Relevant bibliographies by topics / LES numerical simulations

Contents

  1. Journal articles
  2. Dissertations / Theses
  3. Books
  4. Book chapters
  5. Conference papers
  6. Reports

Academic literature on the topic 'LES numerical simulations'

Author: Grafiati
Published: 4 May 2024

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Journal articles on the topic "LES numerical simulations"

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Kitiashvili, I. N., A. G. Kosovichev, A. A. Wray, and N. N. Mansour. "Numerical simulations of magnetic structures." Proceedings of the International Astronomical Union 6, S273 (August 2010): 315–19. http://dx.doi.org/10.1017/s1743921311015444.

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AbstractWe use 3D radiative MHD simulations of the upper turbulent convection layer for investigation of physical mechanisms of formation of magnetic structures on the Sun. The simulations include all essential physical processes, and are based of the LES (Large-Eddy Simulations) approach for describing the sub-grid scale turbulence. The simulation domain covers the top layer of the convection zone and the lower atmosphere. The results reveal a process of spontaneous formation of stable magnetic structures from an initially weak vertical magnetic field, uniformly distributed in the simulation domain. The process starts concentration of magnetic patches at the boundaries of granular cells, which are subsequently merged together into a stable large-scale structure by converging downdrafts below the surface. The resulting structure represents a compact concentration of strong magnetic field, reaching 6 kG in the interior. It has a cluster-like internal structurization, and is maintained by strong downdrafts extending into the deep layers.
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Zaussinger, F., and H. C. Spruit. "Semiconvection: numerical simulations." Astronomy & Astrophysics 554 (June 2013): A119. http://dx.doi.org/10.1051/0004-6361/201220573.

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CORCAU, Jenica-Ileana, and Liviu DINCA. "MATHEMATICAL MODEL AND NUMERICAL SIMULATIONS FOR PHOTOVOLTAIC PANELS." Review of the Air Force Academy 15, no. 3 (December 14, 2017): 47–56. http://dx.doi.org/10.19062/1842-9238.2017.15.3.5.

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Kik, Tomasz, Marek Slovacek, Jaromir Moravec, and Mojmir Vanek. "Numerical Simulations of Heat Treatment Processes." Applied Mechanics and Materials 809-810 (November 2015): 799–804. http://dx.doi.org/10.4028/www.scientific.net/amm.809-810.799.

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Welding and heat treatment are a modern, high efficient production technologies. During last few years requirements for quality of the welded joints have been constantly increasing in all production areas. Unfortunately, this approach increases the cost of production due to demand of intense experimental or prototype work prior the use of technology to make a final product. Preliminary experiments have to take into account proper chose of welding technology, materials, welding parameters, clamping and final optimization the welding conditions. All of these activities can be supported or even replaced by numerical simulations based on finite elements method. Tremendous advance in field of numerical simulation, facilitates very high correlation of simulation and experimental results bringing this new approach to common use. This paper highlight to usefulness of numerical simulation in heat treatment of bulk materials in various production stages. It was shown that it is possible to predict formation of metallurgical phases, hardness distribution, strains and stresses during and after quenching process. Simulations of different heating conditions and cooling media makes it possible to simulate processes such as heating, quenching, carburizing and nitriding.
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Demeio, Lucio, and James Paul Holloway. "Numerical simulations of BGK modes." Journal of Plasma Physics 46, no. 1 (August 1991): 63–84. http://dx.doi.org/10.1017/s0022377800015956.

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Solutions of the full nonlinear Vlasov–Poisson system for a one-dimensional unmagnetized plasma that correspond to undamped travelling waves near Maxwellian equilibria are analysed numerically using the splitting scheme algorithm. The numerical results are clearly in favour of the existence of such waves and confirm that there is a critical phase velocity below which they cannot be constructed.
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Komissarov, Serguei, and Oliver Porth. "Numerical simulations of jets." New Astronomy Reviews 92 (June 2021): 101610. http://dx.doi.org/10.1016/j.newar.2021.101610.

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Ramunigari, Naveen KumarG, and Debarshi Roy. "Numerical simulations of thrombosis." Chronicles of Young Scientists 4, no. 2 (2013): 130. http://dx.doi.org/10.4103/2229-5186.115552.

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Yasui, Kyuichi. "Numerical simulations for sonochemistry." Ultrasonics Sonochemistry 78 (October 2021): 105728. http://dx.doi.org/10.1016/j.ultsonch.2021.105728.

