Готові списки джерел за темами / Simulation of magnetic fields

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Добірка наукової літератури з теми "Simulation of magnetic fields"

Автор: Grafiati
Опубліковано: 30 травня 2022
Оновлено: 31 липня 2025

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Статті в журналах з теми "Simulation of magnetic fields"

1

Schnack, D. D., Z. Mikić, D. C. Barnes, and G. Van Hoven. "Magnetohydrodynamic simulation of coronal magnetic fields." Computer Physics Communications 59, no. 1 (1990): 21–37. http://dx.doi.org/10.1016/0010-4655(90)90153-r.

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2

Trang, Nguyen Thi Thao, Peter Lott, and Quynh Lan Nguyen. "Magnetic Field in the Universe." Journal of Physics: Conference Series 3040, no. 1 (2025): 012009. https://doi.org/10.1088/1742-6596/3040/1/012009.

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Abstract Magnetic fields permeate the universe and influence physical processes, from compact objects to large cosmic structures. Unlike electric fields, magnetic fields are closely tied to space-time dynamics, governing charged particle motion and producing radiation such as synchrotron and curvature emission. On intergalactic scales, magnetic fields are reshaped during galaxy mergers. Gravitational forces drive turbulence, shock waves, and gas inflows that amplify and reorganize magnetic fields. Radio synchrotron emission and polarization mapping observations reveal strong, coherent fields i
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3

Füzi, J. "Simulation of neutron motion in magnetic fields—magnetic monochromator." Measurement Science and Technology 19, no. 3 (2008): 034013. http://dx.doi.org/10.1088/0957-0233/19/3/034013.

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4

Uetake, H., N. Hirota, Y. Ikezoe, K. Kitazawa, and K. Miyoshi. "Magnetic-field simulation for shielding from high magnetic fields." Journal of Applied Physics 91, no. 10 (2002): 6991. http://dx.doi.org/10.1063/1.1452672.

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5

Vieira, Gregory B., Eliza Howard, Prannoy Lankapalli, Iesha Phillips, Keith Hoffmeister, and Jackson Holley. "Stray Magnetic Field Variations and Micromagnetic Simulations: Models for Ni0.8Fe0.2 Disks Used for Microparticle Trapping." Micromachines 15, no. 5 (2024): 567. http://dx.doi.org/10.3390/mi15050567.

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Patterned micro-scale thin-film magnetic structures, in conjunction with weak (~few tens of Oe) applied magnetic fields, can create energy landscapes capable of trapping and transporting fluid-borne magnetic microparticles. These energy landscapes arise from magnetic field magnitude variations that arise in the vicinity of the magnetic structures. In this study, we examine means of calculating magnetic fields in the local vicinity of permalloy (Ni0.8Fe0.2) microdisks in weak (~tens of Oe) external magnetic fields. To do this, we employ micromagnetic simulations and the resulting calculations o
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6

Stacy, Athena, Christopher F. McKee, Aaron T. Lee, Richard I. Klein, and Pak Shing Li. "Magnetic fields in the formation of the first stars – II. Results." Monthly Notices of the Royal Astronomical Society 511, no. 4 (2022): 5042–69. http://dx.doi.org/10.1093/mnras/stac372.

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ABSTRACT Beginning with cosmological initial conditions at z = 100, we simulate the effects of magnetic fields on the formation of Population III stars and compare our results with the predictions of Paper I. We use gadget-2 to follow the evolution of the system while the field is weak. We introduce a new method for treating kinematic fields by tracking the evolution of the deformation tensor. The growth rate in this stage of the simulation is lower than expected for diffuse astrophysical plasmas, which have a very low resistivity (high magnetic Prandtl number); we attribute this to the large
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7

Virtanen, I. O. I., A. A. Pevtsov, I. I. Virtanen, and K. Mursula. "Reconstructing solar magnetic fields from historical observations." Astronomy & Astrophysics 652 (August 2021): A79. http://dx.doi.org/10.1051/0004-6361/202140656.

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Context. The evolution of the photospheric magnetic field can be simulated with surface flux transport (SFT) simulations, which allow for the study of the evolution of the entire field, including polar fields, solely using observations of the active regions. However, because only one side of the Sun is visible at a time, active regions that emerge and decay on the far-side are not observed and not included in the simulations. As a result, some flux is missed. Aims. We construct additional active regions and apply them to the far-side of the Sun in an SFT simulation to assess the possible effec
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8

Padoan, Paolo, Tuomas Lunttila, Mika Juvela, et al. "Magnetic Fields in Molecular Clouds." Proceedings of the International Astronomical Union 6, S271 (2010): 187–96. http://dx.doi.org/10.1017/s1743921311017601.

