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Find All Solutions to Cos2x 0

arcsin, arccos, arctan, etc

In mathematics, the inverse trigonometric functions (occasionally also called arcus functions,[1] [2] [3] [4] [5] antitrigonometric functions [6] or cyclometric functions [7] [8] [9]) are the inverse functions of the trigonometric functions (with suitably restricted domains). Specifically, they are the inverses of the sine, cosine, tangent, cotangent, secant, and cosecant functions,[10] and are used to obtain an angle from any of the angle's trigonometric ratios. Inverse trigonometric functions are widely used in engineering, navigation, physics, and geometry.

Notation [edit]

Several notations for the inverse trigonometric functions exist. The most common convention is to name inverse trigonometric functions using an arc- prefix: arcsin(x), arccos(x), arctan(x), etc.[6] (This convention is used throughout this article.) This notation arises from the following geometric relationships:[ citation needed ] when measuring in radians, an angle of θ radians will correspond to an arc whose length is , where r is the radius of the circle. Thus in the unit circle, "the arc whose cosine is x" is the same as "the angle whose cosine is x", because the length of the arc of the circle in radii is the same as the measurement of the angle in radians.[11] In computer programming languages, the inverse trigonometric functions are often called by the abbreviated forms asin, acos, atan.[12]

The notations sin−1(x), cos−1(x), tan−1(x), etc., as introduced by John Herschel in 1813,[13] [14] are often used as well in English-language sources[6]—conventions consistent with the notation of an inverse function. This might appear to conflict logically with the common semantics for expressions such as sin2(x), which refer to numeric power rather than function composition, and therefore may result in confusion between multiplicative inverse or reciprocal and compositional inverse.[15] The confusion is somewhat mitigated by the fact that each of the reciprocal trigonometric functions has its own name—for example, (cos(x))−1 = sec(x). Nevertheless, certain authors advise against using it for its ambiguity.[6] [16] Another convention used by a few authors is to use an uppercase first letter, along with a −1 superscript: Sin−1(x), Cos−1(x), Tan−1(x), etc.[17] This potentially avoids confusion with the multiplicative inverse, which should be represented by sin−1(x), cos−1(x), etc.

Since 2009, the ISO 80000-2 standard has specified solely the "arc" prefix for the inverse functions.

Basic concepts [edit]

Principal values [edit]

Since none of the six trigonometric functions are one-to-one, they must be restricted in order to have inverse functions. Therefore, the result ranges of the inverse functions are proper (i.e. strict) subsets of the domains of the original functions.

For example, using function in the sense of multivalued functions, just as the square root function y = x {\displaystyle y={\sqrt {x}}} could be defined from y 2 = x , {\displaystyle y^{2}=x,} the function y = arcsin ( x ) {\displaystyle y=\arcsin(x)} is defined so that sin ( y ) = x . {\displaystyle \sin(y)=x.} For a given real number x , {\displaystyle x,} with 1 x 1 , {\displaystyle -1\leq x\leq 1,} there are multiple (in fact, countably infinite) numbers y {\displaystyle y} such that sin ( y ) = x {\displaystyle \sin(y)=x} ; for example, sin ( 0 ) = 0 , {\displaystyle \sin(0)=0,} but also sin ( π ) = 0 , {\displaystyle \sin(\pi )=0,} sin ( 2 π ) = 0 , {\displaystyle \sin(2\pi )=0,} etc. When only one value is desired, the function may be restricted to its principal branch. With this restriction, for each x {\displaystyle x} in the domain, the expression arcsin ( x ) {\displaystyle \arcsin(x)} will evaluate only to a single value, called its principal value. These properties apply to all the inverse trigonometric functions.

The principal inverses are listed in the following table.

Name Usual notation Definition Domain of x {\displaystyle x} for real result Range of usual principal value
(radians)
Range of usual principal value
(degrees)
arcsine y = arcsin ( x ) {\displaystyle y=\arcsin(x)} x = sin(y) 1 x 1 {\displaystyle -1\leq x\leq 1} π 2 y π 2 {\displaystyle -{\frac {\pi }{2}}\leq y\leq {\frac {\pi }{2}}} 90 y 90 {\displaystyle -90^{\circ }\leq y\leq 90^{\circ }}
arccosine y = arccos ( x ) {\displaystyle y=\arccos(x)} x = cos(y) 1 x 1 {\displaystyle -1\leq x\leq 1} 0 y π {\displaystyle 0\leq y\leq \pi } 0 y 180 {\displaystyle 0^{\circ }\leq y\leq 180^{\circ }}
arctangent y = arctan ( x ) {\displaystyle y=\arctan(x)} x = tan(y) all real numbers π 2 < y < π 2 {\displaystyle -{\frac {\pi }{2}}<y<{\frac {\pi }{2}}} 90 < y < 90 {\displaystyle -90^{\circ }<y<90^{\circ }}
arccotangent y = arccot ( x ) {\displaystyle y=\operatorname {arccot}(x)} x = cot(y) all real numbers 0 < y < π {\displaystyle 0<y<\pi } 0 < y < 180 {\displaystyle 0^{\circ }<y<180^{\circ }}
arcsecant y = arcsec ( x ) {\displaystyle y=\operatorname {arcsec}(x)} x = sec(y) x 1  or x 1 {\displaystyle x\leq -1{\text{ or }}x\geq 1} 0 y < π 2  or π 2 < y π {\displaystyle 0\leq y<{\frac {\pi }{2}}{\text{ or }}{\frac {\pi }{2}}<y\leq \pi } 0 y < 90  or 90 < y 180 {\displaystyle 0^{\circ }\leq y<90^{\circ }{\text{ or }}90^{\circ }<y\leq 180^{\circ }}
arccosecant y = arccsc ( x ) {\displaystyle y=\operatorname {arccsc}(x)} x = csc(y) x 1  or x 1 {\displaystyle x\leq -1{\text{ or }}x\geq 1} π 2 y < 0  or 0 < y π 2 {\displaystyle -{\frac {\pi }{2}}\leq y<0{\text{ or }}0<y\leq {\frac {\pi }{2}}} 90 y < 0  or 0 < y 90 {\displaystyle -90^{\circ }\leq y<0^{\circ }{\text{ or }}0^{\circ }<y\leq 90^{\circ }}

Note: Some authors[ citation needed ] define the range of arcsecant to be ( 0 y < π 2  or π y < 3 π 2 ) {\textstyle (0\leq y<{\frac {\pi }{2}}{\text{ or }}\pi \leq y<{\frac {3\pi }{2}})} , because the tangent function is nonnegative on this domain. This makes some computations more consistent. For example, using this range, tan ( arcsec ( x ) ) = x 2 1 , {\displaystyle \tan(\operatorname {arcsec}(x))={\sqrt {x^{2}-1}},} whereas with the range ( 0 y < π 2  or π 2 < y π ) {\textstyle (0\leq y<{\frac {\pi }{2}}{\text{ or }}{\frac {\pi }{2}}<y\leq \pi )} , we would have to write tan ( arcsec ( x ) ) = ± x 2 1 , {\displaystyle \tan(\operatorname {arcsec}(x))=\pm {\sqrt {x^{2}-1}},} since tangent is nonnegative on 0 y < π 2 , {\textstyle 0\leq y<{\frac {\pi }{2}},} but nonpositive on π 2 < y π . {\textstyle {\frac {\pi }{2}}<y\leq \pi .} For a similar reason, the same authors define the range of arccosecant to be ( π < y π 2 {\textstyle (-\pi <y\leq -{\frac {\pi }{2}}} or 0 < y π 2 ) . {\textstyle 0<y\leq {\frac {\pi }{2}}).}

If x {\displaystyle x} is allowed to be a complex number, then the range of y {\displaystyle y} applies only to its real part.

The table below displays names and domains of the inverse trigonometric functions along with the range of their usual principal values in radians.

Name
Symbol Domain Image/Range Inverse
function
Domain Image of
principal values
sine sin {\displaystyle \sin } : {\displaystyle :} R {\displaystyle \mathbb {R} } {\displaystyle \to } [ 1 , 1 ] {\displaystyle [-1,1]} arcsin {\displaystyle \arcsin } : {\displaystyle :} [ 1 , 1 ] {\displaystyle [-1,1]} {\displaystyle \to } [ π 2 , π 2 ] {\displaystyle \left[-{\tfrac {\pi }{2}},{\tfrac {\pi }{2}}\right]}
cosine cos {\displaystyle \cos } : {\displaystyle :} R {\displaystyle \mathbb {R} } {\displaystyle \to } [ 1 , 1 ] {\displaystyle [-1,1]} arccos {\displaystyle \arccos } : {\displaystyle :} [ 1 , 1 ] {\displaystyle [-1,1]} {\displaystyle \to } [ 0 , π ] {\displaystyle [0,\pi ]}
tangent tan {\displaystyle \tan } : {\displaystyle :} π Z + ( π 2 , π 2 ) {\displaystyle \pi \mathbb {Z} +\left(-{\tfrac {\pi }{2}},{\tfrac {\pi }{2}}\right)} {\displaystyle \to } R {\displaystyle \mathbb {R} } arctan {\displaystyle \arctan } : {\displaystyle :} R {\displaystyle \mathbb {R} } {\displaystyle \to } ( π 2 , π 2 ) {\displaystyle \left(-{\tfrac {\pi }{2}},{\tfrac {\pi }{2}}\right)}
cotangent cot {\displaystyle \cot } : {\displaystyle :} π Z + ( 0 , π ) {\displaystyle \pi \mathbb {Z} +(0,\pi )} {\displaystyle \to } R {\displaystyle \mathbb {R} } arccot {\displaystyle \operatorname {arccot} } : {\displaystyle :} R {\displaystyle \mathbb {R} } {\displaystyle \to } ( 0 , π ) {\displaystyle (0,\pi )}
secant sec {\displaystyle \sec } : {\displaystyle :} π Z + ( π 2 , π 2 ) {\displaystyle \pi \mathbb {Z} +\left(-{\tfrac {\pi }{2}},{\tfrac {\pi }{2}}\right)} {\displaystyle \to } R ( 1 , 1 ) = ( , 1 ] [ 1 , ) {\displaystyle \mathbb {R} \setminus (-1,1)=(-\infty ,-1]\cup [1,\infty )} arcsec {\displaystyle \operatorname {arcsec} } : {\displaystyle :} R ( 1 , 1 ) {\displaystyle \mathbb {R} \setminus (-1,1)} {\displaystyle \to } [ 0 , π ] { π 2 } {\displaystyle [\,0,\;\pi \,]\;\;\;\setminus \left\{{\tfrac {\pi }{2}}\right\}}
cosecant csc {\displaystyle \csc } : {\displaystyle :} π Z + ( 0 , π ) {\displaystyle \pi \mathbb {Z} +(0,\pi )} {\displaystyle \to } R ( 1 , 1 ) {\displaystyle \mathbb {R} \setminus (-1,1)} arccsc {\displaystyle \operatorname {arccsc} } : {\displaystyle :} R ( 1 , 1 ) {\displaystyle \mathbb {R} \setminus (-1,1)} {\displaystyle \to } [ π 2 , π 2 ] { 0 } {\displaystyle \left[-{\tfrac {\pi }{2}},{\tfrac {\pi }{2}}\right]\setminus \{0\}}

The symbol R = ( , ) {\displaystyle \mathbb {R} =(-\infty ,\infty )} denotes the set of all real numbers and Z = { , 2 , 1 , 0 , 1 , 2 , } {\displaystyle \mathbb {Z} =\{\ldots ,\,-2,\,-1,\,0,\,1,\,2,\,\ldots \}} denotes the set of all integers. The set of all integer multiples of π {\displaystyle \pi } is denoted by

π Z := { π n : n Z } = { , 3 π 2 π , π , 0 , π , 2 π , 3 π , 4 π , } = { θ R : sin θ = 0 } . {\displaystyle \pi \mathbb {Z} ~:=~\{\pi n\;:\;n\in \mathbb {Z} \}~=~\{\ldots ,\,-3\pi \,-2\pi ,\,-\pi ,\,0,\,\pi ,\,2\pi ,\,3\pi ,\,4\pi ,\,\ldots \}~=~\{\theta \in \mathbb {R} \;:\;\sin \theta =0\}.}

The symbol {\displaystyle \,\setminus \,} denotes set subtraction so that, for instance, R ( 1 , 1 ) {\displaystyle \mathbb {R} \setminus (-1,1)} is the set of points in R {\displaystyle \mathbb {R} } (that is, real numbers) that are not in the interval ( 1 , 1 ) , {\displaystyle (-1,1),} which in this case is equal to the set of all points in the two intervals ( , 1 ] [ 1 , ) . {\displaystyle (-\infty ,-1]\cup [1,\infty ).} Similarly, [ 0 , π ] { π 2 } {\displaystyle [0,\pi ]\setminus \left\{{\tfrac {\pi }{2}}\right\}} is the set of all points in the interval [ 0 , π ] {\displaystyle [0,\pi ]} that are not equal to π 2 {\displaystyle {\tfrac {\pi }{2}}} while [ π 2 , π 2 ] { 0 } {\displaystyle \left[-{\tfrac {\pi }{2}},{\tfrac {\pi }{2}}\right]\setminus \{0\}} is the set of all points in [ π 2 , π 2 ] {\displaystyle \left[-{\tfrac {\pi }{2}},{\tfrac {\pi }{2}}\right]} that are not equal to 0 , {\displaystyle 0,} which can be written in terms of intervals as

[ π 2 , π 2 ] { 0 } = [ π 2 , 0 ) ( 0 , π 2 ]  and [ 0 , π ] { π 2 } = [ 0 , π 2 ) ( π 2 , π ] . {\displaystyle \left[-{\tfrac {\pi }{2}},{\tfrac {\pi }{2}}\right]\setminus \{0\}=\left[-{\tfrac {\pi }{2}},0\right)\cup \left(0,{\tfrac {\pi }{2}}\right]\qquad {\text{ and }}\qquad [0,\pi ]\setminus \left\{{\tfrac {\pi }{2}}\right\}=\left[0,{\tfrac {\pi }{2}}\,\right)\cup \left({\tfrac {\pi }{2}},\pi \right].}

The Minkowski sum notation π Z + ( 0 , π ) {\textstyle \pi \mathbb {Z} +(0,\pi )} and π Z + ( π 2 , π 2 ) {\displaystyle \pi \mathbb {Z} +\left(-{\frac {\pi }{2}},{\frac {\pi }{2}}\right)} that is used above to concisely write the domains of cot , csc , tan ,  and sec {\displaystyle \cot ,\csc ,\tan ,{\text{ and }}\sec } is now explained.

