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crimp - CRIMP - Manipulation and Processing

- package require
**Tcl 8.5** - package require
**Tk 8.5** - package require
**crimp ?0.2?** - package require
**crimp::core ?0.2?**

**::crimp****histogram***image***::crimp****statistics basic***image***::crimp****statistics otsu***stats***::crimp****add***image1**image2*?*scale*? ?*offset*?**::crimp****alpha blend***foreground**background**alpha***::crimp****alpha set***image**mask***::crimp****alpha opaque***image***::crimp****alpha over***foreground**background***::crimp****atan2***image1**image2***::crimp****blank***type**width**height**value*...**::crimp****crop***image**ww**hn**we**hs***::crimp****cut***image**dx**dy**w**h***::crimp****decimate xy***image**factor**kernel***::crimp****decimate x***image**factor**kernel***::crimp****decimate y***image**factor**kernel***::crimp****degamma***image**y***::crimp****difference***image1**image2***::crimp****downsample xy***image**factor***::crimp****downsample x***image**factor***::crimp****downsample y***image**factor***::crimp****effect charcoal***image***::crimp****effect emboss***image***::crimp****effect sharpen***image***::crimp****expand const***image**ww**hn**we**hs*?*value*...?**::crimp****expand extend***image**ww**hn**we**hs***::crimp****expand mirror***image**ww**hn**we**hs***::crimp****expand replicate***image**ww**hn**we**hs***::crimp****expand wrap***image**ww**hn**we**hs***::crimp****fft forward***image***::crimp****fft backward***image***::crimp****filter ahe***image*?**-border***spec*? ?*radius*?**::crimp****filter convolve***image*?**-border***spec*?*kernel*...**::crimp****filter gauss discrete***image**sigma*?*r*?**::crimp****filter gauss sampled***image**sigma*?*r*?**::crimp****filter mean***image*?**-border***spec*? ?*radius*?**::crimp****filter rank***image*?**-border***spec*? ?*radius*?*percentile*??**::crimp****filter stddev***image*?**-border***spec*? ?*radius*?**::crimp****filter sobel x***image***::crimp****filter sobel y***image***::crimp****filter scharr x***image***::crimp****filter scharr y***image***::crimp****filter prewitt x***image***::crimp****filter prewitt y***image***::crimp****filter roberts x***image***::crimp****filter roberts y***image***::crimp****filter canny sobel***image***::crimp****filter canny deriche***image***::crimp****filter wiener***image**radius***::crimp****gamma***image**y***::crimp****gradient sobel***image***::crimp****gradient scharr***image***::crimp****gradient prewitt***image***::crimp****gradient roberts***image***::crimp****gradient polar***cgradient***::crimp****gradient visual***pgradient***::crimp****hypot***image1**image2***::crimp****integrate***image***::crimp****interpolate xy***image**factor**kernel***::crimp****interpolate x***image**factor**kernel***::crimp****interpolate y***image**factor**kernel***::crimp****invert***image***::crimp****logpolar***image**rwidth**rheight*?*xcenter*? 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?*offset*?**::crimp****kernel fpmake***matrix*?*offset*?**::crimp****kernel transpose***kernel***::crimp****kernel image***kernel***::crimp****map***arg*...**::crimp****mapof***table***::crimp****table compose***f**g***::crimp****table eval wrap***cmd***::crimp****table eval clamp***cmd***<cmd>***x***::crimp****table degamma***y***::crimp****table gamma***y***::crimp****table gauss***sigma***::crimp****table identity****::crimp****table invers****::crimp****table linear wrap***gain**offset***::crimp****table linear clamp***gain**offset***::crimp****table log**?*max*?**::crimp****table solarize***threshold***::crimp****table sqrt**?*max*?**::crimp****table stretch***min**max***::crimp****table threshold above***threshold***::crimp****table threshold below***threshold***::crimp****table threshold inside***min**max***::crimp****table threshold outside***min**max***::crimp****table fgauss discrete***sigma*?*r*?**::crimp****table fgauss sampled***sigma*?*r*?**::crimp****transform affine***a**b**c**d**e**f***::crimp****transform chain***transform*...**::crimp****transform identity****::crimp****transform invert***transform***::crimp****transform projective***a**b**c**d**e**f**g**h***::crimp****transform quadrilateral***src**dst***::crimp****transform reflect line**?*a*?*b***::crimp****transform reflect x****::crimp****transform reflect y****::crimp****transform rotate***theta*?*center*?**::crimp****transform scale***sx**sy***::crimp****transform shear***sx**sy***::crimp****transform translate***dx**dy***::crimp::black_white_vertical****::crimp::bilateral_****image**sigma-space**sigma-range***::crimp::joint_bilateral_****image**wimage**sigma-space**sigma-range***::crimp::color_combine***image**vector***::crimp::color_mix***image**matrix***::crimp::connected_components***image**8connected***::crimp::connected_components_****image**8connected**bgValue***::crimp::euclidean_distance_map_float***image***::crimp::indicator_grey8_float***image***::crimp::hough_grey8***image**emptybucketcolor***::crimp::gaussian_01_float***image**derivative**sigma***::crimp::gaussian_10_float***image**derivative**sigma***::crimp::gaussian_blur_float***image**sigma***::crimp::gaussian_laplacian_float***image**sigma***::crimp::gaussian_gradient_mag_float***image**sigma***::crimp::map_2*_****image**map***::crimp::map2_****image**mapNimage*...*mapNcontrol*...**::crimp::region_sum***image**radius***::crimp::exp_float***image***::crimp::log_float***image***::crimp::log10_float***image***::crimp::offset_float***image**offset***::crimp::pow_float_float***imageBase**imageExponent***::crimp::scale_float***image**factor***::crimp::sqrt_float***image***::crimp::non_max_suppression***imageMagnitude**imageAngle***::crimp::trace_hysteresis***image**low**high***::crimp::window_****image***::crimp::window_****image*

This package, built on top of the **crimp::core** package
provides the majority of CRIMPs power, manipulating and transforming
images in a number of ways.

For a basic introduction of the whole CRIMP eco-system please read
the *CRIMP - Introduction to CRIMP* (sic!).
The basic concepts used here, like images, image types, etc. are
described in the reference manpage for the *CRIMP - Foundation*.
We will not repeat them here, but assume that the reader knows them
already.

In the overall architecture this package resides in the middle layer of the system's architecture, between core and applications, as shown at

Note that the intended audience of this document are the users of
**crimp**. Developers wishing to work on the internals of the
package, but unfamiliar with them, should read ... instead.

**::crimp****histogram***image*This method returns a nested dictionary as its result. The outer dictionary is indexed by the names of the channels in the

*image*. Its values, the inner dictionaries, are indexed by pixel value. The associated values are the number of pixels with that value.The method supports all image types except "grey32". Under the current system the result would be a dictionary with 2^32 keys and values, taking up, roughly, 192 GiByte of memory in the worst case, and 96 GiByte in best case (all counter values shared in a single object).

**::crimp****statistics basic***image*This method returns a nested dictionary as its result. The outer dictionary contains basic information about the image, see the list of keys below. The inner dictionaries hold data about each (color) channel in the image, namely histogram and derived data like minumum pixel value, maximum, etc.

**dimensions**2-element list holding image width and height, in this order.

**height**Image height as separate value.

**pixels**Number of pixels in the image, the product of its width and height.

**type**Type of the image.

**width**Image width as separate value.

**channels**List of the names for the channels in the image.

**channel**A dictionary mapping the names of the image's channels, as listed under key

**channels**, to a dictionary holding the statistics for that channel.**min**The minimal pixel value with a non-zero population.

