Standard deviation
In statistics and probability theory, the standard deviation (SD) (represented by the Greek letter sigma, σ) measures the amount of variation or dispersion from the average.^{[1]} A low standard deviation indicates that the data points tend to be very close to the mean (also called expected value); a high standard deviation indicates that the data points are spread out over a large range of values.
The standard deviation of a random variable, statistical population, data set, or probability distribution is the square root of its variance. It is algebraically simpler though in practice less robust than the average absolute deviation.^{[2]}^{[3]} A useful property of the standard deviation is that, unlike the variance, it is expressed in the same units as the data. Note, however, that for measurements with percentage as the unit, the standard deviation will have percentage points as the unit.
In addition to expressing the variability of a population, the standard deviation is commonly used to measure confidence in statistical conclusions. For example, the margin of error in polling data is determined by calculating the expected standard deviation in the results if the same poll were to be conducted multiple times. The reported margin of error is typically about twice the standard deviation—the halfwidth of a 95 percent confidence interval. In science, researchers commonly report the standard deviation of experimental data, and only effects that fall much farther than two standard deviations away from what would have been expected are considered statistically significant—normal random error or variation in the measurements is in this way distinguished from causal variation. The standard deviation is also important in finance, where the standard deviation on the rate of return on an investment is a measure of the volatility of the investment.
When only a sample of data from a population is available, the term standard deviation of the sample or sample standard deviation can refer to either the abovementioned quantity as applied to those data or to a modified quantity that is a better estimate of the population standard deviation (the standard deviation of the entire population).
Contents
 Basic examples 1

Definition of population values 2
 Discrete random variable 2.1
 Continuous random variable 2.2

Estimation 3
 Uncorrected sample standard deviation 3.1
 Corrected sample standard deviation 3.2
 Unbiased sample standard deviation 3.3
 Confidence interval of a sampled standard deviation 3.4
 Identities and mathematical properties 4

Interpretation and application 5

Application examples 5.1
 Weather 5.1.1
 5.1.2 Particle physics
 Finance 5.1.3
 Geometric interpretation 5.2
 Chebyshev's inequality 5.3
 Rules for normally distributed data 5.4

Application examples 5.1

Relationship between standard deviation and mean 6
 Standard deviation of the mean 6.1

