Perl 5 version 8.9 documentation

- NAME
- SYNOPSIS
- DESCRIPTION
- TRIGONOMETRIC FUNCTIONS
- PLANE ANGLE CONVERSIONS
- RADIAL COORDINATE CONVERSIONS
- GREAT CIRCLE DISTANCES AND DIRECTIONS
- EXAMPLES
- BUGS
- AUTHORS
- LICENSE

Math::Trig - trigonometric functions

- use Math::Trig;
- $x = tan(0.9);
- $y = acos(3.7);
- $z = asin(2.4);
- $halfpi = pi/2;
- $rad = deg2rad(120);
- # Import constants pi2, pip2, pip4 (2*pi, pi/2, pi/4).
- use Math::Trig ':pi';
- # Import the conversions between cartesian/spherical/cylindrical.
- use Math::Trig ':radial';
- # Import the great circle formulas.
- use Math::Trig ':great_circle';

`Math::Trig`

defines many trigonometric functions not defined by the
core Perl which defines only the `sin()`

and `cos()`

. The constant
**pi** is also defined as are a few convenience functions for angle
conversions, and *great circle formulas* for spherical movement.

The tangent

The cofunctions of the sine, cosine, and tangent (cosec/csc and cotan/cot are aliases)

**csc**, **cosec**, **sec**, **sec**, **cot**, **cotan**

The arcus (also known as the inverse) functions of the sine, cosine, and tangent

**asin**, **acos**, **atan**

The principal value of the arc tangent of y/x

**atan2**(y, x)

The arcus cofunctions of the sine, cosine, and tangent (acosec/acsc and acotan/acot are aliases). Note that atan2(0, 0) is not well-defined.

**acsc**, **acosec**, **asec**, **acot**, **acotan**

The hyperbolic sine, cosine, and tangent

**sinh**, **cosh**, **tanh**

The cofunctions of the hyperbolic sine, cosine, and tangent (cosech/csch and cotanh/coth are aliases)

**csch**, **cosech**, **sech**, **coth**, **cotanh**

The area (also known as the inverse) functions of the hyperbolic sine, cosine, and tangent

**asinh**, **acosh**, **atanh**

The area cofunctions of the hyperbolic sine, cosine, and tangent (acsch/acosech and acoth/acotanh are aliases)

**acsch**, **acosech**, **asech**, **acoth**, **acotanh**

The trigonometric constant **pi** and some of handy multiples
of it are also defined.

**pi, pi2, pi4, pip2, pip4**

The following functions

- acoth
- acsc
- acsch
- asec
- asech
- atanh
- cot
- coth
- csc
- csch
- sec
- sech
- tan
- tanh

cannot be computed for all arguments because that would mean dividing by zero or taking logarithm of zero. These situations cause fatal runtime errors looking like this

- cot(0): Division by zero.
- (Because in the definition of cot(0), the divisor sin(0) is 0)
- Died at ...

or

- atanh(-1): Logarithm of zero.
- Died at...

For the `csc`

, `cot`

, `asec`

, `acsc`

, `acot`

, `csch`

, `coth`

,
`asech`

, `acsch`

, the argument cannot be `0`

(zero). For the
`atanh`

, `acoth`

, the argument cannot be `1`

(one). For the
`atanh`

, `acoth`

, the argument cannot be `-1`

(minus one). For the
`tan`

, `sec`

, `tanh`

, `sech`

, the argument cannot be *pi/2 + k *
pi*, where *k* is any integer.

Note that atan2(0, 0) is not well-defined.

Please note that some of the trigonometric functions can break out
from the **real axis** into the **complex plane**. For example
`asin(2)`

has no definition for plain real numbers but it has
definition for complex numbers.

In Perl terms this means that supplying the usual Perl numbers (also known as scalars, please see perldata) as input for the trigonometric functions might produce as output results that no more are simple real numbers: instead they are complex numbers.

The `Math::Trig`

handles this by using the `Math::Complex`

package
which knows how to handle complex numbers, please see Math::Complex
for more information. In practice you need not to worry about getting
complex numbers as results because the `Math::Complex`

takes care of
details like for example how to display complex numbers. For example:

- print asin(2), "\n";

should produce something like this (take or leave few last decimals):

- 1.5707963267949-1.31695789692482i

That is, a complex number with the real part of approximately `1.571`

and the imaginary part of approximately `-1.317`

.

(Plane, 2-dimensional) angles may be converted with the following functions.

**deg2rad**- $radians = deg2rad($degrees);

**grad2rad**- $radians = grad2rad($gradians);

**rad2deg**- $degrees = rad2deg($radians);

**grad2deg**- $degrees = grad2deg($gradians);

**deg2grad**- $gradians = deg2grad($degrees);

**rad2grad**- $gradians = rad2grad($radians);

The full circle is 2 *pi* radians or *360* degrees or *400* gradians.
The result is by default wrapped to be inside the [0, {2pi,360,400}[ circle.
If you don't want this, supply a true second argument:

- $zillions_of_radians = deg2rad($zillions_of_degrees, 1);
- $negative_degrees = rad2deg($negative_radians, 1);

You can also do the wrapping explicitly by rad2rad(), deg2deg(), and grad2grad().

