Auswahl der wissenschaftlichen Literatur zum Thema „Effet MHD“
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Zeitschriftenartikel zum Thema "Effet MHD"
Royani, J. I., H. Khairiyah, F. R. Mira, Karyanti und N. Watanabe. „The effect of callus induction media for somatic embryo formation in Hevea brasiliensis Muell. Arg“. IOP Conference Series: Earth and Environmental Science 1160, Nr. 1 (01.04.2023): 012007. http://dx.doi.org/10.1088/1755-1315/1160/1/012007.
Der volle Inhalt der QuelleGuha, Sanjib, und Niazur Rahim. „The effect of managerial horizon on cash holdings“. Managerial Finance 45, Nr. 8 (12.08.2019): 1092–110. http://dx.doi.org/10.1108/mf-09-2018-0442.
Der volle Inhalt der QuelleMogi, Iwao, und Kazuo Watanabe. „Chiral Recognition of Amino Acids by Magnetoelectrodeposited Cu Film Electrodes“. International Journal of Electrochemistry 2011 (2011): 1–6. http://dx.doi.org/10.4061/2011/239637.
Der volle Inhalt der QuelleChowdhury, Kakali. „MHD Mixed Convective Nanofluid Flow: Effect of Heat Source and Corrugated Boundary“. Nanomedicine & Nanotechnology Open Access 8, Nr. 3 (2023): 1–14. http://dx.doi.org/10.23880/nnoa-16000255.
Der volle Inhalt der QuelleLansford, Jefferson L., Shengjie Chai, Gheath Alatrash, Jeffrey J. Molldrem, Paul M. Armistead und Benjamin G. Vincent. „Integrated In Silico Prediction of Minor Histocompatibility Antigen Peptides in HLA-Matched Allogeneic Stem Cell Transplantation for Acute Myeloid Leukemia“. Blood 128, Nr. 22 (02.12.2016): 3352. http://dx.doi.org/10.1182/blood.v128.22.3352.3352.
Der volle Inhalt der QuelleBenkeblia, Noureddine. „Effect of maleic hydrazide on respiratory parameters of stored onion bulbs (Allium cepa L.)“. Brazilian Journal of Plant Physiology 16, Nr. 1 (April 2004): 47–52. http://dx.doi.org/10.1590/s1677-04202004000100007.
Der volle Inhalt der QuelleAslani, Kyriaki-Evangelia, Lefteris Benos, Efstratios Tzirtzilakis und Ioannis E. Sarris. „Micromagnetorotation of MHD Micropolar Flows“. Symmetry 12, Nr. 1 (10.01.2020): 148. http://dx.doi.org/10.3390/sym12010148.
Der volle Inhalt der QuelleRaptis, A., C. Perdikis und H. S. Takhar. „Effect of thermal radiation on MHD flow“. Applied Mathematics and Computation 153, Nr. 3 (Juni 2004): 645–49. http://dx.doi.org/10.1016/s0096-3003(03)00657-x.
Der volle Inhalt der QuellePALUMBO, L. J., und A. M. PLATZECK. „MHD stationary symmetric flows with Hall effect“. Journal of Plasma Physics 72, Nr. 04 (08.12.2005): 457. http://dx.doi.org/10.1017/s0022377805003958.
Der volle Inhalt der QuelleDang, Khyati, Vinita Makkar und Naresh Sharma. „Mathematical Simulation for MHD Casson Convective Nanofluid Flow Induced by 3D Permeable Sheet with Chemical Effect“. Indian Journal Of Science And Technology 17, Nr. 16 (19.04.2024): 1713–23. http://dx.doi.org/10.17485/ijst/v17i16.117.
Der volle Inhalt der QuelleDissertationen zum Thema "Effet MHD"
Chahine, Robert. „MHD simulations of the Reversed Field Pinch“. Thesis, Lyon, 2017. http://www.theses.fr/2017LYSEC056/document.
