2 # Trigonometric functions, mostly inherited from Math::Complex.
3 # -- Jarkko Hietaniemi, since April 1997
4 # -- Raphael Manfredi, September 1996 (indirectly: because of Math::Complex)
13 use Math::Complex qw(:trig);
15 our($VERSION, $PACKAGE, @ISA, @EXPORT, @EXPORT_OK, %EXPORT_TAGS);
21 my @angcnv = qw(rad2deg rad2grad
25 @EXPORT = (@{$Math::Complex::EXPORT_TAGS{'trig'}},
28 my @rdlcnv = qw(cartesian_to_cylindrical
29 cartesian_to_spherical
30 cylindrical_to_cartesian
31 cylindrical_to_spherical
32 spherical_to_cartesian
33 spherical_to_cylindrical);
35 @EXPORT_OK = (@rdlcnv, 'great_circle_distance', 'great_circle_direction');
37 %EXPORT_TAGS = ('radial' => [ @rdlcnv ]);
40 sub pip2 () { pi / 2 }
50 # Truncating remainder.
54 # Oh yes, POSIX::fmod() would be faster. Possibly. If it is available.
55 $_[0] - $_[1] * int($_[0] / $_[1]);
62 sub rad2rad($) { remt($_[0], pi2) }
64 sub deg2deg($) { remt($_[0], 360) }
66 sub grad2grad($) { remt($_[0], 400) }
68 sub rad2deg ($;$) { my $d = RD * $_[0]; $_[1] ? $d : deg2deg($d) }
70 sub deg2rad ($;$) { my $d = DR * $_[0]; $_[1] ? $d : rad2rad($d) }
72 sub grad2deg ($;$) { my $d = GD * $_[0]; $_[1] ? $d : deg2deg($d) }
74 sub deg2grad ($;$) { my $d = DG * $_[0]; $_[1] ? $d : grad2grad($d) }
76 sub rad2grad ($;$) { my $d = RG * $_[0]; $_[1] ? $d : grad2grad($d) }
78 sub grad2rad ($;$) { my $d = GR * $_[0]; $_[1] ? $d : rad2rad($d) }
80 sub cartesian_to_spherical {
81 my ( $x, $y, $z ) = @_;
83 my $rho = sqrt( $x * $x + $y * $y + $z * $z );
87 $rho ? acos( $z / $rho ) : 0 );
90 sub spherical_to_cartesian {
91 my ( $rho, $theta, $phi ) = @_;
93 return ( $rho * cos( $theta ) * sin( $phi ),
94 $rho * sin( $theta ) * sin( $phi ),
98 sub spherical_to_cylindrical {
99 my ( $x, $y, $z ) = spherical_to_cartesian( @_ );
101 return ( sqrt( $x * $x + $y * $y ), $_[1], $z );
104 sub cartesian_to_cylindrical {
105 my ( $x, $y, $z ) = @_;
107 return ( sqrt( $x * $x + $y * $y ), atan2( $y, $x ), $z );
110 sub cylindrical_to_cartesian {
111 my ( $rho, $theta, $z ) = @_;
113 return ( $rho * cos( $theta ), $rho * sin( $theta ), $z );
116 sub cylindrical_to_spherical {
117 return ( cartesian_to_spherical( cylindrical_to_cartesian( @_ ) ) );
120 sub great_circle_distance {
121 my ( $theta0, $phi0, $theta1, $phi1, $rho ) = @_;
123 $rho = 1 unless defined $rho; # Default to the unit sphere.
