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to compensate for the movement of the satellite about the nominal geostationary position. With the types of antennas used for home reception, the antenna beamwidth is quite broad, and no tracking is necessary. This allows the antenna to be fixed in position, as evidenced by the small antennas used for reception of satellite TV that can be seen fixed to the sides of homes. The three pieces of information that are needed to determine the look angles for the geostationary orbit are 1. The earth-station latitude, denoted here by lE 2. The earth-station longitude, denoted here by fE 3. The longitude of the subsatellite point, denoted here by fSS (often this is just referred to as the satellite longitude) As in Chap. 2, latitudes north will be taken as positive angles, and latitudes south, as negative angles. Longitudes east of the Greenwich meridian will be taken as positive angles, and longitudes west, as negative angles. For example, if a latitude of 40 S is specified, this will be taken as 40 , and if a longitude of 35 W is specified, this will be taken as 35 . In Chap. 2, when calculating the look angles for low-earth-orbit (LEO) satellites, it was necessary to take into account the variation in earth s radius. With the geostationary orbit, this variation has negligible effect on the look angles, and the average radius of the earth will be used. Denoting this by R: R 6371 km (3.5)

Distribution, in a general sense, means sharing something among several individuals. In SAP R/3 systems, there are many processes, services, printers, users, and so forth. Since SAP R/3 is based upon a client/server software concept, distributing the SAP R/3 system means sharing the provided services among the clients and the servers to optimize the performance and the availability and balancing the load of the system. This chapter covers the practical aspects of the client/server components of the SAP R/3 system and the benefits of using this architecture. It deals with such issues as identifying which parts of the system can be distributed and how to plan such distribution. It also describes the main factors to consider when setting up the different parts of R/3: sizing, network, load balancing, and availability. The following sections describe other important and practical details of the R/3 system distribution, for instance, the SAP instance profiles, the operating system directory structure, the process of starting and stopping the system, and which programs you can find under the runtime directory. When setting up the system, there are details that change depending upon whether a central system or a distributed system is built. Here, you find such things as setting up the central system log (the main repository for R/3 problem and error messages) and awareness of the buffer synchronization (so that users don't say, I can see this data from this system and cannot see it from the other one).

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The geometry involving these quantities is shown in Fig. 3.1. Here, ES denotes the position of the earth station, SS the subsatellite point, S the satellite, and d is the range from the earth station to the satellite. The angle is an angle to be determined. There are two types of triangles involved in the geometry of Fig. 3.1, the spherical triangle shown in heavy outline in Fig. 3.2a and the plane triangle of Fig. 3.2b. Considering first the spherical triangle, the sides are all arcs of great circles, and these sides are defined by the angles subtended by them at the center of the earth. Side a is the angle between the radius to the north pole and the radius to the subsatellite point, and it is seen that a 90 . A spherical triangle in which one side is 90 is called a quadrantal triangle. Angle b is the angle between the radius to the earth station and the radius to the subsatellite point. Angle c is the angle between the radius to the earth station and the radius to the north pole. From Fig. 3.2a it is seen that c 90 lE.

There are six angles in all defining the spherical triangle. The three angles A, B, and C are the angles between the planes. Angle A is the angle between the plane containing c and the plane containing b. Angle B is the angle between the plane containing c and the plane containing a. From

For small installations in terms of number of users (this is relative, but say less than 100), you might not have more than one computer server running your SAP applications. In that case, every service is running in the central system: database, central instance application server, background services, and so forth. The only distributed component is the presentation server (SAPGUI) running on a Windows PC or similar. With such installations, a factor to consider making some kind of distribution is the printing strategy, which could be handed over to the presentation servers (normally Windows PCs) using some type of front end printing.

Figure 3.2 (a) The spherical geometry related to Fig. 3.1. (b) The plane triangle s obtained from Fig. 3.1.

In the case of centralized installations, the system layout looks like the picture shown in Fig. 4 1. If the server is powerful enough, this can be a suitable installation for larger SAP user populations. Moreover, this can be a good fit for starting the R/3 implementation, since the fact that it is a centralized configuration does not mean it cannot scale up to meet the growing demands of the system.

Fig. 3.2a, B E SS. It will be shown shortly that the maximum value of B is 81.3 . Angle C is the angle between the plane containing b and the plane containing a. To summarize to this point, the information known about the spherical triangle is a c B 90 90

(3.7) (3.8)

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