Domain of cotangent cot {\displaystyle \cot } and cosecant csc {\displaystyle \csc } : The domains of cot {\displaystyle \,\cot \,} and csc {\displaystyle \,\csc \,} are the same. They are the set of all angles θ {\displaystyle \theta } at which sin θ 0 , {\displaystyle \sin \theta \neq 0,} which can also be written as

π Z + ( 0 , π ) = ( 3 π , 2 π ) ( 2 π , π ) ( π , 0 ) ( 0 , π ) ( π , 2 π ) ( 2 π , 3 π ) ( 3 π , 4 π ) = R π Z . {\displaystyle {\begin{alignedat}{4}\pi \mathbb {Z} +(0,\pi )&~=~\cdots \cup (-3\pi ,-2\pi )\cup (-2\pi ,-\pi )\cup (-\pi ,0)\cup (0,\pi )\cup (\pi ,2\pi )\cup (2\pi ,3\pi )\cup (3\pi ,4\pi )\cup \cdots \\&~=~\mathbb {R} \setminus \pi \mathbb {Z} .\\\end{alignedat}}}

In other words, the domain of cot {\displaystyle \,\cot \,} and csc {\displaystyle \,\csc \,} is the set R π Z {\displaystyle \mathbb {R} \setminus \pi \mathbb {Z} } of all real numbers that are not of the form π n {\displaystyle \pi n} for some integer n . {\displaystyle n.} These points not in the domain (meaning π n {\displaystyle \pi n} for n {\displaystyle n} an integer) are exactly those numbers θ {\displaystyle \theta } at which 0 = sin θ ; {\displaystyle 0=\sin \theta ;} this is because these are also exactly the θ {\displaystyle \theta } at which cot θ = cos θ sin θ {\textstyle \cot \theta ={\frac {\cos \theta }{\sin \theta }}} and csc θ = 1 sin θ {\textstyle \csc \theta ={\frac {1}{\sin \theta }}} would be divided by 0. {\displaystyle 0.}

Domain of tangent tan {\displaystyle \tan } and secant sec {\displaystyle \sec } : The domains of tan {\displaystyle \,\tan \,} and sec {\displaystyle \,\sec \,} are the same. They are the set of all angles θ {\displaystyle \theta } at which cos θ 0 , {\displaystyle \cos \theta \neq 0,} which can also be written as

π Z + ( π 2 , π 2 ) = ( 5 π 2 , 3 π 2 ) ( 3 π 2 , π 2 ) ( π 2 , π 2 ) ( π 2 , 3 π 2 ) ( 3 π 2 , 5 π 2 ) ( 5 π 2 , 7 π 2 ) = R ( π 2 + π Z ) {\displaystyle {\begin{alignedat}{4}\pi \mathbb {Z} +\left(-{\tfrac {\pi }{2}},{\tfrac {\pi }{2}}\right)&~=~\cdots \cup \left(-{\tfrac {5\pi }{2}},-{\tfrac {3\pi }{2}}\right)\cup \left(-{\tfrac {3\pi }{2}},-{\tfrac {\pi }{2}}\right)\cup \left(-{\tfrac {\pi }{2}},{\tfrac {\pi }{2}}\right)\cup \left({\tfrac {\pi }{2}},{\tfrac {3\pi }{2}}\right)\cup \left({\tfrac {3\pi }{2}},{\tfrac {5\pi }{2}}\right)\cup \left({\tfrac {5\pi }{2}},{\tfrac {7\pi }{2}}\right)\cup \cdots \\&~=~\mathbb {R} \setminus \left({\tfrac {\pi }{2}}+\pi \mathbb {Z} \right)\\\end{alignedat}}}

where R ( π 2 + π Z ) {\textstyle \mathbb {R} \setminus \left({\tfrac {\pi }{2}}+\pi \mathbb {Z} \right)} is the set of all real numbers that do not belong to the set

π 2 + π Z : = { π 2 + π n : n Z } = { , π 2 3 π , π 2 2 π , π 2 π , π 2 , π 2 + π , π 2 + 2 π , π 2 + 3 π , } = { , 5 π 2 , 3 π 2 , π 2 , π 2 , 3 π 2 , 5 π 2 , 7 π 2 , } = { θ R : cos θ = 0 } . {\displaystyle {\begin{alignedat}{4}{\tfrac {\pi }{2}}+\pi \mathbb {Z} ~:&=~\left\{{\tfrac {\pi }{2}}+\pi n:n\in \mathbb {Z} \right\}\\[0.3ex]~&=~\left\{\ldots ,\,{\tfrac {\pi }{2}}-3\pi ,\,~~{\tfrac {\pi }{2}}-2\pi ,\,\,~\,~{\tfrac {\pi }{2}}-\pi ,\,~~{\tfrac {\pi }{2}},\,~\,~{\tfrac {\pi }{2}}+\pi ,\,~\,\,~\,{\tfrac {\pi }{2}}+2\pi ,\,~\,\,\,\,{\tfrac {\pi }{2}}+3\pi ,\,\ldots \right\}\\[0.6ex]~&=~\left\{\ldots ,~~\,~-{\tfrac {5\pi }{2}},~~\,~~\;-{\tfrac {3\pi }{2}},~\,~~\,~~-{\tfrac {\pi }{2}},\,~~{\tfrac {\pi }{2}},~~\,~~\,~~\;{\tfrac {3\pi }{2}},~~\,~~\,~~\;~~\,~{\tfrac {5\pi }{2}},~\,~~\,~~\,~~\,~~{\tfrac {7\pi }{2}},\,\ldots \right\}\\[0.6ex]~&=~\{\theta \in \mathbb {R} \;:\;\cos \theta =0\}.\\[0.3ex]\end{alignedat}}}

In other words, the domain of tan {\displaystyle \,\tan \,} and sec {\displaystyle \,\sec \,} is the set of all real numbers that are not of the form π 2 + π n = π + 2 π n 2 = π ( 1 + 2 n ) 2 {\textstyle {\tfrac {\pi }{2}}+\pi n={\tfrac {\pi +2\pi n}{2}}={\tfrac {\pi (1+2n)}{2}}} for some integer n ; {\displaystyle n;} this is also the set of all numbers that are not of the form o 2 π {\textstyle {\tfrac {o}{2}}\pi } for some odd integer o . {\displaystyle o.} These points not in the domain (meaning π 2 + π n {\textstyle {\tfrac {\pi }{2}}+\pi n} for n {\displaystyle n} an integer) are exactly those numbers θ {\displaystyle \theta } at which 0 = cos θ ; {\displaystyle 0=\cos \theta ;} this is because these are also exactly the θ {\displaystyle \theta } at which tan θ = sin θ cos θ {\textstyle \tan \theta ={\frac {\sin \theta }{\cos \theta }}} and sec θ = 1 cos θ {\textstyle \sec \theta ={\frac {1}{\cos \theta }}} would be divided by 0. {\displaystyle 0.}

Solutions to elementary trigonometric equations [edit]

Each of the trigonometric functions is periodic in the real part of its argument, running through all its values twice in each interval of 2 π {\displaystyle 2\pi } :

  • Sine and cosecant begin their period at 2 π k π 2 {\textstyle 2\pi k-{\frac {\pi }{2}}} (where k {\displaystyle k} is an integer), finish it at 2 π k + π 2 , {\textstyle 2\pi k+{\frac {\pi }{2}},} and then reverse themselves over 2 π k + π 2 , {\textstyle 2\pi k+{\frac {\pi }{2}},} to 2 π k + 3 π 2 . {\displaystyle 2\pi k+{\frac {3\pi }{2}}.}
  • Cosine and secant begin their period at 2 π k , {\displaystyle 2\pi k,} finish it at 2 π k + π . {\displaystyle 2\pi k+\pi .} and then reverse themselves over 2 π k + π {\displaystyle 2\pi k+\pi } to 2 π k + 2 π . {\displaystyle 2\pi k+2\pi .}
  • Tangent begins its period at 2 π k π 2 , {\textstyle 2\pi k-{\frac {\pi }{2}},} finishes it at 2 π k + π 2 , {\textstyle 2\pi k+{\frac {\pi }{2}},} and then repeats it (forward) over 2 π k + π 2 {\textstyle 2\pi k+{\frac {\pi }{2}}} to 2 π k + 3 π 2 . {\textstyle 2\pi k+{\frac {3\pi }{2}}.}
  • Cotangent begins its period at 2 π k , {\displaystyle 2\pi k,} finishes it at 2 π k + π , {\displaystyle 2\pi k+\pi ,} and then repeats it (forward) over 2 π k + π {\displaystyle 2\pi k+\pi } to 2 π k + 2 π . {\displaystyle 2\pi k+2\pi .}

This periodicity is reflected in the general inverses, where k {\displaystyle k} is some integer.

The following table shows how inverse trigonometric functions may be used to solve equalities involving the six standard trigonometric functions. It is assumed that the given values θ , {\displaystyle \theta ,} r , {\displaystyle r,} s , {\displaystyle s,} x , {\displaystyle x,} and y {\displaystyle y} all lie within appropriate ranges so that the relevant expressions below are well-defined. Note that "for some k Z {\displaystyle k\in \mathbb {Z} } " is just another way of saying "for some integer k . {\displaystyle k.} "

The symbol {\displaystyle \,\iff \,} is logical equality. The expression "LHS {\displaystyle \,\iff \,} RHS" indicates that either (a) the left hand side (i.e. LHS) and right hand side (i.e. RHS) are both true, or else (b) the left hand side and right hand side are both false; there is no option (c) (e.g. it is not possible for the LHS statement to be true and also simultaneously for the RHS statement to false), because otherwise "LHS {\displaystyle \,\iff \,} RHS" would not have been written (see this footnote[note 1] for an example illustrating this concept).

