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Journal articles on the topic 'Viscoelstic model for binary systems'

Author: Grafiati

Published: 11 March 2023

Last updated: 31 July 2025

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1

Song, Han-Feng, Run-Qian Huang, and Shao-Lan Bi. "A Model for Contact Binary Systems." Chinese Journal of Astronomy and Astrophysics 7, no. 4 (2007): 539–50. http://dx.doi.org/10.1088/1009-9271/7/4/10.

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2

Hale, Barbara N., and Gerald Wilemski. "A scaled nucleation model for ideal binary systems." Chemical Physics Letters 305, no. 3-4 (1999): 263–68. http://dx.doi.org/10.1016/s0009-2614(99)00365-6.

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3

MÜNSTER, GERNOT. "INTERFACE TENSIONS OF BINARY SYSTEMS." International Journal of Modern Physics C 03, no. 05 (1992): 879–87. http://dx.doi.org/10.1142/s0129183192000543.

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In liquid mixtures or analogous binary systems at low temperatures the pure phases may coexist, separated by an interface. The interface tension vanishes according to σ=σ0(1−T/Tc)µ as the temperature T approaches the critical point from below. Similarly the correlation length diverges as ξ=ξ0(T/Tc−1)−ν. For three-dimensional systems the dimensionless product R=σ0(ξ0)2 is universal. This and related universal quantities are investigated by means of a semiclassical expansion in the framework of Φ4 theory, as well as by Monte Carlo calculations in the three-dimensional Ising model.

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4

Retter, Alon, Alexander Liu, and Marc Bos. "Precessing accretion discs in binary systems." International Astronomical Union Colloquium 193 (2004): 391–94. http://dx.doi.org/10.1017/s0252921100011003.

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AbstractSuperhumps – quasi-periodic oscillations at periods a few percent different than the orbital periods – have been observed in several dozen binary systems of various types. It is well-accepted now that they are caused by the precession of the accretion disc. New findings on TV Col, TX Col and V4742 Sgr are presented. These cataclysmic variables (CVs) have exceptional precessing periods that cast strong doubt on the predictions of the Tidal Disc Instability model.

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5

Fei, Xinyu, Lucas T. Brady, Jeffrey Larson, Sven Leyffer, and Siqian Shen. "Binary Control Pulse Optimization for Quantum Systems." Quantum 7 (January 4, 2023): 892. http://dx.doi.org/10.22331/q-2023-01-04-892.

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Quantum control aims to manipulate quantum systems toward specific quantum states or desired operations. Designing highly accurate and effective control steps is vitally important to various quantum applications, including energy minimization and circuit compilation. In this paper we focus on discrete binary quantum control problems and apply different optimization algorithms and techniques to improve computational efficiency and solution quality. Specifically, we develop a generic model and extend it in several ways. We introduce a squared L2-penalty function to handle additional side constra

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6

Romero-Serrano, Antonio, and Arthur D. Pelton. "Extensions of a structural model for binary silicate systems." Metallurgical and Materials Transactions B 26, no. 2 (1995): 305–15. http://dx.doi.org/10.1007/bf02660973.

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7

Sweatman, W. L. "Full Ionisation in Binary-Binary Scattering." Proceedings of the International Astronomical Union 3, S246 (2007): 233–34. http://dx.doi.org/10.1017/s1743921308015652.

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AbstractEncounters between binary stars and single stars and between binary stars and other binary stars play a key role in the dynamics of dense stellar systems. In the simple model, in which stars are approximated by point masses, a number of theoretical and numerical results are known. In particular there exist relationships to help to describe the destruction process of binary stars (ionisation) through three-body encounters between binary and single stars. Here we extend these results to the four-body case involving encounters between pairs of binary stars that lead to a disruption of the

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8

Jardine, M., H. R. Allen, and A. M. T. Pollock. "Magnetic annihilation in colliding-wind binary systems." Symposium - International Astronomical Union 163 (1995): 523–24. http://dx.doi.org/10.1017/s0074180900202611.

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We investigate the possibility that a stagnation-point magnetic reconnection model may account for the particle acceleration necessary for the generation of nonthermal radio emission in the Wolf-Rayet binary systems exemplified by WR140.

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9

Kenoly, Lailani, A. Ken Luu, Celia Toral, et al. "Understanding Binary Systems—a Comparison between COSMIC and MESA." Research Notes of the AAS 7, no. 8 (2023): 167. http://dx.doi.org/10.3847/2515-5172/aced00.