**max**The maximal pixel value with a non-zero population.

**mean**The arithmetic mean (aka average) of pixel values.

**middle**The arithmetic mean of the min and max pixel values.

**median**The median pixel value.

**stddev**The standard deviation of pixel values.

**variance**The variance of pixel values, square of the standard deviation.

**histogram**A dictionary mapping pixel values to population counts.

**hf**The histogram reduced to the population counts, sorted by pixel value to direct indexing into the list by pixel values.

**cdf**The

*cumulative density function*of pixel values. The discrete integral of**hf**.**cdf255**Same as

**cdf**, except scaled down so that the last value in the series is 255.

The method supports all image types except "grey32". Under the current system the result would contain internal dictionaries with 2^32 keys and values, taking up, roughly, 192 GiByte of memory in the worst case, and 96 GiByte in best case (all counter values shared in a single object).

**::crimp****statistics otsu***stats*This method takes a dictionary of basic image statistics as generated by

**crimp statistics basic**and returns an extended dictionary containing a threshold for image binarization computed by Otsu's method (See reference 2). Note that this threshold is computed separately for each channel and stored in the channel specific part of the dictionary, using the key**otsu**.

**::crimp****add***image1**image2*?*scale*? ?*offset*?This method combines the two input images into a result image by performing a pixelwise addition (image1 + image2) followed by division through

*scale*and addition of the*offset*. They default to**1**and**0**respectively, if they are not specified.**::crimp****alpha blend***foreground**background**alpha*This method takes two images of identical dimensions and a blending factor

*alpha*and returns an image which is a mix of both, with each pixel blended per the formulaor, alternatively written

This means that the

*foreground*is returned as is for "*alpha*== 255", and the*background*for "*alpha*== 0". I.e. the argument*alpha*controls the*opacity*of the foreground, with**1**and**0**standing for "fully opaque" and "fully transparent", respectively.The following combinations of fore- and background image types are supported:

Result = Foreground Background ------ ---------- ---------- grey8 grey8 grey8 hsv hsv hsv rgb rgb grey8 rgb rgb rgb rgb rgb rgba rgba rgba grey8 rgba rgba rgb rgba rgba rgba ------ ---------- ----------

**::crimp****alpha set***image**mask*This command takes two images, the input and a

*mask*, and returns an image as result in which the mask is the alpha channel of the input. The result is therefore always of type**rgba**, as the only type supporting an alpha channel.The input image can be of type

**rgb**or**rgba**. In case of the latter the existing alpha channel is replaced, in case of the former an alpha channel is added.For the mask images of type

**grey8**and**rgba**are accepted. In the case of the latter the mask's alpha channel is used as the new alpha channel, in case of the former the mask itself is used.**::crimp****alpha opaque***image*A convenience method over

**alpha set**, giving the*image*a mask which makes it fully opaque.**::crimp****alpha over***foreground**background*This method is similar to

**blend**above, except that there is no global blending parameter. This information is taken from the "alpha" channel of the*foreground*image instead. The blending formula is the same, except that the alpha parameter is now a per-pixel value, and not constant across the image.Due to the need for an alpha channel the

*foreground*has to be of type**rgba**. For the*background*image the types**rgb**and**rgba**are supported.**::crimp****atan2***image1**image2*This method combines the two input images into a result image by computing

at each pixel.

The input is restricted to images of the single-channel types, i.e.

**float**and**grey{8,16,32}**. The result is always of type**float**.An application of this operation is the computation of a gradient's direction from two images representing a gradient in X and Y directions. For the full conversion of such cartesian gradients to a polar representation use the

**crimp hypot**operation to compute the gradient's magnitude at each pixel.**::crimp****blank***type**width**height**value*...This method returns a blank image of the given image type and dimensions. The

*value*s after the dimensions are the pixel values to fill the pixels in the image's channels with, per its type.The method supports the image types

**rgb**,**rgba**,**hsv**,**float**,**fpcomplex**,**grey8**,**grey16**, and**grey32**.For the multi-channel types the method automatically extends the pixel values with

**0**if not enough values were provided.**::crimp****crop***image**ww**hn**we**hs*This method is the counterpart to the

**expand**family of methods, shrinking an*image*by removing a border. The size of this border is specified by the four arguments*ww*,*hn*,*we*, and*hs*which provide the number of pixels to remove from the named edge. See the image below for a graphical representation.**::crimp****cut***image**dx**dy**w**h*This method takes the rectangular region specified through its

*x*/*y*position relative to the upper-left corner of the input*image*and its dimensions, and returns it as its own image.Note that while both

*w*and*h*are allowed to be**0**, resulting in the return of an empty image, they are not allowed to be negative.Further note that it is allowed to specify regions which address pixels outside of the input image. In the result these pixels will be set to

**0**(meaning black, opaque, etc. as per the semantics of the image type).The location of the result is the location of the input, suuitably modified by

*dx*and*dy*.**::crimp****decimate xy***image**factor**kernel***::crimp****decimate x***image**factor**kernel***::crimp****decimate y***image**factor**kernel*This is a convenience method combining the two steps of filtering an image (via

**filter convolve**), followed by a**downsample**step. See the method**interpolate**for the complementary operation.Note that while the

*kernel*argument for**filter convolve**is expected to be the 1D form of a separable low-pass filter no checks are made. The method simply applies both the kernel and its transposed form.The method

**pyramid gauss**is a user of this method.**::crimp****degamma***image**y*This method takes an image, runs it through an

**inverse gamma correction**with parameter*y*, and returns the corrected image as it result. This is an application of method**remap**, using the mapping returned by "**map degamma***y*". This method supports all image types supported by the method**remap**.**::crimp****difference***image1**image2*This method combines the two input images into a result image by taking the pixelwise absolute difference (|image1 - image2|).

**::crimp****downsample xy***image**factor***::crimp****downsample x***image**factor***::crimp****downsample y***image**factor*This method returns an image containing only every

*factor*pixel of the input*image*(in x, y, or both dimensions). The effect is that the input is shrunken by*factor*. It is the complement of method**upsample**.Using the method as is is not recommended because the simple subsampling will cause higher image frequencies to alias into the reduced spectrum, causing artifacts to appear in the result. This is normally avoided by running a low-pass filter over the image before doing downsampling, removing the problematic frequencies.

The

**decimate**method is a convenience method combining these two steps into one.**::crimp****effect charcoal***image*This method applies a charcoal effect to the image, i.e. it returns a

**grey8**image showing the input as if it had been drawn with a charcoal pencil.**::crimp****effect emboss***image*This method applies an embossing effect to the image, i.e. it returns an image of the same type as the input showing the input as if it had been embossed into a metal plate with a stencil of some kind.

**::crimp****effect sharpen***image*This method sharpens the input image, i.e. returns an image of the same type as the input in which the input's edges are emphasized.

**::crimp****expand const***image**ww**hn**we**hs*?*value*...?**::crimp****expand extend***image**ww**hn**we**hs***::crimp****expand mirror***image**ww**hn**we**hs***::crimp****expand replicate***image**ww**hn**we**hs***::crimp****expand wrap***image**ww**hn**we**hs*This set of methods takes an image and expands it by adding a border. The size of this border is specified by the four arguments

*ww*,*hn*,*we*, and*hs*which provide the number of pixels to add at the named edge. See the image below for a graphical representation.The contents of the border's pixels are specified via the border type, the first argument after

**expand**, as per the list below.**const**The additional

*value*s specify the values to use for the color channels of the image. Values beyond the number of channels in the image are ignored. Missing values are generated by replicating the last value, except for the alpha channel, which will be set to**255**. If no values are present they default to**0**.**extend**This is a combination of

**mirror**and**replicate**. The outside pixels are the result of subtracting the outside pixel for**mirror**from the outside pixel for**replicate**(and clamping to the range [0...255]).**mirror**The outside pixels take the value of the associated inside pixels, found by reflecting its coordinates along the relevant edges.

