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NASA Scientific and Technical Aerospace Reports

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20040120896 Georgia Inst. of Tech., Atlanta, GA, USA<br />

Annual Report of the Fusion Research Center, Georgia Institute of Technology, 2003<br />

Stacey, W. M.; M<strong>and</strong>rekas, J.; Dec. 2003; 24 pp.; In English<br />

Report No.(s): PB2004-105911; No Copyright; Avail: CASI; A03, Hardcopy<br />

Contents include the following: Next Step Option Design Studies (DOE Grant ER54350) (Fusion Transmutation of<br />

Nuclear Waste; Toroidal Rotation <strong>and</strong> Radial Electric Field in Edge Pedestal).<br />

NTIS<br />

Nuclear Fusion; Radioactive Wastes<br />

20040120923 Princeton Univ., NJ<br />

MHD Ballooning Instability in the Plasma Sheet<br />

Cheng, C. Z.; Zaharia, S.; Oct. 2003; In English<br />

Report No.(s): DE2004-820113; PPPL-3890; No Copyright; Avail: National <strong>Technical</strong> Information Service (NTIS)<br />

Based on the ideal-MHD model the stability of ballooning modes is investigated by employing realistic 3D<br />

magnetospheric equilibria, in particular for the substorm growth phase. Previous MHD ballooning stability calculations<br />

making use of approximations on the plasma compressibility can give rise to erroneous conclusions. Our results show that<br />

without making approximations on the plasma compressibility the MHD ballooning modes are unstable for the entire plasma<br />

sheet where beta (sub)eq is greater than or equal to 1, <strong>and</strong> the most unstable modes are located in the strong cross-tail current<br />

sheet region in the near-Earth plasma sheet, which maps to the initial brightening location of the breakup arc in the ionosphere.<br />

However, the MHD beq threshold is too low in comparison with observations by AMPTE/CCE at X= -(8 - 9)R(sub)E, which<br />

show that a low-frequency instability is excited only when beq increases over 50. The difficulty is mitigated by considering<br />

the kinetic effects of ion gyrorad ii <strong>and</strong> trapped electron dynamics, which can greatly increase the stabilizing effects of field<br />

line tension <strong>and</strong> thus enhance the beta(sub)eq threshold (Cheng <strong>and</strong> Lui, 1998). The consequence is to reduce the equatorial<br />

region of the unstable ballooning modes to the strong cross-tail current sheet region where the free energy associated with the<br />

plasma pressure gradient <strong>and</strong> magnetic field curvature is maximum.<br />

NTIS<br />

Magnetohydrodynamic Stability; Plasmas (Physics)<br />

20040120925 Princeton Univ., NJ<br />

Turbulence Spreading into Linearly Stable Zone <strong>and</strong> Transport Scaling<br />

Hahm, T. S.; Diamond, P. H.; Lin, Z.; Itoh, K.; Itoh, S. I.; Oct. 2003; In English<br />

Report No.(s): DE2004-820109; PPPL-3887; No Copyright; Avail: National <strong>Technical</strong> Information Service (NTIS)<br />

We study the simplest problem of turbulence spreading corresponding to the spatio-temporal propagation of a patch of<br />

turbulence from a region where it is locally excited to a region of weaker excitation, or even local damping. A single model<br />

equation for the local turbulence intensity I(x, t) includes the effects of local linear growth <strong>and</strong> damping, spatially local<br />

nonlinear coupling to dissipation <strong>and</strong> spatial scattering of turbulence energy induced by nonlinear coupling. In the absence of<br />

dissipation, the front propagation into the linearly stable zone occurs with the property of rapid progression at small t, followed<br />

by slower subdiffusive progression at late times. The turbulence radial spreading into the linearly stable zone reduces the<br />

turbulent intensity in the linearly unstable zone, <strong>and</strong> introduces an additional dependence on the rho* is always equal to rho<br />

i/a to the turbulent intensity <strong>and</strong> the transport scaling. These are in broad, semi-quantitative agreements with a number of<br />

global gyrokinetic simulation results with zonal flows <strong>and</strong> without zonal flows. The front propagation stops when the radial<br />

flux of fluctuation energy from the linearly unstable region is balanced by local dissipation in the linearly stable region.<br />

NTIS<br />

Turbulence; Spreading; Nonlinearity; Energy Dissipation<br />

76<br />

SOLID-STATE PHYSICS<br />

Includes condensed matter physics, crystallography, <strong>and</strong> superconductivity. For related information see also 33 Electronics <strong>and</strong><br />

Electrical Engineering; <strong>and</strong> 36 Lasers <strong>and</strong> Masers.<br />

20040111142 Lockheed Martin Corp., Syracuse, NY, USA<br />

Wafer-Bonded Internal Back-Surface Reflectors for Enhanced TPV Performance<br />

Wang, C. A.; Murphy, P. G.; O’Brien, P. W.; Shiau, D. A.; Anderson, A. C.; Aug. 2002; In English<br />

Report No.(s): DE2004-821703; LM-02K065; No Copyright; Avail: National <strong>Technical</strong> Information Service (NTIS)<br />

299

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