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| int | vips_fwfft () |
| int | vips_invfft () |
| int | vips_freqmult () |
| int | vips_spectrum () |
| int | vips_phasecor () |
To and from Fourier space, filter in Fourier space, convert Fourier-space images to a displayable form.
int vips_fwfft (VipsImage *in,VipsImage **out,...);
Transform an image to Fourier space.
VIPS uses the fftw Fourier Transform library. If this library was not available when VIPS was configured, these functions will fail.
See also: vips_invfft().
[method]
int vips_invfft (VipsImage *in,VipsImage **out,...);
Optional arguments:
real
: only output the real part
Transform an image from Fourier space to real space. The result is complex.
If you are OK with a real result, set real
, it's quicker.
VIPS uses the fftw Fourier Transform library. If this library was not available when VIPS was configured, these functions will fail.
See also: vips_fwfft().
[method]
int vips_freqmult (VipsImage *in,VipsImage *mask,VipsImage **out,...);
Multiply in
by mask
in Fourier space.
in
is transformed to Fourier space, multipled with mask
, then
transformed back to real space. If in
is already a complex image, just
multiply then inverse transform.
See also: vips_invfft(), vips_mask_ideal().
[method]
int vips_spectrum (VipsImage *in,VipsImage **out,...);
Make a displayable (ie. 8-bit unsigned int) power spectrum.
If in
is non-complex, it is transformed to Fourier space. Then the
absolute value is passed through vips_scale() in log mode, and vips_wrap().
See also: vips_fwfft(), vips_scale(), vips_wrap().
[method]
int vips_phasecor (VipsImage *in1,VipsImage *in2,VipsImage **out,...);
Convert the two input images to Fourier space, calculate phase-correlation, back to real space.
See also: vips_fwfft(), vips_cross_phase(),