Mathematics
Mathematical Operators
Base.:-
— Method.-(x)
Unary minus operator.
Base.:+
— Function.+(x, y...)
Addition operator. x+y+z+...
calls this function with all arguments, i.e. +(x, y, z, ...)
.
Base.:-
— Method.-(x, y)
Subtraction operator.
Base.:*
— Method.*(x, y...)
Multiplication operator. x*y*z*...
calls this function with all arguments, i.e. *(x, y, z, ...)
.
Base.:/
— Function./(x, y)
Right division operator: multiplication of x
by the inverse of y
on the right. Gives floating-point results for integer arguments.
Base.:\
— Method.\(x, y)
Left division operator: multiplication of y
by the inverse of x
on the left. Gives floating-point results for integer arguments.
julia> 3 \ 6
2.0
julia> inv(3) * 6
2.0
julia> A = [1 2; 3 4]; x = [5, 6];
julia> A \ x
2-element Array{Float64,1}:
-4.0
4.5
julia> inv(A) * x
2-element Array{Float64,1}:
-4.0
4.5
Base.:^
— Method.^(x, y)
Exponentiation operator. If x
is a matrix, computes matrix exponentiation.
If y
is an Int
literal (e.g. 2
in x^2
or -3
in x^-3
), the Julia code x^y
is transformed by the compiler to Base.literal_pow(^, x, Val{y})
, to enable compile-time specialization on the value of the exponent. (As a default fallback we have Base.literal_pow(^, x, Val{y}) = ^(x,y)
, where usually ^ == Base.^
unless ^
has been defined in the calling namespace.)
julia> 3^5
243
julia> A = [1 2; 3 4]
2×2 Array{Int64,2}:
1 2
3 4
julia> A^3
2×2 Array{Int64,2}:
37 54
81 118
Base.fma
— Function.fma(x, y, z)
Computes x*y+z
without rounding the intermediate result x*y
. On some systems this is significantly more expensive than x*y+z
. fma
is used to improve accuracy in certain algorithms. See muladd
.
Base.muladd
— Function.muladd(x, y, z)
Combined multiply-add, computes x*y+z
in an efficient manner. This may on some systems be equivalent to x*y+z
, or to fma(x,y,z)
. muladd
is used to improve performance. See fma
.
Example
julia> muladd(3, 2, 1)
7
julia> 3 * 2 + 1
7
Base.div
— Function.div(x, y)
÷(x, y)
The quotient from Euclidean division. Computes x/y
, truncated to an integer.
julia> 9 ÷ 4
2
julia> -5 ÷ 3
-1
Base.fld
— Function.fld(x, y)
Largest integer less than or equal to x/y
.
julia> fld(7.3,5.5)
1.0
Base.cld
— Function.cld(x, y)
Smallest integer larger than or equal to x/y
.
julia> cld(5.5,2.2)
3.0
Base.mod
— Function.mod(x, y)
rem(x, y, RoundDown)
The reduction of x
modulo y
, or equivalently, the remainder of x
after floored division by y
, i.e.
x - y*fld(x,y)
if computed without intermediate rounding.
The result will have the same sign as y
, and magnitude less than abs(y)
(with some exceptions, see note below).
When used with floating point values, the exact result may not be representable by the type, and so rounding error may occur. In particular, if the exact result is very close to y
, then it may be rounded to y
.
julia> mod(8, 3)
2
julia> mod(9, 3)
0
julia> mod(8.9, 3)
2.9000000000000004
julia> mod(eps(), 3)
2.220446049250313e-16
julia> mod(-eps(), 3)
3.0
rem(x::Integer, T::Type{<:Integer}) -> T
mod(x::Integer, T::Type{<:Integer}) -> T
%(x::Integer, T::Type{<:Integer}) -> T
Find y::T
such that x
≡ y
(mod n), where n is the number of integers representable in T
, and y
is an integer in [typemin(T),typemax(T)]
. If T
can represent any integer (e.g. T == BigInt
), then this operation corresponds to a conversion to T
.
julia> 129 % Int8
-127
Base.rem
— Function.rem(x, y)
%(x, y)
Remainder from Euclidean division, returning a value of the same sign as x
, and smaller in magnitude than y
. This value is always exact.
julia> x = 15; y = 4;
julia> x % y
3
julia> x == div(x, y) * y + rem(x, y)
true
Base.Math.rem2pi
— Function.rem2pi(x, r::RoundingMode)
Compute the remainder of x
after integer division by 2π
, with the quotient rounded according to the rounding mode r
. In other words, the quantity
x - 2π*round(x/(2π),r)
without any intermediate rounding. This internally uses a high precision approximation of 2π, and so will give a more accurate result than rem(x,2π,r)
if
r == RoundNearest
, then the result is in the interval $[-π, π]$. This will generally be the most accurate result.if
r == RoundToZero
, then the result is in the interval $[0, 2π]$ ifx
is positive,. or $[-2π, 0]$ otherwise.if
r == RoundDown
, then the result is in the interval $[0, 2π]$.if
r == RoundUp
, then the result is in the interval $[-2π, 0]$.
Example
julia> rem2pi(7pi/4, RoundNearest)
-0.7853981633974485
julia> rem2pi(7pi/4, RoundDown)
5.497787143782138
Base.Math.mod2pi
— Function.mod2pi(x)
Modulus after division by 2π
, returning in the range $[0,2π)$.
This function computes a floating point representation of the modulus after division by numerically exact 2π
, and is therefore not exactly the same as mod(x,2π)
, which would compute the modulus of x
relative to division by the floating-point number 2π
.
Example
julia> mod2pi(9*pi/4)
0.7853981633974481
Base.divrem
— Function.divrem(x, y)
The quotient and remainder from Euclidean division. Equivalent to (div(x,y), rem(x,y))
or (x÷y, x%y)
.
julia> divrem(3,7)
(0, 3)
julia> divrem(7,3)
(2, 1)
Base.fldmod
— Function.fldmod(x, y)
The floored quotient and modulus after division. Equivalent to (fld(x,y), mod(x,y))
.
Base.fld1
— Function.fld1(x, y)
Flooring division, returning a value consistent with mod1(x,y)
See also: mod1
.
julia> x = 15; y = 4;
julia> fld1(x, y)
4
julia> x == fld(x, y) * y + mod(x, y)
true
julia> x == (fld1(x, y) - 1) * y + mod1(x, y)
true
Base.mod1
— Function.mod1(x, y)
Modulus after flooring division, returning a value r
such that mod(r, y) == mod(x, y)
in the range $(0, y]$ for positive y
and in the range $[y,0)$ for negative y
.
julia> mod1(4, 2)
2
julia> mod1(4, 3)
1
Base.fldmod1
— Function.Base.://
— Function.//(num, den)
Divide two integers or rational numbers, giving a Rational
result.
julia> 3 // 5
3//5
julia> (3 // 5) // (2 // 1)
3//10
Base.rationalize
— Function.rationalize([T<:Integer=Int,] x; tol::Real=eps(x))
Approximate floating point number x
as a Rational
number with components of the given integer type. The result will differ from x
by no more than tol
. If T
is not provided, it defaults to Int
.
julia> rationalize(5.6)
28//5
julia> a = rationalize(BigInt, 10.3)
103//10
julia> typeof(numerator(a))
BigInt
Base.numerator
— Function.numerator(x)
Numerator of the rational representation of x
.
julia> numerator(2//3)
2
julia> numerator(4)
4
Base.denominator
— Function.denominator(x)
Denominator of the rational representation of x
.
julia> denominator(2//3)
3
julia> denominator(4)
1
Base.:<<
— Function.<<(x, n)
Left bit shift operator, x << n
. For n >= 0
, the result is x
shifted left by n
bits, filling with 0
s. This is equivalent to x * 2^n
. For n < 0
, this is equivalent to x >> -n
.
julia> Int8(3) << 2
12
julia> bits(Int8(3))
"00000011"
julia> bits(Int8(12))
"00001100"
<<(B::BitVector, n) -> BitVector
Left bit shift operator, B << n
. For n >= 0
, the result is B
with elements shifted n
positions backwards, filling with false
values. If n < 0
, elements are shifted forwards. Equivalent to B >> -n
.
