in the rat. PMID:26136062</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26136062','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26136062"><span>Magnetic Capture of a Molecular Biomarker from Synovial <span class="hlt">Fluid</span> in a Rat <span class="hlt">Model</span> of Knee Osteoarthritis.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Yarmola, Elena G; Shah, Yash; Arnold, David P; Dobson, Jon; Allen, Kyle D</p> <p>2016-04-01</p> <p>Biomarker development for osteoarthritis (OA) often begins in rodent <span class="hlt">models</span>, but can be limited by an inability to aspirate synovial <span class="hlt">fluid</span> from a rodent stifle (similar to the human knee). To address this limitation, we have developed a magnetic nanoparticle-<span class="hlt">based</span> technology to collect biomarkers from a rodent stifle, termed magnetic capture. Using a common OA biomarker--the c-terminus telopeptide of type II collagen (CTXII)--magnetic capture was optimized in vitro using bovine synovial <span class="hlt">fluid</span> and then tested in a rat <span class="hlt">model</span> of knee OA. Anti-CTXII antibodies were conjugated to the surface of superparamagnetic iron oxide-containing polymeric particles. Using these anti-CTXII particles, magnetic capture was able to estimate the level of CTXII in 25 μL aliquots of bovine synovial <span class="hlt">fluid</span>; and under controlled conditions, this estimate was unaffected by synovial <span class="hlt">fluid</span> viscosity. Following in vitro testing, anti-CTXII particles were tested in a rat monoiodoacetate <span class="hlt">model</span> of knee OA. CTXII could be magnetically captured from a rodent stifle without the need to aspirate <span class="hlt">fluid</span> and showed tenfold changes in CTXII levels from OA-affected joints relative to contralateral control joints. Combined, these data demonstrate the ability and sensitivity of magnetic capture for post-mortem analysis of OA biomarkers in the rat.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010APS..DMP.M1081G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010APS..DMP.M1081G"><span>Two-<span class="hlt">fluid</span> <span class="hlt">model</span> of a Bose-Einstein condensate in the cavity optomechanical regime</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Goldbaum, Dan; Zhang, Keye; Meystre, Pierre</p> <p>2010-03-01</p> <p>We analyze an atomic Bose-Einstein condensate trapped in a high-Q optical cavity driven by a feeble optical field. The dynamics of the resulting collective density excitation of the condensate are formally analogous to the central <span class="hlt">model</span> system of cavity optomechanics: a radiation pressure driven mechanical oscillator [Brennecke et al., Science 322, 235 (2008)]. However, although BEC-<span class="hlt">based</span> optomechanical systems have several desirable properties, one must also take into account the effect of atom-atom interactions. We treat these interactions via a two-<span class="hlt">fluid</span> <span class="hlt">model</span> that retains the intuitive appeal of the non-interacting two-mode description. We find that the Bogoliubov excitation spectrum of this system comprises a gapped upper branch and a lower branch that can include an unstable excitation mode. [4pt] D. S. Goldbaum, K. Zhang and P. Meystre, Two-<span class="hlt">fluid</span> <span class="hlt">model</span> of a Bose-Einstein condensate in the cavity optomechanical regime, arXiv:0911.3234.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014AGUFM.H21C0748D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AGUFM.H21C0748D"><span>The impact of <span class="hlt">fluid</span> topology on residual saturations - A pore-network <span class="hlt">model</span> study</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Doster, F.; Kallel, W.; van Dijke, R.</p> <p>2014-12-01</p> <p>In two-phase flow in porous media only fractions of the resident <span class="hlt">fluid</span> are mobilised during a displacement process and, in general, a significant amount of the resident <span class="hlt">fluid</span> remains permanently trapped. Depending on the application, entrapment is desirable (geological carbon storage), or it should be obviated (enhanced oil recovery, contaminant remediation). Despite its utmost importance for these applications, predictions of trapped <span class="hlt">fluid</span> saturations for macroscopic systems, in particular under changing displacement conditions, remain challenging. The <span class="hlt">models</span> that aim to represent trapping phenomena are typically empirical and require tracking of the history of the state variables. This exacerbates the experimental verification and the design of sophisticated displacement technologies that enhance or impede trapping. Recently, experiments [1] have suggested that a macroscopic normalized Euler number, quantifying the topology of <span class="hlt">fluid</span> distributions, could serve as a parameter to predict residual saturations <span class="hlt">based</span> on state variables. In these experiments the entrapment of <span class="hlt">fluids</span> was visualised through 3D micro CT imaging. However, the experiments are notoriously time consuming and therefore only allow for a sparse sampling of the parameter space. Pore-network <span class="hlt">models</span> represent porous media through an equivalent network structure of pores and throats. Under quasi-static capillary dominated conditions displacement processes can be <span class="hlt">modeled</span> through simple invasion percolation rules. Hence, in contrast to experiments, pore-network <span class="hlt">models</span> are fast and therefore allow full sampling of the parameter space. Here, we use pore-network <span class="hlt">modeling</span> [2] to critically investigate the knowledge gained through observing and tracking the normalized Euler number. More specifically, we identify conditions under which (a) systems with the same saturations but different normalized Euler numbers lead to different residual saturations and (b) systems with the same saturations and the same</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5238443','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5238443"><span>A Comprehensive Numerical <span class="hlt">Model</span> for Simulating <span class="hlt">Fluid</span> Transport in Nanopores</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Zhang, Yuan; Yu, Wei; Sepehrnoori, Kamy; Di, Yuan</p> <p>2017-01-01</p> <p>Since a large amount of nanopores exist in tight oil reservoirs, <span class="hlt">fluid</span> transport in nanopores is complex due to large capillary pressure. Recent studies only focus on the effect of nanopore confinement on single-well performance with simple planar fractures in tight oil reservoirs. Its impacts on multi-well performance with complex fracture geometries have not been reported. In this study, a numerical <span class="hlt">model</span> was developed to investigate the effect of confined phase behavior on cumulative oil and gas production of four horizontal wells with different fracture geometries. Its pore sizes were divided into five regions <span class="hlt">based</span> on nanopore size distribution. Then, <span class="hlt">fluid</span> properties were evaluated under different levels of capillary pressure using Peng-Robinson equation of state. Afterwards, an efficient approach of Embedded Discrete Fracture <span class="hlt">Model</span> (EDFM) was applied to explicitly <span class="hlt">model</span> hydraulic and natural fractures in the reservoirs. Finally, three fracture geometries, i.e. non-planar hydraulic fractures, non-planar hydraulic fractures with one set natural fractures, and non-planar hydraulic fractures with two sets natural fractures, are evaluated. The multi-well performance with confined phase behavior is analyzed with permeabilities of 0.01 md and 0.1 md. This work improves the analysis of capillarity effect on multi-well performance with complex fracture geometries in tight oil reservoirs. PMID:28091599</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017NatSR...740507Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017NatSR...740507Z"><span>A Comprehensive Numerical <span class="hlt">Model</span> for Simulating <span class="hlt">Fluid</span> Transport in Nanopores</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zhang, Yuan; Yu, Wei; Sepehrnoori, Kamy; di, Yuan</p> <p>2017-01-01</p> <p>Since a large amount of nanopores exist in tight oil reservoirs, <span class="hlt">fluid</span> transport in nanopores is complex due to large capillary pressure. Recent studies only focus on the effect of nanopore confinement on single-well performance with simple planar fractures in tight oil reservoirs. Its impacts on multi-well performance with complex fracture geometries have not been reported. In this study, a numerical <span class="hlt">model</span> was developed to investigate the effect of confined phase behavior on cumulative oil and gas production of four horizontal wells with different fracture geometries. Its pore sizes were divided into five regions <span class="hlt">based</span> on nanopore size distribution. Then, <span class="hlt">fluid</span> properties were evaluated under different levels of capillary pressure using Peng-Robinson equation of state. Afterwards, an efficient approach of Embedded Discrete Fracture <span class="hlt">Model</span> (EDFM) was applied to explicitly <span class="hlt">model</span> hydraulic and natural fractures in the reservoirs. Finally, three fracture geometries, i.e. non-planar hydraulic fractures, non-planar hydraulic fractures with one set natural fractures, and non-planar hydraulic fractures with two sets natural fractures, are evaluated. The multi-well performance with confined phase behavior is analyzed with permeabilities of 0.01 md and 0.1 md. This work improves the analysis of capillarity effect on multi-well performance with complex fracture geometries in tight oil reservoirs.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010MMTA...41.2337B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010MMTA...41.2337B"><span>Probing Reliability of Transport Phenomena <span class="hlt">Based</span> Heat Transfer and <span class="hlt">Fluid</span> Flow Analysis in Autogeneous Fusion Welding Process</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bag, S.; de, A.</p> <p>2010-09-01</p> <p>The transport phenomena <span class="hlt">based</span> heat transfer and <span class="hlt">fluid</span> flow calculations in weld pool require a number of input parameters. Arc efficiency, effective thermal conductivity, and viscosity in weld pool are some of these parameters, values of which are rarely known and difficult to assign a priori <span class="hlt">based</span> on the scientific principles alone. The present work reports a bi-directional three-dimensional (3-D) heat transfer and <span class="hlt">fluid</span> flow <span class="hlt">model</span>, which is integrated with a real number <span class="hlt">based</span> genetic algorithm. The bi-directional feature of the integrated <span class="hlt">model</span> allows the identification of the values of a required set of uncertain <span class="hlt">model</span> input parameters and, next, the design of process parameters to achieve a target weld pool dimension. The computed values are validated with measured results in linear gas-tungsten-arc (GTA) weld samples. Furthermore, a novel methodology to estimate the overall reliability of the computed solutions is also presented.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018OptFT..43...35S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018OptFT..43...35S"><span>Optical fiber F-P magnetic field sensor <span class="hlt">based</span> on magnetostrictive effect of magnetic <span class="hlt">fluid</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Shi, Fuquan; Luo, Yan; Che, Jiajia; Ren, Zhijun; peng, Baojin</p> <p>2018-07-01</p> <p>magnetic field sensor of air-gap Fabry-Perot fiber interferometersis proposed <span class="hlt">based</span> on magnetostrictive effect. The sensor is consisted of single-<span class="hlt">model</span> fiber (SMF), air-gap, no-core fiber (NCF) and magnetic <span class="hlt">fluid</span>. Those are sealed in the capillary, SMF and NCF are connect with air chamber and magnetic <span class="hlt">fluid</span> column. With the presence of an external magnetic field, air chamber cavity length changes because of the magneto-volume variation of magnetic <span class="hlt">fluids</span>. This situation causes a change in the optical path difference. Detection of the drift of interference spectrum leads to the detection of the change in magnetic field. When the magnetic field is parallel to the direction in which the capillary is placed, the sensitivity is 0.2347 nm/mT; when the magnetic <span class="hlt">fluid</span> is perpendicular to the direction in which the capillary is placed, the sensitivity is 0.325 nm/http://mT.%20In.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19990039171&hterms=firenze&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3Dfirenze','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19990039171&hterms=firenze&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3Dfirenze"><span>A Two-<span class="hlt">Fluid</span>, MHD Coronal <span class="hlt">Model</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Suess, S. T.; Wang, A.-H.; Wu, S. T.; Poletto, G.; McComas, D. J.</p> <p>1999-01-01</p> <p>We describe first results from a numerical two-<span class="hlt">fluid</span> MHD <span class="hlt">model</span> of the global structure of the solar Corona. The <span class="hlt">model</span> is two-<span class="hlt">fluid</span> in the sense that it accounts for the collisional energy exchange between protons and electrons. As in our single-<span class="hlt">fluid</span> <span class="hlt">model</span>, volumetric heat and Momentum sources are required to produce high speed wind from Corona] holes, low speed wind above streamers, and mass fluxes similar to the empirical solar wind. By specifying different proton and electron heating functions we obtain a high proton temperature in the coronal hole and a relatively low proton temperature above the streamer (in comparison with the electron temperature). This is consistent with inferences from SOHO/UltraViolet Coronagraph Spectrometer instrument (UVCS), and with the Ulysses/Solar Wind Observations Over the Poles of the Sun instrument (SWOOPS) proton and electron temperature measurements which we show from the fast latitude scan. The density in the coronal hole between 2 and 5 solar radii (2 and 5 R(sub S)) is similar to the density reported from SPARTAN 201.-01 measurements by Fisher and Guhathakurta [19941. The proton mass flux scaled to 1 AU is 2.4 x 10(exp 8)/sq cm s, which is consistent with Ulysses observations. Inside the closed field region, the density is sufficiently high so that the simulation gives equal proton and electron temperatures due to the high collision rate. In open field regions (in the coronal hole and above the streamer) the proton and electron temperatures differ by varying amounts. In the streamer the temperature and density are similar to those reported empirically by Li et al. [1998], and the plasma beta is larger than unity everywhere above approx. 1.5 R(sub S), as it is in all other MHD coronal streamer <span class="hlt">models</span> [e.g., Steinolfson et al., 1982; also G. A. Gary and D. Alexander, Constructing the coronal magnetic field, submitted to Solar Physics, 1998].</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017APS..DPPC11102C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017APS..DPPC11102C"><span>Nonlinear <span class="hlt">Fluid</span> <span class="hlt">Model</span> Of 3-D Field Effects In Tokamak Plasmas</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Callen, J. D.; Hegna, C. C.; Beidler, M. T.</p> <p>2017-10-01</p> <p>Extended MHD codes (e.g., NIMROD, M3D-C1) are beginning to explore nonlinear effects of small 3-D magnetic fields on tokamak plasmas. To facilitate development of analogous physically understandable reduced <span class="hlt">models</span>, a <span class="hlt">fluid-based</span> dynamic nonlinear <span class="hlt">model</span> of these added 3-D field effects in the <span class="hlt">base</span> axisymmetric tokamak magnetic field geometry is being developed. The <span class="hlt">model</span> incorporates kinetic-<span class="hlt">based</span> closures within an extended MHD framework. Key 3-D field effects <span class="hlt">models</span> that have been developed include: 1) a comprehensive modified Rutherford equation for the growth of a magnetic island that includes the classical tearing and NTM perturbed bootstrap current drives, externally applied magnetic field and current drives, and classical and neoclassical polarization current effects, and 2) dynamic nonlinear evolution of the plasma toroidal flow (radial electric field) in response to the 3-D fields. An application of this <span class="hlt">model</span> to RMP ELM suppression precipitated by an ELM crash will be discussed. Supported by Office of Fusion Energy Sciences, Office of Science, Dept. of Energy Grants DE-FG02-86ER53218 and DE-FG02-92ER54139.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/ADA073202','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA073202"><span>Respiratory Adaptations in Acid-<span class="hlt">base</span> Disturbances: Role of Cerebral <span class="hlt">Fluids</span>,</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>1979-06-19</p> <p>The respiratory and metabolic components of acid-<span class="hlt">base</span> homeostasis are defined. A quantitative empirical description of the (incomplete) mutual...literature. Respiratory adaptations in steady acid-<span class="hlt">base</span> disturbances of metabolic origin (hyperventilation with hypocapnia in primary metabolic acidosis, and...hypoventilation with hypercapnia in metabolic alkalosis ) are analyzed as a function of the acidity of the cerebral <span class="hlt">fluids</span> (cerebrospinal and cerebral interstitial <span class="hlt">fluid</span>). (Author)</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://cfpub.epa.gov/si/si_public_record_report.cfm?dirEntryId=340114&Lab=NRMRL&keyword=Sex&actType=&TIMSType=+&TIMSSubTypeID=&DEID=&epaNumber=&ntisID=&archiveStatus=Both&ombCat=Any&dateBeginCreated=&dateEndCreated=&dateBeginPublishedPresented=&dateEndPublishedPresented=&dateBeginUpdated=&dateEndUpdated=&dateBeginCompleted=&dateEndCompleted=&personID=&role=Any&journalID=&publisherID=&sortBy=revisionDate&count=50','EPA-EIMS'); return false;" href="https://cfpub.epa.gov/si/si_public_record_report.cfm?dirEntryId=340114&Lab=NRMRL&keyword=Sex&actType=&TIMSType=+&TIMSSubTypeID=&DEID=&epaNumber=&ntisID=&archiveStatus=Both&ombCat=Any&dateBeginCreated=&dateEndCreated=&dateBeginPublishedPresented=&dateEndPublishedPresented=&dateBeginUpdated=&dateEndUpdated=&dateBeginCompleted=&dateEndCompleted=&personID=&role=Any&journalID=&publisherID=&sortBy=revisionDate&count=50"><span>Research Summary 3-D Computational <span class="hlt">Fluid</span> Dynamics (CFD) <span class="hlt">Model</span> Of The Human Respiratory System</span></a></p> <p><a target="_blank" href="http://oaspub.epa.gov/eims/query.page">EPA Science Inventory</a></p> <p></p> <p></p> <p>The U.S. EPA’s Office of Research and Development (ORD) has developed a 3-D computational <span class="hlt">fluid</span> dynamics (CFD) <span class="hlt">model</span> of the human respiratory system that allows for the simulation of particulate <span class="hlt">based</span> contaminant deposition and clearance, while being adaptable for age, ethnicity,...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28505495','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28505495"><span>Generalized Boussinesq-Scriven surface <span class="hlt">fluid</span> <span class="hlt">model</span> with curvature dissipation for liquid surfaces and membranes.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Aguilar Gutierrez, Oscar F; Herrera Valencia, Edtson E; Rey, Alejandro D</p> <p>2017-10-01</p> <p>Curvature dissipation is relevant in synthetic and biological processes, from fluctuations in semi-flexible polymer solutions, to buckling of liquid columns, tomembrane cell wall functioning. We present a micromechanical <span class="hlt">model</span> of curvature dissipation relevant to <span class="hlt">fluid</span> membranes and liquid surfaces <span class="hlt">based</span> on a parallel surface parameterization and a stress constitutive equation appropriate for anisotropic <span class="hlt">fluids</span> and <span class="hlt">fluid</span> membranes.The derived <span class="hlt">model</span>, aimed at high curvature and high rate of change of curvature in liquid surfaces and membranes, introduces additional viscous modes not included in the widely used 2D Boussinesq-Scriven rheological constitutive equation for surface <span class="hlt">fluids</span>.The kinematic tensors that emerge from theparallel surface parameterization are the interfacial rate of deformation and the surface co-rotational Zaremba-Jaumann derivative of the curvature, which are used to classify all possibledissipative planar and non-planar modes. The curvature dissipation function that accounts for bending, torsion and twist rates is derived and analyzed under several constraints, including the important inextensional bending mode.A representative application of the curvature dissipation <span class="hlt">model</span> to the periodic oscillation in nano-wrinkled outer hair cells show how and why curvature dissipation decreases with frequency, and why the 100kHz frequency range is selected. These results contribute to characterize curvature dissipation in membranes and liquid surfaces. Copyright © 2017 Elsevier Inc. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/426963','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/426963"><span><span class="hlt">Modeling</span> interfacial area transport in multi-<span class="hlt">fluid</span> systems</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>Yarbro, Stephen Lee</p> <p>1996-11-01</p> <p>Many typical chemical engineering operations are multi-<span class="hlt">fluid</span> systems. They are carried out in distillation columns (vapor/liquid), liquid-liquid contactors (liquid/liquid) and other similar devices. An important parameter is interfacial area concentration, which determines the rate of interfluid heat, mass and momentum transfer and ultimately, the overall performance of the equipment. In many cases, the <span class="hlt">models</span> for determining interfacial area concentration are empirical and can only describe the cases for which there is experimental data. In an effort to understand multiphase reactors and the mixing process better, a multi-<span class="hlt">fluid</span> <span class="hlt">model</span> has been developed as part of a research effort to calculate interfacialmore » area transport in several different types of in-line static mixers. For this work, the ensemble-averaged property conservation equations have been derived for each <span class="hlt">fluid</span> and for the mixture. These equations were then combined to derive a transport equation for the interfacial area concentration. The final, one-dimensional <span class="hlt">model</span> was compared to interfacial area concentration data from two sizes of Kenics in-line mixer, two sizes of concurrent jet and a Tee mixer. In all cases, the calculated and experimental data compared well with the highest scatter being with the Tee mixer comparison.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018MS%26E..352a2025R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018MS%26E..352a2025R"><span>Graphene nanoplatelets as high-performance filtration control material in water-<span class="hlt">based</span> drilling <span class="hlt">fluids</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ridha, Syahrir; Ibrahim, Arif; Shahari, Radzi; Fonna, Syarizal</p> <p>2018-05-01</p> <p>The main objective of this work is to evaluate the effectiveness of graphene nanoplatelets (GNP) as filtration control materials in water <span class="hlt">based</span> drilling <span class="hlt">fluids</span>. Three (3) general samples of water <span class="hlt">based</span> drilling <span class="hlt">fluids</span> were prepared including basic potassium chloride (KCl) drilling <span class="hlt">fluids</span>, nanosilica (NS) drilling <span class="hlt">fluids</span> and GNP drilling <span class="hlt">fluids</span>. Several concentrations of NS and GNP were dispersed in controlled formulations of water <span class="hlt">based</span> drilling <span class="hlt">fluids</span>. Standard API filtration tests were carried out for comparison purposes as well as High Temperature High Pressure (HTHP) filtration tests at 150 °F (∼66 °C), 250 °F (∼121 °C) and 350 °F (∼177 °C) at a fixed 500 (∼3.45MPa) psi to study the filtration trend as a function of temperature. Mud cake samples from several tests were selectively chosen and analyzed under Field Emission Scanning Electron Microscope (FESEM) for its morphology. Results from this work show that nanoparticle concentrations play a factor in filtration ability of colloid materials in water <span class="hlt">based</span> drilling <span class="hlt">fluids</span> when studied at elevated temperature. Low temperature filtration, however, shows only small differences in volume in all the drilling <span class="hlt">fluid</span> samples. 0.1 ppb concentrations of GNP reduced the <span class="hlt">fluid</span> loss of 350 °F by 4.6 mL as compared to the similar concentration of NS drilling <span class="hlt">fluids</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1182648','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/1182648"><span>Fracture Propagation, <span class="hlt">Fluid</span> Flow, and Geomechanics of Water-<span class="hlt">Based</span> Hydraulic Fracturing in Shale Gas Systems and Electromagnetic Geophysical Monitoring of <span class="hlt">Fluid</span> Migration</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>Kim, Jihoon; Um, Evan; Moridis, George</p> <p>2014-12-01</p> <p>We investigate fracture propagation induced by hydraulic fracturing with water injection, using numerical simulation. For rigorous, full 3D <span class="hlt">modeling</span>, we employ a numerical method that can <span class="hlt">model</span> failure resulting from tensile and shear stresses, dynamic nonlinear permeability, leak-off in all directions, and thermo-poro-mechanical effects with the double porosity approach. Our numerical results indicate that fracture propagation is not the same as propagation of the water front, because fracturing is governed by geomechanics, whereas water saturation is determined by <span class="hlt">fluid</span> flow. At early times, the water saturation front is almost identical to the fracture tip, suggesting that the fracture is mostlymore » filled with injected water. However, at late times, advance of the water front is retarded compared to fracture propagation, yielding a significant gap between the water front and the fracture top, which is filled with reservoir gas. We also find considerable leak-off of water to the reservoir. The inconsistency between the fracture volume and the volume of injected water cannot properly calculate the fracture length, when it is estimated <span class="hlt">based</span> on the simple assumption that the fracture is fully saturated with injected water. As an example of flow-geomechanical responses, we identify pressure fluctuation under constant water injection, because hydraulic fracturing is itself a set of many failure processes, in which pressure consistently drops when failure occurs, but fluctuation decreases as the fracture length grows. We also study application of electromagnetic (EM) geophysical methods, because these methods are highly sensitive to changes in porosity and pore-<span class="hlt">fluid</span> properties due to water injection into gas reservoirs. Employing a 3D finite-element EM geophysical simulator, we evaluate the sensitivity of the crosswell EM method for monitoring <span class="hlt">fluid</span> movements in shaly reservoirs. For this sensitivity evaluation, reservoir <span class="hlt">models</span> are generated through the coupled</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..19.7255D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..19.7255D"><span><span class="hlt">Fluid</span>-rock geochemical interaction for <span class="hlt">modelling</span> calibration in geothermal exploration in Indonesia</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Deon, Fiorenza; Barnhoorn, Auke; Lievens, Caroline; Ryannugroho, Riskiray; Imaro, Tulus; Bruhn, David; van der Meer, Freek; Hutami, Rizki; Sibarani, Besteba; Sule, Rachmat; Saptadij, Nenny; Hecker, Christoph; Appelt, Oona; Wilke, Franziska</p> <p>2017-04-01</p> <p>Indonesia with its large, but partially unexplored geothermal potential is one of the most interesting and suitable places in the world to conduct geothermal exploration research. This study focuses on geothermal exploration <span class="hlt">based</span> on <span class="hlt">fluid</span>-rock geochemistry/geomechanics and aims to compile an overview on geochemical data-rock properties from important geothermal fields in Indonesia. The research carried out in the field and in the laboratory is performed in the framework of the GEOCAP cooperation (Geothermal Capacity Building program Indonesia- the Netherlands). The application of petrology and geochemistry accounts to a better understanding of areas where operating power plants exist but also helps in the initial exploration stage of green areas. Because of their relevance and geological setting geothermal fields in Java, Sulawesi and the sedimentary basin of central Sumatra have been chosen as focus areas of this study. Operators, universities and governmental agencies will benefit from this approach as it will be applied also to new green-field terrains. By comparing the characteristic of the <span class="hlt">fluids</span>, the alteration petrology and the rock geochemistry we also aim to contribute to compile an overview of the geochemistry of the important geothermal fields in Indonesia. At the same time the rock petrology and <span class="hlt">fluid</span> geochemistry will be used as input data to <span class="hlt">model</span> the reservoir <span class="hlt">fluid</span> composition along with T-P parameters with the geochemical workbench PHREEQC. The field and laboratory data are mandatory for both the implementation and validation of the <span class="hlt">model</span> results.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013SPIE.8661E..0TT','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013SPIE.8661E..0TT"><span>An incompressible <span class="hlt">fluid</span> flow <span class="hlt">model</span> with mutual information for MR image registration</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Tsai, Leo; Chang, Herng-Hua</p> <p>2013-03-01</p> <p>Image registration is one of the fundamental and essential tasks within image processing. It is a process of determining the correspondence between structures in two images, which are called the template image and the reference image, respectively. The challenge of registration is to find an optimal geometric transformation between corresponding image data. This paper develops a new MR image registration algorithm that uses a closed incompressible viscous <span class="hlt">fluid</span> <span class="hlt">model</span> associated with mutual information. In our approach, we treat the image pixels as the <span class="hlt">fluid</span> elements of a viscous <span class="hlt">fluid</span> flow governed by the nonlinear Navier-Stokes partial differential equation (PDE). We replace the pressure term with the body force mainly used to guide the transformation with a weighting coefficient, which is expressed by the mutual information between the template and reference images. To solve this modified Navier-Stokes PDE, we adopted the fast numerical techniques proposed by Seibold1. The registration process of updating the body force, the velocity and deformation fields is repeated until the mutual information weight reaches a prescribed threshold. We applied our approach to the BrainWeb and real MR images. As consistent with the theory of the proposed <span class="hlt">fluid</span> <span class="hlt">model</span>, we found that our method accurately transformed the template images into the reference images <span class="hlt">based</span> on the intensity flow. Experimental results indicate that our method is of potential in a wide variety of medical image registration applications.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5615715','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5615715"><span>Cellulose-<span class="hlt">Based</span> Smart <span class="hlt">Fluids</span> under Applied Electric Fields</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Choi, Kisuk; Gao, Chun Yan; Nam, Jae Do</p> <p>2017-01-01</p> <p>Cellulose particles, their derivatives and composites have special environmentally benign features and are abundant in nature with their various applications. This review paper introduces the essential properties of several types of cellulose and their derivatives obtained from various source materials, and their use in electro-responsive electrorheological (ER) suspensions, which are smart <span class="hlt">fluid</span> systems that are actively responsive under applied electric fields, while, at zero electric field, ER <span class="hlt">fluids</span> retain a liquid-like state. Given the actively controllable characteristics of cellulose-<span class="hlt">based</span> smart ER <span class="hlt">fluids</span> under an applied electric field regarding their rheological and dielectric properties, they can potentially be applied for various industrial devices including dampers and haptic devices. PMID:28891966</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_10");'>10</a></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li class="active"><span>12</span></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_12 --> <div id="page_13" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li class="active"><span>13</span></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="241"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20000053850&hterms=medical+family&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D90%26Ntt%3Dmedical%2Bfamily','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20000053850&hterms=medical+family&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D90%26Ntt%3Dmedical%2Bfamily"><span>Electrorheological <span class="hlt">Fluid</span> <span class="hlt">Based</span> Force Feedback Device</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Pfeiffer, Charles; Bar-Cohen, Yoseph; Mavroidis, Constantinos; Dolgin, Benjamin</p> <p>1999-01-01</p> <p>Parallel to the efforts to develop fully autonomous robots, it is increasingly being realized that there are applications where it is essential to have a fully controlled robot and "feel" its operating conditions, i.e. telepresence. This trend is a result of the increasing efforts to address tasks where humans can perform significantly better but, due to associated hazards, distance, physical limitations and other causes, only robots can be employed to perform these tasks. Such robots need to be assisted by a human that remotely controls the operation. To address the goal of operating robots as human surrogates, the authors launched a study of mechanisms that provide mechanical feedback. For this purpose, electrorheological <span class="hlt">fluids</span> (ERF) are being investigated for the potential application as miniature haptic devices. This family of electroactive <span class="hlt">fluids</span> has the property of changing the viscosity during electrical stimulation. Consequently, ERF can be used to produce force feedback haptic devices for tele-operated control of medical and space robotic systems. Forces applied at the robot end-effector due to a compliant environment are reflected to the user using an ERF device where a change in the system viscosity will occur proportionally to the transmitted force. Analytical <span class="hlt">model</span> and control algorithms are being developed taking into account the non-linearities of these type of devices. This paper will describe the concept and the developed mechanism of ERF <span class="hlt">based</span> force feedback. The test process and the physical properties of this device will be described and the results of preliminary tests will be presented.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27617710','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27617710"><span>A Poroelastic <span class="hlt">Fluid</span>/Structure-Interaction <span class="hlt">Model</span> of Cerebrospinal <span class="hlt">Fluid</span> Dynamics in the Cord With Syringomyelia and Adjacent Subarachnoid-Space Stenosis.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Bertram, C D; Heil, M</p> <p>2017-01-01</p> <p>An existing axisymmetric <span class="hlt">fluid</span>/structure-interaction (FSI) <span class="hlt">model</span> of the spinal cord, pia mater, subarachnoid space, and dura mater in the presence of syringomyelia and subarachnoid-space stenosis was modified to include porous solids. This allowed investigation of a hypothesis for syrinx <span class="hlt">fluid</span> ingress from cerebrospinal <span class="hlt">fluid</span> (CSF). Gross <span class="hlt">model</span> deformation was unchanged by the addition of porosity, but pressure oscillated more in the syrinx and the subarachnoid space below the stenosis. The poroelastic <span class="hlt">model</span> still exhibited elevated mean pressure in the subarachnoid space below the stenosis and in the syrinx. With realistic cord permeability, there was slight oscillatory shunt flow bypassing the stenosis via the porous tissue over the syrinx. Weak steady streaming flow occurred in a circuit involving craniocaudal flow through the stenosis and back via the syrinx. Mean syrinx volume was scarcely altered when the adjacent stenosis bisected the syrinx, but increased slightly when the syrinx was predominantly located caudal to the stenosis. The <span class="hlt">fluid</span> content of the tissues over the syrinx oscillated, absorbing most of the radial flow seeping from the subarachnoid space so that it did not reach the syrinx. To a lesser extent, this cyclic swelling in a boundary layer of cord tissue just below the pia occurred all along the cord, representing a mechanism for exchange of interstitial <span class="hlt">fluid</span> (ISF) and cerebrospinal <span class="hlt">fluid</span> which could explain recent tracer findings without invoking perivascular conduits. The <span class="hlt">model</span> demonstrates that syrinx volume increase is possible when there is subarachnoid-space stenosis and the cord and pia are permeable.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20080022310&hterms=Ansys+CFX&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3DAnsys%2BCFX','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20080022310&hterms=Ansys+CFX&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3DAnsys%2BCFX"><span>A Correlation-<span class="hlt">Based</span> Transition <span class="hlt">Model</span> using Local Variables. Part 1; <span class="hlt">Model</span> Formation</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Menter, F. R.; Langtry, R. B.; Likki, S. R.; Suzen, Y. B.; Huang, P. G.; Volker, S.</p> <p>2006-01-01</p> <p>A new correlation-<span class="hlt">based</span> transition <span class="hlt">model</span> has been developed, which is <span class="hlt">based</span> strictly on local variables. As a result, the transition <span class="hlt">model</span> is compatible with modern computational <span class="hlt">fluid</span> dynamics (CFD) approaches, such as unstructured grids and massive parallel execution. The <span class="hlt">model</span> is <span class="hlt">based</span> on two transport equations, one for intermittency and one for the transition onset criteria in terms of momentum thickness Reynolds number. The proposed transport equations do not attempt to <span class="hlt">model</span> the physics of the transition process (unlike, e.g., turbulence <span class="hlt">models</span>) but from a framework for the implementation of correlation-<span class="hlt">based</span> <span class="hlt">models</span> into general-purpose CFD methods.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28917579','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28917579"><span>Microcirculation in the murine liver: a computational <span class="hlt">fluid</span> dynamic <span class="hlt">model</span> <span class="hlt">based</span> on 3D reconstruction from in vivo microscopy.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Piergiovanni, Monica; Bianchi, Elena; Capitani, Giada; Li Piani, Irene; Ganzer, Lucia; Guidotti, Luca G; Iannacone, Matteo; Dubini, Gabriele</p> <p>2017-10-03</p> <p>The liver is organized in hexagonal functional units - termed lobules - characterized by a rather peculiar blood microcirculation, due to the presence of a tangled network of capillaries - termed sinusoids. A better understanding of the hemodynamics that governs liver microcirculation is relevant to clinical and biological studies aimed at improving our management of liver diseases and transplantation. Herein, we built a CFD <span class="hlt">model</span> of a 3D sinusoidal network, <span class="hlt">based</span> on in vivo images of a physiological mouse liver obtained with a 2-photon microscope. The CFD <span class="hlt">model</span> was developed with Fluent 16.0 (ANSYS Inc., Canonsburg, PA), particular care was taken in imposing the correct boundary conditions representing a physiological state. To account for the remaining branches of the sinusoids, a lumped parameter <span class="hlt">model</span> was used to prescribe the correct pressure at each outlet. The effect of an adhered cell on local hemodynamics is also investigated for different occlusion degrees. The <span class="hlt">model</span> here proposed accurately reproduces the <span class="hlt">fluid</span> dynamics in a portion of the sinusoidal network in mouse liver. Mean velocities and mass flow rates are in agreement with literature values from in vivo measurements. Our approach provides details on local phenomena, hardly described by other computational studies, either focused on the macroscopic hepatic vasculature or <span class="hlt">based</span> on homogeneous porous medium <span class="hlt">model</span>. Copyright © 2017 Elsevier Ltd. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/23988650','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/23988650"><span>[<span class="hlt">Fluid</span> therapy in acute pancreatitis].</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>de-Madaria, Enrique</p> <p>2013-12-01</p> <p>Severe acute pancreatitis (AP) is associated with an increased need for <span class="hlt">fluids</span> due to <span class="hlt">fluid</span> sequestration and, in the most severe cases, with decreased peripheral vascular tone. For several decades, clinical practice guidelines have recommended aggressive <span class="hlt">fluid</span> therapy to improve the prognosis of AP. This recommendation is <span class="hlt">based</span> on theoretical <span class="hlt">models</span>, animal studies, and retrospective studies in humans. Recent studies suggest that aggressive <span class="hlt">fluid</span> administration in all patients with AP could have a neutral or harmful effect. <span class="hlt">Fluid</span> therapy <span class="hlt">based</span> on Ringer's lactate could improve the course of the disease, although further studies are needed to confirm this possibility. Most patients with AP do not require invasive monitoring of hemodynamic parameters to guide <span class="hlt">fluid</span> therapy administration. Moreover, the ability of these parameters to improve prognosis has not been demonstrated. Copyright © 2013 Elsevier España, S.L. and AEEH y AEG. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EPJP..132..388T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EPJP..132..388T"><span>Two <span class="hlt">fluid</span> anisotropic dark energy <span class="hlt">models</span> in a scale invariant theory</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Tripathy, S. K.; Mishra, B.; Sahoo, P. K.</p> <p>2017-09-01</p> <p>Some anisotropic Bianchi V dark energy <span class="hlt">models</span> are investigated in a scale invariant theory of gravity. We consider two non-interacting <span class="hlt">fluids</span> such as dark energy and a bulk viscous <span class="hlt">fluid</span>. Dark energy pressure is considered to be anisotropic in different spatial directions. A dynamically evolving pressure anisotropy is obtained from the <span class="hlt">models</span>. The <span class="hlt">models</span> favour phantom behaviour. It is observed that, in presence of dark energy, bulk viscosity has no appreciable effect on the cosmic dynamics.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19770021888','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19770021888"><span><span class="hlt">FLUID</span>: A numerical interpolation procedure for obtaining thermodynamic and transport properties of <span class="hlt">fluids</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Fessler, T. E.</p> <p>1977-01-01</p> <p>A computer program subroutine, <span class="hlt">FLUID</span>, was developed to calculate thermodynamic and transport properties of pure <span class="hlt">fluid</span> substances. It provides for determining the thermodynamic state from assigned values for temperature-density, pressure-density, temperature-pressure, pressure-entropy, or pressure-enthalpy. Liquid or two-phase (liquid-gas) conditions are considered as well as the gas phase. A van der Waals <span class="hlt">model</span> is used to obtain approximate state values; these values are then corrected for real gas effects by <span class="hlt">model</span>-correction factors obtained from tables <span class="hlt">based</span> on experimental data. Saturation conditions, specific heat, entropy, and enthalpy data are included in the tables for each gas. Since these tables are external to the <span class="hlt">FLUID</span> subroutine itself, <span class="hlt">FLUID</span> can implement any gas for which a set of tables has been generated. (A setup phase is used to establish pointers dynamically to the tables for a specific gas.) Data-table preparation is described. <span class="hlt">FLUID</span> is available in both SFTRAN and FORTRAN</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017HMT....53..305S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017HMT....53..305S"><span>Novel <span class="hlt">models</span> on <span class="hlt">fluid</span>'s variable thermo-physical properties for extensive study on convection heat and mass transfer</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Shang, De-Yi; Zhong, Liang-Cai</p> <p>2017-01-01</p> <p>Our novel <span class="hlt">models</span> for <span class="hlt">fluid</span>'s variable physical properties are improved and reported systematically in this work for enhancement of theoretical and practical value on study of convection heat and mass transfer. It consists of three <span class="hlt">models</span>, namely (1) temperature parameter <span class="hlt">model</span>, (2) polynomial <span class="hlt">model</span>, and (3) weighted-sum <span class="hlt">model</span>, respectively for treatment of temperature-dependent physical properties of gases, temperature-dependent physical properties of liquids, and concentration- and temperature-dependent physical properties of vapour-gas mixture. Two related components are proposed, and involved in each <span class="hlt">model</span> for <span class="hlt">fluid</span>'s variable physical properties. They are basic physic property equations and theoretical similarity equations on physical property factors. The former, as the foundation of the latter, is <span class="hlt">based</span> on the typical experimental data and physical analysis. The latter is built up by similarity analysis and mathematical derivation <span class="hlt">based</span> on the former basic physical properties equations. These <span class="hlt">models</span> are available for smooth simulation and treatment of <span class="hlt">fluid</span>'s variable physical properties for assurance of theoretical and practical value of study on convection of heat and mass transfer. Especially, so far, there has been lack of available study on heat and mass transfer of film condensation convection of vapour-gas mixture, and the wrong heat transfer results existed in widespread studies on the related research topics, due to ignorance of proper consideration of the concentration- and temperature-dependent physical properties of vapour-gas mixture. For resolving such difficult issues, the present novel physical property <span class="hlt">models</span> have their special advantages.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/10960542','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/10960542"><span>Simulation <span class="hlt">model</span> <span class="hlt">based</span> on non-newtonian <span class="hlt">fluid</span> mechanics applied to the evaluation of the embolic effect of emulsions of iodized oil and anticancer drug.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Demachi, H; Matsui, O; Abo, H; Tatsu, H</p> <p>2000-01-01</p> <p>To verify the difference in embolic effect between oil-in-water (O-W) and water-in-oil (W-O) emulsions composed of iodized oil and an anticancer drug, epirubicin, using a simulation <span class="hlt">model</span> <span class="hlt">based</span> on non-Newtonian <span class="hlt">fluid</span> mechanics. Flow curves of pure iodized oil and two types of O-W and W-O emulsions immediately and 1 hr after preparation were examined with a viscometer. Using the yield stress data obtained, we simulated the stagnation of each <span class="hlt">fluid</span> with steady flow in a rigid tube. The W-O emulsions were observed to stagnate in the thin tube at a low pressure gradient. However, the embolic effect of the W-O emulsions decreased 1 hr after preparation. The O-W emulsions were stable and did not stagnate under the conditions in which the W-O emulsions stagnated. The simulation <span class="hlt">model</span> showed that the embolic effect of the W-O emulsions was superior to that of the O-W emulsions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2005JAP....97jQ917S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2005JAP....97jQ917S"><span>Preparation and electrical properties of oil-<span class="hlt">based</span> magnetic <span class="hlt">fluids</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sartoratto, P. P. C.; Neto, A. V. S.; Lima, E. C. D.; Rodrigues de Sá, A. L. C.; Morais, P. C.</p> <p>2005-05-01</p> <p>This paper describes an improvement in the preparation of magnetic <span class="hlt">fluids</span> for electrical transformers. The samples are <span class="hlt">based</span> on surface-coated maghemite nanoparticles dispersed in transformer insulating oil. Colloidal stability at 90°C was higher for oleate-grafted maghemite-<span class="hlt">based</span> magnetic <span class="hlt">fluid</span>, whereas decanoate and dodecanoate-grafted samples were very unstable. Electrical properties were evaluated for samples containing 0.80%-0.0040% maghemite volume fractions. Relative permittivity varied from 8.8 to 2.1 and the minimum value of the loss factor was 12% for the most diluted sample. The resistivity falls in the range of 0.7-2.5×1010Ωm, whereas the ac dielectric strength varied from 70to79kV. These physical characteristics reveal remarkable step forward in the properties of the magnetic <span class="hlt">fluid</span> samples and may result in better operation of electrical transformers.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3217637','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3217637"><span>Lateral <span class="hlt">Fluid</span> Percussion: <span class="hlt">Model</span> of Traumatic Brain Injury in Mice</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Alder, Janet; Fujioka, Wendy; Lifshitz, Jonathan; Crockett, David P.; Thakker-Varia, Smita</p> <p>2011-01-01</p> <p>Traumatic brain injury (TBI) research has attained renewed momentum due to the increasing awareness of head injuries, which result in morbidity and mortality. <span class="hlt">Based</span> on the nature of primary injury following TBI, complex and heterogeneous secondary consequences result, which are followed by regenerative processes 1,2. Primary injury can be induced by a direct contusion to the brain from skull fracture or from shearing and stretching of tissue causing displacement of brain due to movement 3,4. The resulting hematomas and lacerations cause a vascular response 3,5, and the morphological and functional damage of the white matter leads to diffuse axonal injury 6-8. Additional secondary changes commonly seen in the brain are edema and increased intracranial pressure 9. Following TBI there are microscopic alterations in biochemical and physiological pathways involving the release of excitotoxic neurotransmitters, immune mediators and oxygen radicals 10-12, which ultimately result in long-term neurological disabilities 13,14. Thus choosing appropriate animal <span class="hlt">models</span> of TBI that present similar cellular and molecular events in human and rodent TBI is critical for studying the mechanisms underlying injury and repair. Various experimental <span class="hlt">models</span> of TBI have been developed to reproduce aspects of TBI observed in humans, among them three specific <span class="hlt">models</span> are widely adapted for rodents: <span class="hlt">fluid</span> percussion, cortical impact and weight drop/impact acceleration 1. The <span class="hlt">fluid</span> percussion device produces an injury through a craniectomy by applying a brief <span class="hlt">fluid</span> pressure pulse on to the intact dura. The pulse is created by a pendulum striking the piston of a reservoir of <span class="hlt">fluid</span>. The percussion produces brief displacement and deformation of neural tissue 1,15. Conversely, cortical impact injury delivers mechanical energy to the intact dura via a rigid impactor under pneumatic pressure 16,17. The weight drop/impact <span class="hlt">model</span> is characterized by the fall of a rod with a specific mass on the closed</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/21876530','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/21876530"><span>Lateral <span class="hlt">fluid</span> percussion: <span class="hlt">model</span> of traumatic brain injury in mice.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Alder, Janet; Fujioka, Wendy; Lifshitz, Jonathan; Crockett, David P; Thakker-Varia, Smita</p> <p>2011-08-22</p> <p>Traumatic brain injury (TBI) research has attained renewed momentum due to the increasing awareness of head injuries, which result in morbidity and mortality. <span class="hlt">Based</span> on the nature of primary injury following TBI, complex and heterogeneous secondary consequences result, which are followed by regenerative processes (1,2). Primary injury can be induced by a direct contusion to the brain from skull fracture or from shearing and stretching of tissue causing displacement of brain due to movement (3,4). The resulting hematomas and lacerations cause a vascular response (3,5), and the morphological and functional damage of the white matter leads to diffuse axonal injury (6-8). Additional secondary changes commonly seen in the brain are edema and increased intracranial pressure (9). Following TBI there are microscopic alterations in biochemical and physiological pathways involving the release of excitotoxic neurotransmitters, immune mediators and oxygen radicals (10-12), which ultimately result in long-term neurological disabilities (13,14). Thus choosing appropriate animal <span class="hlt">models</span> of TBI that present similar cellular and molecular events in human and rodent TBI is critical for studying the mechanisms underlying injury and repair. Various experimental <span class="hlt">models</span> of TBI have been developed to reproduce aspects of TBI observed in humans, among them three specific <span class="hlt">models</span> are widely adapted for rodents: <span class="hlt">fluid</span> percussion, cortical impact and weight drop/impact acceleration (1). The <span class="hlt">fluid</span> percussion device produces an injury through a craniectomy by applying a brief <span class="hlt">fluid</span> pressure pulse on to the intact dura. The pulse is created by a pendulum striking the piston of a reservoir of <span class="hlt">fluid</span>. The percussion produces brief displacement and deformation of neural tissue (1,15). Conversely, cortical impact injury delivers mechanical energy to the intact dura via a rigid impactor under pneumatic pressure (16,17). The weight drop/impact <span class="hlt">model</span> is characterized by the fall of a rod with a specific</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.V31C0519B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.V31C0519B"><span><span class="hlt">Modelling</span> Laccoliths: <span class="hlt">Fluid</span>-Driven Fracturing in the Lab</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ball, T. V.; Neufeld, J. A.</p> <p>2017-12-01</p> <p>Current <span class="hlt">modelling</span> of the formation of laccoliths neglects the necessity to fracture rock layers for propagation to occur [1]. In magmatic intrusions at depth the idea of fracture toughness is used to characterise fracturing, however an analogue for near surface intrusions has yet to be explored [2]. We propose an analytical <span class="hlt">model</span> for laccolith emplacement that accounts for the energy required to fracture at the tip of an intrusion. For realistic physical parameters we find that a lag region exists between the <span class="hlt">fluid</span> magma front and the crack tip where large negative pressures in the tip cause volatiles to exsolve from the magma. Crucially, the dynamics of this tip region controls the spreading due to the competition between viscous forces and fracture energy. We conduct a series of complementary experiments to investigate <span class="hlt">fluid</span>-driven fracturing of adhered layers and confirm the existence of two regimes: viscosity dominant spreading, controlled by the pressure in the lag region, and fracture energy dominant spreading, controlled by the energy required to fracture layers. Our experiments provide the first observations, and evolution, of a vapour tip. These experiments and our simplified <span class="hlt">model</span> provide insight into the key physical processes in near surface magmatic intrusions with applications to <span class="hlt">fluid</span>-driven fracturing more generally. Michaut J. Geophys. Res. 116(B5), B05205. Bunger & Cruden J. Geophys. Res. 116(B2), B02203.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/111427','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/111427"><span>Analysis of two-phase flow inter-subchannel mass and momentum exchanges by the two-<span class="hlt">fluid</span> <span class="hlt">model</span> approach</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>Ninokata, H.; Deguchi, A.; Kawahara, A.</p> <p>1995-09-01</p> <p>A new void drift <span class="hlt">model</span> for the subchannel analysis method is presented for the thermohydraulics calculation of two-phase flows in rod bundles where the flow <span class="hlt">model</span> uses a two-<span class="hlt">fluid</span> formulation for the conservation of mass, momentum and energy. A void drift <span class="hlt">model</span> is constructed <span class="hlt">based</span> on the experimental data obtained in a geometrically simple inter-connected two circular channel test sections using air-water as working <span class="hlt">fluids</span>. The void drift force is assumed to be an origin of void drift velocity components of the two-phase cross-flow in a gap area between two adjacent rods and to overcome the momentum exchanges at themore » phase interface and wall-<span class="hlt">fluid</span> interface. This void drift force is implemented in the cross flow momentum equations. Computational results have been successfully compared to experimental data available including 3x3 rod bundle data.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27289474','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27289474"><span>A revised <span class="hlt">model</span> of <span class="hlt">fluid</span> transport optimization in Physarum polycephalum.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Bonifaci, Vincenzo</p> <p>2017-02-01</p> <p>Optimization of <span class="hlt">fluid</span> transport in the slime mold Physarum polycephalum has been the subject of several <span class="hlt">modeling</span> efforts in recent literature. Existing <span class="hlt">models</span> assume that the tube adaptation mechanism in P. polycephalum's tubular network is controlled by the sheer amount of <span class="hlt">fluid</span> flow through the tubes. We put forward the hypothesis that the controlling variable may instead be the flow's pressure gradient along the tube. We carry out the stability analysis of such a revised mathematical <span class="hlt">model</span> for a parallel-edge network, proving that the revised <span class="hlt">model</span> supports the global flow-optimizing behavior of the slime mold for a substantially wider class of response functions compared to previous <span class="hlt">models</span>. Simulations also suggest that the same conclusion may be valid for arbitrary network topologies.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JCoPh.357..159S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JCoPh.357..159S"><span>A numerical <span class="hlt">model</span> of two-phase flow at the micro-scale using the volume-of-<span class="hlt">fluid</span> method</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Shams, Mosayeb; Raeini, Ali Q.; Blunt, Martin J.; Bijeljic, Branko</p> <p>2018-03-01</p> <p>This study presents a simple and robust numerical scheme to <span class="hlt">model</span> two-phase flow in porous media where capillary forces dominate over viscous effects. The volume-of-<span class="hlt">fluid</span> method is employed to capture the <span class="hlt">fluid-fluid</span> interface whose dynamics is explicitly described <span class="hlt">based</span> on a finite volume discretization of the Navier-Stokes equations. Interfacial forces are calculated directly on reconstructed interface elements such that the total curvature is preserved. The computed interfacial forces are explicitly added to the Navier-Stokes equations using a sharp formulation which effectively eliminates spurious currents. The stability and accuracy of the implemented scheme is validated on several two- and three-dimensional test cases, which indicate the capability of the method to <span class="hlt">model</span> two-phase flow processes at the micro-scale. In particular we show how the co-current flow of two viscous <span class="hlt">fluids</span> leads to greatly enhanced flow conductance for the wetting phase in corners of the pore space, compared to a case where the non-wetting phase is an inviscid gas.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011AGUFM.H34B..01M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011AGUFM.H34B..01M"><span><span class="hlt">Modeling</span> Coupled Processes for Multiphase <span class="hlt">Fluid</span> Flow in Mechanically Deforming Faults</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>McKenna, S. A.; Pike, D. Q.</p> <p>2011-12-01</p> <p><span class="hlt">Modeling</span> of coupled hydrological-mechanical processes in fault zones is critical for understanding the long-term behavior of <span class="hlt">fluids</span> within the shallow crust. Here we utilize a previously developed cellular-automata (CA) <span class="hlt">model</span> to define the evolution of permeability within a 2-D fault zone under compressive stress. At each time step, the CA <span class="hlt">model</span> calculates the increase in <span class="hlt">fluid</span> pressure within the fault at every grid cell. Pressure surpassing a critical threshold (e.g., lithostatic stress) causes a rupture in that cell, and pressure is then redistributed across the neighboring cells. The rupture can cascade through the spatial domain and continue across multiple time steps. Stress continues to increase and the size and location of rupture events are recorded until a percolating backbone of ruptured cells exists across the fault. Previous applications of this <span class="hlt">model</span> consider uncorrelated random fields for the compressibility of the fault material. The prior focus on uncorrelated property fields is consistent with development of a number of statistical physics <span class="hlt">models</span> including percolation processes and fracture propagation. However, geologic materials typically express spatial correlation and this can have a significant impact on the results of the pressure and permeability distributions. We <span class="hlt">model</span> correlation of the fault material compressibility as a multiGaussian random field with a correlation length defined as the full-width at half maximum (FWHM) of the kernel used to create the field. The FWHM is varied from < 0.001 to approximately 0.47 of the domain size. The addition of spatial correlation to the compressibility significantly alters the <span class="hlt">model</span> results including: 1) Accumulation of larger amounts of strain prior to the first rupture event; 2) Initiation of the percolating backbone at lower amounts of cumulative strain; 3) Changes in the event size distribution to a combined power-law and exponential distribution with a smaller power; and 4) Evolution of the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018E%26ES..113a2138X','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018E%26ES..113a2138X"><span>Study on <span class="hlt">Fluid</span>-solid Coupling Mathematical <span class="hlt">Models</span> and Numerical Simulation of Coal Containing Gas</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Xu, Gang; Hao, Meng; Jin, Hongwei</p> <p>2018-02-01</p> <p><span class="hlt">Based</span> on coal seam gas migration theory under multi-physics field coupling effect, <span class="hlt">fluid</span>-solid coupling <span class="hlt">model</span> of coal seam gas was build using elastic mechanics, <span class="hlt">fluid</span> mechanics in porous medium and effective stress principle. Gas seepage behavior under different original gas pressure was simulated. Results indicated that residual gas pressure, gas pressure gradient and gas low were bigger when original gas pressure was higher. Coal permeability distribution decreased exponentially when original gas pressure was lower than critical pressure. Coal permeability decreased rapidly first and then increased slowly when original pressure was higher than critical pressure.