Autore della sezione: Danielle J. Navarro and David R. Foxcroft

The normal distribution

While the binomial distribution is conceptually the simplest distribution to understand, it is not the most important one. That particular honour goes to the normal distribution, also referred to as “the bell curve” or a “Gaussian distribution”. A normal distribution is described using two parameters: the mean of the distribution µ and the standard deviation of the distribution σ. The notation that we sometimes use to say that a variable X is normally distributed is as follows:

X ~ Normal(µ, σ)

Of course, that is just notation. It does not tell us anything interesting about the normal distribution itself. As was the case with the binomial distribution, I have included the formula for the normal distribution in this book, because I think it is important enough that everyone who learns statistics should at least look at it, but since this is an introductory text I do not want to focus on it, so I have tucked it away in Tabella 7.

Fig. 61 The normal distribution with mean μ = 0 and standard deviation σ = 1. The x-axis corresponds to the value of some variable, and the y-axis tells us something about how likely we are to observe that value. However, notice that the y-axis is labelled “Probability Density” and not “Probability”.

Instead of focusing on the maths, let us try to get a sense for what it means for a variable to be normally distributed. To that end, have a look at Fig. 61 which plots a normal distribution with mean µ = 0 and standard deviation σ = 1. You can see where the name “bell curve” comes from; it looks a bit like a bell. Notice that, unlike the plots that I drew to illustrate the binomial distribution, the picture of the normal distribution in Fig. 61 shows a smooth curve instead of “histogram-like” bars. This is not an arbitrary choice, the normal distribution is continuous whereas the binomial is discrete.[1] For instance, in the dice rolling example from the last section it was possible to get three skulls or four skulls, but impossible to get 3.9 skulls. The figures that I drew in the previous section reflected this fact. In Fig. 59, for instance, there is a bar located at X = 3 and another one at X = 4 but there is nothing in between. Continuous quantities do not have this constraint. For instance, suppose we are talking about the weather. The temperature on a pleasant spring day could be 23 degrees, 24 degrees, 23.9 degrees, or anything in between since temperature is a continuous variable . And so a normal distribution might be quite appropriate for describing spring temperatures.[2]

Fig. 62 Illustration of what happens when you change the mean of a normal distribution. The solid line depicts a normal distribution with a mean of μ = 4. The dashed line shows a normal distribution with a mean of μ = 7. In both cases, the standard deviation is σ = 1. Not surprisingly, the two distributions have the same shape, but the dashed line is shifted to the right.

With this in mind, let us see if we can not get an intuition for how the normal distribution works. First, let us have a look at what happens when we play around with the parameters of the distribution. To that end, Fig. 62 plots normal distributions that have different means but have the same standard deviation. As you might expect, all of these distributions have the same “width”. The only difference between them is that they have been shifted to the left or to the right. In every other respect they are identical. In contrast, if we increase the standard deviation while keeping the mean constant, the peak of the distribution stays in the same place but the distribution gets wider, as you can see in Fig. 63.

Fig. 63 Illustration of what happens when you change the standard deviation of a normal distribution. Both distributions plotted in this figure have a mean of μ = 5, but they have different standard deviations. The solid line plots a distribution with standard deviation σ = 1, and the dashed line shows a distribution with standard deviation σ = 2. As a consequence, both distributions are “centred” on the same spot, but the dashed line is wider than the solid one.

Notice, though, that when we widen the distribution the height of the peak shrinks. This has to happen, in the same way that the heights of the bars that we used to draw a discrete binomial distribution have to sum to 1, the total area under the curve for the normal distribution must equal 1.

Fig. 64 The area under the curve tells you the probability that an observation falls within a particular range. The solid lines plot normal distributions with mean μ = 0 and standard deviation σ = 1. The shaded areas illustrate “areas under the curve” for two important cases. In the left panel, we can see that there is a 68.3% chance that an observation will fall within one standard deviation of the mean. In the right panel, we see that there is a 95.4% chance that an observation will fall within two standard deviations of the mean.

Fig. 65 Two more examples of the “area under the curve” idea. There is a 15.9% chance that an observation is one standard deviation below the mean or smaller (left panel), and a 34.1% chance that the observation is somewhere between one standard deviation below the mean and the mean (right panel). Notice that if you add these two numbers together you get 15.9% + 34.1% = 50%. For normally distributed data, there is a 50% chance that an observation falls below the mean. And of course that also implies that there is a 50% chance that it falls above the mean.