Der volle Inhalt der QuelleThe dynamics of magnetic fusion plasmas in the Reversed Field Pinch (RFP) configuration are studied using an incompressible magnetohydrodynamics (MHD) description. A pseudospectral method combined with a volume penalization method are used to resolve the governing equations in a straight cylinder. Numerical simulations show that the pressure effects on the RFP dynamics cannot be neglected, and thus the _ parameter is not adequate to characterize the importance of pressure in the dynamics. A new parameter, _0r , which is the ratio of the pressure gradient’s magnitude to the Lorentz force’s magnitude, is proposed to be the proper parameter to describe the RFP dynamics. Another investigated influence on the RFP dynamics is the shaping of the poloidal cross-section. Simulations of flows with the same Lundquist number and different cross-sections (circular and elliptic) show a clear change in the spectral behaviour, as well as in the radial turbulent diffusion. Finally, the RFP flows are used to study the dynamo effect. Numerical results show that RFP flows are capable of amplifying a seed magnetic field, which will have tendency to be more nonlinear than the RFP magnetic field in the turbulent regime
Flutet, Vincent. „Etude numérique de la dynamique d'une couche limite turbulente avec effet MHD“. Paris 6, 2007. http://www.theses.fr/2007PA066605.
Der volle Inhalt der QuelleTurbulence is a phenomenon present in most streams. Near a boundary, its main effect is to increase the stream drag. Thus it can be interesting to weaken turbulence in order to decrease drag. Several studies have shown that the use of a magnetic field could weaken turbulence. Indeed, in a conducting fluid moving under a magnetic fluid counter-movement forces appear. This study aims at determining, under both subsonic and supersonic conditions, the effect of a magnetic field on a turbulent channel flow, especially on coherent structures of the boundary layer and on drag. Results have shown an increase of the sensibility to the magnetic field with compressibility. Reorganisation of coherent structures of boundary layer is also shown. A last, magnetic field causes a participation to drag but causes to a decrease in turbulent drag that is more important
Tieriekhov, Kostiantyn. „Applications non-conventionnelles de champs magnétiques à séparation chirale et aux systèmes électrochimiques dynamiques“. Electronic Thesis or Diss., Bordeaux, 2023. http://www.theses.fr/2023BORD0502.
Der volle Inhalt der QuelleHigh-purity enantioseparation is essential for the pharmaceutical and food industries. Conventional chiral separation techniques provide a wide range of methods, all of which rely on chiral selectors - stationary phases or molecules that discriminate enantiomers through stereospecific interaction. Despite the vast number of natural and synthetic selectors currently in use, the increasing demand for enantiopurity is driving research for new and versatile methods.The aim of this thesis is to investigate alternative methods of chiral separation that involve the application of magnetic fields in various configurations. One idea centers around the concept of true and false chirality, which was introduced by L. Barron for dynamic systems of individual objects and physical vector quantities. His discussion explicitly states that neither static magnetic nor electric fields, nor any combination of those, possess true chirality, the feature required to induce enantiomeric discimination. However, his theory suggests a molecular analog of the well-known Faraday effect based on the collinear application of magnetic field to a molecular flow.Alternatively, a perpendicular configuration with the molecular flow involving a ferromagnetic substrate has demonstrated enantiospecific spin interactions, otherwise known as the CISS effect. In this regard, our main objective was the further exploration of such interactions in dynamic conditions of capillary electrophoresis, which provides simple and fast detection, while introducing Ni substrates along the flow of molecules and applying an orthogonal magnetic field.Lastly, the orthogonal configuration of the magnetic field was exploited to study the dynamic behavior of electropolarized objects. The patterns of the resulting rotation, exhibited by different objects under the influence of a magnetohydrodynamic effect, originating from the induced Lorentz force, are shown to be dependent on magnetic field polarity. Their dynamic behavior as a function of time resembles those of falsely chiral systems
Msellak, Khalid. „Electrodéposition métallique sous contrôle MHD : caractérisation physique et électrochimique“. Reims, 2003. http://www.theses.fr/2003REIMS008.