125 my $lat0 = pip2 - $phi0;
126 my $lat1 = pip2 - $phi1;
129 acos(cos( $lat0 ) * cos( $lat1 ) * cos( $theta0 - $theta1 ) +
130 sin( $lat0 ) * sin( $lat1 ) );
133 sub great_circle_direction {
134 my ( $theta0, $phi0, $theta1, $phi1 ) = @_;
136 my $lat0 = pip2 - $phi0;
137 my $lat1 = pip2 - $phi1;
140 atan2(sin($theta0 - $theta1) * cos($lat1),
141 cos($lat0) * sin($lat1) -
142 sin($lat0) * cos($lat1) * cos($theta0 - $theta1));
144 return rad2rad($direction);
151 Math::Trig - trigonometric functions
167 C<Math::Trig> defines many trigonometric functions not defined by the
168 core Perl which defines only the C<sin()> and C<cos()>. The constant
169 B<pi> is also defined as are a few convenience functions for angle
172 =head1 TRIGONOMETRIC FUNCTIONS
182 The cofunctions of the sine, cosine, and tangent (cosec/csc and cotan/cot
185 B<csc>, B<cosec>, B<sec>, B<sec>, B<cot>, B<cotan>
187 The arcus (also known as the inverse) functions of the sine, cosine,
190 B<asin>, B<acos>, B<atan>
192 The principal value of the arc tangent of y/x
196 The arcus cofunctions of the sine, cosine, and tangent (acosec/acsc
197 and acotan/acot are aliases)
199 B<acsc>, B<acosec>, B<asec>, B<acot>, B<acotan>
201 The hyperbolic sine, cosine, and tangent
203 B<sinh>, B<cosh>, B<tanh>
205 The cofunctions of the hyperbolic sine, cosine, and tangent (cosech/csch
206 and cotanh/coth are aliases)
208 B<csch>, B<cosech>, B<sech>, B<coth>, B<cotanh>
210 The arcus (also known as the inverse) functions of the hyperbolic
211 sine, cosine, and tangent
213 B<asinh>, B<acosh>, B<atanh>
215 The arcus cofunctions of the hyperbolic sine, cosine, and tangent
216 (acsch/acosech and acoth/acotanh are aliases)
218 B<acsch>, B<acosech>, B<asech>, B<acoth>, B<acotanh>
220 The trigonometric constant B<pi> is also defined.
224 =head2 ERRORS DUE TO DIVISION BY ZERO
226 The following functions
243 cannot be computed for all arguments because that would mean dividing
244 by zero or taking logarithm of zero. These situations cause fatal
245 runtime errors looking like this
247 cot(0): Division by zero.
248 (Because in the definition of cot(0), the divisor sin(0) is 0)
253 atanh(-1): Logarithm of zero.
256 For the C<csc>, C<cot>, C<asec>, C<acsc>, C<acot>, C<csch>, C<coth>,
257 C<asech>, C<acsch>, the argument cannot be C<0> (zero). For the
258 C<atanh>, C<acoth>, the argument cannot be C<1> (one). For the
259 C<atanh>, C<acoth>, the argument cannot be C<-1> (minus one). For the
260 C<tan>, C<sec>, C<tanh>, C<sech>, the argument cannot be I<pi/2 + k *
261 pi>, where I<k> is any integer.
263 =head2 SIMPLE (REAL) ARGUMENTS, COMPLEX RESULTS
265 Please note that some of the trigonometric functions can break out
266 from the B<real axis> into the B<complex plane>. For example
267 C<asin(2)> has no definition for plain real numbers but it has
268 definition for complex numbers.
270 In Perl terms this means that supplying the usual Perl numbers (also
271 known as scalars, please see L<perldata>) as input for the
272 trigonometric functions might produce as output results that no more
273 are simple real numbers: instead they are complex numbers.
275 The C<Math::Trig> handles this by using the C<Math::Complex> package
276 which knows how to handle complex numbers, please see L<Math::Complex>
277 for more information. In practice you need not to worry about getting
278 complex numbers as results because the C<Math::Complex> takes care of
279 details like for example how to display complex numbers. For example:
283 should produce something like this (take or leave few last decimals):
285 1.5707963267949-1.31695789692482i
287 That is, a complex number with the real part of approximately C<1.571>
288 and the imaginary part of approximately C<-1.317>.
290 =head1 PLANE ANGLE CONVERSIONS
292 (Plane, 2-dimensional) angles may be converted with the following functions.
