Definition and Formula
Standard deviation measures the amount of variation or dispersion in a set of values. For a population, it is calculated using the formula σ = √[Σ(xi - μ)² / N], where σ is the standard deviation, xi are the data points, μ is the population mean, and N is the number of data points. For a sample, use s = √[Σ(xi - x̄)² / (n-1)], where x̄ is the sample mean and n is the sample size. This quantifies how spread out the values are from the mean.
Step-by-Step Calculation Process
To calculate standard deviation: 1) Find the mean by summing all values and dividing by the number of values. 2) Subtract the mean from each value to get deviations. 3) Square each deviation. 4) Sum the squared deviations. 5) Divide by N (population) or n-1 (sample). 6) Take the square root of the result. This process accounts for variability, with larger values indicating greater spread.
Practical Example
Consider the dataset: 2, 4, 4, 4, 5, 5, 7, 9 (n=8). The mean is 5. First, deviations: -3, -1, -1, -1, 0, 0, 2, 4. Squared: 9, 1, 1, 1, 0, 0, 4, 16 (sum=32). For sample: 32 / 7 ≈ 4.57, square root ≈ 2.14. This shows the data spreads about 2.14 units from the mean, illustrating moderate variability.
Importance and Applications
Standard deviation is crucial in statistics for assessing data reliability, risk in finance (e.g., stock volatility), and quality control in manufacturing. It helps identify outliers and compare datasets. A common misconception is that it measures central tendency; instead, it focuses on spread, complementing the mean for a fuller data picture.