Examples
julia> B = BitVector([true, false, true, false, false])
5-element BitArray{1}:
true
false
true
false
false
julia> B << 1
5-element BitArray{1}:
false
true
false
false
false
julia> B << -1
5-element BitArray{1}:
false
true
false
true
false
Base.:>>
— Function.>>(x, n)
Right bit shift operator, x >> n
. For n >= 0
, the result is x
shifted right by n
bits, where n >= 0
, filling with 0
s if x >= 0
, 1
s if x < 0
, preserving the sign of x
. This is equivalent to fld(x, 2^n)
. For n < 0
, this is equivalent to x << -n
.
julia> Int8(13) >> 2
3
julia> bits(Int8(13))
"00001101"
julia> bits(Int8(3))
"00000011"
julia> Int8(-14) >> 2
-4
julia> bits(Int8(-14))
"11110010"
julia> bits(Int8(-4))
"11111100"
>>(B::BitVector, n) -> BitVector
Right bit shift operator, B >> n
. For n >= 0
, the result is B
with elements shifted n
positions forward, filling with false
values. If n < 0
, elements are shifted backwards. Equivalent to B << -n
.
Example
julia> B = BitVector([true, false, true, false, false])
5-element BitArray{1}:
true
false
true
false
false
julia> B >> 1
5-element BitArray{1}:
false
true
false
true
false
julia> B >> -1
5-element BitArray{1}:
false
true
false
false
false
Base.:>>>
— Function.>>>(x, n)
Unsigned right bit shift operator, x >>> n
. For n >= 0
, the result is x
shifted right by n
bits, where n >= 0
, filling with 0
s. For n < 0
, this is equivalent to x << -n
.
For Unsigned
integer types, this is equivalent to >>
. For Signed
integer types, this is equivalent to signed(unsigned(x) >> n)
.
julia> Int8(-14) >>> 2
60
julia> bits(Int8(-14))
"11110010"
julia> bits(Int8(60))
"00111100"
BigInt
s are treated as if having infinite size, so no filling is required and this is equivalent to >>
.
>>>(B::BitVector, n) -> BitVector
Unsigned right bitshift operator, B >>> n
. Equivalent to B >> n
. See >>
for details and examples.
Base.colon
— Function.colon(start, [step], stop)
Called by :
syntax for constructing ranges.
julia> colon(1, 2, 5)
1:2:5
:(start, [step], stop)
Range operator. a:b
constructs a range from a
to b
with a step size of 1, and a:s:b
is similar but uses a step size of s
. These syntaxes call the function colon
. The colon is also used in indexing to select whole dimensions.
Base.range
— Function.range(start, [step], length)
Construct a range by length, given a starting value and optional step (defaults to 1).
Base.OneTo
— Type.Base.OneTo(n)
Define an AbstractUnitRange
that behaves like 1:n
, with the added distinction that the lower limit is guaranteed (by the type system) to be 1.
Base.StepRangeLen
— Type.StepRangeLen{T,R,S}(ref::R, step::S, len, [offset=1])
A range r
where r[i]
produces values of type T
, parametrized by a ref
erence value, a step
, and the len
gth. By default ref
is the starting value r[1]
, but alternatively you can supply it as the value of r[offset]
for some other index 1 <= offset <= len
. In conjunction with TwicePrecision
this can be used to implement ranges that are free of roundoff error.
Base.:==
— Function.==(x, y)
Generic equality operator, giving a single Bool
result. Falls back to ===
. Should be implemented for all types with a notion of equality, based on the abstract value that an instance represents. For example, all numeric types are compared by numeric value, ignoring type. Strings are compared as sequences of characters, ignoring encoding.
Follows IEEE semantics for floating-point numbers.
Collections should generally implement ==
by calling ==
recursively on all contents.
New numeric types should implement this function for two arguments of the new type, and handle comparison to other types via promotion rules where possible.
Base.:!=
— Function.!=(x, y)
≠(x,y)
Not-equals comparison operator. Always gives the opposite answer as ==
. New types should generally not implement this, and rely on the fallback definition !=(x,y) = !(x==y)
instead.
julia> 3 != 2
true
julia> "foo" ≠ "foo"
false
Base.:!==
— Function.!==(x, y)
≢(x,y)
Equivalent to !(x === y)
.
julia> a = [1, 2]; b = [1, 2];
julia> a ≢ b
true
julia> a ≢ a
false
Base.:<
— Function.<(x, y)
Less-than comparison operator. New numeric types should implement this function for two arguments of the new type. Because of the behavior of floating-point NaN values, <
implements a partial order. Types with a canonical partial order should implement <
, and types with a canonical total order should implement isless
.
julia> 'a' < 'b'
true
julia> "abc" < "abd"
true
julia> 5 < 3
false
Base.:<=
— Function.<=(x, y)
≤(x,y)
Less-than-or-equals comparison operator.
julia> 'a' <= 'b'
true
julia> 7 ≤ 7 ≤ 9
true
julia> "abc" ≤ "abc"
true
julia> 5 <= 3
false
Base.:>
— Function.>(x, y)
Greater-than comparison operator. Generally, new types should implement <
instead of this function, and rely on the fallback definition >(x, y) = y < x
.
julia> 'a' > 'b'
false
julia> 7 > 3 > 1
true
julia> "abc" > "abd"
false
julia> 5 > 3
true
Base.:>=
— Function.>=(x, y)
≥(x,y)
Greater-than-or-equals comparison operator.
julia> 'a' >= 'b'
false
julia> 7 ≥ 7 ≥ 3
true
julia> "abc" ≥ "abc"
true
julia> 5 >= 3
true
Base.cmp
— Function.cmp(x,y)
Return -1, 0, or 1 depending on whether x
is less than, equal to, or greater than y
, respectively. Uses the total order implemented by isless
. For floating-point numbers, uses <
but throws an error for unordered arguments.
julia> cmp(1, 2)
-1
julia> cmp(2, 1)
1
julia> cmp(2+im, 3-im)
ERROR: MethodError: no method matching isless(::Complex{Int64}, ::Complex{Int64})
[...]
Base.:~
— Function.~(x)
Bitwise not.
Examples
julia> ~4
-5
julia> ~10
-11
julia> ~true
false
Base.:&
— Function.&(x, y)
Bitwise and.
Examples
julia> 4 & 10
0
julia> 4 & 12
4
Base.:|
— Function.|(x, y)
Bitwise or.
Examples
julia> 4 | 10
14
julia> 4 | 1
5
Base.xor
— Function.xor(x, y)
⊻(x, y)
Bitwise exclusive or of x
and y
. The infix operation a ⊻ b
is a synonym for xor(a,b)
, and ⊻
can be typed by tab-completing \xor
or \veebar
in the Julia REPL.
julia> [true; true; false] .⊻ [true; false; false]
3-element BitArray{1}:
false
true
false
Base.:!
— Function.!(x)
Boolean not.
julia> !true
false
julia> !false
true
julia> .![true false true]
1×3 BitArray{2}:
false true false
!f::Function
Predicate function negation: when the argument of !
is a function, it returns a function which computes the boolean negation of f
. Example:
julia> str = "∀ ε > 0, ∃ δ > 0: |x-y| < δ ⇒ |f(x)-f(y)| < ε"
"∀ ε > 0, ∃ δ > 0: |x-y| < δ ⇒ |f(x)-f(y)| < ε"
julia> filter(isalpha, str)
"εδxyδfxfyε"
julia> filter(!isalpha, str)
"∀ > 0, ∃ > 0: |-| < ⇒ |()-()| < "
&&
— Keyword.x && y
Short-circuiting boolean AND.
||
— Keyword.x || y
Short-circuiting boolean OR.