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AIPC.1877i0001A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AIPC.1877i0001A"><span>Experimental determination of nanofluid specific heat with SiO2 nanoparticles in different <span class="hlt">base</span> <span class="hlt">fluids</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Akilu, S.; Baheta, A. T.; Sharma, K. V.; Said, M. A.</p> <p>2017-09-01</p> <p>Nanostructured ceramic materials have recently attracted attention as promising heat transfer <span class="hlt">fluid</span> additives owing to their outstanding heat storage capacities. In this paper, experimental measurements of the specific heats of SiO2-Glycerol, SiO2-Ethylene Glycol, and SiO2-Glycerol/Ethylene Glycol mixture 60:40 ratio (by mass) nanofluids with different volume concentrations of 1.0-4.0% have been carried out using differential scanning calorimeter at temperatures of 25 °C and 50 °C. Experimental results indicate lower specific heat capacities are found with SiO2 nanofluids compared to their respective <span class="hlt">base</span> <span class="hlt">fluids</span>. The specific heat was decreasing with the increase of concentration, and this decrement depends on upon the type of the <span class="hlt">base</span> <span class="hlt">fluid</span>. It is observed that temperature has a positive impact on the specific heat capacity. Furthermore, the experimental values were compared with the theoretical <span class="hlt">model</span> predictions, and a satisfactory agreement was established.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013SPIE.8688E..19A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013SPIE.8688E..19A"><span>A magneto-rheological <span class="hlt">fluid-based</span> torque sensor for smart torque wrench application</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ahmadkhanlou, Farzad; Washington, Gregory N.</p> <p>2013-04-01</p> <p>In this paper, the authors have developed a new application where MR <span class="hlt">fluid</span> is being used as a sensor. An MR-<span class="hlt">fluid</span> <span class="hlt">based</span> torque wrench has been developed with a rotary MR <span class="hlt">fluid-based</span> damper. The desired set torque ranges from 1 to 6 N.m. Having continuously controllable yield strength, the MR <span class="hlt">fluid-based</span> torque wrench presents a great advantage over the regular available torque wrenches in the market. This design is capable of providing continuous set toque from the lower limit to the upper limit while regular torque wrenches provide discrete set torques only at some limited points. This feature will be especially important in high fidelity systems where tightening torque is very critical and the tolerances are low.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li class="active"><span>13</span></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_13 --> <div id="page_14" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li class="active"><span>14</span></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="261"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/19964526','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/19964526"><span>Deriving a blood-mimicking <span class="hlt">fluid</span> for particle image velocimetry in Sylgard-184 vascular <span class="hlt">models</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Yousif, Majid Y; Holdsworth, David W; Poepping, Tamie L</p> <p>2009-01-01</p> <p>A new blood-mimicking <span class="hlt">fluid</span> (BMF) has been developed for particle image velocimetry (PIV), which enables flow studies in vascular <span class="hlt">models</span> (phantoms). A major difficulty in PIV that affects measurement accuracy is the refraction and distortion of light passing through the interface between the <span class="hlt">model</span> and the <span class="hlt">fluid</span>, due to the difference in refractive index (n) between the two materials. The problem can be eliminated by using a <span class="hlt">fluid</span> with a refractive index matching that of the <span class="hlt">model</span>. Such <span class="hlt">fluids</span> are not commonly available, especially for vascular research where the <span class="hlt">fluid</span> should also have a viscosity similar to human blood. In this work, a blood-mimicking <span class="hlt">fluid</span>, composed of water (47.38% by weight), glycerol (36.94% by weight) and sodium iodide salt (15.68% by weight), was developed for compatibility with our silicone (Sylgard 184; n = 1.414) phantoms. The <span class="hlt">fluid</span> exhibits a dynamic viscosity of 4.31+/-0.03 cP which lies within the range of human blood viscosity (4.4+/-0.6 cP). Both refractive index and viscosity were attained at 22.2+/-0.2 degrees C, which is a feasible room temperature, thus eliminating the need for a temperature-control system. The <span class="hlt">fluid</span> will be used to study hemodynamics in vascular flow <span class="hlt">models</span> fabricated from Sylgard 184.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19790017551','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19790017551"><span>A simple <span class="hlt">model</span> of <span class="hlt">fluid</span> flow and electrolyte balance in the body</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>White, R. J.; Neal, L.</p> <p>1973-01-01</p> <p>The <span class="hlt">model</span> is basically a three-compartment <span class="hlt">model</span>, the three compartments being the plasma, interstitial <span class="hlt">fluid</span> and cellular <span class="hlt">fluid</span>. Sodium, potassium, chloride and urea are the only major solutes considered explicitly. The control of body water and electrolyte distribution is affected via drinking and hormone levels. Basically, the <span class="hlt">model</span> follows the effect of various oral input water loads on solute and water distribution throughout the body.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://cfpub.epa.gov/si/si_public_record_report.cfm?direntryid=319270&keyword=homeland%20security&subject=homeland%20security%20research&showcriteria=2&fed_org_id=111&datebeginpublishedpresented=02/19/2012&dateendpublishedpresented=02/19/2017&sortby=pubdateyear','PESTICIDES'); return false;" href="https://cfpub.epa.gov/si/si_public_record_report.cfm?direntryid=319270&keyword=homeland%20security&subject=homeland%20security%20research&showcriteria=2&fed_org_id=111&datebeginpublishedpresented=02/19/2012&dateendpublishedpresented=02/19/2017&sortby=pubdateyear"><span>Computational <span class="hlt">Fluid</span> Dynamics <span class="hlt">Modeling</span> of Bacillus anthracis ...</span></a></p> <p><a target="_blank" href="http://www.epa.gov/pesticides/search.htm">EPA Pesticide Factsheets</a></p> <p></p> <p></p> <p>Journal Article Three-dimensional computational <span class="hlt">fluid</span> dynamics and Lagrangian particle deposition <span class="hlt">models</span> were developed to compare the deposition of aerosolized Bacillus anthracis spores in the respiratory airways of a human with that of the rabbit, a species commonly used in the study of anthrax disease. The respiratory airway geometries for each species were derived from computed tomography (CT) or µCT images. Both <span class="hlt">models</span> encompassed airways that extended from the external nose to the lung with a total of 272 outlets in the human <span class="hlt">model</span> and 2878 outlets in the rabbit <span class="hlt">model</span>. All simulations of spore deposition were conducted under transient, inhalation-exhalation breathing conditions using average species-specific minute volumes. Four different exposure scenarios were <span class="hlt">modeled</span> in the rabbit <span class="hlt">based</span> upon experimental inhalation studies. For comparison, human simulations were conducted at the highest exposure concentration used during the rabbit experimental exposures. Results demonstrated that regional spore deposition patterns were sensitive to airway geometry and ventilation profiles. Despite the complex airway geometries in the rabbit nose, higher spore deposition efficiency was predicted in the upper conducting airways of the human at the same air concentration of anthrax spores. This greater deposition of spores in the upper airways in the human resulted in lower penetration and deposition in the tracheobronchial airways and the deep lung than that predict</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017APS..DFDL18009L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017APS..DFDL18009L"><span>Phase-resolved <span class="hlt">fluid</span> dynamic forces of a flapping foil energy harvester <span class="hlt">based</span> on PIV measurements</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Liburdy, James</p> <p>2017-11-01</p> <p>Two-dimensional particle image velocimetry measurements are performed in a wind tunnel to evaluate the spatial and temporal <span class="hlt">fluid</span> dynamic forces acting on a flapping foil operating in the energy harvesting regime. Experiments are conducted at reduced frequencies (k = fc/U) of 0.05 - 0.2, pitching angle of, and heaving amplitude of A / c = 0.6. The phase-averaged pressure field is obtained by integrating the pressure Poisson equation. <span class="hlt">Fluid</span> dynamic forces are then obtained through the integral momentum equation. Results are compared with a simple force <span class="hlt">model</span> <span class="hlt">based</span> on the concept of flow impulse. These results help to show the detailed force distributions, their transient nature and aide in understanding the impact of the <span class="hlt">fluid</span> flow structures that contribute to the power production.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28385882','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28385882"><span>Understanding Angiography-<span class="hlt">Based</span> Aneurysm Flow Fields through Comparison with Computational <span class="hlt">Fluid</span> Dynamics.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Cebral, J R; Mut, F; Chung, B J; Spelle, L; Moret, J; van Nijnatten, F; Ruijters, D</p> <p>2017-06-01</p> <p>Hemodynamics is thought to be an important factor for aneurysm progression and rupture. Our aim was to evaluate whether flow fields reconstructed from dynamic angiography data can be used to realistically represent the main flow structures in intracranial aneurysms. DSA-<span class="hlt">based</span> flow reconstructions, obtained during interventional treatment, were compared qualitatively with flow fields obtained from patient-specific computational <span class="hlt">fluid</span> dynamics <span class="hlt">models</span> and quantitatively with projections of the computational <span class="hlt">fluid</span> dynamics fields (by computing a directional similarity of the vector fields) in 15 cerebral aneurysms. The average similarity between the DSA and the projected computational <span class="hlt">fluid</span> dynamics flow fields was 78% in the parent artery, while it was only 30% in the aneurysm region. Qualitatively, both the DSA and projected computational <span class="hlt">fluid</span> dynamics flow fields captured the location of the inflow jet, the main vortex structure, the intrasaccular flow split, and the main rotation direction in approximately 60% of the cases. Several factors affect the reconstruction of 2D flow fields from dynamic angiography sequences. The most important factors are the 3-dimensionality of the intrasaccular flow patterns and inflow jets, the alignment of the main vortex structure with the line of sight, the overlapping of surrounding vessels, and possibly frame rate undersampling. Flow visualization with DSA from >1 projection is required for understanding of the 3D intrasaccular flow patterns. Although these DSA-<span class="hlt">based</span> flow quantification techniques do not capture swirling or secondary flows in the parent artery, they still provide a good representation of the mean axial flow and the corresponding flow rate. © 2017 by American Journal of Neuroradiology.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013MMTB...44..423G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013MMTB...44..423G"><span>Mathematical <span class="hlt">Modeling</span> of <span class="hlt">Fluid</span> Flow in a Water Physical <span class="hlt">Model</span> of an Aluminum Degassing Ladle Equipped with an Impeller-Injector</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Gómez, Eudoxio Ramos; Zenit, Roberto; Rivera, Carlos González; Trápaga, Gerardo; Ramírez-Argáez, Marco A.</p> <p>2013-04-01</p> <p>In this work, a 3D numerical simulation using a Euler-Euler-<span class="hlt">based</span> <span class="hlt">model</span> implemented into a commercial CFD code was used to simulate <span class="hlt">fluid</span> flow and turbulence structure in a water physical <span class="hlt">model</span> of an aluminum ladle equipped with an impeller for degassing treatment. The effect of critical process parameters such as rotor speed, gas flow rate, and the point of gas injection (conventional injection through the shaft vs a novel injection through the bottom of the ladle) on the <span class="hlt">fluid</span> flow and vortex formation was analyzed with this <span class="hlt">model</span>. The commercial CFD code PHOENICS 3.4 was used to solve all conservation equations governing the process for this two-phase <span class="hlt">fluid</span> flow system. The mathematical <span class="hlt">model</span> was reasonably well validated against experimentally measured liquid velocity and vortex sizes in a water physical <span class="hlt">model</span> built specifically for this investigation. From the results, it was concluded that the angular speed of the impeller is the most important parameter in promoting better stirred baths and creating smaller and better distributed bubbles in the liquid. The pumping effect of the impeller is increased as the impeller rotation speed increases. Gas flow rate is detrimental to bath stirring and diminishes the pumping effect of the impeller. Finally, although the injection point was the least significant variable, it was found that the "novel" injection improves stirring in the ladle.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014PhDT.......152C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014PhDT.......152C"><span>A mixed <span class="hlt">fluid</span>-kinetic solver for the Vlasov-Poisson equations</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Cheng, Yongtao</p> <p></p> <p>Plasmas are ionized gases that appear in a wide range of applications including astrophysics and space physics, as well as in laboratory settings such as in magnetically confined fusion. There are two prevailing types of <span class="hlt">modeling</span> strategies to describe a plasma system: kinetic <span class="hlt">models</span> and <span class="hlt">fluid</span> <span class="hlt">models</span>. Kinetic <span class="hlt">models</span> evolve particle probability density distributions (PDFs) in phase space, which are accurate but computationally expensive. <span class="hlt">Fluid</span> <span class="hlt">models</span> evolve a small number of moments of the distribution function and reduce the dimension of the solution. However, some approximation is necessary to close the system, and finding an accurate moment closure that correctly captures the dynamics away from thermodynamic equilibrium is a difficult and still open problem. The main contributions of the present work can be divided into two main parts: (1) a new class of moment closures, <span class="hlt">based</span> on a modification of existing quadrature-<span class="hlt">based</span> moment-closure methods, is developed using bi-B-spline and bi-bubble representations; and (2) a novel mixed solver that combines a <span class="hlt">fluid</span> and a kinetic solver is proposed, which uses the new class of moment-closure methods described in the first part. For the newly developed quadrature-<span class="hlt">based</span> moment-closure <span class="hlt">based</span> on bi-B-spline and bi-bubble representation, the explicit form of flux terms and the moment-realizability conditions are given. It is shown that while the bi-delta system is weakly hyperbolic, the newly proposed <span class="hlt">fluid</span> <span class="hlt">models</span> are strongly hyperbolic. Using a high-order Runge-Kutta discontinuous Galerkin method together with Strang operator splitting, the resulting <span class="hlt">models</span> are applied to the Vlasov-Poisson-Fokker-Planck system in the high field limit. In the second part of this work, results from kinetic solver are used to provide a corrected closure to the <span class="hlt">fluid</span> <span class="hlt">model</span>. This correction keeps the <span class="hlt">fluid</span> <span class="hlt">model</span> hyperbolic and gives <span class="hlt">fluid</span> results that match the moments as computed from the kinetic solution. Furthermore, a prolongation operation</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018SPIE10596E..1HQ','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018SPIE10596E..1HQ"><span>"Shape function + memory mechanism"-<span class="hlt">based</span> hysteresis <span class="hlt">modeling</span> of magnetorheological <span class="hlt">fluid</span> actuators</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Qian, Li-Jun; Chen, Peng; Cai, Fei-Long; Bai, Xian-Xu</p> <p>2018-03-01</p> <p>A hysteresis <span class="hlt">model</span> <span class="hlt">based</span> on "shape function + memory mechanism" is presented and its feasibility is verified through <span class="hlt">modeling</span> the hysteresis behavior of a magnetorheological (MR) damper. A hysteresis phenomenon in resistor-capacitor (RC) circuit is first presented and analyzed. In the hysteresis <span class="hlt">model</span>, the "memory mechanism" originating from the charging and discharging processes of the RC circuit is constructed by adopting a virtual displacement variable and updating laws for the reference points. The "shape function" is achieved and generalized from analytical solutions of the simple semi-linear Duhem <span class="hlt">model</span>. Using the approach, the memory mechanism reveals the essence of specific Duhem <span class="hlt">model</span> and the general shape function provides a direct and clear means to fit the hysteresis loop. In the frame of the structure of a "Restructured phenomenological <span class="hlt">model</span>", the original hysteresis operator, i.e., the Bouc-Wen operator, is replaced with the new hysteresis operator. The comparative work with the Bouc-Wen operator <span class="hlt">based</span> <span class="hlt">model</span> demonstrates superior performances of high computational efficiency and comparable accuracy of the new hysteresis operator-<span class="hlt">based</span> <span class="hlt">model</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20050181429','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20050181429"><span><span class="hlt">Fluids</span> and Combustion Facility: Combustion Integrated Rack Modal <span class="hlt">Model</span> Correlation</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>McNelis, Mark E.; Suarez, Vicente J.; Sullivan, Timothy L.; Otten, Kim D.; Akers, James C.</p> <p>2005-01-01</p> <p>The <span class="hlt">Fluids</span> and Combustion Facility (FCF) is a modular, multi-user, two-rack facility dedicated to combustion and <span class="hlt">fluids</span> science in the US Laboratory Destiny on the International Space Station. FCF is a permanent facility that is capable of accommodating up to ten combustion and <span class="hlt">fluid</span> science investigations per year. FCF research in combustion and <span class="hlt">fluid</span> science supports NASA's Exploration of Space Initiative for on-orbit fire suppression, fire safety, and space system <span class="hlt">fluids</span> management. The Combustion Integrated Rack (CIR) is one of two racks in the FCF. The CIR major structural elements include the International Standard Payload Rack (ISPR), Experiment Assembly (optics bench and combustion chamber), Air Thermal Control Unit (ATCU), Rack Door, and Lower Structure Assembly (Input/Output Processor and Electrical Power Control Unit). The load path through the rack structure is outlined. The CIR modal survey was conducted to validate the load path predicted by the CIR finite element <span class="hlt">model</span> (FEM). The modal survey is done by experimentally measuring the CIR frequencies and mode shapes. The CIR <span class="hlt">model</span> was test correlated by updating the <span class="hlt">model</span> to represent the test mode shapes. The correlated CIR <span class="hlt">model</span> delivery is required by NASA JSC at Launch-10.5 months. The test correlated CIR flight FEM is analytically integrated into the Shuttle for a coupled loads analysis of the launch configuration. The analysis frequency range of interest is 0-50 Hz. A coupled loads analysis is the analytical integration of the Shuttle with its cargo element, the Mini Payload Logistics Module (MPLM), in the Shuttle cargo bay. For each Shuttle launch configuration, a verification coupled loads analysis is performed to determine the loads in the cargo bay as part of the structural certification process.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017APS..DFD.E9004S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017APS..DFD.E9004S"><span>A <span class="hlt">Fluid</span> Structure Algorithm with Lagrange Multipliers to <span class="hlt">Model</span> Free Swimming</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sahin, Mehmet; Dilek, Ezgi</p> <p>2017-11-01</p> <p>A new monolithic approach is prosed to solve the <span class="hlt">fluid</span>-structure interaction (FSI) problem with Lagrange multipliers in order to <span class="hlt">model</span> free swimming/flying. In the present approach, the <span class="hlt">fluid</span> domain is <span class="hlt">modeled</span> by the incompressible Navier-Stokes equations and discretized using an Arbitrary Lagrangian-Eulerian (ALE) formulation <span class="hlt">based</span> on the stable side-centered unstructured finite volume method. The solid domain is <span class="hlt">modeled</span> by the constitutive laws for the nonlinear Saint Venant-Kirchhoff material and the classical Galerkin finite element method is used to discretize the governing equations in a Lagrangian frame. In order to impose the body motion/deformation, the distance between the constraint pair nodes is imposed using the Lagrange multipliers, which is independent from the frame of reference. The resulting algebraic linear equations are solved in a fully coupled manner using a dual approach (null space method). The present numerical algorithm is initially validated for the classical FSI benchmark problems and then applied to the free swimming of three linked ellipses. The authors are grateful for the use of the computing resources provided by the National Center for High Performance Computing (UYBHM) under Grant Number 10752009 and the computing facilities at TUBITAK-ULAKBIM, High Performance and Grid Computing Center.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2007JPhD...40.7046K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2007JPhD...40.7046K"><span>Computational <span class="hlt">modelling</span> of the flow of viscous <span class="hlt">fluids</span> in carbon nanotubes</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Khosravian, N.; Rafii-Tabar, H.</p> <p>2007-11-01</p> <p>Carbon nanotubes will have extensive application in all areas of nano-technology, and in particular in the field of nano-fluidics, wherein they can be used for molecular separation, nano-scale filtering and as nano-pipes for conveying <span class="hlt">fluids</span>. In the field of nano-medicine, nanotubes can be functionalized with various types of receptors to act as bio-sensors for the detection and elimination of cancer cells, or be used as bypasses and even neural connections. <span class="hlt">Modelling</span> <span class="hlt">fluid</span> flow inside nanotubes is a very challenging problem, since there is a complex interplay between the motion of the <span class="hlt">fluid</span> and the stability of the walls. A critical issue in the design of nano-fluidic devices is the induced vibration of the walls, due to the <span class="hlt">fluid</span> flow, which can promote structural instability. It has been established that the resonant frequencies depend on the flow velocity. We have studied, for the first time, the flow of viscous <span class="hlt">fluids</span> through multi-walled carbon nanotubes, using the Euler-Bernoulli classical beam theory to <span class="hlt">model</span> the nanotube as a continuum structure. Our aim has been to compute the effect of the <span class="hlt">fluid</span> flow on the structural stability of the nanotubes, without having to consider the details of the <span class="hlt">fluid</span>-walls interaction. The variations of the resonant frequencies with the flow velocity are obtained for both unembedded nanotubes, and when they are embedded in an elastic medium. It is found that a nanotube conveying a viscous <span class="hlt">fluid</span> is more stable against vibration-induced buckling than a nanotube conveying a non-viscous <span class="hlt">fluid</span>, and that the aspect ratio plays the same role in both cases.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26932024','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26932024"><span>Alternative <span class="hlt">modeling</span> methods for plasma-<span class="hlt">based</span> Rf ion sources.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Veitzer, Seth A; Kundrapu, Madhusudhan; Stoltz, Peter H; Beckwith, Kristian R C</p> <p>2016-02-01</p> <p>Rf-driven ion sources for accelerators and many industrial applications benefit from detailed numerical <span class="hlt">modeling</span> and simulation of plasma characteristics. For instance, <span class="hlt">modeling</span> of the Spallation Neutron Source (SNS) internal antenna H(-) source has indicated that a large plasma velocity is induced near bends in the antenna where structural failures are often observed. This could lead to improved designs and ion source performance <span class="hlt">based</span> on simulation and <span class="hlt">modeling</span>. However, there are significant separations of time and spatial scales inherent to Rf-driven plasma ion sources, which makes it difficult to <span class="hlt">model</span> ion sources with explicit, kinetic Particle-In-Cell (PIC) simulation codes. In particular, if both electron and ion motions are to be explicitly <span class="hlt">modeled</span>, then the simulation time step must be very small, and total simulation times must be large enough to capture the evolution of the plasma ions, as well as extending over many Rf periods. Additional physics processes such as plasma chemistry and surface effects such as secondary electron emission increase the computational requirements in such a way that even fully parallel explicit PIC <span class="hlt">models</span> cannot be used. One alternative method is to develop <span class="hlt">fluid-based</span> codes coupled with electromagnetics in order to <span class="hlt">model</span> ion sources. Time-domain <span class="hlt">fluid</span> <span class="hlt">models</span> can simulate plasma evolution, plasma chemistry, and surface physics <span class="hlt">models</span> with reasonable computational resources by not explicitly resolving electron motions, which thereby leads to an increase in the time step. This is achieved by solving <span class="hlt">fluid</span> motions coupled with electromagnetics using reduced-physics <span class="hlt">models</span>, such as single-temperature magnetohydrodynamics (MHD), extended, gas dynamic, and Hall MHD, and two-<span class="hlt">fluid</span> MHD <span class="hlt">models</span>. We show recent results on <span class="hlt">modeling</span> the internal antenna H(-) ion source for the SNS at Oak Ridge National Laboratory using the <span class="hlt">fluid</span> plasma <span class="hlt">modeling</span> code USim. We compare demonstrate plasma temperature equilibration in two-temperature MHD</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.S31B2755M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.S31B2755M"><span><span class="hlt">Modeling</span> the <span class="hlt">Fluid</span> Withdraw and Injection Induced Earthquakes</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Meng, C.</p> <p>2016-12-01</p> <p>We present an open source numerical code, Defmod, that allows one to <span class="hlt">model</span> the induced seismicity in an efficient and standalone manner. The <span class="hlt">fluid</span> withdraw and injection induced earthquake has been a great concern to the industries including oil/gas, wastewater disposal and CO2 sequestration. Being able to numerically <span class="hlt">model</span> the induced seismicity is long desired. To do that, one has to consider at lease two processes, a steady process that describes the inducing and aseismic stages before and in between the seismic events, and an abrupt process that describes the dynamic fault rupture accompanied by seismic energy radiations during the events. The steady process can be adequately <span class="hlt">modeled</span> by a quasi-static <span class="hlt">model</span>, while the abrupt process has to be <span class="hlt">modeled</span> by a dynamic <span class="hlt">model</span>. In most of the published <span class="hlt">modeling</span> works, only one of these processes is considered. The geomechanicists and reservoir engineers are focused more on the quasi-static <span class="hlt">modeling</span>, whereas the geophysicists and seismologists are focused more on the dynamic <span class="hlt">modeling</span>. The finite element code Defmod combines these two <span class="hlt">models</span> into a hybrid <span class="hlt">model</span> that uses the failure criterion and frictional laws to adaptively switch between the (quasi-)static and dynamic states. The code is capable of <span class="hlt">modeling</span> episodic fault rupture driven by quasi-static loading, e.g. due to reservoir <span class="hlt">fluid</span> withdraw and/or injection, and by dynamic loading, e.g. due to the foregoing earthquakes. We demonstrate a case study for the 2013 Azle earthquake.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017APS..MARS12006S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017APS..MARS12006S"><span>Linear Instability Analysis of non-uniform Bubbly Mixing layer with Two-<span class="hlt">Fluid</span> <span class="hlt">model</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sharma, Subash; Chetty, Krishna; Lopez de Bertodano, Martin</p> <p></p> <p>We examine the inviscid instability of a non-uniform adiabatic bubbly shear layer with a Two-<span class="hlt">Fluid</span> <span class="hlt">model</span>. The Two-<span class="hlt">Fluid</span> <span class="hlt">model</span> is made well-posed with the closure relations for interfacial forces. First, a characteristic analysis is carried out to study the well posedness of the <span class="hlt">model</span> over range of void fraction with interfacial forces for virtual mass, interfacial drag, interfacial pressure. A dispersion analysis then allow us to obtain growth rate and wavelength. Then, the well-posed two-<span class="hlt">fluid</span> <span class="hlt">model</span> is solved using CFD to validate the results obtained with the linear stability analysis. The effect of the void fraction and the distribution profile on stability is analyzed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JSV...394..575K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JSV...394..575K"><span>Damping of a <span class="hlt">fluid</span>-conveying pipe surrounded by a viscous annulus <span class="hlt">fluid</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kjolsing, Eric J.; Todd, Michael D.</p> <p>2017-04-01</p> <p>To further the development of a downhole vibration <span class="hlt">based</span> energy harvester, this study explores how <span class="hlt">fluid</span> velocity affects damping in a <span class="hlt">fluid</span>-conveying pipe stemming from a viscous annulus <span class="hlt">fluid</span>. A linearized equation of motion is formed which employs a hydrodynamic forcing function to <span class="hlt">model</span> the annulus <span class="hlt">fluid</span>. The system is solved in the frequency domain through the use of the spectral element method. The three independent variables investigated are the conveyed <span class="hlt">fluid</span> velocity, the rotational stiffness of the boundary (using elastic springs), and the annulus <span class="hlt">fluid</span> viscosity. It was found that, due to the hydrodynamic functions frequency-dependence, increasing the conveyed <span class="hlt">fluid</span> velocity increases the systems damping ratio. It was also noted that stiffer systems saw the damping ratio increase at a slower rate when compared to flexible systems as the conveyed <span class="hlt">fluid</span> velocity was increased. The results indicate that overestimating the stiffness of a system can lead to underestimated damping ratios and that this error is made worse if the produced <span class="hlt">fluid</span> velocity or annulus <span class="hlt">fluid</span> viscosity is underestimated. A numeric example was provided to graphically illustrate these errors. Approved for publication, LA-UR-15-28006.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70185203','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70185203"><span>Fines classification <span class="hlt">based</span> on sensitivity to pore-<span class="hlt">fluid</span> chemistry</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Jang, Junbong; Santamarina, J. Carlos</p> <p>2016-01-01</p> <p>The 75-μm particle size is used to discriminate between fine and coarse grains. Further analysis of fine grains is typically <span class="hlt">based</span> on the plasticity chart. Whereas pore-<span class="hlt">fluid</span>-chemistry-dependent soil response is a salient and distinguishing characteristic of fine grains, pore-<span class="hlt">fluid</span> chemistry is not addressed in current classification systems. Liquid limits obtained with electrically contrasting pore <span class="hlt">fluids</span> (deionized water, 2-M NaCl brine, and kerosene) are combined to define the soil “electrical sensitivity.” Liquid limit and electrical sensitivity can be effectively used to classify fine grains according to their <span class="hlt">fluid</span>-soil response into no-, low-, intermediate-, or high-plasticity fine grains of low, intermediate, or high electrical sensitivity. The proposed methodology benefits from the accumulated experience with liquid limit in the field and addresses the needs of a broader range of geotechnical engineering problems.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/18818972','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/18818972"><span>Multiscale <span class="hlt">modeling</span> of <span class="hlt">fluid</span> transport in tumors.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Chapman, S Jonathan; Shipley, Rebecca J; Jawad, Rossa</p> <p>2008-11-01</p> <p>A <span class="hlt">model</span> for <span class="hlt">fluid</span> flow through the leaky neovasculature and porous interstitium of a solid tumor is developed. A network of isolated capillaries is analyzed in the limit of small capillary radius, and analytical expressions for the hydraulic conductivities and fractional leakage coefficients derived. This <span class="hlt">model</span> is then homogenized to give a continuum description in terms of the vascular density. The resulting equations comprise a double porous medium with coupled Darcy flow through the interstitium and vasculature.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018MSSP..106..284R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018MSSP..106..284R"><span>External gear pumps operating with non-Newtonian <span class="hlt">fluids</span>: <span class="hlt">Modelling</span> and experimental validation</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Rituraj, Fnu; Vacca, Andrea</p> <p>2018-06-01</p> <p>External Gear Pumps are used in various industries to pump non-Newtonian viscoelastic <span class="hlt">fluids</span> like plastics, paints, inks, etc. For both design and analysis purposes, it is often a matter of interest to understand the features of the displacing action realized by meshing of the gears and the description of the behavior of the leakages for this kind of pumps. However, very limited work can be found in literature about methodologies suitable to <span class="hlt">model</span> such phenomena. This article describes the technique of <span class="hlt">modelling</span> external gear pumps that operate with non-Newtonian <span class="hlt">fluids</span>. In particular, it explains how the displacing action of the unit can be <span class="hlt">modelled</span> using a lumped parameter approach which involves dividing <span class="hlt">fluid</span> domain into several control volumes and internal flow connections. This work is built upon the HYGESim simulation tool, conceived by the authors' research team in the last decade, which is for the first time extended for the simulation of non-Newtonian <span class="hlt">fluids</span>. The article also describes several comparisons between simulation results and experimental data obtained from numerous experiments performed for validation of the presented methodology. Finally, operation of external gear pump with <span class="hlt">fluids</span> having different viscosity characteristics is discussed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFMED21C0840G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFMED21C0840G"><span>Using record player demonstrations as analog <span class="hlt">models</span> for geophysical <span class="hlt">fluids</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Grannan, A. M.; Cheng, J. S.; Hawkins, E. K.; Ribeiro, A.; Aurnou, J. M.</p> <p>2015-12-01</p> <p>All celestial bodies, including stars, planets, satellites, and asteroids, rotate. The influence of rotation on the <span class="hlt">fluid</span> layers in these bodies plays an important and diverse role, affecting many processes including oceanic and atmospheric circulation at the surface and magnetic field generation occurring in the interior. To better understand these large-scale processes, record players and containers of water are used as analog <span class="hlt">models</span> to demonstrate the basic interplay between rotation and <span class="hlt">fluid</span> motions. To contrast between rotating and non-rotating <span class="hlt">fluid</span> motions, coffee creamer and food coloring are used as <span class="hlt">fluid</span> tracers to provide a hands-on method of understanding the influence of rotation on the shapes of the planets, weather patterns, and the alignment of magnetic fields with rotational axes. Such simple demonstrations have been successfully employed for children in public outreach events and for adults in graduate level <span class="hlt">fluid</span> dynamics courses.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19930049573&hterms=solar+two&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Dsolar%2Btwo','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19930049573&hterms=solar+two&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Dsolar%2Btwo"><span>A two-<span class="hlt">fluid</span> <span class="hlt">model</span> of the solar wind</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Sandbaek, O.; Leer, E.; Holzer, T. E.</p> <p>1992-01-01</p> <p>A method is presented for the integration of the two-<span class="hlt">fluid</span> solar-wind equations which is applicable to a wide variety of coronal <span class="hlt">base</span> densities and temperatures. The method involves proton heat conduction, and may be applied to coronal <span class="hlt">base</span> conditions for which subsonic-supersonic solar wind solutions exist.</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/2010APS..DFD.QP004M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010APS..DFD.QP004M"><span>Designing a Robust Micromixer <span class="hlt">Based</span> on <span class="hlt">Fluid</span> Stretching</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Mott, David; Gautam, Dipesh; Voth, Greg; Oran, Elaine</p> <p>2010-11-01</p> <p>A metric for measuring <span class="hlt">fluid</span> stretching <span class="hlt">based</span> on finite-time Lyapunov exponents is described, and the use of this metric for optimizing mixing in microfluidic components is explored. The metric is implemented within an automated design approach called the Computational Toolbox (CTB). The CTB designs components by adding geometric features, such a grooves of various shapes, to a microchannel. The transport produced by each of these features in isolation was pre-computed and stored as an "advection map" for that feature, and the flow through a composite geometry that combines these features is calculated rapidly by applying the corresponding maps in sequence. A genetic algorithm search then chooses the feature combination that optimizes a user-specified metric. Metrics <span class="hlt">based</span> on the variance of concentration generally require the user to specify the <span class="hlt">fluid</span> distributions at inflow, which leads to different mixer designs for different inflow arrangements. The stretching metric is independent of the <span class="hlt">fluid</span> arrangement at inflow. Mixers designed using the stretching metric are compared to those designed using a variance of concentration metric and show excellent performance across a variety of inflow distributions and diffusivities.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017APS..DFDD31005E','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017APS..DFDD31005E"><span>An adjoint-<span class="hlt">based</span> framework for maximizing mixing in binary <span class="hlt">fluids</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Eggl, Maximilian; Schmid, Peter</p> <p>2017-11-01</p> <p>Mixing in the inertial, but laminar parameter regime is a common application in a wide range of industries. Enhancing the efficiency of mixing processes thus has a fundamental effect on product quality, material homogeneity and, last but not least, production costs. In this project, we address mixing efficiency in the above mentioned regime (Reynolds number Re = 1000 , Peclet number Pe = 1000) by developing and demonstrating an algorithm <span class="hlt">based</span> on nonlinear adjoint looping that minimizes the variance of a passive scalar field which <span class="hlt">models</span> our binary Newtonian <span class="hlt">fluids</span>. The numerical method is <span class="hlt">based</span> on the FLUSI code (Engels et al. 2016), a Fourier pseudo-spectral code, which we modified and augmented by scalar transport and adjoint equations. Mixing is accomplished by moving stirrers which are numerically <span class="hlt">modeled</span> using a penalization approach. In our two-dimensional simulations we consider rotating circular and elliptic stirrers and extract optimal mixing strategies from the iterative scheme. The case of optimizing shape and rotational speed of the stirrers will be demonstrated.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018PhFl...30c2108A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018PhFl...30c2108A"><span>Orbitally shaken shallow <span class="hlt">fluid</span> layers. II. An improved wall shear stress <span class="hlt">model</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Alpresa, Paola; Sherwin, Spencer; Weinberg, Peter; van Reeuwijk, Maarten</p> <p>2018-03-01</p> <p>A new <span class="hlt">model</span> for the analytical prediction of wall shear stress distributions at the <span class="hlt">base</span> of orbitally shaken shallow <span class="hlt">fluid</span> layers is developed. This <span class="hlt">model</span> is a generalisation of the classical extended Stokes solution and will be referred to as the potential theory-Stokes <span class="hlt">model</span>. The <span class="hlt">model</span> is validated using a large set of numerical simulations covering a wide range of flow regimes representative of those used in laboratory experiments. It is demonstrated that the <span class="hlt">model</span> is in much better agreement with the simulation data than the classical Stokes solution, improving the prediction in 63% of the studied cases. The central assumption of the model—which is to link the wall shear stress with the surface velocity—is shown to hold remarkably well over all regimes covered.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/6759601-two-dimensional-pattern-metamorphic-fluid-flow-mary-kathleen-australia-fluid-focusing-transverse-dispersion-implications-modeling-fluid-flow','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/6759601-two-dimensional-pattern-metamorphic-fluid-flow-mary-kathleen-australia-fluid-focusing-transverse-dispersion-implications-modeling-fluid-flow"><span>The two-dimensional pattern of metamorphic <span class="hlt">fluid</span> flow at Mary Kathleen, Australia: <span class="hlt">Fluid</span> focusing, transverse dispersion, and implications for <span class="hlt">modeling</span> <span class="hlt">fluid</span> flow</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>Cartwright, I.</p> <p></p> <p>The pattern of [delta][sup 18]O values in layered Corella calc-silicate rocks adjacent to a scapolitized metadolerite dike at Timberu in the Mary Kathleen fold belt illustrates some of the complexities of two-dimensional metamorphic <span class="hlt">fluid</span> flow. <span class="hlt">Fluids</span> flowing from the dike ([delta][sup 18]O = 9-10%) into the calc-silicate rocks lowered calcite [delta][sup 18]O values form 19-20% to as low as 10.3%. Time-integrate advectite <span class="hlt">fluid</span> fluxes varied from 0.72 to > 8.1 m[sup 3]/m[sup 2] over a 4.5-m lateral distance, and there are two distinct channels of higher <span class="hlt">fluid</span> flux. If the duration of <span class="hlt">fluid</span> flow was similar across the outcrop, intrinsicmore » permeabilities varied laterally by at least an order of magnitude. <span class="hlt">Fluid</span> flow was largely focused across lithological layering, with rare excursions parallel to layering, suggesting that (up to 1 m) to those at the isotopic front ([approximately]1.2 m), indicating that the coefficients of transverse and longitudinal dispersion are of similar orders of magnitude. Localities in other terrains probably show similar complex patterns of isotopic resetting that in two dimensions correspond to the predictions of the advective-dispersive transport <span class="hlt">models</span>, but which are difficult to interpret using a one-dimensional analysis. Transverse dispersion during channeled <span class="hlt">fluid</span> flow will potentially reset O-isotope ratios adjacent to the channels and cause decoupling of geochemical parameters during advective and dispersive transport. 43 refs., 5 figs., 2 tabs.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/20459189','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/20459189"><span>Robust and general method for determining surface <span class="hlt">fluid</span> flow boundary conditions in articular cartilage contact mechanics <span class="hlt">modeling</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Pawaskar, Sainath Shrikant; Fisher, John; Jin, Zhongmin</p> <p>2010-03-01</p> <p>Contact detection in cartilage contact mechanics is an important feature of any analytical or computational <span class="hlt">modeling</span> investigation when the biphasic nature of cartilage and the corresponding tribology are taken into account. The <span class="hlt">fluid</span> flow boundary conditions will change <span class="hlt">based</span> on whether the surface is in contact or not, which will affect the interstitial <span class="hlt">fluid</span> pressurization. This in turn will increase or decrease the load sustained by the <span class="hlt">fluid</span> phase, with a direct effect on friction, wear, and lubrication. In laboratory experiments or clinical hemiarthroplasty, when a rigid indenter or metallic prosthesis is used to apply load to the cartilage, there will not be any <span class="hlt">fluid</span> flow normal to the surface in the contact region due to the impermeable nature of the indenter/prosthesis. In the natural joint, on the other hand, where two cartilage surfaces interact, flow will depend on the pressure difference across the interface. Furthermore, in both these cases, the <span class="hlt">fluid</span> would flow freely in non-contacting regions. However, it should be pointed out that the contact area is generally unknown in advance in both cases and can only be determined as part of the solution. In the present finite element study, a general and robust algorithm was proposed to decide nodes in contact on the cartilage surface and, accordingly, impose the <span class="hlt">fluid</span> flow boundary conditions. The algorithm was first tested for a rigid indenter against cartilage <span class="hlt">model</span>. The algorithm worked well for two-dimensional four-noded and eight-noded axisymmetric element <span class="hlt">models</span> as well as three-dimensional <span class="hlt">models</span>. It was then extended to include two cartilages in contact. The results were in excellent agreement with the previous studies reported in the literature.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AGUFM.S33D2470M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFM.S33D2470M"><span>Physics <span class="hlt">based</span> simulation of seismicity induced in the vicinity of a high-pressure <span class="hlt">fluid</span> injection</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>McCloskey, J.; NicBhloscaidh, M.; Murphy, S.; O'Brien, G. S.; Bean, C. J.</p> <p>2013-12-01</p> <p>High-pressure <span class="hlt">fluid</span> injection into subsurface is known, in some cases, to induce earthquakes in the surrounding volume. The increasing importance of ';fracking' as a potential source of hydrocarbons has made the seismic hazard from this effect an important issue the adjudication of planning applications and it is likely that poor understanding of the process will be used as justification of refusal of planning in Ireland and the UK. Here we attempt to understand some of the physical controls on the size and frequency of induced earthquakes using a physics-<span class="hlt">based</span> simulation of the process and examine resulting earthquake catalogues The driver for seismicity in our simulations is identical to that used in the paper by Murphy et al. in this session. <span class="hlt">Fluid</span> injection is simulated using pore <span class="hlt">fluid</span> movement throughout a permeable layer from a high-pressure point source using a lattice Boltzmann scheme. Diffusivities and frictional parameters can be defined independently at individual nodes/cells allowing us to reproduce 3-D geological structures. Active faults in the <span class="hlt">model</span> follow a fractal size distribution and exhibit characteristic event size, resulting in a power-law frequency-size distribution. The <span class="hlt">fluid</span> injection is not hydraulically connected to the fault (i.e. <span class="hlt">fluid</span> does not come into physical contact with the fault); however stress perturbations from the injection drive the seismicity <span class="hlt">model</span>. The duration and pressure-time function of the <span class="hlt">fluid</span> injection can be adjusted to <span class="hlt">model</span> any given injection scenario and the rate of induced seismicity is controlled by the local structures and ambient stress field as well as by the stress perturbations resulting from the <span class="hlt">fluid</span> injection. Results from the rate and state fault <span class="hlt">models</span> of Murphy et al. are incorporated to include the effect of fault strengthening in seismically quite areas. Initial results show similarities with observed induced seismic catalogues. Seismicity is only induced where the active faults have not been</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018PhRvL.120o5301Y','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018PhRvL.120o5301Y"><span>Three-Dimensional Coupled Dynamics of The Two-<span class="hlt">Fluid</span> <span class="hlt">Model</span> in Superfluid 4He: Deformed Velocity Profile of Normal <span class="hlt">Fluid</span> in Thermal Counterflow</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Yui, Satoshi; Tsubota, Makoto; Kobayashi, Hiromichi</p> <p>2018-04-01</p> <p>The coupled dynamics of the two-<span class="hlt">fluid</span> <span class="hlt">model</span> of superfluid 4He is numerically studied for quantum turbulence of the thermal counterflow in a square channel. We combine the vortex filament <span class="hlt">model</span> of the superfluid and the Navier-Stokes equations of normal <span class="hlt">fluid</span>. Simulations of the coupled dynamics show that the velocity profile of the normal <span class="hlt">fluid</span> is deformed significantly by superfluid turbulence as the vortices become dense. This result is consistent with recently performed visualization experiments. We introduce a dimensionless parameter that characterizes the deformation of the velocity profile.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20050137695','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20050137695"><span>Agent-<span class="hlt">Based</span> Chemical Plume Tracing Using <span class="hlt">Fluid</span> Dynamics</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Zarzhitsky, Dimitri; Spears, Diana; Thayer, David; Spears, William</p> <p>2004-01-01</p> <p>This paper presents a rigorous evaluation of a novel, distributed chemical plume tracing algorithm. The algorithm is a combination of the best aspects of the two most popular predecessors for this task. Furthermore, it is <span class="hlt">based</span> on solid, formal principles from the field of <span class="hlt">fluid</span> mechanics. The algorithm is applied by a network of mobile sensing agents (e.g., robots or micro-air vehicles) that sense the ambient <span class="hlt">fluid</span> velocity and chemical concentration, and calculate derivatives. The algorithm drives the robotic network to the source of the toxic plume, where measures can be taken to disable the source emitter. This work is part of a much larger effort in research and development of a physics-<span class="hlt">based</span> approach to developing networks of mobile sensing agents for monitoring, tracking, reporting and responding to hazardous conditions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018E%26ES..108c2001S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018E%26ES..108c2001S"><span>The Research of New Environment-Friendly Oil-<span class="hlt">based</span> Drilling <span class="hlt">Fluid</span> <span class="hlt">Base</span> Oil</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sui, Dianjie; Sun, Yuxue; Zhao, Jingyuan; Zhao, Fulei; Zhu, Xiuyu; Xu, Jianjun</p> <p>2018-01-01</p> <p>In this paper, the heavy hydrocarbon of Daqing is used, and the desulfurization and de-aromatization experiments and refining process are carried out, A <span class="hlt">base</span> oil suitable for oil-<span class="hlt">based</span> drilling <span class="hlt">fluid</span> was developed, and the performance of <span class="hlt">base</span> oil was evaluated, we can know the aromatics content of oil <span class="hlt">base</span> is low, less toxic, less pollution and it can meet the requirement of environmental protection.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19840061397&hterms=facility+management&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3Dfacility%2Bmanagement','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19840061397&hterms=facility+management&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3Dfacility%2Bmanagement"><span>Cryogenic <span class="hlt">Fluid</span> Management Facility</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Eberhardt, R. N.; Bailey, W. J.; Symons, E. P.; Kroeger, E. W.</p> <p>1984-01-01</p> <p>The Cryogenic <span class="hlt">Fluid</span> Management Facility (CFMF) is a reusable test bed which is designed to be carried into space in the Shuttle cargo bay to investigate systems and technologies required to efficiently and effectively manage cryogens in space. The facility hardware is configured to provide low-g verification of <span class="hlt">fluid</span> and thermal <span class="hlt">models</span> of cryogenic storage, transfer concepts and processes. Significant design data and criteria for future subcritical cryogenic storage and transfer systems will be obtained. Future applications include space-<span class="hlt">based</span> and ground-<span class="hlt">based</span> orbit transfer vehicles (OTV), space station life support, attitude control, power and fuel depot supply, resupply tankers, external tank (ET) propellant scavenging, space-<span class="hlt">based</span> weapon systems and space-<span class="hlt">based</span> orbit maneuvering vehicles (OMV). This paper describes the facility and discusses the cryogenic <span class="hlt">fluid</span> management technology to be investigated. A brief discussion of the integration issues involved in loading and transporting liquid hydrogen within the Shuttle cargo bay is also included.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/21895085','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/21895085"><span><span class="hlt">Fluid</span> coupling in a discrete <span class="hlt">model</span> of cochlear mechanics.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Elliott, Stephen J; Lineton, Ben; Ni, Guangjian</p> <p>2011-09-01</p> <p>A discrete <span class="hlt">model</span> of cochlear mechanics is introduced that includes a full, three-dimensional, description of <span class="hlt">fluid</span> coupling. This formulation allows the <span class="hlt">fluid</span> coupling and basilar membrane dynamics to be analyzed separately and then coupled together with a simple piece of linear algebra. The <span class="hlt">fluid</span> coupling is initially analyzed using a wavenumber formulation and is separated into one component due to one-dimensional <span class="hlt">fluid</span> coupling and one comprising all the other contributions. Using the theory of acoustic waves in a duct, however, these two components of the pressure can also be associated with a far field, due to the plane wave, and a near field, due to the evanescent, higher order, modes. The near field components are then seen as one of a number of sources of additional longitudinal coupling in the cochlea. The effects of non-uniformity and asymmetry in the <span class="hlt">fluid</span> chamber areas can also be taken into account, to predict both the pressure difference between the chambers and the mean pressure. This allows the calculation, for example, of the effect of a short cochlear implant on the coupled response of the cochlea. © 2011 Acoustical Society of America</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20150016491','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20150016491"><span>Computational <span class="hlt">Fluid</span> Dynamics <span class="hlt">Based</span> Extraction of Heat Transfer Coefficient in 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>Yang, H. Q.; West, Jeff</p> <p>2015-01-01</p> <p>Current reduced-order thermal <span class="hlt">model</span> for cryogenic propellant tanks is <span class="hlt">based</span> on correlations built for flat plates collected in the 1950's. The use of these correlations suffers from: inaccurate geometry representation; inaccurate gravity orientation; ambiguous length scale; and lack of detailed validation. The work presented under this task uses the first-principles <span class="hlt">based</span> Computational <span class="hlt">Fluid</span> Dynamics (CFD) technique to compute heat transfer from tank wall to the cryogenic <span class="hlt">fluids</span>, and extracts and correlates the equivalent heat transfer coefficient to support reduced-order thermal <span class="hlt">model</span>. The CFD tool was first validated against available experimental data and commonly used correlations for natural convection along a vertically heated wall. Good agreements between the present prediction and experimental data have been found for flows in laminar as well turbulent regimes. The convective heat transfer between tank wall and cryogenic propellant, and that between tank wall and ullage gas were then simulated. The results showed that commonly used heat transfer correlations for either vertical or horizontal plate over predict heat transfer rate for the cryogenic tank, in some cases by as much as one order of magnitude. A characteristic length scale has been defined that can correlate all heat transfer coefficients for different fill levels into a single curve. This curve can be used for the reduced-order heat transfer <span class="hlt">model</span> analysis.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70020242','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70020242"><span>Hydraulic <span class="hlt">modeling</span> of unsteady debris-flow surges with solid-<span class="hlt">fluid</span> interactions</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Iverson, Richard M.</p> <p>1997-01-01</p> <p>Interactions of solid and <span class="hlt">fluid</span> constituents produce the unique style of motion that typifies debris flows. To simulate this motion, a new hydraulic <span class="hlt">model</span> represents debris flows as deforming masses of granular solids variably liquefied by viscous pore <span class="hlt">fluid</span>. The momentum equation of the <span class="hlt">model</span> describes how internal and boundary forces change as coarse-grained surge heads dominated by grain-contact friction grade into muddy debris-flow bodies more strongly influenced by <span class="hlt">fluid</span> viscosity and pressure. Scaling analysis reveals that pore-pressure variations can cause flow resistance in surge heads to surpass that in debris-flow bodies by orders of magnitude. Numerical solutions of the coupled momentum and continuity equations provide good predictions of unsteady, nonuniform motion of experimental debris flows from initiation through deposition.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016APS..DFDD15002H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016APS..DFDD15002H"><span><span class="hlt">Fluid</span> Structure Interaction Analysis on Sidewall Aneurysm <span class="hlt">Models</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hao, Qing</p> <p>2016-11-01</p> <p>Wall shear stress is considered as an important factor for cerebral aneurysm growth and rupture. The objective of present study is to evaluate wall shear stress in aneurysm sac and neck by a <span class="hlt">fluid</span>-structure-interaction (FSI) <span class="hlt">model</span>, which was developed and validated against the particle image velocimetry (PIV) data. In this FSI <span class="hlt">model</span>, the flow characteristics in a straight tube with different asymmetric aneurysm sizes over a range of Reynolds numbers from 200 to 1600 were investigated. The FSI results agreed well with PIV data. It was found that at steady flow conditions, when Reynolds number above 700, one large recirculating vortex would be formed, occupying the entire aneurysm sac. The center of the vortex is located at region near to the distal neck. A pair of counter rotating vortices would however be formed at Reynolds number below 700. Wall shear stresses reached highest level at the distal neck of the aneurysmal sac. The vortex strength, in general, is stronger at higher Reynolds number. <span class="hlt">Fluid</span> Structure Interaction Analysis on Sidewall Aneurysm <span class="hlt">Models</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/23584207','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/23584207"><span>Magnetic timing valves for <span class="hlt">fluid</span> control in paper-<span class="hlt">based</span> microfluidics.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Li, Xiao; Zwanenburg, Philip; Liu, Xinyu</p> <p>2013-07-07</p> <p>Multi-step analytical tests, such as an enzyme-linked immunosorbent assay (ELISA), require delivery of multiple <span class="hlt">fluids</span> into a reaction zone and counting the incubation time at different steps. This paper presents a new type of paper-<span class="hlt">based</span> magnetic valves that can count the time and turn on or off a fluidic flow accordingly, enabling timed <span class="hlt">fluid</span> control in paper-<span class="hlt">based</span> microfluidics. The timing capability of these valves is realized using a paper timing channel with an ionic resistor, which can detect the event of a solution flowing through the resistor and trigger an electromagnet (through a simple circuit) to open or close a paper cantilever valve. <span class="hlt">Based</span> on this principle, we developed normally-open and normally-closed valves with a timing period up to 30.3 ± 2.1 min (sufficient for an ELISA on paper-<span class="hlt">based</span> platforms). Using the normally-open valve, we performed an enzyme-<span class="hlt">based</span> colorimetric reaction commonly used for signal readout of ELISAs, which requires a timed delivery of an enzyme substrate to a reaction zone. This design adds a new <span class="hlt">fluid</span>-control component to the tool set for developing paper-<span class="hlt">based</span> microfluidic devices, and has the potential to improve the user-friendliness of these devices.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19860052315&hterms=passive+thermal+management&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3Dpassive%2Bthermal%2Bmanagement','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19860052315&hterms=passive+thermal+management&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3Dpassive%2Bthermal%2Bmanagement"><span>Cryogenic <span class="hlt">Fluid</span> Management Facility</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Eberhardt, R. N.; Bailey, W. J.