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by partners or was simply lacking Oracle Database 10 g Enterprise Edition was introduced in 2003 with Automatic Storage Management (ASM) and embedded cluster management software, eliminating the need for thirdparty software that provided those capabilities ASM virtualizes storage resources and provides advanced volume management, thus enabling the database and DBA to manage tasks such as striping and mirroring of data The Automatic Database Diagnostics Monitor (ADDM) also first appeared in this release and provided advisory alerts and suggestions for tactics to improve performance based on periodic snapshots of performance in a production environment These suggestions are displayed to DBAs by Enterprise Manager s Grid Control, whose enhanced alerting and management capabilities are critically important when deploying Oracle for large-scale databases and for grid computing In 2005, penguins appeared on stage at Oracle OpenWorld in what was seen as a curious announcement at the time but would have important implications in establishing a complete Oracle platform Oracle announced it would provide support for Red Hat and SUSE Linux and deliver an unbreakable Linux support model Oracle later introduced Oracle Enterprise Linux, which has roots in Red Hat Linux from the open-source community to which Oracle had long provided technology Meanwhile, Oracle had begun work on establishing reference configurations for data warehousing on Linuxbased and other platforms from a variety of platform vendors Taken together, these moves by Oracle and the changes in the deployment strategies at many of Oracle customers led to Oracle s decision to launch a tightly integrated hardware and software platform The initial platform, the HP Oracle Database Machine with Exadata storage, became available in 2008 In 2009, Oracle announced a second generation of the Oracle Exadata Database Machine and a new hardware platform the Sun Oracle Database Machine The acquisition of Sun by Oracle Corporation in 2010 completed the transition of Oracle to a vendor that can design, build, and support complete database hardware and software solutions that are deployed as systems In September 2010, Oracle announced new X2-2 and X2-8 nodes for the Oracle Exadata Database Machine and also announced Solaris 11 as an alternative to the Oracle Enterprise Linux operating system for database server nodes The Unbreakable Enterprise Kernel for Linux was announced at this time to provide support for the large number of processing cores made available in the Exadata Database Machine We ll discuss some implications of the Sun acquisition later in this chapter and some of the likely future directions Table 1-1 summarizes some of the important events and timing that led to the Oracle Exadata Database Machine.

The problems inherent in refracting telescopes, particularly chromatic aberration and lens sag, can be largely overcome by using mirrors instead of lenses as objectives A first-surface mirror, with the silvering on the outside so that the light never passes through glass, can be ground so that it brings light to a focus that does not vary with wavelength Mirrors can be supported from behind, so it is possible to make them larger than lenses without running into the sag problem

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When you compile the program, you will get a compiler error because the keyword to declare an integer is misspelled. Using the IDE dramatically reduces your syntax errors. Depending on how the IDE is configured, any code element that isn t recognized is underlined. If Auto List Members is turned on (Tools Options Text Editor All Languages), the incidence of syntax errors is further reduced. Check the Show All Settings checkbox (and leave it checked) to see these menu options. If any syntax errors remain or if you are using a different editor, then any syntax errors will be caught by the compiler every time you build the project. It is very difficult for a syntax error to slip by into production code.

Isaac Newton designed a reflecting telescope that was free of chromatic aberration His design is still used in many reflecting telescopes today The Newtonian reflector employs a concave objective mounted at one end of a long tube The other end of the tube is open to admit incoming light A small, flat mirror is mounted at a 45-degree angle near the open end of the tube to reflect the focused light through an opening in the side of the tube containing the eyepiece (Fig 17-9A) The flat mirror obstructs some of the incoming light, slightly reducing the effective surface area of the objective mirror As a typical example, suppose that a Newtonian reflector has an objective mirror 20 cm in diameter The total surface area of this mirror is approximately 314 centimeters squared (cm2) If the eyepiece mirror is 3 cm square, its total area is 9 cm2, which is about 3 percent of the total surface area of the objective Newtonian reflectors have limitations Some people find it unnatural to look sideways at objects If the telescope has a long tube, it is necessary to use a ladder to view objects at high elevations These annoyances can be overcome by using a different way to get the light to the eyepiece

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Figure 17-9B shows the design of the Cassegrain reflector The eyepiece mirror is closer to the objective than in the Newtonian design It is not angled, but it is convex The convexity of this mirror increases the effective focal length of the objective mirror Light reflects from the convex mirror and passes through a small hole in the center of the objective containing the eyepiece The Cassegrain reflector can be made with a physically short tube and an objective mirror having a smaller radius of curvature than that of a Newtonian telescope having the same diameter Thus the Cassegrain telescope is less massive and less bulky Cassegrain reflectors with heavy-duty mountings are physically stable, and they can be used at low magnification to obtain wide views of the sky

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When the compiler finds a syntax error, an error message containing the location of the error and a terse explanation will be displayed in the Output window of the IDE. If the error is caused by something such as an unbalanced parenthesis or bracket, or a missing semicolon in C#, then the actual error may not be on the reported line.

Several parameters are significant when determining the effectiveness of a telescope for various applications Here are the most important ones

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