scipy.stats.levy_l#

scipy.stats.levy_l = <scipy.stats._continuous_distns.levy_l_gen object>[source]#

A left-skewed Levy continuous random variable.

As an instance of the rv_continuous class, levy_l object inherits from it a collection of generic methods (see below for the full list), and completes them with details specific for this particular distribution.

See also

levy, levy_stable

Notes

The probability density function for levy_l is:

\[f(x) = \frac{1}{|x| \sqrt{2\pi |x|}} \exp{ \left(-\frac{1}{2|x|} \right)}\]

for \(x <= 0\).

This is the same as the Levy-stable distribution with \(a=1/2\) and \(b=-1\).

The probability density above is defined in the “standardized” form. To shift and/or scale the distribution use the loc and scale parameters. Specifically, levy_l.pdf(x, loc, scale) is identically equivalent to levy_l.pdf(y) / scale with y = (x - loc) / scale. Note that shifting the location of a distribution does not make it a “noncentral” distribution; noncentral generalizations of some distributions are available in separate classes.

Examples

>>> import numpy as np
>>> from scipy.stats import levy_l
>>> import matplotlib.pyplot as plt
>>> fig, ax = plt.subplots(1, 1)

Calculate the first four moments:

>>> mean, var, skew, kurt = levy_l.stats(moments='mvsk')

Display the probability density function (pdf):

>>> # `levy_l` is very heavy-tailed.
>>> # To show a nice plot, let's cut off the lower 40 percent.
>>> a, b = levy_l.ppf(0.4), levy_l.ppf(1)
>>> x = np.linspace(a, b, 100)
>>> ax.plot(x, levy_l.pdf(x),
...        'r-', lw=5, alpha=0.6, label='levy_l pdf')

Alternatively, the distribution object can be called (as a function) to fix the shape, location and scale parameters. This returns a “frozen” RV object holding the given parameters fixed.

Freeze the distribution and display the frozen pdf:

>>> rv = levy_l()
>>> ax.plot(x, rv.pdf(x), 'k-', lw=2, label='frozen pdf')

Check accuracy of cdf and ppf:

>>> vals = levy_l.ppf([0.001, 0.5, 0.999])
>>> np.allclose([0.001, 0.5, 0.999], levy_l.cdf(vals))
True

Generate random numbers:

>>> r = levy_l.rvs(size=1000)

And compare the histogram:

>>> # manual binning to ignore the tail
>>> bins = np.concatenate(([np.min(r)], np.linspace(a, b, 20)))
>>> ax.hist(r, bins=bins, density=True, histtype='stepfilled', alpha=0.2)
>>> ax.set_xlim([x[0], x[-1]])
>>> ax.legend(loc='best', frameon=False)
>>> plt.show()
../../_images/scipy-stats-levy_l-1.png

Methods

rvs(loc=0, scale=1, size=1, random_state=None)

Random variates.

pdf(x, loc=0, scale=1)

Probability density function.

logpdf(x, loc=0, scale=1)

Log of the probability density function.

cdf(x, loc=0, scale=1)

Cumulative distribution function.

logcdf(x, loc=0, scale=1)

Log of the cumulative distribution function.

sf(x, loc=0, scale=1)

Survival function (also defined as 1 - cdf, but sf is sometimes more accurate).

logsf(x, loc=0, scale=1)

Log of the survival function.

ppf(q, loc=0, scale=1)

Percent point function (inverse of cdf — percentiles).

isf(q, loc=0, scale=1)

Inverse survival function (inverse of sf).

moment(order, loc=0, scale=1)

Non-central moment of the specified order.

stats(loc=0, scale=1, moments=’mv’)

Mean(‘m’), variance(‘v’), skew(‘s’), and/or kurtosis(‘k’).

entropy(loc=0, scale=1)

(Differential) entropy of the RV.

fit(data)

Parameter estimates for generic data. See scipy.stats.rv_continuous.fit for detailed documentation of the keyword arguments.

expect(func, args=(), loc=0, scale=1, lb=None, ub=None, conditional=False, **kwds)

Expected value of a function (of one argument) with respect to the distribution.

median(loc=0, scale=1)

Median of the distribution.

mean(loc=0, scale=1)

Mean of the distribution.

var(loc=0, scale=1)

Variance of the distribution.

std(loc=0, scale=1)

Standard deviation of the distribution.

interval(confidence, loc=0, scale=1)

Confidence interval with equal areas around the median.