</p> <p>1985-01-01</p> <p>The Cryogenic <span class="hlt">Fluid</span> Management Facility is a reusable test bed which is designed to be carried within the Shuttle cargo bay to investigate the systems and technologies associated with the efficient management of cryogens in space. Cryogenic <span class="hlt">fluid</span> management consists of the systems and technologies for: (1) liquid storage and supply, including capillary acquisition/expulsion systems which provide single-phase liquid to the user system, (2) both passive and active thermal control systems, and (3) <span class="hlt">fluid</span> transfer/resupply systems, including transfer lines and receiver tanks. The facility contains a storage and supply tank, a transfer line and a receiver tank, configured to provide low-g verification of <span class="hlt">fluid</span> and thermal <span class="hlt">models</span> of cryogenic storage and transfer processes. The facility will provide design data and criteria for future subcritical cryogenic storage and transfer system applications, such as Space Station life support, attitude control, power and fuel depot supply, resupply tankers, external tank (ET) propellant scavenging, and ground-<span class="hlt">based</span> and space-<span class="hlt">based</span> orbit transfer vehicles (OTV).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010AIPC.1298...43G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010AIPC.1298...43G"><span>Development Of Simulation <span class="hlt">Model</span> For <span class="hlt">Fluid</span> Catalytic Cracking</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ghosh, Sobhan</p> <p>2010-10-01</p> <p><span class="hlt">Fluid</span> Catalytic Cracking (FCC) is the most widely used secondary conversion process in the refining industry, for producing gasoline, olefins, and middle distillate from heavier petroleum fractions. There are more than 500 units in the world with a total processing capacity of about 17 to 20% of the crude capacity. FCC catalyst is the highest consumed catalyst in the process industry. On one hand, FCC is quite flexible with respect to it's ability to process wide variety of crudes with a flexible product yield pattern, and on the other hand, the interdependence of the major operating parameters makes the process extremely complex. An operating unit is self balancing and some fluctuations in the independent parameters are automatically adjusted by changing the temperatures and flow rates at different sections. However, a good simulation <span class="hlt">model</span> is very useful to the refiner to get the best out of the process, in terms of selection of the best catalyst, to cope up with the day to day changing of the feed quality and the demands of different products from FCC unit. In addition, a good <span class="hlt">model</span> is of great help in designing the process units and peripherals. A simple empirical <span class="hlt">model</span> is often adequate to monitor the day to day operations, but they are not of any use in handling the other problems such as, catalyst selection or, design / modification of the plant. For this, a kinetic <span class="hlt">based</span> rigorous <span class="hlt">model</span> is required. Considering the complexity of the process, large number of chemical species undergoing "n" number of parallel and consecutive reactions, it is virtually impossible to develop a simulation <span class="hlt">model</span> <span class="hlt">based</span> on the kinetic parameters. The most common approach is to settle for a semi empirical <span class="hlt">model</span>. We shall take up the key issues for developing a FCC <span class="hlt">model</span> and the contribution of such <span class="hlt">models</span> in the optimum operation of the plant.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..1913012W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..1913012W"><span>Analogue <span class="hlt">modelling</span> of caprock failure and sediment mobilisation due to pore <span class="hlt">fluid</span> overpressure in shallow reservoirs</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Warsitzka, Michael; Kukowski, Nina; May, Franz</p> <p>2017-04-01</p> <p>Injection of CO2 in geological formations may cause excess pore <span class="hlt">fluid</span> pressure by enhancing the <span class="hlt">fluid</span> volume in the reservoir rock and by buoyancy-driven flow. If sediments in the reservoir and the caprock are undercompacted, pore <span class="hlt">fluid</span> overpressure can lead to hydro-fractures in the caprock and fluidisation of sediments. Eventually, these processes trigger the formation of pipe structures, gas chimneys, gas domes or sand injections. Generally, such structures serve as high permeable pathways for <span class="hlt">fluid</span> migration through a low-permeable seal layer and have to be considered in risk assessment or <span class="hlt">modelling</span> of caprock integrity of CO2 storage sites. We applied scaled analogue experiments to characterise and quantify mechanisms determining the onset and migration of hydro-fractures in a low-permeable, cohesive caprock and fluidisation of unconsolidated sediments of the reservoir layer. The caprock is simulated by different types of cohesive powder. The reservoir layer consists of granulates with small particle density. Air injected through the <span class="hlt">base</span> of the experiment and additionally through a single needle valve reaching into the analogue material is applied to generate <span class="hlt">fluid</span> pressure within the materials. With this procedure, regional <span class="hlt">fluid</span> pressure increase or a point-like local <span class="hlt">fluid</span> pressure increase (e.g. injection well), respectively, can be simulated. The deformation in the analogue materials is analysed with a particle tracking imaging velocimetry technique. Pressure sensors at the <span class="hlt">base</span> of the experiment and in the needle valve record the air pressure during an experimental run. The structural evolution observed in the experiments reveal that the cohesive cap rock first forms a dome-like anticline. Extensional fractures occur at the hinges of the anticline. A further increase of <span class="hlt">fluid</span> pressure causes a migration of this fractures towards the surface, which is followed by intrusion of reservoir material into the fractures and the collapse of the anticline. The</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFMMR53A..06R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFMMR53A..06R"><span><span class="hlt">Modeling</span> Studies to Constrain <span class="hlt">Fluid</span> and Gas Migration Associated with Hydraulic Fracturing Operations</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Rajaram, H.; Birdsell, D.; Lackey, G.; Karra, S.; Viswanathan, H. S.; Dempsey, D.</p> <p>2015-12-01</p> <p>The dramatic increase in the extraction of unconventional oil and gas resources using horizontal wells and hydraulic fracturing (fracking) technologies has raised concerns about potential environmental impacts. Large volumes of hydraulic fracturing <span class="hlt">fluids</span> are injected during fracking. Incidents of stray gas occurrence in shallow aquifers overlying shale gas reservoirs have been reported; whether these are in any way related to fracking continues to be debated. Computational <span class="hlt">models</span> serve as useful tools for evaluating potential environmental impacts. We present <span class="hlt">modeling</span> studies of hydraulic fracturing <span class="hlt">fluid</span> and gas migration during the various stages of well operation, production, and subsequent plugging. The <span class="hlt">fluid</span> migration <span class="hlt">models</span> account for overpressure in the gas reservoir, density contrast between injected <span class="hlt">fluids</span> and brine, imbibition into partially saturated shale, and well operations. Our results highlight the importance of representing the different stages of well operation consistently. Most importantly, well suction and imbibition both play a significant role in limiting upward migration of injected <span class="hlt">fluids</span>, even in the presence of permeable connecting pathways. In an overall assessment, our <span class="hlt">fluid</span> migration simulations suggest very low risk to groundwater aquifers when the vertical separation from a shale gas reservoir is of the order of 1000' or more. Multi-phase <span class="hlt">models</span> of gas migration were developed to couple flow and transport in compromised wellbores and subsurface formations. These <span class="hlt">models</span> are useful for evaluating both short-term and long-term scenarios of stray methane release. We present simulation results to evaluate mechanisms controlling stray gas migration, and explore relationships between bradenhead pressures and the likelihood of methane release and transport.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016JCoPh.319...28A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016JCoPh.319...28A"><span>Revisiting low-fidelity two-<span class="hlt">fluid</span> <span class="hlt">models</span> for gas-solids transport</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Adeleke, Najeem; Adewumi, Michael; Ityokumbul, Thaddeus</p> <p>2016-08-01</p> <p>Two-phase gas-solids transport <span class="hlt">models</span> are widely utilized for process design and automation in a broad range of industrial applications. Some of these applications include proppant transport in gaseous fracking <span class="hlt">fluids</span>, air/gas drilling hydraulics, coal-gasification reactors and food processing units. Systems automation and real time process optimization stand to benefit a great deal from availability of efficient and accurate theoretical <span class="hlt">models</span> for operations data processing. However, <span class="hlt">modeling</span> two-phase pneumatic transport systems accurately requires a comprehensive understanding of gas-solids flow behavior. In this study we discuss the prevailing flow conditions and present a low-fidelity two-<span class="hlt">fluid</span> <span class="hlt">model</span> equation for particulate transport. The <span class="hlt">model</span> equations are formulated in a manner that ensures the physical flux term remains conservative despite the inclusion of solids normal stress through the empirical formula for modulus of elasticity. A new set of Roe-Pike averages are presented for the resulting strictly hyperbolic flux term in the system of equations, which was used to develop a Roe-type approximate Riemann solver. The resulting scheme is stable regardless of the choice of flux-limiter. The <span class="hlt">model</span> is evaluated by the prediction of experimental results from both pneumatic riser and air-drilling hydraulics systems. We demonstrate the effect and impact of numerical formulation and choice of numerical scheme on <span class="hlt">model</span> predictions. We illustrate the capability of a low-fidelity one-dimensional two-<span class="hlt">fluid</span> <span class="hlt">model</span> in predicting relevant flow parameters in two-phase particulate systems accurately even under flow regimes involving counter-current flow.</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/2017JMMM..431..269K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JMMM..431..269K"><span>Development of <span class="hlt">models</span> of the magnetorheological <span class="hlt">fluid</span> damper</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kazakov, Yu. B.; Morozov, N. A.; Nesterov, S. A.</p> <p>2017-06-01</p> <p>The algorithm for analytical calculation of a power characteristic of magnetorheological (MR) dampers taking into account the rheological properties of MR <span class="hlt">fluid</span> is considered. The nonlinear magnetorheological characteristics are represented by piecewise linear approximation to MR <span class="hlt">fluid</span> areas with different viscosities. The extended calculated power characteristics of a MR damper are received and they coincide with actual results. The finite element <span class="hlt">model</span> of a MR damper is developed; it allows carrying out the analysis of a MR damper taking into account the mutual influence of electromagnetic, hydrodynamic and thermal fields. The results of finite element simulation coincide with analytical solutions that allows using them for design development of a MR damper.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AIPC.1734g0014H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AIPC.1734g0014H"><span>Dynamic <span class="hlt">modelling</span> and simulation of linear Fresnel solar field <span class="hlt">model</span> <span class="hlt">based</span> on molten salt heat transfer <span class="hlt">fluid</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hakkarainen, Elina; Tähtinen, Matti</p> <p>2016-05-01</p> <p>Demonstrations of direct steam generation (DSG) in linear Fresnel collectors (LFC) have given promising results related to higher steam parameters compared to the current state-of-the-art parabolic trough collector (PTC) technology using oil as heat transfer <span class="hlt">fluid</span> (HTF). However, DSG technology lacks feasible solution for long-term thermal energy storage (TES) system. This option is important for CSP technology in order to offer dispatchable power. Recently, molten salts have been proposed to be used as HTF and directly as storage medium in both line-focusing solar fields, offering storage capacity of several hours. This direct molten salt (DMS) storage concept has already gained operational experience in solar tower power plant, and it is under demonstration phase both in the case of LFC and PTC systems. Dynamic simulation programs offer a valuable effort for design and optimization of solar power plants. In this work, APROS dynamic simulation program is used to <span class="hlt">model</span> a DMS linear Fresnel solar field with two-tank TES system, and example simulation results are presented in order to verify the functionality of the <span class="hlt">model</span> and capability of APROS for CSP <span class="hlt">modelling</span> and simulation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMGP33A0963M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMGP33A0963M"><span>Seismoelectric Effects <span class="hlt">based</span> on Spectral-Element Method for Subsurface <span class="hlt">Fluid</span> Characterization</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Morency, C.</p> <p>2017-12-01</p> <p>Present approaches for subsurface imaging rely predominantly on seismic techniques, which alone do not capture <span class="hlt">fluid</span> properties and related mechanisms. On the other hand, electromagnetic (EM) measurements add constraints on the <span class="hlt">fluid</span> phase through electrical conductivity and permeability, but EM signals alone do not offer information of the solid structural properties. In the recent years, there have been many efforts to combine both seismic and EM data for exploration geophysics. The most popular approach is <span class="hlt">based</span> on joint inversion of seismic and EM data, as decoupled phenomena, missing out the coupled nature of seismic and EM phenomena such as seismoeletric effects. Seismoelectric effects are related to pore <span class="hlt">fluid</span> movements with respect to the solid grains. By analyzing coupled poroelastic seismic and EM signals, one can capture a pore scale behavior and access both structural and <span class="hlt">fluid</span> properties.Here, we <span class="hlt">model</span> the seismoelectric response by solving the governing equations derived by Pride and Garambois (1994), which correspond to Biot's poroelastic wave equations and Maxwell's electromagnetic wave equations coupled electrokinetically. We will show that these coupled wave equations can be numerically implemented by taking advantage of viscoelastic-electromagnetic mathematical equivalences. These equations will be solved using a spectral-element method (SEM). The SEM, in contrast to finite-element methods (FEM) uses high degree Lagrange polynomials. Not only does this allow the technique to handle complex geometries similarly to FEM, but it also retains exponential convergence and accuracy due to the use of high degree polynomials. Finally, we will discuss how this is a first step toward full coupled seismic-EM inversion to improve subsurface <span class="hlt">fluid</span> characterization. This work was performed under the auspices of the U.S. Department of Energy by Lawrence Livermore National Laboratory under Contract DE-AC52-07NA27344.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26509253','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26509253"><span>Numerical <span class="hlt">modeling</span> of <span class="hlt">fluid</span>-structure interaction in arteries with anisotropic polyconvex hyperelastic and anisotropic viscoelastic material <span class="hlt">models</span> at finite strains.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Balzani, Daniel; Deparis, Simone; Fausten, Simon; Forti, Davide; Heinlein, Alexander; Klawonn, Axel; Quarteroni, Alfio; Rheinbach, Oliver; Schröder, Joerg</p> <p>2016-10-01</p> <p>The accurate prediction of transmural stresses in arterial walls requires on the one hand robust and efficient numerical schemes for the solution of boundary value problems including <span class="hlt">fluid</span>-structure interactions and on the other hand the use of a material <span class="hlt">model</span> for the vessel wall that is able to capture the relevant features of the material behavior. One of the main contributions of this paper is the application of a highly nonlinear, polyconvex anisotropic structural <span class="hlt">model</span> for the solid in the context of <span class="hlt">fluid</span>-structure interaction, together with a suitable discretization. Additionally, the influence of viscoelasticity is investigated. The <span class="hlt">fluid</span>-structure interaction problem is solved using a monolithic approach; that is, the nonlinear system is solved (after time and space discretizations) as a whole without splitting among its components. The linearized block systems are solved iteratively using parallel domain decomposition preconditioners. A simple - but nonsymmetric - curved geometry is proposed that is demonstrated to be suitable as a benchmark testbed for <span class="hlt">fluid</span>-structure interaction simulations in biomechanics where nonlinear structural <span class="hlt">models</span> are used. <span class="hlt">Based</span> on the curved benchmark geometry, the influence of different material <span class="hlt">models</span>, spatial discretizations, and meshes of varying refinement is investigated. It turns out that often-used standard displacement elements with linear shape functions are not sufficient to provide good approximations of the arterial wall stresses, whereas for standard displacement elements or F-bar formulations with quadratic shape functions, suitable results are obtained. For the time discretization, a second-order backward differentiation formula scheme is used. It is shown that the curved geometry enables the analysis of non-rotationally symmetric distributions of the mechanical fields. For instance, the maximal shear stresses in the <span class="hlt">fluid</span>-structure interface are found to be higher in the inner curve that corresponds to</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20030068130','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20030068130"><span>Internal Flow Thermal/<span class="hlt">Fluid</span> <span class="hlt">Modeling</span> of STS-107 Port Wing in Support of the Columbia Accident Investigation Board</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Sharp, John R.; Kittredge, Ken; Schunk, Richard G.</p> <p>2003-01-01</p> <p>As part of the aero-thermodynamics team supporting the Columbia Accident Investigation Board (CAB), the Marshall Space Flight Center was asked to perform engineering analyses of internal flows in the port wing. The aero-thermodynamics team was split into internal flow and external flow teams with the support being divided between shorter timeframe engineering methods and more complex computational <span class="hlt">fluid</span> dynamics. In order to gain a rough order of magnitude type of knowledge of the internal flow in the port wing for various breach locations and sizes (as theorized by the CAB to have caused the Columbia re-entry failure), a bulk venting <span class="hlt">model</span> was required to input boundary flow rates and pressures to the computational <span class="hlt">fluid</span> dynamics (CFD) analyses. This paper summarizes the <span class="hlt">modeling</span> that was done by MSFC in Thermal Desktop. A venting <span class="hlt">model</span> of the entire Orbiter was constructed in FloCAD <span class="hlt">based</span> on Rockwell International s flight substantiation analyses and the STS-107 reentry trajectory. Chemical equilibrium air thermodynamic properties were generated for SINDA/FLUINT s <span class="hlt">fluid</span> property routines from a code provided by Langley Research Center. In parallel, a simplified thermal mathematical <span class="hlt">model</span> of the port wing, including the Thermal Protection System (TPS), was <span class="hlt">based</span> on more detailed Shuttle re-entry <span class="hlt">modeling</span> previously done by the Dryden Flight Research Center. Once the venting <span class="hlt">model</span> was coupled with the thermal <span class="hlt">model</span> of the wing structure with chemical equilibrium air properties, various breach scenarios were assessed in support of the aero-thermodynamics team. The construction of the coupled <span class="hlt">model</span> and results are presented herein.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/21612956-two-stage-fluid-bed-plasma-gasification-process-solid-waste-valorisation-technical-review-preliminary-thermodynamic-modelling-sulphur-emissions','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/21612956-two-stage-fluid-bed-plasma-gasification-process-solid-waste-valorisation-technical-review-preliminary-thermodynamic-modelling-sulphur-emissions"><span>Two stage <span class="hlt">fluid</span> bed-plasma gasification process for solid waste valorisation: Technical review and preliminary thermodynamic <span class="hlt">modelling</span> of sulphur emissions</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>Morrin, Shane, E-mail: shane.morrin@ucl.ac.uk; Advanced Plasma Power, South Marston Business park, Swindon, SN3 4DE; Lettieri, Paola, E-mail: p.lettieri@ucl.ac.uk</p> <p>2012-04-15</p> <p>Highlights: Black-Right-Pointing-Pointer We investigate sulphur during MSW gasification within a <span class="hlt">fluid</span> bed-plasma process. Black-Right-Pointing-Pointer We review the literature on the feed, sulphur and process principles therein. Black-Right-Pointing-Pointer The need for research in this area was identified. Black-Right-Pointing-Pointer We perform thermodynamic <span class="hlt">modelling</span> of the <span class="hlt">fluid</span> bed stage. Black-Right-Pointing-Pointer Initial findings indicate the prominence of solid phase sulphur. - Abstract: Gasification of solid waste for energy has significant potential given an abundant feed supply and strong policy drivers. Nonetheless, significant ambiguities in the knowledge <span class="hlt">base</span> are apparent. Consequently this study investigates sulphur mechanisms within a novel two stage <span class="hlt">fluid</span> bed-plasma gasification process.more » This paper includes a detailed review of gasification and plasma fundamentals in relation to the specific process, along with insight on MSW <span class="hlt">based</span> feedstock properties and sulphur pollutant therein. As a first step to understanding sulphur partitioning and speciation within the process, thermodynamic <span class="hlt">modelling</span> of the <span class="hlt">fluid</span> bed stage has been performed. Preliminary findings, supported by plant experience, indicate the prominence of solid phase sulphur species (as opposed to H{sub 2}S) - Na and K <span class="hlt">based</span> species in particular. Work is underway to further investigate and validate this.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22482962-alternative-modeling-methods-plasma-based-rf-ion-sources','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22482962-alternative-modeling-methods-plasma-based-rf-ion-sources"><span>Alternative <span class="hlt">modeling</span> methods for plasma-<span class="hlt">based</span> Rf ion sources</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>Veitzer, Seth A., E-mail: veitzer@txcorp.com; Kundrapu, Madhusudhan, E-mail: madhusnk@txcorp.com; Stoltz, Peter H., E-mail: phstoltz@txcorp.com</p> <p></p> <p>Rf-driven ion sources for accelerators and many industrial applications benefit from detailed numerical <span class="hlt">modeling</span> and simulation of plasma characteristics. For instance, <span class="hlt">modeling</span> of the Spallation Neutron Source (SNS) internal antenna H{sup −} source has indicated that a large plasma velocity is induced near bends in the antenna where structural failures are often observed. This could lead to improved designs and ion source performance <span class="hlt">based</span> on simulation and <span class="hlt">modeling</span>. However, there are significant separations of time and spatial scales inherent to Rf-driven plasma ion sources, which makes it difficult to <span class="hlt">model</span> ion sources with explicit, kinetic Particle-In-Cell (PIC) simulation codes. Inmore » particular, if both electron and ion motions are to be explicitly <span class="hlt">modeled</span>, then the simulation time step must be very small, and total simulation times must be large enough to capture the evolution of the plasma ions, as well as extending over many Rf periods. Additional physics processes such as plasma chemistry and surface effects such as secondary electron emission increase the computational requirements in such a way that even fully parallel explicit PIC <span class="hlt">models</span> cannot be used. One alternative method is to develop <span class="hlt">fluid-based</span> codes coupled with electromagnetics in order to <span class="hlt">model</span> ion sources. Time-domain <span class="hlt">fluid</span> <span class="hlt">models</span> can simulate plasma evolution, plasma chemistry, and surface physics <span class="hlt">models</span> with reasonable computational resources by not explicitly resolving electron motions, which thereby leads to an increase in the time step. This is achieved by solving <span class="hlt">fluid</span> motions coupled with electromagnetics using reduced-physics <span class="hlt">models</span>, such as single-temperature magnetohydrodynamics (MHD), extended, gas dynamic, and Hall MHD, and two-<span class="hlt">fluid</span> MHD <span class="hlt">models</span>. We show recent results on <span class="hlt">modeling</span> the internal antenna H{sup −} ion source for the SNS at Oak Ridge National Laboratory using the <span class="hlt">fluid</span> plasma <span class="hlt">modeling</span> code USim. We compare demonstrate plasma temperature equilibration in two</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/24717547','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/24717547"><span>Transesterification reaction for synthesis of palm-<span class="hlt">based</span> ethylhexyl ester and formulation as <span class="hlt">base</span> oil for synthetic drilling <span class="hlt">fluid</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Abdul Habib, Nor Saiful Hafiz; Yunus, Robiah; Rashid, Umer; Taufiq-Yap, Yun H; Abidin, Zurina Zainal; Syam, Azhari Muhammad; Irawan, Sonny</p> <p>2014-01-01</p> <p>The use of vegetable oil-<span class="hlt">based</span> ester as a <span class="hlt">base</span> <span class="hlt">fluid</span> in synthetic drilling <span class="hlt">fluid</span> has become a trend in drilling operations due to its environmental advantages. The transesterification reaction of palm oil methyl ester (POME) with 2-ethylhexanol (2EH) produced 98% of palm oil-<span class="hlt">based</span> ethylhexyl ester in less than 30 minutes. Since the transesterification reaction of POME with 2EH is a reversible reaction, its kinetics was studied in the presence of excess EH and under vacuum. The POME-to-EH molar ratio and vacuum pressure were held constant at 1:2 and 1.5 mbar respectively and the effects of temperature (70 to 110°C) were investigated. Using excess of EH and continual withdrawal of methanol via vacuum promoted the reaction to complete in less than 10 minutes. The rate constant of the reaction (k) obtained from the kinetics study was in the range of 0.44 to 0.66 s⁻¹ and the activation energy was 15.6 kJ.mol⁻¹. The preliminary investigations on the lubrication properties of drilling mud formulated with palm oil-<span class="hlt">based</span> 2EH ester indicated that the <span class="hlt">base</span> oil has a great potential to substitute the synthetic ester-<span class="hlt">based</span> oil for drilling <span class="hlt">fluid</span>. Its high kinematic viscosity provides better lubrication to the drilling <span class="hlt">fluid</span> compared to other ester-<span class="hlt">based</span> oils. The pour point (-15°C) and flash point (204°C) values are superior for the drilling <span class="hlt">fluid</span> formulation. The plastic viscosity, HPHT filtrate loss and emulsion stability of the drilling <span class="hlt">fluid</span> had given acceptable values, while gel strength and yield point could be improved by blending it with proper additives.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016cems.book..385P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016cems.book..385P"><span>A Computational <span class="hlt">Fluid</span> Dynamic <span class="hlt">Model</span> for a Novel Flash Ironmaking Process</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Perez-Fontes, Silvia E.; Sohn, Hong Yong; Olivas-Martinez, Miguel</p> <p></p> <p>A computational <span class="hlt">fluid</span> dynamic <span class="hlt">model</span> for a novel flash ironmaking process <span class="hlt">based</span> on the direct gaseous reduction of iron oxide concentrates is presented. The <span class="hlt">model</span> solves the three-dimensional governing equations including both gas-phase and gas-solid reaction kinetics. The turbulence-chemistry interaction in the gas-phase is <span class="hlt">modeled</span> by the eddy dissipation concept incorporating chemical kinetics. The particle cloud <span class="hlt">model</span> is used to track the particle phase in a Lagrangian framework. A nucleation and growth kinetics rate expression is adopted to calculate the reduction rate of magnetite concentrate particles. Benchmark experiments reported in the literature for a nonreacting swirling gas jet and a nonpremixed hydrogen jet flame were simulated for validation. The <span class="hlt">model</span> predictions showed good agreement with measurements in terms of gas velocity, gas temperature and species concentrations. The relevance of the computational <span class="hlt">model</span> for the analysis of a bench reactor operation and the design of an industrial-pilot plant is discussed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22572342-revisiting-low-fidelity-two-fluid-models-gassolids-transport','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22572342-revisiting-low-fidelity-two-fluid-models-gassolids-transport"><span>Revisiting low-fidelity two-<span class="hlt">fluid</span> <span class="hlt">models</span> for gas–solids 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>Adeleke, Najeem, E-mail: najm@psu.edu; Adewumi, Michael, E-mail: m2a@psu.edu; Ityokumbul, Thaddeus</p> <p></p> <p>Two-phase gas–solids transport <span class="hlt">models</span> are widely utilized for process design and automation in a broad range of industrial applications. Some of these applications include proppant transport in gaseous fracking <span class="hlt">fluids</span>, air/gas drilling hydraulics, coal-gasification reactors and food processing units. Systems automation and real time process optimization stand to benefit a great deal from availability of efficient and accurate theoretical <span class="hlt">models</span> for operations data processing. However, <span class="hlt">modeling</span> two-phase pneumatic transport systems accurately requires a comprehensive understanding of gas–solids flow behavior. In this study we discuss the prevailing flow conditions and present a low-fidelity two-<span class="hlt">fluid</span> <span class="hlt">model</span> equation for particulate transport. The modelmore » equations are formulated in a manner that ensures the physical flux term remains conservative despite the inclusion of solids normal stress through the empirical formula for modulus of elasticity. A new set of Roe–Pike averages are presented for the resulting strictly hyperbolic flux term in the system of equations, which was used to develop a Roe-type approximate Riemann solver. The resulting scheme is stable regardless of the choice of flux-limiter. The <span class="hlt">model</span> is evaluated by the prediction of experimental results from both pneumatic riser and air-drilling hydraulics systems. We demonstrate the effect and impact of numerical formulation and choice of numerical scheme on <span class="hlt">model</span> predictions. We illustrate the capability of a low-fidelity one-dimensional two-<span class="hlt">fluid</span> <span class="hlt">model</span> in predicting relevant flow parameters in two-phase particulate systems accurately even under flow regimes involving counter-current flow.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017APS..MAR.M1354E','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017APS..MAR.M1354E"><span>The isotropic local Wigner-Seitz <span class="hlt">model</span>: An accurate theoretical <span class="hlt">model</span> for the quasi-free electron energy in <span class="hlt">fluids</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Evans, Cherice; Findley, Gary L.</p> <p></p> <p>The quasi-free electron energy V0 (ρ) is important in understanding electron transport through a <span class="hlt">fluid</span>, as well as for <span class="hlt">modeling</span> electron attachment reactions in <span class="hlt">fluids</span>. Our group has developed an isotropic local Wigner-Seitz <span class="hlt">model</span> that allows one to successfully calculate the quasi-free electron energy for a variety of atomic and molecular <span class="hlt">fluids</span> from low density to the density of the triple point liquid with only a single adjustable parameter. This <span class="hlt">model</span>, when coupled with the quasi-free electron energy data and the thermodynamic data for the <span class="hlt">fluids</span>, also can yield optimized intermolecular potential parameters and the zero kinetic energy electron scattering length. In this poster, we give a review of the isotropic local Wigner-Seitz <span class="hlt">model</span> in comparison to previous theoretical <span class="hlt">models</span> for the quasi-free electron energy. All measurements were performed at the University of Wisconsin Synchrotron Radiation Center. This work was supported by a Grants from the National Science Foundation (NSF CHE-0956719), the Petroleum Research Fund (45728-B6 and 5-24880), the Louisiana Board of Regents Support Fund (LEQSF(2006-09)-RD-A33), and the Professional Staff Congress City University of New York.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012AIPC.1479..173R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012AIPC.1479..173R"><span>Mathematical <span class="hlt">modeling</span> of <span class="hlt">fluid</span> flow in aluminum ladles for degasification with impeller - injector</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ramos-Gómez, E.; González-Rivera, C.; Ramírez-Argáez, M. A.</p> <p>2012-09-01</p> <p>In this work a fundamental Eulerian mathematical <span class="hlt">model</span> was developed to simulate <span class="hlt">fluid</span> flow in a water physical <span class="hlt">model</span> of an aluminum ladle equipped with impeller for degassing treatment. The effect of critical process parameters such as rotor speed, gas flow rate on the <span class="hlt">fluid</span> flow and vortex formation was analyzed with this <span class="hlt">model</span>. Commercial CFD code PHOENICS 3.4 was used to solve all conservation equations governing the process for this twophase <span class="hlt">fluid</span> flow system. The mathematical <span class="hlt">model</span> was successfully validated against experimentally measured liquid velocity and turbulent profiles in a physical <span class="hlt">model</span>. From the results it was concluded that the angular speed of the impeller is the most important parameter promoting better stirred baths. Pumping effect of the impeller is increased as impeller rotation speed increases. Gas flow rate is detrimental on bath stirring and diminishes pumping effect of impeller.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010CompM..46...43T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010CompM..46...43T"><span>Role of 0D peripheral vasculature <span class="hlt">model</span> in <span class="hlt">fluid</span>-structure interaction <span class="hlt">modeling</span> of aneurysms</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Torii, Ryo; Oshima, Marie; Kobayashi, Toshio; Takagi, Kiyoshi; Tezduyar, Tayfun E.</p> <p>2010-06-01</p> <p>Patient-specific simulations <span class="hlt">based</span> on medical images such as CT and MRI offer information on the hemodynamic and wall tissue stress in patient-specific aneurysm configurations. These are considered important in predicting the rupture risk for individual aneurysms but are not possible to measure directly. In this paper, <span class="hlt">fluid</span>-structure interaction (FSI) analyses of a cerebral aneurysm at the middle cerebral artery (MCA) bifurcation are presented. A 0D structural recursive tree <span class="hlt">model</span> of the peripheral vasculature is incorporated and its impedance is coupled with the 3D FSI <span class="hlt">model</span> to compute the outflow through the two branches accurately. The results are compared with FSI simulation with prescribed pressure variation at the outlets. The comparison shows that the pressure at the two outlets are nearly identical even with the peripheral vasculature <span class="hlt">model</span> and the flow division to the two branches is nearly the same as what we see in the simulation without the peripheral vasculature <span class="hlt">model</span>. This suggests that the role of the peripheral vasculature in FSI <span class="hlt">modeling</span> of the MCA aneurysm is not significant.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012EGUGA..14.7483G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012EGUGA..14.7483G"><span>Effect of non-linear <span class="hlt">fluid</span> pressure diffusion on <span class="hlt">modeling</span> induced seismicity during reservoir stimulation</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Gischig, V.; Goertz-Allmann, B. P.; Bachmann, C. E.; Wiemer, S.</p> <p>2012-04-01</p> <p>Success of future enhanced geothermal systems relies on an appropriate pre-estimate of seismic risk associated with <span class="hlt">fluid</span> injection at high pressure. A forward-<span class="hlt">model</span> <span class="hlt">based</span> on a semi-stochastic approach was created, which is able to compute synthetic earthquake catalogues. It proved to be able to reproduce characteristics of the seismic cloud detected during the geothermal project in Basel (Switzerland), such as radial dependence of stress drop and b-values as well as higher probability of large magnitude earthquakes (M>3) after shut-in. The <span class="hlt">modeling</span> strategy relies on a simplistic <span class="hlt">fluid</span> pressure <span class="hlt">model</span> used to trigger failure points (so-called seeds) that are randomly distributed around an injection well. The seed points are assigned principal stress magnitudes drawn from Gaussian distributions representative of the ambient stress field. Once the effective stress state at a seed point meets a pre-defined Mohr-Coulomb failure criterion due to a <span class="hlt">fluid</span> pressure increase a seismic event is induced. We assume a negative linear relationship between b-values and differential stress. Thus, for each event a magnitude can be drawn from a Gutenberg-Richter distribution with a b-value corresponding to differential stress at failure. The result is a seismic cloud evolving in time and space. Triggering of seismic events depends on appropriately calculating the transient <span class="hlt">fluid</span> pressure field. Hence an effective continuum reservoir <span class="hlt">model</span> able to reasonably reproduce the hydraulic behavior of the reservoir during stimulation is required. While analytical solutions for pressure diffusion are computationally efficient, they rely on linear pressure diffusion with constant hydraulic parameters, and only consider well head pressure while neglecting <span class="hlt">fluid</span> injection rate. They cannot be considered appropriate in a stimulation experiment where permeability irreversibly increases by orders of magnitude during injection. We here suggest a numerical continuum <span class="hlt">model</span> of non-linear pressure</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013PhDT.......224A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013PhDT.......224A"><span>Characterization and <span class="hlt">modeling</span> of the stress and pore-<span class="hlt">fluid</span> dependent acoustic properties of fractured porous rocks</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Almrabat, Abdulhadi M.</p> <p></p> <p>The thesis presents the results of a study of the characterization and <span class="hlt">modeling</span> of the stress and pore-<span class="hlt">fluid</span> dependent acoustic properties of fractured porous rocks. A new laboratory High Pressure and High Temperature (HPHT) triaxial testing system was developed to characterize the seismic properties of sandstone under different levels of effective stress confinement and changes in pore-<span class="hlt">fluid</span> composition. An intact and fractured of Berea sandstones core samples were used in the experimental studies. The laboratory test results were used to develop analytical <span class="hlt">models</span> for stress-level and pore-<span class="hlt">fluid</span> dependent seismic velocity of sandstones. <span class="hlt">Models</span> for stress-dependent P and S-wave seismic velocities of sandstone were then developed <span class="hlt">based</span> on the assumption that stress-dependencies come from the nonlinear elastic response of micro-fractures contained in the sample under normal and shear loading. The contact shear stiffness was assumed to increase linearly with the normal stress across a micro-fracture, while the contact normal stiffness was assumed to vary as a power law with the micro-fracture normal stress. Both nonlinear fracture normal and shear contact <span class="hlt">models</span> were validated by experimental data available in the literature. To test the dependency of seismic velocity of sandstone on changes in pore-<span class="hlt">fluid</span> composition, another series of tests were conducted where P and S-wave velocities were monitored during injection of supercritical CO 2 in samples of Berea sandstone initially saturated with saline water and under constant confining stress. Changes in seismic wave velocity were measured at different levels of supercritical CO2 saturation as the initial saline water as pore-<span class="hlt">fluid</span> was displaced by supercritical CO 2. It was found that the P- iv wave velocity significantly decreased while the S-wave velocity remained almost constant as the sample supercritical CO2 saturation increased. The dependency of the seismic velocity on changes on pore <span class="hlt">fluid</span> composition during</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018GeoRL..45.3471B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018GeoRL..45.3471B"><span>Episodic Tremor and Slip Explained by <span class="hlt">Fluid</span>-Enhanced Microfracturing and Sealing</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bernaudin, M.; Gueydan, F.</p> <p>2018-04-01</p> <p>Episodic tremor and slow-slip events at the deep extension of plate boundary faults illuminate seismic to aseismic processes around the brittle-ductile transition. These events occur in volumes characterized by overpressurized <span class="hlt">fluids</span> and by near failure shear stress conditions. We present a new <span class="hlt">modeling</span> approach <span class="hlt">based</span> on a ductile grain size-sensitive rheology with microfracturing and sealing, which provides a mechanical and field-<span class="hlt">based</span> explanation of such phenomena. We also <span class="hlt">model</span> pore <span class="hlt">fluid</span> pressure variation as a function of changes in porosity/permeability and strain rate-dependent <span class="hlt">fluid</span> pumping. The <span class="hlt">fluid</span>-enhanced dynamic evolution of microstructures defines cycles of ductile strain localization and implies increase in pore <span class="hlt">fluid</span> pressure. We propose that slow-slip events are ductile processes related to transient strain localization, while nonvolcanic tremor corresponds to fracturing of the whole rock at the peak of pore <span class="hlt">fluid</span> pressure. Our <span class="hlt">model</span> shows that the availability of <span class="hlt">fluids</span> and the efficiency of <span class="hlt">fluid</span> pumping control the occurrence and the P-T conditions of episodic tremor and slip.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20120002024','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20120002024"><span>Three-<span class="hlt">Fluid</span> Magnetohydrodynamic <span class="hlt">Modeling</span> of the Solar Wind in the Outer Heliosphere</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Usmanov, Arcadi V.; Goldstein, Melvyn L.; Matthaeus, William H.</p> <p>2011-01-01</p> <p>We have developed a three-<span class="hlt">fluid</span>, fully three-dimensional magnetohydrodynamic <span class="hlt">model</span> of the solar wind plasma in the outer heliosphere as a co-moving system of solar wind protons, electrons, and interstellar pickup protons, with separate energy equations for each species. Our approach takes into account the effects of electron heat conduction and dissipation of Alfvenic turbulence on the spatial evolution of the solar wind plasma and interplanetary magnetic fields. The turbulence transport <span class="hlt">model</span> is <span class="hlt">based</span> on the Reynolds decomposition of physical variables into mean and fluctuating components and uses the turbulent phenomenologies that describe the conversion of fluctuation energy into heat due to a turbulent cascade. We solve the coupled set of the three-<span class="hlt">fluid</span> equations for the mean-field solar wind and the turbulence equations for the turbulence energy, cross helicity, and correlation length. The equations are written in the rotating frame of reference and include heating by turbulent dissipation, energy transfer from interstellar pickup protons to solar wind protons, and solar wind deceleration due to the interaction with the interstellar hydrogen. The numerical solution is constructed by the time relaxation method in the region from 0.3 to 100 AU. Initial results from the novel <span class="hlt">model</span> are presented.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1395816','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/1395816"><span>Advanced <span class="hlt">Fluid</span> Reduced Order <span class="hlt">Models</span> for Compressible Flow.</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>Tezaur, Irina Kalashnikova; Fike, Jeffrey A.; Carlberg, Kevin Thomas</p> <p></p> <p>This report summarizes fiscal year (FY) 2017 progress towards developing and implementing within the SPARC in-house finite volume flow solver advanced <span class="hlt">fluid</span> reduced order <span class="hlt">models</span> (ROMs) for compressible captive-carriage flow problems of interest to Sandia National Laboratories for the design and qualification of nuclear weapons components. The proposed projection-<span class="hlt">based</span> <span class="hlt">model</span> order reduction (MOR) approach, known as the Proper Orthogonal Decomposition (POD)/Least- Squares Petrov-Galerkin (LSPG) method, can substantially reduce the CPU-time requirement for these simulations, thereby enabling advanced analyses such as uncertainty quantification and de- sign optimization. Following a description of the project objectives and FY17 targets, we overview briefly themore » POD/LSPG approach to <span class="hlt">model</span> reduction implemented within SPARC . We then study the viability of these ROMs for long-time predictive simulations in the context of a two-dimensional viscous laminar cavity problem, and describe some FY17 enhancements to the proposed <span class="hlt">model</span> reduction methodology that led to ROMs with improved predictive capabilities. Also described in this report are some FY17 efforts pursued in parallel to the primary objective of determining whether the ROMs in SPARC are viable for the targeted application. These include the implemen- tation and verification of some higher-order finite volume discretization methods within SPARC (towards using the code to study the viability of ROMs on three-dimensional cavity problems) and a novel structure-preserving constrained POD/LSPG formulation that can improve the accuracy of projection-<span class="hlt">based</span> reduced order <span class="hlt">models</span>. We conclude the report by summarizing the key takeaways from our FY17 findings, and providing some perspectives for future work.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=2914853','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=2914853"><span>Differential Geometry <span class="hlt">Based</span> Multiscale <span class="hlt">Models</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>Wei, Guo-Wei</p> <p>2010-01-01</p> <p>Large chemical and biological systems such as fuel cells, ion channels, molecular motors, and viruses are of great importance to the scientific community and public health. Typically, these complex systems in conjunction with their aquatic environment pose a fabulous challenge to theoretical description, simulation, and prediction. In this work, we propose a differential geometry <span class="hlt">based</span> multiscale paradigm to <span class="hlt">model</span> complex macromolecular systems, and to put macroscopic and microscopic descriptions on an equal footing. In our approach, the differential geometry theory of surfaces and geometric measure theory are employed as a natural means to couple the macroscopic continuum mechanical description of the aquatic environment with the microscopic discrete atom-istic description of the macromolecule. Multiscale free energy functionals, or multiscale action functionals are constructed as a unified framework to derive the governing equations for the dynamics of different scales and different descriptions. Two types of aqueous macromolecular complexes, ones that are near equilibrium and others that are far from equilibrium, are considered in our formulations. We show that generalized Navier–Stokes equations for the <span class="hlt">fluid</span> dynamics, generalized Poisson equations or generalized Poisson–Boltzmann equations for electrostatic interactions, and Newton's equation for the molecular dynamics can be derived by the least action principle. These equations are coupled through the continuum-discrete interface whose dynamics is governed by potential driven geometric flows. Comparison is given to classical descriptions of the <span class="hlt">fluid</span> and electrostatic interactions without geometric flow <span class="hlt">based</span> micro-macro interfaces. The detailed balance of forces is emphasized in the present work. We further extend the proposed multiscale paradigm to micro-macro analysis of electrohydrodynamics, electrophoresis, fuel cells, and ion channels. We derive generalized Poisson–Nernst–Planck equations that</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017MS%26E..276a2010H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017MS%26E..276a2010H"><span>Multi-<span class="hlt">fluid</span> CFD analysis in Process Engineering</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hjertager, B. H.</p> <p>2017-12-01</p> <p>An overview of <span class="hlt">modelling</span> and simulation of flow processes in gas/particle and gas/liquid systems are presented. Particular emphasis is given to computational <span class="hlt">fluid</span> dynamics (CFD) <span class="hlt">models</span> that use the multi-dimensional multi-<span class="hlt">fluid</span> techniques. Turbulence <span class="hlt">modelling</span> strategies for gas/particle flows <span class="hlt">based</span> on the kinetic theory for granular flows are given. Sub <span class="hlt">models</span> for the interfacial transfer processes and chemical kinetics <span class="hlt">modelling</span> are presented. Examples are shown for some gas/particle systems including flow and chemical reaction in risers as well as gas/liquid systems including bubble columns and stirred tanks.</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/2013PhFl...25g6603B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013PhFl...25g6603B"><span><span class="hlt">Modeling</span> the purging of dense <span class="hlt">fluid</span> from a street canyon driven by an interfacial mixing flow and skimming flow</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Baratian-Ghorghi, Z.; Kaye, N. B.</p> <p>2013-07-01</p> <p>An experimental study is presented to investigate the mechanism of flushing a trapped dense contaminant from a canyon by turbulent boundary layer flow. The results of a series of steady-state experiments are used to parameterize the flushing mechanisms. The steady-state experimental results for a canyon with aspect ratio one indicate that dense <span class="hlt">fluid</span> is removed from the canyon by two different processes, skimming of dense <span class="hlt">fluid</span> from the top of the dense layer; and by an interfacial mixing flow that mixes fresh <span class="hlt">fluid</span> down into the dense lower layer (entrainment) while mixing dense <span class="hlt">fluid</span> into the flow above the canyon (detrainment). A <span class="hlt">model</span> is developed for the time varying buoyancy profile within the canyon as a function of the Richardson number which parameterizes both the interfacial mixing and skimming processes observed. The continuous release steady-state experiments allowed for the direct measurement of the skimming and interfacial mixing flow rates for any layer depth and Richardson number. Both the skimming rate and the interfacial mixing rate were found to be power-law functions of the Richardson number of the layer. The <span class="hlt">model</span> results were compared to the results of previously published finite release experiments [Z. Baratian-Ghorghi and N. B. Kaye, Atmos. Environ. 60, 392-402 (2012)], 10.1016/j.atmosenv.2012.06.077. A high degree of consistency was found between the finite release data and the continuous release data. This agreement acts as an excellent check on the measurement techniques used, as the finite release data was <span class="hlt">based</span> on curve fitting through buoyancy versus time data, while the continuous release data was calculated directly by measuring the rate of addition of volume and buoyancy once a steady-state was established. Finally, a system of ordinary differential equations is presented to <span class="hlt">model</span> the removal of dense <span class="hlt">fluid</span> from the canyon <span class="hlt">based</span> on empirical correlations of the skimming and interfacial mixing taken form the steady-state experiments</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1997CoMP..129..198C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1997CoMP..129..198C"><span>Permeability generation and resetting of tracers during metamorphic <span class="hlt">fluid</span> flow: implications for advection-dispersion <span class="hlt">models</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Cartwright, Ian</p> <p></p> <p>Advection-dispersion <span class="hlt">fluid</span> flow <span class="hlt">models</span> implicitly assume that the infiltrating <span class="hlt">fluid</span> flows through an already <span class="hlt">fluid</span>-saturated medium. However, whether rocks contain a <span class="hlt">fluid</span> depends on their reaction history, and whether any initial <span class="hlt">fluid</span> escapes. The behaviour of different rocks may be illustrated using hypothetical marble compositions. Marbles with diverse chemistries (e.g. calcite + dolomite + quartz) are relatively reactive, and will generally produce a <span class="hlt">fluid</span> during heating. By contrast, marbles with more restricted chemistries (e.g. calcite + quartz or calcite-only) may not. If the rock is not <span class="hlt">fluid</span> bearing when <span class="hlt">fluid</span> infiltration commences, mineralogical reactions may produce a reaction-enhanced permeability in calcite + dolomite + quartz or calcite + quartz, but not in calcite-only marbles. The permeability production controls the pattern of mineralogical, isotopic, and geochemical resetting during <span class="hlt">fluid</span> flow. Tracers retarded behind the mineralogical fronts will probably be reset as predicted by the advection-dispersion <span class="hlt">models</span>; however, tracers that are expected to be reset ahead of the mineralogical fronts cannot progress beyond the permeability generating reaction. In the case of very unreactive lithologies (e.g. pure calcite marbles, cherts, and quartzites), the first reaction to affect the rocks may be a metasomatic one ahead of which there is little pervasive resetting of any tracer. Centimetre-scale layering may lead to the formation of self-perpetuating <span class="hlt">fluid</span> channels in rocks that are not <span class="hlt">fluid</span> saturated due to the juxtaposition of reactants. Such layered rocks may show patterns of mineralogical resetting that are not predicted by advection-dispersion <span class="hlt">models</span>. Patterns of mineralogical and isotopic resetting in marbles from a number of terrains, for example: Chillagoe, Marulan South, Reynolds Range (Australia); Adirondack Mountains, Old Woman Mountains, Notch Peak (USA); and Stephen Cross Quarry (Canada) vary as predicted by these <span class="hlt">models</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009EGUGA..1111650S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009EGUGA..1111650S"><span>Characterization of <span class="hlt">fluids</span> and <span class="hlt">fluid-fluid</span> interaction by fiber optic refractive index sensor measurements</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Schmidt-Hattenberger, C.; Weiner, M.; Liebscher, A.; Spangenberg, E.</p> <p>2009-04-01</p> <p>A fiber optic refractive index sensor is tested for continuous monitoring of <span class="hlt">fluid-fluid</span> and <span class="hlt">fluid</span>-gas interactions within the frame of laboratory investigations of CO2 storage, monitoring and safety technology research (COSMOS project, "Geotechnologien" program). The sensor <span class="hlt">bases</span> on a Fabry-Perot white light interferometer technique, where the refractive index (RI) of the solution under investigation is measured by variation of the liquid-filled Fabry-Perot optical cavity length. Such sensor system is typically used for measuring and controlling oil composition and also <span class="hlt">fluid</span> quality. The aim of this study is to test the application of the fiber optic refractive index sensor for monitoring the CO2 dissolution in formation <span class="hlt">fluids</span> (brine, oil, gas) of CO2 storage sites. Monitoring and knowledge of quantity and especially rate of CO2 dissolution in the formation <span class="hlt">fluid</span> is important for any assessment of long-term risks of CO2 storage sites. It is also a prerequisite for any precise reservoir <span class="hlt">modelling</span>. As a first step we performed laboratory experiments in standard autoclaves on a variety of different <span class="hlt">fluids</span> and <span class="hlt">fluid</span> mixtures (technical alcohols, pure water, CO2, synthetic brines, natural formation brine from the Ketzin test site). The RI measurements are partly combined with default electrical conductivity and sonic velocity measurements. The fiber optic refractive index sensor system allows for RI measurements within the range 1.0000 to 1.7000 RI with a resolution of approximately 0.0001 RI. For simple binary <span class="hlt">fluid</span> mixtures first results indicate linear relationships between refractive indices and <span class="hlt">fluid</span> composition. Within the pressure range investigated (up to 60 bar) the data suggest only minor changes of RI with pressure. Further, planned experiments will focus on the determination of i) the temperature dependency of RI, ii) the combined effects of pressure and temperature on RI, and finally iii) the kinetics of CO2 dissolution in realistic formation <span class="hlt">fluids</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018ExFl...59...22L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018ExFl...59...22L"><span>Accurate <span class="hlt">fluid</span> force measurement <span class="hlt">based</span> on control surface integration</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lentink, David</p> <p>2018-01-01</p> <p>Nonintrusive 3D <span class="hlt">fluid</span> force measurements are still challenging to conduct accurately for freely moving animals, vehicles, and deforming objects. Two techniques, 3D particle image velocimetry (PIV) and a new technique, the aerodynamic force platform (AFP), address this. Both rely on the control volume integral for momentum; whereas PIV requires numerical integration of flow fields, the AFP performs the integration mechanically <span class="hlt">based</span> on rigid walls that form the control surface. The accuracy of both PIV and AFP measurements <span class="hlt">based</span> on the control surface integration is thought to hinge on determining the unsteady body force associated with the acceleration of the volume of displaced <span class="hlt">fluid</span>. Here, I introduce a set of non-dimensional error ratios to show which <span class="hlt">fluid</span> and body parameters make the error negligible. The unsteady body force is insignificant in all conditions where the average density of the body is much greater than the density of the <span class="hlt">fluid</span>, e.g., in gas. Whenever a strongly deforming body experiences significant buoyancy and acceleration, the error is significant. Remarkably, this error can be entirely corrected for with an exact factor provided that the body has a sufficiently homogenous density or acceleration distribution, which is common in liquids. The correction factor for omitting the unsteady body force, {{{ {ρ f}} {1 - {ρ f} ( {{ρ b}+{ρ f}} )}.{( {{{{ρ }}b}+{ρ f}} )}}} , depends only on the <span class="hlt">fluid</span>, {ρ f}, and body, {{ρ }}b, density. Whereas these straightforward solutions work even at the liquid-gas interface in a significant number of cases, they do not work for generalized bodies undergoing buoyancy in combination with appreciable body density inhomogeneity, volume change (PIV), or volume rate-of-change (PIV and AFP). In these less common cases, the 3D body shape needs to be measured and resolved in time and space to estimate the unsteady body force. The analysis shows that accounting for the unsteady body force is straightforward to non</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018CNSNS..57..449H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018CNSNS..57..449H"><span><span class="hlt">Modeling</span> meniscus rise in capillary tubes using <span class="hlt">fluid</span> in rigid-body motion approach</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hamdan, Mohammad O.; Abu-Nabah, Bassam A.</p> <p>2018-04-01</p> <p>In this study, a new term representing net flux rate of linear momentum is introduced to Lucas-Washburn equation. Following a <span class="hlt">fluid</span> in rigid-body motion in <span class="hlt">modeling</span> the meniscus rise in vertical capillary tubes transforms the nonlinear Lucas-Washburn equation to a linear mass-spring-damper system. The linear nature of mass-spring-damper system with constant coefficients offers a nondimensional analytical solution where meniscus dynamics are dictated by two parameters, namely the system damping ratio and its natural frequency. This connects the numerous <span class="hlt">fluid</span>-surface interaction physical and geometrical properties to rather two nondimensional parameters, which capture the underlying physics of meniscus dynamics in three distinct cases, namely overdamped, critically damped, and underdamped systems. <span class="hlt">Based</span> on experimental data available in the literature and the understanding meniscus dynamics, the proposed <span class="hlt">model</span> brings a new approach of understanding the system initial conditions. Accordingly, a closed form relation is produced for the imbibition velocity, which equals half of the Bosanquet velocity divided by the damping ratio. The proposed general analytical <span class="hlt">model</span> is ideal for overdamped and critically damped systems. While for underdamped systems, the solution shows fair agreement with experimental measurements once the effective viscosity is determined. Moreover, the presented <span class="hlt">model</span> shows meniscus oscillations around equilibrium height occur if the damping ratio is less than one.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/22138194','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/22138194"><span>Validation of a 3D computational <span class="hlt">fluid</span>-structure interaction <span class="hlt">model</span> simulating flow through an elastic aperture.