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O'Reilly Network Safari Bookshelf Jini Specifications, The, Second Edition The versions of lookup providing this blocking feature each takes s one of its parameters a value of type long that represents the number of milliseconds to wait for the service to be discovered In addition to RemoteException, each of these versions of lookup may throw an InterruptedException One of these blocking versions of lookup implicitly uses a value of one for both the acceptable minimum and the allowable maximum number of service references to discover The other blocking version requires that the entity specify the range through the minMatches and maxMatches parameters, respectively Prior to blocking, each of these versions of lookup first queries each available lookup service in an attempt to retrieve a satisfactory number of matching services Whether or not the method actually blocks is dependent on how many matching service references are found during the query process Blocking occurs only if after querying all of the available lookup services, the number of matching services found is less than the acceptable minimum If the waiting period (measured from when blocking first begins) passes before that minimum number of service references is found, the method will return the service references that have been discovered up to that point If the waiting period passes and no services have been found, null or an empty array (depending on the version of lookup) will be returned If, after querying all of the available lookup services, the number of matching services found is greater than or equal to the specified minimum but less than the specified maximum, the method will return the currently discovered service references without blocking If the initial query process produces the desired maximum number of service references, the method will return the results immediately The blocking versions of lookup are quite useful to entities that cannot proceed until such a service of interest is found If a non positive value is input to the waitDur argument, then the method will not wait It will simply query the available lookup services and employ the return semantics described above The values of the minMatches and maxMatches arguments must both be positive, and maxMatches must be greater than or equal to minMatches; otherwise, an IllegalArgumentException will be thrown The blocking versions of lookup make a concurrency guarantee with respect to the discovery of new lookup services during the wait period That is, while waiting for matching service reference(s) to be discovered, if one or more of the desired but previously unavailable lookup services is discovered and added to the managed set, those new lookup services will also be queried for the service(s) of interest In addition, the blocking versions of lookup throw InterruptedException When an entity invokes either version with valid parameters, the entity may decide during the wait period that it no longer wishes to wait the entire period for the method to return Thus, while the method is blocking on the discovery of matching service(s), it may be interrupted by invoking the interrupt method from the Thread class The intent of this mechanism is to allow the entity to interrupt a blocking lookup in the same way it would a sleeping thread.

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Scanning Code 128 In VS .NET Using Barcode reader for . Make sure a breakpoint is set on the FeatureUninstalling ethod and press F5 to run the project Stsadmexe with the specified command line arguments will run and the breakpoint on the method is hit Even if you decide that debugging these events is too much work you can still get some information about the exceptions that are happening in the FeatureInstalled method If any exceptions are thrown during the deployment process, the deployment process will fail To demonstrate this create a new empty project and add a feature and feature event receiver to it Next, uncomment the FeatureInstalled method and add the code in Listing 5-13.Related: 