**rad2rad**- $radians_wrapped_by_2pi = rad2rad($radians);

**deg2deg**- $degrees_wrapped_by_360 = deg2deg($degrees);

**grad2grad**- $gradians_wrapped_by_400 = grad2grad($gradians);

**Radial coordinate systems** are the **spherical** and the **cylindrical**
systems, explained shortly in more detail.

You can import radial coordinate conversion functions by using the
`:radial`

tag:

- use Math::Trig ':radial';
- ($rho, $theta, $z) = cartesian_to_cylindrical($x, $y, $z);
- ($rho, $theta, $phi) = cartesian_to_spherical($x, $y, $z);
- ($x, $y, $z) = cylindrical_to_cartesian($rho, $theta, $z);
- ($rho_s, $theta, $phi) = cylindrical_to_spherical($rho_c, $theta, $z);
- ($x, $y, $z) = spherical_to_cartesian($rho, $theta, $phi);
- ($rho_c, $theta, $z) = spherical_to_cylindrical($rho_s, $theta, $phi);

**All angles are in radians**.

**Cartesian** coordinates are the usual rectangular *(x, y, z)*-coordinates.

Spherical coordinates, *(rho, theta, pi)*, are three-dimensional
coordinates which define a point in three-dimensional space. They are
based on a sphere surface. The radius of the sphere is **rho**, also
known as the *radial* coordinate. The angle in the *xy*-plane
(around the *z*-axis) is **theta**, also known as the *azimuthal*
coordinate. The angle from the *z*-axis is **phi**, also known as the
*polar* coordinate. The North Pole is therefore *0, 0, rho*, and
the Gulf of Guinea (think of the missing big chunk of Africa) *0,
pi/2, rho*. In geographical terms *phi* is latitude (northward
positive, southward negative) and *theta* is longitude (eastward
positive, westward negative).

**BEWARE**: some texts define *theta* and *phi* the other way round,
some texts define the *phi* to start from the horizontal plane, some
texts use *r* in place of *rho*.

Cylindrical coordinates, *(rho, theta, z)*, are three-dimensional
coordinates which define a point in three-dimensional space. They are
based on a cylinder surface. The radius of the cylinder is **rho**,
also known as the *radial* coordinate. The angle in the *xy*-plane
(around the *z*-axis) is **theta**, also known as the *azimuthal*
coordinate. The third coordinate is the *z*, pointing up from the
**theta**-plane.

Conversions to and from spherical and cylindrical coordinates are
available. Please notice that the conversions are not necessarily
reversible because of the equalities like *pi* angles being equal to
*-pi* angles.

**cartesian_to_cylindrical**- ($rho, $theta, $z) = cartesian_to_cylindrical($x, $y, $z);

**cartesian_to_spherical**- ($rho, $theta, $phi) = cartesian_to_spherical($x, $y, $z);

**cylindrical_to_cartesian**- ($x, $y, $z) = cylindrical_to_cartesian($rho, $theta, $z);

**cylindrical_to_spherical**- ($rho_s, $theta, $phi) = cylindrical_to_spherical($rho_c, $theta, $z);

Notice that when

`$z`

is not 0`$rho_s`

is not equal to`$rho_c`

.**spherical_to_cartesian**- ($x, $y, $z) = spherical_to_cartesian($rho, $theta, $phi);

**spherical_to_cylindrical**- ($rho_c, $theta, $z) = spherical_to_cylindrical($rho_s, $theta, $phi);

Notice that when

`$z`

is not 0`$rho_c`

is not equal to`$rho_s`

.

A great circle is section of a circle that contains the circle diameter: the shortest distance between two (non-antipodal) points on the spherical surface goes along the great circle connecting those two points.

You can compute spherical distances, called **great circle distances**,
by importing the great_circle_distance() function:

- use Math::Trig 'great_circle_distance';
- $distance = great_circle_distance($theta0, $phi0, $theta1, $phi1, [, $rho]);

The *great circle distance* is the shortest distance between two
points on a sphere. The distance is in `$rho`

units. The `$rho`

is
optional, it defaults to 1 (the unit sphere), therefore the distance
defaults to radians.

If you think geographically the *theta* are longitudes: zero at the
Greenwhich meridian, eastward positive, westward negative -- and the
*phi* are latitudes: zero at the North Pole, northward positive,
southward negative. **NOTE**: this formula thinks in mathematics, not
geographically: the *phi* zero is at the North Pole, not at the
Equator on the west coast of Africa (Bay of Guinea). You need to
subtract your geographical coordinates from *pi/2* (also known as 90
degrees).

