جيب (رياضيات)

نطقب:Infobox mathematics function

تحويل نطقب:حساب المثلثات

جيب Sine في الرياضيات هوالنسبة بين الضلع اللقاء لزاوية والوتر في مثلث ذوزاوية قائمة ، بحيثقد يكون الوتر هوالضلع اللقاء للزاوية القائمة.

في رياضيات، تعتبر التوابع مثلثية أوالدوال المثلثية دوال لزاوية هندسية، وهي دوال مهمة عندما نريد دراسة مثلث أوعرض ظواهرِ دورية. يمكن تعريف هذه الدوال كنسبة لأضلاع مثلث قائم الذي يَحتوي تلك الزاويةَ أَوبشكل أكثر عمومية كإحداثيات على دائرة مثلثية أودائرة واحدية (unit circle) . في الرياضيات ، الدوال المثلثية هي دوال ترتبط بالزاوية، وهي مهمة في دراسة المثلثات وتمثيل الظواهر المتكررة (كالموجات). ويمكن تعريف الدوال المثلثية على أنهم نسب بين ضلعين في مثلث قائم فيه الزاوية المعنية، او، وبشكل أوسع. كنسبة بين إحداثيات نقاط على دائرة الوحدة، ويعتبر دوما عند الإشارة إلى المثلثات ان الحديث يدور حول مثلث في سطح مستوي (مستوى إحداثي أوإقليدي) ، وذلك ليكون مجموع الزوايا 180 درجة دائما.

دالة جيب التمام.

وهناك ثلاثة دوال مثلثية أساسية هي:

جا أوالجيب ، ويساوي النسبة بين الضلع اللقاء للزاوية مقسوما على الوتر.
جتا أوجيب التمام ، ويساوي النسبة بين الضلع المجاور للزاوية مقسوما على الوتر.
ظا اوالظل ، ويساوي النسبية بين الضلع اللقاء للزاوية والضلع المجاور لها.

Identities

Exact identities (using radians):

These apply for all values of ${\displaystyle \theta$ .

{\displaystyle \sin(\theta )=\cos \left({\frac {\pi {2 -\theta \right)={\frac {1 {\csc(\theta )

Reciprocal

The reciprocal of sine is cosecant, i.e., the reciprocal of $sin(A)$ is $csc(A)$ , or cosec(A). Cosecant gives the ratio of the length of the hypotenuse to the length of the opposite side:

{\displaystyle \csc(A)={\frac {1 {\sin(A) ={\frac {\textrm {hypotenuse {\textrm {opposite ={\frac {h {a .

Inverse

The usual principal values of the

arcsin(x)

function graphed on the cartesian plane. Arcsin is the inverse of sin.

Calculus

For the sine function:

{\displaystyle f(x)=\sin(x)

The derivative is:

{\displaystyle f'(x)=\cos(x)

The antiderivative is:

{\displaystyle \int f(x)\,dx=-\cos x+C

C denotes the constant of integration.

Other trigonometric functions

The sine and cosine functions are related in multiple ways. The two functions are out of phase by 90°:

{\displaystyle \sin(\pi /2-x)

=

{\displaystyle \cos(x)

for all angles x. Also, the derivative of the function

sin(x)

is

cos(x)

.

It is possible to express any trigonometric function in terms of any other (up to a plus or minus sign, or using the sign function).

Sine in terms of the other common trigonometric functions:

	f θ	Using plus/minus (±)					Using sign function (sgn)
		f θ =	± per Quadrant				f θ =
		f θ =	I	II	III	IV	f θ =
cos	${\displaystyle \sin(\theta )$	${\displaystyle =\pm {\sqrt {1-\cos ^{2 (\theta )$	+	+	−	−	${\displaystyle =\operatorname {sgn \left(\cos \left(\theta -{\frac {\pi {2 \right)\right){\sqrt {1-\cos ^{2 (\theta )$
cos	${\displaystyle \cos(\theta )$	${\displaystyle =\pm {\sqrt {1-\sin ^{2 (\theta )$	+	−	−	+	${\displaystyle =\operatorname {sgn \left(\sin \left(\theta +{\frac {\pi {2 \right)\right){\sqrt {1-\sin ^{2 (\theta )$
cot	${\displaystyle \sin(\theta )$	${\displaystyle =\pm {\frac {1 {\sqrt {1+\cot ^{2 (\theta )$	+	+	−	−	${\displaystyle =\operatorname {sgn \left(\cot \left({\frac {\theta {2 \right)\right){\frac {1 {\sqrt {1+\cot ^{2 (\theta )$
cot	${\displaystyle \cot(\theta )$	${\displaystyle =\pm {\frac {\sqrt {1-\sin ^{2 (\theta ) {\sin(\theta )$	+	−	−	+	${\displaystyle =\operatorname {sgn \left(\sin \left(\theta +{\frac {\pi {2 \right)\right){\frac {\sqrt {1-\sin ^{2 (\theta ) {\sin(\theta )$
tan	${\displaystyle \sin(\theta )$	${\displaystyle =\pm {\frac {\tan(\theta ) {\sqrt {1+\tan ^{2 (\theta )$	+	−	−	+	${\displaystyle =\operatorname {sgn \left(\tan \left({\frac {2\theta +\pi {4 \right)\right){\frac {\tan(\theta ) {\sqrt {1+\tan ^{2 (\theta )$
tan	${\displaystyle \tan(\theta )$	${\displaystyle =\pm {\frac {\sin(\theta ) {\sqrt {1-\sin ^{2 (\theta )$	+	−	−	+	${\displaystyle =\operatorname {sgn \left(\sin \left(\theta +{\frac {\pi {2 \right)\right){\frac {\sin(\theta ) {\sqrt {1-\sin ^{2 (\theta )$
sec	${\displaystyle \sin(\theta )$	${\displaystyle =\pm {\frac {\sqrt {\sec ^{2 (\theta )-1 {\sec(\theta )$	+	−	+	−	${\displaystyle =\operatorname {sgn \left(\sec \left({\frac {4\theta -\pi {2 \right)\right){\frac {\sqrt {\sec ^{2 (\theta )-1 {\sec(\theta )$
sec	${\displaystyle \sec(\theta )$	${\displaystyle =\pm {\frac {1 {\sqrt {1-\sin ^{2 (\theta )$	+	−	−	+	${\displaystyle =\operatorname {sgn \left(\sin \left(\theta +{\frac {\pi {2 \right)\right){\frac {1 {\sqrt {1-\sin ^{2 (\theta )$

Note that for all equations which use plus/minus (±), the result is positive for angles in the first quadrant.

The basic relationship between the sine and the cosine can also be expressed as the Pythagorean trigonometric identity:

{\displaystyle \cos ^{2 (\theta )+\sin ^{2 (\theta )=1\!

where sin²x means (sin(x))².

Properties relating to the quadrants

The four quadrants of a Cartesian coordinate system.

Over the four quadrants of the sine function is as follows.

Quadrant	Degrees	Radians	Value	Sign	Monotony	Convexity
1st Quadrant	${\displaystyle 0^{\circ <x<90^{\circ$	${\displaystyle 0<x<{\frac {\pi {2$	${\displaystyle 0<\sin(x)<1$	${\displaystyle +$	increasing	concave
2nd Quadrant	${\displaystyle 90^{\circ <x<180^{\circ$	${\displaystyle {\frac {\pi {2 <x<\pi$	${\displaystyle 0<\sin(x)<1$	${\displaystyle +$	decreasing	concave
3rd Quadrant	${\displaystyle 180^{\circ <x<270^{\circ$	${\displaystyle \pi <x<{\frac {3\pi {2$	${\displaystyle -1<\sin(x)<0$	${\displaystyle -$	decreasing	convex
4th Quadrant	${\displaystyle 270^{\circ <x<360^{\circ$	${\displaystyle {\frac {3\pi {2 <x<2\pi$	${\displaystyle -1<\sin(x)<0$	${\displaystyle -$	increasing	convex

Points between the quadrants. k is an integer.

The quadrants of the unit circle and of sin x, using the Cartesian coordinate system.

