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NASA Scientific and Technical Aerospace Reports

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calculating power generation <strong>and</strong> usage (power-flow, power contingencies, specific power). The report represents a general<br />

consensus of the nuclear fusion space propulsion system conceptual design community <strong>and</strong> proposes 15 recommendations.<br />

This paper exp<strong>and</strong>s on the Report by providing specific examples illustrating how to apply each of the recommendations.<br />

Author<br />

Design Analysis; Nuclear Fusion; Propulsion<br />

20040112050 <strong>NASA</strong> Glenn Research Center, Clevel<strong>and</strong>, OH, USA<br />

An Operator Method for Field Moments from the Extended Parabolic Wave Equation <strong>and</strong> Analytical Solutions of the<br />

First <strong>and</strong> Second Moments for Atmospheric Electromagnetic Wave Propagation<br />

Manning, Robert M.; [2004]; 21 pp.; In English<br />

Contract(s)/Grant(s): WBS 22-302-20-2F; No Copyright; Avail: CASI; A03, Hardcopy<br />

The extended wide-angle parabolic wave equation applied to electromagnetic wave propagation in r<strong>and</strong>om media is<br />

considered. A general operator equation is derived which gives the statistical moments of an electric field of a propagating<br />

wave. This expression is used to obtain the first <strong>and</strong> second order moments of the wave field <strong>and</strong> solutions are found that<br />

transcend those which incorporate the full paraxial approximation at the outset. Although these equations can be applied to<br />

any propagation scenario that satisfies the conditions of application of the extended parabolic wave equation, the example of<br />

propagation through atmospheric turbulence is used. It is shown that in the case of atmospheric wave propagation <strong>and</strong> under<br />

the Markov approximation (i.e., the delta-correlation of the fluctuations in the direction of propagation), the usual parabolic<br />

equation in the paraxial approximation is accurate even at millimeter wavelengths. The comprehensive operator solution also<br />

allows one to obtain expressions for the longitudinal (generalized) second order moment. This is also considered <strong>and</strong> the<br />

solution for the atmospheric case is obtained <strong>and</strong> discussed. The methodology developed here can be applied to any qualifying<br />

situation involving r<strong>and</strong>om propagation through turbid or plasma environments that can be represented by a spectral density<br />

of permittivity fluctuations.<br />

Author<br />

Electromagnetic Wave Transmission; Wave Propagation; Atmospheric Turbulence; Wave Equations<br />

20040120850 Stanford Linear Accelerator Center, Stanford, CA, USA<br />

Direct Measurement of A(sub b) in Z(sup 0) Decays Using Charged Kaon Tagging<br />

Dec. 1998; 14 pp.; In English<br />

Report No.(s): DE2004-9928; SLAC-PUB-7959; No Copyright; Avail: Department of Energy Information Bridge<br />

We present a direct measurement of the parity-violating asymmetry A(sub b) in the Z(sup 0) to b anti-b coupling using<br />

a new technique to distinguish the b <strong>and</strong> anti-b quarks using charged kaons from B decays. The Z(sup 0) bosons are produced<br />

in e(sup+)e(sup -) collisions at the SLC with longitudinally polarized electrons. b anti-b events are selected using a secondary<br />

vertex mass tag <strong>and</strong> A(sub b) is determined from the left-right forward-backward asymmetry. From the 1994-1995 data<br />

sample, selected from 100,000 hadronic Z(sup 0) decays, we obtain A(sub b)= 0.855(+-) 0. 088(sub stat)(+-) 0. 102(sub sys).<br />

NTIS<br />

Particle Decay; Asymmetry; Quarks; Kaons<br />

20040120852 Fermi National Accelerator Lab., Batavia, IL, USA<br />

pH <strong>and</strong> Resistivity of the BCP Mix Diluted in UPW<br />

Boffo, C.; Connolly, D.; Hicks, D.; Hoffman, J.; May 2004; 18 pp.; In English<br />

Report No.(s): DE2004-823614; FERMILAB-TM-2233; No Copyright; Avail: Department of Energy Information Bridge<br />

Etching plays an important role in the production of superconducting cavities (SRF). As other laboratories engaged in RF<br />

superconductivity R <strong>and</strong> D did, FNAL is also developing a facility for the chemical etching of niobium (Nb) cavities. Two<br />

techniques are common accepted for cavity etching: (1) chemical etching--buffered chemical polishing (BCP); <strong>and</strong> (2)<br />

Electropolishing (EP). Among them, at FNAL it was decided to pursue chemical etching, which is considered a reliable<br />

technique tested by several labs for many years. In the past, numerous mixtures of acids have been tested leading to the actual<br />

buffered chemical polishing mix (BCP) characterized by the following composition by volume: 1 of HF 49 %wt; 1 of<br />

HNO(sub 3) 69.5 %wt; 2 of H(sub 3)PO(sub 4) 85 %wt. Because of the dangerous nature of the chemicals involved, safety<br />

considerations require the development of a proper process <strong>and</strong> a reliable control algorithm. For the post-processing rinsing<br />

of the cavities, one needs to know the expected pH of the water used to rinse the cavity. On the other h<strong>and</strong>, for early detection<br />

of leaks in the hydraulic system, which is done by measuring the conductivity of the rinsing water used in the process, one<br />

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