- $distance = great_circle_distance($lon0, pi/2 - $lat0,
- $lon1, pi/2 - $lat1, $rho);

The direction you must follow the great circle (also known as *bearing*)
can be computed by the great_circle_direction() function:

- use Math::Trig 'great_circle_direction';
- $direction = great_circle_direction($theta0, $phi0, $theta1, $phi1);

Alias 'great_circle_bearing' for 'great_circle_direction' is also available.

- use Math::Trig 'great_circle_bearing';
- $direction = great_circle_bearing($theta0, $phi0, $theta1, $phi1);

The result of great_circle_direction is in radians, zero indicating straight north, pi or -pi straight south, pi/2 straight west, and -pi/2 straight east.

You can inversely compute the destination if you know the starting point, direction, and distance:

- use Math::Trig 'great_circle_destination';
- # $diro is the original direction,
- # for example from great_circle_bearing().
- # $distance is the angular distance in radians,
- # for example from great_circle_distance().
- # $thetad and $phid are the destination coordinates,
- # $dird is the final direction at the destination.
- ($thetad, $phid, $dird) =
- great_circle_destination($theta, $phi, $diro, $distance);

or the midpoint if you know the end points:

- use Math::Trig 'great_circle_midpoint';
- ($thetam, $phim) =
- great_circle_midpoint($theta0, $phi0, $theta1, $phi1);

The great_circle_midpoint() is just a special case of

- use Math::Trig 'great_circle_waypoint';
- ($thetai, $phii) =
- great_circle_waypoint($theta0, $phi0, $theta1, $phi1, $way);

Where the $way is a value from zero ($theta0, $phi0) to one ($theta1,
$phi1). Note that antipodal points (where their distance is *pi*
radians) do not have waypoints between them (they would have an an
"equator" between them), and therefore `undef`

is returned for
antipodal points. If the points are the same and the distance
therefore zero and all waypoints therefore identical, the first point
(either point) is returned.

The thetas, phis, direction, and distance in the above are all in radians.

You can import all the great circle formulas by

- use Math::Trig ':great_circle';

Notice that the resulting directions might be somewhat surprising if
you are looking at a flat worldmap: in such map projections the great
circles quite often do not look like the shortest routes -- but for
example the shortest possible routes from Europe or North America to
Asia do often cross the polar regions. (The common Mercator projection
does **not** show great circles as straight lines: straight lines in the
Mercator projection are lines of constant bearing.)

To calculate the distance between London (51.3N 0.5W) and Tokyo (35.7N 139.8E) in kilometers:

The direction you would have to go from London to Tokyo (in radians, straight north being zero, straight east being pi/2).

The midpoint between London and Tokyo being

or about 69 N 89 E, in the frozen wastes of Siberia.

**NOTE**: you **cannot** get from A to B like this:

- Dist = great_circle_distance(A, B)
- Dir = great_circle_direction(A, B)
- C = great_circle_destination(A, Dist, Dir)

and expect C to be B, because the bearing constantly changes when going from A to B (except in some special case like the meridians or the circles of latitudes) and in great_circle_destination() one gives a constant bearing to follow.

The answers may be off by few percentages because of the irregular (slightly aspherical) form of the Earth. The errors are at worst about 0.55%, but generally below 0.3%.

For small inputs asin() and acos() may return complex numbers even when real numbers would be enough and correct, this happens because of floating-point inaccuracies. You can see these inaccuracies for example by trying theses:

which will print something like this

- -1.11022302462516e-16
- 0.99999999999999988898

even though the expected results are of course exactly zero and one. The formulas used to compute asin() and acos() are quite sensitive to this, and therefore they might accidentally slip into the complex plane even when they should not. To counter this there are two interfaces that are guaranteed to return a real-valued output.

**asin_real**- use Math::Trig qw(asin_real);
- $real_angle = asin_real($input_sin);

Return a real-valued arcus sine if the input is between [-1, 1],

**inclusive**the endpoints. For inputs greater than one, pi/2 is returned. For inputs less than minus one, -pi/2 is returned.**acos_real**- use Math::Trig qw(acos_real);
- $real_angle = acos_real($input_cos);

Return a real-valued arcus cosine if the input is between [-1, 1],

**inclusive**the endpoints. For inputs greater than one, zero is returned. For inputs less than minus one, pi is returned.

Saying `use Math::Trig;`

exports many mathematical routines in the
caller environment and even overrides some (`sin`

, `cos`

). This is
construed as a feature by the Authors, actually... ;-)

The code is not optimized for speed, especially because we use
`Math::Complex`

and thus go quite near complex numbers while doing
the computations even when the arguments are not. This, however,
cannot be completely avoided if we want things like `asin(2)`

to give
an answer instead of giving a fatal runtime error.

Do not attempt navigation using these formulas.

Jarkko Hietaniemi <*jhi!at!iki.fi*> and
Raphael Manfredi <*Raphael_Manfredi!at!pobox.com*>.

This library is free software; you can redistribute it and/or modify it under the same terms as Perl itself.