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Region mass fraction space

Since rank(A) = 2, the stoichiometric subspace in this instance is two-dimensional residing in R mass fraction space. Due to the dimension of the component space, it is not possible to view the entire region in a single plot however, two-dimensional projections onto different component spaces may be performed. This is shown in Figure 9.4. [Pg.291]

Observe that the region is represented by a tetrahedron in mass fraction space. The benefit of generating regions in mass fraction space is that the results are always scaled between 0 and 1. [Pg.294]

Figure 9.8 (a) Full AR for the Van de Vusse system in mass fraction space, (b) AR for the Van de Vusse kinetics, converted to concentration space. The transparent region is the AR obtained for an identical feed point when constant density is assumed. (See color plate section for the color representation of this figure.)... [Pg.295]

We construct the attainable region by noting that the concentration space is a vector field with a rate vector (e.g., in Fig. 1, dC /dC/ = RB/R ) defined at each point. Moreover, we are not restricted to concentration space, but can consider any other variable that satisfies a linear conservation law (e.g., mass fractions, residence time, energy, and temperature—for constant heat capacity and density). The attainable region is an especially powerful concept once it is known, performance of the network can often be determined without the network itself. [Pg.251]

Observe that the shape of the regions is identical to those given in Chapter 8 in concentration space. The values of the extreme points are now given in terms of species mass fractions and molar extents of reaction. [Pg.291]

To compute the equivalent stoichiometric subspace in concentration space, the feed molar flow rates must be converted to a feed concentration vector Cf. The methods described in Chapter 8 for constant density systems may then be applied. The results of the constant density system and the region obtained via mass fractions are shown together in Figure 9.5. [Pg.293]

Figure 9.5 Comparison of stoichiometric subspaces in concentration space obtained for the methane steam reforming system for constant density (hatched regions) to the region obtained via mass fractions (clear region). Figure 9.5 Comparison of stoichiometric subspaces in concentration space obtained for the methane steam reforming system for constant density (hatched regions) to the region obtained via mass fractions (clear region).
The irrational number, known as the golden ratio, is said to be the most irrational of them all. Like other irrationals, it also occurs as the limit of a regular series of rational fractions, in this case the Fibonacci fractions. In nature, it occurs as the convergence limit of the mass fractions of stable nuclides, Z/(y4 — Z). As a clue to its physical meaning, it is noted that the stability of nuclides depends on their space-time environment [4]. In regions where space-time curvature approaches infinity, the mass ratio Z/ A — Z) 1. In the hypothetical situation of zero curvature, matter does not exist. It is inferred that in an intermediate situation of curvature, conducive to the development of biological life, the mass ratio Z/(A — Z) z. [Pg.170]

An extended ILDM method was also developed by Bongers et al. (2002) for specific application in diffusion flames. In their work, the manifold is constructed in composition phase space (PS) instead of composition space, and hence, the chemical ILDM method is extended to the PS-ILDM method. The composition phase space includes not only the species mass fractions and enthalpy but also the diffusive fluxes of species and the diffusive enthalpy flux. The extended equation system therefore is of dimension 2(Ns +1) where Ns is the number of species and hence is twice the dimension of the original system of equations. However, the extension allows the resulting ILDM to take account of diffusion processes that would not be represented by the purely chemical ILDM. Therefore, a low-dimensional slow manifold may be found, even in regions of the flame where there are strong interactions between chemistry and flow. The method is demonstrated for a premixed CO/H2 flame with preferential diffusion. [Pg.253]

Figure 1 Schematic of DC glow-discharge atomization and ionization processes. The sample is the cathode for a DC discharge in 1 Torr Ar. Ions accelerated across the cathode dark space onto the sample sputter surface atoms into the plasma (a). Atoms are ionized in collisions with metastable plasma atoms and with energetic plasma electrons. Atoms sputtered from the sample (cathode) diffuse through the plasma (b). Atoms ionized in the region of the cell exit aperture and passing through are taken into the mass spectrometer for analysis. The largest fraction condenses on the discharge cell (anode) wall. Figure 1 Schematic of DC glow-discharge atomization and ionization processes. The sample is the cathode for a DC discharge in 1 Torr Ar. Ions accelerated across the cathode dark space onto the sample sputter surface atoms into the plasma (a). Atoms are ionized in collisions with metastable plasma atoms and with energetic plasma electrons. Atoms sputtered from the sample (cathode) diffuse through the plasma (b). Atoms ionized in the region of the cell exit aperture and passing through are taken into the mass spectrometer for analysis. The largest fraction condenses on the discharge cell (anode) wall.
Generally, fractional deposition in the lung, as modeled in ICRP 66 (1994), is directly proportional to particle mass density and BR, and inversely proportional to trachea diameter. Other parameters play a relatively minor role in modefing regional deposition within the respiratory tract for adults, adolescents and 10-year-old children. The parameters of anatomical dead space and windspeed are more important to deposition in infants and children. Research into these more sensitive parameters and their distributions may lead to reduction in the uncertainty of... [Pg.272]

Let us now consider one of the phases, thus a region in space occupied by a continuous multicomponent mixture. The actual nature (molecular configuration) of the mixture may be little known imagine, e.g., a liquid ionic solution with various degrees of dissociation, solvatation, etc. One then usually assumes that some equilibria (such as ionic equilibria) are installed very rapidly so that the (instantaneous local) thermodynamic state at a point of the mixture can be defined by the temperature, pressure, and mass (or mole) fractions of certain K components C, —, . The Q are some formal chemical species the... [Pg.571]

The atmosphere is quite clearly and distinctly divided into a series of vertical layers of air (see Fig. 5.4), some of which have already been referred to. The layers are labelled (with increasing z) the troposphere, stratosphere, mesosphere and thermosphere, and they are caused by a combination of photochemistry, air temperature, and the effect of gravity on gas mixing due to convection. As discussed above, air pressure decays exponentially with increasing z, finally reaching the pressure of outer space at a distance >10 km however 99.99 % of the air mass is located below z = 100 km. The depth of identified air layers is therefore a small fraction of the diameter of the Earth (d = 12740 km the thickness of the troposphere is <0.12 % of this value). The stratosphere, which is photochemically the most active region, lies approximately in the range 10 < z < 50 km (the actual boundaries vary with location, season and time of day). [Pg.223]


See other pages where Region mass fraction space is mentioned: [Pg.291]    [Pg.291]    [Pg.294]    [Pg.310]    [Pg.133]    [Pg.22]    [Pg.621]    [Pg.790]    [Pg.544]    [Pg.60]    [Pg.994]    [Pg.284]    [Pg.208]    [Pg.317]    [Pg.14]    [Pg.151]    [Pg.481]    [Pg.501]    [Pg.221]    [Pg.36]    [Pg.468]    [Pg.33]    [Pg.171]    [Pg.176]    [Pg.197]    [Pg.392]    [Pg.268]    [Pg.158]    [Pg.2]    [Pg.134]    [Pg.196]    [Pg.664]    [Pg.362]    [Pg.24]    [Pg.1]    [Pg.41]    [Pg.1]   
See also in sourсe #XX -- [ Pg.287 ]




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Mass fraction space

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