Algorithms for calculating variance play a major role in computational statistics. A key difficulty in the design of good algorithms for this problem is that formulas for the variance may involve sums of squares, which can lead to numerical instability as well as to arithmetic overflow when dealing with large values.

Naïve algorithm

A formula for calculating the variance of an entire population of size N is:

${\displaystyle \sigma ^{2}={\overline {(x^{2})}}-{\bar {x}}^{2}={\frac {\sum _{i=1}^{N}x_{i}^{2}-(\sum _{i=1}^{N}x_{i})^{2}/N}{N}}.}$

Using Bessel's correction to calculate an unbiased estimate of the population variance from a finite sample of n observations, the formula is:

${\displaystyle s^{2}=\left({\frac {\sum _{i=1}^{n}x_{i}^{2}}{n}}-\left({\frac {\sum _{i=1}^{n}x_{i}}{n}}\right)^{2}\right)\cdot {\frac {n}{n-1}}.}$

Therefore, a naïve algorithm to calculate the estimated variance is given by the following:

This algorithm can easily be adapted to compute the variance of a finite population: simply divide by n instead of n − 1 on the last line.

Because SumSq and (Sum×Sum)/n can be very similar numbers, cancellation can lead to the precision of the result to be much less than the inherent precision of the floating-point arithmetic used to perform the computation. Thus this algorithm should not be used in practice,^[1][2] and several alternate, numerically stable, algorithms have been proposed.^[3] This is particularly bad if the standard deviation is small relative to the mean.

def shifted_data_variance(data):
    if len(data) < 2:
        return 0.0
    K = data[0]
    n = Ex = Ex2 = 0.0
    for x in data:
        n += 1
        Ex += x - K
        Ex2 += (x - K) ** 2
    variance = (Ex2 - Ex**2 / n) / (n - 1)
    # use n instead of (n-1) if want to compute the exact variance of the given data
    # use (n-1) if data are samples of a larger population
    return variance

K = Ex = Ex2 = 0.0
n = 0


def add_variable(x):
    global K, n, Ex, Ex2
    if n == 0:
        K = x
    n += 1
    Ex += x - K
    Ex2 += (x - K) ** 2

def remove_variable(x):
    global K, n, Ex, Ex2
    n -= 1
    Ex -= x - K
    Ex2 -= (x - K) ** 2

def get_mean():
    global K, n, Ex
    return K + Ex / n

def get_variance():
    global n, Ex, Ex2
    return (Ex2 - Ex**2 / n) / (n - 1)

Two-pass algorithm

An alternative approach, using a different formula for the variance, first computes the sample mean,

${\displaystyle {\bar {x}}={\frac {\sum _{j=1}^{n}x_{j}}{n}},}$

and then computes the sum of the squares of the differences from the mean,

${\displaystyle {\text{sample variance}}=s^{2}={\dfrac {\sum _{i=1}^{n}(x_{i}-{\bar {x}})^{2}}{n-1}},}$

where s is the standard deviation. This is given by the following code:

def two_pass_variance(data):
    n = len(data)
    mean = sum(data) / n
    variance = sum((x - mean) ** 2 for x in data) / (n - 1)
    return variance

This algorithm is numerically stable if n is small.^[1][4] However, the results of both of these simple algorithms ("naïve" and "two-pass") can depend inordinately on the ordering of the data and can give poor results for very large data sets due to repeated roundoff error in the accumulation of the sums. Techniques such as compensated summation can be used to combat this error to a degree.

Welford's online algorithm

It is often useful to be able to compute the variance in a single pass, inspecting each value ${\displaystyle x_{i}}$ only once; for example, when the data is being collected without enough storage to keep all the values, or when costs of memory access dominate those of computation. For such an online algorithm, a recurrence relation is required between quantities from which the required statistics can be calculated in a numerically stable fashion.

The following formulas can be used to update the mean and (estimated) variance of the sequence, for an additional element x_n. Here, ${\textstyle {\overline {x}}_{n}={\frac {1}{n}}\sum _{i=1}^{n}x_{i}}$ denotes the sample mean of the first n samples ${\displaystyle (x_{1},\dots ,x_{n})}$, ${\textstyle \sigma _{n}^{2}={\frac {1}{n}}\sum _{i=1}^{n}\left(x_{i}-{\overline {x}}_{n}\right)^{2}}$ their biased sample variance, and ${\textstyle s_{n}^{2}={\frac {1}{n-1}}\sum _{i=1}^{n}\left(x_{i}-{\overline {x}}_{n}\right)^{2}}$ their unbiased sample variance.