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Guillaume, F. "Numerical simulations and spectroscopy." École thématique de la Société Française de la Neutronique 12 (2011): 3–14. http://dx.doi.org/10.1051/sfn/201112002.

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Petit, S. "Numerical simulations and magnetism." École thématique de la Société Française de la Neutronique 12 (2011): 105–21. http://dx.doi.org/10.1051/sfn/201112006.

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Dissertations / Theses on the topic "LES numerical simulations"

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Öqvist, Mona. "Numerical simulations of wear." Licentiate thesis, Luleå tekniska universitet, 2000. http://urn.kb.se/resolve?urn=urn:nbn:se:ltu:diva-26185.

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The objective of this licentiate thesis was to study the effect of tool wear for sheet metal forming tools and how the wear process can be simulated in an efficient manner. Three Papers are appended to this licentiate thesis. Paper A covers the influence of tool geometry in deep drawing. In paper B is the way of calculating with finite element analysis described. The wear of a steel cylinder oscillating against a steel plate was studied experimentally. The worn shape of the cylinder was then compared with a numerical simulation of the shape. Paper C shows how numerical simulations can be used to simulate wear of deep drawing tools. The wear of two different deep drawing tools has been investigated. The shape of the tools before and after wear have been compared as well as the stresses and strains in the formed cups.
Godkänd; 2000; 20070317 (ysko)
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Gross, Richard Edward. "Numerical simulations of flux pinning." Thesis, University of Cambridge, 1996. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.243012.

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Demetriou, D. A. "Numerical simulations of interface kinetics." Thesis, University of Cambridge, 2000. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.598490.

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This dissertation's goal is concerned with the development and numerical study of a continuum model, that describes a variety of interface growth phenomena such as fluid displacement in porous media, crystal growth and flux-lines in type-II superconductors. The continuum model is the Quenched-Edwards-Wilkinson (QEW), which is well established in the literature and we restrict ourselves in providing a brief 'derivation' in terms of symmetry considerations. A crucial part of the model is the quenched random medium where the interface moves. The 'adequate' generation of the random background is a crucial ingredient of the simulations and we use a method first employed in fluid mechanics, but never before used in this field. Massive parallel simulations of the resulting system allowed us to verify the presence of a well defined depinning transition between a pinned and moving interface. This is characterized by the presence of a spatial system size (above a certain system size) independent threshold force. The transition appears to fit well the conjecture that the ensemble and time averaged centre of mass velocity, vcm, scales with the applied external driving force, F, according to vcm ~ ((F)/(F)c-1)θ where Fc is the threshold force and θ the velocity critical exponent. The velocity exponent is expected to be a 'universal' quantity independent of model parameters. Based on our work we estimate θ = 0.61 ± 0.06.
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McMillan, Paul. "Numerical simulations of galaxy interaction." Thesis, University of Leicester, 2006. http://hdl.handle.net/2381/433.

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Cosmological theories that include a non-baryonic dynamically cold dark matter (CDM) have been stunningly successful at explaining observations of the universe on large scales. On the scale of individual galaxies, however, observations have been made which call into question the CDM paradigm. In particular, simulations of structure formation show CDM haloes with a density “cusp”, such that in the centre of the halo d ln ρ/d ln r ~1 − 1.5. In contrast, observational studies suggest that CDM haloes have constant density cores. In this thesis I use gravitational N-body simulations to investigate the claim that the dark matter halo cusp can be removed by angular momentum transport from a rotating bar in a disc galaxy. I find that the simulations which were used to support this claim were seriously flawed, and similar simulations designed to mitigate these flaws suggest that this is unlikely to be a mechanism for turning a cusp into a core. In the interests of further work on dark matter haloes, and on other problems in astrophysics, I design and implement a new method for constructing model galaxies with halo, bulge, and disc components. This method avoids the use of an approximation to a Maxwellian velocity distribution. I show that this creates stable galaxy models, well suited to many applications. As an example of these applications, I conduct a thorough investigation of the structural and kinematic properties of the haloes of the remnants of 1:1 mass ratio mergers. I determine that the merger has virtually no effect on the halo cusp strength, but a substantial effect on the halo velocity distribution. The remnant haloes are significantly less spherical that those described in studies of mergers which consider gas cooling. Other properties of the remnants are noted and discussed.
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Pavlovski, G. "Numerical simulations of molecular turbulence." Thesis, Queen's University Belfast, 2004. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.403275.

