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In probability theory and statistics, covariance is a measure of the joint variability of two random variables.^[1] If the greater values of one variable mainly correspond with the greater values of the other variable, and the same holds for the lesser values, (i.e., the variables tend to show similar behavior), the covariance is positive.^[2] In the opposite case, when the greater values of one variable mainly correspond to the lesser values of the other, (i.e., the variables tend to show opposite behavior), the covariance is negative. The sign of the covariance therefore shows the tendency in the linear relationship between the variables. The magnitude of the covariance is not easy to interpret because it is not normalized and hence depends on the magnitudes of the variables. The normalized version of the covariance, the correlation coefficient, however, shows by its magnitude the strength of the linear relation.

A distinction must be made between (1) the covariance of two random variables, which is a population parameter that can be seen as a property of the joint probability distribution, and (2) the sample covariance, which in addition to serving as a descriptor of the sample, also serves as an estimated value of the population parameter.

Definition

The covariance between two jointly distributed real-valued random variables X and Y with finite second moments is defined as the expected product of their deviations from their individual expected values:^[3]

cov⁡(X,Y)=E⁡[(X−E⁡[X])(Y−E⁡[Y])],{displaystyle operatorname {cov} (X,Y)=operatorname {E} {{big [}(X-operatorname {E} [X])(Y-operatorname {E} [Y]){big ]}},}

where E[X] is the expected value of X, also known as the mean of X. The covariance is also sometimes denoted σ_XY or σ(X,Y), in analogy to variance. By using the linearity property of expectations, this can be simplified to the expected value of their product minus the product of their expected values:

cov⁡(X,Y)=E⁡[(X−E⁡[X])(Y−E⁡[Y])]=E⁡[XY−XE⁡[Y]−E⁡[X]Y+E⁡[X]E⁡[Y]]=E⁡[XY]−E⁡[X]E⁡[Y]−E⁡[X]E⁡[Y]+E⁡[X]E⁡[Y]=E⁡[XY]−E⁡[X]E⁡[Y].{displaystyle {begin{aligned}operatorname {cov} (X,Y)&=operatorname {E} left[left(X-operatorname {E} left[Xright]right)left(Y-operatorname {E} left[Yright]right)right]\&=operatorname {E} left[XY-Xoperatorname {E} left[Yright]-operatorname {E} left[Xright]Y+operatorname {E} left[Xright]operatorname {E} left[Yright]right]\&=operatorname {E} left[XYright]-operatorname {E} left[Xright]operatorname {E} left[Yright]-operatorname {E} left[Xright]operatorname {E} left[Yright]+operatorname {E} left[Xright]operatorname {E} left[Yright]\&=operatorname {E} left[XYright]-operatorname {E} left[Xright]operatorname {E} left[Yright].end{aligned}}}

However, when E⁡[XY]≈E⁡[X]E⁡[Y]{displaystyle operatorname {E} [XY]approx operatorname {E} [X]operatorname {E} [Y]}, this last equation is prone to catastrophic cancellation when computed with floating point arithmetic and thus should be avoided in computer programs when the data has not been centered before.^[4]Numerically stable algorithms should be preferred in this case.

For random vectors X∈Rm{displaystyle mathbf {X} in mathbb {R} ^{m}} and Y∈Rn{displaystyle mathbf {Y} in mathbb {R} ^{n}}, the m × n cross covariance matrix is equal to

cov⁡(X,Y)=E⁡[(X−E⁡[X])(Y−E⁡[Y])T]=E⁡[XYT]−E⁡[X]E⁡[Y]T,{displaystyle {begin{aligned}operatorname {cov} (mathbf {X} ,mathbf {Y} )&=operatorname {E} left[(mathbf {X} -operatorname {E} [mathbf {X} ])(mathbf {Y} -operatorname {E} [mathbf {Y} ])^{mathrm {T} }right]\&=operatorname {E} left[mathbf {X} mathbf {Y} ^{mathrm {T} }right]-operatorname {E} [mathbf {X} ]operatorname {E} [mathbf {Y} ]^{mathrm {T} },end{aligned}}}

where m^T is the transpose of the vector (or matrix) m.