**replicate**The outside pixels take the value of the associated edge pixels, i.e. replicating them into the border.

**wrap**The outside pixels take the value of the associated inside pixels, found by toroidial (cyclic) wrapping its coordinates along the relevant edges. This is also called tiling.

**::crimp****fft forward***image***::crimp****fft backward***image*These two methods implement 2D FFT (forward) and inverse FFT (backward).

The input is restricted to images of the single-channel types, i.e.

**float**,**grey{8,16,32}**and**fpcomplex**. The result is always of type**float**for input images other than**fpcomplex**, which returns an image of the same type instead.The former means that it is necessary to split

**rgb**, etc. images into their channels before performing an FFT, and that results of an inverse FFT have to be joined. See the methods**split**and**join**for the relevant operations and their syntax.The latter means that a separate invokation of method

**convert 2grey8**is required when reconstructing an image by inverting its FFT.**::crimp****filter ahe***image*?**-border***spec*? ?*radius*?This method performs adaptive histogram equalization to enhance the contrast of the input image. Each pixel undergoes regular histogram equalization, with the histogram computed from the pixels in the

**N**x**N**square centered on it, where "**N**= 2***radius**+1".The default radius is

**3**, for a 7x7 square.**::crimp****filter convolve***image*?**-border***spec*?*kernel*...This method runs the series of filters specified by the convolution

*kernel*s over the input and returns the filtered result. See the method**kernel**and its sub-methods for commands to create and manipulate suitable kernels.The border specification determines how the input image is expanded (see method

**expand**) to compensate for the shrinkage introduced by the filter itself. The*spec*argument is a list containing the name of the sub-method of**expand**to use, plus any additional arguments this method may need, except for the size of the expansion.By default a black frame is used as the border, i.e. "

*spec*== {const 0}".**::crimp****filter gauss discrete***image**sigma*?*r*?**::crimp****filter gauss sampled***image**sigma*?*r*?These methods apply a discrete or sampled gaussian blur with parameters

*sigma*and kernel*r*adius to the*image*. If the radius is not specified it defaults to the smallest integer greater than "3**sigma*".**::crimp****filter mean***image*?**-border***spec*? ?*radius*?This method applies a mean filter with

*radius*to the image. I.e. each pixel of the result is the mean value of all pixels in the**N**x**N**square centered on it, where "**N**= 2***radius**+1".The default radius is

**3**, for a 7x7 square.*NOTE*. As the mean is known to be in the range defined by the channel this method automatically converts float results back to the channel type. This introduces rounding / quantization errors. As a result of this price being paid the method is able to handle multi-channel images, by automatically splitting, processing, and rejoining its channels.The method

**filter stddev**on the other makes the reverse tradeoff, keeping precision, but unable to handle multi-channel images.**::crimp****filter rank***image*?**-border***spec*? ?*radius*?*percentile*??This method runs a rank-filter over the input and returns the filtered result.

The border specification determines how the input image is expanded (see method

**expand**) to compensate for the shrinkage introduced by the filter itself. The*spec*argument is a list containing the name of the sub-method of**expand**to use, plus any additional arguments this method may need, except for the size of the expansion.By default a black frame is used as the border, i.e. "

*spec*== {const 0}".The

*radius*specifies the (square) region around each pixel which is taken into account by the filter, with the pixel value selected according to the*percentile*. The filter region of each pixel is a square of dimensions "2**radius*+1", centered around the pixel.These two values default to

**3**and**50**, respectively.Typical applications of rank-filters are min-, max-, and median-filters, for percentiles 0, 100, and 50, respectively.

Note that percentiles outside of the range

**0**...**100**make no sense and are clamped to this range.**::crimp****filter stddev***image*?**-border***spec*? ?*radius*?This method applies a stand deviation filter with

*radius*to the image. I.e. each pixel of the result is the standard deviation of all pixel values in the**N**x**N**square centered on it, where "**N**= 2***radius**+1".The default radius is

**3**, for a 7x7 square.*NOTE*. As the standard deviation is often quite small and its precision important the result of this method is always an image of type**float**. Because of this this method is unable to handle multi-channel images as the results of processing their channels cannot be joined back together for the proper type.The method

**filter mean**on the other hand makes the reverse tradeoff, handling multi-channel images, but dropping precision.**::crimp****filter sobel x***image***::crimp****filter sobel y***image***::crimp****filter scharr x***image***::crimp****filter scharr y***image***::crimp****filter prewitt x***image***::crimp****filter prewitt y***image***::crimp****filter roberts x***image***::crimp****filter roberts y***image***::crimp****filter canny sobel***image***::crimp****filter canny deriche***image*These methods are convenience methods implementing a number of standard convolution filters using for edge detection and calculation of image gradients.

See the

**crimp gradient**methods for users of these filters.Also note that the

**x**methods emphasize gradient in the horizontal direction, and thus highlight*vertical*lines, and vice versa for**y**.**::crimp****filter wiener***image**radius*This method filters an image that has been degraded by constant power additive noise. It uses a pixelwise adaptive Filter method based on statistics estimated from a local neighborhood of each pixel. The default value for radius is 2

**::crimp****gamma***image**y*This method takes an image, runs it through a

**gamma correction**with parameter*y*, and returns the corrected image as it result. This is an application of method**remap**, using the mapping returned by "**map gamma***y*". This method supports all image types supported by the method**remap**.**::crimp****gradient sobel***image***::crimp****gradient scharr***image***::crimp****gradient prewitt***image***::crimp****gradient roberts***image*These methods generate two gradient images for the input image, in the X- and Y-directions, using different semi-standard filters. I.e. the result is a cartesian representation of the gradients in the input. The result is a 2-element list containing the X- and Y-gradient images, in this order.

**::crimp****gradient polar***cgradient*This method takes a gradient in cartesian representation (as returned by the above methods) and converts it to polar representation, i.e. magnitude and angle. The result of the method is a 2-element list containing two

**float**images, the magnitude and angle, in this order. The angle is represented in degrees running from 0 to 360.**::crimp****gradient visual***pgradient*This method takes a gradient in polar representation (as returned by method

**gradient polar**) and converts it into a color image (**rgb**) visualizing the gradient.The visualization is easier to understand in HSV space tough, with the angle mapped to Hue, i.e. color, magnitude to Value, and Saturation simply at full.

**::crimp****hypot***image1**image2*This method combines the two input images into a result image by computing

at each pixel.

The input is restricted to images of the single-channel types, i.e.

**float**and**grey{8,16,32}**. The result is always of type**float**.An application of this operation is the computation of the gradient magnitude from two images representing a gradient in X and Y directions. For the full conversion of such cartesian gradients to a polar representation use the

**crimp atan2**operation to compute the gradient's direction at each pixel.**::crimp****integrate***image*This method takes any single-channel image, i.e. of types

**float**and**grey{8,16,32}**, and returns its integral, i.e. a summed area table. The type of the result is always of type**float**.**::crimp****interpolate xy***image**factor**kernel***::crimp****interpolate x***image**factor**kernel***::crimp****interpolate y***image**factor**kernel*This is a convenience method combining the two steps of an

**upsample**, followed by a filter step (via**filter convolve**). See the method**decimate**for the complementary operation.Note that while the

*kernel*argument for**filter convolve**is expected to be 1D form of a separable low-pass filter no checks are made. The method simply applies both the kernel and its transposed form.The methods

**pyramid gauss**and**pyramid laplace**are users of this method.**::crimp****invert***image*This method takes an image, runs it through the

**inverse**function, and returns the modified image as it result. This is an application of method**remap**, using the mapping returned by "**map inverse**". This method supports all image types supported by the method**remap**.**::crimp****logpolar***image**rwidth**rheight*?*xcenter*? ?*ycenter*? ?*corners*?This method takes an

*image*and returns the log-polar transformation of the input. This means that in the result each pixel is described by an angle and the logarithm of the distance to a chosen point.The angle is plotted on the x-axis of the result, as fraction or multiples of degrees, depending on the chosen resolution

*rwidth*. A value of**360**, for example, provides a resolution of 1 degree in the result. The angle is counted from 0 due right (the positive x-axis of the input) counterclockwise.The log of the distance is plotted on the y-axis of the result, with a precision of

*rheight*.The

*center point*is specified as offset*xcenter*,*ycenter*from the center of the input image. I.e. the defaults of (0, 0) for both, when not specified, refer to the center of the input.The optional flag

*corners*specifies whether to include the corners of the input in the result (**true**), or not (**false**). This defaults to**true**, including the corners.**::crimp****matrix***image**matrix*This method takes an image and a 3x3 matrix specified as nested Tcl list (row major order), applies the projective transform represented by the matrix to the image and returns the transformed image as its result.