Rapid calculation methods 7
 Weighted calculation 7.1

Combining standard deviations 8
 Populationbased statistics 8.1
 Samplebased statistics 8.2
 History 9
 See also 10
 References 11
 External links 12
Basic examples
For a finite set of numbers, the standard deviation is found by taking the square root of the average of the squared differences of the values from their average value. For example, consider a population consisting of the following eight values:
 2,\ 4,\ 4,\ 4,\ 5,\ 5,\ 7,\ 9.
These eight data points have the mean (average) of 5:
 \frac{2 + 4 + 4 + 4 + 5 + 5 + 7 + 9}{8} = 5.
First, calculate the difference of each data point from the mean, and square the result of each:
 \begin{array}{lll} (25)^2 = (3)^2 = 9 && (55)^2 = 0^2 = 0 \\ (45)^2 = (1)^2 = 1 && (55)^2 = 0^2 = 0 \\ (45)^2 = (1)^2 = 1 && (75)^2 = 2^2 = 4 \\ (45)^2 = (1)^2 = 1 && (95)^2 = 4^2 = 16. \\ \end{array}
Next, calculate the mean of these values, and take the square root:
 \sqrt{ \frac{9 + 1 + 1 + 1 + 0 + 0 + 4 + 16}{8} } = 2.
This quantity is the population standard deviation, and is equal to the square root of the variance. This formula is valid only if the eight values with which we began form the complete population. If the values instead were a random sample drawn from some larger parent population, then we would have divided by 7 (which is n−1) instead of 8 (which is n) in the denominator of the last formula, and then the quantity thus obtained would be called the sample standard deviation. Dividing by n−1 gives a better estimate of the population standard deviation than dividing by n.
As a slightly more complicated reallife example, the average height for adult men in the United States is about 70 inches, with a standard deviation of around 3 inches. This means that most men (about 68 percent, assuming a normal distribution) have a height within 3 inches of the mean (67–73 inches) – one standard deviation – and almost all men (about 95%) have a height within 6 inches of the mean (64–76 inches) – two standard deviations. If the standard deviation were zero, then all men would be exactly 70 inches tall. If the standard deviation were 20 inches, then men would have much more variable heights, with a typical range of about 50–90 inches. Three standard deviations account for 99.7 percent of the sample population being studied, assuming the distribution is normal (bellshaped).
Definition of population values
Let X be a random variable with mean value μ:
 \operatorname{E}[X] = \mu.\,\!
Here the operator E denotes the average or expected value of X. Then the standard deviation of X is the quantity
 \begin{align} \sigma & = \sqrt{\operatorname E[(X  \mu)^2]}\\ & =\sqrt{\operatorname E[X^2] + \operatorname E[(2 \mu X)] + \operatorname E[\mu^2]} =\sqrt{\operatorname E[X^2] 2 \mu \operatorname E[X] + \mu^2}\\ &=\sqrt{\operatorname E[X^2] 2 \mu^2 + \mu^2} =\sqrt{\operatorname E[X^2]  \mu^2}\\ & =\sqrt{\operatorname E[X^2](\operatorname E[X])^2} \end{align}
(derived using the properties of expected value).
In other words the standard deviation σ (sigma) is the square root of the variance of X; i.e., it is the square root of the average value of (X − μ)^{2}.
The standard deviation of a (univariate) probability distribution is the same as that of a random variable having that distribution. Not all random variables have a standard deviation, since these expected values need not exist. For example, the standard deviation of a random variable that follows a Cauchy distribution is undefined because its expected value μ is undefined.
Discrete random variable
In the case where X takes random values from a finite data set x_{1}, x_{2}, ..., x_{N}, with each value having the same probability, the standard deviation is
 \sigma = \sqrt{\frac{1}{N}\left[(x_1\mu)^2 + (x_2\mu)^2 + \cdots + (x_N  \mu)^2\right]}, {\rm \ \ where\ \ } \mu = \frac{1}{N} (x_1 + \cdots + x_N),
or, using summation notation,
 \sigma = \sqrt{\frac{1}{N} \sum_{i=1}^N (x_i  \mu)^2}, {\rm \ \ where\ \ } \mu = \frac{1}{N} \sum_{i=1}^N x_i.
If, instead of having equal probabilities, the values have different probabilities, let x_{1} have probability p_{1}, x_{2} have probability p_{2}, ..., x_{N} have probability p_{N}. In this case, the standard deviation will be
 \sigma = \sqrt{\sum_{i=1}^N p_i(x_i  \mu)^2} , {\rm \ \ where\ \ } \mu = \sum_{i=1}^N p_i x_i.
Continuous random variable
The standard deviation of a continuous realvalued random variable X with probability density function p(x) is
 \sigma = \sqrt{\int_\mathbf{X} (x\mu)^2 \, p(x) \, dx}, {\rm \ \ where\ \ } \mu = \int_\mathbf{X} x \, p(x) \, dx,
and where the integrals are definite integrals taken for x ranging over the set of possible values of the random variable X.
In the case of a parametric family of distributions, the standard deviation can be expressed in terms of the parameters. For example, in the case of the lognormal distribution with parameters μ and σ^{2}, the standard deviation is [(exp(σ^{2}) − 1)exp(2μ + σ^{2})]^{1/2}.
Estimation
One can find the standard deviation of an entire population in cases (such as standardized testing) where every member of a population is sampled. In cases where that cannot be done, the standard deviation σ is estimated by examining a random sample taken from the population and computing a statistic of the sample, which is used as an estimate of the population standard deviation. Such a statistic is called an estimator, and the estimator (or the value of the estimator, namely the estimate) is called a sample standard deviation, and is denoted by s (possibly with modifiers). However, unlike in the case of estimating the population mean, for which the sample mean is a simple estimator with many desirable properties (unbiased, efficient, maximum likelihood), there is no single estimator for the standard deviation with all these properties, and unbiased estimation of standard deviation is a very technically involved problem. Most often, the standard deviation is estimated using the corrected sample standard deviation (using N − 1), defined below, and this is often referred to as the "sample standard deviation", without qualifiers. However, other estimators are better in other respects: the uncorrected estimator (using N) yields lower mean squared error, while using N − 1.5 (for the normal distribution) almost completely eliminates bias.
Uncorrected sample standard deviation
Firstly, the formula for the population standard deviation (of a finite population) can be applied to the sample, using the size of the sample as the size of the population (though the actual population size from which the sample is drawn may be much larger). This estimator, denoted by s_{N}, is known as the uncorrected sample standard deviation, or sometimes the standard deviation of the sample (considered as the entire population), and is defined as follows:
 s_N = \sqrt{\frac{1}{N} \sum_{i=1}^N (x_i  \overline{x})^2},
where \scriptstyle\{x_1,\,x_2,\,\ldots,\,x_N\} are the observed values of the sample items and \scriptstyle\overline{x} is the mean value of these observations, while the denominator N stands for the size of the sample: this is the square root of the sample variance, which is the average of the squared deviations about the sample mean.
