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| 1 |  |  |  |  |  |  | /* | 
| 2 |  |  |  |  |  |  | *+ | 
| 3 |  |  |  |  |  |  | *  Name: | 
| 4 |  |  |  |  |  |  | *     palUnpcd | 
| 5 |  |  |  |  |  |  |  | 
| 6 |  |  |  |  |  |  | *  Purpose: | 
| 7 |  |  |  |  |  |  | *     Remove pincushion/barrel distortion | 
| 8 |  |  |  |  |  |  |  | 
| 9 |  |  |  |  |  |  | *  Language: | 
| 10 |  |  |  |  |  |  | *     Starlink ANSI C | 
| 11 |  |  |  |  |  |  |  | 
| 12 |  |  |  |  |  |  | *  Type of Module: | 
| 13 |  |  |  |  |  |  | *     Library routine | 
| 14 |  |  |  |  |  |  |  | 
| 15 |  |  |  |  |  |  | *  Invocation: | 
| 16 |  |  |  |  |  |  | *     palUnpcd( double disco, double * x, double * y ); | 
| 17 |  |  |  |  |  |  |  | 
| 18 |  |  |  |  |  |  | *  Arguments: | 
| 19 |  |  |  |  |  |  | *     disco = double (Given) | 
| 20 |  |  |  |  |  |  | *        Pincushion/barrel distortion coefficient. | 
| 21 |  |  |  |  |  |  | *     x = double * (Given & Returned) | 
| 22 |  |  |  |  |  |  | *        On input the distorted X coordinate, on output | 
| 23 |  |  |  |  |  |  | *        the tangent-plane X coordinate. | 
| 24 |  |  |  |  |  |  | *     y = double * (Given & Returned) | 
| 25 |  |  |  |  |  |  | *        On input the distorted Y coordinate, on output | 
| 26 |  |  |  |  |  |  | *        the tangent-plane Y coordinate. | 
| 27 |  |  |  |  |  |  |  | 
| 28 |  |  |  |  |  |  | *  Description: | 
| 29 |  |  |  |  |  |  | *     Remove pincushion/barrel distortion from a distorted [x,y] to give | 
| 30 |  |  |  |  |  |  | *     tangent-plane [x,y]. | 
| 31 |  |  |  |  |  |  |  | 
| 32 |  |  |  |  |  |  | *  Authors: | 
| 33 |  |  |  |  |  |  | *     PTW: Pat Wallace (RAL) | 
| 34 |  |  |  |  |  |  | *     TIMJ: Tim Jenness | 
| 35 |  |  |  |  |  |  | *     {enter_new_authors_here} | 
| 36 |  |  |  |  |  |  |  | 
| 37 |  |  |  |  |  |  | *  Notes: | 
| 38 |  |  |  |  |  |  | *     - The distortion is of the form RP = R*(1+C*R^2), where R is | 
| 39 |  |  |  |  |  |  | *       the radial distance from the tangent point, C is the DISCO | 
| 40 |  |  |  |  |  |  | *       argument, and RP is the radial distance in the presence of | 
| 41 |  |  |  |  |  |  | *       the distortion. | 
| 42 |  |  |  |  |  |  | * | 
| 43 |  |  |  |  |  |  | *     - For pincushion distortion, C is +ve;  for barrel distortion, | 
| 44 |  |  |  |  |  |  | *       C is -ve. | 
| 45 |  |  |  |  |  |  | * | 
| 46 |  |  |  |  |  |  | *     - For X,Y in "radians" - units of one projection radius, | 
| 47 |  |  |  |  |  |  | *       which in the case of a photograph is the focal length of | 
| 48 |  |  |  |  |  |  | *       the camera - the following DISCO values apply: | 
| 49 |  |  |  |  |  |  | * | 
| 50 |  |  |  |  |  |  | *           Geometry          DISCO | 
| 51 |  |  |  |  |  |  | * | 
| 52 |  |  |  |  |  |  | *           astrograph         0.0 | 
| 53 |  |  |  |  |  |  | *           Schmidt           -0.3333 | 
| 54 |  |  |  |  |  |  | *           AAT PF doublet  +147.069 | 
| 55 |  |  |  |  |  |  | *           AAT PF triplet  +178.585 | 
| 56 |  |  |  |  |  |  | *           AAT f/8          +21.20 | 
| 57 |  |  |  |  |  |  | *           JKT f/8          +13.32 | 