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Quaini, A; Canic, S; Glowinski, R; Igo, S; Hartley, C J; Zoghbi, W; Little, S</p> <p>2012-01-10</p> <p>This work presents a validation of a <span class="hlt">fluid</span>-structure interaction computational <span class="hlt">model</span> simulating the flow conditions in an in vitro mock heart chamber <span class="hlt">modeling</span> mitral valve regurgitation during the ejection phase during which the trans-valvular pressure drop and valve displacement are not as large. The mock heart chamber was developed to study the use of 2D and 3D color Doppler techniques in imaging the clinically relevant complex intra-cardiac flow events associated with mitral regurgitation. Computational <span class="hlt">models</span> are expected to play an important role in supporting, refining, and reinforcing the emerging 3D echocardiographic applications. We have developed a 3D computational <span class="hlt">fluid</span>-structure interaction algorithm <span class="hlt">based</span> on a semi-implicit, monolithic method, combined with an arbitrary Lagrangian-Eulerian approach to capture the <span class="hlt">fluid</span> domain motion. The mock regurgitant mitral valve corresponding to an elastic plate with a geometric orifice, was <span class="hlt">modeled</span> using 3D elasticity, while the blood flow was <span class="hlt">modeled</span> using the 3D Navier-Stokes equations for an incompressible, viscous <span class="hlt">fluid</span>. The two are coupled via the kinematic and dynamic conditions describing the two-way coupling. The pressure, the flow rate, and orifice plate displacement were measured and compared with numerical simulation results. In-line flow meter was used to measure the flow, pressure transducers were used to measure the pressure, and a Doppler method developed by one of the authors was used to measure the axial displacement of the orifice plate. The maximum recorded difference between experiment and numerical simulation for the flow rate was 4%, the pressure 3.6%, and for the orifice displacement 15%, showing excellent agreement between the two. Copyright © 2011 Elsevier Ltd. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017PhRvE..95f3302A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017PhRvE..95f3302A"><span>Asymptotic <span class="hlt">modeling</span> of transport phenomena at the interface between a <span class="hlt">fluid</span> and a porous layer: Jump conditions</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Angot, Philippe; Goyeau, Benoît; Ochoa-Tapia, J. Alberto</p> <p>2017-06-01</p> <p>We develop asymptotic <span class="hlt">modeling</span> for two- or three-dimensional viscous <span class="hlt">fluid</span> flow and convective transfer at the interface between a <span class="hlt">fluid</span> and a porous layer. The asymptotic <span class="hlt">model</span> is <span class="hlt">based</span> on the fact that the thickness d of the interfacial transition region Ωfp of the one-domain representation is very small compared to the macroscopic length scale L . The analysis leads to an equivalent two-domain representation where transport phenomena in the transition layer of the one-domain approach are represented by algebraic jump boundary conditions at a fictive dividing interface Σ between the homogeneous <span class="hlt">fluid</span> and porous regions. These jump conditions are thus stated up to first-order in O (d /L ) with d /L ≪1 . The originality and relevance of this asymptotic <span class="hlt">model</span> lies in its general and multidimensional character. Indeed, it is shown that all the jump interface conditions derived for the commonly used 1D-shear flow are recovered by taking the tangential component of the asymptotic <span class="hlt">model</span>. In that case, the comparison between the present <span class="hlt">model</span> and the different <span class="hlt">models</span> available in the literature gives explicit expressions of the effective jump coefficients and their associated scaling. In addition for multi-dimensional flows, the general asymptotic <span class="hlt">model</span> yields the different components of the jump conditions including a new specific equation for the cross-flow pressure jump on Σ .</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28709346','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28709346"><span>Asymptotic <span class="hlt">modeling</span> of transport phenomena at the interface between a <span class="hlt">fluid</span> and a porous layer: Jump conditions.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Angot, Philippe; Goyeau, Benoît; Ochoa-Tapia, J Alberto</p> <p>2017-06-01</p> <p>We develop asymptotic <span class="hlt">modeling</span> for two- or three-dimensional viscous <span class="hlt">fluid</span> flow and convective transfer at the interface between a <span class="hlt">fluid</span> and a porous layer. The asymptotic <span class="hlt">model</span> is <span class="hlt">based</span> on the fact that the thickness d of the interfacial transition region Ω_{fp} of the one-domain representation is very small compared to the macroscopic length scale L. The analysis leads to an equivalent two-domain representation where transport phenomena in the transition layer of the one-domain approach are represented by algebraic jump boundary conditions at a fictive dividing interface Σ between the homogeneous <span class="hlt">fluid</span> and porous regions. These jump conditions are thus stated up to first-order in O(d/L) with d/L≪1. The originality and relevance of this asymptotic <span class="hlt">model</span> lies in its general and multidimensional character. Indeed, it is shown that all the jump interface conditions derived for the commonly used 1D-shear flow are recovered by taking the tangential component of the asymptotic <span class="hlt">model</span>. In that case, the comparison between the present <span class="hlt">model</span> and the different <span class="hlt">models</span> available in the literature gives explicit expressions of the effective jump coefficients and their associated scaling. In addition for multi-dimensional flows, the general asymptotic <span class="hlt">model</span> yields the different components of the jump conditions including a new specific equation for the cross-flow pressure jump on Σ.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JHyDy..30...49K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JHyDy..30...49K"><span>Towards development of enhanced fully-Lagrangian mesh-free computational methods for <span class="hlt">fluid</span>-structure interaction</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Khayyer, Abbas; Gotoh, Hitoshi; Falahaty, Hosein; Shimizu, Yuma</p> <p>2018-02-01</p> <p>Simulation of incompressible <span class="hlt">fluid</span> flow-elastic structure interactions is targeted by using fully-Lagrangian mesh-free computational methods. A projection-<span class="hlt">based</span> <span class="hlt">fluid</span> <span class="hlt">model</span> (moving particle semi-implicit (MPS)) is coupled with either a Newtonian or a Hamiltonian Lagrangian structure <span class="hlt">model</span> (MPS or HMPS) in a mathematically-physically consistent manner. The <span class="hlt">fluid</span> <span class="hlt">model</span> is founded on the solution of Navier-Stokes and continuity equations. The structure <span class="hlt">models</span> are configured either in the framework of Newtonian mechanics on the basis of conservation of linear and angular momenta, or Hamiltonian mechanics on the basis of variational principle for incompressible elastodynamics. A set of enhanced schemes are incorporated for projection-<span class="hlt">based</span> <span class="hlt">fluid</span> <span class="hlt">model</span> (Enhanced MPS), thus, the developed coupled solvers for <span class="hlt">fluid</span> structure interaction (FSI) are referred to as Enhanced MPS-MPS and Enhanced MPS-HMPS. Besides, two smoothed particle hydrodynamics (SPH)-<span class="hlt">based</span> FSI solvers, being developed by the authors, are considered and their potential applicability and comparable performance are briefly discussed in comparison with MPS-<span class="hlt">based</span> FSI solvers. The SPH-<span class="hlt">based</span> FSI solvers are established through coupling of projection-<span class="hlt">based</span> incompressible SPH (ISPH) <span class="hlt">fluid</span> <span class="hlt">model</span> and SPH-<span class="hlt">based</span> Newtonian/Hamiltonian structure <span class="hlt">models</span>, leading to Enhanced ISPH-SPH and Enhanced ISPH-HSPH. A comparative study is carried out on the performances of the FSI solvers through a set of benchmark tests, including hydrostatic water column on an elastic plate, high speed impact of an elastic aluminum beam, hydroelastic slamming of a marine panel and dam break with elastic gate.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20150016531','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20150016531"><span>Generalized <span class="hlt">Fluid</span> System Simulation Program (GFSSP) - Version 6</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Majumdar, Alok; LeClair, Andre; Moore, Ric; Schallhorn, Paul</p> <p>2015-01-01</p> <p>The Generalized <span class="hlt">Fluid</span> System Simulation Program (GFSSP) is a finite-volume <span class="hlt">based</span> general-purpose computer program for analyzing steady state and time-dependent flow rates, pressures, temperatures, and concentrations in a complex flow network. The program is capable of <span class="hlt">modeling</span> real <span class="hlt">fluids</span> with phase changes, compressibility, mixture thermodynamics, conjugate heat transfer between solid and <span class="hlt">fluid</span>, <span class="hlt">fluid</span> transients, pumps, compressors, flow control valves and external body forces such as gravity and centrifugal. The thermo-<span class="hlt">fluid</span> system to be analyzed is discretized into nodes, branches, and conductors. The scalar properties such as pressure, temperature, and concentrations are calculated at nodes. Mass flow rates and heat transfer rates are computed in branches and conductors. The graphical user interface allows users to build their <span class="hlt">models</span> using the 'point, drag, and click' method; the users can also run their <span class="hlt">models</span> and post-process the results in the same environment. The integrated <span class="hlt">fluid</span> library supplies thermodynamic and thermo-physical properties of 36 <span class="hlt">fluids</span>, and 24 different resistance/source options are provided for <span class="hlt">modeling</span> momentum sources or sinks in the branches. Users can introduce new physics, non-linear and time-dependent boundary conditions through user-subroutine.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20140003178','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20140003178"><span>Generalized <span class="hlt">Fluid</span> System Simulation Program, Version 6.0</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Majumdar, A. K.; LeClair, A. C.; Moore, A.; Schallhorn, P. A.</p> <p>2013-01-01</p> <p>The Generalized <span class="hlt">Fluid</span> System Simulation Program (GFSSP) is a finite-volume <span class="hlt">based</span> general-purpose computer program for analyzing steady state and time-dependant flow rates, pressures, temperatures, and concentrations in a complex flow network. The program is capable of <span class="hlt">modeling</span> real <span class="hlt">fluids</span> with phase changes, compressibility, mixture thermodynamics, conjugate heat transfer between solid and <span class="hlt">fluid</span>, <span class="hlt">fluid</span> transients, pumps, compressors and external body forces such as gravity and centrifugal. The thermo-<span class="hlt">fluid</span> system to be analyzed is discretized into nodes, branches, and conductors. The scalar properties such as pressure, temperature, and concentrations are calculated at nodes. Mass flow rates and heat transfer rates are computed in branches and conductors. The graphical user interface allows users to build their <span class="hlt">models</span> using the 'point, drag, and click' method; the users can also run their <span class="hlt">models</span> and post-process the results in the same environment. The integrated <span class="hlt">fluid</span> library supplies thermodynamic and thermo-physical properties of 36 <span class="hlt">fluids</span>, and 24 different resistance/source options are provided for <span class="hlt">modeling</span> momentum sources or sinks in the branches. This Technical Memorandum illustrates the application and verification of the code through 25 demonstrated example problems.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017PhDT.......288M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017PhDT.......288M"><span>Analysis and <span class="hlt">Modeling</span> of Structure Formation in Granular and <span class="hlt">Fluid</span>-Solid Flows</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Murphy, Eric</p> <p></p> <p>Granular and multiphase flows are encountered in a number of industrial processes with particular emphasis in this manuscript given to the particular applications in cement pumping, pneumatic conveying, <span class="hlt">fluid</span> catalytic cracking, CO2 capture, and fast pyrolysis of bio-materials. These processes are often <span class="hlt">modeled</span> using averaged equations that may be simulated using computational <span class="hlt">fluid</span> dynamics. Closure <span class="hlt">models</span> are then required that describe the average forces that arise from both interparticle interactions, e.g. shear stress, and interphase interactions, such as mean drag. One of the biggest hurdles to this approach is the emergence of non-trivial spatio-temporal structures in the particulate phase, which can significantly modify the qualitative behavior of these forces and the resultant flow phenomenology. For example, the formation of large clusters in cohesive granular flows is responsible for a transition from solid-like to <span class="hlt">fluid</span>-like rheology. Another example is found in gas-solid systems, where clustering at small scales is observed to significantly lower in the observed drag. Moreover, there remains the possibility that structure formation may occur at all scales, leading to a lack of scale separation required for traditional averaging approaches. In this context, several <span class="hlt">modeling</span> problems are treated 1) first-principles <span class="hlt">based</span> <span class="hlt">modeling</span> of the rheology of cement slurries, 2) <span class="hlt">modeling</span> the mean solid-solid drag experienced by polydisperse particles undergoing segregation, and 3) <span class="hlt">modeling</span> clustering in homogeneous gas-solid flows. The first and third components are described in greater detail. In the study on the rheology of cements, several sub-problems are introduced, which systematically increase in the number and complexity of interparticle interactions. These interparticle interactions include inelasticity, friction, cohesion, and <span class="hlt">fluid</span> interactions. In the first study, the interactions between cohesive inelastic particles was fully characterized for the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/22526836','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/22526836"><span>A mixture theory <span class="hlt">model</span> of <span class="hlt">fluid</span> and solute transport in the microvasculature of normal and malignant tissues. I. Theory.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Schuff, M M; Gore, J P; Nauman, E A</p> <p>2013-05-01</p> <p>In order to better understand the mechanisms governing transport of drugs, nanoparticle-<span class="hlt">based</span> treatments, and therapeutic biomolecules, and the role of the various physiological parameters, a number of mathematical <span class="hlt">models</span> have previously been proposed. The limitations of the existing transport <span class="hlt">models</span> indicate the need for a comprehensive <span class="hlt">model</span> that includes transport in the vessel lumen, the vessel wall, and the interstitial space and considers the effects of the solute concentration on <span class="hlt">fluid</span> flow. In this study, a general <span class="hlt">model</span> to describe the transient distribution of <span class="hlt">fluid</span> and multiple solutes at the microvascular level was developed using mixture theory. The <span class="hlt">model</span> captures the experimentally observed dependence of the hydraulic permeability coefficient of the capillary wall on the concentration of solutes present in the capillary wall and the surrounding tissue. Additionally, the <span class="hlt">model</span> demonstrates that transport phenomena across the capillary wall and in the interstitium are related to the solute concentration as well as the hydrostatic pressure. The <span class="hlt">model</span> is used in a companion paper to examine <span class="hlt">fluid</span> and solute transport for the simplified case of an axisymmetric geometry with no solid deformation or interconversion of mass.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28596520','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28596520"><span>A Comprehensive Prediction <span class="hlt">Model</span> of Hydraulic Extended-Reach Limit Considering the Allowable Range of Drilling <span class="hlt">Fluid</span> Flow Rate in Horizontal Drilling.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Li, Xin; Gao, Deli; Chen, Xuyue</p> <p>2017-06-08</p> <p>Hydraulic extended-reach limit (HERL) <span class="hlt">model</span> of horizontal extended-reach well (ERW) can predict the maximum measured depth (MMD) of the horizontal ERW. The HERL refers to the well's MMD when drilling <span class="hlt">fluid</span> cannot be normally circulated by drilling pump. Previous <span class="hlt">model</span> analyzed the following two constraint conditions, drilling pump rated pressure and rated power. However, effects of the allowable range of drilling <span class="hlt">fluid</span> flow rate (Q min  ≤ Q ≤ Q max ) were not considered. In this study, three cases of HERL <span class="hlt">model</span> are proposed according to the relationship between allowable range of drilling <span class="hlt">fluid</span> flow rate and rated flow rate of drilling pump (Q r ). A horizontal ERW is analyzed to predict its HERL, especially its horizontal-section limit (L h ). Results show that when Q min  ≤ Q r  ≤ Q max (Case I), L h depends both on horizontal-section limit <span class="hlt">based</span> on rated pump pressure (L h1 ) and horizontal-section limit <span class="hlt">based</span> on rated pump power (L h2 ); when Q min  < Q max  < Q r (Case II), L h is exclusively controlled by L h1 ; while L h is only determined by L h2 when Q r  < Q min  < Q max (Case III). Furthermore, L h1 first increases and then decreases with the increase in drilling <span class="hlt">fluid</span> flow rate, while L h2 keeps decreasing as the drilling <span class="hlt">fluid</span> flow rate increases. The comprehensive <span class="hlt">model</span> provides a more accurate prediction on HERL.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19870000815','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19870000815"><span>Computational <span class="hlt">fluid</span> mechanics utilizing the variational principle of <span class="hlt">modeling</span> damping seals</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Abernathy, J. M.</p> <p>1986-01-01</p> <p>A computational <span class="hlt">fluid</span> dynamics code for application to traditional incompressible flow problems has been developed. The method is actually a slight compressibility approach which takes advantage of the bulk modulus and finite sound speed of all real <span class="hlt">fluids</span>. The finite element numerical analog uses a dynamic differencing scheme <span class="hlt">based</span>, in part, on a variational principle for computational <span class="hlt">fluid</span> dynamics. The code was developed in order to study the feasibility of damping seals for high speed turbomachinery. Preliminary seal analyses have been performed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27771558','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27771558"><span>Speckle tracking and speckle content <span class="hlt">based</span> composite strain imaging for solid and <span class="hlt">fluid</span> filled lesions.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Rabbi, Md Shifat-E; Hasan, Md Kamrul</p> <p>2017-02-01</p> <p>Strain imaging though for solid lesions provides an effective way for determining their pathologic condition by displaying the tissue stiffness contrast, for <span class="hlt">fluid</span> filled lesions such an imaging is yet an open problem. In this paper, we propose a novel speckle content <span class="hlt">based</span> strain imaging technique for visualization and classification of <span class="hlt">fluid</span> filled lesions in elastography after automatic identification of the presence of <span class="hlt">fluid</span> filled lesions. Speckle content <span class="hlt">based</span> strain, defined as a function of speckle density <span class="hlt">based</span> on the relationship between strain and speckle density, gives an indirect strain value for <span class="hlt">fluid</span> filled lesions. To measure the speckle density of the <span class="hlt">fluid</span> filled lesions, two new criteria <span class="hlt">based</span> on oscillation count of the windowed radio frequency signal and local variance of the normalized B-mode image are used. An improved speckle tracking technique is also proposed for strain imaging of the solid lesions and background. A wavelet-<span class="hlt">based</span> integration technique is then proposed for combining the strain images from these two techniques for visualizing both the solid and <span class="hlt">fluid</span> filled lesions from a common framework. The final output of our algorithm is a high quality composite strain image which can effectively visualize both solid and <span class="hlt">fluid</span> filled breast lesions in addition to the speckle content of the <span class="hlt">fluid</span> filled lesions for their discrimination. The performance of our algorithm is evaluated using the in vivo patient data and compared with recently reported techniques. The results show that both the solid and <span class="hlt">fluid</span> filled lesions can be better visualized using our technique and the <span class="hlt">fluid</span> filled lesions can be classified with good accuracy. Copyright © 2016 Elsevier B.V. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2005homm.book.2411B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2005homm.book.2411B"><span>Mesoscale <span class="hlt">Models</span> of <span class="hlt">Fluid</span> Dynamics</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Boghosian, Bruce M.; Hadjiconstantinou, Nicolas G.</p> <p></p> <p>During the last half century, enormous progress has been made in the field of computational materials <span class="hlt">modeling</span>, to the extent that in many cases computational approaches are used in a predictive fashion. Despite this progress, <span class="hlt">modeling</span> of general hydrodynamic behavior remains a challenging task. One of the main challenges stems from the fact that hydrodynamics manifests itself over a very wide range of length and time scales. On one end of the spectrum, one finds the <span class="hlt">fluid</span>'s "internal" scale characteristic of its molecular structure (in the absence of quantum effects, which we omit in this chapter). On the other end, the "outer" scale is set by the characteristic sizes of the problem's domain. The resulting scale separation or lack thereof as well as the existence of intermediate scales are key to determining the optimal approach. Successful treatments require a judicious choice of the level of description which is a delicate balancing act between the conflicting requirements of fidelity and manageable computational cost: a coarse description typically requires <span class="hlt">models</span> for underlying processes occuring at smaller length and time scales; on the other hand, a fine-scale <span class="hlt">model</span> will incur a significantly larger computational cost.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19940025399','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19940025399"><span>Large scale cryogenic <span class="hlt">fluid</span> systems testing</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p></p> <p>1992-01-01</p> <p>NASA Lewis Research Center's Cryogenic <span class="hlt">Fluid</span> Systems Branch (CFSB) within the Space Propulsion Technology Division (SPTD) has the ultimate goal of enabling the long term storage and in-space fueling/resupply operations for spacecraft and reusable vehicles in support of space exploration. Using analytical <span class="hlt">modeling</span>, ground <span class="hlt">based</span> testing, and on-orbit experimentation, the CFSB is studying three primary categories of <span class="hlt">fluid</span> technology: storage, supply, and transfer. The CFSB is also investigating <span class="hlt">fluid</span> handling, advanced instrumentation, and tank structures and materials. Ground <span class="hlt">based</span> testing of large-scale systems is done using liquid hydrogen as a test <span class="hlt">fluid</span> at the Cryogenic Propellant Tank Facility (K-site) at Lewis' Plum Brook Station in Sandusky, Ohio. A general overview of tests involving liquid transfer, thermal control, pressure control, and pressurization is given.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22408184-fluid-model-simulation-simplified-plasma-limiter-based-spectral-element-time-domain-method','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22408184-fluid-model-simulation-simplified-plasma-limiter-based-spectral-element-time-domain-method"><span>A <span class="hlt">fluid</span> <span class="hlt">model</span> simulation of a simplified plasma limiter <span class="hlt">based</span> on spectral-element time-domain method</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>Qian, Cheng; Ding, Dazhi, E-mail: dzding@njust.edu.cn; Fan, Zhenhong</p> <p>2015-03-15</p> <p>A simplified plasma limiter prototype is proposed and the <span class="hlt">fluid</span> <span class="hlt">model</span> coupled with Maxwell's equations is established to describe the operating mechanism of plasma limiter. A three-dimensional (3-D) simplified sandwich structure plasma limiter <span class="hlt">model</span> is analyzed with the spectral-element time-domain (SETD) method. The field breakdown threshold of air and argon at different frequency is predicted and compared with the experimental data and there is a good agreement between them for gas microwave breakdown discharge problems. Numerical results demonstrate that the two-layer plasma limiter (plasma-slab-plasma) has better protective characteristics than a one-layer plasma limiter (slab-plasma-slab) with the same length of gasmore » chamber.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014APS..MARA20005Y','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014APS..MARA20005Y"><span>Lennard-Jones <span class="hlt">fluids</span> in two-dimensional nano-pores. Multi-phase coexistence and <span class="hlt">fluid</span> structure</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Yatsyshin, Petr; Savva, Nikos; Kalliadasis, Serafim</p> <p>2014-03-01</p> <p>We present a number of fundamental findings on the wetting behaviour of nano-pores. A popular <span class="hlt">model</span> for <span class="hlt">fluid</span> confinement is a one-dimensional (1D) slit pore formed by two parallel planar walls and it exhibits capillary condensation (CC): a first-order phase transition from vapour to capillary-liquid (Kelvin shift). Capping such a pore at one end by a third orthogonal wall forms a prototypical two-dimensional (2D) pore. We show that 2D pores possess a wetting temperature such that below this temperature CC remains of first order, above it becomes a continuous phase transition manifested by a slab of capillary-liquid filling the pore from the capping wall. Continuous CC exhibits hysteresis and can be preceded by a first-order capillary prewetting transition. Additionally, liquid drops can form in the corners of the 2D pore (remnant of 2D wedge prewetting). The three <span class="hlt">fluid</span> phases, vapour, capillary-liquid slab and corner drops, can coexist at the pore triple point. Our <span class="hlt">model</span> is <span class="hlt">based</span> on the statistical mechanics of <span class="hlt">fluids</span> in the density functional formulation. The <span class="hlt">fluid-fluid</span> and <span class="hlt">fluid</span>-substrate interactions are dispersive. We analyze in detail the microscopic <span class="hlt">fluid</span> structure, isotherms and full phase diagrams. Our findings also suggest novel ways to control wetting of nano-pores. We are grateful to the European Research Council via Advanced Grant No. 247031 for support.</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://hdl.handle.net/2060/19820010006','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19820010006"><span>Shaded computer graphic techniques for visualizing and interpreting analytic <span class="hlt">fluid</span> flow <span class="hlt">models</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Parke, F. I.</p> <p>1981-01-01</p> <p>Mathematical <span class="hlt">models</span> which predict the behavior of <span class="hlt">fluid</span> flow in different experiments are simulated using digital computers. The simulations predict values of parameters of the <span class="hlt">fluid</span> flow (pressure, temperature and velocity vector) at many points in the <span class="hlt">fluid</span>. Visualization of the spatial variation in the value of these parameters is important to comprehend and check the data generated, to identify the regions of interest in the flow, and for effectively communicating information about the flow to others. The state of the art imaging techniques developed in the field of three dimensional shaded computer graphics is applied to visualization of <span class="hlt">fluid</span> flow. Use of an imaging technique known as 'SCAN' for visualizing <span class="hlt">fluid</span> flow, is studied and the results are presented.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/23802966','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/23802966"><span>Critical asymmetry in renormalization group theory for <span class="hlt">fluids</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Zhao, Wei; Wu, Liang; Wang, Long; Li, Liyan; Cai, Jun</p> <p>2013-06-21</p> <p>The renormalization-group (RG) approaches for <span class="hlt">fluids</span> are employed to investigate critical asymmetry of vapour-liquid equilibrium (VLE) of <span class="hlt">fluids</span>. Three different approaches <span class="hlt">based</span> on RG theory for <span class="hlt">fluids</span> are reviewed and compared. RG approaches are applied to various <span class="hlt">fluid</span> systems: hard-core square-well <span class="hlt">fluids</span> of variable ranges, hard-core Yukawa <span class="hlt">fluids</span>, and square-well dimer <span class="hlt">fluids</span> and <span class="hlt">modelling</span> VLE of n-alkane molecules. Phase diagrams of simple <span class="hlt">model</span> <span class="hlt">fluids</span> and alkanes described by RG approaches are analyzed to assess the capability of describing the VLE critical asymmetry which is suggested in complete scaling theory. Results of thermodynamic properties obtained by RG theory for <span class="hlt">fluids</span> agree with the simulation and experimental data. Coexistence diameters, which are smaller than the critical densities, are found in the RG descriptions of critical asymmetries of several <span class="hlt">fluids</span>. Our calculation and analysis show that the approach coupling local free energy with White's RG iteration which aims to incorporate density fluctuations into free energy is not adequate for VLE critical asymmetry due to the inadequate order parameter and the local free energy functional used in the partition function.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22251970-extinction-properties-single-walled-carbon-nanotubes-two-fluid-model','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22251970-extinction-properties-single-walled-carbon-nanotubes-two-fluid-model"><span>Extinction properties of single-walled carbon nanotubes: Two-<span class="hlt">fluid</span> <span class="hlt">model</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>Moradi, Afshin, E-mail: a.moradi@kut.ac.ir</p> <p></p> <p>The extinction spectra of a single-walled carbon nanotube are investigated, within the framework of the vector wave function method in conjunction with the hydrodynamic <span class="hlt">model</span>. Both polarizations of the incident plane wave (TE and TM with respect to the x-z plane) are treated. Electronic excitations on the nanotube surface are <span class="hlt">modeled</span> by an infinitesimally thin layer of a two-dimensional electron gas represented by two interacting <span class="hlt">fluids</span>, which takes into account the different nature of the σ and π electrons. Numerical results show that strong interaction between the <span class="hlt">fluids</span> gives rise to the splitting of the extinction spectra into two peaksmore » in quantitative agreement with the π and σ + π plasmon energies.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26763732','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26763732"><span>Distribution of crystalloid <span class="hlt">fluid</span> changes with the rate of infusion: a population-<span class="hlt">based</span> study.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Hahn, R G; Drobin, D; Zdolsek, J</p> <p>2016-05-01</p> <p>Crystalloid <span class="hlt">fluid</span> requires 30 min for complete distribution throughout the extracellular <span class="hlt">fluid</span> space and tends to cause long-standing peripheral edema. A kinetic analysis of the distribution of Ringer's acetate with increasing infusion rates was performed to obtain a better understanding of these characteristics of crystalloids. Data were retrieved from six studies in which 76 volunteers and preoperative patients had received between 300 ml and 2375 ml of Ringer's acetate solution at a rate of 20-80 ml/min (0.33-0.83 ml/min/kg). Serial measurements of the blood hemoglobin concentration were used as inputs in a kinetic analysis <span class="hlt">based</span> on a two-volume <span class="hlt">model</span> with micro-constants, using software for nonlinear mixed effects. The micro-constants describing distribution (k12) and elimination (k10) were unchanged when the rate of infusion increased, with half-times of 16 and 26 min, respectively. In contrast, the micro-constant describing how rapidly the already distributed <span class="hlt">fluid</span> left the peripheral space (k21) decreased by 90% when the <span class="hlt">fluid</span> was infused more rapidly, corresponding to an increase in the half-time from 3 to 30 min. The central volume of distribution (V(c)) doubled. The return of Ringer's acetate from the peripheral <span class="hlt">fluid</span> compartment to the plasma was slower with high than with low infusion rates. Edema is a normal consequence of plasma volume expansion with this <span class="hlt">fluid</span>, even in healthy volunteers. The results are consistent with the view that the viscoelastic properties of the interstitial matrix are responsible for the distribution and redistribution characteristics of crystalloid <span class="hlt">fluid</span>. © 2016 The Acta Anaesthesiologica Scandinavica Foundation. Published by John Wiley & Sons Ltd.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015APS..DFDA24003O','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015APS..DFDA24003O"><span><span class="hlt">Fluid</span> dynamic <span class="hlt">modelling</span> of renal pelvic pressure during endoscopic stone removal</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Oratis, Alexandros; Subasic, John; Bird, James; Eisner, Brian</p> <p>2015-11-01</p> <p>Endoscopic kidney stone removal procedures are known to increase internal pressure in the renal pelvis, the kidney's urinary collecting system. High renal pelvic pressure incites systemic absorption of irrigation <span class="hlt">fluid</span>, which can increase the risk of postoperative fever and sepsis or the unwanted absorption of electrolytes. Urologists choose the appropriate surgical procedure <span class="hlt">based</span> on patient history and kidney stone size. However, no study has been conducted to compare the pressure profiles of each procedure, nor is there a precise sense of how the renal pelvic pressure scales with various operational parameters. Here we develop physical <span class="hlt">models</span> for the flow rates and renal pelvic pressure for various procedures. We show that the results of our <span class="hlt">models</span> are consistent with existing urological data on each procedure and that the <span class="hlt">models</span> can predict pressure profiles where data is unavailable.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JCoPh.358...53K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JCoPh.358...53K"><span>Smoothed Particle Hydrodynamics: A consistent <span class="hlt">model</span> for interfacial multiphase <span class="hlt">fluid</span> flow simulations</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Krimi, Abdelkader; Rezoug, Mehdi; Khelladi, Sofiane; Nogueira, Xesús; Deligant, Michael; Ramírez, Luis</p> <p>2018-04-01</p> <p>In this work, a consistent Smoothed Particle Hydrodynamics (SPH) <span class="hlt">model</span> to deal with interfacial multiphase <span class="hlt">fluid</span> flows simulation is proposed. A modification to the Continuum Stress Surface formulation (CSS) [1] to enhance the stability near the <span class="hlt">fluid</span> interface is developed in the framework of the SPH method. A non-conservative first-order consistency operator is used to compute the divergence of stress surface tensor. This formulation benefits of all the advantages of the one proposed by Adami et al. [2] and, in addition, it can be applied to more than two phases <span class="hlt">fluid</span> flow simulations. Moreover, the generalized wall boundary conditions [3] are modified in order to be well adapted to multiphase <span class="hlt">fluid</span> flows with different density and viscosity. In order to allow the application of this technique to wall-bounded multiphase flows, a modification of generalized wall boundary conditions is presented here for using the SPH method. In this work we also present a particle redistribution strategy as an extension of the damping technique presented in [3] to smooth the initial transient phase of gravitational multiphase <span class="hlt">fluid</span> flow simulations. Several computational tests are investigated to show the accuracy, convergence and applicability of the proposed SPH interfacial multiphase <span class="hlt">model</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009SPIE.7426E..0BS','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009SPIE.7426E..0BS"><span>Zirconia coated carbonyl iron particle-<span class="hlt">based</span> magnetorheological <span class="hlt">fluid</span> for polishing</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Shafrir, Shai N.; Romanofsky, Henry J.; Skarlinski, Michael; Wang, Mimi; Miao, Chunlin; Salzman, Sivan; Chartier, Taylor; Mici, Joni; Lambropoulos, John C.; Shen, Rui; Yang, Hong; Jacobs, Stephen D.</p> <p>2009-08-01</p> <p>Aqueous magnetorheological (MR) polishing <span class="hlt">fluids</span> used in magnetorheological finishing (MRF) have a high solids concentration consisting of magnetic carbonyl iron particles and nonmagnetic polishing abrasives. The properties of MR polishing <span class="hlt">fluids</span> are affected over time by corrosion of CI particles. Here we report on MRF spotting experiments performed on optical glasses using a zirconia coated carbonyl iron (CI) particle-<span class="hlt">based</span> MR <span class="hlt">fluid</span>. The zirconia coated magnetic CI particles were prepared via sol-gel synthesis in kg quantities. The coating layer was ~50-100 nm thick, faceted in surface structure, and well adhered. Coated particles showed long term stability against aqueous corrosion. "Free" nano-crystalline zirconia polishing abrasives were co-generated in the coating process, resulting in an abrasivecharged powder for MRF. A viable MR <span class="hlt">fluid</span> was prepared simply by adding water. Spot polishing tests were performed on a variety of optical glasses over a period of 3 weeks with no signs of MR <span class="hlt">fluid</span> degradation or corrosion. Stable material removal rates and smooth surfaces inside spots were obtained.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016APS..DFDD30008H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016APS..DFDD30008H"><span>A thermodynamically consistent <span class="hlt">model</span> for granular-<span class="hlt">fluid</span> mixtures considering pore pressure evolution and hypoplastic behavior</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hess, Julian; Wang, Yongqi</p> <p>2016-11-01</p> <p>A new mixture <span class="hlt">model</span> for granular-<span class="hlt">fluid</span> flows, which is thermodynamically consistent with the entropy principle, is presented. The extra pore pressure described by a pressure diffusion equation and the hypoplastic material behavior obeying a transport equation are taken into account. The <span class="hlt">model</span> is applied to granular-<span class="hlt">fluid</span> flows, using a closing assumption in conjunction with the dynamic <span class="hlt">fluid</span> pressure to describe the pressure-like residual unknowns, hereby overcoming previous uncertainties in the <span class="hlt">modeling</span> process. Besides the thermodynamically consistent <span class="hlt">modeling</span>, numerical simulations are carried out and demonstrate physically reasonable results, including simple shear flow in order to investigate the vertical distribution of the physical quantities, and a mixture flow down an inclined plane by means of the depth-integrated <span class="hlt">model</span>. Results presented give insight in the ability of the deduced <span class="hlt">model</span> to capture the key characteristics of granular-<span class="hlt">fluid</span> flows. We acknowledge the support of the Deutsche Forschungsgemeinschaft (DFG) for this work within the Project Number WA 2610/3-1.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/18352120','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/18352120"><span><span class="hlt">Modeling</span> heat transfer in supercritical <span class="hlt">fluid</span> using the lattice Boltzmann method.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Házi, Gábor; Márkus, Attila</p> <p>2008-02-01</p> <p>A lattice Boltzmann <span class="hlt">model</span> has been developed to simulate heat transfer in supercritical <span class="hlt">fluids</span>. A supercritical viscous <span class="hlt">fluid</span> layer between two plates heated from the bottom has been studied. It is demonstrated that the <span class="hlt">model</span> can be used to study heat transfer near the critical point where the so-called piston effect speeds up the transfer of heat and results in homogeneous heating in the bulk of the layer. We have also studied the onset of convection in a Rayleigh-Bénard configuration. It is shown that our <span class="hlt">model</span> can well predict qualitatively the onset of convection near the critical point, where there is a crossover between the Rayleigh and Schwarzschild criteria.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AGUFM.H23B1249C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFM.H23B1249C"><span>Coupled Hydro-Mechanical <span class="hlt">Modeling</span> of <span class="hlt">Fluid</span> Geological Storage</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Castelletto, N.; Garipov, T.; Tchelepi, H. A.</p> <p>2013-12-01</p> <p>The accurate <span class="hlt">modeling</span> of the complex coupled physical processes occurring during the injection and the post-injection period is a key factor for assessing the safety and the feasibility of anthropogenic carbon dioxide (CO2) sequestration in subsurface formations. In recent years, it has become widely accepted the importance of the coupling between <span class="hlt">fluid</span> flow and geomechanical response in constraining the sustainable pressure buildup caused by <span class="hlt">fluid</span> injection relative to the caprock sealing capacity, induced seismicity effects and ground surface stability [e.g., Rutqvist, 2012; Castelletto et al., 2013]. Here, we present a <span class="hlt">modeling</span> approach <span class="hlt">based</span> on a suitable combination of Finite Volumes (FVs) and Finite Elements (FEs) to solve the coupled system of partial differential equations governing the multiphase flow in a deformable porous medium. Specifically, a FV method is used for the flow problem while the FE method is adopted to address the poro-elasto-plasticity equations. The aim of the present work is to compare the performance and the robustness of unconditionally stable sequential-implicit schemes [Kim et al., 2011] and the fully-implicit method in solving the algebraic systems arising from the discretization of the governing equations, for both normally conditioned and severely ill-conditioned problems. The two approaches are tested against well-known analytical solutions and experimented with in a realistic application of CO2 injection in a synthetic aquifer. References: - Castelletto N., G. Gambolati, and P. Teatini (2013), Geological CO2 sequestration in multi-compartment reservoirs: Geomechanical challenges, J. Geophys. Res. Solid Earth, 118, 2417-2428, doi:10.1002/jgrb.50180. - Kim J., H. A. Tchelepi, and R. Juanes (2011), Stability, accuracy and efficiency of sequential methods for coupled flow and geomechanics, SPE J., 16(2), 249-262. - Rutqvist J. (2012), The geomechanics of CO2 storage in deep sedimentary formations, Geotech. Geol. Eng., 30, 525-551.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26446009','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26446009"><span>Inter-operator Reliability of Magnetic Resonance Image-<span class="hlt">Based</span> Computational <span class="hlt">Fluid</span> Dynamics Prediction of Cerebrospinal <span class="hlt">Fluid</span> Motion in the Cervical Spine.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Martin, Bryn A; Yiallourou, Theresia I; Pahlavian, Soroush Heidari; Thyagaraj, Suraj; Bunck, Alexander C; Loth, Francis; Sheffer, Daniel B; Kröger, Jan Robert; Stergiopulos, Nikolaos</p> <p>2016-05-01</p> <p>For the first time, inter-operator dependence of MRI <span class="hlt">based</span> computational <span class="hlt">fluid</span> dynamics (CFD) <span class="hlt">modeling</span> of cerebrospinal <span class="hlt">fluid</span> (CSF) in the cervical spinal subarachnoid space (SSS) is evaluated. In vivo MRI flow measurements and anatomy MRI images were obtained at the cervico-medullary junction of a healthy subject and a Chiari I malformation patient. 3D anatomies of the SSS were reconstructed by manual segmentation by four independent operators for both cases. CFD results were compared at nine axial locations along the SSS in terms of hydrodynamic and geometric parameters. Intraclass correlation (ICC) assessed the inter-operator agreement for each parameter over the axial locations and coefficient of variance (CV) compared the percentage of variance for each parameter between the operators. Greater operator dependence was found for the patient (0.19 < ICC < 0.99) near the craniovertebral junction compared to the healthy subject (ICC > 0.78). For the healthy subject, hydraulic diameter and Womersley number had the least variance (CV = ~2%). For the patient, peak diastolic velocity and Reynolds number had the smallest variance (CV = ~3%). These results show a high degree of inter-operator reliability for MRI-<span class="hlt">based</span> CFD simulations of CSF flow in the cervical spine for healthy subjects and a lower degree of reliability for patients with Type I Chiari malformation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26146885','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26146885"><span>Openness as a buffer against cognitive decline: The Openness-<span class="hlt">Fluid</span>-Crystallized-Intelligence (OFCI) <span class="hlt">model</span> applied to late adulthood.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Ziegler, Matthias; Cengia, Anja; Mussel, Patrick; Gerstorf, Denis</p> <p>2015-09-01</p> <p>Explaining cognitive decline in late adulthood is a major research area. <span class="hlt">Models</span> using personality traits as possible influential variables are rare. This study tested assumptions <span class="hlt">based</span> on an adapted version of the Openness-<span class="hlt">Fluid</span>-Crystallized-Intelligence (OFCI) <span class="hlt">model</span>. The OFCI <span class="hlt">model</span> adapted to late adulthood predicts that openness is related to the decline in <span class="hlt">fluid</span> reasoning (Gf) through environmental enrichment. Gf should be related to the development of comprehension knowledge (Gc; investment theory). It was also assumed that Gf predicts changes in openness as suggested by the environmental success hypothesis. Finally, the OFCI <span class="hlt">model</span> proposes that openness has an indirect influence on the decline in Gc through its effect on Gf (mediation hypothesis). Using data from the Berlin Aging Study (N = 516, 70-103 years at T1), these predictions were tested using latent change score and latent growth curve <span class="hlt">models</span> with indicators of each trait. The current findings and prior research support environmental enrichment and success, investment theory, and partially the mediation hypotheses. <span class="hlt">Based</span> on a summary of all findings, the OFCI <span class="hlt">model</span> for late adulthood is suggested. (c) 2015 APA, all rights reserved).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018KARJ...30...29S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018KARJ...30...29S"><span>A discrete element <span class="hlt">model</span> for the influence of surfactants on sedimentation characteristics of magnetorheological <span class="hlt">fluids</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Son, Kwon Joong</p> <p>2018-02-01</p> <p>Hindering particle agglomeration and re-dispersion processes, gravitational sedimentation of suspended particles in magnetorheological (MR) <span class="hlt">fluids</span> causes inferior performance and controllability of MR <span class="hlt">fluids</span> in response to a user-specified magnetic field. Thus, suspension stability is one of the principal factors to be considered in synthesizing MR <span class="hlt">fluids</span>. However, only a few computational studies have been reported so far on the sedimentation characteristics of suspended particles under gravity. In this paper, the settling dynamics of paramagnetic particles suspended in MR <span class="hlt">fluids</span> was investigated via discrete element method (DEM) simulations. This work focuses particularly on developing accurate <span class="hlt">fluid</span>-particle and particle-particle interaction <span class="hlt">models</span> which can account for the influence of stabilizing surfactants on the MR <span class="hlt">fluid</span> sedimentation. Effect of the stabilizing surfactants on interparticle interactions was incorporated into the derivation of a reliable contact-impact <span class="hlt">model</span> for DEM computation. Also, the influence of the stabilizing additives on <span class="hlt">fluid</span>-particle interactions was considered by incorporating Stokes drag with shape and wall correction factors into DEM formulation. The results of simulations performed for <span class="hlt">model</span> validation purposes showed a good agreement with the published sedimentation measurement data in terms of an initial sedimentation velocity and a final sedimentation ratio.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017APS..DFDL38003H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017APS..DFDL38003H"><span>A <span class="hlt">fluid</span>-structure interaction <span class="hlt">model</span> of soft robotics using an active strain approach</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hess, Andrew; Lin, Zhaowu; Gao, Tong</p> <p>2017-11-01</p> <p>Soft robotic swimmers exhibit rich dynamics that stem from the non-linear interplay of the <span class="hlt">fluid</span> and immersed soft elastic body. Due to the difficulty of handling the nonlinear two-way coupling of hydrodynamic flow and deforming elastic body, studies of flexible swimmers often employ either one-way coupling strategies with imposed motions of the solid body or some simplified elasticity <span class="hlt">models</span>. To explore the nonlinear dynamics of soft robots powered by smart soft materials, we develop a computational <span class="hlt">model</span> to deal with the two-way <span class="hlt">fluid</span>/elastic structure interactions using the fictitious domain method. To mimic the dynamic response of the functional soft material under external actuations, we assume the solid phase to be neo-Hookean, and employ an active strain approach to incorporate actuation, which is <span class="hlt">based</span> on the multiplicative decomposition of the deformation gradient tensor. We demonstrate the capability of our algorithm by performing a series of numerical explorations that manipulate an elastic structure with finite thickness, starting from simple rectangular or circular plates to soft robot prototypes such as stingrays and jellyfish.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/23188803','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/23188803"><span>A mathematical <span class="hlt">model</span> of <span class="hlt">fluid</span> and gas flow in nanoporous media.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Monteiro, Paulo J M; Rycroft, Chris H; Barenblatt, Grigory Isaakovich</p> <p>2012-12-11</p> <p>The mathematical <span class="hlt">modeling</span> of the flow in nanoporous rocks (e.g., shales) becomes an important new branch of subterranean <span class="hlt">fluid</span> mechanics. The classic approach that was successfully used in the construction of the technology to develop oil and gas deposits in the United States, Canada, and the Union of Soviet Socialist Republics becomes insufficient for deposits in shales. In the present article a mathematical <span class="hlt">model</span> of the flow in nanoporous rocks is proposed. The <span class="hlt">model</span> assumes the rock consists of two components: (i) a matrix, which is more or less an ordinary porous or fissurized-porous medium, and (ii) specific organic inclusions composed of kerogen. These inclusions may have substantial porosity but, due to the nanoscale of pores, tubes, and channels, have extremely low permeability on the order of a nanodarcy (~109-²¹ m² ) or less. These inclusions contain the majority of <span class="hlt">fluid</span>: oil and gas. Our <span class="hlt">model</span> is <span class="hlt">based</span> on the hypothesis that the permeability of the inclusions substantially depends on the pressure gradient. At the beginning of the development of the deposit, boundary layers are formed at the boundaries of the low-permeable inclusions, where the permeability is strongly increased and intensive flow from inclusions to the matrix occurs. The resulting formulae for the production rate of the deposit are presented in explicit form. The formulae demonstrate that the production rate of deposits decays with time following a power law whose exponent lies between -1/2 and -1. Processing of experimental data obtained from various oil and gas deposits in shales demonstrated an instructive agreement with the prediction of the <span class="hlt">model</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19940019872&hterms=crystal+growth+modeling&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Dcrystal%2Bgrowth%2Bmodeling','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19940019872&hterms=crystal+growth+modeling&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Dcrystal%2Bgrowth%2Bmodeling"><span><span class="hlt">Modeling</span> of PCG <span class="hlt">fluid</span> dynamics: Salient results</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Ramachandran, N.</p> <p>1993-01-01</p> <p>Materials processing in space-<span class="hlt">based</span> laboratories has already yielded higher quality crystals during previous space flights, and opportunities for several <span class="hlt">fluids</span> experiments are anticipated during the extended duration missions planned for the future. Crystal growth in space benefits not only from its reduced gravity environment but also from the absence of the hydrostatic pressure which assists certain crystal growth and refinement methods. Gravity-driven phenomena are thus reduced in strength, and a purely diffusive <span class="hlt">fluid</span>'s behavior can be attained. In addition, past materials science experiments have shown that microgravity can also help produce larger crystals. While gravity-related effects are definitely curtailed in space, they are nevertheless present to some degree due to the acceleration environment onboard the spacecraft. This residual acceleration level is comprised of quasi-steady, oscillatory, and transient components, and is caused by a variety of mechanisms. For example, gravity gradient forces produce low frequency disturbances, and the operation of machinery, control thrusters, solar panels, human activity, etc. contribute to higher frequency accelerations. These disturbances are collectively referred to as g-jitter, and they can be deleterious to certain experiments where the minimization of the acceleration level is important. Advanced vibration isolation techniques can be utilized to actively filter out some of the detrimental frequencies and help in obtaining optimum results. However, the successful application of this technology requires the detailed analysis of candidate <span class="hlt">fluids</span> experiments to gauge their response to g-jitter and to determine their acceleration sensitivities. Several crystal growth experiments in the Protein Crystal Growth (PCG) area, besides others, are expected to be carried out on future shuttle flights and on Space Station Freedom. The need for vibration isolation systems or components for microgravity science experiments</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..1919331R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..1919331R"><span>Numerical <span class="hlt">modeling</span> of <span class="hlt">fluid</span> flow in a fault zone: a case of study from Majella Mountain (Italy).</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Romano, Valentina; Battaglia, Maurizio; Bigi, Sabina; De'Haven Hyman, Jeffrey; Valocchi, Albert J.</p> <p>2017-04-01</p> <p>The study of <span class="hlt">fluid</span> flow in fractured rocks plays a key role in reservoir management, including CO2 sequestration and waste isolation. We present a numerical <span class="hlt">model</span> of <span class="hlt">fluid</span> flow in a fault zone, <span class="hlt">based</span> on field data acquired in Majella Mountain, in the Central Apennines (Italy). This fault zone is considered a good analogue for the massive presence of <span class="hlt">fluid</span> migration in the form of tar. Faults are mechanical features and cause permeability heterogeneities in the upper crust, so they strongly influence <span class="hlt">fluid</span> flow. The distribution of the main components (core, damage zone) can lead the fault zone to act as a conduit, a barrier, or a combined conduit-barrier system. We integrated existing information and our own structural surveys of the area to better identify the major fault features (e.g., type of fractures, statistical properties, geometrical and petro-physical characteristics). In our <span class="hlt">model</span> the damage zones of the fault are described as discretely fractured medium, while the core of the fault as a porous one. Our <span class="hlt">model</span> utilizes the dfnWorks code, a parallelized computational suite, developed at Los Alamos National Laboratory (LANL), that generates three dimensional Discrete Fracture Network (DFN) of the damage zones of the fault and characterizes its hydraulic parameters. The challenge of the study is the coupling between the discrete domain of the damage zones and the continuum one of the core. The field investigations and the basic computational workflow will be described, along with preliminary results of <span class="hlt">fluid</span> flow simulation at the scale of the fault.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1992PhFlB...4.3138W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1992PhFlB...4.3138W"><span>Gyro-Landau <span class="hlt">fluid</span> <span class="hlt">models</span> for toroidal geometry</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Waltz, R. E.; Dominguez, R. R.; Hammett, G. W.</p> <p>1992-10-01</p> <p>Gyro-Landau <span class="hlt">fluid</span> <span class="hlt">model</span> equations provide first-order time advancement for a limited number of moments of the gyrokinetic equation, while approximately preserving the effects of the gyroradius averaging and Landau damping. This paper extends the work of Hammett and Perkins [Phys. Rev. Lett. 64, 3019 (1990)] for electrostatic motion parallel to the magnetic field and E×B motion to include the gyroaveraging linearly and the curvature drift motion. The equations are tested by comparing the ion-temperature-gradient mode linear growth rates for the <span class="hlt">model</span> equations with those of the exact gyrokinetic theory over a full range of parameters.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011icov.conf..801S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011icov.conf..801S"><span>FE <span class="hlt">Modelling</span> of the <span class="hlt">Fluid</span>-Structure-Acoustic Interaction for the Vocal Folds Self-Oscillation</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Švancara, Pavel; Horáček, J.; Hrůza, V.</p> <p></p> <p>The flow induced self-oscillation of the human vocal folds in interaction with acoustic processes in the simplified vocal tract <span class="hlt">model</span> was explored by three-dimensional (3D) finite element (FE) <span class="hlt">model</span>. Developed FE <span class="hlt">model</span> includes vocal folds pretension before phonation, large deformations of the vocal fold tissue, vocal folds contact, <span class="hlt">fluid</span>-structure interaction, morphing the <span class="hlt">fluid</span> mesh according the vocal folds motion (Arbitrary Lagrangian-Eulerian approach), unsteady viscous compressible airflow described by the Navier-Stokes equations and airflow separation during the glottis closure. Iterative partitioned approach is used for <span class="hlt">modelling</span> the <span class="hlt">fluid</span>-structure interaction. Computed results prove that the developed <span class="hlt">model</span> can be used for simulation of the vocal folds self-oscillation and resulting acoustic waves. The developed <span class="hlt">model</span> enables to numerically simulate an influence of some pathological changes in the vocal fold tissue on the voice production.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/25679499','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25679499"><span>Cellulose nanoparticles as modifiers for rheology and <span class="hlt">fluid</span> loss in bentonite water-<span class="hlt">based</span> <span class="hlt">fluids</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Li, Mei-Chun; Wu, Qinglin; Song, Kunlin; Qing, Yan; Wu, Yiqiang</p> <p>2015-03-04</p> <p>Rheological and filtration characteristics of drilling <span class="hlt">fluids</span> are considered as two critical aspects to ensure the success of a drilling operation. This research demonstrates the effectiveness of cellulose nanoparticles (CNPs), including microfibrillated cellulose (MFC) and cellulose nanocrystals (CNCs) in enhancing the rheological and filtration performances of bentonite (BT) water-<span class="hlt">based</span> drilling <span class="hlt">fluids</span> (WDFs). CNCs were isolated from MFC through sulfuric acid hydrolysis. In comparison with MFC, the resultant CNCs had much smaller dimensions, more negative surface charge, higher stability in aqueous solutions, lower viscosity, and less evident shear thinning behavior. These differences resulted in the distinctive microstructures between MFC/BT- and CNC/BT-WDFs. A typical "core-shell" structure was created in CNC/BT-WDFs due to the strong surface interactions among BT layers, CNCs, and immobilized water molecules. However, a similar structure was not formed in MFC/BT-WDFs. As a result, CNC/BT-WDFs had superior rheological properties, higher temperature stability, less <span class="hlt">fluid</span> loss volume, and thinner filter cakes than BT and MFC/BT-WDFs. Moreover, the presence of polyanionic cellulose (PAC) further improved the rheological and filtration performances of CNC/BT-WDFs, suggesting a synergistic effect between PAC and CNCs.</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/2006PSSCR...3..195T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2006PSSCR...3..195T"><span>The DC and AC insulating properties of magnetic <span class="hlt">fluids</span> <span class="hlt">based</span> on transformer oil</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Tomo, L.; Marton, K.; Herchl, F.; Kopanský, P.; Potoová, I.; Koneracká, M.; Timko, M.</p> <p>2006-01-01</p> <p>The AC-dielectric breakdown was investigated in magnetic <span class="hlt">fluids</span> <span class="hlt">based</span> on transformer oil TECHNOL US 4000 for two orientations of external magnetic field (B E and B E) and in B = 0. The found results were compared with those obtained formerly for the DC-dielectric breakdown. The observations of the time development of the AC-dielectric breakdown showed the presence of partial discharges long before the complete breakdown occurrence, while for DC-dielectric breakdown a complete breakdown of the gap next to the onset of a measurable ionization was characteristic. The comparison of the AC-dielectric breakdown strengths of pure transformer oil and transformer-oil-<span class="hlt">based</span> magnetic <span class="hlt">fluid</span> showed better dielectric properties of magnetic <span class="hlt">fluid</span> in external magnetic field and comparable, but not worse, in B = 0. Regarding to the better heat transfer, provided by magnetic <span class="hlt">fluids</span>, they could be used in power transformers as insulating <span class="hlt">fluids</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013APS..GECTF2003R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013APS..GECTF2003R"><span>Two-dimensional extended <span class="hlt">fluid</span> <span class="hlt">model</span> for a dc glow discharge with nonlocal ionization source term</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Rafatov, Ismail; Bogdanov, Eugeny; Kudryavtsev, Anatoliy</p> <p>2013-09-01</p> <p>Numerical techniques applied to the gas discharge plasma <span class="hlt">modelling</span> are generally grouped into <span class="hlt">fluid</span> and kinetic (particle) methods, and their combinations which lead to the hybrid <span class="hlt">models</span>. Hybrid <span class="hlt">models</span> usually employ Monte Carlo method to simulate fast electron dynamics, while slow plasma species are described as <span class="hlt">fluids</span>. However, since fast electrons contribution to these <span class="hlt">models</span> is limited to deriving the ionization rate distribution, their effect can be expressed by the analytical approximation of the ionization source function, and then integrating it into the <span class="hlt">fluid</span> <span class="hlt">model</span>. In the context of this approach, we incorporated effect of fast electrons into the ``extended <span class="hlt">fluid</span> <span class="hlt">model</span>'' of glow discharge, using two spatial dimensions. Slow electrons, ions and excited neutral species are described by the <span class="hlt">fluid</span> plasma equations. Slow electron transport (diffusion and mobility) coefficients as well as electron induced reaction rates are determined from the solutions of the electron Boltzmann equation. The self-consistent electric field is calculated using the Poisson equation. We carried out test calculations for the discharge in argon gas. Comparison with the experimental data as well as with the hybrid <span class="hlt">model</span> results exhibits good applicability of the proposed <span class="hlt">model</span>. The work was supported by the joint research grant from the Scientific and Technical Research Council of Turkey (TUBITAK) 212T164 and Russian Foundation for Basic Research (RFBR).