The normal distribution is used to model continuous data with a distribution
symmetric about the mean. It depends on two parameters, the mean µ
and the standard deviation s. If X follows the
normal distribution with mean µ and standard deviation s,
this is by convention written X~N(µ, s
2), because the variance s 2
is a more fundamental quantity in statistical theory.
The density function f(x) is given by
This function is also called the "pdf" for probability density
function. All normal pdf's have the same shape. The curve is symmetric
about the mean µ = E(X), approaches zero at ± infinity and
has points of inflection (changes between 'concave down' and 'concave
up') at µ±s.
Some authors prefer to denote a Normal distribution as N(µ, s) rather than N(µ, s 2). The textbook by Moore and McCabe refers to a Normal distribution according to µ and s. Minitab requires values for µ and s to define a Normal distribution.
In keeping with the more general convention in the statistical literature, this course will assume that the Normal curve is defined according to µ and s 2. That is, X~N(µ, s 2).
For example, if X~N(10, 16) then this implies that µ = 10 and s 2 = 16 (hence s = 4).
The area under a density curve represents relative frequency so any question about relative frequency can be answered by calculating areas under the curve.
In order to obtain these areas for the Normal distribution (i.e. areas
under the curve), it is necessary to express any value of X in terms of the
number of standard deviation units it is away from m
.
This is called the standard normal distribution.
Most introductory statistics textbooks, including this, include a table of the standard Normal distribution. It tabulates the area under the curve of the N(0,1) density function.
Tables in other normal tables may give other areas, e.g.
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