Equation if and only if Solution Expanded form of solution where...
sin θ = y {\displaystyle \sin \theta =y} {\displaystyle \iff } θ = {\displaystyle \theta =\,} ( 1 ) k {\displaystyle (-1)^{k}} arcsin ( y ) {\displaystyle \arcsin(y)} + {\displaystyle +} π k {\displaystyle \pi k} for some k Z {\displaystyle k\in \mathbb {Z} } {\displaystyle \iff } θ = arcsin ( y ) + 2 π h {\displaystyle \theta =\;\;\;\,\arcsin(y)+2\pi h} or
θ = arcsin ( y ) + 2 π h + π {\displaystyle \theta =-\arcsin(y)+2\pi h+\pi }
for some h Z {\displaystyle h\in \mathbb {Z} }
csc θ = r {\displaystyle \csc \theta =r} {\displaystyle \iff } θ = {\displaystyle \theta =\,} ( 1 ) k {\displaystyle (-1)^{k}} arccsc ( r ) {\displaystyle \operatorname {arccsc}(r)} + {\displaystyle +} π k {\displaystyle \pi k} for some k Z {\displaystyle k\in \mathbb {Z} } {\displaystyle \iff } θ = arccsc ( y ) + 2 π h {\displaystyle \theta =\;\;\;\,\operatorname {arccsc}(y)+2\pi h} or
θ = arccsc ( y ) + 2 π h + π {\displaystyle \theta =-\operatorname {arccsc}(y)+2\pi h+\pi }
for some h Z {\displaystyle h\in \mathbb {Z} }
cos θ = x {\displaystyle \cos \theta =x} {\displaystyle \iff } θ = {\displaystyle \theta =\,} ± {\displaystyle \pm \,} arccos ( x ) {\displaystyle \arccos(x)} + {\displaystyle +} 2 {\displaystyle 2} π k {\displaystyle \pi k} for some k Z {\displaystyle k\in \mathbb {Z} } {\displaystyle \iff } θ = arccos ( y ) + 2 π h {\displaystyle \theta =\;\;\;\,\arccos(y)+2\pi h} or
θ = arccos ( y ) + 2 π h {\displaystyle \theta =-\arccos(y)+2\pi h}
for some h Z {\displaystyle h\in \mathbb {Z} }
sec θ = r {\displaystyle \sec \theta =r} {\displaystyle \iff } θ = {\displaystyle \theta =\,} ± {\displaystyle \pm \,} arcsec ( r ) {\displaystyle \operatorname {arcsec}(r)} + {\displaystyle +} 2 {\displaystyle 2} π k {\displaystyle \pi k} for some k Z {\displaystyle k\in \mathbb {Z} } {\displaystyle \iff } θ = arcsec ( y ) + 2 π h {\displaystyle \theta =\;\;\;\,\operatorname {arcsec}(y)+2\pi h} or
θ = arcsec ( y ) + 2 π h {\displaystyle \theta =-\operatorname {arcsec}(y)+2\pi h}
for some h Z {\displaystyle h\in \mathbb {Z} }
tan θ = s {\displaystyle \tan \theta =s} {\displaystyle \iff } θ = {\displaystyle \theta =\,} arctan ( s ) {\displaystyle \arctan(s)} + {\displaystyle +} π k {\displaystyle \pi k} for some k Z {\displaystyle k\in \mathbb {Z} }
cot θ = r {\displaystyle \cot \theta =r} {\displaystyle \iff } θ = {\displaystyle \theta =\,} arccot ( r ) {\displaystyle \operatorname {arccot}(r)} + {\displaystyle +} π k {\displaystyle \pi k} for some k Z {\displaystyle k\in \mathbb {Z} }

For example, if cos θ = 1 {\displaystyle \cos \theta =-1} then θ = π + 2 π k = π + 2 π ( 1 + k ) {\displaystyle \theta =\pi +2\pi k=-\pi +2\pi (1+k)} for some k Z . {\displaystyle k\in \mathbb {Z} .} While if sin θ = ± 1 {\displaystyle \sin \theta =\pm 1} then θ = π 2 + π k = π 2 + π ( k + 1 ) {\textstyle \theta ={\frac {\pi }{2}}+\pi k=-{\frac {\pi }{2}}+\pi (k+1)} for some k Z , {\displaystyle k\in \mathbb {Z} ,} where k {\displaystyle k} will be even if sin θ = 1 {\displaystyle \sin \theta =1} and it will be odd if sin θ = 1. {\displaystyle \sin \theta =-1.} The equations sec θ = 1 {\displaystyle \sec \theta =-1} and csc θ = ± 1 {\displaystyle \csc \theta =\pm 1} have the same solutions as cos θ = 1 {\displaystyle \cos \theta =-1} and sin θ = ± 1 , {\displaystyle \sin \theta =\pm 1,} respectively. In all equations above except for those just solved (i.e. except for sin {\displaystyle \sin } / csc θ = ± 1 {\displaystyle \csc \theta =\pm 1} and cos {\displaystyle \cos } / sec θ = 1 {\displaystyle \sec \theta =-1} ), the integer k {\displaystyle k} in the solution's formula is uniquely determined by θ {\displaystyle \theta } (for fixed r , s , x , {\displaystyle r,s,x,} and y {\displaystyle y} ).

Detailed example and explanation of the "plus or minus" symbol ± {\displaystyle \pm }

The solutions to cos θ = x {\displaystyle \cos \theta =x} and sec θ = x {\displaystyle \sec \theta =x} involve the "plus or minus" symbol ± , {\displaystyle \,\pm ,\,} whose meaning is now clarified. Only the solution to cos θ = x {\displaystyle \cos \theta =x} will be discussed since the discussion for sec θ = x {\displaystyle \sec \theta =x} is the same. We are given x {\displaystyle x} between 1 x 1 {\displaystyle -1\leq x\leq 1} and we know that there is an angle θ {\displaystyle \theta } in some give interval that satisfies cos θ = x . {\displaystyle \cos \theta =x.} We want to find this θ . {\displaystyle \theta .} The formula for the solution involves:

± arccos x . {\displaystyle \pm \arccos x.}

If arccos x = 0 {\displaystyle \,\arccos x=0\,} (which only happens when x = 1 {\displaystyle x=1} ) then + arccos x = 0 {\displaystyle \,+\arccos x=0\,} and arccos x = 0 {\displaystyle \,-\arccos x=0\,} so either way, ± arccos x {\displaystyle \,\pm \arccos x\,} can only be equal to 0. {\displaystyle 0.} But if arccos x 0 , {\displaystyle \,\arccos x\neq 0,\,} which will now be assumed, then the solution to cos θ = x , {\displaystyle \cos \theta =x,} which is written above as

θ = ± arccos x + 2 π k  for some k Z {\displaystyle \,\theta =\pm \arccos x+2\pi k\,\quad {\text{ for some }}k\in \mathbb {Z} }

is shorthand for the following statement:
Either

Because arccos x 0 {\displaystyle \,\arccos x\neq 0\,} and 0 < arccos x π {\displaystyle \,0<\arccos x\leq \pi \,} exactly one of these two equalities can hold. Additional information about θ {\displaystyle \theta } is needed to determine which one holds. For example, suppose that x = 0 {\displaystyle x=0} and that all that is known about θ {\displaystyle \theta } is that π θ π {\displaystyle \,-\pi \leq \theta \leq \pi \,} (and nothing more is known). Then

arccos x = arccos 0 = π 2 {\displaystyle \arccos x=\arccos 0={\frac {\pi }{2}}}

and moreover, in this particular case k = 0 {\displaystyle k=0} (for both the + {\displaystyle \,+\,} case and the {\displaystyle \,-\,} case) and so consequently,

θ = ± arccos x + 2 π k = ± ( π 2 ) + 2 π ( 0 ) = ± π 2 . {\displaystyle \theta ~=~\pm \arccos x+2\pi k~=~\pm \left({\frac {\pi }{2}}\right)+2\pi (0)~=~\pm {\frac {\pi }{2}}.}

This means that θ {\displaystyle \theta } could be either π / 2 {\displaystyle \,\pi /2\,} or π / 2. {\displaystyle \,-\pi /2.} Without additional information it is not possible to determine which of these values θ {\displaystyle \theta } has. An example of some additional information that could determine the value of θ {\displaystyle \theta } would be knowing that the angle is above the x {\displaystyle x} -axis(in which case θ = π / 2 {\displaystyle \theta =\pi /2} ) or alternatively, knowing that it is below the x {\displaystyle x} -axis(in which case θ = π / 2 {\displaystyle \theta =-\pi /2} ).

Transforming equations

The equations above can be transformed by using the reflection and shift identities:[18]

Argument: _ {\displaystyle {\underline {\;~~~~~~~~~~~~~~\;}}} = {\displaystyle =} θ {\displaystyle -\theta } π 2 ± θ {\displaystyle {\frac {\pi }{2}}\pm \theta } π ± θ {\displaystyle \pi \pm \theta } 3 π 2 ± θ {\displaystyle {\frac {3\pi }{2}}\pm \theta } 2 k π ± θ , where k Z {\displaystyle 2k\pi \pm \theta ,\;{\text{where }}k\in \mathbb {Z} }
sin _ {\displaystyle \sin {\underline {\;~~~~~~~~~~~~~~\;}}} = {\displaystyle =} {\displaystyle -} sin θ {\displaystyle \sin \theta } {\displaystyle } cos θ {\displaystyle \cos \theta } {\displaystyle \mp } sin θ {\displaystyle \sin \theta } {\displaystyle -} cos θ {\displaystyle \cos \theta } ± {\displaystyle \pm } sin θ {\displaystyle \sin \theta }
csc _ {\displaystyle \csc {\underline {\;~~~~~~~~~~~~~~\;}}} = {\displaystyle =} {\displaystyle -} csc θ {\displaystyle \csc \theta } {\displaystyle } sec θ {\displaystyle \sec \theta } {\displaystyle \mp } csc θ {\displaystyle \csc \theta } {\displaystyle -} sec θ {\displaystyle \sec \theta } ± {\displaystyle \pm } csc θ {\displaystyle \csc \theta }
cos _ {\displaystyle \cos {\underline {\;~~~~~~~~~~~~~~\;}}} = {\displaystyle =} {\displaystyle } cos θ {\displaystyle \cos \theta } {\displaystyle \mp } sin θ {\displaystyle \sin \theta } {\displaystyle -} cos θ {\displaystyle \cos \theta } ± {\displaystyle \pm } sin θ {\displaystyle \sin \theta } {\displaystyle } cos θ {\displaystyle \cos \theta }
sec _ {\displaystyle \sec {\underline {\;~~~~~~~~~~~~~~\;}}} = {\displaystyle =} {\displaystyle } sec θ {\displaystyle \sec \theta } {\displaystyle \mp } csc θ {\displaystyle \csc \theta } {\displaystyle -} sec θ {\displaystyle \sec \theta } ± {\displaystyle \pm } csc θ {\displaystyle \csc \theta } {\displaystyle } sec θ {\displaystyle \sec \theta }
tan _ {\displaystyle \tan {\underline {\;~~~~~~~~~~~~~~\;}}} = {\displaystyle =} {\displaystyle -} tan θ {\displaystyle \tan \theta } {\displaystyle \mp } cot θ {\displaystyle \cot \theta } ± {\displaystyle \pm } tan θ {\displaystyle \tan \theta } {\displaystyle \mp } cot θ {\displaystyle \cot \theta } ± {\displaystyle \pm } tan θ {\displaystyle \tan \theta }
cot _ {\displaystyle \cot {\underline {\;~~~~~~~~~~~~~~\;}}} = {\displaystyle =} {\displaystyle -} cot θ {\displaystyle \cot \theta } {\displaystyle \mp } tan θ {\displaystyle \tan \theta } ± {\displaystyle \pm } cot θ {\displaystyle \cot \theta } {\displaystyle \mp } tan θ {\displaystyle \tan \theta } ± {\displaystyle \pm } cot θ {\displaystyle \cot \theta }

These formulas imply, in particular, that the following hold:

sin θ = sin ( θ ) = sin ( π + θ ) = sin ( π θ ) = cos ( π 2 + θ ) = cos ( π 2 θ ) = cos ( π 2 θ ) = cos ( π 2 + θ ) = cos ( 3 π 2 θ ) = cos ( 3 π 2 + θ ) cos θ = cos ( θ ) = cos ( π + θ ) = cos ( π θ ) = sin ( π 2 + θ ) = sin ( π 2 θ ) = sin ( π 2 θ ) = sin ( π 2 + θ ) = sin ( 3 π 2 θ ) = sin ( 3 π 2 + θ ) tan θ = tan ( θ ) = tan ( π + θ ) = tan ( π θ ) = cot ( π 2 + θ ) = cot ( π 2 θ ) = cot ( π 2 θ ) = cot ( π 2 + θ ) = cot ( 3 π 2 θ ) = cot ( 3 π 2 + θ ) {\displaystyle {\begin{alignedat}{28}\sin \theta &=-&&\sin(-\theta )&&=-&&\sin(\pi +\theta )&&=&&\sin(\pi -\theta )&&=-&&\cos {\Big (}{\frac {\pi }{2}}+\theta {\Big )}&&=&&\cos {\Big (}{\frac {\pi }{2}}-\theta {\Big )}&&=-&&\cos {\Big (}-{\frac {\pi }{2}}-\theta {\Big )}&&=&&\cos {\Big (}-{\frac {\pi }{2}}+\theta {\Big )}&&=-&&\cos {\bigg (}{\frac {3\pi }{2}}-\theta {\bigg )}&&=-&&\cos {\bigg (}-{\frac {3\pi }{2}}+\theta {\bigg )}\\[0.3ex]\cos \theta &=&&\cos(-\theta )&&=-&&\cos(\pi +\theta )&&=&&\cos(\pi -\theta )&&=&&\sin {\Big (}{\frac {\pi }{2}}+\theta {\Big )}&&=&&\sin {\Big (}{\frac {\pi }{2}}-\theta {\Big )}&&=-&&\sin {\Big (}-{\frac {\pi }{2}}-\theta {\Big )}&&=-&&\sin {\Big (}-{\frac {\pi }{2}}+\theta {\Big )}&&=-&&\sin {\bigg (}{\frac {3\pi }{2}}-\theta {\bigg )}&&=&&\sin {\bigg (}-{\frac {3\pi }{2}}+\theta {\bigg )}\\[0.3ex]\tan \theta &=-&&\tan(-\theta )&&=&&\tan(\pi +\theta )&&=-&&\tan(\pi -\theta )&&=-&&\cot {\Big (}{\frac {\pi }{2}}+\theta {\Big )}&&=&&\cot {\Big (}{\frac {\pi }{2}}-\theta {\Big )}&&=&&\cot {\Big (}-{\frac {\pi }{2}}-\theta {\Big )}&&=-&&\cot {\Big (}-{\frac {\pi }{2}}+\theta {\Big )}&&=&&\cot {\bigg (}{\frac {3\pi }{2}}-\theta {\bigg )}&&=-&&\cot {\bigg (}-{\frac {3\pi }{2}}+\theta {\bigg )}\\[0.3ex]\end{alignedat}}}

where swapping sin csc , {\displaystyle \sin \leftrightarrow \csc ,} swapping cos sec , {\displaystyle \cos \leftrightarrow \sec ,} and swapping tan cot {\displaystyle \tan \leftrightarrow \cot } gives the analogous equations for csc , sec ,  and cot , {\displaystyle \csc ,\sec ,{\text{ and }}\cot ,} respectively.