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Abstract We compare the evolution of binary systems evolved in the MESA stellar evolution code to those in the COSMIC population synthesis code. Our aim is to convey the robustness of the equations that model binary evolution in the COSMIC code, particularly for the cases of high mass stars with closely orbiting compact object companions. Our larger goal is to accurately model the rates of these systems, as they are promising candidates for the progenitor systems behind energetic, longer lasting, radio bright GRB jets. These systems also may be key contributors to the rates of binary black hol

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10

Nekrasov, A. D., S. B. Popov, and V. V. Zhuravlev. "Planet migration in accretion discs in binary systems." Proceedings of the International Astronomical Union 17, S370 (2021): 285–86. http://dx.doi.org/10.1017/s174392132200388x.

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AbstractWe model evolution of exoplanets of S-type in close binary systems at the stage when the companion starts to lose mass via a slow stellar wind. At this stage an accretion disc is formed around the planets’ host. Detailed structure of such discs is calculated in quasi-stationary and non-stationary approaches. We model migration of planets embedded in these discs.

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11

Novik, Keir E., and Peter V. Coveney. "Using Dissipative Particle Dynamics to Model Binary Immiscible Fluids." International Journal of Modern Physics C 08, no. 04 (1997): 909–18. http://dx.doi.org/10.1142/s0129183197000783.

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We investigate the domain growth and phase separation of two-dimensional binary immiscible fluid systems using dissipative particle dynamics. Our results are compared with similar simulations using other techniques, and we conclude that dissipative particle dynamics is a promising method for simulating these systems.

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12

Desai, Malina, Juan Diego Draxl Giannoni, Camille Dunning, et al. "Identifying Ultracool Binary Systems using Machine Learning Methods." Research Notes of the AAS 7, no. 1 (2023): 13. http://dx.doi.org/10.3847/2515-5172/acb54a.

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Abstract Ultracool spectral binaries are unresolved pairs of low-mass stars and brown dwarfs revealed by peculiarities in their combined light spectra. Methods to identify these systems have relied on spectral indices, which have known selection biases. We report on a pilot study examining the application of machine learning methods to identify ultracool spectral binaries. Using a sample of single and binary templates constructed from low-resolution, near-infrared spectra, we trained a random forest model to identify binaries composed of M7–L7 primaries and T1–T8 secondaries. We find that unif

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13

Lin, Chih-Chen, Leo Mark, Timos Sellis, and Christos Faloutsos. "Performance issues in the binary relationship model." Data & Knowledge Engineering 4, no. 3 (1989): 195–221. http://dx.doi.org/10.1016/0169-023x(89)90020-7.

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14

ROOS, W. D., G. J. OLIVIER, and J. J. TERBLANS. "ESTIMATING THE SEGREGATION ENERGIES IN Cu BINARY SYSTEMS." Surface Review and Letters 14, no. 04 (2007): 677–80. http://dx.doi.org/10.1142/s0218625x07010068.

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The segregation energy of diluted species in a matrix can be calculated by first principles. These calculations are generally very computational demanding. The existing empirical models which use the difference in surface tensions to predict the segregation energy are limited, because they do not take the surface orientation of the matrix into account. In this investigation a model was developed which can estimate the segregation energies of segregating species in a binary system. The model makes use of the sublimation energies and takes the orientation of the surface into account. The model s

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15

Rafizadeh, Hamid A. "Mechanical and structural properties of metallic glasses." Canadian Journal of Physics 68, no. 1 (1990): 23–33. http://dx.doi.org/10.1139/p90-004.

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A simple linear-chain model is utilized in calculation of the mechanical and structural properties of metallic glasses. The model calculations of composition-dependent elastic constants show good agreement with the experimental data available for binary metallic glasses. The model is capable of distinguishing different structural characteristics of glassy systems and provides excellent agreement with the radial distribution functions of amorphous cobalt, metal–metalloid, and binary transition metal glasses. The model is not limited to binary systems and can be readily applied to ternary and hi

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16

Rebollo Paz, Maria Berta, Adrian Hugo Buep, and Maximo Baron. "Dielectric properties of binary systems 8. Improved model for alcohol/non polar systems." Journal of Molecular Liquids 38, no. 3-4 (1988): 225–32. http://dx.doi.org/10.1016/0167-7322(88)80020-5.