Notes: It is currently unclear how the output pixel is computed (nearest neighbour, bilinear, etc.) (code inherited from AMG). This requires more reading, and teasing things apart. The transfomred image is clipped to the dimensions of the input image, i.e. pixels from the input may be lost, and pixels in the output may be unset as their input would come from outside of the input.

The operation supports only images of type

**rgba**, and returns images of the same type.**::crimp****max***image1**image2*This method combines the two input images into a result image by taking the pixelwise maximum.

**::crimp****min***image1**image2*This method combines the two input images into a result image by taking the pixelwise minimum.

**::crimp****montage horizontal**?**-align****top**|**center**|**bottom**? ?**-border***spec*?*image*...**::crimp****montage vertical**?**-align****left**|**middle**|**right**? ?**-border***spec*?*image*...The result of these methods is an image where the input images have been placed adjacent to each from left to right (horizontal), or top to bottom (vertical). The input images have to have the same type.

There is no need however for them to have the same height, or width, respectively. When images of different height (width) are used the command will expand them to their common height (width), which is the maximum of all heights (widths). The expansion process is further governed by the values of the

**-align**and**-border**options, with the latter specifying the form of the expansion (see method**expand**for details), and the first specifying how the image is aligned within the expanded space.The

*spec*argument of**-border**is a list containing the name of the sub-method of**expand**to use, plus any additional arguments this method may need, except for the size of the expansion.The default values for

**-align**are**center**and**middle**, centering the image in the space. The default for the**-border**is a black frame, i.e. "*spec*== {const 0}".**::crimp****morph dilate***image***::crimp****morph erode***image*These two methods implement the basic set of morphology operations,

*erosion*, and*dilation*using a flat 3x3 brick as their structuring element. For grayscale, which we have here, these are, mathematically, max and min rank-order filters, i.e.dilate = filter rank 1 99.99 (max) erode = filter rank 1 0.00 (min)

The above definitions assume that background is

**black**, and foreground/object anything but black, usually**white**. Then it is easy to see that**dilate**expands the foreground/white, and erode expands background/black.**::crimp****morph close***image***::crimp****morph open***image*These two methods add to the basic set of morphology operations,

*opening*and*closing*. In terms of erosion and dilation:close = erode o dilate open = dilate o erode

**::crimp****morph gradient***image*The morphological

*gradient*is defined as[dilate $image] - [erode $image]

This can also be expressed as the sum of the external and internal gradients, see below.

**::crimp****morph igradient***image*The morphological

*internal gradient*is defined as$image - [erode image]

**::crimp****morph egradient***image*The morphological

*external gradient*is defined as[dilate $image] - $image

**::crimp****morph tophatw***image*The

*white tophat*transformation is defined as$image - [open $image]

See References 3 to 5 (page 32). This is a greyscale morphology operation which does not properly apply to binary images.

**::crimp****morph tophatb***image*The

*black tophat*transformation is defined as[close $image] - $image

See References 3 to 5 (page 33). This is a greyscale morphology operation which does not properly apply to binary images.

**::crimp****morph toggle***image*The

*toggle map*is defined as0.5 * ([erode $image] + [dilate $image])

See References 5, pages 34 and 35. This is a greyscale morphology operation to sharpen edges.

**::crimp****multiply***image1**image2*This method combines the two input images into a result image by performing a pixelwise multiplication. Note that the result of each multiplication is divided by

**255**to scale it back into the range [0...255].**::crimp****noise random***w**h*This method creates an image of type

**float**with the specified dimensions. The pixels are set to random values in the interval [0...1].**::crimp****noise saltpepper***image*?*density*?**::crimp****noise gaussian***image*?*mean*? ?*variance*?**::crimp****noise speckle***image*?*variance*?These methods add noises of different types to the given image.

**saltpepper**adds salt and pepper noise of the specified*density*. This density must be in the range [0...1]. If not specified it defaults to**0.05**.**gaussian**adds gaussian noise of the specified mean and variance to the image. If not specified the mean and variance default to**0**and**0.05**, respectively. Both must be in the range [0...1].**speckle**adds multiplicative noise of the specified variance to the image. This variance must be in the range [0...1]. If not specified it defaults to**0.05**.**::crimp****psychedelia***width**height**frames*This method creates an

**rgba**image of the specified dimensions according to an algorithm devised by Andrew M. Goth. The*frames*argument specifies how many images are in the series.*Attention:*This method keeps internal global state, ensuring that each call returns a slightly different image. Showing a series of such images as animation provides an effect similar to a lava lamp or hallucination.**::crimp****pyramid run***image**steps**stepcmd*This method provides the core functionality for the generation of image pyramids. The command prefix

*stepcmd*is run*steps*times, first on the*image*, then on the result of the previous step.The assumed signature of

*stepcmd*is**<stepcmd>***image*which is expected to return a list of two elements. The first element (

*result*) is added to the pyramid in building, whereas the second element (*iter*) is used in the next step as the input of the step command.

The final result of the method is a list containing the input

*image*as its first element, followed by the results of the step function, followed by the*iter*element returned by the last step, "*steps*+2" images in total.**::crimp****pyramid gauss***image**steps*This method generates a gaussian image pyramid

*steps*levels deep and returns it as a list of images.The first image in the result is the input, followed by

*steps*successively smaller images, each**decimate**d by a factor two compared to its predecessor, for a total length of "*steps*+1" images.The convolution part of the decimation uses

1/16 [1 4 6 4 1]

as its kernel.

**::crimp****pyramid laplace***image**steps*This method generates a laplacian image pyramid

*steps*levels deep and returns it as a list of images.The first image in the result is the input, followed by

*steps*band pass images (differences of gaussians). The first band pass has the same size as the input image, and each successor is**decimate**d by two. This is followed by one more image, the gaussian of the last step. This image is decimated by two compared to the preceding bandpass image. In total the result contains "*steps*+2" images.The convolution part of the decimation uses

1/16 [1 4 6 4 1]

as its kernel. The internal interpolation used to generate the band pass images (resynthesis) doubles the weights of this kernel for its convolution step.

**::crimp****remap***image**map*...This method is the core primitive for the per-pixel transformation of images, with each pixel (and channels within, if any) handled independently of all others. Applications of this operator provided by this package are (inverse) gamma correction, pixel inversion, and solarization. Many more are possible, especially when considering other colorspaces like HSV. There, for example, it is possible change the saturation of pixels, or shift the hue in arbitrary manner.

