Before purchasing equipment or deciding on a hardware platform, you should have a clear idea of the nature of your communications problem. Most likely, you are reading this book because you need to connect computer networks together in order to share resources and ultimately reach the larger global Internet. The network design you choose to implement should fitthe communications problem you are trying to solve. Do you need to connect a remote site to an Internet connection in the center of your campus? Will your network likely grow to include several remote sites? Will most of your network components be installed in fixed locations, or will your network expand to include hundreds of roaming laptops and other devices?
When solving a complex problem, it is often useful to draw a picture of your resources and problems. In this chapter, we will look at how other people have built wireless networks to solve their communication problems, including diagrams of the essential network structure. We will then cover the networking concepts that define TCP/IP, the primary networking language currently spoken on the Internet. We will then demonstrate several common methods for getting your information to flow efficiently through your network and on to the rest of the world.
Saturday, March 15, 2008
Physics in the Real World
Don't worry if the concepts in this chapter seem challenging. Understanding how radio waves propagate and interact with the environment is a complex field of study in itself. Most people find it difficult to understand phenomena that they can't even see with their own eyes. By now you should understand that radio waves don't travel in a straight, predictable path. To make reliable communication networks, you will need to be able to calculate how much power is needed to cross a given distance, and predict how the waves will travel along the way.
There is much more to learn about radio physics than we have room for here. For more information about this evolving field, see the resources list in Appendix A. Now that you have an idea of how to predict how radio waves will interact in the real world, you are ready to start using them for communications.
There is much more to learn about radio physics than we have room for here. For more information about this evolving field, see the resources list in Appendix A. Now that you have an idea of how to predict how radio waves will interact in the real world, you are ready to start using them for communications.
Calculating with dBs
By far the most important technique when calculating power is calculating with decibels (dB). There is no new physics hidden in this -it is just a convenient method which makes calculations a lot simpler.
The decibel is a dimensionless unit1, that is, it defines a relationship between two measurements of power. It is defined by:
Why are decibels so handy to use? Many phenomena in nature happen to behave in a way we call exponential. For example, the human ear senses a sound to be twice as loud as another one if it has ten times the physical signal.
Another example, quite close to our field of interest, is absorption. Suppose a wall is in the path of our wireless link, and each meter of wall takes away half of the available signal. The result would be:
Here are some commonly used values that are important to remember:
The decibel is a dimensionless unit1, that is, it defines a relationship between two measurements of power. It is defined by:
dB = 10 * Log (P1/P0)
where P1 and P0 can be whatever two values you want to compare. Typically, in our case, this will be some amount of power.
Why are decibels so handy to use? Many phenomena in nature happen to behave in a way we call exponential. For example, the human ear senses a sound to be twice as loud as another one if it has ten times the physical signal.
Another example, quite close to our field of interest, is absorption. Suppose a wall is in the path of our wireless link, and each meter of wall takes away half of the available signal. The result would be:
0 meters = 1 (full signal)
1 meter = 1/2
2 meters = 1/4
3 meters = 1/8
4 meters = 1/16
n meters = 1/2n = 2-n
This is exponential behaviour.
But once we have used the trick of applying the logarithm (log), things become a lot easier: instead of taking a value to the n-th power, we just multiply by n. Instead of multiplying values, we just add.
Here are some commonly used values that are important to remember:
+3 dB = double power
-3 dB = half the power
+10 dB = order of magnitude (10 times power)
-10 dB = one tenth power
In addition to dimensionless dBs, there are a number of relative definitions that are based on a certain base value P0. The most relevant ones for us are:
dBm relative to P0 = 1 mW
dBi relative to an ideal isotropic antenna
An isotropic antenna is a hypothetical antenna that evenly distributes power in all directions. It is approximated by a dipole, but a perfect isotropic antenna cannot be built in reality. The isotropic model is useful for describing the relative power gain of a real world antenna.
Another common (although less convenient) convention for expressing power is in milliwatts. Here are equivalent power levels expressed in milliwatts and dBm:
1 mW = 0 dBm
2 mW = 3 dBm
100 mW = 20 dB
m1 W = 30 dBm
Another example of a dimensionless unit is the percent (%) which can also be used in all kinds of quantities or numbers. While measurements like feet and grams are fixed, dimensionless units represent a relationship.
Subscribe to:
Posts (Atom)