Degrees	Radians ${\displaystyle 0\leq x<2\pi$	Radians	${\displaystyle \sin(x)$	Point type
${\displaystyle 0^{\circ$	${\displaystyle 0$	${\displaystyle 2\pi k$	${\displaystyle 0$	Root, Inflection
${\displaystyle 90^{\circ$	${\displaystyle {\frac {\pi {2$	${\displaystyle 2\pi k+{\frac {\pi {2$	${\displaystyle 1$	Maximum
${\displaystyle 180^{\circ$	${\displaystyle \pi$	${\displaystyle 2\pi k-\pi$	${\displaystyle 0$	Root, Inflection
${\displaystyle 270^{\circ$	${\displaystyle {\frac {3\pi {2$	${\displaystyle 2\pi k-{\frac {\pi {2$	${\displaystyle -1$	Minimum

For arguments outside those in the table, get the value using the fact the sine function has a period of 360° (or 2 $π$ rad): ${\displaystyle \sin(\alpha +360^{\circ )=\sin(\alpha )$ , or use ${\displaystyle \sin(\alpha +180^{\circ )=-\sin(\alpha )$ . Or use ${\displaystyle \cos(x)={\frac {e^{xi +e^{-xi {2$ and ${\displaystyle \sin(x)={\frac {e^{xi -e^{-xi {2i$ . For complement of sine, we have ${\displaystyle \sin(180^{\circ -\alpha )=\sin(\alpha )$ .

Series definition

The sine function (blue) is closely approximated by its Taylor polynomial of degreeسبعة (pink) for a full cycle centered on the origin.

This animation shows how including more and more terms in the partial sum of its Taylor series approaches a sine curve.

Using only geometry and properties of limits, it can be shown that the derivative of sine is cosine, and that the derivative of cosine is the negative of sine.

Using the reflection from the calculated geometric derivation of the sine is with the 4n + k-th derivative at the point 0:

{\displaystyle \sin ^{(4n+k) (0)={\begin{cases 0&{\text{when k=0\\1&{\text{when k=1\\0&{\text{when k=2\\-1&{\text{when k=3\end{cases

This gives the following Taylor series expansion at x = 0. One can then use the theory of Taylor series to show that the following identities hold for all real numbers x (where x is the angle in radians) :

{\displaystyle {\begin{aligned \sin x&=x-{\frac {x^{3 {3! +{\frac {x^{5 {5! -{\frac {x^{7 {7! +\cdots \\[8pt]&=\sum _{n=0 ^{\infty {\frac {(-1)^{n {(2n+1)! x^{2n+1 \\[8pt]\end{aligned

If x were expressed in degrees then the series would contain factors involving powers of π/180: if x is the number of degrees, the number of radians is y = πx /180, so

{\displaystyle {\begin{aligned \sin x_{\mathrm {deg &=\sin y_{\mathrm {rad \\&={\frac {\pi {180 x-\left({\frac {\pi {180 \right)^{3 {\frac {x^{3 {3! +\left({\frac {\pi {180 \right)^{5 {\frac {x^{5 {5! -\left({\frac {\pi {180 \right)^{7 {\frac {x^{7 {7! +\cdots .\end{aligned

The series formulas for the sine and cosine are uniquely determined, up to the choice of unit for angles, by the requirements that

{\displaystyle {\begin{aligned \sin 0=0&{\text{ and \sin {2x =2\sin x\cos x\\\cos ^{2 x+\sin ^{2 x=1&{\text{ and \cos {2x =\cos ^{2 x-\sin ^{2 x\\\end{aligned

The radian is the unit that leads to the expansion with leading coefficient 1 for the sine and is determined by the additional requirement that

{\displaystyle \sin x\approx x{\text{ when x\approx 0.

The coefficients for both the sine and cosine series may therefore be derived by substituting their expansions into the pythagorean and double angle identities, taking the leading coefficient for the sine to be 1, and matching the remaining coefficients.

In general, mathematically important relationships between the sine and cosine functions and the exponential function (see, for example, Euler's formula) are substantially simplified when angles are expressed in radians, rather than in degrees, grads or other units. Therefore, in most branches of mathematics beyond practical geometry, angles are generally assumed to be expressed in radians.