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017APS..DFD.G9001G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017APS..DFD.G9001G"><span>Squid-inspired vehicle design using coupled <span class="hlt">fluid</span>-solid analytical <span class="hlt">modeling</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Giorgio-Serchi, Francesco; Weymouth, Gabriel</p> <p>2017-11-01</p> <p>The need for enhanced automation in the marine and maritime fields is fostering research into robust and highly maneuverable autonomous underwater vehicles. To address these needs we develop design principles for a new generation of soft-bodied aquatic vehicles similar to octopi and squids. In particular, we consider the capability of pulsed-jetting bodies to boost thrust by actively modifying their external body-shape and in this way benefit of the contribution from added-mass variation. We present an analytical formulation of the coupled <span class="hlt">fluid</span>-structure interaction between the elastic body and the ambient <span class="hlt">fluid</span>. The <span class="hlt">model</span> incorporates a number of new salient contributions to the soft-body dynamics. We highlight the role of added-mass variation effects of the external <span class="hlt">fluid</span> in enhancing thrust and assess how the shape-changing actuation is impeded by a confinement-related unsteady inertial term and by an external shape-dependent <span class="hlt">fluid</span> stiffness contribution. We show how the analysis of these combined terms has guided us to the design of a new prototype of a squid-inspired vehicle tuning of the natural frequency of the coupled <span class="hlt">fluid</span>-solid system with the purpose of optimizing its actuation routine.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70033185','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70033185"><span>Management of <span class="hlt">fluid</span> mud in estuaries, bays, and lakes. II: Measurement, <span class="hlt">modeling</span>, and management</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>McAnally, W.H.; Teeter, A.; Schoellhamer, David H.; Friedrichs, C.; Hamilton, D.; Hayter, E.; Shrestha, P.; Rodriguez, H.; Sheremet, A.; Kirby, R.</p> <p>2007-01-01</p> <p>Techniques for measurement, <span class="hlt">modeling</span>, and management of <span class="hlt">fluid</span> mud are available, but research is needed to improve them. <span class="hlt">Fluid</span> mud can be difficult to detect, measure, or sample, which has led to new instruments and new ways of using existing instruments. Multifrequency acoustic fathometers sense neither density nor viscosity and are, therefore, unreliable in measuring <span class="hlt">fluid</span> mud. Nuclear density probes, towed sleds, seismic, and drop probes equipped with density meters offer the potential for accurate measurements. Numerical <span class="hlt">modeling</span> of <span class="hlt">fluid</span> mud requires solving governing equations for flow velocity, density, pressure, salinity, water surface, plus sediment submodels. A number of such <span class="hlt">models</span> exist in one-, two-, and three-dimensional form, but they rely on empirical relationships that require substantial site-specific validation to observations. Management of <span class="hlt">fluid</span> mud techniques can be classified as those that accomplish: Source control, formation control, and removal. Nautical depth, a fourth category, defines the channel bottom as a specific <span class="hlt">fluid</span> mud density or alternative parameter as safe for navigation. Source control includes watershed management measures to keep fine sediment out of waterways and in-water measures such as structures and traps. Formation control methods include streamlined channels and structures plus other measures to reduce flocculation and structures that train currents. Removal methods include the traditional dredging and transport of dredged material plus agitation that contributes to formation control and/or nautical depth. Conditioning of <span class="hlt">fluid</span> mud by dredging and aerating offers the possibility of improved navigability. Two examples—the Atchafalaya Bar Channel and Savannah Harbor—illustrate the use of measurements and management of <span class="hlt">fluid</span> mud.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70042420','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70042420"><span>Integrated geophysical and hydrothermal <span class="hlt">models</span> of flank degassing and <span class="hlt">fluid</span> flow at Masaya Volcano, Nicaragua</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Sanford, Ward E.; Pearson, S.C.P.; Kiyosugi, K.; Lehto, H.L.; Saballos, J.A.; Connor, C.B.</p> <p>2012-01-01</p> <p>We investigate geologic controls on circulation in the shallow hydrothermal system of Masaya volcano, Nicaragua, and their relationship to surface diffuse degassing. On a local scale (~250 m), relatively impermeable normal faults dipping at ~60° control the flowpath of water vapor and other gases in the vadose zone. These shallow normal faults are identified by <span class="hlt">modeling</span> of a NE-SW trending magnetic anomaly of up to 2300 nT that corresponds to a topographic offset. Elevated SP and CO2 to the NW of the faults and an absence of CO2 to the SE suggest that these faults are barriers to flow. TOUGH2 numerical <span class="hlt">models</span> of <span class="hlt">fluid</span> circulation show enhanced flow through the footwalls of the faults, and corresponding increased mass flow and temperature at the surface (diffuse degassing zones). On a larger scale, TOUGH2 <span class="hlt">modeling</span> suggests that groundwater convection may be occurring in a 3-4 km radial fracture zone transecting the entire flank of the volcano. Hot water rising uniformly into the <span class="hlt">base</span> of the <span class="hlt">model</span> at 1 x 10-5 kg/m2s results in convection that focuses heat and <span class="hlt">fluid</span> and can explain the three distinct diffuse degassing zones distributed along the fracture. Our data and <span class="hlt">models</span> suggest that the unusually active surface degassing zones at Masaya volcano can result purely from uniform heat and <span class="hlt">fluid</span> flux at depth that is complicated by groundwater convection and permeability variations in the upper few km. Therefore isolating the effects of subsurface geology is vital when trying to interpret diffuse degassing in light of volcanic activity.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19740017688','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19740017688"><span>ASTP <span class="hlt">fluid</span> transfer measurement experiment. [using breadboard <span class="hlt">model</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Fogal, G. L.</p> <p>1974-01-01</p> <p>The ASTP <span class="hlt">fluid</span> transfer measurement experiment flight system design concept was verified by the demonstration and test of a breadboard <span class="hlt">model</span>. In addition to the breadboard effort, a conceptual design of the corresponding flight system was generated and a full scale mockup fabricated. A preliminary CEI specification for the flight system was also prepared.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018RScI...89b5001T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018RScI...89b5001T"><span>A MEMS SOI-<span class="hlt">based</span> piezoresistive <span class="hlt">fluid</span> flow sensor</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Tian, B.; Li, H. F.; Yang, H.; Song, D. L.; Bai, X. W.; Zhao, Y. L.</p> <p>2018-02-01</p> <p>In this paper, a SOI (silicon-on-insulator)-<span class="hlt">based</span> piezoresistive <span class="hlt">fluid</span> flow sensor is presented; the presented flow sensor mainly consists of a nylon sensing head, stainless steel cantilever beam, SOI sensor chip, printed circuit board, half-cylinder gasket, and stainless steel shell. The working principle of the sensor and some detailed contrastive analysis about the sensor structure were introduced since the nylon sensing head and stainless steel cantilever beam have distinct influence on the sensor performance; the structure of nylon sensing head and stainless steel cantilever beam is also discussed. The SOI sensor chip was fabricated using micro-electromechanical systems technologies, such as reactive ion etching and low pressure chemical vapor deposition. The designed <span class="hlt">fluid</span> sensor was packaged and tested; a calibration installation system was purposely designed for the sensor experiment. The testing results indicated that the output voltage of the sensor is proportional to the square of the <span class="hlt">fluid</span> flow velocity, which is coincident with the theoretical derivation. The tested sensitivity of the sensor is 3.91 × 10-4 V ms2/kg.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014SMaS...23l5013B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014SMaS...23l5013B"><span>Magnetorheology of dimorphic magnetorheological <span class="hlt">fluids</span> <span class="hlt">based</span> on nanofibers</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bombard, Antonio J. F.; Gonçalves, Flavia R.; Morillas, Jose R.; de Vicente, Juan</p> <p>2014-12-01</p> <p>We report a systematic experimental investigation on the use of nanofibers to enhance the magnetorheological (MR) effect in conventional (microsphere-<span class="hlt">based</span>) MR <span class="hlt">fluids</span> formulated in polyalphaolefin oil/1-octanol. Two kinds of nanofibers are employed that have very similar morphology but very different magnetic properties. On the one hand we use non-magnetic goethite nanofibers. On the other hand we employ magnetic chromium dioxide nanofibers. For appropriate concentrations the on-state relative yield stress increases up to 80% when incorporating the nanofibers in the formulation. A similar yield stress enhancement is found for both nanofibers investigated (magnetic and non-magnetic) suggesting that the main factor behind this MR enhancement is the particle shape anisotropy. The relative yield stresses obtained by partial substitution of carbonyl iron particles with nanofibers are significantly larger than those measured in previous works on MR <span class="hlt">fluids</span> formulated by partial substitution with non-magnetic micronsized spherical particles. We also demonstrate that these dimorphic MR <span class="hlt">fluids</span> also exhibit remarkably larger long-term sedimentation stability while keeping the same penetration and redispersibility characteristics.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20020052625&hterms=fluid+mechanic&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3Dfluid%2Bmechanic','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20020052625&hterms=fluid+mechanic&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3Dfluid%2Bmechanic"><span>Experiments and <span class="hlt">Modeling</span> of G-Jitter <span class="hlt">Fluid</span> Mechanics</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Leslie, F. W.; Ramachandran, N.; Whitaker, Ann F. (Technical Monitor)</p> <p>2002-01-01</p> <p>While there is a general understanding of the acceleration environment onboard an orbiting spacecraft, past research efforts in the <span class="hlt">modeling</span> and analysis area have still not produced a general theory that predicts the effects of multi-spectral periodic accelerations on a general class of experiments nor have they produced scaling laws that a prospective experimenter can use to assess how an experiment might be affected by this acceleration environment. Furthermore, there are no actual flight experimental data that correlates heat or mass transport with measurements of the periodic acceleration environment. The present investigation approaches this problem with carefully conducted terrestrial experiments and rigorous numerical <span class="hlt">modeling</span> for better understanding the effect of residual gravity and gentler on experiments. The approach is to use magnetic <span class="hlt">fluids</span> that respond to an imposed magnetic field gradient in much the same way as <span class="hlt">fluid</span> density responds to a gravitational field. By utilizing a programmable power source in conjunction with an electromagnet, both static and dynamic body forces can be simulated in lab experiments. The paper provides an overview of the technique and includes recent results from the experiments.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/664647-development-experimental-validation-sinda-fluint-thermal-fluid-electrical-model-multi-tube-amtec-cell','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/664647-development-experimental-validation-sinda-fluint-thermal-fluid-electrical-model-multi-tube-amtec-cell"><span>Development & experimental validation of a SINDA/FLUINT thermal/<span class="hlt">fluid</span>/electrical <span class="hlt">model</span> of a multi-tube AMTEC cell</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>Hendricks, T.J.; Borkowski, C.A.; Huang, C.</p> <p>1998-01-01</p> <p>AMTEC (Alkali Metal Thermal-to-Electric Conversion) cell development has received increased attention and funding in the space power community because of several desirable performance characteristics compared to current radioisotope thermoelectric generation and solar photovoltaic (PV) power generation. AMTEC cell development is critically dependent upon the ability to predict thermal, <span class="hlt">fluid</span> dynamic and electrical performance of an AMTEC cell which has many complex thermal, <span class="hlt">fluid</span> dynamic and electrical processes and interactions occurring simultaneously. Development of predictive capability is critical to understanding the complex processes and interactions within the AMTEC cell, and thereby creating the ability to design high-performance, cost-effective AMTEC cells. Amore » flexible, sophisticated thermal/<span class="hlt">fluid</span>/electrical <span class="hlt">model</span> of an operating AMTEC cell has been developed using the SINDA/FLUINT analysis software. This <span class="hlt">model</span> can accurately simulate AMTEC cell performance at any hot side and cold side temperature combination desired, for any voltage and current conditions, and for a broad range of cell design parameters involving the cell dimensions, current collector and electrode design, electrode performance parameters, and cell wall and thermal shield emissivity. The <span class="hlt">model</span> simulates the thermal radiation network within the AMTEC cell using RadCAD thermal radiation analysis; hot side, cold side and cell wall conductive and radiative coupling; <span class="hlt">BASE</span> (Beta Alumina Solid Electrode) tube electrochemistry, including electrode over-potentials; the <span class="hlt">fluid</span> dynamics of the low-pressure sodium vapor flow to the condenser and liquid sodium flow in the wick; sodium condensation at the condenser; and high-temperature sodium evaporation in the wick. The <span class="hlt">model</span> predicts the temperature profiles within the AMTEC cell walls, the <span class="hlt">BASE</span> tube temperature profiles, the sodium temperature profile in the artery return, temperature profiles in the evaporator, thermal energy flows</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..1814342Y','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..1814342Y"><span><span class="hlt">Modeling</span> of <span class="hlt">fluid</span> injection and withdrawal induced fault activation using discrete element <span class="hlt">based</span> hydro-mechanical and dynamic coupled simulator</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Yoon, Jeoung Seok; Zang, Arno; Zimmermann, Günter; Stephansson, Ove</p> <p>2016-04-01</p> <p>Operation of <span class="hlt">fluid</span> injection into and withdrawal from the subsurface for various purposes has been known to induce earthquakes. Such operations include hydraulic fracturing for shale gas extraction, hydraulic stimulation for Enhanced Geothermal System development and waste water disposal. Among these, several damaging earthquakes have been reported in the USA in particular in the areas of high-rate massive amount of wastewater injection [1] mostly with natural fault systems. Oil and gas production have been known to induce earthquake where pore <span class="hlt">fluid</span> pressure decreases in some cases by several tens of Mega Pascal. One recent seismic event occurred in November 2013 near Azle, Texas where a series of earthquakes began along a mapped ancient fault system [2]. It was studied that a combination of brine production and waste water injection near the fault generated subsurface pressures sufficient to induced earthquakes on near-critically stressed faults. This numerical study aims at investigating the occurrence mechanisms of such earthquakes induced by <span class="hlt">fluid</span> injection [3] and withdrawal by using hydro-geomechanical coupled dynamic simulator (Itasca's Particle Flow Code 2D). Generic <span class="hlt">models</span> are setup to investigate the sensitivity of several parameters which include fault orientation, frictional properties, distance from the injection well to the fault, amount of <span class="hlt">fluid</span> withdrawal around the injection well, to the response of the fault systems and the activation magnitude. Fault slip movement over time in relation to the diffusion of pore pressure is analyzed in detail. Moreover, correlations between the spatial distribution of pore pressure change and the locations of induced seismic events and fault slip rate are investigated. References [1] Keranen KM, Weingarten M, Albers GA, Bekins BA, Ge S, 2014. Sharp increase in central Oklahoma seismicity since 2008 induced by massive wastewater injection, Science 345, 448, DOI: 10.1126/science.1255802. [2] Hornbach MJ, DeShon HR</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://cfpub.epa.gov/si/si_public_record_report.cfm?dirEntryId=59509&keyword=offshore+AND+drilling&actType=&TIMSType=+&TIMSSubTypeID=&DEID=&epaNumber=&ntisID=&archiveStatus=Both&ombCat=Any&dateBeginCreated=&dateEndCreated=&dateBeginPublishedPresented=&dateEndPublishedPresented=&dateBeginUpdated=&dateEndUpdated=&dateBeginCompleted=&dateEndCompleted=&personID=&role=Any&journalID=&publisherID=&sortBy=revisionDate&count=50','EPA-EIMS'); return false;" href="https://cfpub.epa.gov/si/si_public_record_report.cfm?dirEntryId=59509&keyword=offshore+AND+drilling&actType=&TIMSType=+&TIMSSubTypeID=&DEID=&epaNumber=&ntisID=&archiveStatus=Both&ombCat=Any&dateBeginCreated=&dateEndCreated=&dateBeginPublishedPresented=&dateEndPublishedPresented=&dateBeginUpdated=&dateEndUpdated=&dateBeginCompleted=&dateEndCompleted=&personID=&role=Any&journalID=&publisherID=&sortBy=revisionDate&count=50"><span>ASSESSING THE IMPACT OF SYNTHETIC-<span class="hlt">BASED</span> DRILLING <span class="hlt">FLUIDS</span> ON BENTHIC ORGANISMS IN TEMPERATE WATERS</span></a></p> <p><a target="_blank" href="http://oaspub.epa.gov/eims/query.page">EPA Science Inventory</a></p> <p></p> <p></p> <p>Efforts to enhance the efficiency of oil/gas drilling operations and to minimize hazards to marine ecosystems have resulted in the increased use of synthetic-<span class="hlt">based</span> <span class="hlt">fluids</span> (SBF). SBFs have performance characteristics closely related to oil-<span class="hlt">based</span> <span class="hlt">fluids</span> (OBF) however their lower PA...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19950070448&hterms=Numerical+modeling+fluid+flow+heat+transfer&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3DNumerical%2Bmodeling%2Bfluid%2Bflow%2Bheat%2Btransfer','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19950070448&hterms=Numerical+modeling+fluid+flow+heat+transfer&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3DNumerical%2Bmodeling%2Bfluid%2Bflow%2Bheat%2Btransfer"><span>Analytical <span class="hlt">Model</span> For <span class="hlt">Fluid</span> Dynamics In A Microgravity Environment</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Naumann, Robert J.</p> <p>1995-01-01</p> <p>Report presents analytical approximation methodology for providing coupled <span class="hlt">fluid</span>-flow, heat, and mass-transfer equations in microgravity environment. Experimental engineering estimates accurate to within factor of 2 made quickly and easily, eliminating need for time-consuming and costly numerical <span class="hlt">modeling</span>. Any proposed experiment reviewed to see how it would perform in microgravity environment. <span class="hlt">Model</span> applied in commercial setting for preliminary design of low-Grashoff/Rayleigh-number experiments.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19930032138&hterms=solar+two&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Dsolar%2Btwo','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19930032138&hterms=solar+two&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Dsolar%2Btwo"><span>A parameter study of the two-<span class="hlt">fluid</span> solar wind</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Sandbaek, Ornulf; Leer, Egil; Holzer, Thomas E.</p> <p>1992-01-01</p> <p>A two-<span class="hlt">fluid</span> <span class="hlt">model</span> of the solar wind was introduced by Sturrock and Hartle (1966) and Hartle and Sturrock (1968). In these studies the proton energy equation was integrated neglecting the heat conductive term. Later several authors solved the equations for the two-<span class="hlt">fluid</span> solar wind <span class="hlt">model</span> keeping the proton heat conductive term. Methods where the equations are integrated simultaneously outward and inward from the critical point were used. The equations were also integrated inward from a large heliocentric distance. These methods have been applied to cases with low coronal <span class="hlt">base</span> electron densities and high <span class="hlt">base</span> temperatures. In this paper we present a method of integrating the two-<span class="hlt">fluid</span> solar wind equations using an iteration procedure where the equations are integrated separately and the proton flux is kept constant during the integrations. The technique is applicable for a wide range of coronal <span class="hlt">base</span> densities and temperatures. The method is used to carry out a parameter study of the two-<span class="hlt">fluid</span> solar wind.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/25666503','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25666503"><span>Mathematical <span class="hlt">modelling</span> of <span class="hlt">fluid</span> transport and its regulation at multiple scales.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Chara, Osvaldo; Brusch, Lutz</p> <p>2015-04-01</p> <p>Living matter equals water, to a first approximation, and water transport across barriers such as membranes and epithelia is vital. Water serves two competing functions. On the one hand, it is the fundamental solvent enabling random mobility of solutes and therefore biochemical reactions and intracellular signal propagation. Homeostasis of the intracellular water volume is required such that messenger concentration encodes the stimulus and not inverse volume fluctuations. On the other hand, water flow is needed for transport of solutes to and away from cells in a directed manner, threatening volume homeostasis and signal transduction fidelity of cells. Feedback regulation of <span class="hlt">fluid</span> transport reconciles these competing objectives. The regulatory mechanisms often span across multiple spatial scales from cellular interactions up to the architecture of organs. Open questions relate to the dependency of water fluxes and steady state volumes on control parameters and stimuli. We here review selected mathematical <span class="hlt">models</span> of feedback regulation of <span class="hlt">fluid</span> transport at the cell scale and identify a general "core-shell" structure of such <span class="hlt">models</span>. We propose that <span class="hlt">fluid</span> transport <span class="hlt">models</span> at other spatial scales can be constructed in a generalised core-shell framework, in which the core accounts for the biophysical effects of <span class="hlt">fluid</span> transport whilst the shell reflects the regulatory mechanisms. We demonstrate the applicability of this framework for tissue lumen growth and suggest future experiments in zebrafish to test lumen size regulation mechanisms. Copyright © 2015 Elsevier Ireland Ltd. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.H51C1490W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.H51C1490W"><span>A discontinuous finite element approach to cracking in coupled poro-elastic <span class="hlt">fluid</span> flow <span class="hlt">models</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wilson, C. R.; Spiegelman, M. W.; Evans, O.; Ulven, O. I.; Sun, W.</p> <p>2016-12-01</p> <p>Reaction-driven cracking is a coupled process whereby <span class="hlt">fluid</span>-induced reactions drive large volume changes in the host rock which produce stresses leading to crack propagation and failure. This in turn generates new surface area and <span class="hlt">fluid</span>-flow pathways for subsequent reaction in a potentially self-sustaining system. This mechanism has has been proposed for the pervasive serpentinization and carbonation of peridotite, as well as applications to mineral carbon sequestration and hydrocarbon extraction. The key computational issue in this problem is implementing algorithms that adequately <span class="hlt">model</span> the formation of discrete fractures. Here we present <span class="hlt">models</span> using a discontinuous finite element method for <span class="hlt">modeling</span> fracture formation (Radovitsky et al., 2011). Cracks are introduced along facets of the mesh by the relaxation of penalty parameters once a failure criterion is met. It is fully described in the weak form of the equations, requiring no modification of the underlying mesh structure and allowing <span class="hlt">fluid</span> properties to be easily adjusted along cracked facets. To develop and test the method, we start by implementing the algorithm for the simplified Biot equations for poro-elasticity using the finite element <span class="hlt">model</span> assembler TerraFERMA. We consider hydro-fracking around a borehole (Grassl et al., 2015), where elevated <span class="hlt">fluid</span> pressure in the poro-elastic solid causes it to fail radially in tension. We investigate the effects of varying the Biot coefficient and adjusting the <span class="hlt">fluid</span> transport properties in the vicinity of the crack and compare our results to related dual-graph <span class="hlt">models</span> (Ulven & Sun, submitted). We discuss issues arising from this method, including the formation of null spaces and appropriate preconditioning and solution strategies. Initial results suggest that this method provides a promising way to incorporate cracking into our reactive <span class="hlt">fluid</span> flow <span class="hlt">models</span> and future work aims to integrate the mechanical and chemical aspects of this process.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26862041','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26862041"><span><span class="hlt">Fluid</span> friction and wall viscosity of the 1D blood flow <span class="hlt">model</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Wang, Xiao-Fei; Nishi, Shohei; Matsukawa, Mami; Ghigo, Arthur; Lagrée, Pierre-Yves; Fullana, Jose-Maria</p> <p>2016-02-29</p> <p>We study the behavior of the pulse waves of water into a flexible tube for application to blood flow simulations. In pulse waves both <span class="hlt">fluid</span> friction and wall viscosity are damping factors, and difficult to evaluate separately. In this paper, the coefficients of <span class="hlt">fluid</span> friction and wall viscosity are estimated by fitting a nonlinear 1D flow <span class="hlt">model</span> to experimental data. In the experimental setup, a distensible tube is connected to a piston pump at one end and closed at another end. The pressure and wall displacements are measured simultaneously. A good agreement between <span class="hlt">model</span> predictions and experiments was achieved. For amplitude decrease, the effect of wall viscosity on the pulse wave has been shown as important as that of <span class="hlt">fluid</span> viscosity. Copyright © 2016 Elsevier Ltd. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19970009626','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19970009626"><span>Simulation of Two-<span class="hlt">Fluid</span> Flows by the Least-Squares Finite Element Method Using a Continuum Surface Tension <span class="hlt">Model</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Wu, Jie; Yu, Sheng-Tao; Jiang, Bo-nan</p> <p>1996-01-01</p> <p>In this paper a numerical procedure for simulating two-<span class="hlt">fluid</span> flows is presented. This procedure is <span class="hlt">based</span> on the Volume of <span class="hlt">Fluid</span> (VOF) method proposed by Hirt and Nichols and the continuum surface force (CSF) <span class="hlt">model</span> developed by Brackbill, et al. In the VOF method <span class="hlt">fluids</span> of different properties are identified through the use of a continuous field variable (color function). The color function assigns a unique constant (color) to each <span class="hlt">fluid</span>. The interfaces between different <span class="hlt">fluids</span> are distinct due to sharp gradients of the color function. The evolution of the interfaces is captured by solving the convective equation of the color function. The CSF <span class="hlt">model</span> is used as a means to treat surface tension effect at the interfaces. Here a modified version of the CSF <span class="hlt">model</span>, proposed by Jacqmin, is used to calculate the tension force. In the modified version, the force term is obtained by calculating the divergence of a stress tensor defined by the gradient of the color function. In its analytical form, this stress formulation is equivalent to the original CSF <span class="hlt">model</span>. Numerically, however, the use of the stress formulation has some advantages over the original CSF <span class="hlt">model</span>, as it bypasses the difficulty in approximating the curvatures of the interfaces. The least-squares finite element method (LSFEM) is used to discretize the governing equation systems. The LSFEM has proven to be effective in solving incompressible Navier-Stokes equations and pure convection equations, making it an ideal candidate for the present applications. The LSFEM handles all the equations in a unified manner without any additional special treatment such as upwinding or artificial dissipation. Various bench mark tests have been carried out for both two dimensional planar and axisymmetric flows, including a dam breaking, oscillating and stationary bubbles and a conical liquid sheet in a pressure swirl atomizer.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2007APS..MARP30002K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2007APS..MARP30002K"><span>Light-Induced Gelling in a Micellar <span class="hlt">Fluid</span> <span class="hlt">Based</span> on a Zwitterionic Surfactant.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kumar, Rakesh; Raghavan, Srinivasa</p> <p>2007-03-01</p> <p><span class="hlt">Fluids</span> with photoresponsive rheological properties (i.e. photorheological or PR <span class="hlt">fluids</span>) can be useful in a range of applications, such as in dampers, sensors, and valves for microfluidic or MEMS devices. Previously, we have demonstrated a cationic surfactant-<span class="hlt">based</span> PR <span class="hlt">fluid</span> whose viscosity can be rapidly decreased by UV irradiation. This viscosity decrease was not reversible. Here, we describe a different formulation <span class="hlt">based</span> on a zwitterionic surfactant that shows a rapid increase in viscosity (gelling) upon exposure to UV radiation. The formulation consists of the zwitterionic surfactant and a photosensitive cinnamic acid derivative. Initially, the viscosity of the <span class="hlt">fluid</span> is low indicating the presence of small micelles. Upon UV irradiation, the cinnamic acid derivative is photoisomerized from trans to cis. In turn, the small micelles transform into long wormlike micelles, thus increasing the solution viscosity by more than five orders of magnitude. Small angle neutron scattering (SANS) data confirms the dramatic increase in micelle length. Possible reasons for such changes in micelle dimensions will be discussed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/22695427','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/22695427"><span>Steady-state and time-dependent thermodynamic <span class="hlt">modeling</span> of the effect of intravenous infusion of warm and cold <span class="hlt">fluids</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Barthel, Erik R; Pierce, James R</p> <p>2012-06-01</p> <p>Hypothermia results in vital sign lability, coagulopathy, wound infections, and other sequelae. Normothermia can be restored by several modalities, including passive blanket heating, warm forced-air devices, and active <span class="hlt">fluid</span> warming (AFW). In AFW, intravenously administered <span class="hlt">fluids</span> are heated to 40 to 45 °C to minimize net thermal losses and to raise body temperature. Clinical studies have demonstrated the efficacy of AFW as part of a strategy encompassing several methods, but the isolated contribution of AFW to warming has not been theoretically examined in detail. A calorimetric <span class="hlt">model</span> is derived to determine the functional dependence of warming on patient weight, hypothermia severity, infusion temperature, and volume infused. A second heat transfer <span class="hlt">model</span> is derived to describe the time-dependent temperature changes of the periphery and core after warmed-<span class="hlt">fluid</span> infusion. There is an inverse linear relationship between the patient's initial temperature and the amount of warming achieved with a given volume. In contrast, as the temperature of the infusion approaches the desired final temperature, the volume required for a fixed temperature change increases nonlinearly. For weight-<span class="hlt">based</span> boluses, the temperature change scales appropriately with patient mass. Infusion of 2 L of room-temperature crystalloid results in a decrease in body temperature of approximately one-third degree Celsius in the average normothermic adult. For the heat transfer <span class="hlt">model</span>, previously reported rates of temperature drop and recovery after the intravenous infusion of cold <span class="hlt">fluids</span> are qualitatively reproduced with a blood mixing time of approximately 15 minutes. Our calculations reveal that AFW has a larger measurable beneficial effect for patients with more severe hypothermia, but true rewarming of the patient with AFW alone would require prohibitively large <span class="hlt">fluid</span> volumes (more than 10 L of 40 °C <span class="hlt">fluid</span>) or dangerously hot <span class="hlt">fluid</span> (20 mL/kg of 80 °C <span class="hlt">fluid</span> for a 1 °C increase). The major</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.ncbi.nlm.nih.gov/pubmed/20058187','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/20058187"><span>Partitioned <span class="hlt">fluid</span>-solid coupling for cardiovascular blood flow: left-ventricular <span class="hlt">fluid</span> mechanics.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Krittian, Sebastian; Janoske, Uwe; Oertel, Herbert; Böhlke, Thomas</p> <p>2010-04-01</p> <p>We present a 3D code-coupling approach which has been specialized towards cardiovascular blood flow. For the first time, the prescribed geometry movement of the cardiovascular flow <span class="hlt">model</span> KaHMo (Karlsruhe Heart <span class="hlt">Model</span>) has been replaced by a myocardial composite <span class="hlt">model</span>. Deformation is driven by <span class="hlt">fluid</span> forces and myocardial response, i.e., both its contractile and constitutive behavior. Whereas the arbitrary Lagrangian-Eulerian formulation (ALE) of the Navier-Stokes equations is discretized by finite volumes (FVM), the solid mechanical finite elasticity equations are discretized by a finite element (FEM) approach. Taking advantage of specialized numerical solution strategies for non-matching <span class="hlt">fluid</span> and solid domain meshes, an iterative data-exchange guarantees the interface equilibrium of the underlying governing equations. The focus of this work is on left-ventricular <span class="hlt">fluid</span>-structure interaction <span class="hlt">based</span> on patient-specific magnetic resonance imaging datasets. Multi-physical phenomena are described by temporal visualization and characteristic FSI numbers. The results gained show flow patterns that are in good agreement with previous observations. A deeper understanding of cavity deformation, blood flow, and their vital interaction can help to improve surgical treatment and clinical therapy planning.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2004PhPl...11.5173P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2004PhPl...11.5173P"><span>A Landau <span class="hlt">fluid</span> <span class="hlt">model</span> for dispersive magnetohydrodynamics</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Passot, T.; Sulem, P. L.</p> <p>2004-11-01</p> <p>A monofluid <span class="hlt">model</span> with Landau damping is presented for strongly magnetized electron-proton collisionless plasmas whose distribution functions are close to bi-Maxwellians. This description that includes dynamical equations for the gyrotropic components of the pressure and heat flux tensors, extends the Landau-<span class="hlt">fluid</span> <span class="hlt">model</span> of Snyder, Hammett, and Dorland [Phys. Plasmas 4, 3974 (1997)] by retaining Hall effect and finite Larmor radius corrections. It accurately reproduces the weakly nonlinear dynamics of dispersive Alfvén waves whose wavelengths are large compared to the ion inertial length, whatever their direction of propagation, and also the rapid Landau dissipation of long magnetosonic waves in a warm plasma.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018MS%26E..292a2106M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018MS%26E..292a2106M"><span>Study on the effect of polymeric rheology modifier on the rheological properties of oil-<span class="hlt">based</span> drilling <span class="hlt">fluids</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ma, C.; Li, L.; Yang, Y. P.; Hao, W. W.; Zhang, Q.; Lv, J.</p> <p>2018-01-01</p> <p>A new type of polymeric rheology modifier was synthesized by suspension polymerization, and the effect of rheology modifier on the rheological properties of oil-<span class="hlt">based</span> drilling <span class="hlt">fluids</span> was investigated. The results indicated that the obtained polymer had good capacity of improvement of shearing force of oil-<span class="hlt">based</span> drilling <span class="hlt">fluids</span> under high temperature and high pressure conditions. Moreover, the obtained polymer can improve the stability of oil-<span class="hlt">based</span> drilling <span class="hlt">fluids</span> greatly. As a result, the obtained polymer is a good rheology modifier for oil-<span class="hlt">based</span> drilling <span class="hlt">fluids</span>, and it can optimize oil-<span class="hlt">based</span> drilling <span class="hlt">fluid</span> system with good rheological properties, good static suspension ability for cuttings and environmental protection function. It can play an essential role in safe drilling jobs and improvement of drilling efficiency.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3134331','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3134331"><span>Multi-Physics MRI-<span class="hlt">Based</span> Two-Layer <span class="hlt">Fluid</span>-Structure Interaction Anisotropic <span class="hlt">Models</span> of Human Right and Left Ventricles with Different Patch Materials: Cardiac Function Assessment and Mechanical Stress Analysis</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Tang, Dalin; Yang, Chun; Geva, Tal; Gaudette, Glenn; del Nido, Pedro J.</p> <p>2011-01-01</p> <p>Multi-physics right and left ventricle (RV/LV) <span class="hlt">fluid</span>-structure interaction (FSI) <span class="hlt">models</span> were introduced to perform mechanical stress analysis and evaluate the effect of patch materials on RV function. The FSI <span class="hlt">models</span> included three different patch materials (Dacron scaffold, treated pericardium, and contracting myocardium), two-layer construction, fiber orientation, and active anisotropic material properties. The <span class="hlt">models</span> were constructed <span class="hlt">based</span> on cardiac magnetic resonance (CMR) images acquired from a patient with severe RV dilatation and solved by ADINA. Our results indicate that the patch <span class="hlt">model</span> with contracting myocardium leads to decreased stress level in the patch area, improved RV function and patch area contractility. PMID:21765559</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/of/2005/1137/','USGSPUBS'); return false;" href="https://pubs.usgs.gov/of/2005/1137/"><span>Role of rock/<span class="hlt">fluid</span> characteristics in carbon (CO2) storage and <span class="hlt">modeling</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>Verma, Mahendra K.</p> <p>2005-01-01</p> <p>The presentation ? Role of Rock/<span class="hlt">Fluid</span> Characteristics in Carbon (CO2) Storage and <span class="hlt">Modeling</span> ? was prepared for the meeting of the Environmental Protection Agency (EPA) in Houston, Tex., on April 6?7, 2005. It provides an overview of greenhouse gases, particularly CO2, and a summary of their effects on the Earth?s atmosphere. It presents methods of mitigating the effects of greenhouse gases, and the role of rock and <span class="hlt">fluid</span> properties on CO2 storage mechanisms. It also lists factors that must be considered to adequately <span class="hlt">model</span> CO2 storage.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/12631040','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/12631040"><span>Mathematical <span class="hlt">model</span> of renal elimination of <span class="hlt">fluid</span> and small ions during hyper- and hypovolemic conditions.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Gyenge, Christina C; Bowen, Bruce D; Reed, Rolf K; Bert, Joel L</p> <p>2003-02-01</p> <p>This study is concerned with the formulation of a 'kidney module' linked to the plasma compartment of a larger mathematical <span class="hlt">model</span> previously developed. Combined, these <span class="hlt">models</span> can be used to predict, amongst other things, <span class="hlt">fluid</span> and small ion excretion rates by the kidney; information that should prove useful in evaluating values and trends related to whole-body <span class="hlt">fluid</span> balance for different clinical conditions to establish <span class="hlt">fluid</span> administration protocols and for educational purposes. The renal module assumes first-order, negative-feedback responses of the kidney to changes in plasma volume and/or plasma sodium content from their normal physiological set points. Direct hormonal influences are not explicitly formulated in this empiric <span class="hlt">model</span>. The <span class="hlt">model</span> also considers that the renal excretion rates of small ions other than sodium are proportional to the excretion rate of sodium. As part of the <span class="hlt">model</span> development two aspects are emphasized (1): the estimation of parameters related to the renal elimination of <span class="hlt">fluid</span> and small ions, and (2) <span class="hlt">model</span> validation via comparisons between the <span class="hlt">model</span> predictions and selected experimental data. For validation, <span class="hlt">model</span> predictions of the renal dynamics are compared with new experimental data for two cases: plasma overload resulting from external <span class="hlt">fluid</span> infusion (e.g. infusions of iso-osmolar solutions and/or hypertonic/hyperoncotic saline solutions), and untreated hypo volemic conditions that result from the external loss of blood. The present study demonstrates that the empiric kidney module presented above can provide good short-term predictions with respect to all renal outputs considered here. Physiological implications of the <span class="hlt">model</span> are also presented. Copyright Acta Anaesthesiologica Scandinavica 47 (2003)</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20050220605','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20050220605"><span><span class="hlt">Fluid</span> Distribution for In-space Cryogenic Propulsion</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Lear, William</p> <p>2005-01-01</p> <p>The ultimate goal of this task is to enable the use of a single supply of cryogenic propellants for three distinct spacecraft propulsion missions: main propulsion, orbital maneuvering, and attitude control. A <span class="hlt">fluid</span> distribution system is sought which allows large propellant flows during the first two missions while still allowing control of small propellant flows during attitude control. Existing research has identified the probable benefits of a combined thermal management/power/<span class="hlt">fluid</span> distribution system <span class="hlt">based</span> on the Solar Integrated Thermal Management and Power (SITMAP) cycle. Both a numerical <span class="hlt">model</span> and an experimental <span class="hlt">model</span> are constructed in order to predict the performance of such an integrated thermal management/propulsion system. This research task provides a numerical <span class="hlt">model</span> and an experimental apparatus which will simulate an integrated thermal/power/<span class="hlt">fluid</span> management system <span class="hlt">based</span> on the SITMAP cycle, and assess its feasibility for various space missions. Various modifications are done to the cycle, such as the addition of a regeneration process that allows heat to be transferred into the working <span class="hlt">fluid</span> prior to the solar collector, thereby reducing the collector size and weight. Fabri choking analysis was also accounted for. Finally the cycle is to be optimized for various space missions <span class="hlt">based</span> on a mass <span class="hlt">based</span> figure of merit, namely the System Mass Ratio (SMR). -. 1 he theoretical and experimental results from these <span class="hlt">models</span> are be used to develop a design code (JETSIT code) which is able to provide design parameters for such a system, over a range of cooling loads, power generation, and attitude control thrust levels. The performance gains and mass savings will be compared to those of existing spacecraft systems.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016APS..DPPPO4008S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016APS..DPPPO4008S"><span>Nonaxisymmetric <span class="hlt">modelling</span> in BOUT++; toward global edge <span class="hlt">fluid</span> turbulence in stellarators</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Shanahan, Brendan; Hill, Peter; Dudson, Ben</p> <p>2016-10-01</p> <p>As Wendelstein 7-X has been optimized for neoclassical transport, turbulent transport could potentially become comparable to neoclassical losses. Furthermore, the imminent installation of an island divertor merits global edge <span class="hlt">modelling</span> to determine heat flux profiles and the efficacy of the system. Currently, however, nonaxisymmetric edge plasma <span class="hlt">modelling</span> is limited to either steady state (non-turbulent) transport <span class="hlt">modelling</span>, or computationally expensive gyrokinetics. The implementation of the Flux Coordinate Independent (FCI) approach to parallel derivatives has allowed the extension of the BOUT++ edge <span class="hlt">fluid</span> turbulence framework to nonaxisymmetric geometries. Here we first investigate the implementation of the FCI method in BOUT++ by <span class="hlt">modelling</span> diffusion equations in nonaxisymmetric geometries with and without boundary interaction, and quantify the inherent error. We then present the results of non-turbulent transport <span class="hlt">modelling</span> and compare with analytical theory. The ongoing extension of BOUT++ to nonaxisymmetric configurations, and the prospects of stellarator edge <span class="hlt">fluid</span> turbulence simulations will be discussed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20100040643','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20100040643"><span>Long Duration Life Test of Propylene Glycol Water <span class="hlt">Based</span> Thermal <span class="hlt">Fluid</span> Within Thermal Control Loop</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Le, Hung; Hill, Charles; Stephan, Ryan A.</p> <p>2010-01-01</p> <p>Evaluations of thermal properties and resistance to microbial growth concluded that 50% Propylene Glycol (PG)-<span class="hlt">based</span> <span class="hlt">fluid</span> and 50% de-ionized water mixture was desirable for use as a <span class="hlt">fluid</span> within a vehicle s thermal control loop. However, previous testing with a commercial mixture of PG and water containing phosphate corrosion inhibitors resulted in corrosion of aluminum within the test system and instability of the test <span class="hlt">fluid</span>. This paper describes a follow-on long duration testing and analysis of 50% Propylene Glycol (PG)-<span class="hlt">based</span> <span class="hlt">fluid</span> and 50% de-ionized water mixture with inorganic corrosion inhibitors used in place of phosphates. The test evaluates the long-term <span class="hlt">fluid</span> stability and resistance to microbial and chemical changes</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018PDU....20...41P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018PDU....20...41P"><span>Holographic dark energy from <span class="hlt">fluid</span>/gravity duality constraint by cosmological observations</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Pourhassan, Behnam; Bonilla, Alexander; Faizal, Mir; Abreu, Everton M. C.</p> <p>2018-06-01</p> <p>In this paper, we obtain a holographic <span class="hlt">model</span> of dark energy using the <span class="hlt">fluid</span>/gravity duality. This <span class="hlt">model</span> will be dual to a higher dimensional Schwarzschild black hole, and we would use <span class="hlt">fluid</span>/gravity duality to relate to the parameters of this black hole to such a cosmological <span class="hlt">model</span>. We will also analyze the thermodynamics of such a solution, and discuss the stability <span class="hlt">model</span>. Finally, we use cosmological data to constraint the parametric space of this dark energy <span class="hlt">model</span>. Thus, we will use observational data to perform cosmography for this holographic <span class="hlt">model</span> <span class="hlt">based</span> on <span class="hlt">fluid</span>/gravity duality.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20050215685','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20050215685"><span>Approaches to Validation of <span class="hlt">Models</span> for Low Gravity <span class="hlt">Fluid</span> Behavior</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Chato, David J.; Marchetta, Jeffery; Hochstein, John I.; Kassemi, Mohammad</p> <p>2005-01-01</p> <p>This paper details the author experiences with the validation of computer <span class="hlt">models</span> to predict low gravity <span class="hlt">fluid</span> behavior. It reviews the literature of low gravity <span class="hlt">fluid</span> behavior as a starting point for developing a baseline set of test cases. It examines authors attempts to validate their <span class="hlt">models</span> against these cases and the issues they encountered. The main issues seem to be that: Most of the data is described by empirical correlation rather than fundamental relation; Detailed measurements of the flow field have not been made; Free surface shapes are observed but through thick plastic cylinders, and therefore subject to a great deal of optical distortion; and Heat transfer process time constants are on the order of minutes to days but the zero-gravity time available has been only seconds.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20000075636&hterms=electrical+robots&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3Delectrical%2Brobots','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20000075636&hterms=electrical+robots&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3Delectrical%2Brobots"><span><span class="hlt">Modeling</span> and Design of an Electro-Rheological <span class="hlt">Fluid</span> <span class="hlt">Based</span> Haptic System for Tele-Operation of Space Robots</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Mavroidis, Constantinos; Pfeiffer, Charles; Paljic, Alex; Celestino, James; Lennon, Jamie; Bar-Cohen, Yoseph</p> <p>2000-01-01</p> <p>For many years, the robotic community sought to develop robots that can eventually operate autonomously and eliminate the need for human operators. However, there is an increasing realization that there are some tasks that human can perform significantly better but, due to associated hazards, distance, physical limitations and other causes, only robot can be employed to perform these tasks. Remotely performing these types of tasks requires operating robots as human surrogates. While current "hand master" haptic systems are able to reproduce the feeling of rigid objects, they present great difficulties in emulating the feeling of remote/virtual stiffness. In addition, they tend to be heavy, cumbersome and usually they only allow limited operator workspace. In this paper a novel haptic interface is presented to enable human-operators to "feel" and intuitively mirror the stiffness/forces at remote/virtual sites enabling control of robots as human-surrogates. This haptic interface is intended to provide human operators intuitive feeling of the stiffness and forces at remote or virtual sites in support of space robots performing dexterous manipulation tasks (such as operating a wrench or a drill). Remote applications are referred to the control of actual robots whereas virtual applications are referred to simulated operations. The developed haptic interface will be applicable to IVA operated robotic EVA tasks to enhance human performance, extend crew capability and assure crew safety. The electrically controlled stiffness is obtained using constrained ElectroRheological <span class="hlt">Fluids</span> (ERF), which changes its viscosity under electrical stimulation. Forces applied at the robot end-effector due to a compliant environment will be reflected to the user using this ERF device where a change in the system viscosity will occur proportionally to the force to be transmitted. In this paper, we will present the results of our <span class="hlt">modeling</span>, simulation, and initial testing of such an</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4824672','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4824672"><span>Inter-Operator Dependence of Magnetic Resonance Image-<span class="hlt">Based</span> Computational <span class="hlt">Fluid</span> Dynamics Prediction of Cerebrospinal <span class="hlt">Fluid</span> Motion in the Cervical Spine</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Martin, Bryn A.; Yiallourou, Theresia I.; Pahlavian, Soroush Heidari; Thyagaraj, Suraj; Bunck, Alexander C.; Loth, Francis; Sheffer, Daniel B.; Kröger, Jan Robert; Stergiopulos, Nikolaos</p> <p>2015-01-01</p> <p>For the first time, inter-operator dependence of MRI <span class="hlt">based</span> computational <span class="hlt">fluid</span> dynamics (CFD) <span class="hlt">modeling</span> of cerebrospinal <span class="hlt">fluid</span> (CSF) in the cervical spinal subarachnoid space (SSS) is evaluated. In vivo MRI flow measurements and anatomy MRI images were obtained at the cervico-medullary junction of a healthy subject and a Chiari I malformation patient. 3D anatomies of the SSS were reconstructed by manual segmentation by four independent operators for both cases. CFD results were compared at nine axial locations along the SSS in terms of hydrodynamic and geometric parameters. Intraclass correlation (ICC) assessed the inter-operator agreement for each parameter over the axial locations and coefficient of variance (CV) compared the percentage of variance for each parameter between the operators. Greater operator dependence was found for the patient (0.19<ICC<0.99) near the craniovertebral junction compared to the healthy subject (ICC > 0.78). For the healthy subject, hydraulic diameter and Womersley number had the least variance (CV= ~2%). For the patient, peak diastolic velocity and Reynolds number had the smallest variance (CV= ~3%). These results show a high degree of inter-operator reliability for MRI-<span class="hlt">based</span> CFD simulations of CSF flow in the cervical spine for healthy subjects and a lower degree of reliability for patients with Type I Chiari malformation. PMID:26446009</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/24511922','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/24511922"><span>Group contribution methodology <span class="hlt">based</span> on the statistical associating <span class="hlt">fluid</span> theory for heteronuclear molecules formed from Mie segments.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Papaioannou, Vasileios; Lafitte, Thomas; Avendaño, Carlos; Adjiman, Claire S; Jackson, George; Müller, Erich A; Galindo, Amparo</p> <p>2014-02-07</p> <p>A generalization of the recent version of the statistical associating <span class="hlt">fluid</span> theory for variable range Mie potentials [Lafitte et al., J. Chem. Phys. 139, 154504 (2013)] is formulated within the framework of a group contribution approach (SAFT-γ Mie). Molecules are represented as comprising distinct functional (chemical) groups <span class="hlt">based</span> on a fused heteronuclear molecular <span class="hlt">model</span>, where the interactions between segments are described with the Mie (generalized Lennard-Jonesium) potential of variable attractive and repulsive range. A key feature of the new theory is the accurate description of the monomeric group-group interactions by application of a high-temperature perturbation expansion up to third order. The capabilities of the SAFT-γ Mie approach are exemplified by studying the thermodynamic properties of two chemical families, the n-alkanes and the n-alkyl esters, by developing parameters for the methyl, methylene, and carboxylate functional groups (CH3, CH2, and COO). The approach is shown to describe accurately the <span class="hlt">fluid</span>-phase behavior of the compounds considered with absolute average deviations of 1.20% and 0.42% for the vapor pressure and saturated liquid density, respectively, which represents a clear improvement over other existing SAFT-<span class="hlt">based</span> group contribution approaches. The use of Mie potentials to describe the group-group interaction is shown to allow accurate simultaneous descriptions of the <span class="hlt">fluid</span>-phase behavior and second-order thermodynamic derivative properties of the pure <span class="hlt">fluids</span> <span class="hlt">based</span> on a single set of group parameters. Furthermore, the application of the perturbation expansion to third order for the description of the reference monomeric <span class="hlt">fluid</span> improves the predictions of the theory for the <span class="hlt">fluid</span>-phase behavior of pure components in the near-critical region. The predictive capabilities of the approach stem from its formulation within a group-contribution formalism: predictions of the <span class="hlt">fluid</span>-phase behavior and thermodynamic derivative properties of</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..1813704S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..1813704S"><span>Geochemical <span class="hlt">modeling</span> of subsurface <span class="hlt">fluid</span> generation in the Gulf of Cadiz</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Schmidt, Christopher; Hensen, Christian; Wallmann, Klaus</p> <p>2016-04-01</p> <p>During RV METEOR cruise M86/5 in 2012 a number of deep-sea mud volcanoes were discovered at about 4500 m water depth west of the deformation front of the accretionary wedge in the Gulf of Cadiz (NE Atlantic). <span class="hlt">Fluid</span> flow at these locations is mediated by an active strike-slip fault marking the transcurrent plate boundary between Africa and Eurasia. Geochemical signals of emanating <span class="hlt">fluids</span> have been interpreted as being a mixture of various deep-sourced processes such as the alteration of oceanic crust, clay-mineral dehydration, and recrystallization of carbonaceous, Upper Jurassic sediments (Hensen et al. 2015). In the current study we present results of a geochemical reactive-transport <span class="hlt">model</span> that was designed to simulate major <span class="hlt">fluid</span>-affecting processes, such as the smectite to illite transformation or recrystallization of carbonates in order to provide a proof of concept. Preliminary results show that the <span class="hlt">model</span> is able to reproduce pore water signatures (e.g. for chloride, strontium, 87Sr/86Sr) in subsurface sediments that are similar to those of MV <span class="hlt">fluids</span>. Hensen, C., Scholz, F., Nuzzo, M., Valadares, V., Gràcia, E., Terrinha, P., Liebetrau, V., Kaul, N., Silva, S., Martínez-Loriente, S., Bartolome, R., Piñero, E., Magalhães, V.H., Schmidt, M., Weise, S.M., Cunha, M., Hilario, A., Perea, H., Rovelli, L. and Lackschewitz, K. (2015) Strike-slip faults mediate the rise of crustal-derived <span class="hlt">fluids</span> and mud volcanism in the deep sea. Geology 43, 339-342.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017SMaS...26b5025F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017SMaS...26b5025F"><span>Impact behavior of a high viscosity magnetorheological <span class="hlt">fluid-based</span> energy absorber with a radial flow mode</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Fu, Benyuan; Liao, Changrong; Li, Zhuqiang; Xie, Lei; Zhang, Peng; Jian, Xiaochun</p> <p>2017-02-01</p> <p>High viscosity linear polysiloxane magnetorheological <span class="hlt">fluid</span> (HVLP MRF) was demonstrated with excellent suspension stability. Such material is suitable for application in the magnetorheological energy absorbers (MREAs) under axial impact loading conditions. On this basis, a new energy absorber incorporating a radial valve with high magnetic field utilization and a corrugated tube is proposed. In energy absorption applications where the MREA is rarely if ever used, our MREA takes the ultra-stable HVLP MRF as controlled medium in order for a long-term stability. For MREA performing at very high shear rates where the minor losses are important contributing factors to damping, a nonlinear analytical <span class="hlt">model</span>, <span class="hlt">based</span> on the Herschel-Bulkley flow <span class="hlt">model</span> (HB <span class="hlt">model</span>), is developed taking into account the effects of minor losses (called HBM <span class="hlt">model</span>). The HB <span class="hlt">model</span> parameters are determined by rheological experiments with a commercial shear rheometer. Then, continuity equation and governing differential equation of the HVLP MRF in radial flow are established. <span class="hlt">Based</span> on the HB <span class="hlt">model</span>, the expressions of radial velocity distribution are deduced. The influences of minor losses on pressure drop are analyzed with mean <span class="hlt">fluid</span> velocities. Further, mechanical behavior of the corrugated tube is investigated via drop test. In order to verify the theoretical methodology, a MREA is fabricated and tested using a high-speed drop tower facility with a 600 kg mass at different drop heights and in various magnetic fields. The experiment results show that the HBM <span class="hlt">model</span> is capable of well predicting the impact behavior of the proposed MREA.