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Most people generally prefer not to edit configuration files by hand, but in the case of SAMBA, this may well be the best route to take. While not quite as simple as using a graphical tool, editing the configuration file by hand is not nearly as difficult as it is with other types of servers. This is because the designers of SAMBA went out of their way to create a configuration file syntax that is easy to read, and a set of configuration options that have logical, intuitive names. SAMBA comes with a very well written manual page just for the configuration file. (Give the command man smb.conf to see it.) Some distributions (notably Fedora Core) include a default configuration file with detailed comments to get you started. The SAMBA configuration file is usually located at /etc/samba/smb.conf. If you want to edit the existing file, you can open it in a text editor. (Do this as the superuser if you want to be able to save your changes.) Alternatively, you can change the name of the existing file to something like /etc/samba/smb.conf-old, and create a new one.

Figure 18-4: A portion of an electrical schematic. 3. To make a block of the 1.5-amp fuse, choose Make Block from the Draw toolbar.

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have been a sea of separate protons. neutrons, electrons etc, strongly interacting with each other. The transition from free protons and neutrons into atomic nuclei is the topic of the next chapter. Going back further in time, when the temperature was even hotter. the situation becomes less clear. because the typical energies start to be so high that the laws of physics become less well known. It is believed that at 10 12 Kelvin it stops making sense even to think of protons and neutrons; instead their constituent quarks are free to wander around in a dense sea (rather reminiscently of the way that in some molecules the electrons are not associated with any particular nucleus). The transition where quarks first condense into protons and neutrons is known as the quark-hadron phase transition [hadron being the technical term for bound states of quarks, either baryons (three quarks) or mesons (a quark and an anti-quark)]. Theoretically this picture is appealing, but observational evidence. obtained by colliding heavy nuclei together, is so far scanty at best. The highest particle energies that have been achieved on Earth are generated by particle accelerators and are around 100 GeV (where GeV is a giga-electron volt. i.e. one thousand MeV), corresponding to an effective temperature of about 10 15 Kelvin. This is the highest energy at which we have direct evidence of the physical behaviour of fundamental particles, and that temperature was achieved only 10- 10 seconds after the Big Bang itself. Earlier yet lies the realm of the very early Universe, where speculations concerning laws of physics such as the unification of fundamental forces must be used. A variety of possible behaviours have been proposed; one particularly prominent idea is cosmological inflation. which I'll come to shortly.

Now that you ve used the Layout Wizard once, you can try creating layouts on your own. The Layout Wizard only creates the floating viewports, leaving most of the scaling, the panning, and other tasks up to you.

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extent appears to be a.. under the assumption of Euclidean geomelly. If we lake the object to lie perpendicular 10 the line of sight and to have physical extenl/. the angular diameter distance is therefore

Rotating with grips is very similar to using the ROTATE command. First, choose all of the objects that you want to rotate. Then click any grip to activate it. This becomes the base point. Right-click to open the Grip shortcut menu and choose Rotate. You see the prompt:

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The above-mentioned studies illustrate the variety of corresponding colors experiments that have been completed. Unfortunately, a clear picture of relative model performance does not emerge from the analysis of these results. This is partly due to the fact that the models have changed, and new ones have emerged, since some of the results were published.

As you work, you can turn the region s color overlay on or off or make the color lighter. This color is a visual guide for you. Turning it off won t remove the map region. See the Seeing Your Work Clearly section later in this chapter.

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