| 1 |
# |
| 2 |
# Trigonometric functions, mostly inherited from Math::Complex. |
| 3 |
# -- Jarkko Hietaniemi, since April 1997 |
| 4 |
# -- Raphael Manfredi, September 1996 (indirectly: because of Math::Complex) |
| 5 |
# |
| 6 |
|
| 7 |
require Exporter; |
| 8 |
package Math::Trig; |
| 9 |
|
| 10 |
use 5.006; |
| 11 |
use strict; |
| 12 |
|
| 13 |
use Math::Complex qw(:trig); |
| 14 |
|
| 15 |
our($VERSION, $PACKAGE, @ISA, @EXPORT, @EXPORT_OK, %EXPORT_TAGS); |
| 16 |
|
| 17 |
@ISA = qw(Exporter); |
| 18 |
|
| 19 |
$VERSION = 1.02; |
| 20 |
|
| 21 |
my @angcnv = qw(rad2deg rad2grad |
| 22 |
deg2rad deg2grad |
| 23 |
grad2rad grad2deg); |
| 24 |
|
| 25 |
@EXPORT = (@{$Math::Complex::EXPORT_TAGS{'trig'}}, |
| 26 |
@angcnv); |
| 27 |
|
| 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); |
| 34 |
|
| 35 |
@EXPORT_OK = (@rdlcnv, 'great_circle_distance', 'great_circle_direction'); |
| 36 |
|
| 37 |
%EXPORT_TAGS = ('radial' => [ @rdlcnv ]); |
| 38 |
|
| 39 |
sub pi2 () { 2 * pi } |
| 40 |
sub pip2 () { pi / 2 } |
| 41 |
|
| 42 |
sub DR () { pi2/360 } |
| 43 |
sub RD () { 360/pi2 } |
| 44 |
sub DG () { 400/360 } |
| 45 |
sub GD () { 360/400 } |
| 46 |
sub RG () { 400/pi2 } |
| 47 |
sub GR () { pi2/400 } |
| 48 |
|
| 49 |
# |
| 50 |
# Truncating remainder. |
| 51 |
# |
| 52 |
|
| 53 |
sub remt ($$) { |
| 54 |
# Oh yes, POSIX::fmod() would be faster. Possibly. If it is available. |
| 55 |
$_[0] - $_[1] * int($_[0] / $_[1]); |
| 56 |
} |
| 57 |
|
| 58 |
# |
| 59 |
# Angle conversions. |
| 60 |
# |
| 61 |
|
| 62 |
sub rad2rad($) { remt($_[0], pi2) } |
| 63 |
|
| 64 |
sub deg2deg($) { remt($_[0], 360) } |
| 65 |
|
| 66 |
sub grad2grad($) { remt($_[0], 400) } |
| 67 |
|
| 68 |
sub rad2deg ($;$) { my $d = RD * $_[0]; $_[1] ? $d : deg2deg($d) } |
| 69 |
|
| 70 |
sub deg2rad ($;$) { my $d = DR * $_[0]; $_[1] ? $d : rad2rad($d) } |
| 71 |
|
| 72 |
sub grad2deg ($;$) { my $d = GD * $_[0]; $_[1] ? $d : deg2deg($d) } |
| 73 |
|
| 74 |
sub deg2grad ($;$) { my $d = DG * $_[0]; $_[1] ? $d : grad2grad($d) } |
| 75 |
|
| 76 |
sub rad2grad ($;$) { my $d = RG * $_[0]; $_[1] ? $d : grad2grad($d) } |
| 77 |
|
| 78 |
sub grad2rad ($;$) { my $d = GR * $_[0]; $_[1] ? $d : rad2rad($d) } |
| 79 |
|
| 80 |
sub cartesian_to_spherical { |
| 81 |
my ( $x, $y, $z ) = @_; |
| 82 |
|
| 83 |
my $rho = sqrt( $x * $x + $y * $y + $z * $z ); |
| 84 |
|
| 85 |
return ( $rho, |
| 86 |
atan2( $y, $x ), |
| 87 |
$rho ? acos( $z / $rho ) : 0 ); |
| 88 |
} |
| 89 |
|
| 90 |
sub spherical_to_cartesian { |
| 91 |
my ( $rho, $theta, $phi ) = @_; |
| 92 |
|
| 93 |
return ( $rho * cos( $theta ) * sin( $phi ), |
| 94 |
$rho * sin( $theta ) * sin( $phi ), |
| 95 |
$rho * cos( $phi ) ); |
| 96 |
} |
| 97 |
|
| 98 |
sub spherical_to_cylindrical { |
| 99 |
my ( $x, $y, $z ) = spherical_to_cartesian( @_ ); |
| 100 |
|
| 101 |
return ( sqrt( $x * $x + $y * $y ), $_[1], $z ); |
| 102 |
} |
| 103 |
|
| 104 |
sub cartesian_to_cylindrical { |
| 105 |
my ( $x, $y, $z ) = @_; |
| 106 |
|
| 107 |
return ( sqrt( $x * $x + $y * $y ), atan2( $y, $x ), $z ); |
| 108 |
} |
| 109 |