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Grimshaw, L. "Numerical simulations of ellipsoidal galaxies." Thesis, University of Manchester, 1985. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.370414.

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Cox, Christopher Ian. "Numerical simulations of astrophysical jets." Thesis, University of Cambridge, 1990. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.335736.

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Clarke, Seamus. "Numerical simulations of filamentary clouds." Thesis, Cardiff University, 2016. http://orca.cf.ac.uk/100557/.

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Filamentary structures are observed to be common over a wide range of spatial scales and are strongly linked to star formation. In this thesis I present the results of a range of numerical simulations which investigate the stability, collapse and fragmentation of filaments. The global longitudinal collapse timescale for filaments is found to be considerably longer than for equally dense spheres, allowing sufficient time for local collapse to occur, and to solely occur via the distinctive end-dominated mode. A new freefall timescale equation for filaments is presented, as well as a semi-analytic model of longitudinal collapse. The fragmentation of accreting filaments is found to be more complicated than that of equilibrium filaments, and is dominated by the behaviour of longitudinal gravo-acoustic oscillations. This results in the fastest growing perturbation mode being independent of filament width. The non-equilibrium model presented here allows observers to estimate the age of a fragmenting filament and the mass accretion rate. Simulations of filaments accreting from a inhomogenous, turbulent medium show that turbulence has a large impact on the fragmentation of a filament. When the turbulence is sub-sonic, a filament fragments in a two-tiered hierarchical manner. As the energy in the turbulent field increases, the filament fragments into elongated fibre-like sub-structures. The formation of these fibre-like structures is intimately linked to the vorticity of the velocity field in the filament and the accretion onto the filament. In addition, I present synthetic C18O observations and show that the fibrelike sub-structures appear as velocity-coherent structures, well separated in velocity space, similar to the fibres observed by Hacar & Tafalla (2011).
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Wu, Wenwei. "Chemical reactions in turbulence : numerical studies through direct numerical simulations." Thesis, Littoral, 2021. http://www.theses.fr/2021DUNK0577.

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Le présent travail se concentre sur les propriétés statistiques des scalaires réactifs subissant des réactions chimiques réversibles en turbulence incompressible. Une analyse théorique des propriétés statistiques des scalaires à différents ordres de moments a été réalisée sur la base d'approximations et de modèles convenablement proposés. Les résultats théoriquement dérivés ont ensuite été comparés aux résultats numériques obtenus par simulation numérique directe (DNS). Dans la simulation numérique directe, les dérivés spatiales ont été principalement approximées en utilisant une méthode pseudi-spectrale, car la vitesse turbulente et les champs scalaires sont généralement des conditions aux limites périodiques. Pour les configurations spéciales dans lesquelles la condition aux limites n'est pas périodique, une méthode aux différences finies avec des schémas fins a été utilisée pour approximer les dérivées spatiales. L'intégration temporelle numérique a été mise en oeuvre par un schéma Runge-Kutta du troisième ordre. Tous les travaux menés dans cette thèse sont consacrés aux explorations numériques et théoriques des scalaires réactifs en turbulence incompressible de différentes configurations. Nos résultats suggèrent de nouvelles idées pour de futures études, qui sont discutées dans les conclusions
The present work focuses on the statistical properties of reactive scalars undergoing reversible chemical reactions in incompressible turbulence. Theoretical analysis about the statistical properties of scalars at different order of moments were carried out based on appropriately proposed approximations and models. The theoretically derived results were then compared with numerical results obtained by direct numerical simulation (DNS). In the direct numerical simulation, the spatial derivatives were mainly approximated by using a pseudo-spectral method, since the turbulent velocity and scalar fields are generally of periodic boundary conditions. For the special configurations in which the boundary condition is not periodic, a finite difference method with fine schemes was used to approximate the spatial derivatives. The numerical time integration was implemented by a third order Runge-Kutta scheme. All the works carried out in this thesis are devoted to the numerical and theoretical explorations about reactive scalars is incompressible turbulence of different configurations. Our finding suggest new ideas for future studies, which are discussed in the conclusions
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Wahba, Essam Moustafa. "Hierarchical formulations for numerical flow simulations /." For electronic version search Digital dissertations database. Restricted to UC campuses. Access is free to UC campus dissertations, 2004. http://uclibs.org/PID/11984.