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AbstractSupersonic magneto-hydrodynamic (MHD) turbulence in molecular clouds (MCs) plays an important role in the process of star formation. The effect of the turbulence on the cloud fragmentation process depends on the magnetic field strength. In this work we discuss the idea that the turbulence is super-Alfvénic, at least with respect to the cloud mean magnetic field. We argue that MCs are likely to be born super-Alfvénic. We then support this scenario based on a recent simulation of the large-scale warm interstellar medium turbulence. Using small-scale isothermal MHD turbulence simulation,
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9

Suzuki, Takeru K. "MHD in a Cylindrical Shearing Box. II. Intermittent Bursts and Substructures in MRI Turbulence." Astrophysical Journal 957, no. 2 (2023): 99. http://dx.doi.org/10.3847/1538-4357/acfb88.

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Abstract By performing ideal magnetohydrodynamical (MHD) simulations with weak vertical magnetic fields in unstratified cylindrical shearing boxes with modified boundary treatment, we investigate MHD turbulence excited by magnetorotational instability. The cylindrical simulation exhibits extremely large temporal variation in the magnetic activity compared with the simulation in a normal Cartesian shearing box, although the time-averaged field strengths are comparable in the cylindrical and Cartesian setups. Detailed analysis of the terms describing magnetic energy evolution with “triangle diag
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10

Ye, Jun-Xian, Jia-Mian Hu, Zhan Shi, et al. "Magnetic-Field-Orientation Dependent Magnetoelectric Effect in FeBSiC/PZT/FeBSiC Composites." Advances in Materials Science and Engineering 2014 (2014): 1–5. http://dx.doi.org/10.1155/2014/249526.

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We investigate the magnetic-field-orientation dependent magnetoelectric (ME) effect in the FeBSiC/Pb(Zr,Ti)O3(PZT)/FeBSiC laminates. It is shown that, by only using the bias-magnetic-field dependent ME response measured with the magnetic-field parallel to the surface plane of PZT slab, the magnetic-field-orientation dependent ME coefficient upon magnetic-fields of various amplitudes can be obtained via computer simulations. The simulation results match well the experimental measurements, demonstrating the applicability of the ME laminates-based sensors in detecting magnetic-fields with uncerta
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Дисертації з теми "Simulation of magnetic fields"

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Schumacher, Kristopher Ray. "Direct numerical simulation of ferrofluid turbulence in magnetic fields /." Thesis, Connect to this title online; UW restricted, 2005. http://hdl.handle.net/1773/9892.

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Andreu, Segura Jordi. "Statistical Mechanics of Superparamagnetic Colloidal Dispersions Under Magnetic Fields." Doctoral thesis, Universitat Autònoma de Barcelona, 2013. http://hdl.handle.net/10803/113485.

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Les dispersions col·loïdals, un terme encunyat pel científic escocès Thomas Graham el 1861, han estat objecte d’interès en diferents àrees científiques durant més d'un segle. Una dispersió col·loïdal es caracteritza per l’existència d'una fase dispersa uniformement distribuïda dins un medi dispersiu. Diferents compostos entren dins aquesta categoria, com els aerosols (fum, boira, núvols o pols), les escumes, les emulsions (maionesa o llet) o els gels (mantega o melmelada). Les millores recents en la síntesi de partícules i l'estabilitat col·loïdal han impulsat la millora en el disseny de nous
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3

Ueda, Hiroyuki. "Studies on low-field functional MRI to detect tiny neural magnetic fields." Doctoral thesis, Kyoto University, 2021. http://hdl.handle.net/2433/263666.

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付記する学位プログラム名: 京都大学卓越大学院プログラム「先端光・電子デバイス創成学」<br>京都大学<br>新制・課程博士<br>博士(工学)<br>甲第23205号<br>工博第4849号<br>京都大学大学院工学研究科電気工学専攻<br>(主査)教授 小林 哲生, 教授 松尾 哲司, 特定教授 中村 武恒<br>学位規則第4条第1項該当<br>Doctor of Philosophy (Engineering)<br>Kyoto University<br>DFAM
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4

Cook, Graeme Robert. "Magnetic flux transport simulations : applications to solar and stellar magnetic fields." Thesis, University of St Andrews, 2011. http://hdl.handle.net/10023/2072.