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expected net polarization, while at high inclination, the polarization is reduced by occultation Their analysis was also applied to the variation of polarization from binary systems in which the scattering material consists of a rotating onedimensional plume etween the stars, superposed on an axisymmetric disc They showed that the inclination of the system and the radial structure of the plume can be deduced for suf ciently high inclinations (i > 60 ) The extent to which the method can be generalized to an arbitrarily distributed two-dimensional scattering region was considered via Fourier analysis It was found that the inclination of the system is largely insensitive to the density distribution when the distribution function is of a simple power-law form The question was also raised that for some stars, the polar mass loss will have a greater ionization fraction than the equatorial region, such that the pole might be the dominant source for free electrons In the third paper of this series, Fox (1991) considered the effects of occultation and nite sized-source depolarization, concluding that the net polarization has a complicated inclination dependence, and that the simple result of it being p / sin2 i, obtained by Brown & McLean (1977), does not hold For Be stars with high intrinsic polarizations, the circumstellar envelope must be concentrated either towards equatorial or polar regions, and that a substantial optical depth is required with > 005 The possible variability of the observed polarization from an obliquely rotating envelope has been investigated by Fox (1992), such a scenario having been mooted by others as being an alternative interpretation to diagnoses involving binary motion, but with lack of spectroscopic evidence to add weight to such duplicity The results of the exercise were not too sanguine as it was evident that effects due to rotation about a body axis and binary orbital motion are indistinguishable It was also found that the physical geometry of the obliquely rotating envelope could not be inferred When the light source is considered to have nite extent, discrimination between envelope geometries emerges to some degree as a result of the occultation of parts of the envelope by the extended source Further modelling by Fox (1993a) has emphasized the effect that an extended light source has on the resulting polarization by scattering in circumstellar envelopes If the underlying star is non-spherical, as a result of its large rotational velocity say, its photosphere will also generate a net polarization, adding to that which is produced by scattering within the extended atmosphere This situation has been modelled by Fox (1993a) who found that, in general, the predicted polarization was a factor of 2 3 times larger than what is observed for Be star systems It was also noted that the theoretical models for Be star envelopes had not yet reached a level of sophistication to estimate by polarimetry the number density of free electrons throughout the circumstellar envelope The origin of stellar winds in Be stars may be in uenced by magnetic elds and Fox (1993b) has considered this additional parameter in polarimetric models From his analysis, the range of observed values of p can be explained if the stars possess small magnetic elds of B0 < 100 G Observed increases in p during the onset of a shell phase is indicative of an increased magnetic eld.

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Matrix ECC200 In NET Framework Using Barcode encoder for FDR Fractal dimension reduction (FDR) [ 362] is a novel approach to feature selection based n the concept of fractals the self-similarity exhibited by data on different scales For example, the Sierpinski triangle [113] is constructed from an equilateral triangle, eliminating its middle triangle and repeating this process on the resulting smaller triangles This operation continues in nitely, removing the middle triangles from the newly generated smaller ones The resulting shape is not one-dimensional, however; it is not two-dimensional either as its area is zero, so its intrinsic dimension lies between 1 and 2 This issue is resolved by considering fractional dimensionalities For the Sierpinski triangle its fractal dimension is approximately 158 [308] This concept may be applied to feature selection by considering the change in fractal dimension when certain features are removed from the original dataset under consideration.

A system using a variation of a Foster prism as the polarizer and means for eliminating the contaminating signal from the sky background has been described by Metz (1984) In a later development, Metz (1986) discussed the remedy for the problem of instrumental polarization introduced by the xed superachromatic wave plate which is incorporated after the rotatable one to counter spectral dispersion of the instruments reference axis Compensation for sky contamination was effected in an instrument used by Jain & Srinivasulu (1989) by rotating an eccentrically placed aluminium plate with two semi-circular slots in it, prior to the focal plane of the telescope The principle of the rotating half-wave plate polarimeter has been described earlier in this chapter An instrument using a rotatable achromatic wave plate prior to a Wollaston prism, followed by further geometric separation of the beams, with the signals recorded by photomultipliers and photon counting techniques, has been described by Appenzeller (1967) The design for this is based on that of Hiltner (1959), and is shown in Figure 81, which is in the form of an original sketch by him A dual-beam polarimeter, as sketched out in Figure 84, incorporating a rotatable achromatic wave plate, and capable of spectral studies within stellar line pro les, has been described by Clarke & McLean (1975) For multi-band work, the problem of dispersion of the phase delay of the rotating element was vercome by using a superachromatic design As described in Frecker & Serkowski (1976) such an instrument can be operated over the wavelegth range of 300 nm to 11 m Their system known as MINIPOL , and mentioned earlier, formed the basis of an instrument described by Benedetti (1982) and Magalh es, Benedetti & Roland (1984) which also incorporated a facility for tilt-scanning narrow-band interference lters, following the principles used by Clarke, McLean & Wyllie (1975).

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