|
| 110 |
sub cylindrical_to_cartesian { |
| 111 |
my ( $rho, $theta, $z ) = @_; |
| 112 |
|
| 113 |
return ( $rho * cos( $theta ), $rho * sin( $theta ), $z ); |
| 114 |
} |
| 115 |
|
| 116 |
sub cylindrical_to_spherical { |
| 117 |
return ( cartesian_to_spherical( cylindrical_to_cartesian( @_ ) ) ); |
| 118 |
} |
| 119 |
|
| 120 |
sub great_circle_distance { |
| 121 |
my ( $theta0, $phi0, $theta1, $phi1, $rho ) = @_; |
| 122 |
|
| 123 |
$rho = 1 unless defined $rho; # Default to the unit sphere. |
| 124 |
|
| 125 |
my $lat0 = pip2 - $phi0; |
| 126 |
my $lat1 = pip2 - $phi1; |
| 127 |
|
| 128 |
return $rho * |
| 129 |
acos(cos( $lat0 ) * cos( $lat1 ) * cos( $theta0 - $theta1 ) + |
| 130 |
sin( $lat0 ) * sin( $lat1 ) ); |
| 131 |
} |
| 132 |
|
| 133 |
sub great_circle_direction { |
| 134 |
my ( $theta0, $phi0, $theta1, $phi1 ) = @_; |
| 135 |
|
| 136 |
my $distance = &great_circle_distance; |
| 137 |
|
| 138 |
my $lat0 = pip2 - $phi0; |
| 139 |
my $lat1 = pip2 - $phi1; |
| 140 |
|
| 141 |
my $direction = |
| 142 |
acos((sin($lat1) - sin($lat0) * cos($distance)) / |
| 143 |
(cos($lat0) * sin($distance))); |
| 144 |
|
| 145 |
$direction = pi2 - $direction |
| 146 |
if sin($theta1 - $theta0) < 0; |
| 147 |
|
| 148 |
return rad2rad($direction); |
| 149 |
} |
| 150 |
|
| 151 |
1; |
| 152 |
|
| 153 |
__END__ |
| 154 |
=pod |
| 155 |
|
| 156 |
=head1 NAME |
| 157 |
|
| 158 |
Math::Trig - trigonometric functions |
| 159 |
|
| 160 |
=head1 SYNOPSIS |
| 161 |
|
| 162 |
use Math::Trig; |
| 163 |
|
| 164 |
$x = tan(0.9); |
| 165 |
$y = acos(3.7); |
| 166 |
$z = asin(2.4); |
| 167 |
|
| 168 |
$halfpi = pi/2; |
| 169 |
|
| 170 |
$rad = deg2rad(120); |
| 171 |
|
| 172 |
=head1 DESCRIPTION |
| 173 |
|
| 174 |
C<Math::Trig> defines many trigonometric functions not defined by the |
| 175 |
core Perl which defines only the C<sin()> and C<cos()>. The constant |
| 176 |
B<pi> is also defined as are a few convenience functions for angle |
| 177 |
conversions. |
| 178 |
|
| 179 |
=head1 TRIGONOMETRIC FUNCTIONS |
| 180 |
|
| 181 |
The tangent |
| 182 |
|
| 183 |
=over 4 |
| 184 |
|
| 185 |
=item B<tan> |
| 186 |
|
| 187 |
=back |
| 188 |
|
| 189 |
The cofunctions of the sine, cosine, and tangent (cosec/csc and cotan/cot |
| 190 |
are aliases) |
| 191 |
|
| 192 |
B<csc>, B<cosec>, B<sec>, B<sec>, B<cot>, B<cotan> |
| 193 |
|
| 194 |
The arcus (also known as the inverse) functions of the sine, cosine, |
| 195 |
and tangent |
| 196 |
|
| 197 |
B<asin>, B<acos>, B<atan> |
| 198 |
|
| 199 |
The principal value of the arc tangent of y/x |
| 200 |
|
| 201 |
B<atan2>(y, x) |
| 202 |
|
| 203 |
The arcus cofunctions of the sine, cosine, and tangent (acosec/acsc |
| 204 |
and acotan/acot are aliases) |
| 205 |
|
| 206 |
B<acsc>, B<acosec>, B<asec>, B<acot>, B<acotan> |
| 207 |
|
| 208 |
The hyperbolic sine, cosine, and tangent |
| 209 |
|
| 210 |
B<sinh>, B<cosh>, B<tanh> |
| 211 |
|
| 212 |
The cofunctions of the hyperbolic sine, cosine, and tangent (cosech/csch |
| 213 |
and cotanh/coth are aliases) |
| 214 |
|
| 215 |
B<csch>, B<cosech>, B<sech>, B<coth>, B<cotanh> |