Mathematical Functions
Base.isapprox
— Function.isapprox(x, y; rtol::Real=sqrt(eps), atol::Real=0, nans::Bool=false, norm::Function)
Inexact equality comparison: true
if norm(x-y) <= atol + rtol*max(norm(x), norm(y))
. The default atol
is zero and the default rtol
depends on the types of x
and y
. The keyword argument nans
determines whether or not NaN values are considered equal (defaults to false).
For real or complex floating-point values, rtol
defaults to sqrt(eps(typeof(real(x-y))))
. This corresponds to requiring equality of about half of the significand digits. For other types, rtol
defaults to zero.
x
and y
may also be arrays of numbers, in which case norm
defaults to vecnorm
but may be changed by passing a norm::Function
keyword argument. (For numbers, norm
is the same thing as abs
.) When x
and y
are arrays, if norm(x-y)
is not finite (i.e. ±Inf
or NaN
), the comparison falls back to checking whether all elements of x
and y
are approximately equal component-wise.
The binary operator ≈
is equivalent to isapprox
with the default arguments, and x ≉ y
is equivalent to !isapprox(x,y)
.
julia> 0.1 ≈ (0.1 - 1e-10)
true
julia> isapprox(10, 11; atol = 2)
true
julia> isapprox([10.0^9, 1.0], [10.0^9, 2.0])
true
Base.sin
— Function.sin(x)
Compute sine of x
, where x
is in radians.
Base.cos
— Function.cos(x)
Compute cosine of x
, where x
is in radians.
Base.tan
— Function.tan(x)
Compute tangent of x
, where x
is in radians.
Base.Math.sind
— Function.sind(x)
Compute sine of x
, where x
is in degrees.
Base.Math.cosd
— Function.cosd(x)
Compute cosine of x
, where x
is in degrees.
Base.Math.tand
— Function.tand(x)
Compute tangent of x
, where x
is in degrees.
Base.Math.sinpi
— Function.sinpi(x)
Compute $\sin(\pi x)$ more accurately than sin(pi*x)
, especially for large x
.
Base.Math.cospi
— Function.cospi(x)
Compute $\cos(\pi x)$ more accurately than cos(pi*x)
, especially for large x
.
Base.sinh
— Function.sinh(x)
Compute hyperbolic sine of x
.
Base.cosh
— Function.cosh(x)
Compute hyperbolic cosine of x
.
Base.tanh
— Function.tanh(x)
Compute hyperbolic tangent of x
.
Base.asin
— Function.asin(x)
Compute the inverse sine of x
, where the output is in radians.
Base.acos
— Function.acos(x)
Compute the inverse cosine of x
, where the output is in radians
Base.atan
— Function.atan(x)
Compute the inverse tangent of x
, where the output is in radians.
Base.Math.atan2
— Function.atan2(y, x)
Compute the inverse tangent of y/x
, using the signs of both x
and y
to determine the quadrant of the return value.
Base.Math.asind
— Function.asind(x)
Compute the inverse sine of x
, where the output is in degrees.
Base.Math.acosd
— Function.acosd(x)
Compute the inverse cosine of x
, where the output is in degrees.
Base.Math.atand
— Function.atand(x)
Compute the inverse tangent of x
, where the output is in degrees.
Base.Math.sec
— Function.sec(x)
Compute the secant of x
, where x
is in radians.
Base.Math.csc
— Function.csc(x)
Compute the cosecant of x
, where x
is in radians.
Base.Math.cot
— Function.cot(x)
Compute the cotangent of x
, where x
is in radians.
Base.Math.secd
— Function.secd(x)
Compute the secant of x
, where x
is in degrees.
Base.Math.cscd
— Function.cscd(x)
Compute the cosecant of x
, where x
is in degrees.
Base.Math.cotd
— Function.cotd(x)
Compute the cotangent of x
, where x
is in degrees.
Base.Math.asec
— Function.asec(x)
Compute the inverse secant of x
, where the output is in radians.
Base.Math.acsc
— Function.acsc(x)
Compute the inverse cosecant of x
, where the output is in radians.
Base.Math.acot
— Function.acot(x)
Compute the inverse cotangent of x
, where the output is in radians.
Base.Math.asecd
— Function.asecd(x)
Compute the inverse secant of x
, where the output is in degrees.
Base.Math.acscd
— Function.acscd(x)
Compute the inverse cosecant of x
, where the output is in degrees.
Base.Math.acotd
— Function.acotd(x)
Compute the inverse cotangent of x
, where the output is in degrees.
Base.Math.sech
— Function.sech(x)
Compute the hyperbolic secant of x
Base.Math.csch
— Function.csch(x)
Compute the hyperbolic cosecant of x
.
Base.Math.coth
— Function.coth(x)
Compute the hyperbolic cotangent of x
.
Base.asinh
— Function.asinh(x)
Compute the inverse hyperbolic sine of x
.
Base.acosh
— Function.acosh(x)
Compute the inverse hyperbolic cosine of x
.
Base.atanh
— Function.atanh(x)
Compute the inverse hyperbolic tangent of x
.
Base.Math.asech
— Function.asech(x)
Compute the inverse hyperbolic secant of x
.
Base.Math.acsch
— Function.acsch(x)
Compute the inverse hyperbolic cosecant of x
.
Base.Math.acoth
— Function.acoth(x)
Compute the inverse hyperbolic cotangent of x
.
Base.Math.sinc
— Function.sinc(x)
Compute $\sin(\pi x) / (\pi x)$ if $x \neq 0$, and $1$ if $x = 0$.
Base.Math.cosc
— Function.cosc(x)
Compute $\cos(\pi x) / x - \sin(\pi x) / (\pi x^2)$ if $x \neq 0$, and $0$ if $x = 0$. This is the derivative of sinc(x)
.
Base.Math.deg2rad
— Function.deg2rad(x)
Convert x
from degrees to radians.
julia> deg2rad(90)
1.5707963267948966
Base.Math.rad2deg
— Function.rad2deg(x)
Convert x
from radians to degrees.
julia> rad2deg(pi)
180.0
Base.Math.hypot
— Function.hypot(x, y)
Compute the hypotenuse $\sqrt{x^2+y^2}$ avoiding overflow and underflow.
Examples
julia> a = 10^10;
julia> hypot(a, a)
1.4142135623730951e10
julia> √(a^2 + a^2) # a^2 overflows
ERROR: DomainError:
sqrt will only return a complex result if called with a complex argument. Try sqrt(complex(x)).
Stacktrace:
[1] sqrt(::Int64) at ./math.jl:434
hypot(x...)
Compute the hypotenuse $\sqrt{\sum x_i^2}$ avoiding overflow and underflow.
Base.log
— Method.log(x)
Compute the natural logarithm of x
. Throws DomainError
for negative Real
arguments. Use complex negative arguments to obtain complex results.
There is an experimental variant in the Base.Math.JuliaLibm
module, which is typically faster and more accurate.
Base.log
— Method.log(b,x)
Compute the base b
logarithm of x
. Throws DomainError
for negative Real
arguments.
julia> log(4,8)
1.5
julia> log(4,2)
0.5
Base.log2
— Function.log2(x)
Compute the logarithm of x
to base 2. Throws DomainError
for negative Real
arguments.
Example
julia> log2(4)
2.0
julia> log2(10)
3.321928094887362
Base.log10
— Function.log10(x)
Compute the logarithm of x
to base 10. Throws DomainError
for negative Real
arguments.