${\displaystyle {\bar {x}}_{n}={\frac {(n-1)\,{\bar {x}}_{n-1}+x_{n}}{n}}={\bar {x}}_{n-1}+{\frac {x_{n}-{\bar {x}}_{n-1}}{n}}}$

${\displaystyle \sigma _{n}^{2}={\frac {(n-1)\,\sigma _{n-1}^{2}+(x_{n}-{\bar {x}}_{n-1})(x_{n}-{\bar {x}}_{n})}{n}}=\sigma _{n-1}^{2}+{\frac {(x_{n}-{\bar {x}}_{n-1})(x_{n}-{\bar {x}}_{n})-\sigma _{n-1}^{2}}{n}}.}$

${\displaystyle s_{n}^{2}={\frac {n-2}{n-1}}\,s_{n-1}^{2}+{\frac {(x_{n}-{\bar {x}}_{n-1})^{2}}{n}}=s_{n-1}^{2}+{\frac {(x_{n}-{\bar {x}}_{n-1})^{2}}{n}}-{\frac {s_{n-1}^{2}}{n-1}},\quad n>1}$

These formulas suffer from numerical instability , as they repeatedly subtract a small number from a big number which scales with n. A better quantity for updating is the sum of squares of differences from the current mean, ${\textstyle \sum _{i=1}^{n}(x_{i}-{\bar {x}}_{n})^{2}}$, here denoted ${\displaystyle M_{2,n}}$:

${\displaystyle {\begin{aligned}M_{2,n}&=M_{2,n-1}+(x_{n}-{\bar {x}}_{n-1})(x_{n}-{\bar {x}}_{n})\\[4pt]\sigma _{n}^{2}&={\frac {M_{2,n}}{n}}\\[4pt]s_{n}^{2}&={\frac {M_{2,n}}{n-1}}\end{aligned}}}$

This algorithm was found by Welford,^[5][6] and it has been thoroughly analyzed.^[2][7] It is also common to denote ${\displaystyle M_{k}={\bar {x}}_{k}}$ and ${\displaystyle S_{k}=M_{2,k}}$.^[8]

An example Python implementation for Welford's algorithm is given below.

# For a new value new_value, compute the new count, new mean, the new M2.
# mean accumulates the mean of the entire dataset
# M2 aggregates the squared distance from the mean
# count aggregates the number of samples seen so far
def update(existing_aggregate, new_value):
    (count, mean, M2) = existing_aggregate
    count += 1
    delta = new_value - mean
    mean += delta / count
    delta2 = new_value - mean
    M2 += delta * delta2
    return (count, mean, M2)

# Retrieve the mean, variance and sample variance from an aggregate
def finalize(existing_aggregate):
    (count, mean, M2) = existing_aggregate
    if count < 2:
        return float("nan")
    else:
        (mean, variance, sample_variance) = (mean, M2 / count, M2 / (count - 1))
        return (mean, variance, sample_variance)

This algorithm is much less prone to loss of precision due to catastrophic cancellation, but might not be as efficient because of the division operation inside the loop. For a particularly robust two-pass algorithm for computing the variance, one can first compute and subtract an estimate of the mean, and then use this algorithm on the residuals.

The parallel algorithm below illustrates how to merge multiple sets of statistics calculated online.

Weighted incremental algorithm

The algorithm can be extended to handle unequal sample weights, replacing the simple counter n with the sum of weights seen so far. West (1979)^[9] suggests this incremental algorithm:

def weighted_incremental_variance(data_weight_pairs):
    w_sum = w_sum2 = mean = S = 0

    for x, w in data_weight_pairs:
        w_sum = w_sum + w
        w_sum2 = w_sum2 + w**2
        mean_old = mean
        mean = mean_old + (w / w_sum) * (x - mean_old)
        S = S + w * (x - mean_old) * (x - mean)

    population_variance = S / w_sum
    # Bessel's correction for weighted samples
    # Frequency weights
    sample_frequency_variance = S / (w_sum - 1)
    # Reliability weights
    sample_reliability_variance = S / (w_sum - w_sum2 / w_sum)

Parallel algorithm

Chan et al.^[10] note that Welford's online algorithm detailed above is a special case of an algorithm that works for combining arbitrary sets ${\displaystyle A}$ and ${\displaystyle B}$:

${\displaystyle {\begin{aligned}n_{AB}&=n_{A}+n_{B}\\\delta &={\bar {x}}_{B}-{\bar {x}}_{A}\\{\bar {x}}_{AB}&={\bar {x}}_{A}+\delta \cdot {\frac {n_{B}}{n_{AB}}}\\M_{2,AB}&=M_{2,A}+M_{2,B}+\delta ^{2}\cdot {\frac {n_{A}n_{B}}{n_{AB}}}\\\end{aligned}}}$.

