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It s amazing: Many object functions are extremely well-documented, but the documentation is stored away in some help file deep down on your hard drive. Again, here comes the TypeLibrary to the rescue. It contains help context information that specifies not only the name of the help file but also the page that contains the information about the specific function you wonder about. The help information provided by the TypeLibrary isn t supposed to help you out. Instead, it s provided for programming environments: They can pop up the right help file whenever the programmer hits [F1]. Luckily, this help information is available to your scripts, too! Check out the following script. It wants you to type in the exact name of some command. This time, it won t be enough to just specify part of the name. Your input doesn t need to be case-sensitive, though. See what happens if you type in MsgBox!

Semantic Relations of a Thesaurus DEFINITION A term X has nearly the same meaning as a term Y. EXAMPLE Report is a synonym for document.

where c is the external cavity roundtrip time, Rext is the power reflectivity of the external reflector, R2 is the power reflectivity of the front laser facet, l is the optical path length of the laser cavity and f is the fraction of the reflected field which couples back into the lasing mode. The coupling fraction f is difficult to measure directly in experiments, and so an alternate method of deducing is useful. To characterize experimental feedback rates to the laser, one measures the reduction in the effective threshold current in the presence of feedback. This is illustrated in Figure 4.3, which shows sample light-current curves for a solitary semiconductor laser, and the same laser with optical feedback [25]. It is evident that the current threshold is reduced. In practice, then, the quantity related to that is most easily measured experimentally is the fractional threshold reduction I, which is related to the threshold current with feedback Ith and the sol solitary threshold current Ith as:

In this chapter, several receiver options for TH-IR based UWB systems have been discussed. It is argued that each receiver option has several trade-offs in terms of performance, cost, hardware, and computational complexity, throughput, multiple access capability, etc. Depending on the application and the transceiver requirements, different receivers might be preferable. Currently, the implementation of fully digital and fully coherent reception is not feasible for UWB radio. On the other hand, the performance gap between the low complex receivers and high-performance receivers is very wide. The research opportunities for the transceiver design in UWB radio are wide open. The research is relatively immature compared with other narrowband radio counterparts. There has been some recent efforts to reduce the complexity of the coherent matched ltering-based receivers. These efforts include reducing the number of ngers in a rake reception while trying to keep the performance close as to the all-rake receiver, avoiding the intensive estimation of the time varying channel parameters, developing simple and computationally ef cient channel parameter estimation techniques. In parallel, there are also recent efforts to improve the performance of noncoherent receivers to close the performance gap with respect to the fully coherent receivers. Mainly, the approaches for improving the performance of the noncoherent receivers

color is supported by the device. The color model used in these classes is a 24-bit model. There are 8 bits each for colors red, green, and blue. Of course, not every device can render such variety of colors on the display. This means that mapping of requested colors to available colors will occur, that is, if an application uses colors that a device doesn t support, the device will map to those colors that are supported by the device. You can display fairly good-looking images on small devices by using the low-level APIs. This can be done by using the drawImage method of the Graphics class. It has the following signature:

The next script could be your first real command extension (see Figure 18-4). Save it as DOS.VBS in your Windows folder. From now on, it s easy to switch default hosts. Call the script DOS.VBS without arguments. It switches hosts and reports the active host. Or use DOS on or DOS off as argument. DOS on activates CSCRIPT.EXE, and DOS off activates WSCRIPT.EXE as default host. From now on, right before you start working with your script commands, enter DOS on. Once you are finished, enter DOS off.