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17

Radovic, Ivona, Nikola Grozdanic, Bojan Djordjevic, Slobodan Serbanovic, and Mirjana Kijevcanin. "Prediction of excess molar volumes of binary mixtures by Prigogine-Flory-Patterson (PFP) and extended real association solution (ERAS) models." Journal of the Serbian Chemical Society 82, no. 12 (2017): 1379–90. http://dx.doi.org/10.2298/jsc170817103r.

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In this paper, the Prigogine?Flory?Patterson (PFP) theoretical model and the extended real association solution (ERAS) model for the prediction of the excess molar volumes of 17 binary sets of alcohols (methanol, ethanol, propan-1-ol, butan-1-ol, butan-2-ol and pentan-1-ol) with benzene, chlorobenzene, acetonitrile, hexan-1-amine and n-heptane were tested at 298.15 K and atmospheric pressure. The binary sets contained 333 experimental data points for 11 different compounds. The ERAS model demonstrated better correlative characteristics for binary mixtures comparing to PFP model. The ERAS model

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18

Tiwari, Asim, and Brahma Deo. "Cell Model for Calculation of Activities in Binary Oxide Systems." ISIJ International 35, no. 9 (1995): 1141–44. http://dx.doi.org/10.2355/isijinternational.35.1141.

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19

Prochaska, Krystyna. "ADSORPTION OF EXTRACTANTS AND MODIFIERS IN MIXED BINARY MODEL SYSTEMS." Solvent Extraction and Ion Exchange 14, no. 6 (1996): 1057–75. http://dx.doi.org/10.1080/07366299608918382.

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20

Forster, Robert J., and Larry R. Faulkner. "Kinetic Separation of Faradaic Currents: Binary Monolayers as Model Systems." Analytical Chemistry 67, no. 7 (1995): 1232–39. http://dx.doi.org/10.1021/ac00103a014.

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21

Davis, Michael I. "Four-segment composition model analyses of binary alkanol—water systems." Thermochimica Acta 90 (August 1985): 313–29. http://dx.doi.org/10.1016/0040-6031(85)87109-4.

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22

Davis, Michael I. "Tests of the four-segment model for binary hydroorganic systems." Thermochimica Acta 89 (July 1985): 325–33. http://dx.doi.org/10.1016/0040-6031(85)85505-2.

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23

Haghtalab, Ali, and Marzieh Joda. "Gex-Model Using Local Area Fraction for Binary Electrolyte Systems." International Journal of Thermophysics 28, no. 3 (2007): 876–90. http://dx.doi.org/10.1007/s10765-007-0211-1.

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24

Al-Wardat, M. A. "Model atmosphere parameters of the binary systems COU1289 and COU1291." Astronomische Nachrichten 328, no. 1 (2007): 63–67. http://dx.doi.org/10.1002/asna.200510676.

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25

Lunácek, J. "Application of the Thermodynamic Solution Model of Dilute Binary Systems." physica status solidi (a) 163, no. 2 (1997): 369–75. http://dx.doi.org/10.1002/1521-396x(199710)163:2<369::aid-pssa369>3.0.co;2-6.

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26

Luňáček, J. "Application of the Thermodynamic Solution Model of Dilute Binary Systems." physica status solidi (a) 164, no. 2 (1997): 665–72. http://dx.doi.org/10.1002/1521-396x(199712)164:2<665::aid-pssa665>3.0.co;2-7.

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27

Kamali, Mohamad Javad, Zakarya Kamali, and Gholamhossein Vatankhah. "Thermodynamic Modeling of Surface Tension of Aqueous Electrolyte Solution by Competitive Adsorption Model." Journal of Thermodynamics 2015 (November 2, 2015): 1–8. http://dx.doi.org/10.1155/2015/319704.

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Thermodynamic modeling of surface tension of different electrolyte systems in presence of gas phase is studied. Using the solid-liquid equilibrium, Langmuir gas-solid adsorption, and ENRTL activity coefficient model, the surface tension of electrolyte solutions is calculated. The new model has two adjustable parameters which could be determined by fitting the experimental surface tension of binary aqueous electrolyte solution in single temperature. Then the values of surface tension for other temperatures in binary and ternary system of aqueous electrolyte solution are predicted. The average a

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28

Franchini, Alessia, Rebecca G. Martin, and Stephen H. Lubow. "Multiplanet disc interactions in binary systems." Monthly Notices of the Royal Astronomical Society 491, no. 4 (2019): 5351–60. http://dx.doi.org/10.1093/mnras/stz3175.

