norminv

Normal inverse cumulative distribution function

Syntax

x = norminv(p)

x = norminv(p,mu)

x = norminv(p,mu,sigma)

[x,xLo,xUp] = norminv(p,mu,sigma,pCov)

[x,xLo,xUp] = norminv(p,mu,sigma,pCov,alpha)

Description

x = norminv(p) returns the inverse of the standard normal cumulative distribution function (cdf), evaluated at the probability values in p.

x = norminv(p,mu) returns the inverse of the normal cdf with mean mu and the unit standard deviation, evaluated at the probability values in p.

x = norminv(p,mu,sigma) returns the inverse of the normal cdf with mean mu and standard deviation sigma, evaluated at the probability values in p.

[x,xLo,xUp] = norminv(p,mu,sigma,pCov) also returns the 95% confidence bounds [xLo,xUp] of x when mu and sigma are estimates. pCov is the covariance matrix of the estimated parameters.

[x,xLo,xUp] = norminv(p,mu,sigma,pCov,alpha) specifies the confidence level for the confidence interval [xLo,xUp] to be 100(1–alpha)%.

Examples

Inverse of Standard Normal cdf

Find an interval that contains 95% of the values from a standard normal distribution.

x = norminv([0.025 0.975])

x = 1×2

   -1.9600    1.9600

Note that the interval x is not the only such interval, but it is the shortest. Find another interval.

xl = norminv([0.01 0.96])

xl = 1×2

   -2.3263    1.7507

The interval x1 also contains 95% of the probability, but it is longer than x.

Inverse of Normal Distribution cdf

Compute the inverse of cdf values evaluated at the probability values in p for the normal distribution with mean mu and standard deviation sigma.

p = 0:0.25:1;
mu = 2;
sigma = 1;
x = norminv(p,mu,sigma)

x = 1×5

      -Inf    1.3255    2.0000    2.6745       Inf

Compute the inverse of cdf values evaluated at 0.5 for various normal distributions with different mean parameters.

mu = [-2,-1,0,1,2];
sigma = 1;
x = norminv(0.5,mu,sigma)

x = 1×5

    -2    -1     0     1     2

Confidence Interval of Inverse Normal cdf Value

Find the maximum likelihood estimates (MLEs) of the normal distribution parameters, and then find the confidence interval of the corresponding inverse cdf value.

Generate 1000 normal random numbers from the normal distribution with mean 5 and standard deviation 2.

rng('default') % For reproducibility
n = 1000; % Number of samples
x = normrnd(5,2,[n,1]);

Find the MLEs for the distribution parameters (mean and standard deviation) by using mle.

phat = mle(x)

phat = 1×2

    4.9347    1.9969

muHat = phat(1);
sigmaHat = phat(2);

Estimate the covariance of the distribution parameters by using normlike. The function normlike returns an approximation to the asymptotic covariance matrix if you pass the MLEs and the samples used to estimate the MLEs.

[~,pCov] = normlike([muHat,sigmaHat],x)

pCov = 2×2

    0.0040   -0.0000
   -0.0000    0.0020

Find the inverse cdf value at 0.5 and its 99% confidence interval.

[x,xLo,xUp] = norminv(0.5,muHat,sigmaHat,pCov,0.01)

x = 4.9347

xLo = 4.7721

xUp = 5.0974

x is the inverse cdf value using the normal distribution with the parameters muHat and sigmaHat. The interval [xLo,xUp] is the 99% confidence interval of the inverse cdf value evaluated at 0.5, considering the uncertainty of muHat and sigmaHat using pCov. The 99% confidence interval means the probability that [xLo,xUp] contains the true inverse cdf value is 0.99.

Input Arguments

p — Probability values at which to evaluate inverse of cdf

scalar value in [0,1] | array of scalar values

Probability values at which to evaluate the inverse of the cdf (icdf), specified as a scalar value or an array of scalar values, where each element is in the range [0,1].

If you specify pCov to compute the confidence interval [xLo,xUp], then p must be a scalar value.

To evaluate the icdf at multiple values, specify p using an array. To evaluate the icdfs of multiple distributions, specify mu and sigma using arrays. If one or more of the input arguments p, mu, and sigma are arrays, then the array sizes must be the same. In this case, norminv expands each scalar input into a constant array of the same size as the array inputs. Each element in x is the icdf value of the distribution specified by the corresponding elements in mu and sigma, evaluated at the corresponding element in p.

Example: [0.1,0.5,0.9]

Data Types: single | double

mu — Mean

0 (default) | scalar value | array of scalar values

Mean of the normal distribution, specified as a scalar value or an array of scalar values.

If you specify pCov to compute the confidence interval [xLo,xUp], then mu must be a scalar value.

To evaluate the icdf at multiple values, specify p using an array. To evaluate the icdfs of multiple distributions, specify mu and sigma using arrays. If one or more of the input arguments p, mu, and sigma are arrays, then the array sizes must be the same. In this case, norminv expands each scalar input into a constant array of the same size as the array inputs. Each element in x is the icdf value of the distribution specified by the corresponding elements in mu and sigma, evaluated at the corresponding element in p.

