(mathematics) For a real function defined on an interval, the least upper bound of the function's variation relative to all possible partitions of the interval.
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(mathematics) For a real function defined on an interval, the least upper bound of the function's variation relative to all possible partitions of the interval.
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| Wikipedia: Total variation |
In mathematics, the total variation of a real-valued function ƒ, defined on an interval [a, b] ⊂ R is a measure of the one-dimensional arclength of the curve with parametric equation x → ƒ(x), for x ∈ [a,b]. The total variation of a continuously differentiable function can be given as the integral

The total variation of an arbitrary real valued function ƒ defined on [a,b] is given by the more general formula

where the supremum runs over the set of all partitions P of the given interval.
The total variation of a real-valued integrable function ƒ defined on a bounded domain
,

where
is the set of continuously differentiable vector functions of compact support contained in Ω (in particular Φ | δΩ = 0), and
is the essential supremum norm. When ƒ is differentiable, the above expression simplifies to

because, by the Gauss-Ostrogradsky theorem

and the supremum is attained as

The function f is said to be of bounded variation precisely if its total variation is finite.
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In probability theory, the total variation distance between two probability measures P and Q on a sigma-algebra F is

Informally, this is the largest possible difference between the probabilities that the two probability distributions can assign to the same event.
For a finite alphabet we can write

Sometimes the statistical distance between two probability distributions is also defined without the division by two.
Given a signed measure μ on a measurable space (X,Σ), and its Hahn–Jordan decomposition into the difference of two non-negative measures

its variation is the non-negative measure

and its total variation is defined as

In detail, if E is a measurable subset of X, then

where the supremum is taken over all partitions π of E into a finite number of disjoint measurable subsets. More generally, if μ is a vector measure, then the variation is defined by

where the supremum is as above.
The total variation is a norm defined on the space of measures of bounded variation. The space of measures on a σ-algebra of sets is a Banach space, called the ca space, relative to this norm. It is contained in the larger Banach space, called the ba space, consisting of finitely additive (as opposed to countably additive) measures, also with the same norm.
Total variation can be seen as a non-negative real-valued functional defined on the space of real-valued functions (for the case of functions of one variable) or on the space of integrable functions (for the case of functions of several variables). As a functional, total variation finds applications in several branches of mathematics and engineering, like optimal control, numerical analysis, and calculus of variations, where the solution to a certain problem has to minimize its value. As an example, use of the total variation functional is common in the following two kind of problems
One variable
Several variables
Measure theory
Probability theory
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