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ABSTRACT We investigate the evolution of a multiplanet–disc system orbiting one component of a binary star system. The planet–disc system is initially coplanar but misaligned to the binary orbital plane. The planets are assumed to be giants that open gaps in the disc. We first study the role of the disc in shaping the mutual evolution of the two planets using a secular model for low initial tilt. In general, we find that the planets and the disc do not remain coplanar, in agreement with previous work on the single planet case. Instead, the planets and the disc undergo tilt oscillations. A high

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29

Wang, Yanhan. "Research on Binary Black Hole Systems by Analysis of Gravitational Waves." Highlights in Science, Engineering and Technology 104 (June 11, 2024): 47–53. http://dx.doi.org/10.54097/ys7j9d73.

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The mass ratio, effective spin, and chirp mass are three important properties to describe the binary systems of black holes. The gravitational wave sources can be a breakthrough in the investigation of black holes. The formation of black holes is a significant problem to solve as the electromagnetic waves (light) cannot escape from the black hole, and the gravitational waves can be emitted when the binary systems of black holes or neutron stars merge. Based on the detection of gravitational waves, the process of the formation of black holes can be traced and studied in the binary black holes a

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30

Eggl, Siegfried, Nikolaos Georgakarakos, and Elke Pilat-Lohinger. "Dynamics and Habitability in Binary Star Systems." Proceedings of the International Astronomical Union 9, S310 (2014): 53–57. http://dx.doi.org/10.1017/s1743921314007820.

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AbstractDetermining planetary habitability is a complex matter, as the interplay between a planet's physical and atmospheric properties with stellar insolation has to be studied in a self consistent manner. Standardized atmospheric models for Earth-like planets exist and are commonly accepted as a reference for estimates of Habitable Zones. In order to define Habitable Zone boundaries, circular orbital configurations around main sequence stars are generally assumed. In gravitationally interacting multibody systems, such as double stars, however, planetary orbits are forcibly becoming non circu

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31

Lei, Yuqing, and Alec Solway. "Conflict and competition between model-based and model-free control." PLOS Computational Biology 18, no. 5 (2022): e1010047. http://dx.doi.org/10.1371/journal.pcbi.1010047.

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A large literature has accumulated suggesting that human and animal decision making is driven by at least two systems, and that important functions of these systems can be captured by reinforcement learning algorithms. The “model-free” system caches and uses stimulus–value or stimulus–response associations, and the “model-based” system implements more flexible planning using a model of the world. However, it is not clear how the two systems interact during deliberation and how a single decision emerges from this process, especially when they disagree. Most previous work has assumed that while

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32

Fullard, Andrew G., John T. O’Brien, Wolfgang E. Kerzendorf, et al. "New Mass Estimates for Massive Binary Systems: A Probabilistic Approach Using Polarimetric Radiative Transfer." Astrophysical Journal 930, no. 1 (2022): 89. http://dx.doi.org/10.3847/1538-4357/ac589e.

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Abstract Understanding the evolution of massive binary stars requires accurate estimates of their masses. This understanding is critically important because massive star evolution can potentially lead to gravitational-wave sources such as binary black holes or neutron stars. For Wolf–Rayet (WR) stars with optically thick stellar winds, their masses can only be determined with accurate inclination angle estimates from binary systems which have spectroscopic M sin i measurements. Orbitally phased polarization signals can encode the inclination angle of binary systems, where the WR winds act as s

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33

Koenigsberger, Gloria, Edmundo Moreno, Jorge Cantó, and Alejandro C. Raga. "Binary interaction effects: predictions and observations." Symposium - International Astronomical Union 193 (1999): 38–46. http://dx.doi.org/10.1017/s0074180900204907.

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Observations and predictions of interactions in close and massive binary systems are summarized. Tidal interactions are analyzed using a model which predicts the response of the stellar surface to the external gravitational force of the companion. The possible role of tidal interactions in determining the peculiar behavior of systems like HD 5980 and η Carinae is discussed.

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34

Mark, Leo. "Defining views in the Binary Relationship Model." Information Systems 12, no. 3 (1987): 281–94. http://dx.doi.org/10.1016/0306-4379(87)90006-8.

