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Ingredients Dried ageolet beans Sachet (p. 152) Water or light vegetable stock Garlic cloves, peeled and chopped Salt Olive oil Lemon juice Additional salt Pepper

In the first line all cron messages of err priority and higher are logged to the file /var/log/cron. The second line has all auth messages except those of emerg priority being sent to a local printer lpr3. The third line sends all auth-priv messages to the users root and bob if they are logged in. The fourth sends all news messages of notice or greater priority to a named pipe called /var/log/newspipe (you would need to create this pipe yourself with the mkfifo command).

s Caution When logging to files, syslogd allows you to add a hyphen (-) to the front of the filename like

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this: -/var/log/auth. This tells syslog to not sync the file after writing to it. This is designed to speed up the process of writing to the log. But it can also mean that if your system crashes between write attempts, you will lose data. Unless your logging system is suffering from performance issues, I recommend you do not use this option.

As mentioned previously, this chapter will reuse the code of recipe 3-11, so a basic understanding of spherical billboarding is recommended. For each particle, you ll again define six vertices, which you ll want to define only once so they can be transferred to the graphics card and remain there untouched. For each vertex, you ll want the following data to be available to the vertex shader in the GPU: The original 3D position center of the billboard at the start of the explosion (required for billboarding) (Vector3 = three floats) The texture coordinates (required for billboarding) (Vector2 = two floats) The time at which the particle was created (one float) How long you want the particle to stay alive (one float) The direction in which you want the particle to move (Vector3 = three floats) A random value, which will be used to make each particle behave uniquely (one float) From this data, the GPU can calculate everything it needs to know, based on the current time. For example, it can calculate how long the particle has been alive. When you multiply this age by the direction of the particle, you can find how far it s off the original position of the particle, which was the center of the explosion.

ome things on your hard disk are valuable. Music you purchase online costs money. Pictures and videos from digital cameras are irreplaceable. Documents you spent hours creating required an investment of your time. You wouldn t want to lose those things because of some technical problem or mistake you made. So it s a good idea to keep backups. That way, if you do lose the originals on your hard disk, you can just restore them from your backup copy. In addition to the files you create and use yourself, there are many system files on your hard disk. These are files that Windows Vista needs to function properly. If those files get messed up, your computer may not work correctly. So you need some means of backing up those system files as well. This chapter explains how to back up both your personal files and your system files. Of course, the backups won t do you any good if you can t use them when you need them. So, of course, we ll talk about how to use those backups should the need ever arise to get your system back in shape. We ll also talk about System Protection, which keeps copies of some files around temporarily, to help you fix minor mishaps on the spot, without having to fumble around with external disks.

You can also log to a remote system (see Listing 5-4). Listing 5-4. Logging to a Remote System mail @puppy.yourdomain.com

In this example all mail messages are sent to the host puppy.yourdomain.com on UDP port 514. This requires that the syslogd daemon on puppy is started with the -r option; otherwise, the syslogd port will not be open.

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