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Showing 1 to 20 of 307 for “"Ionized"”.
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Magnetohydrodynamic containment in partially ionized gases
Thesis (Sc. D.)--Massachusetts Institute of Technology, Dept. of Mechanical Engineering, 1962.
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Calculations for charge-transfer in collisions of triply-ionized nitrogen and doubly-ionized sulphur with hydrogen atoms
Submitted by Carolyn Mead (cmead2@illinois.edu) on 2011-06-27T14:28:46Z No. of bitstreams: 1 1980_christensen.pdf: 4732068 bytes, checksum: 8660538e8ef435236d68b745f3b846da (MD5)
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Shock Wave Dispersion in Weakly Ionized Gas
… wave modification in non-equilibrium weakly ionized gases and to clarify the physical mechanisms of the shock wave modification process. The discharge was generated in 99.99% Ar at a gas pressure between 20 and 100 Torr and at a discharge power density less than 10.0 Watts/cm<sup>3</sup>. …
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Ionized Physical Vapor Deposition of Aluminum Oxide
Made available in DSpace on 2017-07-06T18:55:08Z (GMT). No. of bitstreams: 3 Li_Ning_MS.pdf: 51415629 bytes, checksum: c29c8d58534efcdd114931c9fc6f3d8d (MD5) Li_Ning_MS_ABS.pdf: 619486 bytes, checksum: 41ecf59db6588595b2e30243525fce36 (MD5) license.txt: 4813 bytes, checksum: …
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Diagnostics for ionized physical vapor deposition chambers
As the critical dimension of the semiconductor device continues to shrink and aspect ratio continues to rise, more diagnostics are needed to accurately predict the deposition profile of features on the wafer. Traditionally, the incident ion fluxes are considered to be perfectly normal to the wafer …
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Properties of Free Jets of Ionized Nitrogen
Made available in DSpace on 2014-12-09T17:13:50Z (GMT). No. of bitstreams: 1 7013427.pdf: 3814452 bytes, checksum: 83aa5fc04fd3a1e007912e843d61c444 (MD5) Previous issue date: 1969
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Doubly Ionized K-Shell Following Radioactive Decay
Submitted by Carly Hafner (chafner2@illinois.edu) on 2013-09-27T22:43:13Z No. of bitstreams: 1 4183_0001.pdf: 17459179 bytes, checksum: a3c908d3c1647fbfe6831ab308b1be26 (MD5)
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Secondary Plasma Sources for Ionized Physical Vapor Deposition
The helicon antenna sits remotely outside the vacuum system, so all shadowing and contamination problems which the other two sources exhibit are eliminated. Ionization fractions to the substrate of 51 +/- 10% with a deposition rate of 847 +/- 42 A/min. are found. Without the antenna, the ionization …
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Laminar Duct Flow of a Partially Ionized Gas
Made available in DSpace on 2014-12-09T17:13:32Z (GMT). No. of bitstreams: 1 6500776.pdf: 2916483 bytes, checksum: d26b0980a7ceecd7c3c5b1a7e18b98bb (MD5) Previous issue date: 1964
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Fragmentation of magnetically-supported, weakly-ionized molecular clouds
… of isolated, magnetically-supported, weakly- ionized, self-gravitating molecular clouds in three dimensions. Although the model clouds are supported by the magnetic field, high-density, magnetically-supercritical fragments form due to the drift between the ions and the neutrals, ambipolar …
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Particle and energy fluxes in weakly ionized gases
Thesis (Ph. D.)--Massachusetts Institute of Technology, Dept. of Geology and Geophysics, 1963.
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Granular Alloy Film Synthesis Using Ionized Cluster Beam Deposition
… Films are grown by simultaneous deposition of ionized nanoclusters from a beam and of atoms from an evaporation source. The resultant films are of granular structure; that is, they have clusters of nanometer size embedded in a matrix. The potential and advantages of this method in creating a …
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Transport Properties of a Partially Ionized Gas-Solid Suspension
Made available in DSpace on 2014-12-09T17:13:39Z (GMT). No. of bitstreams: 1 6612460.pdf: 2836283 bytes, checksum: 2d383464393675d0c87205c87677b83b (MD5) Previous issue date: 1966
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Turbulent Angular Momentum Transport in Weakly-Ionized Accretion Disks
… transport of angular momentum has revolutionized the field. Much of accretion disk research now focuses on understanding the implications of this mechanism for astrophysical observations. At the same time, the success of this mechanism depends upon a sufficient ionization level in the disk …
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Untangling compact and diffuse ionized emission toward galactic hii regions
HII regions are clouds of ionized hydrogen gas surrounding B0- and O-type stars. The ionized hydrogen in these regions emits both radio recombination line (RRL) and also thermal radio continuum. Diffuse ionized hydrogen, known as the 'Warm Ionized Medium' (WIM) also exists in the Galaxy. The WIM …
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The production and study of a thermally ionized cesium plasma
Thesis (B.S.)--Massachusetts Institute of Technology, Dept. of Physics, 1961.
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