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Books on the topic "LES numerical simulations"

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name, No. Numerical simulations of incompressible flows. Singapore: World Scientific, 2003.

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Gretar, Tryggvason, and United States. National Aeronautics and Space Administration., eds. Numerical simulations of drop collisions. [Washington, DC]: National Aeronautics and Space Administration, 1994.

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Tsang, Leung, Jin Au Kong, Kung-Hau Ding, and Chi On Ao. Scattering of Electromagnetic Waves: Numerical Simulations. New York, USA: John Wiley & Sons, Inc., 2001. http://dx.doi.org/10.1002/0471224308.

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Goldsmith, Roger A. Numerical simulations of Columbus' Atlantic crossings. Woods Hole, Mass: Woods Hole Oceanographic Institution, 1992.

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Idelsohn, Sergio R., ed. Numerical Simulations of Coupled Problems in Engineering. Cham: Springer International Publishing, 2014. http://dx.doi.org/10.1007/978-3-319-06136-8.

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Bramble, James H., Albert Cohen, and Wolfgang Dahmen. Multiscale Problems and Methods in Numerical Simulations. Edited by Claudio Canuto. Berlin, Heidelberg: Springer Berlin Heidelberg, 2003. http://dx.doi.org/10.1007/b13466.

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E, Krist Steven, Hussaini M. Yousuff, and Langley Research Center, eds. Resolution requirements for numerical simulations of transition. Hampton, Va: National Aeronautics and Space Administration, Langley Research Center, 1989.

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Ségol, Geneviève. Classic groundwater simulations: Proving and improving numerical models. Englewood Cliffs, N.J: PTR Prentice Hall, 1994.

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Ségol, G. Classic groundwater simulations: Proving and improving numerical models. Englewood Cliffs, N.J: PTR Prentice Hall, 1994.

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Biro, Susana. Numerical simulations of time-dependent Herbig-Haro jets. Manchester: University of Manchester, 1994.

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Book chapters on the topic "LES numerical simulations"

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Duran, Jacques. "Numerical Simulations." In Partially Ordered Systems, 184–207. New York, NY: Springer New York, 2000. http://dx.doi.org/10.1007/978-1-4612-0499-2_6.

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Giovangigli, Vincent. "Numerical Simulations." In Multicomponent Flow Modeling, 301–15. Boston, MA: Birkhäuser Boston, 1999. http://dx.doi.org/10.1007/978-1-4612-1580-6_12.

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Bisbas, Thomas G. "Numerical Simulations." In SpringerBriefs in Astronomy, 51–67. Cham: Springer International Publishing, 2015. http://dx.doi.org/10.1007/978-3-319-26142-3_4.

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Brachet, M. E. "Numerical Simulations." In Turbulence, 45–49. Boston, MA: Springer US, 1995. http://dx.doi.org/10.1007/978-1-4615-2586-8_8.

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Kratz, Robert, and Peter Wyder. "Numerical Simulations." In Principles of Pulsed Magnet Design, 89–130. Berlin, Heidelberg: Springer Berlin Heidelberg, 2002. http://dx.doi.org/10.1007/978-3-662-04969-3_3.

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Couchman, H. M. P. "Cosmological Simulations." In Numerical Astrophysics, 1–9. Dordrecht: Springer Netherlands, 1999. http://dx.doi.org/10.1007/978-94-011-4780-4_1.

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Nakasato, N., H. Yahagi, and M. Mori. "Parallel Particle Simulations." In Numerical Astrophysics, 395–96. Dordrecht: Springer Netherlands, 1999. http://dx.doi.org/10.1007/978-94-011-4780-4_119.

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Ueda, Kyohei, Yoshikazu Tanaka, Anurag Sahare, Ahmed Elgamal, Zhijian Qiu, Rui Wang, Tong Zhu, et al. "LEAP-ASIA-2019 Simulation Exercise: Comparison of the Type-B and Type-C Numerical Simulations with Centrifuge Test Results." In Model Tests and Numerical Simulations of Liquefaction and Lateral Spreading II, 61–99. Cham: Springer International Publishing, 2024. http://dx.doi.org/10.1007/978-3-031-48821-4_3.