Der volle Inhalt der QuelleThis work analyzes the influence of a magnetic field parallel to the electrode on two electrochemical systems of industrial interest : the deposit of Cu on substrates inducing no epitaxy and deposits of Ni-Fe alloys. The characterization of the deposits was led with several physical and electrochemical techniques. The results show that : The magnetic field does not modify the nucleation of Cu on a conductive substrate (glassy C or Ti) : the only measurable results are the magneto-induced convective effects on the growth of Cu. On TiO2, a phenomenon of anisotropy confirms the existence of a transverse electric field. The phenomenon, sensitive with moderate fields, was put in evidence in a spectacular way under the intense fields available on the LMCI of Grenoble. For electrodeposition of Ni-Fe alloys, the results show that the magnetic field increases the convective rate of the ferrous ions to the electrode. These species inhibit the Ni deposit and lead to alloys considerably enriched in Fe
Riols-Fonclare, Antoine. „Effet dynamo et turbulence magnétohydrodynamique sous-critiques dans les disques d'accrétion“. Toulouse 3, 2014. http://thesesups.ups-tlse.fr/3242/.
Der volle Inhalt der QuelleOne of the main challenges of accretion disk theory in astrophysics is to identify efficient angular momentum transport mechanisms in disks. The most popular scenario is that this transport is due to the magnetohydrodynamic (MHD) turbulence triggered by the magnetorotational instability (MRI), which requires the existence of a magnetic field. This raises the question of the origin and sustainement of such a field in disks. A subcritical nonlinear dynamo process, involving the MRI, may be responsible for the joint excitation of MHD turbulence and magnetic fields in Keplerian shear flow. Similar dynamos driven by other MHD instabilities may also be active in stellar interiors. However, the detailed mechanisms underlying the excitation of the MRI dynamo are not well understood. Numerical results suggest that this mechanism may not be sustained at low magnetic Prandtl number (ratio between viscosity and magnetic diffusivity), a common dissipation regime in accretion disks. The purpose of this thesis has been to understand the physical conditions of excitation of this dynamo and the role of dissipative effects on the transition to self-sustained MHD turbulence. For this purpose, we investigated in detail the nature of the transition and the role of tridimensional nonlinear periodic solutions in this problem. First, we showed that the emergence of chaotic dynamo action is primarily associated with global bifurcations involving such cycles. We then attempted to elucidate the physical origin of the Pm dependence of the transition. Using a detailed energy analysis of several dynamo cycles, we found that "turbulent" diffusion makes the excitation of the dynamo increasingly difficult for decreasing Pm. This very generic effect could be an important determinant of MRI dynamo excitation in disks, and may also limit the efficiency of angular momentum transport by MRI turbulence at low Pm
Marchand, Pierre. „Étude des processus physiques de la formation d'étoiles par effondrement gravo-turbulent“. Thesis, Lyon, 2017. http://www.theses.fr/2017LYSE1154/document.
Der volle Inhalt der QuelleThe angular momentum regulation is a hot topic in star formation. From the molecular cloud to th final star, the system loses most of its angular momentum, and several processes are proposed to explain this phenomenon. We focus on non-ideal magnetohydrodynamics (MHD), which describes the coupling between a fluid and its magnetic field. Its efficiency to regulate the angular momentum in realistic conditions has been shown in several studies. First, we develop a code that computes the chemical equilibrium of elements present in the early stages of star formation. We can therefore obtain the values of coefficients defining the strength of the phyical processes associated with non-ideal MHD. We then take interest in one of them, the Hall effect, still poorly studied in this context. We implement it in the eulerian code RAMSES, and use it to quantify its influence during a gravitational collapse. As predicted by theory, the Hall effect greatly influences the size of the protoplanetary disk, in which planets form, and creates envelopes of gas rotating backward compared to the rest of the system
Leprovost, Nicolas. „Influence des petites échelles sur la dynamique à grande échelle en turbulence hydro et magnétohydrodynamique“. Phd thesis, Université Pierre et Marie Curie - Paris VI, 2004. http://tel.archives-ouvertes.fr/tel-00007809.