| 216 |
|
| 217 |
The arcus (also known as the inverse) functions of the hyperbolic |
| 218 |
sine, cosine, and tangent |
| 219 |
|
| 220 |
B<asinh>, B<acosh>, B<atanh> |
| 221 |
|
| 222 |
The arcus cofunctions of the hyperbolic sine, cosine, and tangent |
| 223 |
(acsch/acosech and acoth/acotanh are aliases) |
| 224 |
|
| 225 |
B<acsch>, B<acosech>, B<asech>, B<acoth>, B<acotanh> |
| 226 |
|
| 227 |
The trigonometric constant B<pi> is also defined. |
| 228 |
|
| 229 |
$pi2 = 2 * B<pi>; |
| 230 |
|
| 231 |
=head2 ERRORS DUE TO DIVISION BY ZERO |
| 232 |
|
| 233 |
The following functions |
| 234 |
|
| 235 |
acoth |
| 236 |
acsc |
| 237 |
acsch |
| 238 |
asec |
| 239 |
asech |
| 240 |
atanh |
| 241 |
cot |
| 242 |
coth |
| 243 |
csc |
| 244 |
csch |
| 245 |
sec |
| 246 |
sech |
| 247 |
tan |
| 248 |
tanh |
| 249 |
|
| 250 |
cannot be computed for all arguments because that would mean dividing |
| 251 |
by zero or taking logarithm of zero. These situations cause fatal |
| 252 |
runtime errors looking like this |
| 253 |
|
| 254 |
cot(0): Division by zero. |
| 255 |
(Because in the definition of cot(0), the divisor sin(0) is 0) |
| 256 |
Died at ... |
| 257 |
|
| 258 |
or |
| 259 |
|
| 260 |
atanh(-1): Logarithm of zero. |
| 261 |
Died at... |
| 262 |
|
| 263 |
For the C<csc>, C<cot>, C<asec>, C<acsc>, C<acot>, C<csch>, C<coth>, |
| 264 |
C<asech>, C<acsch>, the argument cannot be C<0> (zero). For the |
| 265 |
C<atanh>, C<acoth>, the argument cannot be C<1> (one). For the |
| 266 |
C<atanh>, C<acoth>, the argument cannot be C<-1> (minus one). For the |
| 267 |
C<tan>, C<sec>, C<tanh>, C<sech>, the argument cannot be I<pi/2 + k * |
| 268 |
pi>, where I<k> is any integer. |
| 269 |
|
| 270 |
=head2 SIMPLE (REAL) ARGUMENTS, COMPLEX RESULTS |
| 271 |
|
| 272 |
Please note that some of the trigonometric functions can break out |
| 273 |
from the B<real axis> into the B<complex plane>. For example |
| 274 |
C<asin(2)> has no definition for plain real numbers but it has |
| 275 |
definition for complex numbers. |
| 276 |
|
| 277 |
In Perl terms this means that supplying the usual Perl numbers (also |
| 278 |
known as scalars, please see L<perldata>) as input for the |
| 279 |
trigonometric functions might produce as output results that no more |
| 280 |
are simple real numbers: instead they are complex numbers. |
| 281 |
|
| 282 |
The C<Math::Trig> handles this by using the C<Math::Complex> package |
| 283 |
which knows how to handle complex numbers, please see L<Math::Complex> |
| 284 |
for more information. In practice you need not to worry about getting |
| 285 |
complex numbers as results because the C<Math::Complex> takes care of |
| 286 |
details like for example how to display complex numbers. For example: |
| 287 |
|
| 288 |
print asin(2), "\n"; |
| 289 |
|
| 290 |
should produce something like this (take or leave few last decimals): |
| 291 |
|
| 292 |
1.5707963267949-1.31695789692482i |
| 293 |
|
| 294 |
That is, a complex number with the real part of approximately C<1.571> |
| 295 |
