source: trunk/MagicSoft/slalib/unpcd.c@ 10058

Last change on this file since 10058 was 732, checked in by tbretz, 24 years ago
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1#include "slalib.h"
2#include "slamac.h"
3void slaUnpcd ( double disco, double *x, double *y )
4/*
5** - - - - - - - - -
6** s l a U n p c d
7** - - - - - - - - -
8**
9** Remove pincushion/barrel distortion from a distorted [x,y]
10** to give tangent-plane [x,y].
11**
12** Given:
13** disco double pincushion/barrel distortion coefficient
14** x,y double* distorted coordinates
15**
16** Returned:
17** x,y double* tangent-plane coordinates
18**
19** Notes:
20**
21** 1) The distortion is of the form rp = r*(1 + c*r**2), where r is
22** the radial distance from the tangent point, c is the disco
23** argument, and rp is the radial distance in the presence of
24** the distortion.
25**
26** 2) For pincushion distortion, c is +ve;
27** For barrel distortion, c is -ve.
28**
29** 3) For x,y in "radians" - units of one projection radius,
30** which in the case of a photograph is the focal length of
31** the camera - the following disco values apply:
32**
33** geometry disco
34**
35** astrograph 0.0
36** schmidt -0.3333
37** AAT PF doublet +147.069
38** AAT PF triplet +178.585
39** AAT f/8 +21.20
40** JKT f/8 +13.32
41**
42** 4) The present routine is an approximate inverse to the
43** companion routine slaPcd, obtained from two iterations
44** of Newton's method. The mismatch between the slaPcd and
45** slaUnpcd routines is negligible for astrometric applications;
46** To reach 1 milliarcsec at the edge of the AAT triplet or
47** Schmidt field would require field diameters of 2.4 degrees
48** and 42 degrees respectively.
49**
50** Last revision: 11 June 1997
51**
52** Copyright P.T.Wallace. All rights reserved.
53*/
54{
55 double cr2, a, cr2a2, f;
56
57 cr2 = disco * ( *x * *x + *y * *y );
58 a = ( 2.0 * cr2 + 1.0 ) / ( 3.0 * cr2 + 1.0 );
59 cr2a2 = cr2 * a * a;
60 f = ( 2.0 * cr2a2 * a + 1.0 ) / ( 3.0 * cr2a2 + 1.0 );
61 *x *= f;
62 *y *= f;
63}
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