Example
julia> log10(100)
2.0
julia> log10(2)
0.3010299956639812
Base.log1p
— Function.log1p(x)
Accurate natural logarithm of 1+x
. Throws DomainError
for Real
arguments less than -1.
There is an experimental variant in the Base.Math.JuliaLibm
module, which is typically faster and more accurate.
Examples
julia> log1p(-0.5)
-0.6931471805599453
julia> log1p(0)
0.0
Base.Math.frexp
— Function.frexp(val)
Return (x,exp)
such that x
has a magnitude in the interval $[1/2, 1)$ or 0, and val
is equal to $x \times 2^{exp}$.
Base.exp
— Function.exp(x)
Compute the natural base exponential of x
, in other words $e^x$.
Base.exp2
— Function.exp2(x)
Compute $2^x$.
julia> exp2(5)
32.0
Base.exp10
— Function.exp10(x)
Compute $10^x$.
Examples
julia> exp10(2)
100.0
julia> exp10(0.2)
1.5848931924611136
Base.Math.ldexp
— Function.ldexp(x, n)
Compute $x \times 2^n$.
Example
julia> ldexp(5., 2)
20.0
Base.Math.modf
— Function.modf(x)
Return a tuple (fpart,ipart) of the fractional and integral parts of a number. Both parts have the same sign as the argument.
Example
julia> modf(3.5)
(0.5, 3.0)
Base.expm1
— Function.expm1(x)
Accurately compute $e^x-1$.
Base.round
— Method.round([T,] x, [digits, [base]], [r::RoundingMode])
Rounds x
to an integer value according to the provided RoundingMode
, returning a value of the same type as x
. When not specifying a rounding mode the global mode will be used (see rounding
), which by default is round to the nearest integer (RoundNearest
mode), with ties (fractional values of 0.5) being rounded to the nearest even integer.
julia> round(1.7)
2.0
julia> round(1.5)
2.0
julia> round(2.5)
2.0
The optional RoundingMode
argument will change how the number gets rounded.
round(T, x, [r::RoundingMode])
converts the result to type T
, throwing an InexactError
if the value is not representable.
round(x, digits)
rounds to the specified number of digits after the decimal place (or before if negative). round(x, digits, base)
rounds using a base other than 10.
julia> round(pi, 2)
3.14
julia> round(pi, 3, 2)
3.125
Rounding to specified digits in bases other than 2 can be inexact when operating on binary floating point numbers. For example, the Float64
value represented by 1.15
is actually less than 1.15, yet will be rounded to 1.2.
julia> x = 1.15
1.15
julia> @sprintf "%.20f" x
"1.14999999999999991118"
julia> x < 115//100
true
julia> round(x, 1)
1.2
Base.Rounding.RoundingMode
— Type.RoundingMode
A type used for controlling the rounding mode of floating point operations (via rounding
/setrounding
functions), or as optional arguments for rounding to the nearest integer (via the round
function).
Currently supported rounding modes are:
RoundNearest
(default)RoundFromZero
(BigFloat
only)
Base.Rounding.RoundNearest
— Constant.RoundNearest
The default rounding mode. Rounds to the nearest integer, with ties (fractional values of 0.5) being rounded to the nearest even integer.
Base.Rounding.RoundNearestTiesAway
— Constant.RoundNearestTiesAway
Rounds to nearest integer, with ties rounded away from zero (C/C++ round
behaviour).
Base.Rounding.RoundNearestTiesUp
— Constant.RoundNearestTiesUp
Rounds to nearest integer, with ties rounded toward positive infinity (Java/JavaScript round
behaviour).
Base.Rounding.RoundToZero
— Constant.Base.Rounding.RoundUp
— Constant.Base.Rounding.RoundDown
— Constant.Base.round
— Method.round(z, RoundingModeReal, RoundingModeImaginary)
Returns the nearest integral value of the same type as the complex-valued z
to z
, breaking ties using the specified RoundingMode
s. The first RoundingMode
is used for rounding the real components while the second is used for rounding the imaginary components.
Base.ceil
— Function.ceil([T,] x, [digits, [base]])
ceil(x)
returns the nearest integral value of the same type as x
that is greater than or equal to x
.
ceil(T, x)
converts the result to type T
, throwing an InexactError
if the value is not representable.
digits
and base
work as for round
.
Base.floor
— Function.floor([T,] x, [digits, [base]])
floor(x)
returns the nearest integral value of the same type as x
that is less than or equal to x
.
floor(T, x)
converts the result to type T
, throwing an InexactError
if the value is not representable.
digits
and base
work as for round
.
Base.trunc
— Function.trunc([T,] x, [digits, [base]])
trunc(x)
returns the nearest integral value of the same type as x
whose absolute value is less than or equal to x
.
trunc(T, x)
converts the result to type T
, throwing an InexactError
if the value is not representable.
digits
and base
work as for round
.
Base.unsafe_trunc
— Function.unsafe_trunc(T, x)
unsafe_trunc(T, x)
returns the nearest integral value of type T
whose absolute value is less than or equal to x
. If the value is not representable by T
, an arbitrary value will be returned.
Base.signif
— Function.signif(x, digits, [base])
Rounds (in the sense of round
) x
so that there are digits
significant digits, under a base base
representation, default 10. E.g., signif(123.456, 2)
is 120.0
, and signif(357.913, 4, 2)
is 352.0
.
Base.min
— Function.min(x, y, ...)
Return the minimum of the arguments. See also the minimum
function to take the minimum element from a collection.
julia> min(2, 5, 1)
1
Base.max
— Function.max(x, y, ...)
Return the maximum of the arguments. See also the maximum
function to take the maximum element from a collection.
julia> max(2, 5, 1)
5
Base.minmax
— Function.minmax(x, y)
Return (min(x,y), max(x,y))
. See also: extrema
that returns (minimum(x), maximum(x))
.
julia> minmax('c','b')
('b', 'c')
Base.Math.clamp
— Function.clamp(x, lo, hi)
Return x
if lo <= x <= hi
. If x < lo
, return lo
. If x > hi
, return hi
. Arguments are promoted to a common type.
julia> clamp.([pi, 1.0, big(10.)], 2., 9.)
3-element Array{BigFloat,1}:
3.141592653589793238462643383279502884197169399375105820974944592307816406286198
2.000000000000000000000000000000000000000000000000000000000000000000000000000000
9.000000000000000000000000000000000000000000000000000000000000000000000000000000
Base.Math.clamp!
— Function.clamp!(array::AbstractArray, lo, hi)
Restrict values in array
to the specified range, in-place. See also clamp
.
Base.abs
— Function.abs(x)
The absolute value of x
.
When abs
is applied to signed integers, overflow may occur, resulting in the return of a negative value. This overflow occurs only when abs
is applied to the minimum representable value of a signed integer. That is, when x == typemin(typeof(x))
, abs(x) == x < 0
, not -x
as might be expected.
julia> abs(-3)
3
julia> abs(1 + im)
1.4142135623730951
julia> abs(typemin(Int64))
-9223372036854775808
Base.Checked.checked_abs
— Function.Base.checked_abs(x)
Calculates abs(x)
, checking for overflow errors where applicable. For example, standard two's complement signed integers (e.g. Int
) cannot represent abs(typemin(Int))
, thus leading to an overflow.
The overflow protection may impose a perceptible performance penalty.
Base.Checked.checked_neg
— Function.Base.checked_neg(x)
Calculates -x
, checking for overflow errors where applicable. For example, standard two's complement signed integers (e.g. Int
) cannot represent -typemin(Int)
, thus leading to an overflow.
The overflow protection may impose a perceptible performance penalty.
Base.Checked.checked_add
— Function.Base.checked_add(x, y)
Calculates x+y
, checking for overflow errors where applicable.