and the imaginary part of approximately C<-1.317>. |
| 296 |
|
| 297 |
=head1 PLANE ANGLE CONVERSIONS |
| 298 |
|
| 299 |
(Plane, 2-dimensional) angles may be converted with the following functions. |
| 300 |
|
| 301 |
$radians = deg2rad($degrees); |
| 302 |
$radians = grad2rad($gradians); |
| 303 |
|
| 304 |
$degrees = rad2deg($radians); |
| 305 |
$degrees = grad2deg($gradians); |
| 306 |
|
| 307 |
$gradians = deg2grad($degrees); |
| 308 |
$gradians = rad2grad($radians); |
| 309 |
|
| 310 |
The full circle is 2 I<pi> radians or I<360> degrees or I<400> gradians. |
| 311 |
The result is by default wrapped to be inside the [0, {2pi,360,400}[ circle. |
| 312 |
If you don't want this, supply a true second argument: |
| 313 |
|
| 314 |
$zillions_of_radians = deg2rad($zillions_of_degrees, 1); |
| 315 |
$negative_degrees = rad2deg($negative_radians, 1); |
| 316 |
|
| 317 |
You can also do the wrapping explicitly by rad2rad(), deg2deg(), and |
| 318 |
grad2grad(). |
| 319 |
|
| 320 |
=head1 RADIAL COORDINATE CONVERSIONS |
| 321 |
|
| 322 |
B<Radial coordinate systems> are the B<spherical> and the B<cylindrical> |
| 323 |
systems, explained shortly in more detail. |
| 324 |
|
| 325 |
You can import radial coordinate conversion functions by using the |
| 326 |
C<:radial> tag: |
| 327 |
|
| 328 |
use Math::Trig ':radial'; |
| 329 |
|
| 330 |
($rho, $theta, $z) = cartesian_to_cylindrical($x, $y, $z); |
| 331 |
($rho, $theta, $phi) = cartesian_to_spherical($x, $y, $z); |
| 332 |
($x, $y, $z) = cylindrical_to_cartesian($rho, $theta, $z); |
| 333 |
($rho_s, $theta, $phi) = cylindrical_to_spherical($rho_c, $theta, $z); |
| 334 |
($x, $y, $z) = spherical_to_cartesian($rho, $theta, $phi); |
| 335 |
($rho_c, $theta, $z) = spherical_to_cylindrical($rho_s, $theta, $phi); |
| 336 |
|
| 337 |
B<All angles are in radians>. |
| 338 |
|
| 339 |
=head2 COORDINATE SYSTEMS |
| 340 |
|
| 341 |
B<Cartesian> coordinates are the usual rectangular I<(x, y, |
| 342 |
z)>-coordinates. |
| 343 |
|
| 344 |
Spherical coordinates, I<(rho, theta, pi)>, are three-dimensional |
| 345 |
coordinates which define a point in three-dimensional space. They are |
| 346 |
based on a sphere surface. The radius of the sphere is B<rho>, also |
| 347 |
known as the I<radial> coordinate. The angle in the I<xy>-plane |
| 348 |
(around the I<z>-axis) is B<theta>, also known as the I<azimuthal> |
| 349 |
coordinate. The angle from the I<z>-axis is B<phi>, also known as the |
| 350 |
I<polar> coordinate. The `North Pole' is therefore I<0, 0, rho>, and |
| 351 |
the `Bay of Guinea' (think of the missing big chunk of Africa) I<0, |
| 352 |
pi/2, rho>. In geographical terms I<phi> is latitude (northward |
| 353 |
positive, southward negative) and I<theta> is longitude (eastward |
| 354 |
positive, westward negative). |
| 355 |
|
| 356 |
B<BEWARE>: some texts define I<theta> and I<phi> the other way round, |
| 357 |
some texts define the I<phi> to start from the horizontal plane, some |
| 358 |
texts use I<r> in place of I<rho>. |
| 359 |
|
| 360 |