This is a consistent estimator (it converges in probability to the population value as the number of samples goes to infinity), and is the maximumlikelihood estimate when the population is normally distributed. However, this is a biased estimator, as the estimates are generally too low. The bias decreases as sample size grows, dropping off as 1/n, and thus is most significant for small or moderate sample sizes; for n > 75 the bias is below 1%. Thus for very large sample sizes, the uncorrected sample standard deviation is generally acceptable. This estimator also has a uniformly smaller mean squared error than the corrected sample standard deviation.
Corrected sample standard deviation
When discussing the bias, to be more precise, the corresponding estimator for the variance, the biased sample variance:
 s^2_N = \frac{1}{N} \sum_{i=1}^N (x_i  \overline{x})^2,
equivalently the second central moment of the sample (as the mean is the first moment), is a biased estimator of the variance (it underestimates the population variance). Taking the square root to pass to the standard deviation introduces further downward bias, by Jensen's inequality, due to the square root being a concave function. The bias in the variance is easily corrected, but the bias from the square root is more difficult to correct, and depends on the distribution in question.
An unbiased estimator for the variance is given by applying Bessel's correction, using N − 1 instead of N to yield the unbiased sample variance, denoted s^{2}:
 s^2 = \frac{1}{N1} \sum_{i=1}^N (x_i  \overline{x})^2.
This estimator is unbiased if the variance exists and the sample values are drawn independently with replacement. N − 1 corresponds to the number of degrees of freedom in the vector of residuals, \scriptstyle(x_1\overline{x},\; \dots,\; x_n\overline{x}).
Taking square roots reintroduces bias, and yields the corrected sample standard deviation, denoted by s:
 s = \sqrt{\frac{1}{N1} \sum_{i=1}^N (x_i  \overline{x})^2}.
While s^{2} is an unbiased estimator for the population variance, s is a biased estimator for the population standard deviation, though markedly less biased than the uncorrected sample standard deviation. The bias is still significant for small samples (n less than 10), and also drops off as 1/n as sample size increases. This estimator is commonly used, and generally known simply as the "sample standard deviation".
Unbiased sample standard deviation
For unbiased estimation of standard deviation, there is no formula that works across all distributions, unlike for mean and variance. Instead, s is used as a basis, and is scaled by a correction factor to produce an unbiased estimate. For the normal distribution, an unbiased estimator is given by s/c_{4}, where the correction factor (which depends on N) is given in terms of the Gamma function, and equals:
 c_4(N)\,=\,\sqrt{\frac{2}{N1}}\,\,\,\frac{\Gamma\left(\frac{N}{2}\right)}{\Gamma\left(\frac{N1}{2}\right)}.
This arises because the sampling distribution of the sample standard deviation follows a (scaled) chi distribution, and the correction factor is the mean of the chi distribution.
An approximation can be given by replacing N − 1 with N − 1.5, yielding:
 \hat\sigma = \sqrt{ \frac{1}{N  1.5} \sum_{i=1}^n (x_i  \bar{x})^2 },
The error in this approximation decays quadratically (as 1/N^{2}), and it is suited for all but the smallest samples or highest precision: for n = 3 the bias is equal to 1.3%, and for n = 9 the bias is already less than 0.1%.
For other distributions, the correct formula depends on the distribution, but a rule of thumb is to use the further refinement of the approximation:
 \hat\sigma = \sqrt{ \frac{1}{n  1.5  \tfrac14 \gamma_2} \sum_{i=1}^n (x_i  \bar{x})^2 },
where γ_{2} denotes the population excess kurtosis. The excess kurtosis may be either known beforehand for certain distributions, or estimated from the data.
Confidence interval of a sampled standard deviation
The standard deviation we obtain by sampling a distribution is itself not absolutely accurate, both for mathematical reasons (explained here by the confidence interval) and for practical reasons of measurement (measurement error). The mathematical effect can be described by the confidence interval or CI. To show how a larger sample will increase the confidence interval, consider the following examples: For a small population of N=2, the 95% CI of the SD is from 0.45*SD to 31.9*SD. In other words, the standard deviation of the distribution in 95% of the cases can be larger by a factor of 31 or smaller by a factor of 2. For a larger population of N=10, the CI is 0.69*SD to 1.83*SD. So even with a sample population of 10, the actual SD can still be almost a factor 2 higher than the sampled SD. For a sample population N=100, this is down to 0.88*SD to 1.16*SD. To be more certain that the sampled SD is close to the actual SD we need to sample a large number of points.
Identities and mathematical properties
The standard deviation is invariant under changes in location, and scales directly with the scale of the random variable. Thus, for a constant c and random variables X and Y:
 \sigma(c) = 0 \,
 \sigma(X + c) = \sigma(X), \,
 \sigma(cX) = c \sigma(X). \,
The standard deviation of the sum of two random variables can be related to their individual standard deviations and the covariance between them:
 \sigma(X + Y) = \sqrt{\operatorname{var}(X) + \operatorname{var}(Y) + 2 \,\operatorname{cov}(X,Y)}. \,
where \scriptstyle\operatorname{var} \,=\, \sigma^2 and \scriptstyle\operatorname{cov} stand for variance and covariance, respectively.
The calculation of the sum of squared deviations can be related to moments calculated directly from the data. The standard deviation of the population can be computed as:
 \sigma(X) = \sqrt{E[(XE(X))^2]} = \sqrt{E[X^2]  (E[X])^2}.
The sample standard deviation can be computed as:
 \sigma(X) = \sqrt{\frac{N}{N1}} \sqrt{E[(XE(X))^2]}.
For a finite population with equal probabilities at all points, we have
 \sqrt{\frac{1}{N}\sum_{i=1}^N(x_i\overline{x})^2} = \sqrt{\frac{1}{N} \left(\sum_{i=1}^N x_i^2\right)  \overline{x}^2} = \sqrt{\left(\frac{1}{N} \sum_{i=1}^N x_i^2\right)  \left(\frac{1}{N} \sum_{i=1}^{N} x_i\right)^2}.
This means that the standard deviation is equal to the square root of (the average of the squares less the square of the average). See computational formula for the variance for proof, and for an analogous result for the sample standard deviation.
Interpretation and application
A large standard deviation indicates that the data points can spread far from the mean and a small standard deviation indicates that they are clustered closely around the mean.
For example, each of the three populations {0, 0, 14, 14}, {0, 6, 8, 14} and {6, 6, 8, 8} has a mean of 7. Their standard deviations are 7, 5, and 1, respectively. The third population has a much smaller standard deviation than the other two because its values are all close to 7. It will have the same units as the data points themselves. If, for instance, the data set {0, 6, 8, 14} represents the ages of a population of four siblings in years, the standard deviation is 5 years. As another example, the population {1000, 1006, 1008, 1014} may represent the distances traveled by four athletes, measured in meters. It has a mean of 1007 meters, and a standard deviation of 5 meters.