Beyond the input

*image*to transform one or more*maps*are specified which define how each pixel value in the input is mapped to a pixel value in the output. The command will accept at most that many maps as the input image has channels. If there are less maps than channel the last map specified is replicated to cover the other channels. An exception of this is the handling of the alpha channel, should the input image have such. There a missing map is handle as**identity**, i.e. the channel copied as is, without changes.The maps are not Tcl data structures, but images themselves. They have to be of type

**grey8**, and be of dimension 256x1 (width by height).The

**crimp map ...**methods are sources for a number of predefined maps, whereas the**mapof**method allows the construction of maps from Tcl data structures, namely lists of values.This method supports all image types with one or more single-byte channels, i.e. all but

**grey16**,**grey32**,**float**, and**bw**.**::crimp****matchsize***image1**image2*This method takes two images, forces them to be of the same size by expanding the smaller dimensions with black pixels, and then returns a list of the expanded images. The images in the result are in the same order as as arguments.

**::crimp****matchgeo***image**bbox*This method takes an image and a bounding box (list of x, y, w, and h), and expands the image with black pixels to match the box. The result of the expansion is returned.

An error is thrown if the image is not fully contained within the bounding box.

**::crimp****scale***image**scale*This method performs a pixel-wise multiplication of the image with a constant factor. It is currently supported by all

**greyN**image types, plus the types**float**and**fpcomplex**. The first accept an integer scaling factor, whereas the last two accept any floating point number.**::crimp****screen***image1**image2*This method combines the two input images by inverting the multiplication of the inverted input images. I.e.

**::crimp****solarize***image**threshold*This method takes an image, runs it through the

**solarize**function with parameter*threshold*, and returns the modified image as it result. This is also known as the*sabattier effect*. This is an application of method**remap**, using the mapping returned by "**map solarize***threshold*". This method supports all image types supported by the method**remap**.**::crimp****square***image*This is a convenience method equivalent to "

**crimp multiply***image**image*".**::crimp****subtract***image1**image2*?*scale*? ?*offset*?This method combines the two input images into a result image by performing a pixelwise subtraction (image1 - image2) followed by division through

*scale*and addition of the*offset*. They default to**1**and**0**respectively, if they are not specified.**::crimp****threshold global above***image**threshold*This method takes an image, runs it through the

**threshold above**function with parameter*threshold*, and returns the modified image as it result. As the result only contains black and white, i.e. 2 colors, this process is also called*binarization*or foreground/background segmentation. This is an application of method**remap**, using the mapping returned by "**map threshold above***threshold*". This method supports all image types supported by the method**remap**.**::crimp****threshold global below***image**threshold*This method takes an image, runs it through the

**threshold below**function with parameter*threshold*, and returns the modified image as it result. As the result only contains black and white, i.e. 2 colors, this process is also called*binarization*, or foreground/background segmentation. This is an application of method**remap**, using the mapping returned by "**map threshold below***threshold*". This method supports all image types supported by the method**remap**.**::crimp****threshold global inside***image**min**max*This method takes an image, runs it through the

**threshold inside**function with parameters*min*and*max*, and returns the modified image as it result. As the result only contains black and white, i.e. 2 colors, this process is also called*binarization*or foreground/background segmentation. This is an application of method**remap**, using the mapping returned by "**map threshold above***threshold*". This method supports all image types supported by the method**remap**.**::crimp****threshold global outside***image**min**max*This method takes an image, runs it through the

**threshold outside**function with parameters*min*and*max*, and returns the modified image as it result. As the result only contains black and white, i.e. 2 colors, this process is also called*binarization*, or foreground/background segmentation. This is an application of method**remap**, using the mapping returned by "**map threshold below***threshold*". This method supports all image types supported by the method**remap**.**::crimp****threshold global middle***image***::crimp****threshold global mean***image***::crimp****threshold global median***image***::crimp****threshold global otsu***image*These four methods are convenience methods layered on top of

**crimp threshold global below**. They compute the value(s) to perform the thresholding with from the global statistics of the input image, with the element taken named by the method. For reference see the documentation of method**crimp statistics ...**. Note that they treat each color channel in the image separately.**::crimp****threshold local***image**threshold*...This method takes an

*image*and one or more*threshold*maps and returns an image where all pixels of the input which were larger or equal to the corresponding pixel in the map are set to black. All other pixels are set to white. Each map is applied to one color channel of the input image. If there are too many maps the remainder is ignored. If there are not enough maps the last map is replicated.This is the core for all methods of non-global

*binarization*, i.e. foreground/background segmentation. Their differences are just in the calculation of the maps.This method supports all image types with one or more single-byte channels, i.e. all but

**grey16**,**grey32**, and**bw**.**::crimp****upsample xy***image**factor***::crimp****upsample x***image**factor***::crimp****upsample y***image**factor*This method returns an image inserting

*factor*black pixels between each pixel of the input*image*(in x, y, or both dimensions). The effect is that the input is expanded by*factor*. It is the complement of method**downsample**.Using the method as is is not recommended because this simple upsampling will cause copies of the image to appear at the higher image frequencies in the expanded spectrum. This is normally avoided by running a low-pass filter over the image after the upsampling, removing the problematic copies.

The

**interpolate**method is a convenience method combining these two steps into one.**::crimp****wavy***image**offset**adj1**adjb*This method processes the input

*image*according to an algorithm devised by Andrew M. Goth, according to the three parameters*offset*,*adj1*, and*adjb*, and returns the modified image as its result.The operation supports only images of type

**rgba**, and returns images of the same type.**::crimp****flip horizontal***image***::crimp****flip transpose***image***::crimp****flip transverse***image***::crimp****flip vertical***image*This set of methods performs mirroring along the horizontal, vertical and diagonal axes of the input

*image*, returning the mirrored image as their output. Transpose mirrors along the main diagonal, transverse along the secondary diagonal. These two methods also exchange width and height of the image in the output.The methods currently support the image types

**rgb**,**rgba**,**hsv**, and**grey8**.**::crimp****resize**?**-interpolate****nneighbour**|**bilinear**|**bicubic**?*image**w**h*This method takes the input

*image*and resizes it to the specified width*w*and height*h*. In constrast to**cut**this is not done by taking part of the image in the specified size, but by scaling it up or down as needed. In other words, this method is a degenerate case of a projective transform as created by the**transform**methods and used by method**warp projective**(see below).Like the aforementioned general method this method supports all the possible interpolation types, i.e. nearest neighbour, bilinear, and bicubic. By default

**bilinear**interpolation is used, as a compromise between accuracy and speed.**::crimp****rotate cw***image***::crimp****rotate ccw***image*This set of methods rotates the image in steps of 90 degrees, either clockwise and counter to it.

**::crimp****rotate half***image*This methods rotates the image a half-turn, i.e. 180 degrees.

**::crimp****warp field**?**-interpolate****nneighbour**|**bilinear**|**bicubic**?*image**xvec**yvec*This method takes an input image and two images the size of the expected result which provide for each pixel in the result the coordinates to sample in the input to determine the result's color.

This allows the specification of any possible geometric transformation and warping, going beyond even projective transformations.

The two images providing the coordinate information have to be of the same size, which is also the size of the returned result. The type of the result is however specified through the type of the input image.

The method supports all the possible interpolation types, i.e. nearest neighbour, bilinear, and bicubic. By default

**bilinear**interpolation is used, as a compromise between accuracy and speed.**::crimp****warp projective**?**-interpolate****nneighbour**|**bilinear**|**bicubic**?*image**transform*This method accepts a general projective

*transform*as created by the**transform**methods, applies it to the input*image*and returns the projected result.Like the

**resize**method above this method supports all the possible interpolation types, i.e. nearest neighbour, bilinear, and bicubic. By default**bilinear**interpolation is used, as a compromise between accuracy and speed.*Note*that the returned result image is made as large as necessary to contain the whole of the projected input. Depending on the transformation this means that parts of the result can be black, coming from outside of the boundaries of the input. Further, the origin point of the result may conceptually be inside or outside of the result instead of at the top left corner, because of pixels in the input getting projected to negative coordinates. To handle this situation the result will contain the physical coordinates of the conceptual origin point in its meta data, under the hierarchical key**crimp origin**.**::crimp****window***image*This method takes an image, applies a windowing function to it that fades the pixels to black towards the edges, and returns the windowed result.