So for example, by using the equality sin ( π 2 θ ) = cos θ , {\textstyle \sin \left({\frac {\pi }{2}}-\theta \right)=\cos \theta ,} the equation cos θ = x {\displaystyle \cos \theta =x} can be transformed into sin ( π 2 θ ) = x , {\textstyle \sin \left({\frac {\pi }{2}}-\theta \right)=x,} which allows for the solution to the equation sin φ = x {\displaystyle \;\sin \varphi =x\;} (where φ := π 2 θ {\textstyle \varphi :={\frac {\pi }{2}}-\theta } ) to be used; that solution being: φ = ( 1 ) k arcsin ( x ) + π k  for some k Z , {\displaystyle \varphi =(-1)^{k}\arcsin(x)+\pi k\;{\text{ for some }}k\in \mathbb {Z} ,} which becomes:

π 2 θ = ( 1 ) k arcsin ( x ) + π k  for some k Z {\displaystyle {\frac {\pi }{2}}-\theta ~=~(-1)^{k}\arcsin(x)+\pi k\quad {\text{ for some }}k\in \mathbb {Z} }

where using the fact that ( 1 ) k = ( 1 ) k {\displaystyle (-1)^{k}=(-1)^{-k}} and substituting h := k {\displaystyle h:=-k} proves that another solution to cos θ = x {\displaystyle \;\cos \theta =x\;} is:

θ = ( 1 ) h + 1 arcsin ( x ) + π h + π 2  for some h Z . {\displaystyle \theta ~=~(-1)^{h+1}\arcsin(x)+\pi h+{\frac {\pi }{2}}\quad {\text{ for some }}h\in \mathbb {Z} .}

The substitution arcsin x = π 2 arccos x {\displaystyle \;\arcsin x={\frac {\pi }{2}}-\arccos x\;} may be used express the right hand side of the above formula in terms of arccos x {\displaystyle \;\arccos x\;} instead of arcsin x . {\displaystyle \;\arcsin x.\;}

Equal identical trigonometric functions [edit]

The table below shows how two angles θ {\displaystyle \theta } and φ {\displaystyle \varphi } must be related if their values under a given trigonometric function are equal or negatives of each other.

Equation if and only if Solution where... Also a solution to
sin θ {\displaystyle \sin \theta } = {\displaystyle =} sin φ {\displaystyle \sin \varphi } {\displaystyle \iff } θ = {\displaystyle \theta =} ( 1 ) k {\displaystyle (-1)^{k}} φ {\displaystyle \varphi } + {\displaystyle +} π k {\displaystyle \pi k} for some k Z {\displaystyle k\in \mathbb {Z} } csc θ = csc φ {\displaystyle \csc \theta =\csc \varphi }
cos θ {\displaystyle \cos \theta } = {\displaystyle =} cos φ {\displaystyle \cos \varphi } {\displaystyle \iff } θ = {\displaystyle \theta =} ± {\displaystyle \pm \,} φ {\displaystyle \varphi } + {\displaystyle +} 2 {\displaystyle 2} π k {\displaystyle \pi k} for some k Z {\displaystyle k\in \mathbb {Z} } sec θ = sec φ {\displaystyle \sec \theta =\sec \varphi }
tan θ {\displaystyle \tan \theta } = {\displaystyle =} tan φ {\displaystyle \tan \varphi } {\displaystyle \iff } θ = {\displaystyle \theta =} φ {\displaystyle \varphi } + {\displaystyle +} π k {\displaystyle \pi k} for some k Z {\displaystyle k\in \mathbb {Z} } cot θ = cot φ {\displaystyle \cot \theta =\cot \varphi }
sin θ {\displaystyle -\sin \theta } = {\displaystyle =} sin φ {\displaystyle \sin \varphi } {\displaystyle \iff } θ = {\displaystyle \theta =} ( 1 ) k + 1 {\displaystyle (-1)^{k+1}} φ {\displaystyle \varphi } + {\displaystyle +} π k {\displaystyle \pi k} for some k Z {\displaystyle k\in \mathbb {Z} } csc θ = csc φ {\displaystyle -\csc \theta =\csc \varphi }
cos θ {\displaystyle -\cos \theta } = {\displaystyle =} cos φ {\displaystyle \cos \varphi } {\displaystyle \iff } θ = {\displaystyle \theta =} ± {\displaystyle \pm \,} φ {\displaystyle \varphi } + {\displaystyle +} 2 {\displaystyle 2} π k {\displaystyle \pi k} + π {\displaystyle +\,\;\pi } for some k Z {\displaystyle k\in \mathbb {Z} } sec θ = sec φ {\displaystyle -\sec \theta =\sec \varphi }
tan θ {\displaystyle -\tan \theta } = {\displaystyle =} tan φ {\displaystyle \tan \varphi } {\displaystyle \iff } θ = {\displaystyle \theta =} {\displaystyle -} φ {\displaystyle \varphi } + {\displaystyle +} π k {\displaystyle \pi k} for some k Z {\displaystyle k\in \mathbb {Z} } cot θ = cot φ {\displaystyle -\cot \theta =\cot \varphi }
| sin θ | {\displaystyle \left|\sin \theta \right|} = {\displaystyle =} | sin φ | {\displaystyle \left|\sin \varphi \right|} {\displaystyle \iff } θ = {\displaystyle \theta =} ± {\displaystyle \pm } φ {\displaystyle \varphi } + {\displaystyle +} π k {\displaystyle \pi k} for some k Z {\displaystyle k\in \mathbb {Z} } | tan θ | = | tan φ | | csc θ | = | csc φ | | sec θ | = | sec φ | | cot θ | = | cot φ | {\displaystyle {\begin{aligned}\left|\tan \theta \right|&=\left|\tan \varphi \right|\\\left|\csc \theta \right|&=\left|\csc \varphi \right|\\\left|\sec \theta \right|&=\left|\sec \varphi \right|\\\left|\cot \theta \right|&=\left|\cot \varphi \right|\end{aligned}}}
| cos θ | {\displaystyle \left|\cos \theta \right|} = {\displaystyle =} | cos φ | {\displaystyle \left|\cos \varphi \right|}

Relationships between trigonometric functions and inverse trigonometric functions [edit]

Trigonometric functions of inverse trigonometric functions are tabulated below. A quick way to derive them is by considering the geometry of a right-angled triangle, with one side of length 1 and another side of length x , {\displaystyle x,} then applying the Pythagorean theorem and definitions of the trigonometric ratios. Purely algebraic derivations are longer.[ citation needed ] It is worth noting that for arcsecant and arccosecant, the diagram assumes that x {\displaystyle x} is positive, and thus the result has to be corrected through the use of absolute values and the signum (sgn) operation.

θ {\displaystyle \theta } sin ( θ ) {\displaystyle \sin(\theta )} cos ( θ ) {\displaystyle \cos(\theta )} tan ( θ ) {\displaystyle \tan(\theta )} Diagram
arcsin ( x ) {\displaystyle \arcsin(x)} sin ( arcsin ( x ) ) = x {\displaystyle \sin(\arcsin(x))=x} cos ( arcsin ( x ) ) = 1 x 2 {\displaystyle \cos(\arcsin(x))={\sqrt {1-x^{2}}}} tan ( arcsin ( x ) ) = x 1 x 2 {\displaystyle \tan(\arcsin(x))={\frac {x}{\sqrt {1-x^{2}}}}} Trigonometric functions and inverse3.svg
arccos ( x ) {\displaystyle \arccos(x)} sin ( arccos ( x ) ) = 1 x 2 {\displaystyle \sin(\arccos(x))={\sqrt {1-x^{2}}}} cos ( arccos ( x ) ) = x {\displaystyle \cos(\arccos(x))=x} tan ( arccos ( x ) ) = 1 x 2 x {\displaystyle \tan(\arccos(x))={\frac {\sqrt {1-x^{2}}}{x}}} Trigonometric functions and inverse.svg
arctan ( x ) {\displaystyle \arctan(x)} sin ( arctan ( x ) ) = x 1 + x 2 {\displaystyle \sin(\arctan(x))={\frac {x}{\sqrt {1+x^{2}}}}} cos ( arctan ( x ) ) = 1 1 + x 2 {\displaystyle \cos(\arctan(x))={\frac {1}{\sqrt {1+x^{2}}}}} tan ( arctan ( x ) ) = x {\displaystyle \tan(\arctan(x))=x} Trigonometric functions and inverse2.svg
arccot ( x ) {\displaystyle \operatorname {arccot}(x)} sin ( arccot ( x ) ) = 1 1 + x 2 {\displaystyle \sin(\operatorname {arccot}(x))={\frac {1}{\sqrt {1+x^{2}}}}} cos ( arccot ( x ) ) = x 1 + x 2 {\displaystyle \cos(\operatorname {arccot}(x))={\frac {x}{\sqrt {1+x^{2}}}}} tan ( arccot ( x ) ) = 1 x {\displaystyle \tan(\operatorname {arccot}(x))={\frac {1}{x}}} Trigonometric functions and inverse4.svg
arcsec ( x ) {\displaystyle \operatorname {arcsec}(x)} sin ( arcsec ( x ) ) = x 2 1 | x | {\displaystyle \sin(\operatorname {arcsec}(x))={\frac {\sqrt {x^{2}-1}}{|x|}}} cos ( arcsec ( x ) ) = 1 x {\displaystyle \cos(\operatorname {arcsec}(x))={\frac {1}{x}}} tan ( arcsec ( x ) ) = sgn ( x ) x 2 1 {\displaystyle \tan(\operatorname {arcsec}(x))=\operatorname {sgn}(x){\sqrt {x^{2}-1}}} Trigonometric functions and inverse6.svg
arccsc ( x ) {\displaystyle \operatorname {arccsc}(x)} sin ( arccsc ( x ) ) = 1 x {\displaystyle \sin(\operatorname {arccsc}(x))={\frac {1}{x}}} cos ( arccsc ( x ) ) = x 2 1 | x | {\displaystyle \cos(\operatorname {arccsc}(x))={\frac {\sqrt {x^{2}-1}}{|x|}}} tan ( arccsc ( x ) ) = sgn ( x ) x 2 1 {\displaystyle \tan(\operatorname {arccsc}(x))={\frac {\operatorname {sgn}(x)}{\sqrt {x^{2}-1}}}} Trigonometric functions and inverse5.svg

Relationships among the inverse trigonometric functions [edit]

The usual principal values of the arcsin(x) (red) and arccos(x) (blue) functions graphed on the cartesian plane.

The usual principal values of the arctan(x) and arccot(x) functions graphed on the cartesian plane.

Principal values of the arcsec(x) and arccsc(x) functions graphed on the cartesian plane.

