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int | vips_conv () |
int | vips_compass () |
int | vips_convsep () |
int | vips_sharpen () |
int | vips_gaussblur () |
int | vips_spcor () |
int | vips_fastcor () |
These operations convolve an image in some way, or are operations based on simple convolution, or are useful with convolution.
int vips_conv (VipsImage *in
,VipsImage **out
,VipsImage *mask
,...
);
Optional arguments:
precision
: calculation accuracy
layers
: number of layers for approximation
cluster
: cluster lines closer than this distance
Convolution.
Perform a convolution of in
with mask
.
Each output pixel is
calculated as sigma[i]{pixel[i] * mask[i]} / scale + offset, where scale
and offset are part of mask
.
If precision
is VIPS_PRECISION_INTEGER then the convolution is performed
with integer arithmetic and the output image
always has the same VipsBandFormat as the input image.
Convolutions on unsigned 8-bit images are calculated with the processor's vector unit, if possible. Disable this with --vips-novector or IM_NOVECTOR.
If precision
is VIPS_PRECISION_FLOAT then the convolution is performed
with floating-point arithmetic. The output image
is always VIPS_FORMAT_FLOAT
unless in
is VIPS_FORMAT_DOUBLE
, in which case
out
is also VIPS_FORMAT_DOUBLE
.
If precision
is VIPS_PRECISION_APPROXIMATE then the output image
always has the same VipsBandFormat as the input image.
Larger values for layers
give more accurate
results, but are slower. As layers
approaches the mask radius, the
accuracy will become close to exact convolution and the speed will drop to
match. For many large masks, such as Gaussian, n_layers
need be only 10% of
this value and accuracy will still be good.
Smaller values of cluster
will give more accurate results, but be slower
and use more memory. 10% of the mask radius is a good rule of thumb.
int vips_convsep (VipsImage *in
,VipsImage **out
,VipsImage *mask
,...
);
Optional arguments:
precision
: calculation accuracy
layers
: number of layers for approximation
cluster
: cluster lines closer than this distance
Perform a separable convolution of in
with mask
.
See vips_conv()
for a detailed description.
The mask must be 1xn or nx1 elements.
The image is convolved twice: once with mask
and then again with mask
rotated by 90 degrees. This is much faster for certain types of mask
(gaussian blur, for example) than doing a full 2D convolution.
See also: vips_conv()
, vips_gaussmat()
.
int vips_sharpen (VipsImage *in
,VipsImage **out
,...
);
Optional arguments:
radius
: how large a mask to use
x1
: flat/jaggy threshold
y2
: maximum amount of brightening
y3
: maximum amount of darkening
m1
: slope for flat areas
m2
: slope for jaggy areas
Selectively sharpen the L channel of a LAB image. The input image is transformed to VIPS_INTERPRETATION_LABS.
The operation performs a gaussian blur of radius radius
and subtracts
from in
to generate a high-frequency signal. This signal is passed
through a lookup table formed from the five parameters and added back to
in
.
The lookup table is formed like this:
^ y2 |- - - - - ----------- | / | / slope m2 | .../ -x1 | ... | -------------------...----------------------> | ... | x1 |... slope m1 / | / m2 | / | / | / | / | ______/ _ _ _ _ _ _ | -y3 |
For printing, we recommend the following settings (the defaults):
radius == 3 x1 == 1.5 y2 == 20 (don't brighten by more than 20 L*) y3 == 50 (can darken by up to 50 L*) m1 == 1 (some sharpening in flat areas) m2 == 2 (more sharpening in jaggy areas)
If you want more or less sharpening, we suggest you just change the m1 and m2 parameters.
The radius
parameter changes the width of the fringe and can be
adjusted according to the output printing resolution. As an approximate
guideline, use 1 for 4 pixels/mm (CRT display resolution), 2 for 8
pixels/mm, 3 for 12 pixels/mm and 4 for 16 pixels/mm (300 dpi == 12
pixels/mm). These figures refer to the image raster, not the half-tone
resolution.
See also: vips_conv()
.
int vips_gaussblur (VipsImage *in
,VipsImage **out
,double sigma
,...
);
Optional arguments:
precision
: VipsPrecision for blur, default VIPS_PRECISION_INTEGER
min_ampl
: minimum amplitude, default 0.2
This operator runs vips_gaussmat()
and vips_convsep()
for you on an image.
Set min_ampl
smaller to generate a larger, more accurate mask. Set sigma
larger to make the blur more blurry.
See also: vips_gaussmat()
, vips_convsep()
.
int vips_spcor (VipsImage *in
,VipsImage *ref
,VipsImage **out
,...
);
Calculate a correlation surface.
ref
is placed at every position in in
and the correlation coefficient
calculated. The output
image is always float.
The output image is the same size as the input. Extra input edge pixels are made by copying the existing edges outwards.
The correlation coefficient is calculated as:
sumij (ref(i,j)-mean(ref))(inkl(i,j)-mean(inkl)) c(k,l) = ------------------------------------------------ sqrt(sumij (ref(i,j)-mean(ref))^2) * sqrt(sumij (inkl(i,j)-mean(inkl))^2)
where inkl is the area of in
centred at position (k,l).
from Niblack "An Introduction to Digital Image Processing", Prentice/Hall, pp 138.
If the number of bands differs, one of the images must have one band. In this case, an n-band image is formed from the one-band image by joining n copies of the one-band image together, and then the two n-band images are operated upon.
The output image is always float, unless either of the two inputs is double, in which case the output is also double.
See also: vips_fastcor()
.
int vips_fastcor (VipsImage *in
,VipsImage *ref
,VipsImage **out
,...
);
Calculate a fast correlation surface.
ref
is placed at every position in in
and the sum of squares of
differences calculated.
The output image is the same size as the input. Extra input edge pixels are made by copying the existing edges outwards.
If the number of bands differs, one of the images must have one band. In this case, an n-band image is formed from the one-band image by joining n copies of the one-band image together, and then the two n-band images are operated upon.
The output type is uint if both inputs are integer, float if both are float or complex, and double if either is double or double complex. In other words, the output type is just large enough to hold the whole range of possible values.
See also: vips_spcor()
.