**::crimp****convert 2grey32***image***::crimp****convert 2grey16***image***::crimp****convert 2grey8***image***::crimp****convert 2float***image***::crimp****convert 2complex***image***::crimp****convert 2hsv***image***::crimp****convert 2rgba***image***::crimp****convert 2rgb***image***::crimp****convert 2rgb***image*This set of methods all convert their input

*image*to the specified type and returns it as their result. All converters accept an image of the destination type as input and will pass it through unchanged.The converters returning a

**grey8**image support**float**,**rgb**and**rgba**as their input. For multi-channel input they use the ITU-R 601-2 luma transform to merge the color channels.The converters returning a

**grey16**,**grey32**image support only**float**as their input.The converters to HSV support

**rgb**and**rgba**as their input as well.The conversion to

**rgba**accepts only**hsv**as input, adding a blank (fully opaque) alpha channel. For more control over the contents of an image's alpha channel see the methods**setalpha**and**join rgba**.The conversion to

**rgb**accepts both**rgba**and**hsv**images as input.The conversion to

**float**supports only**fpcomplex**as input. It simply strips the imaginary part of the input.The conversion to

**fpcomplex**accepts**float**,**grey8**,**grey16**, and**grey32**as input, and adds a constant**0**imaginary part.**::crimp****complex magnitude***image*This method takes an image of type

**fpcomplex**as input and returns an image of type**float**containing the pixel-wise magnitude of the input.**::crimp****complex 2complex***image*This method takes an image of type

**float**as input and returns an image of type**fpcomplex**with each pixel's real part containing the input, and the imaginary part set to**0**.This method is an alias for

**crimp convert 2complex**.**::crimp****complex imaginary***image*This method takes an image of type

**fpcomplex**as input and returns an image of type**float**containing the pixel-wise**imaginary**part of the input.**::crimp****complex real***image*This method takes an image of type

**fpcomplex**as input and returns an image of type**float**containing the pixel-wise**real**part of the input.This method is an alias for

**crimp convert 2float**as applied to images of type**fpcomplex**.**::crimp****complex conjugate***image*This method takes an image of type

**fpcomplex**as input and returns an image of the same type containing the pixel-wise complex conjugate of the input.**::crimp****join 2hsv***hueImage**satImage**valImage***::crimp****join 2rgba***redImage**greenImage**blueImage**alphaImage***::crimp****join 2rgb***redImage**greenImage**blueImage***::crimp****join 2complex***realImage**imaginaryImage***::crimp****join 2grey16***msbImage**lsbImage***::crimp****join 2grey32***mmsbImage**lmsbImage**mlsbImage**llsbImage*This set of methods is the complement of method

**split**. Each takes a set of**grey8**images and fuses them together into an image of the given type, with each input image becoming one channel of the fusing result, which is returned as the result of the command. All input images have to have the same dimensions.The command

**join 2complex**is an exception regarding the input. It accepts images of type**float**, not**grey8**.The commands

**join 2grey***are slightly different too. As the result has only one color channel, what is to join ? Their pixels are multi-byte, 2 and 4 respectively. The input images are not color channel, but become the msb and lsb of the respective pixel in the result.**::crimp****split***image*This method takes an image of one of the multi-channel types, i.e.

**rgb**,**rgba**,**hsv**, and**fpcomplex**and returns a list of**grey8**images, each of which contains the contents of one of the channels found in the input image.The input image type

**fpcomplex**is an exception regarding the output. It returns images of type**float**, not**grey8**.The method is also able to take an image of one of the single-channel multi-byte types, i.e.

**grey16**, and**grey32**and returns a list of 2 (4)**grey8**images, each of which contains one of the bytes a pixel is made out of, in msb to lsb order.The channel images in the result are provided in the same order as they are accepted by the complementary

**join**method, see above.

**::crimp****read pgm***string*This method returns an image of type

**grey8**containing the data of the portable grey map (PGM) stored in the*string*. The method recognizes images in both plain and raw sub-formats.**::crimp****read ppm***string*This method returns an image of type

**rgb**containing the data of the portable pix map (PPM) stored in the*string*. The method recognizes images in both plain and raw sub-formats.**::crimp****read strimj***string*?*colormap*?This method returns an image of type

**rgba**containing the data of the*strimj*(string image) (See http://wiki.tcl.tk/1846) stored in the*string*.The caller can override the standard mapping from pixel characters to colors by specifying a

*colormap*. This argument is interpreted as dictionary mapping characters to triples of integers in the range [0...255], specifying the red, green, and blue intensities.An example of a strimj is:

@...@.......@.@...... @...@.......@.@...... @...@..@@@..@.@..@@@. @@@@@.@...@.@.@.@...@ @...@.@@@@@.@.@.@...@ @...@.@.....@.@.@...@ @...@.@...@.@.@.@...@ @...@..@@@..@.@..@@@.

**::crimp****gradient grey8***from**to**size***::crimp****gradient rgb***from**to**size***::crimp****gradient rgba***from**to**size***::crimp****gradient hsv***from**to**size*This set of methods takes two "color" (pixel value) arguments and returns an image of height 1 and width

*size*containing a gradient interpolating between these two colors, with*from*in the pixel at the left (x == 0) and*to*at the right (x ==*size*-1).*size*has to be greater than or equal to**2**. An error is thrown if that restriction is not met.The resulting image has the type indicated in the method name. This also specifies what is expected as the contents of the arguments

*from*and*to*. For**grey8**these are simple pixel values in the range 0...255 whereas for the types**rgb**and**hsv**the arguments are triples (3-element lists) specifying the R, G, and B (and H, S, and V respectively) values.**::crimp****register translation***needle**haystack*This method takes two images which are translated copies of each other and returns a dictonary containing the two keys

**Xshift**and**Yshift**, which together specify the translation to apply to the*needle*to place it in the*haystack*.**::crimp****kernel make***matrix*?*scale*? ?*offset*?This method takes a

*matrix*of weights and an optional*scale*factor and returns a structure containing the associated convolution kernel, ready for use by method**filter convolve**.If

*scale*is left unspecified it defaults to the sum of all weights in the matrix.If

*offset*is left unspecified it defaults to 128 if the sum of weights is 0, and 0 else. In effect zero-sum kernels, like the basic edge-detectors, are shifted so that results in the range -128..127 correspond to 0..255.The

*matrix*has the same general format as the pixel matrix for method**read tcl grey8**, i.e. a list of lists (rows) of values, and is treated in the same way, i.e. the number of columns is the maxium length over the row lists, and shorter lists are padded with**128**. The values are expected to be integer numbers in the range -128..127.**::crimp****kernel fpmake***matrix*?*offset*?This method is like

**kernel make**except that the generated kernel is based on floating-point values. Because of this it is not accpeting a scale argument either, it is expected that the kernel weights already have the proper sum.The

*matrix*has the same general format as the pixel matrix for method**read tcl float**, i.e. a list of lists (rows) of values, and is treated in the same way, i.e. the number of columns is the maxium length over the row lists, and shorter lists are padded with**255**. The values are expected to be floating-point numbers.**::crimp****kernel transpose***kernel*This method takes a

*kernel*as returned by the method**kernel make**and returns a transposed kernel, i.e. one where the x- and y-axes are switched. For example(1) (2) {1 2 4 2 1} ==> (4) (2) (1)

This method is its own inverse, i.e. application to its result returns the original input, i.e.