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013PhyS...88c5005S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013PhyS...88c5005S"><span>Simple cubic equation of state applied to hard-sphere, Lennard-Jones <span class="hlt">fluids</span>, simple <span class="hlt">fluids</span> and solids</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sun, Jiu-Xun; Cai, Ling-Cang; Wu, Qiang; Jin, Ke</p> <p>2013-09-01</p> <p><span class="hlt">Based</span> on the expansion and extension of the virial equation of state (EOS) of hard-sphere <span class="hlt">fluids</span> solved by the Percus-Yevick integration equation, a universal cubic (UC) EOS is developed. The UC EOS is applied to <span class="hlt">model</span> hard-sphere and Lennard-Jones (LJ) <span class="hlt">fluids</span>, simple Ar and N2 liquids at low temperatures, and supercritical Ar and N2 <span class="hlt">fluids</span> at high temperatures, as well as ten solids, respectively. The three parameters are determined for the hard-sphere <span class="hlt">fluid</span> by fitting molecular dynamics (MD) simulation data of the third to eighth virial coefficients in the literature; for other <span class="hlt">fluids</span> by fitting isothermal compression data; and for solids by using the Einstein <span class="hlt">model</span>. The results show that the UC EOS gives better results than the Carnahan-Starling EOS for compressibility of hard-sphere <span class="hlt">fluids</span>. The Helmholtz free energy and internal energy for LJ <span class="hlt">fluids</span> are predicted and compared with MD simulation data. The calculated pressures for simple Ar and N2 liquids are compared with experimental data. The agreement is fairly good. Eight three-parameter EOSs are applied to describe isothermals of ten typical solids. It is shown that the UC EOS gives the best precision with correct behavior at high-pressure limitation. The UC EOS considering thermal effects is used to analytically evaluate the isobaric thermal expansivity and isothermal compressibility coefficients. The results are in good agreement with experimental data.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/25219260','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25219260"><span>[Present status and trend of heart <span class="hlt">fluid</span> mechanics research <span class="hlt">based</span> on medical image analysis].</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Gan, Jianhong; Yin, Lixue; Xie, Shenghua; Li, Wenhua; Lu, Jing; Luo, Anguo</p> <p>2014-06-01</p> <p>With introduction of current main methods for heart <span class="hlt">fluid</span> mechanics researches, we studied the characteristics and weakness for three primary analysis methods <span class="hlt">based</span> on magnetic resonance imaging, color Doppler ultrasound and grayscale ultrasound image, respectively. It is pointed out that particle image velocity (PIV), speckle tracking and block match have the same nature, and three algorithms all adopt block correlation. The further analysis shows that, with the development of information technology and sensor, the research for cardiac function and <span class="hlt">fluid</span> mechanics will focus on energy transfer process of heart <span class="hlt">fluid</span>, characteristics of Chamber wall related to blood <span class="hlt">fluid</span> and <span class="hlt">Fluid</span>-structure interaction in the future heart <span class="hlt">fluid</span> mechanics fields.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29776036','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29776036"><span>Entropic lattice Boltzmann <span class="hlt">model</span> for charged leaky dielectric multiphase <span class="hlt">fluids</span> in electrified jets.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Lauricella, Marco; Melchionna, Simone; Montessori, Andrea; Pisignano, Dario; Pontrelli, Giuseppe; Succi, Sauro</p> <p>2018-03-01</p> <p>We present a lattice Boltzmann <span class="hlt">model</span> for charged leaky dielectric multiphase <span class="hlt">fluids</span> in the context of electrified jet simulations, which are of interest for a number of production technologies including electrospinning. The role of nonlinear rheology on the dynamics of electrified jets is considered by exploiting the Carreau <span class="hlt">model</span> for pseudoplastic <span class="hlt">fluids</span>. We report exploratory simulations of charged droplets at rest and under a constant electric field, and we provide results for charged jet formation under electrospinning conditions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/19244007','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/19244007"><span>A diffusion tensor imaging tractography algorithm <span class="hlt">based</span> on Navier-Stokes <span class="hlt">fluid</span> mechanics.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Hageman, Nathan S; Toga, Arthur W; Narr, Katherine L; Shattuck, David W</p> <p>2009-03-01</p> <p>We introduce a <span class="hlt">fluid</span> mechanics <span class="hlt">based</span> tractography method for estimating the most likely connection paths between points in diffusion tensor imaging (DTI) volumes. We customize the Navier-Stokes equations to include information from the diffusion tensor and simulate an artificial <span class="hlt">fluid</span> flow through the DTI image volume. We then estimate the most likely connection paths between points in the DTI volume using a metric derived from the <span class="hlt">fluid</span> velocity vector field. We validate our algorithm using digital DTI phantoms <span class="hlt">based</span> on a helical shape. Our method segmented the structure of the phantom with less distortion than was produced using implementations of heat-<span class="hlt">based</span> partial differential equation (PDE) and streamline <span class="hlt">based</span> methods. In addition, our method was able to successfully segment divergent and crossing fiber geometries, closely following the ideal path through a digital helical phantom in the presence of multiple crossing tracts. To assess the performance of our algorithm on anatomical data, we applied our method to DTI volumes from normal human subjects. Our method produced paths that were consistent with both known anatomy and directionally encoded color images of the DTI dataset.</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/22622213-blended-continuousdiscontinuous-finite-element-method-solving-multi-fluid-plasma-model','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22622213-blended-continuousdiscontinuous-finite-element-method-solving-multi-fluid-plasma-model"><span>A blended continuous–discontinuous finite element method for solving the multi-<span class="hlt">fluid</span> plasma <span class="hlt">model</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>Sousa, E.M., E-mail: sousae@uw.edu; Shumlak, U., E-mail: shumlak@uw.edu</p> <p></p> <p>The multi-<span class="hlt">fluid</span> plasma <span class="hlt">model</span> represents electrons, multiple ion species, and multiple neutral species as separate <span class="hlt">fluids</span> that interact through short-range collisions and long-range electromagnetic fields. The <span class="hlt">model</span> spans a large range of temporal and spatial scales, which renders the <span class="hlt">model</span> stiff and presents numerical challenges. To address the large range of timescales, a blended continuous and discontinuous Galerkin method is proposed, where the massive ion and neutral species are <span class="hlt">modeled</span> using an explicit discontinuous Galerkin method while the electrons and electromagnetic fields are <span class="hlt">modeled</span> using an implicit continuous Galerkin method. This approach is able to capture large-gradient ion and neutralmore » physics like shock formation, while resolving high-frequency electron dynamics in a computationally efficient manner. The details of the Blended Finite Element Method (BFEM) are presented. The numerical method is benchmarked for accuracy and tested using two-<span class="hlt">fluid</span> one-dimensional soliton problem and electromagnetic shock problem. The results are compared to conventional finite volume and finite element methods, and demonstrate that the BFEM is particularly effective in resolving physics in stiff problems involving realistic physical parameters, including realistic electron mass and speed of light. The benefit is illustrated by computing a three-<span class="hlt">fluid</span> plasma application that demonstrates species separation in multi-component plasmas.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018PhyD..370...14C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018PhyD..370...14C"><span>Exact closed-form solutions of a fully nonlinear asymptotic two-<span class="hlt">fluid</span> <span class="hlt">model</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Cheviakov, Alexei F.</p> <p>2018-05-01</p> <p>A fully nonlinear <span class="hlt">model</span> of Choi and Camassa (1999) describing one-dimensional incompressible dynamics of two non-mixing <span class="hlt">fluids</span> in a horizontal channel, under a shallow water approximation, is considered. An equivalence transformation is presented, leading to a special dimensionless form of the system, involving a single dimensionless constant physical parameter, as opposed to five parameters present in the original <span class="hlt">model</span>. A first-order dimensionless ordinary differential equation describing traveling wave solutions is analyzed. Several multi-parameter families of physically meaningful exact closed-form solutions of the two-<span class="hlt">fluid</span> <span class="hlt">model</span> are derived, corresponding to periodic, solitary, and kink-type bidirectional traveling waves; specific examples are given, and properties of the exact solutions are analyzed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/23100209','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/23100209"><span>Irrigation of human prepared root canal--ex vivo <span class="hlt">based</span> computational <span class="hlt">fluid</span> dynamics analysis.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Snjaric, Damir; Carija, Zoran; Braut, Alen; Halaji, Adelaida; Kovacevic, Maja; Kuis, Davor</p> <p>2012-10-01</p> <p>To analyze the influence of the needle type, insertion depth, and irrigant flow rate on irrigant flow pattern, flow velocity, and apical pressure by ex-vivo <span class="hlt">based</span> endodontic irrigation computational <span class="hlt">fluid</span> dynamics (CFD) analysis. Human upper canine root canal was prepared using rotary files. Contrast <span class="hlt">fluid</span> was introduced in the root canal and scanned by computed tomography (CT) providing a three-dimensional object that was exported to the computer-assisted design (CAD) software. Two probe points were established in the apical portion of the root canal <span class="hlt">model</span> for flow velocity and pressure measurement. Three different CAD <span class="hlt">models</span> of 27G irrigation needles (closed-end side-vented, notched open-end, and bevel open-end) were created and placed at 25, 50, 75, and 95% of the working length (WL). Flow rates of 0.05, 0.1, 0.2, 0.3, and 0.4 mL/s were simulated. A total of 60 irrigation simulations were performed by CFD <span class="hlt">fluid</span> flow solver. Closed-end side-vented needle required insertion depth closer to WL, regarding efficient irrigant replacement, compared to open-end irrigation needle types, which besides increased velocity produced increased irrigant apical pressure. For all irrigation needle types and needle insertion depths, the increase of flow rate was followed by an increased irrigant apical pressure. The human root canal shape obtained by CT is applicable in the CFD analysis of endodontic irrigation. All the analyzed values -irrigant flow pattern, velocity, and pressure - were influenced by irrigation needle type, as well as needle insertion depth and irrigant flow rate.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012MMTB...43...39H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012MMTB...43...39H"><span>Computational <span class="hlt">Fluid</span> Dynamic <span class="hlt">Modeling</span> of Zinc Slag Fuming Process in Top-Submerged Lance Smelting Furnace</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Huda, Nazmul; Naser, Jamal; Brooks, Geoffrey; Reuter, Markus A.; Matusewicz, Robert W.</p> <p>2012-02-01</p> <p>Slag fuming is a reductive treatment process for molten zinciferous slags for extracting zinc in the form of metal vapor by injecting or adding a reductant source such as pulverized coal or lump coal and natural gas. A computational <span class="hlt">fluid</span> dynamic (CFD) <span class="hlt">model</span> was developed to study the zinc slag fuming process from imperial smelting furnace (ISF) slag in a top-submerged lance furnace and to investigate the details of <span class="hlt">fluid</span> flow, reaction kinetics, and heat transfer in the furnace. The <span class="hlt">model</span> integrates combustion phenomena and chemical reactions with the heat, mass, and momentum interfacial interaction between the phases present in the system. A commercial CFD package AVL Fire 2009.2 (AVL, Graz, Austria) coupled with a number of user-defined subroutines in FORTRAN programming language were used to develop the <span class="hlt">model</span>. The <span class="hlt">model</span> is <span class="hlt">based</span> on three-dimensional (3-D) Eulerian multiphase flow approach, and it predicts the velocity and temperature field of the molten slag bath, generated turbulence, and vortex and plume shape at the lance tip. The <span class="hlt">model</span> also predicts the mass fractions of slag and gaseous components inside the furnace. The <span class="hlt">model</span> predicted that the percent of ZnO in the slag bath decreases linearly with time and is consistent broadly with the experimental data. The zinc fuming rate from the slag bath predicted by the <span class="hlt">model</span> was validated through macrostep validation process against the experimental study of Waladan et al. The <span class="hlt">model</span> results predicted that the rate of ZnO reduction is controlled by the mass transfer of ZnO from the bulk slag to slag-gas interface and rate of gas-carbon reaction for the specified simulation time studied. Although the <span class="hlt">model</span> is <span class="hlt">based</span> on zinc slag fuming, the basic approach could be expanded or applied for the CFD analysis of analogous systems.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016ThCFD..30..139F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016ThCFD..30..139F"><span>Immersed boundary-finite element <span class="hlt">model</span> of <span class="hlt">fluid</span>-structure interaction in the aortic root</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Flamini, Vittoria; DeAnda, Abe; Griffith, Boyce E.</p> <p>2016-04-01</p> <p>It has long been recognized that aortic root elasticity helps to ensure efficient aortic valve closure, but our understanding of the functional importance of the elasticity and geometry of the aortic root continues to evolve as increasingly detailed in vivo imaging data become available. Herein, we describe a <span class="hlt">fluid</span>-structure interaction <span class="hlt">model</span> of the aortic root, including the aortic valve leaflets, the sinuses of Valsalva, the aortic annulus, and the sinotubular junction, that employs a version of Peskin's immersed boundary (IB) method with a finite element description of the structural elasticity. As in earlier work, we use a fiber-<span class="hlt">based</span> <span class="hlt">model</span> of the valve leaflets, but this study extends earlier IB <span class="hlt">models</span> of the aortic root by employing an incompressible hyperelastic <span class="hlt">model</span> of the mechanics of the sinuses and ascending aorta using a constitutive law fit to experimental data from human aortic root tissue. In vivo pressure loading is accounted for by a backward displacement method that determines the unloaded configuration of the root <span class="hlt">model</span>. Our <span class="hlt">model</span> yields realistic cardiac output at physiological pressures, with low transvalvular pressure differences during forward flow, minimal regurgitation during valve closure, and realistic pressure loads when the valve is closed during diastole. Further, results from high-resolution computations indicate that although the detailed leaflet and root kinematics show some grid sensitivity, our IB <span class="hlt">model</span> of the aortic root nonetheless produces essentially grid-converged flow rates and pressures at practical grid spacings for the high Reynolds number flows of the aortic root. These results thereby clarify minimum grid resolutions required by such <span class="hlt">models</span> when used as stand-alone <span class="hlt">models</span> of the aortic valve as well as when used to provide <span class="hlt">models</span> of the outflow valves in <span class="hlt">models</span> of left-ventricular <span class="hlt">fluid</span> dynamics.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20040010360','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20040010360"><span>A New Modular Approach for Tightly Coupled <span class="hlt">Fluid</span>/Structure Analysis</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Guruswamy, Guru</p> <p>2003-01-01</p> <p>Static aeroelastic computations are made using a C++ executive suitable for closely coupled <span class="hlt">fluid</span>/structure interaction studies. The <span class="hlt">fluid</span> flow is <span class="hlt">modeled</span> using the Euler/Navier Stokes equations and the structure is <span class="hlt">modeled</span> using finite elements. FORTRAN <span class="hlt">based</span> <span class="hlt">fluids</span> and structures codes are integrated under C++ environment. The flow and structural solvers are treated as separate object files. The data flow between <span class="hlt">fluids</span> and structures is accomplished using I/O. Results are demonstrated for transonic flow over partially flexible surface that is important for aerospace vehicles. Use of this development to accurately predict flow induced structural failure will be demonstrated.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011PMB....56.6179R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011PMB....56.6179R"><span>Predictive <span class="hlt">models</span> for pressure-driven <span class="hlt">fluid</span> infusions into brain parenchyma</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Raghavan, Raghu; Brady, Martin</p> <p>2011-10-01</p> <p>Direct infusions into brain parenchyma of biological therapeutics for serious brain diseases have been, and are being, considered. However, individual brains, as well as distinct cytoarchitectural regions within brains, vary in their response to <span class="hlt">fluid</span> flow and pressure. Further, the tissue responds dynamically to these stimuli, requiring a nonlinear treatment of equations that would describe <span class="hlt">fluid</span> flow and drug transport in brain. We here report in detail on an individual-specific <span class="hlt">model</span> and a comparison of its prediction with simulations for living porcine brains. Two critical features we introduced into our model—absent from previous ones, but requirements for any useful simulation—are the infusion-induced interstitial expansion and the backflow. These are significant determinants of the flow. Another feature of our treatment is the use of cross-property relations to obtain individual-specific parameters that are coefficients in the equations. The quantitative results are at least encouraging, showing a high fraction of overlap between the computed and measured volumes of distribution of a tracer molecule and are potentially clinically useful. Several improvements are called for; principally a treatment of the interstitial expansion more fundamentally <span class="hlt">based</span> on poroelasticity and a better delineation of the diffusion tensor of a particle confined to the interstitial spaces.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/1415821-molecular-debye-huckel-theory-solvation-polar-fluids-extension-born-model','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/1415821-molecular-debye-huckel-theory-solvation-polar-fluids-extension-born-model"><span>A molecular Debye-Huckel theory of solvation in polar <span class="hlt">fluids</span>: An extension of the Born <span class="hlt">model</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>Xiao, Tiejun; Song, Xueyu</p> <p></p> <p>A dielectric response theory of solvation beyond the conventional Born <span class="hlt">model</span> for polar <span class="hlt">fluids</span> is presented. The dielectric response of a polar <span class="hlt">fluid</span> is described by a Born response mode and a linear combination of Debye-Hückel-like response modes that capture the nonlocal response of polar <span class="hlt">fluids</span>. The Born mode is characterized by a bulk dielectric constant, while a Debye-Hückel mode is characterized by its corresponding Debye screening length. Both the bulk dielectric constant and the Debye screening lengths are determined from the bulk dielectric function of the polar <span class="hlt">fluid</span>. The linear combination coefficients of the response modes are evaluated inmore » a self-consistent way and can be used to evaluate the electrostatic contribution to the thermodynamic properties of a polar <span class="hlt">fluid</span>. In conclusion, our theory is applied to a dipolar hard sphere <span class="hlt">fluid</span> as well as interaction site <span class="hlt">models</span> of polar <span class="hlt">fluids</span> such as water, where the electrostatic contribution to their thermodynamic properties can be obtained accurately.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1415821-molecular-debye-huckel-theory-solvation-polar-fluids-extension-born-model','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1415821-molecular-debye-huckel-theory-solvation-polar-fluids-extension-born-model"><span>A molecular Debye-Huckel theory of solvation in polar <span class="hlt">fluids</span>: An extension of the Born <span class="hlt">model</span></span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Xiao, Tiejun; Song, Xueyu</p> <p>2017-12-06</p> <p>A dielectric response theory of solvation beyond the conventional Born <span class="hlt">model</span> for polar <span class="hlt">fluids</span> is presented. The dielectric response of a polar <span class="hlt">fluid</span> is described by a Born response mode and a linear combination of Debye-Hückel-like response modes that capture the nonlocal response of polar <span class="hlt">fluids</span>. The Born mode is characterized by a bulk dielectric constant, while a Debye-Hückel mode is characterized by its corresponding Debye screening length. Both the bulk dielectric constant and the Debye screening lengths are determined from the bulk dielectric function of the polar <span class="hlt">fluid</span>. The linear combination coefficients of the response modes are evaluated inmore » a self-consistent way and can be used to evaluate the electrostatic contribution to the thermodynamic properties of a polar <span class="hlt">fluid</span>. In conclusion, our theory is applied to a dipolar hard sphere <span class="hlt">fluid</span> as well as interaction site <span class="hlt">models</span> of polar <span class="hlt">fluids</span> such as water, where the electrostatic contribution to their thermodynamic properties can be obtained accurately.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28340405','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28340405"><span>Population pharmacokinetic <span class="hlt">modeling</span> of furosemide in patients with hypertension and <span class="hlt">fluid</span> overload conditions.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Kodati, Devender; Yellu, Narsimhareddy</p> <p>2017-06-01</p> <p>Furosemide is a loop diuretic drug frequently indicated in hypertension and <span class="hlt">fluid</span> overload conditions such as congestive heart failure and hepatic cirrhosis. The purpose of the study was to establish a population pharmacokinetic <span class="hlt">model</span> for furosemide in Indian hypertensive and <span class="hlt">fluid</span> overload patients, and to evaluate effects of covariates on the volume of distribution (V/F) and oral clearance (CL/F) of furosemide. A total of 188 furosemide plasma sample concentrations from 63 patients with hypertension or <span class="hlt">fluid</span> overload conditions were collected in this study. The population pharmacokinetic <span class="hlt">model</span> for furosemide was built using Phoenix NLME 1.3 software. The covariates included age, sex, body surface area, bodyweight, height and creatinine clearance (CRCL). The pharmacokinetic data of furosemide was adequately explained by a two-compartment linear pharmacokinetic <span class="hlt">model</span> with first-order absorption and an absorption lag-time. The mean values of CL/F and Vd/F of furosemide in the patients were 15.054Lh -1 and 4.419L, respectively. Analysis of covariates showed that CRCL was significantly influencing the clearance of furosemide. The final population pharmacokinetic <span class="hlt">model</span> was demonstrated to be appropriate and effective and it can be used to assess the pharmacokinetic parameters of furosemide in Indian patients with hypertension and <span class="hlt">fluid</span> overload conditions. Copyright © 2017. Published by Elsevier Urban & Partner Sp. z o.o.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018E%26ES..147a2035S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018E%26ES..147a2035S"><span>Evaluation of Working <span class="hlt">Fluids</span> for Organic Rankine Cycle <span class="hlt">Based</span> on Exergy Analysis</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Setiawan, D.; Subrata, I. D. M.; Purwanto, Y. A.; Tambunan, A. H.</p> <p>2018-05-01</p> <p>One of the crucial aspects to determine the performance of Organic Rankine Cycle (ORC) is the selection of appropriate working <span class="hlt">fluids</span>. This paper describes the simulative performance of several organic <span class="hlt">fluid</span> and water as working <span class="hlt">fluid</span> of an ORC <span class="hlt">based</span> on exergy analysis with a heat source from waste heat recovery. The simulation was conducted by using Engineering Equation Solver (EES). The effect of several parameters and thermodynamic properties of working <span class="hlt">fluid</span> was analyzed, and part of them was used as variables for the simulation in order to determine their sensitivity to the exergy efficiency changes. The results of this study showed that water is not appropriate to be used as working <span class="hlt">fluid</span> at temperature lower than 130 °C, because the expansion process falls in saturated area. It was also found that Benzene had the highest exergy efficiency, i.e. about 10.49%, among the dry type working <span class="hlt">fluid</span>. The increasing turbine inlet temperature did not lead to the increase of exergy efficiency when using organic working <span class="hlt">fluids</span> with critical temperature near heat source temperature. Meanwhile, exergy efficiency decreasing linearly with the increasing condenser inlet temperature. In addition, it was found that working <span class="hlt">fluid</span> with high latent heat of vaporization and specific heat exert in high exergy efficiency.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2005AGUFM.T53B1431Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2005AGUFM.T53B1431Z"><span>Development of a New Analog Test System Capable of <span class="hlt">Modeling</span> Tectonic Deformation Incorporating the Effects of Pore <span class="hlt">Fluid</span> Pressure</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zhang, M.; Nakajima, H.; Takeda, M.; Aung, T. T.</p> <p>2005-12-01</p> <p> deep geological disposal concept, besides containing the wastes with engineering methods such as the glassification of the radioactive wastes, the geological formation itself is expected to serve as a natural barrier that retards migration of radionuclides. To evaluate the long-term safety of deep geological disposal, a better understanding of the fate and transport of radionuclides in a geologically heterogeneous environment is necessary. To meet such requirements, a new analog test sandbox <span class="hlt">model</span> system was developed. This <span class="hlt">model</span> system allows the pore <span class="hlt">fluid</span> flows to be controlled during the <span class="hlt">model</span> tests and permits the study of flow and transport phenomena in the deformed heterogeneous <span class="hlt">model</span>. One- or two-dimensional <span class="hlt">fluid</span> flow is controlled using a side-wall piston. Deformation processes can be observed through a transparent front panel, and pore <span class="hlt">fluid</span> movement can be also visualized using a color tracer. In this study, the scaling requirements for analog <span class="hlt">modeling</span>, including pore water pressure, are discussed <span class="hlt">based</span> on the theory of dimensional analysis, supplemented by data from a series of laboratory shear tests, and a detailed description of the <span class="hlt">model</span> system. Preliminary experimental results are presented.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2005JMMM..289..415K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2005JMMM..289..415K"><span>The DC dielectric breakdown strength of magnetic <span class="hlt">fluids</span> <span class="hlt">based</span> on transformer oil</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kopčanský, Peter; Tomčo, Ladislav; Marton, Karol; Koneracká, Martina; Timko, Milan; Potočová, Ivana</p> <p>2005-03-01</p> <p>The DC dielectric breakdown strength of magnetic <span class="hlt">fluids</span> <span class="hlt">based</span> on transformer oil TECHNOL US 4000, with different saturation magnetizations, was investigated in various orientations of external magnetic field. It was shown that the dielectric breakdown strength in H∣∣ E is strongly influenced by the aggregation effects. As a boundary volume concentration of magnetic particles, below which the magnetic <span class="hlt">fluids</span> have better dielectric properties than pure transformer oil, the volume concentration Φ=0.01 was found. Thus magnetic <span class="hlt">fluids</span> with Φ<0.01 are suitable for the use as a high-voltage insulation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016JSG....93...17Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016JSG....93...17Z"><span>Numerical <span class="hlt">modelling</span> of fault reactivation in carbonate rocks under <span class="hlt">fluid</span> depletion conditions - 2D generic <span class="hlt">models</span> with a small isolated fault</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zhang, Yanhua; Clennell, Michael B.; Delle Piane, Claudio; Ahmed, Shakil; Sarout, Joel</p> <p>2016-12-01</p> <p>This generic 2D elastic-plastic <span class="hlt">modelling</span> investigated the reactivation of a small isolated and critically-stressed fault in carbonate rocks at a reservoir depth level for <span class="hlt">fluid</span> depletion and normal-faulting stress conditions. The <span class="hlt">model</span> properties and boundary conditions are <span class="hlt">based</span> on field and laboratory experimental data from a carbonate reservoir. The results show that a pore pressure perturbation of -25 MPa by depletion can lead to the reactivation of the fault and parts of the surrounding damage zones, producing normal-faulting downthrows and strain localization. The mechanism triggering fault reactivation in a carbonate field is the increase of shear stresses with pore-pressure reduction, due to the decrease of the absolute horizontal stress, which leads to an expanded Mohr's circle and mechanical failure, consistent with the predictions of previous poroelastic <span class="hlt">models</span>. Two scenarios for fault and damage-zone permeability development are explored: (1) large permeability enhancement of a sealing fault upon reactivation, and (2) fault and damage zone permeability development governed by effective mean stress. In the first scenario, the fault becomes highly permeable to across- and along-fault <span class="hlt">fluid</span> transport, removing local pore pressure highs/lows arising from the presence of the initially sealing fault. In the second scenario, reactivation induces small permeability enhancement in the fault and parts of damage zones, followed by small post-reactivation permeability reduction. Such permeability changes do not appear to change the original flow capacity of the fault or modify the <span class="hlt">fluid</span> flow velocity fields dramatically.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://cfpub.epa.gov/si/si_public_record_report.cfm?dirEntryId=140827&keyword=environmental+AND+wind+AND+tunnel&actType=&TIMSType=+&TIMSSubTypeID=&DEID=&epaNumber=&ntisID=&archiveStatus=Both&ombCat=Any&dateBeginCreated=&dateEndCreated=&dateBeginPublishedPresented=&dateEndPublishedPresented=&dateBeginUpdated=&dateEndUpdated=&dateBeginCompleted=&dateEndCompleted=&personID=&role=Any&journalID=&publisherID=&sortBy=revisionDate&count=50','EPA-EIMS'); return false;" href="https://cfpub.epa.gov/si/si_public_record_report.cfm?dirEntryId=140827&keyword=environmental+AND+wind+AND+tunnel&actType=&TIMSType=+&TIMSSubTypeID=&DEID=&epaNumber=&ntisID=&archiveStatus=Both&ombCat=Any&dateBeginCreated=&dateEndCreated=&dateBeginPublishedPresented=&dateEndPublishedPresented=&dateBeginUpdated=&dateEndUpdated=&dateBeginCompleted=&dateEndCompleted=&personID=&role=Any&journalID=&publisherID=&sortBy=revisionDate&count=50"><span>THE NOAA/EPA <span class="hlt">FLUID</span> <span class="hlt">MODELING</span> FACILITY'S CONTRIBUTIONS TO THE UNDERSTANDING OF THE ATMOSPHERIC DISPERSION</span></a></p> <p><a target="_blank" href="http://oaspub.epa.gov/eims/query.page">EPA Science Inventory</a></p> <p></p> <p></p> <p>Over the past thirty years, scientists at the Environmental Protection Agency's (EPA) <span class="hlt">Fluid</span> <span class="hlt">Modeling</span> Facility (FMF) have conducted laboratory studies of <span class="hlt">fluid</span> flow and pollutant dispersion within three distinct experimental chambers: a meteorological wind tunnel, a water-channel ...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015IJCFD..29..180P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015IJCFD..29..180P"><span>Multi-<span class="hlt">fluid</span> <span class="hlt">modelling</span> of pulsed discharges for flow control applications</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Poggie, J.</p> <p>2015-02-01</p> <p>Experimental evidence suggests that short-pulse dielectric barrier discharge actuators are effective for speeds corresponding to take-off and approach of large aircraft, and thus are a fruitful direction for flow control technology development. Large-eddy simulations have reproduced some of the main <span class="hlt">fluid</span> dynamic effects. The plasma <span class="hlt">models</span> used in such simulations are semi-empirical, however, and need to be tuned for each flowfield under consideration. In this paper, the discharge physics is examined in more detail with multi-<span class="hlt">fluid</span> <span class="hlt">modelling</span>, comparing a five-moment <span class="hlt">model</span> (continuity, momentum, and energy equations) to a two-moment <span class="hlt">model</span> (continuity and energy equations). A steady-state, one-dimensional discharge was considered first, and the five-moment <span class="hlt">model</span> was found to predict significantly lower ionisation rates and number densities than the two-moment <span class="hlt">model</span>. A two-dimensional, transient discharge problem with an elliptical cathode was studied next. Relative to the two-moment <span class="hlt">model</span>, the five-moment <span class="hlt">model</span> predicted a slower response to the activation of the cathode, and lower electron velocities and temperatures as the simulation approached steady-state. The primary reason for the differences in the predictions of the two <span class="hlt">models</span> can be attributed to the effects of particle inertia, particularly electron inertia in the cathode layer. The computational cost of the five-moment <span class="hlt">model</span> is only about twice that of the simpler variant, suggesting that it may be feasible to use the more sophisticated <span class="hlt">model</span> in practical calculations for flow control actuator design.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27341786','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27341786"><span><span class="hlt">Fluid</span>-structure interaction including volumetric coupling with homogenised subdomains for <span class="hlt">modeling</span> respiratory mechanics.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Yoshihara, Lena; Roth, Christian J; Wall, Wolfgang A</p> <p>2017-04-01</p> <p>In this article, a novel approach is presented for combining standard <span class="hlt">fluid</span>-structure interaction with additional volumetric constraints to <span class="hlt">model</span> <span class="hlt">fluid</span> flow into and from homogenised solid domains. The proposed algorithm is particularly interesting for investigations in the field of respiratory mechanics as it enables the mutual coupling of airflow in the conducting part and local tissue deformation in the respiratory part of the lung by means of a volume constraint. In combination with a classical monolithic <span class="hlt">fluid</span>-structure interaction approach, a comprehensive <span class="hlt">model</span> of the human lung can be established that will be useful to gain new insights into respiratory mechanics in health and disease. To illustrate the validity and versatility of the novel approach, three numerical examples including a patient-specific lung <span class="hlt">model</span> are presented. The proposed algorithm proves its capability of computing clinically relevant airflow distribution and tissue strain data at a level of detail that is not yet achievable, neither with current imaging techniques nor with existing computational <span class="hlt">models</span>. Copyright © 2016 John Wiley & Sons, Ltd. Copyright © 2016 John Wiley & Sons, Ltd.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20050218771&hterms=Post+test+pre+test&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3DPost%2Btest%2Bpre%2Btest','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20050218771&hterms=Post+test+pre+test&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3DPost%2Btest%2Bpre%2Btest"><span><span class="hlt">Fluid</span>-structural dynamics of ground-<span class="hlt">based</span> and microgravity caloric tests</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Kassemi, M.; Oas, J. G.; Deserranno, Dimitri</p> <p>2005-01-01</p> <p>Microgravity caloric tests aboard the 1983 SpaceLab1 mission produced nystagmus results with an intensity comparable to those elicited during post- and pre- flight tests, thus contradicting the basic premise of Barany's convection hypothesis for caloric stimulation. In this work, we present a dynamic <span class="hlt">fluid</span> structural analysis of the caloric stimulation of the lateral semicircular canal <span class="hlt">based</span> on two simultaneous driving forces for the endolymphatic flow: natural convection driven by the temperature-dependent density variation in the bulk <span class="hlt">fluid</span> and expansive convection caused by direct volumetric displacement of the endolymph during the thermal irrigation. Direct numerical simulations indicate that on earth, the natural convection mechanism is dominant. But in the microgravity environment of orbiting spacecraft, where buoyancy effects are mitigated, expansive convection becomes the sole mechanism for producing cupular displacement. A series of transient 1 g and microgravity case studies are presented to delineate the differences between the dynamics of the 1 g and microgravity endolymphatic flows. The impact of these different flow dynamics on the endolymph-cupula <span class="hlt">fluid</span>-structural interactions is also analyzed <span class="hlt">based</span> on the time evolutions of cupular displacement and velocity and the transcupular pressure differences.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/15951623','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/15951623"><span><span class="hlt">Fluid</span>-structural dynamics of ground-<span class="hlt">based</span> and microgravity caloric tests.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Kassemi, M; Oas, J G; Deserranno, Dimitri</p> <p>2005-01-01</p> <p>Microgravity caloric tests aboard the 1983 SpaceLab1 mission produced nystagmus results with an intensity comparable to those elicited during post- and pre- flight tests, thus contradicting the basic premise of Barany's convection hypothesis for caloric stimulation. In this work, we present a dynamic <span class="hlt">fluid</span> structural analysis of the caloric stimulation of the lateral semicircular canal <span class="hlt">based</span> on two simultaneous driving forces for the endolymphatic flow: natural convection driven by the temperature-dependent density variation in the bulk <span class="hlt">fluid</span> and expansive convection caused by direct volumetric displacement of the endolymph during the thermal irrigation. Direct numerical simulations indicate that on earth, the natural convection mechanism is dominant. But in the microgravity environment of orbiting spacecraft, where buoyancy effects are mitigated, expansive convection becomes the sole mechanism for producing cupular displacement. A series of transient 1 g and microgravity case studies are presented to delineate the differences between the dynamics of the 1 g and microgravity endolymphatic flows. The impact of these different flow dynamics on the endolymph-cupula <span class="hlt">fluid</span>-structural interactions is also analyzed <span class="hlt">based</span> on the time evolutions of cupular displacement and velocity and the transcupular pressure differences.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20110015474','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20110015474"><span>Generalized <span class="hlt">Fluid</span> System Simulation Program, Version 5.0-Educational</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Majumdar, A. K.</p> <p>2011-01-01</p> <p>The Generalized <span class="hlt">Fluid</span> System Simulation Program (GFSSP) is a finite-volume <span class="hlt">based</span> general-purpose computer program for analyzing steady state and time-dependent flow rates, pressures, temperatures, and concentrations in a complex flow network. The program is capable of <span class="hlt">modeling</span> real <span class="hlt">fluids</span> with phase changes, compressibility, mixture thermodynamics, conjugate heat transfer between solid and <span class="hlt">fluid</span>, <span class="hlt">fluid</span> transients, pumps, compressors and external body forces such as gravity and centrifugal. The thermofluid system to be analyzed is discretized into nodes, branches, and conductors. The scalar properties such as pressure, temperature, and concentrations are calculated at nodes. Mass flow rates and heat transfer rates are computed in branches and conductors. The graphical user interface allows users to build their <span class="hlt">models</span> using the point, drag and click method; the users can also run their <span class="hlt">models</span> and post-process the results in the same environment. The integrated <span class="hlt">fluid</span> library supplies thermodynamic and thermo-physical properties of 36 <span class="hlt">fluids</span> and 21 different resistance/source options are provided for <span class="hlt">modeling</span> momentum sources or sinks in the branches. This Technical Memorandum illustrates the application and verification of the code through 12 demonstrated example problems.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li class="active"><span>21</span></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_21 --> <div id="page_22" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li class="active"><span>22</span></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li><a href="#" onclick='return showDiv("page_24");'>24</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="421"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/25096081','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25096081"><span>Mesh-free distributed point source method for <span class="hlt">modeling</span> viscous <span class="hlt">fluid</span> motion between disks vibrating at ultrasonic frequency.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Wada, Yuji; Kundu, Tribikram; Nakamura, Kentaro</p> <p>2014-08-01</p> <p>The distributed point source method (DPSM) is extended to <span class="hlt">model</span> wave propagation in viscous <span class="hlt">fluids</span>. Appropriate estimation on attenuation and boundary layer formation due to <span class="hlt">fluid</span> viscosity is necessary for the ultrasonic devices used for acoustic streaming or ultrasonic levitation. The equations for DPSM <span class="hlt">modeling</span> in viscous <span class="hlt">fluids</span> are derived in this paper by decomposing the linearized viscous <span class="hlt">fluid</span> equations into two components-dilatational and rotational components. By considering complex P- and S-wave numbers, the acoustic fields in viscous <span class="hlt">fluids</span> can be calculated following similar calculation steps that are used for wave propagation <span class="hlt">modeling</span> in solids. From the calculations reported the precision of DPSM is found comparable to that of the finite element method (FEM) for a fundamental ultrasonic field problem. The particle velocity parallel to the two bounding surfaces of the viscous <span class="hlt">fluid</span> layer between two rigid plates (one in motion and one stationary) is calculated. The finite element results agree well with the DPSM results that were generated faster than the transient FEM results.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/16877023','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/16877023"><span>A refractometry-<span class="hlt">based</span> glucose analysis of body <span class="hlt">fluids</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Zirk, Kai; Poetzschke, Harald</p> <p>2007-05-01</p> <p>In principle, refractometry appears to be a suitable method for the measurement of glucose concentrations in body <span class="hlt">fluids</span> (such as blood and the intercellular <span class="hlt">fluid</span>), even though the refractive index of the measured samples, as an additive property, is not specific. But, if certain conditions are fulfilled, the glucose content can be calculated using the refractive index in combination with values from a further measurement. This study describes the determination of the glucose content using refractometry in human blood serum derivates, which were selected - due to their ready availability - to be used as a <span class="hlt">model</span> for interstitial <span class="hlt">fluid</span>. Refractometry of body <span class="hlt">fluids</span> requires the elimination of disturbing components from the measurement sample. First of all, a homogenous <span class="hlt">fluid</span> (i.e. consisting of one phase) is required, so that all cells and components in suspension need to be separated out. Furthermore, certain dissolved macromolecular components which are known to disturb the measurement process must also be removed. In human serum samples which had been ultrafiltrated with a range of ultrafilters of different pore sizes, a comparative evaluation showed that only ultrafiltration through a filter with a separation limit of between 3 and 30kDa resulted in maximal reduction of the refractive index (compared to native serum), whereas ultrafilters with greater separation limits did not. The total content of osmotically active solutes (the tonicity) also exerts a clear influence. However, exemplary measurements in blood plasma <span class="hlt">fluid</span> from one volunteer showed that the electrical conductivity is (without an additive component) directly proportional to the osmolality: physiological changes in the state of body hydration (hyperhydration and dehydration) do not lead to any considerable changes in the relation between ionised and uncharged solute particles, but instead result in a sufficiently clear dilution or concentration of the blood <span class="hlt">fluid</span>'s low molecular components. This</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016HydJ...24.1343P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016HydJ...24.1343P"><span>Numerical <span class="hlt">modeling</span> of fracking <span class="hlt">fluid</span> migration through fault zones and fractures in the North German Basin</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Pfunt, Helena; Houben, Georg; Himmelsbach, Thomas</p> <p>2016-09-01</p> <p>Gas production from shale formations by hydraulic fracturing has raised concerns about the effects on the quality of fresh groundwater. The migration of injected fracking <span class="hlt">fluids</span> towards the surface was investigated in the North German Basin, <span class="hlt">based</span> on the known standard lithology. This included cases with natural preferential pathways such as permeable fault zones and fracture networks. Conservative assumptions were applied in the simulation of flow and mass transport triggered by a high pressure boundary of up to 50 MPa excess pressure. The results show no significant <span class="hlt">fluid</span> migration for a case with undisturbed cap rocks and a maximum of 41 m vertical transport within a permeable fault zone during the pressurization. Open fractures, if present, strongly control the flow field and migration; here vertical transport of fracking <span class="hlt">fluids</span> reaches up to 200 m during hydraulic fracturing simulation. Long-term transport of the injected water was simulated for 300 years. The fracking <span class="hlt">fluid</span> rises vertically within the fault zone up to 485 m due to buoyancy. Progressively, it is transported horizontally into sandstone layers, following the natural groundwater flow direction. In the long-term, the injected <span class="hlt">fluids</span> are diluted to minor concentrations. Despite the presence of permeable pathways, the injected fracking <span class="hlt">fluids</span> in the reported <span class="hlt">model</span> did not reach near-surface aquifers, either during the hydraulic fracturing or in the long term. Therefore, the probability of impacts on shallow groundwater by the rise of fracking <span class="hlt">fluids</span> from a deep shale-gas formation through the geological underground to the surface is small.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013PhDT.......319L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013PhDT.......319L"><span>Etude d'un <span class="hlt">modele</span> de Boltzmann sur reseau pour la simulation assistee par ordinateur des <span class="hlt">fluides</span> a plusieurs phases immiscibles</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Leclaire, Sebastien</p> <p></p> <p>The computer assisted simulation of the dynamics of <span class="hlt">fluid</span> flow has been a highly rewarding topic of research for several decades now, in terms of the number of scientific problems that have been solved as a result, both in the academic world and in industry. In the <span class="hlt">fluid</span> dynamics field, simulating multiphase immiscible <span class="hlt">fluid</span> flow remains a challenge, because of the complexity of the interactions at the flow phase interfaces. Various numerical methods are available to study these phenomena, and, the lattice Boltzmann method has been shown in recent years to be well adapted to solving this type of complex flow. In this thesis, a lattice Boltzmann <span class="hlt">model</span> for the simulation of two-phase immiscible flows is studied. The main objective of the thesis is to develop this promising method further, with a view to enhancing its validity. To achieve this objective, the research is divided into five distinct themes. The first two focus on correcting some of the deficiencies of the original <span class="hlt">model</span>. The third generalizes the <span class="hlt">model</span> to support the simulation of N-phase immiscible <span class="hlt">fluid</span> flows. The fourth is aimed at modifying the <span class="hlt">model</span> itself, to enable the simulation of immiscible <span class="hlt">fluid</span> flows in which the density of the phases varies. With the lattice Boltzmann class of <span class="hlt">models</span> studied here, this density variation has been inadequately <span class="hlt">modeled</span>, and, after 20 years, the issue still has not been resolved. The fifth, which complements this thesis, is connected with the lattice Boltzmann method, in that it generalizes the theory of 2D and 3D isotropic gradients for a high order of spatial precision. These themes have each been the subject of a scientific article, as listed in the appendix to this thesis, and together they constitute a synthesis that explains the links between the articles, as well as their scientific contributions, and satisfy the main objective of this research. Globally, a number of qualitative and quantitative test cases <span class="hlt">based</span> on the theory of multiphase <span class="hlt">fluid</span> flows</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017E%26ES...61a2106L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017E%26ES...61a2106L"><span>Numerical simulation of nanofluids <span class="hlt">based</span> on power-law <span class="hlt">fluids</span> with flow and heat transfer</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Li, Lin; Jiang, Yongyue; Chen, Aixin</p> <p>2017-04-01</p> <p>In this paper, we investigate the heat transfer of nanofluids <span class="hlt">based</span> on power-law <span class="hlt">fluids</span> and movement of nanoparticles with the effect of thermophoresis in a rotating circular groove. The velocity of circular groove rotating is a constant and the temperature on the wall is kept to be zero all the time which is different from the temperature of nanofluids in the initial time. The effects of thermophoresis and Brownian diffusion are considered in temperature and concentration equations, and it is assumed that the thermal conductivity of nanofluids is a function of concentration of nanoparticles. <span class="hlt">Based</span> on numerical results, it can be found that nanofluids improve the process of heat transfer than <span class="hlt">base</span> <span class="hlt">fluids</span> in a rotating circular groove. The enhancement of heat transfer increases as the power law index of <span class="hlt">base</span> <span class="hlt">fluids</span> decreases.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2005APS..DFD.EB003G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2005APS..DFD.EB003G"><span>On the Opening of Thick Walled Elastic Tubes: A <span class="hlt">Fluid</span>-Structure <span class="hlt">Model</span> for Acid Reflux</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ghosh, Sudip; Kahrilas, Peter</p> <p>2005-11-01</p> <p>A coupled <span class="hlt">fluid</span>-structure mathematical <span class="hlt">model</span> was developed to quantify rapid opening of thick-walled elastic tubes, a phenomenon underlying biological flows such as gastroesophageal reflux disease (GERD). The wall was <span class="hlt">modeled</span> using non-linear finite deformation theory to predict space-time radial distention of an axisymmetric tube with luminal <span class="hlt">fluid</span> flow. Anisotropic azimuthal and longitudinal muscle-induced stresses were incorporated, and interstitial material properties were assumed isotropic and linearly elastic. <span class="hlt">Fluid</span> flow was <span class="hlt">modeled</span> using lubrication theory with inertial correction. Opening and flow were driven by a specified inflow pressure and zero pressure gradient was specified at outflow. No-slip and surface force balance were applied at the <span class="hlt">fluid</span>-wall interface. Viscoelasticity was <span class="hlt">modeled</span> with ad hoc damping and the evolution of the tube geometry was predicted at mid-layer. A potentially important discovery was made when applied to studies of initiation of opening with GERD: while material stiffness is of minor consequence, small changes in resting lumen distension (˜2 mm diameter) may be a sensitive distinguishing feature of the disease.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013JPhCS.439a2049A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013JPhCS.439a2049A"><span>Design, <span class="hlt">modeling</span> and simulation of MEMS-<span class="hlt">based</span> silicon Microneedles</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Amin, F.; Ahmed, S.</p> <p>2013-06-01</p> <p>The advancement in semiconductor process engineering and nano-scale fabrication technology has made it convenient to transport specific biological <span class="hlt">fluid</span> into or out of human skin with minimum discomfort. <span class="hlt">Fluid</span> transdermal delivery systems such as Microneedle arrays are one such emerging and exciting Micro-Electro Mechanical System (MEMS) application which could lead to a total painless <span class="hlt">fluid</span> delivery into skin with controllability and desirable yield. In this study, we aimed to revisit the problem with <span class="hlt">modeling</span>, design and simulations carried out for MEMS <span class="hlt">based</span> silicon hollow out of plane microneedle arrays for biomedical applications particularly for transdermal drug delivery. An approximate 200 μm length of microneedle with 40 μm diameter of lumen has been successfully shown formed by isotropic and anisotropic etching techniques using MEMS Pro design tool. These microneedles are arranged in size of 2 × 4 matrix array with center to center spacing of 750 μm. Furthermore, comparisons for <span class="hlt">fluid</span> flow characteristics through these microneedle channels have been <span class="hlt">modeled</span> with and without the contribution of the gravitational forces using mathematical <span class="hlt">models</span> derived from Bernoulli Equation. Physical Process simulations have also been performed on TCAD SILVACO to optimize the design of these microneedles aligned with the standard Si-Fabrication lines.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/25017657','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25017657"><span>Immunisations and antibiotics in patients with anterior skull <span class="hlt">base</span> cerebrospinal <span class="hlt">fluid</span> leaks.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Rimmer, J; Belk, C; Lund, V J; Swift, A; White, P</p> <p>2014-07-01</p> <p>There are no UK guidelines for the use of antibiotics and/or immunisations in patients with an active anterior skull <span class="hlt">base</span> cerebrospinal <span class="hlt">fluid</span> leak. This study aimed to define current UK practice in this area and inform appropriate guidelines for ENT surgeons. A web-<span class="hlt">based</span> survey of all members of the British Rhinological Society was carried out and the literature in this area was reviewed. Of those who responded to the survey, 14 per cent routinely give prophylactic antibiotics to patients with cerebrospinal <span class="hlt">fluid</span> leaks, and 34.9 per cent recommend immunisation against at least one organism, most commonly Streptococcus pneumoniae (86.7 per cent). There is no evidence to support the use of antibiotic prophylaxis in patients with a cerebrospinal <span class="hlt">fluid</span> leak. We propose that all such patients are advised to seek immunisation against pneumococcus, meningococcus and haemophilus.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19850009016','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19850009016"><span>Computational <span class="hlt">fluid</span> mechanics utilizing the variational principle of <span class="hlt">modeling</span> damping seals</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Abernathy, J. M.; Farmer, R.</p> <p>1985-01-01</p> <p>An analysis for <span class="hlt">modeling</span> damping seals for use in Space Shuttle main engine turbomachinery is being produced. Development of a computational <span class="hlt">fluid</span> mechanics code for turbulent, incompressible flow is required.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017PhDT.........3D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017PhDT.........3D"><span>Reduced-order <span class="hlt">modeling</span> of <span class="hlt">fluids</span> systems, with applications in unsteady aerodynamics</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Dawson, Scott T. M.</p> <p></p> <p>This thesis focuses on two major themes: <span class="hlt">modeling</span> and understanding the dynamics of rapidly pitching airfoils, and developing methods that can be used to extract <span class="hlt">models</span> and pertinent features from datasets obtained in the study of these and other systems in <span class="hlt">fluid</span> mechanics and aerodynamics. Much of the work utilizes in some capacity dynamic mode decomposition (DMD), a recently developed method to extract dynamical features and <span class="hlt">models</span> from data. The investigation of pitching airfoils includes both wind tunnel experiments and direct numerical simulations. Experiments are performed on a NACA 0012 airfoil undergoing rapid pitching motion, with the focus on developing a switched linear <span class="hlt">modeling</span> framework that can accurately predict unsteady aerodynamic forces and pressure distributions throughout arbitrary pitching motions. Numerical simulations are used to study the behavior of sinusoidally pitching airfoils. By systematically varying the amplitude, frequency, mean angle and axis of pitching, a comprehensive database of results is acquired, from which interesting regions in parameter space are identified and studied. Attention is given to pitching at "preferred" frequencies, where vortex shedding in the wake is excited or amplified, leading to larger lift forces. More generally, the ability to extract nonlinear <span class="hlt">models</span> that describe the behavior of complex <span class="hlt">fluids</span> systems can assist in not only understanding the dominant features of such systems, but also to achieve accurate prediction and control. One potential avenue to achieve this objective is through numerical approximation of the Koopman operator, an infinite-dimensional linear operator capable of describing finite-dimensional nonlinear systems, such as those that might describe the dominant dynamics of <span class="hlt">fluids</span> systems. This idea is explored by showing that algorithms designed to approximate the Koopman operator can indeed be utilized to accurately <span class="hlt">model</span> nonlinear <span class="hlt">fluids</span> systems, even when the data available is</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AIPC.1542.1055D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AIPC.1542.1055D"><span>Dust emission <span class="hlt">modelling</span> around a stockpile by using computational <span class="hlt">fluid</span> dynamics and discrete element method</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Derakhshani, S. M.; Schott, D. L.; Lodewijks, G.</p> <p>2013-06-01</p> <p>Dust emissions can have significant effects on the human health, environment and industry equipment. Understanding the dust generation process helps to select a suitable dust preventing approach and also is useful to evaluate the environmental impact of dust emission. To describe these processes, numerical methods such as Computational <span class="hlt">Fluid</span> Dynamics (CFD) are widely used, however nowadays particle <span class="hlt">based</span> methods like Discrete Element Method (DEM) allow researchers to <span class="hlt">model</span> interaction between particles and <span class="hlt">fluid</span> flow. In this study, air flow over a stockpile, dust emission, erosion and surface deformation of granular material in the form of stockpile are studied by using DEM and CFD as a coupled method. Two and three dimensional simulations are respectively developed for CFD and DEM methods to minimize CPU time. The standard κ-ɛ turbulence <span class="hlt">model</span> is used in a fully developed turbulent flow. The continuous gas phase and the discrete particle phase link to each other through gas-particle void fractions and momentum transfer. In addition to stockpile deformation, dust dispersion is studied and finally the accuracy of stockpile deformation results obtained by CFD-DEM <span class="hlt">modelling</span> will be validated by the agreement with the existing experimental data.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016JGeo..101....1L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016JGeo..101....1L"><span><span class="hlt">Fluids</span> in crustal deformation: <span class="hlt">Fluid</span> flow, <span class="hlt">fluid</span>-rock interactions, rheology, melting and resources</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lacombe, Olivier; Rolland, Yann</p> <p>2016-11-01</p> <p><span class="hlt">Fluids</span> exert a first-order control on the structural, petrological and rheological evolution of the continental crust. <span class="hlt">Fluids</span> interact with rocks from the earliest stages of sedimentation and diagenesis in basins until these rocks are deformed and/or buried and metamorphosed in orogens, then possibly exhumed. <span class="hlt">Fluid</span>-rock interactions lead to the evolution of rock physical properties and rock strength. Fractures and faults are preferred pathways for <span class="hlt">fluids</span>, and in turn physical and chemical interactions between <span class="hlt">fluid</span> flow and tectonic structures, such as fault zones, strongly influence the mechanical behaviour of the crust at different space and time scales. <span class="hlt">Fluid</span> (over)pressure is associated with a variety of geological phenomena, such as seismic cycle in various P-T conditions, hydrofracturing (including formation of sub-horizontal, bedding-parallel veins), fault (re)activation or gravitational sliding of rocks, among others. <span class="hlt">Fluid</span> (over)pressure is a governing factor for the evolution of permeability and porosity of rocks and controls the generation, maturation and migration of economic <span class="hlt">fluids</span> like hydrocarbons or ore forming hydrothermal <span class="hlt">fluids</span>, and is therefore a key parameter in reservoir studies and basin <span class="hlt">modeling</span>. <span class="hlt">Fluids</span> may also help the crust partially melt, and in turn the resulting melt may dramatically change the rheology of the crust.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMNG52A..03Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMNG52A..03Z"><span>Non-Newtonian <span class="hlt">fluid</span> flow in 2D fracture networks</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zou, L.; Håkansson, U.; Cvetkovic, V.