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35

Zander, Roland, Michael Dittmann, and Gerhard M. Schneider. "Dissipative Structures in Demixing Binary Liquid Systems." Zeitschrift für Naturforschung A 45, no. 11-12 (1990): 1309–16. http://dx.doi.org/10.1515/zna-1990-11-1213.

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AbstractThe demixing of a horizontal fluid layer of far-critical composition in the presence of a vertical temperature gradient can cause the formation of dissipative structures and thereby lead to a regular distribution of the precipitate. The occurrence of these convective structures is explained with the model of a Rayleigh-Benard instability (RBI) which is driven by parallel gradients of temperature and concentration. The distribution of the precipitate is a synergetic effect of the macroscopic convective pattern and the local action of the Marangoni flow at the surfaces of the drops. If b

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36

Avitan, Matan, Elena V. Ravve, and Zeev Volkovich. "Assembly Function Recognition in Embedded Systems as an Optimization Problem." Mathematics 12, no. 5 (2024): 658. http://dx.doi.org/10.3390/math12050658.

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Many different aspects of software system development and verification rely on precise function identification in binary code. Recognition of the source Assembly functions in embedded systems is one of the fundamental challenges in binary program analysis. While numerous approaches assume that the functions are given a priori, correct identification of the functions in binaries remains a great issue. This contribution addresses the problem of uncertainty in binary code in identification of functions, which were optimized during compilation. This paper investigates the difference between debug

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37

Miszuda, A., W. Szewczuk та J. Daszyńska-Daszkiewicz. "The eclipsing binary systems with δ Scuti component – I. KIC 10661783". Monthly Notices of the Royal Astronomical Society 505, № 3 (2021): 3206–18. http://dx.doi.org/10.1093/mnras/stab1597.

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ABSTRACT We present a comprehensive study of the eclipsing binary system KIC 10661783. The analysis of the whole Kepler light curve, corrected for the binary effects, reveals a rich oscillation spectrum with 590 significant frequency peaks, 207 of which are independent. In addition to typical δ Scuti (δ Sct) frequencies, we find small-amplitude signals in the low-frequency range that, most probably, are a manifestation of gravity-mode pulsations. We perform binary-evolution computations for this system in order to find an acceptable model describing its current stage. Our models show that the

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38

Hennicker, L., N. D. Kee, T. Shenar, et al. "BOSS-3D: A Binary Object Spectral Synthesis Code in 3D." Proceedings of the International Astronomical Union 16, S366 (2020): 138–43. http://dx.doi.org/10.1017/s174392132200062x.

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AbstractTo decode the information stored within a spectrum, detailed modelling of the physical state is required together with accurate radiative transfer solution schemes. In the analysis of stellar spectra, the numerical model often needs to account for high velocity outflows, multi-dimensional structures, and the effects of binary companions. Focusing now on binary systems, we present the BOSS-3D spectral synthesis code, which is capable of calculating synthetic line profiles for a variety of binary systems. Assuming the state of the circumstellar material to be known, the standard pz-geome

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39

Olsson, Henrik, and Leo Poom. "The Noisy Cue Abstraction Model is Equivalent to the Multiplicative Prototype Model." Perceptual and Motor Skills 100, no. 3 (2005): 819–20. http://dx.doi.org/10.2466/pms.100.3.819-820.

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40

Cheng, Lihong, Lei Feng, and Zhiwu Li. "Model abstraction for discrete-event systems by binary linear programming with applications to manufacturing systems." Science Progress 104, no. 3 (2021): 003685042110308. http://dx.doi.org/10.1177/00368504211030833.

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Model abstraction for finite state automata is helpful for decreasing computational complexity and improving comprehensibility for the verification and control synthesis of discrete-event systems (DES). Supremal quasi-congruence equivalence is an effective method for reducing the state space of DES and its effective algorithms based on graph theory have been developed. In this paper, a new method is proposed to convert the supremal quasi-congruence computation into a binary linear programming problem which can be solved by many powerful integer linear programming and satisfiability (SAT) solve

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41

Tejeda, Emilio, and Jesús A. Toalá. "Geometric Correction for Wind Accretion in Binary Systems." Astrophysical Journal 980, no. 2 (2025): 226. https://doi.org/10.3847/1538-4357/ada953.