Complementary angles:

arccos ( x ) = π 2 arcsin ( x ) arccot ( x ) = π 2 arctan ( x ) arccsc ( x ) = π 2 arcsec ( x ) {\displaystyle {\begin{aligned}\arccos(x)&={\frac {\pi }{2}}-\arcsin(x)\\[0.5em]\operatorname {arccot}(x)&={\frac {\pi }{2}}-\arctan(x)\\[0.5em]\operatorname {arccsc}(x)&={\frac {\pi }{2}}-\operatorname {arcsec}(x)\end{aligned}}}

Negative arguments:

arcsin ( x ) = arcsin ( x ) arccos ( x ) = π arccos ( x ) arctan ( x ) = arctan ( x ) arccot ( x ) = π arccot ( x ) arcsec ( x ) = π arcsec ( x ) arccsc ( x ) = arccsc ( x ) {\displaystyle {\begin{aligned}\arcsin(-x)&=-\arcsin(x)\\\arccos(-x)&=\pi -\arccos(x)\\\arctan(-x)&=-\arctan(x)\\\operatorname {arccot}(-x)&=\pi -\operatorname {arccot}(x)\\\operatorname {arcsec}(-x)&=\pi -\operatorname {arcsec}(x)\\\operatorname {arccsc}(-x)&=-\operatorname {arccsc}(x)\end{aligned}}}

Reciprocal arguments:

arccos ( 1 x ) = arcsec ( x ) arcsin ( 1 x ) = arccsc ( x ) arctan ( 1 x ) = π 2 arctan ( x ) = arccot ( x ) ,  if x > 0 arctan ( 1 x ) = π 2 arctan ( x ) = arccot ( x ) π ,  if x < 0 arccot ( 1 x ) = π 2 arccot ( x ) = arctan ( x ) ,  if x > 0 arccot ( 1 x ) = 3 π 2 arccot ( x ) = π + arctan ( x ) ,  if x < 0 arcsec ( 1 x ) = arccos ( x ) arccsc ( 1 x ) = arcsin ( x ) {\displaystyle {\begin{aligned}\arccos \left({\frac {1}{x}}\right)&=\operatorname {arcsec}(x)\\[0.3em]\arcsin \left({\frac {1}{x}}\right)&=\operatorname {arccsc}(x)\\[0.3em]\arctan \left({\frac {1}{x}}\right)&={\frac {\pi }{2}}-\arctan(x)=\operatorname {arccot}(x)\,,{\text{ if }}x>0\\[0.3em]\arctan \left({\frac {1}{x}}\right)&=-{\frac {\pi }{2}}-\arctan(x)=\operatorname {arccot}(x)-\pi \,,{\text{ if }}x<0\\[0.3em]\operatorname {arccot} \left({\frac {1}{x}}\right)&={\frac {\pi }{2}}-\operatorname {arccot}(x)=\arctan(x)\,,{\text{ if }}x>0\\[0.3em]\operatorname {arccot} \left({\frac {1}{x}}\right)&={\frac {3\pi }{2}}-\operatorname {arccot}(x)=\pi +\arctan(x)\,,{\text{ if }}x<0\\[0.3em]\operatorname {arcsec} \left({\frac {1}{x}}\right)&=\arccos(x)\\[0.3em]\operatorname {arccsc} \left({\frac {1}{x}}\right)&=\arcsin(x)\end{aligned}}}

Useful identities if one only has a fragment of a sine table:

arccos ( x ) = arcsin ( 1 x 2 ) ,  if 0 x 1  , from which you get arccos ( 1 x 2 1 + x 2 ) = arcsin ( 2 x 1 + x 2 ) ,  if 0 x 1 arcsin ( 1 x 2 ) = π 2 sgn ( x ) arcsin ( x ) arccos ( x ) = 1 2 arccos ( 2 x 2 1 ) ,  if 0 x 1 arcsin ( x ) = 1 2 arccos ( 1 2 x 2 ) ,  if 0 x 1 arcsin ( x ) = arctan ( x 1 x 2 ) arccos ( x ) = arctan ( 1 x 2 x ) arctan ( x ) = arcsin ( x 1 + x 2 ) arccot ( x ) = arccos ( x 1 + x 2 ) {\displaystyle {\begin{aligned}\arccos(x)&=\arcsin \left({\sqrt {1-x^{2}}}\right)\,,{\text{ if }}0\leq x\leq 1{\text{ , from which you get }}\\\arccos &\left({\frac {1-x^{2}}{1+x^{2}}}\right)=\arcsin \left({\frac {2x}{1+x^{2}}}\right)\,,{\text{ if }}0\leq x\leq 1\\\arcsin &\left({\sqrt {1-x^{2}}}\right)={\frac {\pi }{2}}-\operatorname {sgn}(x)\arcsin(x)\\\arccos(x)&={\frac {1}{2}}\arccos \left(2x^{2}-1\right)\,,{\text{ if }}0\leq x\leq 1\\\arcsin(x)&={\frac {1}{2}}\arccos \left(1-2x^{2}\right)\,,{\text{ if }}0\leq x\leq 1\\\arcsin(x)&=\arctan \left({\frac {x}{\sqrt {1-x^{2}}}}\right)\\\arccos(x)&=\arctan \left({\frac {\sqrt {1-x^{2}}}{x}}\right)\\\arctan(x)&=\arcsin \left({\frac {x}{\sqrt {1+x^{2}}}}\right)\\\operatorname {arccot}(x)&=\arccos \left({\frac {x}{\sqrt {1+x^{2}}}}\right)\end{aligned}}}

Whenever the square root of a complex number is used here, we choose the root with the positive real part (or positive imaginary part if the square was negative real).

A useful form that follows directly from the table above is

arctan ( x ) = arccos ( 1 1 + x 2 ) ,  if x 0 {\displaystyle \arctan \left(x\right)=\arccos \left({\sqrt {\frac {1}{1+x^{2}}}}\right)\,,{\text{ if }}x\geq 0} .

It is obtained by recognizing that cos ( arctan ( x ) ) = 1 1 + x 2 = cos ( arccos ( 1 1 + x 2 ) ) {\displaystyle \cos \left(\arctan \left(x\right)\right)={\sqrt {\frac {1}{1+x^{2}}}}=\cos \left(\arccos \left({\sqrt {\frac {1}{1+x^{2}}}}\right)\right)} .

From the half-angle formula, tan ( θ 2 ) = sin ( θ ) 1 + cos ( θ ) {\displaystyle \tan \left({\tfrac {\theta }{2}}\right)={\tfrac {\sin(\theta )}{1+\cos(\theta )}}} , we get:

arcsin ( x ) = 2 arctan ( x 1 + 1 x 2 ) arccos ( x ) = 2 arctan ( 1 x 2 1 + x ) ,  if 1 < x 1 arctan ( x ) = 2 arctan ( x 1 + 1 + x 2 ) {\displaystyle {\begin{aligned}\arcsin(x)&=2\arctan \left({\frac {x}{1+{\sqrt {1-x^{2}}}}}\right)\\[0.5em]\arccos(x)&=2\arctan \left({\frac {\sqrt {1-x^{2}}}{1+x}}\right)\,,{\text{ if }}-1<x\leq 1\\[0.5em]\arctan(x)&=2\arctan \left({\frac {x}{1+{\sqrt {1+x^{2}}}}}\right)\end{aligned}}}

Arctangent addition formula [edit]

arctan ( u ) ± arctan ( v ) = arctan ( u ± v 1 u v ) ( mod π ) , u v 1 . {\displaystyle \arctan(u)\pm \arctan(v)=\arctan \left({\frac {u\pm v}{1\mp uv}}\right){\pmod {\pi }}\,,\quad uv\neq 1\,.}

This is derived from the tangent addition formula

tan ( α ± β ) = tan ( α ) ± tan ( β ) 1 tan ( α ) tan ( β ) , {\displaystyle \tan(\alpha \pm \beta )={\frac {\tan(\alpha )\pm \tan(\beta )}{1\mp \tan(\alpha )\tan(\beta )}}\,,}

by letting

α = arctan ( u ) , β = arctan ( v ) . {\displaystyle \alpha =\arctan(u)\,,\quad \beta =\arctan(v)\,.}

In calculus [edit]

Derivatives of inverse trigonometric functions [edit]

The derivatives for complex values of z are as follows:

d d z arcsin ( z ) = 1 1 z 2 ; z 1 , + 1 d d z arccos ( z ) = 1 1 z 2 ; z 1 , + 1 d d z arctan ( z ) = 1 1 + z 2 ; z i , + i d d z arccot ( z ) = 1 1 + z 2 ; z i , + i d d z arcsec ( z ) = 1 z 2 1 1 z 2 ; z 1 , 0 , + 1 d d z arccsc ( z ) = 1 z 2 1 1 z 2 ; z 1 , 0 , + 1 {\displaystyle {\begin{aligned}{\frac {d}{dz}}\arcsin(z)&{}={\frac {1}{\sqrt {1-z^{2}}}}\;;&z&{}\neq -1,+1\\{\frac {d}{dz}}\arccos(z)&{}=-{\frac {1}{\sqrt {1-z^{2}}}}\;;&z&{}\neq -1,+1\\{\frac {d}{dz}}\arctan(z)&{}={\frac {1}{1+z^{2}}}\;;&z&{}\neq -i,+i\\{\frac {d}{dz}}\operatorname {arccot}(z)&{}=-{\frac {1}{1+z^{2}}}\;;&z&{}\neq -i,+i\\{\frac {d}{dz}}\operatorname {arcsec}(z)&{}={\frac {1}{z^{2}{\sqrt {1-{\frac {1}{z^{2}}}}}}}\;;&z&{}\neq -1,0,+1\\{\frac {d}{dz}}\operatorname {arccsc}(z)&{}=-{\frac {1}{z^{2}{\sqrt {1-{\frac {1}{z^{2}}}}}}}\;;&z&{}\neq -1,0,+1\end{aligned}}}

Only for real values of x:

d d x arcsec ( x ) = 1 | x | x 2 1 ; | x | > 1 d d x arccsc ( x ) = 1 | x | x 2 1 ; | x | > 1 {\displaystyle {\begin{aligned}{\frac {d}{dx}}\operatorname {arcsec}(x)&{}={\frac {1}{|x|{\sqrt {x^{2}-1}}}}\;;&|x|>1\\{\frac {d}{dx}}\operatorname {arccsc}(x)&{}=-{\frac {1}{|x|{\sqrt {x^{2}-1}}}}\;;&|x|>1\end{aligned}}}

For a sample derivation: if θ = arcsin ( x ) {\displaystyle \theta =\arcsin(x)} , we get:

d arcsin ( x ) d x = d θ d sin ( θ ) = d θ cos ( θ ) d θ = 1 cos ( θ ) = 1 1 sin 2 ( θ ) = 1 1 x 2 {\displaystyle {\frac {d\arcsin(x)}{dx}}={\frac {d\theta }{d\sin(\theta )}}={\frac {d\theta }{\cos(\theta )\,d\theta }}={\frac {1}{\cos(\theta )}}={\frac {1}{\sqrt {1-\sin ^{2}(\theta )}}}={\frac {1}{\sqrt {1-x^{2}}}}}

Expression as definite integrals [edit]

Integrating the derivative and fixing the value at one point gives an expression for the inverse trigonometric function as a definite integral:

arcsin ( x ) = 0 x 1 1 z 2 d z , | x | 1 arccos ( x ) = x 1 1 1 z 2 d z , | x | 1 arctan ( x ) = 0 x 1 z 2 + 1 d z , arccot ( x ) = x 1 z 2 + 1 d z , arcsec ( x ) = 1 x 1 z z 2 1 d z = π + x 1 1 z z 2 1 d z , x 1 arccsc ( x ) = x 1 z z 2 1 d z = x 1 z z 2 1 d z , x 1 {\displaystyle {\begin{aligned}\arcsin(x)&{}=\int _{0}^{x}{\frac {1}{\sqrt {1-z^{2}}}}\,dz\;,&|x|&{}\leq 1\\\arccos(x)&{}=\int _{x}^{1}{\frac {1}{\sqrt {1-z^{2}}}}\,dz\;,&|x|&{}\leq 1\\\arctan(x)&{}=\int _{0}^{x}{\frac {1}{z^{2}+1}}\,dz\;,\\\operatorname {arccot}(x)&{}=\int _{x}^{\infty }{\frac {1}{z^{2}+1}}\,dz\;,\\\operatorname {arcsec}(x)&{}=\int _{1}^{x}{\frac {1}{z{\sqrt {z^{2}-1}}}}\,dz=\pi +\int _{x}^{-1}{\frac {1}{z{\sqrt {z^{2}-1}}}}\,dz\;,&x&{}\geq 1\\\operatorname {arccsc}(x)&{}=\int _{x}^{\infty }{\frac {1}{z{\sqrt {z^{2}-1}}}}\,dz=\int _{-\infty }^{x}{\frac {1}{z{\sqrt {z^{2}-1}}}}\,dz\;,&x&{}\geq 1\\\end{aligned}}}

When x equals 1, the integrals with limited domains are improper integrals, but still well-defined.