Standard deviation may serve as a measure of uncertainty. In physical science, for example, the reported standard deviation of a group of repeated measurements gives the precision of those measurements. When deciding whether measurements agree with a theoretical prediction, the standard deviation of those measurements is of crucial importance: if the mean of the measurements is too far away from the prediction (with the distance measured in standard deviations), then the theory being tested probably needs to be revised. This makes sense since they fall outside the range of values that could reasonably be expected to occur, if the prediction were correct and the standard deviation appropriately quantified. See prediction interval.
While the standard deviation does measure how far typical values tend to be from the mean, other measures are available. An example is the mean absolute deviation, which might be considered a more direct measure of average distance, compared to the root mean square distance inherent in the standard deviation.
Application examples
The practical value of understanding the standard deviation of a set of values is in appreciating how much variation there is from the average (mean).
Weather
As a simple example, consider the average daily maximum temperatures for two cities, one inland and one on the coast. It is helpful to understand that the range of daily maximum temperatures for cities near the coast is smaller than for cities inland. Thus, while these two cities may each have the same average maximum temperature, the standard deviation of the daily maximum temperature for the coastal city will be less than that of the inland city as, on any particular day, the actual maximum temperature is more likely to be farther from the average maximum temperature for the inland city than for the coastal one.
Particle physics
Particle physics uses a standard of "5 sigma" for the declaration of a discovery.^{[4]} At fivesigma there is only one chance in nearly two million that a random fluctuation would yield the result. This level of certainty prompted the announcement that a particle consistent with the Higgs boson has been discovered in two independent experiments at CERN.^{[5]}
Finance
In finance, standard deviation is often used as a measure of the risk associated with pricefluctuations of a given asset (stocks, bonds, property, etc.), or the risk of a portfolio of assets^{[6]} (actively managed mutual funds, index mutual funds, or ETFs). Risk is an important factor in determining how to efficiently manage a portfolio of investments because it determines the variation in returns on the asset and/or portfolio and gives investors a mathematical basis for investment decisions (known as meanvariance optimization). The fundamental concept of risk is that as it increases, the expected return on an investment should increase as well, an increase known as the risk premium. In other words, investors should expect a higher return on an investment when that investment carries a higher level of risk or uncertainty. When evaluating investments, investors should estimate both the expected return and the uncertainty of future returns. Standard deviation provides a quantified estimate of the uncertainty of future returns.
For example, let's assume an investor had to choose between two stocks. Stock A over the past 20 years had an average return of 10 percent, with a standard deviation of 20 percentage points (pp) and Stock B, over the same period, had average returns of 12 percent but a higher standard deviation of 30 pp. On the basis of risk and return, an investor may decide that Stock A is the safer choice, because Stock B's additional two percentage points of return is not worth the additional 10 pp standard deviation (greater risk or uncertainty of the expected return). Stock B is likely to fall short of the initial investment (but also to exceed the initial investment) more often than Stock A under the same circumstances, and is estimated to return only two percent more on average. In this example, Stock A is expected to earn about 10 percent, plus or minus 20 pp (a range of 30 percent to −10 percent), about twothirds of the future year returns. When considering more extreme possible returns or outcomes in future, an investor should expect results of as much as 10 percent plus or minus 60 pp, or a range from 70 percent to −50 percent, which includes outcomes for three standard deviations from the average return (about 99.7 percent of probable returns).
Calculating the average (or arithmetic mean) of the return of a security over a given period will generate the expected return of the asset. For each period, subtracting the expected return from the actual return results in the difference from the mean. Squaring the difference in each period and taking the average gives the overall variance of the return of the asset. The larger the variance, the greater risk the security carries. Finding the square root of this variance will give the standard deviation of the investment tool in question.
Population standard deviation is used to set the width of Bollinger Bands, a widely adopted technical analysis tool. For example, the upper Bollinger Band is given as x + nσ_{x}. The most commonly used value for n is 2; there is about a five percent chance of going outside, assuming a normal distribution of returns.
Financial time series are known to be nonstationary series, whereas the statistical calculations above, such as standard deviation, apply only to stationary series. To apply the above statistical tools to nonstationary series, the series first must be transformed to a stationary series, enabling use of statistical tools that now have a valid basis from which to work.
Geometric interpretation
To gain some geometric insights and clarification, we will start with a population of three values, x_{1}, x_{2}, x_{3}. This defines a point P = (x_{1}, x_{2}, x_{3}) in R^{3}. Consider the line L = {(r, r, r) : r ∈ R}. This is the "main diagonal" going through the origin. If our three given values were all equal, then the standard deviation would be zero and P would lie on L. So it is not unreasonable to assume that the standard deviation is related to the distance of P to L. And that is indeed the case. To move orthogonally from L to the point P, one begins at the point:
 M = (\overline{x},\overline{x},\overline{x})
whose coordinates are the mean of the values we started out with. A little algebra shows that the distance between P and M (which is the same as the orthogonal distance between P and the line L) is equal to the standard deviation of the vector x_{1}, x_{2}, x_{3}, multiplied by the square root of the number of dimensions of the vector (3 in this case.)
Chebyshev's inequality
An observation is rarely more than a few standard deviations away from the mean. Chebyshev's inequality ensures that, for all distributions for which the standard deviation is defined, the amount of data within a number of standard deviations of the mean is at least as much as given in the following table.
Minimum population  Number of standard deviations from mean 

