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Observing Conditions

If we multiply each equation by the corresponding power of A and write t/(A, t) = 2 (/)A , where the summation goes from n = 1 to infinity, (this is a formal series and no question of convergence arises), we have an equation for U [Pg.67]

We can read off un from the exponential expansion. This is the Gamma distribution, and it is the natural distribution in many kinetic problems see G and H, Chapter 8 and [276]. [Pg.67]

Conditions must be observed and should be made explicit even at the expense of an air of pedantry. [Pg.67]


SWCNTs are imaged as two parallel lines with a separation equal to the tube diameter (Fig. 5). By image simulation it can be shown that under usual observation conditions the black lines correspond to graphene sheets seen edge on in MWCNT as well as in SWCNT tubes [7]. [Pg.17]

The Munsell book standards corresponding to the limiting colors may even serve as material standards for industrial color control. In a material standard system the sample is compared with a standard by eye without the use of any meter or optical instrument. The success and popularity of these systems are largely due to their simplicity of application. The ability of the human eye to compensate for various illuminants and surroundings makes it possible for this system to give results even under mediocre conditions. The most critical work with material standards requires carefully controlled observing conditions. [Pg.12]

With the best observing conditions, it is possible for the trained observer to compete with photoelectric colorimeters for detection of small color differences in samples which can be observed simultaneously. However, the human observer cannot ordinarily make accurate color comparisons over a period of time if memory of sample color is involved. This factor and others, such as variability among observers and color blindness, make it important to control or eliminate the subjective factor in color grading. In this respect, objective methods, which make use of instruments such as spectrophotometers or carefully calibrated colorimeters with conditions of observation carefully standardized, provide the most reliable means of obtaining precise color measurements. [Pg.12]

So far, we considered image deconvolution assuming that the PSF was perfectly known. In practice, this is rarely the case. For instance, when the PSF is measured by a calibration procedure, it is corrupted by some level of noise. Moreover, if the observing conditions change, the calibrated PSF can mismatch the actual PSF. It may even be the case that the PSF cannot be properly calibrated at all, because it is varying too rapidly, or because there is no time or no means to do such a calibration. What can we do to cope with that ... [Pg.416]

Moreover, when the concentration of fluorescent compound is high, inner filter effects reduce the fluorescence intensity depending on the observation conditions (see Chapter 6). In particular, the photons emitted at wavelengths corresponding to the overlap between the absorption and emission spectra can be reabsorbed (radiative transfer). Consequently, when fluorometry is used for a quantitative evaluation of the concentration of a species, it should be kept in mind that the fluorescence intensity is proportional to the concentration only for diluted solutions. [Pg.51]

The traditional limitation of the stereoisomer concept to isomeric compounds with different configurations stems from the idea that configurations are not interconvertible under the observations conditions. ) A definition of stereoisomers on this basis is questionable as its application is then dependent upon observation conditions. It also fails to account for the fact that many mobile interconversions of configurations (e.g. configurations involving tricoordinate Nitrogen or pentacoordinate Phosphorus) are known, as well as thermally stable conformations (e.g. the atropisomers). [Pg.13]

In the enumeration of chirality elements of flexible molecules all arrangements are taken into account which are permitted by the given constraints under the observation conditions. Here, one must always assume a rigid skeletal model and freely rotating ligandsF That arrangement for which the lowest number of chirality elements is found equal zero determines the number of chirality elements for the whole ensemble. [Pg.25]

The risk assessment framework we have described for chemical toxicity is applicable to microbial risk assessment. Once the information is available on microbial hazards, which are for the most part acute (immediately observable) conditions resulting from acute (one-time) exposures, and their dose (pathogen count)-response characteristics, we should be ready to assess the risks associated with any dose of interest. Hazard information for the important pathogens is readily available but, as expected, their dose-response characteristics are much harder to come by. So with pathogen risk assessment we see the same types of uncertainties creeping into the framework as we have encountered for chemicals. [Pg.271]

On the other hand, the X-ray intensity in the hard X-ray band (16 - 28 keV) exhibits much less change than those in the soft X-ray band. The first positive detection was on July 4, 1987. It should be mentioned, however, that the epoch when the hard X-ray intensity exceeded the Ginga detection threshold remains somewhat uncertain. This is because the observing condition was unfavorable in May and June, 1987. Since the detection, the intensity in the hard X-ray band has remained almost constant within the statistical uncertainties through December, 1987. In the January flare, the hard X-ray intensity increased simultaneously by a factor of two, which was however much smaller than the factor of increase in the soft X-ray band. [Pg.403]

Combustion models which consider the thickness of the reaction zone usually accentuate cither heat conduction mechanisms (thermal theory) or the diffusion mechanisms (diffusion theory) and the models are of necessity of limited value. Simpler models in which the reaction zone or flame front is considered to be an infinitesimally thin discontinuity in the flow, while not simulating exactly the observed conditions, allow the model to be of more general utility and many combustion phenomena become easier to understand because of this simplification. It is the latter approach which is discussed first in this paper—i.e., the combustion process is regarded as a wave phenomenon. [Pg.70]

