Re: [PATCH] Simplified magic_setisa() and improved fields.pm
[p5sagit/p5-mst-13.2.git] / lib / Math / Trig / Radial.pm
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f6aed6f8 1package Math::Trig::Radial;
2
3use strict;
4use vars qw(@ISA @EXPORT);
5@ISA = qw(Exporter);
6
7@EXPORT =
8 qw(
9 cartesian_to_cylindrical
10 cartesian_to_spherical
11 cylindrical_to_cartesian
12 cylindrical_to_spherical
13 spherical_to_cartesian
14 spherical_to_cylindrical
15 great_circle_distance
16 );
17
18use Math::Trig;
19
20sub pip2 { pi/2 }
21
22=pod
23
24=head1 NAME
25
26Math::Trig::Radial - spherical and cylindrical trigonometry
27
28=head1 SYNOPSIS
29
30 use Math::Trig::Radial;
31
32 ($rho, $theta, $z) = cartesian_to_cylindrical($x, $y, $z);
33 ($rho, $theta, $phi) = cartesian_to_spherical($x, $y, $z);
34 ($x, $y, $z) = cylindrical_to_cartesian($rho, $theta, $z);
35 ($rho_s, $theta, $phi) = cylindrical_to_spherical($rho_c, $theta, $z);
36 ($x, $y, $z) = spherical_to_cartesian($rho, $theta, $phi);
37 ($rho_c, $theta, $z) = spherical_to_cylindrical($rho_s, $theta, $phi);
38
39=head1 DESCRIPTION
40
41This module contains a few basic spherical and cylindrical
42trigonometric formulas. B<All angles are in radians>, if needed
43use C<Math::Trig> angle unit conversions.
44
45=head2 COORDINATE SYSTEMS
46
47B<Cartesian> coordinates are the usual rectangular I<xyz>-coordinates.
48
49Spherical coordinates are three-dimensional coordinates which define a
50point in three-dimensional space. They are based on a sphere surface.
51The radius of the sphere is B<rho>, also known as the I<radial>
52coordinate. The angle in the I<xy>-plane (around the I<z>-axis) is
53B<theta>, also known as the I<azimuthal> coordinate. The angle from
54the I<z>-axis is B<phi>, also known as the I<polar> coordinate. The
55`North Pole' is therefore I<0, 0, rho>, and the `Bay of Guinea' (think
56Africa) I<0, pi/2, rho>.
57
58Cylindrical coordinates are three-dimensional coordinates which define
59a point in three-dimensional space. They are based on a cylinder
60surface. The radius of the cylinder is B<rho>, also known as the
61I<radial> coordinate. The angle in the I<xy>-plane (around the
62I<z>-axis) is B<theta>, also known as the I<azimuthal> coordinate.
63The third coordinate is the I<z>.
64
65=head2 CONVERSIONS
66
67Conversions to and from spherical and cylindrical coordinates are
68available. Please notice that the conversions are not necessarily
69reversible because of the equalities like I<pi> angles equals I<-pi>
70angles.
71
72=over 4
73
74=item cartesian_to_cylindrical
75
76 ($rho, $theta, $z) = cartesian_to_cylindrical($x, $y, $z);
77
78=item cartesian_to_spherical
79
80 ($rho, $theta, $phi) = cartesian_to_spherical($x, $y, $z);
81
82=item cylindrical_to_cartesian
83
84 ($x, $y, $z) = cylindrical_to_cartesian($rho, $theta, $z);
85
86=item cylindrical_to_spherical
87
88 ($rho_s, $theta, $phi) = cylindrical_to_spherical($rho_c, $theta, $z);
89
90Notice that when C<$z> is not 0 C<$rho_s> is not equal to C<$rho_c>.
91
92=item spherical_to_cartesian
93
94 ($x, $y, $z) = spherical_to_cartesian($rho, $theta, $phi);
95
96=item spherical_to_cylindrical
97
98 ($rho_c, $theta, $z) = spherical_to_cylindrical($rho_s, $theta, $phi);
99
100Notice that when C<$z> is not 0 C<$rho_c> is not equal to C<$rho_s>.
101
102=back
103
104=head2 GREAT CIRCLE DISTANCE
105
106 $distance = great_circle_distance($x0, $y0, $z0, $x1, $y1, $z1 [, $rho]);
107
108The I<great circle distance> is the shortest distance between two
109points on a sphere. The distance is in C<$rho> units. The C<$rho> is
110optional, it defaults to 1 (the unit sphere), therefore the distance
111defaults to radians. The coordinates C<$x0> ... C<$z1> are in
112cartesian coordinates.
113
114=head EXAMPLES
115
116To calculate the distance between London (51.3N 0.5W) and Tokyo (35.7N
117139.8E) in kilometers:
118
119 use Math::Trig::Radial;
120 use Math::Trig;
121
122 my @L = spherical_to_cartesian(1, map { deg2rad $_ } qw(51.3 -0.5));
123 my @T = spherical_to_cartesian(1, map { deg2rad $_ } qw(35.7 139.8));
124
125 $km = great_circle_distance(@L, @T, 6378);
126
127The answer may be off by up to 0.3% because of the irregular (slightly
128aspherical) form of the Earth.
129
130=head2 AUTHOR
131
132Jarkko Hietaniemi F<E<lt>jhi@iki.fiE<gt>>
133
134=cut
135
136sub cartesian_to_spherical {
137 my ( $x, $y, $z ) = @_;
138
139 my $rho = sqrt( $x * $x + $y * $y + $z * $z );
140
141 return ( $rho,
142 atan2( $y, $x ),
143 $rho ? acos( $z / $rho ) : 0 );
144}
145
146sub spherical_to_cartesian {
147 my ( $rho, $theta, $phi ) = @_;
148
149 return ( $rho * cos( $theta ) * sin( $phi ),
150 $rho * sin( $theta ) * sin( $phi ),
151 $rho * cos( $phi ) );
152}
153
154sub spherical_to_cylindrical {
155 my ( $x, $y, $z ) = spherical_to_cartesian( @_ );
156
157 return ( sqrt( $x * $x + $y * $y ), $_[1], $z );
158}
159
160sub cartesian_to_cylindrical {
161 my ( $x, $y, $z ) = @_;
162
163 return ( sqrt( $x * $x + $y * $y ), atan2( $y, $x ), $z );
164}
165
166sub cylindrical_to_cartesian {
167 my ( $rho, $theta, $z ) = @_;
168
169 return ( $rho * cos( $theta ), $rho * sin( $theta ), $z );
170}
171
172sub cylindrical_to_spherical {
173 return ( cartesian_to_spherical( cylindrical_to_cartesian( @_ ) ) );
174}
175
176sub great_circle_distance {
177 my ( $x0, $y0, $z0, $x1, $y1, $z1, $rho ) = @_;
178
179 $rho = 1 unless defined $rho; # Default to the unit sphere.
180
181 my ( $r0, $theta0, $phi0 ) = cartesian_to_spherical( $x0, $y0, $z0 );
182 my ( $r1, $theta1, $phi1 ) = cartesian_to_spherical( $x1, $y1, $z1 );
183
184 my $lat0 = pip2 - $phi0;
185 my $lat1 = pip2 - $phi1;
186
187 return $rho *
188 acos(cos( $lat0 ) * cos( $lat1 ) * cos( $theta0 - $theta1 ) +
189 sin( $lat0 ) * sin( $lat1 ) );
190}
191
1921;
193