This may be useful when, for example, multiple processing units may be assigned to discrete parts of the input.

Chan's method for estimating the mean is numerically unstable when ${\displaystyle n_{A}\approx n_{B}}$ and both are large, because the numerical error in ${\displaystyle \delta ={\bar {x}}_{B}-{\bar {x}}_{A}}$ is not scaled down in the way that it is in the ${\displaystyle n_{B}=1}$ case. In such cases, prefer ${\textstyle {\bar {x}}_{AB}={\frac {n_{A}{\bar {x}}_{A}+n_{B}{\bar {x}}_{B}}{n_{AB}}}}$.

def parallel_variance(n_a, avg_a, M2_a, n_b, avg_b, M2_b):
    n = n_a + n_b
    delta = avg_b - avg_a
    M2 = M2_a + M2_b + delta**2 * n_a * n_b / n
    var_ab = M2 / (n - 1)
    return var_ab

This can be generalized to allow parallelization with AVX, with GPUs, and computer clusters, and to covariance.^[3]

Example

Assume that all floating point operations use standard IEEE 754 double-precision arithmetic. Consider the sample (4, 7, 13, 16) from an infinite population. Based on this sample, the estimated population mean is 10, and the unbiased estimate of population variance is 30. Both the naïve algorithm and two-pass algorithm compute these values correctly.

Next consider the sample (10⁸ + 4, 10⁸ + 7, 10⁸ + 13, 10⁸ + 16), which gives rise to the same estimated variance as the first sample. The two-pass algorithm computes this variance estimate correctly, but the naïve algorithm returns 29.333333333333332 instead of 30.

While this loss of precision may be tolerable and viewed as a minor flaw of the naïve algorithm, further increasing the offset makes the error catastrophic. Consider the sample (10⁹ + 4, 10⁹ + 7, 10⁹ + 13, 10⁹ + 16). Again the estimated population variance of 30 is computed correctly by the two-pass algorithm, but the naïve algorithm now computes it as −170.66666666666666. This is a serious problem with naïve algorithm and is due to catastrophic cancellation in the subtraction of two similar numbers at the final stage of the algorithm.

Higher-order statistics

Terriberry^[11] extends Chan's formulae to calculating the third and fourth central moments, needed for example when estimating skewness and kurtosis:

${\displaystyle {\begin{aligned}M_{3,X}=M_{3,A}+M_{3,B}&{}+\delta ^{3}{\frac {n_{A}n_{B}(n_{A}-n_{B})}{n_{X}^{2}}}+3\delta {\frac {n_{A}M_{2,B}-n_{B}M_{2,A}}{n_{X}}}\\[6pt]M_{4,X}=M_{4,A}+M_{4,B}&{}+\delta ^{4}{\frac {n_{A}n_{B}\left(n_{A}^{2}-n_{A}n_{B}+n_{B}^{2}\right)}{n_{X}^{3}}}\\[6pt]&{}+6\delta ^{2}{\frac {n_{A}^{2}M_{2,B}+n_{B}^{2}M_{2,A}}{n_{X}^{2}}}+4\delta {\frac {n_{A}M_{3,B}-n_{B}M_{3,A}}{n_{X}}}\end{aligned}}}$

Here the ${\displaystyle M_{k}}$ are again the sums of powers of differences from the mean ${\textstyle \sum (x-{\overline {x}})^{k}}$, giving

${\displaystyle {\begin{aligned}&{\text{skewness}}=g_{1}={\frac {{\sqrt {n}}M_{3}}{M_{2}^{3/2}}},\\[4pt]&{\text{kurtosis}}=g_{2}={\frac {nM_{4}}{M_{2}^{2}}}-3.\end{aligned}}}$

For the incremental case (i.e., ${\displaystyle B=\{x\}}$), this simplifies to:

${\displaystyle {\begin{aligned}\delta &=x-m\\[5pt]m'&=m+{\frac {\delta }{n}}\\[5pt]M_{2}'&=M_{2}+\delta ^{2}{\frac {n-1}{n}}\\[5pt]M_{3}'&=M_{3}+\delta ^{3}{\frac {(n-1)(n-2)}{n^{2}}}-{\frac {3\delta M_{2}}{n}}\\[5pt]M_{4}'&=M_{4}+{\frac {\delta ^{4}(n-1)(n^{2}-3n+3)}{n^{3}}}+{\frac {6\delta ^{2}M_{2}}{n^{2}}}-{\frac {4\delta M_{3}}{n}}\end{aligned}}}$

By preserving the value ${\displaystyle \delta /n}$, only one division operation is needed and the higher-order statistics can thus be calculated for little incremental cost.

