The functions sine, cosine and tangent of an angle are sometimes referred to as the primary or basic trigonometric functions. Their usual abbreviations are
and
respectively, where
denotes the angle. The parentheses around the argument of the functions are often omitted, e.g.,
and
if an interpretation is unambiguously possible.
The sine of an angle is defined, in the context of a right triangle, as the ratio of the length of the side that is opposite to the angle divided by the length of the longest side of the triangle (the hypotenuse).

The cosine of an angle in this context is the ratio of the length of the side that is adjacent to the angle divided by the length of the hypotenuse.

The tangent of an angle in this context is the ratio of the length of the side that is opposite to the angle divided by the length of the side that is adjacent to the angle. This is the same as the ratio of the sine to the cosine of this angle, as can be seen by substituting the definitions of
and Failed to parse (MathML with SVG or PNG fallback (recommended for modern browsers and accessibility tools): Invalid response ("Math extension cannot connect to Restbase.") from server "https://wikimedia.org/api/rest_v1/":): {\displaystyle \cos}
from above:

The remaining trigonometric functions secant (
), cosecant (
), and cotangent (Failed to parse (MathML with SVG or PNG fallback (recommended for modern browsers and accessibility tools): Invalid response ("Math extension cannot connect to Restbase.") from server "https://wikimedia.org/api/rest_v1/":): {\displaystyle \cot}
) are defined as the reciprocal functions of cosine, sine, and tangent, respectively. Rarely, these are called the secondary trigonometric functions:

These definitions are sometimes referred to as ratio identities.
Inverse trigonometric functions
The inverse trigonometric functions are partial inverse functions for the trigonometric functions. For example, the inverse function for the sine, known as the inverse sine (
) or arcsine (arcsin or asin), satisfies

and

This article will denote the inverse of a trigonometric function by prefixing its name with "Failed to parse (MathML with SVG or PNG fallback (recommended for modern browsers and accessibility tools): Invalid response ("Math extension cannot connect to Restbase.") from server "https://wikimedia.org/api/rest_v1/":): {\displaystyle \operatorname{arc}}
". The notation is shown in the table below.
Compositions of trig and inverse trig functions

Taking the multiplicative inverse of both sides of the each equation above results in the equations for
The right hand side of the formula above will always be flipped.
For example, the equation for
is:

while the equations for

and

are:

Solutions to elementary trigonometric equations
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
and
all lie within appropriate ranges so that the relevant expressions below are well-defined.
In the table below, "for some
" is just another way of saying "for some integer
"
Equation |
if and only if |
Solution |
where...
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for some
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|
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for some
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for some
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for some
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for some
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for some Failed to parse (MathML with SVG or PNG fallback (recommended for modern browsers and accessibility tools): Invalid response ("Math extension cannot connect to Restbase.") from server "https://wikimedia.org/api/rest_v1/":): {\displaystyle k \in \Z}
|
For example, if
then
for some
While if
then
for some
where
is even if
; odd if
The equations
and
have the same solutions as
and
respectively. In all equations above except for those just solved (i.e. except for
/
and
/
), for fixed
and
the integer
in the solution's formula is uniquely determined by
Other identities
These inverse trigonometric functions are related to one another by the formulas:
![{\displaystyle {\begin{alignedat}{9}{\frac {\pi }{2}}~&=~\arcsin(x)&&+\arccos(x)~&&=~\arctan(r)&&+\operatorname {arccot}(r)~&&=~\operatorname {arcsec}(s)&&+\operatorname {arccsc}(s)\\[0.4ex]\pi ~&=~\arccos(x)&&+\arccos(-x)~&&=~\operatorname {arccot}(r)&&+\operatorname {arccot}(-r)~&&=~\operatorname {arcsec}(s)&&+\operatorname {arcsec}(-s)\\[0.4ex]0~&=~\arcsin(x)&&+\arcsin(-x)~&&=~\arctan(r)&&+\arctan(-r)~&&=~\operatorname {arccsc}(s)&&+\operatorname {arccsc}(-s)\\[1.0ex]\end{alignedat}}}](https://wikimedia.org/api/rest_v1/media/math/render/svg/839db041f421b4af5890106450e2b4d3e9e183d4)
which hold whenever they are well-defined (that is, whenever

are in the domains of the relevant functions).





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