| 58 |  |  |  |  |  |  | * | 
| 59 |  |  |  |  |  |  | *     - The present routine is a rigorous inverse of the companion | 
| 60 |  |  |  |  |  |  | *       routine palPcd.  The expression for RP in Note 1 is rewritten | 
| 61 |  |  |  |  |  |  | *       in the form x^3+a*x+b=0 and solved by standard techniques. | 
| 62 |  |  |  |  |  |  | * | 
| 63 |  |  |  |  |  |  | *     - Cases where the cubic has multiple real roots can sometimes | 
| 64 |  |  |  |  |  |  | *       occur, corresponding to extreme instances of barrel distortion | 
| 65 |  |  |  |  |  |  | *       where up to three different undistorted [X,Y]s all produce the | 
| 66 |  |  |  |  |  |  | *       same distorted [X,Y].  However, only one solution is returned, | 
| 67 |  |  |  |  |  |  | *       the one that produces the smallest change in [X,Y]. | 
| 68 |  |  |  |  |  |  |  | 
| 69 |  |  |  |  |  |  | *  See Also: | 
| 70 |  |  |  |  |  |  | *     palPcd | 
| 71 |  |  |  |  |  |  |  | 
| 72 |  |  |  |  |  |  | *  History: | 
| 73 |  |  |  |  |  |  | *     2000-09-03 (PTW): | 
| 74 |  |  |  |  |  |  | *        SLALIB implementation. | 
| 75 |  |  |  |  |  |  | *     2015-01-01 (TIMJ): | 
| 76 |  |  |  |  |  |  | *        Initial version | 
| 77 |  |  |  |  |  |  | *     {enter_further_changes_here} | 
| 78 |  |  |  |  |  |  |  | 
| 79 |  |  |  |  |  |  | *  Copyright: | 
| 80 |  |  |  |  |  |  | *     Copyright (C) 2000 Rutherford Appleton Laboratory. | 
| 81 |  |  |  |  |  |  | *     Copyright (C) 2015 Tim Jenness | 
| 82 |  |  |  |  |  |  | *     All Rights Reserved. | 
| 83 |  |  |  |  |  |  |  | 
| 84 |  |  |  |  |  |  | *  Licence: | 
| 85 |  |  |  |  |  |  | *     This program is free software; you can redistribute it and/or | 
| 86 |  |  |  |  |  |  | *     modify it under the terms of the GNU General Public License as | 
| 87 |  |  |  |  |  |  | *     published by the Free Software Foundation; either version 3 of | 
| 88 |  |  |  |  |  |  | *     the License, or (at your option) any later version. | 
| 89 |  |  |  |  |  |  | * | 
| 90 |  |  |  |  |  |  | *     This program is distributed in the hope that it will be | 
| 91 |  |  |  |  |  |  | *     useful, but WITHOUT ANY WARRANTY; without even the implied | 
| 92 |  |  |  |  |  |  | *     warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR | 
| 93 |  |  |  |  |  |  | *     PURPOSE. See the GNU General Public License for more details. | 
| 94 |  |  |  |  |  |  | * | 
| 95 |  |  |  |  |  |  | *     You should have received a copy of the GNU General Public License | 
| 96 |  |  |  |  |  |  | *     along with this program.  If not, see . | 
| 97 |  |  |  |  |  |  |  | 
| 98 |  |  |  |  |  |  | *  Bugs: | 
| 99 |  |  |  |  |  |  | *     {note_any_bugs_here} | 
| 100 |  |  |  |  |  |  | *- | 
| 101 |  |  |  |  |  |  | */ | 
| 102 |  |  |  |  |  |  |  | 
| 103 |  |  |  |  |  |  | #if HAVE_CONFIG_H | 
| 104 |  |  |  |  |  |  | #include | 
| 105 |  |  |  |  |  |  | #endif | 
| 106 |  |  |  |  |  |  |  | 
| 107 |  |  |  |  |  |  | #include | 
| 108 |  |  |  |  |  |  |  | 
| 109 |  |  |  |  |  |  | #include "pal.h" | 
| 110 |  |  |  |  |  |  | #include "palmac.h" | 
| 111 |  |  |  |  |  |  |  | 