An example of the online algorithm for kurtosis implemented as described is:

def online_kurtosis(data):
    n = mean = M2 = M3 = M4 = 0

    for x in data:
        n1 = n
        n = n + 1
        delta = x - mean
        delta_n = delta / n
        delta_n2 = delta_n**2
        term1 = delta * delta_n * n1
        mean = mean + delta_n
        M4 = M4 + term1 * delta_n2 * (n**2 - 3*n + 3) + 6 * delta_n2 * M2 - 4 * delta_n * M3
        M3 = M3 + term1 * delta_n * (n - 2) - 3 * delta_n * M2
        M2 = M2 + term1

    # Note, you may also calculate variance using M2, and skewness using M3
    # Caution: If all the inputs are the same, M2 will be 0, resulting in a division by 0.
    kurtosis = (n * M4) / (M2**2) - 3
    return kurtosis

Pébaÿ^[12] further extends these results to arbitrary-order central moments, for the incremental and the pairwise cases, and subsequently Pébaÿ et al.^[13] for weighted and compound moments. One can also find there similar formulas for covariance.

Choi and Sweetman^[14] offer two alternative methods to compute the skewness and kurtosis, each of which can save substantial computer memory requirements and CPU time in certain applications. The first approach is to compute the statistical moments by separating the data into bins and then computing the moments from the geometry of the resulting histogram, which effectively becomes a one-pass algorithm for higher moments. One benefit is that the statistical moment calculations can be carried out to arbitrary accuracy such that the computations can be tuned to the precision of, e.g., the data storage format or the original measurement hardware. A relative histogram of a random variable can be constructed in the conventional way: the range of potential values is divided into bins and the number of occurrences within each bin are counted and plotted such that the area of each rectangle equals the portion of the sample values within that bin:

${\displaystyle H(x_{k})={\frac {h(x_{k})}{A}}}$

where ${\displaystyle h(x_{k})}$ and ${\displaystyle H(x_{k})}$ represent the frequency and the relative frequency at bin ${\displaystyle x_{k}}$ and ${\textstyle A=\sum _{k=1}^{K}h(x_{k})\,\Delta x_{k}}$ is the total area of the histogram. After this normalization, the ${\displaystyle n}$ raw moments and central moments of ${\displaystyle x(t)}$ can be calculated from the relative histogram:

${\displaystyle m_{n}^{(h)}=\sum _{k=1}^{K}x_{k}^{n}H(x_{k})\,\Delta x_{k}={\frac {1}{A}}\sum _{k=1}^{K}x_{k}^{n}h(x_{k})\,\Delta x_{k}}$

${\displaystyle \theta _{n}^{(h)}=\sum _{k=1}^{K}{\Big (}x_{k}-m_{1}^{(h)}{\Big )}^{n}\,H(x_{k})\,\Delta x_{k}={\frac {1}{A}}\sum _{k=1}^{K}{\Big (}x_{k}-m_{1}^{(h)}{\Big )}^{n}h(x_{k})\,\Delta x_{k}}$

where the superscript ${\displaystyle ^{(h)}}$ indicates the moments are calculated from the histogram. For constant bin width ${\displaystyle \Delta x_{k}=\Delta x}$ these two expressions can be simplified using ${\displaystyle I=A/\Delta x}$:

${\displaystyle m_{n}^{(h)}={\frac {1}{I}}\sum _{k=1}^{K}x_{k}^{n}\,h(x_{k})}$

${\displaystyle \theta _{n}^{(h)}={\frac {1}{I}}\sum _{k=1}^{K}{\Big (}x_{k}-m_{1}^{(h)}{\Big )}^{n}h(x_{k})}$

The second approach from Choi and Sweetman^[14] is an analytical methodology to combine statistical moments from individual segments of a time-history such that the resulting overall moments are those of the complete time-history. This methodology could be used for parallel computation of statistical moments with subsequent combination of those moments, or for combination of statistical moments computed at sequential times.

