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NRAO Home > CASA > CASA Toolkit Reference Manual |
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image.convolve - Function
1.1.1 Convolve image with an array or another image
Description
This function performs Fourier-based convolution of an image file by the
given kernel.
If outfile is given, the image is written to the specified disk file. If outfile is left unset, the on-the-fly Image tool generated by this function is associated with a temporary image. This temporary image may be stored in memory or on disk, depending on its size. When the user destroys the generated Image tool (with the done function) this temporary image is deleted.
The kernel is provided as a multi-dimensional array or as the filename of a disk-based image file. The provided kernel can have fewer dimensions than the image being convolved. In this case, it will be padded with degenerate axes. An error will result if the kernel has more dimensions than the image. No additional scaling of the kernel is provided yet.
The scaling of the output image is determined by the argument scale. If this is left unset, then the kernel is normalized to unit sum. If scale is not left unset, then the convolution kernel will be scaled (multiplied) by this value.
Masked pixels will be assigned the value 0.0 before convolution.
The output mask is the combination (logical OR) of the default input pixel mask (if any) and the OTF mask. Any other input pixel masks will not be copied. The function maskhandler should be used if there is a need to copy other masks too.
See also the other convolution functions:
convolve2d, sepconvolve and hanning.
Arguments
Inputs |
| ||
outfile |
| Output image file name. Default is unset.
| |
| allowed: | string |
|
| Default: |
| |
kernel |
| Convolution kernel - An array or an image filename.
Must be specified by the user.
| |
| allowed: | any |
|
| Default: | variant
|
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scale |
| Scale factor. The default behavior is to autoscale
(specified with -1.0).
| |
| allowed: | double | |
| Default: | -1.0 |
|
region |
| Region selection. See ”help par.region” for details.
Default is to use the full image.
| |
| allowed: | variant |
|
| Default: | variant
|
|
mask |
| Mask to use. See help par.mask for more details. The
default setting is none.
| |
| allowed: | any |
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| Default: | variant
|
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overwrite |
| Overwrite (unprompted) the pre-existing output file?
| |
| allowed: | bool |
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| Default: | false |
|
stretch |
| Stretch the mask if necessary and possible? See help
par.stretch for more details.
| |
| allowed: | bool |
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| Default: | false |
|
image
Example
"""
#
print "\t----\t convolve Ex 1 \t----"
# This example presupposes the existence of an input image file, testdata, and a kernel image file, kerneldata.
# Open the input image file:
ia.open(infile=’testdata’)
# Set up a region to be operated upon (in this case, the whole image):
r1 = rg.box()
# Perform the convolution:
im2 = ia.convolve (outfile = ’convout’, overwrite = true, region = r1, kernel = ’kerneldata’)
ia.close()
im2.done()
#
print "\t----\t convolve Ex 2 \t----"
# This example uses an array as the convolution kernel, and presupposes the existence of an input image file, testdata, which we first open:
ia.open(infile=’testdata’)
# Next, create a Python array of some kind to use as a convolution kernel. For example:
from numpy import arange
kernelarray = arange(10)**3
# Set up a region to be operated upon (in this case, the whole image):
r1 = rg.box()
# Perform the convolution:
im3 = ia.convolve (outfile = ’convout2’, overwrite = true, region = r1, kernel = kernelarray)
ia.close()
im3.done()
#
"""
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More information about CASA may be found at the
CASA web page
Copyright © 2016 Associated Universities Inc., Washington, D.C.
This code is available under the terms of the GNU General Public Lincense
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