The (i, j)-th element of this matrix is equal to the covariance cov(X_i, Y_j) between the i-th scalar component of X and the j-th scalar component of Y. In particular, cov(Y, X) is the transpose of cov(X, Y).

For a vector X=[X1X2…Xm]T{displaystyle mathbf {X} ={begin{bmatrix}X_{1}&X_{2}&dots &X_{m}end{bmatrix}}^{mathrm {T} }} of m jointly distributed random variables with finite second moments, its covariance matrix (also known as the variance–covariance matrix) is defined as

Σ(X)=cov⁡(X,X).{displaystyle Sigma (mathbf {X} )=operatorname {cov} (mathbf {X} ,mathbf {X} ).}

Random variables whose covariance is zero are called uncorrelated. Similarly, the components of random vectors whose covariance matrix is zero in every entry outside the main diagonal are also called uncorrelated.

The units of measurement of the covariance cov(X, Y) are those of X times those of Y. By contrast, correlation coefficients, which depend on the covariance, are a dimensionless measure of linear dependence. (In fact, correlation coefficients can simply be understood as a normalized version of covariance.)

Discrete variables

If the random variable pair (X, Y) can take on the values (x_i, y_i) for i = 1, ... , n, with equal probabilities 1/n, then the covariance can be equivalently written in terms of the means E(X){displaystyle E(X)} and E(Y){displaystyle E(Y)} as

cov⁡(X,Y)=1n∑i=1n(xi−E(X))(yi−E(Y)).{displaystyle operatorname {cov} (X,Y)={frac {1}{n}}sum _{i=1}^{n}(x_{i}-E(X))(y_{i}-E(Y)).}

It can also be equivalently expressed, without directly referring to the means, as^[5]

cov⁡(X,Y)=1n2∑i=1n∑j=1n12(xi−xj)⋅(yi−yj)=1n2∑i∑j>i(xi−xj)⋅(yi−yj).{displaystyle operatorname {cov} (X,Y)={frac {1}{n^{2}}}sum _{i=1}^{n}sum _{j=1}^{n}{frac {1}{2}}(x_{i}-x_{j})cdot (y_{i}-y_{j})={frac {1}{n^{2}}}sum _{i}sum _{j>i}(x_{i}-x_{j})cdot (y_{i}-y_{j}).}

More generally, if there are n possible realizations of (X, Y), namely (x_i, y_i) for i = 1, ... , n, but with possibly unequal probabilities p_i , then the covariance is

cov⁡(X,Y)=∑i=1npi⋅(xi−E(X))⋅(yi−E(Y)).{displaystyle operatorname {cov} (X,Y)=sum _{i=1}^{n}p_{i}cdot (x_{i}-E(X))cdot (y_{i}-E(Y)).}

Discrete random variable example

Suppose that X and Y have the following joint probability mass function,^[6] in which the six central cells give the probabilities f(x, y) of the six hypothetical realizations (x, y) = (1, 1), (1, 2), (1, 3), (2, 1), (2,2), and (2, 3):

X can take on two values (1 and 2) while Y can take on three (1, 2, and 3). Their means are μX=3/2{displaystyle mu _{X}=3/2} and μY=2.{displaystyle mu _{Y}=2.} The population standard deviations of X and Y are σX=1/2{displaystyle sigma _{X}=1/2} and σY=1/2.{displaystyle sigma _{Y}={sqrt {1/2}}.} Then:

cov⁡(X,Y)=σXY=∑(x,y)∈Sf(x,y)(x−μX)(y−μY)=(14)(1−32)(1−2)+(14)(1−32)(2−2)+(0)(1−32)(3−2)+(0)(2−32)(1−2)+(14)(2−32)(2−2)+(14)(2−32)(3−2)=14.{displaystyle {begin{aligned}&operatorname {cov} (X,Y)=sigma _{XY}=sum _{(x,y)in S}f(x,y)(x-mu _{X})(y-mu _{Y})\={}&left({frac {1}{4}}right)left(1-{frac {3}{2}}right)(1-2)+left({frac {1}{4}}right)left(1-{frac {3}{2}}right)(2-2)\&{}+(0)left(1-{frac {3}{2}}right)(3-2)+(0)left(2-{frac {3}{2}}right)(1-2)\&{}+left({frac {1}{4}}right)left(2-{frac {3}{2}}right)(2-2)+left({frac {1}{4}}right)left(2-{frac {3}{2}}right)(3-2)\={}&{frac {1}{4}}.end{aligned}}}

