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< xml version="1.0" encoding="utf-8" > <siteMap xmlns="http://schemas.microsoft.com/AspNet/SiteMap-File-1.0" > <siteMapNode url="~/Home.aspx" title="Home" description="Home page"> <siteMapNode url="~/Sales.aspx" title="Sales" description="Sales" > <siteMapNode url="~/Sales_Orders.aspx" title="Orders" description="Orders" /> <siteMapNode url="~/Sales_Stores.aspx" title="Stores" description="Stores" /> </siteMapNode> <siteMapNode url="~/Production.aspx" title="Production" description="Production" /> <siteMapNode url="~/HR.aspx" title="Human Resources" description="HR" /> </siteMapNode> </siteMap>

Always start with one database instance running RMAN with two channels In most cases, two RMAN channels per instance will give you the required throughput gains, although you might gain some improvements with four channels Each RMAN channel is capable of processing about 07 GB/s, and two channels translate to 14 GB/s, which is close to the 2 GB/s throughput limitation of one database server Add instances to run RMAN as required, each with two channels Measure throughput gains, and if you are not getting any additional gains, you stop

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All galaxies emit energy at radio wavelengths, as well as in the infrared (IR), visible, ultraviolet (UV), x-ray, and gamma-ray portions of the EM spectrum Usually, the intensity of the radio emissions from galaxies is related to their classification and their observed visual brightness However, some galaxies emit far more energy at radio wavelengths than we would expect These objects are called radio galaxies The intense radio source known as Cygnus A is one such galaxy When radio telescopes are used to map the details of Cygnus A, a double structure is found The radio emission comes from two different regions located on either side of the visible galaxy Other double galaxies have been observed with radio telescopes Several hypotheses have been put forth in an attempt to find out what is taking place in radio galaxies One theory is that they are pairs of colliding galaxies; the magnetic and electrical fields of the two galaxies interact to produce unusual levels of radio-frequency energy Iosif S Shklovskii of Russia theorized that radio galaxies contain more supernovae than do normal galaxies F Hoyle and W A Fowler have suggested that the tremendous energy of the radio galaxies comes from explosions of the galactic nuclei, following or associated with a catastrophic gravitational collapse In any case, it is believed that the nuclei of the radio galaxies are undergoing radical changes

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The site map is an XML file, as indicated by the first line in the file. The entire hierarchy of the file is contained within a single <sitemap> element that defines the namespace:

As more becomes known about radio galaxies, astronomers hope to further unravel the puzzles of galactic formation and evolution

As a RMAN best practice mentioned earlier, configure RAC services to dictate the database servers that will run RMAN Set DB_RECOVER_FILE_DEST_SIZE to bind space in the FRA for backups This was discussed in the section on RMAN earlier

When attempting to determine the distances to other galaxies and other clusters of galaxies, astronomers use tricks These schemes rely on two assumptions: (1) the average brightnesses of the stars in all galaxies are similar, and (2) the average brightnesses of the galaxies in all clusters are similar

NOTE Typical backup throughput was achieved using a full-rack Exadata Database Machine X2-2 with two instances configured to run RMAN, and each instance with four RMAN channels, with RMAN using image copies, was 71 TB/ Hr The backup was stored on FRA residing inside the Database Machine Recommended Disk Backup Strategy The Oracle MAA strategy for performing backups to disk is the following:

Within the siteMap element is nested exactly one <SiteMapNode> (in this case, Home). Nested within that first <SiteMapNode>, however, is any number of children <SiteMapNode> elements. Each <SiteMapNode> element can in turn have any number of children <SiteMapNode> elements.

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