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GoLive should be able to update all files that were active and checked in the Update dialog box. You will have to update the other files yourself later on. If your update involved moving or renaming files themselves, then, in the Files tab, any file that could not be updated is designated by a green bug error. If your update was changing the content of a Component, pages that were not updated will still have the old Component content, and will not have any warning that the content is now outdated (see the Sharing Components section later for more info). This can help you later, in case you forget the update that was missed. As usual in GoLive, you can open a page and click the Show Errors button on the toolbar to highlight the error on the page. Then, you can repair the error. If only one or two pages need updating, manually locating the bug and performing the update can be effective.

Rimmer and Wyant developed this result in 1975. The values of Cnm and Dnm may be obtained from the interferograms by means of a least-square tting of the measured values of WS and WT to functions (4.26) and (4.27), respectively. There are M k k 1 =2 coef cients Cnm and Dnm . From them we have to determine the N wavefront coef cients Bnm . Expression (4.28) represents a system of M equations with M unknowns, where the unknowns are all Bnm coef cients with the exception of Bn0 . Likewise, expression (4.29) represents a system of M equations with M unknowns, where these unknowns are all Bnm coef cients with the exception of Bnn . If the wavefront has rotational symmetry, Bn0 Bnm 0 for all values of n, it becomes suf cient to use either expression (4.28) or (4.29) and, hence, only one interferogram is necessary. If m is different from n and also different from zero, the value of Bnm is found from each expression. An average of these values is appropriately taken because their difference may be explained by rounding errors in computations. Many alternative approaches to computing the wavefront from the interferogram, generated by a lateral shearing interferometer, have been devised. This includes, for example, Gorshkov and Lysenko (1980) and others. A most interesting one is based on the wavefront expansion in terms of Zernike polynomials, rst described by Rimmer and Wyant (1975) and later revised by Korwan (1983). The wavefront difference function W x; y as well as the wavefront W x; y is expressed as a linear combination of Zernike polynomials. Shen et al. (1997) analytically updated this work. The Zernike polynomial coef cients of the wavefront under test are

First and foremost, make sure your hotspot is easy to use. As much as possible you want to avoid having to help your customers connect up. However, be prepared to offer assistance when someone has difficulty connecting another good reason to keep things simple. You might want to consider printing up a connection guide. Not all of your users are going to have a laptop or mobile device to make the connection they need when they show up at your business. Therefore you may want to consider adding a workstation or terminal for those types of users.

It is an explicit method involving m + 1 steps. Table 10.1 summarizes the method parameters for various m, and is essentially Table 6.6 from Ref. 12. 10.4.2 Adams Moulton Methods The Adams Moulton methods are a modi cation of the Adams Bashforth methods. The Adams Bashforth methods interpolate using the nodes tn , tn 1 , . . . , tn m . On the other hand, the Adams Moulton methods interpolate using the nodes tn+1 , tn , . . . , tn m+1 . Note that the number of nodes is the same in both methods. Consequently, (10.138) becomes

Wired Token Ring networks are still around, but the number of new installations is declining as more new network installations opt toward wired bus network implementations. The need to discuss the wired Token Ring network architecture is due to the fact that there are a number of these networks still deployed in the eld today even though they are considered legacy8 networks. The original design of a Token Ring network was literally a ring where each node of the network was daisy-chained to the next node until the network came back around to the rst node in the ring. There was a ring-in (RI) port and a ring-out (RO) port, with the RO of one station connecting to the RI of the next upstream station on the ring. This would continue until all the network nodes had been connected. The major disadvantage of this network design was that the disruption or disconnection of any one node on the ring brought the whole network down. Newer Token Ring networks were designed using hubs or media access units (MAUs), which allowed for ease in cabling while maintaining the logical ring of the Token Ring network architecture. Figure 212 illustrates the construction of a Token Ring network with two nodes with the use of a two-port MAU.