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Magnetic fields play a key role in a wide variety of phenomena found on the Sun. One such phenomena is the Coronal Mass Ejection (CME) where a large amount of material is ejected from the Sun. CME’s may directly affect the earth, therefore understanding their origin is of key importance for space weather and the near-Earth environment. In this thesis, the nature and evolution of solar magnetic fields is considered through a combination of Magnetic Flux Transport Simulations and Potential Field Source Surface Models. The Magnetic Flux Transport Simulations produce a realistic description of the
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Cui, Han. "Modeling, Implementation, and Simulation of Two-Winding Plate Inductor." Diss., Virginia Tech, 2017. http://hdl.handle.net/10919/78301.

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Design of magnetic component is a key factor in achieving high frequency, high power-density converters. Planar magnetics are widely used in bias power supplies for the benefits of low profile and their compatibility with printed-circuit boards (PCB). The coupled inductors with winding layers sandwiched between two core plates are studied in this dissertation in order to model the self-inductance, winding loss, and core loss. The most challenging task for the plate-core inductor is to model the magnetic field with finite core dimensions, very non-uniform flux pattern, and large fringing flux
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Younas, Irfan. "Simulations of magnetic properties of short superconducting cylinders and coils." Thesis, University of Southampton, 1997. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.242102.

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Sturrock, Zoe. "Numerical simulations of sunspot rotation driven by magnetic flux emergence." Thesis, University of St Andrews, 2017. http://hdl.handle.net/10023/10129.

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Magnetic flux continually emerges from the Sun, rising through the solar interior, emerging at the photosphere in the form of sunspots and expanding into the atmosphere. Observations of sunspot rotations have been reported for over a century and are often accompanied by solar eruptions and flaring activity. In this thesis, we present 3D numerical simulations of the emergence of twisted flux tubes from the uppermost layers of the solar interior, examining the rotational movements of sunspots in the photospheric plane. The basic experiment introduces the mechanism and characteristics of sunspot
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Geng, Annette Monika [Verfasser]. "Numerical Simulations of Magnetic Fields in Interacting Galaxies / Annette Monika Geng." München : Verlag Dr. Hut, 2013. http://d-nb.info/1031845003/34.

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Flaux, Pierrick. "Measurement of the neutron electric dipole moment at the Paul Scherrer Institute : production of magnetic fields." Thesis, Normandie, 2019. http://www.theses.fr/2019NORMC222/document.

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Le travail réalisé au cours de cette thèse concerne le développement du système de bobines de l'expérience n2EDM à l'Institut Paul Sherrer (PSI). Le but de cette expérience est de mettre en évidence de nouvelles sources de violation CP à travers la mesure du moment dipolaire électrique du neutron. L'actuelle limite supérieure sur la mesure de nEDM, $2.9 \cross 10^{-26}$ e.cm (90\% C.L.) à été obtenue par la collaboration RAL-Sussex-ILL en 2006.L'expérience n2EDM vise à améliorer d'un ordre de grandeur la sensibilité statistique en gardant sous contrôle les effets systématiques. Cela requiert l
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Jocher, Agnès. "Control of soot formation in laminar flames by magnetic fields and acoustic waves." Thesis, Paris 6, 2017. http://www.theses.fr/2017PA066043.

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Cette thèse consiste en l'étude expérimentale et numérique des processus de formation des particules de suie au sein des flammes laminaires non-pré-mélangées et partiellement prémélangées sous l'influence d'un champ magnétique ou d'une stimulation acoustique. Dans une premiére étape, la capacité du code CIAO à prédire la fraction volumique de suie dans une flamme axisymétrique est étudiée. Par la suite, deux flammes subissant une stimulation acoustique ont été étudiées. Les résultats peuvent être utilisés pour améliorer les modèles de suie futurs, en particulier concernant les différentes éche
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Книги з теми "Simulation of magnetic fields"

1

Rüdiger, G. Magnetic processes in astrophysics: Theory, simulations, experiments. Wiley-VCH Verlag GmbH & Co. KGaA, 2013.

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2

Looi, Thomas. Magnetic field simulator for microsatellite attitude testing. National Library of Canada, 2002.

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3

Looi, Thomas. Magnetic field simulator for microsatellite attitude testing. University of Toronto, Institute for Aerospace Studies, 2002.