Der volle Inhalt der QuelleLessinnes, Thomas. „Magnetohydrodynamic turbulence modelling: application to the dynamo effect“. Doctoral thesis, Universite Libre de Bruxelles, 2010. http://hdl.handle.net/2013/ULB-DIPOT:oai:dipot.ulb.ac.be:2013/210042.
Der volle Inhalt der QuelleIl est surprenant qu'alors que les mouvements fluides à l'intérieur de ces objets célestes sont turbulents, les champs magnétiques généré soient de grande échelle spatiale et stables sur de longues périodes de temps. De plus, ils peuvent présenter une dynamique temporelle régulière comme c'est le cas pour le champ magnétique solaire dont la polarité s'inverse tous les onze ans.
Décrire et prédire les mouvements d'un fluide turbulent reste l'un des problèmes les plus difficiles de la mécanique classique.
%La description aussi bien analytique que numérique d'un fluide hautement turbulent est d'une effroyable complexité, si pas tout simplement impraticable. Dans cette situation,
Il est donc utile de construire des modèles aussi proches que possible du système de départ mais de moindre complexité de sorte que des études théoriques et numériques deviennent envisageables.
Deux approches ont été considérées ici. D'une part, nous avons développé des modèles présentant un très petit nombre de degrés de liberté (de l'ordre de la dizaine). Une étude analytique est alors possible. Ces modèles ont une dépendance en les paramètres physiques - nombres de Reynolds cinétique et magnétique et injection d'hélicité - qualitativement similaire aux dynamos célestes et expérimentales.
D'autre part, les modèles en couches permettent de caractériser les transferts d'énergie entre les structures de différentes tailles présentes au sein du champ de vitesse. Nous avons développé un nouveau formalisme qui permet d'étudier aussi les échanges avec le champ magnétique.
De plus, nous proposons une étude de la MHD dans le cadre de la décomposition hélicoïdale des champs solénoïdaux - une idée similaire à la décomposition de la lumière en composantes polarisées et que nous sommes les premiers à appliquer à la MHD. Nous avons montré comment exploiter cette approche pour déduire systématiquement des modèles simplifiés de la MHD. En particulier, nos méthodes multiplient le nombre de situations descriptibles par les modèles en couche comme par exemple le problème anisotrope de la turbulence en rotation. Elles permettent aussi de construire des modèles à basse dimension en calquant les résultats de simulations numériques directes. Ces modèles peuvent alors être étudiés à moindre coûts.
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Magnetohydrodynamics (MHD) is both the science and the formalism that describe the motion of an electro-conducting fluid. Such motion may yield the dynamo effect consisting in the spontaneous generation of a large scale stationary magnetic field. This phenomenon is most likely the reason behind the existence of planetary, stellar and galactic magnetic fields.
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Doctorat en Sciences
info:eu-repo/semantics/nonPublished
Giesecke, André. „Box-Simulationen von rotierender Magnetokonvektion im flüssigen Erdkern“. Phd thesis, Universität Potsdam, 2007. http://opus.kobv.de/ubp/volltexte/2007/1360/.
