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are thought to be responsible for the magnetization of the core and hence for the existence of the geomagnetic field Above the outer core lies the mantle, consisting of rock similar to granite (called basaltic rock) The consistency of the mantle would appear solid if you could take a piece of it and hold it in your hand However, on a long time scale and considered in its entirety, it is a fluid mass As the eons pass, the mantle flows much like hot tar or molasses, rising up from the center of the planet toward the surface in some places and descending in other zones One theory holds that this is a mechanism for the transfer of heat from the hot core regions to the surface, where the heat energy ultimately is transferred to the atmosphere and radiated into space The up-and-down currents result in lateral movement near the upper reaches of the mantle The outermost layer, called the crust, floats on top of the mantle and, as the ages pass, moves around on it The lateral movements of the mantle carry chunks of crust along The crust is not a uniform, continuous mass but instead has regions where it is deep (about 30 km, or 20 mi) and other regions where it is shallow (perhaps as thin as 10 km, or 6 mi) The thickest parts of the crust form the continents and larger islands The thin regions lie beneath the seas and oceans Figure 8-3 is a simplified crossCrust

The incremental backup offloading feature of the Exadata Storage Server is able to filter unchanged blocks directly in the storage layer, which further improves the incremental backup performance by only sending changed blocks to RMAN for backup The Exadata Storage Servers are capable of identifying the changed blocks at a finer granularity than the BCT feature As you can see, the BCT and the incremental backup offload features are complementary to one another Best practices indicate that block change tracking provides the most benefit when 20 percent or fewer blocks get modified since the last incremental or full backup When changes are greater than 20 percent, you might still benefit, but you need to evaluate it against the data in your environment

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When you click on Configure Data Source, you invoke a wizard that will walk you through the steps of configuring your data source hooking up the control to the underlying data table(s). The first step is to create (or choose) a data connection as seen in Figure 4-4.

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Configure DB_RECOVERY_FILE_DEST_SIZE The database FRA is used to store database archived logs and other recovery files including backups, and can get filled quickly if the space is not managed properly Use DB_RECOVERY_FILE_DEST_SIZE to bind the space for each database in the FRA If there are multiple databases on the Database Machine, the total combined FRA from all databases should be less than the free space on the ASM diskgroup allocated for FRA In fact, you should leave enough space on the diskgroup to account for disk failures, and preferably for one complete Exadata Storage Server failure Configure RAC Services for backup/restore The best practice is to execute the RMAN backup task across multiple database nodes in the RAC cluster by defining Oracle RAC Services By using Services, you can allocate specific RAC nodes that you would like to take part in servicing the backup load When the RMAN clients connect to the database using Services, they get load balanced and the backup task gets distributed across the nodes defined in the service This ensures even distribution of the CPU load across the database servers and prevents overloading of the resources on just one node

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