Show simple item record

dc.contributor.advisorMiklos Porkolab.en_US
dc.contributor.authorDorris, James Robert, IIIen_US
dc.contributor.otherMassachusetts Institute of Technology. Dept. of Physics.en_US
dc.date.accessioned2011-05-23T15:29:55Z
dc.date.available2011-05-23T15:29:55Z
dc.date.copyright2010en_US
dc.date.issued2010en_US
dc.identifier.urihttp://hdl.handle.net/1721.1/62872
dc.descriptionThesis (Ph. D.)--Massachusetts Institute of Technology, Dept. of Physics, 2010.en_US
dc.descriptionThis electronic version was submitted by the student author. The certified thesis is available in the Institute Archives and Special Collections.en_US
dc.descriptionCataloged from student submitted PDF version of thesis.en_US
dc.descriptionIncludes bibliographical references (p. 203-212).en_US
dc.description.abstractThe DIII-D phase contrast imaging (PCI) diagnostic has been upgraded and used to measure turbulence in the outer plasma region (0.7 < r/a < 1). These upgrades extended its operational range to high frequencies (10 kHz - 10 MHz), short wavelength (2 - 30 cm-1), and improved the signal-to-noise ratio by 10X, as well as provided a novel rotating mask to measure turbulence as a function of propagation angle about the PCI chord. Turbulent fluctuations that propagate perpendicular to the magnetic field direction can be localized by making use of the variation of the magnetic field component perpendicular to the viewing chord as a function of chord height. Long wavelength (IkI . 12 cm-1) turbulence is shown to be a branch in frequency and wave-number space, and is localized to within the instrumental width of the last closed flux surface (LCFS) (r/a & 0.9). Three classes of turbulence with finite (and theoretically unexpected) kII have been identified: (i) modes that are localized in wave-number and mask angle (the high-k and medium-k modes), (ii) a broad (in mask angle) background turbulence, and (iii) a low-k "wing" that smears the main branch structure. These modes are seen to propagate at angles as large as kII/k ~ 0.1 - 0.4. ECH heating is observed to increase the spectral power density in the high-k mode (-24 < k < -18 cm-1), and the parallel wave-numbers are measured to be as large as kII/k ~ 0.15. The applied heating is shown to increase the electron temperature gradient drive (inverse scale-length, 1/LTe) and decrease the ion temperature and density gradient drives (1/LTi and 1/Ln). Using a basic temperature gradient driven drift-wave model in slab geometry, it is shown that finite (and relatively high) kII modes could interact resonantly with ions through the ion cyclotron Doppler resonance terms [xi]±1i = (w± [omega]i)/(kIIvti) ~ 1. These m = / \ 0 terms in the dispersion relation are not included in the derivation of the gyrokinetic equations.en_US
dc.description.statementofresponsibilityby James Robert Dorris III.en_US
dc.format.extent212 p.en_US
dc.language.isoengen_US
dc.publisherMassachusetts Institute of Technologyen_US
dc.rightsM.I.T. theses are protected by copyright. They may be viewed from this source for any purpose, but reproduction or distribution in any format is prohibited without written permission. See provided URL for inquiries about permission.en_US
dc.rights.urihttp://dspace.mit.edu/handle/1721.1/7582en_US
dc.subjectPhysics.en_US
dc.titlePhase contrast imaging measurements and modeling of short wavelength turbulence in the DIII-D tokamaken_US
dc.typeThesisen_US
dc.description.degreePh.D.en_US
dc.contributor.departmentMassachusetts Institute of Technology. Department of Physics
dc.identifier.oclc720929007en_US


Files in this item

Thumbnail

This item appears in the following Collection(s)

Show simple item record