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where T is the number of Julian centuries that have elapsed since noon, January 0, 1900. The GST equation is derived from (Wertz 1984) GST 180 UT s where as is the right ascension of the mean sun. Determine the right ascension of the mean sun for noon on June 5, 2005. 2.40. Assuming that the orbits detailed in Table 2.5 are circular, and using Eq. (2.2) to find the semimajor axis, calculate the regression of the nodes for these orbits. 2.41. Determine the standard zone time in the following zones, for 12 noon GMT: (a) 285 E, (b) 255 E, (c) 45 E, (d) 120 E.

Considerations for Oracle VLDBs (Very Large Databases)

2.42. Determine the GMT for the following local times and locations: (a) 7 A.M. Los Angeles, USA; (b) 1 P.M. Toronto, Canada; (c) 12 noon Baghdad, Iraq; (d) 3 P.M. Tehran, Iran.

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ADC USAF. 1980. Model for Propagation of NORAD Element Sets. Spacetrack Report No. 3. Aerospace Defense Command, U.S. Air Force, December. ADC USAF. 1983. An Analysis of the Use of Empirical Atmospheric Density Models in Orbital Mechanics. Spacetrack Report No. 3. Aerospace Defense Command, U.S. Air Force, February. Arons, A. B. 1965. Development of Concepts of Physics. Addison-Wesley, Reading, MA. Bate, R. R., D. D. Mueller, and J. E. White. 1971. Fundamentals of Astrodynamics. Dover, New York. Celestrak, at http://celestrak.com/NORAD/elements/noaa.txt Duffett-Smith, P. 1986. Practical Astronomy with Your Calculator. Cambridge University Press, New York. Schwalb, A. 1982a. The TIROS-N/NOAA-G Satellite Series. NOAA Technical Memorandum NESS 95, Washington, DC. Schwalb, A. 1982b. Modified Version of the TIROS-N/NOAA A-G Satellite Series (NOAA E-J): Advanced TIROS N (ATN). NOAA Technical Memorandum NESS 116, Washington, DC. Thompson, Morris M. (editor-in-chief). 1966. Manual of Photogrammetry, 3d ed., Vol. 1. American Society of Photogrammetry, New York. Wertz, J. R. (ed.). 1984. Spacecraft Attitude Determination and Control. D. Reidel, Holland.

Follow the general considerations previously described in the section "Oracle File System Design Guidelines" As a brief reminder, remember that the redo logs have very high input/output activity and should be on different disks than the database data itself Also, remember to place the data and index files for a tablespace on separate disks, which is standard in the R/3 installation However, when considering large databases, where additional tablespaces might be necessary, you may need to do some mixing and matching to place the data and index on different file systems The most intensive input/output tablespaces on the SAP system are PSAPSTABD, PSAPCLUD, and PSAPBTABD, as well as corresponding index tablespaces PSAPSTABI, PSAPCLUI, and PSAPBTABI These tables contain most of the transactional data of users' daily work At least try to place these three tablespaces on different disks.

3.1 Introduction A satellite in a geostationary orbit appears to be stationary with respect to the earth, hence the name geostationary. Three conditions are required for an orbit to be geostationary: 1. The satellite must travel eastward at the same rotational speed as the earth. 2. The orbit must be circular. 3. The inclination of the orbit must be zero. The first condition is obvious. If the satellite is to appear stationary, it must rotate at the same speed as the earth, which is constant. The second condition follows from this and from Kepler s second law (Sec. 2.3). Constant speed means that equal areas must be swept out in equal times, and this can only occur with a circular orbit (see Fig. 2.2). The third condition, that the inclination must be zero, follows from the fact that any inclination would have the satellite moving north and south, (see Sec. 2.5 and Fig. 2.3), and hence it would not be geostationary. Movement north and south can be avoided only with zero inclination, which means that the orbit lies in the earth s equatorial plane. Kepler s third law may be used to find the radius of the orbit (for a circular orbit, the semimajor axis is equal to the radius). Denoting the radius by aGSO, then from Eqs. (2.2) and (2.4), a P 4 b 2

The SAPDATA<N> file systems should be used exclusively for the tablespace data and index Do not mix them with operating system files, swap space, or SAP runtime programs The SAPARCH file systems should also be located on a different disk This file system should be sized properly to avoid the archiver stuck problem This well known problem occurs if the saparch file system becomes full and the redo log files can't be archived If this event happens to you, the SAP system becomes inactive, and the update process seems to be in a suspended state The size of transaction log files (redo log files) can positively affect the performance For instance, bigger sizes increase performance but, as a drawback, slow down database startup/shutdown procedures, especially in recover situations Also, if you lose one redo log, more data is lost.

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