Cylindrical coordinates, I<(rho, theta, z)>, are three-dimensional |
| 361 |
coordinates which define a point in three-dimensional space. They are |
| 362 |
based on a cylinder surface. The radius of the cylinder is B<rho>, |
| 363 |
also known as the I<radial> coordinate. The angle in the I<xy>-plane |
| 364 |
(around the I<z>-axis) is B<theta>, also known as the I<azimuthal> |
| 365 |
coordinate. The third coordinate is the I<z>, pointing up from the |
| 366 |
B<theta>-plane. |
| 367 |
|
| 368 |
=head2 3-D ANGLE CONVERSIONS |
| 369 |
|
| 370 |
Conversions to and from spherical and cylindrical coordinates are |
| 371 |
available. Please notice that the conversions are not necessarily |
| 372 |
reversible because of the equalities like I<pi> angles being equal to |
| 373 |
I<-pi> angles. |
| 374 |
|
| 375 |
=over 4 |
| 376 |
|
| 377 |
=item cartesian_to_cylindrical |
| 378 |
|
| 379 |
($rho, $theta, $z) = cartesian_to_cylindrical($x, $y, $z); |
| 380 |
|
| 381 |
=item cartesian_to_spherical |
| 382 |
|
| 383 |
($rho, $theta, $phi) = cartesian_to_spherical($x, $y, $z); |
| 384 |
|
| 385 |
=item cylindrical_to_cartesian |
| 386 |
|
| 387 |
($x, $y, $z) = cylindrical_to_cartesian($rho, $theta, $z); |
| 388 |
|
| 389 |
=item cylindrical_to_spherical |
| 390 |
|
| 391 |
($rho_s, $theta, $phi) = cylindrical_to_spherical($rho_c, $theta, $z); |
| 392 |
|
| 393 |
Notice that when C<$z> is not 0 C<$rho_s> is not equal to C<$rho_c>. |
| 394 |
|
| 395 |
=item spherical_to_cartesian |
| 396 |
|
| 397 |
($x, $y, $z) = spherical_to_cartesian($rho, $theta, $phi); |
| 398 |
|
| 399 |
=item spherical_to_cylindrical |
| 400 |
|
| 401 |
($rho_c, $theta, $z) = spherical_to_cylindrical($rho_s, $theta, $phi); |
| 402 |
|
| 403 |
Notice that when C<$z> is not 0 C<$rho_c> is not equal to C<$rho_s>. |
| 404 |
|
| 405 |
=back |
| 406 |
|
| 407 |
=head1 GREAT CIRCLE DISTANCES AND DIRECTIONS |
| 408 |
|
| 409 |
You can compute spherical distances, called B<great circle distances>, |
| 410 |
by importing the great_circle_distance() function: |
| 411 |
|
| 412 |
use Math::Trig 'great_circle_distance'; |
| 413 |
|
| 414 |
$distance = great_circle_distance($theta0, $phi0, $theta1, $phi1, [, $rho]); |
| 415 |
|
| 416 |
The I<great circle distance> is the shortest distance between two |
| 417 |
points on a sphere. The distance is in C<$rho> units. The C<$rho> is |
| 418 |
optional, it defaults to 1 (the unit sphere), therefore the distance |
| 419 |
defaults to radians. |
| 420 |
|
| 421 |
If you think geographically the I<theta> are longitudes: zero at the |
| 422 |
Greenwhich meridian, eastward positive, westward negative--and the |
| 423 |
I<phi> are latitudes: zero at the North Pole, northward positive, |
| 424 |
southward negative. B<NOTE>: this formula thinks in mathematics, not |
| 425 |
geographically: the I<phi> zero is at the North Pole, not at the |
| 426 |
Equator on the west coast of Africa (Bay of Guinea). You need to |
| 427 |
subtract your geographical coordinates from I<pi/2> (also known as 90 |
| 428 |
degrees). |
| 429 |
|
| 430 |