Properties

• The variance is a special case of the covariance in which the two variables are identical (that is, in which one variable always takes the same value as the other):

cov⁡(X,X)=var⁡(X)≡σ2(X)≡σX2.{displaystyle operatorname {cov} (X,X)=operatorname {var} (X)equiv sigma ^{2}(X)equiv sigma _{X}^{2}.}

• If X, Y, W, and V are real-valued random variables and a, b, c, d are constant ("constant" in this context means non-random), then the following facts are a consequence of the definition of covariance:

cov⁡(X,a)=0cov⁡(X,X)=var⁡(X)cov⁡(X,Y)=cov⁡(Y,X)cov⁡(aX,bY)=abcov⁡(X,Y)cov⁡(X+a,Y+b)=cov⁡(X,Y)cov⁡(aX+bY,cW+dV)=accov⁡(X,W)+adcov⁡(X,V)+bccov⁡(Y,W)+bdcov⁡(Y,V){displaystyle {begin{aligned}operatorname {cov} (X,a)&=0\operatorname {cov} (X,X)&=operatorname {var} (X)\operatorname {cov} (X,Y)&=operatorname {cov} (Y,X)\operatorname {cov} (aX,bY)&=ab,operatorname {cov} (X,Y)\operatorname {cov} (X+a,Y+b)&=operatorname {cov} (X,Y)\operatorname {cov} (aX+bY,cW+dV)&=ac,operatorname {cov} (X,W)+ad,operatorname {cov} (X,V)+bc,operatorname {cov} (Y,W)+bd,operatorname {cov} (Y,V)end{aligned}}}

For a sequence X₁, ..., X_n of random variables, and constants a₁, ..., a_n, we have

σ2(∑i=1naiXi)=∑i=1nai2σ2(Xi)+2∑i,j:i<jaiajcov⁡(Xi,Xj)=∑i,jaiajcov⁡(Xi,Xj){displaystyle sigma ^{2}left(sum _{i=1}^{n}a_{i}X_{i}right)=sum _{i=1}^{n}a_{i}^{2}sigma ^{2}(X_{i})+2sum _{i,j,:,i<j}a_{i}a_{j}operatorname {cov} (X_{i},X_{j})=sum _{i,j}{a_{i}a_{j}operatorname {cov} (X_{i},X_{j})}}

• A useful identity to compute the covariance between two random variables X,Y{displaystyle X,Y} is the Hoeffding's Covariance Identity:^[7]
  

cov⁡(X,Y)=∫R∫RF(X,Y)(x,y)−FX(x)FY(y)dxdy{displaystyle operatorname {cov} (X,Y)=int _{mathbb {R} }int _{mathbb {R} }F_{(X,Y)}(x,y)-F_{X}(x)F_{Y}(y),dx,dy}

where F(X,Y)(x,y){displaystyle F_{(X,Y)}(x,y)} is the joint distribution function of the random vector (X,Y){displaystyle (X,Y)} and FX(x),FY(y){displaystyle F_{X}(x),F_{Y}(y)} are the marginals.