50%  √2 
75%  2 
89%  3 
94%  4 
96%  5 
97%  6 
\scriptstyle 1\frac{1}{k^2}^{[7]}  \scriptstyle k 
\scriptstyle l  \scriptstyle \frac{1}{\sqrt{1l}} 
Rules for normally distributed data
The central limit theorem says that the distribution of an average of many independent, identically distributed random variables tends toward the famous bellshaped normal distribution with a probability density function of:
 f(x;\mu,\sigma^2) = \frac{1}{\sigma\sqrt{2\pi}} e^{ \frac{1}{2}\left(\frac{x\mu}{\sigma}\right)^2 }
where μ is the expected value of the random variables, σ equals their distribution's standard deviation divided by n^{1/2}, and n is the number of random variables. The standard deviation therefore is simply a scaling variable that adjusts how broad the curve will be, though it also appears in the normalizing constant.
If a data distribution is approximately normal, then the proportion of data values within z standard deviations of the mean is defined by:
 Proportion = \operatorname{erf}\left(\frac{z}{\sqrt{2}}\right)
where \scriptstyle\operatorname{erf} is the error function. The proportion that is less than or equal to a number, x, is given by the cumulative distribution function:
 Proportion ≤ x = \frac12\left[1 + \operatorname{erf}\left( \frac{x\mu}{\sigma\sqrt{2}}\right)\right] = \frac12\left[1 + \operatorname{erf}\left( \frac{z}{\sqrt{2}}\right)\right].^{[8]}
If a data distribution is approximately normal then about 68 percent of the data values are within one standard deviation of the mean (mathematically, μ ± σ, where μ is the arithmetic mean), about 95 percent are within two standard deviations (μ ± 2σ), and about 99.7 percent lie within three standard deviations (μ ± 3σ). This is known as the 689599.7 rule, or the empirical rule.
For various values of z, the percentage of values expected to lie in and outside the symmetric interval, CI = (−zσ, zσ), are as follows:
zσ  Percentage within CI  Percentage outside CI  Fraction outside CI 

