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Guide: The Normal Distribution

The normal distribution (Gaussian distribution) is a symmetric, bell-shaped probability distribution characterised by two parameters: the mean μ (centre) and the standard deviation σ (width).

It is the most important distribution in statistics because, due to the Central Limit Theorem, the average of a large number of independent measurements will be approximately normally distributed regardless of the original distribution.

In any normal distribution:

  • 68% of values fall within ±1 standard deviation of the mean
  • 95% of values fall within ±2 standard deviations
  • 99.7% of values fall within ±3 standard deviations

This is why values with z > 3 are considered very unusual — only 0.3% of a normal distribution lies beyond ±3σ.

The PDF (probability density function) gives the relative likelihood of a specific value. The area under the PDF between two points gives the probability of falling in that range.

The CDF (cumulative distribution function) gives P(X ≤ x) — the probability that a randomly drawn value is at most x. The CDF ranges from 0 to 1 and is equivalent to the percentile rank.

The standard normal distribution has μ = 0 and σ = 1. Any normal distribution can be converted to standard normal by computing z-scores: z = (x − μ) / σ.

Use the Z-Score Calculator to perform this standardisation and look up tail probabilities.