A similar series is Gregory's series for arctan, which is obtained by omitting the factorials in the denominator.

Continued fraction

The sine function can also be represented as a generalized continued fraction:

{\displaystyle \sin x={\cfrac {x {1+{\cfrac {x^{2 {2\cdot 3-x^{2 +{\cfrac {2\cdot 3x^{2 {4\cdot 5-x^{2 +{\cfrac {4\cdot 5x^{2 {6\cdot 7-x^{2 +\ddots .

The continued fraction representation can be derived from Euler's continued fraction formula and expresses the real number values, both rational and irrational, of the sine function.

Fixed point

The fixed point iteration x_n+1 = sin x_n with initial value x₀ = 2 converges to 0.

Zero is the only real fixed point of the sine function; in other words the only intersection of the sine function and the identity function is sin(0) = 0.

Arc length

The arc length of the sine curve between ${\displaystyle a$ and ${\displaystyle b$ is ${\displaystyle \int _{a ^{b \!{\sqrt {1+\cos(x)^{2 \,dx$ This integral is an elliptic integral of the second kind.

The arc length for a full period is ${\displaystyle {\frac {4\pi ^{3/2 {\sqrt {2 {\Gamma (1/4)^{2 +{\frac {\Gamma (1/4)^{2 {\sqrt {2\pi =7.640395578\ldots$ where ${\displaystyle 2\pi$

{\displaystyle 1.21600672\times x+0.10317093\sin(2x)-0.00220445\sin(4x)+0.00012584\sin(6x)-0.00001011\sin(8x)+\cdots

Law of sines

The law of sines states that for an arbitrary triangle with sides a, b, and c and angles opposite those sides A, B and C:

{\displaystyle {\frac {\sin A {a ={\frac {\sin B {b ={\frac {\sin C {c .

This is equivalent to the equality of the first three expressions below:

{\displaystyle {\frac {a {\sin A ={\frac {b {\sin B ={\frac {c {\sin C =2R,

where R is the triangle's circumradius.

It can be proven by dividing the triangle into two right ones and using the above definition of sine. The law of sines is useful for computing the lengths of the unknown sides in a triangle if two angles and one side are known. This is a common situation occurring in triangulation, a technique to determine unknown distances by measuring two angles and an accessible enclosed distance.

Special values

Some common angles (θ) shown on the unit circle. The angles are given in degrees and radians, together with the corresponding intersection point on the unit circle, (cos θ, sin θ).

For certain integral numbers x of degrees, the value of sin(x) is particularly simple. A table of some of these values is given below.

x (angle)				sin x
Degrees	Radians	Gradians	Turns	Exact	Decimal
0°	0	0^g	0	0	0
180°	π	200^g	1/2	0	0
15°	1/12π	16 2/3^g	1/24	${\displaystyle {\frac {{\sqrt {6 -{\sqrt {2 {4$	0.258819045102521
165°	11/12π	183 1/3^g	11/24	${\displaystyle {\frac {{\sqrt {6 -{\sqrt {2 {4$	0.258819045102521
30°	1/6π	33 1/3^g	1/12	1/2	0.5
150°	5/6π	166 2/3^g	5/12	1/2	0.5
45°	1/4π	50^g	1/8	${\displaystyle {\frac {\sqrt {2 {2$	0.707106781186548
135°	3/4π	150^g	3/8	${\displaystyle {\frac {\sqrt {2 {2$	0.707106781186548
60°	1/3π	66 2/3^g	1/6	${\displaystyle {\frac {\sqrt {3 {2$	0.866025403784439
120°	2/3π	133 1/3^g	1/3	${\displaystyle {\frac {\sqrt {3 {2$	0.866025403784439
75°	5/12π	83 1/3^g	5/24	${\displaystyle {\frac {{\sqrt {6 +{\sqrt {2 {4$	0.965925826289068
105°	7/12π	116 2/3^g	7/24	${\displaystyle {\frac {{\sqrt {6 +{\sqrt {2 {4$	0.965925826289068
90°	1/2π	100^g	1/4	1	1