Infinite series [edit]

Similar to the sine and cosine functions, the inverse trigonometric functions can also be calculated using power series, as follows. For arcsine, the series can be derived by expanding its derivative, 1 1 z 2 {\textstyle {\tfrac {1}{\sqrt {1-z^{2}}}}} , as a binomial series, and integrating term by term (using the integral definition as above). The series for arctangent can similarly be derived by expanding its derivative 1 1 + z 2 {\textstyle {\frac {1}{1+z^{2}}}} in a geometric series, and applying the integral definition above (see Leibniz series).

arcsin ( z ) = z + ( 1 2 ) z 3 3 + ( 1 3 2 4 ) z 5 5 + ( 1 3 5 2 4 6 ) z 7 7 + = n = 0 ( 2 n 1 ) ! ! ( 2 n ) ! ! z 2 n + 1 2 n + 1 = n = 0 ( 2 n ) ! ( 2 n n ! ) 2 z 2 n + 1 2 n + 1 ; | z | 1 {\displaystyle {\begin{aligned}\arcsin(z)&=z+\left({\frac {1}{2}}\right){\frac {z^{3}}{3}}+\left({\frac {1\cdot 3}{2\cdot 4}}\right){\frac {z^{5}}{5}}+\left({\frac {1\cdot 3\cdot 5}{2\cdot 4\cdot 6}}\right){\frac {z^{7}}{7}}+\cdots \\[5pt]&=\sum _{n=0}^{\infty }{\frac {(2n-1)!!}{(2n)!!}}{\frac {z^{2n+1}}{2n+1}}\\[5pt]&=\sum _{n=0}^{\infty }{\frac {(2n)!}{(2^{n}n!)^{2}}}{\frac {z^{2n+1}}{2n+1}}\,;\qquad |z|\leq 1\end{aligned}}}
arctan ( z ) = z z 3 3 + z 5 5 z 7 7 + = n = 0 ( 1 ) n z 2 n + 1 2 n + 1 ; | z | 1 z i , i {\displaystyle \arctan(z)=z-{\frac {z^{3}}{3}}+{\frac {z^{5}}{5}}-{\frac {z^{7}}{7}}+\cdots =\sum _{n=0}^{\infty }{\frac {(-1)^{n}z^{2n+1}}{2n+1}}\,;\qquad |z|\leq 1\qquad z\neq i,-i}

Series for the other inverse trigonometric functions can be given in terms of these according to the relationships given above. For example, arccos ( x ) = π / 2 arcsin ( x ) {\displaystyle \arccos(x)=\pi /2-\arcsin(x)} , arccsc ( x ) = arcsin ( 1 / x ) {\displaystyle \operatorname {arccsc}(x)=\arcsin(1/x)} , and so on. Another series is given by:[19]

2 ( arcsin ( x 2 ) ) 2 = n = 1 x 2 n n 2 ( 2 n n ) . {\displaystyle 2\left(\arcsin \left({\frac {x}{2}}\right)\right)^{2}=\sum _{n=1}^{\infty }{\frac {x^{2n}}{n^{2}{\binom {2n}{n}}}}.}

Leonhard Euler found a series for the arctangent that converges more quickly than its Taylor series:

arctan ( z ) = z 1 + z 2 n = 0 k = 1 n 2 k z 2 ( 2 k + 1 ) ( 1 + z 2 ) . {\displaystyle \arctan(z)={\frac {z}{1+z^{2}}}\sum _{n=0}^{\infty }\prod _{k=1}^{n}{\frac {2kz^{2}}{(2k+1)(1+z^{2})}}.} [20]

(The term in the sum for n = 0 is the empty product, so is 1.)

Alternatively, this can be expressed as

arctan ( z ) = n = 0 2 2 n ( n ! ) 2 ( 2 n + 1 ) ! z 2 n + 1 ( 1 + z 2 ) n + 1 . {\displaystyle \arctan(z)=\sum _{n=0}^{\infty }{\frac {2^{2n}(n!)^{2}}{(2n+1)!}}{\frac {z^{2n+1}}{(1+z^{2})^{n+1}}}.}

Another series for the arctangent function is given by

arctan ( z ) = i n = 1 1 2 n 1 ( 1 ( 1 + 2 i / z ) 2 n 1 1 ( 1 2 i / z ) 2 n 1 ) , {\displaystyle \arctan(z)=i\sum _{n=1}^{\infty }{\frac {1}{2n-1}}\left({\frac {1}{(1+2i/z)^{2n-1}}}-{\frac {1}{(1-2i/z)^{2n-1}}}\right),}

where i = 1 {\displaystyle i={\sqrt {-1}}} is the imaginary unit.[21]

Continued fractions for arctangent [edit]

Two alternatives to the power series for arctangent are these generalized continued fractions:

arctan ( z ) = z 1 + ( 1 z ) 2 3 1 z 2 + ( 3 z ) 2 5 3 z 2 + ( 5 z ) 2 7 5 z 2 + ( 7 z ) 2 9 7 z 2 + = z 1 + ( 1 z ) 2 3 + ( 2 z ) 2 5 + ( 3 z ) 2 7 + ( 4 z ) 2 9 + {\displaystyle \arctan(z)={\frac {z}{1+{\cfrac {(1z)^{2}}{3-1z^{2}+{\cfrac {(3z)^{2}}{5-3z^{2}+{\cfrac {(5z)^{2}}{7-5z^{2}+{\cfrac {(7z)^{2}}{9-7z^{2}+\ddots }}}}}}}}}}={\frac {z}{1+{\cfrac {(1z)^{2}}{3+{\cfrac {(2z)^{2}}{5+{\cfrac {(3z)^{2}}{7+{\cfrac {(4z)^{2}}{9+\ddots }}}}}}}}}}}

The second of these is valid in the cut complex plane. There are two cuts, from −i to the point at infinity, going down the imaginary axis, and from i to the point at infinity, going up the same axis. It works best for real numbers running from −1 to 1. The partial denominators are the odd natural numbers, and the partial numerators (after the first) are just (nz)2, with each perfect square appearing once. The first was developed by Leonhard Euler; the second by Carl Friedrich Gauss utilizing the Gaussian hypergeometric series.

Indefinite integrals of inverse trigonometric functions [edit]

For real and complex values of z:

arcsin ( z ) d z = z arcsin ( z ) + 1 z 2 + C arccos ( z ) d z = z arccos ( z ) 1 z 2 + C arctan ( z ) d z = z arctan ( z ) 1 2 ln ( 1 + z 2 ) + C arccot ( z ) d z = z arccot ( z ) + 1 2 ln ( 1 + z 2 ) + C arcsec ( z ) d z = z arcsec ( z ) ln [ z ( 1 + z 2 1 z 2 ) ] + C arccsc ( z ) d z = z arccsc ( z ) + ln [ z ( 1 + z 2 1 z 2 ) ] + C {\displaystyle {\begin{aligned}\int \arcsin(z)\,dz&{}=z\,\arcsin(z)+{\sqrt {1-z^{2}}}+C\\\int \arccos(z)\,dz&{}=z\,\arccos(z)-{\sqrt {1-z^{2}}}+C\\\int \arctan(z)\,dz&{}=z\,\arctan(z)-{\frac {1}{2}}\ln \left(1+z^{2}\right)+C\\\int \operatorname {arccot}(z)\,dz&{}=z\,\operatorname {arccot}(z)+{\frac {1}{2}}\ln \left(1+z^{2}\right)+C\\\int \operatorname {arcsec}(z)\,dz&{}=z\,\operatorname {arcsec}(z)-\ln \left[z\left(1+{\sqrt {\frac {z^{2}-1}{z^{2}}}}\right)\right]+C\\\int \operatorname {arccsc}(z)\,dz&{}=z\,\operatorname {arccsc}(z)+\ln \left[z\left(1+{\sqrt {\frac {z^{2}-1}{z^{2}}}}\right)\right]+C\end{aligned}}}

For real x ≥ 1:

arcsec ( x ) d x = x arcsec ( x ) ln ( x + x 2 1 ) + C arccsc ( x ) d x = x arccsc ( x ) + ln ( x + x 2 1 ) + C {\displaystyle {\begin{aligned}\int \operatorname {arcsec}(x)\,dx&{}=x\,\operatorname {arcsec}(x)-\ln \left(x+{\sqrt {x^{2}-1}}\right)+C\\\int \operatorname {arccsc}(x)\,dx&{}=x\,\operatorname {arccsc}(x)+\ln \left(x+{\sqrt {x^{2}-1}}\right)+C\end{aligned}}}

For all real x not between -1 and 1:

arcsec ( x ) d x = x arcsec ( x ) sgn ( x ) ln ( | x + x 2 1 | ) + C arccsc ( x ) d x = x arccsc ( x ) + sgn ( x ) ln ( | x + x 2 1 | ) + C {\displaystyle {\begin{aligned}\int \operatorname {arcsec}(x)\,dx&{}=x\,\operatorname {arcsec}(x)-\operatorname {sgn}(x)\ln \left(\left|x+{\sqrt {x^{2}-1}}\right|\right)+C\\\int \operatorname {arccsc}(x)\,dx&{}=x\,\operatorname {arccsc}(x)+\operatorname {sgn}(x)\ln \left(\left|x+{\sqrt {x^{2}-1}}\right|\right)+C\end{aligned}}}

The absolute value is necessary to compensate for both negative and positive values of the arcsecant and arccosecant functions. The signum function is also necessary due to the absolute values in the derivatives of the two functions, which create two different solutions for positive and negative values of x. These can be further simplified using the logarithmic definitions of the inverse hyperbolic functions:

arcsec ( x ) d x = x arcsec ( x ) arcosh ( | x | ) + C arccsc ( x ) d x = x arccsc ( x ) + arcosh ( | x | ) + C {\displaystyle {\begin{aligned}\int \operatorname {arcsec}(x)\,dx&{}=x\,\operatorname {arcsec}(x)-\operatorname {arcosh} (|x|)+C\\\int \operatorname {arccsc}(x)\,dx&{}=x\,\operatorname {arccsc}(x)+\operatorname {arcosh} (|x|)+C\\\end{aligned}}}

The absolute value in the argument of the arcosh function creates a negative half of its graph, making it identical to the signum logarithmic function shown above.

All of these antiderivatives can be derived using integration by parts and the simple derivative forms shown above.

Example [edit]

Using u d v = u v v d u {\displaystyle \int u\,dv=uv-\int v\,du} (i.e. integration by parts), set

u = arcsin ( x ) d v = d x d u = d x 1 x 2 v = x {\displaystyle {\begin{aligned}u&=\arcsin(x)&dv&=dx\\du&={\frac {dx}{\sqrt {1-x^{2}}}}&v&=x\end{aligned}}}

Then

arcsin ( x ) d x = x arcsin ( x ) x 1 x 2 d x , {\displaystyle \int \arcsin(x)\,dx=x\arcsin(x)-\int {\frac {x}{\sqrt {1-x^{2}}}}\,dx,}

which by the simple substitution w = 1 x 2 , d w = 2 x d x {\displaystyle w=1-x^{2},\ dw=-2x\,dx} yields the final result:

arcsin ( x ) d x = x arcsin ( x ) + 1 x 2 + C {\displaystyle \int \arcsin(x)\,dx=x\arcsin(x)+{\sqrt {1-x^{2}}}+C}

Extension to complex plane [edit]

A Riemann surface for the argument of the relation tan z = x . The orange sheet in the middle is the principal sheet representing arctan x . The blue sheet above and green sheet below are displaced by 2π and −2π respectively.

Since the inverse trigonometric functions are analytic functions, they can be extended from the real line to the complex plane. This results in functions with multiple sheets and branch points. One possible way of defining the extension is:

arctan ( z ) = 0 z d x 1 + x 2 z i , + i {\displaystyle \arctan(z)=\int _{0}^{z}{\frac {dx}{1+x^{2}}}\quad z\neq -i,+i}

where the part of the imaginary axis which does not lie strictly between the branch points (−i and +i) is the branch cut between the principal sheet and other sheets. The path of the integral must not cross a branch cut. For z not on a branch cut, a straight line path from 0 to z is such a path. For z on a branch cut, the path must approach from Re[x] > 0 for the upper branch cut and from Re[x] < 0 for the lower branch cut.

The arcsine function may then be defined as:

arcsin ( z ) = arctan ( z 1 z 2 ) z 1 , + 1 {\displaystyle \arcsin(z)=\arctan \left({\frac {z}{\sqrt {1-z^{2}}}}\right)\quad z\neq -1,+1}

where (the square-root function has its cut along the negative real axis and) the part of the real axis which does not lie strictly between −1 and +1 is the branch cut between the principal sheet of arcsin and other sheets;

arccos ( z ) = π 2 arcsin ( z ) z 1 , + 1 {\displaystyle \arccos(z)={\frac {\pi }{2}}-\arcsin(z)\quad z\neq -1,+1}

which has the same cut as arcsin;

arccot ( z ) = π 2 arctan ( z ) z i , i {\displaystyle \operatorname {arccot}(z)={\frac {\pi }{2}}-\arctan(z)\quad z\neq -i,i}

which has the same cut as arctan;

arcsec ( z ) = arccos ( 1 z ) z 1 , 0 , + 1 {\displaystyle \operatorname {arcsec}(z)=\arccos \left({\frac {1}{z}}\right)\quad z\neq -1,0,+1}

where the part of the real axis between −1 and +1 inclusive is the cut between the principal sheet of arcsec and other sheets;

arccsc ( z ) = arcsin ( 1 z ) z 1 , 0 , + 1 {\displaystyle \operatorname {arccsc}(z)=\arcsin \left({\frac {1}{z}}\right)\quad z\neq -1,0,+1}

which has the same cut as arcsec.