$distance = great_circle_distance($lon0, pi/2 - $lat0, |
| 431 |
$lon1, pi/2 - $lat1, $rho); |
| 432 |
|
| 433 |
The direction you must follow the great circle can be computed by the |
| 434 |
great_circle_direction() function: |
| 435 |
|
| 436 |
use Math::Trig 'great_circle_direction'; |
| 437 |
|
| 438 |
$direction = great_circle_direction($theta0, $phi0, $theta1, $phi1); |
| 439 |
|
| 440 |
The result is in radians, zero indicating straight north, pi or -pi |
| 441 |
straight south, pi/2 straight west, and -pi/2 straight east. |
| 442 |
|
| 443 |
Notice that the resulting directions might be somewhat surprising if |
| 444 |
you are looking at a flat worldmap: in such map projections the great |
| 445 |
circles quite often do not look like the shortest routes-- but for |
| 446 |
example the shortest possible routes from Europe or North America to |
| 447 |
Asia do often cross the polar regions. |
| 448 |
|
| 449 |
=head1 EXAMPLES |
| 450 |
|
| 451 |
To calculate the distance between London (51.3N 0.5W) and Tokyo |
| 452 |
(35.7N 139.8E) in kilometers: |
| 453 |
|
| 454 |
use Math::Trig qw(great_circle_distance deg2rad); |
| 455 |
|
| 456 |
# Notice the 90 - latitude: phi zero is at the North Pole. |
| 457 |
@L = (deg2rad(-0.5), deg2rad(90 - 51.3)); |
| 458 |
@T = (deg2rad(139.8),deg2rad(90 - 35.7)); |
| 459 |
|
| 460 |
$km = great_circle_distance(@L, @T, 6378); |
| 461 |
|
| 462 |
The direction you would have to go from London to Tokyo |
| 463 |
|
| 464 |
use Math::Trig qw(great_circle_direction); |
| 465 |
|
| 466 |
$rad = great_circle_direction(@L, @T); |
| 467 |
|
| 468 |
=head2 CAVEAT FOR GREAT CIRCLE FORMULAS |
| 469 |
|
| 470 |
The answers may be off by few percentages because of the irregular |
| 471 |
(slightly aspherical) form of the Earth. The formula used for |
| 472 |
grear circle distances |
| 473 |
|
| 474 |
lat0 = 90 degrees - phi0 |
| 475 |
lat1 = 90 degrees - phi1 |
| 476 |
d = R * arccos(cos(lat0) * cos(lat1) * cos(lon1 - lon01) + |
| 477 |
sin(lat0) * sin(lat1)) |
| 478 |
|
| 479 |
is also somewhat unreliable for small distances (for locations |
| 480 |
separated less than about five degrees) because it uses arc cosine |
| 481 |
which is rather ill-conditioned for values close to zero. |
| 482 |
|
| 483 |
=head1 BUGS |
| 484 |
|
| 485 |
Saying C<use Math::Trig;> exports many mathematical routines in the |
| 486 |
caller environment and even overrides some (C<sin>, C<cos>). This is |
| 487 |
construed as a feature by the Authors, actually... ;-) |
| 488 |
|
| 489 |
The code is not optimized for speed, especially because we use |
| 490 |
C<Math::Complex> and thus go quite near complex numbers while doing |
| 491 |
the computations even when the arguments are not. This, however, |
| 492 |
cannot be completely avoided if we want things like C<asin(2)> to give |
| 493 |
an answer instead of giving a fatal runtime error. |
| 494 |
|
| 495 |
=head1 AUTHORS |
| 496 |
|
| 497 |
Jarkko Hietaniemi <F<jhi@iki.fi>> and |
| 498 |
Raphael Manfredi <F<Raphael_Manfredi@pobox.com>>. |
| 499 |
|
| 500 |
=cut |
| 501 |
|
| 502 |
# eof |