</p> <p>2017-12-01</p> <p><span class="hlt">Modeling</span> of non-Newtonian <span class="hlt">fluid</span> (e.g., drilling <span class="hlt">fluids</span> and cement grouts) flow in fractured rocks is of interest in many geophysical and industrial practices, such as drilling operations, enhanced oil recovery and rock grouting. In fractured rock masses, the flow paths are dominated by fractures, which are often represented as discrete fracture networks (DFN). In the literature, many studies have been devoted to Newtonian <span class="hlt">fluid</span> (e.g., groundwater) flow in fractured rock using the DFN concept, but few works are dedicated to non-Newtonian <span class="hlt">fluids</span>.In this study, a generalized flow equation for common non-Newtonian <span class="hlt">fluids</span> (such as Bingham, power-law and Herschel-Bulkley) in a single fracture is obtained from the analytical solutions for non-Newtonian <span class="hlt">fluid</span> discharge between smooth parallel plates. Using Monte Carlo sampling <span class="hlt">based</span> on site characterization data for the distribution of geometrical features (e.g., density, length, aperture and orientations) in crystalline fractured rock, a two dimensional (2D) DFN <span class="hlt">model</span> is constructed for generic flow simulations. Due to complex properties of non-Newtonian <span class="hlt">fluids</span>, the relationship between <span class="hlt">fluid</span> discharge and the pressure gradient is nonlinear. A Galerkin finite element method solver is developed to iteratively solve the obtained nonlinear governing equations for the 2D DFN <span class="hlt">model</span>. Using DFN realizations, simulation results for different geometrical distributions of the fracture network and different non-Newtonian <span class="hlt">fluid</span> properties are presented to illustrate the spatial discharge distributions. The impact of geometrical structures and the <span class="hlt">fluid</span> properties on the non-Newtonian <span class="hlt">fluid</span> flow in 2D DFN is examined statistically. The results generally show that <span class="hlt">modeling</span> non-Newtonian <span class="hlt">fluid</span> flow in fractured rock as a DFN is feasible, and that the discharge distribution may be significantly affected by the geometrical structures as well as by the <span class="hlt">fluid</span> constitutive properties.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012APS..DFDH33005P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012APS..DFDH33005P"><span>A universal constraint-<span class="hlt">based</span> formulation for freely moving immersed bodies in <span class="hlt">fluids</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Patankar, Neelesh A.</p> <p>2012-11-01</p> <p>Numerical simulation of moving immersed bodies in <span class="hlt">fluids</span> is now practiced routinely. A variety of variants of these approaches have been published, most of which rely on using a background mesh for the <span class="hlt">fluid</span> equations and tracking the body using Lagrangian points. In this talk, generalized constraint-<span class="hlt">based</span> governing equations will be presented that provide a unified framework for various immersed body techniques. The key idea that is common to these methods is to assume that the entire <span class="hlt">fluid</span>-body domain is a ``<span class="hlt">fluid</span>'' and then to constrain the body domain to move in accordance with its governing equations. The immersed body can be rigid or deforming. The governing equations are developed so that they are independent of the nature of temporal or spatial discretization schemes. Specific choices of time stepping and spatial discretization then lead to techniques developed in prior literature ranging from freely moving rigid to elastic self-propelling bodies. To simulate Brownian systems, thermal fluctuations can be included in the <span class="hlt">fluid</span> equations via additional random stress terms. Solving the fluctuating hydrodynamic equations coupled with the immersed body results in the Brownian motion of that body. The constraint-<span class="hlt">based</span> formulation leads to fractional time stepping algorithms a la Chorin-type schemes that are suitable for fast computations of rigid or self-propelling bodies whose deformation kinematics are known. Support from NSF is gratefully acknowledged.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20110002866','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20110002866"><span>CFD Fuel Slosh <span class="hlt">Modeling</span> of <span class="hlt">Fluid</span>-Structure Interaction in Spacecraft Propellant Tanks with Diaphragms</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Sances, Dillon J.; Gangadharan, Sathya N.; Sudermann, James E.; Marsell, Brandon</p> <p>2010-01-01</p> <p>Liquid sloshing within spacecraft propellant tanks causes rapid energy dissipation at resonant modes, which can result in attitude destabilization of the vehicle. Identifying resonant slosh modes currently requires experimental testing and mechanical pendulum analogs to characterize the slosh dynamics. Computational <span class="hlt">Fluid</span> Dynamics (CFD) techniques have recently been validated as an effective tool for simulating fuel slosh within free-surface propellant tanks. Propellant tanks often incorporate an internal flexible diaphragm to separate ullage and propellant which increases <span class="hlt">modeling</span> complexity. A coupled <span class="hlt">fluid</span>-structure CFD <span class="hlt">model</span> is required to capture the damping effects of a flexible diaphragm on the propellant. ANSYS multidisciplinary engineering software employs a coupled solver for analyzing two-way <span class="hlt">Fluid</span> Structure Interaction (FSI) cases such as the diaphragm propellant tank system. Slosh <span class="hlt">models</span> generated by ANSYS software are validated by experimental lateral slosh test results. Accurate data correlation would produce an innovative technique for <span class="hlt">modeling</span> fuel slosh within diaphragm tanks and provide an accurate and efficient tool for identifying resonant modes and the slosh dynamic response.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014IJMPD..2350023L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014IJMPD..2350023L"><span><span class="hlt">Modeling</span> Dark Energy Through AN Ising <span class="hlt">Fluid</span> with Network Interactions</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Luongo, Orlando; Tommasini, Damiano</p> <p>2014-12-01</p> <p>We show that the dark energy (DE) effects can be <span class="hlt">modeled</span> by using an Ising perfect <span class="hlt">fluid</span> with network interactions, whose low redshift equation of state (EoS), i.e. ω0, becomes ω0 = -1 as in the ΛCDM <span class="hlt">model</span>. In our picture, DE is characterized by a barotropic <span class="hlt">fluid</span> on a lattice in the equilibrium configuration. Thus, mimicking the spin interaction by replacing the spin variable with an occupational number, the pressure naturally becomes negative. We find that the corresponding EoS mimics the effects of a variable DE term, whose limiting case reduces to the cosmological constant Λ. This permits us to avoid the introduction of a vacuum energy as DE source by hand, alleviating the coincidence and fine tuning problems. We find fairly good cosmological constraints, by performing three tests with supernovae Ia (SNeIa), baryonic acoustic oscillation (BAO) and cosmic microwave background (CMB) measurements. Finally, we perform the Akaike information criterion (AIC) and Bayesian information criterion (BIC) selection criteria, showing that our <span class="hlt">model</span> is statistically favored with respect to the Chevallier-Polarsky-Linder (CPL) parametrization.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JMFM...19..423W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JMFM...19..423W"><span>Global Regularity for Several Incompressible <span class="hlt">Fluid</span> <span class="hlt">Models</span> with Partial Dissipation</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wu, Jiahong; Xu, Xiaojing; Ye, Zhuan</p> <p>2017-09-01</p> <p>This paper examines the global regularity problem on several 2D incompressible <span class="hlt">fluid</span> <span class="hlt">models</span> with partial dissipation. They are the surface quasi-geostrophic (SQG) equation, the 2D Euler equation and the 2D Boussinesq equations. These are well-known <span class="hlt">models</span> in <span class="hlt">fluid</span> mechanics and geophysics. The fundamental issue of whether or not they are globally well-posed has attracted enormous attention. The corresponding <span class="hlt">models</span> with partial dissipation may arise in physical circumstances when the dissipation varies in different directions. We show that the SQG equation with either horizontal or vertical dissipation always has global solutions. This is in sharp contrast with the inviscid SQG equation for which the global regularity problem remains outstandingly open. Although the 2D Euler is globally well-posed for sufficiently smooth data, the associated equations with partial dissipation no longer conserve the vorticity and the global regularity is not trivial. We are able to prove the global regularity for two partially dissipated Euler equations. Several global bounds are also obtained for a partially dissipated Boussinesq system.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=2770434','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=2770434"><span>A Diffusion Tensor Imaging Tractography Algorithm <span class="hlt">Based</span> on Navier-Stokes <span class="hlt">Fluid</span> Mechanics</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Hageman, Nathan S.; Toga, Arthur W.; Narr, Katherine; Shattuck, David W.</p> <p>2009-01-01</p> <p>We introduce a <span class="hlt">fluid</span> mechanics <span class="hlt">based</span> tractography method for estimating the most likely connection paths between points in diffusion tensor imaging (DTI) volumes. We customize the Navier-Stokes equations to include information from the diffusion tensor and simulate an artificial <span class="hlt">fluid</span> flow through the DTI image volume. We then estimate the most likely connection paths between points in the DTI volume using a metric derived from the <span class="hlt">fluid</span> velocity vector field. We validate our algorithm using digital DTI phantoms <span class="hlt">based</span> on a helical shape. Our method segmented the structure of the phantom with less distortion than was produced using implementations of heat-<span class="hlt">based</span> partial differential equation (PDE) and streamline <span class="hlt">based</span> methods. In addition, our method was able to successfully segment divergent and crossing fiber geometries, closely following the ideal path through a digital helical phantom in the presence of multiple crossing tracts. To assess the performance of our algorithm on anatomical data, we applied our method to DTI volumes from normal human subjects. Our method produced paths that were consistent with both known anatomy and directionally encoded color (DEC) images of the DTI dataset. PMID:19244007</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JPhCS.795a2056Y','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JPhCS.795a2056Y"><span>A <span class="hlt">model</span> of scientific attitudes assessment by observation in physics learning <span class="hlt">based</span> scientific approach: case study of dynamic <span class="hlt">fluid</span> topic in high school</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Yusliana Ekawati, Elvin</p> <p>2017-01-01</p> <p>This study aimed to produce a <span class="hlt">model</span> of scientific attitude assessment in terms of the observations for physics learning <span class="hlt">based</span> scientific approach (case study of dynamic <span class="hlt">fluid</span> topic in high school). Development of instruments in this study adaptation of the Plomp <span class="hlt">model</span>, the procedure includes the initial investigation, design, construction, testing, evaluation and revision. The test is done in Surakarta, so that the data obtained are analyzed using Aiken formula to determine the validity of the content of the instrument, Cronbach’s alpha to determine the reliability of the instrument, and construct validity using confirmatory factor analysis with LISREL 8.50 program. The results of this research were conceptual <span class="hlt">models</span>, instruments and guidelines on scientific attitudes assessment by observation. The construct assessment instruments include components of curiosity, objectivity, suspended judgment, open-mindedness, honesty and perseverance. The construct validity of instruments has been qualified (rated load factor > 0.3). The reliability of the <span class="hlt">model</span> is quite good with the Alpha value 0.899 (> 0.7). The test showed that the <span class="hlt">model</span> fits the theoretical <span class="hlt">models</span> are supported by empirical data, namely p-value 0.315 (≥ 0.05), RMSEA 0.027 (≤ 0.08)</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013PhDT.......133L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013PhDT.......133L"><span>Numerical <span class="hlt">Modeling</span> of Poroelastic-<span class="hlt">Fluid</span> Systems Using High-Resolution Finite Volume Methods</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lemoine, Grady</p> <p></p> <p>Poroelasticity theory <span class="hlt">models</span> the mechanics of porous, <span class="hlt">fluid</span>-saturated, deformable solids. It was originally developed by Maurice Biot to <span class="hlt">model</span> geophysical problems, such as seismic waves in oil reservoirs, but has also been applied to <span class="hlt">modeling</span> living bone and other porous media. Poroelastic media often interact with <span class="hlt">fluids</span>, such as in ocean bottom acoustics or propagation of waves from soft tissue into bone. This thesis describes the development and testing of high-resolution finite volume numerical methods, and simulation codes implementing these methods, for <span class="hlt">modeling</span> systems of poroelastic media and <span class="hlt">fluids</span> in two and three dimensions. These methods operate on both rectilinear grids and logically rectangular mapped grids. To allow the use of these methods, Biot's equations of poroelasticity are formulated as a first-order hyperbolic system with a source term; this source term is incorporated using operator splitting. Some modifications are required to the classical high-resolution finite volume method. Obtaining correct solutions at interfaces between poroelastic media and <span class="hlt">fluids</span> requires a novel transverse propagation scheme and the removal of the classical second-order correction term at the interface, and in three dimensions a new wave limiting algorithm is also needed to correctly limit shear waves. The accuracy and convergence rates of the methods of this thesis are examined for a variety of analytical solutions, including simple plane waves, reflection and transmission of waves at an interface between different media, and scattering of acoustic waves by a poroelastic cylinder. Solutions are also computed for a variety of test problems from the computational poroelasticity literature, as well as some original test problems designed to mimic possible applications for the simulation code.</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://adsabs.harvard.edu/abs/2014PhDT.......153G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014PhDT.......153G"><span>Physics-<span class="hlt">based</span> animation of large-scale splashing liquids, elastoplastic solids, and <span class="hlt">model</span>-reduced flow</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Gerszewski, Daniel James</p> <p></p> <p>Physical simulation has become an essential tool in computer animation. As the use of visual effects increases, the need for simulating real-world materials increases. In this dissertation, we consider three problems in physics-<span class="hlt">based</span> animation: large-scale splashing liquids, elastoplastic material simulation, and dimensionality reduction techniques for <span class="hlt">fluid</span> simulation. <span class="hlt">Fluid</span> simulation has been one of the greatest successes of physics-<span class="hlt">based</span> animation, generating hundreds of research papers and a great many special effects over the last fifteen years. However, the animation of large-scale, splashing liquids remains challenging. We show that a novel combination of unilateral incompressibility, mass-full FLIP, and blurred boundaries is extremely well-suited to the animation of large-scale, violent, splashing liquids. Materials that incorporate both plastic and elastic deformations, also referred to as elastioplastic materials, are frequently encountered in everyday life. Methods for animating such common real-world materials are useful for effects practitioners and have been successfully employed in films. We describe a point-<span class="hlt">based</span> method for animating elastoplastic materials. Our primary contribution is a simple method for computing the deformation gradient for each particle in the simulation. Given the deformation gradient, we can apply arbitrary constitutive <span class="hlt">models</span> and compute the resulting elastic forces. Our method has two primary advantages: we do not store or compare to an initial rest configuration and we work directly with the deformation gradient. The first advantage avoids poor numerical conditioning and the second naturally leads to a multiplicative <span class="hlt">model</span> of deformation appropriate for finite deformations. One of the most significant drawbacks of physics-<span class="hlt">based</span> animation is that ever-higher fidelity leads to an explosion in the number of degrees of freedom. This problem leads us to the consideration of dimensionality reduction techniques. We present</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1253368','DOE-PATENT-XML'); return false;" href="https://www.osti.gov/servlets/purl/1253368"><span>Heat transfer <span class="hlt">fluids</span> containing nanoparticles</span></a></p> <p><a target="_blank" href="http://www.osti.gov/doepatents">DOEpatents</a></p> <p>Singh, Dileep; Routbort, Jules; Routbort, A.J.; Yu, Wenhua; Timofeeva, Elena; Smith, David S.; France, David M.</p> <p>2016-05-17</p> <p>A nanofluid of a <span class="hlt">base</span> heat transfer <span class="hlt">fluid</span> and a plurality of ceramic nanoparticles suspended throughout the <span class="hlt">base</span> heat transfer <span class="hlt">fluid</span> applicable to commercial and industrial heat transfer applications. The nanofluid is stable, non-reactive and exhibits enhanced heat transfer properties relative to the <span class="hlt">base</span> heat transfer <span class="hlt">fluid</span>, with only minimal increases in pumping power required relative to the <span class="hlt">base</span> heat transfer <span class="hlt">fluid</span>. In a particular embodiment, the plurality of ceramic nanoparticles comprise silicon carbide and the <span class="hlt">base</span> heat transfer <span class="hlt">fluid</span> comprises water and water and ethylene glycol mixtures.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/10047589','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/10047589"><span>Analysis of organophosphate hydraulic <span class="hlt">fluids</span> in U.S. Air force <span class="hlt">base</span> soils</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>David; Seiber</p> <p>1999-04-01</p> <p>Tri-aryl and tri-alkyl organophosphates (TAPs) have been used extensively as flame-retardant hydraulic <span class="hlt">fluids</span> and <span class="hlt">fluid</span> additives in commercial and military aircraft. Up to 80% of the consumption of these <span class="hlt">fluids</span> has been estimated to be lost to unrecovered leakage. Tri-aryl phosphate components of these <span class="hlt">fluids</span> are resistant to volatilization and solubilization in water, thus, their primary environmental fate pathway is sorption to soils. Environmental audits of military air <span class="hlt">bases</span> generally do not include quantification of these compounds in soils. We have determined the presence and extent of TAP contamination in soil samples from several U.S. Air Force <span class="hlt">bases</span>. Soils were collected, extracted, and analyzed using GC/FPD and GC/MS. Tricresyl phosphate was the most frequently found TAP in soil, ranging from 0.02 to 130 ppm. Other TAPs in soils included triphenyl phosphate and isopropylated triphenyl phosphate. Observations are made regarding the distribution, typical concentrations, persistence, and need for further testing of TAPs in soils at military installations. Additionally, GC and mass spectral data for these TAPs are presented, along with methods for their extraction, sample clean-up, and quantification.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27813272','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27813272"><span>Experiment for validation of <span class="hlt">fluid</span>-structure interaction <span class="hlt">models</span> and algorithms.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Hessenthaler, A; Gaddum, N R; Holub, O; Sinkus, R; Röhrle, O; Nordsletten, D</p> <p>2017-09-01</p> <p>In this paper a <span class="hlt">fluid</span>-structure interaction (FSI) experiment is presented. The aim of this experiment is to provide a challenging yet easy-to-setup FSI test case that addresses the need for rigorous testing of FSI algorithms and <span class="hlt">modeling</span> frameworks. Steady-state and periodic steady-state test cases with constant and periodic inflow were established. Focus of the experiment is on biomedical engineering applications with flow being in the laminar regime with Reynolds numbers 1283 and 651. Flow and solid domains were defined using computer-aided design (CAD) tools. The experimental design aimed at providing a straightforward boundary condition definition. Material parameters and mechanical response of a moderately viscous Newtonian <span class="hlt">fluid</span> and a nonlinear incompressible solid were experimentally determined. A comprehensive data set was acquired by using magnetic resonance imaging to record the interaction between the <span class="hlt">fluid</span> and the solid, quantifying flow and solid motion. Copyright © 2016 The Authors. International Journal for Numerical Methods in Biomedical Engineering published by John Wiley & Sons Ltd.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/5923429','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/5923429"><span>Determining temperature limits of drilling <span class="hlt">fluids</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>Thuren, J.B.; Chenevert, M.E.; Huang, W.T.W.</p> <p></p> <p>A capillary three tube viscometer has been designed which allows the measurement of rheological properties of time dependent non-Newtonian <span class="hlt">fluids</span> in laminar flow at high temperture and pressure. The objective of this investigation is to determine the temperature stability of clay-water suspensions containing various drilling <span class="hlt">fluid</span> additives. The additives studied consisted of viscosifiers, filtrate reducers, and chemical thinners. The temperature range studied is from room temperature to 550{sup 0}F. The system pressure is consistently maintained above the vapor pressure. The Bentonite and water standardized <span class="hlt">base</span> mud used is equivalent to a 25 ppB <span class="hlt">fluid</span>. Stabilization of the <span class="hlt">base</span> mud ismore » necessary to obtain steady state laminar flow conditions and to obtain reliable temperature thinning effects with each temperature interval under investigation. Generally the temperature levels are maintained for one hour until 550{sup 0}F is attained. The last interval is then maintained until system <span class="hlt">fluid</span> degradation occurs. Rheological measurements are obtained from differential pressure transducers located in a three diameter tube test section and externally at ambient conditions from a Baroid Rotational Viscometer. The power law <span class="hlt">model</span> for non-Newtonian <span class="hlt">fluids</span> is used to correlate the data.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19770025891','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19770025891"><span><span class="hlt">Fluid</span> mechanical <span class="hlt">model</span> of the Helmholtz resonator</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Hersh, A. S.; Walker, B.</p> <p>1977-01-01</p> <p>A semi-empirical <span class="hlt">fluid</span> mechanical <span class="hlt">model</span> of the acoustic behavior of Helmholtz resonators is presented which predicts impedance as a function of the amplitude and frequency of the incident sound pressure field and resonator geometry. The <span class="hlt">model</span> assumes that the particle velocity approaches the orifice in a spherical manner. The incident and cavity sound fields are connected by solving the governing oscillating mass and momentum conservation equations. The <span class="hlt">model</span> is in agreement with the Rayleigh slug-mass <span class="hlt">model</span> at low values of incident sound pressure level. At high values, resistance is predicted to be independent of frequency, proportional to the square root of the amplitude of the incident sound pressure field, and virtually independent of resonator geometry. Reactance is predicted to depend in a very complicated way upon resonator geometry, incident sound pressure level, and frequency. Nondimensional parameters are defined that divide resonator impedance into three categories corresponding to low, moderately low, and intense incident sound pressure amplitudes. The two-microphone method was used to measure the impedance of a variety of resonators. The data were used to refine and verify the <span class="hlt">model</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22598801-magnetic-field-sensor-based-cascaded-microfiber-coupler-magnetic-fluid','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22598801-magnetic-field-sensor-based-cascaded-microfiber-coupler-magnetic-fluid"><span>Magnetic field sensor <span class="hlt">based</span> on cascaded microfiber coupler with magnetic <span class="hlt">fluid</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>Mao, Lianmin; Su, Delong; Wang, Zhaofang</p> <p></p> <p>A kind of magnetic field sensor <span class="hlt">based</span> on cascaded microfiber coupler with magnetic <span class="hlt">fluid</span> is proposed and experimentally demonstrated. The magnetic <span class="hlt">fluid</span> is utilized as the cladding of the fused regions of the cascaded microfiber coupler. As the interference valley wavelength of the sensing structure is sensitive to the ambient variation, considering the magnetic-field-dependent refractive index of magnetic <span class="hlt">fluid</span>, the proposed structure is employed for magnetic field sensing. The effective coupling length for each coupling region of the as-fabricated cascaded microfiber coupler is 6031 μm. The achieved sensitivity is 125 pm/Oe, which is about three times larger than that of the previouslymore » similar structure <span class="hlt">based</span> on the single microfiber coupler. Experimental results indicate that the sensing sensitivity can be easily improved by increasing the effective coupling length or cascading more microfiber couplers. The proposed magnetic field sensor is attractive due to its low cost, immunity to electromagnetic interference, as well as high sensitivity, which also has the potentials in other tunable all-fiber photonic devices, such as filter.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19910009677','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19910009677"><span>A gravitational test of wave reinforcement versus <span class="hlt">fluid</span> density <span class="hlt">models</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Johnson, Jacqueline Umstead</p> <p>1990-01-01</p> <p>Spermatozoa, protozoa, and algae form macroscopic patterns somewhat analogous to thermally driven convection cells. These bioconvective patterns have attracted interest in the <span class="hlt">fluid</span> dynamics community, but whether in all cases these waves were gravity driven was unknown. There are two conflicting theories, one gravity dependent (<span class="hlt">fluid</span> density <span class="hlt">model</span>), the other gravity independent (wave reinforcement theory). The primary objectives of the summer faculty fellows were to: (1) assist in sample collection (spermatozoa) and preparation for the KC-135 research airplane experiment; and (2) to collaborate on ground testing of bioconvective variables such as motility, concentration, morphology, etc., in relation to their macroscopic patterns. Results are very briefly given.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018ResPh...8..869M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018ResPh...8..869M"><span>Scrutinization of thermal radiation, viscous dissipation and Joule heating effects on Marangoni convective two-phase flow of Casson <span class="hlt">fluid</span> with <span class="hlt">fluid</span>-particle suspension</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Mahanthesh, B.; Gireesha, B. J.</p> <p>2018-03-01</p> <p>The impact of Marangoni convection on dusty Casson <span class="hlt">fluid</span> boundary layer flow with Joule heating and viscous dissipation aspects is addressed. The surface tension is assumed to vary linearly with temperature. Physical aspects of magnetohydrodynamics and thermal radiation are also accounted. The governing problem is <span class="hlt">modelled</span> under boundary layer approximations for <span class="hlt">fluid</span> phase and dust particle phase and then Runge-Kutta-Fehlberg method <span class="hlt">based</span> numeric solutions are established. The momentum and heat transport mechanisms are focused on the result of distinct governing parameters. The Nusselt number is also calculated. It is established that the rate of heat transfer can be enhanced by suspending dust particles in the <span class="hlt">base</span> <span class="hlt">fluid</span>. The temperature field of <span class="hlt">fluid</span> phase and temperature of dust phase are quite reverse for thermal dust parameter. The radiative heat, viscous dissipation and Joule heating aspects are constructive for thermal fields of <span class="hlt">fluid</span> and dust phases. The velocity of dusty Casson <span class="hlt">fluid</span> dominates the velocity of dusty <span class="hlt">fluid</span> while this trend is opposite in the case of temperature. Moreover qualitative behaviour of <span class="hlt">fluid</span> phase and dust phase temperature/velocity are similar.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22490156-hamiltonian-fluid-closures-vlasov-ampere-equations-from-water-bags-moment-models','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22490156-hamiltonian-fluid-closures-vlasov-ampere-equations-from-water-bags-moment-models"><span>Hamiltonian <span class="hlt">fluid</span> closures of the Vlasov-Ampère equations: From water-bags to N moment <span class="hlt">models</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>Perin, M.; Chandre, C.; Tassi, E.</p> <p>2015-09-15</p> <p>Moment closures of the Vlasov-Ampère system, whereby higher moments are represented as functions of lower moments with the constraint that the resulting <span class="hlt">fluid</span> system remains Hamiltonian, are investigated by using water-bag theory. The link between the water-bag formalism and <span class="hlt">fluid</span> <span class="hlt">models</span> that involve density, <span class="hlt">fluid</span> velocity, pressure and higher moments is established by introducing suitable thermodynamic variables. The cases of one, two, and three water-bags are treated and their Hamiltonian structures are provided. In each case, we give the associated <span class="hlt">fluid</span> closures and we discuss their Casimir invariants. We show how the method can be extended to an arbitrary numbermore » of fields, i.e., an arbitrary number of water-bags and associated moments. The thermodynamic interpretation of the resulting <span class="hlt">models</span> is discussed. Finally, a general procedure to derive Hamiltonian N-field <span class="hlt">fluid</span> <span class="hlt">models</span> is proposed.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19850017811','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19850017811"><span>Description, validation, and modification of the Guyton <span class="hlt">model</span> for space-flight applications. Part A. Guyton <span class="hlt">model</span> of circulatory, <span class="hlt">fluid</span> and electrolyte control. Part B. Modification of the Guyton <span class="hlt">model</span> for circulatory, <span class="hlt">fluid</span> and electrolyte control</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Leonard, J. I.</p> <p>1985-01-01</p> <p>The mathematical <span class="hlt">model</span> that has been a cornerstone for the systems analysis of space-flight physiological studies is the Guyton <span class="hlt">model</span> describing circulatory, <span class="hlt">fluid</span> and electrolyte regulation. The <span class="hlt">model</span> and the modifications that are made to permit simulation and analysis of the stress of weightlessness are described.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/10484445','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/10484445"><span>Transport of <span class="hlt">fluid</span> and solutes in the body II. <span class="hlt">Model</span> validation and implications.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Gyenge, C C; Bowen, B D; Reed, R K; Bert, J L</p> <p>1999-09-01</p> <p>A mathematical <span class="hlt">model</span> of short-term whole body <span class="hlt">fluid</span>, protein, and ion distribution and transport developed earlier [see companion paper: C. C. Gyenge, B. D. Bowen, R. K. Reed, and J. L. Bert. Am. J. Physiol. 277 (Heart Circ. Physiol. 46): H1215-H1227, 1999] is validated using experimental data available in the literature. The <span class="hlt">model</span> was tested against data measured for the following three types of experimental infusions: 1) hyperosmolar saline solutions with an osmolarity in the range of 2,000-2,400 mosmol/l, 2) saline solutions with an osmolarity of approximately 270 mosmol/l and composition comparable with Ringer solution, and 3) an isosmotic NaCl solution with an osmolarity of approximately 300 mosmol/l. Good agreement between the <span class="hlt">model</span> predictions and the experimental data was obtained with respect to the trends and magnitudes of <span class="hlt">fluid</span> shifts between the intra- and extracellular compartments, extracellular ion and protein contents, and hematocrit values. The <span class="hlt">model</span> is also able to yield information about inaccessible or difficult-to-measure system variables such as intracellular ion contents, cellular volumes, and <span class="hlt">fluid</span> fluxes across the vascular capillary membrane, data that can be used to help interpret the behavior of the system.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2007PhDT........24J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2007PhDT........24J"><span>Development of a magneto-rheological <span class="hlt">fluid</span> <span class="hlt">based</span> hybrid actuation system</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>John, Shaju</p> <p></p> <p>A hybrid hydraulic actuation system is proposed as an active pitch link for rotorcraft applications. Such an active pitch link can be used to implement Individual Blade Control (IBC) techniques for vibration and noise reduction, in addition to providing primary control for the helicopter. Conventional technologies like electric motors and hydraulic actuators have major disadvantages when it come to applications on a rotating environment. Centralized hydraulic system require the use of mechanically complex hydraulic slip rings and electric motors have high precision mechanical moving parts that make them unattractive in application with high centrifugal load. The high energy density of smart materials can be used to design hydraulic actuators in a compact package. MagnetoRheological (MR) <span class="hlt">fluids</span> can be used as the working <span class="hlt">fluid</span> in such a hybrid hydraulic actuation system to implement a valving system with no moving parts. Thus, such an actuation system can be theoretically well-suited for application in a rotating environment. To develop an actuation system <span class="hlt">based</span> on an active material stack and MR fluidic valves, a fundamental understanding of the hydraulic circuit is essential. In order to address this issue, a theoretical <span class="hlt">model</span> was developed to understand the effect of pumping chamber geometry on the pressure losses in the pumping chamber. Three dimensional analytical <span class="hlt">models</span> were developed for steady and unsteady flow and the results were correlated to results obtained from Computation <span class="hlt">Fluid</span> Dynamic simulation of <span class="hlt">fluid</span> flow inside the pumping chamber. Fundamental understanding regarding the pressure losses in a pumping chamber are obtained from the <span class="hlt">modeling</span> process. Vortices that form in the pumping chamber (during intake) and the discharge tube (during discharge) are identified as a major cause of pressure loss in the chamber. The role of vortices during dynamic operation is also captured through a frequency domain <span class="hlt">model</span>. Extensive experimental studies were</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/15548880','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/15548880"><span>Electrowetting (EW)-<span class="hlt">based</span> valve combined with hydrophilic teflon microfluidic guidance in controlling continuous <span class="hlt">fluid</span> flow.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Cheng, Ji-Yen; Hsiung, Lo-Chang</p> <p>2004-12-01</p> <p>Electrowetting (EW)-<span class="hlt">based</span> techniques have been widely used in manipulating discrete liquid. However, few articles discussed the controlling of continuous <span class="hlt">fluid</span> flow by using EW-<span class="hlt">based</span> techniques. In this paper, an EW-<span class="hlt">based</span> valve combined with plasma-modified Teflon surface, which serves as a microfluidic guidance, in controlling continuous <span class="hlt">fluid</span> flow has been demonstrated. The plasma-modified Teflon surface is firstly demonstrated for confining continuous <span class="hlt">fluid</span> flow. The EW-<span class="hlt">based</span> microfluidic device possesses the functions of a valve and a microchannel without complex moving parts and grooved microchannels. The quantitative characteristics of the EW-<span class="hlt">based</span> valve are also studied. Propylene carbonate (PC) is firstly demonstrated as the working liquid in the EW-<span class="hlt">based</span> device because of its applications in parallel oligonucleotide synthesis. It is found that lower valve actuation voltage reduces the deterioration of the valve and improves the valve stability.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018FlDyR..50b5508R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018FlDyR..50b5508R"><span>New developments in isotropic turbulent <span class="hlt">models</span> for FENE-P <span class="hlt">fluids</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Resende, P. R.; Cavadas, A. S.</p> <p>2018-04-01</p> <p>The evolution of viscoelastic turbulent <span class="hlt">models</span>, in the last years, has been significant due to the direct numeric simulation (DNS) advances, which allowed us to capture in detail the evolution of the viscoelastic effects and the development of viscoelastic closures. New viscoelastic closures are proposed for viscoelastic <span class="hlt">fluids</span> described by the finitely extensible nonlinear elastic-Peterlin constitutive <span class="hlt">model</span>. One of the viscoelastic closure developed in the context of isotropic turbulent <span class="hlt">models</span>, consists in a modification of the turbulent viscosity to include an elastic effect, capable of predicting, with good accuracy, the behaviour for different drag reductions. Another viscoelastic closure essential to predict drag reduction relates the viscoelastic term involving velocity and the tensor conformation fluctuations. The DNS data show the high impact of this term to predict correctly the drag reduction, and for this reason is proposed a simpler closure capable of predicting the viscoelastic behaviour with good performance. In addition, a new relation is developed to predict the drag reduction, quantity <span class="hlt">based</span> on the trace of the tensor conformation at the wall, eliminating the need of the typically parameters of Weissenberg and Reynolds numbers, which depend on the friction velocity. This allows future developments for complex geometries.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017PhyA..483...36K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017PhyA..483...36K"><span>An agent-<span class="hlt">based</span> method for simulating porous <span class="hlt">fluid</span>-saturated structures with indistinguishable components</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kashani, Jamal; Pettet, Graeme John; Gu, YuanTong; Zhang, Lihai; Oloyede, Adekunle</p> <p>2017-10-01</p> <p>Single-phase porous materials contain multiple components that intermingle up to the ultramicroscopic level. Although the structures of the porous materials have been simulated with agent-<span class="hlt">based</span> methods, the results of the available methods continue to provide patterns of distinguishable solid and <span class="hlt">fluid</span> agents which do not represent materials with indistinguishable phases. This paper introduces a new agent (hybrid agent) and category of rules (intra-agent rule) that can be used to create emergent structures that would more accurately represent single-phase structures and materials. The novel hybrid agent carries the characteristics of system's elements and it is capable of changing within itself, while also responding to its neighbours as they also change. As an example, the hybrid agent under one-dimensional cellular automata formalism in a two-dimensional domain is used to generate patterns that demonstrate the striking morphological and characteristic similarities with the porous saturated single-phase structures where each agent of the ;structure; carries semi-permeability property and consists of both <span class="hlt">fluid</span> and solid in space and at all times. We conclude that the ability of the hybrid agent to change locally provides an enhanced protocol to simulate complex porous structures such as biological tissues which could facilitate <span class="hlt">models</span> for agent-<span class="hlt">based</span> techniques and numerical methods.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016RMRE...49.2845W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016RMRE...49.2845W"><span>An Analytical <span class="hlt">Model</span> for Assessing Stability of Pre-Existing Faults in Caprock Caused by <span class="hlt">Fluid</span> Injection and Extraction in a Reservoir</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wang, Lei; Bai, Bing; Li, Xiaochun; Liu, Mingze; Wu, Haiqing; Hu, Shaobin</p> <p>2016-07-01</p> <p>Induced seismicity and fault reactivation associated with <span class="hlt">fluid</span> injection and depletion were reported in hydrocarbon, geothermal, and waste <span class="hlt">fluid</span> injection fields worldwide. Here, we establish an analytical <span class="hlt">model</span> to assess fault reactivation surrounding a reservoir during <span class="hlt">fluid</span> injection and extraction that considers the stress concentrations at the fault tips and the effects of fault length. In this <span class="hlt">model</span>, induced stress analysis in a full-space under the plane strain condition is implemented <span class="hlt">based</span> on Eshelby's theory of inclusions in terms of a homogeneous, isotropic, and poroelastic medium. The stress intensity factor concept in linear elastic fracture mechanics is adopted as an instability criterion for pre-existing faults in surrounding rocks. To characterize the fault reactivation caused by <span class="hlt">fluid</span> injection and extraction, we define a new index, the "fault reactivation factor" η, which can be interpreted as an index of fault stability in response to <span class="hlt">fluid</span> pressure changes per unit within a reservoir resulting from injection or extraction. The critical <span class="hlt">fluid</span> pressure change within a reservoir is also determined by the superposition principle using the in situ stress surrounding a fault. Our parameter sensitivity analyses show that the fault reactivation tendency is strongly sensitive to fault location, fault length, fault dip angle, and Poisson's ratio of the surrounding rock. Our case study demonstrates that the proposed <span class="hlt">model</span> focuses on the mechanical behavior of the whole fault, unlike the conventional methodologies. The proposed method can be applied to engineering cases related to injection and depletion within a reservoir owing to its efficient computational codes implementation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012AIPC.1503...89A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012AIPC.1503...89A"><span>A Lattice-Boltzmann <span class="hlt">model</span> to simulate diffractive nonlinear ultrasound beam propagation in a dissipative <span class="hlt">fluid</span> medium</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Abdi, Mohamad; Hajihasani, Mojtaba; Gharibzadeh, Shahriar; Tavakkoli, Jahan</p> <p>2012-12-01</p> <p>Ultrasound waves have been widely used in diagnostic and therapeutic medical applications. Accurate and effective simulation of ultrasound beam propagation and its interaction with tissue has been proved to be important. The nonlinear nature of the ultrasound beam propagation, especially in the therapeutic regime, plays an important role in the mechanisms of interaction with tissue. There are three main approaches in current computational <span class="hlt">fluid</span> dynamics (CFD) methods to <span class="hlt">model</span> and simulate nonlinear ultrasound beams: macroscopic, mesoscopic and microscopic approaches. In this work, a mesoscopic CFD method <span class="hlt">based</span> on the Lattice-Boltzmann <span class="hlt">model</span> (LBM) was investigated. In the developed method, the Boltzmann equation is evolved to simulate the flow of a Newtonian <span class="hlt">fluid</span> with the collision <span class="hlt">model</span> instead of solving the Navier-Stokes, continuity and state equations which are used in conventional CFD methods. The LBM has some prominent advantages over conventional CFD methods, including: (1) its parallel computational nature; (2) taking microscopic boundaries into account; and (3) capability of simulating in porous and inhomogeneous media. In our proposed method, the propagating medium is discretized with a square grid in 2 dimensions with 9 velocity vectors for each node. Using the developed <span class="hlt">model</span>, the nonlinear distortion and shock front development of a finiteamplitude diffractive ultrasonic beam in a dissipative <span class="hlt">fluid</span> medium was computed and validated against the published data. The results confirm that the LBM is an accurate and effective approach to <span class="hlt">model</span> and simulate nonlinearity in finite-amplitude ultrasound beams with Mach numbers of up to 0.01 which, among others, falls within the range of therapeutic ultrasound regime such as high intensity focused ultrasound (HIFU) beams. A comparison between the HIFU nonlinear beam simulations using the proposed <span class="hlt">model</span> and pseudospectral methods in a 2D geometry is presented.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..1919270F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..1919270F"><span>A simplified <span class="hlt">model</span> to evaluate the effect of <span class="hlt">fluid</span> rheology on non-Newtonian flow in variable aperture fractures</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Felisa, Giada; Ciriello, Valentina; Longo, Sandro; Di Federico, Vittorio</p> <p>2017-04-01</p> <p><span class="hlt">Modeling</span> of non-Newtonian flow in fractured media is essential in hydraulic fracturing operations, largely used for optimal exploitation of oil, gas and thermal reservoirs. Complex <span class="hlt">fluids</span> interact with pre-existing rock fractures also during drilling operations, enhanced oil recovery, environmental remediation, and other natural phenomena such as magma and sand intrusions, and mud volcanoes. A first step in the <span class="hlt">modeling</span> effort is a detailed understanding of flow in a single fracture, as the fracture aperture is typically spatially variable. A large bibliography exists on Newtonian flow in single, variable aperture fractures. Ultimately, stochastic <span class="hlt">modeling</span> of aperture variability at the single fracture scale leads to determination of the flowrate under a given pressure gradient as a function of the parameters describing the variability of the aperture field and the <span class="hlt">fluid</span> rheological behaviour. From the flowrate, a flow, or 'hydraulic', aperture can then be derived. The equivalent flow aperture for non-Newtonian <span class="hlt">fluids</span> of power-law nature in single, variable aperture fractures has been obtained in the past both for deterministic and stochastic variations. Detailed numerical <span class="hlt">modeling</span> of power-law <span class="hlt">fluid</span> flow in a variable aperture fracture demonstrated that pronounced channelization effects are associated to a nonlinear <span class="hlt">fluid</span> rheology. The availability of an equivalent flow aperture as a function of the parameters describing the <span class="hlt">fluid</span> rheology and the aperture variability is enticing, as it allows taking their interaction into account when <span class="hlt">modeling</span> flow in fracture networks at a larger scale. A relevant issue in non-Newtonian fracture flow is the rheological nature of the <span class="hlt">fluid</span>. The constitutive <span class="hlt">model</span> routinely used for hydro-fracturing <span class="hlt">modeling</span> is the simple, two-parameter power-law. Yet this <span class="hlt">model</span> does not characterize real <span class="hlt">fluids</span> at low and high shear rates, as it implies, for shear-thinning <span class="hlt">fluids</span>, an apparent viscosity which becomes unbounded for zero shear rate</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.H13E1432A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.H13E1432A"><span>The Impact of Solid Surface Features on <span class="hlt">Fluid-Fluid</span> Interface Configuration</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Araujo, J. B.; Brusseau, M. L. L.</p> <p>2017-12-01</p> <p>Pore-scale <span class="hlt">fluid</span> processes in geological media are critical for a broad range of applications such as radioactive waste disposal, carbon sequestration, soil moisture distribution, subsurface pollution, land stability, and oil and gas recovery. The continued improvement of high-resolution image acquisition and processing have provided a means to test the usefulness of theoretical <span class="hlt">models</span> developed to simulate pore-scale <span class="hlt">fluid</span> processes, through the direct quantification of interfaces. High-resolution synchrotron X-ray microtomography is used in combination with advanced visualization tools to characterize <span class="hlt">fluid</span> distributions in natural geologic media. The studies revealed the presence of <span class="hlt">fluid-fluid</span> interface associated with macroscopic features on the surfaces of the solids such as pits and crevices. These features and respective <span class="hlt">fluid</span> interfaces, which are not included in current theoretical or computational <span class="hlt">models</span>, may have a significant impact on accurate simulation and understanding of multi-phase flow, energy, heat and mass transfer processes.</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('http://adsabs.harvard.edu/abs/2017JChPh.147u4502X','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JChPh.147u4502X"><span>A molecular Debye-Hückel theory of solvation in polar <span class="hlt">fluids</span>: An extension of the Born <span class="hlt">model</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Xiao, Tiejun; Song, Xueyu</p> <p>2017-12-01</p> <p>A dielectric response theory of solvation beyond the conventional Born <span class="hlt">model</span> for polar <span class="hlt">fluids</span> is presented. The dielectric response of a polar <span class="hlt">fluid</span> is described by a Born response mode and a linear combination of Debye-Hückel-like response modes that capture the nonlocal response of polar <span class="hlt">fluids</span>. The Born mode is characterized by a bulk dielectric constant, while a Debye-Hückel mode is characterized by its corresponding Debye screening length. Both the bulk dielectric constant and the Debye screening lengths are determined from the bulk dielectric function of the polar <span class="hlt">fluid</span>. The linear combination coefficients of the response modes are evaluated in a self-consistent way and can be used to evaluate the electrostatic contribution to the thermodynamic properties of a polar <span class="hlt">fluid</span>. Our theory is applied to a dipolar hard sphere <span class="hlt">fluid</span> as well as interaction site <span class="hlt">models</span> of polar <span class="hlt">fluids</span> such as water, where the electrostatic contribution to their thermodynamic properties can be obtained accurately.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29221403','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29221403"><span>A molecular Debye-Hückel theory of solvation in polar <span class="hlt">fluids</span>: An extension of the Born <span class="hlt">model</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Xiao, Tiejun; Song, Xueyu</p> <p>2017-12-07</p> <p>A dielectric response theory of solvation beyond the conventional Born <span class="hlt">model</span> for polar <span class="hlt">fluids</span> is presented. The dielectric response of a polar <span class="hlt">fluid</span> is described by a Born response mode and a linear combination of Debye-Hückel-like response modes that capture the nonlocal response of polar <span class="hlt">fluids</span>. The Born mode is characterized by a bulk dielectric constant, while a Debye-Hückel mode is characterized by its corresponding Debye screening length. Both the bulk dielectric constant and the Debye screening lengths are determined from the bulk dielectric function of the polar <span class="hlt">fluid</span>. The linear combination coefficients of the response modes are evaluated in a self-consistent way and can be used to evaluate the electrostatic contribution to the thermodynamic properties of a polar <span class="hlt">fluid</span>. Our theory is applied to a dipolar hard sphere <span class="hlt">fluid</span> as well as interaction site <span class="hlt">models</span> of polar <span class="hlt">fluids</span> such as water, where the electrostatic contribution to their thermodynamic properties can be obtained accurately.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27278968','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27278968"><span>Should early amputation impact initial <span class="hlt">fluid</span> therapy algorithms in burns resuscitation? A retrospective analysis using 3D <span class="hlt">modelling</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Staruch, Robert M T; Beverly, A; Lewis, D; Wilson, Y; Martin, N</p> <p>2017-02-01</p> <p>While the epidemiology of amputations in patients with burns has been investigated previously, the effect of an amputation on burn size and its impact on <span class="hlt">fluid</span> management have not been considered in the literature. <span class="hlt">Fluid</span> resuscitation volumes are <span class="hlt">based</span> on the percentage of the total body surface area (%TBSA) burned calculated during the primary survey. There is currently no consensus as to whether the <span class="hlt">fluid</span> volumes should be recalculated after an amputation to compensate for the new body surface area. The aim of this study was to <span class="hlt">model</span> the impact of an amputation on burn size and predicted <span class="hlt">fluid</span> requirement. A retrospective search was performed of the database at the Queen Elizabeth Hospital Birmingham Regional Burns Centre to identify all patients who had required an early amputation as a result of their burn injury. The search identified 10 patients over a 3-year period. Burn injuries were then mapped using 3D <span class="hlt">modelling</span> software. BurnCase3D is a computer program that allows accurate plotting of burn injuries on a digital mannequin adjusted for height and weight. Theoretical <span class="hlt">fluid</span> requirements were then calculated using the Parkland formula for the first 24 h, and Herndon formula for the second 24 h, taking into consideration the effects of the amputation on residual burn size. This study demonstrated that amputation can have an unpredictable effect on burn size that results in a significant deviation from predicted <span class="hlt">fluid</span> resuscitation volumes. This discrepancy in <span class="hlt">fluid</span> estimation may cause iatrogenic complications due to over-resuscitation in burn-injured casualties. Combining a more accurate estimation of postamputation burn size with goal-directed <span class="hlt">fluid</span> therapy during the resuscitation phase should enable burn care teams to optimise patient outcomes. Published by the BMJ Publishing Group Limited. For permission to use (where not already granted under a licence) please go to http://www.bmj.com/company/products-services/rights-and-licensing/.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20050170452','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20050170452"><span><span class="hlt">Fluid</span> Film Bearing Code Development</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p></p> <p>1995-01-01</p> <p>The next generation of rocket engine turbopumps is being developed by industry through Government-directed contracts. These turbopumps will use <span class="hlt">fluid</span> film bearings because they eliminate the life and shaft-speed limitations of rolling-element bearings, increase turbopump design flexibility, and reduce the need for turbopump overhauls and maintenance. The design of the <span class="hlt">fluid</span> film bearings for these turbopumps, however, requires sophisticated analysis tools to <span class="hlt">model</span> the complex physical behavior characteristic of <span class="hlt">fluid</span> film bearings operating at high speeds with low viscosity <span class="hlt">fluids</span>. State-of-the-art analysis and design tools are being developed at the Texas A&M University under a grant guided by the NASA Lewis Research Center. The latest version of the code, HYDROFLEXT, is a thermohydrodynamic bulk flow analysis with <span class="hlt">fluid</span> compressibility, full inertia, and fully developed turbulence <span class="hlt">models</span>. It can predict the static and dynamic force response of rigid and flexible pad hydrodynamic bearings and of rigid and tilting pad hydrostatic bearings. The Texas A&M code is a comprehensive analysis tool, incorporating key <span class="hlt">fluid</span> phenomenon pertinent to bearings that operate at high speeds with low-viscosity <span class="hlt">fluids</span> typical of those used in rocket engine turbopumps. Specifically, the energy equation was implemented into the code to enable <span class="hlt">fluid</span> properties to vary with temperature and pressure. This is particularly important for cryogenic <span class="hlt">fluids</span> because their properties are sensitive to temperature as well as pressure. As shown in the figure, predicted bearing mass flow rates vary significantly depending on the <span class="hlt">fluid</span> <span class="hlt">model</span> used. Because cryogens are semicompressible <span class="hlt">fluids</span> and the bearing dynamic characteristics are highly sensitive to <span class="hlt">fluid</span> compressibility, <span class="hlt">fluid</span> compressibility effects are also <span class="hlt">modeled</span>. The code contains <span class="hlt">fluid</span> properties for liquid hydrogen, liquid oxygen, and liquid nitrogen as well as for water and air. Other <span class="hlt">fluids</span> can be handled by the code provided that the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016JChPh.144w4502W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016JChPh.144w4502W"><span>Corresponding-states behavior of an ionic <span class="hlt">model</span> <span class="hlt">fluid</span> with variable dispersion interactions</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Weiss, Volker C.</p> <p>2016-06-01</p> <p>Guggenheim's corresponding-states approach for simple <span class="hlt">fluids</span> leads to a remarkably universal representation of their thermophysical properties. For more complex <span class="hlt">fluids</span>, such as polar or ionic ones, deviations from this type of behavior are to be expected, thereby supplying us with valuable information about the thermodynamic consequences of the interaction details in <span class="hlt">fluids</span>. Here, the gradual transition of a simple <span class="hlt">fluid</span> to an ionic one is studied by varying the relative strength of the dispersion interactions compared to the electrostatic interactions among the charged particles. In addition to the effects on the reduced surface tension that were reported earlier [F. Leroy and V. C. Weiss, J. Chem. Phys. 134, 094703 (2011)], we address the shape of the coexistence curve and focus on properties that are related to and derived from the vapor pressure. These quantities include the enthalpy and entropy of vaporization, the boiling point, and the critical compressibility factor Zc. For all of these properties, the crossover from simple to characteristically ionic <span class="hlt">fluid</span> is seen once the dispersive attraction drops below 20%-40% of the electrostatic attraction (as measured for two particles at contact). Below this threshold, ionic <span class="hlt">fluids</span> display characteristically low values of Zc as well as large Guggenheim and Guldberg ratios for the reduced enthalpy of vaporization and the reduced boiling point, respectively. The coexistence curves are wider and more skewed than those for simple <span class="hlt">fluids</span>. The results for the ionic <span class="hlt">model</span> <span class="hlt">fluid</span> with variable dispersion interactions improve our understanding of the behavior of real ionic <span class="hlt">fluids</span>, such as inorganic molten salts and room temperature ionic liquids, by gauging the importance of different types of interactions for thermodynamic properties.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009JChPh.131w4115V','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009JChPh.131w4115V"><span><span class="hlt">Modeling</span> the nanoscale viscoelasticity of <span class="hlt">fluids</span> by bridging non-Markovian fluctuating hydrodynamics and molecular dynamics simulations</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Voulgarakis, Nikolaos K.; Satish, Siddarth; Chu, Jhih-Wei</p> <p>2009-12-01</p> <p>A multiscale computational method is developed to <span class="hlt">model</span> the nanoscale viscoelasticity of <span class="hlt">fluids</span> by bridging non-Markovian fluctuating hydrodynamics (FHD) and molecular dynamics (MD) simulations. To capture the elastic responses that emerge at small length scales, we attach an additional rheological <span class="hlt">model</span> parallel to the macroscopic constitutive equation of a <span class="hlt">fluid</span>. The widely used linear Maxwell <span class="hlt">model</span> is employed as a working choice; other <span class="hlt">models</span> can be used as well. For a <span class="hlt">fluid</span> that is Newtonian in the macroscopic limit, this approach results in a parallel Newtonian-Maxwell <span class="hlt">model</span>. For water, argon, and an ionic liquid, the power spectrum of momentum field autocorrelation functions of the parallel Newtonian-Maxwell <span class="hlt">model</span> agrees very well with those calculated from all-atom MD simulations. To incorporate thermal fluctuations, we generalize the equations of FHD to work with non-Markovian rheological <span class="hlt">models</span> and colored noise. The fluctuating stress tensor (white noise) is integrated in time in the same manner as its dissipative counterpart and numerical simulations indicate that this approach accurately preserves the set temperature in a FHD simulation. By mapping position and velocity vectors in the molecular representation onto field variables, we bridge the non-Markovian FHD with atomistic MD simulations. Through this mapping, we quantitatively determine the transport coefficients of the parallel Newtonian-Maxwell <span class="hlt">model</span> for water and argon from all-atom MD simulations. For both <span class="hlt">fluids</span>, a significant enhancement in elastic responses is observed as the wave number of hydrodynamic modes is reduced to a few nanometers. The mapping from particle to field representations and the perturbative strategy of developing constitutive equations provide a useful framework for <span class="hlt">modeling</span> the nanoscale viscoelasticity of <span class="hlt">fluids</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2008AGUFM.V11A2011A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2008AGUFM.V11A2011A"><span>Geochemical <span class="hlt">Modeling</span> of Zinc Silicate Ore Formation from Sedimentary Hydrothermal <span class="hlt">Fluids</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Appold, M. S.