Der volle Inhalt der QuelleBox-simulations of rotating magnetoconvection in the Earth's fluid core. Simulations of the 3D MHD-equations have been performed using the code NIRVANA. The equations for compressible rotating magnetoconvection are numerically solved in a Cartesian box assuming conditions roughly suitable for the geodynamo. The characteristics of averaged quantities like the turbulence intensity and the turbulent heat flux that are caused by the combined action of the small-scale fluctuations are computed. The correlation length of the turbulence significantly depends on the strength and orientation of the magnetic field and the anisotropic behavior of the turbulence intensity induced by Coriolis and Lorentz force is considerably more pronounced for faster rotation. The development of an isotropic behavior on the small scales -- as it is observed in pure rotating convection -- vanishes even for weak magnetic fields, which results in a turbulent flow that is dominated by the vertical component. In the presence of a horizontal magnetic field the vertical turbulent heat flux slightly increases with increasing field strength, so that cooling of the rotating system is facilitated. Horizontal transport of heat is always directed westwards and towards the poles. The latter might be a source of a large-scale meridional flow whereas the first would be important in global simulations in case of non-axisymmetric boundary conditions for the heat flux. The mean electromotive force describing the generation of mean magnetic flux by turbulence in the rotating fluid is directly calculated from the simulations and the corresponding α-coefficients are derived. Due to the very weak density stratification, the α-effect changes its sign in the middle of the box. It is positive at the top and negative at the bottom of the convective instable layer. For strong magnetic fields we also find a clear downward advection of the mean magnetic field. Finally the quenching behavior of the α-effect in dependence of the imposed magnetic field strength is presented. A geodynamo-model is constructed, which is based on an α-effect that has been computed from the box simulations. For a highly restricted class of radial α-profiles the linear α^2-model exhibits oscillating solutions on a timescale given by the turbulent diffusion time. The basic properties of the periodic solutions are presented and the influence of the inner core size on the characteristics of the critical range that allows for oscillating solutions is shown. Reversals are interpreted as half of such an oscillation. They are rather seldom events because they can only occur if the α-profile exists long enough within the small critical range that allows for periodic solutions. Due to strong fluctuations on the convective timescale the probability of such a reversal is very small. Finally, a simple non-linear mean-field model with reasonable input parameters based on the box-simulations demonstrates the plausibility of the presented theory with a long-time series of a (geo-)dynamo reversal sequence.
Persson, Åsa, und Bengt Sundberg. „Effekter av utbildning till personer som lever med epilepsi : en litteraturöversikt“. Thesis, Hälsohögskolan, Högskolan i Jönköping, HHJ, Avd. för omvårdnad, 2014. http://urn.kb.se/resolve?urn=urn:nbn:se:hj:diva-23959.
Der volle Inhalt der QuelleBackground: Living with epilepsy leads to increased psychological stress. People with epilepsy often have insufficient knowledge about the disease and the need for education is essential. The person needs to learn the symptoms and ways to avoid exposing themselves to situations that may trigger seizures. Health professionals have an important role in education, counseling and support to people with epilepsy and their families. The aim of this literature overview was to describe and evaluate the effects of education to people with epilepsy and / or its family. To answer this, a literature overview was selected as a method consisting of scientific articles with a quantitative approach. The result showed that to educate individuals and / or its family in the knowledge of epilepsy and self-care ability could be successfully be carried out. Quality of life in people with epilepsy does not seem to get effect of patient education. The conclusion was that education seems to have positive effect for people with epilepsy on knowledge and self-care ability. Continued research with randomized, controlled trials with larger sample would be of great value to further increase the knowledge about the effects of education in people living with epilepsy.
Bücher zum Thema "Effet MHD"
Goreham, Steve. The mad, mad, mad world of climatism: Mankind and climate change mania. New Lenox, IL: New Lenox Books, 2013.
Den vollen Inhalt der Quelle findenHoxter, Holly Nicole. The Snowball Effect. New York: HarperCollins, 2010.
Den vollen Inhalt der Quelle findenHealth Effects Research Laboratory (Research Triangle Park, N.C.), Hrsg. Cerebellar histogenesis in rats exposed to 2450 MHz microwave radiation: Project summary. Research Triangle Park, NC: U.S. Environmental Protection Agency, Health Effects Research Laboratory, 1988.
Den vollen Inhalt der Quelle findenHealth Effects Research Laboratory (Research Triangle Park, N.C.), Hrsg. Cerebellar histogenesis in rats exposed to 2450 MHz microwave radiation: Project summary. Research Triangle Park, NC: U.S. Environmental Protection Agency, Health Effects Research Laboratory, 1988.
Den vollen Inhalt der Quelle finden1935-, Gandhi Om P., und Health Effects Research Laboratory (Research Triangle Park, N.C.), Hrsg. Behavior, physiology, and energy deposition in rats chronically exposed to 2450 MHz radiation: Project summary. Research Triangle Park, NC: U.S. Environmental Protection Agency, Health Effects Research Laboratory, 1988.
