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The rst method can be achieved through the use of a Fourier transform Unfortunately, this approach consumes a lot in terms of power supply and complexity of the corresponding electronics As the power consumption of a GNSS receiver is a major concern, other directions were investigated The second approach adopts a different philosophy The idea is to try all the possibilities in the frequency and time domains at once, that is, in parallel The quasiimmediate electronic architecture would have as many processing channels as there are elementary possibilities Let us consider a frequency step of 10 Hz for a complete range of 10 kHz (that is, +5 kHz); this leads to a thousand possibilities Let us also consider a GPS C/A code of 1023 chips and an elementary time step of one chip, this leads to another thousand possibilities The complete search domain then consists of about one million possibilities.

If it is possible to build an electronic device including one million parallel channels, then the treatment of all the possible combinations in time and frequency for one satellite can be achieved in one clock time duration In fact, this should allow, in one clock time, all the correlation values to be output, but the processing of the correct location of the peak still has to be computed Note that current receivers have typically between 14 and 20 channels, which are usually used by associating one channel with a given satellite The search process is then conducted in a sequential mode One of the rst industrial realizations incorporated 32,000 parallel correlators Further products have exhibited more than 200,000 correlators in parallel.

HARILAOS G. SANDALIDIS and PETER STAVROULAKIS Telecommunication Systems Institute, Chania, Crete, Greece

Since a PIFS is longer than an SIFS, a poll is never issued, eg, between Data and ACK frames; hence a poll frame does not interrupt an ongoing frame exchange The PC continues the aforementioned procedure until the CFP expires A particular control frame, CF-End, is broadcast by the AP as the last frame within a CFP to indicate the end of the CFP (see Fig 14) [1, 2, 4] The PCF has many problems that have been reported in the literature [4] Among many others, erratic beacon frame delay and inde nite transmission duration of the polled stations are the most important drawbacks At the TBTT, the PC schedules the beacon as the next frame to be transmitted, but the beacon can only be transmitted when the medium has been determined to be.

Another way to track very low signals is to use the characteristic of pseudo random noise features, by using the fact that it is not random at all and that if you know what you are searching for, it is possible to integrate the energy held in a code by repeating the correlation a few times in a row Of course, this requires the correlation to be followed and kept as time goes on This approach is called the long integration There are two kinds of long integration, depending on whether the integration is carried out in a time continuous manner or at some discrete times Coherent long integration is limited, in GPS, by the global form of the signal..

The simplest thing you can do with labels is list the ones you are already using. Listing 11-1 shows a script to do just that. It uses the Utils.pm module created earlier in the book, as do the rest of the scripts in this chapter.

The Windows CE file system API functions access files and directories by means of a file handle. Like any other Windows CE handle type, such as a window handle, a file handle is an identifier for referencing an object managed by the Windows CE kernel. In this case the object is a file or directory. As we will see, the function used for opening and creating files returns a handle to the specified file. Functions for reading and writing files require a file handle in order to access the right file. In short, any operation that a Windows CE application may perform on a file or directory requires a valid file handle.

Analysis of Variance for the Weight-Loss Data SS 373.6667 131.6667 242.0000 232.5000 67.5000 35.0000 130.0000 606.1667 df 14 2 12 15 1 2 12 29 MS 65.8334 20.1667 67.5000 17.5000 10.8333 F [2 3]a 3.26 p .074