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Abstract The Bondi–Hoyle–Lyttleton (BHL) accretion model is widely used to describe how a compact object accretes material from a companion's stellar wind in binary systems. However, its standard implementation becomes inaccurate when the wind velocity (v w) is comparable to or less than the orbital velocity (v o), predicting nonphysical accretion efficiencies above unity. This limits its applicability to systems with low wind-to-orbital velocity ratios (w = v w/v o ≤ 1), such as symbiotic systems. We revisit the implementation of the BHL model and introduce a geometric correction factor that

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42

Manouan, Wedjers Max Robin, Daouda Karidioula, Edouard Koffi Kouassi, Patrick Kouame Aquoi, and David Boa. "Estimation of the Thermodynamic Properties of Mixing Binary Systems Based on Silver Nitrate and Alkali Nitrates using Ionic Model." International Journal of Chemical and Process Engineering Research 9, no. 1 (2022): 56–67. http://dx.doi.org/10.18488/65.v9i1.3202.

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This work was devoted to the formulation of thermodynamic properties of binary systems of molten salts by using an ionic model which requires three physical parameters for each salt : the crystal lattice energy, the latent heat of melting and the sum of the ionic radii. This formulation, whose adjustable parameters have been obtained by smoothing from the experimental mixing properties available in the literature, allowed us to calculate the molar enthalpies of mixing for twelve (12) binary systems of alkali nitrate and silver nitrate. The different results obtained show satisfactory general a

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43

Wróbel, Marek, and Andriy Burbelko. "A Diffusion Model of Binary Systems Controlled by Chemical Potential Gradient." Journal of Casting & Materials Engineering 6, no. 2 (2022): 39–44. http://dx.doi.org/10.7494/jcme.2022.6.2.39.

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The paper presents a model of diffusion in a single phase with chemical potential gradient as the driving force of the process. Fick’s laws are strictly empirical and the assumption that the concentration gradients are the driving forces of diffusion is far from precise. Instead, the gradient of chemical potential μi of component i is the real driving force. The matter of governing equations of models that incorporate this approach will be raised and discussed in this article. One of more important features is the ability to acquire results where diffusion against the concentration gradient ma

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44

Parkin, E. R., and J. M. Pittard. "A 3D dynamical model of the colliding winds in binary systems." Monthly Notices of the Royal Astronomical Society 388, no. 3 (2008): 1047–61. http://dx.doi.org/10.1111/j.1365-2966.2008.13511.x.

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45

Zhou, Mi, Xigang Yuan, Yahui Zhang, and K. T. Yu. "Local Composition Based Maxwell–Stefan Diffusivity Model for Binary Liquid Systems." Industrial & Engineering Chemistry Research 52, no. 31 (2013): 10845–52. http://dx.doi.org/10.1021/ie4010157.

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46

Salvador, J. R., T. Alamo, D. R. Ramirez, and D. Muñoz de la Peña. "Model predictive control of partially fading memory systems with binary inputs." Journal of Process Control 64 (April 2018): 141–51. http://dx.doi.org/10.1016/j.jprocont.2018.02.006.

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47

Ferrari, Fabio, Michèle Lavagna, and Kathleen C. Howell. "Dynamical model of binary asteroid systems through patched three-body problems." Celestial Mechanics and Dynamical Astronomy 125, no. 4 (2016): 413–33. http://dx.doi.org/10.1007/s10569-016-9688-x.

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48

Laaksonen, Ari, and Markku Kulmala. "An explicit cluster model for binary nuclei in water–alcohol systems." Journal of Chemical Physics 95, no. 9 (1991): 6745–48. http://dx.doi.org/10.1063/1.461513.

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49

Kuus, M., H. Kirss, E. Siimer, and L. Kudryavtseva. "APPLICATION OF THE UNIFAC MODEL TO BINARY SYSTEMS CONTAINING AROMA COMPOUNDS." Proceedings of the Estonian Academy of Sciences. Chemistry 41, no. 2 (1992): 62. http://dx.doi.org/10.3176/chem.1992.2.03.

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50

Khosroshahi, Elmira Fanaei, Amir Heydari, Behruz Mirzayi, and Amir Nasser Shamkhali. "A model to calculate concentration-dependent surface tension of binary systems." Fluid Phase Equilibria 423 (September 2016): 34–42. http://dx.doi.org/10.1016/j.fluid.2016.04.007.

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