Den vollen Inhalt der Quelle finden1935-, Gandhi Om P., und Health Effects Research Laboratory (Research Triangle Park, N.C.), Hrsg. Behavior, physiology, and energy deposition in rats chronically exposed to 2450 MHz radiation: Project summary. Research Triangle Park, NC: U.S. Environmental Protection Agency, Health Effects Research Laboratory, 1988.
Den vollen Inhalt der Quelle findenBornmalm-Jardelöw, Gunilla. Högre utbildning och arbetsmarknad: En studie med tillämpningar på svenska förhållanden. [Gothenburg: Nationalekonomiska institutionen, Handelshögskolan vid Göteborgs universitet, 1988.
Den vollen Inhalt der Quelle findenOverrein, Øystein. Virkninger av motorferdsel på fauna og vegetasjon: Kunnskapsstatus med relevans for Svalbard. Tromsø: Norsk Polarinstitutt, 2002.
Den vollen Inhalt der Quelle findenMitchell, Juliet. Mad men and Medusas: Reclaiming hysteria and the effect of sibling relationships on the human condition. London: Penguin, 2000.
Den vollen Inhalt der Quelle findenMitchell, Juliet. Mad men and Medusas: Reclaiming hysteria and the effect of sibling relationships on the human condition. London: Allen Lane The Penguin Press, 2000.
Den vollen Inhalt der Quelle findenBuchteile zum Thema "Effet MHD"
Ferrone, S., M. De Felice, M. C. Turco, L. Corbo und S. Venuta. „Effect of Anti-HLA Class I Monoclonal Antibodies on the Proliferation of T Cells Induced by PHA-P. Comparison with the Effect on T Cell Activation via the CD2 and CD3 Pathways“. In MHC + X, 100–106. Berlin, Heidelberg: Springer Berlin Heidelberg, 1988. http://dx.doi.org/10.1007/978-3-642-74026-8_16.
Der volle Inhalt der QuelleAhmed, Nazibuddin. „MHD Flow with Soret Effect and Induced Magnetic Field“. In Thermal and Solutal Convection in Some Hydromagnetic Flows, 69–91. Singapore: Springer Nature Singapore, 2022. http://dx.doi.org/10.1007/978-981-19-7153-2_4.
Der volle Inhalt der QuelleLiao, Yingke, Guiping Zhu und Jie Wang. „Numerical Simulation of the Electrode Degradation Effect on Faraday MHD Accelerator“. In 2023 Asia-Pacific International Symposium on Aerospace Technology (APISAT 2023) Proceedings, 158–67. Singapore: Springer Nature Singapore, 2024. http://dx.doi.org/10.1007/978-981-97-4010-9_12.
Der volle Inhalt der QuelleHouerou, H. N. „Global Change: Population, Land-Use and Vegetation in the Mediterranean Basin by the Mid-21st Century“. In Greenhouse Effect, Sea Level and Drought, 301–67. Dordrecht: Springer Netherlands, 1990. http://dx.doi.org/10.1007/978-94-009-0701-0_19.
Der volle Inhalt der QuelleBojarevics, Valdis. „MHD of Aluminium Cells with the Effect of Channels and Cathode Perturbation Elements“. In Light Metals 2013, 609–14. Hoboken, NJ, USA: John Wiley & Sons, Inc., 2013. http://dx.doi.org/10.1002/9781118663189.ch104.
Der volle Inhalt der QuelleBojarevics, Valdis. „Effect of Cathode Collector Copper Inserts on the Hall-Héroult Cell MHD Stability“. In Light Metals 2016, 933–38. Cham: Springer International Publishing, 2016. http://dx.doi.org/10.1007/978-3-319-48251-4_157.
Der volle Inhalt der QuelleBojarevics, Valdis. „Effect of Cathode Collector Copper Inserts on the Hall-HéRoult Cell MHD Stability“. In Light Metals 2016, 933–38. Hoboken, NJ, USA: John Wiley & Sons, Inc., 2016. http://dx.doi.org/10.1002/9781119274780.ch157.