A more general identity for covariance matrices

Let X be a random vector with covariance matrix Σ(X), and let A be a matrix that can act on X. The covariance matrix of the matrix-vector product A X is:

Σ(AX)=E⁡[AXXTAT]−E⁡[AX]E⁡[XTAT]=AΣ(X)AT.{displaystyle Sigma (mathbf {A} mathbf {X} )=operatorname {E} [mathbf {A} mathbf {X} mathbf {X} ^{mathrm {T} }mathbf {A} ^{mathrm {T} }]-operatorname {E} [mathbf {A} mathbf {X} ]operatorname {E} [mathbf {X} ^{mathrm {T} }mathbf {A} ^{mathrm {T} }]=mathbf {A} Sigma (mathbf {X} )mathbf {A} ^{mathrm {T} }.}

This is a direct result of the linearity of expectation and is useful
when applying a linear transformation, such as a whitening transformation, to a vector.

Uncorrelatedness and independence

If X and Y are independent, then their covariance is zero.^[8] This follows because under independence,

E⁡[XY]=E⁡[X]⋅E⁡[Y].{displaystyle operatorname {E} [XY]=operatorname {E} [X]cdot operatorname {E} [Y].}

The converse, however, is not generally true. For example, let X be uniformly distributed in [−1, 1] and let Y = X². Clearly, X and Y are dependent, but

cov⁡(X,Y)=cov⁡(X,X2)=E⁡[X⋅X2]−E⁡[X]⋅E⁡[X2]=E⁡[X3]−E⁡[X]E⁡[X2]=0−0⋅E⁡[X2]=0.{displaystyle {begin{aligned}operatorname {cov} (X,Y)&=operatorname {cov} (X,X^{2})\&=operatorname {E} [Xcdot X^{2}]-operatorname {E} [X]cdot operatorname {E} [X^{2}]\&=operatorname {E} left[X^{3}right]-operatorname {E} [X]operatorname {E} [X^{2}]\&=0-0cdot operatorname {E} [X^{2}]\&=0.end{aligned}}}

In this case, the relationship between Y and X is non-linear, while
correlation and covariance are measures of linear dependence between two variables.
This example shows that if two variables are uncorrelated, that does not in general imply that they are independent. However, if two variables are jointly normally distributed (but not if they are merely individually normally distributed), uncorrelatedness does imply independence.

Relationship to inner products

Many of the properties of covariance can be extracted elegantly by observing that it satisfies similar properties to those of an inner product:

1. 
   bilinear: for constants a and b and random variables X, Y, Z, cov(aX + bY, Z) = a cov(X, Z) + b cov(Y, Z);


2. symmetric: cov(X, Y) = cov(Y, X);


3. 
   positive semi-definite: σ²(X) = cov(X, X) ≥ 0 for all random variables X, and cov(X, X) = 0 implies that X is a constant random variable (K).

In fact these properties imply that the covariance defines an inner product over the quotient vector space obtained by taking the subspace of random variables with finite second moment and identifying any two that differ by a constant. (This identification turns the positive semi-definiteness above into positive definiteness.) That quotient vector space is isomorphic to the subspace of random variables with finite second moment and mean zero; on that subspace, the covariance is exactly the L² inner product of real-valued functions on the sample space.

As a result, for random variables with finite variance, the inequality

|cov⁡(X,Y)|≤σ2(X)σ2(Y){displaystyle |operatorname {cov} (X,Y)|leq {sqrt {sigma ^{2}(X)sigma ^{2}(Y)}}}

holds via the Cauchy–Schwarz inequality.

Proof: If σ²(Y) = 0, then it holds trivially. Otherwise, let random variable

Z=X−cov⁡(X,Y)σ2(Y)Y.{displaystyle Z=X-{frac {operatorname {cov} (X,Y)}{sigma ^{2}(Y)}}Y.}

Then we have

0≤σ2(Z)=cov⁡(X−cov⁡(X,Y)σ2(Y)Y,X−cov⁡(X,Y)σ2(Y)Y)=σ2(X)−(cov⁡(X,Y))2σ2(Y).{displaystyle {begin{aligned}0leq sigma ^{2}(Z)&=operatorname {cov} left(X-{frac {operatorname {cov} (X,Y)}{sigma ^{2}(Y)}}Y,X-{frac {operatorname {cov} (X,Y)}{sigma ^{2}(Y)}}Yright)\[12pt]&=sigma ^{2}(X)-{frac {(operatorname {cov} (X,Y))^{2}}{sigma ^{2}(Y)}}.end{aligned}}}