Logarithmic forms [edit]

These functions may also be expressed using complex logarithms. This extends their domains to the complex plane in a natural fashion. The following identities for principal values of the functions hold everywhere that they are defined, even on their branch cuts.

arcsin ( z ) = i ln ( 1 z 2 + i z ) = i ln ( 1 z 2 i z ) = arccsc ( 1 z ) arccos ( z ) = i ln ( i 1 z 2 + z ) = π 2 arcsin ( z ) = arcsec ( 1 z ) arctan ( z ) = i 2 ln ( i z i + z ) = i 2 ln ( 1 + i z 1 i z ) = arccot ( 1 z ) arccot ( z ) = i 2 ln ( z + i z i ) = i 2 ln ( i z 1 i z + 1 ) = arctan ( 1 z ) arcsec ( z ) = i ln ( i 1 1 z 2 + 1 z ) = π 2 arccsc ( z ) = arccos ( 1 z ) arccsc ( z ) = i ln ( 1 1 z 2 + i z ) = i ln ( 1 1 z 2 i z ) = arcsin ( 1 z ) {\displaystyle {\begin{aligned}\arcsin(z)&{}=-i\ln \left({\sqrt {1-z^{2}}}+iz\right)=i\ln \left({\sqrt {1-z^{2}}}-iz\right)&{}=\operatorname {arccsc} \left({\frac {1}{z}}\right)\\[10pt]\arccos(z)&{}=-i\ln \left(i{\sqrt {1-z^{2}}}+z\right)={\frac {\pi }{2}}-\arcsin(z)&{}=\operatorname {arcsec} \left({\frac {1}{z}}\right)\\[10pt]\arctan(z)&{}=-{\frac {i}{2}}\ln \left({\frac {i-z}{i+z}}\right)=-{\frac {i}{2}}\ln \left({\frac {1+iz}{1-iz}}\right)&{}=\operatorname {arccot} \left({\frac {1}{z}}\right)\\[10pt]\operatorname {arccot}(z)&{}=-{\frac {i}{2}}\ln \left({\frac {z+i}{z-i}}\right)=-{\frac {i}{2}}\ln \left({\frac {iz-1}{iz+1}}\right)&{}=\arctan \left({\frac {1}{z}}\right)\\[10pt]\operatorname {arcsec}(z)&{}=-i\ln \left(i{\sqrt {1-{\frac {1}{z^{2}}}}}+{\frac {1}{z}}\right)={\frac {\pi }{2}}-\operatorname {arccsc}(z)&{}=\arccos \left({\frac {1}{z}}\right)\\[10pt]\operatorname {arccsc}(z)&{}=-i\ln \left({\sqrt {1-{\frac {1}{z^{2}}}}}+{\frac {i}{z}}\right)=i\ln \left({\sqrt {1-{\frac {1}{z^{2}}}}}-{\frac {i}{z}}\right)&{}=\arcsin \left({\frac {1}{z}}\right)\end{aligned}}}

Generalization [edit]

Because all of the inverse trigonometric functions output an angle of a right triangle, they can be generalized by using Euler's formula to form a right triangle in the complex plane. Algebraically, this gives us:

c e θ i = c cos ( θ ) + c i sin ( θ ) {\displaystyle ce^{\theta i}=c\cos(\theta )+ci\sin(\theta )}

or

c e θ i = a + b i {\displaystyle ce^{\theta i}=a+bi}

where a {\displaystyle a} is the adjacent side, b {\displaystyle b} is the opposite side, and c {\displaystyle c} is the hypotenuse. From here, we can solve for θ {\displaystyle \theta } .

e ln ( c ) + θ i = a + b i ln c + θ i = ln ( a + b i ) θ = Im ( ln ( a + b i ) ) {\displaystyle {\begin{aligned}e^{\ln(c)+\theta i}&=a+bi\\\ln c+\theta i&=\ln(a+bi)\\\theta &=\operatorname {Im} \left(\ln(a+bi)\right)\end{aligned}}}

or

θ = i ln ( a + b i c ) = i ln ( c a + b i ) {\displaystyle \theta =-i\ln \left({\frac {a+bi}{c}}\right)=i\ln \left({\frac {c}{a+bi}}\right)}

Simply taking the imaginary part works for any real-valued a {\displaystyle a} and b {\displaystyle b} , but if a {\displaystyle a} or b {\displaystyle b} is complex-valued, we have to use the final equation so that the real part of the result isn't excluded. Since the length of the hypotenuse doesn't change the angle, ignoring the real part of ln ( a + b i ) {\displaystyle \ln(a+bi)} also removes c {\displaystyle c} from the equation. In the final equation, we see that the angle of the triangle in the complex plane can be found by inputting the lengths of each side. By setting one of the three sides equal to 1 and one of the remaining sides equal to our input z {\displaystyle z} , we obtain a formula for one of the inverse trig functions, for a total of six equations. Because the inverse trig functions require only one input, we must put the final side of the triangle in terms of the other two using the Pythagorean Theorem relation

a 2 + b 2 = c 2 {\displaystyle a^{2}+b^{2}=c^{2}}

The table below shows the values of a, b, and c for each of the inverse trig functions and the equivalent expressions for θ {\displaystyle \theta } that result from plugging the values into the equations above and simplifying.

a b c θ θ simplified θ a , b R arcsin ( z ) 1 z 2 z 1 i ln ( 1 z 2 + z i 1 ) = i ln ( 1 z 2 + z i ) Im ( ln ( 1 z 2 + z i ) ) arccos ( z ) z 1 z 2 1 i ln ( z + i 1 z 2 1 ) = i ln ( z + z 2 1 ) Im ( ln ( z + z 2 1 ) ) arctan ( z ) 1 z 1 + z 2 i ln ( 1 + z 2 1 + z i ) = i 2 ln ( i + z i z ) Im ( ln ( 1 + z i ) ) arccot ( z ) z 1 z 2 + 1 i ln ( z 2 + 1 z + i ) = i 2 ln ( z i z + i ) Im ( ln ( z + i ) ) arcsec ( z ) 1 z 2 1 z i ln ( 1 + i z 2 1 z ) = i ln ( 1 z + 1 z 2 1 ) Im ( ln ( 1 + 1 z 2 ) ) arccsc ( z ) z 2 1 1 z i ln ( z 2 1 + i z ) = i ln ( 1 1 z 2 + i z ) Im ( ln ( z 2 1 + i ) ) {\displaystyle {\begin{aligned}&a&&b&&c&&\theta &&\theta _{\text{simplified}}&&\theta _{a,b\in \mathbb {R} }\\\arcsin(z)\ \ &{\sqrt {1-z^{2}}}&&z&&1&&-i\ln \left({\frac {{\sqrt {1-z^{2}}}+zi}{1}}\right)&&=-i\ln \left({\sqrt {1-z^{2}}}+zi\right)&&\operatorname {Im} \left(\ln \left({\sqrt {1-z^{2}}}+zi\right)\right)\\\arccos(z)\ \ &z&&{\sqrt {1-z^{2}}}&&1&&-i\ln \left({\frac {z+i{\sqrt {1-z^{2}}}}{1}}\right)&&=-i\ln \left(z+{\sqrt {z^{2}-1}}\right)&&\operatorname {Im} \left(\ln \left(z+{\sqrt {z^{2}-1}}\right)\right)\\\arctan(z)\ \ &1&&z&&{\sqrt {1+z^{2}}}&&i\ln \left({\frac {\sqrt {1+z^{2}}}{1+zi}}\right)&&={\frac {i}{2}}\ln \left({\frac {i+z}{i-z}}\right)&&\operatorname {Im} \left(\ln \left(1+zi\right)\right)\\\operatorname {arccot}(z)\ \ &z&&1&&{\sqrt {z^{2}+1}}&&i\ln \left({\frac {\sqrt {z^{2}+1}}{z+i}}\right)&&={\frac {i}{2}}\ln \left({\frac {z-i}{z+i}}\right)&&\operatorname {Im} \left(\ln \left(z+i\right)\right)\\\operatorname {arcsec}(z)\ \ &1&&{\sqrt {z^{2}-1}}&&z&&-i\ln \left({\frac {1+i{\sqrt {z^{2}-1}}}{z}}\right)&&=-i\ln \left({\frac {1}{z}}+{\sqrt {{\frac {1}{z^{2}}}-1}}\right)&&\operatorname {Im} \left(\ln \left(1+{\sqrt {1-z^{2}}}\right)\right)\\\operatorname {arccsc}(z)\ \ &{\sqrt {z^{2}-1}}&&1&&z&&-i\ln \left({\frac {{\sqrt {z^{2}-1}}+i}{z}}\right)&&=-i\ln \left({\sqrt {1-{\frac {1}{z^{2}}}}}+{\frac {i}{z}}\right)&&\operatorname {Im} \left(\ln \left({\sqrt {z^{2}-1}}+i\right)\right)\\\end{aligned}}}

In this sense, all of the inverse trig functions can be thought of as specific cases of the complex-valued log function. Since this definition works for any complex-valued z {\displaystyle z} , this definition allows for hyperbolic angles as outputs and can be used to further define the inverse hyperbolic functions. Elementary proofs of the relations may also proceed via expansion to exponential forms of the trigonometric functions.

Example proof [edit]

sin ( ϕ ) = z ϕ = arcsin ( z ) {\displaystyle {\begin{aligned}\sin(\phi )&=z\\\phi &=\arcsin(z)\end{aligned}}}

Using the exponential definition of sine, one obtains

z = e ϕ i e ϕ i 2 i {\displaystyle z={\frac {e^{\phi i}-e^{-\phi i}}{2i}}}

Let

ξ = e ϕ i {\displaystyle \xi =e^{\phi i}}

Solving for ϕ {\displaystyle \phi }

z = ξ 1 ξ 2 i 2 i z = ξ 1 ξ ξ 2 i z 1 ξ = 0 ξ 2 2 i ξ z 1 = 0 ξ = i z ± 1 z 2 = e ϕ i ϕ i = ln ( i z ± 1 z 2 ) ϕ = i ln ( i z ± 1 z 2 ) {\displaystyle {\begin{aligned}z&={\frac {\xi -{\frac {1}{\xi }}}{2i}}\\2iz&={\xi -{\frac {1}{\xi }}}\\\xi -2iz-{\frac {1}{\xi }}&=0\\\xi ^{2}-2i\xi z-1&=0\\\xi &=iz\pm {\sqrt {1-z^{2}}}=e^{\phi i}\\\phi i&=\ln \left(iz\pm {\sqrt {1-z^{2}}}\right)\\\phi &=-i\ln \left(iz\pm {\sqrt {1-z^{2}}}\right)\end{aligned}}}

(the positive branch is chosen)

ϕ = arcsin ( z ) = i ln ( i z + 1 z 2 ) {\displaystyle \phi =\arcsin(z)=-i\ln \left(iz+{\sqrt {1-z^{2}}}\right)}
Color wheel graphs of inverse trigonometric functions in the complex plane

Complex arcsin.jpg

Complex arccos.jpg

Complex arctan.jpg

Complex ArcCot.jpg

Complex ArcSec.jpg

Complex ArcCsc.jpg

arcsin ( z ) {\displaystyle \arcsin(z)} arccos ( z ) {\displaystyle \arccos(z)} arctan ( z ) {\displaystyle \arctan(z)} arccot ( z ) {\displaystyle \operatorname {arccot}(z)} arcsec ( z ) {\displaystyle \operatorname {arcsec}(z)} arccsc ( z ) {\displaystyle \operatorname {arccsc}(z)}

Applications [edit]

Finding the angle of a right triangle [edit]

A right triangle with sides relative to an angle at the A {\displaystyle A} point.

Inverse trigonometric functions are useful when trying to determine the remaining two angles of a right triangle when the lengths of the sides of the triangle are known. Recalling the right-triangle definitions of sine and cosine, it follows that

θ = arcsin ( opposite hypotenuse ) = arccos ( adjacent hypotenuse ) . {\displaystyle \theta =\arcsin \left({\frac {\text{opposite}}{\text{hypotenuse}}}\right)=\arccos \left({\frac {\text{adjacent}}{\text{hypotenuse}}}\right).}

Often, the hypotenuse is unknown and would need to be calculated before using arcsine or arccosine using the Pythagorean Theorem: a 2 + b 2 = h 2 {\displaystyle a^{2}+b^{2}=h^{2}} where h {\displaystyle h} is the length of the hypotenuse. Arctangent comes in handy in this situation, as the length of the hypotenuse is not needed.