| 112 |  |  |  |  |  |  | /* copysign is C99 */ | 
| 113 |  |  |  |  |  |  | #if HAVE_COPYSIGN | 
| 114 |  |  |  |  |  |  | # define COPYSIGN copysign | 
| 115 |  |  |  |  |  |  | #else | 
| 116 |  |  |  |  |  |  | # define COPYSIGN(a,b) DSIGN(a,b) | 
| 117 |  |  |  |  |  |  | #endif | 
| 118 |  |  |  |  |  |  |  | 
| 119 | 2 |  |  |  |  |  | void palUnpcd( double disco, double * x, double *y ) { | 
| 120 |  |  |  |  |  |  |  | 
| 121 |  |  |  |  |  |  | const double THIRD = 1.0/3.0; | 
| 122 |  |  |  |  |  |  |  | 
| 123 |  |  |  |  |  |  | double rp,q,r,d,w,s,t,f,c,t3,f1,f2,f3,w1,w2,w3; | 
| 124 |  |  |  |  |  |  | double c2; | 
| 125 |  |  |  |  |  |  |  | 
| 126 |  |  |  |  |  |  | /*  Distance of the point from the origin. */ | 
| 127 | 2 |  |  |  |  |  | rp = sqrt( (*x)*(*x)+(*y)*(*y)); | 
| 128 |  |  |  |  |  |  |  | 
| 129 |  |  |  |  |  |  | /*  If zero, or if no distortion, no action is necessary. */ | 
| 130 | 2 | 50 |  |  |  |  | if (rp != 0.0 && disco != 0.0) { | 
| 131 |  |  |  |  |  |  |  | 
| 132 |  |  |  |  |  |  | /*     Begin algebraic solution. */ | 
| 133 | 2 |  |  |  |  |  | q = 1.0/(3.0*disco); | 
| 134 | 2 |  |  |  |  |  | r = rp/(2.0*disco); | 
| 135 | 2 |  |  |  |  |  | w = q*q*q+r*r; | 
| 136 |  |  |  |  |  |  |  | 
| 137 |  |  |  |  |  |  | /* Continue if one real root, or three of which only one is positive. */ | 
| 138 | 2 | 100 |  |  |  |  | if (w > 0.0) { | 
| 139 |  |  |  |  |  |  |  | 
| 140 | 1 |  |  |  |  |  | d = sqrt(w); | 
| 141 | 1 |  |  |  |  |  | w = r+d; | 
| 142 | 1 | 50 |  |  |  |  | s = COPYSIGN(pow(fabs(w),THIRD),w); | 
| 143 | 1 |  |  |  |  |  | w = r-d; | 
| 144 | 1 | 50 |  |  |  |  | t = COPYSIGN(pow(fabs(w),THIRD),w); | 
| 145 | 1 |  |  |  |  |  | f = s+t; | 
| 146 |  |  |  |  |  |  |  | 
| 147 |  |  |  |  |  |  | } else { | 
| 148 |  |  |  |  |  |  | /* Three different real roots:  use geometrical method instead. */ | 
| 149 | 1 |  |  |  |  |  | w = 2.0/sqrt(-3.0*disco); | 
| 150 | 1 |  |  |  |  |  | c = 4.0*rp/(disco*w*w*w); | 
| 151 | 1 |  |  |  |  |  | c2 = c*c; | 
| 152 | 1 | 50 |  |  |  |  | s = sqrt(1.0-DMIN(c2,1.0)); | 
| 153 | 1 |  |  |  |  |  | t3 = atan2(s,c); | 
| 154 |  |  |  |  |  |  |  | 
| 155 |  |  |  |  |  |  | /* The three solutions. */ | 
| 156 | 1 |  |  |  |  |  | f1 = w*cos((PAL__D2PI-t3)/3.0); | 
| 157 | 1 |  |  |  |  |  | f2 = w*cos((t3)/3.0); | 
| 158 | 1 |  |  |  |  |  | f3 = w*cos((PAL__D2PI+t3)/3.0); | 
| 159 |  |  |  |  |  |  |  | 
| 160 |  |  |  |  |  |  | /* Pick the one that moves [X,Y] least. */ | 
| 161 | 1 |  |  |  |  |  | w1 = fabs(f1-rp); | 
| 162 | 1 |  |  |  |  |  | w2 = fabs(f2-rp); | 
| 163 | 1 |  |  |  |  |  | w3 = fabs(f3-rp); | 
| 164 | 1 | 50 |  |  |  |  | if (w1 < w2) { | 
| 165 | 1 | 50 |  |  |  |  | f = ( w1 < w3 ? f1 : f3 ); | 
| 166 |  |  |  |  |  |  | } else { | 
| 167 | 0 | 0 |  |  |  |  | f = ( w2 < w3 ? f2 : f3 ); | 
| 168 |  |  |  |  |  |  | } | 
| 169 |  |  |  |  |  |  | } | 
| 170 |  |  |  |  |  |  |  | 
| 171 |  |  |  |  |  |  | /* Remove the distortion. */ | 
| 172 | 2 |  |  |  |  |  | f = f/rp; | 
| 173 | 2 |  |  |  |  |  | *x *= f; | 
| 174 | 2 |  |  |  |  |  | *y *= f; | 
| 175 |  |  |  |  |  |  | } | 
| 176 | 2 |  |  |  |  |  | } |