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Grain types

Water-Vapor Permeability. Water-vapor permeabiUty depends on the polymer used for the coating layer and its stmcture. Vinyl-coated fabrics have Httie water-vapor permeabiUty due to the coating layer. Although polyurethane polymer is water-vapor permeable, urethane-coated fabrics also have low permeabiUty values due to their soHd layer stmcture. On the other hand, man-made leathers have good permeabiUty values as high as that of leather due to their porous layer stmcture. The permeabiUty of grain-type is lower than that of suede-type, influenced by finishing method. [Pg.92]

Figure 4. Photomicrograph of TS-23, a coarse-grained Type B1 inclusion from... Figure 4. Photomicrograph of TS-23, a coarse-grained Type B1 inclusion from...
A schematic summary presentation of four of these grain types is given in Figure 16.1. [Pg.274]

Type 14-Year Improved Howitzer — 692g in 3 increments of Mk 2 square grain Type 92 Gun — 4000g in 2 increments of Mark 3 strip... [Pg.457]

Backscattered electron image of a portion of a fine-grained Type A CAI in the Efremovka CV3 chondrite. This inclusion consists of nodules of spinel (sp) surrounded by anorthite (an) and thin rims of pyroxene (px). This CAI may be an aggregate of condensates. [Pg.203]

Fig. 3. Using the carbon replica technique, this is an electron micrograph of an Eastman Kodak T-Grain type emulsion of silver bromide that contains some iodide. (Photo by Dr. Donald L Black, Eastman Kodak Company)... Fig. 3. Using the carbon replica technique, this is an electron micrograph of an Eastman Kodak T-Grain type emulsion of silver bromide that contains some iodide. (Photo by Dr. Donald L Black, Eastman Kodak Company)...
Siwela, M., Taylor, J. R. N., de Milliano, W. A. J., and Duodu, K. G. (2007). Occurrence and location of tannins in finger millet grain and antioxidant activity of different grain types. Cereal Chem. 84,169-174. [Pg.261]

Grain Type Median Grain Size (pm) Specific Surface Area(m2g- ) BET-Measured Surface Area / Geometric Predicted Surface Area... [Pg.84]

Surface Relative Relative Specific Grain Type Roughness Surface Surface Areas... [Pg.84]

Walter L.M. (1983) The dissolution kinetics of shallow water carbonate grain types Effects of mineralogy, microstructure and dolution chemistry. Ph.D. dissertation, Univ. Miami, Miami, FL. [Pg.674]

Figure 2.7 Histograms of 12C/13C ratios of presolar SiC (all grain types), SiC X grains, and graphite. The solar ratio is indicated by the dashed line. Observed ranges of 12C/13C ratios in AGB stars and J-type carbon stars are shown for comparison. Figure 2.7 Histograms of 12C/13C ratios of presolar SiC (all grain types), SiC X grains, and graphite. The solar ratio is indicated by the dashed line. Observed ranges of 12C/13C ratios in AGB stars and J-type carbon stars are shown for comparison.
Type 96 How — 2930g in 5 increments of Mk 2 square grains Type 45 Gun j Type 7-Year Gun ... [Pg.457]

Type Y and Z Grains Type A + B Grains Type X Grains... [Pg.20]

Grain type Noble-gas components Size Abundance Stellar sources... [Pg.22]

Figure 3 Nitrogen and carbon isotopic ratios of individual presolar SiC grains. Because rare grain types were located by automatic ion imaging, the number of grains of different types do not correspond to their abundances in the meteorites these abundances are given in the legend (sources Alexander, 1993 Hoppe et al, 1994, 1996a Nittler et al, 1995 Huss et al, 1997 Amari et al, 2001a,b,c). Figure 3 Nitrogen and carbon isotopic ratios of individual presolar SiC grains. Because rare grain types were located by automatic ion imaging, the number of grains of different types do not correspond to their abundances in the meteorites these abundances are given in the legend (sources Alexander, 1993 Hoppe et al, 1994, 1996a Nittler et al, 1995 Huss et al, 1997 Amari et al, 2001a,b,c).
Clayton D. D., Arnett W. D., Kane J., and Meyer B. S. (1997) Type X silicon carbide presolar grains type la supernova condensates Artropliyi. J. 486, 824-834. [Pg.39]

Be /3-decays to °B with a half-life of 1.5 Myr. Evidence for its former existence in the solar system is provided by excesses of B/"B correlated with Be/B ratio (Figure 4), first found within coarse-grained (type B) CAIs from Allende (McKeegan et al., 2000a). From the slope of the correlation line, McKeegan et al. calculated an initial °Be/ Be = (9.5 1.9) X lO at the time corresponding to isotopic closure of the Be-B system. This discovery was rapidly confirmed and extended by analyses of a variety of CAIs of types A and B, and a FUN inclusion from various... [Pg.441]

It may sound like a paradox, but currently, in optimizing for a parallel computer most of the effort should be spent on making sure that the individual node performance is as good as possible. This is a consequence of the power of the individual node compared to the network latency and bandwidth. In short, the current parallel machines are of large grain type. The parallel algorithm used should make every effort to communicate as seldom as possible. For a best performance it often means that a particular calculated value, needed on several nodes, can actually be recalculated more quickly on each node, compared to communicating it to the nodes where it is needed. This is the parallel form of the classic optimization trade-off between memory and CPU cycles. [Pg.247]


See other pages where Grain types is mentioned: [Pg.358]    [Pg.358]    [Pg.90]    [Pg.94]    [Pg.29]    [Pg.274]    [Pg.29]    [Pg.151]    [Pg.1290]    [Pg.1429]    [Pg.424]    [Pg.157]    [Pg.358]    [Pg.358]    [Pg.112]    [Pg.85]    [Pg.182]    [Pg.329]    [Pg.570]    [Pg.195]    [Pg.23]    [Pg.23]    [Pg.32]    [Pg.35]    [Pg.523]    [Pg.3589]    [Pg.3595]    [Pg.3631]    [Pg.358]    [Pg.358]    [Pg.1556]   


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