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4

Schwarm, Fritz-Walter. Monte Carlo Simulation of Cyclotron Lines in Strong Magnetic Fields - Theory and Application. Friedrich-Alexander-Universität Erlangen-Nürnberg (FAU), 2017.

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5

United States. National Aeronautics and Space Administration., ed. Current collection in a magnetic field: Final report of E.N. Krivorutsky, Spring 1997. National Aeronautics and Space Administration, 1997.

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6

Japan-Hungary Joint Seminar on Applied Electromagnetics in Materials and Computational Technology (5th 1998 Budapest, Hungary). Applied electromagnetics and computational technology II: Proceedings of the 5th Japan-Hungary Joint Seminar on Applied Electromagnetics in Materials and Computational Technology : Budapest, Hungary, September 24-26, 1998. IOS Press, 2000.

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7

Japan-Hungary Joint Seminar on Applied Electromagnetics in Materials and Computational Technology (4th 1996 Fukuyama, Japan). Applied electromagnetics and computational technology: Proceedings of the 4th Japan-Hungary Joint Seminar on Applied Electromagnetics in Materials and Computational Technology, Fukuyama, Japan, July 1-3, 1996. IOS Press, 1996.

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8

Anwane, S. W. Fundamentals of electromagnetic fields: A computer approach. Infinity Science Press, 2007.

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9

K, Wright, and United States. National Aeronautics and Space Administration., eds. A study entitled research on orbital plasma-electrodynamics: Progress report, period of performance, March 27, 1994 - June 29, 1994. National Aeronautics and Space Administration, 1994.

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10

Programme, United Nations Environment, International Labour Organisation, World Health Organization, and International Radiation Protection Association, eds. Magnetic fields. World Health Organization, 1987.

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Частини книг з теми "Simulation of magnetic fields"

1

Yoshida, Kinjiro, Hiroshi Takami, Shinichi Ogusa, and Dai Yokota. "FEM Dynamics Simulation of Controlled-PM LSM Maglev Vehicle." In Electric and Magnetic Fields. Springer US, 1995. http://dx.doi.org/10.1007/978-1-4615-1961-4_75.

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2

Nabeta, Silvio I., Albert Foggia, Marcel Ivanes, Jean-Louis Coulomb, and Gilbert Reyne. "A Finite-Element Simulation of an Out-of-Phase Synchronization of a Synchronous Machine." In Electric and Magnetic Fields. Springer US, 1995. http://dx.doi.org/10.1007/978-1-4615-1961-4_27.

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3

Bishop, Robert C., Paul R. Shapiro, and Daniel C. Barnes. "Magnetohydrodynamic Simulation of the Evolution of Large-Scale Magnetic Fields in Disk Galaxies." In Galactic and Intergalactic Magnetic Fields. Springer Netherlands, 1990. http://dx.doi.org/10.1007/978-94-009-0569-6_44.

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4

Lipatov, Alexander S. "Magnetic Field Reconnection Simulation." In The Hybrid Multiscale Simulation Technology. Springer Berlin Heidelberg, 2002. http://dx.doi.org/10.1007/978-3-662-05012-5_10.

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Hardee, Philip E., and Michael L. Norman. "Numerical Simulation of Weakly Magnetized Propagating Slab Jets." In Accretion Disks and Magnetic Fields in Astrophysics. Springer Netherlands, 1989. http://dx.doi.org/10.1007/978-94-009-2401-7_21.

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Stone, James M., Michael L. Norman, and Dimitri Mihalas. "Numerical Simulation of Mass Outflows from Star Forming Regions." In Accretion Disks and Magnetic Fields in Astrophysics. Springer Netherlands, 1989. http://dx.doi.org/10.1007/978-94-009-2401-7_22.

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Molteni, D. A. P., and G. Giannone. "Three Dimensional Simulation of Accretion Disks with Smoothed Particle Hydrodynamics." In Accretion Disks and Magnetic Fields in Astrophysics. Springer Netherlands, 1989. http://dx.doi.org/10.1007/978-94-009-2401-7_15.

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Zaninetti, L. "Contour Simulations of Astrophysical Jets." In Galactic and Intergalactic Magnetic Fields. Springer Netherlands, 1990. http://dx.doi.org/10.1007/978-94-009-0569-6_144.