The overflow protection may impose a perceptible performance penalty.
Base.Checked.checked_sub
— Function.Base.checked_sub(x, y)
Calculates x-y
, checking for overflow errors where applicable.
The overflow protection may impose a perceptible performance penalty.
Base.Checked.checked_mul
— Function.Base.checked_mul(x, y)
Calculates x*y
, checking for overflow errors where applicable.
The overflow protection may impose a perceptible performance penalty.
Base.Checked.checked_div
— Function.Base.checked_div(x, y)
Calculates div(x,y)
, checking for overflow errors where applicable.
The overflow protection may impose a perceptible performance penalty.
Base.Checked.checked_rem
— Function.Base.checked_rem(x, y)
Calculates x%y
, checking for overflow errors where applicable.
The overflow protection may impose a perceptible performance penalty.
Base.Checked.checked_fld
— Function.Base.checked_fld(x, y)
Calculates fld(x,y)
, checking for overflow errors where applicable.
The overflow protection may impose a perceptible performance penalty.
Base.Checked.checked_mod
— Function.Base.checked_mod(x, y)
Calculates mod(x,y)
, checking for overflow errors where applicable.
The overflow protection may impose a perceptible performance penalty.
Base.Checked.checked_cld
— Function.Base.checked_cld(x, y)
Calculates cld(x,y)
, checking for overflow errors where applicable.
The overflow protection may impose a perceptible performance penalty.
Base.Checked.add_with_overflow
— Function.Base.add_with_overflow(x, y) -> (r, f)
Calculates r = x+y
, with the flag f
indicating whether overflow has occurred.
Base.Checked.sub_with_overflow
— Function.Base.sub_with_overflow(x, y) -> (r, f)
Calculates r = x-y
, with the flag f
indicating whether overflow has occurred.
Base.Checked.mul_with_overflow
— Function.Base.mul_with_overflow(x, y) -> (r, f)
Calculates r = x*y
, with the flag f
indicating whether overflow has occurred.
Base.abs2
— Function.abs2(x)
Squared absolute value of x
.
julia> abs2(-3)
9
Base.copysign
— Function.copysign(x, y) -> z
Return z
which has the magnitude of x
and the same sign as y
.
Examples
julia> copysign(1, -2)
-1
julia> copysign(-1, 2)
1
Base.sign
— Function.sign(x)
Return zero if x==0
and $x/|x|$ otherwise (i.e., ±1 for real x
).
Base.signbit
— Function.signbit(x)
Returns true
if the value of the sign of x
is negative, otherwise false
.
Examples
julia> signbit(-4)
true
julia> signbit(5)
false
julia> signbit(5.5)
false
julia> signbit(-4.1)
true
Base.flipsign
— Function.flipsign(x, y)
Return x
with its sign flipped if y
is negative. For example abs(x) = flipsign(x,x)
.
julia> flipsign(5, 3)
5
julia> flipsign(5, -3)
-5
Base.sqrt
— Function.sqrt(x)
Return $\sqrt{x}$. Throws DomainError
for negative Real
arguments. Use complex negative arguments instead. The prefix operator √
is equivalent to sqrt
.
Base.isqrt
— Function.isqrt(n::Integer)
Integer square root: the largest integer m
such that m*m <= n
.
julia> isqrt(5)
2
Base.Math.cbrt
— Function.cbrt(x::Real)
Return the cube root of x
, i.e. $x^{1/3}$. Negative values are accepted (returning the negative real root when $x < 0$).
The prefix operator ∛
is equivalent to cbrt
.
julia> cbrt(big(27))
3.000000000000000000000000000000000000000000000000000000000000000000000000000000
Base.real
— Method.real(z)
Return the real part of the complex number z
.
julia> real(1 + 3im)
1
Base.imag
— Function.imag(z)
Return the imaginary part of the complex number z
.
julia> imag(1 + 3im)
3
Base.reim
— Function.reim(z)
Return both the real and imaginary parts of the complex number z
.
julia> reim(1 + 3im)
(1, 3)
Base.conj
— Function.conj(z)
Compute the complex conjugate of a complex number z
.
julia> conj(1 + 3im)
1 - 3im
conj(v::RowVector)
Returns a ConjArray
lazy view of the input, where each element is conjugated.
Example
julia> v = [1+im, 1-im].'
1×2 RowVector{Complex{Int64},Array{Complex{Int64},1}}:
1+1im 1-1im
julia> conj(v)
1×2 RowVector{Complex{Int64},ConjArray{Complex{Int64},1,Array{Complex{Int64},1}}}:
1-1im 1+1im
Base.angle
— Function.angle(z)
Compute the phase angle in radians of a complex number z
.
Base.cis
— Function.cis(z)
Return $\exp(iz)$.
Base.binomial
— Function.binomial(n, k)
Number of ways to choose k
out of n
items.
Example
julia> binomial(5, 3)
10
julia> factorial(5) ÷ (factorial(5-3) * factorial(3))
10
Base.factorial
— Function.factorial(n)
Factorial of n
. If n
is an Integer
, the factorial is computed as an integer (promoted to at least 64 bits). Note that this may overflow if n
is not small, but you can use factorial(big(n))
to compute the result exactly in arbitrary precision. If n
is not an Integer
, factorial(n)
is equivalent to gamma(n+1)
.
julia> factorial(6)
720
julia> factorial(21)
ERROR: OverflowError()
[...]
julia> factorial(21.0)
5.109094217170944e19
julia> factorial(big(21))
51090942171709440000
Base.gcd
— Function.gcd(x,y)
Greatest common (positive) divisor (or zero if x
and y
are both zero).
Examples
julia> gcd(6,9)
3
julia> gcd(6,-9)
3
Base.lcm
— Function.lcm(x,y)
Least common (non-negative) multiple.
Examples
julia> lcm(2,3)
6
julia> lcm(-2,3)
6
Base.gcdx
— Function.gcdx(x,y)
Computes the greatest common (positive) divisor of x
and y
and their Bézout coefficients, i.e. the integer coefficients u
and v
that satisfy $ux+vy = d = gcd(x,y)$. $gcdx(x,y)$ returns $(d,u,v)$.
Examples
julia> gcdx(12, 42)
(6, -3, 1)
julia> gcdx(240, 46)
(2, -9, 47)
Bézout coefficients are not uniquely defined. gcdx
returns the minimal Bézout coefficients that are computed by the extended Euclidean algorithm. (Ref: D. Knuth, TAoCP, 2/e, p. 325, Algorithm X.) For signed integers, these coefficients u
and v
are minimal in the sense that $|u| < |y/d|$ and $|v| < |x/d|$. Furthermore, the signs of u
and v
are chosen so that d
is positive. For unsigned integers, the coefficients u
and v
might be near their typemax
, and the identity then holds only via the unsigned integers' modulo arithmetic.
Base.ispow2
— Function.ispow2(n::Integer) -> Bool
Test whether n
is a power of two.
Examples
julia> ispow2(4)
true
julia> ispow2(5)
false
Base.nextpow2
— Function.nextpow2(n::Integer)
The smallest power of two not less than n
. Returns 0 for n==0
, and returns -nextpow2(-n)
for negative arguments.
Examples
julia> nextpow2(16)
16
julia> nextpow2(17)
32
Base.prevpow2
— Function.prevpow2(n::Integer)
The largest power of two not greater than n
. Returns 0 for n==0
, and returns -prevpow2(-n)
for negative arguments.
Examples
julia> prevpow2(5)
4
julia> prevpow2(0)
0
Base.nextpow
— Function.nextpow(a, x)
The smallest a^n
not less than x
, where n
is a non-negative integer. a
must be greater than 1, and x
must be greater than 0.