[transpose [transpose $K]] == $K

**::crimp****kernel image***kernel*This method extracts and returns the internal image used to store the

*kernel*'s coefficients.**::crimp****map***arg*...This method accepts the same sub-methods and arguments as are accepted by the

**table**method below. In contrast to**table**the result is not a list of values, but a map image directly suitable as argument to the**remap**method.**::crimp****mapof***table*This method accepts a list of 256 values, constructs a map image directly suitable as argument to the

**remap**method, and returns this map image as its result.**::crimp****table compose***f**g*This accepts two lookup tables (aka functions) specified as lists of 256 values, constructs the composite function f(g(x)), and then returns this new function as its result.

**::crimp****table eval wrap***cmd***::crimp****table eval clamp***cmd*This method returns a list of 256 values, the result of running the values 0 to 255 through the function specified by the command prefix

*cmd*. The results returned by the command prefix are rounded to the nearest integer and then forced into the domain [0..255] by either wrapping them around (modulo 256), or clamping them to the appropriate border, i.e 0, and 255 respectively.The signature of the command prefix is

**<cmd>***x*which is expected to return a number in the range [0..255]. While the result should be an integer number it is allowed to be a float, the caller takes care to round the result to the nearest integer.

**::crimp****table degamma***y*This method returns a list of 256 values, the result of running the values 0 to 255 through the

**inverse gamma correction**with parameter*y*. This inverse correction, defined in the domain of [0..1] for both argument and result, is defined as:Scaling of argument and result into the domain [0..255] of pixel values, and rounding results to the nearest integer, causes the actual definition used to be

**::crimp****table gamma***y*This method returns a list of 256 values, the result of running the values 0 to 255 through the

**gamma correction**with parameter*y*. This correction, defined in the domain of [0..1] for both argument and result, is defined as:Scaling of argument and result into the domain [0..255] of pixel values, and rounding results to the nearest integer, causes the actual definition used to be

**::crimp****table gauss***sigma*This method returns a list of 256 values, the result of running the values 0 to 255 through the

**sampled gauss**function with parameter*sigma*. This function is defined as:**::crimp****table identity**This method returns a list of 256 values, the result of running the values 0 to 255 through the

**identity**function, which is defined as**::crimp****table invers**This method returns a list of 256 values, the result of running the values 0 to 255 through the

**inverse**function, which is defined as**::crimp****table linear wrap***gain**offset***::crimp****table linear clamp***gain**offset*This method returns a list of 256 values, the result of running the values 0 to 255 through a simple linear function with parameters

*gain*(the slope) and*offset*. The results are rounded to the nearest integer and then forced into the domain [0..255] by either wrapping them around (modulo 256), or clamping them to the appropriate border, i.e 0, and 255 respectively. Thus the relevant definitions arefor the wrapped case, and

when clamping.

**::crimp****table log**?*max*?This method returns a list of 256 values, the result of running the values 0 to 255 through the

**log-compression**function with parameter*max*. This parameter is the maximum pixel value the function is for, this value, and all larger will be mapped to 255. This function is defined as:**::crimp****table solarize***threshold*This method returns a list of 256 values, the result of running the values 0 to 255 through the

**solarize**function, with parameter*threshold*. This function is defined as:Note how the function is the

**identity**for values under the threshold, and the**inverse**for values at and above it. Its application to an image produces what is known as either*solarization*or*sabattier effect*.**::crimp****table sqrt**?*max*?This method returns a list of 256 values, the result of running the values 0 to 255 through the

**sqrt-compression**function with parameter*max*. This parameter is the maximum pixel value the function is for, this value, and all larger will be mapped to 255. This function is defined as:**::crimp****table stretch***min**max*This is a convenience method around

**table linear**which maps*min*to 0, and*max*to 255, with linear interpolation in between. Values below*min*and above*max*are clamped to 0 and 255 respectively.**::crimp****table threshold above***threshold*This method returns a list of 256 values, the result of running the values 0 to 255 through a

**thresholding**(or*binarization*) function, with parameter*threshold*. This function is defined as:**::crimp****table threshold below***threshold*This method returns a list of 256 values, the result of running the values 0 to 255 through a

**thresholding**(or*binarization*) function, with parameter*threshold*. This function is defined as:**::crimp****table threshold inside***min**max*This method returns a list of 256 values, the result of running the values 0 to 255 through a

**thresholding**(or*binarization*) function, with parameters*min*and*max*. This function is defined as:**::crimp****table threshold outside***min**max*This method returns a list of 256 values, the result of running the values 0 to 255 through a

**thresholding**(or*binarization*) function, with parameters*min*and*max*. This function is defined as:**::crimp****table fgauss discrete***sigma*?*r*?**::crimp****table fgauss sampled***sigma*?*r*?This method computes the table for a discrete or sampled gaussian with parameters

*sigma*and kernel*r*adius. If the radius is not specified it defaults to the smallest integer greater than "3**sigma*".**::crimp****transform affine***a**b**c**d**e**f*This method returns the affine transformation specified by the 2x3 matrix

|a b c| |d e f|

Note that it is in general easier to use the methods

**rotate**,**scale**, and**translate****scale**to generate the desired transformation piecemal and then use**chain**to chain the pieces together.**::crimp****transform chain***transform*...This method computes and returns the projective transformation equivalent to the application of the specified transformations to a 2d point in the given order, i.e with the transformation at the beginning of the argument list applied first, then the one after it, etc.

**::crimp****transform identity**This method returns the projective identity

*transform*ation.**::crimp****transform invert***transform*This method computes and returns the inverse of the specified projective

*transform*ation.**::crimp****transform projective***a**b**c**d**e**f**g**h*This method returns the projective transformation specified by the 3x3 matrix

|a b c| |d e f| |g h 1|

Note that for the affine subset of projective transformation it is in general easier to use the methods

**rotate**,**scale**, and**translate****scale**to generate the desired transformation piecemal and then use**chain**to chain the pieces together.And for a true perspective transformation specification through

**quadrilateral**should be simpler as well.**::crimp****transform quadrilateral***src**dst*This method returns the projective transformation which maps the quadrilateral

*src*on to the quadrilateral*dst*.Each quadrilateral is specified as a list of 4 points, each point a pair of x- and y-coordinates.

The 4 points of each quadrilateral define its corners starting at the top left and going in clock-wise order.

**::crimp****transform reflect line**?*a*?*b*This methods returns the projective transformation which reflects the image about an arbitrary line specified by the two points

*a*and*b*, each point a pair of x- and y-coordinates.. If point*a*is not specified it defaults to (0,0), i.e. the coordinate origin.**::crimp****transform reflect x**This methods returns the projective transformation which reflects the image about the x-axis.

**::crimp****transform reflect y**This methods returns the projective transformation which reflects the image about the y-axis.

**::crimp****transform rotate***theta*?*center*?This methods returns the projective transformation which rotates the image by the angle

*theta*around the point*center*. If the latter is not specified {0 0} is assumed. The point, if present, is specified as pair of x- and y-coordinates.The angle is specified in degrees, with

**0**not rotating the image at all. Positive values cause a counterclockwise rotation, negative values a clockwise one.**::crimp****transform scale***sx**sy*This methods returns the projective transformation which scales an image by factor

*sx*in width, and*sy*in height. Values larger than**1**expand the image along the specified dimension, while values less than**1**shrink it. Negative values flip the respective axis.**::crimp****transform shear***sx**sy*This methods returns the projective transformation which shears an image by factor

*sx*along the width, and*sy*along the height.**::crimp****transform translate***dx**dy*This methods returns the projective transformation which translates an image by

*dx*pixels along the x-axis, and*dx*pixels along the y-axis. Values larger than**0**move the image to the right, or down, along the specified dimension, while values less than**0**move it to the left, or up.

