Notes on the Normal Distribution and Standard Deviation
Notation and core ideas
Sigma (σ) denotes the standard deviation; it measures the variation or spread of a random variable around its mean. It answers: how far, on average, data deviate from the mean.
The standard deviation is a measure of spread with the same units as the variable X.
Common shorthand: the normal distribution is often written as X ~ N(μ, σ^2), where
μ is the mean (center of the distribution),
σ is the standard deviation, and
σ^2 is the variance.
The statement “X is normal” typically means X is distributed normally, i.e., X ~ N(μ, σ^2).
Observed values are written in lowercase x; random variables are written in uppercase X.
The phrase “norm is normalized” refers to standardizing a normal variable to a standard normal form.
Normal distribution basics
Distribution notation: X∼N(μ,σ2) which means X has a normal distribution with mean μ and variance σ^2.
Mean and variance:
Mean: E[X]=μ
Variance: Var(X)=σ2
Standard deviation: SD(X)=σ
The normal distribution is symmetric and bell-shaped; many real-valued phenomena are modeled as approximately normal when they are the sum of many small independent effects (Central Limit Theorem).
Standardization (normalization) to the standard normal
Standardization transforms X into a standard normal variable Z with mean 0 and variance 1:
Z = X \2{\mu}{\sigma} = \frac{X - μ}{σ}
Z∼N(0,1)
Purpose: enables comparison across different normal distributions and facilitates use of standard normal tables (z-tables) for probabilities.
If you know μ and σ, you can convert any X to Z and read probabilities from the standard normal distribution.
Worked example
Suppose a measurement X has parameters μ = 100 and σ = 15.
If X = 115, the standardized value is
Z=15115−100=1
Interpretation: the observed value 115 is 1 standard deviation above the mean.
If X is exactly 100, then Z = 0 (at the mean).
Probability density and cumulative concepts (normal case)
PDF of X when X ~ N(μ, σ^2):
fX(x)=σ2π1exp(−2σ2(x−μ)2)
CDF (probability up to x):
F<em>X(x)=P(X≤x)=∫</em>−∞xfX(t)dt
Probability within an interval:
P(a≤X≤b)=∫<em>abf</em>X(x)dx
For many practical purposes, probabilities are computed via standard normal tables or software using the z-score transformation.
Notational pitfalls and clarifications
Distinguish: uppercase X (random variable) vs lowercase x (a realized value).
When we write X ~ N(μ, σ^2), we mean the distribution of the random variable X, not a specific observed value.
The term “normalized” commonly refers to converting to the standard normal form via Z = (X - μ)/σ.
Connections and relevance
The normal model is a foundational assumption in many statistical methods (confidence intervals, hypothesis tests, regression residuals) due to the Central Limit Theorem and mathematical convenience.
Real-world relevance: measurement error, natural phenomena with many small additive effects, and standardization for comparability across datasets.