Examples
julia> nextpow(2, 7)
8
julia> nextpow(2, 9)
16
julia> nextpow(5, 20)
25
julia> nextpow(4, 16)
16
See also prevpow
.
Base.prevpow
— Function.prevpow(a, x)
The largest a^n
not greater than x
, where n
is a non-negative integer. a
must be greater than 1, and x
must not be less than 1.
Examples
julia> prevpow(2, 7)
4
julia> prevpow(2, 9)
8
julia> prevpow(5, 20)
5
julia> prevpow(4, 16)
16
See also nextpow
.
Base.nextprod
— Function.nextprod([k_1, k_2,...], n)
Next integer greater than or equal to n
that can be written as $\prod k_i^{p_i}$ for integers $p_1$, $p_2$, etc.
Example
julia> nextprod([2, 3], 105)
108
julia> 2^2 * 3^3
108
Base.invmod
— Function.invmod(x,m)
Take the inverse of x
modulo m
: y
such that $x y = 1 \pmod m$, with $div(x,y) = 0$. This is undefined for $m = 0$, or if $gcd(x,m) \neq 1$.
Examples
julia> invmod(2,5)
3
julia> invmod(2,3)
2
julia> invmod(5,6)
5
Base.powermod
— Function.powermod(x::Integer, p::Integer, m)
Compute $x^p \pmod m$.
Examples
julia> powermod(2, 6, 5)
4
julia> mod(2^6, 5)
4
julia> powermod(5, 2, 20)
5
julia> powermod(5, 2, 19)
6
julia> powermod(5, 3, 19)
11
Base.Math.gamma
— Function.gamma(x)
Compute the gamma function of x
.
Base.Math.lgamma
— Function.lgamma(x)
Compute the logarithm of the absolute value of gamma
for Real
x
, while for Complex
x
compute the principal branch cut of the logarithm of gamma(x)
(defined for negative real(x)
by analytic continuation from positive real(x)
).
Base.Math.lfact
— Function.lfact(x)
Compute the logarithmic factorial of a nonnegative integer x
. Equivalent to lgamma
of x + 1
, but lgamma
extends this function to non-integer x
.
Base.Math.beta
— Function.beta(x, y)
Euler integral of the first kind $\operatorname{B}(x,y) = \Gamma(x)\Gamma(y)/\Gamma(x+y)$.
Base.Math.lbeta
— Function.lbeta(x, y)
Natural logarithm of the absolute value of the beta
function $\log(|\operatorname{B}(x,y)|)$.
Base.ndigits
— Function.ndigits(n::Integer, b::Integer=10)
Compute the number of digits in integer n
written in base b
. The base b
must not be in [-1, 0, 1]
.
Examples
julia> ndigits(12345)
5
julia> ndigits(1022, 16)
3
julia> base(16, 1022)
"3fe"
Base.widemul
— Function.widemul(x, y)
Multiply x
and y
, giving the result as a larger type.
julia> widemul(Float32(3.), 4.)
1.200000000000000000000000000000000000000000000000000000000000000000000000000000e+01
Base.Math.@evalpoly
— Macro.@evalpoly(z, c...)
Evaluate the polynomial $\sum_k c[k] z^{k-1}$ for the coefficients c[1]
, c[2]
, ...; that is, the coefficients are given in ascending order by power of z
. This macro expands to efficient inline code that uses either Horner's method or, for complex z
, a more efficient Goertzel-like algorithm.
julia> @evalpoly(3, 1, 0, 1)
10
julia> @evalpoly(2, 1, 0, 1)
5
julia> @evalpoly(2, 1, 1, 1)
7
Statistics
Base.mean
— Function.mean(f::Function, v)
Apply the function f
to each element of v
and take the mean.
julia> mean(√, [1, 2, 3])
1.3820881233139908
julia> mean([√1, √2, √3])
1.3820881233139908
mean(v[, region])
Compute the mean of whole array v
, or optionally along the dimensions in region
.
Julia does not ignore NaN
values in the computation. For applications requiring the handling of missing data, the DataArrays.jl
package is recommended.
Base.mean!
— Function.mean!(r, v)
Compute the mean of v
over the singleton dimensions of r
, and write results to r
.
Base.std
— Function.std(v[, region]; corrected::Bool=true, mean=nothing)
Compute the sample standard deviation of a vector or array v
, optionally along dimensions in region
. The algorithm returns an estimator of the generative distribution's standard deviation under the assumption that each entry of v
is an IID drawn from that generative distribution. This computation is equivalent to calculating sqrt(sum((v - mean(v)).^2) / (length(v) - 1))
. A pre-computed mean
may be provided. If corrected
is true
, then the sum is scaled with n-1
, whereas the sum is scaled with n
if corrected
is false
where n = length(x)
.
Julia does not ignore NaN
values in the computation. For applications requiring the handling of missing data, the DataArrays.jl
package is recommended.
Base.stdm
— Function.stdm(v, m::Number; corrected::Bool=true)
Compute the sample standard deviation of a vector v
with known mean m
. If corrected
is true
, then the sum is scaled with n-1
, whereas the sum is scaled with n
if corrected
is false
where n = length(x)
.
Julia does not ignore NaN
values in the computation. For applications requiring the handling of missing data, the DataArrays.jl
package is recommended.
Base.var
— Function.var(v[, region]; corrected::Bool=true, mean=nothing)
Compute the sample variance of a vector or array v
, optionally along dimensions in region
. The algorithm will return an estimator of the generative distribution's variance under the assumption that each entry of v
is an IID drawn from that generative distribution. This computation is equivalent to calculating sum(abs2, v - mean(v)) / (length(v) - 1)
. If corrected
is true
, then the sum is scaled with n-1
, whereas the sum is scaled with n
if corrected
is false
where n = length(x)
. The mean mean
over the region may be provided.
Julia does not ignore NaN
values in the computation. For applications requiring the handling of missing data, the DataArrays.jl
package is recommended.
Base.varm
— Function.varm(v, m[, region]; corrected::Bool=true)
Compute the sample variance of a collection v
with known mean(s) m
, optionally over region
. m
may contain means for each dimension of v
. If corrected
is true
, then the sum is scaled with n-1
, whereas the sum is scaled with n
if corrected
is false
where n = length(x)
.
Julia does not ignore NaN
values in the computation. For applications requiring the handling of missing data, the DataArrays.jl
package is recommended.
Base.middle
— Function.middle(x)
Compute the middle of a scalar value, which is equivalent to x
itself, but of the type of middle(x, x)
for consistency.
middle(x, y)
Compute the middle of two reals x
and y
, which is equivalent in both value and type to computing their mean ((x + y) / 2
).
middle(range)
Compute the middle of a range, which consists of computing the mean of its extrema. Since a range is sorted, the mean is performed with the first and last element.
julia> middle(1:10)
5.5
middle(a)
Compute the middle of an array a
, which consists of finding its extrema and then computing their mean.
julia> a = [1,2,3.6,10.9]
4-element Array{Float64,1}:
1.0
2.0
3.6
10.9
julia> middle(a)
5.95
Base.median
— Function.median(v[, region])
Compute the median of an entire array v
, or, optionally, along the dimensions in region
. For an even number of elements no exact median element exists, so the result is equivalent to calculating mean of two median elements.
Julia does not ignore NaN
values in the computation. For applications requiring the handling of missing data, the DataArrays.jl
package is recommended.
Base.median!
— Function.median!(v)
Like median
, but may overwrite the input vector.
Base.quantile
— Function.quantile(v, p; sorted=false)
Compute the quantile(s) of a vector v
at a specified probability or vector p
. The keyword argument sorted
indicates whether v
can be assumed to be sorted.
The p
should be on the interval [0,1], and v
should not have any NaN
values.
