Location and Scale in the Normal Model
A normal model is often used when measurements fluctuate around a typical value and are described on a particular measurement scale. Its two parameters answer different questions: where is the distribution centered? and how spread out is it? Keeping those roles distinct makes it possible to change units, compare observations to a standard reference, and calculate probabilities without repeatedly integrating a new density.
In this tutorial, \(\mu\) is the location and \(\sigma\) is the scale. The scale is positive, and the variance is its square. This distinction is important because normal notation conventionally places the variance—not the standard deviation—in the second argument.
The density formula is a shifted and rescaled version of the standard normal density: \(f_X(x)=\sigma^{-1}\phi((x-\mu)/\sigma)\). The factor \(1/\sigma\) adjusts the density height when the horizontal scale changes; it ensures the density still integrates to one. The standardization \(z=(x-\mu)/\sigma\) expresses a value as its signed distance from \(\mu\), measured in units of \(\sigma\).
Standardizing a Normal Variable
The standard normal variable gives one common scale for all normal models. The following result justifies standardization directly from the density.
Proof. The map \(x\mapsto z=(x-\mu)/\sigma\) is strictly increasing, with inverse \(x=\mu+\sigma z\) and derivative \(dx/dz=\sigma\). Applying the change-of-variables formula to the density of \(X\),
Thus \(Z\) has the standard normal density. Since the transformation is increasing, the event \(X\le x\) is exactly the event \(Z\le (x-\mu)/\sigma\), giving the stated CDF formula. \(\square\)
The parameters also have their usual moment interpretation. The standard normal density is symmetric about zero, so its mean is zero. For the variance, integration by parts gives
In the integration by parts, use \(z^2e^{-z^2/2}=z(ze^{-z^2/2})\); the boundary term \(-ze^{-z^2/2}\) tends to zero at both limits, and the remaining integral is the normalized Gaussian integral. Since \(X=\mu+\sigma Z\), linearity of expectation and the variance rule for multiplication by a constant yield \(E[X]=\mu\) and \(\operatorname{Var}(X)=\sigma^2\). This confirms why \(\mu\) is called location and \(\sigma\) scale.
Worked Example: Standardizing a Measurement
Suppose an adult’s resting heart rate \(X\), in beats per minute, is modeled as \(N(70,8^2)\). Find the standardized value for \(X=82\), and express the probability that the heart rate is at most 82.
The location is \(\mu=70\), and the scale is \(\sigma=8\) beats per minute. Therefore,
The observation is 1.5 standard deviations above the model’s location. By the standardization result, \(P(X\le82)=\Phi(1.5)\). Using the supplied standard normal value \(\Phi(1.5)\approx0.9332\), the probability is approximately \(0.9332\). The standardization determines which standard normal probability is needed; evaluating \(\Phi\) numerically is a separate table or software step.
Affine Changes of Location and Scale
A measurement may be shifted or recorded in different units. If \(Y=a+bX\), the constant \(a\) shifts every value and \(b\) multiplies every value. For a normal variable, the transformed distribution remains normal. The absolute value of \(b\) matters for spread: a negative multiplier reverses direction but cannot produce a negative standard deviation.
Proof. The inverse transformation is \(x=(y-a)/b\), and its absolute derivative is \(1/|b|\). The change-of-variables formula gives
Because \(\phi(u)=\phi(-u)\), the last density can be written with denominator \(|b|\sigma\) inside its squared argument:
This is the normal density with location \(a+b\mu\) and scale \(|b|\sigma\), so its variance is \(b^2\sigma^2\). \(\square\)
For probability calculations, standardize the endpoints. If \(l<u\), continuity of the normal distribution means endpoint inclusion does not change the probability, and
The upper standardized endpoint appears first because the CDF gives probability to the left of its argument. For an affine transformation with a negative multiplier, it is usually safest to transform the event carefully or use the transformed normal model and order the resulting endpoints from low to high.
Worked Example: Probability Within an Interval
Let \(X\sim N(70,8^2)\). Calculate \(P(62\le X\le82)\).
Standardize each endpoint using the same location and scale:
Thus the event becomes \(-1\le Z\le1.5\), and subtracting the lower-tail probabilities gives
The interval contains approximately \(77.45\%\) of the modeled probability. Both endpoints must be standardized: using only the upper endpoint would give the probability below 82, not the probability between 62 and 82.
Worked Example: A Negative Multiplier and a Transformed Interval
Suppose \(X\sim N(4,1.5^2)\) and a reported score is \(Y=20-2X\). Find \(P(10<Y\le16)\).
First transform the model. Here \(a=20\) and \(b=-2\), so \(Y\) has location \(20-2(4)=12\), scale \(|-2|(1.5)=3\), and variance \(3^2=9\). Hence \(Y\sim N(12,9)\). Directly standardizing the ordered score endpoints gives
Therefore,
As a check on the negative sign, transform the event back to \(X\). The inequality \(10<20-2X\le16\) gives \(2\le X<5\): the upper bound on \(Y\) produces the lower bound on \(X\), while the lower bound on \(Y\) produces the upper bound on \(X\). Standardizing these \(X\)-endpoints gives \((2-4)/1.5=-4/3\) and \((5-4)/1.5=2/3\). Thus the probability is \(\Phi(2/3)-\Phi(-4/3)\), which equals the previous expression by the symmetry identity \(\Phi(-z)=1-\Phi(z)\).
Common Mistakes and Why the Parameterization Matters
The location-scale form is useful because it separates a model’s shape from its units. Standardization lets a single reference distribution handle calculations for many choices of \(\mu\) and \(\sigma\). Affine transformations then account for recoding, unit conversion, or a score that reverses direction. These operations are common in measurement and modeling, but they are also frequent sources of avoidable errors.
- Using the variance as the scale. In \(N(\mu,\sigma^2)\), the standardizing denominator is \(\sigma\), not \(\sigma^2\). If the model is \(N(70,64)\), its scale is \(8\), not \(64\).
- Forgetting the absolute value for a negative multiplier. If \(Y=a+bX\), its standard deviation is \(|b|\sigma\), even when \(b<0\). Its variance is \(b^2\sigma^2\).
- Leaving an inequality unreversed after dividing by a negative number. When transforming an event through \(Y=a+bX\) with \(b<0\), the order of the bounds reverses. Check the transformed bounds by testing a value or use the model for \(Y\) directly.
- Subtracting CDF values in the wrong order. For an interval, subtract the CDF at the lower endpoint from the CDF at the upper endpoint.
Check Your Understanding
For each question, keep the scale distinct from the variance and show how the endpoints or parameters are transformed.
- If \(X\sim N(12,25)\), what are its location and scale, and what is the standardized value of \(X=17\)?
- For \(X\sim N(50,10^2)\), express \(P(40\le X\le65)\) using \(\Phi\), without evaluating the CDFs.
- If \(X\sim N(3,2^2)\) and \(Y=5+4X\), state the location, scale, and variance of \(Y\).
- If \(X\sim N(0,1)\) and \(Y=8-3X\), what is the location and scale of \(Y\), and why is its scale positive?
- Explain why standardizing both endpoints is necessary when calculating the probability that a normal variable falls within an interval.