Der volle Inhalt der QuelleBojarevics, Valdis. „MHD of Aluminium Cells with the Effect of Channels and Cathode Perturbation Elements“. In Light Metals 2013, 609–14. Cham: Springer International Publishing, 2003. http://dx.doi.org/10.1007/978-3-319-65136-1_104.
Der volle Inhalt der QuelleSingh, Alok, Savita Singh und Sudhir Kumar Sharma. „Mathematical Modeling: Magnetic Field Effect on Oscillatory MHD Couette Two Dimensional Flow Regime“. In Lecture Notes in Mechanical Engineering, 439–49. Singapore: Springer Nature Singapore, 2023. http://dx.doi.org/10.1007/978-981-19-8517-1_33.
Der volle Inhalt der QuelleAhmed, Nazibuddin, und Bijoy Krishna Taid. „MHD Forced Convection from an Infinite Horizontal Porous Plate with Thermal Diffusion Effect“. In Advances in Intelligent Systems and Computing, 253–68. Singapore: Springer Nature Singapore, 2023. http://dx.doi.org/10.1007/978-981-19-8054-1_14.
Der volle Inhalt der QuelleKonferenzberichte zum Thema "Effet MHD"
Frisbie, C. Daniel. „Electrolyte gated transistors and inverters operating at 10 MHz (Conference Presentation)“. In Organic and Hybrid Field-Effect Transistors XXI, herausgegeben von Oana D. Jurchescu und Iain McCulloch. SPIE, 2022. http://dx.doi.org/10.1117/12.2633938.
Der volle Inhalt der QuelleLitwin, C. „Microinstabilities effect on MHD modes“. In Radio−frequency power in plasmas. AIP, 1989. http://dx.doi.org/10.1063/1.38490.
Der volle Inhalt der QuelleKrasilnikov, Arthur, Valeriy Knotko und Valentin Bityurin. „MHD Effect Study at High Frequency Plasmatron“. In 42nd AIAA Aerospace Sciences Meeting and Exhibit. Reston, Virigina: American Institute of Aeronautics and Astronautics, 2004. http://dx.doi.org/10.2514/6.2004-1198.
Der volle Inhalt der QuelleHamba, Fujihiro. „DYNAMO EFFECT IN MHD TURBULENT CHANNEL FLOW“. In Sixth International Symposium on Turbulence and Shear Flow Phenomena. Connecticut: Begellhouse, 2009. http://dx.doi.org/10.1615/tsfp6.1110.
Der volle Inhalt der QuelleSingh, Ranjit J., und Trushar Gohil. „EFFECT OF MHD ON RAYLEIGH-BENARD CONVECTION“. In Proceedings of the 24th National and 2nd International ISHMT-ASTFE Heat and Mass Transfer Conference (IHMTC-2017). Connecticut: Begellhouse, 2018. http://dx.doi.org/10.1615/ihmtc-2017.2650.
Der volle Inhalt der QuelleShalybkov, Dima. „Taylor-Couette flow stability: effect of vertical density stratification and azimuthal magnetic fields“. In MHD COUETTE FLOWS: Experiments and Models. AIP, 2004. http://dx.doi.org/10.1063/1.1832146.
Der volle Inhalt der QuelleAnwari, Makbul, und Sukarsan. „Effect of magnetic field on a Diagonal MHD Accelerator“. In 2008 IEEE Vehicle Power and Propulsion Conference (VPPC). IEEE, 2008. http://dx.doi.org/10.1109/vppc.2008.4677759.
Der volle Inhalt der QuelleLin, Zuowei, Yan Peng, Lingzhi Zhao, Ciwen Sha, Yuyu Xu, Ran Li und Jason Jia. „Analytical Study on End Effect of Liquid Metal MHD Generator“. In 38th Plasmadynamics and Lasers Conference. Reston, Virigina: American Institute of Aeronautics and Astronautics, 2007. http://dx.doi.org/10.2514/6.2007-4514.