Quantiles are computed via linear interpolation between the points ((k-1)/(n-1), v[k])
, for k = 1:n
where n = length(v)
. This corresponds to Definition 7 of Hyndman and Fan (1996), and is the same as the R default.
Julia does not ignore NaN
values in the computation. For applications requiring the handling of missing data, the DataArrays.jl
package is recommended. quantile
will throw an ArgumentError
in the presence of NaN
values in the data array.
Hyndman, R.J and Fan, Y. (1996) "Sample Quantiles in Statistical Packages", The American Statistician, Vol. 50, No. 4, pp. 361-365
Base.quantile!
— Function.quantile!([q, ] v, p; sorted=false)
Compute the quantile(s) of a vector v
at the probabilities p
, with optional output into array q
(if not provided, a new output array is created). The keyword argument sorted
indicates whether v
can be assumed to be sorted; if false
(the default), then the elements of v
may be partially sorted.
The elements of p
should be on the interval [0,1], and v
should not have any NaN
values.
Quantiles are computed via linear interpolation between the points ((k-1)/(n-1), v[k])
, for k = 1:n
where n = length(v)
. This corresponds to Definition 7 of Hyndman and Fan (1996), and is the same as the R default.
Julia does not ignore NaN
values in the computation. For applications requiring the handling of missing data, the DataArrays.jl
package is recommended. quantile!
will throw an ArgumentError
in the presence of NaN
values in the data array.
Hyndman, R.J and Fan, Y. (1996) "Sample Quantiles in Statistical Packages", The American Statistician, Vol. 50, No. 4, pp. 361-365
Base.cov
— Function.cov(x[, corrected=true])
Compute the variance of the vector x
. If corrected
is true
(the default) then the sum is scaled with n-1
, whereas the sum is scaled with n
if corrected
is false
where n = length(x)
.
cov(X[, vardim=1, corrected=true])
Compute the covariance matrix of the matrix X
along the dimension vardim
. If corrected
is true
(the default) then the sum is scaled with n-1
, whereas the sum is scaled with n
if corrected
is false
where n = size(X, vardim)
.
cov(x, y[, corrected=true])
Compute the covariance between the vectors x
and y
. If corrected
is true
(the default), computes $\frac{1}{n-1}\sum_{i=1}^n (x_i-\bar x) (y_i-\bar y)^*$ where $*$ denotes the complex conjugate and n = length(x) = length(y)
. If corrected
is false
, computes $rac{1}{n}sum_{i=1}^n (x_i-\bar x) (y_i-\bar y)^*$.
cov(X, Y[, vardim=1, corrected=true])
Compute the covariance between the vectors or matrices X
and Y
along the dimension vardim
. If corrected
is true
(the default) then the sum is scaled with n-1
, whereas the sum is scaled with n
if corrected
is false
where n = size(X, vardim) = size(Y, vardim)
.
Base.cor
— Function.cor(x)
Return the number one.
cor(X[, vardim=1])
Compute the Pearson correlation matrix of the matrix X
along the dimension vardim
.
cor(x, y)
Compute the Pearson correlation between the vectors x
and y
.
cor(X, Y[, vardim=1])
Compute the Pearson correlation between the vectors or matrices X
and Y
along the dimension vardim
.
Signal Processing
Fast Fourier transform (FFT) functions in Julia are implemented by calling functions from FFTW.
Base.DFT.fft
— Function.fft(A [, dims])
Performs a multidimensional FFT of the array A
. The optional dims
argument specifies an iterable subset of dimensions (e.g. an integer, range, tuple, or array) to transform along. Most efficient if the size of A
along the transformed dimensions is a product of small primes; see nextprod()
. See also plan_fft()
for even greater efficiency.
A one-dimensional FFT computes the one-dimensional discrete Fourier transform (DFT) as defined by
A multidimensional FFT simply performs this operation along each transformed dimension of A
.
Julia starts FFTW up with 1 thread by default. Higher performance is usually possible by increasing number of threads. Use
FFTW.set_num_threads(Sys.CPU_CORES)
to use as many threads as cores on your system.This performs a multidimensional FFT by default. FFT libraries in other languages such as Python and Octave perform a one-dimensional FFT along the first non-singleton dimension of the array. This is worth noting while performing comparisons. For more details, refer to the Noteworthy Differences from other Languages section of the manual.
Base.DFT.fft!
— Function.fft!(A [, dims])
Same as fft
, but operates in-place on A
, which must be an array of complex floating-point numbers.
Base.DFT.ifft
— Function.ifft(A [, dims])
Multidimensional inverse FFT.
A one-dimensional inverse FFT computes
A multidimensional inverse FFT simply performs this operation along each transformed dimension of A
.
Base.DFT.ifft!
— Function.ifft!(A [, dims])
Same as ifft
, but operates in-place on A
.
Base.DFT.bfft
— Function.bfft(A [, dims])
Similar to ifft
, but computes an unnormalized inverse (backward) transform, which must be divided by the product of the sizes of the transformed dimensions in order to obtain the inverse. (This is slightly more efficient than ifft
because it omits a scaling step, which in some applications can be combined with other computational steps elsewhere.)
Base.DFT.bfft!
— Function.bfft!(A [, dims])
Same as bfft
, but operates in-place on A
.
Base.DFT.plan_fft
— Function.plan_fft(A [, dims]; flags=FFTW.ESTIMATE; timelimit=Inf)
Pre-plan an optimized FFT along given dimensions (dims
) of arrays matching the shape and type of A
. (The first two arguments have the same meaning as for fft
.) Returns an object P
which represents the linear operator computed by the FFT, and which contains all of the information needed to compute fft(A, dims)
quickly.
To apply P
to an array A
, use P * A
; in general, the syntax for applying plans is much like that of matrices. (A plan can only be applied to arrays of the same size as the A
for which the plan was created.) You can also apply a plan with a preallocated output array Â
by calling A_mul_B!(Â, plan, A)
. (For A_mul_B!
, however, the input array A
must be a complex floating-point array like the output Â
.) You can compute the inverse-transform plan by inv(P)
and apply the inverse plan with P \ Â
(the inverse plan is cached and reused for subsequent calls to inv
or \
), and apply the inverse plan to a pre-allocated output array A
with A_ldiv_B!(A, P, Â)
.
The flags
argument is a bitwise-or of FFTW planner flags, defaulting to FFTW.ESTIMATE
. e.g. passing FFTW.MEASURE
or FFTW.PATIENT
will instead spend several seconds (or more) benchmarking different possible FFT algorithms and picking the fastest one; see the FFTW manual for more information on planner flags. The optional timelimit
argument specifies a rough upper bound on the allowed planning time, in seconds. Passing FFTW.MEASURE
or FFTW.PATIENT
may cause the input array A
to be overwritten with zeros during plan creation.
plan_fft!
is the same as plan_fft
but creates a plan that operates in-place on its argument (which must be an array of complex floating-point numbers). plan_ifft
and so on are similar but produce plans that perform the equivalent of the inverse transforms ifft
and so on.
Base.DFT.plan_ifft
— Function.plan_ifft(A [, dims]; flags=FFTW.ESTIMATE; timelimit=Inf)
Same as plan_fft
, but produces a plan that performs inverse transforms ifft
.
Base.DFT.plan_bfft
— Function.plan_bfft(A [, dims]; flags=FFTW.ESTIMATE; timelimit=Inf)
Same as plan_fft
, but produces a plan that performs an unnormalized backwards transform bfft
.
Base.DFT.plan_fft!
— Function.plan_fft!(A [, dims]; flags=FFTW.ESTIMATE; timelimit=Inf)
Same as plan_fft
, but operates in-place on A
.
Base.DFT.plan_ifft!
— Function.plan_ifft!(A [, dims]; flags=FFTW.ESTIMATE; timelimit=Inf)
Same as plan_ifft
, but operates in-place on A
.