</p> <p>2008-12-01</p> <p>Sediment-hosted zinc deposits dominated by willemite (Zn2SiO4) instead of sphalerite (ZnS) are known from several prominent occurrences worldwide, including Vazante, Brazil, the Aroona Trend, Australia, Kabwe, Zambia, Berg Aukas, Namibia, and Abu Samar, Sudan. Although willemite-dominant zinc deposits appear to be much less common and are on average smaller than sphalerite-dominant zinc deposits, they nonetheless represent major enrichments of zinc in the Earth's crust, reaching sizes on the order of 1's to 10's of millions of tons and grades commonly between 20 and 40%. Sediment-hosted willemite- and sphalerite-dominant deposits share many similarities including their predominantly carbonate host rocks, gangue mineralogy, presumed derivation from sedimentary basinal brines, and spatial proximity. However, the conditions and processes that led to one style of mineralization versus the other have only recently begun to be investigated. The current study presents solubility, reaction path, and reactive transport <span class="hlt">modeling</span> results that attempt to define more clearly the conditions that favor willemite ore formation in sedimentary basins, with a focus on the Vazante deposit. Solubility calculations for willemite and sphalerite as a function of temperature, pH, salinity, and oxidation potential were carried out using a simple 3 molal NaCl solution saturated with respect to quartz. The results show that (1) willemite solubility is relatively insensitive to changes in temperature and oxidation potential whereas sphalerite solubility decreases sharply with decreasing temperature and oxidation potential, (2) willemite solubility decreases more strongly than sphalerite with increasing pH, (3) willemite and sphalerite have a similar strong decrease in solubility with decreasing salinity. The results support a previously proposed genetic <span class="hlt">model</span> for a willemite-dominant, sphalerite-subordinate ore body like Vazante in which a hot, acidic, metal-rich ore <span class="hlt">fluid</span> mixed with a cooler</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2008CompM..43...39T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2008CompM..43...39T"><span>Interface projection techniques for <span class="hlt">fluid</span>-structure interaction <span class="hlt">modeling</span> with moving-mesh methods</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Tezduyar, Tayfun E.; Sathe, Sunil; Pausewang, Jason; Schwaab, Matthew; Christopher, Jason; Crabtree, Jason</p> <p>2008-12-01</p> <p>The stabilized space-time <span class="hlt">fluid</span>-structure interaction (SSTFSI) technique developed by the Team for Advanced Flow Simulation and <span class="hlt">Modeling</span> (T★AFSM) was applied to a number of 3D examples, including arterial <span class="hlt">fluid</span> mechanics and parachute aerodynamics. Here we focus on the interface projection techniques that were developed as supplementary methods targeting the computational challenges associated with the geometric complexities of the <span class="hlt">fluid</span>-structure interface. Although these supplementary techniques were developed in conjunction with the SSTFSI method and in the context of air-fabric interactions, they can also be used in conjunction with other moving-mesh methods, such as the Arbitrary Lagrangian-Eulerian (ALE) method, and in the context of other classes of FSI applications. The supplementary techniques currently consist of using split nodal values for pressure at the edges of the fabric and incompatible meshes at the air-fabric interfaces, the FSI Geometric Smoothing Technique (FSI-GST), and the Homogenized <span class="hlt">Modeling</span> of Geometric Porosity (HMGP). Using split nodal values for pressure at the edges and incompatible meshes at the interfaces stabilizes the structural response at the edges of the membrane used in <span class="hlt">modeling</span> the fabric. With the FSI-GST, the <span class="hlt">fluid</span> mechanics mesh is sheltered from the consequences of the geometric complexity of the structure. With the HMGP, we bypass the intractable complexities of the geometric porosity by approximating it with an “equivalent”, locally-varying fabric porosity. As test cases demonstrating how the interface projection techniques work, we compute the air-fabric interactions of windsocks, sails and ringsail parachutes.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2001AGUFM.T22C0941P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2001AGUFM.T22C0941P"><span>Three-Dimensional <span class="hlt">Modeling</span> of <span class="hlt">Fluid</span> and Heat Transport in an Accretionary Complex</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Paula, C. A.; Ge, S.; Screaton, E. J.</p> <p>2001-12-01</p> <p>As sediments are scraped off of the subducting oceanic crust and accreted to the overriding plate, the rapid loading causes pore pressures in the underthrust sediments to increase. The change in pore pressure drives <span class="hlt">fluid</span> flow and heat transport within the accretionary complex. <span class="hlt">Fluid</span> is channeled along higher permeability faults and fractures and expelled at the seafloor. In this investigation, we examined the effects of sediment loading on <span class="hlt">fluid</span> flow and thermal transport in the decollement at the Barbados Ridge subduction zone. Both the width and thickness of the Barbados Ridge accretionary complex increase from north to south. The presence of mud diapers south of the Tiburon Rise and an observed southward decrease in heat flow measurements indicate that the increased thickness of the southern Barbados accretionary prism affects the transport of chemicals and heat by <span class="hlt">fluids</span>. The three-dimensional geometry and physical properties of the accretionary complex were utilized to construct a three-dimensional <span class="hlt">fluid</span> flow/heat transport <span class="hlt">model</span>. We calculated the pore pressure change due to a period of sediment loading and added this to steady-state pressure conditions to generate initial conditions for transient simulations. We then examined the diffusion of pore pressure and possible perturbation of the thermal regime over time due to loading of the underthrust sediments. The <span class="hlt">model</span> results show that the sediment-loading event was sufficient to create small temperature fluctuations in the decollement zone. The magnitude of temperature fluctuation in the decollement was greatest at the deformation front but did not vary significantly from north to south of the Tiburon Rise.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20130012776','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20130012776"><span>Computational <span class="hlt">Modeling</span> of Cephalad <span class="hlt">Fluid</span> Shift for Application to Microgravity-Induced Visual Impairment</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Nelson, Emily S.; Best, Lauren M.; Myers, Jerry G.; Mulugeta, Lealem</p> <p>2013-01-01</p> <p>An improved understanding of spaceflight-induced ocular pathology, including the loss of visual acuity, globe flattening, optic disk edema and distension of the optic nerve and optic nerve sheath, is of keen interest to space medicine. Cephalad <span class="hlt">fluid</span> shift causes a profoundly altered distribution of <span class="hlt">fluid</span> within the compartments of the head and body, and may indirectly generate phenomena that are biomechanically relevant to visual function, such as choroidal engorgement, compromised drainage of blood and cerebrospinal <span class="hlt">fluid</span> (CSF), and altered translaminar pressure gradient posterior to the eye. The experimental body of evidence with respect to the consequences of <span class="hlt">fluid</span> shift has not yet been able to provide a definitive picture of the sequence of events. On earth, elevated intracranial pressure (ICP) is associated with idiopathic intracranial hypertension (IIH), which can produce ocular pathologies that look similar to those seen in some astronauts returning from long-duration flight. However, the clinically observable features of the Visual Impairment and Intracranial Pressure (VIIP) syndrome in space and IIH on earth are not entirely consistent. Moreover, there are at present no experimental measurements of ICP in microgravity. By its very nature, physiological measurements in spaceflight are sparse, and the space environment does not lend itself to well-controlled experiments. In the absence of such data, numerical <span class="hlt">modeling</span> can play a role in the investigation of biomechanical causal pathways that are suspected of involvement in VIIP. In this work, we describe the conceptual framework for <span class="hlt">modeling</span> the altered compartmental <span class="hlt">fluid</span> distribution that represents an equilibrium <span class="hlt">fluid</span> distribution resulting from the loss of hydrostatic pressure gradient.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018EJPh...39c5002S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018EJPh...39c5002S"><span>A non-traditional <span class="hlt">fluid</span> problem: transition between theoretical <span class="hlt">models</span> from Stokes’ to turbulent flow</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Salomone, Horacio D.; Olivieri, Néstor A.; Véliz, Maximiliano E.; Raviola, Lisandro A.</p> <p>2018-05-01</p> <p>In the context of <span class="hlt">fluid</span> mechanics courses, it is customary to consider the problem of a sphere falling under the action of gravity inside a viscous <span class="hlt">fluid</span>. Under suitable assumptions, this phenomenon can be <span class="hlt">modelled</span> using Stokes’ law and is routinely reproduced in teaching laboratories to determine terminal velocities and <span class="hlt">fluid</span> viscosities. In many cases, however, the measured physical quantities show important deviations with respect to the predictions deduced from the simple Stokes’ <span class="hlt">model</span>, and the causes of these apparent ‘anomalies’ (for example, whether the flow is laminar or turbulent) are seldom discussed in the classroom. On the other hand, there are various variable-mass problems that students tackle during elementary mechanics courses and which are discussed in many textbooks. In this work, we combine both kinds of problems and analyse—both theoretically and experimentally—the evolution of a system composed of a sphere pulled by a chain of variable length inside a tube filled with water. We investigate the effects of different forces acting on the system such as weight, buoyancy, viscous friction and drag force. By means of a sequence of mathematical <span class="hlt">models</span> of increasing complexity, we obtain a progressive fit that accounts for the experimental data. The contrast between the various <span class="hlt">models</span> exposes the strengths and weaknessess of each one. The proposed experience can be useful for integrating concepts of elementary mechanics and <span class="hlt">fluids</span>, and is suitable as laboratory practice, stressing the importance of the experimental validation of theoretical <span class="hlt">models</span> and showing the <span class="hlt">model</span>-building processes in a didactic framework.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19990035926','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19990035926"><span>Proper Orthogonal Decomposition in Optimal Control of <span class="hlt">Fluids</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Ravindran, S. S.</p> <p>1999-01-01</p> <p>In this article, we present a reduced order <span class="hlt">modeling</span> approach suitable for active control of <span class="hlt">fluid</span> dynamical systems <span class="hlt">based</span> on proper orthogonal decomposition (POD). The rationale behind the reduced order <span class="hlt">modeling</span> is that numerical simulation of Navier-Stokes equations is still too costly for the purpose of optimization and control of unsteady flows. We examine the possibility of obtaining reduced order <span class="hlt">models</span> that reduce computational complexity associated with the Navier-Stokes equations while capturing the essential dynamics by using the POD. The POD allows extraction of certain optimal set of basis functions, perhaps few, from a computational or experimental data-<span class="hlt">base</span> through an eigenvalue analysis. The solution is then obtained as a linear combination of these optimal set of basis functions by means of Galerkin projection. This makes it attractive for optimal control and estimation of systems governed by partial differential equations. We here use it in active control of <span class="hlt">fluid</span> flows governed by the Navier-Stokes equations. We show that the resulting reduced order <span class="hlt">model</span> can be very efficient for the computations of optimization and control problems in unsteady flows. Finally, implementational issues and numerical experiments are presented for simulations and optimal control of <span class="hlt">fluid</span> flow through channels.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018OptLT.100..244X','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018OptLT.100..244X"><span><span class="hlt">Modelling</span> of <span class="hlt">fluid</span> flow phenomenon in laser+GMAW hybrid welding of aluminum alloy considering three phase coupling and arc plasma shear stress</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Xu, Guoxiang; Li, Pengfei; Cao, Qingnan; Hu, Qingxian; Gu, Xiaoyan; Du, Baoshuai</p> <p>2018-03-01</p> <p>The present study aims to develop a unified three dimensional numerical <span class="hlt">model</span> for fiber laser+GMAW hybrid welding, which is used to study the <span class="hlt">fluid</span> flow phenomena in hybrid welding of aluminum alloy and the influence of laser power on weld pool dynamic behavior. This <span class="hlt">model</span> takes into account the coupling of gas, liquid and metal phases. Laser heat input is described using a cone heat source <span class="hlt">model</span> with changing peak power density, its height being determined <span class="hlt">based</span> on the keyhole size. Arc heat input is <span class="hlt">modeled</span> as a double ellipsoid heat source. The arc plasma flow and droplet transfer are simulated through the two simplified <span class="hlt">models</span>. The temperature and velocity fields for different laser powers are calculated. The computed results are in general agreement with the experimental data. Both the peak and average values of <span class="hlt">fluid</span> flow velocity during hybrid welding are much higher than those of GMAW. At a low level of laser power, both the arc force and droplet impingement force play a relatively large role on <span class="hlt">fluid</span> flow in the hybrid welding. Keyhole depth always oscillates within a range. With an increase in laser power, the weld pool behavior becomes more complex. An anti-clockwise vortex is generated and the stability of keyhole depth is improved. Besides, the effects of laser power on different driving forces of <span class="hlt">fluid</span> flow in weld pool are also discussed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EPJP..132..197H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EPJP..132..197H"><span>Experimental analysis to improving thermosyphon (TPCT) thermal efficiency using nanoparticles/<span class="hlt">based</span> <span class="hlt">fluids</span> (water)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hoseinzadeh, S.; Sahebi, S. A. R.; Ghasemiasl, R.; Majidian, A. R.</p> <p>2017-05-01</p> <p>In the present study an experimental set-up is used to investigate the effect of a nanofluid as a working <span class="hlt">fluid</span> to increase thermosyphon efficiency. Nanofluids are a new form of heat transfer media prepared by suspending metallic and nonmetallic nanoparticles in a <span class="hlt">base</span> <span class="hlt">fluid</span>. The nanoparticles added to the <span class="hlt">fluid</span> enhance the thermal characteristics of the <span class="hlt">base</span> <span class="hlt">fluid</span>. The nanofluid used in this experiment was a mixture of water and nanoparticles prepared with 0.5%, 1%, 1.5%, or 2% (v) concentration of silicon carbide (SiC) nanoparticles and 1%, 2% and 3% (v) concentration of aluminum oxide (Al2O3) in an ultrasonic homogenizer. The results indicate that the SiC/water and Al2O3/water nanofluids increase the thermosyphon performance. The efficiency of the thermosyphon using the 2% (v) (SiC) nanoparticles nanofluid was 1.11 times that of pure water and the highest efficiency occurs for the 3% (Al2O3) nanoparticle concentration with input power of 300 W. The decrease in the temperature difference between the condenser and evaporator confirms these enhancements.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014AGUFM.H13P..07W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AGUFM.H13P..07W"><span>Simulation of Two-Phase Flow <span class="hlt">Based</span> on a Thermodynamically Constrained Averaging Theory Flow <span class="hlt">Model</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Weigand, T. M.; Dye, A. L.; McClure, J. E.; Farthing, M. W.; Gray, W. G.; Miller, C. T.</p> <p>2014-12-01</p> <p>The thermodynamically constrained averaging theory (TCAT) has been used to formulate general classes of porous medium <span class="hlt">models</span>, including new <span class="hlt">models</span> for two-<span class="hlt">fluid</span>-phase flow. The TCAT approach provides advantages that include a firm connection between the microscale, or pore scale, and the macroscale; a thermodynamically consistent basis; explicit inclusion of factors such as interfacial areas, contact angles, interfacial tension, and curvatures; and dynamics of interface movement and relaxation to an equilibrium state. In order to render the TCAT <span class="hlt">model</span> solvable, certain closure relations are needed to relate <span class="hlt">fluid</span> pressure, interfacial areas, curvatures, and relaxation rates. In this work, we formulate and solve a TCAT-<span class="hlt">based</span> two-<span class="hlt">fluid</span>-phase flow <span class="hlt">model</span>. We detail the formulation of the <span class="hlt">model</span>, which is a specific instance from a hierarchy of two-<span class="hlt">fluid</span>-phase flow <span class="hlt">models</span> that emerge from the theory. We show the closure problem that must be solved. Using recent results from high-resolution microscale simulations, we advance a set of closure relations that produce a closed <span class="hlt">model</span>. Lastly, we use locally conservative spatial discretization and higher order temporal discretization methods to approximate the solution to this new <span class="hlt">model</span> and compare the solution to the traditional <span class="hlt">model</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2002AGUFM.H21B0799B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2002AGUFM.H21B0799B"><span><span class="hlt">Modeling</span> <span class="hlt">Fluid</span> Flow and Microbial Reactions in the Peru Accretionary Complex</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bekins, B. A.; Matmon, D.</p> <p>2002-12-01</p> <p>Accretionary complexes are sites where sediment compaction and deeper reactions drive large-scale flow systems that can affect global solute budgets. Extensive <span class="hlt">modeling</span> and drilling studies have elucidated the origin of the <span class="hlt">fluids</span>, pore pressures, duration of flow, and major flow paths in these settings. An important research goal is to quantify the effect of these flow systems on global chemical budgets of reactive solutes such as carbon. The Peru margin represents an end member setting that can serve as a basis to extend the results to other margins. The sediments are relatively high in organic carbon with an average value of 2.6%. The subduction rate at ~9 cm/yr and taper angle at 14-17° are among the largest in the world. Recent microbial studies on Ocean Drilling Program Leg 201 at the Peru accretionary margin provide many key elements needed to quantify the processes affecting organic carbon in an accretionary complex. Pore water chemistry data from Site 1230 located in the Peru accretionary prism indicate that sulfate reduction is important in the top 8 mbsf. Below this depth, methanogenesis is the dominant process and methane concentrations are among the highest measured at any site on Leg 201. The presence of high methane concentrations at shallow depths suggests that methane is transported upward in the prism by <span class="hlt">fluid</span> flow. Measurements of in-situ pore pressures and temperatures also support the presence of upward <span class="hlt">fluid</span> flow. A single in-situ pressure measurement at ~100 mbsf indicated an overpressure of 0.14 MPa. For a reasonable formation permeability of ~ 10-16 m2, the measured overpressure is adequate to produce flow at a rate of ~5 mm/yr. This rate is comparable to previous <span class="hlt">model</span> estimates for flow rates in the Peru accretionary prism. In addition, curvature in the downhole temperature profile can best be explained by upward <span class="hlt">fluid</span> flow of 1-10 mm/yr. These data are used to constrain a two-dimensional coupled <span class="hlt">fluid</span> flow and reactive transport <span class="hlt">model</span></p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017APS..DPPU11032S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017APS..DPPU11032S"><span>Studies of Plasma Instabilities using Unstructured Discontinuous Galerkin Method with the Two-<span class="hlt">Fluid</span> Plasma <span class="hlt">Model</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Song, Yang; Srinivasan, Bhuvana</p> <p>2017-10-01</p> <p>The discontinuous Galerkin (DG) method has the advantage of resolving shocks and sharp gradients that occur in neutral <span class="hlt">fluids</span> and plasmas. An unstructured DG code has been developed in this work to study plasma instabilities using the two-<span class="hlt">fluid</span> plasma <span class="hlt">model</span>. Unstructured meshes are known to produce small and randomized grid errors compared to traditional structured meshes. Computational tests for Rayleigh-Taylor instabilities in radially-converging flows are performed using the MHD <span class="hlt">model</span>. Choice of grid geometry is not obvious for simulations of instabilities in these circular configurations. Comparisons of the effects for different grids are made. A 2D magnetic nozzle simulation using the two-<span class="hlt">fluid</span> plasma <span class="hlt">model</span> is also performed. A vacuum boundary condition technique is applied to accurately solve the Riemann problem on the edge of the plume.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/22934022','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/22934022"><span>An integrated <span class="hlt">fluid</span>-chemical <span class="hlt">model</span> toward <span class="hlt">modeling</span> the formation of intra-luminal thrombus in abdominal aortic aneurysms.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Biasetti, Jacopo; Spazzini, Pier Giorgio; Swedenborg, Jesper; Gasser, T Christian</p> <p>2012-01-01</p> <p>Abdominal Aortic Aneurysms (AAAs) are frequently characterized by the presence of an Intra-Luminal Thrombus (ILT) known to influence their evolution biochemically and biomechanically. The ILT progression mechanism is still unclear and little is known regarding the impact of the chemical species transported by blood flow on this mechanism. Chemical agonists and antagonists of platelets activation, aggregation, and adhesion and the proteins involved in the coagulation cascade (CC) may play an important role in ILT development. Starting from this assumption, the evolution of chemical species involved in the CC, their relation to coherent vortical structures (VSs) and their possible effect on ILT evolution have been studied. To this end a <span class="hlt">fluid</span>-chemical <span class="hlt">model</span> that simulates the CC through a series of convection-diffusion-reaction (CDR) equations has been developed. The <span class="hlt">model</span> involves plasma-phase and surface-bound enzymes and zymogens, and includes both plasma-phase and membrane-phase reactions. Blood is <span class="hlt">modeled</span> as a non-Newtonian incompressible <span class="hlt">fluid</span>. VSs convect thrombin in the domain and lead to the high concentration observed in the distal portion of the AAA. This finding is in line with the clinical observations showing that the thickest ILT is usually seen in the distal AAA region. The proposed <span class="hlt">model</span>, due to its ability to couple the <span class="hlt">fluid</span> and chemical domains, provides an integrated mechanochemical picture that potentially could help unveil mechanisms of ILT formation and development.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4090431','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4090431"><span>Synthesis and Performance Evaluation of a New Deoiling Agent for Treatment of Waste Oil-<span class="hlt">Based</span> Drilling <span class="hlt">Fluids</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>Liu, Pingting; Huang, Zhiyu; Deng, Hao; Wang, Rongsha; Xie, Shuixiang</p> <p>2014-01-01</p> <p>Oil-<span class="hlt">based</span> drilling <span class="hlt">fluid</span> is used more and more in the field of oil and gas exploration. However, because of unrecyclable treating agent and hard treatment conditions, the traditional treating technologies of waste oil-<span class="hlt">based</span> drilling <span class="hlt">fluid</span> have some defects, such as waste of resource, bulky equipment, complex treatment processes, and low oil recovery rate. In this work, switchable deoiling agent (SDA), as a novel surfactant for treatment of waste oil-<span class="hlt">based</span> drilling <span class="hlt">fluid</span>, was synthesized by amine, formic acid, and formaldehyde solution. With this agent, the waste oil-<span class="hlt">based</span> drilling <span class="hlt">fluid</span> can be treated without complex process and expensive equipment. Furthermore, the agent used in the treatment can be recycled, which reduces waste of resource and energy. The switch performance, deoiling performance, structural characterization, and mechanisms of action are studied. The experimental results show that the oil content of the recycled oil is higher than 96% and more than 93% oil in waste oil-<span class="hlt">based</span> drilling <span class="hlt">fluid</span> can be recycled. The oil content of the solid residues of deoiling is less than 3%. PMID:25045749</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/25045749','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25045749"><span>Synthesis and performance evaluation of a new deoiling agent for treatment of waste oil-<span class="hlt">based</span> drilling <span class="hlt">fluids</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Liu, Pingting; Huang, Zhiyu; Deng, Hao; Wang, Rongsha; Xie, Shuixiang</p> <p>2014-01-01</p> <p>Oil-<span class="hlt">based</span> drilling <span class="hlt">fluid</span> is used more and more in the field of oil and gas exploration. However, because of unrecyclable treating agent and hard treatment conditions, the traditional treating technologies of waste oil-<span class="hlt">based</span> drilling <span class="hlt">fluid</span> have some defects, such as waste of resource, bulky equipment, complex treatment processes, and low oil recovery rate. In this work, switchable deoiling agent (SDA), as a novel surfactant for treatment of waste oil-<span class="hlt">based</span> drilling <span class="hlt">fluid</span>, was synthesized by amine, formic acid, and formaldehyde solution. With this agent, the waste oil-<span class="hlt">based</span> drilling <span class="hlt">fluid</span> can be treated without complex process and expensive equipment. Furthermore, the agent used in the treatment can be recycled, which reduces waste of resource and energy. The switch performance, deoiling performance, structural characterization, and mechanisms of action are studied. The experimental results show that the oil content of the recycled oil is higher than 96% and more than 93% oil in waste oil-<span class="hlt">based</span> drilling <span class="hlt">fluid</span> can be recycled. The oil content of the solid residues of deoiling is less than 3%.</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/2012IJCFD..26..193D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012IJCFD..26..193D"><span>A heterogeneous system <span class="hlt">based</span> on GPU and multi-core CPU for real-time <span class="hlt">fluid</span> and rigid body simulation</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>da Silva Junior, José Ricardo; Gonzalez Clua, Esteban W.; Montenegro, Anselmo; Lage, Marcos; Dreux, Marcelo de Andrade; Joselli, Mark; Pagliosa, Paulo A.; Kuryla, Christine Lucille</p> <p>2012-03-01</p> <p>Computational <span class="hlt">fluid</span> dynamics in simulation has become an important field not only for physics and engineering areas but also for simulation, computer graphics, virtual reality and even video game development. Many efficient <span class="hlt">models</span> have been developed over the years, but when many contact interactions must be processed, most <span class="hlt">models</span> present difficulties or cannot achieve real-time results when executed. The advent of parallel computing has enabled the development of many strategies for accelerating the simulations. Our work proposes a new system which uses some successful algorithms already proposed, as well as a data structure organisation <span class="hlt">based</span> on a heterogeneous architecture using CPUs and GPUs, in order to process the simulation of the interaction of <span class="hlt">fluids</span> and rigid bodies. This successfully results in a two-way interaction between them and their surrounding objects. As far as we know, this is the first work that presents a computational collaborative environment which makes use of two different paradigms of hardware architecture for this specific kind of problem. Since our method achieves real-time results, it is suitable for virtual reality, simulation and video game <span class="hlt">fluid</span> simulation problems.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/25005435','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25005435"><span>Effects of <span class="hlt">fluid</span> structure interaction in a three dimensional <span class="hlt">model</span> of the spinal subarachnoid space.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Cheng, Shaokoon; Fletcher, David; Hemley, Sarah; Stoodley, Marcus; Bilston, Lynne</p> <p>2014-08-22</p> <p>It is unknown whether spinal cord motion has a significant effect on cerebrospinal <span class="hlt">fluid</span> (CSF) pressure and therefore the importance of including <span class="hlt">fluid</span> structure interaction (FSI) in computational <span class="hlt">fluid</span> dynamics <span class="hlt">models</span> (CFD) of the spinal subarachnoid space (SAS) is unclear. This study aims to determine the effects of FSI on CSF pressure and spinal cord motion in a normal and in a stenosis <span class="hlt">model</span> of the SAS. A three-dimensional patient specific <span class="hlt">model</span> of the SAS and spinal cord were constructed from MR anatomical images and CSF flow rate measurements obtained from a healthy human being. The area of SAS at spinal level T4 was constricted by 20% to represent the stenosis <span class="hlt">model</span>. FSI simulations in both <span class="hlt">models</span> were performed by running ANSYS CFX and ANSYS Mechanical in tandem. Results from this study show that the effect of FSI on CSF pressure is only about 1% in both the normal and stenosis <span class="hlt">models</span> and therefore show that FSI has a negligible effect on CSF pressure. Crown Copyright © 2014. Published by Elsevier Ltd. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018AdWR..116..153L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018AdWR..116..153L"><span>A lattice Boltzmann investigation of steady-state <span class="hlt">fluid</span> distribution, capillary pressure and relative permeability of a porous medium: Effects of <span class="hlt">fluid</span> and geometrical properties</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Li, Zi; Galindo-Torres, Sergio; Yan, Guanxi; Scheuermann, Alexander; Li, Ling</p> <p>2018-06-01</p> <p>Simulations of simultaneous steady-state two-phase flow in the capillary force-dominated regime were conducted using the state-of-the-art Shan-Chen multi-component lattice Boltzmann <span class="hlt">model</span> (SCMC-LBM) <span class="hlt">based</span> on two-dimensional porous media. We focused on analyzing the <span class="hlt">fluid</span> distribution (i.e., WP <span class="hlt">fluid</span>-solid, NP <span class="hlt">fluid</span>-solid and <span class="hlt">fluid-fluid</span> interfacial areas) as well as the capillary pressure versus saturation curve which was affected by <span class="hlt">fluid</span> and geometrical properties (i.e., wettability, adhesive strength, pore size distribution and specific surface area). How these properties influenced the relative permeability versus saturation relation through apparent effective permeability and threshold pressure gradient was also explored. The SCMC-LBM simulations showed that, a thin WP <span class="hlt">fluid</span> film formed around the solid surface due to the adhesive <span class="hlt">fluid</span>-solid interaction, resulting in discrete WP <span class="hlt">fluid</span> distributions and reduction of the WP <span class="hlt">fluid</span> mobility. Also, the adhesive interaction provided another source of capillary pressure in addition to capillary force, which, however, did not affect the mobility of the NP <span class="hlt">fluid</span>. The film <span class="hlt">fluid</span> effect could be enhanced by large adhesive strength and fine pores in heterogeneous porous media. In the steady-state infiltration, not only the NP <span class="hlt">fluid</span> but also the WP <span class="hlt">fluid</span> were subjected to the capillary resistance. The capillary pressure effect could be alleviated by decreased wettability, large average pore radius and improved <span class="hlt">fluid</span> connectivity in heterogeneous porous media. The present work <span class="hlt">based</span> on the SCMC-LBM investigations elucidated the role of film <span class="hlt">fluid</span> as well as capillary pressure in the two-phase flow system. The findings have implications for ways to improve the macroscopic flow equation <span class="hlt">based</span> on balance of force for the steady-state infiltration.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/15834688','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/15834688"><span>A mathematical <span class="hlt">model</span> of electrolyte and <span class="hlt">fluid</span> transport across corneal endothelium.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Fischbarg, J; Diecke, F P J</p> <p>2005-01-01</p> <p>To predict the behavior of a transporting epithelium by intuitive means can be complex and frustrating. As the number of parameters to be considered increases beyond a few, the task can be termed impossible. The alternative is to <span class="hlt">model</span> epithelial behavior by mathematical means. For that to be feasible, it has been presumed that a large amount of experimental information is required, so as to be able to use known values for the majority of kinetic parameters. However, in the present case, we are <span class="hlt">modeling</span> corneal endothelial behavior beginning with experimental values for only five of eleven parameters. The remaining parameter values are calculated assuming cellular steady state and using algebraic software. With that as <span class="hlt">base</span>, as in preceding treatments but with a distribution of channels/transporters suited to the endothelium, temporal cell and tissue behavior are computed by a program written in Basic that monitors changes in chemical and electrical driving forces across cell membranes and the paracellular pathway. We find that the program reproduces quite well the behaviors experimentally observed for the translayer electrical potential difference and rate of <span class="hlt">fluid</span> transport, (a) in the steady state, (b) after perturbations by changes in ambient conditions HCO3-, Na+, and Cl- concentrations), and (c) after challenge by inhibitors (ouabain, DIDS, Na+- and Cl(-)-channel inhibitors). In addition, we have used the program to compare predictions of translayer <span class="hlt">fluid</span> transport by two competing theories, electro-osmosis and local osmosis. Only predictions using electro-osmosis fit all the experimental data.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20120014612','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20120014612"><span>Scaling of Lift Degradation Due to Anti-Icing <span class="hlt">Fluids</span> <span class="hlt">Based</span> Upon the Aerodynamic Acceptance Test</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Broeren, Andy P.; Riley, James T.</p> <p>2012-01-01</p> <p>In recent years, the FAA has worked with Transport Canada, National Research Council Canada (NRC) and APS Aviation, Inc. to develop allowance times for aircraft operations in ice-pellet precipitation. These allowance times are critical to ensure safety and efficient operation of commercial and cargo flights. Wind-tunnel testing with uncontaminated anti-icing <span class="hlt">fluids</span> and <span class="hlt">fluids</span> contaminated with simulated ice pellets had been carried out at the NRC Propulsion and Icing Wind Tunnel (PIWT) to better understand the flowoff characteristics and resulting aerodynamic effects. The percent lift loss on the thin, high-performance wing <span class="hlt">model</span> tested in the PIWT was determined at 8 angle of attack and used as one of the evaluation criteria in determining the allowance times. Because it was unclear as to how performance degradations measured on this <span class="hlt">model</span> were relevant to an actual airplane configuration, some means of interpreting the wing <span class="hlt">model</span> lift loss was deemed necessary. This paper describes how the lift loss was related to the loss in maximum lift of a Boeing 737-200ADV airplane through the Aerodynamic Acceptance Test (AAT) performed for <span class="hlt">fluids</span> qualification. A loss in maximum lift coefficient of 5.24 percent on the B737-200ADV airplane (which was adopted as the threshold in the AAT) corresponds to a lift loss of 7.3 percent on the PIWT <span class="hlt">model</span> at 8 angle of attack. There is significant scatter in the data used to develop the correlation related to varying effects of the anti-icing <span class="hlt">fluids</span> that were tested and other factors. A statistical analysis indicated the upper limit of lift loss on the PIWT <span class="hlt">model</span> was 9.2 percent. Therefore, for cases resulting in PIWT <span class="hlt">model</span> lift loss from 7.3 to 9.2 percent, extra scrutiny of the visual observations is required in evaluating <span class="hlt">fluid</span> performance with contamination.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20120018061','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20120018061"><span>Scaling of Lift Degradation Due to Anti-Icing <span class="hlt">Fluids</span> <span class="hlt">Based</span> Upon the Aerodynamic Acceptance Test</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Broeren, Andy; Riley, Jim</p> <p>2012-01-01</p> <p>In recent years, the FAA has worked with Transport Canada, National Research Council Canada (NRC) and APS Aviation, Inc. to develop allowance times for aircraft operations in ice-pellet precipitation. These allowance times are critical to ensure safety and efficient operation of commercial and cargo flights. Wind-tunnel testing with uncontaminated anti-icing <span class="hlt">fluids</span> and <span class="hlt">fluids</span> contaminated with simulated ice pellets had been carried out at the NRC Propulsion and Icing Wind Tunnel (PIWT) to better understand the flow-off characteristics and resulting aerodynamic effects. The percent lift loss on the thin, high-performance wing <span class="hlt">model</span> tested in the PIWT was determined at 8 deg. angle of attack and used as one of the evaluation criteria in determining the allowance times. Because it was unclear as to how performance degradations measured on this <span class="hlt">model</span> were relevant to an actual airplane configuration, some means of interpreting the wing <span class="hlt">model</span> lift loss was deemed necessary. This paper describes how the lift loss was related to the loss in maximum lift of a Boeing 737-200ADV airplane through the Aerodynamic Acceptance Test (AAT) performed for <span class="hlt">fluids</span> qualification. A loss in maximum lift coefficient of 5.24% on the B737-200ADV airplane (which was adopted as the threshold in the AAT) corresponds to a lift loss of 7.3% on the PIWT <span class="hlt">model</span> at 8 deg. angle of attack. There is significant scatter in the data used to develop the correlation related to varying effects of the anti-icing <span class="hlt">fluids</span> that were tested and other factors. A statistical analysis indicated the upper limit of lift loss on the PIWT <span class="hlt">model</span> was 9.2%. Therefore, for cases resulting in PIWT <span class="hlt">model</span> lift loss from 7.3% to 9.2%, extra scrutiny of the visual observations is required in evaluating <span class="hlt">fluid</span> performance with contamination.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2008GGG.....9.6010B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2008GGG.....9.6010B"><span>Strontium isotope constraints on <span class="hlt">fluid</span> flow in the sheeted dike complex of fast spreading crust: Pervasive <span class="hlt">fluid</span> flow at Pito Deep</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Barker, A. K.; Coogan, L. A.; Gillis, K. M.; Weis, D.</p> <p>2008-06-01</p> <p><span class="hlt">Fluid</span> flow through the axial hydrothermal system at fast spreading ridges is investigated using the Sr-isotopic composition of upper crustal samples recovered from a tectonic window at Pito Deep (NE Easter microplate). Samples from the sheeted dike complex collected away from macroscopic evidence of channelized <span class="hlt">fluid</span> flow, such as faults and centimeter-scale hydrothermal veins, show a range of 87Sr/86Sr from 0.7025 to 0.7030 averaging 0.70276 relative to a protolith with 87Sr/86Sr of ˜0.7024. There is no systematic variation in 87Sr/86Sr with depth in the sheeted dike complex. Comparison of these new data with the two other localities that similar data sets exist for (ODP Hole 504B and the Hess Deep tectonic window) reveals that the extent of Sr-isotope exchange is similar in all of these locations. <span class="hlt">Models</span> that assume that <span class="hlt">fluid</span>-rock reaction occurs during one-dimensional (recharge) flow lead to significant decreases in the predicted extent of isotopic modification of the rock with depth in the crust. These <span class="hlt">model</span> results show systematic misfits when compared with the data that can only be avoided if the <span class="hlt">fluid</span> flow is assumed to be focused in isolated channels with very slow <span class="hlt">fluid</span>-rock exchange. In this scenario the <span class="hlt">fluid</span> at the <span class="hlt">base</span> of the crust is little modified in 87Sr/86Sr from seawater and thus unlike vent <span class="hlt">fluids</span>. Additionally, this <span class="hlt">model</span> predicts that some rocks should show no change from the fresh-rock 87Sr/86Sr, but this is not observed. Alternatively, <span class="hlt">models</span> in which <span class="hlt">fluid</span>-rock reaction occurs during upflow (discharge) as well as downflow, or in which <span class="hlt">fluids</span> are recirculated within the hydrothermal system, can reproduce the observed lack of variation in 87Sr/86Sr with depth in the crust. Minimum time-integrated <span class="hlt">fluid</span> fluxes, calculated from mass balance, are between 1.5 and 2.6 × 106 kg m-2 for all areas studied to date. However, new evidence from both the rocks and a compilation of vent <span class="hlt">fluid</span> compositions demonstrates that some Sr is leached from the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5707624','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5707624"><span>Pressure-Responsive, Surfactant-Free CO2-<span class="hlt">Based</span> Nanostructured <span class="hlt">Fluids</span></span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p></p> <p>2017-01-01</p> <p>Microemulsions are extensively used in advanced material and chemical processing. However, considerable amounts of surfactant are needed for their formulation, which is a drawback due to both economic and ecological reasons. Here, we describe the nanostructuration of recently discovered surfactant-free, carbon dioxide (CO2)-<span class="hlt">based</span> microemulsion-like systems in a water/organic-solvent/CO2 pressurized ternary mixture. “Water-rich” nanodomains embedded into a “water-depleted” matrix have been observed and characterized by the combination of Raman spectroscopy, molecular dynamics simulations, and small-angle neutron scattering. These single-phase <span class="hlt">fluids</span> show a reversible, pressure-responsive nanostructuration; the “water-rich” nanodomains at a given pressure can be instantaneously degraded/expanded by increasing/decreasing the pressure, resulting in a reversible, rapid, and homogeneous mixing/demixing of their content. This pressure-triggered responsiveness, together with other inherent features of these <span class="hlt">fluids</span>, such as the absence of any contaminant in the ternary mixture (e.g., surfactant), their spontaneous formation, and their solvation capability (enabling the dissolution of both hydrophobic and hydrophilic molecules), make them appealing complex <span class="hlt">fluid</span> systems to be used in molecular material processing and in chemical engineering. PMID:28846386</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://eric.ed.gov/?q=propulsion&pg=3&id=EJ682152','ERIC'); return false;" href="https://eric.ed.gov/?q=propulsion&pg=3&id=EJ682152"><span>Using <span class="hlt">Models</span> at the Mesoscopic Scale in Teaching Physics: Two Experimental Interventions in Solid Friction and <span class="hlt">Fluid</span> Statics</span></a></p> <p><a target="_blank" href="http://www.eric.ed.gov/ERICWebPortal/search/extended.jsp?_pageLabel=advanced">ERIC Educational Resources Information Center</a></p> <p>Besson, Ugo; Viennot, Laurence</p> <p>2004-01-01</p> <p>This article examines the didactic suitability of introducing <span class="hlt">models</span> at an intermediate (i.e. mesoscopic) scale in teaching certain subjects, at an early stage. The design and evaluation of two short sequences <span class="hlt">based</span> on this rationale will be outlined: one bears on propulsion by solid friction, the other on <span class="hlt">fluid</span> statics in the presence of gravity.…</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://cfpub.epa.gov/si/si_public_record_report.cfm?dirEntryId=159447&keyword=fluid+AND+cfd&actType=&TIMSType=+&TIMSSubTypeID=&DEID=&epaNumber=&ntisID=&archiveStatus=Both&ombCat=Any&dateBeginCreated=&dateEndCreated=&dateBeginPublishedPresented=&dateEndPublishedPresented=&dateBeginUpdated=&dateEndUpdated=&dateBeginCompleted=&dateEndCompleted=&personID=&role=Any&journalID=&publisherID=&sortBy=revisionDate&count=50','EPA-EIMS'); return false;" href="https://cfpub.epa.gov/si/si_public_record_report.cfm?dirEntryId=159447&keyword=fluid+AND+cfd&actType=&TIMSType=+&TIMSSubTypeID=&DEID=&epaNumber=&ntisID=&archiveStatus=Both&ombCat=Any&dateBeginCreated=&dateEndCreated=&dateBeginPublishedPresented=&dateEndPublishedPresented=&dateBeginUpdated=&dateEndUpdated=&dateBeginCompleted=&dateEndCompleted=&personID=&role=Any&journalID=&publisherID=&sortBy=revisionDate&count=50"><span>A FRAMEWORK FOR FINE-SCALE COMPUTATIONAL <span class="hlt">FLUID</span> DYNAMICS AIR QUALITY <span class="hlt">MODELING</span> AND ANALYSIS</span></a></p> <p><a target="_blank" href="http://oaspub.epa.gov/eims/query.page">EPA Science Inventory</a></p> <p></p> <p></p> <p>This paper discusses a framework for fine-scale CFD <span class="hlt">modeling</span> that may be developed to complement the present Community Multi-scale Air Quality (CMAQ) <span class="hlt">modeling</span> system which itself is a computational <span class="hlt">fluid</span> dynamics <span class="hlt">model</span>. A goal of this presentation is to stimulate discussions on w...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFM.H51U..05N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.H51U..05N"><span><span class="hlt">Modeling</span>, Uncertainty Quantification and Sensitivity Analysis of Subsurface <span class="hlt">Fluid</span> Migration in the Above Zone Monitoring Interval of a Geologic Carbon Storage</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Namhata, A.; Dilmore, R. M.; Oladyshkin, S.; Zhang, L.; Nakles, D. V.</p> <p>2015-12-01</p> <p>Carbon dioxide (CO2) storage into geological formations has significant potential for mitigating anthropogenic CO2 emissions. An increasing emphasis on the commercialization and implementation of this approach to store CO2 has led to the investigation of the physical processes involved and to the development of system-wide mathematical <span class="hlt">models</span> for the evaluation of potential geologic storage sites and the risk associated with them. The sub-system components under investigation include the storage reservoir, caprock seals, and the above zone monitoring interval, or AZMI, to name a few. Diffusive leakage of CO2 through the caprock seal to overlying formations may occur due to its intrinsic permeability and/or the presence of natural/induced fractures. This results in a potential risk to environmental receptors such as underground sources of drinking water. In some instances, leaking CO2 also has the potential to reach the ground surface and result in atmospheric impacts. In this work, <span class="hlt">fluid</span> (i.e., CO2 and brine) flow above the caprock, in the region designated as the AZMI, is <span class="hlt">modeled</span> for a leakage event of a typical geologic storage system with different possible boundary scenarios. An analytical and approximate solution for radial migration of <span class="hlt">fluids</span> in the AZMI with continuous inflow of <span class="hlt">fluids</span> from the reservoir through the caprock has been developed. In its present form, the AZMI <span class="hlt">model</span> predicts the spatial changes in pressure - gas saturations over time in a layer immediately above the caprock. The <span class="hlt">modeling</span> is performed for a benchmark case and the data-driven approach of arbitrary Polynomial Chaos (aPC) Expansion is used to quantify the uncertainty of the <span class="hlt">model</span> outputs <span class="hlt">based</span> on the uncertainty of <span class="hlt">model</span> input parameters such as porosity, permeability, formation thickness, and residual brine saturation. The recently developed aPC approach performs stochastic <span class="hlt">model</span> reduction and approximates the <span class="hlt">models</span> by a polynomial-<span class="hlt">based</span> response surface. Finally, a global</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EPJWC.14009013E','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EPJWC.14009013E"><span>Numerical <span class="hlt">models</span> for <span class="hlt">fluid</span>-grains interactions: opportunities and limitations</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Esteghamatian, Amir; Rahmani, Mona; Wachs, Anthony</p> <p>2017-06-01</p> <p>In the framework of a multi-scale approach, we develop numerical <span class="hlt">models</span> for suspension flows. At the micro scale level, we perform particle-resolved numerical simulations using a Distributed Lagrange Multiplier/Fictitious Domain approach. At the meso scale level, we use a two-way Euler/Lagrange approach with a Gaussian filtering kernel to <span class="hlt">model</span> <span class="hlt">fluid</span>-solid momentum transfer. At both the micro and meso scale levels, particles are individually tracked in a Lagrangian way and all inter-particle collisions are computed by a Discrete Element/Soft-sphere method. The previous numerical <span class="hlt">models</span> have been extended to handle particles of arbitrary shape (non-spherical, angular and even non-convex) as well as to treat heat and mass transfer. All simulation tools are fully-MPI parallel with standard domain decomposition and run on supercomputers with a satisfactory scalability on up to a few thousands of cores. The main asset of multi scale analysis is the ability to extend our comprehension of the dynamics of suspension flows <span class="hlt">based</span> on the knowledge acquired from the high-fidelity micro scale simulations and to use that knowledge to improve the meso scale <span class="hlt">model</span>. We illustrate how we can benefit from this strategy for a fluidized bed, where we introduce a stochastic drag force <span class="hlt">model</span> derived from micro-scale simulations to recover the proper level of particle fluctuations. Conversely, we discuss the limitations of such <span class="hlt">modelling</span> tools such as their limited ability to capture lubrication forces and boundary layers in highly inertial flows. We suggest ways to overcome these limitations in order to enhance further the capabilities of the numerical <span class="hlt">models</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017SPIE10164E..2FH','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017SPIE10164E..2FH"><span>Sound transmission analysis of partially treated MR <span class="hlt">fluid-based</span> sandwich panels using finite element method</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hemmatian, M.; Sedaghati, R.</p> <p>2017-04-01</p> <p>This study aims at developing a finite element <span class="hlt">model</span> to predict the sound transmission loss (STL) of a multilayer panel partially treated with a Magnetorheological (MR) <span class="hlt">fluid</span> core layer. MR <span class="hlt">fluids</span> are smart materials with promising controllable rheological characteristics in which the application of an external magnetic field instantly changes their rheological properties. Partial treatment of sandwich panels with MR <span class="hlt">fluid</span> core layer provides an opportunity to change stiffness and damping of the structure without significantly increasing the mass. The STL of a finite sandwich panel partially treated with MR <span class="hlt">fluid</span> is <span class="hlt">modeled</span> using the finite element (FE) method. Circular sandwich panels with clamped boundary condition and elastic face sheets in which the core layer is segmented circumferentially is considered. The MR <span class="hlt">fluid</span> core layer is considered as a viscoelastic material with complex shear modulus with the magnetic field and frequency dependent storage and loss moduli. Neglecting the effect of the panel's vibration on the pressure forcing function, the work done by the acoustic pressure is expressed as a function of the blocked pressure in order to calculate the force vector in the equation of the motion of the panel. The governing finite element equation of motion of the MR sandwich panel is then developed to predict the transverse vibration of the panel which can then be utilized to obtain the radiated sound using Green's function. The developed <span class="hlt">model</span> is used to conduct a systematic parametric study on the effect of different locations of MR <span class="hlt">fluid</span> treatment on the natural frequencies and the STL.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22660755-corresponding-states-behavior-ionic-model-fluid-variable-dispersion-interactions','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22660755-corresponding-states-behavior-ionic-model-fluid-variable-dispersion-interactions"><span>Corresponding-states behavior of an ionic <span class="hlt">model</span> <span class="hlt">fluid</span> with variable dispersion interactions</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>Weiss, Volker C., E-mail: volker.weiss@bccms.uni-bremen.de</p> <p>2016-06-21</p> <p>Guggenheim’s corresponding-states approach for simple <span class="hlt">fluids</span> leads to a remarkably universal representation of their thermophysical properties. For more complex <span class="hlt">fluids</span>, such as polar or ionic ones, deviations from this type of behavior are to be expected, thereby supplying us with valuable information about the thermodynamic consequences of the interaction details in <span class="hlt">fluids</span>. Here, the gradual transition of a simple <span class="hlt">fluid</span> to an ionic one is studied by varying the relative strength of the dispersion interactions compared to the electrostatic interactions among the charged particles. In addition to the effects on the reduced surface tension that were reported earlier [F. Leroymore » and V. C. Weiss, J. Chem. Phys. 134, 094703 (2011)], we address the shape of the coexistence curve and focus on properties that are related to and derived from the vapor pressure. These quantities include the enthalpy and entropy of vaporization, the boiling point, and the critical compressibility factor Z{sub c}. For all of these properties, the crossover from simple to characteristically ionic <span class="hlt">fluid</span> is seen once the dispersive attraction drops below 20%–40% of the electrostatic attraction (as measured for two particles at contact). Below this threshold, ionic <span class="hlt">fluids</span> display characteristically low values of Z{sub c} as well as large Guggenheim and Guldberg ratios for the reduced enthalpy of vaporization and the reduced boiling point, respectively. The coexistence curves are wider and more skewed than those for simple <span class="hlt">fluids</span>. The results for the ionic <span class="hlt">model</span> <span class="hlt">fluid</span> with variable dispersion interactions improve our understanding of the behavior of real ionic <span class="hlt">fluids</span>, such as inorganic molten salts and room temperature ionic liquids, by gauging the importance of different types of interactions for thermodynamic properties.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22617042-large-deviations-stochastic-models-two-dimensional-second-grade-fluids','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22617042-large-deviations-stochastic-models-two-dimensional-second-grade-fluids"><span>Large Deviations for Stochastic <span class="hlt">Models</span> of Two-Dimensional Second Grade <span class="hlt">Fluids</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>Zhai, Jianliang, E-mail: zhaijl@ustc.edu.cn; Zhang, Tusheng, E-mail: Tusheng.Zhang@manchester.ac.uk</p> <p>2017-06-15</p> <p>In this paper, we establish a large deviation principle for stochastic <span class="hlt">models</span> of incompressible second grade <span class="hlt">fluids</span>. The weak convergence method introduced by Budhiraja and Dupuis (Probab Math Statist 20:39–61, 2000) plays an important role.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JNET...43..185A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JNET...43..185A"><span>A Thermodynamically Consistent Approach to Phase-Separating Viscous <span class="hlt">Fluids</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Anders, Denis; Weinberg, Kerstin</p> <p>2018-04-01</p> <p>The de-mixing properties of heterogeneous viscous <span class="hlt">fluids</span> are determined by an interplay of diffusion, surface tension and a superposed velocity field. In this contribution a variational <span class="hlt">model</span> of the decomposition, <span class="hlt">based</span> on the Navier-Stokes equations for incompressible laminar flow and the extended Korteweg-Cahn-Hilliard equations, is formulated. An exemplary numerical simulation using C1-continuous finite elements demonstrates the capability of this <span class="hlt">model</span> to compute phase decomposition and coarsening of the moving <span class="hlt">fluid</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20170008954','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20170008954"><span>Numerical <span class="hlt">Modeling</span> of an Integrated Vehicle <span class="hlt">Fluids</span> System Loop for Pressurizing a Cryogenic Tank</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>LeClair, A. C.; Hedayat, A.; Majumdar, A. K.</p> <p>2017-01-01</p> <p>This paper presents a numerical <span class="hlt">model</span> of the pressurization loop of the Integrated Vehicle <span class="hlt">Fluids</span> (IVF) system using the Generalized <span class="hlt">Fluid</span> System Simulation Program (GFSSP). The IVF propulsion system, being developed by United Launch Alliance to reduce system weight and enhance reliability, uses boiloff propellants to drive thrusters for the reaction control system as well as to run internal combustion engines to develop power and drive compressors to pressurize propellant tanks. NASA Marshall Space Flight Center (MSFC) conducted tests to verify the functioning of the IVF system using a flight-like tank. GFSSP, a finite volume <span class="hlt">based</span> flow network analysis software developed at MSFC, has been used to support the test program. This paper presents the simulation of three different test series, comparison of numerical prediction and test data and a novel method of presenting data in a dimensionless form. The paper also presents a methodology of implementing a compressor map in a system level code.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29388421','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29388421"><span>Electrorheological <span class="hlt">Fluids</span> with High Shear Stress <span class="hlt">Based</span> on Wrinkly Tin Titanyl Oxalate.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Wu, Jinghua; Zhang, Lei; Xin, Xing; Zhang, Yang; Wang, Hui; Sun, Aihua; Cheng, Yuchuan; Chen, Xinde; Xu, Gaojie</p> <p>2018-02-21</p> <p>Electrorheological (ER) <span class="hlt">fluids</span> are considered as a type of smart <span class="hlt">fluids</span> because their rheological characteristics can be altered through an electric field. The discovery of giant ER effect revived the researchers' interest in the ER technological area. However, the poor stability including the insufficient dynamic shear stress, the large leakage current density, and the sedimentation tendency still hinders their practical applications. Herein, we report a facile and scalable coprecipitation method for synthesizing surfactant-free tin titanyl oxalate (TTO) particles with tremella-like wrinkly microstructure (W-TTO). The W-TTO-<span class="hlt">based</span> ER <span class="hlt">fluids</span> exhibit enhanced ER activity compared to that of the pristine TTO because of the improved wettability between W-TTO and the silicone oil. In addition, the static yield stress and leakage current of W-TTO ER <span class="hlt">fluids</span> also show a fine time stability during the 30 day tests. More importantly, the dynamic shear stress of W-TTO ER <span class="hlt">fluids</span> can remain stable throughout the shear rate range, which is valuable for their use in engineering applications. The results in this work provided a promising strategy to solving the long-standing problem of ER <span class="hlt">fluid</span> stability. Moreover, this convenient route of synthesis may be considered a green approach for the mass production of giant ER materials.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20050203838&hterms=Cardiovascular&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D60%26Ntt%3DCardiovascular','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20050203838&hterms=Cardiovascular&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D60%26Ntt%3DCardiovascular"><span>MRI-<span class="hlt">Based</span> Computational <span class="hlt">Fluid</span> Dynamics in Experimental Vascular <span class="hlt">Models</span>: Toward the Development of an Approach for Prediction of Cardiovascular Changes During Prolonged Space Missions</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Spirka, T. A.; Myers, J. G.; Setser, R. M.; Halliburton, S. S.; White, R. D.; Chatzimavroudis, G. P.</p> <p>2005-01-01</p> <p>A priority of NASA is to identify and study possible risks to astronauts health during prolonged space missions [l]. The goal is to develop a procedure for a preflight evaluation of the cardiovascular system of an astronaut and to forecast how it will be affected during the mission. To predict these changes, a computational cardiovascular <span class="hlt">model</span> must be constructed. Although physiology data can be used to make a general <span class="hlt">model</span>, a more desirable subject-specific <span class="hlt">model</span> requires anatomical, functional, and flow data from the specific astronaut. MRI has the unique advantage of providing images with all of the above information, including three-directional velocity data which can be used as boundary conditions in a computational <span class="hlt">fluid</span> dynamics (CFD) program [2,3]. MRI-<span class="hlt">based</span> CFD is very promising for reproduction of the flow patterns of a specific subject and prediction of changes in the absence of gravity. The aim of this study was to test the feasibility of this approach by reconstructing the geometry of MRI-scanned arterial <span class="hlt">models</span> and reproducing the MRI-measured velocities using CFD simulations on these geometries.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1991Ap%26SS.181...61R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1991Ap%26SS.181...61R"><span>Inhomogeneous generalizations of Bianchi type VIh <span class="hlt">models</span> with perfect <span class="hlt">fluid</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Roy, S. R.; Prasad, A.</p> <p>1991-07-01</p> <p>Inhomogeneous universes admitting an Abelian G2 of isometry and filled with perfect <span class="hlt">fluid</span> have been derived. These contain as special cases exact homogeneous universes of Bianchi type VIh. Many of these universes asymptotically tend to homogeneous Bianchi VIh universes. The <span class="hlt">models</span> have been discussed for their physical and kinematical behaviors.</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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