90 degree increments:

x in degrees	0°	90°	180°	270°	360°
x in radians	0	π/2	π	3π/2	2π
x in gons	0	100^g	200^g	300^g	400^g
x in turns	0	1/4	1/2	3/4	1
sin x	0	1	0	-1	0

Other values not listed above:

{\displaystyle \sin {\frac {\pi {60 =\sin 3^{\circ ={\frac {(2-{\sqrt {12 ){\sqrt {5+{\sqrt {5 +({\sqrt {10 -{\sqrt {2 )({\sqrt {3 +1) {16

{\displaystyle \sin {\frac {\pi {30 =\sin 6^{\circ ={\frac {{\sqrt {30-{\sqrt {180 -{\sqrt {5 -1 {8

{\displaystyle \sin {\frac {\pi {20 =\sin 9^{\circ ={\frac {{\sqrt {10 +{\sqrt {2 -{\sqrt {20-{\sqrt {80 {8

{\displaystyle \sin {\frac {\pi {15 =\sin 12^{\circ ={\frac {{\sqrt {10+{\sqrt {20 +{\sqrt {3 -{\sqrt {15 {8

{\displaystyle \sin {\frac {\pi {10 =\sin 18^{\circ ={\frac {{\sqrt {5 -1 {4 ={\tfrac {1 {2 \varphi ^{-1

{\displaystyle \sin {\frac {7\pi {60 =\sin 21^{\circ ={\frac {(2+{\sqrt {12 ){\sqrt {5-{\sqrt {5 -({\sqrt {10 +{\sqrt {2 )({\sqrt {3 -1) {16

{\displaystyle \sin {\frac {\pi {8 =\sin 22.5^{\circ ={\frac {\sqrt {2-{\sqrt {2 {2

{\displaystyle \sin {\frac {2\pi {15 =\sin 24^{\circ ={\frac {{\sqrt {3 +{\sqrt {15 -{\sqrt {10-{\sqrt {20 {8

{\displaystyle \sin {\frac {3\pi {20 =\sin 27^{\circ ={\frac {{\sqrt {20+{\sqrt {80 -{\sqrt {10 +{\sqrt {2 {8

{\displaystyle \sin {\frac {11\pi {60 =\sin 33^{\circ ={\frac {({\sqrt {12 -2){\sqrt {5+{\sqrt {5 +({\sqrt {10 -{\sqrt {2 )({\sqrt {3 +1) {16

{\displaystyle \sin {\frac {\pi {5 =\sin 36^{\circ ={\frac {\sqrt {10-{\sqrt {20 {4

{\displaystyle \sin {\frac {13\pi {60 =\sin 39^{\circ ={\frac {(2-{\sqrt {12 ){\sqrt {5-{\sqrt {5 +({\sqrt {10 +{\sqrt {2 )({\sqrt {3 +1) {16

{\displaystyle \sin {\frac {7\pi {30 =\sin 42^{\circ ={\frac {{\sqrt {30+{\sqrt {180 -{\sqrt {5 +1 {8

Relationship to complex numbers

An illustration of the complex plane. The imaginary numbers are on the vertical coordinate axis.

Sine is used to determine the imaginary part of a complex number given in polar coordinates (r,φ):

{\displaystyle z=r(\cos \varphi +i\sin \varphi )

the imaginary part is:

{\displaystyle \operatorname {Im (z)=r\sin \varphi

r and φ represent the magnitude and angle of the complex number respectively. i is the imaginary unit. z is a complex number.

Although dealing with complex numbers, sine's parameter in this usage is still a real number. Sine can also take a complex number as an argument.

Sine with a complex argument

{\displaystyle \sin z

sin(z) as a vector field

{\displaystyle \sin(\theta )

is the imaginary part of

{\displaystyle \mathrm {e ^{\mathrm {i \theta

.

The definition of the sine function for complex arguments z:

{\displaystyle {\begin{aligned \sin z&=\sum _{n=0 ^{\infty {\frac {(-1)^{n {(2n+1)! z^{2n+1 \\&={\frac {e^{iz -e^{-iz {2i \\&={\frac {\sinh \left(iz\right) {i \end{aligned

where i² = −1, and sinh is hyperbolic sine. This is an entire function. Also, for purely real x,

{\displaystyle \sin x=\operatorname {Im (e^{ix ).

