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laser, the mirror, and even the laser beam itself because the occupants of the space vessel have temporarily filled it with smoke to make the viewing easy for us (They have their pressure suits on so that they can breathe) What we see is depicted in Fig 16-3 The laser beam still travels in straight lines, and it still travels at 3 108 m/s relative to us This is true because of Einstein s axiom concerning the speed of light and our own hypothesis to the effect that light rays always appear to travel in straight lines as long as we are not accelerating However, the rays have to travel farther than 3 m to get across the ship The ship is going so fast that by the time the ray of light has reached the mirror from the laser, the ship has moved a significant distance forward The same thing happens as the ray returns to the sensor from the mirror As a result of this, it will seem to us, as we watch the ship from Earth, to take more than 20 ns for the laser beam to go across the ship and back As the ship goes by, time appears to slow down inside it, as seen from a stationary point of view Inside the ship, though, the speed of time seems entirely normal The faster the ship goes, the greater is this discrepancy As the speed of the ship approaches the speed of light, the time dilation factor can become large indeed; in theory, there is no limit to how great it can become You can visualize this by imagining Fig 16-3 stretched out horizontally so that the light rays have to travel almost parallel to the direction of motion, as seen from the stationary reference frame.

ASM automatically stripes files across multiple physical disks, which increases the access performance by spreading I/O over multiple disk heads This placement avoids excessive hot spots in disk files, and also contributes to better I/O performance ASM normally creates stripes based on the size of the allocation unit (AU) assigned to a disk group, but for some files, such as redo logs, ASM stripes are smaller to reduce I/O latency on these crucial files The I/O performance produced by ASM is roughly equivalent to the performance of a raw partition, without having the more extensive management overhead of raw storage In some cases, such as a stretch cluster, where nodes of a cluster are widely separated, ASM can give better performance by reading from a more local mirrored copy of data, rather than trying to access the primary copy at a more distant location This capability is configured by means of an initialization parameter Oracle Database 11g Release 2 introduced a new performance feature for ASM called Intelligent Data Placement A disk is circular, which means that the outer tracks of the disk are moving faster than the inner tracks, resulting in faster read times for data on the outer tracks You can specify that data for a file or an entire disk group is either on the outside or inside of the disk, providing better performance for the outer sections This Intelligent Data Placement works well with two disk groups, one for data and one for the Fast Recovery Area (FRA), which is used for backups The FRA can go on the inner tracks of the disk, ceding the better-performing sections to the data disk groups that are in active production use

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There exists a mathematical relationship between the speed of the space ship in the foregoing mind experiment and the extent to which time is

In terms of disk storage, ASM provides an availability solution by automatically mirroring data in a disk group Mirroring data means making an extra copy of the data in the event of a block or disk failure, similar to the functionality provided by redundant arrays of inexpensive disks (RAID) disks You can choose to mirror data once, to assure reliability if a single point of failure occurs, or twice, to assure reliability even if a second failure should occur You also have the option of not mirroring data, which you might choose if you are using ASM with a RAID disk that already provided mirroring, although ASM mirroring is specifically designed to support database access You can assign mirroring on the basis of individual files to implement different levels of redundancy for different scenarios

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Position of laser/sensor Figure 16-3 This is what an external observer sees as the laser-clock-equipped

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dilated Let tship be the number of seconds that appear to elapse on the moving ship as 1 s elapses as measured by a clock next to us as we sit in our Earth-based observatory Let u be the speed of the ship as a fraction of the speed of light Then tship (1 u2) 1/2

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