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Haugen, N. E. L., A. Brandenburg, and W. Dobler. "High-Resolution Simulations of Nonhelical MHD Turbulence." In Magnetic Fields and Star Formation. Springer Netherlands, 2004. http://dx.doi.org/10.1007/978-94-017-0491-5_5.

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Kurgan, Eugeniusz. "Numerical Simulation of Anisotropic Shielding of Weak Magnetic Fields." In Computational Science - ICCS 2004. Springer Berlin Heidelberg, 2004. http://dx.doi.org/10.1007/978-3-540-24687-9_32.

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Тези доповідей конференцій з теми "Simulation of magnetic fields"

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Konda, Taraka Sriram, Jegyasu Gupta, Amit Baran Dey, Ratnajit Bhattacharjee, and Debabrata Sikdar. "Interdigitated Metasurfaces for Enabling Homogeneously Boosted Magnetic Fields during $1.5$T MRI Scans." In 2024 International Conference on Numerical Simulation of Optoelectronic Devices (NUSOD). IEEE, 2024. http://dx.doi.org/10.1109/nusod62083.2024.10723399.

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Wong, Denise, Jeremy Wang, Edward Steager, and Vijay Kumar. "Control of Multiple Magnetic Micro Robots." In ASME 2015 International Design Engineering Technical Conferences and Computers and Information in Engineering Conference. American Society of Mechanical Engineers, 2015. http://dx.doi.org/10.1115/detc2015-47683.

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A magnetic micro robot is a microscopic magnet that is controlled by a system of electromagnetic coils that generate a magnetic field to manipulate the magnetic robot. A major challenge for manipulating multiple magnets at microscale is that the applied field affects the entire workspace, making it difficult to address individual magnets. In this paper, we propose a system where electromagnetic coils are close to the magnets being manipulated to exploit spatial non-uniformities in the magnetic field. Our model considers the magnetic field generated by the electromagnetic coils and the magnetic
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3

Heft, Sara, Günter Bärwolff, Theodore E. Simos, George Psihoyios, Ch Tsitouras, and Zacharias Anastassi. "Crystal Melt Modeling and Simulation with Magnetic Fields." In NUMERICAL ANALYSIS AND APPLIED MATHEMATICS ICNAAM 2011: International Conference on Numerical Analysis and Applied Mathematics. AIP, 2011. http://dx.doi.org/10.1063/1.3636936.

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Dallas, W. J., and W. Kullmann. "Imaging of biological currents from magnetic fields: simulation." In OSA Annual Meeting. Optica Publishing Group, 1985. http://dx.doi.org/10.1364/oam.1985.thp4.

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Since our algorithm for reconstructing generating currents from magnetic-field measurements uses a vector-Fourier space description of the imaging process, we cast the simulation in these terms. Using the Maxwell equations for static fields, we synthesize the magnetic field which would be generated by a current density distribution. Because we use the discrete Fourier transform, care is taken to configure the current so that the continuity equation is satisfied. We also take into account the spatial-frequency warping and the special form of bounding functions that are required by the discretiz
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Özbey, Arzu, Mehrdad Karimzadehkhouei, Evrim Kurtoğlu, and Ali Koşar. "Simulation of Magnetic Actuation of Ferrofluids in Microtubes." In ASME 2013 11th International Conference on Nanochannels, Microchannels, and Minichannels. American Society of Mechanical Engineers, 2013. http://dx.doi.org/10.1115/icnmm2013-73153.

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Magnetic actuation of ferrofluids with dynamic magnetic fields is one of the most promising research areas with its wide and different potential application areas such as biomedical and micropumping applications. Ferrofluid has the potential of opening up new possibilities. To have more understanding about various fields of engineering, more research should be conducted by considering both the experimental and modeling aspects. The most important parameters determining the flow property, flow rates and overall system efficiency are the quality and the topology of magnetic fields used in these
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Chukwuemeka, Edison E., and Ingmar M. Schoegl. "Numerical Simulation of the Effect of Magnetic Fields on Soot Formation in Laminar Non-Premixed Flames." In ASME 2021 Power Conference. American Society of Mechanical Engineers, 2021. http://dx.doi.org/10.1115/power2021-64859.