The package contains a number of primitives which are either not really useful to a regular user, or have not gotten a nice interface yet, possibly because it is not clear how that interface should look like.

These primitives are collected here, so that they are not forgotten, i.e. as a reminder to either make them properly available, document as internal/undocumented/etc, or remove them.

**::crimp::black_white_vertical**Generates a fixed checker board image. The output is 256x256

**grey8**image, with 16x16 blocks. Debug use only, so far.**::crimp::bilateral_****image**sigma-space**sigma-range***::crimp::joint_bilateral_****image**wimage**sigma-space**sigma-range*Regular and cross bilateral filters. Still looking buggy, possibly bad memory accesses.

**::crimp::color_combine***image**vector*This operation combines the channels of the input into a single

**grey8**value, the result of performing a scalar product of each pixel with the 3x1*vector*(**float**image).**::crimp::color_mix***image**matrix*This operation mixes the color channels of the input, the result of performing a matrix multiplication of each pixel with the 3x3

*matrix*(**float**image).**::crimp::connected_components***image**8connected***::crimp::connected_components_****image**8connected**bgValue*Computing (labeling) the connected components of the input image, using either 4- or 8-neighbourhood. The primitives accepting a background value use it to distinguish foreground and background and coalesce the latter into a single component, even if its area is disconnected.

The result is always of type

**grey32**, to have enough range for the label counters.**::crimp::euclidean_distance_map_float***image***::crimp::indicator_grey8_float***image*These two operations together allow the creation of distance maps from images, i.e. watershed diagrams. Currently only used in a demonstration for this.

**::crimp::hough_grey8***image**emptybucketcolor*Hough transformation of an image. Currently only used in a demonstration so far.

**::crimp::gaussian_01_float***image**derivative**sigma***::crimp::gaussian_10_float***image**derivative**sigma***::crimp::gaussian_blur_float***image**sigma***::crimp::gaussian_laplacian_float***image**sigma***::crimp::gaussian_gradient_mag_float***image**sigma*Fast gaussian filters and derivatives, applied in X and Y directions, i.e. rows and coluimns of the input image. The

*derivative*is either**0**Gaussian

**1**Gradient

**2**Laplacian

The methods

**01**and**10**apply a gaussian or derivative to the image, in X and Y directions, respectively. I.e. they operate on the rows, or columns of the image, respectively.**blur**applies a gaussian blur in both directions, i.e.output = gauss10 (gauss01 (image))

**laplacian**returns an approximation of the scalar second derivative, the*laplacian*of the image. It is computed by applying a laplacian of a gaussian, for both X and Y directions, and adding the results, i.e.:laplace20 (gauss01 (image)) + laplace02 (gauss20 (image))

**gradient_mag**returns the magnitude of the image gradient. It is computed by applying a gradient of gaussian to X and Y directions, and computing the length of the resulting 2-vector (euclidean norm), i.e.hypot (gauss10 (grad10 (image)), gauss10 (grad01 (image)))

**::crimp::map_2*_****image**map*Operators applying a piecewise linear

*map*to the input image. The map is stored in a Tcl list containing 2 elements, each a bytearray. The first stores the abscissaes delineating the intervals, the second the ordinates at these interval borders. The format of the binary data depends on the types of input and output values (byte, int, float, ...).For conversion a pixel value is searched for in the intervals of abscissae. With both the interval and the fraction inside of it known the output is then linearly interpolated from the associated ordinates. The search is a binary one, assuming that the abscissae are sorted from smaller to larger. If the input value is outside of the defined intervals the outputs associated with the min and max abscissae are returned, respectively.

Not exposed yet, unclear how the higher level API should look like.

**::crimp::map2_****image**mapNimage*...*mapNcontrol*...Primitives applying per-pixel transformations to multi-channel images (HSV, RGB, RGBA). Each channel is transformed with one map image per channel, and one integer index per channel selecting the control channel. Each map is a 256x256

**grey8**image indexed by the pixel data of the channel to be mapped in X, and the pixel data of the chosen control channel in Y. This enables effects like hue-dependent changes to saturation or value, value dependent color-shifts, etc.Not exposed yet, unclear how the higher level API should look like.

**::crimp::region_sum***image**radius*Takes a

*summed area table*as input and computes the sums for square windows of the*radius*around each pixel. Time is constant per pixel, independent of the radius, because of the nature of the input. Only used internally so far.**::crimp::exp_float***image***::crimp::log_float***image***::crimp::log10_float***image***::crimp::offset_float***image**offset***::crimp::pow_float_float***imageBase**imageExponent***::crimp::scale_float***image**factor***::crimp::sqrt_float***image*Only used internally (or demos), in various calculations like arithmetic mean, standard deviation, etc. Might be useful in general, as unary operator.

**::crimp::non_max_suppression***imageMagnitude**imageAngle***::crimp::trace_hysteresis***image**low**high*Abandoned, part of an older attempt at canny edge detection.

**::crimp::window_****image***::crimp::window_****image*Window the image by decreasing luma from center to the edges using an inverse square law. Currently only used internally, as part of the translational registration. Might be useful in general.

Simon Perreault and Patrick Hebert, "Median Filtering in Constant Time", 2007 http://nomis80.org/ctmf.html

Nobuyuki Otsu, "A threshold selection method from gray-level histograms", 1979 http://en.wikipedia.org/wiki/Otsu%27s_method

Leptonica, "The Tophat and H-dome transforms", http://www.leptonica.com/grayscale-morphology.html#TOPHAT-HDOME

P. Peterlin, "Morphological Operations: An Overview", http://www.inf.u-szeged.hu/ssip/1996/morpho/morphology.html

Adrien Bousseau, "Mathematical Morphology", PDF at http://artis.imag.fr/Members/Adrien.Bousseau/morphology/

affine, affine transform, alpha, alpha blending, alpha channel, average, binarization, black tophat, blending, canny, chain transforms, charcoal, clockwise, closing, composite blending, composition, computer vision, const expansion, convolution filter, counter-clockwise, cropping, cut region, cyclic wrap expansion, dilation, document processing, edge shrinking, edge-detection, effect, emboss, erosion, expansion, extend expansion, external gradient, extract rectangle, extract region, fast fourier transform, fft, filter, flip, fourier transform, gamma correction, geometry, gradient, histogram, hypot, identity transforms, image, integral image, internal gradient, inverse fourier transform, inversion, invert transforms, log-compression, log-polar transformation, matrix, max, max-filter, mean, mean filter, median, median-filter, middle, min, min-filter, mirror, mirror expansion, montage, morphology, opening, otsu threshold, perspective, perspective transform, photo, pixel mapping, prewitt, projective, projective transform, quadrilateral, rank-order filter, raw transform, rectangle cut, rectangle extraction, reflect, reflect about aix, reflect about line, reflective transforms, region cut, region of interest, remapping, replicate edge expansion, rescale, resize, roberts, rotate, rotate about a point, rotate transforms, rotation, sabattier effect, scale, scale transforms, scaling, scharr, sharpen, shear, shearing transforms, shrinking, sobel, solarization, sqrt-compression, standard deviation filter, statistics, stddev, summed area table, threshold, thresholding, toggle map, tophat, toroidal wrap expansion, transform, transform affine, transform chaining, transform identity, transform inversion, transform perspective, transform projective, transform reflect, transform rotation, transform scale, transform shear, transform translate, transform, fast fourier, transform, fourier, transform, inverse fourier, transformation, log-polar, translate, translate transforms, translation, variance, vector, vector-field, warp, white tophat, windowing, wrap expansion

Copyright © 2011 Andreas Kupries

Copyright © 2011 Documentation, Andreas Kupries