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The Global ETD Search service is a free service for researchers
to find electronic theses and dissertations. This service is
provided by the
Networked Digital Library of Theses and Dissertations.
Our metadata is collected from universities around the world. If you manage a university/consortium/country archive and want to be added, details can be found on the NDLTD website.
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Showing 11 to 20 of 322 (0.058 seconds)Spelling suggestions: "subject:"magnetohydrodynamic""
| 11 |
The effect of interparticle forces on fluidization regimes: a study of magnetized fluidized bedsLee, Woo-Kul 29 April 1994 (has links)
Graduation date: 1994
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| 12 |
An experimental study of the motion of a hydrogen plasma stream in a linear quadrupole magnetic fieldBarney, Gerald Orville, January 1967 (has links)
Thesis (Ph. D.)--University of Wisconsin, 1967. / Typescript. Vita. eContent provider-neutral record in process. Description based on print version record. Includes bibliographical references.
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| 13 |
Cosmological magnetic fields in the early universeChristensson, Mattias January 2001 (has links)
No description available.
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| 14 |
An analytical study of laminar free convection about a vertical flat plate in an electrically conducting fluid with presence of uniform transverse magnetic and electrical fields /Sun, Yung Ho January 1962 (has links)
No description available.
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| 15 |
A study of low frequency oscillations in a rarefied magnetoplasma /Block, Joseph Leon January 1968 (has links)
No description available.
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| 16 |
A study of hydromagnetic wavesHudson, Billy Charles. January 1960 (has links)
Call number: LD2668 .T4 1960 H69
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| 17 |
Heat transfer to a MHD fluid in a flat duct with constant heat flux at the wallsKnieper, Philip J. January 1965 (has links)
Call number: LD2668 .T4 1965 K69 / Master of Science
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| 18 |
MAGNETOHYDRODYNAMIC DYNAMO IN DISC-LIKE ASTROPHYSICAL BODIES.STEPINSKI, TOMASZ FRANCISZEK. January 1986 (has links)
Magnetohydrodynamic dynamo in disc-like astrophysical bodies has been considered for some time. Important astrophysical objects like accretion discs, protostellar and protoplanetary nebulae and galaxies are thought to regenerate a magnetic field through a dynamo mechanism. Although there is a well developed theory for describing the regeneration of magnetic field in these objects, there are not any specific methods how to calculate such magnetic fields in general case. In this work, after a description of the dynamo theory, the specific method for solving the nonspherical dynamo is introduced. The unique feature of this method is accommodation of variable magnetic diffusivity in order to model the shape of a disc-like body. The detailed construction of the method is presented, as well as description of mathematical and numerical methods used for obtaining the solution. The method of checking the model with respect to well established spherical models is also presented. Finally, some examples are calculated and discussion is given on the behaviour of calculated magnetic field and possible astrophysical implications.
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| 19 |
A numerical study of magnetic and non-magnetic geophysical fluid dynamicsFotheringham, Paul January 2000 (has links)
No description available.
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| 20 |
Lattice Boltzmann magnetohydrodynamicsWood, Andrew Maclean January 1999 (has links)
No description available.
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