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Point selection errors

Long Range Heterogeneity (or Point Selection) Error errors of this type are nonrandom and arise from existence of spatially localized hot spots in the sampling target such errors can be identified and reduced by taking many sampling increments to form the final sample. [Pg.449]

The selection to minimize absolute error [Eq. (6)] calls for optimization algorithms different from those of the standard least-squares problem. Both problems have simple and extensively documented solutions. A slight advantage of the LP solution is that it does not need to be solved for the points for which the approximation error is less than the selected error threshold. In contrast, the least squares problem has to be solved with every newly acquired piece of data. The LP problem can effectively be solved with the dual simplex algorithm, which allows the solution to proceed recursively with the gradual introduction of constraints corresponding to the new data points. [Pg.189]

Fig. 12.6. Observable baryons in the Universe as a function of time. The curves represent the total mass density in stars (in Af0Mpc-3) from Rudnick et al. (2003) based on a survey of near-infrared selected galaxies in the Hubble Deep Field South, assuming a Salpeter(O.l) IMF. (For a Kennicutt (1983) IMF, the numbers would be approximately halved.) The points with error bars show the cosmic density of H I from DLAs and sub-DLAs at various redshifts, uncorrected for obscuration, while the point at bottom right shows the present-day density of H i clouds determined by Zwaan et al. (2005). The typical H I co-moving volume density corresponds to S2Hi — 0.7 x 10-3 (taking h = 0.65). After Peroux, Dessauges-Zavatsky, D Odorico et al. (2005). Fig. 12.6. Observable baryons in the Universe as a function of time. The curves represent the total mass density in stars (in Af0Mpc-3) from Rudnick et al. (2003) based on a survey of near-infrared selected galaxies in the Hubble Deep Field South, assuming a Salpeter(O.l) IMF. (For a Kennicutt (1983) IMF, the numbers would be approximately halved.) The points with error bars show the cosmic density of H I from DLAs and sub-DLAs at various redshifts, uncorrected for obscuration, while the point at bottom right shows the present-day density of H i clouds determined by Zwaan et al. (2005). The typical H I co-moving volume density corresponds to S2Hi — 0.7 x 10-3 (taking h = 0.65). After Peroux, Dessauges-Zavatsky, D Odorico et al. (2005).
While field crews collect the samples, the chemist verifies their types and quantities by comparing the COC Forms, Sample Tracking Logs, and other field records to the SAP specifications. The chemist interacts with the field crews for the resolution of errors in the sampling point selection, sample containers and preservation or COC Form errors. The chemist also serves as a point of contact with the laboratory, if any technical issues arise during sample analysis. [Pg.284]

IV.8 are represented the expected percentage errors in kA arising only from the errors of analysis. It turns out that this analytical error is about the same for all orders of reaction from zero to four and depends chiefly on the extent of reaction occurring between the two points selected. [Pg.88]

For compression, other threshold selection criteria include the compression ratio (CR), the mean-square error (MSE), and the local point-wise error of approximation, which are discussed in more detail in [13]. In this chapter, the universal threshold given in Eq. (13) will be used for both filtering and compression. Two thresholding techniques have been studied Hard thresholding and Soft thresholding [4,6,22] ... [Pg.132]

To add error bars, click on one of the points to highlight all points on the graph. In Chart Tools, Layout, select Error Bars and choose More Error Bars Options. For Error Amount, choose Custom and Specify Value. For both Positive Error Value and Negative Error Value, enter D4 D9. You just told the spreadsheet to use 95% confidence intervals for error bars. When you click OK, the graph has both jc and y error bars. Click on any jc error bar and press Delete to remove all jc error bars. [Pg.97]

The most reliable estimates of the parameters are obtained from multiple measurements, usually a series of vapor-liquid equilibrium data (T, P, x and y). Because the number of data points exceeds the number of parameters to be estimated, the equilibrium equations are not exactly satisfied for all experimental measurements. Exact agreement between the model and experiment is not achieved due to random and systematic errors in the data and due to inadequacies of the model. The optimum parameters should, therefore, be found by satisfaction of some selected statistical criterion, as discussed in Chapter 6. However, regardless of statistical sophistication, there is no substitute for reliable experimental data. [Pg.44]

Heats of Vapon a/ion andFusion. A simple linear summation of most of the Lyderson groups (187) has been proposed for heat of vaporization at the normal boiling point and heat of fusion at atmospheric pressure for a wide variety of organic compounds (188). Average errors of 1.2 and 4.3% for group contribution-based estimations of heats of vaporization for selected n- and iso-alkanes, respectively, have been reported (215). [Pg.253]

Feedback Control In a feedback control loop, the controlled variable is compared to the set point R, with the difference, deviation, or error e acted upon by the controller to move m in such a way as to minimize the error. This ac tion is specifically negative feedback, in that an increase in deviation moves m so as to decrease the deviation. (Positive feedback would cause the deviation to expand rather than diminish and therefore does not regulate.) The action of the controller is selectable to allow use on process gains of both signs. [Pg.718]

Successful recrystallization of an impure solid is usually a function of solvent selection. The ideal solvent, of course, dissolves a large amount of the compound at the boiling point but very little at a lower temperature. Such a solvent or solvent mixture must exist (one feels) for the compound at hand, but its identification may necessitate a laborious trial and error search. Solvent polarity and boiling point are probably the most important factors in selection. Benzhydrol, for example, is only slightly soluble in 30-60 petroleum ether at the boiling point but readily dissolves in 60-90° petroleum ether at the boiling point. [Pg.182]

Regarding current ab initio calculations it is probably fair to say that they are not really ab initio in every respect since they incorporate many empirical parameters. For example, a standard HF/6-31G calculation would generally be called "ab initio", but all the exponents and contraction coefficients in the basis set are selected by fitting to experimental data. Some say that this feature is one of the main reasons for the success of the Pople basis sets. Because they have been fit to real data these basis sets, not surprisingly, are good at reproducing real data. This is said to occur because the basis set incorporates systematical errors that to a large extent cancel the systematical errors in the Hartree-Fock approach. These features are of course not limited to the Pople sets. Any basis set with fixed exponent and/or contraction coefficients have at some point been adjusted to fit some data. Clearly it becomes rather difficult to demarcate sharply between so-called ab initio and semi-empirical methods.4... [Pg.96]


See other pages where Point selection errors is mentioned: [Pg.449]    [Pg.450]    [Pg.449]    [Pg.450]    [Pg.191]    [Pg.45]    [Pg.108]    [Pg.78]    [Pg.254]    [Pg.254]    [Pg.20]    [Pg.2365]    [Pg.2448]    [Pg.158]    [Pg.176]    [Pg.195]    [Pg.255]    [Pg.97]    [Pg.105]    [Pg.117]    [Pg.185]    [Pg.141]    [Pg.255]    [Pg.175]    [Pg.176]    [Pg.209]    [Pg.1081]    [Pg.58]    [Pg.274]    [Pg.326]    [Pg.338]    [Pg.421]    [Pg.253]    [Pg.673]    [Pg.742]    [Pg.2564]    [Pg.53]    [Pg.257]    [Pg.269]   
See also in sourсe #XX -- [ Pg.450 ]




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