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AbstractThis chapter presents a summary of Type-B and Type-C numerical simulations submitted by nine numerical simulation teams that participated in the LEAP-ASIA-2019 prediction campaign, with the results of a selected set of centrifuge model tests on the seismic behavior of a uniform-density, 20-m-long, and 5-degree sandy slope. Time histories of response accelerations, excess pore water pressures, and lateral displacements at the ground surface are compared to the experimental results. A majority of Type-B and Type-C numerical simulations were capable of simulating well the experimental trends observed in the centrifuge tests; in particular, Type-C simulations were found to capture the measured responses more accurately by adjusting the model parameters. Although it is quite challenging to perfectly capture all measured responses (e.g., accelerations, pore pressures, and displacements), the simulation exercises demonstrate that the numerical simulations can be further improved by accumulating high-quality experimental results as a database.
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Hock, Kiel, François Méot, and Vasiliy Morozov. "Spin Dynamics Tutorial: Numerical Simulations." In Polarized Beam Dynamics and Instrumentation in Particle Accelerators, 315–408. Cham: Springer International Publishing, 2023. http://dx.doi.org/10.1007/978-3-031-16715-7_14.

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AbstractNumerical simulations are inescapable steps in spin dynamics studies and in the design of polarized beam accelerators and optical components. An integral part of the Summer 2021 USPAS Spin Class teachings, under the form of a 2-week miniworkshop, this chapter is also an initiation to the field, “hands on”: in a first Section, numerical simulation exercises are proposed which cover many of the theoretical aspects of hadron and electron spin dynamics addressed during the lectures, including resonant depolarization; preservation methods such as harmonic orbit correction, tune jump, the use of an ac dipole, or snakes; the effect of synchrotron radiation; spin diffusion and its suppression; spin matching. A second Section is dedicated to detailed solutions of these simulation exercises and includes tight comparisons of numerical outcomes and theoretical expectations from the lectures.
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Gupta, Abhishek K. "Monte Carlo Simulations." In Numerical Methods using MATLAB, 69–80. Berkeley, CA: Apress, 2014. http://dx.doi.org/10.1007/978-1-4842-0154-1_6.

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Conference papers on the topic "LES numerical simulations"

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Martini, F., C. J. Bean, and S. S. Dolan. "Structures - Numerical Simulations." In 61st EAGE Conference and Exhibition. European Association of Geoscientists & Engineers, 1999. http://dx.doi.org/10.3997/2214-4609.201407945.

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Gonzalez, Esteban. "Numerical Simulations of Screech." In 51st AIAA/SAE/ASEE Joint Propulsion Conference. Reston, Virginia: American Institute of Aeronautics and Astronautics, 2015. http://dx.doi.org/10.2514/6.2015-3965.

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"Theoretical investigations numerical simulations." In 2004 Second International Workshop Ultrawideband and Ultrashort Impulse Signals. IEEE, 2004. http://dx.doi.org/10.1109/uwbus.2004.1388052.

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Liu, Xuan, R. Trebino, and Arlee V. Smith. "Numerical Simulations of GRENOUILLE." In Frontiers in Optics. Washington, D.C.: OSA, 2006. http://dx.doi.org/10.1364/fio.2006.jwd34.

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Aoun, Mohamed, Rachid Malti, Franc¸ois Levron, and Alain Oustaloup. "Numerical Simulations of Fractional Systems." In ASME 2003 International Design Engineering Technical Conferences and Computers and Information in Engineering Conference. ASMEDC, 2003. http://dx.doi.org/10.1115/detc2003/vib-48389.

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This paper deals with the design and simulation of continuous-time models with fractional differentiation orders. Two new methods are proposed. The first is an improvement of the approximation of the fractional integration operator using recursive poles and zeros proposed by Oustaloup (1995) and Lin (2001). The second improves the simulation schema by using a modal representation.
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Nobari, M., and G. Tryggvason. "Numerical simulations of drop collisions." In 32nd Aerospace Sciences Meeting and Exhibit. Reston, Virigina: American Institute of Aeronautics and Astronautics, 1994. http://dx.doi.org/10.2514/6.1994-835.

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Jo, Soo W., S. A. Sherif, and William E. Lear. "Numerical Simulations of Bubble Pumps." In ASME 2012 Pressure Vessels and Piping Conference. American Society of Mechanical Engineers, 2012. http://dx.doi.org/10.1115/pvp2012-78867.