Example: [0 1 2; 0 1 2]

Data Types: single | double

sigma — Standard deviation

1 (default) | positive scalar value | array of positive scalar values

Standard deviation of the normal distribution, specified as a positive scalar value or an array of positive scalar values.

If you specify pCov to compute the confidence interval [xLo,xUp], then sigma must be a scalar value.

To evaluate the icdf at multiple values, specify p using an array. To evaluate the icdfs of multiple distributions, specify mu and sigma using arrays. If one or more of the input arguments p, mu, and sigma are arrays, then the array sizes must be the same. In this case, norminv expands each scalar input into a constant array of the same size as the array inputs. Each element in x is the icdf value of the distribution specified by the corresponding elements in mu and sigma, evaluated at the corresponding element in p.

Example: [1 1 1; 2 2 2]

Data Types: single | double

pCov — Covariance of estimates

2-by-2 numeric matrix

Covariance of the estimates mu and sigma, specified as a 2-by-2 matrix.

If you specify pCov to compute the confidence interval [xLo,xUp], then p, mu, and sigma must be scalar values.

You can estimate mu and sigma by using mle, and estimate the covariance of mu and sigma by using normlike. For an example, see Confidence Interval of Inverse Normal cdf Value.

Data Types: single | double

alpha — Significance level

0.05 (default) | scalar in the range (0,1)

Significance level for the confidence interval, specified as a scalar in the range (0,1). The confidence level is 100(1–alpha)%, where alpha is the probability that the confidence interval does not contain the true value.

Example: 0.01

Data Types: single | double

Output Arguments

x — icdf values

scalar value | array of scalar values

icdf values, evaluated at the probability values in p, returned as a scalar value or an array of scalar values. x is the same size as p, mu, and sigma after any necessary scalar expansion. Each element in x is the icdf value of the distribution specified by the corresponding elements in mu and sigma, evaluated at the corresponding element in p.

xLo — Lower confidence bound for x

scalar value | array of scalar values

Lower confidence bound for x, returned as a scalar value or an array of scalar values. xLo has the same size as x.

xUp — Upper confidence bound for x

scalar value | array of scalar values

Upper confidence bound for x, returned as a scalar value or an array of scalar values. xUp has the same size as x.

More About

Normal Distribution

The normal distribution is a two-parameter family of curves. The first parameter, µ, is the mean. The second parameter, σ, is the standard deviation.

The standard normal distribution has zero mean and unit standard deviation.

The normal inverse function is defined in terms of the normal cdf as

$$x=F^{-1}(p|\mu ,\sigma )=\{x:F(x|\mu ,\sigma )=p\},$$

where

$$p=F(x|\mu ,\sigma )=\frac{1}{\sigma \sqrt{2\pi }}{\displaystyle {\int }_{-\infty }^x{e}^{\frac{-{(t-\mu )}^2}{2{\sigma }^2}}}dt.$$

The result x is the solution of the integral equation where you supply the desired probability p.

Algorithms

• The norminv function uses the inverse complementary error function erfcinv. The relationship between norminv and erfcinv is

  $$\text{norminv}(p)=-\sqrt{2}\text{erfcinv}(2p)$$

  The inverse complementary error function erfcinv(x) is defined as erfcinv(erfc(x))=x, and the complementary error function erfc(x) is defined as

  $$\text{erfc}(x)=1-\text{erf}(x)=\frac{2}{\sqrt{\pi }}{\displaystyle {\int }_x^{\infty }{e}^{-t^2}dt}.$$

• The norminv function computes confidence bounds for x by using the delta method. norminv(p,mu,sigma) is equivalent to mu + sigma*norminv(p,0,1). Therefore, the norminv function estimates the variance of mu + sigma*norminv(p,0,1) using the covariance matrix of mu and sigma by the delta method, and finds the confidence bounds using the estimates of this variance. The computed bounds give approximately the desired confidence level when you estimate mu, sigma, and pCov from large samples.

Alternative Functionality

• norminv is a function specific to normal distribution. Statistics and Machine Learning Toolbox™ also offers the generic function icdf, which supports various probability distributions. To use icdf, create a NormalDistribution probability distribution object and pass the object as an input argument or specify the probability distribution name and its parameters. Note that the distribution-specific function norminv is faster than the generic function icdf.

References

[1] Abramowitz, M., and I. A. Stegun. Handbook of Mathematical Functions. New York: Dover, 1964.

[2] Evans, M., N. Hastings, and B. Peacock. Statistical Distributions. 2nd ed. Hoboken, NJ: John Wiley & Sons, Inc., 1993.

Extended Capabilities

C/C++ Code Generation
Generate C and C++ code using MATLAB® Coder™.

GPU Arrays

Accelerate code by running on a graphics processing unit (GPU) using Parallel Computing Toolbox™.

This function fully supports GPU arrays. For more information, see Run MATLAB Functions on a GPU (Parallel Computing Toolbox).

Version History

Introduced before R2006a