294 $radians = deg2rad($degrees);
295 $radians = grad2rad($gradians);
297 $degrees = rad2deg($radians);
298 $degrees = grad2deg($gradians);
300 $gradians = deg2grad($degrees);
301 $gradians = rad2grad($radians);
303 The full circle is 2 I<pi> radians or I<360> degrees or I<400> gradians.
304 The result is by default wrapped to be inside the [0, {2pi,360,400}[ circle.
305 If you don't want this, supply a true second argument:
307 $zillions_of_radians = deg2rad($zillions_of_degrees, 1);
308 $negative_degrees = rad2deg($negative_radians, 1);
310 You can also do the wrapping explicitly by rad2rad(), deg2deg(), and
313 =head1 RADIAL COORDINATE CONVERSIONS
315 B<Radial coordinate systems> are the B<spherical> and the B<cylindrical>
316 systems, explained shortly in more detail.
318 You can import radial coordinate conversion functions by using the
321 use Math::Trig ':radial';
323 ($rho, $theta, $z) = cartesian_to_cylindrical($x, $y, $z);
324 ($rho, $theta, $phi) = cartesian_to_spherical($x, $y, $z);
325 ($x, $y, $z) = cylindrical_to_cartesian($rho, $theta, $z);
326 ($rho_s, $theta, $phi) = cylindrical_to_spherical($rho_c, $theta, $z);
327 ($x, $y, $z) = spherical_to_cartesian($rho, $theta, $phi);
328 ($rho_c, $theta, $z) = spherical_to_cylindrical($rho_s, $theta, $phi);
330 B<All angles are in radians>.
332 =head2 COORDINATE SYSTEMS
334 B<Cartesian> coordinates are the usual rectangular I<(x, y,
337 Spherical coordinates, I<(rho, theta, pi)>, are three-dimensional
338 coordinates which define a point in three-dimensional space. They are
339 based on a sphere surface. The radius of the sphere is B<rho>, also
340 known as the I<radial> coordinate. The angle in the I<xy>-plane
341 (around the I<z>-axis) is B<theta>, also known as the I<azimuthal>
342 coordinate. The angle from the I<z>-axis is B<phi>, also known as the
343 I<polar> coordinate. The `North Pole' is therefore I<0, 0, rho>, and
344 the `Bay of Guinea' (think of the missing big chunk of Africa) I<0,
345 pi/2, rho>. In geographical terms I<phi> is latitude (northward
346 positive, southward negative) and I<theta> is longitude (eastward
347 positive, westward negative).
349 B<BEWARE>: some texts define I<theta> and I<phi> the other way round,
350 some texts define the I<phi> to start from the horizontal plane, some
351 texts use I<r> in place of I<rho>.
353 Cylindrical coordinates, I<(rho, theta, z)>, are three-dimensional
354 coordinates which define a point in three-dimensional space. They are
355 based on a cylinder surface. The radius of the cylinder is B<rho>,
356 also known as the I<radial> coordinate. The angle in the I<xy>-plane
357 (around the I<z>-axis) is B<theta>, also known as the I<azimuthal>
358 coordinate. The third coordinate is the I<z>, pointing up from the
361 =head2 3-D ANGLE CONVERSIONS
363 Conversions to and from spherical and cylindrical coordinates are
364 available. Please notice that the conversions are not necessarily
365 reversible because of the equalities like I<pi> angles being equal to
370 =item cartesian_to_cylindrical
372 ($rho, $theta, $z) = cartesian_to_cylindrical($x, $y, $z);
374 =item cartesian_to_spherical
376 ($rho, $theta, $phi) = cartesian_to_spherical($x, $y, $z);
378 =item cylindrical_to_cartesian
380 ($x, $y, $z) = cylindrical_to_cartesian($rho, $theta, $z);
382 =item cylindrical_to_spherical
384 ($rho_s, $theta, $phi) = cylindrical_to_spherical($rho_c, $theta, $z);
