/src/libvips/libvips/create/mask_ideal.c
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1 | | /* creates an ideal filter. |
2 | | * |
3 | | * 02/01/14 |
4 | | * - from ideal.c |
5 | | */ |
6 | | |
7 | | /* |
8 | | |
9 | | This file is part of VIPS. |
10 | | |
11 | | VIPS is free software; you can redistribute it and/or modify |
12 | | it under the terms of the GNU Lesser General Public License as published by |
13 | | the Free Software Foundation; either version 2 of the License, or |
14 | | (at your option) any later version. |
15 | | |
16 | | This program is distributed in the hope that it will be useful, |
17 | | but WITHOUT ANY WARRANTY; without even the implied warranty of |
18 | | MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the |
19 | | GNU Lesser General Public License for more details. |
20 | | |
21 | | You should have received a copy of the GNU Lesser General Public License |
22 | | along with this program; if not, write to the Free Software |
23 | | Foundation, Inc., 51 Franklin Street, Fifth Floor, Boston, MA |
24 | | 02110-1301 USA |
25 | | |
26 | | */ |
27 | | |
28 | | /* |
29 | | |
30 | | These files are distributed with VIPS - http://www.vips.ecs.soton.ac.uk |
31 | | |
32 | | */ |
33 | | |
34 | | /* |
35 | | #define VIPS_DEBUG |
36 | | */ |
37 | | |
38 | | #ifdef HAVE_CONFIG_H |
39 | | #include <config.h> |
40 | | #endif /*HAVE_CONFIG_H*/ |
41 | | #include <glib/gi18n-lib.h> |
42 | | |
43 | | #include <stdio.h> |
44 | | #include <string.h> |
45 | | #include <stdlib.h> |
46 | | #include <math.h> |
47 | | |
48 | | #include <vips/vips.h> |
49 | | |
50 | | #include "pcreate.h" |
51 | | #include "point.h" |
52 | | #include "pmask.h" |
53 | | |
54 | | G_DEFINE_TYPE(VipsMaskIdeal, vips_mask_ideal, VIPS_TYPE_MASK); |
55 | | |
56 | | static double |
57 | | vips_mask_ideal_point(VipsMask *mask, double dx, double dy) |
58 | 0 | { |
59 | 0 | VipsMaskIdeal *ideal = (VipsMaskIdeal *) mask; |
60 | 0 | double fc = ideal->frequency_cutoff; |
61 | |
|
62 | 0 | double dist2 = dx * dx + dy * dy; |
63 | 0 | double fc2 = fc * fc; |
64 | |
|
65 | 0 | return dist2 <= fc2 ? 0.0 : 1.0; |
66 | 0 | } |
67 | | |
68 | | static void |
69 | | vips_mask_ideal_class_init(VipsMaskIdealClass *class) |
70 | 1 | { |
71 | 1 | GObjectClass *gobject_class = G_OBJECT_CLASS(class); |
72 | 1 | VipsObjectClass *vobject_class = VIPS_OBJECT_CLASS(class); |
73 | 1 | VipsMaskClass *mask_class = VIPS_MASK_CLASS(class); |
74 | | |
75 | 1 | gobject_class->set_property = vips_object_set_property; |
76 | 1 | gobject_class->get_property = vips_object_get_property; |
77 | | |
78 | 1 | vobject_class->nickname = "mask_ideal"; |
79 | 1 | vobject_class->description = _("make an ideal filter"); |
80 | | |
81 | 1 | mask_class->point = vips_mask_ideal_point; |
82 | | |
83 | 1 | VIPS_ARG_DOUBLE(class, "frequency_cutoff", 6, |
84 | 1 | _("Frequency cutoff"), |
85 | 1 | _("Frequency cutoff"), |
86 | 1 | VIPS_ARGUMENT_REQUIRED_INPUT, |
87 | 1 | G_STRUCT_OFFSET(VipsMaskIdeal, frequency_cutoff), |
88 | 1 | 0.0, 1000000.0, 0.5); |
89 | 1 | } |
90 | | |
91 | | static void |
92 | | vips_mask_ideal_init(VipsMaskIdeal *ideal) |
93 | 0 | { |
94 | 0 | ideal->frequency_cutoff = 0.5; |
95 | 0 | } |
96 | | |
97 | | /** |
98 | | * vips_mask_ideal: |
99 | | * @out: (out): output image |
100 | | * @width: image size |
101 | | * @height: image size |
102 | | * @frequency_cutoff: threshold at which filter ends |
103 | | * @...: %NULL-terminated list of optional named arguments |
104 | | * |
105 | | * Optional arguments: |
106 | | * |
107 | | * * @nodc: don't set the DC pixel |
108 | | * * @reject: invert the filter sense |
109 | | * * @optical: coordinates in optical space |
110 | | * * @uchar: output a uchar image |
111 | | * |
112 | | * Make an ideal high- or low-pass filter, that is, one with a sharp cutoff |
113 | | * positioned at @frequency_cutoff, where @frequency_cutoff is in |
114 | | * the range 0 - 1. |
115 | | * |
116 | | * This operation creates a one-band float image of the specified size. |
117 | | * The image has |
118 | | * values in the range [0, 1] and is typically used for multiplying against |
119 | | * frequency domain images to filter them. |
120 | | * Masks are created with the DC component at (0, 0). The DC pixel always |
121 | | * has the value 1.0. |
122 | | * |
123 | | * Set @nodc to not set the DC pixel. |
124 | | * |
125 | | * Set @optical to position the DC component in the centre of the image. This |
126 | | * makes the mask suitable for multiplying against optical Fourier transforms. |
127 | | * See vips_wrap(). |
128 | | * |
129 | | * Set @reject to invert the sense of |
130 | | * the filter. For example, low-pass becomes low-reject. |
131 | | * |
132 | | * Set @uchar to output an 8-bit unsigned char image rather than a |
133 | | * float image. In this case, pixels are in the range [0 - 255]. |
134 | | * |
135 | | * See also: vips_mask_ideal(), vips_mask_ideal_ring(), |
136 | | * vips_mask_ideal_band(), vips_mask_butterworth(), |
137 | | * vips_mask_butterworth_ring(), vips_mask_butterworth_band(), |
138 | | * vips_mask_gaussian(), vips_mask_gaussian_ring(), |
139 | | * vips_mask_gaussian_band(). |
140 | | * |
141 | | * Returns: 0 on success, -1 on error |
142 | | */ |
143 | | int |
144 | | vips_mask_ideal(VipsImage **out, int width, int height, |
145 | | double frequency_cutoff, ...) |
146 | 0 | { |
147 | 0 | va_list ap; |
148 | 0 | int result; |
149 | |
|
150 | 0 | va_start(ap, frequency_cutoff); |
151 | 0 | result = vips_call_split("mask_ideal", ap, out, width, height, |
152 | 0 | frequency_cutoff); |
153 | 0 | va_end(ap); |
154 | |
|
155 | 0 | return result; |
156 | 0 | } |