Base.DFT.plan_bfft!
— Function.plan_bfft!(A [, dims]; flags=FFTW.ESTIMATE; timelimit=Inf)
Same as plan_bfft
, but operates in-place on A
.
Base.DFT.rfft
— Function.rfft(A [, dims])
Multidimensional FFT of a real array A
, exploiting the fact that the transform has conjugate symmetry in order to save roughly half the computational time and storage costs compared with fft
. If A
has size (n_1, ..., n_d)
, the result has size (div(n_1,2)+1, ..., n_d)
.
The optional dims
argument specifies an iterable subset of one or more dimensions of A
to transform, similar to fft
. Instead of (roughly) halving the first dimension of A
in the result, the dims[1]
dimension is (roughly) halved in the same way.
Base.DFT.irfft
— Function.irfft(A, d [, dims])
Inverse of rfft
: for a complex array A
, gives the corresponding real array whose FFT yields A
in the first half. As for rfft
, dims
is an optional subset of dimensions to transform, defaulting to 1:ndims(A)
.
d
is the length of the transformed real array along the dims[1]
dimension, which must satisfy div(d,2)+1 == size(A,dims[1])
. (This parameter cannot be inferred from size(A)
since both 2*size(A,dims[1])-2
as well as 2*size(A,dims[1])-1
are valid sizes for the transformed real array.)
Base.DFT.brfft
— Function.brfft(A, d [, dims])
Similar to irfft
but computes an unnormalized inverse transform (similar to bfft
), which must be divided by the product of the sizes of the transformed dimensions (of the real output array) in order to obtain the inverse transform.
Base.DFT.plan_rfft
— Function.plan_rfft(A [, dims]; flags=FFTW.ESTIMATE; timelimit=Inf)
Pre-plan an optimized real-input FFT, similar to plan_fft
except for rfft
instead of fft
. The first two arguments, and the size of the transformed result, are the same as for rfft
.
Base.DFT.plan_brfft
— Function.plan_brfft(A, d [, dims]; flags=FFTW.ESTIMATE; timelimit=Inf)
Pre-plan an optimized real-input unnormalized transform, similar to plan_rfft
except for brfft
instead of rfft
. The first two arguments and the size of the transformed result, are the same as for brfft
.
Base.DFT.plan_irfft
— Function.plan_irfft(A, d [, dims]; flags=FFTW.ESTIMATE; timelimit=Inf)
Pre-plan an optimized inverse real-input FFT, similar to plan_rfft
except for irfft
and brfft
, respectively. The first three arguments have the same meaning as for irfft
.
Base.DFT.FFTW.dct
— Function.dct(A [, dims])
Performs a multidimensional type-II discrete cosine transform (DCT) of the array A
, using the unitary normalization of the DCT. The optional dims
argument specifies an iterable subset of dimensions (e.g. an integer, range, tuple, or array) to transform along. Most efficient if the size of A
along the transformed dimensions is a product of small primes; see nextprod
. See also plan_dct
for even greater efficiency.
Base.DFT.FFTW.dct!
— Function.dct!(A [, dims])
Same as dct!
, except that it operates in-place on A
, which must be an array of real or complex floating-point values.
Base.DFT.FFTW.idct
— Function.idct(A [, dims])
Computes the multidimensional inverse discrete cosine transform (DCT) of the array A
(technically, a type-III DCT with the unitary normalization). The optional dims
argument specifies an iterable subset of dimensions (e.g. an integer, range, tuple, or array) to transform along. Most efficient if the size of A
along the transformed dimensions is a product of small primes; see nextprod
. See also plan_idct
for even greater efficiency.
Base.DFT.FFTW.idct!
— Function.idct!(A [, dims])
Same as idct!
, but operates in-place on A
.
Base.DFT.FFTW.plan_dct
— Function.plan_dct(A [, dims [, flags [, timelimit]]])
Pre-plan an optimized discrete cosine transform (DCT), similar to plan_fft
except producing a function that computes dct
. The first two arguments have the same meaning as for dct
.
Base.DFT.FFTW.plan_dct!
— Function.plan_dct!(A [, dims [, flags [, timelimit]]])
Same as plan_dct
, but operates in-place on A
.
Base.DFT.FFTW.plan_idct
— Function.plan_idct(A [, dims [, flags [, timelimit]]])
Pre-plan an optimized inverse discrete cosine transform (DCT), similar to plan_fft
except producing a function that computes idct
. The first two arguments have the same meaning as for idct
.
Base.DFT.FFTW.plan_idct!
— Function.plan_idct!(A [, dims [, flags [, timelimit]]])
Same as plan_idct
, but operates in-place on A
.
Base.DFT.fftshift
— Method.fftshift(x)
Swap the first and second halves of each dimension of x
.
Base.DFT.fftshift
— Method.fftshift(x,dim)
Swap the first and second halves of the given dimension or iterable of dimensions of array x
.
Base.DFT.ifftshift
— Function.ifftshift(x, [dim])
Undoes the effect of fftshift
.
Base.DSP.filt
— Function.filt(b, a, x, [si])
Apply filter described by vectors a
and b
to vector x
, with an optional initial filter state vector si
(defaults to zeros).
Base.DSP.filt!
— Function.filt!(out, b, a, x, [si])
Same as filt
but writes the result into the out
argument, which may alias the input x
to modify it in-place.
Base.DSP.deconv
— Function.deconv(b,a) -> c
Construct vector c
such that b = conv(a,c) + r
. Equivalent to polynomial division.
Base.DSP.conv
— Function.conv(u,v)
Convolution of two vectors. Uses FFT algorithm.
Base.DSP.conv2
— Function.conv2(u,v,A)
2-D convolution of the matrix A
with the 2-D separable kernel generated by the vectors u
and v
. Uses 2-D FFT algorithm.
conv2(B,A)
2-D convolution of the matrix B
with the matrix A
. Uses 2-D FFT algorithm.
Base.DSP.xcorr
— Function.xcorr(u,v)
Compute the cross-correlation of two vectors.
The following functions are defined within the Base.FFTW
module.
Base.DFT.FFTW.r2r
— Function.r2r(A, kind [, dims])
Performs a multidimensional real-input/real-output (r2r) transform of type kind
of the array A
, as defined in the FFTW manual. kind
specifies either a discrete cosine transform of various types (FFTW.REDFT00
, FFTW.REDFT01
, FFTW.REDFT10
, or FFTW.REDFT11
), a discrete sine transform of various types (FFTW.RODFT00
, FFTW.RODFT01
, FFTW.RODFT10
, or FFTW.RODFT11
), a real-input DFT with halfcomplex-format output (FFTW.R2HC
and its inverse FFTW.HC2R
), or a discrete Hartley transform (FFTW.DHT
). The kind
argument may be an array or tuple in order to specify different transform types along the different dimensions of A
; kind[end]
is used for any unspecified dimensions. See the FFTW manual for precise definitions of these transform types, at http://www.fftw.org/doc.
The optional dims
argument specifies an iterable subset of dimensions (e.g. an integer, range, tuple, or array) to transform along. kind[i]
is then the transform type for dims[i]
, with kind[end]
being used for i > length(kind)
.
See also plan_r2r
to pre-plan optimized r2r transforms.
Base.DFT.FFTW.r2r!
— Function.r2r!(A, kind [, dims])
Same as r2r
, but operates in-place on A
, which must be an array of real or complex floating-point numbers.
Base.DFT.FFTW.plan_r2r
— Function.plan_r2r(A, kind [, dims [, flags [, timelimit]]])
Pre-plan an optimized r2r transform, similar to plan_fft
except that the transforms (and the first three arguments) correspond to r2r
and r2r!
, respectively.
Base.DFT.FFTW.plan_r2r!
— Function.