For purely imaginary numbers:

{\displaystyle \sin iy=i\sinh y.

It is also sometimes useful to express the complex sine function in terms of the real and imaginary parts of its argument:

{\displaystyle {\begin{aligned \sin(x+iy)&=\sin x\cos iy+\cos x\sin iy\\&=\sin x\cosh y+i\cos x\sinh y.\end{aligned

Partial fraction and product expansions of complex sine

Using the partial fraction expansion technique in complex analysis, one can find that the infinite series

{\displaystyle {\begin{aligned \sum _{n=-\infty ^{\infty {\frac {(-1)^{n {z-n ={\frac {1 {z -2z\sum _{n=1 ^{\infty {\frac {(-1)^{n {n^{2 -z^{2 \end{aligned

both converge and are equal to ${\displaystyle {\frac {\pi {\sin \pi z$ . Similarly, one can show that

{\displaystyle {\begin{aligned {\frac {\pi ^{2 {\sin ^{2 (\pi z) =\sum _{n=-\infty ^{\infty {\frac {1 {(z-n)^{2 .\end{aligned

Using product expansion technique, one can derive

{\displaystyle {\begin{aligned \sin \pi z=\pi z\prod _{n=1 ^{\infty {\Bigl ( 1-{\frac {z^{2 {n^{2 {\Bigr ) .\end{aligned

Usage of complex sine

sin z is found in the functional equation for the Gamma function,

{\displaystyle \Gamma (s)\Gamma (1-s)={\pi \over \sin \pi s ,

which in turn is found in the functional equation for the Riemann zeta-function,

{\displaystyle \zeta (s)=2(2\pi )^{s-1 \Gamma (1-s)\sin(\pi s/2)\zeta (1-s).

As a holomorphic function, sin z is a 2D solution of Laplace's equation:

{\displaystyle \Delta u(x_{1 ,x_{2 )=0.

It is also related with level curves of pendulum.

Complex graphs

**Sine function in the complex plane**

real component	imaginary component	magnitude

**Arcsine function in the complex plane**

real component	imaginary component	magnitude

History

While the early study of trigonometry can be traced to antiquity, the trigonometric functions as they are in use today were developed in the medieval period. The chord function was discovered by Hipparchus of Nicaea (180–125 BCE) and Ptolemy of Roman Egypt (90–165 CE).

The function sine (and cosine) can be traced to the functions used in Gupta period (320 to 550 CE) Indian astronomy (Aryabhatiya, Surya Siddhanta), via translation from Sanskrit to Arabic and then from Arabic to Latin.

The first published use of the abbreviations 'sin', 'cos', and 'tan' is by the 16th century French mathematician Albert Girard; these were further promulgated by Euler (see below). The Opus palatinum de triangulis of Georg Joachim Rheticus, a student of Copernicus, was probably the first in Europe to define trigonometric functions directly in terms of right triangles instead of circles, with tables for all six trigonometric functions; this work was finished by Rheticus' student Valentin Otho in 1596.

In a paper published in 1682, Leibniz proved that sin x is not an algebraic function of x.Roger Cotes computed the derivative of sine in his Harmonia Mensurarum (1722).Leonhard Euler's Introductio in analysin infinitorum (1748) was mostly responsible for establishing the analytic treatment of trigonometric functions in Europe, also defining them as infinite series and presenting "Euler's formula", as well as the near-modern abbreviations sin., cos., tang., cot., sec., and cosec.

Etymology

Etymologically, the word sine derives from the Sanskrit word for chord, jiva*(jya being its more popular synonym). This was transliterated in Arabic as jiba جــيــب, which however is meaningless in that language and abbreviated jb جــــب . Since Arabic is written without short vowels, "jb" was interpreted as the word jaib جــيــب, which means "bosom". When the Arabic texts were translated in the 12th century into Latin by Gerard of Cremona, he used the Latin equivalent for "bosom", sinus (which means "bosom" or "bay" or "fold"). Gerard was probably not the first scholar to use this translation, Robert of Chester appears to have preceded him and there is evidence of even earlier usage. The English form sine was introduced in the 1590s.