Calculating the sample covariance

The sample covariances among K variables based on N observations of each, drawn from an otherwise unobserved population, are given by the K-by-K matrix q¯=[qjk]{displaystyle textstyle {overline {mathbf {q} }}=left[q_{jk}right]} with the entries

qjk=1N−1∑i=1N(Xij−X¯j)(Xik−X¯k),{displaystyle q_{jk}={frac {1}{N-1}}sum _{i=1}^{N}left(X_{ij}-{bar {X}}_{j}right)left(X_{ik}-{bar {X}}_{k}right),}

which is an estimate of the covariance between
variable j and variable k.

The sample mean and the sample covariance matrix are unbiased estimates of the mean and the covariance matrix of the random vector X{displaystyle textstyle mathbf {X} }, a vector whose jth element (j = 1, ..., K) is one of the random variables. The reason the sample covariance matrix has N−1{displaystyle textstyle N-1} in the denominator rather than N{displaystyle textstyle N} is essentially that the population mean E⁡(X){displaystyle operatorname {E} (X)} is not known and is replaced by the sample mean X¯{displaystyle mathbf {bar {X}} }. If the population mean E⁡(X){displaystyle operatorname {E} (X)} is known, the analogous unbiased estimate is given by

qjk=1N∑i=1N(Xij−E⁡(Xj))(Xik−E⁡(Xk)).{displaystyle q_{jk}={frac {1}{N}}sum _{i=1}^{N}left(X_{ij}-operatorname {E} (X_{j})right)left(X_{ik}-operatorname {E} (X_{k})right).}

Comments

The covariance is sometimes called a measure of "linear dependence" between the two random variables. That does not mean the same thing as in the context of linear algebra (see linear dependence). When the covariance is normalized, one obtains the Pearson correlation coefficient, which gives the goodness of the fit for the best possible linear function describing the relation between the variables. In this sense covariance is a linear gauge of dependence.

Applications

In genetics and molecular biology

Covariance is an important measure in biology. Certain sequences of DNA are conserved more than others among species, and thus to study secondary and tertiary structures of proteins, or of RNA structures, sequences are compared in closely related species. If sequence changes are found or no changes at all are found in noncoding RNA (such as microRNA), sequences are found to be necessary for common structural motifs, such as an RNA loop. In genetics, covariance serves a basis for computation of Genetic Relationship Matrix (GRM) (aka kinship matrix), enabling inference on population structure from sample with no known close relatives as well as inference on estimation of heritability of complex traits.

In financial economics

Covariances play a key role in financial economics, especially in portfolio theory and in the capital asset pricing model. Covariances among various assets' returns are used to determine, under certain assumptions, the relative amounts of different assets that investors should (in a normative analysis) or are predicted to (in a positive analysis) choose to hold in a context of diversification.

In meteorological and oceanographic data assimilation

The covariance matrix is important in estimating the initial conditions required for running weather forecast models. The 'forecast error covariance matrix' is typically constructed between perturbations around a mean state (either a climatological or ensemble mean). The 'observation error covariance matrix' is constructed to represent the magnitude of combined observational errors (on the diagonal) and the correlated errors between measurements (off the diagonal). This is an example of its widespread application to Kalman filtering and more general state estimation for time-varying systems.

In micrometeorology

The eddy covariance technique is a key atmospherics measurement technique where the covariance between instantaneous deviation in vertical wind speed from the mean value and instantaneous deviation in gas concentration is the basis for calculating the vertical turbulent fluxes.

In feature extraction

The covariance matrix is used to capture the spectral variability of a signal.^[9]

See also

References

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External links

Look up covariance in Wiktionary, the free dictionary.

• 
  Hazewinkel, Michiel, ed. (2001) [1994], "Covariance", Encyclopedia of Mathematics, Springer Science+Business Media B.V. / Kluwer Academic Publishers, ISBN 978-1-55608-010-4
  


• MathWorld page on calculating the sample covariance


• Covariance Tutorial using R


• Covariance and Correlation