of rally and race cars, as well as his own concourse winning Audi 90 quattro. He is a qualified engineer A 1994 UrS4, right-hand drive, living happily in Australia. The car has 59,000 miles on the odome- ter the car, and, on dyno testing, always had excessively rich AFR ratios and excessively low power. I
Riley, Shawn J.
-Being Cities - Michigan 27 UR1b Well-Being Detroit - Michigan 28 UR2a Assess Cities 29 January 13, 2003 #12;Michigan State of the State 28 Page ii item page UR2b Assess Detroit 29 UR4a1 Schools - Michigan Cities 30 - Detroit City 34 UR4b2 Roads - Detroit City 35 UR4b3 Public Transportation - Detroit City 35 UR4b4 Housing
Morden, Margaret Elizabeth
was then broken down into four one-meter grids called upper left (UL), upper right (UR), lower left (LL) and lower right (LR, '. These one-meter grids were then further div1ded into 4 half- meter squares des1gnated by numerals. This system enabled one... type (Append1ces I and II), with the1r significant deta1ls noted, making the information accessible for future study. UL 1 UL 2 UR 1 UR 2 UL3 UL4 UR3 UR4 LL1 LL 2 LR1 LR 2 LL3 LL4 LR3 LR 4 I11. 4. Section of Grid System on Glass W?eck 22 30 24...
G. M. von Hippel
This new version of TaylUR is based on a completely new core, which now is able to compute the numerical values of all of a complex-valued function's partial derivatives up to an arbitrary order, including mixed partial derivatives.
Recommendations and Justifications To Remove Use Restrictions Established under the U.S. Department of Energy, National Nuclear Security Administration Nevada Field Office Federal Facility Agreement and Consent Order, Revision 0
Birney, Cathleen; Krauss, Mark J
This document is part of an effort to reevaluate 37 FFACO and Administrative URs against the current Soils Risk-Based Corrective Action Evaluation Process. After reviewing 37 existing FFACO and Administrative URs, 3 URs addressed in this document have sufficient information to determine that these current URs may be removed, based on the RBCA criteria. This document presents recommendations on modifications to existing URs that will be consistent with the RBCA criteria.
Hua-Xing Chen; V. Dmitrasinovic; Hiroshi Toki
We study the SU(3) linear sigma model for the pseudoscalar mesons in the Gaussian Functional Approximation (GFA). We use the SU(3) linear sigma model Lagrangian with nonet scalar and pseudo-scalar mesons including symmetry breaking terms. In the GFA, we take the Gaussian Ansatz for the ground state wave function and apply the variational method to minimize the ground state energy. We derive the gap equations for the dressed meson masses, which are actually just variational parameters in the GFA method. We use the Bethe-Salpeter equation for meson-meson scattering which provides the masses of the physical nonet mesons. We construct the projection operators for the flavor SU(3) in order to work out the scattering T-matrix in an efficient way. In this paper, we discuss the properties of the Nambu-Goldstone bosons in various limits of the chiral $U_L(3)\\times U_R(3)$ symmetry.
of 1'58. Two taste . !-n. lo . !ere us?i' ? an oxf crt fin& non-evi srt taste 2! nel. The iix?ort fan?!1 ?nnioted ci' cix i?ricul+ur 3 an' ' ech!inicfll ollege of TeXaa SmplOyc . ;!!lc !lad OX?O"S" VO t&. at(~?" eX; erf enCe O"8 were Cap ?le Of' c... '. ?ET iCTEi TIAL FCF T"XAS FOFTIFIN R&X 38 67 CiiAPTER X B IHL IOGRAP HY AH '-'IX GiiAFEFRUIT JUICE CO', ~LUCIO". '. S. 74 80 Figure ', ''o. Page l. 2 ~ 3. Relationship between Index of Fading, Visual Color, and Lycopene and Carotene pie...
B. C. Kelly; T. A. McKay
We describe the application of the `shapelet' linear decomposition of galaxy images to multi-wavelength morphological classification using the $u,g,r,i,$ and $z$-band images of 1519 galaxies from the Sloan Digital Sky Survey. We utilize elliptical shapelets to remove to first-order the effect of inclination on morphology. After decomposing the galaxies we perform a principal component analysis on the shapelet coefficients to reduce the dimensionality of the spectral morphological parameter space. We give a description of each of the first ten principal component's contribution to a galaxy's spectral morphology. We find that galaxies of different broad Hubble type separate cleanly in the principal component space. We apply a mixture of Gaussians model to the 2-dimensional space spanned by the first two principal components and use the results as a basis for classification. Using the mixture model, we separate galaxies into three classes and give a description of each class's physical and morphological properties. We find that the two dominant mixture model classes correspond to early and late type galaxies, respectively. The third class has, on average, a blue, extended core surrounded by a faint red halo, and typically exhibits some asymmetry. We compare our method to a simple cut on $u-r$ color and find the shapelet method to be superior in separating galaxies. Furthermore, we find evidence that the $u-r=2.22$ decision boundary may not be optimal for separation between early and late type galaxies, and suggest that the optimal cut may be $u-r \\sim 2.4$.