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Flux variation

Fig. 12. Burn-out flux variation resulting from using the different throttling valves shown in Fig. 11 [from Styrikovitch (SI7)]. Fig. 12. Burn-out flux variation resulting from using the different throttling valves shown in Fig. 11 [from Styrikovitch (SI7)].
If one of the stars in the binary is not a neutron star, then the tests become less precise. Suppose that one observes the optical light from the companion to a neutron star. In addition to the spectral information that allows measurement of P and i i, one also has photometric information (e.g., the total optical flux from the companion). The companion is distorted into a pear shape by the gravity of the neutron star, with the point towards the neutron star. Therefore, from the side there is more projected area and hence greater flux than from either end. If the orbit is edge-on (i = 90°) then the flux varies maximally if the orbit is face-on (i = 0°) then there is no variation. Therefore, by modeling the system one can estimate the inclination from the flux variations. This is called the method of ellipsoidal light curves (Avni Bahcall 1975). [Pg.33]

However, one must be careful because in an LMXB the optical emission from the accretion disk (whether in the outer, cool regions or as reprocessed X-ray emission) can outshine the companion by a large factor. This makes spectral lines difficult to measure and also complicates the ellipsoidal light curve technique. The ideal systems to study are therefore transient systems, which undergo periods of active mass transfer (often for a few weeks to a few months) before lapsing into quiescence, where there is little to no mass transfer. During quiescence, the companion is still distorted by the gravity of the neutron star, hence the flux variations still occur, but without any contamination by the accretion disk. There is a relatively new approach similar to this that... [Pg.33]

The concept of PAUR II is summarised schematically in the following way Stratospheric ozone variations, tropospheric ozone variations, aerosol origin and composition variations UV-B flux variations and variations in photodissociation rates Induced modulation and feedback of tropospheric O3 and other photochemical species Comparison of calculations with campaign observations. [Pg.58]

The film thickness uniformity and film composition depend, in part, on the molecular or atomic flux variation across a substrate. This flux variation is a function of the directionality of the evaporation source (i.e., the molecular-beam distribution) and the orientation of the substrate relative to the source (7). In this section, the fundamental equations that describe the distribution of the incident flux will be introduced, along with the solution of these equations for the evaporation of group II-VI compound-semiconductor materials. [Pg.190]

TURBOUNQ, is also available as discussed in the Preface. In this program, the dimensionless wall heat flux variation is assumed to be of the form ... [Pg.296]

Air flows over a wide t-m long flat plate which has a uniform surface temperature of 80°C, the temperature of the air ahead of the plate being 20°C. The air velocity is such that the Reynolds number bas J on the length of the plate is 5 x 106. Derive an expression for the local wall heat flux variation along the plate. Use the Reynolds analogy and assume the boundary layer transition occurs at a Reynolds number of 10 ... [Pg.300]

The dependence of Ych on the deuterium flux density has not yet been clarified sufficiently well. A summary of various published data of the CD4 yield is displayed in Fig. 1.5a as a function of the flux density of the back ground plasma (deuterium) [6,26]. The flux variations have been obtained either by density scans or for the limiter cases (TEXTOR) by a radial movement of the limiters. These published data suffer from some inconsistencies due to different experimental conditions (electron temperature, surface temperature). The photon efficiency from which particle fluxes are derived [27] depends on the electron temperature. The chemical reactivity [6] depends... [Pg.14]

Rhodes, M. J., Laussmann, P., Villain, F., and Geldart, D. Measurement of radial and axial solids flux variations in the riser of a circulating fluidized bed, in Circulating Fluidized Bed Technology II (P. Basu and J. F. Large, eds.), p. 155. Pergamon Press, 1988. [Pg.145]

Samples were purified before activation using the solvent extraction procedure of Hahn et al. (22) with thenoyltrifluoroacetone as the ligand. An activation routine was developed to avoid subsequent contamination with aluminum, to allow the excape of Ar, to monitor flux variations, and to facilitate spectrum stripping of residues of manganese, aluminum, and sodltun (15). The advent of high efficiency germanium detectors has significantly reduced the... [Pg.79]

The permeation, selectivity, and flux variation with methanol concentration has been explained using the solubiUty parameter approach Copolymers of acrylonitrile with methyl methacrylate and vinyl acetate showed good selectivity and moderate flux Membrane (I) gave high selectivity and acceptable flux... [Pg.130]

Jaffrin et al. [57] have made a hydrodynamic comparison between the rotating disk and the VSEP system based on the flux achieved under similar maximum shear rates for baker s yeast microfiltration with an 0.2 p,m ME and skim mUk UF at 50 kDa. They found that the flux variation with time in these two modules was nearly identical when they were operated at the same maximum shear rate, suggesting the dominant effect of shear rate on the filtration performance. [Pg.217]

Since the subsystem is bounded by a zero-flux surface at all stages of the variations generated by F, the zero-flux variational constraint (eqn (8.117)) applies. In the present case it assumes the form... [Pg.395]

Orders of magnitude from Chapter 16 suggest that, for materials of the type discussed there, variation in A B ratio will be dominated by the static effect, with only small deviations related to the concurrent fluxes. Variation in stress will be basically as in Figures 18.4 or 18.5, but modified on account of interchange of A and B in the same manner that Figure 16.11c modifies Figure 16.11a. [Pg.196]

Summers, M.E., D.F. Strobel, R.M. Bevilacqua, X. Zhu, M.T. DeLand, M. Allen, and G.M. Keating, A model study of the response of mesopheric ozone to the short-term solar ultraviolet flux variations. J Geophys Res 95, 22,523, 1990. [Pg.438]

Figure 3.35 Effect of recirculation rate (cross-flow velocity) on flux variation with concentration. Figure 3.35 Effect of recirculation rate (cross-flow velocity) on flux variation with concentration.
Let us now first consider the reversible losses in RE-Co magnets. By way of example, fig. 40 shows for five commercially important types of sintered magnets the reversible flux variations on heating up to 250 °C, measured at p —2.5. It is seen that the reversible loss (or the temperature coefficient of Bd, which is the average slope of such curves over a defined temperature interval), is primarily... [Pg.196]

The effects of viscous dissipation on the thermal entrance problem with the uniform wall heat flux boundary condition can be found in Brinkman [27], Tyagi [6], Ou and Cheng [28], and Basu and Roy [29]. Other effects, such as inlet temperature, internal heat source, and wall heat flux variation, are reviewed by Shah and London [1] in detail. [Pg.314]

This increase can be determined by measuring either the cesium or xenon isotopic ratios. These results combined with the low flux fission yields can then be used to calculate the cross section of Xe135. The ideal experiment would be one in which the flux remains constant during the entire irradiation so that the amount of Xe136 present at any time is not dependent on flux variations. This approach has been used by Fickel and Tomlinson 28), who arrived at a value of 3.2 X 106 barns (1 barn = 10-24 cm2) for the neutron cross section of Xe136. Cross sections of other fission products have been measured 12, 63, 76) although the conditions in these experiments were such that the effect of flux variations could not be evaluated. [Pg.331]


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See also in sourсe #XX -- [ Pg.172 ]




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