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A bubble pump is a key component for diffusion-absorption refrigeration systems operating at a single pressure. Nevertheless, research focusing on bubble pumps is not widely found in the literature. In this study, a bubble pump model with a shape of vertical tube subjected to a uniform heat flux from the tube outer surface is numerically simulated. A saturated ammonia-water solution enters the bubble pump inlet and receives heat from the pump wall along the entire pump length. During the process, most of the ammonia in the solution vaporizes, and the remaining solution is lifted by the buoyant force created by the ammonia vapor. A numerical model was implemented by employing a commercial CFD code. The applicability of the numerical model implemented in the code to the present numerical simulations was validated through a comparative study referring to experimental data of a boiling phase change flow of water in a vertical pipe being subjected to a uniform heat flux. To investigate the influence of the bubble pump’s geometrical dimension and the heat input on the operating status and performance, numerical simulations were performed for four bubble pumps with different diameters subjected to five amounts of heat flux. Simulation results are provided in terms of the flow parameters including void fraction, and vapor and liquid velocities. The simulated spatial distributions of the flow parameters were found to have steep gradients in the radial direction near the pump wall due to the heating from the pump wall. In addition, simulated flow parameters were compared to those in previous one-dimensional (1-D) work for the same problem. It was found that the void fraction profiles along the pump length simulated in this study seem to be similar to those in 1-D models, but somewhat different quantitatively. Based on the results, the present numerical simulation model of the bubble pump is considered to be useful for certain industrial applications.
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Bounds, D. G. "Numerical simulations of Boltzmann Machines." In AIP Conference Proceedings Volume 151. AIP, 1986. http://dx.doi.org/10.1063/1.36220.

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Sawai, Hidetomo, Kei Kotake, Shoichi Yamada, Stefan Immler, and Kurt Weiler. "Numerical Simulations of Magnetorotational Supernovae." In SUPERNOVA 1987A: 20 YEARS AFTER: Supernovae and Gamma-Ray Bursters. AIP, 2007. http://dx.doi.org/10.1063/1.2803577.

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Krueger, Stefan. "Launching Evaluation By Numerical Simulations." In Drydocks, Launching & Shiplift. RINA, 2003. http://dx.doi.org/10.3940/rina.dry.2003.19.

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Reports on the topic "LES numerical simulations"

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Hemez, Francois M. Confidence in Numerical Simulations. Office of Scientific and Technical Information (OSTI), February 2015. http://dx.doi.org/10.2172/1170704.

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Fang, H., Philip Michael Gullett, Alexander Slepoy, Mark F. Horstemeyer, Michael I. Baskes, Gregory John Wagner, and Mo Li. Numerical tools for atomistic simulations. Office of Scientific and Technical Information (OSTI), January 2004. http://dx.doi.org/10.2172/918395.

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Fasel, Hermann F. Numerical Simulations of Wall Jets. Fort Belvoir, VA: Defense Technical Information Center, July 1997. http://dx.doi.org/10.21236/ada329611.

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Bedell, K. S., J. E. Gubernatis, R. T. Scalettar, and G. T. Zimanyi. Numerical simulations of disordered superconductors. Office of Scientific and Technical Information (OSTI), December 1997. http://dx.doi.org/10.2172/563278.

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Dai, William. Numerical Diffusion (Mixing) of Material in Numerical Simulations of Hydrodynamics. Office of Scientific and Technical Information (OSTI), April 2021. http://dx.doi.org/10.2172/1778735.

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Petersson, N. Anders, Bjorn Sjogreen, and Samuel Schrauth. Numerical simulations of realistic grating compressors. Office of Scientific and Technical Information (OSTI), October 2018. http://dx.doi.org/10.2172/1481090.

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Dai, William, Theodore Carney, Robert Pelak, Jeffrey Peterson, and Kenneth Cleveland. Numerical Simulations of Non-Proliferation Experiments. Office of Scientific and Technical Information (OSTI), May 2022. http://dx.doi.org/10.2172/1871438.

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Lefrancois, A., J. Benterou, F. Roeske, and E. Roos. Diameter Effect In Initiating Explosives, Numerical Simulations. Office of Scientific and Technical Information (OSTI), February 2006. http://dx.doi.org/10.2172/893995.

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Nelson, Anthony C. Numerical simulations of cylindrical and spherical implosions. Office of Scientific and Technical Information (OSTI), August 2011. http://dx.doi.org/10.2172/1090668.

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Okuda, H. Numerical simulations on the magnetopause current layer. Office of Scientific and Technical Information (OSTI), December 1990. http://dx.doi.org/10.2172/6303880.

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