Software implementations

The sine function, along with other trigonometric functions, is widely available across programming languages and platforms. In computing, it is typically abbreviated to sin.

Some CPU architectures have a built-in instruction for sine, including the Intel x87 FPUs since the 80387.

In programming languages, sin is typically either a built-in function or found within the language's standard math library.

For example, the C standard library defines sine functions within math.h: sin(double), sinf(float), and sinl(long double). The parameter of each is a floating point value, specifying the angle in radians. Each function returns the same data type as it accepts. Many other trigonometric functions are also defined in math.h, such as for cosine, arc sine, and hyperbolic sine (sinh).

Similarly, Python defines math.sin(x) within the built-in math module. Complex sine functions are also available within the cmath module, e.g. cmath.sin(z). CPython's math functions call the C math library, and use a double-precision floating-point format.

There is no standard algorithm for calculating sine. IEEE 754-2008, the most widely used standard for floating-point computation, does not address calculating trigonometric functions such as sine. Algorithms for calculating sine may be balanced for such constraints as speed, accuracy, portability, or range of input values accepted. This can lead to different results for different algorithms, especially for special circumstances such as very large inputs, e.g. sin(1022 ).

A once common programming optimization, used especially in 3D graphics, was to pre-calculate a table of sine values, for example one value per degree. This allowed results to be looked up from a table rather than being calculated in real time. With modern CPU architectures this method may offer no advantage.^[]

The CORDIC algorithm is commonly used in scientific calculators.

انظر أيضاً

Āryabhaṭa's sine table
Bhaskara I's sine approximation formula
Discrete sine transform
Euler's formula
Generalized trigonometry
Hyperbolic function
Law of sines
List of periodic functions
List of trigonometric identities
Madhava series
Madhava's sine table
Optical sine theorem
Polar sine — a generalization to vertex angles
Proofs of trigonometric identities
Sinc function
Sine and cosine transforms
Sine integral
Sine quadrant
Sine wave
Sine–Gordon equation
Sinusoidal model
Trigonometric functions

Notes

^ See Ahlfors, pages 43–44.
^ math.stackexchange questions : why-are-the-phase-portrait-of-the-simple-plane-pendulum-and-a-domain-coloring-of ... Archived 2014-03-30 at the Wayback Machine.
^ خطأ استشهاد: وسم <ref> غير سليم؛ لا نص تم توفيره للمراجع المسماة Boyer, Carl B. 1991 p. 210
^ Nicolás Bourbaki (1994). Elements of the History of Mathematics. Springer.
^ "Why the sine has a simple derivative Archived 2011-07-20 at the Wayback Machine.", in Historical Notes for Calculus Teachers Archived 2011-07-20 at the Wayback Machine. by V. Frederick Rickey Archived 2011-07-20 at the Wayback Machine.
^ See Merzbach, Boyer (2011).
^ Eli Maor (1998), Trigonometric Delights, Princeton: Princeton University Press, p. 35-36.
^ Victor J. Katz (2008), A History of Mathematics, Boston: Addison-Wesley, 3rd. ed., p. 253, sidebar 8.1. "Archived copy" (PDF). Archived (PDF) from the original on 2015-04-14. Retrieved 2015-04-09. CS1 maint: archived copy as title (link)
^ Smith, D.E. (1958) [1925], History of Mathematics, I, Dover, p. 202, ISBN 0-486-20429-4
^ Grand Challenges of Informatics, Paul Zimmermann. September 20, 2006 – p. 14/31 "Archived copy" (PDF). Archived (PDF) from the original on 2011-07-16. Retrieved 2010-09-11. CS1 maint: archived copy as title (link)

References

Traupman, John C. (1966), The New College Latin & English Dictionary, Toronto: Bantam, ISBN 0-553-27619-0
Webster's Seventh New Collegiate Dictionary, Springfield: G. & C. Merriam Company, 1969