386 Notice that when C<$z> is not 0 C<$rho_s> is not equal to C<$rho_c>.
388 =item spherical_to_cartesian
390 ($x, $y, $z) = spherical_to_cartesian($rho, $theta, $phi);
392 =item spherical_to_cylindrical
394 ($rho_c, $theta, $z) = spherical_to_cylindrical($rho_s, $theta, $phi);
396 Notice that when C<$z> is not 0 C<$rho_c> is not equal to C<$rho_s>.
400 =head1 GREAT CIRCLE DISTANCES AND DIRECTIONS
402 You can compute spherical distances, called B<great circle distances>,
403 by importing the great_circle_distance() function:
405 use Math::Trig 'great_circle_distance';
407 $distance = great_circle_distance($theta0, $phi0, $theta1, $phi1, [, $rho]);
409 The I<great circle distance> is the shortest distance between two
410 points on a sphere. The distance is in C<$rho> units. The C<$rho> is
411 optional, it defaults to 1 (the unit sphere), therefore the distance
414 If you think geographically the I<theta> are longitudes: zero at the
415 Greenwhich meridian, eastward positive, westward negative--and the
416 I<phi> are latitudes: zero at the North Pole, northward positive,
417 southward negative. B<NOTE>: this formula thinks in mathematics, not
418 geographically: the I<phi> zero is at the North Pole, not at the
419 Equator on the west coast of Africa (Bay of Guinea). You need to
420 subtract your geographical coordinates from I<pi/2> (also known as 90
423 $distance = great_circle_distance($lon0, pi/2 - $lat0,
424 $lon1, pi/2 - $lat1, $rho);
426 The direction you must follow the great circle can be computed by the
427 great_circle_direction() function:
429 use Math::Trig 'great_circle_direction';
431 $direction = great_circle_direction($theta0, $phi0, $theta1, $phi1);
433 The result is in radians, zero indicating straight north, pi or -pi
434 straight south, pi/2 straight west, and -pi/2 straight east.
436 Notice that the resulting directions might be somewhat surprising if
437 you are looking at a flat worldmap: in such map projections the great
438 circles quite often do not look like the shortest routes-- but for
439 example the shortest possible routes from Europe or North America to
440 Asia do often cross the polar regions.
444 To calculate the distance between London (51.3N 0.5W) and Tokyo
445 (35.7N 139.8E) in kilometers:
447 use Math::Trig qw(great_circle_distance deg2rad);
449 # Notice the 90 - latitude: phi zero is at the North Pole.
450 @L = (deg2rad(-0.5), deg2rad(90 - 51.3));
451 @T = (deg2rad(139.8),deg2rad(90 - 35.7));
453 $km = great_circle_distance(@L, @T, 6378);
455 The direction you would have to go from London to Tokyo
457 use Math::Trig qw(great_circle_direction);
459 $rad = great_circle_direction(@L, @T);
461 =head2 CAVEAT FOR GREAT CIRCLE FORMULAS
463 The answers may be off by few percentages because of the irregular
464 (slightly aspherical) form of the Earth. The formula used for
465 grear circle distances
467 lat0 = 90 degrees - phi0
468 lat1 = 90 degrees - phi1
469 d = R * arccos(cos(lat0) * cos(lat1) * cos(lon1 - lon01) +
470 sin(lat0) * sin(lat1))
472 is also somewhat unreliable for small distances (for locations
473 separated less than about five degrees) because it uses arc cosine
474 which is rather ill-conditioned for values close to zero.
478 Saying C<use Math::Trig;> exports many mathematical routines in the
479 caller environment and even overrides some (C<sin>, C<cos>). This is
480 construed as a feature by the Authors, actually... ;-)
482 The code is not optimized for speed, especially because we use
483 C<Math::Complex> and thus go quite near complex numbers while doing
484 the computations even when the arguments are not. This, however,
485 cannot be completely avoided if we want things like C<asin(2)> to give
486 an answer instead of giving a fatal runtime error.
490 Jarkko Hietaniemi <F<jhi@iki.fi>> and
491 Raphael Manfredi <F<Raphael_Manfredi@pobox.com>>.