However, the solubility condition (see the section entitled Observing Conditions in this chapter for more detail) that must be imposed is easily seen to be that the average of L[(c0)] must be zero and... [Pg.12]

TT heoretical equilibrium models can be established for oxidation-reduc-- tion systems in natural waters in much the same way that acid-base or solubility models have been developed and found useful in interpreting observed concentrations of ions and other materials. To relate the theoretical models for redox processes to observed conditions and processes in the aquatic environment is, however, much more difficult and cannot be done as rigorously. Primarily this situation occurs because true oxidation-reduction equilibrium is not observed in any natural aquatic system this is partly because of the extreme slowness of most oxidation-... [Pg.276]

Ordinarily we think of empirical validation, validation in terms of testable consequences that produce physical effects, but this is misleading. Any effect, whether interpreted as physical or nonphysical, is ultimately an experience in the observer s mind. All that is essentially required to validate a theory is that it predict that when a certain experience (observed condition) has occurred, another (predicted) kind of experience will follow, under specified experiential conditions. Thus a perfectly scientific theory may be based on data that have no physical existence. [Pg.208]

Brenguier et al. (2003) discussed the results of eight series of aircraft measurements of the microphysical characteristics of marine stratocumulus clouds in a broad range of observation conditions (different physico-chemical properties of aerosol, number density values in the interval 50 cm 3-25 cm-3, etc.)- The unique complex of synchronous observations of the microphysical and radiative characteristics of cloud cover obtained can be used to assess the indirect impact of aerosol on clouds and climate based on analysis of the ratio between the cloud optical thickness and effective radius of cloud droplets. Correlation between these values is usually negative, but in a heavily polluted atmosphere it can be positive. From the observational data obtained during ACE-2, the polluted systems of clouds turned out to be somewhat drier and therefore thinner, resulting in the positive correlation between the indirect impact of aerosol on climate and the effective radius of droplets. [Pg.43]

It is important to have the correct set of variables specified as independent and dependent to meet the modeling objectives. For monitoring objectives observed conditions, including the aforementioned independent variables (FICs, TICs, etc.) and many of the "normally" (for simulation and optimization cases) dependent variables (FIs, TIs, etc.) are specified as independent, while numerous equipment performance parameters are specified as dependent. These equipment performance parameters include heat exchanger heat transfer coefficients, heterogeneous catalyst "activities" (representing the relative number of active sites), distillation column efficiencies, and similar parameters for compressors, gas and steam turbines, resistance-to-flow parameters (indicated by pressure drops), as well as many others. These equipment performance parameters are independent in simulation and optimization model executions. [Pg.125]

For a somewhat more accurate estimate of the apparent source size in particular emission and observation conditions, numerical methods of Fourier optics can be used. In this framework, the effective source size can be obtained either by backpropagation of the wavefront (at a specific wavenumber) to the source position, or by simulating the radiation focusing at optical magnification equal to 1. To illustrate this, we have considered two cases an IR beamline at the NSLS (0.8 GeV storage ring) normalized at 1000 mA (electron source size = 550 p,m horizontal, 70 (im vertical) and an IR beamline at SOFFIT, (2.75 GeV - electron source... [Pg.66]

Definition A molecule is chemically chiral under given observation conditions if there is one momentary geometry of that molecule, which cannot be superimposed on its mirror image by using only rotations, translations, and those intramolecular motions that can occur under the observation conditions. [Pg.166]

Note that this differs from Lord Kelvin s notion in that it involves the observation conditions and the intramolecular motions that can occur under those conditions. It is known, for example, that under suitable conditions, some molecules which cannot be superimposed on their mirror image by any combination of rotations and translations may nevertheless convert to their mirror image by intramolecular motions alone such molecules cannot be observed as chiral under the stated conditions. In particular, this definition of chemical chirality gives meaning to the concept... [Pg.166]

Definition An ensemble of molecules is chemically achiral under given observation conditions if and only if it is composed of racemic pairs of enantiomers and achiral molecules. [Pg.168]

The planetary reflectance spectral data constituting Table 10.1 traditionally have been obtained with Earth-based telescopes. Such remote-sensed measurements are limited by telescope availability, favourable observational conditions, and optimum viewing alignments of the planetary objects. As a result,... [Pg.424]

Furthermore, one would not expect to observe conditions where a —l due to hydrodynamic influences, where water must be squeezed out of the way as two particles or aggregates approach one another. As shown by Han and Lawler [3], under Brownian motion equal sized spheres should have a maximum collision efficiency somewhat less than one (interpolating from their Fig. 4, 100 nm spheres would have a maximum a = 0.7, 5 pirn. spheres would have a maximum a = 0.45). If all retarding influences are considered, then, as is the case when measurements are conducted in the laboratory, it is unlikely under the majority of common conditions for collision efficiencies to approach unity. [Pg.518]


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