Before moving on, I want to point out one important characteristic of the normal distribution. Irrespective of what the actual mean and standard deviation are, 68.3% of the area falls within 1 standard deviation of the mean. Similarly, 95.4% of the distribution falls within two standard deviations of the mean, and 99.7% of the distribution is within three standard deviations. This idea is illustrated in Fig. 64, see also Fig. 65.

Probability density

There is something I have been trying to hide throughout my discussion of the normal distribution, something that some introductory textbooks omit completely. They might be right to do so. This “thing” that I am hiding is weird and counter-intuitive even by the admittedly distorted standards that apply in statistics. Fortunately, it is not something that you need to understand at a deep level in order to do basic statistics. Rather, it is something that starts to become important later on when you move beyond the basics. So, if it does not make complete sense, do not worry too much, but try to make sure that you follow the gist of it.

Throughout my discussion of the normal distribution there is been one or two things that do not quite make sense. Perhaps you noticed that the y-axis in these figures is labelled “Probability Density” rather than “Density”. Maybe you noticed that I used p(X) instead of P(X) when giving the formula for the normal distribution.

As it turns out, what is presented here is not actually a probability, it is something else. To understand what that something is you have to spend a little time thinking about what it really means to say that X is a continuous variable . Let us say we are talking about the temperature outside. The thermometer tells me it is 23 degrees, but I know that is not really true. It is not exactly 23 degrees. Maybe it is 23.1 degrees, I think to myself. But I know that that is not really true either because it might actually be 23.09 degrees. But I know that… well, you get the idea. The tricky thing with genuinely continuous quantities is that you never really know exactly what they are.

Now think about what this implies when we talk about probabilities. Suppose that tomorrow’s maximum temperature is sampled from a normal distribution with mean 23 and standard deviation 1. What is the probability that the temperature will be exactly 23 degrees? The answer is “zero”, or possibly “a number so close to zero that it might as well be zero”. Why is this? It is like trying to throw a dart at an infinitely small dart board. No matter how good your aim, you will never hit it. In real life you will never get a value of exactly 23. It will always be something like 23.1 or 22.99998 or suchlike. In other words, it is completely meaningless to talk about the probability that the temperature is exactly 23 degrees. However, in everyday language if I told you that it was 23 degrees outside and it turned out to be 22.9998 degrees you probably would not call me a liar. Because in everyday language “23 degrees” usually means something like “somewhere between 22.5 and 23.5 degrees”. And while it does not feel very meaningful to ask about the probability that the temperature is exactly 23 degrees, it does seem sensible to ask about the probability that the temperature lies between 22.5 and 23.5, or between 20 and 30, or any other range of temperatures.

The point of this discussion is to make clear that when we are talking about continuous distributions it is not meaningful to talk about the probability of a specific value. However, what we can talk about is the probability that the value lies within a particular range of values. To find out the probability associated with a particular range what you need to do is calculate the “area under the curve”. We have seen this concept already, in Fig. 64 the shaded areas shown depict genuine probabilities (e.g., in the left panel of Fig. 64 it shows the probability of observing a value that falls within one standard deviation of the mean).

That explains part of the story. I have explained a little bit about how continuous probability distributions should be interpreted (i.e., area under the curve is the key thing). But what does the formula for p(x) that I described earlier actually mean? Obviously, p*(x) does not describe a probability, but what is it? The name for this quantity p(x) is a probability density, and in terms of the plots we have been drawing it corresponds to the height of the curve. The densities themselves are not meaningful in and of themselves, but they are “rigged” to ensure that the area under the curve is always interpretable as genuine probabilities. To be honest, that is about as much as you really need to know for now.[3]

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[1]

There is a subtle and somewhat frustrating characteristic of continuous distributions that makes the y-axis behave a bit oddly – the height of the curve here is not actually the probability of observing a particular x value. On the other hand, it is true that the heights of the curve tells you which x values are more likely (the higher ones!; see the section ref:` Probability density <probability_density>` for all the annoying details).

[2]

In practice, the normal distribution is so handy that people tend to use it even when the variable is not actually continuous. As long as there are enough categories (e.g., Likert scale responses to a questionnaire), it is pretty standard practice to use the normal distribution as an approximation. This works out much better in practice than you would think.

[3]

For those readers who know a little calculus, I will give a slightly more precise explanation. In the same way that probabilities are non-negative numbers that must sum to 1, probability densities are non-negative numbers that must integrate to 1 (where the integral is taken across all possible values of X). To calculate the probability that X falls between a and b we calculate the definite integral of the density function over the corresponding range, \(\int_a^b p(x) \ dx\). If you do not remember or never learned calculus, do not worry about this. It is not needed for this book.