0.674490σ  50%  50%  1 / 2 
0.994458σ  68%  32%  1 / 3.125 
1σ  68.2689492%  31.7310508%  1 / 3.1514872 
1.281552σ  80%  20%  1 / 5 
1.644854σ  90%  10%  1 / 10 
1.959964σ  95%  5%  1 / 20 
2σ  95.4499736%  4.5500264%  1 / 21.977895 
2.575829σ  99%  1%  1 / 100 
3σ  99.7300204%  0.2699796%  1 / 370.398 
3.290527σ  99.9%  0.1%  1 / 1000 
3.890592σ  99.99%  0.01%  1 / 10000 
4σ  99.993666%  0.006334%  1 / 15787 
4.417173σ  99.999%  0.001%  1 / 100000 
4.5σ  99.9993204653751%  0.0006795346249%  3.4 / 1000000 (on each side of mean) 
4.891638σ  99.9999%  0.0001%  1 / 1000000 
5σ  99.9999426697%  0.0000573303%  1 / 1744278 
5.326724σ  99.99999%  0.00001%  1 / 10000000 
5.730729σ  99.999999%  0.000001%  1 / 100000000 
6σ  99.9999998027%  0.0000001973%  1 / 506797346. 
6.109410σ  99.9999999%  0.0000001%  1 / 1000000000. 
6.466951σ  99.99999999%  0.00000001%  1 / 2147483647. 
6.806502σ  99.999999999%  0.000000001%  1 / 2147483647. 
7σ  99.9999999997440%  0.000000000256%  1 / 2147483647. 
Relationship between standard deviation and mean
The mean and the standard deviation of a set of data are descriptive statistics usually reported together. In a certain sense, the standard deviation is a "natural" measure of statistical dispersion if the center of the data is measured about the mean. This is because the standard deviation from the mean is smaller than from any other point. The precise statement is the following: suppose x_{1}, ..., x_{n} are real numbers and define the function:
 \sigma(r) = \sqrt{\frac{1}{N1} \sum_{i=1}^N (x_i  r)^2}.
Using calculus or by completing the square, it is possible to show that σ(r) has a unique minimum at the mean:
 r = \overline{x}.\,
Variability can also be measured by the coefficient of variation, which is the ratio of the standard deviation to the mean. It is a dimensionless number.
Standard deviation of the mean
Often, we want some information about the precision of the mean we obtained. We can obtain this by determining the standard deviation of the sampled mean. Assuming statistical independence of the values in the sample, the standard deviation of the mean is related to the standard deviation of the distribution by:
 \sigma_{\text{mean}} = \frac{1}{\sqrt{N}}\sigma
where N is the number of observations in the sample used to estimate the mean. This can easily be proven with (see basic properties of the variance):
 \begin{align} \operatorname{var}(X) &\equiv \sigma^2_X\\ \operatorname{var}(X_1+X_2) &\equiv \operatorname{var}(X_1) + \operatorname{var}(X_2)\\ \operatorname{var}(cX_1) &\equiv c^2 \, \operatorname{var}(X_1) \end{align}
hence
 \begin{align} \operatorname{var}(\text{mean}) &= \operatorname{var}\left (\frac{1}{N} \sum_{i=1}^N X_i \right) = \frac{1}{N^2}\operatorname{var}\left (\sum_{i=1}^N X_i \right ) \\ &= \frac{1}{N^2}\sum_{i=1}^N \operatorname{var}(X_i) = \frac{N}{N^2} \operatorname{var}(X) = \frac{1}{N} \operatorname{var} (X). \end{align}
Resulting in:
 \sigma_\text{mean} = \frac{\sigma}{\sqrt{N}}.
It should be emphasized that in order to estimate standard deviation of the mean \sigma_\text{mean} it is necessary to know standard deviation of the entire population \sigma beforehand. However, in most applications this parameter is unknown. For example, if series of 10 measurements of previously unknown quantity is performed in laboratory, it is possible to calculate resulting sample mean and sample standard deviation, but it is impossible to calculate standard deviation of the mean.
Rapid calculation methods
The following two formulas can represent a running (repeatedly updated) standard deviation. A set of two power sums s_{1} and s_{2} are computed over a set of N values of x, denoted as x_{1}, ..., x_{N}:
 \ s_j=\sum_{k=1}^N{x_k^j}.
Given the results of these running summations, the values N, s_{1}, s_{2} can be used at any time to compute the current value of the running standard deviation:
 \sigma = \frac{\sqrt{Ns_2s_1^2} }{N}
Where :\ N=s_0=\sum_{k=1}^N{x_k^0}.
Similarly for sample standard deviation,
 s = \sqrt{\frac{Ns_2s_1^2}{N(N1)}}.
In a computer implementation, as the three s_{j} sums become large, we need to consider roundoff error, arithmetic overflow, and arithmetic underflow. The method below calculates the running sums method with reduced rounding errors.^{[9]} This is a "one pass" algorithm for calculating variance of n samples without the need to store prior data during the calculation. Applying this method to a time series will result in successive values of standard deviation corresponding to n data points as n grows larger with each new sample, rather than a constantwidth sliding window calculation.
For k = 1, ..., n:
 \begin{align} A_0 &= 0\\ A_k &= A_{k1}+\frac{x_kA_{k1}}{k} \end{align}
where A is the mean value.
 \begin{align} Q_0 &= 0\\ Q_k &= Q_{k1}+\frac{k1}{k} (x_kA_{k1})^2 = Q_{k1}+ (x_kA_{k1})(x_kA_k)\\ \end{align}
Note: Q_1 = 0 since k1 = 0 or x_1 = A_1
Sample variance:
 s^2_n=\frac{Q_n}{n1}
Population variance:
 \sigma^2_n=\frac{Q_n}{n}
Weighted calculation
When the values x_{i} are weighted with unequal weights w_{i}, the power sums s_{0}, s_{1}, s_{2} are each computed as:
 \ s_j=\sum_{k=1}^N{w_k x_k^j}.\,
And the standard deviation equations remain unchanged. Note that s_{0} is now the sum of the weights and not the number of samples N.
The incremental method with reduced rounding errors can also be applied, with some additional complexity.
A running sum of weights must be computed for each k from 1 to n:
 \begin{align} W_0 &= 0\\ W_k &= W_{k1} + w_k \end{align}
and places where 1/n is used above must be replaced by w_{i}/W_{n}:
 \begin{align} A_0 &= 0\\ A_k &= A_{k1}+\frac{w_k}{W_k}(x_kA_{k1})\\ Q_0 &= 0\\ Q_k &= Q _{k1} + \frac{w_k W_{k1}}{W_k}(x_kA_{k1})^2 = Q_{k1}+w_k(x_kA_{k1})(x_kA_k) \end{align}
In the final division,
 \sigma^2_n=\frac{Q_n}{W_n}\,
and
 s^2_n = \frac{n'}{n'1}\sigma^2_n\,
where n is the total number of elements, and n' is the number of elements with nonzero weights. The above formulas become equal to the simpler formulas given above if weights are taken as equal to one.
Combining standard deviations
Populationbased statistics
The populations of sets, which may overlap, can be calculated simply as follows:
 \begin{align} &&N_{X \cup Y} &= N_X + N_Y  N_{X \cap Y}\\ X \cap Y = \varnothing &\Rightarrow &N_{X \cap Y} &= 0\\ &\Rightarrow &N_{X \cup Y} &= N_X + N_Y \end{align}
Standard deviations of nonoverlapping (X ∩ Y = ∅) subpopulations can be aggregated as follows if the size (actual or relative to one another) and means of each are known:
 \begin{align} \mu_{X \cup Y} &= \frac{ N_X \mu_X + N_Y \mu_Y }{N_X + N_Y} \\ \sigma_{X\cup Y} &= \sqrt{ \frac{N_X \sigma_X^2 + N_Y \sigma_Y^2}{N_X + N_Y} + \frac{N_X N_Y}{(N_X+N_Y)^2}(\mu_X  \mu_Y)^2 } \end{align}
For example, suppose it is known that the average American man has a mean height of 70 inches with a standard deviation of three inches and that the average American woman has a mean height of 65 inches with a standard deviation of two inches. Also assume that the number of men, N, is equal to the number of women. Then the mean and standard deviation of heights of American adults could be calculated as:
 \begin{align} \mu &= \frac{N\cdot70 + N\cdot65}{N + N} = \frac{70+65}{2} = 67.5 \\ \sigma &= \sqrt{ \frac{3^2 + 2^2}{2} + \frac{(7065)^2}{2^2} } = \sqrt{12.75} \approx 3.57 \end{align}
For the more general case of M nonoverlapping populations, X_{1} through X_{M}, and the aggregate population \scriptstyle X \,=\, \bigcup_i X_i:

\begin{align} \mu_X &= \frac{ \sum_i N_{X_i}\mu_{X_i} }{ \sum_i N_{X_i} } \\ \sigma_X &= \sqrt{ \frac{ \sum_i N_{X_i}(\sigma_{X_i}^2 + \mu_{X_i}^2) }{ \sum_i N_{X_i} }  \mu_X^2 } = \sqrt{ \frac{ \sum_i N_{X_i}\sigma_{X_i}^2 }{ \sum_i N_{X_i} } + \frac{ \sum_{i
where

X_i \cap X_j = \varnothing, \quad \forall\ i
If the size (actual or relative to one another), mean, and standard deviation of two overlapping populations are known for the populations as well as their intersection, then the standard deviation of the overall population can still be calculated as follows:
 \begin{align} \mu_{X \cup Y} &= \frac{1}{N_{X \cup Y}}\left(N_X\mu_X + N_Y\mu_Y  N_{X \cap Y}\mu_{X \cap Y}\right)\\ \sigma_{X \cup Y} &= \sqrt{\frac{1}{N_{X \cup Y}}\left(N_X[\sigma_X^2 + \mu _X^2] + N_Y[\sigma_Y^2 + \mu _Y^2]  N_{X \cap Y}[\sigma_{X \cap Y}^2 + \mu _{X \cap Y}^2]\right)  \mu_{X\cup Y}^2} \end{align}
If two or more sets of data are being added together datapoint by datapoint, the standard deviation of the result can be calculated if the standard deviation of each data set and the covariance between each pair of data sets is known:
 \sigma_X = \sqrt{\sum_i{\sigma_{X_i}^2} + \sum_{i,j}\operatorname{cov}(X_i,X_j)}
For the special case where no correlation exists between any pair of data sets, then the relation reduces to the rootmeansquare:

\begin{align} &\operatorname{cov}(X_i, X_j) = 0,\quad \forall i
Samplebased statistics
Standard deviations of nonoverlapping (X ∩ Y = ∅) subsamples can be aggregated as follows if the actual size and means of each are known:
 \begin{align} \mu_{X \cup Y} &= \frac{1}{N_{X \cup Y}}\left(N_X\mu_X + N_Y\mu_Y\right)\\ \sigma_{X \cup Y} &= \sqrt{\frac{1}{N_{X \cup Y}  1}\left([N_X  1]\sigma_X^2 + N_X\mu_X^2 + [N_Y  1]\sigma_Y^2 + N_Y\mu _Y^2  [N_X + N_Y]\mu_{X \cup Y}^2\right) } \end{align}
For the more general case of M nonoverlapping data sets, X_{1} through X_{M}, and the aggregate data set \scriptstyle X \,=\, \bigcup_i X_i:
 \begin{align} \mu_X &= \frac{1}{\sum_i { N_{X_i}}} \left(\sum_i { N_{X_i} \mu_{X_i}}\right)\\ \sigma_X &= \sqrt{\frac{1}{\sum_i {N_{X_i}  1}} \left( \sum_i { \left[(N_{X_i}  1) \sigma_{X_i}^2 + N_{X_i} \mu_{X_i}^2\right] }  \left[\sum_i {N_{X_i}}\right]\mu_X^2 \right) } \end{align}
where:

X_i \cap X_j = \varnothing,\quad \forall i
If the size, mean, and standard deviation of two overlapping samples are known for the samples as well as their intersection, then the standard deviation of the aggregated sample can still be calculated. In general:
 \begin{align} \mu_{X \cup Y} &= \frac{1}{N_{X \cup Y}}\left(N_X\mu_X + N_Y\mu_Y  N_{X\cap Y}\mu_{X\cap Y}\right)\\ \sigma_{X \cup Y} &= \sqrt{ \frac\mu_{X \cup Y}^2}{N_{X \cup Y}  1} } \end{align}
History
The term standard deviation was first used^{[10]} in writing by Karl Pearson^{[11]} in 1894, following his use of it in lectures. This was as a replacement for earlier alternative names for the same idea: for example, Gauss used mean error.^{[12]} It may be worth noting in passing that the mean error is mathematically distinct from the standard deviation.
See also
 68–95–99.7 rule
 Accuracy and precision
 Chebyshev's inequality An inequality on location and scale parameters
 Cumulant
 Deviation (statistics)
 Distance correlation Distance standard deviation
 Error bar
 Geometric standard deviation
 Mahalanobis distance generalizing number of standard deviations to the mean
 Mean absolute error
 Percentile
 Pooled variance pooled standard deviation
 Raw score
 Robust standard deviation
 Root mean square
 Sample size
 Samuelson's inequality
 Six Sigma
 Standard error
 Volatility (finance)
 Yamartino method for calculating standard deviation of wind direction
References
 ^ Bland, J.M.; Altman, D.G. (1996). "Statistics notes: measurement error.". Bmj, 312(7047), 1654. Retrieved 22 November 2013.
 ^
 ^ Walker, Helen (1931). Studies in the History of the Statistical Method. Baltimore, MD: Williams & Wilkins Co. pp. 24–25.
 ^ "CERN  Accelerating science". Public.web.cern.ch. Retrieved 20130810.
 ^ "CERN experiments observe particle consistent with longsought Higgs boson  CERN press office". Press.web.cern.ch. 20120704. Retrieved 20130810.
 ^ "What is Standard Deviation". Pristine. Retrieved 20111029.
 ^ Ghahramani, Saeed (2000). Fundamentals of Probability (2nd Edition). Prentice Hall: New Jersey. p. 438.
 ^ Eric W. Weisstein. "Distribution Function". MathWorldA Wolfram Web Resource. Retrieved 20140930.
 ^ Welford, BP (August 1962). "Note on a Method for Calculating Corrected Sums of Squares and Products". Technometrics 4 (3): 419–420.
 ^ Dodge, Yadolah (2003). The Oxford Dictionary of Statistical Terms. Oxford University Press.
 ^
 ^ Miller, Jeff. "Earliest Known Uses of Some of the Words of Mathematics".
External links
 Hazewinkel, Michiel, ed. (2001), "Quadratic deviation",
 A simple way to understand Standard Deviation
 Standard Deviation – an explanation without maths
 Standard Deviation, an elementary introduction
 Standard Deviation while Financial Modeling in Excel
 Standard Deviation, a simpler explanation for writers and journalists
 The concept of Standard Deviation is shown in this 8foottall (2.4 m) Probability Machine (named Sir Francis) comparing stock market returns to the randomness of the beans dropping through the quincunx pattern. on YouTube from Index Funds Advisors IFA.com


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