If ${\displaystyle Q}$ sets of statistical moments are known: ${\displaystyle (\gamma _{0,q},\mu _{q},\sigma _{q}^{2},\alpha _{3,q},\alpha _{4,q})\quad }$ for ${\displaystyle q=1,2,\ldots ,Q}$, then each ${\displaystyle \gamma _{n}}$ can be expressed in terms of the equivalent ${\displaystyle n}$ raw moments:

${\displaystyle \gamma _{n,q}=m_{n,q}\gamma _{0,q}\qquad \quad {\textrm {for}}\quad n=1,2,3,4\quad {\text{ and }}\quad q=1,2,\dots ,Q}$

where ${\displaystyle \gamma _{0,q}}$ is generally taken to be the duration of the ${\displaystyle q^{th}}$ time-history, or the number of points if ${\displaystyle \Delta t}$ is constant.

The benefit of expressing the statistical moments in terms of ${\displaystyle \gamma }$ is that the ${\displaystyle Q}$ sets can be combined by addition, and there is no upper limit on the value of ${\displaystyle Q}$.

${\displaystyle \gamma _{n,c}=\sum _{q=1}^{Q}\gamma _{n,q}\quad \quad {\text{for }}n=0,1,2,3,4}$

where the subscript ${\displaystyle _{c}}$ represents the concatenated time-history or combined ${\displaystyle \gamma }$. These combined values of ${\displaystyle \gamma }$ can then be inversely transformed into raw moments representing the complete concatenated time-history

${\displaystyle m_{n,c}={\frac {\gamma _{n,c}}{\gamma _{0,c}}}\quad {\text{for }}n=1,2,3,4}$

Known relationships between the raw moments (${\displaystyle m_{n}}$) and the central moments (${\displaystyle \theta _{n}=\operatorname {E} [(x-\mu )^{n}])}$) are then used to compute the central moments of the concatenated time-history. Finally, the statistical moments of the concatenated history are computed from the central moments:

${\displaystyle \mu _{c}=m_{1,c}\qquad \sigma _{c}^{2}=\theta _{2,c}\qquad \alpha _{3,c}={\frac {\theta _{3,c}}{\sigma _{c}^{3}}}\qquad \alpha _{4,c}={\frac {\theta _{4,c}}{\sigma _{c}^{4}}}-3}$

Covariance

Very similar algorithms can be used to compute the covariance.

def naive_covariance(data1, data2):
    n = len(data1)
    sum1 = sum(data1)
    sum2 = sum(data2)
    sum12 = sum([i1 * i2 for i1, i2 in zip(data1, data2)])

    covariance = (sum12 - sum1 * sum2 / n) / n
    return covariance

def shifted_data_covariance(data_x, data_y):
    n = len(data_x)
    if n < 2:
        return 0
    kx = data_x[0]
    ky = data_y[0]
    Ex = Ey = Exy = 0
    for ix, iy in zip(data_x, data_y):
        Ex += ix - kx
        Ey += iy - ky
        Exy += (ix - kx) * (iy - ky)
    return (Exy - Ex * Ey / n) / n

def two_pass_covariance(data1, data2):
    n = len(data1)
    mean1 = sum(data1) / n
    mean2 = sum(data2) / n

    covariance = 0
    for i1, i2 in zip(data1, data2):
        a = i1 - mean1
        b = i2 - mean2
        covariance += a * b / n
    return covariance

def online_covariance(data1, data2):
    meanx = meany = C = n = 0
    for x, y in zip(data1, data2):
        n += 1
        dx = x - meanx
        meanx += dx / n
        meany += (y - meany) / n
        C += dx * (y - meany)

    population_covar = C / n
    # Bessel's correction for sample variance
    sample_covar = C / (n - 1)

def online_weighted_covariance(data1, data2, data3):
    meanx = meany = 0
    wsum = wsum2 = 0
    C = 0
    for x, y, w in zip(data1, data2, data3):
        wsum += w
        wsum2 += w * w
        dx = x - meanx
        meanx += (w / wsum) * dx
        meany += (w / wsum) * (y - meany)
        C += w * dx * (y - meany)

    population_covar = C / wsum
    # Bessel's correction for sample variance
    # Frequency weights
    sample_frequency_covar = C / (wsum - 1)
    # Reliability weights
    sample_reliability_covar = C / (wsum - wsum2 / wsum)

See also

• Kahan summation algorithm
• Squared deviations from the mean
• Yamartino method

References

External links

• Weisstein, Eric W. "Sample Variance Computation". MathWorld.