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Abstract Characteristics of non-premixed flames such as flame height and lift-off height are affected by the presence of magnetic fields due to the paramagnetic properties of some combustion species. However, it is unknown whether magnetic fields can be used to reduce the emission of pollutants in non-premixed flames. In general, pollutant emissions are reduced in combustion systems if the mixing of combustion species is enhanced during the process. Since paramagnetic combustion species such as O2, O, OH, HO2, etc have a preferential motion direction in the presence of magnetic fields, there i
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Uesaka, Y. "Recorded magnetizations and magnetic fields in media derived by computer simulation." In International Magnetics Conference. IEEE, 1989. http://dx.doi.org/10.1109/intmag.1989.690117.

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Guoguang, Zhang, and Jiao Yuheng. "Calculation and Simulation of Magnetic Dipole Fields in Seawater." In 2020 IEEE 3rd International Conference of Safe Production and Informatization (IICSPI). IEEE, 2020. http://dx.doi.org/10.1109/iicspi51290.2020.9332465.

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Afanas'ev, V. P., A. M. Chaly, V. A. Kuptsov, and S. M. Shkol'nik. "Numerical Simulation of Cathode Spot Motion in Magnetic Fields." In 2006 International Symposium on Discharges and Electrical Insulation in Vacuum. IEEE, 2006. http://dx.doi.org/10.1109/deiv.2006.357297.

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Lonkar, Amrita K., Francisco Palacios, and Juan J. Alonso. "Simulation of Reacting Flows in Magnetic Fields with Preconditioning." In 44th AIAA Plasmadynamics and Lasers Conference. American Institute of Aeronautics and Astronautics, 2013. http://dx.doi.org/10.2514/6.2013-2754.

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Звіти організацій з теми "Simulation of magnetic fields"

1

Novokhatski, A. Simulation of Electron Cloud Multipacting in Solenoidal Magnetic Field. Office of Scientific and Technical Information (OSTI), 2004. http://dx.doi.org/10.2172/826697.

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2

Tzeferacos, Petros. Simulations of Laser Experiments to Study the Origin of Cosmic Magnetic Fields. Office of Scientific and Technical Information (OSTI), 2020. http://dx.doi.org/10.2172/1637538.

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3

Romanov, Gennady, and Vladimir Kashikhin. Simulation of RF Cavity Dark Current in Presence of Helical Magnetic Field. Office of Scientific and Technical Information (OSTI), 2010. http://dx.doi.org/10.2172/992658.

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4

Lee, Jyeching, and Shana Groeschler. Transient Simulation of a Rotating Conducting Cylinder in a Transverse Magnetic Field. Defense Technical Information Center, 2016. http://dx.doi.org/10.21236/ad1016771.

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5

Smolin, J. A. Simulation and measurement of an electron beam in a wiggler magnetic field. Office of Scientific and Technical Information (OSTI), 1989. http://dx.doi.org/10.2172/5866535.

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Lin, Yu. COLLABORATIVE RESEARCH: PARTICLE SIMULATION OF COLLISIONLESS MAGNETIC RECONNECTION UNDER FINITE GUIDE FIELD. Office of Scientific and Technical Information (OSTI), 2022. http://dx.doi.org/10.2172/1843577.

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7

Glatzmaier, G. A., R. Hollerbach, and P. H. Roberts. A study by computer simulation of the generation and evolution of the Earth`s magnetic field. Office of Scientific and Technical Information (OSTI), 1995. http://dx.doi.org/10.2172/200713.

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8

H. Qin and X. Guan. Variational Symplectic Integrator for Long-Time Simulations of the Guiding-Center Motion of Charged Particles in General Magnetic Fields. Office of Scientific and Technical Information (OSTI), 2008. http://dx.doi.org/10.2172/960290.

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9

Nestleroth and Alers. L51946 Enhanced Implementation of MFL Using EMAT Sensors to Detect External Coating Disbondment. Pipeline Research Council International, Inc. (PRCI), 2002. http://dx.doi.org/10.55274/r0010676.

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Анотація:
External coatings are used routinely to protect transmission pipelines from conditions that promote corrosion. However, over time coatings may disbond, allowing corrosion to occur. To detect metal loss due to corrosion defects, transmission pipeline operators often use magnetic flux leakage (MFL) in-line inspection tools. These tools do not detect the cause of an actual problem, i.e., failure of a coating and the presence of a corrosive environment; rather, they detect only the result, i.e., a defect that may permanently alter the pressure capacity of the pipeline. Metal loss is the most commo
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10

Laties, V., and S. Stern. Magnetic fields and behavior. Office of Scientific and Technical Information (OSTI), 1990. http://dx.doi.org/10.2172/6866669.

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