θ = arctan ( opposite adjacent ) . {\displaystyle \theta =\arctan \left({\frac {\text{opposite}}{\text{adjacent}}}\right)\,.}

For example, suppose a roof drops 8 feet as it runs out 20 feet. The roof makes an angle θ with the horizontal, where θ may be computed as follows:

θ = arctan ( opposite adjacent ) = arctan ( rise run ) = arctan ( 8 20 ) 21.8 . {\displaystyle \theta =\arctan \left({\frac {\text{opposite}}{\text{adjacent}}}\right)=\arctan \left({\frac {\text{rise}}{\text{run}}}\right)=\arctan \left({\frac {8}{20}}\right)\approx 21.8^{\circ }\,.}

In computer science and engineering [edit]

Two-argument variant of arctangent [edit]

The two-argument atan2 function computes the arctangent of y / x given y and x, but with a range of (−π,π]. In other words, atan2(y,x) is the angle between the positive x-axis of a plane and the point (x,y) on it, with positive sign for counter-clockwise angles (upper half-plane, y > 0), and negative sign for clockwise angles (lower half-plane, y < 0). It was first introduced in many computer programming languages, but it is now also common in other fields of science and engineering.

In terms of the standard arctan function, that is with range of (− π / 2 , π / 2 ), it can be expressed as follows:

atan2 ( y , x ) = { arctan ( y x ) x > 0 arctan ( y x ) + π y 0 , x < 0 arctan ( y x ) π y < 0 , x < 0 π 2 y > 0 , x = 0 π 2 y < 0 , x = 0 undefined y = 0 , x = 0 {\displaystyle \operatorname {atan2} (y,x)={\begin{cases}\arctan \left({\frac {y}{x}}\right)&\quad x>0\\\arctan \left({\frac {y}{x}}\right)+\pi &\quad y\geq 0,\;x<0\\\arctan \left({\frac {y}{x}}\right)-\pi &\quad y<0,\;x<0\\{\frac {\pi }{2}}&\quad y>0,\;x=0\\-{\frac {\pi }{2}}&\quad y<0,\;x=0\\{\text{undefined}}&\quad y=0,\;x=0\end{cases}}}

It also equals the principal value of the argument of the complex number x +i y.

This limited version of the function above may also be defined using the tangent half-angle formulae as follows:

atan2 ( y , x ) = 2 arctan ( y x 2 + y 2 + x ) {\displaystyle \operatorname {atan2} (y,x)=2\arctan \left({\frac {y}{{\sqrt {x^{2}+y^{2}}}+x}}\right)}

provided that either x > 0 or y ≠ 0. However this fails if given x ≤ 0 and y = 0 so the expression is unsuitable for computational use.

The above argument order (y, x) seems to be the most common, and in particular is used in ISO standards such as the C programming language, but a few authors may use the opposite convention (x, y) so some caution is warranted. These variations are detailed at atan2.

Arctangent function with location parameter [edit]

In many applications[22] the solution y {\displaystyle y} of the equation x = tan ( y ) {\displaystyle x=\tan(y)} is to come as close as possible to a given value < η < {\displaystyle -\infty <\eta <\infty } . The adequate solution is produced by the parameter modified arctangent function

y = arctan η ( x ) := arctan ( x ) + π rni ( η arctan ( x ) π ) . {\displaystyle y=\arctan _{\eta }(x):=\arctan(x)+\pi \,\operatorname {rni} \left({\frac {\eta -\arctan(x)}{\pi }}\right)\,.}

The function rni {\displaystyle \operatorname {rni} } rounds to the nearest integer.

Numerical accuracy [edit]

For angles near 0 and π, arccosine is ill-conditioned and will thus calculate the angle with reduced accuracy in a computer implementation (due to the limited number of digits).[23] Similarly, arcsine is inaccurate for angles near −π/2 and π/2.

See also [edit]

  • Inverse exsecant
  • Inverse versine
  • Inverse hyperbolic functions
  • List of integrals of inverse trigonometric functions
  • List of trigonometric identities
  • Trigonometric function
  • Trigonometric functions of matrices

Notes [edit]

  1. ^ To clarify, suppose that it is written "LHS {\displaystyle \,\iff \,} RHS" where LHS (which abbreviates left hand side) and RHS are both statements that can individually be either be true or false. For example, if θ {\displaystyle \theta } and s {\displaystyle s} are some given and fixed numbers and if the following is written: tan θ = s θ = arctan ( s ) + π k  for some k Z {\displaystyle \tan \theta =s\,\iff \,\theta =\arctan(s)+\pi k\quad {\text{ for some }}k\in \mathbb {Z} } then LHS is the statement " tan θ = s {\displaystyle \tan \theta =s} ". Depending on what specific values θ {\displaystyle \theta } and s {\displaystyle s} have, this LHS statement can either be true or false. For instance, LHS is true if θ = 0 {\displaystyle \theta =0} and s = 0 {\displaystyle s=0} (because in this case tan θ = tan 0 = s {\displaystyle \tan \theta =\tan 0=s} ) but LHS is false if θ = 0 {\displaystyle \theta =0} and s = 2 {\displaystyle s=2} (because in this case tan θ = tan 0 = s {\displaystyle \tan \theta =\tan 0=s} which is not equal to s = 2 {\displaystyle s=2} ); more generally, LHS is false if θ = 0 {\displaystyle \theta =0} and s 0. {\displaystyle s\neq 0.} Similarly, RHS is the statement " θ = arctan ( s ) + π k {\displaystyle \theta =\arctan(s)+\pi k} for some k Z {\displaystyle k\in \mathbb {Z} } ". The RHS statement can also either true or false (as before, whether the RHS statement is true or false depends on what specific values θ {\displaystyle \theta } and s {\displaystyle s} have). The logical equality symbol {\displaystyle \,\iff \,} means that (a) if the LHS statement is true then the RHS statement is also necessarily true, and moreover (b) if the LHS statement is false then the RHS statement is also necessarily false. Similarly, {\displaystyle \,\iff \,} also means that (c) if the RHS statement is true then the LHS statement is also necessarily true, and moreover (d) if the RHS statement is false then the LHS statement is also necessarily false.

References [edit]

  • Abramowitz, Milton; Stegun, Irene A., eds. (1972). Handbook of Mathematical Functions with Formulas, Graphs, and Mathematical Tables. New York: Dover Publications. ISBN978-0-486-61272-0.
  1. ^ Taczanowski, Stefan (1978-10-01). "On the optimization of some geometric parameters in 14 MeV neutron activation analysis". Nuclear Instruments and Methods. ScienceDirect. 155 (3): 543–546. Bibcode:1978NucIM.155..543T. doi:10.1016/0029-554X(78)90541-4.
  2. ^ Hazewinkel, Michiel (1994) [1987]. Encyclopaedia of Mathematics (unabridged reprint ed.). Kluwer Academic Publishers / Springer Science & Business Media. ISBN978-155608010-4.
  3. ^ Ebner, Dieter (2005-07-25). Preparatory Course in Mathematics (PDF) (6 ed.). Department of Physics, University of Konstanz. Archived (PDF) from the original on 2017-07-26. Retrieved 2017-07-26 .
  4. ^ Mejlbro, Leif (2010-11-11). Stability, Riemann Surfaces, Conformal Mappings - Complex Functions Theory (PDF) (1 ed.). Ventus Publishing ApS / Bookboon. ISBN978-87-7681-702-2. Archived from the original (PDF) on 2017-07-26. Retrieved 2017-07-26 .
  5. ^ Durán, Mario (2012). Mathematical methods for wave propagation in science and engineering. 1: Fundamentals (1 ed.). Ediciones UC. p. 88. ISBN978-956141314-6.
  6. ^ a b c d Hall, Arthur Graham; Frink, Fred Goodrich (January 1909). "Chapter II. The Acute Angle [14] Inverse trigonometric functions". Written at Ann Arbor, Michigan, USA. Trigonometry. Part I: Plane Trigonometry. New York, USA: Henry Holt and Company / Norwood Press / J. S. Cushing Co. - Berwick & Smith Co., Norwood, Massachusetts, USA. p. 15. Retrieved 2017-08-12 . […] α = arcsinm : It is frequently read "arc-sine m" or "anti-sine m," since two mutually inverse functions are said each to be the anti-function of the other. […] A similar symbolic relation holds for the other trigonometric functions. […] This notation is universally used in Europe and is fast gaining ground in this country. A less desirable symbol, α = sin-1 m , is still found in English and American texts. The notation α = inv sin m is perhaps better still on account of its general applicability. […]
  7. ^ Klein, Christian Felix (1924) [1902]. Elementarmathematik vom höheren Standpunkt aus: Arithmetik, Algebra, Analysis (in German). 1 (3rd ed.). Berlin: J. Springer.
  8. ^ Klein, Christian Felix (2004) [1932]. Elementary Mathematics from an Advanced Standpoint: Arithmetic, Algebra, Analysis. Translated by Hedrick, E. R.; Noble, C. A. (Translation of 3rd German ed.). Dover Publications, Inc. / The Macmillan Company. ISBN978-0-48643480-3 . Retrieved 2017-08-13 .
  9. ^ Dörrie, Heinrich (1965). Triumph der Mathematik. Translated by Antin, David. Dover Publications. p. 69. ISBN978-0-486-61348-2.
  10. ^ Weisstein, Eric W. "Inverse Trigonometric Functions". mathworld.wolfram.com . Retrieved 2020-08-29 .
  11. ^ Beach, Frederick Converse; Rines, George Edwin, eds. (1912). "Inverse trigonometric functions". The Americana: a universal reference library. 21.
  12. ^ John D. Cook (2021-02-11). "Trig functions across programming languages". Retrieved 2021-03-10 .
  13. ^ Cajori, Florian (1919). A History of Mathematics (2 ed.). New York, NY: The Macmillan Company. p. 272.
  14. ^ Herschel, John Frederick William (1813). "On a remarkable Application of Cotes's Theorem". Philosophical Transactions. Royal Society, London. 103 (1): 8. doi:10.1098/rstl.1813.0005.
  15. ^ "Inverse Trigonometric Functions | Brilliant Math & Science Wiki". brilliant.org . Retrieved 2020-08-29 .
  16. ^ Korn, Grandino Arthur; Korn, Theresa M. (2000) [1961]. "21.2.-4. Inverse Trigonometric Functions". Mathematical handbook for scientists and engineers: Definitions, theorems, and formulars for reference and review (3 ed.). Mineola, New York, USA: Dover Publications, Inc. p. 811. ISBN978-0-486-41147-7.
  17. ^ Bhatti, Sanaullah; Nawab-ud-Din; Ahmed, Bashir; Yousuf, S. M.; Taheem, Allah Bukhsh (1999). "Differentiation of Trigonometric, Logarithmic and Exponential Functions". In Ellahi, Mohammad Maqbool; Dar, Karamat Hussain; Hussain, Faheem (eds.). Calculus and Analytic Geometry (1 ed.). Lahore: Punjab Textbook Board. p. 140.
  18. ^ Abramowitz & Stegun 1972, p. 73, 4.3.44
  19. ^ Borwein, Jonathan; Bailey, David; Gingersohn, Roland (2004). Experimentation in Mathematics: Computational Paths to Discovery (1 ed.). Wellesley, MA, USA: A. K. Peters. p. 51. ISBN978-1-56881-136-9.
  20. ^ Hwang Chien-Lih (2005), "An elementary derivation of Euler's series for the arctangent function", The Mathematical Gazette, 89 (516): 469–470, doi:10.1017/S0025557200178404, S2CID 123395287
  21. ^ S. M. Abrarov and B. M. Quine (2018), "A formula for pi involving nested radicals", The Ramanujan Journal, 46 (3): 657–665, arXiv:1610.07713, doi:10.1007/s11139-018-9996-8, S2CID 119150623
  22. ^ when a time varying angle crossing ± π / 2 {\displaystyle \pm \pi /2} should be mapped by a smooth line instead of a saw toothed one (robotics, astromomy, angular movement in general)[ citation needed ]
  23. ^ Gade, Kenneth (2010). "A non-singular horizontal position representation" (PDF). The Journal of Navigation. Cambridge University Press. 63 (3): 395–417. Bibcode:2010JNav...63..395G. doi:10.1017/S0373463309990415.

External links [edit]

  • Weisstein, Eric W. "Inverse Tangent". MathWorld.

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Source: https://en.wikipedia.org/wiki/Inverse_trigonometric_functions