Der volle Inhalt der QuelleMunipalli, Ramakanth, Shashi Aithal und Vijaya Shankar. „Effect of Wall Conduction in Proposed MHD Enhanced Hypersonic Vehicles“. In 12th AIAA International Space Planes and Hypersonic Systems and Technologies. Reston, Virigina: American Institute of Aeronautics and Astronautics, 2003. http://dx.doi.org/10.2514/6.2003-6921.
Der volle Inhalt der QuelleParent, Bernard, Prasanna T. Rajendran, Robert W. Moses, Christopher O. Johnston, F. M. Cheatwood, Sergey O. Macheret und Justin Little. „Effect of Plasma Sheaths on Earth Re-entry MHD Processes“. In AIAA SCITECH 2022 Forum. Reston, Virginia: American Institute of Aeronautics and Astronautics, 2022. http://dx.doi.org/10.2514/6.2022-0980.
Der volle Inhalt der QuelleBerichte der Organisationen zum Thema "Effet MHD"
R.B. White, Ya.I. Kolesnichenko, V.V. Lutsenko und V.S. Marchenko. Effect of Trapped Energetic Ions on MHD Activity in Spherical Tori. Office of Scientific and Technical Information (OSTI), Mai 2002. http://dx.doi.org/10.2172/798181.
Der volle Inhalt der QuelleChu, M. S., J. M. Greene, T. H. Jensen, R. L. Miller, A. Bondeson, R. W. Johnson und M. E. Mauel. Effect of toroidal plasma flow and flow shear on global MHD modes. Office of Scientific and Technical Information (OSTI), Januar 1995. http://dx.doi.org/10.2172/10118062.
Der volle Inhalt der QuelleOno, M., D. Stutman und Y. S. Hwang. Investigation of the effect of resistive MHD modes on spherical torus performance in CDX-U. Office of Scientific and Technical Information (OSTI), Januar 1997. http://dx.doi.org/10.2172/304212.
Der volle Inhalt der QuelleLi, wanlin, jie Yun, siying He, ziqi Zhou und ling He. Effect of different exercise therapies on fatigue in maintenance hemodialysis patients:A Bayesian Network Meta-analysis. INPLASY - International Platform of Registered Systematic Review and Meta-analysis Protocols, November 2022. http://dx.doi.org/10.37766/inplasy2022.11.0144.
Der volle Inhalt der QuelleNatesan, K. Characterization of deposits and effect of deposits on corrosion of materials for MHD balance-of-plant applications. Office of Scientific and Technical Information (OSTI), Dezember 1993. http://dx.doi.org/10.2172/142545.
Der volle Inhalt der QuelleNelson, Gena, Angela Crawford und Jessica Hunt. A Systematic Review of Research Syntheses for Students with Mathematics Learning Disabilities and Difficulties. Boise State University, Albertsons Library, Januar 2022. http://dx.doi.org/10.18122/sped.143.boisestate.
Der volle Inhalt der QuelleD.I. Simon, E. Marmar, N.L. Bretz, R. Bravenec und R.F. Parsells. Optical and Mechanical Design of C-Mod Motional Stark Effect Diagnostic. Office of Scientific and Technical Information (OSTI), November 1999. http://dx.doi.org/10.2172/14501.
Der volle Inhalt der QuelleAdamovich, Igor V. Experimental and Computational Study of the Effect of MHD Forces on Stability and Separation of Nonequilibrium Ionized Supersonic Flow. Fort Belvoir, VA: Defense Technical Information Center, Juli 2005. http://dx.doi.org/10.21236/ada437407.
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Der volle Inhalt der QuelleJeppsson, Knut-Håkan, Madeleine Magnusson, Sara Bergström Nilsson, Lisa Ekman, Louise Winblad von Walter, Lars-Erik Jansson, Håkan Landin und Christer Bergsten. Fiberströ till mjölkkor – effekt på djurvälfärd, djurhälsa, mjölkkvalitet och kostnaden för strömedel. Fakulteten för landskapsarkitektur, trädgårds- och växtproduktionsvetenskap, Sveriges lantbruksuniversitet, 2023. http://dx.doi.org/10.54612/a.5nqtckgl7i.
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